WEBVTT - Does Mars Have a Liquid Center?

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<v Speaker 1>Hey, Jorgey, I have a food engineering question for you.

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<v Speaker 1>Food engineering. We're trying to melt ice cream with a

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<v Speaker 1>particle collider, not yet, but now I'm gonna go try that.

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<v Speaker 1>Now I'm wondering how they engineer foods with a liquid

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<v Speaker 1>center inside. Okay, now you're trying to make our candy

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<v Speaker 1>with liquid inside? Yeah? Or like, how do they make

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<v Speaker 1>peanut butter vealed pretzels? That's a billion dollars secret. I

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<v Speaker 1>can't just reveal it. We might get sued. Alright, I

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<v Speaker 1>guess we should stick to revealing big science secrets. Yeah.

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<v Speaker 1>I don't think we'll get sued for those. They're usually

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<v Speaker 1>free and maybe also useless. You said it not mean. Hi.

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<v Speaker 1>I am more Hammon cartoonists and the creator of PhD comics. Hi.

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<v Speaker 1>I'm Daniel. I'm a particle physicist, and I do enjoy

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<v Speaker 1>me a peanut butter field pretzel. Really, why can't you

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<v Speaker 1>just put the peanut butter on the outside. It's a

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<v Speaker 1>totally different taste experience, man, I mean this can't be compared. Plus,

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<v Speaker 1>I admire the engineering. Somehow they baked this pretzel around

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<v Speaker 1>the peanut butter. It's incredible. You think that's how they

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<v Speaker 1>do it. They formed the bread around the peanut butter.

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<v Speaker 1>Actually did some research about this. It was the basis

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<v Speaker 1>of a big lawsuit. And there's a fancy co extrusion

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<v Speaker 1>process where they have the pretzel dough around the peanut

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<v Speaker 1>butter and then they bake it. Co extrusion. Wow, that

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<v Speaker 1>sounds like a heavy duty physics term. You should google it.

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<v Speaker 1>They used to find some really fun YouTube videos about

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<v Speaker 1>the interior of these factories. Pretty fascinating food engineering. And

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<v Speaker 1>by experiments, you mean you tried it at home a

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<v Speaker 1>bunch of times, or you ate a bunch of pretzels

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<v Speaker 1>with peanut butter. I ate a bunch of pretzels. I

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<v Speaker 1>tried the chocolate covered versions, the non chocolate cover versions.

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<v Speaker 1>I'm in the name of science. Have you tried coach

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<v Speaker 1>twinging butter and pretzels? That's the next level heart attack recipe.

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<v Speaker 1>You should sell that idea to Ben and Jerry's. But anyways,

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<v Speaker 1>welcome to our podcast, Daniel and Jorge Explain the Universe,

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<v Speaker 1>a production of I Heart Radio in which we extrude

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<v Speaker 1>ideas about the universe into your head without breaking your skull. Somehow,

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<v Speaker 1>we wrap your mind around the peanut butter field delicious

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<v Speaker 1>secrets of the universe. We talk about all of the

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<v Speaker 1>crazy stuff happening deep out in crazy space, and all

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<v Speaker 1>the tiny stuff happening in between your toes and the

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<v Speaker 1>smallest particles. We break down quantum mechanics, We talk about

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<v Speaker 1>astrophysics and everything in between. Wait, I thought that the

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<v Speaker 1>science secrets that we reveal our the pretzel part that

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<v Speaker 1>surrounds the yummy peanut butter inside of our punts. It

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<v Speaker 1>could be I was thinking of my brain is the

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<v Speaker 1>peanut butter and my skull is the pretzel. You just

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<v Speaker 1>ruined that vision of deliciousness for me. Every time you

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<v Speaker 1>bite into one of those from now on, just think

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<v Speaker 1>I'm eating Daniel's head, not mom goodness, let's please hitit

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<v Speaker 1>that out. But anyways, we do like to talk about

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<v Speaker 1>the universe and all of it's amazing goodness inside and

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<v Speaker 1>everything that you can quote through it, inside of it,

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<v Speaker 1>and all the things that you can discover because it's

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<v Speaker 1>the big cosmos and there are wonderful things out there

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<v Speaker 1>hiding in plain sight, that's right. And the more we

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<v Speaker 1>look out into the universe, the more we discover these

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<v Speaker 1>surprises and the more questions we have about exactly how

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<v Speaker 1>things work, what layers they're in, and how they're organized

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<v Speaker 1>and how they got that way, right, because we can

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<v Speaker 1>see the universe and touch it and probe, but who

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<v Speaker 1>knows what's line underneath the surface, what is at the

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<v Speaker 1>core of the universe and how it works. And everything

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<v Speaker 1>that's out there has a history. The Moon, the Earth, Mars,

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<v Speaker 1>every planet, every star has a sometimes billion years long history,

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<v Speaker 1>a crazy story that tells us how it got to

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<v Speaker 1>be the way it is today. And unraveling that story

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<v Speaker 1>is like the biggest, most delicious detective mystery in the universe.

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<v Speaker 1>Figuring out what exactly happened to the object. Can we

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<v Speaker 1>tell just by looking on the outside or just by

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<v Speaker 1>looking through a telescope, exactly what the story is of

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<v Speaker 1>this heavenly body? Yeah, because we want to know, right,

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<v Speaker 1>the species as human beings, were curious about where things

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<v Speaker 1>came from and how they got to be the way

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<v Speaker 1>they got to be, and that's all part of their history,

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<v Speaker 1>and it's all they're inside of the things for looking at. Yeah,

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<v Speaker 1>we showed up in this universe basically the last minute,

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<v Speaker 1>and a lot of stuff happened before we got here.

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<v Speaker 1>So it's fun to unravel those stories and figure out

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<v Speaker 1>have things looked this way for a long time? The

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<v Speaker 1>things used to be really different. Does that mean things

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<v Speaker 1>are going to change? It's all just part of like

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<v Speaker 1>becoming conscious beings and exploring the world that we find

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<v Speaker 1>around us. So today we'll be talking about one of

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<v Speaker 1>these mysteries. Line underneath the surface of our own neighborhood.

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<v Speaker 1>It's something that we can see almost every night, but

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<v Speaker 1>that is kind of hidden from us, right, that's right.

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<v Speaker 1>We have questions about what's beneath our feet, and we

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<v Speaker 1>have questions about what's beneath the feet of potential neighbors.

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<v Speaker 1>You mean the actual neighbors. Like is your neighbor sitting

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<v Speaker 1>on top of a giant oil well or something? Yeah,

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<v Speaker 1>maybe there's like a huge peanut butter deposit under my

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<v Speaker 1>neighbor's house and I could sell that to that factory. Yeah,

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<v Speaker 1>instead of liquid gold, that's liquid saturated fats. Well, it's

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<v Speaker 1>peanut butter technically a liquid or is it a solid?

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<v Speaker 1>I guess it depends if it's smooth or what's the

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<v Speaker 1>other one crunching? What is the phase diagram of peanut butter?

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<v Speaker 1>Can it sublimate into a gas? I wonder. I don't

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<v Speaker 1>know if anybody's ever done that experiment. You mean, like

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<v Speaker 1>go straight into a gas form of peanut butter, like

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<v Speaker 1>you can invade peanut butter. Not recommended, folks, not recommended.

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<v Speaker 1>Our lawyers have not vetted that statement. Please do not

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<v Speaker 1>vape peanut butter. You could clog through your lungs directly

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<v Speaker 1>with peanut butter. But if you do vape peanut butter,

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<v Speaker 1>tell us about it, because we're curious that may will

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<v Speaker 1>be another billion dollar industry who knows, or a billion

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<v Speaker 1>dollar lawsuit. We're about to get hit with people who

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<v Speaker 1>use it to cure their pretzel addiction, and then they'll

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<v Speaker 1>need some patches, some peanut butter patches. Anyways, Yeah, we'll

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<v Speaker 1>be tackling one such mystry in our own solar system,

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<v Speaker 1>so to be on the podcast, we'll be asking the question,

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<v Speaker 1>does Mars have a solid or liquid core? I guess

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<v Speaker 1>the question is Mars hardcore or softcore? Is it a

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<v Speaker 1>hard boiled egg or a soft boiled egg? Exactly? I

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<v Speaker 1>think it's a super fascinating question, and it's fun for

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<v Speaker 1>me because I think about like when people were asking

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<v Speaker 1>this question about the Earth, you know, for a long time,

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<v Speaker 1>we didn't really know, like, hey, what's the Earth made

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<v Speaker 1>out of? It's just one big rock? Or is there

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<v Speaker 1>something crazy going on under our own feet? And now

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<v Speaker 1>that we have a little bit of a sense of

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<v Speaker 1>what's going on inside the Earth, we can ask similar

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<v Speaker 1>questions about other planets, and so it's fascinating to wonder, like,

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<v Speaker 1>are they different, are they the same? What's going on?

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<v Speaker 1>I guess just to verify, the Earth has a softcore. Right,

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<v Speaker 1>The inside of our planet is molten, right, It's like

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<v Speaker 1>melted rock. Yeah, there's some melted rock and a lot

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<v Speaker 1>of melted metal, melted iron, liquid nickel, all this kind

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<v Speaker 1>of stuff flowing underneath our feet. It's part of why

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<v Speaker 1>we have, for example, a magnetic field. I see now,

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<v Speaker 1>I guess, is it possible for a planet of our

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<v Speaker 1>size to have a solid core? Like, wouldn't all that pressure,

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<v Speaker 1>gravity pressure eventually kind of I don't know, melt the

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<v Speaker 1>stuff inside. Yeah. The reason that we do have a

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<v Speaker 1>liquid core is because of all that temperature and pressure,

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<v Speaker 1>and that comes from both the gravitational pressure and also

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<v Speaker 1>the decay of the isotopes inside the Earth that helped

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<v Speaker 1>keep it hot. But it's not going to be that

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<v Speaker 1>way forever. You know, we got a certain spoonful of Earth,

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<v Speaker 1>and eventually it's gonna cool off. I think we estimated

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<v Speaker 1>once on this podcast that it's going to take more

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<v Speaker 1>than a hundred billion years before the Earth cools, So

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<v Speaker 1>we got some time, and you know, the Sun is

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<v Speaker 1>going to go red super giant before that, so it's

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<v Speaker 1>not going to be our number one problem. But other

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<v Speaker 1>planets are different sizes and so they will have different

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<v Speaker 1>cooling off times. It's gonna be a while before we're cool.

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<v Speaker 1>I can relate to that. Hey, we're gonna be young

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<v Speaker 1>and hot for a long time. Think about it that way.

