WEBVTT - How do you make gold?

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<v Speaker 1>Daniel, you were wish you'd studied a more practical science.

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<v Speaker 1>What do you mean, I think you know what I mean?

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<v Speaker 1>You study? You mean, should I have studied something that

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<v Speaker 1>has actual practical applications that could help people in their

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<v Speaker 1>everyday lives. Yeah, you know, something that saves people's lives

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<v Speaker 1>for example, or you know, or turned lead into gold. Well,

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<v Speaker 1>those are great examples because those are the two things

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<v Speaker 1>that particle physics actually does do. I thought turning lead

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<v Speaker 1>into goal was alchemy, you know, a pseudoscience from hundreds

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<v Speaker 1>of years ago. It used to be pseudoscience, but now

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<v Speaker 1>we have made it real science. Particle physics can actually

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<v Speaker 1>do this, but as always there's a catch. Welcome to

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<v Speaker 1>our podcast This is Daniel and Jorge Explain the Universe,

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<v Speaker 1>a production of My Heart Radio, in which we look

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<v Speaker 1>all around the universe and try to find fascinating little

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<v Speaker 1>nuggets of intellectual gold, or turn mysterious nuggets of intellectual

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<v Speaker 1>lead into nuggets of understandable intellectual gold. That's right. We

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<v Speaker 1>are podcasts alchemists turning bad jokes into comedy gold. That's right.

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<v Speaker 1>We turned the mysterious into the understandable. Physics can do anything.

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<v Speaker 1>We still haven't figured out teleportation or anti gravity or

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<v Speaker 1>warp drives or um, you know, how to make my

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<v Speaker 1>internet actually go quickly? Still a mystery for me for sure.

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<v Speaker 1>Here at my house. We'll probably figure out teleportation before

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<v Speaker 1>we figure out fast internet at home. Yeah, which one

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<v Speaker 1>is more impossible? I don't know. If I could just

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<v Speaker 1>teleport the data from Netflix to my TV, I wouldn't

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<v Speaker 1>need the Internet. Maybe that is how they do it,

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<v Speaker 1>That's how they should do it. At least somebody over

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<v Speaker 1>at Netflix is pouring a billion dollars into their teleportation

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<v Speaker 1>department right now. So to be on the podcast, we

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<v Speaker 1>are tackling a topic that used to be considered magic

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<v Speaker 1>hundreds of years ago. Right, alchemy, This idea that you

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<v Speaker 1>can transmute or transform one element into a totally different element.

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<v Speaker 1>That's right, And that was back in the day when

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<v Speaker 1>they thought that what we consider the elements were the

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<v Speaker 1>fundamental building blocks of the universe. You know, they were like, here,

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<v Speaker 1>we found these things that make up everything, and you

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<v Speaker 1>combine them in different ways to make cool stuff. But

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<v Speaker 1>they seem to be sort of the basic building blocks.

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<v Speaker 1>They hadn't yet broken them up and found the smaller

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<v Speaker 1>bits and so it made sense that people were like, well,

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<v Speaker 1>is it possible to change one kind of thing into

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<v Speaker 1>another kind of thing? Because you know, one kind of

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<v Speaker 1>thing like lead, you can find it not to without

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<v Speaker 1>much difficulty, and it's not that valuable, while other kinds

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<v Speaker 1>of things like tremendously valuable. So it seemed appealing not

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<v Speaker 1>just from the economic point of view, but from the

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<v Speaker 1>sort of deep understanding point of view, like can we

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<v Speaker 1>turn one thing into another kind of thing? To be

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<v Speaker 1>on the burg and we'll be talking about how do

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<v Speaker 1>you make gold? How do you make the shiny golden

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<v Speaker 1>stuff that everybody, every human seems to want for some

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<v Speaker 1>weird and almost arbitrary reasons. That's right, well, that's economics, right,

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<v Speaker 1>it's all arbitrary. And it's not just about how do

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<v Speaker 1>we make gold or how could you make gold? Or

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<v Speaker 1>could you fabricate gold in your garage? But it's like

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<v Speaker 1>how does the universe make gold? Like where does gold

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<v Speaker 1>come from? Right? What was it created during the Big Bang?

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<v Speaker 1>Is it made in the core of the earth. Is

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<v Speaker 1>it all made the lab of somebody somewhere in Europe,

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<v Speaker 1>you know, underground somewhere, or is there some other mysterious

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<v Speaker 1>process How is gold made? Are we going to be

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<v Speaker 1>selling gold making kids at the end of this podcast, Daniel,

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<v Speaker 1>you could probably make a lot of money. Just be

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<v Speaker 1>a box of lead with some instructions that say, Step one,

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<v Speaker 1>race a quadrillion dollars. Step two, build a particle collider. Done,

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<v Speaker 1>we have a particle collider. You just need to apply

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<v Speaker 1>for time at the large age on collider. So yeah,

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<v Speaker 1>we'll send you a lump of gold and instructions for

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<v Speaker 1>how to get to CERN. Step one, apply fill out

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<v Speaker 1>this application. Yeah, first send us and you'll get these

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<v Speaker 1>incredible items. Technically it would be a real thing like

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<v Speaker 1>it is, actually the steps of how to make gold. Yeah,

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<v Speaker 1>you really can. I think it's sort of cool that

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<v Speaker 1>we have understood the way the universe works, the sort

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<v Speaker 1>of elemental understanding, to a point where we do see

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<v Speaker 1>how these things are put together. We can understand them

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<v Speaker 1>from the ground up. You know, how to assemble protons

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<v Speaker 1>and neutrons and what makes something gold and something else.

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<v Speaker 1>Led to the point where we can actually change them

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<v Speaker 1>from one to the other. I mean, it's not economically feasible,

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<v Speaker 1>but we do have the power. We have conquered this

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<v Speaker 1>barrier of the elements Yeah, Well, why do you think

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<v Speaker 1>humans are so fascinated with gold, like, out of all

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<v Speaker 1>the elements? Why? Why? Why is gold too special in

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<v Speaker 1>human culture? I think I have to refer to a

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<v Speaker 1>comment made by my good friend and wise comic, who said,

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<v Speaker 1>humans like sparkly things. That's something my grandma always used

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<v Speaker 1>to say. Why is it every time you say something

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<v Speaker 1>sort of wise, you just attribute it to your grandma?

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<v Speaker 1>She was a wise woman. I think it's just your humility.

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<v Speaker 1>You don't want to come off sounding like you think

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<v Speaker 1>your intelligence you should be this to this fictional grandma.

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<v Speaker 1>I think I just don't want to reveal that I

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<v Speaker 1>have no idea where I got that quote. Let's so

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<v Speaker 1>anonymous becomes Jorge's grandma. Yeah, so people like shiny, sparkly things,

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<v Speaker 1>and that's what gold is. Right. It doesn't staying right,

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<v Speaker 1>it doesn't rust when you make something out of goal.

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<v Speaker 1>It just always stays shining right. That's what's special about it. Yeah,

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<v Speaker 1>of course, And the other special thing is that it's rare. Right,

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<v Speaker 1>you don't find a lump of goal under every rock.

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<v Speaker 1>It's not in lots of places, and so because it's

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<v Speaker 1>hard to get, that makes it valuable, right, but it's

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<v Speaker 1>sort of this weird thing. I mean, my kids ask

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<v Speaker 1>me this question, like why is gold cost so much?

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<v Speaker 1>And it really is just you know, something we've all

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<v Speaker 1>decided on. You know, It's this weird thing I never

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<v Speaker 1>really understood about economics, is that the value of something

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<v Speaker 1>is really just what people are willing to pay for it.

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<v Speaker 1>So we all decided that, you know, something else was

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<v Speaker 1>better than gold, and we were willing to pay for it,

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<v Speaker 1>and we would have created this enormous wealth, right right, Yeah,

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<v Speaker 1>Welcome to the new podcast Daniel and Jorge explain economics. Dane,

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<v Speaker 1>Orge are clueless about economics and pontificate ignorantly. Now, but

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<v Speaker 1>there is something special about gold itself as a metal, right,

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<v Speaker 1>It is shinier than most other elements, right, and it

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<v Speaker 1>doesn't rust, and it's it's easy to make smooth. Right,

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<v Speaker 1>It's something there's something special about it. Yeah, it's malleable

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<v Speaker 1>in this cool way, you know, but it's it's still arbitrary.

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<v Speaker 1>It's you know, it's like beauty, right, it's just what

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<v Speaker 1>we decide. We think it's cool, we think it's interesting,

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<v Speaker 1>and we think it looks good and jewelry and stuff.

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<v Speaker 1>You know, why is gold so much more valuable than silver.

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<v Speaker 1>You know, it is more rare, and people do like

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<v Speaker 1>it more, but it holds a special place. You know,

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<v Speaker 1>do you think it's somehow related to our evolution to

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<v Speaker 1>sort of like sunlight and you know, shiny light and

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<v Speaker 1>gold that particularly gold color. Oh man, I think that

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<v Speaker 1>whole field of science is bologna. Is like attempt to

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<v Speaker 1>evolutionary psychology, like this attempt to say like maybe we

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<v Speaker 1>act this way because it could have been preferential and

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<v Speaker 1>the savannah or something like. I think that you can

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<v Speaker 1>you can explain almost anything using that kind of logic. Well, anyway,

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<v Speaker 1>so it's rare on Earth, and that's an interesting question.

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<v Speaker 1>Why is it rarer? And how do you how is

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<v Speaker 1>it made? And could we make it here in the

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<v Speaker 1>lab for example? Yeah, exactly, and h you know, if

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<v Speaker 1>you start thinking about like where this stuff comes from,

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<v Speaker 1>you might wonder like how does this stuff all get made?

