WEBVTT - Shkadov Thrusters: Moving the Solar System

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<v Speaker 1>Brought to you by Toyota. Let's go places. Welcome to

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<v Speaker 1>Forward Thinking. Hello, and welcome to Forward Thinking, the podcast

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<v Speaker 1>that looks at the future and says, but it's the

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<v Speaker 1>scatter of thrust that really drives you insane. I'm Joe

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<v Speaker 1>McCormick and I'm Lauren bulk Obama, and our regular host

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<v Speaker 1>Jonathan Strickland is not with us today because he is

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<v Speaker 1>out in the field on assignment. Yes, doing things that

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<v Speaker 1>we cannot tell you about yet. No. I would say

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<v Speaker 1>that he's out discovering the amazing technology of tomorrow. But

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<v Speaker 1>really what he's probably doing is posing for selfies with

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<v Speaker 1>very muscular men. Yes, that is entirely likely. You can

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<v Speaker 1>watch the House Stuff Works dot Com channel on YouTube

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<v Speaker 1>to find out more about that in a few weeks. Yeah,

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<v Speaker 1>so today we wanted to address a listener request episode.

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<v Speaker 1>Our listener, Keith on Facebook, has asked us to talk

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<v Speaker 1>about all kinds of topics and we can't do them

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<v Speaker 1>all at once, so we decided to pick the coolest,

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<v Speaker 1>weirdest one of the bunch, being Stellar Engines. Stellar Engines.

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<v Speaker 1>Now I know what the gearheads and the audience are thinking.

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<v Speaker 1>Cadillac V eight right, the classic Cadillac V eight Stellar

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<v Speaker 1>out of this world? Right? Yeah? Oh man, they don't

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<v Speaker 1>make them like that anymore, or I don't know, they

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<v Speaker 1>might still make those spoiler alert, I don't know anything

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<v Speaker 1>about cars, um, But no, the use of the word

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<v Speaker 1>stellar here actually refers to the more classical sense, as

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<v Speaker 1>in stars. Yes, stars turned into engines. Put to our

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<v Speaker 1>own devious uses, what would a star based engine even be? Um?

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<v Speaker 1>As it turns out, it's real complicated, y'all, And it's

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<v Speaker 1>really weird and really really cool. This is one of

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<v Speaker 1>the coolest ideas I think we've looked at in a while.

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<v Speaker 1>And it's also kind of cool because it's not even

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<v Speaker 1>close to reality. So this is going to be one

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<v Speaker 1>of our more on the speculative end. So yeah, this

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<v Speaker 1>is not one of those like twenty to forty year

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<v Speaker 1>kind of things that we usually wind up talking about

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<v Speaker 1>on the show. This is so far out there thousand

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<v Speaker 1>years in the optimistic sense. So, okay, let us talk

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<v Speaker 1>about interstellar travel. Sure, well, we all know that one

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<v Speaker 1>day we may want or even need to travel to

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<v Speaker 1>another solar system. And what's wrong with our solar system? Joe? Well,

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<v Speaker 1>you know, it's just in our Solar system. You get

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<v Speaker 1>board being in the same place for a long time.

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<v Speaker 1>I know, after a while, just seeing the same planets

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<v Speaker 1>going around and around over and over. Don't you ever

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<v Speaker 1>get tired of Mars? Yeah? Yeah, you get that interstellar

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<v Speaker 1>wonder lust. Well, it's not just boredom and uh and

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<v Speaker 1>discontent that might make us want to look to another

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<v Speaker 1>solar system in our galaxy solar on we over time,

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<v Speaker 1>our son is going to get into some trouble. Have

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<v Speaker 1>you heard about this? H Well, I mean it's pretty

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<v Speaker 1>much a bad seed. Yeah. Well, okay, so today we

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<v Speaker 1>have our our healthy yellow son, the one that makes

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<v Speaker 1>Superman as powerful as he is. Not all sons are

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<v Speaker 1>like this, and in fact, sons have a lifetime, just

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<v Speaker 1>like living organisms do. They sort of increase and decrease

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<v Speaker 1>in luminosity at different periods of their life, and eventually

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<v Speaker 1>they use up all of their stellar stuff. Right, the

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<v Speaker 1>fuel that they that they fuse, the hydrogen that they're

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<v Speaker 1>fusing to be that healthy yellow star. You know, it's

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<v Speaker 1>not infinite, so this can be bad for planets orbiting

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<v Speaker 1>the star. In October, there was a NASA blog post

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<v Speaker 1>that was explaining that a team of astronomers had recently

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<v Speaker 1>discovered evidence through a ground based telescope that there was

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<v Speaker 1>this red giant star called beat plus forty eight seven

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<v Speaker 1>forty and it was swelling to completely engulf a planet

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<v Speaker 1>formerly in its or it So how did they figure

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<v Speaker 1>this out? I thought this was really interesting. They realized

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<v Speaker 1>the star had quote the fumes of a scorched planet

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<v Speaker 1>in its atmosphere unquote, So the star aida planet. And

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<v Speaker 1>we figured it out by smelling the star's breath, uh

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<v Speaker 1>telescopically nonetheless, right, So yeah, they smelled its breath with

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<v Speaker 1>spectroscopic analysis, so that you know, looked at the colors, uh,

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<v Speaker 1>the luminosity coming off of the Sun, and they can

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<v Speaker 1>look at what materials are in that based on that data,

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<v Speaker 1>and they found that the star contained lots of the

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<v Speaker 1>element lithium. Oh yeah, that's not something that you usually

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<v Speaker 1>find in a red giant, right that That would be

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<v Speaker 1>a very weird thing to find a bunch of in

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<v Speaker 1>a in a star like that, because typically lithium gets

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<v Speaker 1>destroyed inside stars over a long period of time, and

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<v Speaker 1>red giants tend to be old. But you might find

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<v Speaker 1>lithium in a star if it's if it's being produced

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<v Speaker 1>by the consumption of another big chunk of matter, and

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<v Speaker 1>that's what they figured out happened. There had been another

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<v Speaker 1>planet there that probably spiraled into this red giant as

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<v Speaker 1>it heated and swoll on up, and it was like

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<v Speaker 1>oh no, no, no no, and it ate the planet.

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<v Speaker 1>It it quote ingested the planet. Okay, so this is

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<v Speaker 1>eventually going to happen to our son and our planet.

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<v Speaker 1>And I'm not talking about like in the next twenty

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<v Speaker 1>to forty years that this is. This is a few

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<v Speaker 1>billion years down the line, yes, right. One of the

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<v Speaker 1>researchers who found the evidence of this said that the

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<v Speaker 1>same kind of fate could be in line for the

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<v Speaker 1>inner planets of our Solar system within about five billion years.

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<v Speaker 1>Now five billion years. It's it's hard to get two

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<v Speaker 1>worked up about five billion years. Personally, I worry a lot,

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<v Speaker 1>but yeah, I'm not. I can't actually be worried about that.

