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>Imagine pointing an antenna up at a completely dark, quiet

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<v Speaker 2>patch of the night sky and catching a literal laser beam,

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<v Speaker 2>and not just any laser beam, but one fired when

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<v Speaker 2>the universe was just this chaotic toddler.

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<v Speaker 3>Yeah, it's pretty wild to think about, right.

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<v Speaker 2>I mean, we are talking about an undeniable signal that

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<v Speaker 2>has been traveling toward Earth for over eight billion years.

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<v Speaker 2>This thing originated from an era long before our solar

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<v Speaker 2>system even you know, coalesced exactly.

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<v Speaker 3>It's ancient history hitting our receivers right now.

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<v Speaker 2>Hey, we're unpacking a record breaking natural space laser. It

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<v Speaker 2>was detected by the Meerkat radio telescope in South Africa,

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<v Speaker 2>and we're going to look at the mechanical, the quantum

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<v Speaker 2>and the astrophysical realities of how you even capture a

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<v Speaker 2>signal from the deep past.

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<v Speaker 3>And we'll get into what a hydroxyl megamaser actually is too,

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<v Speaker 3>because that's a huge part of the puzzle.

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<v Speaker 2>Yes, definitely, and ultimately we want to figure out what

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<v Speaker 2>the violent collision of two ancient galaxies reveals about the

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<v Speaker 2>structural evolution of the cosmos. So you know, for anyone

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<v Speaker 2>listening who has ever felt totally overwhelmed by the sheer

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<v Speaker 2>scale of the universe, you're about to get a front

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<v Speaker 2>row seat to an ultimate cosmic time machine.

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<v Speaker 3>It really is a time machine. I mean, the detection

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<v Speaker 3>of this specific signal fundamentally alters our timeline for observational astronomy. Also, well,

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<v Speaker 3>we're looking at a system situated at a redshift of

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<v Speaker 3>roughly z equals one.

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<v Speaker 2>Okay, let's unpack that for a second.

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<v Speaker 3>Sure, so at that distance, we aren't just observing a

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<v Speaker 3>distant object. We're observing the universe and it was less

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<v Speaker 3>than half its current age, which is just.

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<v Speaker 2>A mind boggling scale of time.

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<v Speaker 4>It really is.

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<v Speaker 3>And the fact that we can capture the specific quantum

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<v Speaker 3>signature of a molecule from that epoch and do so

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<v Speaker 3>in a fraction of the time previously thought possible, it

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<v Speaker 3>proves that our transition into this new era of wide

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<v Speaker 3>field radio astronomy is already yielding structural insights into the

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<v Speaker 3>cosmic dawn.

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<v Speaker 2>Let's start right there, actually the concept of redshift and

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<v Speaker 2>looking back in time, because I mean, for anyone who

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<v Speaker 2>follows astrophysics, the basic idea that light has a speed

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<v Speaker 2>limit is pretty well understood, right, Well, it takes time

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<v Speaker 2>to travel. Yeah, so we know that looking across space

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<v Speaker 2>is looking back in time. It's like, well, it's like

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<v Speaker 2>a letter in the mail. If a friend overseas sends

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<v Speaker 2>you a letter, the news is old by the time

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<v Speaker 2>you actually read it.

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<v Speaker 4>That's a great analogy. Yeah.

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<v Speaker 3>Yeah, in space, the light is the letter exactly.

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<v Speaker 2>But what I want to dig into is the physical

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<v Speaker 2>reality of what an eight billion year transit does to

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<v Speaker 2>that letter. Because when a galaxy at z equals one

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<v Speaker 2>fires off a burst of radio waves, that wave has

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<v Speaker 2>to travel through a universe that is actively expanding. Right, Yes,

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<v Speaker 2>the space itself is expanding, So by the time it

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<v Speaker 2>hits the Meerkat telescope, we aren't just dealing with a

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<v Speaker 2>faint signal. We were dealing with a stretched one.

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<v Speaker 3>That is the crucial mechanical difference between local astronomy and

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<v Speaker 3>cosmological astronomy. It's called cosmological red shift. The expansion of

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<v Speaker 3>the universe is a metric expansion of space itself. So

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<v Speaker 3>as the radiophotons emitted by this ancient galaxy travel toward Earth,

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<v Speaker 3>the physical space they're traveling through stretches.

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<v Speaker 2>And so the photon gets stretched with it exactly.

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<v Speaker 3>Consequently, the actual physical wavelength of the photon is stretched out,

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<v Speaker 3>which lowers its frequency.

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<v Speaker 2>Okay, So if a molecule in that distant galaxy emits

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<v Speaker 2>a radio wave at a specific resting frequency, say like

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<v Speaker 2>sixteen hundred and sixty five megahertz, it.

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<v Speaker 3>Absolutely does not arrive at Earth at sixteen sixty five

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<v Speaker 3>mega it says the stretching right, Because it has traveled

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<v Speaker 3>for eight billion years. The expansion of the universe is

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<v Speaker 3>stretched that wave down to around half of its original frequency.

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<v Speaker 2>Wow. So the engineers and astronomers running meerkat they had

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<v Speaker 2>to tune their receivers to a completely different frequency band

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<v Speaker 2>than they would use if they were looking for that

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<v Speaker 2>exact same molecule in our own Milky Way.

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<v Speaker 4>Yes, they did.

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<v Speaker 3>They had to mathematically predict how much the universe had

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<v Speaker 3>expanded over those eight billion years, calculate the resulting frequency drop,

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<v Speaker 3>and literally just listen.

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<v Speaker 2>There that is. I mean, that's just an insane level

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<v Speaker 2>of precision.

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<v Speaker 3>It's incredible, And this tells us something profound about the

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<v Speaker 3>environment we are observing too, Like what, well, when we

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<v Speaker 3>look at a galaxy at a redshift of one, we

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<v Speaker 3>are looking at an era often referred to as the

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<v Speaker 3>tail end of cosmic noon.

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<v Speaker 2>Cosmic noon. I love that term.

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<v Speaker 3>It's a great descriptor. See in the local universe, the

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<v Speaker 3>one immediately around us. Today, galaxies are relatively.

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<v Speaker 2>Quiet, like our Milky Way exactly.

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<v Speaker 3>The Milky Way forms a few solar masses worth of

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<v Speaker 3>stars per year. The gas fractions are lower. The metallicity,

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<v Speaker 3>which is the amount of elements heavier than helium, is higher.

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<v Speaker 2>Right, because generations of stars have already lived and died

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<v Speaker 2>and seated the galaxy with heavy elements.

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<v Speaker 3>Spot On and major galaxy mergers are relatively infrequent now.

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<v Speaker 3>But at z equals one, the universe was structurally different.

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<v Speaker 2>It was that chaotic Toddler phase.

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<v Speaker 3>Yeah, the gas fractions and galaxies were significantly higher. They

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<v Speaker 3>were churning out stars at incredible rates and massive violent

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<v Speaker 3>mergers between galaxies were a dominant driver of cosmic evolution.

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<v Speaker 2>Which perfectly sets the stage for the specific signal they found.

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<v Speaker 2>So they detected a hydroxyl megamaser.

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<v Speaker 4>It did.

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<v Speaker 2>Now, wait, when I hear the word laser or maser,

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<v Speaker 2>the visual is usually a highly collimated beam like a

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<v Speaker 2>sci fi blaster or a synthetic optical cavity with mirrors

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<v Speaker 2>on either end, bouncing photons back and forth to build

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<v Speaker 2>up intensity.

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<v Speaker 4>Right, that's the artificial way we build them on Earth.

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<v Speaker 2>But galaxy isn't a manufactured machine. So how does a massive,

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<v Speaker 2>uncontained cloud of hydroxyl gas maintain the population and version

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<v Speaker 2>needed for a laser without the photons just scattering in

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<v Speaker 2>random directions.

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<v Speaker 3>It's a really good question. It requires a highly specific

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<v Speaker 3>set of environmental conditions that only exist in these extreme environments.

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<v Speaker 2>Okay, laid on me.

