WEBVTT - Black Holes, Part 1: Phantom

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<v Speaker 1>My World. Welcome to Stuff to Blow your Mind from

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<v Speaker 1>how Stuff Works dot com. Hey, welcome to Stuff to

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<v Speaker 1>Blow your Mind. My name is Robert Lamb and I'm

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<v Speaker 1>Joe McCormick, and today is going to be part one

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<v Speaker 1>of a multi part episode on on a topic that

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<v Speaker 1>I know you came back from New York with a fever.

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<v Speaker 1>For Robert, We're gonna be talking about black holes, that's right. Yeah,

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<v Speaker 1>I attended, Uh, I attended a talk at the World

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<v Speaker 1>Science Festival that I believe I mentioned in our previous

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<v Speaker 1>sort of World Science Festival roundup episode that I just

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<v Speaker 1>thought did a great job of providing an overview of

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<v Speaker 1>black holes and uh help straighten out a few of

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<v Speaker 1>the details for me. Yeah, I realized we have talked

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<v Speaker 1>about black holes on the podcast before, but you haven't

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<v Speaker 1>really I felt given it, given them proper, do We haven't.

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<v Speaker 1>We haven't really uh looked at black holes with the

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<v Speaker 1>attention that they deserve. Yeah, And of course, even in

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<v Speaker 1>doing a multi part series, we're not gonna be able

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<v Speaker 1>to cover every interesting thing about black holes. So this

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<v Speaker 1>is gonna be kind of a grab bag of things

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<v Speaker 1>that seemed interesting to us. So in this first episode,

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<v Speaker 1>we're gonna be talking mainly about the history of the idea,

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<v Speaker 1>where it came from, how we arrived at this bizarre

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<v Speaker 1>conclusion about the cosmos that we live in. In the

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<v Speaker 1>second episode, we're going to be focusing mainly on like

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<v Speaker 1>how we get a look at these things. And in

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<v Speaker 1>the third episode, I think we're gonna explore some of

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<v Speaker 1>the strangest avenues of thought that you can contemplate with

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<v Speaker 1>regard to black holes, like what's it like to fall

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<v Speaker 1>into one? Or what happens when a black hole collapses?

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<v Speaker 1>Does it does it create something on the inside? Yeah,

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<v Speaker 1>And I want to acknowledge that black holes, I feel

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<v Speaker 1>are kind of a challenging topic to tackle some people.

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<v Speaker 1>I mean, certainly from a like a physics standpoint, yes,

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<v Speaker 1>but but also just in terms of becoming engaged with

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<v Speaker 1>the idea, because I know there are plenty of you

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<v Speaker 1>out there like, yeah, black holes, let's do this. I

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<v Speaker 1>love I love science I love science fiction. I think

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<v Speaker 1>King of of all my favorite black hole related movies.

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<v Speaker 1>But I know other people are a little hesitant because ultimately,

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<v Speaker 1>black holes are a concept that have very little impact

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<v Speaker 1>on our personal lives and the scope of the universe.

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<v Speaker 1>That we observe and interact in. Well, they don't have

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<v Speaker 1>any people in them, right. I mean a lot of times,

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<v Speaker 1>I think when people look up to space and they say,

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<v Speaker 1>you know, I want to be interested in it, but

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<v Speaker 1>there's if there's no people up there, it's hard to

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<v Speaker 1>feel like I'm following a story or narrative. Or can

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<v Speaker 1>I even imagine a person there, because obviously there are

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<v Speaker 1>no people on Mars. But I can, But I can

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<v Speaker 1>imagine a future in which there are people on Mars.

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<v Speaker 1>I can. I can imagine multiple different sci fi scenarios,

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<v Speaker 1>many of which match up reasonably well with scientific expectations,

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<v Speaker 1>and and that can allow me to engage myself in

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<v Speaker 1>Mars more. But unfortunately, if you know anything about black holes,

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<v Speaker 1>you know that it's not even possible to say colonies

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<v Speaker 1>a black hole. You can't have singular and knots going

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<v Speaker 1>in there to see what's on the inside. Or you could,

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<v Speaker 1>but it just wouldn't be very useful for us on

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<v Speaker 1>the outside, or I guess very useful for those getting

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<v Speaker 1>ripped apart on the inside. Right. And I think another

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<v Speaker 1>challenge with black holes is that when they have played

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<v Speaker 1>a key role in science fiction and been made ultimately

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<v Speaker 1>kind of relatable concepts. Uh, the films don't really do

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<v Speaker 1>much with the science. They don't really do a great

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<v Speaker 1>job about really conveying what a black hole is. For instance,

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<v Speaker 1>I have to admit that my first introduction to black

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<v Speaker 1>holes was the nineteen seventy nine Walt Disney sci fi

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<v Speaker 1>movie The black Hole. Oh, Robert, I've never seen this one,

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<v Speaker 1>but I'm excited. I'm excited for you to tell me

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<v Speaker 1>about it. Tell me about it, fill my brain. All right,

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<v Speaker 1>we'll just briefly. I'll try not to go on too

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<v Speaker 1>long about this, because this is a film I loved

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<v Speaker 1>as a child and I still look back on finally today.

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<v Speaker 1>But it lands in a weird spot for a science

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<v Speaker 1>fiction film because it's it's not as fun and original

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<v Speaker 1>as nineteen seventy seven Star Wars, and of course it's

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<v Speaker 1>nowhere near as high minded and scientifically savvy as ninety

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<v Speaker 1>eight two thousand and one of Space Odyssey. But then again,

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<v Speaker 1>you know what is Instead, it's kind of an old

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<v Speaker 1>fashioned Jules Verne esque tale of space explorers who wind

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<v Speaker 1>up on a space station that's circling a black hole,

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<v Speaker 1>and the station's run by a mad scientist whose only

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<v Speaker 1>attendance are robots and lowbottomized androids. There's ultimately some fairly

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<v Speaker 1>horrific and and kind of ambitious stuff mixed in there,

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<v Speaker 1>but you're also faced with just kind of a maximum

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<v Speaker 1>dosage of of of of late seventies big budget cinema.

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<v Speaker 1>Like all the actors you would expect to show up

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<v Speaker 1>do show up. Ernest borg nine, Anthony Perkins, great, Maximilian

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<v Speaker 1>Shell shows up as the villain. How about Harry Dean Stanton?

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<v Speaker 1>Uh no, no, Dean Stanton, as I recall, And you

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<v Speaker 1>also have one of the Bottoms brothers, timoth Bottoms, No, no,

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<v Speaker 1>no one one of the other ones. Not not last

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<v Speaker 1>picture was it last picture show? Yeah, less picture show, Yeah,

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<v Speaker 1>not last picture shows bottoms, but but but one of

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<v Speaker 1>the other ones some other bottoms yes, okay. And also

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<v Speaker 1>slim pickings, slim pickings. Yeah, he's the voice of a

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<v Speaker 1>robhid just busted up robot it had It is really

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<v Speaker 1>cool robots in it. I gotta see this. The trailer

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<v Speaker 1>is pretty great for it. H In fact, if we

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<v Speaker 1>if we can play it, I would like to just

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<v Speaker 1>throw in just a clip from this trailer. There is

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<v Speaker 1>an inexorable force in the cosmos, where time and space converge,

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<v Speaker 1>a place beyond men's vision but not to his reach.

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<v Speaker 1>It is the most misdious and awesome point in the universe,

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<v Speaker 1>whether here and now maybe forever. The black hole in

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<v Speaker 1>this film, the actual black hole that we're presented with,

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<v Speaker 1>it's it's it's presented like a vortex. It's it's more

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<v Speaker 1>in keeping with the charybdis whirlpool of Greek myth. You know, this,

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<v Speaker 1>this terrible thing that you're on the verge of falling into.

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<v Speaker 1>It's ultimately treated with more religious reverence than scientific, which

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<v Speaker 1>of course is pretty much what happens later on in

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<v Speaker 1>the film Event Horizon, which I also love, but it's

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<v Speaker 1>hardly a scientific tour to force. Were you watching Event

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<v Speaker 1>Horizon recently, Robert, Yes, I was. I started watching it

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<v Speaker 1>again last night, but only made it about ten minutes

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<v Speaker 1>in before my ambient kicked in, because that's a horrible idea.

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<v Speaker 1>It's it's not really not ten minutes end, because you

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<v Speaker 1>get past the scary stuff and then you're just done

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<v Speaker 1>a spaceship, and then you realize it's time to go

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<v Speaker 1>to bed. I realized that the spaceship in that movie

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<v Speaker 1>it's like the only leather punk spaceship I've ever seen

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<v Speaker 1>in science fiction. It's like, you know, those like black

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<v Speaker 1>leather wrist bands with the metal studs on them. It's

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<v Speaker 1>that as a spaceship, it is very industrious, especially the uh,

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<v Speaker 1>the core that you end up exploring. But but hopefully

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<v Speaker 1>we'll get to talk about event Arizon a little bit

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<v Speaker 1>more in one of the future episodes. But basically the

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<v Speaker 1>idea is it's got a black hole and that's how

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<v Speaker 1>you get to Hell. I think, yeah, which again is

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<v Speaker 1>kind of the idea that has explored in Disney's a

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<v Speaker 1>black Hole as well. So there's people in it, well,

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<v Speaker 1>there are things in it, humanoids that you end up

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<v Speaker 1>with characters traveling through it. It's ultimately the confusing part

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<v Speaker 1>is that both films kind of treat a black hole

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<v Speaker 1>more like a wormhole, which is a separate thing altogether,

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<v Speaker 1>but that is ultimately more relatable I think to us

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<v Speaker 1>the idea of like a magic tunnel that goes somewhere.

