WEBVTT - Why Is the Moon So Big?

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<v Speaker 1>Hey, please take a second and leave us a review

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<v Speaker 1>on Apple Podcasts, Spotify, or wherever you listen to the podcast.

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<v Speaker 1>Thanks a lot. Hey, Welcome to Science Stuff, the production

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<v Speaker 1>of iHeartRadio. I'm poor, Hey Champ, and today we are

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<v Speaker 1>going to the Moon. You might think you know the moon,

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<v Speaker 1>but actually it is full of scientific mysteries. We're going

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<v Speaker 1>to be talking about where the moon came from, what

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<v Speaker 1>it's made out of, and what it can tell us

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<v Speaker 1>about how life started on Earth. So get ready to

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<v Speaker 1>go over the moon as we tackle the unanswered questions

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<v Speaker 1>about our mysterious moon enjoying. Hey everyone, Today we're talking

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<v Speaker 1>to doctor Matt Siegler. Doctor Ziegler is a planetary scientist

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<v Speaker 1>at the University of Hawaii who works on several missions

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<v Speaker 1>for NASA and the European Space Agency, including did You

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<v Speaker 1>Are the miss mission to put astronauts back on the Moon.

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<v Speaker 1>He's going to answer three questions for us. Number one,

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<v Speaker 1>where did the moon come from? As it turns out,

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<v Speaker 1>it's really unusual for us to have such a big moon.

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<v Speaker 1>Number two, why does the moon always faces the same way?

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<v Speaker 1>Wasn't always the case? And number three, why are we

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<v Speaker 1>going back to the moon? It turns out scientists have

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<v Speaker 1>identified a deep mystery about the Moon that might have

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<v Speaker 1>huge implications for space travel and our search for extraterrest

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<v Speaker 1>deal life. So here's my conversation with doctor Matt Siegler. Well,

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<v Speaker 1>thank you doctor Siegler for joining us again.

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<v Speaker 2>Okay, welcome.

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<v Speaker 1>The last time we talked it was New Year's and

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<v Speaker 1>we talked about how the Earth goes around the Sun.

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<v Speaker 1>And now we're getting close to the lunar New Year,

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<v Speaker 1>so I thought it would be interesting to talk about

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<v Speaker 1>the moon.

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<v Speaker 2>Okay, that's actually my specialties. That's great to talk about

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<v Speaker 2>something that I know.

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<v Speaker 1>Are you saying you're a lunatic?

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<v Speaker 2>Yes, yeah, we're proud to call ourselves lunatics.

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<v Speaker 1>Well, in what ways is our moon unusual in the

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<v Speaker 1>Solar System?

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<v Speaker 2>Okay? Well, the weirdest thing about our moon is how

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<v Speaker 2>big it is compared to Earth. There are a couple

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<v Speaker 2>of moons out there, some of Saturn's moons and a

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<v Speaker 2>couple of Jupiter's moons that are about the size of

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<v Speaker 2>our moon or even a little bigger. But those planets

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<v Speaker 2>are huge, right, you could fit I think it's thirteen

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<v Speaker 2>hundred earths inside of Jupiter, right, Wow, huh. And so

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<v Speaker 2>their biggest moon is a very small moon compared to

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<v Speaker 2>the size of its body, meaning.

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<v Speaker 1>Like if Jupiter had a moon that's proportionately the same

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<v Speaker 1>size as our moon, it would be like the size

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<v Speaker 1>of Saturn or something.

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<v Speaker 2>Yeah, it would be like the size of Neptune at least.

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<v Speaker 2>So yeah, And the only other planet that, if you

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<v Speaker 2>want to call it a planet that has a similar

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<v Speaker 2>is Pluto.

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<v Speaker 3>Right.

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<v Speaker 1>Oh, no, no, we don't talk about Pluto in this podcast.

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<v Speaker 2>You don't talk about about plu.

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<v Speaker 1>We don't know.

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<v Speaker 2>Pluto has a moon that's about a tenth of its

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<v Speaker 2>size or something like that.

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<v Speaker 1>But plut itself is very small, smaller than us, right,

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<v Speaker 1>smaller than our moon kind of.

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<v Speaker 2>Yeah, Pluto is around it could fit inside the continental US.

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<v Speaker 2>So it's a pretty small body.

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<v Speaker 1>Okay, Oh, that's a very polite way to say it.

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<v Speaker 1>It's a small body. Yes, yes, small body.

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<v Speaker 2>So that's the weirdest thing about our moon is how

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<v Speaker 2>big it is compared to us.

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<v Speaker 1>So that's the first mystery about the moon. Why is

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<v Speaker 1>it so big? None of the other planets have a

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<v Speaker 1>moon this big.

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<v Speaker 3>Why is that?

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<v Speaker 1>Well, as it turns out, Charles Darwin's Sun George Darwin

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<v Speaker 1>had a theory about that.

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<v Speaker 2>So that's actually a funny part of the history is

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<v Speaker 2>our moon is relatively large. It's about the size of

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<v Speaker 2>the Pacific Ocean basin, and so Charles Darwin's son, I

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<v Speaker 2>believe George Darwin first theorized that the Moon might have

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<v Speaker 2>been created from the Earth by being spit out of

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<v Speaker 2>the Pacific Ocean basin, and the Pacific Ocean was the

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<v Speaker 2>hole left behind. So that's a good way to remember

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<v Speaker 2>the size of the Moon is roughly the size of

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<v Speaker 2>the Pacific Ocean, because that was one of the first thoughts, Well, well,

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<v Speaker 2>we have a hole here on Earth that's about the

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<v Speaker 2>size of the moon.

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<v Speaker 1>Yeah, maybe that's came It was like a giant pimple

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<v Speaker 1>that just popped off the Earth. That was the theory, yes, yes,

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<v Speaker 1>or the Darwin giant pimple theory. Yeah, George Darwin didn't

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<v Speaker 1>quite get thinks is right as this famous dad Charles Darwin,

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<v Speaker 1>or did he?

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<v Speaker 2>Now we kind of think it's crazy, but really how

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<v Speaker 2>we think the moon formed now was not all that different.

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<v Speaker 2>It's just that that spitting out happened in a big

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<v Speaker 2>event when something the size of Mars or so collided

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<v Speaker 2>into the early Earth and caused that event where material

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<v Speaker 2>got spit out and formed the moon.

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<v Speaker 1>That's a wild theory, Like we have a moon that's

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<v Speaker 1>like gray white, but we think it happened because some

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<v Speaker 1>giant mini planet crashed into the original Earth.

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<v Speaker 2>Yeah, so that's the idea is the original early Solar

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<v Speaker 2>system was full of things that were flying all around,

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<v Speaker 2>and some of them collided into each other, and the

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<v Speaker 2>debris of that collision formed something kind of like a

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<v Speaker 2>ring of Saturn around the Earth. Right, it was a ring,

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<v Speaker 2>and then that coalesced together and became the Moon.

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<v Speaker 1>So like our Earth is a mix of those two

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<v Speaker 1>original planets, and the Moon is a mix of those

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<v Speaker 1>two original planets.

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<v Speaker 2>Exactly.

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<v Speaker 1>Yes, scientists think the way the moon form was that

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<v Speaker 1>a planet the size of Mars crashed into a pre

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<v Speaker 1>Earth planet about four and a half billion years ago,

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<v Speaker 1>and then the debris from that crash clumped together and

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<v Speaker 1>formed the Moon. But here's a big question, how do

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<v Speaker 1>we know that? What makes us think that's how the

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<v Speaker 1>Moon formed. Well, it turns out this idea started when

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<v Speaker 1>we first walked on the Moon.

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<v Speaker 2>And this explains basically what we found when the Apollo

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<v Speaker 2>samples were returned in the nineteen sixties and seventies. Huh,

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<v Speaker 2>was that a lot of the isotopes of atoms were

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<v Speaker 2>incredibly similar between the Earth and the Moon.

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<v Speaker 1>What do you mean isotopes?

