WEBVTT - Will A Gamma Ray Burst Kill You?

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<v Speaker 1>Hey, Jorge, do you worry much about things from space

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<v Speaker 1>coming to kill you? Not until right now? Why should I? Well,

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<v Speaker 1>it depends. It depends on what. Well, if there was

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<v Speaker 1>nothing you could do to prepare for or prevent it,

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<v Speaker 1>would you still want to know? Yeah? I think so.

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<v Speaker 1>It'd be nice to know. Um, so you can get

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<v Speaker 1>my things in order, and you know, get a couple

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<v Speaker 1>of finish that TV series I I've been watching. In

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<v Speaker 1>that case, I highly recommend you pay attention to this

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<v Speaker 1>episode of our podcast because it's going to prepare you.

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<v Speaker 1>Why should I listen to the episode or finish my

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<v Speaker 1>TV series? I'm confused? What should I do? Daniel? I imagine, Well,

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<v Speaker 1>we're recording this episode. You do sound this tracked sometimes? Well,

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<v Speaker 1>I say, she'd multitask exactly. There's a you know, death

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<v Speaker 1>from space is coming, so you've got to get stuff done.

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<v Speaker 1>I feel like the universe is huge and there's there's

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<v Speaker 1>a million things out there that can kills instantly at

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<v Speaker 1>any time. Are you saying there's something in particular I

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<v Speaker 1>should be worried about. Stay tuned find out. Hi. I'm Borhand.

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<v Speaker 1>I'm a cartoonist and the creator of the comic strip

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<v Speaker 1>piled Higher and Deeper or PhD comics. He's also a

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<v Speaker 1>shill for big banana corporations, but you'll hear more about

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<v Speaker 1>that later. I'm Daniel. I'm a particle physicist and a

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<v Speaker 1>part time podcast host and amateur baker, and also a

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<v Speaker 1>shill for Marvel Comics and DC whatever. Man, I'm totally

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<v Speaker 1>a DC guy. That's why he sold out to Marvel,

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<v Speaker 1>because it's the most successful, more successful franchise. Well, I

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<v Speaker 1>am still waiting for that check, by the way, for

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<v Speaker 1>selling out to Marvel. I think I think they're waiting

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<v Speaker 1>for um Tony Stark design it. Yeah. Well I was

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<v Speaker 1>fact checking their Pin Particle episodes and I sent them

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<v Speaker 1>a long list of corrections and never heard back. So

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<v Speaker 1>maybe I'm maybe they don't want to hear from me anymore.

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<v Speaker 1>I know the scientific advisor of the at My Movies.

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<v Speaker 1>He's a buddy, so I could we could just have

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<v Speaker 1>the whole podcast with him, really, because I got a

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<v Speaker 1>few things to say about the pin particle and the

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<v Speaker 1>quantum realm. Now he's a quantum physicist. Are you sure

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<v Speaker 1>you're you're off for the for the challenge? Well, he's

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<v Speaker 1>either right or he's wrong. There's no in between, right, No,

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<v Speaker 1>he is, he's both. No, he's right and wrong at

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<v Speaker 1>the same time. That's right. Yeah. Anyway, this is our podcast,

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<v Speaker 1>Daniel and Jorge Explain the Universe, a production of I

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<v Speaker 1>Heart Radio, where we talk about all the amazing and

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<v Speaker 1>mysterious things are that are out there in the universe

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<v Speaker 1>that may or may not kill you instantly. That's right.

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<v Speaker 1>That Sometimes we talked about the real universe. Sometimes we

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<v Speaker 1>talk about the Marvel universe, or the DC universe, or

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<v Speaker 1>the Banana universe, whatever is interesting today. Yeah, and so

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<v Speaker 1>today on the podcast, we are going to talk about

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<v Speaker 1>a very interesting topic. That's right. Today's topic is gamma

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<v Speaker 1>ray bursts. A bunch of listeners wrote in and asked

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<v Speaker 1>us to explain gamma ray bursts. What are they? Can

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<v Speaker 1>they kill us? Can they really turned Bruce Banner into

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<v Speaker 1>the Hulk? What's going on? Please break it down? Wait,

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<v Speaker 1>gamma ray births. I thought we were talking about Billy

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<v Speaker 1>ray Cires. I thought, isn't that the weird thing from

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<v Speaker 1>space that we were No, Billy ray Cirus. His career

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<v Speaker 1>is based on getting irradiated by gamma ray bursts. That's

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<v Speaker 1>the connection. He used to be a mild mannered singer,

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<v Speaker 1>and then he got gamma rays and now he's like

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<v Speaker 1>crazy Billy ray Cirus, all right, and so gamma rays

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<v Speaker 1>are involved. I totally made that up. That is completely fabricated.

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<v Speaker 1>I apologize to Billy ray Cirius and all of his

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<v Speaker 1>fans for implying that the mere mortal could not have

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<v Speaker 1>written that music the hokey pokey. So he didn't write

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<v Speaker 1>the hokey pokey anyway. But but gamma rays do play

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<v Speaker 1>a big role in the Marvel universe, right, because back

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<v Speaker 1>when gamma rays were the crazy thing people were worried about.

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<v Speaker 1>It showed up in comic books all the time. And

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<v Speaker 1>that's how Bruce Banner got turned into the Hulk. That's right.

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<v Speaker 1>And I'm surprised you know this fact about the Marvel universe.

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<v Speaker 1>I thought you were a d C guy. Well, you know,

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<v Speaker 1>Marvel is not paying me, so I figured i'd do

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<v Speaker 1>some research. So yeah, so he he gets irradiated by

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<v Speaker 1>gamma rays and some kind of accident and that's what

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<v Speaker 1>turns him into the Hulk. And so these are like magic,

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<v Speaker 1>mysterious raise right, that's right. And you know, I gotta

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<v Speaker 1>wonder about this origin story the Hulk, Like, do you

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<v Speaker 1>think they're trying to make it seem like it's his fault?

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<v Speaker 1>Like crazy scientists just wants to learn about the universe,

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<v Speaker 1>doesn't care about the risks to humanity gets irradiated, Like

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<v Speaker 1>is that like a moral punishment like tisk tisk, You

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<v Speaker 1>shouldn't be playing with these forces you don't understand. Yeah,

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<v Speaker 1>for sure. Wait are you saying that comic books can

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<v Speaker 1>have like literary you know, secret mess it is and

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<v Speaker 1>thieves and they're definitely there's definitely literary. I don't know

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<v Speaker 1>if it's so secret though. I just wonder about like

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<v Speaker 1>how is interpreted at the time, you know, like our

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<v Speaker 1>scientists like the leading edge, they're bringing us into the

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<v Speaker 1>atomic age, look at all the wonderful things we're getting

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<v Speaker 1>out of science, or is it like I'm kind of

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<v Speaker 1>scared of science. Scientists don't seem trustworthy, look at all

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<v Speaker 1>the crazy stuff they're doing. I think it was a

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<v Speaker 1>It's supposed to be kind of a take on you

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<v Speaker 1>know Dr jackl and Mr Hyde, you know, the scientists

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<v Speaker 1>who's trying to understand things and playing maybe with things

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<v Speaker 1>he doesn't quite fully understand, and then he he gets

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<v Speaker 1>turned into a superhero and into a multiple near franchise

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<v Speaker 1>we kind of worked out for the scientists. Yeah, so

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<v Speaker 1>the lesson is everybody should do crazy radiation experiments in

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<v Speaker 1>their basement, right, you know what? Gamma rays do feature

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<v Speaker 1>a lot in comics from a long time ago, and

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<v Speaker 1>they are a real thing. Gamma rays really are a

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<v Speaker 1>real thing, and gamma ray bursts are a real thing,

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<v Speaker 1>and so we thought it'd be fun to do an

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<v Speaker 1>episode where we explain it. Um. It turns out that

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<v Speaker 1>they are quite a scientistic puzzle. Um. For a long time,

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<v Speaker 1>physicists have not understood where they came from and what's

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<v Speaker 1>generating them. And should we be worried about them? Yeah?

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<v Speaker 1>Should we worry about them exactly? And are we all

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<v Speaker 1>going to turn into the Hulk? And how do you

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<v Speaker 1>feel about that anyway? And should you watch your TV?

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<v Speaker 1>I don't, Well, you mean, what happens if you turn

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<v Speaker 1>into the Hulk and you have all those TV shows recorded?

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<v Speaker 1>Do you think the Hulk likes to watch the same

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<v Speaker 1>TV show as you do? Do you need like separate

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<v Speaker 1>tvrs for when you're in Hulk mode when you're not

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<v Speaker 1>in Hulk mode? You know, I don't think the Hulk

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<v Speaker 1>would get past, you know, the pilot episode of most

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<v Speaker 1>TV shows. You know, you'd probably smash the TV right away.

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<v Speaker 1>No stars from no unnecessary dialogue. That sounds like how

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<v Speaker 1>my son reviews in most television shows really pretty much

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<v Speaker 1>talking too much talking. Where is the action? Exactly exactly?

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<v Speaker 1>They sound pretty cool. Gamma rays, right, gamma rays. I

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<v Speaker 1>mean it sounds like some sort of new kind of

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<v Speaker 1>ray energy, Yeah, exactly. Does it have a positive connotation

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<v Speaker 1>to you, like, oh my god, look at this amazing

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<v Speaker 1>source of energy, all the good we can do for

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<v Speaker 1>the world, or does have a negative connotation like is

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<v Speaker 1>this a weapon that's gonna kill me? I think it

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<v Speaker 1>just sounds like something out of science fiction, you know,

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<v Speaker 1>like if you called it, like, um, puppy dog rays,

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<v Speaker 1>I'd be like, Oh, that's cute, it's safe. What you

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<v Speaker 1>called it? Like? You know whathero can I can't let

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<v Speaker 1>that go. I can't let it go. What if a

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<v Speaker 1>scientist is experimenting with puppy dog rays and gets irradiated,

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<v Speaker 1>what kind of superhero does he turn into? The UK puppy,

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<v Speaker 1>The hush puppy goes around licking everybody, snuggling with them.

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<v Speaker 1>The husky, the husky. There you go, husky exactly, the

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<v Speaker 1>green husky, which sounds pretty adorable. But no, yeah, they

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<v Speaker 1>sound mysterious. They sound revery sci fi, right, like gamma

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<v Speaker 1>Like all you have to just pick a Greek letter

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<v Speaker 1>and marry it to like a scientific physics term and

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<v Speaker 1>you have something sci fi. Yeah, yeah, exactly. Now you're right.