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<v Speaker 1>That sounds very hard corn, all right, But they were

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<v Speaker 1>asking questions about Mars. Does Mars have a solid or

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<v Speaker 1>liquid core? And it's kind of a big deal, right

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<v Speaker 1>because it might tell us whether or not Mars is

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<v Speaker 1>still you know, sort of young and active, and it

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<v Speaker 1>might tell us also what our future might be for

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<v Speaker 1>that's right. And I think it's just a question that

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<v Speaker 1>people have when they look up into the sky and

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<v Speaker 1>they wonder, you know, is that planet over there a

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<v Speaker 1>lot like our planet or is it totally different? And

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<v Speaker 1>what does that mean about the nature of planets and

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<v Speaker 1>planets in other solar systems, and it's to me just

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<v Speaker 1>really connects with this basic, simple initial curiosity we have

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<v Speaker 1>when we look up at the sky, we wonder what

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<v Speaker 1>those things are like. Hey, but before we answer this question,

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<v Speaker 1>we wanted to answer a question from one of our listeners,

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<v Speaker 1>perhaps our youngest listener. That's right. You may remember last

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<v Speaker 1>week we talked about Hannah, who was home sick from school.

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<v Speaker 1>She's two and a half years old. She lives in

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<v Speaker 1>Australia and she wanted to hear Daniel and Jorge. So

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<v Speaker 1>I reached out to her dad and asked him, Hey,

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<v Speaker 1>does Hannah have any questions she wants us to answer

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<v Speaker 1>while she's homesick? And he asked her what questions she

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<v Speaker 1>had for day own Jorge, and she said, monkey, wait? Monkey?

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<v Speaker 1>Is her question? Was her first question or answer to

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<v Speaker 1>the universe and everything in it? I don't know. It's

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<v Speaker 1>hard to get in the mind of a two and

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<v Speaker 1>a half year old sometimes. But then he asked her again,

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<v Speaker 1>and so here's Hannah's real question. How and how my

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<v Speaker 1>land home? Why is the Larne shine? Oh that's adorable.

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<v Speaker 1>It's like a little tiny little nerd. Yeah, and she

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<v Speaker 1>has the same curiosity. Today we're talking about Mars and

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<v Speaker 1>what's in it, But you know, she's looking up in

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<v Speaker 1>the sky and she's wondering, why is that thing up

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<v Speaker 1>there glowing at me? It has the same root of curiosity.

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<v Speaker 1>I see you're saying that it taps into that same

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<v Speaker 1>like looking up at the sky and wondering what's going

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<v Speaker 1>on out there? Yeah, exactly why is that thing up

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<v Speaker 1>there doing that thing that it's doing? Well? Really quickly?

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<v Speaker 1>Then what is the answer for Hannah? Why does the

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<v Speaker 1>moon shine? Yeah, Hannah, the reason the moon shines, especially

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<v Speaker 1>at night, is that it's actually reflecting light from the Sun.

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<v Speaker 1>Even though you can't see the sun at night, the

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<v Speaker 1>sun can see the moon, and so the Sun's light

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<v Speaker 1>bounces off the moon and down to your eyeball. So

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<v Speaker 1>at night you're kind of seeing the sun by seeing

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<v Speaker 1>it reflect off the moon. So moonlight is all just

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<v Speaker 1>reflected sunlight. Right. Do you think she's asking about moonshine

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<v Speaker 1>as well? Why does my dad drink so much moonshine?

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<v Speaker 1>I don't know. I think that's a question for her

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<v Speaker 1>dad and his father. There nothing wrong with moonshine, nothing

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<v Speaker 1>wrong with the little moonshine. All right, well, Hannah, that's

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<v Speaker 1>to your answer. The moon shines because it bounces light

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<v Speaker 1>from the sun, so it looks like it glows, but

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<v Speaker 1>really it's just kind of like a mirror, just reflecting

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<v Speaker 1>and getting lit up by the sun. That's right, all right,

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<v Speaker 1>Well back to our question, those marks have a solid

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<v Speaker 1>or liquid core? This is a pretty interesting question, and

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<v Speaker 1>we were wondering, as usual, if people out there and

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<v Speaker 1>new the answer to this billion year question. So thanks

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<v Speaker 1>to everybody who volunteered to answer this question as usual.

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<v Speaker 1>If you'd like to participate for future episodes, please write

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<v Speaker 1>to me two questions at Daniel and Jorge dot com.

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<v Speaker 1>Think about it first. Second, do you think Mars is

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<v Speaker 1>solid or liquid on the inside. Here's what people had

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<v Speaker 1>to say. Yes, they might be a big diamond inside it.

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<v Speaker 1>Now I think Mars has hot liquid. Yes, it does

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<v Speaker 1>completely solid, because Mars doesn't have any radioactive isotopes inside

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<v Speaker 1>the core. Keep it hot and keep it liquid. I'm

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<v Speaker 1>going to say, yes, Mars has a solid core of

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<v Speaker 1>iron or nickel or some other heavy element, just like Earth. Yes,

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<v Speaker 1>Mars has a solid core. It has no obvious plate

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<v Speaker 1>tectonics going on it obviously had some sort of tectonic

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<v Speaker 1>activity going on at some time, and the magnetic field

0:11:49.120 --> 0:11:53.360
<v Speaker 1>is almost non existent. So I think if we were

0:11:53.440 --> 0:11:55.960
<v Speaker 1>to dig deeper, I think we'd find it does have

0:11:56.040 --> 0:11:59.440
<v Speaker 1>a solid core. I don't think Mars has a significant

0:11:59.480 --> 0:12:04.040
<v Speaker 1>magnetic field because solar radiation is a concern for explorers.

0:12:04.880 --> 0:12:07.120
<v Speaker 1>I would say it cooled down at least a billion

0:12:07.200 --> 0:12:09.480
<v Speaker 1>years ago to a solid all the way through to

0:12:09.559 --> 0:12:15.440
<v Speaker 1>its core. Yes, I think it has and used to

0:12:15.480 --> 0:12:22.280
<v Speaker 1>be more powerful and active. But judging by the strength

0:12:22.400 --> 0:12:28.680
<v Speaker 1>of the magnetic field and the atmosphere, it weakened in time.

0:12:29.840 --> 0:12:34.200
<v Speaker 1>Probably that will happen to Earth to I don't know

0:12:34.320 --> 0:12:38.480
<v Speaker 1>for sure, but kind of this is the way I

0:12:38.520 --> 0:12:42.120
<v Speaker 1>think it would go. Mars does have a solid core.

0:12:42.400 --> 0:12:45.040
<v Speaker 1>End of story. I see you remember you saying in

0:12:45.040 --> 0:12:49.760
<v Speaker 1>an earlier podcast that Mars does not have um an

0:12:49.760 --> 0:12:54.880
<v Speaker 1>electromagnetic field protecting it because it doesn't have a solid core.

0:12:56.480 --> 0:13:01.080
<v Speaker 1>So I'm going to say no, all right, some pretty

0:13:01.120 --> 0:13:03.880
<v Speaker 1>definitive answers here. I feel like people were pretty confident

0:13:04.280 --> 0:13:07.559
<v Speaker 1>about their answers here. They're like, yes, definitely, this, definitely,

0:13:07.600 --> 0:13:11.320
<v Speaker 1>that definitely peanut butter, A big hot diamond. I like

0:13:11.400 --> 0:13:13.200
<v Speaker 1>that one. Why do you think people are so confident

0:13:13.280 --> 0:13:14.800
<v Speaker 1>this time? I think that a lot of people have

0:13:14.920 --> 0:13:18.600
<v Speaker 1>heard that Mars is smaller and cooled faster, doesn't have

0:13:18.679 --> 0:13:21.960
<v Speaker 1>volcanoes on the surface or a magnetic field, and so

0:13:22.040 --> 0:13:24.440
<v Speaker 1>I think that leads people to suspect that it might

0:13:24.520 --> 0:13:27.680
<v Speaker 1>just be a big lump of hard rock, unlike the

0:13:27.760 --> 0:13:31.240
<v Speaker 1>Earth and the story. All right, thanks for joining us, um,

0:13:31.280 --> 0:13:35.520
<v Speaker 1>But there's more, I see, there's more to the story.

0:13:35.720 --> 0:13:37.920
<v Speaker 1>There is more to the story, Yes, exactly. I think

0:13:37.920 --> 0:13:41.280
<v Speaker 1>there's some really interesting nuances here that these listeners will learn.

0:13:41.480 --> 0:13:43.720
<v Speaker 1>All right, well, let's dig into it. First of all, Daniel,

0:13:43.720 --> 0:13:47.400
<v Speaker 1>why is this question interesting to you, I guess and

0:13:47.440 --> 0:13:50.079
<v Speaker 1>to physicists and generally to the public. Why should we

0:13:50.120 --> 0:13:53.679
<v Speaker 1>care whether Mars is hardcore or soft and squishy on

0:13:53.720 --> 0:13:56.160
<v Speaker 1>the inside. Yeah, Well, for me, there's sort of two

0:13:56.240 --> 0:14:00.000
<v Speaker 1>levels there. One is just inherent curiosity, like I have questions,

0:14:00.080 --> 0:14:02.840
<v Speaker 1>is about what's inside stuff. You know, you ever get

0:14:02.840 --> 0:14:04.400
<v Speaker 1>a rock and you crack it open, you find a

0:14:04.400 --> 0:14:08.080
<v Speaker 1>crystal inside. There's like a joy there discovering something you

0:14:08.120 --> 0:14:10.360
<v Speaker 1>didn't expect, and so you always want to like look

0:14:10.400 --> 0:14:13.440
<v Speaker 1>inside stuff to see what's there. Maybe there's something hidden,

0:14:13.480 --> 0:14:15.880
<v Speaker 1>maybe there's a mystery. You know, that's why we explore

0:14:15.920 --> 0:14:17.840
<v Speaker 1>the universe. We don't just sit back and think about

0:14:17.880 --> 0:14:19.920
<v Speaker 1>it in our minds the way the Greeks do. So

0:14:19.960 --> 0:14:22.120
<v Speaker 1>we sort of want to know what's out there because

0:14:22.160 --> 0:14:24.760
<v Speaker 1>we could be shocked, we could be surprised. Mars couldn't

0:14:24.760 --> 0:14:27.360
<v Speaker 1>be like hollow on the inside and filled with aliens

0:14:27.440 --> 0:14:29.840
<v Speaker 1>or something. So we definitely want to go look and

0:14:29.880 --> 0:14:32.560
<v Speaker 1>see what's inside this stuff. But also I think there's

0:14:32.560 --> 0:14:35.160
<v Speaker 1>a question about just sort of the nature of planets,

0:14:35.280 --> 0:14:38.240
<v Speaker 1>Like we have an interest in how many planets are

0:14:38.240 --> 0:14:40.440
<v Speaker 1>out there, how do they form, what do they look like?

