WEBVTT - We Are Stardust

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<v Speaker 1>Welcome to Stuff to Blow Your Mind from how Stuff

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<v Speaker 1>Works dot com. Hey, welcome to Stuff to Blow your Mind.

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<v Speaker 1>My name is Robert Lamb and I'm Julie Douglas. I

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<v Speaker 1>find it interesting, Julie, that that we can as humans

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<v Speaker 1>can take solace and find some sort of spiritual almost

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<v Speaker 1>spiritual comfort in the idea of a supernova, which is

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<v Speaker 1>something that's worth discussing this podcast that is, on one level,

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<v Speaker 1>is so far removed from us. I mean, it's a

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<v Speaker 1>it's a it's a Titanic event, one of the most

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<v Speaker 1>powerful events that that regularly occurs in the universe, and

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<v Speaker 1>it takes place vast distances of both time and space,

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<v Speaker 1>and yet we can find something in there to connect

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<v Speaker 1>with and to to to take solace in and and

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<v Speaker 1>leave it feeling better about our place in this vast

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<v Speaker 1>sea of cosmos. What's the life stile goal in Macro Right,

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<v Speaker 1>it's a dying star and it's absolutely brilliant. Right, it's

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<v Speaker 1>visual fireworks. It's a star that suddenly increases greatly in

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<v Speaker 1>brightness because of a catastrophic explosion that ejects most of

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<v Speaker 1>its mass. So it's a dramatic storyline. So because you

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<v Speaker 1>know how could you not be caught by this, this

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<v Speaker 1>thing that is imploding and ejecting most of its mass. Yeah,

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<v Speaker 1>I mean it's the death of a star. It's kind

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<v Speaker 1>of like the death of a guy. Like we're totally

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<v Speaker 1>into that idea as well. Yeah yeah, um. And it's

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<v Speaker 1>really powerful and the core of a massive star runs

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<v Speaker 1>out of nuclear fuel, right, this is this is the

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<v Speaker 1>sad part. I guess you could sit sad. It's not

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<v Speaker 1>so much sad and collapses under its own gravity to

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<v Speaker 1>form an ultra dense object known as a neutron star.

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<v Speaker 1>But only so much material can compress into the neutron stars,

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<v Speaker 1>so some of the original stars collapsing gaseous outer layers

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<v Speaker 1>can't fit, so instead they sort of bounce off the

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<v Speaker 1>neutron star, and then this triggers a shock wave that

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<v Speaker 1>bulldozes back were the outer layers and blows the star

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<v Speaker 1>to smithereens. Yeah. The way, the way I really like

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<v Speaker 1>to think about it is basically, you have a situation

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<v Speaker 1>where a working star, a functional living star, is having

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<v Speaker 1>to burn massive amounts of energy to expand against the

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<v Speaker 1>force of its own crushing gravity. So I like to

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<v Speaker 1>think of it like a poorly run but well financed business,

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<v Speaker 1>you know, where there's a lot of moneys, a lot

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<v Speaker 1>of money is being spent to keep keep up these offices.

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<v Speaker 1>It's like, uh, the company that Tom have havever heard

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<v Speaker 1>a season sorry his character in Parks and Rector. It's

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<v Speaker 1>just spen in all this just mad money and they're

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<v Speaker 1>not actually bringing money in, but all this money is

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<v Speaker 1>being spent to keep it out. And then what happens

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<v Speaker 1>was it Tommy Fresh Industries or something like it was

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<v Speaker 1>something along those lines, and they were hiring NBA stars

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<v Speaker 1>just hang out at the off the hands from cocktails

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<v Speaker 1>to people, um and uh. And then of course they

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<v Speaker 1>run out of money and it just collapses. And that's

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<v Speaker 1>kind of what happens with with the Star. Um. It

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<v Speaker 1>reaches the point where there's nothing else to burn to

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<v Speaker 1>sustain it, to to to keep it fight against its

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<v Speaker 1>own massive gravity. And when that happens, it collapses. In

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<v Speaker 1>some cases you end up with a singularity, you end

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<v Speaker 1>up with a black hole. But in other cases you

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<v Speaker 1>end up with this enormous explosion that Jettison's uh, you know,

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<v Speaker 1>all the shrimp cocktail and NBA stars elsewhere it happened

