WEBVTT - Which planet has the most moons?

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<v Speaker 1>The Moon really doesn't get enough love. Of all of

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<v Speaker 1>the features of the night sky. It's the only one

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<v Speaker 1>with real texture visible to the naked eye. Everything else

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<v Speaker 1>is either just a tiny distant point or an overwhelming

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<v Speaker 1>ball of fire. There's nothing else out there that you

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<v Speaker 1>can just sit and stare at and appreciate the feeling

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<v Speaker 1>of looking through a gulf in space. We are here

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<v Speaker 1>on a rock in space, and there's another whole rock

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<v Speaker 1>right over there, so far away yet so weirdly big,

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<v Speaker 1>that we can see it and see features on it.

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<v Speaker 1>It challenges the mind, forcing you to come to griffs

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<v Speaker 1>with our cosmic context of massive balls of rock spinning

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<v Speaker 1>through a dark ocean. And there's so much more that

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<v Speaker 1>moons do. Moons tell us about the history of the

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<v Speaker 1>Solar System and help reveal what's going on inside their planets.

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<v Speaker 1>They have volcanoes and weird colors and shoot jets of

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<v Speaker 1>water into space. They might even harbor life. Seeing Jupiter's

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<v Speaker 1>moons is what led Galileo to understand the structure of

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<v Speaker 1>our Solar system. And the thing that our moon has

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<v Speaker 1>misled us about is their number. Having one big, fat

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<v Speaker 1>moon is not normal planets, and our Solar system have

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<v Speaker 1>many moons, so many fabulous moons. So on this episode,

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<v Speaker 1>we're going to give moons the love they deserve. Welcome

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<v Speaker 1>to Daniel and Kelly's Extraordinary moon Malicious Universe.

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<v Speaker 2>Hello. I'm Kelly Waitersmith. I study parasites and space, and

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<v Speaker 2>I am not above jokes that involve mooning.

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<v Speaker 1>Hiel, I'm a particle physicist, and I can't tell you

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<v Speaker 1>how long it's been since I mooned somebody.

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<v Speaker 2>Oh, yes, that was a joy to hear about mooning

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<v Speaker 2>jokes when I was a kid. I don't remember actually

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<v Speaker 2>mooning anyone in my teens. I was a bit of

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<v Speaker 2>an insecure teen. But but ah, yes, I remember being

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<v Speaker 2>mooned as.

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<v Speaker 1>A teen and as an adult. Kelly, can I ask

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<v Speaker 1>you how long has it been since you mooned anybody?

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<v Speaker 2>I plead the fifth I married a man whose last

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<v Speaker 2>name is Wiener, and so my sense of humor has

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<v Speaker 2>become a bit more juvenile.

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<v Speaker 1>Fill in the gaps yourself, everybody, that's.

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<v Speaker 2>Right answer, Daniel. My question for you is, so today

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<v Speaker 2>we are talking about moons. Have you ever heard of

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<v Speaker 2>a convincing story of the moon influencing someone's behavior? Oh?

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<v Speaker 1>I mean, I can imagine the moon influencing the tides,

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<v Speaker 1>and the tides definitely influence people, m h.

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<v Speaker 2>But you don't buy the like, you know, more people

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<v Speaker 2>come into the er on a full moon.

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<v Speaker 1>People do all all sorts of weird stuff, and I

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<v Speaker 1>wouldn't be surprised if people acted weirder on a full

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<v Speaker 1>moon and there were more visits to the er. So

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<v Speaker 1>I'm gonna have to play the fifth on that one.

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<v Speaker 2>Yeah, I mean, I don't think I buy that people

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<v Speaker 2>are like more kooky on full moon nights unless they

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<v Speaker 2>have been convinced that they ought to be more like

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<v Speaker 2>risk taking on full moon nights and it's on their

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<v Speaker 2>mind than I can imagine like they sort of have

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<v Speaker 2>psyched themselves out. But I do like, if I get

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<v Speaker 2>up early in the morning and it's brighter because of

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<v Speaker 2>a full moon, I'll be more likely to like go

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<v Speaker 2>jogging or something. And so I can imagine maybe people

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<v Speaker 2>going out and doing more stuff outside during a full

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<v Speaker 2>moon and maybe being more likely to like accidentally get

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<v Speaker 2>hit by a car or something like that. And of

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<v Speaker 2>course we were talking about how some organisms are influenced

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<v Speaker 2>by the tide and so their's circadian rhythms are influenced

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<v Speaker 2>by the tide, so their behaviors are influenced by the tide.

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<v Speaker 2>But yeah, I don't think I buy that animals or

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<v Speaker 2>people are more likely to be doing kooky crazy stuff

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<v Speaker 2>because it's a full moon or anything like that.

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<v Speaker 1>But I don't know. People are weird, and I think

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<v Speaker 1>if you work in an er, you see the weirdest

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<v Speaker 1>side of people. I remember Katrina worked at a hospital

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<v Speaker 1>in Geneva, and near the entrance they had a huge

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<v Speaker 1>display of the weirdest stuff they had pulled out of

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<v Speaker 1>people's throats and other holes. Oh no, and boy was

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<v Speaker 1>there some weird stuff there.

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<v Speaker 2>Oh. I did once for a research project look for

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<v Speaker 2>papers describing things that had been pulled from orifices. And

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<v Speaker 2>we are an inventive species, and if it turns out

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<v Speaker 2>that our inventive behaviors are tied to full moons, then

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<v Speaker 2>we might be happy that we have only one moon

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<v Speaker 2>and not many moons.

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<v Speaker 1>And the moon figures so prominently in the sky and

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<v Speaker 1>in our literature and in our imaginations that it's easy

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<v Speaker 1>to imagine that aliens would look up to their sky

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<v Speaker 1>and see the same thing. Or if you're a science

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<v Speaker 1>fiction off third to imagine alien seeing a radically different sky,

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<v Speaker 1>many moons, or something similarly weird. And there are lots

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<v Speaker 1>of examples in science fiction of multiple suns or multiple

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<v Speaker 1>moons or other variations on our experience, but you don't

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<v Speaker 1>actually have to go that far visiting another solar system

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<v Speaker 1>to see examples of multiple moons.

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<v Speaker 2>And if I can just plug my friend's book for

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<v Speaker 2>a second, Under Alien Skies by Phil Plait is an

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<v Speaker 2>amazing book describing what might be like to visit alien

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<v Speaker 2>planets and look at their skies. And Phil was a

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<v Speaker 2>guest on our show early on when you and I

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<v Speaker 2>started podcasting together.

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<v Speaker 1>That's right, and everything he writes is insightful, well informed,

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<v Speaker 1>and fun, so go check it out.

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<v Speaker 2>Yes, all right, so you asked our extraordinaries which planet

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<v Speaker 2>has the most moons?

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<v Speaker 1>That's right, And if you would like to contribute for

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<v Speaker 1>this segment of the show in future episodes, please don't

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<v Speaker 1>be shy. We would love to add your voice to

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<v Speaker 1>the chorus. In the meantime, think about it for yourself

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<v Speaker 1>for a moment. Which planet in our solar system do

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<v Speaker 1>you think has the most moons? Here's what the extraordinaries

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<v Speaker 1>had to say.

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<v Speaker 3>And believe it's Jupiter. That has the most moons. I

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<v Speaker 3>think they just discovered a couple more, But technically really

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<v Speaker 3>depends on what you define as moon, because rings are

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<v Speaker 3>just particles orbiting the planet as well. In our Solar system,

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<v Speaker 3>the planet with the most moons is probably Saturn.

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<v Speaker 1>Outside of the Solar System, I have no clue.

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<v Speaker 3>I would say Jupiter because of how big it is,

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<v Speaker 3>but then it might have pulled some moons into it,

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<v Speaker 3>So maybe Saturn has the most because it sits in

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<v Speaker 3>a sweet spot.

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<v Speaker 1>What do you think, glenn on? Going straight for Jupiter? Why?

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<v Speaker 1>Because it has the most moons? All right?

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<v Speaker 3>My initial thought would be Saturn or Jupiter, but I

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<v Speaker 3>have been reading recent news reports about many new discoveries

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<v Speaker 3>of moons around Jupiter, so I'm going to go with Jupiter.

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<v Speaker 1>All right, So most votes for Jupiter. Kelly. If you

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<v Speaker 1>hadn't read the outline, what would you have done?

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<v Speaker 2>Cod Ah, I love that you think that I read

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<v Speaker 2>the outline.

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<v Speaker 1>Giving you the benefit of the doubt here just in case.

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<v Speaker 2>No, I'm kidding. I did read the outline, so I

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<v Speaker 2>would have guessed Saturn or Jupiter, or I would have

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<v Speaker 2>guessed that because this is a dKu episode, maybe the

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<v Speaker 2>answer is we don't know, because maybe maybe it's hard

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<v Speaker 2>to count all the moons and we aren't sure if

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<v Speaker 2>Saturn or Jupiter is the winner.

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<v Speaker 1>Yet that's probably the right answer. Actually, Also it depends

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<v Speaker 1>on what you mean by moon, the definition, which is

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<v Speaker 1>always evolving as we discover more stuff out there in

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<v Speaker 1>the Solar system, because though humans like to make tidy

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<v Speaker 1>categories for the things that are orbiting the Sun, in

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<v Speaker 1>reality the universe is chaotic and there's just like a

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<v Speaker 1>huge smooth spectrum of stuff from tiny little dust grains

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<v Speaker 1>all the way up to Jupiter and basically everything in between.

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<v Speaker 1>And if you try to put everything in boxes and

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<v Speaker 1>make artificial dotted lines to separate it, you'll find a

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<v Speaker 1>bunch of stuff in fuzzy category and you'll argue about

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<v Speaker 1>whether it's a moon or whether it's not a moon,

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<v Speaker 1>and that will probably change the answer.

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<v Speaker 2>Well, at least that's a bit more satisfying than like

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<v Speaker 2>our discussion on the ort cloud, where you're like, actually,

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<v Speaker 2>we're not even really sure there's an ork cloud, and

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<v Speaker 2>so you know, I was a little worried you we

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<v Speaker 2>were going to be like, actually, we're not even sure

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<v Speaker 2>that there's moons that could be an optical illusion. But anyway, Okay,

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<v Speaker 2>we're sure that there's moons. We're not quite sure where

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<v Speaker 2>the cutoff should be, but we've arbitrarily said it somewhere.

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<v Speaker 1>Yeah, exactly. So first let's clarify what we mean by

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<v Speaker 1>a moon. And this has a fascinating history, even just

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<v Speaker 1>the word is fairly recent and modern. Astronomically, the category

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<v Speaker 1>officially is natural satellite, and we use the word moon

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<v Speaker 1>sort of colloquially after the moon of Earth. Historically, people

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<v Speaker 1>called our moon a planet, like until Copernicus in fifteen hundred,

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<v Speaker 1>the term planet was basically used to describe like things

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<v Speaker 1>that move in the sky, which we assume to move

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<v Speaker 1>around the Earth, and the moon was just like another thing,

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<v Speaker 1>like the other planets, and like the Sun that people

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<v Speaker 1>assumed moved around the Earth. Then, of course Galileo saw

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<v Speaker 1>the moons of Jupiter and thought, ooh, the planets themselves

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<v Speaker 1>are like mini systems, and so you can have this

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<v Speaker 1>hierarchical structure, and so it's not required for everything to

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<v Speaker 1>orbit one thing or to orbit the Earth, and so

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<v Speaker 1>that gives way to a more nuanced structure of the

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<v Speaker 1>Solar System. And now you have to have different words

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<v Speaker 1>to define these things that are not directly orbiting the sun,

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<v Speaker 1>but are orbiting something that is orbiting the sun.

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<v Speaker 2>Okay, now, hold on, So recently you asked me what

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<v Speaker 2>killyfish means, and then you ask me what hymenopterin means.

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<v Speaker 1>Oh no, are we about to get some linguistic revenge?

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<v Speaker 2>Gosh? I hope so, because usually when I'm like, oh,

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<v Speaker 2>I'm about to get Daniel, You're like, oh, because Daniel

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<v Speaker 2>just knows. But I see you're about to hit your keyboard.

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<v Speaker 2>Does the word moon mean something? Did they take that

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<v Speaker 2>from something else? Yes?

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<v Speaker 1>Yes, so you know, the Latin name for the moon

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<v Speaker 1>is Luna. But the word moon itself actually comes from

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<v Speaker 1>the Old English word, which comes from a Germanic word,

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<v Speaker 1>which comes from a Proto Indo European word which might

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<v Speaker 1>be related to the measurement of time. And so yes,

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<v Speaker 1>the moon has this like ancient historical meaning connected with,

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<v Speaker 1>you know, the passage of time. And that's super fun

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<v Speaker 1>because we know that, like looking at patterns in the

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<v Speaker 1>sky is how a lot of ancient peoples first developed

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<v Speaker 1>like astronomy and mathematics and you know, trying to predict

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<v Speaker 1>the future. So it's like a deep rabbit hole all

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<v Speaker 1>the way to the origins of astronomy.

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<v Speaker 2>Okay, I mean that's it's not quite as much fun

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<v Speaker 2>as I was hoping, but like sort of fun. All right.

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<v Speaker 1>So you're hoping it was related to butts, weren't you?

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<v Speaker 2>I mean probably, like, yes, the act of dropping one's

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<v Speaker 2>pants is what I was hoping for, but maybe this

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<v Speaker 2>is I got to keep this kid friendly. Also, teeny

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<v Speaker 2>pet peeve of mine. I feel like, whenever you're referring

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<v Speaker 2>to the moon of Earth, you need to be careful

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<v Speaker 2>to capitalize it because we're referring to it's a specific moon.

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<v Speaker 2>Then the other moons can get a lower case because

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<v Speaker 2>we're referring to moons in general exactly.

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<v Speaker 1>And you know, for a long time, we refer to

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<v Speaker 1>all of these things as just satellites, so instead of

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<v Speaker 1>calling them moons, you would say the satellites of Jupiter.

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<v Speaker 1>Then with Sputnak and the advent of artificial satellites, you know,

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<v Speaker 1>half a century ago it became very awkward to constantly

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<v Speaker 1>say artificial satellite, natural satellite, artificial satellite. And you know,

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<v Speaker 1>English is constantly smoothing and shortening things, and so people

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<v Speaker 1>just started referring to artificial satellites as satellites, and then

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<v Speaker 1>instead of referring to natural satellites, they just called everything moons,

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<v Speaker 1>sort of colloquially after our moon. So technically, astronomically we

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<v Speaker 1>have natural satellites and artificial satellites, but more practically we

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<v Speaker 1>have satellites, which mean artificial satellites which are not moons

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<v Speaker 1>or natural satellites, and then natural satellites that we call moons.

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<v Speaker 2>And I think the word sputnik is just the Russian

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<v Speaker 2>word for satellite.

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<v Speaker 1>Yeah. And then aside from the linguistic fuzziness, there is

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<v Speaker 1>also this question of like, well, what makes something a moon?

