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 Astronomy 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, and welcome back to the show we are. We're

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<v Speaker 2>absolutely thrilled to have you with us today because we

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<v Speaker 2>are looking up, way, way up exactly. We're turning our

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<v Speaker 2>gaze toward one of the most baffling, high energy mysteries

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<v Speaker 2>in the well, in the entire known universe. We're talking

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<v Speaker 2>about a phenomenon that has basically been taunting astronomers for

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<v Speaker 2>what nearly two decades now.

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<v Speaker 3>It really has. I mean, it's one of those cosmic

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<v Speaker 3>puzzles that just you know, refuses to fit into the box.

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<v Speaker 3>It has kept a lot of very smart people awake

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<v Speaker 3>at night, just staring at data screens.

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<v Speaker 2>We're talking, of course, about fast radio.

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<v Speaker 3>Bursts or frb's for sure.

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<v Speaker 2>I've always loved that name, Fast radio bursts. Yeah, it

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<v Speaker 2>just sounds so urgent, it sounds like a warning, and

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<v Speaker 2>the description it really matches the name, right. These are

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<v Speaker 2>essentially cosmic flickers.

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<v Speaker 3>Flicker is a good word, but it almost understates the

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<v Speaker 3>violence of it. These are millisecond long flashes of radio waves.

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<v Speaker 3>They appear out of nowhere. They just scream across the

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<v Speaker 3>cosmos with this incredible brightness.

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<v Speaker 2>And when you say incredible, you mean.

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<v Speaker 3>I mean releasing as much energy in a fraction of

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<v Speaker 3>a second as our sun does in days or weeks,

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<v Speaker 3>or for some of them, even a century.

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<v Speaker 2>A century's worth of solar energy in a millisecond, and

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<v Speaker 2>then lah, they're gone.

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<v Speaker 3>Silence.

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<v Speaker 2>That is the part that gets me every time we

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<v Speaker 2>discuss this topic, the sheer scale of the energy versus

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<v Speaker 2>the brevity of the event. It's like a camera flash

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<v Speaker 2>that blinds you from across the room m m, but

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<v Speaker 2>the camera is actually located in another galaxy entirely.

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<v Speaker 3>That is a fantastic way to visualize it. And because

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<v Speaker 3>they're so bright and so short, for the longest time,

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<v Speaker 3>the big question, the obsession really has been what is

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<v Speaker 3>the engine driving these things? What kind of cosmic beast

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<v Speaker 3>has the power to scream that loud that fast?

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<v Speaker 2>Right, It's the classic celestial Who do unit are they?

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<v Speaker 2>You know, lonely isolated stars just screaming into the void.

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<v Speaker 3>Is it a cataclysmic explosion where something is being destroyed

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<v Speaker 3>or is.

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<v Speaker 2>There something more complex, maybe even more structural, going on.

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<v Speaker 3>It has been a massive open question in astrophysics for

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<v Speaker 3>a long time. There were more theories than there were

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<v Speaker 3>observed bursts.

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<v Speaker 2>But that's changing, and that's why we're here today. We're

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<v Speaker 2>unpacking a major, major break in the.

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<v Speaker 3>Case we are And this isn't just a theory or

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<v Speaker 3>some computer simulation running in a basement somewhere. This is well,

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<v Speaker 3>the paper calls it decisive evidence, Okay, published just recently

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<v Speaker 3>on January sixteenth, twenty twenty six, in the journal Science.

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<v Speaker 2>And this comes from a huge international team.

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<v Speaker 3>Right, a massive collaboration, yeah, including researchers from the University

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<v Speaker 3>of Hong Kong or HKU. And the headline is just

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<v Speaker 3>it's astonishing at least some of these FRB sources, they're

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<v Speaker 3>not living the single life.

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<v Speaker 2>They are in relationships. I like that. Even stars need

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<v Speaker 2>a plus one exactly.

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<v Speaker 3>They are in binary stellar systems. They have companions, and

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<v Speaker 3>that well a lot changes everything about how we understand them.

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<v Speaker 2>So today we are starting a full investigation. We're going

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<v Speaker 2>to unpack this discovery piece by piece. We're going to

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<v Speaker 2>meet the detective in this story, a massive telescope called

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<v Speaker 2>the China Sky.

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<v Speaker 3>I, and we'll look at the subject, a specific repeating

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<v Speaker 3>burse source known as FRB two two zero five and

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<v Speaker 3>two nine A.

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<v Speaker 2>And we're going to talk about a smoking gun event,

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<v Speaker 2>a little something called an RM flare. And just to

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<v Speaker 2>give you a roadnap, this isn't just about finding a

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<v Speaker 2>second star. It's about how a really boring observation, literally

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<v Speaker 2>staring and nothing happening for months, suddenly turned into a

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<v Speaker 2>discovery that might just change our understanding of the architecture

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<v Speaker 2>of the universe.

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<v Speaker 3>It's a great story. It's about patients, the physics of

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<v Speaker 3>light and well stellar weather.

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<v Speaker 2>I love stories where boredom pays off. It gives me

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<v Speaker 2>hope for my own life. So let's set the scene.

