WEBVTT

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<v Speaker 1>Welcome to Bedtime Astronomy. Explore the wonders of the cosmos

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<v Speaker 1>with our soothing Bedtime Astronomy podcast. Each episode offers a

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<v Speaker 1>gentle journey through the stars, planets, and beyond, perfect for

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<v Speaker 1>unwinding after a long day. Let's travel through the mysteries

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<v Speaker 1>of the universe as you drift off into a peaceful

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<v Speaker 1>slumber under the night sky.

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<v Speaker 2>Imagine looking up at the night sky and seeing a

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<v Speaker 2>star just erupt right. For centuries, that's what astronomers saw.

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<v Speaker 2>A nova would flare up, and we'd log it as

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<v Speaker 2>this sudden, intense flash of light would get incredibly bright

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<v Speaker 2>and then, you know, slowly and predictably fade away.

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<v Speaker 3>That was the entire story. A simple impulsive explosion. That

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<v Speaker 3>was the model.

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<v Speaker 2>But the actual moment, the blast itself, the shape of

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<v Speaker 2>it unfolding in real time, that was always hitting from us.

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<v Speaker 2>It was just a frustratingly blurry point of light.

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<v Speaker 3>It was a fundamental imitation. I mean, we could measure

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<v Speaker 3>the total light output perfectly, we could analyze the energy,

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<v Speaker 3>we could clock the timing down to the second, all

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<v Speaker 3>the numbers, all the numbers, but the actual physical movement

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<v Speaker 3>of the material, the way it was flowing, whether there

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<v Speaker 3>were lumps, how things were interacting. That was all just

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<v Speaker 3>an inference. It was a guess based on computer models.

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<v Speaker 2>We just didn't have a telescope big enough to see

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<v Speaker 2>the details exactly.

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<v Speaker 3>We lack the resolving power to confirm the mechanics of

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<v Speaker 3>the detonation itself.

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<v Speaker 2>Well, that era of inference is officially over, and for you,

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<v Speaker 2>the curious learner, our mission today is to get right

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<v Speaker 2>into this extraordinary scientific breakthrough, the first high definition images

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<v Speaker 2>of stellar explosion.

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<v Speaker 3>Yeah, this is huge.

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<v Speaker 2>We're going to break down the recent findings from a

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<v Speaker 2>major study in Nature Astronomy and look at exactly how

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<v Speaker 2>scientists managed to capture these stellar eruptions, these novy in

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<v Speaker 2>really unprecedented details.

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<v Speaker 3>And these images they don't just tweak the old models,

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<v Speaker 3>they completely overturned in the decades old assumption that a

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<v Speaker 3>nova is this single symmetrical puff of material.

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<v Speaker 2>It's not a simple balloon inflating.

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<v Speaker 3>Not at all. We now have visual proof of these

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<v Speaker 3>incredibly complex, non uniform shakes. We're talking multidirectional jets, we're

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<v Speaker 3>talking about dramatically delayed injections. It's a whole new ballgame.

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<v Speaker 2>Okay, let's really unpack this because to appreciate just how

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<v Speaker 2>big of a loop this is, we need to understand

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<v Speaker 2>the baseline. We need to get into the physics of

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<v Speaker 2>what's actually exploding here.

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<v Speaker 3>All right, So we are focusing on nova, and it's

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<v Speaker 3>so important to distinguish a nova from his more famous cousin, the.

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<v Speaker 2>Supernova, right, not the same thing at all, not even close.

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<v Speaker 3>A supernova is the final catastrophic death of a massive star.

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<v Speaker 3>It's a one time event that completely destroys the star.

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<v Speaker 2>The nova, on the other hand, is a cyclical thing.

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<v Speaker 2>It happens on a star that's well, technically it's already dead, right,

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<v Speaker 2>that's the key.

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<v Speaker 3>It's a surface level explosion on a dead star that's

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<v Speaker 3>locked into this fatal cosmic dance with the companion.

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<v Speaker 2>So if the star is already dead, what does that

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<v Speaker 2>actually mean and what kind of dead star are we

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<v Speaker 2>talking about here?

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<v Speaker 3>We're talking about a white dwarf. This is the remnant

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<v Speaker 3>of a star like our own Sun. After it exhausts

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<v Speaker 3>its main nuclear fuel, it sheds its outer layers and

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<v Speaker 3>the core collapses down into this incredibly dense, super hot object.

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<v Speaker 2>So you've got something with the mass of the Sun

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<v Speaker 2>squeeze into the size of what the Earth.

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<v Speaker 3>About the size of the Earth. Yeah, it can have

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<v Speaker 3>up to one point four times the mass of the

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<v Speaker 3>Sun crammed into that tiny volume, and that density, that

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<v Speaker 3>concentration of mass is what gives it this immense gravitational pull.

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<v Speaker 2>And it's not held up by normal pressure like a

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<v Speaker 2>regular star. It's something else, something exotics precisely.

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<v Speaker 3>Its structure is maintained by something called electron degeneracy pressure.

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<v Speaker 3>It's a quantum mechanical effect. The electrons are packed in

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<v Speaker 3>so tightly that they physically resist being compressed any further.

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<v Speaker 2>So it's stable. It's basically an inert stellar core just

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<v Speaker 2>sitting there.

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<v Speaker 3>It is. It's stable and inert, but its immense gravity

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<v Speaker 3>is still very very active, and that's what sets the

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<v Speaker 3>stage to the explosion.