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<v Speaker 1>to the universe. Yeah, and it's really helpful to use

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<v Speaker 1>these supernova nova plural to actually study the universe, right,

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<v Speaker 1>because it's something that we can see, something that we

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<v Speaker 1>know about. UM. It used to be that we thought

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<v Speaker 1>this was terribly uncommon, but it turns out that it is. Uh,

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<v Speaker 1>these stars exploding, this very violent catastrophic events are more

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<v Speaker 1>common than we thought. UM. And again just so you

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<v Speaker 1>guys understand, um, how immense this is. They emit in

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<v Speaker 1>a few seconds and energy equivalent to what they've emitted

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<v Speaker 1>for their entire lifetime. UM. Our galaxy is about twelve

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<v Speaker 1>billion years old, so we have seen well not you

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<v Speaker 1>and I when you guys out there personally, but two

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<v Speaker 1>hundred million stars exploded during its lifetime. Right. Yeah, I

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<v Speaker 1>was looking at a at a study where from April

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<v Speaker 1>two thousand three to August two thousand and six, the Canada, France,

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<v Speaker 1>Hawaii telescope watch four parts of the sky. Each section

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<v Speaker 1>that it looked at was about sixteen times the area

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<v Speaker 1>of a full moon, and which is roughly one of

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<v Speaker 1>the entire sky. And during that time period they observed

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<v Speaker 1>two hundred forty one Type one A supernova. So just

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<v Speaker 1>to give you an idea of like how often these

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<v Speaker 1>things are happening. Um. And actually I did a blog post.

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<v Speaker 1>The guy did a neat thing where he he set

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<v Speaker 1>this to music, like he sped it up. And then

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<v Speaker 1>every time there's a supernova and one of these quadrants

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<v Speaker 1>that lights up and there's a note and it's really cool. Yeah,

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<v Speaker 1>and it's it's a great event. I believe in nineteen

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<v Speaker 1>eighty seven they were actually able to uh witnessed an

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<v Speaker 1>explosion of the nineteen seven nine seven a supernova which

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<v Speaker 1>they had had their telescopes trained on. Uh. But you know,

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<v Speaker 1>I'm vniched down. They actually blew up and they were

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<v Speaker 1>able to study it quite carefully. Um. But again it

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<v Speaker 1>brings back to this this whole idea that you put forth,

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<v Speaker 1>which is, you know, we can't help but look up

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<v Speaker 1>in the night sky and feel connected. And now that

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<v Speaker 1>we know a lot more about a supernova, we can

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<v Speaker 1>better understand that these raw materials hurling out in the

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<v Speaker 1>universe are actually very deeply connected to our existence. Yeah,

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<v Speaker 1>which is I mean you look back at like just

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<v Speaker 1>sort of religious and spiritual ideas. I mean everybody, it's

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<v Speaker 1>probably not everybody, but but you see a lot of

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<v Speaker 1>people into the idea of being, say, a child of

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<v Speaker 1>God or being or having some sort of a connection

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<v Speaker 1>to a spiritual or heavenly realm. So strip away religious

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<v Speaker 1>and spirituality and uh and just look at science. And

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<v Speaker 1>that's what what we're looking at here, the idea that

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<v Speaker 1>there is a connection between these titanic and timeless events,

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<v Speaker 1>uh playing out in the cosmos and our own small,

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<v Speaker 1>uh little lives. Yeah, and let's talk just a little

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<v Speaker 1>bit about sort of the nuts and bolts of the

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<v Speaker 1>supernervo so that we can all sort of get a

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<v Speaker 1>firm understanding of what's happening at the center of a supernova.

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<v Speaker 1>So a star can go supernova in one of two waves.

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<v Speaker 1>There's type one supernova, in which a star accumulates matter

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<v Speaker 1>from a nearby neighbor until runaway nuclear reaction nick nites.

