WEBVTT - Lab 006: Starchella

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<v Speaker 1>All right, everybody, it's the mid term. It is the

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<v Speaker 1>midterms that we're halfway through the season. Yep, we're at

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<v Speaker 1>episode six. How do y'all feel? I hope y'all have

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<v Speaker 1>been studying and are ready for this quiz we're about

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<v Speaker 1>to post. Don't worry, there'll be a curve. Anybody took

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<v Speaker 1>a class with me, you will know that it's not

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<v Speaker 1>how it goes. I'm TT and I'm Zachiah and from

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<v Speaker 1>Spotify Studios. This is Dope Labs. Okay, so did you

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<v Speaker 1>watch Homecoming? Did I how many times have you watched it? Right?

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<v Speaker 1>I've only watched it one time, but I'm planning on

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<v Speaker 1>watching it after this because I feel like every morning

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<v Speaker 1>I need to I need to wake up two hours

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<v Speaker 1>early so I can start Homecoming and really get my

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<v Speaker 1>mind right for it'll be everyone's daily devotional. That's exactly

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<v Speaker 1>what it's like. I mean, she's been stre on y'all's next, okay,

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<v Speaker 1>but she's really saying like, bow down for real, Yeah,

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<v Speaker 1>you have no choice. She showed us her not only

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<v Speaker 1>that she is, you know, at the top of her

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<v Speaker 1>game as far as vocals and entertaining, but also that

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<v Speaker 1>she has the work ethic of there's not really nothing

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<v Speaker 1>to compare her to she You have to have the

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<v Speaker 1>Beyonce work ethic. That's the that's the new gold standard, honestly,

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<v Speaker 1>Like Beyonce said that basically all she was eating was

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<v Speaker 1>air molecules and eight counts for a year and a half.

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<v Speaker 1>I don't understand. She was like, I rehears four months

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<v Speaker 1>with the band and then four months with the dancers,

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<v Speaker 1>and I was like, huh what, I don't do anything

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<v Speaker 1>with that much advanced notice. I couldn't even get that prepared.

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<v Speaker 1>If I wanted to write like something's happening in four months,

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<v Speaker 1>I'm like, Okay, get back to me in three months

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<v Speaker 1>and twenty five days. Yeah, I'll let you know if

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<v Speaker 1>I'm up for it. It was just great to see

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<v Speaker 1>that type of passion, you know, and just somebody that

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<v Speaker 1>was just working day and night. Right, And why is

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<v Speaker 1>Beyonce never out of breath? Ever? I don't know if

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<v Speaker 1>she has a built in what's those things that the respirator.

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<v Speaker 1>I don't know if she has a built in respirator.

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<v Speaker 1>I don't know what's going on. I'm like, she was

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<v Speaker 1>dropping down, getting up, moving around with the dancers and

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<v Speaker 1>I'm like, the dancers gotta be tired. They not singing,

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<v Speaker 1>They not singing, and they're heaving okay yeah, and Beyonce

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<v Speaker 1>is like, y'all all right back there. I'm like, man,

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<v Speaker 1>I would have had to crush up some a leave

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<v Speaker 1>and make a paste. I would put the paste on

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<v Speaker 1>my knees and saran rappids. I could not move like

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<v Speaker 1>that for that long. That's crazy, just aching, And I'm like,

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<v Speaker 1>do you know how do you get better than Beyonce?

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<v Speaker 1>You don't. I think the only person who it's possible

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<v Speaker 1>is Blue because she's watching Beyonce. She had Beyonce's breast milk.

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<v Speaker 1>I think that's the only way you can get the

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<v Speaker 1>levels Beyonce. You gotta have ingested her breast milk. Yeah.

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<v Speaker 1>But I mean, when you think about it, that's the

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<v Speaker 1>reason why we called somebody like Beyonce a star. Yeah,

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<v Speaker 1>that's sheer star power for real. It's so concentrated it

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<v Speaker 1>hurts your eyes to even look at her. It's not

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<v Speaker 1>the sequence. Yeah, the sequence aren't even doing it. It's

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<v Speaker 1>Beyonce herself. It's it's our ara and we're just all

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<v Speaker 1>just happy to be there. She's a star and I'm

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<v Speaker 1>just Stardust, just hanging out. Like so today we're gonna

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<v Speaker 1>talk about stars and not just superstars here on Earth.

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<v Speaker 1>We want to talk about the stars in our sky,

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<v Speaker 1>but we actually think that there's a lot of similarities

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<v Speaker 1>between the two, between the stars and the sky and

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<v Speaker 1>Beyonce absolutely. Okay, so let's get into the recitation. So

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<v Speaker 1>let's start with what we know. We know that Beyonce

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<v Speaker 1>is unlike anybody else on this planet, and we also

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<v Speaker 1>know that stars are very unique. So we know that

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<v Speaker 1>the Sun is a star. Yes, we know the Sun

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<v Speaker 1>is a star. I know a little bit about those planets.

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<v Speaker 1>Men are from Venus, I mean, what does that from Mars?

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<v Speaker 1>Women are from Venus? Okay, yeah, which, but I also

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<v Speaker 1>know that that's actually not true. Yeah, and all here

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<v Speaker 1>on Earth. And then we also know that, you know,

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<v Speaker 1>that's saying that we learned in probably like middle school.

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<v Speaker 1>My very educated mother just served us nine pizzas or

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<v Speaker 1>something like that. But something happened to Pluto. Yeah, people

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<v Speaker 1>not talking about it. Yeah, so that was supposed to

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<v Speaker 1>let you know, like Murcury, Venus, Earth, Mars, your mother

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<v Speaker 1>didn't serve the rights and I remember that's just good Okay,

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<v Speaker 1>so I got to go back to middle school. Basically,

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<v Speaker 1>the other thing we know is the big Dipper and

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<v Speaker 1>a little dipper. Right, there are constellations, but that's it.

