WEBVTT - How old is the earth?

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<v Speaker 1>Hey, Daniel, do you keep a family photo album? You know,

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<v Speaker 1>we used to, but these days it's all digital. I

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<v Speaker 1>think Mark Zuckerberg owns all of our family photos. It

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<v Speaker 1>owns your family period. Probably that too. But and how

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<v Speaker 1>do you feel when you look back and see pictures

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<v Speaker 1>of yourself when you were younger? Um? I try to

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<v Speaker 1>ignore all those signs of aging, you know, pretend that

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<v Speaker 1>I looked the same ten or twenty years ago as

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<v Speaker 1>I do today. I see myself as a fine wine

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<v Speaker 1>because you have turned, because I just get more expensive

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<v Speaker 1>the older I get. For some reason. Well, you know,

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<v Speaker 1>I've known you for over ten years or so, and

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<v Speaker 1>I can I can say with confidence for those people

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<v Speaker 1>listening that you are so or no Paul Rudd. Unfortunately

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<v Speaker 1>that's true in many ways, unfortunately. But it is kind

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<v Speaker 1>of interesting how little clues can show you how old

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<v Speaker 1>someone is or how old something is. Right, It's true,

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<v Speaker 1>you know, a few wrinkles here and a few gray

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<v Speaker 1>hairs there, and all of a sudden, you look like

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<v Speaker 1>you're in your midlife crisis. What's that look like a

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<v Speaker 1>look of panic? It's a look of gravitas. I always

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<v Speaker 1>remember how dan Quail died his temples gray and which

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<v Speaker 1>not look so much like a little boy Dan quail Man.

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<v Speaker 1>That's a that's a reference that totally tells everyone how

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<v Speaker 1>old you are. Nobody's fascinating how almost everything around us

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<v Speaker 1>ages right. Everything from people around you, to the rocks

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<v Speaker 1>around you, um to the buildings around you always show

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<v Speaker 1>their signs of age. Nothing in this world is permanent.

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<v Speaker 1>Hi am poor handmade cartoonists and the creator of PhD comics. Hi.

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<v Speaker 1>I'm Daniel. I'm a particle physicist, and I'm young and spry,

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<v Speaker 1>and I have not written any web comics, but I'm

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<v Speaker 1>the co author of the book We Have No Idea

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<v Speaker 1>All about the unknown Questions in the Universe. And welcome

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<v Speaker 1>to our podcast, Daniel and Jorge Explain the Universe, a

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<v Speaker 1>production of I Heart Radio, in which we take weird

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<v Speaker 1>and amazing and young and old stuff in the universe

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<v Speaker 1>and try to explain it to you, and not just

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<v Speaker 1>telling you the answers, but sometimes digging in deeply and

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<v Speaker 1>explaining how we know so that you can explain it

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<v Speaker 1>to skeptical folks around you. Yeah, we try to get

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<v Speaker 1>you to think about the world around you and even

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<v Speaker 1>the world you're standing on right now or sitting on

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<v Speaker 1>or lying down on and one of the depending depending

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<v Speaker 1>on how old you are. But one of the goals

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<v Speaker 1>of this podcast is for you to have sort of

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<v Speaker 1>a new perspective on the world around you. We want

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<v Speaker 1>you to see everything around you as sort of a clue,

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<v Speaker 1>something that can tell you how the world works, that

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<v Speaker 1>can reveal secrets. I can answer questions because almost every

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<v Speaker 1>question we have about the universe, the answers are all

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<v Speaker 1>around us, and it just takes sort of a trained

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<v Speaker 1>mind and a careful eye to see those clues everywhere.

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<v Speaker 1>And so there are clues all around you about where

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<v Speaker 1>we come from and how long we've been here, and

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<v Speaker 1>how long everything has been here? Right, Yeah, exactly. And

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<v Speaker 1>sometimes answers are easy and obvious, and sometimes the answers

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<v Speaker 1>are mind mogglingly surprising. And so today on the podcast,

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<v Speaker 1>we'll be tackling, quite possibly the oldest question on earth.

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<v Speaker 1>Would you say that's true, Daniel, is that who stole

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<v Speaker 1>my dessert? Um? I think the answer is obvious, obviously,

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<v Speaker 1>it's your your children. Well you know, Um, that's actually

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<v Speaker 1>a question my kids asked me today. Um, when was

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<v Speaker 1>dessert invented? It sounds like a topic for a pope,

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<v Speaker 1>you know, if that falls into a physics question. But

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<v Speaker 1>it's sort of a fascinating question, and they were actually

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<v Speaker 1>hypothesizing that dessert might be older than people that maybe,

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<v Speaker 1>like our prehuman ancestors, enjoyed a sweet, sweet treat after dinner.

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<v Speaker 1>What do you think the little bacteria the good that

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<v Speaker 1>well the ocean? They're like, you know, I could use

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<v Speaker 1>a little two remy suit after consuming the other other bacteria.

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<v Speaker 1>I don't know if we have enough in common with

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<v Speaker 1>bacteria to say what they might like, but I can

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<v Speaker 1>imagine it's some pre human homaid, you know, eating some

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<v Speaker 1>berries and going and that goes nicely with my antelope

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<v Speaker 1>or whatever they had for dinner. Well anyway, so so weely. Uh.

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<v Speaker 1>What I mean by it's the oldest question on Earth

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<v Speaker 1>is that it's it's probably really the oldest question that

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<v Speaker 1>could be on Earth, right, Yeah, I think that's probably true,

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<v Speaker 1>And it's a it's an important question, right. It's the

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<v Speaker 1>kind of question that we'd like to dig into because

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<v Speaker 1>it's the kind of question where the answer could change

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<v Speaker 1>the way we think about life and the universe and

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<v Speaker 1>the humanity's rolling it right, it has all sorts of

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<v Speaker 1>things to do with with creation and the context of

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<v Speaker 1>our lives and therefore how we should live our lives

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<v Speaker 1>and whether they have meanings and so to be. On

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<v Speaker 1>the podcast, we'll be tackling the question how old is

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<v Speaker 1>the Earth? And is it even polite to ask? That's right?

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<v Speaker 1>And what does the earth do when he gets upset?

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<v Speaker 1>All right, when he gets offended? Um? And not just

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<v Speaker 1>how old had any worked? One? Has the Earth had

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<v Speaker 1>any work? One? Is it trying to? I think the

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<v Speaker 1>Earth looks great. Doesn't look a day past four billion? Um?

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<v Speaker 1>It is full of buetos. They're probably right, um. And

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<v Speaker 1>just as important as the question how old is the

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<v Speaker 1>Earth and the answer, which is you know, just a number,

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<v Speaker 1>is how do we know? How do we have confidence

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<v Speaker 1>in this answer? Because you know, there are people out

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<v Speaker 1>there who hold beliefs about the various age of the Earth.

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<v Speaker 1>And one of our listeners actually wrote in and said, hey,

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<v Speaker 1>could you tell me how we know the age of

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<v Speaker 1>the Earth, so that when I discussed with my friends

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<v Speaker 1>who have strong opinions about the age of the Earth,

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<v Speaker 1>I can tell them not just what scientists think, but

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<v Speaker 1>how they know it. Yeah, And that's the thing I

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<v Speaker 1>think we always try to do in this podcast, right,

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<v Speaker 1>is try to get at how people know these things,

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<v Speaker 1>not just tell people what scientists know, but how they

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<v Speaker 1>know it. That's right, And that also helps you understand

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<v Speaker 1>with what confidence we know it, Like is this just

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<v Speaker 1>sort of an educated guess the back of the envelope

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<v Speaker 1>calculation or is this something that people have been working

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<v Speaker 1>on for hundreds of years and we have great confidence

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<v Speaker 1>and have it nailed down to like point oh one percent.

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<v Speaker 1>And it's important because different things in science are are

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<v Speaker 1>known well and some things since science are are known

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<v Speaker 1>not very well. So it's important to know how we know. Yeah,

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<v Speaker 1>And so how old is the Earth is the question

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<v Speaker 1>for today, and it's kind of um, I think it's

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<v Speaker 1>a question most people know a little bit about, right.

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<v Speaker 1>I mean, I think everyone knows or has a sense

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<v Speaker 1>that the Earth is very old. Yeah, but you know,

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<v Speaker 1>that sense that the Earth is like extremely old, like

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<v Speaker 1>many orders of magnitude older than you or me or

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<v Speaker 1>your parents, you know, is a fairly modern idea. I

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<v Speaker 1>think thousands of years ago people thought the Earth was

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<v Speaker 1>only hundreds or thousands of years old. They thought it

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<v Speaker 1>might have been created fairly recently, and it was only

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<v Speaker 1>sort of in the eighteen hundreds that people started to

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<v Speaker 1>understand that there were processes around us that we could see,

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<v Speaker 1>specifically rocks and evolutions or geology and biology started to

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<v Speaker 1>give hints that the answer was much much bigger than

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<v Speaker 1>anything anybody had imagined. And I think that's wonderful. I

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<v Speaker 1>I love to live in a scientific era like that,

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<v Speaker 1>where you're where something you thought you knew is upended

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<v Speaker 1>and replaced with a completely different answer. That's like oors

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<v Speaker 1>a magnitude bigger. Wow, is that really true? Like it

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<v Speaker 1>only in the last couple of hundred years do we

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<v Speaker 1>have a sense of how old the Earth really is?

