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>Are we alone? I mean, it's the ultimate cosmic question,

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<v Speaker 2>isn't it. It really drives so much of our science,

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<v Speaker 2>our speculation.

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<v Speaker 3>It absolutely does. And for generations of this search for

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<v Speaker 3>extraterrestrial technological civilizations etcs as we call them, it's been

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<v Speaker 3>fueled by this image of finding something huge.

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<v Speaker 2>Right like beings way way beyond us, cosmic architects, maybe

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<v Speaker 2>galactic empires, wielding you know, unimaginable power, that kind.

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<v Speaker 3>Of thing exactly. That's been the dream. Yet despite all

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<v Speaker 3>our efforts, better telescopes, more sense searches, the universe is

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<v Speaker 3>just quiet, very quiet.

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<v Speaker 2>And that quiet isn't just a letdown. It's a genuine

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<v Speaker 2>scientific puzzle, a big one.

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<v Speaker 3>It truly is one of the most perplexing.

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<v Speaker 2>Really yeah, and that's why we're doing this deep dive today.

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<v Speaker 2>We've got some fascinating sources suggesting a really different take,

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<v Speaker 2>almost well, almost simple.

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<v Speaker 3>A radical idea in its own way.

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<v Speaker 2>Totally. We're going to unpack this concept called radical mundanity.

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<v Speaker 2>The core idea, maybe the reason we haven't found aliens

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<v Speaker 2>isn't because they're super rare or hiding, but because they're

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<v Speaker 2>just well ordinary, Yeah, too mundane for us to notice easily.

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<v Speaker 3>And we're digging into the work of doctor Robin Corbett here.

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<v Speaker 3>His research, it was published on the r arcsoof pre

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<v Speaker 3>print server, offers this theoretical framework. Okay, he basically investigates

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<v Speaker 3>the chances of finding etcs if we assume this mundanity

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<v Speaker 3>idea is correct, and it's vital research because it challenges

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<v Speaker 3>that whole super science bias in SETI.

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<v Speaker 2>Right, it might change what we should even be looking

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<v Speaker 2>for exactly.

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<v Speaker 3>And why we're hearing this cosmic silence.

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<v Speaker 2>So it all comes back that famous question from doctor

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<v Speaker 2>Enrico Fermi way back in nineteen fifty the one we

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<v Speaker 2>still can't answer, where is everybody?

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<v Speaker 3>That question just cuts right to the heart of it,

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<v Speaker 3>doesn't it the Fermi paradox, It really does, and the

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<v Speaker 3>paradox itself it's the stark clash between what we expect

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<v Speaker 3>and what we actually see, or rather, what we don't see.

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<v Speaker 2>The expectation comes from the sheer numbers, right, billions of galaxies,

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<v Speaker 2>billions of stars.

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<v Speaker 3>In each hundreds of billions. Yeah, and we now know

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<v Speaker 3>planets are everywhere, almost every star seems to have them,

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<v Speaker 3>and loads are in that Goldilocks zone, the habitable zone.

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<v Speaker 2>So statistically, even if life is incredibly rare, multiply that

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<v Speaker 2>tiny chance by the gazillions of planets out there.

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<v Speaker 3>You should get a galaxy buzzing with life, and a

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<v Speaker 3>lot of it should be intelligent technological. Given the billions

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<v Speaker 3>of years the universe has been.

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<v Speaker 2>Around, plenty of time for civilizations to pop up, grow,

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<v Speaker 2>maybe even spread out. We should see sign somewhere.

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<v Speaker 3>That's the expectation, but the observation still zero. Absolutely no

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<v Speaker 3>definitive proof, no giant alien constructions, no obvious signals, no

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<v Speaker 3>you know, take me to your leader moments.

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<v Speaker 2>Nothing.

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<v Speaker 3>It's this gap, the high probability versus the stark quiet

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<v Speaker 3>reality that pushes fields like astrobiology, SETI exoplanet science forward.

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<v Speaker 3>We have to figure out why our assumptions don't match

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<v Speaker 3>what we're seeing.

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<v Speaker 2>If that assumption of like cosmic grandeur keeps getting shot down,

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<v Speaker 2>then something fundamental in our thinking must be off.

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<v Speaker 3>And for decades, the answers people came up with for

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<v Speaker 3>the Fermi paradox tended towards while the sources call them

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<v Speaker 3>extreme scenarios.

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<v Speaker 2>Okay, yeah, let's touch on those briefly, because this new

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<v Speaker 2>idea is supposed to replace them, right exactly.

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<v Speaker 3>So, the first big category is that life is just rare,

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<v Speaker 3>or it destroys itself. This often involves the idea of

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<v Speaker 3>the great filter.

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<v Speaker 2>The great filter like some massive hurdle that's almost impossible

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<v Speaker 2>for life to get past.

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<v Speaker 3>Right, And maybe that filter is behind us. Maybe just

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<v Speaker 3>getting life started from non life, or jumping from single

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<v Speaker 3>cells to complex creatures like us, maybe that was the

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<v Speaker 3>incredibly rare event. If so, hey, maybe we're first or

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<v Speaker 3>one of the very few.