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<v Speaker 2>So normally an atom will have the same number of

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<v Speaker 2>protons and neutrons, and so an isotope is one that

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<v Speaker 2>has different numbers of neutrons.

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<v Speaker 1>Okay than the normal one I see. And so it's

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<v Speaker 1>where for the isotopes on Earth to match the ones

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<v Speaker 1>on the Moon.

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<v Speaker 2>Yeah, So that turns out to be one of the

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<v Speaker 2>key identifiers of where something formed in the early Solar

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<v Speaker 2>System is it's the isotopes of its different atoms, and

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<v Speaker 2>particularly good one is oxygen.

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<v Speaker 1>It turns out you can tell exactly where in the

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<v Speaker 1>Solar System a piece of rock comes from by its isotopes.

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<v Speaker 1>Like a piece of rock has more of one kind

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<v Speaker 1>of oxygen or carbon, you can tell it came from

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<v Speaker 1>close to the Sun, or near Jupiter, or way out

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<v Speaker 1>at the edges of the Solar system.

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<v Speaker 2>So we think the whole Solar System essentially was a

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<v Speaker 2>big cloud of gas and dust that was leftover from

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<v Speaker 2>some other star that exploded, right, huh, And that cloud

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<v Speaker 2>kind of collust around the early Sun, and then when

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<v Speaker 2>that Sun turned on, you know, very early in the

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<v Speaker 2>Solar system four point six billion years ago, it heated

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<v Speaker 2>that cloud and basically boiled off different isotope ratios as

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<v Speaker 2>you went different distance from the Sun. And then when

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<v Speaker 2>the planets formed, out of those different isotopic ratios as

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<v Speaker 2>a function of distance away from the Sun, they seem

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<v Speaker 2>to have checked those isotopes permanently after that.

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<v Speaker 1>Interesting, it's like the rocks have a tag that says

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<v Speaker 1>where in the Solar System formed.

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<v Speaker 2>Yeah, so when we see a meteorite that we have

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<v Speaker 2>identified has come from Mars or a meteorite from the

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<v Speaker 2>Asteroid belt, these will have different oxygen isotope ratios than

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<v Speaker 2>the Earth. But the Moon has almost the same as

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<v Speaker 2>the Earth, like too incredible precision, such that the only

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<v Speaker 2>way that we can explain it was that they essentially

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<v Speaker 2>formed together as a single body. Okay, and so the

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<v Speaker 2>Earth and the Moon are incredibly similar, and it could

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<v Speaker 2>be that it's just kind of telling us they formed

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<v Speaker 2>at the exact same distance from the Sun. But the

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<v Speaker 2>precision in which they match seems to only be explained

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<v Speaker 2>if they really formed together in this idea of the

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<v Speaker 2>giant impact or simple.

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<v Speaker 1>I see the match is too good. It's just too

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<v Speaker 1>identical to the Earth.

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<v Speaker 2>Yeah, Like these are identical twins, you know, they had

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<v Speaker 2>to be born from the same mother.

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<v Speaker 1>I see the DNA says their siblings, same mother, same father.

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<v Speaker 2>Okay, And so there were lots of theory going around,

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<v Speaker 2>and as far as I understand it, there was some

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<v Speaker 2>international meeting about this in the early nineteen eighties and

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<v Speaker 2>there was a lot of debate, and then out came

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<v Speaker 2>the giant impact as the winner, and it's kind of

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<v Speaker 2>been the standard since then.

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<v Speaker 1>Interesting. So it's not like we have some smoking gun

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<v Speaker 1>that says that this is what happened, or that there

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<v Speaker 1>was a camera or somebody saw this happened. It's like, well,

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<v Speaker 1>we can't think of anything else, and this is the

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<v Speaker 1>only thing that we have left.

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<v Speaker 2>Yeah, and everything that we find out knew about the

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<v Speaker 2>Moon seems to fit with the theory of the giant impact.

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<v Speaker 2>Like what like one of the things we found out

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<v Speaker 2>was from seismometers on the Moon. We've been able to

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<v Speaker 2>figure out that the Moon has a fairly small iron core, right,

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<v Speaker 2>and the Earth actually has a really big iron core

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<v Speaker 2>for its size. And so where did this extra iron

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<v Speaker 2>on the Earth come from and the lack of iron

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<v Speaker 2>on the Moon come from. Well, it may have been

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<v Speaker 2>that you had this big impact and then more the

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<v Speaker 2>iron went into the big object than into the small

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<v Speaker 2>on it.

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<v Speaker 3>Oh.

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<v Speaker 1>I see, what do you think the junior Darwin would

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<v Speaker 1>feel now that you've disproven his theory and not lived

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<v Speaker 1>up to the greatness of the Darwin name.

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<v Speaker 2>I don't know. I think scientists by nature like to

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<v Speaker 2>know the truth or the facts about the matter, and

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<v Speaker 2>if an idea that we clung to turns out to

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<v Speaker 2>be wrong, we should kind of give it up.

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<v Speaker 3>Yeah.

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<v Speaker 2>So I think that was a strong philosophy of science

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<v Speaker 2>then and it still is today.

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<v Speaker 1>Nice all right, when we come back, we're going to

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<v Speaker 1>tackle the second big mystery about the moon, which is

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<v Speaker 1>why is the Moon always facing us the same way?

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<v Speaker 1>In case you haven't noticed, every time you look at

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<v Speaker 1>the Moon, no matter where you are on the planet

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<v Speaker 1>or what time of the month or year, it is,

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<v Speaker 1>the features on the Moon always look the same, even

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<v Speaker 1>though it's spinning around the Earth. How can it be

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<v Speaker 1>that it's training at just the right rate for it

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<v Speaker 1>to always look the same to us?

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<v Speaker 3>We'll answer that.

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<v Speaker 1>Question and more after the break.

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<v Speaker 3>We'll be right back. Hey, we'll come back.

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<v Speaker 1>We're answering questions about the moon, and so far we've

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<v Speaker 1>talked about where the moon came from four and a

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<v Speaker 1>half billion years ago and how scientists figured out what happened.

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<v Speaker 1>Now we're going to answer another big question about the moon,

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<v Speaker 1>which is why is the Moon always facing us the

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<v Speaker 1>same way? If you think about it, the Earth is

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<v Speaker 1>going around the Sun, but the Earth doesn't always face

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<v Speaker 1>the same way to the Sun. If you were standing

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<v Speaker 1>on the surface of the Sun, the Earth would look

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<v Speaker 1>like it's spinning and it would look different every time

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<v Speaker 1>you see it. But you can't say that about the Moon.

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<v Speaker 1>The features of the Moon always look the same to us.

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<v Speaker 1>The only people in history that have gotten in a

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<v Speaker 1>different view of the Moon are the Apollo astronauts that

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<v Speaker 1>went there back in the nineteen sixties. Well, the reason

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<v Speaker 1>that the Moon always looks the same to us, according

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<v Speaker 1>to Professor Matt Ziegler, has to do with the fact

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<v Speaker 1>that the Moon isn't round. Okay, next question, Matt, why

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<v Speaker 1>is the Moon always facing the same way to us?

0:12:18.720 --> 0:12:22.360
<v Speaker 2>Okay, So the moon is what we call tidally locked

0:12:23.040 --> 0:12:26.200
<v Speaker 2>which essentially means one side is always facing us.

0:12:26.280 --> 0:12:29.640
<v Speaker 1>Right. Is that another characteristic of science.

0:12:30.960 --> 0:12:33.200
<v Speaker 2>If you don't know, we give it a fancy name

0:12:33.280 --> 0:12:38.240
<v Speaker 2>and basically says this is all we know about it. Yeah.

0:12:38.280 --> 0:12:40.600
<v Speaker 2>So a lot of moons in the Solar System are

0:12:40.640 --> 0:12:42.040
<v Speaker 2>also tidally.

0:12:41.600 --> 0:12:43.640
<v Speaker 1>Locked, not just our moon.

0:12:43.760 --> 0:12:47.760
<v Speaker 2>Like Jupiter's moons gets large. Four moons are all tidally locked.

