WEBVTT - Is our solar system weird?

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<v Speaker 1>Ay, Daniel, When you were growing up, when did you

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<v Speaker 1>first realize that the rest of the world was not

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<v Speaker 1>like the neighborhood you lived in. Mmm, well, I grew

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<v Speaker 1>up in Los Alngos, where I was surrounded by people

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<v Speaker 1>with pH d s, and now I live on campus

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<v Speaker 1>at you see Irvine, also surrounded by people with PhDs.

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<v Speaker 1>Are you saying that's not typical? First of all, I

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<v Speaker 1>feel a little sad for you. The second, I think

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<v Speaker 1>maybe you need to travel more. Hey, I mean I

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<v Speaker 1>have lots of friends who don't have PhDs like me,

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<v Speaker 1>And you mean you do know I have a PhD. Right, Oh,

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<v Speaker 1>that's true. Actually, well, I'm sure one of my friends

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<v Speaker 1>out there doesn't have a PhD in something. Probably sometimes

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<v Speaker 1>you have to leave your comfort zone to discover what

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<v Speaker 1>the rest of the world or the universe is. Like.

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<v Speaker 1>Hi am or hand Ma cartoonists and the creator of

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<v Speaker 1>PhD comics. Hi, I'm Daniel. I'm a particle physicist by

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<v Speaker 1>day and a podcaster by night. It makes it sound

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<v Speaker 1>like you're a superhero. Like you you put on a

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<v Speaker 1>costume and you go and fight crime and discover things. Wait,

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<v Speaker 1>which is the alter ego and which is a superhero.

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<v Speaker 1>Ag are you saying particle physicists are superheroes or podcasters? Well,

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<v Speaker 1>since I'm not a physicist, I would say the podcasters

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<v Speaker 1>are the superhero. That's right. By day, a boring, run

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<v Speaker 1>of the mill particle physicists like the kind you meet

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<v Speaker 1>at your grocery store every day. No more like during

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<v Speaker 1>the day. You're a physicist scientists supervillain during night, then

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<v Speaker 1>you try to fix fixed by being a podcaster. That's right,

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<v Speaker 1>And I take off my glasses to reveal my secret

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<v Speaker 1>podcast identity. You shave your beard every night never. That

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<v Speaker 1>is the source of my knowledge and inspiration, source of

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<v Speaker 1>your source of professor male professor's powers. That's right. I

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<v Speaker 1>am the Samson of physics. Before I grew this beard,

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<v Speaker 1>I never achieved anything in science. Oh man, what if

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<v Speaker 1>you could a got Does that cut your productivity? You

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<v Speaker 1>can have? It's nonlinear. Well, welcome to our podcast, Daniel

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<v Speaker 1>and Jorge Explain the Universe, a production of I Heart

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<v Speaker 1>Radio in which we tackle all things about the universe

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<v Speaker 1>that are mysterious, that are amazing, that are bonkers, from

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<v Speaker 1>how the universe was formed, to how big is it?

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<v Speaker 1>To how old the Earth is, to whether or not

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<v Speaker 1>your facial hair determines your evil or innocence yep. Or

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<v Speaker 1>whether being a podcaster makes you a superhero or not.

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<v Speaker 1>I think we all know the answer to that one.

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<v Speaker 1>But basically, we talk about all the things that are

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<v Speaker 1>interesting and different and fascinating about our universe right especially

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<v Speaker 1>the things around us, and we try to focus on

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<v Speaker 1>the things that science is asking right now, the questions

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<v Speaker 1>in the minds of scientists. We try to take you

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<v Speaker 1>to the cutting edge of current science and then do

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<v Speaker 1>obscurify it. We don't use complicated words like de obscurify.

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<v Speaker 1>We try to make things clear and understandable. You just

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<v Speaker 1>contradicted yourself there. I feel like we try to explain

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<v Speaker 1>things in the simplest way possible. When we explain it

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<v Speaker 1>are explaining, we use the most complicated words possible. Hey,

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<v Speaker 1>this is Daniel Jorge explained the universe, not Daniel Jorge

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<v Speaker 1>explained the explaining and then welcome through new podcast Daniel

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<v Speaker 1>and Jorge explain. Daniel and Jorge explain the universe. That's right,

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<v Speaker 1>the spinoff podcast exactly. I'm looking forward to that one.

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<v Speaker 1>A lot of TV shows now having like an aftershow,

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<v Speaker 1>So that's the better off solid podcasts. Yeah, let's talk

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<v Speaker 1>Daniel and Jorge podcast. Doesn't that need to have somebody

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<v Speaker 1>else on it though, where they can ridicule all of

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<v Speaker 1>our jokes. Yeah, let's pretend to be some other person. Oh,

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<v Speaker 1>there you go. I'll be David and you'll be Gearmo.

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<v Speaker 1>David and Jose. David Jose ridiculed Daniel and Jorge. Al right, well, yeah,

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<v Speaker 1>we talked about all the things scientists want to know

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<v Speaker 1>and um and how they look at the universe as well, right, Like,

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<v Speaker 1>you know, one way to look at the universe is

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<v Speaker 1>to compare it to the things around us. That's right,

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<v Speaker 1>and something we're always trying to do in sciences. Understand

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<v Speaker 1>our context is understand where we live, because hey, this

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<v Speaker 1>is our planet in our solar system. We'd like to

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<v Speaker 1>know is the rest of the of the universe similar

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<v Speaker 1>to what we're finding around us or is it totally different? Yeah,

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<v Speaker 1>because we like the Earth presumably, and it's pretty comfortable.

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<v Speaker 1>And I'm pro Earth. Your pro it's pretty I'm taking

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<v Speaker 1>a controversial opinion here at night, you're pro probably during

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<v Speaker 1>the day your entire Earth. Well, it's not like particle

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<v Speaker 1>physicists threatened to destroy the universe at any moment, so

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<v Speaker 1>on purpose, right, Hey, intentions matter. Okay, I'm sure they

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<v Speaker 1>matter once we're all made out of dissolved particles now.

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<v Speaker 1>But we want to understand the world around us, and

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<v Speaker 1>we want to understand if there are other worlds out there,

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<v Speaker 1>and we'd also just like to know is the thing

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<v Speaker 1>that we've been studying for the entire history of science

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<v Speaker 1>is it normal? Is it typical? Or are we studying

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<v Speaker 1>something which turns out to be really unusual and that

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<v Speaker 1>we can't generalize from to get sort of deeper truths

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<v Speaker 1>about the nature of the universe. Yeah, we like the Earth,

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<v Speaker 1>we like our solar system, but um is the rest

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<v Speaker 1>of the universe like us. And we're an amazing moment

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<v Speaker 1>in human history when we're for the first time really

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<v Speaker 1>getting glimpses for what the rest of the universe looked like.

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<v Speaker 1>You know, for thousands of years, all we could see

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<v Speaker 1>where other stars, but didn't even know if there were

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<v Speaker 1>other planets out there. And then fairly recently in human history,

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<v Speaker 1>thousands of years ago we discovered that there are other

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<v Speaker 1>planets out there. And now super recently, just like twenty

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<v Speaker 1>years ago, we've begun seeing planets around other stars. So

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<v Speaker 1>we can now ask and answer this question people have

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<v Speaker 1>been wondering about four thousands and thousands of years. So

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<v Speaker 1>today on the podcast, we'll be asking the question, is

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<v Speaker 1>our solar system weird or typical? And either way we

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<v Speaker 1>love it. Right, it's our solar system, whatever label you

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<v Speaker 1>put on it, we like it. But we're still curious.

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<v Speaker 1>Is it sort of the oddball solar system it's the

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<v Speaker 1>only one we've been studying for a long time, or

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<v Speaker 1>is it pretty typical? Yeah, this is a really cool question.

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<v Speaker 1>And because you know, I think we grew we grew

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<v Speaker 1>up in this solar system, right, and we don't have

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<v Speaker 1>we have no idea whether it's every other solar system

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<v Speaker 1>looks like this one, or whether we're like, it's really weird,

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<v Speaker 1>odd special gem or disaster, depending on how things work

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<v Speaker 1>out of a solar system. Yeah, and it's all we

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<v Speaker 1>could have studied for the long this time because our

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<v Speaker 1>telescopes couldn't see any further, so we were limited to

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<v Speaker 1>only looking at our cosmic neighborhood, to studying our planet

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<v Speaker 1>and the ones nearby, and so of course we were

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<v Speaker 1>curious what else was out there in the rest of

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<v Speaker 1>the universe. But imagine if you had only lived in

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<v Speaker 1>your hometown your whole life, and you never received any

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<v Speaker 1>news in the outside world, and so you didn't know

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<v Speaker 1>that people eight differently in other countries, and people went

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<v Speaker 1>to the bathroom differently in other countries, and dressed differently

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<v Speaker 1>and spoke differently. You imagined that everything else in the

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<v Speaker 1>world was sort of like your hometown. That's where we

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<v Speaker 1>are right now in science we're wondering if those other

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<v Speaker 1>solar systems are totally different or just the same as ours. Yeah,

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<v Speaker 1>you're saying humanity sort of like a like those mirror

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<v Speaker 1>cats you've seen documentaries. We were just finally sticking our

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<v Speaker 1>head out of the hole in the ground that we've

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<v Speaker 1>been living in and looking around this. Yeah, but we've

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<v Speaker 1>been desperate to do it for for a long time,

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<v Speaker 1>and we've only recently built a technology that's let us

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<v Speaker 1>see other solar systems and start to get an answer

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<v Speaker 1>to this question, because you know, I feel like most

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<v Speaker 1>people just assume that the rest of the universe looks

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<v Speaker 1>like our solar system and our planet, right Like, if

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<v Speaker 1>you look at most science fiction TV shows and movies,

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<v Speaker 1>you know, everywhere they go, it sort of looks suspiciously

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<v Speaker 1>like Earth. Yeah, And I think that's a failure of imagination,

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<v Speaker 1>especially on the part of science fiction. When you fly

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<v Speaker 1>to another planet and you know, hey, it has oxygen

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<v Speaker 1>on it and trees and hills and water that looks

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<v Speaker 1>just like ours, and oh, people on it that look

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<v Speaker 1>just like ours, but their foreheads are slightly wrinkly. I

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<v Speaker 1>think that's a failure of imagination. But it's also sort

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<v Speaker 1>of understandable because it's hard to imagine things totally different

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<v Speaker 1>from anything you've ever seen before. That's why good science

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<v Speaker 1>fiction is rare. Did you just insult All Star Trek

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<v Speaker 1>and Star Wars that was supposed to be sort of

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<v Speaker 1>like a subtweet? Didn't mention it by name, but yeah, yeah.