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<v Speaker 1>But of course, actual black holes don't exist on a

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<v Speaker 1>scale that that directly influences individual human life for life

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<v Speaker 1>on Earth, except in our study of them. But the

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<v Speaker 1>bottom line is that they're They're just a physical reality

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<v Speaker 1>of our universe. They're not some sort of evil, malignant force.

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<v Speaker 1>They are just a physical part of the universe. At

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<v Speaker 1>the same time, though, I would say they are astounding

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<v Speaker 1>and one of the most interesting things in the universe

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<v Speaker 1>because they are the absolute extremists of of what we

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<v Speaker 1>know about physics. They're sort of like the test cases.

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<v Speaker 1>They're the exceptions. They break things that and that. For

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<v Speaker 1>that reason, they're interesting to scientists because we can look

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<v Speaker 1>at them and say, okay, what happens in these extreme

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<v Speaker 1>cases where you know, where we can't necessarily see inside

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<v Speaker 1>to know the answer. So at this point some of

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<v Speaker 1>you might be asking, well, well, what is a black hole?

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<v Speaker 1>Just lay lay out the basic definition. If it's not

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<v Speaker 1>a wormhole, it's not a gateway to Hell, then then

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<v Speaker 1>what are we talking about here? Well, in short, we're

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<v Speaker 1>talking about regions of space where the gravity is so

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<v Speaker 1>intense that light cannot escape the poll and the gravity

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<v Speaker 1>is that intense because matter is compressed to a very

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<v Speaker 1>small space and they range in size. For instance, primordial

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<v Speaker 1>black holes are no larger than a single atom, but

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<v Speaker 1>they contain the mass of a terrestrial Mount him So

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<v Speaker 1>Mount everest crunched down to the side of an atom.

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<v Speaker 1>It's pretty dense. A stellar black hole might be ten

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<v Speaker 1>kilometers in diameter, but would boast the mass of twenty suns,

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<v Speaker 1>for instance. And then finally you have the supermassive black hole. Uh,

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<v Speaker 1>the types of black holes that that that that live

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<v Speaker 1>at the centers of galaxies. Uh. And these would have

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<v Speaker 1>the mass of millions of suns compressed to a sphere

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<v Speaker 1>the size of a single solar system. That's extreme compression. Yeah,

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<v Speaker 1>a little harder to even think about it. Like I

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<v Speaker 1>find that the mountain atom uh comparison is maybe a

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<v Speaker 1>little more impactful for the human imagination. But still we're

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<v Speaker 1>talking about considerable, considerable consolidation of mass. Now we call

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<v Speaker 1>them black holes because light cannot escape them. Optically, they

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<v Speaker 1>appear as an absence. We can't see inside them, but

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<v Speaker 1>we can observe the effect of say, of of this

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<v Speaker 1>intense gravity on the surrounding environment. And despite the fact

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<v Speaker 1>that we can't see inside them, as we'll talk about

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<v Speaker 1>a couple of times as we go along, that doesn't

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<v Speaker 1>necessarily mean we don't see anything around them. In fact,

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<v Speaker 1>they can often put on quite a show. Yeah, I

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<v Speaker 1>hate to lean into the horror movie implications here, but

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<v Speaker 1>it's kind of like imagine the uh, the house from

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<v Speaker 1>the Texas Chainsaw Mask. Here, you can't see any of

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<v Speaker 1>the teenagers dying inside it from the outside, but you

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<v Speaker 1>see them like moving towards the house. You see a

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<v Speaker 1>lot of of random hippie activity on the outside, and

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<v Speaker 1>it gives you an idea of what might be going

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<v Speaker 1>on in the inside. Actually came up with an analogy

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<v Speaker 1>I was going to use in the next episode, but

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<v Speaker 1>maybe I'll go ahead and say it. So this is

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<v Speaker 1>a little less grizzly than what you said, but kind

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<v Speaker 1>of similar. So, uh, imagine you've got like a haunted

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<v Speaker 1>house ride in an amusement park, and the ride, the

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<v Speaker 1>part of the ride that you ride in is the

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<v Speaker 1>soundproof box where nobody can hear anything on the outside.

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<v Speaker 1>So you've got everybody in line to get in the ride,

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<v Speaker 1>to get in the soundproof box and go through the

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<v Speaker 1>haunted house. And as you're hurting tourists towards this soundproof box,

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<v Speaker 1>even though you can't hear any of the screams inside

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<v Speaker 1>the box, you will hear more and more sort of

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<v Speaker 1>nervous chatter and laughter and shrieks as people are approaching

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<v Speaker 1>the door, but then once you shut the door, bye bye.

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<v Speaker 1>I like that we both independently came up with haunted

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<v Speaker 1>house explanations for black holes. Personally, I seriously doubt that

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<v Speaker 1>the Texas Chainsaw House is haunted or contains a black hole. Now,

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<v Speaker 1>now it's important to note in all of this that

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<v Speaker 1>I really think we should try and get away from

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<v Speaker 1>thinking of black holes as essentially galactus or or some

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<v Speaker 1>sort of other unstoppable, insatiable cosmic devour that just destroys

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<v Speaker 1>and consumes everything, which is kind of hard because, as

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<v Speaker 1>we've discussed before in the show, like that's a classic

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<v Speaker 1>mythic trope, like the idea of some entity that will

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<v Speaker 1>consume the Sun. I mean, it's key to these various

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<v Speaker 1>eclipse mythologies that we've discussed in the past. But a

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<v Speaker 1>black hole is not, uh, this thing is just going

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<v Speaker 1>to eat the entire universe. They're bound by physics, so stars, planets,

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<v Speaker 1>whole galaxies may orbit around them. And I've seen it

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<v Speaker 1>pointed out before by NASA that if our Sun were

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<v Speaker 1>a black hole of equal mass, the Earth would not

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<v Speaker 1>fall in. Yeah, that's a point I've read many times before.

0:12:12.280 --> 0:12:14.400
<v Speaker 1>So what would happen to the Earth if the Sun

0:12:14.480 --> 0:12:17.240
<v Speaker 1>turned into a black hole? The Earth would keep orbiting. Yeah,

0:12:17.559 --> 0:12:20.120
<v Speaker 1>So again, to come back to the Texas Chainsaw mascure House,

0:12:20.720 --> 0:12:23.120
<v Speaker 1>it's it's not like the Texas Chainsaw Masscure House is

0:12:23.160 --> 0:12:26.120
<v Speaker 1>just going to suck in everybody in the surrounding area

0:12:26.200 --> 0:12:28.760
<v Speaker 1>and collapse the town. Now, the town continues to thrive. Yeah,

0:12:28.760 --> 0:12:30.520
<v Speaker 1>the next door neighbors, they just keep going to work,

0:12:30.800 --> 0:12:33.520
<v Speaker 1>they saying, keep selling barbecue. Everything's fine. And I also

0:12:33.559 --> 0:12:36.640
<v Speaker 1>think again, the whole aspect of this is a stumbling

0:12:36.640 --> 0:12:39.160
<v Speaker 1>block because it tends to encourage us to think of

0:12:39.320 --> 0:12:42.760
<v Speaker 1>black holes less as what they presumably are and more

0:12:42.800 --> 0:12:46.040
<v Speaker 1>like wormholes. Okay, so it's like it's like a tunnel

0:12:46.120 --> 0:12:50.280
<v Speaker 1>you can go through. Yeah, yeah, But ultimately, a singularity

0:12:50.440 --> 0:12:53.600
<v Speaker 1>is not a gateway. It doesn't go anywhere other than

0:12:53.679 --> 0:12:57.240
<v Speaker 1>to the center of its gravity. Their celestial objects that

0:12:57.280 --> 0:13:00.400
<v Speaker 1>just happened to be massive on a scale that's really

0:13:00.400 --> 0:13:03.440
<v Speaker 1>harder to square with human experience. Well, I can tell already,

0:13:03.520 --> 0:13:06.480
<v Speaker 1>Robert that you're running into issues with the language that

0:13:06.559 --> 0:13:10.160
<v Speaker 1>we have to use to describe things, because there is

0:13:10.320 --> 0:13:14.440
<v Speaker 1>no language, I mean, the only language we have is

0:13:14.520 --> 0:13:18.280
<v Speaker 1>like normal terrestrial vocabulary, and then the metaphors we build

0:13:18.280 --> 0:13:23.040
<v Speaker 1>out of that normal terrestrial vocabulary, so inevitably our language

0:13:23.080 --> 0:13:27.280
<v Speaker 1>will ultimately fail to have words that, at a fundamental

0:13:27.360 --> 0:13:31.320
<v Speaker 1>level really communicate the nature of celestial objects, you know,

0:13:31.360 --> 0:13:35.880
<v Speaker 1>powerful objects, huge objects like black holes. So we we

0:13:35.960 --> 0:13:38.719
<v Speaker 1>just have to use metaphors, right, and the idea of

0:13:38.720 --> 0:13:41.000
<v Speaker 1>a black hole is a metaphor. Yeah, and it's it's

0:13:41.000 --> 0:13:43.800
<v Speaker 1>a challenge for science communication for sure. A lot of

0:13:43.840 --> 0:13:46.920
<v Speaker 1>great black hole studies come out, and then you look

0:13:46.960 --> 0:13:50.440
<v Speaker 1>at the headlines that that are used right to to

0:13:50.520 --> 0:13:54.120
<v Speaker 1>relate these findings, and it's it's I often get a

0:13:54.240 --> 0:13:57.160
<v Speaker 1>laugh out of it because the world leader model is

0:13:57.200 --> 0:13:59.800
<v Speaker 1>so often employed and you end up hearing reading about

0:14:00.040 --> 0:14:04.840
<v Speaker 1>hannibal black holes, gobbling black holes, eating black holes, barfing

0:14:04.880 --> 0:14:08.440
<v Speaker 1>black holes. Yeah, it's so anthropomorphised in a really visceral way.