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<v Speaker 2>This wasn't a lucky snapshot, was it. This wasn't someone

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<v Speaker 2>just pointing a telescope at the sky at random and

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<v Speaker 2>boom they get lucky.

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<v Speaker 3>This is a scakeout, oh precisely. This is a long term,

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<v Speaker 3>calculated stakeout. And to understand why this is so special

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<v Speaker 3>and why we haven't found this before. We have to

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<v Speaker 3>talk about the tool they used, the Fast telescope.

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<v Speaker 2>Fast FAST that stands for the five hundred meter aperture spherical.

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<v Speaker 3>Telescope located in Guzu, China. It's the world's largest filled

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<v Speaker 3>aperture radio telescope. When we say China Sky, we aren't kidding.

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<v Speaker 3>The scale of this thing is. It's just hard to wrap.

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<v Speaker 2>Your head around five hundred meters across. If you filled

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<v Speaker 2>that dish with water, you're not talking about a pool,

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<v Speaker 2>you're talking about a lake.

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<v Speaker 3>You could fit entire neighborhoods inside the dish. And in

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<v Speaker 3>radio astronomy, size is everything.

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<v Speaker 2>Size matters, it really does.

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<v Speaker 3>The larger the dish, the more radio waves you can catch.

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<v Speaker 3>It's like having a bigger bucket in.

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<v Speaker 2>The rain, right, a bigger bucket catches more.

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<v Speaker 3>In this case, the drops are these incredibly faint radio

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<v Speaker 3>signals from billions of light years away. The sensitivity of

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<v Speaker 3>Fast is what makes this kind of detailed monitoring even possible.

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<v Speaker 3>It can hear whispers that other telescopes might miss entirely.

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<v Speaker 2>So they've got this massive ear listening to the sky

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<v Speaker 2>and they didn't just listen to static. They pointed this

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<v Speaker 2>massive ear at a very very specific.

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<v Speaker 3>Target FRB two two zero five two nine.

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<v Speaker 2>A, which I have to say sounds like a license plate.

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<v Speaker 3>It does. It's not the most poetic man. Astronomers are

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<v Speaker 3>great at math, not always great at branding. Yeah, but

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<v Speaker 3>that license plate represents an active repeating source and it's

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<v Speaker 3>located about two point five billion light years away.

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<v Speaker 2>Okay, before we go any further, let's pause on that

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<v Speaker 2>word repeating, because that is a crucial distinction in this field,

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<v Speaker 2>isn't it.

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<v Speaker 3>It's everything.

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<v Speaker 2>My understanding is that most of these fast radio bursts

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<v Speaker 2>they happen once and then they never happen again.

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<v Speaker 3>That's right. The vast majority of FOI we've ever detected

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<v Speaker 3>are one offs, a flash, and then silence forever from

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<v Speaker 3>that spot in the sky.

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<v Speaker 2>And those must be incredibly hard to study.

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<v Speaker 3>Oh they're a nightmare because you can't predict them. You

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<v Speaker 3>don't know where to look until it's already over. It's

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<v Speaker 3>like trying to study a lightning bolt without knowing where

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<v Speaker 3>the storm is, or trying.

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<v Speaker 2>To study a car crash after the tow truck has

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<v Speaker 2>already left.

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

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<v Speaker 3>is different.

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<v Speaker 2>A repeater is a gift.

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<v Speaker 3>It is a gift. It flashes again and again. It

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<v Speaker 3>gives you a specific address in the sky to focus on.

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<v Speaker 3>It says hey, I'm over here, keep watching.

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<v Speaker 2>Which means you can keep the camera rolling, so to speak.

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<v Speaker 3>Exactly. Repeaters allow for long term monitoring. You can watch

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<v Speaker 3>them over time to see if anything in their environment changes.

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<v Speaker 3>You can track their behavior, their patterns. And that is

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<v Speaker 3>exactly what the FRB Key Science Program has been doing

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<v Speaker 3>since twenty twenty.

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<v Speaker 2>And this program was co led by Professor Bingzhang, the

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<v Speaker 2>chair Professor of Astrophysics.

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<v Speaker 3>At HKU CORRECT and they decided to keep a very

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<v Speaker 3>close watch on this one specific source FRB two two

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<v Speaker 3>zero five two nine A.

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<v Speaker 2>And this is where the human element comes in, the patience.

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<v Speaker 3>Here is where the patien's part of science really comes

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<v Speaker 3>into play. I think people often imagine science as these

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<v Speaker 3>constant Eureka moments happening every day in the.

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<v Speaker 2>Lab, right the flashing light bulbs over people's heads.

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<v Speaker 3>But often it just looks like monotony. For seventeen months

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<v Speaker 3>they watched this source.

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<v Speaker 2>Seventeen months is almost a year and a half of

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<v Speaker 2>just staring.

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<v Speaker 3>And for seventeen months, the data appeared well, unremarkable, unremarkable,

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<v Speaker 3>just doing its normal thing, blinking occasionally, standard repeating FRB behavior.

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<v Speaker 3>The signal looked clean, consistent, and frankly a bit boring.

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<v Speaker 2>I can just imagine the researchers checking the data every morning.

