Episode #485 from 1:11:59

Extreme temperatures

So you're trying to reach 100 million degrees. How do you get to that temperature fast? And by the way, what can you say to help somebody like me understand what 100 million degrees is like? It seems insane. What does that world look like? I guess just everything is moving really fast. Like you said, you can't put anything mechanical in there. Yeah, so a couple of key things happened. When gas is that hot, there's... We talk about the states of matter. You have solids, where ice, it's cold. The atoms are now bound in a lattice structure together. They're held together. And then liquid, you've broken a lot of that lattice structure. They can move around. They have some kinetic energy, but they're still pretty contained, they stay in the bowl. Keep heating it, now you're in gas. And now these particles are free to move around. They're moving around, they're bouncing off of each other all the time, and you can keep heating it from there, and that's where we talk about some more phases of matter. We can add a little bit more physics here. We talk about rarefied gasses.

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So you're trying to reach 100 million degrees. How do you get to that temperature fast? And by the way, what can you say to help somebody like me understand what 100 million degrees is like? It seems insane. What does that world look like? I guess just everything is moving really fast. Like you said, you can't put anything mechanical in there. Yeah, so a couple of key things happened. When gas is that hot, there's... We talk about the states of matter. You have solids, where ice, it's cold. The atoms are now bound in a lattice structure together. They're held together. And then liquid, you've broken a lot of that lattice structure. They can move around. They have some kinetic energy, but they're still pretty contained, they stay in the bowl. Keep heating it, now you're in gas. And now these particles are free to move around. They're moving around, they're bouncing off of each other all the time, and you can keep heating it from there, and that's where we talk about some more phases of matter. We can add a little bit more physics here. We talk about rarefied gasses.

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Extreme temperatures chapter timestamp | David Kirtley: Nuclear Fusion, Plasma Physics, and the Future of Energy | EpisodeIndex