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<v Speaker 1>Before it was totally up in the air. Yeah, it

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<v Speaker 1>was up in the air until about the eighteen hundreds,

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<v Speaker 1>and then people started trying to do calculations and they're like, well,

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<v Speaker 1>how long would it take to form a planet, you know,

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<v Speaker 1>so you gathered it together with gravity, or you know,

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<v Speaker 1>how how long would it take to lay down layers

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<v Speaker 1>of rock? You know, how long would it take glaciers

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<v Speaker 1>to this kind of stuff? And you know, geology is

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<v Speaker 1>a fairly young field and that you know, it's a

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<v Speaker 1>couple of hundred years old and so people started to

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<v Speaker 1>look around, and as soon as they started to explore

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<v Speaker 1>these geological processes, they realized, wow, this stuff takes a

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<v Speaker 1>long time. And you know, it's sort of like um

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<v Speaker 1>walking into a room and seeing somebody has written a

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<v Speaker 1>book that's like five million pages long, and you're like, wow,

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<v Speaker 1>you've been in this room a long time, you know,

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<v Speaker 1>so it shocks you into realizing the things things are

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<v Speaker 1>a much different scale than you imagined. And that's the

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<v Speaker 1>we've seen the story the earth all around us. We

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<v Speaker 1>realize it's staggeringly long, much longer than we imagined, and that, yeah,

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<v Speaker 1>that's a fairly new idea. Yeah, that's a lot of

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<v Speaker 1>party you've missed exactly we should. Things have been around

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<v Speaker 1>for a long time. Do you have a fear of

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<v Speaker 1>missing out? There? Is that fomo about what happened? All

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<v Speaker 1>the good desserts? Fear of being in parties? Actually, to

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<v Speaker 1>be honest, what about all the desserts? The usually have

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<v Speaker 1>good dessertsive party old desserts or I just like I

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<v Speaker 1>just like a fine dessert. Wine? So you should you

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<v Speaker 1>show U at the beginning of the party, how the

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<v Speaker 1>desserts drink the wine and then go home? That's how

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<v Speaker 1>you know you're old or that was like a good

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<v Speaker 1>party to me. That is how your age old track exactly.

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<v Speaker 1>That's very age appropriate. Um. The beginning of this field

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<v Speaker 1>like becoming scientific before that was just speculation of the

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<v Speaker 1>beginning of the field. Becoming scientific was in the eighteen hundreds. Um.

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<v Speaker 1>But still that's very inaccurate. Like looking at rocks gives

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<v Speaker 1>you clues about the sort of order of magnitude, But

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<v Speaker 1>then people wanted to know very precisely, and that took

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<v Speaker 1>that took some time to to like basically defined clocks

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<v Speaker 1>inside the earth, clocks that have been ticking since it

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<v Speaker 1>was born. And that's in the end signs of aging, Yeah,

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<v Speaker 1>signs of aging, very precise signs of aging that could

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<v Speaker 1>tell us how old the earth was. So you're saying, like,

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<v Speaker 1>you know, the people who started the United States, like

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<v Speaker 1>the founding father fathers, like the Founding Fathers, they had

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<v Speaker 1>no idea how old we've been around, Like did they

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<v Speaker 1>think we've been around for a few thousand years? For

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<v Speaker 1>a few but didn't they know about the you know,

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<v Speaker 1>like ancient Egypt and things like that. Yeah, but you

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<v Speaker 1>know that's thousands of years, and so I think they

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<v Speaker 1>had the idea that the Earth was, you know, thousands,

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<v Speaker 1>many thousands of years old, right, because that's as long

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<v Speaker 1>as written history is, and so they imagine it's on

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<v Speaker 1>that time scale because that's the oldest thing, you know.

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<v Speaker 1>And that's basically the game is like find the oldest

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<v Speaker 1>thing you know and then assume that that's basically the

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<v Speaker 1>age of the world, right, And that's frankly what we're

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<v Speaker 1>still doing, um, except that we think that we found

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<v Speaker 1>stuff that comes from the very beginning of the world.

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<v Speaker 1>But you know, they knew about stuff that was thousands

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<v Speaker 1>of years old, so they had no reason to believe

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<v Speaker 1>that the Earth might be millions or even God forbid,

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<v Speaker 1>billions of years old, right. Plus I think those guys

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<v Speaker 1>are pretty religious, all right. So it is an age

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<v Speaker 1>old question and one that a lot of people have

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<v Speaker 1>had answers to and seems seemed to have answers to.

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<v Speaker 1>But we were wondering what people out there right now

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<v Speaker 1>in the world think about this question. Yeah, and this

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<v Speaker 1>is one this is a set of interviews. I was

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<v Speaker 1>very curious to see what people thought. I was wondering

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<v Speaker 1>if I would run into some sort of young Earth

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<v Speaker 1>folks who thought the Earth was from biblical ages and uh,

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<v Speaker 1>and even those people who were scientific. I was wondering, like,

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<v Speaker 1>how precisely do people know the age of the Earth.

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<v Speaker 1>So this I was very fascinating to hear the answers

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<v Speaker 1>like is it a million years, a bazillion years, twenty

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<v Speaker 1>seven point two bazillion? And so, as usual, Daniel went

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<v Speaker 1>out and asked people on the street how old they

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<v Speaker 1>thought the Earth was. So think about it for a second.

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<v Speaker 1>If you ran into a physicist in the street, uh today,

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<v Speaker 1>how would you answer this question? And no googling. Well,

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<v Speaker 1>here's what people had to say. Um, I have no

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<v Speaker 1>idea probably billion years. I don't exactly, but my understanding

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<v Speaker 1>is it's a couple of hundred million years old. Okay,

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<v Speaker 1>you know how we know? So I don't actually like

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<v Speaker 1>my my physics knowledge is pretty limited. Um. I think

0:11:54.600 --> 0:11:58.280
<v Speaker 1>like we've used carbon dating to date things within various

0:11:58.280 --> 0:12:02.120
<v Speaker 1>geological epox but I don't actually know how we arrived

0:12:02.160 --> 0:12:06.880
<v Speaker 1>at the calculation of the Earth stage and maybe three

0:12:06.960 --> 0:12:14.920
<v Speaker 1>billion years, tens of million years, four billion years, and

0:12:14.960 --> 0:12:18.160
<v Speaker 1>how do we know rock formation? It's probably like millions

0:12:18.160 --> 0:12:20.760
<v Speaker 1>of years old. I feel like, all right, Um, a

0:12:20.800 --> 0:12:24.080
<v Speaker 1>lot of millions and billions, right, yeah, exactly, not not

0:12:24.200 --> 0:12:26.160
<v Speaker 1>a whole lot of really specific answers. I have to

0:12:26.160 --> 0:12:28.840
<v Speaker 1>say I was a little bit disappointed. I guess I

0:12:28.880 --> 0:12:31.080
<v Speaker 1>thought people were more interested in this, Like I remember

0:12:31.120 --> 0:12:33.440
<v Speaker 1>wanting to know this number as precisely as possible when

0:12:33.480 --> 0:12:36.120
<v Speaker 1>I was a kid. I was really curious about this, um,

0:12:36.200 --> 0:12:37.760
<v Speaker 1>and so I was a little surprised that people were

0:12:37.840 --> 0:12:40.200
<v Speaker 1>just sort of knew it was super old and were

0:12:40.240 --> 0:12:43.360
<v Speaker 1>satisfied and didn't really care about the details. Although I'll

0:12:43.360 --> 0:12:46.760
<v Speaker 1>say every single person here after I asked them the

0:12:46.880 --> 0:12:49.079
<v Speaker 1>question then they did turn around and ask me. They're like, well,

0:12:49.120 --> 0:12:51.520
<v Speaker 1>how old is the Earth? So they wanted to know

0:12:51.679 --> 0:12:54.559
<v Speaker 1>abous just hadn't really spend any time looking it up.

0:12:54.600 --> 0:12:56.920
<v Speaker 1>All right, Well, let's get started on this topic, Daniel

0:12:56.960 --> 0:12:59.040
<v Speaker 1>and so, um. First of all, I think I feel

0:12:59.080 --> 0:13:01.520
<v Speaker 1>like we should define what we mean by the Earth

0:13:02.040 --> 0:13:04.360
<v Speaker 1>by the age of the Earth, right, Like, um, do

0:13:04.400 --> 0:13:07.560
<v Speaker 1>you mean like the the planet, like the ball that

0:13:07.640 --> 0:13:10.760
<v Speaker 1>it's Earth, or the rocks in the Earth, or the

0:13:10.840 --> 0:13:12.720
<v Speaker 1>atoms that are that make up the Earth? What do

0:13:12.720 --> 0:13:14.760
<v Speaker 1>you mean, like what's the age of the Earth. Yeah,

0:13:14.800 --> 0:13:18.040
<v Speaker 1>it turns out that that's a bit of a fuzzy question, right,

0:13:18.120 --> 0:13:21.760
<v Speaker 1>because the Earth has a sort of continuous history. It's

0:13:21.800 --> 0:13:24.920
<v Speaker 1>not like somebody snapped their fingers and boom, there was

0:13:24.960 --> 0:13:28.319
<v Speaker 1>the Earth. And you can start from the clock from then, right, Um,

0:13:28.360 --> 0:13:31.240
<v Speaker 1>that you know of, right, that we know of, that's right, unless,

0:13:31.280 --> 0:13:33.600
<v Speaker 1>of course it was a simulation, which case things is easy.