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<v Speaker 2>That's the optimistic few sort of. Yeah, But the filter

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<v Speaker 2>could be ahead of us.

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<v Speaker 3>Too, right, that's the more chilling possibility. Maybe civilizations inevitably

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<v Speaker 3>hit a wall, runaway climate change, nuclear war, maybe some

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<v Speaker 3>kind of out of control AI.

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<v Speaker 2>They just snuff themselves out before they can really go interstellar.

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<v Speaker 3>Pretty much in that case, advanced civilizations might exist, but

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<v Speaker 3>they're either incredibly rare or they just don't last very

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<v Speaker 3>long on a cosmic timescale.

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<v Speaker 2>Okay, so that's one set of ideas.

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<v Speaker 3>What else, then you've got explanations where life is common

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<v Speaker 3>but they have reasons to stay quiet. The famous one

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<v Speaker 3>is the dark forest hypothesis.

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<v Speaker 2>Ah, yeah, from science fiction, but scientists discuss it seriously,

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<v Speaker 2>the idea that the universe is dangerous.

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<v Speaker 3>Exactly if resources are limited. Announcing your existence could paint

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<v Speaker 3>a target on your back. Any new kid on the

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<v Speaker 3>block might be seen as a threat by older, more

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<v Speaker 3>established civilizations.

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<v Speaker 2>So they practic is extreme radio silence, stay hidden to survive.

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<v Speaker 3>Right, which implies they also have the tech to detect

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<v Speaker 3>others who aren't being quiet and maybe silence them. It

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<v Speaker 3>suggests a pretty predatory cosmos.

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<v Speaker 2>Yikes. Okay, and the last classic.

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<v Speaker 3>One, the zoo hypothesis. This one's a bit more benign,

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<v Speaker 3>but still requires immense technological superiority.

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<v Speaker 2>They know we're here, but they're just watching, like we're

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<v Speaker 2>a cosmic nature preserve sort of.

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<v Speaker 3>Yeah, they deliberately avoid contact, maybe following some kind of

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<v Speaker 3>prime directive not to interfere with our development.

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<v Speaker 2>But again that implies. They're so advanced they can enforce

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<v Speaker 2>this across huge distances. They're essentially galactic zoo keepers.

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<v Speaker 3>That's the key point. All these traditional explanations. They rely

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<v Speaker 3>on extremes, extreme rarity because of a filter, extreme silence,

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<v Speaker 3>because of danger, extreme power to run a zoo.

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<v Speaker 2>They all assume that if a civilization survives past our stage,

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<v Speaker 2>it becomes some kind of cosmic powerhouse, a super science society,

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<v Speaker 2>as you said precisely.

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<v Speaker 3>But what if that core assumption is wrong. What if

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<v Speaker 3>the choice isn't just between cosmic gods and total emptiness.

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<v Speaker 2>What if most advanced life is well just a bit

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<v Speaker 2>more advanced than us, not godlike at all.

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<v Speaker 3>That's the door radical mundanity opens. But first we need

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<v Speaker 3>a way to measure advancement, right, ye, a scale.

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<v Speaker 2>Right which brings us to Kardashchev.

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<v Speaker 3>Exactly to get away from just philosophical handwaving and talk

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<v Speaker 3>about physics energy. Doctor Corbett's study uses the Kardashev scale.

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<v Speaker 3>It's a classic model from a Soviet astronomer, Nikolai Kardashchev.

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<v Speaker 2>And it basically ranks civilizations by how much energy they

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<v Speaker 2>can use.

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<v Speaker 3>Right, that's the benchmark, that's it purely based on power consumption,

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<v Speaker 3>which is a fundamental constraint. And it's a logarithmic scale, remember.

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<v Speaker 2>Meaning the jumps between levels are enormous. Not just a

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<v Speaker 2>little bit more power, but orders of magnitude.

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<v Speaker 3>More astronomical leaps. So let's start at the bottom room.

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<v Speaker 3>Type I civilization. This is a civilization that controls all

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<v Speaker 3>the energy available on its home planet.

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<v Speaker 2>So we're talking weather control, tapping all gethermal wind, solar,

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<v Speaker 2>maybe advanced fusion power, basically managing the entire planet's energy budget.

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<v Speaker 3>Total planetary energy management. Yeah, something like ten to the

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<v Speaker 3>sixteen watts. Humanity, for context, is still climbing towards that.

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<v Speaker 3>Carl Sagan estimated US around point seven maybe point seventy three.

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<v Speaker 3>Now we're not quite there yet.

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<v Speaker 2>Okay, So Type I is planetary mastery. What's type two?

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<v Speaker 3>Type two civilization, Now you take a colossal jump. This

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<v Speaker 3>civilization harnesses the total energy output of its host star.

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<v Speaker 2>It's entire star like our sun.

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<v Speaker 3>Yep, for a star like our sun, that's about ten

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<v Speaker 3>to the twenty six watts. That's ten billion times more

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<v Speaker 3>energy than a Type I civilization uses. This is where

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<v Speaker 3>you get into proper superscience man.