0:12:48.000 --> 0:12:51.880
<v Speaker 2>So one face of Io is always facing Jupiter, one

0:12:51.920 --> 0:12:54.120
<v Speaker 2>face of Europa is always facing Jupiter.

0:12:54.360 --> 0:12:57.320
<v Speaker 1>Whow, we're not alone. Our moon is not the only one.

0:13:00.040 --> 0:13:04.280
<v Speaker 1>The moon is what scientists call tidally locked, which basically

0:13:04.320 --> 0:13:08.719
<v Speaker 1>means it's always facing us the same way. But there

0:13:08.840 --> 0:13:11.480
<v Speaker 1>is a reason why this happens, and it has to

0:13:11.520 --> 0:13:14.960
<v Speaker 1>do with how gooey the Earth and the Moon are.

0:13:16.320 --> 0:13:21.120
<v Speaker 2>This happens essentially because of how gooey an object is.

0:13:21.600 --> 0:13:22.040
<v Speaker 3>Uh huh.

0:13:22.080 --> 0:13:25.800
<v Speaker 2>So if something's spinning and it's gooey inside, it can

0:13:25.840 --> 0:13:27.000
<v Speaker 2>dissipate energy.

0:13:27.160 --> 0:13:30.200
<v Speaker 1>Okay, meaning like if you were spinning a water balloon.

0:13:30.640 --> 0:13:34.040
<v Speaker 2>Yeah. Or a good analogy is if you're spinning a

0:13:34.400 --> 0:13:38.000
<v Speaker 2>hard boiled egg versus a normal egg. Right, the hard

0:13:38.040 --> 0:13:40.480
<v Speaker 2>boiled egg will spin and spin and spin, right, but

0:13:40.520 --> 0:13:43.640
<v Speaker 2>the non heart boiled egg will slow itself down pretty

0:13:43.679 --> 0:13:47.559
<v Speaker 2>quickly because that ah, yeah, that goo inside is kind

0:13:47.559 --> 0:13:50.679
<v Speaker 2>of churning around and dissipating energy of that spin.

0:13:51.040 --> 0:13:53.040
<v Speaker 1>I see, if I spin a raw egg in space,

0:13:53.280 --> 0:13:57.440
<v Speaker 1>it'll eventually slow down because the liquid inside is losing energy.

0:13:57.600 --> 0:14:01.520
<v Speaker 2>Yeah, And so something akin to this happens inside of

0:14:01.559 --> 0:14:04.520
<v Speaker 2>a body like the Moon that initially early on at

0:14:04.559 --> 0:14:07.880
<v Speaker 2>least had a large liquid inside of it, right.

0:14:07.880 --> 0:14:11.280
<v Speaker 1>Oh. It initially the Moon was gooey, oh yeah, because

0:14:11.280 --> 0:14:14.320
<v Speaker 1>it was formed from the giant impact right, which was

0:14:14.720 --> 0:14:19.000
<v Speaker 1>really hot and made a lot of things melt. What

0:14:19.120 --> 0:14:21.960
<v Speaker 1>doctor Ziegler is saying is that when the Moon formed,

0:14:22.120 --> 0:14:25.480
<v Speaker 1>it was probably spinning really fast, but the inside of

0:14:25.480 --> 0:14:29.720
<v Speaker 1>it was gooey. It was melted rock or lava. It

0:14:29.800 --> 0:14:32.520
<v Speaker 1>was still hot from one the huge collision that formed

0:14:32.520 --> 0:14:36.160
<v Speaker 1>the Moon happened, and that melted inside made the Moon

0:14:36.280 --> 0:14:37.200
<v Speaker 1>stop spinning.

0:14:37.920 --> 0:14:38.640
<v Speaker 3>It's sort of like.

0:14:38.600 --> 0:14:41.320
<v Speaker 1>If you take a regular plastic water bottle and you

0:14:41.400 --> 0:14:43.320
<v Speaker 1>try to toss it up into the air so that

0:14:43.400 --> 0:14:47.200
<v Speaker 1>it spins, it'll eventually stop spinning in mid air, and

0:14:47.240 --> 0:14:49.040
<v Speaker 1>that's because the water inside.

0:14:48.720 --> 0:14:50.120
<v Speaker 3>Of it slashes around.

0:14:50.880 --> 0:14:54.200
<v Speaker 1>Well, the same thing happened to the Moon, and actually

0:14:54.400 --> 0:14:56.720
<v Speaker 1>it's also happening to the Earth.

0:14:57.920 --> 0:15:00.520
<v Speaker 2>And the Moon is doing this today to the Earth. Actually,

0:15:01.400 --> 0:15:04.880
<v Speaker 2>and so the Earth is actually slowing down. Right, Our

0:15:04.960 --> 0:15:07.920
<v Speaker 2>day is twenty four hours now. It used to be

0:15:08.040 --> 0:15:11.120
<v Speaker 2>twenty two hours, and earlier on in the Earth's history

0:15:11.200 --> 0:15:15.000
<v Speaker 2>it was as short as four hours. So we think

0:15:15.040 --> 0:15:18.480
<v Speaker 2>when the Earth and Moon formed that the Earth day

0:15:18.600 --> 0:15:19.880
<v Speaker 2>was about four hours long.

0:15:20.280 --> 0:15:22.840
<v Speaker 1>Really, yeah, we were spinning that fast.

0:15:23.080 --> 0:15:26.360
<v Speaker 2>Yeah, and then the Moon has caused us to slow

0:15:26.360 --> 0:15:28.920
<v Speaker 2>down that we're now at twenty four hours a day.

0:15:29.320 --> 0:15:32.680
<v Speaker 2>What maybe in a billion years will be at twenty

0:15:32.720 --> 0:15:34.920
<v Speaker 2>five hours a day or something like that. Right.

0:15:35.080 --> 0:15:38.640
<v Speaker 1>Oh, so the reason the day feels this long is because.

0:15:38.400 --> 0:15:38.880
<v Speaker 3>Of the moon.

0:15:39.280 --> 0:15:40.520
<v Speaker 2>Yeah, it's the moon's fault.

0:15:40.880 --> 0:15:43.040
<v Speaker 1>You had a long day, Blame the moon. Howl of

0:15:43.080 --> 0:15:43.400
<v Speaker 1>the moon.

0:15:43.720 --> 0:15:46.640
<v Speaker 2>Yeah, but if your day was too short, if it

0:15:46.800 --> 0:15:48.920
<v Speaker 2>went by too fast, then think the moon.

0:15:49.000 --> 0:15:50.360
<v Speaker 1>Right, Oh yeah, that's right, that's right.

0:15:50.440 --> 0:15:53.200
<v Speaker 2>So the same way that the Earth day is slowly

0:15:53.200 --> 0:15:56.600
<v Speaker 2>getting longer because the Earth is slowing its spin, the

0:15:56.600 --> 0:15:59.440
<v Speaker 2>Moon went through something similar. It's just because the Moon

0:15:59.520 --> 0:16:03.000
<v Speaker 2>is a lot smaller, it happened a lot faster. Basically.

0:16:03.160 --> 0:16:06.840
<v Speaker 1>Okay, maybe take me back, So we had this big crash,

0:16:07.040 --> 0:16:09.320
<v Speaker 1>A lot of stuff went out there into space eventually

0:16:09.320 --> 0:16:12.760
<v Speaker 1>formed the moon. The moon had a squishy inside, meaning

0:16:12.800 --> 0:16:14.359
<v Speaker 1>like it was lava inside.

0:16:14.000 --> 0:16:17.440
<v Speaker 2>Right basically, right, Yeah, basically it's magma if it's not erupted.

0:16:19.000 --> 0:16:21.920
<v Speaker 1>Not the whole other episode. It was magma or lava

0:16:22.360 --> 0:16:25.280
<v Speaker 1>melted rock. It was melted rock, and it was spinning

0:16:25.440 --> 0:16:26.120
<v Speaker 1>super fast.

0:16:26.400 --> 0:16:26.720
<v Speaker 3>Yeah.

