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>Picture this it is. It's September twenty twenty three.

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<v Speaker 3>Right.

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<v Speaker 2>You are just going about your normal day, maybe pouring

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<v Speaker 2>a cup of coffee, sitting in traffic, just taking.

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<v Speaker 3>A breath, a completely ordinary Tuesday, exactly.

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<v Speaker 2>But right at that exact moment, high above our heads,

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<v Speaker 2>NASA's Fermi satellite registers an event in the cosmos so

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<v Speaker 2>staggeringly powerful that, for a brief, just a fleeting fraction

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<v Speaker 2>of a second, a single explosion outshines entire galaxies.

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<v Speaker 3>It's almost hard to wrap your head around the scale

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<v Speaker 3>of it.

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<v Speaker 2>It really is talking about a concentrated burst of light

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<v Speaker 2>that dwarfs the combined output of billions of stars billions,

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<v Speaker 2>and it gets registered in the astronomical community as GRB

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<v Speaker 2>two three zero nine zero six A, which.

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<v Speaker 3>Is a highly peculiar immensely violent class of phenomena.

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<v Speaker 2>Right, a short gamma ray burst. So okay, let's unpack

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<v Speaker 2>this because trying to mentally process an explosion that outshines

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<v Speaker 2>a galaxy, it requires looking at the actual mechanics of

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<v Speaker 2>what triggers it.

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<v Speaker 3>And the culprits. In this case, we're two neutron.

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<v Speaker 2>Stars, dead crushed remnants of massive stars.

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<v Speaker 3>Exactly stars that spiral together and collided hundreds of millions

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<v Speaker 3>of years ago.

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<v Speaker 2>We are going to map out exactly how an explosion

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<v Speaker 2>of that magnitude happens. But more importantly, we're going to

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<v Speaker 2>look at how this distant, chaotic violence is fundamentally connected

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<v Speaker 2>to the jewelry.

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<v Speaker 3>You wear and the iron and the blood flowing through

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<v Speaker 3>your veins right now.

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<v Speaker 2>Yeah, So, just starting with the sheer physics of what

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<v Speaker 2>the Fermi satellite recorded that day.

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<v Speaker 3>It really challenges our everyday understanding of scale. I mean,

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<v Speaker 3>to get a blast that outshines of galaxy, you need

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<v Speaker 3>a mechanism that converts mass into energy with terrifying.

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<v Speaker 2>Efficiency, right, And that is where the neutron stars come in.

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<v Speaker 3>Because we aren't talking about active fusing stars like our sun.

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<v Speaker 3>We were looking at the absolute extreme limit of material density, the.

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<v Speaker 2>Very limit before black hole.

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<v Speaker 3>Forms, precisely when a giant star dies and its core collapses.

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<v Speaker 3>That gravitational crush is so intense that electrons and protons

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<v Speaker 3>are physically forced together.

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<v Speaker 2>They just get mashed into neutrons.

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<v Speaker 3>We'll mashed together to become neutrons, and the result is

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<v Speaker 3>a sphere maybe ten or twelve.

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<v Speaker 2>Miles across, basically the size of a small city.

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<v Speaker 3>A small city, yeah yeah, but it contains the mass

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<v Speaker 3>of an entire sun.

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<v Speaker 2>Which is wild like a single teaspoon of neutrons star

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<v Speaker 2>material would weigh what billions of tons?

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<v Speaker 3>Billions of tons just one teaspoon, So hundreds of millions

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<v Speaker 3>of years ago, two of these ultra dense remnants found

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<v Speaker 3>themselves locked in a decaying orbit.

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<v Speaker 2>Just circling each other.

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<v Speaker 3>Circling, spiraling toward each other, accelerating to a significant fraction

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<v Speaker 3>of the speed of.

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<v Speaker 2>Light until they ultimately collided.

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<v Speaker 3>In that kinetic impact and the resulting instantaneous release of

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<v Speaker 3>high energy radiation that is what washed over the Fermi

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<v Speaker 3>satellite in twenty twenty three.

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<v Speaker 2>Just visualizing a city sized atomic nucleus crashing into another

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<v Speaker 2>one at near light speed, it is.

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<v Speaker 3>The ultimate cosmic hammer and anvil.

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<v Speaker 2>Yeah, that's a perfect way to put it. But the

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<v Speaker 2>blast didn't happen in a vacuum, which brings us to

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<v Speaker 2>the actual location of the collision.

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<v Speaker 3>The cosmic crime scene.

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<v Speaker 2>Right, the cosmic crime scene, because this wasn't some localized

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<v Speaker 2>event in our own galactic backyard, not at all. The

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<v Speaker 2>environment where this happened is a faint galaxy situated inside

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<v Speaker 2>a much larger group of galaxies, and it's a staggering

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<v Speaker 2>eight point five billion light years away from us.

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<v Speaker 3>The eight point five billion year travel time provides really

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<v Speaker 3>essential context here because think about it, the Earth itself

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<v Speaker 3>is only about four point five billion years old.

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<v Speaker 2>So this light was already on its way.

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<v Speaker 3>The high energy photons from this gamma ray burs had

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<v Speaker 3>already been traveling through the void of space for four

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<v Speaker 3>billion years before our solar system even coalesced from a cloud.

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<v Speaker 2>Of dust, before there was even an Earth to eventually

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<v Speaker 2>hit exactly.

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<v Speaker 3>But locating an event that far back in time and

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<v Speaker 3>that far away in space is an incredibly difficult piece

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<v Speaker 3>of astronomical detective work.

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<v Speaker 2>Because Fermi just gives you the general area right right.

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<v Speaker 3>FORMI is a fantastic instrument for detecting gamma rays. But

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<v Speaker 3>gamma rays are notoriously hard to focus. They don't bounce

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<v Speaker 3>off traditional mirror. This blast tree through art They blastraight through.

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<v Speaker 3>So SERMI can tell us that a massive burst happened,

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<v Speaker 3>and it can give us a general patch of.

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<v Speaker 2>Sky, but it can't pinpoint the exact street address.

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<v Speaker 3>No, it's too wide of a net.

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<v Speaker 2>It's kind of like hearing a sonic boom.

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<v Speaker 3>Oh, that's a great analogy.