0:14:08.440 --> 0:14:10.840
<v Speaker 1>I mean you almost want to imagine that there are

0:14:10.920 --> 0:14:14.800
<v Speaker 1>articles about dating black holes, swipe right black holes. But

0:14:14.840 --> 0:14:16.559
<v Speaker 1>it's it's kind of a your damned if you do,

0:14:16.600 --> 0:14:18.320
<v Speaker 1>your damned if you don't situation. It's kind of like

0:14:18.360 --> 0:14:22.760
<v Speaker 1>when you when when we even anthropomorphize evolution to some extent,

0:14:23.200 --> 0:14:26.440
<v Speaker 1>we treat it like a person, right, And I mean,

0:14:27.160 --> 0:14:29.960
<v Speaker 1>on one hand, I acknowledge, yes, one should not do that.

0:14:30.000 --> 0:14:33.440
<v Speaker 1>You fall into, you know, potential traps by doing it.

0:14:33.640 --> 0:14:36.280
<v Speaker 1>But at the same time, you ultimately are trying to

0:14:37.360 --> 0:14:42.680
<v Speaker 1>put some fairly complex ideas into a form that people

0:14:42.720 --> 0:14:45.880
<v Speaker 1>can really consume. Well, you can talk about evolution without

0:14:45.880 --> 0:14:49.360
<v Speaker 1>anthropomorphizing it or you know, treating it like a person

0:14:49.480 --> 0:14:52.120
<v Speaker 1>with intentions. It's possible to do that. It can just

0:14:52.200 --> 0:14:55.720
<v Speaker 1>get really tedious to constantly be talking that way. So

0:14:55.760 --> 0:14:58.880
<v Speaker 1>we and we inevitably in these discussions, if we're just

0:14:58.920 --> 0:15:01.800
<v Speaker 1>trying to move things long and you know, move at

0:15:01.800 --> 0:15:04.440
<v Speaker 1>a brisk pace, we end up using the shorthand. And

0:15:04.480 --> 0:15:06.880
<v Speaker 1>the same thing happens for black holes. Black holes, we

0:15:07.000 --> 0:15:11.040
<v Speaker 1>end up using these colloquial shorthands to describe them that

0:15:11.080 --> 0:15:14.720
<v Speaker 1>are based on Earth metaphors that don't really get at

0:15:14.760 --> 0:15:17.200
<v Speaker 1>the truth of what it's like to have the geometry

0:15:17.200 --> 0:15:20.720
<v Speaker 1>of space time warped by this gravitational anomaly. Now, one

0:15:20.720 --> 0:15:23.000
<v Speaker 1>of the really fascinating things about black holes, though, is

0:15:23.040 --> 0:15:25.400
<v Speaker 1>that we we simply we didn't simply look into the

0:15:25.440 --> 0:15:29.600
<v Speaker 1>sky and observe them. Uh. It all began with the math.

0:15:29.720 --> 0:15:33.640
<v Speaker 1>It began with with with some some very bright individuals

0:15:34.160 --> 0:15:38.040
<v Speaker 1>crunching the numbers and seeing them as a possibility. Yeah,

0:15:38.080 --> 0:15:40.160
<v Speaker 1>and that's one of the things that makes black holes

0:15:40.200 --> 0:15:44.040
<v Speaker 1>so interesting. They weren't like stars. They weren't you know, stars.

0:15:44.080 --> 0:15:46.400
<v Speaker 1>We could look up and know something was there, and

0:15:46.400 --> 0:15:50.360
<v Speaker 1>then over time gradually make observations to refine our knowledge

0:15:50.400 --> 0:15:53.080
<v Speaker 1>of what stars are. Right, black holes weren't like that.

0:15:53.120 --> 0:15:56.320
<v Speaker 1>We had to work them out from first principles and

0:15:56.360 --> 0:15:59.360
<v Speaker 1>then say, okay, is there a way we could observe them?

0:15:59.400 --> 0:16:02.480
<v Speaker 1>It worked actually the opposite way. Yeah, that's the beautiful

0:16:02.520 --> 0:16:04.920
<v Speaker 1>part we see because we see it paying off. We

0:16:04.920 --> 0:16:07.800
<v Speaker 1>we we we we end up looking out into the

0:16:07.800 --> 0:16:11.520
<v Speaker 1>cosmos and observing the very things that we have simulated

0:16:11.960 --> 0:16:15.600
<v Speaker 1>with math and physics. The great astrophysicists Supermania and Chandra

0:16:15.680 --> 0:16:19.000
<v Speaker 1>Sheker had in a prologue to his book The Mathematical

0:16:19.080 --> 0:16:22.440
<v Speaker 1>Theory of black Holes, he wrote, quote, the black holes

0:16:22.480 --> 0:16:26.360
<v Speaker 1>of nature are the most perfect macroscopic objects there are

0:16:26.480 --> 0:16:29.840
<v Speaker 1>in the universe. The only elements in their construction are

0:16:29.840 --> 0:16:32.640
<v Speaker 1>our concepts of space and time. All right, Well, on

0:16:32.680 --> 0:16:34.280
<v Speaker 1>that note, we're gonna take a quick break, and when

0:16:34.280 --> 0:16:36.600
<v Speaker 1>we come back. We are going to jump into the

0:16:36.680 --> 0:16:41.480
<v Speaker 1>history of black holes. Thank you, thank alright, we're back.

0:16:41.880 --> 0:16:44.120
<v Speaker 1>So previously we were just talking about how black holes

0:16:44.160 --> 0:16:47.240
<v Speaker 1>began as an idea before they were observed in nature.

0:16:47.280 --> 0:16:50.560
<v Speaker 1>They started as something that people worked out from principles

0:16:50.600 --> 0:16:53.800
<v Speaker 1>they had established through other means, rather than something we

0:16:53.880 --> 0:16:57.200
<v Speaker 1>looked up into the heavens and saw. And there's there's

0:16:57.200 --> 0:16:59.840
<v Speaker 1>a really great book about this actually that I want

0:16:59.840 --> 0:17:02.240
<v Speaker 1>to for two because it's one of the sources I

0:17:02.320 --> 0:17:04.320
<v Speaker 1>used in working on this episode. But it's called black

0:17:04.320 --> 0:17:07.720
<v Speaker 1>Hole by Marcia Bartoustiac, and it's a it's a book

0:17:07.760 --> 0:17:09.960
<v Speaker 1>just about the history of the idea of the black hole,

0:17:10.000 --> 0:17:13.000
<v Speaker 1>how it went from the idea of gravity to something

0:17:13.040 --> 0:17:17.440
<v Speaker 1>that we now do experiments on with with cosmological detection equipment.

0:17:18.040 --> 0:17:20.120
<v Speaker 1>So the story of the black hole can really be connected,

0:17:20.160 --> 0:17:24.480
<v Speaker 1>I think, to the broader story of the discovery of gravity. Uh.

0:17:24.520 --> 0:17:27.640
<v Speaker 1>You know, we often don't even bother to think anymore,

0:17:27.760 --> 0:17:31.000
<v Speaker 1>why do objects fall down and not up? But I, oh,

0:17:31.160 --> 0:17:34.040
<v Speaker 1>I sometimes wonder like do kids still have this thought?

0:17:34.359 --> 0:17:38.560
<v Speaker 1>Do kids ask this sometimes or are they exposed to

0:17:38.640 --> 0:17:41.199
<v Speaker 1>the theories we have of gravity before they even have

0:17:41.320 --> 0:17:44.320
<v Speaker 1>the chance to ask that question naturally, you know, that's

0:17:44.400 --> 0:17:48.720
<v Speaker 1>that's a great question, because I they certainly grasp the

0:17:48.840 --> 0:17:51.600
<v Speaker 1>idea and the reality of gravity is just one of

0:17:51.640 --> 0:17:54.600
<v Speaker 1>the realities of the natural world that they've evolved to

0:17:54.640 --> 0:17:56.840
<v Speaker 1>thrive him. Of course we understand how it works, but

0:17:57.000 --> 0:18:00.040
<v Speaker 1>why yeah, yeah, you know my own personal experience, I

0:18:00.040 --> 0:18:02.040
<v Speaker 1>don't know that I've ever had a conversation with my

0:18:02.080 --> 0:18:05.800
<v Speaker 1>son about gravity um or at least not when he

0:18:05.880 --> 0:18:09.240
<v Speaker 1>was old enough to to appreciate it. I'm gonna have

0:18:09.280 --> 0:18:11.639
<v Speaker 1>to make a mission of explaining it to him. But

0:18:11.840 --> 0:18:14.679
<v Speaker 1>he also he may know already because he listens to

0:18:15.240 --> 0:18:18.000
<v Speaker 1>to educational podcasts, so he when I mentioned black holes,

0:18:18.000 --> 0:18:20.000
<v Speaker 1>he was like, oh, yeah, black holes. I was listening

0:18:20.040 --> 0:18:22.280
<v Speaker 1>to a while in the world about black holes, so

0:18:22.480 --> 0:18:24.280
<v Speaker 1>he already had a already had a leg up on

0:18:24.320 --> 0:18:26.160
<v Speaker 1>the concept. Well, I mean, it's one of those things

0:18:26.240 --> 0:18:28.119
<v Speaker 1>where most of us, I think, even people who are

0:18:28.160 --> 0:18:31.360
<v Speaker 1>aware of general relativity, we sort of have the idea

0:18:31.480 --> 0:18:34.000
<v Speaker 1>that we understand how gravity works, but then sit down

0:18:34.000 --> 0:18:36.760
<v Speaker 1>and try to put into words like explain it, and

0:18:36.800 --> 0:18:40.400
<v Speaker 1>then you start going, oh, wait a minute. But yeah,

0:18:40.440 --> 0:18:42.280
<v Speaker 1>So it's one of those things that once you've heard

0:18:42.320 --> 0:18:44.159
<v Speaker 1>it you think you've got to grasp on it, but

0:18:44.480 --> 0:18:47.760
<v Speaker 1>even then it can prove tricky to try to explain yourself.

