WEBVTT - Is there Uranium on Uranus?

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<v Speaker 1>Hey, Kelly, are you a fan of astronomy humor? It

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<v Speaker 1>depends as long as we're not making jokes about urinus. Well,

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<v Speaker 1>we'll have to try to avoid falling into that particular hole.

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<v Speaker 1>But personally, I love a good astronomy pun. I have

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<v Speaker 1>more of a plutonic relationship. Oh no, did you just

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<v Speaker 1>make that joke up or did you have to plan it? Okay,

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<v Speaker 1>I've got one for you. Alright. Why don't stars go

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<v Speaker 1>to university? Alright? Why? Because they've already got millions of degrees.

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<v Speaker 1>I'm sorry. Hi, I'm Daniel. I'm a particle physicist and

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<v Speaker 1>a professor at UC Irvine, and I will always laugh

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<v Speaker 1>at astronomy puns. Hi, I'm Kelly Weener Smith. I'm a

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<v Speaker 1>parasitologist at Rice University, and I think my last name

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<v Speaker 1>is hilarious. So I will always laugh at both parasitology

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<v Speaker 1>puns and scatological humor. There's gotta be a lot of

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<v Speaker 1>good puns when you're talking about worms and bugs and

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<v Speaker 1>things that crawling inside other things. So and they get,

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<v Speaker 1>but we try to keep this podcast family friendly, and

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<v Speaker 1>so we will spare you most of those and so

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<v Speaker 1>welcome to the podcast. Daniel and Jorgey explain the Universe,

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<v Speaker 1>in which we talk about all the incredible and amazing

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<v Speaker 1>things out there in the universe. We crack jokes about

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<v Speaker 1>the silly names they get, but we have a deep,

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<v Speaker 1>deep love for the mysteries of the universe and we

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<v Speaker 1>want to explore all of them with you. We think

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<v Speaker 1>it's incredible. It's amazing that this universe is understandable at

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<v Speaker 1>all to our tiny human brains. We want to push

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<v Speaker 1>forward this effort and bring this understanding of the universe

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<v Speaker 1>into all of our minds because everybody out there has

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<v Speaker 1>questions about how the universe works and wants to know

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<v Speaker 1>where it came from and where it's going to go

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<v Speaker 1>and how it all fits together. So thanks very much

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<v Speaker 1>for joining us on our journey of curiosity. My typical

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<v Speaker 1>co host Orge isn't with us today, and so we

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<v Speaker 1>have are wonderful and hilarious and very punny co host Kelly.

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<v Speaker 1>Thanks for joining us. Kelly, thanks for having me. I'm

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<v Speaker 1>super excited about today's question. Awesome, And you know, on

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<v Speaker 1>this podcast we often talk about things that are very

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<v Speaker 1>far away. We're very distant in space and time, but

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<v Speaker 1>we also have questions about things that happen in our backyard.

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<v Speaker 1>We're very curious about the nature of our environment, how

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<v Speaker 1>the Earth formed, how the Solar system formed, how it

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<v Speaker 1>all came together. You have a very broad definition of

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<v Speaker 1>in our backyard. That's true, I guess, parasitologist, when you

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<v Speaker 1>talk about backyard, you mean literally like what's inside my fence, right,

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<v Speaker 1>That's exactly what I mean. Cosmologically speaking, though, our backyard

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<v Speaker 1>to me is like the stuff that formed with us,

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<v Speaker 1>that has like a common history that we could like

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<v Speaker 1>go and visit it and dig up something on an

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<v Speaker 1>asteroid and from that learned something about the Earth. We

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<v Speaker 1>have like answers in common, and actually later on in

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<v Speaker 1>the episode, we're gonna hear a really cool story about

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<v Speaker 1>how asteroids told us something about the history of our

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<v Speaker 1>planet and how uranium was involved. But you might look

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<v Speaker 1>at our planet and think, like, m it looks kind

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<v Speaker 1>of different from the other planets. I mean, like, we have,

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<v Speaker 1>for example, a nice surface, and we have water, and

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<v Speaker 1>we have an atmosphere, and you know the Moon doesn't

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<v Speaker 1>have that, and Jupiter and Saturn and Neptune and Urine

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<v Speaker 1>is these planets all look very different from ours, and

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<v Speaker 1>so you might wonder like did they form differently? Are

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<v Speaker 1>they made of the same stuff? What do we really

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<v Speaker 1>know about what's going on in the rest of the

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<v Speaker 1>Solar System and how is it all connected? And so

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<v Speaker 1>we thought a fun question to dig into would be

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<v Speaker 1>to ask questions about what's going on inside these other

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<v Speaker 1>big planets. That's a great question. I've been reading a

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<v Speaker 1>bit about what is on the various different planets that

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<v Speaker 1>I'm always surprised by, well by how much for lap

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<v Speaker 1>there tends to be, but also the important things that

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<v Speaker 1>seem to be missing, like carbon on the Moon. It's

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<v Speaker 1>gonna be really hard to grow plants on the Moon

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<v Speaker 1>with no carbon. Do you have plans to go plants

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<v Speaker 1>on the Moon? I do not, but plenty of people do.

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<v Speaker 1>Fun fact, the most concentrated carbon in the Moon is

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<v Speaker 1>probably the bags of feces that the Apollo astronauts left behind.

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<v Speaker 1>And this is why I don't get invited to parties.

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<v Speaker 1>Are those frozen remains from the astronauts also useful because

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<v Speaker 1>they contain like the microbiome of those astronauts from what

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<v Speaker 1>they were eating like forty years ago. I don't think

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<v Speaker 1>that microbiome is going to be useful for much anymore.

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<v Speaker 1>But I also think that according to the Outer Space Treaty,

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<v Speaker 1>those bags of feces technically still belong to NASA, So

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<v Speaker 1>I guess it depends on what NASA wants to do

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<v Speaker 1>with them. Well, if they've become an important resource, we

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<v Speaker 1>could end up with an international or interstellar war sparked

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<v Speaker 1>by astronaut remains. So why hasn't someone written about that

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<v Speaker 1>massive lost opportunity? Contact us if you need book ideas, Guys,

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<v Speaker 1>I'm sure somebody out there has written that science fiction

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<v Speaker 1>story already. But we're not so interested in where astronauts

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<v Speaker 1>have left their remains. Were interested in whether there are

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<v Speaker 1>really big, heavy materials on other planets. Some of the

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<v Speaker 1>most exotic, some of the most amazing, some of the

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<v Speaker 1>weirdest things we find on Earth. We are wondering if

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<v Speaker 1>they also exist on other planets. And so today we

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<v Speaker 1>will be asking is there uranium on Uranus? Now? I

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<v Speaker 1>notice you very carefully pronouncing the title of the planet Uranus. Yes,

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<v Speaker 1>very carefully. I have a seven year old at home,

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<v Speaker 1>and so I have to be careful to not edge

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<v Speaker 1>anywhere near that word, otherwise I can't talk to her

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<v Speaker 1>for about three hours because she's laughing too hard and

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<v Speaker 1>me as well. But is there an option to pronounce

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<v Speaker 1>uranium with the same rhythm, like could you say uranium

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<v Speaker 1>your how you even say that uranium? Uran question? I've

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<v Speaker 1>never thought about it. I don't know. Is there uranium

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<v Speaker 1>on Uranus? Sorry, no, we got it backwards. Is there

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<v Speaker 1>is there urinium? Is there uranium on Uranus? There we go,

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<v Speaker 1>and the rest of the podcast would just be us giggling.

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<v Speaker 1>Control yourself. But it is a serious scientific question whether

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<v Speaker 1>uranium only exists on Earth, because you can imagine in

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<v Speaker 1>the future, as we're exploring the Solar System, we might

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<v Speaker 1>want to mind other planets for useful minerals as we're

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<v Speaker 1>powering our spaceships out of the Solar System or even

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<v Speaker 1>around the Solar System. And also to me, it's just

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<v Speaker 1>a fun question to think about, first of all, how

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<v Speaker 1>it was made in the universe and how it is

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<v Speaker 1>distributed and where it ended up. You know, is the

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<v Speaker 1>Earth unique in its collection of heavy metals or is

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<v Speaker 1>maybe uranium like very common on Urinus and other planets.

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<v Speaker 1>So I think the more than just a giggle factor.

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<v Speaker 1>This is a serious sign diffic question, very serious, very serious. Yes,

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<v Speaker 1>so putting on our serious faces. I went out there

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<v Speaker 1>and I asked folks on the internet listeners to this

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<v Speaker 1>show whether they thought there was uranium on Uranus. So,

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<v Speaker 1>if you would like to participate for future rounds the

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<v Speaker 1>podcast and like to play along at home, please write

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<v Speaker 1>to me two questions at Daniel and Jorge dot com.

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<v Speaker 1>I'd love to hear your answers. I know you're out there.

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<v Speaker 1>You've been listening to the podcast for years and they've

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<v Speaker 1>never written in. Today is the day you right in.

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<v Speaker 1>So think about it for a minute before you listen

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<v Speaker 1>to these answers. Do you think there's uranium on Uranus?

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<v Speaker 1>Here's what people had to say. Earth has it, and

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<v Speaker 1>all the other planets like Mercury, Mars, Asteroids and all

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<v Speaker 1>that have uranium, Uranus being in our Solar system should

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<v Speaker 1>have it too. I would say that, yes, there definitely

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<v Speaker 1>has to be at least one atom of uranium on Uranus,

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<v Speaker 1>seeing that uranium is distributed throughout the universe and um

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<v Speaker 1>maybe concentrated more on rocky planets. But my guess is

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<v Speaker 1>if we look really, really hard, we'd find that one atom. Yeah,

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<v Speaker 1>why not? I guess that's it's a pretty big planet

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<v Speaker 1>and it's mostly gas, but I don't think why there

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<v Speaker 1>shouldn't be any other stuff than what it's made out of,

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<v Speaker 1>because meteors and other things are constantly falling into it,

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<v Speaker 1>and I guess they're bound to be some that consists

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<v Speaker 1>of or have some uranium in them. So yeah, I'm

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<v Speaker 1>pretty confident about that. I would guess yes, because you're

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<v Speaker 1>asking it, but I'm not very confident in that answer.

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<v Speaker 1>I'm gonna guess no. Uranus was named by people who

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<v Speaker 1>did not know what uranium is, but they named it

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<v Speaker 1>after a Greek god in Greek mythology. But what do

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<v Speaker 1>I know? Yeah, I would think so because if I'm

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<v Speaker 1>not mistaken, it's a high pressure environment, and I would

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<v Speaker 1>guess that, you know, heavier elements and radioactive elements like

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<v Speaker 1>uranium would develop in a higher pressure environment like Uranus,

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<v Speaker 1>possibly closer towards the core. If there is any uranium

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<v Speaker 1>on ur I don't think that there would be very

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<v Speaker 1>much of it. There is probably a small amount scattered

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<v Speaker 1>to me amongst the war particles from meteorites or just stardust,

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<v Speaker 1>or maybe it has a rocky core, knows. I think

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<v Speaker 1>it's mostly ice of light liquids, small molecules frozen, so

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<v Speaker 1>it probably has a little. But you know, I think

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<v Speaker 1>that two might be related in namesake only, I would

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<v Speaker 1>say yes, definitely, at least one particle. I don't know.

