Daniel and Kelly’s Extraordinary Universe - Listener Questions #12

Episode Date: June 19, 2025

Daniel and Kelly answer questions about neutrons, bananas and Jupiter and find a secret theme that links them all!See omnystudio.com/listener for privacy information....

Transcript
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Starting point is 00:00:00 This is an I-Heart podcast. I'm Dr. Scott Barry Kaufman, host of the psychology podcast. Here's a clip from an upcoming conversation about how to be a better you. When you think about emotion regulation, you're not going to choose an adaptive strategy which is more effortful to use unless you think there's a good outcome. Avoidance is easier. Ignoring is easier. Denials easier.
Starting point is 00:00:25 Complex problem solving takes effort. Listen to the psychology podcast on the. iHeart radio app, Apple Podcasts, or wherever you get your podcasts. I just think the process and the journey is so delicious. That's where all the good stuff is. You just can't live and die by the end result. That's comedian Phoebe Robinson. And yeah, those are the kinds of gems you'll only hear on my podcast, The Bright Side.
Starting point is 00:00:48 I'm your host, Simone Boyce. I'm talking to the brightest minds in entertainment, health, wellness, and pop culture. And every week, we're going places in our communities, our careers, and ourselves. So join me every Monday, and let's find The Bright Side together. Listen to The Bright Side on the IHeartRadio 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?
Starting point is 00:01:20 But the real world is different. Managing life's challenges can be overwhelming. So what do we do? We get support. The Huntsman Mental Health Institute and the Ad Council have mental health. health resources available for you at Love Your Mind Today.org. That's loveyourmindtay.org. See
Starting point is 00:01:36 how much further you can go when you take care of your mental health. Have you ever wished for a change but weren't sure how to make it? Maybe you felt stuck in a job, a place, or even a relationship. I'm Emily Tish Sussman and on she pivots, I dive into the inspiring pivots of women who have taken
Starting point is 00:01:51 big leaps in their lives and careers. I'm Gretchen Whitmer, Jody Sweetie. Monica Patton. Elaine Welteroth. Learn how to get comfortable pivoting because your life is going to full of them. Listen to these women and more on She Pivot's, now on the IHeartRadio app, Apple Podcasts, or wherever you get your podcasts. Are the bananas we eat all the same? Can we save them from that fungal strain? Is Jupiter really only made of gas?
Starting point is 00:02:30 It's definitely got a lot of mess. Biology, physics, archaeology, forestry. Thanks for not asking about chemistry. What diseases do you get from your cat? Well, we'll find the answers to all of that. Whatever questions keep you up at night, Daniel and Kelly's answers will make it right. Welcome to another listener questions episode on Daniel and Kelly's Extraordinary Universe. Hello, I'm Kelly Waitersmith.
Starting point is 00:03:08 I study parasites and space. And you were surprisingly good at Limericks. Well, I don't know about that. I gave a talk in Kentucky, and a woman who is a poet was invited. And she gave a poem about our book, and she encouraged me to be bolder about poetry and not so self-conscious. And I know... It's not good, my rhymes, but I have so much fun and I'm like, that's kind of the point for me, for me, that's the point. Well, I'm Daniel. I'm a particle physicist. I don't pretend to be a poet, but I think the universe is kind of poetic.
Starting point is 00:03:44 Oh, see, I think you're a poet in your own way, because you say very poetic things. Well, if being corny and curious about the universe counts as being poetic, then put me on that list. It's a dad kind of poetry. There you go. Dad poetry. Oh, my gosh. Science dad poetry, that is a new genre. We are pioneering here. Science parent poetry, really.
Starting point is 00:04:06 Yes. Well, you might ask yourself, why would Kelly make her poems public? I don't really know I have a confidence beyond what I ought to. But, you know, there are other questions out there, and our listeners have loads of them. Questions deeper than Kelly's ability to rhyme. We love hearing your questions about the universe. How did it begin? How is it going to end?
Starting point is 00:04:27 Was it all mean? How does it come together to explain everything we are and everything we eat and all the poems we listen to? If you have questions about the nature of the universe and you can't find answers, you've been Googling, you've been asking your neighbors. You don't know any physicists or parasitologists yourself. Please write into us to questions at Daniel and Kelly.org. We love, love to hear from you and you will definitely hear from us. And everybody should have a parasitologist and a physicist in their lives and we are here for you. That's right.
Starting point is 00:04:59 We are filling that hole you didn't know you had in your life. Exactly. And so today we have a bunch of really fun questions about neutrons, about bananas, and about Jupiter. And there's a theme that's going to tie them all together. We'll reveal it at the end. Oh, Daniel's going to be revealing this to Kelly, too, because I didn't see a theme while I was reading our outline. Can't wait to find out. This first question is from Scott Lewis, who thought that neutrons also needed some Daniel and Kelly love after hearing our episode
Starting point is 00:05:27 about protons. Hi, Kelly and Daniel. There have been a number of articles lately discussing the internal complexity of the proton and everything we are learning about it. One article went so far as to describe it as the most complicated thing you can possibly imagine. I've read of unusual tetracork configurations and other weird things that show up in the colliders from time to time. Is the internal structure of a neutron similarly complex?
Starting point is 00:05:59 Do we know less about the guts of a neutron? And if so, is there a reason why they are perhaps more difficult to study? Thank you for everything you guys do. Great job on the program. This is a great question. And you know, Daniel, whenever I hear about neutrons, I think about one of those disaster movies with John Cusack in it, where the world was like falling apart because the neutrons had mutated.
Starting point is 00:06:24 I know. I almost walked out of that movie. I loved John Cusack as a child of the 80s, you know. You can say anything, but don't say anything about neutrons mutating. That's right. That's a line for me. A line. But I got to say I don't really understand neutrons very well. So let's start at the beginning. What are neutrons? And hopefully by the end, I'll be convinced that they won't mutate and I don't have to worry about the world being destroyed. Well, I agree with Scott. Neutrons are just as fascinating, if not more so, than protons. And they don't get it. as much attention because we don't think of them as the building blocks of matter, but they really are. They're essential. Without neutrons, we wouldn't have big complicated atoms that you need for biology and chemistry and bananas, for example. But protons and neutrons are very closely related. Both
Starting point is 00:07:09 of them are made of the same fundamental objects, just different amounts of them. So a proton is made of two upcorks and a down cork. And so the upcork is charged two thirds. The down cork is charged minus one-third. So you add two upcorks and a down-cork, you get a total charge of one. That's the proton. If you switch one of those upcorks for a down-cork, now you have one up-cork with charge two-thirds and two downcorks with charged minus one-third each, you get a neutron because it's neutral. It has zero electric charge. So two downs and an up, neutron. Two ups and a down, proton. Got it. So usually on this show, you hear me complain about how bad physicists are at naming things. Because we are.
Starting point is 00:07:51 Exactly. Yeah. I'm making an accurate observation. But I love that you all have named the thing that holds it all together, glueons. And I'm assuming that's because it sounds like glue, right? Well, the gluons aren't very sticky. Yes. They do hold these things together.
