Daniel and Kelly’s Extraordinary Universe - Listener Questions #45

Episode Date: July 23, 2026

Daniel and Kelly wonder how many Extraordinaries are planning on becoming supervillains as they discuss how to make Jupiter explode, the changing colors of children's hair, and whether or not aliens c...ould discover electromagnetism without iron.See omnystudio.com/listener for privacy information.

Transcript
Discussion (0)
Starting point is 00:00:00 This is an I-Hard podcast. Guaranteed human. Get Bell Pure Fiber Internet with Crave, Netflix, and Disney Plus from $94 a month. Price guaranteed for two years on Internet with a two-year term and auto pay credit. Visit bell.ca for details and to check availability. Bell, connection is everything. Hey, Portlandia fans. Carrie Brownstein and Fred Armisen here.
Starting point is 00:00:23 The Dream of the 90s is alive in podcast form. We're launching Podlandia, A.O. rewatch, our brand new podcast, where we, We revisit every episode of Portlandia together, breaking down sketches, going deep on our iconic characters, and pulling back the curtain on how it all got made. And we'll also be joined by the people who helped bring it all to life. Guestrars, collaborators, and friends, including director Jonathan Chrysall, the mayor himself, Kyle McLaughlin, legendary musician Amy Mann, and many more. Kyle is going for it here. You fully improvised, not just words, but a song. Well, I thought you were all going to write a song.
Starting point is 00:00:56 I remember you thinking that. Listen to Podlandia, AEO rewatch on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. I'm Nick Titoro. You probably know me from NYPD Blue, The Longest Yard, or Spike Least Black Klansman. And on my new podcast, delivering happiness with Nick Titoro, I deliver pizza to a new guest. I've shared a slice with everyone from Seth Rollins. What are you doing? My belt.
Starting point is 00:01:22 To Bill Burr. I don't think I've ever met somebody so exactly out of their mind as I am. And now we even have more great guests coming up, including the great John Tituro. It's called Happiness. Delivering Happiness. And many, many more. Open your free High Heart Radio app. Search Delivering Happiness with Nick Titoro.
Starting point is 00:01:40 And listen now. This is Chelsea Handler from Dear Chelsea. Every week, the news gets worse. The world gets crazier. And Yamanika is here to tell whoever's responsible, you're the problem. Do you know I just found out who Sidney Sweeney was? If he got a bunch of women, then I should have a bunch of men. Do better or do less so I don't have to do so much.
Starting point is 00:02:01 I'm Yamanika and I'm out. Listen to You're the Problem with Yamanika on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast. How would a supervillain get Jupiter to blow? Not that anyone wants to, but would it make a great show? Norwegian kids are often born blonde but end up brunette. Why? Did this help our Viking ancestors fend off some threat? Imagine aliens on a planet without iron to find. Could they still discover magnets and send us messages from their alien minds?
Starting point is 00:02:45 Ooh, whatever questions keep you up at night. Daniel and Kelly's answers will make it right. Welcome to listener questions number 45 on Daniel and Kelly's extraordinary universe. With I study parasites and space and I am getting a little bit concerned at all of the questions we get from our listeners that suggest They're researching how to become supervillains. Hi, I'm Daniel. I'm a particle physicist who loves thinking about aliens, and I'm happy to grow the supervillain demographic in our audience.
Starting point is 00:03:32 And you are. And so, Daniel, give them something to work with. If you were going to be a supervillain, what would you do with your physics or cosmology knowledge to do the most super villainy thing you can think of? I think I've advertised this on the show already. I would gamble or trade away the entire Earth to super intelligent aliens if they could offer us some insight into the deepest questions of the universe. Oh, that's super villainy for sure.
Starting point is 00:04:01 And we all knew that you valued the aliens you've never met much more than every human on this planet. But I'm talking about, like, you know, would you push Jupiter into the Earth or you just, you have very tunnel vision on this alien thing? Wow, you really want me to be a super villain here, huh? I mean, I'm giving the people what they want. I would similarly encourage people to do experiments here on Earth that might even risk the planet. What? Like, when we turned down the Large Hageon Collider, there was a big brouhaha about, is it going to make black holes that gobble up the Earth? And no, the answer is it's not going to.
Starting point is 00:04:36 There are higher energy collisions happening all the time in the atmosphere anyway that are not destroying the Earth. But in my view, actually, I didn't really care. What? Even if it was going to risk the Earth and maybe create a black hole to gobble everything. everything, I was like, let's do it. Because that would be fascinating. This, you know what? I shouldn't ask you these questions because I'm always disappointed afterwards.
Starting point is 00:04:57 I tried to squirrel away from it. Okay, let's move on. Let's go ahead and hear Kenny's question about Jupiter. Kenny is today's supervillain listener. Hi, Daniel. We were talking about Jupiter and then we thought of something a bit scary. Jupiter is the main most of Ivy so it could explode
Starting point is 00:05:19 What if evil space They leans A rad of a planet He destroys a solar system Watch for they done to Huge amounts of oxygen onto the use to make a giant Explosite
Starting point is 00:05:33 Or wistly swat in loads of bananas and dark Chocolate making Jupiter heavy and heavier into its own into a star Watch what happens to Earth Why the earth get blasted apart? But what happened instantly?
Starting point is 00:05:49 Or what do you come to terrifying you staring at? That stayed there for a really long time. Wow, Kenny. What are you planning, man? Well, Kenny does really seem like he's got big plans. And fortunately, we're not going to suggest anything that's of any practical use to him. Okay, that's good. That's good.
Starting point is 00:06:19 Essentially, there are two ways for Kenny's dreams to become reality, via physics or via chemistry. I don't see any biological way to destroy Jupiter, so we're limited to those two basic sciences. I feel like this is one of the reasons why biology is great. But all right, go on. All right. So let's talk about destroying Jupiter via physics. What that means, essentially, is fusion. This is what's already happening at the core of stars.
Starting point is 00:06:45 You have a huge ball of gas, mostly hydrogen. It gets compressed due to gravity that increases the temperature and the pressure. And eventually, you have such high temperature and pressure that fusion goes from essentially impossible, never, never happens to very rarely happens, but happens often enough to release enough heat to increase the chances of fusion or to at least maintain it. So the thing to understand here is that fusion is very sensitive in a nonlinear way to pressure and temperature. You double the pressure and temperature. The rates of fusion don't go up by two. they go by more than two. It's non-linear. And so really big stars, for example, have a lot of gravity. They get really hot. Fusion goes really fast and big stars burn themselves really quickly.
