WEBVTT - How Earth-Like Planets Work

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<v Speaker 1>Welcome to you Stuff you should know from house Stuff

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<v Speaker 1>Works dot com. Hey, and welcome to the podcast. I'm

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<v Speaker 1>Josh Clark. There's Charles W. Chuck Bryant, There's Jerry AND's

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<v Speaker 1>the stuff you should know. Just a few geezas, what not?

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<v Speaker 1>Galizas very good? That was terrible, is what it was.

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<v Speaker 1>I read an article the other day on my people

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<v Speaker 1>find puns so offensive. It's very interesting. Oh yeah, I

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<v Speaker 1>know it is. Yeah, I'm sending my way, will you sure? Thanks,

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<v Speaker 1>You're welcome. Chuck. Yes, have you ever heard of an

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<v Speaker 1>exo planet? Yes? You have. Well that's all I got.

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<v Speaker 1>I'm down. I'm done with Kepler. Kepler is pretty awesome,

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<v Speaker 1>isn't it. Kepler is way awesome. Let's talk about Kepler.

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<v Speaker 1>What is it? Well, Kepler is a guess what you

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<v Speaker 1>call it? A program? Sure, the Kepler Project program. It's

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<v Speaker 1>a mission. Yes, it's all the mission. And since two

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<v Speaker 1>thousand nine they have Their task has been to survey

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<v Speaker 1>the sky in fact, um, well a small patch of

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<v Speaker 1>sky right now. And it's an outer space telescope. Yeah. Sure,

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<v Speaker 1>it's spine on people in the city park. No, no no,

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<v Speaker 1>they shot it out in a space. It's dressed in

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<v Speaker 1>like a silver um jumpsuit, so you can tell it's

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<v Speaker 1>a space telescope and not just like a regular one.

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<v Speaker 1>And uh yeah, it has a little twelve degree um

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<v Speaker 1>field of vision, and what it's doing is just looking

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<v Speaker 1>out into the cosmos in the Milky Way. Still. Yeah,

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<v Speaker 1>specifically near the constellations Sickness and Lira. For now. For now,

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<v Speaker 1>you gotta start somewhere, right, you only have twelve degrees.

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<v Speaker 1>You know, it's not the big ear. It's like a journey.

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<v Speaker 1>You have a thousand miles starts through the singles that. Uh. Basically,

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<v Speaker 1>what they're trying to do is see I think the

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<v Speaker 1>ultimate goal it's just to see what's out there. But

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<v Speaker 1>what they really secretly get giddy about and titter about

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<v Speaker 1>um late at night is finding exoplanets that are like

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<v Speaker 1>our own Earth. I know. I think the whole thing

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<v Speaker 1>was a straight up planet hunting mission. Well yeah, but

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<v Speaker 1>like I said, they're not just like we want to

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<v Speaker 1>find another Earth. They they're like, we want to see

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<v Speaker 1>what's out there because we don't know what's out there. Yes,

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<v Speaker 1>and they get really excited when it's not a big

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<v Speaker 1>giant ball of gas. So the Kepler mission actually the

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<v Speaker 1>first Kepler mission ended this past May because the Kepler

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<v Speaker 1>telescope I think ran out of battery power or something

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<v Speaker 1>like that to turn itself. But they started there. They're

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<v Speaker 1>ramping up the K two mission, which is actually this

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<v Speaker 1>is so amazing to me. I love this stuff. It's

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<v Speaker 1>they're going to use photons light from the Sun to

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<v Speaker 1>move it. Pretty amazing. And the photons are going to

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<v Speaker 1>move this thing called solar power to direct it and

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<v Speaker 1>look in different directions. It is very much so amazing. Um.

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<v Speaker 1>So the whole point is is defined planets. But really,

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<v Speaker 1>like you say, what they're looking for our planets that

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<v Speaker 1>fall within what's called the Goldilocks zone or the habitable zone.

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<v Speaker 1>And there's a couple a couple of different types of zones. Yeah,

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<v Speaker 1>if we're talking the Goldilocks zone, what we mean is

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<v Speaker 1>a planet that, um where there is water that doesn't

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<v Speaker 1>evaporate immediately or freeze. Well, yeah, that's one way to

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<v Speaker 1>put it. You know, flowing water would be great, so

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<v Speaker 1>CEO two that'd be awesome. So the whole Earth earthlike planets, right,

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<v Speaker 1>earthlike is what it what it comes down to, able

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<v Speaker 1>to sustain life, right, and the the whole thing. I've

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<v Speaker 1>read this really interesting article, Chuck, and it was I

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<v Speaker 1>think it was an aon magazine like it is one

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<v Speaker 1>of the greatest online magazines ever created, so interesting, everything

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<v Speaker 1>is so well written. It's just great. A on magazine,

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<v Speaker 1>aon magazine anyway. Um, the the person writing this article said,

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<v Speaker 1>what if our conception of life is really limited? And

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<v Speaker 1>when we think of life, we think of like um

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<v Speaker 1>genetic genetic molecules capable of self replicating, right, like us,

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<v Speaker 1>like life, like anything that that can make new copies

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<v Speaker 1>of itself, cellular reproduction. Right. So, um, what if there's

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<v Speaker 1>life has evolved in many, many other ways, not just

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<v Speaker 1>out an outter of space, but here on this planet,

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<v Speaker 1>Like we could be surrounded by life and not even

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<v Speaker 1>be aware of it because we're not thinking of it

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<v Speaker 1>that way. We're strictly looking for evidence of um DNA

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<v Speaker 1>based life. If life evolved in other ways and it's

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<v Speaker 1>we're surrounded by it, that's pretty neat. That's one of

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<v Speaker 1>those late night college conversations, if you know what I mean.

