WEBVTT - Going Nuclear

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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. Welcome everyone to Forward Thinking, the audio podcast

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<v Speaker 1>where we think about the future talk about what is

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<v Speaker 1>to come. Today, we're going to talk a little bit

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<v Speaker 1>about fusion and what that is. I am Jonathan Strickland,

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<v Speaker 1>I'm Lauren Vocaldon, and I'm Joe McCormick. And so fusion. Yeah,

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<v Speaker 1>we're talking about nuclear reactions. And uh, you guys might

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<v Speaker 1>be familiar with the fact that the world has lots

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<v Speaker 1>of nuclear reactors already, So why aren't we talking about

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<v Speaker 1>fusion as being in the future. Uh, And the reason

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<v Speaker 1>for that is the nuclear reactors that are out there,

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<v Speaker 1>I mean the majority of the ones that are actually

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<v Speaker 1>generating power than well, because there are experimental all the

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<v Speaker 1>ones that are hooked up to a grid. Yeah, are

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<v Speaker 1>fission based, which is where you are essentially, you're you're

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<v Speaker 1>making Adam split apart. In the case of nuclear fission,

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<v Speaker 1>you're using a a type of uranium, and the uranium

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<v Speaker 1>is is going through radioactive decay, which gives off a

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<v Speaker 1>lot of heat. Uranium it's it's because it's heavy, right,

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<v Speaker 1>it's a huge atom. Well, it's it's heavy it's heavy

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<v Speaker 1>and and it does decay right like, especially when you're

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<v Speaker 1>getting it. The specific type of uranium used in nuclear

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<v Speaker 1>reactions is different than just like if you found unrefined uranium.

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<v Speaker 1>It's this is refined uranium that that decays at a

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<v Speaker 1>predictable rate and as it as it decays, it spontaneously

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<v Speaker 1>causes other atoms in the uranium to decay, so it starts.

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<v Speaker 1>Once the reaction starts, it kind of maintains itself for

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<v Speaker 1>a certain amount of time. And what you're essentially doing

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<v Speaker 1>is you are you're you're submerging these these radioactive uranium

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<v Speaker 1>rods in water, which converts the water into steam that

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<v Speaker 1>then turns steam turbines. It's not terribly efficient, but it

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<v Speaker 1>does generate an awful lot of electricity. It's more efficient

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<v Speaker 1>than say a coal generator that is burning coal to

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<v Speaker 1>heat water into steam to turn Yeah, it's it's more

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<v Speaker 1>more efficient than coal combustion. And uh, you know, you're

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<v Speaker 1>generating an entirely different kind of waste instead of instead

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<v Speaker 1>of greenhouse gas emissions, you're you've got this kind of

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<v Speaker 1>nuclear material that's radioactive and harmful to humans, and we'll

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<v Speaker 1>be radio radioactive for a very long time, as it

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<v Speaker 1>turns out. But well, we'll talk about in another episode

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<v Speaker 1>of this of this show, we'll talk about kind of

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<v Speaker 1>a way of trying to use that nuclear to waste

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<v Speaker 1>in a a in a smart way. Okay, So what

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<v Speaker 1>happens in these reactions? We we say that we're splitting

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<v Speaker 1>a heavy atom? Right, Yeah? Why does that create so

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<v Speaker 1>much energy? I bet this has something to do with Einstein, doesn't? Yes?

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<v Speaker 1>It does. Well, you know, for for one thing, you're

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<v Speaker 1>talking about mass and mass converting into energy. You've heard

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<v Speaker 1>of a little equation equals mc squared, right, and that

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<v Speaker 1>that tells us that matter and energies are in some

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<v Speaker 1>way equivalent. Right, Yes, one can produce another, right if

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<v Speaker 1>you if you go back far enough. According to the

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<v Speaker 1>Big Bang theory, there was a point where energy and

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<v Speaker 1>mass were one thing, and then they kind of split apart.

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<v Speaker 1>So they are intrinsically connected to one another. And so

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<v Speaker 1>if you were to convert matter into energy, you get

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<v Speaker 1>a lot of it because you take that mass and

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<v Speaker 1>you multiply it by C squared. C squared that's the

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<v Speaker 1>speed of light squared. So a little bit of mass

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<v Speaker 1>times the speed of light, which is pretty big and

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<v Speaker 1>you square that, then you get the equivalent amount of

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<v Speaker 1>energy out. That's a lot of energy for just a

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<v Speaker 1>tiny bit of mass. So even on the atomic level,

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<v Speaker 1>you're talking about lots of energy when you have these

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<v Speaker 1>these reactions. Now that's fission. Uh. Fusion is something different.