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<v Speaker 1>I don't think that's what the plan is named for,

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<v Speaker 1>but I don't see a reason why it wouldn't have

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<v Speaker 1>some uranium. Thanks so much for those answers. There were

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<v Speaker 1>some really insightful answers in there. And actually, when Daniel

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<v Speaker 1>proposed this question to me, initially, it made me realize

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<v Speaker 1>that I didn't know how uranus got its name and

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<v Speaker 1>I didn't know the answer to this question. And I

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<v Speaker 1>agreed with some of the listeners. I thought, probably there's

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<v Speaker 1>there's at least some uranium and uranus, because it seems

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<v Speaker 1>like they would sort of have to be like maybe

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<v Speaker 1>if it was in a comment or an asteroid that

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<v Speaker 1>slammed into uranus, even if it wasn't made in there,

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<v Speaker 1>it might show up there. But I actually didn't know

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<v Speaker 1>the answer for sure, So I think I was in

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<v Speaker 1>the same boat as a bunch of these listeners. But

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<v Speaker 1>it turns out that I don't know too much about

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<v Speaker 1>uranus and where it got its name. So can you

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<v Speaker 1>tell us a bit about that, Daniel, Yeah, I love

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<v Speaker 1>this question because it has two really fun science stories,

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<v Speaker 1>the story of Uranus and the story of uranium, and

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<v Speaker 1>then it ties them together. So Urin this is a

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<v Speaker 1>really funny planet because it's history is hilarious, honestly, first

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<v Speaker 1>of all, because it was seen many many times before

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<v Speaker 1>anybody even understood that it was a planet. There's like

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<v Speaker 1>so many missed opportunities to make like a cosmic scale discovery,

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<v Speaker 1>leave your mark on humanity. Even back in like one

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<v Speaker 1>b C. Hipparcos saw it, and there's like recordings of

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<v Speaker 1>people seeing this thing in the sky going back to

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<v Speaker 1>like sixteen ninety or seventeen fifty. People like saw it

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<v Speaker 1>and noted it in their journals, but they didn't realize

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<v Speaker 1>it was a planet for a long time. It still

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<v Speaker 1>blows my mind that people in like the BC era,

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<v Speaker 1>we're looking up at space and had enough of a

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<v Speaker 1>knowledge about like what belonged where that they could notice

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<v Speaker 1>that something new had moved in that like needed to

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<v Speaker 1>be identified or something, Because you know, I still look

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<v Speaker 1>up the night sky and I'm like, oh, that's a

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<v Speaker 1>bunch of stuff up there. Even back then, they were

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<v Speaker 1>doing a much better job than I do at cataloguing

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<v Speaker 1>these things, and I find that very impressive. So what

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<v Speaker 1>did they think that it was? Well, a lot of

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<v Speaker 1>people just thought that it was a star. It's sort

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<v Speaker 1>of dim and slowly moving because it's really far out

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<v Speaker 1>there in the Solar System, and you know, the further

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<v Speaker 1>out you are in the Solar System, the slower you orbit,

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<v Speaker 1>like the actual linear speed is slower because the gravitational

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<v Speaker 1>pull on the planet is less, so you move less rapidly.

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<v Speaker 1>So in our sky urine, this doesn't move very fast.

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<v Speaker 1>So some people just thought it was a star that

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<v Speaker 1>like wandered a little bit because you know, it's sort

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<v Speaker 1>of hard to keep track back in the day about

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<v Speaker 1>what was moving in the sky and what was induced

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<v Speaker 1>by the Earth rotation, etcetera, etcetera, And so for a

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<v Speaker 1>long time people just thought it was a star. And

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<v Speaker 1>then the guy who actually discovered it, a guy named Herschel,

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<v Speaker 1>he saw it in the sky and he thought it

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<v Speaker 1>was a comment at first, so he didn't even realize

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<v Speaker 1>it was a planet. So the guy we give credit

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<v Speaker 1>to for discovering it actually thought it was a comment

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<v Speaker 1>when he saw it and recorded it. Don't comments tend

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<v Speaker 1>to move faster than planets. I guess it's like more

0:12:58.360 --> 0:13:00.920
<v Speaker 1>than two years ago. So calculating this stuff was tough.

0:13:01.000 --> 0:13:02.960
<v Speaker 1>But why did you think it was a commet? Well

0:13:03.000 --> 0:13:06.679
<v Speaker 1>because he did the calculation very carefully, because other people

0:13:06.760 --> 0:13:09.400
<v Speaker 1>looked at his results and his data and they calculated

0:13:09.440 --> 0:13:12.120
<v Speaker 1>the orbit from his data and they're like, no, that's

0:13:12.160 --> 0:13:14.840
<v Speaker 1>not the orbit of a comet. That must be a planet.

0:13:14.880 --> 0:13:16.760
<v Speaker 1>You know what's the difference. The difference is that the

0:13:16.760 --> 0:13:19.199
<v Speaker 1>comet is like very eccentric orbit. A lot of these

0:13:19.240 --> 0:13:22.000
<v Speaker 1>things come from like the Ort cloud, like really far

0:13:22.120 --> 0:13:24.600
<v Speaker 1>out there in the Solar System, and then they exume

0:13:24.840 --> 0:13:27.840
<v Speaker 1>in very close to the Sun before zooming out, whereas

0:13:27.840 --> 0:13:30.600
<v Speaker 1>the planet is like a much larger object that's obviously

0:13:30.800 --> 0:13:34.560
<v Speaker 1>cleared its field and orbits with a much more circular orbit.

0:13:34.600 --> 0:13:37.680
<v Speaker 1>Not perfectly circular, but much more circular. And so it

0:13:37.760 --> 0:13:40.760
<v Speaker 1>was other people who looked at Herschel's data and they

0:13:40.880 --> 0:13:43.120
<v Speaker 1>decided it was a planet, and it was only Herschel

0:13:43.200 --> 0:13:45.719
<v Speaker 1>later being like, oh, okay, yeah, I agree with you.

0:13:46.040 --> 0:13:48.319
<v Speaker 1>What I saw was a planet. So like, I don't

0:13:48.360 --> 0:13:51.800
<v Speaker 1>even know why he gets credit for this? There did

0:13:51.800 --> 0:13:53.480
<v Speaker 1>he get to name it? And so then there was

0:13:53.520 --> 0:13:56.719
<v Speaker 1>like a seventy year argument about how to name it.

0:13:56.760 --> 0:14:00.040
<v Speaker 1>So Herschel wanted to name it George's Star, which is

0:14:00.080 --> 0:14:02.840
<v Speaker 1>like a terrible name because it's not a star, so

0:14:02.880 --> 0:14:04.400
<v Speaker 1>he thought he was a comment. He wanted to name

0:14:04.440 --> 0:14:07.080
<v Speaker 1>it after a star, which makes those sense. Other people

0:14:07.280 --> 0:14:10.560
<v Speaker 1>wanted to name it Neptune because we didn't have Neptune yet,

0:14:10.679 --> 0:14:14.040
<v Speaker 1>or Neptune Great Britain, like even more awkward name if

0:14:14.040 --> 0:14:18.439
<v Speaker 1>you can imagine. And finally somebody else suggested naming Uranus

0:14:18.480 --> 0:14:21.200
<v Speaker 1>after the god of the sky, you know, to follow

0:14:21.240 --> 0:14:24.120
<v Speaker 1>this pattern that were naming the planets after these Greek

0:14:24.160 --> 0:14:26.400
<v Speaker 1>and Roman gods. And so there was a long, like

0:14:26.600 --> 0:14:29.600
<v Speaker 1>seventy year battle about what to call this thing. One

0:14:29.600 --> 0:14:32.160
<v Speaker 1>group of people calling it Uranus, another group of people

0:14:32.400 --> 0:14:36.040
<v Speaker 1>calling it George's Star. And it wasn't until eighteen fifty

0:14:36.080 --> 0:14:39.400
<v Speaker 1>when the British Navy the bureaucracy finally accepted the name

0:14:39.520 --> 0:14:42.680
<v Speaker 1>Uranus that it like formally became Uranus. So it was

0:14:42.720 --> 0:14:45.560
<v Speaker 1>like seventy years when people are arguing about like just

0:14:45.600 --> 0:14:48.040
<v Speaker 1>what to call this thing, So like did they know

0:14:48.160 --> 0:14:50.800
<v Speaker 1>what they were doing at the time, because anatomy was

0:14:50.840 --> 0:14:53.680
<v Speaker 1>pretty far along at that point. Did they realize school

0:14:53.760 --> 0:14:57.720
<v Speaker 1>children would be laughing for generations to come, or had

0:14:57.800 --> 0:15:00.120
<v Speaker 1>had all the body parts not been quite named at

0:15:00.120 --> 0:15:02.720
<v Speaker 1>at that point. That is a great question, and it

0:15:02.800 --> 0:15:05.080
<v Speaker 1>might also have to do with like the evolution of

0:15:05.120 --> 0:15:07.800
<v Speaker 1>the British accent. Right, I don't know what that word

0:15:07.920 --> 0:15:10.200
<v Speaker 1>sounded like a hundred and fifty years ago, or what

0:15:10.320 --> 0:15:12.960
<v Speaker 1>those two words that you have in mind sounded like,

0:15:13.040 --> 0:15:15.120
<v Speaker 1>and if they sounded more or less similar, that's a

0:15:15.120 --> 0:15:18.360
<v Speaker 1>great question. Linguists out there or historians of the British

0:15:18.360 --> 0:15:20.600
<v Speaker 1>accent please write to us and let us know how

0:15:20.640 --> 0:15:23.680
<v Speaker 1>similar those two words sounded over the years. We asked

0:15:23.680 --> 0:15:26.920
<v Speaker 1>the big questions we do. We go all the way

0:15:27.000 --> 0:15:29.600
<v Speaker 1>up there and ask all the big questions. But you know,

0:15:29.640 --> 0:15:32.920
<v Speaker 1>it turns out to be scientifically, are really fascinating planet

0:15:33.000 --> 0:15:35.000
<v Speaker 1>for lots of reasons. One reason is that it's a

0:15:35.040 --> 0:15:39.400
<v Speaker 1>great example of a giant planet that's not a gas giant,

0:15:39.800 --> 0:15:42.600
<v Speaker 1>right like Jupiter and Saturn. We call these planets gas

0:15:42.640 --> 0:15:46.680
<v Speaker 1>giants because they're mostly hydrogen, but Neptune and Uranus we

0:15:46.720 --> 0:15:50.520
<v Speaker 1>call them ice giants because they really are a different composition.

0:15:50.680 --> 0:15:52.640
<v Speaker 1>And is that water ice or is that some other

0:15:52.720 --> 0:15:55.400
<v Speaker 1>kind of ice? So there's a mixture of water, ice

0:15:55.560 --> 0:15:59.480
<v Speaker 1>and ammonia and also methane, and the difference is really

0:15:59.520 --> 0:16:01.960
<v Speaker 1>that sort of like a race to get the gas.

0:16:02.360 --> 0:16:04.760
<v Speaker 1>Like in the formation of the Solar System, you start

0:16:04.800 --> 0:16:07.880
<v Speaker 1>out with a huge blob of stuff which is mostly hydrogen,

0:16:08.120 --> 0:16:09.920
<v Speaker 1>and then you know there's some rock and some water

0:16:10.000 --> 0:16:12.520
<v Speaker 1>and some other stuff, but really by mass, it's almost

0:16:12.520 --> 0:16:15.960
<v Speaker 1>all hydrogen, and almost all of it grabbed by the Sun.

0:16:16.160 --> 0:16:18.600
<v Speaker 1>Right the whole Solar system is formed, because the Sun

0:16:18.680 --> 0:16:22.480
<v Speaker 1>begins this gravitational collapse and because it becomes very quickly

0:16:22.520 --> 0:16:25.280
<v Speaker 1>the densest thing, the heaviest thing, then it grabs all

0:16:25.280 --> 0:16:27.920
<v Speaker 1>the gas. Like hydrogen, gas is very light and so

0:16:28.000 --> 0:16:30.520
<v Speaker 1>gravity pulls on it very effectively. So then to have

0:16:30.640 --> 0:16:33.000
<v Speaker 1>any gas, to accumulate any gas, you have to build

0:16:33.080 --> 0:16:35.960
<v Speaker 1>up enough mass to steal some from the forming Sun,

0:16:36.200 --> 0:16:38.880
<v Speaker 1>and so if you don't get big enough fast enough,

0:16:38.960 --> 0:16:42.040
<v Speaker 1>then you don't really get very much gas. So Jupiter

0:16:42.120 --> 0:16:44.600
<v Speaker 1>and Saturn like past this point where they can sort

0:16:44.640 --> 0:16:46.960
<v Speaker 1>of have a runaway effect and grab some of the

0:16:47.000 --> 0:16:49.200
<v Speaker 1>gas before the Sun got almost all of it. But

0:16:49.360 --> 0:16:52.760
<v Speaker 1>Neptune and Uriness didn't get big enough fast enough, so

0:16:52.800 --> 0:16:55.400
<v Speaker 1>they just ended up like a blob of ice and rock.

