WEBVTT - How was radiation discovered?

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<v Speaker 1>Hey, Daniel, would you risk your life for science? It

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<v Speaker 1>might depend on the science we're talking about. Would you

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<v Speaker 1>risk getting eaten if you've got to meet Adians for example? Tempting,

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<v Speaker 1>but I'll pass. How about would you risk speghettification if

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<v Speaker 1>you got to see the inside of a black hole?

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<v Speaker 1>You know, I might actually take that trip. Or would

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<v Speaker 1>you risk deadly radiation to understand the nature of matter? Actually,

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<v Speaker 1>I've kind of already done that. One really does a

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<v Speaker 1>large hadron collider generate deadly radiation? It does, But that's

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<v Speaker 1>not how I've been exposed. How have you been exposed

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<v Speaker 1>to radiation? Well, flying the switzerlanded back like a thousand times,

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<v Speaker 1>you get a lot more radiation at high altitude, really

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<v Speaker 1>you have. Every Transatlantic trip is like a chest X ray.

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<v Speaker 1>I thought you said you've been been by a radioactive

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<v Speaker 1>Swiss spider, and I gained that spider's proportional physics, smart

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<v Speaker 1>and chocolate making ability. I am jorhandmade cartoonists and the

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<v Speaker 1>creator of PhD comics. I'm Daniel. I'm a particle physicist,

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<v Speaker 1>and I like to think of myself as radioactive. Are

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<v Speaker 1>you technically radioactive? Are most people radioactive? At some level,

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<v Speaker 1>like bananas are radioactive. Yeah, so you're probably more radioactive

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<v Speaker 1>than most people. But I grew up in Los Almos,

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<v Speaker 1>New Mexico, where we like to say we all glow

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<v Speaker 1>in the dark. Really, I did grow up in Los Almos,

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<v Speaker 1>but we don't actually like to say that. Well, I

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<v Speaker 1>do eat a lot of bananas, and I do have

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<v Speaker 1>a certain glow about me, i'd like to think, but yeah,

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<v Speaker 1>Welcome to our podcast. Daniel and Jorge explain the university

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<v Speaker 1>production of our Heart Radio, in which we shine a

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<v Speaker 1>radioactive glow into all the mysteries of the universe, the big,

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<v Speaker 1>crazy things that are out there tearing the universe apart,

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<v Speaker 1>the powerful forces that are holding it together, the things

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<v Speaker 1>far from home, and the things right here in our backyard.

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<v Speaker 1>All the mysteries of physics revealed and explained to you.

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<v Speaker 1>That's right, we radiate knowledge and give you an X

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<v Speaker 1>ray view of all of the amazing secrets that are

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<v Speaker 1>out there to discover in the universe, and all of

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<v Speaker 1>the secrets that are yet to be discovered. And all

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<v Speaker 1>the while you can stay home and safe, tucked into

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<v Speaker 1>your couch, sipping that mug of tea and learning about

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<v Speaker 1>the universe. No tinfoil hat needed or leadline hats. That's right.

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<v Speaker 1>This counts exactly zero as part of your annual dose

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<v Speaker 1>of radiation, even though you'll be learning all about it.

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<v Speaker 1>It's right. Well, we're technically getting to people through sound waves,

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<v Speaker 1>not light weights or radiation. That's right. But actually radiation

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<v Speaker 1>is sort of any sort of energetic particle or wave.

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<v Speaker 1>So sound is technically speaking a kind of radiation. So

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<v Speaker 1>we are radiating your ears with our voices. What no it,

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<v Speaker 1>I said a limit? Get you like, if I throw

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<v Speaker 1>a baseball, I'm radiating a baseball. Baseballs are radiation, yes, absolutely, Now,

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<v Speaker 1>the technical definition of radiation is sort of weirdly broad.

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<v Speaker 1>Any kind of light, any kind of particle, any kind

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<v Speaker 1>of way that transmits energy is radiation. But practically speaking,

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<v Speaker 1>when we talk about radiation, we mean very high energy

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<v Speaker 1>particles or higher energy waves that are going to deposit

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<v Speaker 1>a significant amount of energy. And so a flashlight or

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<v Speaker 1>this podcast are not typically categorized as radiation, even though technically,

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<v Speaker 1>according to physicists it is. Well it's a very loaded word,

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<v Speaker 1>isn't it. I mean, especially like in the eighties. I

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<v Speaker 1>feel in the nineties, you know, radiation was such a

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<v Speaker 1>negative thing, and nobody wanted radiation and the thing that

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<v Speaker 1>made you sick. Yeah, exactly. Radiation can be pretty dangerous.

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<v Speaker 1>They're basically these little invisible bullets flying through the universe,

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<v Speaker 1>and they can do real damage. They can fly through

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<v Speaker 1>your cells, they can bust up your DNA, they can

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<v Speaker 1>cause you cancer. And so radiation definitely is something to

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<v Speaker 1>think about and worry about. And it's one of these

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<v Speaker 1>things in the world that's not visible to our naked

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<v Speaker 1>eye yet turns out to be pretty important. So it's

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<v Speaker 1>a key that tells us that there's a lot going

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<v Speaker 1>on in the universe that we can't directly see. Yeah,

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<v Speaker 1>So a big question is how do we even discover

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<v Speaker 1>radiation or even come to believe it exists if it

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<v Speaker 1>is in fact invisible. Yeah, it's part of this story

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<v Speaker 1>of peeling back the nature of reality and figuring out

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<v Speaker 1>that the universe has a lot of stuff going on.

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<v Speaker 1>But to me, it's always fascinating to figure out how

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<v Speaker 1>that came to be, how that understanding sort of filtering

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<v Speaker 1>into human minds, because here we are standing on the

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<v Speaker 1>shoulders of giants, understanding all these things about the way

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<v Speaker 1>the world works. But this required a real shift in

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<v Speaker 1>people's understanding of the nature of the universe. So I'm

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<v Speaker 1>always super interested in those moments, like what was it

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<v Speaker 1>to convinced people? What experiments did people do that revealed that,

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<v Speaker 1>because I hope that will help us understand what experiments

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<v Speaker 1>in the future might again change the way we think

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<v Speaker 1>about the universe. Yeah. So usually people assign this discovery

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<v Speaker 1>to Madame Curie and her experiments, but there's actually more

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<v Speaker 1>to the story, right there is she did not, in

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<v Speaker 1>fact discover radiation. She won a couple of Nobel prizes.

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<v Speaker 1>She was quite a genius. She discovered a lot of stuff,

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<v Speaker 1>but you can't give her credit for discovering radiation. It's

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<v Speaker 1>a fascinating story. Well you can't even define it. I mean, sure,

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<v Speaker 1>then nobody discovered radiation or everyone discovered that's right. The

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<v Speaker 1>first little swimming organism that developed an eyeball, I supposed

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<v Speaker 1>discovered radiation when it used photons to guide itself around

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<v Speaker 1>the primordial soup on Earth. I suppose, yeah, right, like

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<v Speaker 1>the first organism to use or detect light. Right, that

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<v Speaker 1>definitely predates humanity. But I think we should focus on

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<v Speaker 1>the kind of radiation we're talking about, which is you know,

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<v Speaker 1>high energy particles or waves that come from like radioactive decay,

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<v Speaker 1>things that are different from the normal kinds of radiation

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<v Speaker 1>we used to live our lives. We're talking about a

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<v Speaker 1>change in how we've understood the universe. Okay, so it's

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<v Speaker 1>a invisible well, potentially dangerous and obviously very scientifically significant.

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<v Speaker 1>But how was radiation discovered? That's a big question, and

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<v Speaker 1>that's the question we're exploring today. So to the end

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<v Speaker 1>the program, we'll be talking about how was radiation discovered? So,

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<v Speaker 1>as usually, we were wondering how many people out there

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<v Speaker 1>knew how radiation was discovered? So thank you to everybody

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<v Speaker 1>who have volunteered their answers to these tricky physics questions

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<v Speaker 1>without referring to any reference materials, Google or Being or

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<v Speaker 1>ask Jeeves. And if you would like to participate in

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<v Speaker 1>future Baseless Speculations for the podcast, please write to us

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<v Speaker 1>two questions at Daniel and Jorge dot com. Maybe that

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<v Speaker 1>should be the name of that website, Daniel Baseless speculation

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<v Speaker 1>dot com. You might get a lot of hits. Yeah, exactly.

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<v Speaker 1>We just pointed to our book every single time we

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<v Speaker 1>have no idea. Dot com is the answer to all

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<v Speaker 1>these questions. Oh, interesting, interesting marketing technique. Lure people in

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<v Speaker 1>with a juicy website and then sell them a book.

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<v Speaker 1>Yeah exactly. I think they call that click bait. So

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<v Speaker 1>think about it for a second. If someone approached you

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<v Speaker 1>and asked you if you knew how radiation was discovered,

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<v Speaker 1>what would you say. Here's what people had to say.

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<v Speaker 1>I have no idea, but I think it has something

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<v Speaker 1>to do with Marie Curry playing around with some kind

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<v Speaker 1>of radioactive substance and like X raying her hand or

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<v Speaker 1>something like that. Radiation was discovered by Madame Cury. I

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<v Speaker 1>just know that was discovered Marie Cury. I believe radiation

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<v Speaker 1>was discovered by Marie Cury. I don't know how she

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<v Speaker 1>did it. She was probably experimenting with what became known

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<v Speaker 1>as radium and saw it glowing. I think radiation was

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<v Speaker 1>discovered in the eighteen hundreds when some radioactive material uranium

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<v Speaker 1>was glowing in the dark or was unusually hot. All right,

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<v Speaker 1>it looks like Marie Curry and the Curys have a

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<v Speaker 1>pretty good policies because most people went to them as

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<v Speaker 1>the discoverers of radiation. Yeah, she definitely ensconced in popular

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<v Speaker 1>culture as somebody deeply associated with radiation. And you know,

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<v Speaker 1>she actually did have a good publicist late in her career.

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<v Speaker 1>She did a whole tour of the United States giving

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<v Speaker 1>talks all about radiation stuff. So she became quite famous

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<v Speaker 1>and associated with radiation. So that has lasted up to

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<v Speaker 1>the present day, almost a hundred years later. Right, Well,

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<v Speaker 1>we don't want to take away anything that she did

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<v Speaker 1>or that the Crease did. It's really more about definition.

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<v Speaker 1>I think I think she discovered a particular type of

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<v Speaker 1>radiation or I guess we'll get into that, but generally speaking,

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<v Speaker 1>it kind of seems like radiation maybe is a broader

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<v Speaker 1>concept than most people assume it is. There's definitely that,

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<v Speaker 1>and she made important contributions and discovered particular kinds of

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<v Speaker 1>radioactive elopments. Will dig into that, but you're right, radiation

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<v Speaker 1>is a sort of a broader set of things. Radiation

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<v Speaker 1>is not just uranium decays and shoots out deadly particles.