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<v Speaker 1>That's the extent of my knowledge in the North Star

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<v Speaker 1>wherever it is, nor Yeah, that's right, shout out to

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<v Speaker 1>Harriet Tubman. And So I feel like when I started

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<v Speaker 1>talking about space, there's so little that I know, and

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<v Speaker 1>I feel like it's actually holding me back from really

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<v Speaker 1>enjoying some of the films, Like some of the movies

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<v Speaker 1>that I like, I'm like, why is it taking them

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<v Speaker 1>a long time? Is that a short place to go?

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<v Speaker 1>Because I always get gallic sees and universe and solar system,

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<v Speaker 1>I get all those things mixed up, right. I hope

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<v Speaker 1>that after this episode, I'm gonna go back and watch

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<v Speaker 1>Interstellar and just try to see if I can make

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<v Speaker 1>sense of some things. Probably won't. It was a very

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<v Speaker 1>confusing movie.

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<v Speaker 2>You know.

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<v Speaker 1>One of the things I've always been really really interested

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<v Speaker 1>in is like shine and shine and shine and shineing. Yeah,

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<v Speaker 1>like when you think about the sun, how is the

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<v Speaker 1>sun power? What is the fuel? What is power? And Beyonce,

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<v Speaker 1>we saw a little bit of that in Homecoming yeah,

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<v Speaker 1>we did, but I still was like, girl, what's the

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<v Speaker 1>code so I can do a step left, left left,

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<v Speaker 1>jump down? I'm like, I need the eight count so

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<v Speaker 1>I can unlock a better meat. So that's a question

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<v Speaker 1>I'm gonna have off gate, okay, Like what fuels? What's

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<v Speaker 1>the star? What is it? I mean, I know what

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<v Speaker 1>a star is, do we really what makes something a star?

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<v Speaker 1>What makes something to start?

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<v Speaker 2>Like?

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<v Speaker 1>What are the properties? What are the qualities of a star? Right?

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<v Speaker 1>I think I want to know, like what sustains a star?

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<v Speaker 1>Like how does it keep going and going? Because I

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<v Speaker 1>think that they last for ever, right or for a

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<v Speaker 1>long time until they they burn out? But what keeps

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<v Speaker 1>them going for so long? And what determines to burnout? Right? Yeah,

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<v Speaker 1>that's a really good question. And then I also have

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<v Speaker 1>questions about just like constellations and planets in general. I

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<v Speaker 1>know that Pluto isn't a planet anymore, but I don't

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<v Speaker 1>really get what makes a planet, Like how do you

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<v Speaker 1>determine whether something is a planet or not? Yeah? Or constellation?

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<v Speaker 1>We're in constellation? Like the only constellation I really know

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<v Speaker 1>is the Big Dipper Orion's Belt, the stars, the cosmos.

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<v Speaker 1>That's not my strong point, not mine either, Like I

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<v Speaker 1>think I know maybe some physics, U huh, but nah,

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<v Speaker 1>not really. I've always been terrible at that, and so

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<v Speaker 1>you know, we had to call in the reinforcements. Absolutely,

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<v Speaker 1>it's very needed in this episode. So let's get into

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<v Speaker 1>the dissection, and in honor of homecoming, we brought out

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<v Speaker 1>a student this week.

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<v Speaker 2>So my name is Amy Steele, and I'm an astronomy

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<v Speaker 2>PhD Candidate at the University of Maryland. That's fancy speak

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<v Speaker 2>for I'm a student.

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<v Speaker 1>There are some basic things that we know, right T T. Yeah.

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<v Speaker 1>I think one of the things that we know about

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<v Speaker 1>stars is that they're mostly hydrogen gas.

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<v Speaker 2>Hydrogen is the most abundant element in the universe, and

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<v Speaker 2>stars are mostly made up out of hydrogen.

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<v Speaker 1>I understand they're mostly hydrogen, but then what what else?

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<v Speaker 1>In the cores of stars?

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<v Speaker 2>You have fusion going on, where you're combining hydrogen into helium,

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<v Speaker 2>and that process releases not really that much energy, but

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<v Speaker 2>it happens so many times that it ends up being

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<v Speaker 2>a lot of energy.

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<v Speaker 1>Yes, fusion, I remember you explaining that. Yeah, that's when

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<v Speaker 1>you put to nuclei together and it gives off a

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<v Speaker 1>lot of energy.

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<v Speaker 2>That energy comes out at us the light that makes

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<v Speaker 2>us hot.

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<v Speaker 1>So hydrogen is like the IT factor. Yeah, the stars,

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<v Speaker 1>that's what's making them glow, and so that IT factor

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<v Speaker 1>can determine whether or not you're a big star or

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<v Speaker 1>a little star. So that's the difference between being Rihanna

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<v Speaker 1>or Rita Aura. Yeah. But stars have the same risk though, right,

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<v Speaker 1>Like they can run out of fuel or not be relevant. Right,

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<v Speaker 1>So what happens when a star runs out of fuel,

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<v Speaker 1>like or it runs out of hydrogen.

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<v Speaker 2>It's not like a star can go to a gas station.

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<v Speaker 2>So it forms with a set amount of hydrogen and

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<v Speaker 2>it uses up that hydrogen over the course of its lifetime,

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<v Speaker 2>and when that hydrogen is gone, it's gone.

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<v Speaker 1>So wait a second, does that mean that someday that

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<v Speaker 1>the Sun is gonna run out of hydrogen? Yeah, but

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<v Speaker 1>that's still like at least five billion years away. Oh

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<v Speaker 1>so we're good. We're good. Okay, So now we know

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<v Speaker 1>that it's not complete lights out for the Sun. The

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<v Speaker 1>first thing that we have to know about a real

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<v Speaker 1>star is that everything revolves around you, literally, but also

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<v Speaker 1>everything exists because of you. So when the Sun, our

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<v Speaker 1>star was being formed, it was basically like, okay, ladies,

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<v Speaker 1>Dallat's get information.