0:18:47.840 --> 0:18:51.160
<v Speaker 1>But so you know, thousands or maybe millions of people

0:18:51.240 --> 0:18:53.600
<v Speaker 1>must have stopped to wonder this all the time before

0:18:53.640 --> 0:18:55.680
<v Speaker 1>we had a real answer why did things fall down

0:18:55.720 --> 0:18:57.960
<v Speaker 1>instead of up? And for a long time I think

0:18:58.000 --> 0:19:03.400
<v Speaker 1>humans were led astray by this intuitive, false cosmology of geocentrism.

0:19:03.440 --> 0:19:06.399
<v Speaker 1>So if you believe, like Aristotle, that the Earth is

0:19:06.440 --> 0:19:08.760
<v Speaker 1>the center of the universe, it makes a kind of

0:19:08.800 --> 0:19:12.440
<v Speaker 1>intuitive sense that everything would fall toward the center, right

0:19:13.200 --> 0:19:15.239
<v Speaker 1>And then again I sometimes wonder, like, why is that

0:19:15.320 --> 0:19:18.040
<v Speaker 1>even intuitive? Why doesn't everything fall away from the center

0:19:18.040 --> 0:19:20.639
<v Speaker 1>out to the edges. It just feels right enough that

0:19:20.720 --> 0:19:23.679
<v Speaker 1>you can stop thinking about the question basically. But then

0:19:23.720 --> 0:19:26.680
<v Speaker 1>once you introduce the Copernican model, the you know, the

0:19:26.680 --> 0:19:29.760
<v Speaker 1>heliocentric model of the Solar system, and the idea that

0:19:29.800 --> 0:19:31.960
<v Speaker 1>the Earth is not the center of the universe and

0:19:32.000 --> 0:19:34.920
<v Speaker 1>in fact is no kind of privileged place at all.

0:19:34.920 --> 0:19:38.600
<v Speaker 1>It's just another object floating around in space, Suddenly we

0:19:38.720 --> 0:19:41.760
<v Speaker 1>really need an explanation for why objects fall to the

0:19:41.800 --> 0:19:44.639
<v Speaker 1>ground rather than fly off in the opposite direction. And

0:19:44.680 --> 0:19:48.240
<v Speaker 1>the bigger question. Is the force that causes objects to

0:19:48.280 --> 0:19:51.480
<v Speaker 1>fall to the ground the same force that guides planets

0:19:51.480 --> 0:19:54.040
<v Speaker 1>in their orbits around the Sun. I like what you

0:19:54.040 --> 0:19:57.560
<v Speaker 1>said about the geocentric view because I think the geocentric

0:19:57.640 --> 0:20:01.040
<v Speaker 1>view also kind of lines up with our aasic egoic

0:20:01.440 --> 0:20:04.600
<v Speaker 1>experience of the world, Like everything in the world ultimately

0:20:04.600 --> 0:20:07.760
<v Speaker 1>breaks down to what I feel about it, because I

0:20:07.800 --> 0:20:11.359
<v Speaker 1>am the only the only experience, the only worldview you

0:20:11.359 --> 0:20:14.760
<v Speaker 1>know that I that I have control of and one

0:20:15.160 --> 0:20:19.040
<v Speaker 1>percent vision through. And uh. But then if someone would say, actually,

0:20:19.080 --> 0:20:21.000
<v Speaker 1>you're not the most important person in the world. Is

0:20:21.359 --> 0:20:24.120
<v Speaker 1>uh this person over here is that throws everything out

0:20:24.160 --> 0:20:26.480
<v Speaker 1>of out of whack. Well, it makes you realize that

0:20:26.520 --> 0:20:30.120
<v Speaker 1>your egoic view is not even necessarily a coherent view,

0:20:30.280 --> 0:20:32.399
<v Speaker 1>is just something that you can do without having to

0:20:32.400 --> 0:20:35.399
<v Speaker 1>think about. And I would argue the same is largely

0:20:35.440 --> 0:20:39.359
<v Speaker 1>true for geocentric physics. Uh though actually, in a funny way,

0:20:39.400 --> 0:20:42.760
<v Speaker 1>a lot of really intense thinking did go into constructing

0:20:42.760 --> 0:20:46.919
<v Speaker 1>geocentric cosmologies and they look kind of beautiful. But anyway,

0:20:46.920 --> 0:20:50.119
<v Speaker 1>coming back to gravity, so so we know that for example,

0:20:50.240 --> 0:20:54.719
<v Speaker 1>Johannes Kepler suggested that the sun exerted a magnetic force

0:20:54.920 --> 0:20:58.440
<v Speaker 1>that guided the orbits of the planets. Weird to think

0:20:58.480 --> 0:21:01.080
<v Speaker 1>back to a time when they were thinking, Okay, how

0:21:01.080 --> 0:21:04.440
<v Speaker 1>are the planets controlled in there? Or maybe it's magnetism.

0:21:04.440 --> 0:21:07.640
<v Speaker 1>We know magnets exist, that's an attractive force. Maybe that's

0:21:07.680 --> 0:21:11.480
<v Speaker 1>what controls it. And in the sixteen thirties, Descartes proposed

0:21:11.520 --> 0:21:14.399
<v Speaker 1>that the orbits of the planets were guided by swirlings

0:21:14.400 --> 0:21:17.240
<v Speaker 1>in the ether, which was this substance that was believed

0:21:17.280 --> 0:21:19.359
<v Speaker 1>to occupy space. The ether would have been kind of

0:21:19.400 --> 0:21:22.960
<v Speaker 1>like air water, this fluid that occupied empty space, and

0:21:23.000 --> 0:21:27.080
<v Speaker 1>you could have whirlpools or cyclones guiding objects in a

0:21:27.119 --> 0:21:30.000
<v Speaker 1>circular pattern around a center of motion, and that would

0:21:30.000 --> 0:21:32.360
<v Speaker 1>be what would guide orbits in the ether. But then,

0:21:32.400 --> 0:21:34.800
<v Speaker 1>of course we got to Newton. And so in sixteen

0:21:35.119 --> 0:21:40.240
<v Speaker 1>seven Isaac Newton struck gold with the philosophy naturalists Principia Mathematica,

0:21:40.359 --> 0:21:43.000
<v Speaker 1>or the Principia as people usually call it these days,

0:21:43.240 --> 0:21:47.560
<v Speaker 1>and it established the mathematical principles that correctly describe gravity

0:21:47.560 --> 0:21:50.199
<v Speaker 1>and planetary motion, which in effect turn out to be

0:21:50.320 --> 0:21:52.879
<v Speaker 1>the same thing. The motion of the planets dis guided

0:21:52.920 --> 0:21:57.200
<v Speaker 1>by momentum and gravity, and Newton calculated the inverse square

0:21:57.280 --> 0:22:00.000
<v Speaker 1>law of gravity, meaning that as you move away from

0:22:00.000 --> 0:22:03.919
<v Speaker 1>an object, it's gravitational influence is diminished by the square

0:22:04.119 --> 0:22:06.680
<v Speaker 1>of the distance. So what does that mean. That means

0:22:06.720 --> 0:22:10.680
<v Speaker 1>if you double the distance between two objects, the gravitational

0:22:10.760 --> 0:22:13.520
<v Speaker 1>force between them is reduced to a fourth and if

0:22:13.560 --> 0:22:17.399
<v Speaker 1>you quadruple the distance, the gravitational force between them is

0:22:17.480 --> 0:22:21.080
<v Speaker 1>decreased to one sixteen. It's a square of the distance.

0:22:21.400 --> 0:22:23.399
<v Speaker 1>So this indicates that the force of gravity is a

0:22:23.440 --> 0:22:27.639
<v Speaker 1>constant force, spreading out equally in all three dimensions. And

0:22:27.680 --> 0:22:30.520
<v Speaker 1>so a key insight that that Newton has that gravity

0:22:30.560 --> 0:22:33.800
<v Speaker 1>is universal. It applies equally to the objects we drop

0:22:33.880 --> 0:22:35.960
<v Speaker 1>and throw here on Earth, end of the objects we

0:22:36.040 --> 0:22:38.600
<v Speaker 1>see in the night sky. Though it's worth pointing out

0:22:38.600 --> 0:22:40.600
<v Speaker 1>at this stage that we still didn't know what gravity

0:22:40.640 --> 0:22:44.280
<v Speaker 1>actually was other than this mutually attractive force between objects

0:22:44.320 --> 0:22:47.600
<v Speaker 1>with mass. Newton wrote, actually, quote, I have not as

0:22:47.680 --> 0:22:50.359
<v Speaker 1>yet been able to deduce from phenomena the reason for

0:22:50.400 --> 0:22:54.080
<v Speaker 1>these properties of gravity, and I do not feign hypotheses.

