WEBVTT - Galactic Civilization’s End

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<v Speaker 1>Welcome to Stuff to Blow Your Mind from how Stuff

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<v Speaker 1>Works dot com. Hey you welcome to Stuff to Blow

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<v Speaker 1>your Mind. My name is Robert Lamb and I'm Joe McCormick.

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<v Speaker 1>And today we're going to be looking at a question

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<v Speaker 1>about the future a sort of today will be a

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<v Speaker 1>speculative out ing. So the question that we want to

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<v Speaker 1>start with today is the broad one, and then we'll

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<v Speaker 1>break it down into specific, specific ways of looking at

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<v Speaker 1>this question. The question is how long could a technological

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<v Speaker 1>civilization last? And notice that I just used the word

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<v Speaker 1>civilization and technological not necessarily human civilization, since time and

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<v Speaker 1>space scales the kind we're talking about could really blur

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<v Speaker 1>the lines of what it means for a civilization to

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<v Speaker 1>be human or consistently any one biological species. So for now,

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<v Speaker 1>I'd say, let's just define civilization as something like a

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<v Speaker 1>continue this tradition of intelligent behavior. Uh, if you've got

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<v Speaker 1>something like that, Assume a civilization like ours leaves Earth

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<v Speaker 1>and spreads out to colonize other star systems and becomes

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<v Speaker 1>a presence on the galactic stage. How long could a

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<v Speaker 1>civilization like that actually survive into the future. You kind

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<v Speaker 1>of have to think of of civilization as a virus

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<v Speaker 1>spreading through this uh, this galactic and ultimately I as

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<v Speaker 1>a universal host. How how far could it spread? How

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<v Speaker 1>long could it maintain the infection? Um? And it's it

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<v Speaker 1>is challenging at times just to think about it because

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<v Speaker 1>we we can't help but extrapolate what we have now

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<v Speaker 1>and what we know, and we have to do that

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<v Speaker 1>in order to to sort of scale up the model

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<v Speaker 1>of what a galactic civilization might look like. Um. And

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<v Speaker 1>at the because I think back to Star Trek for instance.

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<v Speaker 1>You know, Star Trek is essentially a show about clipper ships.

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<v Speaker 1>It's about seafaring individuals. It's just extrapolated into space and

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<v Speaker 1>then uh, you know, with a lot of cool science

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<v Speaker 1>science and science fictional elements explored within it, exploring the

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<v Speaker 1>planets of potted plants. Yeah. But but ultimately it is

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<v Speaker 1>it is based on the model of the president in

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<v Speaker 1>the past. Um. And then then there's also this this

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<v Speaker 1>element too of just um you know, uh, grandiose pride

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<v Speaker 1>and human accomplishment to to wonder where will we be

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<v Speaker 1>uh in this distant age. It reminds me of of

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<v Speaker 1>a quote from J. M. Coats. He's waiting for the barbarians,

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<v Speaker 1>and which he writes, quote one thought alone preoccupies the

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<v Speaker 1>submerged mind of empire, how not to end, how not

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<v Speaker 1>to die, how to prolong its era. I think that's

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<v Speaker 1>quite true, though, I mean the conception of empire that

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<v Speaker 1>we have is so time limited. I mean people who

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<v Speaker 1>are trying to prolong the empires that were used to

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<v Speaker 1>thinking about, say Cotsy probably has in mind something like

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<v Speaker 1>the British Empire um. That is an empire that, even

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<v Speaker 1>though it existed for a long period of time, was

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<v Speaker 1>on the scale of you know, people's recognizable descendants. You know,

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<v Speaker 1>you would be saying, I want to hand on my

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<v Speaker 1>empire to my child, or my grandchild or my great grandchild.

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<v Speaker 1>Do you do you want to hand on your empire

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<v Speaker 1>to something that is maybe not even recognizably the same

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<v Speaker 1>species as you a million years down the road. Yeah.

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<v Speaker 1>It kind of becomes the situation where one is, say

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<v Speaker 1>passing on a typewriter or or some other piece of technology,

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<v Speaker 1>where you're like, this has been in our family for years,

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<v Speaker 1>and then you're like, well, thanks, but it's and it

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<v Speaker 1>is now obsolete. It is it is kind of useless.

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<v Speaker 1>It's it's actually of more value perhaps now as a

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<v Speaker 1>mere museum piece or just as a metal to be recycled.

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<v Speaker 1>That's true, I guess it. Also it sort of works

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<v Speaker 1>out how you don't have to care about that thing

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<v Speaker 1>that's a million years down the road, whether or not

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<v Speaker 1>you think of that as your direct descendant or not,

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<v Speaker 1>because you care about next generation, and that generation will

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<v Speaker 1>always care about the next generation. It's just an echo

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<v Speaker 1>through through time and space. Yeah. I think one of

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<v Speaker 1>the important things to deep in mind and all of

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<v Speaker 1>this is just to what extent to things UH scale up,

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<v Speaker 1>you know, because we think about the empires and the

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<v Speaker 1>technology we have today and UH, I think is what

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<v Speaker 1>As we proceed through this discussion, it will be reminded

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<v Speaker 1>time and time again that that that human life, human empires,

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<v Speaker 1>they don't really scale up when you start applying them

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<v Speaker 1>to even even at the interplanetary stage, things begin to

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<v Speaker 1>get a little difficult. But certainly when you get beyond

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<v Speaker 1>beyond that, when you talk about UH, an empire that

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<v Speaker 1>spans solar systems or or or manages to spread throughout

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<v Speaker 1>an entire galaxy and human life as well, there are challenges. Obviously,

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<v Speaker 1>there are challenges when we think of of what we

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<v Speaker 1>have now, and even if you achieve some sort of

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<v Speaker 1>biological or digital immortality, um, it's it's difficult to put

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<v Speaker 1>that in context. Yeah. Now, one of the first questions

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<v Speaker 1>that you might ask is, well, how long would it take?

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<v Speaker 1>How long is it gonna take for a galactic civilization

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<v Speaker 1>to emerge? Okay, we gotta get there before we can

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<v Speaker 1>ask how long it will exist or survive? Right, Yeah,

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<v Speaker 1>And this is something that science fiction and authors often

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<v Speaker 1>kind of hatch you out, depending on how into you

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<v Speaker 1>know defining a timeline they are. Now. In his book Cosmos,

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<v Speaker 1>Carl Sagan commented on the Drake equation. Right. So, the

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<v Speaker 1>Drake equation we we've talked about on the show before,

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<v Speaker 1>but if you'll recall, it's essentially an equation put together

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<v Speaker 1>to come up with a rough estimate based on some

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<v Speaker 1>some variables where you can plug in your assumptions for

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<v Speaker 1>the answers UH to figure out how many technological civilizations

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<v Speaker 1>you would expect to find in a galaxy. So basically,

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<v Speaker 1>the short version is you take the number of planets

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<v Speaker 1>that there could be life on and then multiply that

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<v Speaker 1>by some probabilities like the fraction of planets where life emerges,

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<v Speaker 1>the fraction of the is where intelligent life evolves, the

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<v Speaker 1>fraction that's capable of interstellar communication, and the years a

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<v Speaker 1>civilization tends to remain detectable before for whatever reason, uh

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<v Speaker 1>disappearing right. And Sagan pointed out that civilizations might tend

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<v Speaker 1>to destroy themselves soon after reaching the technological phase, but

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<v Speaker 1>that at least some civilizations might learn to live with

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<v Speaker 1>high technology. He figured that, using the Drake equation, if

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<v Speaker 1>just one percent of all emergent technological civilization survived this

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<v Speaker 1>technological adolescence, then there could be millions of civilizations out there. Now,

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<v Speaker 1>there don't appear to be millions of civilizations out there

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<v Speaker 1>well as far as we know, as far as we know.

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<v Speaker 1>But but here's the thing. Sagan and William Newman calculated

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<v Speaker 1>that if a mill that if a million years ago

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<v Speaker 1>a space faring civilization emerged two hundred light years away

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<v Speaker 1>from us and spread outward, survey ships would only just

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<v Speaker 1>now be entering our solar system. And then what would

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<v Speaker 1>that even look like? What would a million year old

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<v Speaker 1>civilization uh, you know manifest as uh? I mean, our

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<v Speaker 1>current and only model outside of sci fi dreams is

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<v Speaker 1>our civilization. It's me. And it's a mere you know,

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<v Speaker 1>tens of thousands of years old, and we've only been

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<v Speaker 1>a technological civilization for a few centuries. So what would

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<v Speaker 1>these presumed immortals even be interested in when it comes

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<v Speaker 1>to exploring and colonizing new worlds? Would they have would

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<v Speaker 1>would they be interested in that at all? Would they

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<v Speaker 1>sort of would they perhaps give up on their colonization efforts,

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<v Speaker 1>uh after they realize that they need to perhaps extend

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<v Speaker 1>their their energy and other directions. It's a good question.

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<v Speaker 1>I mean, I think that it helps, um it helps

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<v Speaker 1>when trying to imagine the future behavior of civilizations, whether

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<v Speaker 1>alien or ours, to try to have as few assumptions

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<v Speaker 1>baked in as possible. And so you can make assumptions

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<v Speaker 1>maybe about what alien psychology might be, like, what their

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<v Speaker 1>their directives are an exploration, but all of those are

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<v Speaker 1>somewhat fallible. One of the things I think we can

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<v Speaker 1>bank on as an assumption about future your civilizations is

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<v Speaker 1>that they will need energy. That that's that's a that's

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<v Speaker 1>a kind of ground level assumption that just you can

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<v Speaker 1>count on that. But then how how might their goals change?

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<v Speaker 1>Like they have energy, they could have all the energy,

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<v Speaker 1>certainly in a world, in a solar system, in across

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<v Speaker 1>multiple systems. But then what do they really want to

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<v Speaker 1>do with it? And and indeed do they want to

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<v Speaker 1>survive the long term challenges of life in our universe

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<v Speaker 1>with their goals understanding? And even experience of time and

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<v Speaker 1>space differ from what we humans value and experience today. Uh,

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<v Speaker 1>it could be, but once you get into those scenarios,

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<v Speaker 1>it's just hard to it's hard to predict anything with

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<v Speaker 1>any confidence. Yeah, I mean so, yeah, this is where

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<v Speaker 1>you get into the really the domain of science fiction. Um,

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<v Speaker 1>I don't Oh, and there's plenty of great science fiction

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<v Speaker 1>along these lines. Yeah. I'm reminded of the various advanced

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<v Speaker 1>Elder civilizations in Ian Ebanks culture books. Um, because beyond

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<v Speaker 1>the the high level involved civilizations that engage with other

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<v Speaker 1>galactic civilizations in these books, there are what's known as

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<v Speaker 1>the sublime. The sublime these are advanced civilizations that basically,

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<v Speaker 1>at some point they just left all of their their

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<v Speaker 1>works behind because they've left the known dimensions of space

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<v Speaker 1>time behind to take up residents in several higher dimensions

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<v Speaker 1>higher dimensions. Now, does this what assumes string theory or

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<v Speaker 1>something like that, in which they're they're tiny higher dimensions

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<v Speaker 1>where you can somehow bacond your consciousness into some kind

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<v Speaker 1>of substrate that can transcend into those hidden dimensions. Well,

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<v Speaker 1>that's where my mind goes to, especially since we've we've

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<v Speaker 1>very recently spoken about dimensions and string theory. Uh. Now

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<v Speaker 1>I haven't I haven't read some of at least one

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<v Speaker 1>of the key books that deals with the sublime in

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<v Speaker 1>the culture A series. But it's basically the idea that

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<v Speaker 1>that suddenly that this particular group has reached a level

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<v Speaker 1>of technological and cultural advancement where they're not even playing

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<v Speaker 1>the same game as we are, that they are perhaps

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<v Speaker 1>not even really experiencing the universe in the same way

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<v Speaker 1>as we are, and they just kind of leave it behind.

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<v Speaker 1>Uh indeed, like a like like like something emerging from

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<v Speaker 1>a chrysalis and uh in taking off into a new

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<v Speaker 1>realm of being. And but in doing this, at the

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<v Speaker 1>same time, it's possible that sublimation uh might actually protect

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<v Speaker 1>them from the truly long term environmental risks of living

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<v Speaker 1>in our universe. So maybe it accomplishes the same go

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<v Speaker 1>But of course that is that is the benefit afforded

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<v Speaker 1>by playing in the realm of imagination. We don't know

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<v Speaker 1>if anything like that is possible or not. So let's

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<v Speaker 1>get into some of the long term environmental challenges of

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<v Speaker 1>of life in a hostile universe. Well, I guess first

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<v Speaker 1>we should look just the planetary level. Yeah, let's start

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<v Speaker 1>with with Earth itself, right, So there are a number

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<v Speaker 1>of factors to consider here, the most obvious being threats

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<v Speaker 1>from within and threats from beyond. So we certainly have

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<v Speaker 1>the ability to drastically damage the life sustaining properties of

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<v Speaker 1>planet Earth. In fact, we are we are currently doing that. Yes, yes,

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<v Speaker 1>with with say greenhouse gas emissions leading to global climate change,

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<v Speaker 1>we are verely hampering the Earth's ability to sustain a

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<v Speaker 1>civilization like ours far into the future. Yeah, the results

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<v Speaker 1>can be catastrophic. Now, could we actually wipe out all

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<v Speaker 1>life on the planet if such an evil aim possessed us?

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<v Speaker 1>I think we would probably have a hard time doing that.

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<v Speaker 1>I mean, life is pretty resilient, but we could come

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<v Speaker 1>frighteningly close. I've seen some estimates for how a large

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<v Speaker 1>enough nuclear war uh could could severely damage and wipe out,

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<v Speaker 1>you know, a significant number of of life forms on

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<v Speaker 1>our planet. I also read get this, um how even

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<v Speaker 1>even an extremely powerful detonation in the Mariana Trench could

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<v Speaker 1>collapse the food chain and wipe out most plant and

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<v Speaker 1>animal life specifically. And this is according to uh x

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<v Speaker 1>k c D s Randall Monroe uh x k c

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<v Speaker 1>d as a science blog and comic series online. Uh He,

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<v Speaker 1>according to his calculations, a fifty three million in megatun

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<v Speaker 1>explosion down in the trench might just do the trick.

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<v Speaker 1>This would be equal to the chicks Aloop impact that

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<v Speaker 1>occurred roughly sixty six million years ago, which led to

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<v Speaker 1>the Cretaceous Paleogene extinction event, and that killed sev of

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<v Speaker 1>all animal and plant species. That was the size of

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<v Speaker 1>a city, and it had the power of a billion

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<v Speaker 1>nuclear bombs. And this brings us to the extinction events

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<v Speaker 1>that can occur due to unchecked space collisions. Yeah, now

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<v Speaker 1>there's there's actually been some evidence to support the idea

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<v Speaker 1>that there's a a twenty six million year cycle linking

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<v Speaker 1>comet showers and global die offs. Yeah, there are people

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<v Speaker 1>who pause it all kinds of like like periods of

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<v Speaker 1>space impacts and what the causes of those might be.

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<v Speaker 1>But one thing we can say is that space impacts

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<v Speaker 1>are just a statistics game. I mean, you're it's just

0:12:48.600 --> 0:12:52.920
<v Speaker 1>a waiting game. Like you know, every so many years,

0:12:52.960 --> 0:12:56.520
<v Speaker 1>you're you're pretty much statistically guaranteed to get X number

0:12:56.840 --> 0:12:59.760
<v Speaker 1>of powerful storms that hit a certain part of the world.