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<v Speaker 1>And then there's the type two supernova. And this is

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<v Speaker 1>sort of the more spectacular version, in which a star

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<v Speaker 1>runs out of nuclear fuel and collapses under its own gravity, right,

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<v Speaker 1>which is the kind of the the collapsing business analogy

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<v Speaker 1>I used earlier. Yes, Yes, what happens is that as

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<v Speaker 1>it begins to die, it eventually runs out of hydrogen

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<v Speaker 1>and then helium fuel at its core. So gradually heavier

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<v Speaker 1>elements build up at the center, and then it becomes

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<v Speaker 1>layered like an onion, with elements becoming lighter towards the

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<v Speaker 1>outside of the star. And this is where we start

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<v Speaker 1>to see the spiraling effect of those materials um throwing

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<v Speaker 1>off of the star. Basically, so that shock wave that

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<v Speaker 1>we talked about earlier, that actually shoots out the whole

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<v Speaker 1>outer part of the star, and the shock waves compressed

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<v Speaker 1>the gas and space, which triggers new star formations. Okay,

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<v Speaker 1>which is really key to us into the universe. Right,

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<v Speaker 1>you have situations, um where just imagine just some empty

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<v Speaker 1>space in the universe where you just have a bunch

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<v Speaker 1>of dust molecules just floating out there doing nothing. Uh.

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<v Speaker 1>You know, it's like a quiet town. I can think

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<v Speaker 1>of it as like a quiet Midwestern town. Everything's just

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<v Speaker 1>going about its business, tumbleweeds. But then what happens, right,

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<v Speaker 1>the hot young rebel on its bike rolls through town,

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<v Speaker 1>right and stirs everybody up. Well, that's kind of what

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<v Speaker 1>happens when a shock wave from a supernova moves through

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<v Speaker 1>these particles. It's it mixes things up a little. Suddenly

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<v Speaker 1>you have pieces colliding into one another you have in

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<v Speaker 1>these little bits of dust begin a process called acretion,

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<v Speaker 1>where the gravity of minute little pieces of matter begin

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<v Speaker 1>drawing in other many pieces of matter until and in

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<v Speaker 1>this snowball effect takes off where it gets grows bigger

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<v Speaker 1>and bigger, eventually becoming uh, planets, stars, new systems, new galaxies.

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<v Speaker 1>And this you know this, this gun slinger, this rebel

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<v Speaker 1>riding into town. This is happening super fast because the

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<v Speaker 1>core of a supernova supernova is larger than the Earth,

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<v Speaker 1>containing about a million times the mass of the Earth.

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<v Speaker 1>So when a star like say the supernova seven A, dies,

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<v Speaker 1>it collapses to the size of the Earth, which then

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<v Speaker 1>collapses to the size of London and approximately one second,

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<v Speaker 1>I mean, this is that's amazing, right, So this, this

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<v Speaker 1>h gunslinger shows up and you know this, this ball

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<v Speaker 1>of fire. And you know, if that's not dramatic enough,

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<v Speaker 1>consider that the materials that spiral off the supernova into

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<v Speaker 1>the universe during its final seconds have been billions of

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<v Speaker 1>the years in the making, right millions. For instance, we

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<v Speaker 1>know that all the hydrogen burns to helium in ten

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<v Speaker 1>million years. So this is what's happening when a star dies, right,

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<v Speaker 1>it starts to take its own material and burn off.

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<v Speaker 1>So all that hydrogen burns to helium in ten million

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<v Speaker 1>years um, and then gravity starts to contract the star,

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<v Speaker 1>making it hotter and hotter, and then helium burns to

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<v Speaker 1>carbon in one million years, and then all the carbon

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<v Speaker 1>burns to form nitrogen in one hundred thousand years. Oxygen

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<v Speaker 1>burns to silicon in ten thousand years, and then during

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<v Speaker 1>the last day, this is the coolest part, the last

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<v Speaker 1>day in the life of the star, all the silicon

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<v Speaker 1>burns to form iron in one day, and this really

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<v Speaker 1>is the death now, since iron is tightly bound um

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<v Speaker 1>in terms of its nucleus and it has nothing to

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<v Speaker 1>give in the form of fuel to the star. The

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<v Speaker 1>really cool thing about this is that these are all

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<v Speaker 1>the elements that the universe is made of, that the

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<v Speaker 1>Earth is made of, and pretty much what we are

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<v Speaker 1>made of. Right, So every atom in your body, according

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<v Speaker 1>according to Lawrence Cross, and he's a theoretical physicist, was

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<v Speaker 1>once in a star that exploded. Two hundred million stars

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<v Speaker 1>have created the elements to make up your body. Hydrogen, carbon,

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<v Speaker 1>and lithium were part of the Big Bang. So this

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<v Speaker 1>is where the beautiful quasi spiritual idea enters the picture.