0:22:55.000 --> 0:22:58.040
<v Speaker 1>And so Newton's laws were widely accepted, especially after they

0:22:58.040 --> 0:23:00.960
<v Speaker 1>were used to correctly predict the reappearing of Halley's comment

0:23:01.359 --> 0:23:07.880
<v Speaker 1>and this leads us to an English natural philosopher, geologist, astronomer, mathematician,

0:23:08.040 --> 0:23:13.160
<v Speaker 1>dabbler in mini domains named John Michelle. That's right, armed

0:23:13.240 --> 0:23:16.720
<v Speaker 1>only with a Newtonian and obviously pre Einsteiny and understanding

0:23:16.720 --> 0:23:21.960
<v Speaker 1>of gravity. Um. John Michelle and Henry Cavendish, Uh, contemplated

0:23:22.000 --> 0:23:25.359
<v Speaker 1>some pretty big cosmological questions, including the scale of the

0:23:25.480 --> 0:23:28.160
<v Speaker 1>universe and the cycle of stars. Yeah, they were really

0:23:28.200 --> 0:23:30.280
<v Speaker 1>ahead of their time in a way. John Michelle for

0:23:30.320 --> 0:23:33.720
<v Speaker 1>a long time was not necessarily recognized as one of

0:23:33.760 --> 0:23:36.480
<v Speaker 1>the earliest people to think about black holes. But but

0:23:36.560 --> 0:23:38.840
<v Speaker 1>he did some interesting work. Yeah. And and to put

0:23:38.880 --> 0:23:41.080
<v Speaker 1>him in within a you know, you have the right

0:23:41.160 --> 0:23:47.159
<v Speaker 1>time scale here. Uh. John Mitchell literally of seventeen and

0:23:47.240 --> 0:23:50.800
<v Speaker 1>Cavendish lived seventeen through eighteen ten. Okay, so what was

0:23:50.880 --> 0:23:53.680
<v Speaker 1>the deal? What? How did they touch on black holes? All? Right? So,

0:23:54.240 --> 0:23:57.080
<v Speaker 1>even in their day, it was known that stars flared up,

0:23:57.280 --> 0:24:01.240
<v Speaker 1>they subsided, and even vanished from the heavens. A popular

0:24:01.320 --> 0:24:04.400
<v Speaker 1>theory of the day was that they had dark spots

0:24:04.520 --> 0:24:06.600
<v Speaker 1>on them, you know, much like the spots that could

0:24:06.640 --> 0:24:10.080
<v Speaker 1>be observed on our own sun, and that this would

0:24:10.080 --> 0:24:14.240
<v Speaker 1>affect visibility. Though theories varied on what those dark spots

0:24:14.520 --> 0:24:17.400
<v Speaker 1>were actually going to be. They might be dark valleys

0:24:17.560 --> 0:24:22.000
<v Speaker 1>or ripples or peaks at a darker core underlying you know,

0:24:22.480 --> 0:24:27.800
<v Speaker 1>outer fluid or gases, um scum, or rock like bodies.

0:24:27.880 --> 0:24:31.440
<v Speaker 1>Even uh, there was all the star scum, yes, your

0:24:31.520 --> 0:24:34.159
<v Speaker 1>star scum. And then there was this cool idea that

0:24:34.480 --> 0:24:38.240
<v Speaker 1>that was also thrown around that you might have flattened stars.

0:24:39.200 --> 0:24:40.600
<v Speaker 1>So these would have been I guess kind of like

0:24:41.760 --> 0:24:46.320
<v Speaker 1>kind of like lenses rotating disks. Yeah, And so if it,

0:24:46.400 --> 0:24:49.480
<v Speaker 1>depending on what how it was facing you, it would

0:24:49.600 --> 0:24:52.200
<v Speaker 1>affect luminosity. So if it turned its edge to you,

0:24:52.480 --> 0:24:56.280
<v Speaker 1>there would obviously be a lot less illumination. So it's

0:24:56.359 --> 0:24:58.720
<v Speaker 1>not exactly the same principle, but I can see that

0:24:58.840 --> 0:25:03.320
<v Speaker 1>being an interesting inside preceding the discovery of things like pulsars.

0:25:04.760 --> 0:25:06.879
<v Speaker 1>So they pondered the structure of the cosmos and the

0:25:06.960 --> 0:25:10.280
<v Speaker 1>nature of stars and eventually hit upon a rather i

0:25:10.320 --> 0:25:13.280
<v Speaker 1>would say, haunting idea. And this was in Sight three.

0:25:13.880 --> 0:25:17.520
<v Speaker 1>What if a star was was massive enough, large enough

0:25:17.560 --> 0:25:21.480
<v Speaker 1>that it attracted back upon itself all the light it admitted,

0:25:21.880 --> 0:25:24.600
<v Speaker 1>in other words, so massive that light itself could not

0:25:24.800 --> 0:25:30.560
<v Speaker 1>achieve escape velocity. This was the idea of the dark star. WHOA,

0:25:31.080 --> 0:25:34.520
<v Speaker 1>Now we should give a little more context and explanation

0:25:34.600 --> 0:25:36.560
<v Speaker 1>to what they're thinking was here. But I have to

0:25:36.680 --> 0:25:40.240
<v Speaker 1>say the name of this paper because it's crazy. The

0:25:40.400 --> 0:25:44.600
<v Speaker 1>paper by John michelle In, presented at the Royal Society

0:25:44.600 --> 0:25:47.160
<v Speaker 1>of London in seven in seventeen eighty three and eighty

0:25:47.200 --> 0:25:51.560
<v Speaker 1>four was quote on the means of discovering the distance, magnitude,

0:25:51.680 --> 0:25:55.280
<v Speaker 1>etcetera of the fixed stars in consequence of the diminution

0:25:55.400 --> 0:25:58.000
<v Speaker 1>of the velocity of their light. In case such a

0:25:58.080 --> 0:26:00.920
<v Speaker 1>diminution should be found to take play sent any of them,

0:26:01.200 --> 0:26:04.639
<v Speaker 1>and such other data should be procured from observations as

0:26:04.680 --> 0:26:07.800
<v Speaker 1>would be farther necessary for that purpose. That's a pretty

0:26:07.840 --> 0:26:09.440
<v Speaker 1>good one. It's got a ring to it. He needs

0:26:09.480 --> 0:26:11.680
<v Speaker 1>like a social media editor working with him. And you

0:26:11.800 --> 0:26:15.720
<v Speaker 1>get that title down. Yeah, So what's what's the clickbait

0:26:15.800 --> 0:26:18.879
<v Speaker 1>title of this paper? Oh you gotta you gotta some

0:26:19.000 --> 0:26:21.520
<v Speaker 1>help fit um. You know a gobbling star in there.

0:26:21.960 --> 0:26:24.840
<v Speaker 1>Let's see, I tried to measure the massive binary stars.

0:26:24.920 --> 0:26:28.359
<v Speaker 1>You can't You won't believe what happened next by the

0:26:28.440 --> 0:26:31.720
<v Speaker 1>way that they figured that. Uh that if you have

0:26:31.840 --> 0:26:33.680
<v Speaker 1>a dark star like this. This would be the case

0:26:33.760 --> 0:26:35.960
<v Speaker 1>if you had a star as dense as our sun,

0:26:36.040 --> 0:26:39.159
<v Speaker 1>but with a radius four nineties seven times larger, and

0:26:39.200 --> 0:26:42.320
<v Speaker 1>it's such it would be difficult to optically observe such

0:26:42.359 --> 0:26:45.960
<v Speaker 1>a star. Yeah, so what what was Michelle doing in

0:26:46.000 --> 0:26:48.760
<v Speaker 1>this paper? As I just alluded to, his main goal,

0:26:48.880 --> 0:26:51.720
<v Speaker 1>the more banal goal was to measure the mass of

0:26:51.840 --> 0:26:54.600
<v Speaker 1>binary stars. So he was armed with, as you said,

0:26:54.680 --> 0:26:58.080
<v Speaker 1>Newton's gravitational laws. People were excited about Newton at the time.

0:26:58.160 --> 0:27:01.080
<v Speaker 1>What you could learn by using Newton so, uh, the

0:27:01.200 --> 0:27:04.240
<v Speaker 1>laws guiding planetary orbits, and he had those in hand,

0:27:04.600 --> 0:27:07.040
<v Speaker 1>and with those you could calculate the masses of two

0:27:07.119 --> 0:27:09.960
<v Speaker 1>stars in a binary system by observing the way they

0:27:10.119 --> 0:27:12.520
<v Speaker 1>orbit one another over the years. If you know how

0:27:12.640 --> 0:27:15.159
<v Speaker 1>wide their orbit is and how long it takes them

0:27:15.200 --> 0:27:18.840
<v Speaker 1>to orbit, you can estimate their mass. But Michell also

0:27:19.000 --> 0:27:22.320
<v Speaker 1>explored the limits of light, so he was working on

0:27:22.440 --> 0:27:24.879
<v Speaker 1>this assumption that light was composed of what was known

0:27:24.920 --> 0:27:28.320
<v Speaker 1>at the time as corpuscles. That makes the light sound

0:27:28.400 --> 0:27:31.320
<v Speaker 1>very romantic, I know, and kind of organic as well. Yeah.