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<v Speaker 3>To understand the mechanism, we really have to look at

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<v Speaker 3>the quantum mechanics of the hydroxyl radical, which is just

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<v Speaker 3>one oxygen atom bonded to one hydrogen atom.

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<v Speaker 2>Okay, oh, which got it?

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<v Speaker 3>In its ground state, the hydroxyl molecule has four very

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<v Speaker 3>close energy levels. We call this hyperfine.

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<v Speaker 2>Structure hyperfine structure. Yeah.

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<v Speaker 3>Yeah, These energy levels are determined by the interaction between

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<v Speaker 3>the magnetic field of the molecule's rotation and the spin

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<v Speaker 3>of its unpaired electron and the hydrogen nucleus.

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<v Speaker 2>So it's like this incredibly delicate magnetic balancing act inside

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<v Speaker 2>the molecule exactly.

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<v Speaker 3>And when the molecule drops from a higher hyperfine state

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<v Speaker 3>to a lower one, it emits a microwave photon at

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<v Speaker 3>a very specific frequency.

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<v Speaker 2>And those are the sixteen sixty five and sixteen sixty

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<v Speaker 2>seven megahertz frequency, as you mentioned earlier.

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<v Speaker 4>Those are the most dominant ones.

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<v Speaker 2>Yes, But just having the gas there isn't enough to

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<v Speaker 2>create a maser, right, because under normal thermal conditions wouldn't

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<v Speaker 2>most of the molecules just sit in the lowest possible

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<v Speaker 2>energy state, right.

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<v Speaker 3>They just be lazy. You need something to push him up.

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<v Speaker 3>You need a pumping mechanism.

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<v Speaker 2>A pump, Okay, what acts as a pump in outer space?

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<v Speaker 3>In the case of a hydroxyl megamaser, the pump is

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<v Speaker 3>usually far infrared.

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<v Speaker 2>Radiation infrared so heat basically.

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<v Speaker 3>Yeah, in a violently merging galaxy, you have colossal bursts

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<v Speaker 3>of star formation and often an actively feeding supermassive black hole,

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<v Speaker 3>an active galactic nucleus or agn.

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<v Speaker 2>Right, because everything is crashing together and igniting.

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<v Speaker 3>Exactly, and these intense energy sources heat up the massive

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<v Speaker 3>clouds of surrounding dust. That warm dust then radiates profusely

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<v Speaker 3>in the far infrared.

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<v Speaker 2>Okay, so the dust is glowing with infrared light.

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<v Speaker 3>And the hydroxyl molecules absorb those specific infrared photons, which

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<v Speaker 3>excites them into higher rotational energy states.

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<v Speaker 2>They soak up the heat.

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<v Speaker 3>Yeah, but they don't stay there, as they quickly decay

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<v Speaker 3>back down. They don't just return to a random distribution.

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<v Speaker 3>The quantum mechanics of the decay preferentially populate the upper

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<v Speaker 3>states of that ground level hyperfine structure.

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<v Speaker 2>Oh I see, so it artificially loads up the higher

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<v Speaker 2>energy levels.

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<v Speaker 3>Yes, this creates the population inversion. You now have more

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<v Speaker 3>molecules in the high energy state than the low energy state.

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<v Speaker 2>So the trap is set. You've got this entire molecular

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<v Speaker 2>cloud just sitting there artificially elevated, waiting for a trigger.

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<v Speaker 3>Yes, and the trigger is a single photon passing through

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<v Speaker 3>the gas at exactly.

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<v Speaker 4>The right frequency.

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<v Speaker 3>Just one photon, just one to start the avalanche. When

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<v Speaker 3>that initial photon interacts with an excited hydroxyl molecule, it

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<v Speaker 3>stimulates a molecule to drop to the lower energy.

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<v Speaker 2>State, and then it releases its own.

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<v Speaker 3>Photon, right but releasing a second photon that is perfectly

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<v Speaker 3>in phase, moving in the exact same direction, but the

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<v Speaker 3>exact same frequency is the first one.

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<v Speaker 2>Ah, So one becomes two.

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<v Speaker 4>Two become four, four become eight.

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<v Speaker 3>It is an exponential cascade of stimulated emission.

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<v Speaker 2>That is so cool. But wait, I want to address

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<v Speaker 2>the mirror question. How does it become a directional beam

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<v Speaker 2>that we can actually detect from eight billion light years away?

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<v Speaker 4>Right without the mirrors?

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<v Speaker 2>Yeah, without mirrors to bounce the light back and forth.

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<v Speaker 2>Doesn't the amplification just kind of happen in every direction

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<v Speaker 2>equally like a light bulb.

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<v Speaker 3>You'd think so, But it comes down to the geometry

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<v Speaker 3>and velocity of the gas clouds. While there are no

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<v Speaker 3>physical mirrors, amplification only happens along paths where the gas

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<v Speaker 3>is velocity coherent.

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<v Speaker 2>Velocity coherent meaning it's all moving at the same speed.

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<v Speaker 3>Essentially, if the gas is swirling chaotically, the Doppler shift

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<v Speaker 3>from the relative motion of the molecules will change the

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<v Speaker 3>frequency of the photons from the perspective of the molecules themselves.

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<v Speaker 2>Oh right, The pitch shifts like an ambulance siren.

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<v Speaker 3>Exactly, and that shift breaks the resonance and stops the

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<v Speaker 3>cascade dead in its tracks.

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<v Speaker 2>So it can't amplify if the gas is turbulent.

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<v Speaker 4>Right.

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<v Speaker 3>However, if you look at a massive disc of gas

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<v Speaker 3>edge on, or if there's a long linear filament of

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<v Speaker 3>gas moving at a uniform velocity relative to the line

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<v Speaker 3>of sight, then.

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<v Speaker 2>The photons can travel immense distances through the cloud without

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<v Speaker 2>being Doppler shifted out of resonance.

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<v Speaker 4>You got it.

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<v Speaker 3>So the maser beam naturally collimates along the paths of

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<v Speaker 3>greatest velocity coherence. It's essentially beaming its signal along very

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<v Speaker 3>specific geometric sidelines.

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<v Speaker 2>And we just happen to be sitting exactly on one

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<v Speaker 2>of those sitelines. That is incredible cosmic.

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<v Speaker 4>Luck, it is.

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<v Speaker 3>But keep in mind, the scale of this emission is

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<v Speaker 3>what justifies the mega prefix in megamser.

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<v Speaker 2>Right, because standard masers exist in our own milky way,

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<v Speaker 2>don't They usually around individual forming stars?

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<v Speaker 3>They do, But a megamser is millions of times more

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<v Speaker 3>luminous than those local ones.

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<v Speaker 2>So this isn't just one star forming.

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<v Speaker 3>No, this is the collective scream of an entire galaxy

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<v Speaker 3>undergoing a catastrophic transformation. The energy required to pump a

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<v Speaker 3>cloud of hydroxyl gas to the point where becomes a

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<v Speaker 3>megamaver is staggering.

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<v Speaker 2>It must take a galaxy ending event.

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<v Speaker 3>It requires the systemic disruption of the entire galaxy. This

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<v Speaker 3>is why hydroxyl megamasers are almost exclusively found in ultra

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<v Speaker 3>luminous infrared galaxies or ulargies eulargies.

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<v Speaker 2>Astronomers and their acronyms I swear, hey it's efficient, but

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<v Speaker 2>ulargies are overwhelmingly the result of major galaxy mergers.

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<v Speaker 3>The detection of this hydroxyl signature is an unequivocal indicator

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<v Speaker 3>that we are looking at a site of masses cosmic trauma.

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<v Speaker 2>Which brings us to the operational reality of how this

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<v Speaker 2>was actually detected. The signal was caught by the Meerkat

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<v Speaker 2>telescope in South Africa in just five hours of observing.

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<v Speaker 3>Time, which is astonishingly fast.

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<v Speaker 2>I am really stuck on that five hour timeframe, even

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<v Speaker 2>with massive bandwidth in the inherent brightness of a mega maser.

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<v Speaker 2>Gathering enough photons from eight billion light years away in

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<v Speaker 2>a single afternoon seems physically impossible.

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<v Speaker 3>Certainly challenges our traditional expectations.

