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Welcome back to Cosmos in a Pod Space and Astronomy series.

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You probably look up at the moon all the time.

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Yeah.

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But have you ever stopped to think about how it got there?

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Hmm, I know I have.

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It's a truly epic origin story.

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It is.

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Cosmic chaos.

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Oh yeah.

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Violent collisions.

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Absolutely.

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And a journey from a molten world

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to the thriving planet we call home.

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That's right.

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Buckle up, it's gonna be a wild ride.

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It's a story that takes us all the way back

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to the very beginning of our solar system.

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Okay.

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4.6 billion years ago.

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Wow.

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Back then.

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Yeah.

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Imagine a swirling disk of gas and dust.

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I'm trying to picture it?

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The remnants of the sun's birth.

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Okay.

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It's in this chaotic cloud that the seeds of earth

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and the moon were sown.

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So how do we go from this swirling cloud of dust

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to a solid planet?

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Doesn't sound like those two things

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go together very well.

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It's a process called accretion.

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Okay.

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It's more exciting than it sounds.

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Think of it like a cosmic snowball effect.

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Tiny particles of dust drawn together by static electricity

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start to clump together.

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As these clumps grow, their gravity increases.

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Makes sense.

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Pulling in more and more material.

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So it's a runaway train.

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Exactly.

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Building and building until you have a planet.

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And these baby planets or protoplanets

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were forming all over the early solar system.

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Got it.

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One of these, of course, was our own earth

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forming in the inner solar system

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where it was hot enough for rocky

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and metallic materials to solidify.

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So earth was basically a giant molten ball

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of rock and metal at this point.

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It was.

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But how did it get its layered structure?

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Okay.

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The core, mantle, and crust.

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We know that's important for a lot of reasons.

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Definitely.

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But I can never remember exactly how it happened.

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That's a great question.

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It's all thanks to a process called differentiation.

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As earth grew and continued to be bombarded

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by space debris, it heated up even more.

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Eventually becoming completely molten.

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So like a giant lava lamp.

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In this molten state, heavier elements,

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like iron and nickel, sank to the center,

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forming the core.

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Meanwhile, lighter elements, like silicates,

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rose to the surface, forming the mantle and crust.

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Oh, right.

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Imagine it like a giant cosmic sorting machine.

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So the heaviest stuff sinks to the bottom

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and the lightest stuff floats to the top.

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Right.

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Just like oil and water.

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That's a good analogy.

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But on a planetary scale.

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And this layering is crucial for everything

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from plate tectonics to the earth's magnetic field.

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Wow.

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It's the foundation of the dynamic planet

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we live on today.

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Okay, so we have earth.

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Yeah.

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A molten, chaotic world.

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Yeah.

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Constantly being bombarded by meteors.

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Definitely not the place to go for a weekend getaway.

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Probably not.

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But what about the moon?

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Where does it fit into this story of fire and brimstone?

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Ah, the moon.

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Its formation is one of the most dramatic chapters

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in earth's early history.

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The leading theory, and it's a good one,

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is the giant impact hypothesis.

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Okay.

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Which suggests that the moon was born

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from a colossal collision.

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Okay, you've gotta give me more details on that one.

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All right.

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Because a colossal collision sounds pretty intense.

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Picture this.

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A Mars-sized protoplanet,

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which scientists have named Theia,

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slams into earth at an incredible speed.

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We're talking about an impact so powerful

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that it vaporizes a good chunk of earth's mantle

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and a significant portion of Theia itself.

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That's absolutely mind-blowing.

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Yeah, it is.

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So what happened to all that vaporized rock and debris

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from this epic cosmic crash?

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I can't even imagine.

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It formed a massive superheated disk of debris

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orbiting the earth over millions of years.

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Wow.

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This debris, drawn together by gravity,

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cooled and coalesced to form, you guessed it, the moon.

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So the moon is like a giant space scar

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from this ancient planetary fender bender.

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You could say that.

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That's incredible.

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But is there any actual evidence to support this theory?

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I mean, it sounds like something out

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of a science fiction movie.

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There's actually quite a bit of evidence.

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First, lunar rocks brought back from the Apollo missions

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have a chemical composition that's

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strikingly similar to Earth's mantle,

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suggesting they have a shared origin.

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So they're like cosmic siblings.

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Exactly.

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Made from the same stardust, but living different lives.

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Second, the moon is surprisingly lacking in volatile elements.

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Volatile elements.

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Things that evaporate easily at relatively low temperatures.

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Got it.

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This makes perfect sense if it formed from material that

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was superheated during a massive impact.