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<v Speaker 2>A stellar system isn't formed for the planets. The planets

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<v Speaker 2>form as a result of the star forming itself. The

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<v Speaker 2>star is the star of the show.

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<v Speaker 1>And all of the planets, the Earth, the Moon, all

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<v Speaker 1>of that is just leftovers from the formation of the Sun.

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<v Speaker 1>We're just a byproduct. We're just like a little crumb.

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<v Speaker 1>The Sun is the cookie.

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<v Speaker 2>The Sun is the cookie, The Sun is the cake.

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<v Speaker 1>It just like we saw in Homecoming, Beyonce was dancing,

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<v Speaker 1>those people are moving around her doing all that stuff.

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<v Speaker 1>But you know, if I had to say, who are

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<v Speaker 1>my favorite planets that orbit Beyonce lay Twins, Yes, Oh

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<v Speaker 1>my goodness. They really know how to shine and they

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<v Speaker 1>probably wouldn't be as well known without Beyonce. Like they

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<v Speaker 1>are stars in their own right. Yeah, don't get me wrong,

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<v Speaker 1>but with Beyonce bringing them close to her definitely took

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<v Speaker 1>them to another level. They're always together. Would they exist

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<v Speaker 1>as real planets? Okay, so let's pull back a bit.

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<v Speaker 1>If our solar system is made up the Sun the

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<v Speaker 1>cookie and we're just the crumbs off the cookie, how

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<v Speaker 1>did the cookie get made? How is the Sun formed?

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<v Speaker 1>We want to see the ingredients. Yea, how many chocolate chips.

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<v Speaker 2>The way that it starts is you have this cloud,

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<v Speaker 2>huge cloud of gas and dust, and there's some little

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<v Speaker 2>bit of motion to.

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<v Speaker 1>It, but you need some kind of external stimulus, like

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<v Speaker 1>you need something else nearby to go off and give

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<v Speaker 1>a little bit of energy. Right, So sometimes it could

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<v Speaker 1>be like a supernova nearby.

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<v Speaker 2>Eventually it'll start to spin and flatten like a pancake.

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<v Speaker 2>Once the conditions are right for hydrogen to start fusing

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<v Speaker 2>into helium, that process that makes stars shine. The star

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<v Speaker 2>turns on and then the leftover bits that stuff starts

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<v Speaker 2>to clump together, possibly sweeping up material as it's orbiting

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<v Speaker 2>its new baby star. And that's how the planets form.

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<v Speaker 1>Lots of these crimes are just aggregating together and making

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<v Speaker 1>bigger cookies. Yeah, bigger crumb balls, right, what are those

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<v Speaker 1>donut holes? Munchkins? Bigger little munchkins. But how do you

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<v Speaker 1>tell this is just a clump of crumbs or this

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<v Speaker 1>is a legit planet?

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<v Speaker 2>So to be a planet, there are these three rules

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<v Speaker 2>that you have to abide by, according to the International

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<v Speaker 2>Astronomical Union.

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<v Speaker 1>So first you have to orbit the Sun. You actually

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<v Speaker 1>have to travel around the Sun and follow that path

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<v Speaker 1>over and over again.

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<v Speaker 2>So this is also why the Moon is not considered

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<v Speaker 2>a planet because its primary orbit is around the Earth.

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<v Speaker 1>So the second thing is that you have to be

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<v Speaker 1>the largest thing in your orbit. And the third thing

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<v Speaker 1>is that you need to be roughly spherical.

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<v Speaker 2>So a lot of the asteroids that you'll see, they're

0:12:15.960 --> 0:12:20.200
<v Speaker 2>elongated or they look like someone took two balls and

0:12:20.280 --> 0:12:21.520
<v Speaker 2>just slapped them together.

0:12:22.080 --> 0:12:25.640
<v Speaker 1>Like an asteroid. Asteroids are just two rocks slammed together,

0:12:25.720 --> 0:12:27.360
<v Speaker 1>and they have this really weird shape. So they could

0:12:27.360 --> 0:12:32.000
<v Speaker 1>never be a planet. Your faith could never you bad built.

0:12:31.880 --> 0:12:35.400
<v Speaker 2>And so you have to have enough mass to have

0:12:35.920 --> 0:12:38.960
<v Speaker 2>smoothed yourself into a roughly spherical shape.

0:12:39.160 --> 0:12:42.200
<v Speaker 1>So now that we have laid down the rules for

0:12:42.240 --> 0:12:44.840
<v Speaker 1>what it takes to be a planet, what about the

0:12:44.880 --> 0:12:47.719
<v Speaker 1>differences we see between the planets, right? I know that

0:12:47.840 --> 0:12:53.640
<v Speaker 1>like Saturn has rings yep, and Neptune is like has

0:12:53.720 --> 0:12:57.280
<v Speaker 1>like a lot of water. I'm just out here guessing.

0:12:58.000 --> 0:13:00.320
<v Speaker 1>Let's see what Amy has to say.

0:13:00.520 --> 0:13:05.760
<v Speaker 2>Venus, Earth, and Mars are all pretty rocky, and then Jupiter, Soturn,

0:13:05.960 --> 0:13:10.640
<v Speaker 2>you're in a Snaptune, those are all gassy. Overall, you

0:13:10.720 --> 0:13:14.320
<v Speaker 2>have the small rocky things close to the star where

0:13:14.320 --> 0:13:17.880
<v Speaker 2>it's hotter, and then you have the things that are

0:13:18.320 --> 0:13:22.240
<v Speaker 2>more full of you know, gases that could potentially be

0:13:22.320 --> 0:13:24.839
<v Speaker 2>boiled away if they were too close to something hot.