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<v Speaker 2>The classic image here is the dice in sphere, or

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<v Speaker 2>maybe a dice and swarm. These massive structures built around

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<v Speaker 2>the star to capture all its light and heat.

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<v Speaker 3>That's the theoretical mechanism. Yes, building something on that scale,

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<v Speaker 3>it boggles the mind. Structures bigger than planet's completely enclosing

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<v Speaker 3>a star.

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<v Speaker 2>And the crucial point for detection is they couldn't hide this,

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<v Speaker 2>could they, even if they wanted to.

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<v Speaker 3>That's the argument physics demands that energy conversion creates waste

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<v Speaker 3>heat thermodynamics. Even a super efficient Type two civilization capturing

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<v Speaker 3>nearly all its stars light.

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<v Speaker 2>Would still radiate heat, waste heat exactly.

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<v Speaker 3>So instead of seeing a normal star, we'd see something

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<v Speaker 3>dimmer invisible light, but with this huge unnatural spike in

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<v Speaker 3>the infrared.

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<v Speaker 2>Spectrum, like a giant heat signature where a star should be. Yeah,

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<v Speaker 2>something that screams.

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<v Speaker 3>Artificial, unmistakably artificial, a massive blob of mid infrared radiation.

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<v Speaker 3>If even one Type two civilization existed in our galaxy

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<v Speaker 3>and had been around for a while.

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<v Speaker 2>We should have spotted that heat signature with our infrared

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<v Speaker 2>surveys like Wyser Spitzer.

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<v Speaker 3>We should have the fact that we've found basically no

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<v Speaker 3>really convincing candidates for these megastructures. That is the Fermi

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<v Speaker 3>paradox in action, it deepens the mystery.

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<v Speaker 2>Okay, so Type two is stellar mastery, and then there's

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<v Speaker 2>type three.

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<v Speaker 3>Type three civilization. This is almost abstract. They harness the

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<v Speaker 3>energy of their entire home galaxy.

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<v Speaker 2>The whole galaxy, billions of.

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<v Speaker 3>Stars, billions of stars, galactic overlords. Essentially, if the type

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<v Speaker 3>three existed, it wouldn't just be detectable, the entire galaxy

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<v Speaker 3>would look fundamentally different. Clearly managed or engineers.

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<v Speaker 2>In our galaxy doesn't look like that at.

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<v Speaker 3>All, not even close. So the clear absence of type

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<v Speaker 3>two and type three civilizations is what really forces this rethink.

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<v Speaker 3>If the super powerful aliens aren't there, what's left.

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<v Speaker 2>Which brings us back to this idea mundanity.

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<v Speaker 3>Right, if the extremes, extreme rarity or extreme power don't

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<v Speaker 3>fit the observations, maybe we've been aiming too high, overestimating

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<v Speaker 3>the technological ceiling for most life.

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<v Speaker 2>Okay, let's really unpack this radical mundanity that doctor Corbett proposes.

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<v Speaker 2>This is where it gets really interesting, kind of flips

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<v Speaker 2>the script.

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<v Speaker 3>The basic idea is surprisingly simple maybe the silence is

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<v Speaker 3>explained if the galaxy just contains a modest number of

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<v Speaker 3>technological civilizations, and crucially, their technology level is only modestly

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<v Speaker 3>highhigher than ours, not Type two or three, maybe Type one,

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<v Speaker 3>or just a bit past it like Type one point

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<v Speaker 3>one exactly. Their technological ceiling is just lower than we've

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<v Speaker 3>often assumed. They never reach the star harnessing stage.

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<v Speaker 2>And Corbett breaks this mundanity down into two parts, right,

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<v Speaker 2>two dimensions.

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<v Speaker 3>Yes, two key aspects working together. First is technological mundanity.

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<v Speaker 3>This is about the physical and practical limits.

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<v Speaker 2>So maybe etcs just don't make the breakthroughs needed for

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<v Speaker 2>type two. Or maybe it's just too expensive or resource intensive.

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<v Speaker 3>Precisely, think about building a dice in sphere. The sheer

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<v Speaker 3>amount of material, the energy investment, the logistical nightmare. Maybe

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<v Speaker 3>it's just fundamentally beyond the reach of a civilization confined

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<v Speaker 3>to its home planet's resources, no matter how smart they are.

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<v Speaker 2>So achieving Type I planetary mastery, that's achievable. It solves

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<v Speaker 2>local problems, ensure sustainability on their world.

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<v Speaker 3>Right they survive, they thrive, perhaps become stable. But that

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<v Speaker 3>leap from managing a planet's energy to managing a star's energy.

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<v Speaker 3>Maybe that gap is just too vast.

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<v Speaker 2>Kind of technological cul de sac around TYPEOD.

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<v Speaker 3>That's a good way to put it. Maybe there are

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<v Speaker 3>fundamental physics limitations or material science barriers, or simply the

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<v Speaker 3>economics are astronomical and make it unfeasible. Stellar engineering stay

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<v Speaker 3>science fiction for them, so.

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<v Speaker 2>Their tech would be recognizable to us in principle, clean fusion,

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<v Speaker 2>maybe efficient interplanetary travel within their own system, advanced computing,

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<v Speaker 2>but still planetary.

