WEBVTT - How do planets get their moons?

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<v Speaker 1>Hey, do you ever wish that we had more moons

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<v Speaker 1>in our night sky?

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<v Speaker 2>Hmmm? I think the universe as moon does enough times.

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<v Speaker 1>Actually, well, I like the moons, and I sometimes wish

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<v Speaker 1>we had more going on in the night sky, like

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<v Speaker 1>lots of little moons.

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<v Speaker 2>But then I wonder if we had the same line

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<v Speaker 2>in Star Wars, you know, where he says that's no moon.

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<v Speaker 2>That wouldn't work.

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<v Speaker 1>Maybe instead of the Death Star, they would have had

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<v Speaker 1>the death constellation.

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<v Speaker 2>Or that song when the moon hits your eye like

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<v Speaker 2>a big pizza pie. That wouldn't work with a lot

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<v Speaker 2>of little moons. I guess it would work with lots

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<v Speaker 2>of mini pizzas.

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<v Speaker 1>The personal pan pizza would have been invented earlier.

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<v Speaker 2>Hi am Horehea, ma cartoonist and the creator of PhD comics.

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<v Speaker 1>Hi I'm Daniel. I'm a particle physicist and a professor

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<v Speaker 1>at UC Irvine, and I'd never really been a fan

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<v Speaker 1>of the pan pizza, of.

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<v Speaker 2>The pan or the pizza or just a combination of

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<v Speaker 2>the two.

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<v Speaker 1>The pizza in the pan. Definitely a thin crust kind

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<v Speaker 1>of guy over here, not.

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<v Speaker 2>A bread fan trying to curb your carbs.

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<v Speaker 1>I like tomato sauce. But I don't like the kiddie

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<v Speaker 1>pool of marinera that they call pizza in Chicago.

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<v Speaker 2>I feel like there's a thin line between a pan

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<v Speaker 2>pizza and like a casserole or like a pot pie.

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<v Speaker 1>It's really just a Midwestern hot dish.

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<v Speaker 2>There you go, But anyways, welcome to our podcast, Daniel

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<v Speaker 2>and Jorge Explain the Universe, a production of iHeartRadio.

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<v Speaker 1>Where we love everything about the universe, the thick ready

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<v Speaker 1>questions and the thin crunchy ones we wonder about how

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<v Speaker 1>everything out there in the universe works. We take a

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<v Speaker 1>big curiosity motivated by it, of the universe and try

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<v Speaker 1>to chew through all of it for you.

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<v Speaker 2>That's right, because the universe is a deep dish of

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<v Speaker 2>amazing facts and incredible things happening in it, full of

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<v Speaker 2>mysteries and wonderful conundrums for us to try to figure out.

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<v Speaker 1>And while physics has made incredible progress in understanding the

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<v Speaker 1>way the world works, we're still answering the kinds of

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<v Speaker 1>questions we've been asking basically forever, just looking around us,

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<v Speaker 1>seeing how the world is and wondering like, why is

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<v Speaker 1>it this way? How did it get to be this way?

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<v Speaker 2>Why does Deep Dish Pizza exist? Fundamental questions? That's what

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<v Speaker 2>we ask here on the podcast, and why doesn't Daniel

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<v Speaker 2>like them?

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<v Speaker 1>We know why Deep Dish Pizza exist for the same

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<v Speaker 1>reason vanilla ice cream exists, because you know, there's a

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<v Speaker 1>whole spectrum of people out there and everybody loves different things.

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<v Speaker 2>Are you saying the universe is kind of cheesy? I

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<v Speaker 2>guess it will definitely give you a heart attack as well.

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<v Speaker 2>There's no topping that joke, but yeah, we like to

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<v Speaker 2>think about the universe and all of the perfecting things

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<v Speaker 2>in it, like how did things come to be the

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<v Speaker 2>way they are? Why are we here? And where are

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<v Speaker 2>we in the universe?

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<v Speaker 1>And what is One of the real, simple but enduring

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<v Speaker 1>joys of being a curious person is just looking up

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<v Speaker 1>at the night sky. Not just being amazed at it's

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<v Speaker 1>beauty and odd at the depth of the view that

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<v Speaker 1>you were looking at, but this shared feeling through time

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<v Speaker 1>that humans one hundred years ago, a thousand years ago,

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<v Speaker 1>twenty five thousand years ago probably looked up at almost

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<v Speaker 1>the same night sky and wondered what was up there

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<v Speaker 1>and why it looked the way it did, and whether

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<v Speaker 1>it could have been different.

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<v Speaker 2>Yeah, you're looking at the exact same sky that our

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<v Speaker 2>ancestors did, full of stars, comments, and even a moon.

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<v Speaker 2>And they probably asked the same question that maybe a

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<v Speaker 2>lot of you have out there, which is, why do

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<v Speaker 2>we have a moon? And is it made out of cheese?

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<v Speaker 2>Is it just a big, flat, giant, floating deep dish

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<v Speaker 2>of cheese.

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<v Speaker 1>It's a spherical pizza. In the end, I have my

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<v Speaker 1>spherical pizza theory of the moon.

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<v Speaker 2>Do you do tell? Give us a slice of that

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<v Speaker 2>knowledge there?

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<v Speaker 1>All right? You called my bluff.

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<v Speaker 2>I got nothing and it was a crusty joke. But yeah,

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<v Speaker 2>sometimes we look out into the universe, into the night sky,

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<v Speaker 2>and we wonder why are things there, and how did

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<v Speaker 2>they come to be the way they are? What's going on?

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<v Speaker 2>And it wasn't just our ancestors that looked up at

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<v Speaker 2>the moon. It's like all of the planet that is

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<v Speaker 2>looking up at the moon, right, it's feeling its facts

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<v Speaker 2>and howling at it and rolling with the tides that

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<v Speaker 2>go along with the moon. The moon has. It makes

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<v Speaker 2>a big difference here on this planet.

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<v Speaker 1>Yeah, and these are not just questions asked by amateur astronomers,

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<v Speaker 1>but planet heiogeologist at the cunning edge are still trying

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<v Speaker 1>to figure out the details of how everything came to

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<v Speaker 1>be in our night sky.

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<v Speaker 2>So to the other podcast, we'll be tackling the question

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<v Speaker 2>how the planets get their moon or moons. Some planets

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<v Speaker 2>have lots of moons, right.

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<v Speaker 1>Yeah, that's right. It turns out our planet is quite

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<v Speaker 1>unusual in having approximately one moon.

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<v Speaker 2>So you do believe in the moon. The moon does exist, right.

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<v Speaker 1>I can see the moon. I know it's there, But.

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<v Speaker 2>How you know it's round? It always looks the same.

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<v Speaker 1>Well, we've been to the moon, so we can see

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<v Speaker 1>all around it, and you can tell that is round. Also,

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<v Speaker 1>the curved edge between the bright side and the dark

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<v Speaker 1>side of the moon tell us that it's going to

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<v Speaker 1>be round.

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<v Speaker 2>Oh right, you get sort of like the shadow of

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<v Speaker 2>it tells you it's round.

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<v Speaker 1>Exactly?

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<v Speaker 2>Is it perfectly round? Is the Moon perfectly round? Or

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<v Speaker 2>is it kind of an ellipsoid like the Earth.

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<v Speaker 1>Nothing in the universe is perfectly round. There are no

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<v Speaker 1>actual circles out there, maybe even not the event horizons

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<v Speaker 1>of black holes due to quantum effects. So the Moon

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<v Speaker 1>is definitely not perfectly round, and it's also pulled into

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<v Speaker 1>something of a football shape thanks to the Earth's gravity.

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<v Speaker 1>Tidal forces on the Moon by the Earth make it

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<v Speaker 1>a little bit oblong.

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<v Speaker 2>Whoa, I guess it's not spinning in the way that

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<v Speaker 2>the Earth is so that you get this centropical force.

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<v Speaker 2>But you're saying that the fact that the Earth is

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<v Speaker 2>pulling on it kind of stretches it out.

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<v Speaker 1>Yeah, it is spinning. It's just spinning at exactly the

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<v Speaker 1>right rate so that the same side of it is

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<v Speaker 1>always facing the Earth. This is called a tidal locking. Eventually,

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<v Speaker 1>the Earth pulls on the Moon to make it oblong,

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<v Speaker 1>and then they get stuck in this stable equilibrium where

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<v Speaker 1>that long bit is always pointing towards the Earth because

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<v Speaker 1>gravity on that long bit is a little stronger, so

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<v Speaker 1>it's sort of like a pendulum dangling towards the Earth.

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<v Speaker 2>Well, it is cool that we have a moon. I

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<v Speaker 2>guess it would to inspire all of these songs and

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<v Speaker 2>all these stories and legends about the moon.

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<v Speaker 1>It is nice to have a moon. It lights up

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<v Speaker 1>otherwise very dark nights, and it's something very close by

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<v Speaker 1>to look at, right, So much of the rest of

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<v Speaker 1>the night sky are just dots. They're so far away

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<v Speaker 1>they look like pinpricks. But the Moon has features on it.

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<v Speaker 1>I remember as a kid looking up at it and

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<v Speaker 1>studying those and like wondering what it would be like

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<v Speaker 1>to walk across it and to be on it, or

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<v Speaker 1>to look at the Earth from the moon. It's cool

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<v Speaker 1>that it's both in the night sky and kind of

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<v Speaker 1>close by.

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<v Speaker 2>Yeah, I guess it's kind of scary to think about it. Actually,

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<v Speaker 2>it's just kind of swinging around the Earth. It's constantly

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<v Speaker 2>falling around the Earth. That's what the Moon is doing.

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<v Speaker 2>And it's big, Like you don't want to mess with

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<v Speaker 2>the moon either.

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<v Speaker 1>Yeah, the Moon is pretty massive. And not only is

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<v Speaker 1>the Earth tugging on the Moon and forcing it to

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<v Speaker 1>face us the same way, but the Moon is doing

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<v Speaker 1>the same thing to Earth. Eventually, the Earth of the

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<v Speaker 1>Moon will both be tidally locked to each other.

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<v Speaker 2>Mmmmm, wait what does that mean? That means that we

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<v Speaker 2>will be going around the moon.

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<v Speaker 1>It means that, given enough time, the Moon will stay

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<v Speaker 1>on the same side of the Earth. The Earth's spin

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<v Speaker 1>and the Moon's spin will balance so that only one

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<v Speaker 1>side of the Earth ever sees the Moon the same way,

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<v Speaker 1>only one side of the Moon ever sees the Earth.

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<v Speaker 2>Wait, what for real. When is that going to happen.

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<v Speaker 1>It's not going to be for billions of years, but

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<v Speaker 1>it has already had an impact, Like the rate that

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<v Speaker 1>the Earth is spinning has slowed down to twenty four

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<v Speaker 1>hours per spin over the last four billion years. Four

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<v Speaker 1>billion years ago, it took about six hours for the

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<v Speaker 1>Earth to spin, So the Moon is slowing down the

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<v Speaker 1>spin of the Earth. Eventually, it will take about forty

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<v Speaker 1>seven of our current days to spin the Earth. That

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<v Speaker 1>will match the Moon's orbital period, and the Earth and

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<v Speaker 1>the Sun will be tidally locked to each other. But

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<v Speaker 1>that wouldn't be for billions of years, and that would

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<v Speaker 1>be assuming that the Sun doesn't gobble the Earth first.

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<v Speaker 2>Yeah, we would have bigger problems in the Moon at

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<v Speaker 2>that point.

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<v Speaker 1>But it would be kind of amazing if you could

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<v Speaker 1>only see the Moon from one half of the Earth.

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<v Speaker 1>It would mean you could grow up your whole life

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<v Speaker 1>and not see the Moon, and then travel to another

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<v Speaker 1>part of the Earth and see the Moon for the

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<v Speaker 1>first time. That would be incredible.

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<v Speaker 2>Whoa which sid gets to have the moon? Can they

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<v Speaker 2>predict that? Or we even have the same We probably

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<v Speaker 2>won't even have the same continents.

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<v Speaker 1>Right, Yeah, not in billions of years exactly.

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<v Speaker 2>I guess we have the moon to thank for having

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<v Speaker 2>more time in our day. Then without the moon that

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<v Speaker 2>things will be a lot more hectic.

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<v Speaker 1>Yeah, that's true. Those of you who like to work

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<v Speaker 1>late at night would have much shorter nights to get

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<v Speaker 1>stuff done.

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<v Speaker 2>I think the people during the day would also have

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<v Speaker 2>a shorter time, right, But it is an interesting question

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<v Speaker 2>how did we get this moon? Like how do planets

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<v Speaker 2>get moons at all? And why do we only have

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<v Speaker 2>one moon versus having lots of moons like other planets

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<v Speaker 2>which have up to eighty four moons.

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<v Speaker 1>It is really fun, fascinating question, and the answer tells

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<v Speaker 1>us a lot about how solar systems form, whether our

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<v Speaker 1>planet is weird, and maybe whether our solar system itself

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<v Speaker 1>is kind of weird.

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<v Speaker 2>Well, you can get all that from the moon.

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<v Speaker 1>You can learn a lot just by asking questions.

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<v Speaker 2>Well, as usual, we were wondering how many people out there?

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<v Speaker 2>I thought about the question of where moons come from

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<v Speaker 2>and how are they form? How do we get ours?

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<v Speaker 2>So as usual Daniel went out there into the internet

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<v Speaker 2>to ask people how do moons form?