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<v Speaker 2>You know, a jet just broke the sound barrier somewhere overhead,

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<v Speaker 2>but you can't point to the exact cubic meter of

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<v Speaker 2>air it happened in just by the sound alone. You

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<v Speaker 2>have to look for the contrail.

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<v Speaker 3>That is exactly it. And finding that cosmic contrail required

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<v Speaker 3>bringing in two two vastly different observational tools.

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<v Speaker 2>NASA's Chandra X ray Observatory and the Hubble Space Telescope.

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<v Speaker 3>Right now, Hubble operates heavily in the visible and near

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<v Speaker 3>infrared spectrum. It excels at showing us the architecture of

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<v Speaker 3>the universe.

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<v Speaker 2>The shapes and structures of the galaxies themselves.

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<v Speaker 3>Yes, but to connect the gamma ray bursts to a

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<v Speaker 3>specific galaxy astronomers.

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<v Speaker 2>Needed Chandra because of the afterglow.

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<v Speaker 3>Decisely after the initial gamma ray flash subsides the explosion

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<v Speaker 3>leaves behind a feeding after glow of lower energy light,

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<v Speaker 3>particularly X rays.

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<v Speaker 2>And astronomy professor Jane Charlton highlighted a really critical reality

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<v Speaker 2>about the specific observation he did. She said that without

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<v Speaker 2>the incredibly precise X ray imaging capabilities of the Chandra observatory,

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<v Speaker 2>this faint host galaxy would have been completely missed.

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<v Speaker 3>Because without the X ray data, you just have a

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<v Speaker 3>picture of thousands of distant galaxies.

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<v Speaker 2>From Hubble, just a sea of smudges, a sea.

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<v Speaker 3>Of smudges, and absolutely no way to know which one

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<v Speaker 3>hosted the explosion. You need Chan to find the glowing

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<v Speaker 3>embers to narrow it down right. What's fascinating here is

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<v Speaker 3>how relying on a single observational method leaves you blind

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<v Speaker 3>to the actual mechanics of the universe.

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<v Speaker 2>You need the layered approach exactly.

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<v Speaker 3>By layering the data, taking the high energy X ray

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<v Speaker 3>pinpoint from Chandra and overlaying it onto the deep optical

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<v Speaker 3>field captured by Hubble, astronomers could drop a literal pin

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<v Speaker 3>on a map eight point five billion light years away.

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<v Speaker 2>They found the host galaxy.

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<v Speaker 3>We found it. But more importantly, Hubble's optical data revealed

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<v Speaker 3>that this galaxy wasn't just sitting in isolation.

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<v Speaker 2>It belongs to a larger group it does.

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<v Speaker 3>And that entire group is currently in the middle of

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<v Speaker 3>a massive, chaotic cosmic merger.

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<v Speaker 2>A galactic pile up. Which is wild because when we

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<v Speaker 2>think of galaxies, we usually picture these serene, majestic pinwheels,

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<v Speaker 2>just slowly rotating in.

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<v Speaker 3>The dark like our own Milky Way looks in artistic renderings, right.

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<v Speaker 2>But the environment where this burst happened is the total

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<v Speaker 2>opposite of serene. These galaxies are actively colliding.

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<v Speaker 3>Their gravitational fields are interacting in real time.

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<v Speaker 2>They are ripping material away from each other, and all

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<v Speaker 2>that turbulence is stirring up massive, massive amounts of new

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<v Speaker 2>star formation.

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<v Speaker 3>And within this chaotic wreckage, astronomers isolated the exact location

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<v Speaker 3>of the.

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<v Speaker 2>Blast inside a structure known as a tible tale a

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<v Speaker 2>tidle tail. Yes, so walk us through what a tidal

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<v Speaker 2>tale actually is physically in the middle of a multi

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<v Speaker 2>galaxy merger.

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<v Speaker 3>To understand a title tale, we really have to look

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<v Speaker 3>at the fluid mechanic of gravity on a massive scale. Galaxies,

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<v Speaker 3>you have to remember, are predominantly empty space.

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<v Speaker 2>Just populated by billions of stars.

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<v Speaker 3>Stars, and vast reservoirs of coal, gas, and dust. So

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<v Speaker 3>when two galaxies pass close to one another, they don't

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<v Speaker 3>usually crash like solid objects.

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<v Speaker 2>They don't just smashed together like rocks.

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<v Speaker 3>No, Instead, their gravitational fields interlock. But gravity follows the

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<v Speaker 3>inverse square.

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<v Speaker 2>Law, meaning its strength drops off exponentially with distance.

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<v Speaker 3>Exactly so, the side of a galaxy see that is

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<v Speaker 3>closest to the intruding galaxy feels a vastly stronger gravitational

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<v Speaker 3>pull than the side facing away.

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<v Speaker 2>It's a differential pole, differential poll. Yeah, it's like taking

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<v Speaker 2>two massive balls of taffy and bring them close together.

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<v Speaker 2>The edges closest to each other grab on, and as

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<v Speaker 2>the bodies continue their momentum, those edges get stretched out

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<v Speaker 2>into long, stringy lines of sugar connecting the two main pieces.

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<v Speaker 3>That is a brilliant way to visualize it.

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<v Speaker 2>Only in this case, the taffy is made of millions

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<v Speaker 2>of stars in interstellar gas, and the strings are hundreds

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<v Speaker 2>of thousands of light years long.

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<v Speaker 3>The taffy analogy perfectly captures the sheer stretching force involved.

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<v Speaker 3>That differential gravitational pull literally strips the outer layers of

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<v Speaker 3>the galaxies away, just heels it off, peels it off,

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<v Speaker 3>drawing out these immense, sweeping ribbons of material into intergalactic space.

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<v Speaker 3>Those ribbons are the tidal tails.

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<v Speaker 2>The elongated shrapnel of a galactic interaction.

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<v Speaker 3>And importantly, those tails are absolutely packed at the cold

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<v Speaker 3>gas and dust that was formally just floating in the

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<v Speaker 3>outer disks of the galaxy.

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<v Speaker 2>So it's yanked out and funneled.

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<v Speaker 3>Funneled into these narrow streams, and as it does, the

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<v Speaker 3>gas violently compresses.

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<v Speaker 2>And when you compress cold gas in space, you basically

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<v Speaker 2>build a cosmic pressure cooker.

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<v Speaker 3>You certainly do.

