WEBVTT - Did Jupiter once have a different orbit?

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<v Speaker 1>Hey, Kelly, how do you feel about moving? It always

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<v Speaker 1>seems like it's going to be exciting, but it's always

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<v Speaker 1>a drag. No. Right, It's like there's always one more

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<v Speaker 1>box of stuff, and by mathematical induction, that means we

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<v Speaker 1>all have infinite totally checks out. I mean I have

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<v Speaker 1>like infinite back pain from my last move. Sometimes I

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<v Speaker 1>wish I had a mobile home so that I wouldn't

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<v Speaker 1>have to pack everything up every time. That is a

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<v Speaker 1>genius solution. I mean, you move more stuff, but you

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<v Speaker 1>do less work because you take your whole house with

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<v Speaker 1>you exactly. I wonder if it's scales. I'm thinking like

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<v Speaker 1>mobile neighborhoods, mobile cities, maybe like mobile planets. Earth is

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<v Speaker 1>just one big mobile home. Man, I didn't realize we

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<v Speaker 1>lived in a cosmic trailer park. I'm Daniel, I'm a

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<v Speaker 1>particle physicist, and I once moved across the Atlantic eleven

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<v Speaker 1>times in four years. Seriously, seriously. This was when I

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<v Speaker 1>was a junior professor and just getting started at the

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<v Speaker 1>Large Hadron Collider and teaching on the West coast of

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<v Speaker 1>the United States. So we actually had a house in

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<v Speaker 1>France and a house in California, and we had to

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<v Speaker 1>go back and forth and back and forth, and back

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<v Speaker 1>and forth and back and forth and back and forth.

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<v Speaker 1>It almost drove my family crazy. Oh my gosh, did

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<v Speaker 1>you have kids at that point? We had two young children,

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<v Speaker 1>one of the whom was born in Switzerland. Oh my goodness.

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<v Speaker 1>I know. It's amazing I'm not divorced. It is. It is.

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<v Speaker 1>I shouldn't have said it is so quickly, but well,

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<v Speaker 1>I'm Kelly Wiener Smith and I'm a parasitologist, and it's

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<v Speaker 1>amazing that I'm not divorced. Also because I moved my

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<v Speaker 1>husband four times during my PhD to different states. But

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<v Speaker 1>you know, I used to think that was bad. And

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<v Speaker 1>now I'm going to go downstairs and tell Zack later

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<v Speaker 1>how easy he has it. So thank you for that.

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<v Speaker 1>That's good. That's my goal is to make other marriages

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<v Speaker 1>look good. We appreciate it. Well. Welcome to the podcast

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<v Speaker 1>Daniel and Jorge Explain the Universe, in which we talk

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<v Speaker 1>about all the crazy and amazing things that we find

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<v Speaker 1>out there in the universe, moving here and there, taking

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<v Speaker 1>our brains from the tiniest little particles down to the

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<v Speaker 1>quantum realm to the vast planets of the outer Solar

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<v Speaker 1>system and all the way to super clusters. Our goal

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<v Speaker 1>is to embrace everything we know and that we don't

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<v Speaker 1>know and explain all of it to you. And as

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<v Speaker 1>you might have guests today on the program, Jorge is

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<v Speaker 1>not here, so we have our fabulous guest host, Kelly

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<v Speaker 1>Weener Smith joining us to talk about all these things

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<v Speaker 1>and ask good questions. Hey, Daniel, I'm excited to be back.

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<v Speaker 1>I had fun lost time. Awesome, great, well, thanks very

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<v Speaker 1>much for joining us. So we started off joking about

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<v Speaker 1>moving houses and moving planets. But this is something I

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<v Speaker 1>think is actually really interesting, is thinking about how the

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<v Speaker 1>planets in our solar system got where they are and

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<v Speaker 1>whether or not they have ever moved. I personally love

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<v Speaker 1>this question because it's one of those questions that, like

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<v Speaker 1>the fact that we have anything that even vaguely resembles

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<v Speaker 1>an answer, makes me sort of proud to be a human. Like,

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<v Speaker 1>how can we even think about these sorts of questions

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<v Speaker 1>and collect data to answer these questions. It just seems

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<v Speaker 1>so mind blowing to begin with the fact that we

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<v Speaker 1>have any answers, even preliminary answers, blows my mind. Well,

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<v Speaker 1>I think it's super fascinating that we even know to

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<v Speaker 1>ask these questions, right, Like, you look at the Solar

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<v Speaker 1>system and we have the planets, and they don't seem

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<v Speaker 1>to be changing from year to year. We have thousands

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<v Speaker 1>of years of astronomical records and so it seems sort

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<v Speaker 1>of stable. So it's sort of absurd even to ask, like,

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<v Speaker 1>could the planets have ever been in another configuration? Could

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<v Speaker 1>the solar system have looked different? It's like very natural

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<v Speaker 1>to think, oh, things are going around the Sun. They've

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<v Speaker 1>been going around the Sun. Of course they were always

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<v Speaker 1>in the same orientation. But something that's happened over the

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<v Speaker 1>last just couple of decades is that we've had a

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<v Speaker 1>chance to glimpse other solar systems. For thousands of years,

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<v Speaker 1>we've only ever seen ours. We had like one example.

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<v Speaker 1>Now we're seeing lots and lots of other solar systems,

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<v Speaker 1>and this gives us a clue that solar systems can

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<v Speaker 1>look different and that there might be a lot of activity,

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<v Speaker 1>that they're actually quite volatile. That is super exciting. So

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<v Speaker 1>for our sample size for these like how many solar

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<v Speaker 1>systems can we see in enough detail where we can

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<v Speaker 1>like count all of the planets and get a bit

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<v Speaker 1>of a sense for what those planets are, like, are

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<v Speaker 1>we talking hundreds, thousands, millions? How big is our data

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<v Speaker 1>set here? It's exciting because it's growing so rapidly, Like

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<v Speaker 1>the first exoplanets were discovered just a few decades ago,

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<v Speaker 1>and now we have thousands, not yet millions. Someday astronomers

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<v Speaker 1>will get to play with the datas that have millions

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<v Speaker 1>of solar systems and ask really detailed questions. But we

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<v Speaker 1>have thousands of solar systems that we can look at

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<v Speaker 1>and we see weird stuff in those solar systems that

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<v Speaker 1>we don't see in our solar system and that makes

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<v Speaker 1>us wonder, like, wait a second, are those solar systems weird?

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<v Speaker 1>Or is our Solar system weird? I need to know

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<v Speaker 1>the answer, And so today on the podcast will be

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<v Speaker 1>asking the question has our Solar system look different? In particular,

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<v Speaker 1>did Jupiter ones have a different orbit? And that's a

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<v Speaker 1>pretty huge question, right because Jupiter is like the biggest

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<v Speaker 1>planet out there, so where it goes has a big impact.

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<v Speaker 1>From one point of view, you could imagine it's basically

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<v Speaker 1>the only planet other than the Sun. Jupiter has like

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<v Speaker 1>of all the mass in the Solar system. Everything else

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<v Speaker 1>is basically a detail compared to Jupiter. So yeah, it's

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<v Speaker 1>a big deal. If Jupiter had been in a different place,

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<v Speaker 1>everything would be different, and so as usual, I was

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<v Speaker 1>curious whether people had this in their minds, like, have

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<v Speaker 1>people imagine the possibility that Jupiter could be in a

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<v Speaker 1>different place? Is that something people have thought about, have

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<v Speaker 1>heard about? So I went out there to the wilds

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<v Speaker 1>of the Internet and I asked people, Hey, do you

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<v Speaker 1>know the answer to this tough physics question that astronomers

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<v Speaker 1>are struggling over. Use no preparation, no googling allowed, Just

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<v Speaker 1>tell me off the top of your head. Here's what

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<v Speaker 1>people had to say. I guess No, there were impacts

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<v Speaker 1>off I guess asteroids and or comets, and I may

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<v Speaker 1>be even bigger objects in the past. So I think

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<v Speaker 1>the orbit of Jupiter was a different one two beion

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<v Speaker 1>years ago. No, I think it was, but I think

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<v Speaker 1>it used to be a lot closer and then it

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<v Speaker 1>moved out through collisions and the collisions, I think Jupiter

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<v Speaker 1>used to be in a different orbit. I know Uranus

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<v Speaker 1>rotates about its access in a way that sideways compared

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<v Speaker 1>to the other planets. Well, I'm not sure if what

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<v Speaker 1>I think happened, is that Uranus and Jupiter collies at

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<v Speaker 1>some point. I suspect that Jupiter has been in its

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<v Speaker 1>current orbit for quite some time, speaking on you know,

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<v Speaker 1>the scale of the formation of our Solar system, but

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<v Speaker 1>I would not at all be surprised if it had

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<v Speaker 1>moved around somewhat during the early formation period of our

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<v Speaker 1>solar system. Would say, yes, well, nothing is permanent, so

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<v Speaker 1>I guess it's at the origin it was part of

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<v Speaker 1>the the Sun or giant cloud of gas. But to me, well,

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<v Speaker 1>it's quite stable orbits, and I don't see why each change,

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<v Speaker 1>except for minor changes such as a collision with that

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<v Speaker 1>other objects. But I would say yes, no, no, Um.

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<v Speaker 1>Jupiter at some point was sitting towards the Sun, but

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<v Speaker 1>it's kinda got locked in by Saturn, probably interaction with

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<v Speaker 1>settled um, something like that. I don't know, you caught me.

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<v Speaker 1>I'll guard here. I don't think that Jupiter has always

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<v Speaker 1>been in its current orbit. I think it formed much

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<v Speaker 1>closer to the Sun, and as it migrated out into

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<v Speaker 1>the Solar System, it cleared a lot of the debris

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<v Speaker 1>and comets and asteroids and dust and everything out of

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<v Speaker 1>its way um and made things a little bit more

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<v Speaker 1>stable here in the inner Solar system, so life could form.

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<v Speaker 1>But I don't think that it started out where it

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<v Speaker 1>currently is. Somebody say no, but I guess, being it's

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<v Speaker 1>so big, it could well have picked up a lot

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<v Speaker 1>of stuff through its time, and as it um, you know,

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<v Speaker 1>it picks up more stuff gets impacted, and I guess

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<v Speaker 1>it's gravitational forces would interact with other planets and stuff around,

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<v Speaker 1>so therefore it get knocked off and moved off its

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<v Speaker 1>little but quite regularly. Maybe, I think almost certainly no. UM.

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<v Speaker 1>I think the current model of how those those system

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<v Speaker 1>was formed UM actually relies on Jupiter migrating inward closer

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<v Speaker 1>to the Sun and then further away. I believe Jupiter

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<v Speaker 1>has moved from its original orbit. I think the original

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<v Speaker 1>orbit was closer to the Sun. All right, Wow, those

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<v Speaker 1>are some great answers from our listeners. When you heard

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<v Speaker 1>that this was even a question that people were thinking about,

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<v Speaker 1>did you have a like, oh my gosh moment or

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<v Speaker 1>did it just seem like an obvious question for you

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<v Speaker 1>to be asking. I had an oh my gosh moment

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<v Speaker 1>and a hope because I thought, oh, that would be

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<v Speaker 1>super cool if Jupiter wasn't always in its current orbit.

