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>Welcome back everyone. Today, we're diving into something truly immense,

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<v Speaker 2>maybe the biggest emptiest structures we know of the cosmic voids.

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<v Speaker 2>These are just these enormous gaps you see in the

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<v Speaker 2>large scale structure of the universe, the places where gravity

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<v Speaker 2>seems weakest and almost everything seems to have well cleared out.

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<v Speaker 2>For a long time, people pretty much assumed they were

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<v Speaker 2>just completely empty, you know, huge black nothings like holes

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<v Speaker 2>punched in space. But now we actually have the tools

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<v Speaker 2>the technology to map these things out see how they evolve.

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<v Speaker 2>So our goal today to really dig into the latest

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<v Speaker 2>findings and figure out what's actually in there. If anything,

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<v Speaker 2>We've pulled together the research to give you the clearest

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<v Speaker 2>possible picture of what these unbelievably vast spaces contain. Because

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<v Speaker 2>the answer isn't just nothing. It's more interesting than that.

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<v Speaker 2>The scale, though it's almost impossible to really get your

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<v Speaker 2>head around. We'll try.

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<v Speaker 3>Yeah, that nothing at all idea is the starting point, absolutely,

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<v Speaker 3>and it's true. They are mostly defined by well by

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<v Speaker 3>what's not there, a profound lack of matter. But the

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<v Speaker 3>key thing, the really crucial insight from the material we

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<v Speaker 3>looked at, is that they aren't, you know, totally one

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<v Speaker 3>hundred percent empty, not across their entire colossal volume. Anyway,

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<v Speaker 3>They're definitely the closest thing to a vacuum we have, sure,

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<v Speaker 3>but there's still structure. There's a great analogy that helps.

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<v Speaker 3>I think I mentioned deserts on Earth. Okay, like say

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<v Speaker 3>the empty Quarter in Arabia. It's defined by a lack

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<v Speaker 3>of water, a lack of big life forms. You wouldn't

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<v Speaker 3>call it teeming, right, definitely not, but it's not lifeless.

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<v Speaker 3>There's still stuff there, maybe some deeprooted plants, insects, maybe

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<v Speaker 3>a tiny mammal hanging on. It's incredibly sparse.

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<v Speaker 2>Right, There is life, just very little.

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<v Speaker 3>Of it exactly. The cosmic voids are basically the Universe's

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<v Speaker 3>version of that, the ultimate sparse environment.

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<v Speaker 2>Okay, so let's really get into that sparseness, that scale,

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<v Speaker 2>because I think you're right. You can't grasp how empty

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<v Speaker 2>a void is until you understand how empty the average

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<v Speaker 2>universe is already, which is pretty staggering in itself. We

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<v Speaker 2>need that baseline. So the observable universe, right, this immense

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<v Speaker 2>volume ninety something billion light years across the material we

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<v Speaker 2>have lays out this fantastic thought experiment. Imagine you could

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<v Speaker 2>take absolutely everything in that whole volume, every planet, star, galaxy,

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<v Speaker 2>gas cloud, and crucially all the dark matter, dark energy too,

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<v Speaker 2>all the stuff, all the stuff, and just spread it

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<v Speaker 2>out perfectly, even like cosmic butter, across the.

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<v Speaker 3>Entire universe, right, a uniform smear.

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<v Speaker 2>What density do you end up with?

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<v Speaker 3>And the result is, well, it's mind boggling, really defines

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<v Speaker 3>the emptiness for city. And you end up with an

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<v Speaker 3>average density of roughly get this, Yeah, one single hydrogen

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<v Speaker 3>atom per cubica.

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<v Speaker 2>The one atom in a cubic meter. Just try to

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<v Speaker 2>picture that a cubic meter. That's a pretty big box, right,

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<v Speaker 2>like arms outstretched, wide, high, deep, and inside that entire volume,

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<v Speaker 2>just one solitary, lonely hydrogen atom floating around. That's the

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<v Speaker 2>average density of everything.

