Daniel and Kelly’s Extraordinary Universe - Listener Questions #5

Episode Date: February 11, 2025

Daniel and Kelly answer questions about chain reactions in space, the chemistry of life, and how a theory is accepted.See omnystudio.com/listener for privacy information....

Transcript
Discussion (0)
Starting point is 00:00:00 This is an I-Heart podcast. December 29th, 1975, LaGuardia Airport. The holiday rush, parents hauling luggage, kids gripping their new Christmas toys. Then, everything changed. There's been a bombing at the TWA terminal. Just a chaotic, chaotic scene. In its wake, a new kind of enemy emerged, terrorism. Listen to the new season of Law and Order criminal justice system on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts.
Starting point is 00:00:40 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, denial is easier, complex problem solving, takes effort. Listen to the psychology podcast on the IHeart radio app, Apple Podcasts, or wherever you get your podcasts. Hi, it's Honey German, and I'm back with season two of my podcast, Grasias, come again. We got you when it comes to the latest in music and entertainment with interviews with some of your favorite Latin artists and celebrities. You didn't have to audition?
Starting point is 00:01:23 No, I didn't audition. I haven't auditioned in like over 25 years. Oh, wow. That's a real G-talk right there. Oh, yeah. We'll talk about all that's viral and trending with a little bit of cheesement and a whole lot of laughs. And, of course, the great bevdas you've come to expect.
Starting point is 00:01:38 Listen to the new season of Dresses Come Again on the Aheart Radio app, Apple Podcast, or wherever you get your podcast. Every case that is a cold case that has DNA. Right now in a backlog will be identified in our lifetime. On the new podcast, America's Crime Lab, Every case has a story to tell, and the DNA holds the truth. He never thought he was going to get caught, and I just looked at my computer screen.
Starting point is 00:02:05 I was just like, ah, gotcha. This technology's already solving so many cases. Listen to America's Crime Lab on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. Are black holes actually black? always built on a carbon stack? Can one star make another explode? What happens if you lick an electrode? Would biology beat physics
Starting point is 00:02:34 in a fair fight? Why is dark chocolate better than white? Hawking predicted that black holes glow. What makes a supernova blow? Biology, physics, archaeology, forestry, really anything other than chemistry. What diseases do you get from your cat? Well, we'll find the answers
Starting point is 00:02:52 to all that. Whatever questions keep you up at night. Daniel and Kelly's answer will make it right. Welcome to another listener questions episode on Daniel and Kelly's Extraordinary Universe. Hello, I'm Kelly Wienersmith. I'm a parasitologist, and today we're talking about chemistry. Hi, I'm Daniel. I'm a particle physicist. Because I don't like chemistry. So what am I even doing here today?
Starting point is 00:03:29 Well, so, Daniel, my question for you today is why is chemistry the worst science? How much time do you have, Kelly? I mean, we've got an hour. No, chemistry is amazing because it's the closest thing we have to explaining magic, like the things that you can see happen with your own eyes. You know, seeing a solid turn into a liquid, turn into a gas is kind of incredible. and the fact that we can take that apart and understand it microscopically is amazing.
Starting point is 00:03:58 And it's so much more concrete than particle physics or even astrophysics sometimes. So I have a lot of respect for the relevance of chemistry, but I really struggle with the complexity of it. Like there's so many different rules to apply in different situations and always to remember all the exceptions and this electron and that electron. And it doesn't have the simplicity that I like in particle physics.
Starting point is 00:04:21 But, you know, hey, that's purely a subjective preference. right? And I'm really glad that there's different kinds of science for different kinds of folks. So we get all the fun different kinds of sciences happening here on our planet. Yeah. No, I agree. And I'm joking. My senior honors research project was in organic chemistry. I minored in chemistry. But man, it was hard taking O-chem over the summer because I'm not good at visualizing things in 3D and seeing those reactions happen in my head is really hard. But I got lucky. So I took it over the summer and it was like four hours of lecture and then two hours of lab like every day of the week. It was intense. I had a group of friends. I was one of six. We called ourselves the benzene
Starting point is 00:04:59 ring because there's six carbons in a benzene ring. I got a chemistry joke. Yay! And we would pull all-nighters on Thursday nights to study for the Friday exams. And I will always think fondly of those people who got me through like the hardest summer of my life. But anyway, I like it. I just find it way harder than just about anything else I have to think of. But, you know, I take a lot of medications then I'm sure would not be around but for the miracle of chemistry. Exactly. I'm ever so grateful for chemistry. And though I take every opportunity to make fun of chemistry,
Starting point is 00:05:31 I also want to make sure people out there understand that I have a lot of respect for it, of course, as a science. And I will say that there are a few listeners who are chemistry professors who write in and say, don't worry, keep joking about chemistry. It makes me laugh. Good, yes. I joke about it the same way I joke about a sibling, where it's like you love them, you're picking fun at them. If somebody else does it, you get a little defensive.
Starting point is 00:05:52 But yes, no, I love chemistry. It's just, man, my brain was not made for chemistry, but I'm so glad other people's brains are. And chemistry, like all kinds of science, inspire people to ask questions, to wonder, like, how does this work? How does this fit together? What are the rules for this? And if you have questions about physics or biology or even chemistry, please write to us and ask your questions. We would love to dig into it to understand the benzene rings and everything else about the universe. We'll bring another expert on to explain them.
Starting point is 00:06:24 And today on the podcast, we'll be doing just that answering questions from listeners. We have a lot of fun questions, including questions about chain reactions in space, which is sort of like super space chemistry, a question about the chemistry of life and a question about what it all means and how we know when to accept a scientific theory. An amazing set of questions. Let's get started by hearing what Tim wanted to know about. I was just listening to your podcast about the brightest thing ever seen in the universe. And it got me thinking is there's such a thing as an event where maybe a chain reaction explosion in space. Maybe it's a binary system supernova with the other star go nova as well. Or instead of maybe just disintegrating planets, is it possible for like the core of a planet to heat up so that? it explodes, just peaked by curiosity and thought I'd ask the question. Thanks.