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<v Speaker 1>Because one of the fun things for me in science

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<v Speaker 1>is revealing surprises. Right If you ask a question and

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<v Speaker 1>then the answer is yeah, it's kind of boring Jupiter

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<v Speaker 1>has always been there. That's not nearly as fun as

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<v Speaker 1>Oh my gosh, it turns out there's a crazy history

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<v Speaker 1>here and we have revealed it. Like you were saying earlier,

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<v Speaker 1>it's incredible that we could, like by gathering small lose

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<v Speaker 1>left by these crazy cosmic events, actually reconstruct something that

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<v Speaker 1>happened billions of years ago. It's like solving a billion

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<v Speaker 1>year old murder mystery. As a biologist, every once in

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<v Speaker 1>a while we will have discussions about like what makes

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<v Speaker 1>humans different than other animals, And you know, clearly being

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<v Speaker 1>able to think about questions like this is one of

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<v Speaker 1>those things that like, certainly we're the only species who's

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<v Speaker 1>wondering that on our planet exactly. So it's super fun.

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<v Speaker 1>And I was really hoping that the answer would be

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<v Speaker 1>something crazy. So it's pretty interesting to learn about. And

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<v Speaker 1>I've also really been enjoying following this Excel planet discovery

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<v Speaker 1>seeing these other solar systems, these other like potential homes

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<v Speaker 1>for aliens where life could be really different because the

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<v Speaker 1>planets are so different from ours. You know, we're sort

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<v Speaker 1>of like trapped in this colloquial way of thinking that

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<v Speaker 1>our kinds of planets are the kinds of planets you have,

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<v Speaker 1>like small rocky planets and the inner Solar system and

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<v Speaker 1>big gas giants and the outside and now it's possible

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<v Speaker 1>to imagine other kinds of areas. So is our configuration

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<v Speaker 1>a typical configuration. It turns out it's not. When we

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<v Speaker 1>look at other solar systems, we see something really weird.

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<v Speaker 1>First of all, we see that most solar systems have

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<v Speaker 1>a lot more planets very close to their star, Like

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<v Speaker 1>between Mercury and the Sun there's basically nothing, But in

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<v Speaker 1>other solar systems there are lots of planets packed in there.

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<v Speaker 1>And in particular, we find these things called hot jupiters.

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<v Speaker 1>Not hot because they're like you know, big on Instagram

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<v Speaker 1>or they're really curvy, hot because they're really close to

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<v Speaker 1>the Sun. Like, we find these planets in other solar

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<v Speaker 1>systems that are really big, like Jupiter size and gas planets,

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<v Speaker 1>but they orbit the star in just like hours or days,

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<v Speaker 1>and like a fraction of the distance between the Sun

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<v Speaker 1>and mercury. So that's a really weird phenomenon to see.

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<v Speaker 1>Shouldn't they like suck each other into each other pretty quickly?

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<v Speaker 1>What's the good physics word for that? How do they

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<v Speaker 1>stay separated if they're both huge and attracting each other

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<v Speaker 1>and are so close now, suck each other in is

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<v Speaker 1>exactly they're all right physics word to use, And that's

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<v Speaker 1>exactly the question people are asking. They're like, hold on

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<v Speaker 1>a second, how do you get such a big planet

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<v Speaker 1>so close to the Sun? Can it last very long?

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<v Speaker 1>Are we seeing something just before it dies? Or can

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<v Speaker 1>that be a stable configuration? And the models suggests that

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<v Speaker 1>they can't have been born that close to the Sun

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<v Speaker 1>and they can't last there very long. And that's the

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<v Speaker 1>clue that got everybody talking and thinking about whether planets

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<v Speaker 1>are moving, because they suspect that these hot jupiters form

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<v Speaker 1>further out and then get sucked in, and so we're

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<v Speaker 1>witnessing sort of like the end of the life cycle

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<v Speaker 1>of these planets before they either get torn apart or

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<v Speaker 1>pulled in. And that's a clue that, like solar systems

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<v Speaker 1>are volatile, there is stuff going on. It's not just

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<v Speaker 1>everybody sedately driving in their lane for billions of years?

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<v Speaker 1>Is Jupiter going to get sucked into our Sun? Not

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<v Speaker 1>before the Sun explodes? Right? Are you worried about Jupiter?

0:12:50.640 --> 0:12:53.120
<v Speaker 1>Have you invested in real estate on Jupiter? Well, you know,

0:12:53.160 --> 0:12:55.679
<v Speaker 1>I was thinking about it. We've been reading about space settlements,

0:12:55.720 --> 0:12:58.120
<v Speaker 1>but no, obviously not nobody's gonna go live on Jupiter.

0:12:58.200 --> 0:13:00.600
<v Speaker 1>But maybe it's moons. I went to read I fantastic

0:13:00.640 --> 0:13:04.120
<v Speaker 1>series and science fiction novels about a civilization in the

0:13:04.200 --> 0:13:06.920
<v Speaker 1>upper clouds of Jupiter. I think it was called Bio

0:13:07.040 --> 0:13:10.240
<v Speaker 1>of a Space Tyrant Man. I loved those books when

0:13:10.240 --> 0:13:13.479
<v Speaker 1>I was a teenager. It was so like fantastically imagined.

0:13:13.800 --> 0:13:15.720
<v Speaker 1>So I hope that one day humans do get to

0:13:15.720 --> 0:13:17.040
<v Speaker 1>live on Jupiter, and I hope that we get to

0:13:17.080 --> 0:13:19.880
<v Speaker 1>keep Jupiter because I like it. I mean, Jupiter is pretty.

0:13:20.040 --> 0:13:22.679
<v Speaker 1>For all the press that like Mars gets recently, Jupiter

0:13:22.760 --> 0:13:25.199
<v Speaker 1>is a gorgeous planet. So maybe we should start by

0:13:25.240 --> 0:13:27.960
<v Speaker 1>thinking about our solar system and understanding of what we

0:13:28.040 --> 0:13:31.160
<v Speaker 1>know about Jupiter, like where it was made, how it

0:13:31.280 --> 0:13:33.600
<v Speaker 1>got formed, and that can give us a clue for

0:13:33.679 --> 0:13:37.040
<v Speaker 1>like why people think there might have been crazy stuff

0:13:37.080 --> 0:13:39.880
<v Speaker 1>going on in our solar system. At the very beginning

0:13:39.880 --> 0:13:42.600
<v Speaker 1>of time. Alright, so tell me about how Jupiter got

0:13:42.640 --> 0:13:44.800
<v Speaker 1>to be where it is. Yes, so we think Jupiter

0:13:44.880 --> 0:13:48.520
<v Speaker 1>is probably born out in the outer Solar system. There's

0:13:48.559 --> 0:13:51.240
<v Speaker 1>this point in the Solar system called the ice line,

0:13:51.800 --> 0:13:55.480
<v Speaker 1>where beyond that it's cold enough for ice to form

0:13:55.640 --> 0:13:58.320
<v Speaker 1>and to stay melted and basically be like a rock

0:13:58.559 --> 0:14:01.800
<v Speaker 1>that you can use and building planetary cores. And it's

0:14:01.800 --> 0:14:04.480
<v Speaker 1>about like three and a half AU. Will remember a

0:14:04.679 --> 0:14:08.520
<v Speaker 1>U isn't one astronomical units the distance between the Sun

0:14:08.640 --> 0:14:11.439
<v Speaker 1>and the Earth, So three and a half times the

0:14:11.559 --> 0:14:13.800
<v Speaker 1>radius of the Earth. Beyond that is the ice line,

0:14:13.880 --> 0:14:16.520
<v Speaker 1>or some people call it the snow line, and out

0:14:16.559 --> 0:14:19.840
<v Speaker 1>there it's easier to make big planets because there's ice

0:14:19.880 --> 0:14:23.320
<v Speaker 1>available to add to your core. So we think that

0:14:23.560 --> 0:14:26.880
<v Speaker 1>the way the Solar system started obviously, have a big

0:14:26.920 --> 0:14:30.000
<v Speaker 1>blob of gas and dust and some shock wave comes

0:14:30.040 --> 0:14:32.200
<v Speaker 1>through it and you get the spark that begins the

0:14:32.200 --> 0:14:34.960
<v Speaker 1>formation of the whole Solar system, which basically means the Sun.

0:14:35.400 --> 0:14:37.880
<v Speaker 1>But the Sun has gathered together a huge amount of

0:14:37.880 --> 0:14:41.160
<v Speaker 1>gas and it has around it a big swirling disk,

0:14:41.480 --> 0:14:43.720
<v Speaker 1>and that's the disc that's going to provide the material

0:14:43.960 --> 0:14:47.200
<v Speaker 1>that forms all of the planets now out past the

0:14:47.240 --> 0:14:51.000
<v Speaker 1>snow line, there's also ice in there. So the ice

0:14:51.080 --> 0:14:53.440
<v Speaker 1>and the rock and the dust gathered together to make

0:14:53.440 --> 0:14:57.760
<v Speaker 1>these protoplanetary cores. They start pulling themselves together and that

0:14:57.880 --> 0:15:01.040
<v Speaker 1>sort of seeds the planets. And so we ended up

0:15:01.080 --> 0:15:05.840
<v Speaker 1>with what four planets out past the ice line? Is

0:15:05.880 --> 0:15:08.640
<v Speaker 1>that pretty common? Like that number and like the size

0:15:08.640 --> 0:15:10.160
<v Speaker 1>of our planets does that match up with what we

0:15:10.160 --> 0:15:12.760
<v Speaker 1>see in other solar systems. We don't know the answer

0:15:12.800 --> 0:15:15.040
<v Speaker 1>to that yet, we haven't seen enough. But also remember

0:15:15.080 --> 0:15:17.040
<v Speaker 1>that we can see a bunch of solar systems, but

0:15:17.120 --> 0:15:19.360
<v Speaker 1>we're not that great at seeing all of them. And

0:15:19.400 --> 0:15:22.240
<v Speaker 1>there's certain kinds of solar systems that are easier to see.

0:15:22.360 --> 0:15:25.880
<v Speaker 1>Like it's easier to see big planets that are closer

0:15:25.920 --> 0:15:29.520
<v Speaker 1>to their Sun because they block more of the Sun's light.

0:15:29.960 --> 0:15:32.080
<v Speaker 1>The way we see these exoplanets is that they block

0:15:32.160 --> 0:15:34.920
<v Speaker 1>the light of their Sun or they tug gravitationally on

0:15:34.960 --> 0:15:37.800
<v Speaker 1>the Sun. So big planets are easier to see. Close

0:15:37.840 --> 0:15:40.560
<v Speaker 1>up planets are easier to see, so far out planets

0:15:40.640 --> 0:15:43.880
<v Speaker 1>harder to spot. Far out small planets harder to spot.

0:15:44.240 --> 0:15:46.800
<v Speaker 1>Does that mean that like super slow moving things we

0:15:46.880 --> 0:15:49.240
<v Speaker 1>probably don't have good data on yet because we wouldn't

0:15:49.240 --> 0:15:51.280
<v Speaker 1>have had a chance to see them pass in front

0:15:51.280 --> 0:15:53.480
<v Speaker 1>of the sun or tug it as it moves around

0:15:53.520 --> 0:15:56.280
<v Speaker 1>to the side. That's exactly right, Yeah, we have to

0:15:56.320 --> 0:15:59.080
<v Speaker 1>watch these things cross their sun, and so basically it's

0:15:59.120 --> 0:16:01.200
<v Speaker 1>best if you can see and pass a few times

0:16:01.200 --> 0:16:03.560
<v Speaker 1>so you can see like a regular interval, so the

0:16:03.600 --> 0:16:06.600
<v Speaker 1>equivalent of several of their years. But if their years

0:16:06.640 --> 0:16:09.360
<v Speaker 1>take like, you know, a hundred earth years to go around,

0:16:09.400 --> 0:16:11.600
<v Speaker 1>then we're not going to have had time to see it.