0:13:34.080 --> 0:13:36.720
<v Speaker 1>But in the case that it wasn't the simulation, we

0:13:36.760 --> 0:13:39.400
<v Speaker 1>have an idea about how the Earth was formed, and

0:13:39.440 --> 0:13:41.120
<v Speaker 1>there's just a lot of stages there, and so you

0:13:41.160 --> 0:13:44.720
<v Speaker 1>have to sort of make an arbitrary definition and into

0:13:44.800 --> 0:13:47.000
<v Speaker 1>like a lot of things in science, you know, Um,

0:13:47.040 --> 0:13:49.080
<v Speaker 1>there's not necessarily a clear and sower. So you just

0:13:49.120 --> 0:13:51.000
<v Speaker 1>define it to be something arbitrary and at least we

0:13:51.040 --> 0:13:53.760
<v Speaker 1>can agree on it. But maybe we should recap sort

0:13:53.760 --> 0:13:55.880
<v Speaker 1>of the brief history of the of the Earth and

0:13:55.880 --> 0:13:58.360
<v Speaker 1>how it was formed, yeah, like how it how it

0:13:58.440 --> 0:14:00.240
<v Speaker 1>came to be. Yeah, And then at some point we're

0:14:00.240 --> 0:14:02.320
<v Speaker 1>gonna say, this is when the earth started, this is

0:14:02.320 --> 0:14:03.839
<v Speaker 1>when the Earth was born. That's right. This is when

0:14:03.840 --> 0:14:06.720
<v Speaker 1>the party began, right, um, Because you know, you invite

0:14:06.720 --> 0:14:08.880
<v Speaker 1>people to party at nine o'clock and then they don't

0:14:08.880 --> 0:14:10.400
<v Speaker 1>show up till ten, and by then you've eating all

0:14:10.400 --> 0:14:14.640
<v Speaker 1>the brownies, um, and parties only really get started at

0:14:14.640 --> 0:14:17.360
<v Speaker 1>one a m. That's right, unless you're in Spain, in

0:14:17.360 --> 0:14:20.160
<v Speaker 1>which cases four am um. But you know, the very

0:14:20.240 --> 0:14:22.920
<v Speaker 1>early history is that we basically started with a huge

0:14:23.280 --> 0:14:25.560
<v Speaker 1>nebula of gas and dust. And this is stuff that's

0:14:25.640 --> 0:14:28.480
<v Speaker 1>left over from the explosions of other stars and just

0:14:28.520 --> 0:14:31.480
<v Speaker 1>gas from the Big Bang. And then of course gravity

0:14:31.520 --> 0:14:33.840
<v Speaker 1>did its thing and it pulls out all that stuff

0:14:33.880 --> 0:14:35.960
<v Speaker 1>together and you get a sun, right, So most of

0:14:35.960 --> 0:14:37.560
<v Speaker 1>the stuff went to the Sun, and then you get

0:14:37.640 --> 0:14:40.440
<v Speaker 1>a disc of stuff that's rotating around the Sun. It's

0:14:40.480 --> 0:14:44.120
<v Speaker 1>like rings around the Sun. And then the gravity pulls

0:14:44.160 --> 0:14:46.960
<v Speaker 1>the stuff in that disc together to turning to turn

0:14:47.040 --> 0:14:50.800
<v Speaker 1>that disc into planets, right, And uh so we think

0:14:50.880 --> 0:14:53.480
<v Speaker 1>that the Solar system started about four and a half

0:14:53.560 --> 0:14:57.720
<v Speaker 1>billion years ago, and it took like a few million

0:14:57.920 --> 0:15:01.040
<v Speaker 1>or a hundred million years to pull all that stuff

0:15:01.040 --> 0:15:04.680
<v Speaker 1>and the disk together into sort of protoplanets. Right. So

0:15:04.720 --> 0:15:06.960
<v Speaker 1>you have this sort of loose collection of stuff that

0:15:07.000 --> 0:15:09.760
<v Speaker 1>gravity is pulled together, and then gravity really gets to

0:15:09.800 --> 0:15:13.200
<v Speaker 1>work and it starts squeezing it and it collects all

0:15:13.200 --> 0:15:15.720
<v Speaker 1>this stuff and the planet heats up and sort of

0:15:15.760 --> 0:15:19.080
<v Speaker 1>melts the metal and you get the iron dropping to

0:15:19.120 --> 0:15:22.640
<v Speaker 1>the core and the crust forming, and so you can

0:15:22.680 --> 0:15:26.000
<v Speaker 1>sort of ask, like, what moment do you count the

0:15:26.120 --> 0:15:28.560
<v Speaker 1>earth forming? Is it like when you have the first

0:15:28.560 --> 0:15:32.360
<v Speaker 1>big cluster of rocks or maybe when it got gravitationally

0:15:32.480 --> 0:15:35.280
<v Speaker 1>heated enough to sort of melt the metals and form

0:15:35.360 --> 0:15:38.240
<v Speaker 1>the core um It's not really very clear. Well, I

0:15:38.240 --> 0:15:41.000
<v Speaker 1>always find this really fascinating because we we talked about

0:15:41.000 --> 0:15:43.880
<v Speaker 1>this the other day, that something like the rings around

0:15:43.880 --> 0:15:47.720
<v Speaker 1>Saturn are only temporary, right, Like at some point those

0:15:47.800 --> 0:15:51.760
<v Speaker 1>rings might turn into little blobs. That's right. Gravity is

0:15:52.000 --> 0:15:55.240
<v Speaker 1>very weak but very very patient, and so it just

0:15:55.360 --> 0:15:57.840
<v Speaker 1>keeps working and you give it enough time, it will

0:15:57.880 --> 0:16:01.120
<v Speaker 1>gather things together. And so this stuff that's orbiting Saturn

0:16:01.200 --> 0:16:04.800
<v Speaker 1>eventually grab gravity will pull it together in two moons.

0:16:05.080 --> 0:16:07.920
<v Speaker 1>Even the asteroid belt, is that at some point gonna

0:16:08.040 --> 0:16:11.080
<v Speaker 1>turn into more planets for our Solar system? Yeah, eventually.

0:16:11.080 --> 0:16:13.280
<v Speaker 1>Gravity it means very slow and those things are mostly

0:16:13.280 --> 0:16:16.520
<v Speaker 1>stable orbits, but eventually that stuff will get pulled together.

0:16:16.840 --> 0:16:19.520
<v Speaker 1>I mean also there's disruption. Right if you just left

0:16:19.520 --> 0:16:22.280
<v Speaker 1>the Solar system all by itself, then yes, eventually you'll

0:16:22.320 --> 0:16:25.640
<v Speaker 1>just gather together into a smaller and smaller number of objects.

0:16:25.680 --> 0:16:28.120
<v Speaker 1>But this disruption from stuff that comes outside, you know

0:16:28.160 --> 0:16:31.800
<v Speaker 1>and comets things from the word cloud. Um even even

0:16:31.840 --> 0:16:35.320
<v Speaker 1>things like supernovas from other solar system can disrupt things

0:16:35.400 --> 0:16:39.360
<v Speaker 1>happening in our solar system. Um. So, But yes, eventually

0:16:39.360 --> 0:16:41.800
<v Speaker 1>gravity will pull all this stuff together. It's really incredible

0:16:42.160 --> 0:16:45.160
<v Speaker 1>what over over these time scales, what gravity can do.

0:16:45.200 --> 0:16:46.840
<v Speaker 1>And that's one of my favorite things. It's just started

0:16:46.840 --> 0:16:51.080
<v Speaker 1>realizing that these processes are really slow, so things must

0:16:51.120 --> 0:16:53.960
<v Speaker 1>have been around for a super long time to make

0:16:54.000 --> 0:16:57.400
<v Speaker 1>it happen, right right, Well, I guess I would maybe

0:16:57.480 --> 0:17:00.160
<v Speaker 1>count that the birth of the Earth is when it

0:17:00.240 --> 0:17:02.840
<v Speaker 1>was form, you know, when all those asteroids and rocks

0:17:02.880 --> 0:17:06.560
<v Speaker 1>out there clumped together into a ball about the size

0:17:06.560 --> 0:17:09.159
<v Speaker 1>of the ball that we have now, like, you know,

0:17:09.200 --> 0:17:11.480
<v Speaker 1>when when it kind of snapped into shape. I would

0:17:11.600 --> 0:17:15.080
<v Speaker 1>maybe count that as the age of when the Earth started. Yeah, yeah,

0:17:15.119 --> 0:17:18.680
<v Speaker 1>and that's totally reasonable. That's totally reasonable. Um. I think

0:17:18.760 --> 0:17:22.000
<v Speaker 1>one common definition is that you measured the age of

0:17:22.000 --> 0:17:24.320
<v Speaker 1>the Earth is sort of the age of the oldest

0:17:24.480 --> 0:17:27.359
<v Speaker 1>rock in the Earth. And then you can ask the question,

0:17:27.359 --> 0:17:29.160
<v Speaker 1>what does it mean for a rock to be old.

0:17:29.200 --> 0:17:31.640
<v Speaker 1>Like you know, a rock is just a gravitational pulled

0:17:31.680 --> 0:17:35.239
<v Speaker 1>together clump of dust. But rocks are are formed right

0:17:35.240 --> 0:17:37.959
<v Speaker 1>there through melt and then they're cooled. And so the

0:17:37.960 --> 0:17:40.760
<v Speaker 1>age of a rock is usually like the last time

0:17:40.800 --> 0:17:43.359
<v Speaker 1>it was melted, right, So it's the time since it

0:17:43.400 --> 0:17:45.720
<v Speaker 1>was last melted, and so a lot of time people

0:17:45.840 --> 0:17:48.320
<v Speaker 1>just like the time that it cooled off, the last

0:17:48.320 --> 0:17:51.120
<v Speaker 1>time it really chilled out. And so you can imagine

0:17:51.160 --> 0:17:53.159
<v Speaker 1>like all these rocks came together, as you said, and

0:17:53.200 --> 0:17:56.120
<v Speaker 1>formed the Earth and got squeezed together and probably melted

0:17:56.400 --> 0:17:59.200
<v Speaker 1>and then cooled right, and the crust at least cooled,

0:17:59.520 --> 0:18:01.359
<v Speaker 1>and so you can asked, like maybe that last moment

0:18:01.400 --> 0:18:04.120
<v Speaker 1>the last moment of cooling of the crust. So the

0:18:04.160 --> 0:18:07.040
<v Speaker 1>age of the oldest cooled rock on the Earth could

0:18:07.080 --> 0:18:09.280
<v Speaker 1>be a definition at the age of the Earth, because otherwise,

0:18:09.280 --> 0:18:11.800
<v Speaker 1>how do you know when these rocks came together? Right?