Starting point is 00:08:07 And so up quarks and down quarks are super fascinating because they're similar to other particles we know like electrons, but they also feel another force, the strong nuclear force. So they're charged. We talked about them having two-third. or negative one-third charge. So they feel electromagnetism. They can shoot off photons. They feel electric fields. But there's another field in the universe that they feel that electrons ignore.
Starting point is 00:08:30 And that's the color field of the strong nuclear force. And vibrations of that field, there are actually eight different ones, are called gluons. And so gluons are the mediator of the strong force the way photons are the mediator of the electromagnetic force. It's just one of the things the universe can do. and electrons have zero color charge, so they just fly through it and ignore it. The way neutrinos, for example, ignore electric fields. But quarks, they feel all of the fields.
Starting point is 00:08:57 The weak field, the strong field, the electromagnetic field, they feel all of them. And the strong field is the strongest one. And so it binds these particles together very, very tightly. So the proton and the neutron are both bound together using gluons. And is there a history behind gluons that's going to like make me think you all aren't clever? Or was it called gluons because it like seems to glue things together? No, we're called the gluons because they glue the nucleus together. Exactly. And there's a whole fascinating history about the discovery of gluons and the personalities involved. It was really
Starting point is 00:09:29 interesting moment with fascinating history. But basically every discovery in particle physics has like cool personalities and controversies. You would say that as a permanent member of that community. They're not always positive stories. There's like arguments and people peeing on other people's experiments and like, you know, these are human stories because, hey, physicists are people. You know, we're just curious about the universe and there are Nobel Prizes at stake. So you don't always get the best side of everybody. They sure smell like people. You walk up to them.
Starting point is 00:09:59 You're like, yeah, you're a person. But anyway, okay, one day we should get the great story behind gluons. But let's talk about how neutrons decay. Yeah. So the fascinating thing that neutrons can do that protons do not do is that they decay. They don't last forever. You have a neutron out there in the universe just by a, itself, it's going to turn into a proton. And the way it does this is that one of those quarks,
Starting point is 00:10:21 the decork, turns into an upcork. So it goes from D to up. Now, it starts out as a decork, which is charged negative one-third, and becomes an upcork, which is charged two-thirds. So to conserve electric charge, it has to emit a negatively charged particle. So it emits a W-minus, which has charged negative one. So all the charges balance out. So this decork emits a W-minus and turns into an upcork, turning the neutron into a proton and then shooting off this W-minus particle. Okay. So neutron, when it becomes a proton, you get a proton and an electron that shoots off. You get a W-minus, not an electron, but you're close because the W-minus doesn't live for very
Starting point is 00:11:03 long. It turns into an electron and an antineutrino. And so that's basically the process is the neutron turns into a proton. In order to balance the charge, it has to carry along an electron eventually, right? Because you start with a neutron at zero charge. You end up with a proton with plus one, and you need the electron with minus one to balance the electric charges. But the universe is not happy with that because the universe also conserves the number of electrons. Like you can't just create electrons willy-nilly.
Starting point is 00:11:33 The universe keeps tabs on that. So if you create an electron, you also have to create an anti-electron. Or it turns out electron neutrinos also count. So if you create an electron and an anti-electron neutrino at the same time, then everything balances out. You've accounted for everything the universe cares about. I think the up-down quarks give me this maybe false sense of understanding what's going on because I just imagine an up arrow and a down arrow. And I'm like, oh, I got it. You just flip the down arrow. Now it's pointing up. But what does it mean to say it emits a W-minus?
Starting point is 00:12:03 Is it just like the change in energy gets expelled? And that's what it means to say emitting a W-minus? We really do think about these things as a pair, where the up on the top and the D on the bottom. And the way we think about it from a sort of theoretical point of view is that the W is the way to go up or down. So there's actually two Ws, the W plus and the W minus. If you want to go from the D to the U, you emit a W minus. If you want to go from the U to the D, you emit a W plus. So these are sort of like stair steps in order to go from one to the other. It's sort of the same way around an atom, an electron can go up and down energy levels
Starting point is 00:12:39 and to do so, it either emits or absorbs a photon. These Ws change the state from a D to a U. And there is a connection to the sort of underlying theoretical structure, which we usually represent using these things called groups where you can transform an object, but it stays within a little predefined set. That's called a group. And so it's deeply connected to the sort of group theory structure,
Starting point is 00:13:01 which I think we should dig into some time on the podcast. Sure. But the basic version is that the up is sort of the higher state and the down is the lower state, but you can move between them using these Ws. Okay, awesome. All right, I think I get that. Thank you.
Starting point is 00:13:14 So you can go from neutron to proton, but protons don't decay into neutrons. Why do neutrons decay? Yeah, great question. Why do neutrons decay and protons don't? Well, neutrons have a higher mass than protons. And so when a neutron decays, it gives off a little bit of energy and turns into a proton. Why is a neutron have a higher mass than a proton? Well, remember, the mass of these guys comes from the bonds between.
Starting point is 00:13:38 the quarks. It's not because the neutron is made of heavier stuff than the protons. These up and down quarks have almost no mass, basically zero compared to the mass of the proton and the neutron. All of the mass of these guys comes from the gluons, the arrangements of the particles. And so the neutron state up, down, down is a higher energy configuration than the up, up, up, down proton state. And so it's just like a higher energy level. The way like around an atom, you know, there's like the 5-2-S state is a higher energy level than like the 2P or whatever. There's all these different energy levels, and they have to do with the arrangements between the particles, the configurations. And so the strong nuclear force, super duper complicated, but this neutron state, the UD state, is higher energy than the UUD.
Starting point is 00:14:21 And so it can decay down. And that's what the universe does. It always starts with massive particles, which decay down into lighter particles. The proton can't decay because there's nothing lighter than the proton. Like you can't find a state that's lighter than the proton. If you turn that other D into a U, for example, it actually would be a higher energy state than the proton. So the proton is sort of like the bottom of the latter. In the same way, the electron is.
Starting point is 00:14:45 The muon can decay into an electron and other stuff. Why doesn't the electron decay? Because there's nothing for it to decay into. It's the lightest particle, and therefore it's stable. Now, we don't know that the proton is actually stable. We've just never seen it decay. And so we can estimate that its lifetime is super duper long because we've watched a bunch of protons for a long time to see if any of them decay and never seen a a single one decay, which means either they're totally stable like they live forever, or they
Starting point is 00:15:11 live for such a long time that we just haven't seen one yet. And that lifetime would be like billions and billions of years. So neutrons are super fascinating because they actually do decay. So we can learn something about what's going on inside them. So in the nucleus of an atom, you have the same number of protons and neutrons, but the number of protons isn't changing over time, but neutrons are decaying into protons. What's going to happen? Are we eventually? not going to have enough neutrons for everything? Yeah, this is really amazing because remember we are talking about neutrons by themselves. A single neutron in the middle of space will decay in about 11 to 12 minutes.
