WEBVTT - Why Do We Have Stars?

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<v Speaker 1>So I was outside the other night with my son

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<v Speaker 1>looking up at the sky, and we were having a

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<v Speaker 1>great time, and he turned to me and he asked

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<v Speaker 1>me a question. He said, Hey, Dad, why are there stars?

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<v Speaker 1>You mean like movie stars? No, No, why astronomical stars?

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<v Speaker 1>He wanted to know. Wow, what did you say? Well?

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<v Speaker 1>I thought he was asking me, like, why do stars exist?

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<v Speaker 1>You know, why do we have bright stars in the sky.

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<v Speaker 1>So of course I give him a long physics explanation

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<v Speaker 1>for you know, how funion works and all this kind

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<v Speaker 1>of stuff. I wonder what it's like to have your

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<v Speaker 1>dad be a physics professor. It's awesome. It's awesome. I

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<v Speaker 1>wonder how many times he's just like dad. I just

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<v Speaker 1>wanted a one sentence answer. I once heard him explaining

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<v Speaker 1>to his friends about black holes, and I thought, Hey,

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<v Speaker 1>that dude is cool because of me. I think cool

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<v Speaker 1>as might not be the appropriate adjective here. But what's

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<v Speaker 1>the What's he satisfied with your explanation? No? Not at all.

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<v Speaker 1>In fact, it turns out I totally misunderstood his question.

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<v Speaker 1>When he asked why are their stars? He didn't mean

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<v Speaker 1>like why does the star burn? He meant like, why

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<v Speaker 1>are their stars? Plural, like why don't we just have

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<v Speaker 1>one star? Right? Or like why isn't everything just spread

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<v Speaker 1>out smoothly in the universe? Why does things clump together

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<v Speaker 1>to make planets and stars and all that stuff? WHOA,

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<v Speaker 1>That is a good question. Yeah, it's a great question.

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<v Speaker 1>It's a kind of question kids ask, right, the kind

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<v Speaker 1>of question you don't necessarily think to ask. It's such

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<v Speaker 1>a basic, simple question. That's a question I have. And

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<v Speaker 1>I'm I'm definitely not five years old. Ye I am

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<v Speaker 1>Morhan and I'm Daniel, and welcome to our podcast, Daniel

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<v Speaker 1>and Jorgey Wayne the Universe, in which we try to

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<v Speaker 1>take everything or anything in the universe, even the obvious

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<v Speaker 1>stuff like stars, and explain it to you. Why is

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<v Speaker 1>it there? How does it work? Do I have to

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<v Speaker 1>worry about it? Can I buy one online? We try

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<v Speaker 1>to answer the smooth questions and also the lumpy questions.

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<v Speaker 1>And today is going to be a bit of a

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<v Speaker 1>lumpy episode. Today on the program, we're asking the question

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<v Speaker 1>why are there stars? The universe has a really strange

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<v Speaker 1>kind of shape. I mean, it's huge, but it's mostly empty, right,

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<v Speaker 1>Like there's vast distances between stars and even vaster ones

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<v Speaker 1>between galaxies. But then you have these hot little points, right,

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<v Speaker 1>all this matter concentrated in these little dots. It's a

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<v Speaker 1>really weird arrangement. Why is it concentrating these little pin points?

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<v Speaker 1>Why isn't more diffuse or why don't all those pin

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<v Speaker 1>points just clumped together? Yeah? Why don't we have just

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<v Speaker 1>one mega star or like a big pudding of delute

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<v Speaker 1>gas everywhere? Right? Why is the universe the way it

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<v Speaker 1>is and not any of those other ways? It could

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<v Speaker 1>have been those ways in some alternate multiverse. It probably

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<v Speaker 1>is those ways, but in those multiverses they don't have

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<v Speaker 1>awesome podcasts to ask this question. Yeah. Yeah, because you

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<v Speaker 1>look at the night sky and it's beautiful, right, I

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<v Speaker 1>mean it's it's like this black void with little white pinpoints.

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<v Speaker 1>But you gotta wonder why does it look that way? Okay,

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<v Speaker 1>so I have to take a digression here an artistic

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<v Speaker 1>question for you or here, which is why do you

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<v Speaker 1>think we find the night sky beautiful? I mean, I agree,

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<v Speaker 1>it's gorgeous. This is the best view in the universe, right,

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<v Speaker 1>But is it necessary do we find it beautiful to

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<v Speaker 1>be evolved to find it beautiful? Is it just chance? Like?

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<v Speaker 1>Could we have evolved in a way. We look up

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<v Speaker 1>at the night stine, We're like, yuck, that's gross. M h. Well,

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<v Speaker 1>I think we have a innate appreciation for sparkly things, right,

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<v Speaker 1>we like we'll all pyromaniacs. Yeah, no, I mean evolved

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<v Speaker 1>evolved from liking water maybe or being attracted to water

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<v Speaker 1>or spark the water. I don't know, sparkling water. They

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<v Speaker 1>had ivan then caved mondays right, Yeah, I think people

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<v Speaker 1>used to carbonate their own water back in cave men days.

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<v Speaker 1>I'm pretty sure that we should have asked that question

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<v Speaker 1>Ryan North when we had him on the podcast. When

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<v Speaker 1>did they invent sparkling water? The greatest invention all time?

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<v Speaker 1>Sparkling water. That's a great question is why are there

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<v Speaker 1>stars and planets as opposed to just having a monotonous,

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<v Speaker 1>monogamous no homogeneous, monochronous, monochromatic Yeah, I mean like a

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<v Speaker 1>plane universe. I guess why do we have stars and

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<v Speaker 1>planets and objects and spark the objects and things rather

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<v Speaker 1>than we're just living in a giant gas cloud. That's right. Yeah,

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<v Speaker 1>So that's the question we're gonna try to tackle today,

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<v Speaker 1>give you a solid answer for it. And so as

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<v Speaker 1>usual before we answer the question we I went out

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<v Speaker 1>and I asked bunch of unsuspecting you see, Irvine students,

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<v Speaker 1>off the top of their head. I asked them that question.

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<v Speaker 1>So think about it at home or wherever you're listening.

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<v Speaker 1>Why do you think there are stars and planets and

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<v Speaker 1>not just a smooth universe? Here's what people had to say.

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<v Speaker 1>Why is the universe so lumpy like? Why doesn't matter

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<v Speaker 1>just spread out totally smoothly and evenly through the universe.

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<v Speaker 1>I want to say gravity, because there's like a certain

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<v Speaker 1>kind of gravity putting things in place. And I have

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<v Speaker 1>no idea. Okay, gravity, it's a result of the big bank.