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<v Speaker 2>The density spikes, the temperature rises, and you trigger a

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<v Speaker 2>massive wave of new star formation, which brings us to

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<v Speaker 2>a specific sequence of events proposed by researcher Simone di Quiara.

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<v Speaker 3>Dikiara's timeline is fascinating.

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<v Speaker 2>Yeah. He laid out this seven hundred million year timeline

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<v Speaker 2>that connects the grand macro scale of this galaxy collision

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<v Speaker 2>directly down to the microscale of those two neutron stars colliding.

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<v Speaker 3>The timeline he outlines is a perfect demonstration of stellar

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<v Speaker 3>evolution accelerated by a chaotic environment.

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<v Speaker 2>So the clock starts roughly seven hundred million years before

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<v Speaker 2>the gamma raypors.

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<v Speaker 3>Right, the galaxies get emerged, the tidal forces stretch out

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<v Speaker 3>the taffy, and a resulting compression in the tidal tail

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<v Speaker 3>triggers the starburst phase.

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<v Speaker 2>Just a massive ignition.

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<v Speaker 3>Millions of new st ignite almost simultaneously within this ribbon

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<v Speaker 3>of debris. But the key here is the type of

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<v Speaker 3>stars being born.

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<v Speaker 2>The compression favors a specific kind.

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<v Speaker 3>The intense compression in a tidal tale heavily favors the

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<v Speaker 3>creation of incredibly massive stars. We are talking O type

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<v Speaker 3>and B type stars that are dozens of times more

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<v Speaker 3>massive than our Sun.

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<v Speaker 2>And the rule with stars is the bigger they are,

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<v Speaker 2>the harder they fall, and the.

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<v Speaker 3>Faster they burn through their fuel.

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<v Speaker 2>Right, a star like our Sun might sip its hydrogen

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<v Speaker 2>for ten billion years, but these massive giants born in

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<v Speaker 2>the tidal tail, they are burning through their nuclear fuel

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<v Speaker 2>at a ridiculous rate.

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<v Speaker 3>They live fast and die young. Astronomically speaking, their life

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<v Speaker 3>spans are mere.

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<v Speaker 2>Blips, just a few million years.

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<v Speaker 3>Within a few million years, these hyper massive stars exhaust

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<v Speaker 3>the hydrogen in their cores, the outward pressure of nuclear fusion.

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<v Speaker 2>Drops, and gravity takes over.

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<v Speaker 3>The star can no longer support its own immense weight

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<v Speaker 3>against the crush of gravity. The core collapses in a

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<v Speaker 3>fraction of a second.

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<v Speaker 2>And the outer layers rebound in a catastrophic supernova explosion.

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<v Speaker 3>Leaving behind the crushed neutron star core we discussed earlier. Now,

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<v Speaker 3>because stars often form in.

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<v Speaker 2>Pairs, binary systems, yes.

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<v Speaker 3>Binary systems, you frequently end up with two massive stars

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<v Speaker 3>orbiting each other that both go supernova.

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<v Speaker 2>Assuming the explosions don't just kick them apart entirely.

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<v Speaker 3>Exactly, assuming they stay gravitationally bound, you are left with

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<v Speaker 3>a compact binary.

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<v Speaker 2>System, two dead neutron stars orbiting a common center of mass,

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<v Speaker 2>just floating inside this tidal.

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<v Speaker 3>Tail, orbiting in the dark.

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<v Speaker 2>So the tidal tale essentially acts as a hyper efficient

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<v Speaker 2>factory for producing pairs of dead neutron stars.

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<v Speaker 3>A factory build from galactic wreckage.

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<v Speaker 2>But they don't just immediately crash into each other. According

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<v Speaker 2>to Dickyar's timeline, they spend hundreds of millions of years

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<v Speaker 2>in a kind of agonizingly slow death spiral. Right, how

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<v Speaker 2>does a binary pair of dead stars eventually close the distance?

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<v Speaker 2>I mean, in a vacuum, shouldn't they just orbit forever?

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<v Speaker 3>If we relied strictly on Newtonian physics, they would orbit forever.

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<v Speaker 3>But in the realm of extreme gravity, Einstein's general relativity

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<v Speaker 3>takes over.

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<v Speaker 2>Okay.

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<v Speaker 3>As these two incredibly dense masses orbit each other, they

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<v Speaker 3>accelerate through the gravitational field, which creates ripples in the

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<v Speaker 3>actual fabric.

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<v Speaker 2>Of space time gravitational waves.

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<v Speaker 3>Yes, gravitational waves. You can think of gravitational waves as

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<v Speaker 3>a mechanism that physically bleeds kinetic energy away from the

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<v Speaker 3>binary system, like friction almost sort of. Yes, As energy

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<v Speaker 3>is radiated away into space, the orbit shrinks. It is

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<v Speaker 3>a slow, relentless process.

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<v Speaker 2>So for hundreds of millions of years, they bleed.

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<v Speaker 3>Energy, spiraling closer and closer, faster and faster, until the

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<v Speaker 3>orbit decays completely.

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<v Speaker 2>And that is the climax of the seven hundred million

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<v Speaker 2>year journey. The compact binary star merger. You touch the

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<v Speaker 2>system violently, shares a part, and it triggers the massive

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<v Speaker 2>short gamma ray bursts that Fermi saw in twenty twenty three.

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<v Speaker 3>If we connect this to the bigger picture, Dikyure's hypothesis

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<v Speaker 3>really redefines how we view the life cycle of a galaxy.

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<v Speaker 3>How so well, the tidal interactions aren't merely the setting

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<v Speaker 3>for this event. The gravitational disruption is the direct trigger.

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<v Speaker 2>It's a chain reaction exactly.

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<v Speaker 3>The chaotic merger forces the compression. The compression forces the

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<v Speaker 3>massive star birth. The massive stars rapidly die to leave

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<v Speaker 3>neutron stars, and the neutron stars decay into a catastrophic merger.

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<v Speaker 2>The largest structures in the universe. Colliding galaxies are directly

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<v Speaker 2>responsible for generating the most concentrated microscopic points of extreme energy.

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<v Speaker 3>It is the ultimate cosmic domino effect.

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<v Speaker 2>That is just incredible. But the final massive explosion, the merger,

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<v Speaker 2>it doesn't just produce a blinding flash of light and

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<v Speaker 2>then fade into history.

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<v Speaker 3>No, it leaves a very permanent mark.