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<v Speaker 3>And scale exactly, still bound by the resources and energy

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<v Speaker 3>available on one world. And the second dimension is numerical mundanity.

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<v Speaker 3>This is about how many there are, right, The hypothesis

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<v Speaker 3>suggests there just aren't that many etcs out there, not

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<v Speaker 3>millions densely packed, but also not zero, just a modest number, a.

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<v Speaker 2>Handful, dozens, maybe scattered across the huge expanse of the galaxy.

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<v Speaker 3>Something like that. Enough to exist, but few enough and

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<v Speaker 3>far enough apart that the chances of us stumbling across

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<v Speaker 3>them or them finding us become pretty low, especially.

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<v Speaker 2>If they're not building giant, flashy megastructure or shouting with

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<v Speaker 2>powerful beacons.

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<v Speaker 3>That's the key connection. If they're only modestly advanced and

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<v Speaker 3>modestly numerous. We're not looking for cosmic gods beaming signals

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<v Speaker 3>across thousands of light years. We're looking for effectively Type

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<v Speaker 3>I planetary engineers quietly managing their infrastructure.

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<v Speaker 2>It changes the whole search paradigm completely.

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<v Speaker 3>The contrast is stark. We've been searching for galactic scale disruptions,

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<v Speaker 3>signs of super science. Radical mundanity says we should be

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<v Speaker 3>looking for quiet.

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<v Speaker 2>Competence civilizations that are successful, stable, but ultimately limited by

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<v Speaker 2>the physics of distance and energy on a galactic scale.

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<v Speaker 3>They just don't have the capability or perhaps the motivation

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<v Speaker 3>to make a huge cosmic splash.

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<v Speaker 2>Okay, so if we accept this premise modestly advanced, modestly

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<v Speaker 2>numerous to the rough, what does that actually mean for

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<v Speaker 2>their ability to, say, explore the galaxy or for us

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<v Speaker 2>to detect them. It implies constraints absolutely.

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<v Speaker 3>If they're mundane, they're still fundamentally bound by physics and

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<v Speaker 3>resource limitations, much like us. Their ability to act on

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<v Speaker 3>a galactic scale is severely curtailed by their Type I

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<v Speaker 3>maybe type one point one energy budget.

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<v Speaker 2>And these constraints are the reason.

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<v Speaker 3>For this silent precisely, a civilization that hasn't cracked stellar

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<v Speaker 3>level energy, can't easily conquer or communicate across the vast

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<v Speaker 3>interstellar voids.

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<v Speaker 2>Let's break down those constraints. Corvett talks about constraint one

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<v Speaker 2>galactic conquest via robotics, even if they wanted to expand,

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<v Speaker 2>maybe for science or survival.

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<v Speaker 3>The sheer scale of the galaxy is a killer app basically,

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<v Speaker 3>even for a civilization a bit ahead of us, say

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<v Speaker 3>type one point one or one point.

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<v Speaker 2>Two, sending probes out like von Neumann, probes that replicate themselves.

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<v Speaker 3>That's often proposed as a solution to the Fermi paradox.

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<v Speaker 3>Why haven't self replicating probes filled the galaxy? But launching

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<v Speaker 3>and sustaining such a program requires unbelievable amounts of energy

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<v Speaker 3>and resources, far beyond a planetary budget.

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<v Speaker 2>Think about our own Voyager probes, huge effort decades later,

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<v Speaker 2>they've barely left the Solar System in galactic.

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<v Speaker 3>Terms exactly, and talk about maybe sending a probe to

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<v Speaker 3>Alpha Centauri just over four light years away, and the

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<v Speaker 3>engineering challenges are already immense. The energy costs are huge.

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<v Speaker 2>Now scale that up. Trying to explore thousands, maybe millions

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<v Speaker 2>of star systems with robotic.

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<v Speaker 3>Probes, the cumulative energy needed to build them, launch them,

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<v Speaker 3>accelerate them to reasonable speeds, maybe decelerate them, ensure they

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<v Speaker 3>work for centuries or millennia. It just likely exceeds the

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<v Speaker 3>energy income of a planet bound civilization.

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<v Speaker 2>So the sheer vastness of space remains a fundamental barrier.

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<v Speaker 2>Interstellar travel is hard even for them.

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<v Speaker 3>It seems plausible, yes, the logistics, the energy cost. It

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<v Speaker 3>acts like a natural break on galactic expansion for any

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<v Speaker 3>civilization that hasn't achieved type two power levels.

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<v Speaker 2>Okay, so widespread physical travel or colonization is probably out

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<v Speaker 2>for mundane civilizations. What about communication that brings us to

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<v Speaker 2>constraint too high powered beacons?

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<v Speaker 3>Yeah, this is a big one for SETI. For decades,

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<v Speaker 3>the hope was we'd detect a deliberate, powerful signal, a beacon.

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<v Speaker 2>Something designed to be noticed across the galaxy shouting we

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<v Speaker 2>are here, like the Wow signal. Maybe, though that wasn't confirmed, right.

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<v Speaker 3>But think about the energy needed to run such a beacon.

