StarTalk Radio - Things You Thought You Knew - Earth’s Spinning Core

Episode Date: February 21, 2023

What happens if Earth’s core is slowing? Neil deGrasse Tyson and comedian Chuck Nice explore the spinning of Earth’s core, the physics of tire pressure, and the science of toast.NOTE: StarTalk+ Pa...trons can listen to this entire episode commercial-free here: https://startalkmedia.com/show/things-you-thought-you-knew-earths-spinning-core/Thanks to our Patrons Gaija, Kyann McMillie, Brett Moorman, Craig Landon, and Ms. Gordon for supporting us this week.Photo Credit: NASA, Public domain, via Wikimedia Commons Subscribe to SiriusXM Podcasts+ on Apple Podcasts to listen to new episodes ad-free and a whole week early.

Transcript
Discussion (0)
Starting point is 00:00:00 This is StarTalk, a Things You Thought You Knew edition. We have three segments ready to roll. One of them is on Earth's core. We're going to follow that with tire pressure. And we're going to round this out with something we've all done before, but I don't know how much thinking you've ever put into it. And it's the art of making toast. No, it's the physics of making toast on StarTalk.
Starting point is 00:00:32 Welcome to StarTalk. Your place in the universe where science and pop culture collide. StarTalk begins right now. Chuck. Chuck. Yes. Hey, man. People have been talking about Earth's core lately. It's been in the news.
Starting point is 00:00:51 It's been in the news. Yeah. Clearly, it's slowing down or something, and now we all have, we have to wait for a scientist to get into a machine that will burrow to the center of the Earth. Where the machine gets stronger as the temperature goes up. As the temperature goes up, right? Okay, okay.
Starting point is 00:01:11 And they might as well have found, what's the Wakanda metal? Oh. Because it's the same. Vibranium. Vibranium. Yeah, they might as well just be vibranium. Vibranium. Yeah. It's stronger. And mine's just being vibranium. Okay.
Starting point is 00:01:30 So, Chuck, do you never leave your couch and watch movies? Believe it or not, I don't even watch a lot of movies. Yeah, but you've got some good fluency there. Yeah. I get to. Yeah. I remember them all, though. That's why I don't watch a lot.
Starting point is 00:01:42 I can never get them out of my head. What's fun is, yes, the latest news is that the core is slowing down. Right. And so that means we're going to have to go there and speed it back. Exactly. So let me just back up. I don't claim to be a geologist. Okay. And maybe we should do a whole show on this, I think,
Starting point is 00:02:03 and bring in one of my geology colleagues, geophysicist colleagues. But I know Earth is a planet. So let me speak of Earth the way an astrophysicist would speak of Earth. Okay. All right? So when planets form, they are not solid initially. Right. All right? They're first gaseous, and then with enough pressure, they might become liquid.
Starting point is 00:02:20 But in any case, once a gravitational field is set up, then heavy things fall to the middle. Right. Because it's not solid yet. Right. Okay? Heavy things fall to the middle. And of all the available ingredients that are just hanging around in the formation of a star system, you get things like, you know, hydrogen and oxygen and silicon and nitrogen and carbon.
Starting point is 00:02:44 Right. And you keep going. And as you get to the heavier elements in the periodic table, iron is very common in the universe and nickel. These ingredients are heavier than silicon and oxygen and carbon. So they fall to the middle. And what floats on the top are light things like rocks. Okay, there you go.
Starting point is 00:03:10 We don't think of SiO2, silicon dioxide. That's a major active ingredient in rocks. We don't think of them as light. We think of rocks as heavy. Right. But they're the lightest thing going on Earth when Earth is forming. And they all float to the top. So our crust is made of light, solid ingredients.
Starting point is 00:03:32 And everything below it is made of heavier ingredients. Like a delicious metal pie. Metal pie, exactly. So nature pre-sifts the ingredients. And what's interesting is protoplanets that did this and then solidified, protoplanets might get slammed later on and their bits and pieces break into asteroids. So some asteroids are made of crustal material. Others are made of core material.
Starting point is 00:04:06 Gotcha. So asteroids made of core material are pre-sifted heavy elements. Gotcha. Such as, like I said, iron and nickel, gold, silver. All these heavy elements are pre-sorted for you if you select a metallic asteroid versus a rocky asteroid. Okay. Now, there's more of the rocky stuff than of the metallic stuff.
Starting point is 00:04:31 So most asteroids are rocky. Some asteroids are metallic. And that's what we have out there. So now we have Earth, which was thankfully not broken apart. It has retained its integrity. Okay? Okay. By the way, there are transition zones
Starting point is 00:04:47 where the metals are trying to descend and the rocky stuff is trying to ascend. And by then, the earth froze, solidified. Froze for its whatever the ingredients are. Solidified and it's stuck in place. And this is how you get like these ore, what do you call these? Deposits?
