WEBVTT - What’s Hidden Inside Planets, with Dr. Sabine Stanley

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<v Speaker 1>Welcome to Stuff to Blow Your Mind production of iHeartRadio.

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<v Speaker 2>Hello, and welcome to Stuff to Blow Your Mind. My

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<v Speaker 2>name is Joe McCormick. My regular co host, Robert Lamb

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<v Speaker 2>is out on vacation the day I'm recording this, but

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<v Speaker 2>he will be back again soon. Today we've got an

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<v Speaker 2>interview for you. This is a chat that I had

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<v Speaker 2>with planetary scientist doctor Sabine Stanley about her twenty twenty

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<v Speaker 2>three book called What's Hidden Inside Planets. This is a

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<v Speaker 2>wonderfully interesting book about the science of planet formation and

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<v Speaker 2>about what we know about the insides of planets near

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<v Speaker 2>and far. A quick bit of author bio before we

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<v Speaker 2>get started here. Doctor Sabine Stanley is a distinguished planetary

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<v Speaker 2>scientist and a key contributor to NASA's Mars Insight mission.

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<v Speaker 2>Holding a PhD in Earth and Planetary Sciences from Harvard

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<v Speaker 2>u University, she focuses on the complexities of planetary interiors.

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<v Speaker 2>Currently a faculty member at a top research university, she

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<v Speaker 2>leads innovative studies in her specialized field. Beyond academia, Doctor

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<v Speaker 2>Stanley is a regular speaker at international scientific conferences and

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<v Speaker 2>serves as a consultant for various space missions. Her research

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<v Speaker 2>has been published in leading scientific journals, earning her multiple

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<v Speaker 2>awards for her contributions to planetary science. With a career

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<v Speaker 2>that blends rigorous research and public engagement, Doctor Stanley remains

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<v Speaker 2>a pivotal voice in the scientific community committed to enhancing

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<v Speaker 2>our cosmic understanding. So I guess now let's jump right

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<v Speaker 2>into our conversation, Doctor Sabine Stanley, Welcome to the podcast.

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<v Speaker 3>Thanks so much for having me.

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<v Speaker 2>So I wanted to start off with the idea something

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<v Speaker 2>you bring up in the preface of your book, which

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<v Speaker 2>is that when non scientists look out at space and

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<v Speaker 2>find things to get excited about, one of the things

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<v Speaker 2>I think that really gets people stirring is the idea

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<v Speaker 2>of an exoplanet with liquid water at the surface, or

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<v Speaker 2>a planet with breathable atmosphere breathable to us. And yet

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<v Speaker 2>you say in your preface that quote, arguably a planet's

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<v Speaker 2>interior is more important than the surface in determining a

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<v Speaker 2>world's fitness for life or ability to withstand the pressures

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<v Speaker 2>put on it by its home star. I think this

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<v Speaker 2>might be really surprising to people. Could you explain this?

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<v Speaker 3>Sure, there are actually two parts to this I would

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<v Speaker 3>say the first is deep inside our planet, in the

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<v Speaker 3>iron core, we actually generate the Earth's magnetic field, and

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<v Speaker 3>magnetic fields when they are generating the core, they come

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<v Speaker 3>all the way out to the surface of the planet

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<v Speaker 3>and they basically surround the planet, and our magnetic field

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<v Speaker 3>acts as this amazing shield stopping these high energy solar

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<v Speaker 3>wind particles from hitting us. Now, when you have these

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<v Speaker 3>high energy particles coming from the Sun, if they actually

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<v Speaker 3>blast it into the planet without the magnetic field there,

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<v Speaker 3>they would work to strip off our atmosphere. They would

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<v Speaker 3>bring high radiation levels to the surface. It would essentially

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<v Speaker 3>not be a really great place to live if we

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<v Speaker 3>didn't have our magnetic field. So one really important thing

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<v Speaker 3>when thinking about is that planet going to be really

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<v Speaker 3>good for say, life to form, is does it have

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<v Speaker 3>a magnetic field and that's really created in deep inside

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<v Speaker 3>the planet. The other aspect of this is that most

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<v Speaker 3>of the reasons that we think the surface of Earth

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<v Speaker 3>is so nice and habitable, right the liquid water, that

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<v Speaker 3>breathable air, all of that is related to a kind

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<v Speaker 3>of recycling process that happens inside Earth. Earth's water a

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<v Speaker 3>lot of it came from outgassing a volcano. So there's

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<v Speaker 3>water deep inside the Earth. When you have volcanic flows

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<v Speaker 3>bringing up magma to the surface, there's lots of gas,

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<v Speaker 3>particles and water in that that eventually makes it out

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<v Speaker 3>into the atmosphere. Carbon dioxide is recycled this way. Water

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<v Speaker 3>is recycled this way. So you can't really just focus

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<v Speaker 3>on the surface. You have to ask how does that

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<v Speaker 3>surface interact with what's going on deep inside planet.

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<v Speaker 2>So when people imagine what's going on deep inside the

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<v Speaker 2>planet and the way it affects the surface, probably what

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<v Speaker 2>first comes to the average non scientist's mind would be

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<v Speaker 2>like earthquakes and volcanic eruptions, But actually it's much more

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<v Speaker 2>entangled than that.

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<v Speaker 3>Yeah. Absolutely, But those are also great examples of ways

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<v Speaker 3>that the interior of our planet is really connected to

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<v Speaker 3>how we experience the surface of a planet. Earthquakes, that's

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<v Speaker 3>because the plates on the surface of the Earth are

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<v Speaker 3>moving around and they descend back into the Earth at

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<v Speaker 3>subduction zones and create these frictional spots between plates that

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<v Speaker 3>create these earthquakes. Right.

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<v Speaker 2>Another great example, there's a false fact that I once

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<v Speaker 2>knew that your book corrected me on if you had

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<v Speaker 2>asked me what was the source of Earth's magnetic field

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<v Speaker 2>that you were just talking about. I would have said

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<v Speaker 2>that it was generated by the spinning of the molten

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<v Speaker 2>liquid core around the Earth's solid iron core because of

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<v Speaker 2>the image of spinning, and I guess there's general knowledge

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<v Speaker 2>that sort of dynamo effect, But in the book you

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<v Speaker 2>explained that that isn't exactly correct. That's not exactly what's

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<v Speaker 2>going on. So what does generate the Earth's magnetic field?

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<v Speaker 3>Yeah, you're absolutely right. This is a common misunderstanding out there,

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<v Speaker 3>even some scientists have it. So it turns out in

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<v Speaker 3>order to generate magnetic fields, you do need to have

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<v Speaker 3>a good electrical conductor, and so having a metal like

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<v Speaker 3>iron in this center of the Earth that helps. You

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<v Speaker 3>do need to have it be liquid or fluid ability

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<v Speaker 3>to move around. But the key thing is the motions

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<v Speaker 3>that can create magnetic fields through, like this dynamo action

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<v Speaker 3>that you talked about. Those motions have to be much

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<v Speaker 3>more complex than just spinning around. So it's not just

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<v Speaker 3>that the Earth is spinning and that's causing it. It's

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<v Speaker 3>actually these like helical type flows that occur because of

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<v Speaker 3>the fact that the Earth is trying to cool down,

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<v Speaker 3>so space is cold. The inside of Earth is hot.

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<v Speaker 3>And so just like if you put a pot of

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<v Speaker 3>soup on the stove, the bottom of the pot is hot,

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<v Speaker 3>the top of the pot is cold. You get that

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<v Speaker 3>boiling action that rolling around. Same thing in the core

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<v Speaker 3>of the Earth, you get these churning motions as the

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<v Speaker 3>hot material at the center of the Earth tries to

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<v Speaker 3>make it up and out to cool down the core

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<v Speaker 3>and then the planet. So it's convection, that's what we

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<v Speaker 3>call it. It's convection. That's the motion that's actually creating

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<v Speaker 3>the magnetic field that Earth has.

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<v Speaker 2>So it's this magnetic dynamo that creates the field that

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<v Speaker 2>can in some ways permit and sustain life on Earth.

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<v Speaker 2>To what extent is Earth unique in this regard? What

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<v Speaker 2>do we know about the presence of a possible dynamo

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<v Speaker 2>in other planets or objects in our Solar system?

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<v Speaker 3>Yeah, great question. So lots of the other planets actually

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<v Speaker 3>do have magnetic field. So all the giant planets, Jupiter, Saturn, Uranus,

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<v Speaker 3>and Neptune, they all have these global magnetic fields generated

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<v Speaker 3>by a dynamo deep inside just like Earth. The smallest

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<v Speaker 3>of the planet's mercury also has a dynamo, and this

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<v Speaker 3>was actually quite a surprise when it was discovered. Now,

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<v Speaker 3>for Mars, it doesn't have a dynamo today, so it

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<v Speaker 3>doesn't have this global MAGNETELD, but it did have one

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<v Speaker 3>in the past. So about four billion years ago, the

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<v Speaker 3>rocks on the surface of Mars were magnetized from a

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<v Speaker 3>dynamo that was active at that time. And then there's Venus.

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<v Speaker 3>For Venus, we have no way to tell if it

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<v Speaker 3>ever had a dynamo in the past. It does not

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<v Speaker 3>have one today.