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<v Speaker 1>You know, how did things begin? You know, did was

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<v Speaker 1>all the stuff in the universe made in the first

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<v Speaker 1>bill a second you know, made during the Big Bang?

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<v Speaker 1>Or would the big bang just make hydrogen and everything

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<v Speaker 1>else gets assembled later? These are really fascinating questions and

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<v Speaker 1>it's the kind of thing that really it's just sort

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<v Speaker 1>of the kind of puzzle that scientists can use to

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<v Speaker 1>understand the mechanisms of the universe, Like what's going on

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<v Speaker 1>in the universe. Can we explain how much hydrogen there is,

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<v Speaker 1>and how much iron there is, and how much of

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<v Speaker 1>this there is. It's a huge amount of really specific

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<v Speaker 1>data that helps us understand what's going on in the universe.

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<v Speaker 1>We let's just build models to try to explain what

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<v Speaker 1>we've seen. And because the data is so specific, there's

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<v Speaker 1>so many different elements and we can measure their abundance.

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<v Speaker 1>It gives us a lot of handles for understanding like

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<v Speaker 1>what's going on inside stars and inside other astrophysical objects. Oh,

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<v Speaker 1>I see. It's kind of a question of did all

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<v Speaker 1>the ingredients for the universe that we see around us

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<v Speaker 1>right now? Was that all there from the beginning at

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<v Speaker 1>the Big Bang? You know, that everything that we need

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<v Speaker 1>to make the universe as it is now get created

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<v Speaker 1>in those first few moments, or that the universe get

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<v Speaker 1>created one way and then the ingredients of a change

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<v Speaker 1>over time exactly. And it's just part of this larger

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<v Speaker 1>question of do we understand what's around us? You know,

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<v Speaker 1>we look around us and we see, okay, we've see

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<v Speaker 1>this this stuff. Do we understand how it got there?

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<v Speaker 1>So we try to tell a story, you know, we

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<v Speaker 1>want to make sure that the story makes sense. Do

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<v Speaker 1>we know how the story began? Do we understand why

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<v Speaker 1>went this way not the other way? And so, as

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<v Speaker 1>a part, it's been like a hundred years we've been

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<v Speaker 1>trying to piece this story together to explain why we

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<v Speaker 1>see what, you know, the stuff we see in the universe,

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<v Speaker 1>and where it is. Can we understand it? So it's

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<v Speaker 1>a pretty big question. And so today on the podcast,

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<v Speaker 1>we're talking about one specific thing, which is gold, and

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<v Speaker 1>so we were wondering how many people out there know

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<v Speaker 1>where gold is made or how it's made. I walked

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<v Speaker 1>around the campus you see, Irvine, and I popped this

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<v Speaker 1>question to a bunch of unsuspecting students or whoever else

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<v Speaker 1>would happen to be around campus that day, and I

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<v Speaker 1>asked them where do you think gold is made? So

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<v Speaker 1>before you listen to these answers, think for yourself for

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<v Speaker 1>a moment do you know where gold is made? And

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<v Speaker 1>if you get the r answer right, you get a

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<v Speaker 1>gold star right, or a lead star or a lead

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<v Speaker 1>star and an application form. Well, here's what people had

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<v Speaker 1>to say. Maybe in the sun on another planet, I'm

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<v Speaker 1>not sure won't be in like fusion in the center

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<v Speaker 1>of Yeah, I'm not sure. I would say a big

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<v Speaker 1>bang like in the Earth's crust through collision. Uh. I

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<v Speaker 1>have no idea chemically or physically like whatever happens within

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<v Speaker 1>the core, like gold aliens, like the species after dat,

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<v Speaker 1>it's just naturally rotted and it becomes gold. Alright, A

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<v Speaker 1>lot of interesting answers, and honestly, they all seem kind

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<v Speaker 1>of plausible to me. You know, some people said that

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<v Speaker 1>gold is made inside of the Earth at the core,

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<v Speaker 1>the core of the Earth, or inside of stars or

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<v Speaker 1>the first ones you mentioned. The ones people said maybe

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<v Speaker 1>it was made inside the earth. That puzzled me for

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<v Speaker 1>a bit until somebody said, you know, kind of like diamonds,

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<v Speaker 1>and then I realized, yeah, that's true. Diamonds really are

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<v Speaker 1>made inside the earth. Is the pressure of the Earth

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<v Speaker 1>on carbon the core that that creates these these incredible crystals,

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<v Speaker 1>And so it is plausible to think, like you know,

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<v Speaker 1>jewels and gold, maybe they're just made in high temperature

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<v Speaker 1>reactions inside the Earth. So I understood the line of

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<v Speaker 1>thinking after a bit. Yeah, because it's it's also kind

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<v Speaker 1>of a rare and valuable thing, and maybe people a

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<v Speaker 1>shid rare and valuable with the things taking a long

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<v Speaker 1>time to make an extreme conditions. Yeah, and like many

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<v Speaker 1>plausible ideas, it's totally wrong. No gold start for you, exactly. Well,

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<v Speaker 1>let's let's get into this idea of gold. What do

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<v Speaker 1>we know about gold? Well, it's shiny and it looks

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<v Speaker 1>good on your finger. Um, But the think the thing

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<v Speaker 1>to understand is that gold is one of the elements, right,

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<v Speaker 1>And the identity of these elements is determined by how

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<v Speaker 1>many protons there are in the nucleus. So remember every

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<v Speaker 1>everything that's elemental is just an atom, right, It's not

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<v Speaker 1>a mixture of different elements. It's it's just an atom,

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<v Speaker 1>and the atom has a nucleus insided and the nucleus

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<v Speaker 1>has protons and neutrons. And the thing that determines the

0:11:44.559 --> 0:11:47.880
<v Speaker 1>identity which element you are? Are you hydrogen, are you helium?

0:11:47.920 --> 0:11:51.839
<v Speaker 1>Are unickel? Are you uranium? Is the number of protons

0:11:51.880 --> 0:11:54.360
<v Speaker 1>in the nucleus, right, Because all these elements they're not

0:11:55.040 --> 0:11:57.640
<v Speaker 1>they're all just variations of the same thing, right, Like

0:11:57.679 --> 0:12:01.520
<v Speaker 1>different combinations of the same thing. Right, used to me

0:12:01.559 --> 0:12:04.199
<v Speaker 1>that we used to think that carbon and oxygen there

0:12:04.360 --> 0:12:07.520
<v Speaker 1>like its own thing in the universe, but actually turned

0:12:07.520 --> 0:12:11.800
<v Speaker 1>out that they're just the same thing, just rearranged differently. Yeah,

0:12:11.840 --> 0:12:14.520
<v Speaker 1>and it's it's more about the numbers. Like, you take

0:12:14.760 --> 0:12:18.080
<v Speaker 1>one proton and one electron, you get hydrogen. Right, you

0:12:18.120 --> 0:12:22.040
<v Speaker 1>add another proton and another electron to balance it out electrically,

0:12:22.360 --> 0:12:24.840
<v Speaker 1>and you get helium. And so it's just the number

0:12:24.960 --> 0:12:28.160
<v Speaker 1>of servings you get, right, that determines which element you are.

0:12:28.440 --> 0:12:31.439
<v Speaker 1>And you're right, it's fascinating that these things aren't fundamental

0:12:31.960 --> 0:12:33.520
<v Speaker 1>but there are just made out of the same things,

0:12:33.520 --> 0:12:37.120
<v Speaker 1>but they're so vastly different. Right, Iron is totally different

0:12:37.120 --> 0:12:40.840
<v Speaker 1>from helium. It's totally different from silicon, from carbon, from oxygen,

0:12:41.160 --> 0:12:43.640
<v Speaker 1>but all these things are made up of the same stuff.

0:12:44.040 --> 0:12:45.840
<v Speaker 1>This is the kind of thing I blows my mind

0:12:45.880 --> 0:12:48.480
<v Speaker 1>every time I think about it, that the the critical

0:12:48.600 --> 0:12:51.080
<v Speaker 1>identity of these things comes not from what they're made

0:12:51.080 --> 0:12:53.400
<v Speaker 1>out of, but just from the arrangements of the particles

0:12:53.400 --> 0:12:55.280
<v Speaker 1>inside them. Yeah, it's kind of like if you think

0:12:55.320 --> 0:12:59.360
<v Speaker 1>about like your favorite recipe of your favorite kind of food, right,

0:12:59.440 --> 0:13:01.920
<v Speaker 1>Like it's you add a lot of ingredients into it,

0:13:01.960 --> 0:13:04.640
<v Speaker 1>but really at the end, all of those ingredients are

0:13:04.920 --> 0:13:08.679
<v Speaker 1>probably just carbon and hydrogen, right, that's true. I don't know.

0:13:08.720 --> 0:13:11.560
<v Speaker 1>I would say the critical issue for baking is whether

0:13:11.640 --> 0:13:14.360
<v Speaker 1>or not includes chocolate. Includes chocolate, it's going to be tasty.

0:13:14.640 --> 0:13:19.480
<v Speaker 1>Otherwise it's a question mark. I don't know. Hast chocolate.

0:13:19.800 --> 0:13:24.160
<v Speaker 1>It's golden wins the gold star. And so the thing

0:13:24.160 --> 0:13:26.400
<v Speaker 1>about gold is that it's pretty heavy, right. It has

0:13:26.400 --> 0:13:28.480
<v Speaker 1>a lot of protons in the nucleus. Right, So as

0:13:28.559 --> 0:13:31.280
<v Speaker 1>you add a proton to a nucleus, it gets heavier

0:13:31.280 --> 0:13:34.079
<v Speaker 1>and heavier, and you walk your way up the periodic table.