Starting point is 00:07:29 Small stars have less pressure and temperature. Fusion at their heart goes very slowly. They can last for billions and billions, maybe even trillions of years. So the amount of stuff you have determines the pressure and temperature, which determines how much fusion is happening. But I feel like fizzling out is very different than exploding, which is what Kenny's, are we going to get to the explosions is what I'm wondering, Daniel? When do the explosions happen? You want some more kabooms? I mean, if the star is big enough and hot enough, then it will blow itself apart.
Starting point is 00:08:06 Okay. Like if you try to make a star that's more than 300 times the mass of the sun, you just can't do it because it's so big, it gets so hot, the fusion is so powerful that it blows itself apart. And you end up with a star of mass around 300 times the mass of the sun. Now we're talking. Because most stars are a balance between gravity and the fusion pressure, the energy that's being released by that fusion. And so when it gets too big, then gravity makes it too hot, then the pressure and temperature
Starting point is 00:08:34 get cranked up, and then fusion wins. So in order to make Jupiter really blow, you'd need it to be 300 times the mass. mass of the sun. And currently, it's about one one thousandths of the mass of the sun. Really? And so you look confused. No, I'm not confused. I'm surprised. I guess I'd assume Jupiter had a lot more mass, but the sun is that much more massy, huh? Oh yeah. I mean, the solar system is basically the sun. Everything else is a crumb. We have a totally distorted view of the solar system because we live on a planet, so we think it's really important. It's like if you live in a tiny town outside New York City, and you think that it should also appear on a map when really it's just New York City,
Starting point is 00:09:15 you know, we're basically irrelevant. We're irrelevant compared to Jupiter. Jupiter is basically irrelevant compared to the Sun. So we're irrelevant squared. Oh, no. Yeah. So what this means is that Kenny has a lot of work to do. There's a few thresholds here.
Starting point is 00:09:28 Like, what would it take to get fusion happen at all in Jupiter? People sometimes imagine this is like an on-off switch. There is fusion happening within Jupiter. It's just very rarely and not enough to do anything. interesting. For fusion to get like hot enough so you start to increase the temperature of Jupiter further to be ignition, it need to be about 80 times its current mass. It's like the minimum size for a star to really glow. They would become like a really dim red dwarf. So not a boom, an explosion, just like a very, very gentle star. As you add mass, it gets brighter and brighter.
Starting point is 00:10:04 You get up to the mass of the sun, which is a slightly above average star. And then you could keep going to get up to the most massive stars in the universe. But it would take an enormous amount of mass. Like there isn't enough mass in the solar system, obviously, to make another star that's 300 times the mass of the sun. You'd need to, like, gather 300 neighboring solar systems and squeeze all of their mass into Jupiter, then you get a really awesome explosion. You better be a very motivated supervillain. That's a lot of work. More realistically, if he gets enough bananas and dark chocolate, like siphons off some mass from the Sun and dumps it into Jupiter, he could get Jupiter to ignite into a star if he cranks up its
Starting point is 00:10:43 mass by a factor of 80. So we're talking 80 Jupiters squeeze together, right? Then you're going to get a very dim red dwarf. That would warm Earth a little bit. Like Jupiter is kind of far away. It's much further from Earth than the sun is. And a red dwarf would be much, much dimmer. But it would have some impact on the Earth. It would also affect the Earth's orbit. Earth's orbit is not just determined by the Sun. Jupiter does play a role. There's a the reason we have like ice ages and all sorts of long-term cycles because Earth is getting tweaked by the other planets. It's a little bit of a chaotic system. These are called Malankovic cycles. And so if Jupiter becomes 80 times its mass, that's going to get more dramatic.
Starting point is 00:11:23 All right. Do we have anything that's more boomy, though, that we could give him as an answer? Is there something else we could do? Chemistry is definitely more boomy than physics in this scenario. I mean, physics and fusion is behind like, you know, atomic bombs. fusion bomb. So that's pretty dramatic, but it's hard to get that kind of density. But you could also do it with chemistry, right? Like, you know, hydrogen famously burns. But what is burning? Burning is a chemical reaction. It's combustion. You take something like hydrogen and oxygen, and you add a spark, and then you get water and energy. Famously, the Hindenburg is hydrogen burning, right? This is why we don't fill in massive tanks with hydrogen anymore because hydrogen and oxygen combust,
Starting point is 00:12:08 oh, the humanity. It's a little surprising we thought it was a good idea initially, but we don't do it anymore. And if you are on a massive hydrogen-filled balloon, don't go out onto the smoking deck. It's not a good idea. No, no, actually, don't smoke. Yes, don't smoke at all for lots of good reasons. Biologists' recommendation. And something I very rarely say is that this little bit of chemistry,
Starting point is 00:12:32 is actually kind of interesting. Because you see oxygen a lot. It's around all the time. You see it in combustion. You see it in lots of reactions. It's also important in biochemistry, right? Oxygen is an electron acceptor. It's important for metabolism.
Starting point is 00:12:47 We breathe in oxygen via our lungs because we need it. And it's all for the same reason, is that oxygen has openings for electrons in a fairly low energy state. And so what you're trying to do in all of these reactions is release energy. And so for that to happen, you need to take something at a high energy level and get it to a lower energy level. So when biochemists talk about electronic sceptors, what they mean is basically there's a valley here.
Starting point is 00:13:13 So if you have rocks on the tops of hills, you can roll them down into this valley and then you can gather that energy. If you have rocks on the top of hills, but it's just hills and there's no valleys, there's nowhere for that energy to go. And so you need valleys. And oxygen is basically a valley, which is a way to release energy. All right. So let's say that Kenny wants to blow up Jupiter with chemistry. How much oxygen does he need? Well, a lot.
Starting point is 00:13:39 Jupiter is about 10 to the 27 kilograms. About 75% of that is hydrogen. So call that like 1 times 10 to 27 kilograms. Oxygen is much more massive than hydrogen. Remember that hydrogen is atomic element number one. It's just a proton. Oxygen is eight protons, right? So it's eight times more mass.