0:18:12.600 --> 0:18:15.720
<v Speaker 1>Otherwise I don't know unless you have, like you know,

0:18:15.920 --> 0:18:18.919
<v Speaker 1>CCTV of the formation of the Solar system. It's pretty

0:18:18.920 --> 0:18:21.560
<v Speaker 1>hard to pin that down. Or you could say, is

0:18:21.560 --> 0:18:23.359
<v Speaker 1>it well, but you just gave me a number you

0:18:23.400 --> 0:18:25.280
<v Speaker 1>said that it was maybe it took around a hundred

0:18:25.320 --> 0:18:29.240
<v Speaker 1>million years to to form that the ball of the Earth. Yeah,

0:18:29.280 --> 0:18:31.600
<v Speaker 1>that's you know, I said, I said between a few

0:18:31.680 --> 0:18:33.920
<v Speaker 1>and a hundred million years, right, So that's a pretty

0:18:33.920 --> 0:18:36.679
<v Speaker 1>big uncertainty. Um, we don't really know how long it

0:18:36.760 --> 0:18:38.840
<v Speaker 1>took and and what moment do you define, like do

0:18:38.840 --> 0:18:41.840
<v Speaker 1>you needed one more rock? Because you know, caustic stuff

0:18:41.960 --> 0:18:45.000
<v Speaker 1>kept getting added to the Earth, and so some people say, well,

0:18:45.080 --> 0:18:46.720
<v Speaker 1>the age of the Earth is sort of just just

0:18:46.880 --> 0:18:49.200
<v Speaker 1>just call it the age of the Solar System because

0:18:49.200 --> 0:18:51.560
<v Speaker 1>that's pretty close to the age of the Earth. Or

0:18:51.680 --> 0:18:54.320
<v Speaker 1>you could say it's the age of the the oldest

0:18:54.440 --> 0:18:56.760
<v Speaker 1>rock on the Earth. So I think both of those

0:18:56.800 --> 0:18:59.199
<v Speaker 1>are sort of acceptable. And anyway, that's really all we

0:18:59.240 --> 0:19:01.800
<v Speaker 1>can probe and end. What we do is we measured

0:19:01.800 --> 0:19:03.919
<v Speaker 1>the age of the oldest rock we can find on

0:19:03.960 --> 0:19:06.199
<v Speaker 1>the Earth, and we say that's pretty close to the

0:19:06.200 --> 0:19:08.480
<v Speaker 1>age of the Earth. So the time that it formed

0:19:08.480 --> 0:19:11.960
<v Speaker 1>into a ball is kind of in between those two numbers, right, Yeah, exactly,

0:19:12.000 --> 0:19:16.640
<v Speaker 1>it's between when the Solar System formed and when the

0:19:16.640 --> 0:19:21.240
<v Speaker 1>ball that is the Earth started getting crusty. Exactly exactly

0:19:21.240 --> 0:19:24.240
<v Speaker 1>when it started getting crusty and grumpy and eating desserted

0:19:24.320 --> 0:19:28.840
<v Speaker 1>parties and going home early like a teenager. The suwhere

0:19:28.880 --> 0:19:32.280
<v Speaker 1>between conception and teenage years that's when you're born. That's

0:19:32.440 --> 0:19:34.080
<v Speaker 1>that's right. And you know, we have the same question

0:19:34.080 --> 0:19:37.720
<v Speaker 1>about people, right, I wonder about that sometimes. You know, Um,

0:19:38.000 --> 0:19:40.720
<v Speaker 1>how do you count somebody's age if there if somebody

0:19:40.800 --> 0:19:44.280
<v Speaker 1>is born premature, they're older. You know, even then somebody

0:19:44.280 --> 0:19:46.359
<v Speaker 1>who was born it was conceived at the same moment

0:19:46.400 --> 0:19:49.360
<v Speaker 1>but then born at full term. So even the age

0:19:49.359 --> 0:19:52.040
<v Speaker 1>of people is sort of hard to define sometimes. All right, well,

0:19:52.080 --> 0:19:55.200
<v Speaker 1>we've determined, we've determined what we mean by the age

0:19:55.240 --> 0:19:57.360
<v Speaker 1>of the Earth, and so now let's get into how

0:19:57.400 --> 0:20:00.119
<v Speaker 1>we know how old the Earth is and what what

0:20:00.160 --> 0:20:15.200
<v Speaker 1>that means. But first let's take a quick break. Okay,

0:20:15.240 --> 0:20:17.720
<v Speaker 1>so we're defining the age of the Earth is how

0:20:17.800 --> 0:20:23.159
<v Speaker 1>old the oldest rock was formed that we know about

0:20:23.480 --> 0:20:26.440
<v Speaker 1>right on Earth. That's right, exactly. Let's say, so when

0:20:26.440 --> 0:20:29.120
<v Speaker 1>the Earth was like a ball of lava, that doesn't count.

0:20:29.280 --> 0:20:33.119
<v Speaker 1>But once it started solidifying, then we're saying that's when

0:20:33.160 --> 0:20:36.760
<v Speaker 1>the Earth was born. Yeah, exactly, because we're imagining that, Yeah,

0:20:36.800 --> 0:20:39.000
<v Speaker 1>we're imagining that with that the formation, the Earth probably

0:20:39.040 --> 0:20:40.960
<v Speaker 1>melted a lot of the rocks because there was this

0:20:41.040 --> 0:20:44.160
<v Speaker 1>early lava period as you as you mentioned, and so

0:20:44.200 --> 0:20:46.440
<v Speaker 1>as it's cooled down and formed the crust, then it

0:20:46.520 --> 0:20:49.320
<v Speaker 1>made rocks and and it turns out we can figure

0:20:49.320 --> 0:20:52.720
<v Speaker 1>out how old a rocky is, and so that's really

0:20:52.760 --> 0:20:55.080
<v Speaker 1>our best handle in figuring out how old the Earth is.

0:20:55.080 --> 0:20:57.480
<v Speaker 1>And in the end it's a lower bound, right we say, well,

0:20:57.800 --> 0:20:59.800
<v Speaker 1>here's an old, super old rock on the Earth, so

0:20:59.800 --> 0:21:02.399
<v Speaker 1>that Earth must be at least that old, because like

0:21:02.440 --> 0:21:05.440
<v Speaker 1>we've talked about, like you mentioned, like um, trying to

0:21:05.480 --> 0:21:07.960
<v Speaker 1>figure out how old Earth is, the only thing we

0:21:08.000 --> 0:21:10.160
<v Speaker 1>can do is sort of look around and see how

0:21:10.200 --> 0:21:12.359
<v Speaker 1>old the things in it are, right, and like, what's

0:21:12.400 --> 0:21:14.280
<v Speaker 1>the oldest thing in it? We know it has to

0:21:14.280 --> 0:21:17.560
<v Speaker 1>be at least that old. Yeah, yeah, exactly. That's about

0:21:17.600 --> 0:21:19.280
<v Speaker 1>all we can do. And you know what you can

0:21:19.320 --> 0:21:21.840
<v Speaker 1>do otherwise is sort of form of theory. You say,

0:21:21.880 --> 0:21:24.359
<v Speaker 1>I have a concept for how this might have worked,

0:21:24.720 --> 0:21:27.160
<v Speaker 1>and then you can fit data to and say, well,

0:21:27.480 --> 0:21:29.800
<v Speaker 1>I expect you know that to see these sort of

0:21:29.880 --> 0:21:31.560
<v Speaker 1>rocks in that case, and you can use that a

0:21:31.680 --> 0:21:33.680
<v Speaker 1>theory to sort of extrapolate a little bit past the

0:21:33.760 --> 0:21:38.600
<v Speaker 1>day to you you observe. But that's very but that's speculative, right,

0:21:38.600 --> 0:21:40.920
<v Speaker 1>it's based on your concept of how things happen. So

0:21:41.280 --> 0:21:43.919
<v Speaker 1>the hardest number, the one that you know best, is

0:21:43.960 --> 0:21:47.080
<v Speaker 1>the oldest thing that you can find. And the oldest

0:21:47.080 --> 0:21:49.679
<v Speaker 1>thing we find our rocks, and and so what we

0:21:49.720 --> 0:21:52.359
<v Speaker 1>do is we try to turn one question into another question.

0:21:52.400 --> 0:21:54.840
<v Speaker 1>The question we can answer is what's the age of

0:21:54.880 --> 0:21:57.439
<v Speaker 1>the oldest rock on the Earth. Wouldn't that tell us

0:21:57.480 --> 0:22:00.479
<v Speaker 1>like if we found a really old raw, what if

0:22:00.480 --> 0:22:03.359
<v Speaker 1>that rock came from before the Earth was formed? Do

0:22:03.440 --> 0:22:05.800
<v Speaker 1>you know what I mean? Yeah, yeah, there are some

0:22:05.840 --> 0:22:09.600
<v Speaker 1>of those actually, like meteorites, Right, meteorites tell us the

0:22:09.600 --> 0:22:12.760
<v Speaker 1>age of the Solar system because we think meteorites were

0:22:12.800 --> 0:22:15.159
<v Speaker 1>formed in the beginning of the Solar system. Right, the

0:22:15.320 --> 0:22:19.280
<v Speaker 1>first stage is gathered together gas and dust into rocks, right,

0:22:19.760 --> 0:22:22.000
<v Speaker 1>And so those rocks from space tell us the age

0:22:22.000 --> 0:22:25.159
<v Speaker 1>of the Solar System. But we can tell which rocks

0:22:25.200 --> 0:22:28.000
<v Speaker 1>came from space and which rocks are from Earth, And

0:22:28.040 --> 0:22:31.840
<v Speaker 1>so we can distinguish those two. How can we tell? Oh,

0:22:31.920 --> 0:22:35.640
<v Speaker 1>they're clearly labeled. You know, they have their turn address, right,

0:22:35.680 --> 0:22:40.240
<v Speaker 1>it says somewhere near Neptune Um. It's it's actually quite

0:22:40.240 --> 0:22:43.560
<v Speaker 1>interesting that the so the distribution of metals in these

0:22:43.680 --> 0:22:46.719
<v Speaker 1>rocks is very different from meteorites than it is for

0:22:46.920 --> 0:22:50.600
<v Speaker 1>rocks on the Earth. It's like a different group of rocks. Yeah,

0:22:50.600 --> 0:22:52.439
<v Speaker 1>it's like they have more nickel in them where they

0:22:52.440 --> 0:22:55.080
<v Speaker 1>have this other rare stuff. And that's a whole other

0:22:55.119 --> 0:22:58.760
<v Speaker 1>fascinating field. Um. And also, so these rocks are different

0:22:58.800 --> 0:23:00.439
<v Speaker 1>from Earth, and they tell us like what else is

0:23:00.440 --> 0:23:02.440
<v Speaker 1>out there in the Solar System and what was out

0:23:02.440 --> 0:23:04.359
<v Speaker 1>there when the Solar system was formed? There like little

0:23:04.400 --> 0:23:07.320
<v Speaker 1>time capsules from the very beginning of the Solar system.

