WEBVTT - Are there planets without a star?

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<v Speaker 1>Hey, Daniel, did you ever want to be an astronaut? Well, yes,

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<v Speaker 1>but I didn't because I'm terrified of the danger and

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<v Speaker 1>the adventure. Yeah, I'm not ready to travel in the

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<v Speaker 1>space until it's safe and routine. Yeah, it is pretty

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<v Speaker 1>dark and scary out there, But isn't that kind of

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<v Speaker 1>the point of space exploration to go out there and

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<v Speaker 1>discover and find new things hiding in the darkness. Yeah,

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<v Speaker 1>and I want other people to go out there take

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<v Speaker 1>those risks, and then I can just read about it

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<v Speaker 1>in the newspaper. Hi am or Handmay, cartoonist and the

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<v Speaker 1>creator of PhD Comics. Hi. I'm Daniel Whitson. I'm a

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<v Speaker 1>particle physicist, and I'm a stay at home adventurer of

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<v Speaker 1>the mind couch Explorer. I'd like to explore this vast

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<v Speaker 1>universe from the comfort of my office. But welcome to

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<v Speaker 1>our podcast, Daniel and Jorge Explain the Universe, a production

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<v Speaker 1>of I Heart Radio, in which we take you on

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<v Speaker 1>an exploration of all the amazing, crazy, monkers, beautiful, nasty, crazy,

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<v Speaker 1>weird things in this universe. Did I say crazy twice?

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<v Speaker 1>That's because the universe is that crazy. It's double crazy.

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<v Speaker 1>I feel like the things we're learning in science every year,

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<v Speaker 1>every decade, every generation are crazier than the things we

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<v Speaker 1>learned before. It's not just that we're learning more, but

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<v Speaker 1>the stuff we're revealing is just more bonkers than anything

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<v Speaker 1>we could have imagined. Don't you feel that way? Well,

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<v Speaker 1>do you think it's crazier than what we thought it

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<v Speaker 1>was before? You know, is it crazier than Greek gods

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<v Speaker 1>and Norse mythology? Well, I think it's maybe less creative,

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<v Speaker 1>but it's definitely crazier. Every generation has had to absorb

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<v Speaker 1>ideas which were very difficult to swallow because they completely

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<v Speaker 1>conflict with our view of the world. You know, the

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<v Speaker 1>universe is expanding, there is no sense of location and time.

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<v Speaker 1>You know, things are fundamentally random. Space curves like these

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<v Speaker 1>are hard things to get your mind around, and they

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<v Speaker 1>get harder and harder as we discover them. Yeah. We

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<v Speaker 1>are not the center of the universe, and the universe

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<v Speaker 1>is not like what we see around are where we are. Yeah,

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<v Speaker 1>and every time we look out into space we discover

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<v Speaker 1>new stuff, weird stuff. Places we thought were empty turned

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<v Speaker 1>out to be filled with interesting, fascinating, weird kinds of matter.

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<v Speaker 1>M Yeah, because that's kind of the history of humanity

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<v Speaker 1>and science. Right, Like, we look around and we assume

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<v Speaker 1>that the whole universe is kind of like where we're at. Right.

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<v Speaker 1>We thought the world was flat because everything seems flat

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<v Speaker 1>around us, And we thought that the Earth was the

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<v Speaker 1>center of the universe because everything seems to provolve around this.

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<v Speaker 1>But then as we learn more that we learn that

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<v Speaker 1>there are more and more different things out there. We

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<v Speaker 1>keep learning that the assumptions we make, that the generalizations

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<v Speaker 1>we make about what we learned here, cannot be applied everywhere.

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<v Speaker 1>And that's the exciting part. That's the moment of discovery,

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<v Speaker 1>when you realize, oh, I thought the universe was this way.

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<v Speaker 1>It turns out it's actually totally different in a way

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<v Speaker 1>I never imagine. We're intellectually maturing as a species by

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<v Speaker 1>discovering our universe and coming to grips with it. And

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<v Speaker 1>it's not always the way we liked it, but it

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<v Speaker 1>turns out to be quite fascinating to the other program

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<v Speaker 1>will be tackling one such idea that you know, maybe

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<v Speaker 1>a lot of people even today think is true, but

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<v Speaker 1>actually it turns out to be much more complex than that.

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<v Speaker 1>That's right, that darkness out there is more filled with

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<v Speaker 1>interesting stuff and rocks than you could have ever imagined. Yeah,

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<v Speaker 1>stuff that's out there hiding in the darkness, other worlds

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<v Speaker 1>out there looking at ours and wondering what would it

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<v Speaker 1>be like to be so close to a nice, warm,

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<v Speaker 1>toasty star. Yeah. So today on the program, we'll be

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<v Speaker 1>tackling the question are there planets without stars and not

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<v Speaker 1>just a movie stars? Right? We're talking about are there

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<v Speaker 1>places in the universe then don't have a son or

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<v Speaker 1>a star near them? I like the one you asked though, Like,

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<v Speaker 1>are their planets out there with only being C list actors?

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<v Speaker 1>That's right? Where everyone uh it only has five seconds

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<v Speaker 1>of fame. You can only be in one movie and

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<v Speaker 1>then your career is over. It's like turn limits for

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<v Speaker 1>for Hollywood actors. That's great, and then that'd be great

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<v Speaker 1>if we got rid of celebrity culture in our society. Yeah, well,

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<v Speaker 1>that won't appeal to any of our celebrity listeners, you know.

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<v Speaker 1>So Hey Brad Pitt, don't worry. You can still come

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<v Speaker 1>on the program. But apparently it works if you If

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<v Speaker 1>you speak badly about somebody don't want to come on

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<v Speaker 1>our show, then that's true. To defend themselves, maybe to

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<v Speaker 1>grab any kind of publicity they can. That's true. Stay

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<v Speaker 1>tuned for our episode in which science fiction authors come

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<v Speaker 1>on the show and respond to our critiques. And when

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<v Speaker 1>we're thinking about the broad universe, you know, you are

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<v Speaker 1>used to thinking about your planet is having one very

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<v Speaker 1>important feature, which is the on And every time you

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<v Speaker 1>think about a planet, you imagine, well, planets form around stars, right,

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<v Speaker 1>and so it's a bit mind bending to imagine that

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<v Speaker 1>the universe might be different. Yeah, a lot of people

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<v Speaker 1>might be surprised to learn that not every planet out

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<v Speaker 1>there is centered around the star. You may be shocked

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<v Speaker 1>to discover that rogue planets are not that rare. That

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<v Speaker 1>the universe may be chalk filled with these floating dark bodies. Yeah,

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<v Speaker 1>and that's the official physics name for them, right, like

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<v Speaker 1>a planet without a star. It's officially called a rogue planet. Yes,

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<v Speaker 1>but you will not be surprised to discover there is

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<v Speaker 1>some controversy about what exactly gets called a rogue planet.

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<v Speaker 1>Oh wow, physicists arguing about what to name something that's

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<v Speaker 1>so rare, not only arguing about whether something is a

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<v Speaker 1>good name, but like what exactly falls into this category?

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<v Speaker 1>You know, the whole Pluto, like is it a planet?

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<v Speaker 1>Is it not a planet? Thing? That's this same controversy

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<v Speaker 1>large interesting because I guess everything is sort of being

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<v Speaker 1>pulled by every star in the universe, So technically there

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<v Speaker 1>there isn't this a planet that's not being pulled by

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<v Speaker 1>a star. I like that. You're sort of saying every

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<v Speaker 1>planet is part of a sum solar system, even if

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<v Speaker 1>it's sort of distant from its star. Right, Well, technically, right,

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<v Speaker 1>don't all solar systems sort of overlap with each other?

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<v Speaker 1>Technically because the force of gravity is infinite has infinite reach. Yeah,

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<v Speaker 1>that's true. The force of gravity is infinite, but at

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<v Speaker 1>some point the force of gravity from these stars is

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<v Speaker 1>basically negligible and there's essentially no effect on these planets,

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<v Speaker 1>and they're more affected. Yeah, negligible, They're more affected by

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<v Speaker 1>the mass of the galaxy. So I think the distinction

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<v Speaker 1>is are you orbiting a star or are you orbiting

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<v Speaker 1>the center of the galaxy? All right, Well, I was

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<v Speaker 1>a little surprised to find out that there are road

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<v Speaker 1>planets out there, and that there are apparently not just

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<v Speaker 1>a few of them. But we were wondering how many

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<v Speaker 1>people out there knew the same fact that there are

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<v Speaker 1>planets out there in space without stars. So I walked

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<v Speaker 1>around campus a you see, Irvine, and I asked folks

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<v Speaker 1>what they thought and if they had a guess for

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<v Speaker 1>how many rogue planets there might be in the universe.

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<v Speaker 1>To think about it for a second, how many planets

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<v Speaker 1>out there in the universe? Would you, guys are out

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<v Speaker 1>there floating without a star. Here's what people had to say.

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<v Speaker 1>I have no clue how many there are. My guests

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<v Speaker 1>understanding from what I think I know is that they're

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<v Speaker 1>by one way or another of something flying by the

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<v Speaker 1>end up injected from the star that they'reth I have

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<v Speaker 1>not do you think does exists? I don't think. I

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<v Speaker 1>can't imagine that that would be not true, honestly, like

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<v Speaker 1>a lot of just like ten, I would have no

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<v Speaker 1>idea how to give a number, Um I would I

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<v Speaker 1>would actually have to say probably a lot, just because

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<v Speaker 1>gravity is so you can get a star really close

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<v Speaker 1>to another set of planets and then it throws them

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<v Speaker 1>off in space. So probably a lot, probably, I think.