Starting point is 00:14:02 So if you want to do the chemical reaction of like H2 plus O2, then four grams of hydrogen means 32 grams of oxygen. So eight times as much. So you want to blow up all of Jupiter, you're going to need like six times the mass of Jupiter in oxygen to make that combustion happen. We're talking 1,800 times the mass of the Earth, all in oxygen, which you've got to find somewhere,
Starting point is 00:14:29 Kenny. Yeah. So this is a very common misconception about supervillains. They're not just lazy misanthropes. You got to work hard to be a supervillain. And you got to have connects. Do you have an oxygen guy, Kenny? Because you're going to need one. That's right. Networking is critical, Kenny. Exactly. Get on LinkedIn. Exactly. And you can't just mix hydrogen and oxygen, right? Because though this reaction is energetically favorable, like it does release energy, there's an activation barrier here. So you're not just like at the top. of a hill rolling down the rock, you're in a little valley at the top of the hill, and you've got to get over the edge of the volcano and then down into the valley.
Starting point is 00:15:09 So that's why you need a spark. You just mix hydrogen oxygen. You don't get the reaction. You need to light a match, and that initial energy gets it going. And then the heat released by the combustion gets it going. That's what we call ignition. Now, that's not a problem in Jupiter. You don't need a match, can you?
Starting point is 00:15:25 Because the core of Jupiter is already very, very hot. The challenge here is mixing. You need enough oxygen mixing with hydrogen in an even way, and oxygen is heavier than helium. So if you just dump it into Jupiter from your spaceship, it's going to all sink to the core. You're not going to get like a smooth combustion. So probably what you're going to get is like a series of planet-wide explosions rather than like a single boom. There's going to be turbulence in the combination. You're going to get like atmospheric detonation fronts.
Starting point is 00:15:57 A lot of the heat is going to get reabsorption. just heating up the gas and expanding it. So you're going to get huge plasma shells. We actually got to see in history a bunch of cool explosions in the atmosphere of Jupiter when a comet struck Jupiter in 1994. And we saw massive fireballs bigger than the Earth, which was really awesome. And you got to watch! I remember this story.
Starting point is 00:16:22 I did get to watch it. Yeah, it was a cool summer for me. Yeah. And this would release a huge amount of energy. You know, it would release probably like 10 to the 8 joules per kilogram. That's a lot of energy. Probably two times 10 to 35 joules in total. That's like 10 to the 18.
Starting point is 00:16:42 It's like a quintillion sar bombas. Wow. Right? Or like 16 times the annual solar output all in one explosion. Holy cow. So it would be dramatic. We would definitely see it here on Earth. We would probably get sunburns.
Starting point is 00:16:57 It might fry us. But I think there's some technical challenges there that I doubt Kenny's going to overcome, so I'm not shy to give him all this advice. You don't know, Kenny, man. Kenny might be a real go-getter. This could be the beginning of Kenny's story. Let's find out. That's right.
Starting point is 00:17:13 And Kenny, if you have any follow-up questions for Daniel, let us know. Thank you for watching my question on your podcast. I look at the atmospheric designated foot on the next weather forecast. Get Bell Pure Fiber Internet with Crave, Netflix, and Disney Plus from $94 a month. Price guaranteed for two years on internet with a two-year term and auto pay credit. Visit bell.ca for details and to check availability. Bell, connection is everything. What's up, fam? I'm sports journalist Ari Chambers.
Starting point is 00:17:53 Hey, what's up, y'all? It's your girl, Sam J. And we're the host of Everyone Watches Women's Sports, a new podcast from Together and I Heart Women's Sports. Because let's be real. Women's sports is giving us way too much to talk about these days. So Kelsey Finler, she became the first female solo roer to go from California to Hawaii. My first thought is like, what's up with the snacks? Like, what are we eating?
Starting point is 00:18:15 The highlights, the rivalries, the breakout stars, the moments to take over your entire timeline. And the conversations that start during the game and somehow keep going all week. Every week, we're breaking down the biggest stories across women's sports. Naomi Osaka, showing us. She beat. Sabalinka. Shout out to you, Naomi. You get the palm, Naomi.
Starting point is 00:18:34 You get the palm for that. Because we're not just interested in what happened. We're interested in why everyone's talking about it. Because everyone watches women's sports. Listen to everyone watches women's sports. On the Iheart radio app. Apple Podcast or wherever you get your podcast. Hey, Portlandia fans.
Starting point is 00:18:52 Carrie Brownstein and Fred Armisen here. You know us or rather you know them. Tony and Candice, Nina and Lance, Spike and yes, the chicken. We've played a lot of iconic characters over of years, but today we're showing up as ourselves to tell you about Podlandia, AEO rewatch, our brand new podcast. Each week, we'll revisit an episode of Portlandia from the very beginning, breaking down the
Starting point is 00:19:13 sketches, exploring the backstories of our most iconic characters, revisiting the Portland locations you know and love, and opening up about our creative process. How did any of this get made? Why do we think that was a good idea? We're ready to talk about it. And we'll also be joined by the people who helped bring it all to life, guest stars, collaborators and friends, including director Jonathan Chrysall, the mayor himself, Kyle McLaughlin,
Starting point is 00:19:36 legendary musician Amy Mann, and many more. Kyle is going for it here. You fully improvised, not just words, but a song, a melody. Well, I thought he was going to write. I thought you were all going to write a song. I remember you thinking that. Listen to Podlandia. Ayo rewatch on the IHeart Radio app,
Starting point is 00:19:54 Apple Podcasts, or wherever you get your podcasts. My first guest is Parix Hotel. Shakira, Luke and Yerin, Samira, and Gracie. I'm so excited for it. You have surprises, many surprises. Welcome to Sweet 305 where the group chat comes to life. What a f***. It's like a way to say like,
Starting point is 00:20:20 Oh, my friend, oh, my friend, hello, Hello, my brother. Look, I never have to be able to be nobody. Except with my kids, my children, my mom. Uff. Uf.
Starting point is 00:20:33 That's incredible, yeah, the telenovela. Novela. You're the only person I know that loves a yellow starburst. It's lemonade. There's no one that you'd like to collaborate with this person. This is Sweet 305. Listen to Sweet 305 with Lele Pons as part of my Culturea Podcast Network on the IHard Radio app, Apple Podcasts, or wherever you get your podcasts. Okay, we're back.