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<v Speaker 2>Right, because the inverse square law dictates that as the

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<v Speaker 2>signal travels, its energy is distributed over an ever expanding sphere.

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<v Speaker 2>By the time it reaches Earth, the flux density should

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<v Speaker 2>be buried so deep in the thermal noise floor that

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<v Speaker 2>a five hour integration shouldn't even register a blip.

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<v Speaker 4>That's the math.

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<v Speaker 2>Yeah, So what is Meerkat doing differently that breaks that expectation?

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<v Speaker 2>How is it drinking from a fire hose of cosmic

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<v Speaker 2>noise and actually finding something?

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<v Speaker 4>Well?

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<v Speaker 3>Meerkat is a marvel of modern radio interferometry, and to

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<v Speaker 3>really understand its efficiency we need to look at both

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<v Speaker 3>its physical architecture and its computational back end.

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<v Speaker 2>Okay, let's start with the physical.

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<v Speaker 3>Meerkat is not a single giant dish. It is an

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<v Speaker 3>array of sixty four individual antennas, each thirteen point five

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<v Speaker 3>meters across, spread out over distances of up to eight kilometers.

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<v Speaker 2>Oh wow, eight kilometers yeah, And.

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<v Speaker 3>By linking these antennas together, astronomers use a technique called

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<v Speaker 3>aperture synthesis to create a virtual telescope that has the

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<v Speaker 3>resolving power of a single dish eight kilometers wide.

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<v Speaker 2>Right, Because in radio astronomy, the resolution is dictated by

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<v Speaker 2>the maximum dist between your antennas, which are called the baselines.

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<v Speaker 2>But resolving power just gives you a sharper image, right,

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<v Speaker 2>It doesn't inherently give you the raw sensitivity to pull

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<v Speaker 2>a hyper faint signal out of the noise in five hours.

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<v Speaker 4>You're right.

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<v Speaker 3>Sensitivity is a function of the total collecting area, the

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<v Speaker 3>system temperature of the receivers.

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<v Speaker 4>And the bandwidth.

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<v Speaker 3>And this is where Meerkat absolutely excels.

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<v Speaker 2>Okay, break that down for me.

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<v Speaker 3>Well, first, the receivers on these antennas are cryogenically cooled,

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<v Speaker 3>like sub zero cool, very sub zero. This is done

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<v Speaker 3>to reduce the internal thermal noise, literally the random jitter

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<v Speaker 3>of electrons in the electronics to an absolute minimal.

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<v Speaker 4>Got it.

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<v Speaker 2>So the equipment itself is whisper.

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<v Speaker 3>Quiet, right, But the real leap forward is the correlator

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<v Speaker 3>and the bandwidth. Meerkat can digitize and process an enormous

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<v Speaker 3>swath of the radio spectrum simultaneously.

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<v Speaker 2>I really want to focus on the data processing side

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<v Speaker 2>of this, because capturing the deity is only half the battle.

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<v Speaker 3>It's arguably the easier half, honestly, right.

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<v Speaker 2>If meerkat has a massive bandwidth and is incredibly sensitive,

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<v Speaker 2>it means it is picking up everything everything. It's capturing

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<v Speaker 2>the ancient hydroxyl megamaser, sure, but it's also capturing the

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<v Speaker 2>microwave background, the synchrotron radiation from our own galaxy, and

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<v Speaker 2>critically all the terrestrial radio frequency interference, the RFI.

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<v Speaker 3>Bane of radio astronomers everywhere.

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<v Speaker 2>Seriously, we are talking about satellite communications, GPS, cell towers,

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<v Speaker 2>airplane radar. How do you isolate an eight billion year

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<v Speaker 2>old windsbur when you are sitting in the middle of

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<v Speaker 2>a planetary scale rock concert.

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<v Speaker 3>That is the defining challenge of modern radio astronomy. And

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<v Speaker 3>the raw data rate from the meercat correlator is on

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<v Speaker 3>the order of.

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<v Speaker 2>Terabytes parabytes, just constantly flowing in constantly.

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<v Speaker 3>To process this, the data is sent to the inter

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<v Speaker 3>University Institute for Data Intensive Astronomy, or Ida, where high

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<v Speaker 3>performance computing clusters run complex calibration pipelines.

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<v Speaker 2>So if we use late noise canceling headphones as a model,

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<v Speaker 2>is the algorithm basically generating an inverse way of the

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<v Speaker 2>terrestrial noise the satellites, the cell phones and subtracting it

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<v Speaker 2>from the raw feed, leaving only the ancient cosmic whisper.

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<v Speaker 3>That's well, it's closer to the reality of the software

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<v Speaker 3>pipeline than a simple filtering analogy, but it's more complex

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<v Speaker 3>than that. How So, the correlator and the subsequent software

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<v Speaker 3>pipelines have to identify the specific phase and amplitude signatures

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<v Speaker 3>of terrestrial.

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<v Speaker 2>RFI phase and amplitides.

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<v Speaker 3>Because terrestrial sources are very nearby, their wavefronts are curved

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<v Speaker 3>when they hit the array across that eight kilometer distance,

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<v Speaker 3>and they appear localized.

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<v Speaker 2>Ah okay, like ripples in a pond radiating from.

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<v Speaker 4>A rock you just throw exactly.

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<v Speaker 3>Conversely, a plane wave arriving from deep space from eight

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<v Speaker 3>billion light years away hits the array with a completely

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<v Speaker 3>different flat phase signature.

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<v Speaker 2>Because it's traveled so far that the curve has essentially

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<v Speaker 2>flattened out.

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<v Speaker 3>Precisely, the algorithms analyze the data in the time frequency domain,

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<v Speaker 3>searching for spikes in power that violate the expected fringe

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<v Speaker 3>patterns of celestial.

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<v Speaker 2>Source, and then it just flags them, It flags.

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<v Speaker 3>Them or mathematically subtracts that interference. It requires trillions of

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00:16:08.200 --> 00:16:11.360
<v Speaker 3>floating point operations per second just to clean the data

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00:16:11.440 --> 00:16:13.759
<v Speaker 3>before you can even begin to look for the science target.

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<v Speaker 3>It's like a high tech car wash for data, a high.

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00:16:16.360 --> 00:16:21.440
<v Speaker 2>Tech car wash running on supercomputers. That's wild. And the

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00:16:21.480 --> 00:16:25.440
<v Speaker 2>wide bandwidth allowed them to do something unprecedented during this observation. Right,

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00:16:25.720 --> 00:16:28.200
<v Speaker 2>they didn't just find the red shifted hydroxyl line.

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00:16:28.279 --> 00:16:29.279
<v Speaker 4>No, they didn't.

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00:16:29.679 --> 00:16:32.320
<v Speaker 3>Because they were capturing such a massive chunk of the spectrum,

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<v Speaker 3>they simultaneously detected the red shifted neutral hydrogen absorption line.

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<v Speaker 2>Simultaneous detection. Wow.

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00:16:38.519 --> 00:16:41.879
<v Speaker 3>Yes, And the simultaneous detection of both the neutral hydrogen

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00:16:41.960 --> 00:16:46.679
<v Speaker 3>or HI and the hydroxyl OH is a massive observational victory.

347
00:16:46.720 --> 00:16:48.039
<v Speaker 2>Why is it such a big deal.

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00:16:48.200 --> 00:16:51.200
<v Speaker 3>Well, neutral hydrogen emits and absorbs radio waves at a

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<v Speaker 3>resting frequency of fourteen hundred and twenty megahertz. Hydroxyl as

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<v Speaker 3>we discussed as around sixteen sixty five and sixteen sixty

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<v Speaker 3>seven megahertz, right.

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<v Speaker 2>So they are pretty far apart on the dial exactly.

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<v Speaker 3>In older narrowband telescopes, you would have to run a

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<v Speaker 3>dedicated observation tuned to the red shifted HI frequency, and

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00:17:08.640 --> 00:17:12.640
<v Speaker 3>a completely separate observation tuned to the red shifted oage frequency.

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00:17:12.240 --> 00:17:15.200
<v Speaker 2>Which takes twice as long, and the conditions might change.