0:16:26.760 --> 0:16:29.400
<v Speaker 2>So we had a fast spinning Earth and a fast

0:16:29.400 --> 0:16:33.240
<v Speaker 2>spinning Moon, and basically them tugging on each other slowed

0:16:33.240 --> 0:16:35.800
<v Speaker 2>each other down. Okay, So if I was a live

0:16:35.920 --> 0:16:38.360
<v Speaker 2>bike there and on Earth, I would die because I

0:16:38.360 --> 0:16:41.360
<v Speaker 2>couldn't breathe and standing on lava. But if I could

0:16:41.360 --> 0:16:44.240
<v Speaker 2>somehow be there, my day would be four hours long,

0:16:44.600 --> 0:16:47.560
<v Speaker 2>and I would see the moon like basically spinning in place.

0:16:47.800 --> 0:16:50.040
<v Speaker 2>The Moon would look different every time I looked at it. Yeah,

0:16:50.080 --> 0:16:52.840
<v Speaker 2>you would see the far side of the moon back then.

0:16:53.160 --> 0:16:56.840
<v Speaker 1>Oh okay, And over time we slowed down and the

0:16:56.880 --> 0:17:00.119
<v Speaker 1>moon slowed down to the point where now it's always

0:17:00.160 --> 0:17:02.960
<v Speaker 1>looking at us the same way. Yes, So is it

0:17:03.160 --> 0:17:05.679
<v Speaker 1>just luck that we just happened to be alive at

0:17:05.680 --> 0:17:07.640
<v Speaker 1>a time when it's spinning. It just the right time

0:17:07.640 --> 0:17:09.720
<v Speaker 1>for it to be always looking at it, or is

0:17:09.760 --> 0:17:10.520
<v Speaker 1>it stuck there?

0:17:10.960 --> 0:17:13.640
<v Speaker 2>I wouldn't say it's that lucky, because we think it's

0:17:13.760 --> 0:17:17.840
<v Speaker 2>stuck very quickly, like in potentially a few thousand years

0:17:17.880 --> 0:17:20.919
<v Speaker 2>to less than a million years, Like the moon slowed

0:17:20.960 --> 0:17:24.840
<v Speaker 2>itself down very quickly. So the moon'spent tidally locked for

0:17:24.960 --> 0:17:28.920
<v Speaker 2>most of Earth's history, really, and then it got stuck there. Yeah,

0:17:28.960 --> 0:17:32.320
<v Speaker 2>and then it's been stuck there. And it's a little

0:17:32.440 --> 0:17:36.240
<v Speaker 2>arbitrary which side ended up stuck facing the Earth. And

0:17:36.280 --> 0:17:39.240
<v Speaker 2>that's still a debate of why the near side of

0:17:39.280 --> 0:17:40.480
<v Speaker 2>the Moon is the near side.

0:17:41.520 --> 0:17:43.800
<v Speaker 1>Okay, you might be wondering, if the Moon went from

0:17:43.840 --> 0:17:47.639
<v Speaker 1>spinning really fast to slowing down, why did it stop.

0:17:48.359 --> 0:17:50.840
<v Speaker 1>It's still going around to Earth, so why didn't the

0:17:50.880 --> 0:17:55.359
<v Speaker 1>Moon suddenly start spinning in place the other way? Well,

0:17:55.359 --> 0:17:57.840
<v Speaker 1>according to doctor Siegler, it all has to do with

0:17:57.920 --> 0:17:59.639
<v Speaker 1>the shape of the moon.

0:18:00.960 --> 0:18:03.840
<v Speaker 2>The Moon isn't a perfect sphere. It's kind of egg

0:18:03.920 --> 0:18:07.000
<v Speaker 2>shaped itself or what rugby ball shaped or whatever you

0:18:07.080 --> 0:18:09.280
<v Speaker 2>want to call it. Yeah, just slightly.

0:18:09.880 --> 0:18:13.040
<v Speaker 1>Yes, the Moon is not perfectly round. You might have

0:18:13.119 --> 0:18:16.400
<v Speaker 1>heard that the Earth is not perfectly round either. It's

0:18:16.440 --> 0:18:19.520
<v Speaker 1>a little wider around the middle or the equator. That's

0:18:19.600 --> 0:18:23.440
<v Speaker 1>because the Earth is spinning, and so it bulges out, but.

0:18:23.400 --> 0:18:24.520
<v Speaker 2>The Moon isn't round.

0:18:24.680 --> 0:18:28.399
<v Speaker 1>In a different way and for a different reason, the

0:18:28.480 --> 0:18:32.400
<v Speaker 1>Moon doesn't bulge out, it's actually stretched out. It looks

0:18:32.400 --> 0:18:35.880
<v Speaker 1>slightly closer to a rugby ball or an American football

0:18:35.880 --> 0:18:39.359
<v Speaker 1>ball with one of the pointy ends pointing at the Earth.

0:18:39.840 --> 0:18:42.480
<v Speaker 1>And the reason it's that shape isn't because it's spinning,

0:18:42.880 --> 0:18:46.080
<v Speaker 1>but because the Earth is pulling on it. As the

0:18:46.119 --> 0:18:49.200
<v Speaker 1>Moon goes in orbit around the Earth, the Earth's gravity

0:18:49.359 --> 0:18:51.560
<v Speaker 1>pulls on the Moon to keep it in that orbit,

0:18:51.920 --> 0:18:56.480
<v Speaker 1>and that causes the Moon to get stretched. And I

0:18:56.480 --> 0:18:59.600
<v Speaker 1>think I came up with a good analogy for tidal logging,

0:18:59.720 --> 0:19:01.240
<v Speaker 1>which is that sort of like if you're in a

0:19:01.280 --> 0:19:04.440
<v Speaker 1>merry go round and someone's at the edge and they're

0:19:04.560 --> 0:19:07.439
<v Speaker 1>about to fall off, like you grabbed their hand to

0:19:07.520 --> 0:19:10.119
<v Speaker 1>keep them in the merry go round, and so the

0:19:10.160 --> 0:19:13.000
<v Speaker 1>centropgal force is pulling them out, but I'm holding their

0:19:13.040 --> 0:19:17.240
<v Speaker 1>hand pulling them in, and so that causes them to stretch, right.

0:19:17.760 --> 0:19:20.679
<v Speaker 2>Okay, Yeah, that would be a good description of it.

0:19:20.800 --> 0:19:23.560
<v Speaker 1>Yeah, okay, And so that's what causes the Moon to

0:19:23.760 --> 0:19:25.800
<v Speaker 1>look sort of like a football shape pointing at us.

0:19:26.160 --> 0:19:29.439
<v Speaker 2>Yeah, and at some point in the Moon's history it

0:19:29.520 --> 0:19:33.280
<v Speaker 2>became solid enough, it cooled off enough that it froze

0:19:33.320 --> 0:19:35.679
<v Speaker 2>in a football shape at that time.

0:19:36.880 --> 0:19:40.679
<v Speaker 1>Okay, so here's what scientists think happened. There was a

0:19:40.720 --> 0:19:43.879
<v Speaker 1>pre Earth planet somewhere close to our current orbit. He

0:19:44.000 --> 0:19:46.639
<v Speaker 1>got smashed by another planet about the size of Mars.

0:19:47.520 --> 0:19:50.000
<v Speaker 1>Some of the debris stayed in place and became the Earth,

0:19:50.640 --> 0:19:53.119
<v Speaker 1>and some of the debris floated out in space and

0:19:53.200 --> 0:19:57.040
<v Speaker 1>became the Moon. This new Moon was an orbit around

0:19:57.080 --> 0:19:59.720
<v Speaker 1>the new Earth, but it was gooey and melted on

0:19:59.760 --> 0:20:02.960
<v Speaker 1>the inside. That made it stop spinning in place. And

0:20:03.119 --> 0:20:05.600
<v Speaker 1>because it was being pulled around in an orbit around

0:20:05.600 --> 0:20:08.400
<v Speaker 1>the Earth, it stretched out a little to be closer

0:20:08.440 --> 0:20:11.320
<v Speaker 1>to the shape of a football pointed back at the Earth.