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<v Speaker 3>To make it powerful enough to cross hundreds or thousands

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<v Speaker 3>of light years and still be detectable above the background noise,

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<v Speaker 3>I have to.

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<v Speaker 2>Keep it running for a long time right, millennia, millions

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<v Speaker 2>of years. You don't know when someone might be listening exactly.

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<v Speaker 3>The total energy expenditure would be astronomical. We're talking about

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<v Speaker 3>potentially diverting a significant fraction of a type by civilization's

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<v Speaker 3>entire energy budget just to maintain this speculative shout into

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<v Speaker 3>the void.

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<v Speaker 2>Would a mundane civilization see that as a sensible use

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<v Speaker 2>of resources.

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<v Speaker 3>Probably not. It seems inefficient, wasteful. Even they'd likely have

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<v Speaker 3>very efficient communication within their own solar system, focused laser beams,

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<v Speaker 3>maybe tight microwave links, perhaps even quantum communication if they've

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<v Speaker 3>cracked that stuff.

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<v Speaker 2>That doesn't spray energy wastefully across.

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<v Speaker 3>The galaxy exactly. So, the lack of obvious powerful beacons

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<v Speaker 3>isn't necessarily proof no one's out there. It might just

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<v Speaker 3>be a sign of their well, they're mundanity, their practicality.

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<v Speaker 3>They don't have the energy to spare for galactic vanity projects.

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<v Speaker 2>Okay, So if they're not physically exploring widely and they're

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<v Speaker 2>not shouting with powerful beacons, how could we possibly detect them?

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<v Speaker 2>That leads to constraint three weak techno signatures.

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<v Speaker 3>This is really the crux of it for future searches.

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<v Speaker 3>If mundane etcs exist, the only signs were likely to

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<v Speaker 3>detect are their unintentional signals.

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<v Speaker 2>Their leakage radiation, like the accidental electromagnetic noise from their technology,

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<v Speaker 2>is leaking out into.

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<v Speaker 3>Space precisely the hum of their civilization, Their equivalent of

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<v Speaker 3>our old TV broadcasts, radar signals, maybe planetary defense grids,

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<v Speaker 3>power transmission, whatever em noiser daily lives generate that isn't

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<v Speaker 3>perfectly contained.

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<v Speaker 2>But you mentioned earlier, even our leakage is getting weaker,

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<v Speaker 2>isn't it as technology gets more efficient?

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<v Speaker 3>It is, And that's a critical point in Corvette's argument.

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<v Speaker 3>Are our early radio and TV was broadcast omnidirectionally, very leaky,

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<v Speaker 3>relatively strong signals. But now we use fiber optics, which

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<v Speaker 3>keeps the signal contained. We use focus satellite beams, low power,

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<v Speaker 3>We're moving to spread spectrum techniques.

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<v Speaker 2>Laser comms all much harder to detect from light years.

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<v Speaker 3>Away, much harder so in etc. That's even just say

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<v Speaker 3>a century or two ahead of us. Technologically, they've likely

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<v Speaker 3>already transitioned to these highly efficient, very low leakage methods.

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<v Speaker 2>They've managed your data with incredible sophistication. Maybe using technologies

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00:17:31.920 --> 00:17:33.839
<v Speaker 2>we haven't even thought of yet, But the result is

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<v Speaker 2>less accidental noise escaping.

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<v Speaker 3>Almost certainly, their whisper would be incredibly faint by the

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<v Speaker 3>time it crossed interstellar distances to reach us.

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<v Speaker 2>So detecting that faint leakage that's a whole different ballgame

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<v Speaker 2>compared to searching for a beacon.

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<v Speaker 3>Hugely different. It needs incredibly sensitive instruments, massive collecting areas,

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<v Speaker 3>sophisticated signal processing to dig that tiny artificial noise out

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<v Speaker 3>from the natural cosmic status. And you need to stare

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<v Speaker 3>at individual star systems for a long time.

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<v Speaker 2>So the silence we hear now might not be an

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<v Speaker 2>empty universe. It might just be the sound of our

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<v Speaker 2>own current technological limitations. We can't hear the whispers yet.

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<v Speaker 3>That's the essence of the radical mundanity explanation for the silence.

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<v Speaker 3>It's a problem of signal strength and detection threshold, not

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<v Speaker 3>necessarily absence.

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<v Speaker 2>Okay, So Corbett took this principle, these constraints and use

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<v Speaker 2>them to test the different possibilities for what the galaxy

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<v Speaker 2>might actually look like.

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<v Speaker 3>Right, He set up a kind of logical framework based

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<v Speaker 3>on those two variables. Number of civilizations many are few

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<v Speaker 3>and their tech level high Type three or mundane Type

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<v Speaker 3>I ish. That gives four possible scenarios.

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<v Speaker 2>And by applying the constraints no obvious megastructures, the difficulty

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<v Speaker 2>of beacons, the faintness of leakage, he could basically rule

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<v Speaker 2>out three of them exactly.