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<v Speaker 1>Like it's pretty clear if you're looking at the Earth

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<v Speaker 1>and the Moon, the Earth is bigger, and so you

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<v Speaker 1>would say that the moon is a moon and the

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<v Speaker 1>Earth is a satellite of the Sun. But physically speaking,

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<v Speaker 1>the Earth and the Moon are orbiting each other, right,

0:12:20.000 --> 0:12:22.360
<v Speaker 1>and there's a center of mass of the Earth Moon system,

0:12:22.640 --> 0:12:25.280
<v Speaker 1>and that is what's orbiting the Sun. And so it's

0:12:25.280 --> 0:12:27.800
<v Speaker 1>a little bit arbitrary to say, Okay, this one's a

0:12:27.800 --> 0:12:30.760
<v Speaker 1>moon and this one's a planet. You can imagine, for example,

0:12:30.800 --> 0:12:32.760
<v Speaker 1>a scenario where you have two objects of the same

0:12:32.800 --> 0:12:37.000
<v Speaker 1>mass orbiting each other, like a binary dwarf planet system,

0:12:37.559 --> 0:12:40.320
<v Speaker 1>which is the moon, which is a planet, right, you

0:12:40.400 --> 0:12:43.920
<v Speaker 1>need some way of categorizing it, and so in our

0:12:44.000 --> 0:12:47.360
<v Speaker 1>Solar system, typically if the center of mass of the

0:12:47.440 --> 0:12:51.000
<v Speaker 1>system is within the surface of one of the objects,

0:12:51.800 --> 0:12:54.680
<v Speaker 1>so that's like, you know, where is the average bit,

0:12:55.080 --> 0:12:57.760
<v Speaker 1>The average bit is under the surface, like between the

0:12:57.800 --> 0:12:59.559
<v Speaker 1>Earth and the Moon. The center of mass of the

0:12:59.600 --> 0:13:03.320
<v Speaker 1>Earth Moon system is within the volume of the Earth.

0:13:03.480 --> 0:13:06.800
<v Speaker 1>Then you say that's the planet and anything else outside

0:13:06.840 --> 0:13:09.839
<v Speaker 1>of that is a moon. It's a little bit arbitrary,

0:13:10.080 --> 0:13:14.360
<v Speaker 1>but it's helpful to settling debates among astronomers, which you know,

0:13:15.000 --> 0:13:16.640
<v Speaker 1>you have to have a reason for those guys to

0:13:16.880 --> 0:13:20.360
<v Speaker 1>stop drinking and go to sleep. And there's the other

0:13:20.440 --> 0:13:23.040
<v Speaker 1>side of it, which is like, well, what's the smallest

0:13:23.120 --> 0:13:27.600
<v Speaker 1>possible moon? Right? Like is every dust grain that's orbiting

0:13:27.640 --> 0:13:31.280
<v Speaker 1>the Earth a natural satellite if it formed naturally? Like,

0:13:31.400 --> 0:13:34.679
<v Speaker 1>is there a lowest cutoff? Is every proton that's in

0:13:34.840 --> 0:13:39.000
<v Speaker 1>orbit around the Earth a satellite? Technically according to the

0:13:39.040 --> 0:13:43.320
<v Speaker 1>definition of natural satellite, yes, those are natural satellites. You

0:13:43.360 --> 0:13:46.360
<v Speaker 1>don't count them as moons of Earth. And later we'll

0:13:46.360 --> 0:13:48.720
<v Speaker 1>talk about how the Earth actually does have a weird

0:13:48.880 --> 0:13:51.960
<v Speaker 1>second body that's kind of orbiting it but not really

0:13:51.960 --> 0:13:54.680
<v Speaker 1>that you could argue is kind of like a second

0:13:54.720 --> 0:13:58.439
<v Speaker 1>moon of the Earth. Anyway, the point is it depends

0:13:58.840 --> 0:14:02.360
<v Speaker 1>on the definition. And so, yeah, Kelly, really nobody knows.

0:14:02.679 --> 0:14:06.280
<v Speaker 2>Yes, yes, I knew, I was right. That's great, But

0:14:07.480 --> 0:14:09.720
<v Speaker 2>it does seem like, you know, you talk to ninety

0:14:09.800 --> 0:14:12.440
<v Speaker 2>nine point nine nine percent of the people on the planet,

0:14:12.480 --> 0:14:16.199
<v Speaker 2>they'd say that Earth has one moon, and is that

0:14:16.360 --> 0:14:18.240
<v Speaker 2>just because that's what we were told as kids and

0:14:18.240 --> 0:14:20.320
<v Speaker 2>it's stuck. But if you talk to an astronomer, they'd

0:14:20.320 --> 0:14:24.360
<v Speaker 2>be like, maybe we have a billion, or like, is

0:14:24.400 --> 0:14:27.920
<v Speaker 2>there essentially a definition that we all agree to for

0:14:28.040 --> 0:14:29.080
<v Speaker 2>convenience sake?

0:14:29.600 --> 0:14:32.920
<v Speaker 1>There is really no lower limit. But we call these

0:14:32.960 --> 0:14:36.120
<v Speaker 1>things moons because they're interesting. They reveal the structure of

0:14:36.160 --> 0:14:40.320
<v Speaker 1>the Solar System. They affect planets because of their tidal forces,

0:14:40.760 --> 0:14:43.800
<v Speaker 1>and tiny little dust grains don't do that as much,

0:14:43.840 --> 0:14:46.080
<v Speaker 1>and so they really are sort of a different kind

0:14:46.120 --> 0:14:48.720
<v Speaker 1>of thing. Even if it is an arbitrary dotted line

0:14:48.720 --> 0:14:51.360
<v Speaker 1>that we draw, and there really isn't a place to

0:14:51.360 --> 0:14:54.040
<v Speaker 1>put it. It doesn't make sense to put an individual

0:14:54.040 --> 0:14:56.680
<v Speaker 1>proton in the same category as the moon of Earth,

0:14:57.040 --> 0:15:00.480
<v Speaker 1>just because they both orbit the Earth, and so is

0:15:00.520 --> 0:15:03.800
<v Speaker 1>a qualitative difference, even if there isn't a crisp line

0:15:03.840 --> 0:15:05.720
<v Speaker 1>that we can draw. And so, no, I don't think

0:15:05.720 --> 0:15:08.240
<v Speaker 1>any astronomer is going to be like, actually, there are

0:15:08.240 --> 0:15:12.000
<v Speaker 1>many moons of Earth, but you know, probably maybe there

0:15:12.040 --> 0:15:13.080
<v Speaker 1>is one out there somewhere.

0:15:13.480 --> 0:15:15.480
<v Speaker 2>Is that what you think astronomers sound like? Because I

0:15:15.480 --> 0:15:17.600
<v Speaker 2>think you got to watch it. There might be some

0:15:17.640 --> 0:15:19.880
<v Speaker 2>astronomers that listen to this show and their feelings might

0:15:19.920 --> 0:15:20.520
<v Speaker 2>get hurt.

0:15:20.840 --> 0:15:24.480
<v Speaker 1>No, I think most astronomers sound like they're really fit.

0:15:24.840 --> 0:15:27.360
<v Speaker 1>They're very suave, but just the annoying ones sound like that.

0:15:27.520 --> 0:15:29.800
<v Speaker 2>Got it? Okay, So you said we have like this

0:15:29.960 --> 0:15:37.000
<v Speaker 2>arbitrary definition. Does this arbitrary definition have some features or

0:15:37.080 --> 0:15:39.720
<v Speaker 2>is it just like, is it always a gut feeling

0:15:39.960 --> 0:15:44.120
<v Speaker 2>or do we have some criteria even if it was

0:15:44.240 --> 0:15:45.880
<v Speaker 2>happened upon somewhat arbitrarily.

0:15:46.440 --> 0:15:51.400
<v Speaker 1>So, typically planets have something like ten thousand times the

0:15:51.440 --> 0:15:53.840
<v Speaker 1>mass of their natural satellite. That's what we tend to

0:15:53.840 --> 0:15:56.320
<v Speaker 1>see in the Solar System. But you know there are

0:15:56.360 --> 0:15:59.200
<v Speaker 1>already exceptions to that, Like the moon is one eightieth

0:15:59.240 --> 0:16:02.520
<v Speaker 1>of the Earth, Pluto has a moon that's one eighth

0:16:03.000 --> 0:16:05.880
<v Speaker 1>of its mass, right, and so like you can make

0:16:05.880 --> 0:16:09.160
<v Speaker 1>these broad categories. Almost all the moons in our Solar

0:16:09.200 --> 0:16:13.160
<v Speaker 1>system have a mass that's less than ten thousands of

0:16:13.200 --> 0:16:16.640
<v Speaker 1>the planetary mass. But there are already major exceptions.

0:16:17.600 --> 0:16:19.760
<v Speaker 2>Well, let's take a break. When we come back, we'll

0:16:19.760 --> 0:16:22.320
<v Speaker 2>talk about why we have moons. And if there are

0:16:22.360 --> 0:16:24.960
<v Speaker 2>any kids hanging out with you while you're listening to

0:16:25.000 --> 0:16:28.280
<v Speaker 2>this episode, kids, don't get any ideas. No mooning your

0:16:28.320 --> 0:16:31.400
<v Speaker 2>parents during the commercial break. When we get back, why

0:16:31.440 --> 0:16:54.880
<v Speaker 2>do we have moons? And we're back, So, Daniel, we

0:16:54.920 --> 0:16:57.880
<v Speaker 2>talked about how moons are defined, but why do we

0:16:57.920 --> 0:17:00.320
<v Speaker 2>have moons in the first place, and why did the Earth,

0:17:00.480 --> 0:17:04.600
<v Speaker 2>clearly the greatest planet in the Solar System, only get one.

0:17:05.160 --> 0:17:07.719
<v Speaker 1>Yeah, this is the most interesting thing about moons, in

0:17:07.720 --> 0:17:10.879
<v Speaker 1>my opinion, is that they reveal something about the history

0:17:10.920 --> 0:17:13.440
<v Speaker 1>of the Solar System. If you read about the Solar

0:17:13.440 --> 0:17:15.080
<v Speaker 1>System and look out at the sky, you get the

0:17:15.080 --> 0:17:18.760
<v Speaker 1>impression that it's this sort of calm parade. There's like

0:17:18.920 --> 0:17:22.040
<v Speaker 1>slow moving truds through space that's been going this way

0:17:22.080 --> 0:17:23.520
<v Speaker 1>for a long time and going to be going this

0:17:23.560 --> 0:17:26.919
<v Speaker 1>way forever. But that's only because we're used to living

0:17:27.160 --> 0:17:31.520
<v Speaker 1>at a sort of human timescale seconds, minutes, even centuries,

0:17:32.080 --> 0:17:34.760
<v Speaker 1>and in those timescales, yeah, not much really happens in

0:17:34.800 --> 0:17:37.679
<v Speaker 1>the Solar System. But the Solar System is very old.

0:17:37.760 --> 0:17:40.600
<v Speaker 1>It's four and a half billion years old, and its

0:17:40.720 --> 0:17:45.400
<v Speaker 1>history is filled with chaos. All sorts of crazy cosmic

0:17:45.440 --> 0:17:49.280
<v Speaker 1>cataclysms have occurred in our Solar System, from planets moving

0:17:49.359 --> 0:17:52.040
<v Speaker 1>in and out and switching orbits and losing planets. And

0:17:52.200 --> 0:17:54.960
<v Speaker 1>moons are a great way to understand this history because

0:17:55.000 --> 0:17:58.040
<v Speaker 1>they are in effect records of this history. And if

0:17:58.080 --> 0:18:00.480
<v Speaker 1>you understand it why a planet has a moon, you

0:18:00.480 --> 0:18:04.159
<v Speaker 1>can understand something about what happened to that planet. So

0:18:04.200 --> 0:18:08.040
<v Speaker 1>there's basically three different ways that planets can get moons,

0:18:08.400 --> 0:18:10.479
<v Speaker 1>from the least interesting all the way up to the

0:18:10.520 --> 0:18:11.600
<v Speaker 1>most exciting.

0:18:12.000 --> 0:18:14.840
<v Speaker 2>Well, I bet we are all super excited for you

0:18:14.920 --> 0:18:17.119
<v Speaker 2>to start with the least interesting. Explanation?

0:18:18.040 --> 0:18:20.320
<v Speaker 1>Was that a great lead in, right, lead into that

0:18:22.000 --> 0:18:26.840
<v Speaker 1>ready to get bored here, I'm in, Well, you don't

0:18:26.880 --> 0:18:29.320
<v Speaker 1>want to drop people with the most exciting one, and

0:18:29.359 --> 0:18:31.000
<v Speaker 1>then you know they're sort of spent and like, I

0:18:31.000 --> 0:18:32.320
<v Speaker 1>don't want to listen to the rest of this. You

0:18:32.400 --> 0:18:33.600
<v Speaker 1>got to build up to it, don't you.

0:18:33.680 --> 0:18:35.200
<v Speaker 2>But you don't even have to tell them there's a

0:18:35.320 --> 0:18:36.480
<v Speaker 2>least interesting option.

0:18:37.680 --> 0:18:40.680
<v Speaker 1>Great, all right, Well, the least interesting is already very

0:18:40.720 --> 0:18:45.400
<v Speaker 1>exciting because it tells you about the formation of the planet.

0:18:45.480 --> 0:18:48.720
<v Speaker 1>So sometimes moons form at the same time as the

0:18:48.720 --> 0:18:51.080
<v Speaker 1>planet in the same way that, like the structure of

0:18:51.119 --> 0:18:54.160
<v Speaker 1>our Solar System, didn't just make a sun, but also

0:18:54.200 --> 0:18:57.200
<v Speaker 1>made a bunch of planets. As those planets are forming,

0:18:57.400 --> 0:18:59.439
<v Speaker 1>they don't just make a planet, they also make their

0:18:59.480 --> 0:19:00.720
<v Speaker 1>own little.

0:19:00.359 --> 0:19:04.159
<v Speaker 2>Orbiting guys and gals space gals.

0:19:04.200 --> 0:19:07.080
<v Speaker 1>I like that. So why does the Solar System have

0:19:07.160 --> 0:19:09.960
<v Speaker 1>this kind of structure? Well, remember that the Solar System

0:19:10.080 --> 0:19:13.679
<v Speaker 1>formed from a central blob that collapse gravitationally. You have

0:19:13.760 --> 0:19:17.560
<v Speaker 1>like a seed somewhere where gravity started this runaway effect.

0:19:17.880 --> 0:19:19.760
<v Speaker 1>It got denser, so it had more gravity, so it

0:19:19.760 --> 0:19:21.399
<v Speaker 1>pulled on stuff, so it got denser, so it had

0:19:21.400 --> 0:19:23.760
<v Speaker 1>more gravity, et cetera, et cetera. But you never just

0:19:23.800 --> 0:19:26.800
<v Speaker 1>have exactly one seed. Sometimes you have like another nearby,

0:19:26.960 --> 0:19:30.479
<v Speaker 1>smaller seed that resists being pulled in because it has

0:19:30.600 --> 0:19:33.399
<v Speaker 1>enough relative velocity, So it goes into orbit and it

0:19:33.400 --> 0:19:37.320
<v Speaker 1>starts gathering its own stuff. So that's how planets form. Right.

0:19:37.320 --> 0:19:40.080
<v Speaker 1>You have this central blog which absorbs most of the mass,

0:19:40.320 --> 0:19:43.520
<v Speaker 1>but then you have these other seeds nearby which sometimes

0:19:43.560 --> 0:19:46.119
<v Speaker 1>form stars and you get like binary star systems. But

0:19:46.200 --> 0:19:49.000
<v Speaker 1>sometimes they're smaller and they'll form planets in the same

0:19:49.040 --> 0:19:52.080
<v Speaker 1>way as that planet is forming. It makes a proto

0:19:52.160 --> 0:19:55.720
<v Speaker 1>planetary disc. Right. It's a big swirling mass of stuff,

0:19:56.000 --> 0:19:58.719
<v Speaker 1>most of which will collapse into the planet, but some

0:19:58.800 --> 0:20:01.240
<v Speaker 1>of it is going fast enough and has its own

0:20:01.320 --> 0:20:05.000
<v Speaker 1>little gravitational seed, so can form an object which comes

0:20:05.040 --> 0:20:07.640
<v Speaker 1>into orbit around the planet rather than falling in.