0:20:11.800 --> 0:20:14.600
<v Speaker 1>Then it cooled off and it got stuck in that shape.

0:20:15.040 --> 0:20:17.280
<v Speaker 1>And once it got stuck in that shape, it became

0:20:17.359 --> 0:20:21.040
<v Speaker 1>tidally locked, with one end of the football always pointing.

0:20:20.920 --> 0:20:21.520
<v Speaker 3>At the Earth.

0:20:22.960 --> 0:20:24.720
<v Speaker 1>Wait, wait, wait, wait, I think what you're saying is

0:20:24.760 --> 0:20:27.199
<v Speaker 1>that just because of the particular history of when the

0:20:27.240 --> 0:20:30.600
<v Speaker 1>Moon cooled is the reason we're always seeing the same side.

0:20:30.640 --> 0:20:34.560
<v Speaker 1>Because if it had stay squisher longer. Maybe the moon

0:20:34.560 --> 0:20:36.600
<v Speaker 1>would be rounder now, less football.

0:20:36.240 --> 0:20:39.120
<v Speaker 2>Shape, maybe, but I think it would still become tidally

0:20:39.160 --> 0:20:40.119
<v Speaker 2>locked eventually.

0:20:40.280 --> 0:20:41.800
<v Speaker 3>Yeah. Okay, that's good.

0:20:42.000 --> 0:20:44.119
<v Speaker 2>That's a good thought. I have to think about that

0:20:44.160 --> 0:20:47.040
<v Speaker 2>one more than live on the air.

0:20:48.600 --> 0:20:50.080
<v Speaker 1>Am I gonna get my name in a paper?

0:20:50.119 --> 0:20:52.800
<v Speaker 2>Now? The cham.

0:20:54.960 --> 0:20:59.680
<v Speaker 1>The cham procrastinating hot football theory of moon tidal walking. Yes,

0:21:01.040 --> 0:21:02.800
<v Speaker 1>rolls off the tongue exactly.

0:21:03.600 --> 0:21:03.919
<v Speaker 3>Okay.

0:21:04.000 --> 0:21:06.880
<v Speaker 1>There are a couple of interesting things about this scenario.

0:21:07.280 --> 0:21:10.200
<v Speaker 1>The first is that the arrangement of having something football

0:21:10.280 --> 0:21:14.720
<v Speaker 1>shape pointing at you in orbit is stable, meaning that

0:21:14.760 --> 0:21:17.920
<v Speaker 1>if the football, for some reason tilton starts to point

0:21:17.960 --> 0:21:21.080
<v Speaker 1>in a different direction, the physics of the orbit will

0:21:21.119 --> 0:21:25.200
<v Speaker 1>make it snap back. Remember the analogy of keeping someone

0:21:25.200 --> 0:21:27.720
<v Speaker 1>from falling off a merry go round if they start

0:21:27.720 --> 0:21:30.760
<v Speaker 1>to twist or turn, the fact that you're grabbing their

0:21:30.840 --> 0:21:33.080
<v Speaker 1>hand and pulling on them towards the center of the

0:21:33.119 --> 0:21:36.640
<v Speaker 1>merry go round means to'll go back to the same position.

0:21:37.200 --> 0:21:39.600
<v Speaker 1>And that is why the moon is always facing us

0:21:39.640 --> 0:21:42.720
<v Speaker 1>the same way. We're basically looking at one of the

0:21:42.760 --> 0:21:46.320
<v Speaker 1>pointy ends of the football shaped moon. It's part of

0:21:46.359 --> 0:21:49.040
<v Speaker 1>the moon that we never see that's the other pointy

0:21:49.160 --> 0:21:53.879
<v Speaker 1>end of the football. Oh I see. So, like if

0:21:53.920 --> 0:21:55.840
<v Speaker 1>I took the moon right now and I flipped it

0:21:55.920 --> 0:21:58.359
<v Speaker 1>one to eighty degrees, we would be looking at the

0:21:58.400 --> 0:22:00.640
<v Speaker 1>different side of the moon, but it would stay locked

0:22:00.640 --> 0:22:05.480
<v Speaker 1>to that side of the moon. Yes, Oh, fascinating. Somebody

0:22:05.520 --> 0:22:06.359
<v Speaker 1>should do that, man.

0:22:06.680 --> 0:22:09.159
<v Speaker 2>Yeah, if they were like a giant impact or someone

0:22:09.359 --> 0:22:12.000
<v Speaker 2>crashed a really really big rocket into the Moon, that

0:22:12.000 --> 0:22:14.840
<v Speaker 2>they were enough to unlock it, you could have imagined

0:22:14.840 --> 0:22:16.680
<v Speaker 2>that it would lock again in that other way.

0:22:17.640 --> 0:22:19.800
<v Speaker 1>Like I'm tired of seeing this side of the moon, Like,

0:22:19.960 --> 0:22:22.320
<v Speaker 1>I'm done with it, Let's see the other side. Somebody's

0:22:22.320 --> 0:22:24.480
<v Speaker 1>give it a little push and it'll lock back to

0:22:24.560 --> 0:22:26.240
<v Speaker 1>the other side exactly. Yeah.

0:22:27.080 --> 0:22:27.399
<v Speaker 3>Okay.

0:22:27.440 --> 0:22:29.280
<v Speaker 1>You might be wondering, why would I want to look

0:22:29.359 --> 0:22:31.960
<v Speaker 1>at the other side of the moon? Is it really

0:22:31.960 --> 0:22:35.199
<v Speaker 1>that different? Well, it turns out that it is different,

0:22:35.480 --> 0:22:37.960
<v Speaker 1>and scientists don't really know why.

0:22:38.680 --> 0:22:40.760
<v Speaker 2>But there are all these weird things we've learned about

0:22:40.800 --> 0:22:42.880
<v Speaker 2>the moon. Now, is that the crust on the far

0:22:42.960 --> 0:22:45.000
<v Speaker 2>side of the moon is a lot thicker than the

0:22:45.040 --> 0:22:47.560
<v Speaker 2>crust on the near side of the moon. Whoa, and

0:22:48.160 --> 0:22:49.720
<v Speaker 2>like the near side of the moon has all the

0:22:49.800 --> 0:22:53.159
<v Speaker 2>lava flows right far side has none of that? What?

0:22:53.960 --> 0:22:56.120
<v Speaker 2>And so why did the near side of the moon

0:22:56.160 --> 0:22:58.280
<v Speaker 2>and the far side of the moon end up so different?

0:22:58.840 --> 0:23:01.800
<v Speaker 2>And is that because of the tidal locking or is

0:23:01.840 --> 0:23:05.600
<v Speaker 2>it a cause of why we tidally locked with this face?

0:23:05.880 --> 0:23:08.719
<v Speaker 1>Did it tidally lock because one side is different than

0:23:08.720 --> 0:23:10.560
<v Speaker 1>the other? Or is one side different than the other

0:23:10.720 --> 0:23:14.119
<v Speaker 1>because it's going around the Earth always facing the same way.

0:23:14.240 --> 0:23:18.160
<v Speaker 2>Yeah, And there are different ideas about what caused that difference.

0:23:18.240 --> 0:23:20.800
<v Speaker 2>That the Moon might have had a giant impact of

0:23:20.840 --> 0:23:25.679
<v Speaker 2>its own that created the difference originally, or that just

0:23:25.920 --> 0:23:28.439
<v Speaker 2>imagine you tidally locked when you're still really close to

0:23:28.480 --> 0:23:30.760
<v Speaker 2>the Earth and the Earth is still a molten ball

0:23:30.800 --> 0:23:35.480
<v Speaker 2>of lava, but it really heats one side more than

0:23:35.560 --> 0:23:38.320
<v Speaker 2>the other. Yeah, and that could cause a difference. So

0:23:38.359 --> 0:23:40.520
<v Speaker 2>there are a number of theories out there of how

0:23:40.600 --> 0:23:43.560
<v Speaker 2>that would cause the near side on the far side

0:23:43.640 --> 0:23:45.600
<v Speaker 2>to be different in the way they are.