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<v Speaker 1>You had matter and antimatter, and they made clumps and

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<v Speaker 1>they kept expanding, and that's just how it occurred. At

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<v Speaker 1>least that's the model that I've heard. There were at

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<v Speaker 1>some point areas where there was a slight greater density,

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<v Speaker 1>and you know, in the matter in the universevity works,

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<v Speaker 1>a greater density will kind of collapse in the greater

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<v Speaker 1>and greater and greater density to you have a galaxy,

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<v Speaker 1>your plans or whatever the ions. Okay, all right, so

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<v Speaker 1>that's pretty interesting. I feel like you should maybe stop

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<v Speaker 1>advertising that they're U s Irvine students because I don't

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<v Speaker 1>know if you're helping the marketing there. I think it's

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<v Speaker 1>wonderful all these U see Irvine students are willing to

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<v Speaker 1>stop and think about a random question from a randy,

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<v Speaker 1>random scruffy looking dude and think about the universe. Likecent

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<v Speaker 1>of people answer these questions. To me, they get full

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<v Speaker 1>credit even just for trying, for thinking about it, for

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<v Speaker 1>engaging right. To me, that's wonderful. When we first started

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<v Speaker 1>this project, I was sure I was going to get

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<v Speaker 1>one percent answers. So the fact that they don't know

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<v Speaker 1>not a big deal. The fact that they try to answer,

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<v Speaker 1>that's wonderful. I think you should try it down the

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<v Speaker 1>streets of New York next and see what kind of

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<v Speaker 1>reaction you get get out of here. Yeah, well, as

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<v Speaker 1>you were suggesting, maybe I should go up to cal

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<v Speaker 1>Tech and see see if they get them more precise answers.

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<v Speaker 1>But everyone seems to say gravity as the answer to

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<v Speaker 1>the question. Yeah, everybody says gravity, And I think that

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<v Speaker 1>comes from everybody's feeling correctly that gravity plays a big role, right.

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<v Speaker 1>Gravity is the thing that made these structures. Gravity is

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<v Speaker 1>which responsible for holding a start together. Gravity controls the

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<v Speaker 1>shape of the galaxy. Gravity certainly plays a big role,

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<v Speaker 1>but I guess the twist is that it's not the

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<v Speaker 1>only thing you need to make stars. Right. Gravity only

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<v Speaker 1>clumps links together if you if you already have small

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<v Speaker 1>clumps to begin with, right, that's right, Gravity is not

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<v Speaker 1>the complete answer. If you had a universe that was

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<v Speaker 1>totally smooth, right, completely smooth, then gravity couldn't do anything

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<v Speaker 1>because each particle in the universe would be pulled both

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<v Speaker 1>left and right with equal force because it would be

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<v Speaker 1>equal amounts of stuff on both sides of it, And

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<v Speaker 1>so every object would be sort of like pinned down

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<v Speaker 1>by gravity. But it couldn't form any structures, right, So

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<v Speaker 1>gravity can't make lumps. It can only exaggerate lumps. Once

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<v Speaker 1>you've gotten a little bit started, we paint that picture

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<v Speaker 1>a little bit more for me. So let's imagine a

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<v Speaker 1>perfectly smooth universe, meaning that all the particles in the

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<v Speaker 1>universe are kind of at the same distance from each

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<v Speaker 1>other as every other particle in the universe exactly. So imagine,

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<v Speaker 1>you know, every particle is on a grid, right, and

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<v Speaker 1>they have one particle every centimeter or something. Right, So

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<v Speaker 1>take a perfectly exact grid. Everyone. Every particle is one

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<v Speaker 1>centimeter apart from the next particle exactly. And if you're

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<v Speaker 1>thinking this is strange and artificial, it's actually very simple, right,

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<v Speaker 1>And it's very natural. The opposite idea that there's one

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<v Speaker 1>place where there's particles are closer together, or they're denser

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<v Speaker 1>and they're denser, or something that's strange, that's unusual, that

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<v Speaker 1>would be like, well, why they're not here. So having

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<v Speaker 1>a perfectly smooth, symmetric universe as a as a starting

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<v Speaker 1>point actually makes the most sense. It's the most natural concept,

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<v Speaker 1>like a perfect jelly or like a perfect crystal exactly,

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<v Speaker 1>like a perfectly smooth chocolate pudding with new lumps in it. Right.

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<v Speaker 1>So if and and if the universe is infinite, you're

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<v Speaker 1>saying that cloud of perfectly ordered particles would not clump

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<v Speaker 1>together exactly. So take one random particle, right, And it

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<v Speaker 1>doesn't matter which one you choose, because we set this

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<v Speaker 1>up so that all the particles are exactly the same.

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<v Speaker 1>So pick one random particle. Now, that particle is going

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<v Speaker 1>to get pulled on by all the other particles in

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<v Speaker 1>the universe due to gravity and other forces. But let's

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<v Speaker 1>just think about gravity right now. Now, Um, there's an

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<v Speaker 1>infinite number of particles pulling it to the left, and

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<v Speaker 1>an infinite number of particles pulling it to the right,

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<v Speaker 1>and up and down to right exactly, and in any

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<v Speaker 1>any way you slice it, you get the same answer. Right. Um,

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<v Speaker 1>you divide the universe into two halves around this particle,

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<v Speaker 1>and one half of the universe is pulling it one way,

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<v Speaker 1>the other half is pulling it the other way. It

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<v Speaker 1>exactly balances out. It cancels perfectly. Right. It's like if

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<v Speaker 1>you have two kids and each one is pulling on

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<v Speaker 1>one arm, You're not going anywhere. Right. Does that happen

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<v Speaker 1>to you often? That's a random hypothetical I just invented.

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<v Speaker 1>It's not that I have two kids who often have

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<v Speaker 1>totally different ideas about what we should do or um,

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<v Speaker 1>where they want to go or where they want to eat.

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<v Speaker 1>That's right, um. And so in this scenario, every particle

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<v Speaker 1>is an equilibrium. Right. There's no way to begin lumpiness

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<v Speaker 1>because everything is being tugged equally left and right or

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<v Speaker 1>up and down, or you know, back and forth. So

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<v Speaker 1>you would the universe would just sit there, It would

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<v Speaker 1>just stay static. It would it wouldn't wouldn't move right, like,

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<v Speaker 1>we would just stay there forever, because every particle would

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<v Speaker 1>just be perfectly bounds where it is. Exactly. It's like

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<v Speaker 1>if you put a ball in the bottom of a bowl, right,

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<v Speaker 1>it's just gonna sit there. It's not gonna go anywhere, right,

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<v Speaker 1>And that's exactly the situation of each of those particles.

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<v Speaker 1>They're sitting in the bottom of a bowl. That bowl

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<v Speaker 1>is the gravitational well made by all the other particles

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<v Speaker 1>in the universe. And so if the universe is infinite,

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<v Speaker 1>then you can apply the same argument to every particle, right.

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<v Speaker 1>And so if you start out with an infinite, smooth universe,

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<v Speaker 1>then you can't get any structure. You can't start to

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<v Speaker 1>build anything. Hold on, you said that if that's only

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<v Speaker 1>if the universe is infinite, But what happens if we

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<v Speaker 1>have this perfect jelly and the universe is finite, meaning

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<v Speaker 1>that at some point ends. Yeah, well, then this argument

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<v Speaker 1>doesn't apply because there's some point um Because then this

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<v Speaker 1>argument only applies to the very center of the universe. Right. Then,

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<v Speaker 1>if the universe is finite, that means that it has

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<v Speaker 1>a center, right, that there's someplace where there's an equal

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<v Speaker 1>amount of stuff to the left and to the right

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<v Speaker 1>and up and down right, and this argument would only

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<v Speaker 1>apply right there, or if you go to the edge

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<v Speaker 1>of all that stuff right. This is again assuming the

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<v Speaker 1>universe is finite. If you go to the edge of

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<v Speaker 1>all that stuff, the argument doesn't hold anymore. You have

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<v Speaker 1>more stuff on one side than on the other. So

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<v Speaker 1>in the scenario of a finite universe, everything would be

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<v Speaker 1>attracted towards the center. Everything would be attracted towards the center.