0:14:40.680 --> 0:14:43.760
<v Speaker 1>Are their potential homes for humanity out there? And to

0:14:43.760 --> 0:14:45.640
<v Speaker 1>get an answers to that, we really need to know

0:14:45.720 --> 0:14:47.800
<v Speaker 1>like how planets warm and what they're made out of

0:14:47.840 --> 0:14:49.200
<v Speaker 1>it that will give us an answer to like what

0:14:49.280 --> 0:14:51.200
<v Speaker 1>they're like on the surface. So we got to know

0:14:51.240 --> 0:14:53.160
<v Speaker 1>how the insides work if we want to figure out

0:14:53.240 --> 0:14:55.760
<v Speaker 1>how the outsides look. Yeah, because you know, it's still

0:14:55.920 --> 0:14:59.360
<v Speaker 1>kind of a big mystery in astrophysics and in science

0:14:59.560 --> 0:15:01.600
<v Speaker 1>is how do the Solar System form and out of

0:15:01.680 --> 0:15:05.160
<v Speaker 1>these planets specifically form in in an early version of

0:15:05.160 --> 0:15:07.000
<v Speaker 1>the solar system, right, and it's still kind of a

0:15:07.000 --> 0:15:09.920
<v Speaker 1>big question. We're still running simulations and trying to figure

0:15:10.040 --> 0:15:12.480
<v Speaker 1>that out. Yeah, we talked about on this podcast we

0:15:12.480 --> 0:15:15.680
<v Speaker 1>don't even really understand how our solar system came to be,

0:15:16.000 --> 0:15:18.920
<v Speaker 1>Like we run models about our solar system doesn't really

0:15:19.000 --> 0:15:21.760
<v Speaker 1>quite make sense, Like why is Mars so small? And

0:15:21.960 --> 0:15:24.560
<v Speaker 1>why do we have very few planets close to our

0:15:24.560 --> 0:15:27.280
<v Speaker 1>Sun whereas many other solar systems have lots and lots

0:15:27.320 --> 0:15:30.600
<v Speaker 1>of planets in between the distance between our Sun and Mercury.

0:15:30.720 --> 0:15:32.400
<v Speaker 1>So we want to know the answer to that question,

0:15:32.440 --> 0:15:35.320
<v Speaker 1>like what is the story of our solar system? For me,

0:15:35.360 --> 0:15:37.560
<v Speaker 1>it drives me crazy to think that there's an exciting,

0:15:37.600 --> 0:15:40.480
<v Speaker 1>traumatic story something that happened here and we just don't

0:15:40.520 --> 0:15:44.960
<v Speaker 1>know it. Maybe were coextruded by the great planet factoring

0:15:45.000 --> 0:15:48.000
<v Speaker 1>the sky, a new creation myth folks born here today

0:15:48.000 --> 0:15:53.440
<v Speaker 1>on the podcast, co extrusion sounds like a good novel name. Yeah,

0:15:53.520 --> 0:15:55.480
<v Speaker 1>And you know, there are folks who do that kind

0:15:55.480 --> 0:15:58.120
<v Speaker 1>of study, like look for other planets and other solar systems.

0:15:58.120 --> 0:16:00.640
<v Speaker 1>They look for exoplanets, and then there's a whole community

0:16:00.680 --> 0:16:03.400
<v Speaker 1>people who just study like the planets in our solar

0:16:03.440 --> 0:16:06.320
<v Speaker 1>system and what's in them. People who dedicate their entire

0:16:06.400 --> 0:16:10.320
<v Speaker 1>research careers to like this question what's inside Mars, And

0:16:10.360 --> 0:16:12.400
<v Speaker 1>you're saying that there might be parallels but the Earth

0:16:12.440 --> 0:16:16.400
<v Speaker 1>as well, Like knowing what happened to Mars might help

0:16:16.480 --> 0:16:19.360
<v Speaker 1>us understand what's happening here in Earth and let us

0:16:19.360 --> 0:16:22.560
<v Speaker 1>study things like earthquakes and what we can expect in

0:16:22.600 --> 0:16:25.200
<v Speaker 1>the future. Absolutely, you never want to just have any

0:16:25.200 --> 0:16:27.320
<v Speaker 1>equals one, right. You don't want to base all of

0:16:27.360 --> 0:16:30.600
<v Speaker 1>your conclusions about how planets work from one example. You

0:16:30.640 --> 0:16:31.840
<v Speaker 1>want to look at a bunch of them. You want

0:16:31.840 --> 0:16:34.240
<v Speaker 1>to population so you can get a sense for what's typical,

0:16:34.360 --> 0:16:37.040
<v Speaker 1>and you can also see the future, Like if Mars

0:16:37.360 --> 0:16:40.560
<v Speaker 1>is smaller and colder than Earth, then in some sense

0:16:40.560 --> 0:16:42.720
<v Speaker 1>it might be what the future of Earth looks like,

0:16:42.880 --> 0:16:45.480
<v Speaker 1>you know, in millions and billions of years. But it'd

0:16:45.480 --> 0:16:47.720
<v Speaker 1>be good to get an understanding of how these processes

0:16:47.760 --> 0:16:49.720
<v Speaker 1>work because we rely on the Earth to have these

0:16:49.800 --> 0:16:53.320
<v Speaker 1>layers in order to have our civilization and our society function.

0:16:53.440 --> 0:16:55.280
<v Speaker 1>So it would be good to know, like the factors

0:16:55.320 --> 0:16:57.880
<v Speaker 1>that control that, What are the forces at play? Are

0:16:57.920 --> 0:17:00.560
<v Speaker 1>things rising or sinking or cooling or eating or what's

0:17:00.600 --> 0:17:03.080
<v Speaker 1>going on inside. So absolutely we want to get a

0:17:03.120 --> 0:17:06.320
<v Speaker 1>better handle on the interior mechanisms of our planet. And

0:17:06.359 --> 0:17:09.240
<v Speaker 1>it's all right there, hidden under the surface, bubbling up

0:17:09.359 --> 0:17:11.840
<v Speaker 1>or maybe just chilling out. Let's get into whether or

0:17:11.840 --> 0:17:15.800
<v Speaker 1>not Mars has a solid or liquid core and whether

0:17:15.880 --> 0:17:31.440
<v Speaker 1>we'll ever know. But first let's take a quick we're

0:17:31.440 --> 0:17:34.520
<v Speaker 1>talking about whether Mars the planet, right, not the Mars bars,

0:17:34.560 --> 0:17:36.760
<v Speaker 1>because we know those have a newgat center, right, But

0:17:37.000 --> 0:17:41.119
<v Speaker 1>isnt a liquid or a solid? Oh no, another you

0:17:41.119 --> 0:17:45.080
<v Speaker 1>have a whole episode on strange matter from in candies.

0:17:45.359 --> 0:17:48.639
<v Speaker 1>Daniel vapes various candies. That's in my new podcast series,

0:17:49.200 --> 0:17:53.119
<v Speaker 1>one episode long. You just blew my mind vaping. What

0:17:53.160 --> 0:17:55.760
<v Speaker 1>does that even mean? Oh my goodness, how could it

0:17:55.760 --> 0:17:58.080
<v Speaker 1>be possible that nobody's ever tried that before, you know,

0:17:58.960 --> 0:18:01.760
<v Speaker 1>after raping other stuff, since somebody must have had that idea.

0:18:02.080 --> 0:18:05.920
<v Speaker 1>Oh man, I think you're in the run business, Daniel. Alright,

0:18:05.920 --> 0:18:07.840
<v Speaker 1>So we're trying to figure out whether Mars has a

0:18:07.920 --> 0:18:10.880
<v Speaker 1>solid or liquid core, not just for curiosity about what's

0:18:10.920 --> 0:18:13.360
<v Speaker 1>going on there, but I might tell about the history

0:18:13.480 --> 0:18:16.399
<v Speaker 1>of our planet and the whole Solar System. And so Daniel,

0:18:16.400 --> 0:18:18.480
<v Speaker 1>you actually went out there and talked to an expert

0:18:18.560 --> 0:18:21.439
<v Speaker 1>on this topic. Right, that's right. I called up a

0:18:21.480 --> 0:18:24.320
<v Speaker 1>colleague of mine, Katherine Johnson. She's at the University of

0:18:24.320 --> 0:18:26.959
<v Speaker 1>British Columbia, and I asked her why she was so

0:18:27.000 --> 0:18:30.040
<v Speaker 1>excited about this particular question. Here's what she had to say.

0:18:30.400 --> 0:18:32.920
<v Speaker 1>So then it's my pleasure to introduce to the program

0:18:32.960 --> 0:18:36.560
<v Speaker 1>professor Katherine Johnson. Catherine said hello to our listeners and

0:18:36.560 --> 0:18:40.120
<v Speaker 1>tell them a little bit about yourself. Hi. So it's

0:18:40.160 --> 0:18:43.520
<v Speaker 1>pressure to be here. And I'm a faculty member at

0:18:43.520 --> 0:18:46.680
<v Speaker 1>the University of British Columbia in Vancouver and also a

0:18:46.720 --> 0:18:50.439
<v Speaker 1>scientist at the Planetary Science Institute a Tucson and I

0:18:50.520 --> 0:18:54.639
<v Speaker 1>work in geophysics in uh sort of planetary science. So

0:18:54.760 --> 0:19:00.080
<v Speaker 1>I'm interested in understanding the interior state and evolution of

0:19:00.080 --> 0:19:04.640
<v Speaker 1>of the planets, moons, and asteroids in our Solar system.

0:19:04.680 --> 0:19:06.960
<v Speaker 1>And tell me why that's exciting for you. What is

0:19:06.960 --> 0:19:09.840
<v Speaker 1>it about the interior of Mars, for example, that makes

0:19:09.840 --> 0:19:12.360
<v Speaker 1>you curious, that makes you wonder what's going on inside there?