Starting point is 00:07:23 Whoa. All right. So I can imagine like looking out at the stars at night and seeing like things starting to explode in a chain reaction and being like, I should have put my kids to bed before this happened. So they couldn't see it. Yeah, I was wondering what inspired this question. Maybe Tim was worried that like if something goes wrong in one star and ends cataclysmically if it could set off a chain reaction that like destroys the whole universe or something. or if we're safe because every star is so far from the other stars that their fates are all independent. Sounds like Tim and I would have a good time catastrophizing together on a Friday night. But it's a great question because it makes us think about the relationship between one star and another
Starting point is 00:08:02 and also what it takes to like send a star to explode or to disintegrate a planet. It is a fun question. It sort of thinks about the whole universe as if they were elements of a chemical reaction, right? That's true. But let's start with what's happening inside of one star and then we'll scale up. to multiple stars. You do have chain reactions happening in each star, right? That's right. Yeah. And a chain reaction essentially is a reaction which sets the stage for itself, you know, which makes it more likely for it to happen. And so like a fire is a chain reaction because the combustion
Starting point is 00:08:33 produces heat and that heat triggers more combustion. And so there's a loop there, right? Or a chain or one link leads to the next link. And as you say, inside a star is a sort of a chain reaction because we have fusion happening inside a star. You have gravity squeezing this hot ball of hydrogen and maybe a little bit of helium together. And it creates the conditions necessary for fusion, heat and density. And then fusion itself produces more heat. And that increases the chances of fusion. The odds of getting fusion grow very steeply with temperature. So the hotter it is, meaning the faster those particles are whizzing around, the more likely you are to have fusion. So heat makes fusion more possible.
Starting point is 00:09:15 Now we have to get to the really exciting part, which is the explosions. Are explosions the result of all of the fusion getting out of control? No. When do we get the explosions? Yeah, essentially. You can think of a star during its normal lifetime during that millions or billions of years that it's burning stably before it explodes as in something of a balance, right? You have gravity squeezing in, right, making things hot and dense. And what it would like to do, if it wasn't constrained, is turn that into a black hole. Right. Gravity is always just pushing and pushing and pushing. And if there was nothing else but gravity, everything would collapse into a black hole. But in the star, you have lots of forces resisting gravity. And when the star is burning, the primary force at the frontier resisting gravity is fusion itself, which is pushing out with radiation, right? It produces all this heat, this energy. It's pushing the star out. So fusion is pushing the star out. Gravity is pushing the star back in. And there's a balance there. And if you upset that balance, then yes,
Starting point is 00:10:13 the star can go kaboom. And there's basically two ways for the star to go supernova. There's the core collapse supernova, and then there's the special fancy type 1A supernova. And the core collapse is the one that we mostly think about. This is like the sort of vanilla supernova. What happens is that fusion is doing its job. It's turning hydrogen into helium.
Starting point is 00:10:35 And then if it's hot enough, it's turning helium into carbon. And if it's hot enough, it's turning that carbon into neon and oxygen and all sorts of heavier stuff all the way up to. to iron, but fusing those heavier elements requires more temperature. So a star might not be hot enough to fuse a certain element. For example, right now, our star can fuse hydrogen, but it can't fuse helium. So what happens to the helium at the core of our star? It just sits there and kind of gets in the way. It's like ash. It's like the product of a fire. And if you have too much of that without climbing over that temperature threshold where you can burn it also, it starts to put the fire
Starting point is 00:11:12 out. So smaller stars reach their hottest temperature and can't burn something. So, for example, our star can't burn helium. If the star was larger, it would get hotter at its core, and it would burn a heavier element, or a heavier element, or an even heavier element, all the way up to iron. When you get up to iron, no star can burn iron and produce energy, because when you fuse iron together, it actually costs energy. It cools the star. So the short version of the story is, At some point, you've done so much fusion and you've made something that you can no longer burn that's interfering with your fusion. And so fusion is failing.
Starting point is 00:11:47 And gravity starts to win. And the star starts to collapse because remember the reason it wasn't collapsing was fusion pushing out against gravity. And now you've knocked out those supports. Gravity wins. The star implodes. And that implosion then triggers a moment when the star is hot enough to do stuff like burn iron and make super heavy elements. And that triggers the explosion, which is the supernova.
Starting point is 00:12:12 So the core collapsed supernova comes when the core is not hot enough to burn the ash that's left over, which then triggers the collapse and then an explosion. That was a great explanation. Okay, so you said, our sun is not hot enough to make iron, so we've got a bunch of helium. Does it matter what form the ash takes? They all explode no matter what kind of ash is made, or do you get a different result if the ash is helium versus if the ash gets to? the iron phase.
Starting point is 00:12:37 Yeah, so not every star is going to go supernova. Like, for example, our star is not going to go supernova. It's not big enough. It's going to accumulate a lot of helium at its core. And then near the very end, it's going to have a brief moment, like maybe minutes in the billions, year-long life cycle of the star, where it can burn that helium in a helium flash and make a little bit of heavier stuff, but it doesn't have enough gravity to actually collapse.
Starting point is 00:13:02 Fusion is going to happen in the outer layers because the core is going to be cold helium. And then you're going to have this helium flash and it's going to blow off those outer layers. And you're going to be left with a white dwarf, which is just a hot blob of stuff. It's not fusing anymore. It's just like a big rock sitting there in space glowing. Just a white dwarf. If it were bigger, then it would have enough gravity to actually collapse and cause a supernova. So our star is not going to become a supernova unless, right, there is a route for white dwarves to become supernovas.
