WEBVTT - How does carbon dating work?

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<v Speaker 1>Hey Daniel, it's been a long time. Did you have

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<v Speaker 1>a nice holiday with your family? We did, thank you

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<v Speaker 1>very much. We did some of our favorite holiday traditions. Oh,

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<v Speaker 1>like like you cooked specific meals that you only cook

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<v Speaker 1>once a year or something like that. Well, you know,

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<v Speaker 1>one of our favorite holiday traditions is a little bit unusual.

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<v Speaker 1>It's trash Day, like when you roll your bins to

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<v Speaker 1>the street because I call that Tuesday. Does that count

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<v Speaker 1>as a holiday? CD? No? No, No. Trash Day is

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<v Speaker 1>a much bigger deal. It's when you take all the

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<v Speaker 1>stuff out of your closets, decide what you actually need,

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<v Speaker 1>and donate or throw away the rest of it. Oh,

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<v Speaker 1>I bet you find some real treasures. You know, every

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<v Speaker 1>year we try to go one layer deeper into the

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<v Speaker 1>archaeology of our closets. Do you think you'll ever reach

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<v Speaker 1>the back. I'm not even convinced a back exists anymore.

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<v Speaker 1>It might just be like an infinite stack of useless junk. Well,

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<v Speaker 1>maybe you'll get lucky and it will have compressed for

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<v Speaker 1>long enough that it will become diamonds or something, or

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<v Speaker 1>be a black hole in there that'll just eat you.

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<v Speaker 1>That's not lucky, that's less lucky. That's still interesting. Hi.

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<v Speaker 1>I'm Daniel. I'm a professor at UC Irvine and a

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<v Speaker 1>particle physicist, and I love throwing stuff away. I'm Kelly

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<v Speaker 1>Wayder Smith. I'm a parasitologist with Rice University, and I

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<v Speaker 1>love throwing stuff away. But my family doesn't know. Do

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<v Speaker 1>you guys have arguments about how many nostalgic elements to keep? Yes,

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<v Speaker 1>that might be the thing we argue about the most often. Actually,

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<v Speaker 1>And are you ever right where they really need something?

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<v Speaker 1>And you're like, Hi, you shouldn't have thrown away that

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<v Speaker 1>melon baller. I knew we would come in Andy very rarely.

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<v Speaker 1>And also, you know, with things like Amazon, it could

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<v Speaker 1>show up at your house in less than a day.

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<v Speaker 1>So even if I'm wrong, you can just get a

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<v Speaker 1>new melon baller. That's true. Amazon has undermined your argument.

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<v Speaker 1>That's right, That's right. You can always just use the spoon.

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<v Speaker 1>Am I right? Well? I feel like you might appreciate

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<v Speaker 1>the melonballer, but you'll appreciate the lack of the melonballer

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<v Speaker 1>even more. You know, nothing is better than negative space.

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<v Speaker 1>If you've succeeded in like cleaning out a closet or

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<v Speaker 1>cleaning out some corner of your room, and then you

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<v Speaker 1>can just appreciate the emptiness. I agree, I like not

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<v Speaker 1>trimping over things in the middle of the night because

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<v Speaker 1>I get up a lot the middle of the night.

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<v Speaker 1>I value that well. Welcome to the podcast Daniel and

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<v Speaker 1>Jorge Explain the Universe, in which we explore the meaning

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<v Speaker 1>of nothingness and the very fabric of space itself. We

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<v Speaker 1>take the whole universe apart from the junk in your closets,

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<v Speaker 1>to the junk between your toes, to the junk that

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<v Speaker 1>fills the whole cosmos. We want to understand it. We

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<v Speaker 1>want to take it apart. We want to understand what

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<v Speaker 1>it means when it's there and it's not there, and

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<v Speaker 1>how it all got to be the way that it is.

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<v Speaker 1>So what are we working on today? Then? Today we

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<v Speaker 1>are thinking about the universe as a sort of mystery.

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<v Speaker 1>I like to think of physicists as like detectives trying

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<v Speaker 1>to crack the murder mystery of the universe, Like what

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<v Speaker 1>happened here? We are showing up at the scene and

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<v Speaker 1>wondering how did it all get to be the way

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<v Speaker 1>that it is? And today you get to be the

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<v Speaker 1>forensic scientist that dates the dead body. That's always a

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<v Speaker 1>good character. That's right, because when you show but the scene,

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<v Speaker 1>you want to understand what happened. You want to put

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<v Speaker 1>things in order. You want to say, what this happened,

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<v Speaker 1>then that happened, then the other happened, like the Solar

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<v Speaker 1>system formed and then the Earth cooled and then life

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<v Speaker 1>evolved on the planet, or the Big Bang happened, and

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<v Speaker 1>then helium formed, and then much much later stars happened.

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<v Speaker 1>The whole point of doing science is to put the

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<v Speaker 1>universe in some sort of order. That's what a story is.

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<v Speaker 1>And I'm a firm believer in the philosophy that human

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<v Speaker 1>thinking is mostly about storytelling. And so in order to

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<v Speaker 1>do that, you have to figure out why, how old

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<v Speaker 1>is stuff, what came before what other stuff? You need

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<v Speaker 1>to have dates and clocks and times if you're going

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<v Speaker 1>to unravel the murder mystery of the universe. And there's

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<v Speaker 1>a lot of different ways that we've done that throughout

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<v Speaker 1>the years, and some of them work better for particular

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<v Speaker 1>kinds of mysteries than others. So what sort of mysteries

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<v Speaker 1>are we solving today? Well, of course we are interested

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<v Speaker 1>in the mysteries of deep time. What happened in the

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<v Speaker 1>first few moments of the universe. How long has the

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<v Speaker 1>Earth been around? And what's been going on? How did

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<v Speaker 1>everything come together? One of my favorite things about dating

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<v Speaker 1>stuff is discovering those surprises, those realizations like wow, oh

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<v Speaker 1>my gosh, the Earth is so much older than anybody

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<v Speaker 1>ever imagined, or that the universe is shockingly old, or

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<v Speaker 1>you know, for some people the universe might be shockingly young.

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<v Speaker 1>Maybe some people bought the universe had been around forever

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<v Speaker 1>or trillions of years. So anytime you get one of

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<v Speaker 1>these dates, it's this glorious moment where you get to

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<v Speaker 1>like pin down the universe and say, ah, now I

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<v Speaker 1>know something about you, and that like eliminates a bunch

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<v Speaker 1>of possibilities. When you're a reader digesting a mystery novel,

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<v Speaker 1>you have like lots of different options in your head.

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<v Speaker 1>Maybe it was this person, maybe it was that person,

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<v Speaker 1>maybe it was this third person. And as you get clues,

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<v Speaker 1>you get to eliminate possibilities, which finally reveals to you

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<v Speaker 1>the truth, right, what actually happened in the universe. The

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<v Speaker 1>story is revealed by elimination, and so those clues are

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<v Speaker 1>absolutely essential. But you're right, Kelly, that there's lots of

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<v Speaker 1>different ways to date things in the universe, and today

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<v Speaker 1>we're gonna be focusing on something a little bit more recent,

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<v Speaker 1>how we can use physics to understand fairly recent history

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<v Speaker 1>here on Earth. Oh, that sounds a lot less disgusting

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<v Speaker 1>than using flymaggots. Fly maggots, what are you talking about?

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<v Speaker 1>That's for dating things like you know, dead bodies that

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<v Speaker 1>you find like what stage are the fly eggs that

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<v Speaker 1>have been laid on the body? So that's you know,

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<v Speaker 1>we're working with like days to weeks there. So are

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<v Speaker 1>we working on that skill or are we working like

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<v Speaker 1>past the writing DiPT in phase. Definitely past the rotting

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<v Speaker 1>corpse phase. But I think you put your finger on

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<v Speaker 1>a really interesting point, which is that there are all

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<v Speaker 1>these clocks build into nature, right like maggots take a

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<v Speaker 1>certain amount of time to digest a corpse, or rocks

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<v Speaker 1>take a certain amount of time to cool, and these

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<v Speaker 1>clocks are things we can take advantage of in order

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<v Speaker 1>to figure out how old things are, how long they've

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<v Speaker 1>been digesting, or how long they've been cooling, or how

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<v Speaker 1>long they've been radioactively decaying. We don't get to like

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<v Speaker 1>design these things go back in the past and like

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<v Speaker 1>leave clocks in place to tell us how long things took. Instead,

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<v Speaker 1>we have to just take advantage of the clocks that

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<v Speaker 1>we find. And some of these clocks, as you say,

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<v Speaker 1>are really short lived, like they tell us about things

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<v Speaker 1>that happened just for over weeks. Some of them can

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<v Speaker 1>tell us about things that happened for billions of years,

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<v Speaker 1>and other ones can tell us about things that happened

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<v Speaker 1>in the last ten fifty thousand years, which is a

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<v Speaker 1>super interesting time for the story of human civilization, how

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<v Speaker 1>we got to be who we are. And of course,

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<v Speaker 1>it turns out physics plays a big role. I love

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<v Speaker 1>learning about this topic because it's so exciting to me

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<v Speaker 1>how we figure out what tools are the best ones

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<v Speaker 1>to use to explore the past. And I specifically like

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<v Speaker 1>hearing about sort of physics and chemistry sorts of tools

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<v Speaker 1>because my sense is that they're a little bit less

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<v Speaker 1>susceptible to uncertainty. So, for example, you know, temperature can

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<v Speaker 1>impact how fast those flies are developing. But maybe today

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<v Speaker 1>you're going to explain to me that chemistry and physics

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<v Speaker 1>aren't that straightforward either. It turns out to be a

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<v Speaker 1>twisty and complicated topic. And of course sewage is involved. Yea,

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<v Speaker 1>my wife is very happy to hear about that. And

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<v Speaker 1>so today on the podcast, we'll be answering the question

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<v Speaker 1>how does radiocarbon dating work? Well, should we start by

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<v Speaker 1>seeing what the listeners think? Yes, absolutely, I was curious

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<v Speaker 1>to hear what people had to say about this. Radiocarbon

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<v Speaker 1>dating is something I think a lot of people have

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<v Speaker 1>heard about. It's on television all the time, and we

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<v Speaker 1>date this and we date that. But I was wondering

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<v Speaker 1>if people like really understood the mechanism of it, like

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<v Speaker 1>what the physics is of these clocks? Why is there

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<v Speaker 1>a clock? Why does it start when you die? And

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<v Speaker 1>how do we read it out? So thanks very much

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<v Speaker 1>to everyone who participates in this segment of the podcast,

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<v Speaker 1>sharing your thoughts without a chance to prepare. If you

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<v Speaker 1>would like to participate in the future, please don't be shy.

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<v Speaker 1>I'll be gentle. It's fun. Just write to me two

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<v Speaker 1>questions at Daniel Njorge dot com. So before you hear

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<v Speaker 1>these answers, think to yourself, do you know how radiocarbon

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<v Speaker 1>dating works? Here's what people had to say. If we

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<v Speaker 1>find some animal spoon, let's say some dinosaur spone, but

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<v Speaker 1>it inside the Earth, and then we calculate the amount

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<v Speaker 1>of carbon cfteen specifically present in it. Through those calculations,

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<v Speaker 1>we can easily calculate the age of that skeleton. I've

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<v Speaker 1>heard it get called carbon fourteen dating before, so that

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<v Speaker 1>makes me think that it has something to do with

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<v Speaker 1>the isotope and the decay of that carbon. Adam, you

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<v Speaker 1>can do tet the age of organic objects by looking

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<v Speaker 1>at the ratio of carbon isotopes. I feel like carbon

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<v Speaker 1>dating is when like two particles of carbon or like connected.

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<v Speaker 1>I don't know, I don't really know anything about that.

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<v Speaker 1>I felt like the answers to these fell into two camps.

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<v Speaker 1>People who sounded like they really knew what they were

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<v Speaker 1>talking about and people who had maybe not even heard

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<v Speaker 1>of carbon dating. And to me, that's it's sort of

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<v Speaker 1>interesting that it's like an either or scenario, like maybe

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<v Speaker 1>either you're into the kinds of TV shows that this

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<v Speaker 1>is shown in, or maybe you're not watching and cis

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<v Speaker 1>or what was that ship bones where the archaeologist was

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<v Speaker 1>doing carbon fourteen dating? Yeah, what do you think? I

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<v Speaker 1>was pretty tickled by the answer that suggested that, like

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<v Speaker 1>carbon fourteen atoms are like hooking up. You know, they're

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<v Speaker 1>like on Tinder, He's still finding each other and making magic.