Starting point is 00:05:07 These loads, these deposits. Right. They can be trapped in places, frozen out from whatever was going on previously. All right? Nice. But the bulk of those materials have separated. Just to make that clear. Okay.
Starting point is 00:05:19 So now, Earth has retained heat from its past. Okay? And so from the formation heat, it is still trying to cool down. Right. All right? Mars is smaller than we are, and so it has more surface compared to its volume. You do the math on that.
Starting point is 00:05:39 It turns out to be correct. And the more surface you have, the more you can radiate away your heat. Gotcha. That's why small animals, mammals, have to eat way more food than larger mammals relative to their body weight because they're radiating away their heat much faster. Right. Because if you look at their surface area compared to their volume, right? This is why babies need extra protection for their body temperature to protect it.
Starting point is 00:06:09 So we did a whole surface area thing. I remember. I was about to say. It relates to that. So we have less surface area for our volume. It'll take us longer to cool. The consequences of this leftover heat is that we, on the crust, which is cooled solid because it's touching the outer air, we are floating on this sort of plastic liquid mantle.
Starting point is 00:06:39 Oh, the lake of fire. Okay, and so we are floating, and that's how you get continental drift. And occasionally, that mantle can punch through, and you get a volcano. Okay. And so we are floating, and that's how you get continental drift. And occasionally, that mantle can punch through, and you get a volcano. Nice. Okay? So you get earthquakes and volcanoes from a lot of this leftover heat. But let's keep going down. Okay.
Starting point is 00:06:54 Down. And now the mixture in the earth is changing. Mm-hmm. And it is so hot, the iron has liquefied. So the outer core of Earth is liquid iron. Damn. Okay? That's how hot it is.
Starting point is 00:07:11 That's got to be hot. It's hot. It's about as hot as the sun's surface, basically. Whoa. Yeah, about 10,000 degrees. You'll melt iron, okay? Take that, Dante. Hell hath no fury like earth's core.
Starting point is 00:07:27 How about that? That's right. All right. So yeah, Dante, you're referring to Inferno, which he describes the descent into hell. That's right. Which if you read that and believe it, you would never commit a sin for the rest of your life.
Starting point is 00:07:41 Ever. It's some pretty devastating descriptions. Yes, exactly. All right. So where are we? So now we have this liquid outer layer. Okay. Well, why isn't it liquid all the way through? Because as you keep going further down,
Starting point is 00:07:57 the pressure is so high that it's compactified into a solid. Look at that. Yes. So it's just as hot, but the pressure is so great, it will not allow it to melt. Yes. Oh, my God. Yes.
Starting point is 00:08:12 So you have a solid iron core center that's surrounded by a liquid core outer. This means the solid core is kind of independent of the rest of the planet. Yes. Because it's only a liquid. It's like lubrication even. Yes. If you want to think about it that way. Oh, my God.
Starting point is 00:08:34 It's like a lava lamp. Yes, Chuck. It's exactly like a lava lamp. No, I forgot. What? They have these blobs that rise and fall. Yeah, they got the blobs in there. Yeah, yeah.
Starting point is 00:08:45 Right, right, right. Exactly. But go ahead. Okay, so by the way, how do we know all this? You can say, have you been there? How do you know? Right, exactly. Let me hear it.
Starting point is 00:08:52 Let me hear it. So how do you know all this? Like, you've been to the center of the Earth? Kind of with our pressure waves, yes. Oh. For every earthquake, once you find the epicenter, which is not too hard, you can triangulate on it. As long as you have earthquake sensors scattered around the world, you can time how long it takes that signal to reach you. In so doing, you can infer the interior structure of the Earth.
Starting point is 00:09:21 Because different materials will transmit those waves at different rates than other materials. So the interior becomes the medium. Correct. And then you're measuring the wave as it moves through the medium, and that allows you to get the information. You can learn if there are edges between sharp boundaries between one
Starting point is 00:09:40 medium and another. Occasionally, you can have a wave that reflects off of a surface. It's a very complex map that you make from all of these signals when they're done. And it's not just earthquakes. You know what else gives you these data? Underground nuclear tests. Oh, wow.