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<v Speaker 1>But with Kepler too, it's looking for planets that could

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<v Speaker 1>sustain a certain brand of life, which is the life

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<v Speaker 1>that we know and the whole thing is predicated on

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<v Speaker 1>the idea that you need water and liquid form to

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<v Speaker 1>be the foundation, the the sustaining foundation of life. And

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<v Speaker 1>so that's what that's what this habitable zone is. It's

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<v Speaker 1>a planet that is far enough away from the Sun

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<v Speaker 1>that it can um. It's it's surface water is not

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<v Speaker 1>going to boil away and turn it into um and

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<v Speaker 1>just just go into the atmosphere far away from its star. Right,

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<v Speaker 1>not necessarily the Sun. Right, it's star is what I mean.

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<v Speaker 1>It's version of our Sun, yes, yes, oh, and but

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<v Speaker 1>it's not so far away that it's not getting enough

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<v Speaker 1>heat so that it just frees. So it's within this

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<v Speaker 1>what's called the circumstellar habitable habitable zone. It's or it's

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<v Speaker 1>in this little distance like we are in our sun.

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<v Speaker 1>Our stars habitable zone are its circumstellar habitable zone, right,

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<v Speaker 1>And so it's looking for planets that um are surrounding

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<v Speaker 1>stars in that little band that's not so close that

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<v Speaker 1>it's too hot and not so far away that it's

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<v Speaker 1>too cold. It's just right. I love it. That's called

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<v Speaker 1>the Goldilocks zone. Yeah, that's the name for it. Um.

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<v Speaker 1>So there are they have the Kepler mission has returned

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<v Speaker 1>UM a lot of startling information like thousands, perhaps tens

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<v Speaker 1>of thousands or hundreds of thousands of planets maybe out there. Um,

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<v Speaker 1>in fact, probably are out there. I think it's forty

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<v Speaker 1>billion in the the Milky Way alone, is what estimates

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<v Speaker 1>are unbelievable in the Milky Way alone. Forty billion Earth

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<v Speaker 1>sized planets, not just all plants. Forty potentially Earth sized

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<v Speaker 1>planets in the Milky Way alone. Yeah. So, like I

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<v Speaker 1>was saying, UM, giant balls of gas are fun gas

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<v Speaker 1>giants like Saturn and Jupiter, they're needo torpedo. But UM,

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<v Speaker 1>as far as science really getting um getting their rocks off,

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<v Speaker 1>these Earth size planets are the ones that that that's

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<v Speaker 1>where the money is, you know, right, And when I

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<v Speaker 1>say money, I don't mean cash money, although if we

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<v Speaker 1>colonize them, I guess it could be cash money. But

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<v Speaker 1>the smaller planets, what they call terrestrial planets earthlike planets,

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<v Speaker 1>UM are terrestrial planets would be a great band name,

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<v Speaker 1>by the way, because they are They have heavy metal

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<v Speaker 1>cores and rocky mantle, and they have smaller orbits, shorter years,

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<v Speaker 1>they're close to the host star. All these things that

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<v Speaker 1>are Earth like, which could mean potentially you know something there,

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<v Speaker 1>so okay, so something living. You've got the circumstellar habitable zone,

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<v Speaker 1>which is not too close to the Sun or not

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<v Speaker 1>too close to the star, not too far away from

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<v Speaker 1>the star. But there's also um a larger habitable zone

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<v Speaker 1>that that kind of if you have that one, great,

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<v Speaker 1>But there's some other qualifications that a planet has to

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<v Speaker 1>hit to be considered habitable, and these are galactic habitable zones, right,

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<v Speaker 1>So part of that is that it has to have

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<v Speaker 1>a heavy metal core, like you say, it's got to

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<v Speaker 1>be terrestrial. It also has to um it can't be

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<v Speaker 1>tidally locked. Right. There's we found actually some planets out

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<v Speaker 1>there that fit the bill, except they are tidally locked

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<v Speaker 1>with their star, which means only one side and the

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<v Speaker 1>same side is always facing the sun, which means that

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<v Speaker 1>that is a very very hot body of water right

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<v Speaker 1>there that's facing the sun. And then on the back side,

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<v Speaker 1>the dark side, it's just completely frozen and since it's

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<v Speaker 1>not turning, the atmosphere is not being um kept around,

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<v Speaker 1>the planet is able to like migrate to like say

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<v Speaker 1>the dark side of the planet and just freeze there.

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<v Speaker 1>That's a great example of how you can have all

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<v Speaker 1>these other things. That planet might be in the habitable

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<v Speaker 1>zone for its star, but it falls out of the

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<v Speaker 1>category of a truly habitable planet because it's missing some

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<v Speaker 1>other factors, for example not being tidally locked. So that

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<v Speaker 1>would be the case with Gliza fight one G. So yes, okay,

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<v Speaker 1>So that is was discovered in two thousand ten, and

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<v Speaker 1>there's been a lot of back and forth between a

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<v Speaker 1>lot of different countries and scientists saying is it really there?

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<v Speaker 1>Is it not there? I think where it lands now is?

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<v Speaker 1>They are pretty sure it's there. Um. But with Glees

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<v Speaker 1>eight one g um, it faces uh the star at

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<v Speaker 1>all times, one side of it does, so it's tightly locked,

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<v Speaker 1>tightly locked. Um. Although it does orbit once every thirty

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<v Speaker 1>seven days, it keeps that face. So basically what they think,

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<v Speaker 1>because if there could be life there, you have what

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<v Speaker 1>they would call an eyeball Earth with a one part

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<v Speaker 1>of this planet having being liquid water right and the

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<v Speaker 1>rest of frozen, so like an eyeball in the middle

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<v Speaker 1>kind of neat. I think what keeps Glees of eight

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<v Speaker 1>one g in the news is the fact that it's

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<v Speaker 1>only twenty point five light years away. Um. And we'll

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<v Speaker 1>talk about some more of these, but a lot of

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<v Speaker 1>them are like over a thousand light years away. So

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<v Speaker 1>let's take a break real quick and we'll get back

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<v Speaker 1>to exoplanets right after this. So check you you touched

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<v Speaker 1>on something I think is very important before we go

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<v Speaker 1>any further there. People say, well, yeah it exists, or no,

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<v Speaker 1>it doesn't exist. And there's a lot of back and

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<v Speaker 1>forth in the scientific community. And the reason is, is

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<v Speaker 1>the as as high powered and awesome as the Kepler

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<v Speaker 1>telescope is it really is. It doesn't look at a

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<v Speaker 1>star and say, oh, look at that planet. That's a

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<v Speaker 1>fine looking planet right there. It looks like, oh yeah,

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<v Speaker 1>I can see water on there and wall like a

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<v Speaker 1>giant pterodactyl like a monkey head. Yes it is. No,

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<v Speaker 1>it can't see these kind of things, right. So there's

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<v Speaker 1>different techniques that are used for hunting planets exoplanets, um,

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<v Speaker 1>that use deduction in a lot of ways in concert

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<v Speaker 1>with these telescopes right to surmise the existence of planets.