0:20:08.160 --> 0:20:10.440
<v Speaker 2>Ah okay, and if it were to slow down, it

0:20:10.440 --> 0:20:11.960
<v Speaker 2>would fall in, but it's not.

0:20:12.119 --> 0:20:14.879
<v Speaker 1>Slowing down exactly. If it were to slow down, then

0:20:14.920 --> 0:20:17.400
<v Speaker 1>it would fall in. And you know, in that initial

0:20:17.440 --> 0:20:19.359
<v Speaker 1>planetary disc there is a lot of friction, and so

0:20:19.400 --> 0:20:21.080
<v Speaker 1>a lot of stuff does fall in. But if you

0:20:21.160 --> 0:20:24.399
<v Speaker 1>survive that and you form, then there's much less friction

0:20:24.480 --> 0:20:26.880
<v Speaker 1>because things have cleared out and you can mostly orbit

0:20:26.920 --> 0:20:29.880
<v Speaker 1>in a stable way. But it depends also on your

0:20:29.960 --> 0:20:33.040
<v Speaker 1>distance from the planet. So for example, if you're too

0:20:33.200 --> 0:20:35.160
<v Speaker 1>close to the planet, you're going to be feeling its

0:20:35.200 --> 0:20:39.040
<v Speaker 1>tidal forces. The planet is a huge gravitational object. And

0:20:39.119 --> 0:20:42.200
<v Speaker 1>remember that gravity depends on distance. The closer you are

0:20:42.280 --> 0:20:45.240
<v Speaker 1>to something, the stronger the gravitational force. The further you

0:20:45.240 --> 0:20:48.159
<v Speaker 1>are from something, the weaker the gravitational force. Now, if

0:20:48.200 --> 0:20:50.640
<v Speaker 1>you are just a point object, that doesn't really matter

0:20:50.680 --> 0:20:52.760
<v Speaker 1>because your front and back are the same thing. But

0:20:52.800 --> 0:20:55.280
<v Speaker 1>if you're big enough that your front and back are

0:20:55.320 --> 0:20:58.280
<v Speaker 1>substantially different, and your front is closer to the planet

0:20:58.280 --> 0:21:00.480
<v Speaker 1>and your back is further from the planet, then a

0:21:00.560 --> 0:21:02.719
<v Speaker 1>planet is going to be pulling on your front harder

0:21:02.760 --> 0:21:06.000
<v Speaker 1>than it's pulling on your back. These are tidal forces. Essentially,

0:21:06.000 --> 0:21:08.400
<v Speaker 1>it's pulling your front and back apart from each other.

0:21:08.680 --> 0:21:10.840
<v Speaker 1>It tends to pull you into like a football shape.

0:21:11.119 --> 0:21:13.959
<v Speaker 1>If you're strong enough internally you're made of diamond, you

0:21:14.000 --> 0:21:16.240
<v Speaker 1>can resist that. But if you're not, you're going to

0:21:16.280 --> 0:21:19.440
<v Speaker 1>get shredded by the tidal forces. This is a mini

0:21:19.560 --> 0:21:23.080
<v Speaker 1>version of like spagetification when you approach a black hole,

0:21:23.600 --> 0:21:26.520
<v Speaker 1>and so a planet has a thing called a roche limit.

0:21:26.720 --> 0:21:29.320
<v Speaker 1>Anything closer to the planet than the roach limit is

0:21:29.359 --> 0:21:32.680
<v Speaker 1>feeling tidal forces that are too strong to survive. Those

0:21:32.680 --> 0:21:35.320
<v Speaker 1>are going to get shredded into like a ring. Anything

0:21:35.359 --> 0:21:38.320
<v Speaker 1>outside the roche limit can hold itself together and stay

0:21:38.359 --> 0:21:38.879
<v Speaker 1>as a moon.

0:21:39.080 --> 0:21:41.320
<v Speaker 2>All right, So you've got your central blob. It's formed

0:21:41.320 --> 0:21:43.720
<v Speaker 2>into a planet. And then I was imagining everything around

0:21:43.760 --> 0:21:47.520
<v Speaker 2>it is a ring. And so I guess when we're

0:21:47.560 --> 0:21:50.600
<v Speaker 2>discussing this roche limit thing, at that point, everything that

0:21:50.640 --> 0:21:52.600
<v Speaker 2>was in the ring has already been sort of pulled

0:21:52.720 --> 0:21:57.400
<v Speaker 2>into the football shape and it got really hard when

0:21:57.400 --> 0:21:59.920
<v Speaker 2>it got pulled into the football shape, and instead of

0:22:00.080 --> 0:22:03.040
<v Speaker 2>getting shredded that it forms the football moon.

0:22:03.480 --> 0:22:06.080
<v Speaker 1>Yeah, you're right. Everything starts as a ring. But if

0:22:06.080 --> 0:22:08.160
<v Speaker 1>you have a ring and it's far enough out, then

0:22:08.240 --> 0:22:10.480
<v Speaker 1>gravity in that ring is going to pull the ring

0:22:10.560 --> 0:22:13.119
<v Speaker 1>together into a moon, ok right, because things in the

0:22:13.119 --> 0:22:15.679
<v Speaker 1>same orbit are going to attract each other along that

0:22:15.840 --> 0:22:18.400
<v Speaker 1>orbit and they'll pull itself together. Now, if you're far

0:22:18.480 --> 0:22:21.080
<v Speaker 1>enough away beyond the roach limit, the planet is not

0:22:21.119 --> 0:22:22.880
<v Speaker 1>going to interfere with that, and you're going to gather

0:22:22.960 --> 0:22:26.080
<v Speaker 1>yourself together into a moon. If you are within the

0:22:26.160 --> 0:22:28.439
<v Speaker 1>roach limit, then the planet is going to interfere with that.

0:22:28.520 --> 0:22:30.200
<v Speaker 1>And as soon as you get any big objects, the

0:22:30.200 --> 0:22:32.520
<v Speaker 1>planet's going to tear them apart or even prevent them

0:22:32.520 --> 0:22:35.080
<v Speaker 1>from forming in the first place, or as we'll talk

0:22:35.119 --> 0:22:37.840
<v Speaker 1>about later. If you have a pre formed object that

0:22:37.920 --> 0:22:40.920
<v Speaker 1>then comes inside the roach limit, the planet will tear

0:22:40.920 --> 0:22:43.719
<v Speaker 1>it apart. So you have rings are formed with the

0:22:43.760 --> 0:22:47.439
<v Speaker 1>planet probably never were moons, if that's really what you're asking.

0:22:47.760 --> 0:22:51.879
<v Speaker 2>Rings that formed with the planet never were moons, but

0:22:51.960 --> 0:22:53.080
<v Speaker 2>could become moons.

0:22:53.880 --> 0:22:56.600
<v Speaker 1>They could become moons if they're outside the roach limit. Yes,

0:22:56.640 --> 0:22:59.640
<v Speaker 1>but rings within the roach limit are probably never were

0:22:59.760 --> 0:23:02.880
<v Speaker 1>moonduns because there's just too strong a tidal force for

0:23:02.920 --> 0:23:04.399
<v Speaker 1>them to pull themselves together.

0:23:05.160 --> 0:23:08.200
<v Speaker 2>So this sounds like an unlikely path to moonhood.

0:23:08.480 --> 0:23:10.800
<v Speaker 1>Yeah, exactly, you need to be outside the roach limit

0:23:11.000 --> 0:23:13.400
<v Speaker 1>in order to be a moon. And so, for example,

0:23:13.520 --> 0:23:15.639
<v Speaker 1>in the Earth moon system, the roach limit is like

0:23:15.680 --> 0:23:19.200
<v Speaker 1>ten thousand kilometers. Anything closer to the Earth than ten

0:23:19.240 --> 0:23:21.560
<v Speaker 1>thousand kilometers you're going to get pulled apart. The Moon

0:23:21.640 --> 0:23:24.840
<v Speaker 1>is safely like three hundred and eighty thousand kilometers away,

0:23:25.119 --> 0:23:28.520
<v Speaker 1>so you're safe. And the Sun also has a roach limit.

0:23:28.720 --> 0:23:32.000
<v Speaker 1>Planets that approach closer than like seven hundred and fifty

0:23:32.040 --> 0:23:35.919
<v Speaker 1>thousand kilometers to the Sun would get shredded. We're safely

0:23:35.960 --> 0:23:38.960
<v Speaker 1>one hundred and fifty million kilometers from the Sun, and

0:23:39.000 --> 0:23:41.040
<v Speaker 1>these roach limits are a little bit fuzzy because an

0:23:41.080 --> 0:23:44.320
<v Speaker 1>object doesn't have a fixed roach limit depends on what

0:23:44.359 --> 0:23:46.440
<v Speaker 1>you're bringing near it. Like if you bring a moon

0:23:46.520 --> 0:23:49.840
<v Speaker 1>made of jello versus the moon made of diamond, they're

0:23:49.880 --> 0:23:51.719
<v Speaker 1>going to get pulled apart at different places, if that

0:23:51.760 --> 0:23:52.240
<v Speaker 1>makes sense.

0:23:52.640 --> 0:23:55.879
<v Speaker 2>And the Moon each year is getting pulled a little

0:23:55.920 --> 0:23:58.840
<v Speaker 2>bit closer to Earth. But it sounds like the difference

0:23:58.880 --> 0:24:01.240
<v Speaker 2>between the roach limit and where the moon is is

0:24:01.320 --> 0:24:03.840
<v Speaker 2>so far there. Oh wait, or is the Moon getting

0:24:03.840 --> 0:24:05.280
<v Speaker 2>farther away from us?

0:24:05.720 --> 0:24:08.200
<v Speaker 1>The Moon is getting further away by the best centimeter

0:24:08.320 --> 0:24:11.400
<v Speaker 1>a year, and it has to do with the angular momentum. Yeah,

0:24:11.400 --> 0:24:12.800
<v Speaker 1>but it is a tidal force effect.

0:24:12.800 --> 0:24:14.720
<v Speaker 2>Also, Okay, are we going to lose the moon?

0:24:14.760 --> 0:24:17.119
<v Speaker 1>Then eventually the Earth and the Moon are going to

0:24:17.119 --> 0:24:19.560
<v Speaker 1>get tidily locked, which will stop this process.

0:24:19.800 --> 0:24:23.600
<v Speaker 2>Okay, good few. Okay, So it sounds like this might

0:24:23.960 --> 0:24:25.960
<v Speaker 2>not be how we got our moon.

0:24:26.840 --> 0:24:28.679
<v Speaker 1>Well, this is not how we got our moon. And

0:24:28.720 --> 0:24:31.640
<v Speaker 1>you can tell which moon's formed with the planet because

0:24:31.640 --> 0:24:34.880
<v Speaker 1>they tend to have a very nice circular orbit and

0:24:34.920 --> 0:24:39.119
<v Speaker 1>to be orbiting the planet around its equator essentially on

0:24:39.160 --> 0:24:41.879
<v Speaker 1>the same axis that the planet is spinning. Because it

0:24:41.920 --> 0:24:44.480
<v Speaker 1>all formed from the same blob of stuff, just like

0:24:44.640 --> 0:24:47.159
<v Speaker 1>most of the planets in the Solar System are orbiting

0:24:47.200 --> 0:24:50.840
<v Speaker 1>the Sun around the same axis that the Sun is rotating,

0:24:50.880 --> 0:24:53.359
<v Speaker 1>because it all came from the same original blob of stuff.

0:24:53.800 --> 0:24:57.040
<v Speaker 1>So if you find a moon around a planet and

0:24:57.080 --> 0:24:59.879
<v Speaker 1>it's got a mostly circular orbit and it's orbiting around

0:25:00.000 --> 0:25:03.080
<v Speaker 1>and the same axis as a planet is spinning, probably

0:25:03.160 --> 0:25:04.560
<v Speaker 1>it formed with the planet.

0:25:04.840 --> 0:25:09.080
<v Speaker 2>WHOA, we got through the boring stuff. All right, Actually

0:25:09.320 --> 0:25:11.320
<v Speaker 2>I thought that was really cool. But okay, so let's

0:25:11.400 --> 0:25:11.800
<v Speaker 2>move on.

0:25:12.080 --> 0:25:17.200
<v Speaker 1>Relatively boring, relatively super exciting, just not the most exciting

0:25:17.240 --> 0:25:18.600
<v Speaker 1>thing we'll talk about today, all.

0:25:18.600 --> 0:25:20.600
<v Speaker 2>Right, all right, so let's move on to something way

0:25:20.640 --> 0:25:22.480
<v Speaker 2>more epic. What's the next method?

0:25:22.800 --> 0:25:26.439
<v Speaker 1>The next method is to capture something. Imagine an object

0:25:26.520 --> 0:25:28.800
<v Speaker 1>that's floating through the Solar System and it comes near

0:25:28.840 --> 0:25:31.679
<v Speaker 1>a planet. Planets have a lot of gravity. If it

0:25:31.720 --> 0:25:34.360
<v Speaker 1>comes in at the right velocity, in the right distance

0:25:34.359 --> 0:25:37.520
<v Speaker 1>and the right angle, it can basically enter orbit around

0:25:37.560 --> 0:25:40.320
<v Speaker 1>a planet the way like a spaceship can approach a

0:25:40.359 --> 0:25:42.760
<v Speaker 1>planet and go into orbit around it, or you can

0:25:42.840 --> 0:25:46.480
<v Speaker 1>launch a satellite into orbit. If visiting rock has the

0:25:46.560 --> 0:25:49.800
<v Speaker 1>right trajectory, it can be captured by a planet. And

0:25:49.840 --> 0:25:52.640
<v Speaker 1>you can tell moons that have this history because they're

0:25:52.640 --> 0:25:55.320
<v Speaker 1>not made of the same stuff as the planet, and

0:25:55.520 --> 0:25:58.040
<v Speaker 1>because they tend to have like weird orbits, they're highly

0:25:58.080 --> 0:26:02.240
<v Speaker 1>elliptical or they're tilted relative to the axis of rotation

0:26:02.480 --> 0:26:03.160
<v Speaker 1>of the planet.

0:26:03.560 --> 0:26:05.639
<v Speaker 2>How many of these do we think we have in

0:26:05.680 --> 0:26:08.240
<v Speaker 2>our Solar system, because that seems like, depending on where

0:26:08.240 --> 0:26:10.640
<v Speaker 2>they came from, a really cool opportunity for science.

0:26:11.000 --> 0:26:13.679
<v Speaker 1>It is a very cool opportunity for science. And we

0:26:13.760 --> 0:26:17.000
<v Speaker 1>have lots and lots of these examples in the Solar System,

0:26:17.040 --> 0:26:18.480
<v Speaker 1>and we'll talk about a few of them in a

0:26:18.480 --> 0:26:21.280
<v Speaker 1>minute when we do the countdown for the ranking of

0:26:21.320 --> 0:26:24.320
<v Speaker 1>the most moons. But it happens quite a bit. And

0:26:24.320 --> 0:26:27.760
<v Speaker 1>astronomers like to think about the region of a planet

0:26:27.880 --> 0:26:31.320
<v Speaker 1>near a planet where its gravity dominates. Because imagine you're

0:26:31.359 --> 0:26:33.840
<v Speaker 1>some rock and basically you're orbiting the Sun and you

0:26:33.920 --> 0:26:36.760
<v Speaker 1>come near the Earth. How close to the Earth you

0:26:36.840 --> 0:26:39.800
<v Speaker 1>have to get before the Earth's gravity dominates over the

0:26:39.840 --> 0:26:43.800
<v Speaker 1>Sun's gravity. That's called the hill sphere. And if a

0:26:44.119 --> 0:26:46.600
<v Speaker 1>rock enters the hill sphere of a planet, then it

0:26:46.600 --> 0:26:48.400
<v Speaker 1>has a chance to become captured.