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<v Speaker 2>It needs trigger, and that trigger comes from its let's say,

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<v Speaker 2>unfortunate companion star.

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<v Speaker 3>Exactly. This white dwarf is almost always part of a

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<v Speaker 3>close binary system, and it acts like a cosmic thief,

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<v Speaker 3>just pulling material, mostly hydrogen and helium, off its companion.

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<v Speaker 2>It's literally stealing fuel it is.

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<v Speaker 3>This stolen material forms a turbulent, swirling cloud around the

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<v Speaker 3>white dwarf called an accretion disc, and from there it

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<v Speaker 3>spirals down and piles up, forming this shallow, super dense

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<v Speaker 3>layer on the white dwarf's surface.

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<v Speaker 2>Okay, so you have this dead quantum supported core and

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<v Speaker 2>it's now covered in a fresh layer of highly compressed hydrogen.

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<v Speaker 2>What flips the switch? What turns that into a city

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<v Speaker 2>sized hydrogen bomb.

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<v Speaker 3>Well, this is where the specific physics gets really interesting.

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<v Speaker 3>As that hydrogen layer piles up, the immense gravity from

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<v Speaker 3>the white dwarf creates incredible pressure and heat at the

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<v Speaker 3>bottom of that layer. It's being crushed, crushed, and cooked.

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<v Speaker 3>The white dwarf itself is extremely hot, maybe one hundred

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<v Speaker 3>million kelvin, So the base of this new hydrogen envelope

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<v Speaker 3>heats up very quickly.

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<v Speaker 2>But the core itself isn't doing any hugion anymore. It's

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<v Speaker 2>just a hot rock essentially.

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<v Speaker 3>That's right, The core is inert. But here's the key

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<v Speaker 3>to the explosion. That hydrogen layer is supported by the

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<v Speaker 3>same degeneracy pressure as the core, and degenerate matter has

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<v Speaker 3>this weird property where its temperature can skyrocket without its

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<v Speaker 3>pressure immediately increasing to match.

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<v Speaker 2>So in a normal gas, if you heat it up

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<v Speaker 2>it expands and cools.

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<v Speaker 3>Right, it's a natural thermostet.

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<v Speaker 2>But that doesn't happen here.

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<v Speaker 3>It doesn't happen here. The temperature just keeps climbing and climbing.

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<v Speaker 3>It's a runaway heating process. And when it hits the

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<v Speaker 3>critical threshold some are around ten to twenty million kelvin,

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<v Speaker 3>that hydrogen suddenly ignites.

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<v Speaker 2>And we're not talking about a slow burn.

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<v Speaker 3>Oh no, it's a catastrophic, runaway thermonuclear reaction. The CNO

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<v Speaker 3>cycle carbon nitrogen oxygen fusion kicks in, violently, releasing a

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<v Speaker 3>massive amount of energy that finally overcomes the star's gravity.

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<v Speaker 3>It blasts that entire accumulated layer into space at thousands

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<v Speaker 3>of kilometers per second.

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<v Speaker 2>And that's the flash. That's the nova we see, that's

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<v Speaker 2>the nova.

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<v Speaker 3>The star temporarily brightens by many, many orders of magnitude.

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<v Speaker 2>An incredible blast, and yet for all of history we

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<v Speaker 2>could only interpret it. The material expands so fast that

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<v Speaker 2>even our best single telescopes just saw it as that single, smooth,

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<v Speaker 2>unresolved point of light.

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<v Speaker 3>That was the historical observation challenge. Yeah, because they're so

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<v Speaker 3>far away, even something expanding in say five thousand kilometers

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<v Speaker 3>per second still looks like a tiny, slowly growing blob.

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<v Speaker 3>We knew mass was being ejected, but we couldn't resolve

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<v Speaker 3>the geometry.

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<v Speaker 2>The shape, the direction, whether there were jets or clumps.

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<v Speaker 3>All that was hidden in those crucial first few hours

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<v Speaker 3>and days.

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<v Speaker 2>So because the geometry was hidden, the physics of the

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<v Speaker 2>explosion was well. It was based on the assumption that

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<v Speaker 2>it was symmetrical, right, like a perfectly inflated balloon.

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<v Speaker 3>Exactly, and that created a huge knowledge gap, I mean understanding.

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<v Speaker 3>The geometry is everything because it dictates how the ejected

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<v Speaker 3>material interacts with itself.

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<v Speaker 2>If it's a smooth sphere, the physics is pretty.

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<v Speaker 3>Straight, relatively simple, yes, But if you have multiple outflows

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<v Speaker 3>or lumpy bits or directed jets, then they're going to crash.

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<v Speaker 2>Into each other and that's where things get interesting.

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<v Speaker 3>That's where you get intense shockwaves, and those shockwaves are

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<v Speaker 3>where the highest energy physics, the particle acceleration, takes place.

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<v Speaker 3>Before this study, the true complexity of those shock powered

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<v Speaker 3>processes was a complete mystery. We were modeling simple physics

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<v Speaker 3>because we couldn't see the complex reality.

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<v Speaker 2>So, given this massive barrier, this fundamental limit of distance

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<v Speaker 2>and resolution, what was the breakthrough? How did we finally

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<v Speaker 2>see the physics as it happened.

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<v Speaker 3>The answer is a really advanced technique called long baseline

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<v Speaker 3>optical inoferometry.