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<v Speaker 3>It's almost nothing.

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<v Speaker 2>It's practically nothing. We only think the universe is dense

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<v Speaker 2>because while most of that matter is crammed into tiny

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<v Speaker 2>spots like Earth or the Sun or our galaxy.

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<v Speaker 3>Exactly, gravity pulls it together.

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<v Speaker 2>The air you're breathing right now, the chair you're sitting on,

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<v Speaker 2>that's trillions upon trillions of times denser than that cosmic average.

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<v Speaker 3>It's wild, it is wild. Ye, it's almost impossible to

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<v Speaker 3>visualize that kind of vacuum. I mean, even if you

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<v Speaker 3>took that cubic meter box and sucked all the air out,

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<v Speaker 3>cooled it to absolute zero, it would still be way

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<v Speaker 3>denser than the universe's average. The vastness is just ugh.

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<v Speaker 2>Okay, so that's our baseline, one atom cubic meter on average.

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<v Speaker 2>Now here's where the voids come in and just blow

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<v Speaker 2>that away, because they are way emptier than that already

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<v Speaker 2>incredibly sparse average.

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<v Speaker 3>Right, This is where it gets really interesting. They are

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<v Speaker 3>the emptiest of the empty.

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<v Speaker 2>So how much emptier?

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<v Speaker 3>Well, when scientists model these structures, a typical void, averaging

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<v Speaker 3>its density across its whole span edge to edge, comes

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<v Speaker 3>out at only about one fifth, So twenty percent of

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<v Speaker 3>that average universal density twenty percent.

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<v Speaker 2>Okay, at first that sounds maybe not that much nuss,

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<v Speaker 2>but wait.

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<v Speaker 3>Exactly, but remember what the average was. It was already

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<v Speaker 3>basically zero one atom per cubic meter.

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<v Speaker 2>So twenty percent of almost nothing is even closer to nothing.

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<v Speaker 3>Precisely, if the average universe is one hydrogen atom per

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<v Speaker 3>cubic meter, avoid averages out to only point two hydrogen atoms.

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<v Speaker 2>Per cubic meter zero point two, so less than one

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<v Speaker 2>atom per cubic meter on average inside Avoid.

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<v Speaker 3>Yeah. To put in another way, think about that box again.

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<v Speaker 3>Instead of needing one cubic meter to find on average,

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<v Speaker 3>one atom inside a void, you'd need a volume five

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<v Speaker 3>times bigger five cubic meters, a huge space just to

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<v Speaker 3>find that single, lonely hydrogen atom on average.

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<v Speaker 2>Wow. Okay, that really drives home the scale of the desolation.

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<v Speaker 3>I guess it really does. It fundamentally changes how you

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<v Speaker 3>think about emptiness. And importantly, that twenty percent figure, that's

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<v Speaker 3>itself a bit misleading because it's an average density for

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<v Speaker 3>the entire void, including its edges, its boundaries.

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<v Speaker 2>Yeah, right, and the edges are presumably where they bump

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<v Speaker 2>up against the denser parts of the universe exactly.

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<v Speaker 3>They border the filaments and walls of the cosmic web,

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<v Speaker 3>where there's more matter, So those boundary regions are naturally

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<v Speaker 3>a bit denser relatively speaking, they pull the average up.

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<v Speaker 2>So if you could somehow just measure the very center

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<v Speaker 2>the deep interior, it would.

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<v Speaker 3>Be much much lower than twenty percent of the average density,

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<v Speaker 3>way sparser. The vast majority of a void's volume is

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<v Speaker 3>far emptier than even that zero point two atoms per

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<v Speaker 3>cubic meter suggests.

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<v Speaker 2>Okay, so they're these super vacuums basically, but like you said,

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<v Speaker 2>not totally easier. So what is that remaining trace amount

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<v Speaker 2>of stuff? What contributes to that tiny bit of density.

