Daniel and Kelly’s Extraordinary Universe - The mysterious sources of the Van Allen radiation belts

Episode Date: November 3, 2020

Daniel and Jorge talk about the strange belts of particles surrounding the Earth, and the South Atlantic Anomaly 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 This is an I-Heart podcast. December 29th, 1975, LaGuardia Airport. The holiday rush, parents hauling luggage, kids gripping their new Christmas toys. Then, everything changed. There's been a bombing at the TWA terminal. Just a chaotic, chaotic scene. In its wake, a new kind of enemy emerged, terrorism. Listen to the new season of Law and Order Criminal Justice System
Starting point is 00:00:33 on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. In sitcoms, when someone has a problem, they just blurt it out and move on. Well, I lost my job and my parakeet is missing. How is your day? But the real world is different. Managing life's challenges can be overwhelming. So, what do we do? We get support.
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Starting point is 00:01:16 Michelle Obama. Folks find it hard to hate up close. And when you get to know people and you're sitting in their kitchen tables and they're talking like we're talking, you know, you hear our story, how we grew up, how Barack grew up. And you get a chance for people to unpack and get beyond race.
Starting point is 00:01:32 All the Smoke featuring Michelle Obama. To hear this podcast and more, open your free IHeartRadio app. Search all the smoke and listen now. Hey, Jorge, did you know that we have a planetary defense system? Nice. Does it involve giant lasers? Not that I'm worried. wear of. And how can it work? Well, this system actually predated the development of lasers by billions of
Starting point is 00:02:02 years, and it's actually totally natural. Oh, nice. Does that mean it's organic or vegan, vegan lasers? Absolutely. No animals were hurt, but it's actually not all good. Now you have me worried. Yeah, it turns out there's a big hole in our planetary defense system. Really? I bet it's our fault. Was it caused by the lasers? No, actually, the hole is also. also natural and it has a really cool name. Uh-oh. What's it called? It's called the South Atlantic Anomily. Hi, I'm Orhey. I'm a cartoonist and the creator of PhD comics.
Starting point is 00:02:52 Hi, I'm Daniel. I'm a particle physicist, and I'm actually not in favor of giant planetary lasers. What do you mean? How can you be anti-giant lasers? Aren't all lasers good or at least fun to shoot? Exactly. A giant planetary laser that you build in the first act must be pointed at some planet by Act 3. Is this in the science fiction movie you're writing? It is, but it's also true. You know, you develop some massive laser capable of defending
Starting point is 00:03:21 the Earth. That thing will eventually get pointed at someplace on the Earth. Uh, well, um, I mean, if you build it on Earth, it's kind of hard to point it at ourselves. Super villains will find a way. Hmm. I see. I guess the aliens just need a giant mirror and then we're toast. Exactly. Exactly. That wasn't such a great idea after all. Yeah. Welcome to our podcast. Daniel and Jorge explained the universe, a production of IHeard Radio. In which we don't worry so much about zapping aliens with lasers, but instead we like to think about all the mysteries of the universe, all the things that are. deep out there, misunderstood, not understood, that are currently being investigated by scientists.
Starting point is 00:04:01 And also the things that are nearby, the things right around us that we are still probing. Yeah, because there is a lot of stuff out there in the universe. In fact, the whole universe is filled with stuff. And some of it is pretty amazing and incredible to learn about and to discover. But some of it can be kind of harmful. It certainly can be. And there's this consistent story that every time we do something new to explore space, send up a new satellite, build a new kind of telescope, we see something totally unexpected, something that makes
Starting point is 00:04:28 scientists go, what? Are you sure? Did you check your calibrations? And these are wonderful opportunities to learn how the universe works. Every time we get surprised, there's an opportunity to learn something new. So what happens in your movie, Daniel? Does a scientist go, what? That needs more calibration. Shift DF filters on it. Yeah, exactly. You know the story. Some grad student finds something weird. His professor doesn't believe him and disregards it. And that ends up being the downfall of humanity. And then somehow the handsome physics professor ends up saving the world. Wearing a white lab coat.
Starting point is 00:05:01 It's the worst movie ever. Sorry, pressing the laser button. Accidentally leaning on the laser button. Yeah, it sometimes seems like we are just this rock floating out in space. And there's a lot of stuff that can happen out there, you know? Asteroids or solar winds. There's a lot of stuff sort of coming to get us. Yeah, when you look out into space and you see all those stars, it seems amazing that you can see so far,
Starting point is 00:05:23 that we can probe the distant depths of the universe and ask questions about what happened billions of years ago and light years away. But what you're looking through is not actually empty. The space between us and those stars between us and those explosions is not empty. It's full of incredible interactive stuff. And there's a lot to learn just by looking at the things
Starting point is 00:05:43 right around our own planet. Yeah, we live in kind of busy neighborhood, right? I mean, it's not apparent to the eye, but there is a lot of stuff swirling around it. Exactly. Most of the universe is actually invisible. There are neutrinos, there's dark matter, there's all sorts of stuff all around you that you cannot see. So remember, you are only seeing a little slice of the universe, the part that radiates in the visible spectrum that you can detect. Most of the universe is invisible to you. But science has built new kinds of eyeballs, new ways to explore the universe and to reveal what's actually happening. And it turns out that right around our planet, there's some really amazing things, swooshing and swirling.
Starting point is 00:06:23 So today on the podcast, we'll be asking the question. What are the Van Allen radiation belt? Now, Daniel, are these, is this like a heavy metal rock band? Isn't Van Allen, the name for a rock band? Van Halen. I'm thinking Van Halen. It's a crossover between heavy metal and karate. Yeah, does it involve heavy metals?
Starting point is 00:06:47 If you go beyond black belt in karate, then you get like a uranium belt or plutonium belt. And so, yes, those would be heavy metal radiation belts. Oh, man. We just smashed heavy metal and karate for no good reason, really. That's right. And then you make a band. Because these are radiation belts.