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Makes sense.

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All those volatile elements would have been blasted off

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into space.

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Like the impact flash baked the moon.

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Right.

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Leaving behind a very specific set of ingredients.

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Exactly.

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I never thought about it that way.

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Is there any other evidence that supports the giant impact

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theory?

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Is there?

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Think about our seasons, which are caused by the Earth's tilt

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on its axis.

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That tilt, that 23.5 degree angle,

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is likely a direct result of the giant impact.

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The collision would have knocked Earth off kilter,

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giving it the tilt we know today.

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So the moon's birth not only shaped our planet physically,

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but also gave us the seasons.

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And as a result, our climate.

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It's a pretty amazing chain of events.

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Yeah, it is.

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And we're only just starting to understand all the ways

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the moon has shaped the Earth.

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What's fascinating to me is that the early Earth-moon system

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would have looked vastly different from what

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we see today.

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OK, I'm definitely intrigued by this.

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All right.

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Paint me a picture of this early Earth-moon relationship.

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Imagine a much larger moon.

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OK, a larger moon.

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A massive glowing orb dominating the night sky.

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Wow.

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Remember, it was much closer to Earth back then.

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Right.

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And because of that proximity, the gravitational pull

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between them was much stronger, generating much stronger tidal

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forces on Earth.

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You're talking about mega tsunamis.

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We've got it.

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Way bigger than anything we see today, right?

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Yeah.

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I can imagine all that extra gravity causing some seriously

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extreme tides.

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Those incredible tidal forces also

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influenced Earth's rotation, slowly but surely putting

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the brakes on how fast it spins.

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In fact, those tidal interactions still

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happen today.

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They do.

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And are pushing the moon further away from Earth.

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Really?

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Albeit very, very slowly.

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So the moon is slowly drifting away from us.

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It is.

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A little bit every year.

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That's right.

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What a bittersweet thought.

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But I guess all good things must change.

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That's true.

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Even on a cosmic scale.

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This raises an important question for me.

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Yeah.

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What role did the moon play in making

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Earth habitable in the first place?

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Yeah, that's a good question.

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It sounds like it did a lot more than just cause tides.

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That's an excellent question.

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Oh.

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We know that the moon played a crucial role in stabilizing

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Earth's axial tilt.

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Right.

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And that stability is really important.

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It is.

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Without the moon's influence, Earth's tilt

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would fluctuate wildly, causing extreme and unpredictable

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climate swings.

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Exactly.

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So we're talking ice ages popping up randomly,

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tropical heat waves in the Arctic, basically, climate

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chaos.

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I could see how that would make it pretty hard for life

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to get a foothold.

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Very likely that complex life, as we know it,

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could never have evolved under those conditions.

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That makes sense.

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So the moon wasn't just a pretty face in the night sky.

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It acted as our planet's silent guardian,

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keeping our climate stable and allowing life to thrive.

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It really makes you appreciate all the things

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the moon does for us.

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Yeah, it does.

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And to think all that came from a giant cosmic collision

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billions of years ago.

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It's pretty remarkable.

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But even after the moon's formation,

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Earth was still a pretty wild and hostile place, right?

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Oh, it was.

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It wasn't exactly a paradise yet.

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You're right.

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It was still a world in transition.

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OK.

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But things were definitely starting to calm down a bit.

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So things were getting better.

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The constant bombardment from meteors began to ease,

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and Earth began to cool, allowing

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its crust to solidify.

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Volcanic activity became more prevalent,

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releasing gases from Earth's interior, which

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helped form the first atmosphere.

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So Earth was basically exhaling its first breath.

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And that was the beginning of the atmosphere we breathe today.

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You could say that.

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That's amazing.

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Of course, that early atmosphere was nothing

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like the air we breathe today.

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I can imagine.

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It was a hazy mix of carbon dioxide, methane, water vapor.

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Right.

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Not exactly a healthy mix for us humans.

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Definitely not.

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But this was a crucial step in Earth's journey

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toward habitability.

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This is such an incredible story.

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It is.

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But I'm sure there's a lot more to uncover about this early

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Earth and all the changes that happened.

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There is.

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It feels like we've only just scratched the surface.

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You're right about that.

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There's so much more to explore.

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Yeah.

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Maybe this is a good place to pause and pick up

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the rest of this epic tale in part two.

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I'm already hooked.

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Let's definitely continue this deep dive.

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Sounds good to me.

281
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We'll pick up right where we left off.

282
00:09:24,360 --> 00:09:26,200
Welcome back to Cosmos in a Pod.