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<v Speaker 1>Thanks very much to everybody who participates in this segment

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<v Speaker 1>of the podcast. If you've been listening for a while

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<v Speaker 1>and thinking about participating, please let me encourage you. It's fun,

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<v Speaker 1>it's easy. Everybody enjoys it. Write to me two questions

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<v Speaker 1>at Danielandjorge dot com.

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<v Speaker 2>So think about it for a second. How do you

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<v Speaker 2>think planets get their moons? Here's what people had to say.

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<v Speaker 3>I think that most moons form from cloud discs around planets,

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<v Speaker 3>and that Satan's rings are a picture of that process

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<v Speaker 3>going on.

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<v Speaker 4>Moons on form? How planet form? So they're small rocks

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<v Speaker 4>and then they hit each other and create bigger ones.

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<v Speaker 4>So when a planet is created, maybe when it gets created,

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<v Speaker 4>some debris goes out and then creates like a miniature

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<v Speaker 4>planet aka a moon.

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<v Speaker 2>Maybe I suppose the moon is just a small planet.

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<v Speaker 2>It's kind of just a planet that gets trapped by

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<v Speaker 2>another planet. Right, they're just rocks.

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<v Speaker 5>There's got to be like at least six ways moon forms.

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<v Speaker 5>I don't know, like things crashing together. Apparently we might

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<v Speaker 5>have stolen the Moon from Venus. Maybe probably a bunch

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<v Speaker 5>of other ways they could form too.

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<v Speaker 6>I think Moon's form either just sort of alongside they're

0:10:40.840 --> 0:10:46.080
<v Speaker 6>planet like Lucky, or from collisions like our own moon

0:10:47.440 --> 0:10:51.600
<v Speaker 6>came from an impact. Those are, I guess, the only

0:10:51.640 --> 0:10:52.320
<v Speaker 6>two I really know.

0:10:52.559 --> 0:10:56.480
<v Speaker 7>I would say that this is a collisions between among

0:10:57.240 --> 0:11:01.640
<v Speaker 7>asteroids planets, and then you have planet that has been

0:11:01.920 --> 0:11:04.320
<v Speaker 7>hit by an asteroid, and a small chunk of this

0:11:04.400 --> 0:11:07.400
<v Speaker 7>planet would be placed in a sort of an orbit,

0:11:07.480 --> 0:11:08.400
<v Speaker 7>and then you get the Moon.

0:11:08.520 --> 0:11:11.240
<v Speaker 8>I think it's when space dust is orbiting a planet

0:11:11.760 --> 0:11:15.760
<v Speaker 8>and then it clumps together into the Moon eventually, or if,

0:11:15.840 --> 0:11:21.240
<v Speaker 8>like an asteroid, is caught in the gravitational pool of

0:11:21.320 --> 0:11:24.640
<v Speaker 8>a planet and falls into its orbit.

0:11:24.880 --> 0:11:28.240
<v Speaker 1>I think Moon's form from asteroids and other bits of

0:11:28.280 --> 0:11:31.320
<v Speaker 1>space debris that get trapped in a planet's orbit.

0:11:31.559 --> 0:11:33.960
<v Speaker 9>I think that moon's form around planets the same way

0:11:34.120 --> 0:11:37.880
<v Speaker 9>that planets form around stars. I think that basically there's

0:11:37.880 --> 0:11:40.319
<v Speaker 9>a bunch of junk floating around the planet that aggregates

0:11:40.360 --> 0:11:42.319
<v Speaker 9>into a moon or moons.

0:11:42.520 --> 0:11:46.280
<v Speaker 2>All right, a lot of interesting answers here. Somebody said

0:11:46.320 --> 0:11:50.400
<v Speaker 2>at least six ways, that's all they said, But only

0:11:50.520 --> 0:11:54.880
<v Speaker 2>at least six he or she had six ways in mind.

0:11:55.000 --> 0:11:57.720
<v Speaker 1>M reminds me that Paul Simon's song just get on

0:11:57.760 --> 0:12:01.319
<v Speaker 1>the bus, gus don't need to discuss much. Yeah, there

0:12:01.400 --> 0:12:04.040
<v Speaker 1>must be six ways to get a moon.

0:12:04.200 --> 0:12:07.320
<v Speaker 2>Sounds like clickbait. Six ways so we can get a moon.

0:12:07.559 --> 0:12:11.040
<v Speaker 2>The sixth one will totally amaze you. Maybe we should

0:12:11.040 --> 0:12:14.040
<v Speaker 2>be learning from this listener and how to title our

0:12:14.440 --> 0:12:17.600
<v Speaker 2>podcast episodes. Although that you hear BuzzFeed is going down,

0:12:17.640 --> 0:12:20.320
<v Speaker 2>it's going out of business or BuzzFeed news.

0:12:20.440 --> 0:12:22.360
<v Speaker 1>Do you think there's a lesson there for us podcasters?

0:12:22.600 --> 0:12:25.480
<v Speaker 2>Yeah, I think there are six amazing lessons. The sixth

0:12:25.520 --> 0:12:27.160
<v Speaker 2>one will totally astound you.

0:12:27.280 --> 0:12:28.160
<v Speaker 1>I can't wait to hear.

0:12:28.360 --> 0:12:30.480
<v Speaker 2>But yeah, a lot of interesting theories here from people.

0:12:30.880 --> 0:12:33.440
<v Speaker 2>Some people think it happens from like a collision. Some

0:12:33.480 --> 0:12:37.199
<v Speaker 2>people think we stole it from another planet? Is that true?

0:12:37.320 --> 0:12:39.480
<v Speaker 1>The truth is that there are lots of different ways

0:12:39.520 --> 0:12:42.000
<v Speaker 1>to get moons, and we'll dig into several of them today.

0:12:42.200 --> 0:12:44.839
<v Speaker 2>M The sixth one will amaze you.

0:12:46.800 --> 0:12:47.520
<v Speaker 1>If we get there.

0:12:47.679 --> 0:12:50.280
<v Speaker 2>If we get that right, know for sure we'll get there.

0:12:50.760 --> 0:12:54.480
<v Speaker 2>Question is how long before we get there? Will we

0:12:54.520 --> 0:12:56.840
<v Speaker 2>do it before the hour is up? Towards a close call?

0:12:57.040 --> 0:12:59.360
<v Speaker 2>All right, Well, let's start with the basics, Daniel, how

0:12:59.360 --> 0:13:01.160
<v Speaker 2>would you define a moon? Like what is a moon?

0:13:01.440 --> 0:13:03.360
<v Speaker 2>And what's the difference between a moon and like a

0:13:03.440 --> 0:13:06.320
<v Speaker 2>satellite or an asteroid or just a space jump.

0:13:06.440 --> 0:13:08.800
<v Speaker 1>Yeah, this is an interesting question in astronomy. We have

0:13:08.880 --> 0:13:12.000
<v Speaker 1>all these categories we've invented to describe the kinds of

0:13:12.000 --> 0:13:14.720
<v Speaker 1>things we've seen out there, and then we find things

0:13:14.720 --> 0:13:17.440
<v Speaker 1>that break those categories, and it turns out there are

0:13:17.480 --> 0:13:20.520
<v Speaker 1>no real hard divisions and bright lines between stuff. It's

0:13:20.559 --> 0:13:22.960
<v Speaker 1>just sort of like where humans like to draw a

0:13:23.000 --> 0:13:25.679
<v Speaker 1>dotted line between things, and so it's kind of a

0:13:25.720 --> 0:13:29.040
<v Speaker 1>mess what a moon is signs. Originally they called these

0:13:29.040 --> 0:13:32.520
<v Speaker 1>things natural satellites, Like when you look at Jupiter and

0:13:32.559 --> 0:13:34.880
<v Speaker 1>you see things going around it, you call those satellites

0:13:34.880 --> 0:13:36.920
<v Speaker 1>of Jupiter. And for a long time, like before the

0:13:36.960 --> 0:13:40.000
<v Speaker 1>space age, the word moon just referred to the moon

0:13:40.040 --> 0:13:42.400
<v Speaker 1>of the Earth, which is the name of our moon.

0:13:42.559 --> 0:13:46.600
<v Speaker 1>But then we started launching artificial satellites, and so when

0:13:46.640 --> 0:13:49.880
<v Speaker 1>Sputnik went up, people called it an artificial satellite. But

0:13:49.960 --> 0:13:52.400
<v Speaker 1>that's sort of awkward and a mouthful, so people didn't

0:13:52.400 --> 0:13:55.680
<v Speaker 1>like saying artificial satellite. They just start calling it satellite,

0:13:55.840 --> 0:13:59.079
<v Speaker 1>and so that makes natural satellite kind of awkward.

0:13:58.679 --> 0:14:05.000
<v Speaker 2>To say organic satellite exactly, or farm raised satellites.

0:14:04.600 --> 0:14:06.720
<v Speaker 1>But natural satellite is kind of a mouthful, and so

0:14:06.960 --> 0:14:11.160
<v Speaker 1>now people, even scientists, sometimes say moons. Technically, we have

0:14:11.280 --> 0:14:14.480
<v Speaker 1>artificial satellites, things we have launched in due space, and

0:14:14.480 --> 0:14:18.080
<v Speaker 1>then we have natural satellites, things that are in orbit anyway,

0:14:18.200 --> 0:14:20.560
<v Speaker 1>naturally without the influence of humans.

0:14:20.720 --> 0:14:22.840
<v Speaker 2>But wait, wait, I think I've seen NASA call the

0:14:23.320 --> 0:14:25.720
<v Speaker 2>moons of Jupiter the moons of Jupiter. They never say

0:14:25.760 --> 0:14:26.880
<v Speaker 2>the satellites of Jupiter.

0:14:27.040 --> 0:14:29.920
<v Speaker 1>That's right. So technically we have artificial satellite and we

0:14:29.960 --> 0:14:32.880
<v Speaker 1>have natural satellite, though typically we just say satellite for

0:14:33.000 --> 0:14:36.480
<v Speaker 1>artificial satellite, and now we say moon for natural satellite,

0:14:36.520 --> 0:14:39.640
<v Speaker 1>even in scientific publications and like official press releases. So

0:14:39.720 --> 0:14:42.760
<v Speaker 1>now moon has come to mean natural satellite.

0:14:43.480 --> 0:14:45.120
<v Speaker 2>I see. But I guess if you put the in

0:14:45.160 --> 0:14:47.600
<v Speaker 2>front of it, then it's our moon. Like the moon

0:14:47.880 --> 0:14:50.840
<v Speaker 2>is our moon, but then other moons are just moons.

0:14:51.440 --> 0:14:55.120
<v Speaker 1>Yeah, exactly, the moon is our moon or Luna if

0:14:55.120 --> 0:14:57.880
<v Speaker 1>you prefer. And moon with a lowercase M means any

0:14:58.000 --> 0:14:59.280
<v Speaker 1>kind of natural satellite.

0:15:00.040 --> 0:15:01.960
<v Speaker 2>I guess you can have rocks, and you can have

0:15:02.120 --> 0:15:02.840
<v Speaker 2>the rock.

0:15:05.400 --> 0:15:07.400
<v Speaker 1>Exactly. We have lots of rocks in orbit, but I

0:15:07.440 --> 0:15:09.880
<v Speaker 1>don't think we have the rock in orbit yet, though

0:15:09.920 --> 0:15:12.240
<v Speaker 1>I haven't seen fast and Furious twenty seven or whichever

0:15:12.280 --> 0:15:13.120
<v Speaker 1>one has space.

0:15:14.000 --> 0:15:16.920
<v Speaker 2>I'm assureing the next one there, they'll you know, speed

0:15:17.000 --> 0:15:19.160
<v Speaker 2>up a ramp and somehow make it up to space

0:15:20.040 --> 0:15:23.080
<v Speaker 2>and crash into a space station. While he jumps and

0:15:23.160 --> 0:15:24.920
<v Speaker 2>also launches a rocket launcher.

0:15:25.360 --> 0:15:27.440
<v Speaker 1>He's got to flex his muscles at some point. Another

0:15:27.520 --> 0:15:30.560
<v Speaker 1>question is size, Like, is every object that's orbiting the

0:15:30.600 --> 0:15:33.920
<v Speaker 1>Earth a moon? Every tiny little rock is at a

0:15:34.040 --> 0:15:37.440
<v Speaker 1>moon of the Earth. Officially, there's no lower limit, right,

0:15:37.480 --> 0:15:40.520
<v Speaker 1>Like every natural object with an orbit around the planet,

0:15:40.760 --> 0:15:42.440
<v Speaker 1>technically you could call it a moon.

0:15:42.680 --> 0:15:44.760
<v Speaker 2>Wait what I mean? No, at some point, it's just

0:15:44.800 --> 0:15:46.080
<v Speaker 2>the rock, right.

0:15:45.920 --> 0:15:48.040
<v Speaker 1>The moon is just a rock. Also makes the Moon

0:15:48.120 --> 0:15:51.760
<v Speaker 1>different from other rocks orbiting the planet is just the size,

0:15:52.160 --> 0:15:55.920
<v Speaker 1>and there is no official lower limit to the size

0:15:55.920 --> 0:15:58.040
<v Speaker 1>of a moon. You could have a moon of any size,

0:15:58.080 --> 0:16:00.720
<v Speaker 1>and any limit you place is going to be totally ourary, right.

0:16:01.640 --> 0:16:03.640
<v Speaker 2>I wonder if the definition also has to do with

0:16:03.800 --> 0:16:07.560
<v Speaker 2>how stable its orbit is. Like, if I just throw

0:16:07.560 --> 0:16:10.680
<v Speaker 2>a rock and into space, it's kind of orbiting the

0:16:10.680 --> 0:16:12.200
<v Speaker 2>Earth for a little bit, does that mean it's a.