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00:17:15.279 --> 00:17:19.440
<v Speaker 3>Right, But Meerkat's fractional bandwidth is so wide that both

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00:17:19.440 --> 00:17:23.880
<v Speaker 3>of these vastly separated, heavily red shifted lines fell perfectly

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00:17:23.960 --> 00:17:25.759
<v Speaker 3>within a single observing window.

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00:17:26.039 --> 00:17:28.279
<v Speaker 2>But why is capturing both of them at the exact

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<v Speaker 2>same time so critical?

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00:17:30.519 --> 00:17:30.599
<v Speaker 1>Like?

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00:17:30.720 --> 00:17:34.079
<v Speaker 2>What does the combination of hydrogen absorption and hydroxyl emission

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00:17:34.400 --> 00:17:36.559
<v Speaker 2>tell us that we couldn't figure out from just one

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00:17:36.640 --> 00:17:37.039
<v Speaker 2>or the other.

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00:17:37.279 --> 00:17:40.559
<v Speaker 3>It breaks the degeneracy of the galaxy's internal kinematics.

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<v Speaker 2>Okay, English, please.

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00:17:41.880 --> 00:17:42.440
<v Speaker 4>Right, sorry.

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<v Speaker 3>The hydroxyl megamaser is an emission line. It is adding

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<v Speaker 3>energy to the spectrum. It tells us where the dense,

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00:17:48.480 --> 00:17:52.440
<v Speaker 3>highly excited molecular gas is, which usually traces the intense

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00:17:52.480 --> 00:17:55.920
<v Speaker 3>starburst regions or the immediate vicinity of the act of

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<v Speaker 3>galactic nucleus.

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<v Speaker 2>So the emission shows us where the fire is exactly.

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<v Speaker 3>Neutral hydrogen, however, was seen.

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<v Speaker 2>In absorption, meaning it's blocking light.

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00:18:03.960 --> 00:18:08.279
<v Speaker 3>Yes, this means there's a massive cloud of cold, unexcited

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00:18:08.319 --> 00:18:11.559
<v Speaker 3>atomic gas sitting in front of the radio continuum source

379
00:18:11.599 --> 00:18:13.960
<v Speaker 3>of the galaxy absorbing the background light.

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00:18:14.200 --> 00:18:16.480
<v Speaker 2>Oh wow, so you have a cold cloud casting a

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00:18:16.519 --> 00:18:18.400
<v Speaker 2>shadow over the glowing core.

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00:18:18.279 --> 00:18:21.400
<v Speaker 3>Spot on and by measuring the Doppler shift of the

383
00:18:21.400 --> 00:18:24.519
<v Speaker 3>emission line against the Doppler shift of the absorption line,

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00:18:24.680 --> 00:18:27.960
<v Speaker 3>astronomers can map the physical geometry of the merger.

385
00:18:28.039 --> 00:18:30.039
<v Speaker 2>Because they can see what parts are moving toward us

386
00:18:30.039 --> 00:18:31.079
<v Speaker 2>in which are moving away.

387
00:18:31.359 --> 00:18:35.319
<v Speaker 3>Yes, they can literally see the cold gas falling inward

388
00:18:35.400 --> 00:18:39.480
<v Speaker 3>toward the core, fueling the massive starburst that is simultaneously

389
00:18:39.519 --> 00:18:40.559
<v Speaker 3>firing off the maser.

390
00:18:40.839 --> 00:18:43.640
<v Speaker 2>So it provides a three dimensional anatomical map of a

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00:18:43.720 --> 00:18:46.240
<v Speaker 2>galaxy in the throes of a catastrophic collision.

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00:18:46.359 --> 00:18:47.400
<v Speaker 4>That's exactly what it does.

393
00:18:47.480 --> 00:18:49.640
<v Speaker 2>That is just phenomenal. But wait, I have to go

394
00:18:49.720 --> 00:18:53.039
<v Speaker 2>back to the five hour thing, because even with cryogenically

395
00:18:53.039 --> 00:18:57.680
<v Speaker 2>cooled receivers, an eight kilometer virtual aperture, and supercomputers running

396
00:18:57.759 --> 00:19:01.559
<v Speaker 2>terabytes of phase referencing algorithms, the math for a five

397
00:19:01.599 --> 00:19:05.000
<v Speaker 2>hour detection of a z equals one megamser still feels

398
00:19:05.039 --> 00:19:05.920
<v Speaker 2>pushed beyond.

399
00:19:05.680 --> 00:19:07.319
<v Speaker 4>The limit your right to be skeptical.

400
00:19:07.480 --> 00:19:10.400
<v Speaker 2>Yeah, the inverse square law is unforgiving. There had to

401
00:19:10.400 --> 00:19:14.440
<v Speaker 2>be an environmental variable, something outside the telescope's hardware, that

402
00:19:14.680 --> 00:19:18.400
<v Speaker 2>amplified the flux density to a detectable threshold in such

403
00:19:18.400 --> 00:19:19.160
<v Speaker 2>a short window.

404
00:19:19.319 --> 00:19:23.480
<v Speaker 3>You are entirely correct. The inherent luminosity of the megamaser

405
00:19:23.799 --> 00:19:27.519
<v Speaker 3>combined with the extreme sensitivity of meerkat would not have

406
00:19:27.559 --> 00:19:30.079
<v Speaker 3>been enough to achieve this detection in five hours.

407
00:19:30.200 --> 00:19:32.400
<v Speaker 2>Huh, I knew it. So what happened?

408
00:19:32.480 --> 00:19:36.440
<v Speaker 3>The observation required a massive multiplier, and nature provided one

409
00:19:36.480 --> 00:19:41.200
<v Speaker 3>through the mechanics of general relativity. The signal was gravitationally lensed.

410
00:19:41.680 --> 00:19:44.559
<v Speaker 2>Gravitational lensing. Okay, this is where we shift from quantum

411
00:19:44.559 --> 00:19:47.759
<v Speaker 2>mechanics to the macrophysics of space time. We do, indeed,

412
00:19:47.839 --> 00:19:51.880
<v Speaker 2>because gravitational lensing fundamentally relies on mass warping the fabric

413
00:19:51.920 --> 00:19:52.559
<v Speaker 2>of the universe.

414
00:19:52.640 --> 00:19:57.079
<v Speaker 3>Right, exactly, according to Einstein's general theory of relativity, mass

415
00:19:57.119 --> 00:20:01.119
<v Speaker 3>dictates how spacetime curves, and spacetime dictates how mass and

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00:20:01.200 --> 00:20:01.880
<v Speaker 3>light moves.

417
00:20:02.039 --> 00:20:02.279
<v Speaker 2>Right.

418
00:20:02.440 --> 00:20:05.160
<v Speaker 3>If you have a massive object like a massive foreground

419
00:20:05.160 --> 00:20:08.920
<v Speaker 3>elliptical or disk galaxy, sitting precisely between Earth and a

420
00:20:09.000 --> 00:20:10.559
<v Speaker 3>distant background source.

421
00:20:10.440 --> 00:20:11.279
<v Speaker 2>It creates a dip.

422
00:20:11.440 --> 00:20:15.160
<v Speaker 3>Yeah, the gravitational field of that foreground galaxy creates a

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00:20:15.240 --> 00:20:18.799
<v Speaker 3>deep potential well in space time. When the radio waves

424
00:20:18.839 --> 00:20:22.960
<v Speaker 3>from our distant megamaser enter that well, their paths are bent.

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00:20:23.039 --> 00:20:25.519
<v Speaker 2>So the light isn't traveling in a straight line anymore.

426
00:20:25.559 --> 00:20:29.599
<v Speaker 2>It's following the geodesic the curve of space time created

427
00:20:29.720 --> 00:20:31.279
<v Speaker 2>by that intervening galaxy.

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00:20:31.440 --> 00:20:35.599
<v Speaker 3>Yes, and the geometric consequence of this bending is magnification.

429
00:20:36.519 --> 00:20:39.920
<v Speaker 3>The gravitational lens takes light rays that would have normally

430
00:20:39.960 --> 00:20:42.880
<v Speaker 3>missed Earth entirely, raysed that we're heading off to empty space,

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00:20:43.279 --> 00:20:45.160
<v Speaker 3>and bends them back toward our line of sight.