283
00:09:26,200 --> 00:09:29,800
Last time we left off with Earth finally

284
00:09:29,800 --> 00:09:31,760
starting to chill out a bit after the drama

285
00:09:31,760 --> 00:09:32,840
of the moon's formation.

286
00:09:32,840 --> 00:09:33,340
Right.

287
00:09:33,340 --> 00:09:35,960
The cosmic dust had settled literally.

288
00:09:35,960 --> 00:09:39,360
We had a layered Earth, a brand new moon,

289
00:09:39,360 --> 00:09:42,200
and those first oceans were starting to form.

290
00:09:42,200 --> 00:09:44,000
It's really incredible.

291
00:09:44,000 --> 00:09:45,500
I'm ready to hear what happened next.

292
00:09:45,500 --> 00:09:47,320
This is where things get really exciting,

293
00:09:47,320 --> 00:09:50,200
because this is when Earth starts on its path

294
00:09:50,200 --> 00:09:52,520
to becoming the habitable planet we know and love.

295
00:09:52,520 --> 00:09:54,280
OK, set the scene for me.

296
00:09:54,280 --> 00:09:57,240
What did Earth actually look like at this point?

297
00:09:57,240 --> 00:09:59,480
Imagine a world that's still pretty hot.

298
00:09:59,480 --> 00:10:00,040
Hot.

299
00:10:00,040 --> 00:10:03,400
Volcanoes are erupting everywhere,

300
00:10:03,400 --> 00:10:07,000
spewing out lava and gases into the atmosphere.

301
00:10:07,000 --> 00:10:07,920
OK.

302
00:10:07,920 --> 00:10:10,600
The sky wouldn't have been that clear blue we're used to.

303
00:10:10,600 --> 00:10:11,120
I see.

304
00:10:11,120 --> 00:10:14,880
It would have been a hazy mix of carbon dioxide, methane,

305
00:10:14,880 --> 00:10:16,000
and water vapor.

306
00:10:16,000 --> 00:10:17,760
Not exactly breathable.

307
00:10:17,760 --> 00:10:18,640
No, not at all.

308
00:10:18,640 --> 00:10:21,880
How did we go from that toxic soup to the air we have now?

309
00:10:21,880 --> 00:10:25,800
Well, one of the key players was those newly formed oceans.

310
00:10:25,800 --> 00:10:26,960
Oh, the oceans?

311
00:10:26,960 --> 00:10:29,600
Remember, Earth was still cooling down as it did.

312
00:10:29,600 --> 00:10:30,100
Yeah.

313
00:10:30,100 --> 00:10:33,760
All that water vapor in the atmosphere started to condense

314
00:10:33,760 --> 00:10:35,720
and fell as torrential rain.

315
00:10:35,720 --> 00:10:37,400
Like mega rain.

316
00:10:37,400 --> 00:10:39,400
Talk about a bad hair day.

317
00:10:39,400 --> 00:10:40,320
I'd say so.

318
00:10:40,320 --> 00:10:42,920
This rain filled the huge basins that eventually

319
00:10:42,920 --> 00:10:44,440
became our oceans.

320
00:10:44,440 --> 00:10:47,440
So the oceans were like giant air purifiers,

321
00:10:47,440 --> 00:10:50,320
sucking up some of those harmful gases from the atmosphere.

322
00:10:50,320 --> 00:10:51,960
That's a great way to think about it.

323
00:10:51,960 --> 00:10:54,920
The oceans played a huge role in regulating

324
00:10:54,920 --> 00:10:57,480
what the early atmosphere was made of.

325
00:10:57,480 --> 00:11:00,240
They absorbed a lot of that carbon dioxide,

326
00:11:00,240 --> 00:11:03,720
which eventually got locked away in rocks and sediments.

327
00:11:03,720 --> 00:11:06,240
So they were cleaning up the atmosphere.

328
00:11:06,240 --> 00:11:07,360
Yeah, in a way.

329
00:11:07,360 --> 00:11:10,000
OK, so the oceans were like a giant carbon sink.

330
00:11:10,000 --> 00:11:10,520
Exactly.

331
00:11:10,520 --> 00:11:13,680
Pulling CO2 out of the air and cooling down the planet even

332
00:11:13,680 --> 00:11:14,160
more.

333
00:11:14,160 --> 00:11:16,440
And all that cooling was essential for life

334
00:11:16,440 --> 00:11:17,160
as we know it.

335
00:11:17,160 --> 00:11:17,840
Oh, ice?