Starting point is 00:15:47 So you might be wondering, why isn't everything inside me? Why aren't all my neutrons turning into protons and then like, you know, everything is going haywire? Because the neutron is stable if it's inside the atom. It's unstable and will decay into a proton when it's outside by itself. But inside the atom, all of its other neutron and proton buddies, stabilize it. That's really weird, right? What's going on? What's some really interesting strong force stuff is happening there because when the neutrons and the protons are together in the nucleus, they're not just like packed in like tennis balls. They're interacting with each other, right? These
Starting point is 00:16:20 things are quarks with gluons holding them together, but they're not completely sealed off from anything else. If you're like on one side of the gluon, you might be closer to one of the corks or closer to one of the other corks. So you can actually feel the corks inside the neutron if you're nearby it. And so the Atom is not just like a bunch of tennis balls totally sealed off. They're interacting with each other. There's this little residual strong force. That's actually what holds the nucleus together. Friends help you hold everything together.
Starting point is 00:16:46 Yes, exactly. And so inside a nucleus, neutrons can live a long, long time. Sometimes they can live forever. Like take a carbon atom. Carbon has a bunch of neutrons in the nuclei. Those neutrons will live forever. You have a carbon atom, we think you could just sit in space for a zillion, zillion, zillion years. Other elements are not as stable, like uranium, for example, will break down.
Starting point is 00:17:08 And one of the ways it does is through these kinds of decays. And so neutrons can either crack open your nucleus if they're not quite stable enough or they can help it stay together. Like the reason the nucleus stays together, all these protons, which otherwise are pushing each other apart, is because the neutrons are there in between to help stabilize it, to pull them together with the strong force and to keep the protons from pulling themselves apart. So neutrons are really the glue that holds the whole universe together.
Starting point is 00:17:33 I feel like you could write nerdy hallmark cards. I love you and your neutrons. That's right. You hold me together. You're my proton. You keep me from decay. That's right. But there's also still a bunch of mysteries about the neutron.
Starting point is 00:17:53 Like we think we understand the basic story here. But, you know, particle physicists nerds always want to drill down and say, do we really understand it? Let's make a bunch of really precise measurements. in different ways and see if there's anything surprising. So there's this mystery right now in exactly how long the neutron does live. How do we ask that question? So people came up with two very different ways to measure like how long does a neutron take to decay. There's the bottle method and the beam method.
Starting point is 00:18:21 And the bottle method is pretty simple. It says take a bunch of neutrons, cool them down so they're not flying around everywhere, put them in a bottle, and then just wait and see how many you have. Like, you know, plot them over time. The way we study radioactive decay or any kind of random process is you start with a bunch of them and you wait to see how long does it take until you have half as many. And that's the characteristic lifetime. And so that's what they do.
Starting point is 00:18:44 And they get a number. It's like 14 minutes and 39 seconds. It's the characteristic lifetime of a neutron. This is a really cool experiment. They do in Los Alamos, New Mexico, actually, my hometown. And they have these ultra-cold neutrons. They've chilled them down to like mill of Kelvin inside this container. call the bathtub. It's like one meter in diameter. They just like fill it with neutrons and count
Starting point is 00:19:06 them and then wait to see what happens. And so they get their number and you know, these are serious dudes. They take it very seriously. They've accounted for all sorts of uncertainty. They have cross-checks, whatever. They're very confident in their number. But there's another experiment, the beam experiment, and they don't get the same answer. What? How much does it differ by? The beam experiment makes a neutron beam. And you know, we said that neutrons decay into protons, right? So they had this clever idea like, oh, neutrons are actually really hard to count. The other guys have this complicated, sophisticated, sophisticated equipment to count neutrons. They're hard.
Starting point is 00:19:36 Let's just count the protons. If neutrons are decaying into protons, let's just count the protons. And so they fly it through an electromagnetic field, filter out the protons, and count those. And they get a different answer. They get a slightly longer answer by nine seconds. So instead of 14 minutes and 39 seconds, they get 14 minutes and 48 seconds. So they think neutrons live a little bit longer than the bathtub guys. But don't you have to at least know how many neutrons you're starting with? Because if you get 10 protons, but you don't know how many neutrons you started with, how do you know the rate of decay?
Starting point is 00:20:08 Yeah, good question. They know how many neutrons they've started with because they know how they produce the neutrons. And so they think they've accounted for that. But you know, something is going on here. Like it's the same process. They should get the same answer. So either somebody's made a subtle error totally possible, right? And they both worked really, really hard to reduce these uncertainties. Often in this scenario, you get two experiments. They get different measurements, but they both have large uncertainties and they overlap. And then they both work really, really hard to refine their experiments. And usually as the uncertainty shrink, the results converge into one answer. You're like, okay, cool. The universe is coherent. But what's happening here is that the uncertainties are shrinking, but the answers are not getting closer together.
Starting point is 00:20:48 So they're getting more and more confident in their discrepancy, which means, hey, maybe there's some new interesting physics. Maybe the neutron, like the boring vanilla particle, most people, who aren't excited about is actually the portal to discovering the nature of the universe. You all are pros at silver linings. Well, this is a really fun idea that maybe neutrons don't just decay to protons. Maybe sometimes neutrons decay into something else
Starting point is 00:21:15 like dark matter. And so in the neutron beam, what's happening is these neutrons are just disappearing into dark matter and those guys are not measuring it. So maybe the bathtub guys are right because they're actually measuring the neutrons. Whereas the guys who are assuming they turn into protons, they're the ones getting the wrong answer because it's not always going to protons. Sometimes it's going to dark matter.
Starting point is 00:21:35 And we can't measure dark matter, right? We do not have ways to measure dark matter. Certainly not in these beams. And so this is really interesting and really important because it could be an indication of something that's happening. And it's also important because it helps us understand the early universe. You know, the very early universe, we had like corks and gluons flying around and things cooled down into hydrogen. and briefly also forming some helium. And that ratio of hydrogen and helium is super important
Starting point is 00:22:02 because it tells us something about the density of corks at that time and what the early universe was really like. And we need neutrons in order to form helium. Like you can't form helium without neutrons. You can't just squeeze protons together. You have to have those neutrons to facilitate. But if the neutrons decay a little bit faster, then they aren't around as long to make helium.
Starting point is 00:22:22 If neutrons decay slower, there are more of them to stick around and make helium. More helium means smaller, longer-lasting star. So it has this like cascading effect on the whole history of the universe. Super fascinating. Anyway, neutrons really amazing. Thank you very much, Scott, for asking about this. And I hope that we've answered all of your questions about neutrons and inspired new ones. Let's hear what Scott has to say about our story of neutrons. Hi, Daniel and Kelly. Thank you for the thoughtful answer. It seems like the neutron has a PR problem, and I'm just not okay with that state of affairs. Neutrons do some very cool and rather important things, and the world really needs to know.
Starting point is 00:23:05 As a follow-up question, if a free neutron decays in a matter of minutes, does that imply that the study of neutron guts is practically more difficult than the study of proton guts? Thanks again for everything you guys do. Great question. Well, we can study neutrons because there are lots of them, but seeing them fall apart is actually useful because it gives us something to measure, to predict, to calculate. Protons, on the other hand, just sit there. So we have to do some work to smash them or poke them to learn anything.
Starting point is 00:23:36 So neutrons are actually being helpful. A foot washed up a shoe with some bones in it. They had no idea who it was. Most everything was burned up pretty good from the fire. Not a whole lot was salvageable. These are the coldest of cold cases, but everything is about to change. Every case that is a cold case that has DNA. Right now in a backlog will be identified in our lifetime.