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<v Speaker 1>And so the question is are those science fiction movies right?

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<v Speaker 1>Are Are there really other earths out there? Are other

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<v Speaker 1>solar systems like ours? Or are we unique in this universe?

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<v Speaker 1>And so, as usual, we were wondering how what people

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<v Speaker 1>thought about this question, whether people thought that we are

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<v Speaker 1>unique or whether things are very different out there in

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<v Speaker 1>the verse. So I walk around campus and I asked

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<v Speaker 1>random students about other random solar systems. I think, for

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<v Speaker 1>a moment, do you think other solar systems look like ours?

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<v Speaker 1>Is our solar system typical or is our solar system

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<v Speaker 1>going to turn out to be really weird? The galactic oddball.

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<v Speaker 1>Here's what people had to say. From what I know,

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<v Speaker 1>it's typical. Um, I mean it depends what you say.

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<v Speaker 1>Typical is considering there billions of stars, but it's not unusual. No,

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<v Speaker 1>I have no idea. It's probably random. If there were

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<v Speaker 1>gases on a planet that were closer to the Sun

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<v Speaker 1>or like star, maybe they would like dissipate faster. I

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<v Speaker 1>think that it's ranks. I think you say I do

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<v Speaker 1>not know. I think it's random, and I think it's

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<v Speaker 1>going to be different Because our solar system it revolves

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<v Speaker 1>around the Sun. I think other systems are gonna be different.

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<v Speaker 1>So what do you think of those answers? Or pretty good?

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<v Speaker 1>I thought I felt like people had a strong opinion

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<v Speaker 1>about this topic. You know, everyone said I think it's X.

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<v Speaker 1>Nobody said I don't know or only one. Only a

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<v Speaker 1>few people said I had no idea, But a lot

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<v Speaker 1>of people that were like, I think I have an

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<v Speaker 1>opinion about this. Yeah, given that nobody really knows the

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<v Speaker 1>answer to this question, I was a little surprised at

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<v Speaker 1>the strength of people's opinions. I mean, I often ask

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<v Speaker 1>people questions and they go, I have no idea quantum what.

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<v Speaker 1>But this time people had an opinion. And maybe that's

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<v Speaker 1>just because people have thought about this. They've wondered what

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<v Speaker 1>other solar systems look like. They've thought about traveling to

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<v Speaker 1>the stars and walking on those planets and wondered if

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<v Speaker 1>they would be like ours. I wonder if you would

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<v Speaker 1>get different answers if you caveat each time you ask

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<v Speaker 1>these questions, If you caveat them with oh, and by

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<v Speaker 1>the way, some of the smartest people in the world

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<v Speaker 1>don't know the answer to this, I would be so

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<v Speaker 1>much less fun. Who would want to answer that? Nobody?

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<v Speaker 1>I love when people speculated. I of seeing them in

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<v Speaker 1>their minds sort of take this question on and sometimes

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<v Speaker 1>for the first time and formulate an answer. And my

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<v Speaker 1>favorite moments are when you can see somebody giving an

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<v Speaker 1>answer that sort of surprises themselves. They think about it,

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<v Speaker 1>they give an answer that, oh, I didn't realize I

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<v Speaker 1>do think that. That's fascinating. Makes me wonder how much

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<v Speaker 1>we actually think about the things we say. Sometimes I'm

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<v Speaker 1>just listening to my own self talking, I'm like, what

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<v Speaker 1>did he just say? So that's the question of the day.

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<v Speaker 1>Is is our solar system unique? Or is it pretty typical?

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<v Speaker 1>And if it's not typical, how different could it be

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<v Speaker 1>out there? And you should count yourself lucky to live

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<v Speaker 1>in a time when we will know the answer to

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<v Speaker 1>this question. Some of the greatest minds in history, Galileo Einstein, Newton,

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<v Speaker 1>even recent people like Richard Feynman, they looked up at

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<v Speaker 1>the stars and they wondered if other solar systems look

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<v Speaker 1>like ours. They all died not knowing the answer. All

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<v Speaker 1>you have to do is listen to this podcast. Yeah,

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<v Speaker 1>so you're welcome. Are you taking it for all the

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<v Speaker 1>scientific discoveries? Thank you? Or hey who personally built the

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<v Speaker 1>Hubble space telescope with his own hands? I signed the

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<v Speaker 1>back of it. I don't know if anyone will ever

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<v Speaker 1>you drew a doodle on it? Are you the official

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<v Speaker 1>cartoonist of the space telescope? Technically you can't prove that

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<v Speaker 1>I didn't sign the back of the Hubble telescope. Oh

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<v Speaker 1>I need another telescope trained on the space telescope to

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<v Speaker 1>see the back of it. I wonder if anybody ever

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<v Speaker 1>does that, But yeah, do you think so? Yeah, it's

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<v Speaker 1>an interesting question. I'm sure a lot of people have

0:12:25.920 --> 0:12:28.920
<v Speaker 1>asked before. So let's break it down for people, Daniel.

0:12:29.000 --> 0:12:32.320
<v Speaker 1>Let's talk about our solar system, and then let's talk

0:12:32.360 --> 0:12:35.400
<v Speaker 1>about what other solar system. Well, we know about other

0:12:35.440 --> 0:12:39.400
<v Speaker 1>solar systems out there, right, and our solar system is

0:12:39.440 --> 0:12:42.800
<v Speaker 1>actually quite fascinating because it has some sort of trends

0:12:42.840 --> 0:12:45.480
<v Speaker 1>in it. And you have to remember that all of

0:12:45.520 --> 0:12:47.840
<v Speaker 1>our knowledge of solar systems and how they're formed, all

0:12:47.840 --> 0:12:51.120
<v Speaker 1>of our theories how solar systems were built, have been

0:12:51.160 --> 0:12:54.000
<v Speaker 1>developed over decades or hundreds of years based on just

0:12:54.080 --> 0:12:58.079
<v Speaker 1>this one example, our solar system. So you know, we

0:12:58.160 --> 0:13:01.680
<v Speaker 1>sort of tuned these theories to describe what we've seen here,

0:13:01.800 --> 0:13:04.000
<v Speaker 1>and now comes the big test to see whether these

0:13:04.080 --> 0:13:07.200
<v Speaker 1>theories can be applied and explain other solar systems, right,

0:13:07.200 --> 0:13:09.440
<v Speaker 1>Because I think maybe people a lot of people don't

0:13:09.440 --> 0:13:13.360
<v Speaker 1>realize that we can't. Just up until very very recently,

0:13:13.400 --> 0:13:16.320
<v Speaker 1>and only just now barely, we haven't really been able

0:13:16.400 --> 0:13:19.400
<v Speaker 1>to like take a telescope pointing at another star and

0:13:19.720 --> 0:13:23.319
<v Speaker 1>see another solar system, right like it's up until very

0:13:23.400 --> 0:13:26.760
<v Speaker 1>very recently, it's been a complete mystery. What other solar

0:13:26.800 --> 0:13:29.600
<v Speaker 1>systems look like? Yeah, the first planet around another star

0:13:29.800 --> 0:13:32.840
<v Speaker 1>was seen just over twenty years ago, so it's a

0:13:32.920 --> 0:13:36.040
<v Speaker 1>blip in human history and even in scientific history. But

0:13:36.200 --> 0:13:38.320
<v Speaker 1>even before we talk about the other solar systems, our

0:13:38.360 --> 0:13:41.480
<v Speaker 1>solar system is interesting, like there are some weird trends

0:13:41.480 --> 0:13:43.880
<v Speaker 1>in it. You know, the first four planets in the

0:13:43.880 --> 0:13:47.240
<v Speaker 1>Solar System are all rocky planets. Planets basically come in

0:13:47.280 --> 0:13:51.319
<v Speaker 1>two flavors, rocky or gassy. It sounds like sounds like

0:13:51.360 --> 0:13:55.880
<v Speaker 1>a bad ice cream shop. Yeah, like like like what

0:13:55.960 --> 0:13:57.959
<v Speaker 1>happens when I like those into olm prison goes to

0:13:58.000 --> 0:14:01.480
<v Speaker 1>an ice cream shop? Yeah, well, the first four planets

0:14:01.520 --> 0:14:04.480
<v Speaker 1>have surfaces on them, right, You've got Mercury, Venus, Earth,

0:14:04.480 --> 0:14:07.760
<v Speaker 1>and Mars. These are basically balls of rock, rock and metal.

0:14:08.280 --> 0:14:11.080
<v Speaker 1>And so we call those rocky planets. And there's no

0:14:11.200 --> 0:14:13.760
<v Speaker 1>gas planets in the inner flour And said, you know

0:14:13.840 --> 0:14:16.320
<v Speaker 1>the four rocky planets, then you have the asteroid belt

0:14:16.320 --> 0:14:18.520
<v Speaker 1>that we dug into in a recent episode. And then

0:14:18.640 --> 0:14:21.200
<v Speaker 1>after the asteroid belt, you've got the gas giants and

0:14:21.200 --> 0:14:23.880
<v Speaker 1>the ice giants. You got Saturned, You've got Jupiter, you've

0:14:23.880 --> 0:14:26.880
<v Speaker 1>got Urinus and Neptune, and those are pretty different from

0:14:26.920 --> 0:14:28.960
<v Speaker 1>the inner planets. Is there a reason we don't have

0:14:29.120 --> 0:14:33.040
<v Speaker 1>liquid planets or like wet planets or like giant balls

0:14:33.080 --> 0:14:36.080
<v Speaker 1>of of a liquid floating around. Well, we can't have

0:14:36.280 --> 0:14:38.800
<v Speaker 1>liquid planets. In the far Solar System. We have basically

0:14:38.880 --> 0:14:41.240
<v Speaker 1>ice giants Uranus and Neptune. A huge fraction of them

0:14:41.280 --> 0:14:43.200
<v Speaker 1>is made of water, but it's frozen. Of course, it's

0:14:43.200 --> 0:14:45.640
<v Speaker 1>too cold out there. There is of course water here

0:14:45.680 --> 0:14:47.720
<v Speaker 1>on Earth. But could you have just like an entire

0:14:47.840 --> 0:14:50.400
<v Speaker 1>drop of water be a planet, that would be pretty amazing.