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<v Speaker 1>But at least we we may worry for you know,

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<v Speaker 1>our descendants or the or our you know, the robots

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<v Speaker 1>built by our descendants that take over the planet, or

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<v Speaker 1>the distant future progeny of zebras. I care about future zebras,

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<v Speaker 1>Zebra babies of the future, right, right, well, unfortunately for

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<v Speaker 1>the zebra babies, they won't be able to wait for

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<v Speaker 1>the Sun to all out eat the Earth started. That

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<v Speaker 1>bad stuff will happen way before that actual consumption, right. So, yeah,

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<v Speaker 1>as the intensity of solar radiation bombarding the Earth slowly

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<v Speaker 1>gets stronger, and it just will steadily over time, Earth

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<v Speaker 1>will at some point become unable to sustain life. So

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<v Speaker 1>in there was a three dimensional climate model devised by

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<v Speaker 1>the and I apologize to French speakers out there, but

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<v Speaker 1>I'm going to try to say it the Laboratoire day

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<v Speaker 1>meteorology dynamic. Dynamic, Yeah, I don't. Yeah. So this climate

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<v Speaker 1>model that they came up with predicted that the solar

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<v Speaker 1>radiation will increase the Earth's surface temperature enough to boil

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<v Speaker 1>the oceans and cause Earth to lose all its liquid

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<v Speaker 1>water in about one billion years. That is a much

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<v Speaker 1>tighter deadline of Sun eating us. Okay, so before then,

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<v Speaker 1>I gotta find a plan. B We we can't just

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<v Speaker 1>wait it out. So a pretty straightforward one would be

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<v Speaker 1>to move to move to a nicer neighborhood, find a

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<v Speaker 1>new planet in another solar system, and get all of

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<v Speaker 1>the humans there or all of the zebra people of

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<v Speaker 1>the future grandchildren. But moving all of these organisms to

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<v Speaker 1>a new planet might not be so easy. So we've

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<v Speaker 1>talked about the problems with interstellar travel unless you've got

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<v Speaker 1>a spaceship that goes the speed of light or faster,

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<v Speaker 1>and we all know the problems with that. You know,

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<v Speaker 1>Einstein's special relativity says you can't go faster than the

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<v Speaker 1>speed of light. We may someday come up with some

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<v Speaker 1>crazy way to bind that rule, but we shouldn't bank

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<v Speaker 1>on it right now. It seems kind of like a

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<v Speaker 1>law of physics. So unless you can get pretty near

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<v Speaker 1>the speed of light, the journey between stars becomes prohibitively long,

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<v Speaker 1>like probably thousands of years. Uh. The nearest star to

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<v Speaker 1>Earth is the tiny red dwarf star Proximus Centauri, which

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<v Speaker 1>is in the Alpha Centauri system. It's about four point

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<v Speaker 1>two light years or about thirty nine point nine trillion

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<v Speaker 1>kilometers away. At the speed Voyager left the Solar System,

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<v Speaker 1>which is around thirty seven thousand miles per hour, I

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<v Speaker 1>see slight variations on that would be about you know,

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<v Speaker 1>almost sixty thousand kilometers per hour, which is the quickest

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<v Speaker 1>that anything that has survived its a journey thus far

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<v Speaker 1>has ever moved, right, Yeah, and so at that rate

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<v Speaker 1>it would take Yeah, it would take about eighty thousand

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<v Speaker 1>years to reach Proximus Centauri. Uh, that's I mean, I

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<v Speaker 1>guess if you're talking in the scheme of of a

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<v Speaker 1>billion years, that's not so long. But tightening that up

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<v Speaker 1>would be preferable, especially if that's just the journey to

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<v Speaker 1>a kind of crappy star up, if we're being really honest, Yeah,

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<v Speaker 1>it's this little red dwarf. I mean, you've got to

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<v Speaker 1>you can't just go to any star with the spaceship.

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<v Speaker 1>You need to find a planet to sustain life, right,

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<v Speaker 1>and not all planets are suitable for habitation. In fact,

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<v Speaker 1>most probably aren't. It could be too hot, too cold,

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<v Speaker 1>just in a constant bath of radiation. There might be

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<v Speaker 1>a gas giant that's full of radiation itself, and of

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<v Speaker 1>course you can't walk around on it. A good Earth

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<v Speaker 1>is really hard to find. There's the other problem of

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<v Speaker 1>once you're on the way, how do you keep yourself alive?

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<v Speaker 1>How do you keep supplying yourself with food, energy, air,

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<v Speaker 1>protection from radiation? In interstellar space, you could work on

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<v Speaker 1>building sort of generation sustaining starships with ways of continuously

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<v Speaker 1>creating new energy, maintaining an earthlike environment, etcetera. But then

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<v Speaker 1>you're almost talking about having to build a second Earth

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<v Speaker 1>to travel with you, and we're already on this perfectly

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<v Speaker 1>good Earth. If the problem is the Sun, why not

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<v Speaker 1>find a new son, Why not find a new Sun.

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<v Speaker 1>So the idea here becomes that we could take everything

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<v Speaker 1>we have with us when we travel to a new

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<v Speaker 1>new solar system, literally every single thing we have, including

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<v Speaker 1>the Earth, and for the journey at least including the Sun,

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<v Speaker 1>because we are using it as an engine. An engine.

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<v Speaker 1>You say, and engine, and I say, actually, I didn't

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<v Speaker 1>say it at all. Well, no, this idea comes from

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<v Speaker 1>others who have come before us. Who I mean, Yeah,

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<v Speaker 1>I literally just said it out loud. But it wasn't

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<v Speaker 1>my idea. Who were physicists who had incredibly strange and

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<v Speaker 1>very cool ideas. So where does this idea of a

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<v Speaker 1>stellar engine come from? Well, the original paper we want

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<v Speaker 1>to look at is something from October of nine, and

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<v Speaker 1>it was when the Russian physicist Leonage Skodov proposed a

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<v Speaker 1>really interesting idea atty Congress of the International Astronomical Federation

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<v Speaker 1>meeting in Brighton in the UK. And he said, what

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<v Speaker 1>if you could turn an entire solar system into a

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<v Speaker 1>vehicle or in his own words, quote a thruster for

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<v Speaker 1>solar system motion control? How on Earth would that work?

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<v Speaker 1>Or how on the galactic plane would that work? Yeah,

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<v Speaker 1>we don't even have words for this context. It's really strange.

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<v Speaker 1>So to clarify, the solar system is not motionless now,

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<v Speaker 1>oh no, of course not. It's moving all over the place.

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<v Speaker 1>We're not all over the place. I mean, there's there's

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<v Speaker 1>a system of movement which it follows. Yeah. Well, just

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<v Speaker 1>like the planets in our solar system or in orbit

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<v Speaker 1>around the Sun. Our solar system is in orbit around

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<v Speaker 1>the center of gravity of the Milky Way Galaxy, and

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<v Speaker 1>of course the Milky Way Galaxy self is moving. But

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<v Speaker 1>we're talking about controlling the trajectory of motion within the galaxy.

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<v Speaker 1>So what did he have in mind. Here's the basic

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<v Speaker 1>setup that Shadow envisioned. So you create a spherical arc mirror,

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<v Speaker 1>basically a giant curved mirror that's a concave one facing

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<v Speaker 1>our Sun on the inside. So imagine sort of a

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<v Speaker 1>giant contact lens with the inside of it the curved

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<v Speaker 1>inner side being a reflective mirror surface and that's pointed

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<v Speaker 1>toward the star, in this case, our sun, like like

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<v Speaker 1>like putting a like putting a big bowl of a

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<v Speaker 1>few feet away from a grape. Yeah, yeah, sure. So

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<v Speaker 1>this mirror would have a couple of forces acting on it.