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<v Speaker 1>So you think it's like seven or like a billion? Jeeus? Um, Well,

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<v Speaker 1>in a in a big universe, I don't know if

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<v Speaker 1>we could count. No, I think every planet. I think

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<v Speaker 1>interested pretty good mix of reactions. Yeah, a lot of

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<v Speaker 1>open minds. I love the people who say the universe

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<v Speaker 1>is so big you can never say no, you can

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<v Speaker 1>never say that something doesn't exist. I think that's a

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<v Speaker 1>great attitude because technically, in an infinite universe, anything can happen, right,

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<v Speaker 1>and anything is happening. Yeah, in an infinite universe, everything

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<v Speaker 1>that can happen eventually will happen and is happening somewhere.

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<v Speaker 1>So it's a good attitude. Now, we don't know the

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<v Speaker 1>universe is infinite, but it's definitely pretty big right somewhere

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<v Speaker 1>out there. There's a version of this podcast in which

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<v Speaker 1>you and I are the A List celebrities. That's not

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<v Speaker 1>this version. What are you saying? I don't I'm confused.

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<v Speaker 1>I think we're run out of letters letters. That's right

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<v Speaker 1>with the Triple A. We're the Triple We're Triple A celebrities,

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<v Speaker 1>which sounds good, but really, welcome to the minor the

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<v Speaker 1>Ego podcast, folks. Yeah, so, um, but people seem sort

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<v Speaker 1>of skeptical. I mean, some people said yes, but it

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<v Speaker 1>sort of seemed like yes, probably, but probably it's probably

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<v Speaker 1>not very common, that's right, and it's immediately a fascinating question.

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<v Speaker 1>It's the kind of thing you might not ever think about.

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<v Speaker 1>You think, oh, well, planet is of course they form

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<v Speaker 1>around stars, and that's reasonable because stars form from the

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<v Speaker 1>gravitational collapse of stuff, and plants do the same thing,

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<v Speaker 1>and so you should imagine they formed together. They're probably

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<v Speaker 1>associate with each other. You probably don't ever think that

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<v Speaker 1>there are dark bodies floating out there in between the stars.

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<v Speaker 1>But as soon as somebody suggested to you, then you

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<v Speaker 1>have to wonder, well do we know, how do we know?

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<v Speaker 1>Have we looked? Could we see them? And immediately it's

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<v Speaker 1>a question you need to know the answer to. Yeah,

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<v Speaker 1>because if it's a lot, then they would be pretty

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<v Speaker 1>uh interesting, I guess, or dangerous because what if one

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<v Speaker 1>of them hits us? Yeah, it's a little bit dangerous.

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<v Speaker 1>But also it just changes sort of your your view

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<v Speaker 1>of the universe. I mean, what if there are more

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<v Speaker 1>rogue planets out there than non rogue planets, then your

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<v Speaker 1>whole view of like what is a planet has to

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<v Speaker 1>all of a sudden change from oh, they're all around

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<v Speaker 1>stars to well, my sense of a planet is unusual

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<v Speaker 1>is a typical? Oh I see, it could be that

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<v Speaker 1>our kind of planet is the minority. Yeah, exactly, Just

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<v Speaker 1>like we discovered that our kind of matter is a

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<v Speaker 1>small fraction of all the matter in the universe. All

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<v Speaker 1>of a sudden, things we thought were typical are now weird.

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<v Speaker 1>It'd be like discovering their more continents out there. Or

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<v Speaker 1>you know, you grow up in your family eats a

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<v Speaker 1>dinner a certain way, and then you go to a

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<v Speaker 1>friend's house you discover, oh man, my family is weird.

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<v Speaker 1>We are and we don't use utensils at home or

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<v Speaker 1>whatever it is. You know, it's it's maturing in that

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<v Speaker 1>same way, right, It's expanding your horizon and your idea

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<v Speaker 1>of the universe. And that's why this is such a

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<v Speaker 1>fun opportunity to learn something new about the universe. All right,

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<v Speaker 1>so let's get into it. Daniel Wood exactly is a

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<v Speaker 1>rogue planet. Right, So let's begin with technical definitional stuff

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<v Speaker 1>that we could argue about easily for half an hour.

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<v Speaker 1>And and and very importantly, is there a first rogue

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<v Speaker 1>planet called rogue one? Well, the movie rights for that

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<v Speaker 1>one I've already been locked up, unfortunately. Yeah, Well they're

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<v Speaker 1>not definitely not making a sequel of that one. I

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<v Speaker 1>liked it. I liked it, but you know, Rogue two's

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<v Speaker 1>agent is not exactly getting a lot of traction in Hollywood.

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<v Speaker 1>But a rogue planet is a planet that's not orbiting

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<v Speaker 1>a star. And you said earlier, and you're right that

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<v Speaker 1>every planet feels the gravity from every star in the galaxy,

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<v Speaker 1>but you have to look at its motion, like the

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<v Speaker 1>motion of the Earth is that we are orbiting our star.

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<v Speaker 1>We're moving around our star. But if we were a

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<v Speaker 1>rogue planet, then our primary motion would just be around

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<v Speaker 1>the center of the galaxy. Would be the same category

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<v Speaker 1>as the stars, like our star orbits the center of

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<v Speaker 1>the galaxy. It's a planet that's not sort of trapped

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<v Speaker 1>by the gravitational well or pool of a star. Yeah,

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<v Speaker 1>we liked to in goo a Solar System as an

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<v Speaker 1>object because it's gravitationally bound that the dominant gravitational force

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<v Speaker 1>on every object in the Solar System is the Sun.

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<v Speaker 1>So it's like the Sun has its own little neighborhood

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<v Speaker 1>in which it's gravity is more powerful than any other gravity.

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<v Speaker 1>Or I guess maybe not not just that it's more powerful,

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<v Speaker 1>but it's powerful enough to to sort of trap things

0:12:23.640 --> 0:12:26.240
<v Speaker 1>in its vicinity. Yeah, it's a stable to let it

0:12:26.280 --> 0:12:29.439
<v Speaker 1>go exactly. But you know, the galaxy is big, and

0:12:29.559 --> 0:12:32.480
<v Speaker 1>there are a lot of stars, but they're not that many,

0:12:32.559 --> 0:12:35.880
<v Speaker 1>and so there's a lot of room out there between stars. Remember,

0:12:35.920 --> 0:12:38.960
<v Speaker 1>we're you know, light years away from the nearest star,

0:12:39.040 --> 0:12:41.440
<v Speaker 1>which makes a huge amount of space for stuff to

0:12:41.440 --> 0:12:43.800
<v Speaker 1>be floating between the stars. Oh, I see, So there's

0:12:43.800 --> 0:12:45.520
<v Speaker 1>a lot of room for you to be out there

0:12:45.800 --> 0:12:49.920
<v Speaker 1>without falling into the you know, the trap of the

0:12:50.000 --> 0:12:52.840
<v Speaker 1>gravitational pool of a star. Yeah, if you mapped the

0:12:52.840 --> 0:12:55.840
<v Speaker 1>Milky Way onto Earth, for example, you know, you have

0:12:55.920 --> 0:12:58.680
<v Speaker 1>like one house here in Los Angeles and another house

0:12:58.720 --> 0:13:01.520
<v Speaker 1>like in Kansas, and another house like in New York City,

0:13:02.000 --> 0:13:04.440
<v Speaker 1>and there'll be a lot of room between those that

0:13:04.520 --> 0:13:06.439
<v Speaker 1>you could rogue around it. Yeah, you can have a

0:13:06.520 --> 0:13:08.839
<v Speaker 1>rogue cabin in the woods and never have to get

0:13:08.880 --> 0:13:12.400
<v Speaker 1>close to anybody. And I guess more importantly, you could

0:13:12.440 --> 0:13:15.080
<v Speaker 1>be so far away from my house and your house

0:13:15.080 --> 0:13:18.120
<v Speaker 1>in Kansas, Dad, you wouldn't feel the need to sort

0:13:18.120 --> 0:13:20.559
<v Speaker 1>of go visit. Yeah, and you could largely ignore them.

0:13:20.559 --> 0:13:23.400
<v Speaker 1>You know, those stars would just be other slightly more

0:13:23.440 --> 0:13:25.880
<v Speaker 1>bright stars in the sky, and you wouldn't feel their

0:13:25.880 --> 0:13:28.920
<v Speaker 1>gravitational pull strongly enough to get sucked into one of them.

0:13:29.000 --> 0:13:30.839
<v Speaker 1>All right, So then what's the definition then that it's

0:13:30.920 --> 0:13:35.280
<v Speaker 1>it's a planet, meaning like a ball of stuff? Is

0:13:35.320 --> 0:13:37.920
<v Speaker 1>that what it means? What is exactly a planet? Yeah?

0:13:37.920 --> 0:13:41.320
<v Speaker 1>Well that's where it gets tricky, right. Um. These are

0:13:41.559 --> 0:13:46.640
<v Speaker 1>either things that were formed in other solar systems and

0:13:46.679 --> 0:13:51.480
<v Speaker 1>then ejected, or you could also think about stars that

0:13:51.600 --> 0:13:55.240
<v Speaker 1>never sort of got started, like failed stars. You know

0:13:55.280 --> 0:13:57.520
<v Speaker 1>what if a star never sort of turns on because

0:13:57.559 --> 0:14:00.400
<v Speaker 1>it's not big enough to burn, is that a rogue

0:14:00.400 --> 0:14:02.960
<v Speaker 1>planet or is that a failed star? Is a heated

0:14:03.000 --> 0:14:05.800
<v Speaker 1>debate in astronomy, But both of those things are out

0:14:05.840 --> 0:14:08.000
<v Speaker 1>there well in a way sort of Jube, isn't Jupiter

0:14:08.160 --> 0:14:10.280
<v Speaker 1>also kind of a failed star? Like it could have

0:14:10.280 --> 0:14:13.200
<v Speaker 1>been a star but it wasn't. Yeah, And if Jupiter

0:14:13.280 --> 0:14:15.960
<v Speaker 1>had formed far enough away from the Sun on its own,

0:14:15.960 --> 0:14:17.800
<v Speaker 1>if it was like the center of its own little

0:14:17.800 --> 0:14:21.760
<v Speaker 1>gravitational neighborhood, we would call it a sub brown dwarf star.