0:14:50.440 --> 0:14:53.840
<v Speaker 1>I think the pressure from it would probably crystallize the inside.

0:14:53.880 --> 0:14:57.320
<v Speaker 1>So basically become an ice planet with a ocean around it,

0:14:58.000 --> 0:15:02.080
<v Speaker 1>kind of like a Europa or what's what's the wound

0:15:02.120 --> 0:15:05.280
<v Speaker 1>that's like a giant ocean. Yeah, Europa has a huge,

0:15:05.320 --> 0:15:08.680
<v Speaker 1>actually thick crust of ice on top and then a

0:15:08.800 --> 0:15:11.720
<v Speaker 1>layer of water underneath, like an ocean underneath, and then

0:15:11.800 --> 0:15:13.760
<v Speaker 1>we don't know what's inside of that. So that's like

0:15:13.800 --> 0:15:15.840
<v Speaker 1>an eminem sort of. But as the reason we don't

0:15:15.840 --> 0:15:19.480
<v Speaker 1>have liquid planets, just just depending on the elements that

0:15:19.520 --> 0:15:21.520
<v Speaker 1>we have in our Solar system, I don't think you

0:15:21.560 --> 0:15:25.400
<v Speaker 1>can make a blob of of liquid water large enough

0:15:25.760 --> 0:15:28.320
<v Speaker 1>stay liquid because the core of it would just be

0:15:28.320 --> 0:15:30.400
<v Speaker 1>too dense. It would form a solid, like by the

0:15:30.440 --> 0:15:32.640
<v Speaker 1>time it got big enough to be called the planet,

0:15:33.120 --> 0:15:35.760
<v Speaker 1>would it would totally not be liquid. Yeah, the gravitational

0:15:35.800 --> 0:15:38.160
<v Speaker 1>pressure would make the inside of it become a solid

0:15:38.280 --> 0:15:40.920
<v Speaker 1>or or something more dense, so it wouldn't be liquid anymore.

0:15:41.120 --> 0:15:43.080
<v Speaker 1>Do you have this fantasy of swimming through like a

0:15:43.120 --> 0:15:48.200
<v Speaker 1>planet sized pool of water? The universe is biggest swimming pool.

0:15:48.200 --> 0:15:51.960
<v Speaker 1>That would be pretty cool, nothing but a huge drop

0:15:51.960 --> 0:15:53.320
<v Speaker 1>of water the size of the Earth and then a

0:15:53.360 --> 0:15:57.680
<v Speaker 1>single diving boards. You're like, you think you have an

0:15:57.680 --> 0:16:02.920
<v Speaker 1>infinity pool. I have a planet universe universe infinity pool.

0:16:03.960 --> 0:16:05.720
<v Speaker 1>But no, we don't have any liquid planets in our

0:16:05.720 --> 0:16:08.920
<v Speaker 1>solar system. But hey, maybe you know, we'll find planets

0:16:08.960 --> 0:16:11.040
<v Speaker 1>in other solar systems that are liquids and that will

0:16:11.080 --> 0:16:14.040
<v Speaker 1>prove us wrong, and maybe liquid planets are possible, but

0:16:14.080 --> 0:16:16.320
<v Speaker 1>we don't happen to have any in our solar systems.

0:16:16.320 --> 0:16:19.240
<v Speaker 1>That we have four rocky planets the asteroid belt and

0:16:19.280 --> 0:16:22.280
<v Speaker 1>then the gas giants and the ice giants. And you're saying,

0:16:22.280 --> 0:16:24.080
<v Speaker 1>that's kind of funny in that it's sort of like

0:16:24.120 --> 0:16:28.080
<v Speaker 1>a pattern, like it's four rocky asteroid belt gas giants.

0:16:28.080 --> 0:16:32.960
<v Speaker 1>It's not like rocky gas, rocky gas gas gas rocky. Yeah,

0:16:33.000 --> 0:16:36.000
<v Speaker 1>it doesn't seem random. Here's a question from a listener,

0:16:36.040 --> 0:16:40.200
<v Speaker 1>Camille who thought just the same thing. Hello, Danielle and Jey.

0:16:40.600 --> 0:16:43.160
<v Speaker 1>One of the recent episodes I have listened to your show,

0:16:43.160 --> 0:16:46.000
<v Speaker 1>which was all about the asteroid belt, you, daniel mentioned

0:16:46.000 --> 0:16:48.480
<v Speaker 1>that there must be a reason why we have solid

0:16:48.640 --> 0:16:52.480
<v Speaker 1>rocky planets before the asteroid belt and then only gas

0:16:52.520 --> 0:16:56.320
<v Speaker 1>giants afterwards. But you never got to answering this question,

0:16:56.440 --> 0:16:58.360
<v Speaker 1>is there a reason we know? Why? Is it like

0:16:58.480 --> 0:17:01.800
<v Speaker 1>this that we see these kind of pattern other stuff?

0:17:02.040 --> 0:17:05.280
<v Speaker 1>I'm dying to know. That's such a good point. Thank

0:17:05.320 --> 0:17:08.320
<v Speaker 1>you Camille for sending in that question. And every time

0:17:08.359 --> 0:17:10.280
<v Speaker 1>you see a pattern, you think maybe there's a reason

0:17:10.520 --> 0:17:12.680
<v Speaker 1>and you want to untangle that reason. Now, it's very

0:17:12.800 --> 0:17:16.480
<v Speaker 1>dangerous when you're drawing conclusions from one example. If you

0:17:16.560 --> 0:17:19.080
<v Speaker 1>visit somebody's house and they're like, oh, look, their family

0:17:19.240 --> 0:17:22.080
<v Speaker 1>is boy boy, boy, boy boy, girl, girl, girl, girl girl,

0:17:22.359 --> 0:17:24.359
<v Speaker 1>you're going to conclude there's a reason, right that they

0:17:24.400 --> 0:17:26.440
<v Speaker 1>all have younger girls and older boys. But if you're

0:17:26.440 --> 0:17:28.960
<v Speaker 1>only looking at one house, you're gonna be totally wrong.

0:17:29.080 --> 0:17:32.480
<v Speaker 1>That would be kind of impolite to ask Daniel. You're like,

0:17:32.520 --> 0:17:35.720
<v Speaker 1>did you guys try are you're doing something different? You

0:17:35.720 --> 0:17:39.560
<v Speaker 1>know when you um um, you know you'd be desperate

0:17:39.560 --> 0:17:43.640
<v Speaker 1>to know though, you'd be super curious. And also, there's

0:17:43.680 --> 0:17:45.959
<v Speaker 1>lots of families where it's like five boys and then

0:17:46.000 --> 0:17:47.600
<v Speaker 1>a girl, and you know that they were trying for

0:17:47.640 --> 0:17:49.760
<v Speaker 1>a girl and they finally got one and that's when

0:17:49.760 --> 0:17:52.119
<v Speaker 1>they stopped having kids. That's when they're like, we're a

0:17:52.160 --> 0:17:55.800
<v Speaker 1>closing shop. Yeah, so maybe our source systems close shops

0:17:55.840 --> 0:17:59.959
<v Speaker 1>after after Neptune or uranus. We're done trying to make

0:18:00.000 --> 0:18:05.560
<v Speaker 1>a liquid planet. It's not happening. We're sorry, we're trying

0:18:05.560 --> 0:18:07.679
<v Speaker 1>to make a giant swimming pool, but you know, it

0:18:07.760 --> 0:18:09.720
<v Speaker 1>just hasn't happened. That's right. The kid's gotta go swim

0:18:09.760 --> 0:18:12.320
<v Speaker 1>somewhere else. But so we do have some explanations we've

0:18:12.359 --> 0:18:14.360
<v Speaker 1>cooked up, but of course the proviso is, we don't

0:18:14.400 --> 0:18:16.399
<v Speaker 1>know if this works until we try to apply to

0:18:16.440 --> 0:18:19.639
<v Speaker 1>other solar systems. And the basic idea is that you

0:18:19.680 --> 0:18:23.879
<v Speaker 1>don't get gas giants close into the sun because the

0:18:23.920 --> 0:18:26.800
<v Speaker 1>Sun has all this radiation it spewing up the solar wind,

0:18:27.119 --> 0:18:30.800
<v Speaker 1>and that basically blows out all the light elements, the hydrogen,

0:18:30.960 --> 0:18:32.919
<v Speaker 1>the helium, all the stuff you need to make a

0:18:32.960 --> 0:18:35.560
<v Speaker 1>gas giant, all the gas. It blows it away from

0:18:35.560 --> 0:18:37.800
<v Speaker 1>the Sun. So that's why you don't have gas giants

0:18:37.800 --> 0:18:40.479
<v Speaker 1>close up to their star. It's kind of like a cloud.