0:19:12.640 --> 0:19:14.960
<v Speaker 1>So you know, one of the reasons that I like

0:19:15.080 --> 0:19:17.560
<v Speaker 1>to think about other planets is really to try to

0:19:17.640 --> 0:19:20.000
<v Speaker 1>understand our own planet better. I think you know, for me,

0:19:20.160 --> 0:19:24.080
<v Speaker 1>that's one of the major motivations to try to understand

0:19:24.080 --> 0:19:26.960
<v Speaker 1>planets in our own solar system, especially in the inner

0:19:27.000 --> 0:19:31.840
<v Speaker 1>Solar system right where we have Mercury, Venus, the Earth, Mars,

0:19:31.840 --> 0:19:35.120
<v Speaker 1>our own Moon, and they're all completely different from each other,

0:19:35.320 --> 0:19:38.280
<v Speaker 1>even though they started in somewhat similar at least with

0:19:38.320 --> 0:19:41.600
<v Speaker 1>the exception of the Moon, started in somewhat similar ways.

0:19:41.800 --> 0:19:44.119
<v Speaker 1>And so a lot of this really has to do

0:19:44.640 --> 0:19:47.679
<v Speaker 1>with their interiors and how they are interiors of like

0:19:48.240 --> 0:19:52.840
<v Speaker 1>shaped their histories. All right, Thank you, Katherine. And so

0:19:53.040 --> 0:19:55.359
<v Speaker 1>you went and chatted with her about this topic, Yeah,

0:19:55.359 --> 0:19:57.840
<v Speaker 1>I did. We had a really fun conversation after all

0:19:57.880 --> 0:20:00.440
<v Speaker 1>about it. Learned a lot of gory details of how

0:20:00.440 --> 0:20:04.040
<v Speaker 1>the project works and the politics of getting her instrument

0:20:04.119 --> 0:20:06.159
<v Speaker 1>up and on Mars and how that all works. It

0:20:06.240 --> 0:20:07.960
<v Speaker 1>was a lot of fun. Thanks Catherine very much for

0:20:08.080 --> 0:20:11.440
<v Speaker 1>educating me about your research. She has an instrument on Mars.

0:20:11.480 --> 0:20:16.160
<v Speaker 1>She does exactly. She helped design and build this seizedmometer

0:20:16.280 --> 0:20:17.840
<v Speaker 1>that they have on Mars, which is one of the

0:20:17.840 --> 0:20:21.359
<v Speaker 1>ways they figure out what's inside. Interesting because that is

0:20:21.400 --> 0:20:23.080
<v Speaker 1>sort of a way they do it here on Earth. Right,

0:20:23.200 --> 0:20:25.840
<v Speaker 1>we haven't actually like dug a hole or a little

0:20:25.840 --> 0:20:28.159
<v Speaker 1>people to the center of the earth. We have just

0:20:28.320 --> 0:20:31.720
<v Speaker 1>models and kind of sound and sound wave detections on

0:20:31.720 --> 0:20:33.600
<v Speaker 1>the surface, right, that's right. We have dug in only

0:20:33.760 --> 0:20:37.440
<v Speaker 1>very shallow holes relatively speaking, into the earth, and so

0:20:37.520 --> 0:20:40.960
<v Speaker 1>we have not actually probed physically the center of the Earth.

0:20:41.000 --> 0:20:43.200
<v Speaker 1>But we do have a pretty good picture of what's

0:20:43.200 --> 0:20:46.880
<v Speaker 1>going on inside the earth because of earthquakes. Every time

0:20:46.920 --> 0:20:49.520
<v Speaker 1>there's an earthquake, it's like the earth rings sort of

0:20:49.560 --> 0:20:51.840
<v Speaker 1>like a bell, and the waves they don't just like

0:20:52.040 --> 0:20:55.080
<v Speaker 1>shake the outer crust, they propagate all the way through

0:20:55.119 --> 0:20:58.280
<v Speaker 1>the interior. And when waves cross a threshold, like when

0:20:58.280 --> 0:21:00.639
<v Speaker 1>you go from solid to liquid, or the quit to solid,

0:21:00.680 --> 0:21:03.480
<v Speaker 1>or one kind of metal or to another, you get reflections.

0:21:03.480 --> 0:21:05.480
<v Speaker 1>Just like when light hits a piece of glass, most

0:21:05.480 --> 0:21:07.679
<v Speaker 1>of it goes through, but some of it reflects. So

0:21:07.760 --> 0:21:10.560
<v Speaker 1>these reflections and the interior of the earth make for

0:21:10.680 --> 0:21:13.439
<v Speaker 1>really complicated patterns. But if you have a bunch of

0:21:13.440 --> 0:21:16.160
<v Speaker 1>seized momometers all over the earth that measure the shaking,

0:21:16.480 --> 0:21:19.000
<v Speaker 1>you can get a really nice picture of exactly how

0:21:19.000 --> 0:21:21.879
<v Speaker 1>this wave propagated through the earth. And then from that

0:21:21.920 --> 0:21:23.560
<v Speaker 1>you can back out like, oh, there must have been

0:21:23.560 --> 0:21:25.440
<v Speaker 1>a layer here, and it must have been a layer there,

0:21:25.720 --> 0:21:28.840
<v Speaker 1>and you can make really detailed measurements about the composition

0:21:28.880 --> 0:21:31.159
<v Speaker 1>and the density and the flow of those layers. And

0:21:31.200 --> 0:21:33.440
<v Speaker 1>so she has some instruments on Mars, and are the

0:21:33.560 --> 0:21:35.719
<v Speaker 1>earthquakes on Mars as she is, she can measure there

0:21:35.720 --> 0:21:42.200
<v Speaker 1>are no earthquakes on Mars. There are Mars quakes, Martian quakes. Yeah,

0:21:42.200 --> 0:21:44.520
<v Speaker 1>they actually only have one sized momometer on Mars, so

0:21:44.520 --> 0:21:46.480
<v Speaker 1>it's a little trickier, but we'll dig into it in

0:21:46.520 --> 0:21:48.560
<v Speaker 1>detail in a few minutes, all right. And I like

0:21:48.600 --> 0:21:51.920
<v Speaker 1>how she talked about how every planet is different and

0:21:51.960 --> 0:21:54.800
<v Speaker 1>how like the insights tell you a lot about your history.

0:21:55.400 --> 0:21:57.200
<v Speaker 1>I guess that's true for people to write like you

0:21:57.240 --> 0:21:59.160
<v Speaker 1>can look at my veins and be like, this guy

0:21:59.200 --> 0:22:03.040
<v Speaker 1>hit a lot of peanut butter. Unfortunately, sometimes our interiors

0:22:03.080 --> 0:22:06.399
<v Speaker 1>do reveal our history exactly, and every planet has a

0:22:06.480 --> 0:22:09.360
<v Speaker 1>very different story. And the thing that always surprises me

0:22:09.440 --> 0:22:12.520
<v Speaker 1>is to realize that these stories change with time. You know,

0:22:12.520 --> 0:22:14.600
<v Speaker 1>It's not like Venus has always looking the way it

0:22:14.640 --> 0:22:16.920
<v Speaker 1>does today and that Mars has always looked the way

0:22:16.960 --> 0:22:19.199
<v Speaker 1>it does today. You know, right now, the surface of

0:22:19.240 --> 0:22:22.840
<v Speaker 1>Mars is very cool and inactive. But scientists think that

0:22:22.880 --> 0:22:26.200
<v Speaker 1>Mars had volcanoes active on its surface up to maybe

0:22:26.240 --> 0:22:29.520
<v Speaker 1>like a million years ago, which is basically no time

0:22:29.560 --> 0:22:32.760
<v Speaker 1>at all in the billions of years history of Mars.

0:22:32.800 --> 0:22:35.680
<v Speaker 1>So like, this is an active story that's still developing.

0:22:35.920 --> 0:22:38.760
<v Speaker 1>We're in the middle of history. We are history is

0:22:38.800 --> 0:22:41.479
<v Speaker 1>being made exactly all right, Well, maybe it step us

0:22:41.480 --> 0:22:44.240
<v Speaker 1>through here. Why do we think Mars might have a

0:22:44.400 --> 0:22:47.919
<v Speaker 1>solid core? Like where did this idea first come from?

0:22:47.960 --> 0:22:49.760
<v Speaker 1>And why do we need to assume that? Well, you know,

0:22:49.800 --> 0:22:51.640
<v Speaker 1>we just didn't know for a long time. I think

0:22:51.720 --> 0:22:54.440
<v Speaker 1>the popular conception is that Mars has a solid core

0:22:54.640 --> 0:22:58.280
<v Speaker 1>just because it's smaller and colder. Right, Mars is really

0:22:58.320 --> 0:23:00.720
<v Speaker 1>weird and small. People might not realized. But it has

0:23:00.760 --> 0:23:03.280
<v Speaker 1>like a tenth of the mass of the Earth, so

0:23:03.320 --> 0:23:06.560
<v Speaker 1>it's really a much smaller chunk of stuff than the

0:23:06.560 --> 0:23:08.720
<v Speaker 1>Earth is. Well, I really a ten I knew it

0:23:08.760 --> 0:23:11.840
<v Speaker 1>was smaller, but I didn't know it's ten times smaller, lighter. Yeah,

0:23:11.840 --> 0:23:15.240
<v Speaker 1>it's you know, maybe ten but it's just like not

0:23:15.320 --> 0:23:17.840
<v Speaker 1>really that much stuff. And people think that it might

0:23:17.880 --> 0:23:20.160
<v Speaker 1>be Jupiter's fault, you know, Jupiter might have come into

0:23:20.200 --> 0:23:23.680
<v Speaker 1>the inner solar system earlier on, like millions and billions

0:23:23.680 --> 0:23:25.760
<v Speaker 1>of years ago, and sort of pushed away a lot

0:23:25.760 --> 0:23:28.199
<v Speaker 1>of the stuff that might have helped make Mars bigger.

