WEBVTT - TechStuff Classic: TechStuff Experiments With Fusion

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<v Speaker 1>Welcome to tech Stuff, a production from I Heart Radio.

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<v Speaker 1>Hey there, and welcome to tech Stuff. I'm your host,

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<v Speaker 1>Jonathan Strickland. I'm an executive producer with I Heart Radio

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<v Speaker 1>and I love all things tech. And it's Friday. That

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<v Speaker 1>means it's time for a classic episode of tech Stuff.

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<v Speaker 1>And this one originally published on April fIF two thousand thirteen.

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<v Speaker 1>It's called tex Stuff Experiments with Fusion. So let's listen in.

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<v Speaker 1>We're talking nuclear fusion and to uh kind of give

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<v Speaker 1>you an idea of what nuclear fusion is, how we

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<v Speaker 1>are trying to harness nuclear fusion as a source of

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<v Speaker 1>energy production, really electricity production. Uh, and it's it's being

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<v Speaker 1>tended as one of the technologies of the feature that

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<v Speaker 1>is going to give us unlimited energy. And how far

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<v Speaker 1>away is it? Twenty to thirty to fifty years And

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<v Speaker 1>every year it seems like we're still at the lead

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<v Speaker 1>to fifty years. Yeah, yeah, it's that's one of those

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<v Speaker 1>things that scientists will often Riley kind of joke about

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<v Speaker 1>that the technology is always twenty years away. And uh,

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<v Speaker 1>and you know, it's because the challenges that we need

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<v Speaker 1>to overcome are quite impressive. Doesn't doesn't mean we won't

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<v Speaker 1>do it because human beings are amazing, you know, we innovate,

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<v Speaker 1>we event but but let's let's kind of first of

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<v Speaker 1>all talk about the difference between fusion and fission. Fission

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<v Speaker 1>is the kind of a nuclear process that is used

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<v Speaker 1>in our nuclear power plants today. So if you are

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<v Speaker 1>familiar with the nuclear power plants things like you know there,

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<v Speaker 1>of course they're the famous ones that have suffered catastrophic

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<v Speaker 1>failures like Three Mile Island or Chernobyl. Uh. But these

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<v Speaker 1>are the the reactors where they split up larger atoms

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<v Speaker 1>into smaller atoms and as a result, a great deal

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<v Speaker 1>of energy is given off really in the form of heat,

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<v Speaker 1>which is then harnessed to convert water into steam, which

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<v Speaker 1>turns steam turbines which are connected to electrical generators generating electricity.

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<v Speaker 1>So really it's just a very very efficient way of

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<v Speaker 1>heating up a lot of water really quickly and making

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<v Speaker 1>it do work. Yes, a very efficient, very radioactive steam generator. Yeah. Yeah,

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<v Speaker 1>And that's one of the big issues with the fission

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<v Speaker 1>power plants obviously, is that it uses nuclear radioactive material,

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<v Speaker 1>not just nuclear material, radioactive material, and that it doesn't

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<v Speaker 1>the radioactivity is still very much a factor once that

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<v Speaker 1>reaction is finished four thousands and thousands of years, right. Yeah.

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<v Speaker 1>Generally speaking, only about three percent of the uranium in

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<v Speaker 1>a uranium rod is used up in a fission reactor

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<v Speaker 1>before the waste has to be disposed of because it

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<v Speaker 1>will continue to heat up until it reaches a point

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<v Speaker 1>that's too hot and the reactor itself can suffer a failure.

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<v Speaker 1>You have, that's what you have, the meltdown. Yeah. Uh.

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<v Speaker 1>There are some uh, some approaches that are suggesting that

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<v Speaker 1>we take another pass at that nuclear waste and use

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<v Speaker 1>that in a second round by immersing it in a

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<v Speaker 1>molten salt the waist annihilating molten salt reactor, which I

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<v Speaker 1>still I just can't I can't get over the the

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<v Speaker 1>annihilator part of the waist annihilator. Uh. Yeah. So this

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<v Speaker 1>this reactor would it's still a fission reactor, but it

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<v Speaker 1>would immerse the radioactive material the uranium in a molten

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<v Speaker 1>salt and use that to control the heat in a

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<v Speaker 1>in a way that would allow you to use that

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<v Speaker 1>material for longer, so you'd be able to get more

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<v Speaker 1>use out of the same radioactive material and reduce the

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<v Speaker 1>life of the actual radioactive elements at the at the

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<v Speaker 1>final output, I think it would only be radioactive. It

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<v Speaker 1>would only be reactive for another years. Yeah, so still

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<v Speaker 1>well beyond our lifetimes right now. But not something that

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<v Speaker 1>you would say, alright, generation and generations and generations are

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<v Speaker 1>going to have to be aware of that. You don't

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<v Speaker 1>have to start, you know, programming things that people, you know,

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<v Speaker 1>languages that don't exist yet want to be able to understand.

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<v Speaker 1>How do I how do I create a pictograph that

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<v Speaker 1>shows exactly do not go in here? Wessed it up

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<v Speaker 1>really hard? Right in ten thousand years, English may not

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<v Speaker 1>even be a thing anymore. So, um so yeah, I

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<v Speaker 1>mean that's that's one of those possible solutions. But fusion

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<v Speaker 1>is very different. Fission all about splitting atoms apart. Fusion

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<v Speaker 1>is about being buddy buddy and bringing atoms together. This

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<v Speaker 1>is this is the kind of of process that we

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<v Speaker 1>see happening in stars, including the sun. Did the sun

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<v Speaker 1>being a star? Yes, yes, Well I'm just making sure

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<v Speaker 1>people know that. And despite what my one of my

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<v Speaker 1>favorite bands has said in a cover of a song,

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<v Speaker 1>actually the sun is not really a massive incandescent gas,

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<v Speaker 1>the gigantic nuclear fulness. But they did correct it in

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<v Speaker 1>a later song and say it was a miasma of

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<v Speaker 1>incandesc and plasma. So they did go back and correct it,

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<v Speaker 1>but they were actually quoting an old song from a

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<v Speaker 1>science album for kids, which was to explain the process

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<v Speaker 1>of fusion and how the Sun generates energy and light

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<v Speaker 1>and uh. And the way it happens is it takes

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<v Speaker 1>these hydrogen atoms, and because the Sun is so massive

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<v Speaker 1>and dense, there's a huge amount of gravity there and

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<v Speaker 1>it's creating an enormous amount of pressure and heat. So

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<v Speaker 1>the heat is stripping those hydrogen atoms of their electrons,

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<v Speaker 1>creating ions. Um that creates ions, and in a pure

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<v Speaker 1>hydrogen atom is just a proton and an electron, so

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<v Speaker 1>that electron goes away. Now you've just got a proton there.

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<v Speaker 1>And so you have these protons now that are zipping

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<v Speaker 1>around an incredible um and being pressed together really tightly

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<v Speaker 1>by the amazing force of gravity. And at the Sun's

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<v Speaker 1>core where this is the strongest, these atoms are banging

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<v Speaker 1>up against each other so fast and so close that

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<v Speaker 1>one of the other fundamental forces in the universe overacts

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<v Speaker 1>the electromagnetic force. Now, the four forces in the universe

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<v Speaker 1>include gravity, which is the weakest, but is the it

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<v Speaker 1>is the most effective over huge distances. You have electromagnetic force,

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<v Speaker 1>and then you have the strong and weak nuclear forces. Now,

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<v Speaker 1>the strong force is what holds nucleic particles together. It's

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<v Speaker 1>like the glue that keeps a nucleus together, right, right,

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<v Speaker 1>So if you were able to get two protons close

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<v Speaker 1>enough to each other, uh, the strong nuclear force would

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<v Speaker 1>be strong enough to counteract the electromagnetic force. That's it's

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<v Speaker 1>naturally driving them apart. Because protons both have a positive charge.