0:18:41.200 --> 0:18:42.840
<v Speaker 1>It gets too close to the Sun, which is kind

0:18:42.840 --> 0:18:45.920
<v Speaker 1>of wish evaprate. Yeah, and so that's sort of the

0:18:45.960 --> 0:18:49.199
<v Speaker 1>explanation for why you have rocky planets close in. And

0:18:49.240 --> 0:18:52.520
<v Speaker 1>then in the outer planets it's colder, and so instead

0:18:52.520 --> 0:18:54.720
<v Speaker 1>of having liquid water, you have ice, and then that

0:18:54.840 --> 0:18:57.359
<v Speaker 1>ice helps the core of the planet's form. You're like,

0:18:57.680 --> 0:19:00.159
<v Speaker 1>you know, how does the planet form? Anyway, You the

0:19:00.200 --> 0:19:03.320
<v Speaker 1>initial sort of disc of stuff from the that formed

0:19:03.320 --> 0:19:05.520
<v Speaker 1>the whole Solar System, and some of it is spinning

0:19:05.600 --> 0:19:07.720
<v Speaker 1>so it doesn't fall into the star. And then in

0:19:07.800 --> 0:19:10.520
<v Speaker 1>the outer reaches, it's cold enough that you have ice

0:19:10.760 --> 0:19:13.879
<v Speaker 1>and that helps accumulate the gravity very slowly gather the

0:19:13.920 --> 0:19:16.360
<v Speaker 1>stuff together. Because you have ice out there, it can

0:19:16.359 --> 0:19:19.760
<v Speaker 1>sort of add ice to your basic planet core and

0:19:19.800 --> 0:19:22.320
<v Speaker 1>they can get big enough to suck up all the

0:19:22.400 --> 0:19:25.920
<v Speaker 1>gas and the hydrogen in the helium. Because remember hydrogen

0:19:26.000 --> 0:19:28.480
<v Speaker 1>helium is very light, which means it's hard to hold onto.

0:19:28.520 --> 0:19:31.679
<v Speaker 1>You need a huge gravitational mass to attract that. So

0:19:31.720 --> 0:19:33.600
<v Speaker 1>to make a gas giant, you have to form a

0:19:33.680 --> 0:19:37.040
<v Speaker 1>really big core of some metals and some ice in

0:19:37.119 --> 0:19:38.960
<v Speaker 1>order to pull in the rest of the gas. And

0:19:39.040 --> 0:19:41.280
<v Speaker 1>that can only happen in the outer reaches of the

0:19:41.280 --> 0:19:43.879
<v Speaker 1>solar system, where you have ice. And so the reason

0:19:43.960 --> 0:19:46.119
<v Speaker 1>you get gas giants and the outer Solar system is

0:19:46.280 --> 0:19:49.200
<v Speaker 1>because that's where the gas is and because that's where

0:19:49.200 --> 0:19:52.400
<v Speaker 1>the ice is to help pull those light gases together

0:19:52.760 --> 0:19:55.240
<v Speaker 1>into a gas giant. At least that's our theory, and

0:19:55.280 --> 0:19:57.879
<v Speaker 1>that's based on just what we've observed, all right. So

0:19:58.200 --> 0:20:01.679
<v Speaker 1>that explains why our solar system looks to wait us,

0:20:01.720 --> 0:20:05.360
<v Speaker 1>why it's like rocky in the middle and then gassie

0:20:05.520 --> 0:20:08.560
<v Speaker 1>out there in the edges of it. And so that's

0:20:08.640 --> 0:20:10.359
<v Speaker 1>kind of the picture of our solar system. We have

0:20:10.400 --> 0:20:14.280
<v Speaker 1>a yellow sun, some rocky planets, some asteroids, and then

0:20:14.480 --> 0:20:19.359
<v Speaker 1>giant gas balls um swirling around the edges of them, precisely.

0:20:19.440 --> 0:20:22.240
<v Speaker 1>And remember we've been aware of this for decades and

0:20:22.320 --> 0:20:24.920
<v Speaker 1>decades and decades and so we had a long time

0:20:24.960 --> 0:20:27.440
<v Speaker 1>to cook up this model based on just this one

0:20:27.600 --> 0:20:31.080
<v Speaker 1>solar system. It's become very fine tuned and and very

0:20:31.080 --> 0:20:34.240
<v Speaker 1>sort of baroque to explain exactly what we're seeing. And

0:20:34.280 --> 0:20:36.720
<v Speaker 1>so now comes the test. Now we get to apply

0:20:36.840 --> 0:20:39.160
<v Speaker 1>it to other solar systems and see if it also

0:20:39.200 --> 0:20:41.800
<v Speaker 1>explains what we see out there. Yeah, all right, so

0:20:41.880 --> 0:20:45.840
<v Speaker 1>let's get into what other solar systems look like. But

0:20:45.960 --> 0:21:01.320
<v Speaker 1>first let's take a quick break. All right, we're talking

0:21:01.359 --> 0:21:04.199
<v Speaker 1>about how our solar system may or may not be

0:21:04.280 --> 0:21:07.000
<v Speaker 1>different than other solar systems out there, and we know

0:21:07.080 --> 0:21:09.199
<v Speaker 1>that we have a pretty good picture you're saying, of

0:21:09.240 --> 0:21:11.320
<v Speaker 1>our solar system, and it's taken as a while, but

0:21:11.400 --> 0:21:13.760
<v Speaker 1>we can have a good idea of how our solar

0:21:13.800 --> 0:21:17.439
<v Speaker 1>system formed sort of and or white looks like rocky

0:21:17.480 --> 0:21:20.440
<v Speaker 1>planets and then gas giants. And so now the question

0:21:20.640 --> 0:21:23.800
<v Speaker 1>is is this what other solar systems look like like?

0:21:23.840 --> 0:21:26.600
<v Speaker 1>If I went to a nearby star, would I also

0:21:26.640 --> 0:21:30.359
<v Speaker 1>see you know, a similar sun, similar rocky planets in

0:21:30.359 --> 0:21:34.480
<v Speaker 1>the middle, and similar gas giants on the edges? Yea,

0:21:34.560 --> 0:21:36.800
<v Speaker 1>So maybe we should start from the center, right from

0:21:36.840 --> 0:21:39.240
<v Speaker 1>the star. That is, of course the easiest thing to see.

0:21:39.560 --> 0:21:41.800
<v Speaker 1>Our star is something we call a yellow dwarf, and

0:21:41.840 --> 0:21:44.560
<v Speaker 1>it turns out that even our kind of star is unusual.

0:21:45.000 --> 0:21:47.600
<v Speaker 1>Only like ten of the stars in our galaxy are

0:21:47.720 --> 0:21:49.919
<v Speaker 1>yellow dwarfs. The rest are something else we call a

0:21:50.040 --> 0:21:54.600
<v Speaker 1>red dwarf. And these names have to do with not

0:21:54.720 --> 0:21:57.120
<v Speaker 1>just like the size of the Sun, but also how

0:21:57.160 --> 0:21:59.840
<v Speaker 1>old the Sun is. Right, Yeah, they tell you something

0:22:00.200 --> 0:22:02.640
<v Speaker 1>where the Sun is in its life cycle. And there's

0:22:02.680 --> 0:22:04.800
<v Speaker 1>lots of different sort of paths that a sun can

0:22:04.840 --> 0:22:08.600
<v Speaker 1>take depending on how much mass it's started with. And

0:22:08.600 --> 0:22:11.760
<v Speaker 1>we had a whole episode about stellar evolution, and based

0:22:11.760 --> 0:22:13.639
<v Speaker 1>on the size that the Sun started with, they will

0:22:13.680 --> 0:22:16.199
<v Speaker 1>follow a certain path, And so the name of the

0:22:16.200 --> 0:22:18.600
<v Speaker 1>star tells you sort of which path it's on and

0:22:18.640 --> 0:22:21.840
<v Speaker 1>sort of how far along that path is. But most

0:22:21.880 --> 0:22:24.680
<v Speaker 1>of the stars in our galaxy are red dwarfs, which

0:22:24.720 --> 0:22:27.639
<v Speaker 1>mean that they're older than our Sun, and they're colder

0:22:27.760 --> 0:22:30.399
<v Speaker 1>and they're smaller. So if you want as much heat

0:22:30.680 --> 0:22:32.399
<v Speaker 1>that we as we feel on Earth, you'd have to

0:22:32.400 --> 0:22:35.320
<v Speaker 1>be closer to the star than you would be to ours.

0:22:35.320 --> 0:22:37.639
<v Speaker 1>So our sun is kind of is big for compared

0:22:37.680 --> 0:22:40.040
<v Speaker 1>to other stars in the universe, and it's also kind

0:22:40.080 --> 0:22:42.520
<v Speaker 1>of young, right, Like I think we're sort of like

0:22:42.560 --> 0:22:45.359
<v Speaker 1>in the teenage years of our shunt. It's big compared

0:22:45.400 --> 0:22:47.200
<v Speaker 1>to most of the stars in the galaxy. Of course,

0:22:47.320 --> 0:22:49.639
<v Speaker 1>there are other stars out there that totally dwarf it.

0:22:49.720 --> 0:22:53.840
<v Speaker 1>There these huge giants out there that are fantastically bigger

0:22:54.040 --> 0:22:56.760
<v Speaker 1>than our star, but they're unusual. Most of the stars

0:22:56.760 --> 0:23:00.639
<v Speaker 1>in the galaxy are smaller and colder and older than ours.

0:23:00.800 --> 0:23:03.879
<v Speaker 1>And ours is also different in another really fascinating way,

0:23:04.160 --> 0:23:07.320
<v Speaker 1>in that it's by itself. Our star doesn't have a

0:23:07.320 --> 0:23:10.639
<v Speaker 1>companion star. It's not like there's another star orbiting. It

0:23:10.640 --> 0:23:14.320
<v Speaker 1>turns out most stars actually formed together to like a

0:23:14.359 --> 0:23:17.439
<v Speaker 1>pair of stars. Right, So our son is all alone,

0:23:17.920 --> 0:23:21.880
<v Speaker 1>or or as uh Emma Watson would sage, where our

0:23:21.880 --> 0:23:25.760
<v Speaker 1>son is self partnered. Yea, our star is like the

0:23:25.880 --> 0:23:29.760
<v Speaker 1>runaway teenage star. It's all by itself in this lonely universe.