0:16:11.640 --> 0:16:15.160
<v Speaker 1>So slow moving things, small things, things far from their

0:16:15.200 --> 0:16:17.720
<v Speaker 1>son are harder to see. So that's a long way

0:16:17.760 --> 0:16:20.440
<v Speaker 1>of saying we don't have an unbiased picture of what's

0:16:20.440 --> 0:16:22.480
<v Speaker 1>going on in these other solar systems. And we have

0:16:22.520 --> 0:16:25.000
<v Speaker 1>to try to play this game of wondering, like, well,

0:16:25.040 --> 0:16:26.920
<v Speaker 1>if we see only one of them, do we imagine

0:16:26.920 --> 0:16:29.160
<v Speaker 1>that there are a thousand? Or if we only see

0:16:29.200 --> 0:16:30.880
<v Speaker 1>two of those, do we imagine there are a hundred.

0:16:30.920 --> 0:16:33.760
<v Speaker 1>We have to estimate like how good we are seeing them,

0:16:34.000 --> 0:16:36.240
<v Speaker 1>so we can like invert that and imagine what's actually

0:16:36.280 --> 0:16:38.760
<v Speaker 1>there that we're missing. But there's a lot that we're missing.

0:16:38.760 --> 0:16:42.120
<v Speaker 1>Still interesting Yeah, it's really fascinating. And so that's why

0:16:42.160 --> 0:16:44.960
<v Speaker 1>we focus on our solar system because it's here, it's relevant,

0:16:45.000 --> 0:16:47.000
<v Speaker 1>and it's one that we can study in great detail.

0:16:47.120 --> 0:16:49.280
<v Speaker 1>But those other solar systems do give us a lot

0:16:49.360 --> 0:16:52.000
<v Speaker 1>of clues. Back to jo Butter, we think that it

0:16:52.120 --> 0:16:54.920
<v Speaker 1>must have had to form and the outer Solar System

0:16:55.200 --> 0:16:57.640
<v Speaker 1>because that's basically the only place to make these big

0:16:57.680 --> 0:17:00.920
<v Speaker 1>gas giants. I mean, you need now of ice and

0:17:01.120 --> 0:17:03.560
<v Speaker 1>enough rock to pull together to make this big core

0:17:03.880 --> 0:17:06.600
<v Speaker 1>to grab a bunch of gas. Remember, everything in the

0:17:06.600 --> 0:17:09.480
<v Speaker 1>Solar system is competing with the Sun. In the inner

0:17:09.520 --> 0:17:11.960
<v Speaker 1>Solar system, is not that much gas left because the

0:17:12.040 --> 0:17:13.840
<v Speaker 1>Sun has slurped it all up. So to make a

0:17:13.880 --> 0:17:16.280
<v Speaker 1>gas giant, really have to be far enough away from

0:17:16.280 --> 0:17:18.840
<v Speaker 1>the Sun to get any of the gas, and you

0:17:18.880 --> 0:17:21.199
<v Speaker 1>have to be past the snow line, so you can

0:17:21.240 --> 0:17:24.320
<v Speaker 1>have ice accumulated in your core and get big enough

0:17:24.320 --> 0:17:26.400
<v Speaker 1>that you can grab some of the gas before all

0:17:26.480 --> 0:17:30.880
<v Speaker 1>spirals into the Sun. Anyway, Okay, so Jupiter was formed

0:17:30.920 --> 0:17:33.439
<v Speaker 1>in the outer Solar System and it's still in the

0:17:33.440 --> 0:17:37.160
<v Speaker 1>outer Solar system. So after the break, let's talk about

0:17:37.160 --> 0:17:54.600
<v Speaker 1>why we think it moved. Okay, so Jupiter is where

0:17:54.640 --> 0:17:56.679
<v Speaker 1>we would expect it to be, given how we expect

0:17:56.720 --> 0:17:59.879
<v Speaker 1>that it formed, So why would we suspect that it

0:18:00.080 --> 0:18:02.359
<v Speaker 1>had moved at any point. Yeah, it seems at first

0:18:02.359 --> 0:18:04.640
<v Speaker 1>like it might be a simple story. Right, Jupiter had

0:18:04.680 --> 0:18:07.600
<v Speaker 1>to form somewhere in the neighborhood where it is today,

0:18:07.880 --> 0:18:10.159
<v Speaker 1>and so the simplest explanation is, well, maybe it just

0:18:10.280 --> 0:18:12.840
<v Speaker 1>formed there and stayed there. Why do we imagine it

0:18:12.920 --> 0:18:15.560
<v Speaker 1>ever took a tour in the inner Solar System? And

0:18:15.600 --> 0:18:18.520
<v Speaker 1>the reason is that the inner Solar System looks weird,

0:18:18.600 --> 0:18:22.480
<v Speaker 1>like we can't explain the Inner Solar System in that picture.

0:18:22.480 --> 0:18:25.199
<v Speaker 1>Our models of how the Solar System came together. We

0:18:25.280 --> 0:18:27.840
<v Speaker 1>run a bunch of like simulations and try to explain

0:18:28.080 --> 0:18:31.040
<v Speaker 1>how we got Venus and Earth and Mars. None of

0:18:31.080 --> 0:18:33.720
<v Speaker 1>the models that we run actually match up with what

0:18:33.800 --> 0:18:37.200
<v Speaker 1>we see. How are they different? Well, in particular, Mars

0:18:37.320 --> 0:18:40.320
<v Speaker 1>is really weird, Like Mars is a nice little planet,

0:18:40.480 --> 0:18:43.600
<v Speaker 1>but it's really small, Like Mars is like ten percent

0:18:43.800 --> 0:18:47.120
<v Speaker 1>of the mass of the Earth. That's a really small planet.

0:18:47.320 --> 0:18:49.800
<v Speaker 1>And in all our models of the Solar System, Mars

0:18:49.800 --> 0:18:52.119
<v Speaker 1>should be a lot bigger, like as you get further

0:18:52.200 --> 0:18:55.240
<v Speaker 1>out from the Sun, there's more material available because the

0:18:55.240 --> 0:18:57.960
<v Speaker 1>Sun hasn't stolen at all, and so you expect a

0:18:58.080 --> 0:19:00.440
<v Speaker 1>planet forming around there to be like about the size

0:19:00.440 --> 0:19:02.480
<v Speaker 1>of the Earth or even bigger. You know, as you

0:19:02.520 --> 0:19:05.040
<v Speaker 1>go to the outer Solar System, things get bigger, right,

0:19:05.080 --> 0:19:08.680
<v Speaker 1>So why is Mars so tiny? Why is it so little?

0:19:08.960 --> 0:19:10.840
<v Speaker 1>So as you get farther out in the Solar System,

0:19:10.880 --> 0:19:13.080
<v Speaker 1>things should get bigger. But Jupiter is the biggest and

0:19:13.080 --> 0:19:15.679
<v Speaker 1>it's not the most far out, So why is Saturn

0:19:15.720 --> 0:19:18.200
<v Speaker 1>smaller than Jupiter? Then? Oh, yeah, that's a great question.

0:19:18.320 --> 0:19:20.600
<v Speaker 1>There's a whole other fun story about a sounder Jupiter,

0:19:20.640 --> 0:19:24.040
<v Speaker 1>maybe switching locations and the whole dance of Uranus and

0:19:24.119 --> 0:19:26.440
<v Speaker 1>Neptune that they might have done. But you're right, there's

0:19:26.440 --> 0:19:28.600
<v Speaker 1>a balance there because you want to be far enough

0:19:28.600 --> 0:19:31.160
<v Speaker 1>away from the Sun so it doesn't steal all the material,

0:19:31.359 --> 0:19:33.320
<v Speaker 1>but as you get even further away from the Sun

0:19:33.480 --> 0:19:36.440
<v Speaker 1>you run out of material also, right, Obviously there aren't

0:19:36.480 --> 0:19:39.359
<v Speaker 1>like super giant planets twice as far away as Jupiter,

0:19:39.760 --> 0:19:42.160
<v Speaker 1>and so this is something of like a peak location there.

0:19:42.320 --> 0:19:44.400
<v Speaker 1>Jupiter is probably sitting right there in the spot where

0:19:44.400 --> 0:19:46.920
<v Speaker 1>you can make the biggest planet. But the question remains

0:19:46.960 --> 0:19:49.480
<v Speaker 1>like why is Mars so a little what happened to

0:19:49.600 --> 0:19:52.919
<v Speaker 1>make Mars so tiny? And it's not just Mars? Like

0:19:52.960 --> 0:19:55.960
<v Speaker 1>the asteroid belt is also kind of weird, like we

0:19:56.000 --> 0:19:58.800
<v Speaker 1>don't really understand how it formed the way it did. Again,

0:19:59.200 --> 0:20:01.439
<v Speaker 1>we run these model let's start from just the gas cloud,

0:20:01.640 --> 0:20:03.760
<v Speaker 1>and you don't get an asteroid belt that looks the

0:20:03.760 --> 0:20:07.160
<v Speaker 1>way it does. Specifically, our asteroid belt is weird because

0:20:07.200 --> 0:20:09.879
<v Speaker 1>it has both like rocky objects that seems like they

0:20:09.880 --> 0:20:12.560
<v Speaker 1>came from the inner Solar System. Plus they have a

0:20:12.600 --> 0:20:15.000
<v Speaker 1>bunch of icy objects, the kinds of things you would

0:20:15.040 --> 0:20:18.000
<v Speaker 1>find like in the Kuiper Belt or deeper further out

0:20:18.000 --> 0:20:20.800
<v Speaker 1>in the Solar system. So there're these like pieces of

0:20:20.840 --> 0:20:23.080
<v Speaker 1>evidence you were talking earlier about like how could we

0:20:23.160 --> 0:20:26.080
<v Speaker 1>possibly find clues about things that happened so long ago?