0:23:07.560 --> 0:23:09.639
<v Speaker 1>And they actually tell us another interesting story. Right, So

0:23:09.720 --> 0:23:12.080
<v Speaker 1>those rocks, we can tell how old they are, and

0:23:12.119 --> 0:23:14.719
<v Speaker 1>they tell us how old the Solar system is. So

0:23:14.760 --> 0:23:16.560
<v Speaker 1>we can answer two questions. We can find a bunch

0:23:16.560 --> 0:23:18.280
<v Speaker 1>of rocks. We can say, oh, these came from somewhere

0:23:18.280 --> 0:23:20.800
<v Speaker 1>in the Solar System. There x y z old. These

0:23:20.920 --> 0:23:23.359
<v Speaker 1>rocks are here on Earth, they're only you know, ABC

0:23:23.520 --> 0:23:25.560
<v Speaker 1>old all right. So then so it all comes down

0:23:25.560 --> 0:23:27.200
<v Speaker 1>to the question of how do you tell how old

0:23:27.240 --> 0:23:30.760
<v Speaker 1>the rock is, yeah, right, exactly exactly, or a meteorite

0:23:30.840 --> 0:23:32.240
<v Speaker 1>which is the same, which is the same because the

0:23:32.280 --> 0:23:34.879
<v Speaker 1>meteorite is just basically a rock from space that landed

0:23:34.920 --> 0:23:36.760
<v Speaker 1>on Earth. And the way we do it is something

0:23:36.800 --> 0:23:41.400
<v Speaker 1>called radiometric dating, which is not the same as carbon dating, right,

0:23:41.960 --> 0:23:43.720
<v Speaker 1>but it works in which is not the same as

0:23:44.000 --> 0:23:47.040
<v Speaker 1>online dating either. It turns out to be actually kind

0:23:47.080 --> 0:23:49.120
<v Speaker 1>of similar. There's a lot of swiping, there's a lot

0:23:49.160 --> 0:23:55.760
<v Speaker 1>of lying about your age as well. Um. No, carbon

0:23:55.880 --> 0:23:58.520
<v Speaker 1>dating and radio metric dating have similar principles, and we

0:23:58.520 --> 0:24:01.000
<v Speaker 1>should have a whole podcast episode of how carbon dating works.

0:24:01.000 --> 0:24:05.480
<v Speaker 1>Carbondating relates to organic stuff like living beings. Radiometric dating

0:24:05.640 --> 0:24:08.679
<v Speaker 1>relates to how how old rocks are. Okay, so you

0:24:08.720 --> 0:24:11.000
<v Speaker 1>find a rock and you're you're staring at it, and

0:24:11.000 --> 0:24:14.040
<v Speaker 1>you're like, I wonder when this rock became a rock? Yeah,

0:24:14.080 --> 0:24:18.240
<v Speaker 1>exactly when this turn from lava to this heavy thing

0:24:18.359 --> 0:24:21.320
<v Speaker 1>that I'm holding, And so you can we can actually tell, right,

0:24:21.400 --> 0:24:23.120
<v Speaker 1>we can look at the stuff in it and tell

0:24:23.119 --> 0:24:26.119
<v Speaker 1>how old window was formed, how many millions of years

0:24:26.160 --> 0:24:30.320
<v Speaker 1>ago exactly? And I have so much respect for scientists

0:24:30.480 --> 0:24:32.480
<v Speaker 1>who develop these techniques. You know, they look at the

0:24:32.560 --> 0:24:34.360
<v Speaker 1>rock and they say, I want to know how old

0:24:34.400 --> 0:24:37.200
<v Speaker 1>this rock is. How could I tell? Can I find

0:24:37.280 --> 0:24:40.280
<v Speaker 1>something inside the rock that I can use as a clock,

0:24:40.640 --> 0:24:44.600
<v Speaker 1>something which changes reliably and steadily every year, so that

0:24:44.640 --> 0:24:47.800
<v Speaker 1>I can count it and and project back and figure

0:24:47.840 --> 0:24:50.840
<v Speaker 1>out when that clock started or something. And this is

0:24:50.880 --> 0:24:53.240
<v Speaker 1>hard to do, you know. You have to find something

0:24:53.280 --> 0:24:57.160
<v Speaker 1>which is steady and reliable and can be calibrated. Um,

0:24:57.200 --> 0:24:59.520
<v Speaker 1>it's not trivial, right. You can't just say, oh, I'm

0:24:59.560 --> 0:25:01.560
<v Speaker 1>just gonna your X Y Z property. You have to

0:25:01.640 --> 0:25:05.000
<v Speaker 1>invent these techniques. And it takes time and sweat and tears,

0:25:05.359 --> 0:25:08.199
<v Speaker 1>and so I have so much respect for folks who

0:25:08.280 --> 0:25:10.240
<v Speaker 1>did this. And and in the case of rocks, it

0:25:10.240 --> 0:25:12.200
<v Speaker 1>turns out to be very dependent on the special kind

0:25:12.240 --> 0:25:18.560
<v Speaker 1>of mineral called zircon. Zircon like the fake diamond like, yeah,

0:25:18.560 --> 0:25:22.120
<v Speaker 1>it's related exactly. Zirconium and zircon is a special kind

0:25:22.160 --> 0:25:26.320
<v Speaker 1>of mineral. And it's special because it has two properties. One,

0:25:26.840 --> 0:25:29.720
<v Speaker 1>it likes it's a crystal, and it likes to absorb

0:25:29.880 --> 0:25:32.720
<v Speaker 1>uranium into it right, gobbles up uranium. So when the

0:25:32.800 --> 0:25:35.920
<v Speaker 1>rock forms, if it has some zircon, then it will

0:25:35.960 --> 0:25:39.919
<v Speaker 1>grab any uranium that's around it. And the second important property,

0:25:40.000 --> 0:25:42.320
<v Speaker 1>but wait, what is zircon made out of? Is it?

0:25:42.680 --> 0:25:45.560
<v Speaker 1>What is it like a made out of iron or

0:25:45.720 --> 0:25:48.679
<v Speaker 1>what is it carbon? What is this mineral made out

0:25:48.680 --> 0:25:52.960
<v Speaker 1>of it? I think it's made out of leftover desserts. No,

0:25:53.119 --> 0:25:58.160
<v Speaker 1>it's it's a mineral um. It's made out of zirconium

0:25:58.440 --> 0:26:03.040
<v Speaker 1>and silicon and oxygen. Oh Sirgonium is like an element

0:26:03.280 --> 0:26:07.119
<v Speaker 1>like carbon or irn. Yes, Zirconium is an element, and

0:26:07.200 --> 0:26:10.760
<v Speaker 1>it's sort of like a silver metal. It's atomic number forty.

0:26:10.960 --> 0:26:12.720
<v Speaker 1>It's you know, it doesn't really play a lot of

0:26:12.800 --> 0:26:15.119
<v Speaker 1>roles and stuff other than like cubics urconium. It's not

0:26:15.240 --> 0:26:17.200
<v Speaker 1>like a famous metal like some of its friends and

0:26:17.280 --> 0:26:21.200
<v Speaker 1>neighbors um, but it plays an important role in aging rocks.

0:26:21.240 --> 0:26:23.840
<v Speaker 1>So this element is all around us and to all

0:26:23.880 --> 0:26:26.840
<v Speaker 1>the rocks, and it forms a special crystal. You're saying

0:26:27.760 --> 0:26:31.640
<v Speaker 1>that when it forms, it likes to capture or uranium.

0:26:31.640 --> 0:26:34.600
<v Speaker 1>That's right. It captures uranium and it really rejects lead.

0:26:34.960 --> 0:26:37.880
<v Speaker 1>So the moment that the rock is created, it creates

0:26:37.880 --> 0:26:41.159
<v Speaker 1>a special thing, which is zircon with just uranium in it.

0:26:41.359 --> 0:26:44.960
<v Speaker 1>And you might wonder like, well, how is that helpful? Right? Well, uranium,

0:26:44.960 --> 0:26:47.600
<v Speaker 1>as you might know, is radioactive. It doesn't just sit

0:26:47.640 --> 0:26:52.159
<v Speaker 1>around and stay uranium forever. It very reliably decays and

0:26:52.200 --> 0:26:55.160
<v Speaker 1>it decays into lead. But wait, why does the durk

0:26:55.280 --> 0:26:58.840
<v Speaker 1>circon like uranium and white, doesn't it? You mean, like

0:26:58.840 --> 0:27:01.200
<v Speaker 1>when it forms the crystal les, it forms a little

0:27:01.240 --> 0:27:05.119
<v Speaker 1>structure and it just it just likes uranium like uranium

0:27:05.160 --> 0:27:07.760
<v Speaker 1>likes being inside of zircon crystal. I mean, I don't

0:27:07.760 --> 0:27:09.439
<v Speaker 1>want to get in the mind of uranium on the

0:27:09.440 --> 0:27:12.520
<v Speaker 1>mind of zircon. I mean, they did some carbon dating

0:27:12.680 --> 0:27:16.320
<v Speaker 1>online and they decided they were a good match. Um,

0:27:16.359 --> 0:27:19.240
<v Speaker 1>but no, there's some chemical some business with the chemical bonds.