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<v Speaker 1>The idea that are humble, little fragile body that are

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<v Speaker 1>in the process of growing old and dying. Uh contain uh,

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<v Speaker 1>the elements that were once a part of the of

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<v Speaker 1>one of the most colossal, powerful events that regularly happens

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<v Speaker 1>in the universe, And they were once the part part

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<v Speaker 1>of stars. We're we're made out of these stars were

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<v Speaker 1>made out of the celestial gods. We are kind of

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<v Speaker 1>like the trickle down from that. Yeah. So if you

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<v Speaker 1>look at in the night sky and you fill an

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<v Speaker 1>affinity with it, then it's because we you know, it's

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<v Speaker 1>the building blocks of us. Right, And Lawrence Cross says,

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<v Speaker 1>you know, the atoms in your left hand probably came

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<v Speaker 1>from a different star than your right hand. He says,

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<v Speaker 1>I mean, this is a great quote. It really is

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<v Speaker 1>the most poetic thing I know about physics. You are

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<v Speaker 1>all stardust. You couldn't be here if stars hadn't exploded,

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<v Speaker 1>because the elements carbon, nitrogen, oxygen, iron, all the things

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<v Speaker 1>that matter for evolution and for life weren't created at

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<v Speaker 1>the beginning of time. They were created in the nuclear

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<v Speaker 1>furnaces of stars. And the only way for them to

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<v Speaker 1>get in your body is if those stars were kind

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<v Speaker 1>enough to explode. He says, so forget Jesus, the stars

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<v Speaker 1>died so that you could be here today. Well, we'll see.

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<v Speaker 1>That's nice. And now I've also read estimates that of

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<v Speaker 1>the mass in our bodies has actually started us. So

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<v Speaker 1>it's a good chunk. It's a good chunk. And it

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<v Speaker 1>just sounds better to say all of it though, because

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<v Speaker 1>no one wants to be like, like we are divine.

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<v Speaker 1>You know, that's that's a weird percentage. Why I just

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<v Speaker 1>go for a hundreds, right, yeah, exactly, why not? Uh,

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<v Speaker 1>let's not split hairs. But um, you know, it's an

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<v Speaker 1>interesting perspective when you think about that your existence in

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<v Speaker 1>a in a the universe. And we actually just did

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<v Speaker 1>a podcast concerning black swans. Black swans being these events

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<v Speaker 1>that out liars that seem like, you know, you couldn't

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<v Speaker 1>predict them. Um, and this idea that black swans are

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<v Speaker 1>everywhere all the time, and in fact our existence is

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<v Speaker 1>a black swan, right um. And Lawrence Cross would actually

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<v Speaker 1>say that there's there's many black swans in this universe.

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<v Speaker 1>We just have to look for them. And we have

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<v Speaker 1>a lot many more connections to the universe than just

0:12:08.800 --> 0:12:11.240
<v Speaker 1>being you know, part of Stardust. Ruminate on that for

0:12:11.240 --> 0:12:13.640
<v Speaker 1>just a moment, and we will be back with more

0:12:13.920 --> 0:12:21.640
<v Speaker 1>on the cosmic origins of your atoms. All right, we're back,

0:12:21.720 --> 0:12:24.079
<v Speaker 1>and we're actually going to discuss a few other um

0:12:24.640 --> 0:12:27.760
<v Speaker 1>kind of trippy cosmic connections that you can make to

0:12:28.240 --> 0:12:32.040
<v Speaker 1>the outer dark without having to really as much on

0:12:32.080 --> 0:12:36.000
<v Speaker 1>the whole star dust supernova situation. Okay, here's here's one.

0:12:36.640 --> 0:12:40.720
<v Speaker 1>Are we possibly the extraterrestrials that we've been talking about? Ah,

0:12:41.160 --> 0:12:43.959
<v Speaker 1>you are, of course talking about exogenesis. I am talking

0:12:44.000 --> 0:12:47.280
<v Speaker 1>about the idea that life immer originates not on Earth

0:12:47.880 --> 0:12:50.640
<v Speaker 1>but somewhere else, the raw materials for it at least, right,

0:12:50.720 --> 0:12:53.640
<v Speaker 1>that the raw materials at least or you know, you

0:12:53.640 --> 0:12:56.640
<v Speaker 1>could go crazy and say, get into some ancient alien stuff,

0:12:56.679 --> 0:12:59.600
<v Speaker 1>but that's uh, that's for another podcast for this though.