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<v Speaker 1>If you have gravity pulling it towards the sun, the

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<v Speaker 1>Sun's gravity pulling it towards the Sun, right, and since

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<v Speaker 1>it would be a very large structure, it would also

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<v Speaker 1>have some gravitational force of its own. Uh. Then it

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<v Speaker 1>would also have radiation pressure pushing it away like a

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<v Speaker 1>solar sale. We've talked about solar sales before. Yeah. Yeah,

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<v Speaker 1>because the radiation, the electromagnetic radiation from the Sun does

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<v Speaker 1>have a pushing force. Yeah, we don't really feel it

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<v Speaker 1>normally because it's a very relatively tiny force, but on

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<v Speaker 1>a huge reflective surface in space, it makes a difference.

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<v Speaker 1>The sunlight pushes, so the mirror would become settled in

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<v Speaker 1>a place where these forces equalize, the solar radiation pushing

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<v Speaker 1>the mirror out and the gravity pulling it in. But

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<v Speaker 1>solar radiation would reflect off of the mirror instead of

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<v Speaker 1>radiating out into space like it normally does, and it

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<v Speaker 1>reflects back in the direction it came from towards the Sun.

0:13:44.640 --> 0:13:49.600
<v Speaker 1>Shadow's idea was that you could use this system to

0:13:49.760 --> 0:13:53.360
<v Speaker 1>control or at least help direct the motion of the

0:13:53.400 --> 0:13:56.400
<v Speaker 1>Sun and with the Sun, the rest of the Solar system. Now,

0:13:57.040 --> 0:13:58.920
<v Speaker 1>Lauren and I spent a lot of time staring at

0:13:58.960 --> 0:14:02.640
<v Speaker 1>some math we toe really didn't understand ch time. We're

0:14:02.679 --> 0:14:04.960
<v Speaker 1>not We're not astrophysicists, y'all. Yeah, let to see if

0:14:04.960 --> 0:14:06.560
<v Speaker 1>we could say a little bit more about the way

0:14:06.559 --> 0:14:10.680
<v Speaker 1>this thrust is generated. But if it is not abundantly clear,

0:14:10.880 --> 0:14:14.880
<v Speaker 1>we are not astrophysicists. And suffice to say, the experts

0:14:14.960 --> 0:14:18.160
<v Speaker 1>know what they're talking about. You could, in theory, use

0:14:18.280 --> 0:14:21.000
<v Speaker 1>one of these things they say to perturb the motion

0:14:21.040 --> 0:14:23.320
<v Speaker 1>of a star within the galaxy. Yes, and that is

0:14:23.320 --> 0:14:27.920
<v Speaker 1>the official terminology that I've seen people use, perturb, which

0:14:27.960 --> 0:14:29.840
<v Speaker 1>I think is just a really great verb to to

0:14:29.920 --> 0:14:33.080
<v Speaker 1>apply to the Sun. Like you're annoying. I could perturb

0:14:33.200 --> 0:14:36.240
<v Speaker 1>the Sun, turb the heck out of that Sun. Well,

0:14:36.360 --> 0:14:38.640
<v Speaker 1>the Sun started it, I mean, we didn't tell it

0:14:38.680 --> 0:14:40.880
<v Speaker 1>to swell into a red giant and eat the Earth,

0:14:42.000 --> 0:14:44.840
<v Speaker 1>all right, So so so so we've got these this

0:14:44.840 --> 0:14:48.360
<v Speaker 1>this dish and this this mirror and all of this

0:14:48.440 --> 0:14:52.360
<v Speaker 1>is creating thrust in a direction to move the Sun,

0:14:52.400 --> 0:14:54.320
<v Speaker 1>to move the Sun in the Solar system with it. Right,

0:14:54.400 --> 0:14:57.920
<v Speaker 1>So we would call this a class a stellar engine

0:14:58.000 --> 0:15:01.920
<v Speaker 1>or a scatterw thruster, and it would be sort of

0:15:01.960 --> 0:15:05.280
<v Speaker 1>like a giant steering wheel for the Solar System, driving

0:15:05.320 --> 0:15:08.200
<v Speaker 1>it where in the galaxy we wanted to go, and

0:15:08.240 --> 0:15:12.480
<v Speaker 1>the movement would be really slow. We need to stipulate that, Yeah,

0:15:12.600 --> 0:15:15.880
<v Speaker 1>very very slow. The obvious advantage though, would be that

0:15:16.040 --> 0:15:19.640
<v Speaker 1>we wouldn't have to leave the Earth our home, or

0:15:19.680 --> 0:15:23.440
<v Speaker 1>the Sun our energy source until we arrived at our

0:15:23.480 --> 0:15:27.400
<v Speaker 1>destination in another Solar system. And then the final idea

0:15:27.440 --> 0:15:30.800
<v Speaker 1>of this, the sort of ultimate conclusion, is that we

0:15:30.800 --> 0:15:34.560
<v Speaker 1>could plan the movement of our Scotov thruster just so

0:15:34.640 --> 0:15:38.760
<v Speaker 1>that Earth could be deposited into a circular orbit around

0:15:38.840 --> 0:15:42.760
<v Speaker 1>another star. Yeah, once you get the Solar system close

0:15:42.880 --> 0:15:46.640
<v Speaker 1>enough to a new solar system, you just kind of

0:15:46.720 --> 0:15:49.320
<v Speaker 1>let it get nudged in, right, You line it up

0:15:49.360 --> 0:15:51.880
<v Speaker 1>just so that the Earth gets captured by the gravity

0:15:51.920 --> 0:15:55.040
<v Speaker 1>of the new star. And then we're back in business

0:15:55.240 --> 0:16:00.000
<v Speaker 1>and we can keep making new Zebra children cities. Yeah,

0:16:00.040 --> 0:16:06.240
<v Speaker 1>Zebra robot children cities. Indeed, now I know this sounds

0:16:06.280 --> 0:16:09.040
<v Speaker 1>super sci fi, and to be honest, it really is.

0:16:09.120 --> 0:16:12.040
<v Speaker 1>I mean, we don't have the capability of building anything

0:16:12.120 --> 0:16:15.280
<v Speaker 1>like this right now, but it is an idea worth

0:16:15.320 --> 0:16:19.480
<v Speaker 1>taking seriously, even just for the very long view of

0:16:19.520 --> 0:16:22.720
<v Speaker 1>the survival of our species or maybe you know, our

0:16:22.520 --> 0:16:28.760
<v Speaker 1>our our terrestrial organic form, whatever that might be. There

0:16:28.920 --> 0:16:31.160
<v Speaker 1>is a great article that we were looking at in

0:16:31.240 --> 0:16:34.640
<v Speaker 1>Popular Mechanics from July of last year that actually examines

0:16:34.800 --> 0:16:38.160
<v Speaker 1>how you would build a scatter of thruster. That was

0:16:38.200 --> 0:16:41.080
<v Speaker 1>really helpful. Yeah, yeah, because there's so much that you

0:16:41.080 --> 0:16:44.400
<v Speaker 1>have to take into consideration here, um, like like where