0:16:55.640 --> 0:16:57.760
<v Speaker 1>So like the Moon and Mars didn't get most of

0:16:57.800 --> 0:17:01.080
<v Speaker 1>those gas either, and then Earth got theres from getting

0:17:01.120 --> 0:17:03.640
<v Speaker 1>collided with stuff. Yeah, and we have a whole fun

0:17:03.640 --> 0:17:06.080
<v Speaker 1>episode about how the Earth got its atmosphere. It had

0:17:06.119 --> 0:17:08.240
<v Speaker 1>a little bit of gas in the beginning, but then

0:17:08.280 --> 0:17:11.120
<v Speaker 1>it was mostly stolen away by the Sun and blown off,

0:17:11.160 --> 0:17:14.520
<v Speaker 1>and then it later recreated its atmosphere from volcanoes and

0:17:14.560 --> 0:17:17.320
<v Speaker 1>commentary collisions. It's an incredible story. And that's one of

0:17:17.359 --> 0:17:19.399
<v Speaker 1>the things I love about these questions is that it

0:17:19.440 --> 0:17:22.520
<v Speaker 1>tells you the rich, rich history of the Solar System.

0:17:22.720 --> 0:17:25.159
<v Speaker 1>It's not just like, oh, the planets formed and then

0:17:25.160 --> 0:17:27.520
<v Speaker 1>they were zooming around for four and a half billion years.

0:17:27.560 --> 0:17:31.479
<v Speaker 1>Like there are twists and turns and new characters and

0:17:31.520 --> 0:17:34.639
<v Speaker 1>like lost characters, and probably planets that existed in the

0:17:34.640 --> 0:17:36.920
<v Speaker 1>Solar System for millions or billions of years which are

0:17:36.920 --> 0:17:39.840
<v Speaker 1>now lost because they've been thrown out when Jupiter went

0:17:39.920 --> 0:17:43.159
<v Speaker 1>like in and then out again. It's a crazy story.

0:17:43.240 --> 0:17:45.560
<v Speaker 1>It's like a soap opera, and it's amazing we've figured

0:17:45.600 --> 0:17:49.320
<v Speaker 1>any of it out. So Urinest didn't managed to grab

0:17:49.359 --> 0:17:51.600
<v Speaker 1>this stuff and then it didn't have the like help

0:17:51.720 --> 0:17:54.399
<v Speaker 1>that Earth had to get it with all of that

0:17:54.440 --> 0:17:56.000
<v Speaker 1>other stuff, and so that's how it ended up with

0:17:56.040 --> 0:17:58.080
<v Speaker 1>not a lot of gas, that's right, And so we

0:17:58.119 --> 0:18:01.280
<v Speaker 1>don't actually know that much about what's in Urinus. We

0:18:01.320 --> 0:18:04.760
<v Speaker 1>have a model roughly for what it looks like, but

0:18:04.840 --> 0:18:07.320
<v Speaker 1>it's important to realize that we haven't really studied it

0:18:07.440 --> 0:18:09.720
<v Speaker 1>very much. We've looked at it with telescopes. We sent

0:18:09.920 --> 0:18:12.480
<v Speaker 1>one probe by it voyage or two, but that's really

0:18:12.560 --> 0:18:16.199
<v Speaker 1>the only close flyby of Uranus we've ever had. And

0:18:16.240 --> 0:18:18.480
<v Speaker 1>so we have a model for what's going on inside it,

0:18:18.520 --> 0:18:22.160
<v Speaker 1>which comes mostly from these models of solar system formation,

0:18:22.240 --> 0:18:24.480
<v Speaker 1>like what do we think had time to get in there?

0:18:24.680 --> 0:18:27.879
<v Speaker 1>And that model looks like a rocky core, so like

0:18:28.040 --> 0:18:31.320
<v Speaker 1>basically a huge rock about like half of the mass

0:18:31.320 --> 0:18:33.439
<v Speaker 1>of the Earth, and that's at the very center of it,

0:18:33.480 --> 0:18:36.160
<v Speaker 1>and then it's surrounded most of the mass of urine.

0:18:36.160 --> 0:18:39.200
<v Speaker 1>Is is this icy mantle and you know, we say ice,

0:18:39.240 --> 0:18:43.360
<v Speaker 1>but it's mostly like a big water ammonia ocean. It's

0:18:43.400 --> 0:18:45.920
<v Speaker 1>like liquid or it's or it's fluid. At least it's

0:18:46.000 --> 0:18:48.520
<v Speaker 1>under a lot of pressure, so it can still move

0:18:48.600 --> 0:18:51.280
<v Speaker 1>and flow. So do the way the Earth's mantle can,

0:18:51.400 --> 0:18:54.000
<v Speaker 1>but you wouldn't say necessarily that it's liquid. So I

0:18:54.040 --> 0:18:55.960
<v Speaker 1>think I'm getting confused yet. So so we you know,

0:18:55.960 --> 0:18:57.960
<v Speaker 1>when we were talking about it not picking up a

0:18:57.960 --> 0:18:59.919
<v Speaker 1>bunch of stuff, where did all this water in them

0:19:00.000 --> 0:19:01.680
<v Speaker 1>when you come from? Was? Was that just stuff it

0:19:01.720 --> 0:19:04.359
<v Speaker 1>got lucky to grab initially or did it come somewhere

0:19:04.359 --> 0:19:06.240
<v Speaker 1>else from Earth? I feel like I already asked this question,

0:19:06.320 --> 0:19:08.919
<v Speaker 1>but now I'm confused about where all this water came from. Right,

0:19:08.920 --> 0:19:11.639
<v Speaker 1>So there's a huge amount of water and ice and

0:19:11.680 --> 0:19:14.800
<v Speaker 1>ammonia in the Solar system. So the initial formation of

0:19:14.800 --> 0:19:17.400
<v Speaker 1>the Solar system, you have this cloud of hydrogen. Most

0:19:17.400 --> 0:19:20.159
<v Speaker 1>of the hydrogen went to the gas giants, but the

0:19:20.240 --> 0:19:22.360
<v Speaker 1>other stuff is heavier, it's slower, and so it's sort

0:19:22.400 --> 0:19:25.600
<v Speaker 1>of more likely to accumulate where it was initially. And

0:19:25.640 --> 0:19:27.840
<v Speaker 1>this stuff is far enough out from the Sun that

0:19:27.920 --> 0:19:30.880
<v Speaker 1>it stays frozen, so like the water is an ice

0:19:30.960 --> 0:19:33.480
<v Speaker 1>form and the ammonia is frozen. And so all of

0:19:33.480 --> 0:19:36.080
<v Speaker 1>this stuff that formed Urineus and Neptune and that was

0:19:36.119 --> 0:19:37.919
<v Speaker 1>the stuff that was sort of in the outskirts of

0:19:37.960 --> 0:19:41.119
<v Speaker 1>the Solar system originally, and then just sort of like coalesced. Like.

0:19:41.240 --> 0:19:44.040
<v Speaker 1>Even further out in the Solar System is the Earth Cloud,

0:19:44.080 --> 0:19:47.760
<v Speaker 1>which is a bunch more frozen objects that become comets,

0:19:47.760 --> 0:19:50.639
<v Speaker 1>and those are also just balls of ice. So everything

0:19:50.640 --> 0:19:53.000
<v Speaker 1>that's really really far out in the Solar System is

0:19:53.000 --> 0:19:55.359
<v Speaker 1>basically just rock and ice at this point, and it

0:19:55.400 --> 0:19:58.840
<v Speaker 1>pulls together to form these ice giant planets. I'm with

0:19:58.880 --> 0:20:00.880
<v Speaker 1>you now. So the core of it is this big rock,

0:20:01.080 --> 0:20:04.719
<v Speaker 1>and then outside of that, like thirteen masses of the Earth,

0:20:05.280 --> 0:20:08.560
<v Speaker 1>is this hot, dense fluid. It's not frozen, right, It's

0:20:08.600 --> 0:20:11.600
<v Speaker 1>called ice, but it's not frozen. It's it's very confusing,

0:20:11.760 --> 0:20:14.680
<v Speaker 1>so it's sort of like an ocean. It's more like liquid,

0:20:14.760 --> 0:20:17.920
<v Speaker 1>but it's not technically in that phase. So chemists out

0:20:17.920 --> 0:20:20.080
<v Speaker 1>there would be particular about how this is referred to,

0:20:20.280 --> 0:20:23.000
<v Speaker 1>but they do definitely call it an ice, and that's

0:20:23.000 --> 0:20:26.040
<v Speaker 1>what most of Urinus is. And then outside of that,

0:20:26.080 --> 0:20:29.000
<v Speaker 1>there's like an envelope. There's an atmosphere that's like another

0:20:29.080 --> 0:20:31.160
<v Speaker 1>half the mass of the Earth, and that has some

0:20:31.280 --> 0:20:33.639
<v Speaker 1>hydrogen and some other gases in it. That's sort of

0:20:33.640 --> 0:20:36.560
<v Speaker 1>like the triple layers of Uranus. So I watch a

0:20:36.600 --> 0:20:39.040
<v Speaker 1>bunch of kids shows with my kids, and I feel

0:20:39.040 --> 0:20:41.400
<v Speaker 1>like the one fact about Urinus that we always hear

0:20:41.640 --> 0:20:44.080
<v Speaker 1>is that it rotates on its side. Do we know

0:20:44.680 --> 0:20:47.960
<v Speaker 1>why it's rotated? Why all those layers are rotating the

0:20:48.000 --> 0:20:50.520
<v Speaker 1>wrong way? Did it get hit by something and sort

0:20:50.560 --> 0:20:54.520
<v Speaker 1>of knocked off kilter. It's super cool that it's doing that, because,

0:20:54.560 --> 0:20:57.720
<v Speaker 1>as you say, it's evidence that something happened, And the

0:20:57.760 --> 0:21:00.399
<v Speaker 1>reason it has to be evidence that something happened is

0:21:00.440 --> 0:21:03.600
<v Speaker 1>that we're pretty sure a planet can't just naturally form

0:21:03.680 --> 0:21:06.560
<v Speaker 1>that way. You notice that, like all the planets are

0:21:06.640 --> 0:21:08.600
<v Speaker 1>sort of in the same plane. That's the plane we

0:21:08.640 --> 0:21:11.879
<v Speaker 1>call the ecliptic, and it's also very well aligned with

0:21:11.880 --> 0:21:15.199
<v Speaker 1>how the Sun rotates, So the Sun is spinning as well. Right,

0:21:15.240 --> 0:21:16.800
<v Speaker 1>it's not just sitting there in the center of the

0:21:16.840 --> 0:21:19.879
<v Speaker 1>Solar System. It spins and the planets spin around it,

0:21:19.920 --> 0:21:22.560
<v Speaker 1>and each of the planets then spin around their axes,

0:21:22.920 --> 0:21:25.640
<v Speaker 1>and almost all of this spin is in the same direction,

0:21:26.040 --> 0:21:27.919
<v Speaker 1>Like if you drew a line between the north and

0:21:27.920 --> 0:21:29.919
<v Speaker 1>the south pole of the Sun, that would give you

0:21:30.000 --> 0:21:33.000
<v Speaker 1>an axis, and most of the Solar System is on

0:21:33.040 --> 0:21:36.000
<v Speaker 1>a plane perpendicular to that, and most of the planets

0:21:36.160 --> 0:21:39.040
<v Speaker 1>rotate around their own axis that's parallel to the Sun's axis.

0:21:39.040 --> 0:21:41.840
<v Speaker 1>So for most of the Solar System it's very well organized.