Starting point is 00:24:08 A small lab in Texas is cracking the code on DNA. Using new scientific tools, they're finding clues in evidence so tiny you might just miss it. He never thought he was going to get caught. And I just looked at my computer screen. And I was just like, ah, gotcha. On America's Crime Lab, we'll learn about victims and survivors. And you'll meet the team behind the scenes at Othrum, the Houston Lab that takes on the most hopeless cases to finally solve the unsolvable.
Starting point is 00:24:39 Listen to America's Crime Lab on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. I'm Dr. Joy Harden Bradford. And in session 421 of Therapy for Black Girls, I sit down with Dr. Othia and Billy Shott to explore how our hair connects to our identity, mental health, and the ways we heal. Because I think hair is a complex language system, right? In terms of it can tell how old you are, your marital status, where you're from, you're a spiritual belief. But I think with social media, there's like a hyper fixation and observation of our hair, right?
Starting point is 00:25:14 That this is sometimes the first thing someone sees when we make a post or a real. It's how our hair is styled. We talk about the important role hairstylists play in our community, the pressure to always look put together, and how breaking up with perfection can actually free us. Plus, if you're someone who gets anxious about flying,
Starting point is 00:25:33 don't miss session 418 with Dr. Angela Neil Barnett, where we dive into managing flight anxiety. Listen to therapy for black girls on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast. Get fired up, y'all. Season two of Good Game with Sarah Spain is underway. We just welcomed one of my favorite people and an incomparable soccer icon,
Starting point is 00:25:55 Megan Rapino, to the show, and we had a blast. We talked about her recent 40th birthday celebrations, co-hosting a podcast with her fiance Sue Bird, watching former teammates retire and more. Never a dull moment with Pino. Take a listen. What do you miss the most about being a pro athlete? The final. The final. And the locker room. I really, really, like, you just, you can't replicate, You can't get back. Showing up to locker room every morning just to shit talk. We've got more incredible guests
Starting point is 00:26:26 like the legendary Candice Parker and college superstar A.Z. Fudd. I mean, seriously, y'all. The guest list is absolutely stacked for season two. And, you know, we're always going to keep you up to speed on all the news and happenings around the women's sports world as well. So make sure you listen to Good Game with Sarah Spain on the IHeart Radio app, Apple Podcasts,
Starting point is 00:26:44 or wherever you get your podcasts. Presented by Capital One, founding part partner of I Heart Women's Sports. The OGs of uncensored motherhood are back and badder than ever. I'm Erica. And I'm Mila. And we're the host of the Good Mom's Bad Choices podcast, brought to you by the Black Effect Podcast Network every Wednesday.
Starting point is 00:27:02 Historically, men talk too much. And women have quietly listened. And all that stops here. If you like witty women, then this is your tribes. With guests like Corinne Steffens. I've never seen so many women protect predatory men. And then me too happen. And then everybody else want to get pissed off because the white said it was okay.
Starting point is 00:27:18 Problem. My oldest daughter, her first day in ninth grade, and I called to ask how I was going. She was like, oh, dad, all they were doing was talking about your thing in class. I ruined my baby's first day of high school. And slumflower. What turns me on is when a man sends me money. Like, I feel the moisture between my legs when the man sends me money.
Starting point is 00:27:37 I'm like, oh, my God, it's go time. You actually sent it? Listen to the Good Mom's Bad Choices podcast every Wednesday on the Black Effect Podcast Network. The I Heart Radio app, Apple Podcast, or wherever you go to find your podcast. All right, so I got to tell you, I'm on the edge of my seat trying to figure out what ties together all of the three questions that we got today. It's still not clear to me, other than the fact that, like, bananas are made of protons and neutrons. Is that it? Was it that simple?
Starting point is 00:28:13 No, that's not it. It's more than that. It's got to be more than that. So our next question is about bananas. Matt from Discord had this question. Hi Daniel and Kelly. This is Matt from Indiana. I was walking through the grocery store and noticed there are all sorts of varieties of peppers red, green, tiny, big, yellow, orange, tons of apple varieties, red, delicious, Granny Smith. And then I got to the bananas. Just bananas, plain bananas no matter where I go. And then I found out that most bananas we eat are banana clones. So why banana clones and not from seeds is what I'm carrying. of thanks in advance and thanks for giving me an excuse to say bananas way too many times oh man so i was excited to have an opportunity to read more about bananas so let's start with banana reproduction bananas can reproduce in two different ways they reproduce sexually by making seeds
Starting point is 00:29:11 and they reproduce asexually by producing suckers hold on wait i have a question already okay great first of all bananas reproduce or banana trees reproduce right because the bananas themselves are just part of the banana tree, right? Yeah, yeah, yes. You're right. You're right. I was being lazy with my words. Although, I'm going to call you on it because bananas aren't really trees. I think technically they're herbs. Really? Do you remember one of our other episodes we were talking about the anatomy of the tree and how it forms rings? Bananas are just taxonomically, distantly related. They don't form
Starting point is 00:29:43 that way. They just kind of have like a stalk that's really trunk and tree-like in the middle. But they're not like typical trees. Wow. All right. So banana trees are not trees. I've already learned something. And what part of the plant is the banana? Is it fruit the way an apple is? Is this something else weird? I remember strawberries or something totally different. Which part of the plant are we actually snacking on? It is the fruit. Okay. Yeah, yeah. What do you mean by strawberries aren't really the fruit? I'm confused. Didn't we do an episode where like strawberries are actually the seed or something? I don't remember. I remember learning something surprising about strawberries. Strawberry seeds are on the outside, which is atypical. But was that the whole fact? I don't remember anymore. Biology doesn't stay in my head as long as physics does. Oh, no. Busted. Let's get away from this.
Starting point is 00:30:27 So back to bananas. Bananas are the fruit, but they're not technically growing on trees because I thought fruit had to grow on trees. No, I mean like strawberries aren't growing on trees. Mm, all right, cool. Although I guess maybe we're not quite sure if strawberries are fruits. We're all confused today. I'm not sure.
Starting point is 00:30:42 It doesn't mean the people aren't sure. Okay, got it, got it. I'm far for an expert. All right, so bananas can reproduce sexually or asexually, you were telling us. Yes. And so what happens with the asexual reproduction is that the giant stalk that looks like a trunk at the bottom underground, in addition to its roots, it's producing what are called suckers. And these suckers come out from the mother plant and pop up along the sides. And they are essentially just clones of the mom. And they'll stay connected for a while. But you can cut them off, move them somewhere else. And now you've got a new banana plant. And why do biologists call them suckers? I mean, that makes me think of the things on an octopus's tentacle. Are these like an octopus tentacles sticking out through the ground or what's going on here?
Starting point is 00:31:24 Do they suck in some way? I don't know the history, but it's just a much more fun name than any of you guys would have come up with. I'm kidding. Gluons is a great name. I wish we had called some particle the suckers that would have been really fun. You might discover a new particle and I think that's what you should name it. In the suckers beam. That's right.