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<v Speaker 1>And if you've ever taken to magnets and tried to

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<v Speaker 1>stick the two positive ends together, it resists to you.

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<v Speaker 1>It doesn't want to do that thing. But when you

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<v Speaker 1>get them to within one alliant of a millimeter of

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<v Speaker 1>each other, yeah, then that will that will go away,

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<v Speaker 1>or it will be overcome by the strong exactly. Yeah,

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<v Speaker 1>so you have to get them really really close together. Now,

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<v Speaker 1>at that pomp point, when you have fused to hydrogen

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<v Speaker 1>protons together, you have created a different element. Hydrogen has

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<v Speaker 1>now become helium at a temperature millions of degrees. So yeah,

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<v Speaker 1>we can't see we might both be that, they might

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<v Speaker 1>be giants. I'll be seeing them in a week to

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<v Speaker 1>come into Atlanta. By the time you guys hear this,

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<v Speaker 1>I've already seen it and the show was awesome, I guess.

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<v Speaker 1>So anyway, the the protons have fused together to form helium.

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<v Speaker 1>But here's the interesting thing. In that process. The mass

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<v Speaker 1>of that helium atom is slightly less than the combined

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<v Speaker 1>masses of the two hydrogen atoms that fused together to

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<v Speaker 1>make the helium. Why is that, Jonathan, Some that mass

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<v Speaker 1>gets converted into energy. Now, there's a little equation you

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<v Speaker 1>may have heard of called E equals MC squared. I

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<v Speaker 1>think I think some some guy named Einstein was talking

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<v Speaker 1>about that. I don't know. Listen here Einstein. Yeah, Einstein

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<v Speaker 1>came up with this idea where he came up with

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<v Speaker 1>the theory and and turns out that it looks like

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<v Speaker 1>it's true energy equals mass times this square or the

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<v Speaker 1>speed of light squared, rather not the square speed of light,

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<v Speaker 1>but the speed of light squared. So speed of light

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<v Speaker 1>is a big, big, big, big number. Then you square

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<v Speaker 1>it and it's even bigger, bigger, and you multiply financially bigger. Yeah,

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<v Speaker 1>and multiply that times whatever the mass is. You get

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<v Speaker 1>your energy output and so essentially, what this equation tells

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<v Speaker 1>us is that a tiny little bit of mass, once

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<v Speaker 1>converted into energy, will be an enormous amount of energy

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<v Speaker 1>the same thing. And also the mass and energy never

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<v Speaker 1>really go way, and they are simply converted. Exactly. We

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<v Speaker 1>cannot create or destroy energy, but what we can do

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<v Speaker 1>is convert energy to mass and mass to energy. At

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<v Speaker 1>least in theory. Now, if we were to convert energy

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<v Speaker 1>to mass, it would take an awful lot of energy

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<v Speaker 1>to make just a little bit of mass. Which is

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<v Speaker 1>why I always go crazy when I read the Harry

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<v Speaker 1>Potter books and people conjure stuff out of thin air,

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<v Speaker 1>because I think, do you you just destroyed like three

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<v Speaker 1>solar systems in order to do that, clearly pulling them

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<v Speaker 1>from a parallel dimension or something like that. Yes, so

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<v Speaker 1>there's just a people in a parallel dimension' Like it's

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<v Speaker 1>so cold, there's a there's a really huge room of

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<v Speaker 1>requirement somewhere. That's all right, Now you're talking about language.

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<v Speaker 1>So yeah, a little bit of mass creates a lot

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<v Speaker 1>of energy. So even though we're talking tiny atomic measurements

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<v Speaker 1>here where we have the helium atom, which has got

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<v Speaker 1>a lower mass than the two combined hydrogen atoms that

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<v Speaker 1>still puts off quite a bit of energy. And and

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<v Speaker 1>the Sun is doing this all the time with tons

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<v Speaker 1>of hydrogen converting to helium every day. All right, so

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<v Speaker 1>massive amount of energy that's being that's being admitted, I mean,

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<v Speaker 1>and if it weren't being emitted, then there would be

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<v Speaker 1>a life on this planet. And we know it works,

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<v Speaker 1>you know, so we conserve this. This is this is

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<v Speaker 1>as far as we can tell real science. Yes, so

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<v Speaker 1>we know it works, we know we can do it.

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<v Speaker 1>In fact, we have done it. We've reproduced it here

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<v Speaker 1>on Earth. We'll get into that in a little bit.

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<v Speaker 1>But the question was if the Sun does this, if

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<v Speaker 1>that's how the Sun does this, could we create energy

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<v Speaker 1>here on Earth using a similar method, Knowing that on

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<v Speaker 1>Earth the conditions are very different from the core of

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<v Speaker 1>the Sun. We don't have that gravity or that heat

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<v Speaker 1>that is allowing the Sun to overcome the right. Yeah,

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<v Speaker 1>this and this, and the gravity is the really important part,

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<v Speaker 1>because that gravity is what's allowing that this nuclear fusion

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<v Speaker 1>process to happen at a temperature that would actually be

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<v Speaker 1>lower than it we would need here on Earth because

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<v Speaker 1>we don't have that gravity. We don't have the ability

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<v Speaker 1>to compress the atoms as tightly together as we would

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<v Speaker 1>if if we had the Sun's gravity. We have to

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<v Speaker 1>we have to overcome that with even more heat. Yeah,

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<v Speaker 1>the Sun only needs about fifteen million degrees kelvin. Only

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<v Speaker 1>am easily fifteen million kelvin. Sorry sorry, yeah, yeah, yeah,

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<v Speaker 1>my my bad. I always do that. I did it

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<v Speaker 1>once and one of our great listeners corrected me. And

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<v Speaker 1>that's the only reason, because our listeners are awesome and

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<v Speaker 1>they let me know when I've done something silly like that,

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<v Speaker 1>completely ridiculous, the only reason I know, So, thank you listeners.

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<v Speaker 1>Um so, so, yeah, the Sun only needs about fifteen

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<v Speaker 1>million kelvin. In order to do this here on Earth,

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<v Speaker 1>it would be something like a hundred million. Yeah, so

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<v Speaker 1>we're talking massive amounts of energy that we would need

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<v Speaker 1>here on Earth to compensate for the fact that we

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<v Speaker 1>don't have that gravity there to help us with this reaction. Um. Now,

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<v Speaker 1>in the Sun, you're talking about the pure hydrogen encountering

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<v Speaker 1>other pure hydrogen. So one proton, one electron, the electrons

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<v Speaker 1>get stripped away, the protons get fused together. But on Earth,

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<v Speaker 1>we've discovered that there's a better combination to go with

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<v Speaker 1>it requires less energy than it would if we were

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<v Speaker 1>to use pure hydrogen. Right, It's it's relatively difficult to

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<v Speaker 1>run into pure hydrogen here. Yeah, you would have to

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<v Speaker 1>you would have to essentially split the hydrogen off of

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<v Speaker 1>something else. There's lots of hydrogen on Earth. We have

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<v Speaker 1>no shortage of it. Yeah, it's just connected to lots

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<v Speaker 1>of other stuff. So. Um. The two types of the

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<v Speaker 1>two isotopes of hydrogen and isotope by the way, means

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<v Speaker 1>that you have more or fewer neutrons than whatever the

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<v Speaker 1>the atom typically has. But it's or it's it's a

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<v Speaker 1>different number of neutrons than the base version of that atom,

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<v Speaker 1>but it's um same number of protons, same number of electrons.

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<v Speaker 1>So an isotope is one isotope of hydrogen is a deuterium,

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<v Speaker 1>which is also known as heavy hydrogen, and it has

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<v Speaker 1>one proton and one neutron, So typically you would not

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<v Speaker 1>have a neutron with hydrogen. Deuterium does have a neutron.