336
00:11:17,840 --> 00:11:20,760
As the temperatures dropped, more and more of the water

337
00:11:20,760 --> 00:11:23,180
vapor in the atmosphere condensed,

338
00:11:23,180 --> 00:11:25,400
which eventually led to clearer skies

339
00:11:25,400 --> 00:11:28,120
and a more temperate, stable climate.

340
00:11:28,120 --> 00:11:30,160
So it was starting to look like a place

341
00:11:30,160 --> 00:11:31,120
we could actually live.

342
00:11:31,120 --> 00:11:32,080
Yeah, it was.

343
00:11:32,080 --> 00:11:35,440
We're getting closer and closer to the Earth we recognize.

344
00:11:35,440 --> 00:11:38,840
But there's still one big piece missing.

345
00:11:38,840 --> 00:11:39,400
Oxygen.

346
00:11:39,400 --> 00:11:39,920
Right.

347
00:11:39,920 --> 00:11:41,320
Where did that come from?

348
00:11:41,320 --> 00:11:42,640
Oxygen.

349
00:11:42,640 --> 00:11:43,280
The big one.

350
00:11:43,280 --> 00:11:44,280
The breath of life.

351
00:11:44,280 --> 00:11:45,520
That's a whole other story.

352
00:11:45,520 --> 00:11:47,080
I found a fascinating one.

353
00:11:47,080 --> 00:11:47,720
Is it really?

354
00:11:47,720 --> 00:11:51,560
See, the early atmosphere hardly had any free oxygen.

355
00:11:51,560 --> 00:11:56,440
It wasn't until photosynthetic organisms evolved billions

356
00:11:56,440 --> 00:11:57,560
of years later.

357
00:11:57,560 --> 00:11:58,320
So way later.

358
00:11:58,320 --> 00:12:00,960
That oxygen levels really started to rise.

359
00:12:00,960 --> 00:12:04,000
So those tiny bacteria are responsible for all

360
00:12:04,000 --> 00:12:05,080
the oxygen we breathe.

361
00:12:05,080 --> 00:12:05,760
Yeah.

362
00:12:05,760 --> 00:12:08,200
You're talking about those microscopic bacteria, right?

363
00:12:08,200 --> 00:12:09,800
They were just doing their thing,

364
00:12:09,800 --> 00:12:11,480
pumping out oxygen as a byproduct.

365
00:12:11,480 --> 00:12:12,680
But it was a side effect.

366
00:12:12,680 --> 00:12:14,760
And completely transformed the Earth's

367
00:12:14,760 --> 00:12:16,360
atmosphere in the process.

368
00:12:16,360 --> 00:12:18,560
It's incredible how these tiny creatures made

369
00:12:18,560 --> 00:12:19,600
such a huge impact.

370
00:12:19,600 --> 00:12:20,560
It's mind blowing.

371
00:12:20,560 --> 00:12:21,280
It is.

372
00:12:21,280 --> 00:12:24,880
The very air we breathe is a result of billions

373
00:12:24,880 --> 00:12:26,560
of years of their hard work.

374
00:12:26,560 --> 00:12:27,280
Yeah.

375
00:12:27,280 --> 00:12:28,200
Isn't that amazing?

376
00:12:28,200 --> 00:12:30,040
It really makes you appreciate those little guys,

377
00:12:30,040 --> 00:12:30,600
doesn't it?

378
00:12:30,600 --> 00:12:31,280
For sure.

379
00:12:31,280 --> 00:12:33,560
Let's shift gears back to the moon for a second.

380
00:12:33,560 --> 00:12:34,080
All right.

381
00:12:34,080 --> 00:12:37,360
We talked about how it stabilized Earth's tilt.

382
00:12:37,360 --> 00:12:40,520
But are there any other big ways the moon affected our planet?

383
00:12:40,520 --> 00:12:41,680
Oh, absolutely.

384
00:12:41,680 --> 00:12:42,080
OK.

385
00:12:42,080 --> 00:12:43,000
What else did it do?

386
00:12:43,000 --> 00:12:45,520
The moon's influence on Earth is way more profound

387
00:12:45,520 --> 00:12:47,120
than most people realize.

388
00:12:47,120 --> 00:12:47,880
Like what?

389
00:12:47,880 --> 00:12:51,000
Its gravity is the main driver of our ocean tides.

390
00:12:51,000 --> 00:12:52,160
Oh, the tides.

391
00:12:52,160 --> 00:12:54,360
Which create that rhythmic ebb and flow

392
00:12:54,360 --> 00:12:56,560
we see along our coastlines.

393
00:12:56,560 --> 00:12:58,680
Tides are definitely beautiful to look at.