Starting point is 00:13:33 White dwarves are just hot stuff sitting there in space, not fusing. Gravity is trying to squeeze them, but it's resisting because of the chemical strength of the stuff. The same reason why, like, the Earth doesn't collapse into a black hole. It's got chemical strength supporting it. But if something comes along and pours extra material onto the white dwarf, then it can increase its gravity, and gravity can overcome that strength and cause it to collapse and make a special Type 1a supernova. This happens if you have a white dwarf that has, like, a sister star nearby,
Starting point is 00:14:03 and it eats some of that sister star, and then it gets triggered. into a supernova. So that's the second kind of supernova. So our star could eventually have a Type 1A supernova, but it's not going to have a core collapse supernova. So, have we already gotten to part of the answer then for why you don't get chain reactions because some of the stars in between can't explode.
Starting point is 00:14:25 They're just not the right kind. They're little. They don't have sisters. They can eat. Why do we always get to cannibalism? I don't know. We do. And so you can't get the chain reaction
Starting point is 00:14:34 because there's a lot of stars, you know, in the line that are just not capable of exploring. Yeah, you need the right kind of star. And so the answer to this question is that it's very unlikely to have lots of chain reactions, but it could be possible if you set up the conditions just perfectly. And I'm a big science
Starting point is 00:14:50 fiction reader. And so when I got this question from Tamer was reminded of this snippet from a Larry Niven novel Ringworld. And there's a scene where they talk about how in the center of the galaxy the stars are all packed together really, really close. One star goes Nova. It releases a lot of heat.
Starting point is 00:15:06 gamma rays and that heats of the neighboring star which would then blow and it sets off a chain reaction. So it's super cool idea that you can have this like set of fireworks going off in the galaxy. But in order to make this work, you really need exactly the right conditions. And what he describes in Ringworld probably wouldn't happen the way he described it, because adding heat to a star doesn't actually cause it to explode. Remember we talked about core collapse supernova. The reason they collapse is because they're not hot enough. They can no longer do fusion to burn the ash that's at their core. So adding heat to a star actually supports it, actually makes it more likely to live longer. It prevents its collapse. It doesn't trigger its
Starting point is 00:15:47 collapse. These stars explode because they no longer have fusion happening at their core. Is that true even if the ash is iron? Like the end of the process, even adding more heat won't help? Yeah, exactly, because the process of fusing iron saps heat from the core. So you have a bunch iron there and the star is trying to fuse it, but that fusion process is gobbling the energy instead of creating energy. It's like the opposite of a chain reaction. And if you have an external source of heat that's fueling that, that's providing that energy, then you can sustain the star longer. So a core collapse supernova isn't triggered by external heat, like radiation from another star. But the other kind of supernova, the type 1A supernova, is triggered externally, right? You have a
Starting point is 00:16:31 white dwarf, which otherwise wasn't going to go supernova, and you get a deposition of new material from some neighboring star, that does trigger it to go over this threshold and then go supernova. And so I asked a friend of mine, David Vartagnan, he's a scientist who studies supernovas. He's a Hubble Einstein fellow with the Carnegie Observatories, and he said, quote, this may be possible for thermonuclear supernova, which requires some version of runaway nuclear chain reactions on the stellar surface. It's possible to chain this if situations are just right. So the idea is that you have like a series of these white dwarves and you add material to one of them, it goes supernova and then deposits material on the next nearby white dwarf, which
Starting point is 00:17:13 causes that to go supernova. Dot, dot, dot, dot. You have a chain reaction. So do my kids have anything to worry about? No, your kids do not have anything to worry about. But if you are designing a universe and you want to see this happen, you might be able to arrange it. So if your kids grow up to be God or masters of their own domain, they could set up a supernova chain reaction if they so desire. Malevolent gods, not the nice ones. Also, Vartagnan, super cool last name, like the polar opposite of Wienersmith. I guess maybe it reminds me of D'Artagnan, like the Three Musketeers.
Starting point is 00:17:46 Okay, on that note, let's get back in touch with Tim and see if he feels like his question was answered. Thanks for the awesome question, Tim. Hope you like the answer. Oh, thanks for answering my question, Daniel and Kelly. Yeah, you answered it. I'm pretty excited to know that under the right circumstances, it can happen so that it's possible, but it doesn't sound like we're going to have a spectacular fireworks show up exploding stars in our night sky anytime soon.
Starting point is 00:18:14 So glad your kids are safe, and thanks for answering my question. December 29th, 1975, LaGuardia Airport. The holiday rush, parents hauling luggage, kids gripping their new Christmas toys. Then, at 6.33 p.m., everything changed. There's been a bombing at the TWA terminal. Apparently, the explosion actually impelled metal glass. The injured were being loaded into ambulances, just, a chaotic, chaotic scene.
Starting point is 00:18:59 In its wake, a new kind of enemy emerged, and it was here to stay. Terrorism. Law and Order Criminal Justice System is back. In season two, we're turning our focus to a threat that hides in plain sight. That's harder to predict and even harder to stop. Listen to the new season of Law and Order Criminal Justice System on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast.
Starting point is 00:19:27 My boyfriend's professor is way too friendly, and now I'm seriously suspicious. Oh, wait a minute, Sam. Maybe her boyfriend's just looking for extra credit. Well, Dakota, it's back to school week on the OK Storytime podcast, so we'll find out soon. This person writes, my boyfriend has been hanging out with his young professor a lot. He doesn't think it's a problem, but I don't trust her. Now, he's insisting we get to know each other, but I just want her gone. Now, hold up.
Starting point is 00:19:53 Isn't that against school policy? That sounds totally inappropriate. Well, according to this person, this is her boyfriend's former professor, and they're the same age. And it's even more likely that they're cheating. He insists there's nothing between them. I mean, do you believe him? Well, he's certainly trying to get this person to believe him because he now wants them both to meet. So, do we find out if this person's boyfriend really cheated with his professor or not?