0:26:48.680 --> 0:26:52.480
<v Speaker 2>And was hill a guy or gal was Hill an astronomer,

0:26:53.280 --> 0:26:55.840
<v Speaker 2>presumably not one with the voice like you were making before.

0:26:59.480 --> 0:27:01.800
<v Speaker 1>Yes, it was an astronomer and someone who thought about

0:27:01.960 --> 0:27:05.320
<v Speaker 1>the early formation of the Solar System, because remember, back

0:27:05.320 --> 0:27:08.359
<v Speaker 1>in the early days, things weren't as well cleared outs.

0:27:08.520 --> 0:27:12.280
<v Speaker 1>There were lots of rocks floating around Jupiter and Saturn

0:27:12.480 --> 0:27:14.840
<v Speaker 1>moved into the inner Solar System and then back out,

0:27:14.880 --> 0:27:17.919
<v Speaker 1>and that threw lots of asteroids everywhere, So there were

0:27:18.000 --> 0:27:20.639
<v Speaker 1>lots of scattered objects. Some of them just get lost

0:27:20.960 --> 0:27:24.360
<v Speaker 1>at a fly outside the Solar System. Eventually maybe get

0:27:24.359 --> 0:27:26.960
<v Speaker 1>captured by another Solar system. Some of them will get

0:27:27.000 --> 0:27:29.719
<v Speaker 1>captured by other planets. But each one is like a

0:27:29.760 --> 0:27:33.520
<v Speaker 1>time capsule of crazy events that happened in our Solar system.

0:27:33.720 --> 0:27:37.439
<v Speaker 2>It sounds like if a giant object comes in that

0:27:37.480 --> 0:27:39.919
<v Speaker 2>would cause a lot of chaos in the process, Like

0:27:40.440 --> 0:27:42.720
<v Speaker 2>does it cause? I mean, I guess if it's small

0:27:42.800 --> 0:27:44.800
<v Speaker 2>enough relative to a planet that it can get captured,

0:27:44.800 --> 0:27:46.520
<v Speaker 2>it's probably not going to cause a lot of chaos

0:27:46.600 --> 0:27:49.280
<v Speaker 2>for the planet that captures it. So maybe it's not

0:27:49.280 --> 0:27:52.360
<v Speaker 2>going to cause that much chaos. How chaotic is this, Daniel.

0:27:53.760 --> 0:27:56.520
<v Speaker 1>Well, the bigger the thing, the more chaos it causes, right,

0:27:56.600 --> 0:27:59.680
<v Speaker 1>because the more gravitational pull it has. But the Solar

0:27:59.680 --> 0:28:01.840
<v Speaker 1>System already has a lot of chaos in it because

0:28:01.920 --> 0:28:04.000
<v Speaker 1>every system that has more than two bodies in it

0:28:04.080 --> 0:28:06.880
<v Speaker 1>is chaotic. You know, it's called the three body problem.

0:28:07.160 --> 0:28:10.400
<v Speaker 1>You can't have very many stable configurations of three objects

0:28:10.520 --> 0:28:13.280
<v Speaker 1>orbiting each other, and the only way to do that

0:28:13.440 --> 0:28:15.600
<v Speaker 1>is to have configurations where like two of them are

0:28:15.640 --> 0:28:17.879
<v Speaker 1>really really far from the other one. So even just

0:28:17.920 --> 0:28:20.960
<v Speaker 1>having like Earth, Sun and Jupiter already is a little

0:28:20.960 --> 0:28:23.399
<v Speaker 1>bit chaotic. Jupiter is pulling on the Earth. That's one

0:28:23.440 --> 0:28:25.800
<v Speaker 1>of the reasons why our orbits are changing, and we

0:28:25.920 --> 0:28:29.000
<v Speaker 1>have these Malkovich cycles where we get further and closer

0:28:29.040 --> 0:28:31.159
<v Speaker 1>from the Sun. So there's already a little bit of

0:28:31.240 --> 0:28:34.240
<v Speaker 1>chaos in the Solar System. So something coming in from

0:28:34.240 --> 0:28:37.399
<v Speaker 1>the outside is definitely going to inject more chaos, and

0:28:37.480 --> 0:28:40.840
<v Speaker 1>most likely chaos causes us to lose things. Being captured

0:28:40.880 --> 0:28:42.840
<v Speaker 1>is rare because you have to come in at like

0:28:42.880 --> 0:28:45.440
<v Speaker 1>the right angle, and you can't be close enough that

0:28:45.480 --> 0:28:47.760
<v Speaker 1>you enter the atmosphere and then drag and then hit

0:28:47.800 --> 0:28:49.920
<v Speaker 1>the planet, and not so far that you're going to

0:28:49.920 --> 0:28:52.760
<v Speaker 1>miss the hillsphere. So it's really just like quite a

0:28:52.880 --> 0:28:55.800
<v Speaker 1>narrow window for things to get captured. So the things

0:28:55.880 --> 0:28:57.920
<v Speaker 1>in the Solar system that are captured are a tiny

0:28:58.000 --> 0:29:01.000
<v Speaker 1>fraction of all the chaos that has flown through our

0:29:01.000 --> 0:29:01.640
<v Speaker 1>solar system.

0:29:02.040 --> 0:29:05.080
<v Speaker 2>So most of the stuff that does get captured and

0:29:05.080 --> 0:29:08.240
<v Speaker 2>become a moon, do we know where it tends to

0:29:08.280 --> 0:29:08.720
<v Speaker 2>come from?

0:29:08.960 --> 0:29:11.240
<v Speaker 1>We don't because we haven't studied a lot of these enough.

0:29:11.240 --> 0:29:14.400
<v Speaker 1>We haven't like landed on them or done spectrometry on

0:29:14.440 --> 0:29:16.720
<v Speaker 1>them in great detail. And you'll see the ones we

0:29:16.760 --> 0:29:19.040
<v Speaker 1>have studied we already have a lot of questions about.

0:29:20.080 --> 0:29:24.200
<v Speaker 2>Well. I also thought that that was pretty awesome, But

0:29:24.320 --> 0:29:27.240
<v Speaker 2>now we're going to get to the most awesome explanation,

0:29:27.400 --> 0:29:30.360
<v Speaker 2>which is collisions, and I agree that is probably the

0:29:30.400 --> 0:29:33.440
<v Speaker 2>most awesome out of all the explanations. So all right, collisions,

0:29:33.640 --> 0:29:34.640
<v Speaker 2>hit me with it, Daniel.

0:29:35.240 --> 0:29:37.920
<v Speaker 1>So imagine you have a planet and it's doing its thing,

0:29:38.040 --> 0:29:41.520
<v Speaker 1>and then like another planet comes and snacks into it,

0:29:42.080 --> 0:29:45.640
<v Speaker 1>and the two planets are vaporized essentially, and they have

0:29:45.720 --> 0:29:50.240
<v Speaker 1>to like coalesce again into molten blobs, and that process

0:29:50.280 --> 0:29:53.720
<v Speaker 1>doesn't always give two objects of the same size. This

0:29:54.040 --> 0:29:56.880
<v Speaker 1>is the leading theory for the formation of Earth. And

0:29:57.000 --> 0:30:00.600
<v Speaker 1>its moon. That there was a proto Earth with a

0:30:00.680 --> 0:30:03.120
<v Speaker 1>huge moon and it was smacked into by like a

0:30:03.280 --> 0:30:08.320
<v Speaker 1>Mars sized planet, which essentially vaporized the surface of the Earth,

0:30:08.760 --> 0:30:11.440
<v Speaker 1>and a huge chunk of stuff was then thrown out

0:30:11.480 --> 0:30:14.600
<v Speaker 1>into orbit, gathered into a ring as it cooled, and

0:30:14.640 --> 0:30:18.720
<v Speaker 1>then formed into a moon. And there's lots of evidence

0:30:18.760 --> 0:30:20.840
<v Speaker 1>of this from the fact that, like the Moon is

0:30:20.880 --> 0:30:23.520
<v Speaker 1>made out of basically the same stuff as the Earth,

0:30:23.920 --> 0:30:26.400
<v Speaker 1>and because of the way the Moon formed and cooled,

0:30:26.720 --> 0:30:29.680
<v Speaker 1>you can tell that had fairly recent activity on it. Also,

0:30:29.880 --> 0:30:32.720
<v Speaker 1>recent studies of the mantle of the Earth has shown

0:30:32.800 --> 0:30:36.640
<v Speaker 1>like actual deposition from this original protoplanet that hid it.

0:30:36.640 --> 0:30:39.920
<v Speaker 1>It's like there's bits of that still leaving an imprint

0:30:39.960 --> 0:30:43.040
<v Speaker 1>on the inner part of the Earth. It's really fascinating,

0:30:43.480 --> 0:30:45.640
<v Speaker 1>and so essentially that like I don't know if that

0:30:45.800 --> 0:30:47.560
<v Speaker 1>really adds a moon or if it just sort of

0:30:47.600 --> 0:30:50.920
<v Speaker 1>like deletes a planet and it creates two new objects.

0:30:51.200 --> 0:30:53.640
<v Speaker 2>All right, So I'm adding a qualifier to my earlier statement,

0:30:53.680 --> 0:30:55.320
<v Speaker 2>this is the most awesome way to make a moon,

0:30:55.400 --> 0:30:58.680
<v Speaker 2>as long as it never happens again in my lifetime

0:30:58.720 --> 0:30:59.600
<v Speaker 2>to my planets.

0:30:59.720 --> 0:31:00.520
<v Speaker 1>Yeah, exactly.

0:31:00.640 --> 0:31:02.960
<v Speaker 2>But it's awesome that it happened long ago.

0:31:03.320 --> 0:31:05.240
<v Speaker 1>It would have been very dramatic to watch, right. I

0:31:05.240 --> 0:31:07.720
<v Speaker 1>wouldn't mind seeing this happen to another planet. You would

0:31:07.800 --> 0:31:09.920
<v Speaker 1>learn a lot about this Solar System as long as,

0:31:09.960 --> 0:31:12.959
<v Speaker 1>of course, nobody was living on it. No critics were

0:31:12.960 --> 0:31:14.320
<v Speaker 1>harmed in this cosmic collision.

0:31:14.480 --> 0:31:17.240
<v Speaker 2>Okay, So let's assume that there are no microbes on Mars.

0:31:17.800 --> 0:31:20.560
<v Speaker 2>If something like this happened to Mars and we were

0:31:20.600 --> 0:31:23.600
<v Speaker 2>watching it, would there be any implications for us, like

0:31:23.680 --> 0:31:26.520
<v Speaker 2>maybe junk would get thrown off Mars and would hit

0:31:26.680 --> 0:31:28.960
<v Speaker 2>up Yeah, would anything happen to us if this happened

0:31:28.960 --> 0:31:29.360
<v Speaker 2>to Mars.

0:31:29.480 --> 0:31:31.800
<v Speaker 1>Oh, for sure, we would be hit by debris from it.

0:31:32.000 --> 0:31:35.400
<v Speaker 1>We're already hit by debris from Mars. When things hit

0:31:35.400 --> 0:31:38.120
<v Speaker 1>the surface of Mars, stuff is thrown out into space

0:31:38.160 --> 0:31:39.760
<v Speaker 1>and some of it lands on the Earth. We have

0:31:39.840 --> 0:31:41.920
<v Speaker 1>found rocks on the surface of the Earth that we

0:31:42.000 --> 0:31:46.720
<v Speaker 1>know come from Mars because they're geologically incompatible with Earth's

0:31:46.760 --> 0:31:51.440
<v Speaker 1>history and perfectly compatible with Mars. So that already happens

0:31:51.440 --> 0:31:55.600
<v Speaker 1>that like Mars's garbage lands on Earth. So if Mars

0:31:55.640 --> 0:31:59.760
<v Speaker 1>gets like massively slammed by a huge impactor and basically shredded,

0:32:00.040 --> 0:32:02.160
<v Speaker 1>then some significant fraction of it is definitely going to

0:32:02.240 --> 0:32:02.640
<v Speaker 1>hit Earth.

0:32:02.720 --> 0:32:05.640
<v Speaker 2>Yeah, given that you are willing to sacrifice all of

0:32:05.720 --> 0:32:09.160
<v Speaker 2>humanity just to talk to aliens for thirty seconds, would

0:32:09.160 --> 0:32:12.560
<v Speaker 2>you risk Earth getting hit by large chunks of Mars

0:32:12.600 --> 0:32:15.480
<v Speaker 2>just so you could see how this would all play out?

0:32:15.640 --> 0:32:18.480
<v Speaker 1>For sure? Plus we would get samples of Mars here

0:32:18.520 --> 0:32:21.560
<v Speaker 1>on Earth. You're the word, Well, how valuable that is? Like,

0:32:21.720 --> 0:32:25.040
<v Speaker 1>we have this incredible, complicated plan to dig up stuff

0:32:25.040 --> 0:32:26.680
<v Speaker 1>on the surface of Mars and send it back to

0:32:26.720 --> 0:32:29.680
<v Speaker 1>Earth for study. So valuable scientifically, but it's going to

0:32:29.720 --> 0:32:32.640
<v Speaker 1>bring back, like, you know, a small amount of Mars.

0:32:32.720 --> 0:32:35.600
<v Speaker 1>If you could like deliver huge chunks of Mars dropped

0:32:35.600 --> 0:32:38.040
<v Speaker 1>into the Pacific or something, Yeah, let's do it.

0:32:38.800 --> 0:32:41.680
<v Speaker 2>One of us studies life and one of us studies

0:32:41.760 --> 0:32:45.040
<v Speaker 2>non life, and it is very clear which one does

0:32:45.080 --> 0:32:45.840
<v Speaker 2>which right now?

0:32:46.720 --> 0:32:49.120
<v Speaker 1>All right, And while the history of Earth's moon and

0:32:49.160 --> 0:32:51.400
<v Speaker 1>this collision is really fastening into a lot of deep

0:32:51.440 --> 0:32:54.200
<v Speaker 1>signs we could dig into there. Today's episode is not

0:32:54.280 --> 0:32:56.920
<v Speaker 1>just a history of Earth's moon, but we wanted to

0:32:57.000 --> 0:33:00.240
<v Speaker 1>do a ranking of which planets have the most.

0:33:00.320 --> 0:33:05.760
<v Speaker 2>Moons, all right, And so we know unfortunately that the

0:33:05.840 --> 0:33:08.080
<v Speaker 2>answer is not Earth.

0:33:08.440 --> 0:33:12.480
<v Speaker 1>That's right, and in shortstanding tradition established on this episode,

0:33:12.600 --> 0:33:15.880
<v Speaker 1>we're going to start with the least exciting examples first.

0:33:16.160 --> 0:33:20.600
<v Speaker 2>That's right, okay, and so well, should we start closest

0:33:20.600 --> 0:33:21.080
<v Speaker 2>to the Sun?