Starting point is 00:07:04 They're not even made out of metal. But those are radioactive metals, you know. But anyway, then you get together with your friends and you have crazy long hair and dance around in leotards. And yes, you can be a heavy metal band. But yeah, so apparently there's a lot of stuff going out there in space, especially right around us. And some of this stuff is called the Van Goghap. down in Radiation Belt. So we were wondering how many people out there knew what this was
Starting point is 00:07:28 and what their mean at it. That's right. So as usual, I asked for volunteers on the internet to speculate without any background information about the next set of questions for the podcast. And if you'd like to volunteer and hear your own speculation on the podcast, please write to us to questions at danielanhorpe.com. I'm not sure. It sounds like something that a superhero would wear when he wants to irradiate the bad guy. Man, if you would not ask me about, Van Halen and their belts, probably I could tell you something, but at this moment I don't know about Van Allen. I vaguely remember this as being like a zone just outside of the planet that's like a zone of energized particles that are kind of held in place by, I don't know, the planet's gravitational pole, magnetic pole, something like that. The charged particles from solar winds that are sort of captured in giant expanding halos around the Earth, something like that, or two giant ears, sort of mouse ears around the Earth, but I don't know what they do or why they're captured or what effects they have.
Starting point is 00:08:40 It is a ring of radiation somewhere in space around Earth, maybe between Venus or between Mars and Earth, where there's just an intention. amount of radiation that would be very uninhabitable. Even if we would pass through it, it would cause a lot of damage to electronics or to anyone inside a ship. All right. So pretty good guesses. Somebody did relate it to the late, great, and awesome Eddie Van Halen. That's right.
Starting point is 00:09:13 Eddie Van Halen, one of the greatest rock and roll guitarists of all time who recently passed away. Yeah, but not everyone seemed to know what it is. Didn't ring a lot of bells for people. No, but it did sound like somebody out there has a movie they want to pitch, a superhero, wearing radiation belts to irradiate the bad guys. Somebody, quote unquote. That's totally not me. It sounded a lot like you.
Starting point is 00:09:37 You think I would interview myself and insert my own ideas into these interviews? That's a genius idea. I can't believe I didn't have, actually. I know you interview your family all the time. I can recognize their voices now. All right. Well, I hadn't had that idea. But now, some point in the future, I will insert myself doing a false accent into one of these.
Starting point is 00:09:55 And I'm going to wait to see if you spot it. Well, either way, it's a great idea for a sequel for your current size fiction novel. So, yeah, so I'm guessing it has something to do with radiation or particles or electrons and protons floating out in space, maybe in a circular way to call it a belt. So, Daniel, what are the Van Allen radiation belts? So exactly as you say, these are huge belts of radioactive particle, not belts around me or around your waste, but around the earth. So the earth is spinning and then also spinning around the earth are all these charged particles that are zooming around very high speeds in these well-defined regions, these belts, and there's more than one of them. Now, are they going in a circle or are they just
Starting point is 00:10:37 hanging out in the form of a circle? No, they're definitely moving and they are more in the shape of a donut because they're whizzing around the earth and they're sort of organized or heavily near the equator. Okay. These are sort of amazing because they were a total surprise when they were discovered. And they were one of the first discoveries of the space age. You know, after Sputnik came out, the U.S. was racing and it gets stuff up there and it sent something into space. And it was very primitive in the 50s. We were just sort of like shooting rockets in the space with little devices on them.
Starting point is 00:11:08 And the guy Van Allen decided to send up basically a Geiger counter and say, like, how much radiation is there in space? And so this was a, they sent up a satellite? Like it was a satellite or just a rocket that went up and down? It was a satellite. So it would orbit the Earth and collect a bunch of data over lots of orbits. And on board it was a Geiger counter and a tape recorder. And the data got beamed down to the Earth using a couple of antennas. But nobody expected there to be much radiation.
Starting point is 00:11:35 They thought, you know, space is mostly empty. We're going to send this up here and we're going to see the radiation from the ground decreasing gradually as it goes up. But instead what they saw was that when you go out into space, There's an incredible amount of radiation. This is the first time people understood that space was basically radioactive. Oh, man. But it couldn't have gone up that far, right?
Starting point is 00:11:57 So this belt is that close to the Earth? The belt is pretty close to the Earth. And so it's broken up into two main belts. There's the inner belt and then these are the outer belt. And the inner belt is not that far above the Earth's surface. It's like one fifth of the radius of the Earth above the Earth surface. So you don't have to go that high up. Yeah, that is pretty close.
Starting point is 00:12:18 It's pretty close. And it stretches out to about twice the radius of the Earth. So it's 0.2-2 Earth radii. That's the inner belt. Now, is this belt sort of like near the equator or is it more like a over-the-shoulder strap or is it like a halo? It's like a really big donut about the same height as the Earth. So there's not very much over the poles, but there's a lot over the equator. It's like if you put the Earth inside of a donut and it just barely fits in the hole.
Starting point is 00:12:44 Yeah, exactly. The earth is sitting in a donut hole of radiation, which is whizzing around the earth at very high speeds and high intensity. And so there's this inner belt. And then weirdly, there's a gap. And then there's an outer belt. So there's two belts with like this gap in between them. It's a jelly-filled donut. It's like a donut with a donut with a donut inside of it and an extra hole inside of that. It's like the turduckin of pastries. Oh, man. And it has radiation. And it'll kill you if you eat it, exactly. And it plays heavy metal music. And so there's this inner belt and then there's the outer belt. And sometimes occasionally there's a very short-lived third belt that lives between them. What? What do you mean short-lived?
Starting point is 00:13:30 Like it comes on and off? Comes on and off. Like you'll get it. It'll hang out for like a month or so and then it'll dissipate. The inner belt and the outer belt are pretty stable. The inner belt more stable than the outer belt. But this third one, it comes occasionally. and then disappears.
Starting point is 00:13:45 And so it's been a bit of a mystery for the last 60 years, what's making these belts? Why do they come and go sometimes? Why is there a gap in between them? And only recently NASA's been sending up satellites to probe these things and to get some more definitive data,
Starting point is 00:13:59 which has led to some pretty interesting answers about what's making these belts, where these particles come from, why they have the weird shapes that they do. And we have it pretty well mapped. Like we're pretty sure it's a donut shape. What I guess, what I mean is like, you know,
Starting point is 00:14:12 you see it more if you launch a rocket from the equator than if you launch a rocket from the North Pole. Yeah, we have it pretty well mapped now. NASA sent out probes in the early 2010s, the Van Allen probes to map these things and get a lot of data. And they found some amazing things like there's this gap between them. And the gap between them is pretty sharp. Like the outer belt starts at sort of like a wall. Now, when NASA report described it like the particles in the outer belt look like they were being repelled by a sheet of glass. It's like a very well-defined edge to the inner side of this outer belt.