0:16:12.160 --> 0:16:14.760
<v Speaker 1>Moon that's not really in orbit? Right? I don't know

0:16:14.760 --> 0:16:16.960
<v Speaker 1>how strong you are. Recently haven't seen you in a while,

0:16:17.040 --> 0:16:18.720
<v Speaker 1>But I don't think you could throw a rock and

0:16:18.760 --> 0:16:21.360
<v Speaker 1>actually get it into orbit. It has to be in orbit.

0:16:21.520 --> 0:16:24.880
<v Speaker 2>Oh yeah, do you want to make that bet? I'll

0:16:24.880 --> 0:16:27.400
<v Speaker 2>bet you a billion dollars because with a billion dollars

0:16:27.400 --> 0:16:29.720
<v Speaker 2>I can come into space and throw the rock.

0:16:30.560 --> 0:16:32.400
<v Speaker 1>If you get a rock orbiting the Earth, I will

0:16:32.440 --> 0:16:34.760
<v Speaker 1>campaign NASA to let you name it officially.

0:16:35.480 --> 0:16:37.440
<v Speaker 2>Well, if you get me on a rocket ship into

0:16:37.440 --> 0:16:40.040
<v Speaker 2>space to throw a rock, we'll start the whole process.

0:16:40.160 --> 0:16:42.800
<v Speaker 1>But we can look at the typical sizes of these things,

0:16:43.240 --> 0:16:45.880
<v Speaker 1>and like in our Solar system there are a few

0:16:46.080 --> 0:16:49.440
<v Speaker 1>hundred of these moons. There's six planets that have moons,

0:16:49.480 --> 0:16:51.520
<v Speaker 1>for a total of two hundred and twenty six moons,

0:16:51.560 --> 0:16:54.920
<v Speaker 1>and typically the planet to moon mass ratio is at

0:16:55.000 --> 0:16:58.280
<v Speaker 1>least ten thousand to one, so moons typically have a

0:16:58.400 --> 0:17:01.200
<v Speaker 1>much smaller mass than the planet they orbit.

0:17:01.440 --> 0:17:04.320
<v Speaker 2>Wait, there are six planets in our Solar system with moons.

0:17:04.400 --> 0:17:05.520
<v Speaker 2>Who doesn't have a moon?

0:17:05.840 --> 0:17:09.480
<v Speaker 1>Neither Mercury nor Venus have moons. That's probably because they're

0:17:09.480 --> 0:17:12.680
<v Speaker 1>too close to the Sun and so tidal disruption basically

0:17:12.720 --> 0:17:13.960
<v Speaker 1>pulls those moons away.

0:17:14.240 --> 0:17:16.720
<v Speaker 2>Oh interesting, and I just figured out that's probably what

0:17:16.760 --> 0:17:19.119
<v Speaker 2>the listener meant when they said at least six ways.

0:17:19.240 --> 0:17:25.280
<v Speaker 1>Oh nice. Probably every moon has a unique story, m

0:17:26.240 --> 0:17:29.800
<v Speaker 1>they have their own origin story. Of course, our moon

0:17:29.920 --> 0:17:32.760
<v Speaker 1>is a big exception to this ten thousand to one rule, right,

0:17:32.760 --> 0:17:35.240
<v Speaker 1>because the mass of the Moon is about one eightieth

0:17:35.480 --> 0:17:37.840
<v Speaker 1>of the mass of the Earth. It's like more than

0:17:37.960 --> 0:17:40.880
<v Speaker 1>one percent of the mass of the Earth. So it's

0:17:40.880 --> 0:17:43.200
<v Speaker 1>a big honk and moon it's very unusual.

0:17:43.600 --> 0:17:46.840
<v Speaker 2>So most of the moons in the Solar System, some

0:17:46.920 --> 0:17:48.960
<v Speaker 2>of them are as big as our moon, but you're

0:17:49.000 --> 0:17:52.280
<v Speaker 2>saying that the ratio compared to their planet, most of

0:17:52.320 --> 0:17:52.919
<v Speaker 2>them are small.

0:17:53.520 --> 0:17:56.120
<v Speaker 1>Most of them are small exactly. And then there's the case,

0:17:56.119 --> 0:17:59.440
<v Speaker 1>for example, of Pluto. Pluto has a moon which is Sharon,

0:17:59.520 --> 0:18:02.480
<v Speaker 1>which is one eighth of its mass, and so like

0:18:02.520 --> 0:18:05.399
<v Speaker 1>we call Pluto a dwarf planet, and we call Sharon

0:18:05.600 --> 0:18:08.440
<v Speaker 1>a moon of Pluto. But you know, you could also

0:18:08.600 --> 0:18:11.920
<v Speaker 1>argue that it's really like a dwarf planet binary system,

0:18:12.000 --> 0:18:14.120
<v Speaker 1>which one is a planet and which one is the moon?

0:18:14.200 --> 0:18:15.560
<v Speaker 1>It all gets kind of fuzzy.

0:18:15.680 --> 0:18:19.040
<v Speaker 2>Whoa, it's like a double planet.

0:18:19.119 --> 0:18:19.399
<v Speaker 7>Man.

0:18:21.000 --> 0:18:23.520
<v Speaker 1>One way to distinguish the two scenarios, like having a

0:18:23.560 --> 0:18:26.400
<v Speaker 1>double planet or a planet with a moon. Is whether

0:18:26.480 --> 0:18:30.160
<v Speaker 1>the center of mass of the system is within the

0:18:30.200 --> 0:18:32.359
<v Speaker 1>surface of one of them. If you find the point

0:18:32.400 --> 0:18:35.439
<v Speaker 1>that averages where all the mass is, the point around

0:18:35.480 --> 0:18:38.159
<v Speaker 1>which the two objects really are orbiting, if that is

0:18:38.400 --> 0:18:41.320
<v Speaker 1>underground one of the two objects, and you call the

0:18:41.359 --> 0:18:43.359
<v Speaker 1>more massive one a planet and the other one a moon.

0:18:43.560 --> 0:18:46.840
<v Speaker 1>Otherwise you call it a binary system. Again, that's still

0:18:46.960 --> 0:18:49.200
<v Speaker 1>kind of arbitrary, right, We're just like giving these things

0:18:49.280 --> 0:18:52.000
<v Speaker 1>names and drawing lines between them. Really, there's just a

0:18:52.080 --> 0:18:54.520
<v Speaker 1>bunch of different rocks out there in the universe orbiting

0:18:54.520 --> 0:18:54.880
<v Speaker 1>each other.

0:18:55.760 --> 0:18:58.119
<v Speaker 2>Except also, Pluto is not a planet, So can you

0:18:58.160 --> 0:19:00.959
<v Speaker 2>have a moon around something that's not planet? Like can

0:19:01.040 --> 0:19:02.880
<v Speaker 2>you can moon or can a moon have a moon?

0:19:03.800 --> 0:19:05.880
<v Speaker 1>You can have a moon around a dwarf planet, though

0:19:05.920 --> 0:19:07.720
<v Speaker 1>maybe you would want to call it a dwarf moon.

0:19:07.880 --> 0:19:11.640
<v Speaker 1>I don't know. And it's possible in principle to have

0:19:11.800 --> 0:19:15.000
<v Speaker 1>moons around moons. There are asteroids that have moons.

0:19:15.520 --> 0:19:19.040
<v Speaker 2>Wait what, and you still call them moons, not master moons.

0:19:19.119 --> 0:19:21.880
<v Speaker 1>Some people want to call them moonlits or moon moons

0:19:22.359 --> 0:19:23.080
<v Speaker 1>like the moon of a.

0:19:23.040 --> 0:19:26.040
<v Speaker 2>Moon or moony's or mini moons.

0:19:26.160 --> 0:19:28.199
<v Speaker 1>And there are even some moons, like Rhea has its

0:19:28.240 --> 0:19:30.600
<v Speaker 1>own ring system Saturn's moon Rhea.

0:19:30.760 --> 0:19:34.600
<v Speaker 2>Wait what some moons can have rings? Yeah, because they

0:19:34.640 --> 0:19:36.439
<v Speaker 2>have so many mini moons.

0:19:36.560 --> 0:19:39.600
<v Speaker 1>If you're big enough that you dominate the gravitational environment nearby,

0:19:39.680 --> 0:19:41.280
<v Speaker 1>then yeah, you can have your own rings.

0:19:41.320 --> 0:19:44.080
<v Speaker 2>I mean, I guess technically anything can have a satellite, right,

0:19:44.119 --> 0:19:46.439
<v Speaker 2>Like I can take a baseball, put in into space

0:19:46.520 --> 0:19:49.680
<v Speaker 2>and then knock a you know, a speck of dust

0:19:49.680 --> 0:19:50.640
<v Speaker 2>in orbit around it.

0:19:50.640 --> 0:19:53.200
<v Speaker 1>Right, yeah, exactly. That wouldn't be a planet or even

0:19:53.200 --> 0:19:56.320
<v Speaker 1>a dwarf planet, but it would have an orbiting object.

0:19:56.960 --> 0:19:59.960
<v Speaker 1>Is that a natural satellite? I'm not quite sure.

0:19:59.800 --> 0:20:01.399
<v Speaker 2>A what else do we know about moons?

0:20:01.520 --> 0:20:03.879
<v Speaker 1>If you try to dig into the ancient history of moons,

0:20:03.920 --> 0:20:07.680
<v Speaker 1>it gets quite confusing to read about because until Copernicus,

0:20:07.880 --> 0:20:10.679
<v Speaker 1>moons were actually called planets, like the Moon itself was

0:20:10.720 --> 0:20:13.240
<v Speaker 1>referred to as a planet. Like when you talked about

0:20:13.240 --> 0:20:16.240
<v Speaker 1>astronomy in the fifteen hundreds, you said the planet Mars,

0:20:16.280 --> 0:20:20.360
<v Speaker 1>the planet Venus, the planet Luna. And it wasn't until Kepler,

0:20:20.520 --> 0:20:22.560
<v Speaker 1>who was thinking about how these things orbit each other,

0:20:22.560 --> 0:20:25.399
<v Speaker 1>who had a better understanding of these orbits, that we

0:20:25.440 --> 0:20:28.439
<v Speaker 1>started calling the moon a satellite of the Earth, and

0:20:28.480 --> 0:20:31.119
<v Speaker 1>then the satellites of Jupiter are of course the moons

0:20:31.160 --> 0:20:34.119
<v Speaker 1>of Jupiter. So there's a really fun interesting history to

0:20:34.160 --> 0:20:34.800
<v Speaker 1>these words.

0:20:34.960 --> 0:20:37.359
<v Speaker 2>Wait, really, so like, for a moment in human history,

0:20:37.400 --> 0:20:41.000
<v Speaker 2>we thought the Moon was another planet orbiting the Solar System.

0:20:41.240 --> 0:20:42.920
<v Speaker 2>Technically it is orbiting the Sun.

0:20:43.200 --> 0:20:45.240
<v Speaker 1>Yeah, it is orbiting the Sun, and it is orbiting

0:20:45.240 --> 0:20:47.440
<v Speaker 1>the Earth. Right, it's not that we thought the Moon

0:20:47.560 --> 0:20:50.119
<v Speaker 1>was a planet like Mars. It's just that we categorized

0:20:50.160 --> 0:20:52.320
<v Speaker 1>all these things the same way. All these words are

0:20:52.359 --> 0:20:54.680
<v Speaker 1>just buckets, right, and they're just like grab a bunch

0:20:54.760 --> 0:20:56.600
<v Speaker 1>of the stuff that's out there and gather it all

0:20:56.640 --> 0:20:59.600
<v Speaker 1>into a conceptual bucket. And where the lines between these

0:20:59.640 --> 0:21:02.160
<v Speaker 1>buckets is a little bit arbitrary. And so it used

0:21:02.160 --> 0:21:04.360
<v Speaker 1>to be that we lumped the moon in with the planets.

0:21:04.680 --> 0:21:07.240
<v Speaker 1>Now we have a separate category for things that orbit

0:21:07.280 --> 0:21:08.320
<v Speaker 1>the planets.

0:21:09.280 --> 0:21:11.639
<v Speaker 2>Shoot for the Moon. I guess when you're naming things,

0:21:11.760 --> 0:21:14.159
<v Speaker 2>all right, well, let's get a little deeper into where

0:21:14.200 --> 0:21:16.920
<v Speaker 2>the Moon came from, Where do moons in general come from,

0:21:16.960 --> 0:21:19.480
<v Speaker 2>how do other planets get their moons, and what does

0:21:19.520 --> 0:21:22.399
<v Speaker 2>it all mean about the history of the Solar System.

0:21:22.560 --> 0:21:37.479
<v Speaker 2>But first let's take a quick break, all right, we're

0:21:37.520 --> 0:21:40.840
<v Speaker 2>getting a little looney here talking about the moon and

0:21:40.880 --> 0:21:43.399
<v Speaker 2>how we got it and how do planets get their moons.

0:21:43.560 --> 0:21:46.320
<v Speaker 1>It is really fun in ancient question to wonder why

0:21:46.359 --> 0:21:48.560
<v Speaker 1>that thing is in our sky and why Jupiter has

0:21:48.600 --> 0:21:51.359
<v Speaker 1>more moons than we do. And if history had been different,

0:21:51.440 --> 0:21:53.320
<v Speaker 1>would we have had a bunch of moons? What would

0:21:53.359 --> 0:21:55.919
<v Speaker 1>it be like to live in that scenario? Could we

0:21:56.080 --> 0:21:59.240
<v Speaker 1>sail as well? If the ties were crazy and complicated

0:21:59.359 --> 0:22:02.080
<v Speaker 1>from having like fifteen different little moons? Hmmm?