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00:20:45.599 --> 00:20:48.279
<v Speaker 2>It literally acts as nature's magnifying glass.

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00:20:48.319 --> 00:20:48.880
<v Speaker 4>It really does.

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00:20:49.079 --> 00:20:51.200
<v Speaker 2>But how do we know for certain that it's lens? Like,

435
00:20:51.200 --> 00:20:54.480
<v Speaker 2>how can astronomers tell the difference between a background galaxy

436
00:20:54.519 --> 00:20:58.240
<v Speaker 2>that is just intrinsically incredibly bright and a fainter galaxy

437
00:20:58.279 --> 00:21:01.240
<v Speaker 2>that just happens to be magnified by a foreground mass.

438
00:21:01.559 --> 00:21:05.200
<v Speaker 3>It leaves a distinct spatial signature. A gravitational lens doesn't

439
00:21:05.240 --> 00:21:07.759
<v Speaker 3>just make the object brighter, It distorts.

440
00:21:07.279 --> 00:21:09.240
<v Speaker 2>Its shape, distorts it how well.

441
00:21:09.640 --> 00:21:12.640
<v Speaker 3>Depending on the exact alignment, the background source could be

442
00:21:12.680 --> 00:21:16.200
<v Speaker 3>split into multiple distinct images, or if the alignment is

443
00:21:16.240 --> 00:21:19.359
<v Speaker 3>nearly perfect. The light is smeared into a complete circle

444
00:21:19.400 --> 00:21:20.799
<v Speaker 3>around the foreground.

445
00:21:20.279 --> 00:21:22.039
<v Speaker 2>Mass oh like an Einstein ring.

446
00:21:22.160 --> 00:21:25.599
<v Speaker 3>Exactly an Einstein ring. While the total flux the amount

447
00:21:25.640 --> 00:21:28.799
<v Speaker 3>of energy we receive is magnified by a specific factor

448
00:21:29.160 --> 00:21:33.359
<v Speaker 3>denoted as my The surface brightness of the source is conserved.

449
00:21:32.920 --> 00:21:34.319
<v Speaker 2>So it just looks bigger on the sky.

450
00:21:34.720 --> 00:21:37.839
<v Speaker 3>Right the lens increases the apparent solid angle of the

451
00:21:37.839 --> 00:21:41.759
<v Speaker 3>source on the sky. The meercat data, combined with multi

452
00:21:41.880 --> 00:21:47.039
<v Speaker 3>wavelength follow up observations, revealed this characteristic spatial distortion, and.

453
00:21:46.960 --> 00:21:50.559
<v Speaker 2>That magnification factor was what finally bumped the signal to

454
00:21:50.640 --> 00:21:52.440
<v Speaker 2>noise ratio over the line.

455
00:21:52.200 --> 00:21:54.400
<v Speaker 3>High enough to bump the signal to noise ratio of

456
00:21:54.440 --> 00:21:57.640
<v Speaker 3>the megamaser over the detection threshold in just five.

457
00:21:57.480 --> 00:22:01.200
<v Speaker 2>Hours, which highlights a fascinating synergy modern astrophysics. I mean,

458
00:22:01.200 --> 00:22:05.359
<v Speaker 2>we build these incredibly sophisticated, computationally heavy innerferometers on Earth,

459
00:22:05.599 --> 00:22:08.359
<v Speaker 2>but their ultimate reach is still dictated by the chaotic

460
00:22:08.519 --> 00:22:10.119
<v Speaker 2>random geometry of the universe.

461
00:22:10.200 --> 00:22:12.240
<v Speaker 4>We are very much at the mercy of the cosmos.

462
00:22:12.480 --> 00:22:15.440
<v Speaker 2>We are using nature's own optics to extend the baseline

463
00:22:15.440 --> 00:22:19.160
<v Speaker 2>of human engineering. It's poetic almost, But I want to

464
00:22:19.200 --> 00:22:22.279
<v Speaker 2>pivot back to the source itself, to the astrophysics of

465
00:22:22.319 --> 00:22:23.400
<v Speaker 2>the merging galaxy.

466
00:22:23.559 --> 00:22:24.400
<v Speaker 4>See you the trime.

467
00:22:24.599 --> 00:22:29.359
<v Speaker 2>Right. We establish that the hydroxyl megamaser requires a massive

468
00:22:29.359 --> 00:22:32.640
<v Speaker 2>injection of infrared energy to pump the molecules, and that

469
00:22:32.720 --> 00:22:36.279
<v Speaker 2>this points to a violent galaxy merger. Let's walk through

470
00:22:36.319 --> 00:22:40.559
<v Speaker 2>the anatomy of that merger. When two galaxies collide, what

471
00:22:40.720 --> 00:22:43.319
<v Speaker 2>is the physical sequence of events that leads to this

472
00:22:43.440 --> 00:22:44.240
<v Speaker 2>extreme state.

473
00:22:44.680 --> 00:22:47.240
<v Speaker 3>Well, the term collision can sometimes be a bit misleading

474
00:22:47.279 --> 00:22:49.200
<v Speaker 3>because galaxies are mostly empty space.

475
00:22:49.640 --> 00:22:52.359
<v Speaker 2>Right, It's not like two brick walls hitting each other exactly.

476
00:22:52.440 --> 00:22:56.559
<v Speaker 3>When two massive galaxies merge, the individual stars almost never collide.

477
00:22:56.559 --> 00:22:59.519
<v Speaker 3>They just pass right by each other. Instead, the dominant

478
00:22:59.519 --> 00:23:01.400
<v Speaker 3>forces are gravitational and.

479
00:23:01.400 --> 00:23:04.559
<v Speaker 2>Hydrodynamic hydrodynamics, so fluid dynamics the gas.

480
00:23:04.920 --> 00:23:07.920
<v Speaker 3>Yes, As the two galaxies approach each other, their mutual

481
00:23:07.920 --> 00:23:12.559
<v Speaker 3>gravitational pull induces massive tidal forces. These forces disrupt the

482
00:23:12.720 --> 00:23:16.079
<v Speaker 3>ordered rotational orbits of the stars and the gas, throwing

483
00:23:16.119 --> 00:23:18.079
<v Speaker 3>off long tidal tales of material.

484
00:23:18.319 --> 00:23:21.359
<v Speaker 2>So the structural integrity of the spiral arms, the disc

485
00:23:21.559 --> 00:23:23.559
<v Speaker 2>everything is completely shredded completely.

486
00:23:23.640 --> 00:23:25.960
<v Speaker 3>It looks like a train wreck. But the most crucial

487
00:23:26.000 --> 00:23:29.440
<v Speaker 3>interaction happens with the interstellar medium, the massive clouds of

488
00:23:29.519 --> 00:23:30.440
<v Speaker 3>gas and dust.

489
00:23:30.759 --> 00:23:34.519
<v Speaker 2>Because, unlike the stars, the gas clouds actually do hit

490
00:23:34.559 --> 00:23:35.599
<v Speaker 2>each other exactly.

491
00:23:36.119 --> 00:23:40.559
<v Speaker 3>These hydrodynamic collisions create massive shock waves that compress the gas,

492
00:23:41.160 --> 00:23:45.079
<v Speaker 3>triggering an explosive wave of star formation across the interacting system.

493
00:23:45.240 --> 00:23:47.960
<v Speaker 2>Heyce the massive infrared heat we talked about earlier.

494
00:23:48.119 --> 00:23:48.319
<v Speaker 4>Right.

495
00:23:48.759 --> 00:23:52.599
<v Speaker 3>Furthermore, the tidal forces strip the gas of its angular momentum.

496
00:23:52.640 --> 00:23:55.240
<v Speaker 2>Wait, sorry, interrupt, but bi angular momentum you mean like

497
00:23:55.279 --> 00:23:57.359
<v Speaker 2>it's rotational spin around the galaxy?