0:16:44.440 --> 0:16:47.360
<v Speaker 1>do we get the material for creating a mirror of

0:16:47.560 --> 0:16:51.040
<v Speaker 1>this size and capacity? Right? Because exactly how big is

0:16:51.040 --> 0:16:54.400
<v Speaker 1>the mirror we're talking about here? Um? Yeah, you know,

0:16:54.560 --> 0:16:59.400
<v Speaker 1>just hundreds of millions of miles across. It would have

0:16:59.480 --> 0:17:02.720
<v Speaker 1>to be in in diameter greater than the distance from

0:17:02.720 --> 0:17:05.680
<v Speaker 1>the Earth to the Sun. Um, and it would which

0:17:05.680 --> 0:17:08.280
<v Speaker 1>would probably mean that would have to weigh some sextillion

0:17:08.520 --> 0:17:13.040
<v Speaker 1>or septillion, like even up to septillion pounds. And if

0:17:13.080 --> 0:17:16.199
<v Speaker 1>you need a concept of what that's like, I'm crossing

0:17:16.200 --> 0:17:19.119
<v Speaker 1>concepts a little bit here, but that's that's roughly the

0:17:19.160 --> 0:17:24.080
<v Speaker 1>mass uh of like Pluto or the Moon, or Mercury

0:17:24.280 --> 0:17:26.760
<v Speaker 1>or Mars. It's a little bit, it's a little bit.

0:17:26.800 --> 0:17:29.920
<v Speaker 1>It weighs a little bit less than Earth itself. So

0:17:30.160 --> 0:17:33.560
<v Speaker 1>so we we don't really have like a factory that

0:17:33.640 --> 0:17:36.240
<v Speaker 1>could build this. We do not have a spare Earth

0:17:36.600 --> 0:17:40.720
<v Speaker 1>to to to to create this mirror out of. But hey,

0:17:40.800 --> 0:17:44.439
<v Speaker 1>we do have those other planets just mentioned. Oh no,

0:17:44.880 --> 0:17:48.320
<v Speaker 1>are you talking about dismantling a planet and making a

0:17:48.359 --> 0:17:51.720
<v Speaker 1>megastructure out of it? I'm not talking about that, but

0:17:51.880 --> 0:17:55.240
<v Speaker 1>scientists certainly are. Yeah. Yeah, you'd you'd have to build

0:17:55.240 --> 0:17:57.919
<v Speaker 1>it out of something um kind of light and and

0:17:58.000 --> 0:18:00.520
<v Speaker 1>foil like relatively on the on the scale of metals,

0:18:00.520 --> 0:18:04.520
<v Speaker 1>something like chematite would be really good for that. That's

0:18:04.560 --> 0:18:06.600
<v Speaker 1>sort of like an iron ore. Yeah. Yeah, and you

0:18:06.640 --> 0:18:09.520
<v Speaker 1>could mind something like that out of the planet Mercury.

0:18:09.560 --> 0:18:14.040
<v Speaker 1>And so if you basically disassembled Mercury and and I

0:18:14.080 --> 0:18:16.200
<v Speaker 1>can still not hear that word without just thinking, let

0:18:16.240 --> 0:18:21.680
<v Speaker 1>no disassemble, Stephanie um. But but yeah, if you took

0:18:21.720 --> 0:18:26.200
<v Speaker 1>apart Mercury and used the entire planet to build this,

0:18:26.200 --> 0:18:30.520
<v Speaker 1>this sale this mirror, then you could make it work. Wow,

0:18:31.800 --> 0:18:34.600
<v Speaker 1>I mean that is crazy, But then again, we are

0:18:34.720 --> 0:18:37.760
<v Speaker 1>we are talking about sort of a a multi generational

0:18:37.840 --> 0:18:41.200
<v Speaker 1>project that would have to be pretty far in the future. Yeah,

0:18:41.240 --> 0:18:43.320
<v Speaker 1>and we would miss mercury. I'm sure it would mess

0:18:43.400 --> 0:18:47.000
<v Speaker 1>up astrology a whole lot. I know, right, but wait

0:18:47.000 --> 0:18:49.359
<v Speaker 1>a minute, no, no, no, no more mercury and retrograde.

0:18:49.400 --> 0:18:51.679
<v Speaker 1>That's a bad thing, right, the thing people don't like.

0:18:51.760 --> 0:18:53.919
<v Speaker 1>You know, it's terrible. It's like I lost my keys

0:18:54.040 --> 0:19:00.520
<v Speaker 1>mercury did it something to that extent. Yeah, and and

0:19:00.560 --> 0:19:02.720
<v Speaker 1>so so it sounds crazy, but um, it's actually a

0:19:02.720 --> 0:19:05.000
<v Speaker 1>lot less crazy than trying to catch a lot of

0:19:05.040 --> 0:19:07.920
<v Speaker 1>asteroids or something like that to do the same job.

0:19:09.040 --> 0:19:13.200
<v Speaker 1>And and of course, by when I said that you

0:19:13.600 --> 0:19:16.879
<v Speaker 1>would be disassembling mercury, I did not mean Joe, and

0:19:16.920 --> 0:19:19.040
<v Speaker 1>I didn't mean that the Royal you. This would probably

0:19:19.080 --> 0:19:21.040
<v Speaker 1>be a job for robots. Yeah. Yeah, I would have

0:19:21.040 --> 0:19:24.280
<v Speaker 1>to be some kind of a massive fleet of robots

0:19:24.359 --> 0:19:27.040
<v Speaker 1>doing this autonomously. I mean, it just really wouldn't make

0:19:27.080 --> 0:19:29.240
<v Speaker 1>sense to go try to put people on mercury to

0:19:29.320 --> 0:19:32.840
<v Speaker 1>mind its surface. Uh No, that would go poorly for people.

0:19:33.119 --> 0:19:37.919
<v Speaker 1>So we're talking now essentially about mining mercury to create

0:19:37.960 --> 0:19:40.800
<v Speaker 1>all this, or to turn into a thin sheet of

0:19:40.920 --> 0:19:45.520
<v Speaker 1>reflective foil to put in space in a static position

0:19:46.240 --> 0:19:49.680
<v Speaker 1>at the Sun to reflect all this radiation to generate

0:19:49.840 --> 0:19:53.800
<v Speaker 1>thrust to move the Sun. Yeah, okay, okay, I'm with

0:19:53.840 --> 0:19:57.399
<v Speaker 1>you so far. What are some things we might have

0:19:57.480 --> 0:20:00.280
<v Speaker 1>to worry about when doing this, just to you know,

0:20:00.800 --> 0:20:03.639
<v Speaker 1>concerns we should keep in mind while building a giant

0:20:03.640 --> 0:20:07.320
<v Speaker 1>space mirror. Um. Well, I would want to make sure

0:20:07.359 --> 0:20:11.040
<v Speaker 1>that we take pains to to not you know, either

0:20:11.240 --> 0:20:14.879
<v Speaker 1>freeze or fry the Earth with this mirror thing, because

0:20:15.119 --> 0:20:17.720
<v Speaker 1>the these that the mirror would probably be somewhere near

0:20:17.760 --> 0:20:20.080
<v Speaker 1>the orbit of the Earth in order to make the

0:20:20.160 --> 0:20:24.119
<v Speaker 1>materials stable. Um, we wouldn't want to melt the mirror either.