0:22:02.400 --> 0:22:05.440
<v Speaker 2>Interesting? Yeah, that would affect the tides, right, But that

0:22:05.440 --> 0:22:06.919
<v Speaker 2>wouldn't affect navigation, would it.

0:22:06.920 --> 0:22:09.000
<v Speaker 1>It wouldn't affect navigation, but it would affect when it's

0:22:09.040 --> 0:22:11.359
<v Speaker 1>easy to launch your ships or not, and so it

0:22:11.400 --> 0:22:13.800
<v Speaker 1>might affect lots of industries and exploration.

0:22:14.160 --> 0:22:16.199
<v Speaker 2>M Also, if you're a were wolf, it would be

0:22:16.240 --> 0:22:19.840
<v Speaker 2>pretty complicated, right, probably, just you know, just the planet ahead.

0:22:20.760 --> 0:22:22.840
<v Speaker 1>Maybe you change into one kind of wolf for one

0:22:22.880 --> 0:22:24.879
<v Speaker 1>moon and another kind of wolf for another moon, and

0:22:24.920 --> 0:22:27.440
<v Speaker 1>like a Pomeranian for the little moon or a shitsu.

0:22:29.040 --> 0:22:31.840
<v Speaker 2>Yeah, there you go, different moons for different breeds.

0:22:31.600 --> 0:22:33.600
<v Speaker 1>Two moons up in the sky. Then you're a hybrid, right,

0:22:33.800 --> 0:22:35.520
<v Speaker 1>This sounds like a fun science fiction story.

0:22:35.600 --> 0:22:37.200
<v Speaker 2>It sounds like a great Ya novel.

0:22:39.080 --> 0:22:40.159
<v Speaker 1>So many spin offs.

0:22:40.200 --> 0:22:42.560
<v Speaker 2>All right, we talked about the word moon is kind

0:22:42.560 --> 0:22:45.879
<v Speaker 2>of flexible and it's not quite super well defined, but

0:22:46.040 --> 0:22:48.200
<v Speaker 2>basically it just kind of means like a big rock

0:22:48.280 --> 0:22:50.800
<v Speaker 2>circling around a bigger rock. Right, that's right.

0:22:50.840 --> 0:22:53.320
<v Speaker 1>It's a big rock orbiting another big rock.

0:22:53.520 --> 0:22:55.760
<v Speaker 2>And as you said, six of the planets in our

0:22:55.800 --> 0:22:59.280
<v Speaker 2>Solar system have them. Venus and Mercury don't because I

0:22:59.280 --> 0:23:01.879
<v Speaker 2>guess they're too hot, you said. And if they had moons,

0:23:01.880 --> 0:23:04.840
<v Speaker 2>then the Sun would have disrupted its orbit and probably

0:23:04.920 --> 0:23:06.960
<v Speaker 2>made it crash into the planet, right or fly away.

0:23:07.080 --> 0:23:08.879
<v Speaker 1>Yeah, it's all about the tidal forces. It makes it

0:23:08.920 --> 0:23:12.240
<v Speaker 1>basically impossible for Mercury or Venus to have moons and

0:23:12.280 --> 0:23:14.560
<v Speaker 1>to keep them. It's because they're so close to the Sun.

0:23:14.600 --> 0:23:18.080
<v Speaker 1>It's not their actual temperature, it's the gravitational tidal forces

0:23:18.080 --> 0:23:18.640
<v Speaker 1>from the Sun.

0:23:18.880 --> 0:23:21.399
<v Speaker 2>All right, Well, what do we know about where moons

0:23:21.400 --> 0:23:22.440
<v Speaker 2>come from and how they're form?

0:23:22.640 --> 0:23:24.280
<v Speaker 1>So you can tell a lot about where a moon

0:23:24.320 --> 0:23:26.679
<v Speaker 1>came from based on what it's made out of and

0:23:26.760 --> 0:23:29.439
<v Speaker 1>how it's orbiting. If a moon is mostly in a

0:23:29.600 --> 0:23:32.800
<v Speaker 1>circular orbit, and the circular orbit follows the tilt of

0:23:32.840 --> 0:23:36.600
<v Speaker 1>the planet, so for example, it's orbiting around the equator

0:23:36.680 --> 0:23:39.399
<v Speaker 1>in mostly a circle. Then it's very likely that that

0:23:39.520 --> 0:23:43.000
<v Speaker 1>moon came from the same stuff that formed the planet.

0:23:43.280 --> 0:23:45.560
<v Speaker 1>Remember how planets form in the beginning, it's a big

0:23:45.640 --> 0:23:48.679
<v Speaker 1>cloud of gas and dust that forms the whole Solar System.

0:23:48.800 --> 0:23:50.680
<v Speaker 1>Most of the gas is gobbled up by the star

0:23:50.760 --> 0:23:53.240
<v Speaker 1>as it forms, and our Sun has ninety ninety percent

0:23:53.480 --> 0:23:55.359
<v Speaker 1>of the mass of the Solar System. But if you

0:23:55.400 --> 0:23:57.719
<v Speaker 1>get a little isolated pocket of heavy stuff that has

0:23:57.760 --> 0:24:00.439
<v Speaker 1>its own gravity and can gather itself together, then you

0:24:00.440 --> 0:24:02.600
<v Speaker 1>can get a planet. So a planet sort of forms

0:24:02.640 --> 0:24:05.200
<v Speaker 1>the same way the Solar System does. It's the gravitational

0:24:05.280 --> 0:24:06.800
<v Speaker 1>collapse of a big blob of.

0:24:06.760 --> 0:24:09.280
<v Speaker 2>Stuff, right, And initially it's just kind of like a

0:24:09.320 --> 0:24:13.000
<v Speaker 2>big cloud of rocks and dust that's spinning or has

0:24:13.080 --> 0:24:14.160
<v Speaker 2>kind of an overall spin.

0:24:14.800 --> 0:24:17.240
<v Speaker 1>Exactly. The reason you get moons around planets is the

0:24:17.280 --> 0:24:20.280
<v Speaker 1>same reason you get planets around stars. Right. You don't

0:24:20.320 --> 0:24:22.480
<v Speaker 1>just get all the mass of the Solar System collapsing

0:24:22.560 --> 0:24:24.560
<v Speaker 1>into the Sun. You get these little pockets that have

0:24:24.640 --> 0:24:27.040
<v Speaker 1>enough gravity to form themselves together and then are moving

0:24:27.080 --> 0:24:30.040
<v Speaker 1>at high enough speed that they can resist falling into

0:24:30.119 --> 0:24:33.080
<v Speaker 1>the Sun. Now, around those planets, of course, you also

0:24:33.160 --> 0:24:35.679
<v Speaker 1>have little clouds of gas and dust. Some of it

0:24:35.720 --> 0:24:38.199
<v Speaker 1>collapses into the planet, most of it, but some of

0:24:38.240 --> 0:24:41.680
<v Speaker 1>it pulls itself together and has enough velocity to avoid

0:24:42.119 --> 0:24:45.320
<v Speaker 1>falling into the planet. And so if you have enough

0:24:45.359 --> 0:24:47.600
<v Speaker 1>velocity and you can pull yourself together, then you can

0:24:47.600 --> 0:24:50.439
<v Speaker 1>form like a little planet's planet, a little miniature system

0:24:50.480 --> 0:24:52.680
<v Speaker 1>around the planet, the same way the planet is going

0:24:52.720 --> 0:24:53.320
<v Speaker 1>around the Sun.

0:24:53.560 --> 0:24:56.360
<v Speaker 2>Right, because I guess gravity. That's how gravity works, right,

0:24:56.400 --> 0:24:59.600
<v Speaker 2>Like everything is attracted to everything else. It's not just

0:24:59.640 --> 0:25:01.960
<v Speaker 2>like we're attract it to the Sun or juice attracted

0:25:02.200 --> 0:25:06.159
<v Speaker 2>to the planet Earth. It's like I'm attracted to my

0:25:06.320 --> 0:25:08.800
<v Speaker 2>car and to this base bomb, the base will attracted

0:25:08.840 --> 0:25:10.520
<v Speaker 2>to me. And so if we were out in space,

0:25:11.160 --> 0:25:13.040
<v Speaker 2>we would both be falling towards the Earth, but then

0:25:13.080 --> 0:25:15.040
<v Speaker 2>we would there would also be an attraction between us.

0:25:15.080 --> 0:25:18.000
<v Speaker 2>And sometimes I think what you're saying is that if

0:25:18.200 --> 0:25:21.520
<v Speaker 2>a clump of dirt and rocks when the planet is forming,

0:25:21.560 --> 0:25:24.040
<v Speaker 2>it's kind of far enough out there, it will clump

0:25:24.080 --> 0:25:25.879
<v Speaker 2>together before it clumps with the Earth.

0:25:26.040 --> 0:25:28.680
<v Speaker 1>Yeah, that's exactly right. And there's sort of two steps there.

0:25:29.119 --> 0:25:32.760
<v Speaker 1>One is have enough velocity, like are you spinning fast

0:25:32.840 --> 0:25:35.880
<v Speaker 1>enough that you can basically get in orbit around the planet,

0:25:35.960 --> 0:25:38.560
<v Speaker 1>And that's how you get like a protoplanetary disc. The

0:25:38.600 --> 0:25:41.240
<v Speaker 1>planet forms and have some stuff out there that hasn't

0:25:41.280 --> 0:25:43.920
<v Speaker 1>fallen into the planet. So initially it's like a disc

0:25:44.280 --> 0:25:47.120
<v Speaker 1>and that can pull itself together using gravity into a ring.

0:25:47.359 --> 0:25:49.280
<v Speaker 1>And then there's a question of whether that ring can

0:25:49.320 --> 0:25:52.439
<v Speaker 1>pull itself together into a moon or not. Sometimes it

0:25:52.480 --> 0:25:55.800
<v Speaker 1>stays a ring and sometimes it forms a moon, and

0:25:55.840 --> 0:25:58.879
<v Speaker 1>that depends on how close you are to that planet.

0:25:59.119 --> 0:26:01.680
<v Speaker 1>If you're really really close to that planet, close to

0:26:01.720 --> 0:26:04.159
<v Speaker 1>than what we call the Roche limit, then tile forces

0:26:04.160 --> 0:26:05.879
<v Speaker 1>from the planet are too strong. If you try to

0:26:05.880 --> 0:26:08.280
<v Speaker 1>form a moon, the tile forces will tear it apart.

0:26:08.560 --> 0:26:11.720
<v Speaker 1>If you're outpast the Roche limit, then the tidle forces

0:26:11.720 --> 0:26:14.240
<v Speaker 1>are weak and you can gather together into a moon.

0:26:14.440 --> 0:26:16.879
<v Speaker 1>So you have to have enough velocity to avoid falling

0:26:16.920 --> 0:26:19.200
<v Speaker 1>into the planet, and then you have to be out

0:26:19.280 --> 0:26:22.119
<v Speaker 1>past the Roche limit to have a ring get turned

0:26:22.160 --> 0:26:22.840
<v Speaker 1>into a moon.

0:26:23.880 --> 0:26:26.760
<v Speaker 2>Because I think, as we've talked about before, gravity kind

0:26:26.800 --> 0:26:29.439
<v Speaker 2>of depends on the distance between two things. Right. So

0:26:29.840 --> 0:26:32.560
<v Speaker 2>if you're really close to the Earth, then like the

0:26:32.560 --> 0:26:34.560
<v Speaker 2>difference between one side of the Moon and the other

0:26:34.600 --> 0:26:38.040
<v Speaker 2>side of the Moon is they experience very different gravitational forces.

0:26:38.080 --> 0:26:40.960
<v Speaker 2>But maybe if you're far out and beyond this limit,

0:26:41.040 --> 0:26:44.560
<v Speaker 2>then you don't see this difference in pull from the

0:26:44.600 --> 0:26:48.119
<v Speaker 2>Earth between one and and the other, which kind of

0:26:48.200 --> 0:26:49.040
<v Speaker 2>lets you clump together.

0:26:49.680 --> 0:26:52.119
<v Speaker 1>You'll still always feel that difference, right, and like the

0:26:52.160 --> 0:26:55.280
<v Speaker 1>Moon does feel that difference. That's why we talked about earlier.

0:26:55.359 --> 0:26:58.199
<v Speaker 1>The Moon is a football. It is being pulled by

0:26:58.200 --> 0:27:00.560
<v Speaker 1>the Earth's tidal forces, but it's far and away that

0:27:00.640 --> 0:27:03.320
<v Speaker 1>those tidle forces are not strong enough to tear it apart.

0:27:03.440 --> 0:27:06.520
<v Speaker 1>The roach limit for the Earth is around ten thousand kilometers.

0:27:06.680 --> 0:27:08.840
<v Speaker 1>The Moon is like three hundred and eighty five thousand

0:27:08.880 --> 0:27:11.880
<v Speaker 1>kilometers away, so it's well past the roach limit. If

0:27:11.920 --> 0:27:14.000
<v Speaker 1>the Moon was much much closer, if it was like

0:27:14.119 --> 0:27:16.720
<v Speaker 1>less than ten thousand kilometers from the surface of the Earth,

0:27:17.000 --> 0:27:19.640
<v Speaker 1>the Earth would tear it apart with those tidal forces

0:27:19.680 --> 0:27:22.000
<v Speaker 1>into a massive ring system instead.