0:27:19.240 --> 0:27:22.199
<v Speaker 1>You know, the way the crystal structure of zircon forms

0:27:22.560 --> 0:27:25.760
<v Speaker 1>fits very nicely with uranium and doesn't fit very nicely

0:27:25.760 --> 0:27:29.320
<v Speaker 1>with lead. Right, Yeah, So like a rock, you have

0:27:29.359 --> 0:27:32.000
<v Speaker 1>a have a bunch of lava and it cools and

0:27:32.040 --> 0:27:34.960
<v Speaker 1>it slowly turns into rock. And in that process is

0:27:34.960 --> 0:27:37.639
<v Speaker 1>when you you're saying this crystal form, yeah, and zirkon

0:27:37.800 --> 0:27:39.280
<v Speaker 1>is it doesn't have to be all over the rock.

0:27:39.320 --> 0:27:40.960
<v Speaker 1>It's not like a whole rock full of zirkon. It

0:27:41.040 --> 0:27:43.919
<v Speaker 1>is just these little chips of zircon. And what they

0:27:43.960 --> 0:27:46.040
<v Speaker 1>do is they repel all the lead inside them and

0:27:46.040 --> 0:27:50.040
<v Speaker 1>they grab some uranium and your uranium is like a clock.

0:27:50.440 --> 0:27:54.000
<v Speaker 1>It decays very reliably. So every million years or so,

0:27:54.080 --> 0:27:58.800
<v Speaker 1>some uranium turns into lead. And so after one million years,

0:27:59.080 --> 0:28:02.240
<v Speaker 1>some fraction the uranium and then zircon has turned into lead.

0:28:02.600 --> 0:28:06.040
<v Speaker 1>After two million years, another fraction has turned into lead.

0:28:06.160 --> 0:28:09.760
<v Speaker 1>After a billion years, a very predictable fraction is turned

0:28:09.800 --> 0:28:12.200
<v Speaker 1>into lead. So what you do is you take a rock,

0:28:12.600 --> 0:28:15.480
<v Speaker 1>you look at that, you find some zircon crystals, and

0:28:15.520 --> 0:28:18.280
<v Speaker 1>you ask how much of the uranium has turned into lead,

0:28:18.320 --> 0:28:20.720
<v Speaker 1>and that tells you how much time it's had to

0:28:20.840 --> 0:28:23.360
<v Speaker 1>turn into lead. It's kind of like a like an

0:28:23.359 --> 0:28:26.320
<v Speaker 1>aging process, right like wine. If you leave wine there,

0:28:26.400 --> 0:28:31.520
<v Speaker 1>it's gonna change, it's characteristic, it's gonna change into something

0:28:31.520 --> 0:28:33.880
<v Speaker 1>else exactly, and you need something. That's why it works

0:28:33.880 --> 0:28:35.760
<v Speaker 1>so well as a clock, because uranium is something that

0:28:35.800 --> 0:28:38.400
<v Speaker 1>we know reliably. We understand it, We know how it decays,

0:28:38.480 --> 0:28:40.280
<v Speaker 1>we know how long it takes, we know, you know,

0:28:41.240 --> 0:28:44.400
<v Speaker 1>after a hundred thousand years, what fraction of uranium atoms

0:28:44.400 --> 0:28:46.600
<v Speaker 1>will turn into lead. And the other key thing, of

0:28:46.640 --> 0:28:49.000
<v Speaker 1>course is that it starts with a blank slate. That

0:28:49.080 --> 0:28:51.959
<v Speaker 1>when you form these zircon crystals, it rejects lead. Right,

0:28:52.040 --> 0:28:54.520
<v Speaker 1>So you start out like with an empty bucket, and

0:28:54.520 --> 0:28:58.080
<v Speaker 1>then slowly the uranium bucket fills the lead bucket. And

0:28:58.080 --> 0:29:00.600
<v Speaker 1>so you can just measure the uranium lead fraction and

0:29:00.640 --> 0:29:04.120
<v Speaker 1>that tells you how long the uranium has been turning

0:29:04.120 --> 0:29:06.959
<v Speaker 1>into lead. It's really amazing. It's it's really just chance

0:29:07.040 --> 0:29:09.480
<v Speaker 1>that this happens, that somebody figured this out. So like

0:29:09.520 --> 0:29:11.800
<v Speaker 1>if you find a rock and you find a little

0:29:12.200 --> 0:29:16.360
<v Speaker 1>little zircon chip inside of it, and it's like, let's

0:29:16.360 --> 0:29:18.400
<v Speaker 1>say it's full of uranium, then you know it's a

0:29:18.440 --> 0:29:21.040
<v Speaker 1>pretty new rock exactly. But if it's full of lead,

0:29:21.080 --> 0:29:24.160
<v Speaker 1>then you know it's really old rock exactly. It's exactly right.

0:29:24.480 --> 0:29:28.400
<v Speaker 1>So rock start start out pure uranium, no lead, and

0:29:28.440 --> 0:29:31.400
<v Speaker 1>then as they age, the uranium turns into lead. And

0:29:31.440 --> 0:29:34.040
<v Speaker 1>so a rock with almost no uranium is going to

0:29:34.120 --> 0:29:37.920
<v Speaker 1>be like super duper old, right, And new lead can't

0:29:38.040 --> 0:29:40.800
<v Speaker 1>just like come in from the outside because now it's crystallized, right,

0:29:41.280 --> 0:29:43.800
<v Speaker 1>It's hard for lead to get in any other way.

0:29:44.000 --> 0:29:45.720
<v Speaker 1>All the only way you can get lead inside the

0:29:45.760 --> 0:29:48.840
<v Speaker 1>zircon is for uranium to turn into lead. So the

0:29:49.160 --> 0:29:51.840
<v Speaker 1>rock sort of you might say like it's spoils or

0:29:52.200 --> 0:29:56.160
<v Speaker 1>ages by looking at that. Yeah, like you, it turns

0:29:56.160 --> 0:29:59.760
<v Speaker 1>into lead right exactly, And whether it's spoils or ages

0:29:59.800 --> 0:30:02.160
<v Speaker 1>be to fully depends on you know, your preference for

0:30:02.240 --> 0:30:04.720
<v Speaker 1>how rocks taste. I suppose whether you swipe right or

0:30:04.800 --> 0:30:07.080
<v Speaker 1>left for rocks. But you know, it took a long

0:30:07.120 --> 0:30:10.040
<v Speaker 1>time to figure this out. People tried all sorts of

0:30:10.080 --> 0:30:13.000
<v Speaker 1>other strategies first before they discovered this one. And there's

0:30:13.160 --> 0:30:16.200
<v Speaker 1>lots of scientific careers and pH d PCs that were

0:30:16.240 --> 0:30:18.640
<v Speaker 1>frustrated in people trying to figure out a way to

0:30:18.680 --> 0:30:22.440
<v Speaker 1>do radiometric dating before people stumbled onto this one. Wow,

0:30:22.480 --> 0:30:24.120
<v Speaker 1>and this is not one of these things that you

0:30:24.400 --> 0:30:27.920
<v Speaker 1>um have to calibrate, right because I imagine you have

0:30:28.120 --> 0:30:35.880
<v Speaker 1>probably very scientific information about the decay of uranium, right like,

0:30:35.880 --> 0:30:39.320
<v Speaker 1>it's very physics space like. You don't have to calibrate

0:30:39.360 --> 0:30:41.280
<v Speaker 1>it to anything else, do you. You're right, And we

0:30:41.320 --> 0:30:44.920
<v Speaker 1>can basically use simple physics arguments to argue how long

0:30:45.040 --> 0:30:47.880
<v Speaker 1>uranium takes to decay and to lead and uh, and

0:30:47.920 --> 0:30:51.360
<v Speaker 1>so it gives us pretty clear descriptions, but you know,

0:30:51.440 --> 0:30:54.760
<v Speaker 1>we also want to get confidence in it, and so

0:30:54.800 --> 0:30:58.280
<v Speaker 1>what people do to have various other sort of radiometric

0:30:58.360 --> 0:31:01.600
<v Speaker 1>methods not just uranium to lead, but other stuff, things

0:31:01.640 --> 0:31:04.600
<v Speaker 1>that decay faster, things that decay slower, and so you

0:31:04.640 --> 0:31:07.600
<v Speaker 1>can use those to sort of cross calibrate, but uranium

0:31:07.640 --> 0:31:10.120
<v Speaker 1>to let this sort of the cleanest one. But you know,

0:31:10.160 --> 0:31:12.160
<v Speaker 1>like everywhere in science, you want to check everything three

0:31:12.160 --> 0:31:15.240
<v Speaker 1>different ways, um and then make sure you get consistent answers.