0:27:31.400 --> 0:27:35.040
<v Speaker 1>So the corepuscles of light collections of particles, which, given

0:27:35.160 --> 0:27:37.280
<v Speaker 1>what we know about light today is sort of partially

0:27:37.400 --> 0:27:40.840
<v Speaker 1>correct and partially incorrect, right like we know we know

0:27:40.960 --> 0:27:43.560
<v Speaker 1>it's now given that light can be measured in particle

0:27:43.680 --> 0:27:46.399
<v Speaker 1>units known as photons, but can also behave like a wave.

0:27:46.800 --> 0:27:50.080
<v Speaker 1>But operating on this earlier assumption that light was composed

0:27:50.160 --> 0:27:53.960
<v Speaker 1>of these corpuscles these particles, Michell noted that light, like

0:27:54.119 --> 0:27:58.000
<v Speaker 1>anything else, must have an escape velocity. So the normal

0:27:58.080 --> 0:28:00.359
<v Speaker 1>illustration of this is you stand on the evace of

0:28:00.400 --> 0:28:02.600
<v Speaker 1>the Earth, you throw a baseball straight up in the

0:28:02.680 --> 0:28:05.680
<v Speaker 1>air at a hundred kilometers an hour, it'll fall back

0:28:05.680 --> 0:28:07.359
<v Speaker 1>down to the ground. And if you throw it at

0:28:07.400 --> 0:28:10.200
<v Speaker 1>two hundred kilometers an hour, it will travel up farther,

0:28:10.400 --> 0:28:12.600
<v Speaker 1>but it will still fall back down. If you just

0:28:12.840 --> 0:28:16.040
<v Speaker 1>keep throwing it up at greater and greater velocities each time,

0:28:16.080 --> 0:28:18.679
<v Speaker 1>eventually it's going to reach a velocity where, if it's

0:28:18.720 --> 0:28:21.320
<v Speaker 1>at the right angle, it doesn't fall straight back down

0:28:21.359 --> 0:28:23.760
<v Speaker 1>to the ground, but instead can go into orbit around

0:28:23.800 --> 0:28:26.080
<v Speaker 1>the planet. And if you keep throwing it straight up

0:28:26.160 --> 0:28:29.600
<v Speaker 1>at a great enough velocity, eventually it will actually escape

0:28:29.640 --> 0:28:32.119
<v Speaker 1>the planet's gravity and fly off into space and not

0:28:32.440 --> 0:28:35.800
<v Speaker 1>fall back down to Earth. And specifically, how fast an

0:28:35.880 --> 0:28:39.680
<v Speaker 1>object needs to be traveling to leave Earth's gravity is

0:28:39.840 --> 0:28:42.040
<v Speaker 1>eleven point two kilometers per second. If you can go

0:28:42.200 --> 0:28:44.520
<v Speaker 1>that fast, you can leave. If not, you're stuck here

0:28:44.560 --> 0:28:47.160
<v Speaker 1>with the rest of us. Uh. And a funny side

0:28:47.200 --> 0:28:49.680
<v Speaker 1>here is that you ever think about the idea of

0:28:49.720 --> 0:28:54.040
<v Speaker 1>a terrestrial alien planet with so much mass essentially that

0:28:54.160 --> 0:28:57.640
<v Speaker 1>it prohibits the aliens who live there from practicing space

0:28:57.720 --> 0:29:02.080
<v Speaker 1>exploration when also to just so so stocky they had

0:29:02.160 --> 0:29:04.600
<v Speaker 1>trouble with it. Yeah, I mean, who knows how that

0:29:04.600 --> 0:29:07.240
<v Speaker 1>would change their culture and all that. But uh, but yeah,

0:29:07.280 --> 0:29:09.520
<v Speaker 1>I mean you could imagine a more massive planet that

0:29:09.640 --> 0:29:13.080
<v Speaker 1>had a greater escape velocity might just make it the

0:29:13.120 --> 0:29:15.360
<v Speaker 1>case that you could never come up with a technology

0:29:15.480 --> 0:29:17.840
<v Speaker 1>that could get you out of the planet's gravity. Well,

0:29:18.040 --> 0:29:21.040
<v Speaker 1>this is my entire read on the the the horror

0:29:21.080 --> 0:29:23.920
<v Speaker 1>film phantasm, by the way, is that they have that

0:29:24.080 --> 0:29:26.280
<v Speaker 1>portal that goes to another world. Well, how did they

0:29:26.320 --> 0:29:29.560
<v Speaker 1>get here in the first place? Yeah, I guess they

0:29:29.600 --> 0:29:31.840
<v Speaker 1>sent the tall man. And the tall man is tall

0:29:31.960 --> 0:29:34.920
<v Speaker 1>because he's supposed to be on a high gravity planet,

0:29:34.960 --> 0:29:36.960
<v Speaker 1>and it like you know, straightens them out and makes

0:29:37.000 --> 0:29:38.720
<v Speaker 1>them taller on our planet. And then they have to

0:29:38.760 --> 0:29:41.479
<v Speaker 1>crunch those corpses down into dwarves so that they can

0:29:41.600 --> 0:29:45.320
<v Speaker 1>labor on the on the high gravity world. You know,

0:29:45.480 --> 0:29:48.800
<v Speaker 1>it's it's a really smart concept. It it really gets

0:29:48.840 --> 0:29:52.880
<v Speaker 1>at things that make you think, uh phantasm, Yeah, yeah,

0:29:53.200 --> 0:29:56.120
<v Speaker 1>I mean, it's just mysterious enough to get your brain working,

0:29:56.320 --> 0:29:59.040
<v Speaker 1>you know. Oh you know when Silicon Valley saw that ball,

0:29:59.160 --> 0:30:00.880
<v Speaker 1>they were all like, I could to design one of those.

0:30:01.040 --> 0:30:06.000
<v Speaker 1>I can make that ball. Yeah I Pentagon, come on, yeah,

0:30:06.920 --> 0:30:09.720
<v Speaker 1>I one day, we'll see him. Now. So coming back

0:30:09.800 --> 0:30:13.720
<v Speaker 1>to John Michelle, So what he believed was that you

0:30:13.800 --> 0:30:16.040
<v Speaker 1>got these core pustles of light and they they've got

0:30:16.120 --> 0:30:18.160
<v Speaker 1>an escape velocity as well, and what they have to

0:30:18.240 --> 0:30:20.360
<v Speaker 1>do to shine away from a star is escape the

0:30:20.400 --> 0:30:25.000
<v Speaker 1>stars gravity. And fortunately, as Michelle, light travels very very fast,

0:30:25.120 --> 0:30:28.080
<v Speaker 1>so this doesn't normally happen. But he realized as we

0:30:28.160 --> 0:30:30.600
<v Speaker 1>were saying, that if a star have has enough mass,

0:30:31.120 --> 0:30:34.040
<v Speaker 1>even according to this new Tonian model of physics, before

0:30:34.080 --> 0:30:38.320
<v Speaker 1>we had relativity, before we had Einstein, even on Newtonian mechanics,

0:30:38.880 --> 0:30:42.160
<v Speaker 1>you could imagine a star so big with so much

0:30:42.200 --> 0:30:45.280
<v Speaker 1>gravity that even light could not escape it and would

0:30:45.280 --> 0:30:47.920
<v Speaker 1>always get pulled back down. And like you said Robert.

0:30:48.280 --> 0:30:51.120
<v Speaker 1>The number he came up with was that a star

0:30:51.360 --> 0:30:54.280
<v Speaker 1>four hundred and ninety seven times the escape velocity of

0:30:54.320 --> 0:30:57.720
<v Speaker 1>our sun would prevent all light from leaving. And to

0:30:57.800 --> 0:31:01.280
<v Speaker 1>read a quote from Michelle's work, the existence of bodies

0:31:01.360 --> 0:31:04.920
<v Speaker 1>under these circumstances, we could have no information from sight.

0:31:05.480 --> 0:31:09.720
<v Speaker 1>Yet if other luminous bodies should happen to revolve about them,

0:31:10.240 --> 0:31:13.800
<v Speaker 1>we might still perhaps from the motions of those revolving bodies,

0:31:13.920 --> 0:31:17.320
<v Speaker 1>infer the existence of the central ones with some degree

0:31:17.360 --> 0:31:20.680
<v Speaker 1>of probability, as this might afford a clue to some

0:31:20.840 --> 0:31:24.520
<v Speaker 1>of the apparent irregularities of revolving bodies, which would not

0:31:24.680 --> 0:31:29.200
<v Speaker 1>be easily explicable on any other hypothesis. So Michelle's planting

0:31:29.240 --> 0:31:32.680
<v Speaker 1>a clue there for how we could detect black holes

0:31:32.800 --> 0:31:36.360
<v Speaker 1>or objects that did not allow light to escape before

0:31:36.480 --> 0:31:39.680
<v Speaker 1>we've even discovered relativity. And I wanted to drive home

0:31:39.720 --> 0:31:44.920
<v Speaker 1>again that this was the eighteenth century. Yeah, this is so,

0:31:45.080 --> 0:31:47.040
<v Speaker 1>this is this is pretty out their thought from the

0:31:47.120 --> 0:31:49.760
<v Speaker 1>time by by far. And I should point out that

0:31:49.960 --> 0:31:52.480
<v Speaker 1>Sir William Herschel also argued on the basis of the

0:31:52.560 --> 0:31:56.400
<v Speaker 1>particulate theory of light the corpuscles that nebulae could be

0:31:56.520 --> 0:32:00.440
<v Speaker 1>made of agglomerations of particles of light captured by gravity,

0:32:00.480 --> 0:32:02.880
<v Speaker 1>is sort of sort of held in place by gravity.