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<v Speaker 1>There's a broader set of things. We consider radiation not

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<v Speaker 1>just ordinary light. But it starts, for example, with X rays,

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<v Speaker 1>Like X rays are just high energy photons, but we

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<v Speaker 1>consider them radiation. Yeah, I guess you're saying earlier that

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<v Speaker 1>any light is considered radiation. Even sound is considered radiation,

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<v Speaker 1>even like heat, I guess heat is radiation. Yeah, exactly,

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<v Speaker 1>you radiate heat. You run a lap and you get

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<v Speaker 1>really hot, you are radiating heat out into the universe.

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<v Speaker 1>And everything in the universe that has a temperature gives

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<v Speaker 1>off heat, and so everything in the universe is radiating constantly.

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<v Speaker 1>Radiation is everywhere. But that's sort of again the sort

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<v Speaker 1>of technical physical term for it. When we talk about radiation,

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<v Speaker 1>we think about sort of damaging radiation, radiation that's long

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<v Speaker 1>been invisible to us and reveals something different about how

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<v Speaker 1>the world works. And it was really crucial in understanding

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<v Speaker 1>things like the nature of the atom and the deep

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<v Speaker 1>structure of matter. Right, Well, we knew about light for

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<v Speaker 1>a long time. I mean, it's it's kind of in

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<v Speaker 1>the Bible, Daniel, that they'll be light. It was like

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<v Speaker 1>the first thing is that a reference book. I wasn't

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<v Speaker 1>familiar with that, you know, God at all. I think

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<v Speaker 1>there's some rata for that one. It's probably the most

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<v Speaker 1>impact factor of wall puplications in the history of man. Yeah,

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<v Speaker 1>I submitted something, but it got rejected by the referees.

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<v Speaker 1>So I mean of course, we've known about light for

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<v Speaker 1>a long time, So I guess when when do you

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<v Speaker 1>draw the line as us having discovered radiation, Like, is

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<v Speaker 1>it x rays? Is that the first kind of you know,

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<v Speaker 1>powerful kind of radiation invisible that we've discovered. Yeah, I

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<v Speaker 1>think the discovery of X rays really marked the turning point.

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<v Speaker 1>It's the time we discovered that there are ways to

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<v Speaker 1>transmit energy or other kinds of light that are different

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<v Speaker 1>from the kind of visible light we were familiar with.

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<v Speaker 1>And this specifically was a kind of light that we

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<v Speaker 1>saw could sort of pass through walls and pass through barriers,

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<v Speaker 1>and so it really was doing something different from the

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<v Speaker 1>kind of visible light we were familiar with. And that's

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<v Speaker 1>exactly how it was discovered. I see, like, if you're

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<v Speaker 1>shine a flashlight, it gets blocked by the wall. But

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<v Speaker 1>if you shine an X ray tube at at a wall,

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<v Speaker 1>it will go right through. It will go through most

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<v Speaker 1>of it. Yeah, exactly. And that's why we call it,

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<v Speaker 1>you know, X raying something because X rays passed through

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<v Speaker 1>the soft tissue of your body, but not your bones,

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<v Speaker 1>and so they reveal what's going on inside. And so

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<v Speaker 1>radiation is interesting because they can do these things in

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<v Speaker 1>visible light can't do. But also because it has this power,

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<v Speaker 1>it penetrates and so it reveals what's the inside, all right,

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<v Speaker 1>So then how do we discover X rays? So X

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<v Speaker 1>rays discovered by this guy Runken. And this guy was

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<v Speaker 1>a character. I think you'd like this. He actually was

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<v Speaker 1>kicked out of high school as a student because he

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<v Speaker 1>drew a caricature of one of his teachers, which is

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<v Speaker 1>not very flattering, and so he's sort of a physicist

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<v Speaker 1>and a cartoonist. I almost got exposed from my school

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<v Speaker 1>for the exact same reason, actually exactly. I didn't this

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<v Speaker 1>caricature one teacher, I did all of them. Well then

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<v Speaker 1>maybe there's a Nobel prize in your future. Yeah, stay tuned.

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<v Speaker 1>But he was doing experiments at the time with these

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<v Speaker 1>things called Crooks tubes. We talked about these before because

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<v Speaker 1>they were how electrons were discovered. They're basically just these

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<v Speaker 1>glass tubes that are mostly have vacuum in them. You

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<v Speaker 1>have an anode and a cathode with voltage across them,

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<v Speaker 1>and so you pull electrons off. People have seen these

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<v Speaker 1>seeing before and you get these beams, these glowing beams

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<v Speaker 1>inside that look really cool because the electrons were like

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<v Speaker 1>knocking off atoms and ionizing them, and people were doing

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<v Speaker 1>lots of experiments with them trying to understand what they were.

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<v Speaker 1>And again J. J. Thompson used them to discover the electrons.

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<v Speaker 1>But Runkin was really interested in whether or not the

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<v Speaker 1>rays that were being produced inside these tubes could pass

0:12:28.080 --> 0:12:30.200
<v Speaker 1>through the glass. He was curious to see what they

0:12:30.200 --> 0:12:34.680
<v Speaker 1>could get through. But these rays were originally electrons, like

0:12:34.679 --> 0:12:37.360
<v Speaker 1>like a stream of electrons or or were they light?

0:12:37.640 --> 0:12:39.760
<v Speaker 1>These were a stream of electrons and that's what J. J.

0:12:39.840 --> 0:12:42.840
<v Speaker 1>Thompson discovered. But the glow that you saw that was

0:12:42.960 --> 0:12:45.760
<v Speaker 1>visible light. And so the electrons would knock into a

0:12:45.800 --> 0:12:49.199
<v Speaker 1>few atoms inside the tube, ionized them, they would give

0:12:49.240 --> 0:12:51.000
<v Speaker 1>off some light, and then they would decay back to

0:12:51.040 --> 0:12:53.920
<v Speaker 1>their ground state. So what people were sort of ooing

0:12:53.960 --> 0:12:57.680
<v Speaker 1>and aweing over, we're seeing a beam of electrons exciting

0:12:57.720 --> 0:13:00.840
<v Speaker 1>the gas inside the tube. Okay, but just clear the

0:13:00.840 --> 0:13:03.480
<v Speaker 1>the X ray is not the electrons and X rays

0:13:03.559 --> 0:13:05.480
<v Speaker 1>is a light beam, right, that's right. The X ray

0:13:05.600 --> 0:13:07.719
<v Speaker 1>is not an electron electron as a particle, and X

0:13:07.880 --> 0:13:10.040
<v Speaker 1>ray is a piece of light. Right, It's a photon

0:13:10.160 --> 0:13:13.120
<v Speaker 1>of a specific energy. But this is what Runkin started

0:13:13.160 --> 0:13:15.360
<v Speaker 1>with He started with these tubes and he was playing

0:13:15.360 --> 0:13:18.640
<v Speaker 1>around with them, and he accidentally discovered that they also

0:13:18.800 --> 0:13:22.760
<v Speaker 1>generate X rays, like along with the electrons or when

0:13:22.760 --> 0:13:25.520
<v Speaker 1>the electrons hit stuff. So the electrons, one of the

0:13:25.520 --> 0:13:27.240
<v Speaker 1>things they do is they generate a glow that you

0:13:27.240 --> 0:13:30.079
<v Speaker 1>can see with your naked eye, but they also sometimes

0:13:30.120 --> 0:13:32.360
<v Speaker 1>generate X rays, and we can get into the whole

0:13:32.360 --> 0:13:35.760
<v Speaker 1>details of exactly how that happens, how they're accelerated and radios.

0:13:35.760 --> 0:13:39.040
<v Speaker 1>But sometimes they generate visible light in our spectrum, and

0:13:39.120 --> 0:13:42.120
<v Speaker 1>sometimes they generate photons that are higher energy, and these

0:13:42.160 --> 0:13:44.840
<v Speaker 1>are X rays. So he was interested in understanding, like

0:13:45.280 --> 0:13:47.760
<v Speaker 1>what is this thing generating? Can it pass through the

0:13:47.800 --> 0:13:50.320
<v Speaker 1>glass walls of the tube. So what he did was

0:13:50.320 --> 0:13:53.880
<v Speaker 1>he built a big black box, like a light proof box.

0:13:54.440 --> 0:13:57.240
<v Speaker 1>And his idea was, I'm gonna put this box around

0:13:57.360 --> 0:14:00.200
<v Speaker 1>my tube. I'm gonna see what light is show mind,

0:14:00.240 --> 0:14:03.320
<v Speaker 1>and the inside of the box from this tube, so

0:14:03.360 --> 0:14:05.439
<v Speaker 1>I can see sort of like you know what, light

0:14:05.520 --> 0:14:07.760
<v Speaker 1>comes out of the tube and hits the side of

0:14:07.800 --> 0:14:11.600
<v Speaker 1>the box. So I guess he wanted to know. He

0:14:11.600 --> 0:14:13.800
<v Speaker 1>thought he was trapping the light that was coming from

0:14:13.800 --> 0:14:16.800
<v Speaker 1>the Catherine tube, but actually he saw that the light

0:14:16.920 --> 0:14:19.560
<v Speaker 1>kind of leaked outside of it. Yeah, exactly, he turned

0:14:19.600 --> 0:14:21.680
<v Speaker 1>off the lights in his laboratory just to sort of

0:14:21.720 --> 0:14:23.680
<v Speaker 1>like get things warmed up, and he was going to

0:14:23.800 --> 0:14:26.000
<v Speaker 1>look inside the box to see if he could see

0:14:26.040 --> 0:14:29.000
<v Speaker 1>like light on the inside walls of the box. But

0:14:29.120 --> 0:14:31.520
<v Speaker 1>before he did that, he noticed that he saw this

0:14:31.680 --> 0:14:35.640
<v Speaker 1>weird light outside the box on the wall of his laboratory,

0:14:35.800 --> 0:14:38.040
<v Speaker 1>and he was like, what's that over there? And it

0:14:38.040 --> 0:14:40.280
<v Speaker 1>turns out he had a special sort of screen over

0:14:40.320 --> 0:14:43.240
<v Speaker 1>there just happened to be in the right location that

0:14:43.280 --> 0:14:46.600
<v Speaker 1>can receive X rays and glows when it hits X rays,

0:14:47.040 --> 0:14:49.560
<v Speaker 1>And so he discovered that the light doesn't just go

0:14:49.680 --> 0:14:53.000
<v Speaker 1>through the glass. It also went through his box all

0:14:53.000 --> 0:14:54.560
<v Speaker 1>the way out to the side of his lab and

0:14:54.640 --> 0:14:57.320
<v Speaker 1>hit this special screen. So it was quite by accident

0:14:57.360 --> 0:15:00.760
<v Speaker 1>that he discovered these X rays. Whoa was a special

0:15:00.800 --> 0:15:03.200
<v Speaker 1>screen that he just had that that seems like such

0:15:03.200 --> 0:15:06.960
<v Speaker 1>an accidental discovery. It's totally an accidental discovery. And it's

0:15:06.960 --> 0:15:10.520
<v Speaker 1>a special screen covered with a material that phosphoresces, so

0:15:10.560 --> 0:15:13.400
<v Speaker 1>it absorbs photons at one wavelength and then it gives

0:15:13.400 --> 0:15:16.240
<v Speaker 1>off photons at a different wavelength. So it's a wavelength

0:15:16.320 --> 0:15:18.800
<v Speaker 1>shifting effect. And this is the kind of thing we

0:15:18.840 --> 0:15:20.840
<v Speaker 1>do all the time in physics these days. We absorb

0:15:21.080 --> 0:15:23.560
<v Speaker 1>photons of one thing and it give off photons of

0:15:23.600 --> 0:15:26.360
<v Speaker 1>another color. So he happened to have a screen covered

0:15:26.360 --> 0:15:29.880
<v Speaker 1>in this material. It was a barrio phosphorescent material that

0:15:29.920 --> 0:15:32.720
<v Speaker 1>could absorb X rays and glow in the visible light.