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<v Speaker 1>And then you have tritium, which is called also called

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<v Speaker 1>heavy heavy hydrogen, so it's extra heavy. He's not heavy,

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<v Speaker 1>he's my tritium. Uh. And this is a proton that

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<v Speaker 1>has two neutrons. Uh so the same still the same element,

0:13:15.920 --> 0:13:19.520
<v Speaker 1>it's just a different isotope. Now deuterium, we've got a

0:13:19.520 --> 0:13:21.440
<v Speaker 1>lot of that here on Earth. Yeah, it can be

0:13:21.480 --> 0:13:25.200
<v Speaker 1>extracted from seawater. It's not radioactive or anything. Yeah, it's

0:13:25.240 --> 0:13:28.480
<v Speaker 1>not dangerous um that but yeah, you can. You can

0:13:28.520 --> 0:13:33.920
<v Speaker 1>find deuterium in in ocean water. Um. You cannot find

0:13:33.920 --> 0:13:38.840
<v Speaker 1>tritium very easily, mostly because it's not completely stable. It

0:13:38.840 --> 0:13:41.599
<v Speaker 1>does tend to decay and it's just it has a

0:13:41.600 --> 0:13:43.840
<v Speaker 1>half life of about ten years. But you can. You

0:13:43.880 --> 0:13:46.560
<v Speaker 1>can get it from lithium. Yeah, you you if you

0:13:46.600 --> 0:13:51.040
<v Speaker 1>take lithium, the metal lithium, not the medication, the metal lithium,

0:13:51.120 --> 0:13:53.640
<v Speaker 1>and you bombard it with neutrons, then one of the

0:13:53.679 --> 0:13:56.240
<v Speaker 1>things you get out of that is tritium. So that

0:13:56.440 --> 0:13:59.000
<v Speaker 1>is one way to get the treatium and it we

0:13:59.120 --> 0:14:01.400
<v Speaker 1>found out that treaty um and deuterium, if you try

0:14:01.440 --> 0:14:04.360
<v Speaker 1>to fuse those two together, then you get helium and

0:14:04.440 --> 0:14:09.160
<v Speaker 1>a neutron out of that reaction, and uh, it requires

0:14:09.240 --> 0:14:13.160
<v Speaker 1>less energy than than other combinations. Do write these are

0:14:13.160 --> 0:14:16.400
<v Speaker 1>the current forms of fusion that are possible on our planet.

0:14:16.520 --> 0:14:19.880
<v Speaker 1>Are our deuterium tritium. Hey guys, hope you're enjoying this

0:14:19.960 --> 0:14:22.080
<v Speaker 1>classic episode of tech stuff. We're going to take a

0:14:22.160 --> 0:14:32.640
<v Speaker 1>quick break to thank our sponsors. All right, let's get

0:14:32.640 --> 0:14:35.480
<v Speaker 1>back to fusion. So we've got the deuterium in the

0:14:35.520 --> 0:14:38.840
<v Speaker 1>sea water. We can bombard some lithium with some neutrons

0:14:38.880 --> 0:14:41.760
<v Speaker 1>and get some tritium out of that. We're ready to

0:14:42.440 --> 0:14:46.800
<v Speaker 1>introduce the deuterium to the tritium and uh and and

0:14:46.840 --> 0:14:50.080
<v Speaker 1>make a date and have them fused together in a

0:14:50.200 --> 0:14:53.520
<v Speaker 1>single unit of helium and shoot off an extra neutron

0:14:53.840 --> 0:14:55.920
<v Speaker 1>and a lot of energy. What do we need to do?

0:14:56.640 --> 0:14:59.359
<v Speaker 1>So we know that we're going to be using deuterium

0:14:59.400 --> 0:15:02.920
<v Speaker 1>and tritium because that's the the most efficient way that

0:15:02.960 --> 0:15:05.520
<v Speaker 1>we've found so far to be able to do. It's

0:15:05.560 --> 0:15:07.800
<v Speaker 1>the easiest for for us to use deuterium. Deuterium would

0:15:07.800 --> 0:15:10.880
<v Speaker 1>actually be more efficient, but it's more difficult to get started.

0:15:11.280 --> 0:15:13.880
<v Speaker 1>I see, I see so right, So we we might

0:15:13.920 --> 0:15:16.600
<v Speaker 1>get more energy output with deuterium deuterium, but it would

0:15:16.600 --> 0:15:19.600
<v Speaker 1>also require more energy to get the whole thing started, right,

0:15:19.640 --> 0:15:21.880
<v Speaker 1>which is kind of the entire problem with fusion. Yeah,

0:15:22.680 --> 0:15:24.320
<v Speaker 1>that's that's that's the bigges, all right, we'll just go

0:15:24.360 --> 0:15:26.120
<v Speaker 1>ahead and say that one of the biggest challenges we

0:15:26.160 --> 0:15:29.160
<v Speaker 1>face with fusion is the fact that in order to

0:15:29.280 --> 0:15:31.480
<v Speaker 1>make a fusion reaction here on Earth, you have to

0:15:31.480 --> 0:15:34.040
<v Speaker 1>pour in a great deal of energy so that you

0:15:34.080 --> 0:15:38.760
<v Speaker 1>can create the the the the situation you need to hear,

0:15:38.800 --> 0:15:41.160
<v Speaker 1>you're replicating what goes on in a star. That's really

0:15:41.360 --> 0:15:44.000
<v Speaker 1>a lot of temperature, a lot of pressure. So in

0:15:44.120 --> 0:15:46.520
<v Speaker 1>order to do that without all that pressure here on Earth,

0:15:46.560 --> 0:15:49.480
<v Speaker 1>we've got to pour and even more temperature. So that's

0:15:49.520 --> 0:15:52.320
<v Speaker 1>the big challenge is how do you create a reaction

0:15:52.360 --> 0:15:55.000
<v Speaker 1>that's going to generate more energy through the output than

0:15:55.040 --> 0:15:58.520
<v Speaker 1>it required to start it. So if it requires more

0:15:58.640 --> 0:16:00.640
<v Speaker 1>energy to go in, then you get out. You have

0:16:00.680 --> 0:16:03.640
<v Speaker 1>an energy sync. You actually you're in the red and

0:16:03.680 --> 0:16:06.520
<v Speaker 1>that's not really useful. I mean, it's it's pretty it's

0:16:06.520 --> 0:16:09.760
<v Speaker 1>still pretty cool, yeah, but just doesn't commercially viable. I

0:16:09.760 --> 0:16:12.880
<v Speaker 1>guess if you want to make helium, uh, they're probably

0:16:15.480 --> 0:16:18.400
<v Speaker 1>we are running out. I mean, but still that's a

0:16:18.400 --> 0:16:21.320
<v Speaker 1>lot of energy you're pouring into making some balloons float

0:16:21.880 --> 0:16:24.400
<v Speaker 1>or cooling the large Hadron collider. However you want to

0:16:24.400 --> 0:16:26.040
<v Speaker 1>think about it, all right, but so so we do

0:16:26.120 --> 0:16:28.640
<v Speaker 1>have we do. There's two main ways that we are

0:16:28.680 --> 0:16:31.600
<v Speaker 1>experimenting with this on Earth, and one of those it's

0:16:31.640 --> 0:16:35.800
<v Speaker 1>called magnetic confinement. Right, So magnetic confinement is what was

0:16:36.000 --> 0:16:40.720
<v Speaker 1>used in the joint European Torus or jet fusion reactor.