0:33:21.400 --> 0:33:24.280
<v Speaker 1>Yes, and that coincidentally starts us at the end of

0:33:24.280 --> 0:33:27.080
<v Speaker 1>the list the planets with the least moons, and that

0:33:27.120 --> 0:33:30.640
<v Speaker 1>would be Mercury and Venus. Both of these planets have

0:33:31.040 --> 0:33:32.280
<v Speaker 1>zero moons.

0:33:32.840 --> 0:33:33.280
<v Speaker 2>Why.

0:33:33.760 --> 0:33:35.800
<v Speaker 1>The reason is that they are so close to the

0:33:35.880 --> 0:33:39.640
<v Speaker 1>Sun that the Sun's tidal forces will perturb any orbits.

0:33:40.200 --> 0:33:43.160
<v Speaker 1>Like it's really hard to have a three body system

0:33:43.440 --> 0:33:45.800
<v Speaker 1>if those three are close to each other. The only

0:33:45.840 --> 0:33:48.160
<v Speaker 1>way to have a three body stable system is if

0:33:48.160 --> 0:33:50.760
<v Speaker 1>two of them are far enough away. So, for example,

0:33:51.120 --> 0:33:52.760
<v Speaker 1>the Sun and the Earth and the Moon is a

0:33:52.800 --> 0:33:55.520
<v Speaker 1>three body system. Why is that stable Because the Moon

0:33:55.560 --> 0:33:57.800
<v Speaker 1>and the Earth are fairly close to each other and

0:33:58.080 --> 0:34:00.840
<v Speaker 1>both fairly far away from the Sun. If you bring

0:34:00.880 --> 0:34:03.640
<v Speaker 1>that two body system close enough to the Sun, then

0:34:03.720 --> 0:34:05.760
<v Speaker 1>it becomes a three body system and the whole thing

0:34:05.880 --> 0:34:09.120
<v Speaker 1>is chaotic. So basically, the Sun is going to be

0:34:09.160 --> 0:34:11.640
<v Speaker 1>pulling on those moons in a way that makes none

0:34:11.640 --> 0:34:12.960
<v Speaker 1>of those orbits stable.

0:34:13.160 --> 0:34:14.719
<v Speaker 2>So it sounds like you've just said that the Earth

0:34:14.760 --> 0:34:17.520
<v Speaker 2>is the closest planet that could possibly have a moon

0:34:17.719 --> 0:34:21.040
<v Speaker 2>in our solar system. Yeah, how much closer could the

0:34:21.160 --> 0:34:24.000
<v Speaker 2>Earth be and still have a moon? Are we essentially

0:34:24.040 --> 0:34:24.600
<v Speaker 2>at the limit?

0:34:24.760 --> 0:34:28.560
<v Speaker 1>Yeah, great question. It is possible for Mercury or Venus

0:34:28.600 --> 0:34:30.960
<v Speaker 1>to have a moon. It's just that their hill sphere

0:34:31.120 --> 0:34:34.480
<v Speaker 1>is really really small. So for example, for Mercury to

0:34:34.520 --> 0:34:36.840
<v Speaker 1>have a moon, you'd have to have a moon that

0:34:37.000 --> 0:34:40.160
<v Speaker 1>orbits like pretty close above the surface, which would be

0:34:40.280 --> 0:34:43.880
<v Speaker 1>like a super high velocity, And then Mercury would have

0:34:43.920 --> 0:34:46.520
<v Speaker 1>to have like no atmosphere at all because you wouldn't

0:34:46.520 --> 0:34:49.040
<v Speaker 1>want any drag and no like mountains for the moon

0:34:49.080 --> 0:34:52.040
<v Speaker 1>to smash into. So in principle, it is possible for

0:34:52.120 --> 0:34:54.319
<v Speaker 1>Mercury to have a moon, and Venus is like a

0:34:54.480 --> 0:34:57.000
<v Speaker 1>very thick atmosphere, so this should be tricky. But they

0:34:57.040 --> 0:34:58.799
<v Speaker 1>don't have a moon, and it'd be very hard for

0:34:58.840 --> 0:35:01.520
<v Speaker 1>them to get one. You could bring the Earth closer

0:35:01.560 --> 0:35:03.640
<v Speaker 1>to the Sun and still have a moon. We're quite

0:35:03.680 --> 0:35:06.600
<v Speaker 1>a cozy distance from the Sun. I don't know exactly

0:35:06.600 --> 0:35:08.000
<v Speaker 1>the number of how close it could be.

0:35:08.239 --> 0:35:11.800
<v Speaker 2>Okay, Well, Daniel had hinted earlier that there is one

0:35:12.000 --> 0:35:16.239
<v Speaker 2>other candidate for a moon for Earth, and after the

0:35:16.280 --> 0:35:18.120
<v Speaker 2>break he's going to tell you about it.

0:35:18.080 --> 0:35:20.040
<v Speaker 1>And we're going to hear Kelly try to pronounce it.

0:35:20.280 --> 0:35:44.319
<v Speaker 2>Oh, we're back, and there is one other object in

0:35:44.360 --> 0:35:48.160
<v Speaker 2>the sky that is a potential candidate for another moon

0:35:48.280 --> 0:35:52.640
<v Speaker 2>for Earth. It is colloquially referred to as the space being.

0:35:53.440 --> 0:35:56.520
<v Speaker 1>And uh, how was that pronounced, Kelly? Oh?

0:35:56.600 --> 0:36:01.560
<v Speaker 2>I was trying to avoid it, Kriefney. I probably got

0:36:01.560 --> 0:36:03.440
<v Speaker 2>it right on the first try. Right, how would you

0:36:03.520 --> 0:36:09.400
<v Speaker 2>say it? Daniel? Are you looking up the pronunciation? That's cheating,

0:36:09.719 --> 0:36:10.480
<v Speaker 2>that's cheating.

0:36:12.680 --> 0:36:15.200
<v Speaker 1>I have no idea how to pronounce this. It is

0:36:15.280 --> 0:36:18.080
<v Speaker 1>such a weird word. I don't even know the etymology

0:36:18.120 --> 0:36:22.160
<v Speaker 1>of it is, or why anybody would choose this unpronounceable word.

0:36:22.600 --> 0:36:25.359
<v Speaker 1>C r u I t h n E.

0:36:25.640 --> 0:36:27.319
<v Speaker 2>I wait, you're not even going to try And you

0:36:27.360 --> 0:36:28.040
<v Speaker 2>had me do it.

0:36:28.120 --> 0:36:32.520
<v Speaker 1>First about to you interrupted me as I was about

0:36:32.560 --> 0:36:34.840
<v Speaker 1>to give it a try. I was gonna say I

0:36:34.840 --> 0:36:39.000
<v Speaker 1>would call it krithne also, but it's probably something weirder,

0:36:39.040 --> 0:36:41.280
<v Speaker 1>you know, anytime you have these weird combinations of vowels

0:36:41.280 --> 0:36:43.840
<v Speaker 1>in English, you're like, oh, actually it's Croithney or something.

0:36:44.440 --> 0:36:47.400
<v Speaker 1>So I have no idea. Let's call it the space bean.

0:36:47.719 --> 0:36:50.160
<v Speaker 2>That's great, And I'll note the three times you and

0:36:50.200 --> 0:36:55.080
<v Speaker 2>I said it. We did say it differently each time. Yeah, okay,

0:36:55.200 --> 0:36:58.200
<v Speaker 2>all right, through time. That's right. Tell me about the

0:36:58.239 --> 0:36:58.759
<v Speaker 2>space bean.

0:36:59.239 --> 0:37:02.200
<v Speaker 1>So obviously, the Earth has the Moon, which is the

0:37:02.239 --> 0:37:04.399
<v Speaker 1>major moon and the real moon we consider. But there's

0:37:04.440 --> 0:37:07.279
<v Speaker 1>also this funny object called the space bean. This is

0:37:07.320 --> 0:37:10.600
<v Speaker 1>a rock like five kilometers in diameter, and it's not

0:37:10.719 --> 0:37:12.920
<v Speaker 1>shaped like a bean. You might think, oh, does it

0:37:12.960 --> 0:37:15.240
<v Speaker 1>look like a kidney bean or a pindo bean or something.

0:37:15.440 --> 0:37:17.520
<v Speaker 1>It's just that it has a funny orbit. So its

0:37:17.640 --> 0:37:21.880
<v Speaker 1>orbit is kind of being shaped. So it's got this

0:37:21.960 --> 0:37:25.600
<v Speaker 1>elliptical orbit and principle it's orbiting the Sun and not

0:37:25.680 --> 0:37:28.200
<v Speaker 1>the Earth, but it's close enough to the Earth that

0:37:28.239 --> 0:37:30.799
<v Speaker 1>the Earth is also tugging on it, and so it's

0:37:30.840 --> 0:37:34.200
<v Speaker 1>in resonance with the Earth like it's a complicated three

0:37:34.280 --> 0:37:38.279
<v Speaker 1>body system that has found this stability to it. And

0:37:38.360 --> 0:37:41.560
<v Speaker 1>so if you look at its orbit relative to the Earth,

0:37:41.640 --> 0:37:44.720
<v Speaker 1>it moves in this sort of bean shaped pattern. Again

0:37:44.880 --> 0:37:48.080
<v Speaker 1>relative to the Earth, it's not really orbiting the Earth.

0:37:48.120 --> 0:37:50.200
<v Speaker 1>I mean sometimes the Earth is on one side of

0:37:50.239 --> 0:37:52.640
<v Speaker 1>the Sun and the space bean is on the other

0:37:52.800 --> 0:37:57.440
<v Speaker 1>side of the Sun. So it's more like how Jupiter

0:37:58.040 --> 0:38:02.040
<v Speaker 1>has asteroids that follow it and precede it in its orbit,

0:38:02.520 --> 0:38:06.120
<v Speaker 1>because those are stable points, the grange points in the

0:38:06.200 --> 0:38:07.719
<v Speaker 1>Jupiter Sun system.

0:38:07.880 --> 0:38:09.440
<v Speaker 2>Those are the Trojans, right.

0:38:09.320 --> 0:38:12.000
<v Speaker 1>Yes, exactly, the Trojans and the Greeks. You got to

0:38:12.080 --> 0:38:18.879
<v Speaker 1>keep them separated, that's right, exactly. And in the same way,

0:38:19.080 --> 0:38:22.680
<v Speaker 1>there are like some stable patterns in the Earth Sun system,

0:38:23.080 --> 0:38:25.359
<v Speaker 1>and this object has fallen into one of them.

0:38:25.760 --> 0:38:28.239
<v Speaker 2>Danielle, I have very strong opinions that this is not

0:38:28.400 --> 0:38:32.680
<v Speaker 2>a moon. This just does not feel like a moon

0:38:32.719 --> 0:38:34.279
<v Speaker 2>at all. Given what you've just told me. What do

0:38:34.320 --> 0:38:36.239
<v Speaker 2>you think, yes or no? Thumbs up? Thumbs down?

0:38:37.480 --> 0:38:39.319
<v Speaker 1>I mean, it's a fuzzy thing, but I would have

0:38:39.400 --> 0:38:43.280
<v Speaker 1>to say no, right they probably also it's not really captured,

0:38:43.320 --> 0:38:46.960
<v Speaker 1>but it is gravitationally influenced by the Earth. It's not

0:38:47.080 --> 0:38:49.680
<v Speaker 1>just in orbit around the Sun on its own. But

0:38:49.719 --> 0:38:51.879
<v Speaker 1>the thing that pushes me against calling it a moon

0:38:52.160 --> 0:38:54.320
<v Speaker 1>is it never really gets very close to the Earth.

0:38:54.719 --> 0:38:56.719
<v Speaker 1>The closest it ever gets to the Earth is like

0:38:56.840 --> 0:38:59.719
<v Speaker 1>seven and a half million miles away, which is like

0:39:00.160 --> 0:39:05.200
<v Speaker 1>thirty times farther than our current moon. So officially astronomers

0:39:05.200 --> 0:39:10.160
<v Speaker 1>call this a quasi satellite, which is like such a fudge.

0:39:09.920 --> 0:39:15.840
<v Speaker 2>Word, wishy washy. It doesn't influence our songs or mythology.

0:39:16.560 --> 0:39:21.000
<v Speaker 2>I'm I'm not emotionally feeling any connection to the space bean.

0:39:21.200 --> 0:39:23.439
<v Speaker 1>I say no, even in our family, which are big

0:39:23.480 --> 0:39:26.239
<v Speaker 1>lovers of beans and promoters of beans and every part

0:39:26.280 --> 0:39:28.959
<v Speaker 1>of people's lives. I don't think we're pro space bean

0:39:29.160 --> 0:39:30.200
<v Speaker 1>being promoted to Moon.

0:39:30.640 --> 0:39:32.799
<v Speaker 2>I call beino on the space bean.

0:39:35.960 --> 0:39:39.839
<v Speaker 1>All right. So Earth has one moon and the space bean.

0:39:40.560 --> 0:39:42.680
<v Speaker 1>So let's take a step up and talk about Mars.

0:39:42.920 --> 0:39:46.040
<v Speaker 1>Mars has two moons, and both of these moons are

0:39:46.040 --> 0:39:49.560
<v Speaker 1>fascinating because both of them are very likely captured objects

0:39:50.040 --> 0:39:53.280
<v Speaker 1>not formed with the Mars. And they also have awesome

0:39:53.360 --> 0:39:57.920
<v Speaker 1>names Phobos and demos. These things mean fear and dread.

0:39:58.719 --> 0:40:01.160
<v Speaker 2>Who means that they were having a bad day when

0:40:01.160 --> 0:40:01.799
<v Speaker 2>they named them.

0:40:01.840 --> 0:40:04.720
<v Speaker 1>I bet dark, right? So dark?

0:40:04.960 --> 0:40:06.920
<v Speaker 2>Oh, but Mars is the god of war, right, so

0:40:06.960 --> 0:40:09.360
<v Speaker 2>of course you name the moon's something dark.

0:40:09.960 --> 0:40:12.480
<v Speaker 1>Yeah, exactly, And as we'll hear later on, the name

0:40:12.520 --> 0:40:14.800
<v Speaker 1>of the moons does keep in the theme of the

0:40:14.880 --> 0:40:17.160
<v Speaker 1>name of the planet, which is kind of cool, honestly.

0:40:18.440 --> 0:40:21.400
<v Speaker 1>So Phobos is the closer one. It's larger, It's like

0:40:21.440 --> 0:40:24.880
<v Speaker 1>twenty two kilometers in size. It orbits Mars three times

0:40:24.960 --> 0:40:29.120
<v Speaker 1>every Earth day and is slowly losing its orbit because

0:40:29.160 --> 0:40:32.040
<v Speaker 1>of the atmospheric drag from being so close. So in

0:40:32.080 --> 0:40:37.680
<v Speaker 1>fifty million years, just after elon Musk finishes terraforming, Phobos

0:40:37.800 --> 0:40:40.759
<v Speaker 1>is gonna hit Mars. So that's gonna be a cataclysm. Yeah.

0:40:40.760 --> 0:40:43.680
<v Speaker 1>I know he's really worried about like the Sun expanding

0:40:43.760 --> 0:40:46.080
<v Speaker 1>and eventually destroying the Earth in a billion years, but

0:40:46.200 --> 0:40:47.440
<v Speaker 1>like this is much sooner.

0:40:48.360 --> 0:40:52.080
<v Speaker 2>But you know, you could Phobos is pretty small. Yeah,

0:40:52.120 --> 0:40:55.440
<v Speaker 2>you could push Phobos to a different orbit or something.