0:20:26.359 --> 0:20:28.800
<v Speaker 1>Like these are the things that have puzzled scientists for

0:20:28.840 --> 0:20:32.280
<v Speaker 1>a long time. So is the asteroid belt inside the

0:20:32.320 --> 0:20:35.720
<v Speaker 1>ice line or on the Jupiter side of the ice line? Yeah,

0:20:35.760 --> 0:20:38.240
<v Speaker 1>the asteroid belt is really weird. Actually part of his

0:20:38.440 --> 0:20:41.440
<v Speaker 1>inside the ice line, the part that's like closer to Mars,

0:20:41.480 --> 0:20:44.280
<v Speaker 1>remember it sits between Mars and Jupiter. But it also

0:20:44.320 --> 0:20:46.680
<v Speaker 1>extends kind of far out, and part of it actually

0:20:47.240 --> 0:20:50.600
<v Speaker 1>is in orbit with Jupiter. Like it's not all between

0:20:50.720 --> 0:20:53.919
<v Speaker 1>Mars and Jupiter. There's these big blobs of asteroids that

0:20:53.960 --> 0:20:57.000
<v Speaker 1>are in Jupiter's orbit just sort of like rotated away

0:20:57.000 --> 0:20:59.520
<v Speaker 1>from them, like you know, thirty degrees around the thirty

0:20:59.520 --> 0:21:02.040
<v Speaker 1>degrees the other direction, and stuff is sort of like

0:21:02.080 --> 0:21:04.840
<v Speaker 1>sloshing back and forth. So some of it's definitely out

0:21:04.880 --> 0:21:07.840
<v Speaker 1>there past the ice line and can stay frozen, and

0:21:07.880 --> 0:21:11.440
<v Speaker 1>some of it's a little bit closer. Interest. Yeah, and

0:21:11.520 --> 0:21:14.520
<v Speaker 1>so we have these mysteries, and I love that. This

0:21:14.600 --> 0:21:16.920
<v Speaker 1>is like the way we do science. You know, we say, well,

0:21:16.960 --> 0:21:19.280
<v Speaker 1>we think we understand how the solar system works, but

0:21:19.800 --> 0:21:22.600
<v Speaker 1>let's double check. Let's run a bunch of models and

0:21:22.720 --> 0:21:26.000
<v Speaker 1>see if what we get matches up with what we

0:21:26.119 --> 0:21:29.440
<v Speaker 1>actually expected. And when you see those weird deviations, when

0:21:29.440 --> 0:21:32.080
<v Speaker 1>you see something that doesn't make sense, that's when you

0:21:32.119 --> 0:21:34.560
<v Speaker 1>know you might have found something. So it's like when

0:21:34.600 --> 0:21:38.320
<v Speaker 1>your model doesn't work is a potential discovery moment. It

0:21:38.359 --> 0:21:41.280
<v Speaker 1>isn't that how we figured out how humans figured out

0:21:41.280 --> 0:21:43.480
<v Speaker 1>that was it? Neptune was out there, something was not

0:21:43.520 --> 0:21:45.760
<v Speaker 1>working mathematically, so there had to be another planet out

0:21:45.760 --> 0:21:49.280
<v Speaker 1>there exactly. Yeah, there's all these times when something hasn't

0:21:49.320 --> 0:21:51.240
<v Speaker 1>quite worked, just like you're saying, the orbits of the

0:21:51.240 --> 0:21:53.920
<v Speaker 1>planets don't quite make sense, and that's been a clue.

0:21:54.000 --> 0:21:56.600
<v Speaker 1>Is to like a huge discovery, but always makes me

0:21:56.640 --> 0:21:59.280
<v Speaker 1>think about like all the other times when your model

0:21:59.320 --> 0:22:01.159
<v Speaker 1>doesn't work and it just because like you have a

0:22:01.160 --> 0:22:04.359
<v Speaker 1>bug where you did something stupid, you know, and you

0:22:04.400 --> 0:22:07.640
<v Speaker 1>can't be like, oh my gosh, maybe I've discovered something fantastic.

0:22:07.920 --> 0:22:10.480
<v Speaker 1>Sort of frustrating part of science. Yeah, usually for me,

0:22:10.560 --> 0:22:13.000
<v Speaker 1>it's just a bug, but I'll keep all me out hope.

0:22:14.280 --> 0:22:16.040
<v Speaker 1>We have that experience all the time. It's a large

0:22:16.040 --> 0:22:18.480
<v Speaker 1>hage on collider because we're always on the lookout for

0:22:18.600 --> 0:22:22.359
<v Speaker 1>something unexplained, something new, something weird, some new particle that

0:22:22.440 --> 0:22:25.399
<v Speaker 1>we've just created, or mini black hole or something, and

0:22:25.480 --> 0:22:28.440
<v Speaker 1>it might be evidenced by some deviation in the data

0:22:28.600 --> 0:22:31.320
<v Speaker 1>compared to what we expect. But we see that all

0:22:31.359 --> 0:22:34.920
<v Speaker 1>the time, especially young students make mistakes and they see

0:22:34.920 --> 0:22:37.120
<v Speaker 1>something weird, like oh my gosh, did I discover something

0:22:37.240 --> 0:22:39.199
<v Speaker 1>like yeah, well, you discovered that you don't know how

0:22:39.240 --> 0:22:42.639
<v Speaker 1>to run this program correctly. You discovered that you're missing

0:22:42.640 --> 0:22:46.280
<v Speaker 1>a bracket. But yeah, exactly, you discovered that bugs are

0:22:46.320 --> 0:22:48.960
<v Speaker 1>easy to insert in programs, but you also you don't

0:22:49.000 --> 0:22:51.640
<v Speaker 1>want to squash their enthusiasm. Right, It's wonderful to see

0:22:51.640 --> 0:22:54.520
<v Speaker 1>this in young scientists, to imagine that they could be

0:22:54.560 --> 0:22:57.359
<v Speaker 1>the ones making some discovering this could be a historic moment.

0:22:57.480 --> 0:22:59.280
<v Speaker 1>So I like to tell them stories like this, because

0:22:59.320 --> 0:23:02.040
<v Speaker 1>it does act really happens sometimes, Right, Sometimes we run

0:23:02.080 --> 0:23:04.639
<v Speaker 1>these models and we see something weird and it means

0:23:04.720 --> 0:23:07.760
<v Speaker 1>something real about the universe. Awesome. We can all keep

0:23:07.800 --> 0:23:11.080
<v Speaker 1>our fingers across the will have those amazing moments where

0:23:11.080 --> 0:23:13.399
<v Speaker 1>it's not you not being smart enough, it's actually the

0:23:13.480 --> 0:23:16.639
<v Speaker 1>universe revealing herself to you. And so we're trying to understand,

0:23:16.680 --> 0:23:19.080
<v Speaker 1>like how our solar system got to be weird the

0:23:19.080 --> 0:23:20.840
<v Speaker 1>way it is. Why don't we have a bunch of

0:23:20.840 --> 0:23:24.639
<v Speaker 1>other planets close to the star? Why is mar so small?

0:23:25.000 --> 0:23:27.040
<v Speaker 1>Why is the asteroid belt the way it is? This

0:23:27.200 --> 0:23:31.200
<v Speaker 1>weird mix of rocky and icy objects. So we've taken

0:23:31.200 --> 0:23:34.400
<v Speaker 1>clues from these other solar systems that have big planets

0:23:34.440 --> 0:23:37.280
<v Speaker 1>really close to their stars. One idea initially was like

0:23:37.480 --> 0:23:40.280
<v Speaker 1>maybe Jupiters formed close to the Sun. And then like

0:23:40.520 --> 0:23:43.840
<v Speaker 1>drifted out and along the way sort of messed up

0:23:43.880 --> 0:23:46.480
<v Speaker 1>things in the Solar system. But you just told us

0:23:46.760 --> 0:23:48.600
<v Speaker 1>that it needed to be out there where there's ice

0:23:48.640 --> 0:23:51.000
<v Speaker 1>in order to form. Could it have possibly formed near

0:23:51.000 --> 0:23:53.640
<v Speaker 1>the Earth? So people spend a while trying to cook

0:23:53.720 --> 0:23:56.560
<v Speaker 1>up these models and wondering like maybe there's a way

0:23:56.600 --> 0:23:59.560
<v Speaker 1>to have a hot jupiter that survives, or maybe there's

0:23:59.560 --> 0:24:01.960
<v Speaker 1>a way to form a planet really close to the star.

0:24:02.080 --> 0:24:04.960
<v Speaker 1>Maybe there are other methods. So you know, this idea

0:24:05.000 --> 0:24:08.119
<v Speaker 1>of how you form a jupiter is sort of one model,

0:24:08.119 --> 0:24:10.680
<v Speaker 1>but there are other models. There's like, you know, gravitational

0:24:10.720 --> 0:24:13.280
<v Speaker 1>instabilities that maybe stuff smashed together to make like an

0:24:13.320 --> 0:24:16.600
<v Speaker 1>unusually large object, which then like gathered together a bunch

0:24:16.600 --> 0:24:18.520
<v Speaker 1>of stuff. And people have been working on these things

0:24:18.520 --> 0:24:20.520
<v Speaker 1>and trying to put them together, and you know, this

0:24:20.600 --> 0:24:24.240
<v Speaker 1>is the kind of creativity that's inspired by basically a mystery.

0:24:24.280 --> 0:24:26.920
<v Speaker 1>But it doesn't seem to really be working, Like there's

0:24:26.960 --> 0:24:30.720
<v Speaker 1>just not enough gas and not enough mass close to

0:24:30.760 --> 0:24:33.639
<v Speaker 1>the star, and also it's just too warm, Like a

0:24:33.680 --> 0:24:35.840
<v Speaker 1>lot of this stuff, if you did happen to form

0:24:35.880 --> 0:24:39.040
<v Speaker 1>a big object, would get blown apart by the sun.

0:24:39.080 --> 0:24:42.280
<v Speaker 1>The Sun just like boil the gas off of that planet.

0:24:42.480 --> 0:24:45.119
<v Speaker 1>And it also probably just like holding apart by the

0:24:45.200 --> 0:24:47.800
<v Speaker 1>tidal forces. Remember that the Sun has a lot of

0:24:47.800 --> 0:24:50.639
<v Speaker 1>gravity and it tugs on everything. But if you're a

0:24:50.640 --> 0:24:53.240
<v Speaker 1>really big object, it's going to tug on the part

0:24:53.240 --> 0:24:55.399
<v Speaker 1>of you that's closer to the star more than it

0:24:55.480 --> 0:24:57.440
<v Speaker 1>tugs on the part of you that's far from the star.

0:24:57.960 --> 0:25:00.360
<v Speaker 1>And that's effectively the same thing as trying to pull

0:25:00.440 --> 0:25:03.440
<v Speaker 1>you apart. And that's why, for example, you get close

0:25:03.440 --> 0:25:06.280
<v Speaker 1>to a black hole, you won't survive, because you'll get

0:25:06.320 --> 0:25:09.840
<v Speaker 1>pulled apart by the relative difference in the gravity at

0:25:09.880 --> 0:25:13.400
<v Speaker 1>your feet and at your head. It's called spaghettification, one

0:25:13.400 --> 0:25:16.480
<v Speaker 1>of the best physics words out there. And so now

0:25:16.520 --> 0:25:20.280
<v Speaker 1>imagine like making a big gas giant. You've accomplished the impossible.

0:25:20.280 --> 0:25:22.720
<v Speaker 1>You've formed a gas giant close to your star. What's

0:25:22.720 --> 0:25:25.200
<v Speaker 1>going to happen The star pretty quickly is going to

0:25:25.320 --> 0:25:29.040
<v Speaker 1>spaghettify Jupiter. And like, that's a lot of spaghetti. I'm

0:25:29.080 --> 0:25:32.600
<v Speaker 1>there for that. I love spaghetti. So are people still

0:25:32.600 --> 0:25:36.040
<v Speaker 1>work on that question or have scientists pretty much decided like, okay,

0:25:36.080 --> 0:25:38.840
<v Speaker 1>this is not the answer. There's always somebody is still

0:25:38.920 --> 0:25:40.960
<v Speaker 1>working on that question. Right. There are people out there

0:25:41.080 --> 0:25:43.040
<v Speaker 1>who think that it might have been possible to make

0:25:43.080 --> 0:25:45.000
<v Speaker 1>a Jupiter close to the star, and they're working on

0:25:45.080 --> 0:25:48.000
<v Speaker 1>their models, and in that line of thinking, they're hoping

0:25:48.440 --> 0:25:51.199
<v Speaker 1>that you've made this jupiter close to the star and

0:25:51.200 --> 0:25:54.760
<v Speaker 1>that it's somehow we don't know how, then drifted out

0:25:54.960 --> 0:25:58.000
<v Speaker 1>to the outer Solar System and in doing so has

0:25:58.080 --> 0:26:00.560
<v Speaker 1>perturbed the asteroid belt and in doing so has like

0:26:01.000 --> 0:26:04.040
<v Speaker 1>stolen a lot of the material that might have made Mars.