0:13:34.320 --> 0:13:36.920
<v Speaker 1>And as an aside, did you start with hydrogen? Right?

0:13:37.240 --> 0:13:40.720
<v Speaker 1>You start hydrogen is like the simplest atom is just

0:13:40.800 --> 0:13:43.800
<v Speaker 1>one proton and one electron, That's right, That's the first

0:13:43.800 --> 0:13:45.640
<v Speaker 1>thing you would make. And that's the first thing that

0:13:45.679 --> 0:13:48.880
<v Speaker 1>the universe did make in fact, and still it's what

0:13:49.120 --> 0:13:51.240
<v Speaker 1>most of the universe is. Most of the universe, like

0:13:51.320 --> 0:13:55.560
<v Speaker 1>seventy four percent of the universe is hydrogen. And uh.

0:13:55.679 --> 0:13:58.240
<v Speaker 1>And then then the reason is that it's the simplest thing, right,

0:13:58.800 --> 0:14:00.960
<v Speaker 1>But as you walk your way the periodic table, you

0:14:00.960 --> 0:14:03.280
<v Speaker 1>add a proton, you get more and more complex stuff.

0:14:03.720 --> 0:14:06.080
<v Speaker 1>And this is how we knew that there were gaps

0:14:06.080 --> 0:14:08.600
<v Speaker 1>in the periodic table. Right. We we said, okay, we

0:14:08.600 --> 0:14:10.199
<v Speaker 1>see this element, we see that element, we see the

0:14:10.240 --> 0:14:13.520
<v Speaker 1>other element. We can measure how many protons there are

0:14:13.520 --> 0:14:15.000
<v Speaker 1>in the nucleus of an element, and then we put

0:14:15.040 --> 0:14:16.960
<v Speaker 1>them in place, and then we could tell oh, look

0:14:17.200 --> 0:14:19.680
<v Speaker 1>there's nothing with you know, this number of protons. How

0:14:19.680 --> 0:14:22.000
<v Speaker 1>can we haven't found anything with that number of protons.

0:14:22.240 --> 0:14:23.960
<v Speaker 1>So we go look forward and we try to make

0:14:24.000 --> 0:14:26.440
<v Speaker 1>it or this kind of stuff. It's it's cool that

0:14:26.480 --> 0:14:29.000
<v Speaker 1>the identity of the elements determined just by the number

0:14:29.040 --> 0:14:32.160
<v Speaker 1>of protons. Yeah, until you start with hydrogen, and then

0:14:32.240 --> 0:14:34.600
<v Speaker 1>you add a proton and you get helium, and then

0:14:34.640 --> 0:14:38.080
<v Speaker 1>you add another proton, and it just you go up

0:14:38.200 --> 0:14:40.920
<v Speaker 1>up the list of elements and at some point you

0:14:40.960 --> 0:14:43.560
<v Speaker 1>get to gold. Right, that's right. And you know, there's

0:14:43.560 --> 0:14:45.920
<v Speaker 1>a hundred and some elements that we've discovered or created

0:14:45.920 --> 0:14:48.240
<v Speaker 1>by now, and each one is so different and their

0:14:48.240 --> 0:14:51.600
<v Speaker 1>properties are determined really just by how many protons, which

0:14:51.600 --> 0:14:54.040
<v Speaker 1>determines how many electrons you need to balance it, and

0:14:54.080 --> 0:14:56.760
<v Speaker 1>then how those atoms interact, so like why are some

0:14:56.840 --> 0:14:58.960
<v Speaker 1>of the metallic and some of them are conductors, and

0:14:59.280 --> 0:15:01.840
<v Speaker 1>some of them are really active and some are inactive.

0:15:02.040 --> 0:15:04.880
<v Speaker 1>All of that is determined just by how the electrons

0:15:05.000 --> 0:15:07.520
<v Speaker 1>fill out their orbitals, right, whether they like to interact

0:15:07.560 --> 0:15:10.080
<v Speaker 1>with other atoms or not, And that in turn is

0:15:10.120 --> 0:15:12.720
<v Speaker 1>determined by how many protons are in the nucleus. So

0:15:12.760 --> 0:15:15.480
<v Speaker 1>it's really just proton counting. So you're saying gold is

0:15:15.480 --> 0:15:19.920
<v Speaker 1>really just like a fat hydrogen. It's like a crowd

0:15:19.920 --> 0:15:22.480
<v Speaker 1>of hydrogen. Yeah, it's just a cluster of a hydrogen

0:15:22.800 --> 0:15:24.960
<v Speaker 1>and the kind of right, And but then then that

0:15:25.080 --> 0:15:28.400
<v Speaker 1>really changes its behaviors. It totally changes this behavior. And

0:15:28.440 --> 0:15:30.080
<v Speaker 1>it's the other thing I understand is that it's not

0:15:30.160 --> 0:15:32.560
<v Speaker 1>easy to do, right. It's not that you can just

0:15:32.720 --> 0:15:36.480
<v Speaker 1>very easily take two hydrogen atoms and make helium out

0:15:36.480 --> 0:15:38.800
<v Speaker 1>of them. And the reason is that the nuclei don't

0:15:38.880 --> 0:15:42.160
<v Speaker 1>like to hang out together. The nuclei nucleus of hydrogen

0:15:42.200 --> 0:15:45.320
<v Speaker 1>atom is a proton which is positively charged. So they're

0:15:45.320 --> 0:15:47.000
<v Speaker 1>going to repel each other. And we had a whole

0:15:47.000 --> 0:15:50.400
<v Speaker 1>podcast episode about this recently. How does this happen? And

0:15:50.440 --> 0:15:52.960
<v Speaker 1>you know, they will repel each other unless you force

0:15:53.080 --> 0:15:55.720
<v Speaker 1>them together. You get them close enough together, the strong

0:15:55.840 --> 0:15:58.880
<v Speaker 1>nuclear force takes over and then it attracts the quarks

0:15:59.000 --> 0:16:01.400
<v Speaker 1>inside those proton on to tract each other, and they

0:16:01.440 --> 0:16:04.680
<v Speaker 1>overcome that. We call that the Coolomb barrier because Coolumb

0:16:04.720 --> 0:16:07.920
<v Speaker 1>is the guy who first thought about electromagnetic force electrostatic

0:16:07.960 --> 0:16:10.000
<v Speaker 1>forces that repel each other. Yeah, I hear. He was

0:16:10.000 --> 0:16:13.200
<v Speaker 1>a cool guy. Yeah, but there were some barriers to

0:16:13.240 --> 0:16:15.320
<v Speaker 1>getting to know him. But it's like they snapped together, right,

0:16:15.320 --> 0:16:17.480
<v Speaker 1>Like they repel each other, but at some point they

0:16:17.480 --> 0:16:19.720
<v Speaker 1>get so close that they snapped together and they become

0:16:19.760 --> 0:16:21.600
<v Speaker 1>a different element. Yeah, you can think of it's sort

0:16:21.600 --> 0:16:24.760
<v Speaker 1>of like, um, hiking into a volcano. Right, You're walking

0:16:24.840 --> 0:16:28.640
<v Speaker 1>up the hill and it's getting harder and harder and harder. Right, Um,

0:16:28.680 --> 0:16:30.600
<v Speaker 1>it's steeper, and the sizes are getting steper and steper

0:16:30.600 --> 0:16:33.720
<v Speaker 1>and steeper. It's it's easier to roll down away from

0:16:33.760 --> 0:16:35.280
<v Speaker 1>the center of the volcano, but once you get to

0:16:35.320 --> 0:16:37.000
<v Speaker 1>the top, right, it's very easy to just like fall

0:16:37.080 --> 0:16:39.160
<v Speaker 1>into the center. And so it's sort of that way,

0:16:39.320 --> 0:16:43.080
<v Speaker 1>and then you die a horrible death, right, or you

0:16:43.160 --> 0:16:46.400
<v Speaker 1>fuse beautifully into something new. Right, you rise out of

0:16:46.440 --> 0:16:50.280
<v Speaker 1>the ashes like a phoenix something else than beautiful. Um. Yeah,

0:16:50.320 --> 0:16:52.000
<v Speaker 1>So you push them together hard enough, and that's what

0:16:52.040 --> 0:16:54.960
<v Speaker 1>we call fusion. You you get the strong nuclear force

0:16:55.000 --> 0:16:57.280
<v Speaker 1>to take over and it makes a new nucleus, right

0:16:57.320 --> 0:16:59.320
<v Speaker 1>and it and it becomes something totally different. So this

0:16:59.400 --> 0:17:02.400
<v Speaker 1>is alchemy, right, changing one element into another. Turns out

0:17:02.440 --> 0:17:04.680
<v Speaker 1>you just gotta push hard enough, you know, or take

0:17:04.680 --> 0:17:07.160
<v Speaker 1>protons out, and you can change what something is. Okay,

0:17:07.160 --> 0:17:09.239
<v Speaker 1>So that's how you make gold. You take hydrogen and

0:17:09.280 --> 0:17:11.280
<v Speaker 1>you just keep building it up and at some point

0:17:11.320 --> 0:17:13.159
<v Speaker 1>you go through all the elements and you get to

0:17:13.320 --> 0:17:15.480
<v Speaker 1>the shiny stuff. Right, that's right. But that's not easy

0:17:15.560 --> 0:17:18.240
<v Speaker 1>to do, right, you. It's really hard to squeeze these

0:17:18.240 --> 0:17:20.639
<v Speaker 1>things together. They don't like to be together, right, It's

0:17:20.640 --> 0:17:23.000
<v Speaker 1>not a configuration they like. So the question really is

0:17:23.040 --> 0:17:25.399
<v Speaker 1>not how do you make gold, but like, where in

0:17:25.440 --> 0:17:28.160
<v Speaker 1>the universe does this happen? How is it even possible?