0:13:00.080 --> 0:13:02.000
<v Speaker 1>Space impacts are the same way. There are a bunch

0:13:02.000 --> 0:13:04.640
<v Speaker 1>of objects out there, they're flying around, and you can

0:13:04.679 --> 0:13:07.960
<v Speaker 1>just calculate it out over certain periods of time, statistically

0:13:07.960 --> 0:13:10.559
<v Speaker 1>you're going to be hit by X number of objects

0:13:10.559 --> 0:13:13.520
<v Speaker 1>above a certain mass. So when you're we're talking about

0:13:13.559 --> 0:13:17.959
<v Speaker 1>a human civilization, uh, surviving however many you know, thousands

0:13:18.040 --> 0:13:20.439
<v Speaker 1>upon thousands upon thousands of years, certainly reaching like the

0:13:20.559 --> 0:13:25.080
<v Speaker 1>million or two million. Your point. If you want life

0:13:25.200 --> 0:13:29.800
<v Speaker 1>to continue on Earth, then you have to do something

0:13:29.920 --> 0:13:34.160
<v Speaker 1>about the potential impacts. Because defense, Yeah, you gotta have

0:13:34.200 --> 0:13:38.040
<v Speaker 1>planetary defense, which is something that uh that people are

0:13:38.080 --> 0:13:41.079
<v Speaker 1>working on. Uh we've discussed it on the show before.

0:13:41.080 --> 0:13:43.400
<v Speaker 1>It's still not as much of a priority as it

0:13:43.440 --> 0:13:47.079
<v Speaker 1>should be. You have all of these uh, these politicians

0:13:47.880 --> 0:13:51.520
<v Speaker 1>out there, you know, making campaign promises and talking about

0:13:51.600 --> 0:13:55.120
<v Speaker 1>what they're gonna do for for for to improve everyone's life,

0:13:55.360 --> 0:13:58.120
<v Speaker 1>and it always floors me that this is not something

0:13:58.160 --> 0:14:00.319
<v Speaker 1>that people take up because this is one of the

0:14:00.400 --> 0:14:03.160
<v Speaker 1>This is perhaps the only, or at least one of

0:14:03.160 --> 0:14:05.240
<v Speaker 1>the very few causes where we can say this is

0:14:05.280 --> 0:14:07.959
<v Speaker 1>something we can do to save the world. This is

0:14:08.000 --> 0:14:10.840
<v Speaker 1>something we can do to protect the planet. Yeah, what

0:14:10.840 --> 0:14:13.880
<v Speaker 1>what if there? That was like a what if that

0:14:13.960 --> 0:14:18.240
<v Speaker 1>was a campaign platform? It was basically civilization level defense.

0:14:18.400 --> 0:14:22.840
<v Speaker 1>So your your campaign platform is fight climate change, protect

0:14:22.840 --> 0:14:25.960
<v Speaker 1>the planet from space object impacts, and let's say the

0:14:25.960 --> 0:14:28.560
<v Speaker 1>other big one would be prepared for the next superflu

0:14:30.520 --> 0:14:32.080
<v Speaker 1>It makes sense to me, I mean, I guess the

0:14:32.080 --> 0:14:35.560
<v Speaker 1>the the the counter argument here is that most these

0:14:35.600 --> 0:14:40.160
<v Speaker 1>are these are generally longer term threats. Uh, so people

0:14:40.200 --> 0:14:44.200
<v Speaker 1>are going to be less inclined to let it impact

0:14:44.200 --> 0:14:49.800
<v Speaker 1>their voting behavior. It's frustrating. But anyway, uh some other

0:14:49.880 --> 0:14:52.600
<v Speaker 1>problems that, of course so be as we've discussed before.

0:14:52.760 --> 0:14:55.240
<v Speaker 1>Venus offers an example of this of a sort of

0:14:55.240 --> 0:14:58.800
<v Speaker 1>worst case runaway greenhouse effect that could leave a planet,

0:14:58.840 --> 0:15:01.840
<v Speaker 1>even a planet like Earth, uninhabitable, And there are also

0:15:01.960 --> 0:15:06.200
<v Speaker 1>various long term scenarios involving the world's oceans, the magnetosphere,

0:15:06.600 --> 0:15:08.200
<v Speaker 1>which if you listen to the show, you know that

0:15:08.240 --> 0:15:12.320
<v Speaker 1>the magnetosphere plays a vital role in protecting our planet

0:15:12.400 --> 0:15:15.560
<v Speaker 1>from silver and cosmic radiation, and if something were to

0:15:15.600 --> 0:15:19.320
<v Speaker 1>happen to that, then we're unprotected. There are also biological

0:15:19.360 --> 0:15:23.160
<v Speaker 1>threats from within Earth's biosphere. That's right. You have to

0:15:23.200 --> 0:15:28.080
<v Speaker 1>consider the likes of Peter Ward's media hYP hypothesis. I

0:15:28.160 --> 0:15:30.760
<v Speaker 1>was actually not familiar with this. This is a kind

0:15:30.800 --> 0:15:35.720
<v Speaker 1>of an opposite of the Gaia hypothesis and uh, the

0:15:35.760 --> 0:15:41.360
<v Speaker 1>Medeia hypothesis is that multicellular life is a suicidal superorganism

0:15:41.480 --> 0:15:44.880
<v Speaker 1>leading to microbial triggered mass extinctions. I mean, whether you

0:15:44.920 --> 0:15:48.520
<v Speaker 1>buy the framing is a suicidal superorganism, it is clear

0:15:48.640 --> 0:15:51.120
<v Speaker 1>that there have been times in the past where life

0:15:51.200 --> 0:15:54.800
<v Speaker 1>on Earth caused massive extinctions of other types of life

0:15:54.800 --> 0:15:57.360
<v Speaker 1>on Earth. I mean, we think about the oxygenation of

0:15:57.360 --> 0:15:59.920
<v Speaker 1>our atmosphere that we are now adapted to was initially

0:16:00.080 --> 0:16:03.520
<v Speaker 1>tragedy that killed killed off tons of life, and then

0:16:03.520 --> 0:16:06.360
<v Speaker 1>of course we've seen this this particular primate species rise

0:16:06.480 --> 0:16:09.600
<v Speaker 1>up and uh and and alter the atmosphere from a

0:16:09.720 --> 0:16:12.560
<v Speaker 1>very early time. And then of course there are the

0:16:12.640 --> 0:16:15.960
<v Speaker 1>outside context problems to consider, which, of course is a

0:16:16.080 --> 0:16:18.720
<v Speaker 1>term that was coined by Ian M. Banks but has

0:16:18.760 --> 0:16:24.560
<v Speaker 1>been used since then by various other authors and even scientists.

0:16:24.760 --> 0:16:27.800
<v Speaker 1>You call them outside context problems to consider, but sort

0:16:27.800 --> 0:16:30.480
<v Speaker 1>of the nature of them means that what you can't

0:16:30.520 --> 0:16:33.960
<v Speaker 1>consider the right right. Yeah. Banks said that an outside

0:16:33.960 --> 0:16:36.960
<v Speaker 1>context problem is the sort of thing most civilizations encounter

0:16:37.120 --> 0:16:39.920
<v Speaker 1>just once, in which they tend to encounter rather in

0:16:39.960 --> 0:16:43.080
<v Speaker 1>the same way as sentence encounters a full stop. Um.

0:16:43.640 --> 0:16:46.000
<v Speaker 1>So yeah, if we could. The classic example, of course

0:16:46.120 --> 0:16:49.880
<v Speaker 1>is um, if you have a primitive terrestrial society and

0:16:49.960 --> 0:16:54.840
<v Speaker 1>then uh, a colonial force shows up with advanced technology,

0:16:55.160 --> 0:16:57.440
<v Speaker 1>you know, and then to extrapolate that into space, an

0:16:57.480 --> 0:17:00.320
<v Speaker 1>alien civilization shows up with it with advanced head ology.

0:17:00.360 --> 0:17:02.440
<v Speaker 1>But of course, when the thing about the the alien

0:17:02.480 --> 0:17:06.480
<v Speaker 1>consideration is that a lot of very intelligent folks have

0:17:06.520 --> 0:17:10.520
<v Speaker 1>thought about this problem. There are even some rudimentary plans

0:17:10.560 --> 0:17:13.760
<v Speaker 1>in place to deal with it when it occurs, you know,

0:17:13.760 --> 0:17:16.639
<v Speaker 1>people who think about first contact. So it's not really

0:17:16.880 --> 0:17:20.679
<v Speaker 1>a completely outside contact problem. Yeah. You could look at

0:17:20.680 --> 0:17:23.200
<v Speaker 1>a lot of science fiction as us doing our very

0:17:23.240 --> 0:17:27.880
<v Speaker 1>best to use our imaginations to prepare for this potential conflict. Right.

0:17:28.400 --> 0:17:30.600
<v Speaker 1>But one of the big hard limits for life on

0:17:30.760 --> 0:17:34.399
<v Speaker 1>Earth uh and in our solar system itself, concerns the

0:17:34.440 --> 0:17:36.760
<v Speaker 1>life cycle of our son. Now maybe we should take

0:17:36.760 --> 0:17:39.560
<v Speaker 1>a quick break and then come back to UH to

0:17:39.720 --> 0:17:42.520
<v Speaker 1>discuss and weep in anguish over the death of the Sun.

0:17:43.119 --> 0:17:47.679
<v Speaker 1>Than alright, we're back. So we we've talked about the

0:17:47.680 --> 0:17:50.159
<v Speaker 1>life cycle of the Sun before on this show, but

0:17:50.240 --> 0:17:54.080
<v Speaker 1>just to refresh, this is basically how it it works.

0:17:54.080 --> 0:17:56.320
<v Speaker 1>So our son has been going strong for four point

0:17:56.359 --> 0:17:59.400
<v Speaker 1>five billion years and it has another five billion years

0:17:59.440 --> 0:18:03.320
<v Speaker 1>left in the town. When the courts roughly speaking, roughly speaking, now,

0:18:03.320 --> 0:18:05.280
<v Speaker 1>when the core runs out of hydrogen fuel, it's going

0:18:05.359 --> 0:18:08.240
<v Speaker 1>to contract under the weight of gravity. Some hydrogen fusion

0:18:08.240 --> 0:18:10.199
<v Speaker 1>will occur in the upper layers at this point. But

0:18:10.600 --> 0:18:13.240
<v Speaker 1>as a depleted core contracts, it heats up, and this

0:18:13.320 --> 0:18:16.240
<v Speaker 1>heats the upper layers of the Sun, causing them to expand.

0:18:16.280 --> 0:18:18.639
<v Speaker 1>And as the outer layers expand, the radius of the

0:18:18.680 --> 0:18:21.200
<v Speaker 1>Sun will increase and it will become a red giant.

0:18:21.440 --> 0:18:23.720
<v Speaker 1>And the radius of the of a red giant son,

0:18:23.840 --> 0:18:27.240
<v Speaker 1>our red giant son would be a hundred times what

0:18:27.320 --> 0:18:29.800
<v Speaker 1>it is now. It's not good. Now, that's that's not

0:18:29.840 --> 0:18:33.000
<v Speaker 1>good for anybody, because this would this would put the

0:18:33.560 --> 0:18:36.239
<v Speaker 1>put the the the the outside of the Sun just

0:18:36.359 --> 0:18:39.399
<v Speaker 1>beyond the Earth's orbit, and some scientists have estimated that

0:18:39.440 --> 0:18:41.680
<v Speaker 1>this would just vaporize our planet, but there's also a

0:18:41.680 --> 0:18:44.480
<v Speaker 1>good chance it would push Earth and its moon outward

0:18:44.560 --> 0:18:48.400
<v Speaker 1>after consuming mercury and venus. In any case, whatever it does,

0:18:48.520 --> 0:18:51.679
<v Speaker 1>it does not sound like a survivable event for the

0:18:51.720 --> 0:18:55.080
<v Speaker 1>inhabitants of Earth. That's right, It's just it's it's bad news.

0:18:55.400 --> 0:18:57.760
<v Speaker 1>And long before this happens, say in a mirror one

0:18:57.800 --> 0:19:00.520
<v Speaker 1>to two billion years, the Earth is gonna go hot

0:19:00.640 --> 0:19:04.639
<v Speaker 1>enough to to boil away its oceans as well. And

0:19:04.680 --> 0:19:07.680
<v Speaker 1>if we're looking really long term, um, here's how it'll

0:19:07.680 --> 0:19:10.919
<v Speaker 1>it'll all play out. According to Ethan Seagull, who wrote

0:19:11.160 --> 0:19:13.640
<v Speaker 1>how our Solar System will end in the Far Future

0:19:13.640 --> 0:19:16.600
<v Speaker 1>for Forbes. Uh. He says that in nine point five

0:19:16.600 --> 0:19:19.439
<v Speaker 1>billion years, the sunile collapse into a white dwarf, and

0:19:19.480 --> 0:19:22.520
<v Speaker 1>the remaining dead worlds will continue to orbit it, and

0:19:22.520 --> 0:19:26.000
<v Speaker 1>eventually the white dwarf will go dark in the inevitable

0:19:26.040 --> 0:19:29.560
<v Speaker 1>collision between it and another black dwarf will blast apart

0:19:29.640 --> 0:19:31.960
<v Speaker 1>the remnants of our solar system. So all that and

0:19:32.000 --> 0:19:34.040
<v Speaker 1>the Sun doesn't even get to turn into a black hole.