Starting point is 00:31:41 So they can basically clone themselves, make little mini versions. or they can actually get it on with their neighbors. That's right. And there's something like a thousand species of plants that could be called banana plants. Oh. So there's a lot of diversity. But at some point in the past, so like bananas don't fossilize, so it's hard to know exactly when humans started eating bananas. But way before written records were a thing for our species, what we think happened was that a banana plant had a mutation and it didn't produce seeds.
Starting point is 00:32:12 and you would know if your banana had seeds in it because the seeds produced by lots of banana plants are big and hard and it would be very unpleasant to eat a banana with seeds in it. And so bananas don't have seeds and some human must have found this tree and they were like, oh, this is solid. There's nothing that cracks my teeth in this plant. And so they took the suckers and that got propagated. But this is like prehistory because we don't have records of it.
Starting point is 00:32:38 We don't know when this happened. That's right. Yeah. So could it also have been the product of like, human breeding, we found like a plant with smaller seeds and another one and then crossbred them and pushed them in that direction? Or do you think it's more likely just like one random mutation? Artificial selection could have helped it along. I believe our understanding is that this happened before humans really had enough of an understanding to engage in artificial selection on purpose. But it certainly could have been the case that Joe had a plant that had two
Starting point is 00:33:10 seeds in it and Sally had a plant that only had one and everybody wanted the suckers from Sally's plant because that's way better. And over time, that process could have played out. But I don't think it was purposeful initially. And so that was the last sexual reproduction of these bananas that were eating. And every reproduction of banana trees since that moment has been asexual. So my understanding is that there have been strains that have arisen through this process. So it didn't necessarily happen just once. It could have happened in like five different banana trees in different areas and now you've got these different clonal lineages. But there's still all of those wild banana species out there that are still producing seeds. I see. Okay. So around the 1900s,
Starting point is 00:33:47 there was a strain of bananas called the Gros Michel, which means big mic. It sounds so much fancier in French. It does. But the big mic was everywhere. And I'm going to bum everybody out, which is exactly what everybody expects for me. Apparently, the Gromichelle bananas tasted better than the bananas we have now. Wow. But they were all clones. And so these were being grown all over the world. Bananas were getting huge.
Starting point is 00:34:14 They were being shipped all over the world. And a fungal infection broke out. Oh, no. And because all of the Gromichelles were clones, they were all susceptible. And it decimated the bananas around the world. Sacre blue. Sacre blue. We're sorry, French speakers.
Starting point is 00:34:31 Wait, do you know what the Gros Michel tasted like? Do we have, like, written records? or living people who have eaten them who can tell us about this banana that none of us will ever eat? There probably are some people still alive who have eaten it. I think it was just a sweeter tasting banana
Starting point is 00:34:46 than what we have now. I know. The lost bananas. I know. It is sad. It is sad. Is there somebody out there who's like going to de-extinctify the Groschelle?
Starting point is 00:34:56 That sounds like a billion-dollar idea right there. Yeah. So there might be someone who's still maintaining the suckers from the Groschel in some lab somewhere. but it remains susceptible to Panama disease, which is what we call this fungal disease that wiped out the bananas.
Starting point is 00:35:11 So somebody maybe could bring it back, but when the Gromyshell declined, the Cavendish arose. And the Cavendish must have just been a slightly different strain that happened to be resistant to the dominant fungal strain at the time. And so Cavendish, if you live in North America,
Starting point is 00:35:29 this is the banana that you find on your grocery shelf. So if you go to Harris Teeter or you go to Target or you go to Cresor, Kroger, or you go to Trader Joe's or Whole Foods. Those are all the same banana genotypes. They're clones everywhere you go. They all have the same DNA, you're saying. They all have the same code in their DNA.
Starting point is 00:35:46 There could be a couple mutations, but they are very similar. Wow. Amazing. In countries like Africa and India, they have a greater appreciation for other banana varieties. So there are other parts of the world where you can get other kinds of bananas, but in the U.S., we get this one. I've traveled in Mexico and the grocery stores there, they have lots of different kinds of bananas. They have like little dark red bananas that taste a little bit like strawberries and, you know, big fat bananas and all sorts of stuff. It's a lot of fun. Yeah.
Starting point is 00:36:11 And plantains are fairly popular in the U.S. And I think that's another strain where there were no seeds that were made and then that got propagated by suckers. But in the 1990s, bad news. Oh, no. The Cavendish gets affected by Panama disease. So this fungal disease has continued to evolve while the Cavendish is staying still in this. evolutionary arms race because it's just a clone that we propagate over and over and over again. And there's now a strain of Panama disease that is going after the Cavendish bananas.
Starting point is 00:36:44 Why do they hate us so much? I know. I know. Fungus is the worst. Except when it's helping us make beer and bread and all sorts of other yummy things. You know, I guess whenever you say a blanket statement, you're almost always going to be wrong. Some of them are really fun guys, actually. Oh, dad jokes. Dad poetry. Okay. So now we've got Panama disease and it is spreading. And so there are some people who will be concerned. What happens if the Cavendish declines? Do we have something waiting to replace it? And the answer is no. No. No. What? What are these people doing? Get on it, food scientists. There is a lot of money and bananas. So there's a lot of people working on it. The first thing that they're doing to try to slow the decline is biocontrol. efforts. So if you go to a major banana plantation and you want to go amongst the trees, you have to
Starting point is 00:37:37 suit up in sterilized clothes. You have to put on boots and then walk through a sterilizing solution. And you have to do that every time you walk from like one plot of bananas to another because the way the fungus transmits is in the soil. So if you get like dirt in your boots and then you walk in another area, you can transmit that. Wow. So it's a pain in the rear end. And like every truck that comes in and out has to get sprayed. But if they do find a tree that's infected, they have to dump fungicides into the soil, kill everything in that area,
Starting point is 00:38:08 cover it with urea, which I think just also changes soil chemistry, making it more likely to kill the fungus. Cover it with the tarp so that birds don't walk on it and then bring the fungus somewhere else. The next zone of plants also get like fungicides and herbicides injected into the soil. And then the zone after that,
Starting point is 00:38:25 you have to check. Like every month you have to do like a survey to make sure none of them have it. And so it's intense. Bodge is just so hard to control. It's always wriggling and squirming out of our control. Yes. Oh, man, an invasive species. I feel like it's such an interesting conversation about when do you just give up. Like, it's not worth trying to get starlings out of the U.S. anymore. They're not going anywhere. They're here. Anyway. Well, what about bananas? Is there anything else we can do? Like, can't we somehow protect our bananas or cross them with other wild species or something?
Starting point is 00:38:55 Yeah, I can hear the panic building in your voice. Don't worry. We have a couple. options. I like banana bread, okay? I know. Me too. Zach makes a good banana bread. I don't get in the kitchen, but he does a great job. So genetic engineering is one solution. And they have, in fact, added genes from other plants, I think tomato, to make the Cavendish resistant to Panama disease. And this works. It is resistant. But in the European Union, I believe you're not allowed to sell genetically modified plants. And in the United States, there's a lot of people who feel very squeamish about genetically modified plants. And so the industry has decided that this can't be the solution.