Starting point is 00:09:58 And those are especially valuable geophysically because you know exactly where the test occurred. So there's less uncertainty in where the epicenter is. You hear that, North Korea? We're on to you. So you add up all these data, and you can reconstruct what the center of the Earth, what the entire structure of the earth would be like. Wow. Okay, without ever having gone there. That's amazing. Yeah, and these are pressure,
Starting point is 00:10:30 basically sound waves as they go through. Yeah, exactly. That's crazy. Yeah, so it's pretty cool. That is. It's pretty cool. And by the way, it doesn't reflect too often, forever, because it slowly damps out, and then you have no signal at all. Right. But there's enough, these things are huge deposits of energy when they occur, and the earthquakes and the like. And so it's enough energy to make it through Earth and back. But again, you need sensors. Otherwise, it's a waste, right?
Starting point is 00:10:57 Yeah, exactly. Okay, seismometers basically is what you need. Okay, so another thing. We know from physics that moving electrical charges create magnetic fields. Right. Okay? Faraday first noticed this. Mm-hmm.
Starting point is 00:11:20 Okay? He, and vice versa, okay? So you can move a charge. There's a magnetic field that's created around it. You can take a charge, move it in a magnetic field, and the magnetic field will induce a current in the wire. So, Faraday did this. So, he had a magnetic field, took a wire,
Starting point is 00:11:43 moved the wire through the magnetic field, and an amp meter moved. The needle moved because current was introduced into the wire. That's how electricity is made today. Exactly. It's what a turbine is, all right? You're moving wires through a magnetic field, creating a current. Wow.
Starting point is 00:12:01 And with power plants, everything about a power plant is so that you can sit there and move wires through a magnetic field. That's so amazing. It's such a simple, simple concept. It's a simple concept. And that's just scaled up to this huge form. It's amazing. It feeds the civilization. When Faraday first demonstrated this, and there's just a little meter, he's like, that's cute, Michael.
Starting point is 00:12:24 Okay, what's Michael been doing today? There just a little meter he's like that's cute michael okay what's michael been doing today all right there's a little meter that's a nice toy and there's a famous quote maybe apocryphal when asked uh when he asked for more funding and he says of what value is this to the british crown and and the british empire and he don't know, sir, but one day you will tax it. Wow. That's how you make electricity. All right, let's get back to the earth. That is also how you talk to any government anywhere.
Starting point is 00:12:56 Yes, yes, if you're a scientist and an inventor. So you have this liquid layer. If you have a liquid layer, then the iron can move within that liquid, and iron is an electrical conductor, as we've known since childhood, with the iron filings on the magnets. On the sheet of paper, yeah. So, when you have these electrons provided by the iron moving, it creates a magnetic field, and that is the origin of Earth's magnetic field. There you go. That's the origin.
Starting point is 00:13:33 That's super cool. Okay, and it's something called a dynamo phenomenon, where you have this circulation, and this continues. And by the way, as is true for the sun and in many astrophysical objects, the dynamo runs a course of life where it gets stronger, then it gets weaker, and then it gets
Starting point is 00:13:53 stronger again, but with the opposite polarity. Oh, I'm like a phoenix, baby. Oh, so we have evidence from iron that has been spewed forth from volcanoes that then solidified in place, capturing the magnetic field at the time that the field was laid. And we see evidence every several hundred thousand years of the magnetic field of Earth flipping back and forth. Oh, look at that.
Starting point is 00:14:25 So that's on a cycle, okay? The sun's magnetic field flips on an 11-year cycle. Look at that. Okay, sun has an 11-year cycle, and every 11 years, it gets more luminosity and less luminosity. But every 11 years, it'll do the same thing, but with the poles reversed. Okay.
Starting point is 00:14:43 Okay. Okay, so now, let's get back to this. The core basically rotates with the surface of the Earth. Okay. But occasionally will rotate a little faster. All righty. Slow down, and then a little slower. Okay.
Starting point is 00:15:00 All right? So we're all comparing it relative to we on the surface. And the recent measurements showed that the solid core of the Earth was trailing behind Earth's surface. Earth, wait up! Right, right. So presumably, this has always been happening. It's not like there's something new. But there's a periodicity of this that they're estimating to be about 70 years,
Starting point is 00:15:24 There's a periodicity of this that they're estimating to be about 70 years, where it'll slow down, catch up again, overtake us, and then return. So these measurements are affirmations that the core has its own sort of rhythms inside the liquid iron within the rest of the Earth that's rotating around it. All I know is this whole thing was worth it just to hear the word periodicity oh oh i mean i don't know where you pulled that we use that word all the time oh my god yeah the rhythms of the universe uh to find them we track their periodicity oh look at it let me tell you something if you gave that to like um you know the people like always and stay free and they they would love you because that is that's a beautiful word what i'll tell you right now you will talk about feminine products
Starting point is 00:16:24 yes i'm saying like that's what you're talking about there products on television? Yes, I'm saying. That's what you're talking about? There's so much stigma unnecessarily attached. Right, right. But instead it's just like, hi, yes, I'm going to need some periodicity products. Thank you.