0:32:03.360 --> 0:32:06.600
<v Speaker 1>So essentially that we have the groundwork here for what

0:32:06.680 --> 0:32:09.320
<v Speaker 1>would eventually become the concept of a black hole, even

0:32:09.360 --> 0:32:11.760
<v Speaker 1>though they certainly were not calling it a black hole. No,

0:32:12.240 --> 0:32:15.200
<v Speaker 1>and uh one more thinker, we should mention somebody who

0:32:15.320 --> 0:32:18.760
<v Speaker 1>often gets credited, maybe more often than Michelle, or at

0:32:18.840 --> 0:32:21.080
<v Speaker 1>least used to get credited more often than John Michelle

0:32:21.560 --> 0:32:25.680
<v Speaker 1>is Pierre Simon de Laplace. So, in seventeen ninety six,

0:32:25.800 --> 0:32:28.480
<v Speaker 1>with the upheaval of the French Revolution still in effect,

0:32:28.880 --> 0:32:32.880
<v Speaker 1>the French astronomer and general scholar kind of Renaissance Guy

0:32:33.240 --> 0:32:37.600
<v Speaker 1>Pierre Simon de Laplace published Exposition du System dumont or

0:32:37.680 --> 0:32:40.000
<v Speaker 1>the System of the World, And in this book he

0:32:40.160 --> 0:32:45.000
<v Speaker 1>hypothesized the existence of cores, obscures, or hidden bodies or

0:32:45.200 --> 0:32:48.560
<v Speaker 1>dark bodies of those dark bodies out there. So so

0:32:48.720 --> 0:32:51.960
<v Speaker 1>he wrote, quote, a luminous star of the same density

0:32:52.040 --> 0:32:54.560
<v Speaker 1>as the Earth, and whose diameter should be two hundred

0:32:54.560 --> 0:32:57.760
<v Speaker 1>and fifty times larger than that of the Sun, would not,

0:32:58.320 --> 0:33:01.360
<v Speaker 1>in consequence of its attraction and allow any of its

0:33:01.480 --> 0:33:04.440
<v Speaker 1>rays to arrive at us. It is therefore possible that

0:33:04.560 --> 0:33:08.040
<v Speaker 1>the largest luminous bodies in the universe may, through this cause,

0:33:08.560 --> 0:33:12.840
<v Speaker 1>be invisible. Now, notice that Laplace estimated a different required

0:33:12.920 --> 0:33:15.040
<v Speaker 1>size to prevent the escape of light. This is because

0:33:15.080 --> 0:33:18.080
<v Speaker 1>he expected stars to have a different density than Michelle did.

0:33:18.400 --> 0:33:21.000
<v Speaker 1>But either way, I love that idea. So he's saying,

0:33:21.240 --> 0:33:24.120
<v Speaker 1>it's possible that the biggest things out there in the

0:33:24.280 --> 0:33:27.280
<v Speaker 1>universe are completely invisible to us. We we wouldn't even

0:33:27.320 --> 0:33:29.840
<v Speaker 1>know they were there. Now, rounding up from this, we

0:33:29.920 --> 0:33:33.320
<v Speaker 1>know that Michelle and Laplace were certainly ahead of their time,

0:33:33.360 --> 0:33:35.440
<v Speaker 1>but they were also wrong about a lot of stuff,

0:33:35.600 --> 0:33:38.280
<v Speaker 1>just owing to the time that they lived. Like that,

0:33:38.400 --> 0:33:40.680
<v Speaker 1>they didn't know lots of things about physics and about

0:33:40.720 --> 0:33:43.360
<v Speaker 1>astronomy that we did. When they imagine stars getting so

0:33:43.520 --> 0:33:46.080
<v Speaker 1>big that no light could escape their gravity, they imagine,

0:33:46.120 --> 0:33:49.120
<v Speaker 1>for one thing, stars scaling up simply by getting bigger

0:33:49.240 --> 0:33:52.560
<v Speaker 1>at a constant density. And then they also imagined light

0:33:52.720 --> 0:33:55.880
<v Speaker 1>being a projection of particles that would be slowed down

0:33:56.040 --> 0:33:59.480
<v Speaker 1>by gravity. So let's complicate the picture with some Einstein.

0:34:00.200 --> 0:34:02.840
<v Speaker 1>Let's do it. We're into the twentieth century now, during

0:34:02.880 --> 0:34:06.680
<v Speaker 1>the opening decades of the twentieth century German theoretical physicist

0:34:06.880 --> 0:34:09.240
<v Speaker 1>Albert Einstein in is the picture. He was born eighteen

0:34:09.280 --> 0:34:12.719
<v Speaker 1>seventy nine died ninety and he gave us a new

0:34:12.880 --> 0:34:16.680
<v Speaker 1>theory of gravitation, the general theory of relativity, and it

0:34:16.880 --> 0:34:21.200
<v Speaker 1>entails the idea that massive objects distort space time. And

0:34:21.320 --> 0:34:23.960
<v Speaker 1>we experienced this as gravity. Okay, So this is a

0:34:24.239 --> 0:34:26.480
<v Speaker 1>change in the idea of gravity. Instead of being a

0:34:26.680 --> 0:34:31.200
<v Speaker 1>force that that objects exert on each other, general relativity

0:34:31.200 --> 0:34:35.520
<v Speaker 1>imagines gravity as indentations in the geometry of the space

0:34:35.600 --> 0:34:38.560
<v Speaker 1>time we inhabit. That's right. Now, there's a there's a

0:34:38.560 --> 0:34:41.080
<v Speaker 1>wonderful experiment that I always like to fall back on

0:34:41.680 --> 0:34:43.360
<v Speaker 1>to kind of explain this, And in fact, there's a

0:34:43.480 --> 0:34:45.239
<v Speaker 1>video of this on stuff to Blow your Mind dot com,

0:34:45.280 --> 0:34:46.680
<v Speaker 1>and i'll i'll try and put a link to it

0:34:46.719 --> 0:34:49.360
<v Speaker 1>on the landing page for this episode. But basically it

0:34:49.400 --> 0:34:52.760
<v Speaker 1>involves taking a plastic sheet, having it stretched out generally

0:34:52.840 --> 0:34:55.240
<v Speaker 1>like if you stretch it over a hula hoop, okay,

0:34:55.760 --> 0:35:00.160
<v Speaker 1>and then you apply weighted balls onto the sheet, so

0:35:00.360 --> 0:35:01.800
<v Speaker 1>you know, you might have something that's the size of

0:35:01.840 --> 0:35:05.239
<v Speaker 1>a baseball up until up up scaling up to things

0:35:05.280 --> 0:35:07.759
<v Speaker 1>about the size of say a bowling ball, all right,

0:35:07.840 --> 0:35:10.960
<v Speaker 1>and when you place those on the sheet, it distorts

0:35:11.080 --> 0:35:13.560
<v Speaker 1>the sheet. It distorts the space time that is the

0:35:13.640 --> 0:35:17.120
<v Speaker 1>surface of that sheet. Right, So normal planets and stars

0:35:17.239 --> 0:35:19.759
<v Speaker 1>might be things on the sheets sort of like baseballs

0:35:19.880 --> 0:35:23.000
<v Speaker 1>or golf balls or something causing these small indentations where

0:35:23.280 --> 0:35:26.640
<v Speaker 1>generally things can move around them and not cause there

0:35:26.640 --> 0:35:28.440
<v Speaker 1>wouldn't really be much of an issue until you got

0:35:28.560 --> 0:35:30.480
<v Speaker 1>very close, and then you'd start to kind of circle

0:35:30.520 --> 0:35:33.560
<v Speaker 1>around or have your path diverted as you passed by

0:35:33.680 --> 0:35:36.759
<v Speaker 1>one of them, owing to the indentations they make in

0:35:36.840 --> 0:35:40.359
<v Speaker 1>the topography of the sheet. But imagine you've got, say,

0:35:40.440 --> 0:35:43.279
<v Speaker 1>like a big hunk of depleted uranium, and you put

0:35:43.360 --> 0:35:45.480
<v Speaker 1>that on the sheet like the densest thing you can

0:35:45.560 --> 0:35:48.719
<v Speaker 1>come across, and it's gonna bend the sheet down in

0:35:48.840 --> 0:35:52.720
<v Speaker 1>this crazy kind of suction that will for a certain

0:35:52.840 --> 0:35:55.399
<v Speaker 1>radius around it pull all kinds of stuff in. Yeah,

0:35:55.400 --> 0:35:57.480
<v Speaker 1>you try and roll a marble then across the sheet,

0:35:57.520 --> 0:35:59.279
<v Speaker 1>and it doesn't stand a chance it's going to be

0:35:59.320 --> 0:36:02.719
<v Speaker 1>sucked in. Can't it can't say roll past and just

0:36:02.800 --> 0:36:06.000
<v Speaker 1>get its path diverted. Suddenly things will just get sucked

0:36:06.040 --> 0:36:08.440
<v Speaker 1>all the way in and never come out. And so this,

0:36:08.600 --> 0:36:11.240
<v Speaker 1>in essence is the general theory of relativity. And again

0:36:11.280 --> 0:36:14.520
<v Speaker 1>it differs from the Newtonian model in which gravity wasn't

0:36:14.560 --> 0:36:17.240
<v Speaker 1>innate force, right, which Newton didn't know how to explain,

0:36:17.360 --> 0:36:19.839
<v Speaker 1>and I respect he didn't try to explain. He just said,

0:36:19.880 --> 0:36:22.160
<v Speaker 1>this is how it is. I'll write equations showing you

0:36:22.520 --> 0:36:24.279
<v Speaker 1>how to solve for it and how to predict how

0:36:24.320 --> 0:36:26.000
<v Speaker 1>it works. But I'm not going to say what it is.