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<v Speaker 1>Fusion is what happens in the sun. So you know, right, yes, yes, Uh,

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<v Speaker 1>it's when instead of splitting atoms, you are fusing them. Yeah.

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<v Speaker 1>Celestial stars, by the way, not stars. Um first, well,

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<v Speaker 1>it's do this and and and As much as I

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<v Speaker 1>would love to go on about how the Sun is

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<v Speaker 1>a massive incandescent gas, the gigant techniclear fairness, where hydrogen

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<v Speaker 1>is built into helium and a temperature millions of degrees. Uh.

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<v Speaker 1>Which is a song that they Might Be Giants made popular.

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<v Speaker 1>It was actually a song that was on a science

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<v Speaker 1>album for kids. I have the original track. It's amazing,

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<v Speaker 1>but they Might Be Giants actually went back and corrected

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<v Speaker 1>that because, of course science has later found that that's

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<v Speaker 1>kind of an oversimplification of what the sun is cover

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<v Speaker 1>going on and ignoring Joe. Uh. So, fusion is when

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<v Speaker 1>you are fusing two atoms together. Generally speaking, you want

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<v Speaker 1>to start with light atoms and fuse them. And the

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<v Speaker 1>way you have to do this is, well, there are

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<v Speaker 1>certain fundamental forces that are in the universe. Okay, You've

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<v Speaker 1>got an electromagnetic force, that's one of them. And then

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<v Speaker 1>there's the strong nuclear force. Now, strong nuclear force, that's

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<v Speaker 1>the force that holds these sub atomic particles together. And

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<v Speaker 1>it's really really strong. But it were works on incredibly

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<v Speaker 1>short distances. Okay, so when it when it comes into effect,

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<v Speaker 1>it's incredibly strong. Okay. But so in a fusion reaction,

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<v Speaker 1>you're you're taking little hydrogen atoms, the smallest atoms that

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<v Speaker 1>there are, single proton, and you're fusing them together to

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<v Speaker 1>create helium atoms which have two protons. Right, if we have,

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<v Speaker 1>say a hydrogen balloon, why doesn't this happen inside the balloon.

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<v Speaker 1>Why don't the hydrogen atoms spontaneously fused together to create

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<v Speaker 1>helium atoms? All? Right? That distance is a really big

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<v Speaker 1>problem because when I'm saying really close distance, I'm talking

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<v Speaker 1>really really close to one trillion of a millimeter, I think,

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<v Speaker 1>is how close things have to be diffused. Now, those

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<v Speaker 1>protons that are in a hydrogen atom, they have a

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<v Speaker 1>positive charge, right, So positive charges don't like each other,

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<v Speaker 1>like charges repel one another, right right, Like, So if

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<v Speaker 1>you take two positive ends of a magnet and try

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<v Speaker 1>to smooh them together, Yeah, you're gonna feel that push.

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<v Speaker 1>It'll it'll feel like it's pushing against you. So what

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<v Speaker 1>you have to do is you have to actually get

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<v Speaker 1>those atoms close enough. Uh. You have to overcome the

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<v Speaker 1>electromagnetic force, so that the strong nuclear force takes hold,

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<v Speaker 1>which requires you to put a lot of energy into

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<v Speaker 1>the system for this to work. Now, with the Sun,

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<v Speaker 1>that energy ends up being gravity and heat. You've got

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<v Speaker 1>this intense amount of heat in the Sun. It's stripping

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<v Speaker 1>the protons of their electrons. It's becoming a plasma. A

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<v Speaker 1>plasma is an ionized gas, and it's exactly what it

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<v Speaker 1>sounds like. You've got ions. These are charged atoms because

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<v Speaker 1>they have either gained or lost an electron. In this case,

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<v Speaker 1>lost electrons um it's and those electrons roam freely throughout

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<v Speaker 1>the plasma. So anyway you've got you have to create

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<v Speaker 1>a plasma first, so you have to pour energy into it.

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<v Speaker 1>Plasma it's like fire. It's incredibly hot. Saying that plasma

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<v Speaker 1>is like fires like saying a fumble of water is

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<v Speaker 1>like an ocean, yes, but not but it doesn't get

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<v Speaker 1>the scale. Yeah, so very pressurized. Right, So you've got

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<v Speaker 1>you've got this incredibly hot uh, these incredibly hot atoms

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<v Speaker 1>that are getting closer and closer to each other. You're

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<v Speaker 1>forcing them together and then if they get close enough,

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<v Speaker 1>that strong nuclear force is going to be strong enough

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<v Speaker 1>to bind them two together. Now here's the really interesting thing. Uh,

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<v Speaker 1>the mass of that new nucleus in the case of

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<v Speaker 1>hydrogen becoming helium, the mass of that new nucleus is

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<v Speaker 1>actually less than the product of the two hydrogen nuclei.