0:23:28.480 --> 0:23:31.080
<v Speaker 1>That might be one reason why Mars is small. But that's,

0:23:31.160 --> 0:23:33.359
<v Speaker 1>you know, just a mystery. But in the end, Mars

0:23:33.400 --> 0:23:35.440
<v Speaker 1>is a smaller chunk of stuff, and a smaller chunk

0:23:35.480 --> 0:23:38.120
<v Speaker 1>of stuff doesn't have as much gravity, so it doesn't

0:23:38.119 --> 0:23:40.920
<v Speaker 1>have as much pressure and high temperature stuff and its interior,

0:23:41.240 --> 0:23:44.199
<v Speaker 1>and it cools faster. So there's this sense that Mars is,

0:23:44.240 --> 0:23:46.879
<v Speaker 1>like being a smaller rock, has a less chance to

0:23:46.920 --> 0:23:49.399
<v Speaker 1>have a molten core than Earth does. Like you know,

0:23:49.560 --> 0:23:52.200
<v Speaker 1>asteroids out there don't have molten corks. They're not big

0:23:52.320 --> 0:23:55.680
<v Speaker 1>enough to generate that pressure and temperate in their interiors. Oh,

0:23:55.720 --> 0:23:57.960
<v Speaker 1>I see, So that's where I guess you might first

0:23:57.960 --> 0:24:01.240
<v Speaker 1>assume that Mars has a solid core, and we also

0:24:01.280 --> 0:24:04.159
<v Speaker 1>know just have a magnetic field, right, I mean, I

0:24:04.160 --> 0:24:06.800
<v Speaker 1>guess if I said this, like they took a compass

0:24:06.840 --> 0:24:08.680
<v Speaker 1>to Mars and it didn't work. Yeah, there's lots of

0:24:08.720 --> 0:24:11.680
<v Speaker 1>satellites orbiting Mars looking for magnetic fields and they don't

0:24:11.720 --> 0:24:13.280
<v Speaker 1>have one. But if you look at some of the

0:24:13.359 --> 0:24:16.439
<v Speaker 1>rocks on Mars, you can see fossil evidence for a

0:24:16.480 --> 0:24:19.359
<v Speaker 1>magnetic field. That means that we know that Mars used

0:24:19.400 --> 0:24:22.080
<v Speaker 1>to have a magnetic field. So that sort of adds

0:24:22.119 --> 0:24:24.600
<v Speaker 1>to the narrative, like maybe Mars when it was young

0:24:24.760 --> 0:24:29.360
<v Speaker 1>and hot, literally had a flowing interior core that generated

0:24:29.359 --> 0:24:32.399
<v Speaker 1>this magnetic field. But it's gone now, and so maybe

0:24:32.400 --> 0:24:35.119
<v Speaker 1>that like locked up and there's no longer any motion

0:24:35.200 --> 0:24:36.720
<v Speaker 1>in the core. Yeah. I used to be a lot

0:24:36.720 --> 0:24:40.000
<v Speaker 1>more magnetic when I was younger, and otter too, but no,

0:24:40.119 --> 0:24:42.000
<v Speaker 1>I'm just cool. Yeah, back when you had a better

0:24:42.040 --> 0:24:46.840
<v Speaker 1>interior flow. Yeah, back when were his clogged with candy killings?

0:24:47.160 --> 0:24:48.879
<v Speaker 1>All right, So then where did this idea that it

0:24:48.920 --> 0:24:51.160
<v Speaker 1>could be liquid? And I mean, it seems pretty reasonable

0:24:51.200 --> 0:24:54.240
<v Speaker 1>for it to be solid and likely, but what makes

0:24:54.280 --> 0:24:56.639
<v Speaker 1>this thing it could have a liquid core? Well, you know,

0:24:56.720 --> 0:24:58.959
<v Speaker 1>we just don't know, And so one question is like,

0:24:59.119 --> 0:25:01.480
<v Speaker 1>maybe we think it has a solid core, but let's

0:25:01.560 --> 0:25:04.800
<v Speaker 1>go check. Remember a lot of the amazing discoveries we've

0:25:04.880 --> 0:25:07.480
<v Speaker 1>made in history come from just sort of checking off

0:25:07.560 --> 0:25:10.080
<v Speaker 1>things where we didn't expect to find anything interesting. Like

0:25:10.440 --> 0:25:13.800
<v Speaker 1>let's check to see how quickly galaxies rotate. Oh my, gosh,

0:25:13.880 --> 0:25:16.920
<v Speaker 1>they're rotating way too fast. That's how we discovered dark matter.

0:25:17.240 --> 0:25:19.680
<v Speaker 1>Let's check to see what happens when we shoot photons

0:25:19.680 --> 0:25:22.159
<v Speaker 1>at this metal that seems boring. Oh my gosh, we

0:25:22.200 --> 0:25:25.399
<v Speaker 1>discover quantum mechanics. So there's lots of wonderful opportunities to

0:25:25.400 --> 0:25:28.120
<v Speaker 1>discover things when you just sort of do basic checks.

0:25:28.119 --> 0:25:30.159
<v Speaker 1>So that's number one. I guess you don't want to

0:25:30.200 --> 0:25:32.440
<v Speaker 1>go around the university just assuming things right. You want

0:25:32.440 --> 0:25:35.640
<v Speaker 1>to actually make sure. Yeah, that's why we do experiments right,

0:25:35.680 --> 0:25:38.679
<v Speaker 1>because often the results are a surprise, and those are

0:25:38.680 --> 0:25:41.240
<v Speaker 1>the most delicious times in science, right when you get

0:25:41.280 --> 0:25:44.399
<v Speaker 1>a result that surprises you, that doesn't make sense, it

0:25:44.440 --> 0:25:47.280
<v Speaker 1>conflicts with your idea of the universe, and that's how

0:25:47.320 --> 0:25:49.680
<v Speaker 1>you learn, right, that's what science is. But then people

0:25:49.720 --> 0:25:53.200
<v Speaker 1>also realize that we didn't actually have conclusive evidence that

0:25:53.560 --> 0:25:55.719
<v Speaker 1>Mars had a solid core, that you could build a

0:25:55.800 --> 0:25:58.360
<v Speaker 1>model of Mars with a liquid core that was still

0:25:58.440 --> 0:26:01.200
<v Speaker 1>consistent with everything we saw and we knew about Mars.

0:26:01.400 --> 0:26:03.640
<v Speaker 1>But I guess maybe the question is could it be liquid?

0:26:03.680 --> 0:26:06.400
<v Speaker 1>I mean, if it doesn't have a magnetic field, wouldn't that,

0:26:06.600 --> 0:26:08.400
<v Speaker 1>you know, tell us that it has a solid core,

0:26:08.760 --> 0:26:13.119
<v Speaker 1>not necessarily, because the magnetic field actually requires two different things.

0:26:13.160 --> 0:26:16.760
<v Speaker 1>It requires some liquid, but it also requires flow, Like

0:26:16.800 --> 0:26:19.000
<v Speaker 1>that liquid has to be in motion. There needs to

0:26:19.000 --> 0:26:22.040
<v Speaker 1>be some sort of like circulation of that liquid. Because

0:26:22.040 --> 0:26:24.600
<v Speaker 1>remember the dynamo effect that gives you a magnetic field

0:26:24.880 --> 0:26:27.760
<v Speaker 1>doesn't just come from having liquid sitting around. It comes

0:26:27.760 --> 0:26:31.920
<v Speaker 1>from currents right ionized particles in motion. So it's possible

0:26:32.000 --> 0:26:34.560
<v Speaker 1>that Mars has a liquid, but that liquid isn't flowing

0:26:34.600 --> 0:26:37.480
<v Speaker 1>in the right way to give you a magnetic field. Oh,

0:26:37.560 --> 0:26:40.159
<v Speaker 1>I see. It could just be like liquid center just

0:26:40.200 --> 0:26:42.320
<v Speaker 1>sitting there. Yeah. Or you could have a liquid layer

0:26:42.359 --> 0:26:45.000
<v Speaker 1>between two other solid layers and it could just be

0:26:45.040 --> 0:26:47.360
<v Speaker 1>sort of like too thin to have the right kind

0:26:47.400 --> 0:26:50.119
<v Speaker 1>of rotating currents. Or it might just be the like

0:26:50.359 --> 0:26:53.520
<v Speaker 1>the heat difference between that liquid layer and the next

0:26:53.560 --> 0:26:55.919
<v Speaker 1>layer isn't great enough to get like the convection. You

0:26:56.000 --> 0:26:58.280
<v Speaker 1>need to have flow, don't. You also need like to

0:26:58.359 --> 0:27:01.199
<v Speaker 1>have special metals in that you know, liquid layer for

0:27:01.240 --> 0:27:03.640
<v Speaker 1>you to get the magnetic field, Like is an iron

0:27:04.359 --> 0:27:06.639
<v Speaker 1>in our molten core a big part of why we

0:27:06.680 --> 0:27:08.879
<v Speaker 1>have a magnetic field, yeah, exactly, And so you need

0:27:08.920 --> 0:27:11.480
<v Speaker 1>to be open to those possibilities. We do think, based

0:27:11.520 --> 0:27:14.520
<v Speaker 1>on density estimates, that there is a big iron nickel

0:27:14.560 --> 0:27:17.000
<v Speaker 1>core to Mars. So the question is really is some

0:27:17.040 --> 0:27:19.239
<v Speaker 1>of it liquid or is it all solid? But you're right,

0:27:19.240 --> 0:27:21.640
<v Speaker 1>you need some metal. If you had just like a

0:27:21.640 --> 0:27:24.399
<v Speaker 1>core of you know, ceramic or whatever, something that was

0:27:24.400 --> 0:27:27.280
<v Speaker 1>totally insulating, then you couldn't get a magnetic feel from

0:27:27.320 --> 0:27:29.520
<v Speaker 1>that has to conduct electricity. So it could have a

0:27:29.600 --> 0:27:32.760
<v Speaker 1>liquid core. Mars could look sort of small and cold,

0:27:32.880 --> 0:27:35.920
<v Speaker 1>but it could be inside you know, frosthing or seating

0:27:36.040 --> 0:27:40.360
<v Speaker 1>or you know, have a soft, squishy center or layer. Absolutely,

0:27:40.560 --> 0:27:43.000
<v Speaker 1>and that's a really exciting moment in science when you realize,

0:27:43.119 --> 0:27:45.560
<v Speaker 1>hold on a second, you know, everything we thought was

0:27:45.600 --> 0:27:50.320
<v Speaker 1>true could be different. This other theories actually totally consistent

0:27:50.359 --> 0:27:53.160
<v Speaker 1>with everything we know. And that's exciting because it gives

0:27:53.160 --> 0:27:55.639
<v Speaker 1>you like two possibilities to explore. It gives you an

0:27:55.640 --> 0:27:58.240
<v Speaker 1>opportunity to be surprised. Then, I guess the big question

0:27:58.280 --> 0:28:00.760
<v Speaker 1>then is if it could be liquid inside, how could

0:28:00.840 --> 0:28:03.040
<v Speaker 1>we ever know? I mean, we're sitting here, thousands and

0:28:03.040 --> 0:28:06.600
<v Speaker 1>thousands of miles away, sending small robots one at a time.