Starting point is 00:14:46 And these particles, they're sort of swirling around like a carousel or are they like, I don't know, going around in circles within the donut? They are swirling around. Like all around the earth or just spinning in place? They are going all around the earth. So they're sort of like in orbit around the earth. But the force that's holding them there, of course, is not gravity because gravity is way too weak to hang on to a particle. But yeah, they're all going all the way around the earth. zooming around at really high speeds.
Starting point is 00:15:12 Wow. And now are we the only planet that has them or do we see them on other planets or other things in space? We see them in other planets. Jupiter, for example, has really massive radiation belts and so does Saturn. And basically every planet that has any kind of stable magnetic field will have these kinds of particles. Interestingly, the sun doesn't have radiation belts mostly because its magnetic field flips too often. It's got this crazy 11-year cycle where the magnetic field, the north and south pole flip every 11 years. And as we'll talk about in a minute, it's really the magnetic field of a planet that makes these belts and creates their structure. And so that's why the sun doesn't have one, but all the big planets with stable magnetic fields do.
Starting point is 00:15:54 Yeah, I figured it had something to do with the magnetic field. But we can see them in other planets, too? But how? But they're invisible. They are. I mean, these are particles. And so you don't see them with a naked eye. But if you're clever, you can detect them. And these particles do occasionally radiate. And so if you look for them carefully, you can certainly see them. And we send probes to those planets. And so I've seen, for example, maps of the radiation belts around Jupiter. And it looks similar. It's like a big fat donut.
Starting point is 00:16:20 Although, in that case, it's more like a really big basketball inside a small inner tube because the radiation belt is not as tall as Jupiter. It's more focused around the equator in that sense. Now, does it also have jelly in it? Or maybe it's a different kind of jelly? Or maybe it's a cream donut? It's actually kind of stormy, you know, because Jupiter is crazy on the surface. It's always getting mixed up and colorful.
Starting point is 00:16:45 So maybe it's like different kinds of jelly, yeah. It's more like sprinkles. All right, well, let's get into where these radiation belts could be coming from and why they're important. Where are they protecting us from? But first, let's take a quick break. The holiday rush, parents hauling luggage, kids gripping their new Christmas toys. Then, at 6.33 p.m., everything changed.
Starting point is 00:17:24 There's been a bombing at the TWA terminal. Apparently the explosion actually impelled metal, glass. The injured were being loaded into ambulances, just a chaotic, chaotic scene. In its wake, a new kind of enemy emerged, and it was here to stay. Terrorism. Law and Order Criminal Justice System is back. In Season 2, we're turning our focus to a threat that hides in plain sight. That's harder to predict and even harder to stop.
Starting point is 00:17:57 Listen to the new season of Law and Order Criminal Justice System on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. My boyfriend's professor is way too friendly, and now I'm seriously suspicious. Oh, wait a minute, Sam. Maybe her boyfriend's just looking for extra credit. Well, Dakota, it's back to school week on the OK Storytime podcast, so we'll find out soon. This person writes, my boyfriend has been hanging out with his young professor a lot. He doesn't think it's a problem, but I don't trust her.
Starting point is 00:18:27 Now, he's insisting we get to know each other, but I just want her gone. Now, hold up. Isn't that against school policy? That sounds totally inappropriate. Well, according to this person, this is her boyfriend's former professional. and they're the same age. And it's even more likely that they're cheating. He insists there's nothing between them.
Starting point is 00:18:43 I mean, do you believe him? Well, he's certainly trying to get this person to believe him because he now wants them both to meet. So, do we find out if this person's boyfriend really cheated with his professor or not? To hear the explosive finale, listen to the OK Storytime podcast on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast. I'm Dr. Scott Barry Kaufman, host of the Psychology Podcast. Here's a clip from an upcoming conversation about exploring human.
Starting point is 00:19:07 potential. I was going to schools to try to teach kids these skills and I get eye rolling from teachers or I get students who would be like, it's easier to punch someone in the face. When you think about emotion regulation, like you're not going to choose an adaptive strategy which is more effortful to use unless you think there's a good outcome as a result of it if it's going to be beneficial to you. Because it's easy to say like go you go blank yourself, right? It's easy. It's easy to just drink the extra beer. It's easy to ignore, to suppress, seeing your colleagues, who's bothering you and just, like, walk the other way. Avoidance is easier.
Starting point is 00:19:41 Ignoring is easier. Denial is easier. Drinking is easier. Yelling, screaming is easy. Complex problem solving. Meditating. You know, takes effort. Listen to the psychology podcast on the Iheart radio app,
Starting point is 00:19:56 Apple Podcasts, or wherever you get your podcasts. All right, Daniel, we're talking about the Van Allen radiation belts, which I guess are pretty important to the Earth. And they must be doing some sort of protecting because we talked about them being a planetary defense system, maybe better than lasers. And they form a big charged donut, radioactive donut around the Earth. So I guess the big question is, where do they come from? Yeah, actually, they got stuck in our planetary defense system. We have this awesome planetary defense system, which is basically just our magnetic field. And, you know, the magnetic field is generated by, like, crazy, sloshing, hot, melted metal inside the earth, rotating at, like, different speeds than the Earth does.
Starting point is 00:20:50 And it creates this enormous magnetic field. And then anytime a charged particle comes towards the Earth, the magnetic field does its job and bends it. So the reason that we're not, like, constantly inundated with radiation from space produced from supernovas or from our sun is because of the Earth, the magnetic field does it. is because of the magnetic field. But the radiation belts themselves are basically like particles that got trapped in our magnetic field. Instead of getting like deflected and pinging off somewhere else or funneling up and going to become northern or southern lights, they get trapped around the center and they get stuck basically in orbit around the planet. Interesting forever?