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<v Speaker 1>It was a clever the cuff response there. Yeah, I

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<v Speaker 1>like our listeners are funny, funny people, absolutely, and I

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<v Speaker 1>had a lot of fun digging into the details of this.

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<v Speaker 1>This is not something I use in my research and

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<v Speaker 1>so not something i'd really ever wrapped my mind around.

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<v Speaker 1>And one of my favorite things about this podcast is

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<v Speaker 1>that I get an excuse to go off and learn

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<v Speaker 1>about something I always wanted to understand but never really

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<v Speaker 1>given myself the time to dig into. So thanks for

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<v Speaker 1>the listener who suggested this topic. How can listeners suggest

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<v Speaker 1>topics to you? Just shoot you an email. Absolutely, if

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<v Speaker 1>there's something you'd like to understand, please just write to

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<v Speaker 1>me to questions at Daniel and jorhe dot com. We

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<v Speaker 1>put it on our list and we get to every

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<v Speaker 1>single one eventually. And I'm with you. There are a

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<v Speaker 1>few things I enjoy more than an excuse to study

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<v Speaker 1>a topic that's interesting that isn't part of my research program.

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<v Speaker 1>I know, And it's weird that sometimes you feel like

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<v Speaker 1>you need an excuse, you know, you don't just like

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<v Speaker 1>get to slice off a few hours of your day

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<v Speaker 1>and go read about how something works. For some reason,

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<v Speaker 1>I feel like I have to give myself the opportunity

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<v Speaker 1>and having to do a podcast on it, explained of

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<v Speaker 1>the books is a good excuse to go and actually

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<v Speaker 1>learn how something works. That is one of the weird

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<v Speaker 1>things about academia. You don't feel like you have a

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<v Speaker 1>lot of time to just sit and think. But I too,

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<v Speaker 1>have created a bunch of tricks in my life, you know, like, oh,

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<v Speaker 1>I'm going to write a book about ten emerging technology,

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<v Speaker 1>so I have to read about all of them and

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<v Speaker 1>so yeah, but at least we have these tricks, all right.

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<v Speaker 1>So what is carbon fourteen? Right? So, radiocarbon dating or

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<v Speaker 1>carbon fourteen dating uses this weird form of carbon called

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<v Speaker 1>carbon fourteen. And when we say carbon fourteen, that number

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<v Speaker 1>fourteen tells us how many nucleons there are in the atom.

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<v Speaker 1>So remember that an atom has electrons around it, and

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<v Speaker 1>in the nucleus there are protons and neutrons. Now, usually

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<v Speaker 1>carbon has six protons and six neutrons, and so that's

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<v Speaker 1>carbon twelve. That's like the vanilla kind of carbon, the

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<v Speaker 1>kind that makes up most of you. And if it's

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<v Speaker 1>in carbon dioxide, and everywhere in the atmosphere. So that's

0:11:56.000 --> 0:11:59.880
<v Speaker 1>carbon twelve, which is stable. Carbon fourteen is a weird

0:12:00.240 --> 0:12:03.000
<v Speaker 1>version of carbon. It's still carbon, So there are six

0:12:03.080 --> 0:12:06.840
<v Speaker 1>protons inside, but there's two extra neutrons, so it's like

0:12:06.880 --> 0:12:10.240
<v Speaker 1>a heavier nucleus. So that's what carbon fourteen is. And

0:12:10.320 --> 0:12:13.200
<v Speaker 1>do those neutrons want to stay there or do they

0:12:13.200 --> 0:12:15.680
<v Speaker 1>want to escape? So you know, the stability of the

0:12:15.800 --> 0:12:19.920
<v Speaker 1>nucleus is a really interesting and complicated question. Some collections

0:12:19.920 --> 0:12:23.680
<v Speaker 1>of protons and neutrons are stable. You can build carbon

0:12:23.760 --> 0:12:26.200
<v Speaker 1>twelve and have it sit in space and come back

0:12:26.240 --> 0:12:29.320
<v Speaker 1>a billion years later and it'll still be carbon twelve.

0:12:29.400 --> 0:12:32.520
<v Speaker 1>Other constructions are not stable, Like you had two more

0:12:32.600 --> 0:12:34.760
<v Speaker 1>neutrons and all of a sudden you have carbon fourteen.

0:12:34.880 --> 0:12:37.600
<v Speaker 1>It's not stable. It will fall apart after a few

0:12:37.679 --> 0:12:40.320
<v Speaker 1>thousand years. And this all comes down to how those

0:12:40.320 --> 0:12:43.880
<v Speaker 1>protons and neutrons like to put themselves together inside the nucleus.

0:12:43.960 --> 0:12:46.640
<v Speaker 1>Remember that the nucleus is only protons and neutrons, and

0:12:46.720 --> 0:12:50.520
<v Speaker 1>the protons are positively charged. The neutrons are neutral, of course,

0:12:50.600 --> 0:12:52.559
<v Speaker 1>and so initially you might wonder, like, well, how does

0:12:52.559 --> 0:12:56.000
<v Speaker 1>the nucleus stay together anyway? It's all positive charges. Why

0:12:56.000 --> 0:12:58.440
<v Speaker 1>don't they just blow each other apart? And there is

0:12:58.559 --> 0:13:01.320
<v Speaker 1>that desire, right, They definitely are pushing against each other,

0:13:01.760 --> 0:13:03.920
<v Speaker 1>But on the other hand, they're held together by a

0:13:04.040 --> 0:13:07.640
<v Speaker 1>much stronger force. The strong nuclear force sticks the protons

0:13:07.640 --> 0:13:10.720
<v Speaker 1>and the neutrons all together. So it's a delicate balance

0:13:10.760 --> 0:13:13.760
<v Speaker 1>in some cases between the strong force sticking it together

0:13:13.920 --> 0:13:16.840
<v Speaker 1>and the electromagnetic force trying to push it apart. You

0:13:16.840 --> 0:13:19.240
<v Speaker 1>have one prototon and one neutron held together by the

0:13:19.240 --> 0:13:22.240
<v Speaker 1>strong nuclear force. That's stable. And then when you've got

0:13:22.280 --> 0:13:25.120
<v Speaker 1>extra neutrons floating around so that they don't pair evenly,

0:13:25.600 --> 0:13:27.760
<v Speaker 1>is that what makes it unstable? Yeah, that's right. You

0:13:27.760 --> 0:13:30.760
<v Speaker 1>can actually think about the construction of the nucleus in

0:13:30.800 --> 0:13:34.080
<v Speaker 1>a similar way to how we think about electron orbitals.

0:13:34.440 --> 0:13:37.400
<v Speaker 1>You remember learning in like high school chemistry. The electrons

0:13:37.440 --> 0:13:40.199
<v Speaker 1>aren't all just buzzing around the nucleus the same way.

0:13:40.400 --> 0:13:42.920
<v Speaker 1>It's like one in the lowest energy level and another

0:13:42.920 --> 0:13:44.840
<v Speaker 1>one in the next energy level. They sort of fill

0:13:44.960 --> 0:13:46.760
<v Speaker 1>up and they get to like more and more elaborate

0:13:46.840 --> 0:13:49.199
<v Speaker 1>orbitals as they get to higher and higher energy. Well,

0:13:49.200 --> 0:13:51.800
<v Speaker 1>the nucleus is constructed sort of in the same way.

0:13:52.000 --> 0:13:54.520
<v Speaker 1>The picture you often have of the nucleus is just

0:13:54.600 --> 0:13:57.560
<v Speaker 1>like a scoopful of protons and neutrons, But that's not

0:13:57.600 --> 0:14:01.160
<v Speaker 1>really very accurate. It's more like there are shells, you're

0:14:01.200 --> 0:14:04.200
<v Speaker 1>like an inner core or protons and neutrons have clicked together,

0:14:04.320 --> 0:14:06.840
<v Speaker 1>and then you can surround that with another layer of

0:14:06.880 --> 0:14:10.040
<v Speaker 1>like protons and neutrons, and the most stable atoms are

0:14:10.040 --> 0:14:13.640
<v Speaker 1>the ones where those layers are filled. You've like clicked

0:14:13.679 --> 0:14:15.679
<v Speaker 1>in all the protons and neutrons. It's sort of like

0:14:15.800 --> 0:14:18.480
<v Speaker 1>making a roman arch. When you have all the bricks together,

0:14:18.679 --> 0:14:21.520
<v Speaker 1>they click together to make a very stable structure. If

0:14:21.520 --> 0:14:24.520
<v Speaker 1>you're just missing one, then it can be very unstable.

0:14:24.800 --> 0:14:29.240
<v Speaker 1>So I didn't do great in high school chemistry? Is

0:14:29.280 --> 0:14:32.000
<v Speaker 1>the reason that that sounds new to me? Because we've

0:14:32.080 --> 0:14:34.960
<v Speaker 1>learned this in the twenty plus years since I've been

0:14:35.000 --> 0:14:36.760
<v Speaker 1>in high school? Or is that something we usually just

0:14:36.760 --> 0:14:39.120
<v Speaker 1>sort of, you know, skip over in high school, or

0:14:39.240 --> 0:14:41.840
<v Speaker 1>what's the story there? How long have we known that? Well?

0:14:41.840 --> 0:14:43.520
<v Speaker 1>I think we're gonna have to interview your high school

0:14:43.560 --> 0:14:45.920
<v Speaker 1>chemistry teacher to really find the answer to that. Let's

0:14:46.200 --> 0:14:48.880
<v Speaker 1>dig deep into your past. In fact, we have them

0:14:48.920 --> 0:14:53.000
<v Speaker 1>here on the podcast Surprise Surprise is Your Life, Kelly,

0:14:53.080 --> 0:14:54.880
<v Speaker 1>I don't think they like to be very much. Let's

0:14:54.880 --> 0:14:58.280
<v Speaker 1>move on. No, my high school chemistry teacher would not

0:14:58.280 --> 0:15:01.920
<v Speaker 1>be happy to hear from me either. I think it's

0:15:01.960 --> 0:15:04.960
<v Speaker 1>a combination of both things. We have understood what's going

0:15:04.960 --> 0:15:07.600
<v Speaker 1>on in the nucleus much much better in the last

0:15:07.640 --> 0:15:10.080
<v Speaker 1>few decades because we've been shooting stuff at it and

0:15:10.160 --> 0:15:12.080
<v Speaker 1>breaking it up and seeing what's inside of it, and

0:15:12.320 --> 0:15:15.120
<v Speaker 1>it's a hard project. We've also been building heavier and

0:15:15.160 --> 0:15:18.560
<v Speaker 1>heavier nuclei to understand, like what are the limits of stability?

0:15:18.800 --> 0:15:21.760
<v Speaker 1>How many protons and neutrons can you stick together and

0:15:21.880 --> 0:15:24.800
<v Speaker 1>have something which will stick around for billions of years.

0:15:24.880 --> 0:15:26.800
<v Speaker 1>We have a whole podcast episode about what are the

0:15:26.880 --> 0:15:29.640
<v Speaker 1>heaviest stable atoms And we think, for example, there might

0:15:29.680 --> 0:15:32.240
<v Speaker 1>be an island of stability where you get like hundreds

0:15:32.280 --> 0:15:35.160
<v Speaker 1>of protons and neutrons stuck together to make new super

0:15:35.240 --> 0:15:38.520
<v Speaker 1>heavy stable elements nobody's ever seen before. So it's a

0:15:38.560 --> 0:15:40.760
<v Speaker 1>complex field of study and it's probably not taught in

0:15:40.840 --> 0:15:44.480
<v Speaker 1>high school chemistry because it's evolving, and also because it's messy,

0:15:44.800 --> 0:15:47.480
<v Speaker 1>and I don't think that high school sophomores aren't necessarily

0:15:47.520 --> 0:15:49.400
<v Speaker 1>ready for it. I'm not sure that I was ready

0:15:49.400 --> 0:15:52.480
<v Speaker 1>for the electron stuff either, But all right, so these

0:15:52.480 --> 0:15:54.840
<v Speaker 1>things aren't stable, and every once in a while the

0:15:54.960 --> 0:15:58.600
<v Speaker 1>neutrons get picked out. How long are we talking before

0:15:58.640 --> 0:16:02.840
<v Speaker 1>the neutrons get picked doubt? Does it take like weeks? Years, millennia?