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<v Speaker 1>It does stay fit. But the cool thing about it

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<v Speaker 1>is that it's actually also science e Like, there's are

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<v Speaker 1>a lot of really interesting science behind gamma ray bursts. Yeah,

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<v Speaker 1>and a big mystery, right, there was a big mystery

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<v Speaker 1>about them. Yeah. Yeah, So I was wondering what people

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<v Speaker 1>knew about gamma ray bursts. Were they worried about them?

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<v Speaker 1>Do they know what they mean? Do they know what

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<v Speaker 1>a gamma ray is at all? So, as usual, Daniel

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<v Speaker 1>went out there and asked people on the street, random strangers,

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<v Speaker 1>what they thought a gamma ray was. And these interviews

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<v Speaker 1>happened partially on the campus of you see, Irvine, and

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<v Speaker 1>also partially at the Irvine Spectrum. So you're gonna get

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<v Speaker 1>a selection of students and random people. What's the Irvine Spectrum?

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<v Speaker 1>What's the Irvine Spectrum? Oh my god, how do you

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<v Speaker 1>not know about that people like you in in Orange County?

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<v Speaker 1>Is it like the range from Dark Based Dark Baby.

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<v Speaker 1>I never realized the dramatic irony of Irvine calling anything

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<v Speaker 1>a spectrum because there is no spectrum. You're right, um, No,

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<v Speaker 1>it's a big mall here in Irvine. People actually like

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<v Speaker 1>fly here from Japan, stay in a hotel and just

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<v Speaker 1>shop of the mall and then like fly back. It's crazy. Really,

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<v Speaker 1>is it like a fancy or is it like a

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<v Speaker 1>mega Minnesota Malvey America's I'm not the right person to

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<v Speaker 1>evaluate malls. I spent as a little time in them

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<v Speaker 1>as possible. I was there because my kids were in

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<v Speaker 1>spring break and I took them to a movie, And

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<v Speaker 1>while they were in the movie, I interviewed people about

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<v Speaker 1>Gamma rays. You didn't go into the movie with them, No, No,

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<v Speaker 1>I stood outside looking like a weirdo, asking people weird

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<v Speaker 1>science questions. All right, well, those of you at home,

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<v Speaker 1>think about it for a second. If you if a

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<v Speaker 1>random physicist approach you outside of a movie theater in

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<v Speaker 1>a fancy mall and ask you, what is the gammerie,

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<v Speaker 1>what would you say? Good? Step away, ster, You'd say,

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<v Speaker 1>I didn't fly here from Japan, just to answer your

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<v Speaker 1>questions security security. One fascinating thing is that on campus

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<v Speaker 1>a U s I nine nine of people will answer

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<v Speaker 1>my questions, whereas it the spectrum, only like one in

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<v Speaker 1>ten are willing to answer questions. Really huh yeah, I

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<v Speaker 1>wonder whether that why that is. I don't know. So

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<v Speaker 1>here's what people had to say. First question is have

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<v Speaker 1>you ever heard about gamma ray burst? Do you know

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<v Speaker 1>what that is? No? No, I don't know, but I've

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<v Speaker 1>heard of it because they definitely has to do something

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<v Speaker 1>with UV light. It's like a sun ray. I'm assuming

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<v Speaker 1>it's just I know that it modifies like your DNA

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<v Speaker 1>or something. I could just blast your DNA and that

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<v Speaker 1>could cause some damage to you, like severely. Yeah. Yeah,

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<v Speaker 1>so that's about it, but not too into a Gamma

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<v Speaker 1>rebers a kind of game or I don't know. Yes,

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<v Speaker 1>but the star explodes and it will admit a lot

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<v Speaker 1>of frequency of photons and the country a large exposure

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<v Speaker 1>identific because it will be high. I will make Gamma

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<v Speaker 1>explosion something okay, and it's a something to worry about.

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<v Speaker 1>I don't think it will be that powerful that makes

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<v Speaker 1>us worry. It depends on how close the stories Honestly,

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<v Speaker 1>I couldn't tell you, all right, because I have something

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<v Speaker 1>with stars or m it's when the sun explodes or something, right,

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<v Speaker 1>something is it's something to worry about, I would seem

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<v Speaker 1>so yeah, alright, so pretty binary response. Right. Most people

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<v Speaker 1>didn't know or they knew all about it, Yeah, exactly

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<v Speaker 1>a lot of people have never heard about them, or

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<v Speaker 1>like it tickled something in their brain maybe, but they

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<v Speaker 1>were not able to say anything concrete about it. But

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<v Speaker 1>some folks clearly had done some reading. Yeah, but nobody

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<v Speaker 1>mentioned the Hulk. No, nobody mentioned the Hulk. Um though

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<v Speaker 1>you know, I've been bulking up recently, so I sort

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<v Speaker 1>of digging for compliments there. But no, I didn't get me.

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<v Speaker 1>Did you paid yourself green as well? Know that? And

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<v Speaker 1>you're not allowed to be green and irvine. It's only

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<v Speaker 1>beige allowed. Oh, the beige Hulk. That would be the

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<v Speaker 1>irvine version. So that's sound. They sound pretty mysterious. Gamma rays, um,

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<v Speaker 1>so what are they done? And let's break it down

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<v Speaker 1>for people? What are gamma rays? So in the end

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<v Speaker 1>of gamma ray is not as exotic as it sounds.

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<v Speaker 1>It's just a kind of photon. So remember photons are

0:12:15.800 --> 0:12:20.679
<v Speaker 1>the particle that carry electromagnetic radiation. So all light you know,

0:12:21.000 --> 0:12:24.840
<v Speaker 1>radio waves to visible light, to X rays and all

0:12:24.880 --> 0:12:27.400
<v Speaker 1>the way up to gamma rays, they're all just photons

0:12:27.440 --> 0:12:31.080
<v Speaker 1>of different frequencies. They're just light wiggling at different wavelengths.

0:12:31.280 --> 0:12:33.760
<v Speaker 1>And we called different parts of the spectrum different things

0:12:33.800 --> 0:12:36.520
<v Speaker 1>because they were discovered different times, and we treat them

0:12:36.559 --> 0:12:39.280
<v Speaker 1>differently or the qualitatively different. But in the end, they're

0:12:39.280 --> 0:12:42.839
<v Speaker 1>all just parts of the electromagnetic spectrum. So wait, did

0:12:42.840 --> 0:12:45.360
<v Speaker 1>they think before that they were different, like a different

0:12:45.400 --> 0:12:48.439
<v Speaker 1>kind of ray or particle or was this before they

0:12:48.600 --> 0:12:51.800
<v Speaker 1>even knew about particles. Yeah, before we even knew about particles,

0:12:51.800 --> 0:12:54.480
<v Speaker 1>and we knew about rays, like we had cathode rays

0:12:54.559 --> 0:12:56.840
<v Speaker 1>and stuff like that in X rays, and we didn't

0:12:56.920 --> 0:12:59.839
<v Speaker 1>understand for a long time that rays were particles. And

0:13:00.000 --> 0:13:02.439
<v Speaker 1>and later they unified a lot of these different things

0:13:03.120 --> 0:13:05.600
<v Speaker 1>um and understood them all just be parts of the

0:13:05.640 --> 0:13:07.720
<v Speaker 1>same thing. So they just thought it was like a

0:13:08.320 --> 0:13:10.920
<v Speaker 1>just like a different kind of ray, Yeah, like a

0:13:10.960 --> 0:13:14.080
<v Speaker 1>different kind of beam of something. Yeah, because particles at

0:13:14.080 --> 0:13:16.720
<v Speaker 1>different energy, photons at different energy act really different. You know,

0:13:16.760 --> 0:13:20.240
<v Speaker 1>photons that are the visible wavelength, you can see them.

0:13:20.240 --> 0:13:23.600
<v Speaker 1>They look green. For example, photons that are high enough

0:13:23.679 --> 0:13:26.319
<v Speaker 1>energy to penetrate through you and give you a picture

0:13:26.320 --> 0:13:28.840
<v Speaker 1>of your bones. You know, we call those X rays. Uh,

0:13:28.880 --> 0:13:31.880
<v Speaker 1>they're just photons of a higher energy. But qualitatively they

0:13:31.960 --> 0:13:35.560
<v Speaker 1>seem different, right, And so before we understood a lot

0:13:35.600 --> 0:13:38.120
<v Speaker 1>more about how things worked, they we treated them like

0:13:38.160 --> 0:13:40.679
<v Speaker 1>different things. But that's that's the whole goal of physics, right,

0:13:40.720 --> 0:13:43.160
<v Speaker 1>is to take a bunch of disparate phenomena, things that

0:13:43.200 --> 0:13:46.920
<v Speaker 1>don't seem related, and discover that they're actually connected. They're

0:13:46.920 --> 0:13:49.480
<v Speaker 1>all just different parts of the same thing, different sides

0:13:49.480 --> 0:13:52.040
<v Speaker 1>of the same die. I guess they thought there were

0:13:52.160 --> 0:13:55.240
<v Speaker 1>different things because they they're made differently, right, Like you

0:13:55.320 --> 0:13:58.959
<v Speaker 1>make cather raise one way and you make visible light

0:13:59.000 --> 0:14:01.120
<v Speaker 1>another way, and you make gamma rays different way, and

0:14:01.160 --> 0:14:04.200
<v Speaker 1>so they thought, hey, these are just different things that

0:14:04.240 --> 0:14:06.280
<v Speaker 1>come out when you do these other things. Yeah, you

0:14:06.320 --> 0:14:08.640
<v Speaker 1>make them differently, and they behave differently, Like one of

0:14:08.679 --> 0:14:10.559
<v Speaker 1>them can penetrate through the wall and the other one

0:14:10.600 --> 0:14:13.320
<v Speaker 1>can't write. And so if you don't have a microscopic

0:14:13.400 --> 0:14:16.480
<v Speaker 1>understanding of it, it makes sense to categorize them differently. Um,

0:14:16.640 --> 0:14:18.480
<v Speaker 1>so it's pretty cool later when you stitch it all

0:14:18.480 --> 0:14:21.920
<v Speaker 1>together and realize that these are all just different flavors

0:14:21.960 --> 0:14:24.640
<v Speaker 1>of the same thing, or different colors quite literally of

0:14:24.680 --> 0:14:28.000
<v Speaker 1>the same thing. And gamma rays specifically are the very

0:14:28.120 --> 0:14:31.520
<v Speaker 1>very high edge of that spectrum. So anything that's you know,

0:14:31.600 --> 0:14:34.840
<v Speaker 1>like a million times more energetic than a visible photon,

0:14:35.480 --> 0:14:37.440
<v Speaker 1>you call it a gamma ray. It's not like a

0:14:37.480 --> 0:14:40.240
<v Speaker 1>hard cut off and not like a little below and like, sorry,

0:14:40.360 --> 0:14:42.040
<v Speaker 1>you don't get to be a gamma ray. You know,