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<v Speaker 2>Let's move beyond just the numbers. What can we actually

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<v Speaker 2>see or detect in there?

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<v Speaker 3>Right? What are the contents?

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<v Speaker 2>Yeah, our deep galaxy surveys, the ones looking for the

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<v Speaker 2>faintest light over huge distances. They do find things. It's sparse,

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<v Speaker 2>very sparse, but it's specific stuff. We see things like

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<v Speaker 2>dim dwarf galaxies, these little, often kind of raggedy looking

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<v Speaker 2>clumps of stars, galaxies that just didn't have enough material

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<v Speaker 2>nearby to grow big and grand. Like the Milky Way.

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<v Speaker 3>The runs of the galactic litter, basically pretty much.

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<v Speaker 2>And we also detect these incredibly thin, tenuous threads of gas,

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<v Speaker 2>mostly hydrogen, sometimes linking these dwarf galaxies.

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<v Speaker 3>Whispers of matter.

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<v Speaker 2>Yeah, exactly. These are structures that are unbelievably hard to spot.

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<v Speaker 2>They're so dim they push our telescopes right to the limit,

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<v Speaker 2>but they are there. It confirms the voids aren't perfect holes.

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<v Speaker 2>They have some some sparse furniture, maybe mostly near the edges.

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<v Speaker 3>That's the stuff. Yeah, the baryonic matter, as we call it,

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<v Speaker 3>the normal matter, like the dust motes you might see

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<v Speaker 3>floating in a sunbeam in an otherwise empty room. Okay,

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<v Speaker 3>but the picture gets way more complex and honestly more

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<v Speaker 3>fascinating when we factor in the invisible stuff dark matter.

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<v Speaker 2>Ah right, the mysterious scaffolding of the universe. We can't

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<v Speaker 2>see it, but it's what like eighty five percent of

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<v Speaker 2>the matter out there.

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<v Speaker 3>Something like that. Yeah. It's gravity dictates where everything else goes,

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<v Speaker 3>and even though we can't observe it directly, we can

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<v Speaker 3>model its behavior with incredible precision using supercomputers.

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<v Speaker 2>Okay, so what do those simulations show happening inside the voids?

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<v Speaker 2>Is the dark matter just not there, not at all.

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<v Speaker 3>This is what's so cool. The simulations show that the

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<v Speaker 3>voids aren't just smooth, empty holes in the dark matter

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<v Speaker 3>distribution either. They actually contain entire mini cosmic webs made

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<v Speaker 3>of dark matter.

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<v Speaker 2>Mini webs inside the voids, like a ghost structure within

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<v Speaker 2>the emptiness.

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<v Speaker 3>Exactly a ghostly hidden scaffolding. Think of the main cosmic web,

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<v Speaker 3>the big one, like this massive three D spot structure,

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<v Speaker 3>or a network of connected filaments and walls. Okay, yeah,

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<v Speaker 3>the voids are the huge holes in that sponge. But

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<v Speaker 3>the simulations show that even within those giant holes, dark

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<v Speaker 3>matter is still there, just at incredibly low densities, and

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<v Speaker 3>its gravity, even though it's super wank, is still enough

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<v Speaker 3>to pull it into finer, sparser structures.

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<v Speaker 2>So it's like webs within webs.

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<v Speaker 3>Pretty much. The source material we reviewed actually knows this complexity.

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<v Speaker 3>It describes how voids seem to be divided into smaller subvoids,

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<v Speaker 3>and those subvoids might be further divided into sub subvoids,

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<v Speaker 3>all defined by these incredibly faint filments of dark matter. Wow,

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<v Speaker 3>and this structure, this pattern repeating at smaller scales, even

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<v Speaker 3>in the emptiest regions gives it what the researchers call

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<v Speaker 3>a slight fractal character.

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<v Speaker 2>Fractal like those repeating patterns in mathematics.