0:16:41.320 --> 0:16:43.800
<v Speaker 1>And this was sort of a test reactor. It wasn't

0:16:43.920 --> 0:16:48.200
<v Speaker 1>meant to be, uh like an electrical generator, right right,

0:16:48.240 --> 0:16:50.000
<v Speaker 1>It wasn't a power plant. It was more science is

0:16:50.080 --> 0:16:52.680
<v Speaker 1>cool than anything else. But and this is a good

0:16:52.680 --> 0:16:55.440
<v Speaker 1>point to say that, you know, ultimately the way we

0:16:55.480 --> 0:16:58.600
<v Speaker 1>would generate electricity with these is not that we have

0:16:58.680 --> 0:17:03.480
<v Speaker 1>some magical like power. Yeah. They just dug into the

0:17:03.480 --> 0:17:05.879
<v Speaker 1>bolts and then it pulls. Yeah. This is still a

0:17:05.920 --> 0:17:08.399
<v Speaker 1>steam generator. Yeah, which is which is really interesting to

0:17:08.400 --> 0:17:11.040
<v Speaker 1>me because you know, this is technically this is steam punk.

0:17:11.119 --> 0:17:17.159
<v Speaker 1>I mean, yeah, we're essentially harnessing the power of the

0:17:15.280 --> 0:17:21.080
<v Speaker 1>stom the stars themselves to turn water into steam. Yeah,

0:17:21.320 --> 0:17:23.560
<v Speaker 1>it's still it's still converting water to steam to turn

0:17:24.640 --> 0:17:28.080
<v Speaker 1>really efficiently and a lot of water because you're talking

0:17:28.080 --> 0:17:30.679
<v Speaker 1>about a lot of heat. So then that's the That's

0:17:30.720 --> 0:17:32.359
<v Speaker 1>the other thing is that if if you could have

0:17:32.440 --> 0:17:34.919
<v Speaker 1>used the same amount of energy, you used to start

0:17:34.960 --> 0:17:40.399
<v Speaker 1>the reaction to heat up some water and get a

0:17:40.400 --> 0:17:43.200
<v Speaker 1>better effect than Obviously, this makes no sense. I mean,

0:17:43.200 --> 0:17:45.040
<v Speaker 1>that's the whole point is that we have to find

0:17:45.040 --> 0:17:48.240
<v Speaker 1>a way to do a fusion reaction where we're getting

0:17:48.280 --> 0:17:50.800
<v Speaker 1>more energy than we're putting into it. Otherwise, just take

0:17:50.840 --> 0:17:54.240
<v Speaker 1>the reactor out and just direct your energy to water directly,

0:17:54.520 --> 0:17:58.879
<v Speaker 1>take out the middleman. But magnetic confinement you mentioned it

0:17:59.000 --> 0:18:04.680
<v Speaker 1>uses a really powerful magnetic field to hold the ionized

0:18:04.960 --> 0:18:08.880
<v Speaker 1>gas in place. An Ionized gas is plasma. So plasma

0:18:08.960 --> 0:18:11.199
<v Speaker 1>is a gas where you've got free roaming electrons. That

0:18:11.400 --> 0:18:13.959
<v Speaker 1>is what the sun is. That's you know, all that

0:18:14.000 --> 0:18:16.840
<v Speaker 1>heat has stripped away the electrons, you've poured energy in,

0:18:17.400 --> 0:18:20.720
<v Speaker 1>You've pushed the electrons away. You've got these free flowing

0:18:21.240 --> 0:18:26.600
<v Speaker 1>uh nuclei inside the plasma. And then the magnetic field

0:18:26.680 --> 0:18:30.800
<v Speaker 1>starts to press all of these nuclei together until you

0:18:30.840 --> 0:18:33.640
<v Speaker 1>are able to fuse them. And what you get ore

0:18:34.359 --> 0:18:38.919
<v Speaker 1>helium atoms and free neutrons. The neutrons fly off and

0:18:38.960 --> 0:18:42.960
<v Speaker 1>they hit what they call blankets, blankets of lithium. Yeah, blankets.

0:18:43.320 --> 0:18:45.760
<v Speaker 1>Lithium is in the blanket as well, yes, and that

0:18:45.760 --> 0:18:48.679
<v Speaker 1>that means that because remember, if you bombard lithium with

0:18:48.680 --> 0:18:51.280
<v Speaker 1>a neutron, you create tritium, which means that you can

0:18:51.320 --> 0:18:54.280
<v Speaker 1>continually create part of the fuel source you need for

0:18:54.280 --> 0:18:56.960
<v Speaker 1>this reactually while you're in the middle of the process. Yeah,

0:18:56.960 --> 0:18:59.360
<v Speaker 1>it's pretty pretty neat. Yeah, And it's also giving off

0:18:59.359 --> 0:19:01.080
<v Speaker 1>a lot of energy in the form of heat, which

0:19:01.160 --> 0:19:04.160
<v Speaker 1>is then heating up the water to turn into steam, etcetera, etcetera.

0:19:04.640 --> 0:19:08.600
<v Speaker 1>So that's magnetic confinement. Um, and we use different things

0:19:08.600 --> 0:19:11.680
<v Speaker 1>to heat up the plasma, like we might use microwaves

0:19:11.760 --> 0:19:15.720
<v Speaker 1>or lasers or electricity or I think that that accelerator

0:19:15.840 --> 0:19:20.119
<v Speaker 1>driven neutral particle beams are our our integral in the

0:19:21.000 --> 0:19:25.000
<v Speaker 1>international through nuclear experimental reactor or either which is the

0:19:25.000 --> 0:19:28.440
<v Speaker 1>one in France. Yes, it comes from France. That one,

0:19:29.119 --> 0:19:33.920
<v Speaker 1>Yes it does. That one is still being built and

0:19:34.200 --> 0:19:38.399
<v Speaker 1>it's it's projected to be finished and protected, projected to

0:19:38.400 --> 0:19:42.119
<v Speaker 1>be online by although whether or not that is a

0:19:42.160 --> 0:19:45.520
<v Speaker 1>true fact or not is you know, remains to be seen. Yeah. Yeah,

0:19:45.560 --> 0:19:48.480
<v Speaker 1>So if it stays on target, then we'll be able

0:19:48.520 --> 0:19:52.359
<v Speaker 1>to say by you know, if this is actually a

0:19:52.440 --> 0:19:56.280
<v Speaker 1>viable means of generating electricity for us. By the way,

0:19:57.119 --> 0:20:01.119
<v Speaker 1>the Chamber has a special name. It's a it's a

0:20:01.960 --> 0:20:04.680
<v Speaker 1>how did how do we decided that this tacomac. Yeah,

0:20:06.040 --> 0:20:08.280
<v Speaker 1>we've got Tacomax here in Atlantic. Yeah, so it keeps

0:20:08.320 --> 0:20:11.040
<v Speaker 1>throwing me out. Taco Mac is a is a restaurant

0:20:11.119 --> 0:20:16.000
<v Speaker 1>chain in Atlanta that has obviously tacos. But this is toomac.

0:20:16.400 --> 0:20:20.200
<v Speaker 1>It's actually a Russian acronym for heroidal chamber with axial

0:20:20.240 --> 0:20:23.399
<v Speaker 1>magnetic field, which basically means it's a donut. It's a

0:20:23.440 --> 0:20:30.040
<v Speaker 1>magnetic it's a magnetic donut, magnetic donut. Yeah. And granted

0:20:30.080 --> 0:20:31.840
<v Speaker 1>this is this is a you know, the Eider version

0:20:31.920 --> 0:20:34.960
<v Speaker 1>is a is a hundred foot tall, twenty three thousand ton,

0:20:35.560 --> 0:20:40.560
<v Speaker 1>million part donut, enormous magnetic donut. Yeah. And the reason

0:20:40.640 --> 0:20:42.879
<v Speaker 1>for the donut shape is they've found that that is

0:20:42.960 --> 0:20:47.600
<v Speaker 1>the most effective way of of containing the plasma in

0:20:47.600 --> 0:20:51.360
<v Speaker 1>this really tight field so that you can have these

0:20:51.359 --> 0:20:54.960
<v Speaker 1>fusion reactions take place. So we've got magnetic confinement. There's

0:20:54.960 --> 0:20:59.439
<v Speaker 1>another method which has receives some some attention early on,

0:20:59.560 --> 0:21:01.359
<v Speaker 1>and there's still some labs, like there's some in the

0:21:01.400 --> 0:21:04.280
<v Speaker 1>United States that are still looking at this approach, and

0:21:04.280 --> 0:21:06.560
<v Speaker 1>it may even turn out that this ends up generating

0:21:06.600 --> 0:21:10.000
<v Speaker 1>more energy in the long run than the magnetic confinement.

