Stuff You Should Know - SYSK Selects: Can Nuclear Fusion Reactors Save The World?

Episode Date: March 28, 2020

The world’s energy consumption is ruining the planet but for decades physicists have been working on what could solve the world’s energy and climate change woes for centuries to come – nuclear f...usion. Learn about building stars on Earth in this classic episode. Learn more about your ad-choices at https://www.iheartpodcastnetwork.comSee omnystudio.com/listener for privacy information.

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Starting point is 00:00:00 On the podcast, Hey Dude, the 90s called, David Lasher and Christine Taylor, stars of the cult classic show, Hey Dude, bring you back to the days of slip dresses and choker necklaces. We're gonna use Hey Dude as our jumping off point, but we are going to unpack and dive back into the decade of the 90s.
Starting point is 00:00:17 We lived it, and now we're calling on all of our friends to come back and relive it. Listen to Hey Dude, the 90s called on the iHeart radio app, Apple Podcasts, or wherever you get your podcasts. Hey, I'm Lance Bass, host of the new iHeart podcast, Frosted Tips with Lance Bass. Do you ever think to yourself, what advice would Lance Bass
Starting point is 00:00:37 and my favorite boy bands give me in this situation? If you do, you've come to the right place because I'm here to help. And a different hot, sexy teen crush boy bander each week to guide you through life. Tell everybody, ya everybody, about my new podcast and make sure to listen so we'll never, ever have to say. Bye, bye, bye.
Starting point is 00:00:57 Listen to Frosted Tips with Lance Bass on the iHeart radio app, Apple Podcasts, or wherever you listen to podcasts. Hey everyone, it's me, Josh, and for this week's SYSK Selects, I've chosen, can nuclear fusion reactors save the world? Well, it turns out, probably, if we can just figure out how to build one properly.
Starting point is 00:01:18 Well, sit back, buckle up, and prepare to be titillated with what I find to be the most arousing, amazing form of future energy around. Enjoy. Welcome to Stuff You Should Know, a production of iHeartRadio's How Stuff Works. Hey, welcome to the podcast. I'm Josh Clark.
Starting point is 00:01:48 There's Charles W. Chuck Bryant. There's Jerry, who's barrel laughs. And this is Stuff You Should Know. She gave us the old quick start. Yeah. Like, I don't want to hear any more impressive record. Yeah, she knows that shuts me up, or at least cuts off whatever conversation
Starting point is 00:02:04 I'm chiding her to. It was great. I'm telling you, if we could release the 20 seconds before each show, as its own show. Yeah. That would be terrible. No one would care. No.
Starting point is 00:02:14 We'd think it was funny. Everybody else would be like, you edit this out for a reason. Yep. So, Chuck, how you doing? Great. Have you ever been to Asan, Provence, France? No.
Starting point is 00:02:28 Is that a place? Yeah. No, I haven't. It is a rustic little town in Provence, and it is strangely, maybe even ironically, in the non-hipster use, but in the actual, yeah, it's a real word. Definition of the word.
Starting point is 00:02:46 Also, site to one of the most futuristic engineering projects humanity's ever undertaken. Meat, or meat, it's the sound it makes. Oh, I thought you're mocking me. No, no, no. For being thrilled by the thought of this thing. No, it is kind of funny that this thing's in a sleepy little town.
Starting point is 00:03:03 Yeah. It's like a hamlet, maybe even. CERN in Switzerland, that's not in the city, is it? No. You can't build these things in cities. That's why they're in sleepy towns. Exactly. Because no one knows they're being poisoned.
Starting point is 00:03:12 Yeah, and you can push the mayor around pretty easy. Exactly. This thing is called ITER, I-T-E-R, which is an acronym for the International Thermonuclear Experimental Reactor. That's right. Which really gets the point across. Did you know the word acronym is an acronym?
Starting point is 00:03:31 That's not true. Okay. I just wanted to see how long you would try and sort it out in your head. I would have kept going another 30 seconds, maybe. That would have been a great joke. Okay, I just kept it going like, I'm not gonna tell you. I would have been, I would have,
Starting point is 00:03:44 maybe 15 seconds, you would have gotten that much more. Sure. So, I wouldn't have looked it up. I would have figured it out myself. Anyway, ITER is this colossal engineering project. Somebody compared it to the pyramids at Giza. Oh, wow. Yeah, that's exciting stuff.
Starting point is 00:04:03 Sure. The thing is, it's a nuclear fusion reactor, and it's the culmination of decades of attempts to create a nuclear fusion reactor. Yes. It's going to run down, and we'll talk about the difference in a minute. Yeah.
Starting point is 00:04:20 But fusion has been very elusive, and nowhere is it more apparent than in the ITER project. Yeah. Because this thing is going to cost it approximately $50 billion when it's completed. $50 billion. They started in 1993. They're hoping to turn on the switch in 2020,
Starting point is 00:04:42 but it's looking like 2023 or 2024, and it won't be starting to produce anything until the 2040s at the earliest. So, what's the point? I'll tell you the point. Yeah. If we can figure out nuclear fusion, Chuck, the worlds, literally the world's energy problems
Starting point is 00:05:03 will be solved for millennia. Yeah. If we can just figure this out, we will have a almost no radio activity nuclear option. Yeah. Almost limitless fuel supply. Yeah. Totally green, clean.
Starting point is 00:05:21 No pollution, no greenhouse emissions. Right, and with plenty of energy to spare. Yeah. Using the already extant infrastructure we have to supply power. Like, you don't have to completely rebuild everything. You can just, to the electrical cables outside, it'll be the exact same thing.