Starting point is 00:21:26 Or do they just sort of like circle around and then shoot off? Well, it's different for the two different stories. The inner radiation belt is much more stable. Those are particles that are sort of like tightly balanced. to the earth and it's really pretty fixed now they don't stay in there forever they can impact the atmosphere they can get knocked out it's a little chaotic but the lifetime inside the radiation belt can be pretty long the outer one though is much more like a free-form cloud it's further away from the earth the magnetic field is weaker it's more controlled by the stuff outside the earth
Starting point is 00:21:55 and like the solar winds so that has sort of a fluffy outer edge and things can come and leave much more quickly but the inner one is much more tightly bound i see it's sort of like bugs trap in your windshield. Like your windshield protects you from the bugs, but when the bugs hit it, they kind of get stuck there. Exactly. Exactly. If the bugs were like orbiting your car
Starting point is 00:22:17 at very, very high speeds, then yeah, it would be a perfect analogy. Well, I guess I mean they get stuck in our sort of protective shell of a magnetic field. Yeah, exactly. The thing that's protecting us gets them stuck on our surface.
Starting point is 00:22:28 Yeah. We need some giant windshield wipers. Actually, we'll talk about that. And there are some really cool ideas for how to reduce the amount of radiation stuck in these belts. Oh. So what are these belts mostly made out of? And what's in them? You might imagine that most of the particles in the belts just come from the sun because
Starting point is 00:22:46 you know the sun pumps out a huge amount of radiation, protons and electrons and a few other things. But interestingly, the stuff in the inner parts of the belt is not mostly from our solar system. A lot of that stuff comes from cosmic rays. And it has to be really high energy to get all the way down. towards the earth. How far down towards the earth depends on how much energy you have because the higher energy particles aren't deflected as much by the magnetic field. So in this inner belt, we mostly have protons that are really high energy that have come from cosmic ray collisions where the cosmic rays have come from like somewhere else deep in the galaxy. Wow. So our magnetic
Starting point is 00:23:24 field is that strong that it can deflect super high energy particles from deep in space that well? It certainly can, not all of them, right? And some of these particles, the really super duper highest energy particles, they definitely make it through the magnetic field and hit the atmosphere and create showers. And that's a whole fascinating area of study that we've talked about where are these cosmic crates coming from. And so we're sort of glad that some of them make it through. But those are really rare, right?
Starting point is 00:23:50 The frequency of the particles drops really quickly as the energy goes up. So the very high energy ones can penetrate through the magnetic field and get to Earth, but there aren't very many of them. The lower energy ones is much more of them, but they're more easily deflected by the magnetic field. So there's a whole spectrum there. So it's electrons and protons. That doesn't sound too harmful, I guess, does it? It's mostly protons in the inner one.
Starting point is 00:24:14 But these protons have a lot of energy. And for example, one of these protons can penetrate like more than a centimeter of lead. And so you definitely do not want to get hit by this shower of protons. Oh, wow. Yeah, protons, I guess, are the ones that can give you cancer. right? I mean, they go in and they mess up your DNA. Yeah, they are tiny bullets and they will tear through your body and mess stuff up and rupt your cells and mess up your DNA. And there's a lot of these things that, you know,
Starting point is 00:24:41 the flux is really intense. You know, it's like millions per square centimeter per second. And the numbers are even higher for electrons. And so it's a really intense amount of radiation. And that's because it just sort of builds up, you know, like cosmic rays just keep coming and keep refreshing it. And so it's a constant source of radiation. You need those windshield wipers up stat. Yeah, there's a lot of bugs out there in space. But I guess what do you compare it to? Is it, I don't know, like a PET scan here on Earth?
Starting point is 00:25:08 Or is it much more intense than that? These are much more dangerous than a PET scan, which is carefully tuned to give you the minimum amount of ionizing radiation necessary. The intensities here are just much, much higher and much more dangerous. But, you know, it's not just protons out there. There are also some electrons. And until recently, nobody really understood, like, are these electrons also coming from cosmic rays or is there some other source of them? People were sort of confused because they
Starting point is 00:25:34 didn't really understand the energy spectrum of the electrons. And so they couldn't really tell where they were coming from. They didn't look like they were coming from the sun. They didn't look like they were coming from the sun. And they didn't really believe that they were coming from cosmic rays. But then there was a really cool experiment done by a bunch of students at UC Boulder. They sent up a tiny little device to measure this radiation. They attached it to one of these little cube sats, you know how they can send up these tiny little satellites with little devices on them. So they built this thing. It's like the size of a burrito and weighs about 10 pounds. And they called it reptile, which stands for relativistic electron and proton telescope
Starting point is 00:26:13 integrated little experiment, which is a pretty cute acronym. And they got some really interesting cutting edge data. So this is like a science experiment done by students at a university to actually learned something about the nature of the radiation around us. Wow. What did they learn? They showed that the energy of these electrons is actually totally consistent with the spectrum you would expect from cosmic rays. So what happens is cosmic rays come in and it hits some particle and you get a bunch of
Starting point is 00:26:40 neutrons flying out. Neutrons don't last forever on their own. They fall apart. They turn into a proton and an electron. So they think that the source of these electrons is actually the same as the source of the protons because the spectrum of the energy of the electrons looks exactly like you would expect from this mechanism from cosmic rays. Now, are these the ones coming from the sun or from some mysterious far away object?
Starting point is 00:27:03 These are not the ones coming from the sun. These are probably coming from supernova and something else far away in our galaxy because they're too high energy to reliably be coming from the sun. So it's sort of awesome because we're like catching these things from supernovas, from other stars deep in our galaxy. We're slurping them up and storing them in our radiation belt. It's sort of awesome. I mean, yes, it's deadly and it's dangerous.
Starting point is 00:27:25 dangerous, but it's also kind of cool and exotic. It's like picking up a shell from a beach. And wondering like where in the planet that shell came from. Yeah, exactly. And so we could have this collection of protons, electrons around the earth, each one from a different place in the galaxy, right? What a cool set of souvenirs. And so that's the inner belt. And is the outer belt sort of the same, just fluffier? Or does it actually have jelly in it? And can you mix it in with your burrito, your reptile burrito? Reptile burritos eating donuts. The outer one is actually, quite different. It's mostly electrons. So the inner one is mostly protons and the outer one is
Starting point is 00:27:59 mostly electrons. Interesting. Now, what would make that different? Why would it be different? Well, the protons have more momentum, right? You can speed up our proton to higher energies because it has more mass for the same charge. It doesn't radiate that energy off as quickly. And so that's why protons tend to penetrate into the inner belt more than electrons do. It's the same reason why we have proton colliders instead of electron colliders. You accelerate electrons to really high speeds. They tend to mostly radiate that energy off by giving off photons. Protons don't do that as much, so it's easier to get them to have a lot of energy. So the outer belt is mostly electrons that couldn't penetrate to the inner belt.