0:17:28.160 --> 0:17:30.080
<v Speaker 1>All right, let's get into that, and let's start with

0:17:30.119 --> 0:17:33.200
<v Speaker 1>a big bang. But first let's take a quick break.

0:17:45.920 --> 0:17:48.439
<v Speaker 1>All right. We're talking about how to make gold, and

0:17:48.480 --> 0:17:50.680
<v Speaker 1>so we know how to make it, which is you

0:17:50.680 --> 0:17:54.479
<v Speaker 1>you build up hydrogen atom up until you get into

0:17:54.960 --> 0:17:57.159
<v Speaker 1>the different elements and eventually you get to gold. But

0:17:57.200 --> 0:18:00.240
<v Speaker 1>it's a pretty extreme process, like you need a lot

0:18:00.240 --> 0:18:02.439
<v Speaker 1>of energy. That's right, you really do need a lot

0:18:02.480 --> 0:18:05.760
<v Speaker 1>of energy. Um. It's not something that's easy to do. Um.

0:18:05.880 --> 0:18:08.359
<v Speaker 1>And as usual a little with a hard physics question,

0:18:08.400 --> 0:18:11.320
<v Speaker 1>Let's start with the Big Bang, right, because the creator

0:18:11.400 --> 0:18:13.800
<v Speaker 1>of all things. Right, And you might think, well, the

0:18:13.800 --> 0:18:16.000
<v Speaker 1>Big Bang, that was pretty hot and dense, and so

0:18:16.040 --> 0:18:18.600
<v Speaker 1>maybe all that stuff was just made in the very beginning, yeah,

0:18:18.640 --> 0:18:22.320
<v Speaker 1>because everything was compressed, and so I would think maybe

0:18:22.359 --> 0:18:24.320
<v Speaker 1>a lot of gold was made in the Big Bang. Yeah,

0:18:24.359 --> 0:18:26.320
<v Speaker 1>but it takes a while to get the gold right,

0:18:26.359 --> 0:18:28.800
<v Speaker 1>and so, and the Big Bang turns out was pretty short.

0:18:29.240 --> 0:18:30.879
<v Speaker 1>You know, there was on a whole lot of time

0:18:30.960 --> 0:18:34.119
<v Speaker 1>there to make stuff. The when the Big Bang started,

0:18:34.160 --> 0:18:36.000
<v Speaker 1>it was really hot and dense. But also remember it

0:18:36.080 --> 0:18:38.680
<v Speaker 1>was expanding really fast, right, that's the bang part of it.

0:18:39.160 --> 0:18:41.480
<v Speaker 1>And so the universe started out really hot and dense,

0:18:41.520 --> 0:18:44.840
<v Speaker 1>but it cooled off pretty quickly. The temperature dropped very rapidly,

0:18:45.240 --> 0:18:47.439
<v Speaker 1>so there was actually only about twenty minutes. I mean,

0:18:47.440 --> 0:18:49.639
<v Speaker 1>I think it's kind of hilarious to talk about earlier

0:18:49.680 --> 0:18:52.320
<v Speaker 1>universe in terms of like minutes you know, in days

0:18:52.359 --> 0:18:53.719
<v Speaker 1>and stuff like that. It's not like there was an

0:18:53.720 --> 0:18:56.560
<v Speaker 1>Earth on the Sun back then to even create these

0:18:56.600 --> 0:18:59.600
<v Speaker 1>the meanings of these time units. But after about twenty

0:18:59.600 --> 0:19:02.520
<v Speaker 1>minutes after the Big Bang on somebody's watch, the universe

0:19:02.520 --> 0:19:05.200
<v Speaker 1>cooled down so that this kind of fusion wasn't possible anymore.

0:19:05.680 --> 0:19:07.520
<v Speaker 1>So the things that were made in the Big Bang,

0:19:07.520 --> 0:19:11.119
<v Speaker 1>of course, we're fundamental particles, you know, corks and electrons

0:19:11.119 --> 0:19:13.359
<v Speaker 1>and stuff like this, and the corks came together to

0:19:13.400 --> 0:19:16.040
<v Speaker 1>make protons, and the protons electrons found each other to

0:19:16.080 --> 0:19:18.360
<v Speaker 1>make hydrogen, and there was a little bit of time

0:19:18.440 --> 0:19:20.639
<v Speaker 1>left and they could make some helium and a few

0:19:20.760 --> 0:19:23.679
<v Speaker 1>bits of trace elements higher up to like brillium or

0:19:23.720 --> 0:19:26.240
<v Speaker 1>maybe boron and stuff. But really the Big Bang was

0:19:26.280 --> 0:19:29.040
<v Speaker 1>all about making hydrogen and helium. You're saying kind of

0:19:29.080 --> 0:19:31.879
<v Speaker 1>like the party was over before they could make gold.

0:19:32.960 --> 0:19:35.320
<v Speaker 1>They wasted a lot of time dancing, and then they

0:19:35.400 --> 0:19:36.800
<v Speaker 1>ran out of time at the end and they hadn't

0:19:36.840 --> 0:19:39.520
<v Speaker 1>really finished their homework. Yeah, kind of right. That's that's

0:19:39.520 --> 0:19:41.240
<v Speaker 1>what you're saying, is that it was intense in the

0:19:41.280 --> 0:19:44.240
<v Speaker 1>Big Bang, but then by the time that you would

0:19:44.240 --> 0:19:47.119
<v Speaker 1>get to making gold, everything was already spread out and

0:19:47.160 --> 0:19:49.080
<v Speaker 1>cooled off. Yeah, and the thing that blows my mind

0:19:49.119 --> 0:19:52.600
<v Speaker 1>the most is that the story hasn't really changed after

0:19:52.680 --> 0:19:55.600
<v Speaker 1>twenty minutes. Twenty minutes into the universe, the universe was

0:19:56.000 --> 0:20:01.400
<v Speaker 1>seventies five percent hydrogen and twenty five fish percent helium.

0:20:01.520 --> 0:20:03.919
<v Speaker 1>And that's basically the story now. I mean, there's like

0:20:04.040 --> 0:20:07.280
<v Speaker 1>one percent left over that's like other heavier stuff and that,

0:20:07.320 --> 0:20:09.159
<v Speaker 1>you know, that's the bit we're talking about. That's the

0:20:09.160 --> 0:20:11.159
<v Speaker 1>bit to make up me and you and all the

0:20:11.200 --> 0:20:14.199
<v Speaker 1>interesting stuff in the universe that's not hydrogen helium. But

0:20:14.240 --> 0:20:16.359
<v Speaker 1>it's really we're really just playing with the one percent.

0:20:16.760 --> 0:20:18.520
<v Speaker 1>Most of the stuff in the universe is still the

0:20:18.800 --> 0:20:21.080
<v Speaker 1>baryonic matter at least, we're not even talking about dark

0:20:21.119 --> 0:20:23.400
<v Speaker 1>matter and dark energy. We're talking about atomic matter. There's

0:20:23.440 --> 0:20:26.360
<v Speaker 1>still hydrogen and helium, and so all the changes, all

0:20:26.359 --> 0:20:29.200
<v Speaker 1>the kind of visible changes in the universe from you know,

0:20:29.240 --> 0:20:32.520
<v Speaker 1>a crazy cloud of nothing of chaos in two stars

0:20:32.520 --> 0:20:35.960
<v Speaker 1>and planets and galaxies. That that's you. You're saying, that's

0:20:35.960 --> 0:20:38.439
<v Speaker 1>only really the one percent. Yeah, exactly, we are the

0:20:38.480 --> 0:20:43.960
<v Speaker 1>one percent. Well, I don't know how much you know,

0:20:44.000 --> 0:20:46.520
<v Speaker 1>how my cartoons get paid, but you know, I'm more

0:20:46.520 --> 0:20:53.119
<v Speaker 1>in the five five. Okay, so in the Big Bang

0:20:53.200 --> 0:20:54.960
<v Speaker 1>and not a lot of gold was made, you're saying,

0:20:55.000 --> 0:20:58.560
<v Speaker 1>that's right. Basically you get hydrogen helium and then gravity

0:20:58.600 --> 0:21:01.359
<v Speaker 1>takes over. Right, You have these huge clouds of hydrogen

0:21:01.880 --> 0:21:04.480
<v Speaker 1>and um and they're cool and they're neutral, right, So

0:21:04.520 --> 0:21:07.800
<v Speaker 1>electromagnetism is not really doing much anymore. And then gravity

0:21:07.840 --> 0:21:09.879
<v Speaker 1>takes over and it starts to pull this stuff together.

0:21:10.440 --> 0:21:13.280
<v Speaker 1>These big nebula and these gas clouds get clumped together

0:21:13.280 --> 0:21:16.680
<v Speaker 1>by gravity until things get dense enough that they start

0:21:16.680 --> 0:21:19.960
<v Speaker 1>to heat upright, Gravitational pressure pushes on them, and you

0:21:20.040 --> 0:21:22.280
<v Speaker 1>get stars. And so that's what a lot of people said.