0:14:22.280 --> 0:14:24.480
<v Speaker 1>But because it formed around our star, we call it

0:14:24.520 --> 0:14:26.920
<v Speaker 1>a planet. And so there's a lot of energy spent

0:14:26.960 --> 0:14:30.160
<v Speaker 1>in astronomy arguing about these names and definitions. And wait,

0:14:30.160 --> 0:14:33.200
<v Speaker 1>you're saying that if Jupiter wasn't in our solar system,

0:14:33.240 --> 0:14:35.720
<v Speaker 1>if it was out there, it would be considered a

0:14:35.760 --> 0:14:38.200
<v Speaker 1>star even though it's not burning. Yeah, there's a whole

0:14:38.240 --> 0:14:41.880
<v Speaker 1>category of stars called brown dwarfs and sub brown dwarfs

0:14:41.920 --> 0:14:45.400
<v Speaker 1>that are just not big enough to ignite fusion and

0:14:45.480 --> 0:14:48.080
<v Speaker 1>to burn and to glow. But why still call them

0:14:48.080 --> 0:14:50.840
<v Speaker 1>a star if they're not ignited? I'm burning, see what

0:14:50.880 --> 0:14:52.960
<v Speaker 1>I mean. People have strong feelings about this, like you do.

0:14:53.040 --> 0:14:57.280
<v Speaker 1>Apparently in your mind you think, you think, if it's

0:14:57.280 --> 0:14:58.920
<v Speaker 1>got to be burning to be a star, right, Well,

0:14:58.960 --> 0:15:01.280
<v Speaker 1>other people think, oh know, it's a failed star. That's

0:15:01.280 --> 0:15:03.080
<v Speaker 1>a kind of star, all right, So that's kind of

0:15:03.120 --> 0:15:06.200
<v Speaker 1>the definition. It's a ball of stuff, or maybe the

0:15:06.200 --> 0:15:08.640
<v Speaker 1>definition is kind of fuzzy, but generally speaking, a rogue

0:15:08.640 --> 0:15:10.720
<v Speaker 1>planet is a ball of stuff. It could be gas.

0:15:10.840 --> 0:15:15.000
<v Speaker 1>Could be rock too, right, rocks or gas or you know,

0:15:15.000 --> 0:15:19.000
<v Speaker 1>it's compressed matter kind of um just to make it

0:15:19.000 --> 0:15:21.720
<v Speaker 1>different than a cloud. And it's floating out there in space,

0:15:22.320 --> 0:15:26.920
<v Speaker 1>not in the orbit of a star. Whatever that could mean.

0:15:29.480 --> 0:15:31.560
<v Speaker 1>That's right, it's a it's a dense blob of stuff.

0:15:31.600 --> 0:15:34.520
<v Speaker 1>Primarily orbiting the center of the galaxy instead of orbiting

0:15:34.520 --> 0:15:37.560
<v Speaker 1>another star. All right, let's get into how we can

0:15:37.600 --> 0:15:40.120
<v Speaker 1>see them even though it's dark out during space and

0:15:40.160 --> 0:15:42.360
<v Speaker 1>how many there are out there in the universe. But

0:15:42.480 --> 0:15:57.560
<v Speaker 1>first let's take a quick break. All right, I know

0:15:57.640 --> 0:16:01.320
<v Speaker 1>there are floating planets out there in the universe in

0:16:01.320 --> 0:16:04.880
<v Speaker 1>our galaxy that don't have a star. They're called road planets,

0:16:04.960 --> 0:16:07.880
<v Speaker 1>and there might be a lot of them. So first

0:16:07.920 --> 0:16:09.880
<v Speaker 1>of all, I guess, how do we even see them

0:16:09.880 --> 0:16:12.440
<v Speaker 1>if it's they're not burning bright and they're not near

0:16:12.440 --> 0:16:15.280
<v Speaker 1>a star for them to shine, Um, how do we

0:16:15.520 --> 0:16:18.360
<v Speaker 1>know they're there? It's tricky, right, These are dark objects.

0:16:18.400 --> 0:16:20.640
<v Speaker 1>They are not shining, they're not emitting light, and as

0:16:20.640 --> 0:16:22.680
<v Speaker 1>you say, they're not close enough to any star to

0:16:22.760 --> 0:16:26.960
<v Speaker 1>reflect light like like exoplanets are. So it's not easy

0:16:27.000 --> 0:16:28.720
<v Speaker 1>to spot them, which is why for a long time

0:16:28.760 --> 0:16:31.720
<v Speaker 1>we didn't even know that they existed. Um, but there

0:16:31.760 --> 0:16:34.960
<v Speaker 1>are two ways to see them. One is you get

0:16:35.040 --> 0:16:38.200
<v Speaker 1>really lucky, and one is close enough that we can

0:16:38.240 --> 0:16:42.840
<v Speaker 1>see them in the infrared. Remember, these things are not burning,

0:16:42.920 --> 0:16:45.720
<v Speaker 1>so they're not shining visible light, but they still have

0:16:45.840 --> 0:16:49.000
<v Speaker 1>some heat to them and everything in the universe that

0:16:49.080 --> 0:16:53.720
<v Speaker 1>has a temperature also radiates some energy, usually in the infrared,

0:16:54.240 --> 0:16:56.520
<v Speaker 1>and so sort of glowing in the infrared. And we

0:16:56.600 --> 0:17:00.160
<v Speaker 1>have infrared telescopes, I see, because we I think we're

0:17:00.240 --> 0:17:03.520
<v Speaker 1>used to thinking of like asteroids and things out there

0:17:03.560 --> 0:17:06.760
<v Speaker 1>in spaces being cold, but you could have, for example,

0:17:06.840 --> 0:17:09.280
<v Speaker 1>like the Earth is kind of warm by itself. The

0:17:09.320 --> 0:17:10.960
<v Speaker 1>Earth is kind of warm. And even if we were

0:17:11.040 --> 0:17:14.280
<v Speaker 1>ten or fifty kelvin. And I want to give props

0:17:14.280 --> 0:17:16.000
<v Speaker 1>to the person out there who wrote in to remind

0:17:16.000 --> 0:17:19.199
<v Speaker 1>me that it's not degrees kelvin, it's just kelvin. But

0:17:19.359 --> 0:17:21.520
<v Speaker 1>even if we were just ten or fifty kelvin, we

0:17:21.520 --> 0:17:25.960
<v Speaker 1>would still radiate. Everything that's above absolute zero radiates some energy.

0:17:26.000 --> 0:17:29.080
<v Speaker 1>It's called black body radiation. Oh, I see. It sort

0:17:29.119 --> 0:17:33.200
<v Speaker 1>of shines in the infrared. Yeah. And there's a telescope

0:17:33.240 --> 0:17:36.600
<v Speaker 1>called the Wise telescope w I S E, which is

0:17:36.600 --> 0:17:38.400
<v Speaker 1>really good at seeing this stuff, and it's really good

0:17:38.400 --> 0:17:41.080
<v Speaker 1>in the infrared. And so if it's close enough that

0:17:41.240 --> 0:17:44.240
<v Speaker 1>you can spot them directly with the Wise telescope, but

0:17:44.320 --> 0:17:46.560
<v Speaker 1>it has to be pretty close. So like if our

0:17:46.600 --> 0:17:49.280
<v Speaker 1>son suddenly went out and there was no more light

0:17:49.320 --> 0:17:51.920
<v Speaker 1>in our solar system, you could still maybe see the

0:17:52.040 --> 0:17:55.200
<v Speaker 1>Earth and all the other planets. Yeah, you could, precisely.

0:17:55.280 --> 0:17:58.159
<v Speaker 1>And we do this to study other solar systems. We

0:17:58.200 --> 0:18:00.000
<v Speaker 1>look at them in the visible light and we also

0:18:00.040 --> 0:18:02.360
<v Speaker 1>look at them in the infrared to try to get

0:18:02.359 --> 0:18:04.360
<v Speaker 1>a glimpse for like, what is the stuff out there

0:18:04.400 --> 0:18:07.359
<v Speaker 1>that's not blowing. It's still there, it's giving off different

0:18:07.400 --> 0:18:09.640
<v Speaker 1>kinds of radiation. So we have lots of different ways

0:18:09.640 --> 0:18:12.719
<v Speaker 1>of looking at the sky. The infrared, X ray, radio,

0:18:13.000 --> 0:18:15.240
<v Speaker 1>These are all just different kinds of light though. They're

0:18:15.240 --> 0:18:18.800
<v Speaker 1>all just different parts of the electromagnetic spectrum. But different

0:18:18.800 --> 0:18:21.320
<v Speaker 1>things out there glow in different parts of these spectrums.