0:19:34.200 --> 0:19:36.120
<v Speaker 1>That's right, the Sun will never get to turn into

0:19:36.160 --> 0:19:39.680
<v Speaker 1>a black it's not massive enough. Uh, and yet it

0:19:39.720 --> 0:19:43.480
<v Speaker 1>will wreak havoc. Nonetheless, So what's our fight or flight

0:19:43.520 --> 0:19:47.119
<v Speaker 1>response here? Well, it obviously means if our civilization is

0:19:47.160 --> 0:19:51.159
<v Speaker 1>going to survive into the realm of say billions of years,

0:19:51.200 --> 0:19:54.320
<v Speaker 1>if you're on the billions order of magnitude for the future,

0:19:54.480 --> 0:19:57.320
<v Speaker 1>we can't stay here, that's right. We've got to build ships,

0:19:57.320 --> 0:20:00.520
<v Speaker 1>We've got to build colonies. We've got to estab colonies

0:20:00.520 --> 0:20:03.879
<v Speaker 1>on other worlds and other systems as well. Or perhaps

0:20:03.920 --> 0:20:07.000
<v Speaker 1>we do something to just move the Earth itself, because

0:20:07.000 --> 0:20:11.240
<v Speaker 1>as we ascend the Kardashian scale, such things do theoretically

0:20:11.240 --> 0:20:14.119
<v Speaker 1>become possible. Sure, at least in theory. For instance, we

0:20:14.119 --> 0:20:18.119
<v Speaker 1>can harness comments and asteroids so they gravitationally slingshot past

0:20:18.200 --> 0:20:20.320
<v Speaker 1>Earth and move us into a wider orbit away from

0:20:20.320 --> 0:20:23.960
<v Speaker 1>the Sun. We could build planetary sunshades that have the

0:20:24.000 --> 0:20:27.879
<v Speaker 1>same effect, or or very or even just sort of

0:20:27.920 --> 0:20:32.000
<v Speaker 1>turn the Earth into a spaceship of sorts, you know,

0:20:32.080 --> 0:20:35.399
<v Speaker 1>just take it with us. Well, there are versions, like,

0:20:35.560 --> 0:20:38.639
<v Speaker 1>for example, there is one idea that's not for moving

0:20:38.760 --> 0:20:41.159
<v Speaker 1>planets so much as it is for moving stars. But

0:20:41.200 --> 0:20:44.040
<v Speaker 1>I wonder if similar principles could be applied to planets,

0:20:44.800 --> 0:20:48.439
<v Speaker 1>where it's known as the Scatoff thruster if you're read

0:20:48.480 --> 0:20:51.160
<v Speaker 1>about the Yeah, so this is for stars. But what

0:20:51.400 --> 0:20:53.560
<v Speaker 1>it would do would be would be sort of a

0:20:53.720 --> 0:20:58.680
<v Speaker 1>large reflective encasement for part of a star that would

0:20:58.720 --> 0:21:03.320
<v Speaker 1>cause a positive radi asian pressure in one direction back

0:21:03.359 --> 0:21:06.160
<v Speaker 1>against the star. And by reflecting all of this radiation

0:21:06.240 --> 0:21:08.280
<v Speaker 1>back in the direction of the star, you could actually

0:21:08.320 --> 0:21:11.000
<v Speaker 1>steer the movement of a star. One wonders if you

0:21:11.000 --> 0:21:14.240
<v Speaker 1>could create some kind of similar solar sale like thing

0:21:14.520 --> 0:21:17.040
<v Speaker 1>for a planet. Then again, the planet is not emitting

0:21:17.160 --> 0:21:18.879
<v Speaker 1>radiation the way a star is, So I don't know,

0:21:18.920 --> 0:21:22.440
<v Speaker 1>maybe maybe possible, maybe not, Yeah, or ultimately we could

0:21:22.440 --> 0:21:24.640
<v Speaker 1>just leave it behind, move on to better worlds, make

0:21:24.680 --> 0:21:28.280
<v Speaker 1>better worlds. Exodus from an uninhabitable Earth has been a

0:21:28.280 --> 0:21:31.960
<v Speaker 1>sci fi staple for decades, going back at least to

0:21:32.000 --> 0:21:34.879
<v Speaker 1>the nineteen thirties. That's when British sci fi author Olaf

0:21:35.320 --> 0:21:38.359
<v Speaker 1>Stapleton wrote about it and uh during the events of

0:21:38.400 --> 0:21:41.639
<v Speaker 1>Frank Herbert's Dune, Old Earth is said to be an

0:21:41.720 --> 0:21:45.480
<v Speaker 1>uninhabited waste. Oh yeah, do they ever go there? I

0:21:45.520 --> 0:21:48.480
<v Speaker 1>don't not. In the the original books that they might

0:21:48.600 --> 0:21:52.439
<v Speaker 1>have something that takes place in the more recent Dune

0:21:52.560 --> 0:21:55.000
<v Speaker 1>franchise books, but I have not read them, so I

0:21:55.000 --> 0:21:59.640
<v Speaker 1>would love to hear from from hardcore Dune readers on that. Now.

0:22:00.119 --> 0:22:03.120
<v Speaker 1>When it comes to moving the planet, though, we also

0:22:03.160 --> 0:22:05.960
<v Speaker 1>see some work there in science fiction. Sci fi writer

0:22:06.119 --> 0:22:09.600
<v Speaker 1>Stanley Schmidt explored it in nineteen and Ian M. Banks

0:22:09.640 --> 0:22:12.359
<v Speaker 1>also wrote about it. So we're kind of climbing a

0:22:12.400 --> 0:22:16.639
<v Speaker 1>Kardashian scale of destruction here. So planetary power and the

0:22:16.640 --> 0:22:19.800
<v Speaker 1>ability to save one's planet in some sense, then solar

0:22:19.840 --> 0:22:22.720
<v Speaker 1>system power and the ability to save oneself or roll

0:22:22.840 --> 0:22:25.960
<v Speaker 1>with the changes to a single star system. But what

0:22:26.040 --> 0:22:28.440
<v Speaker 1>about beyond that? What about the fate of galaxies in

0:22:28.480 --> 0:22:31.720
<v Speaker 1>the universe itself. Yeah, yeah, that's a good question. I

0:22:31.720 --> 0:22:33.600
<v Speaker 1>guess that's where we have to go next. Now, before

0:22:33.600 --> 0:22:36.240
<v Speaker 1>we do that, we should pause for the reality check

0:22:36.320 --> 0:22:39.440
<v Speaker 1>and and not ignore the much much nearer, more salient

0:22:39.520 --> 0:22:42.439
<v Speaker 1>threats facing our species right now. We mentioned some of

0:22:42.440 --> 0:22:46.000
<v Speaker 1>those earlier, primarily things like climate change in all of

0:22:46.000 --> 0:22:50.800
<v Speaker 1>its myriad downstream effects, killer pandemics like the next super flu,

0:22:50.920 --> 0:22:54.600
<v Speaker 1>the threat of space impacts, nuclear war. Maybe some people

0:22:54.600 --> 0:22:57.440
<v Speaker 1>would throw artificial intelligence in there. I don't know. That's

0:22:57.480 --> 0:22:59.639
<v Speaker 1>that seems like a much bigger question mark to me.

0:23:00.560 --> 0:23:02.520
<v Speaker 1>But I think the big ones we really know to

0:23:02.560 --> 0:23:05.040
<v Speaker 1>be concerned about, based on the most solid science, would

0:23:05.040 --> 0:23:07.880
<v Speaker 1>be things like climate change in pandemics. We know those

0:23:07.880 --> 0:23:10.399
<v Speaker 1>are real threats right now. We have to be fighting

0:23:10.400 --> 0:23:13.480
<v Speaker 1>and preparing today if we want to thrive in the future. Uh.

0:23:13.480 --> 0:23:15.320
<v Speaker 1>And of course we've discussed those in the past and

0:23:15.359 --> 0:23:18.400
<v Speaker 1>we will revisit them in the future. But to continue

0:23:18.400 --> 0:23:21.919
<v Speaker 1>today's thought experiment, let's let's go that next step. So

0:23:21.960 --> 0:23:26.520
<v Speaker 1>we imagine our technological behaviors can be changed, and we

0:23:26.600 --> 0:23:29.760
<v Speaker 1>beat back global climate change, we survive all these other

0:23:29.840 --> 0:23:33.359
<v Speaker 1>threats in the near term, We expand our space exploration

0:23:33.400 --> 0:23:37.000
<v Speaker 1>and colonization ability. We spread out our civilization so that

0:23:37.040 --> 0:23:40.199
<v Speaker 1>no one local event in any individual solar system can

0:23:40.240 --> 0:23:43.760
<v Speaker 1>bring it to an end. When do much bigger concerns

0:23:43.880 --> 0:23:47.960
<v Speaker 1>like the space, time, and energy dynamics of the larger

0:23:48.080 --> 0:23:52.520
<v Speaker 1>universe start to actually become a threat to our survival, Well,

0:23:52.760 --> 0:23:56.959
<v Speaker 1>not anytime soon, right, but but as far as we know,

0:23:57.000 --> 0:23:58.760
<v Speaker 1>as far as we know, but there are predictions for

0:23:58.800 --> 0:24:02.200
<v Speaker 1>how it might go down. The sort of universal apocalypse.

0:24:02.800 --> 0:24:07.440
<v Speaker 1>In fact, they're there at least four main models here.

0:24:08.440 --> 0:24:11.159
<v Speaker 1>We're gonna start with the two older models. One is

0:24:11.200 --> 0:24:14.000
<v Speaker 1>the Big Freeze. Uh. And this has to do with

0:24:14.160 --> 0:24:18.000
<v Speaker 1>just an eternally expanding universe. Uh. And we know the

0:24:18.040 --> 0:24:21.200
<v Speaker 1>universe is expanding. Uh. So the idea here is that

0:24:21.320 --> 0:24:24.080
<v Speaker 1>everything expands to the point where there's just heat death

0:24:24.160 --> 0:24:27.280
<v Speaker 1>across the universe, the triumph of entropy in your life

0:24:27.359 --> 0:24:30.199
<v Speaker 1>with just a cold, dead universe. According to some of

0:24:30.200 --> 0:24:32.800
<v Speaker 1>the models. One thing that can often be misleading about

0:24:32.800 --> 0:24:34.959
<v Speaker 1>the idea of the heat death of the universe is

0:24:35.000 --> 0:24:37.200
<v Speaker 1>that if you if you're not familiar with this term,

0:24:37.200 --> 0:24:39.680
<v Speaker 1>it sounds like that might be hot. It's not hot.

0:24:39.720 --> 0:24:42.840
<v Speaker 1>It's the opposite. It means it means usable energy gets

0:24:42.840 --> 0:24:46.760
<v Speaker 1>converted into heat, which is entropy energy you can't use,

0:24:47.040 --> 0:24:50.840
<v Speaker 1>and everything is just this cold bath of slightly above

0:24:50.880 --> 0:24:54.760
<v Speaker 1>absolute zero radiation. Now, the the other side of that,

0:24:54.840 --> 0:24:57.320
<v Speaker 1>of course, is the idea that what if things expand

0:24:57.320 --> 0:25:01.000
<v Speaker 1>to the point and then they retract uh in a

0:25:01.040 --> 0:25:05.359
<v Speaker 1>collapsing mechanism. This was this would lead to what is

0:25:05.560 --> 0:25:09.280
<v Speaker 1>considered the big crunch. So the universe stops expanding, crunches

0:25:09.320 --> 0:25:12.960
<v Speaker 1>back down over time into the reverse of the Big Bang.

0:25:13.240 --> 0:25:16.960
<v Speaker 1>That doesn't sound good for you know, but yeah, but

0:25:17.000 --> 0:25:18.600
<v Speaker 1>this would be this would be a hot death as

0:25:18.640 --> 0:25:22.040
<v Speaker 1>a cold as opposed to a cold death. Now, back

0:25:22.080 --> 0:25:26.720
<v Speaker 1>in nineteen seventy nine, physicist Freeman Dyson. Dyson is still

0:25:26.760 --> 0:25:28.679
<v Speaker 1>with us as of this recording. He was born in

0:25:30.640 --> 0:25:34.000
<v Speaker 1>But he pondered just how these two possibilities would impact

0:25:34.119 --> 0:25:38.080
<v Speaker 1>humanity or whatever humanity becomes over the course of time,

0:25:38.480 --> 0:25:42.040
<v Speaker 1>and he was he was pretty optimistic. Yeah, we should

0:25:42.040 --> 0:25:44.000
<v Speaker 1>know that this paper we're gonna be talking about is

0:25:44.200 --> 0:25:47.960
<v Speaker 1>fantastically readable. But Dyson was working with the knowledge available

0:25:48.000 --> 0:25:50.439
<v Speaker 1>to him at the time in nineteen seventy nine. So,

0:25:50.520 --> 0:25:53.360
<v Speaker 1>for example, this predates the discoveries that seemed to indicate

0:25:53.359 --> 0:25:56.960
<v Speaker 1>that the expansion of the universe is accelerating. Dyson didn't

0:25:56.960 --> 0:26:00.800
<v Speaker 1>know that at the time. At the time, he vote, quote,

0:26:00.800 --> 0:26:04.040
<v Speaker 1>the prevailing view holds the future of open and closed

0:26:04.119 --> 0:26:07.560
<v Speaker 1>universe versus this being the idea that to a closed

0:26:07.600 --> 0:26:10.800
<v Speaker 1>universe is one that will eventually collapse into the Big crunch,

0:26:11.200 --> 0:26:13.440
<v Speaker 1>and an open universe is one that will just continue

0:26:13.480 --> 0:26:18.240
<v Speaker 1>to expand towards this big freeze. He said, uh uh,

0:26:18.440 --> 0:26:20.919
<v Speaker 1>quote the future of open and closed universe is to

0:26:21.000 --> 0:26:24.200
<v Speaker 1>be equally dismal. According to this view, we have only

0:26:24.280 --> 0:26:27.040
<v Speaker 1>the choice of being fried in a closed universe or

0:26:27.160 --> 0:26:29.880
<v Speaker 1>frozen in an open one. And he can He goes

0:26:29.960 --> 0:26:33.119
<v Speaker 1>on regrettably, I have to concur with es verdict that

0:26:33.200 --> 0:26:35.520
<v Speaker 1>in the case, in this case, we have no escape

0:26:35.560 --> 0:26:38.040
<v Speaker 1>from frying. No matter how deep we burrow into the

0:26:38.040 --> 0:26:41.240
<v Speaker 1>earth to shield ourselves from the ever increasing fury of

0:26:41.240 --> 0:26:45.000
<v Speaker 1>the blue shifted background radiation, we can only postpone by

0:26:45.000 --> 0:26:48.879
<v Speaker 1>a few million years. Are miserable? End? Oh wow, I

0:26:48.960 --> 0:26:51.520
<v Speaker 1>was just thinking. So the blue shifting of radiation means

0:26:51.560 --> 0:26:55.800
<v Speaker 1>that if radiation sources are accelerating towards you, the radiation

0:26:55.840 --> 0:26:59.359
<v Speaker 1>they emit gets uped in frequency, gets blue shifted up higher.

0:26:59.640 --> 0:27:03.240
<v Speaker 1>So does that mean like radio waves, the cosmic microwave

0:27:03.240 --> 0:27:06.400
<v Speaker 1>background radiation and all that as it closes in towards

0:27:06.440 --> 0:27:09.400
<v Speaker 1>you gets blue shifted up and turned into gamma rays.