394
00:12:58,680 --> 00:12:59,360
They are.

395
00:12:59,360 --> 00:13:01,040
But they also do so much more than that.

396
00:13:01,040 --> 00:13:02,440
Yeah, that's right.

397
00:13:02,440 --> 00:13:04,560
I've heard they have a huge impact on marine life

398
00:13:04,560 --> 00:13:06,040
and entire ecosystems.

399
00:13:06,040 --> 00:13:06,600
You're right.

400
00:13:06,600 --> 00:13:08,160
They're not just a pretty sight.

401
00:13:08,160 --> 00:13:08,680
Right.

402
00:13:08,680 --> 00:13:13,120
Tides play a critical role in how nutrients get distributed,

403
00:13:13,120 --> 00:13:16,240
how ocean waters mix, and even the life cycles

404
00:13:16,240 --> 00:13:18,040
of tons of marine organisms.

405
00:13:18,040 --> 00:13:18,640
Wow.

406
00:13:18,640 --> 00:13:21,560
So the moon isn't just Earth's celestial companion.

407
00:13:21,560 --> 00:13:22,200
No.

408
00:13:22,200 --> 00:13:25,160
It's a vital force shaping the planet's oceans

409
00:13:25,160 --> 00:13:26,480
and the life within them.

410
00:13:26,480 --> 00:13:29,400
You could even say that the moon's influence

411
00:13:29,400 --> 00:13:33,200
is woven into the very fabric of life on Earth.

412
00:13:33,200 --> 00:13:34,440
That's a cool way to put it.

413
00:13:34,440 --> 00:13:36,280
It's pretty profound when you think about it.

414
00:13:36,280 --> 00:13:38,680
And we can't forget that the moon is slowly

415
00:13:38,680 --> 00:13:40,080
drifting away from us.

416
00:13:40,080 --> 00:13:40,600
Right.

417
00:13:40,600 --> 00:13:41,920
We talked about that before.

418
00:13:41,920 --> 00:13:44,400
What kind of long-term impact will that have?

419
00:13:44,400 --> 00:13:47,800
I mean, is the Earth going to be OK without its moon?

420
00:13:47,800 --> 00:13:49,240
That's an important question.

421
00:13:49,240 --> 00:13:49,720
It is.

422
00:13:49,720 --> 00:13:53,680
As the moon moves further away, its gravitational pull

423
00:13:53,680 --> 00:13:55,520
on Earth weakens.

424
00:13:55,520 --> 00:13:58,400
Means the tides will become less pronounced,

425
00:13:58,400 --> 00:14:01,160
and Earth's rotation will keep slowing down.

426
00:14:01,160 --> 00:14:02,160
Oh, OK.

427
00:14:02,160 --> 00:14:04,320
Which means, you guessed it, longer days.

428
00:14:04,320 --> 00:14:05,800
Longer days sound pretty good to me.

429
00:14:05,800 --> 00:14:07,280
More time to get things done right.

430
00:14:07,280 --> 00:14:07,760
Right.

431
00:14:07,760 --> 00:14:11,520
So we'll have more time to enjoy those beach sunsets,

432
00:14:11,520 --> 00:14:12,960
even if the waves aren't as big.

433
00:14:12,960 --> 00:14:13,960
It's a trade-off.

434
00:14:13,960 --> 00:14:14,440
Yeah.

435
00:14:14,440 --> 00:14:16,200
But it's also a powerful reminder

436
00:14:16,200 --> 00:14:18,320
that nothing stays the same.

437
00:14:18,320 --> 00:14:18,840
That's true.

438
00:14:18,840 --> 00:14:20,320
Even on a cosmic scale.

439
00:14:20,320 --> 00:14:20,840
I see.

440
00:14:20,840 --> 00:14:23,280
The Earth-Moon system is always changing.

441
00:14:23,280 --> 00:14:25,880
And it's fascinating to see how these changes have influenced

442
00:14:25,880 --> 00:14:29,320
our planet's past and will continue to shape its future.

443
00:14:29,320 --> 00:14:32,320
The moon really has shaped so much of what we see around us.

444
00:14:32,320 --> 00:14:33,080
Yeah.

445
00:14:33,080 --> 00:14:35,840
Everything from our oceans to the length of our days,

446
00:14:35,840 --> 00:14:37,400
even the air we breathe.

447
00:14:37,400 --> 00:14:39,400
It's a testament to how interconnected

448
00:14:39,400 --> 00:14:40,760
the universe really is.

449
00:14:40,760 --> 00:14:41,280
It is.