0:18:21.320 --> 0:18:23.480
<v Speaker 1>So the most direct way is to look for them

0:18:23.520 --> 0:18:26.320
<v Speaker 1>in the infrared. But they have to be really close by,

0:18:26.520 --> 0:18:28.520
<v Speaker 1>Oh I see, because otherwise it would be too faint

0:18:28.600 --> 0:18:30.919
<v Speaker 1>to see them. Yeah, Because these things are small and

0:18:31.000 --> 0:18:34.119
<v Speaker 1>pretty faint, and so they're pretty hard to spot. The

0:18:34.160 --> 0:18:36.600
<v Speaker 1>best way to see these things is to look for

0:18:36.640 --> 0:18:40.440
<v Speaker 1>a little star eclipse. What well, if you have a

0:18:40.480 --> 0:18:43.000
<v Speaker 1>big dark object somewhere out there in the universe and

0:18:43.000 --> 0:18:46.240
<v Speaker 1>it passes between you and a star, then what happens

0:18:46.359 --> 0:18:49.480
<v Speaker 1>It blocks the light from that star momentarily like a

0:18:49.560 --> 0:18:53.080
<v Speaker 1>one time eclipse. Yes, like a one time eclipse, one

0:18:53.080 --> 0:18:55.679
<v Speaker 1>time ever eclipse, one time ever. Yeah. And so you

0:18:55.680 --> 0:18:58.600
<v Speaker 1>can see these things if you very carefully watch all

0:18:58.600 --> 0:19:00.960
<v Speaker 1>the stars in the sky and wait for a blip.

0:19:01.200 --> 0:19:04.720
<v Speaker 1>But there's something really fascinating because you might expect that,

0:19:04.840 --> 0:19:07.560
<v Speaker 1>like a star eclipse would dim the star, that it

0:19:07.600 --> 0:19:10.199
<v Speaker 1>would go out for a minute and then come back, right,

0:19:10.200 --> 0:19:13.600
<v Speaker 1>that's you'd expect, But this is really weird. Gravitational effect.

0:19:13.600 --> 0:19:16.639
<v Speaker 1>If the rogue planet or whatever it is alien ship

0:19:16.960 --> 0:19:20.920
<v Speaker 1>is big enough, then it has a gravitational lensing effect.

0:19:20.960 --> 0:19:23.920
<v Speaker 1>It acts like a big lens in space. Because remember

0:19:24.240 --> 0:19:27.840
<v Speaker 1>gravity is the bending of space. So gravity can change

0:19:27.880 --> 0:19:30.720
<v Speaker 1>the direction of light. We'll just block the light, they'll

0:19:31.160 --> 0:19:33.520
<v Speaker 1>bend the light. I mean that sort of happens here

0:19:33.560 --> 0:19:36.200
<v Speaker 1>on Earth too when there's an eclipse, right, doesn't the

0:19:36.320 --> 0:19:38.560
<v Speaker 1>light sort of go around the Moon when it's blocking

0:19:38.560 --> 0:19:40.600
<v Speaker 1>the sign a little bit? It does a little bit. Yeah,

0:19:40.800 --> 0:19:43.520
<v Speaker 1>And in this case it can actually enhance the strength

0:19:43.520 --> 0:19:45.720
<v Speaker 1>of that star because it acts like a lens. It

0:19:45.800 --> 0:19:48.720
<v Speaker 1>gathers more light and it focuses it all on the Earth.

0:19:49.119 --> 0:19:51.639
<v Speaker 1>So what actually happens when you get a micro lensing

0:19:51.680 --> 0:19:54.160
<v Speaker 1>event they call it, is that the star gets brighter,

0:19:54.440 --> 0:19:57.920
<v Speaker 1>not just a darker or like darker and lighter. Yeah,

0:19:57.960 --> 0:20:00.520
<v Speaker 1>it actually gets brighter. It gets enhanced, right, it gets

0:20:00.560 --> 0:20:04.240
<v Speaker 1>amplified by this micro lensing, and so the very center

0:20:04.280 --> 0:20:06.720
<v Speaker 1>of it is blocked out. But you're gathering light from

0:20:06.720 --> 0:20:09.440
<v Speaker 1>nearby and focusing it onto the earth. You actually get

0:20:09.480 --> 0:20:12.000
<v Speaker 1>more of the starlight when it goes by. It's an

0:20:12.000 --> 0:20:15.760
<v Speaker 1>eclipse that makes it the start look brighter. Yeah, recisely.

0:20:15.800 --> 0:20:18.680
<v Speaker 1>It's really fun. And the telescope to see these things

0:20:18.800 --> 0:20:22.800
<v Speaker 1>has a really awesome name. It's called the OGLE telescope.

0:20:23.400 --> 0:20:27.920
<v Speaker 1>I thought I thought it was already too much to

0:20:28.000 --> 0:20:32.360
<v Speaker 1>have a wise telescope. W I s e this one.

0:20:32.680 --> 0:20:35.320
<v Speaker 1>I want to look at things called the OGLE if

0:20:35.359 --> 0:20:37.560
<v Speaker 1>you want to sit on the couch and ogle the universe,

0:20:37.880 --> 0:20:43.880
<v Speaker 1>and you do it using the optical Gravitational Lensing Experiment OGL. Wow,

0:20:44.720 --> 0:20:47.480
<v Speaker 1>you guys probably pop some champagne when you came up

0:20:47.520 --> 0:20:49.240
<v Speaker 1>with that name. So those are the two ways you

0:20:49.240 --> 0:20:51.680
<v Speaker 1>can see him. You can see them either through micro

0:20:51.760 --> 0:20:56.359
<v Speaker 1>lensing or anti eclipses or directly through the infrared. And

0:20:56.440 --> 0:20:58.399
<v Speaker 1>so what do we know about them? Do we know

0:20:59.200 --> 0:21:02.119
<v Speaker 1>are they sort of round like our planets necessarily, or

0:21:02.160 --> 0:21:05.800
<v Speaker 1>do they look like giant asteroids or what do we

0:21:05.880 --> 0:21:08.360
<v Speaker 1>expect them to look like? Yeah, we expect that they're

0:21:08.400 --> 0:21:12.080
<v Speaker 1>mostly round because anything that's big enough gravity will make

0:21:12.080 --> 0:21:15.399
<v Speaker 1>it round. You know, gravity is powerful, and if you've

0:21:15.400 --> 0:21:17.560
<v Speaker 1>got a bit that's sticking out, eventually it's going to

0:21:17.720 --> 0:21:20.480
<v Speaker 1>roll down. And so you have something that's big enough

0:21:20.520 --> 0:21:23.360
<v Speaker 1>to have strong gravity, it's going to get around. Oh,

0:21:23.440 --> 0:21:25.720
<v Speaker 1>I see, And you expect these to be big, right,

0:21:25.760 --> 0:21:28.760
<v Speaker 1>I guess if you're If you're calling them planets, there's

0:21:28.760 --> 0:21:32.280
<v Speaker 1>a certain size associated with that name, isn't there? Like

0:21:32.320 --> 0:21:35.879
<v Speaker 1>Pluto got demoted because it wasn't big enough. Yeah, But

0:21:35.880 --> 0:21:38.879
<v Speaker 1>the really amazing part is that probably there's a whole

0:21:38.920 --> 0:21:43.200
<v Speaker 1>spectrum of sizes, from like things bigger than Jupiter down

0:21:43.240 --> 0:21:46.920
<v Speaker 1>to Earth size things down to just rocks, and the

0:21:47.040 --> 0:21:51.359
<v Speaker 1>number is probably inversely proportional to the size. So there

0:21:51.400 --> 0:21:54.320
<v Speaker 1>are a certain number of Jupiter sized ones, and they're

0:21:54.320 --> 0:21:57.440
<v Speaker 1>probably more Earth sized ones, and then probably like a

0:21:57.680 --> 0:22:01.119
<v Speaker 1>xillion times more just box out there. But at some

0:22:01.160 --> 0:22:04.360
<v Speaker 1>point they're just called rocks. You wouldn't call them planets, right,

0:22:04.760 --> 0:22:07.800
<v Speaker 1>At some point they're called planets and then dwarf planets,

0:22:08.000 --> 0:22:11.480
<v Speaker 1>and then yeah, just comets or rocks or dust. Right,

0:22:11.720 --> 0:22:13.480
<v Speaker 1>and you know, some of these things have come to

0:22:13.560 --> 0:22:17.160
<v Speaker 1>our solar system. Remember Omama and the comment that came

0:22:17.240 --> 0:22:21.040
<v Speaker 1>through UM in December. These are just rocks from other

0:22:21.080 --> 0:22:23.800
<v Speaker 1>solar system that flew through our Solar system. Wow, there

0:22:23.800 --> 0:22:27.600
<v Speaker 1>are Jupiter size planets out there, just floating in space,

0:22:27.720 --> 0:22:31.000
<v Speaker 1>not being bound to any star, just doing their own thing.

0:22:31.280 --> 0:22:33.679
<v Speaker 1>And that was the question when people first thought about this.

0:22:33.720 --> 0:22:36.080
<v Speaker 1>They thought, are they out there? Let's go look for them,

0:22:36.400 --> 0:22:39.000
<v Speaker 1>and so they started using these two approaches, and what

0:22:39.119 --> 0:22:41.960
<v Speaker 1>they found sort of boggled the mind. Right, they found

0:22:41.960 --> 0:22:45.600
<v Speaker 1>more than they expected. Yeah, they found that there's something

0:22:45.680 --> 0:22:50.080
<v Speaker 1>like around one Jupiter sized rogue planet for every star

0:22:50.240 --> 0:22:52.760
<v Speaker 1>in the Milky Way. So there's hundreds of millions of

0:22:52.800 --> 0:22:56.600
<v Speaker 1>these Jupiter size rogue planets out there. Yeah, more like

0:22:56.640 --> 0:22:59.920
<v Speaker 1>a hundred billion, yeah, because it's not about a hundred

0:23:00.040 --> 0:23:02.800
<v Speaker 1>billion stars in the Milky Way. And a few years

0:23:02.800 --> 0:23:05.200
<v Speaker 1>ago there was a really exciting result. Some people said

0:23:05.240 --> 0:23:07.919
<v Speaker 1>that there might be like two to four Jupiter size

0:23:08.080 --> 0:23:11.479
<v Speaker 1>rogue planets out there for every single star, so like

0:23:11.720 --> 0:23:15.280
<v Speaker 1>hundreds of billions, and everybody was like reacted just the

0:23:15.320 --> 0:23:19.040
<v Speaker 1>way you did, like what And then another experiment did

0:23:19.080 --> 0:23:21.880
<v Speaker 1>some measurements and they came back to everybody, calm down.