0:14:42.040 --> 0:14:44.200
<v Speaker 1>it's sort of a rough thing, um, but there's no

0:14:44.720 --> 0:14:49.240
<v Speaker 1>upper limit. It's like a it's like a soft definition. Yeah,

0:14:49.360 --> 0:14:51.920
<v Speaker 1>that's what point does it? And the photon become trying

0:14:51.960 --> 0:14:55.760
<v Speaker 1>from a regular photon to ama. Well, you know, I

0:14:55.800 --> 0:14:59.040
<v Speaker 1>think photons would be insalted be called regular photons. You know,

0:14:59.040 --> 0:15:01.680
<v Speaker 1>they're all special Okay, they all can do something that

0:15:01.760 --> 0:15:05.600
<v Speaker 1>no other photon can do. That's right. Sorry, they're all bright,

0:15:05.680 --> 0:15:07.640
<v Speaker 1>shining points of light. Yeah. I mean, is there's some

0:15:07.680 --> 0:15:09.320
<v Speaker 1>colors that you like more than others? Or hey are

0:15:09.360 --> 0:15:14.880
<v Speaker 1>you you know, are you a colorist? But I've worked

0:15:14.920 --> 0:15:18.280
<v Speaker 1>with a lot of colorists. Yeah, that's true. You are

0:15:18.280 --> 0:15:21.520
<v Speaker 1>a cartoonists. You should be pro color man um. Yeah,

0:15:21.520 --> 0:15:23.840
<v Speaker 1>so you got radio waves the very very low edge,

0:15:23.880 --> 0:15:27.160
<v Speaker 1>and then you got um infrared right just below what

0:15:27.200 --> 0:15:28.840
<v Speaker 1>we can see. Then you've got the visible spectrum. The

0:15:28.920 --> 0:15:32.320
<v Speaker 1>radio waves are the bottom. Radio waves are the very

0:15:32.520 --> 0:15:35.840
<v Speaker 1>longest wavelengths are the lowest energy. Exactly the way you

0:15:35.880 --> 0:15:38.360
<v Speaker 1>said at the bottom makes it sound judgmental. You know,

0:15:38.920 --> 0:15:43.120
<v Speaker 1>radio ways are awesome, they're super powerful and fantastic and

0:15:43.440 --> 0:15:46.920
<v Speaker 1>the reasons we can see black holes and stuff like that. Um,

0:15:46.960 --> 0:15:48.760
<v Speaker 1>But yeah, radio waves are at the bottom in terms

0:15:48.760 --> 0:15:52.200
<v Speaker 1>of energy. Then you get infrared, then you get the

0:15:52.280 --> 0:15:56.160
<v Speaker 1>visible spectrum. Then you get X rays, right, and then

0:15:56.200 --> 0:15:58.320
<v Speaker 1>you get there just above the ultra violet, you get

0:15:58.400 --> 0:16:00.360
<v Speaker 1>X rays and then you get gamma rays. So emorys

0:16:00.400 --> 0:16:03.440
<v Speaker 1>are the hardest, fastest, most energetic kind of photon you

0:16:03.480 --> 0:16:06.400
<v Speaker 1>can have. But they're all photons, Like, they're all the

0:16:06.440 --> 0:16:11.240
<v Speaker 1>same particle through just kind of vibrating differently or the

0:16:11.400 --> 0:16:15.080
<v Speaker 1>different wavelength or sizes. What's the difference. Yeah, they're all photons.

0:16:15.120 --> 0:16:16.640
<v Speaker 1>They all travel at the speed of light. But the

0:16:16.640 --> 0:16:20.560
<v Speaker 1>difference is the frequency, right, how often they are wiggling. Right. Remember,

0:16:20.560 --> 0:16:25.520
<v Speaker 1>photons are vibrations of the electromagnetic field, right, and they

0:16:25.560 --> 0:16:28.520
<v Speaker 1>oscillate and the speed at which they oscillate that gives

0:16:28.520 --> 0:16:31.080
<v Speaker 1>you the frequency. Right, how many times per second do

0:16:31.160 --> 0:16:32.920
<v Speaker 1>they go up and down? Does they let the magnetic

0:16:32.920 --> 0:16:36.160
<v Speaker 1>fields go up and down? And they're all moving at

0:16:36.160 --> 0:16:40.560
<v Speaker 1>the speed of light? One radio photons moving at the

0:16:40.560 --> 0:16:43.040
<v Speaker 1>same speed as a gamma ray photon. That's right. If

0:16:43.080 --> 0:16:45.840
<v Speaker 1>you had a race, and you had a source of

0:16:45.960 --> 0:16:48.360
<v Speaker 1>radio waves and a source of gamma rays, and you

0:16:48.400 --> 0:16:50.480
<v Speaker 1>shot them at each other, they would have different energies

0:16:50.480 --> 0:16:53.360
<v Speaker 1>but move at the same speed. They all travel at

0:16:53.360 --> 0:16:55.200
<v Speaker 1>the speed of light, even if they have different energies.

0:16:55.240 --> 0:16:57.000
<v Speaker 1>That feels kind of weird, right, because you're used to

0:16:57.040 --> 0:16:59.800
<v Speaker 1>thinking of energy and speed is closely connected. But this

0:16:59.880 --> 0:17:02.040
<v Speaker 1>is something different. They have no mass and they travel

0:17:02.040 --> 0:17:04.520
<v Speaker 1>at the speed of light. Um, they all have the

0:17:04.560 --> 0:17:07.159
<v Speaker 1>same speed, but they have different energies, which means they

0:17:07.160 --> 0:17:10.760
<v Speaker 1>have different frequencies and different wavelengths. Right. The wavelength and

0:17:10.760 --> 0:17:14.440
<v Speaker 1>the frequency are closely connected. Higher the frequency, the shorter

0:17:14.560 --> 0:17:17.920
<v Speaker 1>the wavelength. And uh yeah, let's talk about that a

0:17:17.960 --> 0:17:33.800
<v Speaker 1>little bit more. But first quick break. Okay, so gamma

0:17:33.840 --> 0:17:37.240
<v Speaker 1>rays are photons, but they have not just a little bit,

0:17:37.320 --> 0:17:39.920
<v Speaker 1>but a lot more energy than the regular photons that

0:17:40.080 --> 0:17:43.760
<v Speaker 1>we see every day. That's right, a million times, that's yeah,

0:17:43.800 --> 0:17:45.879
<v Speaker 1>that's a lot. It's a lot. If I shot gamma

0:17:45.960 --> 0:17:48.639
<v Speaker 1>rays at you, they would deposit a lot more energy

0:17:48.680 --> 0:17:51.120
<v Speaker 1>in you than normal light, right, And also they can

0:17:51.119 --> 0:17:53.560
<v Speaker 1>penetrate into you much further, like, well it would, they

0:17:53.560 --> 0:17:56.239
<v Speaker 1>would deliver a million times more energy. Right, You need

0:17:56.280 --> 0:17:59.600
<v Speaker 1>a million photons to be equal to one gamma ray

0:17:59.640 --> 0:18:03.240
<v Speaker 1>photon exactly. And so gamma rays are dangerous. They can't

0:18:03.400 --> 0:18:06.200
<v Speaker 1>turn you into the Hulk probably, but they could give

0:18:06.240 --> 0:18:09.520
<v Speaker 1>you cancer, right, they can shatter your DNA and and

0:18:09.560 --> 0:18:11.680
<v Speaker 1>all sorts of crazy stuff inside your body. You don't

0:18:11.680 --> 0:18:14.600
<v Speaker 1>want gamma rays, Okay, So they're just regular photons, but

0:18:14.640 --> 0:18:17.600
<v Speaker 1>they're they're just an upper spectrum of light, that's right,

0:18:17.640 --> 0:18:20.200
<v Speaker 1>they're the high ended spectrum. They are dangerous, much more

0:18:20.240 --> 0:18:23.240
<v Speaker 1>dangerous than normal light because they can damage your DNA, right,

0:18:23.760 --> 0:18:27.400
<v Speaker 1>they can. They can cause errors in DNA which get copied,

0:18:27.440 --> 0:18:30.239
<v Speaker 1>and that's a big source of cancer. So what they

0:18:30.240 --> 0:18:32.640
<v Speaker 1>are is not very mysterious, right, Like we can make

0:18:32.640 --> 0:18:35.160
<v Speaker 1>them here on Earth, that's right, Yeah, exactly, we can

0:18:35.160 --> 0:18:38.080
<v Speaker 1>make gamma rays here on Earth. Um and gamma rays

0:18:38.080 --> 0:18:41.080
<v Speaker 1>are produced by radioactive elements all the time, right, they're

0:18:41.119 --> 0:18:45.160
<v Speaker 1>just high energy photons from radioactive decays. So there are

0:18:45.160 --> 0:18:48.840
<v Speaker 1>gamma rays around one of them just hit you right now. Um. Yes,

0:18:48.880 --> 0:18:51.760
<v Speaker 1>So gamma rays themselves not mysterious. We know all about them.

0:18:51.960 --> 0:18:55.359
<v Speaker 1>We can make them. Um. The question is what out

0:18:55.400 --> 0:18:59.400
<v Speaker 1>there might be making gamma rays. And that's the fascinating

0:18:59.400 --> 0:19:02.680
<v Speaker 1>part of the story. That's um the interesting mystery, right

0:19:03.080 --> 0:19:05.240
<v Speaker 1>is that we know the gamma rays are produced when

0:19:05.280 --> 0:19:07.639
<v Speaker 1>we do experience with with nuclear weapons. Right, you do,

0:19:07.720 --> 0:19:10.000
<v Speaker 1>you blow up a nuclear bomb, You're gonna produce a

0:19:10.040 --> 0:19:13.320
<v Speaker 1>lot of gamma rays. So when in the Cold War,

0:19:13.480 --> 0:19:16.359
<v Speaker 1>when we had trees with with with the Russians saying

0:19:16.600 --> 0:19:18.800
<v Speaker 1>no testing or whatever, we sent up a bunch of

0:19:18.840 --> 0:19:21.600
<v Speaker 1>satellites to verify that they weren't testing trying to detect

0:19:21.720 --> 0:19:26.159
<v Speaker 1>gamma rays from nuclear explosions. And um, I don't know

0:19:26.160 --> 0:19:27.840
<v Speaker 1>if they found that. They haven't released that. But what

0:19:27.920 --> 0:19:30.520
<v Speaker 1>they did discover is a bunch of gamma rays not

0:19:30.720 --> 0:19:33.320
<v Speaker 1>coming from the Soviet Union, not coming from somewhere else

0:19:33.359 --> 0:19:37.080
<v Speaker 1>on Earth, not coming from the mountain volcano layer of

0:19:37.119 --> 0:19:40.560
<v Speaker 1>some evil villain, but instead coming from deep in space.