0:27:09.880 --> 0:27:12.719
<v Speaker 1>I get something like that. That's that's That's what I'm

0:27:12.760 --> 0:27:16.280
<v Speaker 1>getting from this. But this is with the closed universe model, right,

0:27:16.440 --> 0:27:20.040
<v Speaker 1>and and he he largely avoids the quote unquote claustrophobic

0:27:20.119 --> 0:27:22.080
<v Speaker 1>nature of the closed universe in this paper, but he

0:27:22.119 --> 0:27:25.399
<v Speaker 1>does offer this. Uh, this idea, he says, supposing that

0:27:25.440 --> 0:27:28.720
<v Speaker 1>we discover the universe to be naturally closed and doomed

0:27:28.720 --> 0:27:32.960
<v Speaker 1>to collapse, is it conceivable that by intelligent intervention converting

0:27:33.080 --> 0:27:36.399
<v Speaker 1>matter into radiation and causing energy to flow purposefully on

0:27:36.440 --> 0:27:39.520
<v Speaker 1>a cosmic scale, we could break open a closed universe

0:27:39.560 --> 0:27:42.640
<v Speaker 1>and change the topology of space time so that only

0:27:42.680 --> 0:27:44.600
<v Speaker 1>a part of it would collapse, in another part of

0:27:44.640 --> 0:27:51.040
<v Speaker 1>it would expand forever. Uh. Yeah, I would call that optimistic. Yeah,

0:27:51.080 --> 0:27:52.919
<v Speaker 1>but I mean he's he's basically throwing it out here

0:27:52.920 --> 0:27:55.400
<v Speaker 1>and saying, look, I'm not sure how this would work exactly,

0:27:55.800 --> 0:28:00.080
<v Speaker 1>but if we're talking about a significantly advanced civilization, this

0:28:00.520 --> 0:28:03.040
<v Speaker 1>sounds like the kind of thing such a civilization would

0:28:03.080 --> 0:28:05.960
<v Speaker 1>be into doing and maybe maybe have the ability to

0:28:06.440 --> 0:28:09.800
<v Speaker 1>do it. Yeah. Uh. One thing I like about Dyson's

0:28:09.800 --> 0:28:14.280
<v Speaker 1>attitude here is that he he's essentially saying, you know, physicists,

0:28:14.920 --> 0:28:18.840
<v Speaker 1>you should explore extreme implications. Uh. He starts off his

0:28:18.880 --> 0:28:22.359
<v Speaker 1>paper by talking about Stephen Weinberg, the Stephen Weinberg quote

0:28:22.760 --> 0:28:24.880
<v Speaker 1>that the problem with physicists is not that they take

0:28:24.920 --> 0:28:27.639
<v Speaker 1>their theories too seriously, but that they don't take them

0:28:27.680 --> 0:28:30.719
<v Speaker 1>seriously enough. You know that they scoff at some of

0:28:30.760 --> 0:28:34.680
<v Speaker 1>the discussing some of the more outlandish implications of theories

0:28:34.720 --> 0:28:36.760
<v Speaker 1>that we know to be good theories and are confirmed

0:28:36.800 --> 0:28:39.880
<v Speaker 1>by evidence. Uh, and Dyson's like, no, let's get into

0:28:39.880 --> 0:28:42.360
<v Speaker 1>the weirdness. Okay, we've got a theory. We think it's

0:28:42.360 --> 0:28:44.800
<v Speaker 1>a good theory because it predicts all the stuff we see.

0:28:45.040 --> 0:28:48.640
<v Speaker 1>What does it imply? What are the weirdest things that implies? Again,

0:28:48.680 --> 0:28:52.520
<v Speaker 1>this paper is uh is really readable, very accessible, especially

0:28:52.560 --> 0:28:55.520
<v Speaker 1>for a paper that has so many equations in it.

0:28:56.280 --> 0:28:59.680
<v Speaker 1>But but he also has some some very helpful timetable

0:28:59.720 --> 0:29:02.760
<v Speaker 1>scale els. For instance, he has his table one summary

0:29:02.800 --> 0:29:05.560
<v Speaker 1>of time scales, and he he holds it in a

0:29:05.600 --> 0:29:09.120
<v Speaker 1>closed universe, you'd have a total duration for the universe

0:29:09.480 --> 0:29:12.000
<v Speaker 1>of ten to the eleventh power years or a hundred

0:29:12.000 --> 0:29:14.520
<v Speaker 1>billion years. And and then when he looks at the

0:29:14.560 --> 0:29:18.800
<v Speaker 1>open universe, he basically takes it by by order of magnitude.

0:29:19.480 --> 0:29:22.400
<v Speaker 1>So he taught this is what he says, quote, it

0:29:22.480 --> 0:29:25.040
<v Speaker 1>takes about ten to the six or one million years

0:29:25.080 --> 0:29:27.960
<v Speaker 1>to evolve a new species tend to the seventh power,

0:29:28.080 --> 0:29:31.160
<v Speaker 1>or ten million years to evolve a genus tend to

0:29:31.200 --> 0:29:33.560
<v Speaker 1>the eighth power or a hundred million years to evolve

0:29:33.600 --> 0:29:37.080
<v Speaker 1>a class ten to the ninth power, or one billion

0:29:37.160 --> 0:29:40.040
<v Speaker 1>years to evolve a phylum in less than ten to

0:29:40.120 --> 0:29:43.680
<v Speaker 1>the tenth power years, or ten billion years to evolve

0:29:43.720 --> 0:29:47.160
<v Speaker 1>all the way from the primeval slime to Homo sapience.

0:29:47.520 --> 0:29:51.200
<v Speaker 1>I'm not sure if his taxonomic organization of of time

0:29:51.240 --> 0:29:55.000
<v Speaker 1>scales of evolution is exactly right, but I mean he's

0:29:55.000 --> 0:29:58.360
<v Speaker 1>working essentially with orders of magnetzya. He's definitely rounding up.

0:29:59.400 --> 0:30:02.320
<v Speaker 1>He's so, for example, he says, you know, less than

0:30:02.360 --> 0:30:05.720
<v Speaker 1>ten billion years, I guess that's actually that's a fair

0:30:05.800 --> 0:30:07.920
<v Speaker 1>number to work with if you're just trying to estimate

0:30:08.400 --> 0:30:12.280
<v Speaker 1>galactic evolution, right, because you're ultimately trying You're you're dealing

0:30:12.360 --> 0:30:14.400
<v Speaker 1>with with life and life on Earth, which is just

0:30:14.520 --> 0:30:18.680
<v Speaker 1>a pin drop in the in in terms of cosmic history.

0:30:18.960 --> 0:30:20.479
<v Speaker 1>But you're you're, so you have to work with these

0:30:20.720 --> 0:30:25.120
<v Speaker 1>exceedingly large orders of magnitude, right, But but playing with

0:30:25.200 --> 0:30:29.280
<v Speaker 1>rough orders of magnitude gives you more, essentially more room

0:30:29.360 --> 0:30:31.480
<v Speaker 1>to play around. So life on Earth has not been

0:30:31.520 --> 0:30:33.600
<v Speaker 1>around for ten billion years, but it's been around for

0:30:33.680 --> 0:30:36.000
<v Speaker 1>more than one billion years, So you can essentially just

0:30:36.160 --> 0:30:38.640
<v Speaker 1>round up or down to the nearest order of magnitude.

0:30:39.200 --> 0:30:43.760
<v Speaker 1>Now ultimately for an open universe scenario. He does say

0:30:43.800 --> 0:30:45.760
<v Speaker 1>that he does think it's pretty hopeful. He says, quote,

0:30:45.800 --> 0:30:48.360
<v Speaker 1>so far as we can imagine into the future, things

0:30:48.400 --> 0:30:51.920
<v Speaker 1>continue to happen in the open cosmology, history has no

0:30:52.080 --> 0:30:56.160
<v Speaker 1>heir and his in this paper. His basic breakdown in

0:30:56.200 --> 0:30:59.400
<v Speaker 1>this paper is that consciousness is not bound to biology

0:30:59.440 --> 0:31:03.320
<v Speaker 1>of it is structural. Then we can move beyond the body.

0:31:03.640 --> 0:31:07.920
<v Speaker 1>We can become digital machines, we can become uh, you know,

0:31:08.000 --> 0:31:12.600
<v Speaker 1>black clouds of particles. That intelligence doesn't necessarily have to

0:31:12.640 --> 0:31:16.560
<v Speaker 1>be confined to flesh beings anymore. And he had There's

0:31:16.600 --> 0:31:18.720
<v Speaker 1>also an interesting point in this where he talks about

0:31:19.360 --> 0:31:23.600
<v Speaker 1>immortal computing, which I hadn't really thought about. He says, quote,

0:31:23.600 --> 0:31:27.320
<v Speaker 1>a society with finite material resources can never build a

0:31:27.360 --> 0:31:32.000
<v Speaker 1>digital memory beyond a certain finite capacity. Therefore, digital memory

0:31:32.120 --> 0:31:34.760
<v Speaker 1>cannot be adequate to the needs of a life form

0:31:34.840 --> 0:31:39.080
<v Speaker 1>planning to survive indefinitely. Fortunately, there is no limited principle

0:31:39.120 --> 0:31:42.360
<v Speaker 1>to the capacity of an analog memory built out of

0:31:42.400 --> 0:31:47.000
<v Speaker 1>a fixed number of components in an expanding universe. For example,

0:31:47.280 --> 0:31:50.400
<v Speaker 1>a physical quantity such as the angle between two stars

0:31:50.440 --> 0:31:53.640
<v Speaker 1>and the sky can be used as an analog memory unit.

0:31:54.000 --> 0:31:56.400
<v Speaker 1>The capacity of this memory unit is equal to the

0:31:56.480 --> 0:31:59.760
<v Speaker 1>number of significant binary digits to which the angle can

0:31:59.760 --> 0:32:03.760
<v Speaker 1>be measured. As the universe expands and the stars recede,

0:32:04.040 --> 0:32:07.120
<v Speaker 1>the number of significant digits in this angle will increase

0:32:07.360 --> 0:32:11.720
<v Speaker 1>logarithmically with time. Measurements of atomic frequencies and energy levels

0:32:11.760 --> 0:32:14.520
<v Speaker 1>can also, in principle be measured with a number of

0:32:14.560 --> 0:32:18.440
<v Speaker 1>significant figures proportional too, and then he refers to an

0:32:18.440 --> 0:32:22.280
<v Speaker 1>equation log T. Therefore, an immortal civilization should ultimately find

0:32:22.360 --> 0:32:25.760
<v Speaker 1>ways to code its archives in an analog memory with

0:32:25.880 --> 0:32:29.880
<v Speaker 1>capacity growing like log T. Such a memory will put

0:32:29.920 --> 0:32:34.120
<v Speaker 1>severe constraints on the rate of acquisition of permanent new knowledge,

0:32:34.320 --> 0:32:37.360
<v Speaker 1>but at least it is not forbid it altogether. WHOA,

0:32:38.160 --> 0:32:40.440
<v Speaker 1>So I love that because he's he's really thinking big

0:32:40.480 --> 0:32:44.240
<v Speaker 1>about about how even you know, memory and recorded history

0:32:44.240 --> 0:32:48.400
<v Speaker 1>would work with a civilization that is this far advanced

0:32:48.440 --> 0:32:50.760
<v Speaker 1>beyond what we have now. Again, what we have now

0:32:50.880 --> 0:32:54.120
<v Speaker 1>does not scale up well, So ultimately Dyson is taking

0:32:54.160 --> 0:32:58.960
<v Speaker 1>a very optimistic view of the ways that intelligence civilization

0:32:59.080 --> 0:33:03.040
<v Speaker 1>could adapt to the changing physical environment of the universe.

0:33:03.080 --> 0:33:08.240
<v Speaker 1>At large, right, but again this was this was We've

0:33:08.240 --> 0:33:11.560
<v Speaker 1>had some some some changes since then. And in fact

0:33:12.120 --> 0:33:17.440
<v Speaker 1>BBC writer Adam Becker reached out to Dyson in um

0:33:17.480 --> 0:33:20.080
<v Speaker 1>on the matter of of of the expansion in our

0:33:20.160 --> 0:33:24.040
<v Speaker 1>universe seeming to accelerate, which which puts a new spin

0:33:24.120 --> 0:33:27.680
<v Speaker 1>on everything that we've discussed thus far. And uh, and

0:33:27.720 --> 0:33:29.560
<v Speaker 1>so he reached out to Dyson, and Dyson said that

0:33:29.600 --> 0:33:32.719
<v Speaker 1>he's he's far less optimistic, and that the most optimistic

0:33:32.800 --> 0:33:36.160
<v Speaker 1>view is that perhaps the acceleration will slow down on

0:33:36.240 --> 0:33:38.880
<v Speaker 1>its own, because he points out, we we don't know

0:33:38.920 --> 0:33:42.000
<v Speaker 1>what's accelerating it, so it's still possible that it could

0:33:42.040 --> 0:33:46.880
<v Speaker 1>stop um or slow down. Otherwise, Uh, he says, our

0:33:46.920 --> 0:33:50.560
<v Speaker 1>descendants will lose touch with most galaxies, drastically limiting the

0:33:50.600 --> 0:33:53.560
<v Speaker 1>available energy that he's discussing in these models. And that

0:33:53.640 --> 0:33:55.880
<v Speaker 1>sets us up in a pretty key way to talk

0:33:55.920 --> 0:33:58.760
<v Speaker 1>about one of the papers we wanted to discuss today,

0:33:59.000 --> 0:34:02.200
<v Speaker 1>a new paper from the physicist Dan Hooper. But first, Robert,

0:34:02.240 --> 0:34:05.440
<v Speaker 1>did you want to mention a couple of other hypothesized

0:34:05.440 --> 0:34:08.319
<v Speaker 1>ways that the universe could end? Yeah, yeah, they we'll

0:34:08.320 --> 0:34:11.720
<v Speaker 1>throw these out here. The first one is the big change.

0:34:12.560 --> 0:34:16.520
<v Speaker 1>This is in this a bubble of new lower temperature

0:34:16.600 --> 0:34:20.200
<v Speaker 1>vacuum emerges in our own universe and expands at the

0:34:20.239 --> 0:34:24.120
<v Speaker 1>speed of light, converting everything in our universe. As Adam

0:34:24.160 --> 0:34:27.080
<v Speaker 1>Becker wrote in that BBCO in his BBC article how

0:34:27.160 --> 0:34:32.200
<v Speaker 1>will the universe end? And could anything survive? Um quote,

0:34:32.239 --> 0:34:36.440
<v Speaker 1>the properties of fundamental particles like electrons and quarks could

0:34:36.440 --> 0:34:40.880
<v Speaker 1>be entirely different inside the bubble, radically rewriting the rules

0:34:40.880 --> 0:34:45.080
<v Speaker 1>of chemistry and perhaps preventing atoms from forming. Plus a

0:34:45.280 --> 0:34:47.920
<v Speaker 1>dark energy inside the bubble might behave in a different matter,

0:34:48.000 --> 0:34:52.640
<v Speaker 1>perhaps causing collapse rather than expansion. So um this this

0:34:52.680 --> 0:34:55.800
<v Speaker 1>sounds like a very problematic scenario if it where to

0:34:55.840 --> 0:34:59.040
<v Speaker 1>come to pass. It almost is love craft Ian and

0:34:59.080 --> 0:35:02.040
<v Speaker 1>it's uh and it's a scope right, the idea that

0:35:02.360 --> 0:35:05.920
<v Speaker 1>suddenly here is an emergence of a part of our

0:35:06.000 --> 0:35:09.000
<v Speaker 1>space that is not bound by the same rules. Yeah.

0:35:10.000 --> 0:35:11.919
<v Speaker 1>Nice laws of physics you've got. There be a shame

0:35:11.960 --> 0:35:18.840
<v Speaker 1>if something happened to them. Now. Another another apocalyptic scenario

0:35:18.960 --> 0:35:22.000
<v Speaker 1>for the universe is the Big Rip and this one

0:35:22.360 --> 0:35:25.799
<v Speaker 1>was presented by Robert Caldwell of Dartmouth College in two

0:35:25.880 --> 0:35:30.040
<v Speaker 1>thousand three based on the idea of phantom dark energy,

0:35:30.080 --> 0:35:33.120
<v Speaker 1>in which the intensity of dark energy increases as the

0:35:33.200 --> 0:35:38.279
<v Speaker 1>universe expands. So it's the density of of dark energy

0:35:38.400 --> 0:35:40.880
<v Speaker 1>right now, as we understand it is pretty low, but

0:35:40.920 --> 0:35:44.320
<v Speaker 1>if it builds up, it would rip the universe to shreds.

0:35:44.320 --> 0:35:47.200
<v Speaker 1>So maybe overcoming the other forces, Like right now we

0:35:47.239 --> 0:35:52.560
<v Speaker 1>see dark energy increasing the distance between the galaxies out there.