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<v Speaker 3>Sort of yeah. It means the basic pattern of the

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<v Speaker 3>cosmic web, filaments connecting denser nodes surrounding emptier regions, seems

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<v Speaker 3>to repeat itself even down here at these incredibly low

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<v Speaker 3>densities within the voids themselves. It's a remarkable hint about

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<v Speaker 3>how fundamental that web structure is to the universe's architecture.

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<v Speaker 2>Why is that significant, though? Does it tell something important

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<v Speaker 2>that there's this faint, fractal structure even in the voids.

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<v Speaker 3>I think it does. It shows that gravity dominated by

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<v Speaker 3>dark matter, is always at work shaping things, even where

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<v Speaker 3>there's almost nothing to shape.

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<v Speaker 2>Right, It's not just chaos in there.

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<v Speaker 3>No, That fractal character suggests that even the weakest gravitational

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<v Speaker 3>fields operating over cosmic time still impose order and structure.

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<v Speaker 3>It prevents even the voids from becoming perfectly uniform. It

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<v Speaker 3>shows structure formation is still happening, just incredibly slowly and

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<v Speaker 3>on a tiny scale compared to the main web. It

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<v Speaker 3>tells us the void isn't just a hole. It's an

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<v Speaker 3>integral structured part of the cosmic landscape.

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<v Speaker 2>So the big cosmic web has these holes the voids,

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<v Speaker 2>but the holes themselves have this faint ghost scaffolding inside,

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<v Speaker 2>making even smaller holes within them.

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<v Speaker 3>It's a good way to picture it, and we have

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<v Speaker 3>to keep coming back to those boundaries, those edges we

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<v Speaker 3>talked about, right.

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<v Speaker 2>The reason the average density isn't even.

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<v Speaker 3>Lower exactly that twenty percent average figure relies heavily on

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<v Speaker 3>the material clinging near the void's perimeter. The voids don't

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<v Speaker 3>just stop, they as the source puts it butt up

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<v Speaker 3>against walls and clusters and filaments of the main, denser

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<v Speaker 3>cosmic web.

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<v Speaker 2>It's like the shallow edge of a deep lake. Right.

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<v Speaker 2>The edges make the average depth seem less than it

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<v Speaker 2>is in the middle.

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<v Speaker 3>Perfect analogy. Those boundary regions are by definition less void like.

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<v Speaker 3>They have more dwarf galaxies, more gas, more dark matter

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<v Speaker 3>influence from the nearby structures, so.

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<v Speaker 2>They disproportionately bump up that overall average density figure, masking

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<v Speaker 2>just how profoundly empty the real core of the void is, which.

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<v Speaker 3>Brings us to the next step. Yeah, if we really

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<v Speaker 3>want to talk about true, unadulterated emptiness, cosmic scale loneliness.

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<v Speaker 3>We have to mentally zoom past those edges, past the

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<v Speaker 3>dim little galaxies, past those faint gas thres We need

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<v Speaker 3>to go deep into the interior. Okay, we need to

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<v Speaker 3>focus on the deepest, most isolated regions of the void's heartland.

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<v Speaker 2>This is where it gets really extreme, isn't it.

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<v Speaker 3>This is it. These areas millions of light years away

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<v Speaker 3>from any significant structure, any major gravitational pull. This is

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<v Speaker 3>where the sources talk about the truly lifeless portions.

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<v Speaker 2>Existing lifeless in terms of lacking structure, lacking anything pretty much.

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<v Speaker 3>The information uses some really evocative comparisons to places on Earth,

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<v Speaker 3>trying to give us a sense of the desolation.

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<v Speaker 2>Yeah, I saw those places like the Katara Depression and

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<v Speaker 2>the Sahara or the empty Quartered desert or bad Water

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<v Speaker 2>Basin in Death Valley, places known for being about as

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<v Speaker 2>barren and dry as Earth gets.

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<v Speaker 3>Right, trying to anchor this cosmic emptiness to something terrestrial.