0:16:03.080 --> 0:16:06.040
<v Speaker 1>What are we looking at? So every atom is different. Uranium,

0:16:06.080 --> 0:16:08.480
<v Speaker 1>for example, has a half life which is like the

0:16:08.560 --> 0:16:12.320
<v Speaker 1>age of the Earth, but carbon fourteen only lasts about

0:16:12.400 --> 0:16:15.000
<v Speaker 1>fifty seven hundred years. Now, remember when we say that,

0:16:15.040 --> 0:16:17.360
<v Speaker 1>we don't mean that there's like a little clock inside

0:16:17.400 --> 0:16:20.560
<v Speaker 1>every carbon and when the time expires, it dies. What

0:16:20.600 --> 0:16:22.480
<v Speaker 1>we mean is that that's how long it takes, like

0:16:22.720 --> 0:16:26.680
<v Speaker 1>a population of carbon atoms for half of them to decay.

0:16:27.080 --> 0:16:31.120
<v Speaker 1>Each individual one might take longer or less time, because

0:16:31.160 --> 0:16:35.200
<v Speaker 1>fundamentally it's a quantum mechanical effect. There's a randomness to

0:16:35.240 --> 0:16:38.560
<v Speaker 1>win these things decay. So like five seven hundred years,

0:16:38.640 --> 0:16:41.120
<v Speaker 1>that's much longer than any of us live. And so

0:16:41.480 --> 0:16:44.360
<v Speaker 1>certainly there was no scientists who was sitting around, you know,

0:16:44.400 --> 0:16:46.800
<v Speaker 1>watching these things for five thousand, seven hundred years. How

0:16:46.800 --> 0:16:49.160
<v Speaker 1>do we figure something like that out? That's a great question,

0:16:49.240 --> 0:16:51.760
<v Speaker 1>And you know if it did take fifty seven hundred

0:16:51.800 --> 0:16:54.840
<v Speaker 1>years for every carbon atom to decay, then you couldn't

0:16:54.880 --> 0:16:57.760
<v Speaker 1>measure that half life without waiting for the first one

0:16:57.800 --> 0:17:00.560
<v Speaker 1>to decay, would literally take thousands of year years After

0:17:00.600 --> 0:17:03.040
<v Speaker 1>one thousand years or three thousand years, you would have

0:17:03.080 --> 0:17:05.879
<v Speaker 1>seen none decay, and you still wouldn't know is the

0:17:05.920 --> 0:17:09.000
<v Speaker 1>half life five thousand years or five billion years right?

0:17:09.119 --> 0:17:12.600
<v Speaker 1>And you wouldn't get ten year. You need a very

0:17:12.680 --> 0:17:16.640
<v Speaker 1>understanding department chare that's right. And so it's the statistical

0:17:16.720 --> 0:17:19.440
<v Speaker 1>nature of that, the randomness that really helps you because

0:17:19.840 --> 0:17:22.840
<v Speaker 1>even though the half life is five thousand, seven hundred years,

0:17:22.880 --> 0:17:25.240
<v Speaker 1>after one hundred years, there is a chance that a

0:17:25.280 --> 0:17:27.640
<v Speaker 1>few of them will have decayed. So all you need

0:17:27.760 --> 0:17:31.320
<v Speaker 1>is like a lot of carbon atoms, millions and billions

0:17:31.320 --> 0:17:33.679
<v Speaker 1>and zillions. Unfortunately, there are a lot of them around,

0:17:33.880 --> 0:17:36.520
<v Speaker 1>and you just watch for a few years or even

0:17:36.560 --> 0:17:38.760
<v Speaker 1>a few months, and a few of them will decay,

0:17:38.800 --> 0:17:41.679
<v Speaker 1>and from that you can extrapolate. Right as soon as

0:17:41.680 --> 0:17:43.440
<v Speaker 1>you start to see some of them decay, you know

0:17:43.680 --> 0:17:45.959
<v Speaker 1>how likely it is for any of them to decay,

0:17:46.119 --> 0:17:48.440
<v Speaker 1>and from that you can calculate how long it would

0:17:48.480 --> 0:17:50.960
<v Speaker 1>take for half of them to decay as a decay

0:17:51.000 --> 0:17:53.600
<v Speaker 1>is does it go from carbon fourteen the carbon thirteen,

0:17:53.640 --> 0:17:57.000
<v Speaker 1>the carbon twelves, or does it go right from fourteen

0:17:57.040 --> 0:17:59.760
<v Speaker 1>to twelve? Does it lose two neutrons all in one step?

0:18:00.040 --> 0:18:04.000
<v Speaker 1>So actually, carbon fourteen doesn't decay to carbon twelve. What

0:18:04.080 --> 0:18:07.679
<v Speaker 1>it does when it decays is that it goes to nitrogen.

0:18:07.880 --> 0:18:13.080
<v Speaker 1>Like normal nitrogen is nitrogen fourteen, but it has seven protons.

0:18:13.480 --> 0:18:16.199
<v Speaker 1>So you go from something which has eight neutrons and

0:18:16.480 --> 0:18:20.240
<v Speaker 1>six protons that's carbon fourteen, into something that has seven

0:18:20.320 --> 0:18:23.080
<v Speaker 1>neutrons and seven protons. So you take one of the

0:18:23.119 --> 0:18:26.600
<v Speaker 1>neutrons and you do a beta decay into a proton,

0:18:26.680 --> 0:18:30.879
<v Speaker 1>and now carbon fourteen has flipped into nitrogen fourteen. And

0:18:30.920 --> 0:18:32.840
<v Speaker 1>to me, this is really cool because this is the

0:18:32.920 --> 0:18:36.080
<v Speaker 1>quantum mechanics of it. Like carbon fourteen is not totally stable,

0:18:36.119 --> 0:18:38.640
<v Speaker 1>but it's also not totally unstable, like it will stick

0:18:38.680 --> 0:18:41.240
<v Speaker 1>around for a long long time. It's like a particle

0:18:41.400 --> 0:18:45.159
<v Speaker 1>trapped in a little potential well, and nitrogen fourteen is

0:18:45.200 --> 0:18:48.440
<v Speaker 1>other state it can flip into is also a little

0:18:48.440 --> 0:18:51.680
<v Speaker 1>potential well. And like classically, if you had a particle

0:18:52.000 --> 0:18:54.399
<v Speaker 1>trapped in a little well, it could never get out.

0:18:54.840 --> 0:18:57.600
<v Speaker 1>So what happens is that this atom switches from one

0:18:57.680 --> 0:19:00.760
<v Speaker 1>state to another state even though there's like a potential

0:19:00.800 --> 0:19:04.160
<v Speaker 1>barrier in between it. It does this by quantum tunneling.

0:19:04.240 --> 0:19:07.119
<v Speaker 1>It's like an electron stuck in one little hole that

0:19:07.240 --> 0:19:09.359
<v Speaker 1>ends up in another little hole, even though it doesn't

0:19:09.359 --> 0:19:12.119
<v Speaker 1>have the energy to go over the barrier. So carbon

0:19:12.160 --> 0:19:16.639
<v Speaker 1>fourteen turns into nitrogen fourteen through this random quantum mechanical

0:19:16.720 --> 0:19:19.639
<v Speaker 1>tunneling process that lets a switch from one state to

0:19:19.720 --> 0:19:23.119
<v Speaker 1>a lower energy state without having enough energy to actually

0:19:23.119 --> 0:19:25.840
<v Speaker 1>go over the barrier in between them. That's another thing

0:19:25.840 --> 0:19:28.600
<v Speaker 1>I'm amazed we ever managed to figure out. I know,

0:19:28.720 --> 0:19:31.440
<v Speaker 1>so like quantum mechanics is happening all over the place

0:19:31.480 --> 0:19:35.040
<v Speaker 1>in the atmosphere right in front of us. That's crazy.

0:19:35.200 --> 0:19:38.040
<v Speaker 1>So where do we get carbon fourteen in the first place? Yeah,

0:19:38.119 --> 0:19:40.720
<v Speaker 1>carbon fourteen only sticks around for a few thousand years.

0:19:40.720 --> 0:19:43.000
<v Speaker 1>So you might wonder, like the Earth is billions of

0:19:43.080 --> 0:19:45.200
<v Speaker 1>years old, why do we have a new carbon fourteen?

0:19:45.600 --> 0:19:47.560
<v Speaker 1>And the only reason we do is that we have

0:19:47.600 --> 0:19:50.400
<v Speaker 1>a source of it, right, this new carbon fourteen being

0:19:50.440 --> 0:19:54.440
<v Speaker 1>made all the time, and of course it comes from space.

0:19:55.240 --> 0:19:58.040
<v Speaker 1>The Earth is not just sitting out in empty space.

0:19:58.200 --> 0:20:02.080
<v Speaker 1>Space is very far from We're being inundated with high

0:20:02.160 --> 0:20:05.480
<v Speaker 1>energy particles all the time, from the Sun, from black

0:20:05.520 --> 0:20:08.920
<v Speaker 1>hole accretion disks, from other galaxies. All sorts of stuff

0:20:08.920 --> 0:20:12.040
<v Speaker 1>are smashing into the Earth all the time. And then

0:20:12.119 --> 0:20:14.560
<v Speaker 1>we call these things cosmic rays, and when they hit

0:20:14.600 --> 0:20:18.120
<v Speaker 1>the upper atmosphere, they cause all sorts of reactions. They

0:20:18.119 --> 0:20:20.960
<v Speaker 1>smash into stuff and they change it. What happens is

0:20:21.240 --> 0:20:24.960
<v Speaker 1>a cosmic ray will smash into like a proton that's

0:20:24.960 --> 0:20:28.359
<v Speaker 1>in nitrogen, which is seven P seven N, and convert

0:20:28.400 --> 0:20:32.240
<v Speaker 1>it into a neutron. So you have nitrogen fourteen smash

0:20:32.359 --> 0:20:34.640
<v Speaker 1>banging with a proton, and you end up with carbon

0:20:34.720 --> 0:20:38.200
<v Speaker 1>fourteen because one of those protons has gotten converted into

0:20:38.200 --> 0:20:41.800
<v Speaker 1>a neutron. WHOA Okay, And that's all happening in the

0:20:41.840 --> 0:20:44.560
<v Speaker 1>atmosphere and not happening much on Earth, Is that right?

0:20:44.600 --> 0:20:47.159
<v Speaker 1>That's right, It's happening mostly in the upper atmosphere. Cosmic

0:20:47.280 --> 0:20:50.520
<v Speaker 1>rays can't just fly through the atmosphere. They interact with particles.