Starting point is 00:20:14 To hear the explosive finale, listen to the OK Storytime podcast on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast. I'm Dr. Joy Harden Bradford, and in session 421 of therapy for black girls, I sit down with Dr. Afea and Billy Shaka 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 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. We talk about the important role hairstylists play in our community,
Starting point is 00:20:59 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, 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,
Starting point is 00:21:19 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, 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. And the locker room. I really, really, like, you just, you can't replicate,
Starting point is 00:21:54 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 00:22:14 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. All right, so next we have a question from Julian from our Discord. Daniel, if somebody wants to play with us on Discord, where do they find the link to our Discord? Go to our website, www.danielandkelly.org, and you'll see an invitation there to the Discord. wherever you can come and talk and ask questions and make silly jokes. And be our friends.
Starting point is 00:22:55 All right, so let's listen to a question from a New Zealander. Hi, Daniel and Kelly. I'm Julian from New Zealand, a long-time fan of the pod. What I'm interested in hearing is your opinion on the possibility of non-carbon-based life. Given the practically infinite size of the universe, it seems to me that we should consider other life chemistries as probable rather than possible. But I'm interested to hear your thoughts on this. and whether there would be any practical way for us to search for biomarkers from other life forms. Thanks and keep up the great work. Bye. I love this kind of question because it takes us like out of the mindset that life on Earth is the only way life can be.
Starting point is 00:23:34 So I'm dying to hear your thoughts about this, Kelly. Yeah, well, so I was really excited when I got this question because it had the word life in it. And then as I dug a little farther in, I realized this was a chemistry question. And I remain excited. But here we go. let's do this. All right. So there's about 94 naturally occurring elements on the periodic table, but the scaffold for life seems to be made of carbon in every case that we've ever looked at. So why carbon and why not something else? So there's 94 naturally occurring elements. So you're talking about basically
Starting point is 00:24:07 the building blocks of life out there in the universe. But if we're starting on a rocky planet, I guess we're assuming that there's like a good chunk of silica and carbon and this kind of stuff because that's what you need to make a rocky planet, right? Yep. All right, cool. You said that the sun makes everything up to iron. Is that right? Yeah, that's right.
Starting point is 00:24:26 So we would expect everything up to iron to be fairly plentable in the universe. Is that fair to say? Yeah, although there's a fascinating distribution of which elements are more common and which ones are less common, which involves a lot of chemistry. We'll dig into it one day. So the three criteria to sort of like enter us in here is one, abundance. So you wouldn't expect no bellium to be the best. to be the backbone for life because there's not a lot of it out there.
Starting point is 00:24:50 But the more common things, you know, they'd be easier for organic organisms to find and incorporate into their bodies. And so what are some of these common atoms? So the universe is mostly hydrogen, you know, because we started with hydrogen and stars have been making heavier stuff for a while, but we're pretty early on in the history of the universe. So mostly hydrogen, like 74% of the universe by mass fraction is hydrogen. And then a big chunk of it is helium, so like 24% of it. which is already like most of the universe. You've got 74% plus 24% leaves only 2% of the universe is left.
Starting point is 00:25:25 But the next one is kind of a surprise. It's oxygen. Right. Oxygen is much more common than anything else. That's not hydrogen or helium. And then you got carbon and neon and then iron. So those are the most common building blocks in the universe. Okay.
Starting point is 00:25:40 All right. So let's go from there. So, all right. So abundance is criteria one. Yeah. So you need stuff that's abundant. So we're not surprised to find out that it's carbon. Although carbon, as you're noted, is not as abundant as things like hydrogen,
Starting point is 00:25:51 but there's still plenty of it on Earth, for example. And then the next criteria is that it needs to be versatile and able to make a lot of complex molecules. So the proteins that we have, these are very complex. They fold up in different ways. They're made up of lots of different kinds of elements. And the signaling molecules that bacteria make, like every biological organism has lots and lots of super complex molecules that it uses to carry out all of its various functions.
Starting point is 00:26:18 So it's thought that ideally you would end up with atoms that are able to bind with the most stuff. And as we move our way across the periodic table, moving across the columns, when you get to the column that carbon is at the top of, the stuff in that column are able to bond with four other things. And the reason for that is that they've got, now we're getting into electron shells. And I totally went down a like mental rabbit hole being like, like, oh, but electrons, they're not really like particles. Does it make sense to think of them
Starting point is 00:26:49 this way in shells anymore? Because maybe their entire functions and let's not go down that rabbit hole for today. Or maybe we should. No, in terms of bonds, I think it's totally reasonable to count the number of electrons because even if electrons are waves or particles or something else, alien, they follow the rules of quantum mechanics, which dictate how many you can have in each energy level. And that's what determines the whole structure of the periodic table, right? The reason we put carbon and silicon and germanium and tin and lead in the same column is that they all need four electrons to complete a shell and if all of the electrons are filled in the shell then the atom doesn't like to interact very much is very happy and so carbon and silicon both need four
Starting point is 00:27:30 electrons to complete their shell and so i think you're saying that's why they like to interact with four things so they can interact with as many as four things or they can interact with fewer and have like double bonds with one of those things for example but their ability to interact with the maximum number of things that you can get interactions with on the periodic table allows them to form these super complicated molecules that are necessary for complex life. So can I ask you a naive chemistry question? Like, I don't understand why carbon is in this situation where it can make the most bonds. Like, I get that it has four valence electrons out of the octet, and so it needs four more.
Starting point is 00:28:09 But then you got nitrogen. It's got five. Why can't it use its five electrons? or you got boron, it's only got three. It could take five more electrons. Why can nothing make five bonds? Well, good start. Okay, nitrogen tends to bond with three other things to fill its eight, to get to eight,
Starting point is 00:28:27 whereas boron tends to donate its three to other things, as opposed to bonding with five things. I see. So carbon sits right there in the sweet spot out of the octet. It's got four so it can make four bonds. That's pretty cool. Yes, and so it's in the position to be the backbone four, are the most complicated kinds of molecules that you can make.