0:31:15.400 --> 0:31:17.520
<v Speaker 1>All right, that's pretty cool. That's how we can tell

0:31:17.560 --> 0:31:21.520
<v Speaker 1>how old the rock is. Man, rock can't lie. I

0:31:21.600 --> 0:31:24.840
<v Speaker 1>can't lie about its age. That's right, that's right. You

0:31:24.880 --> 0:31:27.120
<v Speaker 1>can lie, but we'll know you are. All right, Let's

0:31:27.120 --> 0:31:29.400
<v Speaker 1>get into the answer now, Daniel, how old Earth is

0:31:29.480 --> 0:31:32.560
<v Speaker 1>and how old the Solar system is. But first let's

0:31:32.720 --> 0:31:48.840
<v Speaker 1>take another quick break. All right, Daniel, Let's let's break

0:31:48.880 --> 0:31:52.120
<v Speaker 1>it down for people. How old is the Earth, or

0:31:52.480 --> 0:31:55.480
<v Speaker 1>at least the oldest rocks on Earth. The oldest rocks

0:31:55.480 --> 0:31:57.920
<v Speaker 1>on Earth come from Australia. And I don't know why,

0:31:57.960 --> 0:32:00.440
<v Speaker 1>but that's not surprising to me. It seems like Australia

0:32:00.520 --> 0:32:04.120
<v Speaker 1>is the land of extremes, and so you expect the craziest, weirdest,

0:32:04.120 --> 0:32:07.760
<v Speaker 1>oldest rock to be in Australia. And they have the

0:32:07.760 --> 0:32:12.520
<v Speaker 1>biggest spiders, the biggest crocodiles and the oldest rocks, the

0:32:12.560 --> 0:32:16.880
<v Speaker 1>deadliest everything, the biggest, best stars and the best podcast

0:32:16.920 --> 0:32:19.360
<v Speaker 1>listening fans. Right. Um, you know, we've got a lot

0:32:19.400 --> 0:32:22.000
<v Speaker 1>of good email questions from Australia. But the oldest rock

0:32:22.040 --> 0:32:24.960
<v Speaker 1>on Earth come from the jack Hills of Australia and

0:32:25.000 --> 0:32:29.040
<v Speaker 1>it's four point zero four billion years old. So these

0:32:29.040 --> 0:32:31.719
<v Speaker 1>are rocks that we do we have to dig up

0:32:31.720 --> 0:32:34.040
<v Speaker 1>for them, dig for them or are they were they

0:32:34.440 --> 0:32:37.520
<v Speaker 1>pretty close to the surface or yeah, it's it's fascinating.

0:32:37.520 --> 0:32:40.040
<v Speaker 1>Actually these rocks just sort of sit on outcrops and

0:32:40.160 --> 0:32:43.600
<v Speaker 1>people recently discovered that they have that the oldest rocks

0:32:43.600 --> 0:32:46.880
<v Speaker 1>are there, and you know it's um. The Earth itself,

0:32:46.920 --> 0:32:49.840
<v Speaker 1>of course, has had lots of geologic activity and so

0:32:49.920 --> 0:32:52.200
<v Speaker 1>some of these really old rocks get buried and then

0:32:52.240 --> 0:32:54.560
<v Speaker 1>there's geological activity that brings them up to the surface,

0:32:54.800 --> 0:32:57.320
<v Speaker 1>and so it just happens to be at this spot

0:32:57.400 --> 0:33:00.600
<v Speaker 1>on the Earth, these really old rocks got pushed up

0:33:00.680 --> 0:33:02.960
<v Speaker 1>and so they're not that far underground there on these

0:33:02.960 --> 0:33:06.160
<v Speaker 1>outcropping of rocks in Western Australia, but you almost kind

0:33:06.160 --> 0:33:08.200
<v Speaker 1>of expect them to be close to the surface, right,

0:33:08.240 --> 0:33:11.280
<v Speaker 1>because that's you know, I would imagine that if we

0:33:11.280 --> 0:33:13.760
<v Speaker 1>were once a ball of lava, then the stuff sort

0:33:13.800 --> 0:33:16.360
<v Speaker 1>of cools from the outside inwards. That's true. But you know,

0:33:16.360 --> 0:33:20.360
<v Speaker 1>then there's all these sedimentary processes where old things get buried. Um.

0:33:20.440 --> 0:33:22.760
<v Speaker 1>But then there's tectonic activity and all sorts of other

0:33:22.800 --> 0:33:26.360
<v Speaker 1>crazy stuff that brings stuff up and mixes everything around. Um.

0:33:26.480 --> 0:33:27.840
<v Speaker 1>And so there's a lot of stuff going on there.

0:33:27.840 --> 0:33:30.120
<v Speaker 1>I think it's not that not that simple. Um. But

0:33:30.200 --> 0:33:32.280
<v Speaker 1>in the end, the oldest thing we found on Earth

0:33:32.720 --> 0:33:35.520
<v Speaker 1>is uh, is almost four and a half billion years old.

0:33:35.680 --> 0:33:39.120
<v Speaker 1>Is four billion, four hundred and four million years old.

0:33:39.520 --> 0:33:41.600
<v Speaker 1>And you know, that's a staggering answer. It's hard to

0:33:41.640 --> 0:33:46.680
<v Speaker 1>really comprehend what that means. For billion years old, that's

0:33:47.240 --> 0:33:49.840
<v Speaker 1>a lot. It's a it's a lot of dessert parties. Yeah,

0:33:49.880 --> 0:33:53.440
<v Speaker 1>I mean, if theysed, a lot of party missed. Yeah.

0:33:53.600 --> 0:33:55.239
<v Speaker 1>I think I think what you said earlier about how

0:33:55.240 --> 0:33:58.040
<v Speaker 1>we came to the party pretty late. It's sort of shocking.

0:33:58.080 --> 0:34:00.000
<v Speaker 1>You know, the first people to like learn these number,

0:34:00.000 --> 0:34:02.520
<v Speaker 1>first to know that the Earth was billions of years old,

0:34:02.880 --> 0:34:05.960
<v Speaker 1>it must have made humans feel sort of small and

0:34:06.040 --> 0:34:09.719
<v Speaker 1>recent and uh. And you know, maybe transient tried like

0:34:10.040 --> 0:34:11.960
<v Speaker 1>the Earth has had a long history and we are

0:34:12.000 --> 0:34:14.239
<v Speaker 1>only the very last little bit of it. Yeah. I

0:34:14.239 --> 0:34:17.439
<v Speaker 1>mean it's a difference between I mean human histories maybe

0:34:17.560 --> 0:34:20.440
<v Speaker 1>what like ten thousand two years old? Yeah, a hundred

0:34:20.440 --> 0:34:24.080
<v Speaker 1>thousand if you're really generous. Yeah, but the Earth has

0:34:24.080 --> 0:34:27.680
<v Speaker 1>been around for four point four billion years old exactly.

0:34:28.040 --> 0:34:30.360
<v Speaker 1>It's not too impressed. It's been there, It's seen a

0:34:30.360 --> 0:34:33.839
<v Speaker 1>lot of stuff. You know, it'll be here, remember done. Um.

0:34:33.920 --> 0:34:35.560
<v Speaker 1>You know, people always talk about how humans are going

0:34:35.600 --> 0:34:38.200
<v Speaker 1>to destroy the Earth, and uh, I don't think that's likely.

0:34:38.400 --> 0:34:41.799
<v Speaker 1>I think the humans might destroy ourselves or life on Earth,

0:34:41.880 --> 0:34:44.640
<v Speaker 1>but the Earth will be here when we're done. Unless

0:34:45.160 --> 0:34:47.120
<v Speaker 1>I hear some physics are trying to make black holes

0:34:47.360 --> 0:34:49.840
<v Speaker 1>down at the Large Mattern Collider. Yeah, but we just

0:34:49.840 --> 0:34:52.640
<v Speaker 1>want to understand the universe. Man, We're not threatening the world.

0:34:52.840 --> 0:34:55.360
<v Speaker 1>There's no danger there. Trust me, And can I have

0:34:55.400 --> 0:34:59.080
<v Speaker 1>ten more billion dollars to build a bigger one one

0:34:59.160 --> 0:35:02.399
<v Speaker 1>year for every one daughter, for every year that the earth?

0:35:03.440 --> 0:35:05.719
<v Speaker 1>That's right, That sounds good. Um, But you know, that's

0:35:05.719 --> 0:35:08.439
<v Speaker 1>the oldest rock on Earth that we think is part

0:35:08.560 --> 0:35:11.120
<v Speaker 1>of the Earth. It was part of the formation of

0:35:11.160 --> 0:35:13.360
<v Speaker 1>the Earth. But of course we have found rocks on

0:35:13.440 --> 0:35:16.480
<v Speaker 1>Earth that are meteorites, right, they came from space that

0:35:16.560 --> 0:35:19.920
<v Speaker 1>are older than the Earth itself. So late comers to

0:35:19.960 --> 0:35:22.080
<v Speaker 1>the party, that's right. They heard there was something cool

0:35:22.120 --> 0:35:24.120
<v Speaker 1>happening down here in the third rock from the Sun,

0:35:24.239 --> 0:35:26.640
<v Speaker 1>and they they've fell on in to figure it out.