0:23:22.240 --> 0:23:25.320
<v Speaker 1>It looks like there's probably just about one jupiter size road.

0:23:26.080 --> 0:23:28.040
<v Speaker 1>And I was like, that's still crazy. I mean, I

0:23:28.080 --> 0:23:31.159
<v Speaker 1>was thinking like there might be ten in the whole galaxy.

0:23:31.640 --> 0:23:34.800
<v Speaker 1>Turns out there's billions and billions of these things, and

0:23:34.840 --> 0:23:38.080
<v Speaker 1>those are the Jupiter sized ones. The milky ways litter

0:23:38.200 --> 0:23:41.520
<v Speaker 1>with these. Yeah, they're everywhere, and if as you go

0:23:41.640 --> 0:23:45.000
<v Speaker 1>down the mass scale right like Earth size planets, there

0:23:45.080 --> 0:23:48.439
<v Speaker 1>might be ten or even a hundred times as many. Wow,

0:23:48.880 --> 0:23:55.400
<v Speaker 1>it's just traffic out there. It's pretty messages stuff. Nobody's

0:23:55.440 --> 0:23:57.720
<v Speaker 1>cleaned up, right. We formed all these solar systems and

0:23:57.760 --> 0:24:00.440
<v Speaker 1>that all the leftover base are just still out there.

0:24:00.800 --> 0:24:03.200
<v Speaker 1>But you know, it gets more and more uncertain. As

0:24:03.240 --> 0:24:05.960
<v Speaker 1>the size of the object we're talking about gets smaller,

0:24:06.040 --> 0:24:09.280
<v Speaker 1>it's harder to see, and so we've seen fewer of them,

0:24:09.280 --> 0:24:12.760
<v Speaker 1>so we're making more of an extrapolation with more uncertainty.

0:24:13.040 --> 0:24:16.440
<v Speaker 1>We're in early days of understanding this, and in five, ten,

0:24:16.800 --> 0:24:19.520
<v Speaker 1>fifty years we'll have a much better handle on it.

0:24:19.680 --> 0:24:21.720
<v Speaker 1>But right now it's pretty uncertain. Are they going to

0:24:21.840 --> 0:24:23.800
<v Speaker 1>keep on floating out there? Or will will all of

0:24:23.840 --> 0:24:26.560
<v Speaker 1>these planets eventually kind of fall into a star. Think

0:24:26.600 --> 0:24:30.240
<v Speaker 1>about what happens when a big Jupiter's eye planet approaches

0:24:30.240 --> 0:24:34.280
<v Speaker 1>a star. It's not that easy to fall into orbit. Remember,

0:24:34.359 --> 0:24:37.440
<v Speaker 1>orbit requires being in the right location, having the right direction,

0:24:37.520 --> 0:24:40.959
<v Speaker 1>and the right velocity. Much more likely is that you

0:24:41.000 --> 0:24:43.000
<v Speaker 1>come into a solar system and you just sort of

0:24:43.040 --> 0:24:47.679
<v Speaker 1>like mess it up. Yeah, you perturb the gravitational, the

0:24:47.800 --> 0:24:51.000
<v Speaker 1>nice cozy gravitational orbits of everybody that's been there for

0:24:51.040 --> 0:24:53.800
<v Speaker 1>billions of years, and you make more rogue planets like

0:24:54.040 --> 0:24:55.879
<v Speaker 1>you come in and you bust up a family. If

0:24:55.880 --> 0:24:58.080
<v Speaker 1>a Jupiter sized planet came into our solar system, we

0:24:58.119 --> 0:25:00.560
<v Speaker 1>would probably lose a planet or two. Well, I hope

0:25:00.600 --> 0:25:05.879
<v Speaker 1>it's not Earth. They can take Pluto, Neptune. You know,

0:25:05.960 --> 0:25:09.240
<v Speaker 1>we don't even we don't even care about those. Wow,

0:25:09.320 --> 0:25:12.080
<v Speaker 1>they haven't even arrived yet. And you're and you're already

0:25:12.440 --> 0:25:17.360
<v Speaker 1>at the negotiating table offering up our neighbors. What has

0:25:17.480 --> 0:25:20.800
<v Speaker 1>urine has done for me lately? Oh? Come on, it's

0:25:21.000 --> 0:25:24.240
<v Speaker 1>comic fodder. Urine is really I would give away Neptune first,

0:25:25.040 --> 0:25:29.199
<v Speaker 1>I see it's less funny. I see you need you

0:25:29.240 --> 0:25:31.080
<v Speaker 1>want you want to planet around you can make fun

0:25:31.080 --> 0:25:33.280
<v Speaker 1>of it. Yeah, exactly, some some planet has to be

0:25:33.280 --> 0:25:34.960
<v Speaker 1>the butt of all of our jokes. So okay, So

0:25:35.000 --> 0:25:39.000
<v Speaker 1>it's not likely because they're if they're already floating out there,

0:25:39.040 --> 0:25:41.439
<v Speaker 1>you know, careening through space, it's unlikely for them to

0:25:41.600 --> 0:25:44.240
<v Speaker 1>stop at any particular start. They'll just kind of bounce

0:25:44.320 --> 0:25:47.200
<v Speaker 1>around from solar system to solar system. It is possible,

0:25:47.240 --> 0:25:49.800
<v Speaker 1>it's possible for our start to capture a new planet,

0:25:50.280 --> 0:25:52.560
<v Speaker 1>and people wonder about the history of our Solar system,

0:25:52.600 --> 0:25:55.080
<v Speaker 1>you know, like some of our planets have weird orbits.

0:25:55.160 --> 0:25:57.840
<v Speaker 1>Is it possible they were captured? But if you just

0:25:57.920 --> 0:26:01.760
<v Speaker 1>shoot a planet at a star, most of the trajectories

0:26:01.760 --> 0:26:04.280
<v Speaker 1>will lead to it just being like whipped around and

0:26:04.359 --> 0:26:07.480
<v Speaker 1>shot out into space and probably losing some of its planets.

0:26:07.600 --> 0:26:09.840
<v Speaker 1>I guess. Then that gets us to the question of

0:26:09.880 --> 0:26:14.560
<v Speaker 1>how these planets even formed. If they are not in

0:26:14.600 --> 0:26:18.320
<v Speaker 1>a solar system, and they were, probably they can be

0:26:18.400 --> 0:26:20.560
<v Speaker 1>captured by a solar sism. Where did they even come from?

0:26:20.680 --> 0:26:23.040
<v Speaker 1>So let's tackle that question. But first let's take a

0:26:23.080 --> 0:26:38.640
<v Speaker 1>quick break, all right, So where do rogue planets come from.

0:26:38.720 --> 0:26:41.960
<v Speaker 1>Is there like a rogue planet factory somewhere? Is there

0:26:41.960 --> 0:26:45.440
<v Speaker 1>a rogue nation of planets where all of these planets

0:26:45.800 --> 0:26:48.800
<v Speaker 1>go rogue from their rogue nation. Well, it depends on

0:26:48.840 --> 0:26:51.520
<v Speaker 1>how you define a rogue planet. There is a big

0:26:51.560 --> 0:26:55.080
<v Speaker 1>population of them that were probably formed around a star,

0:26:55.720 --> 0:26:58.240
<v Speaker 1>just like Earth and Jupiter and all of our planets.

0:26:58.520 --> 0:27:00.679
<v Speaker 1>They were part of some big cloud out of gas

0:27:00.720 --> 0:27:03.359
<v Speaker 1>and dust and rocks which coalesced to form a star

0:27:03.560 --> 0:27:07.520
<v Speaker 1>and planets. But remember that's not like organized. Nobody planned

0:27:07.560 --> 0:27:10.240
<v Speaker 1>our Solar system, and so in the early days of

0:27:10.240 --> 0:27:13.400
<v Speaker 1>our Solar system, stuff was pretty chaotic. It's not like

0:27:13.600 --> 0:27:15.679
<v Speaker 1>everybody had cleared it up and say, everybody in this

0:27:15.800 --> 0:27:18.560
<v Speaker 1>lane become Earth and everybody over here. You had stuff

0:27:18.600 --> 0:27:22.520
<v Speaker 1>sort of bouncing around more. It was more disorganized, and

0:27:22.560 --> 0:27:26.280
<v Speaker 1>so stuff got ejected. So some planets that were formed

0:27:26.280 --> 0:27:28.720
<v Speaker 1>in the early days of our Solar system probably got

0:27:28.720 --> 0:27:31.600
<v Speaker 1>ejected are now out there and planets we have a

0:27:31.640 --> 0:27:34.760
<v Speaker 1>lost brother out there or sister. Yeah, we almost certainly do.

0:27:35.359 --> 0:27:38.359
<v Speaker 1>And it's almost certainly almost certainly we um. It's a

0:27:38.359 --> 0:27:41.920
<v Speaker 1>fun question to ask, like what fraction of planets end

0:27:42.000 --> 0:27:45.439
<v Speaker 1>up in stable orbits and what fraction get ejected? Um,

0:27:45.480 --> 0:27:48.359
<v Speaker 1>And you know we're looking at our Solar system billions

0:27:48.359 --> 0:27:51.399
<v Speaker 1>of years in. It's basically after everything has settled down,

0:27:51.600 --> 0:27:54.000
<v Speaker 1>you know, in our Solar system, people think, for example,

0:27:54.080 --> 0:27:57.480
<v Speaker 1>like Saturn and Jupiter might have once had different orbits

0:27:57.480 --> 0:28:00.480
<v Speaker 1>that might have been in a different order because we

0:28:00.560 --> 0:28:03.640
<v Speaker 1>had more things. Yeah, and that there was a third planet,

0:28:03.720 --> 0:28:07.639
<v Speaker 1>another icy giant, which got ejected from the Solar system.