0:28:06.960 --> 0:28:09.800
<v Speaker 1>How are we going to find out what's inside? Daniel. Yeah, Well,

0:28:09.840 --> 0:28:11.840
<v Speaker 1>it turns out we have lots of different ways to

0:28:11.840 --> 0:28:14.280
<v Speaker 1>prove this question, some of which we can do without

0:28:14.320 --> 0:28:16.880
<v Speaker 1>actually going to the surface of Mars. One of them

0:28:16.920 --> 0:28:19.679
<v Speaker 1>is really cool is that they measure basically how squishy

0:28:19.800 --> 0:28:23.320
<v Speaker 1>Mars is. They have a satellite which rotates around Mars

0:28:23.520 --> 0:28:26.080
<v Speaker 1>and basically it's imaging its surface and making a picture

0:28:26.080 --> 0:28:28.800
<v Speaker 1>of like the shape of Mars, how spherical is it?

0:28:29.040 --> 0:28:32.520
<v Speaker 1>Because Mars, like everything else, is getting squeezed by the Sun.

0:28:32.880 --> 0:28:36.080
<v Speaker 1>Remember we talked about tidal forces, how the gravitational force

0:28:36.119 --> 0:28:38.840
<v Speaker 1>on an object is stronger on the side that's closer

0:28:38.880 --> 0:28:41.320
<v Speaker 1>to the Sun than further from the Sun. Or for example,

0:28:41.360 --> 0:28:44.760
<v Speaker 1>this is why Jupiter's moon Io has hot interior, because

0:28:44.760 --> 0:28:48.040
<v Speaker 1>it's getting squeezed by these tidal forces. Well, Mars is

0:28:48.040 --> 0:28:51.000
<v Speaker 1>getting squeezed by the Sun, and it would get squeezed

0:28:51.000 --> 0:28:54.200
<v Speaker 1>differently if it had a liquid center or some liquid

0:28:54.280 --> 0:28:57.040
<v Speaker 1>layers than if it was totally solid. Basically would get

0:28:57.040 --> 0:29:00.200
<v Speaker 1>squished more So by measuring really precisely the shape of

0:29:00.240 --> 0:29:02.720
<v Speaker 1>Mars as it spins and goes around the Sun, you

0:29:02.760 --> 0:29:04.480
<v Speaker 1>can get a sense for whether or not it has

0:29:04.480 --> 0:29:06.960
<v Speaker 1>a liquid layer. You mean, like as it goes around

0:29:06.960 --> 0:29:09.640
<v Speaker 1>the Sun or as it spins around its axis. Yeah,

0:29:09.720 --> 0:29:11.840
<v Speaker 1>basically the important thing is which side of it is

0:29:11.880 --> 0:29:14.040
<v Speaker 1>facing the Sun, because that's the part that's getting sort

0:29:14.040 --> 0:29:17.160
<v Speaker 1>of pulled towards the Sun really, and as it spins

0:29:17.160 --> 0:29:19.360
<v Speaker 1>and as it moves around the Sun, a different part

0:29:19.400 --> 0:29:22.040
<v Speaker 1>of it is facing the Sun, and so it's getting squeezed.

0:29:22.160 --> 0:29:25.160
<v Speaker 1>So if it was a solid rock, then it wouldn't

0:29:25.200 --> 0:29:27.920
<v Speaker 1>get really deformed by the gravity of the Sun much

0:29:27.960 --> 0:29:30.280
<v Speaker 1>as it goes around. But if it was liquid inside,

0:29:30.320 --> 0:29:32.040
<v Speaker 1>it might you know, kind of wish, kind of like

0:29:32.040 --> 0:29:35.479
<v Speaker 1>a drop of water in space. Yeah, exactly, That's exactly

0:29:35.480 --> 0:29:38.080
<v Speaker 1>what happens, and so we can measure that, and that

0:29:38.160 --> 0:29:40.520
<v Speaker 1>gives us some clue about whether or not there's a

0:29:40.560 --> 0:29:43.520
<v Speaker 1>liquid or solid layer inside Mars. All right, well, let's

0:29:43.520 --> 0:29:45.120
<v Speaker 1>get into some of the other ways we can tell

0:29:45.200 --> 0:29:48.600
<v Speaker 1>if Mars is soft and squishy on the inside or

0:29:48.640 --> 0:29:50.720
<v Speaker 1>if it's hardcore. So let's get into that. But first

0:29:50.800 --> 0:30:07.280
<v Speaker 1>let's take another quick break. Alright, is Mars hardcore or

0:30:07.520 --> 0:30:10.880
<v Speaker 1>is it just a big squishy or person inside. Now,

0:30:10.920 --> 0:30:12.880
<v Speaker 1>we talked about how we can tell, and we can

0:30:12.880 --> 0:30:16.280
<v Speaker 1>tell sometimes by the tidal effects of the Sun on

0:30:16.320 --> 0:30:19.640
<v Speaker 1>its shape. So that's one way, and that's happening to

0:30:19.840 --> 0:30:22.680
<v Speaker 1>us here on Earth. To Daniel, our Earth is getting squished. Yeah,

0:30:22.720 --> 0:30:25.680
<v Speaker 1>our Earth gets squished by the Sun and by the moon. Right,

0:30:25.880 --> 0:30:27.920
<v Speaker 1>the reason that we have tides in our ocean is

0:30:27.960 --> 0:30:30.680
<v Speaker 1>that the Moon is having exactly that same effect on

0:30:30.720 --> 0:30:34.000
<v Speaker 1>our liquid exterior, and then the Sun has that effect

0:30:34.080 --> 0:30:37.400
<v Speaker 1>on our liquid interior because it squeezes the whole planet.

0:30:37.440 --> 0:30:39.520
<v Speaker 1>All right, Well, what are some of the other ways

0:30:39.520 --> 0:30:43.480
<v Speaker 1>we could tell if Mars is soft or our inside.

0:30:43.560 --> 0:30:45.960
<v Speaker 1>Another way they do it is by measuring it's wobble.

0:30:46.120 --> 0:30:48.480
<v Speaker 1>So Mars is spinning and it's going around the Sun,

0:30:48.800 --> 0:30:51.920
<v Speaker 1>and they measure its orbit very very precisely. And something

0:30:51.920 --> 0:30:54.520
<v Speaker 1>with a liquid center will spin a little bit differently

0:30:54.600 --> 0:30:57.120
<v Speaker 1>than something with a solid center, because the liquid center,

0:30:57.120 --> 0:30:59.920
<v Speaker 1>for example, might not be keeping up with the rest

0:31:00.000 --> 0:31:01.840
<v Speaker 1>of the object, right, it might be flowing at a

0:31:01.880 --> 0:31:04.400
<v Speaker 1>different rate, and that's will affect how Mars sort of

0:31:04.440 --> 0:31:08.280
<v Speaker 1>wobbles as it goes around the Sun and changes its orbit.

0:31:08.680 --> 0:31:13.120
<v Speaker 1>Really because of like conservation of angular momentum, or is

0:31:13.160 --> 0:31:16.560
<v Speaker 1>it just like you know, like moving around a water

0:31:16.600 --> 0:31:18.959
<v Speaker 1>bottle with water in it. It just creates a lot

0:31:18.960 --> 0:31:22.280
<v Speaker 1>of kind of inner forces that kind of throw you off. Yeah. Well,

0:31:22.320 --> 0:31:24.640
<v Speaker 1>there is definitely a different moment of inertia for an

0:31:24.720 --> 0:31:28.120
<v Speaker 1>object that has liquid inside of it because the distributed differently,

0:31:28.160 --> 0:31:30.320
<v Speaker 1>like the density is different, right, So you can get

0:31:30.360 --> 0:31:33.280
<v Speaker 1>a sense for the interior density. But then also, as

0:31:33.320 --> 0:31:35.560
<v Speaker 1>you say, you're gonna get like flows and it's not

0:31:35.600 --> 0:31:37.840
<v Speaker 1>necessarily going to catch up to the rest of Mars.

0:31:38.320 --> 0:31:40.040
<v Speaker 1>And so you can tell sort of like you know,

0:31:40.080 --> 0:31:42.560
<v Speaker 1>the difference between having a liquid and solid based on

0:31:42.640 --> 0:31:45.960
<v Speaker 1>how sort of the angle of Mars spin changes as

0:31:46.000 --> 0:31:47.760
<v Speaker 1>it goes around it. Think of it's sort of like

0:31:47.760 --> 0:31:49.920
<v Speaker 1>a top. You know, a top that has a liquid

0:31:49.920 --> 0:31:52.200
<v Speaker 1>center will spin differently than the top that doesn't have

0:31:52.240 --> 0:31:54.640
<v Speaker 1>a liquid center. Right, Well, a top of the liquid

0:31:54.680 --> 0:31:57.560
<v Speaker 1>tender would slow down faster, wouldn't it. It depends on

0:31:57.600 --> 0:31:59.880
<v Speaker 1>if the liquid is initially spinning. I guess. So that

0:32:00.000 --> 0:32:02.960
<v Speaker 1>another way we can tell we can very carefully kind

0:32:02.960 --> 0:32:05.720
<v Speaker 1>of study the orbit of Mars. Yeah, but then the

0:32:05.720 --> 0:32:07.720
<v Speaker 1>most precise way, of course is to get down to

0:32:07.760 --> 0:32:11.200
<v Speaker 1>the surface and actually measure Mars quakes and use those

0:32:11.240 --> 0:32:14.680
<v Speaker 1>to get an internal picture of what's going on inside Mars. Oh,

0:32:14.720 --> 0:32:18.040
<v Speaker 1>I see, like get onto Mars surface and measure how

0:32:18.800 --> 0:32:22.480
<v Speaker 1>you know, sound ways to travel through the planet precisely.