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<v Speaker 2>It sounds incredibly complex, but the basic idea is a

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<v Speaker 2>clever way to shoot the system right, to get around

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<v Speaker 2>the problem of building impossibly large telescopes.

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<v Speaker 3>That's a perfect way to describe it. Look, if you

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<v Speaker 3>want higher resolution, the ability to see finer details, you

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<v Speaker 3>just need a bigger mirror, a bigger aperture.

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<v Speaker 2>Building a single mirror beyond what eight or ten meters

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<v Speaker 2>in diameter is just an immense engineering challenge.

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<v Speaker 3>Immensely complex and incredibly expensive. Yeah. So interferometry solves this

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<v Speaker 3>by combining the light waves from multiple physically separate telescopes.

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<v Speaker 2>So instead of one giant, one hundred meters mirror, you

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<v Speaker 2>can have, say, a handful of smaller mirrors spread out

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<v Speaker 2>over one hundred.

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<v Speaker 3>Meters exactly, and the combined system acts as if it

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<v Speaker 3>were a single giant telescope whose diameter is equal to

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<v Speaker 3>the maximum distance between any two of the smaller ones.

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<v Speaker 2>It creates a synthetic aperture.

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<v Speaker 3>That's the term. The resolution you get is dictated by

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<v Speaker 3>that longest baseline, not the size of the individual mirrors,

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<v Speaker 3>and this lets astronomers achieve resolutions equivalent to a mirror

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<v Speaker 3>hundreds of meters across. It's just phenomenal.

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<v Speaker 2>And we should stress this isn't some brand new, untested idea.

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<v Speaker 2>This is the same powerful technique that was crucial for

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<v Speaker 2>the Event Horizon telescope project, the.

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<v Speaker 3>One that gave is the first ever image of a

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<v Speaker 3>black hole shadow.

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<v Speaker 2>Right, So when we're talking about resolving power, this is

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<v Speaker 2>the absolute cutting edge.

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<v Speaker 3>It really is. And the specific facility that pulled off

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<v Speaker 3>this nova breakthrough is the Center for High Angular Resolution Astronomy.

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<v Speaker 3>The Chair Array app in California.

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<v Speaker 2>Tell us about that setup because it's at a really

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<v Speaker 2>historic site, but the tech itself is I mean, it's

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<v Speaker 2>borderline science fiction.

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<v Speaker 3>It's a wonderful marriage of history in the future. The

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<v Speaker 3>Chair Array is at the Mount Wilson Observatory in the

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<v Speaker 3>San Gabriel Mountains, which is famous for Edwin Hubble's work

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<v Speaker 3>discovering the expansion.

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<v Speaker 2>Of the universe, a legendary place in astronomy.

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<v Speaker 3>Absolutely, and the array itself consists of six one meter telescopes.

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<v Speaker 3>These six telescopes are arranged very precisely along three arms

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<v Speaker 3>in a big y shape. The longest distance between any

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<v Speaker 3>two of them is three hundred and thirty meters, so.

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<v Speaker 2>You're getting the resolving power of a three hundred and

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<v Speaker 2>thirty meter telescope. That's just it's mind boggling. But it

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<v Speaker 2>requires this almost impossible feat of engineering. You have to

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<v Speaker 2>get the light from all six separate telescopes to arrive

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<v Speaker 2>at the central lab at the exact same time.

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<v Speaker 3>Down to fractions of a wavelength light.

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<v Speaker 2>How do you even do that?

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<v Speaker 3>That is the core technical challenge. It's called maintaining coherence.

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<v Speaker 3>Light travels at a finite speed, so you have to

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<v Speaker 3>compensate for the different distances. Chera uses these incredibly precise

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<v Speaker 3>systems of movable mirrors on railway tracks. They're called delay lines.

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<v Speaker 2>And they're all inside sealed vacuum pipes right to keep

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<v Speaker 2>the atmosphere from messing.

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<v Speaker 3>With the light correct The light from eachy telescope is

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<v Speaker 3>beamed into these vacuum pipes, and these delay lines physically

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<v Speaker 3>move back and forth, constantly adjusting the path length of

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<v Speaker 3>the light to make sure all six beams are perfectly

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<v Speaker 3>synchronized when they meet and interfere in the central lab.

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<v Speaker 2>The precision must be on the order of nanometers.

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<v Speaker 3>It is. They have to align the light paths with

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<v Speaker 3>unbelievable accuracy to track the interference pattern the fringes and

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<v Speaker 3>build up a coherent image. And it's all happening in

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<v Speaker 3>real time. Because the Earth is rotating, the object is

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<v Speaker 3>moving across the sky, those pathlengths are constantly changing.

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<v Speaker 2>That level of coordination is already a huge feed. But

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<v Speaker 2>for something like a nova, I mean, you can plan

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<v Speaker 2>for years to image a static target like a black hole.

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<v Speaker 2>A nova just appears.

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<v Speaker 3>And that's what makes this so impressive. It requires immense

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<v Speaker 3>operational flexibility. A nova can brighten dramatically in less than

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<v Speaker 3>a day. The team has to be able to drop everything,

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<v Speaker 3>pivot the entire array, all six telescopes, all the optics,

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<v Speaker 3>all the synchronization, and lock onto this new target immediately.

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<v Speaker 2>It's high stakes, rapid response science.

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<v Speaker 3>It really is. But the visual data from Shira, as

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<v Speaker 3>powerful as it was, was only half the picture. They

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<v Speaker 3>used a really smart, complimentary approach to double.