Starting point is 00:05:40 Yeah, you can just go to a nuclear fusion reactor and press the button that says fusion, and it'll all of a sudden join atoms instead of split them. Exactly. It's that easy. That's what the difference is. With fission, you're splitting atoms and you're gaining energy from that.
Starting point is 00:05:52 With fusion, you're smacking them in together and you're gaining even more energy because you're exploiting a different fundamental force. Yeah, and that, I was being coy. Clearly there is no button because we would have pushed it a long time ago. Yeah. And when I say no pollution
Starting point is 00:06:08 and no greenhouse emissions before the pedantic among you right in, we know that just even shipping something from here to there causes pollution and greenhouse emissions. Good, good, good. But we're talking about that the output of the reactor itself is very green.
Starting point is 00:06:23 So if you want to know all about ITER, well, we're gonna talk about it here or there because it's just, you just can't talk about nuclear fusion reactors and not mention ITER. But if you wanna know a lot about ITER, there is a really great article called A Star in a Bottle. And it's by a person named Rafi Kachadurian, Kachadurian, and it was written in the New Yorker
Starting point is 00:06:43 not too long ago. And man, it is every detail you wanna know about the ITER project written really well. And it's long, but it's totally worth the read. Yeah, it's all over the news lately. And for good reason, you said a lot of energy. I have a stat, gonna throw back to the old days here. Per kilogram of fuel, if we're talking fusion and fission.
Starting point is 00:07:06 Lay it on me. Fusion produces four times more energy than fission. I saw seven. It's probably one of the things where it's like four to five to 10 or something. I found four times and 10 million times more than coal. Yeah. 10 million times the energy as coal.
Starting point is 00:07:25 And that's with equal fuel per kilogram of fuel. Right. It's just, I mean, it is the future. Yeah, and you can say, well, that's great because we want 18 million times the amount of power that coal provides. You can say, well, there buddy, you can also bring it backwards
Starting point is 00:07:39 because you can supply an awful lot of power then with a lot less fuel. Yeah. Like the advantage of nuclear fusion are mind boggling. Sure. And very few downsides, which we'll get to, of course. Yeah. I mean, like really genuinely,
Starting point is 00:07:56 it's not just like some, like here's all the great stuff about it and just don't pay attention to all these like really horrible aspects. Yes. Like there really aren't too many downsides. The downside is we are at this moment incapable of successfully creating a commercially viable nuclear fusion reactor.
Starting point is 00:08:16 That's right. But we've got an understanding of what the challenges are ahead of us thanks to the last 50 or so years of really, really, really smart physicists working on the problem of nuclear fusion. And the great inspiration for nuclear fusion is the sun. The sun and all stars like it
Starting point is 00:08:37 are enormous, immense nuclear fusion reactors. So if you are building a nuclear fusion reactor here on Earth, you're essentially creating a star. And that is a very difficult thing to do, it turns out. Yeah, the sun creates, I know we talked about the sun in our very famous episode on the sun. The sun creates 620 million metric tons.
Starting point is 00:09:03 It fuses 620 million metric tons of hydrogen at its core every second. So every second at the sun's core, it produces enough power to light up New York City for 100 years. New York City? Every second. And that's the sun.
Starting point is 00:09:18 And all we wanna do is do the same thing on a much smaller scale. That's all? I think the guy, there's this kid who built one in his garage and he said he wanted to, I saw this Ted talk, he wanted to create a star in a box is what he called it. Yeah, I've seen it like this New Yorker
Starting point is 00:09:35 called it a star in a bottle. Yeah, this kid's name is Taylor Wilson and he's a nuclear physicist and he's like 16. Wow. He's like Stygie Hauser. Yeah, he created a successful one and the key though is not to be able to create the fusion. The key is to be able to harness enough plasma
Starting point is 00:09:55 which we'll get to at a high enough temperature and density for there to be a net power gain. You can create fusion but in order to get out more than you're putting in is the only thing that matters because what you wanna do is create electricity. Exactly, there's two huge challenges right now to nuclear fusion. We pretty much understand it enough to start it going
Starting point is 00:10:16 and get energy from it. The problem is material science isn't at a point where it can build a containment vessel to really house a thermonuclear reactor. Yeah. And then the other big obstacle is like you said, net energy gain. Like if you're putting in as much or more energy
Starting point is 00:10:37 then you're getting out of your nuclear reactor then you're wasting energy and it's the opposite of what you're supposed to be doing. Yeah, they're not just trying to impress people with their science knowledge. No, but up to the- They're trying to create energy. Up to now though, Chuck, every single thermonuclear reactor
Starting point is 00:10:53 that's ever been built has just been impressing people with knowledge. Like they haven't gotten any net energy out of a single thermonuclear fusion reactor. Oh, see I have that they have, right now they're up to like 10, presently they're at 10 megawatts. Oh, is that right?
Starting point is 00:11:12 Yeah. And that's more than they put into it. A net gain of 10 megawatts currently. Everything I saw was when we turn this thing on it should have a net gain. But I didn't see that they've actually done it. Yeah, 10 megawatts now and Iter is gonna produce 500 megawatts
Starting point is 00:11:29 once it's fully operational. Right, so the next challenge then is this. If we're already getting a net energy gain out of it then that means that the net energy gain is it's not sustainable. Like you said, you wanna keep the thing going so you don't have to keep starting from scratch to power it up.
Starting point is 00:11:49 You want it to basically be self-sustaining so you just have to add a little more fuel to it. That's the dream. So let's talk about the history of fusion reactors, Chuck. Yeah, it kind of goes back to this guy named Lyman Spitzer. He's a 36 year old Princeton astrophysicist and this was in the 1950s.