0:23:47.920 --> 0:23:50.359
<v Speaker 1>In other words, we sort of know why the moon

0:23:50.520 --> 0:23:53.120
<v Speaker 1>is always facing us the same way, but we don't

0:23:53.160 --> 0:23:56.280
<v Speaker 1>know why it's this side of the Moon that's facing us.

0:23:56.760 --> 0:23:59.680
<v Speaker 1>It could have been random, or there could be more things,

0:23:59.800 --> 0:24:04.160
<v Speaker 1>but the moon and its history that we don't know about. Okay,

0:24:04.200 --> 0:24:06.439
<v Speaker 1>when we come back, we're going to tackle the last

0:24:06.600 --> 0:24:10.600
<v Speaker 1>mystery of the Moon, and it's a big one. It's

0:24:10.640 --> 0:24:13.719
<v Speaker 1>a secret that could determine the future of space travel

0:24:14.080 --> 0:24:17.639
<v Speaker 1>and it could help us understand the reason why there's

0:24:17.800 --> 0:24:20.720
<v Speaker 1>life on Earth. So stay with us.

0:24:21.160 --> 0:24:22.120
<v Speaker 3>We'll be right back.

0:24:32.720 --> 0:24:35.680
<v Speaker 1>Hey, welcome back. We're not going to tackle the big

0:24:35.760 --> 0:24:39.320
<v Speaker 1>open questions about the Moon. It turns out there's a

0:24:39.320 --> 0:24:42.159
<v Speaker 1>lot we don't know about the Moon, including a question

0:24:42.400 --> 0:24:45.480
<v Speaker 1>that might have huge implications for the future of space

0:24:45.520 --> 0:24:49.160
<v Speaker 1>travel and what we know about how life started on Earth.

0:24:49.720 --> 0:24:53.320
<v Speaker 1>Here's doctor Matt Ziegler, a planetary scientist involved in the

0:24:53.359 --> 0:25:01.359
<v Speaker 1>New Artemis mission stake astronauts back to the Moon. Okay, Matt,

0:25:01.720 --> 0:25:04.359
<v Speaker 1>what don't we know about the Moon? What are some

0:25:04.400 --> 0:25:06.639
<v Speaker 1>of the biggest mysteries we're trying to figure out right now?

0:25:06.840 --> 0:25:11.320
<v Speaker 2>Oh? Yeah, that depends on which subdiscipline of lunar science

0:25:11.359 --> 0:25:11.720
<v Speaker 2>you're in.

0:25:11.840 --> 0:25:15.520
<v Speaker 1>I think, really, what flavor of lunatic are you? So?

0:25:16.240 --> 0:25:18.520
<v Speaker 2>One thing we don't know about is what's on the

0:25:18.560 --> 0:25:19.440
<v Speaker 2>interior of the Moon.

0:25:19.680 --> 0:25:20.159
<v Speaker 1>We don't know.

0:25:20.640 --> 0:25:22.919
<v Speaker 2>Yeah, we have lots of pictures of the surface of

0:25:22.920 --> 0:25:25.320
<v Speaker 2>the Moon. We know that sometimes stuff came up from

0:25:25.320 --> 0:25:27.200
<v Speaker 2>the surface of the moon, But we want to figure

0:25:27.240 --> 0:25:30.560
<v Speaker 2>out what's going on inside of the moon and how.

0:25:30.359 --> 0:25:32.440
<v Speaker 1>Wait wait before in the episode, you told me that

0:25:32.640 --> 0:25:34.760
<v Speaker 1>we know how much iron is inside the moon.

0:25:35.119 --> 0:25:38.120
<v Speaker 2>Yeah, we know kind of basic things that like, the

0:25:38.119 --> 0:25:41.800
<v Speaker 2>moon has these different layers and they're about this big.

0:25:42.080 --> 0:25:44.560
<v Speaker 2>And we know that because in the nineteen seventies we

0:25:44.640 --> 0:25:48.800
<v Speaker 2>had seismometers around the moon that we're recording moonquakes.

0:25:49.080 --> 0:25:49.520
<v Speaker 3>Uh huh.

0:25:49.520 --> 0:25:53.719
<v Speaker 2>And so from listening to a moonquake, you can tell

0:25:54.000 --> 0:25:56.159
<v Speaker 2>kind of how thick the different layers are, what the

0:25:56.200 --> 0:25:59.800
<v Speaker 2>density of the interior is, but you don't really know

0:25:59.840 --> 0:26:03.400
<v Speaker 2>the composition entirely. You're kind of guessing based on density.

0:26:03.640 --> 0:26:05.200
<v Speaker 2>And so one of the ways you can figure out

0:26:05.200 --> 0:26:08.920
<v Speaker 2>the composition is by measuring how much heat is coming out.

0:26:09.760 --> 0:26:12.320
<v Speaker 1>Yes, it turns out we don't know exactly what the

0:26:12.440 --> 0:26:15.760
<v Speaker 1>inside of the Moon is made out of. So one

0:26:15.800 --> 0:26:18.359
<v Speaker 1>project doctor Siger is working on is to take the

0:26:18.400 --> 0:26:22.760
<v Speaker 1>moon's temperature. There are radioactive elements inside the Moon that

0:26:22.800 --> 0:26:26.280
<v Speaker 1>are giving off heat, and so by burying thermometers all

0:26:26.320 --> 0:26:29.920
<v Speaker 1>over the moon, you could reconstruct what all those radioactive

0:26:29.920 --> 0:26:31.080
<v Speaker 1>elements are.

0:26:32.560 --> 0:26:35.840
<v Speaker 2>And just this last year about a year ago now,

0:26:35.920 --> 0:26:39.280
<v Speaker 2>we had the first geothermal heat flow probe since then

0:26:39.520 --> 0:26:42.119
<v Speaker 2>land on the Moon with one of these missions that's

0:26:42.240 --> 0:26:43.680
<v Speaker 2>kind of leading up to Artemis.

0:26:44.200 --> 0:26:46.600
<v Speaker 1>Basically, we put a thermometer on the Moon.

0:26:46.880 --> 0:26:50.160
<v Speaker 2>Yeah, we drilled the thermometer about a meter down below

0:26:50.200 --> 0:26:53.320
<v Speaker 2>the nerve. And if we do this in enough locations

0:26:53.440 --> 0:26:55.719
<v Speaker 2>around the Moon, we can start to put together this

0:26:55.840 --> 0:26:59.400
<v Speaker 2>picture of how the heat producing elements are different around

0:26:59.480 --> 0:27:00.159
<v Speaker 2>the whole Moon.

0:27:00.440 --> 0:27:03.119
<v Speaker 1>Okay, And so the mystery is what exactly's in there?

0:27:03.240 --> 0:27:04.520
<v Speaker 1>What could be inside the moon?

0:27:04.760 --> 0:27:07.480
<v Speaker 2>Yeah? Is the material in the Moon the same or

0:27:07.520 --> 0:27:10.280
<v Speaker 2>different than the material deep inside of Earth? Right? And

0:27:10.320 --> 0:27:13.120
<v Speaker 2>that gets back to this idea did the Moon form

0:27:13.200 --> 0:27:13.800
<v Speaker 2>from the Earth?

0:27:14.080 --> 0:27:14.240
<v Speaker 1>Right?

0:27:14.359 --> 0:27:17.879
<v Speaker 2>We know that these oxygen isotopes and sauch are telling

0:27:17.960 --> 0:27:20.240
<v Speaker 2>us that the Moon and the Earth seemed to form together,

0:27:20.359 --> 0:27:22.960
<v Speaker 2>but the composition of the deep interior is going to

0:27:23.040 --> 0:27:25.960
<v Speaker 2>be another data point telling us did they form from

0:27:26.000 --> 0:27:26.720
<v Speaker 2>the same spot?

0:27:26.880 --> 0:27:28.600
<v Speaker 1>I see, what if you find that the inside of

0:27:28.640 --> 0:27:32.000
<v Speaker 1>the Moon is made out of cheese.