0:12:59.640 --> 0:13:02.679
<v Speaker 1>You're talking about, um, the idea that the raw materials

0:13:03.320 --> 0:13:08.160
<v Speaker 1>end up arriving here um via asteroids meteor rides. So yeah, yeah,

0:13:08.200 --> 0:13:10.320
<v Speaker 1>And it turns out of Antarctica is really helpful in

0:13:10.360 --> 0:13:13.400
<v Speaker 1>trying to study this because it's just this vast white

0:13:13.520 --> 0:13:19.360
<v Speaker 1>landscape right, really easy to spot meteorites, particularly Martian meteorites.

0:13:19.760 --> 0:13:22.840
<v Speaker 1>And since we have looked at the soil composition on Mars,

0:13:22.880 --> 0:13:25.560
<v Speaker 1>we already know that when we find a meteorite that

0:13:25.679 --> 0:13:28.080
<v Speaker 1>it could have come from Mars when we slice it

0:13:28.080 --> 0:13:30.520
<v Speaker 1>and dish it and look at the composition. So what

0:13:30.640 --> 0:13:35.000
<v Speaker 1>has become apparent is that we are polluted regularly from

0:13:35.160 --> 0:13:38.520
<v Speaker 1>material from Mars and vice versa. So materialist from Earth

0:13:38.559 --> 0:13:40.600
<v Speaker 1>getting knocked out from the surface, and they also make

0:13:40.640 --> 0:13:44.320
<v Speaker 1>their way to Mars. Um. Now sometimes we send things

0:13:44.360 --> 0:13:46.640
<v Speaker 1>to Mars too. It's true we did have little care

0:13:46.679 --> 0:13:51.520
<v Speaker 1>packages um cookies, but we also known Again, this was

0:13:51.600 --> 0:13:54.840
<v Speaker 1>Laurence Cruss talking about that microbes in this Siberian desert

0:13:54.920 --> 0:13:57.920
<v Speaker 1>can exist without water under harsh conditions for months or

0:13:57.960 --> 0:14:01.320
<v Speaker 1>even years uh and in door mis state, and he

0:14:01.400 --> 0:14:04.320
<v Speaker 1>says no doubt that if microbes existed in a rock

0:14:04.400 --> 0:14:06.680
<v Speaker 1>on Mars, it could make a six month trip to

0:14:06.720 --> 0:14:09.079
<v Speaker 1>Earth once they were knocked out from this service with

0:14:09.120 --> 0:14:12.040
<v Speaker 1>no problem. So the big question is did life on

0:14:12.080 --> 0:14:15.960
<v Speaker 1>Earth arise here or somewhere else? Maybe we are all

0:14:16.080 --> 0:14:19.960
<v Speaker 1>the extraterrestrials right, And the process of life traveling from

0:14:19.960 --> 0:14:23.520
<v Speaker 1>one planet to another is called pan spermium. And we

0:14:23.560 --> 0:14:25.800
<v Speaker 1>have an article on how stuff Works about space collisions.

0:14:25.800 --> 0:14:26.920
<v Speaker 1>If you look, if you just go to a house

0:14:26.920 --> 0:14:29.320
<v Speaker 1>stuff works dot com, type in space collisions and you'll

0:14:29.320 --> 0:14:32.680
<v Speaker 1>find a cool little article talking about various cosmic heavy

0:14:32.720 --> 0:14:37.000
<v Speaker 1>hitters smacking together. And also um the idea of pants spermia,

0:14:37.080 --> 0:14:39.680
<v Speaker 1>the idea of life spreading from one world to another. Yeah,

0:14:39.760 --> 0:14:43.360
<v Speaker 1>and he also uh mourns across us people to think

0:14:43.400 --> 0:14:49.080
<v Speaker 1>about taking a breath, think about oxygen for just one moment. Okay,

0:14:49.080 --> 0:14:51.680
<v Speaker 1>now I can say this. Consider that life evolved on

0:14:51.720 --> 0:14:54.360
<v Speaker 1>Earth for two billion years before it began to produce

0:14:54.400 --> 0:14:59.720
<v Speaker 1>and use oxygen. Organisms use photosynthesis, which use carbon carbon dioxide,