Starting point is 00:12:09 And he was recruited to work on the H-bomb and went out and got a copy of a paper that was released from Germany, I think, right? That had done previous experiments. No, in Argentina. Oh, Argentina? Yeah, they announced that they had successfully built a fusion reactor.
Starting point is 00:12:29 Right, so he gets this paper, goes on a ski trip, starts thinking about how he can do this, takes a little break from his job building the H-bomb and figures out, you know, I think it's possible if we can harness this plasma, I guess we should just go ahead and define what plasma is since we keep saying it. Well, there's the normal three energy states
Starting point is 00:12:52 that we're familiar with, water, solid, and gas, liquid, solid, and gas, right? Right. There's a fourth one, it's plasma. And plasma is basically like an energetic gas where the temperatures are so high that whatever atoms you put into it, the electrons are stripped off
Starting point is 00:13:09 and allowed to move around freely. Right. Basically, the surface of the sun is plasma. That's what plasma is, it's a gas, it's a roiling gas, it's really hard to control and is really unpredictable. Which is when you see the sun like that rippling, wavy looking thing, that's plasma. Right, and the reason the sun manages to stay together
Starting point is 00:13:27 is because it is enormously massive and has a ton of gravity at its core. Yeah, we don't have that advantage here on Earth. We don't, so we try to make up for that by increasing the temperature. That's right. And he was onto it way back then in the 1950s. If we can just harness this, if we can just get hot enough,
Starting point is 00:13:45 and he created a tabletop device called the Stellarator, and it was in a figure eight position. It was a pipe in a figure eight. Yeah. And this would keep things from banging into walls theoretically. Yeah. And he was onto something because,
Starting point is 00:14:01 well, we'll get to Lockheed later, but they're using a similar device now, a figure eight. Oh yeah? Yeah. I didn't realize that was a figure eight. It is, which is weird because what they eventually found out was that a donut shape was really the key to get that net gain.
Starting point is 00:14:16 So the reason that they found out that a donut shape worked was because in the, I think the late 50s, the US had run up against the wall. They're saying like, okay, we've got this, but we can't control the plasma. Because think about it, what you're trying to do is create a star inside something, but it can't touch any of the vessel that it's in,
Starting point is 00:14:40 or else it'll just completely erupt it, right? Yeah, they compared it to holding jelly in rubber bands. Right, it was just like you can't, they couldn't figure out how to control the plasma. So when the US ran up against this wall, they said, hey, rest of the world, we're gonna declassify what Lyman Spitzer has been doing. Help us out.
Starting point is 00:15:01 And like we'll share, if you guys share, and it turns out that the Russians had already come up against this problem and licked it, they figured out that if you put the thing in what's called a toroidal shape, a donut shape, using electromagnets, you contain the plasma essentially. And the donut shape itself was pretty ingenious, but the real stroke of genius was by running
Starting point is 00:15:28 electromagnets in rings around the donut. So it's like you have a donut and you put a bunch of earrings around it, right? And those are electromagnets, so you're creating an electromagnetic force field, which contains the plasma, but then you also put an electromagnetic force field in the middle of the plasma.
Starting point is 00:15:48 So not only does it heat it up to the temperatures you want, it also stabilizes it further. So the Russians had invented what they call the Taka Mac, which is this donut shape, nuclear fusion reactor that basically became the standard for the next 50 years or so. Yeah, you basically could achieve a really dense, super hot plasma.
Starting point is 00:16:11 And we'll get into temperatures and stuff in a bit, but since we can't create that kind of pressure that they have in the sun due to their gravity, their gravity, the sun's gravity. You know, the sun and all those people. Like you said, we had to make up for it here on Earth with temperatures. Right, because apparently if you are in the middle
Starting point is 00:16:30 of a nuclear reactor, a nuclear fusion reactor, you're going to find that the temperatures inside are about six times hotter than the core of the sun, not even the surface of the sun, the core of the sun. And the reason why it has to be so much hotter is because like you said, we can't replicate that density. We can get to those temperatures that we need, but we can't get to that density,
Starting point is 00:16:52 so we have to make up for it. On the podcast, HeyDude, the 90s, called David Lasher and Christine Taylor, stars of the cult classic show, Hey Dude, bring you back to the days of slipdresses and choker necklaces. We're going to use Hey Dude as our jumping off point, but we are going to unpack and dive back into the decade of the 90s.
Starting point is 00:17:18 We lived it, and now we're calling on all of our friends to come back and relive it. It's a podcast packed with interviews, co-stars, friends, and nonstop references to the best decade ever. Do you remember going to Blockbuster? Do you remember Nintendo 64? Do you remember getting Frosted Tips? Was that a cereal?
Starting point is 00:17:36 No, it was hair. Do you remember AOL Instant Messenger and the dial-up sound like poltergeist? So leave a code on your best friend's beeper because you'll want to be there when the nostalgia starts flowing. Each episode will rival the feeling of taking out the cartridge from your Game Boy,
Starting point is 00:17:50 blowing on it and popping it back in as we take you back to the 90s. Listen to, Hey Dude, the 90s called on the iHeart radio app, Apple Podcasts, or wherever you get your podcasts. Hey, I'm Lance Bass, host of the new iHeart podcast, Frosted Tips with Lance Bass. The hardest thing can be knowing who to turn to
Starting point is 00:18:08 when questions arise or times get tough or you're at the end of the road. Ah, okay, I see what you're doing. Do you ever think to yourself, what advice would Lance Bass and my favorite boy bands give me in this situation? If you do, you've come to the right place because I'm here to help.
Starting point is 00:18:22 This, I promise you. Oh God. Seriously, I swear. And you won't have to send an SOS because I'll be there for you. Oh man. And so my husband, Michael. Um, hey, that's me.