0:27:21.920 --> 0:27:23.800
<v Speaker 2>Where some of the rocks in that ring are going

0:27:23.840 --> 0:27:24.600
<v Speaker 2>at different speeds.

0:27:24.640 --> 0:27:26.320
<v Speaker 1>Right, it would be pretty cool to see the Moon

0:27:26.440 --> 0:27:28.840
<v Speaker 1>get torn up into rocks. Not all of them would

0:27:28.960 --> 0:27:31.760
<v Speaker 1>have the same velocity originally as the Moon. I'm sure

0:27:31.800 --> 0:27:34.159
<v Speaker 1>it would be somewhat destructive and chaotic. Some of them

0:27:34.160 --> 0:27:35.600
<v Speaker 1>would end up falling to the Earth, some of them

0:27:35.640 --> 0:27:37.199
<v Speaker 1>would get lost, and some of them would end up

0:27:37.200 --> 0:27:37.680
<v Speaker 1>in orbit.

0:27:37.880 --> 0:27:40.400
<v Speaker 2>Cool And I think that, as you said, also applies

0:27:40.400 --> 0:27:42.000
<v Speaker 2>to planets, right like you kind of have to be

0:27:42.040 --> 0:27:44.280
<v Speaker 2>a certain distance away from the Sun just to form

0:27:44.320 --> 0:27:44.920
<v Speaker 2>a planet, too.

0:27:45.200 --> 0:27:47.439
<v Speaker 1>Exactly, if you're too close to the Sun, then the

0:27:47.480 --> 0:27:51.640
<v Speaker 1>Sun's tidal forces, which are very powerful, will pull you apart.

0:27:51.800 --> 0:27:53.760
<v Speaker 1>So the roche limit for the Sun is like seven

0:27:53.840 --> 0:27:56.520
<v Speaker 1>hundred and fifty thousand kilometers. So if the Earth was

0:27:56.600 --> 0:27:59.200
<v Speaker 1>that close to the Sun, not only will we be fried,

0:27:59.240 --> 0:28:01.240
<v Speaker 1>of course, but the Sun would pull us apart with

0:28:01.359 --> 0:28:05.120
<v Speaker 1>its tidal forces. As you said, the gravitational force depends

0:28:05.160 --> 0:28:07.719
<v Speaker 1>on the distance, and so the Sun's gravit on the

0:28:07.760 --> 0:28:09.720
<v Speaker 1>near side of the Earth would be so much more

0:28:09.760 --> 0:28:11.879
<v Speaker 1>powerful than the Sun's gravity in the far side of

0:28:11.880 --> 0:28:14.520
<v Speaker 1>the Earth. It's effectively pulling us apart, and the Earth

0:28:14.880 --> 0:28:17.439
<v Speaker 1>is not strong enough to survive if it's closer than

0:28:17.480 --> 0:28:20.879
<v Speaker 1>seven hundred and fifty thousand kilometers. Fortunately, we're like one

0:28:20.960 --> 0:28:24.120
<v Speaker 1>hundred and fifty million kilometers from the Sun, so we're

0:28:24.119 --> 0:28:27.360
<v Speaker 1>nowhere near the Roche limit. And this isn't like an exact,

0:28:27.440 --> 0:28:29.840
<v Speaker 1>hard and fast number, it's like approximate. It depends on

0:28:29.880 --> 0:28:32.119
<v Speaker 1>the mass of the object, and it depends on structural

0:28:32.119 --> 0:28:34.080
<v Speaker 1>features of it, Like if you had a planet made

0:28:34.080 --> 0:28:36.520
<v Speaker 1>out of diamond, it could get closer to the Sun

0:28:36.680 --> 0:28:38.080
<v Speaker 1>than a planet made out of gravel.

0:28:39.360 --> 0:28:41.920
<v Speaker 2>But I guess generally speaking, it depends on the size

0:28:41.960 --> 0:28:44.080
<v Speaker 2>of the thing in the middle, Like the Sun has

0:28:44.120 --> 0:28:47.200
<v Speaker 2>a very big roach limit and the Earth as a

0:28:47.200 --> 0:28:47.719
<v Speaker 2>smaller one.

0:28:47.800 --> 0:28:49.920
<v Speaker 1>Yeah, that's true. You can get closer to the Earth,

0:28:50.160 --> 0:28:51.960
<v Speaker 1>then you can get to the Sun. But if you

0:28:51.960 --> 0:28:54.560
<v Speaker 1>see a moon around a planet and it's orbiting in

0:28:54.640 --> 0:28:58.040
<v Speaker 1>a circular orbit and it mostly has the same angle

0:28:58.080 --> 0:29:01.120
<v Speaker 1>or momentum as the planet, then you suspect that probably

0:29:01.280 --> 0:29:03.800
<v Speaker 1>came from the same stuff that made the planet, and

0:29:03.840 --> 0:29:06.360
<v Speaker 1>when that planet coalesced into stuff, not all of it

0:29:06.400 --> 0:29:08.920
<v Speaker 1>got turned into the planet, some of it got left

0:29:08.960 --> 0:29:12.320
<v Speaker 1>over and turned into a moon. So circular orbits with

0:29:12.400 --> 0:29:16.960
<v Speaker 1>the same anglermentum probably came from the same protoplanetary disk

0:29:17.320 --> 0:29:18.280
<v Speaker 1>that formed the planet.

0:29:19.800 --> 0:29:22.880
<v Speaker 2>Okay, So then if a moon is orbiting a planet

0:29:23.080 --> 0:29:26.800
<v Speaker 2>kind of in the same plane as the planet is spinning,

0:29:27.560 --> 0:29:30.280
<v Speaker 2>then most likely they're like siblings, kind of like they

0:29:30.320 --> 0:29:33.000
<v Speaker 2>were born at the same time from the same stuff.

0:29:33.680 --> 0:29:36.360
<v Speaker 1>Yeah, I suppose you could say so though, sort of

0:29:36.360 --> 0:29:38.520
<v Speaker 1>the scenario where like one twin is really big and

0:29:38.560 --> 0:29:39.440
<v Speaker 1>the other one is tiny.

0:29:39.560 --> 0:29:41.280
<v Speaker 2>Yeah, they're fraternal twins.

0:29:42.280 --> 0:29:44.960
<v Speaker 1>Exactly, and probably one it's pretty grumpy about not getting.

0:29:44.760 --> 0:29:46.600
<v Speaker 2>As much of dinner, all right. So that's one way

0:29:46.600 --> 0:29:49.200
<v Speaker 2>that maybe a moon can form, which is like it's

0:29:49.240 --> 0:29:51.320
<v Speaker 2>borne along with the planet, and you can sort of

0:29:51.320 --> 0:29:53.880
<v Speaker 2>tell which ones those are, Which of those do we

0:29:53.920 --> 0:29:56.120
<v Speaker 2>have in our Solar system, Like, is our moon one

0:29:56.120 --> 0:29:56.400
<v Speaker 2>of them?

0:29:56.480 --> 0:29:58.760
<v Speaker 1>Our moon is not one of those. Our moon is

0:29:58.760 --> 0:30:01.200
<v Speaker 1>actually a very weird case. Most of the moons in

0:30:01.200 --> 0:30:03.680
<v Speaker 1>the Solar System do not have nice circular orbits that

0:30:03.720 --> 0:30:05.880
<v Speaker 1>are orbiting with the planets. In fact, most of them

0:30:06.200 --> 0:30:09.600
<v Speaker 1>have elliptical orbits that have weird tilts. And that suggests

0:30:09.600 --> 0:30:11.280
<v Speaker 1>a completely different history for how.

0:30:11.160 --> 0:30:14.520
<v Speaker 2>That moon formed, necessarily, because like I wonder if maybe

0:30:14.720 --> 0:30:16.560
<v Speaker 2>the moon was formed as a sibling, but then it

0:30:16.640 --> 0:30:21.320
<v Speaker 2>got not by something and then it got a skewed orbit.

0:30:21.400 --> 0:30:24.040
<v Speaker 1>Yeah, that's certainly possible, but we think that most of

0:30:24.080 --> 0:30:27.240
<v Speaker 1>the ones with skewed orbits, that with tilted orbits that precess,

0:30:27.280 --> 0:30:31.480
<v Speaker 1>for example, are probably captured objects, things that came nearby

0:30:31.600 --> 0:30:34.479
<v Speaker 1>and were grabbed onto by the gravity of that planet.

0:30:34.560 --> 0:30:36.560
<v Speaker 1>You're right, it's possible for moon to be formed with

0:30:36.560 --> 0:30:38.760
<v Speaker 1>a planet and then get tilted through a collision. You

0:30:38.760 --> 0:30:40.680
<v Speaker 1>can tell the difference by looking at what that moon

0:30:40.760 --> 0:30:42.600
<v Speaker 1>is made out of. Is it made out of basically

0:30:42.600 --> 0:30:45.280
<v Speaker 1>the same stuff that formed the planet, or is it

0:30:45.320 --> 0:30:47.800
<v Speaker 1>made out of something totally weird and different. So that's

0:30:47.800 --> 0:30:50.640
<v Speaker 1>sort of like the key piece of information for distinguishing.

0:30:50.240 --> 0:30:53.160
<v Speaker 2>Like a DNA test prove of your siblings or not.

0:30:54.120 --> 0:30:56.800
<v Speaker 2>All right, well, then what does not having a circular

0:30:56.920 --> 0:30:58.480
<v Speaker 2>orbit tell you about the moon.

0:30:58.560 --> 0:31:01.120
<v Speaker 1>It tells you that probably it was captured, that the

0:31:01.160 --> 0:31:04.000
<v Speaker 1>planet is formed, and the moon comes from somewhere else.

0:31:04.040 --> 0:31:07.000
<v Speaker 1>It's like an asteroid or a dwarf planet or something

0:31:07.280 --> 0:31:09.640
<v Speaker 1>that was floating around and just came too close to

0:31:09.680 --> 0:31:12.560
<v Speaker 1>this massive object and its gravity took over. There's a

0:31:12.640 --> 0:31:15.360
<v Speaker 1>vicinity of a massive object we called the hill sphere,

0:31:15.360 --> 0:31:18.320
<v Speaker 1>which is the region sort of where its gravity dominates,

0:31:18.320 --> 0:31:21.520
<v Speaker 1>where everything else that's far away can basically be neglected,

0:31:21.560 --> 0:31:23.960
<v Speaker 1>and if an object passes within the hillsphere, it's a

0:31:24.000 --> 0:31:25.840
<v Speaker 1>candidate for getting captured.

0:31:26.000 --> 0:31:28.520
<v Speaker 2>But isn't that kind of weird? Or isn't it kind

0:31:28.520 --> 0:31:30.840
<v Speaker 2>of unlikely that you'll just kind of catch a big

0:31:30.960 --> 0:31:33.120
<v Speaker 2>rock out there and it'll have just the right speed

0:31:33.160 --> 0:31:35.960
<v Speaker 2>and distance to fall into a stable orbit, Like, aren't

0:31:35.960 --> 0:31:38.320
<v Speaker 2>stable orbits kind of hard to get into?

0:31:38.560 --> 0:31:40.840
<v Speaker 1>It is unlikely and it is weird. You're right. You

0:31:40.840 --> 0:31:43.520
<v Speaker 1>have to match the radius and the velocity. Like the

0:31:43.600 --> 0:31:46.080
<v Speaker 1>reason the Earth is in a stable orbit is because

0:31:46.120 --> 0:31:48.720
<v Speaker 1>it has the right velocity for our radius. You have

0:31:48.720 --> 0:31:51.560
<v Speaker 1>to be moving in a certain velocity at a given radius.

0:31:51.280 --> 0:31:53.240
<v Speaker 2>Like if we slowed down at all in our orbit,

0:31:53.280 --> 0:31:55.480
<v Speaker 2>we would start to spiral into the Sun. Right.

0:31:55.600 --> 0:31:58.600
<v Speaker 1>First orbit is actually quasi stable. So if we slowed

0:31:58.640 --> 0:32:01.640
<v Speaker 1>down a little bit, gravitational forces what actually pushes back

0:32:01.680 --> 0:32:03.920
<v Speaker 1>towards our orbit? But that's a whole other topic.

0:32:04.280 --> 0:32:05.920
<v Speaker 2>Like if you slow down a lot, though.