0:21:10.040 --> 0:21:12.720
<v Speaker 1>But we're still trying to figure that out. It's called

0:21:12.800 --> 0:21:16.159
<v Speaker 1>inertial confinement, right, And this is using laser beams or

0:21:16.200 --> 0:21:19.520
<v Speaker 1>ion beams to squeeze and heat that hydrogen plasma. Yeah.

0:21:19.680 --> 0:21:24.200
<v Speaker 1>In this case, really they take a pellet a frozen hydrogen,

0:21:24.760 --> 0:21:27.879
<v Speaker 1>so you have deuterium and tritium in an actual physical pellet.

0:21:27.960 --> 0:21:31.080
<v Speaker 1>So you're talking super cold, yeah yeah, and and and

0:21:31.119 --> 0:21:33.320
<v Speaker 1>peace sized, I mean like little bitty thing. Yeah. And

0:21:33.359 --> 0:21:36.399
<v Speaker 1>you're using these these lasers or ions to heat that

0:21:36.440 --> 0:21:40.439
<v Speaker 1>pellet into a plasma almost instantaneously. I mean you're just

0:21:40.640 --> 0:21:43.880
<v Speaker 1>you're bombarding it with an enormous amount of energy. And

0:21:44.520 --> 0:21:47.920
<v Speaker 1>essentially what's happening is that all right, if you've ever

0:21:47.960 --> 0:21:51.119
<v Speaker 1>seen the magic trick where the magician walks up to

0:21:51.480 --> 0:21:54.640
<v Speaker 1>the the the dining table with all the beautiful glassware

0:21:54.640 --> 0:21:57.960
<v Speaker 1>and everything that's perched perfectly on the tablecloth, and then

0:21:57.960 --> 0:21:59.800
<v Speaker 1>he grabs the table cloth because it a quick jerk

0:21:59.800 --> 0:22:02.800
<v Speaker 1>and anything stays therein bankmen failed to do and Gus

0:22:02.880 --> 0:22:06.560
<v Speaker 1>Fuster exactly. Yeah, it's the same same sort of idea here,

0:22:06.600 --> 0:22:10.040
<v Speaker 1>and that you are heating it up so fast that

0:22:10.119 --> 0:22:13.439
<v Speaker 1>because it's because this is a compressed pellet and the

0:22:13.560 --> 0:22:15.960
<v Speaker 1>lasers are actually compressing it. Our ions are compressing it

0:22:16.040 --> 0:22:20.760
<v Speaker 1>even further as it's being heated up. Before the electromagnetic

0:22:20.840 --> 0:22:23.439
<v Speaker 1>force has the opportunity to push the atoms apart, the

0:22:23.480 --> 0:22:27.240
<v Speaker 1>strong nuclear force fuses them together and so kind of implodes. Yeah,

0:22:27.240 --> 0:22:31.440
<v Speaker 1>so you've gotta do. I mean, it's happening super fast now,

0:22:32.040 --> 0:22:35.120
<v Speaker 1>the fraction and like one millionth of a second, I think,

0:22:35.200 --> 0:22:38.400
<v Speaker 1>is how fast this happens. It's insane and and uh,

0:22:38.640 --> 0:22:41.760
<v Speaker 1>it's there are other differences between the initial confinement and

0:22:41.840 --> 0:22:45.080
<v Speaker 1>magnetic confinement. With magnetic convironment, the goal is to find

0:22:45.080 --> 0:22:48.840
<v Speaker 1>a way to have ongoing fusion reactions so that you

0:22:48.920 --> 0:22:52.600
<v Speaker 1>don't have to just generate electricity or generate heat and spurts.

0:22:52.600 --> 0:22:55.840
<v Speaker 1>That you could actually have a maintained reaction that goes

0:22:55.880 --> 0:22:58.119
<v Speaker 1>on for an extended amount of time to generate as

0:22:58.200 --> 0:23:02.240
<v Speaker 1>much electricity as is needed, whereas inertial confinement you'd have

0:23:02.280 --> 0:23:05.359
<v Speaker 1>to set up multiple essentially multiple targets right right, because

0:23:05.680 --> 0:23:07.440
<v Speaker 1>the way that the way that one of them works

0:23:07.520 --> 0:23:11.399
<v Speaker 1>At the National Ignition Facility of Lawrenceville, Livermore, laboratory in

0:23:11.440 --> 0:23:14.640
<v Speaker 1>the United States in California, I believe UM it uses

0:23:14.680 --> 0:23:17.320
<v Speaker 1>a hundred ninety two laser beams to focus on a

0:23:17.359 --> 0:23:20.320
<v Speaker 1>single point in a test chamber UM and this single

0:23:20.320 --> 0:23:23.080
<v Speaker 1>point is where that little piece sized bit of hy

0:23:23.359 --> 0:23:26.440
<v Speaker 1>hydrogen is sitting. And and so you know, they're they're

0:23:26.480 --> 0:23:31.280
<v Speaker 1>working on ways to focus the lasers better and essentially

0:23:31.320 --> 0:23:33.639
<v Speaker 1>have multiple pellets and and also yeah, and and to

0:23:33.720 --> 0:23:36.760
<v Speaker 1>have to have chambers, multiple chambers with multiple pellets that

0:23:36.800 --> 0:23:39.199
<v Speaker 1>are going off in succession so that you create a

0:23:39.240 --> 0:23:42.879
<v Speaker 1>continuous and quoting quotation marks in the air reaction. So

0:23:42.920 --> 0:23:45.880
<v Speaker 1>it's it's a challenging thing. And if if they are

0:23:45.920 --> 0:23:48.359
<v Speaker 1>able to crack it, it has the potential to create

0:23:48.520 --> 0:23:51.800
<v Speaker 1>quite a bit of electricity, uh so much so that

0:23:52.200 --> 0:23:55.800
<v Speaker 1>we could start to really take the load off of

0:23:55.960 --> 0:23:59.560
<v Speaker 1>things like fossil fuel based power plants. Right right Their

0:23:59.760 --> 0:24:03.720
<v Speaker 1>talk about UM with with inertial confinement a fifty two

0:24:03.800 --> 0:24:07.360
<v Speaker 1>hundred times more energy UM output than than you would

0:24:07.400 --> 0:24:09.920
<v Speaker 1>have to put in, whereas the numbers that I've seen

0:24:09.920 --> 0:24:12.880
<v Speaker 1>for it or anyway are more like seven times. So

0:24:13.280 --> 0:24:15.560
<v Speaker 1>you know, either way, you're still getting a lot of

0:24:15.640 --> 0:24:19.280
<v Speaker 1>energy out and we're not there yet no one has

0:24:19.400 --> 0:24:21.920
<v Speaker 1>No one has created a fusion reactor here on Earth

0:24:22.400 --> 0:24:24.960
<v Speaker 1>that has been efficient enough for it to be a

0:24:24.960 --> 0:24:29.240
<v Speaker 1>meaningful way to create electricity. Uh, because you would be

0:24:29.280 --> 0:24:32.680
<v Speaker 1>losing energy on the deal. So if these work out,

0:24:32.800 --> 0:24:35.200
<v Speaker 1>it's going to be fantastic. There are there are a

0:24:35.240 --> 0:24:37.119
<v Speaker 1>lot of challenges here. I mean, you can imagine, if