Starting point is 00:18:33 Yeah, we know that, Michael. And a different hot, sexy teen crush boy bander each week to guide you through life, step by step. Oh, not another one. Kids, relationships, life in general can get messy. You may be thinking, this is the story of my life. Just stop now. If so, tell everybody, yeah, everybody
Starting point is 00:18:51 about my new podcast and make sure to listen. So we'll never, ever have to say bye, bye, bye. Listen to Frosted Tips with Lance Bass on the iHeart Radio app, Apple podcast, or wherever you listen to podcasts. So Chuck, we're talking about nuclear fusion. And there's, it's actually surprisingly understandable at its most basic core.
Starting point is 00:19:26 Yeah, you're fusing atoms. It's not the hardest thing in the world to wrap your head around. Yeah, so with fission, we're splitting atoms. You're taking an atom and you're splitting its nuclei apart. You're splitting the neutrons and the protons apart from one another. And when you do that, one of the four fundamental forces,
Starting point is 00:19:42 electromagnetic force, pushes them away. And you get this burst of energy. With fusion, you're taking nuclei from different atoms. You're taking protons and neutrons. And you're smashing them together. And when you do that, you're unleashing what's called the strong force, which appropriately enough is stronger than electromagnetic force, which
Starting point is 00:20:05 is why nuclear fusion yields more energy than nuclear fission. Yeah, Einstein himself said, each time you smash these things together, you're going to lose a little bit of mass. And that little bit of mass is a ton of energy, as it turns out. That's right, the famous E equals mc squared. Yeah, and I don't think he realized in 1905,
Starting point is 00:20:24 or maybe Einstein did. Einstein probably did. Yeah, Einstein probably did. I would guess he did. So the problem is, even though it is very easy to smash some protons together, there is a tremendous amount of resistance to that smashing together. They don't want to smash together.
Starting point is 00:20:39 No, because it's just like if you take a magnet, two magnets, and you put the positive poles toward one another, they repel one another, right? Same thing. That's the same principle on an atomic level, too. If you take protons, which are positively charged particles, and try to put them together, they repel one another. And the closer you get them together,
Starting point is 00:21:01 the stronger the repellent force is, the electromagnetic force, right? But if you can get them close enough, the electromagnetic force is overcome by that strong force, the strong nuclear force, and they become bound together. Because the strong force is that one of those four fundamental forces of the universe,
Starting point is 00:21:21 and that is the force that keeps atoms together. And that force is stronger than the force that repels like-charged particles. Yeah, and when you talk about close, they need to be within one times 10 to the negative 15 meters of one another. Right, so that is... In order to fuse. If you'll indulge me.
Starting point is 00:21:41 Sure, are you going to read a bunch of zeros? Yeah. It's.0000000001 meters apart. Right. That's how close they have to be. That's right. To get them to accept one another and to fuse. Right.
Starting point is 00:21:59 I think I have a theory that if they're not fusing because they think they're going to be made into a bomb, and if we told them that we were creating energy, they might be more willing to fuse together. Yeah, because protons are peaceniks. Everybody knows that. Sure. So when they do fuse together, right,
Starting point is 00:22:16 when you do cross that threshold and the strong force takes over and overcomes the electromagnetic force, like we said, a tremendous amount of energy is released. And it's released, in part, in the form of neutrinos, neutrons, right, which are neutral particles, which suddenly start carrying a tremendous amount of kinetic energy. So let's say you have one atom, you got another atom,
Starting point is 00:22:42 and they're both like, I'm not getting close to you. We're not going to get to... Okay, we got together. Yes. That force, that mass that's displaced, is transferred through the neutron that gets kicked off of the atom, right? Yeah.
Starting point is 00:22:56 And is carried out. Now, a neutron doesn't have any kind of positive or negative charge. It's neutral. It's a neutron. Which means that it can pass through the very electromagnetic fields that are keeping this plasma
Starting point is 00:23:10 where this reaction is taking place together. Once that happens, Chuck, it can go out to what's called a blanket wall and a thermonuclear reactor, warm it, and then that heat is transferred into a water cooling system. The water's warmed up, turns steam, which I guess moves the turbine,
Starting point is 00:23:32 and then all of a sudden, the turbine's producing electricity. Yeah, it's funny how it gets so complex, but all you're still trying to do is create steam to move it, turn a turbine. It's like hooking the ISS up to a horse. Right. You know?
Starting point is 00:23:45 Move it over there. So there are a few types of fusion reactions. The ultimate goal, right now what we can do on a small scale is what's called a deuterium tritium reaction. That's the one that we can currently achieve. That's one atom of deuterium and one atom of tritium,
Starting point is 00:24:06 combining to form a helium-4 atom and a neutron. The ultimate goal, I mean, that's good, and that'll create a lot of energy, but there are a few downsides. Tritium is radioactive for one. Do you have to mine it from lithium? Yeah. And lithium's fairly rare.
Starting point is 00:24:21 Sure. The ultimate goal is to reach deuterium-deuterium reactions, which is two deuterium atoms combining to form that helium-3 and a neutron, and you can get that from the seawater. It's abundant, almost limitless, and I couldn't find this, but I think clean water can be a residual effect of this.
Starting point is 00:24:42 Am I wrong? I don't know if it's, well, you're probably not injecting water, but to get the deuterium, I mean desalination plants are the key to the future as far as supplying the world with fresh water. Yeah, I thought I saw somewhere where it was an actual byproduct,
Starting point is 00:24:58 but yeah, but then I couldn't find it, so I'm not sure if that's right or not. You know what? You just jogged my memory. I feel like in a hydrogen-powered car, water is one of the byproducts. So maybe so. Yeah.