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<v Speaker 1>So that makes me wonder if that mass went somewhere

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<v Speaker 1>it did? You've that that mass that is lost when

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<v Speaker 1>these two atoms, these two nuclei fused together to make

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<v Speaker 1>one nucleus, is converted into energy, which is energy in

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<v Speaker 1>the form of heat. So again, if you create a

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<v Speaker 1>fusion reaction, it creates a lot of heat, which can

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<v Speaker 1>you know, depending on how you use it, can actually

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<v Speaker 1>help create more reactions down the line, like in say

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<v Speaker 1>the sun. Um. So the challenge here, you've got the

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<v Speaker 1>the equals mc squared again, so you get a lot

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<v Speaker 1>of energy for this tiny little sub atomic particle that

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<v Speaker 1>you know, this nucleus that is slightly less mass than

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<v Speaker 1>the product of the two nuclear that formed it. You

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<v Speaker 1>get a lot of energy out of that, but but

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<v Speaker 1>you have to pour a lot of energy into the

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<v Speaker 1>system first to even get to that fusion reaction. And

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<v Speaker 1>that's the problem that we have right now, is the

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<v Speaker 1>idea of how do we do this in such an

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<v Speaker 1>efficient way that the energy we get out makes sense

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<v Speaker 1>compared to energy we pour in now, or it's significantly greater. Yeah,

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<v Speaker 1>if we if we can do that, if we can

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<v Speaker 1>figure that out, fusion has some amazing promises you're talking

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<v Speaker 1>about as an energy sources, as a source of just

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<v Speaker 1>great electricity like vission. Right exactly. If if we can

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<v Speaker 1>get to the point where we have solved the problem

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<v Speaker 1>of of getting more energy out of this process than

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<v Speaker 1>we have to create to put into it, then because

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<v Speaker 1>we're talking about things like hydrogen, you could end up

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<v Speaker 1>with an energy surplus pretty quickly. Yeah. Well, don't they say,

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<v Speaker 1>I mean the amount of energy you get out of

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<v Speaker 1>a fusion burn is it's hundreds of millions of times

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<v Speaker 1>more than the energy you get from an equivalent fossil

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<v Speaker 1>fuel burn. Depending on how many reactions you're talking about.

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<v Speaker 1>I think it's actually four million times if I think

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<v Speaker 1>about it, like if you're talking about one single reaction,

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<v Speaker 1>it's like four million times the amount of energy would

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<v Speaker 1>get out of burning coal or oil. And I mean

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<v Speaker 1>that's incredible, right, And I mean that's like the the

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<v Speaker 1>you know, these tiny little reactions that do require a

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<v Speaker 1>lot of energy to start them. No, no carbon emissions,

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<v Speaker 1>right right, and uh, plentiful resources. Right. So how if

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<v Speaker 1>you want to make a fusion reactor reactor here on Earth,

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<v Speaker 1>what do you have to put into it? Well, at first,

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<v Speaker 1>you've got to create a reactor that can withstand tremendous

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<v Speaker 1>amount of heat. All right, we'll get there in a minute.

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<v Speaker 1>But what is the fuel. It's it's two isotopes of hydrogen,

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<v Speaker 1>and an isotope means that it's a it's an atom

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<v Speaker 1>of that element with a different number of neutrons. Yeah. Yeah,

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<v Speaker 1>you have to get that to fuse them together. Yes,

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<v Speaker 1>and you and the two you need are deuterium and tritium. Yeah,

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<v Speaker 1>those are the ones that are currently being used. Yeah.

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<v Speaker 1>Those are not hard to get at all. From what

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<v Speaker 1>I read like, deuterium is just abundant in the ocean.

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<v Speaker 1>You you scoop up some ocean water and a glass

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<v Speaker 1>and there's deuterium in it, right, Yeah. I've often refused

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<v Speaker 1>to go into the ocean because it was just deterium

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<v Speaker 1>with it. Yeah yeah, but now yeah, that's and smell

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<v Speaker 1>the deuterium in the air. The other I think is

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<v Speaker 1>a created from from lithium, I believe, and so it's

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<v Speaker 1>a little yeah yeah, so it's it's a little bit

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<v Speaker 1>more expensive and to produce. Currently, the two different kinds

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<v Speaker 1>of of fusion reactors that they use both have a

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<v Speaker 1>deuterium and tritium reactions, and they're working on some that

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<v Speaker 1>are a duty arium deuterium reactions, which would be a