0:32:06.000 --> 0:32:07.720
<v Speaker 1>Yes, if we slowed down a lot, we would fall

0:32:07.760 --> 0:32:09.480
<v Speaker 1>in towards the Sun. If we sped up a bunch,

0:32:09.640 --> 0:32:12.360
<v Speaker 1>we would be ejected from the Solar system. And so

0:32:12.440 --> 0:32:14.920
<v Speaker 1>you have to have this match between these two quantities,

0:32:15.320 --> 0:32:17.680
<v Speaker 1>and it's not trivial for that to happen. Not only

0:32:17.680 --> 0:32:19.080
<v Speaker 1>do you have to have the right velocity and the

0:32:19.160 --> 0:32:21.719
<v Speaker 1>right radius, but you also have to lose energy in

0:32:21.800 --> 0:32:24.080
<v Speaker 1>order to fall into an orbit. Any object that falls

0:32:24.120 --> 0:32:27.400
<v Speaker 1>into the Solar System by definition has enough energy to

0:32:27.560 --> 0:32:30.560
<v Speaker 1>escape because it came from outside the Solar System. And

0:32:30.600 --> 0:32:33.440
<v Speaker 1>so if it just passes through on like a hyperbolic trajectory,

0:32:33.800 --> 0:32:36.440
<v Speaker 1>you know it has enough kinetic energy to climb out

0:32:36.440 --> 0:32:38.920
<v Speaker 1>of the gravitational well of the Solar System because it

0:32:38.960 --> 0:32:41.560
<v Speaker 1>came from outside the gravitational well. So in order to

0:32:41.600 --> 0:32:43.360
<v Speaker 1>get captured it not only does it have to come

0:32:43.400 --> 0:32:45.760
<v Speaker 1>in at the right radius and the right velocity, got

0:32:45.800 --> 0:32:48.280
<v Speaker 1>to lose a little bit of energy so that no

0:32:48.360 --> 0:32:50.840
<v Speaker 1>longer has the energy to escape. That can happen if

0:32:50.840 --> 0:32:53.560
<v Speaker 1>you like drag on the atmosphere the planet a little bit,

0:32:53.600 --> 0:32:55.720
<v Speaker 1>which gives you a little bit of friction, or maybe

0:32:55.720 --> 0:32:58.800
<v Speaker 1>another moon steals a little bit of your energy. So like,

0:32:58.840 --> 0:33:01.440
<v Speaker 1>the more moons you have and the puffier your atmosphere,

0:33:01.560 --> 0:33:03.920
<v Speaker 1>the more likely you are to be able to capture

0:33:03.960 --> 0:33:05.440
<v Speaker 1>an object that comes near you.

0:33:06.120 --> 0:33:09.080
<v Speaker 2>M it's kind of interesting to think of this idea

0:33:09.160 --> 0:33:11.719
<v Speaker 2>that planets like the Earth has a kind of a

0:33:11.720 --> 0:33:14.240
<v Speaker 2>halo kind of right, like a big sphere around it.

0:33:14.240 --> 0:33:17.640
<v Speaker 2>It's basically like a giant net. Like whatever falls into it,

0:33:17.640 --> 0:33:19.040
<v Speaker 2>it's gonna get sucked in.

0:33:19.400 --> 0:33:21.200
<v Speaker 1>Yeah, exactly. And if you fall in too far and

0:33:21.240 --> 0:33:23.000
<v Speaker 1>you slow don too far, then of course you're going

0:33:23.040 --> 0:33:25.600
<v Speaker 1>to burn up as you enter the atmosphere. So it's

0:33:25.600 --> 0:33:28.520
<v Speaker 1>a delicate operation. This is also think that sometimes a

0:33:28.560 --> 0:33:31.400
<v Speaker 1>pair of objects that are orbiting each other can fall

0:33:31.440 --> 0:33:33.920
<v Speaker 1>in the hillsphere and then one of them can get

0:33:33.960 --> 0:33:36.400
<v Speaker 1>captured and the other one can get ejected. So all

0:33:36.440 --> 0:33:38.800
<v Speaker 1>these sort of complicated things have to go just right

0:33:39.240 --> 0:33:41.360
<v Speaker 1>in order for a planet to capture a moon.

0:33:42.200 --> 0:33:45.520
<v Speaker 2>And by capturing, that's a nice word for stealing, right right,

0:33:45.560 --> 0:33:46.920
<v Speaker 2>I guess you're like trapping.

0:33:48.560 --> 0:33:50.720
<v Speaker 1>You're dancing, you're dancing with them, have of that?

0:33:50.880 --> 0:33:51.800
<v Speaker 2>Oh I see see?

0:33:52.160 --> 0:33:52.360
<v Speaker 3>Is that?

0:33:52.400 --> 0:33:55.480
<v Speaker 2>Where our that listener who mentioned earlier that maybe we

0:33:55.560 --> 0:33:57.840
<v Speaker 2>got our moon by stealing it from Venus? Is that?

0:33:58.120 --> 0:33:59.080
<v Speaker 2>Is there some truth to that?

0:34:00.080 --> 0:34:02.880
<v Speaker 1>We don't think that our moon was stolen from Venus,

0:34:02.880 --> 0:34:04.400
<v Speaker 1>but we do think that lots of the moons of

0:34:04.480 --> 0:34:06.920
<v Speaker 1>Jupiter and Saturn, for example, and these guys have like

0:34:07.000 --> 0:34:10.839
<v Speaker 1>dozens of moons come from scattered objects in the early

0:34:10.920 --> 0:34:14.240
<v Speaker 1>Solar system. Remember that very early on things were forming.

0:34:14.400 --> 0:34:16.560
<v Speaker 1>There may even have been more planets than the ones

0:34:16.600 --> 0:34:20.080
<v Speaker 1>we have now, and everything was quite chaotic. So now

0:34:20.080 --> 0:34:22.560
<v Speaker 1>we have sort of an orderly solar system where everything

0:34:22.640 --> 0:34:25.280
<v Speaker 1>is in place because it's been in place for so long,

0:34:25.719 --> 0:34:27.960
<v Speaker 1>and things that were not in place have been lost

0:34:28.040 --> 0:34:30.279
<v Speaker 1>or captured or fallen into the Sun. But in the

0:34:30.320 --> 0:34:32.279
<v Speaker 1>early days there were a lot of things going in

0:34:32.320 --> 0:34:35.480
<v Speaker 1>crazy orbits and crazy trajectories, and so Jupiter and Saturn

0:34:35.600 --> 0:34:37.279
<v Speaker 1>sort of like hoovered up a bunch of them.

0:34:37.560 --> 0:34:39.520
<v Speaker 2>So like, if you look at the moons of Jupiter,

0:34:39.560 --> 0:34:41.600
<v Speaker 2>for example, they're not all going to be like lined

0:34:41.640 --> 0:34:44.240
<v Speaker 2>up in a plane like our solar system. They probably

0:34:44.280 --> 0:34:46.680
<v Speaker 2>all have like crazy orbits around Jupiter.

0:34:46.760 --> 0:34:49.000
<v Speaker 1>Right, Yeah, that's exactly right, and that's why we think

0:34:49.000 --> 0:34:51.360
<v Speaker 1>that most of these were captured. Also, in the cases

0:34:51.360 --> 0:34:53.200
<v Speaker 1>that we've been able to try to study what these

0:34:53.239 --> 0:34:55.239
<v Speaker 1>moons are made out of, they're all made out of

0:34:55.280 --> 0:34:57.360
<v Speaker 1>totally different things, and so it doesn't look like they

0:34:57.480 --> 0:34:59.920
<v Speaker 1>formed from the same sort of scoop of solar systems

0:35:00.120 --> 0:35:01.879
<v Speaker 1>off that Jupiter did.

0:35:02.320 --> 0:35:03.960
<v Speaker 2>That's what you were saying, like you can check the

0:35:04.040 --> 0:35:06.720
<v Speaker 2>DNA basically the DNA of the moon and the planet

0:35:06.800 --> 0:35:08.600
<v Speaker 2>to see if they came from the same stuff, and

0:35:08.640 --> 0:35:10.080
<v Speaker 2>sometimes they don't, right.

0:35:10.640 --> 0:35:13.080
<v Speaker 1>Yeah, exactly. That's still tricky to do because we haven't

0:35:13.200 --> 0:35:15.840
<v Speaker 1>landed on those moons and like really taken samples that

0:35:15.880 --> 0:35:18.600
<v Speaker 1>we can study. But we can like do spectroscopy, we

0:35:18.600 --> 0:35:20.640
<v Speaker 1>can see the light that bounces off of them, we

0:35:20.640 --> 0:35:23.239
<v Speaker 1>can see what they emit, these kind of things. We

0:35:23.320 --> 0:35:25.640
<v Speaker 1>have done some flybys, and so we have ideas for

0:35:25.719 --> 0:35:27.719
<v Speaker 1>what these moons are probably made out of.

0:35:29.120 --> 0:35:31.520
<v Speaker 2>And in the early Solar system, like you said, things

0:35:31.560 --> 0:35:34.400
<v Speaker 2>were like there were probably like rock giant rocks flying

0:35:34.400 --> 0:35:37.279
<v Speaker 2>all over the place, and so it wouldn't be that

0:35:37.360 --> 0:35:40.360
<v Speaker 2>weird for some of them to fall into orbit around

0:35:40.600 --> 0:35:42.960
<v Speaker 2>like a passing Jupiter or Centurn. So is that how

0:35:43.000 --> 0:35:45.000
<v Speaker 2>we got our moon? Did we capture it or steal

0:35:45.000 --> 0:35:45.640
<v Speaker 2>it from somebody?

0:35:45.719 --> 0:35:47.600
<v Speaker 1>So we think our moon is unusual because it doesn't

0:35:47.640 --> 0:35:50.719
<v Speaker 1>fall into either of these categories. We don't think that

0:35:50.719 --> 0:35:53.080
<v Speaker 1>the Moon was formed with the Earth. We also don't

0:35:53.080 --> 0:35:56.800
<v Speaker 1>think that a wholly formed moon was captured by the Earth. Instead,

0:35:56.840 --> 0:35:59.239
<v Speaker 1>we think it comes from a collision. We think that

0:35:59.280 --> 0:36:02.480
<v Speaker 1>there was the proto Earth, this early planet, and then

0:36:02.480 --> 0:36:05.680
<v Speaker 1>there was another Mars like planet that came by and

0:36:05.760 --> 0:36:09.480
<v Speaker 1>smashed into the Earth, and there was this incredible collision

0:36:09.680 --> 0:36:12.440
<v Speaker 1>where essentially these two planets merged, but they left a

0:36:12.600 --> 0:36:16.360
<v Speaker 1>huge debris ring, and then that debris ring pulled together

0:36:16.680 --> 0:36:17.479
<v Speaker 1>and made the Moon.

0:36:17.719 --> 0:36:20.759
<v Speaker 2>Does our moon have an orbit that's around our equator

0:36:20.920 --> 0:36:21.640
<v Speaker 2>or is it tilted?

0:36:21.760 --> 0:36:24.360
<v Speaker 1>The Moon doesn't have a totally random orbit relatively angular

0:36:24.400 --> 0:36:27.120
<v Speaker 1>momentum of the Earth, because the two objects are essentially

0:36:27.160 --> 0:36:30.799
<v Speaker 1>formed by the combined angularmentum of this collision. So you

0:36:30.840 --> 0:36:33.200
<v Speaker 1>get this collision and basically you start from scratch. You

0:36:33.239 --> 0:36:35.600
<v Speaker 1>have a new blob of stuff which is then going

0:36:35.640 --> 0:36:38.480
<v Speaker 1>to coalesce again into a planet and a moon. And

0:36:38.520 --> 0:36:40.960
<v Speaker 1>so there is a relationship of course between the Earth's

0:36:40.960 --> 0:36:43.719
<v Speaker 1>spin and the Moon's orbit, and that's because they come

0:36:43.760 --> 0:36:46.800
<v Speaker 1>from this combined blob from this collision.

0:36:46.840 --> 0:36:49.040
<v Speaker 2>It's pretty dramatic. I think you can look up videos

0:36:49.040 --> 0:36:51.920
<v Speaker 2>of simulations of it online. It's like the Earth, the

0:36:51.960 --> 0:36:54.600
<v Speaker 2>proto Earth before Earth was just hanging out and then

0:36:54.640 --> 0:36:57.640
<v Speaker 2>this giant rock just slams into it. It all sort

0:36:57.640 --> 0:37:00.880
<v Speaker 2>of explodes together, but then gravity pulls it together into

0:37:01.200 --> 0:37:02.320
<v Speaker 2>Earth and the Moon.

0:37:02.239 --> 0:37:04.640
<v Speaker 1>Exactly, and the early Moon, we think, was much much

0:37:04.760 --> 0:37:07.480
<v Speaker 1>closer to the Earth, something like a tenth of its

0:37:07.520 --> 0:37:11.080
<v Speaker 1>current orbit, and then over time it spirals out and

0:37:11.200 --> 0:37:13.800
<v Speaker 1>ends up becoming tightly locked to the Earth. One reason

0:37:13.840 --> 0:37:15.399
<v Speaker 1>we think this is that we've been to the Moon

0:37:15.440 --> 0:37:17.480
<v Speaker 1>and we've been able to land on it and study

0:37:17.480 --> 0:37:19.680
<v Speaker 1>what it's made out of, and we see that it's

0:37:19.719 --> 0:37:21.480
<v Speaker 1>made out of a lot of stuff that's very very

0:37:21.520 --> 0:37:23.719
<v Speaker 1>similar to what the Earth is made out of, which

0:37:23.760 --> 0:37:26.200
<v Speaker 1>suggests that they do have some sort of common origin.

0:37:27.320 --> 0:37:30.400
<v Speaker 2>And does the Earth also sort of have moon like

0:37:30.840 --> 0:37:32.920
<v Speaker 2>materials in it that are not like the rest of

0:37:32.960 --> 0:37:33.360
<v Speaker 2>the Earth.