0:15:33.080 --> 0:15:35.520
<v Speaker 1>And he was like, what's that over there, and did

0:15:35.520 --> 0:15:38.120
<v Speaker 1>a bunch of experiments, and he discovered that it could

0:15:38.160 --> 0:15:40.640
<v Speaker 1>pass through his box, and it could pass through lots

0:15:40.680 --> 0:15:43.400
<v Speaker 1>of other things, but that it wouldn't pass through metal,

0:15:43.480 --> 0:15:46.600
<v Speaker 1>for example. Now, was this the first time that, you know,

0:15:46.760 --> 0:15:50.320
<v Speaker 1>humans kind of got the idea that light can go

0:15:50.560 --> 0:15:53.200
<v Speaker 1>through things, or did we already kind of know that

0:15:53.240 --> 0:15:56.000
<v Speaker 1>there are things in nature that can go through things? Now,

0:15:56.000 --> 0:15:58.080
<v Speaker 1>this is the first time we understood that light could

0:15:58.080 --> 0:16:00.920
<v Speaker 1>pass through something that we thought was the wise solid.

0:16:01.440 --> 0:16:04.040
<v Speaker 1>And famously, the first X ray picture he ever took

0:16:04.320 --> 0:16:06.960
<v Speaker 1>was of his wife's hand, and you could see her

0:16:07.000 --> 0:16:09.640
<v Speaker 1>hand with its wedding ring on it, and he showed

0:16:09.640 --> 0:16:11.040
<v Speaker 1>it to her and he thought, this is gonna be

0:16:11.040 --> 0:16:13.800
<v Speaker 1>so romantic and awesome. She was actually really creeped out,

0:16:14.040 --> 0:16:16.160
<v Speaker 1>and she thought oh my gosh, I've seen my own death,

0:16:16.400 --> 0:16:19.200
<v Speaker 1>because she'd seemed like her own skeleton inside her hand.

0:16:19.800 --> 0:16:22.040
<v Speaker 1>And I think it really changed the way people felt

0:16:22.080 --> 0:16:25.800
<v Speaker 1>about like the solidity of stuff. Right, you think of

0:16:25.840 --> 0:16:29.400
<v Speaker 1>yourself as solid and opaque, but you're not. You're transparent

0:16:29.640 --> 0:16:32.640
<v Speaker 1>in some wavelengths of light, in your opaque in other

0:16:32.720 --> 0:16:35.920
<v Speaker 1>wavelengths of light. So then from that they they invented

0:16:36.240 --> 0:16:38.920
<v Speaker 1>X rays, you know, for medical purposes. Yeah, things happened

0:16:39.000 --> 0:16:42.760
<v Speaker 1>really fast because people very quickly understood how powerful this was.

0:16:42.800 --> 0:16:44.960
<v Speaker 1>Like you could see broken bones inside the body, or

0:16:45.000 --> 0:16:47.680
<v Speaker 1>you could see if you're tiled, it's swallowed something metal,

0:16:48.080 --> 0:16:50.640
<v Speaker 1>and so just seeing inside the body without having to

0:16:50.720 --> 0:16:54.720
<v Speaker 1>cut it open was immediately and enormously powerful. And within

0:16:54.760 --> 0:16:57.680
<v Speaker 1>a year people were using it in hospitals. And it

0:16:57.720 --> 0:17:00.120
<v Speaker 1>wasn't hard to make X rays, like Crookes tubes were

0:17:00.000 --> 0:17:02.720
<v Speaker 1>a thing that already existed, and so the technology sort

0:17:02.760 --> 0:17:05.560
<v Speaker 1>of was all around. It just took the right combination

0:17:05.640 --> 0:17:07.399
<v Speaker 1>of knowing what to do and how to do it.

0:17:08.200 --> 0:17:11.159
<v Speaker 1>And he went on to win the first Nobel Prize

0:17:11.160 --> 0:17:14.120
<v Speaker 1>in physics just a few years later. Really the first one,

0:17:14.960 --> 0:17:17.760
<v Speaker 1>the first one, yeah, exactly, and you know it sort

0:17:17.800 --> 0:17:20.240
<v Speaker 1>of satisfies all the requirements. It teaches you something deep

0:17:20.280 --> 0:17:23.240
<v Speaker 1>about the universe and also made a very big impact

0:17:23.320 --> 0:17:26.520
<v Speaker 1>on humanity. Wo and it sounds like it was really

0:17:26.520 --> 0:17:31.080
<v Speaker 1>more about discovering the screen is a combination. You have

0:17:31.160 --> 0:17:32.919
<v Speaker 1>to have the radiation and you have to have a

0:17:32.960 --> 0:17:36.280
<v Speaker 1>screen that can receive it. Right, X rays are invisible

0:17:36.320 --> 0:17:38.399
<v Speaker 1>to us, and so if they can just fly through

0:17:38.400 --> 0:17:40.480
<v Speaker 1>the universe and fly through a wall to see them,

0:17:40.680 --> 0:17:42.600
<v Speaker 1>you have to put something in their path that they

0:17:42.640 --> 0:17:46.600
<v Speaker 1>will interact with and that transform that information into something

0:17:46.840 --> 0:17:50.800
<v Speaker 1>your eyeballs can see. All right, Well, that's X ray radiation,

0:17:50.960 --> 0:17:53.880
<v Speaker 1>which is light radiation. But I guess the more popular

0:17:53.960 --> 0:17:56.919
<v Speaker 1>kind of radiation, or at least in people's consciousness, is

0:17:57.040 --> 0:18:00.560
<v Speaker 1>particle radiation. And that's where the curies come in. And

0:18:00.600 --> 0:18:03.520
<v Speaker 1>so let's get into that kind of radiation. But first,

0:18:03.600 --> 0:18:18.560
<v Speaker 1>let's take a quick break. All right, we're talking about

0:18:19.280 --> 0:18:22.800
<v Speaker 1>radiation and how it was discovered and how you should

0:18:22.880 --> 0:18:26.280
<v Speaker 1>probably wear sunscreen when you're outside and near particle colliders?

0:18:26.359 --> 0:18:31.119
<v Speaker 1>Would that help Daniel and near physicists? Probably because they

0:18:31.160 --> 0:18:34.159
<v Speaker 1>they're so shiny and beaming. Well, they just had to

0:18:34.160 --> 0:18:37.399
<v Speaker 1>do these crazy experiments which sometimes you know, do damage

0:18:37.440 --> 0:18:40.280
<v Speaker 1>their own help. All right, Well, I guess we talked

0:18:40.280 --> 0:18:42.680
<v Speaker 1>about X ray radiation, which which is really just light

0:18:43.000 --> 0:18:46.640
<v Speaker 1>at higher frequencies that can pass through things, and some

0:18:46.640 --> 0:18:51.000
<v Speaker 1>people associate that with radiation. But maybe the more common

0:18:51.000 --> 0:18:53.760
<v Speaker 1>type of radiation that people think of is kind of

0:18:53.800 --> 0:18:56.880
<v Speaker 1>the dangerous kind, I guess, the nuclear kind, and that's

0:18:57.000 --> 0:18:59.680
<v Speaker 1>more like particle radiation. Yeah, and X rays, of course

0:18:59.720 --> 0:19:02.840
<v Speaker 1>also dangerous. They can deposit a lot of energy in

0:19:02.920 --> 0:19:05.960
<v Speaker 1>your skin, and they can cause cancer and UV radiation

0:19:06.000 --> 0:19:08.840
<v Speaker 1>all that stuff, So it's definitely dangerous. But particle radiation

0:19:09.040 --> 0:19:11.720
<v Speaker 1>also very dangerous and more famous because I think of

0:19:11.760 --> 0:19:16.040
<v Speaker 1>the radioactive decays involved in nuclear physics, for example. But

0:19:16.359 --> 0:19:21.280
<v Speaker 1>particle radiation was discovered pretty soon after particles were discovered. Remember,

0:19:21.280 --> 0:19:25.119
<v Speaker 1>the whole idea of a particle didn't really exist until J. J.

0:19:25.200 --> 0:19:28.720
<v Speaker 1>Thompson discovered the electron in the late eighteen hundreds. You know,

0:19:28.800 --> 0:19:31.880
<v Speaker 1>this notion that everything was made out of tiny little bits,

0:19:31.880 --> 0:19:34.359
<v Speaker 1>and we could find those things and we could associate

0:19:34.600 --> 0:19:37.320
<v Speaker 1>like a tiny dot in space with mass and with

0:19:37.359 --> 0:19:40.840
<v Speaker 1>other quantities. This is a whole new idea in physics

0:19:41.080 --> 0:19:43.159
<v Speaker 1>at the time. It's not something which had existed for

0:19:43.200 --> 0:19:45.600
<v Speaker 1>a long time right before, Like light was just like

0:19:45.640 --> 0:19:48.760
<v Speaker 1>a beam, right, like pure energy kind of. Yeah, the

0:19:48.800 --> 0:19:51.600
<v Speaker 1>wave properties of light were dominant, and people thought about

0:19:51.760 --> 0:19:54.960
<v Speaker 1>light as a wave. They thought about matter and waves existing.

0:19:55.280 --> 0:19:57.040
<v Speaker 1>But the whole idea that things were made out of

0:19:57.040 --> 0:19:59.680
<v Speaker 1>tiny particles, or that these tiny particles could fly through

0:19:59.720 --> 0:20:04.000
<v Speaker 1>space invisibly and hurt you, for example, this was brand new,

0:20:04.280 --> 0:20:07.080
<v Speaker 1>but it was discovered pretty soon after the electron was

0:20:07.119 --> 0:20:11.320
<v Speaker 1>discovered again in the late eighteen hundreds, like the next year. Yeah,

0:20:11.359 --> 0:20:14.000
<v Speaker 1>and it was spurred by the discovery of X rays.