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<v Speaker 2>But honestly, even those analogies feel like they fall short,

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<v Speaker 2>massively short.

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<v Speaker 3>Oh, they absolutely do, because when we talk about these

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<v Speaker 3>core void regions, we're not talking about a few hundred

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<v Speaker 3>kilometers of desert. We're talking about volumes of space where

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<v Speaker 3>there's essentially nothing for distances up to millions of light years, millions.

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<v Speaker 2>Of light years, not meters, not kilometers light years, an

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<v Speaker 2>almost unbroken vacuum stretching further than many galaxies are wide.

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<v Speaker 3>It just resets your whole perspective on empty Traveling from

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<v Speaker 3>one random particle, maybe a stray hydgen atam, maybe a

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<v Speaker 3>dark matter particle that happens to be zipping through to

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<v Speaker 3>the next particle, that journey could take longer than it

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<v Speaker 3>takes light to cross entire galaxy clusters.

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<v Speaker 2>Millions of years for light to cross the gap between stray.

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<v Speaker 3>Particles potentially yeah, in those deepest cores.

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<v Speaker 2>So if the density is effectively zero over such huge scales,

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<v Speaker 2>why even call it a void with structure? Why isn't

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<v Speaker 2>it just incredibly empty space? Is there anything physically stopping

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<v Speaker 2>it from being a perfect absolute vacuum.

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<v Speaker 3>That's a really good question. Why isn't it just nothing?

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<v Speaker 3>The reason it's classified as avoid is structural, right, It's

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<v Speaker 3>defined by its location between the denser filaments of the

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<v Speaker 3>cosmic web. It's the space carved out by gravity pulling

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<v Speaker 3>matter away from it.

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<v Speaker 2>Okay, so its existence is defined by what's around.

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<v Speaker 3>It largely yes, and physically, is it a perfect vacuum, No,

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<v Speaker 3>because quantum fluctuations can still in principle create particle antiparticle pairs,

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<v Speaker 3>though they annihilate quickly, and just random chance dictates that

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<v Speaker 3>some particles will eventually pass through any given volume, even

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<v Speaker 3>if incredibly and frequently.

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<v Speaker 2>So not technically one hundred point zero zero percent empty,

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<v Speaker 2>but practically practically.

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<v Speaker 3>It's the closest thing imaginable. And crucially, the dark matter

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<v Speaker 3>simulations back this up. They show this profound level of

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<v Speaker 3>emptiness right in the cores of the voids. The random

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<v Speaker 3>particle presence is so incredibly low. The source material really

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<v Speaker 3>emphasizes this that if you were sitting in one spot

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<v Speaker 3>waiting for say a hydrogen atom or a dark matter

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<v Speaker 3>particle to pass by, you'd have to wait a really

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<v Speaker 3>really long time before the next.

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<v Speaker 2>One really really long time measured in cosmic time scales.

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<v Speaker 3>Problem well, easily, it's a vacuum so profound that meaningful

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<v Speaker 3>particle interactions or collisions just don't happen. It's stillness on

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<v Speaker 3>an unimaginable scale.

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<v Speaker 2>Okay, the sheer depth of emptiness, this near total vacuum

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<v Speaker 2>in the void core. It sets up this incredible thought experiment,

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<v Speaker 2>one that really stood out in the research we looked at.

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<v Speaker 2>It almost bridges physics and well philosophy.

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<v Speaker 3>It really does. It forces you to think about the

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<v Speaker 3>link between the physical structure of the universe, where we

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<v Speaker 3>happen to be located, and what that means for life,

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<v Speaker 3>for knowledge, for civilization itself.

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<v Speaker 2>Right, So let's unpack it. The scenario post is, what

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<v Speaker 2>if what if our solar system, the Sun, Earth, all

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<v Speaker 2>the planets, wasn't where it is now, inside a galaxy,

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<v Speaker 2>inside a filament of the cosmic web. What if somehow

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<v Speaker 2>it was transported deep into the core of one of

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<v Speaker 2>these massive voids, millions of light years from.