Starting point is 00:21:10 We're transitioning from answering questions from potential super villains to helping people understand their children's hands. Which is a tough question. And so, all right, we are going to hear two questions from listeners because I got a very similar question from two different folks. And so let's hear Mark and Ephraim's questions about what the heck is going on with their kids' heads. Hi, Daniel and Kelly. This is Ephraim from Arlington, Massachusetts.
Starting point is 00:21:36 I just listened to the discussion of gray hair and listener questions number 29, which totally overturned what I previously read about how gray hair works. Kelly's mention of hair follicle. with lasting four to six years, made me wonder if this same turnover in the follicle population relates to how some children's hair color changes. I was blonde as a very young child up to about age five and brown-haired ever since, well, except for the red in my beard, which has now gone gray. My number one son did roughly the same thing, though his blonde hair lasted perhaps a year longer than mine had. Hello, Kelly and Dan. In my little Norwegian
Starting point is 00:22:17 town in southern Wisconsin, we have all these little children who start out with whitish blonde hair, including my kids, who by the time they are in high school at brown hair, does this have to do with the six-year cycle of a hair follicle? What evolutionary advantage would changing hair color have had in Hunter-gatherer Scandinavia? Thank you. Mark. Can I start with a funny story about my son's hair color? Oh, yes. Tell us. What is your son's hair color and why is it hilarious? Well, okay, So he was originally born with really dark hair, like the color of mine before I started going gray. And then he started losing it from the top of his head first. And so he had like a bald patch on the top of his head.
Starting point is 00:23:00 And he was the chunkiest baby ever. He had like more rolls on his thighs than I've ever seen a baby have, which was absolutely adorable. But anyway, he had a definite Danny DeVito stage, which I thought was so cute. Every time I looked at him, I would chuckle and think about Danny DeVito. Is Danny DeVito like the epitome of cute, though? I mean, no, but my son was. And so sometimes as a mom, you hold very, you know, discordant ideas in your head, and it's fine. Because, you know, I will admit that when I see babies, some of them are very cute.
Starting point is 00:23:37 Not every baby is cute. And I feel like people think it's weird to say that, but it's true. Like, some babies look like Richard Nixon, you know, or Churchill. And that's not cute. I 100% agree. Some babies are not cute. I'll go on the record with you there. This is going to be the last episode people listen to of our podcast.
Starting point is 00:23:55 But I'm sure your little Danny DeVito was very cute. It was so cute. And anyway, he ended up being a, you know, blonde hair, blue-eyed cutie. And he would have been cute if he had still had dark hair too. But anyway, how does our hair end up one color or another? So maybe that's a good place to start. Yeah. And the answer is, it's complicated.
Starting point is 00:24:15 And I feel like when we were in elementary school, we were told that this was something that was pretty easy to figure out. Like if you have two brown-headed parents, you're probably going to have a brown-headed kid. And I guess I got the sense when I was younger that this was like a dominant recessive, easy trait to figure out. Researching it, that absolutely does not seem to be the case. There's like 100 genes or something that contribute to the color of your hair.
Starting point is 00:24:39 One of the more important ones is a receptor whose name I won't say so that I don't have to hear it from Daniel, but it's a receptor. Look at that. I've trained you. I don't even need to be here anymore. You've learned. Arf, wharf.
Starting point is 00:24:52 Anyway, so. But I have to say, I've done this experiment myself. Oh. Because I have dark hair and dark eyes, and my wife, with her Danish Irish heritage, has blonde hair and light-colored eyes and light-skinned. And both of my kids have light-colored hair and light-colored eyes. And, you know, the simple understanding of biology
Starting point is 00:25:13 She's like, my traits are dominant, and hers are excessive, and yet hers won out. Well. So it must be more complicated. Or she cloned herself in the lab. I mean, I wouldn't put it past her. She's a very smart biologist. But, yes, these things are complicated. And so the thing that gives your hair color is a pigment that we have two versions of.
Starting point is 00:25:33 We have a version that gives you, like, black and brown colors and a version that gives you sort of blonde, reddish sorts of colors. And we have receptors. in our hair follicles and the cells that are important for making hair color. And those receptors essentially, they'll get bound by a hormone. And if they get bound by a hormone, they're like, bam, I'm making more black, for example. Okay. And so it's all about like what receptors you have and the hormone messages that are being sent to those receptors.
Starting point is 00:26:03 So I think this is fascinating because it's more complex than people usually imagine where, like, you have things encoded in your genes that your body does. Instead, you have things encoded in your genes that your body can do, and whether it does them, depends on whether it gets messages like, okay, now do this. Yes. Like you have this library of capacities and only some things actually get turned on. That's fascinating.
Starting point is 00:26:25 Yeah, right. And so my understanding is that part of the story about why hair color can change when kiddos are very young is that when you are in your mom, you're getting bathed in her hormones. So the receptors in your body are getting messages that your body's not producing, but your mom's body is. And so that can influence your hair color. And I wish you all had just seen Kelly's little dance she did when she said, you're in your mom. I mean, it's probably a great place to be.
Starting point is 00:26:55 You're like getting all cozy there. You're like, hmm. I mean, I personally was a baby who stayed in the womb for an extra couple weeks until they eventually had to kick me out. And so, you know, I imagine it's a lovely place in there. Much easier than real life. But anyway, so partly when you're very young, you're getting exposed to the hormones that your mom makes. But then as you get older, you start making your own hormones and you start making more of your own hormones or different kinds of hormones. And so the messages that your hair receptors are getting change over time. Okay.
Starting point is 00:27:32 And that explains why your hair can go from being one color when you're young to another color when you're older. And it's apparently very common for, light-haired kids to end up having darker hair. And part of that has to do with like hormones during puberty. You start, you know, making more hormones. Those hormones are also talking to your hair receptors. But your hair doesn't change color overnight because of something that we talked about in listener questions episode number 25.
Starting point is 00:28:01 And this is the episode that was being referred to by the listeners, where they were, we were talking about why you sometimes go gray after a very stressful event. Oh, I see. And so this is the hair cycle. And the idea here is that each follicle on your head has a cycle where for something like four to six years, your hair is growing continuously. Did you just say wherefore, as in, you know, like colonial times transition sentences? Did I? I don't know.