0:19:42.080 --> 0:19:46.080
<v Speaker 1>So the mysteries that we're getting bombarded by gamma rays,

0:19:46.200 --> 0:19:49.240
<v Speaker 1>but we don't know, we didn't know really came from. Yeah.

0:19:49.280 --> 0:19:51.399
<v Speaker 1>And the really fascinating thing about them is that it's

0:19:51.440 --> 0:19:54.040
<v Speaker 1>not like a continual source. It's not just like you know,

0:19:54.080 --> 0:19:57.280
<v Speaker 1>the solar wind where it's just like constantly coming. They

0:19:57.280 --> 0:20:00.240
<v Speaker 1>come in bursts. And that's really interesting because it you

0:20:00.240 --> 0:20:04.399
<v Speaker 1>think like something happened, something created this, like some big

0:20:04.440 --> 0:20:08.640
<v Speaker 1>event occurred and must have produced this burst, right, And

0:20:08.680 --> 0:20:10.399
<v Speaker 1>that's a clue. It's like, what's going on out there

0:20:10.400 --> 0:20:13.320
<v Speaker 1>seems feels like a message or a clue about something

0:20:13.480 --> 0:20:16.480
<v Speaker 1>fascinating that's happening somewhere else in the universe. So what

0:20:16.520 --> 0:20:19.639
<v Speaker 1>do you mean by a burst? Like we we suddenly, um,

0:20:19.800 --> 0:20:22.080
<v Speaker 1>suddenly we're washed by a bunch of gamma rays and

0:20:22.080 --> 0:20:26.000
<v Speaker 1>then it stops. Yeah, and it's exactly like a huge

0:20:26.040 --> 0:20:27.800
<v Speaker 1>pile them come all at once, you know, it's like

0:20:27.840 --> 0:20:30.800
<v Speaker 1>a big flash in the sky, like quite literally a

0:20:30.840 --> 0:20:33.520
<v Speaker 1>big flash in the sky. And then the other fascinating

0:20:33.560 --> 0:20:36.119
<v Speaker 1>thing is that there are two kinds is like short

0:20:36.160 --> 0:20:39.040
<v Speaker 1>gamma ray bursts. One that ones that last much less

0:20:39.040 --> 0:20:41.560
<v Speaker 1>than a second, like less than half a second, and

0:20:41.560 --> 0:20:44.320
<v Speaker 1>then there's ones that last like twenty or thirty seconds,

0:20:44.920 --> 0:20:46.840
<v Speaker 1>um and it's not like a continuous range. It's not

0:20:46.880 --> 0:20:49.600
<v Speaker 1>like you know, every gamma ray burst is you know, um,

0:20:49.640 --> 0:20:52.480
<v Speaker 1>some somewhere less than thirty seconds, and there's a smooth distribution.

0:20:52.520 --> 0:20:56.000
<v Speaker 1>There's like two bumps if you made histogram, like a

0:20:56.000 --> 0:20:57.720
<v Speaker 1>lot of them. A lot of them peak at like

0:20:57.840 --> 0:20:59.600
<v Speaker 1>zero point three seconds, and a lot of them peak

0:20:59.600 --> 0:21:02.400
<v Speaker 1>it like the earty seconds. So there's definitely two kinds

0:21:02.440 --> 0:21:06.960
<v Speaker 1>of bursts happening. It kind of sounds like Morse quote exactly,

0:21:07.240 --> 0:21:10.600
<v Speaker 1>some very slow message. That's the exciting thing, Right, you

0:21:10.800 --> 0:21:12.920
<v Speaker 1>don't know what's creating this. You don't know is out

0:21:12.920 --> 0:21:14.960
<v Speaker 1>there making it, and it could be anything. It could

0:21:15.000 --> 0:21:17.359
<v Speaker 1>be like some new kind of star you never saw before,

0:21:17.560 --> 0:21:21.520
<v Speaker 1>or it could be some bizarre galactic race sending you

0:21:21.640 --> 0:21:27.080
<v Speaker 1>messages over decades, right, who knows? Planet Hulk. Yeah, because

0:21:27.320 --> 0:21:29.679
<v Speaker 1>it's they're not very common. It's not like they're happening

0:21:29.680 --> 0:21:32.800
<v Speaker 1>all the time, you know. Um, these days are estimated

0:21:32.840 --> 0:21:35.480
<v Speaker 1>that we about what about one per day hits the Earth.

0:21:35.880 --> 0:21:39.879
<v Speaker 1>So we first to take these with cold warp satellites. Yeah,

0:21:39.920 --> 0:21:42.480
<v Speaker 1>exactly what do people think, Like, did they think was

0:21:42.520 --> 0:21:44.639
<v Speaker 1>a glitch or at first they had no idea they're like,

0:21:44.680 --> 0:21:47.000
<v Speaker 1>what you know. First, I'm sure they thought, are the

0:21:47.080 --> 0:21:49.720
<v Speaker 1>Soviets testing and outer space? Maybe they're already at the

0:21:49.720 --> 0:21:52.719
<v Speaker 1>Moon or something. Right, Um, we could tell they were

0:21:52.720 --> 0:21:54.320
<v Speaker 1>coming from out of space. Yeah, we could tell they

0:21:54.320 --> 0:21:56.440
<v Speaker 1>were coming from outer space. Absolutely, we could tell the

0:21:56.480 --> 0:21:58.639
<v Speaker 1>direction of And you know, they didn't release a lot

0:21:58.720 --> 0:22:01.280
<v Speaker 1>of details because all this in nation comes from like

0:22:01.600 --> 0:22:06.399
<v Speaker 1>classified satellites. Um, as scientists, we sometimes wonder, like we

0:22:06.440 --> 0:22:08.520
<v Speaker 1>spend all this money trying to get satellites up in

0:22:08.560 --> 0:22:12.320
<v Speaker 1>space to answer scientists scientific questions, but the budget for

0:22:12.520 --> 0:22:16.439
<v Speaker 1>defense is much bigger, and there's a huge network of

0:22:16.520 --> 0:22:19.920
<v Speaker 1>defense satellites listening for stuff and telescopes and all sorts

0:22:19.920 --> 0:22:22.440
<v Speaker 1>of stuff, and we wonder sometimes like could we use

0:22:22.480 --> 0:22:25.159
<v Speaker 1>that network for science, Like it's so much bigger and

0:22:25.200 --> 0:22:28.080
<v Speaker 1>more powerful. Of course it's not designed to do science,

0:22:28.119 --> 0:22:31.040
<v Speaker 1>but sometimes it can accidentally do signs, and that's what

0:22:31.119 --> 0:22:33.360
<v Speaker 1>happened here. So we don't know a lot of details

0:22:33.400 --> 0:22:37.439
<v Speaker 1>about the technical capabilities of these Department of Defense satellites.

0:22:37.920 --> 0:22:40.760
<v Speaker 1>But after a few years, the d D realized, Okay,

0:22:40.760 --> 0:22:43.359
<v Speaker 1>this is not Russian's this is something weird and interesting

0:22:43.359 --> 0:22:45.879
<v Speaker 1>from outer space, and so they declassified this data and

0:22:45.880 --> 0:22:48.199
<v Speaker 1>shared it with the scientific community, and that's what they

0:22:48.280 --> 0:22:50.280
<v Speaker 1>used to discover what they were. Yeah, that was the

0:22:50.320 --> 0:22:52.040
<v Speaker 1>first hint. And then the scientists were like, we have

0:22:52.119 --> 0:22:54.560
<v Speaker 1>no idea, what is this. Let's study it some more

0:22:55.000 --> 0:22:57.040
<v Speaker 1>and there's a lesson. They're also folks like if the

0:22:57.080 --> 0:23:00.280
<v Speaker 1>government did discover aliens, they would probably turn it over

0:23:00.320 --> 0:23:02.840
<v Speaker 1>to the scientific community to help them figure it out. Right,

0:23:02.880 --> 0:23:07.639
<v Speaker 1>that's basically what happened here, right. Weird enough Hollywood movies, Daniel,

0:23:07.680 --> 0:23:11.320
<v Speaker 1>and they always try to cover it up. Yeah, I

0:23:11.359 --> 0:23:13.320
<v Speaker 1>should be a consultant in some of those Hollywood movies

0:23:13.320 --> 0:23:21.240
<v Speaker 1>because I have better ideas. So then the scientific community said, well, wow,

0:23:21.280 --> 0:23:23.159
<v Speaker 1>we have no idea what could make this And it

0:23:23.200 --> 0:23:24.880
<v Speaker 1>was really it was a puzzle for a long time.

0:23:25.400 --> 0:23:28.520
<v Speaker 1>So um, because it's it's uh, they knew it wasn't

0:23:28.560 --> 0:23:31.639
<v Speaker 1>coming from the sun, right, And these these weren't just

0:23:31.680 --> 0:23:34.960
<v Speaker 1>like a little small burst. These are really bright bursts, right,

0:23:35.000 --> 0:23:37.320
<v Speaker 1>that's right, They're really bright. And so the first thing

0:23:37.359 --> 0:23:39.480
<v Speaker 1>you do in astronomy when you see a signal you

0:23:39.520 --> 0:23:41.119
<v Speaker 1>don't know what it is, you try to figure out

0:23:41.160 --> 0:23:43.680
<v Speaker 1>where it's coming from. Right, you pointed in the sky,

0:23:43.840 --> 0:23:45.960
<v Speaker 1>if you can connect it with something in this in

0:23:46.000 --> 0:23:48.119
<v Speaker 1>the sky, then you think, oh, it's came from there, right,

0:23:48.160 --> 0:23:50.400
<v Speaker 1>pretty simple stuff. So they know it didn't come from

0:23:50.400 --> 0:23:53.439
<v Speaker 1>the Sun. They also didn't seem to be coming from

0:23:53.480 --> 0:23:57.080
<v Speaker 1>anything in our galaxy. Like we know where we are

0:23:57.160 --> 0:24:00.520
<v Speaker 1>relative to the galaxy, and so some signals being generated

0:24:00.520 --> 0:24:03.040
<v Speaker 1>by some like new kind of star or some activity

0:24:03.080 --> 0:24:05.800
<v Speaker 1>in our galaxy, it's going to be mostly coming from

0:24:05.880 --> 0:24:08.159
<v Speaker 1>the direction of the center of the galaxy or the

0:24:08.160 --> 0:24:11.760
<v Speaker 1>plane of the galaxy. Right, But these things were coming

0:24:11.760 --> 0:24:16.040
<v Speaker 1>from every direction, like random directions. So suggest that's not

0:24:16.200 --> 0:24:19.000
<v Speaker 1>something happening in our galaxy, but something coming to us

0:24:19.320 --> 0:24:24.200
<v Speaker 1>from other galaxies. Wow. So for something to be that

0:24:24.280 --> 0:24:26.840
<v Speaker 1>far away and for us to feel it and to

0:24:26.920 --> 0:24:30.200
<v Speaker 1>get so many of these photons, it's like at the source,

0:24:30.240 --> 0:24:31.920
<v Speaker 1>it must be huge, right, Like it must be like

0:24:31.960 --> 0:24:35.800
<v Speaker 1>a huge bright explosion. Yeah. Absolutely, It's kind of scary

0:24:35.840 --> 0:24:38.520
<v Speaker 1>to think about because these gamma ray bursts they're like

0:24:38.600 --> 0:24:41.520
<v Speaker 1>as powerful as like a star, you know, when when

0:24:41.520 --> 0:24:44.120
<v Speaker 1>they hit us, the light from the gamma ray burst

0:24:44.200 --> 0:24:45.800
<v Speaker 1>is about as much energy as the life from a

0:24:45.840 --> 0:24:49.520
<v Speaker 1>star in our galaxy. Right. But but if it but

0:24:49.560 --> 0:24:53.040
<v Speaker 1>if it came from really far away then, I mean

0:24:53.080 --> 0:24:55.960
<v Speaker 1>that must have and it probably sprayed that much in

0:24:56.000 --> 0:24:58.280
<v Speaker 1>all directions. Right, Well, we actually don't know about that.