0:21:42.080 --> 0:21:44.000
<v Speaker 1>And that's not like a coincidence. It's not like it

0:21:44.080 --> 0:21:46.200
<v Speaker 1>just happened to end up that way, like we could

0:21:46.200 --> 0:21:48.960
<v Speaker 1>have had planets in any random direction. It comes from

0:21:49.040 --> 0:21:52.440
<v Speaker 1>angular momentum conservation. Like when something is spinning, it has

0:21:52.480 --> 0:21:54.399
<v Speaker 1>to keep spinning. There's no way like for it to

0:21:54.480 --> 0:21:57.480
<v Speaker 1>stop spinning unless you come in with something from the outside,

0:21:57.640 --> 0:21:59.920
<v Speaker 1>like if you start a top spinning in space is

0:22:00.080 --> 0:22:02.440
<v Speaker 1>just going to keep going forever. And that's what happened

0:22:02.480 --> 0:22:05.879
<v Speaker 1>with the Solar system, is that it collapses gravitationally but

0:22:06.040 --> 0:22:08.120
<v Speaker 1>has to keep spinning, and so it has to keep

0:22:08.119 --> 0:22:11.439
<v Speaker 1>spinning around that original axis. It can collapse sort of

0:22:11.800 --> 0:22:13.760
<v Speaker 1>parallel to that axis, which is why you get a

0:22:13.760 --> 0:22:17.359
<v Speaker 1>flat disc, but the disc itself can't collapse much further

0:22:17.440 --> 0:22:20.240
<v Speaker 1>because it has to keep spinning. So everything spinning sort

0:22:20.400 --> 0:22:24.040
<v Speaker 1>along the same axis. So to get urinous knocked over

0:22:24.080 --> 0:22:27.280
<v Speaker 1>on its side requires, as you said, like some huge

0:22:27.520 --> 0:22:31.480
<v Speaker 1>rock like a lost moon or another planet somehow that

0:22:31.560 --> 0:22:34.119
<v Speaker 1>banged into it and knocked it over. So it's really

0:22:34.240 --> 0:22:37.120
<v Speaker 1>is evidence of like an incredible cosmic collision. I feel

0:22:37.119 --> 0:22:38.840
<v Speaker 1>like I'm just going to go ahead and blame Jupiter

0:22:38.960 --> 0:22:41.959
<v Speaker 1>because it seems like the answer for so many things is, well,

0:22:42.080 --> 0:22:44.919
<v Speaker 1>Jupiter did something weird and that might not be consistent,

0:22:45.080 --> 0:22:47.080
<v Speaker 1>but I'm going to go ahead and blame Jupiter anyway,

0:22:47.119 --> 0:22:50.080
<v Speaker 1>because is that your parenting strategy? You like, you pick

0:22:50.119 --> 0:22:52.280
<v Speaker 1>one kid who's always to blame. You're like, look, I

0:22:52.320 --> 0:22:55.160
<v Speaker 1>didn't see it, but it's usually you. But I pretty

0:22:55.240 --> 0:22:57.679
<v Speaker 1>much know the Actually it's the dog that I usually

0:22:57.960 --> 0:23:01.280
<v Speaker 1>There you go. The dog is the source of chaos. Yes,

0:23:01.400 --> 0:23:04.440
<v Speaker 1>you know. I think that's an underappreciated role of dogs

0:23:04.520 --> 0:23:06.760
<v Speaker 1>in human history. You know, it's just taken the blame

0:23:06.840 --> 0:23:10.680
<v Speaker 1>for other people's misdeeds or farts around the campfire or

0:23:10.680 --> 0:23:14.760
<v Speaker 1>all sorts of stuff. She is the scapegoat, but she's

0:23:14.800 --> 0:23:17.800
<v Speaker 1>a good sport about it, all right. Well, so now

0:23:17.840 --> 0:23:21.280
<v Speaker 1>we're all on board about what urineus is like, so

0:23:21.359 --> 0:23:23.280
<v Speaker 1>I think it's time that we take a little break

0:23:23.400 --> 0:23:39.160
<v Speaker 1>and then we'll get to uranium. Okay, so now we've

0:23:39.200 --> 0:23:43.359
<v Speaker 1>talked about what we know about uranus, and uranus and

0:23:43.840 --> 0:23:48.399
<v Speaker 1>uranium sound really similar. So let's learn about uranium and

0:23:48.440 --> 0:23:50.800
<v Speaker 1>see if there's any connection. There, So there actually is

0:23:50.920 --> 0:23:54.600
<v Speaker 1>some connection in the name. I mentioned earlier that when

0:23:54.600 --> 0:23:56.280
<v Speaker 1>they discovered the planet there was a bit of an

0:23:56.320 --> 0:23:59.440
<v Speaker 1>argument about what to name it, And so Uranium was

0:23:59.520 --> 0:24:03.560
<v Speaker 1>discovered about eight years after Uranus, and the guy who

0:24:03.720 --> 0:24:07.800
<v Speaker 1>named uranium uranium did so sort of to vote for

0:24:08.119 --> 0:24:10.560
<v Speaker 1>Uranus as the name of the planet. He was like,

0:24:10.640 --> 0:24:14.199
<v Speaker 1>naming uranium after this newly discovered planet. He wanted to

0:24:14.240 --> 0:24:19.000
<v Speaker 1>influence the astronomy community towards the name Uranus. WHOA, So

0:24:19.119 --> 0:24:21.000
<v Speaker 1>did he have any influence? Like he did it? But

0:24:21.119 --> 0:24:22.800
<v Speaker 1>did it matter? Do we know? I don't know. We

0:24:22.840 --> 0:24:25.119
<v Speaker 1>have to run the counter experiment or we see what

0:24:25.119 --> 0:24:27.480
<v Speaker 1>would have happened if he hadn't done that. I'm not sure,

0:24:27.840 --> 0:24:30.119
<v Speaker 1>but I think it was always going to be Uranus.

0:24:30.160 --> 0:24:31.480
<v Speaker 1>It was just, you know, it's going to be a

0:24:31.480 --> 0:24:34.080
<v Speaker 1>matter of time before the British bureaucracy gave it up.

0:24:34.160 --> 0:24:37.399
<v Speaker 1>What a kind of crumby reason for naming an element, though, like,

0:24:37.800 --> 0:24:41.320
<v Speaker 1>unless there's some astronomy connection there to just be like no, no,

0:24:41.359 --> 0:24:43.880
<v Speaker 1>I really want you to do this naming thing. But anyway,

0:24:43.920 --> 0:24:46.359
<v Speaker 1>I guess you know, we're all humans. Our logic is

0:24:46.400 --> 0:24:49.359
<v Speaker 1>sometimes convoluted. Yeah, And you know, you discover something, you

0:24:49.400 --> 0:24:51.320
<v Speaker 1>get to name it. You don't always have a good reason.

0:24:51.359 --> 0:24:53.359
<v Speaker 1>As we talked about a lot on this podcast, some

0:24:53.440 --> 0:24:56.000
<v Speaker 1>of these names are pretty whimsical and pretty ridiculous. I mean,

0:24:56.000 --> 0:24:59.000
<v Speaker 1>there's like Berkeley m and California UM and Americum, and

0:24:59.280 --> 0:25:01.960
<v Speaker 1>the names the elements are pretty silly, fair enough, some

0:25:02.040 --> 0:25:04.439
<v Speaker 1>of them are fun to say, like you SI, But

0:25:04.520 --> 0:25:06.639
<v Speaker 1>as we talked about earlier, the planets each have a

0:25:06.640 --> 0:25:09.399
<v Speaker 1>really cool story. Each of the elements also has a

0:25:09.520 --> 0:25:13.159
<v Speaker 1>really really cool story that goes back much much further

0:25:13.600 --> 0:25:16.640
<v Speaker 1>than the story of our particular solar system. So tell

0:25:16.720 --> 0:25:18.800
<v Speaker 1>us about how this one was found. So the important

0:25:18.800 --> 0:25:22.680
<v Speaker 1>thing to understand about uranium is that it's not made primordially,

0:25:23.000 --> 0:25:25.600
<v Speaker 1>like the very beginning of the universe, when things are

0:25:25.600 --> 0:25:28.640
<v Speaker 1>super hot and dance in these particles whizzing around everywhere,

0:25:28.720 --> 0:25:31.720
<v Speaker 1>and then things are cooling down. Just after the Big Bang,

0:25:31.760 --> 0:25:35.400
<v Speaker 1>we get atoms formed, but mostly we just made hydrogen

0:25:35.520 --> 0:25:38.520
<v Speaker 1>and a very small amount of helium. So the very

0:25:38.520 --> 0:25:42.240
<v Speaker 1>early universe is basically just like a huge hydrogen cloud,

0:25:42.640 --> 0:25:46.240
<v Speaker 1>definitely no uranium. So uranium does not date back to

0:25:46.320 --> 0:25:49.000
<v Speaker 1>the beginning of the Big Bang like the electrons in

0:25:49.000 --> 0:25:51.360
<v Speaker 1>your body, and the protons in your body are probably

0:25:51.480 --> 0:25:56.560
<v Speaker 1>older than every uranium nucleus out there, so uranium came later, Right,

0:25:56.600 --> 0:25:59.480
<v Speaker 1>It took a while to make uranium in our universe.

0:25:59.600 --> 0:26:01.280
<v Speaker 1>It's really cool, and we're gonna do a whole podcast

0:26:01.280 --> 0:26:04.199
<v Speaker 1>episode focused just on like what is out there in

0:26:04.200 --> 0:26:06.640
<v Speaker 1>the universe and how is made in the relative population

0:26:06.680 --> 0:26:09.320
<v Speaker 1>of all these materials, because they all tell such cool stories,

0:26:09.440 --> 0:26:11.600
<v Speaker 1>and it took a while for people to figure out, like, well,

0:26:11.680 --> 0:26:14.199
<v Speaker 1>where did all the rest of this stuff come from? Like,

0:26:14.240 --> 0:26:17.960
<v Speaker 1>once they realized that you couldn't make anything heavier than

0:26:18.040 --> 0:26:20.639
<v Speaker 1>helium or a little bit of lithium in the Big Bang,

0:26:20.960 --> 0:26:23.040
<v Speaker 1>they had to look around to find a place in

0:26:23.080 --> 0:26:26.080
<v Speaker 1>the universe to make these heavier elements, and it took

0:26:26.080 --> 0:26:27.919
<v Speaker 1>people a while, but they figured out that some of

0:26:27.920 --> 0:26:31.000
<v Speaker 1>the elements could be made, of course, inside stars, and

0:26:31.160 --> 0:26:34.000
<v Speaker 1>it's the intense heat and pressure that allows you to

0:26:34.000 --> 0:26:37.080
<v Speaker 1>make these things. Yes, stars operate by fusion, right, so

0:26:37.080 --> 0:26:39.800
<v Speaker 1>they are glowing and super hot, and they're this exciting

0:26:39.920 --> 0:26:43.440
<v Speaker 1>balance between gravity which is compressing all of this stuff.

0:26:43.440 --> 0:26:45.560
<v Speaker 1>It's like a runaway effect where you got this huge

0:26:45.600 --> 0:26:49.320
<v Speaker 1>compression of all this hydrogen gas, and then fusion. If

0:26:49.359 --> 0:26:52.960
<v Speaker 1>you get all these protons close enough together, you squeeze

0:26:52.960 --> 0:26:55.560
<v Speaker 1>them together, you overcome the fact that they like to

0:26:55.600 --> 0:26:58.480
<v Speaker 1>repel each other because they're both too positive charges, and

0:26:58.480 --> 0:27:02.560
<v Speaker 1>eventually they form heavier off So two hydrogen atoms confused

0:27:02.560 --> 0:27:05.640
<v Speaker 1>together to form helium and helium confused together to form

0:27:05.640 --> 0:27:08.000
<v Speaker 1>heavier stuff. And if you have a big enough star,

0:27:08.080 --> 0:27:10.920
<v Speaker 1>then the products of one fusion cycle, like the helium

0:27:10.920 --> 0:27:14.000
<v Speaker 1>from fusing hydrogen, can become the fuel for the next one,

0:27:14.280 --> 0:27:16.200
<v Speaker 1>and then the fuel for the next one, and really

0:27:16.240 --> 0:27:19.159
<v Speaker 1>big stars they develop these incredible layers we have like

0:27:19.400 --> 0:27:22.160
<v Speaker 1>hydrogen on the outside, and then a layer of helium,

0:27:22.240 --> 0:27:24.000
<v Speaker 1>and then a layer of something heavier and a layer

0:27:24.040 --> 0:27:26.560
<v Speaker 1>of something heavy go calcium and oxygen, and all the

0:27:26.600 --> 0:27:30.720
<v Speaker 1>way up, and the biggest stars they confuse stuff all

0:27:30.760 --> 0:27:34.240
<v Speaker 1>the way up to iron. So iron is element fifty six,

0:27:34.560 --> 0:27:37.240
<v Speaker 1>and it means that at the core something is fusing

0:27:37.320 --> 0:27:40.520
<v Speaker 1>two elements together and producing iron. And that's where a

0:27:40.600 --> 0:27:42.480
<v Speaker 1>lot of these elements that are too heavy to have