0:32:22.840 --> 0:32:25.720
<v Speaker 1>And they did this originally on the Viking Landers. They

0:32:25.760 --> 0:32:28.920
<v Speaker 1>actually had seized moometers on the first two Viking Landers,

0:32:29.360 --> 0:32:31.640
<v Speaker 1>but it didn't really work like one of them, it

0:32:31.640 --> 0:32:34.560
<v Speaker 1>didn't deploy, so it didn't get onto the surface, and

0:32:34.640 --> 0:32:38.240
<v Speaker 1>the other one only ever heard one Mars quake, but

0:32:38.280 --> 0:32:41.040
<v Speaker 1>it was before it was actually touching the surface, and

0:32:41.040 --> 0:32:43.680
<v Speaker 1>so it was this very sort of controversial event in

0:32:43.800 --> 0:32:47.600
<v Speaker 1>planetary science community. Had Viking heard of Mars quake or not,

0:32:48.200 --> 0:32:52.600
<v Speaker 1>and so before inside landed on Mars fairly recently, nobody

0:32:52.680 --> 0:32:55.400
<v Speaker 1>knew if there actually were Mars quakes or if it

0:32:55.480 --> 0:32:58.360
<v Speaker 1>was just totally quiet thing. I guess, well, maybe first

0:32:58.360 --> 0:33:00.520
<v Speaker 1>of all, let's take a step back and maybe mentioned

0:33:00.520 --> 0:33:02.760
<v Speaker 1>briefly how you can use sound waves to tell what

0:33:02.800 --> 0:33:05.760
<v Speaker 1>the core looks like like the sound waves traveled differently

0:33:05.800 --> 0:33:08.040
<v Speaker 1>if there was liquid or solid. Yeah, just like we

0:33:08.080 --> 0:33:10.120
<v Speaker 1>do for the Earth, as we talked about earlier. If

0:33:10.120 --> 0:33:13.040
<v Speaker 1>there are Mars quakes, then they generate these compression waves,

0:33:13.040 --> 0:33:16.440
<v Speaker 1>and those compression waves will bounce off of interior layers,

0:33:16.560 --> 0:33:19.120
<v Speaker 1>and so if there's a interface between the layers, like

0:33:19.360 --> 0:33:22.720
<v Speaker 1>a solid mantle and then a liquid layer. Then you'll

0:33:22.760 --> 0:33:25.200
<v Speaker 1>have the sound waves bounce off differently than it's just

0:33:25.360 --> 0:33:28.720
<v Speaker 1>all solid, just like light going through glass or hitting water.

0:33:28.880 --> 0:33:31.160
<v Speaker 1>When you transfer from one medium to another or from

0:33:31.160 --> 0:33:33.560
<v Speaker 1>one density to another, you're gonna get all sorts of

0:33:33.600 --> 0:33:36.440
<v Speaker 1>complicated reflections. And if you measure the sound waves on

0:33:36.480 --> 0:33:38.520
<v Speaker 1>the surface, then you can get a picture of that.

0:33:38.760 --> 0:33:40.400
<v Speaker 1>It can give you a map of the interior of

0:33:40.400 --> 0:33:43.640
<v Speaker 1>the planet I see, and then from the density map

0:33:43.720 --> 0:33:46.040
<v Speaker 1>you can maybe infer like, oh, this part is less dense,

0:33:46.080 --> 0:33:49.239
<v Speaker 1>it must be liquid. But also those transition points are

0:33:49.240 --> 0:33:52.560
<v Speaker 1>really important. You can tell where the transition points are

0:33:52.880 --> 0:33:56.520
<v Speaker 1>by telling when the reflection happened in exactly the direction

0:33:56.600 --> 0:33:59.360
<v Speaker 1>that the wave wind. And we actually have confirmation that

0:33:59.400 --> 0:34:02.800
<v Speaker 1>there are Mars quakes, like we've seen them or felt them,

0:34:02.920 --> 0:34:05.320
<v Speaker 1>or do we know for sure? Yeah, we actually do

0:34:05.400 --> 0:34:08.400
<v Speaker 1>have now. So the inside lander that's sitting on Mars,

0:34:08.480 --> 0:34:11.200
<v Speaker 1>it has the seized momometer on it. And so the

0:34:11.280 --> 0:34:13.960
<v Speaker 1>lander landed and then put out this cute little bubble

0:34:14.160 --> 0:34:16.600
<v Speaker 1>which sits on the surface of Mars, and it's shielded

0:34:16.640 --> 0:34:18.799
<v Speaker 1>from the sun and from the wind, and it just

0:34:18.960 --> 0:34:21.880
<v Speaker 1>listens to the surface of Mars. So before they landed,

0:34:21.880 --> 0:34:24.359
<v Speaker 1>they had all these theories about how you might get

0:34:24.480 --> 0:34:27.960
<v Speaker 1>Mars quakes even without any tectonic activity. Right, there's no

0:34:28.200 --> 0:34:31.360
<v Speaker 1>like plates on Mars. You don't have like earthquakes on

0:34:31.400 --> 0:34:33.640
<v Speaker 1>Mars the same way you have on Earth because you

0:34:33.680 --> 0:34:36.560
<v Speaker 1>don't have tectonic activity. But they thought that you would

0:34:36.560 --> 0:34:39.239
<v Speaker 1>still have little Mars quakes. So they landed this thing

0:34:39.280 --> 0:34:42.480
<v Speaker 1>on Mars and they saw like four hundred and fifty

0:34:42.560 --> 0:34:47.360
<v Speaker 1>Mars quakes in two thousand nineteen. Wait, what four hundred

0:34:47.560 --> 0:34:51.040
<v Speaker 1>Mars quakes a year? Yeah, so more than one every day.

0:34:51.120 --> 0:34:53.640
<v Speaker 1>And these are pretty small. Little quakes are like, you know,

0:34:53.800 --> 0:34:56.280
<v Speaker 1>things that the sizedmometer could pick up but you wouldn't

0:34:56.320 --> 0:34:59.720
<v Speaker 1>necessarily notice. Could it be the Mars inside their caves

0:34:59.800 --> 0:35:03.000
<v Speaker 1>kind partying or something jumping up and down. It's actually

0:35:03.000 --> 0:35:05.799
<v Speaker 1>really fascinating. In order to understand whether they could be

0:35:05.960 --> 0:35:09.600
<v Speaker 1>quakes on Mars without tectonic activity, right, without these tectonic

0:35:09.600 --> 0:35:11.920
<v Speaker 1>plates smashing into each other, they look to see if

0:35:11.920 --> 0:35:16.319
<v Speaker 1>there are earthquakes on Earth far away from the plate boundaries,

0:35:16.640 --> 0:35:18.319
<v Speaker 1>and it turns out that there are, So you can

0:35:18.360 --> 0:35:21.120
<v Speaker 1>get earthquakes even where you don't have plates that can

0:35:21.160 --> 0:35:23.640
<v Speaker 1>come from like the sun heating up big slabs of

0:35:23.719 --> 0:35:27.800
<v Speaker 1>rock which then expand, or things happening underneath that affect

0:35:27.880 --> 0:35:30.960
<v Speaker 1>you know, how the crust is moving. And so from

0:35:31.000 --> 0:35:33.319
<v Speaker 1>those models, they expected there to be a bunch of

0:35:33.320 --> 0:35:35.320
<v Speaker 1>Mars quakes, and then they put this thing on Mars

0:35:35.320 --> 0:35:38.440
<v Speaker 1>and they actually see these quakes. Interesting, like, even if

0:35:38.480 --> 0:35:40.879
<v Speaker 1>there are no liquid core, and there are in any

0:35:40.920 --> 0:35:44.480
<v Speaker 1>like big giant plates of rock floating and crashing into

0:35:44.520 --> 0:35:46.600
<v Speaker 1>each other, you can still get earthquakes just from a

0:35:46.680 --> 0:35:49.160
<v Speaker 1>rock just sitting there getting keated out by the sun. Yeah,

0:35:49.320 --> 0:35:52.080
<v Speaker 1>and that's not something that we understand very very well,

0:35:52.160 --> 0:35:54.480
<v Speaker 1>and so it's something they're curious about. They were really

0:35:54.480 --> 0:35:56.359
<v Speaker 1>curious when they landed this thing, like what we see

0:35:56.360 --> 0:35:58.440
<v Speaker 1>with the level of quakes we expected, or where they

0:35:58.480 --> 0:36:00.320
<v Speaker 1>be a lot more than we expected, will be a

0:36:00.360 --> 0:36:03.600
<v Speaker 1>lot quieter than we expected. They had some pretty good arguments,

0:36:03.600 --> 0:36:06.000
<v Speaker 1>but they just weren't sure. You know. That's why we

0:36:06.040 --> 0:36:08.160
<v Speaker 1>go explore the Solar system. And so we measured four

0:36:08.520 --> 0:36:12.560
<v Speaker 1>and fifty Mars quakes in and then twenty they stopped

0:36:12.560 --> 0:36:16.040
<v Speaker 1>because of the pandemic. Also, No, that's just the latest

0:36:16.080 --> 0:36:18.400
<v Speaker 1>data that they've released, so that's the latest result. But

0:36:18.440 --> 0:36:20.880
<v Speaker 1>you know, they're still analyzing data. This is an active

0:36:20.880 --> 0:36:23.840
<v Speaker 1>area research. They're still collecting data, and they're still waiting

0:36:24.160 --> 0:36:27.000
<v Speaker 1>for a really big quake. So far, they've seen sort

0:36:27.000 --> 0:36:29.160
<v Speaker 1>of a lot of small quakes, and I think they're

0:36:29.160 --> 0:36:31.640
<v Speaker 1>a little bit disappointed. They were hoping for like a

0:36:31.640 --> 0:36:33.840
<v Speaker 1>bunch of big ones, because the big ones are the

0:36:33.840 --> 0:36:36.160
<v Speaker 1>ones that carry a lot of energy and really help

0:36:36.200 --> 0:36:39.160
<v Speaker 1>them see the interior. With the smaller quakes, it doesn't

0:36:39.160 --> 0:36:42.000
<v Speaker 1>penetrate as deeply, so you can't really tell what's going on.

0:36:42.440 --> 0:36:44.440
<v Speaker 1>So they're sort of hanging out waiting to get lucky.

0:36:44.560 --> 0:36:47.480
<v Speaker 1>So they have detected Mars quakes, but there aren't big

0:36:47.600 --> 0:36:49.760
<v Speaker 1>enough for them to sort of be able to see

0:36:49.920 --> 0:36:52.560
<v Speaker 1>much about the inter core. They're not as big as

0:36:52.600 --> 0:36:55.360
<v Speaker 1>they hoped, but you know, they are clever scientists, and

0:36:55.400 --> 0:36:58.640
<v Speaker 1>so they've developed fancy new ideas for how to use

0:36:58.680 --> 0:37:01.560
<v Speaker 1>these to see the interior here anyway, and it's not

0:37:01.719 --> 0:37:04.279
<v Speaker 1>as powerful as they would have hoped until they get

0:37:04.320 --> 0:37:06.600
<v Speaker 1>like a really big one in all of Mars rings

0:37:06.640 --> 0:37:08.879
<v Speaker 1>like a bell. But they have been able to get

0:37:08.880 --> 0:37:11.640
<v Speaker 1>a pretty good picture for what's going on all right, well,

0:37:11.680 --> 0:37:15.080
<v Speaker 1>then that's out there on Mars, and Katherine Johnson is

0:37:15.120 --> 0:37:17.239
<v Speaker 1>one of the scientists on it. So what did she

0:37:17.280 --> 0:37:19.520
<v Speaker 1>say that we've found so far? So I asked her

0:37:19.560 --> 0:37:22.040
<v Speaker 1>to give me the insight on Mars and tell me

0:37:22.080 --> 0:37:24.200
<v Speaker 1>what's going on in the interior. And here's what she

0:37:24.280 --> 0:37:26.360
<v Speaker 1>had to say. So, we've had a good idea for

0:37:26.640 --> 0:37:30.399
<v Speaker 1>quite a while now a decade or so, that the

0:37:30.440 --> 0:37:33.840
<v Speaker 1>deepest interior of Mars is at least partly fluid, but

0:37:33.880 --> 0:37:37.000
<v Speaker 1>we haven't been able to confirm it with seismology, and

0:37:37.120 --> 0:37:39.600
<v Speaker 1>that's something that we're hoping to do with the Insight

0:37:39.800 --> 0:37:42.560
<v Speaker 1>mission that's currently on Mars. And the other thing that

0:37:42.600 --> 0:37:46.200
<v Speaker 1>we really haven't known is how big it's core is.