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<v Speaker 1>So um, there's three main techniques that even these telescopes

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<v Speaker 1>us Like the Kepler telescope is it uses a photometer

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<v Speaker 1>which senses light, right, and it'll look at a star,

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<v Speaker 1>are and it'll just keep looking at the star, looking

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<v Speaker 1>at the star. It's got a really good Uh, something

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<v Speaker 1>weird just happened at the star got dim and then

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<v Speaker 1>it went back to normal light. And what just happened

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<v Speaker 1>was probably a planet orbited in between the telescope and

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<v Speaker 1>the star, which dim the light of the star. That's right.

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<v Speaker 1>They called that a transit and that technique is called

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<v Speaker 1>the transit method. And so they, like you said, they

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<v Speaker 1>use that photometer and um, if they see that dim

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<v Speaker 1>that's a lead in the right direction. Yeah, and now

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<v Speaker 1>it doesn't prove anything, no, so that that that planet

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<v Speaker 1>becomes a candidate planet. So they go back and they

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<v Speaker 1>look at it. And if they say, use a different technique,

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<v Speaker 1>or if they um, if they come up with the

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<v Speaker 1>same data using that same technique again and again, then

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<v Speaker 1>most likely that planet does exist and it becomes a right,

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<v Speaker 1>it becomes a confirmed planet. So it goes from a

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<v Speaker 1>candidate planet to a confirmed planet. Um. And there's a

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<v Speaker 1>lot of criticism in this side actific community because when

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<v Speaker 1>a candidate planet is found, it is far from being

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<v Speaker 1>proven as existing. But um, it's very frequently rushed out

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<v Speaker 1>to the media, which treats it like a new planet's

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<v Speaker 1>been discovered and we know all about it, when we

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<v Speaker 1>really don't even know for a fact it exists, And

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<v Speaker 1>very infrequently the science behind having to deduce its existence

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<v Speaker 1>is explained in in the in the articles that are

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<v Speaker 1>written about them. So it just gets rushed to press

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<v Speaker 1>a little too premisuarly to keep that public interest up,

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<v Speaker 1>you know. Yeah, but it wouldn't hurt to also educate

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<v Speaker 1>the public at the same time. So a lot of

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<v Speaker 1>people say, oh, well that we just discovered a new

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<v Speaker 1>planet where it's still a candidate planet and it doesn't

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<v Speaker 1>we don't necessarily know it exists. It's a good point, um.

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<v Speaker 1>So that the transit method is is the one where

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<v Speaker 1>the light pulses, the star pulses, well, it dims because

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<v Speaker 1>the planet comes in between the telescope and the yeah star.

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<v Speaker 1>Then you have the wobble method, which is pretty neat

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<v Speaker 1>in itself. Um. It looks for changes in relative velocity

0:14:07.720 --> 0:14:12.200
<v Speaker 1>caused by the gravitational pull of another nearby planet. So

0:14:12.360 --> 0:14:14.880
<v Speaker 1>basically what happens is they use the spectrum of light

0:14:14.920 --> 0:14:18.720
<v Speaker 1>for this one and they analyze that spectrum around this

0:14:19.040 --> 0:14:22.200
<v Speaker 1>uh what they think could be a planet. It planet

0:14:22.240 --> 0:14:27.920
<v Speaker 1>it planet it can planet it so, thank you. So

0:14:27.960 --> 0:14:30.400
<v Speaker 1>what happens is if it is being pulled by another planet,

0:14:30.400 --> 0:14:33.000
<v Speaker 1>when it surges towards Earth and then away, it causes

0:14:33.080 --> 0:14:37.120
<v Speaker 1>variations in that light spectrum. So when it comes towards Earth, um,

0:14:37.200 --> 0:14:39.560
<v Speaker 1>it shortens a wavelength and you see a blue spectrum

0:14:39.600 --> 0:14:42.720
<v Speaker 1>more um. When it goes away from Earth, it lengthens

0:14:42.760 --> 0:14:45.440
<v Speaker 1>and you see red more So it's almost like a

0:14:45.520 --> 0:14:50.280
<v Speaker 1>color pulse. Uh. And that is the Wobble method. So

0:14:50.400 --> 0:14:55.520
<v Speaker 1>that's number two. And that's the Doppler effect. Uh is it? Yeah,

0:14:55.640 --> 0:14:59.320
<v Speaker 1>but with light instead of sound. But the Compler effect

0:14:59.400 --> 0:15:02.320
<v Speaker 1>is only sound. No, it's any kind of wavelength. Oh

0:15:02.360 --> 0:15:04.840
<v Speaker 1>I thought the Doppler effect was strictly sound. No, it's

0:15:04.880 --> 0:15:09.120
<v Speaker 1>it's it's any I'm telling you. It's the thing that

0:15:09.200 --> 0:15:15.720
<v Speaker 1>links bats to earthlike planets, to Doppler to a passing ambulance. Yes, man,

0:15:15.720 --> 0:15:19.120
<v Speaker 1>I'm so psyched about the Doppler effect. Uh. And you

0:15:19.160 --> 0:15:20.880
<v Speaker 1>want to go ahead and hit us up with that