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<v Speaker 1>All everyone, all the particles would just go towards the center.

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<v Speaker 1>And then what would happen? Man, I think it would

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<v Speaker 1>get like a huge star or a massive black hole,

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<v Speaker 1>or it would be a pretty crazy party, So the

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<v Speaker 1>universe would be just one star or one black hole.

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<v Speaker 1>I'm because I would be pretty complicated, but I think, yeah,

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<v Speaker 1>you would end up with one really big blob of matter, um,

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<v Speaker 1>and it would be you know, it wouldn't be compally

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<v Speaker 1>compressed into a point because matter resists being compressed and

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<v Speaker 1>and if it was spinning right then that keeps it

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<v Speaker 1>from being compressed further. Um. I don't know if anybody's

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<v Speaker 1>really studied what would happen if you just like had

0:12:11.720 --> 0:12:15.319
<v Speaker 1>a huge universized blob of finite matter and then let

0:12:15.360 --> 0:12:18.800
<v Speaker 1>it collapse. That would be fascinating. So it would be

0:12:19.040 --> 0:12:22.240
<v Speaker 1>kind of this one just one, not two, not three,

0:12:22.320 --> 0:12:25.400
<v Speaker 1>just one giant lump of stuff. That's right. And even

0:12:25.400 --> 0:12:29.400
<v Speaker 1>in that scenario where the universe is perfectly smooth but finite, right,

0:12:29.840 --> 0:12:33.400
<v Speaker 1>you can't get any asymmetries. Everything has to be perfectly

0:12:33.400 --> 0:12:35.920
<v Speaker 1>balanced in every direction. Right. Yes, you have a center,

0:12:35.960 --> 0:12:38.480
<v Speaker 1>so everything's attracted towards the center, but you can't like

0:12:39.000 --> 0:12:42.000
<v Speaker 1>make stars clumping along the way as they're getting dragged

0:12:42.000 --> 0:12:44.640
<v Speaker 1>towards the center. Still has to be perfectly smooth because

0:12:44.640 --> 0:12:47.240
<v Speaker 1>it's the same in every direction, right, In order to

0:12:47.280 --> 0:12:49.120
<v Speaker 1>get the kind of structure that we see when we

0:12:49.120 --> 0:12:50.720
<v Speaker 1>look at the night sky, you have like a star

0:12:50.800 --> 0:12:53.079
<v Speaker 1>here and no star there, and or galaxy here and

0:12:53.440 --> 0:12:57.079
<v Speaker 1>galaxy there. That's and those are asymmetry. So right, that's

0:12:57.080 --> 0:13:00.480
<v Speaker 1>a structure, that's a lump. Yeah, it's a in the

0:13:00.559 --> 0:13:03.720
<v Speaker 1>universe exactly. So that's obviously not the universe we're in.

0:13:03.800 --> 0:13:06.719
<v Speaker 1>We're not in a perfectly smooth, jelly universe, and we're

0:13:06.760 --> 0:13:12.080
<v Speaker 1>not living in one giant, singular super cluster of stuff.

0:13:12.720 --> 0:13:15.560
<v Speaker 1>We live in this kind of a stranger universe, right,

0:13:15.640 --> 0:13:17.320
<v Speaker 1>and thank god we do, right. I mean, it would

0:13:17.360 --> 0:13:20.000
<v Speaker 1>be pretty boring to live in an infinitely smooth pudding

0:13:20.559 --> 0:13:22.960
<v Speaker 1>or even just have like one big star living in

0:13:22.960 --> 0:13:26.720
<v Speaker 1>a perfect jelly. Seems pretty pretty peaceful to me. Again,

0:13:26.760 --> 0:13:28.440
<v Speaker 1>I think you should have a snack before we do

0:13:28.520 --> 0:13:31.240
<v Speaker 1>this podcast. Okay, although, as you tell you tend towards

0:13:31.240 --> 0:13:33.240
<v Speaker 1>these food analogies that I think it just reflects what

0:13:33.360 --> 0:13:37.439
<v Speaker 1>you're feeling rather than what you're thinking. Well, let's let's

0:13:37.720 --> 0:13:39.800
<v Speaker 1>get into how lumpy the universe is and how it

0:13:39.880 --> 0:13:42.360
<v Speaker 1>got that way. But first let's take a quick break.

0:13:54.880 --> 0:13:57.400
<v Speaker 1>All right, So we don't live in a perfectly smooth universe,

0:13:57.440 --> 0:13:59.280
<v Speaker 1>and we don't live in a universe such as one

0:13:59.480 --> 0:14:04.280
<v Speaker 1>giant cluster, black hole, slash star. That's not the universe

0:14:04.280 --> 0:14:06.319
<v Speaker 1>we'll live in, right, We are actually in a very

0:14:06.400 --> 0:14:09.520
<v Speaker 1>lumpy universe. Yeah, And the universe, the structure universe is

0:14:09.520 --> 0:14:12.280
<v Speaker 1>really fascinating. We should dig into it really deeply in

0:14:12.320 --> 0:14:14.560
<v Speaker 1>another podcast episode and talk about it and why it

0:14:14.640 --> 0:14:16.520
<v Speaker 1>is this way in that way. Um, but let's just

0:14:16.559 --> 0:14:19.360
<v Speaker 1>review briefly sort of where we are in the universe,

0:14:20.000 --> 0:14:23.840
<v Speaker 1>the the status of the lumps, the level of lumpiness

0:14:23.840 --> 0:14:26.080
<v Speaker 1>of the universe. Yeah, so we we are sitting here

0:14:26.120 --> 0:14:29.000
<v Speaker 1>on Earth presumably, that's right. We are two lumps on

0:14:29.040 --> 0:14:32.320
<v Speaker 1>a rock. Yeah. Um, presumably most of our listeners are

0:14:32.560 --> 0:14:34.240
<v Speaker 1>on Earth. And if you're not, by the way, if

0:14:34.240 --> 0:14:36.040
<v Speaker 1>you're listening to this podcast and you're not on Earth,

0:14:36.160 --> 0:14:40.480
<v Speaker 1>we really want to hear from you. Yeah. Absolutely, But

0:14:40.600 --> 0:14:43.160
<v Speaker 1>we are in a big rock around rock, going around

0:14:43.280 --> 0:14:47.320
<v Speaker 1>a sun, a star, and that's our solar system, right,

0:14:47.440 --> 0:14:49.880
<v Speaker 1>and even that is super lumpy. I mean from the

0:14:49.880 --> 0:14:52.680
<v Speaker 1>point of view of like how smooth this stuff distributed.

0:14:53.080 --> 0:14:55.200
<v Speaker 1>You know, people are probably familiar with how far away

0:14:55.240 --> 0:14:57.880
<v Speaker 1>the Sun is. It's you know, it takes a time

0:14:57.920 --> 0:15:00.000
<v Speaker 1>for light to even get there. It's minutes and minute,

0:15:00.000 --> 0:15:02.000
<v Speaker 1>it's in minutes, right, And the Sun itself is a

0:15:02.120 --> 0:15:05.560
<v Speaker 1>huge blov of matter, but it's super far away. You know.