0:14:59.760 --> 0:15:03.160
<v Speaker 1>and all those little dudes produce little puffs of oxygen,

0:15:03.280 --> 0:15:05.880
<v Speaker 1>and over millions of years, created more and more oxygen

0:15:05.880 --> 0:15:08.640
<v Speaker 1>in our atmosphere until boom here we are taking it

0:15:08.680 --> 0:15:12.120
<v Speaker 1>for granted. Um, he says. Lawrence Croft says that in

0:15:12.200 --> 0:15:15.160
<v Speaker 1>every breath you take, they're an average of at least

0:15:15.200 --> 0:15:18.600
<v Speaker 1>ten oxygen atoms from the dying breath of Caesar. When

0:15:18.640 --> 0:15:24.080
<v Speaker 1>he said at brute wow, he's waxing poetic hardcore on this.

0:15:24.480 --> 0:15:26.680
<v Speaker 1>He totally he's pulling out all the stops because he's like,

0:15:26.680 --> 0:15:28.400
<v Speaker 1>you know, it's not just as as I think he

0:15:28.520 --> 0:15:31.320
<v Speaker 1>referred to it before, just a bunch of dead people's

0:15:31.320 --> 0:15:33.840
<v Speaker 1>breath that we're taking in. Yeah, because because I mean,

0:15:33.920 --> 0:15:36.040
<v Speaker 1>we're also you could also say, oh, I'm also drawing

0:15:36.080 --> 0:15:39.400
<v Speaker 1>in the breath of every inane thing that has ever

0:15:39.440 --> 0:15:43.320
<v Speaker 1>been said by a politician, Hollywood starlets, the dark side

0:15:43.320 --> 0:15:45.240
<v Speaker 1>of that. But it's true. Every time you breathe, you're

0:15:45.240 --> 0:15:48.520
<v Speaker 1>breathing in atoms of everyone who has ever lived. So

0:15:48.600 --> 0:15:50.440
<v Speaker 1>you know, if there's someone sitting next to you that

0:15:50.480 --> 0:15:53.680
<v Speaker 1>you just might be annoyed with, you just feel like,

0:15:53.720 --> 0:15:55.840
<v Speaker 1>oh man, I can't I can't muster any sort of

0:15:55.840 --> 0:15:58.560
<v Speaker 1>empathy for this person. Uh. You know, you just have

0:15:58.600 --> 0:16:00.440
<v Speaker 1>to realize that we actually are all eat out of

0:16:00.440 --> 0:16:03.080
<v Speaker 1>the same material um, and we're all breathing the same

0:16:03.240 --> 0:16:07.120
<v Speaker 1>funky breath of the earth. But it reminds me of

0:16:07.160 --> 0:16:09.680
<v Speaker 1>the I did a block pist a while back about

0:16:09.720 --> 0:16:13.120
<v Speaker 1>the the idea that all drinking water was poo at

0:16:13.120 --> 0:16:16.480
<v Speaker 1>one point, which again Lawrence Cross will say he has

0:16:16.520 --> 0:16:19.640
<v Speaker 1>some interesting things to say about that. Um. He says

0:16:19.760 --> 0:16:23.200
<v Speaker 1>that it's just really interesting. He says, every time you

0:16:23.320 --> 0:16:26.160
<v Speaker 1>drink in water, you're drinking in the sweat from your parents,

0:16:26.200 --> 0:16:30.400
<v Speaker 1>coupling that created you. I know, I know, even this,

0:16:30.680 --> 0:16:33.760
<v Speaker 1>this fancy lacroix in my hand, it seems so pure,

0:16:35.000 --> 0:16:37.800
<v Speaker 1>so wide spread our materials. We just and and he

0:16:37.840 --> 0:16:40.160
<v Speaker 1>says also, like any sort of exprement from any sort

0:16:40.160 --> 0:16:42.520
<v Speaker 1>of sludge that ever existed on this earth, you're also

0:16:42.600 --> 0:16:44.840
<v Speaker 1>taking it. But this is really cool too. If you

0:16:44.880 --> 0:16:46.720
<v Speaker 1>prick your finger and drop a drop of your blood

0:16:46.720 --> 0:16:49.760
<v Speaker 1>in the Thames, for instance, Um, a year later, you