0:15:20.960 --> 0:15:24.560
<v Speaker 1>last one micro lensing that's pretty neat too, yes. So, um,

0:15:24.680 --> 0:15:28.680
<v Speaker 1>when you have a star and another star passes, if

0:15:28.680 --> 0:15:31.040
<v Speaker 1>you're looking at a star with say if um, like

0:15:31.080 --> 0:15:34.760
<v Speaker 1>the the Kepler telescope, which the Kepler telescope strictly uses

0:15:34.760 --> 0:15:39.360
<v Speaker 1>the transit method from what I understands, So you have

0:15:39.400 --> 0:15:43.520
<v Speaker 1>another telescope that that is more open minded. Yeah. UM,

0:15:43.560 --> 0:15:46.680
<v Speaker 1>And you're looking at a star and another star comes

0:15:46.720 --> 0:15:50.160
<v Speaker 1>in between you and the star. You're looking at that

0:15:50.360 --> 0:15:53.400
<v Speaker 1>star that's in the foreground, that's in between you and

0:15:53.440 --> 0:15:57.960
<v Speaker 1>the original star. UM actually takes the light and acts

0:15:58.000 --> 0:16:01.480
<v Speaker 1>as a kind of a magnifying lens and intensifies the

0:16:01.560 --> 0:16:04.320
<v Speaker 1>light of the star behind it thanks to its gravity.

0:16:04.400 --> 0:16:08.720
<v Speaker 1>This is called micro lensing. Right. If a planet falls

0:16:08.760 --> 0:16:12.200
<v Speaker 1>into that that's an orbit around that other star falls

0:16:12.360 --> 0:16:16.240
<v Speaker 1>in line with this, it takes that um that micro

0:16:16.360 --> 0:16:20.040
<v Speaker 1>lensing effect and amplifies it even further. And then you

0:16:20.080 --> 0:16:23.960
<v Speaker 1>can calculate, based on the amplification of the micro lensing effect,

0:16:24.520 --> 0:16:27.520
<v Speaker 1>the mass of all of the stars and this new

0:16:27.560 --> 0:16:31.440
<v Speaker 1>mystery planet that just came into into line with this orbit. UM,

0:16:31.560 --> 0:16:35.520
<v Speaker 1>And they use that mind blowingly enough to deduce the

0:16:36.360 --> 0:16:39.960
<v Speaker 1>presence of planets around stars too. So you've got these

0:16:39.960 --> 0:16:44.320
<v Speaker 1>three methods and all of them though again it's really

0:16:44.480 --> 0:16:48.200
<v Speaker 1>important to remember this, all of these used deduction, Like

0:16:48.440 --> 0:16:52.720
<v Speaker 1>none of these planets have been visually observed. They are

0:16:52.840 --> 0:16:58.840
<v Speaker 1>all deduced to exist based on um, the mathematical evidence

0:16:59.560 --> 0:17:02.280
<v Speaker 1>that there's something going on here, like that this light

0:17:02.360 --> 0:17:05.879
<v Speaker 1>is dimming, this color is changing, or the light is

0:17:05.960 --> 0:17:08.800
<v Speaker 1>being amplified by something, and it all has to do

0:17:08.840 --> 0:17:12.080
<v Speaker 1>with mass and gravity. It's pretty amazing. Yeah, alright, so

0:17:12.119 --> 0:17:13.959
<v Speaker 1>we'll take a little break here and come back and

0:17:13.960 --> 0:17:18.040
<v Speaker 1>talk about some of these exo planets and if there

0:17:18.040 --> 0:17:40.000
<v Speaker 1>are people living there, there aren't so chuck. Remember we

0:17:40.040 --> 0:17:42.920
<v Speaker 1>mentioned the transit method. You can also use these things

0:17:42.960 --> 0:17:46.119
<v Speaker 1>to deduce even more stuff about these planets once you

0:17:46.200 --> 0:17:51.920
<v Speaker 1>confirm they exist. Personality, right, it's signed like kind of things. Um.

0:17:51.960 --> 0:17:59.480
<v Speaker 1>There's something called transit spectroscopy which uses the apparently the

0:17:59.560 --> 0:18:03.560
<v Speaker 1>atmosp fear of a planet leaves a certain kind of

0:18:03.680 --> 0:18:08.399
<v Speaker 1>mark on the light that it messes with in the

0:18:08.440 --> 0:18:11.159
<v Speaker 1>star that you're looking at. So not only are you

0:18:11.280 --> 0:18:14.720
<v Speaker 1>deducing that the planets there, you're deducing by the effect

0:18:15.040 --> 0:18:17.639
<v Speaker 1>that that planet has on the light the type of

0:18:17.680 --> 0:18:21.880
<v Speaker 1>atmosphere it has as well. So pretty amazing, right, So

0:18:22.280 --> 0:18:25.680
<v Speaker 1>once they figure out that yes, the planet is likely there,

0:18:25.880 --> 0:18:28.480
<v Speaker 1>they go back and look at it and the planet

0:18:28.480 --> 0:18:31.200
<v Speaker 1>goes from a candidate to a confirmed planet, and the

0:18:31.320 --> 0:18:36.720
<v Speaker 1>Kepler Um came up with one thousand and thirty confirmed exoplanets,

0:18:36.760 --> 0:18:40.359
<v Speaker 1>twelve of which are in a Goldilocks zone. Right. Um,

0:18:40.400 --> 0:18:43.880
<v Speaker 1>they really start going to town studying this planet and

0:18:43.920 --> 0:18:46.280
<v Speaker 1>figuring out what its atmosphere is like, where it is

0:18:46.280 --> 0:18:49.480
<v Speaker 1>in relation to the star, what the temperature is, and

0:18:49.520 --> 0:18:52.720
<v Speaker 1>they can tell some pretty amazing stuff about an exo

0:18:52.760 --> 0:18:57.080
<v Speaker 1>planet just from all of these deductions. Yeah, Like, uh,

0:18:57.119 --> 0:18:58.879
<v Speaker 1>I guess let's just talk about a couple of these

0:18:59.040 --> 0:19:03.600
<v Speaker 1>UM the the Gliza. Uh I guess it's a group

0:19:03.640 --> 0:19:08.359
<v Speaker 1>because there are several glazes. There's a gliza. So each

0:19:08.359 --> 0:19:12.160
<v Speaker 1>one of these UM exoplanets is named after the star

0:19:12.320 --> 0:19:15.840
<v Speaker 1>that it orbits. Yeah. So so the Glaza Gleaz is

0:19:15.880 --> 0:19:20.200
<v Speaker 1>a star. Yeah, and it has several potential habitable planets

0:19:20.240 --> 0:19:23.600
<v Speaker 1>around it. We already talked a little bit about five

0:19:23.680 --> 0:19:26.760
<v Speaker 1>eight one G, but there's also a five eight one C.