0:20:24.240 --> 0:20:28.680
<v Speaker 1>That would be pretty bad. Um uh. And and having

0:20:28.680 --> 0:20:34.919
<v Speaker 1>it relatively near by could potentially cause problems with um.

0:20:34.960 --> 0:20:38.919
<v Speaker 1>The the amount of solar radiation that continues to hit

0:20:38.960 --> 0:20:41.200
<v Speaker 1>the Earth, which we want, you know, we enjoy having

0:20:41.240 --> 0:20:45.119
<v Speaker 1>sunlight here. It kind of drives the entire life cycle

0:20:45.240 --> 0:20:49.160
<v Speaker 1>on this planet or can Conversely, we wouldn't want kind

0:20:49.160 --> 0:20:52.040
<v Speaker 1>of extra radiation from the mirror to start hitting the

0:20:52.080 --> 0:20:57.480
<v Speaker 1>Earth and fries completely. Yeah. I've seen some different considerations

0:20:57.560 --> 0:20:59.960
<v Speaker 1>that different thinkers have had on what sort of the

0:21:00.080 --> 0:21:03.359
<v Speaker 1>final heat situation would be with one of these in place,

0:21:03.400 --> 0:21:05.520
<v Speaker 1>because there are different ideas about where you can put

0:21:05.560 --> 0:21:09.720
<v Speaker 1>it relative to the Sun and the Another thing I

0:21:09.720 --> 0:21:13.640
<v Speaker 1>think we should consider is how fast could this thing

0:21:13.720 --> 0:21:16.560
<v Speaker 1>actually go and what are the conditions that would control

0:21:16.880 --> 0:21:21.160
<v Speaker 1>its its speed capabilities? Yeah, we we mentioned this earlier,

0:21:21.240 --> 0:21:24.360
<v Speaker 1>and and I wanted to put into into actual numbers

0:21:24.440 --> 0:21:30.040
<v Speaker 1>exactly how slow this thing would be going UM because okay, okay,

0:21:30.080 --> 0:21:32.760
<v Speaker 1>if the Sun is already moving at some five hundred

0:21:32.800 --> 0:21:36.600
<v Speaker 1>thousand miles per hour UM, that's an incredibly rough estimate,

0:21:36.680 --> 0:21:42.520
<v Speaker 1>you guys, Um, the first few million years of UM

0:21:42.680 --> 0:21:46.920
<v Speaker 1>scoutof thrust could only change our trajectory a little bit. UM.

0:21:47.080 --> 0:21:51.600
<v Speaker 1>One thermodynamicist by the name of Virile bad Askew or

0:21:51.720 --> 0:21:53.919
<v Speaker 1>something to that extent. I'm sorry I didn't look this

0:21:54.000 --> 0:21:57.400
<v Speaker 1>up before the podcast. Um. He's he's from the Polytechnic

0:21:57.520 --> 0:22:02.160
<v Speaker 1>University of in Romania says it could take two hundred

0:22:02.480 --> 0:22:05.520
<v Speaker 1>million years for us to change the trajectory of the

0:22:05.520 --> 0:22:08.200
<v Speaker 1>Sun by as much as a hundred and thirty light years.

0:22:08.720 --> 0:22:11.160
<v Speaker 1>And that's that's on the generous end. He He also

0:22:11.200 --> 0:22:13.240
<v Speaker 1>said that it might be by as little as thirty

0:22:13.400 --> 0:22:17.919
<v Speaker 1>light years. That's I mean, that's a big window. But

0:22:18.000 --> 0:22:20.600
<v Speaker 1>then again, thirty light years is a long way. I

0:22:20.640 --> 0:22:22.680
<v Speaker 1>saw that note you made, and then I was trying

0:22:22.720 --> 0:22:25.959
<v Speaker 1>to figure out, well, what's within thirty light years? Uh?

0:22:26.160 --> 0:22:30.080
<v Speaker 1>I found a website called soul Station. I'm not familiar

0:22:30.080 --> 0:22:32.280
<v Speaker 1>with the source, so I don't know if it's entirely accurate,

0:22:32.280 --> 0:22:35.440
<v Speaker 1>but at least based on what they say, there are

0:22:35.560 --> 0:22:39.040
<v Speaker 1>a hundred and fifty celestial objects within a twenty light

0:22:39.119 --> 0:22:41.800
<v Speaker 1>year radius of Earth. So a lot of these are

0:22:41.840 --> 0:22:44.760
<v Speaker 1>brown dwarfs and stuff that really wouldn't be useful to us.

0:22:44.760 --> 0:22:48.520
<v Speaker 1>But it listed at least to a sequence and seven

0:22:48.600 --> 0:22:52.200
<v Speaker 1>G sequence stars, so I don't know. I mean, I

0:22:52.560 --> 0:22:54.760
<v Speaker 1>could see even within thirty years, you could get to

0:22:54.840 --> 0:22:58.960
<v Speaker 1>a reasonable number of objects out there. Thirty light years yeah, yeah,

0:22:59.040 --> 0:23:01.280
<v Speaker 1>um over there. I mean, it's just just that number

0:23:01.280 --> 0:23:04.800
<v Speaker 1>two hundred million years is a number that I have

0:23:04.880 --> 0:23:09.280
<v Speaker 1>a hard time comprehending. Yeah, it's also worth thinking about

0:23:09.320 --> 0:23:11.639
<v Speaker 1>it in the context of one billion years until the

0:23:11.680 --> 0:23:18.160
<v Speaker 1>oceans boil. So sure, you know it's zebra children. Got

0:23:18.160 --> 0:23:21.359
<v Speaker 1>to keep him in mind. We can't forget the zebra

0:23:21.440 --> 0:23:25.280
<v Speaker 1>children of the future children Okay, alright, have such huge eyes.

0:23:26.680 --> 0:23:31.119
<v Speaker 1>They will they'll be adorable. Um. Okay, so so, so

0:23:31.160 --> 0:23:33.040
<v Speaker 1>all of these problems are kind of sad news for

0:23:33.040 --> 0:23:36.199
<v Speaker 1>anyone who is hoping to build one of these mirrors

0:23:36.359 --> 0:23:40.520
<v Speaker 1>like next week. Um. But they also do offer a

0:23:40.560 --> 0:23:45.200
<v Speaker 1>really promising implication, and that is that any alien civilization

0:23:45.600 --> 0:23:48.119
<v Speaker 1>that could have possibly created one of these could be

0:23:48.119 --> 0:23:51.200
<v Speaker 1>pretty easy for us to spot. That's right. So there

0:23:51.280 --> 0:23:55.720
<v Speaker 1>was a recent paper by Duncan h For again of

0:23:55.760 --> 0:23:58.960
<v Speaker 1>the University of St. Andrew's, and he talked about the

0:23:59.000 --> 0:24:03.080
<v Speaker 1>possibility of king for alien stellar engines as evidence of

0:24:03.119 --> 0:24:05.760
<v Speaker 1>alien life. So we talked a little bit about looking

0:24:05.800 --> 0:24:11.160
<v Speaker 1>for aliens in our episode on the Kardashev scale from January.