0:27:42.480 --> 0:27:45.320
<v Speaker 1>been made in the Big Bang are made. But stars

0:27:45.359 --> 0:27:49.280
<v Speaker 1>can only fuse up to iron, like before iron. Anything

0:27:49.359 --> 0:27:51.600
<v Speaker 1>lighter than iron. If you fuse it, you get a

0:27:51.640 --> 0:27:53.919
<v Speaker 1>byproduct and you get energy out, and that's how the

0:27:53.960 --> 0:27:57.479
<v Speaker 1>star glows. But iron, if you try to fuse iron together,

0:27:57.640 --> 0:28:01.200
<v Speaker 1>it actually costs you energy. So if you fuse iron together,

0:28:01.240 --> 0:28:03.760
<v Speaker 1>you'll cool down the star. You will kill the star

0:28:04.000 --> 0:28:06.439
<v Speaker 1>if you try to fuse iron together. But we have

0:28:06.560 --> 0:28:10.120
<v Speaker 1>stuff higher than iron, and so is stuff higher than

0:28:10.160 --> 0:28:13.040
<v Speaker 1>iron made in dying stars. So for a long time

0:28:13.040 --> 0:28:16.119
<v Speaker 1>people really didn't understand this. They're like, well, stars can't

0:28:16.160 --> 0:28:18.240
<v Speaker 1>make higher than iron. But as you say, obviously we

0:28:18.320 --> 0:28:21.520
<v Speaker 1>have like gold and platinum and plutonium and uranium. Where

0:28:21.520 --> 0:28:24.080
<v Speaker 1>do all these things come from? And so people thought

0:28:24.119 --> 0:28:25.840
<v Speaker 1>for a while, as you said, that maybe they come

0:28:25.880 --> 0:28:29.640
<v Speaker 1>from supernova, that maybe the special conditions when a star

0:28:29.800 --> 0:28:33.480
<v Speaker 1>explodes might be enough to trigger, you know, this kind

0:28:33.480 --> 0:28:37.280
<v Speaker 1>of heavier element fusion. But the story didn't really hang together,

0:28:37.359 --> 0:28:40.120
<v Speaker 1>like it's potentially possible for this to happen, but they

0:28:40.120 --> 0:28:43.280
<v Speaker 1>didn't really see evidence for it around supernova. And the

0:28:43.280 --> 0:28:46.600
<v Speaker 1>problem is that this process is very delicate. Like above iron,

0:28:46.600 --> 0:28:48.880
<v Speaker 1>in order to make something heavier, you need to absorb

0:28:48.960 --> 0:28:52.160
<v Speaker 1>like multiple neutrons at the same time. Like if you

0:28:52.200 --> 0:28:55.320
<v Speaker 1>absorb one neutron, you become very unstable and just break up.

0:28:55.480 --> 0:28:58.520
<v Speaker 1>If you absorb two neutrons, then boom, you can transmute

0:28:58.560 --> 0:29:00.960
<v Speaker 1>into this heavier thing. So you have to like absorb

0:29:01.080 --> 0:29:05.040
<v Speaker 1>to neutrons almost simultaneously. It's called this our process for

0:29:05.240 --> 0:29:07.520
<v Speaker 1>rapid process. And to do that you need like a

0:29:07.560 --> 0:29:09.760
<v Speaker 1>lot of neutrons around you so that you have like

0:29:09.920 --> 0:29:12.120
<v Speaker 1>enough that sometimes you'll get two of them coming in

0:29:12.160 --> 0:29:14.360
<v Speaker 1>at the same time. And that's very difficult to do

0:29:14.480 --> 0:29:17.800
<v Speaker 1>in the environment of a supernova because supernova is expanding,

0:29:17.800 --> 0:29:20.680
<v Speaker 1>it's exploding. And the other problem with supernovas is that

0:29:20.800 --> 0:29:22.920
<v Speaker 1>while they might make some of this stuff, they don't

0:29:22.960 --> 0:29:26.040
<v Speaker 1>really like ejected out there into the Solar system. We

0:29:26.040 --> 0:29:28.360
<v Speaker 1>don't just want to make uranium. We need to make

0:29:28.440 --> 0:29:30.440
<v Speaker 1>uranium and then have it be the seeds for a

0:29:30.480 --> 0:29:33.240
<v Speaker 1>future solar system. If it's just made inside a star

0:29:33.360 --> 0:29:35.680
<v Speaker 1>and then like kept inside the remnant of that star,

0:29:35.760 --> 0:29:37.960
<v Speaker 1>it's not going to end up here on Earth or

0:29:38.200 --> 0:29:41.120
<v Speaker 1>as part of our Solar system. So recently people found

0:29:41.200 --> 0:29:44.880
<v Speaker 1>another way to make these super duper heavy elements that

0:29:45.000 --> 0:29:47.880
<v Speaker 1>wasn't just supernova's suspense is killing me? What is it?

0:29:48.000 --> 0:29:50.080
<v Speaker 1>So the answer to how to get a bunch of

0:29:50.080 --> 0:29:53.240
<v Speaker 1>neutrons together, like a really high density of neutrons, so

0:29:53.320 --> 0:29:55.880
<v Speaker 1>you can do this kind of thing is neutron stars.

0:29:56.040 --> 0:29:59.040
<v Speaker 1>Neutron stars are these remnants of old dead stars, right,

0:29:59.040 --> 0:30:01.200
<v Speaker 1>they've already blown up up and collapse, and they have

0:30:01.240 --> 0:30:05.280
<v Speaker 1>this leftover core that's super incredibly dense. Now, when two

0:30:05.320 --> 0:30:07.920
<v Speaker 1>of these things collide, like two neutron stars in a

0:30:08.000 --> 0:30:11.320
<v Speaker 1>binary system for example, spiral into each other and collide,

0:30:11.560 --> 0:30:16.280
<v Speaker 1>then you get this incredible cataclysmic event of really unparalleled density,

0:30:16.680 --> 0:30:19.120
<v Speaker 1>not enough to become a black hole, but to form

0:30:19.200 --> 0:30:21.680
<v Speaker 1>maybe a larger neutron star or to blow some of

0:30:21.680 --> 0:30:25.800
<v Speaker 1>this stuff out. And so recently, because of gravitational wave observatories,

0:30:25.840 --> 0:30:28.680
<v Speaker 1>we've been able to see these neutron star collisions happen,

0:30:29.080 --> 0:30:31.120
<v Speaker 1>and they're really cool things that you can see the

0:30:31.160 --> 0:30:34.960
<v Speaker 1>gravitational waves that they make like actual shaking of space

0:30:35.040 --> 0:30:37.080
<v Speaker 1>because they're so dense, and you can also look at

0:30:37.120 --> 0:30:39.640
<v Speaker 1>them with telescopes and you can see the light that

0:30:39.760 --> 0:30:41.680
<v Speaker 1>comes from them, so like you can see it in

0:30:41.720 --> 0:30:46.040
<v Speaker 1>two totally different ways, the gravitational waves and in the optical.

0:30:46.200 --> 0:30:48.120
<v Speaker 1>And when they look in the optical they see light

0:30:48.200 --> 0:30:51.040
<v Speaker 1>coming from these and they can see light from like

0:30:51.200 --> 0:30:55.280
<v Speaker 1>excited gold or excited uranium is like gases of golden

0:30:55.360 --> 0:30:59.120
<v Speaker 1>uranium get thrown out into the universe and because they're hot,

0:30:59.160 --> 0:31:02.280
<v Speaker 1>they emit light and it has a particular fingerprint and

0:31:02.320 --> 0:31:04.680
<v Speaker 1>we can see it here on Earth. So we have

0:31:04.800 --> 0:31:07.880
<v Speaker 1>seen the birth of these super heavy elements in neutron

0:31:07.920 --> 0:31:10.800
<v Speaker 1>star collisions. So that's totally wild. So that seems like

0:31:11.280 --> 0:31:15.760
<v Speaker 1>two super rare conditions that need to come together, and

0:31:15.840 --> 0:31:19.320
<v Speaker 1>that has produced everything above iron. So many of those

0:31:19.320 --> 0:31:22.000
<v Speaker 1>things are things that we depend on. And so like,

0:31:22.160 --> 0:31:24.680
<v Speaker 1>did any of that happen in our solar system? How

0:31:24.720 --> 0:31:27.280
<v Speaker 1>did how did it get here? Absolutely none of that

0:31:27.320 --> 0:31:30.320
<v Speaker 1>could happen in our solar system. There's nowhere in our

0:31:30.320 --> 0:31:32.880
<v Speaker 1>solar system that is capable of making these things. Like

0:31:32.920 --> 0:31:35.480
<v Speaker 1>even at the heart of our star, all they can

0:31:35.520 --> 0:31:38.440
<v Speaker 1>do is burn helium or hydrogen. Right, our star is

0:31:38.480 --> 0:31:40.360
<v Speaker 1>not going to be big enough to even make iron.

0:31:40.520 --> 0:31:43.000
<v Speaker 1>And so that means that every heavy metal that you

0:31:43.040 --> 0:31:45.560
<v Speaker 1>see if you're wearing a gold wedding ring right now,

0:31:45.760 --> 0:31:49.000
<v Speaker 1>that gold was made probably in a neutron star collision

0:31:49.280 --> 0:31:53.120
<v Speaker 1>before our solar system was even formed. Right, So all

0:31:53.160 --> 0:31:55.680
<v Speaker 1>of the uranium, all the gold, all the heavy elements

0:31:55.680 --> 0:31:59.080
<v Speaker 1>in our solar system predate our solar system completely, and

0:31:59.120 --> 0:32:02.800
<v Speaker 1>our solar system comes from gathering together the remnants of

0:32:02.840 --> 0:32:06.560
<v Speaker 1>a previous solar system. Some stars died and became neutron

0:32:06.640 --> 0:32:09.400
<v Speaker 1>stars and then collided together and made these heavy elements

0:32:09.600 --> 0:32:13.160
<v Speaker 1>and spewed them out into some gas cloud which then

0:32:13.200 --> 0:32:17.480
<v Speaker 1>coalesced into our solar system, still mostly hydrogen, but with

0:32:17.560 --> 0:32:20.320
<v Speaker 1>a few nuggets of these heavier interesting things to like

0:32:20.360 --> 0:32:22.840
<v Speaker 1>spice it up a little bit. Science is so beautiful,

0:32:22.880 --> 0:32:24.760
<v Speaker 1>you know. You you walk around and now you know

0:32:24.840 --> 0:32:27.520
<v Speaker 1>the stuff and you see the whole world differently. Like anyway,

0:32:27.520 --> 0:32:29.440
<v Speaker 1>the next time I'm walking through a jewelry store, maybe

0:32:29.440 --> 0:32:33.240
<v Speaker 1>I'll appreciate it. It It is really incredible, especially these heavy

0:32:33.240 --> 0:32:36.280
<v Speaker 1>with things like gold and platinum and plutonium and uranium.