0:37:33.440 --> 0:37:34.920
<v Speaker 1>Well, we see that the Earth and the Moon have

0:37:34.960 --> 0:37:37.279
<v Speaker 1>a lot of very similar elements, which sugg they all

0:37:37.320 --> 0:37:39.920
<v Speaker 1>came from the same stuff, But the Moon has fewer

0:37:39.920 --> 0:37:42.960
<v Speaker 1>of like volatile elements things that vaporize at low temperatures

0:37:43.040 --> 0:37:45.920
<v Speaker 1>we're probably lost in this high energy event, and the

0:37:45.960 --> 0:37:48.480
<v Speaker 1>Moon has smaller gravity and so it's not able to

0:37:48.680 --> 0:37:50.719
<v Speaker 1>recapture these things the way the Earth did, so the

0:37:50.760 --> 0:37:53.360
<v Speaker 1>Earth and the Moon don't have exactly the same kinds

0:37:53.400 --> 0:37:55.680
<v Speaker 1>of stuff. The Moon also has a sort of surprisingly

0:37:55.840 --> 0:37:59.800
<v Speaker 1>small iron core which overall makes the Moon have lower density.

0:38:00.080 --> 0:38:02.560
<v Speaker 1>Simulations confirmed that this is what you would expect from

0:38:02.560 --> 0:38:05.200
<v Speaker 1>this kind of collision, that the Moon was formed more

0:38:05.280 --> 0:38:07.479
<v Speaker 1>out of the sort of external debris and the Earth

0:38:07.560 --> 0:38:10.320
<v Speaker 1>sort of got a bigger sampling of the core stuff.

0:38:11.280 --> 0:38:13.440
<v Speaker 2>I guess the Moon is also smaller, so it doesn't

0:38:13.440 --> 0:38:17.560
<v Speaker 2>have as much gravity compressing it, right, making it denser exactly.

0:38:17.960 --> 0:38:19.839
<v Speaker 1>And when they study like what's inside the Moon, they

0:38:19.880 --> 0:38:23.000
<v Speaker 1>find samples that suggest the Moon was molten down to

0:38:23.080 --> 0:38:26.240
<v Speaker 1>like a surprising depth. And you don't expect the small

0:38:26.280 --> 0:38:29.120
<v Speaker 1>body like the Moon to have the gravitational pressure to

0:38:29.320 --> 0:38:31.880
<v Speaker 1>like melt its inerts the way the Earth does. So

0:38:31.920 --> 0:38:34.040
<v Speaker 1>they think that the Moon was probably molten because of

0:38:34.080 --> 0:38:36.760
<v Speaker 1>this collision, not because of its like gravitational pressure.

0:38:37.120 --> 0:38:37.440
<v Speaker 4>Hmm.

0:38:37.640 --> 0:38:40.640
<v Speaker 2>Interesting. And I think they also found like the same

0:38:40.880 --> 0:38:43.600
<v Speaker 2>cheese inside of the Moon as some of the cheese

0:38:43.680 --> 0:38:47.000
<v Speaker 2>we have on Earth too, Right, that's part of the theory.

0:38:49.000 --> 0:38:51.560
<v Speaker 1>Yeah, they found pan pizzas rejected on the surface of

0:38:51.560 --> 0:38:52.840
<v Speaker 1>the Moon that nobody could eat.

0:38:53.000 --> 0:38:56.520
<v Speaker 2>That's right, the same mozzarella, cheese, the same cows, even

0:38:57.280 --> 0:39:00.399
<v Speaker 2>space cows. All right, well, that's the origin of our moon.

0:39:00.520 --> 0:39:03.360
<v Speaker 2>Let's get a little bit into what that means about

0:39:03.400 --> 0:39:07.279
<v Speaker 2>the formation of all moons and the formation of our

0:39:07.320 --> 0:39:10.279
<v Speaker 2>whole Solar system, why we're here, and why are things

0:39:10.320 --> 0:39:12.880
<v Speaker 2>the way they are. But first, let's take another quick break.

0:39:25.600 --> 0:39:27.799
<v Speaker 2>All right, we are coming face to face with the

0:39:28.000 --> 0:39:31.440
<v Speaker 2>lunacy here in the podcast talking about the origin of

0:39:31.520 --> 0:39:35.440
<v Speaker 2>moons and in particular our moon. You're saying, it's interesting because,

0:39:35.719 --> 0:39:37.839
<v Speaker 2>like our moon is sort of a combination of how

0:39:37.920 --> 0:39:40.520
<v Speaker 2>some of these other moons can form. Right, Like, we

0:39:40.600 --> 0:39:43.040
<v Speaker 2>had a proto planet Earth, and when there was a

0:39:43.160 --> 0:39:47.080
<v Speaker 2>visitor that was flying around came near us, it sort

0:39:47.080 --> 0:39:49.400
<v Speaker 2>of got captured or collided with our Earth, and then

0:39:49.440 --> 0:39:51.680
<v Speaker 2>it all became a big mess. And out of that mess,

0:39:52.280 --> 0:39:54.360
<v Speaker 2>you know, the Earth and the Moon forms sort of

0:39:54.400 --> 0:39:58.400
<v Speaker 2>a siblings, but also not siblings, because there was it

0:39:58.480 --> 0:40:01.000
<v Speaker 2>came from a different planet. The stuff.

0:40:01.120 --> 0:40:03.799
<v Speaker 1>There was a big fight early on, and we were left

0:40:03.800 --> 0:40:06.279
<v Speaker 1>over cleaning up the mess. Yeah, it is really fascinating,

0:40:06.320 --> 0:40:09.000
<v Speaker 1>and I love this sort of archaeology, this like detective

0:40:09.040 --> 0:40:13.280
<v Speaker 1>story figuring out what happened billions of years ago, reconstructing

0:40:13.280 --> 0:40:15.279
<v Speaker 1>the story from the clues that are left behind, these

0:40:15.320 --> 0:40:17.919
<v Speaker 1>really subtle hints. You know, why does the Moon seem

0:40:17.960 --> 0:40:19.560
<v Speaker 1>to be made of the same stuff as the Earth,

0:40:19.560 --> 0:40:22.040
<v Speaker 1>but it doesn't have sort of a close circular orbit

0:40:22.040 --> 0:40:24.480
<v Speaker 1>the way you would expect. Why exactly is it so big?

0:40:24.719 --> 0:40:27.719
<v Speaker 1>These stories are really fascinating because we missed so much

0:40:27.760 --> 0:40:29.960
<v Speaker 1>of the Solar System history. You know, like billions of

0:40:30.120 --> 0:40:33.440
<v Speaker 1>years happened with crazy fireworks in the sky and we

0:40:33.440 --> 0:40:35.520
<v Speaker 1>weren't here to look at it. But we can still

0:40:35.520 --> 0:40:36.840
<v Speaker 1>get hints about what happened.

0:40:37.040 --> 0:40:39.759
<v Speaker 2>Hmmm, do you think that's an official job title out there,

0:40:39.760 --> 0:40:42.000
<v Speaker 2>like space archaeologists.

0:40:42.760 --> 0:40:46.000
<v Speaker 1>Space murder mystery, you know, exactly.

0:40:45.800 --> 0:40:49.400
<v Speaker 2>Give me like Indiana solo a combination of Indiana Jones

0:40:49.480 --> 0:40:50.240
<v Speaker 2>and Hands solo.

0:40:51.600 --> 0:40:54.359
<v Speaker 1>And you know, we're still learning stuff about moons, like

0:40:54.560 --> 0:40:57.719
<v Speaker 1>Mars has some funny moons, Phobos and Demos, And the

0:40:57.800 --> 0:41:01.319
<v Speaker 1>smaller of those two moons, Demos, is really tiny. It's

0:41:01.360 --> 0:41:04.800
<v Speaker 1>only like nine miles across, has a really weird shorwt

0:41:04.800 --> 0:41:07.160
<v Speaker 1>of blobby shape to it, and for a long time

0:41:07.160 --> 0:41:10.239
<v Speaker 1>people thought it was probably a captured asteroid because of

0:41:10.280 --> 0:41:13.359
<v Speaker 1>its orbit, but they recently send an orbiter very very

0:41:13.360 --> 0:41:16.160
<v Speaker 1>close to it, super close approach by this spacecraft from

0:41:16.160 --> 0:41:18.839
<v Speaker 1>the UA Emirates. Actually it's called Hope, and they were

0:41:18.840 --> 0:41:21.240
<v Speaker 1>able to study what it's made out of and discover

0:41:21.400 --> 0:41:24.440
<v Speaker 1>that it has sort of the same carbon and organics

0:41:24.480 --> 0:41:27.680
<v Speaker 1>that Mars does, unlike the asteroids, sort of like the

0:41:27.800 --> 0:41:30.640
<v Speaker 1>DNA test you were saying before, which means that Demos

0:41:30.680 --> 0:41:34.600
<v Speaker 1>probably is a chunk of Mars that got blown off

0:41:34.719 --> 0:41:36.480
<v Speaker 1>in some sort of prehistoric collision.

0:41:36.600 --> 0:41:38.400
<v Speaker 2>Isn't that also kind of the theey of how we

0:41:38.440 --> 0:41:41.360
<v Speaker 2>got life on Earth, like a possible way that maybe

0:41:41.400 --> 0:41:43.480
<v Speaker 2>Mars got hit by something. It threw a bunch of

0:41:43.600 --> 0:41:46.279
<v Speaker 2>rocks out into space. Some of them became Demos, the

0:41:46.320 --> 0:41:48.360
<v Speaker 2>moon of Mars, and maybe some of them came to

0:41:48.400 --> 0:41:50.240
<v Speaker 2>Earth bringing like little bacteria.

0:41:50.280 --> 0:41:53.880
<v Speaker 1>Perhaps we're very sure that rocks from Mars have landed

0:41:53.920 --> 0:41:56.320
<v Speaker 1>on Earth. We have found them and their geology matches

0:41:56.360 --> 0:41:59.160
<v Speaker 1>Mars and doesn't match Earth. So there's no controversy about

0:41:59.160 --> 0:42:03.000
<v Speaker 1>whether visions from asteroids on planets can knock stuff off

0:42:03.000 --> 0:42:05.320
<v Speaker 1>into outer space and have it land on other planets.

0:42:05.440 --> 0:42:08.120
<v Speaker 1>Whether there's life in those rocks that then seeded life

0:42:08.160 --> 0:42:12.120
<v Speaker 1>on Earth totally open question. There was this famous misdiscovery

0:42:12.400 --> 0:42:14.959
<v Speaker 1>about twenty years ago when they found these weird little

0:42:15.000 --> 0:42:18.000
<v Speaker 1>shapes inside a Martian rock on Earth, and they made

0:42:18.000 --> 0:42:20.319
<v Speaker 1>this announcement that they were certain that there was life

0:42:20.320 --> 0:42:23.000
<v Speaker 1>in them, that these shapes could only be made by life.

0:42:23.160 --> 0:42:25.960
<v Speaker 1>But then later analysis demonstrated that you could make those

0:42:25.960 --> 0:42:29.399
<v Speaker 1>things without life. So there's no concrete proof that life

0:42:29.440 --> 0:42:32.840
<v Speaker 1>has traveled between planets on an asteroid, but it's totally

0:42:32.920 --> 0:42:35.799
<v Speaker 1>possible for it to happen. And Demos definitely is a

0:42:35.920 --> 0:42:38.680
<v Speaker 1>chunk of Mars floating in space. Sort of like if

0:42:38.680 --> 0:42:40.960
<v Speaker 1>you went out into space and you found like Manhattan

0:42:41.239 --> 0:42:43.759
<v Speaker 1>floating out in space, you'd be like, whoa, Where'd this

0:42:43.800 --> 0:42:44.280
<v Speaker 1>come from?

0:42:44.520 --> 0:42:45.920
<v Speaker 2>Yeah, well people wonder about that.

0:42:46.640 --> 0:42:50.879
<v Speaker 1>Now, what's the story? How did Manhattan get so weird?

0:42:50.880 --> 0:42:53.799
<v Speaker 2>Where did New Yorkers come from their lunatics?

0:42:53.880 --> 0:42:56.319
<v Speaker 1>But they have the best pizza, right, so I don't

0:42:56.360 --> 0:42:57.560
<v Speaker 1>want to have to go out of space to get

0:42:57.600 --> 0:42:59.480
<v Speaker 1>my pizza.

0:43:00.200 --> 0:43:02.839
<v Speaker 2>You just insulted everyone in Chicago. He lost a big

0:43:02.920 --> 0:43:03.960
<v Speaker 2>chunk of our listenership.

0:43:04.080 --> 0:43:06.520
<v Speaker 1>I love Chicago, I love Chicago wins, and I love

0:43:06.560 --> 0:43:09.239
<v Speaker 1>the Chicagoans love Chicago pizza. That's all fine with me.

0:43:09.480 --> 0:43:11.640
<v Speaker 2>All right, Well, what does all of this tells about

0:43:11.680 --> 0:43:14.319
<v Speaker 2>the formation of the Solar System and how we ended

0:43:14.400 --> 0:43:16.200
<v Speaker 2>up where we are and how we are.

0:43:16.440 --> 0:43:18.320
<v Speaker 1>It's a story that we are still unraveling.

0:43:18.400 --> 0:43:18.520
<v Speaker 5>Right.

0:43:18.560 --> 0:43:21.080
<v Speaker 1>We're still learning about our moon, We're still learning about

0:43:21.080 --> 0:43:25.520
<v Speaker 1>our neighbor's moons. We're still discovering moons. Right. Saturn recently

0:43:25.560 --> 0:43:28.160
<v Speaker 1>past Jupiter. I think in the number of moons that

0:43:28.239 --> 0:43:30.799
<v Speaker 1>it has, each one tells us a little bit of

0:43:30.840 --> 0:43:33.160
<v Speaker 1>the story of the Solar system, and what we're looking

0:43:33.200 --> 0:43:35.799
<v Speaker 1>for now are like more details for that story. As

0:43:35.840 --> 0:43:39.560
<v Speaker 1>you said earlier, we're asking questions like can moons have moons?