0:21:22.680 --> 0:21:26.840
<v Speaker 1>They said that maybe gold is made inside of stars

0:21:26.880 --> 0:21:31.800
<v Speaker 1>because stars are pretty hot and uh, and there's a

0:21:31.840 --> 0:21:34.440
<v Speaker 1>lot of pressure and there's a lot of explosives going

0:21:34.480 --> 0:21:37.840
<v Speaker 1>on inside. So is gold made inside of stars? The

0:21:37.880 --> 0:21:40.879
<v Speaker 1>answer is no, Actually, stars are not capable of making

0:21:40.920 --> 0:21:43.240
<v Speaker 1>gold um. And I understand why a lot of people

0:21:43.240 --> 0:21:45.320
<v Speaker 1>thought of that, because I think it's pretty commonly known

0:21:45.400 --> 0:21:47.840
<v Speaker 1>these days that you know, we are all all star dust,

0:21:47.920 --> 0:21:49.840
<v Speaker 1>and that's a really cool concept. You know that the

0:21:49.920 --> 0:21:52.480
<v Speaker 1>stuff that makes us up is not made here or

0:21:52.520 --> 0:21:54.480
<v Speaker 1>not made on Earth, or you know that it was

0:21:54.520 --> 0:21:57.200
<v Speaker 1>made inside a star or somewhere else a long time ago,

0:21:57.440 --> 0:21:59.520
<v Speaker 1>which then blew up. And that that part is true,

0:21:59.600 --> 0:22:01.520
<v Speaker 1>that a lot of the elements that make us up,

0:22:01.560 --> 0:22:04.240
<v Speaker 1>the heavier elements, are made inside of stars. And we'll

0:22:04.280 --> 0:22:06.040
<v Speaker 1>go through it in a little bit of detail. But

0:22:06.040 --> 0:22:08.760
<v Speaker 1>it turns out stars are not capable of making things

0:22:08.800 --> 0:22:11.440
<v Speaker 1>heavier than like nickel or iron. Wait, you're saying Carl

0:22:11.440 --> 0:22:14.400
<v Speaker 1>Sagan lied to us. Is that what you're saying here

0:22:14.400 --> 0:22:18.000
<v Speaker 1>officially on the podcast? Well, no, no, If you're not

0:22:18.119 --> 0:22:20.240
<v Speaker 1>made of gold, then Carl Sagan was correct. If you

0:22:20.280 --> 0:22:26.920
<v Speaker 1>are made of gold, then yeah, so our animatronic gold

0:22:26.960 --> 0:22:31.200
<v Speaker 1>plated AI listeners, you are exempt from Carl Sagan's wisdom. Okay,

0:22:31.359 --> 0:22:33.159
<v Speaker 1>got it, got it. It's good to know, you know,

0:22:33.600 --> 0:22:36.119
<v Speaker 1>just in case I was made out of goal. Yeah. Well,

0:22:36.119 --> 0:22:37.640
<v Speaker 1>you know, I haven't seen you in a few days,

0:22:37.680 --> 0:22:40.200
<v Speaker 1>and maybe you did get replaced by a gold plated

0:22:40.280 --> 0:22:44.119
<v Speaker 1>robot who knows. Okay, So, so you're saying a star

0:22:44.280 --> 0:22:48.400
<v Speaker 1>by itself chugging along doesn't make gold. No, And what's

0:22:48.400 --> 0:22:51.320
<v Speaker 1>happening inside a star is that it's fusing, right, it's

0:22:51.320 --> 0:22:54.040
<v Speaker 1>doing that thing we talked about earlier with pushing the

0:22:54.119 --> 0:22:57.600
<v Speaker 1>hydrogen nuclei together close enough that the strong force takes

0:22:57.640 --> 0:23:00.680
<v Speaker 1>over and it makes helium nucleus. Right, and the key

0:23:00.720 --> 0:23:03.720
<v Speaker 1>thing to understand is that that's not an energy neutral

0:23:04.000 --> 0:23:06.520
<v Speaker 1>um event. What happens when you do that is you

0:23:06.600 --> 0:23:10.479
<v Speaker 1>release energy. There's less energy in a helium nucleus than

0:23:10.520 --> 0:23:13.960
<v Speaker 1>there is in two hydrogen nuclei. So when you form

0:23:14.000 --> 0:23:17.080
<v Speaker 1>the helium nucleus, this energy left over, it releases energy.

0:23:17.119 --> 0:23:19.760
<v Speaker 1>It's like burning, right, That's what burning is. There's less

0:23:19.840 --> 0:23:22.680
<v Speaker 1>energy stored in wood ash than there is in wood,

0:23:22.680 --> 0:23:25.280
<v Speaker 1>which is why when you burn it, energy is released

0:23:25.320 --> 0:23:27.600
<v Speaker 1>as fire. It's kind of like when you take two

0:23:27.960 --> 0:23:30.880
<v Speaker 1>three year olds who are hyperactive and then smash them together.

0:23:31.280 --> 0:23:34.880
<v Speaker 1>Sitting that with an iPad iPad, Suddenly there's a lot

0:23:34.920 --> 0:23:39.080
<v Speaker 1>of leftover energy. That's right. I've never noticed them heating up,

0:23:39.160 --> 0:23:41.280
<v Speaker 1>but I'm sure. But because of conservation of energy that

0:23:41.280 --> 0:23:45.000
<v Speaker 1>that energy does go somewhere. The energy goes to the

0:23:45.040 --> 0:23:49.720
<v Speaker 1>parents or like except the how come parents are always

0:23:49.800 --> 0:23:51.480
<v Speaker 1>napping while their kids are on the iPad? I'm not

0:23:51.520 --> 0:23:54.680
<v Speaker 1>sure how the how the energy flow works. So there's

0:23:54.680 --> 0:23:57.400
<v Speaker 1>a limit to what you can make inside of a star. Yeah,

0:23:57.440 --> 0:23:59.000
<v Speaker 1>and so that's the burning of a star. Right, That's

0:23:59.040 --> 0:24:01.240
<v Speaker 1>what makes the star hot is it does this process.

0:24:01.240 --> 0:24:03.800
<v Speaker 1>It releases energy and that allows it to do more. Right,

0:24:04.160 --> 0:24:06.080
<v Speaker 1>and you can do more. You can take the helium nuclei,

0:24:06.200 --> 0:24:08.639
<v Speaker 1>you can fuse them together. And the same thing is

0:24:08.640 --> 0:24:11.600
<v Speaker 1>true that if use two helium nuclei to get something heavier,

0:24:11.680 --> 0:24:14.280
<v Speaker 1>and energy is released, and you can keep doing that

0:24:14.320 --> 0:24:16.159
<v Speaker 1>and keep doing that, and keep doing that, and energy

0:24:16.240 --> 0:24:18.600
<v Speaker 1>keeps being released and you get heavier and heavier stuff

0:24:18.640 --> 0:24:20.920
<v Speaker 1>up to like nickel or up to iron. Right, but

0:24:20.960 --> 0:24:25.320
<v Speaker 1>then it iron, something special happens, right, because iron is

0:24:25.359 --> 0:24:28.720
<v Speaker 1>kind of a special is at a special place in

0:24:28.760 --> 0:24:31.600
<v Speaker 1>the periodic table. Yeah, this is really interesting fact about

0:24:31.600 --> 0:24:34.000
<v Speaker 1>how you put nuclei together. And remember the thing that

0:24:34.040 --> 0:24:36.560
<v Speaker 1>holds a nucleus together is the strong force. Right, There's

0:24:36.560 --> 0:24:38.760
<v Speaker 1>a bunch of protons and the strong forces holding them

0:24:38.760 --> 0:24:42.800
<v Speaker 1>together by linking the corks inside the protons. But once

0:24:42.800 --> 0:24:45.280
<v Speaker 1>you get to iron, there's more energy stored in the

0:24:45.280 --> 0:24:47.800
<v Speaker 1>heavier combinations. So if you want to take two iron

0:24:47.880 --> 0:24:51.000
<v Speaker 1>nuclei and fuse them together to make whatever to iron

0:24:51.080 --> 0:24:54.040
<v Speaker 1>nuclei make, then you need to add energy. Right, you

0:24:54.080 --> 0:24:56.640
<v Speaker 1>need to pour energy into that to make the heavier thing.

0:24:56.880 --> 0:24:59.880
<v Speaker 1>So the result is that you're cooling the star instead

0:24:59.880 --> 0:25:03.880
<v Speaker 1>of burning, right, But it doesn't actually cool it does

0:25:03.960 --> 0:25:06.640
<v Speaker 1>it does absorb some of the energy from the star. Yeah,

0:25:06.680 --> 0:25:09.000
<v Speaker 1>if that happened, and it happened a lot, then it

0:25:09.000 --> 0:25:10.639
<v Speaker 1>would cool the star. And so the thing you have

0:25:10.680 --> 0:25:13.359
<v Speaker 1>to understand is that stars are like um, they're like

0:25:13.560 --> 0:25:16.560
<v Speaker 1>a balance, right. They're fusing all the time. They're making

0:25:16.600 --> 0:25:19.520
<v Speaker 1>this heavier stuff and that's releasing energy. But then that

0:25:19.520 --> 0:25:22.159
<v Speaker 1>stuff is also getting blown apart because it's an incredible

0:25:22.160 --> 0:25:24.760
<v Speaker 1>place in there is all these photons. You have photo disintegration.