0:13:25.559 --> 0:13:28.959
<v Speaker 1>Those are farther out. Oh So that makes sense, right,

0:13:29.040 --> 0:13:31.440
<v Speaker 1>because if we have any of those gassy things, they

0:13:31.480 --> 0:13:33.360
<v Speaker 1>need to be in the core somewhere where they're protected

0:13:33.360 --> 0:13:35.440
<v Speaker 1>from the sun. Otherwise they're all evaporated off and all

0:13:35.480 --> 0:13:37.840
<v Speaker 1>we have left is the rock exactly. So these planets

0:13:37.840 --> 0:13:40.360
<v Speaker 1>are set up perfectly in order to sustain themselves. So

0:13:40.440 --> 0:13:43.480
<v Speaker 1>that's really interesting because that's kind of what Amy's job is.

0:13:43.520 --> 0:13:46.920
<v Speaker 1>So she looks at debris from the formation of stars

0:13:47.440 --> 0:13:48.920
<v Speaker 1>and she tries to figure out what they're made of.

0:13:49.040 --> 0:13:51.560
<v Speaker 1>So not our star, not the sun, but the formation

0:13:51.600 --> 0:13:53.959
<v Speaker 1>of other stars. She looks at the debris around them. Well,

0:13:54.000 --> 0:13:57.040
<v Speaker 1>why is there something going on with that? Like? Why

0:13:57.080 --> 0:14:00.440
<v Speaker 1>is that stuff important? If it's just debris. When I

0:14:00.440 --> 0:14:02.280
<v Speaker 1>think of debris, I think of trash on the side

0:14:02.280 --> 0:14:05.040
<v Speaker 1>of the road, just blowing in the wind, But any things,

0:14:05.080 --> 0:14:05.680
<v Speaker 1>it's important.

0:14:05.840 --> 0:14:10.439
<v Speaker 2>Knowing what those asteroids and comments are made of is

0:14:10.880 --> 0:14:14.080
<v Speaker 2>pretty important in terms of figuring out how the Solar

0:14:14.120 --> 0:14:14.880
<v Speaker 2>system formed.

0:14:15.160 --> 0:14:17.800
<v Speaker 1>In other words, in order to understand how a star

0:14:18.080 --> 0:14:20.960
<v Speaker 1>is formed, you got to know what's going on around it.

0:14:21.080 --> 0:14:24.800
<v Speaker 2>You want to see what the material around those stars

0:14:24.840 --> 0:14:28.000
<v Speaker 2>it's made of, so that we can begin to assess

0:14:28.320 --> 0:14:32.480
<v Speaker 2>just how unique or not unique the rocky material in

0:14:32.520 --> 0:14:34.080
<v Speaker 2>our solar system actually is.

0:14:34.400 --> 0:14:39.360
<v Speaker 1>Yes, and this gets me to my favorite thing, aliens. Right,

0:14:39.400 --> 0:14:41.680
<v Speaker 1>because if the dust and rocks that surround other stars

0:14:41.680 --> 0:14:44.160
<v Speaker 1>are similar to the dust and rocks that surround our star,

0:14:44.320 --> 0:14:46.280
<v Speaker 1>the Sun, it helps us put our own star, our

0:14:46.280 --> 0:14:49.600
<v Speaker 1>solar system in context. I feel like if those dust

0:14:49.640 --> 0:14:51.480
<v Speaker 1>and rocks look like our dust and rocks, that means

0:14:51.480 --> 0:14:53.480
<v Speaker 1>there could be an Earth in their solar system. Oh,

0:14:53.520 --> 0:14:56.360
<v Speaker 1>I see where you're going. So you think that it's

0:14:56.480 --> 0:15:01.360
<v Speaker 1>possible for there to be another Beyonce in another universe?

0:15:01.920 --> 0:15:05.600
<v Speaker 1>Highly unlikely, but could it be. I feel like it's

0:15:05.600 --> 0:15:09.000
<v Speaker 1>more likely that there's Aliens then there's another Beyonce. Do

0:15:09.040 --> 0:15:14.280
<v Speaker 1>you think it's possible that Yonce is an extra terrestrial? Absolutely?

0:15:14.840 --> 0:15:17.720
<v Speaker 1>Her a salon that would make complete sense to me.

0:15:17.960 --> 0:15:20.600
<v Speaker 1>Let me tell you something, if you said, heyby Ransom, test,

0:15:20.920 --> 0:15:24.800
<v Speaker 1>Beyonce does not have the same composition as the rest

0:15:24.800 --> 0:15:29.920
<v Speaker 1>of y'all. I would say accurate, not surprised. The odds

0:15:29.920 --> 0:15:33.120
<v Speaker 1>are in her favor. Okay, she got different kind of dust,

0:15:33.280 --> 0:15:37.200
<v Speaker 1>she had different interstellar debris, everything different. It's crazy to

0:15:37.240 --> 0:15:41.200
<v Speaker 1>think that our solar system is just one of many

0:15:41.240 --> 0:15:44.680
<v Speaker 1>solar systems that's in our galaxy, and then our galaxy

0:15:44.760 --> 0:15:47.160
<v Speaker 1>is just one tiny part of this huge universe. Right.

0:15:47.200 --> 0:15:49.640
<v Speaker 1>You remember in Men in Black? When did you watch

0:15:49.680 --> 0:15:51.840
<v Speaker 1>Men in Black? Yeah, at the end of the first

0:15:51.880 --> 0:15:55.040
<v Speaker 1>Men in Black, when they were looking for that ball

0:15:55.160 --> 0:15:57.280
<v Speaker 1>thing and it turned out to be a marble and

0:15:57.320 --> 0:15:59.040
<v Speaker 1>it was all these galaxies and stuff like that. That was

0:15:59.040 --> 0:16:01.440
<v Speaker 1>the only time that my brain was able to understand

0:16:02.000 --> 0:16:04.400
<v Speaker 1>that there are other galaxies out there. I was like,

0:16:05.120 --> 0:16:08.600
<v Speaker 1>there's other galaxies, and these aliens are just playing marbles

0:16:08.760 --> 0:16:11.200
<v Speaker 1>with the galaxies. But when we get back, we're going

0:16:11.240 --> 0:16:13.360
<v Speaker 1>to start talking about things that are outside of our

0:16:13.400 --> 0:16:16.080
<v Speaker 1>solar system. And we've just been talking about things that

0:16:16.080 --> 0:16:18.680
<v Speaker 1>are in our solar system, our sun and the planets

0:16:18.680 --> 0:16:21.000
<v Speaker 1>around it. But there are whole other solar systems just

0:16:21.120 --> 0:16:30.240
<v Speaker 1>like ours. Y'all thought y'all have a special didn't you.