0:24:11.640 --> 0:24:15.360
<v Speaker 1>But here's Forgan's idea. It goes pretty much like this.

0:24:15.840 --> 0:24:20.400
<v Speaker 1>We already have astronomical projects that are looking for the

0:24:20.440 --> 0:24:24.479
<v Speaker 1>transit of exoplanets across other stars in the galaxy. So

0:24:24.600 --> 0:24:27.919
<v Speaker 1>you have a telescope stare at the light produced by

0:24:27.920 --> 0:24:31.320
<v Speaker 1>a star, and then you try to observe changes in

0:24:31.440 --> 0:24:34.320
<v Speaker 1>that light produced by the star to see if it

0:24:34.320 --> 0:24:37.959
<v Speaker 1>would be consistent with a planet passing between us and

0:24:38.000 --> 0:24:41.439
<v Speaker 1>the star and blocking part of its light. Of course,

0:24:41.680 --> 0:24:45.800
<v Speaker 1>an alien civilization that built a megastructure like a Scattov

0:24:45.920 --> 0:24:50.200
<v Speaker 1>thruster might also be detectable in the same kinds of data.

0:24:50.640 --> 0:24:53.520
<v Speaker 1>So in a paper called on the possibility of detecting

0:24:53.600 --> 0:24:58.639
<v Speaker 1>Class A Stellar Engines using Exoplanet transit curves, Forgan tries

0:24:58.680 --> 0:25:01.560
<v Speaker 1>to model the kind of light curves we would see

0:25:01.920 --> 0:25:04.760
<v Speaker 1>if we were observing exoplanet transit on a star that

0:25:04.880 --> 0:25:09.480
<v Speaker 1>had a Scatoff thruster. So though the probability he rates

0:25:09.520 --> 0:25:12.199
<v Speaker 1>of finding evidence for one of these things based on

0:25:12.240 --> 0:25:15.280
<v Speaker 1>the methods and data we have available now is pretty low,

0:25:16.000 --> 0:25:19.120
<v Speaker 1>we might have a more optimistic outlook once we compare

0:25:19.240 --> 0:25:24.640
<v Speaker 1>this strategy with other directed tools for SETI. Yeah, anyway,

0:25:24.680 --> 0:25:27.879
<v Speaker 1>I thought that was pretty cool. Even if we can't

0:25:28.000 --> 0:25:31.840
<v Speaker 1>save our own planet with a scout Out thruster, we

0:25:31.840 --> 0:25:34.439
<v Speaker 1>could at least maybe use it to know that there

0:25:34.440 --> 0:25:37.720
<v Speaker 1>are other civilizations out there that are more proactive than

0:25:37.760 --> 0:25:43.240
<v Speaker 1>we are. Yeah. Yeah, Although, speaking of saving our planet,

0:25:43.359 --> 0:25:47.199
<v Speaker 1>I wanted to discuss a couple other reasons that we

0:25:47.320 --> 0:25:49.680
<v Speaker 1>might have to do such a thing. Right, So, even

0:25:49.760 --> 0:25:52.919
<v Speaker 1>maybe before our planet swells into a red giant or

0:25:53.000 --> 0:25:55.400
<v Speaker 1>boils the oceans. In a billion years, we might really

0:25:55.440 --> 0:25:59.360
<v Speaker 1>need to move our sun around. Yeah. Yeah, there are

0:25:59.400 --> 0:26:04.240
<v Speaker 1>a couple relatively smaller reasons for this. Um. So, Joe,

0:26:04.440 --> 0:26:07.040
<v Speaker 1>have you have you ever been worried about an asteroid

0:26:07.080 --> 0:26:10.919
<v Speaker 1>or comet hitting the Earth? That is exactly the reason

0:26:11.160 --> 0:26:15.199
<v Speaker 1>I've been hollowing out a cavern under my house to

0:26:15.560 --> 0:26:19.040
<v Speaker 1>dwell in after the big one hits. We've got canned food,

0:26:19.280 --> 0:26:23.359
<v Speaker 1>We've got lots of VHS tapes of sci fi movies

0:26:23.400 --> 0:26:27.479
<v Speaker 1>from the eighties. I think we'll be good. A zebra. Yeah, Okay, Well,

0:26:27.640 --> 0:26:30.840
<v Speaker 1>I've got a new source for your paranoia. Okay. Interstellar

0:26:31.320 --> 0:26:37.520
<v Speaker 1>gas and dust clouds. Oh it sounds dusty. It sounds

0:26:37.640 --> 0:26:41.520
<v Speaker 1>not terrifying at all. Actually, But what's important to keep

0:26:41.520 --> 0:26:45.600
<v Speaker 1>in mind here is that, Okay, space is not all space,

0:26:46.119 --> 0:26:48.400
<v Speaker 1>not all empty space. There's some stuff out there. There's

0:26:48.440 --> 0:26:50.920
<v Speaker 1>lots of stuff. In addition to stars and planets and

0:26:50.960 --> 0:26:53.879
<v Speaker 1>all of that, there are these giant clouds of gas

0:26:53.880 --> 0:26:57.160
<v Speaker 1>and dust that are floating around in the interstellar medium

0:26:57.280 --> 0:27:00.600
<v Speaker 1>between star systems. These things could count for as much

0:27:00.600 --> 0:27:04.240
<v Speaker 1>as fifteent of the matter visible um visible across the

0:27:04.240 --> 0:27:06.399
<v Speaker 1>electromagnetic spectrum. Not that like you can see with the

0:27:06.480 --> 0:27:10.600
<v Speaker 1>naked eye, um, in our Milky Way galaxy. And according

0:27:10.640 --> 0:27:13.840
<v Speaker 1>to one Michael Richmond of the Rochester Institute of Technology,

0:27:14.000 --> 0:27:18.679
<v Speaker 1>that's some ten billion sons worth of stuff. Yikes, bunches

0:27:18.680 --> 0:27:23.240
<v Speaker 1>of stuff. That stuff in question is mostly molecular hydrogen

0:27:23.400 --> 0:27:27.120
<v Speaker 1>with just a tad bit of helium and dust for

0:27:27.119 --> 0:27:29.280
<v Speaker 1>for for lack of a better word, just just little

0:27:29.440 --> 0:27:36.240
<v Speaker 1>microparticles things. Um. And yeah, none of that is terrifying. Um.

0:27:36.280 --> 0:27:39.520
<v Speaker 1>But if we happened to go through one, it would

0:27:39.600 --> 0:27:43.040
<v Speaker 1>be bad. Through one cloud of a cloud of the stuff,

0:27:43.040 --> 0:27:44.760
<v Speaker 1>it would be bad. Yes. And if you are shaky

0:27:44.800 --> 0:27:47.720
<v Speaker 1>on the whole good bad thing, um, let me explain

0:27:47.840 --> 0:27:50.600
<v Speaker 1>bad with a shout out to Jeffrey Winter's who wrote

0:27:50.640 --> 0:27:52.800
<v Speaker 1>a really good piece for Discover magazine back in two

0:27:52.880 --> 0:27:55.680
<v Speaker 1>thousand eight called how a cloud of space dust could

0:27:55.680 --> 0:27:59.960
<v Speaker 1>wipe out life on Earth. Yay, okay, let's hear it

0:28:00.760 --> 0:28:05.480
<v Speaker 1>all right. So the Solar system is surrounded by the heliosphere, right, Um,

0:28:05.520 --> 0:28:09.480
<v Speaker 1>that's that thing that the Voyager satellites passed through well

0:28:09.560 --> 0:28:12.560
<v Speaker 1>a while ago, but we found out about it recently. Um.