450
00:14:41,280 --> 00:14:44,240
Every single object, every event,

451
00:14:44,240 --> 00:14:47,920
is part of a larger cosmic web influencing and being

452
00:14:47,920 --> 00:14:49,960
influenced by everything around it.

453
00:14:49,960 --> 00:14:51,920
It really makes you feel small, but also connected

454
00:14:51,920 --> 00:14:53,840
to something much bigger than yourself.

455
00:14:53,840 --> 00:14:57,080
That's one of the most amazing things about studying space.

456
00:14:57,080 --> 00:14:57,600
Yeah.

457
00:14:57,600 --> 00:14:59,600
It gives you that sense of wonder and connection

458
00:14:59,600 --> 00:15:01,240
to something truly grand.

459
00:15:01,240 --> 00:15:02,320
I completely agree.

460
00:15:02,320 --> 00:15:02,920
OK.

461
00:15:02,920 --> 00:15:06,240
We've covered so much ground in this deep dive.

462
00:15:06,240 --> 00:15:09,200
The moon's dramatic birth, its influence on Earth.

463
00:15:09,200 --> 00:15:11,720
We even talked about Earth's first breath.

464
00:15:11,720 --> 00:15:13,840
But I have a feeling there's more to this story.

465
00:15:13,840 --> 00:15:14,360
There is.

466
00:15:14,360 --> 00:15:14,880
Am I right?

467
00:15:14,880 --> 00:15:15,520
You are.

468
00:15:15,520 --> 00:15:18,640
There's another sign to this Earth-Moon relationship.

469
00:15:18,640 --> 00:15:23,240
And it's a bit more, let's just say, controversial.

470
00:15:23,240 --> 00:15:23,840
OK.

471
00:15:23,840 --> 00:15:25,120
Now I'm really intrigued.

472
00:15:25,120 --> 00:15:25,600
All right.

473
00:15:25,600 --> 00:15:27,280
I can't wait to hear more.

474
00:15:27,280 --> 00:15:28,720
Let's dive into that in part three.

475
00:15:28,720 --> 00:15:29,640
Sounds good to me.

476
00:15:29,640 --> 00:15:30,140
OK.

477
00:15:30,140 --> 00:15:30,880
Stay tuned.

478
00:15:30,880 --> 00:15:33,200
Welcome back to the final part of our deep dive

479
00:15:33,200 --> 00:15:36,000
into this incredible Earth-Moon relationship.

480
00:15:36,000 --> 00:15:37,920
It's been quite the journey so far.

481
00:15:37,920 --> 00:15:40,520
Last time, you hinted at a more controversial side

482
00:15:40,520 --> 00:15:41,280
of the story.

483
00:15:41,280 --> 00:15:43,080
I'm dying to know what we're getting into.

484
00:15:43,080 --> 00:15:45,200
Well, even though scientists mostly

485
00:15:45,200 --> 00:15:47,440
agree on the basics of the moon's formation

486
00:15:47,440 --> 00:15:50,040
and its effect on Earth, there are some areas

487
00:15:50,040 --> 00:15:51,360
where opinions differ.

488
00:15:51,360 --> 00:15:52,120
That makes sense.

489
00:15:52,120 --> 00:15:54,320
Sometimes those differences get pretty heated.

490
00:15:54,320 --> 00:15:56,440
I love a good scientific debate.

491
00:15:56,440 --> 00:15:57,200
Bring it on.

492
00:15:57,200 --> 00:15:57,880
OK.

493
00:15:57,880 --> 00:15:59,920
What are some of these controversial areas?

494
00:15:59,920 --> 00:16:01,960
One of the biggest debates revolves

495
00:16:01,960 --> 00:16:05,240
around the finer points of the giant impact hypothesis

496
00:16:05,240 --> 00:16:07,280
itself.

497
00:16:07,280 --> 00:16:10,200
The giant impact hypothesis.

498
00:16:10,200 --> 00:16:11,000
Remember Thea.

499
00:16:11,000 --> 00:16:11,680
Thea, right?

500
00:16:11,680 --> 00:16:14,040
That Mars-sized proto planet we talked about,

501
00:16:14,040 --> 00:16:16,280
the one that supposedly slammed into Earth.

502
00:16:16,280 --> 00:16:17,480
Of course.

503
00:16:17,480 --> 00:16:20,520
The moon's famous or infamous parent.

504
00:16:20,520 --> 00:16:21,960
Well, some scientists are starting

505
00:16:21,960 --> 00:16:25,000
to question whether Thea actually existed at all.

506
00:16:25,000 --> 00:16:25,960
Hold on.