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<v Speaker 2>Anything new, Nope, anything weird, nope, just seventeen months of

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<v Speaker 2>steady as she goes. I mean, why keep looking? If

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<v Speaker 2>I stared at a wall for seventeen months and it

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<v Speaker 2>didn't move, I would probably stop staring.

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<v Speaker 3>Well, you need that baseline. That's the key. If you

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<v Speaker 3>don't know what normal looks like, you can't possibly recognize abnormal.

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<v Speaker 3>Ah okay, you have to know the resting heartbeat of

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<v Speaker 3>the system before you can diagnose in arrhythmia. You need

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<v Speaker 3>the control group.

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<v Speaker 2>That's a fair point. You can't spot the anomaly if

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<v Speaker 2>you don't know the pattern exactly.

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<v Speaker 3>And then near the end of twenty twenty three, the

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<v Speaker 3>boredom broke.

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<v Speaker 2>The turning point, the exciting part.

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<v Speaker 3>The data suddenly spiked. Something changed drastically in the signal

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<v Speaker 3>they were receiving.

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<v Speaker 2>Okay, so let's unpack that change, because this is where

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<v Speaker 2>we get into the real physics of the discovery. Yeah,

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<v Speaker 2>this wasn't just the signal got louder right, It wasn't

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<v Speaker 2>just a volume knob being turned up.

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<v Speaker 3>No, not at all. It was about the quality of

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<v Speaker 3>the light, specifically something called polarization.

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<v Speaker 2>Polarization. Okay, I think most of us have heard that word,

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<v Speaker 2>probably in the context of what sunglasses we do.

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<v Speaker 3>That's the perfect daily life analogy. Think about light from

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<v Speaker 3>the sun or a light bulb. Usually, the light waves

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<v Speaker 3>are vibrating in all directions at once, up and down,

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<v Speaker 3>left and right, diagonally. It's a chaotic jumble of vibration,

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<v Speaker 3>like a crowd.

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<v Speaker 2>Of people walking in every direction at a busy intersection.

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<v Speaker 3>Perfect but polarized light is disciplined. All the waves are

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<v Speaker 3>vibrating in the same plane. Imagine shaking a rope. If

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<v Speaker 3>you shake it up and down, the wave is vertical.

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<v Speaker 3>If you shake it side to side, the wave is horizontal.

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<v Speaker 3>That's polarization.

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<v Speaker 2>And these FRBs have what nearly perfect polarization.

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<v Speaker 3>Near one hundred percent linear polarization. So it's like someone

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<v Speaker 3>is shaking a rope across the universe in a very

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<v Speaker 3>specific direction. It's an incredibly pure signal and polarized sunglasses.

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<v Speaker 2>They work by blocking the waves that aren't lined.

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<v Speaker 3>Up correctly exactly. They act like a tiny picket fence.

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<v Speaker 3>If you shake that rope up and down, it can

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<v Speaker 3>pass through the vertical slats of the.

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<v Speaker 2>Fence, but if you shake it side to side, the.

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<v Speaker 3>Fence stops it. That's how they cut down on glare.

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<v Speaker 2>Okay, So we have these perfectly oriented waves. Let's just

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<v Speaker 2>say they're vibrating up and down and they're traveling through

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<v Speaker 2>space for two point five billion years. They're headed toward Earth.

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<v Speaker 2>What happens to them.

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<v Speaker 3>On the way, Well, space isn't perfectly empty, especially not

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<v Speaker 3>the space right around the source of the burst. As

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<v Speaker 3>these radio waves travel, they might pass through what we

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<v Speaker 3>call magnetized plasma.

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<v Speaker 2>Magnetized plasma. That sounds like something from a sci fi weapon.

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<v Speaker 3>It sounds exotic, but it's actually one of the most

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<v Speaker 3>common things in the universe. Plasma is just a gas

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<v Speaker 3>that's been superheated until the electrons are ripped off the atoms.

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<v Speaker 3>It's a hot charge soup, okay, And magnetize just means

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<v Speaker 3>there's a magnetic field running through it.

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<v Speaker 2>So we have our rope wave traveling through this hot

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<v Speaker 2>magnetic soup. What does the soup do to the rope?

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<v Speaker 3>It twists it, It twists it, it rotates the angle

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<v Speaker 3>of the vibration. This effect is called Ferritaday rotation. So

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<v Speaker 3>if the waves started out vibrating up and down, after

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<v Speaker 3>passing through the magnetized plasma, it might be vibrating diagonally

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<v Speaker 3>or even completely side to side by the time it

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<v Speaker 3>gets to us.

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<v Speaker 2>So the plasma literally grabs the wave and physically spins

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<v Speaker 2>the orientation.

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<v Speaker 3>That's a great way to think of it. And the

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<v Speaker 3>more dense the plasma is, or the stronger the magnetic field,

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<v Speaker 3>the more it twists. And we can measure that twist.

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<v Speaker 2>Wow.

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<v Speaker 3>We use a metric called the rotation measure, or RM

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<v Speaker 3>for short.

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<v Speaker 2>So the RM is basically a number that tells you

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<v Speaker 2>how much has this signal been twisted by the stuff

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<v Speaker 2>it flew through to get to us.