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<v Speaker 1>lot easier because since the tritium is made from lithium,

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<v Speaker 1>it's kind of expensive, and then you could just use

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<v Speaker 1>the seawater essentially. In any case, the fuel is totally abundant, right,

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<v Speaker 1>much more so than for example, uranium, right fuels exactly,

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<v Speaker 1>So then that there you have an energy surplus, which

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<v Speaker 1>would be an amazing and kind of like unimaginable world

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<v Speaker 1>compared to the one we live in right now. So

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<v Speaker 1>I etricity is free, then we can do as much

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<v Speaker 1>as we want, Well, maybe not free, because there are

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<v Speaker 1>some challenges, right, right, right, So there's the challenge of

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<v Speaker 1>building a reactor that's going to withstand the heat. If

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<v Speaker 1>it's this, if it's this greater deal, why aren't we

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<v Speaker 1>doing it yet? That's part of it is that it's

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<v Speaker 1>expensive to build a reactor that can withstand the tremendous

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<v Speaker 1>amount of heat that would be given off. And again,

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<v Speaker 1>the reaction here, the fusion reaction, that heat that you're generating,

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<v Speaker 1>you're doing it. You're doing the same thing with that

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<v Speaker 1>heat that you would do with the fission reactor. You're

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<v Speaker 1>using it to heat up water to turn steam turbines.

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<v Speaker 1>It's not magic, yeah, yeah, the fusan the fusion doesn't

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<v Speaker 1>just automatic create electricity and suddenly all the lights go

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<v Speaker 1>bright in the entire city. It's actually turning steam turbine.

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<v Speaker 1>But we are talking about like a hundred million kelvin

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<v Speaker 1>something on that magnitude like actually like six times hotter

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<v Speaker 1>than the Sun, I believe times. Then the core of

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<v Speaker 1>the Sun, well, see the core of the Sun, and

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<v Speaker 1>so the fusion reactions go on in the core of

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<v Speaker 1>the Sun. And so but it's got its tremendous gravity

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<v Speaker 1>to help it. Out here on Earth, we don't have

0:12:27.160 --> 0:12:29.640
<v Speaker 1>that kind of gravity. So, right, the Sun's a pressure cooker,

0:12:30.160 --> 0:12:32.960
<v Speaker 1>and our reactor would not be a pressure cook right,

0:12:33.000 --> 0:12:35.280
<v Speaker 1>not in the same way at least, So you've got

0:12:35.280 --> 0:12:38.440
<v Speaker 1>to find a way to contain this heat. And obviously,

0:12:38.480 --> 0:12:40.560
<v Speaker 1>if you think about it like um, if this is

0:12:40.600 --> 0:12:44.480
<v Speaker 1>something that's causing hydrogen atoms to fuse together and you

0:12:44.520 --> 0:12:47.760
<v Speaker 1>put it against any material surface, it's going to melt it.

0:12:47.840 --> 0:12:51.240
<v Speaker 1>You know, it's it's going to cause major damage that

0:12:51.280 --> 0:12:53.920
<v Speaker 1>the reactor won't be able to sustain itself. So what

0:12:53.960 --> 0:12:56.640
<v Speaker 1>do you do. You have to contain that plasma in

0:12:56.720 --> 0:12:59.679
<v Speaker 1>some way, in a way that it doesn't have contact

0:12:59.720 --> 0:13:02.480
<v Speaker 1>with the outer walls of the containment chamber. And there

0:13:02.480 --> 0:13:06.560
<v Speaker 1>are two main methods that we've used to try and

0:13:06.720 --> 0:13:12.440
<v Speaker 1>control plasma. Each way has multiple versions of it, but

0:13:12.559 --> 0:13:16.680
<v Speaker 1>the two main ways we're using lasers or as I

0:13:16.720 --> 0:13:21.359
<v Speaker 1>used to say on textuff lasers, that's that's inertial confinement,

0:13:21.600 --> 0:13:25.200
<v Speaker 1>yes uh. And then there's h using magnetism. So you're

0:13:25.240 --> 0:13:29.560
<v Speaker 1>trying to contain the plasma so that it's the reactions

0:13:29.600 --> 0:13:31.800
<v Speaker 1>are happening exactly where you want them to. It's not

0:13:31.880 --> 0:13:34.440
<v Speaker 1>going to. I mean, heat is not something that radiates

0:13:34.440 --> 0:13:38.440
<v Speaker 1>out indefinitely, so it dissipates very quickly. Actually, so you

0:13:38.480 --> 0:13:42.040
<v Speaker 1>can have a very intensely hot reaction happening and a

0:13:42.200 --> 0:13:46.960
<v Speaker 1>very localized point and not melt the surface of the earth.