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<v Speaker 3>Anything, right plunk down in the middle of that profound emptiness.

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<v Speaker 2>What would that even look like? What would the consequences be?

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<v Speaker 3>Well, the immediate visual impact, according the analysis is just chilling,

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<v Speaker 3>and it dictates everything else. From Earth looking up at

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<v Speaker 3>the night sky, there would be no stars, no stars

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<v Speaker 3>at all, none, absolutely zero. The only things you'd see

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<v Speaker 3>in the sky would be the Sunday obviously, our Moon,

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<v Speaker 3>and the other planets in our own solar system.

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<v Speaker 2>That's it.

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<v Speaker 3>Everything else will be projected against a backdrop of perfect, unending,

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<v Speaker 3>unbroken blackness.

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<v Speaker 2>Wow. Just imagine that, looking up at night and seeing

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<v Speaker 2>nothing but pitch black. Maybe Mars or Jupiter is a

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<v Speaker 2>point of light, but absolutely nothing else forever.

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<v Speaker 3>We totally take the story night sky for granted, don't we.

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<v Speaker 3>It's the constant wallpaper of our existence completely.

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<v Speaker 2>Yeah, but we only see those stars. We only know

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<v Speaker 2>we're in a galaxy because we happen to live in

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<v Speaker 2>a relatively dense neighborhood, a brightly lit street.

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<v Speaker 3>Cosmically speaking, exactly, being in a void changes everything for discovery.

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<v Speaker 3>If you're that civilization on void Earth, the nearest external

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<v Speaker 3>galaxy isn't just far away, it's millions of light years.

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<v Speaker 2>Away, and without any nearby stars galaxies, how would you

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<v Speaker 2>even know it was out there? How would you even

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<v Speaker 2>begin to look?

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<v Speaker 3>That's the challenge. Even if this hypothetical avoid civilization developed

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<v Speaker 3>telescopes just as powerful as ours today. Say they built

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<v Speaker 3>their own version of the James webspased telescope. Okay, that

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<v Speaker 3>nearest galaxy, millions of light years distant, would appear as

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<v Speaker 3>just the source describes it as a faint, dim smudge

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<v Speaker 3>in the extreme distance.

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<v Speaker 2>A smudge, not even a point of light, just a

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<v Speaker 2>barely detectable, fuzzy patch.

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<v Speaker 3>Barely detectable, fainter than the faintest star we could see

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<v Speaker 3>with the naked eye. It would require immense effort, long exposures,

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<v Speaker 3>complex filtering just to confirm it's even there.

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<v Speaker 2>So this leads to a really profound, almost unsettling question,

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<v Speaker 2>doesn't it. If you're that civilization, you look up, you

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<v Speaker 2>see blackness in your local planets, would you ever even

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<v Speaker 2>develop astronomy beyond just mapping your own solar system?

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<v Speaker 3>Would the motivation be there?

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<v Speaker 2>Right? Would you pour resources into building incredibly advanced telescopes

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<v Speaker 2>just to hunt for a single, incredibly faint smudge millions

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<v Speaker 2>of light years away, especially when there's no guarantee you'll

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<v Speaker 2>find anything at all.

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<v Speaker 3>Think about the development of astronomy here on Earth. It

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<v Speaker 3>was driven by observing the patterns of nearby bright objects, stars, planets,

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<v Speaker 3>the Milky Way arching across the sky, that gave us

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<v Speaker 3>data questions, the drive to build better instruments. But in

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<v Speaker 3>the void, in the void, astronomical observation beyond your own

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<v Speaker 3>system would be incredibly tedious, expensive, and give almost no

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<v Speaker 3>immediate payoff the incenting to become cosmologists to study the

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00:17:25.559 --> 00:17:28.720
<v Speaker 3>universe beyond your own backyard, it would be incredibly low.