0:26:04.080 --> 0:26:06.199
<v Speaker 1>But I don't think that it's a mainstream idea. I mean,

0:26:06.200 --> 0:26:09.119
<v Speaker 1>there's always somebody out there, you know, smoking a banana,

0:26:09.119 --> 0:26:11.679
<v Speaker 1>appeals and thinking about it. And I encourage that, and

0:26:11.680 --> 0:26:14.840
<v Speaker 1>that kind of creativity is wonderful, and you know, diversity

0:26:14.880 --> 0:26:18.600
<v Speaker 1>of ideas is also very very important for the scientific method.

0:26:18.760 --> 0:26:21.280
<v Speaker 1>But I don't think the leading idea is that you

0:26:21.400 --> 0:26:23.919
<v Speaker 1>form a hot jupiter close to the Sun and that

0:26:24.040 --> 0:26:27.320
<v Speaker 1>it then drifts out into the outer Solar system. Okay,

0:26:27.320 --> 0:26:31.160
<v Speaker 1>so it started in the outer Solar System and then

0:26:31.400 --> 0:26:33.760
<v Speaker 1>it went on a cool vacation towards the Sun and

0:26:33.840 --> 0:26:38.400
<v Speaker 1>decided it preferred skiing. Yeah, And so we don't think

0:26:38.440 --> 0:26:40.959
<v Speaker 1>that this idea of it's starting an inner solar system

0:26:41.359 --> 0:26:45.000
<v Speaker 1>and moving out makes much sense. And another clue is

0:26:45.040 --> 0:26:48.000
<v Speaker 1>that when we look at these other solar systems, the

0:26:48.000 --> 0:26:50.440
<v Speaker 1>ones that have hot jupiters, and we wonder, like, how

0:26:50.480 --> 0:26:53.360
<v Speaker 1>are they made and how could that survive? There's some

0:26:53.400 --> 0:26:56.600
<v Speaker 1>evidence that we're looking at our really young solar systems,

0:26:56.760 --> 0:26:59.639
<v Speaker 1>solo systems that haven't been around for very long. And

0:26:59.680 --> 0:27:03.320
<v Speaker 1>so one explanation for how hot jupiters even exist is

0:27:03.320 --> 0:27:06.280
<v Speaker 1>that they're transient, that they're gonna be absorbed by the

0:27:06.320 --> 0:27:09.280
<v Speaker 1>star that we're seeing them before they get spaghettified and

0:27:09.280 --> 0:27:12.000
<v Speaker 1>sucked in and basically just become part of the star.

0:27:12.560 --> 0:27:15.760
<v Speaker 1>Because we don't tend to see hot jupiters in older

0:27:15.800 --> 0:27:19.199
<v Speaker 1>solar systems. Ah, so it started in the outer solar system,

0:27:19.359 --> 0:27:21.280
<v Speaker 1>it got sucked in, and we are seeing it at

0:27:21.280 --> 0:27:23.480
<v Speaker 1>a point where it is sort of in the process

0:27:23.640 --> 0:27:26.680
<v Speaker 1>of soon to be absorbed by the sun. Is that right?

0:27:26.840 --> 0:27:29.240
<v Speaker 1>That's the leading explanation for why we are seeing hot

0:27:29.280 --> 0:27:31.880
<v Speaker 1>jupiters in other solar systems. But you know, of course

0:27:32.000 --> 0:27:35.040
<v Speaker 1>that doesn't answer the question of our solar system because

0:27:35.080 --> 0:27:37.520
<v Speaker 1>we don't have a hot Jupiter, right, But we still

0:27:37.560 --> 0:27:40.879
<v Speaker 1>have to explain what happened in the inner Solar System.

0:27:40.920 --> 0:27:43.720
<v Speaker 1>So we have Jupiter starting in the outer Solar System,

0:27:43.760 --> 0:27:46.040
<v Speaker 1>we think that makes more sense. We don't have it

0:27:46.080 --> 0:27:48.639
<v Speaker 1>currently in the Inner Solar System. So then there's this

0:27:48.760 --> 0:27:51.040
<v Speaker 1>question of like, well, how could it have perturbed things

0:27:51.119 --> 0:27:53.280
<v Speaker 1>in the inner Solar System? You know, it's sort of

0:27:53.320 --> 0:27:55.480
<v Speaker 1>like got an alibi. It's like I was born here

0:27:55.560 --> 0:27:58.680
<v Speaker 1>and I'm still here. Why are you looking at me? Right? Okay,

0:27:58.720 --> 0:28:00.760
<v Speaker 1>So the progress we've made so far are is that

0:28:01.200 --> 0:28:04.280
<v Speaker 1>there's an explanation that we don't think is right. So

0:28:04.680 --> 0:28:07.919
<v Speaker 1>let's try another explanation and see if we can maybe

0:28:08.040 --> 0:28:10.040
<v Speaker 1>solve some of the problems with what's happening with Mars

0:28:10.040 --> 0:28:25.680
<v Speaker 1>and the asteroid belt after we take a break. Okay,

0:28:25.680 --> 0:28:28.159
<v Speaker 1>So we feel pretty confident that Jupiter started in the

0:28:28.160 --> 0:28:30.720
<v Speaker 1>outer Solar System and it didn't start in the Inner

0:28:30.720 --> 0:28:33.640
<v Speaker 1>Solar System and then move out. So if it started

0:28:33.640 --> 0:28:36.040
<v Speaker 1>in the outer Solar System and it's still there, now,

0:28:36.640 --> 0:28:39.440
<v Speaker 1>does that mean at some point Jupiter sort of toyed

0:28:39.480 --> 0:28:42.440
<v Speaker 1>with the idea of a summer vacation and then decided

0:28:42.520 --> 0:28:44.880
<v Speaker 1>it preferred the cold and went back to go skiing.

0:28:44.920 --> 0:28:47.080
<v Speaker 1>Did it come to the Sun and then leave. I know,

0:28:47.160 --> 0:28:49.959
<v Speaker 1>this is that moment in the Murder mystery where you're like,

0:28:50.480 --> 0:28:53.280
<v Speaker 1>this person was home all evening. Hold on a second

0:28:53.400 --> 0:28:56.480
<v Speaker 1>to actually have a way to account for all their whereabouts.

0:28:56.520 --> 0:28:58.640
<v Speaker 1>Could they have snuck out and committed the murder and

0:28:58.640 --> 0:29:01.800
<v Speaker 1>then come back in time? How fast are those trains?

0:29:02.280 --> 0:29:04.400
<v Speaker 1>We can't leave Jupiter in the outer Solar System for

0:29:04.440 --> 0:29:07.480
<v Speaker 1>its whole history. But now we have a crazier idea,

0:29:07.520 --> 0:29:11.800
<v Speaker 1>which is maybe Jupiter did trend into the inner Solar

0:29:11.840 --> 0:29:14.920
<v Speaker 1>System just like all those other hot jupiters were seeing

0:29:14.920 --> 0:29:18.560
<v Speaker 1>in other solar systems, but that it stopped and it

0:29:18.640 --> 0:29:21.400
<v Speaker 1>turned around and it went back out to the outer

0:29:21.560 --> 0:29:25.560
<v Speaker 1>Solar system. So this is called the Grand Tach hypothesis.

0:29:25.880 --> 0:29:29.000
<v Speaker 1>Seeing Jupiter's like a sailboat that like sailed into the

0:29:29.000 --> 0:29:31.760
<v Speaker 1>inner Solar System and then sailed back out. This is

0:29:31.760 --> 0:29:34.160
<v Speaker 1>blowing my mind. So let's break it into two parts.

0:29:34.160 --> 0:29:36.520
<v Speaker 1>I guess, So, how did it get pulled in? Just

0:29:36.600 --> 0:29:39.720
<v Speaker 1>through the typical gravity pulled it in? Yeah, so you

0:29:39.760 --> 0:29:41.920
<v Speaker 1>have to cast your mind back to the very very

0:29:41.960 --> 0:29:44.680
<v Speaker 1>early days of the Solar system. Solar system we think

0:29:44.800 --> 0:29:47.760
<v Speaker 1>is about four or five billion years old and we're

0:29:47.800 --> 0:29:50.600
<v Speaker 1>talking about things that happened in the first few million years.

0:29:50.920 --> 0:29:53.360
<v Speaker 1>You shouldn't be imagining a bunch of planets around the star.

0:29:53.600 --> 0:29:56.040
<v Speaker 1>You should be imagining a star and then a huge

0:29:56.320 --> 0:29:59.400
<v Speaker 1>disc of gas and dust, and then inside that gas

0:29:59.400 --> 0:30:02.280
<v Speaker 1>and dusk, we're forming planets. But they're not like clear,

0:30:02.320 --> 0:30:05.320
<v Speaker 1>they're not like totally separated. If you were doing astronomy

0:30:05.320 --> 0:30:07.840
<v Speaker 1>back then, you would have a really hard time seeing

0:30:07.880 --> 0:30:10.360
<v Speaker 1>any planets because there's so much gas and dust everywhere.

0:30:10.680 --> 0:30:12.800
<v Speaker 1>So the beginning of the story in the first few

0:30:12.840 --> 0:30:16.040
<v Speaker 1>million years is that, like proto Jupiter has formed, but

0:30:16.120 --> 0:30:18.360
<v Speaker 1>it's not as far out as it is now. It's

0:30:18.360 --> 0:30:21.160
<v Speaker 1>only like three and a half au like right there

0:30:21.200 --> 0:30:23.200
<v Speaker 1>on the snow line. As we were saying earlier, like

0:30:23.520 --> 0:30:26.160
<v Speaker 1>the peak place to make a gas giant is just

0:30:26.280 --> 0:30:28.719
<v Speaker 1>pass where things freeze, so you can gather ice and

0:30:28.800 --> 0:30:31.120
<v Speaker 1>rocks and dust, but not so far out that things

0:30:31.120 --> 0:30:34.920
<v Speaker 1>are getting dilute. So Jubiter forms there and then it

0:30:35.240 --> 0:30:38.520
<v Speaker 1>drifts into the inner Solar system. As you're asking, like

0:30:38.680 --> 0:30:41.320
<v Speaker 1>what makes that happen, it's it just the Sun's gravity,

0:30:41.640 --> 0:30:44.760
<v Speaker 1>and you know anything can orbit stable. The Sun obviously

0:30:45.040 --> 0:30:47.040
<v Speaker 1>has a lot of gravity, but The reason, like the

0:30:47.040 --> 0:30:49.960
<v Speaker 1>Earth is not falling into the Sun right now is

0:30:50.000 --> 0:30:51.440
<v Speaker 1>that we have a lot of speed. We're in a

0:30:51.480 --> 0:30:55.320
<v Speaker 1>stable orbit. So we think Jupiter probably wasn't a stable orbit.