0:20:50.520 --> 0:20:52.320
<v Speaker 1>It's sort of like running into a crowd, right, You're

0:20:52.320 --> 0:20:55.080
<v Speaker 1>going to bang into all the other particles. Because cosmic

0:20:55.160 --> 0:20:57.560
<v Speaker 1>rays they're just particles. They sound spooky and weird, but

0:20:57.600 --> 0:20:59.720
<v Speaker 1>they're just particles. So these things are created in the

0:21:00.160 --> 0:21:02.639
<v Speaker 1>atmosphere and then they sort of drift down to the

0:21:02.640 --> 0:21:04.639
<v Speaker 1>rest of the planet. Okay, all right, so now we

0:21:04.720 --> 0:21:07.560
<v Speaker 1>know how we get carbon fourteen, and we should take

0:21:07.560 --> 0:21:10.720
<v Speaker 1>a break and when we come back, we'll talk about

0:21:10.880 --> 0:21:13.680
<v Speaker 1>how it goes from the atmosphere to being incorporated into

0:21:13.720 --> 0:21:31.440
<v Speaker 1>living things. And we're back. Okay. So carbon fourteen, made

0:21:31.480 --> 0:21:35.600
<v Speaker 1>by cosmic rays in the atmosphere, falls down towards the

0:21:35.640 --> 0:21:38.840
<v Speaker 1>living stuff that lives below. And then what happens, Daniel,

0:21:39.000 --> 0:21:42.639
<v Speaker 1>So carbon fourteen interacts with oxygen in the atmosphere to

0:21:42.680 --> 0:21:45.800
<v Speaker 1>make carbon dioxide, and so now you have these special

0:21:45.880 --> 0:21:48.920
<v Speaker 1>molecules of carbon dioxide. Most of the carbon dioxide in

0:21:48.960 --> 0:21:52.080
<v Speaker 1>the atmosphere has carbon twelve in its normal stuff, but

0:21:52.200 --> 0:21:55.919
<v Speaker 1>about one in a trillion has a carbon fourteen atom,

0:21:56.240 --> 0:21:59.800
<v Speaker 1>So it's carbon fourteen plus two normal oxygens. And this

0:21:59.840 --> 0:22:02.560
<v Speaker 1>is just floating out there around in the atmosphere. And

0:22:02.560 --> 0:22:05.640
<v Speaker 1>so when plants, for example, do photosynthesis and they breathe

0:22:05.720 --> 0:22:08.879
<v Speaker 1>in carbon dioxide, most of the time they're breathing in

0:22:09.080 --> 0:22:13.120
<v Speaker 1>normal vanilla carbon dioxide, but sometimes one in a trillion

0:22:13.240 --> 0:22:16.520
<v Speaker 1>to get the extra spicy version of carbon dioxide that

0:22:16.520 --> 0:22:19.320
<v Speaker 1>has carbon fourteen in it, so they take it in

0:22:19.680 --> 0:22:22.639
<v Speaker 1>and then when you eat your impossible burger, which is

0:22:22.680 --> 0:22:24.960
<v Speaker 1>made out of plants, you're eating that carbon fourteen that

0:22:25.000 --> 0:22:28.800
<v Speaker 1>got incorporated into the plant. So do plants have more

0:22:28.960 --> 0:22:33.199
<v Speaker 1>carbon fourteen than animals because they're sucking so much of

0:22:33.200 --> 0:22:35.440
<v Speaker 1>it out of the atmosphere or is that not how

0:22:35.480 --> 0:22:39.520
<v Speaker 1>it works? Carbon fourteen definitely flows through the sort of biosphere,

0:22:39.560 --> 0:22:41.560
<v Speaker 1>and its richest at the source. Like if you go

0:22:41.600 --> 0:22:45.000
<v Speaker 1>into the upper atmosphere, that's the highest fraction of carbon fourteen.

0:22:45.280 --> 0:22:47.480
<v Speaker 1>As you get further and further away from the source,

0:22:47.720 --> 0:22:50.200
<v Speaker 1>you get less and less carbon fourteen because it starts

0:22:50.200 --> 0:22:53.440
<v Speaker 1>to decay. Now it decays a really, really slowly, So

0:22:53.520 --> 0:22:56.000
<v Speaker 1>like most plants and most animals on the surface have

0:22:56.080 --> 0:22:58.879
<v Speaker 1>about as much carbon fourteen in them as exist in

0:22:58.920 --> 0:23:01.480
<v Speaker 1>the upper atmosphere. Like the bottom of the ocean, the

0:23:01.600 --> 0:23:05.639
<v Speaker 1>deep ocean doesn't interact with the atmosphere as often, and

0:23:05.680 --> 0:23:08.360
<v Speaker 1>so the rate of carbon fourteen down there is much

0:23:08.440 --> 0:23:10.720
<v Speaker 1>less because it takes longer to get down there, and

0:23:10.720 --> 0:23:13.200
<v Speaker 1>by the time it does, some of it has decayed.

0:23:13.760 --> 0:23:16.600
<v Speaker 1>And so like deep ocean animals tend to have less

0:23:16.640 --> 0:23:19.680
<v Speaker 1>carbon fourteen than like birds that live in the high

0:23:19.720 --> 0:23:22.439
<v Speaker 1>atmosphere or you know, cows that live on the surface.

0:23:22.480 --> 0:23:25.679
<v Speaker 1>We can actually map the carbon fourteen fraction over the

0:23:25.680 --> 0:23:28.719
<v Speaker 1>biosphere and see how that flows. Okay, And so in general,

0:23:28.760 --> 0:23:31.840
<v Speaker 1>we're also not really interested in like you know, there

0:23:31.840 --> 0:23:35.119
<v Speaker 1>are one hundred units of carbon fourteen in a tree.

0:23:35.200 --> 0:23:40.200
<v Speaker 1>We're interested in the relative amounts of carbon twelve compared

0:23:40.240 --> 0:23:43.200
<v Speaker 1>to carbon fourteen. Is that right? So it's about relative

0:23:43.200 --> 0:23:46.200
<v Speaker 1>amounts as opposed to absolute quantities. Yeah, exactly. And this

0:23:46.280 --> 0:23:49.400
<v Speaker 1>is the really fascinating bit about carbon fourteen. Right. First

0:23:49.440 --> 0:23:51.359
<v Speaker 1>of all, it's a natural clock. It's this thing that

0:23:51.440 --> 0:23:54.439
<v Speaker 1>happens in the universe. You create carbon fourteen, you have

0:23:54.440 --> 0:23:58.119
<v Speaker 1>about fifty seven hundred years until it decays. The fascinating

0:23:58.119 --> 0:24:00.359
<v Speaker 1>thing about carbon fourteen is that we use it to

0:24:00.480 --> 0:24:04.439
<v Speaker 1>date when something dies, right, we can tell when something

0:24:04.480 --> 0:24:07.639
<v Speaker 1>has died. And when I first heard about this, I thought, what,

0:24:08.000 --> 0:24:11.119
<v Speaker 1>how does like the carbon know that you've died. Is

0:24:11.119 --> 0:24:13.159
<v Speaker 1>it like as soon as you die your carbon fourteen

0:24:13.200 --> 0:24:16.000
<v Speaker 1>atoms start ticking or something. I thought that was really weird,

0:24:16.040 --> 0:24:19.000
<v Speaker 1>because you know, life and death is this holistic property

0:24:19.000 --> 0:24:21.800
<v Speaker 1>of an object, and like the carbon fourteen doesn't care

0:24:21.880 --> 0:24:24.359
<v Speaker 1>if you're alive or dead. Right, So the reason that

0:24:24.400 --> 0:24:27.240
<v Speaker 1>carbon fourteen is sensitive to your moment of death is

0:24:27.320 --> 0:24:29.680
<v Speaker 1>because of what you stop doing when you die, which

0:24:29.760 --> 0:24:32.479
<v Speaker 1>is you stop breathing and you stop eating, so you

0:24:32.520 --> 0:24:36.000
<v Speaker 1>stop getting new carbon fourteen. So all the carbon fourteen

0:24:36.080 --> 0:24:39.120
<v Speaker 1>in your body is always decaying. Like that clock started

0:24:39.240 --> 0:24:41.399
<v Speaker 1>when the cosmic array hit in the upper atmosphere, and

0:24:41.400 --> 0:24:43.600
<v Speaker 1>maybe it took a few hundred years before you ate

0:24:43.640 --> 0:24:46.520
<v Speaker 1>that carbon fourteen, and so that clock has already started.

0:24:46.600 --> 0:24:49.080
<v Speaker 1>What doesn't happen anymore when you die is that you

0:24:49.119 --> 0:24:51.879
<v Speaker 1>don't get any fresh carbon fourteen, and so now the

0:24:51.920 --> 0:24:54.439
<v Speaker 1>carbon fourteen in your body is decaying and it's not

0:24:54.560 --> 0:24:57.600
<v Speaker 1>being replaced. So something that died a long time ago

0:24:57.720 --> 0:25:00.320
<v Speaker 1>will have almost no carbon fourteen in it. If you

0:25:00.359 --> 0:25:02.639
<v Speaker 1>died ten minutes ago, you still have a lot of

0:25:02.680 --> 0:25:05.200
<v Speaker 1>carbon fourteen in you. So it's not really like the

0:25:05.240 --> 0:25:07.760
<v Speaker 1>moment of death. It's more like the moment you stopped

0:25:07.840 --> 0:25:11.239
<v Speaker 1>participating in the biosphere, which I guess is really the

0:25:11.280 --> 0:25:13.880
<v Speaker 1>same thing. Do you like the microbes that break you

0:25:14.000 --> 0:25:17.760
<v Speaker 1>down put some more carbon fourteen in there to mess

0:25:17.800 --> 0:25:19.760
<v Speaker 1>the clock up a little. I guess it doesn't matter,

0:25:19.760 --> 0:25:22.080
<v Speaker 1>because if the half life is five thousand, seven hundred years,

0:25:22.119 --> 0:25:24.639
<v Speaker 1>we're talking about like a week or two of microbes

0:25:24.680 --> 0:25:27.159
<v Speaker 1>messing up the values. Yeah, good question. I guess it

0:25:27.200 --> 0:25:30.199
<v Speaker 1>depends a little bit if they're aerobic or an aerobic. Right,

0:25:30.240 --> 0:25:32.240
<v Speaker 1>are they consuming CO two? I'll have to ask a

0:25:32.320 --> 0:25:35.320
<v Speaker 1>microbiologist about that. Check in with my wife about it later.

0:25:35.359 --> 0:25:38.800
<v Speaker 1>I thank you, no one. Yeah, that's right, that's very convenient.

0:25:39.040 --> 0:25:41.200
<v Speaker 1>And so this has a really interesting history. It was

0:25:41.280 --> 0:25:44.520
<v Speaker 1>like in the forties that people figured out, oh maybe

0:25:44.560 --> 0:25:47.800
<v Speaker 1>this is possible. People were studying carbon fourteen just from

0:25:47.880 --> 0:25:50.080
<v Speaker 1>like a chemistry point of view, like what is this stuff?

0:25:50.320 --> 0:25:52.600
<v Speaker 1>How long does it last? And at the time, you know,

0:25:52.600 --> 0:25:55.400
<v Speaker 1>we didn't really understand the nucleus very well. People were

0:25:55.440 --> 0:25:58.320
<v Speaker 1>making estimates for how long it might last, and the

0:25:58.359 --> 0:26:00.720
<v Speaker 1>measurements they made were really surprised, and they discovered, oh,

0:26:00.720 --> 0:26:03.399
<v Speaker 1>my gosh, this stuff lasts a lot longer than we thought.

0:26:03.600 --> 0:26:06.520
<v Speaker 1>They expected to have a much shorter half life, like

0:26:06.800 --> 0:26:09.720
<v Speaker 1>tens or hundreds of years, so when they discovered that

0:26:09.760 --> 0:26:12.639
<v Speaker 1>it has a half life of almost six thousand years,

0:26:12.800 --> 0:26:16.160
<v Speaker 1>they were surprised. But it also opened up this really

0:26:16.160 --> 0:26:19.800
<v Speaker 1>cool possibility. Why were they surprised, Like, did we expect

0:26:20.400 --> 0:26:24.040
<v Speaker 1>that half lives would be like similar between objects on

0:26:24.080 --> 0:26:27.960
<v Speaker 1>the periodic table and they ended up not being similar. Yes,

0:26:28.000 --> 0:26:30.680
<v Speaker 1>there are reason they were surprised, or just sometimes sizes surprising.