0:25:25.119 --> 0:25:27.119
<v Speaker 1>So you're like make something heavy and then you blow

0:25:27.119 --> 0:25:29.040
<v Speaker 1>it up because of heavy photons or hitting it. Then

0:25:29.040 --> 0:25:30.720
<v Speaker 1>you make something heavy and you blow it up, and

0:25:30.720 --> 0:25:34.400
<v Speaker 1>it's sort of gradually accumulating heavier and heavier stuff, right,

0:25:34.520 --> 0:25:36.280
<v Speaker 1>But you also got to keep the star burning. If

0:25:36.280 --> 0:25:39.160
<v Speaker 1>the star doesn't stay hot enough, then it collapses. Right.

0:25:39.200 --> 0:25:42.439
<v Speaker 1>Then it's you can no longer support itself from gravity winds.

0:25:42.920 --> 0:25:45.399
<v Speaker 1>So if you start getting too much heavy stuff like

0:25:45.440 --> 0:25:48.280
<v Speaker 1>the iron and the nickel and the stuff that if

0:25:48.320 --> 0:25:51.000
<v Speaker 1>you do fuse it, it it costs you energy. That's the

0:25:51.040 --> 0:25:53.000
<v Speaker 1>death knell of a star. That's when a star starts

0:25:53.040 --> 0:25:56.159
<v Speaker 1>to die. Yeah. So it's like it burns all its fuel,

0:25:56.320 --> 0:25:58.399
<v Speaker 1>it turns it into iron, and then it can't do

0:25:58.480 --> 0:26:01.040
<v Speaker 1>anything with the iron anymore. Exactly to do something with

0:26:01.080 --> 0:26:03.600
<v Speaker 1>the iron take some somebody adding energy, and so that's

0:26:03.600 --> 0:26:05.840
<v Speaker 1>when the star starts to go out. Right, When it's

0:26:05.880 --> 0:26:08.800
<v Speaker 1>fuel is no longer fuel, it's something that requires work

0:26:08.840 --> 0:26:10.800
<v Speaker 1>instead of releasing energy. It's kind of like when you

0:26:10.920 --> 0:26:13.840
<v Speaker 1>when you burn a fire, right, would you throw the

0:26:13.840 --> 0:26:16.960
<v Speaker 1>logs in and eventually the logs turn into ash and

0:26:17.520 --> 0:26:19.320
<v Speaker 1>you can't do anything with that, right, you can't burn

0:26:19.359 --> 0:26:21.280
<v Speaker 1>it anymore, that's right. Yeah, you could do something with

0:26:21.320 --> 0:26:23.680
<v Speaker 1>the ash, but it might require energy to do it, right,

0:26:23.800 --> 0:26:25.640
<v Speaker 1>So you don't have that. It's not a self sustaining

0:26:25.680 --> 0:26:29.000
<v Speaker 1>thing anymore. It's a self extinguishing thing. Yeah, So your

0:26:29.040 --> 0:26:30.959
<v Speaker 1>fire goes out. Yeah, and so your fire goes out,

0:26:31.000 --> 0:26:33.960
<v Speaker 1>and that's what happens. Right, stars burn, they make heavier

0:26:33.960 --> 0:26:36.239
<v Speaker 1>stuff that they can't burn anymore, so they've used up

0:26:36.240 --> 0:26:38.600
<v Speaker 1>their fuel and then they go out and you know,

0:26:38.600 --> 0:26:41.639
<v Speaker 1>they spread that stuff back out into the universe. There's

0:26:41.680 --> 0:26:44.440
<v Speaker 1>the solar wind right, they're spewing particles out from the sun,

0:26:44.600 --> 0:26:46.360
<v Speaker 1>from the star all the time. That spreads them out,

0:26:46.840 --> 0:26:50.159
<v Speaker 1>or they go supernova and you know, they collapse and

0:26:50.200 --> 0:26:52.840
<v Speaker 1>then explode and they spew all their stuff out into

0:26:52.880 --> 0:26:56.280
<v Speaker 1>the universe. And one really cool thing is that then

0:26:56.320 --> 0:26:59.480
<v Speaker 1>that stuff gets gathered back together to make a new star.

0:27:00.040 --> 0:27:02.800
<v Speaker 1>So we've had these cycles of stars. We had original

0:27:02.880 --> 0:27:06.600
<v Speaker 1>first stars that just burned hydrogen and turned into helium,

0:27:06.680 --> 0:27:08.960
<v Speaker 1>and then those blew up, you know, and we had

0:27:08.960 --> 0:27:12.560
<v Speaker 1>different kinds of stars that primarily burned helium and heavier stuff,

0:27:12.800 --> 0:27:14.960
<v Speaker 1>and those blew up, and then we had different kind

0:27:14.960 --> 0:27:16.919
<v Speaker 1>of stars. And so it takes a few cycles of

0:27:16.960 --> 0:27:20.000
<v Speaker 1>stars to even get up to stars capable of making

0:27:20.040 --> 0:27:25.000
<v Speaker 1>things like iron and nickel. Oh, I say, and those

0:27:25.000 --> 0:27:28.040
<v Speaker 1>first stars are no longer even existing, Like, we haven't

0:27:28.080 --> 0:27:29.960
<v Speaker 1>seen any of those first stars and the ones that

0:27:30.000 --> 0:27:33.399
<v Speaker 1>are pure hydrogen. Yeah, the first cycle of stars, the

0:27:33.400 --> 0:27:36.960
<v Speaker 1>original stars, the o G stars, Right, we've we've recently

0:27:37.080 --> 0:27:39.919
<v Speaker 1>thought we might have seen a hint of evidence of them,

0:27:39.960 --> 0:27:42.280
<v Speaker 1>but nobody's ever actually seen them directly. They're so old,

0:27:42.560 --> 0:27:45.480
<v Speaker 1>they happened so long ago, they're very difficult to see.

0:27:45.560 --> 0:27:47.960
<v Speaker 1>That's a whole other interesting podcast about the history of

0:27:48.000 --> 0:27:51.680
<v Speaker 1>stars that we know of nobody has seen. Yeah, that's right.

0:27:52.160 --> 0:27:54.760
<v Speaker 1>And the other fascinating fact that so many interesting things

0:27:54.760 --> 0:27:57.040
<v Speaker 1>about this is that most of the really heavy stuff,

0:27:57.040 --> 0:27:59.119
<v Speaker 1>like the iron and the nickel, is made in the

0:27:59.240 --> 0:28:01.920
<v Speaker 1>last few moments of a star's life. Like, those things

0:28:01.920 --> 0:28:04.040
<v Speaker 1>are hard to make. Even though you know it is

0:28:04.160 --> 0:28:07.840
<v Speaker 1>energetically favorable to produce iron, it's a really small effect,

0:28:07.840 --> 0:28:09.120
<v Speaker 1>and so you don't make a lot of it until

0:28:09.160 --> 0:28:12.080
<v Speaker 1>the last few moments. Most of that stuff happens just

0:28:12.240 --> 0:28:14.960
<v Speaker 1>before the supernova, as that the outer bits of the

0:28:14.960 --> 0:28:18.000
<v Speaker 1>star collapsing, those are the perfect times to make iron

0:28:18.000 --> 0:28:20.240
<v Speaker 1>and nickel. So like most of the iron and the

0:28:20.320 --> 0:28:22.959
<v Speaker 1>nickel in the universe was made in the last few moments,

0:28:23.000 --> 0:28:26.440
<v Speaker 1>just before star went supernova. Yeah, and but that's kind

0:28:26.440 --> 0:28:29.320
<v Speaker 1>of the limit, right, yeah, exactly. These stars can't make

0:28:29.359 --> 0:28:31.879
<v Speaker 1>things that are heavier. So for a long time people

0:28:31.880 --> 0:28:34.560
<v Speaker 1>wonder It's like, well, we have this great model of stars.

0:28:34.600 --> 0:28:37.160
<v Speaker 1>We can explain how they made iron, how they made nickel,

0:28:37.200 --> 0:28:39.640
<v Speaker 1>all this stuff, but what about this other stuff we see?

0:28:39.680 --> 0:28:43.960
<v Speaker 1>Because there is stuff in the universe, it's heavier uranium, plutonium, gold,

0:28:44.280 --> 0:28:46.480
<v Speaker 1>all this stuff. Where does that come from? Well, let's

0:28:46.520 --> 0:28:49.720
<v Speaker 1>get into that. Let's get into whether supernova are able

0:28:49.760 --> 0:28:52.160
<v Speaker 1>to make these things and whether they can make gold.

0:28:52.560 --> 0:29:08.840
<v Speaker 1>But first let's take a quick break, alright, so start

0:29:08.920 --> 0:29:12.120
<v Speaker 1>checking along. Can't make gold. I can only sort of

0:29:12.120 --> 0:29:14.240
<v Speaker 1>go up to iron. And that's even only when it

0:29:14.400 --> 0:29:17.080
<v Speaker 1>blows up, right, Yeah, that's right after a few cycles

0:29:17.120 --> 0:29:21.440
<v Speaker 1>and during the blow up. So then how does gold

0:29:21.520 --> 0:29:24.360
<v Speaker 1>get made? It's not in supernova's. It's not in supernova.