0:28:07.680 --> 0:28:09.919
<v Speaker 1>Like you look at the organization of our Solar system

0:28:09.960 --> 0:28:11.960
<v Speaker 1>for clues, and you're like, this looks weird. You know,

0:28:12.000 --> 0:28:14.920
<v Speaker 1>would make more sense if this crazy thing happened. And

0:28:14.960 --> 0:28:19.359
<v Speaker 1>that's how we ended up with this configuration of our planets. Oh. Interesting,

0:28:19.480 --> 0:28:22.000
<v Speaker 1>that's right, because the Solar System didn't always look like

0:28:22.040 --> 0:28:25.480
<v Speaker 1>the Solar System. No. And remember Earth had a massive

0:28:25.520 --> 0:28:28.440
<v Speaker 1>collision with like a planet sized object which led to

0:28:28.480 --> 0:28:31.399
<v Speaker 1>the formation of the Moon. Where did that thing come from? Well,

0:28:31.440 --> 0:28:36.200
<v Speaker 1>probably our Solar system and so and now it's been obliterated. Okay.

0:28:36.200 --> 0:28:39.080
<v Speaker 1>So so that's one way you can create a rogue

0:28:39.080 --> 0:28:41.880
<v Speaker 1>planet out there in spaces. You it's born in a

0:28:41.880 --> 0:28:44.800
<v Speaker 1>Solar System along with other planets, but then the other

0:28:44.960 --> 0:28:47.440
<v Speaker 1>planets sort of get together and and kind of vote,

0:28:47.640 --> 0:28:51.360
<v Speaker 1>vote that planet out. That's right, planet survivor. But you know,

0:28:51.440 --> 0:28:53.320
<v Speaker 1>from that planets point of view, they're probably like, I

0:28:53.360 --> 0:28:55.960
<v Speaker 1>never wanted to be in a solar system anyway. It's

0:28:55.960 --> 0:28:58.960
<v Speaker 1>so much more exciting out here in the backwoods. I

0:28:59.040 --> 0:29:03.400
<v Speaker 1>see much cooler out here. It is much cooler out there. Um.

0:29:03.480 --> 0:29:05.880
<v Speaker 1>And it could also be, as we talked about earlier,

0:29:06.080 --> 0:29:09.560
<v Speaker 1>that something comes by and perturbs and nice stable solar system,

0:29:09.760 --> 0:29:12.080
<v Speaker 1>like a black hole comes near a solar system and

0:29:12.280 --> 0:29:14.800
<v Speaker 1>perturbs it and sucks out some of the planets, or

0:29:14.840 --> 0:29:17.920
<v Speaker 1>even just you know, another passing rogue planet. So solar

0:29:17.960 --> 0:29:20.640
<v Speaker 1>systems are not that stable. So so those are rogue

0:29:20.760 --> 0:29:23.360
<v Speaker 1>orphan planets I guess you could call um. Then you

0:29:23.360 --> 0:29:26.160
<v Speaker 1>can also have like true road planets or like uh,

0:29:27.200 --> 0:29:31.520
<v Speaker 1>independently formed road planets, feral planets, maybe we can say

0:29:32.080 --> 0:29:35.640
<v Speaker 1>native planets. These are the ones that you were saying

0:29:35.880 --> 0:29:38.600
<v Speaker 1>don't really count as a star, and they're called sub

0:29:38.600 --> 0:29:42.840
<v Speaker 1>brown dwarf stars, and they're just clumps of matter that

0:29:43.000 --> 0:29:45.760
<v Speaker 1>started to form together but didn't get enough to form

0:29:45.880 --> 0:29:49.719
<v Speaker 1>enough gravitational pressure that you would get hydrogen fusion at

0:29:49.760 --> 0:29:52.400
<v Speaker 1>the core of it, and so you never start to burn,

0:29:52.880 --> 0:29:56.200
<v Speaker 1>because you could just have dust out there and gas

0:29:56.320 --> 0:29:58.760
<v Speaker 1>and just have it. If there's nothing around it, it'll

0:29:58.840 --> 0:30:01.160
<v Speaker 1>just come together as a clump. It will come together

0:30:01.200 --> 0:30:04.400
<v Speaker 1>as a clump. Eventually gravity wins. Right. Gravity is so

0:30:04.480 --> 0:30:08.360
<v Speaker 1>weak but so patient, and it just pulls this stuff

0:30:08.360 --> 0:30:11.200
<v Speaker 1>together whatever you started with. And you know, you might

0:30:11.200 --> 0:30:13.000
<v Speaker 1>wonder like how does that start? And that's a whole

0:30:13.000 --> 0:30:16.600
<v Speaker 1>other fascinating topic. People think that these clouds of gas

0:30:16.600 --> 0:30:19.560
<v Speaker 1>and dust and maybe like a supernova shock wave passes

0:30:19.600 --> 0:30:23.160
<v Speaker 1>through it and that triggers the coalescing. Anyway, we'll talk

0:30:23.200 --> 0:30:26.200
<v Speaker 1>about that in another episode. But whatever you got around

0:30:26.200 --> 0:30:28.680
<v Speaker 1>you forms into a blob and if it's not bright

0:30:28.800 --> 0:30:31.440
<v Speaker 1>enough to burn into a star, then it becomes to

0:30:31.520 --> 0:30:35.000
<v Speaker 1>tonight to start fusion. Right, that's what you yeah, Because

0:30:35.000 --> 0:30:36.440
<v Speaker 1>you know, if you just have a rock out there,

0:30:36.440 --> 0:30:38.960
<v Speaker 1>it's not enough to start fusion. You need enough mass

0:30:39.000 --> 0:30:41.560
<v Speaker 1>that the gravity sort of takes over and you start

0:30:41.600 --> 0:30:46.240
<v Speaker 1>that star and then it's basically a sub brown dwarf star. Man,

0:30:46.680 --> 0:30:49.240
<v Speaker 1>I'm just gonna pass judgment right now, Daniel. I think

0:30:49.240 --> 0:30:52.880
<v Speaker 1>I don't think they should be called stars, alright, Just

0:30:53.040 --> 0:30:56.280
<v Speaker 1>climbing a sub brown dwarves or something. So would you

0:30:56.280 --> 0:31:00.479
<v Speaker 1>call them a rogue planet then? Yeah? Right? Independent? An

0:31:00.480 --> 0:31:04.120
<v Speaker 1>independent planet or yeah, why not? Is there an argument

0:31:04.120 --> 0:31:06.840
<v Speaker 1>against calling them a road planet? Well, some people think that,

0:31:06.880 --> 0:31:09.040
<v Speaker 1>you know, a planet is something that formed around a star,

0:31:09.480 --> 0:31:12.000
<v Speaker 1>and so that a rogue planet. I think the generally

0:31:12.040 --> 0:31:14.600
<v Speaker 1>acceptable term is that a rogue planet something was around

0:31:14.600 --> 0:31:17.840
<v Speaker 1>a star and then got lost. It went rogue. You

0:31:17.880 --> 0:31:21.640
<v Speaker 1>can't you can't be born rogue in astronomy, apparently, I

0:31:21.800 --> 0:31:24.720
<v Speaker 1>see if by planet you mean something that forms around

0:31:24.720 --> 0:31:29.080
<v Speaker 1>a star, then technically I think that doesn't form with

0:31:29.080 --> 0:31:31.320
<v Speaker 1>it around a star is not a planet. But this

0:31:31.360 --> 0:31:33.600
<v Speaker 1>is all semantics, but it's just what people decided to

0:31:33.600 --> 0:31:35.920
<v Speaker 1>call this thing, so they can have words that they

0:31:35.960 --> 0:31:38.640
<v Speaker 1>communicate with and all mean the same thing. Or maybe

0:31:38.640 --> 0:31:40.800
<v Speaker 1>they just like arguing about this stuff at meetings. That's

0:31:40.840 --> 0:31:42.960
<v Speaker 1>probably true also, or maybe if what do you mean

0:31:43.000 --> 0:31:47.000
<v Speaker 1>by star is just like celestial objects, um, then this

0:31:47.120 --> 0:31:50.680
<v Speaker 1>could be sort of a non shining star. Yeah, and

0:31:50.720 --> 0:31:53.200
<v Speaker 1>these things sort of go the same way as the

0:31:53.280 --> 0:31:55.880
<v Speaker 1>rogue planets. That is, when it comes to stars. We

0:31:55.960 --> 0:31:58.680
<v Speaker 1>know more about bigger stars because they burn bright and

0:31:58.760 --> 0:32:01.680
<v Speaker 1>we can see them. It's hard to spot brown dwarfs

0:32:01.680 --> 0:32:04.280
<v Speaker 1>and sub brown dwarfs because they don't shine like stars.

0:32:04.720 --> 0:32:07.200
<v Speaker 1>We think that the number of these things grows very

0:32:07.280 --> 0:32:09.320
<v Speaker 1>quickly though, as you dial down the mass of the

0:32:09.320 --> 0:32:12.360
<v Speaker 1>object from bright star to sub brown dwarf to just

0:32:12.520 --> 0:32:16.000
<v Speaker 1>dark little blob. So there's a lot more sub brown

0:32:16.120 --> 0:32:19.200
<v Speaker 1>dwarfs out there than there are burning stars. There are

0:32:19.240 --> 0:32:21.400
<v Speaker 1>more failed stars and stars. Is that what you're saying?