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<v Speaker 2>Check their work, so they weren't just relying on the

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<v Speaker 2>images alone.

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<v Speaker 3>No, the sharp images from the interferometry told them the

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<v Speaker 3>shape and the structure, but they complimented that data with

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<v Speaker 3>spectra gathered from major observatories like Gemini.

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<v Speaker 2>And the spectra that's like the chemical fingerprint of the

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<v Speaker 2>guests exactly.

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<v Speaker 3>Yeah. It tells you it's velocity, its density, it's temperature,

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<v Speaker 3>it's chemical composition, all the physics.

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<v Speaker 2>So you have the geometry from one instrument and the

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<v Speaker 2>physics from another, and you can marry them up.

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<v Speaker 3>And this is where their confidence just soared. The study

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<v Speaker 3>found what they called a powerful one to one confirmation.

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<v Speaker 3>As soon as a new high velocity feature appeared in the.

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<v Speaker 2>Spectra, meaning a burst of fast moving gas or a

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<v Speaker 2>strong collision.

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<v Speaker 3>That spectroscopic signal lined up perfectly with a new structure,

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<v Speaker 3>a new lump or jet that simultaneously appeared in the

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<v Speaker 3>interferometric images.

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<v Speaker 2>That's the smoking gun. It proves you're not just seeing

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<v Speaker 2>some kind of optical artifact, you're visually confirming the physics.

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<v Speaker 3>It validated the entire process. One of the co authors

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<v Speaker 3>called it an extraordinary leap forward, and he's not wrong.

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<v Speaker 3>We are now literally watching the material as it's blasted

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<v Speaker 3>into space and connecting that directly to the physics of

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<v Speaker 3>how it's happening. We've gone from theorizing about how shockwaves

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<v Speaker 3>form to directly observing them form.

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<v Speaker 2>And what that new window immediately showed was that the

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<v Speaker 2>simple spherical model of a nova is well, it's just wrong.

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<v Speaker 3>It's completely insfie.

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<v Speaker 2>The team managed to image two novae that erupted in

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<v Speaker 2>twenty twenty one, and they couldn't have been more different

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<v Speaker 2>from each other. That variability is really the heart of

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<v Speaker 2>this whole discovery.

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<v Speaker 3>Absolutely, the contrast between these two novae, V one seventy

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<v Speaker 3>before hercules and V fourteen oh five cassiopa is the

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<v Speaker 3>direct evidence that's forcing us to rewrite the textbooks. We're

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<v Speaker 3>seeing this incredible variety of ejection pathways.

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<v Speaker 2>Which proves that the final shape isn't just about the

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<v Speaker 2>energy of the blast, right, it.

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<v Speaker 3>Must be highly dependent on other factors, like the white

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<v Speaker 3>dwarf's rotation, or its magnetic field, or the shape of

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<v Speaker 3>the material it's stealing.

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<v Speaker 2>Okay, let's get into the first case, nova V one

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<v Speaker 2>sits seventy four hercules. The sources described this one as

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<v Speaker 2>one of the fastest stellar explosions ever recorded. What do

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<v Speaker 2>we mean by fast.

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<v Speaker 3>We mean blindingly fast. V one cs seventy four hercules

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<v Speaker 3>peaked in brightness and then faded away in just a

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<v Speaker 3>few days, just days, just a few days. A more

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<v Speaker 3>typical nova might take weeks or even months to go

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<v Speaker 3>through its whole cycle. So this rapid elevilution meant that

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<v Speaker 3>the crucial early stages, the initial ejection of material, were

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<v Speaker 3>all compressed into this tiny observational.

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<v Speaker 2>Window, which makes the fact that they caught it with

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<v Speaker 2>Chara even more incredible.

294
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<v Speaker 3>It's a huge achievement. And what they saw in this

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00:14:13.399 --> 00:14:16.879
<v Speaker 3>first couple of days, I mean, the geometry is stunningly asymmetrical,

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<v Speaker 3>not a sphere, not even close to his sphere. The

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00:14:19.960 --> 00:14:22.559
<v Speaker 3>images taken just two point two and three point two

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00:14:22.679 --> 00:14:26.519
<v Speaker 3>days after the explosion revealed the immediate formation of two

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00:14:26.639 --> 00:14:29.240
<v Speaker 3>distinct perpendicular outflows of gas.

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<v Speaker 2>Perpendicular, so not just two jets shooting out from the poles,

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<v Speaker 2>but two sets of jets at right angles to each other.

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00:14:35.879 --> 00:14:38.200
<v Speaker 3>That's what the data shows. We're talking about high speed

303
00:14:38.279 --> 00:14:41.200
<v Speaker 3>jets of material shooting out almost at right angles. It's

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00:14:41.240 --> 00:14:43.639
<v Speaker 3>an incredibly complex shape to form so quickly.

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00:14:43.759 --> 00:14:46.639
<v Speaker 2>That implies the explosion's engine isn't uniform at all. What

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00:14:46.720 --> 00:14:49.960
<v Speaker 2>kind of physics could possibly drive flows like that.

307
00:14:49.960 --> 00:14:53.320
<v Speaker 3>That's the million dollar question now, and it's probably tied

308
00:14:53.360 --> 00:14:57.039
<v Speaker 3>to the system's rotation and magnetic fields. A rapidly spinning

309
00:14:57.080 --> 00:15:00.440
<v Speaker 3>white dwarf can easily form a bipolar outflow, you know,

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<v Speaker 3>two jets shooting from the poles.