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<v Speaker 3>That is a perfect summary. The higher the RM number,

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<v Speaker 3>the more stuff it flew through, or the more magnetic

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<v Speaker 3>that stuff was.

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<v Speaker 2>Okay, so let's go back to our stakeout. We have

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<v Speaker 2>seventeen months of data from FAST.

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<v Speaker 3>And during the seventeen months the rotation measure, that amount

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<v Speaker 3>of twist was pretty constant. It had a steady low value.

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<v Speaker 2>Which tells us the environment around the FRB was.

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<v Speaker 3>Stable, very stable. The light was passing through the same

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<v Speaker 3>amount of stuff every single day. Normal, boring, predictable.

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<v Speaker 2>And then came late twenty twenty.

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<v Speaker 3>Three entered doctor Ye Lee from the Purple Mountain Observatory.

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<v Speaker 3>Doctor Lee was analyzing the data and noted an abrupt,

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<v Speaker 3>massive increase in the rotation measure.

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<v Speaker 2>How massive very time? Did it? Double?

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<v Speaker 3>Yeah, it increased by more than a factor of one hundred.

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<v Speaker 2>WHOA Okay, that is not a blip, that's not a

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<v Speaker 2>measurement error. That is a fundamental distortion.

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<v Speaker 3>It was a massive distortion. The signal was being twisted

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<v Speaker 3>wildly compared to what they had seen for the last

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<v Speaker 3>year and a half. And here's the key piece of evidence.

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<v Speaker 3>This spike didn't stay forever. It rapidly declined and returned

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<v Speaker 3>to normal over a period of just two weeks.

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<v Speaker 2>So seventeen months of normal, two weeks of extreme twisting,

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<v Speaker 2>and then right back normal.

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<v Speaker 3>The team dubbed this event an RM flare.

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<v Speaker 2>An RM flare, it sounds dramatic, so let's put on

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<v Speaker 2>our detective hats here. If the twist comes from passing

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<v Speaker 2>through plasma. Then a sudden, massive increase in the twist

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<v Speaker 2>means that a very dense, very magnetized plasma suddenly crossed

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<v Speaker 2>the line of sight between Earth and the FRB.

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<v Speaker 3>That's the only logical conclusion.

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<v Speaker 2>We like analogies, So is this like Imagine we're looking

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<v Speaker 2>at a flashlight being that's the FRB, and for seventeen months,

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<v Speaker 2>the air between us and.

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<v Speaker 3>The flashlight is clear, perfectly clear, and.

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<v Speaker 2>Then suddenly a thick cloud of smoke blows right across

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<v Speaker 2>the beam.

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<v Speaker 3>That is a great analogy. The smoke would distort the

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<v Speaker 3>light light, make it shimmer and change. In this case,

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<v Speaker 3>the smoke is a clump of magnetized plasma, and because

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<v Speaker 3>it only lasted two weeks, we know that this clump

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<v Speaker 3>was moving, it crossed the path and then cleared out.

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<v Speaker 2>So we have a smoking gun or maybe a passing

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<v Speaker 2>cloud of plasma. But where did the plasma come from?

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<v Speaker 2>The FRB is two point five billion light years away.

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<v Speaker 2>We can't just send a drone to check it out.

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<v Speaker 3>No, we have to deduce it. And this is where

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<v Speaker 3>we move to the next phase of our investigation. Identifying

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<v Speaker 3>the culprit connecting the dots.

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<v Speaker 2>Okay, we have twisted radio waves, we have a temporary

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<v Speaker 2>cloud of plasma. How do we get from that to

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<v Speaker 2>binary star system? I mean, why couldn't it just be

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<v Speaker 2>a random cloud floating by in deep space?

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<v Speaker 3>It comes down to probability and physics. Deep space is

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<v Speaker 3>actually pretty empty. The chances of a random dense cloud

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<v Speaker 3>just happening to drift by exactly in front of this

300
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<v Speaker 3>one tiny source are astronomically low. You need a source

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<v Speaker 3>for that plasma, You need an engine that produces it nearby.

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<v Speaker 2>You need a smoke machine to make the smoke exactly.

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<v Speaker 3>And Professor Bingsang provided the explanation. He said, the natural

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<v Speaker 3>explanation for a sudden plasma cloud appearing and disappearing like

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<v Speaker 3>that is a companion star, a neighbor, a very close neighbor.

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<v Speaker 3>Imagine the FRB source, which we're pretty sure as a

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00:14:16.840 --> 00:14:18.559
<v Speaker 3>magnetar and we can get to that in a minute.

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<v Speaker 3>Just sitting there in space and right next to it,

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<v Speaker 3>organing around it is another star, maybe something massive or

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<v Speaker 3>maybe something more like our sun.

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<v Speaker 2>Okay, so they're dancing around each other, a binary system,

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<v Speaker 2>two stars locked together by gravity.

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<v Speaker 3>And just like our son, other stars are active. They

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<v Speaker 3>aren't just calm, glowing balls. They're volatile, they have weather.

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<v Speaker 3>Sometimes they burp.

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<v Speaker 2>They burp.

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<v Speaker 3>Technically, it's called a coronal mass ejection, or a CME.

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<v Speaker 3>You've probably heard of solar storms, oh right, We hear.