0:20:14.040 --> 0:20:16.240
<v Speaker 1>Like everybody in the world was very excited about the

0:20:16.280 --> 0:20:18.920
<v Speaker 1>X ray discovery made a huge wave in the world

0:20:18.920 --> 0:20:27.760
<v Speaker 1>of physics. Pun definitely intended and I thought it was unintentional. No,

0:20:28.040 --> 0:20:30.480
<v Speaker 1>And this bit about the screen that you latched onto.

0:20:30.600 --> 0:20:33.680
<v Speaker 1>This guy Beck Carrell, he also was really excited about that.

0:20:33.880 --> 0:20:37.199
<v Speaker 1>He thought it's really cool for something to absorb energy

0:20:37.240 --> 0:20:40.400
<v Speaker 1>in one wavelength and emit in another. To absorb one

0:20:40.480 --> 0:20:43.080
<v Speaker 1>kind of energy and emit another kind of thing. It's

0:20:43.119 --> 0:20:46.439
<v Speaker 1>called luminescence. And he thought he was really exciting and

0:20:46.480 --> 0:20:48.879
<v Speaker 1>he wanted to follow up in this and make also

0:20:49.000 --> 0:20:52.040
<v Speaker 1>some kind of crazy discovery and he came from a

0:20:52.080 --> 0:20:55.040
<v Speaker 1>long line of physicists people have been studying this sort

0:20:55.080 --> 0:20:58.159
<v Speaker 1>of kind of thing of generation of heat and energy.

0:20:58.680 --> 0:21:01.240
<v Speaker 1>So he did a series of experiments with uranium crystals

0:21:01.359 --> 0:21:04.159
<v Speaker 1>and he was the first to discover particle radiation. So

0:21:04.200 --> 0:21:07.800
<v Speaker 1>he actually came well before the curies. So interesting. Well,

0:21:07.840 --> 0:21:11.120
<v Speaker 1>apparently his father was also a physicist and a radiation

0:21:11.160 --> 0:21:14.360
<v Speaker 1>physicist too. That's right. He actually came from several generations

0:21:14.359 --> 0:21:16.639
<v Speaker 1>of physicists and they all had the same job. They

0:21:16.680 --> 0:21:19.040
<v Speaker 1>all had like the same chair in the head of

0:21:19.080 --> 0:21:21.879
<v Speaker 1>the natural science department in Paris, and so it was

0:21:21.920 --> 0:21:25.320
<v Speaker 1>sort of like a hereditary position almost. He's like a

0:21:25.440 --> 0:21:28.600
<v Speaker 1>legacy physicist in France. So his father looked into radiation,

0:21:28.640 --> 0:21:31.080
<v Speaker 1>but he didn't discover it. His father also had been

0:21:31.080 --> 0:21:35.600
<v Speaker 1>studying uranium crystals, and after Beccarel discovered radiation, people went

0:21:35.640 --> 0:21:37.720
<v Speaker 1>back and looked at his father's notebooks and there was

0:21:37.760 --> 0:21:41.920
<v Speaker 1>plenty of evidence in his father's notebooks to document evidence

0:21:41.960 --> 0:21:44.680
<v Speaker 1>of radiation, but his father just sort of didn't put

0:21:44.720 --> 0:21:47.919
<v Speaker 1>it together. And this is something you can do in physics.

0:21:47.920 --> 0:21:50.120
<v Speaker 1>When people make a big discovery, you can look back

0:21:50.119 --> 0:21:52.440
<v Speaker 1>at people who might have discovered it. If they had

0:21:52.440 --> 0:21:55.560
<v Speaker 1>only believed their results or followed up on something they

0:21:55.600 --> 0:21:59.720
<v Speaker 1>didn't understand. It sort of missed opportunities in physics. I

0:21:59.800 --> 0:22:02.840
<v Speaker 1>one know, if you want people to see that or

0:22:03.240 --> 0:22:05.359
<v Speaker 1>it's just kind of a little bit embarrassing from a

0:22:05.359 --> 0:22:08.360
<v Speaker 1>physics point of view. I think it's super fascinating from

0:22:08.359 --> 0:22:10.520
<v Speaker 1>a sort of history of science point of view. You

0:22:10.600 --> 0:22:13.200
<v Speaker 1>get a result that you don't understand or doesn't make sense,

0:22:13.359 --> 0:22:15.280
<v Speaker 1>do you always follow up on it or do you

0:22:15.280 --> 0:22:18.520
<v Speaker 1>sort of leave it behind? And those missed opportunities, you know,

0:22:18.560 --> 0:22:21.560
<v Speaker 1>those times when signs could have gone differently if somebody

0:22:21.560 --> 0:22:24.359
<v Speaker 1>had taken a different path and thought about something different

0:22:24.440 --> 0:22:27.360
<v Speaker 1>or had a different conversation at a conference. It's fascinating

0:22:27.400 --> 0:22:30.359
<v Speaker 1>to me to imagine the sort of alternate universes in

0:22:30.400 --> 0:22:33.320
<v Speaker 1>which we discovered things in different orders, because that's what

0:22:33.400 --> 0:22:35.920
<v Speaker 1>everyone wants in their tombstone, you know. Could have won

0:22:35.920 --> 0:22:39.199
<v Speaker 1>a Nobel prize. Yeah, But they did these experiments with

0:22:39.440 --> 0:22:42.880
<v Speaker 1>uranium crystals. So uranium was a thing, it was known,

0:22:43.000 --> 0:22:45.640
<v Speaker 1>it wasn't understood what it was doing, but they were

0:22:45.680 --> 0:22:48.080
<v Speaker 1>doing early studies with it. And essentially what they did

0:22:48.080 --> 0:22:50.760
<v Speaker 1>basically is they just put it next to photographic plates,

0:22:51.000 --> 0:22:53.639
<v Speaker 1>Like photographs were a thing back then, so they just

0:22:53.720 --> 0:22:56.359
<v Speaker 1>wrapped them in paper and put them next to photographic plates,

0:22:56.359 --> 0:22:58.879
<v Speaker 1>and they wanted to see what would happen. Oh right,

0:22:58.920 --> 0:23:02.320
<v Speaker 1>because they had photo grass at that time, and that

0:23:02.400 --> 0:23:04.360
<v Speaker 1>it is also kind of like magic, like light hits

0:23:04.400 --> 0:23:07.119
<v Speaker 1>it and or not hit it and it changes color. Yeah, exactly.

0:23:07.160 --> 0:23:10.800
<v Speaker 1>It's a special process that absorbs photons and develops in

0:23:10.840 --> 0:23:13.119
<v Speaker 1>a different way based on you know, the amount of

0:23:13.119 --> 0:23:15.680
<v Speaker 1>photons that hit it. To really sort of awesome chemical

0:23:15.760 --> 0:23:19.560
<v Speaker 1>process for absorbing things and taking data. And back before

0:23:19.560 --> 0:23:22.800
<v Speaker 1>we had computers and digital cameras and stuff, everything was analog.

0:23:23.160 --> 0:23:26.000
<v Speaker 1>This was a powerful way to do science experiments. But

0:23:26.080 --> 0:23:29.040
<v Speaker 1>Beckerel sort of started off on the wrong track. Remember

0:23:29.080 --> 0:23:31.720
<v Speaker 1>he was interested in luminescence. He thought if you took

0:23:31.760 --> 0:23:34.320
<v Speaker 1>these uranium crystals and you left them in the sun,

0:23:34.720 --> 0:23:36.800
<v Speaker 1>that they would absorb a bunch of energy from the

0:23:36.840 --> 0:23:40.080
<v Speaker 1>sun and then they might glow in some new invisible way.

0:23:40.480 --> 0:23:42.880
<v Speaker 1>So he put these uranium crystals in the sun, then

0:23:42.880 --> 0:23:45.440
<v Speaker 1>he wrapped them in paper to block an invisible light,

0:23:45.720 --> 0:23:48.119
<v Speaker 1>and he put them next to these photographic plates. So

0:23:48.160 --> 0:23:50.199
<v Speaker 1>he was hoping maybe he would like find a new

0:23:50.240 --> 0:23:52.280
<v Speaker 1>way to make X rays, or that they would admit

0:23:52.320 --> 0:23:54.840
<v Speaker 1>in the X ray because X rays had just been discovered,

0:23:54.840 --> 0:23:58.760
<v Speaker 1>all right, So he saw radiation and X rays and

0:23:58.800 --> 0:24:00.919
<v Speaker 1>he thought, hey, I wonder if that works everything. So

0:24:00.960 --> 0:24:03.120
<v Speaker 1>do do you think he tried a bunch of different materials,

0:24:03.119 --> 0:24:05.640
<v Speaker 1>not just these uranium crystals. Yeah, he tried a bunch

0:24:05.680 --> 0:24:09.359
<v Speaker 1>of different materials wondering what would glow. But these uranium salts,

0:24:09.400 --> 0:24:11.919
<v Speaker 1>these uranium crystals were the things that gave him the

0:24:12.000 --> 0:24:15.200
<v Speaker 1>best results. But that's not actually the most interesting part

0:24:15.200 --> 0:24:17.800
<v Speaker 1>of his discovery. I mean, first he did that, he said,

0:24:17.800 --> 0:24:20.000
<v Speaker 1>I'm gonna put these things out in the sun. Then

0:24:20.040 --> 0:24:21.879
<v Speaker 1>I'm gonna wrap them in paper to block in a

0:24:21.960 --> 0:24:24.439
<v Speaker 1>visible light and see if they make an impact on

0:24:24.480 --> 0:24:27.200
<v Speaker 1>the photographic plates. And they did so he thought, oh,

0:24:27.280 --> 0:24:31.280
<v Speaker 1>that's cool. But then he accidentally left a bunch of

0:24:31.320 --> 0:24:35.280
<v Speaker 1>them in a drawer next to these photographic plates without

0:24:35.359 --> 0:24:38.399
<v Speaker 1>shining them in the sun, so he sort of messed

0:24:38.480 --> 0:24:40.400
<v Speaker 1>up his experiment. He thought it was necessary to leave

0:24:40.440 --> 0:24:42.240
<v Speaker 1>it in in the sun to absorb energy and then it

0:24:42.280 --> 0:24:45.480
<v Speaker 1>would give off this radiation, but he accidentally left over

0:24:45.480 --> 0:24:48.600
<v Speaker 1>the weekend a bunch of iranium crystals next to one

0:24:48.640 --> 0:24:51.440
<v Speaker 1>of these photographic plates and came back the next week

0:24:51.720 --> 0:24:54.080
<v Speaker 1>and said, m oops for guys to leave this stuff

0:24:54.080 --> 0:24:56.480
<v Speaker 1>in the sun. But let's just develop this film and

0:24:56.520 --> 0:25:02.600
<v Speaker 1>see what it says. What seriously, seriously, total accident, total accident.