0:30:55.360 --> 0:30:58.520
<v Speaker 1>But remember it wasn't on its own. It's still surrounded

0:30:58.520 --> 0:31:01.080
<v Speaker 1>by a lot of gas and us that hasn't gotten

0:31:01.120 --> 0:31:04.120
<v Speaker 1>pulled into any planet. So the idea is that it

0:31:04.200 --> 0:31:06.840
<v Speaker 1>interacted with that gas and dust, which basically slowed it

0:31:06.920 --> 0:31:10.520
<v Speaker 1>down and started falling in towards the Sun. That must

0:31:10.560 --> 0:31:14.200
<v Speaker 1>have been very scary for Jupiter. I know, it's like

0:31:14.400 --> 0:31:17.520
<v Speaker 1>this inextricable fall, right, you know that you're like rolling

0:31:17.520 --> 0:31:20.440
<v Speaker 1>in towards this huge burning ball of plasma and there's

0:31:20.480 --> 0:31:23.960
<v Speaker 1>basically nothing you can do about it. So very dramatic moment.

0:31:24.320 --> 0:31:27.160
<v Speaker 1>And these gases eventually, you know, spiraled in and they

0:31:27.200 --> 0:31:30.360
<v Speaker 1>fell into the Sun, and Jupiter was spiraling and also

0:31:30.440 --> 0:31:33.239
<v Speaker 1>and so the idea is that it passed through the

0:31:33.280 --> 0:31:37.200
<v Speaker 1>inner Solar System and along the way it gobbled up

0:31:37.240 --> 0:31:41.160
<v Speaker 1>a lot of material which eventually would have otherwise led

0:31:41.200 --> 0:31:44.320
<v Speaker 1>to a larger Mars. How far in did it go?

0:31:44.440 --> 0:31:47.360
<v Speaker 1>Did it get like Earth close or just Mars close,

0:31:47.800 --> 0:31:50.160
<v Speaker 1>not quite Earth close. We think that it came into

0:31:50.200 --> 0:31:53.160
<v Speaker 1>like about one and a half a you. And that's

0:31:53.200 --> 0:31:55.880
<v Speaker 1>why we still have Earth as a pretty reasonable size,

0:31:56.200 --> 0:31:58.959
<v Speaker 1>because Jupiter came in and it either like gobbled up

0:31:58.960 --> 0:32:02.000
<v Speaker 1>the material to make ours or scattered it and threw

0:32:02.040 --> 0:32:04.640
<v Speaker 1>it into the sun. But these things in the inner

0:32:04.680 --> 0:32:07.280
<v Speaker 1>Solar system were a bit more protected. Okay, so part

0:32:07.320 --> 0:32:09.680
<v Speaker 1>of Jupiter should have been in Mars. It's like those twins,

0:32:09.680 --> 0:32:11.080
<v Speaker 1>you know, where like one of them eat the other

0:32:11.120 --> 0:32:13.360
<v Speaker 1>one and you still have like a jaw or whatever

0:32:13.600 --> 0:32:16.560
<v Speaker 1>inside the body of the adult. Those are the craziest stories.

0:32:16.640 --> 0:32:19.160
<v Speaker 1>I don't think they're actually eating the other one, but yes,

0:32:19.200 --> 0:32:21.840
<v Speaker 1>I know where you're going with that. Well, you don't

0:32:21.880 --> 0:32:23.880
<v Speaker 1>believe in the evil twin theory that twins can eat

0:32:23.880 --> 0:32:25.880
<v Speaker 1>each other in the roomb. I was reading about this

0:32:25.960 --> 0:32:28.200
<v Speaker 1>the other day, and I think it's they like absorb

0:32:28.480 --> 0:32:32.200
<v Speaker 1>eating suggests a bit more intention that I think is

0:32:32.200 --> 0:32:34.280
<v Speaker 1>actually happening in there. You know, I'm going to use

0:32:34.280 --> 0:32:36.400
<v Speaker 1>that next time I eat my kids cookies. I'm like,

0:32:36.520 --> 0:32:39.360
<v Speaker 1>I didn't eat your cookies, I just absorbed them. And

0:32:39.560 --> 0:32:43.880
<v Speaker 1>Kelly the biologist, she tells me that's different. And then

0:32:43.920 --> 0:32:46.080
<v Speaker 1>your children remind you that you are not a fetus.

0:32:46.120 --> 0:32:48.920
<v Speaker 1>You're a grown man. You can make decisions, and so

0:32:49.040 --> 0:32:50.440
<v Speaker 1>you know, let them know that they can call me

0:32:50.480 --> 0:32:53.080
<v Speaker 1>if they need back up. All right, I'll give them

0:32:53.120 --> 0:32:57.440
<v Speaker 1>your number. Anyways, So Jupiter's out there like unintentionally absorbing

0:32:57.440 --> 0:33:00.480
<v Speaker 1>the materials that Mars would have needed to get larger

0:33:00.800 --> 0:33:03.240
<v Speaker 1>and scattering a bunch of other stuff, and so it

0:33:03.320 --> 0:33:06.640
<v Speaker 1>came into about one and a half a U. And

0:33:06.640 --> 0:33:08.960
<v Speaker 1>that actually explains a lot about what's going on in

0:33:09.000 --> 0:33:11.440
<v Speaker 1>our inner Solar system. That's why there are no like

0:33:11.560 --> 0:33:14.600
<v Speaker 1>other rocky planets after Mars. We think there might have

0:33:14.640 --> 0:33:17.720
<v Speaker 1>also been other planets out there that were forming that

0:33:17.800 --> 0:33:20.400
<v Speaker 1>Jupiter just like nudged into the Sun. So why did

0:33:20.400 --> 0:33:22.600
<v Speaker 1>it nudge them into the Sun as opposed to pulling

0:33:22.640 --> 0:33:25.000
<v Speaker 1>it into Jupiter. Yeah, we don't know. It could have

0:33:25.040 --> 0:33:27.640
<v Speaker 1>been either fate, right, this is very chaotic, and so

0:33:27.720 --> 0:33:30.520
<v Speaker 1>it depends exactly on how big they were and how

0:33:30.560 --> 0:33:32.840
<v Speaker 1>they were aligned, and so the fate of these planets

0:33:32.920 --> 0:33:35.560
<v Speaker 1>could be like fall into the Sun or get absorbed

0:33:35.560 --> 0:33:38.200
<v Speaker 1>by Jupiter, or even get tossed out of the Solar

0:33:38.240 --> 0:33:41.440
<v Speaker 1>system entirely. Like Jupiter is a big bully, right, It's

0:33:41.480 --> 0:33:44.320
<v Speaker 1>so much bigger than Earth and Mars, and it comes

0:33:44.320 --> 0:33:47.520
<v Speaker 1>in and it doesn't take very much to really disrupt

0:33:47.560 --> 0:33:51.400
<v Speaker 1>the inner Solar System. Okay, so how does this describe

0:33:51.400 --> 0:33:54.480
<v Speaker 1>what happened or does this help explain what happened with

0:33:54.560 --> 0:33:57.520
<v Speaker 1>the asteroid belt. Yeah, so it actually all really fits

0:33:57.560 --> 0:34:01.000
<v Speaker 1>together beautifully, because to explain the after oid belt, you

0:34:01.040 --> 0:34:04.720
<v Speaker 1>need Jupiter to get back out to where it was. Right.

0:34:04.760 --> 0:34:07.600
<v Speaker 1>The asteroid belt has rocky stuff in it from the

0:34:07.600 --> 0:34:10.239
<v Speaker 1>inner Solar System, but also I see stuff from the

0:34:10.280 --> 0:34:13.360
<v Speaker 1>outer Solar System, and so if you could somehow turn

0:34:13.520 --> 0:34:17.000
<v Speaker 1>Jupiter around, right, we've seen all these other solar systems.

0:34:17.040 --> 0:34:20.719
<v Speaker 1>Also that these big gas giants sometimes fall slowly in

0:34:20.840 --> 0:34:23.080
<v Speaker 1>towards the star, and we think that in most cases

0:34:23.120 --> 0:34:26.040
<v Speaker 1>probably they just end up inside the star. They didn't

0:34:26.080 --> 0:34:28.880
<v Speaker 1>happen in our case. So we need Jupiter move somehow

0:34:28.960 --> 0:34:31.759
<v Speaker 1>to the outer Solar System, and in doing so we

0:34:31.840 --> 0:34:34.400
<v Speaker 1>think that it will have disrupted the asteroid belt and

0:34:34.480 --> 0:34:37.399
<v Speaker 1>also disrupted the Kuiper Belt, like pulled some of those

0:34:37.440 --> 0:34:40.800
<v Speaker 1>objects towards the inner Solar System, so that the asteroid

0:34:40.800 --> 0:34:43.360
<v Speaker 1>belt then has like a weird mixture of these like

0:34:43.520 --> 0:34:47.040
<v Speaker 1>further out objects and these inner objects. And that's why

0:34:47.040 --> 0:34:50.160
<v Speaker 1>we see these like icy objects and rocky objects in

0:34:50.200 --> 0:34:52.759
<v Speaker 1>our asteroid belt. If we can get Jupiter to go

0:34:52.920 --> 0:34:56.759
<v Speaker 1>in and then come back out, that's fascinating. So now,

0:34:56.760 --> 0:35:00.200
<v Speaker 1>how you told us that Jupiter probably slowed down own

0:35:00.239 --> 0:35:03.200
<v Speaker 1>and that's what caused it to get pulled in. So

0:35:03.280 --> 0:35:07.120
<v Speaker 1>for Jupiter to go back out again, what is required

0:35:07.200 --> 0:35:09.399
<v Speaker 1>for that? Doesn't have to start speeding up and then

0:35:09.440 --> 0:35:13.240
<v Speaker 1>also kind of get nudged. Why did it leave? Well, Jupiter,

0:35:13.360 --> 0:35:17.000
<v Speaker 1>we think probably was saved by its friend Saturn, because

0:35:17.160 --> 0:35:19.920
<v Speaker 1>Saturn has the same fate, right, Saturn, also a big

0:35:19.960 --> 0:35:24.360
<v Speaker 1>gas giant, also probably surrounded by big swarming clouds of gas,

0:35:24.600 --> 0:35:28.360
<v Speaker 1>getting slowed down drifting in towards the Inner Solar System.

0:35:28.680 --> 0:35:31.280
<v Speaker 1>To imagine Jupiter like the big brother and then Saturn

0:35:31.360 --> 0:35:33.799
<v Speaker 1>like the younger sister or the younger brother, following in

0:35:33.880 --> 0:35:36.360
<v Speaker 1>behind it, having sort of the same fate and seeing

0:35:36.360 --> 0:35:39.399
<v Speaker 1>what's happening to Jupiter. But the calculations suggests that it's

0:35:39.440 --> 0:35:42.440
<v Speaker 1>possible that as these two things get close to the

0:35:42.480 --> 0:35:45.560
<v Speaker 1>Inner Solar System that they then start tugging on each other,

0:35:45.920 --> 0:35:49.960
<v Speaker 1>and that their gravitational interaction makes this weird resonance where

0:35:49.960 --> 0:35:52.640
<v Speaker 1>they're pushing on each other and they're passing around the Sun.