Starting point is 00:25:10 All right, don't quote me on that, though. At the very least, it's a great way to create energy. Right, and what you also can get tritium from helium, I believe. So even now with the deuterium tritium reactions that we're working on, there's already a workaround, you know? Like you can create a thermonuclear reactor
Starting point is 00:25:33 that's a breeding reactor to where the byproduct helium can be used to harvest more of the fuel you're using, tritium. Yeah, and aren't we running low on helium? We are, which is like, remember when we were talking about the dirgeable, the zeppelin, which one was it? Blooms, how blimps work.
Starting point is 00:25:50 Yeah, and then a long time ago, we did one on the Mars turbine. Yeah, Mars turbine. Yeah, but yes, there's very clearly a helium shortage, and the idea that we're just using it for party balloons rather than this is scary. Yeah, and don't be confused. We say things like deuterium,
Starting point is 00:26:09 and it sounds super complex. All that is hydrogen with an extra neutron. Yeah, it's an isotope. Yeah. So there's three isotopes of hydrogen, and they're all still the same element. They're all still hydrogen, but they have different configurations
Starting point is 00:26:22 as far as their neutrons go. So, proteome is a hydrogen isotope with one proton and no neutrons. Deuterium is a hydrogen isotope with one proton and one neutron, and tritium is a hydrogen isotope with one proton and two neutrons. And like you said, tritium is radioactive,
Starting point is 00:26:40 but the beauty of it is you need very, very, very little of it to fuel a nuclear fusion reactor, and it becomes a stable helium, a non-radioactive helium in the reactor. So you don't have this leftover radioactive fuel. Isn't that awesome? I think they said there's an, it would be equivalent of the radiation
Starting point is 00:27:01 we just see every day and walking around on the street, right? Yes, the background radiation, I believe. I saw that too. The thing is, is the parts to the nuclear reactor themselves will become irradiated over time. Apparently though, compared to the kind of radioactivity that's generated from nuclear fission,
Starting point is 00:27:22 this stuff you could just disassemble and bury in the desert for a hundred years, go back and dig back up, and it'll be totally inactivated. So it's, the stuff that is radioactive is extraordinarily manageable. Yeah, it is, and like I said, we don't wanna make it sound like this is perfect.
Starting point is 00:27:39 There is, they do predict the short to medium term radioactive waste problem, and they say that's due to activation of the structural materials. Right, the actual thermonuclear device itself. Yeah, and while you don't need much tritium, even a few grams of tritium is problematic, but hopefully, you know, there's no accident.
Starting point is 00:28:02 Although they say accidents with these, if you just turn the power off, it stops everything. It's not like a chain reaction can occur, like a fission reactor, or it's out of your control. There's not a meltdown, which also, if you wanna know more about that, go listen to our How Nuclear Meltdowns Work episode.
Starting point is 00:28:20 That was pretty good. We released it right after Fukushima, but it applies to all fission reactors. That's right. So the goal is ultimately deuterium-deuterium reactions, where you're pairing those together. That sounds clean. It does. And the reason why is, again, it's abundant fuel.
Starting point is 00:28:36 You can get it from desalinating seawater, and then secondly, it's not radioactive at any point. So it wouldn't make the thermonuclear reactor itself radioactive, too. That's right. The reason why we're not doing that already is because we can't achieve the temperatures necessary. That's right, which leads us to the two big stumbling blocks.
Starting point is 00:28:57 Everyone knows this is a great idea. There's no one out there saying, oh, I don't know about this fusion thing. Creating a star in a box sounds kind of weird. The problem is the barriers that we have here on planet Earth, which is one, temperature, and two, pressure. We have achieved the temperature, which is, the requirement is 100 million Kelvin.
Starting point is 00:29:20 Like you said, that's about six times hotter than the sun's core, which is pretty intense. And the other is pressure. Like we said, we need to get them within, I'm not gonna make you read all those zeros again, but smash them that close in order to fuse. And since we don't have that kind of mass and gravity that the sun does, there are a few pretty genius ways
Starting point is 00:29:42 that we're working around that. Yeah, there's basically two as it stands. And then the Lockheed Martin one, which a lot of people are skeptical about, we should say, is kind of a variation on one theme. But there's basically, there's two ways that we figured out to create nuclear fusion reactors so far.
Starting point is 00:30:01 One is using magnetic confinement. And the other is using inertial confinement. So magnetic confinement uses that Takamak technology. Yeah, it's sort of like CERN, it's using magnets to create pressure. I guess in CERN's case, we're using it to create speed. But in this case, it's to create pressure. Right, so what you're doing is,
Starting point is 00:30:24 you have this donut-shaped chamber, and that's your reaction chamber. And then again, rings around the donut that go around the inside and outside of the donut. I know I'm kind of imagining wonderful donuts too. We're going Homer Simpson here. They create electromagnetic fields. Now remember, this plasma is hydrogen gas
Starting point is 00:30:45 that's been heated up to a temperature so hot that the electrons just float off and move around freely. And because of this higher temperature, these particles have become really, really energized. So they're moving and bouncing all over the place and the pressure's building up. But because electrons are negatively charged and because protons are positively charged,
Starting point is 00:31:06 if you use alternating electromagnetic fields, you can contain this plasma. So that this incredibly hot gas that's six times hotter than the core of the sun can be contained within the electromagnetic fields. That's right. And we talked about power in, power out. You'd need about 70 megawatts of power
Starting point is 00:31:26 to create this, to start this fusion reaction, but you're going to yield about 500 megawatts. That's the EIDER project, I believe. Yeah, that's the EIDER. And that's only a 300 to 500 second reaction. But like we said earlier, the eventual goal is that it's sustaining itself. Right.