0:19:27.400 --> 0:19:30.280
<v Speaker 1>It is twelve thousand miles in diameter UM, which is

0:19:30.320 --> 0:19:34.280
<v Speaker 1>not too much bigger than Earth um, and makes one

0:19:34.320 --> 0:19:39.080
<v Speaker 1>complete revolution in thirteen Earth days, which means it's too hot,

0:19:39.480 --> 0:19:42.719
<v Speaker 1>but it balances that out because it has a surface

0:19:42.720 --> 0:19:48.439
<v Speaker 1>temperature one uh that of our Sun, which means potentially,

0:19:48.640 --> 0:19:52.080
<v Speaker 1>and again this is all speculation. Potentially the temperature range

0:19:52.080 --> 0:19:54.560
<v Speaker 1>on the surface of five eight one C could be

0:19:55.000 --> 0:19:58.720
<v Speaker 1>thirty two degrees to two degrees fahrenheit, such as in

0:19:58.760 --> 0:20:01.919
<v Speaker 1>the wheelhouse. It isn the wheelhouse. I think further study

0:20:02.000 --> 0:20:05.760
<v Speaker 1>has kind of discarded the idea that um gleeza vibe

0:20:05.800 --> 0:20:10.080
<v Speaker 1>eight one c is habitable. Yeah, it's pretty quick right

0:20:10.320 --> 0:20:13.199
<v Speaker 1>as far as breaking news goes. But you raise a

0:20:13.280 --> 0:20:17.439
<v Speaker 1>really good point that if this thing has a revolution

0:20:18.160 --> 0:20:22.560
<v Speaker 1>a year that's thirteen days long, the there's no part

0:20:22.600 --> 0:20:25.080
<v Speaker 1>of the planet that's going to get cool enough to

0:20:25.280 --> 0:20:30.119
<v Speaker 1>even things out. It's gonna just stay too hot. And conversely,

0:20:30.200 --> 0:20:33.960
<v Speaker 1>if the thing has a year that lasts too long,

0:20:34.320 --> 0:20:36.840
<v Speaker 1>it's gonna it's not gonna get hot enough. It's gonna

0:20:36.880 --> 0:20:43.040
<v Speaker 1>stay cool. So that's another galactic habitable zone factor. Well,

0:20:43.160 --> 0:20:45.679
<v Speaker 1>I love him, man, keep them coming. I know. I

0:20:45.760 --> 0:20:48.080
<v Speaker 1>basically went and looked today. I was like, what are

0:20:48.080 --> 0:20:52.040
<v Speaker 1>the most likely habitable exoplanets? And an article from a

0:20:52.119 --> 0:20:55.040
<v Speaker 1>year ago has a top five that's different from an

0:20:55.080 --> 0:20:58.280
<v Speaker 1>article now, Like that's how quickly things change, right, Well,

0:20:58.320 --> 0:21:02.240
<v Speaker 1>I mean these things were all just basically theoretical, like

0:21:02.280 --> 0:21:05.520
<v Speaker 1>we assumed that, you know, a star would have planets

0:21:06.440 --> 0:21:09.080
<v Speaker 1>orbiting it, but it wasn't until the Coupler mission within

0:21:09.119 --> 0:21:10.639
<v Speaker 1>the last like ten years or so, I think it

0:21:10.680 --> 0:21:18.320
<v Speaker 1>was from the Arecibo telescope was the first confirmed exo

0:21:18.320 --> 0:21:22.560
<v Speaker 1>planet to be detected. And that was but once Kepler

0:21:22.720 --> 0:21:26.080
<v Speaker 1>started going, it's they started to come like hard and fast.

0:21:26.720 --> 0:21:29.879
<v Speaker 1>And once they started and people started rushing to press,

0:21:30.520 --> 0:21:32.919
<v Speaker 1>then the science is having to retract them now and

0:21:33.000 --> 0:21:36.160
<v Speaker 1>things are going from yeah, well, well there's a new

0:21:36.160 --> 0:21:38.200
<v Speaker 1>exit planet that we could just travel to now if

0:21:38.200 --> 0:21:42.040
<v Speaker 1>we wanted to to. This thing actually doesn't exist or

0:21:42.160 --> 0:21:46.359
<v Speaker 1>it's not really habitable. I looked. The most recent one

0:21:46.400 --> 0:21:48.840
<v Speaker 1>I found was from like three months ago and May

0:21:48.880 --> 0:21:52.720
<v Speaker 1>of this year, and they say, I believe this was

0:21:52.760 --> 0:21:55.720
<v Speaker 1>from space dot Com said that Kepler forty eight B

0:21:56.640 --> 0:22:00.560
<v Speaker 1>is the most earthlike planet yet that we've discovered. Um

0:22:00.560 --> 0:22:03.040
<v Speaker 1>it orbits a distant star in the constellation of Lira,

0:22:03.200 --> 0:22:08.960
<v Speaker 1>which is where Kepler is looking. Which eight B. It

0:22:08.960 --> 0:22:11.160
<v Speaker 1>gets really confusing. They need to start naming these things,

0:22:11.320 --> 0:22:14.040
<v Speaker 1>they do, you know, So four thirty eight B is

0:22:14.160 --> 0:22:18.240
<v Speaker 1>a little bit bigger than Earth, uh more heat than

0:22:18.359 --> 0:22:22.600
<v Speaker 1>Earth than what we received from the Sun though. UH.