507
00:16:25,960 --> 00:16:28,200
Are you saying that the moon's origin story might

508
00:16:28,200 --> 00:16:30,880
be based on a ghost planet?

509
00:16:30,880 --> 00:16:31,760
Maybe not a ghost.

510
00:16:31,760 --> 00:16:32,260
OK.

511
00:16:32,260 --> 00:16:33,920
But perhaps more of a phantom.

512
00:16:33,920 --> 00:16:35,160
A phantom planet.

513
00:16:35,160 --> 00:16:38,480
Some of the newer models suggest that the object that hit Earth

514
00:16:38,480 --> 00:16:41,240
was much smaller than initially thought.

515
00:16:41,240 --> 00:16:41,740
OK.

516
00:16:41,740 --> 00:16:43,000
How much smaller?

517
00:16:43,000 --> 00:16:45,840
It might have been closer to the size of the moon itself.

518
00:16:45,840 --> 00:16:48,960
So instead of a head-on collision with a planet,

519
00:16:48,960 --> 00:16:51,240
it was more of a cosmic side swipe.

520
00:16:51,240 --> 00:16:53,120
That's one possibility.

521
00:16:53,120 --> 00:16:53,620
I see.

522
00:16:53,620 --> 00:16:56,040
And if the impactor was smaller, it

523
00:16:56,040 --> 00:16:59,240
might explain why we haven't found any distinct traces

524
00:16:59,240 --> 00:17:01,600
of Thea in the Earth-moon system.

525
00:17:01,600 --> 00:17:03,600
It's like trying to find a needle in a haystack

526
00:17:03,600 --> 00:17:05,440
if you don't even know what kind of needle you're looking for.

527
00:17:05,440 --> 00:17:06,800
Exactly.

528
00:17:06,800 --> 00:17:08,920
And that leads to another point of contention,

529
00:17:08,920 --> 00:17:10,040
the composition of the moon.

530
00:17:10,040 --> 00:17:11,720
Yeah, the moon's made of cheese, right?

531
00:17:11,720 --> 00:17:13,640
Well, lunar rocks do have some things

532
00:17:13,640 --> 00:17:15,280
in common with Earth's mantle.

533
00:17:15,280 --> 00:17:15,780
Right.

534
00:17:15,780 --> 00:17:16,680
We talked about that.

535
00:17:16,680 --> 00:17:18,680
There are also some subtle differences.

536
00:17:18,680 --> 00:17:20,200
So it's not a perfect match.

537
00:17:20,200 --> 00:17:21,000
Yeah.

538
00:17:21,000 --> 00:17:23,160
Like, they're from the same family,

539
00:17:23,160 --> 00:17:25,280
but they have their own distinct personalities.

540
00:17:25,280 --> 00:17:27,280
That's the idea.

541
00:17:27,280 --> 00:17:29,160
These differences have led some scientists

542
00:17:29,160 --> 00:17:32,520
to come up with other theories to explain how the moon formed.

543
00:17:32,520 --> 00:17:33,160
Really?

544
00:17:33,160 --> 00:17:35,600
So they think maybe it wasn't a giant impact after all.

545
00:17:35,600 --> 00:17:39,040
They're not ready to completely give up on the giant impact,

546
00:17:39,040 --> 00:17:41,280
but they're exploring other possibilities too.

547
00:17:41,280 --> 00:17:42,920
OK, spill the beans.

548
00:17:42,920 --> 00:17:45,040
What are some of these alternative theories?

549
00:17:45,040 --> 00:17:47,880
Well, one idea that's gaining some traction

550
00:17:47,880 --> 00:17:49,440
is that the moon might have formed

551
00:17:49,440 --> 00:17:51,600
from multiple smaller impacts.

552
00:17:51,600 --> 00:17:52,520
Multiple impacts.

553
00:17:52,520 --> 00:17:54,840
Rather than one gigantic event.

554
00:17:54,840 --> 00:17:55,560
Wow.

555
00:17:55,560 --> 00:17:59,080
Imagine a series of collisions over millions of years.

556
00:17:59,080 --> 00:17:59,760
Oh, wow.

557
00:17:59,760 --> 00:18:02,800
Each one contributing to a growing disk of debris

558
00:18:02,800 --> 00:18:04,600
that eventually became the moon.

559
00:18:04,600 --> 00:18:06,640
So instead of one big bang, it was

560
00:18:06,640 --> 00:18:10,400
more of a slow and steady cosmic construction project.

561
00:18:10,400 --> 00:18:11,080
Exactly.