Starting point is 00:31:45 Which is just a beautiful concept. Yeah. So basically what they do is they have the gas is injected into the chamber, the hydrogen gas. And then there's the electromagnetic fields that are holding the plasma in place. But then remember, we said the Russians figured out that if you put an electromagnetic field
Starting point is 00:32:03 in the middle of the whole thing, it will stabilize that plasma, but it also heats it up. So it serves this double purpose. And then just to add a little extra temperature, they shoot it with microwaves and some other stuff, and then heat it up. And then as the plasma goes crazy and all the fusion energy is released, the neutrons move their way outside
Starting point is 00:32:23 of the electromagnetic field into the blanket, which they heat up. And the heat energy is transferred to power that turbine or move the horse down the lane. And it's just creating steam. Yeah, I mean, that's what EIDER is doing right now. That's what they're trying to prove. And then also, as EIDER is spending billions and billions
Starting point is 00:32:43 and billions of dollars and running into tons of delays, it's an amazing project. Lockheed Martin basically just came out and said, oh, by the way, this thing that you're trying to do that's going to be 100 feet tall and require staggering amounts of energy and money, we're doing one that puts out the same amount of energy as yours, but it's a 10th of the size, which
Starting point is 00:33:07 means it's almost out of the gate commercially viable. Yeah, that is their Skunk Works division of Lockheed. And they announced this like three days ago here in mid-October, and they've gotten a lot of blowback from the scientific community. Because they wouldn't release data. They don't have data. They said it's a high beta device right now
Starting point is 00:33:28 and kind of shut out the scientific community as far as questions go. And every scientist that I saw interviewed for this said, they're trying to get some attention to get some partners to join in. Well, yeah, plus it makes you want to run out and buy Lockheed Martin stock, because if one company can figure out how to create a thermonuclear fusion reactor here on Earth
Starting point is 00:33:51 that's scalable. That fits in a truck. Yeah, that person would be very wealthy. Yeah, so it's a dubious claim, but they're working toward a good thing. I'm not like poo-pooing the whole thing. But until they have hard data and some proof, then I think the scientific community's
Starting point is 00:34:07 got their arms folded right now. Yeah, and they have released some details. It's just not detailed enough for a scientist. It's detailed enough for Aviation Week. I bought it. Yeah. They wrote an article on it, and basically what the guy they interviewed was saying
Starting point is 00:34:21 was that over at Eiter, they have a low beta ratio, which is the amount of electromagnetism that you need compared to the amount of plasma you can put into the chamber. So there's like 5% plasma to 95% electromagnetism just to keep this plasma thing from just blowing up, because that can happen. They might not melt down, but if everything went wrong,
Starting point is 00:34:48 the whole thing could blow up. Well, and you know what an atomic bomb is. It's a fusion reaction. Right. This is a lot of those all put together in 100 foot tower. This guy was saying that the beta ratio for their machine is like 100%. So what he was saying is they figured out a way,
Starting point is 00:35:07 and again, it's not very detailed, but they figured out a way to contain the plasma, but in a way that also allows it to expand, because if you think about it, the more plasma there is, the more hydrogen atoms there are, the more hydrogen atoms, more isotopes there are, the more nuclear fusion reactions or events you can have, the more energy you can yield.
Starting point is 00:35:28 So they're saying they figured out how to contain the plasma, but again, like you said, the scientific community is really skeptical, because they think it's just a PR stunt. Well, I think they made the mistake by saying they invented a magicometer to make it all happen, and don't ask about it. Yeah, right.
Starting point is 00:35:46 I did see, though, that where Lockheed was using the figure 8 stellarator configuration, and I think that's true. I found a couple more sources that were kind of vague about it, and I think the details on it are just vague period, but I don't know why they would have been in the donut shape if the figure 8 was 1950s technology that's sort of been disproven. Well, supposedly their whole jam
Starting point is 00:36:09 was that even in the donut, in the tokamak, this donut-shaped reactor, plasma has a tendency to just move around and make its way out. Like it's still not fully contained, and they're using something basically mirrors to catch the plasma that's getting out and moving it to parts of the electromagnetic field that are less dense. So if there's a bunch of protons in this part of the field,
Starting point is 00:36:36 that field is being strained, but then maybe there's not that many protons over here, so they use mirrors to direct the protons to the low density area of the field, to even the whole thing out, which makes sense. But again, if you're not releasing data, don't expect the scientific community to buy it. You got that right.
Starting point is 00:36:53 So there's another way to build a thermonuclear reactor that's currently being worked on, too, and we'll talk about that right after this. Stuff you should know. On the podcast, HeyDude the 90s called David Lasher and Christine Taylor, stars of the cult classic show Hey Dude, bring you back to the days of slip dresses and choker necklaces.
Starting point is 00:37:17 We're going to use Hey Dude as our jumping off point, but we are going to unpack and dive back into the decade of the 90s. We lived it, and now we're calling on all of our friends to come back and relive it. It's a podcast packed with interviews, co-stars, friends, and nonstop references to the best decade ever. Do you remember going to Blockbuster?