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<v Speaker 2>You bring up Venus, and there's a funny thing you

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<v Speaker 2>mentioned toward the end of the book, which is the

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<v Speaker 2>frustrations that Venus presents planetary scientists, especially the ones who

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<v Speaker 2>want to study the interior of the planet. Why is

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<v Speaker 2>Venus so frustrating? Why is it so hard to study?

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<v Speaker 3>Yeah, Venus is the worst planet in the Solar System.

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<v Speaker 3>I'm just going to put that out there right now.

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<v Speaker 3>Here's the issue, right, it's really hard to study the

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<v Speaker 3>insides of planets. You don't have access to it. You

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<v Speaker 3>can't drill down and study the core of a planet

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<v Speaker 3>that way, so you have to develop all these really

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<v Speaker 3>clever methods to try and figure out what's going on

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<v Speaker 3>deep inside the Earth. A lot of methods that are

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<v Speaker 3>kind of like what doctors use to figure out what's

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<v Speaker 3>going on inside the human body. Right, We do scans

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<v Speaker 3>of things, we use gravity, we use magnetic fields, we

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<v Speaker 3>use seismology. So then you try and use any of

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<v Speaker 3>these techniques on Venus, and they don't work for a

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<v Speaker 3>variety of different reasons. So first of all, let's say

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<v Speaker 3>we wanted to use seismology, right, So the waves that

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<v Speaker 3>pass through a planet when you have an earthquake, for example,

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<v Speaker 3>on Earth, the speed of those waves is completely determined

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<v Speaker 3>by the material properties they are passing through. So we

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<v Speaker 3>actually learn a lot about what the materials are inside

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<v Speaker 3>the Earth by looking at how fast these seismic waves

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<v Speaker 3>travel through it. You want to do this on Venus, Sorry,

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<v Speaker 3>the surface is a horrible temperature, and the atmosphere is

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<v Speaker 3>made of sulphuric acid, and the pressure is ninety two

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<v Speaker 3>atmospheric pressures, so it's just the materials are just going

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<v Speaker 3>to melt and dissolve basically, so no chance to do that.

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<v Speaker 3>Then you try and use a magnetic field, right, Having

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<v Speaker 3>a magnetic field is a great way to learn about

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<v Speaker 3>the interior of a planet. As soon as you know

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<v Speaker 3>a planet has a global magnetic field, you know, it's

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<v Speaker 3>got a liquid molten electrical conductor in its interior, and

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<v Speaker 3>it's got those churning motions. Well, Venus doesn't have that,

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<v Speaker 3>so we can't use that. And you try and say, okay, well,

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<v Speaker 3>why don't we just observe the surface and look at

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<v Speaker 3>the rotation of the surface, for example, while Venus has

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<v Speaker 3>this horribly opaque atmosphere that you can't actually look through

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<v Speaker 3>and try to do that. And then one of my

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<v Speaker 3>favorite things about Venus is that when you look at

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<v Speaker 3>all the planets, all the planets, you know we talk

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<v Speaker 3>about planets being spheres, they're not spheres. They're actually kind

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<v Speaker 3>of bulgy oblate spheroids, we call them. So they're fatter

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<v Speaker 3>across the equator than they are at the poles, and

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<v Speaker 3>that bulging of the equator is because of the fact

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<v Speaker 3>that the planet's spin. Now we can use that information

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<v Speaker 3>how bulgey a planet is to actually tell what material

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<v Speaker 3>is inside it, how dense it is inside it. And

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<v Speaker 3>you go and try and do this at Venus, and

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<v Speaker 3>Venus is rotating so slowly that it basically has no bulge.

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<v Speaker 3>So we can't use that either. Basically, Venus is just

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<v Speaker 3>very frustrating doesn't want us to know anything about its interior.

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<v Speaker 2>So there's a great section in the chapter Gazing Outward

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<v Speaker 2>where in this chapter you're talking about the formation of

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<v Speaker 2>our Solar System from the orig original molecular cloud that

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<v Speaker 2>came together to make the Sun and the planets the

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<v Speaker 2>protoplanetary disc. And you talk about how the interesting ways

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<v Speaker 2>the connections between the features of that initial cloud and

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<v Speaker 2>features of the current Solar System and even everyday life

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<v Speaker 2>on Earth. So, for example, the elemental composition of that

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<v Speaker 2>vast cloud determines the elements that make our Solar System,

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<v Speaker 2>but also more interesting and subtle things like how the

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<v Speaker 2>slight initial rotation of that cloud governs so much about

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<v Speaker 2>our world. Could you talk about some of these connections

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<v Speaker 2>between the properties of the cloud and the way the

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<v Speaker 2>Solar System is now?

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<v Speaker 3>Yeah? Absolutely, So. I remember once sitting there and just thinking,

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<v Speaker 3>you know, okay, yeah, we know that the planet's orbit

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<v Speaker 3>around the Sun, we know that the planets are spinning.

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<v Speaker 3>Why is everything spinning all right? Why don't doesn't anything

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<v Speaker 3>just stay still? And the answer has to do with

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<v Speaker 3>this great concept in physics called angular momentum conservation. So basically,

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<v Speaker 3>you can't just change the spin of something without putting

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<v Speaker 3>a lot of torque on it, like forcing it. Right.

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<v Speaker 3>And so then you put something out in the middle

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<v Speaker 3>of nowhere, a molecular cloud, right, and you don't have

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<v Speaker 3>anything really torquing it or anything, and you ask, well,

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<v Speaker 3>how much spin is it going to have? And it's

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<v Speaker 3>going to have some random amount, right, like nothing's perfectly

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<v Speaker 3>isolated and still, so you take all those particles in

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<v Speaker 3>the molecular cloud and you add up all their spins,

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<v Speaker 3>and a lot of them will cancel out. Someone will

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<v Speaker 3>be spinning in one direction, other particles will be spinning

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<v Speaker 3>in the other direction. And you add it all up

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<v Speaker 3>and it almost all cancels out except for a little bit.

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<v Speaker 3>And that little bit in a molecular cloud. Here's the

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<v Speaker 3>amazing thing. Once gravity gets hold of that molecular cloud,

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<v Speaker 3>it starts gravitationally collapsing to eventually form our solar system.

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<v Speaker 3>That amount of spinning just increases and increases and increases

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<v Speaker 3>as the cloud gets smaller and smaller and smaller. And

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<v Speaker 3>you have a total understanding. People have a total understanding

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<v Speaker 3>of this effect. If you've ever watched, for example, figure

0:11:57.480 --> 0:12:00.320
<v Speaker 3>skaters who are about to do a jump with a

0:12:00.320 --> 0:12:02.240
<v Speaker 3>spin it and they pull their arms in. As soon

0:12:02.240 --> 0:12:05.280
<v Speaker 3>as you make something more compact, it spins faster, even

0:12:05.320 --> 0:12:07.320
<v Speaker 3>though you don't do anything to it. And the same

0:12:07.320 --> 0:12:10.320
<v Speaker 3>thing happened to the molecular cloud. As it became smaller

0:12:10.360 --> 0:12:12.640
<v Speaker 3>and smaller and smaller, it spin faster and faster and faster.

0:12:12.679 --> 0:12:15.280
<v Speaker 3>And that's what led to all the spinning we have

0:12:15.800 --> 0:12:18.120
<v Speaker 3>in the Solar System now. And this is true not

0:12:18.200 --> 0:12:20.320
<v Speaker 3>just of our Solar System. We can look out and

0:12:20.360 --> 0:12:23.400
<v Speaker 3>see other Solar systems forming. We can see other planets

0:12:23.440 --> 0:12:26.240
<v Speaker 3>around other stars. They're all spinning too. It's all the

0:12:26.440 --> 0:12:29.080
<v Speaker 3>kind of we share that among all the planets.

0:12:29.520 --> 0:12:33.880
<v Speaker 2>We call the roughly spherical objects that orbit stars planets,

0:12:33.920 --> 0:12:37.120
<v Speaker 2>and we call the objects that orbit planets moons. But

0:12:37.520 --> 0:12:41.480
<v Speaker 2>are there any other material differences between a planet and

0:12:41.520 --> 0:12:43.360
<v Speaker 2>the moon? Are there even any trends?

0:12:44.400 --> 0:12:47.680
<v Speaker 3>Yeah, it's a great question. So moons can be complicated.

0:12:47.720 --> 0:12:50.040
<v Speaker 3>So in reality, if you're someone like me who's interested

0:12:50.080 --> 0:12:53.079
<v Speaker 3>in the interior of planets, you're just as happy to

0:12:53.120 --> 0:12:56.240
<v Speaker 3>consider moon's planets. Right, Moons for their they're made of

0:12:56.360 --> 0:12:59.160
<v Speaker 3>similar stuff. They have the same laws of physics that

0:12:59.200 --> 0:13:02.800
<v Speaker 3>govern their interior. We have moons that have magnetic fields. Ganymede,

0:13:02.800 --> 0:13:04.840
<v Speaker 3>which is a moon of Jupiter, actually has a magnetic

0:13:04.880 --> 0:13:07.640
<v Speaker 3>field generated in its core. So we study the same

0:13:07.679 --> 0:13:12.120
<v Speaker 3>processes on these bodies. Where moons can be a little

0:13:12.120 --> 0:13:16.720
<v Speaker 3>bit different than planets, there's a lot bigger possibility of

0:13:16.760 --> 0:13:19.040
<v Speaker 3>where they came from compared to where they ended up.