Starting point is 00:16:39 And I'm totally cool with that. Okay, all right. Thank you. Mom, send me to the store to get your periodicity stuff. Okay. All right. So anyway, so we're still trying to figure out what it means that we have this 70-year cycle in the center of the Earth. Right. But right now, Earth's magnetic field is weakening.
Starting point is 00:16:56 Okay. But it's not going to go away in anybody's lifetime, so nothing would worry about it. Right. lifetime, so nothing, I wouldn't worry about it. Right. And by the way, there's no evidence of extinction when the magnetic field went to zero and then went back up when it
Starting point is 00:17:12 flips. There's no, so because people say, well, the magnetic field's protecting us from the dangerous rays of the sun. And it may be, but whatever damage it caused, it's not even a blip in the fossil record. Everybody's going to be okay.
Starting point is 00:17:27 The fish are underwater. The particles don't hit them ever, right? So fish don't give a... They don't care. Everybody's fine, except Harold. He was in the wrong place at the wrong time. Harold, we're sorry. What?
Starting point is 00:17:41 That is totally a fish name. The clueless fish named Harold. The clueless fish named Harold. The clueless fish, Harold. That is so the name of the clueless fish. Who got fried when the poles flipped. That's what you get for trying to use those legs that you should have stayed in the ocean. Stay in the ocean, Harold. Any time we evolve yet.
Starting point is 00:18:04 All right, we got to end it there, Chuck. So that's my little bit, but I'd like to hear this all from the mind and the brain of a geologist. So we'll try to do
Starting point is 00:18:13 a whole show on that. Yeah, it's all fascinating. I love it. You got it. We got to take a quick break, but when we come back, more things you thought
Starting point is 00:18:21 you knew. We're going to be talking about tire pressure. Hey, I'm Roy Hill Percival, and I support StarTalk on Patreon. Bringing the universe down to earth, this is StarTalk with Neil deGrasse Tyson. This is StarTalk with Neil deGrasse Tyson. Welcome back to StarTalk Things You Thought You Knew, segment two. Chuck, we're going to talk about tire pressure.
Starting point is 00:18:57 All right. Are you ready for tire pressure? I'm really not. Yeah. But this is good. You know, hey, listen, I feel really not. But this is good. You know, hey, listen. I feel like this. At this point, you know, we done paddled out. It's time to ride the wave.
Starting point is 00:19:14 That's the way I feel. We're out there. Just let's do it. Bring it on. We're out here. You say tire pressure. I'm like, you got to be zen enough to go ahead and jump up. It's time to get up and surf this wave.
Starting point is 00:19:26 All right, let's do it. So tire pressure. First of all, if you have a tire with, quote, no air in it, of course there's air in it because the atmospheric air is in it. Okay? And atmosphere has its own pressure. And this is the weight of a column of air from Earth's surface all the way up to the edge of the atmosphere. If you had found a way to weigh this, I think we might have talked about this in another explainer. But if you have like one square inch or one square anything, but one
Starting point is 00:19:57 square inch and weigh that column of air, it will weigh 14.7 pounds. Okay? Nice. And the way air works, fluids work, is that pressure, I would say, yes, it's sitting on the scale, but that pressure manifests in every direction because the molecules
Starting point is 00:20:12 are vibrating in every direction. So, so right now, I have 14.7 pounds per square inch on one side of my hand and on the other,
Starting point is 00:20:21 above, bottom, and so everything's all equaled out. So I don't even notice it that's why you're not getting crushed by your 14 pound correct air just every doesn't make a correct because it's pushing down on you and pushing up it's even whereas if i have a suction cup and i press out the air that would otherwise be balancing it. I press it out.
Starting point is 00:20:47 Yeah. So now I say, lift up the suction cup. You say, I can't. It's sucking me down. No, it's not. Why can't you pick up the suction cup? 14.7 pounds. Per square inch pressing down.
Starting point is 00:20:57 Per square inch is pushing it down. It's really not sucking anything. Yeah, suction cups don't suck. They don't suck. They got a bad cups don't suck. They don't suck. They got a bad rap for so long. They don't suck. Okay. They don't suck.
Starting point is 00:21:11 So if you had 10 square inches of area on the suction cup, I can ask you how much force would it take to pull the suction cup off the surface? So I got to go 10 square inches times 14.7 pounds per and then push back in that opposite direction. Okay, that gets you 147 pounds. So if you can pull 147 pounds or more, it pops right up.