0:40:55.800 --> 0:40:58.000
<v Speaker 1>Yeah, yeah, probably you could. You could strap a bunch

0:40:58.040 --> 0:40:59.960
<v Speaker 1>of starships on it and push it to It's not

0:41:00.120 --> 0:41:02.319
<v Speaker 1>that big, right, It's twenty two kilometers, so it's it's

0:41:02.320 --> 0:41:03.000
<v Speaker 1>not enormous.

0:41:03.200 --> 0:41:06.360
<v Speaker 2>I mean, there is so many problems with living on Mars.

0:41:06.520 --> 0:41:08.160
<v Speaker 2>I don't know that this is the one that's the

0:41:08.200 --> 0:41:08.960
<v Speaker 2>show stopper.

0:41:09.880 --> 0:41:13.320
<v Speaker 1>No, just added to your list. And Demos is even smaller.

0:41:13.320 --> 0:41:17.960
<v Speaker 1>It's thirteen kilometers and slowered orbits further out every thirty hours.

0:41:18.560 --> 0:41:21.360
<v Speaker 1>And there was a recent visit to Demos, Like we

0:41:21.400 --> 0:41:24.000
<v Speaker 1>didn't land on it, but it came to a close approach.

0:41:24.239 --> 0:41:27.640
<v Speaker 1>This is actually a satellite launched by the Emirates and

0:41:27.760 --> 0:41:31.440
<v Speaker 1>their orbiter called Hope. So this Hope orbiter visited Demos

0:41:31.640 --> 0:41:34.320
<v Speaker 1>and looked at it carefully and learned something interesting. People

0:41:34.320 --> 0:41:37.560
<v Speaker 1>had long thought that Demos was a captured asteroid, and

0:41:37.600 --> 0:41:40.680
<v Speaker 1>Phobos almost certainly is. But it turns out that Demos

0:41:40.760 --> 0:41:44.799
<v Speaker 1>actually has a composition more similar to Mars than we expected,

0:41:45.120 --> 0:41:48.359
<v Speaker 1>so it probably isn't a captured asteroid, and yet it's

0:41:48.400 --> 0:41:51.120
<v Speaker 1>in this weird orbit, so it doesn't seem like it

0:41:51.239 --> 0:41:54.440
<v Speaker 1>formed with the planet. And the solution is that probably

0:41:55.040 --> 0:41:57.920
<v Speaker 1>Demos is an object that was tossed up from some

0:41:58.120 --> 0:42:02.520
<v Speaker 1>other major collision. Right, So, like something hit Mars, and

0:42:02.520 --> 0:42:05.160
<v Speaker 1>as we talked about this, like blows up chunks of

0:42:05.200 --> 0:42:07.439
<v Speaker 1>Mars out into space, some of which land on Earth,

0:42:07.480 --> 0:42:09.680
<v Speaker 1>but some of which could be in just the right

0:42:09.719 --> 0:42:12.640
<v Speaker 1>angle to end up in orbit. So Demos is like

0:42:12.680 --> 0:42:14.400
<v Speaker 1>a rejected piece of Mars.

0:42:14.760 --> 0:42:14.920
<v Speaker 3>Ah.

0:42:15.040 --> 0:42:16.920
<v Speaker 2>But that's not how I think of the Moon. I

0:42:16.920 --> 0:42:19.360
<v Speaker 2>don't think of it as a rejected piece of the Earth.

0:42:19.680 --> 0:42:23.240
<v Speaker 2>You watch your language Daniel, the moon might be listening.

0:42:23.960 --> 0:42:26.799
<v Speaker 1>I mean, its name is dread Okay, I don't think

0:42:26.800 --> 0:42:29.560
<v Speaker 1>it needs to be dressed up in happy language, all right.

0:42:29.480 --> 0:42:32.240
<v Speaker 2>All right, it's probably the goth equivalent of a moon. Yeah,

0:42:32.320 --> 0:42:32.800
<v Speaker 2>mm hmmm.

0:42:33.360 --> 0:42:35.600
<v Speaker 1>And these are moons. We've known about it for quite

0:42:35.640 --> 0:42:38.440
<v Speaker 1>a while. They were seen in the late eighteen hundreds

0:42:38.719 --> 0:42:41.959
<v Speaker 1>by astronomer aesof Hall, So not as long as we've

0:42:41.960 --> 0:42:44.320
<v Speaker 1>known about Jupiter's moons. But like you know, one hundred

0:42:44.320 --> 0:42:47.200
<v Speaker 1>and fifty years or so, these are not recent discoveries.

0:42:47.400 --> 0:42:50.000
<v Speaker 2>Wait, we knew about Jupiter's moons before we knew about

0:42:50.000 --> 0:42:50.920
<v Speaker 2>Mars's moons.

0:42:51.480 --> 0:42:55.439
<v Speaker 1>Yeah, Galileo discovered the first moons of Jupiter. Wow. Yeah,

0:42:55.520 --> 0:42:59.040
<v Speaker 1>quite a long time ago. But those moons are huge, right,

0:42:59.080 --> 0:43:00.640
<v Speaker 1>Some of those are big enough that they would be

0:43:00.719 --> 0:43:03.120
<v Speaker 1>planets if they weren't in orbit around Jupiter.

0:43:03.320 --> 0:43:07.120
<v Speaker 2>Holy cow. All right, So we've got Earth has one

0:43:07.239 --> 0:43:12.160
<v Speaker 2>moon and a bean, Mars has two moons. Does anybody

0:43:12.200 --> 0:43:13.560
<v Speaker 2>have three moons?

0:43:14.040 --> 0:43:14.800
<v Speaker 1>No?

0:43:14.800 --> 0:43:20.320
<v Speaker 2>No, all right, do give me four moons? Nope, five moons,

0:43:20.400 --> 0:43:20.920
<v Speaker 2>five moons.

0:43:21.000 --> 0:43:25.160
<v Speaker 1>We have Pluto right now. Pluto, of course, famous for

0:43:25.200 --> 0:43:28.000
<v Speaker 1>being an astronomical fuzzy territory. Is it a planet, is

0:43:28.040 --> 0:43:32.560
<v Speaker 1>it a dwarf planet? Whatever. Also, it has this weird moon, Sharon.

0:43:33.160 --> 0:43:36.759
<v Speaker 1>So Sharon is super weird because it's almost as big

0:43:36.800 --> 0:43:39.759
<v Speaker 1>as Pluto. It's half the size of Pluto, right, and

0:43:39.800 --> 0:43:42.520
<v Speaker 1>so it really challenges the whole concept of a moon.

0:43:43.000 --> 0:43:45.800
<v Speaker 1>It's more natural to think of the Pluto Sharon system

0:43:46.080 --> 0:43:50.880
<v Speaker 1>its binary dwarf planets. Basically, the reason that Pluto was

0:43:50.880 --> 0:43:53.759
<v Speaker 1>demoted from a planet to dwarf planet is that there's

0:43:53.880 --> 0:43:56.160
<v Speaker 1>many things like Pluto out there, and so if you

0:43:56.200 --> 0:43:58.520
<v Speaker 1>include Pluto, then you've got to include like hundreds and

0:43:58.600 --> 0:44:00.719
<v Speaker 1>hundreds of these things. And people didn't one hundreds and

0:44:00.800 --> 0:44:03.759
<v Speaker 1>hundreds of planets. Why not, I don't know, because they

0:44:03.760 --> 0:44:06.160
<v Speaker 1>wanted to think planets are special because we're on one,

0:44:06.280 --> 0:44:08.799
<v Speaker 1>and they wanted to be a protected category. This whole

0:44:08.800 --> 0:44:12.920
<v Speaker 1>thing is like so arbitrary and cultural and ridiculous. But anyway,

0:44:13.200 --> 0:44:15.279
<v Speaker 1>if you demote it to a dwarf planet, then you

0:44:15.320 --> 0:44:18.600
<v Speaker 1>really should think about Pluto and Sharon as tidally locked

0:44:18.800 --> 0:44:20.320
<v Speaker 1>binary dwarf planets.

0:44:20.680 --> 0:44:24.279
<v Speaker 2>WHOA, And so because you're not referring to Sharon as

0:44:24.400 --> 0:44:27.120
<v Speaker 2>a moon, does that mean that the center of mass

0:44:27.800 --> 0:44:30.160
<v Speaker 2>is somewhere between Pluto and Sharon.

0:44:30.320 --> 0:44:33.080
<v Speaker 1>Okay, yeah, so technically it is a moon, but like

0:44:33.719 --> 0:44:37.560
<v Speaker 1>it violates that definition as well. Okay, yeah, so really

0:44:37.560 --> 0:44:42.920
<v Speaker 1>fascinating system. Plus there's four more small moons. Hubble discovered

0:44:42.960 --> 0:44:45.839
<v Speaker 1>these just like twenty years ago, that there's four more

0:44:45.960 --> 0:44:48.880
<v Speaker 1>little bits orbiting the Pluto Sharon system. So it's a

0:44:48.920 --> 0:44:52.040
<v Speaker 1>really complex little system. They're orbiting each other and then

0:44:52.200 --> 0:44:55.320
<v Speaker 1>orbiting the two of them are four smaller moons further out.

0:44:55.760 --> 0:44:56.800
<v Speaker 1>So it's crazy.

0:44:56.920 --> 0:44:59.000
<v Speaker 2>It's crazy that we know any of this in my

0:44:59.160 --> 0:45:03.160
<v Speaker 2>fat so far away and that's amazing.

0:45:03.239 --> 0:45:06.520
<v Speaker 1>Go us, it's amazing. And there's probably more small moons

0:45:06.560 --> 0:45:09.920
<v Speaker 1>around Pluto. We just haven't seen them, right, because Pluto

0:45:10.080 --> 0:45:13.240
<v Speaker 1>is super far win. Even Hubble is challenged to see

0:45:13.280 --> 0:45:16.000
<v Speaker 1>tiny little moons that are not glowing right. You can

0:45:16.040 --> 0:45:19.320
<v Speaker 1>only see them when photons leave the Sun happy to

0:45:19.440 --> 0:45:23.120
<v Speaker 1>bounce off of these dark objects and come back to Earth.

0:45:23.600 --> 0:45:25.720
<v Speaker 1>And so if that doesn't happen, you don't see it.

0:45:25.719 --> 0:45:28.279
<v Speaker 1>It's too small, you don't see it. And so there's

0:45:28.280 --> 0:45:31.920
<v Speaker 1>almost certainly more moons of Pluto yet to be discovered.

0:45:32.040 --> 0:45:34.080
<v Speaker 1>You could find them and name them after your dog.

0:45:34.400 --> 0:45:38.200
<v Speaker 2>Well, I like that idea, Melo and Biscuit moons. But

0:45:38.480 --> 0:45:41.600
<v Speaker 2>I did read the outline, so I know that even

0:45:41.640 --> 0:45:44.839
<v Speaker 2>if we missed a handful of moons around Pluto, that

0:45:44.880 --> 0:45:48.000
<v Speaker 2>would not give Pluto the wind. So I'm guessing Pluto's

0:45:48.040 --> 0:45:50.160
<v Speaker 2>not going to win. So who is next in our list?

0:45:50.400 --> 0:45:52.000
<v Speaker 1>So next up in the ranking we got to go

0:45:52.040 --> 0:45:56.880
<v Speaker 1>all the way up to sixteen moons. Neptune has sixteen moons,

0:45:57.239 --> 0:46:00.080
<v Speaker 1>all of which are named after water gods, which is

0:46:00.160 --> 0:46:04.680
<v Speaker 1>super awesome. Maybe of course Neptune Poseidon, god of the sea,

0:46:04.800 --> 0:46:07.920
<v Speaker 1>and Neptune has a really dramatic moon with probably a

0:46:08.000 --> 0:46:11.480
<v Speaker 1>very dramatic history. So its biggest moon is called Triton,

0:46:11.719 --> 0:46:15.520
<v Speaker 1>and it was actually discovered only seventeen days after Neptune

0:46:15.560 --> 0:46:19.080
<v Speaker 1>itself was discovered. It's super fun, exactly, and the whole

0:46:19.120 --> 0:46:21.720
<v Speaker 1>history of the discovery of Neptune is really fascinating because

0:46:22.320 --> 0:46:27.000
<v Speaker 1>you can see Neptune in Galileo's logbook, like he was

0:46:27.040 --> 0:46:29.160
<v Speaker 1>observing Jupiter and he was looking at the moons, and

0:46:29.200 --> 0:46:31.440
<v Speaker 1>it just so happens that if you're looking in that

0:46:31.480 --> 0:46:34.560
<v Speaker 1>direction in the sky at that time of year, that

0:46:34.719 --> 0:46:37.200
<v Speaker 1>you would see Neptune. And he saw it there, but

0:46:37.239 --> 0:46:39.560
<v Speaker 1>he thought it was a star, and so it's there

0:46:39.600 --> 0:46:41.960
<v Speaker 1>in his log book. You can go back and reconstruct it.

0:46:42.239 --> 0:46:44.680
<v Speaker 1>And it wasn't until two hundred years later that people

0:46:44.719 --> 0:46:47.120
<v Speaker 1>figured out where Neptune was and saw it because of

0:46:47.160 --> 0:46:51.560
<v Speaker 1>its pull on Urinus. A really whole fascinating scientific history story.

0:46:51.600 --> 0:46:53.640
<v Speaker 1>I love when there's a discovery made, then you can

0:46:53.680 --> 0:46:56.360
<v Speaker 1>go back and find oh, this data actually already existed.

0:46:56.400 --> 0:46:59.000
<v Speaker 1>We could have made that discovery earlier if people had

0:46:59.080 --> 0:46:59.879
<v Speaker 1>recognized it.

0:47:00.120 --> 0:47:03.239
<v Speaker 2>Those are fun moments, yes, amazing, although not fun if

0:47:03.280 --> 0:47:06.720
<v Speaker 2>you're alive to realize that you missed. You missed that moment.

0:47:07.000 --> 0:47:09.360
<v Speaker 1>But what it says is that there's probably data in

0:47:09.400 --> 0:47:13.120
<v Speaker 1>a logbook right now that is enough to support some

0:47:13.239 --> 0:47:15.839
<v Speaker 1>crazy discovery, and we won't realize it until somebody else

0:47:15.840 --> 0:47:20.520
<v Speaker 1>figures it out. Anyway, Trenton is incredible because it orbits

0:47:20.719 --> 0:47:25.279
<v Speaker 1>retrograde to Neptune's rotation. So most moons orbit the same

0:47:25.360 --> 0:47:29.200
<v Speaker 1>direction the planet spins, because either they're formed with the

0:47:29.239 --> 0:47:32.920
<v Speaker 1>moon or they're captured that way. But Trident orbits the

0:47:32.960 --> 0:47:38.480
<v Speaker 1>opposite direction that Neptune spins, which is crazy, and probably

0:47:38.520 --> 0:47:41.279
<v Speaker 1>this is because it's captured. It's some huge object that

0:47:41.320 --> 0:47:42.400
<v Speaker 1>Neptune captured.

0:47:42.640 --> 0:47:45.160
<v Speaker 2>I always thought that retrograde was just a word you

0:47:45.200 --> 0:47:49.600
<v Speaker 2>heard in astrology horoscopes. No, it just means that you're

0:47:49.880 --> 0:47:52.440
<v Speaker 2>orbiting the opposite of the Okay.

0:47:52.360 --> 0:47:55.760
<v Speaker 1>Yeah, exactly like when planets go into retrograde, it's because

0:47:55.800 --> 0:47:58.120
<v Speaker 1>relative to the Earth, they're moving the opposite direction.

0:47:58.560 --> 0:47:59.840
<v Speaker 2>WHOA okay.