0:13:19.320 --> 0:13:24.240
<v Speaker 3>So for example, the rocky planets in the Inner Solar System, Mercury, Venus, Earth, Mars,

0:13:24.640 --> 0:13:27.800
<v Speaker 3>they all pretty much formed close to where they are now.

0:13:28.480 --> 0:13:31.800
<v Speaker 3>Some moons actually come from very far away and then

0:13:31.840 --> 0:13:34.120
<v Speaker 3>get trapped in the gravitational field of a planet and

0:13:34.160 --> 0:13:36.160
<v Speaker 3>then become a moon there. And that happens a lot,

0:13:36.160 --> 0:13:38.600
<v Speaker 3>for example in the Outer Solar System. So if you

0:13:38.679 --> 0:13:41.480
<v Speaker 3>look at Jupiter or Neptune or any of these planets,

0:13:41.480 --> 0:13:43.600
<v Speaker 3>some of their moons are on these really weird orbits.

0:13:43.640 --> 0:13:46.600
<v Speaker 3>They're like orbiting in the opposite direction as the planet

0:13:46.679 --> 0:13:49.480
<v Speaker 3>is spinning. They're not around the equator at all. And

0:13:49.559 --> 0:13:52.800
<v Speaker 3>those moons we think are actually captured basically comets. They're

0:13:53.080 --> 0:13:56.320
<v Speaker 3>captured comets or asteroids that were doing their own thing

0:13:56.679 --> 0:13:59.640
<v Speaker 3>got gravitationally kicked into the Solar System a little bit

0:13:59.679 --> 0:14:02.600
<v Speaker 3>close in and then got trapped around a planet. So

0:14:02.640 --> 0:14:06.000
<v Speaker 3>you can actually find some bodies orbiting these planets that

0:14:06.000 --> 0:14:08.800
<v Speaker 3>were probably formed much further away, and so in that sense,

0:14:08.840 --> 0:14:20.960
<v Speaker 3>that's a little bit different than what you see with planets.

0:14:21.320 --> 0:14:24.520
<v Speaker 2>One of the most shocking facts that you discussed in

0:14:24.560 --> 0:14:28.880
<v Speaker 2>the book concerns the formation of the Earth's moon. Now,

0:14:29.000 --> 0:14:31.600
<v Speaker 2>I know the leading theory on the formation of the

0:14:31.600 --> 0:14:37.240
<v Speaker 2>Earth's moon is the giant impact idea, but specifically, the

0:14:37.320 --> 0:14:41.040
<v Speaker 2>thing that you introduced to me was how rapidly the

0:14:41.080 --> 0:14:44.640
<v Speaker 2>Earth's moon was probably formed according to the leading theory

0:14:44.640 --> 0:14:46.320
<v Speaker 2>of its origin. Could you explain this.

0:14:46.640 --> 0:14:50.120
<v Speaker 3>Yeah, this blows my mind. By the way, so we're

0:14:50.280 --> 0:14:52.400
<v Speaker 3>somewhat I think people have heard of this theory that

0:14:52.520 --> 0:14:57.480
<v Speaker 3>something about the size of Mars, usually called they crashed

0:14:57.520 --> 0:15:00.120
<v Speaker 3>into Earth, had this kind of glancing impact into pro

0:15:00.160 --> 0:15:02.480
<v Speaker 3>to Earth Earth. This was like four point five billion

0:15:02.560 --> 0:15:07.200
<v Speaker 3>years ago, and that crash caused some of that body

0:15:07.240 --> 0:15:10.720
<v Speaker 3>and some of the Earth to get kind of blasted

0:15:10.720 --> 0:15:14.160
<v Speaker 3>off the surface of the planet and small chunks were

0:15:14.160 --> 0:15:16.240
<v Speaker 3>put into orbit. And then you ask the question, Okay,

0:15:16.320 --> 0:15:19.040
<v Speaker 3>so now you have this disk of material surrounding the Earth.

0:15:19.400 --> 0:15:21.360
<v Speaker 3>How long did it take for that disk of material

0:15:21.440 --> 0:15:24.680
<v Speaker 3>to become the Moon a single object? Now, that disk

0:15:24.720 --> 0:15:27.000
<v Speaker 3>of material followed the same laws of physics as the

0:15:27.040 --> 0:15:31.000
<v Speaker 3>planet's forming out of the disc. Initially on gravity caused collisions.

0:15:31.000 --> 0:15:33.720
<v Speaker 3>Some of those collisions caused things to clump together. Eventually,

0:15:33.880 --> 0:15:36.440
<v Speaker 3>the Moon grew and grew and grew, and estimates suggest

0:15:36.480 --> 0:15:39.280
<v Speaker 3>it took forty years for this to happen. Now, when

0:15:39.280 --> 0:15:42.520
<v Speaker 3>you're talking about things in astronomy and in Earth science,

0:15:43.000 --> 0:15:45.960
<v Speaker 3>you're working on millions of years, billions of years. Those

0:15:45.960 --> 0:15:48.360
<v Speaker 3>are the types of lengths of time we're used to.

0:15:48.800 --> 0:15:51.520
<v Speaker 3>So talking about a process that takes forty years is

0:15:51.600 --> 0:15:54.120
<v Speaker 3>just shocking. And so I always have this image in

0:15:54.120 --> 0:15:56.560
<v Speaker 3>my head, and this is obviously impossible because it was

0:15:56.560 --> 0:15:58.240
<v Speaker 3>four point five billion years ago, But I have this

0:15:58.280 --> 0:16:01.440
<v Speaker 3>image in my head of like some parents sitting down

0:16:01.480 --> 0:16:04.240
<v Speaker 3>with their kids and the parents going, you know, when

0:16:04.280 --> 0:16:06.320
<v Speaker 3>I was your age, there was no moon in the

0:16:06.360 --> 0:16:08.840
<v Speaker 3>sky kind of thing, right like that. It's on a

0:16:09.080 --> 0:16:12.480
<v Speaker 3>human generational timescale that this changed.

0:16:13.040 --> 0:16:16.400
<v Speaker 2>That's truly unbelievable. And you actually mentioned several other things

0:16:16.440 --> 0:16:19.200
<v Speaker 2>about the Moon that I didn't quite know about and

0:16:19.280 --> 0:16:22.480
<v Speaker 2>were so interesting one is that it's a parent magnitude

0:16:22.560 --> 0:16:25.960
<v Speaker 2>from the Earth was larger initially, I guess because it

0:16:26.000 --> 0:16:28.640
<v Speaker 2>was closer. But you also mentioned something called a fossil

0:16:28.920 --> 0:16:31.520
<v Speaker 2>bulge in the moon. Could you explain these?

0:16:31.920 --> 0:16:34.280
<v Speaker 3>So when the Moon formed, it was much closer to

0:16:34.320 --> 0:16:38.160
<v Speaker 3>the Earth, and since then it's been slowly receding away

0:16:38.200 --> 0:16:41.440
<v Speaker 3>from the Earth. And we can even measure this change

0:16:41.480 --> 0:16:43.840
<v Speaker 3>in distance of the Moon to the Earth. And that's

0:16:43.880 --> 0:16:47.680
<v Speaker 3>happening because of really interesting gravitational interaction between the Moon

0:16:48.200 --> 0:16:50.520
<v Speaker 3>and the Earth. And it's the same reason, for example,

0:16:50.560 --> 0:16:54.440
<v Speaker 3>that the Moon only shows us one face, so tidal interactions,

0:16:54.480 --> 0:16:57.440
<v Speaker 3>the fact that you know, the Earth's not a perfect sphere,

0:16:57.480 --> 0:16:59.360
<v Speaker 3>the Moon's not a perfect sphere, and they tug on

0:16:59.400 --> 0:17:02.000
<v Speaker 3>each other when are not kind of facing the right way.

0:17:02.760 --> 0:17:07.000
<v Speaker 3>That has caused the Moon to start moving further away.

0:17:07.040 --> 0:17:09.520
<v Speaker 3>It's also caused the Earth to start slowing down its

0:17:09.640 --> 0:17:12.480
<v Speaker 3>rotation a little bit, and so over time, the Moon's

0:17:12.560 --> 0:17:14.320
<v Speaker 3>moving further away and it's going to make it smaller

0:17:14.359 --> 0:17:17.040
<v Speaker 3>and smaller and smaller. And one reason we know all

0:17:17.080 --> 0:17:22.040
<v Speaker 3>of this is that the moon, if you look at

0:17:22.040 --> 0:17:24.080
<v Speaker 3>how bulgy it is, Like I talked about how spinning

0:17:24.119 --> 0:17:27.440
<v Speaker 3>objects have this bulge on them. The Moon is too

0:17:27.520 --> 0:17:30.399
<v Speaker 3>bulgy for how fast it's spinning right now, and the

0:17:30.440 --> 0:17:32.239
<v Speaker 3>only way to explain that is it must have been

0:17:32.280 --> 0:17:35.119
<v Speaker 3>spinning faster in the past. And the only way for

0:17:35.200 --> 0:17:37.159
<v Speaker 3>it to have been spinning faster in the past is

0:17:37.160 --> 0:17:39.439
<v Speaker 3>if it was much closer to the Earth, because we

0:17:39.560 --> 0:17:42.080
<v Speaker 3>know it's locked. It's day is locked to the Earth's

0:17:42.680 --> 0:17:45.200
<v Speaker 3>you know, it's always facing the Earth the same side,

0:17:45.359 --> 0:17:49.000
<v Speaker 3>so it had to have a much faster spin in

0:17:49.080 --> 0:17:50.920
<v Speaker 3>order to get that bulge that it had.