0:22:22.680 --> 0:22:25.800
<v Speaker 1>It's small though, which means it is UM just because

0:22:25.800 --> 0:22:29.200
<v Speaker 1>it's twelve percent larger means it's seventy has a seventy

0:22:29.640 --> 0:22:34.000
<v Speaker 1>chance of being rocky like Earth. UH. It is four

0:22:34.240 --> 0:22:36.320
<v Speaker 1>d and seventy light years away, which is not too

0:22:36.320 --> 0:22:39.240
<v Speaker 1>bad considering some of these are thousands and thousands of

0:22:39.320 --> 0:22:42.360
<v Speaker 1>light years away. UH completes an orbit around its star

0:22:42.480 --> 0:22:44.959
<v Speaker 1>every thirty five days, which is about ten times as

0:22:45.000 --> 0:22:51.320
<v Speaker 1>fast as Earth. UM. And basically the Harvard Smithsonian Center

0:22:51.400 --> 0:22:56.080
<v Speaker 1>of astro UH for Astrophysics said that UM, they announced

0:22:56.119 --> 0:22:59.280
<v Speaker 1>this one along with seven other planets UM in the

0:22:59.359 --> 0:23:03.840
<v Speaker 1>same habit of ball zone. So decent chance. But UM,

0:23:03.880 --> 0:23:06.720
<v Speaker 1>like I said this this, By the time this comes out,

0:23:06.800 --> 0:23:11.680
<v Speaker 1>this may be old news and debunked. Who knows. UM.

0:23:11.840 --> 0:23:14.440
<v Speaker 1>There's another one that I think they discovered even more recently,

0:23:14.480 --> 0:23:18.560
<v Speaker 1>which is Kepler fifty two B and it's light years

0:23:18.600 --> 0:23:22.640
<v Speaker 1>away UM, and it is an earthlike planet. I think

0:23:22.720 --> 0:23:27.480
<v Speaker 1>it's UM like uh si larger in diameter than the

0:23:27.520 --> 0:23:31.879
<v Speaker 1>Earth UM, but it's still Earth like. It is a

0:23:31.880 --> 0:23:35.879
<v Speaker 1>super Earth, yes, UM. No, that automatically qualifies it as

0:23:35.880 --> 0:23:38.960
<v Speaker 1>a super Earth. So it's it's Earth size, but it's

0:23:38.960 --> 0:23:41.280
<v Speaker 1>not so big that it's like a gas giant. It's

0:23:41.359 --> 0:23:45.720
<v Speaker 1>terrestrial likely um. And it's in the Goldilocks zone for

0:23:45.920 --> 0:23:50.960
<v Speaker 1>its star um, and they're pretty excited about it. Actually.

0:23:51.200 --> 0:23:54.680
<v Speaker 1>I think the it has a mass that's five or

0:23:54.760 --> 0:23:59.359
<v Speaker 1>six times Earth's and so you would be you you

0:23:59.359 --> 0:24:02.679
<v Speaker 1>would feel about double your weight or you would weigh double.

0:24:03.280 --> 0:24:06.159
<v Speaker 1>Well you do here. But they think that if we

0:24:06.200 --> 0:24:10.040
<v Speaker 1>did sink colonists there, their bodies would adapt to be

0:24:10.080 --> 0:24:13.440
<v Speaker 1>like working out all the time. Um, but you would

0:24:13.480 --> 0:24:15.960
<v Speaker 1>become super strong, and if you came back to Earth

0:24:16.200 --> 0:24:19.119
<v Speaker 1>you could just beat everybody up. Interesting because you'd be

0:24:19.119 --> 0:24:22.480
<v Speaker 1>twice as strong. Pretty cool, huh, it'd be great. That's

0:24:22.520 --> 0:24:25.040
<v Speaker 1>the point of space travel is to find ways to

0:24:25.200 --> 0:24:28.160
<v Speaker 1>just walk around and come back and beat everybody up

0:24:28.160 --> 0:24:31.120
<v Speaker 1>on Earth. It's a bully program. That is a good question, though,

0:24:31.160 --> 0:24:33.680
<v Speaker 1>what's the point of all this? If these things are

0:24:33.800 --> 0:24:40.159
<v Speaker 1>light years away? What's what's the point? Um geez, just

0:24:40.280 --> 0:24:44.159
<v Speaker 1>to keep looking beyond? I mean, isn't that exploration the

0:24:44.200 --> 0:24:47.760
<v Speaker 1>whole point? I guess, because it's not like we could

0:24:48.000 --> 0:24:50.359
<v Speaker 1>colonize any of these places, well not now. But I

0:24:50.400 --> 0:24:53.400
<v Speaker 1>think that some people have an eye toward that that

0:24:53.640 --> 0:25:00.200
<v Speaker 1>the if we ever do figure out interstellar travel, um,

0:25:00.240 --> 0:25:02.360
<v Speaker 1>it would be really good to know where we could

0:25:02.400 --> 0:25:06.280
<v Speaker 1>go and take off our helmets and breathe. Yeah, I

0:25:06.359 --> 0:25:08.080
<v Speaker 1>think of it more in the opposite way, like you

0:25:08.119 --> 0:25:10.520
<v Speaker 1>can't stop doing stuff like this. No, I agree with

0:25:10.520 --> 0:25:12.320
<v Speaker 1>because then you've just I don't know, then you're just

0:25:12.840 --> 0:25:16.359
<v Speaker 1>you've given up. You're an isolationist. Yeah, you're adults living

0:25:16.400 --> 0:25:20.280
<v Speaker 1>on Earth and o'tre I'm just gonna die anyway. Well,

0:25:20.359 --> 0:25:23.760
<v Speaker 1>the other thing that they're looking for that that exoplanets

0:25:24.280 --> 0:25:26.960
<v Speaker 1>searches bring into the fold is steady the search for

0:25:27.119 --> 0:25:31.719
<v Speaker 1>estratra extra extraterrestrial intelligence or just the search for life

0:25:32.160 --> 0:25:36.760
<v Speaker 1>um elsewhere. And again, if you're looking at planets that

0:25:36.800 --> 0:25:40.719
<v Speaker 1>can sustain humans, they could conceivably sustain other types of

0:25:40.760 --> 0:25:44.639
<v Speaker 1>life as well. So we're hedging our bets for the future.