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<v Speaker 2>Right, That makes sense the path of least resistance.

312
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<v Speaker 3>But perpendicular flows suggests something even more complex is going on,

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<v Speaker 3>maybe a pre existing structure that the blast is hitting,

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<v Speaker 3>or perhaps a rapidly tumbling or tilted magnetic field that's

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<v Speaker 3>channeling the plasma in multiple directions at once.

316
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<v Speaker 2>So this is direct visual evidence of multiple interacting ejections,

317
00:15:21.759 --> 00:15:23.200
<v Speaker 2>not one single puff.

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<v Speaker 3>That's the takeaway. And what's critical is that this complex

319
00:15:26.720 --> 00:15:30.440
<v Speaker 3>geometry immediately explained the high energy data they were seeing

320
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<v Speaker 3>at the same.

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00:15:30.879 --> 00:15:32.159
<v Speaker 2>Time, the gamma rays.

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00:15:32.279 --> 00:15:35.279
<v Speaker 3>The gamma rays the images from Shara showed these fast

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00:15:35.320 --> 00:15:38.919
<v Speaker 3>moving jets colliding with slower moving gas that was probably

324
00:15:38.960 --> 00:15:42.000
<v Speaker 3>ejected just a little bit earlier. This violent collision is

325
00:15:42.039 --> 00:15:45.279
<v Speaker 3>the perfect setup for generating intense shockwaves, and.

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00:15:45.240 --> 00:15:47.480
<v Speaker 2>We now know those shockwaves are the source of the

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<v Speaker 2>gamma rays that NASA's Fermi Space telescope saw.

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<v Speaker 3>It was direct, irrefutable proof the geometric complexity is driving

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00:15:54.919 --> 00:15:55.960
<v Speaker 3>the high energy physics.

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<v Speaker 2>Okay, so that's one star that just rushed through its

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<v Speaker 2>explosion with this specta tacular jet driven chaos. But then

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<v Speaker 2>we look at the other one, nova V fourteen oh

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00:16:04.879 --> 00:16:07.559
<v Speaker 2>five Cassiopa, and it seems to be operating on a

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00:16:07.600 --> 00:16:08.799
<v Speaker 2>totally different schedule.

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00:16:09.000 --> 00:16:11.879
<v Speaker 3>V fourteen oh five Cassiopa was the polar opposite in

336
00:16:11.960 --> 00:16:15.480
<v Speaker 3>many ways. It evolved much more slowly, which isn't unheard of.

337
00:16:16.159 --> 00:16:20.799
<v Speaker 3>But the central surprise here was a clear, dramatic physical delay.

338
00:16:20.919 --> 00:16:25.000
<v Speaker 3>This nova showed the first clear evidence of a delayed expulsion.

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00:16:24.559 --> 00:16:27.600
<v Speaker 2>A delay. What does that mean? The explosion happened, but

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00:16:27.639 --> 00:16:28.759
<v Speaker 2>the material didn't leave.

341
00:16:29.120 --> 00:16:33.480
<v Speaker 3>Essentially, yes, the star held onto its outer layer's material

342
00:16:33.799 --> 00:16:35.080
<v Speaker 3>for more than fifty days.

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00:16:35.720 --> 00:16:39.240
<v Speaker 2>Fifty so for almost two months. The thermonuclear runaway had

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00:16:39.240 --> 00:16:41.519
<v Speaker 2>already happened on the surface, but the material was just

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00:16:41.720 --> 00:16:42.320
<v Speaker 2>stuck there.

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00:16:42.440 --> 00:16:45.679
<v Speaker 3>That's right. The energy was generated, but the stellar envelope

347
00:16:45.720 --> 00:16:49.080
<v Speaker 3>didn't fully disperse. It was contained somehow.

348
00:16:49.279 --> 00:16:52.240
<v Speaker 2>That's incredible. I mean, the pressure from a runaway thermal

349
00:16:52.279 --> 00:16:56.639
<v Speaker 2>pulse should be enormous and immediate. What could possibly hold

350
00:16:56.720 --> 00:16:58.240
<v Speaker 2>it in for fifty days?

351
00:16:58.440 --> 00:17:02.279
<v Speaker 3>It suggests there was some power full confining mechanism, perhaps

352
00:17:02.279 --> 00:17:05.960
<v Speaker 3>an incredibly strong and compressed magnetic field acting like a

353
00:17:06.000 --> 00:17:10.000
<v Speaker 3>cage trapping the plasma, or maybe an unusually dense initial

354
00:17:10.079 --> 00:17:13.079
<v Speaker 3>envelope that needed a lot more sustained energy to finally

355
00:17:13.119 --> 00:17:14.440
<v Speaker 3>overcome the star's gravity.

356
00:17:14.559 --> 00:17:17.680
<v Speaker 2>Whatever the cause, the consequences when that containment finally failed

357
00:17:17.799 --> 00:17:19.039
<v Speaker 2>must have been spectacular.

358
00:17:19.200 --> 00:17:22.160
<v Speaker 3>They were. When the material was finally expelled after that

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00:17:22.200 --> 00:17:27.279
<v Speaker 3>fifty day confinement, it erupted violently. This triggered new incredibly

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00:17:27.279 --> 00:17:29.960
<v Speaker 3>intense shocks, like a spring that's been compressed for two

361
00:17:30.000 --> 00:17:31.720
<v Speaker 3>months and is suddenly released.