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00:14:49.559 --> 00:14:51.759
<v Speaker 2>About those with our own sun all the time. When

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<v Speaker 2>the Sun spits out a huge cloud of stuff that

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<v Speaker 2>can mess with our satellites or create the northern lights.

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00:14:56.600 --> 00:14:58.879
<v Speaker 3>That's the one. And that stuff it spits out is

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00:14:58.919 --> 00:15:02.519
<v Speaker 3>a massive clump you guessed it, magnetized plasma.

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<v Speaker 2>It is.

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00:15:03.159 --> 00:15:07.720
<v Speaker 3>So the scenario they proposes this, the companion star launches

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<v Speaker 3>a CME, a big blob of plasma. This blob physically

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<v Speaker 3>moves out into space, and in this specific case, its

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00:15:15.679 --> 00:15:18.320
<v Speaker 3>path took it right in front of the FRB source

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<v Speaker 3>from our perspective.

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<v Speaker 2>So it moves right between us and the FRB exactly.

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<v Speaker 3>It didn't block it completely, but it put a very

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<v Speaker 3>dense magnetized filter in front of it. The radio waves

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<v Speaker 3>from the FRB had to pass through this fresh blob

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<v Speaker 3>of plasma to get to Earth. That causes the massive

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<v Speaker 3>twist the RM flare.

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<v Speaker 2>And as the blob keeps moving on its trajectory.

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<v Speaker 3>The distortion fades, and after about two weeks, the coast

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<v Speaker 3>is clear, the blob is moved past our line of sight,

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<v Speaker 3>and the signal goes right back to normal.

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<v Speaker 2>That is incredible detective work. You're watching a tiny blip

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<v Speaker 2>of light, you see it get twisted, and from that

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00:15:50.399 --> 00:15:52.759
<v Speaker 2>you realize, oh, the guy standing next to him and

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00:15:52.799 --> 00:15:53.240
<v Speaker 2>just sneezed.

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<v Speaker 3>That is effectively what happened, a stellar sneeze. Yeah, and

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<v Speaker 3>the math backs it up completely.

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<v Speaker 2>This is where Professor yuan pe Yang from U nine

347
00:16:02.200 --> 00:16:03.879
<v Speaker 2>University comes into the picture, isn't it?

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00:16:04.159 --> 00:16:08.559
<v Speaker 3>Yes? Professor Yang ran the numbers. They calculated the size

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00:16:08.600 --> 00:16:10.879
<v Speaker 3>and the density of the plasma clump that would be

350
00:16:10.919 --> 00:16:13.879
<v Speaker 3>required to cause that specific amount of distortion they saw,

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00:16:14.480 --> 00:16:17.639
<v Speaker 3>and it matched perfectly with the known properties of CMEs

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00:16:18.159 --> 00:16:20.759
<v Speaker 3>launched by our own sun and other stars we've studied

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<v Speaker 3>in the Milky Way.

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<v Speaker 2>So it fits the profile.

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<v Speaker 3>If fits the profile perfectly, if it walks like a

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00:16:25.440 --> 00:16:28.240
<v Speaker 3>duck and quacks like a duck, or in this case,

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00:16:28.320 --> 00:16:31.480
<v Speaker 3>if it twists light exactly like a solar flare, it.

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<v Speaker 2>Is probably a solar flare from a neighborstar. I just

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00:16:34.159 --> 00:16:36.799
<v Speaker 2>want to clarify something for you. The listener. Though. We

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00:16:36.840 --> 00:16:39.120
<v Speaker 2>didn't see this companion star, did we We didn't take

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<v Speaker 2>an optical picture of it.

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00:16:40.279 --> 00:16:43.919
<v Speaker 3>No, absolutely not. At two point five billion light years,

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00:16:44.480 --> 00:16:47.919
<v Speaker 3>Trying to visually see a standard star sitting right next

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<v Speaker 3>to a bright, flaring FRB source is basically impossible with

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00:16:52.240 --> 00:16:55.399
<v Speaker 3>current tech. It's too far and way too faint compared

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<v Speaker 3>to the burst itself. We saw it through its.

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00:16:57.960 --> 00:16:59.759
<v Speaker 2>Inflow, through the mess it made exactly.

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<v Speaker 3>It's all the plasma throughout. It's like seeing footprints up

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<v Speaker 3>here in the snow. You don't see the person who

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00:17:04.920 --> 00:17:06.839
<v Speaker 3>made them, but you know for a fact someone just

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00:17:06.880 --> 00:17:07.400
<v Speaker 3>walked by.

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00:17:07.720 --> 00:17:10.599
<v Speaker 2>That's a great image. Or seeing leaves rustle in the wind.

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<v Speaker 2>You don't see the wind, but you see its effects precisely.

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<v Speaker 3>And we should mention this wasn't just fast working entirely

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00:17:16.839 --> 00:17:21.680
<v Speaker 3>alone in a vacuum. Australia's Parks telescope also contributed continuous

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00:17:21.759 --> 00:17:24.960
<v Speaker 3>radio observations which helped verify these findings. It was a

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00:17:25.000 --> 00:17:26.599
<v Speaker 3>real cross hemisphere effort.