0:15:05.640 --> 0:15:08.200
<v Speaker 1>The size of the Earth is enormous and the size

0:15:08.240 --> 0:15:09.800
<v Speaker 1>of the Sun is enormous, but the size of the

0:15:09.840 --> 0:15:14.040
<v Speaker 1>distance between them dwarfs both of them. Right, So even

0:15:14.080 --> 0:15:16.600
<v Speaker 1>just the solar system is really really lumpy in that

0:15:16.640 --> 0:15:19.280
<v Speaker 1>sense that the matter is concentrated and not spread out.

0:15:19.720 --> 0:15:22.640
<v Speaker 1>And then our solarcism is inside of a galaxy. Right,

0:15:23.640 --> 0:15:26.240
<v Speaker 1>and that's even lumpier from that point of view, right,

0:15:26.280 --> 0:15:29.960
<v Speaker 1>Like the distance between stars is huge compared to the

0:15:29.960 --> 0:15:32.720
<v Speaker 1>size of the stars. And it had some sort of structure, right,

0:15:32.720 --> 0:15:36.720
<v Speaker 1>Like the galaxy has spirals and it's kind of thicker

0:15:36.760 --> 0:15:39.280
<v Speaker 1>and more dense in the middle. Right, there's no structure

0:15:39.640 --> 0:15:42.120
<v Speaker 1>at that scale too. Yeah, the galaxy told me it

0:15:42.160 --> 0:15:44.520
<v Speaker 1>doesn't like when you talk about it's thickening waistline rhead.

0:15:45.000 --> 0:15:51.560
<v Speaker 1>But it's true. It sparkly. I'm talking about its sparkliness.

0:15:51.880 --> 0:15:55.040
<v Speaker 1>It's beautiful. It's beautiful, the milky way. Um, yeah, exactly.

0:15:55.040 --> 0:15:56.920
<v Speaker 1>We got all these stars, hundred billions of stars, but

0:15:56.960 --> 0:15:59.080
<v Speaker 1>they're not just a blob, right, They're not just distributed

0:15:59.160 --> 0:16:01.520
<v Speaker 1>evenly all THEO. For a long time people thought that's

0:16:01.280 --> 0:16:03.920
<v Speaker 1>what happened, But now we know that they're arranged in

0:16:03.920 --> 0:16:07.720
<v Speaker 1>this amazing swirl pattern right or the center of the galaxy.

0:16:07.760 --> 0:16:09.400
<v Speaker 1>And then we have these arms that come out and

0:16:09.440 --> 0:16:12.760
<v Speaker 1>because it's rotating, those arms sort of dragged behind it,

0:16:13.320 --> 0:16:15.560
<v Speaker 1>and uh, and you get this amazing swirl and then

0:16:15.560 --> 0:16:17.960
<v Speaker 1>you can keep going like the galaxy is part of

0:16:17.960 --> 0:16:21.480
<v Speaker 1>a supercluster of galaxies and that's super. No, you missed one?

0:16:21.680 --> 0:16:23.720
<v Speaker 1>What you missed one? The galaxy is part of a

0:16:23.760 --> 0:16:26.880
<v Speaker 1>cluster of galaxies, right, And when we talk about a cluster,

0:16:27.000 --> 0:16:29.920
<v Speaker 1>we mean things that are gravitationally bound to each other,

0:16:29.960 --> 0:16:32.960
<v Speaker 1>that essentially are orbiting each other over billions and billions

0:16:33.000 --> 0:16:36.320
<v Speaker 1>of years. So we and ours is called the local group,

0:16:36.440 --> 0:16:40.000
<v Speaker 1>right Like our cluster of galaxies is very imaginatively called

0:16:40.040 --> 0:16:43.400
<v Speaker 1>the local group. I know that sounds like a temporary

0:16:43.480 --> 0:16:45.240
<v Speaker 1>name somebody came up with, like, oh, I need to

0:16:45.280 --> 0:16:47.400
<v Speaker 1>call this something and talk to my advisor, and then

0:16:47.400 --> 0:16:49.120
<v Speaker 1>it just stuck and they're like, dang, and I should

0:16:49.160 --> 0:16:52.960
<v Speaker 1>have named it after my dog. What's the opposite of local?

0:16:53.200 --> 0:16:57.520
<v Speaker 1>Like basically, just here, it means the galaxies near us, right,

0:16:58.040 --> 0:17:02.520
<v Speaker 1>It's pretty lame name. Um yeah, so that's the cluster.

0:17:03.000 --> 0:17:05.760
<v Speaker 1>You know, our galaxy cluster is green and you know

0:17:06.520 --> 0:17:12.480
<v Speaker 1>local sources locally, that's right. I don't think it's vegan,

0:17:12.800 --> 0:17:22.160
<v Speaker 1>but at least it's local, right. Um yeah, exactly. Our

0:17:22.200 --> 0:17:24.879
<v Speaker 1>galaxy is part of a structure of of other with

0:17:25.040 --> 0:17:29.920
<v Speaker 1>other galaxies. Even that cluster is part of another structure

0:17:29.960 --> 0:17:33.000
<v Speaker 1>in the universe, right. Yeah. They call those superclusters, and

0:17:33.040 --> 0:17:37.560
<v Speaker 1>these are basically clusters of clusters another imaginative name. Huh.

0:17:37.680 --> 0:17:39.920
<v Speaker 1>And again you might ask, like, are these totally arbitrary?

0:17:39.920 --> 0:17:42.080
<v Speaker 1>Is just making this up? Could you have organized it differently?

0:17:42.280 --> 0:17:44.640
<v Speaker 1>The answers, No, there's some science behind it. We think

0:17:44.680 --> 0:17:48.159
<v Speaker 1>about how these groups operate, you know, And essentially a

0:17:48.240 --> 0:17:52.000
<v Speaker 1>supercluster is not just a really really big cluster, it's

0:17:52.080 --> 0:17:56.000
<v Speaker 1>a cluster of clusters, meaning that the each cluster inside

0:17:56.000 --> 0:17:59.720
<v Speaker 1>a supercluster is gravitationally bound to itself, and then those

0:17:59.760 --> 0:18:02.880
<v Speaker 1>things themselves are gravitationally bound to each other, and that's

0:18:02.880 --> 0:18:05.199
<v Speaker 1>what makes the super clustered. They're sort of trapped in

0:18:05.240 --> 0:18:08.520
<v Speaker 1>a sort of gravitational bubble almost. Yeah, the way like

0:18:08.760 --> 0:18:11.280
<v Speaker 1>you know, the Earth and the Moon are a gravitational system, right,

0:18:11.280 --> 0:18:13.880
<v Speaker 1>which is embedded inside the Solar System, which is embedded

0:18:13.880 --> 0:18:17.000
<v Speaker 1>inside the galaxy. Right, you might say it's arbitrary to

0:18:17.040 --> 0:18:18.760
<v Speaker 1>define whether or not the Moon is part of the

0:18:18.760 --> 0:18:20.760
<v Speaker 1>Earth system, of the Solar System, whatever. Really makes much

0:18:20.760 --> 0:18:22.919
<v Speaker 1>more sense to consider the Earth to be part of

0:18:22.960 --> 0:18:25.239
<v Speaker 1>our system, and then the Solar System may be part

0:18:25.280 --> 0:18:27.280
<v Speaker 1>of the galaxy, rather than just say like, oh, it's

0:18:27.280 --> 0:18:30.439
<v Speaker 1>all one big galaxy. So that's why we get these hierarchies,