0:24:58.320 --> 0:25:00.880
<v Speaker 1>We don't know um that much about how they're made,

0:25:00.920 --> 0:25:04.320
<v Speaker 1>So it could be like um like blaze oars and

0:25:04.359 --> 0:25:08.240
<v Speaker 1>pulsars that they're concentrated in in some directions, like along

0:25:08.280 --> 0:25:11.720
<v Speaker 1>the magnetic polls. But whatever it is, they're super bright

0:25:11.800 --> 0:25:15.679
<v Speaker 1>at the source because remember, other galaxies are crazy far away,

0:25:15.800 --> 0:25:19.000
<v Speaker 1>Like other stars are far away inside our galaxy, but

0:25:19.119 --> 0:25:22.119
<v Speaker 1>other galaxies are like an order of magnitude further away.

0:25:22.200 --> 0:25:24.879
<v Speaker 1>So to even see those galaxies as hard, you have

0:25:24.960 --> 0:25:27.600
<v Speaker 1>to add up all the hundreds of billions of stars

0:25:27.600 --> 0:25:30.160
<v Speaker 1>in those galaxies just to see them. So to see

0:25:30.400 --> 0:25:33.240
<v Speaker 1>one object from that galaxy being as bright as a

0:25:33.280 --> 0:25:36.119
<v Speaker 1>star in our galaxy, I mean you have to do

0:25:36.160 --> 0:25:38.880
<v Speaker 1>the math. That's crazy, Um no, you I think, yeah,

0:25:38.880 --> 0:25:40.520
<v Speaker 1>you were telling me earlier. You did the math, and

0:25:40.520 --> 0:25:45.840
<v Speaker 1>it's about one million trillion times brighter than the Sun exactly.

0:25:45.960 --> 0:25:48.320
<v Speaker 1>That's how far away these things are. In order for

0:25:48.400 --> 0:25:50.800
<v Speaker 1>us to see them as bright as a star in

0:25:50.840 --> 0:25:54.399
<v Speaker 1>our galaxy, they have to be a million trillion times

0:25:54.440 --> 0:25:56.480
<v Speaker 1>brighter than the sun. But that's a fun thing to say,

0:25:56.480 --> 0:26:00.520
<v Speaker 1>isn't it a million trillion? Like say axillion? You know,

0:26:00.800 --> 0:26:02.919
<v Speaker 1>I don't even bother. I don't even know how many zeros.

0:26:02.920 --> 0:26:06.520
<v Speaker 1>It is a lot like bony swoops of ice cream?

0:26:06.560 --> 0:26:11.960
<v Speaker 1>Would you like a million trillion? Just a whole bunch

0:26:13.800 --> 0:26:16.600
<v Speaker 1>more than more than a million. It's it's a million

0:26:16.640 --> 0:26:19.880
<v Speaker 1>times a trillion. It's a million times a trillion times

0:26:20.040 --> 0:26:24.080
<v Speaker 1>the Sun, which is already really bright. You know. That

0:26:24.320 --> 0:26:26.360
<v Speaker 1>means there's stuff going on in the universe out there

0:26:26.400 --> 0:26:29.840
<v Speaker 1>all the time. That's a million trillion times brighter than

0:26:29.880 --> 0:26:32.879
<v Speaker 1>the Sun. Yeah, exactly. And so we think they come

0:26:32.920 --> 0:26:35.160
<v Speaker 1>from other galaxies. But that's a bit of a puzzle, right,

0:26:35.200 --> 0:26:38.760
<v Speaker 1>Like why only from other galaxies and not from hours? Um,

0:26:38.800 --> 0:26:40.600
<v Speaker 1>how are they? What are these things that are making

0:26:40.600 --> 0:26:43.200
<v Speaker 1>these gamma ray bers? How can they be so crazy powerful?

0:26:43.960 --> 0:26:46.800
<v Speaker 1>You mean we should be if they were common in

0:26:46.840 --> 0:26:49.560
<v Speaker 1>our galaxy, we would be getting them a lot more

0:26:50.080 --> 0:26:55.040
<v Speaker 1>from the sides of the galaxy, right, like we would notice. Yeah, well,

0:26:55.080 --> 0:26:58.880
<v Speaker 1>either they don't happen very often, in which case it's

0:26:58.920 --> 0:27:02.000
<v Speaker 1>more likely to see them from other galaxies than from ours, right,

0:27:02.040 --> 0:27:06.120
<v Speaker 1>because there are more other galaxies than ours, right, um,

0:27:06.280 --> 0:27:09.080
<v Speaker 1>or our galaxy is different from other galaxies in some way,

0:27:09.119 --> 0:27:12.080
<v Speaker 1>which is why we don't see them from our galaxy. Well, well,

0:27:12.160 --> 0:27:14.120
<v Speaker 1>I was You were telling me also that there's more

0:27:14.240 --> 0:27:17.720
<v Speaker 1>energy in one second of these gamma ray burs than

0:27:17.920 --> 0:27:20.520
<v Speaker 1>possibly all the energy that our Sun will give in

0:27:20.600 --> 0:27:23.600
<v Speaker 1>its entire life. That's right, It's a huge amount of energy.

0:27:24.040 --> 0:27:26.159
<v Speaker 1>This is one of the funnest things about space and

0:27:26.200 --> 0:27:29.120
<v Speaker 1>about astronomy, right, it's just the crazy numbers, you know, like,

0:27:29.480 --> 0:27:32.280
<v Speaker 1>can you wrap your mind around how much energy is

0:27:32.280 --> 0:27:35.000
<v Speaker 1>going to be put out by the Sun over billions

0:27:35.000 --> 0:27:37.399
<v Speaker 1>of years. I don't think it's possible for humans to

0:27:37.440 --> 0:27:39.359
<v Speaker 1>grasp this kind of stuff. I mean, even just the

0:27:39.400 --> 0:27:42.679
<v Speaker 1>time scale billions of years. You know, it's hard for

0:27:42.800 --> 0:27:45.359
<v Speaker 1>humans that live for such a flicker to understand and

0:27:45.400 --> 0:27:49.080
<v Speaker 1>then integrate all the energy of this million earth ball

0:27:49.160 --> 0:27:52.480
<v Speaker 1>of fire and then focus that all into one second.

0:27:52.600 --> 0:27:54.800
<v Speaker 1>I mean, it's uh, it burns a hole in my mind.

0:27:55.840 --> 0:27:58.720
<v Speaker 1>It turns into the Hulk. Yeah, exactly. If you took

0:27:58.760 --> 0:28:02.399
<v Speaker 1>the Earth right and you collided it with the anti Earth,

0:28:02.480 --> 0:28:05.159
<v Speaker 1>like a antimatter version of the Earth, right, so you

0:28:05.240 --> 0:28:08.040
<v Speaker 1>converted all of the mass from the Earth into energy.

0:28:08.400 --> 0:28:10.960
<v Speaker 1>You know, it's it's it's crazy powerful. Right. For example,

0:28:11.000 --> 0:28:13.840
<v Speaker 1>if you collided to raisins out of raisin and an

0:28:13.840 --> 0:28:16.200
<v Speaker 1>anti raisin, it would have as much energy as a

0:28:16.280 --> 0:28:18.600
<v Speaker 1>nuclear weapon. Right, So it's a huge amount of energy

0:28:18.640 --> 0:28:20.960
<v Speaker 1>is stored in a raisin. Now imagine doing that for

0:28:21.000 --> 0:28:23.480
<v Speaker 1>the Earth. Right, You'd have to do that for a

0:28:23.760 --> 0:28:27.240
<v Speaker 1>hundred copies of the Earth to get as much energy

0:28:27.320 --> 0:28:30.439
<v Speaker 1>as is stored in these gamma ray bursts. What if

0:28:30.440 --> 0:28:33.880
<v Speaker 1>you collide a hulk in an anti hulk they both

0:28:33.920 --> 0:28:38.600
<v Speaker 1>get piste off. Yeah, dude's mash it's each each other

0:28:39.880 --> 0:28:43.480
<v Speaker 1>and and anti smash they would you know up as well?

0:28:43.520 --> 0:28:45.440
<v Speaker 1>I don't know, but you are generating a huge list

0:28:45.480 --> 0:28:47.320
<v Speaker 1>of great ideas for the next Marvel movies. I hope

0:28:47.320 --> 0:28:51.200
<v Speaker 1>you're you're patenting these? Yeah yeah, Mark Ruffo will call me.

0:28:53.080 --> 0:28:56.160
<v Speaker 1>But yeah, So okay, let's so let's get into what

0:28:56.360 --> 0:29:00.120
<v Speaker 1>could be generating these game ray bers and are they dangerous?