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<v Speaker 2>The implications are just huge. If you don't see other

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<v Speaker 2>galaxies easily, you have.

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<v Speaker 3>No visible evidence for them.

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<v Speaker 2>You wouldn't see the large scale structure the cosmic web

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<v Speaker 2>because the walls are too far away. You wouldn't have

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<v Speaker 2>easily measurable markers for things like red shift, which is

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<v Speaker 2>how we figured out distances and the expansion of the universe.

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<v Speaker 3>Exactly measuring red shift relies on having lots of galaxies

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<v Speaker 3>at different distances to compare if your nearest neighbor is

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<v Speaker 3>millions of light years off and looks like a smudge,

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<v Speaker 3>good Lucke building a Hubble diagram.

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<v Speaker 2>So they might never discover the expanding universe very likely not.

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<v Speaker 2>They might never conceive of the Big Bang.

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<v Speaker 3>How could they? The evidence would be almost completely hidden

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<v Speaker 3>from them.

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<v Speaker 2>Their entire understanding of physics of reality might be limited

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<v Speaker 2>to just their own star system floating alone in an eternal,

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<v Speaker 2>unchanging darkness.

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<v Speaker 3>Which leads to that ultimate chilling question the source material poses.

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<v Speaker 3>Would they even know that the rest of the universe

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<v Speaker 3>is out there?

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<v Speaker 2>Would they even suspect it, or would they conclude that

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<v Speaker 2>their solar system is the entire universe.

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<v Speaker 3>It's a profound thought. It really makes you realize how

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<v Speaker 3>much of our own scientific understanding are Cosmology. Our physics

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<v Speaker 3>isn't just a result of human ingenuity. It's also heavily

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<v Speaker 3>dependent on our location, our lucky vantage point.

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<v Speaker 2>We're lucky to live in a busy neighborhood.

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<v Speaker 3>We really are. We're lucky to be bathed in the

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<v Speaker 3>light from nearby stars and galaxies, lucky to be close

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<v Speaker 3>enough to the large scale structure that we can actually

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<v Speaker 3>map it out. Our ability to measure things like red

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<v Speaker 3>shift and the Hubble flow is only easy because we

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<v Speaker 3>have thousands millions of galaxies relatively close by to study.

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<v Speaker 2>If those data points were all millions of light years away.

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<v Speaker 3>The task of discovering cosmology would be almost insurmountably difficult,

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<v Speaker 3>maybe impossible.

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<v Speaker 2>It really puts things in perspective. So let's just quickly

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<v Speaker 2>recap the journey we took today. We started by trying

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<v Speaker 2>to grasp the average emptiness of the universe.

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<v Speaker 3>Which is already stunningly empty, about one hydrogen atom per

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<v Speaker 3>cubic meter on average.

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<v Speaker 2>Then we plunged into the voids, finding their average density

381
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<v Speaker 2>is even lower, around twenty percent of that maybe point

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<v Speaker 2>two hydrogen atoms per cubic meter.

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<v Speaker 3>But realizing that number is skewed high by the denser

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<v Speaker 3>edges of the voids.

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<v Speaker 2>Right and from there we went into the true deep core,

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<v Speaker 2>the heart of the void.

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<v Speaker 3>Where the emptiness becomes almost absolute, essentially zero density for

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<v Speaker 3>millions of light years at a stretch broken only by

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<v Speaker 3>the rarest stray particle or the ghost structure of dark matter.

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<v Speaker 2>The main takeaway then, is that voids aren't just holes.

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<v Speaker 2>They're fundamental components of the universe's structure. They define the

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<v Speaker 2>walls and filaments by their very.