0:13:47.240 --> 0:13:49.480
<v Speaker 1>You know. It's not not like we suddenly see the

0:13:49.840 --> 0:13:53.559
<v Speaker 1>fusion reaction go out of control and goodbye, you know, Seattle.

0:13:53.880 --> 0:13:58.000
<v Speaker 1>It's not not quite that that dramatic. But but but

0:13:58.080 --> 0:14:01.000
<v Speaker 1>the magnetism was the one that I think has received

0:14:01.000 --> 0:14:05.320
<v Speaker 1>the most attention recently. That's the method that was used

0:14:05.320 --> 0:14:09.480
<v Speaker 1>at the joint European Taurus or Jet reactor. And then

0:14:09.559 --> 0:14:14.240
<v Speaker 1>for us, that's the word. It means doughnut basically, right, Okay,

0:14:14.840 --> 0:14:18.839
<v Speaker 1>it does, Actually it means bear claw. Now, Taurus is

0:14:18.880 --> 0:14:21.920
<v Speaker 1>a it's a shape. It's a three dimensional shapes like

0:14:22.000 --> 0:14:24.120
<v Speaker 1>what we would call it donut. Yeah. Yeah, Well, it

0:14:24.160 --> 0:14:26.640
<v Speaker 1>turns out that the easiest way to get plasma to

0:14:26.760 --> 0:14:30.000
<v Speaker 1>flow this this crazy hydrogen plasma to flow through this

0:14:30.040 --> 0:14:32.240
<v Speaker 1>magnetic field is in a donut shape. And we're talking

0:14:32.240 --> 0:14:34.480
<v Speaker 1>about a doughnut that's like a hundred feet tall, ways

0:14:34.840 --> 0:14:38.320
<v Speaker 1>twenty three thousand tons um and is made of some

0:14:38.480 --> 0:14:42.280
<v Speaker 1>million parts. So yeah, it's the Homer Simpson dream donut. Yes,

0:14:42.400 --> 0:14:46.480
<v Speaker 1>yes so. Uh so JET the Joint European Taurus UH

0:14:47.160 --> 0:14:51.600
<v Speaker 1>used this magnetic confinement method and UH and at its

0:14:51.640 --> 0:14:55.440
<v Speaker 1>at its height, was able to produce reactions where they

0:14:55.440 --> 0:14:59.040
<v Speaker 1>would get a little over half the amount of energy

0:14:59.080 --> 0:15:02.320
<v Speaker 1>they needed to to start the reaction. So, in other words,

0:15:02.320 --> 0:15:06.000
<v Speaker 1>their efficiency was somewhere around in the mid sixty percentile.

0:15:06.600 --> 0:15:10.080
<v Speaker 1>So that's not great. I mean, obviously you're you're losing energy.

0:15:10.120 --> 0:15:14.360
<v Speaker 1>It's very promising, it's pretty cool, but yeah, yeah, you couldn't.

0:15:14.360 --> 0:15:16.120
<v Speaker 1>That wouldn't be a power generator. That would be a

0:15:16.120 --> 0:15:19.400
<v Speaker 1>power sink because you would always be putting more power

0:15:19.560 --> 0:15:21.600
<v Speaker 1>into starting the reaction than you were getting out of

0:15:21.640 --> 0:15:24.920
<v Speaker 1>the reaction. But there are other facilities that are similar

0:15:24.960 --> 0:15:28.720
<v Speaker 1>to the JET one that are in various stages of

0:15:28.760 --> 0:15:32.440
<v Speaker 1>construction right now that may give off way more energy

0:15:32.480 --> 0:15:37.440
<v Speaker 1>than it was required to start, like the International Thermonuclear

0:15:37.560 --> 0:15:43.480
<v Speaker 1>Experimental Reactor or EITER, which is in France, but its

0:15:43.480 --> 0:15:46.600
<v Speaker 1>supposed to generate ten times more power that requires to

0:15:46.600 --> 0:15:51.320
<v Speaker 1>to start the fusion process. So if it's you know,

0:15:51.440 --> 0:15:54.240
<v Speaker 1>even even then it's just the beginning, right, ten times

0:15:54.560 --> 0:15:57.800
<v Speaker 1>what you put into it is. It sounds great, but uh,

0:15:58.160 --> 0:16:02.000
<v Speaker 1>but we only hopefully go up from there. Sure, fusion

0:16:02.040 --> 0:16:04.120
<v Speaker 1>is one of those funny things that for years and

0:16:04.200 --> 0:16:06.800
<v Speaker 1>years people have been saying it's right around the corner,