0:48:00.640 --> 0:48:03.640
<v Speaker 1>And so probably what happened here is that Neptune had

0:48:03.680 --> 0:48:06.520
<v Speaker 1>a tidy little set of moons and then Triton came

0:48:06.560 --> 0:48:09.839
<v Speaker 1>in and destroyed all of them because it came in

0:48:09.880 --> 0:48:12.040
<v Speaker 1>and it did not it went the wrong direction. It's

0:48:12.080 --> 0:48:15.040
<v Speaker 1>like driving a semi the wrong way on a freeway, right,

0:48:15.160 --> 0:48:17.640
<v Speaker 1>not cool. Yeah, And so it looks like all the

0:48:17.719 --> 0:48:20.719
<v Speaker 1>other moons, the other fifteen moons of Neptune are re

0:48:20.880 --> 0:48:24.680
<v Speaker 1>accretions of the rubble disc from Triton's capture. So Triton

0:48:24.680 --> 0:48:28.359
<v Speaker 1>comes in destroys all the moons, and then eventually they

0:48:28.400 --> 0:48:32.400
<v Speaker 1>gathered themselves together into these pathetic little objects, you know,

0:48:32.520 --> 0:48:34.720
<v Speaker 1>just remnants of this collision with Triton.

0:48:35.040 --> 0:48:37.840
<v Speaker 2>So how could you know the difference between moons that

0:48:37.880 --> 0:48:42.640
<v Speaker 2>were there before and moons that recollected after Triton destroyed everything?

0:48:43.239 --> 0:48:46.640
<v Speaker 1>So they're not in tidy circular orbits around Neptune. So

0:48:46.680 --> 0:48:49.600
<v Speaker 1>they probably are not there historically since the beginning, right,

0:48:49.640 --> 0:48:52.319
<v Speaker 1>because they're affected by this collision, and they seem to

0:48:52.320 --> 0:48:55.000
<v Speaker 1>be all sort of mixed up, a various mishmashs of

0:48:55.040 --> 0:48:58.200
<v Speaker 1>the moons and they're sort of loosely held and so

0:48:58.280 --> 0:49:00.880
<v Speaker 1>they haven't like formed together for a long time.

0:49:01.160 --> 0:49:04.320
<v Speaker 2>Amazing. And then is that all of Neptune's moons.

0:49:04.800 --> 0:49:06.800
<v Speaker 1>Those are the ones we found, and you know, these

0:49:06.840 --> 0:49:10.439
<v Speaker 1>distant planets probably have many smaller moons orbiting far out

0:49:10.440 --> 0:49:13.000
<v Speaker 1>that we just haven't been able to see. But next

0:49:13.040 --> 0:49:17.000
<v Speaker 1>up in the list is Urinus. Urinus has twenty nine moons,

0:49:17.640 --> 0:49:20.319
<v Speaker 1>and these are so many that it's useful to categorize them.

0:49:20.400 --> 0:49:23.640
<v Speaker 1>You've got the inner moons. These are like really small

0:49:23.760 --> 0:49:28.160
<v Speaker 1>objects just above the roche limit, just able to hold

0:49:28.239 --> 0:49:32.399
<v Speaker 1>themselves together. And many of these are found like last year,

0:49:32.719 --> 0:49:37.000
<v Speaker 1>so twenty twenty five with James web'space telescope. They are

0:49:37.040 --> 0:49:39.520
<v Speaker 1>so small and dark that they are not visible in

0:49:39.600 --> 0:49:42.239
<v Speaker 1>the optical and you can only see them in the infrared,

0:49:42.880 --> 0:49:45.759
<v Speaker 1>and so that's why James Web can see them. Move

0:49:45.800 --> 0:49:49.080
<v Speaker 1>a little bit further out. And you've got five major moons,

0:49:49.560 --> 0:49:51.839
<v Speaker 1>some of these are big enough to have things like

0:49:52.160 --> 0:49:56.040
<v Speaker 1>volcanism and internal magma and flow on the inside of them.

0:49:56.680 --> 0:50:00.440
<v Speaker 1>The largest one is Titania, which is one twenty the

0:50:00.480 --> 0:50:03.600
<v Speaker 1>mass of our moon, and this we've known about for

0:50:03.680 --> 0:50:08.799
<v Speaker 1>like more than two hundred years. Are you gonna make

0:50:08.840 --> 0:50:13.680
<v Speaker 1>a Titania urinus joke? Kelly has lost at people.

0:50:16.480 --> 0:50:18.959
<v Speaker 4>I have been trying to not make any comments because

0:50:19.000 --> 0:50:21.120
<v Speaker 4>I feel like there's nothing good that I can say.

0:50:21.600 --> 0:50:24.799
<v Speaker 4>But you know, all the other moons were named after

0:50:24.880 --> 0:50:28.200
<v Speaker 4>things similar, and so you know, I'm wondering, You're why,

0:50:28.560 --> 0:50:33.680
<v Speaker 4>you know, why is it Titania and not you know,

0:50:34.160 --> 0:50:38.440
<v Speaker 4>other butt related things, and so I'm just I'm not gonna, okay,

0:50:38.520 --> 0:50:42.000
<v Speaker 4>but I'm gonna focus on the science and ask you, Daniel,

0:50:42.400 --> 0:50:45.000
<v Speaker 4>is this the first moon we've talked about that could

0:50:45.080 --> 0:50:46.399
<v Speaker 4>have volcanism?

0:50:46.640 --> 0:50:48.680
<v Speaker 1>It is, yes, exactly.

0:50:48.440 --> 0:50:50.439
<v Speaker 2>What an adult I am right now.

0:50:50.120 --> 0:50:52.479
<v Speaker 1>For those of us just after the holidays who've eaten

0:50:52.520 --> 0:50:55.600
<v Speaker 1>a big meal and then, you know, produced something titanic

0:50:55.640 --> 0:50:58.560
<v Speaker 1>of our own and wondered, I wonder if that has

0:50:58.600 --> 0:51:03.840
<v Speaker 1>its own gravity could produce volcanism of its own? You know, yes, exactly,

0:51:04.280 --> 0:51:06.799
<v Speaker 1>And so the history here is also funny because it

0:51:06.880 --> 0:51:10.440
<v Speaker 1>was discovered in seventeen eighty seven, just after the planet

0:51:10.480 --> 0:51:13.640
<v Speaker 1>itself was discovered. But the guy who discovered Titania also

0:51:13.719 --> 0:51:17.160
<v Speaker 1>claimed the discovery four more moons which don't exist. What

0:51:17.600 --> 0:51:20.879
<v Speaker 1>so they were like spurious moons which later people are like, yeah,

0:51:20.920 --> 0:51:22.560
<v Speaker 1>I don't see those. I don't know what you were

0:51:22.560 --> 0:51:25.279
<v Speaker 1>looking at. And so the history here is a little

0:51:25.320 --> 0:51:25.880
<v Speaker 1>bit checkered.

0:51:25.960 --> 0:51:35.320
<v Speaker 2>Did he name the other moons like rectum war fits geer?

0:51:35.920 --> 0:51:40.239
<v Speaker 1>Moving on, outside of the major moons are ten more

0:51:40.320 --> 0:51:43.239
<v Speaker 1>irregular moons, some of which just discovered in the last

0:51:43.239 --> 0:51:45.600
<v Speaker 1>couple of years. So you know, this is an area

0:51:45.640 --> 0:51:48.400
<v Speaker 1>where we are actively learning new things about these planets.

0:51:48.600 --> 0:51:51.040
<v Speaker 2>Amazing, and what makes an irregular moon? Is it the shape?

0:51:51.280 --> 0:51:54.040
<v Speaker 1>Mm hmm. These things are not like big enough to

0:51:54.120 --> 0:51:57.480
<v Speaker 1>have pulled themselves into spheres, and so they're like weird blobs.

0:51:57.719 --> 0:52:01.520
<v Speaker 1>Some of them were also with weird orbits, probably captured objects. Cool,

0:52:01.840 --> 0:52:04.480
<v Speaker 1>all right. So then stepping up to Jupiter, this was

0:52:04.560 --> 0:52:08.360
<v Speaker 1>most people's candidate for having the most moons, just because

0:52:08.480 --> 0:52:11.200
<v Speaker 1>Jupiter is the mostest of most of the stuff, right,

0:52:11.320 --> 0:52:13.880
<v Speaker 1>It's got most of the non sun mass in the

0:52:13.920 --> 0:52:18.600
<v Speaker 1>Solar System, and indeed it has almost one hundred moons. Wow, right,

0:52:19.440 --> 0:52:23.000
<v Speaker 1>seven counted? Ninety seven moons counted for Jupiter so far,

0:52:23.719 --> 0:52:26.480
<v Speaker 1>the largest four of which were discovered hundreds of years

0:52:26.480 --> 0:52:27.640
<v Speaker 1>ago by Galileo.

0:52:27.920 --> 0:52:29.360
<v Speaker 2>WHOA, way to go, Galileo.

0:52:29.520 --> 0:52:30.120
<v Speaker 1>Yeah, exactly.

0:52:30.200 --> 0:52:32.760
<v Speaker 2>Could we all count as moons of the Sun should

0:52:32.760 --> 0:52:33.480
<v Speaker 2>the Sun win?

0:52:35.040 --> 0:52:38.920
<v Speaker 1>Are you moons of the Sun? Well? I think moons

0:52:38.920 --> 0:52:39.440
<v Speaker 1>of the Sun we.

0:52:39.440 --> 0:52:41.560
<v Speaker 2>Call planets, right, yeah, yeah, okay, I'm sorry, I'll put

0:52:41.560 --> 0:52:44.799
<v Speaker 2>down the banana peels. Let's all right, the last four

0:52:44.840 --> 0:52:48.359
<v Speaker 2>discovered by Galileo. Way to go, Galileo. Let's talk about Io.

0:52:48.480 --> 0:52:49.320
<v Speaker 2>I like Io.

0:52:49.520 --> 0:52:52.480
<v Speaker 1>Yeah, these moons are huge and likely formed with Jupiter.

0:52:52.520 --> 0:52:55.799
<v Speaker 1>They're in nice orbits around Jupiter. Io is bigger than

0:52:55.800 --> 0:52:57.799
<v Speaker 1>our moon. A lot of people think the moon is

0:52:57.800 --> 0:53:01.000
<v Speaker 1>the biggest moon in the Solar system. Not true, not

0:53:01.080 --> 0:53:03.520
<v Speaker 1>even the second biggest moon in the Solar system. Io

0:53:03.680 --> 0:53:05.600
<v Speaker 1>is not even the biggest moon in the Solar system.

0:53:05.840 --> 0:53:07.759
<v Speaker 1>But it is larger than our moon.

0:53:08.040 --> 0:53:10.799
<v Speaker 2>What moon is the biggest? Daniel We'll get there.

0:53:10.960 --> 0:53:14.200
<v Speaker 1>Oh okay, all right, all right, But Io, of course

0:53:14.320 --> 0:53:18.279
<v Speaker 1>super awesome because it has hundreds of active volcanoes on it,

0:53:18.680 --> 0:53:21.200
<v Speaker 1>and some of these things shoot plumes out like five

0:53:21.360 --> 0:53:25.680
<v Speaker 1>hundred kilometers above the surface. It's the most geologically active

0:53:25.719 --> 0:53:27.520
<v Speaker 1>object in the Solar System.

0:53:27.719 --> 0:53:28.120
<v Speaker 2>Wow.

0:53:28.200 --> 0:53:30.560
<v Speaker 1>Yeah. The reason it's got so much going on is

0:53:30.600 --> 0:53:33.000
<v Speaker 1>that it's pretty close to Jupiter, and so these tidal

0:53:33.040 --> 0:53:35.840
<v Speaker 1>forces from Jupiter are not strong enough to pull it apart,

0:53:36.160 --> 0:53:38.480
<v Speaker 1>but they do squeeze it into a football. And then

0:53:38.560 --> 0:53:41.560
<v Speaker 1>Io also is orbiting, so which part of Io is

0:53:41.560 --> 0:53:44.839
<v Speaker 1>getting squeezed into a football shape is changing, so sort

0:53:44.840 --> 0:53:47.120
<v Speaker 1>of from Io's point of view, if you're just looking

0:53:47.160 --> 0:53:49.600
<v Speaker 1>at it, it's a football, but like different parts of

0:53:49.640 --> 0:53:52.319
<v Speaker 1>it are getting footballed as it orbits Jupiter and as

0:53:52.360 --> 0:53:55.560
<v Speaker 1>it spins, so that creates a lot of internal friction.

0:53:56.040 --> 0:53:58.600
<v Speaker 1>It's just like Jupiter is reaching out with huge cosmic

0:53:58.680 --> 0:54:02.359
<v Speaker 1>hands and squeezing this thing. It's like kneading dough, right,

0:54:02.440 --> 0:54:06.160
<v Speaker 1>And so this is tidal heating. So just this gravitational

0:54:06.160 --> 0:54:09.799
<v Speaker 1>interaction between Io and Jupiter is enough to heat up

0:54:09.840 --> 0:54:12.560
<v Speaker 1>the inside of Io, and that's where you get all

0:54:12.600 --> 0:54:14.920
<v Speaker 1>these flows inside of it and this cracking of the

0:54:14.920 --> 0:54:16.560
<v Speaker 1>surface and all these volcanoes.

0:54:16.800 --> 0:54:19.920
<v Speaker 2>So is Io really hot in some spots.

0:54:19.520 --> 0:54:22.839
<v Speaker 1>Then inside of it is very toasty, yes.

0:54:22.600 --> 0:54:27.640
<v Speaker 2>Absolutely all right, But Europa. Is Europa really hot?

0:54:27.760 --> 0:54:30.640
<v Speaker 1>Eurrope is fascinating because it's icy on the surface, right,

0:54:30.719 --> 0:54:34.640
<v Speaker 1>so it's got like a crust of ice. But we've

0:54:34.680 --> 0:54:37.320
<v Speaker 1>done studies of it and we've seen that Jupiter's magnetic

0:54:37.360 --> 0:54:42.799
<v Speaker 1>field creates a current inside Europa. What which means probably

0:54:43.040 --> 0:54:47.080
<v Speaker 1>there's salt water which is capable of conducting electricity inside.

0:54:47.120 --> 0:54:50.680
<v Speaker 1>So probably you have like ten kilometers of ice and

0:54:50.719 --> 0:54:56.040
<v Speaker 1>below that maybe like one hundred kilometers of subsurface ocean. Wow,

0:54:56.120 --> 0:54:58.439
<v Speaker 1>And we think that that's water because as you get

0:54:58.480 --> 0:55:00.560
<v Speaker 1>closer to the center of Europa, like with many of

0:55:00.560 --> 0:55:03.920
<v Speaker 1>these moons, tidal heating makes things warm, and so not

0:55:04.000 --> 0:55:06.480
<v Speaker 1>only is it directly heated because of the friction, but

0:55:06.560 --> 0:55:09.920
<v Speaker 1>also they're probably like geothermal vents or hydrothermal vents on

0:55:09.960 --> 0:55:12.520
<v Speaker 1>a moon, where we're heat from the core from this

0:55:12.600 --> 0:55:16.040
<v Speaker 1>tidal heating is then leaking up equivalent to like a volcano.

0:55:16.600 --> 0:55:20.360
<v Speaker 1>So you could have enormous quantities of liquid water under

0:55:20.600 --> 0:55:22.800
<v Speaker 1>this frozen surface on Europa.

0:55:23.000 --> 0:55:24.840
<v Speaker 2>I would love to know if there's life there.