Starting point is 00:28:36 But still coming from the same source, cosmic rays. Well, they don't actually think it comes from cosmic rays because the outer belt actually varies a lot more. So the outer belt, if you watch it, it changes quickly, like on the timescales of days and weeks, it grows, it shrinks, but it changes shape. And you shouldn't see this kind of thing if the source is cosmic rays. Cosmic rays are pretty steady. I mean, you're averaging over a lot of supernovas and a lot of activity from lots of different stars. And so on average, there's, you know, some seasonal
Starting point is 00:29:03 variations, but not on the timescales that we're seeing. So people have been wondering, what is the source of this outer belt? It's not cosmic rays. Is it like, you know, plasma that's floating around the solar system? Is it something else? Is it like, you know, driving through a cloud of bugs kind of? Like, is that, that's what you mean, right? Like, maybe out there in space are there clouds of electrons that we sometimes go through. Yeah, exactly. And so what it looks like is that the
Starting point is 00:29:31 magnetic field is actually tearing atoms apart, atoms of stuff that are just floating out there in the solar system and then yanking the electrons and actually accelerating them. And so the source of most of these electrons is not like interstellar plasma or something else. It's actually neutral atoms that are getting
Starting point is 00:29:47 torn apart to create these protons and electrons and then the electrons get accelerated and turned in. into this outer cloud. Wow. I think I have new respect for magnetic field. It's like out there ripping it up. It's doing a lot.
Starting point is 00:30:01 Yeah, it's doing a lot. And it's also really buffeted by solar storms. So if you have like a lot of activity on the sun, like there's a huge ejection of material or, you know, something happens on the surface of the sun, then you get a huge dump of particles towards the earth. So the solar wind is not constant. It's varying a lot. We call this solar weather.
Starting point is 00:30:20 When there's a lot of activity, you call it a solar storm, which is an awesome. potential title for my science fiction movie and it can really change the shape of this it can wash away part of this outer belt it can contribute to it so this outer belt is much more dynamic it fluctuates a lot more what do you call a sunny day in a solar weather forecast extra sunny bad news toast for toast burnt toast exactly well i guess my one question is so these are particles trapped in our magnetic field does that mean that like the protons are going one way around Earth and all those electrons are going the other way, they go along depending on their charge. Like it'd be cool if, you know, we actually, in that ring of stuff, there's like two masses of
Starting point is 00:31:04 particles going opposite ways. Yeah, you know, I hadn't thought about that before. I think you're right, though, because as you say, magnetic fields bend particles based on their charge, but it bends positive particles and negative particles in the other direction, which is why, for example, at the collider, we actually have two beams. We have a beam of protons going one way and a beam going the other way. they have to have different magnets to bend in opposite directions
Starting point is 00:31:26 and so I think you're right I think the opposite charge would lead them to go the other direction so I think protons are probably circling the earth in the other direction from electrons yeah interesting so it's like a double belt and they can wade to each other
Starting point is 00:31:39 as they pass right every time they race you around the earth hey still trapped here yes me too and then sort of amazingly there's this gap in between them it's not like it's a gradual change from protons to electrons
Starting point is 00:31:52 That's what you might expect, that like higher energy particles penetrate more deeply and you get more protons near the surface and more electrons further away and it's a smooth variation. But no, there's a gap and there's like a shell. Like the inside of this outer belt is like a wall. And then there's almost nothing for a little while between the inner and outer belts. Wow. What do they think is causing this sudden gap? They think it's actually radiation from the earth. If you send photons up out into space, then it basically scatters.
Starting point is 00:32:22 those electrons. It pushes them out further into space. And so the kind of radiation you need, the right energy to bounce those electrons away from the Earth is like at radio waves. And so if you beamed a bunch of radio waves from the Earth, you could like push some of that radiation back out into space. What? Are you saying our TV and radio signals are pushing these electrons out? Yes, they are a little bit. But mostly it's not coming from our broadcast or from this podcast. Mostly it's coming from lightning. When you have lightning in clouds, it generates a lot of photons.
Starting point is 00:32:55 That's what you see. But also generates photons and spectrums you cannot see. It generates a lot of radio waves, which is one reason why electrical storms make it hard to listen to the radio. And so a lot of the reason that there's this inner wall to the outer belt is because of radio waves from lightning pushing those electrons out into space. Wow, that's wild. It's pretty crazy, yeah.
Starting point is 00:33:16 I was going to say maybe now that everything's going digital, we'll see a decrease in the radio signals. But now they were getting more storms due to climate change, we might actually seem more lightning. Oh, man. It's all connected, Daniel. It's all connected, yeah. And so tell me about the third belt.
Starting point is 00:33:35 There's a third belt that is sometimes there and sometimes not. Yeah, so for a long time, people thought there was only two belts. And then NASA sent up these probes in like 2011, 2012. And they found a surprise. They found this third pocket. It's between the first belt and the third belt. right in this safety zone in between them. And people were surprised to see it.
Starting point is 00:33:53 Wait, it's in between the two belts. In between the two belts. Yeah, exactly. So like another layer of jelly, right, inside your cronut or whatever it is that we're building this crazy pastry physical concoction. I think it's a pro nut because it's got protons in it. Electro nuts. And it was right there in between, like in the safe zone where people hadn't seen radiation
Starting point is 00:34:12 before. And that was sort of surprising. And then they were surprised again because it disappeared. And so there's this third belt. It sometimes comes and doesn't last for very long. Is it seasonal or is it random? It's actually seasonal but not based on Earth seasons. It comes from the solar storms.
Starting point is 00:34:29 So sometimes the sun will send like a huge wave of particles towards the earth. And some of them will get like past this lightning belt and past the magnetic field and end up stuck in the safe zone and slosh around for a little while before they get cleared out. Or maybe they join the other belt. Does it all get kind of smooshed at some point? Yeah. Maybe they get slurped down to the lower belt or ejected out to the outer belt. But the name that scientists have for this kind of event when the sun like really pours particles at us is pretty awesome. It's called a space tsunami.