Starting point is 00:21:34 Or you can cheat and pop open a little curl in the edge and then let nature... Air slips in and then it just comes off. See, that's letting nature help you out. Okay, so the point is, if you fill a tire to what we call 10 pounds per square inch, that's 10 pounds on top of the air pressure that's already in there. That's all I'm saying.
Starting point is 00:21:57 Right. All right, so first of all, just lay that out. All right, so now, have you noticed, or perhaps not, that on bicycle tires, the thinner, the skinnier the tube, the what? The less air you should keep putting in it once it gets hard, because it will pop. Okay. I'm telling you. From experience, okay? Okay, if you look at the ratings of thin tires,
Starting point is 00:22:30 in essentially every case, depending on what they're made of, but in every case, they have a higher pounds per square inch rating than the bigger tires. Okay? Higher. Okay. Period. I didn't know that, to be honest that yes okay so now watch i this is this
Starting point is 00:22:47 is the first i'm ever hearing because you never gotta pay attention okay well no i'm gonna tell you why because i come from the times when you would fill your tire and then you just push down on it and if you can actually push it and flatten it, you're like, now push the more air in. Oh, that was how you measured. That's how you measured it. And then once you couldn't do that, you'd be like, all right, it's time to go. You want to use a gauge, okay? Right, exactly.
Starting point is 00:23:14 All right. So, and the gauge is calibrated to not count air pressure. All right? So that's how they work. All right, so now watch. Here you go. All right, so now watch. Here you go.
Starting point is 00:23:28 So, the pounds per square inch equals the pounds per square inch of your tires in contact with the road, okay? You sitting on your bicycle, and the bicycle has tires, and the tires are in contact with the road, obviously, the heavier you are, the flatter the tire is going to look. Okay? True.
Starting point is 00:23:57 Okay? You know this. Well, yeah. Why does the tire flatten if you're heavier? Why does it do that? I'm going to tell you why. Because at all times, the pressure inside the tire per square inch times the square inches of tire in contact with the road
Starting point is 00:24:20 has to equal your weight plus the weight of the bicycle. At all times. Wow. At all times. Okay. Okay. So. So. Okay. All right. So, if I have a big tire, like a kid's tire, okay, if I have one of those kind of tires, and it's huge, it might take 30 pounds per square inch. That's not uncommon. Okay? 20 to 30 pounds per square inch. And there's a square inch of it in contact in the back and a square inch in contact with the front. Add those up.
Starting point is 00:24:59 It is holding up 60 pounds. That could be the weight of the bicycle plus the weight of the kid. Okay? You put a heavy kid on there, the bicycle plus the weight of the kid. Okay? You put a heavy kid on there, the bicycle has to hold up more weight against the air pressure in the tires. So the tires flatten a little more, adding more surface area. Okay? Adding more area so that now you go the air pressure times the square inches in touch with the ground, and now that'll equal the weight of the heavier kid.
Starting point is 00:25:27 Okay. So I, I'm heavy. All right? I'm 260 pounds right now. Okay? All right. Okay. So now, I ride a bicycle with very narrow tires.
Starting point is 00:25:41 The air pressure in those tires is 130 pounds per square inch. 130 pounds, okay, per tire. So watch what happens. I deflate it to that amount, and those tires will flatten to slightly more than a square inch per tire. Because it's my weight plus the weight of the 22-pound bicycle. It's got to hold up 280 pounds. So it's going to flatten slightly more than a square inch on each, and that is my tire. Okay? Okay. So farm tractors have huge tires.
Starting point is 00:26:25 Right. huge tires. Right. Huge tires. In that way, they put relatively low air pressure in them. That way, when the tires roll over the crops, it does minimal damage. Right. Because you're not digging in. You don't read that. The pressure. Okay. Brilliant. You don't need that. Spread out the pressure. Okay?
Starting point is 00:26:47 Brilliant. You can still hold up the tractor if you get enough area coming down. Otherwise, you'd be leaving deep tracks in the road, and you can't have that. Not in your farm. Oh, it's like dune buggies. They all have big, giant, wide, like, balloon tires. So, well, that one is to increase traction on sand, okay? Yeah, but they don't dig into the sand.
Starting point is 00:27:09 But they don't dig into the sand, correct. And so tire pressure is all about how much weight are you holding up. And they will tell you in your car, if you're going to carry a heavy load, increase the air pressure in your tires so that your tires don't flatten out. Okay? If you increase the pressure from let's say, you know, 35 pounds to 45 pounds
Starting point is 00:27:34 per square inch, that gets you extra support in all of your tires. In a typical car, you know, how wide is a tire? You know, it might be a foot, you know, 9 inches. 18 inches is a typical? You know, it might be a foot, you know, nine inches. 18 inches is a typical tire. No, no.