0:18:30.640 --> 0:18:32.639
<v Speaker 1>and it's amazing that we have these hierarchies, you know,

0:18:32.680 --> 0:18:34.840
<v Speaker 1>and like also because you can zoom down right and

0:18:34.840 --> 0:18:36.719
<v Speaker 1>you get like down to the atom and things are

0:18:36.800 --> 0:18:39.840
<v Speaker 1>orbiting and stuff. So we have this over incredible the

0:18:40.000 --> 0:18:45.400
<v Speaker 1>different distances from microscopic to what megascopic we have similar

0:18:45.400 --> 0:18:47.800
<v Speaker 1>structures of things orbiting each other and right on these

0:18:47.840 --> 0:18:51.080
<v Speaker 1>on these large scales, like an infinite Russian doll, you

0:18:51.119 --> 0:18:54.280
<v Speaker 1>can stack them up almost infinitely, seems yeah, but infinite,

0:18:54.280 --> 0:18:56.120
<v Speaker 1>we don't know, right, We talked about that another time,

0:18:56.160 --> 0:18:59.800
<v Speaker 1>Like we think the universe probably has the smallest scale,

0:19:00.119 --> 0:19:02.480
<v Speaker 1>and when we talk about the structure of the galaxy

0:19:02.560 --> 0:19:04.720
<v Speaker 1>as the structure of the the universe, and another podcast episode

0:19:04.720 --> 0:19:07.240
<v Speaker 1>we'll talk about the biggest structures in the university is

0:19:07.280 --> 0:19:09.720
<v Speaker 1>a whole other fascinating topic. You can keep going in.

0:19:09.720 --> 0:19:12.080
<v Speaker 1>There are bigger, bigger structures, right. Well, there's a point

0:19:12.080 --> 0:19:15.560
<v Speaker 1>where they stop. Yeah, at some point they stop. At

0:19:15.600 --> 0:19:19.119
<v Speaker 1>some point they stop. There's an end to the Russian doll,

0:19:19.280 --> 0:19:21.600
<v Speaker 1>as far as we know, there is. There's the largest

0:19:21.640 --> 0:19:23.960
<v Speaker 1>Russian doll. Yeah. Um, anyway, but that's the topic for

0:19:24.000 --> 0:19:28.200
<v Speaker 1>another another day. Let's talk about why why we have structure. Yeah,

0:19:28.200 --> 0:19:30.080
<v Speaker 1>the point is that there is structure, right, Like, we're

0:19:30.119 --> 0:19:32.880
<v Speaker 1>not in a smooth universe and we're not just one

0:19:32.920 --> 0:19:36.520
<v Speaker 1>giant lump. There is like texture to the universe, right,

0:19:36.520 --> 0:19:40.399
<v Speaker 1>there's features, there's things to look at, there's good stuff

0:19:40.440 --> 0:19:44.960
<v Speaker 1>to see exactly, and as our you see I question

0:19:45.040 --> 0:19:49.240
<v Speaker 1>answers earlier said gravity is responsible for forming those things.

0:19:49.240 --> 0:19:52.000
<v Speaker 1>But gravity couldn't start those structures, right, That was the

0:19:52.000 --> 0:19:54.480
<v Speaker 1>point we were making earlier. So the point is that

0:19:54.520 --> 0:19:57.960
<v Speaker 1>gravity can't make lumps. When you start a lump, gravity

0:19:57.960 --> 0:20:00.399
<v Speaker 1>will accelerate like a chain reaction. Right, when you have

0:20:00.520 --> 0:20:03.119
<v Speaker 1>one point that's denser than everything else, it will have

0:20:03.160 --> 0:20:06.320
<v Speaker 1>a stronger gravitational pull and it'll start to attract stuff

0:20:06.359 --> 0:20:09.080
<v Speaker 1>and then look at heavier and have a stronger gravitational pull,

0:20:09.359 --> 0:20:11.919
<v Speaker 1>and it will feed on itself. But if everything is smooth,

0:20:12.000 --> 0:20:14.400
<v Speaker 1>then you can't. So the question is, so gravity can

0:20:14.400 --> 0:20:17.600
<v Speaker 1>make lumps bigger, but the question really comes down to

0:20:17.880 --> 0:20:20.119
<v Speaker 1>where did the first lumps come from. It's kind of

0:20:20.160 --> 0:20:23.760
<v Speaker 1>like gravity can roll a snowball down the hill, but

0:20:23.840 --> 0:20:28.320
<v Speaker 1>it can't sort of start the snowball rolling, Yeah, exactly, exactly,

0:20:28.359 --> 0:20:30.360
<v Speaker 1>Like once it's rolling, it gets bigger and lump here.

0:20:30.400 --> 0:20:33.560
<v Speaker 1>But you need some sort of something to get that

0:20:33.640 --> 0:20:35.760
<v Speaker 1>snowball going. Yeah, you have to knock it out of

0:20:35.800 --> 0:20:41.920
<v Speaker 1>equilibrium to get it to get things snowballing exactly. Okay,

0:20:44.480 --> 0:20:47.000
<v Speaker 1>all right, So how did the universe key head lumps?

0:20:47.320 --> 0:20:50.560
<v Speaker 1>How is it not perfectly smooth or one giant? So

0:20:50.600 --> 0:20:52.479
<v Speaker 1>that was a big mystery for a long time, right,

0:20:52.520 --> 0:20:55.840
<v Speaker 1>because it's very natural to think that the universe started symmetrically.

0:20:56.160 --> 0:20:58.119
<v Speaker 1>I think probably the most popular model for how the

0:20:58.160 --> 0:21:01.680
<v Speaker 1>universe started is the universe versus infinite and that has

0:21:01.760 --> 0:21:03.920
<v Speaker 1>infinite amount of matter in it, and that was created

0:21:03.920 --> 0:21:07.240
<v Speaker 1>in the first moments, right that we don't understand at all.

0:21:07.680 --> 0:21:09.800
<v Speaker 1>But not understanding it means we want to start with

0:21:09.840 --> 0:21:12.600
<v Speaker 1>the simplest idea. Okay, And it's not very simple to

0:21:12.640 --> 0:21:14.760
<v Speaker 1>imagine the creation of an infinite universe with an infinite

0:21:14.760 --> 0:21:16.720
<v Speaker 1>amount of stuff in it. But if you're gonna go there,

0:21:17.200 --> 0:21:19.359
<v Speaker 1>it makes more sense to say that the universe starts

0:21:19.359 --> 0:21:22.360
<v Speaker 1>out smooth. That's where this idea of smoothness comes right, right,

0:21:22.400 --> 0:21:26.080
<v Speaker 1>like simplicity, because the opposite like, oh, that the universe

0:21:26.160 --> 0:21:28.679
<v Speaker 1>was created with some initial lumpiness, that's weird. Because then

0:21:28.720 --> 0:21:31.320
<v Speaker 1>you have to ask why this lumpingness, Why not that lumpiness?