Starting point is 00:28:30 I'm trying to think about what I'm going to say next. And so I've already forgotten what I said. How to for hair, herewith. Much ado about hair today. There you go. Anyway. So it takes some time for these things to register. Well, yeah. So your hair will grow for four to six years, but then your hair will take a break. And it will rest. And during that resting stage, the cells that produce pigments that go into your hair die.
Starting point is 00:28:56 And then you have stem cells that will produce more of the pigment-making cells. And those new, fresh baby-like pigment-making cells will go down into your hair follicle to start the cycle again. Got it. And so you need one set of cells to die and a new set of cells to come in with their new instructions reflecting the new hormone milieu and your teenage body before you start getting that change in hair color. I see. So it's not just that we shouldn't think of ourselves as having one hair color, but instead we should think of ourselves as capable of producing a spectrum. And the color that's actually on your head somehow reflects the history of the hormone. that your hair cells have received, but also in a time-delayed way
Starting point is 00:29:43 because cells have to die and be replaced. So in some sense, like a person who has brown hair is telling me that, like, over the last few years, their hair cells have received the hormones to produce brown. Yes-ish. But just to clarify, like, you said that we've got a gradient of hair colors. I don't think I have anything in me that could make me make red. hair. Like, I don't, nothing. Nothing. There's nothing that could happen in the world. I will not.
Starting point is 00:30:13 Asteroid impact. I don't think that I have the genes for like the right kind of receptors or something like that. So I'm not capable of producing red hair, but I am capable of producing, you know, like a range of browny black colors or something like that. So our genomes can control the sort of spectrum that hormones can influence. That makes a lot of sense. Okay. Or at least that is how I understood it while I was doing the reading. So hopefully that's totally correct. If not, write to me and tell me I'm wrong. I always want to know. And is it like an on-off thing? You know, if I get no hormones, am I producing blonde? And then I have to get hormones to produce brown? Or is that I need to get the blonde hormones or get the brown hormones?
Starting point is 00:30:55 I think it's a little more complicated. So it can depend on like how many copies of the genes you have for certain receptors. And so if you have like both copies of the genes for a certain receptor you're like more likely to produce brown and you're more receptive to the amounts of hormones that are in your body. But we have now slammed into the wall of Kelly's knowledge at 100 miles an hour. So summary is it's complicated. Right. It is complicated. Over 100 genes involved, it sounds like. And it changes over the course of your life as your hormones change over the course of your life. So the listeners also wanted to know if it was evolutionarily advantageous. that their babies were going from blonde-headed babies to darker-haired babies.
Starting point is 00:31:44 Right. And at the end of the day, I think the answer is probably not. We don't, like, we probably don't know. I can't see a benefit of, like, you know, does a blonde-haired baby hide better in the snow? And, like, if you, you know, worried about predators around. And I can't come up with a good explanation. And it's not about, like, blonde-haired babies are cuter because we know that moms will find their own babies cute, even if they do look like Richard Nixon.
Starting point is 00:32:07 Or Danny DeVee. He was the cutest. Anyway. So I looked for hypotheses that people came up with. And the closest I could come up with is that blonde and red hair might just be a side effect of needing to have a lighter colored skin when you live in areas that get less sunlight. So UV light is important for us for the production of vitamin D. And so if you live in areas that get less sunlight or darker for more times of the year, having lighter skin allows you to absorb more of that UV light and helps you with problems related to vitamin D. And so as our skin lightened, we might have ended up with lighter hair as sort of a side effect of the lighter skin because a lot of the same pigments that go in your hair are also found in your skin.
Starting point is 00:32:59 So this doesn't tell us why it's beneficial for your hair color to change. from when you're a baby to when you're an adult. But I think the point is that hair color in general, like having a variety of hair colors isn't really something that selection has probably acted on. It's probably just something that got pulled along because of something that was happening to our skin. And so you wouldn't necessarily expect there to be an evolutionary advantage to your
Starting point is 00:33:26 hair going from blonde to darker colored when hair color is just sort of like pulled along because of selection on something else anyway. Right. And so this is sort of a subtle point in evolution, at least for a physicist, that it's not necessary for every trait you have, even ones that have survived selection, to be individually advantageous. They can just be linked to something else, which is an advantage. So, for example, of being a physicist is an advantage, but it also means you have a terrible sense of humor, then you might ask, like, how do all these people with terrible sense of humor
Starting point is 00:34:01 find mates and have children and whatever. And the answer is because of their amazing physics knowledge. And that's the reason to survive. Just as an example to illustrate the point. That seems like two hurdles to get over, but instead of just one. But I think I understand what you were trying to get at there. But I want to be really clear that like the stuff that I just said was pretty handwavy. I was trying to find some answer other than, I don't know, but I wanted to give at least a guess.
Starting point is 00:34:27 Anyway, I don't think we really know the answer, but that might be what's going on. All right, cool. Okay, so I think that that answers our listeners' questions, and so let's go ahead and see what they had to say. Hello again, Daniel and Kelly. Thanks for returning to the subject, taking some time to answer further questions about hair color. I think I understand a little more now. I understand how both genes and hormones play into the variability of hair color. color across people and across time.
Starting point is 00:35:00 And more than that, I think I understand something about how these questions and answers work because I knew that Kelly was going to say, it's complicated, about three seconds before Kelly said, it's complicated. Thanks again. Kelly, your answer on hair color was very informative and I actually learned something. Thank you. Get Bell Pure Fiber Internet with Crave, Netflix, and Disney Plus from $94 a month. Price guaranteed for two years on Internet with a two-year term and auto pay credit.
Starting point is 00:35:41 Visit bell.ca for details and to check availability. Bell, connection is everything. What's up, fam? I'm sports journalist Ari Chambers. Hey, what's up, y'all? It's your girl, Sam J. And we're the host of Everyone Watches Women's Sports, a new podcast from Together and I-Heart Women's Sports. Because let's be real. Women's sports is giving us way too much to talk about.
Starting point is 00:35:59 about these days. So Kelsey Finler, she became the first female solo rower to go from California to Hawaii. My first thought is like, what's up with the snacks? Like, what are we eating? The highlights, the rivalries, the breakout stars, the moments to take over your entire timeline. And the conversations that start during the game and somehow keep going all week. Every week, we're breaking down the biggest stories across women's sports. Naomi Osaka showing out, she beat Sabalinka.