0:17:51.359 --> 0:17:55.639
<v Speaker 2>With exoplanets, we often hear about the habitable zone of

0:17:55.680 --> 0:17:58.600
<v Speaker 2>a star, the area of the distance out from a

0:17:58.640 --> 0:18:01.880
<v Speaker 2>star that we believe there could be the conditions possible

0:18:01.920 --> 0:18:05.440
<v Speaker 2>for life to arise. But an interesting fact you mentioned

0:18:05.600 --> 0:18:09.040
<v Speaker 2>is that if a faraway exoplanet astronomer we're looking at

0:18:09.119 --> 0:18:12.639
<v Speaker 2>our Solar system, they would see not one but three

0:18:12.840 --> 0:18:16.760
<v Speaker 2>planets within our habitable zone, Earth, Venus, and Mars. But

0:18:17.080 --> 0:18:19.080
<v Speaker 2>neither of the other two planets, Mars or Venus are

0:18:19.240 --> 0:18:23.520
<v Speaker 2>especially hospitable now, and Venus is really inhospitable. So what

0:18:23.760 --> 0:18:27.760
<v Speaker 2>does that tell us about looking for exoplanets that could

0:18:27.800 --> 0:18:29.440
<v Speaker 2>sustain life elsewhere?

0:18:29.880 --> 0:18:31.520
<v Speaker 3>I think it tells us that we have to be

0:18:32.560 --> 0:18:36.200
<v Speaker 3>a little more subtle in how we figure out whether

0:18:36.400 --> 0:18:38.800
<v Speaker 3>a planet is a good candidate for some of that

0:18:38.880 --> 0:18:42.520
<v Speaker 3>might have life or not. Right, totally, get why we

0:18:42.560 --> 0:18:45.240
<v Speaker 3>are using these criteria right now. Right, what's the distance

0:18:45.280 --> 0:18:49.119
<v Speaker 3>from a planet star at which the temperatures are just

0:18:49.200 --> 0:18:51.360
<v Speaker 3>right so that water could be liquid on the surface

0:18:51.400 --> 0:18:53.520
<v Speaker 3>if there was water there. That's kind of the condition

0:18:53.560 --> 0:18:58.200
<v Speaker 3>we're using now. But as mentioned, planets are complicated, and

0:18:58.440 --> 0:19:01.239
<v Speaker 3>you could have a planet that comple letly changes its

0:19:01.280 --> 0:19:04.520
<v Speaker 3>surface temperature through a greenhouse, a runaway greenhouse effect. That's

0:19:04.560 --> 0:19:07.560
<v Speaker 3>what happened on Venus. Right, Venus is getting not that

0:19:07.680 --> 0:19:10.520
<v Speaker 3>much more heat from the Sun as we are, but

0:19:10.760 --> 0:19:13.600
<v Speaker 3>it happened to go through this climate process, this runaway

0:19:13.600 --> 0:19:16.040
<v Speaker 3>greenhouse that made the temperture on the surface incredibly hot

0:19:16.080 --> 0:19:19.199
<v Speaker 3>and not able to sustain any water. The water all

0:19:19.240 --> 0:19:22.159
<v Speaker 3>evaporated off of Venus. So we have to be a

0:19:22.200 --> 0:19:24.639
<v Speaker 3>little bit more careful. We need to understand the dynamics

0:19:24.640 --> 0:19:27.640
<v Speaker 3>of what's going on inside the bodies and outside, because

0:19:27.640 --> 0:19:30.960
<v Speaker 3>that's what creates the atmospheres. Another great example of this,

0:19:31.040 --> 0:19:33.240
<v Speaker 3>I think we also need to kind of broaden the

0:19:33.320 --> 0:19:36.960
<v Speaker 3>search for habitable worlds, let's say, because if you look

0:19:37.000 --> 0:19:39.600
<v Speaker 3>in our Solar system, aside from Earth, the next best

0:19:39.640 --> 0:19:42.760
<v Speaker 3>place to possibly look for where life might form are

0:19:42.800 --> 0:19:45.920
<v Speaker 3>actually in the water oceans of some of the moons

0:19:45.920 --> 0:19:48.680
<v Speaker 3>in the outer Solar System. Now, these oceans are buried

0:19:48.960 --> 0:19:52.480
<v Speaker 3>like miles beneath the surface, but they're liquid water, they

0:19:52.480 --> 0:19:57.520
<v Speaker 3>have energy sources, they have complex carbon molecules, all the

0:19:57.600 --> 0:19:59.879
<v Speaker 3>kind of ingredients that we think might be important for life.

0:20:00.040 --> 0:20:03.280
<v Speaker 3>So I think we need to think more carefully about

0:20:03.280 --> 0:20:06.480
<v Speaker 3>what the conditions are for life on exoplanets out there,

0:20:07.440 --> 0:20:10.119
<v Speaker 3>and we might end up finding life in places we

0:20:10.160 --> 0:20:10.920
<v Speaker 3>didn't expect.

0:20:11.720 --> 0:20:15.240
<v Speaker 2>So when trying to understand what's inside planets, we've talked

0:20:15.240 --> 0:20:20.280
<v Speaker 2>about using detection methods for like magnetic fields and seismic

0:20:20.320 --> 0:20:23.720
<v Speaker 2>research and things like that. But what can isolated pieces

0:20:23.760 --> 0:20:28.160
<v Speaker 2>of physical evidence like meteorites and diamonds tell us about

0:20:28.240 --> 0:20:30.440
<v Speaker 2>how planets are formed and what's inside them.

0:20:30.920 --> 0:20:32.920
<v Speaker 3>Yeah, this is one of my favorite things in the world.

0:20:32.960 --> 0:20:35.320
<v Speaker 3>So I'm going to start with the diamonds thing. We

0:20:35.440 --> 0:20:37.760
<v Speaker 3>really would like to actually have samples from deep inside

0:20:37.760 --> 0:20:39.199
<v Speaker 3>the Earth, because that would be the best way to

0:20:39.200 --> 0:20:42.439
<v Speaker 3>study it. It's impossible to do this, we can't drill

0:20:42.600 --> 0:20:45.199
<v Speaker 3>deeper than about eight miles or something like that, right,

0:20:45.280 --> 0:20:49.080
<v Speaker 3>and the earth goes down about almost three thousand miles, right,

0:20:49.160 --> 0:20:52.960
<v Speaker 3>So this is just not possible, luckily for us. Sometimes

0:20:52.960 --> 0:20:55.400
<v Speaker 3>the Earth brings samples from the deep up to the surface,

0:20:55.520 --> 0:20:57.720
<v Speaker 3>and one thing it does is it brings up diamonds.

0:20:57.920 --> 0:21:00.639
<v Speaker 3>Lots of people know about diamonds because they're important in

0:21:00.840 --> 0:21:03.719
<v Speaker 3>say the jewelry industry, things like that, And when you're

0:21:03.760 --> 0:21:05.840
<v Speaker 3>someone who's a jeweler, what you really care about are

0:21:05.880 --> 0:21:08.520
<v Speaker 3>these pure diamonds, the things that are just pure carbon

0:21:08.560 --> 0:21:11.600
<v Speaker 3>and diamond form. When you're a geologist or someone who's

0:21:11.600 --> 0:21:13.560
<v Speaker 3>studying the in tier of the earth, you want the

0:21:13.680 --> 0:21:17.600
<v Speaker 3>impure diamonds. You want the diamonds where some little bit

0:21:17.640 --> 0:21:19.159
<v Speaker 3>of the interior of the Earth got stuck in the

0:21:19.160 --> 0:21:21.399
<v Speaker 3>middle of the diamond as it was forming. And because

0:21:21.400 --> 0:21:25.000
<v Speaker 3>diamonds are so hard, they actually maintain their pressure, and

0:21:25.040 --> 0:21:27.639
<v Speaker 3>so when they come up to the surface, that little

0:21:27.680 --> 0:21:30.240
<v Speaker 3>bit of material from deep inside the Earth actually stays

0:21:30.280 --> 0:21:33.520
<v Speaker 3>preserved in the inside of that diamond. And so we

0:21:33.520 --> 0:21:36.160
<v Speaker 3>can actually study materials how they are in the deep

0:21:36.160 --> 0:21:38.800
<v Speaker 3>interior of the Earth by looking at these inclusions in

0:21:38.840 --> 0:21:41.080
<v Speaker 3>the diamonds when they come to the surface. So that's

0:21:41.080 --> 0:21:45.400
<v Speaker 3>one thing. Now, meteorites are like the best Christmas gift

0:21:45.440 --> 0:21:48.919
<v Speaker 3>anyone could ever get from other planets. Right. Basically, you

0:21:49.040 --> 0:21:51.960
<v Speaker 3>have some sort of collision or something that happened far

0:21:52.040 --> 0:21:54.479
<v Speaker 3>away that caused a piece of a planet or an

0:21:54.520 --> 0:21:57.080
<v Speaker 3>asteroid to get knocked off. Eventually that piece of the

0:21:57.080 --> 0:22:00.120
<v Speaker 3>asteroid came near Earth and some of it landed on

0:22:00.119 --> 0:22:04.560
<v Speaker 3>Earth and we can go and collect it. That's rarely

0:22:04.560 --> 0:22:07.240
<v Speaker 3>where you have samples of the insides of other planets,

0:22:07.240 --> 0:22:10.080
<v Speaker 3>and we even have meteorites that are very iron rich

0:22:10.160 --> 0:22:14.800
<v Speaker 3>that come from the cores of previous planetary asteroid like

0:22:14.880 --> 0:22:18.280
<v Speaker 3>bodies that got broken up. So one of the best

0:22:18.280 --> 0:22:20.800
<v Speaker 3>pieces of evidence we have for what's in our core

0:22:21.040 --> 0:22:23.120
<v Speaker 3>is actually looking at the cores of other bodies. They're

0:22:23.119 --> 0:22:27.000
<v Speaker 3>all very similar. They all have this iron rich cores

0:22:27.040 --> 0:22:29.480
<v Speaker 3>that eventually come to Earth and we get to study them.