Starting point is 00:28:45 I have another basic question, which is like, why do we call life carbon-based? Like, I get carbon is useful, but like, why can't we just have a big mix of different kinds of chemistries? Why does carbon have to be in everything, in every part of life? So I think part of why we end up with a lot of carbon as the backbone to a lot of this stuff is because carbon not only can bind with a lot of things, but it also forms really strong bonds, so it's stable. the kind of molecules that it makes are stable.
Starting point is 00:29:13 So, for example, if you moved down the column that has carbon to other things that are also able to bond for things, silicon can also bond for things, but that bonding is happening in an even farther out shell. And because it's farther away from the nucleus, the bonds that it forms are less strong. You're saying that silicon is like carbon in the outermost electron orbitals, but it's a more complex heavier nucleus. So it's got more electrons. so this outermost electron orbitals are further from the core and they're not as tightly bound and so things are a little more loosey-goosey. Yeah, so carbon has two shells, an inner shell with two electrons and then this outer shell with four and then the ability to bond to four other things.
Starting point is 00:29:53 And then silicon has three shells. And so it's got two in the center, eight the one out from that, and then it's got four in the outer one and the ability to bind with four other things. But because that shell where the binding is happening is farther away from the nucleus, the bonds that it produces are weaker. And so the thought is that when chemical reactions happen, a lot of times what's happening is that one of the things that bonds to, for example, like a carbon backbone, you know,
Starting point is 00:30:22 gets sort of like pulled off when a reaction happens. And when something gets pulled off, carbon is strong enough that the backbone stays together and that molecule stays complete. But when you've got silicone as the backbone, when something breaks off as part of reaction, that process of breaking off could also break the backbone of the silicon. And so the idea is that carbon is not only something that allows you to make super complex molecules, but it's also strong enough to allow reactions to happen.
Starting point is 00:30:51 I think if you had anything else that was like creating the backbone for these complicated molecules, the thought is they wouldn't be complex enough or they wouldn't be strong enough to survive reactions. So you need some sort of backbone to hold things together while you have this sort of interaction, these chemistry of life happening. Yes, yes. And so through this conversation, we've hit on the three criteria, the abundance, versatility and complexity, which is those bonding sites, and then the stability when reactions are happening.
Starting point is 00:31:20 So those are the three things that we think are most important. We've talked about why silicon is thought to maybe not be ideal for these reactions. So you'll often hear discussions about, like, well, could life be silicon? based. And one reason we think that's unlikely is because you might get a lot more breakdown of chemical structures when reactions happen. But another thought, water is really important for a lot of biological processes. In fact, when we look to see where we think life is in the universe, one of the criteria we use is whether or not there's water there. Water is a helpful solvent, which means it helps move around like nutrients and molecules and stuff like that. But when carbon binds with
Starting point is 00:31:59 water, you make carbon dioxide, which is like a gas that like we can breathe out. But when silicon binds with water, you make silicon dioxide, which is sand. And so it's thought that sand is probably not something that's like conducive to the creation of life. And so that is another proposed reason why we don't see silicon based life forms. Although some labs have managed to do like directed evolution studies to get more silicon into molecules. But I feel like that's very different than a molecule as part of a living being that has no carbon at all. So that all does make sense to me as an explanation for like why the kind of life that we have needs carbon and why having even silicon wouldn't make the kind of life we have possible.
Starting point is 00:32:47 But it doesn't convince me that a totally different kind of life wouldn't be possible. I mean, if we sat here before there was any life and we were just like looking at atoms and speculating like, hey, what could be complicated enough to have weird? things like life arise, I don't know, that we would have been able to predict, like, carbon is useful. There's a lot of complexity in the universe that we fail to predict. So isn't it possible that silicon is complex enough to do something else, which could be the basis of life, even if it's, like, very different and maybe even pretty sandy? Yeah, I think maybe. And also, you know, if you move over to nitrogen, where you've got three binding sites instead of four, it's not
Starting point is 00:33:25 immediately obvious to me that you couldn't have simple life. with a little bit less complexity and that you need four and nitrogen wouldn't be enough. And so I did find myself, while I was reading through these explanations, wondering if we are to some extent a little bit too constrained in our thinking
Starting point is 00:33:41 based on the life that we observe here. But, you know, on the other hand, you know, maybe you would have expected to have seen a couple examples of like nitrogenous life on this planet. Here on Earth, you mean, yeah. Yeah, here on Earth, but we don't see that. Yeah, so I don't know,
Starting point is 00:33:55 but different temperature or pressure conditions might make nitrogen or silicon-based life a little bit more likely to exist, but this is their current, I think, best understanding of why it's carbon-based based on our n-of-one of life forms that happen to have carbon backbones. Well, why do you think it is that we have one kind of life here on Earth? Like, all life shares the same basic biochemistry, and we think there's probably a single common ancestor. Why don't we live on a planet where life arose independently multiple times and coexists. Is it for the same reason that we have like one species of humans
Starting point is 00:34:30 because we kill all the other ones and we can't tolerate it? Or do you think it just arose once? I really don't know. I need answers, Kelly. I need answers. I don't think anyone knows. Calm down, Daniel. You know that on this podcast we usually don't have the answers.
Starting point is 00:34:43 I know, but it's so frustrating. It is surprising to me that like in one ocean we didn't end up with, you know, in one puddle, like a rose. and then in another puddle on the other side of the planet, life arose. And we still see signs of both of those. I don't know. I don't know. I'd love to know the answer, but I don't.
Starting point is 00:35:02 It's so frustrating to only have this one example and to not know how to generalize and what's typical and what's weird. So it'd be fun to find even just one more example of life somewhere else. And maybe on that planet there's several different kinds of life and several different kinds of chemistries of that life would be amazing. That would be absolutely amazing. And it would blow my mind if we found, like, for example, bacteria in the lava tubes or underground on Mars. And if it ended up that that was like an independent evolution of life, I feel like that would be the coolest discovery of my lifetime for sure.