Starting point is 00:37:37 Do you remember Nintendo 64? Do you remember getting Frosted Tips? Was that a cereal? No, it was hair. Do you remember AOL Instant Messenger and the dial-up sound like poltergeist? So leave a code on your best friend's beeper, because you'll want to be there when the nostalgia starts
Starting point is 00:37:50 flowing. Each episode will rival the feeling of taking out the cartridge from your Game Boy, blowing on it and popping it back in as we take you back to the 90s. Listen to HeyDude the 90s called on the iHeart radio app, Apple Podcasts, or wherever you get your podcasts. Hey, I'm Lance Bass, host of the new iHeart podcast,
Starting point is 00:38:09 Frosted Tips with Lance Bass. The hardest thing can be knowing who to turn to when questions arise or times get tough, or you're at the end of the road. Ah, OK, I see what you're doing. Do you ever think to yourself, what advice would Lance Bass and my favorite boy bands give me in this situation? If you do, you've come to the right place,
Starting point is 00:38:26 because I'm here to help. This, I promise you. Oh, god. Seriously, I swear. And you won't have to send an SOS, because I'll be there for you. Oh, man. And so will my husband, Michael.
Starting point is 00:38:38 Um, hey, that's me. Yep, we know that, Michael, and a different hot, sexy teen crush boy bander each week to guide you through life, step by step. Oh, not another one. Kids, relationships, life in general can get messy. You may be thinking, this is the story of my life. Just stop now.
Starting point is 00:38:53 If so, tell everybody, yeah, everybody, about my new podcast, and make sure to listen, so we'll never, ever have to say bye, bye, bye. Listen to Frosted Tips with Lance Bass on the iHeart Radio App, Apple Podcasts, or wherever you listen to podcasts. So, buddy, magnetic confinement is pretty neat. And we talked about that, and that's understandable. And I love it.
Starting point is 00:39:29 I want to date it. But internal confinement, I want to marry, because it has lasers. At the National Ignition Facility at Lawrence Livermore Laboratory, they are actually using laser beams. They have a device called the NIF device, where they focus 192 laser beams on a single point in a 10-meter diameter target chamber called a hall realm.
Starting point is 00:39:54 That's got to be German. And basically, inside that target chamber, they have a little tiny pea-sized pellet of deuterium tritium and a little plastic cylinder. It's funny that it can be plastic somehow. Yeah, you'd think it would introduce impurities or something into it. Yeah, or it would need to be like iron or something.
Starting point is 00:40:10 I don't know. It just seems unstable. But that is 1.8 million joules of power from these lasers. They're just going to heat the cylinder up, generate some x-rays, and then that radiation will convert that pellet into plasma and compress it. So again, they're creating plasma, but instead of smashing it together with magnets,
Starting point is 00:40:30 they're super heating it with lasers. So that's your money's on that one. You like that one more. I just think it's neat because I like lasers. But that's your preference of the two. Yes. Well, actually, whichever one works is going to be my preference. OK.
Starting point is 00:40:44 And that one will yield 50 to 100 times more energy out than energy put in. I got you. So that's a good goal. So yeah, I guess basically the whole point of magnetic confinement is that if you can do without electromagnets, you have a more simple and elegant solution.
Starting point is 00:41:03 Oh, you mean the internal confinement? Inertial. Inertial. Yeah, that's what I mean. Inertial confinement, basically the whole thing just happens so fast, you don't even need these magnets to confine plasma because you're not creating the sustained ignition, right?
Starting point is 00:41:17 Yeah, I might have said internal confinement before, by the way. It's inertial. Yeah, I know. That's all right. So what about cold fusion, buddy? That was all the rage. I remember back in the 80s.
Starting point is 00:41:26 Yeah, because in 1989, some researchers said that they successfully created nuclear fusion using just room temperature stuff, like palladium. They took palladium and. Banana peels and beer cans. Pretty much. Heavy water, which had deuterium in it. And they put the whole thing together
Starting point is 00:41:48 and created nuclear fusion without the high temperatures, hence the name cold fusion. And if you can get around these high temperatures, then you work out the whole material science problem, right? And if you work out the whole material science problem, then it's a desirable thing to have cold fusion. The problem is a lot of scientists
Starting point is 00:42:10 tried to replicate these guys' findings and weren't able to, so basically they were kicked to the curb. So does that mean, has cold fusion been abandoned? Or are people still trying to get on that train? No, in 2005, some UCLA researchers basically said, we think we might have this thing down. And they did.
Starting point is 00:42:29 That's something called pyroelectric crystal fusion. Pyroelectric fusion. They use a crystal. Yeah, where basically it's the same result. They do what would be called cold fusion. The problem is, is it has a negative net energy yield. You have to put in a lot more energy than you get out of it. Right.
Starting point is 00:42:49 Well, that's no good. No. Eider seems like they are making headway more than Lockheed despite their claim. They are being, like we said, it's in Europe. And it's being financed by a bunch of different countries. The US is in, but they're kicking in, I think, the least amount.
Starting point is 00:43:08 Only about 17 million euros last year. Of course, we contributed dollars, but they're giving it to us in euros. Right. I think the EU spends the most, about 80 million. South Korea and China kicked in about 20 and 19 million, respectively, each. And I saw earlier where Russia was involved,
Starting point is 00:43:27 but then I didn't see what they had contributed financially. Yeah, they're definitely involved still. Are they still? All right, well, maybe they're just, we're writing a chit for them for later. They'll just pay us back. Right. But it is a very expensive prospect.
Starting point is 00:43:42 And you need countries getting together for something like this is not the kind of thing that the US can take on on their own, I guess, unless you're Lockheed Martin. Right. And you don't have to prove your data. Right. So that's nuclear fusion.
Starting point is 00:43:54 We'll see what happens. Yeah, you got anything else? Man, no, I just say everybody should go read a star in a bottle on The New Yorker. It's really, really good. Yeah, it's pretty neat. You can also go to Instructables if you want to build a nuclear fusion reactor in your garage.