0:26:31.320 --> 0:26:34.159
<v Speaker 1>They were surprised because we just didn't understand the nucleus

0:26:34.200 --> 0:26:36.280
<v Speaker 1>of the atom very well. I mean, this is the forties, right,

0:26:36.359 --> 0:26:38.760
<v Speaker 1>Quantum mechanics were very very new, and so all of

0:26:38.800 --> 0:26:41.320
<v Speaker 1>our calculations of how things work in the nucleus were

0:26:41.400 --> 0:26:43.680
<v Speaker 1>very very rough and a lot of handwaving. I mean

0:26:43.760 --> 0:26:47.680
<v Speaker 1>even today, it's not easy to do these calculations to say,

0:26:47.720 --> 0:26:49.480
<v Speaker 1>like what would be the mass of this particle or

0:26:49.520 --> 0:26:51.959
<v Speaker 1>how stable would that be. You know, we have theories

0:26:52.040 --> 0:26:54.959
<v Speaker 1>about whether the super heavy elements would be stable, but

0:26:55.040 --> 0:26:57.160
<v Speaker 1>we can't say these things for certain because we don't

0:26:57.160 --> 0:27:00.240
<v Speaker 1>know how to do a lot of these calculations. Because

0:27:00.280 --> 0:27:03.879
<v Speaker 1>the strong nuclear force is very complicated. It's very very strong,

0:27:03.880 --> 0:27:06.560
<v Speaker 1>which means the calculations are very very sensitive to getting

0:27:06.560 --> 0:27:08.639
<v Speaker 1>things wrong. It's a kind of calculation where if you

0:27:08.680 --> 0:27:10.720
<v Speaker 1>start to get things a little bit wrong, the wrongness

0:27:10.800 --> 0:27:13.520
<v Speaker 1>gets amplified by the strength of the force instead of

0:27:13.560 --> 0:27:16.440
<v Speaker 1>like a decaying away. Like with gravity, if you get

0:27:16.440 --> 0:27:18.960
<v Speaker 1>the location of an asteroid a little bit wrong, it's

0:27:18.960 --> 0:27:21.560
<v Speaker 1>not going to propagate to becoming really really wrong later

0:27:21.640 --> 0:27:23.560
<v Speaker 1>on because gravity is so weak, so you can make

0:27:23.600 --> 0:27:26.000
<v Speaker 1>approximations and mostly get the right answer at least for

0:27:26.040 --> 0:27:28.760
<v Speaker 1>the foreseeable future. With the strong force, as soon as

0:27:28.800 --> 0:27:31.320
<v Speaker 1>you get something a little bit wrong, everything goes totally wrong.

0:27:31.400 --> 0:27:34.640
<v Speaker 1>So the short version is that nuclear physics is hard. Well,

0:27:34.640 --> 0:27:37.040
<v Speaker 1>that's not surprising, and so maybe they shouldn't have been

0:27:37.080 --> 0:27:41.000
<v Speaker 1>surprised because nuclear physics is hard. Okay. So you had

0:27:41.040 --> 0:27:43.240
<v Speaker 1>mentioned at the top of the show that sewage was

0:27:43.280 --> 0:27:45.320
<v Speaker 1>gonna come into the story at some point, and so

0:27:45.359 --> 0:27:47.480
<v Speaker 1>I'm hoping that now that we're talking about, you know,

0:27:47.720 --> 0:27:50.320
<v Speaker 1>when we figure out the whole carbon fourteen thing, is

0:27:50.320 --> 0:27:52.119
<v Speaker 1>this when we get to talk about the sewage. This

0:27:52.200 --> 0:27:54.800
<v Speaker 1>is when we get to talk about the sewage. Absolutely yea.

0:27:55.320 --> 0:27:58.760
<v Speaker 1>So it was in mid nineteen forties and Willard Libby,

0:27:59.080 --> 0:28:02.040
<v Speaker 1>who was at Berkeley, learned about these results that carbon

0:28:02.119 --> 0:28:05.600
<v Speaker 1>fourteen was surprisingly long lasting, and he thought, hey, that

0:28:05.640 --> 0:28:07.920
<v Speaker 1>would be a really cool way to figure out how

0:28:07.960 --> 0:28:10.640
<v Speaker 1>long something has been dead. And so what he did

0:28:11.080 --> 0:28:12.719
<v Speaker 1>is he moved to a new job at the University

0:28:12.720 --> 0:28:15.719
<v Speaker 1>of Chicago and he proposed this idea. He said, oh,

0:28:15.800 --> 0:28:18.280
<v Speaker 1>maybe this will work. And the first thing they did

0:28:18.440 --> 0:28:22.840
<v Speaker 1>was to study methane from the Boston sewage system. Right,

0:28:22.840 --> 0:28:25.840
<v Speaker 1>So methane is a gas, right, that's produced when sewage

0:28:25.840 --> 0:28:29.320
<v Speaker 1>basically ferments. Right, my grooves are consuming your sewage. And

0:28:29.320 --> 0:28:31.880
<v Speaker 1>so they gathered this and they measured the carbon fourteen

0:28:31.920 --> 0:28:35.960
<v Speaker 1>fraction in methane basically from Boston's dark matter, and then

0:28:36.000 --> 0:28:40.120
<v Speaker 1>they compared that to how much carbon fourteen there was

0:28:40.200 --> 0:28:43.080
<v Speaker 1>in methane from fossil fuels, right, Like the methane that

0:28:43.160 --> 0:28:45.720
<v Speaker 1>maybe you burn in your house comes from plants that

0:28:45.840 --> 0:28:49.000
<v Speaker 1>died millions and millions and millions of years ago. And

0:28:49.080 --> 0:28:51.240
<v Speaker 1>what they found is no surprise to us now, is

0:28:51.280 --> 0:28:53.840
<v Speaker 1>that the methane from the Boston sewis system has a

0:28:53.840 --> 0:28:56.560
<v Speaker 1>lot of carbon fourteen and the methane from fossil fuels

0:28:56.640 --> 0:28:59.760
<v Speaker 1>has none. All Right, So that's beginning to tell us

0:28:59.760 --> 0:29:02.640
<v Speaker 1>the limits for how we can use carbon fourteen for dating.

0:29:02.720 --> 0:29:06.400
<v Speaker 1>But I'll know you said that Libby had moved to Chicago,

0:29:07.040 --> 0:29:10.040
<v Speaker 1>but he looked at the Boston sewage is there, just like,

0:29:10.200 --> 0:29:12.880
<v Speaker 1>is Boston sewage the best sewage? Why did you travel

0:29:12.920 --> 0:29:16.200
<v Speaker 1>all the way to Boston? Was the Chicago sewage wasn't

0:29:16.240 --> 0:29:19.959
<v Speaker 1>disgusting enough. I'm sure those people who live in Boston

0:29:20.000 --> 0:29:22.360
<v Speaker 1>are very proud of their sewage. I have a little

0:29:22.400 --> 0:29:24.760
<v Speaker 1>glimpse into this because of my wife's research. You know,

0:29:24.880 --> 0:29:27.320
<v Speaker 1>she studies the microbes and sewage, and it can be

0:29:27.360 --> 0:29:30.240
<v Speaker 1>surprisingly tricky to get access to it. So I suspect

0:29:30.320 --> 0:29:33.120
<v Speaker 1>it's just a question of like politics and access. Not

0:29:33.160 --> 0:29:36.480
<v Speaker 1>every waste management system is interested in having scientists like

0:29:36.600 --> 0:29:40.320
<v Speaker 1>dig around in their facility, while others are you free

0:29:40.360 --> 0:29:43.840
<v Speaker 1>to share the science gold that is flowing through their pipes?

0:29:47.040 --> 0:29:49.480
<v Speaker 1>Politics and sewage? Yeah, so I suspect they had a

0:29:49.520 --> 0:29:52.760
<v Speaker 1>good Boston connect, you know, for some real primo Boston

0:29:52.880 --> 0:29:56.560
<v Speaker 1>sewage got it okay. So so by the time you

0:29:56.640 --> 0:30:00.800
<v Speaker 1>ask petroleum, there's no carbon fourteen and you start losing

0:30:00.800 --> 0:30:03.880
<v Speaker 1>carbon fourteen when you die. So can you use this for?

0:30:04.440 --> 0:30:06.760
<v Speaker 1>Is this helpful for like certain kinds of fossils? What

0:30:06.840 --> 0:30:08.600
<v Speaker 1>kind of things that we use this for? So far,

0:30:08.840 --> 0:30:11.320
<v Speaker 1>you can use this for basically anything that's died in

0:30:11.360 --> 0:30:15.280
<v Speaker 1>the last maybe fifty thousand years, because those things were

0:30:15.320 --> 0:30:18.840
<v Speaker 1>accumulating carbon fourteen as they were alive and participating in

0:30:18.840 --> 0:30:21.560
<v Speaker 1>the biosphere, and as soon as they died, then they

0:30:21.560 --> 0:30:25.360
<v Speaker 1>stopped and the carbon fourteen started to decay away. Now,

0:30:25.400 --> 0:30:27.560
<v Speaker 1>things that are much much older than that, they just

0:30:27.600 --> 0:30:30.440
<v Speaker 1>have zero carbon fourteen. So you can't tell is this

0:30:30.480 --> 0:30:32.880
<v Speaker 1>thing one hundred thousand years old or one hundred million

0:30:32.960 --> 0:30:35.960
<v Speaker 1>years old or four billion years old, because you just

0:30:36.080 --> 0:30:38.520
<v Speaker 1>get zero. So what you got to do is measure

0:30:38.840 --> 0:30:42.120
<v Speaker 1>the carbon fourteen to carbon twelve ratio in your thing,

0:30:42.280 --> 0:30:45.080
<v Speaker 1>and then you can extrapolate back to when did this

0:30:45.120 --> 0:30:48.880
<v Speaker 1>thing last have the sort of normal rate of carbon fourteen?

0:30:49.240 --> 0:30:52.760
<v Speaker 1>Got it all right, So dinosaurs are out, but helpful

0:30:52.840 --> 0:30:58.320
<v Speaker 1>for things like human archaeology questions exactly. Human archaeology was

0:30:58.360 --> 0:31:02.400
<v Speaker 1>really like revolutionized this subject. The first time that they

0:31:02.560 --> 0:31:05.800
<v Speaker 1>used it was actually to date some Egyptian tombs. These

0:31:05.840 --> 0:31:08.400
<v Speaker 1>are some things that archaeologically we already knew what the

0:31:08.480 --> 0:31:12.480
<v Speaker 1>dates were based on writing and other analysis, Like archaeologists

0:31:12.520 --> 0:31:15.480
<v Speaker 1>already knew when somebody had been buried, and now they

0:31:15.480 --> 0:31:18.280
<v Speaker 1>were able to take a sample and measure the carbon

0:31:18.360 --> 0:31:20.920
<v Speaker 1>fourteen fraction in like a piece of linen or in

0:31:20.960 --> 0:31:25.160
<v Speaker 1>a piece of wood from the tomb and independently establish

0:31:25.400 --> 0:31:28.520
<v Speaker 1>the date of the death of that object, like here's

0:31:28.520 --> 0:31:31.920
<v Speaker 1>when the tree that formed this plank must have been killed,

0:31:32.280 --> 0:31:35.560
<v Speaker 1>or here's when this plant was harvested to make this linen.

0:31:35.880 --> 0:31:39.360
<v Speaker 1>And that's really powerful. It's like a completely separate clock

0:31:39.400 --> 0:31:43.320
<v Speaker 1>that lines up archaeologically with your records. Okay, So one,

0:31:43.360 --> 0:31:45.800
<v Speaker 1>that's awesome, and two I bet this has been used

0:31:45.840 --> 0:31:48.960
<v Speaker 1>at some point in ways that have made people angry,

0:31:48.960 --> 0:31:50.640
<v Speaker 1>like people who thought they had a thing that was

0:31:50.680 --> 0:31:52.600
<v Speaker 1>old but it ended up not being that old, or

0:31:52.680 --> 0:31:56.040
<v Speaker 1>the other way around. But before I ask you about that,

0:31:56.680 --> 0:32:12.960
<v Speaker 1>let's take another quick break. All right, So has this

0:32:13.040 --> 0:32:16.320
<v Speaker 1>method been used in a way that ended up making

0:32:16.320 --> 0:32:21.000
<v Speaker 1>people like why do I feel like you're digging for

0:32:21.000 --> 0:32:24.120
<v Speaker 1>the controversy here? Keey? Well, you know it makes good radio.

0:32:25.440 --> 0:32:28.600
<v Speaker 1>It does absolutely. Yeah, this is a really cool technique

0:32:28.640 --> 0:32:30.720
<v Speaker 1>and it's powerful because they can date things to like

0:32:30.840 --> 0:32:33.479
<v Speaker 1>within a few decades. You know. The thing is that

0:32:33.520 --> 0:32:36.440
<v Speaker 1>there's a lot of carbon in living stuff, and the

0:32:36.520 --> 0:32:39.320
<v Speaker 1>more carbon you have, the more preciser measurement can be.