0:21:31.359 --> 0:21:34.200
<v Speaker 1>Who made that choice? Right? And uh so it was

0:21:34.240 --> 0:21:37.840
<v Speaker 1>a big puzzle for a long time. Um, And there's

0:21:37.840 --> 0:21:40.159
<v Speaker 1>really only one way that we know of that you

0:21:40.200 --> 0:21:44.160
<v Speaker 1>can make lumpiness out of smoothness. There's only one thing

0:21:44.200 --> 0:21:47.560
<v Speaker 1>in physics that's capable of doing that, Meaning there's only

0:21:47.640 --> 0:21:51.840
<v Speaker 1>one thing they can add features to something that should

0:21:51.920 --> 0:21:55.560
<v Speaker 1>be perfectly plain. That's right, what you need there's something

0:21:55.600 --> 0:22:00.400
<v Speaker 1>that's not deterministic, something which has a random element to it, right,

0:22:00.400 --> 0:22:03.280
<v Speaker 1>because if every particle universe starts in the same situation,

0:22:03.520 --> 0:22:05.520
<v Speaker 1>then they should all have the same future. Which you

0:22:05.560 --> 0:22:07.679
<v Speaker 1>need is to distinguish them somehow, for this one have

0:22:07.720 --> 0:22:09.520
<v Speaker 1>a different future than that one, for this one, have

0:22:09.520 --> 0:22:12.320
<v Speaker 1>a different experience somehow. The only thing we know they

0:22:12.359 --> 0:22:15.680
<v Speaker 1>can do that that can break determinism is quantum mechanics.

0:22:15.720 --> 0:22:20.240
<v Speaker 1>Because quantum mechanics has real randomness in it. Is that

0:22:20.320 --> 0:22:23.520
<v Speaker 1>the source then of randomness in the universe. Like without

0:22:23.600 --> 0:22:27.760
<v Speaker 1>quantum mechanics, we would all be perfectly smooth. Yeah, exactly,

0:22:27.840 --> 0:22:30.040
<v Speaker 1>But there was still another puzzle, right, So quantum mechanics

0:22:30.080 --> 0:22:32.480
<v Speaker 1>gives you randomness, but you know, quantum mechanics does not

0:22:32.520 --> 0:22:35.439
<v Speaker 1>something you notice. You don't like drive around and notice

0:22:35.600 --> 0:22:38.600
<v Speaker 1>random stuff happening from quantum mechannicals, Like if my phone

0:22:38.680 --> 0:22:41.800
<v Speaker 1>is here, it's not here and there, that's right. I mean,

0:22:41.840 --> 0:22:44.320
<v Speaker 1>maybe your bank accounts seems to fluctuate randomly, but there

0:22:44.320 --> 0:22:48.120
<v Speaker 1>actually is an explanation. My bank account could use more physics,

0:22:48.119 --> 0:22:53.919
<v Speaker 1>for sure. I am a quantum mechanic accountant, quantom accountant

0:22:54.560 --> 0:22:56.960
<v Speaker 1>um exactly. And that's why quantum mechanics took such a

0:22:57.000 --> 0:23:00.000
<v Speaker 1>long time to discover, because people thought the universe was deterministic.

0:23:00.000 --> 0:23:02.720
<v Speaker 1>I thought two particles in the same situation would always

0:23:02.760 --> 0:23:05.199
<v Speaker 1>have the same future. I see, there's no reason for

0:23:05.240 --> 0:23:08.080
<v Speaker 1>them to be different. Like if you create a universe

0:23:08.840 --> 0:23:11.879
<v Speaker 1>without quantum mechanics, there's no reason for all the particles

0:23:11.920 --> 0:23:14.240
<v Speaker 1>to be different. There's nothing that gives it that initial

0:23:14.680 --> 0:23:19.280
<v Speaker 1>randomness exactly. The problem is that quantum mechanics is a

0:23:19.280 --> 0:23:22.320
<v Speaker 1>tiny amount of randomness, right, it's at the particle scale.

0:23:22.600 --> 0:23:26.159
<v Speaker 1>It's super duper small, right, these tiny little fluctuations, And

0:23:26.200 --> 0:23:28.320
<v Speaker 1>what are we talking about concretely, we're talking about like

0:23:28.840 --> 0:23:31.560
<v Speaker 1>particles being created out of the vacuum. Quantum mechanics can

0:23:31.560 --> 0:23:33.720
<v Speaker 1>do that. It can take energy and just turn it

0:23:33.720 --> 0:23:35.879
<v Speaker 1>into particles and then they can turn back into energy.

0:23:36.520 --> 0:23:38.800
<v Speaker 1>Or you know, this particle can have a chance to

0:23:38.880 --> 0:23:40.719
<v Speaker 1>go left or right, and you know, maybe this one

0:23:40.760 --> 0:23:43.080
<v Speaker 1>goes left and another one goes right. This kind of stuff,

0:23:43.080 --> 0:23:46.880
<v Speaker 1>it's really really tiny effects, not really enough to get

0:23:46.880 --> 0:23:50.440
<v Speaker 1>gravity going because gravity is super duper weak, right, Gravity

0:23:50.480 --> 0:23:54.240
<v Speaker 1>needs more than the tiniest little discrepancy. I mean, if

0:23:54.240 --> 0:23:56.440
<v Speaker 1>you've given billions of years. But the kicker is that

0:23:56.480 --> 0:23:58.879
<v Speaker 1>the universe used to be small, right, that's the twist.

0:23:59.000 --> 0:24:01.600
<v Speaker 1>Ending is that the universe used to be really tiny

0:24:01.640 --> 0:24:04.400
<v Speaker 1>and small. That's right, And so the very first moments

0:24:04.400 --> 0:24:07.240
<v Speaker 1>of the universe were super dramatic. What happened in the

0:24:07.280 --> 0:24:10.960
<v Speaker 1>first first moments of the universe was inflation. Inflation is

0:24:11.000 --> 0:24:14.120
<v Speaker 1>this idea that the universe used to be much denser

0:24:14.400 --> 0:24:17.000
<v Speaker 1>and then it got stretched out, it got inflated, right,

0:24:17.040 --> 0:24:19.840
<v Speaker 1>And that's just not stuff moving through space. This is

0:24:19.880 --> 0:24:23.720
<v Speaker 1>the actual expansion of space itself, meaning things got stretched right,

0:24:24.160 --> 0:24:27.119
<v Speaker 1>more space was made everything I'm blown and inflated and

0:24:27.119 --> 0:24:32.520
<v Speaker 1>blown up. What that means is that the microscopic became macroscopic.

0:24:32.800 --> 0:24:34.879
<v Speaker 1>We'll step us through this. So you're saying, this is

0:24:34.920 --> 0:24:37.440
<v Speaker 1>all this all goes back to the Big Bang, right,

0:24:37.640 --> 0:24:39.239
<v Speaker 1>Everything goes back to the Big Bang in the end.

0:24:39.240 --> 0:24:41.760
<v Speaker 1>You can blame everything in the Big Bang technically, I

0:24:41.800 --> 0:24:46.040
<v Speaker 1>guess yeah, um officer, I was speeding because the Big

0:24:46.040 --> 0:24:51.320
<v Speaker 1>Bang dot dot dot dot dot. I blame the universe. YadA, YadA, YadA,

0:24:51.320 --> 0:24:56.040
<v Speaker 1>I was speeding quantum mechanics. That gets me out of

0:24:56.040 --> 0:24:58.600
<v Speaker 1>every ticket, trust me. Before we keep going, let's take

0:24:58.640 --> 0:25:14.200
<v Speaker 1>a short break. Yeah, so the universe used to be very,

0:25:14.280 --> 0:25:17.119
<v Speaker 1>very small, and that's where these that's where quantum mechanics

0:25:17.119 --> 0:25:18.959
<v Speaker 1>played a big role, right, Yeah, And be careful when

0:25:19.000 --> 0:25:20.840
<v Speaker 1>you say the universe used to be very small, because

0:25:20.840 --> 0:25:23.480
<v Speaker 1>we're still saying the universe was infinite, right, and an

0:25:23.480 --> 0:25:26.359
<v Speaker 1>infinite amount of stuff in it, but it was denser, right.