0:25:02.840 --> 0:25:04.360
<v Speaker 1>And he thought, well, you know, I guess I did

0:25:04.400 --> 0:25:06.720
<v Speaker 1>this weird experiment where I skipped the step with the sun.

0:25:07.080 --> 0:25:09.320
<v Speaker 1>Let's see what happens. And he developed it and the

0:25:09.400 --> 0:25:12.359
<v Speaker 1>picture looked exactly the same, which tells him that it

0:25:12.400 --> 0:25:15.240
<v Speaker 1>didn't need to absorb energy from the sun. It wasn't

0:25:15.480 --> 0:25:18.400
<v Speaker 1>luminescence where it was slurping in energy from the sun

0:25:18.440 --> 0:25:21.000
<v Speaker 1>and then changing it into X rays or something. It

0:25:21.119 --> 0:25:24.359
<v Speaker 1>was different. The uranium crystals were just giving off energy

0:25:24.520 --> 0:25:26.840
<v Speaker 1>on their own. They were just like a source of

0:25:26.880 --> 0:25:31.480
<v Speaker 1>some new kind of radiation, some new kind of invisible ray. Right,

0:25:31.680 --> 0:25:34.440
<v Speaker 1>that's really what he thought, Right, something invisible is coming

0:25:34.440 --> 0:25:37.840
<v Speaker 1>out of this, and this invisible thing somehow had energy. Yeah,

0:25:38.000 --> 0:25:40.800
<v Speaker 1>and you didn't have to put in energy. It's not

0:25:40.840 --> 0:25:43.200
<v Speaker 1>like with the Crooks too, where you have to apply electricity.

0:25:43.400 --> 0:25:46.199
<v Speaker 1>And it generated energy for the electrons which generated the

0:25:46.359 --> 0:25:48.960
<v Speaker 1>X rays. And it wasn't like phosphorescence where you have

0:25:49.040 --> 0:25:50.960
<v Speaker 1>to sit out in the sun and absorb the energy

0:25:51.000 --> 0:25:53.200
<v Speaker 1>and then give it off. It was just like pumping

0:25:53.240 --> 0:25:56.399
<v Speaker 1>out this invisible energy. And now we know that it

0:25:56.480 --> 0:25:59.439
<v Speaker 1>was alpha radiation and beta radiation, but he didn't know

0:25:59.480 --> 0:26:00.960
<v Speaker 1>that at the time, and he just knew he was

0:26:01.000 --> 0:26:04.040
<v Speaker 1>admitting some crazy new rays. And then he also won

0:26:04.119 --> 0:26:05.960
<v Speaker 1>a Nobel Prize for it, right, he won like the

0:26:05.960 --> 0:26:08.320
<v Speaker 1>third one he did, he won the third one, but

0:26:08.520 --> 0:26:12.280
<v Speaker 1>just barely. He discovered this, and the day after he

0:26:12.400 --> 0:26:15.720
<v Speaker 1>made this discovery he gave a presentation at like the

0:26:15.800 --> 0:26:19.640
<v Speaker 1>local scientific society, and he beat out some English physicists

0:26:19.640 --> 0:26:23.480
<v Speaker 1>who made the discovery like later that week. What we what?

0:26:23.480 --> 0:26:25.360
<v Speaker 1>But if he gave the presentation, then the other one

0:26:25.720 --> 0:26:29.239
<v Speaker 1>technically didn't the discovery or I guess he wasn't at

0:26:29.240 --> 0:26:31.320
<v Speaker 1>the presentation. He wasn't there yet, because you know the

0:26:31.320 --> 0:26:33.680
<v Speaker 1>world was much smaller, so you could give a whole

0:26:33.680 --> 0:26:36.360
<v Speaker 1>presentation and a society and friends, and nobody would hear

0:26:36.359 --> 0:26:39.439
<v Speaker 1>about it in England until weeks later or so. And

0:26:39.480 --> 0:26:43.240
<v Speaker 1>so Sylvanis Thompson made very very similar experiments, very similar

0:26:43.240 --> 0:26:46.159
<v Speaker 1>discoveries just a few days later and lost out on

0:26:46.200 --> 0:26:49.520
<v Speaker 1>the Nobel Prize because Beckerel made this discovery and was

0:26:49.640 --> 0:26:52.080
<v Speaker 1>very quick to report it. Oh, I see Beckrell was

0:26:52.119 --> 0:26:56.400
<v Speaker 1>in another country. Yes, this is in France. Interesting. Wow,

0:26:56.440 --> 0:26:59.480
<v Speaker 1>that's crazy. Two people in two different countries make the

0:26:59.560 --> 0:27:03.800
<v Speaker 1>same fundamental discovery almost a week apart, and there was

0:27:03.840 --> 0:27:06.840
<v Speaker 1>no internet. There was no internet. But this is all

0:27:06.920 --> 0:27:10.080
<v Speaker 1>spurred by Runkin's discovery of X rays and like cracked

0:27:10.119 --> 0:27:12.480
<v Speaker 1>open a whole new area of research. People looking for

0:27:12.520 --> 0:27:15.080
<v Speaker 1>these invisible rays. How can we find them, what's making them?

0:27:15.080 --> 0:27:17.680
<v Speaker 1>What kinds are out there? And it really did sparkle,

0:27:17.920 --> 0:27:20.359
<v Speaker 1>you know, a whole new field of research, all right.

0:27:20.480 --> 0:27:24.240
<v Speaker 1>So then that's where we get to Madame Curie and

0:27:24.480 --> 0:27:26.840
<v Speaker 1>Pierre Curie and that that this is kind of where

0:27:26.880 --> 0:27:30.000
<v Speaker 1>their story starts, right like the year after, Yeah, exactly,

0:27:30.000 --> 0:27:31.920
<v Speaker 1>this is where their story starts. So they came in

0:27:32.400 --> 0:27:35.880
<v Speaker 1>after Beckarel had already discovered radiation and Runkin had discovered

0:27:36.000 --> 0:27:38.920
<v Speaker 1>X rays, and they were really interested in this. And

0:27:39.000 --> 0:27:42.760
<v Speaker 1>Curie herself has a really fascinating backstory. Remember it's very

0:27:42.800 --> 0:27:47.159
<v Speaker 1>difficult for women in science to have any position and

0:27:47.200 --> 0:27:50.320
<v Speaker 1>to have any engagement, to even get an education. She

0:27:50.480 --> 0:27:53.280
<v Speaker 1>and her sister, for example, had to take turns working

0:27:53.520 --> 0:27:55.600
<v Speaker 1>and going to school. They had this deal where one

0:27:55.640 --> 0:27:56.960
<v Speaker 1>of them would work and the other one would go

0:27:56.960 --> 0:27:59.240
<v Speaker 1>to school, and then they took turns. And you have

0:27:59.359 --> 0:28:02.399
<v Speaker 1>to be really dedicated and sort of fend off all

0:28:02.400 --> 0:28:05.000
<v Speaker 1>out of societal pressure even to get to have an education,

0:28:05.040 --> 0:28:07.520
<v Speaker 1>not to mention be a scientist at the leading edge

0:28:07.520 --> 0:28:11.639
<v Speaker 1>of physics knowledge. Yeah, it's amazing, pretty powerful story. So

0:28:11.720 --> 0:28:13.880
<v Speaker 1>she was in France and she I guess she knew

0:28:13.920 --> 0:28:17.560
<v Speaker 1>about Beckarel's discovery. She knew about Beckarel's discovery, but most

0:28:17.600 --> 0:28:19.880
<v Speaker 1>of the world was more excited about the X rays,

0:28:20.000 --> 0:28:23.000
<v Speaker 1>like these new uranium rays that they called them you raise.

0:28:23.359 --> 0:28:25.399
<v Speaker 1>People are like, Okay, that's cool, but X rays are

0:28:25.440 --> 0:28:28.359
<v Speaker 1>better because they're easier to use, they're faster, they're cheaper

0:28:28.359 --> 0:28:31.520
<v Speaker 1>than make sharper images. But she was really interested in

0:28:31.560 --> 0:28:33.640
<v Speaker 1>these you rays. She was like, what are these? What's

0:28:33.720 --> 0:28:36.840
<v Speaker 1>making them? What does it tell us about the atom

0:28:37.160 --> 0:28:39.840
<v Speaker 1>that these things are just being created out of there?

0:28:40.120 --> 0:28:43.000
<v Speaker 1>And she was working with her husband, Pierre, and they

0:28:43.040 --> 0:28:45.880
<v Speaker 1>had this really cool device, this thing called an electrometer,

0:28:46.240 --> 0:28:49.680
<v Speaker 1>and he could basically measure very sensitively how well things

0:28:49.760 --> 0:28:53.200
<v Speaker 1>could conduct electricity. And Pierre had developed this technology from

0:28:53.200 --> 0:28:56.800
<v Speaker 1>his earlier research, which was into pezo electronics, these little

0:28:56.840 --> 0:29:00.200
<v Speaker 1>devices which create electricity if you squeeze them or move

0:29:00.240 --> 0:29:03.000
<v Speaker 1>if you apply electrical voltage across them. So we had

0:29:03.000 --> 0:29:05.880
<v Speaker 1>this technology and they applied it to the study these

0:29:05.880 --> 0:29:08.840
<v Speaker 1>you rays, and they found something pretty cool, which is

0:29:08.880 --> 0:29:11.200
<v Speaker 1>that if you have a bunch of uranium, the air

0:29:11.400 --> 0:29:14.800
<v Speaker 1>around the uranium tends to get ionized. They can conduct

0:29:14.920 --> 0:29:18.680
<v Speaker 1>electricity more easily than if you don't have uranium around

0:29:19.200 --> 0:29:21.320
<v Speaker 1>I see. And that was a big clue that it

0:29:21.400 --> 0:29:23.680
<v Speaker 1>was maybe giving all some kind of energy. Yeah, that

0:29:23.760 --> 0:29:26.160
<v Speaker 1>was a big clue that it was shooting out something

0:29:26.200 --> 0:29:28.800
<v Speaker 1>because it was like changing the air, right, This energy

0:29:28.880 --> 0:29:31.120
<v Speaker 1>was coming out and it was changing the air around

0:29:31.120 --> 0:29:34.400
<v Speaker 1>the uranium. And Pierre and Marie they took like no

0:29:34.600 --> 0:29:38.520
<v Speaker 1>safety precautions. They gotta readiated so much in their research.