Starting point is 00:35:01 No. What? That sounds like, I don't know, like a Japanese anime maybe or. It sounds like a Japanese anime I definitely want to watch for sure. Space tsunami, meaning like suddenly the sun is acting up and so it sends a huge wave of something. stuff at us. Yeah, exactly. See, it's a perfect name because it immediately describes exactly what he's talking about. I wouldn't go as far as perfect, Daniel. I would maybe call it a solar tsunami. That sounds better. A solar tsunami. All right, yeah, cool. But it's spelled with a T.
Starting point is 00:35:34 It's like T-S-O-L-A-R. Solar tsunami. I like it. All right, so that's where they think this third belt comes from is when the sun is acting up. And so, but what makes the particles get trapped in between, why wouldn't they go to the outer belt? Yeah, I guess it's, you know, some fraction of the particles end up in the inner belt and some of them in the outer belt, but there are also some fraction that can push past this sort of lightning barrier that have more energy than can be sustained in the outer belt and penetrate past that lightning barrier, but don't quite have enough to get to the inner belt. And then, you know, eventually they get cleared. You don't have this constant source of stuff. The reason we don't have a constant third belt in there is
Starting point is 00:36:13 you don't have a constant influx and you do have a process that's clearing them out. All right, well, that's super fascinating. Let's get into why these belts are important or why they point to something important about our magnetic field. First, let's take another quick break. December 29th, 1975, LaGuardia Airport. The holiday rush, parents hauling luggage,
Starting point is 00:36:43 kids gripping their new Christmas toys, Then, at 6.33 p.m., everything changed. There's been a bombing at the TWA terminal. Apparently, the explosion actually impelled metal glass. The injured were being loaded into ambulances. Just a chaotic, chaotic scene. In its wake, a new kind of enemy emerged, and it was here to stay. Terrorism.
Starting point is 00:37:13 Law and order, criminal justice system is, Back. In season two, we're turning our focus to a threat that hides in plain sight. That's harder to predict and even harder to stop. Listen to the new season of Law and Order Criminal Justice System on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. My boyfriend's professor is way too friendly, and now I'm seriously suspicious. Oh, wait a minute, Sam. Maybe her boyfriend's just looking for extra credit. Well, Dakota, it's back to school. week on the OK Story Time podcast, so we'll find out soon. This person writes, my boyfriend has been hanging out with his young professor a lot. He doesn't think it's a problem, but I don't trust her. Now, he's insisting we get to know each other, but I just want her gone.
Starting point is 00:37:58 Now, hold up. Isn't that against school policy? That sounds totally inappropriate. Well, according to this person, this is her boyfriend's former professor, and they're the same age. And it's even more likely that they're cheating. He insists there's nothing between them. I mean, do you believe him? Well, he's certainly trying to get this person to believe him because he now wants them
Starting point is 00:38:15 both the meets. So do we find out if this person's boyfriend really cheated with his professor or not? To hear the explosive finale, listen to the OK Storytime podcast on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast. I'm Dr. Scott Barry Kaufman, host of the psychology podcast. Here's a clip from an upcoming conversation about exploring human potential. I was going to schools to try to teach kids these skills and I get eye rolling from teachers or I get students who would be like, it's easier to punch someone in the face. When you think about emotion regulation, like, you're not going to choose an adaptive strategy, which is more effortful to use unless you think there's a good outcome as a result of it, if it's going to be
Starting point is 00:38:56 beneficial to you. Because it's easy to say, like, go you, go blank yourself, right? It's easy. It's easy to just drink the extra beer. It's easy to ignore, to suppress, seeing a colleague who's bothering you and just, like, walk the other way. Avoidance is easier. Ignoring is easier. Denial is easier. Drinking is easier. Yelling, screaming is easy. Complex problem solving, meditating, you know, takes effort. Listen to the psychology podcast on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. Van Halen radiation belts, although they are pretty, there's a lot of lightning involved here in electricity and decadent lifestyle of donuts.
Starting point is 00:39:47 So I feel like it's sort of a tribute to Eddie Van Halen. I think if Van Halen had been around, the next album would have been called Solar Tsunami. That does sound like a heavy metal album name, yeah. Yeah, and these things are fascinating, not just because, you know, scientifically we're always interested when we see something new because it raises questions, why is this happening, why is it not happening, but also there are lots of practical invocations to these things. Yeah, these belts are important? Like, are they useful to us in any way? Well, they could actually be useful. You know, these are particles zooming around at really high speeds.
Starting point is 00:40:19 And there's not just protons and not just electrons. There are also some antimatter there. You know, some cosmic rays are antimatter. And sometimes collisions of cosmic rays on the Earth's atmosphere create antimatter. And so there is antimatter up there trapped in these fields sort of slurping around. And antimatter is pretty useful stuff. I mean, you could fuel like a matter, anti-matter reactor using antimatter. But it's pretty hard to make antimatter. Wait, these clouds, these belts have anti-matter in them? They do. They have some anti-protons. So their protons swirling around in one direction, but going around the other direction, there's some anti-protons. Don't they hit the regular protons and explode and annihilate? They certainly do. And as intense as
Starting point is 00:41:04 the flux is, you know, it's also pretty dilute. If you shoot one, one proton and another proton, you're not likely to actually get a collision. You have to have like a little cloud of them really smash into each other just to have one or two collisions. Like at the Hajon Collider, we collide bunches of 10 to the 10 protons against each other, sometimes get one, two, five collisions. So it's not that easy actually to shoot a tiny particle at another one. But aren't they opposite charge? So don't they attract each other? They do, but they're also moving at really high speeds. It's like you're driving down the freeway and you see somebody really attractive going the other way,
Starting point is 00:41:36 Maybe you shot your phone number really fast as they go by, but, you know, the chances of actually making a connection are small. I've never tried that dating method, Daniel. Is that how physicists approach their love life? Well, there's a reason you haven't met a lot of people who met their spouse that way, because I don't think it works. They're in the highway. The highway of love. Anyway, there are some antiprotons out there, and antiprotons are not easy to make. Like, we've made some at CERN in order to study, but we have like picograms of antimatter we've
Starting point is 00:42:11 made over years and years and years. But up in these belts is a lot more antimatter than we've ever made here on Earth. So you can imagine like scooping some of it up and using it to fuel your expedition to a neighboring star by pouring it into your anti-matter powered spaceship. Oh, wow. I guess antimatter is sort of like volatile. It's like you can use it as something to burn to give you energy. Yeah, exactly.