498
00:23:57.519 --> 00:24:01.319
<v Speaker 3>Exactly, Yeah, it's spin. The gas is usually orbiting nicely,

499
00:24:01.400 --> 00:24:04.880
<v Speaker 3>but the collision scrambles that, and without angular momentum to

500
00:24:04.960 --> 00:24:07.960
<v Speaker 3>keep it in orbit, millions of solar masses of gas

501
00:24:08.000 --> 00:24:11.799
<v Speaker 3>suddenly plunged straight down toward the gravitational center of the merging.

502
00:24:11.480 --> 00:24:13.640
<v Speaker 2>System, and sitting in the center of each of those

503
00:24:13.680 --> 00:24:16.160
<v Speaker 2>original galaxies is a supermassive black.

504
00:24:15.960 --> 00:24:19.279
<v Speaker 3>Hole, exactly two of them, now heading toward the same

505
00:24:19.319 --> 00:24:23.039
<v Speaker 3>center point. The sudden influx of gas funnels directly into

506
00:24:23.079 --> 00:24:28.279
<v Speaker 3>the central regions, creating a massive, dense circumnuclear.

507
00:24:27.480 --> 00:24:30.000
<v Speaker 2>Disc, a giant buffet for the black holes.

508
00:24:29.839 --> 00:24:34.200
<v Speaker 3>A very messy buffet. This disc feeds the supermassive black holes,

509
00:24:34.279 --> 00:24:38.640
<v Speaker 3>turning them into highly luminous active galactic nuclei. The intense

510
00:24:38.759 --> 00:24:42.000
<v Speaker 3>radiation from these feeding black holes, combined with the extreme

511
00:24:42.079 --> 00:24:46.079
<v Speaker 3>density of young hot stars in the nuclear region, heats

512
00:24:46.119 --> 00:24:47.559
<v Speaker 3>the surrounding dust cocoon.

513
00:24:47.839 --> 00:24:50.960
<v Speaker 2>And there it is. That's the exact environment, the dense

514
00:24:51.039 --> 00:24:54.920
<v Speaker 2>molecular gas, the intense far infrared radiation field required to

515
00:24:55.000 --> 00:24:56.720
<v Speaker 2>pump the hydroxyl megamaser.

516
00:24:56.880 --> 00:24:58.680
<v Speaker 4>That's it. You've built the laser.

517
00:24:58.480 --> 00:25:01.839
<v Speaker 2>And this massive dust coccroon also explains why radio astronomy

518
00:25:01.880 --> 00:25:04.519
<v Speaker 2>is a necessary tool. Here, doesn't it If you pointed

519
00:25:04.559 --> 00:25:08.160
<v Speaker 2>an optical telescope like Hubble or Web, well, web isn't

520
00:25:08.160 --> 00:25:10.119
<v Speaker 2>the red. But if you used an optical telescope on

521
00:25:10.119 --> 00:25:12.480
<v Speaker 2>this merging system, you wouldn't see the black holes.

522
00:25:12.680 --> 00:25:14.559
<v Speaker 3>You wouldn't even see the peak of the starburst and

523
00:25:14.640 --> 00:25:18.039
<v Speaker 3>optical light. You would just see a dark, obscuring smear

524
00:25:18.079 --> 00:25:19.400
<v Speaker 3>of dust.

525
00:25:19.079 --> 00:25:22.759
<v Speaker 2>Because the optical light, the ultraviolet light from the young stars,

526
00:25:22.880 --> 00:25:26.240
<v Speaker 2>is completely absorbed and scattered by the dust greens.

527
00:25:26.440 --> 00:25:29.880
<v Speaker 3>That is the principle of dust extinction. Optical wavelengths are

528
00:25:29.920 --> 00:25:32.680
<v Speaker 3>similar in size to the dust greens themselves, so they

529
00:25:32.720 --> 00:25:35.279
<v Speaker 3>interact strongly and get absorbed or scattered.

530
00:25:35.400 --> 00:25:37.400
<v Speaker 2>Like trying to drive through a thick fog with your

531
00:25:37.480 --> 00:25:39.960
<v Speaker 2>high beams on, the light just reflects back at you.

532
00:25:40.240 --> 00:25:44.799
<v Speaker 3>Great analogy, But radio waves operating at wavelengths of centimeters

533
00:25:44.839 --> 00:25:48.599
<v Speaker 3>or meters are vastly larger than the dust grains. They

534
00:25:48.640 --> 00:25:51.559
<v Speaker 3>pass through the obscuring torus completely unimpeded.

535
00:25:51.680 --> 00:25:55.559
<v Speaker 2>So the megamaser is a beacon punching directly through the dust.

536
00:25:55.720 --> 00:25:58.240
<v Speaker 3>It allows us to probe the gas kinematics within the

537
00:25:58.279 --> 00:26:01.319
<v Speaker 3>central parseex of the merger, right where the action is.

538
00:26:01.559 --> 00:26:04.519
<v Speaker 2>And what's happening in those central parsex is arguably the

539
00:26:04.559 --> 00:26:08.960
<v Speaker 2>most extreme physics in the universe. We have two supermassive

540
00:26:09.000 --> 00:26:12.480
<v Speaker 2>black holes, each potentially billions of times the mass of

541
00:26:12.480 --> 00:26:14.640
<v Speaker 2>our Sun, that have been dragged to the center of

542
00:26:14.680 --> 00:26:16.759
<v Speaker 2>this newly formed mega galaxy.

543
00:26:16.880 --> 00:26:18.640
<v Speaker 3>It's an unimaginable amount of mass.

544
00:26:18.640 --> 00:26:21.000
<v Speaker 2>Well, what happens to them next? They don't just immediately

545
00:26:21.039 --> 00:26:22.119
<v Speaker 2>fuse together, do they?

546
00:26:22.480 --> 00:26:23.160
<v Speaker 4>No, they don't.

547
00:26:23.519 --> 00:26:26.839
<v Speaker 3>They undergo a complex orbital evolution driven only is something

548
00:26:26.839 --> 00:26:27.920
<v Speaker 3>called dynamical friction.

549
00:26:28.160 --> 00:26:31.319
<v Speaker 2>Dynamical friction, how does friction work in space?

550
00:26:31.519 --> 00:26:34.720
<v Speaker 3>As the two supermassive black holes move through the dense

551
00:26:34.759 --> 00:26:38.400
<v Speaker 3>background of stars and gas in the core, their immense

552
00:26:38.480 --> 00:26:41.359
<v Speaker 3>gravity pulls a wake of material behind.

553
00:26:41.079 --> 00:26:42.920
<v Speaker 2>Them, like a boat moving through water.

554
00:26:43.160 --> 00:26:47.319
<v Speaker 3>Yes, and this wake of material exerts a backward gravitational

555
00:26:47.359 --> 00:26:50.960
<v Speaker 3>pull on the black holes, slowly sapping their orbital energy.

556
00:26:51.279 --> 00:26:53.359
<v Speaker 2>Oh I see, So it acts as a drag force.

557
00:26:53.440 --> 00:26:56.880
<v Speaker 3>Exactly because of this drag, they begin to spiral inward,

558
00:26:57.039 --> 00:27:00.000
<v Speaker 3>forming a binary supermassive black hole system.

559
00:27:00.480 --> 00:27:02.839
<v Speaker 2>This is what we refer to as the final parsec

560
00:27:02.920 --> 00:27:04.440
<v Speaker 2>problem in astrophysics.

561
00:27:04.519 --> 00:27:04.680
<v Speaker 4>Right.

562
00:27:04.799 --> 00:27:07.920
<v Speaker 2>Yes, it is the idea that dynamical friction works really

563
00:27:07.960 --> 00:27:10.640
<v Speaker 2>well at large distances to bring the black holes close together.

564
00:27:10.680 --> 00:27:13.720
<v Speaker 2>But as their orbit shrinks, they eventually scatter all the

565
00:27:13.799 --> 00:27:17.279
<v Speaker 2>nearby stars out of the core like a gravitational slingshot.

566
00:27:17.400 --> 00:27:19.079
<v Speaker 3>Right, they clear out their own neighborhood, and.