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00:17:26.799 --> 00:17:29.640
<v Speaker 2>So we have the evidence, we have the culprit, a

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00:17:29.680 --> 00:17:33.240
<v Speaker 2>messy neighbor star. What does this mean for the big picture.

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00:17:33.599 --> 00:17:36.519
<v Speaker 2>Let's move to the implications here. Why does it matter

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00:17:36.599 --> 00:17:38.400
<v Speaker 2>so much if an FRB has a buddy.

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00:17:38.799 --> 00:17:41.960
<v Speaker 3>This is where it gets really fascinating for astrophysics, because

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00:17:41.960 --> 00:17:45.880
<v Speaker 3>this discovery helps solidify the identity of the FRB source

384
00:17:45.920 --> 00:17:49.079
<v Speaker 3>itself engine the engine. For a long time, the leading

385
00:17:49.119 --> 00:17:52.359
<v Speaker 3>suspect for what creates frb's has been a magnetar.

386
00:17:52.559 --> 00:17:55.480
<v Speaker 2>A magnetar, which is arguably the most metal thing in

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00:17:55.519 --> 00:17:56.440
<v Speaker 2>the entire universe.

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00:17:56.519 --> 00:17:59.400
<v Speaker 3>It really is. A magnetar is a type of neutron star,

389
00:17:59.480 --> 00:18:02.240
<v Speaker 3>so it's the crushed, collapsed core of a dead star,

390
00:18:02.640 --> 00:18:05.880
<v Speaker 3>and it's incredibly dense. A single teaspoon of it would

391
00:18:05.880 --> 00:18:06.279
<v Speaker 3>weigh a.

392
00:18:06.240 --> 00:18:08.400
<v Speaker 2>Billion tons a billion tons.

393
00:18:08.160 --> 00:18:11.279
<v Speaker 3>But its defining feature is the magnetic field. It has

394
00:18:11.319 --> 00:18:14.799
<v Speaker 3>a magnetic field that is trillions of times stronger than Earth's.

395
00:18:14.720 --> 00:18:17.240
<v Speaker 2>So strong it would literally rip you apart the atomic

396
00:18:17.319 --> 00:18:18.559
<v Speaker 2>level if you got anywhere near it.

397
00:18:18.599 --> 00:18:23.480
<v Speaker 3>That's the one. These are extreme, extreme objects, and the

398
00:18:23.599 --> 00:18:26.079
<v Speaker 3>kind of energy required to produce a fast radio burst

399
00:18:26.160 --> 00:18:28.960
<v Speaker 3>fits perfectly with what a magnetar can output during a

400
00:18:29.000 --> 00:18:31.599
<v Speaker 3>stark wick or a magnetic reconnection event.

401
00:18:31.680 --> 00:18:33.640
<v Speaker 2>But there's been a puzzle, a huge puzzle.

402
00:18:33.720 --> 00:18:36.799
<v Speaker 3>If all FRBs are magnetars, why do some repeat and

403
00:18:36.839 --> 00:18:39.839
<v Speaker 3>some don't? Why are some one and done, while others,

404
00:18:39.960 --> 00:18:42.079
<v Speaker 3>like our friend ever B two two zero five two

405
00:18:42.160 --> 00:18:44.119
<v Speaker 3>nine A keep flashing over and over.

406
00:18:44.440 --> 00:18:48.680
<v Speaker 2>That is the million dollar question. Is it a different

407
00:18:48.720 --> 00:18:51.359
<v Speaker 2>type of star or is it just in a different situation?

408
00:18:51.559 --> 00:18:54.680
<v Speaker 3>And this discovery of a binary system points directly at

409
00:18:54.720 --> 00:18:56.279
<v Speaker 3>the different situation answer.

410
00:18:56.400 --> 00:18:58.279
<v Speaker 2>The relationship changes the behavior.

411
00:18:58.000 --> 00:19:01.160
<v Speaker 3>Itrid be the key. Professor binghas Zeg proposes what he

412
00:19:01.200 --> 00:19:05.000
<v Speaker 3>calls a unified physical picture. The hypothesis is that perhaps

413
00:19:05.079 --> 00:19:08.440
<v Speaker 3>all FRBs really do originate from magnetars, but the ones

414
00:19:08.440 --> 00:19:10.799
<v Speaker 3>that repeat maybe they repeat because they are in a

415
00:19:10.839 --> 00:19:11.640
<v Speaker 3>binary system.

416
00:19:11.759 --> 00:19:15.519
<v Speaker 2>So the partner star is somehow instigating it or enabling it.

417
00:19:15.519 --> 00:19:18.039
<v Speaker 3>It could be a number of things. The interactions in

418
00:19:18.079 --> 00:19:21.799
<v Speaker 3>a binary system might create a preferred geometry or a

419
00:19:21.839 --> 00:19:25.079
<v Speaker 3>specific environment around the magnetar that makes the bursts easier

420
00:19:25.079 --> 00:19:28.839
<v Speaker 3>for us to detect repeatedly. Or maybe the companion star

421
00:19:28.960 --> 00:19:32.920
<v Speaker 3>is feeding material to the magnetar, which fuels more frequent bursts.