Starting point is 00:27:48 Cross? Yeah. What are you, riding the Indy 500? 18 inches? Yeah, okay. All right. I'll give it to you. I don't know.
Starting point is 00:27:58 We're both city people, so, you know. Well, yeah, I mean, I drive an SUV, though. Oh, okay, fine. They're sitting on 18s. It's an SUV. You, yeah. I mean, I drive an SUV, though. Oh, okay. Fine. They're sitting on 18s. It's an SUV. You said car. Excuse me.
Starting point is 00:28:10 I'm really not the car. Mr. SUV. Okay, fine. So a car might be that. And it's not electric, and I'm very ashamed. But I'm buying an electric car. So I know you already have one. So eventually. All right.
Starting point is 00:28:21 I'm late to the game. So here's what you do. You can do this experiment at home. Go look at how much of your tire is touching the ground. Measure that, okay? Front to back and then across the width. So you'll get two measurements. It might be like five inches front to back,
Starting point is 00:28:37 flattening on the ground. And then measure the width of the tire. Multiply those numbers by each other. That's the square inches per tire. Multiply those numbers by each other. That's the square inches per tire. Multiply that by four, and that's going to give you the weight of your car. Get out of here. That's pretty wild. I mean, that makes sense just from what you just said.
Starting point is 00:28:56 There's only one problem. I do not give a damn how much my car weighs. Don't do it. Chuck, do it for science. Okay. Chuck, do it for science. Okay. I will do it for science. You should get somewhere between, you're an SUV,
Starting point is 00:29:11 somewhere between 1,500 pounds and a ton, 2,000, something like that. Okay. But all just by making the square inches. So, sorry, you have to know
Starting point is 00:29:21 what your tire pressure is first. Okay? Right. And then get your square square in the sidewall. Or maybe if you're a modern car, it tells you on the dashboard. And so you got four tires and get the area. So it's front to back in contact and then the width. Multiply those two numbers, then multiply by four,
Starting point is 00:29:42 and multiply by your air pressure. That's the weight of your car., that's the weight of your car. And that's the weight of your car. And so it's a way to weigh your car without going to a scale. Because your tires are doing it all by themselves. And now all I need to do is figure out the calculation to
Starting point is 00:29:57 put Aunt Gail and Uncle Daryl in the back seat. That's a different calculation. So it'll either flatten the tires some more, so then the car has given itself a way to hold them up, or you increase the air pressure so that at the same area in contact with the ground, it holds them up.
Starting point is 00:30:15 Okay? That's right. And generally, they tell you to increase the air pressure because it's better for gas mileage and things. Yeah. Right on. All right, you got it, dude. I love it.
Starting point is 00:30:24 That's cool. There's math in everything in the world. It really is. I got to tell you, I was worried when you said time pressure. I really was. I was worried, man. We got to take a quick break, but when we come back,
Starting point is 00:30:40 Chuck and I are going to talk about the physics of toast on StarTalk. We're back. StarTalk. Things You Thought You Knew Edition. Segment three. Chuck, we're going to talk about the physics of making
Starting point is 00:31:06 toast. Okay. All right. I'm just saying. You know, sometimes when you bring these up, man, I feel like you just, like you're punking me. You know what I mean? Because I'm like, I'm just like, let me just
Starting point is 00:31:22 see what I can get Chuck to go along with. Astrophysics of making toast. It's like Neil deGrasse Tyson, right? World-renowned scientist and science communicator. Chuck, I'd love to talk to you about something scientifically relevant. Oh, Neil, please do tell. Let's talk toast.
Starting point is 00:31:41 What? All right, so here's the deal. Okay. All right, and I don't know if you ever paid attention to what's going on inside a toaster. Okay. All right. Listen. But it's fascinating.
Starting point is 00:31:51 I have smoked a lot of weed. I have been high out of my mind. I have never looked at the toaster and went, I wonder what's going on in there. All right. Here's the thing. Okay. Here's the thing. Okay. Here's the thing. Toast, if you're going to toast fresh bread.
Starting point is 00:32:09 Okay. Okay. It will spend most of its time in the toaster, most of the time, not browning. Okay. And is this fresh white bread? Because that would make sense. Yes. It's easier to see the browning on white bread. So this is a white bread example.
Starting point is 00:32:31 But can you blame it? Because let's be honest. In bread society, you know, white bread has it the best. They got to that. Why would I want to give up? But the seven grain blended model is coming along. Okay. So here's the thing.