0:35:52.640 --> 0:35:54.799
<v Speaker 1>They're tugging on each other in the same way. So

0:35:54.840 --> 0:35:57.640
<v Speaker 1>they do this like weird dance. Like imagine two people

0:35:57.719 --> 0:36:01.040
<v Speaker 1>spinning and both letting go and they flown out of

0:36:01.080 --> 0:36:03.440
<v Speaker 1>the inner Solar System. I know, it's crazy. It's like

0:36:03.480 --> 0:36:06.719
<v Speaker 1>Saturn like dove in after Jupiter and saved them both. Right,

0:36:07.080 --> 0:36:09.480
<v Speaker 1>they could have ended very badly. Yeah, there's got to

0:36:09.520 --> 0:36:11.400
<v Speaker 1>be a buddy comedy that could be written about this

0:36:11.560 --> 0:36:16.759
<v Speaker 1>or something that's wild exactly. And so that's maybe the

0:36:16.800 --> 0:36:20.120
<v Speaker 1>story that Jupiter started in the outer Solar system, got

0:36:20.160 --> 0:36:22.960
<v Speaker 1>tugged in as it's got slowed down by all this gas,

0:36:23.160 --> 0:36:26.360
<v Speaker 1>and then got saved by Saturn. And that would explain

0:36:26.400 --> 0:36:29.399
<v Speaker 1>why Mars is so small, and it would explain why

0:36:29.440 --> 0:36:32.920
<v Speaker 1>the asteroid belt has the weird composition that it does have.

0:36:33.440 --> 0:36:35.799
<v Speaker 1>And so is that the only explanation we have for

0:36:35.840 --> 0:36:38.600
<v Speaker 1>how Jupiter got thrown back out again? Or is that

0:36:38.680 --> 0:36:42.120
<v Speaker 1>just the top explanation right now? That's the top explanation.

0:36:42.200 --> 0:36:44.640
<v Speaker 1>And we don't think that it's very likely. I mean

0:36:44.680 --> 0:36:46.799
<v Speaker 1>we think that in most cases, when you have a

0:36:46.840 --> 0:36:50.080
<v Speaker 1>big gas giant that falls towards your star, it ends

0:36:50.080 --> 0:36:52.440
<v Speaker 1>in the way you would expect that it falls towards

0:36:52.480 --> 0:36:55.480
<v Speaker 1>the star and gets gobbled up, And so most solar

0:36:55.520 --> 0:36:57.960
<v Speaker 1>systems that have basically a Jupiter, we think that it

0:36:58.000 --> 0:37:00.600
<v Speaker 1>doesn't last for very long. So that means our solar

0:37:00.640 --> 0:37:05.040
<v Speaker 1>system is probably weird, right, that we're unusual for keeping

0:37:05.080 --> 0:37:07.319
<v Speaker 1>this big gas giant and having it back in the

0:37:07.360 --> 0:37:10.040
<v Speaker 1>outer Solar system in a stable way after all the

0:37:10.080 --> 0:37:12.799
<v Speaker 1>gas and dust have cleared out. Now Jupiter can go

0:37:13.040 --> 0:37:15.200
<v Speaker 1>back out to the past the ice line and hang

0:37:15.239 --> 0:37:17.480
<v Speaker 1>out for billions of years. That would suggest that the

0:37:17.560 --> 0:37:20.080
<v Speaker 1>reason we're weird is because we also have a Saturn.

0:37:20.640 --> 0:37:24.400
<v Speaker 1>So do other solar systems without hot jupiters also have

0:37:24.520 --> 0:37:27.560
<v Speaker 1>a Saturn equivalent? Yeah, great question. I don't think we

0:37:27.600 --> 0:37:30.000
<v Speaker 1>know the answer to that, because these planets are much

0:37:30.040 --> 0:37:33.320
<v Speaker 1>harder to spot, right, We're talking about things five six

0:37:33.440 --> 0:37:38.000
<v Speaker 1>seven a U that only passed their son every few years. Right, Like,

0:37:38.200 --> 0:37:41.320
<v Speaker 1>if you were observing our Solar system from really far away,

0:37:41.560 --> 0:37:44.320
<v Speaker 1>Jupiter and Sounder would not be that easy to spot

0:37:44.400 --> 0:37:47.240
<v Speaker 1>because while they're pretty big, they're also really far away

0:37:47.239 --> 0:37:49.640
<v Speaker 1>from the Sun and it takes them years and years

0:37:49.680 --> 0:37:52.000
<v Speaker 1>to orbit, so you would have to be watching our

0:37:52.040 --> 0:37:55.120
<v Speaker 1>solar system for a long time with a really good

0:37:55.120 --> 0:37:58.319
<v Speaker 1>telescope before you discovered Jupiter and Saturn. So that's not

0:37:58.480 --> 0:38:00.960
<v Speaker 1>something that we're really sort of good at knowing about

0:38:00.960 --> 0:38:03.919
<v Speaker 1>other solar systems. Yet so far, we mostly know what's

0:38:03.920 --> 0:38:06.600
<v Speaker 1>going on in the inner Solar system for big, fast

0:38:06.640 --> 0:38:10.400
<v Speaker 1>moving planets around their star. So astronomers have like incredible

0:38:10.440 --> 0:38:12.520
<v Speaker 1>job security because we're gonna need to watch for hundreds

0:38:12.560 --> 0:38:15.600
<v Speaker 1>of years to get these data and tuarly the government's

0:38:15.640 --> 0:38:18.000
<v Speaker 1>going to pay for all of it, exactly. Yeah, And

0:38:18.040 --> 0:38:20.759
<v Speaker 1>it's incredible what we have learned so far. You know,

0:38:20.800 --> 0:38:23.480
<v Speaker 1>we've learned so much about how our solar system is

0:38:23.520 --> 0:38:26.759
<v Speaker 1>weird to compare to the other solar systems that's out there,

0:38:26.760 --> 0:38:29.280
<v Speaker 1>and that's sort of like cool, like, hey, our solar

0:38:29.320 --> 0:38:32.399
<v Speaker 1>system is awesome and special. It's also a little bit

0:38:32.480 --> 0:38:35.680
<v Speaker 1>disheartening because if you believe in aliens, or you want

0:38:35.719 --> 0:38:37.520
<v Speaker 1>to believe in aliens, and you want to think that

0:38:37.560 --> 0:38:40.399
<v Speaker 1>there are lots of opportunities for life out there, it

0:38:40.480 --> 0:38:43.440
<v Speaker 1>makes the story a little bit harder because to have

0:38:43.480 --> 0:38:46.640
<v Speaker 1>a solar system like ours and a planet like ours,

0:38:46.960 --> 0:38:49.360
<v Speaker 1>you need this sort of special thing to happen, this

0:38:49.640 --> 0:38:52.440
<v Speaker 1>dance of the two gas giants to clear out the

0:38:52.480 --> 0:38:56.520
<v Speaker 1>inner Solar System and then also save themselves and being

0:38:56.520 --> 0:38:58.960
<v Speaker 1>the outer Solar system. You know, we think that Jupiter

0:38:59.239 --> 0:39:01.400
<v Speaker 1>probably protect the Earth from a lot of sort of

0:39:01.560 --> 0:39:04.759
<v Speaker 1>incoming bombardment because it's so big. It's like hoovering up

0:39:04.760 --> 0:39:07.520
<v Speaker 1>all the comets and other stuff. So it's a special

0:39:07.560 --> 0:39:11.440
<v Speaker 1>configuration we have. You've kind of bummed me out. You know.

0:39:11.480 --> 0:39:13.839
<v Speaker 1>At the beginning of this conversation, when we were talking

0:39:13.840 --> 0:39:16.680
<v Speaker 1>about how big our data set is, I was thinking,

0:39:16.719 --> 0:39:18.680
<v Speaker 1>all right, that's got to be good for the Drake equation.

0:39:18.719 --> 0:39:21.640
<v Speaker 1>You know, we're like adding all of these possible solar

0:39:21.640 --> 0:39:23.960
<v Speaker 1>systems that might have earthlike planets. But now what you're

0:39:24.000 --> 0:39:26.920
<v Speaker 1>telling me is probably a lot of the ones that

0:39:26.960 --> 0:39:29.920
<v Speaker 1>are out there don't have earthlike planets. And now I'm

0:39:30.000 --> 0:39:32.160
<v Speaker 1>kind of bummed, yeah, a little bit. And we've been

0:39:32.200 --> 0:39:35.000
<v Speaker 1>excited to find what we thought were earthlike planets in

0:39:35.040 --> 0:39:38.440
<v Speaker 1>these other solar systems, ones about the right radius, about

0:39:38.480 --> 0:39:40.719
<v Speaker 1>the right distance from the star. But what we don't

0:39:40.760 --> 0:39:43.160
<v Speaker 1>know is if they really have the right composition to

0:39:43.320 --> 0:39:46.440
<v Speaker 1>be an Earth. You know, it might be that Jupiter

0:39:46.560 --> 0:39:48.480
<v Speaker 1>came through the Inner Solar System and it cleared out

0:39:48.520 --> 0:39:51.520
<v Speaker 1>a lot of gas, etcetera, etcetera, And so we ended

0:39:51.600 --> 0:39:54.160
<v Speaker 1>up with a planet just the right combination of stuff

0:39:54.320 --> 0:39:57.120
<v Speaker 1>to have life. If Jupiter hadn't come through the Inner

0:39:57.120 --> 0:39:59.600
<v Speaker 1>Solar System, Earth might have been a little bit bigger

0:39:59.640 --> 0:40:01.759
<v Speaker 1>and then might have been more gas, So we might

0:40:01.760 --> 0:40:03.839
<v Speaker 1>have ended up with a very different composition. You can

0:40:03.880 --> 0:40:07.440
<v Speaker 1>imagine like a super Earth that's like choked in hydrogen

0:40:07.800 --> 0:40:10.399
<v Speaker 1>instead of having the atmosphere that we have you other way,

0:40:10.440 --> 0:40:13.480
<v Speaker 1>like Venus is just like choked in CEO two. It's

0:40:13.600 --> 0:40:16.400
<v Speaker 1>very oppressive. And so it might be a lot of

0:40:16.400 --> 0:40:19.319
<v Speaker 1>the planets we're seeing in these other Solar systems are

0:40:19.480 --> 0:40:22.400
<v Speaker 1>not actually sort of habitable in the way that we

0:40:22.440 --> 0:40:25.359
<v Speaker 1>would hope for. They're not really copies of Earth. They

0:40:25.400 --> 0:40:27.920
<v Speaker 1>might have the right size roughly and being roughly the

0:40:28.000 --> 0:40:30.279
<v Speaker 1>right position, but that doesn't mean to have the same

0:40:30.320 --> 0:40:36.800
<v Speaker 1>conditions as Earth. Man, we're lucky. Oh we're special. We're special.

0:40:36.840 --> 0:40:39.279
<v Speaker 1>I'm gonna go with lucky. But maybe life is better

0:40:39.320 --> 0:40:42.160
<v Speaker 1>if you go with special. So did Jupiter go like

0:40:42.320 --> 0:40:44.359
<v Speaker 1>back to where it came from or did it end

0:40:44.440 --> 0:40:46.440
<v Speaker 1>up a little closer a little farther out than where

0:40:46.480 --> 0:40:48.640
<v Speaker 1>it was before. It ended up a little farther out.