Starting point is 00:42:35 you combine it with matter and it turns 100% into energy, into electricity or whatever you need. And that's much more efficient than any other kind of fuel we have. Even like fusion or fission or anything else is not nearly as efficient as antimatter. So antimatter is a great source of fuel. I mean, there's lots of practical questions there about can you bottle it and can you safely store it and will your ship blow up and stuff like this? Yeah, small practical matters. Dot, dot, dot, dot. Like will you die in the process?
Starting point is 00:43:04 I'm sure if we invite our guitarist slash engineer on board, you know, Eddie Van Halen slash Van Allen will figure this out for us. All right. So it's something that NASA is actually considering, like going out there and catching some of these shooting stars or shooting Antrimet. Yeah, but, you know, considering is pretty broad. NASA considers a lot of stuff because that's sort of their job
Starting point is 00:43:26 to think broadly and crazily. They have this group called the NASA Institute for Advanced Concepts, which, you know, makes me think of just like people, literally throwing stuff against the wall to see if it'll stick. And that's great. And I love that kind of like blue sky brainstorming to see
Starting point is 00:43:41 maybe this could be a good thing. Mostly though, it's dangerous. Like mostly the radiation belts are a big annoyance. When we send astronauts up into space or even just satellites up into space, we're sending them through these radiation belts and it can be quite deadly.
Starting point is 00:43:55 Yeah. Are they like more dangerous than regular cosmic race? Or do you consider them cosmic rays? Because I know we've talked about like astronauts and space stations needing shielding and sunblock on them to keep them safe. Is this all part of, you know, just like the regular thing you have to watch out for in space? Or does it only come up in certain situations?
Starting point is 00:44:16 You definitely have to watch out for cosmic rays whenever you're in space because you don't have the protection of the Earth's atmosphere or our magnetic field. But this is a spot with really intense radiation to one of the most dangerous places in space. So you have to be really careful when you go through it. You know, there are billions of electrons per square center. meter per second flying through these clouds. And these protons are really high energy. Like I said, they can penetrate even like a centimeter of lead.
Starting point is 00:44:43 And so this is pretty crazy stuff. So you don't want to spend a lot of time in these belts. I see. Now, do our like space shuttle and space stations kind of watch out to try to stay clear of these radiation belts or are they always in them? No, they try to stay clear of them. There's this safe zone and you try to go above them and below them. And so you definitely don't want to spend a lot of time hanging out in these radiation
Starting point is 00:45:03 belt. You want to avoid that, you know, if you care about the life cycle of your astronauts, which we do, but also for your satellites. If you don't want jelly all over your space station. Also for your satellites, right, these can damage delicate electronics. And so you don't want a really high flux of protons tearing through your delicate electronics or your solar panels for any reason, even if there's nobody living on your space station or on your satellite. Yeah, you were saying that they also interfere with our wireless communications here on Earth. Absolutely. Yeah, I mean, it's a huge source of radiation. And so when there's like a solar storm and these things get bigger and more dramatic, then there's particles bouncing around everywhere. And some of our wireless communication strategy rely on bouncing off the top of the atmosphere, right? Like sending radio waves up and having them bounce back. And so this can be interfered with when there's a lot of extra activity in the Van Allen radiation belts. Sounds like a little bit of a nuisance actually, sort of like a byproduct of protecting ourselves, sort of like the bugs in the windshield.
Starting point is 00:46:03 Could we wipe them off the windshield at some point? Wouldn't that make things safer in space? Yeah, and people are working on this stuff and these two totally crazy sounding ideas for how to like cleanse the planet of these things. Giant wipers. Giant wipers. One of them literally is giant wipers.
Starting point is 00:46:21 And so what they're going to do is they're going to send something up. It's called the high volt system. And you have a satellite which is like a really long wire behind it and the wires held at really high voltage. And so basically just... What? It is a wiper. It's literally a space wiper. It's the kind of thing you would see in space balls.
Starting point is 00:46:38 But it would like fly around the planet with this high voltage tether. And that would be strong enough to just like kick these particles out of their geomagnetic orbit. And then they would just drift off into space. And they estimate that just like fly this thing around for a couple months, a few months of wiping. And you've reduced the radiation belts by 99%. No way. What? That is a pretty sensitive.
Starting point is 00:47:03 sensible idea, actually, to be honest. Just wipe them off. Yeah, just repel them. It's like you're repelling them kind of, right? Yeah, you're repelling them exactly. It sounds a little crazy. I mean, you have this really long tether, really high voltage. It could fry like, you know, a person or a satellite. But, you know,
Starting point is 00:47:19 if you think about where you're going and where all the other satellites are and manage all that, then I suppose it could work. Wow. Now, would that help us if we got rid of these radiation belts? Would it make life easier for everyone in general? Yeah, it would reduce danger to satellites and two astronauts and that kind of stuff.
Starting point is 00:47:36 They have another system that's not quite as bonkers, maybe not as fun. And that's just to beam a bunch of radio waves out into space. We talked about how radio waves from lightning help keep the radiation belts from getting closer to the earth and they create this safe zone. So if you just pumped up the radio waves that we were broadcasting, you could help penetrate these radiation belts and cleanse them. You could like puncture them, create a leak and some of them would flow out. Wait, wait, wait.
Starting point is 00:48:02 So radio waves are light, right? Yeah, radio waves are light. So you're saying we can shoot lasers at them. Radio lasers, yeah. Or we could just, you know, broadcast this podcast in laser form up out into space. Oh, wow. Our voices right now could be helping to cleanse, give the earth a little bit of a cleanse. Shoot, electrons, shoot, get out of here.
Starting point is 00:48:24 Get out of here. Yeah. Here, this part will be especially efficient. Nice job. But there are people up there in Alaska building these things and exploring this to see can we pump enough radio waves
Starting point is 00:48:39 out past the earth to help actually push away some of this radiation. There's a real thing people are actually doing right now. I wonder if there's some like, did these belts accumulate over time or is it pretty stable
Starting point is 00:48:52 right now? Because I wonder if like it might get worse. It might get worse. You know, we've been studying with them for about 60 years since they were discovered, but only in the last 10 years So we have really a lot of specific data.