0:32:39.600 --> 0:32:41.560
<v Speaker 1>So you can like pin down to within a few

0:32:41.560 --> 0:32:45.040
<v Speaker 1>decades when something died, and for example, when people discovered,

0:32:45.080 --> 0:32:48.800
<v Speaker 1>like the Dead Sea Scrolls, these ancient scrolls outside of

0:32:48.880 --> 0:32:51.160
<v Speaker 1>Jerusalem that have been in the desert for who knows

0:32:51.200 --> 0:32:52.920
<v Speaker 1>how long, and what may have been one of the

0:32:52.960 --> 0:32:56.160
<v Speaker 1>earliest written records of you know, the books of the Bible.

0:32:56.320 --> 0:32:59.080
<v Speaker 1>People wanted to know like, are these real? Are they

0:32:59.160 --> 0:33:01.440
<v Speaker 1>actually thousands of years old? Or is this like a

0:33:01.480 --> 0:33:05.440
<v Speaker 1>forgery from last week that's been stained with tea? And

0:33:06.280 --> 0:33:09.120
<v Speaker 1>so they were able to use radiocarbon dating to confirm

0:33:09.200 --> 0:33:12.560
<v Speaker 1>that these things were one thousand, nine hundred and seventeen

0:33:12.640 --> 0:33:15.160
<v Speaker 1>years old, which really told people like, these are an

0:33:15.200 --> 0:33:18.000
<v Speaker 1>ancient relic. You know, these are not created recently, or

0:33:18.000 --> 0:33:21.240
<v Speaker 1>at least the materials on which they were made are

0:33:21.360 --> 0:33:24.440
<v Speaker 1>fairly old. So either it's a really old book or

0:33:24.480 --> 0:33:27.320
<v Speaker 1>it's new writing on a really old sheet of paper. Well,

0:33:27.560 --> 0:33:29.760
<v Speaker 1>I'm gonna have to give you that. That's awesome. That's

0:33:29.800 --> 0:33:32.680
<v Speaker 1>not what I asked. I asked you for controversy that

0:33:32.840 --> 0:33:35.920
<v Speaker 1>you gave me confirmation. But still all right, so that's

0:33:35.920 --> 0:33:39.000
<v Speaker 1>pretty awesome. Well this controversy. Also, you may have heard

0:33:39.040 --> 0:33:41.640
<v Speaker 1>about the Shroud of Turin. This is this piece of

0:33:41.680 --> 0:33:44.720
<v Speaker 1>cloth that I think is held in Milan. That's supposed

0:33:44.720 --> 0:33:47.320
<v Speaker 1>to have like the face of Jesus on it, and

0:33:47.400 --> 0:33:50.520
<v Speaker 1>the mythology around it is that it wrapped to Jesus's

0:33:50.560 --> 0:33:53.360
<v Speaker 1>corpse and was sort of imprinted by the power of

0:33:53.440 --> 0:33:57.400
<v Speaker 1>his un don't know, spiritual personality with his face. And

0:33:57.480 --> 0:34:00.520
<v Speaker 1>so this is a relic that's been celebrated in people

0:34:00.560 --> 0:34:03.280
<v Speaker 1>like pilgrimage to go and see it, and so they

0:34:03.400 --> 0:34:06.440
<v Speaker 1>radiocarbon dated it and discovered Oops, it's actually from the

0:34:06.520 --> 0:34:09.919
<v Speaker 1>fourteenth century, which means it's pretty old. It's like six

0:34:10.040 --> 0:34:13.680
<v Speaker 1>hundred years old. But the plants that made this shroud

0:34:14.160 --> 0:34:18.080
<v Speaker 1>were grown and planted like fourteen hundred years after Jesus died.

0:34:18.440 --> 0:34:22.520
<v Speaker 1>That's disappointing. Is it safe to assume that there are

0:34:22.560 --> 0:34:26.880
<v Speaker 1>people who don't buy the science on this to this day? Oh? Absolutely,

0:34:26.920 --> 0:34:29.640
<v Speaker 1>the way people deny evolution or that the Earth is

0:34:29.719 --> 0:34:33.719
<v Speaker 1>round or the dinosaurs existed well before humans. There are

0:34:33.760 --> 0:34:36.880
<v Speaker 1>people who say radiocarbon dating is not reliable and that

0:34:36.960 --> 0:34:39.759
<v Speaker 1>you can't use it, especially, you know, when it contradicts

0:34:39.760 --> 0:34:42.200
<v Speaker 1>their belief. The thing I love about the Shroud of

0:34:42.360 --> 0:34:45.360
<v Speaker 1>Tern story is not just that it reveals that the

0:34:45.360 --> 0:34:47.880
<v Speaker 1>whole thing is a hoax, but it's an ancient hoax.

0:34:48.160 --> 0:34:51.640
<v Speaker 1>The hoax is now hundreds of years old, right, the

0:34:51.680 --> 0:34:56.000
<v Speaker 1>hoax itself is of historical interest. That's how old it is. Right,

0:34:56.640 --> 0:34:59.000
<v Speaker 1>A six hundred year old hoax is pretty cool. Okay,

0:34:59.040 --> 0:35:01.560
<v Speaker 1>it's not the face of g but wow, that's really

0:35:01.560 --> 0:35:03.680
<v Speaker 1>cool insight and like what people were doing and why

0:35:03.719 --> 0:35:05.480
<v Speaker 1>they wanted to do it and all sorts of stuff.

0:35:05.520 --> 0:35:08.720
<v Speaker 1>I love how like today's mundanity, right, and even lies

0:35:08.880 --> 0:35:13.400
<v Speaker 1>can turn into something fascinating for future anthropologists. Yeah, know,

0:35:13.520 --> 0:35:16.480
<v Speaker 1>humans have enjoyed messing with each other for a really

0:35:16.520 --> 0:35:19.319
<v Speaker 1>long time. It's good to know that. But it is

0:35:19.400 --> 0:35:22.240
<v Speaker 1>tricky to date things with carbon fourteen because it turns

0:35:22.239 --> 0:35:24.719
<v Speaker 1>out that the assumption we made at the beginning that

0:35:24.800 --> 0:35:27.680
<v Speaker 1>like carbon fourteen is produced in the upper atmosphere and

0:35:27.800 --> 0:35:32.360
<v Speaker 1>spreads around mostly evenly to everything, it's not exactly true,

0:35:32.960 --> 0:35:35.160
<v Speaker 1>and so you got to like make some corrections and

0:35:35.239 --> 0:35:38.600
<v Speaker 1>calibrations to get things as precise as you'd like. So, like,

0:35:38.840 --> 0:35:43.040
<v Speaker 1>how not exact are we talking here? Like you know

0:35:43.600 --> 0:35:45.600
<v Speaker 1>the flies that you find in bodies? I think things

0:35:45.600 --> 0:35:49.200
<v Speaker 1>like temperature impact development time. How many things impact our

0:35:49.239 --> 0:35:52.359
<v Speaker 1>ability to date things based on carbon fourteen? And are

0:35:52.360 --> 0:35:54.600
<v Speaker 1>they things that we can learn about and control for

0:35:55.440 --> 0:35:57.840
<v Speaker 1>or no, yes, absolutely we can learn about them. And

0:35:57.880 --> 0:36:00.640
<v Speaker 1>it's like a whole field of people calib rating carbon

0:36:00.680 --> 0:36:04.440
<v Speaker 1>fourteen dating. We first discovered this actually when carbon fourteen

0:36:04.520 --> 0:36:08.239
<v Speaker 1>dating got some Egyptian tombs wrong, like some of them

0:36:08.239 --> 0:36:11.040
<v Speaker 1>were bang on the archaeological records, and other ones that

0:36:11.200 --> 0:36:15.200
<v Speaker 1>archaeologists were pretty sure about. Radiocarbon dating got a little wrong,

0:36:15.200 --> 0:36:17.840
<v Speaker 1>and people thought, hmm, that's weird. I wonder what it means.

0:36:18.400 --> 0:36:21.440
<v Speaker 1>And so they discovered a few interesting effects. For example,

0:36:21.560 --> 0:36:25.279
<v Speaker 1>carbon fourteen production is not constant over time. If you

0:36:25.280 --> 0:36:27.880
<v Speaker 1>want to assume that you can extrapolate backwards from the

0:36:27.880 --> 0:36:31.960
<v Speaker 1>carbon fourteen ratio today to the carbon fourteen ratio when

0:36:31.960 --> 0:36:34.680
<v Speaker 1>this object died, you have to assume the carbon fourteen

0:36:34.760 --> 0:36:36.920
<v Speaker 1>is being replenished at the same rate over time. But

0:36:36.960 --> 0:36:40.440
<v Speaker 1>it turns out that it's not that there's a variation

0:36:40.640 --> 0:36:44.239
<v Speaker 1>in the carbon fourteen rates in the atmosphere. Whoa is

0:36:44.280 --> 0:36:47.759
<v Speaker 1>that because cosmic rays hit us at different rates? Is

0:36:47.800 --> 0:36:49.879
<v Speaker 1>this like a solar Now that's not a solar wind thing?

0:36:50.120 --> 0:36:54.080
<v Speaker 1>Do we know? Yeah? Why? I am confused. It's really

0:36:54.120 --> 0:36:57.000
<v Speaker 1>interesting and there's some cool physics there. One is that, yes,

0:36:57.080 --> 0:36:59.799
<v Speaker 1>cosmic rays have sort of like seasons that are not

0:37:00.080 --> 0:37:03.440
<v Speaker 1>holy constant. It's sort of like the solar weather. You know,

0:37:03.520 --> 0:37:06.680
<v Speaker 1>where these cosmic grays come from depend on like magnetic

0:37:06.719 --> 0:37:09.279
<v Speaker 1>fields and the galaxy. You know, what's going on with

0:37:09.360 --> 0:37:12.239
<v Speaker 1>the objects that are created them. So there's those kinds

0:37:12.239 --> 0:37:15.160
<v Speaker 1>of effects. But we can actually measure that in independent

0:37:15.239 --> 0:37:20.040
<v Speaker 1>ways because they can look at super ancient trees, right.

0:37:20.120 --> 0:37:23.960
<v Speaker 1>Trees are really cool because they grow and they add rings,

0:37:24.000 --> 0:37:26.880
<v Speaker 1>and those new rings interact with the biosphere, but the

0:37:26.960 --> 0:37:31.160
<v Speaker 1>old rings don't. So every year a tree is basically

0:37:31.200 --> 0:37:34.560
<v Speaker 1>like taking a sample of the carbon fourteen fraction in

0:37:34.600 --> 0:37:37.600
<v Speaker 1>the atmosphere and storing it forever. And so if you

0:37:37.680 --> 0:37:40.520
<v Speaker 1>slice open a really old tree and look back at

0:37:40.520 --> 0:37:43.160
<v Speaker 1>the carbon fourteen fraction in each of the rings, you

0:37:43.200 --> 0:37:46.120
<v Speaker 1>can get like a history of the carbon fourteen fraction

0:37:46.400 --> 0:37:48.560
<v Speaker 1>at the time that the tree was growing. Do you

0:37:48.640 --> 0:37:50.799
<v Speaker 1>not happen to know what the oldest tree we've done

0:37:50.840 --> 0:37:53.239
<v Speaker 1>that on is. Are we talking about like hundreds of

0:37:53.320 --> 0:37:55.799
<v Speaker 1>years worth of data? A thousands. We have lots that

0:37:55.800 --> 0:37:58.200
<v Speaker 1>are hundreds of years and a few that are thousands

0:37:58.200 --> 0:38:00.840
<v Speaker 1>of years, and so that really helped us calibrate like

0:38:00.880 --> 0:38:05.279
<v Speaker 1>the more recent fluctuations in carbon fourteen. But also humans

0:38:05.360 --> 0:38:08.960
<v Speaker 1>have really altered the carbon fourteen fraction in the atmosphere.