0:25:26.359 --> 0:25:29.280
<v Speaker 1>It used to be more squished when it was created,

0:25:29.359 --> 0:25:30.960
<v Speaker 1>and then it was and then all that stuff was

0:25:31.040 --> 0:25:34.840
<v Speaker 1>stretched out due to inflation. Oh. I see, So it's

0:25:34.880 --> 0:25:37.640
<v Speaker 1>like an infinite ruler getting stretched. It's still infinite, right,

0:25:37.960 --> 0:25:40.360
<v Speaker 1>I see. So you're saying that the features we've see

0:25:40.359 --> 0:25:45.480
<v Speaker 1>in the universe today are really just the quantum features

0:25:45.520 --> 0:25:49.160
<v Speaker 1>that we used to have when we were denser, not smaller.

0:25:49.800 --> 0:25:52.720
<v Speaker 1>But now when inflation happened at the Big Bang, everything

0:25:52.760 --> 0:25:56.240
<v Speaker 1>all these small fluctuations got way way bigger. Yeah, it's

0:25:56.320 --> 0:25:59.000
<v Speaker 1>like an ant man right where he can. He can

0:25:59.119 --> 0:26:01.640
<v Speaker 1>make things much much of it. Right, ants can be enormous,

0:26:01.680 --> 0:26:03.840
<v Speaker 1>and then they can do construction projects and you can

0:26:04.080 --> 0:26:06.119
<v Speaker 1>ride in the back of a butterfly and cool stuff.

0:26:06.600 --> 0:26:10.399
<v Speaker 1>Take the microscopic and make it macroscopic. Right, So the

0:26:10.400 --> 0:26:15.679
<v Speaker 1>timeline is the universe is created perfectly smooth, right, little

0:26:15.760 --> 0:26:19.160
<v Speaker 1>quantum fluctuations happen a little bit this, one particle moves

0:26:19.160 --> 0:26:20.960
<v Speaker 1>a little bit this way, one particle moves a little

0:26:20.960 --> 0:26:24.679
<v Speaker 1>bit that way. Then inflation takes over and blows that

0:26:24.840 --> 0:26:28.960
<v Speaker 1>up right and inflates. It makes those tiny little fluctuations

0:26:29.000 --> 0:26:33.160
<v Speaker 1>into bigger fluctuations enough to see gravity, and then gravity

0:26:33.200 --> 0:26:36.639
<v Speaker 1>takes over for the next fourteen billion years. YadA, YadA, YadA.

0:26:36.680 --> 0:26:43.359
<v Speaker 1>I was speeding officer. I'm telling you that story works

0:26:43.400 --> 0:26:46.960
<v Speaker 1>every time. Yeah, they probably fall asleep before you finish.

0:26:48.760 --> 0:26:54.840
<v Speaker 1>Another physics professor, you just let him go. So you're saying,

0:26:55.000 --> 0:26:58.040
<v Speaker 1>the universe used to be small or denser, and and

0:26:58.119 --> 0:27:02.359
<v Speaker 1>everything was smoother at that scale, except that if we

0:27:02.400 --> 0:27:05.440
<v Speaker 1>didn't have quantum mechanics, but we still had inflation. Then

0:27:05.520 --> 0:27:09.000
<v Speaker 1>we would have exploded the universe or expanded universe, and

0:27:09.119 --> 0:27:12.440
<v Speaker 1>it would remain smooth. Yes, exactly, it would remain smooth

0:27:13.040 --> 0:27:15.479
<v Speaker 1>because we had those quantum fluctuations that a little bit

0:27:15.480 --> 0:27:19.639
<v Speaker 1>of random this at the beginning gave the universe texture exactly.

0:27:19.920 --> 0:27:22.840
<v Speaker 1>And those little fluctuations were random, right, and they could

0:27:22.840 --> 0:27:26.160
<v Speaker 1>have been different, different random throws of the universe dice,

0:27:26.400 --> 0:27:28.560
<v Speaker 1>and we would have a completely different structure. I mean,

0:27:28.760 --> 0:27:31.040
<v Speaker 1>I think the kinds of structures we would have would

0:27:31.080 --> 0:27:33.560
<v Speaker 1>still be the same. We would still have galaxies and stars, whatever,

0:27:33.720 --> 0:27:35.960
<v Speaker 1>but they would be arranged differently. So you might ask,

0:27:36.160 --> 0:27:38.840
<v Speaker 1>why do we have a galaxy here and not there?

0:27:39.080 --> 0:27:41.520
<v Speaker 1>And you can trace the answer that all the way

0:27:41.560 --> 0:27:46.280
<v Speaker 1>back to one little particle fluctuating my millibil of seconds

0:27:46.359 --> 0:27:48.760
<v Speaker 1>after the Big Bang. If it fluctuated this way, we

0:27:48.840 --> 0:27:51.000
<v Speaker 1>get this galaxy. We fluctuated that way, we get a

0:27:51.040 --> 0:27:53.600
<v Speaker 1>different galaxy, or in the same galaxy in a different place.

0:27:54.400 --> 0:27:58.000
<v Speaker 1>That you said that that provided the seeds for the structure,

0:27:58.080 --> 0:28:01.040
<v Speaker 1>meaning it would have and it expanded, it would have

0:28:01.080 --> 0:28:04.440
<v Speaker 1>been smooth, but it had these kind of slightly small

0:28:04.960 --> 0:28:09.160
<v Speaker 1>shades of a texture, and those those shades became exaggerated

0:28:09.160 --> 0:28:11.600
<v Speaker 1>by gravity, and then things started to clump around those

0:28:11.760 --> 0:28:14.679
<v Speaker 1>little shades of texture exactly. And we can see this.

0:28:14.760 --> 0:28:16.800
<v Speaker 1>We can look back in time and we can see

0:28:16.840 --> 0:28:20.040
<v Speaker 1>this progression happening. Like if you look back deep, deep

0:28:20.040 --> 0:28:22.199
<v Speaker 1>into the history of the universe, you see the first

0:28:22.320 --> 0:28:24.600
<v Speaker 1>light that we can see, which comes from about three

0:28:25.040 --> 0:28:27.480
<v Speaker 1>eighty thousand years after the Big Bang. It's the cosmic

0:28:27.520 --> 0:28:30.520
<v Speaker 1>microwave background. We've talked about a few times. This light

0:28:30.640 --> 0:28:33.000
<v Speaker 1>is really really smooth. It's almost the same no matter

0:28:33.080 --> 0:28:34.680
<v Speaker 1>where you look at it. It's like the same color,

0:28:34.800 --> 0:28:37.960
<v Speaker 1>the same temperature, whatever. But if you measure it really

0:28:38.080 --> 0:28:42.560
<v Speaker 1>carefully that you can see little variations, tiny little fractions

0:28:43.000 --> 0:28:46.520
<v Speaker 1>of colder and hotter spots. Those that took four hundred

0:28:46.520 --> 0:28:49.680
<v Speaker 1>thousand years just to get that far right, those are

0:28:49.800 --> 0:28:53.960
<v Speaker 1>the seeds of from this quantum fluctuations exaggerated by gravity

0:28:54.000 --> 0:28:56.840
<v Speaker 1>for four hundred thousand years, then propagated forward in time.