0:37:46.760 --> 0:37:49.160
<v Speaker 1>This is really important because we don't know exactly how

0:37:49.200 --> 0:37:51.400
<v Speaker 1>big it is. The trade off is it could be

0:37:51.560 --> 0:37:54.560
<v Speaker 1>smaller and pure metal or a bit bigger with some

0:37:54.960 --> 0:37:58.080
<v Speaker 1>light stuff mixed in with it. So it seems like

0:37:58.200 --> 0:38:02.319
<v Speaker 1>Mars does have liquid in its core. Really they can tell, Yeah,

0:38:02.520 --> 0:38:05.200
<v Speaker 1>it's at least partly fluid. That's what she said. And

0:38:05.360 --> 0:38:08.279
<v Speaker 1>all these different methods that we've been using, the Wibble method,

0:38:08.360 --> 0:38:12.080
<v Speaker 1>the Wobble method, and these seismic methods all sort of

0:38:12.120 --> 0:38:14.960
<v Speaker 1>tell the same story that there is some liquid in

0:38:15.000 --> 0:38:18.160
<v Speaker 1>the interior of Mars, interesting like at the core or

0:38:18.200 --> 0:38:20.960
<v Speaker 1>as a layer, probably as a layer on the outer core,

0:38:21.239 --> 0:38:23.000
<v Speaker 1>just like with the Earth. You know, in the Earth,

0:38:23.040 --> 0:38:25.520
<v Speaker 1>as you go into the Earth, you have the mantle

0:38:25.840 --> 0:38:27.440
<v Speaker 1>and then you have sort of an outer core and

0:38:27.600 --> 0:38:31.160
<v Speaker 1>inter core, and there you have like increasing temperature and pressure.

0:38:31.400 --> 0:38:34.040
<v Speaker 1>At first, temperature winds and things are like hot and melty,

0:38:34.280 --> 0:38:36.960
<v Speaker 1>and then as you get to the very center, pressure winds.

0:38:37.040 --> 0:38:39.839
<v Speaker 1>Even though things are still really hot, pressure takes over

0:38:39.880 --> 0:38:41.960
<v Speaker 1>and you have a solid core. So they think that's

0:38:41.960 --> 0:38:44.520
<v Speaker 1>probably what's happening on Mars. Also, you have this core

0:38:44.600 --> 0:38:48.440
<v Speaker 1>that's like eight kilometers and radius and the outer layers

0:38:48.480 --> 0:38:51.400
<v Speaker 1>of it probably liquid, so they feel pretty confident. Then

0:38:51.440 --> 0:38:54.239
<v Speaker 1>they know the answer. So all of our listeners were,

0:38:54.280 --> 0:38:57.439
<v Speaker 1>how wrong, or most of them were, as I would

0:38:57.440 --> 0:39:00.759
<v Speaker 1>have been, But that's pretty surprising. So they found that

0:39:00.880 --> 0:39:03.680
<v Speaker 1>Mars does have a liquid center, Yeah, exactly. Mars is

0:39:03.719 --> 0:39:06.160
<v Speaker 1>still hot and young, and I was surprised as well.

0:39:06.200 --> 0:39:08.640
<v Speaker 1>You know, I also expected Mars to be solid because

0:39:08.680 --> 0:39:11.200
<v Speaker 1>it seems cold and it's small, and I expected things

0:39:11.239 --> 0:39:13.279
<v Speaker 1>will have cooled off and for all the reasons we

0:39:13.280 --> 0:39:15.640
<v Speaker 1>gave before, it seemed like a reasonable guest, but you

0:39:15.719 --> 0:39:18.040
<v Speaker 1>never know until you actually go out there and measure it.

0:39:18.280 --> 0:39:20.920
<v Speaker 1>There are surprises out there waiting for us, and so

0:39:20.960 --> 0:39:23.600
<v Speaker 1>we are still learning a lot about how planets form

0:39:23.800 --> 0:39:26.600
<v Speaker 1>and how they develop into their middle age. Can you

0:39:26.600 --> 0:39:29.319
<v Speaker 1>still call it lava or magma or would it be

0:39:29.360 --> 0:39:31.880
<v Speaker 1>like marthma. I'm not sure what the name of it

0:39:31.880 --> 0:39:34.239
<v Speaker 1>would be, but this is stuff much much deeper than

0:39:34.239 --> 0:39:36.880
<v Speaker 1>the outer layers, right, Magma is actually part of the

0:39:36.920 --> 0:39:39.839
<v Speaker 1>crust that's become liquid because it's become really hot. We're

0:39:39.840 --> 0:39:42.880
<v Speaker 1>talking about stuff that's below the crust, below the mantle,

0:39:43.120 --> 0:39:46.759
<v Speaker 1>down into the core itself, like the real interior Mars.

0:39:46.800 --> 0:39:49.200
<v Speaker 1>This other question of like is there magma still on

0:39:49.239 --> 0:39:53.400
<v Speaker 1>Mars is another fascinating question because vulcanism on Mars seems

0:39:53.440 --> 0:39:55.920
<v Speaker 1>to have ended fairly recently, so it could be that

0:39:56.080 --> 0:39:59.160
<v Speaker 1>inside the crust of Mars there is still some sort

0:39:59.160 --> 0:40:02.719
<v Speaker 1>of hot mac interesting. That's cool. Maybe when we get

0:40:02.760 --> 0:40:06.120
<v Speaker 1>there we could use that for energy. Is that possible, Yeah, absolutely,

0:40:06.120 --> 0:40:08.160
<v Speaker 1>it's possible. You know, I guess it wouldn't be called

0:40:08.280 --> 0:40:14.840
<v Speaker 1>geo thermal energy and be called like mart show thermal energy, yeah,

0:40:15.440 --> 0:40:19.440
<v Speaker 1>mio thermal energy. But Mars has a thicker crust we

0:40:19.520 --> 0:40:21.279
<v Speaker 1>think than the Earth does. We think the crust is

0:40:21.320 --> 0:40:24.400
<v Speaker 1>like fifty to a hundred kilometers thick, so it's probably

0:40:24.400 --> 0:40:26.640
<v Speaker 1>colder and thicker. So it might be harder to find

0:40:26.719 --> 0:40:29.600
<v Speaker 1>a spot where there's still like you know, active magma.

0:40:29.640 --> 0:40:31.480
<v Speaker 1>We don't even know if there is still. But you know,

0:40:31.560 --> 0:40:34.520
<v Speaker 1>Mars had is like volcanic history for billions of years,

0:40:34.600 --> 0:40:37.440
<v Speaker 1>which seems to have ended kind of recently, so it

0:40:37.480 --> 0:40:39.920
<v Speaker 1>would be a surprise if there was totally cold and

0:40:40.000 --> 0:40:42.239
<v Speaker 1>quiet in the interior in terms of the crust. So

0:40:42.239 --> 0:40:46.360
<v Speaker 1>it's just another flavor of peanut butter, maybe crusty, smooth,

0:40:46.440 --> 0:40:50.000
<v Speaker 1>crunchy and crusty. Mars is very multifacet that it is

0:40:50.040 --> 0:40:52.320
<v Speaker 1>not just two layers, man, There are layers and layers

0:40:52.320 --> 0:40:55.399
<v Speaker 1>and layers. Mars was co co co co extruded. All right,

0:40:55.520 --> 0:40:58.360
<v Speaker 1>Well that's a pretty surprising answer, and thank you to

0:40:58.480 --> 0:41:00.799
<v Speaker 1>Katherine Johnson for helping us out. And it just goes

0:41:00.840 --> 0:41:03.160
<v Speaker 1>to show you how many surprises are out there waiting

0:41:03.239 --> 0:41:06.640
<v Speaker 1>in our own backyard or in our neighbor's backyard, and

0:41:06.680 --> 0:41:08.799
<v Speaker 1>you just have to go out there and check, or

0:41:08.840 --> 0:41:11.240
<v Speaker 1>at least, you know, spent a few billion dollars building

0:41:11.239 --> 0:41:14.320
<v Speaker 1>a little robot doesn't for you? Yeah, exactly, build a

0:41:14.320 --> 0:41:17.040
<v Speaker 1>big robot and use it to investigate your neighbor's backyard.

0:41:17.120 --> 0:41:19.640
<v Speaker 1>See how that goes, See how that works out. You

0:41:19.719 --> 0:41:22.360
<v Speaker 1>might call the solar system police on you use it

0:41:22.400 --> 0:41:25.440
<v Speaker 1>to steal their peanut Butterfield pretzels or their vapen so

0:41:25.480 --> 0:41:28.440
<v Speaker 1>you can do some experiments at home. All right, Well,

0:41:28.480 --> 0:41:31.439
<v Speaker 1>we hope you enjoyed then and came away thinking that

0:41:31.680 --> 0:41:33.960
<v Speaker 1>maybe the even our own backyard, It's not what it

0:41:34.000 --> 0:41:37.120
<v Speaker 1>seems sometimes, so keep its gloring, keep asking questions, and

0:41:37.160 --> 0:41:47.640
<v Speaker 1>thanks for tuning in. See you next time. Thanks for listening,

0:41:47.640 --> 0:41:50.360
<v Speaker 1>and remember that Daniel and Jorge Explain the Universe is

0:41:50.400 --> 0:41:53.880
<v Speaker 1>a production of I Heart Radio. For more podcast from

0:41:53.920 --> 0:41:57.680
<v Speaker 1>my Heart Radio, visit the i heart Radio app, Apple Podcasts,

0:41:57.800 --> 0:42:00.080
<v Speaker 1>or wherever you listen to your favorite show. This