0:29:00.240 --> 0:29:15.680
<v Speaker 1>But let's take a quick break. All right, So we're

0:29:15.680 --> 0:29:18.960
<v Speaker 1>talking about gamma ray berths, which are different than Billy

0:29:19.000 --> 0:29:23.040
<v Speaker 1>ray shires. We've established that and that they're also just

0:29:23.160 --> 0:29:26.280
<v Speaker 1>regular photons but super highly energetic, and we're getting these

0:29:26.320 --> 0:29:29.600
<v Speaker 1>crazy births from out of space. So, Daniel, what could

0:29:29.600 --> 0:29:33.040
<v Speaker 1>be causing these births? What could be out there making

0:29:33.080 --> 0:29:36.440
<v Speaker 1>these that we were feeling them so so um energetic

0:29:36.480 --> 0:29:39.360
<v Speaker 1>here on Earth. Well, the short answer is we don't

0:29:39.440 --> 0:29:43.360
<v Speaker 1>really know very well. We have now recently some hypotheses

0:29:43.440 --> 0:29:45.840
<v Speaker 1>that might work, but the truth is we don't really

0:29:45.880 --> 0:29:49.440
<v Speaker 1>know um. And remember, there's two kinds of gamma ray bursus,

0:29:49.560 --> 0:29:52.719
<v Speaker 1>the short and the long. Short last less than a second,

0:29:52.880 --> 0:29:55.800
<v Speaker 1>and the long last like thirty seconds. And the best

0:29:55.840 --> 0:29:58.280
<v Speaker 1>guesses these days are that the short ones are due

0:29:58.320 --> 0:30:01.520
<v Speaker 1>to neutron stars that are in a binary system, so

0:30:01.520 --> 0:30:04.360
<v Speaker 1>they're orbiting each other, and when they do this, they

0:30:04.400 --> 0:30:07.120
<v Speaker 1>lose energy slowly so that they rotate around each other

0:30:07.120 --> 0:30:09.640
<v Speaker 1>and get closer and closer and closer and eventually collide.

0:30:10.000 --> 0:30:13.080
<v Speaker 1>And this is exciting stuff astronomically, because we recently saw

0:30:13.160 --> 0:30:16.640
<v Speaker 1>like gravitational waves coming from neutron star collisions and we

0:30:16.680 --> 0:30:19.480
<v Speaker 1>confirmed that like all of the gold in the universe

0:30:19.600 --> 0:30:22.400
<v Speaker 1>is probably made in neutron star collisions and all sorts

0:30:22.400 --> 0:30:25.720
<v Speaker 1>of crazy stuff. But the we think it might also

0:30:25.840 --> 0:30:28.400
<v Speaker 1>produce these gamma ray bursts because it's a huge amount

0:30:28.400 --> 0:30:30.920
<v Speaker 1>of energy and if you read the details about it,

0:30:30.920 --> 0:30:33.520
<v Speaker 1>it's crazy. That means that there's a short birth. Right,

0:30:33.560 --> 0:30:37.000
<v Speaker 1>there's their point three seconds long, and you're saying they generate, Like,

0:30:37.040 --> 0:30:39.960
<v Speaker 1>that's how fast these neutron stars are crashing into each other,

0:30:40.440 --> 0:30:43.240
<v Speaker 1>the whole thing that's about point three seconds. No, it's um.

0:30:43.280 --> 0:30:46.760
<v Speaker 1>The bursts itself, they think comes from the crust of

0:30:46.800 --> 0:30:51.720
<v Speaker 1>the neutron stars um being crushed by the gravitational pressure

0:30:51.720 --> 0:30:53.920
<v Speaker 1>from the other neutron stars. Remember, if you're close to

0:30:53.920 --> 0:30:56.600
<v Speaker 1>a really heavy object, you get these tidal forces because

0:30:56.600 --> 0:30:59.520
<v Speaker 1>gravity acts differently on things further away and closer up,

0:30:59.560 --> 0:31:02.640
<v Speaker 1>so you basically they get massaged. So two neutron stars

0:31:02.640 --> 0:31:06.080
<v Speaker 1>are like massaging each other just before they collide, which

0:31:06.120 --> 0:31:10.320
<v Speaker 1>is making the crust of them um basically shake and crack.

0:31:10.760 --> 0:31:13.600
<v Speaker 1>So you're getting these like earthquakes on the surface of

0:31:13.600 --> 0:31:17.240
<v Speaker 1>neutron stars just before they collide. That might be generating

0:31:17.280 --> 0:31:19.840
<v Speaker 1>these crazy fast bursts of gamma rays. I mean, it

0:31:19.880 --> 0:31:22.080
<v Speaker 1>sounds like science fiction, right. If I pitched that to Marvel,

0:31:22.120 --> 0:31:24.120
<v Speaker 1>they'd be like, that's sorry, that's too far out there,

0:31:24.680 --> 0:31:27.360
<v Speaker 1>But we think that's actually happening. It's really like you're

0:31:27.440 --> 0:31:30.800
<v Speaker 1>colliding to suns. Right, you're exactly. They get neutron star

0:31:30.960 --> 0:31:33.160
<v Speaker 1>taking a neutron star and used to smash them together

0:31:33.280 --> 0:31:36.560
<v Speaker 1>and in that point three seconds it explodes, right. Yeah,

0:31:36.560 --> 0:31:38.400
<v Speaker 1>But I have to remind you that our previous episode

0:31:38.400 --> 0:31:41.600
<v Speaker 1>about neutron stars, you complain that neutron stars aren't really stars.

0:31:41.640 --> 0:31:46.120
<v Speaker 1>They should just be called neutron balls because they don't glow. Okay,

0:31:46.120 --> 0:31:49.880
<v Speaker 1>so when you smash the balls together, that's where you

0:31:49.920 --> 0:31:51.400
<v Speaker 1>get there. And I have to say a lot of

0:31:51.440 --> 0:31:53.640
<v Speaker 1>our listeners on Twitter agreed with you that they should

0:31:53.640 --> 0:31:55.920
<v Speaker 1>be called balls. Yeah, exactly, they should be demoted from

0:31:55.920 --> 0:31:58.640
<v Speaker 1>starts to balls. Yeah. You sound surprised that people on

0:31:58.680 --> 0:32:01.720
<v Speaker 1>Twitter agree with me. I'm surprised that people it's on

0:32:01.720 --> 0:32:08.360
<v Speaker 1>Twitter agree with anybody. Congratulations, you've unified social media with overalls.

0:32:08.440 --> 0:32:15.720
<v Speaker 1>Yeah exactly. We have located a few of them, like

0:32:15.800 --> 0:32:18.600
<v Speaker 1>neutron star collisions. We can see in other ways. Right,

0:32:18.840 --> 0:32:22.040
<v Speaker 1>we can see them from their gravitational wave emissions that

0:32:22.160 --> 0:32:24.320
<v Speaker 1>that's pretty rare, but we can see them from the

0:32:24.320 --> 0:32:27.200
<v Speaker 1>bright flashes of visible light that they produce. And so

0:32:27.280 --> 0:32:29.840
<v Speaker 1>the Trick has been watching these things for years and

0:32:29.960 --> 0:32:33.680
<v Speaker 1>basically constructing dedicated satellites that are looking for these things.

0:32:33.960 --> 0:32:35.760
<v Speaker 1>And the key is that they don't last very long.

0:32:35.960 --> 0:32:37.640
<v Speaker 1>So what you want to do is as soon as

0:32:37.640 --> 0:32:39.400
<v Speaker 1>you see one, you've got to point all your good

0:32:39.400 --> 0:32:42.480
<v Speaker 1>telescopes at it. So the science community become much better

0:32:42.520 --> 0:32:45.320
<v Speaker 1>at that building dedicated telescopes that look for these things,

0:32:45.360 --> 0:32:47.880
<v Speaker 1>and then everybody swivels over to look at it at

0:32:47.880 --> 0:32:50.680
<v Speaker 1>the same time, which gives you a good review of it.

0:32:50.800 --> 0:32:53.560
<v Speaker 1>But you only have points three seconds, yeah, exactly. You

0:32:54.000 --> 0:32:56.640
<v Speaker 1>gotta be fast, um for these really fast ones. And

0:32:56.680 --> 0:32:59.200
<v Speaker 1>so some of these telescopes are all hooked up, like

0:32:59.280 --> 0:33:02.040
<v Speaker 1>the firm me tell lescope that's orbiting the Earth has

0:33:02.040 --> 0:33:04.960
<v Speaker 1>a gamma ray burst detector and when it's when it

0:33:05.040 --> 0:33:07.200
<v Speaker 1>finds something and it immediately sends a message. And then

0:33:07.240 --> 0:33:10.520
<v Speaker 1>telescopes on Earth point in that direction and try to capture, um,

0:33:10.600 --> 0:33:12.440
<v Speaker 1>you know, the last bits of the of the burst

0:33:12.520 --> 0:33:15.880
<v Speaker 1>before it disappears, and also to capture anything else coming

0:33:15.960 --> 0:33:18.160
<v Speaker 1>from that direction. And that's where we got these clues.

0:33:18.560 --> 0:33:21.240
<v Speaker 1>We started watching the guy more carefully and seeing what

0:33:21.320 --> 0:33:23.960
<v Speaker 1>else was coming from the direction of the gamma ray bursts,

0:33:24.120 --> 0:33:26.640
<v Speaker 1>and that gave people ideas about what could be happening

0:33:26.680 --> 0:33:28.760
<v Speaker 1>that could be causing them. So you get an idea like, oh,

0:33:28.760 --> 0:33:31.040
<v Speaker 1>maybe it's neutron stars, in which case we should see

0:33:31.080 --> 0:33:33.320
<v Speaker 1>this and that and the other thing also, And then

0:33:33.320 --> 0:33:35.560
<v Speaker 1>they started to pick those things up. Okay, so that's

0:33:35.600 --> 0:33:37.840
<v Speaker 1>the short birds, that's where they we think they come from.

0:33:37.880 --> 0:33:40.840
<v Speaker 1>What about the long burst, the thirty second ones? Yeah,

0:33:40.840 --> 0:33:46.080
<v Speaker 1>the long bursts come from super duper supernova's right? Um? Yeah,

0:33:47.440 --> 0:33:51.800
<v Speaker 1>super duper supernovas. Is that the technical that like a

0:33:51.840 --> 0:33:56.160
<v Speaker 1>million trillion supernovas, that's a super duper ice cream sunday.

0:33:56.240 --> 0:33:59.880
<v Speaker 1>You know, the technical term is a hypernova hypernova? Yeah,

0:34:00.200 --> 0:34:04.240
<v Speaker 1>oh man, but I prefer superduper supernova because it sounds

0:34:04.240 --> 0:34:07.000
<v Speaker 1>better than supernova. So they're not just a supernova. They're

0:34:07.040 --> 0:34:11.279
<v Speaker 1>like extra special, the extra special, extra big big implosions.