0:29:38.840 --> 0:29:40.640
<v Speaker 1>There are all these moments you can read about in

0:29:40.680 --> 0:29:43.080
<v Speaker 1>their lab notebooks where they're like, Pierre has been sick

0:29:43.120 --> 0:29:45.720
<v Speaker 1>every single day for the last three months. I wonder

0:29:45.720 --> 0:29:48.959
<v Speaker 1>if it's coinciding with all these experiments we've done, whatever,

0:29:50.360 --> 0:29:53.640
<v Speaker 1>And they just kept going. It was pretty incredible. They

0:29:53.680 --> 0:29:57.440
<v Speaker 1>were really pretty sick during this whole period. Like nine ten,

0:29:57.680 --> 0:29:59.600
<v Speaker 1>which is a very intense period of their research, and

0:29:59.600 --> 0:30:03.000
<v Speaker 1>discover they're basically sick the whole time. And they never

0:30:03.040 --> 0:30:06.880
<v Speaker 1>really associated like all this illness with the research they

0:30:06.920 --> 0:30:08.960
<v Speaker 1>were doing. I'm not sure if that was like a

0:30:09.040 --> 0:30:12.880
<v Speaker 1>cognitive choice, like let's not influence our research with these

0:30:12.920 --> 0:30:15.920
<v Speaker 1>petty details of life, or if they knew and they

0:30:15.960 --> 0:30:18.280
<v Speaker 1>just sort of didn't care because it just we're so

0:30:18.360 --> 0:30:21.280
<v Speaker 1>hungry to reveal the knowledge. Well, technically, we don't know.

0:30:21.360 --> 0:30:23.080
<v Speaker 1>I mean, they could have just been, you know, on

0:30:23.120 --> 0:30:28.000
<v Speaker 1>a rash of eating badgers. I suppose so, but you know,

0:30:28.080 --> 0:30:30.040
<v Speaker 1>you look at the pattern of damage to their bodies,

0:30:30.080 --> 0:30:33.360
<v Speaker 1>like their fingertips had the really terrible damage to them.

0:30:33.560 --> 0:30:36.360
<v Speaker 1>You know, Murray Curie, she's now like a hero in France.

0:30:36.400 --> 0:30:39.440
<v Speaker 1>Of course, they moved her ashes from wherever they had

0:30:39.440 --> 0:30:42.000
<v Speaker 1>been born just about twenty years ago. They moved them

0:30:42.000 --> 0:30:44.240
<v Speaker 1>to the Pantheon in Paris, which is where you know,

0:30:44.320 --> 0:30:47.120
<v Speaker 1>France inters the ashes and the remains of its most

0:30:47.200 --> 0:30:51.640
<v Speaker 1>highly revered citizens. And those ashes were still radioactive. This

0:30:51.720 --> 0:30:57.240
<v Speaker 1>is like, you know, seventy years later, Yeah, exactly. She

0:30:57.360 --> 0:31:01.680
<v Speaker 1>definitely hurt herself for science, Her legacy lives. She was

0:31:01.720 --> 0:31:05.080
<v Speaker 1>really fascinated with this fact that the uranium the U

0:31:05.200 --> 0:31:08.280
<v Speaker 1>raise could change the air around them, and this is

0:31:08.320 --> 0:31:10.880
<v Speaker 1>what led her to this hypothesis that it wasn't like chemical,

0:31:11.240 --> 0:31:13.920
<v Speaker 1>It's not like the electron is giving off some energy

0:31:14.000 --> 0:31:16.360
<v Speaker 1>that it's absorbed from some other way. She thought it

0:31:16.400 --> 0:31:19.400
<v Speaker 1>was something deep in the atom, that the atoms themselves

0:31:19.480 --> 0:31:22.920
<v Speaker 1>or maybe not stable, that there was something changing internally

0:31:22.920 --> 0:31:25.000
<v Speaker 1>and it was giving off this energy. And of course

0:31:25.040 --> 0:31:28.120
<v Speaker 1>now we know she's right, it was radioactive to Kay,

0:31:28.160 --> 0:31:30.440
<v Speaker 1>but this was a really big and sort of bold

0:31:30.520 --> 0:31:33.200
<v Speaker 1>idea at the time. Right well, at this point in

0:31:33.240 --> 0:31:35.840
<v Speaker 1>our history, we knew about the atom, and we knew

0:31:35.880 --> 0:31:38.320
<v Speaker 1>about the kind of structure of it. We knew about

0:31:38.320 --> 0:31:41.480
<v Speaker 1>the electron, but we hadn't yet even discovered the nucleus

0:31:41.480 --> 0:31:45.000
<v Speaker 1>of the atom. It wasn't ntil Rutherford bombarded gold foil

0:31:45.160 --> 0:31:47.960
<v Speaker 1>with radiation later that we understood that there was like

0:31:48.000 --> 0:31:50.600
<v Speaker 1>a hard center to the atom that had a nucleus.

0:31:50.840 --> 0:31:53.400
<v Speaker 1>God forbid, you know, understanding the proton and the neutron

0:31:53.440 --> 0:31:56.000
<v Speaker 1>inside of it. At the time, after J. J. Thompson

0:31:56.040 --> 0:31:59.000
<v Speaker 1>discovered the electron, he thought that matter was like a

0:31:59.000 --> 0:32:03.560
<v Speaker 1>bunch of electrons floating in a positively charged jelly, and

0:32:03.640 --> 0:32:06.320
<v Speaker 1>so we didn't really even understand the structure of the atom.

0:32:06.400 --> 0:32:09.080
<v Speaker 1>So this is a really big leap for anybody to make. Yeah,

0:32:09.080 --> 0:32:10.920
<v Speaker 1>I mean, she's saying that it comes from deep within

0:32:10.960 --> 0:32:13.000
<v Speaker 1>the atom, but we didn't even know there was an atom. Well,

0:32:13.000 --> 0:32:14.760
<v Speaker 1>we knew there were atoms, we just didn't really know

0:32:14.840 --> 0:32:17.360
<v Speaker 1>like what was going on inside there. We didn't really

0:32:17.440 --> 0:32:20.200
<v Speaker 1>understand there was a hard nucleus that was made out

0:32:20.240 --> 0:32:23.400
<v Speaker 1>of these smaller particles. So yeah, it's a pretty big leap.

0:32:23.680 --> 0:32:26.600
<v Speaker 1>All right, let's get into her actual experiment in which

0:32:26.600 --> 0:32:30.000
<v Speaker 1>he discovered this nuclear radiation and what that means and

0:32:30.040 --> 0:32:33.120
<v Speaker 1>what other types of radiation were surrounded by. But first

0:32:33.200 --> 0:32:48.000
<v Speaker 1>let's take another quick break. All Right, we're talking about

0:32:48.000 --> 0:32:51.920
<v Speaker 1>the discovery of radiation, and we're up to Marie Currey

0:32:52.080 --> 0:32:58.560
<v Speaker 1>and her discovery that the nuclei of atoms also radiate things,

0:32:59.000 --> 0:33:01.360
<v Speaker 1>because we knew about X ray radiation, but we didn't

0:33:01.360 --> 0:33:05.360
<v Speaker 1>know about this particular kind which is coming from the nucleus. Yeah,

0:33:05.360 --> 0:33:07.400
<v Speaker 1>and we didn't even really know about the nucleus yet.

0:33:07.440 --> 0:33:09.920
<v Speaker 1>So this is giving us an inside that there's something

0:33:10.040 --> 0:33:13.280
<v Speaker 1>inside the atom, some mechanism which is capable of generating

0:33:13.360 --> 0:33:18.680
<v Speaker 1>powerful particle radiation. And so this was discovered originally in uranium, right,

0:33:18.720 --> 0:33:21.440
<v Speaker 1>Beckarel saw that it happened. But what the curious did

0:33:21.480 --> 0:33:24.360
<v Speaker 1>was that they sort of refined it. They discovered that

0:33:24.560 --> 0:33:28.400
<v Speaker 1>uranium itself was radioactive, but that there were variations of

0:33:28.560 --> 0:33:33.280
<v Speaker 1>uranium or that was even more radioactive than pure uranium itself,

0:33:33.480 --> 0:33:36.000
<v Speaker 1>which suggested that there might be something else in there,

0:33:36.120 --> 0:33:40.000
<v Speaker 1>even more radioactive. Oh, I see interesting, Like it's possible

0:33:40.040 --> 0:33:44.560
<v Speaker 1>to make an element like an atom the extra radioactive. Yeah, exactly.

0:33:44.600 --> 0:33:47.400
<v Speaker 1>They were working with this material called pitch blend, which

0:33:47.440 --> 0:33:50.400
<v Speaker 1>is a version of uranium ore, and they discovered that

0:33:50.480 --> 0:33:53.240
<v Speaker 1>before you purified it, before you purified it to make

0:33:53.320 --> 0:33:57.400
<v Speaker 1>just pure uranium, it was actually more radioactive. So they

0:33:57.400 --> 0:34:00.000
<v Speaker 1>had this hypothesis that there was something else in there,

0:34:00.040 --> 0:34:04.040
<v Speaker 1>a new element that was even more radioactive than uranium.

0:34:04.120 --> 0:34:07.280
<v Speaker 1>So they developed this technique to purify it, and a

0:34:07.320 --> 0:34:09.359
<v Speaker 1>lot of the time they spent, a lot of their

0:34:09.400 --> 0:34:13.480
<v Speaker 1>actual science was in this process of isolating this bit.

0:34:13.760 --> 0:34:16.799
<v Speaker 1>It took them, for example, three years of work on

0:34:16.880 --> 0:34:19.960
<v Speaker 1>pitch blend just to isolate a tenth of a gram

0:34:20.000 --> 0:34:24.239
<v Speaker 1>of this new substance. That's crazy. I imagine most people

0:34:24.280 --> 0:34:26.600
<v Speaker 1>think of radioactive things is like rocks or something, but

0:34:26.760 --> 0:34:29.520
<v Speaker 1>for them, this is probably like a powder or something. Right, Yeah,

0:34:29.560 --> 0:34:32.120
<v Speaker 1>these are like salts, right. They're grinding them up, they're

0:34:32.120 --> 0:34:34.840
<v Speaker 1>purifying that. They're doing chemistry to try to separate the

0:34:34.840 --> 0:34:36.920
<v Speaker 1>bits from the other, like does this dissolve in that?

0:34:37.239 --> 0:34:39.279
<v Speaker 1>How do we pull this thing apart? So it really

0:34:39.320 --> 0:34:42.319
<v Speaker 1>is sort of chemical. And what they discovered is that

0:34:42.360 --> 0:34:46.440
<v Speaker 1>there really is something in there that's more radioactive than uranium,

0:34:46.840 --> 0:34:48.719
<v Speaker 1>and so they're big discovery was the discovery of a

0:34:48.800 --> 0:34:53.000
<v Speaker 1>new element, which Marie called polonium after her native Poland.