0:35:52.560 --> 0:35:55.400
<v Speaker 1>But things that are gravitationally bound to each other, or

0:35:55.480 --> 0:35:59.839
<v Speaker 1>say bound by the nuclear force that holds atoms together, Uh,

0:36:00.000 --> 0:36:02.759
<v Speaker 1>that stuff is pretty safe from dark energy. If dark

0:36:02.840 --> 0:36:05.600
<v Speaker 1>energy said no, I'm going to overcome your gravity, overcome

0:36:05.640 --> 0:36:08.000
<v Speaker 1>your nuclear force, that would be a problem. Yeah, this

0:36:08.080 --> 0:36:11.000
<v Speaker 1>is This is how Caldwell described it in his in

0:36:11.040 --> 0:36:15.480
<v Speaker 1>his presentation quote, the positive phantom energy density becomes infinite

0:36:15.520 --> 0:36:19.200
<v Speaker 1>in finite time, overcoming all other forms of matters, such

0:36:19.200 --> 0:36:23.600
<v Speaker 1>as that of gravitational repulsion, rapidly bringing our brief epoch

0:36:23.680 --> 0:36:27.120
<v Speaker 1>of cosmic structure to a close. The phantom energy rips

0:36:27.120 --> 0:36:31.120
<v Speaker 1>apart the Milky Way solar system, Earth, and ultimately the molecules, adams,

0:36:31.200 --> 0:36:35.440
<v Speaker 1>nuclei and nucleons of which we are composed before the

0:36:35.480 --> 0:36:38.919
<v Speaker 1>death of the universe in a big rip. Who gives

0:36:38.920 --> 0:36:43.120
<v Speaker 1>a rip. So so that sounds that sounds terrifying as well.

0:36:43.200 --> 0:36:45.520
<v Speaker 1>And on that note, let's take one more quick break

0:36:45.560 --> 0:36:49.960
<v Speaker 1>and then we'll return to the discussion. Thank you, all right,

0:36:49.960 --> 0:36:53.759
<v Speaker 1>we're back. Okay. So what spurred this whole conversation was

0:36:53.960 --> 0:36:57.000
<v Speaker 1>that we wanted to talk about a highly speculative but

0:36:57.239 --> 0:37:00.920
<v Speaker 1>very fun paper that just was just published online by

0:37:00.960 --> 0:37:05.080
<v Speaker 1>the physicist Dan Hooper, in which Hooper tries to imagine

0:37:05.160 --> 0:37:10.600
<v Speaker 1>and scientifically characterize a survival strategy for a galactic civilization

0:37:10.680 --> 0:37:12.719
<v Speaker 1>that sees the writing on the wall about the long

0:37:12.840 --> 0:37:15.560
<v Speaker 1>term fate of the universe and decides it wants to

0:37:15.600 --> 0:37:18.879
<v Speaker 1>survive as long as possible, because it turns out, if

0:37:18.920 --> 0:37:22.200
<v Speaker 1>you are a galactic civilization, you don't need to wait

0:37:22.400 --> 0:37:25.560
<v Speaker 1>until the cold death of the entire universe to have

0:37:25.640 --> 0:37:29.360
<v Speaker 1>a problem. You just have to discover that usable energy

0:37:29.400 --> 0:37:33.200
<v Speaker 1>is becoming scarce where you live. Hooper's paper is called

0:37:33.360 --> 0:37:37.120
<v Speaker 1>Life versus Dark Energy, How an advanced civilization could resist

0:37:37.200 --> 0:37:40.600
<v Speaker 1>the accelerating expansion of the Universe. Uh. And we should

0:37:40.640 --> 0:37:42.400
<v Speaker 1>point out that this has not been published in a

0:37:42.520 --> 0:37:44.360
<v Speaker 1>peer of view journal yet or anything. This is just

0:37:44.400 --> 0:37:47.440
<v Speaker 1>something he put out on the internet ahead of publications

0:37:47.480 --> 0:37:49.520
<v Speaker 1>so people could comment on it and talk about it.

0:37:49.800 --> 0:37:51.920
<v Speaker 1>I think it may eventually come out in the Journal

0:37:51.920 --> 0:37:55.319
<v Speaker 1>of Cosmology and Astroparticle Physics, but we'll pay attention there.

0:37:55.320 --> 0:37:58.839
<v Speaker 1>But as always with anything that hasn't been uh been

0:37:58.880 --> 0:38:01.799
<v Speaker 1>put through peer of view yet, grain assault. So who

0:38:01.880 --> 0:38:05.239
<v Speaker 1>is Dan Hooper? He is an associate professor of astronomy

0:38:05.280 --> 0:38:08.360
<v Speaker 1>and astrophysics at the University of Chicago, and he's a

0:38:08.400 --> 0:38:12.120
<v Speaker 1>senior scientist and the head of the Theoretical Astrophysics Group

0:38:12.200 --> 0:38:15.319
<v Speaker 1>at Fermi National Accelerator Laboratory. And a lot of his

0:38:15.360 --> 0:38:18.960
<v Speaker 1>work focuses on the intersection between particle physics and the

0:38:19.040 --> 0:38:22.560
<v Speaker 1>evolution of the universe at large. So he's interested on

0:38:22.600 --> 0:38:24.800
<v Speaker 1>where the biggest stuff we know about in the smallest

0:38:24.840 --> 0:38:27.919
<v Speaker 1>stuff we know about effect one another. So what's what's

0:38:27.920 --> 0:38:32.560
<v Speaker 1>Hooper's argument about the future survival of a galactic civilization. Well,

0:38:32.680 --> 0:38:35.440
<v Speaker 1>he turns his attention to dark energy what we've just

0:38:35.480 --> 0:38:38.320
<v Speaker 1>been talking about, So on the scale of the universe

0:38:38.360 --> 0:38:41.319
<v Speaker 1>at large, not necessarily in our own local neighborhood, but

0:38:41.400 --> 0:38:46.040
<v Speaker 1>averaged across the entire observable sky, we've discovered that the

0:38:46.160 --> 0:38:49.360
<v Speaker 1>energy that dominates the vacuum of space is not gravity,

0:38:49.719 --> 0:38:53.000
<v Speaker 1>not electromagnetism, not any of the normal forces that govern

0:38:53.080 --> 0:38:56.920
<v Speaker 1>our lives and our solar system, but a poorly understood

0:38:56.920 --> 0:38:59.840
<v Speaker 1>form of energy that we call dark energy, which drives

0:39:00.160 --> 0:39:05.239
<v Speaker 1>expansion of the universe. So mass and gravitation attract objects

0:39:05.239 --> 0:39:08.480
<v Speaker 1>to one another, dark energy drives them apart. It's the

0:39:08.600 --> 0:39:12.520
<v Speaker 1>energy that causes the space between galaxies to spread, meaning

0:39:12.560 --> 0:39:15.040
<v Speaker 1>that the whole universe is growing larger and all the

0:39:15.120 --> 0:39:18.320
<v Speaker 1>stuff within it is growing farther apart, and the galaxy

0:39:18.400 --> 0:39:21.520
<v Speaker 1>is farthest away from us are receding from us the fastest.

0:39:22.000 --> 0:39:24.200
<v Speaker 1>So as far as we know right now, dark energy

0:39:24.320 --> 0:39:27.440
<v Speaker 1>might not have any practical applications for life bound to

0:39:27.480 --> 0:39:31.240
<v Speaker 1>Planet Earth outside of scientific research, that is. But then again,

0:39:31.600 --> 0:39:34.520
<v Speaker 1>we should know better than to dismiss the usefulness of

0:39:34.520 --> 0:39:38.000
<v Speaker 1>any scientific discovery ahead of time. I'm always reminded of

0:39:38.000 --> 0:39:40.920
<v Speaker 1>the English physicists who is credited as one of the

0:39:40.920 --> 0:39:45.040
<v Speaker 1>discoveries of the electron, J. J. Thompson, who originally thought

0:39:45.080 --> 0:39:48.480
<v Speaker 1>that the electron, which he was calling it the corpuscles uh.

0:39:48.480 --> 0:39:50.680
<v Speaker 1>He thought this particle he had discovered would not be

0:39:50.800 --> 0:39:54.080
<v Speaker 1>very useful outside of the lab, had no idea had

0:39:54.080 --> 0:39:57.640
<v Speaker 1>anything to do with electricity. But Hooper points out how

0:39:57.800 --> 0:40:01.480
<v Speaker 1>once a civilization expands to a S and scale and

0:40:01.560 --> 0:40:05.600
<v Speaker 1>its energy needs scale with that expansion, dark energy becomes

0:40:05.600 --> 0:40:09.239
<v Speaker 1>a pressing concern for the future of that civilization. And

0:40:09.280 --> 0:40:11.920
<v Speaker 1>this is because dark energy presents us the future of

0:40:11.920 --> 0:40:18.040
<v Speaker 1>an encroaching cosmic horizon. So we are unable to interact

0:40:18.080 --> 0:40:21.520
<v Speaker 1>with anything beyond what's known as our cosmic horizon. This

0:40:21.600 --> 0:40:25.160
<v Speaker 1>is the distance beyond which it is impossible to see

0:40:25.440 --> 0:40:28.960
<v Speaker 1>because light from beyond this distance will never have time

0:40:29.200 --> 0:40:34.000
<v Speaker 1>to reach us. Beyond that distance, everything is causally cut

0:40:34.040 --> 0:40:36.800
<v Speaker 1>off from us. We can't see it, we can't talk

0:40:36.880 --> 0:40:39.680
<v Speaker 1>to it or travel to it. Uh. You can think

0:40:39.719 --> 0:40:42.239
<v Speaker 1>about it this way with an analogy. Imagine that the

0:40:42.280 --> 0:40:45.719
<v Speaker 1>city or the neighborhood you live in is expanding. Are

0:40:45.719 --> 0:40:48.080
<v Speaker 1>you there, Robert, Yeah, I'm there. It seems to be

0:40:48.120 --> 0:40:51.239
<v Speaker 1>the case. Actually no, no, no no, no. What you're thinking

0:40:51.320 --> 0:40:53.920
<v Speaker 1>of is the increasing density of the city you live in.

0:40:54.040 --> 0:40:56.960
<v Speaker 1>More stuff is filling it. But instead you actually need

0:40:57.000 --> 0:41:01.399
<v Speaker 1>to think of exactly the opposite. The distance between your

0:41:01.480 --> 0:41:06.719
<v Speaker 1>house and other buildings is steadily increasing at an accelerating rate,

0:41:07.400 --> 0:41:10.080
<v Speaker 1>so at normal walking speed. You say, used to be

0:41:10.160 --> 0:41:12.600
<v Speaker 1>able to walk to the post office or the grocery

0:41:12.680 --> 0:41:15.000
<v Speaker 1>store and then back to your house in what half

0:41:15.000 --> 0:41:18.800
<v Speaker 1>an hour something like that, But as the distance between

0:41:18.880 --> 0:41:22.680
<v Speaker 1>your house and these locations expands, the trip starts to

0:41:22.719 --> 0:41:26.680
<v Speaker 1>take forty five minutes than an hour, then longer and

0:41:26.800 --> 0:41:30.440
<v Speaker 1>longer at normal walking speed. Now you could try to

0:41:30.520 --> 0:41:33.319
<v Speaker 1>walk faster, you could run, ride a bike, drive a car,

0:41:33.440 --> 0:41:36.320
<v Speaker 1>and this would help. But eventually, as the space between

0:41:36.320 --> 0:41:40.919
<v Speaker 1>the locations keeps expanding faster and faster, even these more

0:41:40.920 --> 0:41:44.680
<v Speaker 1>powerful vehicles and methods of travel will take longer and

0:41:44.719 --> 0:41:48.719
<v Speaker 1>longer to get you between locations, until eventually you reach

0:41:48.719 --> 0:41:52.560
<v Speaker 1>a point where no vehicle you can get can make

0:41:52.600 --> 0:41:55.920
<v Speaker 1>the trip because the distance between the two points expands

0:41:56.080 --> 0:41:58.680
<v Speaker 1>faster than you can travel. You could travel toward the

0:41:58.719 --> 0:42:01.440
<v Speaker 1>grocery store at maximum speed for the rest of your

0:42:01.480 --> 0:42:04.359
<v Speaker 1>life and never get there, and this would mean that

0:42:04.400 --> 0:42:07.920
<v Speaker 1>the grocery store has crossed beyond your cosmic horizon from

0:42:08.000 --> 0:42:11.560
<v Speaker 1>your house. Uh So, now, beyond the cosmic horizon of

0:42:11.560 --> 0:42:14.440
<v Speaker 1>the real universe, there might be lots of other stuff

0:42:14.760 --> 0:42:17.200
<v Speaker 1>we can only see to our cosmic horizon, and beyond

0:42:17.239 --> 0:42:20.600
<v Speaker 1>that it's possible there are other galaxies, stars, planets, but

0:42:20.680 --> 0:42:23.799
<v Speaker 1>because the interaction, our ability to interact with all that

0:42:23.800 --> 0:42:26.400
<v Speaker 1>stuff is cut off by the speed of light, we

0:42:26.440 --> 0:42:29.080
<v Speaker 1>will never be able to touch it. We can't land

0:42:29.080 --> 0:42:32.320
<v Speaker 1>on those planets, we can't send messages to those civilizations

0:42:32.400 --> 0:42:35.239
<v Speaker 1>or get messages from them. We're just cut off by

0:42:35.280 --> 0:42:37.319
<v Speaker 1>the universal speed limit of the speed of light and

0:42:37.320 --> 0:42:39.320
<v Speaker 1>a vacuum. So, for instance, if you had this vast

0:42:39.400 --> 0:42:45.360
<v Speaker 1>galaxy spanning uh Empire where everything everything is kind of compartmentalized.

0:42:45.360 --> 0:42:47.279
<v Speaker 1>You have all these different divisions of the empire, and

0:42:47.320 --> 0:42:50.600
<v Speaker 1>maybe they're they're not even in direct communication anymore. They

0:42:50.680 --> 0:42:54.960
<v Speaker 1>just kind of have periodic updates about what culture and

0:42:55.120 --> 0:42:58.279
<v Speaker 1>life is like in these distant places. But eventually you

0:42:58.320 --> 0:43:00.480
<v Speaker 1>reach the point where they're just too far from each

0:43:00.520 --> 0:43:03.040
<v Speaker 1>other for there to ever be contact again. Well, it

0:43:03.080 --> 0:43:05.440
<v Speaker 1>would depend on how far away from each other they are,

0:43:05.480 --> 0:43:10.640
<v Speaker 1>because if they're within a galaxy or even within nearby galaxies,

0:43:10.719 --> 0:43:13.240
<v Speaker 1>within what's known as the local group. The local group

0:43:13.320 --> 0:43:16.640
<v Speaker 1>is a cluster of roughly fifty something nearby galaxies, they

0:43:16.680 --> 0:43:20.120
<v Speaker 1>will probably one day merge into the same big old clump.

0:43:20.680 --> 0:43:23.800
<v Speaker 1>The local group is gravitationally bound, so we're going to

0:43:23.920 --> 0:43:26.359
<v Speaker 1>pretty much stick together with the other stuff in the

0:43:26.360 --> 0:43:29.480
<v Speaker 1>local group. So it's the galaxies far far away we

0:43:29.560 --> 0:43:32.080
<v Speaker 1>have to worry about. Right. So if if, for instance,

0:43:32.080 --> 0:43:35.080
<v Speaker 1>if Star Wars films were actually made in a galaxy

0:43:35.080 --> 0:43:38.200
<v Speaker 1>far far away beyond the local group, and they have

0:43:38.239 --> 0:43:40.600
<v Speaker 1>to be shipped back to us, there would reach a

0:43:40.600 --> 0:43:43.040
<v Speaker 1>point where we could receive no more new Star Wars films.