Starting point is 00:44:12 You can do so. You're not going to create energy, because like we said, you're going to be putting more than you get out. But there are instructions, and that kid did it. His is a little more advanced than the Instructables one, obviously. But yeah. Nice.
Starting point is 00:44:27 The 16-year-old kid. Yeah, he's amazing, because his was legit. He's done more than that, too. His TED talk was pretty impressive. Cool. He's like working on with home and security already for various projects that have nothing to do with this. Yeah, I'm sure.
Starting point is 00:44:41 Yeah. Well, if you want to learn more about nuclear fusion, you can type those words in the search bar howstuffworks.com. And since I said that, it's time for a listener mail. And Chuck, before we do listener mail, I want to give a shout out to our Kiva team. Yeah, for those of you who don't know,
Starting point is 00:44:58 we did a podcast many years back on microlending. And Kiva, K-I-V-A dot org, is an organization where you can loan entrepreneurs and, well, it used to be just developing countries. Now you can do it here in North America as well. $20 at a time that you can get paid back for. You can get your money back if you're not happy. Or you can just keep re-loaning that money,
Starting point is 00:45:23 and it helps them get their small business going. And we started Kiva team many years ago, and it is killing it. So you got some stats for us. So basically, as of October 19, we have loaned, our team has loaned $2.7 million to people in developing countries and in the US here and there. And the big one is we've exceeded 100,000 loans by our team.
Starting point is 00:45:54 Our team only has 8,079 members. So to all 8,079 of you guys, thank you. Way to go. Congratulations. Yes, and thanks as always to Glenn and Sonya, our de facto Kiva, what would you call them? Presidents? Presidents.
Starting point is 00:46:09 Presidents of the stuff you should know team? Yep. Captains of the stuff you should know team? No, presidents. OK, presidents. Presidentes. Glenn's like, yes, president. Yeah, they've been really keeping it going for us.
Starting point is 00:46:21 Yeah, and sometimes we'll forget, and Glenn will nudge us, hey guys, remember the Kiva team, we should mention it. Right. So the next goal we have is for $3 million in loans, and we're on our way to it. So come join us. We don't begrudge people who are late to the party. Just go to kiva.org slash teams slash stuff you should know,
Starting point is 00:46:43 and you can sign up. That's right. So now it's time for Listener Mail, right? Indeed, sir. I'm going to call this a skywriting follow-up from Australia. Hey guys, recently listened to how skywriting works, and it reminded me of something. Although this may not be suitable for Listener Mail,
Starting point is 00:47:00 which I disagree, actually, because I'm reading it. Clearly. I was maybe eight or nine when a few friends and I were out on the street playing and doing things that nine-year-olds would do. It's so awkward to say that. So you're not replacing something right there? No.
Starting point is 00:47:17 They were just doing nine-year-old things. OK. It's good, clean, fun. We looked up and saw a plane starting to skywrite, and we're instantly intrigued at what was being written. They started with an H and then an O. This went on for maybe 20 minutes, until finally the word Hooters was
Starting point is 00:47:30 crawled across the sky, albeit backwards. So I guess they had the Hooters Restaurant chicken wing chain in Australia. I guess they're a rich kid. Yeah. Really immature, rich kid. Yeah, or that. My brain couldn't comprehend how this person managed
Starting point is 00:47:47 to screw up writing a word backwards. The best reason my childish brain could come with is that skywriting took place somewhere between us and a group of people that it was initially intended for, and that I just thought it was written up and downwards rather than across the sky. Until now, I never understood or bothered to learn why it was like that.
Starting point is 00:48:06 So thank you for keeping the podcast great and allowing me to figure that out. That is from Marlin. Oh, boy. Hapura-chi-chi. Hapura-chi-chi. Nice. Have you ever seen a word like that?
Starting point is 00:48:24 Hapura-chi. Hapura-chi. Marlin from Sydney, Australia. Man. Thanks a lot, Marlin H. And that's Marlin with an A, even. Oh, yeah? Marlin.
Starting point is 00:48:38 Well, thanks a lot, Marlin. And we're going to say it like that. Sure. If you have an awesome last name and want to share it with us, you can tweet to us at syskpodcast. You can join us on facebook.com slash stuffyoushouldknow. You can send us an email to stuffpodcast.howstuffworks.com. And as always, join us at our home on the web,
Starting point is 00:48:57 stuffyoushouldknow.com. Stuff You Should Know is a production of I Heart Radio's How Stuff Works. For more podcasts from I Heart Radio, visit the I Heart Radio app. Apple podcasts are wherever you listen to your favorite shows. On the podcast, Hey Dude, the 90s, called David Lasher and Christine Taylor,
Starting point is 00:49:20 stars of the cult classic show, Hey Dude, bring you back to the days of slip dresses and choker necklaces. We're going to use Hey Dude as our jumping off point, but we are going to unpack and dive back into the decade of the 90s. We lived it, and now we're calling on all of our friends to come back and relive it.
Starting point is 00:49:38 Listen to Hey Dude, the 90s, called on the I Heart Radio app, Apple podcasts, or wherever you get your podcasts. Hey, I'm Lance Bass, host of the new I Heart podcast, Frosted Tips with Lance Bass. Do you ever think to yourself, what advice would Lance Bass and my favorite boy bands give me in this situation? If you do, you've come to the right place,
Starting point is 00:49:58 because I'm here to help. And a different hot, sexy teen crush boy bander each week to guide you through life. Tell everybody, yeah, everybody, about my new podcast, and make sure to listen so we'll never, ever have to say bye, bye, bye. Listen to Frosted Tips with Lance Bass on the I Heart Radio app, Apple podcast, or wherever you listen to podcasts.

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