0:24:37.119 --> 0:24:39.919
<v Speaker 1>we're talking about using these incredible amounts of heat, you

0:24:39.960 --> 0:24:42.159
<v Speaker 1>have to be able to design a reactor that can

0:24:42.240 --> 0:24:44.919
<v Speaker 1>withstand handle it. Yeah, and that's tough. It's not an

0:24:44.920 --> 0:24:47.399
<v Speaker 1>easy thing to do. So that's a big challenge. And

0:24:47.400 --> 0:24:50.199
<v Speaker 1>then well we've got other ones as well. And again

0:24:50.600 --> 0:24:53.800
<v Speaker 1>scientists will say like it's about twenty years away. Hopefully

0:24:54.080 --> 0:24:56.840
<v Speaker 1>they're right right now. I think one of the challenges

0:24:56.880 --> 0:25:00.040
<v Speaker 1>is almost a societal challenge because people here fusion and

0:25:00.600 --> 0:25:04.240
<v Speaker 1>they think fission and they think radioactive and meltdown and

0:25:04.320 --> 0:25:08.320
<v Speaker 1>not in my backyard and etcetera. Whereas fusion is potentially

0:25:08.320 --> 0:25:12.800
<v Speaker 1>anyway loads safer than a fission reactor, you don't you're

0:25:12.800 --> 0:25:15.400
<v Speaker 1>not talking about you know, your output is a neutron

0:25:15.800 --> 0:25:19.200
<v Speaker 1>and helium. It's not a heavy radioactive material that's going

0:25:19.240 --> 0:25:23.040
<v Speaker 1>to have a half life of several thousand years. It's

0:25:23.400 --> 0:25:27.719
<v Speaker 1>stuff that is harmless once you have harnessed it. Uh So,

0:25:27.760 --> 0:25:29.159
<v Speaker 1>really the question would be, you know, as long as

0:25:29.200 --> 0:25:32.080
<v Speaker 1>the reactor is well made and solid, you don't have

0:25:32.119 --> 0:25:36.160
<v Speaker 1>to worry about this heat escaping or the other kind

0:25:36.200 --> 0:25:39.320
<v Speaker 1>of of a mechanical failure. Well, like like any other

0:25:39.880 --> 0:25:43.520
<v Speaker 1>steam turbine generator, it's going to have an impact on

0:25:43.520 --> 0:25:45.240
<v Speaker 1>the environment and that you know, you're going to be

0:25:45.280 --> 0:25:47.919
<v Speaker 1>taking in water and and that's an impact, and it's

0:25:47.920 --> 0:25:49.959
<v Speaker 1>going to be putting off steam, which is an impact.

0:25:50.040 --> 0:25:51.480
<v Speaker 1>And there are a lot of there are a lot

0:25:51.520 --> 0:25:54.760
<v Speaker 1>of designs I've seen where they have built in a

0:25:54.840 --> 0:25:57.800
<v Speaker 1>system where they condense the steam back down into the water,

0:25:57.840 --> 0:26:00.520
<v Speaker 1>so it becomes a closed loop. So least then you

0:26:00.560 --> 0:26:03.199
<v Speaker 1>are I mean, you still probably have a loss. I

0:26:03.240 --> 0:26:06.120
<v Speaker 1>mean it's it's hard to create a perfectly closed loop.

0:26:06.560 --> 0:26:08.679
<v Speaker 1>But if you could, then you could just essentially use

0:26:08.760 --> 0:26:11.359
<v Speaker 1>the same water over and over and over again, because

0:26:11.400 --> 0:26:12.680
<v Speaker 1>you know, the steam is just going to condense in

0:26:12.720 --> 0:26:14.440
<v Speaker 1>the water and then the water will go back into

0:26:14.480 --> 0:26:16.639
<v Speaker 1>steam once you heat it up. Yeah, and so and again,

0:26:16.680 --> 0:26:18.080
<v Speaker 1>you know, even if you do have even if you

0:26:18.080 --> 0:26:19.920
<v Speaker 1>do have a loss, you're not going to be having

0:26:20.040 --> 0:26:22.440
<v Speaker 1>Blanky the three eyed fish in the river outside, right,

0:26:22.520 --> 0:26:25.400
<v Speaker 1>So so yeah, there's you know, and and who knows,

0:26:25.440 --> 0:26:29.359
<v Speaker 1>maybe that'll really generate enough helium for us. I mostly

0:26:29.440 --> 0:26:32.439
<v Speaker 1>joke about that because I seriously doubt there's any useful

0:26:32.480 --> 0:26:35.560
<v Speaker 1>way to harness and a huge amount of helium from

0:26:35.600 --> 0:26:39.080
<v Speaker 1>these reactions. Guys, I hope you're not fused too closely

0:26:39.320 --> 0:26:42.000
<v Speaker 1>with this topic because we need to take another quick break,

0:26:42.000 --> 0:26:52.919
<v Speaker 1>but we'll be right back. Cold fusion is kind of

0:26:52.960 --> 0:26:54.560
<v Speaker 1>what it sounds like. I mean, the idea is what

0:26:54.640 --> 0:26:57.600
<v Speaker 1>it sounds like, and it's it's not actually cold. It's

0:26:57.640 --> 0:27:01.159
<v Speaker 1>more room temperature room to infusion, but that's less of

0:27:01.160 --> 0:27:04.879
<v Speaker 1>a fun buzzword, so compared to a hundred million degree reaction,

0:27:05.040 --> 0:27:09.800
<v Speaker 1>it's comed um, but no. Cold fusion is the idea

0:27:09.840 --> 0:27:13.720
<v Speaker 1>that view would be able to create these reactions, these

0:27:13.720 --> 0:27:18.119
<v Speaker 1>fusion reactions at essentially room temperature and still get energy

0:27:18.200 --> 0:27:20.320
<v Speaker 1>off of them, which, if it were true, would be

0:27:20.400 --> 0:27:22.560
<v Speaker 1>huge because that would mean that we wouldn't have to

0:27:22.560 --> 0:27:25.600
<v Speaker 1>pour in so much energy to start the reaction. You

0:27:25.720 --> 0:27:29.480
<v Speaker 1>just have to set up the right situation and harnestly

0:27:30.200 --> 0:27:33.720
<v Speaker 1>the energy that comes off of it and make free

0:27:33.800 --> 0:27:36.639
<v Speaker 1>energy for everybody, right, proponents of it. I like to

0:27:36.680 --> 0:27:40.480
<v Speaker 1>call it low energy nuclear reactions. Yeah, because cold fusion

0:27:40.480 --> 0:27:43.439
<v Speaker 1>definitely has a stigma against it now. And that's the

0:27:43.480 --> 0:27:46.879
<v Speaker 1>reason for that, all right. So, so there were a

0:27:46.920 --> 0:27:50.680
<v Speaker 1>pair of scientists, Pons and Fleishman, who published a paper

0:27:51.160 --> 0:27:55.960
<v Speaker 1>that was that that became really famous, and it was

0:27:56.000 --> 0:27:58.960
<v Speaker 1>that this they were talking about a reaction that that

0:27:59.000 --> 0:28:02.600
<v Speaker 1>they observed that gave off more energy than it should

0:28:02.640 --> 0:28:06.639
<v Speaker 1>have based upon what they did. Right. What happened was

0:28:06.960 --> 0:28:10.240
<v Speaker 1>they put an electrode of pollitium into a thermis of

0:28:10.240 --> 0:28:13.639
<v Speaker 1>heavy water of tridium oxide um and charged it with

0:28:13.680 --> 0:28:19.080
<v Speaker 1>an electrical current, and I supposedly the pollitium catalyzed fusion

0:28:19.119 --> 0:28:22.600
<v Speaker 1>by allowing the du tritium atoms to snuggle up. So,