0:34:11.719 --> 0:34:14.560
<v Speaker 1>And this is still something that's not very well understood. Um,

0:34:14.600 --> 0:34:17.440
<v Speaker 1>you know, why do some supernovas produce gamma ray bursts

0:34:17.440 --> 0:34:20.520
<v Speaker 1>and some don't. But they did this modeling and they said, Okay,

0:34:20.560 --> 0:34:23.160
<v Speaker 1>if there is a big supernova, then we expect that

0:34:23.280 --> 0:34:25.759
<v Speaker 1>after the gamma ray bursts, we should see a bunch

0:34:25.800 --> 0:34:29.279
<v Speaker 1>of X rays because the gas nearby the supernova is

0:34:29.280 --> 0:34:31.520
<v Speaker 1>going to collide and then emit, and so they did

0:34:31.560 --> 0:34:34.480
<v Speaker 1>some complicated modeling and made predictions, and in fact they

0:34:34.520 --> 0:34:38.520
<v Speaker 1>see this afterglow, after the after these long gamma ray bursts,

0:34:38.560 --> 0:34:41.400
<v Speaker 1>they see X rays. So those are slightly lower energy

0:34:41.480 --> 0:34:44.480
<v Speaker 1>photons in the spectrum that they expect if it was

0:34:44.520 --> 0:34:48.160
<v Speaker 1>a supernova. So it partially answers the question because it

0:34:48.160 --> 0:34:51.000
<v Speaker 1>tells us these long gamma ray bursts probably come from

0:34:51.040 --> 0:34:54.480
<v Speaker 1>these crazy hypernovas. But we have hypernovas in the Milky Way,

0:34:54.520 --> 0:34:56.960
<v Speaker 1>and there's lots of hypernovas and not that many gamma

0:34:57.040 --> 0:34:59.360
<v Speaker 1>ray birsts. So is it like a special kind of

0:34:59.440 --> 0:35:02.719
<v Speaker 1>hypernova or only in some cases, or that's the kind

0:35:02.719 --> 0:35:04.960
<v Speaker 1>of thing. They're still trying to figure out what you're saying,

0:35:05.120 --> 0:35:10.839
<v Speaker 1>we need another term special super duper supernova, all hypernovas

0:35:10.880 --> 0:35:12.440
<v Speaker 1>are special or he I don't know why you have

0:35:12.480 --> 0:35:15.480
<v Speaker 1>to be so judgmental today. What's next? Or you can

0:35:15.520 --> 0:35:19.160
<v Speaker 1>have to call go for like hyper special, extra cool,

0:35:19.840 --> 0:35:25.719
<v Speaker 1>super califragilistic on top super dupernova. Yeah, so it's it's

0:35:25.760 --> 0:35:28.120
<v Speaker 1>still a puzzle. We don't understand it, right, we don't

0:35:28.200 --> 0:35:31.879
<v Speaker 1>understand why they made Sometimes um, some people think that

0:35:31.880 --> 0:35:34.560
<v Speaker 1>that if a supernova collapses like in a certain way,

0:35:34.640 --> 0:35:37.120
<v Speaker 1>then it creates this cloud of stuff around it which

0:35:37.120 --> 0:35:39.719
<v Speaker 1>absorbs the gamma rays and other times the gamma rays

0:35:39.760 --> 0:35:42.440
<v Speaker 1>poked through and then shoot out everywhere else. But it

0:35:42.440 --> 0:35:45.640
<v Speaker 1>would make sense that a supernova or killernova or hypernova

0:35:45.719 --> 0:35:48.319
<v Speaker 1>or whatever could generate this much energy because that's a

0:35:48.400 --> 0:35:52.000
<v Speaker 1>huge event, right, these massive stars imploding, So that that

0:35:52.000 --> 0:35:53.719
<v Speaker 1>definitely could explain it. I feel like next time you

0:35:53.719 --> 0:35:55.840
<v Speaker 1>should start a little bit more modestly so that you

0:35:55.880 --> 0:35:59.759
<v Speaker 1>have room to grow. You known, you discover something big

0:36:00.000 --> 0:36:03.360
<v Speaker 1>is called like a modest nova or like a just

0:36:03.440 --> 0:36:07.040
<v Speaker 1>a regular note, you have room to grow. No, I

0:36:07.080 --> 0:36:09.680
<v Speaker 1>like going the way McDonald's went for their drink sizes.

0:36:09.719 --> 0:36:11.960
<v Speaker 1>You know, you start with medium, which is already huge,

0:36:13.080 --> 0:36:17.800
<v Speaker 1>and then you escalate. Um. Yeah, exactly, And so that's

0:36:17.840 --> 0:36:20.759
<v Speaker 1>a that's probably what's causing it, but we don't really

0:36:20.840 --> 0:36:24.120
<v Speaker 1>understand it in detail, and it's important that we understand

0:36:24.120 --> 0:36:26.160
<v Speaker 1>it because we want to understand, like, is one of

0:36:26.200 --> 0:36:28.279
<v Speaker 1>these things going to happen in the middleky way? How

0:36:28.280 --> 0:36:30.040
<v Speaker 1>often are these things going to be hitting us? Do

0:36:30.120 --> 0:36:33.440
<v Speaker 1>we have to worry? So it's important to understand this stuff. Yeah,

0:36:33.520 --> 0:36:35.719
<v Speaker 1>it's weird that there would be things that were not

0:36:35.960 --> 0:36:39.440
<v Speaker 1>we can't quite explain out there. Yeah, exactly, especially things

0:36:39.480 --> 0:36:42.680
<v Speaker 1>that could kill us. Right, So it's like, I think

0:36:42.719 --> 0:36:46.160
<v Speaker 1>it's worth funding politicians out there with the purse strings,

0:36:46.200 --> 0:36:49.080
<v Speaker 1>you know, maybe by one less fighter jet and to

0:36:49.200 --> 0:36:51.759
<v Speaker 1>pay for another telescope to look at gamma rays. Wait,

0:36:51.800 --> 0:36:54.640
<v Speaker 1>so could these things kill us? Or I think you're

0:36:54.640 --> 0:36:57.560
<v Speaker 1>telling me earlier that you know, if the right concentration

0:36:57.640 --> 0:37:00.680
<v Speaker 1>hits us at the right moment, it could really fried

0:37:00.880 --> 0:37:04.919
<v Speaker 1>and turns into toast. Yeah, exactly. The key is how

0:37:05.000 --> 0:37:08.680
<v Speaker 1>far away it happens, right, So, gamma ray bursts from

0:37:08.719 --> 0:37:11.399
<v Speaker 1>other galaxies, we're far enough away that by the time

0:37:11.400 --> 0:37:14.400
<v Speaker 1>it gets here, you know, those gamma rays are filling

0:37:14.440 --> 0:37:19.040
<v Speaker 1>out a sphere that's the size of the distance between galaxies.

0:37:19.280 --> 0:37:21.120
<v Speaker 1>So it's a huge number of gamma rays, a lot

0:37:21.120 --> 0:37:23.520
<v Speaker 1>of energy, but it's spread out over a huge sphere.

0:37:24.080 --> 0:37:27.560
<v Speaker 1>If a gamma ray burst happens nearby, yikes, you know,

0:37:27.920 --> 0:37:31.320
<v Speaker 1>a gamma ray burst could basically sterilize an entire solar system.

0:37:31.360 --> 0:37:34.399
<v Speaker 1>If it happened nearby, that would be pretty we would

0:37:34.400 --> 0:37:36.919
<v Speaker 1>literally be toast. We would what what would the Earth

0:37:37.680 --> 0:37:39.560
<v Speaker 1>look like? Well, it would be like a flash sunburn,

0:37:39.600 --> 0:37:41.480
<v Speaker 1>wouldn't it Like half the Earth would be okay, but

0:37:41.520 --> 0:37:45.160
<v Speaker 1>the other half would be toast. Yeah, exactly half the

0:37:45.160 --> 0:37:47.399
<v Speaker 1>Earth would be totally fried and the other half would

0:37:47.400 --> 0:37:50.799
<v Speaker 1>be okay. Um, yeah, that that's exactly what happened. And

0:37:50.840 --> 0:37:53.280
<v Speaker 1>it depends again on the intensity. If it's really really intense,

0:37:53.719 --> 0:37:55.279
<v Speaker 1>you know, then it's going to get down to the

0:37:55.360 --> 0:37:58.200
<v Speaker 1>atmosphere and we're all gonna either get fried or get

0:37:58.280 --> 0:38:02.920
<v Speaker 1>cancer or die pretty quick. Um. If it's slightly less intense, right,

0:38:03.160 --> 0:38:05.800
<v Speaker 1>our atmosphere does protect us. The ozone and the atmosphere

0:38:05.800 --> 0:38:07.799
<v Speaker 1>and stuff like that protects us from gamma rays. Like

0:38:08.040 --> 0:38:10.440
<v Speaker 1>focus you out there wondering, we're getting hit once per

0:38:10.520 --> 0:38:12.680
<v Speaker 1>day from these gamma rays from other galaxies. Why don't

0:38:12.680 --> 0:38:15.440
<v Speaker 1>we all have cancer already? Well, some of us do

0:38:15.560 --> 0:38:17.799
<v Speaker 1>have cancer, and some of that is because of gamma rays,

0:38:17.880 --> 0:38:21.520
<v Speaker 1>but mostly the atmosphere protects us. And so if it's

0:38:21.560 --> 0:38:24.480
<v Speaker 1>not too close, then our atmosphere will protect us. But

0:38:24.880 --> 0:38:27.560
<v Speaker 1>the atmosphere has a limit, like the gamma rays they

0:38:27.680 --> 0:38:30.120
<v Speaker 1>use up the ozone. So if you have a really

0:38:30.160 --> 0:38:33.400
<v Speaker 1>big burst of gamma rays from pretty nearby, not not

0:38:33.480 --> 0:38:35.719
<v Speaker 1>close enough, that it's going to fry you instantly, but

0:38:35.880 --> 0:38:37.400
<v Speaker 1>it might use up a lot of the ozone and

0:38:37.400 --> 0:38:40.040
<v Speaker 1>the atmosphere and they will be sort of left unprotected

0:38:40.040 --> 0:38:43.040
<v Speaker 1>for a while until the ozone builds back up. So, um,

0:38:43.200 --> 0:38:45.360
<v Speaker 1>that could be a bad situation. Well, I think it was.

0:38:45.400 --> 0:38:47.920
<v Speaker 1>It's interesting to think that maybe you were saying that

0:38:48.520 --> 0:38:51.400
<v Speaker 1>maybe these these could be the limiting factors in in

0:38:51.560 --> 0:38:55.440
<v Speaker 1>how life how widespread life could be in the universe, right,

0:38:55.480 --> 0:38:58.600
<v Speaker 1>Like these are basically kind of a like a check

0:38:58.600 --> 0:39:00.680
<v Speaker 1>on life in the universe. Like, if we didn't have

0:39:01.400 --> 0:39:03.960
<v Speaker 1>gamma ray burst, maybe there would be more life out

0:39:03.960 --> 0:39:06.799
<v Speaker 1>there in the universe. Yeah, it's actually interesting because it

0:39:06.800 --> 0:39:09.239
<v Speaker 1>goes both ways, right, Like some galaxies, if they have

0:39:09.280 --> 0:39:11.719
<v Speaker 1>a lot of these stars that are going supernova and

0:39:11.719 --> 0:39:14.880
<v Speaker 1>making these gamma ray bursts, then it's pretty hard to

0:39:14.920 --> 0:39:17.520
<v Speaker 1>get life started because it's just so much crazy radiation.