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<v Speaker 3>Let's walk through the eliminations. The first two are fairly straightforward,

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<v Speaker 3>based on the lack of super science evidence. Hypothesis one

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<v Speaker 3>many civilizations AMD very high technological level false. If there

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<v Speaker 3>were many Type two or three civilizations, the galaxy would

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<v Speaker 3>be obviously teeming with astro engineering projects and their heat signatures.

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<v Speaker 2>It isn't simple enough. What's next.

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<v Speaker 3>Hypothesis two very few civilizations A and D very high

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<v Speaker 3>technological level also seems false. Even just one or two

375
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<v Speaker 3>Type two civilizations, if they've been around for millions of years,

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<v Speaker 3>should have had enough time and power to become detectable.

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<v Speaker 3>They're waste heat, maybe probes, something should be visible somewhere.

378
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<v Speaker 3>The silence argues against this too, right.

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<v Speaker 2>No supercivilizations, whether common or rare, so the answer must

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<v Speaker 2>lie with mundane technology. But there are two options there.

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<v Speaker 3>Now it gets interesting. Hypothesis three many civilizations A and

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<v Speaker 3>d mundane technological level. Corbett argues this one is also

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<v Speaker 3>likely false.

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<v Speaker 2>Wait, why if they're mundane, they're quiet, But if there

385
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<v Speaker 2>are lots of them, wouldn't the combined whispers add up.

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<v Speaker 2>Wouldn't we eventually detect something just by sheer numbers.

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<v Speaker 3>That's the critical point. If there were truly many, maybe

388
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<v Speaker 3>thousands or millions, scattered through the galaxy, even if each

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<v Speaker 3>one only leaks a tiny bit of radiation, the cumulative

390
00:20:05.440 --> 00:20:10.880
<v Speaker 3>effect becomes significant. Statistically, some should be relatively close by, close.

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<v Speaker 2>Enough for even their faint leakage to be detectable with

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<v Speaker 2>our current or near future capabilities.

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00:20:16.079 --> 00:20:20.000
<v Speaker 3>Plausibly, yes, over the decade SETI has been active. If

394
00:20:20.000 --> 00:20:23.519
<v Speaker 3>the galaxy was densely populated with Type BI civilizations, we

395
00:20:23.599 --> 00:20:27.160
<v Speaker 3>probably should have picked up some persistent, structured, artificial looking

396
00:20:27.200 --> 00:20:30.359
<v Speaker 3>noise by now, even if it was weak. The profound

397
00:20:30.480 --> 00:20:34.359
<v Speaker 3>lack of such signals suggests the population density isn't that high.

398
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<v Speaker 2>So the silence is just because they're individually quiet. It's

399
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<v Speaker 2>also because there aren't that many of them overall.

400
00:20:39.799 --> 00:20:42.920
<v Speaker 3>That's the inference. The lack of any compelling signal, beacon

401
00:20:43.119 --> 00:20:47.160
<v Speaker 3>or lukage forces us away from the many mundane scenario.

402
00:20:46.880 --> 00:20:50.039
<v Speaker 2>Which leaves only one possibility standing in his framework.

403
00:20:49.720 --> 00:20:52.680
<v Speaker 3>The last one. The conclusion that seems to best fit

404
00:20:52.759 --> 00:20:55.480
<v Speaker 3>the observed silence if you accept the premise of mundanity,

405
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<v Speaker 3>is very few civilizations with mundane technological level.

406
00:21:00.000 --> 00:21:03.480
<v Speaker 2>Okay, so that's the synthesis of radical mundanity. Not empty,

407
00:21:03.640 --> 00:21:08.359
<v Speaker 2>not teeming with gods, but yeah, sparsely populated, with civilizations

408
00:21:08.440 --> 00:21:10.960
<v Speaker 2>kind of like us, just maybe a bit further down the.

409
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<v Speaker 3>Road, exactly a modest number scattered across the vastness. They're successful,

410
00:21:15.720 --> 00:21:18.960
<v Speaker 3>they made it past whatever filters lead to technology, but

411
00:21:19.039 --> 00:21:23.279
<v Speaker 3>they are fundamentally constrained by planetary resources and energy. They're

412
00:21:23.319 --> 00:21:26.960
<v Speaker 3>not cosmic architects. Their type I maybe type one point

413
00:21:27.000 --> 00:21:30.880
<v Speaker 3>one engineers grappling with the same issues of interstellar distance

414
00:21:30.920 --> 00:21:32.200
<v Speaker 3>and energy costs.

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00:21:31.920 --> 00:21:35.000
<v Speaker 2>That we are, and that explains the silence. They lack

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00:21:35.039 --> 00:21:38.640
<v Speaker 2>the sheer power to make obvious signals or structures, and

417
00:21:38.680 --> 00:21:41.759
<v Speaker 2>there aren't enough of them for their combined faint leakage

418
00:21:41.960 --> 00:21:43.519
<v Speaker 2>to be easily detectable by us.

419
00:21:43.599 --> 00:21:47.359
<v Speaker 3>Yet it resolves the Fermi paradox quite elegantly, really, without

420
00:21:47.400 --> 00:21:51.200
<v Speaker 3>needing galaxy wide catastrophes or hidden watchers it's an explanation

421
00:21:51.279 --> 00:21:54.119
<v Speaker 3>rooted in plausible physical and economic limits.