362
00:17:31.839 --> 00:17:34.519
<v Speaker 2>And I'm guessing fermisaw a burst of gamma rays from

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00:17:34.519 --> 00:17:36.400
<v Speaker 2>this one too, a huge.

364
00:17:36.039 --> 00:17:39.559
<v Speaker 3>Burst of gamma rays, Yeah, which provided even more support

365
00:17:39.839 --> 00:17:42.720
<v Speaker 3>for this shock driven model of high energy emission.

366
00:17:42.799 --> 00:17:46.279
<v Speaker 2>So what's fascinating here is the sheer variability. You look

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00:17:46.279 --> 00:17:49.160
<v Speaker 2>at just two events and you get one that's immediate

368
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<v Speaker 2>perpendicular jets and another that's a fifty day magnetic cage scenario.

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00:17:54.000 --> 00:17:57.839
<v Speaker 3>It completely shatters the idea of a standard nova. It

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00:17:57.880 --> 00:18:01.160
<v Speaker 3>tells us that the local environment, the white dwarf's magnetic field,

371
00:18:01.200 --> 00:18:04.279
<v Speaker 3>it's spin, the density of the material, it's stealing all

372
00:18:04.319 --> 00:18:07.240
<v Speaker 3>of that dictates the outcome. The geometry is everything, and

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00:18:07.240 --> 00:18:08.960
<v Speaker 3>the geometry is wildly diverse.

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<v Speaker 2>So we have the visual proof of the geometry, We

375
00:18:11.480 --> 00:18:13.440
<v Speaker 2>have the timeline of the ejection. Now we have to

376
00:18:13.440 --> 00:18:17.680
<v Speaker 2>connect the docks. Why does seeing these structural details, the

377
00:18:17.680 --> 00:18:20.920
<v Speaker 2>perpendicular jets, the fifty day delay, why does that matter

378
00:18:21.000 --> 00:18:24.799
<v Speaker 2>so much to the broader field of high energy astrophysics.

379
00:18:24.039 --> 00:18:26.920
<v Speaker 3>Because it directly solves a major puzzle from the last decade,

380
00:18:26.920 --> 00:18:29.240
<v Speaker 3>which is where are all these high energy gamma rays

381
00:18:29.279 --> 00:18:30.400
<v Speaker 3>in our galaxy coming from?

382
00:18:30.440 --> 00:18:32.400
<v Speaker 2>We knew novae were one of the sources.

383
00:18:32.759 --> 00:18:38.640
<v Speaker 3>Right before Shara, NASA's FIRMI Large Area Telescope had detected

384
00:18:38.799 --> 00:18:42.640
<v Speaker 3>JIV emission that's gig electron BOLG gamma rays from more

385
00:18:42.680 --> 00:18:46.640
<v Speaker 3>than twenty novae. This established them as significant galactic gamma

386
00:18:46.680 --> 00:18:47.400
<v Speaker 3>ray factories.

387
00:18:47.519 --> 00:18:50.359
<v Speaker 2>We knew the factory existed, but we didn't know how

388
00:18:50.400 --> 00:18:53.799
<v Speaker 2>the machinery inside actually worked. We assumed it with shockwaves,

389
00:18:53.960 --> 00:18:55.400
<v Speaker 2>but that was just a theory.

390
00:18:55.519 --> 00:18:57.440
<v Speaker 3>It was a very strong theory, but it was still

391
00:18:57.480 --> 00:19:02.039
<v Speaker 3>a theory. These new images provide the direct proof. They

392
00:19:02.079 --> 00:19:05.000
<v Speaker 3>allow us to definitively tie the gamma rays seen by

393
00:19:05.079 --> 00:19:08.400
<v Speaker 3>Fermi not to the initial flash, but directly to those

394
00:19:08.440 --> 00:19:09.440
<v Speaker 3>colliding outflows.

395
00:19:09.680 --> 00:19:12.559
<v Speaker 2>The visual structures are the engines creating the high energy

396
00:19:12.640 --> 00:19:13.759
<v Speaker 2>radiation precisely.

397
00:19:14.039 --> 00:19:18.000
<v Speaker 3>It's a remarkable piece of validation. If novae were truly spherical,

398
00:19:18.480 --> 00:19:22.480
<v Speaker 3>those shockwaves would dissipate quickly and symmetrically. You probably wouldn't

399
00:19:22.480 --> 00:19:24.640
<v Speaker 3>get such intense gamma rays. It's the fact that the

400
00:19:24.640 --> 00:19:27.839
<v Speaker 3>ejecta are lumpy and messy and colliding that creates the

401
00:19:27.839 --> 00:19:29.759
<v Speaker 3>perfect conditions for particle acceleration.

402
00:19:29.960 --> 00:19:34.160
<v Speaker 2>This elevates novae from just being pretty fireworks in the galaxy.

403
00:19:33.880 --> 00:19:37.599
<v Speaker 3>To being, as the Source Material calls them, laboratories for

404
00:19:37.680 --> 00:19:40.839
<v Speaker 3>extreme physics. This is where we get to study how

405
00:19:40.960 --> 00:19:44.640
<v Speaker 3>energy is transferred in the cosmos in a real world setting.