0:23:30.720 --> 0:23:33.760
<v Speaker 1>Of other stars in the universe are totally different than

0:23:33.800 --> 0:23:37.080
<v Speaker 1>our sun. Yeah. Yeah, so right there. If you want

0:23:37.080 --> 0:23:39.520
<v Speaker 1>to extrapolate from our solar system to others, you have

0:23:39.560 --> 0:23:42.160
<v Speaker 1>to be careful because most solar systems have a very

0:23:42.240 --> 0:23:44.600
<v Speaker 1>different kind of star. And that doesn't mean it's going

0:23:44.640 --> 0:23:46.920
<v Speaker 1>to be a completely different solar system where that it's

0:23:46.920 --> 0:23:49.320
<v Speaker 1>impossible to live there. But it means you want the

0:23:49.359 --> 0:23:51.199
<v Speaker 1>same amount of heat. For example, you have to be

0:23:51.320 --> 0:23:54.800
<v Speaker 1>closer up, so the Goldilocks zone for these stars is

0:23:54.840 --> 0:23:59.160
<v Speaker 1>smaller than it is for our star. The sun is colder,

0:23:59.240 --> 0:24:01.640
<v Speaker 1>and then you need to be closer to it to

0:24:01.720 --> 0:24:03.880
<v Speaker 1>be to have any life as we know it here

0:24:03.920 --> 0:24:06.680
<v Speaker 1>on Earth. Yeah, to have liquid water on the surface,

0:24:06.680 --> 0:24:09.560
<v Speaker 1>for example, which is basically what you need to have life,

0:24:10.080 --> 0:24:13.520
<v Speaker 1>we think life as we defined it. Right, Then they

0:24:13.600 --> 0:24:15.200
<v Speaker 1>need to be close enough to the star to get

0:24:15.320 --> 0:24:18.400
<v Speaker 1>enough radiation, and that would be closer to those smaller,

0:24:18.480 --> 0:24:21.720
<v Speaker 1>colder stars than ours. And so ninety percent of stars

0:24:21.760 --> 0:24:23.800
<v Speaker 1>are different out there, which means that if you are

0:24:23.800 --> 0:24:26.639
<v Speaker 1>in another planet, in another solar system, you know, ninety

0:24:26.680 --> 0:24:28.760
<v Speaker 1>percent of the time, it's not going to look like

0:24:29.000 --> 0:24:30.600
<v Speaker 1>it looks like you're it's not going to look like

0:24:30.640 --> 0:24:36.280
<v Speaker 1>a bright yellow you know son. Yeah, it would be

0:24:36.280 --> 0:24:38.480
<v Speaker 1>a little redder and a little colder. It sounds like

0:24:38.520 --> 0:24:41.439
<v Speaker 1>maybe in a lot of or most solar systems out there,

0:24:41.440 --> 0:24:43.640
<v Speaker 1>it would look like in Star Wars where they see

0:24:43.680 --> 0:24:47.160
<v Speaker 1>two sons in the horizon. Yeah, most of them have companions,

0:24:47.240 --> 0:24:50.680
<v Speaker 1>and those aren't necessarily super close together. Sometimes the companions

0:24:50.680 --> 0:24:53.520
<v Speaker 1>can be kind of far apart. But yeah, most stars

0:24:53.520 --> 0:24:56.760
<v Speaker 1>have another star pretty close by and they're orbiting each other.

0:24:56.960 --> 0:25:00.000
<v Speaker 1>But ours is by itself, and that's that's more unused

0:25:00.040 --> 0:25:03.280
<v Speaker 1>dual than typical. So already our star is unusual in

0:25:03.359 --> 0:25:05.679
<v Speaker 1>two ways, and that it's by itself, and that it's

0:25:05.720 --> 0:25:08.560
<v Speaker 1>a yellow dwarf. So already our solar system is is

0:25:08.600 --> 0:25:12.080
<v Speaker 1>pretty odd compared to the universe. Well, now, let's let's

0:25:12.080 --> 0:25:15.280
<v Speaker 1>talk about the Earth. Is a planet like Planet Earth,

0:25:15.480 --> 0:25:17.920
<v Speaker 1>the weird to have in a solar system out there?

0:25:18.040 --> 0:25:19.879
<v Speaker 1>Or is it pretty common? It turns out that the

0:25:19.920 --> 0:25:22.440
<v Speaker 1>most common planet to have in one of these solar

0:25:22.440 --> 0:25:25.679
<v Speaker 1>systems is not the Earth. It's something called a super Earth.

0:25:26.280 --> 0:25:30.000
<v Speaker 1>It's a rocky planet that's like ten or fifteen times

0:25:30.040 --> 0:25:33.879
<v Speaker 1>bigger than the Earth. And they categorize these planets in

0:25:33.920 --> 0:25:37.560
<v Speaker 1>other solar systems by giving them names relative to our planets,

0:25:37.640 --> 0:25:40.080
<v Speaker 1>like define the various categories. So like you have an

0:25:40.080 --> 0:25:42.080
<v Speaker 1>Earth planet or a super Earth up to you know,

0:25:42.400 --> 0:25:45.199
<v Speaker 1>ten or fifteen times the Earth. Anything bigger than that,

0:25:45.240 --> 0:25:47.879
<v Speaker 1>they call it like a mini Neptune. So that's the

0:25:48.000 --> 0:25:51.960
<v Speaker 1>names of these categories. And most solar systems have a

0:25:52.000 --> 0:25:54.320
<v Speaker 1>super Earth. It's the most common planet out there. Now,

0:25:54.400 --> 0:25:57.159
<v Speaker 1>you'll notice we don't have a super Earth. There's no

0:25:57.280 --> 0:25:59.879
<v Speaker 1>planet in our solar system that's a rocky planet that

0:26:00.000 --> 0:26:02.280
<v Speaker 1>it's like ten times the size of Earth. Is the

0:26:02.320 --> 0:26:05.760
<v Speaker 1>Earth the biggest rocky planet in our solar system? Yeah,

0:26:05.800 --> 0:26:08.040
<v Speaker 1>the Earth and Venus Venus is almost as big as

0:26:08.040 --> 0:26:10.840
<v Speaker 1>the Earth. Mars and Mercury are much smaller. And so

0:26:10.880 --> 0:26:13.639
<v Speaker 1>the Earth is the biggest rocky planet in our solar system.

0:26:13.800 --> 0:26:15.960
<v Speaker 1>But most solar systems you would find one that's like

0:26:16.119 --> 0:26:18.800
<v Speaker 1>ten or fifteen times bigger, bigger in terms of like

0:26:18.840 --> 0:26:21.600
<v Speaker 1>the radius or like the you know, there's the weight

0:26:21.640 --> 0:26:23.960
<v Speaker 1>of it. Yeah, ten times the mass, which doesn't quite

0:26:24.000 --> 0:26:26.440
<v Speaker 1>correspond to ten times the radius because you know, there's

0:26:26.440 --> 0:26:29.479
<v Speaker 1>some nonlinear effects there. But it's a lot more stuff, right,

0:26:29.560 --> 0:26:33.240
<v Speaker 1>So ten times as many rocks came together to form

0:26:33.280 --> 0:26:36.160
<v Speaker 1>a planet, and so we don't really know what that means.

0:26:36.160 --> 0:26:38.560
<v Speaker 1>This is something we've only recently figured out. We don't

0:26:38.560 --> 0:26:40.879
<v Speaker 1>know if that means that the distribution of rocks in

0:26:40.920 --> 0:26:43.800
<v Speaker 1>our solar system was different when it formed, or maybe

0:26:43.800 --> 0:26:45.840
<v Speaker 1>there was a super big planet, but it got broken up.

0:26:46.119 --> 0:26:48.680
<v Speaker 1>We don't really know. Is this just random that we

0:26:48.760 --> 0:26:51.400
<v Speaker 1>not unlucky, or is there some important reason for why

0:26:51.400 --> 0:26:53.800
<v Speaker 1>our solar system looks different in this important way. We

0:26:53.920 --> 0:26:56.080
<v Speaker 1>just don't know. So that if there are scientists on

0:26:56.119 --> 0:26:58.400
<v Speaker 1>those other earths, they would probably say that we live

0:26:58.440 --> 0:27:02.439
<v Speaker 1>in many Earth. Yeah, they would say, hey, look at

0:27:02.440 --> 0:27:05.160
<v Speaker 1>this weird solar system we found. It has only many

0:27:05.280 --> 0:27:07.920
<v Speaker 1>rocky planets. How cute. Look at those tiny little planets,

0:27:09.200 --> 0:27:11.920
<v Speaker 1>Baby Earth's look at those tiny little people with tiny heads.

0:27:13.760 --> 0:27:16.240
<v Speaker 1>Not only is our solar system weird in that that

0:27:16.320 --> 0:27:19.560
<v Speaker 1>our Sun is weird, but also our Earth is really weird.

0:27:20.080 --> 0:27:23.400
<v Speaker 1>So most earths out there are much much bigger. Yeah,

0:27:23.440 --> 0:27:25.760
<v Speaker 1>and some solar systems we found out there just have

0:27:26.000 --> 0:27:28.640
<v Speaker 1>more planets sort of tucked in close to the Sun.