0:34:54.600 --> 0:34:56.840
<v Speaker 1>I see, because like if you take a uranium atom

0:34:56.880 --> 0:35:00.480
<v Speaker 1>and you give it extra protons and new tron's, then

0:35:00.520 --> 0:35:04.160
<v Speaker 1>it becomes a different element. Yeah. Actually, uranium breaks down, right,

0:35:04.160 --> 0:35:07.120
<v Speaker 1>It splits open, it's unstable, and it turns into other

0:35:07.160 --> 0:35:11.400
<v Speaker 1>stuff now we know, into thorium and into radium and

0:35:11.440 --> 0:35:14.600
<v Speaker 1>eventually into polonium and all sorts of stuff. So if

0:35:14.600 --> 0:35:16.799
<v Speaker 1>you have a bunch of uranium, it eventually turns into

0:35:16.800 --> 0:35:20.560
<v Speaker 1>this combination of other elements. It breaks open and turns

0:35:20.600 --> 0:35:24.200
<v Speaker 1>into smaller, lighter elements, some of which are more radioactive

0:35:24.200 --> 0:35:27.200
<v Speaker 1>than uranium itself. So I guess you could say her

0:35:27.280 --> 0:35:31.040
<v Speaker 1>discovery was kind of about nuclear physics, right, even before

0:35:31.040 --> 0:35:33.280
<v Speaker 1>we knew there was a nucleus. She sort of maybe

0:35:33.320 --> 0:35:36.600
<v Speaker 1>intuited that, you know, there's something going on here inside

0:35:36.600 --> 0:35:40.399
<v Speaker 1>of matter and atoms that can somehow, you know, give

0:35:40.400 --> 0:35:45.040
<v Speaker 1>off energy and change into different elements. Right, that's maybe

0:35:45.120 --> 0:35:47.440
<v Speaker 1>was sort of a big contribution, and not so much

0:35:47.440 --> 0:35:50.000
<v Speaker 1>about the radiation, but just kind of about the nature

0:35:50.360 --> 0:35:54.000
<v Speaker 1>of the insides of atoms. Yeah, exactly what the radiation

0:35:54.080 --> 0:35:56.520
<v Speaker 1>reveals about the structure of atoms and the structure of

0:35:56.560 --> 0:35:59.960
<v Speaker 1>matter itself. And you're right, it's totally fascinating to see

0:36:00.000 --> 0:36:03.160
<v Speaker 1>one element turned into another element, and if it does

0:36:03.200 --> 0:36:06.399
<v Speaker 1>that by giving off a particle, that tells you that

0:36:06.480 --> 0:36:09.640
<v Speaker 1>what defines an element must be something related to its

0:36:09.680 --> 0:36:12.560
<v Speaker 1>particle content. Right, You're giving off a piece and you

0:36:12.640 --> 0:36:15.040
<v Speaker 1>turn into something else. That tells you that peace was

0:36:15.120 --> 0:36:17.520
<v Speaker 1>essential for you to be uranium or for you to

0:36:17.600 --> 0:36:20.920
<v Speaker 1>be radium. So that was pretty fascinating clue into the

0:36:20.960 --> 0:36:24.279
<v Speaker 1>structure of the atom itself yet early nuclear physics. And

0:36:24.360 --> 0:36:27.200
<v Speaker 1>so she went on to win the Nobel Prize in

0:36:27.280 --> 0:36:30.760
<v Speaker 1>nineteen o three, same year she got her pH d thesis.

0:36:30.800 --> 0:36:34.080
<v Speaker 1>Oh my goodness, yeah, pretty awesome. Not only the first

0:36:34.120 --> 0:36:36.440
<v Speaker 1>woman to win a Nobel Prize in physics, but the

0:36:36.480 --> 0:36:40.239
<v Speaker 1>first woman in France to receive a PhD. Wow, I

0:36:40.280 --> 0:36:43.759
<v Speaker 1>wonder which one is more significant in a way. So

0:36:43.800 --> 0:36:46.760
<v Speaker 1>she was also in on the third Nobel Prize ever. Yeah,

0:36:47.000 --> 0:36:50.279
<v Speaker 1>she and her husband, Pierre and Beckerel all won the

0:36:50.280 --> 0:36:53.120
<v Speaker 1>Nobel Prize in nineteen o three. But you know, obviously

0:36:53.160 --> 0:36:56.399
<v Speaker 1>she was very deserving, but the initial nomination was only

0:36:56.440 --> 0:36:59.800
<v Speaker 1>for Pierre and Bequerel. They excluded her, probably because she

0:37:00.000 --> 0:37:03.200
<v Speaker 1>as a woman. But Pierre insisted that, hey, look Marie

0:37:03.239 --> 0:37:05.200
<v Speaker 1>has done at least as much work as anybody else.

0:37:05.200 --> 0:37:07.600
<v Speaker 1>She's very deserving. So she ended up being included in

0:37:07.600 --> 0:37:12.120
<v Speaker 1>the Nobel Prize. Great husband there, yeah exactly. Unfortunately he

0:37:12.280 --> 0:37:15.560
<v Speaker 1>died tragically. He was hit by a horse cart filled

0:37:15.600 --> 0:37:19.200
<v Speaker 1>with heavy equipment and was crushed one day, no way

0:37:19.239 --> 0:37:22.080
<v Speaker 1>after all this, so he was killed by horse radiation

0:37:22.200 --> 0:37:27.080
<v Speaker 1>a way exactly. Horses are an energetic particle. I suppose.

0:37:27.520 --> 0:37:29.960
<v Speaker 1>Now we shouldn't laugh over anybody's death. It was tragic

0:37:29.960 --> 0:37:32.719
<v Speaker 1>and it was very difficult for Marie, but she persevered

0:37:33.040 --> 0:37:36.880
<v Speaker 1>and she did a bunch more chemistry and isolated another element, radium,

0:37:37.239 --> 0:37:39.840
<v Speaker 1>for which she won the nineteen eleven Nobel Prize, this

0:37:39.880 --> 0:37:43.480
<v Speaker 1>time in chemistry. Also, it's rare how many people get

0:37:43.520 --> 0:37:46.799
<v Speaker 1>a Nobel Prize for their PhD work. Almost nobody, right,

0:37:47.000 --> 0:37:49.160
<v Speaker 1>not very many. There was the guy who got the

0:37:49.160 --> 0:37:52.719
<v Speaker 1>Nobel Prize for his pH d work. He discovered the

0:37:52.800 --> 0:37:56.560
<v Speaker 1>binary pulsars, which were an excellent test of general relativity.

0:37:57.120 --> 0:37:59.640
<v Speaker 1>Fascinating story there is that he did this work as

0:37:59.640 --> 0:38:02.160
<v Speaker 1>a p h d student. It wasn't really understood or

0:38:02.239 --> 0:38:05.240
<v Speaker 1>appreciated at the time, so he actually left the field

0:38:05.400 --> 0:38:07.640
<v Speaker 1>and then won the Nobel Prize and ended up coming

0:38:07.640 --> 0:38:10.200
<v Speaker 1>back and getting to do more research. So that's pretty fun.

0:38:10.400 --> 0:38:12.640
<v Speaker 1>He was like selling cars and then he gets a

0:38:12.680 --> 0:38:15.680
<v Speaker 1>call not quite that far. He was working in the

0:38:15.680 --> 0:38:18.279
<v Speaker 1>computing division, I think at Princeton, and then he won

0:38:18.320 --> 0:38:19.799
<v Speaker 1>the Nobel Prize and they called him up and they

0:38:19.840 --> 0:38:23.120
<v Speaker 1>were like, so, how big an office would you like? Yeah,

0:38:23.160 --> 0:38:26.560
<v Speaker 1>it's weird to kind of peak that early in your career, right,

0:38:27.120 --> 0:38:30.280
<v Speaker 1>Although Marie kept going. She won a second Nobel Prize,

0:38:30.280 --> 0:38:33.280
<v Speaker 1>and even her daughter won one. Two. Yes, her daughter

0:38:33.320 --> 0:38:37.000
<v Speaker 1>and her daughter's husband worked together again. On radiation and

0:38:37.040 --> 0:38:40.759
<v Speaker 1>they induced artificial radioactivity. They took an element which was

0:38:40.800 --> 0:38:45.279
<v Speaker 1>not radioactive, alunium, and then bombarded it with radiation and

0:38:45.320 --> 0:38:48.240
<v Speaker 1>they made it radioactive. And so that was a pretty

0:38:48.280 --> 0:38:52.160
<v Speaker 1>interesting discovery and they won the Nobel Prize in so

0:38:52.239 --> 0:38:54.520
<v Speaker 1>there's a lot of Nobel Prizes in the Curie family.

0:38:55.160 --> 0:38:58.560
<v Speaker 1>All Right, Well, then at this point, I guess radiation

0:38:58.640 --> 0:39:00.600
<v Speaker 1>is pretty much discovered. I mean, and we sort of

0:39:01.080 --> 0:39:03.560
<v Speaker 1>at that point they knew about X rays and then

0:39:03.600 --> 0:39:08.319
<v Speaker 1>also about kind of particle radiation coming from the nu kids. Yeah,

0:39:08.320 --> 0:39:11.080
<v Speaker 1>and everybody thought that radiation came from stuff, right. We

0:39:11.120 --> 0:39:14.680
<v Speaker 1>had found it in oars, from metals deep within the earth,

0:39:15.080 --> 0:39:17.919
<v Speaker 1>and so people thought, well, if there's radiation around, it's

0:39:17.920 --> 0:39:20.799
<v Speaker 1>coming from the ground beneath us. So people thought if

0:39:20.800 --> 0:39:24.360
<v Speaker 1>you went higher up, like higher altitude, the radiation should decrease,

0:39:24.440 --> 0:39:26.359
<v Speaker 1>right because you're further away from the Earth and all

0:39:26.440 --> 0:39:30.000
<v Speaker 1>these sources of radiation. But people who did measurements found

0:39:30.040 --> 0:39:32.520
<v Speaker 1>something really strange. They found it as you went up

0:39:32.560 --> 0:39:35.680
<v Speaker 1>to the tops of mountains, the amount of radiation seemed

0:39:35.719 --> 0:39:39.359
<v Speaker 1>to be increasing, and that was weird and surprising to people. Right. Yeah,

0:39:39.480 --> 0:39:42.919
<v Speaker 1>that's when we discovered cosmic radiation. Yeah, exactly. So there's

0:39:42.920 --> 0:39:47.640
<v Speaker 1>this wonderfully hilarious pioneering physicist named Victor Hess. This guy

0:39:47.800 --> 0:39:50.320
<v Speaker 1>was born in the castle and his father was a

0:39:50.440 --> 0:39:53.880
<v Speaker 1>royal forester to a prince, and he did these amazing

0:39:53.920 --> 0:39:57.319
<v Speaker 1>experiments where he went up on a balloon with his

0:39:57.400 --> 0:40:01.440
<v Speaker 1>equipment he improved on Pierre's electroscope to measure like ionization

0:40:01.520 --> 0:40:03.880
<v Speaker 1>due to radiation, and he went up on balloons. But

0:40:03.920 --> 0:40:05.759
<v Speaker 1>you couldn't just like send up the balloon and then

0:40:05.800 --> 0:40:07.839
<v Speaker 1>get the data later right like the way we do now,

0:40:07.920 --> 0:40:10.360
<v Speaker 1>because there's no way to record this information. So he

0:40:10.400 --> 0:40:13.719
<v Speaker 1>actually went on these balloon chips himself, like sometimes up

0:40:13.719 --> 0:40:17.319
<v Speaker 1>at night, really high in the atmosphere, a great personal risk.