0:32:36.320 --> 0:32:38.920
<v Speaker 1>They're so difficult to make, and so that tells you

0:32:39.240 --> 0:32:42.440
<v Speaker 1>that something crazy must have happened really far away, a

0:32:42.480 --> 0:32:45.680
<v Speaker 1>really long time ago. And so yeah, these elements on

0:32:45.760 --> 0:32:49.560
<v Speaker 1>your fingers are much older than the Earth itself, right,

0:32:49.640 --> 0:32:51.920
<v Speaker 1>Like that gold has been hanging out before the Earth

0:32:52.040 --> 0:32:54.920
<v Speaker 1>was even formed, and it's it's super amazing. Yeah, so

0:32:54.960 --> 0:32:58.520
<v Speaker 1>this stuff got made and not in our solar system

0:32:58.600 --> 0:33:00.800
<v Speaker 1>but it ended up in our solar system, and so

0:33:01.480 --> 0:33:03.600
<v Speaker 1>because it was made before our solar system, is it

0:33:03.680 --> 0:33:07.960
<v Speaker 1>sort of evenly distributed between the stuff that we have

0:33:08.080 --> 0:33:09.880
<v Speaker 1>in our solar system or did it sort of get

0:33:09.920 --> 0:33:12.800
<v Speaker 1>clumpy and sucked into certain bodies and not others. That

0:33:12.960 --> 0:33:15.040
<v Speaker 1>is a great question, and that is really the heart

0:33:15.120 --> 0:33:17.200
<v Speaker 1>of the question. We haven't been able to study that

0:33:17.280 --> 0:33:20.240
<v Speaker 1>in great detail because the only example we really can

0:33:20.360 --> 0:33:23.000
<v Speaker 1>study is the Earth and then the few things that

0:33:23.120 --> 0:33:26.000
<v Speaker 1>fall to the Earth from space. You know, like you

0:33:26.040 --> 0:33:29.040
<v Speaker 1>could ask the question, do asteroids have the same composition

0:33:29.080 --> 0:33:32.240
<v Speaker 1>of stuff as the Earth? And do things further out

0:33:32.320 --> 0:33:35.600
<v Speaker 1>have the same composition of stuff? So the short answers

0:33:35.680 --> 0:33:38.280
<v Speaker 1>we don't know exactly. We know that there are variations

0:33:38.400 --> 0:33:40.600
<v Speaker 1>because of where you are in the Solar system, like

0:33:40.880 --> 0:33:42.880
<v Speaker 1>the further out you are there tend to be different

0:33:42.920 --> 0:33:46.960
<v Speaker 1>things than closer in. But one clue is that uranium

0:33:47.160 --> 0:33:51.400
<v Speaker 1>is very very abundant. It's very very widespread. It's like

0:33:51.440 --> 0:33:55.160
<v Speaker 1>actually the fifty one most common element on the Earth,

0:33:55.520 --> 0:33:56.960
<v Speaker 1>which you know, it doesn't sound it's not in the

0:33:56.960 --> 0:33:59.480
<v Speaker 1>top ten or anything, but for us, such a big

0:33:59.520 --> 0:34:02.240
<v Speaker 1>heavy element, and there's you know, more than a hundred elements.

0:34:02.560 --> 0:34:05.200
<v Speaker 1>It's pretty far up there. And is it about that

0:34:05.280 --> 0:34:08.719
<v Speaker 1>common in asteroids and comments and stuff as well, or

0:34:08.920 --> 0:34:11.640
<v Speaker 1>we really only know that ranking forth. We know that

0:34:11.760 --> 0:34:13.880
<v Speaker 1>ranking well for Earth and a lot of the asteroids

0:34:13.880 --> 0:34:16.279
<v Speaker 1>are different. But when we study asteroids, we also do

0:34:16.360 --> 0:34:19.120
<v Speaker 1>see these things in asteroids. And you know, something else

0:34:19.120 --> 0:34:22.759
<v Speaker 1>that's I think not widely understood is that uranium is everywhere.

0:34:22.880 --> 0:34:25.560
<v Speaker 1>It's basically in all of the sands, in every rock.

0:34:26.160 --> 0:34:28.600
<v Speaker 1>The biggest supply of uranium we have on Earth is

0:34:28.640 --> 0:34:32.239
<v Speaker 1>actually in the Earth's oceans. There's an incredible amount of

0:34:32.320 --> 0:34:35.319
<v Speaker 1>uranium just dissolved into the oceans. And these days people

0:34:35.360 --> 0:34:37.920
<v Speaker 1>are thinking about trying to get uranium out of the

0:34:37.920 --> 0:34:40.600
<v Speaker 1>water because it might be cheaper than digging it out

0:34:40.600 --> 0:34:45.360
<v Speaker 1>of the ground. So uranium is everywhere all over the planet,

0:34:45.440 --> 0:34:48.359
<v Speaker 1>but it must be in very low levels because none

0:34:48.400 --> 0:34:50.600
<v Speaker 1>of us are worried about getting cancer from swimming in

0:34:50.600 --> 0:34:54.000
<v Speaker 1>the ocean, Is that right? That's right. Uranium is sort

0:34:54.040 --> 0:34:57.239
<v Speaker 1>of just part of this radioactive background that exists from

0:34:57.239 --> 0:35:00.840
<v Speaker 1>living on Earth. You know, the Earth is slightly radio active. Also,

0:35:00.920 --> 0:35:04.480
<v Speaker 1>we get radiation from the sky, you know, from cosmic rays,

0:35:04.560 --> 0:35:07.440
<v Speaker 1>and so yeah, there is some effect on our DNA

0:35:07.719 --> 0:35:12.080
<v Speaker 1>from naturally present uranium in the soil, just like there's

0:35:12.480 --> 0:35:15.479
<v Speaker 1>effect on our DNA from muns coming from the sky

0:35:15.560 --> 0:35:19.120
<v Speaker 1>that occasionally like change something or you know, create an error.

0:35:19.120 --> 0:35:21.640
<v Speaker 1>And that's I think an important part of evolution. I

0:35:21.640 --> 0:35:24.399
<v Speaker 1>think evolution. It would have happened differently if we had

0:35:24.480 --> 0:35:27.120
<v Speaker 1>no radioactive elements on Earth. It would have lowered the

0:35:27.160 --> 0:35:30.200
<v Speaker 1>number of mutations that occur. Right, it's not something necessarily

0:35:30.239 --> 0:35:32.719
<v Speaker 1>to be worried about. So you shouldn't, you know, isolate

0:35:32.800 --> 0:35:34.880
<v Speaker 1>uranium and eat a lot of it or anything. But

0:35:35.160 --> 0:35:38.000
<v Speaker 1>it is definitely present all around us. Interesting, and how

0:35:38.040 --> 0:35:40.759
<v Speaker 1>how long have we known about uranium? So uranium was

0:35:40.840 --> 0:35:45.760
<v Speaker 1>also discovered or just after uranus, right, and so only

0:35:45.840 --> 0:35:48.520
<v Speaker 1>like more than a hundred years. And it was discovered

0:35:48.600 --> 0:35:51.080
<v Speaker 1>sort of accidentally by a chemist who was just playing

0:35:51.120 --> 0:35:54.560
<v Speaker 1>around with something called pitch blend and dissolving it with stuff,

0:35:54.600 --> 0:35:56.560
<v Speaker 1>and he came up with something that felt to him

0:35:56.600 --> 0:36:00.360
<v Speaker 1>like a new undiscovered element. And it was like hundred

0:36:00.440 --> 0:36:04.279
<v Speaker 1>years later the people realized that it was radioactive. So

0:36:04.320 --> 0:36:07.759
<v Speaker 1>they had been like studying it without knowing they should

0:36:07.800 --> 0:36:11.040
<v Speaker 1>be careful. I guess we didn't understand radio activity until

0:36:11.080 --> 0:36:14.680
<v Speaker 1>much later. Exactly this was the discovery of radioactivity. So

0:36:15.080 --> 0:36:18.000
<v Speaker 1>uranium is a really important role in science itself. It's

0:36:18.040 --> 0:36:21.319
<v Speaker 1>the late eighteen hundreds when Beckerel sort of left a

0:36:21.320 --> 0:36:24.560
<v Speaker 1>bunch of uranium on a photography plate in a drawer

0:36:24.760 --> 0:36:26.319
<v Speaker 1>and he came back to found that it had like

0:36:26.440 --> 0:36:29.279
<v Speaker 1>imprinted itself on the plate. It was like in a

0:36:29.360 --> 0:36:32.719
<v Speaker 1>darkened drawer, no light in there, but somehow these blobs

0:36:32.719 --> 0:36:36.200
<v Speaker 1>of uranium left an imprint of fog on this plate,

0:36:36.640 --> 0:36:38.640
<v Speaker 1>and so he realized, hold on a second, there's something

0:36:38.640 --> 0:36:41.320
<v Speaker 1>going on here. And that was the discovery of radiation

0:36:41.719 --> 0:36:45.120
<v Speaker 1>that some materials like shoot out these particles that can

0:36:45.239 --> 0:36:47.759
<v Speaker 1>fog a plate, and you know, that stimulated the curies

0:36:48.040 --> 0:36:50.680
<v Speaker 1>and they discovered radium, and that, you know, really triggered

0:36:51.320 --> 0:36:54.040
<v Speaker 1>much of nuclear physics and modern physics. So it was

0:36:54.080 --> 0:36:56.880
<v Speaker 1>a real turning point sort in science, this discovery of

0:36:57.040 --> 0:37:00.360
<v Speaker 1>uranium as a radioactive element. I love these exam couples

0:37:00.360 --> 0:37:02.600
<v Speaker 1>of dumb luck, you know, like whoops, I put my

0:37:02.719 --> 0:37:06.479
<v Speaker 1>uranium down on a photography plate. And now the whole

0:37:06.480 --> 0:37:10.960
<v Speaker 1>direction of sciences is shifting rapidly to understand what radioactivity means.

0:37:11.000 --> 0:37:13.560
<v Speaker 1>And it's pretty cool. Would you rather make a like

0:37:13.760 --> 0:37:17.239
<v Speaker 1>historic discovery through dumb luck so you have a nice anecdote,

0:37:17.480 --> 0:37:20.480
<v Speaker 1>or through like the sheer force of your brilliance. I mean,

0:37:20.640 --> 0:37:23.680
<v Speaker 1>I think I'd probably feel my ego would feel better

0:37:23.760 --> 0:37:26.000
<v Speaker 1>if I did it through the sheer force of my brilliance.

0:37:26.040 --> 0:37:29.120
<v Speaker 1>But I'll take it anyway it comes. So randomness is

0:37:29.120 --> 0:37:31.319
<v Speaker 1>good too. Yeah. I love these stories of people like

0:37:31.480 --> 0:37:35.000
<v Speaker 1>looking for one thing and then accidentally discovering something else

0:37:35.080 --> 0:37:37.280
<v Speaker 1>because it reminds me to keep in my mind open

0:37:37.360 --> 0:37:39.600
<v Speaker 1>and to keep my eyes wide because you never know

0:37:40.040 --> 0:37:42.080
<v Speaker 1>in what experiment is going to be the hints of

0:37:42.120 --> 0:37:45.319
<v Speaker 1>something like a crazy discovery. And usually once you've made

0:37:45.320 --> 0:37:48.040
<v Speaker 1>a discovery, people can go back through history and find

0:37:48.160 --> 0:37:51.040
<v Speaker 1>evidence for it beforehand, just like now we know ur

0:37:51.080 --> 0:37:53.239
<v Speaker 1>in this is a planet. We can see in data

0:37:53.280 --> 0:37:56.520
<v Speaker 1>collected hundreds of years earlier and people's log notebooks like, oh,

0:37:56.600 --> 0:37:58.759
<v Speaker 1>you could have discovered this, you have the data right here.

0:37:58.920 --> 0:38:02.719
<v Speaker 1>People have missed opportunities to make incredible discoveries because they

0:38:02.719 --> 0:38:05.239
<v Speaker 1>weren't looking for them or they didn't think about that,

0:38:05.560 --> 0:38:07.880
<v Speaker 1>And so it's a message there's like keep your mind

0:38:07.920 --> 0:38:10.560
<v Speaker 1>open because you never know you know what the universe

0:38:10.640 --> 0:38:12.879
<v Speaker 1>is telling you right now. You never know when you're

0:38:12.960 --> 0:38:17.399
<v Speaker 1>fumbling towards a discovery. And the uranium we have here

0:38:17.400 --> 0:38:19.600
<v Speaker 1>on Earth is a really interesting story because it comes

0:38:19.600 --> 0:38:22.919
<v Speaker 1>in two different flavors. It's two isotopes of uranium. Most

0:38:22.960 --> 0:38:24.800
<v Speaker 1>of the uranium we have here on Earth is two

0:38:24.880 --> 0:38:27.600
<v Speaker 1>thirty eight, which is pretty stable as a half life

0:38:27.600 --> 0:38:29.799
<v Speaker 1>of like four and a half billion years, but it's

0:38:29.840 --> 0:38:32.600
<v Speaker 1>not as useful for things like fission if you want

0:38:32.600 --> 0:38:35.600
<v Speaker 1>to make weapons or reactors. The other kind is called

0:38:35.719 --> 0:38:38.960
<v Speaker 1>uranium two thirty five, and it's much better for making

0:38:39.000 --> 0:38:41.960
<v Speaker 1>things like reactors, but it's pretty rare. So like most

0:38:42.000 --> 0:38:44.439
<v Speaker 1>of the stuff when you mind, it is uranium two

0:38:44.440 --> 0:38:47.440
<v Speaker 1>thirty eight. And then if you want to do reactors

0:38:47.520 --> 0:38:50.600
<v Speaker 1>or build weapons, you have to isolate and enhance the

0:38:50.680 --> 0:38:53.600
<v Speaker 1>fraction of uranium two thirty five. So that's why you

0:38:53.640 --> 0:38:57.160
<v Speaker 1>hear about like centrifuges because they separate the different isotopes

0:38:57.239 --> 0:38:59.080
<v Speaker 1>by weight so you can get more of the two

0:38:59.120 --> 0:39:01.760
<v Speaker 1>thirty five that you need. Yeah, this is such a

0:39:01.800 --> 0:39:04.719
<v Speaker 1>weird element for humanity. Like in the one hand, I'm

0:39:04.719 --> 0:39:08.279
<v Speaker 1>a huge fan of nuclear power plants because they put

0:39:08.280 --> 0:39:10.080
<v Speaker 1>out less carbon, and on the other hand, I just

0:39:10.120 --> 0:39:12.919
<v Speaker 1>don't know if humanity can handle it, because you can

0:39:12.960 --> 0:39:15.719
<v Speaker 1>also turn it into weapons, and it doesn't take too

0:39:15.719 --> 0:39:19.640
<v Speaker 1>many idiots to make trouble. And anyway, these things are complicated.