0:16:41.520 --> 0:16:45.280
<v Speaker 1>And we're back, so we've been talking mostly about our

0:16:45.320 --> 0:16:49.920
<v Speaker 1>solar system, our Sun, our Earth, and the neighboring plants

0:16:49.960 --> 0:16:52.680
<v Speaker 1>around it. But our solar system is just a small

0:16:52.800 --> 0:16:55.560
<v Speaker 1>part of the Milky Way galaxy. And the Milky Way

0:16:55.640 --> 0:16:59.280
<v Speaker 1>has over two hundred billion stars in it, which means

0:16:59.400 --> 0:17:02.640
<v Speaker 1>billions of the planets, dust and debris that are a

0:17:02.680 --> 0:17:06.280
<v Speaker 1>byproduct from the formation of those stars, and enough gas

0:17:06.320 --> 0:17:08.840
<v Speaker 1>and dust to make billions more. But when we think

0:17:08.840 --> 0:17:10.919
<v Speaker 1>about that, how big is the Milky Way really?

0:17:11.080 --> 0:17:13.719
<v Speaker 2>So one way that you can think about that is

0:17:14.280 --> 0:17:16.200
<v Speaker 2>in terms.

0:17:15.800 --> 0:17:17.000
<v Speaker 1>Of light years.

0:17:17.640 --> 0:17:21.320
<v Speaker 2>So a light year is a distance that light travels

0:17:21.359 --> 0:17:21.920
<v Speaker 2>in one year.

0:17:22.560 --> 0:17:26.800
<v Speaker 1>That distance a light year is huge, huge, As an

0:17:26.840 --> 0:17:30.640
<v Speaker 1>understatement for real, one light year is five point nine

0:17:30.960 --> 0:17:35.400
<v Speaker 1>trillion miles. So you can do a round trip from

0:17:35.480 --> 0:17:40.480
<v Speaker 1>the Earth to the Sun over thirty thousand times. That's crazy.

0:17:40.640 --> 0:17:44.720
<v Speaker 2>And the size of the Milky Way galaxy going from

0:17:44.760 --> 0:17:49.280
<v Speaker 2>one end to the other is about one hundred thousand

0:17:49.560 --> 0:17:50.119
<v Speaker 2>light years.

0:17:50.160 --> 0:17:52.439
<v Speaker 1>So now we're just this is just getting ridiculous. So

0:17:53.080 --> 0:17:55.240
<v Speaker 1>we already said it's crazy, you're gonna go over thirty

0:17:55.240 --> 0:17:57.879
<v Speaker 1>thousand times to Sun back to dirt, to Sun back

0:17:57.920 --> 0:18:00.080
<v Speaker 1>to dirt. Now you're telling me multiply that by one

0:18:00.119 --> 0:18:05.679
<v Speaker 1>hundred thousand too much, cannot compute and that's so crazy. Right,

0:18:05.680 --> 0:18:08.120
<v Speaker 1>So when we think about all those miles that makes

0:18:08.200 --> 0:18:11.520
<v Speaker 1>up our Milky Way, and then we're in our galaxy,

0:18:11.560 --> 0:18:16.919
<v Speaker 1>we're saying there are over two hundred billion stars. I

0:18:16.960 --> 0:18:19.480
<v Speaker 1>think about us being able to see those stars. Like

0:18:19.520 --> 0:18:21.320
<v Speaker 1>I used to go look at the stars at my grandparents'

0:18:21.320 --> 0:18:22.719
<v Speaker 1>house and they didn't have a lot of light pollutions,

0:18:22.760 --> 0:18:26.000
<v Speaker 1>so you can kind of see everything. And it just

0:18:26.080 --> 0:18:29.000
<v Speaker 1>really occurred to me, like, hey, girl, you looking at

0:18:29.440 --> 0:18:34.440
<v Speaker 1>other solar systems that are light years away, and because

0:18:34.480 --> 0:18:36.439
<v Speaker 1>they're light years away, that light has to travel to me.

0:18:36.720 --> 0:18:38.639
<v Speaker 1>That's not even what it looks like anymore. Oh, Like,

0:18:39.000 --> 0:18:40.960
<v Speaker 1>refresh the screen. I want to see what the stars

0:18:40.960 --> 0:18:44.199
<v Speaker 1>look like right now? How do we make sense of

0:18:44.240 --> 0:18:46.160
<v Speaker 1>all that? Like the only thing I really remember about

0:18:46.200 --> 0:18:48.040
<v Speaker 1>the stars was being able to see the Big Dipper

0:18:48.400 --> 0:18:50.760
<v Speaker 1>and the Little Dipper, right, but I don't really know, Like,

0:18:51.080 --> 0:18:53.120
<v Speaker 1>how do we determine what a constellation is?

0:18:53.280 --> 0:18:58.320
<v Speaker 2>Constellations are just a way of dividing up the sky

0:18:58.680 --> 0:19:02.639
<v Speaker 2>or the celestial sphere into different regions.

0:19:02.720 --> 0:19:06.760
<v Speaker 1>So currently we have eighty eight constellations, So like, how

0:19:06.760 --> 0:19:09.240
<v Speaker 1>on the surface of the Earth we have different countries

0:19:09.480 --> 0:19:15.280
<v Speaker 1>cities states. Similarly, constellations help us organize the sky, and

0:19:15.359 --> 0:19:18.119
<v Speaker 1>constellations have served a lot of practical purposes over the years,

0:19:18.480 --> 0:19:21.560
<v Speaker 1>like agriculture. Yeah, way back before calendars, people used to

0:19:21.600 --> 0:19:24.080
<v Speaker 1>use constellations to keep track of when the harvest crops.