0:29:24.400 --> 0:29:27.920
<v Speaker 1>Supernovas are responsible for like the heaviest stuff that stars

0:29:27.960 --> 0:29:29.920
<v Speaker 1>can make, right, And people have done a lot of

0:29:29.920 --> 0:29:32.400
<v Speaker 1>extensive work on this and modeling and trying to understand

0:29:32.680 --> 0:29:36.280
<v Speaker 1>are there weird kinds of supernovas? Are their special circumstances

0:29:36.640 --> 0:29:41.560
<v Speaker 1>under which super dupernovas Meganova's. There actually are things called

0:29:41.800 --> 0:29:46.960
<v Speaker 1>killing novas and hypernovas and stuff like that. That sounds

0:29:46.960 --> 0:29:49.520
<v Speaker 1>like a hell of a Helennova. Hell, that's the California

0:29:49.600 --> 0:29:53.800
<v Speaker 1>version Helenova or HELENNOVAA. It's one of the most dramatic

0:29:53.840 --> 0:29:57.120
<v Speaker 1>events in the universe that's responsible for making gold and

0:29:57.200 --> 0:30:00.680
<v Speaker 1>platinum and all that heavy stuff. And we only recently

0:30:00.680 --> 0:30:03.040
<v Speaker 1>figured out what this is and what happens is not

0:30:03.160 --> 0:30:05.560
<v Speaker 1>the collapse of a single star into like a neutron

0:30:05.640 --> 0:30:09.280
<v Speaker 1>star or something really heavy. It's when two stars collide.

0:30:09.800 --> 0:30:12.400
<v Speaker 1>So sometimes you'll have like two neutron stars that are

0:30:12.440 --> 0:30:15.280
<v Speaker 1>near each other. And remember neutron stars with this really,

0:30:15.280 --> 0:30:17.760
<v Speaker 1>really dense stuff. We had an episode recently about density,

0:30:18.160 --> 0:30:21.040
<v Speaker 1>and you know, like a teaspoon of neutron star weighs

0:30:21.040 --> 0:30:24.400
<v Speaker 1>as much as like a million Eiffel towers. Right, it's ridiculous.

0:30:24.640 --> 0:30:28.600
<v Speaker 1>So already you have this crazy intense environment. Now imagine

0:30:28.640 --> 0:30:31.280
<v Speaker 1>two of those things and they're near each other, and

0:30:31.320 --> 0:30:33.960
<v Speaker 1>they're orbiting each other, and they're pulling each other together,

0:30:34.240 --> 0:30:37.840
<v Speaker 1>and eventually, boom, they collide. They collapse into one object.

0:30:38.040 --> 0:30:40.280
<v Speaker 1>That's how gold is made. That's the only way we know.

0:30:40.680 --> 0:30:43.280
<v Speaker 1>That's the only way we know. The gold and all

0:30:43.600 --> 0:30:47.080
<v Speaker 1>the other stuff heavier than iron is primarily made in

0:30:47.160 --> 0:30:51.280
<v Speaker 1>the collapses of neutron stars. And like, it's a crazy idea, right,

0:30:51.560 --> 0:30:54.520
<v Speaker 1>And for a long time people thought, but neutron star collapses,

0:30:54.560 --> 0:30:56.600
<v Speaker 1>like how often can that happen? Can there really be

0:30:56.760 --> 0:30:59.200
<v Speaker 1>enough of that to make all the gold? But they

0:30:59.200 --> 0:31:02.080
<v Speaker 1>collapse and and they explode out into the universe. Because

0:31:02.120 --> 0:31:05.880
<v Speaker 1>if it collapses, doesn't keep all the goal inside of it. Yeah,

0:31:05.920 --> 0:31:08.080
<v Speaker 1>they collide, they make gold, and then some a lot

0:31:08.080 --> 0:31:11.280
<v Speaker 1>of it is ejected. Yeah, so they explode, and uh,

0:31:11.440 --> 0:31:15.920
<v Speaker 1>we discover this recently because we saw gravitational waves. These

0:31:15.920 --> 0:31:19.320
<v Speaker 1>things are heavy enough, they're big enough, and they're moving

0:31:19.440 --> 0:31:23.480
<v Speaker 1>fast enough, they're accelerating enough they actually cause gravitational waves,

0:31:23.600 --> 0:31:26.880
<v Speaker 1>these ripples in space and time itself. We had a

0:31:26.880 --> 0:31:29.160
<v Speaker 1>whole podcast episode about that about how we saw like

0:31:29.440 --> 0:31:33.480
<v Speaker 1>black holes merging and neutron star collisions, and we see

0:31:33.480 --> 0:31:36.080
<v Speaker 1>this because they're so heavy that they make these ripples

0:31:36.080 --> 0:31:39.920
<v Speaker 1>in space. Remember, really massive stuff bend space. That's what

0:31:40.000 --> 0:31:42.080
<v Speaker 1>gravity is. And so if you have something like that

0:31:42.160 --> 0:31:46.120
<v Speaker 1>moving really quickly accelerating, then it's gravitational field is wiggling,

0:31:46.200 --> 0:31:48.760
<v Speaker 1>and it's wiggling in a way to send waves through

0:31:48.840 --> 0:31:51.880
<v Speaker 1>space that we can actually detect. Yeah. So, um, so

0:31:51.920 --> 0:31:54.640
<v Speaker 1>that's why gold is so rare. It's that it can

0:31:54.760 --> 0:31:59.000
<v Speaker 1>only be made in these super rare events, which is

0:31:59.160 --> 0:32:02.240
<v Speaker 1>to neutrons ares which just happened to be close enough

0:32:02.240 --> 0:32:04.280
<v Speaker 1>to each other to merge. That's right. The thing that

0:32:04.360 --> 0:32:06.440
<v Speaker 1>it's interesting is that it's not as rare as we

0:32:06.480 --> 0:32:11.000
<v Speaker 1>thought before we turned on Ligo, this gravitational wave detector.

0:32:11.400 --> 0:32:13.280
<v Speaker 1>They turned it on, they knew what it could see,

0:32:13.400 --> 0:32:15.400
<v Speaker 1>but what they didn't know is how often is their

0:32:15.400 --> 0:32:19.040
<v Speaker 1>stuff to see. Like, you build this amazing telescope, you're

0:32:19.040 --> 0:32:21.760
<v Speaker 1>this gravitational wave detector. You're looking out into the universe

0:32:21.800 --> 0:32:23.520
<v Speaker 1>with sort of a new set of eyes for the

0:32:23.600 --> 0:32:25.880
<v Speaker 1>first time. You don't know if it's going to be

0:32:25.960 --> 0:32:28.560
<v Speaker 1>like a big party or total darkness. We just really

0:32:28.560 --> 0:32:31.040
<v Speaker 1>had no idea. And the cool thing is that just

0:32:31.160 --> 0:32:34.240
<v Speaker 1>after they turned it on, boom they saw a gravitational wave,

0:32:34.280 --> 0:32:36.120
<v Speaker 1>and then left. Next week, boom they saw another one.

0:32:36.320 --> 0:32:38.200
<v Speaker 1>So it turns out this stuff happens a little bit

0:32:38.200 --> 0:32:41.800
<v Speaker 1>more often than people were we're thinking. So it's not

0:32:41.960 --> 0:32:44.480
<v Speaker 1>that unlikely to see new dron stars, which is why

0:32:44.520 --> 0:32:47.880
<v Speaker 1>gold is rare, but not like impossible to find or

0:32:47.880 --> 0:32:50.840
<v Speaker 1>anything heavier than gold, right, because anything heavier than gold

0:32:50.920 --> 0:32:53.960
<v Speaker 1>you also need these rare events. Yeah, exactly. All the plutonium,

0:32:53.960 --> 0:32:56.160
<v Speaker 1>all the uranium, all that kind of stuff that's made

0:32:56.160 --> 0:32:59.920
<v Speaker 1>that's heavier than gold was created in this incredible cosm

0:33:00.120 --> 0:33:03.320
<v Speaker 1>collisions of neutron stars. And we know that because we

0:33:03.360 --> 0:33:05.440
<v Speaker 1>saw one recently, So we saw it with a gravitational

0:33:05.480 --> 0:33:08.880
<v Speaker 1>wave detector. We also saw the collision using other telescopes.

0:33:09.000 --> 0:33:11.520
<v Speaker 1>So this is called multi messenger because you see the

0:33:11.560 --> 0:33:14.800
<v Speaker 1>same event with light and with gravitational waves. And then

0:33:14.840 --> 0:33:17.600
<v Speaker 1>we could look at what happened and and look at

0:33:17.680 --> 0:33:20.000
<v Speaker 1>you know, the the emissions of the stuff nearby, and

0:33:20.040 --> 0:33:22.880
<v Speaker 1>we could see that there was gold just afterwards where

0:33:22.880 --> 0:33:26.560
<v Speaker 1>there wasn't gold before. Oh no kidding, It got shiny

0:33:26.960 --> 0:33:29.800
<v Speaker 1>like it twinkled a little extra. All these bracelets were

0:33:29.840 --> 0:33:32.160
<v Speaker 1>made and all these nice rings, you know, stuff I

0:33:32.160 --> 0:33:34.720
<v Speaker 1>think would be really wonderful. Um. Now you could see

0:33:34.800 --> 0:33:36.959
<v Speaker 1>because of the way it absorbs light from behind it

0:33:37.000 --> 0:33:40.160
<v Speaker 1>and the midst light. Gold has a characteristic signature, so

0:33:40.200 --> 0:33:43.000
<v Speaker 1>we could see gold having been made. Pretty awesome. Kind

0:33:43.000 --> 0:33:44.760
<v Speaker 1>of like if you close your eyes and you're listening

0:33:44.760 --> 0:33:47.360
<v Speaker 1>out into the universe, you will hear gold being made

0:33:47.520 --> 0:33:51.920
<v Speaker 1>kind of right like pop pop pop pop um. If

0:33:51.960 --> 0:33:54.120
<v Speaker 1>you close your eyes and listen to the universe, I

0:33:54.120 --> 0:33:57.960
<v Speaker 1>don't know what you're gonna hear, um, but yeah there is. Yeah,