562
00:18:11,080 --> 00:18:13,720
Kind of like how Earth's atmosphere formed bit by bit.

563
00:18:13,720 --> 00:18:15,560
And this multiple impact idea could

564
00:18:15,560 --> 00:18:17,320
explain some of the differences we see

565
00:18:17,320 --> 00:18:19,360
in the composition of lunar rocks.

566
00:18:19,360 --> 00:18:22,640
So the jury's still out on exactly how the moon came to be.

567
00:18:22,640 --> 00:18:23,760
It seems that way.

568
00:18:23,760 --> 00:18:26,440
But the giant impact remains the leading contender.

569
00:18:26,440 --> 00:18:27,400
For now, it does.

570
00:18:27,400 --> 00:18:29,280
It sounds like there's still a lot of active research

571
00:18:29,280 --> 00:18:30,240
happening in this area.

572
00:18:30,240 --> 00:18:31,360
Absolutely.

573
00:18:31,360 --> 00:18:32,880
But that's the beauty of science.

574
00:18:32,880 --> 00:18:33,480
It is.

575
00:18:33,480 --> 00:18:35,040
It's always evolving.

576
00:18:35,040 --> 00:18:35,520
Right.

577
00:18:35,520 --> 00:18:38,280
New discoveries and new models can change our understanding

578
00:18:38,280 --> 00:18:41,080
and lead to new and exciting theories.

579
00:18:41,080 --> 00:18:42,680
So we're always learning something new.

580
00:18:42,680 --> 00:18:44,960
It's a journey, not a destination.

581
00:18:44,960 --> 00:18:45,640
I like that.

582
00:18:45,640 --> 00:18:46,760
I like that analogy.

583
00:18:46,760 --> 00:18:48,000
It really is.

584
00:18:48,000 --> 00:18:51,400
Like a cosmic puzzle where we're slowly

585
00:18:51,400 --> 00:18:52,600
putting the pieces together.

586
00:18:52,600 --> 00:18:53,360
Uh-huh.

587
00:18:53,360 --> 00:18:54,560
And we've come a long way.

588
00:18:54,560 --> 00:18:56,760
But there's still more pieces to find.

589
00:18:56,760 --> 00:19:00,360
Every new piece we find helps us paint a more complete picture

590
00:19:00,360 --> 00:19:02,280
of our solar system's history.

591
00:19:02,280 --> 00:19:04,600
This has been an incredible deep dive.

592
00:19:04,600 --> 00:19:05,280
It has been.

593
00:19:05,280 --> 00:19:07,720
We've explored the moon's explosive birth.

594
00:19:07,720 --> 00:19:08,920
Yeah, it was pretty dramatic.

595
00:19:08,920 --> 00:19:10,720
Its influence on Earth.

596
00:19:10,720 --> 00:19:12,600
Profound, really.

597
00:19:12,600 --> 00:19:14,600
And even dove into some of the controversies

598
00:19:14,600 --> 00:19:15,560
about its origins.

599
00:19:15,560 --> 00:19:18,000
Yeah, always interesting to see where opinions differ.

600
00:19:18,000 --> 00:19:20,240
It's amazing to think about all the things we've learned

601
00:19:20,240 --> 00:19:22,440
about our celestial companion.

602
00:19:22,440 --> 00:19:25,040
It's been a fantastic journey through billions

603
00:19:25,040 --> 00:19:26,480
of years of cosmic history.

604
00:19:26,480 --> 00:19:27,280
It really has.

605
00:19:27,280 --> 00:19:30,640
Full of awe, beauty, and a little bit of mystery.

606
00:19:30,640 --> 00:19:32,520
The best part is that there's still so much

607
00:19:32,520 --> 00:19:34,200
left to explore and discover.

608
00:19:34,200 --> 00:19:35,880
That's what keeps science going.

609
00:19:35,880 --> 00:19:36,360
It does.

610
00:19:36,360 --> 00:19:38,960
There's always something new to learn, a new question to ask.

611
00:19:38,960 --> 00:19:42,000
So to all our listeners out there, keep looking up,

612
00:19:42,000 --> 00:19:44,360
stay curious, and never stop exploring

613
00:19:44,360 --> 00:19:45,880
the wonders of the cosmos.

614
00:19:45,880 --> 00:19:48,440
And don't forget to subscribe to Cosmos in a Pod

615
00:19:48,440 --> 00:19:51,000
and check out our YouTube channel for more deep dives

616
00:19:51,000 --> 00:19:52,960
into the universe's mysteries.

617
00:19:52,960 --> 00:20:04,600
Thanks for joining us.