Starting point is 00:32:45 And let me tell you something. Pumpernickel, there goes your property values in the bread box. I forgot all about Pumpernickel. That's some dark ass bread right there. Tell me right now. Go ahead. Never mind. I'm about to get us in trouble.
Starting point is 00:33:04 I'm going to stop. All right. So if you to get us in trouble. I'm going to stop. All right. So, if you observe the bread, most of the time, 90% of the time, I didn't know exactly, but it's very high percent of the time it's in the toaster,
Starting point is 00:33:15 it doesn't change color at all. Oh, my God. Okay. Because it can't change color as long as it's moist. Okay. Because the highest temperature you can heat the bread is 212 degrees, and that's not hot enough to toast the bread.
Starting point is 00:33:36 I gotcha. I mean, that really does make sense. It's like trying to start a fire with green kindling. You can't. Right. You can't. In. You can't. In fact, if you put a green log on an already established fire, the log is not going to ignite.
Starting point is 00:33:51 You know what's going to happen? It's going to hiss out all the moisture for the next hour. Yep. All right? Because the log can't get hotter than the highest temperature that water can get. And the water that's in the log tops out at 212 degrees. So you're going to have a 212 degree log until there's no water left. That's cool. And then
Starting point is 00:34:09 it'll ignite. That's right. Oh, wow. Okay. So your toast in the toaster, if you keep looking at it, it's going to be your white toast. It's going to be white and white and white. And what the heat is doing, it's like, get out of there, you water molecules. Right. Get out. Get out. And it's only doing it to the top edge, not the middle because the heat is only hitting the top the outer edges right
Starting point is 00:34:29 right so so the heat is like uh uh the black toast matters movement yeah chuck you you need race counseling okay Face counseling, okay? Thank you. All right. So go ahead. All right. So once all of the moisture on that outer edge of the bread has evaporated, it can now toast the bread. By breaking apart the bread molecules, the proteins, and the carbohydrates, revealing the carbon, the proteins, and the carbohydrates revealing the carbon. The carbon is black, okay?
Starting point is 00:35:10 If you leave the bread in too long, it's completely black, all right? But you have all this golden tip. That all happens in like the last minute that your toast is in there because it took all the rest of that time to heat up the water and evaporate it. That is pretty doggone cool to be honest and i i got a little excited when you said that because i've never considered it however i don't have a toaster i have a um a toaster oven i don't use okay so okay so in in the oven or any oven if you're going to use a broiler right the same thing same thing. Same thing. You layer the bread. Exactly.
Starting point is 00:35:46 And you're checking it. That's right. And you keep checking it. And you say, it's not making progress. Let me go away for five minutes. No. Because the moment the moisture is gone, that sucker browns in instants. Okay?
Starting point is 00:35:59 So it's not a linear phenomenon. No, it's kind of like if it were a graph, it would bump along the bottom, and then all of a sudden it shoots straight up almost. Yeah, almost straight up. Almost straight up. And I know this because just the other day, it's so weird now, I can't believe that I'm recalling this.
Starting point is 00:36:18 I said, what's taking this toast so damn long? You can't say that. what's taking this toast so damn long? You're the dead saint. And then I turned, I went into the refrigerator, I pulled out some butter and fig spread. And I went back and the toast was brown. There it is.
Starting point is 00:36:44 So that is so wild. You lived this experience. I lived this experience. It's also why you can boil water in a paper cup. Okay. Okay, and I've done this experiment many times. So wait, yeah, I mean, yeah, you just drop the paper cup inside the pot of boiling water, okay? No, no, no, that's not what it, no.
Starting point is 00:37:04 So you can take a paper cup and you have to be careful about this because some paper cups have rims on the bottom that are not actively touching the water on the inside. That will burn, okay? But if you have a wide enough bottom and you have like a Bunsen burner, remember these?
Starting point is 00:37:19 I remember. And you put the flame on the paper cup in the bottom. If the paper cup has water in it, what is the hottest temperature the paper cup in the bottom. If the paper cup has water in it, what is the hottest temperature the paper can get? The temperature of the water. Okay, and so it'll sit there and boil the water. And it'll keep boiling the water until all the water evaporates. Then your paper cup burns.
Starting point is 00:37:38 This is why it's so hard to burn someone at the stake. You think, oh, let me just ignite you. This is very medieval here. Let me put you on the stake and just ignite you. You can't just ignite, okay? You have all this liquid in you. Right. The real reason why this is very difficult to do is because we have laws against that now. That's why. That's the real reason. That's the actual reason. It's difficult. Thank you. Let me get out of my medieval. So what they would do, especially the Catholic Church, to make sure you would burn, that sometimes they would burn you upside down.