0:19:24.480 --> 0:19:27.720
<v Speaker 1>That's just crazy. Or navigation. You know, Molana, yes, is

0:19:27.800 --> 0:19:30.560
<v Speaker 1>out there on the sea. You say the line where

0:19:30.560 --> 0:19:34.320
<v Speaker 1>this guy needs to see it calls me, that's exactly

0:19:34.320 --> 0:19:37.119
<v Speaker 1>the part where I start tearing up. And she was

0:19:37.119 --> 0:19:40.280
<v Speaker 1>putting her hand up and navigating that boat. Yeah, same thing.

0:19:40.440 --> 0:19:42.920
<v Speaker 1>And the interesting thing about constellations is that even though

0:19:42.920 --> 0:19:45.280
<v Speaker 1>we look at them and say like, oh, this is

0:19:45.760 --> 0:19:48.600
<v Speaker 1>this constellation, it's the Big Dipper, Little Dipper, Orion's belt.

0:19:49.760 --> 0:19:52.080
<v Speaker 1>Two things that I found really interesting. One is that

0:19:52.119 --> 0:19:54.639
<v Speaker 1>those stars aren't necessarily close to each other, right, So

0:19:54.720 --> 0:19:58.040
<v Speaker 1>you could have a star that's really bright and it's

0:19:58.040 --> 0:20:00.359
<v Speaker 1>close to you, or a star here that's dim, but

0:20:00.400 --> 0:20:03.080
<v Speaker 1>it's dim because it's super far away compared to that

0:20:03.119 --> 0:20:05.119
<v Speaker 1>bright star. And then the other thing is that the

0:20:05.200 --> 0:20:07.520
<v Speaker 1>names we use for constellations, most of them come from

0:20:07.560 --> 0:20:11.880
<v Speaker 1>like Greek mythology or ancient Roman stories, but they weren't

0:20:11.920 --> 0:20:14.560
<v Speaker 1>the only ones that were looking at the star. Come on, somebody,

0:20:14.840 --> 0:20:17.919
<v Speaker 1>so the Messiah. Native American tribes, all of these different

0:20:18.000 --> 0:20:21.160
<v Speaker 1>groups have had different names for those constellations in the sky,

0:20:21.800 --> 0:20:23.880
<v Speaker 1>but only some of those names are in your textbook,

0:20:24.160 --> 0:20:29.040
<v Speaker 1>SIPs Tea. I ain't saying, but I'm just saying so

0:20:29.119 --> 0:20:31.640
<v Speaker 1>in our galaxy, constellations are there to help us make

0:20:31.680 --> 0:20:34.240
<v Speaker 1>sense of things. But there are other things in our

0:20:34.240 --> 0:20:36.960
<v Speaker 1>galaxy that, no matter how hard we try, they may

0:20:37.040 --> 0:20:40.720
<v Speaker 1>never make sense. Like black holes. We just got the

0:20:40.840 --> 0:20:44.240
<v Speaker 1>very first picture of a black hole a couple weeks ago,

0:20:44.600 --> 0:20:47.919
<v Speaker 1>and I don't know about you, but that terrified me.

0:20:48.080 --> 0:20:50.400
<v Speaker 1>I don't want to see a black hole. Everybody dies

0:20:50.440 --> 0:20:52.080
<v Speaker 1>in the movies when there's a black hole. Right, that

0:20:52.119 --> 0:20:54.440
<v Speaker 1>black hole isn't even in our galaxy. I don't need

0:20:54.480 --> 0:20:57.680
<v Speaker 1>that disrupting the space time continuum. Let things be as

0:20:57.720 --> 0:21:00.600
<v Speaker 1>they are. Right. And so now people say, oh, pretty

0:21:00.640 --> 0:21:03.160
<v Speaker 1>soon we should have a picture of a black hole

0:21:03.440 --> 0:21:06.080
<v Speaker 1>in our galaxy. No, I don't want no smoke from

0:21:06.080 --> 0:21:08.560
<v Speaker 1>a black hole. Listen, leave it be. It might not

0:21:08.640 --> 0:21:11.720
<v Speaker 1>light flash photography. You need to carry on as you were.

0:21:11.800 --> 0:21:15.760
<v Speaker 1>It's like the Sas squad. Stop looking for it. Black holes.

0:21:16.040 --> 0:21:19.680
<v Speaker 2>I just my brain kind of gets a little too

0:21:19.720 --> 0:21:22.320
<v Speaker 2>hot when I try to make sense of black holes.

0:21:22.359 --> 0:21:25.640
<v Speaker 1>Black Holes are massive pits where gravitational force is so

0:21:25.680 --> 0:21:31.720
<v Speaker 1>strong it sucks in everything in its path, debris, dust, planets, light.

0:21:32.280 --> 0:21:34.840
<v Speaker 1>And the way a black hole is formed is when

0:21:34.920 --> 0:21:39.040
<v Speaker 1>a star dies and collapses in on itself. I got

0:21:39.080 --> 0:21:41.240
<v Speaker 1>some stuff to throw on a black hole. I've got

0:21:41.280 --> 0:21:43.959
<v Speaker 1>plenty stuff to throw on the black hole. Take mine, Witchie.

0:21:45.200 --> 0:21:49.640
<v Speaker 2>The Milky Way our galaxy. We have our own supermassive

0:21:49.640 --> 0:21:53.840
<v Speaker 2>black hole, and it's called Sagittaries a star, and we

0:21:54.080 --> 0:21:58.480
<v Speaker 2>just looked at a sort of an image of one

0:21:59.280 --> 0:22:03.720
<v Speaker 2>in the galaxy see M. Eighty seven, which is really exciting.

0:22:04.240 --> 0:22:07.399
<v Speaker 1>So we do know we have one Sabarius a star.