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<v Speaker 2>That collision fundamentally alters the chemistry of the universe around it,

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<v Speaker 2>because when those two neutron stars slam together, the physics

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<v Speaker 2>get so extreme that they create a phenomenon called a killinova.

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<v Speaker 3>A killinova, yes.

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<v Speaker 2>And a killinova is basically the universe's premiere heavy metal forge.

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<v Speaker 3>The term forge is incredibly accurate. There when we observe

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<v Speaker 3>killinova emissions, we are seeing the brightly glowing, rapidly expanding

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00:14:09.320 --> 00:14:12.519
<v Speaker 3>halo of radioactive material ejected during.

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<v Speaker 2>The collision, just blasting our words.

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00:14:14.200 --> 00:14:16.200
<v Speaker 3>And to understand why this is a forge, we have

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00:14:16.279 --> 00:14:17.840
<v Speaker 3>to look at how elements are created in.

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<v Speaker 2>The first place, like in normal stars.

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00:14:19.639 --> 00:14:23.840
<v Speaker 3>Right, normal stars synthesize light elements hydrogen and helium, helium

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00:14:23.879 --> 00:14:26.120
<v Speaker 3>into carbon, oxygen all the way up to iron.

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00:14:26.279 --> 00:14:28.919
<v Speaker 2>But iron is the wall, right, the dead end.

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00:14:29.240 --> 00:14:33.840
<v Speaker 3>Iron is the absolute limit for normal stellar fusion. Fusing

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00:14:33.879 --> 00:14:36.919
<v Speaker 3>iron requires more energy than it releases, so a normal

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00:14:36.960 --> 00:14:38.000
<v Speaker 3>star just stops there.

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00:14:38.600 --> 00:14:41.919
<v Speaker 2>So to get past iron to create elements heavier than iron,

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00:14:42.000 --> 00:14:46.200
<v Speaker 2>like gold, platinum, or uranium, you need something way more intense.

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<v Speaker 3>You need an environment with an overwhelming abundance of free

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<v Speaker 3>neutrons and incomprehensible energy.

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00:14:51.440 --> 00:14:54.320
<v Speaker 2>Because neutrons have no electrical charge. Exactly, if you try

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00:14:54.360 --> 00:14:57.960
<v Speaker 2>to mash to positively charged atomic nuclei together, they just

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00:14:58.039 --> 00:15:00.600
<v Speaker 2>repel each other. But a neutron you can just slip

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<v Speaker 2>right past the defenses and bury itself in the nucleus.

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<v Speaker 3>That is the core mechanism of what astrophysicists call the

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00:15:06.799 --> 00:15:10.720
<v Speaker 3>rapid neutron capture process the R process. The R process.

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<v Speaker 3>During the fraction of a second when the two neutron

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<v Speaker 3>stars collide, the environment is flooded with a density of

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<v Speaker 3>free neutrons that exists almost nowhere else in the universe.

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<v Speaker 2>Just a total deluge of neutrons.

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00:15:21.360 --> 00:15:25.000
<v Speaker 3>Atomic nuclei are bombarded with these neutrons so rapidly that

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<v Speaker 3>they capture them before they even have a chance to

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<v Speaker 3>undergo radioactive decay.

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00:15:29.000 --> 00:15:31.000
<v Speaker 2>So the nucleus just balloons in size.

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<v Speaker 3>It balloons, becomes highly unstable, and then finally decays into

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<v Speaker 3>a stable, incredibly heavy element.

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00:15:37.200 --> 00:15:40.120
<v Speaker 2>And the kilinova is the site of this R process.

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<v Speaker 3>The explosion creates elements like gold and platinum, and the

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00:15:43.440 --> 00:15:46.639
<v Speaker 3>kinetic force of the blast physically scatters them outward into

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<v Speaker 3>the surrounding interstellar medium.

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00:15:48.440 --> 00:15:51.440
<v Speaker 2>Which actually solves a massive puzzle in astronomy too. It

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00:15:51.480 --> 00:15:55.480
<v Speaker 2>really does, because for years astronomers looking at interacting galaxies

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00:15:55.639 --> 00:15:59.519
<v Speaker 2>notice something strange. They were seeing heightened levels of heavy

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<v Speaker 2>elements like gold and platinum, specifically located in the halos.

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00:16:03.480 --> 00:16:07.080
<v Speaker 2>The chaotic outer fringes of these merging galaxies, and it

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00:16:07.080 --> 00:16:10.000
<v Speaker 2>did make sense, right, Why is the heavy stuff floating

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00:16:10.039 --> 00:16:12.080
<v Speaker 2>way out in the cosmic suburbs exactly?

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00:16:12.159 --> 00:16:16.360
<v Speaker 3>And the observation of GRB two three zero nine zero

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00:16:16.399 --> 00:16:20.440
<v Speaker 3>six A within a tidal tail provides a highly elegant,

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00:16:20.720 --> 00:16:22.679
<v Speaker 3>observable solution to that mystery.

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00:16:22.720 --> 00:16:23.679
<v Speaker 2>It's the smoking gun.

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00:16:23.960 --> 00:16:27.159
<v Speaker 3>It is the interacting galaxies draw out the tidal tails

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<v Speaker 3>into the outer halos. The tails greed the massive stars.

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00:16:30.399 --> 00:16:34.759
<v Speaker 3>The stars leave the neutron binaries, the binaries merge into kilnova.

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00:16:34.320 --> 00:16:37.440
<v Speaker 2>And there are process sprays those newly forged heavy elements

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<v Speaker 2>directly into that outer galactic envelope.

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00:16:40.080 --> 00:16:44.240
<v Speaker 3>The environment forces the creation of the forge, exactly where

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<v Speaker 3>we see the resulting metals.

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00:16:45.600 --> 00:16:47.919
<v Speaker 2>Here's where it gets really interesting, because we've been talking

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<v Speaker 2>about galaxies eight point five billion light years away, but

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<v Speaker 2>this cosmic alchemy is intimately tied to you, the listener,

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<v Speaker 2>very intimately tied. Professor Jane Charlton reviewed the data from

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<v Speaker 2>this event and noted that it gives us a rare

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<v Speaker 2>glimpse into how destruction acts as a catalyst for creation.

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<v Speaker 3>The universe doesn't just destroy, it aggressively.

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<v Speaker 2>Recycled, aggressively recycles.