0:43:43.040 --> 0:43:44.879
<v Speaker 1>It would be a tragedy, wouldn't it. That's why we're

0:43:44.880 --> 0:43:47.880
<v Speaker 1>stockpiling them now. We're getting as many per year as possible,

0:43:47.920 --> 0:43:51.120
<v Speaker 1>because eventually it's going to pass beyond the cosmic horizon.

0:43:51.160 --> 0:43:53.440
<v Speaker 1>Oh no, wait, I don't want to be misinterpreted, because

0:43:53.440 --> 0:43:55.759
<v Speaker 1>I know there are actually people who like hate the

0:43:55.880 --> 0:43:59.440
<v Speaker 1>last Jedi. I am not one of those. I liked

0:43:59.480 --> 0:44:02.040
<v Speaker 1>it too. Um, but yeah, I've seen this all over

0:44:02.080 --> 0:44:04.640
<v Speaker 1>the internet. People are like, people are like pulling their

0:44:04.640 --> 0:44:07.479
<v Speaker 1>hair out about how much they hated. I don't understand. Yeah,

0:44:07.520 --> 0:44:09.560
<v Speaker 1>I mean they're talking about making a Boba Fett movie, Like,

0:44:09.640 --> 0:44:14.080
<v Speaker 1>do not disappoint like five year old Robert lamb and

0:44:14.080 --> 0:44:17.120
<v Speaker 1>and and and ruin the possibility of a boa Fett

0:44:17.160 --> 0:44:19.239
<v Speaker 1>movie for because I know that that he really wants

0:44:19.239 --> 0:44:21.200
<v Speaker 1>to see it now. We'll come back to the cosmic

0:44:21.239 --> 0:44:23.520
<v Speaker 1>horizon and the universal speed limit in just a minute,

0:44:23.560 --> 0:44:26.960
<v Speaker 1>but uh to to shift our attention to another issue.

0:44:27.600 --> 0:44:31.200
<v Speaker 1>It's often supposed that far far future civilization can keep

0:44:31.239 --> 0:44:35.280
<v Speaker 1>itself alive and create usable energy by harvesting the energy

0:44:35.560 --> 0:44:39.040
<v Speaker 1>from stars, and this is a good strategy. We we

0:44:39.120 --> 0:44:42.440
<v Speaker 1>often think about future energy sources. We think about what like, oh,

0:44:42.560 --> 0:44:47.360
<v Speaker 1>cold fusion or something like that, but these are paltry

0:44:47.440 --> 0:44:50.839
<v Speaker 1>energy sources. Any kind of like human made reactor that

0:44:50.880 --> 0:44:53.960
<v Speaker 1>we can can feasibly think of right now would be

0:44:54.000 --> 0:44:57.799
<v Speaker 1>a very paltry energy source compared to what's already out there,

0:44:57.840 --> 0:45:00.120
<v Speaker 1>which is the Sun right that. I mean, that is

0:45:00.120 --> 0:45:04.080
<v Speaker 1>the energy source for everything that we hold dear. I mean,

0:45:04.120 --> 0:45:06.640
<v Speaker 1>there's there's a reason that we we have worshiped it

0:45:06.640 --> 0:45:09.480
<v Speaker 1>as a god in in previous ages because it it

0:45:09.600 --> 0:45:13.360
<v Speaker 1>essentially is the almighty in our solar system. It is

0:45:13.400 --> 0:45:15.520
<v Speaker 1>our creator. It is everything you know. I mean, it

0:45:15.640 --> 0:45:18.279
<v Speaker 1>is a thing I used to say that I haven't

0:45:18.280 --> 0:45:20.239
<v Speaker 1>thought of in a while, but I still stand by.

0:45:20.320 --> 0:45:23.399
<v Speaker 1>Is that when you think about energy sources, really it's

0:45:23.600 --> 0:45:26.239
<v Speaker 1>with a few caveats, it's all solar Yeah, Like if

0:45:26.239 --> 0:45:30.080
<v Speaker 1>you're eating a steak or or a Caesar salad, what

0:45:30.160 --> 0:45:34.040
<v Speaker 1>have you, you were eating uh, converted sunlight, Like this

0:45:34.080 --> 0:45:36.319
<v Speaker 1>is sunlight you were eating. That's where the energy came from.

0:45:36.360 --> 0:45:40.000
<v Speaker 1>It's just you're getting it downstream coal or oil or

0:45:40.080 --> 0:45:42.520
<v Speaker 1>something like that that you would burn. Fossil fuels that

0:45:42.560 --> 0:45:46.360
<v Speaker 1>you burn have chemical energy baked into them that was

0:45:46.400 --> 0:45:50.640
<v Speaker 1>created when ancient organisms photosynthesized with the with the energy

0:45:50.640 --> 0:45:53.160
<v Speaker 1>of sunlight. They took carbon out of the air, used

0:45:53.160 --> 0:45:55.600
<v Speaker 1>the energy from sunlight to make that into sugar that

0:45:55.680 --> 0:45:58.359
<v Speaker 1>turned into chemicals later down the road that you're now

0:45:58.440 --> 0:46:01.680
<v Speaker 1>burning to power your car. And this is why Kardaschef

0:46:01.800 --> 0:46:05.560
<v Speaker 1>Scale level two is to simply master a sign to

0:46:05.640 --> 0:46:09.080
<v Speaker 1>say all this energy that is uh, it's maintaining the

0:46:09.160 --> 0:46:12.400
<v Speaker 1>solar system. This is now all mine, right uh, And

0:46:12.440 --> 0:46:14.279
<v Speaker 1>so how would you do that? I mean to come

0:46:14.280 --> 0:46:16.600
<v Speaker 1>back to Freeman Dyson. We've discussed on the show before

0:46:16.640 --> 0:46:19.640
<v Speaker 1>the idea of the Dyson's Fear. The Dyson's Fear comes

0:46:19.640 --> 0:46:22.400
<v Speaker 1>to us from Freeman Dyson, and he basically says, you know,

0:46:23.440 --> 0:46:26.000
<v Speaker 1>a civilization in the future that has a lot of

0:46:26.000 --> 0:46:28.360
<v Speaker 1>technological power and wants to get the most bang for

0:46:28.400 --> 0:46:33.960
<v Speaker 1>its buck will just completely surround its star with the

0:46:34.000 --> 0:46:37.279
<v Speaker 1>equivalent of solar panels, right. And this brings me back

0:46:37.320 --> 0:46:39.799
<v Speaker 1>to Star Trek, because I earlier was talking about Star

0:46:39.880 --> 0:46:42.120
<v Speaker 1>Trek and you know, scaling up of our current models

0:46:42.160 --> 0:46:44.319
<v Speaker 1>of life and all I do have to point out

0:46:44.360 --> 0:46:47.120
<v Speaker 1>that Star Trek the next Generation is the first place

0:46:47.239 --> 0:46:50.920
<v Speaker 1>I saw any mention or depiction of a Dycen sphere.

0:46:51.320 --> 0:46:54.400
<v Speaker 1>And it blew me away then, and it still blows

0:46:54.400 --> 0:46:57.919
<v Speaker 1>me away now. Yeah. I mean, it's fantastic to think about. Uh.

0:46:57.960 --> 0:47:00.279
<v Speaker 1>And one of the ways that it's actually relevant to us.

0:47:00.280 --> 0:47:03.000
<v Speaker 1>I mean, obviously it could be relevant in the far

0:47:03.080 --> 0:47:05.120
<v Speaker 1>future if we wanted to try to build something like this.

0:47:05.520 --> 0:47:09.239
<v Speaker 1>It's not technologically relevant to us today, except in the

0:47:09.280 --> 0:47:13.719
<v Speaker 1>sense that if we're doing say CT and we want

0:47:13.760 --> 0:47:17.160
<v Speaker 1>to look for ways of detecting alien civilizations out there

0:47:17.200 --> 0:47:20.040
<v Speaker 1>that maybe aren't beaming us radio signals on purpose or

0:47:20.080 --> 0:47:23.600
<v Speaker 1>anything like that. One thing that Dyson proposed is, hey,

0:47:23.680 --> 0:47:25.759
<v Speaker 1>you know, we could look for Dyson's fears out there.

0:47:25.800 --> 0:47:27.680
<v Speaker 1>I don't think he called them dycens fears, but I

0:47:27.719 --> 0:47:31.719
<v Speaker 1>don't know Dycen spears Dyson clouds, but I don't know,

0:47:32.000 --> 0:47:34.319
<v Speaker 1>I'm not true to what extent he referred to them

0:47:34.320 --> 0:47:37.120
<v Speaker 1>with his own name somehow I doubt it. I don't remember,

0:47:37.200 --> 0:47:42.360
<v Speaker 1>but uh, if he did, that kind of be awesome anyway. No,

0:47:42.520 --> 0:47:44.120
<v Speaker 1>but I mean he was like, you know, you could

0:47:44.160 --> 0:47:46.000
<v Speaker 1>look for this kind of thing, and so people people

0:47:46.040 --> 0:47:48.160
<v Speaker 1>have looked for this kind of thing. It would have

0:47:48.200 --> 0:47:50.120
<v Speaker 1>a certain kind of signature. One of the things that

0:47:50.160 --> 0:47:53.240
<v Speaker 1>we could observe about a Dicen sphere is that if

0:47:53.440 --> 0:47:56.880
<v Speaker 1>it completely surrounded a star and turned all of the

0:47:56.920 --> 0:48:01.319
<v Speaker 1>stars solar radiation into usable in gy that could be

0:48:01.400 --> 0:48:04.560
<v Speaker 1>used by the civilization somehow to survive after all, that,

0:48:04.600 --> 0:48:06.640
<v Speaker 1>it would have to have a waste product, which would

0:48:06.640 --> 0:48:09.080
<v Speaker 1>be heat, which we would be able to see as

0:48:09.160 --> 0:48:13.520
<v Speaker 1>infrared radiation, like submillimeter infrared radiation. And so if you

0:48:13.560 --> 0:48:16.840
<v Speaker 1>see like darkened stars out there that are not producing

0:48:16.880 --> 0:48:19.080
<v Speaker 1>any kind of light you can see, but are producing

0:48:19.120 --> 0:48:22.080
<v Speaker 1>infrared radiation and the certain kind of with a certain

0:48:22.160 --> 0:48:26.040
<v Speaker 1>kind of band, you've gotta wondering, is this just a

0:48:26.200 --> 0:48:30.720
<v Speaker 1>giant hot ball that's taken everything a son's got, using

0:48:30.719 --> 0:48:34.560
<v Speaker 1>it and then spitting some heat into space. Now, because

0:48:34.680 --> 0:48:37.200
<v Speaker 1>sons and stars are already plentiful and they're already a

0:48:37.280 --> 0:48:39.840
<v Speaker 1>great source of energy. I think it is a fairly

0:48:40.000 --> 0:48:43.239
<v Speaker 1>safe assumption to think that if there is a galactic

0:48:43.280 --> 0:48:46.279
<v Speaker 1>civilization anywhere, will try to make use of something like

0:48:46.360 --> 0:48:49.840
<v Speaker 1>a dicensephere, maybe not exactly the original design, but he

0:48:49.960 --> 0:48:53.640
<v Speaker 1>will try to use stars as an energy source to

0:48:53.719 --> 0:48:57.960
<v Speaker 1>sustain the civilization and feed its people and power its

0:48:58.000 --> 0:49:00.319
<v Speaker 1>machines and do all that kind of stuff. And they're

0:49:00.320 --> 0:49:03.200
<v Speaker 1>gonna need more than one. Yeah, and as the civilization

0:49:03.239 --> 0:49:06.120
<v Speaker 1>scales up, it will need more and more energy needs

0:49:06.160 --> 0:49:10.400
<v Speaker 1>scale up with population increasing. So what if your galaxy

0:49:10.600 --> 0:49:14.920
<v Speaker 1>runs short on stars? You've got them all sphered up,

0:49:15.880 --> 0:49:18.680
<v Speaker 1>all the usable ones, and you're getting all the energy

0:49:18.719 --> 0:49:21.160
<v Speaker 1>you need from them, but your population is still growing.

0:49:21.800 --> 0:49:23.680
<v Speaker 1>What do you do then? Yeah? I mean you're essentially

0:49:23.760 --> 0:49:26.400
<v Speaker 1>using all of your farmland here to produce the crops

0:49:26.400 --> 0:49:29.440
<v Speaker 1>that are necessary for life, or that the model of

0:49:29.480 --> 0:49:31.960
<v Speaker 1>life that you've built. And uh, yeah, what what do

0:49:32.000 --> 0:49:34.160
<v Speaker 1>you do when you maxed out? And then what do

0:49:34.160 --> 0:49:36.120
<v Speaker 1>you do when say one of the stars blinks out

0:49:36.120 --> 0:49:39.279
<v Speaker 1>on you? Uh, You're gonna have to scale back on

0:49:39.360 --> 0:49:41.719
<v Speaker 1>what you can do as an empire. Stars also have

0:49:41.800 --> 0:49:44.800
<v Speaker 1>finite lifespans. You eventually are going to need new stars

0:49:44.800 --> 0:49:47.600
<v Speaker 1>to replace the old ones that are that are running

0:49:47.600 --> 0:49:49.799
<v Speaker 1>down their fuel. Now, one thing you could do is

0:49:49.840 --> 0:49:53.800
<v Speaker 1>just continually keep expanding, right, You could expand other galaxies.

0:49:53.880 --> 0:49:56.120
<v Speaker 1>I mean, this is this is very crazy and very

0:49:56.120 --> 0:49:58.719
<v Speaker 1>far future, because we don't have anything like the ability

0:49:58.760 --> 0:50:01.319
<v Speaker 1>to travel to another gal see today. But if you

0:50:01.360 --> 0:50:04.680
<v Speaker 1>imagine one of these Cardashev three type civilizations that has

0:50:04.760 --> 0:50:08.400
<v Speaker 1>mastered in an entire galaxy, it could spread to other galaxies.

0:50:08.440 --> 0:50:11.680
<v Speaker 1>It could keep on expanding. But we're limited to our

0:50:11.760 --> 0:50:14.880
<v Speaker 1>local group right now. Because if you imagine just trying

0:50:14.880 --> 0:50:19.160
<v Speaker 1>to continue expanding to other galaxies beyond into the far future,

0:50:19.480 --> 0:50:21.560
<v Speaker 1>you would eventually come up against the problem we were

0:50:21.560 --> 0:50:25.480
<v Speaker 1>mentioning earlier, the cosmological horizon problem. That's right, because even

0:50:25.560 --> 0:50:27.880
<v Speaker 1>if you imagine and that releast is what I'm imagining,

0:50:27.960 --> 0:50:30.800
<v Speaker 1>is that you know, just cosmic marauders. And this is

0:50:30.840 --> 0:50:34.680
<v Speaker 1>something that is Hawking has has touched on himself. Uh,

0:50:34.680 --> 0:50:36.400
<v Speaker 1>and to a certain extent I think was touched on

0:50:36.480 --> 0:50:39.400
<v Speaker 1>and that uh in the film Chronicles of Riddic and

0:50:39.440 --> 0:50:41.839
<v Speaker 1>that it's kind of what the necromongers were doing, right.