0:16:07.000 --> 0:16:10.200
<v Speaker 1>and it's never We've never gone around that corner. Yet

0:16:10.240 --> 0:16:13.400
<v Speaker 1>it's always it's always twenty to fifty years away. It's

0:16:13.440 --> 0:16:16.320
<v Speaker 1>why all super fancy technology. Yeah, it's one of those

0:16:16.320 --> 0:16:19.400
<v Speaker 1>things where, like like the singularity, it's always twenty to

0:16:19.480 --> 0:16:22.360
<v Speaker 1>fifty years away. But we have made real progress. We have,

0:16:22.680 --> 0:16:26.160
<v Speaker 1>we have we're a lot closer than we used to be,

0:16:26.400 --> 0:16:28.200
<v Speaker 1>and we do need to take just a quick moment

0:16:28.240 --> 0:16:33.280
<v Speaker 1>to talk about cold fusion. Which is cold fusion well,

0:16:33.400 --> 0:16:34.880
<v Speaker 1>we don't even have to say the quote. I mean,

0:16:34.880 --> 0:16:39.280
<v Speaker 1>it's it's an accepted term for something that is unproven scientific.

0:16:39.400 --> 0:16:42.840
<v Speaker 1>Imagine people who people who advocate it don't like that

0:16:42.960 --> 0:16:45.120
<v Speaker 1>term anymore, do they? That they try to like hide

0:16:45.120 --> 0:16:49.600
<v Speaker 1>it under different terminology. Pons and Fleischmann, the paraphysicists who

0:16:50.080 --> 0:16:54.440
<v Speaker 1>became famous for experiments that they thought proved or at

0:16:54.480 --> 0:16:57.360
<v Speaker 1>least indicated that cold fusion is a thing. And by

0:16:57.360 --> 0:16:59.480
<v Speaker 1>the way, cold fusion is this idea that you can

0:16:59.520 --> 0:17:06.960
<v Speaker 1>create fusion reactions among certain light atomic elements at close

0:17:07.000 --> 0:17:10.560
<v Speaker 1>to room temperature, so so so that energy barrier that

0:17:10.640 --> 0:17:13.840
<v Speaker 1>you need to make the reaction start goes away. Well,

0:17:13.880 --> 0:17:15.480
<v Speaker 1>I mean, and if this were true, it would be

0:17:15.480 --> 0:17:17.800
<v Speaker 1>a miracle. It would just I mean, we would have

0:17:17.880 --> 0:17:20.600
<v Speaker 1>limitless energy right now. It would be Doc Browne's mr

0:17:20.640 --> 0:17:22.719
<v Speaker 1>fusion on the back of it. Would Yeah, I mean

0:17:23.400 --> 0:17:26.840
<v Speaker 1>we would. Everyone could have a fusion reactor at home

0:17:27.200 --> 0:17:30.360
<v Speaker 1>that would provide more than enough power to run absolutely everything,

0:17:30.440 --> 0:17:33.680
<v Speaker 1>all the time, every day, and there would never be

0:17:34.000 --> 0:17:36.520
<v Speaker 1>there wouldn't even be a need for an electric grid anymore.

0:17:36.640 --> 0:17:39.000
<v Speaker 1>You can see why people would want it. Yeah, The

0:17:39.359 --> 0:17:41.720
<v Speaker 1>problem is that the science just doesn't seem to work out.

0:17:41.760 --> 0:17:44.800
<v Speaker 1>But Ponds and Fleishman did some, uh some studies that

0:17:45.480 --> 0:17:48.959
<v Speaker 1>initially seemed very promising. A few labs even reported that

0:17:49.000 --> 0:17:52.560
<v Speaker 1>they had replicated the results, but upon further examination, it

0:17:52.680 --> 0:17:55.840
<v Speaker 1>seemed like all the results were brought into question. There

0:17:55.840 --> 0:17:59.480
<v Speaker 1>were questions about measurement techniques, about the equipment that was

0:17:59.520 --> 0:18:02.320
<v Speaker 1>actually being used to take measurements, about the fact that

0:18:02.400 --> 0:18:04.800
<v Speaker 1>some of the results were falling within the margin of error,

0:18:04.840 --> 0:18:06.680
<v Speaker 1>which means that you can't really be sure that you're

0:18:06.760 --> 0:18:09.840
<v Speaker 1>looking at a result. Um. The whole thing that they

0:18:09.840 --> 0:18:12.200
<v Speaker 1>were saying was that they were getting more energy out

0:18:12.240 --> 0:18:15.520
<v Speaker 1>of a reaction than they expected. Like it was it

0:18:15.560 --> 0:18:19.320
<v Speaker 1>was beyond what the what science would tell you would