0:38:09.360 --> 0:38:12.200
<v Speaker 1>For example, we've been burning a lot of fossil fuels

0:38:12.200 --> 0:38:15.520
<v Speaker 1>over the last couple of hundred years. Fossil fuels have

0:38:15.719 --> 0:38:19.440
<v Speaker 1>carbon but no carbon fourteen, so we've been releasing a

0:38:19.480 --> 0:38:22.680
<v Speaker 1>lot of carbon twelve into the atmosphere, really bringing down

0:38:22.920 --> 0:38:26.400
<v Speaker 1>the carbon fourteen fraction in the atmosphere. So, like, human

0:38:26.440 --> 0:38:29.440
<v Speaker 1>effects have really changed this and made it more complicated

0:38:29.480 --> 0:38:31.759
<v Speaker 1>to interpret the past. Wow. So like if you were

0:38:32.239 --> 0:38:35.359
<v Speaker 1>an alien trying to age stuff that was happening down

0:38:35.400 --> 0:38:38.840
<v Speaker 1>here on Earth, and you wanted to age something you know,

0:38:38.960 --> 0:38:41.280
<v Speaker 1>thousands of years from now that happened during our period,

0:38:42.160 --> 0:38:44.600
<v Speaker 1>it would be a mess. It would be a mess

0:38:44.920 --> 0:38:47.840
<v Speaker 1>if you didn't have ways to calibrate it. And so fortunately,

0:38:47.880 --> 0:38:50.560
<v Speaker 1>like trees can help us understand these things. Because trees

0:38:50.560 --> 0:38:52.279
<v Speaker 1>have been around for hundreds of years since, we can

0:38:52.360 --> 0:38:55.360
<v Speaker 1>understand the effect the humans have had on the carbon

0:38:55.400 --> 0:38:59.239
<v Speaker 1>fourteen fraction in the atmosphere. But more confusingly, we've had

0:38:59.239 --> 0:39:03.040
<v Speaker 1>effects in both directions. So burning fossil fuels lowers the

0:39:03.080 --> 0:39:06.400
<v Speaker 1>carbon fourteen fraction because you're pumping out super old carbon

0:39:06.520 --> 0:39:09.440
<v Speaker 1>where everything has already decayed. But nuclear testing in the

0:39:09.520 --> 0:39:13.359
<v Speaker 1>atmosphere increases the carbon fourteen fraction because it makes new

0:39:13.400 --> 0:39:16.400
<v Speaker 1>carbon fourteen. Is all this radiation and all the products

0:39:16.400 --> 0:39:20.080
<v Speaker 1>of the nuclear testing makes lots and lots of carbon fourteen,

0:39:20.360 --> 0:39:22.960
<v Speaker 1>much more than it's made from cosmic rays. So like

0:39:23.080 --> 0:39:25.480
<v Speaker 1>in the middle of this century, we had like twice

0:39:25.520 --> 0:39:28.759
<v Speaker 1>as much carbon fourteen in the atmosphere as we usually do.

0:39:28.920 --> 0:39:33.880
<v Speaker 1>Where the worst that'll be another interesting problem for the

0:39:33.920 --> 0:39:36.560
<v Speaker 1>aliens to solve. Then where did all this carbon fourteen

0:39:36.640 --> 0:39:38.840
<v Speaker 1>come from? Oh, they were setting off nuclear weapons in

0:39:38.880 --> 0:39:42.839
<v Speaker 1>the sky, of course there were. It's fascinating because there's

0:39:42.840 --> 0:39:45.919
<v Speaker 1>two sides to that. Archaeologists are frustrated by that because

0:39:45.920 --> 0:39:48.920
<v Speaker 1>we're like poisoning the historical record and making it harder

0:39:48.960 --> 0:39:52.560
<v Speaker 1>to figure out when things came from. But geologists actually

0:39:52.560 --> 0:39:55.480
<v Speaker 1>really like it because it's like a really bright signal.

0:39:55.560 --> 0:39:57.840
<v Speaker 1>They're like, Okay, cool, we can use this to calibrate

0:39:57.880 --> 0:40:00.120
<v Speaker 1>and we can tell when something happened because the so

0:40:00.200 --> 0:40:03.120
<v Speaker 1>much carbon fourteen in that layer. So geologists, I think

0:40:03.120 --> 0:40:05.839
<v Speaker 1>would like us to be like regularly nuking the atmosphere

0:40:05.960 --> 0:40:09.759
<v Speaker 1>in predictable and periodic ways because it leaves like this

0:40:10.160 --> 0:40:12.680
<v Speaker 1>ruler back in the record. You know, I know a

0:40:12.719 --> 0:40:15.680
<v Speaker 1>geologist I think is not quite that self interested, but

0:40:16.280 --> 0:40:19.000
<v Speaker 1>I can imagine him thinking that that's a silver lining

0:40:19.080 --> 0:40:22.239
<v Speaker 1>of an awful thing. Humans are complicated. So yeah, so

0:40:22.280 --> 0:40:24.400
<v Speaker 1>you have to take all this into account, and you

0:40:24.440 --> 0:40:26.560
<v Speaker 1>have to know, like what was the rate of carbon

0:40:26.600 --> 0:40:29.520
<v Speaker 1>fourteen in the atmosphere over the last few thousand years.

0:40:29.520 --> 0:40:31.560
<v Speaker 1>And you also have to take into account where you

0:40:31.640 --> 0:40:34.200
<v Speaker 1>have found something. If you found it in the deep ocean,

0:40:34.239 --> 0:40:36.360
<v Speaker 1>then it was going to get less carbon fourteen to

0:40:36.480 --> 0:40:38.200
<v Speaker 1>begin with, and then if you found it in the

0:40:38.239 --> 0:40:42.440
<v Speaker 1>upper atmosphere. Also, the different hemispheres of Earth have different

0:40:42.480 --> 0:40:46.160
<v Speaker 1>depositions of carbon fourteen because there's different like patterns of winds,

0:40:46.520 --> 0:40:49.960
<v Speaker 1>and the North and the South hemisphere actually have totally separate,

0:40:50.080 --> 0:40:53.640
<v Speaker 1>independent wind systems that don't really mix very well. So

0:40:53.680 --> 0:40:56.920
<v Speaker 1>there's less carbon fourteen in the southern atmosphere because it's

0:40:56.960 --> 0:40:59.920
<v Speaker 1>like more surface area of ocean which sucks up more

0:41:00.040 --> 0:41:02.920
<v Speaker 1>carbon fourteen, and there's more carbon fourteen in the northern

0:41:02.960 --> 0:41:05.920
<v Speaker 1>hemisphere where this is less ocean surface. Do you have

0:41:06.040 --> 0:41:08.440
<v Speaker 1>any sense for like for the hemisphere thing, are we

0:41:08.480 --> 0:41:11.480
<v Speaker 1>talking like if you didn't correct for that, you'd be

0:41:11.560 --> 0:41:14.520
<v Speaker 1>off by about ten years or a thousand years, or

0:41:14.560 --> 0:41:15.880
<v Speaker 1>it just kind of depends on a lot of other

0:41:15.920 --> 0:41:18.920
<v Speaker 1>stuff too. These all are really small effects, and everybody

0:41:18.960 --> 0:41:21.360
<v Speaker 1>wants really precise dating of things, you know, down to

0:41:21.400 --> 0:41:23.480
<v Speaker 1>the decades, and so this is the kind of thing

0:41:23.520 --> 0:41:26.440
<v Speaker 1>that happens in science. First, you have a very approximate effect.

0:41:26.480 --> 0:41:28.960
<v Speaker 1>You're like, okay, let's just assume carbon fourteen is constant

0:41:29.000 --> 0:41:32.360
<v Speaker 1>everywhere and over time. What do we get? Oh my gosh,

0:41:32.400 --> 0:41:35.160
<v Speaker 1>it can teach us something already. Then you start to

0:41:35.200 --> 0:41:37.520
<v Speaker 1>hone in on the details you want, like the second

0:41:37.640 --> 0:41:39.719
<v Speaker 1>digit to be accurate, and then the third, and then

0:41:39.800 --> 0:41:42.400
<v Speaker 1>the fourth, and by now we're like, you know, seventy

0:41:42.480 --> 0:41:45.239
<v Speaker 1>years into this research project, we're getting down to the

0:41:45.320 --> 0:41:47.560
<v Speaker 1>nitty greedy details. So a lot of these things will

0:41:47.600 --> 0:41:51.759
<v Speaker 1>affect our estimate for the dates of things by decades

0:41:51.920 --> 0:41:54.959
<v Speaker 1>or maybe up to hundreds of years, not thousands of years.

0:41:54.960 --> 0:41:57.000
<v Speaker 1>It's not going to like up end everything we thought

0:41:57.040 --> 0:42:00.560
<v Speaker 1>we knew. We also need a really precise estimate of

0:42:00.600 --> 0:42:02.960
<v Speaker 1>the half life of carbon fourteen, right, we have to

0:42:03.080 --> 0:42:06.000
<v Speaker 1>be able to calibrate this clock to know how long

0:42:06.080 --> 0:42:09.200
<v Speaker 1>does it take carbon fourteen two decay? And as you said,

0:42:09.200 --> 0:42:11.600
<v Speaker 1>you can't wait around for five thousand years, which would

0:42:11.640 --> 0:42:13.920
<v Speaker 1>be the best way to get an accurate measurement. But

0:42:13.960 --> 0:42:16.600
<v Speaker 1>people have been developing more and more precise experiments with

0:42:16.680 --> 0:42:19.799
<v Speaker 1>like larger samples of carbon fourteen, So they actually had

0:42:19.800 --> 0:42:23.759
<v Speaker 1>to update the official half life of carbon fourteen from

0:42:23.760 --> 0:42:27.560
<v Speaker 1>fifty five sixty eight later to fifty seven thirty so

0:42:27.640 --> 0:42:29.680
<v Speaker 1>a change of like one hundred and fifty years. And

0:42:29.719 --> 0:42:32.960
<v Speaker 1>this is super fascinating because it then required a change

0:42:32.960 --> 0:42:36.239
<v Speaker 1>of all the archaeological dates. Like all the archaeologists who

0:42:36.320 --> 0:42:38.160
<v Speaker 1>thought that their thing was data to a certain date. Oops,

0:42:38.160 --> 0:42:41.120
<v Speaker 1>they got updated because the nuclear physicists or the chemists

0:42:41.320 --> 0:42:43.839
<v Speaker 1>got the number wrong. Does that mean that you get

0:42:43.920 --> 0:42:48.399
<v Speaker 1>to redo all of your publications with the updated date

0:42:48.440 --> 0:42:50.239
<v Speaker 1>and double the number of lines you have on your

0:42:50.239 --> 0:42:53.680
<v Speaker 1>CV because in that case, thank you physicists. It means

0:42:53.680 --> 0:42:55.600
<v Speaker 1>that there's a bunch of papers out there with old

0:42:55.680 --> 0:42:58.560
<v Speaker 1>dates that we now like no need corrections. You can't

0:42:58.600 --> 0:43:01.279
<v Speaker 1>just read the old pay in archaeology and take the

0:43:01.360 --> 0:43:03.400
<v Speaker 1>dates and face value. You have to know when that

0:43:03.520 --> 0:43:07.280
<v Speaker 1>date was calculated. Like what effects did they take into account?

0:43:07.560 --> 0:43:10.040
<v Speaker 1>And what effects do we now take into account? So

0:43:10.080 --> 0:43:13.600
<v Speaker 1>the whole thing has gotten really really complicated. That is frustrating,

0:43:13.760 --> 0:43:16.719
<v Speaker 1>but it also has been an enormous boon to archaeology.

0:43:17.080 --> 0:43:20.400
<v Speaker 1>I mean, what a powerful tool, Like anything that was alive,

0:43:20.719 --> 0:43:23.880
<v Speaker 1>now you can date the moment of its death. And

0:43:23.920 --> 0:43:25.960
<v Speaker 1>that's not a perfect tool, right, It still thinks like

0:43:26.040 --> 0:43:28.560
<v Speaker 1>when was this metal forged? Well, we can't tell because

0:43:28.560 --> 0:43:32.239
<v Speaker 1>it was never alive. It doesn't participate in the carbon biosphere,

0:43:32.360 --> 0:43:34.960
<v Speaker 1>So you can't date like jewelry, you know, or swords

0:43:35.040 --> 0:43:36.920
<v Speaker 1>or stuff like that, but you can look at what

0:43:37.040 --> 0:43:39.480
<v Speaker 1>else is in a grave and you can tell maybe

0:43:39.480 --> 0:43:43.480
<v Speaker 1>when that person died. And before this, archaeologists had much

0:43:43.520 --> 0:43:46.840
<v Speaker 1>more rudimentary methods. You know, they had this like layer

0:43:46.920 --> 0:43:49.640
<v Speaker 1>method where they would like count down from the ground

0:43:49.680 --> 0:43:52.760
<v Speaker 1>and try to like find things that they knew happened

0:43:52.760 --> 0:43:55.480
<v Speaker 1>that they could use to like sandwich when their relics

0:43:55.680 --> 0:43:58.359
<v Speaker 1>might have been buried. So it was very, very rough.