0:40:17.760 --> 0:40:20.640
<v Speaker 1>But he discovered that as you went up higher and higher,

0:40:20.680 --> 0:40:24.920
<v Speaker 1>even above mountaintops, the amount of radiation increased dramatically. So

0:40:25.040 --> 0:40:27.600
<v Speaker 1>this pointed to something really new and interesting that most

0:40:27.640 --> 0:40:30.600
<v Speaker 1>of the radiation that we were feeling around us wasn't

0:40:30.640 --> 0:40:33.160
<v Speaker 1>coming from the earth beneath us, but from the skies

0:40:33.200 --> 0:40:36.480
<v Speaker 1>above us. I guess once you sort of understand that

0:40:36.520 --> 0:40:40.240
<v Speaker 1>there are invisible, you know, things flying around you coming

0:40:40.239 --> 0:40:42.279
<v Speaker 1>from the earth, and kind of makes you wonder where

0:40:42.280 --> 0:40:44.520
<v Speaker 1>else are these things coming from, or where else can

0:40:44.560 --> 0:40:47.000
<v Speaker 1>you find them exactly? And every time you discover a

0:40:47.040 --> 0:40:49.600
<v Speaker 1>new way to look at the universe, you are bound

0:40:49.600 --> 0:40:53.000
<v Speaker 1>to find something surprising. So discovery of radiation not just

0:40:53.040 --> 0:40:55.200
<v Speaker 1>showed us what was inside the atom and helped us

0:40:55.200 --> 0:40:57.920
<v Speaker 1>see inside our bodies. It also helped us see the

0:40:58.040 --> 0:41:00.640
<v Speaker 1>universe in a new way and to see really really

0:41:00.680 --> 0:41:04.240
<v Speaker 1>bright sources of this new kind of information. And most

0:41:04.239 --> 0:41:06.560
<v Speaker 1>of it was coming from space, and so that was

0:41:06.560 --> 0:41:09.760
<v Speaker 1>a big question mark for decades, like what is making

0:41:09.920 --> 0:41:13.160
<v Speaker 1>radiation out in space and shooting it at us? And

0:41:13.200 --> 0:41:15.680
<v Speaker 1>that's an area of research still today, Like we understand

0:41:15.719 --> 0:41:17.879
<v Speaker 1>a lot of the source of that cosmic radiation now,

0:41:17.880 --> 0:41:20.240
<v Speaker 1>but not all of it, right, Yeah, it's a big mystery.

0:41:20.320 --> 0:41:22.520
<v Speaker 1>It's like it could be anything. Yeah, at the time,

0:41:22.520 --> 0:41:24.799
<v Speaker 1>people really didn't understand. Now we know that a lot

0:41:24.840 --> 0:41:27.280
<v Speaker 1>of that radiation comes from the Sun, it's the solar wind,

0:41:27.520 --> 0:41:30.320
<v Speaker 1>and also comes from outside our solar system, from the galaxy,

0:41:30.600 --> 0:41:32.759
<v Speaker 1>from the black hole at the center of the Milky Way,

0:41:32.760 --> 0:41:35.080
<v Speaker 1>for example, emits a lot of radiation, and other crazy

0:41:35.080 --> 0:41:37.680
<v Speaker 1>stuff out there emits radiation. But there's still a lots

0:41:37.719 --> 0:41:40.320
<v Speaker 1>of this radiation from space that we do not understand.

0:41:40.320 --> 0:41:43.440
<v Speaker 1>The very very high energy particles very tip of that

0:41:43.520 --> 0:41:46.960
<v Speaker 1>spectrum are higher energy than anything we understand can make.

0:41:47.480 --> 0:41:50.600
<v Speaker 1>So radiation is still telling us about the universe and

0:41:50.600 --> 0:41:52.759
<v Speaker 1>giving us clues about things out there that we don't

0:41:52.760 --> 0:41:55.640
<v Speaker 1>know about. I'm guessing the scientists just wanted a better

0:41:55.719 --> 0:41:57.359
<v Speaker 1>view out of his lab. So he's like, I mighta

0:41:57.360 --> 0:42:00.400
<v Speaker 1>put it on a balloon. Yeah, I don't know. Or

0:42:00.440 --> 0:42:02.239
<v Speaker 1>maybe he needed a break from whatever was going on

0:42:02.280 --> 0:42:04.319
<v Speaker 1>in his life and you just need an excuse to

0:42:04.320 --> 0:42:08.120
<v Speaker 1>take a flight this castle to watch castle drama. It's

0:42:08.160 --> 0:42:10.480
<v Speaker 1>like I'm hopping down my balloon to do signs as

0:42:10.520 --> 0:42:12.399
<v Speaker 1>we all do. If they ad made a reality show

0:42:12.440 --> 0:42:14.360
<v Speaker 1>about it, that would have been the dramatic ending to

0:42:14.400 --> 0:42:17.680
<v Speaker 1>an episode as he floats away in his balloon. All right, Well,

0:42:17.719 --> 0:42:20.880
<v Speaker 1>I think that's just a really interesting kind of view

0:42:20.920 --> 0:42:24.239
<v Speaker 1>into how we came to see that there are a

0:42:24.239 --> 0:42:27.040
<v Speaker 1>lot of things that we can't see, right, because how

0:42:27.040 --> 0:42:28.920
<v Speaker 1>else would you know that there's things there if we

0:42:28.960 --> 0:42:31.160
<v Speaker 1>can't see them or hear them. Yeah, and this is

0:42:31.200 --> 0:42:34.319
<v Speaker 1>a pattern in physics that we keep discovering that their

0:42:34.560 --> 0:42:37.800
<v Speaker 1>entire segments of the universe we didn't know anything about

0:42:37.880 --> 0:42:40.480
<v Speaker 1>because for a long time they were invisible to us.

0:42:40.840 --> 0:42:43.360
<v Speaker 1>The discovery of dark matter, for example, we know that

0:42:43.440 --> 0:42:46.520
<v Speaker 1>dark matters out there. It's all around us, it's streaming everywhere.

0:42:46.520 --> 0:42:49.759
<v Speaker 1>It contains vast amounts of information about what's going on

0:42:49.840 --> 0:42:51.920
<v Speaker 1>in the universe and how it was born and how

0:42:51.920 --> 0:42:54.880
<v Speaker 1>it came to be, and we only recently discovered it exists.

0:42:55.280 --> 0:42:58.440
<v Speaker 1>And that tells us that there's almost certainly more stuff

0:42:58.480 --> 0:43:00.560
<v Speaker 1>going on that we haven't yet to open and we

0:43:00.600 --> 0:43:04.359
<v Speaker 1>haven't discovered. That will tell a future physicists crazy things

0:43:04.360 --> 0:43:07.320
<v Speaker 1>about the universe that we cannot yet even anticipate. Yeah,

0:43:07.440 --> 0:43:09.920
<v Speaker 1>and it kind of also reminds you that physics can

0:43:09.960 --> 0:43:13.000
<v Speaker 1>be dangerous, you know, like you're probing the unknown, you're

0:43:13.040 --> 0:43:16.759
<v Speaker 1>exposing yourself to things, yet you don't know whether or

0:43:16.760 --> 0:43:18.680
<v Speaker 1>not the exist or not, or what they're doing to

0:43:18.719 --> 0:43:21.040
<v Speaker 1>your body. Right, that's right. I've eaten a lot of

0:43:21.120 --> 0:43:23.440
<v Speaker 1>very dangerous airline food and all of my trips to

0:43:23.440 --> 0:43:26.440
<v Speaker 1>the large hage On collider. So yeah, your ashes will

0:43:26.480 --> 0:43:30.080
<v Speaker 1>probably glow too, Daniel. All that swift that you're eating,

0:43:30.200 --> 0:43:34.080
<v Speaker 1>it's probably radioactive, Yes, fund is probably not good for you.

0:43:34.400 --> 0:43:36.960
<v Speaker 1>But it's delicious. Yeah, all right, Well that's a pretty

0:43:37.080 --> 0:43:40.239
<v Speaker 1>fascinating trip down science history lane, and I hope it

0:43:40.320 --> 0:43:42.560
<v Speaker 1>encourages all of you who are curious about things we

0:43:42.600 --> 0:43:46.320
<v Speaker 1>don't understand, things we have not yet unraveled, to follow

0:43:46.400 --> 0:43:48.800
<v Speaker 1>up those threads. If you see something you don't understand,

0:43:49.040 --> 0:43:51.160
<v Speaker 1>try to figure it out. If something doesn't make sense

0:43:51.200 --> 0:43:54.480
<v Speaker 1>to you, ask yourself questions until it does. Because remember

0:43:54.760 --> 0:43:57.840
<v Speaker 1>that the history of science is just people being curious,

0:43:57.880 --> 0:44:00.319
<v Speaker 1>trying to figure stuff out, and pushing full word on

0:44:00.360 --> 0:44:03.040
<v Speaker 1>the envelope of human knowledge. Right, yeah, you two can

0:44:03.080 --> 0:44:05.239
<v Speaker 1>win a Nobel prize even if you get kicked out

0:44:05.280 --> 0:44:10.200
<v Speaker 1>of high school for drawing cartoons. That's not an exaggeration.

0:44:10.280 --> 0:44:12.360
<v Speaker 1>All right, Well, we hope you enjoyed that. Thanks for

0:44:12.440 --> 0:44:22.880
<v Speaker 1>joining us, See you next time. Thanks for listening, and

0:44:22.920 --> 0:44:25.640
<v Speaker 1>remember that Daniel and Jorge Explain the Universe is a

0:44:25.680 --> 0:44:29.120
<v Speaker 1>production of I Heart Radio or more podcast for my

0:44:29.239 --> 0:44:32.799
<v Speaker 1>Heart Radio, visit the I Heart Radio Apple Apple Podcasts,

0:44:32.920 --> 0:44:35.280
<v Speaker 1>or wherever you listen to your favorite shows.