0:18:19.320 --> 0:18:23.040
<v Speaker 1>happen based upon what was going on. But it hasn't

0:18:23.119 --> 0:18:26.000
<v Speaker 1>borne any fruit, despite the fact that both Ponds and

0:18:26.040 --> 0:18:30.080
<v Speaker 1>Fleischmann for many years continued to uh to to really

0:18:30.119 --> 0:18:33.400
<v Speaker 1>work in this They they originally called it infusion. That's

0:18:33.400 --> 0:18:35.720
<v Speaker 1>not a joke, that really is true. Uh, they call

0:18:35.760 --> 0:18:40.240
<v Speaker 1>it infusion. It was t that not like the letter

0:18:40.320 --> 0:18:43.000
<v Speaker 1>in an infusion, which is weird. Which is weird because

0:18:43.040 --> 0:18:45.440
<v Speaker 1>if you know anything about if you if you know

0:18:45.480 --> 0:18:49.760
<v Speaker 1>anything about in rays, in rays were something that, uh

0:18:50.119 --> 0:18:53.320
<v Speaker 1>that some scientists believed were a thing until they tried

0:18:53.359 --> 0:18:55.719
<v Speaker 1>to look into it and realized there was nothing there

0:18:55.760 --> 0:18:58.399
<v Speaker 1>like in rays where these things that existed until you

0:18:58.440 --> 0:19:00.960
<v Speaker 1>looked for them, and then they didn't. So it seems

0:19:01.000 --> 0:19:02.359
<v Speaker 1>to me, it seems funny to me that you would

0:19:02.359 --> 0:19:05.399
<v Speaker 1>call it in fusion within rays being such a big

0:19:05.400 --> 0:19:09.240
<v Speaker 1>scandal in the scientific community. But anyway, uh, cold fusion. Yeah,

0:19:09.320 --> 0:19:12.760
<v Speaker 1>it just didn't seem to have any merit to it.

0:19:12.800 --> 0:19:14.280
<v Speaker 1>And there have been a lot of people who looked

0:19:14.280 --> 0:19:16.600
<v Speaker 1>into it since then. There are plenty of people out

0:19:16.640 --> 0:19:20.720
<v Speaker 1>there on the Internet who really hope that it turns

0:19:20.720 --> 0:19:22.760
<v Speaker 1>out that cold fusion really does have something to it

0:19:22.760 --> 0:19:25.560
<v Speaker 1>and it makes sense, right, Like that would solve everyone's

0:19:25.600 --> 0:19:31.040
<v Speaker 1>problems for energy. Yeah, Sadly, from my own personal perspective,

0:19:31.080 --> 0:19:33.480
<v Speaker 1>I think you might as well wish for fairies and

0:19:33.480 --> 0:19:38.399
<v Speaker 1>clap your hands based upon the scientific evidence that we

0:19:38.480 --> 0:19:40.400
<v Speaker 1>have in front of us. Now, that's not to say

0:19:40.440 --> 0:19:43.040
<v Speaker 1>that someone won't find some way of making it work

0:19:43.080 --> 0:19:46.200
<v Speaker 1>in the future. Maybe they will, but based upon what

0:19:46.240 --> 0:19:51.720
<v Speaker 1>we know right now, it seems unlikely, like, well, incredibly unlikely.

0:19:52.760 --> 0:19:54.920
<v Speaker 1>But this doesn't mean now Here's one of the main

0:19:54.960 --> 0:19:58.560
<v Speaker 1>reasons I think we needed to bring this up is that, um,

0:19:58.680 --> 0:20:02.160
<v Speaker 1>people hear about the fail years of cold fusion, and

0:20:02.440 --> 0:20:05.040
<v Speaker 1>they that makes them think, oh, fusion, it's a fusion.

0:20:06.800 --> 0:20:12.440
<v Speaker 1>Hot fusion has serious potential, right Yeah, No, hot fusion

0:20:12.520 --> 0:20:15.400
<v Speaker 1>is definitely one of those things that could work if

0:20:15.400 --> 0:20:18.160
<v Speaker 1>we get the system efficient enough. Like if I turn,

0:20:18.880 --> 0:20:22.680
<v Speaker 1>if the International Thermonuclear Experimental Reactor does in fact work out,

0:20:23.200 --> 0:20:26.000
<v Speaker 1>then that will show that fusion is a viable means

0:20:26.080 --> 0:20:29.840
<v Speaker 1>of generating energy. And that, and we know it's legitimate,

0:20:29.920 --> 0:20:33.480
<v Speaker 1>the son's there, but but whether or not we can