0:43:58.840 --> 0:44:01.800
<v Speaker 1>And now we have this whittle measure for these objects

0:44:01.840 --> 0:44:05.040
<v Speaker 1>when they died. It's super powerful. It's super powerful. But

0:44:05.080 --> 0:44:07.520
<v Speaker 1>I wonder if there was also a generation of scientists

0:44:07.560 --> 0:44:09.680
<v Speaker 1>who are like, you know, the whole reason I got

0:44:09.680 --> 0:44:12.000
<v Speaker 1>into archaeologies because I don't want to be in the lab,

0:44:12.520 --> 0:44:14.480
<v Speaker 1>and now I have to be in the lab to

0:44:14.520 --> 0:44:16.960
<v Speaker 1>get these dates. But on the other hand, I think

0:44:17.000 --> 0:44:21.080
<v Speaker 1>we all benefit when we get to more accurate, precise information. Yeah,

0:44:21.120 --> 0:44:24.600
<v Speaker 1>I think that's probably true. After this was discovered, very rapidly,

0:44:24.640 --> 0:44:26.760
<v Speaker 1>a bunch of labs were set up around the world

0:44:26.800 --> 0:44:29.480
<v Speaker 1>to start doing radiocarbon dating. So it's not the kind

0:44:29.520 --> 0:44:32.000
<v Speaker 1>of thing that like a typical archaeologist so does in

0:44:32.080 --> 0:44:36.240
<v Speaker 1>the field, or every archaeologist has their own radiocarbon setup.

0:44:36.400 --> 0:44:38.319
<v Speaker 1>It's a little bit of an involved process. What you

0:44:38.360 --> 0:44:41.040
<v Speaker 1>have to do is measure the carbon fourteen ratio. In

0:44:41.080 --> 0:44:42.480
<v Speaker 1>the old days, what they did was just sort of

0:44:42.480 --> 0:44:45.919
<v Speaker 1>like count the radiation emitted because it's emitting beta rays

0:44:46.280 --> 0:44:49.600
<v Speaker 1>when it's decaying. So that was the old strategy. More

0:44:49.640 --> 0:44:53.319
<v Speaker 1>recently they have a more precise strategy which uses mass spectrometer.

0:44:53.480 --> 0:44:56.400
<v Speaker 1>So it takes a sample of it, accelerates it bends

0:44:56.400 --> 0:44:58.960
<v Speaker 1>it through a magnetic field, and then it'll bend more

0:44:59.080 --> 0:45:01.160
<v Speaker 1>if it has low mass ass unless if it has

0:45:01.280 --> 0:45:03.880
<v Speaker 1>high mass. So it gives you like a spectrum of

0:45:03.920 --> 0:45:06.839
<v Speaker 1>the mass of the object that you're sampling, and you

0:45:06.840 --> 0:45:09.760
<v Speaker 1>can tell how much carbon fourteen, how much carbon twelve

0:45:09.840 --> 0:45:11.920
<v Speaker 1>is in there. You don't have to wait for the

0:45:11.960 --> 0:45:14.960
<v Speaker 1>carbon fourteen to decay, so you're getting to take advantage

0:45:14.960 --> 0:45:17.719
<v Speaker 1>of all the carbon fourteen in there, not just the

0:45:17.760 --> 0:45:20.319
<v Speaker 1>ones that happen to be decaying as you're watching. So

0:45:20.320 --> 0:45:23.120
<v Speaker 1>these are pretty specialized techniques now, and I think most

0:45:23.160 --> 0:45:26.520
<v Speaker 1>archaeologists like will send a sample to the lab rather

0:45:26.560 --> 0:45:28.560
<v Speaker 1>than like doing it themselves. So I think you still

0:45:28.600 --> 0:45:31.680
<v Speaker 1>have like old school Indiana Jones types out there in

0:45:31.680 --> 0:45:37.319
<v Speaker 1>the field, gathering stuff, plundering sites, civilization exactly. Oh man,

0:45:37.360 --> 0:45:40.520
<v Speaker 1>the ethics of archaeology not something I want to get into. Yeah,

0:45:40.640 --> 0:45:43.799
<v Speaker 1>nuralistic was science, Yeah, but then sending those samples to

0:45:43.840 --> 0:45:46.040
<v Speaker 1>a lab to do the dating. So you probably have

0:45:46.040 --> 0:45:49.640
<v Speaker 1>like a division. You know, you have the radiocarbon archaeologists

0:45:49.680 --> 0:45:51.160
<v Speaker 1>in the lab and the folks who are not in

0:45:51.200 --> 0:45:54.239
<v Speaker 1>the lab. Okay, well, let's step away from the ethical

0:45:54.320 --> 0:45:59.200
<v Speaker 1>quandaries presented to us by archaeology and talk about dinosaurs.

0:45:59.600 --> 0:46:03.680
<v Speaker 1>So sorry, So we've we've established, unfortunately early on, that

0:46:03.760 --> 0:46:06.640
<v Speaker 1>carbon fourteen is not help for dinosaurs. Is there something

0:46:06.680 --> 0:46:10.000
<v Speaker 1>we can use if we're interested in when a dinosaur bone,

0:46:10.600 --> 0:46:14.400
<v Speaker 1>you know, when the dinosaur died. Dinosaurs are tricky, absolutely,

0:46:14.440 --> 0:46:17.360
<v Speaker 1>because this clock has all run out. All carbon fourteen

0:46:17.400 --> 0:46:20.160
<v Speaker 1>that was in dinosaurs has now decayed. So what you

0:46:20.239 --> 0:46:24.280
<v Speaker 1>need are longer clocks. We did an episode about using

0:46:24.560 --> 0:46:28.640
<v Speaker 1>uranium to date stuff because there's this cool relationship between

0:46:28.760 --> 0:46:32.040
<v Speaker 1>uranium and lead. Uranium two thirty eight and uranium two

0:46:32.040 --> 0:46:35.280
<v Speaker 1>thirty five has half lives of more than a million years,

0:46:35.360 --> 0:46:38.720
<v Speaker 1>and so they're useful for dating stuff that's super duper old.

0:46:38.840 --> 0:46:41.480
<v Speaker 1>And when they form, this cool thing happens. They get

0:46:41.480 --> 0:46:45.600
<v Speaker 1>these zircon crystals zi r c N, And when those

0:46:45.640 --> 0:46:48.799
<v Speaker 1>zircon crystals form, they reject any lead and they like

0:46:48.920 --> 0:46:52.000
<v Speaker 1>expel lead from inside the crystal. So when they're formed,

0:46:52.160 --> 0:46:55.680
<v Speaker 1>they're like lead free, but they do take uranium in them,

0:46:56.040 --> 0:46:59.520
<v Speaker 1>and uranium decays into lead, so each one is like

0:46:59.560 --> 0:47:01.720
<v Speaker 1>a little hawk. Could you pick up a zircon crystal

0:47:01.920 --> 0:47:04.360
<v Speaker 1>and measure how much lead is inside of it, you

0:47:04.360 --> 0:47:07.360
<v Speaker 1>can tell when it was formed. So now we're dating

0:47:07.400 --> 0:47:11.279
<v Speaker 1>like when a rock cooled into these crystals, which is

0:47:11.320 --> 0:47:14.040
<v Speaker 1>pretty cool. That's awesome, And so then you measure in

0:47:14.040 --> 0:47:16.960
<v Speaker 1>the rock around the fossils or something. Yeah, exactly. Now,

0:47:17.120 --> 0:47:20.960
<v Speaker 1>dinosaur bones don't have this stuff in them, but sometimes

0:47:21.000 --> 0:47:24.759
<v Speaker 1>around the dinosaur bones there's like cooled magma, so this

0:47:25.000 --> 0:47:29.360
<v Speaker 1>igneous rock. Because fossils only form in sedimentary rock. But

0:47:29.400 --> 0:47:32.080
<v Speaker 1>if you have like layers of igneous rock above and

0:47:32.160 --> 0:47:35.279
<v Speaker 1>below your fossil, then you can use the zircon crystals

0:47:35.280 --> 0:47:38.480
<v Speaker 1>in those rocks to figure out when those crystals were

0:47:38.520 --> 0:47:41.400
<v Speaker 1>formed and therefore racket your dinosaur bones, so you can

0:47:41.480 --> 0:47:46.240
<v Speaker 1>tell roughly when it must have existed. Yea science. Science.

0:47:46.600 --> 0:47:48.479
<v Speaker 1>I was always puzzled as a kid when people would

0:47:48.480 --> 0:47:50.520
<v Speaker 1>talk about like the age of rocks. I'm like, what

0:47:50.600 --> 0:47:53.080
<v Speaker 1>does that mean? Like when is a rock born? Right,

0:47:53.120 --> 0:47:55.680
<v Speaker 1>it's not. Rock was never alive. And there's only later

0:47:55.719 --> 0:47:58.440
<v Speaker 1>that I understood that they're talking about when the rock cooled.

0:47:58.719 --> 0:48:01.080
<v Speaker 1>Because you have like that block of magma. It was

0:48:01.120 --> 0:48:03.680
<v Speaker 1>still basically rock. It was just like liquid rock. But

0:48:03.680 --> 0:48:06.280
<v Speaker 1>it's when it's cooled into a rock and formed crystal.

0:48:06.480 --> 0:48:09.160
<v Speaker 1>That's what they're interested in. That's what they're measuring. It's

0:48:09.160 --> 0:48:12.120
<v Speaker 1>like saying, how old is my ice cube? Well, you know,

0:48:12.160 --> 0:48:14.680
<v Speaker 1>the water in it has been water forever, but it's

0:48:14.719 --> 0:48:16.239
<v Speaker 1>only been an ice cube since you put it in

0:48:16.239 --> 0:48:19.000
<v Speaker 1>the freezer last Tuesday. So that's like the age of

0:48:19.040 --> 0:48:20.960
<v Speaker 1>your ice cube in the same way. It's a good

0:48:20.960 --> 0:48:23.040
<v Speaker 1>way to explain it. So yeah, that's the story of

0:48:23.120 --> 0:48:27.920
<v Speaker 1>radiocarbon dating, this incredible cool process where clocks are created

0:48:27.960 --> 0:48:30.560
<v Speaker 1>in the upper atmosphere and then drift down into the

0:48:30.600 --> 0:48:34.880
<v Speaker 1>biosphere inhaled by plants eaten by you and then stop

0:48:34.960 --> 0:48:37.920
<v Speaker 1>ticking and as soon as you stop eating and breathing.

0:48:38.080 --> 0:48:40.600
<v Speaker 1>Thanks very much Kelly for joining us on this trip

0:48:40.719 --> 0:48:44.000
<v Speaker 1>into debunking the Shroud of Turn and confirming the Dead

0:48:44.040 --> 0:48:46.680
<v Speaker 1>Sea scrolls. Thanks for bringing me along up the trip.

0:48:46.719 --> 0:48:49.800
<v Speaker 1>I had a great time, all right, and thanks everyone

0:48:49.840 --> 0:48:52.080
<v Speaker 1>for listening, And if you have questions about how something works,

0:48:52.120 --> 0:48:54.480
<v Speaker 1>please don't be shy, right to us to questions at

0:48:54.600 --> 0:49:02.680
<v Speaker 1>Dangel and Jorge dot com. Tune in next time. Bye,

0:49:06.400 --> 0:49:09.200
<v Speaker 1>Thanks for listening, and remember that Daniel and Jorge Explain

0:49:09.280 --> 0:49:13.160
<v Speaker 1>the Universe is a production of iHeartRadio or more podcast

0:49:13.320 --> 0:49:17.200
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0:49:17.320 --> 0:49:19.680
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