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00:20:06.799 --> 00:20:10.559
<v Speaker 3>Absence exactly, and while they aren't technically perfectly empty, they

394
00:20:10.599 --> 00:20:13.640
<v Speaker 3>have those dwarf galaxies, the gas threads, the dark matter

395
00:20:13.680 --> 00:20:16.720
<v Speaker 3>mini webs. The level of sheer desolation in their cores

396
00:20:16.759 --> 00:20:19.319
<v Speaker 3>is a type of vacuum that's genuinely hard for us

397
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<v Speaker 3>living here in our dense galaxy to truly wrap our minds.

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00:20:23.160 --> 00:20:25.960
<v Speaker 2>Around, which loops us right back to that void civilization

399
00:20:26.039 --> 00:20:28.480
<v Speaker 2>thought experiment. Because of the sources we looked at, and

400
00:20:28.599 --> 00:20:30.319
<v Speaker 2>with a really provocative twist on that.

401
00:20:30.319 --> 00:20:32.559
<v Speaker 3>Yeah, turning the question back on ourselves.

402
00:20:32.119 --> 00:20:34.960
<v Speaker 2>If a civilization and avoid might never know the rest

403
00:20:34.960 --> 00:20:37.920
<v Speaker 2>of the universe exists because the evidence is too faint,

404
00:20:38.039 --> 00:20:40.359
<v Speaker 2>too far, well, what might we be missing?

405
00:20:40.599 --> 00:20:44.960
<v Speaker 3>What crucial aspects of reality, What fundamental structures or forces

406
00:20:45.400 --> 00:20:48.960
<v Speaker 3>might be hidden from us simply because of our particular location.

407
00:20:49.240 --> 00:20:50.920
<v Speaker 2>How much of what we think we know about the

408
00:20:50.920 --> 00:20:53.960
<v Speaker 2>cosmos is just down to the good fortune of living

409
00:20:54.000 --> 00:20:57.279
<v Speaker 2>inside a bright, busy galactic filament where certain things are

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00:20:57.279 --> 00:20:57.960
<v Speaker 2>easy to see.

411
00:20:58.160 --> 00:21:00.759
<v Speaker 3>Yeah, it's a humbling thought, isn't it. Are there other

412
00:21:00.880 --> 00:21:05.160
<v Speaker 3>cosmic structures, maybe operating on even larger scales or involving

413
00:21:05.160 --> 00:21:09.359
<v Speaker 3>physics we haven't conceived of, that are currently invisible to

414
00:21:09.440 --> 00:21:11.759
<v Speaker 3>us because we don't have the right perspective or the

415
00:21:11.799 --> 00:21:13.839
<v Speaker 3>signals are too weak from our vantage point?

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00:21:13.880 --> 00:21:17.279
<v Speaker 2>What undiscovered cosmic realities are hiding out there simply because

417
00:21:17.319 --> 00:21:19.240
<v Speaker 2>we're not in the right place or looking in the

418
00:21:19.279 --> 00:21:20.559
<v Speaker 2>right way to see them? Yet?

419
00:21:20.839 --> 00:21:24.079
<v Speaker 3>It really underscores why things like large scale simulations are

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00:21:24.079 --> 00:21:26.640
<v Speaker 3>so vital. They help us model the parts of the

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00:21:26.720 --> 00:21:29.759
<v Speaker 3>universe we can't easily see, like the full extent of

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00:21:29.799 --> 00:21:33.359
<v Speaker 3>the dark matter web and the true structure within these voids.

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00:21:33.359 --> 00:21:37.039
<v Speaker 2>Because we can only directly observe this relatively small, brightly

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00:21:37.079 --> 00:21:40.559
<v Speaker 2>lit fraction of everything from where we sit. The simulations

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<v Speaker 2>help us map the architecture of the whole thing, both

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<v Speaker 2>the crowded places and the vast, profound absences. And understanding

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<v Speaker 2>that absence, the void is just as critical as understanding

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<v Speaker 2>the galaxies themselves. It's all part of the same incredible

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<v Speaker 2>cosmic structure, a structure we're still just beginning to comprehends

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<v Speaker 3>Us