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<v Speaker 3>I love that the recycling process is really the foundation

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<v Speaker 3>of our physical reality. We tend to view massive cosmic

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00:17:18.640 --> 00:17:22.799
<v Speaker 3>explosions as endpoints, the death of stars right game over,

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00:17:22.920 --> 00:17:25.759
<v Speaker 3>But chemically speaking, they are seeding mechanisms.

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00:17:25.920 --> 00:17:27.799
<v Speaker 2>Think about the gold right here on Earth, like if

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00:17:27.839 --> 00:17:30.039
<v Speaker 2>you are wearing a gold ring right now, or just

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00:17:30.079 --> 00:17:32.640
<v Speaker 2>holding a smartphone that relies on trace amounts of gold

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00:17:32.640 --> 00:17:33.480
<v Speaker 2>and its microchips.

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00:17:33.599 --> 00:17:36.079
<v Speaker 3>Earth didn't make that gold, no, and our.

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00:17:36.000 --> 00:17:40.319
<v Speaker 2>Sun cannot make that gold. Every single atom of gold

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00:17:40.319 --> 00:17:42.839
<v Speaker 2>on this planet was forged in the rare process of

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<v Speaker 2>a kilinovo.

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00:17:43.799 --> 00:17:45.799
<v Speaker 3>Which is astonishing to think about.

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00:17:46.160 --> 00:17:49.440
<v Speaker 2>Billions of years ago, somewhere in the cosmos, neutron stars

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00:17:49.519 --> 00:17:52.759
<v Speaker 2>smashed into each other, and the shrapnel from that distant

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00:17:52.839 --> 00:17:56.279
<v Speaker 2>violence eventually drifted into the cloud of gas that formed

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<v Speaker 2>our solar system.

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00:17:57.559 --> 00:18:01.359
<v Speaker 3>You are interacting with the wreckage of a cosmic collision

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00:18:01.440 --> 00:18:03.279
<v Speaker 3>on a daily basis.

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00:18:02.880 --> 00:18:04.759
<v Speaker 2>And it goes deeper than the metal in your phone.

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00:18:04.799 --> 00:18:06.240
<v Speaker 2>It goes straight into your biology.

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00:18:06.359 --> 00:18:10.759
<v Speaker 3>Yes, Charlton made a point to connect this astrophysical process

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00:18:11.279 --> 00:18:14.039
<v Speaker 3>to the very physiological mechanisms keeping us alive.

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00:18:14.240 --> 00:18:16.519
<v Speaker 2>The heavier elements in our bodies.

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00:18:16.119 --> 00:18:19.680
<v Speaker 3>Particularly iron. Iron has an extraordinary origin It is the

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<v Speaker 3>central atom in the heme group of hemoglobin.

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00:18:22.559 --> 00:18:25.960
<v Speaker 2>The protein in red blood cells that binds to oxygen.

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00:18:26.200 --> 00:18:29.079
<v Speaker 3>Exactly when you take a breath, oxygen from your lungs

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00:18:29.079 --> 00:18:31.599
<v Speaker 3>binds to the iron in your blood to be transported

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00:18:31.599 --> 00:18:34.839
<v Speaker 3>to every cell in your body. Without that specific atomic structure,

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00:18:35.200 --> 00:18:37.599
<v Speaker 3>respiration as we know it completely fails.

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00:18:37.799 --> 00:18:39.359
<v Speaker 2>And the origin of that iron.

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00:18:39.279 --> 00:18:42.359
<v Speaker 3>It was synthesized in the cores of dyeing massive stars

390
00:18:42.799 --> 00:18:46.640
<v Speaker 3>just before they went supernova. The current estimate is that

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00:18:46.680 --> 00:18:49.599
<v Speaker 3>the iron coursing through your veins right now is an

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00:18:49.640 --> 00:18:54.119
<v Speaker 3>amalgamation of material forged in the explosive depths of roughly

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00:18:54.200 --> 00:18:57.599
<v Speaker 3>ten thousand different massive stars in the Milky Way's history.

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00:18:57.920 --> 00:19:01.079
<v Speaker 2>The human body is essentially a mosaic constructed from the

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00:19:01.079 --> 00:19:04.599
<v Speaker 2>remains of ten thousand dead stars. It is every time

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00:19:04.640 --> 00:19:07.200
<v Speaker 2>your heart pumps, you were relying on heavy elements that

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00:19:07.240 --> 00:19:10.039
<v Speaker 2>were forged in a pressure cooker billions of years before

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00:19:10.079 --> 00:19:11.079
<v Speaker 2>Earth even existed.

399
00:19:11.200 --> 00:19:14.880
<v Speaker 3>Ten thousand stars had to live, burn fiercely, and detonate

400
00:19:15.000 --> 00:19:17.839
<v Speaker 3>violently just to see the gas cloud that would eventually

401
00:19:17.880 --> 00:19:18.880
<v Speaker 3>allow you to exist.

402
00:19:19.079 --> 00:19:21.519
<v Speaker 2>It completely reframes how you look at the night sky.

403
00:19:21.839 --> 00:19:24.079
<v Speaker 2>It's not just an empty void with pretty lights. It

404
00:19:24.160 --> 00:19:27.319
<v Speaker 2>is the active machinery that manufactured the chemistry required for

405
00:19:27.400 --> 00:19:28.359
<v Speaker 2>complex life, and.

406
00:19:28.319 --> 00:19:31.680
<v Speaker 3>The timescale required for that machinery to operate is deeply humbling.

407
00:19:32.000 --> 00:19:34.319
<v Speaker 3>The universe operates with a profound patience.

408
00:19:34.480 --> 00:19:36.440
<v Speaker 2>Hundreds of millions of years just for.

409
00:19:36.400 --> 00:19:40.000
<v Speaker 3>The initial galaxies to interact. Then it took millions of

410
00:19:40.079 --> 00:19:43.640
<v Speaker 3>years for the massive stars to form and die, hundreds

411
00:19:43.680 --> 00:19:46.960
<v Speaker 3>of millions more for the neutron binaries to decay and merge,

412
00:19:47.400 --> 00:19:48.960
<v Speaker 3>scattering their payload.

413
00:19:48.759 --> 00:19:50.880
<v Speaker 2>Just a slow, methodical process.