Starting point is 00:36:28 Shout out to you, Naomi. You get the palm, Naomi. You get the calm for that. Because we're not just interested in what happened. We're interested in why everyone's talking about it. Because everyone watches women's sports. Listen to everyone watches women's sports. On the IHeart Radio app.
Starting point is 00:36:41 Apple Podcasts or wherever you get your podcast. Hey, Portlandia fans. Carrie Brownstein and Fred Armisen here. You know us or rather you know them. Tony and Candace, Nina and Lance, Spike and yes, the chicken. We've played a lot of iconic characters over the years, but today we're showing up as ourselves
Starting point is 00:37:00 to tell you about Podlandia. AEO rewatch, our brand new podcast. Each week, we'll revisit an episode of Portlandia from the very beginning, breaking down the sketches, exploring the backstories of our most iconic characters, revisiting the Portland locations you know and love, and opening up about our creative process. How did any of this get made? Why do we think that was a good idea?
Starting point is 00:37:21 We're ready to talk about it. And we'll also be joined by the people who helped bring it all to life. Guest stars, collaborators, and friends, including director Jonathan Chrysler, the mayor himself, Kyle McLaughlin, legendary musician Amy Mann and many more. Kyle is going for it here. You fully improvised, not just words, but a song, a melody. I thought he was going to write.
Starting point is 00:37:41 I thought you were all going to write a song. I remember you thinking that. Listen to Podlandia. Ayo rewatch on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. My first guest is Perix Hortton, Shakira, Luke and Yerrin, Samira and Gracie. I'm so excited. on a bouncy bed. You have surprises?
Starting point is 00:38:08 Many surprises. Welcome to Sweet 305, where the group chat comes to life. What a . It's like a way to say like, Oh, my God, my friend, oh, my brother. What a . Look, I never have I've ever been with nobody, except with my
Starting point is 00:38:23 sisters, my kids, my children. See my amante. Uff! That incredible, yeah, the telenovela. You're the only person I know that loves a Yellow Starburst. It's flammated. There's someone that you like you say,
Starting point is 00:38:39 I'd like to collaborate with this person. This is Sweet 305. Listen to Sweet 305 with Lele Pons as part of my Cultura podcast network on the Iheart Radio app, Apple Podcast, or wherever you get your podcasts.
Starting point is 00:38:55 We're back, and now we've got a question from Don in Palm Springs, California. This is Don Valene in Palm Springs, California. Daniel and Kelly, thank you for your podcast. There's always something new for me to learn. Suppose there's no iron in the surface layer of a planet. How would an intelligent being who has evolved on that planet discover magnetism? Are other elements sufficiently magnetic or likely sufficiently plentiful to take the place of iron in discovering magnetism?
Starting point is 00:39:37 Is understanding magnetism and likely electricity as well a necessary condition for a civilization to advance to a scientific level where they could receive and send signals through space? space other than whatever visible light they could see. And of course, so far all planets with any intelligent life have had iron on or near their surface. I wonder how delayed their scientific progress would have been without iron. All right, Don, thank you for thinking so deeply about the experience of intelligent aliens living on a planet without iron. Really fascinating thought experiment. Daniel already wants to be your BFF. Well, I think before we answer Don's question about an alternative planet, we have to remind everybody how we discovered magnets and how it fed into our ability to send radio signals to potential aliens.
Starting point is 00:40:34 Give it to me, Daniel. Magnets have been known almost forever. I mean, basically before we have any recorded histories. So historians refer to this as in antiquity, which basically means we've known about this forever. And we can't tell when it was discovered. And that's because we have a lot of iron on our planet, and there's a lot of magnets just sort of lying around. And historically, they call these things load stones. So you have iron, and it gets oxidized with oxygen, again, our friend, because oxygen likes to bind them with everything.
Starting point is 00:41:03 And it makes something called magnetite, and it'll just, like, sit on the surface and be magnetic. And so we have writings from, like, ancient Greece and China and India, people writing about these rocks they found. that will attract iron. And so this has been known forever. And did they use that iron for anything, like to forge swords and stuff? Yeah. So once we got to the Iron Age and people were like smelting iron and making iron and stuff, then people noticed this.
Starting point is 00:41:32 And then using magnets for practical purposes like navigation, that's actually much more recent. It's like maybe a thousand years ago in China and in Europe, the people figured out this whole connection between magnets and directions. on the earth. So people have been using magnets in technology for about a thousand years, but it was only a couple of hundred years ago that people connected electricity, obviously also known in antiquity, you know, lightning and static electricity, to magnetism. And these were really important experiments by Orsted. Essentially, he connected electricity and magnetism
Starting point is 00:42:08 because he accidentally ran a bunch of currents through wires near a compass and saw the compass Twitch. And he was like, wait a second. Why is it when I have electricity, it affects the magnets? That was the first observed connection between electricity and magnetism, and that led to a whole avalanche, you know, Amper's law, the Beosovart law, eventually unification by James Clerk Maxwell in the 1860s of electricity and magnetism into a single coherent theory of a combined phenomenon. That's when we realized, these two things are just the front and back of a single elephant. They're not completely separate phenomena. We've just noticed them differently and never connected them. And Maxwell showed us how they're intimately connected. They're really just one
Starting point is 00:42:53 phenomena. This tangent's not going to go too far, I promise. But like 1854 is when John Snow figured out the cholera pump stuff. So check out our cholera episodes. What an amazing time it must have been to be alive when we're figuring all of this stuff out. We're like, oh, it's, you know, you don't get cholera because you're breathing stuff in. It's in the water. Of course, you live in a time where the water could give you cholera, that's less good. But like, we're figuring out all of this stuff is about electricity and magnetism. Yeah. Like, it must have been really exciting. Yeah, and I hope that in 150 years, podcasters wax philosophical about how amazing it was to be alive now when we're figuring all this stuff out, because there's still a huge amount of stuff to figure out about the universe
Starting point is 00:43:31 and biology and even chemistry. Oh, whoa, even chemistry. And it is chemistry that tells us basically why iron is so amazing. Iron is a great way. way to discover magnetism because, number one, there's a lot of it. The Earth is like 32% iron. So there's just a whole bunch of iron on Earth. And that's not unusual for rocky planets because stars make iron. Stars member are doing fusion. They're squeezing protons together to make helium and that helium gets squeezed together. You get carbon and oxygen and neon and heavier stuff. And if the star is hot enough to squeeze together these heavier elements, you can keep doing that all the way up. to iron. Above iron, it costs energy to fuse heavy elements together, so stars don't make a whole
Starting point is 00:44:20 lot of stuff above iron. So iron is sort of the natural endpoint for stars fusion process of manufacturing heavy elements. So there's a ton of it in the universe. And that's why it dominates our planet's core. And that's very helpful because it's really, really good at making magnets. Remember where magnetism comes from. Electricity comes from electric charges. You can have like an electron, it makes an electric field. We don't have magnetic charges in the same way, but there's this connection between electricity and magnetism that a moving electric charge will make a magnetic field. So you take your electron, you move it in a circle, you get a magnetic field. That's how an electromagnet works. Or if you have an electron and it has a spin to it, that kind of quantum mechanical motion will