0:39:19.680 --> 0:39:22.920
<v Speaker 1>Thanks humanity, it is complicated. And it's also interesting that

0:39:23.080 --> 0:39:26.279
<v Speaker 1>the uranium two thirty five, the stuff that's useful for this,

0:39:26.400 --> 0:39:29.000
<v Speaker 1>is sort of going away because it's half life is

0:39:29.080 --> 0:39:32.320
<v Speaker 1>much shorter. It's only seven hundred million years, which sounds

0:39:32.320 --> 0:39:34.520
<v Speaker 1>like a long time, but what it means is that,

0:39:34.560 --> 0:39:37.560
<v Speaker 1>like the useful fraction of uranium over the history of

0:39:37.600 --> 0:39:40.279
<v Speaker 1>the Earth is dropping sort of steadily, like we have

0:39:40.320 --> 0:39:43.040
<v Speaker 1>a lot less of two thirty five than we did

0:39:43.080 --> 0:39:45.279
<v Speaker 1>a long time ago, and if you wait like another

0:39:45.320 --> 0:39:47.640
<v Speaker 1>few hundred million years, it's going to be even less.

0:39:47.760 --> 0:39:50.640
<v Speaker 1>We did a whole podcast episode once about a naturally

0:39:50.680 --> 0:39:54.680
<v Speaker 1>occurring fission reactor because like a billion or two years ago,

0:39:54.880 --> 0:39:58.120
<v Speaker 1>there was a uranium deposit in Africa that was rich

0:39:58.239 --> 0:39:59.840
<v Speaker 1>enough in you two thirty five that it was b

0:40:00.000 --> 0:40:04.280
<v Speaker 1>ethically a nuclear reactor naturally created that burned for hundreds

0:40:04.320 --> 0:40:06.200
<v Speaker 1>of thousands of years, and I'm like, heat it up

0:40:06.280 --> 0:40:09.880
<v Speaker 1>this rock underground, but that can't happen anymore, because uranium

0:40:10.560 --> 0:40:13.680
<v Speaker 1>doesn't occur in enough density anymore for that kind of

0:40:13.680 --> 0:40:15.640
<v Speaker 1>stuff to happen. So we have to like dig it

0:40:15.640 --> 0:40:18.840
<v Speaker 1>out of the ground and use centrifuges to enhance the

0:40:18.920 --> 0:40:21.440
<v Speaker 1>fraction of our uranium that has two thirty five. So

0:40:21.560 --> 0:40:24.840
<v Speaker 1>note humanity the clock is taking up figuring out fusion.

0:40:26.440 --> 0:40:28.680
<v Speaker 1>On that note, let's take a break and we'll come

0:40:28.719 --> 0:40:43.640
<v Speaker 1>back and hear a little bit more about uranium. Okay,

0:40:43.640 --> 0:40:46.800
<v Speaker 1>so we've talked a little bit about the way humanity

0:40:47.160 --> 0:40:51.319
<v Speaker 1>is helped are hurt by uranium two thirty five. Let's

0:40:51.400 --> 0:40:53.359
<v Speaker 1>hear a little bit more about some of the other

0:40:53.600 --> 0:40:58.440
<v Speaker 1>properties about uranium. So you told us that it has

0:40:58.480 --> 0:41:00.600
<v Speaker 1>a high atomic weight because it's high or than iron.

0:41:00.640 --> 0:41:03.440
<v Speaker 1>So you need these very particular situations so that you

0:41:03.480 --> 0:41:06.200
<v Speaker 1>can get it. If you had like a chunk of

0:41:06.560 --> 0:41:09.840
<v Speaker 1>uranium sitting on your table, you'd probably be scared. But

0:41:10.000 --> 0:41:12.359
<v Speaker 1>what would it look like? Yeah, that's a cool question. Well,

0:41:12.480 --> 0:41:16.319
<v Speaker 1>it's actually malleable. It's like not that hard. It's it's

0:41:16.400 --> 0:41:20.600
<v Speaker 1>denser than lead, but it's it's soft and it's silvery white,

0:41:20.640 --> 0:41:23.120
<v Speaker 1>so it's actually kind of pretty, you know, I mean,

0:41:23.160 --> 0:41:25.399
<v Speaker 1>I wouldn't recommend doing any art with it, but it's

0:41:25.440 --> 0:41:27.480
<v Speaker 1>kind of a cool looking thing. And it's cool that

0:41:27.760 --> 0:41:30.920
<v Speaker 1>every element has its own like sort of feel to it, right,

0:41:30.960 --> 0:41:33.719
<v Speaker 1>It's own like texture and color and look, and that

0:41:33.840 --> 0:41:36.640
<v Speaker 1>all of these properties, the difference between uranium and the

0:41:36.680 --> 0:41:39.680
<v Speaker 1>other things, just come out of the structure of the atom. Right,

0:41:39.680 --> 0:41:42.680
<v Speaker 1>We're talking about how the electrons fill their orbitals and

0:41:42.719 --> 0:41:46.400
<v Speaker 1>all of this stuff. It's incredibly rich and interesting that

0:41:46.480 --> 0:41:49.520
<v Speaker 1>all of these elements have such different properties. I love

0:41:49.560 --> 0:41:52.040
<v Speaker 1>that about the universe that like a few very simple

0:41:52.080 --> 0:41:54.960
<v Speaker 1>things coming together in lots of different ways can make

0:41:55.080 --> 0:41:59.080
<v Speaker 1>so many interesting different kinds of materials. That is totally epic.

0:41:59.200 --> 0:42:00.960
<v Speaker 1>And I think it's interest thing that you mentioned art

0:42:01.120 --> 0:42:04.400
<v Speaker 1>because when we moved to our permanent house, what what

0:42:04.440 --> 0:42:06.560
<v Speaker 1>we hope is our permanent house. I wanted to go

0:42:06.600 --> 0:42:10.799
<v Speaker 1>out and gets to wear dishwear because I think they

0:42:10.800 --> 0:42:13.440
<v Speaker 1>look really nice. And I was warned by someone that

0:42:13.560 --> 0:42:16.360
<v Speaker 1>I shouldn't get the red ones because the red ones

0:42:16.520 --> 0:42:19.560
<v Speaker 1>are radioactive because of uranium. Can you tell us more

0:42:19.600 --> 0:42:22.080
<v Speaker 1>about that uranium mix as well with lots of other

0:42:22.120 --> 0:42:25.319
<v Speaker 1>things and forms all sorts of interesting uranium oxides and

0:42:25.360 --> 0:42:28.200
<v Speaker 1>some of these have a really spectacular color. Um. You know,

0:42:28.360 --> 0:42:30.680
<v Speaker 1>some of them are yellow, some of them are very red.

0:42:31.160 --> 0:42:33.520
<v Speaker 1>And you know, if you're trying to create colors like

0:42:33.560 --> 0:42:35.560
<v Speaker 1>these days, it's easy to do digitally, right, you just

0:42:35.640 --> 0:42:37.799
<v Speaker 1>dial in whatever pixel you want. But if you're out

0:42:37.800 --> 0:42:39.959
<v Speaker 1>there working with your hands and you want to create dyes,

0:42:40.040 --> 0:42:42.759
<v Speaker 1>you need to find natural sources of color. And so

0:42:42.960 --> 0:42:46.719
<v Speaker 1>uranium made this really sort of bright, vivid red that

0:42:46.840 --> 0:42:49.520
<v Speaker 1>was hard to duplicate in other ways. And so before

0:42:49.560 --> 0:42:53.760
<v Speaker 1>we understood like really the dangers of radiation and radioactivity,

0:42:53.960 --> 0:42:56.680
<v Speaker 1>uranium was used all sorts of places to make these

0:42:56.719 --> 0:42:58.399
<v Speaker 1>kind of things, and in your dinner wear, so you're

0:42:58.400 --> 0:43:00.120
<v Speaker 1>like sitting at the dinner table and you're play it

0:43:00.200 --> 0:43:03.359
<v Speaker 1>is like shooting particles into your body. I guess that's

0:43:03.360 --> 0:43:07.280
<v Speaker 1>okay because there hasn't been a strong correlation between Fiesta

0:43:07.320 --> 0:43:09.919
<v Speaker 1>wear and cancer, I guess, or or was that bad?

0:43:10.120 --> 0:43:12.120
<v Speaker 1>I don't think it's okay. I don't think they're making

0:43:12.120 --> 0:43:14.000
<v Speaker 1>it anymore, you know, for the same reasons that like

0:43:14.040 --> 0:43:17.560
<v Speaker 1>they're no longer using glowing wrist watch faces. You know

0:43:17.600 --> 0:43:20.440
<v Speaker 1>that like glow with radiation. I think it's sort of

0:43:20.480 --> 0:43:23.320
<v Speaker 1>like lead in the sense that more radiation is definitely

0:43:23.320 --> 0:43:26.200
<v Speaker 1>more bad for you, and you want to limit your exposure.

0:43:26.520 --> 0:43:28.239
<v Speaker 1>You know, we used to like take X rays all

0:43:28.280 --> 0:43:30.920
<v Speaker 1>the time, and the X rays would like be super powerful,

0:43:31.040 --> 0:43:33.120
<v Speaker 1>much stronger than we needed in order to see clearly,

0:43:33.160 --> 0:43:35.759
<v Speaker 1>because we didn't understand the danger of X rays. So

0:43:35.800 --> 0:43:37.880
<v Speaker 1>now I think we work really hard to limit our

0:43:37.920 --> 0:43:40.480
<v Speaker 1>exposure to radiation. Yeah, but that sounds like a good plan.

0:43:40.520 --> 0:43:42.640
<v Speaker 1>And I didn't end up getting the Fiesta wear because

0:43:42.640 --> 0:43:44.240
<v Speaker 1>I didn't feel like I could get a good handle

0:43:44.280 --> 0:43:47.000
<v Speaker 1>on how dangerous it was. But uranium also tells us

0:43:47.040 --> 0:43:49.120
<v Speaker 1>a lot about the history of the Earth as well.

0:43:49.239 --> 0:43:51.960
<v Speaker 1>This is really fun story about a geologist trying to

0:43:52.040 --> 0:43:54.600
<v Speaker 1>understand the age of the Earth and trying to solve

0:43:54.600 --> 0:43:58.280
<v Speaker 1>the puzzle by actually looking for an asteroid that crashed

0:43:58.360 --> 0:44:01.560
<v Speaker 1>onto the Earth. He wants to know if rocks on

0:44:01.760 --> 0:44:03.920
<v Speaker 1>that he found in the Earth were actually the oldest

0:44:03.960 --> 0:44:06.359
<v Speaker 1>things that one could find. He was looking to see

0:44:06.360 --> 0:44:09.160
<v Speaker 1>if things in the Solar System might be even older

0:44:09.200 --> 0:44:11.279
<v Speaker 1>than the rocks we find on the Earth, because you know,

0:44:11.320 --> 0:44:12.640
<v Speaker 1>if you're trying to date the Earth and you're just

0:44:12.680 --> 0:44:15.279
<v Speaker 1>like looking around for rocks, you wonder, like, well, it's

0:44:15.320 --> 0:44:17.960
<v Speaker 1>his rock, as old as the Earth itself. So he

0:44:18.000 --> 0:44:21.680
<v Speaker 1>actually went out to Meteor Crater, this huge crater in

0:44:21.800 --> 0:44:25.160
<v Speaker 1>Arizona that you should totally visit if you're ever in Arizona.