0:20:33.520 --> 0:20:35.960
<v Speaker 1>harness it in a way that makes sense is still

0:20:35.960 --> 0:20:40.800
<v Speaker 1>the question. Uh. It does look promising, but even even

0:20:40.840 --> 0:20:44.160
<v Speaker 1>the optimists are still saying it's, you know, thirty forty

0:20:44.240 --> 0:20:48.720
<v Speaker 1>years away, So, uh, what is it here? Lockheed skunk

0:20:48.800 --> 0:20:50.840
<v Speaker 1>Work says that they can make fusion work in the

0:20:50.880 --> 0:20:54.520
<v Speaker 1>next few years. Well yeah, but then it'll only work

0:20:54.560 --> 0:20:59.640
<v Speaker 1>in area fifty one anyway, So it's a really interesting

0:20:59.720 --> 0:21:01.560
<v Speaker 1>con sept. I really hope it does work out. It

0:21:01.600 --> 0:21:05.840
<v Speaker 1>would be a huge benefit and the idea of you know,

0:21:06.000 --> 0:21:08.119
<v Speaker 1>think about it, if you're if you're using this this

0:21:08.200 --> 0:21:11.080
<v Speaker 1>method to create energy, then you suddenly that the whole

0:21:11.520 --> 0:21:14.360
<v Speaker 1>question about how do we create clean energy is answered

0:21:14.440 --> 0:21:16.760
<v Speaker 1>and we don't have to you know, things like wind

0:21:16.840 --> 0:21:21.080
<v Speaker 1>turbines and solar farms, which are you know, problematic right now,

0:21:21.480 --> 0:21:25.240
<v Speaker 1>inefficient Relatively they're relatively inefficient. You have to find very

0:21:25.240 --> 0:21:28.800
<v Speaker 1>specific places to be able to harness that kind of stuff.

0:21:29.359 --> 0:21:31.520
<v Speaker 1>And uh, you know, there's a question of whether or

0:21:31.520 --> 0:21:34.200
<v Speaker 1>not the amount we could harvest would meet our demand.

0:21:34.640 --> 0:21:37.000
<v Speaker 1>This would answer all those questions. Me we would easily

0:21:37.040 --> 0:21:40.560
<v Speaker 1>meet our demand. For at least the foreseeable future. You know,

0:21:40.640 --> 0:21:42.880
<v Speaker 1>never say never. Eventually we could get to a point

0:21:42.960 --> 0:21:45.600
<v Speaker 1>where even fusion might seem like, well, we need the

0:21:45.640 --> 0:21:47.840
<v Speaker 1>next big thing. But at that point we'd probably be

0:21:47.880 --> 0:21:50.800
<v Speaker 1>off planet Earth and yeah, we just be harnessing the

0:21:50.840 --> 0:21:53.840
<v Speaker 1>stars themselves, which we are going to talk about at

0:21:53.840 --> 0:21:56.440
<v Speaker 1>some point, yeah we will, but not today. Today, we're

0:21:56.440 --> 0:21:58.800
<v Speaker 1>going to wrap this up. So guys, if you have

0:21:58.960 --> 0:22:01.959
<v Speaker 1>enjoyed this, if you have of suggestions for future topics,

0:22:01.960 --> 0:22:04.119
<v Speaker 1>if you want to chime in on the discussion about fusion,

0:22:04.160 --> 0:22:06.160
<v Speaker 1>and if you want to say that I'm a denier

0:22:06.280 --> 0:22:08.480
<v Speaker 1>because I don't think cold fusion is gonna work, you

0:22:08.520 --> 0:22:11.000
<v Speaker 1>can let us know. We have our website at f

0:22:11.280 --> 0:22:14.480
<v Speaker 1>w thinking dot com. You can read our blogs, you

0:22:14.520 --> 0:22:16.840
<v Speaker 1>can watch the videos, you can listen to the podcasts,

0:22:16.960 --> 0:22:18.959
<v Speaker 1>and of course there are the links to all of

0:22:18.960 --> 0:22:22.720
<v Speaker 1>our presences on various social networks, so you can find

0:22:22.800 --> 0:22:25.760
<v Speaker 1>us on Facebook, Twitter, and Google Plus. We look forward

0:22:25.760 --> 0:22:27.359
<v Speaker 1>to hearing from you, and we will taught to you

0:22:27.400 --> 0:22:33.199
<v Speaker 1>again really soon. For more on this topic and the

0:22:33.240 --> 0:22:47.679
<v Speaker 1>future of technology, visit forward thinking dot com, brought to

0:22:47.680 --> 0:22:50.080
<v Speaker 1>you by Toyota. Let's go places