Starting point is 00:49:03 They're just sort of mysterious for decades and decades. And in the last 10 years, we've been sending up satellites to get better pictures of what's out there and how it's changing. And that's when, for example, we learned that there is this third belt. And so it's kind of new to have like a detailed concrete map of these radiation belts. So we don't have a lot of depth of our time information. We think the inner belt is pretty stable and the outer one is a bit more fuzzy. But it could be that there are longer cycles we're unaware of. Do you think it's helping or do you think it's maybe killing our magnetic field on Earth?
Starting point is 00:49:36 Because that could be a problem. That would be a problem. But I think our magnetic field is pretty robust. I mean, it's generated inside the Earth. And so I don't think there's any danger that these particles are going to use it up or damage it in any way. But, you know, our magnetic field actually does have a weakness to it. What? Like an Achilles heel or kryptonite weakness?
Starting point is 00:49:56 Yeah, just like that. no it's much more like an Achilles heel because you know that the earth spins of course but that the earth's magnetic axis doesn't exactly match the rotational axis right like the physical north pole around which the earth spins is not in the same place as the magnetic north pole right it's a little skewed it's a little tilted it's a little skewed yeah but there's another shift which is important which is that the center at the magnetic field like if you drew a line through the magnetic north and south poles,
Starting point is 00:50:28 that doesn't line up with the center of the earth that's shifted a little bit. Oh, so and that creates a hole in the magnetic field? It means that in some places on the surface of the earth, the magnetic field is weaker
Starting point is 00:50:39 than other places. Like if you're on the spot on the earth where the center of the magnetic field is on the other side of the center of the earth, then you're further from the source of the magnetic field, and so the magnetic field is weaker.
Starting point is 00:50:51 So on one side of the earth, the magnetic field is a little bit stronger And on the other side, it's a little bit weaker. And where it's weaker, these radiation belts dip down closer to the surface of the Earth. Because they're not as repelled. Yeah, because they're not as repelled. And so this is called the South Atlantic anomaly because there's basically like a hole in the magnetic field. It's not technically a hole.
Starting point is 00:51:12 It's more like a weakness over the South Atlantic. It's over the ocean. But it extends out to, you know, like Argentina and Brazil. And that's where the magnetic field is a little bit weaker. And these radiation belts come the closest to the earth. Oh, and it turns with the Earth too, right? Because I guess our magnetic field turns with the Earth. Yeah, it turns with the Earth.
Starting point is 00:51:31 And it has a real effect. You know, like, I used to do science with this Fermi telescope that would take pictures of the center of the galaxy and look for dark matter. But anytime it passed anywhere near the South Atlantic anomaly, it just saw craziness. Like, you just couldn't do any science. It was just like bathed in radiation. And so we had like special parts of our code. We're like, are you near Brazil? If so, you know, throw away the data.
Starting point is 00:51:52 Wow. Turn on the windshield wiper. Exactly. exactly because you are hitting a lot of bugs wow pretty interesting so it sort of sounds like the byproduct of staying safe in space you know it's just all the stuff we collect as we go through or the solar system
Starting point is 00:52:08 yeah absolutely we would much prefer to have these radiation belts orbiting our earth than have that radiation deposited on the earth right as you say it's better to have the bugs on the windshield than in your teeth but it'd be nice to turn those wipers on occasionally and sort of cleanse ourselves because it's right there and it's zooming around and it's high flux
Starting point is 00:52:26 and it's quite deadly. Or not the windshield weapons would maybe collect them in a way like you said. It might be possible to collect them and use them for something good. Yeah, it would be pretty awesome if we were creating antimatter
Starting point is 00:52:38 with the earth and collecting it and using it to travel to other stars that would be pretty cool. Or even power things here on Earth. Like could we have anti-matter solar panels in space?
Starting point is 00:52:50 And then you transmit the charge through a giant wire to Earth which also... Healthy windshield wipe your debris. I want to see this movie for sure. And I want to eat donuts while doing heavy metal radiation karate chops while we're doing it. There you go. You can do it all, Daniel.
Starting point is 00:53:08 All right. Well, it's again just an interesting lesson just about all the things that are out there in space that we can't see but are there. And they're doing some amazing physics in the process and telling us a lot about our sun and about what's in space. That's right, and it reminds you that there's a lot of accessible mysteries right here on Earth. There are amazing things happening in black holes and supernovas really far away, but there are still a lot of things we have left to figure out about the way the universe works and what's going on in our very own neighborhood. Yeah, so think about it next time you look up up into the sky at night or even during the day.
Starting point is 00:53:45 There's, that there are giant donuts in the sky. Just don't take a bite. Thanks for listening and remember that Daniel and Jorge Explain the Universe is a production of IHeartRadio. For more podcasts from IHeartRadio, visit the IHeartRadio app, Apple Podcasts, or wherever you listen to your favorite shows. December 29th, 1975, LaGuardia Airport. The holiday rush, parents hauling luggage, kids gripping their new Christmas toys. Then, everything changed. There's been a bombing at the TWA terminal, just a chaotic, chaotic scene.
Starting point is 00:54:43 In its wake, a new kind of enemy emerged, terrorism. Listen to the new season of Law and Order Criminal Justice System on the IHeart Radio app, Apple Podcast. or wherever you get your podcasts. In sitcoms, when someone has a problem, they just blurt it out and move on. Well, I lost my job and my parakeet is missing. How is your day? But the real world is different. Managing life's challenges can be overwhelming.
Starting point is 00:55:14 So, what do we do? We get support. The Huntsman Mental Health Institute and the Ad Council have mental health resources available for you at loveyourmindtay.org. That's loveyourmindtay.org. See how much further you can go when you take care of your mental health. Tune in to All the Smoke Podcast, where Matt and Stacks sit down with former first lady, Michelle Obama. Folks find it hard to hate up close. And when you get to know people, you're sitting in their kitchen tables, and they're talking like we're talking.
Starting point is 00:55:44 You know, you hear our story, how we grew up, how I grew up, and you get a chance for people to unpack and get beyond race. All the Smoke featuring Michelle Obama. To hear this podcast and more, open your free iHeart radio app, search all the smoke and listen now. This is an iHeart podcast.

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