0:28:56.880 --> 0:28:59.280
<v Speaker 1>Give gravity another few billion years, and you start to

0:28:59.320 --> 0:29:02.280
<v Speaker 1>get things like stars and galaxies and all that stuff. Right,

0:29:02.400 --> 0:29:05.440
<v Speaker 1>But we can see these quantum fluctuations from the early universe.

0:29:05.440 --> 0:29:10.239
<v Speaker 1>It's like the pattern that made our our cosmos was

0:29:10.280 --> 0:29:13.800
<v Speaker 1>totally random. It was totally random, exactly. And we think

0:29:13.920 --> 0:29:17.320
<v Speaker 1>quantum mechanics is truly random, right, not like there's some

0:29:17.440 --> 0:29:20.040
<v Speaker 1>hidden process that's controlling it that we don't understand. We

0:29:20.080 --> 0:29:22.600
<v Speaker 1>think it's really truly random. As mind blowing as it

0:29:22.680 --> 0:29:25.920
<v Speaker 1>is for anything in the universe to be honestly truly random,

0:29:26.240 --> 0:29:29.040
<v Speaker 1>it is, and it affects our universe is structure at

0:29:29.080 --> 0:29:32.600
<v Speaker 1>the deepest level. Right. Wow, it's amazing to think that

0:29:32.640 --> 0:29:34.880
<v Speaker 1>the reason you and I are here, or the whole

0:29:34.880 --> 0:29:37.560
<v Speaker 1>Earth this year, or the whole Sun and our solericism,

0:29:37.600 --> 0:29:40.240
<v Speaker 1>or even maybe even our galaxies here is just the

0:29:40.240 --> 0:29:43.960
<v Speaker 1>the random fluctuation of one little tiny particle way back

0:29:43.960 --> 0:29:46.720
<v Speaker 1>in the Big Bang. Yeah, it's the truth, man, The

0:29:46.720 --> 0:29:49.880
<v Speaker 1>truth is stranger than fiction. That's why. That's why I'm

0:29:49.880 --> 0:29:53.000
<v Speaker 1>a physicist, because you know, the universe will always alarm you.

0:29:53.200 --> 0:29:56.480
<v Speaker 1>The universe is like weirder and hotter and nastier and

0:29:56.560 --> 0:30:01.440
<v Speaker 1>crazier and stranger than anything human could or invent. Right, Well,

0:30:01.480 --> 0:30:04.760
<v Speaker 1>depends on how crazy and weird you are. But how

0:30:04.840 --> 0:30:10.440
<v Speaker 1>hot and where you are that's a whole different podcast.

0:30:15.480 --> 0:30:18.160
<v Speaker 1>So um, I'll have to play this podcast for my son,

0:30:18.240 --> 0:30:20.920
<v Speaker 1>But that basically answers this question, right, like why do

0:30:20.960 --> 0:30:23.600
<v Speaker 1>we have stars and not to the smooth distribution of matter,

0:30:23.720 --> 0:30:26.760
<v Speaker 1>you need two elements. You need quantum mechanics to give

0:30:26.800 --> 0:30:29.760
<v Speaker 1>you any fluctuation to avoid the smoothness, to break the

0:30:30.040 --> 0:30:32.440
<v Speaker 1>balance exactly, to break the balance, and then you need

0:30:32.640 --> 0:30:35.360
<v Speaker 1>inflation to blow it up so that it matters, and

0:30:35.400 --> 0:30:38.320
<v Speaker 1>that gravity can then take over. So it's a complicated

0:30:38.400 --> 0:30:43.440
<v Speaker 1>dance to Gravity takes these small fluctuations and basically exacerbates them, right,

0:30:43.440 --> 0:30:48.600
<v Speaker 1>it makes them, yeah, lumpier and clumpier than than it started. Yeah,

0:30:48.640 --> 0:30:50.719
<v Speaker 1>but remember gravity can only take little lumps and make

0:30:50.720 --> 0:30:53.840
<v Speaker 1>them into bigger lumps, right, It can't make lumps if

0:30:53.880 --> 0:30:58.120
<v Speaker 1>something is totally smooth. All right. Thanks to everyone for

0:30:58.160 --> 0:31:01.320
<v Speaker 1>listening to this lumpy episode and for listening to my

0:31:01.440 --> 0:31:05.200
<v Speaker 1>long explanation to my son's short question. Yeah, and whether

0:31:05.280 --> 0:31:09.040
<v Speaker 1>you're a movie star like Tom Cruise or just a

0:31:09.160 --> 0:31:12.400
<v Speaker 1>scruffy physicists, if you have any question or lumpy or

0:31:12.400 --> 0:31:15.120
<v Speaker 1>smooth or why or why do you have to be

0:31:15.360 --> 0:31:17.880
<v Speaker 1>a movie star or a scruffy physicist? Are you saying

0:31:17.880 --> 0:31:23.600
<v Speaker 1>you can't be both? That that no you can totally

0:31:23.680 --> 0:31:27.000
<v Speaker 1>be both. Totally. Yeah, don't ask me for a counterexample.

0:31:27.040 --> 0:31:29.320
<v Speaker 1>I can't think of one. Maybe maybe in another random

0:31:29.440 --> 0:31:32.600
<v Speaker 1>role of the universe. That's right. Why are you not

0:31:32.680 --> 0:31:39.239
<v Speaker 1>a movie star? Dad? Quantum mechanics, So whether you are

0:31:39.280 --> 0:31:41.720
<v Speaker 1>any of these things, if you have any questions, but

0:31:41.800 --> 0:31:45.160
<v Speaker 1>you can write us at feedback at Daniel and Jorge

0:31:45.320 --> 0:31:47.880
<v Speaker 1>dot com. We love getting your email, We love answering

0:31:47.960 --> 0:31:51.479
<v Speaker 1>questions on Twitter, so get in touch, send us your thoughts.

0:31:51.640 --> 0:31:53.040
<v Speaker 1>And so the next time you look out into the

0:31:53.160 --> 0:31:55.680
<v Speaker 1>night sky and you see all those sparkly stars, just

0:31:55.760 --> 0:31:59.520
<v Speaker 1>think everything is there. You are there because the one

0:32:00.000 --> 0:32:02.080
<v Speaker 1>and them part of them. But you still have to

0:32:02.080 --> 0:32:05.400
<v Speaker 1>pay your taxes and your speeding tickets unless you can

0:32:05.400 --> 0:32:16.920
<v Speaker 1>talk your way out of them. If you still have

0:32:16.960 --> 0:32:20.360
<v Speaker 1>a question after listening to all these explanations, please drop

0:32:20.440 --> 0:32:22.520
<v Speaker 1>us a line. We'd love to hear from you. You

0:32:22.520 --> 0:32:25.959
<v Speaker 1>can find us at Facebook, Twitter, and Instagram at Daniel

0:32:26.000 --> 0:32:29.520
<v Speaker 1>and Jorge That's one word, or email us at feedback

0:32:29.560 --> 0:32:40.520
<v Speaker 1>at Daniel and Orge dot com.