414
00:19:50.960 --> 00:19:54.160
<v Speaker 3>Then it took billions of years for that scattered stardust

415
00:19:54.200 --> 00:19:57.200
<v Speaker 3>the iron the goal the carbon to coalesce in the

416
00:19:57.200 --> 00:20:02.279
<v Speaker 3>interstellar medium, collapse into a protoplanetary disk and form the Earth.

417
00:20:02.000 --> 00:20:05.359
<v Speaker 2>And then billions of years of biological evolution on top

418
00:20:05.400 --> 00:20:05.839
<v Speaker 2>of that.

419
00:20:05.839 --> 00:20:09.599
<v Speaker 3>For organisms to develop the complex metabolic pathways to actually

420
00:20:09.680 --> 00:20:13.920
<v Speaker 3>utilize that iron for respiration. We are the beneficiaries of

421
00:20:13.960 --> 00:20:16.640
<v Speaker 3>a supply chain that has been running for billions of years.

422
00:20:17.000 --> 00:20:19.960
<v Speaker 2>But even with all of these profound connections and everything

423
00:20:20.000 --> 00:20:22.440
<v Speaker 2>we have deduced from the light of GRB two three

424
00:20:22.519 --> 00:20:25.640
<v Speaker 2>zero nine zero six A, the cosmos isn't handing over

425
00:20:25.680 --> 00:20:26.400
<v Speaker 2>all its secrets.

426
00:20:26.440 --> 00:20:27.079
<v Speaker 3>No, it never does.

427
00:20:27.200 --> 00:20:29.880
<v Speaker 2>There is still a significant amount of ambiguity surrounding this

428
00:20:29.960 --> 00:20:32.599
<v Speaker 2>specific event. The detective work is far from over.

429
00:20:32.839 --> 00:20:35.920
<v Speaker 3>The nature of observational astronomy is that every answer refines

430
00:20:35.960 --> 00:20:39.319
<v Speaker 3>our models, but it also exposes the limitations of our

431
00:20:39.319 --> 00:20:40.920
<v Speaker 3>current instruments.

432
00:20:40.480 --> 00:20:43.519
<v Speaker 2>And in the case of this specific burst, the most

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00:20:43.599 --> 00:20:46.559
<v Speaker 2>pressing unsolved mystery is its exact.

434
00:20:46.160 --> 00:20:49.119
<v Speaker 3>Redshift, which translates to its exact distance.

435
00:20:49.319 --> 00:20:53.279
<v Speaker 2>Right. Our current spectroscopic data places it at an estimated

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00:20:53.359 --> 00:20:57.000
<v Speaker 2>eight point five billion light years away, but the host

437
00:20:57.119 --> 00:21:01.000
<v Speaker 2>galaxy is so incredibly faint and the data is noisy

438
00:21:01.119 --> 00:21:03.599
<v Speaker 2>enough that there is a margin of error.

439
00:21:03.480 --> 00:21:05.039
<v Speaker 3>A fairly significant one.

440
00:21:04.839 --> 00:21:08.119
<v Speaker 2>Because redshift is essentially how we measure distance in an

441
00:21:08.160 --> 00:21:09.119
<v Speaker 2>expanding universe.

442
00:21:09.200 --> 00:21:10.000
<v Speaker 3>Right. That's right.

443
00:21:10.200 --> 00:21:13.519
<v Speaker 2>As light travels toward us over billions of years, the

444
00:21:13.559 --> 00:21:17.960
<v Speaker 2>actual fabric of space is stretching, which stretches the light waves,

445
00:21:18.079 --> 00:21:20.599
<v Speaker 2>shifting them toward the red end of the spectrum.

446
00:21:20.119 --> 00:21:22.160
<v Speaker 3>The red or the light the farther it traveled.

447
00:21:22.359 --> 00:21:25.279
<v Speaker 2>But if a galaxy is barely a smudge on Hubble's lens,

448
00:21:25.599 --> 00:21:28.839
<v Speaker 2>getting a clean read on that stretched light is really tough,

449
00:21:29.039 --> 00:21:31.480
<v Speaker 2>and if the current estimates are off, this explosion might

450
00:21:31.519 --> 00:21:32.960
<v Speaker 2>be even further away than we think.

451
00:21:33.119 --> 00:21:36.039
<v Speaker 3>Precisely, if the actual red shift is on the higher

452
00:21:36.119 --> 00:21:39.440
<v Speaker 3>end of the possible spectrum, it would significantly push back

453
00:21:39.519 --> 00:21:42.400
<v Speaker 3>the distance in the timeline, making it much older. It

454
00:21:42.400 --> 00:21:45.160
<v Speaker 3>would make GRB two three zero nine zero six A

455
00:21:45.599 --> 00:21:47.519
<v Speaker 3>one of the most distant and therefore one of the

456
00:21:47.559 --> 00:21:50.960
<v Speaker 3>earliest short gamma ray bursts ever recorded in human history.

457
00:21:51.079 --> 00:21:53.720
<v Speaker 2>Meaning we are looking at the r process heavy element

458
00:21:53.799 --> 00:21:58.079
<v Speaker 2>forge operating incredibly early in the universe's lifespan.

459
00:21:57.640 --> 00:21:59.759
<v Speaker 3>Which raises an important question, but the future of our

460
00:21:59.759 --> 00:22:03.119
<v Speaker 3>open servational infrastructure. Well, we've pushed Chandra and Hubble to

461
00:22:03.160 --> 00:22:05.920
<v Speaker 3>their absolute limits to find this one bullet hole.

462
00:22:06.039 --> 00:22:07.079
<v Speaker 2>We need better eyes.

463
00:22:07.119 --> 00:22:11.240
<v Speaker 3>Exactly. While Chandra and Hubble have defined a generation of astrophysics,

464
00:22:11.480 --> 00:22:15.720
<v Speaker 3>they simply cannot resolve the faint spectroscopic signatures of galaxies

465
00:22:15.960 --> 00:22:18.599
<v Speaker 3>at the very edge of the observable universe with the

466
00:22:18.640 --> 00:22:20.039
<v Speaker 3>precision we now require.

467
00:22:20.200 --> 00:22:21.680
<v Speaker 2>So what's the next step.

468
00:22:21.640 --> 00:22:24.079
<v Speaker 3>To lock down the true distance of this burst and

469
00:22:24.119 --> 00:22:27.839
<v Speaker 3>to deeply map the tidal structures of these ancient galactic mergers.