Starting point is 00:39:31 It just would not be financially viable. Wow. So he could save the bananas, but still it's not good enough. Not good enough. And so the last thing that they're trying are breeding experiments. So apparently something like one in 10,000 bananas will produce a seed. Sometimes it like still slips through. So you can search bananas for that seed and then cross the cavendish with other species of
Starting point is 00:39:54 wild bananas. And so there are some efforts to cross breed, but the problem is like the Cavendish, it's actually an absolute marvel of a fruit. You know, it comes in its own packaging that ripens over the course of a week while it is in transit to you. So it arrives to you, mostly unbruised and now perfectly ready to eat. And the various crosses that they've done have produced bananas that are like, you know, maybe they're yellow. Maybe they still have a good, you know, outer coating. but so far they haven't been able to find anything that meets all of their criteria and is delicious. I was reading about one banana that looks like a cavendish and tastes good,
Starting point is 00:40:34 but it's described as an acid banana, which doesn't sound delicious, but it just doesn't taste like the cavendish. And so right now they haven't been able to find anything to replace the cavendish in what some people would say is a more sort of natural method. So that's where we are. Are we going to have a banana in one to two decades? We'll have to wait and see. Oh, my gosh.
Starting point is 00:40:55 Our children or our grandchildren might never know the taste of bananas the way we don't know the taste of the Gromyshell. I know. It could be tragic. I mean, think of how many babies had bananas as their very first food or something. Like, it could be that my kids' first foods were smushed up bananas. My memory is a sieve, so I don't know exactly what I fed them the first time, but it could have been a banana. And, you know, there's something else fascinating about bananas, which is that they are radioactive. Is that going to be the connection?
Starting point is 00:41:23 Don't give it away, Kelly. But yes, inside bananas, there's naturally occurring potassium 40, which is unstable. And the neutrons inside potassium 40 decay. And so if you are hanging around a banana, it will emit high energy electrons and anti-neutrinos, which is technically radiation. Oh, would we all be better off without bananas in our life? I don't know. Bananas contribute to the natural radiation background, which I'm sure affects the mutation rate. So it's made all of us who we are.
Starting point is 00:41:53 Oh, wow. Okay. On that deep dad poetry notes, let's find out if Matt found this answer satisfactory. And we'd also like to take this moment to thank Matt for being an amazing moderator of our Discord channel. And if you want to join us on Discord, go to Daniel and Kelly.org, not dot com. Although dot com appears to be a dead link now because the other Daniel and Kelly got married and their website is down. Which means either the wedding went wonderfully and they don't care about it anymore or, maybe something didn't go so well. Oh, man, I'm hoping for the former. Yes, good luck, Daniel
Starting point is 00:42:25 and Kelly. Yes. But please do join us on the Discord with lots of people are asking questions and having conversations about science and pizza and all sorts of crazy stuff. Go to Danielankelly.org to find the link to join the Discord. And let's hear what Matt had to say. That answer was beautiful. Thank you so much. Now I know more about banana suckers than I've ever wanted to know. And also, thanks for giving me a shout out on the Discord for being an administrator there. And we really do hope other people will join, just like Daniel said, please join us. We'll answer any questions you have. Have a wonderful day, guys. Thanks. A foot washed up a shoe with some bones in it. They had no idea who it was.
Starting point is 00:43:11 Most everything was burned up pretty good from the fire that not a whole lot was salvageable. These are the coldest of cold cases, but everything is about to change. Every case that is a cold case that has DNA right now in a backlog will be identified in our lifetime. A small lab in Texas is cracking the code on DNA. Using new scientific tools, they're finding clues in evidence so tiny you might just miss it. He never thought he was going to get caught. And I just looked at my computer screen. I was just like, ah, gotcha.
Starting point is 00:43:44 On America's crime lab, we'll learn about victims and survivors. And you'll meet the team behind the scenes at office. behind the scenes at Othrum, the Houston Lab that takes on the most hopeless cases to finally solve the unsolvable. Listen to America's Crime Lab on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. I'm Dr. Joy Harden Bradford, and in session 421 of therapy for black girls, I sit down with Dr. Ophia and Billie Shaka to explore how our hair connects to our identity, mental health,
Starting point is 00:44:17 and the ways we heal. Because I think hair is a complex language system, right? In terms of it can tell how old you are, your marital status, where you're from, you're a spiritual belief. But I think with social media, there's like a hyperfixation and observation of our hair, right? That this is sometimes the first thing someone sees when we make a post or a reel is how our hair is styled. You talk about the important role hairstylists play in our community, the pressure to always look put together, and how breaking up with perfection can actually free us. Plus, if you're someone who gets anxious about flying,
Starting point is 00:44:53 don't miss Session 418 with Dr. Angela Neil Barnett, where we dive into managing flight anxiety. Listen to Therapy for Black Girls on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast. Get fired up, y'all. Season 2 of Good Game with Sarah Spain is underway. We just welcomed one of my favorite people and an incomparable soccer icon,
Starting point is 00:45:15 Megan Rapino to the show, and we had a blast. We talked about her recent 40th birthday celebrations, co-hosting a podcast with her fiancé Sue Bird, watching former teammates retire and more. Never a dull moment with Pino. Take a listen. What do you miss the most about being a pro athlete? The final. The final.
Starting point is 00:45:34 And the locker room. I really, really, like, you just can't replicate, you can't get back. Showing up to locker room every morning just to shit talk. We've got more incredible guests like the legendary Candace Parker and college superstar AZ Fudd. I mean, seriously, y'all. The guest list is absolutely stacked for season two. And, you know, we're always going to keep you up to speed on all the news and happenings around the women's sports world as well.
Starting point is 00:45:59 So make sure you listen to Good Game with Sarah Spain on the IHeart radio app, Apple Podcasts, or wherever you get your podcasts. Presented by Capital One, founding partner of IHeart Women's Sports. The OGs of Uncensored Motherhood are back and badder than ever. And I'm Mila. And we're the host of the Good Mom's Bad Choices podcast, brought to you by the Black Effect Podcast Network every Wednesday. Historically, men talk too much. And women have quietly listened. And all that stops here.
Starting point is 00:46:27 If you like witty women, then this is your tribes. With guests like Corinne Steffens. I've never seen so many women protect predatory men. And then me too happened. And then everybody else wanted to get pissed off because the white said it was okay. Problem. My oldest daughter, her first day in ninth grade, and I called to ask how it was going. She was like,
Starting point is 00:46:44 All they were doing was talking about your thing in class. I ruined my baby's first day of high school. And slumflower. What turns me on is when a man sends me money. Like, I feel the moisture between my legs when the man sends me money. I'm like, oh my God, it's go time. You actually sent it? Listen to the Good Mom's Bad Choices podcast every Wednesday on the Black Effect Podcast Network.
Starting point is 00:47:06 The IHeart Radio app, Apple Podcast, or wherever you go to find your podcast. All right, we're back and we are answering questions from listeners. There's a special secret theme of today's podcast that's going to tie all of these questions together. Let's see how long it takes Kelly to figure it out. How many lifetimes? The next question is from Steve, who has a question about the biggest, gaseiest planet in the solar system. That isn't Uranus. Sorry, I had to.