0:27:29.280 --> 0:27:31.719
<v Speaker 1>Like we found this one solar system it's called the

0:27:31.720 --> 0:27:36.879
<v Speaker 1>Trappist System. It has seven planets within six million miles

0:27:36.880 --> 0:27:40.240
<v Speaker 1>of their sun. Remember, the Earth is like ninety million

0:27:40.320 --> 0:27:44.080
<v Speaker 1>miles from our Sun, So they have seven planets tucked

0:27:44.080 --> 0:27:47.840
<v Speaker 1>in like around the distance that Mercury is. Wow, just

0:27:47.920 --> 0:27:51.000
<v Speaker 1>spinning around like like crazy. Yeah, I'm just spinning around

0:27:51.040 --> 0:27:53.920
<v Speaker 1>like crazy. So most of the solar systems we've seen

0:27:54.160 --> 0:27:57.400
<v Speaker 1>have more planets close to the Sun than ours. Now,

0:27:57.760 --> 0:27:59.840
<v Speaker 1>this is hard to know. It might be that there's

0:27:59.840 --> 0:28:02.960
<v Speaker 1>a bias here because it's harder to see planets that

0:28:03.000 --> 0:28:06.399
<v Speaker 1>are far from the Sun because the way we observe them. Remember,

0:28:06.400 --> 0:28:08.880
<v Speaker 1>as we see planets like passing in front of the Sun,

0:28:09.200 --> 0:28:10.880
<v Speaker 1>and if a planet is going around the Sun every

0:28:11.080 --> 0:28:13.320
<v Speaker 1>hundred years, it just doesn't pass in front of the

0:28:13.359 --> 0:28:16.040
<v Speaker 1>Sun is often, so it's easier for us to see

0:28:16.080 --> 0:28:18.960
<v Speaker 1>planets that are close to their Sun. So it might

0:28:19.000 --> 0:28:21.240
<v Speaker 1>be that there's a bias that we're finding the weird

0:28:21.280 --> 0:28:23.760
<v Speaker 1>ones first. But they don't think so. They think they've

0:28:23.800 --> 0:28:26.120
<v Speaker 1>accounted for that effect and they think it's still real

0:28:26.240 --> 0:28:28.600
<v Speaker 1>that the average solar system out there has more planets

0:28:28.600 --> 0:28:31.920
<v Speaker 1>close to the Sun than ours. Interesting, so the average

0:28:32.240 --> 0:28:36.080
<v Speaker 1>solar system out there is busier, yeah, especially close in

0:28:36.400 --> 0:28:39.520
<v Speaker 1>like more I guess, more concentrated. It's like a traffic

0:28:39.560 --> 0:28:47.320
<v Speaker 1>jam every day, all day for the for for eternity literally. Yeah.

0:28:47.320 --> 0:28:49.040
<v Speaker 1>But on the other hand, it means it's not as

0:28:49.080 --> 0:28:51.680
<v Speaker 1>hard to get from planet to planet, like your neighboring

0:28:51.680 --> 0:28:53.720
<v Speaker 1>planet is more like a neighbor, you know, you could

0:28:53.760 --> 0:28:56.440
<v Speaker 1>jump from planet to planet. Wouldn't take hundreds of days

0:28:56.480 --> 0:28:58.480
<v Speaker 1>like it would take for us to get from Earth

0:28:58.520 --> 0:29:00.120
<v Speaker 1>to Mars. You could get to the next planet it

0:29:00.160 --> 0:29:03.040
<v Speaker 1>in you know, just a few days. Right, and maybe

0:29:03.080 --> 0:29:06.120
<v Speaker 1>even more dangerous to write, because all those planets that

0:29:06.160 --> 0:29:10.040
<v Speaker 1>close together, they some of them could crash into each other, right, yeah,

0:29:10.120 --> 0:29:12.720
<v Speaker 1>and they can also affect each other's orbits. Right, planets

0:29:12.720 --> 0:29:15.360
<v Speaker 1>are big, and remember these planets are not tiny things,

0:29:15.920 --> 0:29:18.240
<v Speaker 1>and so they can tweak each other's orbits. Theres lots

0:29:18.280 --> 0:29:22.400
<v Speaker 1>more weird gravitational interactions, and we've also seen that we've

0:29:22.400 --> 0:29:25.480
<v Speaker 1>seen that a lot of these solar systems have weird orbits.

0:29:25.520 --> 0:29:28.320
<v Speaker 1>Like in our Solar system, things are very neatly laid out,

0:29:28.680 --> 0:29:31.800
<v Speaker 1>like the planets are sort of equally spaced, and everything

0:29:31.880 --> 0:29:34.920
<v Speaker 1>is separated, and everything is mostly flat in a single

0:29:34.960 --> 0:29:39.120
<v Speaker 1>plane and pretty circular, though not completely. But other Solar

0:29:39.160 --> 0:29:42.120
<v Speaker 1>systems the orbits were seeing are really eccentric. They are

0:29:42.200 --> 0:29:45.280
<v Speaker 1>much less circular, some of them, Like there's one for example,

0:29:45.280 --> 0:29:48.000
<v Speaker 1>I looked up and it goes from being just a

0:29:48.040 --> 0:29:50.560
<v Speaker 1>few million miles of its from its star on one

0:29:50.560 --> 0:29:53.760
<v Speaker 1>side to two hundred million miles on the other, so

0:29:53.920 --> 0:29:57.200
<v Speaker 1>like it's super close and then whizzes out really far away, right,

0:29:57.240 --> 0:30:00.920
<v Speaker 1>Because orbits can be not just circular or oval shaped,

0:30:00.920 --> 0:30:03.600
<v Speaker 1>they can also be kind of off center from the Sun,

0:30:03.840 --> 0:30:06.640
<v Speaker 1>kind of like comets have these weird elliptical orbits that

0:30:06.640 --> 0:30:08.760
<v Speaker 1>are like go really far out and then come back

0:30:08.760 --> 0:30:11.640
<v Speaker 1>in really close, right. Yeah, And commets don't have to

0:30:11.640 --> 0:30:13.880
<v Speaker 1>be sort of on the plane of the planets. And

0:30:13.920 --> 0:30:16.160
<v Speaker 1>what we're seeing is that other solar systems don't always

0:30:16.200 --> 0:30:18.600
<v Speaker 1>have the same orderly plane, that the planets are all

0:30:18.680 --> 0:30:21.360
<v Speaker 1>all on different planes, and we don't know what that means.

0:30:21.400 --> 0:30:23.440
<v Speaker 1>We don't know, like is that typical and our solar

0:30:23.440 --> 0:30:27.000
<v Speaker 1>system is just kind of weirdly randomly well ordered, or

0:30:27.120 --> 0:30:29.240
<v Speaker 1>maybe something happened in those solar systems there were some

0:30:29.280 --> 0:30:31.680
<v Speaker 1>collisions because everything was so crowded in and they got

0:30:31.800 --> 0:30:34.520
<v Speaker 1>tugged and thrown off into weird orbits. We just don't know.

0:30:34.680 --> 0:30:37.600
<v Speaker 1>I feel like we're getting more and more into the

0:30:37.680 --> 0:30:41.360
<v Speaker 1>idea that maybe our solar system is really weird. It's

0:30:41.360 --> 0:30:43.520
<v Speaker 1>like we have a weird Sun and a weird Earth,

0:30:43.600 --> 0:30:46.960
<v Speaker 1>and a weird, weird arrangement of planets and a weird orbit.

0:30:47.600 --> 0:30:50.240
<v Speaker 1>It's like it's just right. Yeah, And we're like that

0:30:50.320 --> 0:30:51.880
<v Speaker 1>kid that went to school for the first time and

0:30:51.880 --> 0:30:55.000
<v Speaker 1>discovered that his family is really, really weird. Nobody else

0:30:55.040 --> 0:30:58.160
<v Speaker 1>eats peanut butter pickle sandwiches for lunch and dresses in

0:30:58.240 --> 0:31:00.680
<v Speaker 1>that weird way or whatever. And the other thing that

0:31:00.840 --> 0:31:03.800
<v Speaker 1>I found really fascinating is that, you know, in our

0:31:03.800 --> 0:31:06.120
<v Speaker 1>Solar system we have all the gas giants on the outside.

0:31:06.200 --> 0:31:08.400
<v Speaker 1>We thought we had an explanation for that, that the

0:31:08.440 --> 0:31:10.920
<v Speaker 1>gas was blown out by the solar wind. But in

0:31:11.000 --> 0:31:14.320
<v Speaker 1>other solar systems we find these planets we call hot jupiters,

0:31:14.760 --> 0:31:18.360
<v Speaker 1>big gas giants that are close to their stars, close

0:31:18.480 --> 0:31:23.080
<v Speaker 1>enough to be hot. Right, they're trending, that's right, exactly,

0:31:23.240 --> 0:31:26.280
<v Speaker 1>they're viral jupiters. No. But for example, there's a system

0:31:26.720 --> 0:31:28.760
<v Speaker 1>um I won't pronounce the name because it's just letters

0:31:28.760 --> 0:31:31.720
<v Speaker 1>and numbers, but there's a Jupiter sized planet that's so

0:31:31.760 --> 0:31:35.400
<v Speaker 1>close to its star at orbits every two days. What

0:31:35.600 --> 0:31:38.680
<v Speaker 1>it's whipping around the Sun every two days. Yeah, but

0:31:38.720 --> 0:31:41.600
<v Speaker 1>it's the size of Jupiter, and so people wonder, like,

0:31:41.680 --> 0:31:44.720
<v Speaker 1>how did this planet form? There's not enough gas in

0:31:44.760 --> 0:31:47.320
<v Speaker 1>our understanding in the center of the Solar system, to

0:31:47.440 --> 0:31:50.800
<v Speaker 1>form a gas giant. Right, the gas either fell into

0:31:50.800 --> 0:31:53.520
<v Speaker 1>the Sun to form the star or got blown out

0:31:53.640 --> 0:31:56.280
<v Speaker 1>by that star into the outer reaches of those solar systems. So,

0:31:56.480 --> 0:31:59.160
<v Speaker 1>how do you make a hot jupiter if it's just

0:31:59.200 --> 0:32:01.240
<v Speaker 1>a cloud of as when in it just kind of

0:32:01.480 --> 0:32:03.840
<v Speaker 1>you know, whipping around that fast wheed it just kind

0:32:03.840 --> 0:32:08.680
<v Speaker 1>of break apart or dissolver smear. But no, it's somehow

0:32:08.720 --> 0:32:10.800
<v Speaker 1>it's spinning around every two days. Yeah, and maybe it

0:32:10.800 --> 0:32:13.400
<v Speaker 1>has a really strong magnetic field which helps protected from

0:32:13.440 --> 0:32:16.320
<v Speaker 1>the solar radiation and the solar wind from blowing it apart.

0:32:16.680 --> 0:32:18.680
<v Speaker 1>We don't know. And one idea is that maybe it

0:32:18.760 --> 0:32:21.200
<v Speaker 1>did form on the outer reaches of that solar system,

0:32:21.320 --> 0:32:24.200
<v Speaker 1>but then sort of moved up, like bumped the other

0:32:24.240 --> 0:32:26.400
<v Speaker 1>planets out of the way to get closer to the Sun.