0:25:45.000 --> 0:25:47.359
<v Speaker 1>We're also looking to see if we're alone out there

0:25:47.480 --> 0:25:49.400
<v Speaker 1>or not. Imagine there are people out there that thinks

0:25:49.440 --> 0:25:51.480
<v Speaker 1>there's a big waste of time and money though probably

0:25:51.600 --> 0:25:58.800
<v Speaker 1>you know, whatevs. The adults, the isolationists, you got anything

0:25:58.800 --> 0:26:01.239
<v Speaker 1>else right now? Oh? This is uh, this is good.

0:26:01.280 --> 0:26:03.159
<v Speaker 1>Stuff is a little heady and it's such a rapidly

0:26:03.240 --> 0:26:05.800
<v Speaker 1>changing thing. Yeah, we could revisit this easily. Yeah, I

0:26:05.800 --> 0:26:10.080
<v Speaker 1>mean this will be outdated in six months. But tops, Hey,

0:26:10.600 --> 0:26:13.560
<v Speaker 1>we we like to do these topical things every now

0:26:13.600 --> 0:26:17.600
<v Speaker 1>and then. Uh, if you want to know more about

0:26:18.000 --> 0:26:20.560
<v Speaker 1>earth like planets, you can type that into the search

0:26:20.640 --> 0:26:23.640
<v Speaker 1>part how stuff forks dot com. And since I said

0:26:23.640 --> 0:26:28.880
<v Speaker 1>search parts, time for listener mail. I'm gonna call this,

0:26:29.320 --> 0:26:35.320
<v Speaker 1>uh road rage and no not road rage. Citizens arrest. Okay,

0:26:35.600 --> 0:26:39.080
<v Speaker 1>there's kind of a difference, big difference. Guys. Have a

0:26:39.119 --> 0:26:41.480
<v Speaker 1>citizens rest story. Um from two thousand one. I was

0:26:41.480 --> 0:26:44.359
<v Speaker 1>a naive nineteen year old behind the wheel of the

0:26:44.359 --> 0:26:47.320
<v Speaker 1>first car ever bought myself when I was rear ended. Um.

0:26:47.359 --> 0:26:48.960
<v Speaker 1>It was two thousand one, so we didn't have cell

0:26:49.000 --> 0:26:51.840
<v Speaker 1>phones and there was no phone booth nearby, so we

0:26:51.840 --> 0:26:54.239
<v Speaker 1>could not call the highway patrol or police. The other

0:26:54.320 --> 0:26:56.760
<v Speaker 1>driver had insurance, but did not have a valid driver's license,

0:26:56.800 --> 0:26:59.119
<v Speaker 1>only an expired one. Later found out he obtained a

0:26:59.160 --> 0:27:02.520
<v Speaker 1>license during a window time when the Governator of California

0:27:02.880 --> 0:27:06.159
<v Speaker 1>announced him to be issued to undocumented persons who had

0:27:06.160 --> 0:27:09.480
<v Speaker 1>emigrated without completing all their legal steps yet. So basically

0:27:09.520 --> 0:27:11.679
<v Speaker 1>this guy got in a window had it license at

0:27:11.680 --> 0:27:14.680
<v Speaker 1>one point it was expired. I got my crunch car

0:27:14.720 --> 0:27:17.440
<v Speaker 1>home that afternoon and, at the suggestion of my parents,

0:27:17.480 --> 0:27:20.160
<v Speaker 1>called the local cops to file a police report since

0:27:20.200 --> 0:27:21.800
<v Speaker 1>we couldn't do one at the scene in the accident.

0:27:22.119 --> 0:27:23.960
<v Speaker 1>The officer that came out to my home was the

0:27:24.000 --> 0:27:28.399
<v Speaker 1>most militant, sour woman in law enforcement that I have

0:27:28.480 --> 0:27:33.440
<v Speaker 1>ever had the pleasure or displeasure I'm encountering. She impatiently

0:27:33.480 --> 0:27:36.520
<v Speaker 1>asked the questions and took notes, all while sneering at me.

0:27:36.800 --> 0:27:38.280
<v Speaker 1>When I got to the part about the other driver

0:27:38.480 --> 0:27:41.760
<v Speaker 1>having expired license, she literally yelled at me for not

0:27:41.840 --> 0:27:45.320
<v Speaker 1>placing him under citizens arrest. Mind you, this was a

0:27:45.320 --> 0:27:48.480
<v Speaker 1>car full of men. I was a nineteen year old

0:27:48.480 --> 0:27:51.560
<v Speaker 1>girl who weighed a hundred pounds and was four ft ten,

0:27:52.000 --> 0:27:54.760
<v Speaker 1>and she chastised me for not placing an entire car

0:27:54.840 --> 0:27:57.800
<v Speaker 1>full of grown men under citizens arrest for driving on

0:27:57.840 --> 0:28:01.760
<v Speaker 1>an expired license. Uh. She went on about how many

0:28:01.840 --> 0:28:05.280
<v Speaker 1>undocumented persons have criminal records and can be very dangerous,

0:28:05.280 --> 0:28:07.120
<v Speaker 1>and this would have been a good opportunity to get

0:28:07.160 --> 0:28:12.160
<v Speaker 1>them deported. Well, this is an explosive listener mail. Yeah,

0:28:12.520 --> 0:28:15.159
<v Speaker 1>or a car full of potentially dangerous men. Maybe you