Starting point is 00:47:44 Hi, Daniel and Kelly. This is Steve from BC, Canada. I have a controversial take here. Could it be said that there is no such thing as a gas giant? Because these planets have so much pressure that gas becomes liquefied. So aren't they really liquid planets? Maybe liquid giants? Sure, they are composed of liquid elements that are gaseous to earthlings living in earthly pressures, but they are not Earth, and they don't have earthly pressures. So we should be calling them liquid giants, don't you think? I think it's about high time that we do a deep dive into the inner workings of gas planets. What really are they?
Starting point is 00:48:28 All right. So Steve is asking a question about the science of Jupiter, but also about the name of the category that Jupiter finds itself in, gas giants. Are they really gassy? Should we be calling them liquid giants? These are good questions, Steve. These are great questions. Yeah, and you've got to tell Jupiter would lay off the beans. No, no, we're pro beans. Even if it makes you gassy, Katrina would tell me that beans makes everything better.
Starting point is 00:48:52 Nobody knows better than Katrina. She certainly does. She certainly does. All right, so let's dig into it. What in the end is Jupiter made out of? Well, Jupiter, like Earth and the Sun, formed from this big blob of stuff that the whole solar system was made out of. And, you know, the solar system is mostly just the Sun. Like, the Sun has not. 99. Something percent of all the mass in the solar system. Basically, you have a much larger cloud of stuff that our solar system and other solar systems formed from, but there was in there some seed, some gravitational over density that pulled stuff together to form our solar system. And mostly that just collapsed into the center. And most of it was hydrogen because that's what
Starting point is 00:49:32 the universe started out at, as in 14 billion years later, we're still mostly hydrogen. And so the sun is mostly hydrogen. But near the sun, there were also other little little. areas of over-density that managed to pull themselves together and hold themselves together and resist the sun's attraction. And that's how the planet's formed. So you get small rocky planets like Earth and the inner solar system because the sun then blew away their atmospheres. But far enough out away from the sun, the sun's radiation didn't blast away all the helium and hydrogen. And there was ice out there. Things were cold enough to form ice crystals. So you had a little bit of an advantage to make bigger planets that could grab a little bit more mass. So Jupiter is just a
Starting point is 00:50:11 scoop of the original proto-solar system that everything else is made out of. Oh, so it's a better representation of the proto-solar system than Earth? Yeah, absolutely. Earth once had an atmosphere of hydrogen the way that the sun does and the way Jupiter does, but it was blown away by the early sun. And so the Earth is not a great representation of what the solar system is. And actually, we're going to do an episode pretty soon about how we know what the universe is made out of.
Starting point is 00:50:34 And it was a big shocker when we discovered that most of the universe is not made of the same stuff as the Earth. the Earth is an unusual helping of solar system or universe material. Thankfully for us. Yes, exactly. Thank you for us. That's why we have bananas. No, that's not the secret theme.
Starting point is 00:50:51 So Jupiter is mostly hydrogen, right? By mass, the outside is like 76% hydrogen and then 24% helium and then just like trace tiny other stuff, like a little bit of carbon, a little bit of oxygen, a little bit of sulfur, a little bit of neon. But the atmosphere, which is just really an artificial designation of like a certain layer within Jupiter is mostly hydrogen and helium. What would be the arbitrary divider for Jupiter? I do think of Jupiter as being just gas all the way through.
Starting point is 00:51:20 And maybe that's just because it's called a gas giant. So what is the dividing line or dividing criteria for the atmosphere versus the interior? Yeah, so it's a little bit arbitrary, but basically you have layers of stuff that get denser and denser as you go in. So you start out the very outer layers of Jupiter are cloud. layers. And so these are like ammonia crystals, there's really high winds, but it's mostly gaseous hydrogen with these clouds of ammonia crystals. And that's what you see when you look at Jupiter, you know, like the rings and the red spot and all this stuff. These are like
Starting point is 00:51:53 weather patterns in those clouds in the very, very top layer of Jupiter's atmosphere. But then once you penetrate through those layers of clouds, like 50 kilometers of clouds or so, below that there's liquid hydrogen, right? And so hydrogen is an atom, but it also forms H2, which is a molecule, and then it has various phases. And it depends on the temperature and depends on the pressure. And so you start out with gaseous hydrogen, and then you squeeze it down and you get liquid hydrogen. And so this stuff flows, right? It's just denser. And so you might say, all right, we're not really in the atmosphere anymore because now we have a liquid. And, you know, here on Earth, we consider the atmosphere the gaseous part. And then the surface,
Starting point is 00:52:36 is where you have like solid rock and also liquid. But it's not quite so simple on Jupiter because it's not as clear and crisp. Like here on Earth, you know, you have liquid and above it is gas. And like if you're swimming in the ocean, you can very clearly tell the crisp difference. But on Jupiter, they don't really have the same distinct transition between liquid and gas. And so you have this like gradual transition between gaseous hydrogen and liquid hydrogen. What's really going on here is that molecular hydrogen, if you look at its phase diagram, am. There are some pressures and temperatures where it's gas and some pressures and temperatures
Starting point is 00:53:10 where it's liquid. But there's this critical point, this temperature and pressure above which it's not really gas and not really liquid. And this transition is sort of, therefore, gradual. There's this sort of super critical fluid. It's not really technically a liquid. It's not really technically a gas. It has some similarity to both. And so the reason you can't just say like, oh, this is the surface of Jupiter is that as you descend, it just sort of gets denser and denser until eventually it feels like liquid. And if you rose back up, it would get less and less dense, and then it would just sort of feel like gas.
Starting point is 00:53:42 But it's a gradual transition rather than an abrupt one the way it is here on Earth. I see we have yet again accidentally forayed into chemistry. But I understand it better now. And as you descend, the weather gets really, really weird. So you get this like helium neon rain. What? Yeah, I know. It's really crazy.
Starting point is 00:54:00 And not something I think you should dance and sing in, for example. But there's just sort of rain-like droplets. And what's happening is that you have helium and neon in the upper atmosphere, but they come together and form these drops, which then sink and depleting the abundance of these elements in the upper atmosphere. And they fall down to lower levels of the atmosphere. And this is all very speculative. You know, there are people who think, for example, like on Saturn, there might be conditions that cause diamonds to rain, you know, like formation of diamonds in the atmosphere because the intense pressure, which then fall below. But a lot of this is speculative. This is like people running models and thinking maybe this is what happens.
Starting point is 00:54:37 And it's super cool. But, you know, the big picture story here is that we really don't understand this stuff. A lot of this is just speculation. Which is why we need more money to go out there and find out. We definitely do. And then things get even weirder. As you squeeze it down, as you go down further towards the center of Jupiter, you're getting higher temperature and higher pressure. Then you reach this region where the hydrogen is metallic.
Starting point is 00:55:00 And metallic is a really weird term to apply. to hydrogen because in astronomy, usually they say, well, you have helium and you have hydrogen, everything else they call a metal. So if you talk about the metallicity of stars, it means how much of the star is not hydrogen, how much of it is not helium, everything else they call a metal. Chemists have a different meaning for what is a metal, right? They're thinking about things where the electrons are flowing because the atoms are sort of linked together and the electrons are not attached to individual atoms.