0:55:25.200 --> 0:55:28.920
<v Speaker 1>I know, right, so much possibility there for life. And

0:55:28.960 --> 0:55:31.920
<v Speaker 1>the cool thing is that sometimes it shoots stuff out

0:55:31.960 --> 0:55:35.439
<v Speaker 1>into space because you get cracks and geysers, and there's

0:55:35.440 --> 0:55:38.680
<v Speaker 1>a mission being sent Europa Clipper to go and sample

0:55:38.719 --> 0:55:42.440
<v Speaker 1>these things, like look for microbes or whatever, tiny alien

0:55:42.480 --> 0:55:44.520
<v Speaker 1>octopi or something so exciting.

0:55:45.120 --> 0:55:47.319
<v Speaker 2>Yeah, okay, all right, let's get to the largest moon now.

0:55:47.760 --> 0:55:50.560
<v Speaker 1>So the largest moon in the Solar System is Ganymede,

0:55:50.560 --> 0:55:53.440
<v Speaker 1>also Jupiter's moon. This thing is two times the mass

0:55:53.440 --> 0:55:55.839
<v Speaker 1>of our moon. Wow. So if you're like impressed by

0:55:55.840 --> 0:55:59.279
<v Speaker 1>our moon, like Ganymede is bigger than our moon by

0:55:59.280 --> 0:56:00.520
<v Speaker 1>a factor of.

0:56:00.200 --> 0:56:03.960
<v Speaker 2>Two, Well, don't rub it in. Our moon's doing a

0:56:04.000 --> 0:56:05.160
<v Speaker 2>good job.

0:56:06.520 --> 0:56:08.520
<v Speaker 1>Again. I mean, is big enough to have an atmosphere,

0:56:08.680 --> 0:56:12.200
<v Speaker 1>probably has a lot of oxygen in it, also very

0:56:12.280 --> 0:56:14.279
<v Speaker 1>likely to have a subsurface ocean. We think it has

0:56:14.320 --> 0:56:17.280
<v Speaker 1>a metal core. This thing has its own magnetic field.

0:56:17.680 --> 0:56:18.480
<v Speaker 1>It's a monster.

0:56:18.719 --> 0:56:21.160
<v Speaker 2>But I'm guessing you wouldn't want to live there because

0:56:21.160 --> 0:56:24.560
<v Speaker 2>proximity to Jupiter would make it uninhabitable. Is that right?

0:56:24.840 --> 0:56:27.440
<v Speaker 1>Yes, Jupiter puts out a lot of radiation. It's not

0:56:27.480 --> 0:56:29.279
<v Speaker 1>a star like the Sun, and it's not even a

0:56:29.280 --> 0:56:32.440
<v Speaker 1>brown dwarf. There's no fusion happening inside of it, but

0:56:32.480 --> 0:56:35.200
<v Speaker 1>there's still a lot of radiation being pumped off of Jupiter,

0:56:35.280 --> 0:56:36.960
<v Speaker 1>so not a safe place to live without a lot

0:56:37.000 --> 0:56:40.319
<v Speaker 1>of shielding, but often the place you'll find settlements in

0:56:40.800 --> 0:56:43.680
<v Speaker 1>very well written hard sci fi novels, for example, like.

0:56:43.680 --> 0:56:47.480
<v Speaker 2>The Expanse exactly all right, So Jupiter's got one hundred moons?

0:56:47.480 --> 0:56:49.279
<v Speaker 2>Are there any other moons that we need to talk

0:56:49.320 --> 0:56:51.080
<v Speaker 2>about before we move on to our winter?

0:56:51.480 --> 0:56:53.360
<v Speaker 1>So the third largest moon in the Solar system is

0:56:53.400 --> 0:56:56.799
<v Speaker 1>also a moon of Jupiter. It's Callisto. Calisto is super

0:56:56.800 --> 0:56:59.240
<v Speaker 1>interesting because its surface, unlike some of the other ones,

0:56:59.320 --> 0:57:02.840
<v Speaker 1>is very very old, so lots of craters on the

0:57:02.880 --> 0:57:06.760
<v Speaker 1>surface of Calisto. Europa, in contrast, has like a really

0:57:06.800 --> 0:57:10.759
<v Speaker 1>smooth surface, very young surface. It's constantly being reformed, so

0:57:10.760 --> 0:57:13.400
<v Speaker 1>you get a crater, it gets deleted. Callisto is showing

0:57:13.440 --> 0:57:16.120
<v Speaker 1>all of its scars, which means it's a great way

0:57:16.160 --> 0:57:18.360
<v Speaker 1>to understand the history of the Solar system, like when

0:57:18.560 --> 0:57:20.320
<v Speaker 1>was there a lot of impacts? When wasn't there?

0:57:20.440 --> 0:57:26.720
<v Speaker 2>Calisto sounds beautiful, but in a different way. Daniel, all right,

0:57:26.760 --> 0:57:28.920
<v Speaker 2>So Daniel, drum roll please.

0:57:31.720 --> 0:57:33.960
<v Speaker 1>The drama has been removed by the process of elimination.

0:57:34.160 --> 0:57:37.840
<v Speaker 1>But the winner is Saturn, and not by a little

0:57:37.840 --> 0:57:42.120
<v Speaker 1>bit Saturn has two hundred and seventy four moons right

0:57:42.360 --> 0:57:45.760
<v Speaker 1>Jupiter at ninety seven, Saturn has two hundred and seventy four.

0:57:45.800 --> 0:57:51.200
<v Speaker 1>It's crazy and these moons are amazing. Also, the biggest

0:57:51.200 --> 0:57:54.160
<v Speaker 1>one is Titan. This thing is more massive than the

0:57:54.160 --> 0:57:57.680
<v Speaker 1>planet Mercury. Okay, it's not a small moon. It's huge.

0:57:58.120 --> 0:58:00.680
<v Speaker 1>You've known about it for hundreds of years. Discovered by

0:58:00.720 --> 0:58:05.040
<v Speaker 1>Huygens in sixteen fifty five. Another one of my favorite

0:58:05.080 --> 0:58:09.320
<v Speaker 1>moons in the Solar system is ensuladis this thing like

0:58:09.400 --> 0:58:12.320
<v Speaker 1>Europa amidst jets of ice, probably because it has a

0:58:12.360 --> 0:58:16.440
<v Speaker 1>subsurface ocean. It's another great candidate for where life could form.

0:58:16.840 --> 0:58:19.880
<v Speaker 1>But maybe my favorite moon in the Solar system is

0:58:19.920 --> 0:58:23.360
<v Speaker 1>this moon of Saturn called Yupitus, which is the craziest

0:58:23.480 --> 0:58:26.960
<v Speaker 1>name for a moon. But it's shaped like a walnut.

0:58:27.320 --> 0:58:31.120
<v Speaker 1>It has this enormous ridge all the way around its equator,

0:58:31.520 --> 0:58:35.200
<v Speaker 1>like this vast set of mountains, and then the top

0:58:35.240 --> 0:58:37.280
<v Speaker 1>half of it is black and the bottom half of

0:58:37.320 --> 0:58:39.919
<v Speaker 1>it is white. It's like a black and white cookie. Yes,

0:58:40.680 --> 0:58:44.560
<v Speaker 1>this thing is crazy, exactly. Somebody took a huge space

0:58:44.640 --> 0:58:47.840
<v Speaker 1>walnut and dipped half of it in frosting. It's unbelievable.

0:58:48.480 --> 0:58:50.840
<v Speaker 1>So Saturn has all of these moons, most of them

0:58:50.960 --> 0:58:53.720
<v Speaker 1>are very far from Saturn, like two hundred and fifty

0:58:53.720 --> 0:58:57.280
<v Speaker 1>plus of these moons are distant from Saturn, orbiting with

0:58:57.360 --> 0:59:01.600
<v Speaker 1>high inclinations, almost certainly captured objects of Saturn. Saturn is

0:59:01.640 --> 0:59:04.080
<v Speaker 1>in a great place to capture all of these objects,

0:59:04.360 --> 0:59:07.600
<v Speaker 1>many of which are were like scattered by Jupiter, so

0:59:07.880 --> 0:59:10.440
<v Speaker 1>sort of like the garbage collector of the Solar system.

0:59:10.560 --> 0:59:12.720
<v Speaker 2>Okay, yes, you were able to tell us that Mercury

0:59:12.760 --> 0:59:14.800
<v Speaker 2>and Venus are too close to the Sun. That's why

0:59:14.800 --> 0:59:17.960
<v Speaker 2>they probably don't have any And Saturn probably has the

0:59:18.000 --> 0:59:20.600
<v Speaker 2>most because it's just in a good position to.

0:59:20.520 --> 0:59:23.360
<v Speaker 1>Pick up junk exactly. It's got a lot of gravity,

0:59:23.680 --> 0:59:26.560
<v Speaker 1>and it's far away from the Sun, and it's nearby Jupiter,

0:59:26.600 --> 0:59:29.840
<v Speaker 1>which creates lots of stuff tossing off of it exactly.

0:59:29.920 --> 0:59:32.920
<v Speaker 1>So over the years it's picked up a lot of moons.

0:59:33.200 --> 0:59:36.480
<v Speaker 2>Amazing. If you could visit any moon, Daniel, would it

0:59:36.480 --> 0:59:39.040
<v Speaker 2>be Yapitus? Is that how you said it?

0:59:39.560 --> 0:59:42.720
<v Speaker 1>Well, there's another moon of Saturn called Rhea, which they

0:59:42.720 --> 0:59:47.160
<v Speaker 1>think might have rings, right, because moons can have rings

0:59:47.240 --> 0:59:49.960
<v Speaker 1>usually that's unusual because the tidal effects of the planet

0:59:49.960 --> 0:59:52.800
<v Speaker 1>will disrupt it. And this is why, for example, moons

0:59:52.880 --> 0:59:56.160
<v Speaker 1>tend to not have moons, but it's easier to have

0:59:56.280 --> 0:59:59.840
<v Speaker 1>rings than moons because they're basically already torn into shreds.

1:00:00.240 --> 1:00:02.000
<v Speaker 1>So that would be pretty awesome to be on a

1:00:02.080 --> 1:00:04.640
<v Speaker 1>moon of Saturn, see the rings of Saturn and the

1:00:04.760 --> 1:00:07.600
<v Speaker 1>rings of Rhea around it. That would be pretty awesome.

1:00:07.680 --> 1:00:08.880
<v Speaker 2>That would be absolutely epic.

1:00:08.960 --> 1:00:11.960
<v Speaker 1>Yeah, and not included in today's list are the three

1:00:12.120 --> 1:00:15.200
<v Speaker 1>hundred and thirty four minor planets in our Solar system

1:00:15.360 --> 1:00:16.640
<v Speaker 1>that have their own moons.

1:00:16.840 --> 1:00:17.120
<v Speaker 2>Wow.

1:00:17.200 --> 1:00:21.280
<v Speaker 1>These things you might call moon moons or moonlitz aw.

1:00:21.720 --> 1:00:24.600
<v Speaker 2>Moonlits is cute, but moon moons is funner.

1:00:24.920 --> 1:00:29.080
<v Speaker 1>Yeah, exactly. Moon moons technically reserved for moons that have

1:00:29.200 --> 1:00:32.120
<v Speaker 1>their own moons. We haven't found any of those yet,

1:00:32.160 --> 1:00:34.320
<v Speaker 1>but it depends on you whether you call these minor

1:00:34.320 --> 1:00:37.520
<v Speaker 1>planets moons. And we're all looking forward to the day

1:00:37.640 --> 1:00:42.280
<v Speaker 1>when we can discover exo moons moons around planets in

1:00:42.400 --> 1:00:46.520
<v Speaker 1>other Solar systems. It's particularly tricky because the techniques that

1:00:46.560 --> 1:00:50.240
<v Speaker 1>we have for finding exoplanets are good at finding planets

1:00:50.240 --> 1:00:52.600
<v Speaker 1>like really close to the Sun that are really big

1:00:52.920 --> 1:00:55.439
<v Speaker 1>and it's hard for those planets to have moons they're

1:00:55.440 --> 1:00:58.240
<v Speaker 1>so close to their star. But people are working on this,

1:00:58.640 --> 1:01:02.400
<v Speaker 1>and direct imaging of planetary discs might help us discover

1:01:02.560 --> 1:01:03.400
<v Speaker 1>exo moons.

1:01:03.680 --> 1:01:05.920
<v Speaker 2>I am hoping that this happens in my lifetime. I

1:01:05.920 --> 1:01:07.320
<v Speaker 2>don't know. There's been a lot of I mean, just

1:01:07.360 --> 1:01:09.919
<v Speaker 2>hearing you talk today, there's been a lot of cool

1:01:09.920 --> 1:01:13.360
<v Speaker 2>stuff in our solar system that's been discovered in our lifetimes.

1:01:13.800 --> 1:01:16.080
<v Speaker 2>I don't know. Maybe we'll start discovering even more cool

1:01:16.080 --> 1:01:18.160
<v Speaker 2>stuff in other solar systems in our lifetimes. I don't

1:01:18.160 --> 1:01:19.000
<v Speaker 2>think it's impossible.

1:01:19.120 --> 1:01:21.640
<v Speaker 1>Yeah, and I should say there are already candidates for

1:01:21.800 --> 1:01:24.959
<v Speaker 1>exo moons because in some of these eclipse methods, where

1:01:24.960 --> 1:01:27.240
<v Speaker 1>like a planet passes in front of the star, you

1:01:27.280 --> 1:01:30.120
<v Speaker 1>can see deviations from those that might be consistent with

1:01:30.160 --> 1:01:32.880
<v Speaker 1>the moon going around that. But these are just candidates

1:01:32.880 --> 1:01:35.360
<v Speaker 1>and unconfirmed, and of course there's lots of controversy. So

1:01:35.400 --> 1:01:37.960
<v Speaker 1>I think we might be on the verge of discovering

1:01:38.080 --> 1:01:38.920
<v Speaker 1>exo moons.

1:01:39.120 --> 1:01:43.120
<v Speaker 2>Well, stay tuned. If we find moon moons or exo moons,

1:01:43.320 --> 1:01:44.120
<v Speaker 2>we will let you know.

1:01:45.200 --> 1:01:48.520
<v Speaker 1>And one day when we visit another system studying their

1:01:48.560 --> 1:01:51.720
<v Speaker 1>moons will help us understand the history of that solar system,

1:01:51.760 --> 1:01:55.760
<v Speaker 1>the cataclysms, the captures, the collisions, everything that went down

1:01:55.920 --> 1:01:57.240
<v Speaker 1>in their cosmic.

1:01:56.880 --> 1:01:59.360
<v Speaker 2>Chaos, all of the chaos from the kind of boring

1:01:59.400 --> 1:02:02.040
<v Speaker 2>stuff Daniel will still tell us about anyway, so the

1:02:02.160 --> 1:02:05.480
<v Speaker 2>much more exciting stuff, all of which we'll explain in

1:02:05.520 --> 1:02:08.160
<v Speaker 2>an exciting way. Here a Daniel and kill.

1:02:08.160 --> 1:02:12.280
<v Speaker 1>All exciting because some of it's more boring anyway. Thanks

1:02:12.280 --> 1:02:14.200
<v Speaker 1>for tuning in, everyone, and for ficking it out for

1:02:14.240 --> 1:02:17.240
<v Speaker 1>this countdown for which planet has the most moons.

1:02:24.160 --> 1:02:28.000
<v Speaker 2>Daniel and Kelly's Extraordinary Universe is produced by iHeartRadio. We

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