0:27:31.920 --> 0:27:34.359
<v Speaker 2>Well then then we better go there and mind the cheese.

0:27:36.720 --> 0:27:40.960
<v Speaker 2>It's hard milking cows. And I don't know, I think

0:27:41.000 --> 0:27:44.520
<v Speaker 2>it still might be cheaper to get cheese from cows

0:27:44.520 --> 0:27:45.000
<v Speaker 2>on the Earth.

0:27:45.119 --> 0:27:47.280
<v Speaker 1>But I don't know, but it's moon cheese. You can

0:27:47.400 --> 0:27:50.080
<v Speaker 1>charge your premium, Yes, exactly.

0:27:52.119 --> 0:27:53.680
<v Speaker 3>Okay. The last mystery.

0:27:53.320 --> 0:27:56.359
<v Speaker 1>Doctor Seeger brought up about the Moon is a pretty

0:27:56.359 --> 0:27:59.399
<v Speaker 1>interesting one. It's tied to the new Artemis missions that

0:27:59.440 --> 0:28:02.040
<v Speaker 1>you might have seen in the news, where we're bringing

0:28:02.119 --> 0:28:06.040
<v Speaker 1>astronauts back to the Moon and what they find could

0:28:06.119 --> 0:28:09.040
<v Speaker 1>revolutionize the future of space travel.

0:28:10.480 --> 0:28:12.679
<v Speaker 2>I would say. Another big mystery and one of the

0:28:12.680 --> 0:28:16.719
<v Speaker 2>big motivators of the Artemis program coming up to the

0:28:16.760 --> 0:28:20.800
<v Speaker 2>Moon and the whole international exploration of the Moon is

0:28:20.800 --> 0:28:22.600
<v Speaker 2>is their ice at the poles of the Moon.

0:28:23.040 --> 0:28:24.280
<v Speaker 1>Oh, we don't know.

0:28:24.680 --> 0:28:27.960
<v Speaker 2>No, So we have craters, and because the Moon has

0:28:28.000 --> 0:28:30.760
<v Speaker 2>a very low tilt, a crater near the pole will

0:28:30.840 --> 0:28:33.040
<v Speaker 2>literally be a place where the sun don't shine.

0:28:33.200 --> 0:28:35.920
<v Speaker 1>Right, I see, it's the moon hole. The moon hill

0:28:35.960 --> 0:28:39.360
<v Speaker 1>is where the sun don't shine. Yes, yes, it turns

0:28:39.400 --> 0:28:42.040
<v Speaker 1>out there might be places on the Moon with water

0:28:42.160 --> 0:28:44.840
<v Speaker 1>on it. At the north and south poles of the Moon,

0:28:45.160 --> 0:28:47.760
<v Speaker 1>there are craters so deep that they never get hit

0:28:47.800 --> 0:28:50.680
<v Speaker 1>by light from the sun, and because they never feel

0:28:50.680 --> 0:28:53.560
<v Speaker 1>the heat of the sun, they are super cold, which

0:28:53.640 --> 0:28:55.600
<v Speaker 1>means they could be full of ice.

0:28:56.920 --> 0:28:59.400
<v Speaker 2>And so these places on the surface of the Moon,

0:28:59.560 --> 0:29:03.040
<v Speaker 2>because get no direct sunlight, actually can be colder than

0:29:03.080 --> 0:29:06.920
<v Speaker 2>like the surface of Pluto. Whoa, And so any water

0:29:07.080 --> 0:29:10.680
<v Speaker 2>molecules that land there, you know, maybe a comet hit

0:29:10.720 --> 0:29:13.120
<v Speaker 2>the Moon, or maybe an asteroid that had like water

0:29:13.360 --> 0:29:16.800
<v Speaker 2>in its rock materials hit the Moon. Ah, that water

0:29:16.920 --> 0:29:18.680
<v Speaker 2>should stick at the poles.

0:29:19.760 --> 0:29:22.720
<v Speaker 1>That's right, there could be huge lakes of ice inside

0:29:22.720 --> 0:29:25.600
<v Speaker 1>of craters in the North and South poles of the Moon.

0:29:25.960 --> 0:29:27.920
<v Speaker 1>You might have heard on a previous episode of this

0:29:28.000 --> 0:29:31.720
<v Speaker 1>podcast or somewhere else that scientists think most of the

0:29:31.760 --> 0:29:34.840
<v Speaker 1>water that we have here on Earth actually came from

0:29:34.920 --> 0:29:38.200
<v Speaker 1>asteroids or comets that flew here from the far edges

0:29:38.240 --> 0:29:40.640
<v Speaker 1>of the Solar System. In other words, most of the

0:29:40.680 --> 0:29:43.640
<v Speaker 1>water that you drink that makes up your body could

0:29:43.680 --> 0:29:47.880
<v Speaker 1>be important. Well, the same thing probably happened on the Moon.

0:29:48.360 --> 0:29:50.920
<v Speaker 1>Must have also been hit with comets and asteroids full

0:29:50.960 --> 0:29:54.360
<v Speaker 1>of water, except that on the Moon, because there's no atmosphere,

0:29:54.800 --> 0:29:58.040
<v Speaker 1>most of that water probably evaporated into space when it

0:29:58.080 --> 0:30:02.640
<v Speaker 1>got hit by sunlight, except potentially in the craters on

0:30:02.720 --> 0:30:04.720
<v Speaker 1>the north and South poles of the Moon.

0:30:05.240 --> 0:30:06.360
<v Speaker 3>And if there's water.

0:30:06.120 --> 0:30:10.120
<v Speaker 1>There, it could have a big impact onto things. The

0:30:10.160 --> 0:30:16.520
<v Speaker 1>first is space traveling, and we're hoping that that ice

0:30:16.680 --> 0:30:19.160
<v Speaker 1>is there, both because we want, you know, astronauts to

0:30:19.240 --> 0:30:22.400
<v Speaker 1>drink martinis on the Moon and could generally stay alive

0:30:22.560 --> 0:30:23.600
<v Speaker 1>and hydrated.

0:30:23.280 --> 0:30:26.400
<v Speaker 2>Yes, and hydrated, and also that if you saw the

0:30:26.440 --> 0:30:29.720
<v Speaker 2>Space Shuttle ever launch, it had a big cloud coming out.

0:30:30.000 --> 0:30:34.080
<v Speaker 2>What that was was mostly steam. Right, So water is

0:30:34.200 --> 0:30:34.880
<v Speaker 2>rocket fuel.

0:30:35.120 --> 0:30:39.080
<v Speaker 1>You could make rocket fuel out of water. Yeah, that's right.

0:30:39.200 --> 0:30:42.479
<v Speaker 1>You can turn water into rocket fuel. It's a process

0:30:42.560 --> 0:30:46.160
<v Speaker 1>called electrolysis where you separate the H two O into

0:30:46.400 --> 0:30:49.480
<v Speaker 1>H and oh, and once you have oxygen gas and

0:30:49.600 --> 0:30:53.280
<v Speaker 1>hydrogen gas, it can burn those to push rockets further

0:30:53.360 --> 0:30:54.520
<v Speaker 1>out into space.

0:30:55.960 --> 0:30:59.520
<v Speaker 2>So basically, if we can find enough ice on the Moon,

0:31:00.040 --> 0:31:03.560
<v Speaker 2>the Moon also becomes a fueling station for our exploration

0:31:03.640 --> 0:31:07.600
<v Speaker 2>of the universe. Right, that's wow. That's another exciting thing

0:31:07.640 --> 0:31:08.120
<v Speaker 2>about it.

0:31:09.040 --> 0:31:11.600
<v Speaker 1>And the other exciting thing about finding water on the

0:31:11.640 --> 0:31:14.840
<v Speaker 1>Moon is that if there is water there in deep craters,

0:31:15.160 --> 0:31:18.040
<v Speaker 1>it would be sort of an untouched record how water

0:31:18.160 --> 0:31:22.360
<v Speaker 1>came to our solar system neighborhood billions of years ago.