0:22:30.080 --> 0:22:32.960
<v Speaker 2>This reminds me there's an object that you mentioned several

0:22:33.000 --> 0:22:35.120
<v Speaker 2>times in the book that I feel like I can

0:22:35.160 --> 0:22:38.760
<v Speaker 2>tell you are especially excited about, and it is the

0:22:39.440 --> 0:22:43.960
<v Speaker 2>asteroid sixteen Psyche. What makes Psyche so exciting?

0:22:44.400 --> 0:22:46.399
<v Speaker 3>So, first of all, there is a mission on its

0:22:46.440 --> 0:22:48.199
<v Speaker 3>way to Psyche right now, So we are going to

0:22:48.200 --> 0:22:50.600
<v Speaker 3>study this asteroid up close and personal, and I'm very

0:22:50.640 --> 0:22:53.239
<v Speaker 3>excited about that. I think in our Solar System, we're

0:22:53.320 --> 0:22:55.320
<v Speaker 3>used to different kinds of worlds. Right You've got the

0:22:55.400 --> 0:22:58.320
<v Speaker 3>rocky worlds of the inner planets in the Solar System,

0:22:58.520 --> 0:23:00.719
<v Speaker 3>You've got the gas giants like that Are and Saturn.

0:23:00.880 --> 0:23:03.320
<v Speaker 3>You've got the water worlds like you're in a a Neptune,

0:23:03.320 --> 0:23:05.160
<v Speaker 3>and even some of the moons we can consider water

0:23:05.200 --> 0:23:09.679
<v Speaker 3>World's Europa Enceladus moons like that. Sixteen. Psyche is a

0:23:09.720 --> 0:23:13.400
<v Speaker 3>metal world. So this is a body that is mostly

0:23:13.440 --> 0:23:16.920
<v Speaker 3>made of iron. It's mostly metal, and we just haven't

0:23:16.960 --> 0:23:20.400
<v Speaker 3>seen that before. And I'm really excited about what it's

0:23:20.440 --> 0:23:22.920
<v Speaker 3>going to be like to go look at this thing

0:23:23.040 --> 0:23:25.439
<v Speaker 3>and you know, answer questions like, hmm, what does a

0:23:25.440 --> 0:23:28.320
<v Speaker 3>crater look like on a body that's mostly made of metal? Is?

0:23:28.359 --> 0:23:30.320
<v Speaker 3>What does a volcano look like on this thing? Does

0:23:30.320 --> 0:23:32.919
<v Speaker 3>it have a magnetic field? What's really going on on

0:23:32.960 --> 0:23:35.600
<v Speaker 3>the surface. So it's very exciting. It's a new type

0:23:35.600 --> 0:23:38.280
<v Speaker 3>of planetary body that we've never gotten to see up

0:23:38.280 --> 0:23:39.080
<v Speaker 3>close and personal.

0:23:40.359 --> 0:23:43.120
<v Speaker 2>I think you mentioned the idea of a metal volcano.

0:23:44.440 --> 0:23:47.040
<v Speaker 2>That's a real thing. What does that mean?

0:23:47.480 --> 0:23:49.720
<v Speaker 3>We're going to find out, But imagine this is you know,

0:23:49.800 --> 0:23:52.880
<v Speaker 3>this is an asteroid that's big enough that it could

0:23:52.880 --> 0:23:54.919
<v Speaker 3>have stuff going on in the interior. You could have

0:23:55.240 --> 0:23:58.200
<v Speaker 3>some of them iron from the interior being liquid and

0:23:58.600 --> 0:24:02.480
<v Speaker 3>getting kind of taken up out of the interior onto

0:24:02.520 --> 0:24:05.960
<v Speaker 3>the surface at these volcanic vents. So, yeah, we might

0:24:06.080 --> 0:24:08.399
<v Speaker 3>get to see a metal volcano up close.

0:24:09.560 --> 0:24:12.800
<v Speaker 2>Coming back to looking inside planets, if you go beyond

0:24:12.880 --> 0:24:15.679
<v Speaker 2>Earth and even beyond the rocky planets, one of the

0:24:15.680 --> 0:24:20.240
<v Speaker 2>most fascinating questions to ponder is what's inside the gas

0:24:20.280 --> 0:24:24.800
<v Speaker 2>planets and the ice giants. I suspect you've seen the

0:24:24.840 --> 0:24:27.600
<v Speaker 2>many variations on the article or video. What is it

0:24:27.720 --> 0:24:30.720
<v Speaker 2>like to fall into Jupiter or something like that. It's

0:24:30.760 --> 0:24:34.040
<v Speaker 2>clearly a captivating question because we see these outer cloud

0:24:34.080 --> 0:24:37.760
<v Speaker 2>layers and there's just this you question, like, obviously, you

0:24:37.840 --> 0:24:40.639
<v Speaker 2>imagine you're denser than some outer part of that cloud

0:24:40.720 --> 0:24:42.879
<v Speaker 2>layer and you could sync down into it, and you've

0:24:42.920 --> 0:24:45.919
<v Speaker 2>got to wonder what's inside. So what do we know

0:24:45.960 --> 0:24:49.760
<v Speaker 2>about what is inside the gas giants and the ice giants?

0:24:50.160 --> 0:24:52.280
<v Speaker 3>Yeah, this is one of my favorite things to talk about.

0:24:52.400 --> 0:24:55.960
<v Speaker 3>So we are so accustomed to how materials behave in

0:24:56.000 --> 0:24:57.800
<v Speaker 3>the types of conditions we have here on the surface

0:24:57.840 --> 0:24:59.800
<v Speaker 3>of the Earth. If I just say the word water,

0:25:00.200 --> 0:25:02.639
<v Speaker 3>you have a natural instinctive reaction to what water is.

0:25:02.680 --> 0:25:04.960
<v Speaker 3>It's either that liquid in my glass, or maybe it's

0:25:04.960 --> 0:25:08.400
<v Speaker 3>frozen on some ice somewhere, or it's water vapor that's

0:25:08.400 --> 0:25:12.240
<v Speaker 3>causing fog. Right, you put water under the high pressures

0:25:12.280 --> 0:25:14.240
<v Speaker 3>and high temperatures that are deep inside planets, it's a

0:25:14.280 --> 0:25:17.159
<v Speaker 3>completely different beast. Same thing is true for hydrogen. So

0:25:17.240 --> 0:25:19.840
<v Speaker 3>let's start there. Hydrogen the most kind of the simplest

0:25:19.880 --> 0:25:22.560
<v Speaker 3>element we have, thing that we're used to being in

0:25:22.640 --> 0:25:26.119
<v Speaker 3>gaseous form. Now in Jupiter and in Saturn. As you

0:25:26.240 --> 0:25:29.959
<v Speaker 3>keep descending into the planet, temperatures are rising, you get

0:25:30.000 --> 0:25:32.720
<v Speaker 3>to millions of degrees, you can get to millions of

0:25:32.760 --> 0:25:36.440
<v Speaker 3>atmospheres of pressure. Hydrogen is a very different material under

0:25:36.440 --> 0:25:39.160
<v Speaker 3>that pressure, and in fact, is you squeeze a hydrogen molecule,

0:25:39.440 --> 0:25:42.159
<v Speaker 3>you basically allow So imagine hydrogen molecule. You got a

0:25:42.200 --> 0:25:44.440
<v Speaker 3>proton at the center and the nucleus, and you got

0:25:44.440 --> 0:25:47.359
<v Speaker 3>this electron floating around. You squeeze enough of those close

0:25:47.400 --> 0:25:51.040
<v Speaker 3>together the electrons essentially get freed from the protons and

0:25:51.040 --> 0:25:53.159
<v Speaker 3>you create what's called what we call a metal. So

0:25:53.200 --> 0:25:57.120
<v Speaker 3>you can actually have metallic hydrogen going on inside Jupiter

0:25:57.200 --> 0:26:00.560
<v Speaker 3>and Saturn, and it's a great electrical Conductor's actually where

0:26:00.640 --> 0:26:03.840
<v Speaker 3>Jupiter creates its magnetic field, same with Saturn. So that's

0:26:03.920 --> 0:26:06.760
<v Speaker 3>kind of a material we're not expected. Interestingly, helium take

0:26:06.800 --> 0:26:11.080
<v Speaker 3>another one, the second most simple element we have, helium.