Starting point is 00:35:35 And I think this is a really healthy way to think, like, let's look at the example we have and let's wonder which of these things might be different. It's a good way to like try to think outside the box, even though it's really hard for us to imagine what else could be out there. And I'm sure that we're failing to describe the complexity of non-Earth life. But at least we're making the effort, right? We're like trying to understand what could be outside the box of our thinking. You mentioned briefly how water is super important for life on Earth. But then I think you said something about how it's maybe not necessary, how you could have life without water.
Starting point is 00:36:08 What could replace water? So there's lakes of liquid ethane and methane on Titan, which is a moon of Saturn. And it's possible that these could be used as solvents to sort of move stuff around a living organism instead of water if you don't have water present. And maybe this could create different kinds of life forms or create the sort of conditions necessary for something else to become the backbone of life instead of carbon. But I think we're a little bit far away from sending probes out there to deliver samples back. But fun NASA. That's right. We're doing as much as we can to try to think our way outside the box. But really what we got to do is actually climb
Starting point is 00:36:46 outside the box, go to these crazy places in our own backyard where there could be other examples of life right there waiting for us to discover them. And the crazy thing is that all it does is cost money, right? And we spend like more money on an aircraft carrier than it would cost to discover life on Titan. So let's go do it, people. Let's go buy some knowledge. Sounds like a good investment to me. Chaching. All right, Julian, I did my best with the chemistry question. But if you don't feel like you got a sufficient answer, let us know. And maybe we'll have to pull in a chemist to help us answer this question.
Starting point is 00:37:24 But I'm looking forward to hearing what you had to say. Hi, Daniel and Kelly. First off, I was a little bit worried that I might get kicked off the Discord channel for asking such a chemistry-heavy question. But it was really inspiring to hear you guys working at it and tackling a subject where you're not necessarily the most comfortable. And so thanks very much. And that does definitely answer my question.
Starting point is 00:37:46 Thanks again. Cheers. Bye. December 29th, 1975, LaGuardia Airport. The holiday rush, parents hauling luggage, kids gripping their new Christmas toys. Then, at 6.33 p.m., everything changed. There's been a bombing at the T.W. the UA terminal. Apparently, the explosion actually impelled metal glass.
Starting point is 00:38:23 The injured were being loaded into ambulances, just a chaotic, chaotic scene. In its wake, a new kind of enemy emerged, and it was here to stay. Terrorism. Law and order, criminal justice system is back. In season two, we're turning our focus to a threat that hides in plain sight. That's harder to predict and even hard. harder to stop. Listen to the new season of law and order criminal justice system on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts.
Starting point is 00:39:00 My boyfriend's professor is way too friendly and now I'm seriously suspicious. Wait a minute, Sam. Maybe her boyfriend's just looking for extra credit. Well, Dakota, it's back to school week on the OK Storytime podcast, so we'll find out soon. This person writes, my boyfriend has been hanging out with his young professor a lot. He doesn't is a problem, but I don't trust her. Now he's insisting we get to know each other, but I just want her gone. Now hold up. Isn't that against school policy? That sounds totally inappropriate. Well, according to this person, this is her boyfriend's former professor and they're the same age. It's even more likely that they're cheating. He insists there's nothing between them.
Starting point is 00:39:33 I mean, do you believe him? Well, he's certainly trying to get this person to believe him because he now wants them both to meet. So, do we find out if this person's boyfriend really cheated with his professor or not? To hear the explosive finale, listen to the OK Storytime podcast. on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast. I'm Dr. Joy Harden-Brandt Bradford, and in session 421 of therapy for black girls, I sit down with Dr. Athea and Billy Shaka 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?
Starting point is 00:40:06 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. 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. 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, don't miss session 418 with Dr. Angela
Starting point is 00:40:40 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, 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.
Starting point is 00:41:13 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 the 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. 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.
Starting point is 00:42:03 All right, now for something a little more philosophical. I was listening to your episode about thinking like a physicist. It got me thinking about different theories that I've been proposed over the last few decades, which led me to hawking radiation. There isn't any observational or experimental data confirm hawking radiation, yet the physics community seems to have accepted it. My question is, why do some theories get accepted and others don't? Please help me figure out where my thought process might be wrong. Thank you for all you do. All right. Great question, Eric. I love this because it dives into the process of science itself. Not as much the science questions we're asking, but how as a community we like
Starting point is 00:42:41 decide that something is part of the canon or something is not. It's a great question. It's a great question. Let's start, though, with what is Hawking radiation? So we can then, you know, compare other theories to it. Hawking radiation is an amazing little bit of science. We've talked in the podcast a lot about the biggest question in modern physics is how to reconcile gravity with quantum mechanics. Nobody knows how to do it. This program of quantum gravity, we've talked about string theory, we've talked about post quantum gravity, there's loop quantum gravity, all sorts of efforts, nobody knows how to do it. Nobody's had any success except Stephen Hawking figured out like one little corner of it.
Starting point is 00:43:22 He used a really clever mathematical trick to understand what happens to quantum fields when they're near a black hole. So he doesn't have like the big answer to how to unify these things or what is the gravity of particles or to do all. the calculations, he just was able to figure out what happens to quantum fields when they're near a black hole using a really clever little mathematical trick. And how did he do that? It's totally worth digging into it for a minute because the story of Hawking radiation, as it's often
Starting point is 00:43:54 told in popular science accounts, is pretty much totally wrong and doesn't describe what was actually done and what Hawking actually figured out. The popular story is a story of what happens to particles. So you have fields near an event horizon, and they fluctuate and create like a particle, anti-particle pair. One particle falls into the black hole, and the other one doesn't, and so escapes, and that's your Hawking radiation. And the problem with that account is that that's not at all what we think happens. We don't know how to describe that.