0:28:15.160 --> 0:28:17.800
<v Speaker 1>should not try and place under citizens rests would be

0:28:17.840 --> 0:28:20.720
<v Speaker 1>my idea. At this point, my father had enough of

0:28:20.760 --> 0:28:23.000
<v Speaker 1>her shenanigans and asked her to leave. That was the

0:28:23.040 --> 0:28:25.240
<v Speaker 1>end of that, but we still chuckled this day over

0:28:25.280 --> 0:28:28.560
<v Speaker 1>the absurdity of her suggestion. Uh. And she goes on

0:28:28.640 --> 0:28:30.760
<v Speaker 1>to say that the guy in the car and the

0:28:30.840 --> 0:28:33.159
<v Speaker 1>dudes were very nice, and the exchange insurance and it

0:28:33.200 --> 0:28:36.520
<v Speaker 1>wasn't like a bad scene or anything. So, um, it

0:28:36.640 --> 0:28:42.200
<v Speaker 1>just sounds like this officer was not a very nice persons. Like, yeah,

0:28:42.240 --> 0:28:45.520
<v Speaker 1>and every cop that we heard from after citizen arrest

0:28:45.520 --> 0:28:50.080
<v Speaker 1>said don't do it, and this lady saying, now try it.

0:28:50.320 --> 0:28:52.720
<v Speaker 1>A little four ft tin lady shot on a car

0:28:52.760 --> 0:28:55.480
<v Speaker 1>full of men, and um, all of sudden, you want

0:28:55.480 --> 0:28:57.160
<v Speaker 1>to point out that I forgot that one of the

0:28:57.200 --> 0:29:01.040
<v Speaker 1>most legendary Remember I was trying to think of famous

0:29:01.040 --> 0:29:06.960
<v Speaker 1>citizens arrests. The most legendary of all time is, uh,

0:29:07.280 --> 0:29:11.000
<v Speaker 1>the night Stalker. Oh yeah, he got arrested by a

0:29:11.040 --> 0:29:14.479
<v Speaker 1>citizen by citizens Like he was checked the knight Stalker

0:29:14.520 --> 0:29:19.240
<v Speaker 1>did no not him? Richard Richard Ramirez. He was recognized

0:29:19.240 --> 0:29:20.880
<v Speaker 1>out on this because they eventually found out who he

0:29:20.920 --> 0:29:23.600
<v Speaker 1>was and blasted his face out everywhere in this group

0:29:23.640 --> 0:29:27.400
<v Speaker 1>of Hispanic women saw him and started screaming in uh

0:29:27.440 --> 0:29:30.640
<v Speaker 1>in Spanish like night stalker, night stalker. And he was

0:29:30.920 --> 0:29:35.080
<v Speaker 1>gang piled by like fifteen people and cops had to

0:29:35.080 --> 0:29:37.680
<v Speaker 1>pull people off. He was almost beaten to death. So

0:29:38.600 --> 0:29:40.959
<v Speaker 1>I guess you would call that a citizen's arrest. I

0:29:40.960 --> 0:29:43.640
<v Speaker 1>would call that, yes, yeah, like a good one, yeah,

0:29:43.840 --> 0:29:46.320
<v Speaker 1>an effective one. Yeah, well they got a serial killer.

0:29:46.360 --> 0:29:49.080
<v Speaker 1>You always gotta feel good about that citizens arrest. Yeah.

0:29:49.080 --> 0:29:50.840
<v Speaker 1>I fell down the rabbit hole of reading all about

0:29:50.840 --> 0:29:54.960
<v Speaker 1>that guy recently. Yeah. Yeah, man, what a crazy time

0:29:54.960 --> 0:29:56.520
<v Speaker 1>to be living in l A. I bet people were

0:29:57.160 --> 0:29:58.880
<v Speaker 1>because there was no rhyme or reason and it was

0:29:58.960 --> 0:30:01.720
<v Speaker 1>like one night, then two nights later, than three nights later,

0:30:01.760 --> 0:30:05.400
<v Speaker 1>than two nights later, and just crazy, awful, awful things.

0:30:05.840 --> 0:30:08.560
<v Speaker 1>That was like The Zodiac, one of my favorite movies

0:30:08.600 --> 0:30:10.880
<v Speaker 1>of all times. Zodiac. It's a great movie. That was

0:30:10.920 --> 0:30:13.960
<v Speaker 1>a great one. But then you read ramirez is background

0:30:14.600 --> 0:30:18.880
<v Speaker 1>and it's like abusive father, Um, this crazy uncle that

0:30:18.920 --> 0:30:23.160
<v Speaker 1>was in Vietnam that showed him pictures of like decapitated bodies,

0:30:23.400 --> 0:30:26.200
<v Speaker 1>and you know, he was dropped on his head like

0:30:26.240 --> 0:30:29.880
<v Speaker 1>three times, like he had a whole list of things

0:30:30.440 --> 0:30:33.560
<v Speaker 1>that's like how to become a serial killer. And uh

0:30:33.760 --> 0:30:37.240
<v Speaker 1>so it's two times you're fine, that third time you

0:30:37.320 --> 0:30:39.720
<v Speaker 1>get dropped on your head, that's big. And let's not

0:30:39.760 --> 0:30:41.600
<v Speaker 1>say every head trauma leads to that, but they think

0:30:41.640 --> 0:30:43.680
<v Speaker 1>it could have something to do in cases like that.

0:30:44.320 --> 0:30:48.040
<v Speaker 1>It was just it was very sad and fascinating. Yep,

0:30:48.680 --> 0:30:53.360
<v Speaker 1>do you have a particular article you recommend on the dude? Uh? No, Okay,

0:30:53.800 --> 0:30:57.080
<v Speaker 1>well look, come up. Yeah, uh if you want to

0:30:57.160 --> 0:31:01.600
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0:31:01.680 --> 0:31:03.920
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0:31:05.320 --> 0:31:08.400
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