0:31:23.360 --> 0:31:27.240
<v Speaker 2>It's kind of like flypaper and it essentially should record

0:31:27.440 --> 0:31:30.160
<v Speaker 2>the delivery of this water to the Moon.

0:31:30.920 --> 0:31:33.360
<v Speaker 1>It might tell us like, yes, we did get water

0:31:33.480 --> 0:31:35.960
<v Speaker 1>from asteroids or comets.

0:31:35.560 --> 0:31:38.160
<v Speaker 2>Yeah, and tell us you know where the sources of

0:31:38.200 --> 0:31:41.400
<v Speaker 2>our water came from. Yeah, And this is really important

0:31:41.440 --> 0:31:45.200
<v Speaker 2>for understanding the big pictures of like, well, could there

0:31:45.240 --> 0:31:48.480
<v Speaker 2>be life somewhere else out there? Right, because now we're

0:31:48.480 --> 0:31:51.480
<v Speaker 2>finding all these other solar systems. And did the same

0:31:51.600 --> 0:31:55.840
<v Speaker 2>thing that caused water to somehow come from outside the

0:31:55.880 --> 0:31:59.920
<v Speaker 2>outer Solar System to Earth? Is that a common process

0:32:00.040 --> 0:32:02.320
<v Speaker 2>that happens in every solar system or is it a

0:32:02.360 --> 0:32:05.320
<v Speaker 2>weird thing that only happened in our Solar system?

0:32:05.560 --> 0:32:05.760
<v Speaker 3>Yeah?

0:32:05.960 --> 0:32:08.040
<v Speaker 2>That you would have a planet that's warm enough to

0:32:08.080 --> 0:32:11.440
<v Speaker 2>live on because we're close but also wet.

0:32:11.760 --> 0:32:14.640
<v Speaker 1>We want to know more about why Earth has water

0:32:14.880 --> 0:32:17.200
<v Speaker 1>because water is the key ingredient in life.

0:32:17.520 --> 0:32:22.040
<v Speaker 2>Yes, and the Moon holds a record of water that

0:32:22.120 --> 0:32:23.000
<v Speaker 2>the Earth does not.

0:32:23.280 --> 0:32:25.760
<v Speaker 1>You're making the Moon seem like a really good tourist stop,

0:32:26.000 --> 0:32:27.880
<v Speaker 1>Like it might have fuel for you to go to

0:32:27.920 --> 0:32:30.760
<v Speaker 1>other parts of the universe. It might have some good

0:32:30.960 --> 0:32:33.840
<v Speaker 1>history so you can read while you're there. Yeah, and

0:32:34.040 --> 0:32:38.360
<v Speaker 1>it might have some cheese inside also for your snacks. Exactly.

0:32:38.920 --> 0:32:41.600
<v Speaker 2>Yeah, So in a thousand years, the Moon might be

0:32:41.640 --> 0:32:46.520
<v Speaker 2>the wall drugs. You'll see signs for a thousand miles

0:32:46.560 --> 0:32:47.480
<v Speaker 2>before you get to the name.

0:32:48.280 --> 0:32:49.800
<v Speaker 1>It might be the BUCkies of space.

0:32:50.400 --> 0:32:52.720
<v Speaker 2>Yes, the moon is, but we've only got one.

0:32:53.800 --> 0:32:55.920
<v Speaker 1>Well, the buggies are really hard to find too, aren't they.

0:32:56.600 --> 0:32:56.800
<v Speaker 2>Yeah?

0:32:56.880 --> 0:33:02.320
<v Speaker 1>Yeah, all right, last question, Matt. When you step out

0:33:02.360 --> 0:33:04.960
<v Speaker 1>in a warm Hawaiian night you see the full moon,

0:33:05.200 --> 0:33:05.960
<v Speaker 1>what are you thinking that?

0:33:07.400 --> 0:33:10.680
<v Speaker 2>Well, just last night, I think we're out and I

0:33:10.720 --> 0:33:12.800
<v Speaker 2>saw the moon with my kids, and I said, you know,

0:33:13.080 --> 0:33:15.479
<v Speaker 2>in a couple of weeks, there's going to be people

0:33:15.800 --> 0:33:20.800
<v Speaker 2>behind that thing, right, And that thought alone is pretty

0:33:21.120 --> 0:33:24.840
<v Speaker 2>neat and exciting. Yeah, that there will be people there,

0:33:25.200 --> 0:33:27.840
<v Speaker 2>and maybe you know, in a few years it will

0:33:27.880 --> 0:33:29.520
<v Speaker 2>be all of us, right, a lot of us going

0:33:30.200 --> 0:33:33.520
<v Speaker 2>going to this gas station in the sky. Yeah, And

0:33:33.560 --> 0:33:36.600
<v Speaker 2>it's just neat to look at the Moon and knowing

0:33:36.640 --> 0:33:39.760
<v Speaker 2>about some of this history, of all the processes that

0:33:39.800 --> 0:33:42.400
<v Speaker 2>happened on the Moon, from the delivery of ice to

0:33:42.600 --> 0:33:45.040
<v Speaker 2>volcanoes on the surface of the Moon. There's a lot

0:33:45.080 --> 0:33:47.760
<v Speaker 2>of exciting stuff that you can imagine going on up there,

0:33:47.920 --> 0:33:51.040
<v Speaker 2>and you can imagine it differently on the moon because

0:33:51.080 --> 0:33:53.640
<v Speaker 2>you can see it. You know, I see Jupiter in

0:33:53.640 --> 0:33:56.000
<v Speaker 2>the night sky, and I can imagine what's going on

0:33:56.040 --> 0:33:59.200
<v Speaker 2>in that dot maybe. But the Moon is somehow this

0:33:59.280 --> 0:34:02.960
<v Speaker 2>thing that we all can relate to because it's still something.

0:34:03.040 --> 0:34:04.720
<v Speaker 2>We can see it from the Earth.

0:34:04.920 --> 0:34:06.840
<v Speaker 1>And it is a part of the Earth, right.

0:34:06.920 --> 0:34:10.120
<v Speaker 2>Yeah, it appears to be part of the Earth and

0:34:10.200 --> 0:34:13.160
<v Speaker 2>part of our formation of the Earth. And we're part

0:34:13.200 --> 0:34:15.759
<v Speaker 2>of the Earth, right We're made of the material from

0:34:15.760 --> 0:34:18.080
<v Speaker 2>the Earth too, So the moon is.

0:34:18.000 --> 0:34:22.640
<v Speaker 3>Our brother, all right.

0:34:22.960 --> 0:34:26.520
<v Speaker 1>So to recap scientists think our moon came from the

0:34:26.680 --> 0:34:30.279
<v Speaker 1>random collision of two small planets. The moon is always

0:34:30.320 --> 0:34:32.720
<v Speaker 1>facing us the same way because it's shaped a little

0:34:32.760 --> 0:34:35.759
<v Speaker 1>like an American football. We're not one hundred percent sure

0:34:36.040 --> 0:34:39.279
<v Speaker 1>what's inside of it. It could still be cheese. And

0:34:39.640 --> 0:34:42.240
<v Speaker 1>the moon might in the future serve as a gas

0:34:42.239 --> 0:34:46.040
<v Speaker 1>station for our exploration of the cosmos. So if all of

0:34:46.080 --> 0:34:49.239
<v Speaker 1>that doesn't turn you into a lunatic, I don't know

0:34:49.280 --> 0:34:53.080
<v Speaker 1>what will. Thanks for joining us. See you next time

0:34:56.080 --> 0:34:59.439
<v Speaker 1>you've been listening to science stuff. Production of Heart Radio

0:35:00.280 --> 0:35:03.239
<v Speaker 1>written and produced by me or Hey Cham, edited by

0:35:03.280 --> 0:35:07.200
<v Speaker 1>Rose Seguda, Executive producer Jerry Rowland, and audio engineer and

0:35:07.200 --> 0:35:10.640
<v Speaker 1>mixer Kasey Pegram, and you can follow me on social media.

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0:35:20.360 --> 0:35:23.320
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