0:28:12.600 --> 0:28:15.760
<v Speaker 1>And and it's a protective wall of solar wind which

0:28:15.840 --> 0:28:19.240
<v Speaker 1>is plasma that's radiated out by the Sun. Um. It's

0:28:19.280 --> 0:28:21.720
<v Speaker 1>magnetic at the edges, and it helps keep the planets

0:28:21.760 --> 0:28:25.640
<v Speaker 1>in our system safe from from interstellar particles and radiation.

0:28:26.280 --> 0:28:29.600
<v Speaker 1>And and the thing is, astronomers think that we've been

0:28:29.720 --> 0:28:33.119
<v Speaker 1>in a really clear section of interstellar space for the

0:28:33.160 --> 0:28:36.760
<v Speaker 1>past five million years or so. Um. If we were

0:28:36.840 --> 0:28:39.720
<v Speaker 1>to hit one of these clouds of gas and dust,

0:28:39.840 --> 0:28:44.080
<v Speaker 1>it would bombard our heliosphere, pushing it from from way

0:28:44.080 --> 0:28:47.480
<v Speaker 1>outside of Pluto's orbit down into the orbit of of

0:28:47.520 --> 0:28:52.160
<v Speaker 1>like Saturn or Uranus. Yeah. Um, And we're not super

0:28:52.160 --> 0:28:55.080
<v Speaker 1>sure what effects this would have on Earth. UM that

0:28:55.120 --> 0:28:58.400
<v Speaker 1>the heliosphere would probably still protect us from a bunch

0:28:58.480 --> 0:29:01.640
<v Speaker 1>of this cloud, but some of it would probably reach

0:29:01.680 --> 0:29:05.240
<v Speaker 1>the Earth and the hydrogen that that composes most of

0:29:05.240 --> 0:29:07.960
<v Speaker 1>the cloud could start seeping into our atmosphere and reacting

0:29:07.960 --> 0:29:11.520
<v Speaker 1>with our oxygen, which would change our air supply for

0:29:11.560 --> 0:29:15.840
<v Speaker 1>the worse for us certainly. UM. And furthermore and more

0:29:15.880 --> 0:29:20.160
<v Speaker 1>cosmic rays would be hitting the planet, which would endanger um,

0:29:20.160 --> 0:29:22.720
<v Speaker 1>you know, our stuff and our people in orbit, and

0:29:22.760 --> 0:29:26.160
<v Speaker 1>also greatly increase our radiation exposure here on the ground.

0:29:27.240 --> 0:29:31.680
<v Speaker 1>So bad times. We do not want this to happen. Um. Unfortunately,

0:29:31.720 --> 0:29:34.800
<v Speaker 1>these clouds are really hard for us to spot. We

0:29:34.880 --> 0:29:37.320
<v Speaker 1>do know that there is one less than a trillion

0:29:37.400 --> 0:29:41.320
<v Speaker 1>miles away, which is approximately two d and fifty times

0:29:41.320 --> 0:29:44.960
<v Speaker 1>the distance from Earth to Pluto. If that helps. It

0:29:45.000 --> 0:29:46.760
<v Speaker 1>doesn't really help me, to be honest, but it's a

0:29:46.760 --> 0:29:51.480
<v Speaker 1>good number, um uh, which which which means that we

0:29:51.520 --> 0:29:54.600
<v Speaker 1>could collide with the sucker in only two thousand, five

0:29:54.680 --> 0:29:58.040
<v Speaker 1>hundred years. Oh, that's pretty soon. That's that's way sooner.

0:29:58.240 --> 0:30:02.760
<v Speaker 1>Probably can't build a shut up thruster. Hey, don't don't

0:30:02.800 --> 0:30:08.720
<v Speaker 1>underestimate future human zebra. Okay, maybe maybe sure, get that

0:30:08.800 --> 0:30:12.840
<v Speaker 1>fleet out there, tear down Mercury. Nobody cares about Mercury.

0:30:12.920 --> 0:30:15.800
<v Speaker 1>Get it done right, right, Okay, So we could at least,

0:30:15.840 --> 0:30:19.959
<v Speaker 1>say maybe maybe possible, assuming all this works is as planned,

0:30:20.280 --> 0:30:22.360
<v Speaker 1>that would be a very good reason to have one

0:30:22.400 --> 0:30:24.920
<v Speaker 1>of these things active. Oh but then again, you know,

0:30:25.200 --> 0:30:27.600
<v Speaker 1>it does take a while to get it started moving

0:30:27.640 --> 0:30:30.280
<v Speaker 1>in the in the direction, So I don't know, but

0:30:30.320 --> 0:30:32.440
<v Speaker 1>at least maybe we we can have one in time

0:30:32.480 --> 0:30:36.280
<v Speaker 1>to dodge the next one. Yeah, And furthermore, there's other

0:30:36.320 --> 0:30:38.680
<v Speaker 1>stuff out there that we that we do need to

0:30:38.720 --> 0:30:43.800
<v Speaker 1>be tangentially concerned about such as close passage to another

0:30:43.880 --> 0:30:50.080
<v Speaker 1>star system. Oh yeah, yeah, so so astronomers, uh, whose

0:30:50.160 --> 0:30:51.880
<v Speaker 1>job it is to this kind of thing, have been

0:30:51.920 --> 0:30:56.440
<v Speaker 1>projecting nearby stars paths out into the past and future,

0:30:56.760 --> 0:31:02.520
<v Speaker 1>some ten million years each because why not, of course, Yeah,

0:31:02.640 --> 0:31:04.080
<v Speaker 1>you want to know where stars are going to be,

0:31:04.960 --> 0:31:07.560
<v Speaker 1>and they found that in the past ten million years,

0:31:07.640 --> 0:31:11.680
<v Speaker 1>it's pretty likely that no stars have passed closer than

0:31:12.120 --> 0:31:17.080
<v Speaker 1>three light years away from us. Okay, but in only

0:31:18.400 --> 0:31:22.680
<v Speaker 1>thousand years, Uh, Proximus Centauri and Alpha Centauri could both

0:31:22.720 --> 0:31:27.360
<v Speaker 1>be inside that range. Yeah. Um, so what happens when

0:31:27.440 --> 0:31:30.920
<v Speaker 1>a star gets close to us, Well, we're not sure,

0:31:31.280 --> 0:31:34.520
<v Speaker 1>but it could be close enough to disturb another feature

0:31:34.600 --> 0:31:39.000
<v Speaker 1>of interstellar space, which is the conjectured or cloud, which

0:31:39.280 --> 0:31:44.200
<v Speaker 1>is the uh supposedly is the icy band loosely connected

0:31:44.240 --> 0:31:47.160
<v Speaker 1>to the Solar System and is where comets come from. Right,

0:31:47.200 --> 0:31:50.320
<v Speaker 1>It's what goes way way out there into the darkness,

0:31:50.360 --> 0:31:53.520
<v Speaker 1>and we can't see the stuff in it always. Yeah. Yeah,