0:40:48.640 --> 0:40:50.480
<v Speaker 1>It like it wanted to go out. In the excerpts,

0:40:50.520 --> 0:40:52.120
<v Speaker 1>you know, it was born in the suburbs, and it

0:40:52.200 --> 0:40:54.160
<v Speaker 1>came to the inner city, and then it decided in

0:40:54.200 --> 0:40:57.280
<v Speaker 1>its retirement it wanted to live further out. So it

0:40:57.320 --> 0:40:59.799
<v Speaker 1>started out at three and a half a U. Came

0:40:59.840 --> 0:41:02.239
<v Speaker 1>in and probably about one and a half and now

0:41:02.280 --> 0:41:05.440
<v Speaker 1>it's comfortably out around five point two a U. I

0:41:05.440 --> 0:41:07.719
<v Speaker 1>can totally understand how Jupiter feels. I was born in

0:41:07.760 --> 0:41:10.200
<v Speaker 1>the suburbs and then I moved to a big city

0:41:10.280 --> 0:41:12.600
<v Speaker 1>and now I live out in the country where nobody

0:41:12.640 --> 0:41:16.160
<v Speaker 1>else is. So I feel your Jupiter. Well, it thanks

0:41:16.200 --> 0:41:18.799
<v Speaker 1>a lot to feel Jupiter. And the story doesn't end there.

0:41:19.120 --> 0:41:21.440
<v Speaker 1>What we talked about is like the first few million

0:41:21.600 --> 0:41:24.080
<v Speaker 1>years of the Solar System. But there's still a lot

0:41:24.120 --> 0:41:27.680
<v Speaker 1>of interesting planetary dynamics that need to be explained. Like

0:41:28.040 --> 0:41:32.040
<v Speaker 1>we think that maybe Uranus and Neptune switched places at

0:41:32.080 --> 0:41:35.200
<v Speaker 1>some point, and that Jupiter and Saturn may not have

0:41:35.320 --> 0:41:37.600
<v Speaker 1>sort of ended up where they are now, that it

0:41:37.640 --> 0:41:39.279
<v Speaker 1>may have taken a little while, and they may have

0:41:39.440 --> 0:41:42.840
<v Speaker 1>also done some later migrations we're talking like five hundred

0:41:42.880 --> 0:41:45.640
<v Speaker 1>million years after the start of the Solar system, So

0:41:46.000 --> 0:41:47.839
<v Speaker 1>we like to think about the Solar system is sort

0:41:47.880 --> 0:41:49.600
<v Speaker 1>of like it is what it is, and it's been

0:41:49.640 --> 0:41:51.920
<v Speaker 1>what it's been. But if you did it like in

0:41:52.000 --> 0:41:54.719
<v Speaker 1>time lapse over like hundreds of millions of years, it

0:41:54.760 --> 0:41:57.319
<v Speaker 1>would seem pretty chaotic. It would seem like, wow, there's

0:41:57.320 --> 0:42:00.400
<v Speaker 1>really something happening there. So that this idea of Jupiter

0:42:00.640 --> 0:42:04.960
<v Speaker 1>moving in and out, is this like totally accepted by

0:42:05.000 --> 0:42:09.120
<v Speaker 1>the mainstream or is this just sort of a theory

0:42:09.200 --> 0:42:13.200
<v Speaker 1>that some people ascribe to. How broadly is this idea accepted? Yeah,

0:42:13.239 --> 0:42:16.520
<v Speaker 1>it's somewhere in between. The astronomers I spoke to think

0:42:16.600 --> 0:42:20.600
<v Speaker 1>it's like probably the most plausible explanation. But you know,

0:42:20.600 --> 0:42:22.799
<v Speaker 1>there's a lot of details still to get right, and

0:42:22.840 --> 0:42:25.080
<v Speaker 1>our models are just going to keep getting better and better,

0:42:25.120 --> 0:42:27.719
<v Speaker 1>and then we could ask more and more detailed questions.

0:42:27.880 --> 0:42:30.680
<v Speaker 1>And right now the models explain Mars, but as we

0:42:30.760 --> 0:42:32.960
<v Speaker 1>make those models better, we can ask more specific questions

0:42:32.960 --> 0:42:35.480
<v Speaker 1>about like why does Mars have the composition that it

0:42:35.560 --> 0:42:38.319
<v Speaker 1>does and why does it get exactly this small and

0:42:38.400 --> 0:42:41.480
<v Speaker 1>not larger? And maybe as we do those studies we'll

0:42:41.520 --> 0:42:44.160
<v Speaker 1>find discrepancies and things that don't work, and then we'll

0:42:44.160 --> 0:42:47.120
<v Speaker 1>need to modify this model. Or maybe there's some other

0:42:47.239 --> 0:42:50.040
<v Speaker 1>crazy part of this story that we haven't even thought

0:42:50.040 --> 0:42:52.800
<v Speaker 1>of yet that could be revealed by some little detail

0:42:53.160 --> 0:42:56.839
<v Speaker 1>that some student uncovers. So, given the gaps in our

0:42:56.960 --> 0:42:59.439
<v Speaker 1>data sets, which are caused by things that are hard

0:42:59.480 --> 0:43:02.880
<v Speaker 1>to remove, like really really slow moving planets, what do

0:43:02.920 --> 0:43:05.640
<v Speaker 1>you think the chance is that by the time you

0:43:05.719 --> 0:43:09.160
<v Speaker 1>and I are, you know, retiring, that will be able

0:43:09.200 --> 0:43:12.239
<v Speaker 1>to say, like, definitely, that's what Jupiter. You know, maybe

0:43:12.239 --> 0:43:14.360
<v Speaker 1>we'll never be able to say definitely, but we feel

0:43:14.520 --> 0:43:17.120
<v Speaker 1>super confident that that's what Jupiter did. Is this a

0:43:17.160 --> 0:43:19.200
<v Speaker 1>problem that could get solved soon or are we looking

0:43:19.239 --> 0:43:21.880
<v Speaker 1>at decades and decades before we can really get a

0:43:21.880 --> 0:43:24.400
<v Speaker 1>good answer. Well, that depends, Kelly, how long until you

0:43:24.480 --> 0:43:27.520
<v Speaker 1>plan to retire. I'm not sure I'm ever going to retire.

0:43:27.640 --> 0:43:29.920
<v Speaker 1>But you know, the the average age of a woman

0:43:29.960 --> 0:43:32.800
<v Speaker 1>in the US when they die is what seven seventy

0:43:32.800 --> 0:43:35.839
<v Speaker 1>seven something like that, So that time scale, I think

0:43:35.880 --> 0:43:38.600
<v Speaker 1>that our understanding of our solar system and other solar

0:43:38.600 --> 0:43:42.759
<v Speaker 1>systems is going to be continually revolutionized, basically every ten

0:43:42.840 --> 0:43:46.120
<v Speaker 1>years for the next hundred years, because we are just

0:43:46.239 --> 0:43:49.200
<v Speaker 1>at the very beginning of understanding how these things work,

0:43:49.440 --> 0:43:52.120
<v Speaker 1>because we have just started to look and to see

0:43:52.280 --> 0:43:54.799
<v Speaker 1>these other planets, and we're going to find lots more

0:43:54.840 --> 0:43:57.960
<v Speaker 1>surprises once we developed telescopes that are better at these things.

0:43:58.320 --> 0:44:01.240
<v Speaker 1>Was James web launches and t to us more about

0:44:01.320 --> 0:44:05.080
<v Speaker 1>cold planets. James Webb's an infrared telescope that can see

0:44:05.120 --> 0:44:07.120
<v Speaker 1>things that are not just quite as hot, that can

0:44:07.120 --> 0:44:11.600
<v Speaker 1>see like cold disks of protoplanetary formation and actually maybe

0:44:11.600 --> 0:44:15.080
<v Speaker 1>individual planets that glow in the infrared. So we have

0:44:15.160 --> 0:44:18.640
<v Speaker 1>a lot more information coming, and if the universe holds

0:44:18.680 --> 0:44:22.000
<v Speaker 1>true to its reputation, it will be filled with surprises

0:44:22.080 --> 0:44:26.040
<v Speaker 1>that upend our ideas. So probably by the time we retire,

0:44:26.040 --> 0:44:29.400
<v Speaker 1>people will look back at these ideas as quaint and goofy,

0:44:29.719 --> 0:44:31.800
<v Speaker 1>and then we'll have a much more interesting idea, probably

0:44:31.840 --> 0:44:35.120
<v Speaker 1>filled with dramatic events we haven't even considered. You know,

0:44:35.239 --> 0:44:37.960
<v Speaker 1>it's a really fascinating time to be alive with the

0:44:38.040 --> 0:44:39.959
<v Speaker 1>kind of data that we're able to collect right now,

0:44:40.200 --> 0:44:41.759
<v Speaker 1>It really is. It's a kind of time that makes

0:44:41.800 --> 0:44:44.320
<v Speaker 1>me just want to like live another ten years because

0:44:44.560 --> 0:44:47.560
<v Speaker 1>the things we're learning are just blowing our minds. You know.

0:44:47.600 --> 0:44:50.279
<v Speaker 1>It makes me wonder, like, what would a children's book

0:44:50.320 --> 0:44:53.759
<v Speaker 1>about the Solar system say in a hundred years, right, Like,

0:44:54.080 --> 0:44:56.880
<v Speaker 1>I would love, I would kill to travel forward in

0:44:56.920 --> 0:45:01.600
<v Speaker 1>time and steal children's books about science. Well, this suggests

0:45:01.600 --> 0:45:03.960
<v Speaker 1>that biology needs more funding because we need people to

0:45:04.160 --> 0:45:07.840
<v Speaker 1>be working on the problem of immortality. Don't give me that.

0:45:07.880 --> 0:45:09.759
<v Speaker 1>On my campus, we have like ten times as many

0:45:09.800 --> 0:45:13.359
<v Speaker 1>biologists as businists already. Alright, alright, fair enough, but I

0:45:13.400 --> 0:45:16.000
<v Speaker 1>love biologists literally, I mean, I'm married to one. So

0:45:16.040 --> 0:45:19.200
<v Speaker 1>I'm definitely pro biology. More funding for all the sciences

0:45:19.360 --> 0:45:22.600
<v Speaker 1>so we can unravel these amazing mysteries of the universe.

0:45:22.920 --> 0:45:25.799
<v Speaker 1>There you go, agreed. Alright, something we can agree on.

0:45:26.239 --> 0:45:28.880
<v Speaker 1>So thank you everybody for joining us on this tour

0:45:29.160 --> 0:45:32.280
<v Speaker 1>of the early days of our solar system, the dramatic

0:45:32.360 --> 0:45:35.080
<v Speaker 1>story of Jupiter's visit to the inner Solar System and

0:45:35.120 --> 0:45:37.960
<v Speaker 1>how it might explain everything that we're seeing, all the

0:45:38.080 --> 0:45:40.759
<v Speaker 1>mysteries about the size of Mars and the composition of

0:45:40.840 --> 0:45:43.560
<v Speaker 1>the asteroid belt. Thank you very much for sharing your

0:45:43.600 --> 0:45:46.120
<v Speaker 1>curiosity with us. And thank you again to Kelly, our

0:45:46.200 --> 0:45:49.240
<v Speaker 1>wonderful guest host for joining us on today's episode, Thanks

0:45:49.239 --> 0:45:51.120
<v Speaker 1>for having me on the show, and thanks for listening everyone.

0:45:51.160 --> 0:46:00.360
<v Speaker 1>It was a lot of fun, alright, tune in next time. Yeah,

0:46:01.200 --> 0:46:04.040
<v Speaker 1>thanks for listening, and remember that Daniel and Jorge Explain

0:46:04.080 --> 0:46:07.040
<v Speaker 1>the Universe is a production of I Heart Radio. Or

0:46:07.120 --> 0:46:10.040
<v Speaker 1>more podcast from my heart Radio, visit the I heart

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<v Speaker 1>Radio app, Apple Podcasts, or wherever you listen to your

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<v Speaker 1>favorite shows. H