Starting point is 00:44:23 That would require understanding, like, how gravity affects particles, and, you know, are those particles real anyway? Really what Hawking did was he thought about the mathematical solutions to the quantum wave equations like quantum fields have waves in them. Those waves are particles or other kinds of ripples and they slosh around and they follow rules. Those are wave equations, just like the mathematics that describes waves in the ocean or waves in traffic. Waves are everywhere. And the equations that describe quantum fields are also wave equations. And when you solve wave equations, you have to make sure that they line up on top of each other and they match what you see at
Starting point is 00:44:59 boundaries and stuff like this. This is how we figure out like reflection and refraction of light. sorts of wave equation stuff. And he figured out what happens to those waves if you have a weird barrier, an event horizon. You add that to your quantum fields, and he showed that what happens is you have to have a wave coming out of that event horizon. So the short version is that the mathematics of quantum fields require some outgoing radiation from an event horizon if the quantum fields are ever going to work. So you don't have to know what the gravity is for particles or what's happening inside that
Starting point is 00:45:33 event horizon. while you have an event horizon, but very generally, any time that's an event horizon near a quantum field, there's going to be outgoing radiation. So that's really what hawking radiation is. That's the prediction. And again, we don't have a complete description of quantum gravity or understand how gravity affects little particles, but he predicts that there's this radiation that comes out of event horizons just to make the wave equation work for quantum fields. Okay, so this is a prediction, but it hasn't been tested. So for something that you can't test, you can still feel pretty good about it if it predicts a lot of other things. So, like, how good in general is the evidence, even if we can't directly test it?
Starting point is 00:46:12 There's absolutely no evidence for hawking radiation. Okay. But it's very cool because it connects to other kinds of physics. It also lets you think about black holes thermodynamically. It lets you think about black holes as things that have temperature. In our universe, everything that's made out of some kind of matter has a temperature and glows. Like the sun obviously glows. It's really hot. But the earth also glows. It just glows in a wavelength of light that we can't see. It glows in the infrared. And you glow, which is why, like, if somebody puts on night vision goggles, they can see you because they're seeing you in the infrared, the light that you glow in. And your temperature determines what you glow in. So as you get hotter, you glow in higher frequency light, which is why, for example, metal, when you heat it up, gets red hot and then white hot, for example. That's all just black body radiation. everything that has a temperature glows.
Starting point is 00:47:04 So now if black holes glow, you can describe them as having a temperature, which is pretty cool. Ha-ha, thermodynamics joke. And it lets you use a whole other branch of mathematics and physics that we've developed for hundreds of years and apply it to black holes and think about their entropy and stuff like this. So people have been having a lot of fun using black holes as a concept and playing around with the mathematics of it. There's absolutely no evidence for hawking radiation because if, If Hawking radiation does exist in the universe, black holes are too far away and hawking radiation is too dim for us to see it. So it's possible that black holes are all out there emitting this hawking radiation,
Starting point is 00:47:44 but we've never seen it. And it's very hard to imagine how we could in the near future, unless we made artificial black holes here on Earth to study their radiation. All right. So Stephen Hawking is like the rock star of physics, a rock star. You all have like three. And so to what extent do you think this theory has been, like, quote, unquote, accepted because he's a rock star? Well, I think this theory helped make him a rock star, right?
Starting point is 00:48:11 So there's some cause and effect there. But Eric's question is a good one. Like, why do people pick up on this theory and run with it and build on top of it and other stuff is sort of dismissed? You know, we have like Stephen Wolfram's got a theory of everything that not very many people are working on, hasn't become accepted. Lots of fringe theories out there that nobody's taking up. You know, you have to remember that, like, science is not some official institution where things like it graded and accepted or rejected. It's just a bunch of people, and people work on the things they're excited about. And the reason hawking radiation has become kind of mainstream is that because it opened the door to working out other things.
Starting point is 00:48:51 Thinking about black holes as thermodynamic objects and calculating their temperature and thinking about information, it sort of left things for people to do and to work on and to build on top of them. but you know that's just personal judgment people decided hey this is fun and interesting i'm going to go work on this and so people just sort of vote with their feet whereas other ideas that might be more valid or better descriptions of nature are not getting as much attention because maybe there's not an obvious problem to work on or there's nothing to do there or it just doesn't seem as fun people have a sort of a simplistic view of how science works and what is science and think that like science has to be experimentally proven before it's accepted but there's
Starting point is 00:49:34 no official stamp of accepted science it's just what are people doing what are people working on what are people thinking about and so it's possible that we could discover that hawking was totally wrong or it could be that hawking's ideas lead us to understand quantum gravity in some way or it could be that it's a dead end that he was able to figure this one thing out but it doesn't give us an opportunity to discover anything else. Yeah, so ruminating a little bit more on the human side of science, I imagine that when you pick a theory that you want to spend your career on, you probably want to pick a theory that you think is one of the ones that has the highest chance of being right.
Starting point is 00:50:09 I know that people are okay with working on theories and finding out that they're wrong because that is an answer and answers are important. But I think that probably you pick the ones you want to be correct. But I wonder if when you're picking these ideas, how much does it also have to do with what is testable and what's not, like, even if you think an idea is correct, but you can't really test it directly, and maybe that makes it hard to, like, get grants to fund your lab or something. Like, how do you think these various human factors sort of all add up? Yeah, I think in theoretical physics, whether it's immediately testable is not always one of the
Starting point is 00:50:42 top considerations. I think one of the top considerations is, can I make progress in a reasonable amount of time? Like, personally, as a scientist, when I choose projects, I could choose to work on really big questions like, hey, what came before the Big Bang? But I have no way to make progress on that in a reasonable amount of time. And as a scientist, I have to produce science regularly. So I have to choose projects where I can make some progress. And I think this is a really important thing for young scientists to learn is to spot opportunities. Like, hey, here's something where if we spend a couple years on this, we can actually learn something given the resources and the skills that we have. Right. So it's sort of like spotting a business opportunity.