0:16:49.800 --> 0:16:51.640
<v Speaker 1>could take a tablespoon of water from the ocean and

0:16:51.680 --> 0:16:53.520
<v Speaker 1>there would be some of the atoms of your blood

0:16:53.520 --> 0:16:57.880
<v Speaker 1>in that water. According to Lawrence Cross, Yeah, it does

0:16:57.960 --> 0:17:00.640
<v Speaker 1>drive home the interconnectedness of it all, and that there

0:17:00.720 --> 0:17:03.800
<v Speaker 1>is um. I mean, we don't stand outside the cycle

0:17:03.920 --> 0:17:06.560
<v Speaker 1>of mass and matter and energy. That we are a

0:17:06.640 --> 0:17:09.639
<v Speaker 1>part of this. Uh, we are part of cosmos. Really,

0:17:09.720 --> 0:17:12.920
<v Speaker 1>you know that's true. So often we think of science

0:17:13.000 --> 0:17:16.240
<v Speaker 1>is something separate from us rather than within us. Yeah,

0:17:16.280 --> 0:17:18.560
<v Speaker 1>I mean, that's just that's just the where our minds work,

0:17:18.600 --> 0:17:20.600
<v Speaker 1>and it's one of the reasons we end up, you know,

0:17:20.640 --> 0:17:23.959
<v Speaker 1>having all these blinders to figuring out how consciousness works

0:17:23.960 --> 0:17:26.160
<v Speaker 1>and how can we end up creating all these uh

0:17:26.600 --> 0:17:29.960
<v Speaker 1>uh these ideas of spirituality and religion. She sort of

0:17:29.960 --> 0:17:32.439
<v Speaker 1>peep beyond those blinders that you're forced to recognize that

0:17:32.520 --> 0:17:34.600
<v Speaker 1>we are a part of the universe. It's it's the

0:17:34.720 --> 0:17:37.200
<v Speaker 1>hippie dippi as that may sound, you know, it's we are.

0:17:37.240 --> 0:17:39.719
<v Speaker 1>I mean, there you go. Okay, so now you've all

0:17:39.720 --> 0:17:41.479
<v Speaker 1>put us in a mood for a little Carl. Second,

0:17:42.000 --> 0:17:43.760
<v Speaker 1>why don't you hit us with a little well, yeah,

0:17:43.760 --> 0:17:45.800
<v Speaker 1>that imagine A number of people were like, how are

0:17:45.800 --> 0:17:47.520
<v Speaker 1>they going to mention that Carl Sagan quote or not?

0:17:47.720 --> 0:17:49.160
<v Speaker 1>What's a matter with these people there? In fact, they're

0:17:49.160 --> 0:17:51.480
<v Speaker 1>already writing the emails. How could you leave out the

0:17:51.480 --> 0:17:54.200
<v Speaker 1>Carl Sagon quote? Well, I have the Car sagend quote

0:17:54.240 --> 0:17:57.639
<v Speaker 1>here for you. And interesting fact, we considered, um, trying

0:17:57.680 --> 0:17:59.639
<v Speaker 1>to get somebody to do a Car Sagan voice for

0:17:59.760 --> 0:18:03.320
<v Speaker 1>us for this, but there was a lot of discussion about, well,

0:18:03.560 --> 0:18:05.520
<v Speaker 1>he doesn't really do a Carl Sagan voice. He does

0:18:05.560 --> 0:18:07.800
<v Speaker 1>a Kermit the Frog voice that kind of sounds like,

0:18:07.880 --> 0:18:10.840
<v Speaker 1>kind of sounds like Carl Sagan. Do do we do

0:18:10.920 --> 0:18:13.600
<v Speaker 1>we get him to do this in his current voice?

0:18:13.640 --> 0:18:15.360
<v Speaker 1>Do we ask him to tweak it into a Sagan?

0:18:15.840 --> 0:18:17.879
<v Speaker 1>Is that cool? Is that because we love Sagan, we

0:18:17.880 --> 0:18:20.199
<v Speaker 1>don't want to and we love Kermit, you know, right,

0:18:20.240 --> 0:18:21.560
<v Speaker 1>And then there's an other dude in the office that

0:18:21.560 --> 0:18:24.440
<v Speaker 1>always wears a turtleneck. But then that doesn't quite come across. Yeah,

0:18:24.440 --> 0:18:26.359
<v Speaker 1>that only works if you're in the studio with us.