Starting point is 00:38:16 And that way will control the blood or the blood would drain. And as the blood drains, then you have no liquid left in you and you burn faster. Or you can burn in other directions where you retain the blood. left in you and you burn faster. Or you can burn in other directions where you retain the blood because if you don't want the blood to come out, there's some other religious ritual where the whole person has to be burned, including their blood.
Starting point is 00:38:32 But then the blood has to still evaporate before any... So you'll die before all that happens, of course. But in terms of igniting the body, you know what I'm saying? It just doesn't simply happen that way. And this is sped up if you have fast-moving air, hot air across the food. Yes.
Starting point is 00:38:50 This is like a wind heat factor. Mm-hmm. We have an explainer on wind chill factor and wind heat factors. Yes. Okay? Because if it's cold and the wind is blowing, you feel colder. Colder. Right.
Starting point is 00:39:03 If it's hot and the air that's blowing is hotter than your skin temperature, you'll feel hotter. Right. Okay? So, if you put food in, let's say, an air fryer. Yes. What does that mean? Okay. So, they are going to brown your food fast because they're moving hot air across and they're evaporating any possible moisture on that surface.
Starting point is 00:39:27 And the faster the wind goes, the faster you'll evaporate it, and the faster you can get to the browning. Can't live without an air fryer. I'm sorry. It's amazing. They're wonderful. Yeah, they're really air toasters. Yes.
Starting point is 00:39:38 Because, you know, unless the surface is sprinkled with oil, and then the oil will fry the, you know, you can heat the oil. So you're still oil frying, but you're using air to heat the oil to fry the food. Right. But if it didn't have any oil, it's just a fast toaster. Yeah, exactly. You mean I spent $400 on a toaster? Yes, you did. Yes, you did.
Starting point is 00:40:06 Yes, you did. You did indeed. So that's everything you wanted to know about toast and why it's not a linear process. Well, that was fun. And what don't you do? You can do this experiment. Okay.
Starting point is 00:40:20 Take a slice of bread. Okay. Leave it out until it just gets hard. A little crusty. Okay. Right. Just leave it out. Just leave it out.
Starting point is 00:40:28 Okay. It won't get crusty. It'll just get hard. Yeah. It's no longer squishy. And then you have another one that's squishy that you just took out of the bag. Okay. They're both at the same temperature.
Starting point is 00:40:39 Right. Okay. Now put them both in your toaster oven. We're both in the toaster. And the one that had the lost moisture will toast 10 times faster. Okay. Oh, yeah. Oh, there you go. So, yeah. And it's already on its way to being toast. That's right. You leave it out.
Starting point is 00:41:00 Why do you keep leaving the bread out? I'm toasting the bread, man. I'm toasting the bread. I'm toasting the bread. Pre-toasting it. Pre-toasting it. It's a pre-toast. And one other thing, a reminder of how surface deep the color is. Okay. Because it's only what that sort of radio of energy can touch.
Starting point is 00:41:18 And anything's behind anything else. It's not seeing your toaster thing, all right? So, a reminder of that is if you happen to burn the toast, you just take a bread knife, or a knife, not, you know, a knife and scrape off the black. Right. And then there's like this, and you can
Starting point is 00:41:34 salvage many a burnt toast that way. Or, you could just accept the fact that it is black and enjoy it for its beautiful blackness. You could do that as well. Yeah, Chuck totally, definitely needs race therapy. I know, I know.
Starting point is 00:41:55 I can't help it. So, maybe that's more than you ever cared to know about making toast. No. I just thought I'd put that. The thermodynamics of toasting. That is awesome. We got a title that's more than you ever cared to know about making toast. No. I just thought I'd put that. The thermodynamics of toasting. That is awesome.
Starting point is 00:42:07 We got a title that's just that. The thermodynamics of toasting. Okay, of toast. Yeah, of toast. And the takeaway here is, however long you're staring at the unbrowned toast, let that not be the measure of how much longer you have to wait. Yes. I know this firsthand. Absolutely. Yeah, yeah. You got it. All right, how much longer you have to wait. Yes. I know this firsthand.
Starting point is 00:42:26 Absolutely. Yeah, yeah. You got it. All right, that's all we had time for, Chuck. Oh, that was great. That was great. That was great. That was yet another edition of Things You Thought You Knew from StarTalk.
Starting point is 00:42:38 Chuck, always good to have you. I'm Neil deGrasse Tyson, your personal astrophysicist, as always, bidding you to keep looking up.

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