406
00:19:44.839 --> 00:19:47.759
<v Speaker 2>I love that phrase. Let's dig into that. What do

407
00:19:47.839 --> 00:19:50.519
<v Speaker 2>we mean when we say novae are labs for studying

408
00:19:50.519 --> 00:19:54.319
<v Speaker 2>shock physics and particle acceleration. What's actually happening in those collisions.

409
00:19:54.720 --> 00:19:57.640
<v Speaker 3>We're talking about natural particle accelerators that are far more

410
00:19:57.680 --> 00:20:01.000
<v Speaker 3>powerful than anything we could build on Earth. The shockwaves

411
00:20:01.000 --> 00:20:07.319
<v Speaker 3>from these collisions are incredibly efficient at scooping up charged particles, protons, electrons,

412
00:20:07.720 --> 00:20:10.160
<v Speaker 3>and accelerating them to near the speed of light, and.

413
00:20:10.119 --> 00:20:13.720
<v Speaker 2>This happens through a process called diffusive shock acceleration, or

414
00:20:13.759 --> 00:20:14.880
<v Speaker 2>the Fermi mechanism.

415
00:20:15.119 --> 00:20:18.200
<v Speaker 3>That's the one. The basic idea is that particles get

416
00:20:18.200 --> 00:20:21.000
<v Speaker 3>trapped near the shock front and bounce back and forth

417
00:20:21.039 --> 00:20:24.039
<v Speaker 3>across it repeatedly. It's like a cosmic pinball.

418
00:20:23.640 --> 00:20:25.759
<v Speaker 2>Game, and with each bounce they gain energy.

419
00:20:25.799 --> 00:20:28.519
<v Speaker 3>They get a kick of energy with every single pass,

420
00:20:28.559 --> 00:20:31.720
<v Speaker 3>and they do this over and over rapidly accelerating until

421
00:20:31.720 --> 00:20:34.240
<v Speaker 3>they have enough energy to produce gamma rays, which are

422
00:20:34.279 --> 00:20:35.720
<v Speaker 3>the highest energy form of light.

423
00:20:36.000 --> 00:20:39.079
<v Speaker 2>And because Chara gives us the precise visual of when

424
00:20:39.119 --> 00:20:41.440
<v Speaker 2>the collisions happen and what the shape of the colliding

425
00:20:41.480 --> 00:20:44.480
<v Speaker 2>material is, we can now test our models of that

426
00:20:44.559 --> 00:20:46.960
<v Speaker 2>acceleration process with real data.

427
00:20:47.319 --> 00:20:51.000
<v Speaker 3>That's the key. Before these models were mostly tested in

428
00:20:51.079 --> 00:20:55.000
<v Speaker 3>much bigger and much messier systems like supernova remnants. Nov

429
00:20:55.119 --> 00:20:58.359
<v Speaker 3>are smaller, they happen much more frequently in our own galaxy,

430
00:20:58.400 --> 00:21:02.359
<v Speaker 3>and they evolve faster, which makes them fantastic accessible laboratories.

431
00:21:02.599 --> 00:21:06.720
<v Speaker 2>So this isn't just about understanding one type of stellar explosion.

432
00:21:07.039 --> 00:21:08.599
<v Speaker 2>It's about fundamental physics.

433
00:21:08.799 --> 00:21:11.519
<v Speaker 3>It's about the origin of cosmic rays. It's about how

434
00:21:11.519 --> 00:21:14.720
<v Speaker 3>particles get energized throughout the universe, and it all comes

435
00:21:14.759 --> 00:21:18.359
<v Speaker 3>back to challenging that long held view that nova eruptions

436
00:21:18.400 --> 00:21:21.759
<v Speaker 3>are simple single events. That model is dead.

437
00:21:22.119 --> 00:21:24.440
<v Speaker 2>So if we connect this to the bigger picture, this

438
00:21:24.559 --> 00:21:27.799
<v Speaker 2>means we can finally draw a direct cohesive line all

439
00:21:27.799 --> 00:21:30.400
<v Speaker 2>the way from the nuclear reactions on the star's surface.

440
00:21:30.359 --> 00:21:32.599
<v Speaker 3>The geometry of the material flows that result.

441
00:21:32.400 --> 00:21:34.759
<v Speaker 2>From it, and finally to the high energy gamma rays

442
00:21:34.759 --> 00:21:37.200
<v Speaker 2>that are produced by those flows. It's the whole chain

443
00:21:37.240 --> 00:21:39.039
<v Speaker 2>of events observed from start.

444
00:21:38.799 --> 00:21:42.240
<v Speaker 3>To finish exactly. It's linking the microphysics of the surface

445
00:21:42.480 --> 00:21:45.119
<v Speaker 3>to the macrophysics of the shockwaves and the ultra high

446
00:21:45.240 --> 00:21:48.839
<v Speaker 3>energy output. This reshapes our models of how even relatively

447
00:21:48.880 --> 00:21:53.000
<v Speaker 3>small stellar events like novae contribute to the energetic budget

448
00:21:53.000 --> 00:21:53.839
<v Speaker 3>of the Milky Way.

449
00:21:53.920 --> 00:21:57.720
<v Speaker 2>It's taken hypothesis and turning it into observed, tested reality.

450
00:21:58.400 --> 00:22:00.680
<v Speaker 2>Knowing the gamma rays come from shock is one thing,

451
00:22:00.960 --> 00:22:04.599
<v Speaker 2>but actually seeing the messy jets and delayed explosions that

452
00:22:04.680 --> 00:22:08.039
<v Speaker 2>create those shocks. That's the ultimate confirmation, and.