0:28:23.000 --> 0:28:25.360
<v Speaker 1>in other words, they were able to create a fusion

0:28:25.400 --> 0:28:28.479
<v Speaker 1>reaction at a at a very low temperature comparatively speaking,

0:28:28.960 --> 0:28:31.960
<v Speaker 1>and the temperature and that they observed an excess of

0:28:32.040 --> 0:28:35.000
<v Speaker 1>energy being given off by this. So they were like, eureka,

0:28:35.119 --> 0:28:38.440
<v Speaker 1>we have found a way to create electricity or really

0:28:38.480 --> 0:28:42.840
<v Speaker 1>to create energy through this reaction. And then a few

0:28:42.960 --> 0:28:46.720
<v Speaker 1>labs tried to replicate their results, and early results seemed

0:28:46.840 --> 0:28:49.800
<v Speaker 1>to replicate it at least in a couple of instances,

0:28:50.000 --> 0:28:54.040
<v Speaker 1>but upon further study, it seemed like most of those

0:28:54.040 --> 0:28:59.200
<v Speaker 1>successes were due to either mechanical error like someone someone

0:28:59.240 --> 0:29:02.160
<v Speaker 1>miss read spread that something, or it was a poorly

0:29:02.200 --> 0:29:06.160
<v Speaker 1>calibrated sensor, or yeah, exactly like like there was there

0:29:06.160 --> 0:29:09.400
<v Speaker 1>always seemed to be something wrong with the experiment that

0:29:09.520 --> 0:29:12.320
<v Speaker 1>put whatever, the results were within the margin of error,

0:29:12.640 --> 0:29:14.880
<v Speaker 1>and if it's within the margin of error, you cannot

0:29:15.000 --> 0:29:19.120
<v Speaker 1>really be sure that you've got an actual positive result.

0:29:19.960 --> 0:29:23.960
<v Speaker 1>So Ponds and Flashman continued to talk about their studies

0:29:23.960 --> 0:29:28.080
<v Speaker 1>and continue to be proponents of this idea, but it

0:29:28.320 --> 0:29:34.600
<v Speaker 1>increasingly became sort of kind of a pathological science, is

0:29:34.640 --> 0:29:37.600
<v Speaker 1>what other scientists were calling it, you know, which essentially

0:29:37.600 --> 0:29:40.239
<v Speaker 1>means joke and science talk. Now they were saying that

0:29:40.480 --> 0:29:43.760
<v Speaker 1>there was no real proof of it working, that the

0:29:43.800 --> 0:29:46.560
<v Speaker 1>results were not replicable, which is something that's important in

0:29:46.560 --> 0:29:50.040
<v Speaker 1>science as it turns out, and that there doesn't doesn't

0:29:50.040 --> 0:29:53.120
<v Speaker 1>seem to be any support based upon our understanding of

0:29:53.160 --> 0:29:55.960
<v Speaker 1>the universe that cold fusion could actually be a thing.

0:29:56.600 --> 0:29:58.720
<v Speaker 1>And this wasn't the only time that it's been attempted.

0:29:58.960 --> 0:30:02.360
<v Speaker 1>Back in two th five, E. C. L A researchers

0:30:02.400 --> 0:30:06.320
<v Speaker 1>were working without Hyer electric crystals um to to create

0:30:06.560 --> 0:30:10.840
<v Speaker 1>electric fields in in water. Normal normal, old stuff. And

0:30:11.040 --> 0:30:13.880
<v Speaker 1>in two thousand nine, the U. S. Navy's UH Space

0:30:13.920 --> 0:30:17.440
<v Speaker 1>in Naval Warfare Systems Department was trying some stuff. Yeah,

0:30:17.440 --> 0:30:20.400
<v Speaker 1>and just it doesn't seem to have ever panned out.

0:30:20.400 --> 0:30:24.280
<v Speaker 1>Now there are conspiracy theorists who suggests that perhaps big

0:30:24.400 --> 0:30:28.360
<v Speaker 1>energy companies are suppressing information about cold fusion and have

0:30:28.880 --> 0:30:34.400
<v Speaker 1>compromised the scientific community as such. Uh and therefore cold

0:30:34.400 --> 0:30:36.080
<v Speaker 1>fusion could be a thing, but we don't know about

0:30:36.080 --> 0:30:38.800
<v Speaker 1>it because people are actively working against us from learning

0:30:38.840 --> 0:30:41.040
<v Speaker 1>about it. I would not go so far as to

0:30:41.040 --> 0:30:44.040
<v Speaker 1>say that. I will say that there is enough of

0:30:44.080 --> 0:30:47.800
<v Speaker 1>a stigma against cold fusion and low energy nuclear reactions

0:30:48.400 --> 0:30:54.719
<v Speaker 1>within the literature world that most magazines won't scientific publishing right,

0:30:54.760 --> 0:30:57.240
<v Speaker 1>so they just they dismiss it out of hand. Now

0:30:57.680 --> 0:31:00.400
<v Speaker 1>that I think people can make a legitimate argument that

0:31:00.600 --> 0:31:04.120
<v Speaker 1>is probably shortsighted, that that they should, they should at

0:31:04.200 --> 0:31:07.440
<v Speaker 1>least consider them so that other scientists have the opportunity

0:31:07.520 --> 0:31:11.120
<v Speaker 1>to observe the to to learn about the results, try

0:31:11.120 --> 0:31:14.200
<v Speaker 1>and replicate it, and then that's how we can at

0:31:14.240 --> 0:31:17.040
<v Speaker 1>least at least make a consideration about it before, rather

0:31:17.080 --> 0:31:19.840
<v Speaker 1>than dismissing it out of hand as Yeah, I think

0:31:19.840 --> 0:31:21.920
<v Speaker 1>I think dismissing it out of hand ends up just

0:31:22.240 --> 0:31:25.200
<v Speaker 1>creating more fuel for the conspiracy theorists. Now, personally, I

0:31:25.280 --> 0:31:28.680
<v Speaker 1>don't think there's anything to it. Counter counter culture. What's

0:31:28.760 --> 0:31:32.240
<v Speaker 1>the I was I was lectured about the terminology conspiracy theorists.

0:31:32.840 --> 0:31:35.959
<v Speaker 1>I'm sorry that the conspiracy theorists hate the term conspiracy theorist.

0:31:36.240 --> 0:31:39.800
<v Speaker 1>I'm really sorry about that. Um So anyway, Yeah, we're

0:31:39.800 --> 0:31:42.480
<v Speaker 1>gonna have Ben and Madden here, Hunter, bring them on.

0:31:42.760 --> 0:31:45.560
<v Speaker 1>I will bends my arch nemesis. Everyone knows that, so

0:31:46.000 --> 0:31:47.840
<v Speaker 1>uh And if you didn't know that, now you do.

0:31:48.160 --> 0:31:50.440
<v Speaker 1>I called him my arch nemesis the very first day

0:31:50.440 --> 0:31:53.760
<v Speaker 1>I met him, six years ago. So and it has

0:31:53.800 --> 0:31:56.880
<v Speaker 1>held true. We, by the way, share trains to train

0:31:57.000 --> 0:31:59.160
<v Speaker 1>rights together and chat all the way and talk about music.

0:31:59.280 --> 0:32:02.760
<v Speaker 1>Very very little actual arch nemesis story. He's about as

0:32:02.840 --> 0:32:05.760
<v Speaker 1>lazy a hero as I am, lazy as supervillain. So

0:32:05.880 --> 0:32:08.560
<v Speaker 1>really nothing happens, really is that how it works out?