0:43:39.800 --> 0:43:42.120
<v Speaker 1>A lot of people think that it's impossible for the

0:43:42.120 --> 0:43:44.600
<v Speaker 1>same reason that like Mercury and Venus don't have moons

0:43:44.719 --> 0:43:47.600
<v Speaker 1>from the tidal forces of the Sun, that Jupiter's moons

0:43:47.640 --> 0:43:50.120
<v Speaker 1>probably can't have their own moons because of the tidal

0:43:50.200 --> 0:43:53.840
<v Speaker 1>forces of Jupiter. But you know, Saturn's moon Rhea probably

0:43:53.840 --> 0:43:57.640
<v Speaker 1>has rings which even though they're disrupted by the title forces,

0:43:57.719 --> 0:44:00.479
<v Speaker 1>they can still be in orbit around Rhea. And there's

0:44:00.560 --> 0:44:03.560
<v Speaker 1>like hundreds of minor planets deep out there in the

0:44:03.560 --> 0:44:06.440
<v Speaker 1>Solar system that do have their own moons, like Pluto.

0:44:06.600 --> 0:44:09.280
<v Speaker 1>But beyond that, we're also looking into other solar systems

0:44:09.320 --> 0:44:11.480
<v Speaker 1>to try to understand whether the moons that we have

0:44:11.800 --> 0:44:15.359
<v Speaker 1>are weird or typical? Right, Like, we only so far

0:44:15.520 --> 0:44:18.000
<v Speaker 1>have this one solar system to study at this level

0:44:18.040 --> 0:44:20.160
<v Speaker 1>of detail. Twenty years ago, we were able to see

0:44:20.200 --> 0:44:22.759
<v Speaker 1>planets around other stars, which tells us a lot about

0:44:22.760 --> 0:44:25.560
<v Speaker 1>whether the planets in our solar systems are weird. Now

0:44:25.560 --> 0:44:28.160
<v Speaker 1>we're pushing those boundaries to try to look for moons

0:44:28.280 --> 0:44:32.480
<v Speaker 1>in other solar systems. This thing we call exo moons

0:44:32.520 --> 0:44:34.800
<v Speaker 1>to try to discover if the distribution of moons that

0:44:34.840 --> 0:44:38.440
<v Speaker 1>we have is strange or pretty typical in the universe.

0:44:38.520 --> 0:44:40.640
<v Speaker 2>Well, that's wild. How are we seeing moons and other

0:44:40.680 --> 0:44:43.839
<v Speaker 2>planets outside of our solar system? Can we see them

0:44:43.920 --> 0:44:46.280
<v Speaker 2>or do we have to infer them from the gravity.

0:44:46.560 --> 0:44:48.840
<v Speaker 1>So there's a few ways that we discover planets, and

0:44:48.880 --> 0:44:51.680
<v Speaker 1>we can try to apply those ways to discover moons.

0:44:51.960 --> 0:44:54.839
<v Speaker 1>One of the early ways we discovered planets around other

0:44:54.880 --> 0:44:58.640
<v Speaker 1>stars was seeing their gravitational impact on the star, and

0:44:58.680 --> 0:45:01.280
<v Speaker 1>that would wiggle the star and cause like a change

0:45:01.320 --> 0:45:04.080
<v Speaker 1>in the frequency of the light, this Doppler shift, and

0:45:04.120 --> 0:45:06.160
<v Speaker 1>so we could discover that there was something pulling on

0:45:06.239 --> 0:45:08.480
<v Speaker 1>that star. We don't think that method will work for

0:45:08.600 --> 0:45:11.480
<v Speaker 1>discovering moons because it's really hard to distinguish the gravitational

0:45:11.520 --> 0:45:13.560
<v Speaker 1>effect of a little moon around a planet from the

0:45:13.560 --> 0:45:16.120
<v Speaker 1>planet itself. What we do think is possible is the

0:45:16.200 --> 0:45:20.000
<v Speaker 1>transit method, this eclipse method, where a planet passes in

0:45:20.000 --> 0:45:22.000
<v Speaker 1>front of a star and dips the light that comes

0:45:22.040 --> 0:45:24.239
<v Speaker 1>from it, And if that happens in a regular way,

0:45:24.320 --> 0:45:27.600
<v Speaker 1>we can tell that these little microeclipses come from a planet. Well,

0:45:27.600 --> 0:45:29.960
<v Speaker 1>if those eclipses have their own little dips in them,

0:45:30.280 --> 0:45:33.719
<v Speaker 1>because the moon going around the planet sometimes blocks this

0:45:33.880 --> 0:45:36.480
<v Speaker 1>life from the star and sometimes doesn't, then you can

0:45:36.520 --> 0:45:42.000
<v Speaker 1>discover moons around those planets. So like microeclipses within microeclipses.

0:45:42.120 --> 0:45:45.200
<v Speaker 2>Wow, exo eclipses exo exo moon eclipses.

0:45:45.320 --> 0:45:47.919
<v Speaker 1>Yeah, they're like eclipses squared. And we don't have any

0:45:47.960 --> 0:45:50.680
<v Speaker 1>confirmed exo moons yet, though there are a couple of

0:45:50.719 --> 0:45:54.480
<v Speaker 1>candidates from the Kepler telescope that look promising, but people

0:45:54.480 --> 0:45:58.279
<v Speaker 1>can't yet agree whether that actually is the discovery of

0:45:58.320 --> 0:46:01.920
<v Speaker 1>a moon. And more recently, we've developed this incredible technology

0:46:01.960 --> 0:46:05.280
<v Speaker 1>to do direct imaging of exoplanets, like telescopes that actually

0:46:05.360 --> 0:46:09.440
<v Speaker 1>take pictures of planets around other stars. Blows my mind.

0:46:09.480 --> 0:46:11.560
<v Speaker 1>I never thought that would be possible. A lot of

0:46:11.560 --> 0:46:13.960
<v Speaker 1>it involves like blocking out the light from the star

0:46:14.040 --> 0:46:16.440
<v Speaker 1>itself so you can see the ring around it. And

0:46:16.480 --> 0:46:19.799
<v Speaker 1>sometimes that lets us see planets being formed. So we

0:46:19.800 --> 0:46:22.439
<v Speaker 1>can see, for example, a star with a planetary disc

0:46:22.560 --> 0:46:24.960
<v Speaker 1>around it. And in one case we have a direct

0:46:25.040 --> 0:46:28.520
<v Speaker 1>image of a protoplanetary disc which seems to have a

0:46:28.560 --> 0:46:31.520
<v Speaker 1>planet with its own disc around it. So like you

0:46:31.520 --> 0:46:33.480
<v Speaker 1>can see the planet and it's got like a bunch

0:46:33.480 --> 0:46:36.040
<v Speaker 1>of stuff around it, and maybe that stuff will form

0:46:36.080 --> 0:46:36.680
<v Speaker 1>into a moon.

0:46:37.920 --> 0:46:39.040
<v Speaker 2>You can see the rings in it.

0:46:39.239 --> 0:46:41.520
<v Speaker 1>Yeah, exactly. You can see this disc that's going to

0:46:41.640 --> 0:46:44.200
<v Speaker 1>form it either into rings or moons or something.

0:46:44.280 --> 0:46:46.359
<v Speaker 2>Yeah, it's pretty mind blowing because I wonder like if

0:46:46.360 --> 0:46:48.040
<v Speaker 2>a lot of people know that you can actually see

0:46:48.040 --> 0:46:50.279
<v Speaker 2>the moons of Jupiter kind of with your naked eye,

0:46:50.360 --> 0:46:52.319
<v Speaker 2>or at least with a small telescope. You don't need

0:46:52.360 --> 0:46:54.399
<v Speaker 2>like a super amazing telescope. You can just use something

0:46:54.400 --> 0:46:55.839
<v Speaker 2>you can buy for your house and you can see

0:46:55.840 --> 0:46:56.640
<v Speaker 2>the moons of Jupiter.

0:46:56.719 --> 0:46:58.960
<v Speaker 1>Yeah, it doesn't take a fancy telescope. It was one

0:46:59.000 --> 0:47:01.040
<v Speaker 1>of the first things that Galla saw when he pointed

0:47:01.040 --> 0:47:02.799
<v Speaker 1>a telescope at the sky. It was one of the

0:47:02.800 --> 0:47:04.560
<v Speaker 1>first people to ever do this, and he saw the

0:47:04.640 --> 0:47:06.640
<v Speaker 1>moons of Jupiter. It's not hard. You can do it,

0:47:06.640 --> 0:47:09.520
<v Speaker 1>and it's pretty exciting to see Jupiter expand from this

0:47:09.640 --> 0:47:11.799
<v Speaker 1>tiny dot you can see with the naked eye to

0:47:11.920 --> 0:47:14.480
<v Speaker 1>this whole orbital system with its own dynamics.

0:47:14.840 --> 0:47:18.200
<v Speaker 2>H pretty cool. All right. Well, one thing that's day

0:47:18.200 --> 0:47:20.560
<v Speaker 2>announced recently is that we're sending more people to the Moon.

0:47:20.719 --> 0:47:22.960
<v Speaker 1>That's right, if Elon Musk ever gets that starship off

0:47:23.000 --> 0:47:23.400
<v Speaker 1>the ground.

0:47:23.520 --> 0:47:26.319
<v Speaker 2>No, the new artem is missions right, It isn't one

0:47:26.360 --> 0:47:27.920
<v Speaker 2>of the plants to send more people to the moon.

0:47:28.040 --> 0:47:30.040
<v Speaker 1>Yeah, that's exciting. It'd be cool to go back to

0:47:30.080 --> 0:47:32.279
<v Speaker 1>the Moon. With all of our advanced technology, we can

0:47:32.440 --> 0:47:35.360
<v Speaker 1>take more detailed measurements. We can map its magnetic field,

0:47:35.400 --> 0:47:38.399
<v Speaker 1>we can understand its geology and its history even better. Yeah.

0:47:38.440 --> 0:47:40.200
<v Speaker 2>I wonder why kind of pizza they would eat there though?

0:47:40.880 --> 0:47:43.520
<v Speaker 2>It's a deep dish because there's not much that much gravity.

0:47:43.560 --> 0:47:45.160
<v Speaker 2>So can you have a deep dish pizza?

0:47:46.000 --> 0:47:48.279
<v Speaker 1>Probably every pizza would rise a lot more because there

0:47:48.280 --> 0:47:49.400
<v Speaker 1>isn't gravity, right.

0:47:49.320 --> 0:47:51.480
<v Speaker 2>Oh, my goodness. In space, every pizza is a deep

0:47:51.520 --> 0:47:53.719
<v Speaker 2>dish pizza. That's why you're not going to Earth.

0:47:53.840 --> 0:47:57.080
<v Speaker 1>Danu or maybe astronaut pizza is just freeze dried and

0:47:57.120 --> 0:48:00.880
<v Speaker 1>gross no matter where it comes from.

0:48:01.239 --> 0:48:03.239
<v Speaker 2>I guess there's something one way to find out to

0:48:03.280 --> 0:48:06.799
<v Speaker 2>take the podcast to space. All right, Well that kind

0:48:06.800 --> 0:48:09.480
<v Speaker 2>of answers our question. How the Moon's form basically two

0:48:09.520 --> 0:48:13.360
<v Speaker 2>main ways, right, They either capture something flying by in space,

0:48:13.600 --> 0:48:16.480
<v Speaker 2>or they form together with the planet, or some combination

0:48:16.560 --> 0:48:20.319
<v Speaker 2>of the tube where something comes from space crashes into you,

0:48:20.560 --> 0:48:22.880
<v Speaker 2>creates a big mess, and then you both sort of

0:48:22.920 --> 0:48:24.640
<v Speaker 2>form together or reform together.

0:48:24.800 --> 0:48:26.880
<v Speaker 1>And the incredible thing is that by looking at the

0:48:26.880 --> 0:48:29.840
<v Speaker 1>Moon today we can mostly figure out how that happened,

0:48:29.840 --> 0:48:32.160
<v Speaker 1>how this huge space rock ended up in orbit around

0:48:32.200 --> 0:48:33.160
<v Speaker 1>the planet. Yeah.

0:48:33.160 --> 0:48:34.680
<v Speaker 2>And the cool thing is that you can see the

0:48:34.719 --> 0:48:37.000
<v Speaker 2>Moon almost every night. Every night you step outside of

0:48:37.000 --> 0:48:39.840
<v Speaker 2>your house, you can see this giant rock floating in

0:48:39.920 --> 0:48:43.319
<v Speaker 2>space there for us to see, pretty shiny, pretty bright.

0:48:44.560 --> 0:48:47.240
<v Speaker 1>It's nice to have one big, fat moon. I agree.

0:48:47.480 --> 0:48:49.799
<v Speaker 2>All right, Well, we hope you enjoyed that. Thanks for

0:48:49.880 --> 0:48:51.680
<v Speaker 2>joining us, See you next time.

0:48:59.480 --> 0:49:02.360
<v Speaker 1>Thanks for listening, and remember that Daniel and Jorge Explain

0:49:02.400 --> 0:49:06.399
<v Speaker 1>the Universe is a production of iHeartRadio. For more podcasts

0:49:06.400 --> 0:49:11.080
<v Speaker 1>from iHeartRadio, visit the iHeartRadio, app, Apple podcasts, or wherever

0:49:11.120 --> 0:49:12.840
<v Speaker 1>you listen to your favorite shows.