453
00:22:07.960 --> 00:22:10.559
<v Speaker 3>It means we can start asking much more specific questions.

454
00:22:11.079 --> 00:22:13.559
<v Speaker 3>We can use the geometry to infer things about the

455
00:22:13.599 --> 00:22:17.599
<v Speaker 3>white dwarf's rotation speed, its magnetic field, and the accretion rate,

456
00:22:17.720 --> 00:22:20.440
<v Speaker 3>all of which drive these dramatic and varied explosions.

457
00:22:20.759 --> 00:22:23.559
<v Speaker 2>This has been incredible, going from the weirdness of electron

458
00:22:23.599 --> 00:22:26.559
<v Speaker 2>degeneracy pressure all the way to aligning light beams with

459
00:22:26.599 --> 00:22:29.559
<v Speaker 2>a nanometer precision. We've gone from seeing novae as these

460
00:22:29.599 --> 00:22:33.839
<v Speaker 2>simple flashes to understanding them as these complex, geometrically rich events.

461
00:22:33.960 --> 00:22:37.160
<v Speaker 3>You have the immediate perpendicular jets of V sixteen seventy

462
00:22:37.200 --> 00:22:38.400
<v Speaker 3>four hercules on one.

463
00:22:38.200 --> 00:22:40.839
<v Speaker 2>Hand, and on the other you have the dramatic fifty

464
00:22:40.920 --> 00:22:44.359
<v Speaker 2>day delayed eruption of V fourteen oh five cassiophs, completely

465
00:22:44.400 --> 00:22:45.559
<v Speaker 2>different beasts, and.

466
00:22:45.480 --> 00:22:47.920
<v Speaker 3>We have to remember this is just the beginning. The

467
00:22:48.000 --> 00:22:50.480
<v Speaker 3>lead author of the study set as much the fact

468
00:22:50.519 --> 00:22:53.160
<v Speaker 3>that they found such complex and varied shapes in just

469
00:22:53.200 --> 00:22:57.319
<v Speaker 3>their first two detailed observations suggest the field is wide open.

470
00:22:57.839 --> 00:23:01.359
<v Speaker 2>There's probably a whole zoo of other shapes and behaviors out.

471
00:23:01.200 --> 00:23:05.200
<v Speaker 3>There, a whole zoo. With more observations, scientists can start

472
00:23:05.240 --> 00:23:08.680
<v Speaker 3>answering the really big questions about the diverse ways stars

473
00:23:08.680 --> 00:23:11.480
<v Speaker 3>shed their mass and influence the universe around them.

474
00:23:11.920 --> 00:23:15.279
<v Speaker 2>The era of the unresolved point of light is definitely over.

475
00:23:15.920 --> 00:23:19.319
<v Speaker 2>Novae which we once thought were pretty straightforward, are now

476
00:23:19.359 --> 00:23:22.160
<v Speaker 2>revealed to be so much richer and more fascinating than

477
00:23:22.200 --> 00:23:25.559
<v Speaker 2>we ever imagined, and that fascination really leads us to

478
00:23:25.599 --> 00:23:28.240
<v Speaker 2>our final thought for you with the learner think about it.

479
00:23:28.440 --> 00:23:32.400
<v Speaker 3>We observe two novae, just two, and they displayed wildly

480
00:23:32.440 --> 00:23:36.480
<v Speaker 3>different behaviors. One was fast with perpendicular flows, likely driven

481
00:23:36.519 --> 00:23:38.839
<v Speaker 3>by rotation or magnetism.

482
00:23:38.359 --> 00:23:40.759
<v Speaker 2>And the other was a slow burn a fifty day delay,

483
00:23:40.960 --> 00:23:43.279
<v Speaker 2>probably caused by some kind of magnetic cage.

484
00:23:43.519 --> 00:23:46.039
<v Speaker 3>The fact that you see such extreme variability in a

485
00:23:46.079 --> 00:23:49.839
<v Speaker 3>statistical sample of two will that suggests that the cosmos

486
00:23:49.880 --> 00:23:52.599
<v Speaker 3>is holding a huge number of geometrical surprises for us.

487
00:23:52.880 --> 00:23:55.839
<v Speaker 2>So if the universe showed us two fundamentally different ways

488
00:23:55.839 --> 00:23:58.000
<v Speaker 2>for a star to explode right out of the gate,

489
00:23:58.559 --> 00:24:02.759
<v Speaker 2>what other unexpected scene and maybe even bizarre mechanisms are

490
00:24:02.759 --> 00:24:03.200
<v Speaker 2>out there.

491
00:24:03.359 --> 00:24:09.000
<v Speaker 3>Could we see corkscrewing jets, or episodic stuttering bursts, or

492
00:24:09.039 --> 00:24:12.039
<v Speaker 3>maybe three way collisions from a truly chaotic magnetic field.

493
00:24:12.039 --> 00:24:12.680
<v Speaker 3>We just don't know.

494
00:24:12.839 --> 00:24:16.000
<v Speaker 2>The stellar physics textbooks are clearly due for a major rewrite,

495
00:24:16.279 --> 00:24:18.519
<v Speaker 2>and we'll be watching these guys right alongside the Cheera

496
00:24:18.599 --> 00:24:20.880
<v Speaker 2>team to find out what new chapter they uncover next.

497
00:25:00.279 --> 00:25:11.519
<v Speaker 3>The Nassai