0:32:22.320 --> 0:32:29.120
<v Speaker 1>Big surprise, right? There are more waiters than celebrities in Hollywood. Wow.

0:32:29.160 --> 0:32:33.239
<v Speaker 1>The analogies just keep keep on rewarding us here. It

0:32:33.240 --> 0:32:36.120
<v Speaker 1>turns out what we've learned here in Los Angeles does

0:32:36.160 --> 0:32:38.520
<v Speaker 1>apply to the rest of the universe. In this one case,

0:32:39.360 --> 0:32:42.040
<v Speaker 1>l A is the center of the universe. Obviously, it

0:32:42.120 --> 0:32:44.360
<v Speaker 1>has taught us something about template is a template for

0:32:44.360 --> 0:32:49.000
<v Speaker 1>the rest of the universe. That is terrifying. That is terrifying, alright, cool,

0:32:49.000 --> 0:32:52.400
<v Speaker 1>So it's pretty interesting to know, to understand, to to

0:32:52.560 --> 0:32:55.360
<v Speaker 1>have a sense that there are giant planets out there

0:32:55.400 --> 0:32:58.719
<v Speaker 1>floating in space without a home. You know, they're just

0:32:58.840 --> 0:33:01.840
<v Speaker 1>cruising through space like a like a spaceship. I guess, yeah,

0:33:01.920 --> 0:33:03.480
<v Speaker 1>And you have to wonder, like, what would it be

0:33:03.560 --> 0:33:05.680
<v Speaker 1>like to stand on the surface of that planet in

0:33:06.160 --> 0:33:10.160
<v Speaker 1>perpetual night. You have no seasons, you right, you could

0:33:10.200 --> 0:33:12.280
<v Speaker 1>do a lot of great astronomy, right because you have

0:33:12.320 --> 0:33:15.280
<v Speaker 1>no sun to interfere with your telescopes. You could have

0:33:15.320 --> 0:33:17.960
<v Speaker 1>a walk around that planet, go all the way around,

0:33:18.000 --> 0:33:20.120
<v Speaker 1>and you would only see the night sky with stars

0:33:20.120 --> 0:33:22.320
<v Speaker 1>in it. Yeah, but you could stay up all night long,

0:33:22.560 --> 0:33:32.920
<v Speaker 1>every night. You would never get a sunburn's right, that industry,

0:33:33.200 --> 0:33:37.400
<v Speaker 1>that industry would just not take off. Good for astronomers,

0:33:37.400 --> 0:33:40.400
<v Speaker 1>bad for practicing gamble. Yeah, and also makers a swimsuits,

0:33:40.440 --> 0:33:43.680
<v Speaker 1>probably because you know it'd be pretty cold. Right. We

0:33:43.800 --> 0:33:46.640
<v Speaker 1>rely on our Sun not just for sunlight but also

0:33:46.760 --> 0:33:51.280
<v Speaker 1>for the warmth, and it provides something like point nine

0:33:51.480 --> 0:33:54.680
<v Speaker 1>seven percent of the energy on the surface of the

0:33:54.680 --> 0:33:58.000
<v Speaker 1>Earth comes directly from the Sun. Really, but aren't there

0:33:58.080 --> 0:34:00.520
<v Speaker 1>planets in our Solar system that are like super hot

0:34:00.840 --> 0:34:02.960
<v Speaker 1>by themselves or is it all also from the Sun?

0:34:03.280 --> 0:34:05.800
<v Speaker 1>There are like Venus is super hot, but all that

0:34:05.920 --> 0:34:07.880
<v Speaker 1>energy comes from the Sun. And the reason it's super

0:34:07.920 --> 0:34:11.399
<v Speaker 1>hot is that has these thick clouds that trap that energy.

0:34:11.440 --> 0:34:14.080
<v Speaker 1>So all the surface energy from all the on all

0:34:14.080 --> 0:34:16.600
<v Speaker 1>the planets in our Solar system is almost all from

0:34:16.600 --> 0:34:18.600
<v Speaker 1>the Sun. But that's from on the surface, if you

0:34:18.640 --> 0:34:20.480
<v Speaker 1>wanted to live on the surface and have a view

0:34:20.480 --> 0:34:23.799
<v Speaker 1>of the night sky. But technically, could you in one

0:34:23.800 --> 0:34:26.800
<v Speaker 1>of these road planets, could you like evolve life inside

0:34:26.800 --> 0:34:29.240
<v Speaker 1>of it where where it is warm? You might because,

0:34:29.280 --> 0:34:31.440
<v Speaker 1>as you say, the core of our planet is warm,

0:34:31.440 --> 0:34:34.960
<v Speaker 1>and that's not from the Sun, that's from the gravitational pressure. Right,

0:34:34.960 --> 0:34:38.080
<v Speaker 1>the Earth is also being squeezed and melt the rock,

0:34:38.440 --> 0:34:41.360
<v Speaker 1>and from the radioactive decays that are happening inside that

0:34:41.480 --> 0:34:45.040
<v Speaker 1>rock that radiates a little bit of energy. And so

0:34:45.120 --> 0:34:47.960
<v Speaker 1>there is you know, there are hot spots underground. And

0:34:48.000 --> 0:34:50.279
<v Speaker 1>so if you're on one of these rogue planets safe

0:34:50.280 --> 0:34:53.760
<v Speaker 1>for example, the Earth went rogue, right, what would happen? Well,

0:34:54.040 --> 0:34:57.319
<v Speaker 1>their ocean good? Not good? Right? You throw away all

0:34:57.360 --> 0:35:00.960
<v Speaker 1>your sunscreen, Sorry about that, and the the oceans would

0:35:01.040 --> 0:35:04.759
<v Speaker 1>freeze and the atmosphere would like turn to snow and

0:35:04.800 --> 0:35:06.920
<v Speaker 1>just like accumulate on the surface of the Earth, which

0:35:06.960 --> 0:35:09.680
<v Speaker 1>would be crazy. But if you go down deep enough,

0:35:09.719 --> 0:35:12.080
<v Speaker 1>they would still be warmth, and so there might be

0:35:12.200 --> 0:35:15.319
<v Speaker 1>enough energy sort of bubbling up through the crust to

0:35:15.440 --> 0:35:20.080
<v Speaker 1>keep like a layer of water melted. Oh. Interesting, you

0:35:20.080 --> 0:35:23.040
<v Speaker 1>could have like underground oceans. Yeah, you could have underground

0:35:23.080 --> 0:35:25.240
<v Speaker 1>oceans that the Earth would be covered in layer of ice,

0:35:25.480 --> 0:35:27.879
<v Speaker 1>but a mile or maybe two miles down there could

0:35:27.880 --> 0:35:30.319
<v Speaker 1>still be water and it might be warm enough to

0:35:30.400 --> 0:35:33.239
<v Speaker 1>sustain life. So you would throw your sunscreen, but not

0:35:33.400 --> 0:35:36.600
<v Speaker 1>your swimsuit. Try to take your swimsuit or maybe your

0:35:36.640 --> 0:35:38.200
<v Speaker 1>wet suit, because I don't think it's going to be

0:35:38.360 --> 0:35:41.560
<v Speaker 1>very warm. But you could find like you know, cracks

0:35:41.600 --> 0:35:45.359
<v Speaker 1>in the Earth's mantle underground where there's geothermal energy, and

0:35:45.520 --> 0:35:48.040
<v Speaker 1>there are there is life the very bottom of the ocean,

0:35:48.040 --> 0:35:50.560
<v Speaker 1>clustered around these thermal vents. Yeah, and they don't have

0:35:50.600 --> 0:35:52.879
<v Speaker 1>any sunlight that you just live off of the hot

0:35:52.920 --> 0:35:55.640
<v Speaker 1>water from these events. They've been planning for this for

0:35:55.680 --> 0:35:58.399
<v Speaker 1>a long time. Yeah, they're ready for They're ready for Earth,

0:35:58.480 --> 0:36:01.319
<v Speaker 1>Bill Rode. They're the rogue life right there, ready to

0:36:01.360 --> 0:36:04.360
<v Speaker 1>take over when Earth goes rogue. There are the waiting

0:36:04.600 --> 0:36:06.759
<v Speaker 1>waiting to rise up. But I think what I what

0:36:06.800 --> 0:36:08.719
<v Speaker 1>I'm saying is that that that could happen in one

0:36:08.760 --> 0:36:10.879
<v Speaker 1>of these rogue planets out there. I mean, there could

0:36:10.880 --> 0:36:13.480
<v Speaker 1>be like a giant floating Jupiter out there in space.

0:36:13.520 --> 0:36:17.839
<v Speaker 1>It's actually like a spaceship full of life under the surface. Yeah,

0:36:17.920 --> 0:36:19.960
<v Speaker 1>and it doesn't have to be that life evolves on

0:36:19.960 --> 0:36:22.319
<v Speaker 1>a planet and then it goes rogue. I think you're saying, like,

0:36:22.520 --> 0:36:25.120
<v Speaker 1>could life evolve on a planet when it's a rogue

0:36:25.160 --> 0:36:26.960
<v Speaker 1>And I think the answer is yeah. You could have

0:36:27.320 --> 0:36:30.680
<v Speaker 1>a good water on a rogue planet and life could evolve,

0:36:30.880 --> 0:36:33.760
<v Speaker 1>and it could evolve under like a mile of ice

0:36:34.400 --> 0:36:37.479
<v Speaker 1>and never see the sky. Right, it might not even

0:36:37.520 --> 0:36:40.800
<v Speaker 1>be aware that the universe is larger than its ocean.