0:22:07.680 --> 0:22:11.440
<v Speaker 1>But I'm a little nervous. Right where are you a

0:22:11.560 --> 0:22:14.359
<v Speaker 1>black hole in our galaxy? And are you close to us?

0:22:14.359 --> 0:22:16.760
<v Speaker 1>That's what I write, because are we like right on

0:22:16.800 --> 0:22:18.800
<v Speaker 1>the edge? Are we about to fall in? Are we

0:22:18.880 --> 0:22:20.920
<v Speaker 1>in danger? Earth? You in danger? Girl?

0:22:22.680 --> 0:22:26.200
<v Speaker 2>So we are not close to the center of our galaxy.

0:22:26.320 --> 0:22:28.520
<v Speaker 2>We are in the outskirts. We are in the boonies.

0:22:28.680 --> 0:22:30.879
<v Speaker 1>I want to be I don't want to be in

0:22:30.880 --> 0:22:33.280
<v Speaker 1>the city next to the black hole. Another thing that

0:22:33.320 --> 0:22:34.840
<v Speaker 1>can happen when the star dies is that it can

0:22:34.880 --> 0:22:36.840
<v Speaker 1>become a white dwarf. What's that?

0:22:37.240 --> 0:22:39.680
<v Speaker 2>So if the sun is a flame, then a white

0:22:39.720 --> 0:22:42.480
<v Speaker 2>dwarf is the ember after the flame is gone.

0:22:42.920 --> 0:22:44.600
<v Speaker 1>I think a black hole is like something that leaves

0:22:44.600 --> 0:22:48.280
<v Speaker 1>this gaping opening and everybody misses them. Like Nipsey Hustle,

0:22:48.880 --> 0:22:51.879
<v Speaker 1>a black black hole. Rest in peace will never be

0:22:51.960 --> 0:22:54.600
<v Speaker 1>the same, and so like it affects affects everybody. But

0:22:54.640 --> 0:22:56.600
<v Speaker 1>then a white dwarf is a star that kind of

0:22:56.720 --> 0:23:00.520
<v Speaker 1>just has, you know, run its course and it's now,

0:23:00.920 --> 0:23:04.680
<v Speaker 1>you know, a legend or something like that, like we'll

0:23:04.720 --> 0:23:08.159
<v Speaker 1>never forget the shine it had, and now they're just

0:23:08.520 --> 0:23:10.800
<v Speaker 1>enjoying their time as a white dwarf. Kind of like

0:23:10.840 --> 0:23:13.880
<v Speaker 1>Diana Ross. She not dead, she's not dead, but she's

0:23:14.000 --> 0:23:19.320
<v Speaker 1>her career is her singing career is done. She's not singing.

0:23:20.280 --> 0:23:23.080
<v Speaker 1>She just did something recently because it was her seventy

0:23:23.119 --> 0:23:27.000
<v Speaker 1>fifth Oh god, okay, let's do something. Let's keep it.

0:23:27.000 --> 0:23:29.840
<v Speaker 1>It's perfect. This reminds me of that time when I

0:23:29.840 --> 0:23:32.439
<v Speaker 1>said Anita Baker and you thought I met Josephine Baker.

0:23:33.760 --> 0:23:35.680
<v Speaker 1>Every time I think about that time and You're like

0:23:35.760 --> 0:23:39.840
<v Speaker 1>the lady in black and white with the bananas. Who

0:23:39.880 --> 0:23:42.160
<v Speaker 1>knows who knows? Who? Can never be really sure about

0:23:42.200 --> 0:23:45.800
<v Speaker 1>who's Anita Baker and who's Josephine Baker? No one. I

0:23:45.840 --> 0:23:59.760
<v Speaker 1>love it. So that was a lot for both of us, right,

0:24:00.320 --> 0:24:02.840
<v Speaker 1>I mean, we are in our recording studio and it

0:24:02.920 --> 0:24:06.200
<v Speaker 1>is hot in here from all of us being like what,

0:24:06.520 --> 0:24:11.640
<v Speaker 1>my brain is overheated. But I think we learned a lot,

0:24:11.800 --> 0:24:14.080
<v Speaker 1>and there was one thing that I think that Amy

0:24:14.080 --> 0:24:16.800
<v Speaker 1>brought up that is very very cool. It brought me

0:24:16.840 --> 0:24:19.520
<v Speaker 1>a lot of hope. Yes, maybe there is a future

0:24:19.520 --> 0:24:19.880
<v Speaker 1>for us.

0:24:21.320 --> 0:24:23.399
<v Speaker 2>This is so cheesy, but I'm gonna say it anyway.

0:24:23.920 --> 0:24:26.360
<v Speaker 2>It's just that we're made of star stuff and it's

0:24:26.359 --> 0:24:27.399
<v Speaker 2>so cool to think about.

0:24:27.880 --> 0:24:29.000
<v Speaker 1>I love it.

0:24:29.119 --> 0:24:31.080
<v Speaker 2>All of the things that we have on the Earth

0:24:31.240 --> 0:24:35.200
<v Speaker 2>that are heavier than hydrogen were formed through the evolution

0:24:35.920 --> 0:24:36.919
<v Speaker 2>of stars.