0:50:42.360 --> 0:50:44.160
<v Speaker 1>I don't think they're doing it with stars. But you know,

0:50:44.200 --> 0:50:47.960
<v Speaker 1>they had the whole kind of like life sucking undead um,

0:50:48.520 --> 0:50:51.839
<v Speaker 1>you know, ravager kind of thing going on. I mean

0:50:51.880 --> 0:50:54.040
<v Speaker 1>I never saw Chronicles. Well, yeah, you've got to see it.

0:50:54.040 --> 0:50:57.040
<v Speaker 1>I've seen Pitch Black at your recommendation. Well, that's the

0:50:57.200 --> 0:51:00.239
<v Speaker 1>necessary precursor to Chronicles of Riddic. You should see it.

0:51:00.280 --> 0:51:03.600
<v Speaker 1>Is Keith David in it? Yes, okay, yeah, it's it's

0:51:03.640 --> 0:51:07.000
<v Speaker 1>it's fun. It's fun. But yeah, I'm picturing a marauding

0:51:07.320 --> 0:51:11.200
<v Speaker 1>um interstellar civilization. It just goes from one system to

0:51:11.239 --> 0:51:14.240
<v Speaker 1>the next, using up sons and then spitting them out again.

0:51:14.440 --> 0:51:16.719
<v Speaker 1>But eventually they're going to reach that point where there

0:51:16.760 --> 0:51:20.799
<v Speaker 1>are no new sons to conquer. And Alexander wept where

0:51:20.800 --> 0:51:22.759
<v Speaker 1>there were no worlds to conquer. Yeah, and then you're

0:51:22.800 --> 0:51:25.640
<v Speaker 1>just left to uh just stew in the in the

0:51:25.960 --> 0:51:29.640
<v Speaker 1>cosmic darkness. Uh So, if we're gonna keep expanding, we

0:51:29.719 --> 0:51:33.120
<v Speaker 1>need stars, and if we run out of local stars,

0:51:33.560 --> 0:51:35.880
<v Speaker 1>we're gonna have to get him from somewhere else. And

0:51:35.960 --> 0:51:39.840
<v Speaker 1>Hooper writes, quote over the next approximately one billion years,

0:51:40.160 --> 0:51:44.800
<v Speaker 1>so basically times the age of the Earth. He writes,

0:51:45.080 --> 0:51:48.920
<v Speaker 1>all stars residing beyond the local group will fall beyond

0:51:49.120 --> 0:51:54.640
<v Speaker 1>the cosmic horizon and become not only unobservable but entirely inaccessible.

0:51:55.200 --> 0:51:57.600
<v Speaker 1>So he's saying, like, we're going to run out of

0:51:57.719 --> 0:52:01.440
<v Speaker 1>time if if you know, a civilization doesn't do something

0:52:01.520 --> 0:52:03.480
<v Speaker 1>early on, it's going to run out of time to

0:52:03.560 --> 0:52:06.360
<v Speaker 1>get at all those extra stars to give them, to

0:52:06.400 --> 0:52:09.840
<v Speaker 1>give them more energy. So you've got stars speeding away,

0:52:09.880 --> 0:52:12.040
<v Speaker 1>how do you make use of them for the future.

0:52:12.280 --> 0:52:15.120
<v Speaker 1>Hooper has an idea. What if you go out to

0:52:15.160 --> 0:52:18.799
<v Speaker 1>those stars, you go snag them, and then you use

0:52:18.920 --> 0:52:22.520
<v Speaker 1>the Dyson's fears that you build around them as a drive.

0:52:23.120 --> 0:52:26.600
<v Speaker 1>We talked earlier about the idea of scattow thrusters and

0:52:26.680 --> 0:52:29.560
<v Speaker 1>things like that. What if you used a Dyson sphere

0:52:29.680 --> 0:52:34.720
<v Speaker 1>to steer and drive a star back home to where

0:52:34.800 --> 0:52:39.080
<v Speaker 1>your civilization is, so that you can hoard stars from

0:52:39.160 --> 0:52:43.279
<v Speaker 1>the entire universe at large and keep them nearby to

0:52:43.520 --> 0:52:46.399
<v Speaker 1>use them for the future before they go beyond your

0:52:46.440 --> 0:52:49.320
<v Speaker 1>cosmic reach. I think we should call this star jacking.

0:52:49.920 --> 0:52:52.080
<v Speaker 1>That's what it sounds like to me. It's star hoarding.

0:52:53.200 --> 0:52:56.280
<v Speaker 1>And so the the emitted radiation from a star could

0:52:56.280 --> 0:52:59.120
<v Speaker 1>provide some thrust which could be used at least in theory,

0:52:59.160 --> 0:53:01.080
<v Speaker 1>to steer a star are and it s Dyson's fear

0:53:01.120 --> 0:53:05.239
<v Speaker 1>in a particular direction, meaning that you know, this civilization

0:53:05.239 --> 0:53:08.160
<v Speaker 1>could gather stars close together and keep them from expanding

0:53:08.160 --> 0:53:10.960
<v Speaker 1>out of reach and great leaks in the lifespan of

0:53:11.000 --> 0:53:13.920
<v Speaker 1>their civilization. But there are limits on this, and a

0:53:13.960 --> 0:53:17.920
<v Speaker 1>lot of Hooper's paper is used to calculate types of

0:53:18.040 --> 0:53:21.400
<v Speaker 1>stars that would be fruitful for this. Only certain types

0:53:21.440 --> 0:53:25.160
<v Speaker 1>of stars would work, mainly stars somewhat within the range

0:53:25.239 --> 0:53:28.120
<v Speaker 1>of the mass of our Sun, because stars that are

0:53:28.200 --> 0:53:31.319
<v Speaker 1>much bigger tend to be older or tend to not

0:53:31.400 --> 0:53:33.960
<v Speaker 1>have as much life left in them. Yeah, you don't

0:53:33.960 --> 0:53:35.680
<v Speaker 1>want to go to the trouble of Jack and those

0:53:35.719 --> 0:53:38.480
<v Speaker 1>stars if they're just going to burn out or collapse

0:53:38.560 --> 0:53:40.560
<v Speaker 1>before you can make use of them exactly. So this

0:53:40.640 --> 0:53:43.359
<v Speaker 1>is a problem. The bigger stars would not have enough

0:53:43.400 --> 0:53:46.000
<v Speaker 1>life left in them to survive the journey back to

0:53:46.160 --> 0:53:49.000
<v Speaker 1>the home base, and so they're not really worth hoarding.

0:53:49.400 --> 0:53:51.920
<v Speaker 1>On the other hand, stars much smaller than our Sun

0:53:52.000 --> 0:53:55.560
<v Speaker 1>would not provide enough energy to drive the star to

0:53:55.680 --> 0:53:59.720
<v Speaker 1>its central star Hoarde fast enough before it passed beyond

0:53:59.840 --> 0:54:02.440
<v Speaker 1>the cosmic horizon, and so there is kind of a

0:54:02.440 --> 0:54:06.040
<v Speaker 1>Goldilocks star. You know, a Goldilocks star that you want

0:54:06.120 --> 0:54:08.480
<v Speaker 1>that that is big enough to give you enough energy,

0:54:08.920 --> 0:54:11.120
<v Speaker 1>that's small enough that it's still going to have plenty

0:54:11.160 --> 0:54:12.839
<v Speaker 1>of life left in it by the time you get

0:54:12.880 --> 0:54:16.560
<v Speaker 1>at home, And that's the kind you want to bring home. Interestingly,

0:54:17.040 --> 0:54:20.480
<v Speaker 1>Hooper points out that if alien civilizations anywhere out there

0:54:20.520 --> 0:54:24.120
<v Speaker 1>are doing this quote, this would not be a subtle activity,

0:54:25.600 --> 0:54:27.480
<v Speaker 1>so we should be able to detect it. Kind of

0:54:27.520 --> 0:54:30.440
<v Speaker 1>like the original idea of the Dicen sphere. If anybody

0:54:30.440 --> 0:54:33.040
<v Speaker 1>out there is doing anything like this, you've got a

0:54:33.080 --> 0:54:36.399
<v Speaker 1>galactic civilization in one of those galaxies far out there,

0:54:36.800 --> 0:54:39.840
<v Speaker 1>and it's making these kinds of preparations for the future.

0:54:40.239 --> 0:54:42.839
<v Speaker 1>This could give us a new path to setty observation.

0:54:43.160 --> 0:54:45.680
<v Speaker 1>Can we look out at galaxies out there and detect

0:54:45.760 --> 0:54:50.839
<v Speaker 1>the removal, transport, and hoarding of certain kinds of stars? Yeah,

0:54:50.840 --> 0:54:52.439
<v Speaker 1>I mean it makes it makes sense. Like you said,

0:54:52.440 --> 0:54:54.200
<v Speaker 1>this would not be a subtle act. This would be

0:54:54.239 --> 0:54:55.960
<v Speaker 1>the kind of thing that we would conceive will be

0:54:56.040 --> 0:54:58.960
<v Speaker 1>able to observe. Yeah, and so Hooper writes, quote, such

0:54:59.000 --> 0:55:02.120
<v Speaker 1>a civilization could pier as a region up to tens

0:55:02.200 --> 0:55:05.319
<v Speaker 1>of mega par sex and radius in which most or

0:55:05.360 --> 0:55:08.400
<v Speaker 1>all of the stars lighter than about two solar masses

0:55:08.719 --> 0:55:12.839
<v Speaker 1>are surrounded by Dyson's fears. Now that's a cool image. Yes,

0:55:13.719 --> 0:55:16.480
<v Speaker 1>the star hoarde, the star hoard Yeah, there the empire

0:55:16.520 --> 0:55:19.640
<v Speaker 1>of the star hoarders or star jackers, which whichever one,

0:55:19.760 --> 0:55:22.040
<v Speaker 1>whichever one you want to use. Star jacking is the verb,

0:55:22.200 --> 0:55:24.640
<v Speaker 1>the star hoarde is the Now the star jackers work

0:55:24.719 --> 0:55:27.920
<v Speaker 1>for the star hoarders. Yeah, and then our only hope

0:55:27.960 --> 0:55:30.480
<v Speaker 1>is to just, I guess, somehow present a case that

0:55:30.560 --> 0:55:34.840
<v Speaker 1>we're we're worth keeping around, like we're culturally interesting enough,

0:55:35.480 --> 0:55:37.600
<v Speaker 1>or maybe they have rules. Maybe they don't take stars

0:55:37.640 --> 0:55:40.360
<v Speaker 1>from systems with the inhabited worlds. I don't know, I

0:55:40.400 --> 0:55:44.880
<v Speaker 1>could go virtually anyway. Yeah, maybe they only use stars

0:55:44.920 --> 0:55:49.279
<v Speaker 1>from inhabited worlds. Now, of course, with an idea this

0:55:49.600 --> 0:55:52.080
<v Speaker 1>far out there, you at least want to hear what

0:55:52.200 --> 0:55:55.040
<v Speaker 1>some other scientists in the field have to say. Fortunately,

0:55:55.040 --> 0:55:56.840
<v Speaker 1>there was a right of this in Science News that

0:55:56.920 --> 0:56:00.520
<v Speaker 1>got some quotes from some other astrophysicists, for example, the

0:56:00.520 --> 0:56:04.799
<v Speaker 1>theoretical astrophysicist Katie Mack of North Carolina State University. They

0:56:04.840 --> 0:56:06.920
<v Speaker 1>asked her opinion and She pointed out that, you know,

0:56:07.600 --> 0:56:10.520
<v Speaker 1>one thing is that you might have an easier time

0:56:10.560 --> 0:56:13.759
<v Speaker 1>surviving if you just uproot your civilization and move it

0:56:13.800 --> 0:56:16.600
<v Speaker 1>to a different galaxy cluster that's got a bunch of

0:56:16.600 --> 0:56:19.719
<v Speaker 1>different stars you could use. So instead of bringing all

0:56:19.719 --> 0:56:23.080
<v Speaker 1>the stars to you, you just go where they're already are,

0:56:23.200 --> 0:56:27.040
<v Speaker 1>a whole bunch of already untapped stars the Marauder model, Yeah,

0:56:27.520 --> 0:56:31.000
<v Speaker 1>and settle in there. But then again, you know, maybe

0:56:31.040 --> 0:56:33.120
<v Speaker 1>they maybe there are reasons they want to stay where

0:56:33.120 --> 0:56:36.080
<v Speaker 1>they are. It might be easier to send out autonomous

0:56:36.160 --> 0:56:40.640
<v Speaker 1>star collection, you know, robots that would build Dyson's fears

0:56:40.640 --> 0:56:42.480
<v Speaker 1>around stars and bring them home than it would be

0:56:42.520 --> 0:56:46.200
<v Speaker 1>to move the conscious inhabitants of a place. Maybe they

0:56:46.280 --> 0:56:50.239
<v Speaker 1>like where they are and the movement would be stressful. Yeah,

0:56:50.320 --> 0:56:52.600
<v Speaker 1>I mean, ultimately, who's going to argue with them? Right? Right?

0:56:52.880 --> 0:56:54.520
<v Speaker 1>Because they would be where would they be on the

0:56:54.560 --> 0:56:58.720
<v Speaker 1>Kardashi of scale, they would be between two and three,

0:56:58.800 --> 0:57:00.640
<v Speaker 1>Perhaps they would be threes. I don't know, three, it's

0:57:00.680 --> 0:57:03.719
<v Speaker 1>pretty lofty. Oh yeah, I think we're talking about a

0:57:03.800 --> 0:57:08.160
<v Speaker 1>level three cardship civilization right here. You're you're controlling a galaxy.

0:57:08.160 --> 0:57:10.400
<v Speaker 1>If you're going out to other galaxies to get stars

0:57:10.480 --> 0:57:13.080
<v Speaker 1>to bring home. Yeah, yeah, you would be Yeah, so

0:57:13.120 --> 0:57:15.520
<v Speaker 1>I guess you would be a little beyond three. You

0:57:15.560 --> 0:57:19.200
<v Speaker 1>would be up towards us. You would be moving towards four. Whatever.

0:57:19.360 --> 0:57:21.960
<v Speaker 1>Four would be like if we can even comprehend such

0:57:21.960 --> 0:57:24.800
<v Speaker 1>a thing, a mastery of the local group or something.

0:57:25.440 --> 0:57:29.479
<v Speaker 1>The physicist Avy Loeb of Harvard University also points out

0:57:29.840 --> 0:57:32.400
<v Speaker 1>the same issue that you know, it might not be

0:57:32.560 --> 0:57:36.240
<v Speaker 1>necessary to go get stars from other places, because he says, quote,

0:57:36.320 --> 0:57:38.960
<v Speaker 1>nature did it for us. You've already got There are

0:57:38.960 --> 0:57:42.320
<v Speaker 1>places in the universe where they're huge clusters of galaxies

0:57:42.360 --> 0:57:44.680
<v Speaker 1>that are all sort of near by each other, and

0:57:44.760 --> 0:57:46.440
<v Speaker 1>maybe it would be better to go to one of

0:57:46.440 --> 0:57:49.720
<v Speaker 1>those galaxy clusters that's got lots of stars already there.