0:18:26.400 --> 0:18:29.280
<v Speaker 1>So I'm just gonna read it in my serious voice.

0:18:29.320 --> 0:18:32.800
<v Speaker 1>I guess matter is much older than life. Billions of

0:18:32.880 --> 0:18:36.000
<v Speaker 1>years before the Sun and Earth even formed, Adams were

0:18:36.000 --> 0:18:38.880
<v Speaker 1>being synthesized in the insides of hot stars and then

0:18:38.880 --> 0:18:42.480
<v Speaker 1>returned to space when the stars blew themselves up. Newly

0:18:42.560 --> 0:18:45.479
<v Speaker 1>formed planets were made out of the stellar debris, and

0:18:45.560 --> 0:18:48.560
<v Speaker 1>Earth and every living thing are made of star stuff

0:18:50.040 --> 0:18:54.639
<v Speaker 1>like that, like yeah, yeah, yeah, this the star stuff

0:18:54.720 --> 0:18:58.160
<v Speaker 1>is is um Yeah, that's it's just a great quote

0:18:58.200 --> 0:19:00.280
<v Speaker 1>and it really and he drives some some much of

0:19:00.320 --> 0:19:02.439
<v Speaker 1>what Sagan did so well that he was able to

0:19:02.480 --> 0:19:07.400
<v Speaker 1>convey this uh, this passion for uh, for for cosmos,

0:19:07.440 --> 0:19:10.080
<v Speaker 1>for for the universe, for for space, for sciences, for

0:19:10.400 --> 0:19:13.480
<v Speaker 1>you know, neuroscience, and another related to areas as well,

0:19:13.680 --> 0:19:15.640
<v Speaker 1>was able to relay that passion for it and make

0:19:15.720 --> 0:19:17.960
<v Speaker 1>it feel like a part of us and not something

0:19:17.960 --> 0:19:21.600
<v Speaker 1>that we stood apart from indeed, incidentally, there is also

0:19:22.080 --> 0:19:24.880
<v Speaker 1>around the same time about the late sixties of when

0:19:25.520 --> 0:19:28.040
<v Speaker 1>when Sagan was thinking about this stuff and formulating these,

0:19:28.160 --> 0:19:31.639
<v Speaker 1>uh these ideas, you also had a young Joni Mitchell

0:19:31.840 --> 0:19:37.119
<v Speaker 1>wrote wrote a song called Woodstock, which features the lyrics

0:19:37.160 --> 0:19:39.720
<v Speaker 1>were start us we're golden, We're billion year old carbon

0:19:40.080 --> 0:19:41.680
<v Speaker 1>And as we close out the podcast, you were actually

0:19:41.680 --> 0:19:44.800
<v Speaker 1>gonna play a portion of a cover by the by

0:19:44.800 --> 0:19:47.720
<v Speaker 1>the band Austra all of that song wood Stock that

0:19:47.800 --> 0:19:52.439
<v Speaker 1>I find particularly snazzy. So but before we get to

0:19:52.480 --> 0:19:54.960
<v Speaker 1>that real quick, if you need to contact us and

0:19:55.000 --> 0:19:56.840
<v Speaker 1>you want to reach out to us about anything we've

0:19:56.840 --> 0:19:58.879
<v Speaker 1>talked about in this podcast or other podcasts, you can

0:19:58.920 --> 0:20:01.480
<v Speaker 1>find us on Facebook as stuff to Blow the Mind,

0:20:01.560 --> 0:20:03.480
<v Speaker 1>and you can find us on Twitter as blow the Mind.

0:20:03.840 --> 0:20:05.600
<v Speaker 1>And you can always drop us a line at blow

0:20:05.640 --> 0:20:08.200
<v Speaker 1>the Mind. At how stuff Works dot com, we are

0:20:08.560 --> 0:20:26.600
<v Speaker 1>start we are, we are. We be sure to check

0:20:26.600 --> 0:20:29.760
<v Speaker 1>out our new video podcast, Stuff from the Future. Join

0:20:29.800 --> 0:20:32.320
<v Speaker 1>how Stuff Work staff as we explore the most promising

0:20:32.400 --> 0:20:34.720
<v Speaker 1>and perplexing possibilities of tomorrow.