0:33:58.000 --> 0:34:00.360
<v Speaker 1>if you listen to the gravitational waves, you hear these

0:34:00.440 --> 0:34:04.040
<v Speaker 1>crazy events that that that the is wear gold and

0:34:04.040 --> 0:34:05.920
<v Speaker 1>heavy stuff is made. So it's not made in the

0:34:05.960 --> 0:34:08.800
<v Speaker 1>Earth's crust, and it's not made in the normal burning

0:34:08.800 --> 0:34:12.360
<v Speaker 1>of stars. It's only made in these special crazy collisions

0:34:12.360 --> 0:34:14.799
<v Speaker 1>of two dead stars. So I feel like that makes

0:34:14.840 --> 0:34:18.360
<v Speaker 1>it even more special than diamonds, you know, like diamonds

0:34:18.520 --> 0:34:22.240
<v Speaker 1>just made here on Earth. But gold, that's that's only

0:34:22.280 --> 0:34:26.920
<v Speaker 1>made in in the uh the marriage of two giants

0:34:27.280 --> 0:34:29.319
<v Speaker 1>neutron stars. No, I think you're right, and I think

0:34:29.760 --> 0:34:31.799
<v Speaker 1>you know, the De Beers Corporation will not be very

0:34:31.800 --> 0:34:34.759
<v Speaker 1>interested in sponsoring this podcast. But diamonds, you're right, they're

0:34:34.800 --> 0:34:36.840
<v Speaker 1>not that special. You know, they're just created by a

0:34:36.880 --> 0:34:38.920
<v Speaker 1>lot of pressure here in the center of the Earth.

0:34:38.960 --> 0:34:41.000
<v Speaker 1>But we are not capable of making gold on Earth.

0:34:41.000 --> 0:34:44.439
<v Speaker 1>There's certainly not nowhere in their solar system are there

0:34:44.440 --> 0:34:47.720
<v Speaker 1>the conditions to make gold, and so it is pretty unusual.

0:34:47.800 --> 0:34:49.200
<v Speaker 1>But you know, but but you said you can make

0:34:49.239 --> 0:34:53.000
<v Speaker 1>that at the large hadron collider. You're right, You're right,

0:34:53.040 --> 0:34:54.799
<v Speaker 1>we can make it at a large hadron collider. So

0:34:55.000 --> 0:34:57.920
<v Speaker 1>naturally produced gold, you know, fusing of lighter stuff. What

0:34:58.000 --> 0:35:00.200
<v Speaker 1>we do with a large agron collider. Actually, as we

0:35:00.200 --> 0:35:02.080
<v Speaker 1>can take gold, we can take lead, which is heavier

0:35:02.080 --> 0:35:04.759
<v Speaker 1>than gold, and we can strip off some of the protons, right,

0:35:04.800 --> 0:35:07.400
<v Speaker 1>you can shoot like neutrons and stuff at it to

0:35:07.480 --> 0:35:09.600
<v Speaker 1>sort of break it apart and take off some of

0:35:09.640 --> 0:35:12.799
<v Speaker 1>the protons to turn some lead into some gold. But

0:35:12.800 --> 0:35:14.800
<v Speaker 1>we can only do it in a really really low levels,

0:35:14.880 --> 0:35:17.440
<v Speaker 1>Like you can't take a block of lead, and you

0:35:17.480 --> 0:35:19.960
<v Speaker 1>need to turn each atom one at a time into gold,

0:35:19.960 --> 0:35:24.120
<v Speaker 1>which is why we cost a quadrillion dollars. I see,

0:35:24.160 --> 0:35:26.360
<v Speaker 1>you make it the other way. You don't fuse it together.

0:35:26.560 --> 0:35:28.960
<v Speaker 1>You strip down lead to make gold. Yeah, so it's

0:35:28.960 --> 0:35:31.080
<v Speaker 1>pretty much cheating because the lead also was made in

0:35:31.120 --> 0:35:33.359
<v Speaker 1>the collision of neutron stars, right, so we're taking that

0:35:33.440 --> 0:35:35.960
<v Speaker 1>we're just like turning it into gold. So it's like

0:35:36.160 --> 0:35:38.920
<v Speaker 1>it's a very unsatisfying sort of monkey paw answer, right, Like,

0:35:38.960 --> 0:35:41.400
<v Speaker 1>can you make lead into gold? Yes? So Carl Sagan

0:35:41.440 --> 0:35:44.279
<v Speaker 1>didn't lie to us. You did. That's a fairly safe

0:35:44.320 --> 0:35:49.160
<v Speaker 1>assumption in general. Um, but I don't think I've said

0:35:49.200 --> 0:35:51.759
<v Speaker 1>anything incorrect. We can turn lead into gold, it's just

0:35:51.840 --> 0:35:54.080
<v Speaker 1>not the most of the goal that you find is

0:35:54.120 --> 0:35:56.080
<v Speaker 1>not made in the large head on colider, all right,

0:35:56.200 --> 0:35:58.160
<v Speaker 1>So that's pretty pretty cool to know. So the next

0:35:58.160 --> 0:36:02.080
<v Speaker 1>time you see your wedding maybe, or you're pendant or

0:36:02.160 --> 0:36:04.600
<v Speaker 1>something made out of gold out there, you should think

0:36:04.640 --> 0:36:08.400
<v Speaker 1>about that. It wasn't made here on Earth. It wasn't

0:36:08.719 --> 0:36:11.600
<v Speaker 1>made inside of a star. It was made in a giant,

0:36:12.520 --> 0:36:17.799
<v Speaker 1>really cataclysmic, crazy explosion of two giants neutron stars. That's right.

0:36:17.920 --> 0:36:21.439
<v Speaker 1>Two neutron stars gave their lives so that you could

0:36:21.520 --> 0:36:23.880
<v Speaker 1>have that ring with that bracelet and give it to

0:36:23.920 --> 0:36:26.360
<v Speaker 1>your special person. So you know, I think for a

0:36:26.400 --> 0:36:29.200
<v Speaker 1>moment about what they sacrificed and then exploited out into

0:36:29.200 --> 0:36:32.879
<v Speaker 1>space and somehow, some way it made it into here

0:36:33.239 --> 0:36:36.600
<v Speaker 1>and into the Earth and into your finger. Yeah. So

0:36:36.760 --> 0:36:40.200
<v Speaker 1>every atom of gold has a really interesting life story,

0:36:40.320 --> 0:36:43.239
<v Speaker 1>much more interesting than you write. Is existed for a

0:36:43.320 --> 0:36:48.680
<v Speaker 1>long time. Well, I was made in the large hadron colliders.

0:36:49.120 --> 0:36:51.759
<v Speaker 1>You know, that's why you're so shiny and brilliant. No,

0:36:52.000 --> 0:36:54.600
<v Speaker 1>every element you know that that you're made out of

0:36:55.120 --> 0:36:57.040
<v Speaker 1>is pretty stable. They were not made on Earth, they

0:36:57.040 --> 0:36:59.400
<v Speaker 1>were not rearranged on Earth. They've been that element for

0:36:59.560 --> 0:37:02.919
<v Speaker 1>billion of years. They've survived being created inside a star

0:37:03.040 --> 0:37:05.719
<v Speaker 1>or inside the collisions of neutron stars, and they've had

0:37:05.760 --> 0:37:08.759
<v Speaker 1>their personality for billions of years and they're just temporarily

0:37:08.800 --> 0:37:12.160
<v Speaker 1>for this brief moment part of you. All right, Well,

0:37:12.200 --> 0:37:15.160
<v Speaker 1>we hope you enjoyed that discussion and learn a little

0:37:15.160 --> 0:37:18.440
<v Speaker 1>bit about where the heavy elements come from. And I

0:37:18.480 --> 0:37:21.600
<v Speaker 1>hope you enjoyed that golden neuggative of intellectual thought. And

0:37:21.640 --> 0:37:23.400
<v Speaker 1>if you want to inject some gold and send it

0:37:23.400 --> 0:37:26.279
<v Speaker 1>to us, send it to me my addresses. That's right.

0:37:26.560 --> 0:37:28.400
<v Speaker 1>Thanks for tuning in. And if you have a question

0:37:28.440 --> 0:37:32.400
<v Speaker 1>about our crazy, golden, beautiful, nasty, weird universe, send it

0:37:32.400 --> 0:37:35.279
<v Speaker 1>to us. I have questions at Daniel and Jorge dot com.

0:37:35.440 --> 0:37:38.040
<v Speaker 1>We love your emails. See you next time. All right,

0:37:38.080 --> 0:37:48.040
<v Speaker 1>thanks for listening. If you still have a question after

0:37:48.120 --> 0:37:51.239
<v Speaker 1>listening to all these explanations, please drop us a line.

0:37:51.280 --> 0:37:53.400
<v Speaker 1>We'd love to hear from you. You can find us

0:37:53.440 --> 0:37:57.239
<v Speaker 1>at Facebook, Twitter, and Instagram at Daniel and Jorge that's

0:37:57.280 --> 0:38:00.640
<v Speaker 1>one word, or email us at Feedback at Daniel and

0:38:00.760 --> 0:38:04.200
<v Speaker 1>Jorge dot com. Thanks for listening, and remember that Daniel

0:38:04.239 --> 0:38:06.719
<v Speaker 1>and Jorge Explain the Universe is a production of I

0:38:06.960 --> 0:38:10.399
<v Speaker 1>Heart Radio. For more podcast from my Heart Radio, visit

0:38:10.440 --> 0:38:13.920
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0:38:14.040 --> 0:38:19.440
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