Starting point is 00:55:29 And that's what we're talking about here. This is like the chemical version of a metal. Does it mean that the atoms are flowing? Are we using the chemistry definition now? Yeah, we're using the chemistry definition because what happens is you take those H2 molecules, you squeeze them together and the hydrogen forms something like a lattice, right? Instead of having individual H2 molecules, which have some interaction, you know, because of the polarity of them.
Starting point is 00:55:52 Now you're squeezing them together so the electrons can just jump from one hydrogen to another hydrogen to another one. It's like a big crystal. It's not quite as tight, but it conducts electricity, right? Normally, hydrogen does not conduct any electricity, but you squeeze it together, you make it dense enough, it will conduct. And so it has this like bulk lattice phase with de-localized electrons in it. And this is something people have been thinking for decades and decades, and only the last few
Starting point is 00:56:18 years have they been able to convincingly make this stuff in the lab by recreating these conditions and seeing it actually conduct electricity. So this is this huge chunk of Jupiter, which is hydrogen squeezed so tight that we think It's basically one enormous conductor. So when you touch metallic hydrogen, is it hard, like the metals that I am thinking of? Or are we still in a sort of like gassy, liquidy kind of phase? Yeah, great question. Not something we understand super well, but I don't recommend you lick it if somebody has some metallic hydrogen.
Starting point is 00:56:51 It's hard to imagine what it would be like to touch it because you can't have it around unless it's under very, very high pressure. So it's not like somebody could hand you a chunk of metallic hydrogen that you could like even consider licking. Okay. It's just going to be like super duper dense material. Got it. Okay. I don't want to die for this podcast. Probably not tasty.
Starting point is 00:57:08 I'd recommend a banana for a snack instead of metallic hydrogen. Wait, hold on. What is the connection then? Is the connection that there's a part of Jupiter that's solid like a banana? And the equipment we use to study neutrons is solid too? Daniel, I just don't know. Well, Jupiter is active, right? The same way the sun is, it's a big hot thing.
Starting point is 00:57:27 And so it radiates. There's no fusion going on inside Jupiter. but you know the pressure and the temperature are very high and so there is a lot of radiation being emitted. If you wanted to, for example, establish a base on one of the moons of Jupiter, you really have to worry about the Jupiter wind, the Jovian winds, very high energy particles shooting at you. So just like a banana and just like a neutron, you have to worry about radiation if you're going to live near any of these things. Radiation is the theme. It's a particle, of course. I'm not trying to be tricky about it. Well, I got it before the end of the episode almost.
Starting point is 00:58:03 So, bravo, Kelly. Congratulations. You get a banana. If I had a grow, Michelle, I would share it with you. Oh, thank you. So then we can dig down even deeper into Jupiter, and eventually you get to stuff that's not hydrogen. So we think there's a really thick atmosphere. Metallic hydrogen is up to like maybe 80% of the radius.
Starting point is 00:58:19 If you go down to like 30 to 50% of the radius of Jupiter, there is stuff down there that's solid. It's like made of rock, the same kind of stuff that the Earth is made out of. And it's not small. It's like 30 to 50% of the radius of Jupiter. It's a really big chunk of ice and rock. But, you know, it's buried under an incredibly thick layer of hydrogen. And so if you're really hardcore about it, you could say, well, that's the surface because
Starting point is 00:58:43 everything else is a gas. It's hydrogen. But, you know, it's not in a gas phase. It's in a metallic phase or it's in a super critical fluid phase. And so you could, if you dove really deep into Jupiter, stand on a rocky, quote, unquote, surface. But I don't think you could still call Jupiter a rocky planet. All right, yep. I'm giving it to the astronomers.
Starting point is 00:59:03 I think gas giant is a reasonable name. And also it gives many school kids lots of chuckles. And so I think it's great. Yeah, but it is confusing, right? Because we call it a gas giant because it's mostly made of hydrogen. But hydrogen is not always in a gaseous state, especially in Jupiter. Most of the gas on Jupiter is metallic. So you could also call it a metallic giant and be like kind of correct.
Starting point is 00:59:25 That does sound cooler. It does sound more metal. That's right. That's right. All right. So I think we've concluded that astronomy names are very confusing and maybe there's no way to do it right. But it's fun to dig into anyway. And so Steve from BC, let us know if we answered your question about Jupiter. Thanks, Daniel and Kelly, for answering my question. That was really insightful to know that Jupiter could be really a metal giant. But it makes me think now about how we've named Earth.
Starting point is 00:59:55 You know, Earth has a lot of gas and we depend on that gas. And, you know, Now, how much different is the amount of gas and rock ratio than Jupiter? I mean, would it be correct to say that Earth is a gas midget? Thanks again for answering my question. You're still my favorite podcast. Keep the great answers coming. And thank you for being such great science communicators. Well, thank you for all of the wonderful questions we got today.
Starting point is 01:00:19 And we hope to hear from you. Send us your questions at questions at Danielankelly.org. We answer every question and some of the questions even end up on the show. We do love to hear from you, and we love to hear that you are curious, that you share our passion to understand the universe, how it works, from the bananas all the way out to the galaxies. So join us on the Discord, write to us at Questions at Daniel and Kelly.org. Let us know you're out there. Daniel and Kelly's Extraordinary Universe is produced by IHeart Radio. We would love to hear from you.
Starting point is 01:00:56 We really would. We want to know what questions you have about this extraordinary universe. We want to know your thoughts on recent shows, suggestions for future shows. If you contact us, we will get back to you. We really mean it. We answer every message. Email us at questions at danielandkelly.org. Or you can find us on social media.
Starting point is 01:01:17 We have accounts on X, Instagram, Blue Sky, and on all of those platforms, you can find us at D and K Universe. Don't be shy. Write to us. I'm Dr. Scott Barry Kaufman, host of the psychology podcast. Here's a clip from an upcoming conversation about how to be a better you. When you think about emotion regulation, we're not going to choose an adaptive strategy which is more effortful to use unless you think there's a good outcome.
Starting point is 01:01:46 Avoidance is easier. Ignoring is easier. Denials easier. Complex problem solving. It takes effort. Listen to the psychology podcast on the iHeart Radio app, Apple Podcasts, or wherever you get your podcasts. We're siblings. Like, you fight, you disagree. It's really hard to be in a partnership. You judge. Yeah, you judge each other.
Starting point is 01:02:07 You lead differently. And we've gotten to that edge. Hey, I'm Simone Boyce, host to The Bright Side. And this week, I'm joined by Hollywood Power Sisters, Aaron and Sarah Foster. They're getting real about boundaries, rejection. Plus, what's next for their hit Netflix series, nobody wants this. Listen to The Bright Side on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast.
Starting point is 01:02:30 I always had to be so good, no one could ignore me. Carve my path with data and drive. But some people only see who I am on paper. The paper ceiling. The limitations from degree screens to stereotypes that are holding back over 70 million stars. Workers skilled through alternative routes rather than a bachelor's degree.
Starting point is 01:02:50 It's time for skills to speak for themselves. Find resources for breaking through barriers at tailorpapersealing.org. by Opportunity at Work and the Ad Council. 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,
Starting point is 01:03:11 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. 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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