0:26:11.760 --> 0:26:14.440
<v Speaker 3>You do the same thing. The helium. Turns out that

0:26:14.520 --> 0:26:17.400
<v Speaker 3>in the outer layers of Jupiter and Saturn in the atmosphere,

0:26:17.440 --> 0:26:20.080
<v Speaker 3>helium and hydrogen are nicely mixed. Right. It's kind of

0:26:20.160 --> 0:26:22.840
<v Speaker 3>like if you put salt in water or sugar in

0:26:22.880 --> 0:26:25.320
<v Speaker 3>water warm water and you stir it. They're nicely mixed.

0:26:25.320 --> 0:26:27.520
<v Speaker 3>You can't kind of separate them, but you put them

0:26:27.600 --> 0:26:31.320
<v Speaker 3>under high enough pressure. When this hydrogen becomes a nice metal,

0:26:31.600 --> 0:26:33.600
<v Speaker 3>the helium no longer wants to stay mixed in it,

0:26:33.840 --> 0:26:37.359
<v Speaker 3>and so helium will actually kind of exolt out of

0:26:37.359 --> 0:26:40.119
<v Speaker 3>the hydrogen and become these droplets, and then helium's heavier

0:26:40.119 --> 0:26:44.240
<v Speaker 3>than hydrogen, so they drop out. It rains helium inside

0:26:44.320 --> 0:26:46.879
<v Speaker 3>Jupiter and Saturn. So I think that's really cool. Then

0:26:46.920 --> 0:26:48.520
<v Speaker 3>you get to the ice giants, where you have a

0:26:48.520 --> 0:26:53.600
<v Speaker 3>lot more complicated molecules methane, ammonia, and you say, okay,

0:26:53.680 --> 0:26:56.000
<v Speaker 3>what happens to those things under high pressure, and you

0:26:56.040 --> 0:27:00.440
<v Speaker 3>can get things, for example, like super ionic water that's

0:27:00.440 --> 0:27:03.960
<v Speaker 3>actually formed in where all the oxygen atoms form a

0:27:04.000 --> 0:27:06.920
<v Speaker 3>nice lattice and all the hydrogen the protons that would

0:27:06.960 --> 0:27:09.240
<v Speaker 3>make up water in the H two O flow freely

0:27:09.320 --> 0:27:11.240
<v Speaker 3>between it, something we've never seen on the surface of

0:27:11.280 --> 0:27:15.600
<v Speaker 3>the Earth. And you can even make a diamond ocean

0:27:15.720 --> 0:27:19.360
<v Speaker 3>deep inside Neptune and Uranus. It's been hypothesized that the

0:27:19.400 --> 0:27:23.560
<v Speaker 3>carbon in things like carbon dioxide and methane ends up

0:27:23.920 --> 0:27:26.200
<v Speaker 3>in the diamond phase deep inside, but then it melts,

0:27:26.200 --> 0:27:29.320
<v Speaker 3>so you actually get a liquid diamond ocean. Diamond actually

0:27:29.359 --> 0:27:31.560
<v Speaker 3>has this really cool property that water on the surface

0:27:31.560 --> 0:27:34.040
<v Speaker 3>of the Earth also has, and that's right near that

0:27:34.080 --> 0:27:38.600
<v Speaker 3>freezing point. The solid phase is slightly less dense than

0:27:38.640 --> 0:27:40.439
<v Speaker 3>the liquid phase, which is why we have, for example,

0:27:40.480 --> 0:27:45.080
<v Speaker 3>icebergs that can float on water. Here. The same is

0:27:45.119 --> 0:27:48.920
<v Speaker 3>true deep inside Uranus and Neptune. Diamond bergs would actually

0:27:48.960 --> 0:27:52.320
<v Speaker 3>float on a diamond seed deep inside Uranus and Neptune.

0:27:52.359 --> 0:27:55.720
<v Speaker 3>So these are just material behavior that we just have

0:27:55.880 --> 0:27:57.600
<v Speaker 3>no experience with here on the surface of the Earth,

0:27:57.600 --> 0:27:58.680
<v Speaker 3>and I love thinking about it.

0:27:59.119 --> 0:28:03.320
<v Speaker 2>Yeah, simultaneously wonderful and frustrating that it violates our intuition,

0:28:03.440 --> 0:28:05.960
<v Speaker 2>so you can't really picture it. You want to be

0:28:06.000 --> 0:28:09.840
<v Speaker 2>able to, but you can't with the idea of superheated

0:28:09.840 --> 0:28:12.119
<v Speaker 2>ices and things like that. But it reminds me of

0:28:12.200 --> 0:28:15.119
<v Speaker 2>actually things closer to home. You talk about other ways

0:28:15.119 --> 0:28:19.159
<v Speaker 2>that even the interior of the Earth also violates our

0:28:19.200 --> 0:28:24.120
<v Speaker 2>intuitions about how materials work. For example, I think there's

0:28:24.160 --> 0:28:25.680
<v Speaker 2>a part in the book where you talk about how

0:28:26.600 --> 0:28:30.800
<v Speaker 2>it's hard for people to understand sometimes that parts of

0:28:30.840 --> 0:28:34.720
<v Speaker 2>the mantle migrate up and down even though the mantle

0:28:34.920 --> 0:28:37.360
<v Speaker 2>is solid not liquid. Is that right?

0:28:37.920 --> 0:28:41.320
<v Speaker 3>That's absolutely right. So I think there's also a big

0:28:41.360 --> 0:28:44.400
<v Speaker 3>misunderstanding out there that you think because you see at volcanos,

0:28:44.440 --> 0:28:46.880
<v Speaker 3>you see this magma coming up being all liquid, you

0:28:46.920 --> 0:28:49.160
<v Speaker 3>think that means that the interior of the earth, the mantle,

0:28:49.560 --> 0:28:52.400
<v Speaker 3>is all liquid, And that's absolutely not true. The rock

0:28:52.560 --> 0:28:56.040
<v Speaker 3>inside the mantle of the Earth is solid, it's very solid.

0:28:56.680 --> 0:28:59.920
<v Speaker 3>That doesn't mean it can't flow. So we do see

0:29:00.440 --> 0:29:05.200
<v Speaker 3>that rock move around, it moves on really slow timescales,

0:29:05.240 --> 0:29:07.440
<v Speaker 3>so it can take hundreds of millions of years for

0:29:07.480 --> 0:29:09.920
<v Speaker 3>a rock to make it from say the core mantle boundary,

0:29:10.000 --> 0:29:12.440
<v Speaker 3>up to the surface of the Earth. But it does flow,

0:29:12.480 --> 0:29:14.600
<v Speaker 3>it does move around, and the only reason we see

0:29:14.960 --> 0:29:17.960
<v Speaker 3>it in its liquid state at the surface is because

0:29:18.160 --> 0:29:21.240
<v Speaker 3>it was under a lot of pressure deep inside the Earth.

0:29:21.280 --> 0:29:23.959
<v Speaker 3>Pressures increase incredibly as you go down, and so that

0:29:24.320 --> 0:29:26.760
<v Speaker 3>it was basically pressure frozen. It was basically made a

0:29:26.880 --> 0:29:29.160
<v Speaker 3>solid because of the high pressure, and then you bring

0:29:29.200 --> 0:29:31.200
<v Speaker 3>that up to the surface and you release the pressure

0:29:31.400 --> 0:29:34.320
<v Speaker 3>and everything kind of expands out and becomes the magma

0:29:34.400 --> 0:29:35.600
<v Speaker 3>the liquid that you see.

0:29:35.760 --> 0:29:39.840
<v Speaker 2>There is a strange feature Towards the end of your book.

0:29:39.840 --> 0:29:41.800
<v Speaker 2>There's a great section where you just sort of like

0:29:42.360 --> 0:29:47.880
<v Speaker 2>explore all of the different strange aspects of planets, especially

0:29:47.920 --> 0:29:50.520
<v Speaker 2>like the ice giants and the gas giants. So you

0:29:50.560 --> 0:29:53.160
<v Speaker 2>talk about the helium ray and the diamond rain. You

0:29:53.200 --> 0:29:57.840
<v Speaker 2>also talk about why Uranus and Neptune have strange multi

0:29:57.880 --> 0:30:01.160
<v Speaker 2>polar magnetic fields. Does does that mean? Where does that

0:30:01.200 --> 0:30:01.760
<v Speaker 2>come from?

0:30:02.240 --> 0:30:04.360
<v Speaker 3>Imagine back to when we only really knew about the

0:30:04.360 --> 0:30:07.800
<v Speaker 3>Earth's magnetic field, right, and Earth's magnetic field the most

0:30:07.800 --> 0:30:11.280
<v Speaker 3>common feature about it is it looks like a die pole.

0:30:11.320 --> 0:30:13.600
<v Speaker 3>So there's a north pole and there's a south pole,

0:30:13.920 --> 0:30:17.120
<v Speaker 3>and the magnetic field lines connect them. When we started

0:30:17.160 --> 0:30:20.280
<v Speaker 3>exploring other planetary bodies, we started to see this happen

0:30:20.320 --> 0:30:24.920
<v Speaker 3>a lot. So Jupiter and Saturn also very dipolar. Mercury dipolar.