567
00:27:19.079 --> 00:27:22.720
<v Speaker 2>Once the stars are gone, the friction stops. So technically,

568
00:27:22.759 --> 00:27:26.000
<v Speaker 2>shouldn't the black holes just orbit each other forever, separated

569
00:27:26.079 --> 00:27:29.039
<v Speaker 2>by about a parsec? Unable to close that final distance,

570
00:27:29.680 --> 00:27:30.079
<v Speaker 2>That was.

571
00:27:30.000 --> 00:27:34.240
<v Speaker 3>A significant theoretical hurdle. For many years, theorists couldn't figure

572
00:27:34.279 --> 00:27:38.160
<v Speaker 3>out how to get them to actually merge. However, systems

573
00:27:38.240 --> 00:27:41.440
<v Speaker 3>like our hydroxyl megamaser provide the solution.

574
00:27:41.759 --> 00:27:42.400
<v Speaker 2>The gas.

575
00:27:42.519 --> 00:27:45.440
<v Speaker 3>The massive influx of gas we discuss the exact same

576
00:27:45.519 --> 00:27:49.279
<v Speaker 3>gas feeding the maser provides the necessary drag. The black

577
00:27:49.279 --> 00:27:53.519
<v Speaker 3>holes embed themselves in a massive viscous gas disc, so.

578
00:27:53.559 --> 00:27:56.839
<v Speaker 2>Even if the stars are gone, the gas is still there, dragging.

579
00:27:56.519 --> 00:27:57.640
<v Speaker 4>Them down exactly.

580
00:27:57.960 --> 00:28:00.680
<v Speaker 3>The torque from this gas disc continues to drain their

581
00:28:00.720 --> 00:28:04.319
<v Speaker 3>angular momentum, allowing them to cross that final parsec.

582
00:28:03.960 --> 00:28:06.559
<v Speaker 2>And as they spiral closer and closer, they enter the

583
00:28:06.599 --> 00:28:09.519
<v Speaker 2>final stage of their evolution, the point where the orbital

584
00:28:09.599 --> 00:28:12.480
<v Speaker 2>velocities reach a significant fraction of the speed of light.

585
00:28:12.599 --> 00:28:15.359
<v Speaker 3>Yes, and that's when things get truly relativistic.

586
00:28:15.480 --> 00:28:17.480
<v Speaker 2>They begin to emit gravitational waves.

587
00:28:17.559 --> 00:28:20.720
<v Speaker 3>The sheer mass and acceleration of the binary system warp

588
00:28:20.759 --> 00:28:24.559
<v Speaker 3>space time so severely that they radiate their orbital energy

589
00:28:24.559 --> 00:28:27.920
<v Speaker 3>away in the form of low frequency nanohertz gravitational waves.

590
00:28:28.039 --> 00:28:30.920
<v Speaker 2>So the mega maser is effectively the precursor signal.

591
00:28:31.200 --> 00:28:36.079
<v Speaker 3>It highlights the dense, gas rich environment that guarantees these

592
00:28:36.079 --> 00:28:39.039
<v Speaker 3>black holes will eventually merge, and when they do, they

593
00:28:39.039 --> 00:28:42.400
<v Speaker 3>will release a cataclysmic burst of gravitational wave energy that

594
00:28:42.480 --> 00:28:44.359
<v Speaker 3>will ripple across the entire universe.

595
00:28:44.680 --> 00:28:47.799
<v Speaker 2>So catching the z equals one mega maser isn't just

596
00:28:47.839 --> 00:28:51.640
<v Speaker 2>about finding a distant molecule. It is about actively mapping

597
00:28:51.720 --> 00:28:56.039
<v Speaker 2>the evolutionary pipeline of supermassive black hole mergers at the

598
00:28:56.039 --> 00:28:57.559
<v Speaker 2>peak of cosmic activity.

599
00:28:57.880 --> 00:28:59.079
<v Speaker 4>That's the real science here.

600
00:28:59.119 --> 00:29:02.079
<v Speaker 2>And because Meerkat proved this can be done rapidly in

601
00:29:02.240 --> 00:29:04.759
<v Speaker 2>just five hours with the aid of a lens, it

602
00:29:04.799 --> 00:29:08.200
<v Speaker 2>really forces a paradigm shift in how we approach observational

603
00:29:08.200 --> 00:29:09.440
<v Speaker 2>astronomy going forward.

604
00:29:09.519 --> 00:29:10.359
<v Speaker 4>It absolutely does.

605
00:29:10.480 --> 00:29:14.160
<v Speaker 2>We are no longer limited to targeted, deeply integrated observations

606
00:29:14.200 --> 00:29:17.240
<v Speaker 2>of single objects over hundreds of hours. We are moving

607
00:29:17.240 --> 00:29:19.599
<v Speaker 2>into the era of massive synoptic surveys.

608
00:29:19.680 --> 00:29:22.200
<v Speaker 3>That is the true legacy of this detection. Meerkat is

609
00:29:22.200 --> 00:29:25.440
<v Speaker 3>a pathfinder. It is a precursor facility for the Square

610
00:29:25.480 --> 00:29:27.759
<v Speaker 3>Kilometer Array or SKA.

611
00:29:27.480 --> 00:29:30.480
<v Speaker 2>Which will be the largest and most sensitive radio observatory

612
00:29:30.480 --> 00:29:31.680
<v Speaker 2>ever constructed.

613
00:29:31.279 --> 00:29:34.279
<v Speaker 3>By a wide margin. The skaa mitarray will be built

614
00:29:34.279 --> 00:29:38.799
<v Speaker 3>in South Africa, integrating the existing Meerkat dishes and adding hundreds.

615
00:29:38.400 --> 00:29:42.200
<v Speaker 2>More, hundreds more. That is going to be a massive footprint.

616
00:29:42.519 --> 00:29:46.839
<v Speaker 3>And meanwhile, the next generation very large array. The NGVLA

617
00:29:47.359 --> 00:29:50.319
<v Speaker 3>is being developed in the US to cover higher frequency ranges.

618
00:29:50.759 --> 00:29:53.720
<v Speaker 2>The leap in sensitivity and baseline coverage with the SKA

619
00:29:53.759 --> 00:29:56.799
<v Speaker 2>will be exponential. I mean, if meerkat can pull a

620
00:29:56.920 --> 00:30:00.839
<v Speaker 2>lensed megamser out of the noise in five hour, what

621
00:30:00.920 --> 00:30:03.960
<v Speaker 2>does the data stream look like when the SKA comes online.

622
00:30:04.000 --> 00:30:07.680
<v Speaker 3>Honestly, the data rate will scale from terabytes to.

623
00:30:07.640 --> 00:30:10.640
<v Speaker 2>Petabytes petabytes, that's a million gigabytes.

624
00:30:10.839 --> 00:30:14.000
<v Speaker 3>The processing requirements will be so immense that the data

625
00:30:14.079 --> 00:30:17.960
<v Speaker 3>cannot be recorded and analyzed later. It physically can't be stored.

626
00:30:18.240 --> 00:30:21.400
<v Speaker 3>It must be processed in real time by dedicated supercomputing

627
00:30:21.440 --> 00:30:22.920
<v Speaker 3>clusters distributed globally.

628
00:30:23.160 --> 00:30:24.839
<v Speaker 2>So the car wash has to run while the car

629
00:30:24.920 --> 00:30:26.519
<v Speaker 2>is driving at one thousand miles an hour.

630
00:30:26.640 --> 00:30:28.960
<v Speaker 3>That's one way to put it. The algorithms we discuss,

631
00:30:29.039 --> 00:30:32.839
<v Speaker 3>the RFI mitigation, the phase referencing, the cross correlation. They

632
00:30:32.839 --> 00:30:36.079
<v Speaker 3>will rely heavily on machine learning to automate the extraction

633
00:30:36.160 --> 00:30:36.720
<v Speaker 3>of signals.

634
00:30:36.839 --> 00:30:38.319
<v Speaker 2>Human eyes won't even be able to look at all

635
00:30:38.359 --> 00:30:38.880
<v Speaker 2>the data.

636
00:30:39.039 --> 00:30:41.720
<v Speaker 3>Never the SKAA will not just find one or two

637
00:30:41.799 --> 00:30:45.319
<v Speaker 3>of these high redshift megamasers. It will conduct blind surveys

638
00:30:45.359 --> 00:30:49.079
<v Speaker 3>of the sky, potentially detecting hundreds or thousands of them.