470
00:22:28.359 --> 00:22:32.319
<v Speaker 3>We are entirely dependent on next generation observatories.

471
00:22:31.839 --> 00:22:34.279
<v Speaker 2>Like the James Web Space telescope.

472
00:22:33.720 --> 00:22:38.119
<v Speaker 3>Instruments operating with the infrared sensitivity of JWST, combined with

473
00:22:38.200 --> 00:22:41.720
<v Speaker 3>proposed future high energy X ray probes, will be required

474
00:22:41.759 --> 00:22:45.160
<v Speaker 3>to really dissect the chemistry of these distant chaotic environments.

475
00:22:45.400 --> 00:22:47.680
<v Speaker 2>We are always building a bigger lens to see a

476
00:22:47.720 --> 00:22:48.880
<v Speaker 2>little deeper into the dark.

477
00:22:49.000 --> 00:22:49.440
<v Speaker 3>Always.

478
00:22:49.440 --> 00:22:52.519
<v Speaker 2>But here is the ultimate twist to this entire story.

479
00:22:53.039 --> 00:22:57.119
<v Speaker 2>We've been looking outward this whole time, studying this chaotic

480
00:22:57.400 --> 00:23:02.519
<v Speaker 2>galactic merger eight point five billion light years away, analyzing

481
00:23:02.559 --> 00:23:05.759
<v Speaker 2>the tidal tales and the Kilanova forges right. But the

482
00:23:05.759 --> 00:23:08.839
<v Speaker 2>physics we are observing out there are eventually coming for us.

483
00:23:09.039 --> 00:23:09.599
<v Speaker 3>Yes they are.

484
00:23:09.839 --> 00:23:13.680
<v Speaker 2>Professor Charlton reminded us of a very sobering fact. Having

485
00:23:13.759 --> 00:23:17.680
<v Speaker 2>neighbors in the universe is common. Galaxies are highly social,

486
00:23:17.839 --> 00:23:19.160
<v Speaker 2>they cluster, and our.

487
00:23:19.000 --> 00:23:22.000
<v Speaker 3>Own Milky Way galaxy has a very massive.

488
00:23:21.559 --> 00:23:23.400
<v Speaker 2>Neighbor, the Andromata galaxy.

489
00:23:23.519 --> 00:23:27.000
<v Speaker 3>It is the closest major spiral galaxy to our own,

490
00:23:27.319 --> 00:23:30.720
<v Speaker 3>located approximately two point five million light years away.

491
00:23:30.519 --> 00:23:33.240
<v Speaker 2>Which seems far, but on a cosmic scale, it's right

492
00:23:33.240 --> 00:23:33.720
<v Speaker 2>next door.

493
00:23:33.839 --> 00:23:35.480
<v Speaker 3>It's right next door. If you look at it in

494
00:23:35.519 --> 00:23:38.079
<v Speaker 3>the night sky today, it appears as a faint, stable

495
00:23:38.160 --> 00:23:41.640
<v Speaker 3>smudge of light, but the gravitational dynamics between the Milky

496
00:23:41.680 --> 00:23:43.799
<v Speaker 3>Way and Andromeda are already locked in.

497
00:23:43.880 --> 00:23:44.759
<v Speaker 2>The gears are turning.

498
00:23:44.920 --> 00:23:47.640
<v Speaker 3>The two galaxies are gravitationally bound, and they are currently

499
00:23:47.680 --> 00:23:49.200
<v Speaker 3>accelerating toward one another.

500
00:23:49.319 --> 00:23:51.960
<v Speaker 2>The space between us is shrinking every second.

501
00:23:52.119 --> 00:23:55.720
<v Speaker 3>As Charlton pointed out, living in a galactic group is standard,

502
00:23:55.880 --> 00:23:59.319
<v Speaker 3>but undergoing a major merger is a completely transformative event.

503
00:24:00.119 --> 00:24:03.480
<v Speaker 3>The Milky Way, that event is an absolute certainty.

504
00:24:03.680 --> 00:24:06.880
<v Speaker 2>It is a cosmic inevitability. In roughly four to five

505
00:24:07.000 --> 00:24:10.519
<v Speaker 2>billion years, the Milky Way and Andromeda are going to collide.

506
00:24:10.839 --> 00:24:13.759
<v Speaker 3>And as we've learned from studying GRB two three zero

507
00:24:13.880 --> 00:24:17.400
<v Speaker 3>nine zer six A, galaxies don't just gently bump into

508
00:24:17.480 --> 00:24:17.880
<v Speaker 3>each other.

509
00:24:18.000 --> 00:24:21.720
<v Speaker 2>No, they don't. When Andromeda arrives, our serene spiral structure

510
00:24:21.759 --> 00:24:25.640
<v Speaker 2>is going to be completely obliterated. The exact same chaotic

511
00:24:25.640 --> 00:24:28.759
<v Speaker 2>physics we just mapped out eight point five billion light

512
00:24:28.880 --> 00:24:30.759
<v Speaker 2>years away are going to happen right here in our

513
00:24:30.799 --> 00:24:31.440
<v Speaker 2>local space.

514
00:24:31.720 --> 00:24:34.839
<v Speaker 3>The parallels to our future are undeniable. It's going to

515
00:24:34.880 --> 00:24:37.680
<v Speaker 3>be a mess, a spectacular mess. As the two immense

516
00:24:37.759 --> 00:24:41.440
<v Speaker 3>dark matter halos and stellar disks intersect, the differential gravitational

517
00:24:41.440 --> 00:24:44.160
<v Speaker 3>forces will tear both galaxies apart the night.

518
00:24:44.000 --> 00:24:47.039
<v Speaker 2>Sky from Earth, assuming the Earth still exists in some form,

519
00:24:47.079 --> 00:24:49.519
<v Speaker 2>would be totally unrecognizable.

520
00:24:48.759 --> 00:24:52.359
<v Speaker 3>Completely alien. Massive tidle Tales will be violently drawn out

521
00:24:52.400 --> 00:24:55.240
<v Speaker 3>from the Milky Way and Andromeda, stretching hundreds of thousands

522
00:24:55.279 --> 00:24:57.799
<v Speaker 3>of light years into the intergalactic medium.

523
00:24:57.519 --> 00:25:00.599
<v Speaker 2>Just massive ribbons of taffy of taffy.