0:30:25.720 --> 0:30:28.400
<v Speaker 3>When the Voyager two mission, which was the only mission

0:30:28.440 --> 0:30:30.000
<v Speaker 3>that we have that has gone out to Uranus and

0:30:30.080 --> 0:30:32.840
<v Speaker 3>Neptune and basically just flew by for a little while,

0:30:33.280 --> 0:30:36.640
<v Speaker 3>when it got to first Urinus, which is closer, it

0:30:36.680 --> 0:30:39.560
<v Speaker 3>didn't see a dipolar field. It saw this multipolar fields.

0:30:39.600 --> 0:30:41.200
<v Speaker 3>There were a bunch of North poles and a bunch

0:30:41.240 --> 0:30:43.920
<v Speaker 3>of South poles all over the planet. I remember reading

0:30:43.960 --> 0:30:46.800
<v Speaker 3>about some of this history of when this happened in

0:30:46.800 --> 0:30:49.680
<v Speaker 3>the eighties, and people, you know, weren't expecting that. So

0:30:49.720 --> 0:30:51.680
<v Speaker 3>the first question you have is, all, well, maybe maybe

0:30:51.800 --> 0:30:55.040
<v Speaker 3>something broke, maybe the magnetometer is not working properly or

0:30:55.080 --> 0:30:56.680
<v Speaker 3>something like that, and they did lots of tests and

0:30:56.680 --> 0:30:58.640
<v Speaker 3>they make sure that wasn't the case. Then you get

0:30:58.640 --> 0:31:01.800
<v Speaker 3>out to Neptune and it's also this multipolar field, and

0:31:01.840 --> 0:31:03.960
<v Speaker 3>so you got to say, hmm, well, were we just

0:31:04.080 --> 0:31:06.680
<v Speaker 3>wrong about the fact that magnetic fields are supposed to

0:31:06.680 --> 0:31:11.040
<v Speaker 3>be dipolar, and the fact that Uranus and Neptune happen

0:31:11.120 --> 0:31:14.240
<v Speaker 3>to be the only water rich planets in the Solar System,

0:31:14.240 --> 0:31:17.120
<v Speaker 3>these ice giants, and they happen to be the only

0:31:17.120 --> 0:31:19.120
<v Speaker 3>ones with multipolar fields, then you got to start saying,

0:31:19.160 --> 0:31:22.320
<v Speaker 3>maybe there's a causal relationship with there, right, So I've

0:31:22.360 --> 0:31:24.160
<v Speaker 3>spent a lot of time thinking about that and trying

0:31:24.160 --> 0:31:26.720
<v Speaker 3>to think about how you create multipolar fields in an

0:31:26.760 --> 0:31:28.920
<v Speaker 3>ice giant, And it turns out that there are some

0:31:28.960 --> 0:31:31.560
<v Speaker 3>features in an ice giant that might make multipolar fields

0:31:31.600 --> 0:31:34.680
<v Speaker 3>more likely to occur. Turns out that the dynamo region

0:31:34.880 --> 0:31:37.280
<v Speaker 3>can be really thin in these bodies, so you just

0:31:37.320 --> 0:31:40.360
<v Speaker 3>have this really thin shell where the conditions are just

0:31:40.480 --> 0:31:44.479
<v Speaker 3>right for convection to occur in a good electrical conductor

0:31:44.480 --> 0:31:47.040
<v Speaker 3>and create a magnetic field. When you have this really

0:31:47.080 --> 0:31:51.760
<v Speaker 3>thin shell, you can't make big global dipolar fields. Nothing's

0:31:51.800 --> 0:31:54.280
<v Speaker 3>communicating the right way. All the length skills are too small.

0:31:54.440 --> 0:31:57.120
<v Speaker 3>So maybe you get more multipolar fields that way. People

0:31:57.120 --> 0:31:59.960
<v Speaker 3>are still studying this that we're really looking forward to

0:32:00.160 --> 0:32:03.520
<v Speaker 3>new mission, hopefully to Uranus sometime in the next decade,

0:32:04.080 --> 0:32:06.000
<v Speaker 3>so that we can study the magnetic field up close

0:32:06.000 --> 0:32:07.479
<v Speaker 3>and the interior of the planet, so that we can

0:32:07.560 --> 0:32:08.400
<v Speaker 3>understand the connection.

0:32:09.040 --> 0:32:12.080
<v Speaker 2>We have a basic idea of the types of planets

0:32:12.080 --> 0:32:15.040
<v Speaker 2>that can exist from our own Solar system. We have,

0:32:15.080 --> 0:32:17.400
<v Speaker 2>you know, the inner rocky planets. We have the gas giants,

0:32:17.440 --> 0:32:19.160
<v Speaker 2>we have the ice giants, and then we have these

0:32:19.200 --> 0:32:22.840
<v Speaker 2>other planets that we're familiar with from looking at other stars,

0:32:23.240 --> 0:32:26.080
<v Speaker 2>like the hot Jupiters and the super earths and so forth.

0:32:26.640 --> 0:32:29.400
<v Speaker 2>But there is a new planet type that you introduced

0:32:29.400 --> 0:32:31.720
<v Speaker 2>me to in this book. I don't think i'd ever

0:32:31.760 --> 0:32:35.840
<v Speaker 2>heard of it before, the hypothetical carbon planet. That sounds

0:32:35.920 --> 0:32:37.920
<v Speaker 2>so strange. What is the deal with this?

0:32:38.720 --> 0:32:41.680
<v Speaker 3>Yeah, you know, it's interesting when you look in our

0:32:41.680 --> 0:32:43.920
<v Speaker 3>Solar system, and let's say you look at the rocks

0:32:44.000 --> 0:32:48.000
<v Speaker 3>inside the Earth. They're mostly made of what we call silicates,

0:32:48.160 --> 0:32:52.680
<v Speaker 3>so they have silicon and oxygen atoms combined together, magnesium silicates,

0:32:52.720 --> 0:32:55.680
<v Speaker 3>aluminum silicates. This is kind of what defines the chemistry

0:32:55.720 --> 0:32:58.080
<v Speaker 3>of the rocks on the Earth, and all of that

0:32:58.240 --> 0:33:01.280
<v Speaker 3>was determined by the ratio of carbon to oxygen to

0:33:01.360 --> 0:33:06.360
<v Speaker 3>magnesium in the protoplanetary disk that formed and eventually became

0:33:06.400 --> 0:33:08.640
<v Speaker 3>all the materials we have. Now, if you go to

0:33:08.680 --> 0:33:12.800
<v Speaker 3>some other solar systems out there, they might have slightly

0:33:12.840 --> 0:33:18.880
<v Speaker 3>different ratios. And if nebula out there that eventually forms

0:33:18.880 --> 0:33:20.720
<v Speaker 3>a star with planets around it happened to have a

0:33:20.760 --> 0:33:23.920
<v Speaker 3>little bit more carbon, then the types of rocks that

0:33:23.960 --> 0:33:25.600
<v Speaker 3>you form, the types of minerals that you form, can

0:33:25.600 --> 0:33:28.040
<v Speaker 3>be very different, and you can actually create planets that

0:33:28.080 --> 0:33:30.520
<v Speaker 3>are mostly made of carbon, that have a much higher

0:33:30.560 --> 0:33:32.720
<v Speaker 3>carbon content than what we have here on Earth. It's

0:33:32.760 --> 0:33:36.920
<v Speaker 3>a geologist kind of like dreamscape to think about, what

0:33:37.040 --> 0:33:39.280
<v Speaker 3>if the chemistry was just slightly different because there's just

0:33:39.320 --> 0:33:42.640
<v Speaker 3>a little bit more of some tiny sub element. Right, Remember,

0:33:42.680 --> 0:33:45.680
<v Speaker 3>our solar system was mostly hydrogen and helium, and it

0:33:45.720 --> 0:33:48.200
<v Speaker 3>was just little bits of these rocks that eventually became

0:33:48.800 --> 0:33:52.840
<v Speaker 3>the Earth. And now you just slightly tweak the ratio

0:33:52.920 --> 0:33:56.240
<v Speaker 3>of those elements in extrasolar planets and you could create

0:33:56.240 --> 0:33:57.280
<v Speaker 3>completely different worlds.

0:33:57.920 --> 0:34:02.920
<v Speaker 2>Last question. You already mentioned why the upcoming study of

0:34:03.040 --> 0:34:05.800
<v Speaker 2>asteroid sixteen Psyche is going to be so exciting, but

0:34:06.000 --> 0:34:08.759
<v Speaker 2>what are some of the other upcoming missions and experiments

0:34:09.239 --> 0:34:11.560
<v Speaker 2>that you think are likely to teach us the most

0:34:11.600 --> 0:34:14.359
<v Speaker 2>about planetary science. What are you most excited to learn

0:34:14.400 --> 0:34:15.200
<v Speaker 2>in the near future.