639
00:30:49.119 --> 00:30:52.400
<v Speaker 2>It will effectively create a statistical map of cosmic violence.

640
00:30:52.680 --> 00:30:55.279
<v Speaker 2>We will be able to trace the exact merger rate

641
00:30:55.400 --> 00:30:58.519
<v Speaker 2>of galaxies, the evolution of gas fractions, and the build

642
00:30:58.599 --> 00:31:01.319
<v Speaker 2>up of supermassive black holes across the entire history of

643
00:31:01.319 --> 00:31:02.240
<v Speaker 2>the universe.

644
00:31:01.839 --> 00:31:04.039
<v Speaker 3>Which writes the missing chapters of our cosmic history.

645
00:31:04.200 --> 00:31:06.960
<v Speaker 2>And the fact that South Africa is driving this, not

646
00:31:07.240 --> 00:31:11.200
<v Speaker 2>just hosting the hardware, but developing the computational infrastructure at

647
00:31:11.200 --> 00:31:14.960
<v Speaker 2>IDEA and leading the data analysis, it really cements the

648
00:31:15.000 --> 00:31:20.079
<v Speaker 2>shift toward a decentralized global approach to massive data intensive astronomy.

649
00:31:20.160 --> 00:31:22.799
<v Speaker 3>It is a critical development for the global scientific community.

650
00:31:23.319 --> 00:31:26.400
<v Speaker 3>The bottleneck in modern astronomy is no longer photon collection.

651
00:31:26.559 --> 00:31:29.440
<v Speaker 3>We know how build big dishes. The bottleneck is data

652
00:31:29.480 --> 00:31:33.920
<v Speaker 3>processing and algorithmic efficiency. The expertise developed to scrub the

653
00:31:34.000 --> 00:31:38.200
<v Speaker 3>Meerkat data and extract this hyper faint hydroxyl line is

654
00:31:38.240 --> 00:31:41.400
<v Speaker 3>exactly the expertise required to operate the next generation of

655
00:31:41.480 --> 00:31:43.079
<v Speaker 3>global megascience projects.

656
00:31:43.279 --> 00:31:46.319
<v Speaker 2>So we are fundamentally changing our relationship with the universe,

657
00:31:46.880 --> 00:31:50.000
<v Speaker 2>moving from an era of taking static pictures to an

658
00:31:50.039 --> 00:31:54.759
<v Speaker 2>era of continuously monitoring the dynamic structural evolution of space

659
00:31:54.799 --> 00:31:56.119
<v Speaker 2>time itself exactly.

660
00:31:56.359 --> 00:31:59.839
<v Speaker 3>It's astronomy in high definition video instead of polaroids.

661
00:32:00.119 --> 00:32:03.119
<v Speaker 2>We have covered immense ground today, We really have. We've

662
00:32:03.119 --> 00:32:06.160
<v Speaker 2>explored how the metric expansion of the universe stretches the

663
00:32:06.160 --> 00:32:09.519
<v Speaker 2>frequency of an eight billion year old signal, allowing us

664
00:32:09.559 --> 00:32:12.680
<v Speaker 2>to peer into the gas rich, violent environments of the

665
00:32:12.720 --> 00:32:17.160
<v Speaker 2>cosmic dawn. We've decoded the quantum mechanics of the hydroxyl.

666
00:32:16.759 --> 00:32:18.880
<v Speaker 3>Radically hyperfine structure.

667
00:32:18.559 --> 00:32:22.720
<v Speaker 2>Right understanding how far infrared radiation pumps the molecules into

668
00:32:22.759 --> 00:32:26.559
<v Speaker 2>a population inversion, setting the stage for a cascading wave

669
00:32:26.599 --> 00:32:30.519
<v Speaker 2>of stimulated microwave emission. We looked at the engineering marvel

670
00:32:30.519 --> 00:32:34.319
<v Speaker 2>of meercat how it uses aperture synthesis and algorithmic phase

671
00:32:34.359 --> 00:32:37.880
<v Speaker 2>referencing to isolate a hyper faint signal from a deluge

672
00:32:37.880 --> 00:32:39.319
<v Speaker 2>of terrestrial noise.

673
00:32:39.160 --> 00:32:43.599
<v Speaker 3>All while capturing both neutral hydrogen absorption and hydroxyl emission simultaneously.

674
00:32:43.880 --> 00:32:47.160
<v Speaker 2>Yes, and we saw how the mass of a foreground

675
00:32:47.240 --> 00:32:50.559
<v Speaker 2>galaxy warped space time to act as a gravitational lens,

676
00:32:50.880 --> 00:32:54.880
<v Speaker 2>boosting the flux density to a detectable level. Finally, we

677
00:32:54.920 --> 00:32:58.000
<v Speaker 2>broke down the astrophysics of the merger itself, how dynamical

678
00:32:58.039 --> 00:33:02.400
<v Speaker 2>friction and massive gas inflows strip angular momentum, feeding the

679
00:33:02.440 --> 00:33:05.680
<v Speaker 2>supermassive black holes and driving them toward an eventual space

680
00:33:05.799 --> 00:33:07.000
<v Speaker 2>time shattering collision.

681
00:33:07.200 --> 00:33:08.359
<v Speaker 4>That sums it up perfectly.

682
00:33:08.559 --> 00:33:12.440
<v Speaker 2>But there is one final, profound implication of all this

683
00:33:12.839 --> 00:33:16.200
<v Speaker 2>that ties the deep past directly to our immediate present.

684
00:33:16.440 --> 00:33:19.759
<v Speaker 2>Oh yeah, we established that the universe at ze equals

685
00:33:19.799 --> 00:33:23.039
<v Speaker 2>one was dominated by these violent mergers, and that the

686
00:33:23.079 --> 00:33:25.960
<v Speaker 2>supermassive black holes at the centers of these merging galaxies

687
00:33:26.279 --> 00:33:30.759
<v Speaker 2>inevitably spiral inward, emitting nanohertz gravitational waves.

688
00:33:30.480 --> 00:33:31.640
<v Speaker 4>Right the precursor signal.

689
00:33:31.759 --> 00:33:34.440
<v Speaker 2>So think about this. If the early universe was literally

690
00:33:34.440 --> 00:33:37.200
<v Speaker 2>filled with countless galaxy collisions just like the one that

691
00:33:37.240 --> 00:33:40.599
<v Speaker 2>fired this megamaser, the gravitational waves from those billions of

692
00:33:40.640 --> 00:33:42.480
<v Speaker 2>mergers didn't just disappear, well.

693
00:33:42.480 --> 00:33:44.200
<v Speaker 4>They didn't. They propagated outward.

694
00:33:44.240 --> 00:33:47.759
<v Speaker 2>Overlapping and interfering with each other across billions of years.

695
00:33:48.119 --> 00:33:50.440
<v Speaker 2>It means that the very fabric of the space time

696
00:33:50.480 --> 00:33:54.000
<v Speaker 2>you were sitting in right now is subtly constantly vibrating

697
00:33:54.039 --> 00:33:58.000
<v Speaker 2>with the ancient unseen echoes of billions of cosmic wars.

698
00:33:58.000 --> 00:33:59.920
<v Speaker 3>A stochastic gravitational wave.

699
00:33:59.680 --> 00:34:02.920
<v Speaker 2>Back exactly a background on hum of cosmic violence that

700
00:34:02.960 --> 00:34:05.359
<v Speaker 2>we are only just now beginning to detect. It is

701
00:34:05.359 --> 00:34:08.079
<v Speaker 2>a sobering reminder that the violent history of the universe

702
00:34:08.159 --> 00:34:10.880
<v Speaker 2>isn't just something we observe through a telescope. It is

703
00:34:10.920 --> 00:34:14.639
<v Speaker 2>the physical foundation of the reality we inhabit. Something to

704
00:34:14.679 --> 00:34:16.199
<v Speaker 2>think about the next time you look up at a

705
00:34:16.280 --> 00:34:17.000
<v Speaker 2>quiet night sky.