422
00:19:33.240 --> 00:19:36.680
<v Speaker 2>Like stoking a fire. The isolated magnetar might have one

423
00:19:36.720 --> 00:19:39.319
<v Speaker 2>big flare up and then it's done, but the one

424
00:19:39.359 --> 00:19:42.039
<v Speaker 2>with a friend keeps getting more fuel shoveled into the furnace.

425
00:19:42.200 --> 00:19:45.799
<v Speaker 3>That's one possibility an isolated magnetar might just act very

426
00:19:45.799 --> 00:19:49.440
<v Speaker 3>differently than one that's constantly interacting with the companion's gravity,

427
00:19:49.680 --> 00:19:53.480
<v Speaker 3>its stellar wind, its magnetic field. It completely shifts our

428
00:19:53.519 --> 00:19:56.880
<v Speaker 3>understanding from thinking about these as isolated star is screaming

429
00:19:56.880 --> 00:19:59.960
<v Speaker 3>in the dark, to well stellar relationships.

430
00:20:00.079 --> 00:20:04.119
<v Speaker 2>It proves that FRBs aren't just random, isolated explosions. They

431
00:20:04.119 --> 00:20:07.000
<v Speaker 2>can be complex interactions within a dynamic system.

432
00:20:07.279 --> 00:20:10.920
<v Speaker 3>It makes the universe feel a lot more alive. Yeah,

433
00:20:10.920 --> 00:20:14.240
<v Speaker 3>and interconnected. It's not just static points of light. It's systems,

434
00:20:14.279 --> 00:20:15.440
<v Speaker 3>it's orbits, it's.

435
00:20:15.319 --> 00:20:18.400
<v Speaker 2>Weather, it's stellar weather, and we're just now learning how

436
00:20:18.400 --> 00:20:21.799
<v Speaker 2>to read the forecast from billions of light years away exactly.

437
00:20:21.960 --> 00:20:24.799
<v Speaker 3>We used to think of space as this mostly static backdrop,

438
00:20:25.119 --> 00:20:28.680
<v Speaker 3>but this shows it's full of events, flares, ejections, interactions

439
00:20:28.680 --> 00:20:32.319
<v Speaker 3>that happen on human timescales weeks, not millions of years.

440
00:20:32.599 --> 00:20:34.759
<v Speaker 2>So let's just take a moment and summarize this win

441
00:20:34.880 --> 00:20:37.960
<v Speaker 2>for science. Yeah, because this really feels like a victory

442
00:20:38.000 --> 00:20:39.519
<v Speaker 2>lap for the whole team involved.

443
00:20:39.640 --> 00:20:43.480
<v Speaker 3>Absolutely, this is a triumph of collaboration. You have researchers

444
00:20:43.519 --> 00:20:47.720
<v Speaker 3>from HKU, Purple Mountain Observatory, Union University and the University

445
00:20:47.720 --> 00:20:50.359
<v Speaker 3>of Science and Technology of China all working together on this.

446
00:20:50.599 --> 00:20:55.240
<v Speaker 2>Professor Swiffing Wu, who was the lead corresponding author, specifically

447
00:20:55.279 --> 00:20:59.400
<v Speaker 2>mentioned the tireless work and persevering observations. And I think

448
00:20:59.400 --> 00:21:01.839
<v Speaker 2>we really saw that in the story that seventeen months

449
00:21:01.839 --> 00:21:02.880
<v Speaker 2>of watching and waiting.

450
00:21:02.960 --> 00:21:05.759
<v Speaker 3>That's the perseverance right there. And we have to give

451
00:21:05.759 --> 00:21:08.880
<v Speaker 3>credit to the technology. This discovery was only possible because

452
00:21:08.920 --> 00:21:12.119
<v Speaker 3>of the extreme sensitivity of fast the China Sky Eye.

453
00:21:12.720 --> 00:21:15.680
<v Speaker 3>You simply cannot do this science with a smaller telescope.

454
00:21:15.960 --> 00:21:18.559
<v Speaker 3>You need the world's best sensitivity to catch a detail,

455
00:21:18.599 --> 00:21:21.519
<v Speaker 3>to subtle a tiny twist in the light from two

456
00:21:21.599 --> 00:21:23.519
<v Speaker 3>point five billion light years away.

457
00:21:23.720 --> 00:21:26.559
<v Speaker 2>So looking forward, what's next? Now that we know at

458
00:21:26.599 --> 00:21:29.279
<v Speaker 2>least some FRBs are in binary.

459
00:21:28.839 --> 00:21:31.559
<v Speaker 3>Systems, now we need to know the statistics. Is this

460
00:21:31.599 --> 00:21:34.720
<v Speaker 3>a fluke, was FRB two two zero five two nine

461
00:21:34.759 --> 00:21:37.799
<v Speaker 3>a just an oddball? Or is this the standard model

462
00:21:37.799 --> 00:21:41.160
<v Speaker 3>for repeaters? Continued monitoring might tell us how common these

463
00:21:41.200 --> 00:21:42.319
<v Speaker 3>binary systems are.

464
00:21:42.559 --> 00:21:45.880
<v Speaker 2>Are most FRBs married to another star or is.