Starting point is 00:51:23 Oh, there's a market for this and we know how to do it. So let's jump on that. And so in my research, for example, you know, we use machine learning. We're always like looking for ways machine learning can solve problems that weren't solved before. But again, in a reasonable amount of time. So on the theoretical physics side, people are looking for problems where they can make some progress, where there's an opening, but they're not always concerned about like, is this immediately going to be testable? Because science isn't just about experiments, you know, science is a big complex dance that
Starting point is 00:51:53 eventually leads to answers. We hear a lot of criticism of string theory, for example, saying, oh, it's not science because you can't test it. But, you know, it's a precursor to testing. Sometimes it takes something 50 years, 100 years before it bubbles up and produces something that you can test. Doesn't mean that it wasn't science until then, that you retroactively go back and say, okay, now we can test it. So the last 100 years count as science. Whereas if it never leads to something you can test, you say it never was science, I think that's a little bit overly simplistic. All right. Well, so continuing to think out loud here. So you said that you don't work on questions related to the Big Bang because you can't produce science regularly by doing
Starting point is 00:52:29 that. So how do we get questions to these really important problems that take a long time? Is our system just not set up to answer those questions? Or is it something? So, you know, for example, Darwin, he came up with the idea of natural selection, but it was like an idea that was the accumulated result of observations that happened over like maybe decades. But he was publishing a lot of like molest papers along the way or like you know observations on other things so are people working on the really big questions but just sort of slowly in the background while producing something to keep their jobs or like is it harder and harder to get answers to those big questions that take a long time today because of the way our funding system is set up yeah
Starting point is 00:53:09 there are people working on big questions a great example are things we call quantum foundations like which of the quantum mechanical interpretations of reality are real the Copenhagen interpretation, the many world's interpretation, how do we grapple with all that? Everybody thinks that's a big problem. A lot of people have no idea how to make progress on it. And so it's sort of a bit of a dangerous thing to dig into for like a young scientist because you could jump into it, work for a couple years, make no progress, and then what do you have to show for yourself? So it's the kind of thing that people who are well established with like tenured positions, i.e. like Sean Carroll can dig into and try to make some progress on. And everybody understands
Starting point is 00:53:46 it's really important. But yeah, it's hard to know if you're going to make any progress. And so a lot of people don't work on that. There are also some places that specifically fund this kind of work because they realize, hey, it's really important for people to be thinking about these big questions or we're never going to make any progress on them. And so there's some places that specifically write grants just to support that kind of research. But they're pretty few and far in between. The bigger picture tendency in science, I think, is towards short-term promises. A lot of grant. that you write require you to know what you're going to learn in advance and to have a lot of preliminary data because this is arms race in science you know this lab has already set up to do that that lab has already set up to do that and so a lot of science is more about these sort of short-term results which i think is a shame because we should be doing science as exploratory research say hey let's see what happens if we give a bunch of smart people money and time and see what they figure out agreed that's a big complaint of mine for the system all right well have we said everything that we want to say about eric's question i think so if i had to sum it up i would say to eric that there is no such thing as
Starting point is 00:54:56 accepted science or not accepted science there's just the kind of things people are working on right now that people are excited about and it's a personal decision not some like institutional label we put on ideas and let's see what eric has to say about that answer i daniel kelly this does help me understand better how science works. I tend to make the mistake of thinking science is monolithic with nothing but cold hard facts. And I forget that behind the science are human beings. My idea of the scientific method comes from high school, which took a more simplistic approach. I think it is more accurate to say science is more the art of human curiosity than just cold hard facts. It is, after all, human beings and all their complexities that ultimately strive to unravel the mysteries of the
Starting point is 00:55:43 universe through a blend of creativity and skepticism. And ultimately, if it is a good idea that can stand scrutiny, it will become accepted. Hocking radiation is a prime example of this. Thank you, Daniel and Kelly, for taking the time to help me understand the process of science a bit more, and I certainly appreciate everything you do. Take care. Daniel and Kelly's Extraordinary Universe is produced by IHeart Radio. We would love to hear from you. We really would. We want to know what questions you have about this extraordinary universe.
Starting point is 00:56:25 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 daniel and Kelly.org. Or you can find us on social media. We have accounts on X, Instagram, Blue Sky, And on all of those platforms, you can find us at D and K Universe.
Starting point is 00:56:48 Don't be shy. Write to us. December 29th, 1975, LaGuardia Airport. The holiday rush, parents hauling luggage, kids gripping their new Christmas toys. Then, everything changed. There's been a bombing at the TWA terminal. Just a chaotic, chaotic scene. in its wake a new kind of enemy emerged terrorism listen to the new season of law and order criminal justice system on the iheart radio app apple podcasts or wherever you get your podcasts
Starting point is 00:57:25 every case that is a cold case that has DNA right now in a backlog will be identified in our lifetime on the new podcast america's crime lab every case has a story to tell and the DNA holds the truth he never thought he was going to get caught. And I just looked at my computer screen. I was just like, ah, got you. This technology is already solving so many cases. Listen to America's Crime Lab on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. Hi, it's Honey German, and I'm back with season two of my podcast. Grazias, come again.
Starting point is 00:58:02 We got you when it comes to the latest in music and entertainment with interviews with some of your favorite Latin artists and celebrities. You didn't have to audition? No, I didn't audition. audition in like over 25 years. Oh, wow. That's a real G-talk right there. Oh, yeah. We'll talk about all that's viral and trending with a little bit of cheesement and a whole lot of laughs. And of course, the great Vibras you've come to expect. Listen to the new season of Dresses Come Again on the IHeartRadio app, Apple Podcast, or wherever you get your podcast. I'm Dr. Scott Barry Kaufman, host of the Psychology Podcast. Here's a clip from an upcoming conversation about how to be a
Starting point is 00:58:42 the 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. Complex problem solving takes effort. Listen to the psychology podcast on the Iheart radio app, Apple Podcasts, or wherever you get your podcasts. This is an IHeart podcast.

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