0:34:15.719 --> 0:34:17.799
<v Speaker 3>Okay, there are two missions that I'm most excited about,

0:34:17.800 --> 0:34:19.520
<v Speaker 3>and I actually have nothing to do with these missions,

0:34:19.520 --> 0:34:22.359
<v Speaker 3>so I'm just a super fan of these missions. The

0:34:22.400 --> 0:34:25.480
<v Speaker 3>first one is the Europa Clipper mission, which is going

0:34:25.480 --> 0:34:28.200
<v Speaker 3>to go to a moon of Jupiter named Europa, scheduled

0:34:28.239 --> 0:34:32.919
<v Speaker 3>launch next year. And Europa is an exciting place because

0:34:32.960 --> 0:34:35.719
<v Speaker 3>it's this icy moon of Jupiter and we know that

0:34:35.760 --> 0:34:38.840
<v Speaker 3>it has a liquid water ocean buried beneath the surface,

0:34:39.400 --> 0:34:41.719
<v Speaker 3>and we think it has all the ingredients you might

0:34:41.719 --> 0:34:44.640
<v Speaker 3>think of as necessary for life. So the plan is

0:34:44.680 --> 0:34:47.959
<v Speaker 3>to go there and see try to get a sense

0:34:48.000 --> 0:34:50.480
<v Speaker 3>of what that ocean is made of. Are there complex

0:34:50.520 --> 0:34:52.680
<v Speaker 3>molecules in there that are kind of what we would

0:34:52.719 --> 0:34:54.840
<v Speaker 3>consider the building blocks of life, things like that. So

0:34:54.880 --> 0:34:57.879
<v Speaker 3>that's one really exciting. The other one is actually another moon.

0:34:58.960 --> 0:35:02.479
<v Speaker 3>There's a mission called Drag and Fly, which is scheduled. Yeah,

0:35:02.480 --> 0:35:03.719
<v Speaker 3>you know it's going to be a good mission when

0:35:03.719 --> 0:35:06.480
<v Speaker 3>it has a cool name, right, So Dragonfly is scheduled

0:35:06.520 --> 0:35:10.280
<v Speaker 3>to go to Saturn's moon Titan. Now Titan, in my opinion,

0:35:10.400 --> 0:35:12.960
<v Speaker 3>is probably one of the coolest places in the Solar

0:35:12.960 --> 0:35:17.720
<v Speaker 3>System to think about. It's the only other planetary body

0:35:17.760 --> 0:35:22.319
<v Speaker 3>out there to have nitrogen as its main based thick atmosphere.

0:35:22.360 --> 0:35:24.160
<v Speaker 3>So the Earth is the other planet, right, so it

0:35:24.160 --> 0:35:26.680
<v Speaker 3>has some similarities to it. It's the only other body

0:35:26.719 --> 0:35:29.280
<v Speaker 3>out there that we have seen liquids running on the surface.

0:35:29.520 --> 0:35:31.560
<v Speaker 3>So just like on Earth we have rivers and seas

0:35:31.600 --> 0:35:34.160
<v Speaker 3>and oceans, Titan has rivers and seas and oceans on

0:35:34.200 --> 0:35:37.560
<v Speaker 3>the surface. Now there's a catch, they're not water. Those

0:35:37.640 --> 0:35:39.640
<v Speaker 3>rivers and season oceans are actually made of things like

0:35:39.760 --> 0:35:43.440
<v Speaker 3>methane and ethane, so not you know, fun places. But

0:35:43.520 --> 0:35:47.720
<v Speaker 3>Titan has this thick atmosphere and it's also incredibly small,

0:35:47.920 --> 0:35:50.760
<v Speaker 3>so it has a really low gravity. So my favorite

0:35:50.760 --> 0:35:53.560
<v Speaker 3>fact about Titan is that it's really easy to fly there.

0:35:54.000 --> 0:35:58.040
<v Speaker 3>So you could strap some cardboard on your arms and

0:35:58.120 --> 0:36:01.359
<v Speaker 3>flap them on the surface of Titan could fly right.

0:36:01.400 --> 0:36:03.880
<v Speaker 3>So this is amazing. So the Dragonfly mission has decided

0:36:03.920 --> 0:36:07.480
<v Speaker 3>to take advantage of it. So it's sending essentially an octacopper,

0:36:07.600 --> 0:36:09.800
<v Speaker 3>so it's two quad copters, so think of a helicopter,

0:36:09.840 --> 0:36:13.120
<v Speaker 3>but with eight different blade things. It's sending this thing

0:36:13.160 --> 0:36:15.520
<v Speaker 3>out there. It's going to be able to land on

0:36:15.560 --> 0:36:18.200
<v Speaker 3>the surface, do a bunch of science and then take

0:36:18.239 --> 0:36:20.759
<v Speaker 3>off again, look around, figure out where it wants to

0:36:20.760 --> 0:36:23.520
<v Speaker 3>go next, travel quite long distances, and then land again

0:36:23.560 --> 0:36:24.920
<v Speaker 3>and do more science. So this is going to be

0:36:24.920 --> 0:36:29.719
<v Speaker 3>the first time we're able to study this world very locally, right,

0:36:29.840 --> 0:36:32.560
<v Speaker 3>like touch it, and also fly around to very different

0:36:32.600 --> 0:36:35.319
<v Speaker 3>parts of it. And Titans exciting because it has all

0:36:35.360 --> 0:36:37.360
<v Speaker 3>the building blocks of life. We know there's a liquid

0:36:37.360 --> 0:36:40.799
<v Speaker 3>water ocean underneath. We know it has complex chemicals, those

0:36:40.840 --> 0:36:44.200
<v Speaker 3>hydrocarbons like methane and ethane. We know it has energy sources.

0:36:44.280 --> 0:36:46.960
<v Speaker 3>So we really want to understand a lot of the

0:36:47.000 --> 0:36:49.279
<v Speaker 3>processes that we think are important in the creation of

0:36:49.320 --> 0:36:51.719
<v Speaker 3>life are going to be happening on Titan, and we're

0:36:51.760 --> 0:36:53.040
<v Speaker 3>excited to study them up close.

0:36:53.560 --> 0:36:56.520
<v Speaker 2>Doctor Sabine Stanley, thank you so much for joining us today.

0:36:56.520 --> 0:36:57.880
<v Speaker 2>It's been a real pleasure to talk.

0:36:58.320 --> 0:36:58.799
<v Speaker 3>Thanks so much.

0:36:58.880 --> 0:37:03.880
<v Speaker 2>This was fun, all right. If you would like to

0:37:03.960 --> 0:37:06.800
<v Speaker 2>check out the book for yourself again, it is called

0:37:07.040 --> 0:37:11.960
<v Speaker 2>What's Hidden Inside Planets from twenty twenty three, available in

0:37:12.000 --> 0:37:15.280
<v Speaker 2>audiobook form as well if that's your medium of choice.

0:37:16.440 --> 0:37:18.880
<v Speaker 2>Quick note about our show if you are new to it.

0:37:18.880 --> 0:37:21.440
<v Speaker 2>Stuff to Blow your Mind is a science and culture

0:37:21.480 --> 0:37:26.560
<v Speaker 2>podcast with core episodes on Tuesdays and Thursdays of every week.

0:37:26.680 --> 0:37:29.680
<v Speaker 2>Usually I'm joined by my co host, Robert Lamb. He's

0:37:29.680 --> 0:37:32.399
<v Speaker 2>out on vacation this week, but he will be back

0:37:32.440 --> 0:37:35.879
<v Speaker 2>again soon, let's see. Mondays of each week we read

0:37:35.920 --> 0:37:39.280
<v Speaker 2>back messages from the Stuff to Blow your Mind email address,

0:37:39.320 --> 0:37:42.200
<v Speaker 2>which I'll give out in just a moment. On Wednesdays

0:37:42.200 --> 0:37:45.799
<v Speaker 2>of each week, we feature a short form scripted podcast

0:37:45.880 --> 0:37:50.080
<v Speaker 2>called The Artifact or the Monster Fact or even There

0:37:50.080 --> 0:37:53.600
<v Speaker 2>are some new types of facts coming online. You'll learn

0:37:53.640 --> 0:37:58.080
<v Speaker 2>about them soon. Also, we have a show that airs

0:37:58.120 --> 0:38:01.080
<v Speaker 2>every Friday that is a movie. This is sort of

0:38:01.120 --> 0:38:04.800
<v Speaker 2>a more informal thing that Rob and I do every Friday.

0:38:04.840 --> 0:38:07.640
<v Speaker 2>It is called Weird House Cinema, where we just watch

0:38:07.960 --> 0:38:12.839
<v Speaker 2>and discuss strange films, good or bad, well known or obscure.

0:38:12.880 --> 0:38:15.840
<v Speaker 2>We take them all weird movies on Weird House Cinema,

0:38:15.880 --> 0:38:18.880
<v Speaker 2>and then on Saturdays we run an episode from the Vault,

0:38:19.000 --> 0:38:22.240
<v Speaker 2>an older episode of the show. Huge thanks as always

0:38:22.280 --> 0:38:26.200
<v Speaker 2>to our excellent audio producer JJ Posway. If you would

0:38:26.280 --> 0:38:28.400
<v Speaker 2>like to get in touch with us with feedback on

0:38:28.520 --> 0:38:30.960
<v Speaker 2>this episode or any other, to suggest a topic for

0:38:31.000 --> 0:38:33.760
<v Speaker 2>the future, or just to say hello. You can email

0:38:33.840 --> 0:38:45.240
<v Speaker 2>us at contact at stuff to Blow your Mind dot com.

0:38:45.360 --> 0:38:48.279
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0:39:05.000 --> 0:39:05.600
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