465
00:21:45.880 --> 00:21:49.000
<v Speaker 3>This a rare couple exactly? Is this the exception or

466
00:21:49.079 --> 00:21:51.279
<v Speaker 3>is this the rule? We just don't know yet. We

467
00:21:51.359 --> 00:21:54.759
<v Speaker 3>simply need more data, more stakeouts.

468
00:21:54.319 --> 00:21:58.000
<v Speaker 2>More staring at boring stars for months at a time,

469
00:21:58.160 --> 00:21:59.759
<v Speaker 2>just waiting for them to do something interesting.

470
00:22:00.119 --> 00:22:01.359
<v Speaker 3>That's how discoveries are made.

471
00:22:01.640 --> 00:22:03.640
<v Speaker 2>Well, I think this whole exploration has given us a

472
00:22:03.680 --> 00:22:05.839
<v Speaker 2>completely new way to look at those little flashes in

473
00:22:05.880 --> 00:22:06.240
<v Speaker 2>the sky.

474
00:22:06.440 --> 00:22:07.440
<v Speaker 3>It certainly has for me.

475
00:22:07.759 --> 00:22:10.680
<v Speaker 2>Let's synthesize this entire journey before we let you go. Yeah,

476
00:22:10.880 --> 00:22:14.920
<v Speaker 2>we started with a mysterious flash, a cosmic flicker from

477
00:22:14.960 --> 00:22:17.240
<v Speaker 2>two point five billion light years away.

478
00:22:17.359 --> 00:22:20.240
<v Speaker 3>We had a massive telescope in China staring at it

479
00:22:20.319 --> 00:22:22.920
<v Speaker 3>unblinking for seventeen straight months.

480
00:22:22.960 --> 00:22:25.039
<v Speaker 2>Then we saw a sudden two week twist in the

481
00:22:25.079 --> 00:22:26.599
<v Speaker 2>signal that RM flare.

482
00:22:26.440 --> 00:22:28.519
<v Speaker 3>And we use that twist to realize that a neighbor

483
00:22:28.559 --> 00:22:31.680
<v Speaker 3>star had, in effect sneezed a cloud of plasma right

484
00:22:31.720 --> 00:22:33.079
<v Speaker 3>across our line of sight.

485
00:22:33.160 --> 00:22:36.759
<v Speaker 2>A stellar sneeze caught on tape from across the universe.

486
00:22:37.480 --> 00:22:38.799
<v Speaker 2>It's an incredible story.

487
00:22:39.160 --> 00:22:42.000
<v Speaker 3>It's a reminder that the universe is just so dynamic.

488
00:22:42.359 --> 00:22:46.559
<v Speaker 3>Even things that seem stable, like a repeating signal, can

489
00:22:46.599 --> 00:22:50.160
<v Speaker 3>be subjected to these sudden, violent weather events caused by

490
00:22:50.160 --> 00:22:50.880
<v Speaker 3>their neighbors.

491
00:22:50.960 --> 00:22:53.599
<v Speaker 2>It really makes you think, if we can detect a

492
00:22:53.640 --> 00:22:58.039
<v Speaker 2>star sneezing from two point five billion light years away

493
00:22:58.079 --> 00:23:00.000
<v Speaker 2>just by looking at how it twists a radius.

494
00:23:00.880 --> 00:23:03.319
<v Speaker 3>It raises a pretty provocative question, doesn't it it.

495
00:23:03.240 --> 00:23:07.119
<v Speaker 2>Does, What other invisible events are we missing? What else

496
00:23:07.200 --> 00:23:09.279
<v Speaker 2>is happening out there in the dark between the stars

497
00:23:09.559 --> 00:23:12.359
<v Speaker 2>that we just haven't built the right filter to see yet,

498
00:23:12.599 --> 00:23:14.640
<v Speaker 2>simply because we aren't staring at the right spot for

499
00:23:14.680 --> 00:23:15.240
<v Speaker 2>long enough.

500
00:23:15.359 --> 00:23:17.839
<v Speaker 3>That is the question that keeps the next generation of

501
00:23:17.839 --> 00:23:21.519
<v Speaker 3>astronomers employed, and it's exactly why we keep building bigger

502
00:23:21.559 --> 00:23:22.680
<v Speaker 3>and better telescopes.

503
00:23:22.799 --> 00:23:24.880
<v Speaker 2>Thank you so much for breaking this all down with us.

504
00:23:24.960 --> 00:23:27.759
<v Speaker 2>It has been a really fascinating look at the binary

505
00:23:27.799 --> 00:23:29.839
<v Speaker 2>secret of fast radio bursts.

506
00:23:29.839 --> 00:23:31.839
<v Speaker 3>My pleasure. It's always good to look up.

507
00:23:31.799 --> 00:23:35.680
<v Speaker 2>And to you listening. Keep looking up. You never know

508
00:23:35.720 --> 00:23:37.920
<v Speaker 2>what you might see if you just stare long enough.

509
00:23:38.680 --> 00:23:42.279
<v Speaker 2>Thanks for joining our investigation today. Goodbye for now, see

510
00:23:42.319 --> 00:25:05.720
<v Speaker 2>you next time. The School dass U