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<v Speaker 2>And the big takeaway, maybe the most important part, is

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<v Speaker 2>that it doesn't mean we're alone.

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<v Speaker 3>Not at all. It actually makes detection seem well, not imminent,

425
00:22:03.279 --> 00:22:07.279
<v Speaker 3>but potentially achievable. It's just incredibly difficult. We're not looking

426
00:22:07.279 --> 00:22:10.440
<v Speaker 3>for a foghorn, We're listening for a pin drop miles

427
00:22:10.480 --> 00:22:12.359
<v Speaker 3>away in a noisy room.

428
00:22:12.559 --> 00:22:15.160
<v Speaker 2>The neighbors are home, they're just not having a loud party.

429
00:22:15.160 --> 00:22:16.839
<v Speaker 2>They're quietly managing their household.

430
00:22:16.960 --> 00:22:17.880
<v Speaker 3>That's a great analogy.

431
00:22:17.960 --> 00:22:21.559
<v Speaker 2>Yeah, So this shift in perspective that doctor Corbett offers,

432
00:22:21.599 --> 00:22:25.119
<v Speaker 2>it's pretty fundamental. It suggests the reason for the paradox

433
00:22:25.200 --> 00:22:30.799
<v Speaker 2>isn't some grand, terrifying cosmic drama, but maybe just a

434
00:22:30.920 --> 00:22:33.079
<v Speaker 2>lack of cosmic extravagance exactly.

435
00:22:33.160 --> 00:22:35.880
<v Speaker 3>The universe might be less like Star Wars with galaxy

436
00:22:35.920 --> 00:22:39.839
<v Speaker 3>spanning empires, and more well just big and mostly empty,

437
00:22:40.160 --> 00:22:44.759
<v Speaker 3>with occasional pockets of quiet, competent planet bound life. Less

438
00:22:44.839 --> 00:22:47.759
<v Speaker 3>terrifying perhaps, but maybe more constrained.

439
00:22:47.960 --> 00:22:50.119
<v Speaker 2>And if this whole radical mondanity idea is on the

440
00:22:50.200 --> 00:22:52.799
<v Speaker 2>right track, it has huge implications for how we actually

441
00:22:52.880 --> 00:22:54.119
<v Speaker 2>do set how we search.

442
00:22:54.400 --> 00:22:58.440
<v Speaker 3>Absolutely massive implications. It means we should probably deprioritize searching

443
00:22:58.440 --> 00:23:01.440
<v Speaker 3>for those super powerful obvious beacons or giant dice In's

444
00:23:01.480 --> 00:23:04.720
<v Speaker 3>fear heat signatures. They might simply not exist in large numbers,

445
00:23:04.759 --> 00:23:05.519
<v Speaker 3>if at all.

446
00:23:05.519 --> 00:23:09.160
<v Speaker 2>Instead, the focus has to shift entirely to detecting that

447
00:23:09.480 --> 00:23:11.759
<v Speaker 2>faint incidental leakage radiation.

448
00:23:11.759 --> 00:23:14.680
<v Speaker 3>That becomes the prime target. The search needs to become

449
00:23:14.680 --> 00:23:18.079
<v Speaker 3>more surgical, more patient. We need extreme sensitivity and the

450
00:23:18.119 --> 00:23:21.960
<v Speaker 3>ability to filter out natural noise sources very effectively, and.

451
00:23:22.000 --> 00:23:24.960
<v Speaker 2>Corvid's study actually suggests this might be within reach.

452
00:23:25.079 --> 00:23:28.359
<v Speaker 3>Historically speaking, it does offer that optimistic note for perhaps

453
00:23:28.440 --> 00:23:31.839
<v Speaker 3>the first time. He argues detecting this faint leakage might

454
00:23:31.880 --> 00:23:35.000
<v Speaker 3>not be centuries away, but it requires the next generation

455
00:23:35.079 --> 00:23:35.759
<v Speaker 3>of instruments.

456
00:23:35.960 --> 00:23:40.119
<v Speaker 2>He mentions this square kilometer array SKA specifically, right that

457
00:23:40.240 --> 00:23:42.920
<v Speaker 2>huge radio telescope project being built now.

458
00:23:43.079 --> 00:23:46.200
<v Speaker 3>Yes, the SKA, or potentially the generation of telescopes that

459
00:23:46.240 --> 00:23:46.880
<v Speaker 3>comes after it.

460
00:23:47.000 --> 00:23:50.319
<v Speaker 2>Why is the SKA so suited for this mundane search.

461
00:23:50.519 --> 00:23:53.519
<v Speaker 3>Because its design goals are exactly what's needed. It's aiming

462
00:23:53.559 --> 00:23:56.839
<v Speaker 3>to be the most sensitive radio telescope ever constructed, with

463
00:23:56.920 --> 00:24:00.279
<v Speaker 3>an enormous collecting area spread over huge distance.

464
00:24:00.480 --> 00:24:02.680
<v Speaker 2>So it can pick up incredibly faint signals.