0:24:36.640 --> 0:24:39.040
<v Speaker 1>And we're made of those elements. We are made of

0:24:39.119 --> 0:24:43.000
<v Speaker 1>the same elements of a star of the sun. Beyonce

0:24:43.440 --> 0:24:47.440
<v Speaker 1>Beyonce too. I'm gonna say it with even more conviction

0:24:47.600 --> 0:24:50.240
<v Speaker 1>now when I tell people you can't shave me, I say,

0:24:50.240 --> 0:24:53.600
<v Speaker 1>you can't shave the sun. And I really want to telescope, Like,

0:24:54.040 --> 0:24:57.000
<v Speaker 1>after thinking about this, is it gonna it's gonna make me? Yeah, man,

0:24:57.040 --> 0:24:58.480
<v Speaker 1>it's not gonna be good for it. I mean for me,

0:24:58.560 --> 0:25:00.440
<v Speaker 1>it'll be bad if I got to tell us, because

0:25:00.840 --> 0:25:04.639
<v Speaker 1>the idea of that much space around me, it crushes

0:25:04.680 --> 0:25:08.119
<v Speaker 1>my brain where I'm just like, I'm not even the

0:25:08.160 --> 0:25:13.159
<v Speaker 1>size of a molecule of hydrogen when you think of

0:25:13.200 --> 0:25:15.879
<v Speaker 1>the universe, when we think about what a molecule of

0:25:15.960 --> 0:25:19.320
<v Speaker 1>hydrogen is to us, we're not even that small. We're

0:25:19.359 --> 0:25:23.960
<v Speaker 1>smaller than that. Good grief and that type of awareness

0:25:24.800 --> 0:25:28.439
<v Speaker 1>paralyzes me. I'm like, ooh, all this space, you are

0:25:28.440 --> 0:25:31.600
<v Speaker 1>now free to roam. I feel like now free to

0:25:31.640 --> 0:25:34.600
<v Speaker 1>roam about the cabin. Yeah, except I'm not. I want

0:25:34.640 --> 0:25:37.080
<v Speaker 1>to get to another galaxy. I'm out of here people,

0:25:37.920 --> 0:25:54.480
<v Speaker 1>I'm trying to get to another rock. So we've always

0:25:54.480 --> 0:25:57.960
<v Speaker 1>structured our seasons as semesters, and everybody knows halfway through

0:25:57.960 --> 0:26:01.240
<v Speaker 1>the semester it's the midterm, and celebrate our midterm. First

0:26:01.240 --> 0:26:03.000
<v Speaker 1>of all, we're gonna be asking y'all a lot of

0:26:03.080 --> 0:26:07.320
<v Speaker 1>questions about those these Verse six episodes. But more importantly,

0:26:07.680 --> 0:26:10.240
<v Speaker 1>we are celebrating with twenty five percent off in the

0:26:10.240 --> 0:26:13.199
<v Speaker 1>Dope Labs store at Dope Labs podcast dot com. Use

0:26:13.240 --> 0:26:18.480
<v Speaker 1>promo code midterm m I d T E r M.

0:26:18.600 --> 0:26:20.879
<v Speaker 1>For more on today's episode, check out our cheat sheet

0:26:20.880 --> 0:26:24.000
<v Speaker 1>and show notes at Dope Labs podcasts dot com. And

0:26:24.080 --> 0:26:26.520
<v Speaker 1>remember the phone lines are always open. You can leave

0:26:26.560 --> 0:26:29.679
<v Speaker 1>us a question or comment or text us. Our number

0:26:29.760 --> 0:26:33.520
<v Speaker 1>is two zero two five six seven seven zero two eight.

0:26:34.000 --> 0:26:38.080
<v Speaker 1>That's two zero two five six seven seven zero two eight.

0:26:38.359 --> 0:26:40.760
<v Speaker 1>You can find us on Twitter and Instagram at Dope

0:26:40.840 --> 0:26:43.679
<v Speaker 1>Labs podcast. T T is on Twitter and Instagram at

0:26:43.760 --> 0:26:46.840
<v Speaker 1>dr Underscore t s h O. And you can find

0:26:46.920 --> 0:26:50.639
<v Speaker 1>Zakia on Twitter and Instagram at z Said So. And

0:26:50.680 --> 0:26:52.480
<v Speaker 1>if you do love the show, don't forget to follow

0:26:52.560 --> 0:26:54.679
<v Speaker 1>us on Spotify or wherever else you listen to your

0:26:54.680 --> 0:26:58.040
<v Speaker 1>podcast Special Things Today to our guest Amy Steal. You

0:26:58.040 --> 0:27:00.440
<v Speaker 1>can learn more about her work and today's sh notes

0:27:00.440 --> 0:27:03.160
<v Speaker 1>on Dope lap podcast dot com. Our producer is Jenny

0:27:03.200 --> 0:27:06.119
<v Speaker 1>Rattle at Mask. Mixing and sound designed by Hannis Brown.

0:27:06.280 --> 0:27:09.800
<v Speaker 1>Original theme music by Taka Yasuzawa and Alex sugi Ura.

0:27:09.960 --> 0:27:13.560
<v Speaker 1>Additional music by Elijah Alex Harvey. Dope Labs is brought

0:27:13.560 --> 0:27:15.560
<v Speaker 1>to you by three M and is a production of

0:27:15.600 --> 0:27:19.080
<v Speaker 1>Spotify Studios and Mega Own Media Group, and is executive

0:27:19.080 --> 0:27:26.560
<v Speaker 1>produced by us T. T. Shadia and Zakiah Wattley. What's that?

0:27:27.200 --> 0:27:29.399
<v Speaker 1>Missy Elliott had that song? All I know is the

0:27:29.400 --> 0:27:32.040
<v Speaker 1>Tyree song? Yeah, there's that one. The signs of love,

0:27:32.080 --> 0:27:35.400
<v Speaker 1>These are the signs of love making. Hey are you

0:27:35.480 --> 0:27:47.480
<v Speaker 1>that Zodie yack freak looking for fuckercon? But then that

0:27:47.680 --> 0:27:54.080
<v Speaker 1>Beyonce and Missy Elliott? Which one? Oh wait, you know,

0:27:55.320 --> 0:27:57.040
<v Speaker 1>I don't. I don't know what you're talking about. You

0:27:57.080 --> 0:28:00.360
<v Speaker 1>just said, whoa, I don't know what's song that you're

0:28:00.359 --> 0:28:02.840
<v Speaker 1>trying to shame. No, I'm not trying to say I'm

0:28:02.880 --> 0:28:04.960
<v Speaker 1>trying to get to where you at. Let me look

0:28:04.960 --> 0:28:05.280
<v Speaker 1>it up.