0:44:25.200 --> 0:44:28.120
<v Speaker 1>It's incredible. It's just like a flat expanse and then

0:44:28.160 --> 0:44:31.720
<v Speaker 1>this incredible scoop, just like dug out of the Earth

0:44:32.239 --> 0:44:34.680
<v Speaker 1>by this meteor that hit a long long time ago.

0:44:34.760 --> 0:44:36.279
<v Speaker 1>He went down into the center of it and they

0:44:36.320 --> 0:44:39.200
<v Speaker 1>have like a chunk of the original meteor and they

0:44:39.280 --> 0:44:41.719
<v Speaker 1>let him sample it. And he looked at that rock

0:44:41.760 --> 0:44:45.120
<v Speaker 1>and he used uranium actually to date the age of

0:44:45.160 --> 0:44:48.320
<v Speaker 1>that asteroid. So did he get lucky because that asteroid

0:44:48.360 --> 0:44:51.799
<v Speaker 1>has uranium. Well, uranium is almost everywhere, right, It's in

0:44:51.840 --> 0:44:54.600
<v Speaker 1>almost every single rock in the Solar System, it turns out.

0:44:54.640 --> 0:44:57.640
<v Speaker 1>But a really interesting thing about uranium is that when

0:44:57.760 --> 0:45:01.080
<v Speaker 1>rocks form, they formed these little crystals called zircons, and

0:45:01.120 --> 0:45:04.759
<v Speaker 1>these crystals, for complicated reasons, they like to slurp in uranium,

0:45:05.000 --> 0:45:08.280
<v Speaker 1>but they reject lead. So like no lead ever forms

0:45:08.280 --> 0:45:11.480
<v Speaker 1>in the center of these zircon crystals. But uranium turns

0:45:11.560 --> 0:45:15.040
<v Speaker 1>into lead at a very regular rate because it decays radioactively.

0:45:15.120 --> 0:45:16.880
<v Speaker 1>So if you have there Basically it's like a clock.

0:45:17.000 --> 0:45:19.880
<v Speaker 1>You have these crystals that start out with uranium and

0:45:19.920 --> 0:45:22.839
<v Speaker 1>then they gradually get lead in them, and you know

0:45:22.920 --> 0:45:24.640
<v Speaker 1>that they had no lead when they were formed because

0:45:24.640 --> 0:45:26.759
<v Speaker 1>the crystals like reject the lead. So if you look

0:45:26.800 --> 0:45:29.080
<v Speaker 1>at one of these crystals, you can tell how long

0:45:29.120 --> 0:45:32.400
<v Speaker 1>it's been around just by counting the uranium and counting

0:45:32.440 --> 0:45:34.520
<v Speaker 1>the lead, and you can figure out like, oh, this

0:45:34.719 --> 0:45:37.440
<v Speaker 1>crystal has been ticking for seven hundred million years or

0:45:37.440 --> 0:45:40.439
<v Speaker 1>for four point two billion years. It's an incredible way

0:45:40.480 --> 0:45:43.400
<v Speaker 1>to date the age of a rock. That is incredible

0:45:43.440 --> 0:45:47.239
<v Speaker 1>and super useful. Thank you physics. Yeah, so this guy

0:45:47.360 --> 0:45:49.640
<v Speaker 1>dug out that crater and he discovered he's the first

0:45:49.640 --> 0:45:52.800
<v Speaker 1>person to really nailed down the age of the Solar

0:45:52.840 --> 0:45:56.200
<v Speaker 1>System to be about four and a half billion years old.

0:45:56.239 --> 0:45:59.880
<v Speaker 1>It's really important discovery, again connected to uranium, and it

0:46:00.160 --> 0:46:02.640
<v Speaker 1>interesting side note is that when he was doing that study,

0:46:02.680 --> 0:46:04.040
<v Speaker 1>he was trying to measure the amount of lead in

0:46:04.080 --> 0:46:07.200
<v Speaker 1>these crystals, and he discovered that his entire lab was

0:46:07.239 --> 0:46:10.120
<v Speaker 1>basically covered in lead. There was lead everywhere. There's lead

0:46:10.120 --> 0:46:11.680
<v Speaker 1>on the walls, it was lead in the air, there

0:46:11.760 --> 0:46:14.680
<v Speaker 1>was lead everywhere. Because of lead in gasoline, and he

0:46:14.760 --> 0:46:17.760
<v Speaker 1>actually led the charge to help remove lead from gasoline

0:46:17.800 --> 0:46:20.400
<v Speaker 1>because he's the one who discovered that we were poisoning

0:46:20.440 --> 0:46:23.680
<v Speaker 1>our environment with lead. Whoa, So, what's this guy's name

0:46:23.880 --> 0:46:27.479
<v Speaker 1>who dated the universe and led the charge against lead.

0:46:27.760 --> 0:46:30.200
<v Speaker 1>His name is Claire Patterson, and he's the one who

0:46:30.239 --> 0:46:33.800
<v Speaker 1>discovered that we're basically poisoning all of our children with lead.

0:46:34.120 --> 0:46:36.120
<v Speaker 1>And he came to this discovery because he wanted to

0:46:36.120 --> 0:46:37.759
<v Speaker 1>know the age of the universe and he was trying

0:46:37.800 --> 0:46:41.120
<v Speaker 1>to use uranium decaying into lead in order to do it.

0:46:41.360 --> 0:46:45.040
<v Speaker 1>That is incredible. So we've talked about how uranium is

0:46:45.160 --> 0:46:47.640
<v Speaker 1>helpful in a lot of different ways, and we're all

0:46:47.680 --> 0:46:51.879
<v Speaker 1>absolutely in awe of uranus. So now to finally put

0:46:51.920 --> 0:46:54.640
<v Speaker 1>it all together. So people have sat with us for

0:46:54.719 --> 0:46:57.560
<v Speaker 1>over fifty minutes and they are waiting for the answer.

0:46:58.400 --> 0:47:05.240
<v Speaker 1>Is there uranium on uranus? What is the answer? As usual,

0:47:05.320 --> 0:47:08.959
<v Speaker 1>the answer is we don't really know because we haven't

0:47:09.000 --> 0:47:11.879
<v Speaker 1>been out there to uranus, so we don't know, but

0:47:12.480 --> 0:47:15.960
<v Speaker 1>we can fairly confidently say that yes, there is, because

0:47:16.160 --> 0:47:18.960
<v Speaker 1>uranium seems to be present in almost every piece of

0:47:19.040 --> 0:47:21.880
<v Speaker 1>rock we find, like afterwards that fall to earth and

0:47:21.880 --> 0:47:24.919
<v Speaker 1>things that we study. They have these heavy elements in them,

0:47:24.920 --> 0:47:28.080
<v Speaker 1>and not just uranium, the other heavy elements in varying mixtures,

0:47:28.120 --> 0:47:30.279
<v Speaker 1>and you can tell something about where these things came

0:47:30.280 --> 0:47:32.399
<v Speaker 1>from based on like how much iron or how much

0:47:32.440 --> 0:47:36.680
<v Speaker 1>nickel and various isotopes they have. But uranium is almost everywhere,

0:47:36.920 --> 0:47:40.360
<v Speaker 1>and so I'm very confident that there is uranium somewhere

0:47:40.440 --> 0:47:44.080
<v Speaker 1>on Uranus in its rocky core, but we're not sure.

0:47:44.280 --> 0:47:47.120
<v Speaker 1>And you know, Uranus remains one of the planets that

0:47:47.239 --> 0:47:49.839
<v Speaker 1>is not very well studied. We only passed it by

0:47:49.880 --> 0:47:52.840
<v Speaker 1>with a probe once. We've never like dropped anything into

0:47:52.920 --> 0:47:55.600
<v Speaker 1>it or tried to dive a probe down into it,

0:47:55.880 --> 0:47:57.680
<v Speaker 1>which I think would be super fun, and you know,

0:47:57.760 --> 0:48:00.120
<v Speaker 1>maybe there's a big surprise down there. I think that

0:48:00.200 --> 0:48:02.960
<v Speaker 1>funders should take note, and they should also consider all

0:48:03.000 --> 0:48:05.160
<v Speaker 1>of the amazing puns and jokes that could be made

0:48:05.160 --> 0:48:08.600
<v Speaker 1>if we invested in studying this question more. And surely

0:48:08.640 --> 0:48:11.200
<v Speaker 1>the money is going to come rolling in dow Yeah, exactly.

0:48:11.320 --> 0:48:14.520
<v Speaker 1>And we have found uranium in other places in the

0:48:14.600 --> 0:48:17.719
<v Speaker 1>galaxy as well. For example, there's a star nearby called

0:48:17.840 --> 0:48:21.160
<v Speaker 1>Krel's Star, and it glows and you can tell what's

0:48:21.160 --> 0:48:24.000
<v Speaker 1>in a star based on how it glows, because every

0:48:24.040 --> 0:48:27.560
<v Speaker 1>element gets excited by different energy levels and gives off

0:48:27.640 --> 0:48:31.040
<v Speaker 1>light at unique frequencies as their own fingerprint. So based

0:48:31.080 --> 0:48:33.239
<v Speaker 1>on the spectrum of a star, you can tell what

0:48:33.320 --> 0:48:36.799
<v Speaker 1>it's burning. And they have found uranium glowing in this star.

0:48:36.920 --> 0:48:38.880
<v Speaker 1>Like we haven't gone out to actually visit it in

0:48:38.920 --> 0:48:40.960
<v Speaker 1>sample it, but we can tell from the light that's

0:48:41.000 --> 0:48:44.399
<v Speaker 1>coming from this star what's in it. And not just that,

0:48:44.440 --> 0:48:47.920
<v Speaker 1>but based on the ratio of these various elements uranium

0:48:47.920 --> 0:48:50.600
<v Speaker 1>and thorium and our knowledge about how they decay, we

0:48:50.640 --> 0:48:53.960
<v Speaker 1>can use that to age these stars. So uranium is

0:48:54.000 --> 0:48:56.160
<v Speaker 1>all over the universe and it's telling us lots of

0:48:56.160 --> 0:48:59.360
<v Speaker 1>fascinating stories about all of the objects that it's hiding inside.

0:48:59.520 --> 0:49:01.480
<v Speaker 1>And we still have so much left to learning. So

0:49:01.600 --> 0:49:04.040
<v Speaker 1>thanks very much for coming on this journey with us

0:49:04.080 --> 0:49:07.560
<v Speaker 1>to learn about uranium and uranus, and thanks to Kelly

0:49:07.640 --> 0:49:10.760
<v Speaker 1>for coming along and refraining from making that most obvious

0:49:10.760 --> 0:49:14.400
<v Speaker 1>of jokes the entire hour. Well you're welcome. I've become

0:49:14.520 --> 0:49:19.000
<v Speaker 1>very mature in my late thirties. Thank you for inviting me.

0:49:19.440 --> 0:49:21.760
<v Speaker 1>I had a lot of fun, even though I didn't

0:49:21.760 --> 0:49:23.840
<v Speaker 1>make all the jokes I wanted to make, and everybody

0:49:23.840 --> 0:49:26.640
<v Speaker 1>out there don't forget to embrace your curiosity and don't

0:49:26.680 --> 0:49:31.560
<v Speaker 1>lose that childlike wonder ed sense of puns about absurd jokes.

0:49:31.680 --> 0:49:34.719
<v Speaker 1>They go hand in hand. Thanks everyone, tune in next time.

0:49:42.600 --> 0:49:45.440
<v Speaker 1>Thanks for listening, and remember that Daniel and Jorge explained.

0:49:45.440 --> 0:49:48.279
<v Speaker 1>The Universe is a production of I Heart Radio. For

0:49:48.480 --> 0:49:51.399
<v Speaker 1>more podcast for my heart Radio, visit the I heart

0:49:51.480 --> 0:49:55.080
<v Speaker 1>Radio app, Apple Podcasts, or wherever you listen to your

0:49:55.120 --> 0:50:01.440
<v Speaker 1>favorite shows. No