Starting point is 00:45:06 also give it a tiny little magnetic field. So electrons are little magnets, essentially. And I Iron has a partially filled outer shell, it's called the 3D sub-shell, and there's room in there for a bunch of electrons. And remember, electrons fill empty slots individually before pairing up, which means that because there's four unpaired electrons, they're all spinning in the same direction. It's not like one up and one down. They all like to fill the up before they fill the down. So iron has a bunch of these unpaired electrons, all spinning in the same direction, making a little
Starting point is 00:45:41 magnetic field. And the atomic spacing of iron is perfect to allow these electrons to like lock their spins and neighboring atoms into parallel alignments. So you get all these electrons from all these iron atoms all pointing in the same direction. And those tiny little magnets add up to a big magnet that sticks to your refrigerator. So ICP was wrong. We know how magnets work. We got this. There's no magic, no mystery there. ICP is right about a lot of stuff. But yeah, not about magnets. Back that up. That up. All right. Let's move on. Magnets. All right. So what if you didn't have iron, right? Iron is great. We used iron in our discovery of magnets. Don is like, well, what if you didn't have it? Could you still discover magnetism? So iron is involved in essentially all naturally occurring very powerful magnets. But it is possible
Starting point is 00:46:31 to have magnetic materials without any iron. So for example, pure nickel is a ferromagnet. Farrow magnets are just like iron. They're easy to align up and they can make permanent magnets. Most of the magnets out there that are nickel magnets are mostly iron, but if you have a very pure deposit of nickel, that will be a pharaoh magnet. On Earth, these things are very, very rare because nickel mixes with stuff, it's hard to find pure nickel. But it is possible. So if you have aliens on a planet with lots of pure nickel deposits, they can use those the way we used loadstones. talk about what pharaoh means? What is a ferro magnet as opposed to a magnet magnet? Yeah, so a ferromagnet
Starting point is 00:47:14 is a material where all of these electrons can be lined up in the same direction and it can stay a magnet. So a ferromagnet, like if you put it near another strong magnet and all of its magnetic regions will get lined up and it'll stay a magnet. A paramagnetic material is one that's only a magnet when it's near another magnet. They don't stay locked in place. And so ferromagnets are what you want. Oh, good. Can we have more? More jargon, Daniel? Oh, we can. Yes, we could bring it also to biological jargon.
Starting point is 00:47:44 Okay. All right, all right, right. What else will make a ferromagnet? So you can use cobalt. Cobaltite is naturally ferromagnetic and it has no iron in it. There's cobalt and arsenic and sulfur in that. It's much less abundant than iron on earth, but it's possible. They're also like neodymium and gadolinium and dysprosium.
Starting point is 00:48:05 these have a really strong magnetic behavior, but mostly with iron. So people are thinking like, what about rare earth materials? Those are magnetic. Mostly those are powerful magnets with iron, combined with iron. Without iron, they're mostly paramagnets, so they're not useful in the same way. So there are some alternative ways to discover magnets. But if you don't have any iron, you probably don't have any pure nickel or cobalt or either. Something went wrong or you're in a weird kind of solar system.
Starting point is 00:48:35 And so let's imagine you have no magnets on your planet. You're an alien civilization. You just have no loadstones, no compasses. Could you still discover electromagnetism and send messages through space? That's what Don is asking. And the answer is yes, because magnetism is connected to electricity. And so if you figure out electricity, you can figure out magnetism without any naturally occurring magnets. Remember how we discover the connection between electricity and electricity.
Starting point is 00:49:05 magnetism is through electrical currents. Orsted had these currents. He had electricity and he discovered, oh, that's magnetic. And it was helpful. He discovered it because it was a magnet nearby, but you don't need any magnets for that. You just have like a couple of wires. You run currents with them. They will attract each other or they will repel each other. They turn into magnets. And so you could start just by discovering like static electricity like we did through amber. You know, you rub amber on cloth. They will accumulate a charge. You observe lightning. You do experiments.
Starting point is 00:49:39 You can definitely discover electricity without any magnetic materials on the surface of your planet. You can develop like natural batteries, all sorts of stuff. And then you start building currents and you see this deflection. You will discover, just like Orsted did, that electric currents produce these magnetic effects. You wouldn't call it magnetism. You would think it's part of electricity. And in that sense, it might even be an advantage. We have the disadvantage of thinking magnets and lightning are totally different things.
Starting point is 00:50:09 The front and the back of the elephant are completely separate. But if you only start from the back of the elephant and then you work your way to the front, then you know already that they're connected. So if you discover magnetism as a part of electricity, that could be even an advantage. What is the link here with communication? The link is that radio waves, the way we like to send messages into space and from person, person to person and the way your cell phone works. These are electromagnetic radiation. So you're sending ripples in the electromagnetic field. An antenna has a bunch of electrons in it that you're wiggling. And so you're wiggling the electric field that it makes. And that's what electromagnetic
Starting point is 00:50:48 radiation is, are wiggles in the electromagnetic field. So if you are going to send messages through space, you have to understand electromagnetism at some level in order to do that. And so that's why Don is interested in this question of like, could you discover electromagnetism, without magnets. And I think the answer is yes, you could discover it purely through electricity. However, you don't have to, right? Like, you can imagine communicating via electromagnetism without really understanding what it is, because light is electromagnetism. And you could be sending messages from planet to planet or even star to star using essentially just optics. Like if you develop very powerful sources of light, even if you don't have a theory of electromagnetism, you could send those
Starting point is 00:51:32 pulses through space, you know, essentially visible light signaling. Like Morse code or something? Like with a laser? Yeah, essentially with a laser, yeah. Morse code or, you know, in the same way that you have signals encoded into radio waves, you can encode a signal into laser pulses through amplitude or through frequency modulation or whatever. So, you know, the bottom line is I think you don't need iron to discover magnetism, but it's an enormous advantage. It's possible to discover otherwise if you have some natural sources of magnets. But the other route is just through pure electricity, which will eventually lead you to understanding magnets anyway, and then theory of electromagnetism,
Starting point is 00:52:13 and then you'll be broadcasting I Love Lucy out into space. But you also don't have to, and you could imagine other ways to send messages maybe to be advanced particle physicists and they send us neutrino bursts or something. And most likely the history of science on that alien planet is even more alien than we could ever imagine. And Daniel's out there transmitting the message. We'll trade humanity for physics facts. And Kelly is out there sending them all sorts of biology jargon. Oh, come on.