465
00:24:03.000 --> 00:24:06.160
<v Speaker 3>That's the plan. Its sensitivity and processing power are being

466
00:24:06.200 --> 00:24:10.680
<v Speaker 3>optimized precisely to pull weak structured signals like leakage radiation

467
00:24:10.920 --> 00:24:13.480
<v Speaker 3>could be out of the cosmic background noise, even from

468
00:24:13.519 --> 00:24:14.599
<v Speaker 3>significant distances.

469
00:24:14.799 --> 00:24:17.759
<v Speaker 2>It's not looking for the shout, it's listening for the whisper.

470
00:24:18.079 --> 00:24:21.400
<v Speaker 3>Perfectly put, the SKA is the kind of tool you'd

471
00:24:21.400 --> 00:24:24.759
<v Speaker 3>build if you believed the radical mundanity hypothesis was correct.

472
00:24:25.200 --> 00:24:28.680
<v Speaker 3>It matches the target. If those quiet Type II civilizations

473
00:24:28.680 --> 00:24:32.160
<v Speaker 3>are out there, the SKA or its successors represent our

474
00:24:32.240 --> 00:24:36.039
<v Speaker 3>best chance yet of finally hearing their faint planetary hum.

475
00:24:36.160 --> 00:24:39.559
<v Speaker 2>So the search gets harder in a way, needing more sensitivity,

476
00:24:39.599 --> 00:24:43.279
<v Speaker 2>more patience, maybe more clever signal analysis, but the target

477
00:24:43.279 --> 00:24:47.839
<v Speaker 2>itself feels more realistic, grounded in physics we actually understand.

478
00:24:47.960 --> 00:24:49.319
<v Speaker 3>I think that's fair to say, we just need to

479
00:24:49.319 --> 00:24:51.799
<v Speaker 3>build much better ears and point them very carefully at

480
00:24:51.839 --> 00:24:52.920
<v Speaker 3>the quietest places.

481
00:24:53.039 --> 00:24:55.519
<v Speaker 2>Okay, that leads us perfectly into a final thought for you,

482
00:24:55.599 --> 00:24:58.559
<v Speaker 2>the listener, to chew on building directly from this idea

483
00:24:58.559 --> 00:24:59.319
<v Speaker 2>of mundanity.

484
00:25:00.079 --> 00:25:03.839
<v Speaker 3>Orbit is right, and radical mundanity holds true if most

485
00:25:03.880 --> 00:25:07.240
<v Speaker 3>etcs really do seem to stall out technologically around the

486
00:25:07.279 --> 00:25:09.599
<v Speaker 3>type I level. What does that imply?

487
00:25:10.000 --> 00:25:13.440
<v Speaker 2>It suggests a kind of universal speed limit on technological growth,

488
00:25:13.440 --> 00:25:14.079
<v Speaker 2>doesn't it?

489
00:25:14.079 --> 00:25:16.680
<v Speaker 3>It could? Does it mean that the real great filter

490
00:25:16.839 --> 00:25:20.599
<v Speaker 3>isn't about getting life started or surviving nuclear war? But

491
00:25:20.640 --> 00:25:24.599
<v Speaker 3>it's actually the monumental challenge of making that leap from

492
00:25:24.720 --> 00:25:29.240
<v Speaker 3>planetary energy mastery type one to stellar energy mastery type two?

493
00:25:29.920 --> 00:25:33.519
<v Speaker 2>Is the silence simply because that jump is fundamentally too hard,

494
00:25:33.640 --> 00:25:37.359
<v Speaker 2>or too expensive, or maybe just physically impossible for any

495
00:25:37.359 --> 00:25:40.759
<v Speaker 2>civilization confined to a planet. Is that the barrier no

496
00:25:40.839 --> 00:25:42.759
<v Speaker 2>one or almost no one crosses.

497
00:25:43.200 --> 00:25:46.519
<v Speaker 3>It's a fascinating possibility. Maybe the silence isn't philosophical. Maybe

498
00:25:46.559 --> 00:25:49.759
<v Speaker 3>it's just engineering and economics on a cosmic scale.

499
00:25:49.880 --> 00:25:52.240
<v Speaker 2>So the provocative question for you is, if there's this

500
00:25:52.319 --> 00:25:55.759
<v Speaker 2>potential technological ceiling around type I, what does that mean

501
00:25:55.799 --> 00:25:58.119
<v Speaker 2>for us? What does our own ceiling look like? Are

502
00:25:58.119 --> 00:26:00.359
<v Speaker 2>we already bumping up against the point where the energy

503
00:26:00.359 --> 00:26:03.720
<v Speaker 2>and resource costs of our next big leaps true interplanetary

504
00:26:03.759 --> 00:26:08.079
<v Speaker 2>infrastructure interstellar probes start to become fundamentally prohibitive for a

505
00:26:08.160 --> 00:26:12.200
<v Speaker 2>planet bound species. Are we closer to our mundane limit

506
00:26:12.279 --> 00:27:15.359
<v Speaker 2>than we think something to ponder.

507
00:27:25.680 --> 00:27:40.000
<v Speaker 3>Arter s