0:57:49.760 --> 0:57:53.120
<v Speaker 1>I mean, it's it's a relative lots of stars, because

0:57:53.280 --> 0:57:55.520
<v Speaker 1>there are lots of stars in our galaxy. But if

0:57:55.520 --> 0:57:58.400
<v Speaker 1>you're talking about this Cardassian you know, three point five

0:57:58.480 --> 0:58:01.960
<v Speaker 1>or four type civilization and it's got ridiculous energy needs,

0:58:02.440 --> 0:58:04.600
<v Speaker 1>then there are places you could go that would have

0:58:04.680 --> 0:58:07.800
<v Speaker 1>more stars nearby already. Right. And again this is assuming

0:58:07.840 --> 0:58:09.600
<v Speaker 1>they don't say, you know, guys, this is a bit nach.

0:58:09.680 --> 0:58:12.439
<v Speaker 1>We don't need this much energy, let's scale back a bit. Yeah,

0:58:12.480 --> 0:58:14.600
<v Speaker 1>But then again, our tribal ancestors could have said that

0:58:14.640 --> 0:58:16.640
<v Speaker 1>about our world today and now here we are and

0:58:16.680 --> 0:58:19.720
<v Speaker 1>we need the energy. True though there we do, see,

0:58:20.360 --> 0:58:22.600
<v Speaker 1>I mean, there obviously is a movement to cut back

0:58:22.960 --> 0:58:27.280
<v Speaker 1>on energy to find more sustainable ways. Uh you know,

0:58:27.320 --> 0:58:30.320
<v Speaker 1>whether that will that argument will win out in the end,

0:58:30.520 --> 0:58:34.760
<v Speaker 1>uh you know, remains an open question. But um, well,

0:58:34.800 --> 0:58:37.160
<v Speaker 1>I would say, I don't know. Maybe maybe you can

0:58:37.240 --> 0:58:38.720
<v Speaker 1>make the case to me, I don't know if any

0:58:38.720 --> 0:58:41.320
<v Speaker 1>good reason that we need to cut back on energy

0:58:41.680 --> 0:58:45.040
<v Speaker 1>itself is just like types of energy, you know, certain

0:58:45.040 --> 0:58:47.600
<v Speaker 1>types of energy are more destructive than others. And if

0:58:47.640 --> 0:58:50.360
<v Speaker 1>we had a truly I mean, I think there is

0:58:50.400 --> 0:58:53.920
<v Speaker 1>no such thing as a perfect energy source, because even

0:58:54.000 --> 0:58:57.600
<v Speaker 1>the most benign forms of energy maybe solar, wind power,

0:58:57.680 --> 0:59:00.560
<v Speaker 1>whatever you have, have some kinds of construction and costs

0:59:00.560 --> 0:59:04.800
<v Speaker 1>and stuff to build the panels. Um. But but there

0:59:04.800 --> 0:59:08.200
<v Speaker 1>are relatively benign forms of energy that I don't I

0:59:08.240 --> 0:59:10.560
<v Speaker 1>don't know. Is there an argument that we shouldn't even

0:59:10.600 --> 0:59:14.720
<v Speaker 1>be trying to maximize our collection of solar energy or something? No?

0:59:14.920 --> 0:59:17.280
<v Speaker 1>I mean it kind of comes down to though, to

0:59:17.440 --> 0:59:21.960
<v Speaker 1>like how much energy can we conceivably harvest? And then

0:59:22.200 --> 0:59:25.120
<v Speaker 1>how are we living our lives in accordance to it?

0:59:25.240 --> 0:59:28.960
<v Speaker 1>You know? Um? So I yeah, I don't see anybody

0:59:28.960 --> 0:59:33.880
<v Speaker 1>as saying let's stop harvesting energy, but but also asking

0:59:33.920 --> 0:59:37.320
<v Speaker 1>the question, is our consumption lining up with our current

0:59:37.400 --> 0:59:40.520
<v Speaker 1>and even near future ability to harvest it? Maybe the

0:59:40.560 --> 0:59:44.000
<v Speaker 1>answer to that is no, right, yeah, but but it's

0:59:44.000 --> 0:59:49.080
<v Speaker 1>certainly based on our own model of intelligent um technological behavior,

0:59:49.240 --> 0:59:52.320
<v Speaker 1>it makes sense that uh, an alien species, we just

0:59:52.360 --> 0:59:57.000
<v Speaker 1>continue to jack as many stars as as as possible

0:59:57.160 --> 1:00:00.880
<v Speaker 1>to sustain itself. I mean, I I like I was

1:00:00.920 --> 1:00:03.439
<v Speaker 1>saying earlier, I think we want to avoid making too

1:00:03.440 --> 1:00:07.919
<v Speaker 1>many assumptions about future civilizations or alien life, because there's

1:00:07.960 --> 1:00:10.360
<v Speaker 1>a lot we just can't know about their minds, about

1:00:10.360 --> 1:00:13.120
<v Speaker 1>their culture and all that. But one thing we pretty

1:00:13.200 --> 1:00:15.960
<v Speaker 1>much know no matter what is they need energy. Yes,

1:00:16.240 --> 1:00:18.040
<v Speaker 1>but I'm saying they could scale back if they if

1:00:18.080 --> 1:00:21.840
<v Speaker 1>they really wanted to. I mean, it's I think that

1:00:22.000 --> 1:00:24.920
<v Speaker 1>is a possibility. And certainly if they see the writing

1:00:24.920 --> 1:00:27.720
<v Speaker 1>on the wall, you know that that energy is going

1:00:27.760 --> 1:00:31.160
<v Speaker 1>to become less abundant, and then it's about survival. Now,

1:00:31.200 --> 1:00:34.640
<v Speaker 1>speaking of survival, um, I do have one last survival

1:00:34.680 --> 1:00:36.880
<v Speaker 1>scheme dimension here, and this one was exploring in that

1:00:36.920 --> 1:00:40.960
<v Speaker 1>Adam Becker BBC article their referenced earlier. Alan Gooth of

1:00:41.080 --> 1:00:44.000
<v Speaker 1>m I T contends that the laws of physics might

1:00:44.560 --> 1:00:48.400
<v Speaker 1>imply that that this is possible, uh, that you could

1:00:48.640 --> 1:00:52.920
<v Speaker 1>essentially escape into a universe of your own making. Yeah. Now,

1:00:52.920 --> 1:00:56.800
<v Speaker 1>it would require vast amounts of energy, which of course

1:00:56.880 --> 1:00:59.560
<v Speaker 1>is we're discussing the players in this kind of game

1:00:59.600 --> 1:01:02.000
<v Speaker 1>would have have. But it might go down like this.

1:01:02.240 --> 1:01:04.280
<v Speaker 1>First of all, you need to create an incredibly dense

1:01:04.320 --> 1:01:08.000
<v Speaker 1>form of matter, so dense that it barely avoids collapsing

1:01:08.000 --> 1:01:11.520
<v Speaker 1>into a black hole, and you quickly clear the matter

1:01:11.560 --> 1:01:14.000
<v Speaker 1>out of the way, forcing the region of space to

1:01:14.080 --> 1:01:17.640
<v Speaker 1>start expanding, and this would jump start, in theory a

1:01:17.640 --> 1:01:21.160
<v Speaker 1>new universe. Quote. As the space in the region expanded,

1:01:21.200 --> 1:01:24.680
<v Speaker 1>the boundary would shrink, creating a bubble of warped space

1:01:24.960 --> 1:01:29.400
<v Speaker 1>where the inside was bigger than the outside, which is

1:01:29.480 --> 1:01:31.520
<v Speaker 1>kind of like it reminds me of the bag of

1:01:31.560 --> 1:01:34.720
<v Speaker 1>holding from Dungeons and Dragons. The Gooth actually compared it

1:01:34.760 --> 1:01:37.720
<v Speaker 1>to the tartest dr who looked it looks bigger on

1:01:37.720 --> 1:01:39.640
<v Speaker 1>the inside. Yeah, yeah, and they on the outside it's

1:01:39.680 --> 1:01:41.600
<v Speaker 1>what a phone phone booth, and then on the inside

1:01:41.600 --> 1:01:45.160
<v Speaker 1>it's this large, expensive room and so forth. So eventually

1:01:45.160 --> 1:01:48.560
<v Speaker 1>the new universe would pinch off from the old doomed universe.

1:01:49.360 --> 1:01:52.400
<v Speaker 1>But he stresses that this might not be possible at all. Sure,

1:01:52.480 --> 1:01:55.680
<v Speaker 1>it depends on a lot of assumptions that could be true,

1:01:56.000 --> 1:01:58.440
<v Speaker 1>but we don't know for sure. But then also the

1:01:58.440 --> 1:02:00.840
<v Speaker 1>other way of looking at things, he says, is it, Uh,

1:02:00.920 --> 1:02:03.800
<v Speaker 1>you know, if if the multiverse model holds true, then

1:02:03.840 --> 1:02:06.200
<v Speaker 1>that's probably our best bet. The universe may end, but

1:02:06.280 --> 1:02:10.760
<v Speaker 1>the multiverse continues eternally. No way that that might mean

1:02:10.800 --> 1:02:14.440
<v Speaker 1>though we can't get there, just some other version of us. Yeah,

1:02:14.520 --> 1:02:16.400
<v Speaker 1>and but that might be the best we can you know,

1:02:16.600 --> 1:02:18.240
<v Speaker 1>for in the end is just to realize, all right,

1:02:18.640 --> 1:02:22.479
<v Speaker 1>we've we've we've jacked a thousand stars, we've hoarded them,

1:02:22.760 --> 1:02:25.600
<v Speaker 1>we've done what we can. But hey, the writings on

1:02:25.640 --> 1:02:28.560
<v Speaker 1>the wall, we're gonna blink out. But somewhere out there

1:02:28.600 --> 1:02:31.920
<v Speaker 1>in the multiverse, Uh, this thing called life is still going.

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<v Speaker 1>I believe in the thing called technological civilization. One final

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<v Speaker 1>note is a side tangent. Well, one thing I loved

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<v Speaker 1>about the Freeman diys in paper we talked about earlier

1:02:41.160 --> 1:02:45.760
<v Speaker 1>from seventy nine, is that at the end he invokes holdings, uh,

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<v Speaker 1>quoting of of G. K. Chesterton on the role of

1:02:48.720 --> 1:02:53.480
<v Speaker 1>human intellect in the future of of of civilization quoting

1:02:53.560 --> 1:02:56.120
<v Speaker 1>from the Ballot of the White Horse by Chesterton, where

1:02:56.120 --> 1:02:59.000
<v Speaker 1>he writes, so rides my soul upon the sea that

1:02:59.120 --> 1:03:02.880
<v Speaker 1>drinks the howling ships, though in black jest at bows

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<v Speaker 1>and nods under the moons with silver rods. I know

1:03:06.680 --> 1:03:10.040
<v Speaker 1>it is roaring at the gods waiting the last eclipse.

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<v Speaker 1>Oh that's nice. So maybe find peaceful ways to survive

1:03:13.560 --> 1:03:15.880
<v Speaker 1>that last eclipse. All right, So there you have it.

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<v Speaker 1>If you want to hear more episodes like this dealing

1:03:19.760 --> 1:03:24.200
<v Speaker 1>with the the long term future of humanity and this

1:03:24.720 --> 1:03:29.040
<v Speaker 1>universe of change and hostility, uh, then you can check

1:03:29.040 --> 1:03:30.600
<v Speaker 1>out all the episodes of Stuff to Blow Your Mind

1:03:30.600 --> 1:03:32.240
<v Speaker 1>at Stuff to Blow your Mind dot com. That's the

1:03:32.280 --> 1:03:35.280
<v Speaker 1>mother ship. That's where you'll also find social media links

1:03:35.320 --> 1:03:39.640
<v Speaker 1>to our Facebook, Twitter, Instagram, you name it. Huge things

1:03:39.760 --> 1:03:42.960
<v Speaker 1>as always to our wonderful audio producers Alex Williams and

1:03:43.000 --> 1:03:45.120
<v Speaker 1>Tary Harrison. If you want to get in touch with

1:03:45.200 --> 1:03:47.360
<v Speaker 1>us to let us know feedback on this episode or

1:03:47.400 --> 1:03:50.400
<v Speaker 1>any other, or to suggest a topic for future episodes,

1:03:50.520 --> 1:03:52.520
<v Speaker 1>or just to say hi, let us know where you

1:03:52.600 --> 1:03:55.280
<v Speaker 1>listen from. You can email us at blow the Mind

1:03:55.320 --> 1:03:57.720
<v Speaker 1>at how Stuff Works dot com. And I want to

1:03:57.760 --> 1:04:00.560
<v Speaker 1>close out here with a really cool tray guy came

1:04:00.600 --> 1:04:05.280
<v Speaker 1>across from the group We Plants Are Happy Plants, titled

1:04:05.360 --> 1:04:08.720
<v Speaker 1>an Incredible Pearl, which makes use of a passage from

1:04:08.760 --> 1:04:12.880
<v Speaker 1>American writer philosopher in ethnobotanist Terrence McKenna, who who we

1:04:12.960 --> 1:04:14.640
<v Speaker 1>discussed on the show in the past. Kind of a

1:04:14.640 --> 1:04:17.880
<v Speaker 1>wizard figure. Yeah yeah, so, uh so check this out.

1:04:17.920 --> 1:04:19.880
<v Speaker 1>If you want to hear more from We Plants Are

1:04:19.880 --> 1:04:23.960
<v Speaker 1>Happy Plants to simply look them up on Spotify or iTunes,

1:04:24.040 --> 1:04:26.120
<v Speaker 1>wherever you get your music. You can also go to

1:04:26.320 --> 1:04:30.040
<v Speaker 1>YouTube dot com, slash w P a h P. We're

1:04:30.080 --> 1:04:33.000
<v Speaker 1>going to have to make a decision about human nature

1:04:34.400 --> 1:04:41.360
<v Speaker 1>to wit. Is this our home to be cherished and nurtured,

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<v Speaker 1>an incredible pearl flung out in a universe of ashes

1:04:46.320 --> 1:04:51.960
<v Speaker 1>and darkness? Or is this a hell world, a tiny,

1:04:52.120 --> 1:04:56.040
<v Speaker 1>confining prison at the edge of a dying universe from

1:04:56.080 --> 1:04:59.640
<v Speaker 1>which it is our destiny to break free and recover

1:04:59.760 --> 1:05:04.000
<v Speaker 1>our higher and hidden nature from which we have become separated.

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<v Speaker 1>You know, this is a choice which as a culture

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<v Speaker 1>we face. Are we to go into the divine imagination

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<v Speaker 1>and create you know, starships the size of Manitoba that

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<v Speaker 1>will apply between here and Andrama and exist in a

1:05:23.600 --> 1:05:30.360
<v Speaker 1>world of our complete syntactical self expression. Or is man's

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<v Speaker 1>place humbler than that? Is that grandiose steeped with megalomania,

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<v Speaker 1>touched with the kind of political taint that's had this

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<v Speaker 1>raping and pillaging ever since we got out of those

1:05:45.200 --> 1:05:49.320
<v Speaker 1>miserable ice bound villages in Jutland or wherever it was.

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<v Speaker 1>Is it that? Or is it our challenge and our destiny?

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<v Speaker 1>It's really a choice about human nature.