0:32:08.640 --> 0:32:10.480
<v Speaker 1>He's he's the hero, you're the villain. I mean, you're

0:32:10.600 --> 0:32:14.600
<v Speaker 1>you're You've got that that's that's the problem, right, I mean,

0:32:14.680 --> 0:32:16.640
<v Speaker 1>I have to be the villain by default by Star

0:32:16.640 --> 0:32:19.560
<v Speaker 1>Trek rules. We got off on a tangent. So anyway,

0:32:19.600 --> 0:32:21.959
<v Speaker 1>so anyway, the science does not seem to hold up

0:32:22.360 --> 0:32:24.400
<v Speaker 1>cold fusion. It just doesn't seem to be There doesn't

0:32:24.440 --> 0:32:28.120
<v Speaker 1>seem to be any support there. Now, maybe there actually

0:32:28.160 --> 0:32:30.440
<v Speaker 1>is a way of doing it. Maybe there is, and

0:32:30.880 --> 0:32:34.440
<v Speaker 1>it's just that whatever results were found were due to

0:32:34.600 --> 0:32:37.640
<v Speaker 1>something else and it just hasn't been discovered in the

0:32:37.680 --> 0:32:41.680
<v Speaker 1>other examples. And maybe it'll turn out that that is

0:32:41.760 --> 0:32:44.600
<v Speaker 1>the answer, which would be amazing, and I think everyone

0:32:44.680 --> 0:32:48.360
<v Speaker 1>really wants that world to exist, absolutely, it would. It

0:32:48.360 --> 0:32:50.760
<v Speaker 1>would mean that our energy problems, we would we would

0:32:50.800 --> 0:32:52.959
<v Speaker 1>be in an energy surplus to the point where when

0:32:52.960 --> 0:32:57.320
<v Speaker 1>you have energy surplus, so many things become possible. Yeah,

0:32:57.320 --> 0:32:59.040
<v Speaker 1>it's it's one of those things that you know that

0:32:59.120 --> 0:33:01.360
<v Speaker 1>you kind of start seeing in something like Star Trek,

0:33:01.400 --> 0:33:04.680
<v Speaker 1>where it's it's just this perfect utopian universe where a

0:33:04.720 --> 0:33:07.160
<v Speaker 1>lot of people don't have to work anymore because we

0:33:07.240 --> 0:33:09.760
<v Speaker 1>have we have free energy, so we have free transportation,

0:33:09.800 --> 0:33:12.920
<v Speaker 1>so we have free food. So yeah, and so obviously

0:33:12.960 --> 0:33:14.840
<v Speaker 1>this would be a pretty great world and I think

0:33:14.840 --> 0:33:18.560
<v Speaker 1>it's pretty cynical, maybe not completely unrealistic to say that

0:33:18.600 --> 0:33:21.880
<v Speaker 1>corporations would suppress such a world for their own gain,

0:33:21.920 --> 0:33:23.800
<v Speaker 1>because I actually think they would have more to gain

0:33:23.960 --> 0:33:26.800
<v Speaker 1>in the utopia version of the world than in the

0:33:26.840 --> 0:33:28.760
<v Speaker 1>current one. But I don't know. I'm not a I'm

0:33:28.760 --> 0:33:31.440
<v Speaker 1>not a CEO of a major corporation, so maybe I

0:33:31.480 --> 0:33:33.160
<v Speaker 1>would think in a different way if I were. I

0:33:33.160 --> 0:33:35.320
<v Speaker 1>can I can see how how changing the status quo

0:33:35.360 --> 0:33:37.360
<v Speaker 1>could be a scary thing. Yeah, and I'm too lazy

0:33:37.400 --> 0:33:42.120
<v Speaker 1>to try again, super villain lazy, so um yeah, anyway,

0:33:42.880 --> 0:33:47.360
<v Speaker 1>it'll I'm interested to see how the the fusion reactors

0:33:47.440 --> 0:33:50.840
<v Speaker 1>like it turn turn out over the next couple of

0:33:50.880 --> 0:33:55.120
<v Speaker 1>decades um. If anyone does make advances in the cold

0:33:55.200 --> 0:33:58.920
<v Speaker 1>fusion field, that would be phenomenal. And you know, while

0:33:58.920 --> 0:34:01.320
<v Speaker 1>I am a skeptic, and I fully admit that I'm

0:34:01.320 --> 0:34:04.120
<v Speaker 1>a skeptic, I'm also a person who if you show

0:34:04.200 --> 0:34:07.680
<v Speaker 1>me evidence that really supports the claim and it's replicable,

0:34:08.120 --> 0:34:10.520
<v Speaker 1>then I'm going to say, like, Okay, you're right. I mean,

0:34:10.560 --> 0:34:13.560
<v Speaker 1>that's that's how science works. That's all right. I am

0:34:13.600 --> 0:34:17.840
<v Speaker 1>willing to say, like, Okay, my my skepticism was was

0:34:17.880 --> 0:34:20.880
<v Speaker 1>not well founded because here we have proofd right, but

0:34:20.960 --> 0:34:23.239
<v Speaker 1>until then, yeah, until then, I'm a skeptic. One of

0:34:23.239 --> 0:34:25.480
<v Speaker 1>my one of my favorite stories about that, there's a

0:34:25.520 --> 0:34:30.000
<v Speaker 1>Scottish physicist named Douglas Morrison who would attend these cold

0:34:30.040 --> 0:34:33.319
<v Speaker 1>fusion conferences every year and and and listen and from

0:34:33.320 --> 0:34:37.120
<v Speaker 1>what I understand, really genuinely listen to these people who

0:34:37.200 --> 0:34:39.719
<v Speaker 1>had these brilliant ideas about about how these things might

0:34:39.760 --> 0:34:42.640
<v Speaker 1>work and how they were supposedly working in their own labs.

0:34:43.000 --> 0:34:45.560
<v Speaker 1>And he would stand up and say, can you please

0:34:45.600 --> 0:34:48.120
<v Speaker 1>make me a cup of tea? And they would go, well,

0:34:48.120 --> 0:34:50.120
<v Speaker 1>I can't produce that much heat yet, and he would go,

0:34:50.200 --> 0:34:54.320
<v Speaker 1>oh yeah. That's the other thing is that if cold fusion,

0:34:54.440 --> 0:34:58.200
<v Speaker 1>if these reactions are actually happening, if if there really

0:34:58.239 --> 0:35:01.319
<v Speaker 1>is something to it, the problem would be can it

0:35:01.400 --> 0:35:04.360
<v Speaker 1>be scaled up to something that's useful? And if it

0:35:04.440 --> 0:35:07.239
<v Speaker 1>can't be scaled up, then it may be that all right, well,

0:35:07.239 --> 0:35:10.120
<v Speaker 1>we've learned something interesting that we didn't know before, which

0:35:10.200 --> 0:35:14.040
<v Speaker 1>is always valuable. But if it's not practical to use

0:35:14.120 --> 0:35:17.160
<v Speaker 1>this in any way of generating electricity, it doesn't actually

0:35:17.160 --> 0:35:20.600
<v Speaker 1>meet the problem that we're trying to solve, So that's

0:35:20.600 --> 0:35:23.520
<v Speaker 1>something else to keep in mind, although personally I'm always

0:35:23.560 --> 0:35:28.080
<v Speaker 1>like knowledge for knowledge sake. Alright, guys, that wraps up

0:35:28.120 --> 0:35:30.839
<v Speaker 1>another classic episode of tech Stuff. Hope you enjoyed it.

0:35:31.200 --> 0:35:34.320
<v Speaker 1>If you have any suggestions for future episodes of tech Stuff,

0:35:34.400 --> 0:35:36.520
<v Speaker 1>let me know. You can send me a message on

0:35:36.560 --> 0:35:40.080
<v Speaker 1>Facebook or on Twitter. I'm Text Stuff h s w

0:35:40.400 --> 0:35:43.640
<v Speaker 1>at both, and I'll talk to you again really soon.

0:35:48.360 --> 0:35:51.359
<v Speaker 1>Text Stuff is an I Heart Radio production. For more

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