0:35:27.040 --> 0:35:31.320
<v Speaker 1>And those rocks are four point five six billion years old,

0:35:31.840 --> 0:35:35.200
<v Speaker 1>So that's like a hundred and fifty million years older

0:35:35.239 --> 0:35:38.239
<v Speaker 1>than the oldest rocks on Earth. That's the oldest meteorite

0:35:38.280 --> 0:35:40.759
<v Speaker 1>that we found. And I think that you were saying

0:35:40.760 --> 0:35:43.719
<v Speaker 1>that that kind of tells us what the oldest media

0:35:44.080 --> 0:35:46.600
<v Speaker 1>right at all is in our solar system, right, Yeah,

0:35:46.680 --> 0:35:49.560
<v Speaker 1>using the same logic, this is the oldest thing we found. Yeah,

0:35:49.680 --> 0:35:51.560
<v Speaker 1>so it's probably the sort of the age of the

0:35:51.560 --> 0:35:54.160
<v Speaker 1>Solar system. Right, that's when we think the gas and

0:35:54.160 --> 0:35:57.799
<v Speaker 1>the dust got accumulated together to form the Sun and

0:35:57.840 --> 0:36:00.160
<v Speaker 1>the planets and all that stuff. But the first age

0:36:00.200 --> 0:36:02.040
<v Speaker 1>of that was to form smaller rocks, and so we

0:36:02.080 --> 0:36:05.719
<v Speaker 1>think these things are remnants of those times. Right, But wait,

0:36:05.760 --> 0:36:08.160
<v Speaker 1>didn't the Sun. Hasn't the Sun our son already been

0:36:08.160 --> 0:36:10.640
<v Speaker 1>through a couple of cycles, Like, hasn't it exploded a

0:36:10.680 --> 0:36:15.359
<v Speaker 1>few times already. Well, our son hasn't exploded, but it's materials, right,

0:36:15.520 --> 0:36:19.480
<v Speaker 1>have been through several solar cycles. Everything around us, all

0:36:19.520 --> 0:36:21.880
<v Speaker 1>that stuff is left over from one or two or

0:36:21.920 --> 0:36:25.319
<v Speaker 1>three solar cycles of a sun lasting for you know,

0:36:25.400 --> 0:36:27.799
<v Speaker 1>one to see three billion years and then blowing up

0:36:27.840 --> 0:36:30.880
<v Speaker 1>and spreading its materials around. So everything around us is

0:36:31.000 --> 0:36:33.560
<v Speaker 1>all all the components of the solar system are probably

0:36:33.719 --> 0:36:36.840
<v Speaker 1>been recycled. But it's not like our son formed and

0:36:36.880 --> 0:36:38.600
<v Speaker 1>then we started in formed and we started it was

0:36:38.600 --> 0:36:41.600
<v Speaker 1>a different from a different star. Oh I see, So

0:36:41.719 --> 0:36:45.439
<v Speaker 1>our current son is is maybe around four point five

0:36:45.520 --> 0:36:48.040
<v Speaker 1>billion years old. Yeah, that's what we think. That's the

0:36:48.080 --> 0:36:51.040
<v Speaker 1>history of our solar system. And remember, for context, the

0:36:51.080 --> 0:36:54.520
<v Speaker 1>Milky Way is something like thirteen billion years old, and

0:36:54.560 --> 0:36:57.239
<v Speaker 1>the universe is just a little bit older than that,

0:36:57.680 --> 0:37:01.319
<v Speaker 1>almost fourteen billion years old. So there's a lot of

0:37:01.400 --> 0:37:05.320
<v Speaker 1>history before even our son, our solar system was formed,

0:37:05.480 --> 0:37:08.400
<v Speaker 1>and then a lot of history before we came around.

0:37:08.880 --> 0:37:11.880
<v Speaker 1>And so like that's the cosmic context that we're standing in.

0:37:12.080 --> 0:37:13.560
<v Speaker 1>And so that's the all this thing we found in

0:37:13.600 --> 0:37:16.480
<v Speaker 1>the solar system, but that's older than all the things

0:37:16.480 --> 0:37:18.920
<v Speaker 1>we found. That is part of the Earth. So somewhere

0:37:18.960 --> 0:37:21.560
<v Speaker 1>between those two numbers is when maybe the ball of

0:37:21.560 --> 0:37:23.600
<v Speaker 1>the Earth form. That's right. That's what we call the

0:37:23.680 --> 0:37:27.040
<v Speaker 1>Joorge date, the Joge definition of the age of the Earth,

0:37:27.960 --> 0:37:32.719
<v Speaker 1>the Bald date or his Bald date. That's right, that's right. Um.

0:37:33.080 --> 0:37:35.279
<v Speaker 1>And so you know there's a window there about a

0:37:35.400 --> 0:37:38.640
<v Speaker 1>hundred and fifty million years, which seems like a huge number,

0:37:38.760 --> 0:37:41.439
<v Speaker 1>you know, that's like, but it's pretty small, I think

0:37:41.480 --> 0:37:45.520
<v Speaker 1>compared to exactly. Geologically speaking, it's a blink of an eye, yeah,

0:37:45.880 --> 0:37:50.960
<v Speaker 1>or universe speaking, it's it's pretty accurate, yeah, exactly. And uh,

0:37:51.040 --> 0:37:53.480
<v Speaker 1>you know, we we know these numbers two plus or

0:37:53.520 --> 0:37:56.160
<v Speaker 1>minus twenty five or fifty million years based on the

0:37:56.200 --> 0:38:00.759
<v Speaker 1>uncertainty of radiometric dating and so um, because of the

0:38:00.840 --> 0:38:03.439
<v Speaker 1>hard work of a lot of scientists to develop these

0:38:03.480 --> 0:38:06.240
<v Speaker 1>things and across check them and understand them across various

0:38:06.280 --> 0:38:10.040
<v Speaker 1>other processes. Now we've looked around us and we've gathered

0:38:10.040 --> 0:38:12.600
<v Speaker 1>these clues from everyday objects around us, you know, the

0:38:12.680 --> 0:38:15.719
<v Speaker 1>rocks at our feet, the rocks in Australia give us

0:38:15.719 --> 0:38:19.480
<v Speaker 1>clues about these fantastic numbers that would just blow the

0:38:19.520 --> 0:38:22.239
<v Speaker 1>minds of our ancestors and those clues were around for

0:38:22.280 --> 0:38:24.680
<v Speaker 1>them to discover also, and so of course that makes

0:38:24.680 --> 0:38:27.640
<v Speaker 1>you wonder, like, what clues are there laying around at

0:38:27.640 --> 0:38:30.080
<v Speaker 1>our feet now that would tell us secrets of the

0:38:30.200 --> 0:38:33.239
<v Speaker 1>universe that our descendants will know and wonder why we

0:38:33.239 --> 0:38:35.839
<v Speaker 1>couldn't figure it out. It's not just like an opinion, right,

0:38:35.920 --> 0:38:39.319
<v Speaker 1>It's pretty based on evidence, and it's pretty based on

0:38:39.480 --> 0:38:42.840
<v Speaker 1>science and physics, the numbers. Yeah, exactly, these things we

0:38:42.880 --> 0:38:45.080
<v Speaker 1>know pretty well. We have a lot of confidence in them.

0:38:45.080 --> 0:38:48.400
<v Speaker 1>People have been working on these processes for decades and decades,

0:38:49.000 --> 0:38:52.360
<v Speaker 1>a lot of you know, grumpy competition between rivals to

0:38:52.400 --> 0:38:54.759
<v Speaker 1>make more and more accurate measurements. You know, this is

0:38:54.760 --> 0:38:57.640
<v Speaker 1>not a conspiracy of scientists all working together in harmony.

0:38:58.000 --> 0:39:00.560
<v Speaker 1>You know, this is a bunch of people racing to

0:39:00.680 --> 0:39:03.600
<v Speaker 1>develop better and better techniques and trying to find older

0:39:03.600 --> 0:39:07.280
<v Speaker 1>and older rocks. Remember, sciences a competitive field, and everybody

0:39:07.280 --> 0:39:09.400
<v Speaker 1>wants to one up the other to get the more accurate,

0:39:09.600 --> 0:39:12.880
<v Speaker 1>the more reliable, the more verifiable answer. So, yeah, we

0:39:12.920 --> 0:39:15.239
<v Speaker 1>have a lot of confidence in this knowledge. Yeah, it's

0:39:15.280 --> 0:39:17.319
<v Speaker 1>like it's all around the evidence, it's all around us,

0:39:17.360 --> 0:39:19.640
<v Speaker 1>and you're you're standing on it. Yeah, exactly, and even

0:39:19.680 --> 0:39:22.160
<v Speaker 1>if you can't do radiometric dating in your head of course,

0:39:22.200 --> 0:39:24.600
<v Speaker 1>because you can't see the xericon crystals. You know, you

0:39:24.680 --> 0:39:26.560
<v Speaker 1>just look around you and you see lots of things

0:39:26.600 --> 0:39:29.640
<v Speaker 1>around you which take a long time to form. You know,

0:39:29.960 --> 0:39:32.560
<v Speaker 1>how long does it take a mountain to form? It's

0:39:32.600 --> 0:39:35.960
<v Speaker 1>a very slow process. And so all around us on

0:39:36.000 --> 0:39:39.000
<v Speaker 1>the Earth we see evidence of very very slow processes

0:39:39.320 --> 0:39:42.200
<v Speaker 1>which have accomplished a great deal, which tells you that

0:39:42.239 --> 0:39:44.439
<v Speaker 1>they've been doing it for a long long time. Yeah,

0:39:44.680 --> 0:39:47.479
<v Speaker 1>like you said, who knows what else is lying under

0:39:47.480 --> 0:39:52.120
<v Speaker 1>our feet? That's right exactly, So I think we answered

0:39:52.160 --> 0:39:54.799
<v Speaker 1>that question about the age of the earth. Yeah, yeah,

0:39:54.840 --> 0:39:59.600
<v Speaker 1>so grab a glass of wine and sit back and enjoy.

0:40:00.320 --> 0:40:03.319
<v Speaker 1>That's right. And uh, no matter how old you are,

0:40:03.400 --> 0:40:06.239
<v Speaker 1>remember you can always enjoy one more brownie. See you

0:40:06.320 --> 0:40:09.120
<v Speaker 1>next time. Thanks for tuning in, and thanks for asking

0:40:09.160 --> 0:40:12.120
<v Speaker 1>great questions. This question was inspired by an email from

0:40:12.120 --> 0:40:14.319
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0:40:14.360 --> 0:40:16.600
<v Speaker 1>to know the answer to, please send it to us

0:40:16.760 --> 0:40:27.880
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0:40:28.000 --> 0:40:30.840
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0:40:30.920 --> 0:40:33.880
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0:40:33.880 --> 0:40:36.719
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0:40:37.040 --> 0:40:40.160
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0:40:40.440 --> 0:40:44.080
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0:40:44.160 --> 0:40:46.840
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0:40:46.920 --> 0:40:50.400
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0:40:50.400 --> 0:40:54.160
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