0:39:18.120 --> 0:39:21.960
<v Speaker 1>On the other hand, you also need a bit of radiation, right, Remember,

0:39:22.000 --> 0:39:24.920
<v Speaker 1>like having a particle fly through and change your DNA

0:39:25.200 --> 0:39:27.920
<v Speaker 1>is a key element to evolution. It allows us to

0:39:27.960 --> 0:39:31.799
<v Speaker 1>explore the evolutionary landscape by adding random mutations. So if

0:39:31.800 --> 0:39:35.800
<v Speaker 1>you had zero radiation, then you wouldn't then evolution wouldn't

0:39:35.840 --> 0:39:38.719
<v Speaker 1>be as effective. Really, Yeah, you need some amount of

0:39:38.760 --> 0:39:42.239
<v Speaker 1>revolution depends on gamma ray bursts. Well, you know, how

0:39:42.280 --> 0:39:44.560
<v Speaker 1>does evolution work, right? You need your children to be

0:39:44.600 --> 0:39:47.400
<v Speaker 1>slightly different from you. Right, they're not just a combination

0:39:47.400 --> 0:39:51.000
<v Speaker 1>of units that happened randomly through biological processes like it.

0:39:51.080 --> 0:39:54.080
<v Speaker 1>Really you're saying really needs radiation from out of space. Well,

0:39:54.120 --> 0:39:57.120
<v Speaker 1>you know there's two main sources there. This transcription errors,

0:39:57.120 --> 0:39:59.600
<v Speaker 1>like when the DNA gets copied there there are mistakes

0:39:59.600 --> 0:40:02.160
<v Speaker 1>that are made. But also, yeah, radiation plays a role

0:40:02.160 --> 0:40:06.759
<v Speaker 1>as well, and so, um, you have a slower rate

0:40:06.800 --> 0:40:09.560
<v Speaker 1>of mutation if you didn't have gamma rays, if you

0:40:09.600 --> 0:40:14.520
<v Speaker 1>didn't have radiation, and so you could explore different evolutionary paths. Um,

0:40:14.719 --> 0:40:16.440
<v Speaker 1>not as quickly if you didn't have radiation. So you

0:40:16.480 --> 0:40:19.040
<v Speaker 1>want just the right amount of radiation, right. So I

0:40:19.080 --> 0:40:21.160
<v Speaker 1>think what you're saying is a physicist here is making

0:40:21.200 --> 0:40:24.239
<v Speaker 1>a statement that basically we're we're all hulk. That kind

0:40:24.239 --> 0:40:28.879
<v Speaker 1>of what you're exactly like every human being is kind

0:40:28.880 --> 0:40:30.719
<v Speaker 1>of like the Hulk. It's not about being the Hulk,

0:40:30.920 --> 0:40:36.200
<v Speaker 1>it's about the radiation you absorbed along the way. Yeah. Um,

0:40:36.239 --> 0:40:39.640
<v Speaker 1>but so far, the closest gamma ray burst we've ever

0:40:39.680 --> 0:40:43.240
<v Speaker 1>seen is like a hundred and thirty million light years away,

0:40:43.680 --> 0:40:46.319
<v Speaker 1>which is still really really far away, which is in

0:40:46.360 --> 0:40:48.680
<v Speaker 1>another galaxy. Right, Yeah, that's in another galaxy, and if

0:40:48.719 --> 0:40:51.839
<v Speaker 1>one happened in our galaxy, that would be tough. But

0:40:51.920 --> 0:40:54.160
<v Speaker 1>we think, I mean, the current estimacies are all really

0:40:54.160 --> 0:40:56.960
<v Speaker 1>really rough. But is that there's like one gamma ray

0:40:57.040 --> 0:41:00.799
<v Speaker 1>burst per galaxy per thousand years. I remember, there's a

0:41:00.840 --> 0:41:03.520
<v Speaker 1>lot of stars in the galaxy, right, hundreds of billions

0:41:03.520 --> 0:41:06.239
<v Speaker 1>of stars, so for one of them to give a

0:41:06.239 --> 0:41:08.680
<v Speaker 1>gama ray burst every thousand years means it's a pretty

0:41:08.760 --> 0:41:11.680
<v Speaker 1>rare event. And that makes sense. So the reason we

0:41:11.719 --> 0:41:13.799
<v Speaker 1>haven't seen any from our Milky Way is probably just

0:41:13.840 --> 0:41:16.239
<v Speaker 1>that hasn't happened yet. So wait, if we get an

0:41:16.239 --> 0:41:20.960
<v Speaker 1>extra special super duper supernova in the Milky Way, that's it, right,

0:41:21.760 --> 0:41:24.759
<v Speaker 1>we're toast. Well, it depends. The Milky Way is a

0:41:24.760 --> 0:41:26.600
<v Speaker 1>big place, so if it happens in the other side

0:41:26.600 --> 0:41:28.319
<v Speaker 1>of the Milky Way, it's a big difference than if

0:41:28.360 --> 0:41:32.040
<v Speaker 1>it happens like next door. Um. Also, we think that

0:41:32.040 --> 0:41:35.080
<v Speaker 1>these gamma ray bursts are directional, that they happened, that

0:41:34.880 --> 0:41:37.879
<v Speaker 1>they fly out in jets from the supernova, just like

0:41:38.960 --> 0:41:41.799
<v Speaker 1>from the pulsars and quasars we talked about. So it

0:41:41.960 --> 0:41:43.520
<v Speaker 1>might not even be aimed at us. It could happen

0:41:43.560 --> 0:41:46.400
<v Speaker 1>next door and we could be fine, or it could

0:41:46.400 --> 0:41:49.440
<v Speaker 1>fry us. Like it it's abused these gamma rays in

0:41:49.440 --> 0:41:52.960
<v Speaker 1>one direction and we might get lucky. Exactly. We're basically

0:41:52.960 --> 0:41:57.759
<v Speaker 1>playing cosmic Russian roulette all the time. So we brought

0:41:57.760 --> 0:42:04.000
<v Speaker 1>it back to Russias crazy. We brought crazy Russian led exactly. So, Um,

0:42:04.040 --> 0:42:06.440
<v Speaker 1>so we don't really know the details of how gamma

0:42:06.520 --> 0:42:08.200
<v Speaker 1>ray birsts are formed that we have a lot better

0:42:08.280 --> 0:42:10.799
<v Speaker 1>understand than we did a few decades ago. Um, we

0:42:10.840 --> 0:42:12.719
<v Speaker 1>don't know how often they happened. We just sort of

0:42:12.800 --> 0:42:16.320
<v Speaker 1>hoping that one doesn't happen. But to me, the crazy

0:42:16.400 --> 0:42:19.880
<v Speaker 1>thing is that gamma ray bursts travel at the speed

0:42:19.920 --> 0:42:23.279
<v Speaker 1>of light, and that is an important consequence. Yeah, because

0:42:23.320 --> 0:42:26.600
<v Speaker 1>you wouldn't see it coming right Exactly. You can't possibly

0:42:26.640 --> 0:42:29.200
<v Speaker 1>have any warning, right unless you can predict that a

0:42:29.239 --> 0:42:30.839
<v Speaker 1>star is going to go super new but and give

0:42:30.840 --> 0:42:32.920
<v Speaker 1>off a gamma ray burst. You're not gonna watch every

0:42:32.920 --> 0:42:35.960
<v Speaker 1>single star and try to predict which one. Um, there's

0:42:36.000 --> 0:42:39.239
<v Speaker 1>no advanced notice right. The first thing you hear about

0:42:39.239 --> 0:42:41.319
<v Speaker 1>a gamer ray burst is when it's washing over you

0:42:41.360 --> 0:42:44.360
<v Speaker 1>and frying your DNA, So there could be one on

0:42:44.520 --> 0:42:46.800
<v Speaker 1>its way right now. How does that make you feel?

0:42:47.120 --> 0:42:51.879
<v Speaker 1>Makes me feel a little crazy toasty? Well, I think

0:42:51.920 --> 0:42:55.120
<v Speaker 1>you know, it seems like, um, there are many surprises

0:42:55.160 --> 0:42:57.760
<v Speaker 1>out there in the universe, and we should be ready

0:42:57.800 --> 0:43:01.080
<v Speaker 1>for them, and we should be excited for them, and

0:43:01.239 --> 0:43:04.200
<v Speaker 1>we should appreciate the being here in the life we

0:43:04.239 --> 0:43:07.000
<v Speaker 1>have because you know, it could really literally be snuffed

0:43:07.000 --> 0:43:10.359
<v Speaker 1>out in a second at any time. That's true. And

0:43:10.640 --> 0:43:12.880
<v Speaker 1>you know, most of these cosmic mysteries just help us

0:43:12.960 --> 0:43:15.880
<v Speaker 1>understand what a beautiful and crazy place this universe is.

0:43:16.480 --> 0:43:18.040
<v Speaker 1>Very few of them are actually going to kill us,

0:43:18.600 --> 0:43:21.600
<v Speaker 1>and so don't worry about it too much, folks. And

0:43:21.640 --> 0:43:24.319
<v Speaker 1>there's nothing you can do anyway, So don't worry about it,

0:43:25.480 --> 0:43:29.759
<v Speaker 1>that's right. Just relax, lower your heart rate, the sun

0:43:29.880 --> 0:43:32.759
<v Speaker 1>is coming down. Just be at peace, like Bruce Bank.

0:43:33.120 --> 0:43:36.400
<v Speaker 1>There you go, exactly. We're all Bruce Banner, see you

0:43:36.440 --> 0:43:47.280
<v Speaker 1>next time. If you still have a question after listening

0:43:47.280 --> 0:43:50.400
<v Speaker 1>to all these explanations, please drop us a line. We'd

0:43:50.400 --> 0:43:53.240
<v Speaker 1>love to hear from you. You can find us at Facebook, Twitter,

0:43:53.320 --> 0:43:57.000
<v Speaker 1>and Instagram at Daniel and Jorge That's one Word, or

0:43:57.120 --> 0:44:01.040
<v Speaker 1>email us at Feedback at Daniel and Jorge dot com.

0:44:01.080 --> 0:44:03.880
<v Speaker 1>Thanks for listening, and remember that Daniel and Jorge Explain

0:44:03.960 --> 0:44:07.200
<v Speaker 1>the Universe is a production I Heart Radio. For more

0:44:07.280 --> 0:44:10.600
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0:44:10.880 --> 0:44:14.360
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