524
00:25:00.720 --> 00:25:05.440
<v Speaker 3>Yes, the interstellar gas within our galaxy will be subjected

525
00:25:05.480 --> 00:25:08.079
<v Speaker 3>to immense shock waves in compression.

526
00:25:07.759 --> 00:25:10.440
<v Speaker 2>And we know exactly what happens when you compress gas

527
00:25:10.440 --> 00:25:13.680
<v Speaker 2>In a title Tale, the cosmic pressure cooker turns on

528
00:25:13.960 --> 00:25:17.480
<v Speaker 2>exactly the Milcomeata merger is going to ignite a furious

529
00:25:17.519 --> 00:25:22.400
<v Speaker 2>firestorm of new star formation. Millions of massive O type

530
00:25:22.400 --> 00:25:26.200
<v Speaker 2>and B type stars will burn fast, go supernova, and

531
00:25:26.359 --> 00:25:29.599
<v Speaker 2>populate our newly formed Title Tales with a massive new

532
00:25:29.640 --> 00:25:31.880
<v Speaker 2>generation of dead neutron stars.

533
00:25:32.119 --> 00:25:35.880
<v Speaker 3>The cycle will repeat itself flawlessly over the subsequent hundreds

534
00:25:35.880 --> 00:25:39.400
<v Speaker 3>of millions of years. Those local binary neutron stars will

535
00:25:39.400 --> 00:25:43.319
<v Speaker 3>bleed their orporal energy via gravitational waves. It will spiral inward,

536
00:25:43.440 --> 00:25:46.160
<v Speaker 3>and eventually our newly merged galaxy will be lit up

537
00:25:46.200 --> 00:25:49.480
<v Speaker 3>by a series of short gamma ray bursts and killinova.

538
00:25:49.000 --> 00:25:51.079
<v Speaker 2>Explosion, setting off the forge again.

539
00:25:50.880 --> 00:25:53.519
<v Speaker 3>And our process will activate in our own cosmic backyard,

540
00:25:53.680 --> 00:25:56.519
<v Speaker 3>heavily enriching the local environment with a massive influx of

541
00:25:56.599 --> 00:25:58.519
<v Speaker 3>newly forged heavy elements.

542
00:25:58.079 --> 00:26:02.359
<v Speaker 2>Fresh gold, fresh platinum, whole new batch. So what does

543
00:26:02.359 --> 00:26:04.319
<v Speaker 2>this all mean for you? It means that you aren't

544
00:26:04.359 --> 00:26:06.400
<v Speaker 2>just a passive observer sitting on a rock in a

545
00:26:06.400 --> 00:26:09.559
<v Speaker 2>static universe, not at all. You are an active participant

546
00:26:09.559 --> 00:26:13.640
<v Speaker 2>in an incredibly violent, incredibly beautiful cycle of cosmic recycling.

547
00:26:14.279 --> 00:26:17.119
<v Speaker 2>The iron currently binding the oxygen in your blood is

548
00:26:17.160 --> 00:26:20.440
<v Speaker 2>the direct physical evidence of ancient stellar destruction.

549
00:26:20.680 --> 00:26:22.640
<v Speaker 3>We exist because stars die.

550
00:26:22.759 --> 00:26:25.920
<v Speaker 2>We are walking, talking proof that destruction is the absolute

551
00:26:25.960 --> 00:26:29.799
<v Speaker 2>prerequisite for creation, and knowing that our entire galaxy is

552
00:26:29.880 --> 00:26:34.000
<v Speaker 2>destined for a cataclysmic collision just proves that the mechanics

553
00:26:34.000 --> 00:26:35.319
<v Speaker 2>of the universe never stop.

554
00:26:35.519 --> 00:26:38.839
<v Speaker 3>It is a profound realization that the violent processes we

555
00:26:38.920 --> 00:26:42.000
<v Speaker 3>observe in the deepest reaches of space are the exact

556
00:26:42.000 --> 00:26:45.359
<v Speaker 3>same processes that engineered our present reality, and.

557
00:26:45.319 --> 00:26:47.680
<v Speaker 2>They are the exact same processes that will dictate our

558
00:26:47.680 --> 00:26:48.400
<v Speaker 2>distant future.

559
00:26:48.519 --> 00:26:51.680
<v Speaker 3>The universe is a continuous engine of transformation, and that.

560
00:26:51.640 --> 00:26:53.279
<v Speaker 2>Leads to a thought. I want to leave you with

561
00:26:53.519 --> 00:26:56.119
<v Speaker 2>a concept to just sit with and mull over long

562
00:26:56.160 --> 00:26:59.079
<v Speaker 2>after you finish listening. We know, as a matter of

563
00:26:59.079 --> 00:27:02.240
<v Speaker 2>measurable physics that the iron pumping through your veins right

564
00:27:02.279 --> 00:27:05.240
<v Speaker 2>now was forged in the violent deaths of ten thousand

565
00:27:05.279 --> 00:27:09.119
<v Speaker 2>ancient stars ten thousand stars. And we know with absolute

566
00:27:09.160 --> 00:27:13.200
<v Speaker 2>gravitational certainty that in four to five billion years, our home,

567
00:27:13.359 --> 00:27:16.759
<v Speaker 2>the Milky Way, will be violently torn apart and smashed

568
00:27:16.799 --> 00:27:20.200
<v Speaker 2>into andromedal. The skies will blaze with new star formation,

569
00:27:20.799 --> 00:27:23.440
<v Speaker 2>monumental tidle tales will whip across the dark, and an

570
00:27:23.599 --> 00:27:26.960
<v Speaker 2>entirely new generation of heavy elements will be forcefully scattered into.

571
00:27:26.799 --> 00:27:28.559
<v Speaker 3>The void, seating the next generation.

572
00:27:29.160 --> 00:27:32.000
<v Speaker 2>So, when our galaxy is finally destroyed and completely remade

573
00:27:32.039 --> 00:27:36.759
<v Speaker 2>by that future collision, what entirely new, unfathomable forms of creation,

574
00:27:36.920 --> 00:27:40.599
<v Speaker 2>what strange new chemistry, or perhaps even what unimaginable new

575
00:27:40.640 --> 00:29:09.119
<v Speaker 2>forms of life might eventually be catalyzed by our own destruction.

576
00:28:03.000 --> 00:28:29.759
<v Speaker 2>Sai