0:32:26.960 --> 0:32:31.000
<v Speaker 1>This could happen, right, Planets can change orders. Wow, So

0:32:31.040 --> 0:32:34.560
<v Speaker 1>you're basically saying that like our nice orderly solar system

0:32:34.600 --> 0:32:37.800
<v Speaker 1>with the rocky planets first and our gas giants out there,

0:32:38.000 --> 0:32:41.920
<v Speaker 1>is maybe not even typical either, Like that sort of arrangement.

0:32:41.960 --> 0:32:44.440
<v Speaker 1>You can have gas giants close to the Sun and

0:32:44.480 --> 0:32:48.160
<v Speaker 1>you could probably have rocky planets out there. Yeah, we've

0:32:48.160 --> 0:32:51.520
<v Speaker 1>seen hot jupiters. We've seen solar systems with gas giants

0:32:51.520 --> 0:32:53.760
<v Speaker 1>close to the Sun, and in some of these it

0:32:53.800 --> 0:32:57.080
<v Speaker 1>does look like maybe they did migrate in from the outside,

0:32:57.160 --> 0:32:59.920
<v Speaker 1>because we don't see like a lot of other inner

0:33:00.040 --> 0:33:03.600
<v Speaker 1>planets nearby. What would happen if Jupiter, for example, moved

0:33:03.600 --> 0:33:06.400
<v Speaker 1>in and tried to take over Venus orbit, well, Earth

0:33:06.480 --> 0:33:09.479
<v Speaker 1>and Mars and Venus and Mercury, we probably get tossed

0:33:09.480 --> 0:33:12.240
<v Speaker 1>out of the Solar system by Jupiter's gravity, And that's

0:33:12.280 --> 0:33:14.440
<v Speaker 1>what we see in these solar systems with a hot Jupiter.

0:33:14.480 --> 0:33:16.800
<v Speaker 1>We don't see a lot of other inner planets, so

0:33:16.840 --> 0:33:19.440
<v Speaker 1>we think maybe, you know, the big gas giant bully

0:33:19.560 --> 0:33:22.280
<v Speaker 1>came in and cleared out the playground, all right. So yeah,

0:33:22.320 --> 0:33:24.400
<v Speaker 1>there's a lot of ways in which our Solar system

0:33:24.680 --> 0:33:26.920
<v Speaker 1>is weird, right in terms of the Sun, the Earth,

0:33:27.000 --> 0:33:30.000
<v Speaker 1>and the gas giants. And so now let's talk about

0:33:30.600 --> 0:33:33.640
<v Speaker 1>UM some of the ideas that scientists have about whether

0:33:33.800 --> 0:33:37.920
<v Speaker 1>solar systems all formed the same way, or whether are

0:33:38.040 --> 0:33:42.520
<v Speaker 1>somehow made it into this special configuration for a special reason. First,

0:33:42.560 --> 0:33:57.440
<v Speaker 1>let's take a quick break a right, So let's talk

0:33:57.440 --> 0:34:00.880
<v Speaker 1>about um. What idea scientists have to explain all these

0:34:01.120 --> 0:34:04.760
<v Speaker 1>weird types of solar systems, like why is ours different?

0:34:05.000 --> 0:34:07.600
<v Speaker 1>How do other system solar systems form? What's the sort

0:34:07.600 --> 0:34:12.399
<v Speaker 1>of prevailing theory about how solar systems are made. Yeah,

0:34:12.480 --> 0:34:14.840
<v Speaker 1>So the theory we had for a long time before

0:34:14.880 --> 0:34:16.840
<v Speaker 1>we saw all these other solar systems, we call that

0:34:16.880 --> 0:34:20.319
<v Speaker 1>the core accretion theory, and it basically says, you start

0:34:20.360 --> 0:34:22.799
<v Speaker 1>from a big rotating blob of gas and dust and

0:34:22.840 --> 0:34:25.840
<v Speaker 1>some ice, and the star forms and the rest of

0:34:25.840 --> 0:34:28.640
<v Speaker 1>it you get you accrete the cores of these planets.

0:34:28.640 --> 0:34:31.400
<v Speaker 1>That just means that like the biggest rock that happens

0:34:31.440 --> 0:34:33.920
<v Speaker 1>to be out there gathers up other rocks around it,

0:34:34.160 --> 0:34:36.440
<v Speaker 1>and they form and they gather more stuff until you

0:34:36.480 --> 0:34:39.120
<v Speaker 1>get stuff big enough stuff to make a planet. And

0:34:39.200 --> 0:34:41.440
<v Speaker 1>that's how we explain how you get Jupiter. For example.

0:34:41.600 --> 0:34:43.759
<v Speaker 1>You're gathering together a bunch of rocks and ice and

0:34:43.840 --> 0:34:46.239
<v Speaker 1>that sucks up all the gas. Also, stuff was just

0:34:46.239 --> 0:34:48.960
<v Speaker 1>floating around and then they just because of gravity, just

0:34:49.120 --> 0:34:53.279
<v Speaker 1>formed into planets like condensation almost. And one the thing

0:34:53.320 --> 0:34:55.360
<v Speaker 1>that people have always wondered about that theory that they

0:34:55.360 --> 0:34:57.720
<v Speaker 1>didn't really like is that it takes a long time.

0:34:58.200 --> 0:35:00.880
<v Speaker 1>I mean gravity is really weak, and we're talking about

0:35:00.880 --> 0:35:03.600
<v Speaker 1>when you start, you're tugging on really small bits, you know,

0:35:04.040 --> 0:35:06.960
<v Speaker 1>bits of gas and bits of dust and tiny little pebbles.

0:35:07.160 --> 0:35:09.240
<v Speaker 1>So it's gonna take a long time to make Jupiter

0:35:09.560 --> 0:35:12.560
<v Speaker 1>out of bits of sand, right, And they worry that

0:35:12.719 --> 0:35:14.880
<v Speaker 1>it takes so long to form the core on this,

0:35:15.280 --> 0:35:17.520
<v Speaker 1>you know, the dust and the ice, that by then

0:35:17.600 --> 0:35:19.680
<v Speaker 1>all the gas will just have floated away or been

0:35:19.719 --> 0:35:22.200
<v Speaker 1>blown away by the solar wind. So there's always been

0:35:22.239 --> 0:35:24.600
<v Speaker 1>this bit of tension like how do you get these

0:35:24.600 --> 0:35:27.919
<v Speaker 1>planets to form soon enough that they can gather any

0:35:27.920 --> 0:35:31.240
<v Speaker 1>of that less leftover gas. So that's the old idea

0:35:31.239 --> 0:35:33.000
<v Speaker 1>and the sort of the concerns people have with it.

0:35:33.239 --> 0:35:36.080
<v Speaker 1>And now that we've seen these other solar systems, they're wondering, well,

0:35:36.120 --> 0:35:38.440
<v Speaker 1>maybe we need new ideas. And so there is a

0:35:38.480 --> 0:35:41.239
<v Speaker 1>new idea on the block. Oh I see, because this

0:35:41.280 --> 0:35:46.000
<v Speaker 1>idea that solar systems kind of form slowly might explain

0:35:46.320 --> 0:35:49.760
<v Speaker 1>may not even explain ours. But looking at other solar systems,

0:35:49.760 --> 0:35:51.440
<v Speaker 1>we're like, oh, whoa, whoa, we don't really have a

0:35:51.520 --> 0:35:53.799
<v Speaker 1>good idea about how solar systems form, because whatever we

0:35:53.840 --> 0:35:55.759
<v Speaker 1>come up with has to work for all of these

0:35:55.800 --> 0:35:59.239
<v Speaker 1>other solar systems. Yeah, and you know you need inspiration

0:35:59.280 --> 0:36:02.360
<v Speaker 1>in science, and this old idea was inspired by this

0:36:02.400 --> 0:36:05.040
<v Speaker 1>one example. Now that we've seen these other examples and

0:36:05.080 --> 0:36:07.680
<v Speaker 1>sort of stretches us in the right way to come

0:36:07.760 --> 0:36:10.320
<v Speaker 1>up with new ideas for how you could explain these examples.

0:36:10.320 --> 0:36:12.440
<v Speaker 1>And so one of these new ideas is called the

0:36:12.520 --> 0:36:16.040
<v Speaker 1>disc instability model. That idea is basically that when the

0:36:16.040 --> 0:36:18.439
<v Speaker 1>Solar system formed, you have this disc, but it wasn't

0:36:18.440 --> 0:36:21.920
<v Speaker 1>like a nice, calm, smooth disc that was slowly formed

0:36:22.160 --> 0:36:24.279
<v Speaker 1>from the rotating blob, but that there was still a

0:36:24.280 --> 0:36:26.040
<v Speaker 1>lot of sort of stuff going on. There's a lot

0:36:26.080 --> 0:36:30.040
<v Speaker 1>of action there, and that these instabilities is action inside

0:36:30.080 --> 0:36:32.440
<v Speaker 1>the disc might be a way to get these planets

0:36:32.480 --> 0:36:35.480
<v Speaker 1>to form sooner and also for them to form closer

0:36:35.520 --> 0:36:38.120
<v Speaker 1>to their stars. But what do you mean disc instability?

0:36:38.200 --> 0:36:42.480
<v Speaker 1>Like there's something extra special going on that makes Jupiters

0:36:42.520 --> 0:36:45.360
<v Speaker 1>and weird planets like that. Yeah. If the model you

0:36:45.440 --> 0:36:47.320
<v Speaker 1>have in your head is sort of like a giant,

0:36:47.440 --> 0:36:51.200
<v Speaker 1>stately cloud which is slowly rotating and then gradually gathering

0:36:51.200 --> 0:36:54.439
<v Speaker 1>together into a flat disc, that's the core creation model.

0:36:54.480 --> 0:36:57.120
<v Speaker 1>It assumes that everything is sort of very smoothly flowing.