0:36:41.000 --> 0:36:43.400
<v Speaker 1>It would be like rogue life. And you have to wonder, like,

0:36:43.520 --> 0:36:46.680
<v Speaker 1>what kind of technology could you evolve? Like, could you

0:36:46.719 --> 0:36:50.680
<v Speaker 1>become intelligent? Could you evolve technology? Could you drill out

0:36:50.680 --> 0:36:52.680
<v Speaker 1>of the ice and then discover that? Imagine what that

0:36:52.719 --> 0:36:54.719
<v Speaker 1>would be like to be that kind of I want

0:36:54.719 --> 0:36:56.840
<v Speaker 1>to read a science fiction novel about life that evolves

0:36:56.840 --> 0:37:00.160
<v Speaker 1>on a rogue planet and develops the technology, drills as

0:37:00.160 --> 0:37:02.440
<v Speaker 1>of the ice, and then discovers Oh my gosh, the

0:37:02.560 --> 0:37:05.880
<v Speaker 1>university is so much bigger than we ever imagined. What

0:37:05.960 --> 0:37:08.799
<v Speaker 1>a moment. Right, There's a story that you and I

0:37:08.840 --> 0:37:11.319
<v Speaker 1>were talking earlier about. The writer thought Chiang, he has

0:37:11.360 --> 0:37:13.160
<v Speaker 1>a story I don't know if you read it, called

0:37:13.200 --> 0:37:15.399
<v Speaker 1>The Tower of Babel where that's kind of the plot

0:37:15.440 --> 0:37:18.360
<v Speaker 1>where they drill through the ceiling of heaven. Oh my gosh,

0:37:18.400 --> 0:37:21.240
<v Speaker 1>I want to read that story. That sounds awesome. Yeah. Alright,

0:37:21.239 --> 0:37:24.760
<v Speaker 1>So that that's kind of possible, is that there are

0:37:25.480 --> 0:37:27.720
<v Speaker 1>and and there are so many of these road planets

0:37:27.719 --> 0:37:30.600
<v Speaker 1>out there that it's it probably is maybe possible that

0:37:30.680 --> 0:37:33.000
<v Speaker 1>there is life and the life started in one of

0:37:33.000 --> 0:37:36.360
<v Speaker 1>these road planets. Yeah, it's very exciting for the possibility

0:37:36.360 --> 0:37:38.279
<v Speaker 1>of alien life, which you know, I'm a fan of.

0:37:38.640 --> 0:37:41.239
<v Speaker 1>You know, recently we've learned that there are a huge

0:37:41.320 --> 0:37:44.040
<v Speaker 1>number of planets around other stars. That was a big

0:37:44.080 --> 0:37:47.160
<v Speaker 1>moment just in astronomy in general, but also for us

0:37:47.160 --> 0:37:50.160
<v Speaker 1>who promote alien life, to realize that there are other

0:37:50.200 --> 0:37:53.680
<v Speaker 1>places for life in the universe around other stars. That

0:37:53.760 --> 0:37:56.840
<v Speaker 1>was exciting. Now we're learning that that's a tiny fraction

0:37:56.880 --> 0:37:58.640
<v Speaker 1>of all the planets out there, and that there's an

0:37:58.800 --> 0:38:02.319
<v Speaker 1>enormous number of these dark rogue planets, and I think

0:38:02.400 --> 0:38:05.120
<v Speaker 1>it's more challenging for life to form on a rogue planet,

0:38:05.239 --> 0:38:08.680
<v Speaker 1>but hey, you've got more opportunities also, right, there's a

0:38:08.880 --> 0:38:13.280
<v Speaker 1>there's like a hundred billion rogue planets the size of Jupiter. Yeah,

0:38:13.520 --> 0:38:16.080
<v Speaker 1>and maybe tend to a hundred times as many Earth

0:38:16.160 --> 0:38:19.240
<v Speaker 1>sized planets out there, and just in our solar systems,

0:38:20.040 --> 0:38:23.600
<v Speaker 1>I mean just in our galaxy that would be getting

0:38:23.640 --> 0:38:27.040
<v Speaker 1>kind of crowded. Just in our galaxy, I mean, I

0:38:27.040 --> 0:38:30.000
<v Speaker 1>mean the galaxy. There's hundreds and hundreds of billions of

0:38:30.000 --> 0:38:33.239
<v Speaker 1>these and and maybe there are hundreds of billions of galaxies.

0:38:33.239 --> 0:38:35.879
<v Speaker 1>So who knows, right there could be a rogue life

0:38:35.880 --> 0:38:37.920
<v Speaker 1>form out there. My money is that there is. I mean,

0:38:37.920 --> 0:38:40.440
<v Speaker 1>it just seems so much more likely. It seems so

0:38:40.480 --> 0:38:43.319
<v Speaker 1>impossible to imagine that nowhere out there, in any of

0:38:43.320 --> 0:38:46.480
<v Speaker 1>these planets has life begun. There's so many opportunities and

0:38:46.520 --> 0:38:49.600
<v Speaker 1>so many ways for life to happen we haven't even imagined.

0:38:50.040 --> 0:38:52.200
<v Speaker 1>I would definitely put my money on there being rogue

0:38:52.239 --> 0:38:55.440
<v Speaker 1>alien life. Can you imagine them bursting out of their

0:38:55.480 --> 0:38:59.399
<v Speaker 1>shell and be like WHOA what is this? Even crazier though,

0:38:59.480 --> 0:39:01.439
<v Speaker 1>is that like one of these rogue planets could pass

0:39:01.560 --> 0:39:05.120
<v Speaker 1>by our solar system, you know, within a few au

0:39:05.360 --> 0:39:08.040
<v Speaker 1>you know, just outside the edge of Pluto, and we

0:39:08.040 --> 0:39:10.680
<v Speaker 1>wouldn't even see it, and they might not even see us,

0:39:11.080 --> 0:39:13.000
<v Speaker 1>And so we could be like there could be like

0:39:13.080 --> 0:39:17.040
<v Speaker 1>cosmic neighbors and zooming by and we're not even paying attention.

0:39:17.280 --> 0:39:20.120
<v Speaker 1>And maybe, just maybe this happened a few billion years ago,

0:39:20.239 --> 0:39:23.200
<v Speaker 1>and maybe, just maybe an asteroid hit that road planet

0:39:23.200 --> 0:39:26.480
<v Speaker 1>and ejected a piece of rock with life that then landed.

0:39:29.000 --> 0:39:30.839
<v Speaker 1>I'm taking it too far, No, I like that. There

0:39:30.840 --> 0:39:34.080
<v Speaker 1>are a lot It's totally possible. It's possible for life

0:39:34.120 --> 0:39:36.839
<v Speaker 1>to have originated somewhere else and then come to Earth.

0:39:36.960 --> 0:39:39.279
<v Speaker 1>All right, Well, that's pretty interesting to know. It just

0:39:39.280 --> 0:39:41.920
<v Speaker 1>sort of makes you look at space and the night

0:39:41.960 --> 0:39:45.040
<v Speaker 1>sky differently. And in all those places where you only

0:39:45.080 --> 0:39:48.880
<v Speaker 1>see blackness, there could be planets out there, floating and

0:39:49.160 --> 0:39:52.440
<v Speaker 1>possibly with life. Yeah, and this life might not be

0:39:52.560 --> 0:39:55.200
<v Speaker 1>looking back at you. It might be hidden under two

0:39:55.239 --> 0:39:58.440
<v Speaker 1>miles of ice, looking up at the inside of its

0:39:58.440 --> 0:40:01.359
<v Speaker 1>ocean and wondering what l is out there? Right, that's

0:40:01.400 --> 0:40:05.239
<v Speaker 1>no interest in being famous like a star, only because

0:40:05.239 --> 0:40:07.680
<v Speaker 1>they don't even know it's possible. Once they get a

0:40:07.760 --> 0:40:13.040
<v Speaker 1>taste of it. Though, Once stay discovered television, it's all over.

0:40:13.920 --> 0:40:15.879
<v Speaker 1>Who doesn't want to be a star? All right, Well,

0:40:15.880 --> 0:40:19.680
<v Speaker 1>we hope you enjoyed that little tour into the blackness

0:40:19.840 --> 0:40:22.480
<v Speaker 1>of space and what could be out there. Waiting for

0:40:22.600 --> 0:40:25.160
<v Speaker 1>us to discover and as usual, you are in no

0:40:25.320 --> 0:40:27.719
<v Speaker 1>danger as you sit on your couch or sit in

0:40:27.760 --> 0:40:29.960
<v Speaker 1>the seat of your car and listen to us helping

0:40:30.000 --> 0:40:33.239
<v Speaker 1>you explore the universe. All right, We hope you enjoyed that.

0:40:33.320 --> 0:40:43.160
<v Speaker 1>See you next time. Before you still have a question

0:40:43.200 --> 0:40:46.640
<v Speaker 1>after listening to all these explanations, please drop us a line.

0:40:46.680 --> 0:40:48.839
<v Speaker 1>We'd love to hear from you. You can find us

0:40:48.840 --> 0:40:52.640
<v Speaker 1>on Facebook, Twitter, and Instagram at Daniel and Jorge That's

0:40:52.640 --> 0:40:56.040
<v Speaker 1>one word, or email us at Feedback at Daniel and

0:40:56.160 --> 0:40:59.600
<v Speaker 1>Jorge dot com. Thanks for listening and remember that Daniel

0:40:59.640 --> 0:41:01.920
<v Speaker 1>and Jorge, Hey, Explain the Universe is a production of

0:41:02.080 --> 0:41:05.440
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0:41:05.600 --> 0:41:09.160
<v Speaker 1>visit the i heart Radio app, Apple Podcasts, or wherever

0:41:09.280 --> 0:41:16.320
<v Speaker 1>you listen to your favorite shows. Yeah