0:31:53.600 --> 0:31:56.960
<v Speaker 1>it's it's maybe about halfway between us and Proximus Centauri

0:31:57.160 --> 0:31:59.200
<v Speaker 1>right now, so it's it's pretty far out there. But

0:31:59.200 --> 0:32:02.720
<v Speaker 1>but comets and can come down into into the range

0:32:03.120 --> 0:32:06.000
<v Speaker 1>of the Solar System, and the disturbance of this cloud

0:32:06.040 --> 0:32:09.560
<v Speaker 1>could send a lot more comets down into the Solar System,

0:32:10.000 --> 0:32:13.200
<v Speaker 1>sort of like just kicking sand into our face. Yeah, basically,

0:32:13.280 --> 0:32:18.600
<v Speaker 1>except it could be deadly sand. Deadly comets, sand Man, Yeah, giant, giant,

0:32:18.720 --> 0:32:25.240
<v Speaker 1>specially deadly because it sounds like comic sands. I'm sorry

0:32:25.280 --> 0:32:27.680
<v Speaker 1>I said that, but let's let's keep it and move on.

0:32:27.960 --> 0:32:32.320
<v Speaker 1>I agree there. There are also other than that, um uh,

0:32:32.680 --> 0:32:35.560
<v Speaker 1>brown dwarf stars to worry about, which are also pretty

0:32:35.560 --> 0:32:39.840
<v Speaker 1>difficult to detect, and at least hundreds of them are

0:32:39.880 --> 0:32:43.440
<v Speaker 1>within a hundred light years of us UM. In the

0:32:43.520 --> 0:32:46.280
<v Speaker 1>nine eighties, there was even a theory that Earth's periodic

0:32:46.320 --> 0:32:50.760
<v Speaker 1>mass extinctions are caused by a star in loose companionship

0:32:50.800 --> 0:32:53.280
<v Speaker 1>with the Sun that swings by every like thirty two

0:32:53.320 --> 0:32:57.400
<v Speaker 1>million years or so. I don't think that's correct, actually,

0:32:57.440 --> 0:32:59.640
<v Speaker 1>I but most scientists agree these days that that that

0:32:59.640 --> 0:33:02.880
<v Speaker 1>that was wrong. Um. They were calling the star Nemesis.

0:33:03.400 --> 0:33:07.600
<v Speaker 1>Oh yeah, Nemesis. Yeah, I've heard, Wait to Nemesis. I

0:33:07.600 --> 0:33:10.160
<v Speaker 1>thought Nemesis was also a planet or is that planet

0:33:10.320 --> 0:33:13.600
<v Speaker 1>x Nibiru? I am not sure. I do know that

0:33:13.640 --> 0:33:15.800
<v Speaker 1>star trek Nemesis was a thing that happened. We need

0:33:15.840 --> 0:33:17.760
<v Speaker 1>to get Ben and Madden here to talk about all

0:33:17.760 --> 0:33:20.800
<v Speaker 1>of the secret planets they don't want us to know about. Well,

0:33:20.840 --> 0:33:22.480
<v Speaker 1>not that Ben and Matt don't want us to know about,

0:33:22.480 --> 0:33:28.960
<v Speaker 1>but they they don't want us to know. Yeah. So

0:33:28.960 --> 0:33:31.800
<v Speaker 1>so there are many many reasons why, you know, you know,

0:33:31.920 --> 0:33:35.840
<v Speaker 1>and all all of these potential dangers will probably come

0:33:35.880 --> 0:33:42.560
<v Speaker 1>into clearer focus as our detection equipment improves and and

0:33:42.560 --> 0:33:44.680
<v Speaker 1>and as we crunch some of those numbers that we

0:33:44.720 --> 0:33:48.800
<v Speaker 1>have already received from some of our telescopes and etcetera.

0:33:49.440 --> 0:33:52.160
<v Speaker 1>But uh, yeah, I think I think it's safe to

0:33:52.160 --> 0:33:57.320
<v Speaker 1>say that we have totally solid reason for wanting to

0:33:57.400 --> 0:34:00.160
<v Speaker 1>be able to move our solar system. And if out

0:34:00.160 --> 0:34:02.440
<v Speaker 1>of Thruster is the way to do it, I say,

0:34:02.520 --> 0:34:05.000
<v Speaker 1>let's start building today. You know, how do we get

0:34:05.040 --> 0:34:08.440
<v Speaker 1>those robots to Mercury's Let's let's get a team of

0:34:08.440 --> 0:34:10.919
<v Speaker 1>people on it. Somebody's got to build the robots first. Well,

0:34:10.960 --> 0:34:13.200
<v Speaker 1>one thing I do want to be clear about is

0:34:13.280 --> 0:34:16.560
<v Speaker 1>that the kind of stellar engine we've been talking about

0:34:16.760 --> 0:34:19.279
<v Speaker 1>is not the only kind of stellar engine. In fact,

0:34:19.360 --> 0:34:22.160
<v Speaker 1>as you probably heard of saying it's a Class A

0:34:22.400 --> 0:34:27.440
<v Speaker 1>stellar engine. There are whole other types of megastructures that

0:34:27.480 --> 0:34:30.880
<v Speaker 1>have been proposed for harnessing a huge amount of the

0:34:31.000 --> 0:34:34.600
<v Speaker 1>energy of a star, and hopefully we can in other

0:34:34.680 --> 0:34:37.120
<v Speaker 1>episodes talk about some of those, Like you may have

0:34:37.200 --> 0:34:41.279
<v Speaker 1>heard of Dyson spheres, which have a great name. They

0:34:41.320 --> 0:34:44.520
<v Speaker 1>have nothing to do with vacuum cleaners. They have everything

0:34:44.560 --> 0:34:50.560
<v Speaker 1>to do with cosmic power, real cosmic power. Yes, uh

0:34:50.600 --> 0:34:52.359
<v Speaker 1>and yeah, yeah, those those are Class B, and there's

0:34:52.360 --> 0:34:55.120
<v Speaker 1>also a Class C. And we have already talked for

0:34:55.239 --> 0:34:57.319
<v Speaker 1>quite a while today, so I think that we're going

0:34:57.360 --> 0:35:01.480
<v Speaker 1>to leave that for another day. Uh. But in the meanwhile,

0:35:01.600 --> 0:35:04.960
<v Speaker 1>if you would like to hear anything specific from us

0:35:05.120 --> 0:35:08.799
<v Speaker 1>other than about more stellar engines, let us know. You

0:35:08.840 --> 0:35:11.879
<v Speaker 1>can write us an email at f W Thinking at

0:35:11.920 --> 0:35:14.840
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0:35:15.000 --> 0:35:19.560
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0:35:19.600 --> 0:35:22.839
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0:35:22.880 --> 0:35:27.000
<v Speaker 1>f W thinking dot com for lots more video and

0:35:27.239 --> 0:35:32.120
<v Speaker 1>podcast and written content. Uh. You can also chastise me

0:35:32.200 --> 0:35:36.080
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0:35:36.120 --> 0:35:38.680
<v Speaker 1>to hear from you, and you will hear from us

0:35:38.719 --> 0:35:45.640
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0:35:45.640 --> 0:35:58.800
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0:35:58.800 --> 0:36:01.280
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