0:36:57.440 --> 0:36:59.279
<v Speaker 1>But if instead it's a bit more turbulent, if this

0:36:59.320 --> 0:37:01.200
<v Speaker 1>is a little bit more chaos in there, you know,

0:37:01.200 --> 0:37:04.200
<v Speaker 1>it's more like a storm and it's being squeezed by

0:37:04.239 --> 0:37:06.200
<v Speaker 1>gravity a little bit, but there's still sort of stuff

0:37:06.239 --> 0:37:08.960
<v Speaker 1>going on inside of it. That's stuff that energy can

0:37:08.960 --> 0:37:11.919
<v Speaker 1>be used to sort of collide stuff together and make

0:37:12.120 --> 0:37:16.080
<v Speaker 1>and from those instabilities form gravitational course that can that

0:37:16.120 --> 0:37:19.480
<v Speaker 1>can gather stuff more rapidly. Oh, and that would explain

0:37:19.520 --> 0:37:23.560
<v Speaker 1>our solar systems or sort of all solar systems. Well,

0:37:23.560 --> 0:37:26.360
<v Speaker 1>it's not a very popular model yet and it's very fresh,

0:37:26.640 --> 0:37:29.600
<v Speaker 1>but it might explain how our solar system got gas

0:37:29.640 --> 0:37:33.080
<v Speaker 1>giants because it unless you form planets more rapidly. And

0:37:33.120 --> 0:37:35.359
<v Speaker 1>it also might explain how you were able to form

0:37:35.400 --> 0:37:38.399
<v Speaker 1>gas giants close to the star, because you could form

0:37:38.440 --> 0:37:41.000
<v Speaker 1>them quickly enough that you could form them before all

0:37:41.040 --> 0:37:44.120
<v Speaker 1>the gas was blown away by the Sun. But it's

0:37:44.160 --> 0:37:46.359
<v Speaker 1>still it's a very fresh model and it hasn't gained

0:37:46.400 --> 0:37:49.040
<v Speaker 1>wide acceptance yet, so it could be like maybe it's

0:37:49.160 --> 0:37:52.080
<v Speaker 1>just like the way solar systems form, is it just

0:37:52.120 --> 0:37:55.640
<v Speaker 1>this very chaotic process and sometimes you get solar systems

0:37:55.680 --> 0:37:59.680
<v Speaker 1>like ours and sometimes you get totally different solar systems. Yeah, precisely.

0:38:00.200 --> 0:38:03.640
<v Speaker 1>And the other idea is about planetary migration. People think

0:38:03.920 --> 0:38:06.520
<v Speaker 1>that maybe it's not unusual for planets to sort of

0:38:06.560 --> 0:38:09.440
<v Speaker 1>tug each other out of orbit and switch spots, you know,

0:38:09.440 --> 0:38:12.880
<v Speaker 1>to take each other's seats. And there's even the idea

0:38:12.920 --> 0:38:15.800
<v Speaker 1>that it could have happened in our Solar system. People

0:38:15.840 --> 0:38:18.400
<v Speaker 1>think that maybe. Yeah, people think that maybe Saturday and

0:38:18.480 --> 0:38:22.120
<v Speaker 1>Jupiter used to have an opposite order, and there was

0:38:22.160 --> 0:38:25.319
<v Speaker 1>another planet out there, a big ice giant, and the

0:38:25.320 --> 0:38:27.680
<v Speaker 1>three of them are sort of in this chaotic bumping

0:38:27.680 --> 0:38:30.680
<v Speaker 1>of each other, and they switched Saturn and Jupiter switched

0:38:30.680 --> 0:38:32.680
<v Speaker 1>and tossed the other planet sort of out to the

0:38:32.680 --> 0:38:34.920
<v Speaker 1>far reaches of the Solar System. And we just did

0:38:34.960 --> 0:38:37.719
<v Speaker 1>a whole episode about planet nine that could explain like

0:38:37.760 --> 0:38:40.359
<v Speaker 1>why planet nine is so far out there. So, yeah,

0:38:40.440 --> 0:38:44.240
<v Speaker 1>you're saying that even if you you form a solar system,

0:38:44.520 --> 0:38:47.120
<v Speaker 1>it can still change. You can still you can still

0:38:47.120 --> 0:38:49.560
<v Speaker 1>switch it around and change the structure of it, even

0:38:49.560 --> 0:38:52.719
<v Speaker 1>when it's sort of stable and floating along. Yeah, and

0:38:52.760 --> 0:38:55.680
<v Speaker 1>that means something interesting for our Solar system. It could

0:38:55.719 --> 0:38:57.520
<v Speaker 1>be in the future if you went away on a

0:38:57.560 --> 0:39:00.600
<v Speaker 1>spaceship for a billion years and came back, that you

0:39:00.600 --> 0:39:03.360
<v Speaker 1>could come back and find the Solar system looking quite different. Right,

0:39:03.440 --> 0:39:06.360
<v Speaker 1>Jupiter might have moved in on Mercury's territory and become

0:39:06.400 --> 0:39:08.920
<v Speaker 1>hot and tossed out all the other planets. We just

0:39:08.960 --> 0:39:11.360
<v Speaker 1>don't know. We don't know if this configuration is stable

0:39:11.680 --> 0:39:14.719
<v Speaker 1>on billions year time scales. That would be pretty cool

0:39:14.760 --> 0:39:16.520
<v Speaker 1>if you left for a few million years and then

0:39:16.560 --> 0:39:19.680
<v Speaker 1>came back and you're like, what happened to my house? Remodeled?

0:39:19.840 --> 0:39:21.839
<v Speaker 1>Just like everybody who goes away to college and comes

0:39:21.880 --> 0:39:25.560
<v Speaker 1>back after Thanksgiving and like, hey, everything looks different. You

0:39:25.640 --> 0:39:29.839
<v Speaker 1>turned my plan into a workout room. All right, Well,

0:39:29.880 --> 0:39:34.880
<v Speaker 1>it sounds like our solar system is not. It is weird,

0:39:35.160 --> 0:39:37.239
<v Speaker 1>that's the answer to the Today's question. It is kind

0:39:37.280 --> 0:39:40.360
<v Speaker 1>of weird in that you know, our son is single

0:39:40.600 --> 0:39:45.520
<v Speaker 1>and hot and young, and we apparently live in a

0:39:45.600 --> 0:39:49.560
<v Speaker 1>mini Earth, are not super Earth. And it's also weird

0:39:49.640 --> 0:39:51.719
<v Speaker 1>that we have all all of our gas giants out

0:39:51.760 --> 0:39:54.799
<v Speaker 1>there floating out there far away from the Sun. And

0:39:54.840 --> 0:39:57.160
<v Speaker 1>so it is because it sounds like it is sort

0:39:57.160 --> 0:39:59.080
<v Speaker 1>of a special case or solar system, like if we

0:39:59.120 --> 0:40:02.400
<v Speaker 1>go to other solar systems. We should be prepared to

0:40:02.800 --> 0:40:05.400
<v Speaker 1>see things that are very different. Yeah, and I'm so

0:40:05.480 --> 0:40:07.320
<v Speaker 1>glad that that's the answer. It would be so boring

0:40:07.360 --> 0:40:10.200
<v Speaker 1>if we discovered every solar system looked like ours, and

0:40:10.239 --> 0:40:12.160
<v Speaker 1>that the idea we have for how the solar system

0:40:12.239 --> 0:40:15.440
<v Speaker 1>formed was pretty much being on. It's exactly what you

0:40:15.480 --> 0:40:17.480
<v Speaker 1>hope for in science, that once you open up new

0:40:17.480 --> 0:40:20.319
<v Speaker 1>eyeballs or build bigger eyeballs, that you see surprises, that

0:40:20.360 --> 0:40:23.040
<v Speaker 1>you learn things, the things that shake up your ideas

0:40:23.120 --> 0:40:25.919
<v Speaker 1>for how our home and our solar system have been made.

0:40:26.360 --> 0:40:28.080
<v Speaker 1>And maybe it gives us a bit of a special

0:40:28.080 --> 0:40:31.480
<v Speaker 1>appreciation for this particular little cute many Earth we find

0:40:31.480 --> 0:40:34.120
<v Speaker 1>ourselves on. Yeah, maybe you'll go to another solar system

0:40:34.200 --> 0:40:36.840
<v Speaker 1>and everybody will have two pH d s. Should be

0:40:36.920 --> 0:40:42.280
<v Speaker 1>like what the Bruce Banner solar system? All right, Well,

0:40:42.600 --> 0:40:44.480
<v Speaker 1>we hope you the next time you think about your

0:40:44.600 --> 0:40:47.520
<v Speaker 1>planet or the solar system we're in, you sort of

0:40:47.560 --> 0:40:50.120
<v Speaker 1>think about how special it is and how weird it is,

0:40:50.160 --> 0:40:53.120
<v Speaker 1>and how unique it is out there in the universe.

0:40:53.480 --> 0:40:55.759
<v Speaker 1>And in five years or twenty years or fifty years,

0:40:55.760 --> 0:40:59.000
<v Speaker 1>we could find even more weird, surprising solar systems out

0:40:59.000 --> 0:41:01.960
<v Speaker 1>there that challenge our very concept of what the universe

0:41:02.000 --> 0:41:05.360
<v Speaker 1>looks like. Yeah, so stay tuned and keep funding science.

0:41:05.600 --> 0:41:15.680
<v Speaker 1>Thanks for tuning in, See you next time. Before you

0:41:15.760 --> 0:41:18.600
<v Speaker 1>still have a question after listening to all these explanations,

0:41:18.719 --> 0:41:21.360
<v Speaker 1>please drop us the line. We'd love to hear from you.

0:41:21.640 --> 0:41:24.520
<v Speaker 1>You can find us on Facebook, Twitter, and Instagram at

0:41:24.800 --> 0:41:27.960
<v Speaker 1>Daniel and Jorge That's one word, or email us at

0:41:28.239 --> 0:41:31.880
<v Speaker 1>Feedback at Daniel and Jorge dot com. Thanks for listening

0:41:31.920 --> 0:41:34.680
<v Speaker 1>and remember that Daniel and Jorge Explain the Universe is

0:41:34.719 --> 0:41:38.200
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