Starting point is 00:52:45 When we meet aliens, is that what you want to talk to them about? You're like, here's the name of that receptor, by the way. I want to say what kind of parasites do you have? Here's a baggie for the stool sample. I think I saw that show. It was called Alien Earth. Oh, no. Okay.
Starting point is 00:53:00 All right, let's send this message over to Palm Springs and see if we have answered Don's question about aliens. Daniel and Kelly, thanks for the thorough and thoughtful discussion. It's interesting to learn about magnetic elements and minerals that are not iron. I've always wanted a magnet that attracted other metals like gold or copper. Some being somewhere has likely already created a magnetic prism that refracts a magnetic field to attract or repel whatever. elements they specify. I suppose that's similar to what the Large Hadron Collider at CERN does
Starting point is 00:53:36 for fundamental particles. Just shrink CERN to fit in your hand, install the app, choose your element, and go asteroid mining. I do have a biology question for Kelly. If iron were very rare at Earth's surface, what color would our blood be? Thank you again. I really enjoy your podcast. Wow, that's a great follow-up question, Don. Okay. So our bodies use a protein called hemoglobin, and iron is used in hemoglobin, and that binds oxygen and brings it to different places in the body. Okay, so you're asking if we don't have iron, what would we do instead? I have no idea what evolution would come up with, but I need to have an answer.
Starting point is 00:54:21 So the answer I'm going to give you is that mollusks, so like clams and stuff, they have hemocyanin, which is a copper binding protein. So instead of iron, it uses copper. So if we lived on a planet with no iron, maybe we would use this to bind oxygen instead. And so if you were using this, the protein turns blue when oxygen is bound to it. So I guess our blood would be blue, which would be kind of epic. Thanks for the question. Don.
Starting point is 00:54:58 Thank you for sharing your curiosity with us. We'd love getting questions from y'all. And you can send us those questions through email at questions at Daniel and Kelly.org. Or you can connect with us at our Discord channel and you can get an invite to our Discord channel by going to Danielandkelly.org. We hope to hear from you. We answer every question.
Starting point is 00:55:17 Daniel usually within 30 seconds. Me usually within about a week. But we answer them all and a subset of them end up on the show. That's right. And thank you for lending us. Your curiosity. Thanks everybody for listening. Please go and do us a favor and rate the show on whatever podcast app you're using.
Starting point is 00:55:40 It really helps people find us. Daniel and Kelly's Extraordinary Universe is edited by the amazing Matt Kesselman. He really is a wizard. You can also find us online on Blue Sky, Instagram, and X, D&K Universe. Come engage with us. You can email us at Questions at Daniel and Kelly.org. We really do want to hear from you. And you can find our website, www.
Starting point is 00:56:05 www. danielandkelly.org, where you'll also find an invitation to join our Discord where everybody comes and talks about the amazing universe. And we also have the most amazing moderators. This is an I-Heart podcast. Thanks for joining us. Hey, Portlandia fans. Carrie Brownstein and Fred Armisen here. The Dream of the 90s is alive in podcast form.
Starting point is 00:56:29 We're launching Podlandia, A.O. rewatch, our brand new podcast, where we revisit every episode. to Portlandia together, breaking down sketches, going deep on our iconic characters, and pulling back the curtain on how it all got made. And we'll also be joined by the people who helped bring it all to life. Guest stars, collaborators, and friends, including director Jonathan Chrysall, the mayor himself, Kyle McLaughlin, legendary musician Amy Mann, and many more. Kyle is going for it here.
Starting point is 00:56:55 You fully improvised, not just words, but a song about it. Well, I thought you were all going to write a song. I remember you thinking that. Listen to Podlandia. rewatch on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. I'm Nick Tuturo. You probably know me from NYPD Blue, the longest yard, or Spike Lee's Black Klansman. And on my new podcast, delivering happiness with Nick Tatoro, I deliver pizza to a new guest.
Starting point is 00:57:21 I've shared a slice with everyone from Seth Rollins. What are you doing, my belt? To Bill Burr. I don't think I've ever met somebody so exactly out of their mind as I am. And now, we even have more great guests coming up, including the great John Tuturo. It's called happiness, delivering happiness. And many, many more.
Starting point is 00:57:39 Open your free high-heart radio app. Search Delivering Happiness with Nick Taturo. And listen now. This is Chelsea Handler from Dear Chelsea. Every week, the news gets worse. The world gets crazier. And Yamanika is here to tell whoever's responsible, you're the problem.
Starting point is 00:57:54 Do you know I just found out who Sidney Sweeney was? If he got a bunch of women, then I should have a bunch of men. Do better or do less so I don't have to do so much. I'm Yamanika, and I'm out. Listen to You're the Problem with Yamanika on the I Heart Radio app, Apple Podcasts, or wherever you get your podcast. On Raiders of the Lost podcast, we explore cinema like no one else, including huge interviews with stars like Ryan Gosling on Project Hail Mary. It was like the Jaws Shark. Didn't always work, came with its own problems.
Starting point is 00:58:29 That's what made it great. The cast of obsession. On set, there was so much magic happening with each scene we were putting together. deep dives into classics like 2001 a Space Odyssey or Fight Club, plus weekly episodes on all industry news. Listen to Raiders of the Lost podcast on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. And for more, follow at Raiders of the Lost podcast and at TikTok Podcast Network on TikTok. This is an IHeart podcast. Guaranteed human.

There aren't comments yet for this episode. Click on any sentence in the transcript to leave a comment.