0:36:26.760 --> 0:36:29.120
<v Speaker 1>Now We've got a pretty idea what it actually is,

0:36:29.520 --> 0:36:34.319
<v Speaker 1>and it's these these distortions in the geometry of space time.

0:36:34.560 --> 0:36:36.879
<v Speaker 1>The funny thing about that is, I think how often

0:36:37.000 --> 0:36:39.960
<v Speaker 1>we still talk about gravity as a force, as if

0:36:39.960 --> 0:36:42.960
<v Speaker 1>it were some kind of like magnetism attracting matter. I mean,

0:36:43.080 --> 0:36:47.439
<v Speaker 1>I honestly think about it that way most of the time. Yeah.

0:36:47.440 --> 0:36:50.000
<v Speaker 1>I mean again, we have to fall back on on

0:36:50.160 --> 0:36:54.600
<v Speaker 1>our experience, and that ends up coloring what we think

0:36:54.680 --> 0:36:58.800
<v Speaker 1>we know about the cosmos. Yeah. And so Einstein definitely

0:36:58.840 --> 0:37:01.120
<v Speaker 1>put he put together the theory radical framework for how

0:37:01.239 --> 0:37:05.319
<v Speaker 1>general relativity works. But one thing you might wonder is, like, Okay, well,

0:37:05.440 --> 0:37:08.560
<v Speaker 1>let's say we're really into Einstein's theory of general relativity.

0:37:08.840 --> 0:37:11.480
<v Speaker 1>How would you ever test whether such a thing were true?

0:37:12.080 --> 0:37:14.120
<v Speaker 1>You know, if you could do all of your Newtonian

0:37:14.200 --> 0:37:17.800
<v Speaker 1>experiments just using Newtonian physics and get the right answers

0:37:17.880 --> 0:37:21.520
<v Speaker 1>on Earth, how would you test to see whether Einstein's

0:37:21.560 --> 0:37:25.359
<v Speaker 1>theory was actually better? So there did come along some demonstrations,

0:37:25.440 --> 0:37:27.759
<v Speaker 1>and one of them, one that proved very decisive for

0:37:27.840 --> 0:37:32.120
<v Speaker 1>public opinion, was in nineteen nineteen when the English astrophysicist

0:37:32.239 --> 0:37:35.120
<v Speaker 1>Arthur Eddington carried out an experiment to test the predictions

0:37:35.160 --> 0:37:37.520
<v Speaker 1>of Einstein's theory. And I think we've talked about this

0:37:37.600 --> 0:37:40.280
<v Speaker 1>experiment on the show before, but one of the predictions

0:37:40.320 --> 0:37:43.480
<v Speaker 1>of general relativity is that light passing directly by a

0:37:43.560 --> 0:37:46.960
<v Speaker 1>massive object like a star should actually be bent by

0:37:47.000 --> 0:37:50.720
<v Speaker 1>a specific predictable amount, depending on how massive the object

0:37:50.880 --> 0:37:53.160
<v Speaker 1>is and how close the light passes. And so a

0:37:53.200 --> 0:37:56.040
<v Speaker 1>pretty easy way to test this would be by say,

0:37:56.120 --> 0:37:58.920
<v Speaker 1>taking a picture of the star field at night and

0:37:59.080 --> 0:38:01.760
<v Speaker 1>noting where all of the stars are, getting the locations

0:38:01.800 --> 0:38:04.840
<v Speaker 1>of those stars, and then watching what happens when the

0:38:05.080 --> 0:38:08.720
<v Speaker 1>Sun passes between the Earth and those stars. It should

0:38:08.840 --> 0:38:12.520
<v Speaker 1>be if Einstein's theory is right, that the light coming

0:38:12.600 --> 0:38:15.399
<v Speaker 1>to us from the star behind the Sun should get

0:38:15.560 --> 0:38:18.080
<v Speaker 1>bent as it's coming right past the Sun. So when

0:38:18.120 --> 0:38:20.640
<v Speaker 1>it's right beside the edge of the Sun, our view

0:38:20.719 --> 0:38:23.960
<v Speaker 1>of it should be displaced and distorted by a very predictable,

0:38:24.080 --> 0:38:27.960
<v Speaker 1>certain small but certain amount. But part of the problem is, well,

0:38:28.000 --> 0:38:30.879
<v Speaker 1>how do you test that, Like, can you usually look

0:38:30.960 --> 0:38:34.319
<v Speaker 1>at the stars if you're looking also at the sun. Yes,

0:38:34.520 --> 0:38:37.120
<v Speaker 1>you need something, you need something special to happen, something

0:38:37.239 --> 0:38:39.880
<v Speaker 1>that that that blocks out the sign. If only there

0:38:39.920 --> 0:38:43.000
<v Speaker 1>were some other object in the sky that was just

0:38:43.320 --> 0:38:46.040
<v Speaker 1>the right size to do that. And for we're very

0:38:46.160 --> 0:38:50.480
<v Speaker 1>fortunate to live in that laboratory by accident. So Earth's

0:38:50.840 --> 0:38:53.239
<v Speaker 1>Earth is very privileged. And here's one way that the

0:38:53.280 --> 0:38:56.080
<v Speaker 1>Copernican principle seems to fail. Earth is very privileged, and

0:38:56.160 --> 0:38:58.839
<v Speaker 1>that our moon is just about the same size as

0:38:58.920 --> 0:39:02.279
<v Speaker 1>the Sun, apparently from our perspective. So the Moon can

0:39:02.440 --> 0:39:06.160
<v Speaker 1>block out the Sun's light during a solar eclipse. And

0:39:06.280 --> 0:39:08.239
<v Speaker 1>if you wait for a solar eclipse, you actually could

0:39:08.320 --> 0:39:10.680
<v Speaker 1>look at the stars that are shooting light at you

0:39:10.920 --> 0:39:14.640
<v Speaker 1>from right beside the Sun from your perspective. So the

0:39:14.800 --> 0:39:17.359
<v Speaker 1>Eddington experiment waited for a solar eclipse when the moon

0:39:17.440 --> 0:39:19.920
<v Speaker 1>passed in front of the Sun, and that eclipse came

0:39:19.960 --> 0:39:23.920
<v Speaker 1>in May nineteen nineteen, passing over Eddington's experimental station on

0:39:24.040 --> 0:39:27.080
<v Speaker 1>prin Cape Island off the western coast of Africa, and

0:39:27.239 --> 0:39:30.160
<v Speaker 1>also over some uh some other astronomers working in the

0:39:30.200 --> 0:39:33.839
<v Speaker 1>Amazon rainforest. And so the eclipse dimmed the light from

0:39:33.880 --> 0:39:36.440
<v Speaker 1>the Sun enough for Ddington and colleagues to take photos

0:39:36.480 --> 0:39:39.160
<v Speaker 1>of the starfield in the background, and they found that

0:39:39.239 --> 0:39:41.920
<v Speaker 1>the Sun did indeed bend the light from the stars

0:39:42.080 --> 0:39:43.920
<v Speaker 1>right around it, and the light was bent by the

0:39:43.960 --> 0:39:48.040
<v Speaker 1>amount predicted by Einstein's general relativity. So this experiment was

0:39:48.120 --> 0:39:51.279
<v Speaker 1>a huge international sensation. It was in all the newspapers,

0:39:51.360 --> 0:39:54.440
<v Speaker 1>and it made Einstein a celebrity. Kind of makes me wonder,

0:39:54.560 --> 0:39:58.719
<v Speaker 1>like what sort of scientific experiment would make headlines in

0:39:58.880 --> 0:40:04.560
<v Speaker 1>major newspapers like front page headlines in major newspapers today. Well, uh,

0:40:05.040 --> 0:40:07.960
<v Speaker 1>skipping ahead a little bit here, but I believe gravitational

0:40:08.040 --> 0:40:13.360
<v Speaker 1>waves uh made some some headlines. They made some I mean, like,

0:40:13.680 --> 0:40:16.160
<v Speaker 1>can you imagine them as like top banner, like beating

0:40:16.200 --> 0:40:18.520
<v Speaker 1>out all the politics and everything like that. Yeah, it

0:40:18.680 --> 0:40:22.880
<v Speaker 1>is it is difficult to imagine it, but yeah, I

0:40:23.400 --> 0:40:25.680
<v Speaker 1>want to say we still have some some hits on

0:40:25.800 --> 0:40:29.160
<v Speaker 1>the way maybe maybe. So now we know that even

0:40:29.200 --> 0:40:31.960
<v Speaker 1>those stars can't slow down light. One of the key

0:40:32.040 --> 0:40:34.920
<v Speaker 1>features of Einstein's work is that the principle of the

0:40:35.000 --> 0:40:38.239
<v Speaker 1>speed of light and a vacuum never changes. Right. We

0:40:38.400 --> 0:40:41.680
<v Speaker 1>do know that very massive objects bend light as the

0:40:41.800 --> 0:40:45.359
<v Speaker 1>light travels along its trajectory through spacetime very near them.

0:40:45.920 --> 0:40:48.960
<v Speaker 1>And this is where we are going to introduce somebody

0:40:49.000 --> 0:40:51.880
<v Speaker 1>who changed the game when it comes to black holes,

0:40:52.080 --> 0:40:55.440
<v Speaker 1>and that is Carl Schwartzhield. We will discuss him when

0:40:55.520 --> 0:40:59.640
<v Speaker 1>we come back from a break. Than alright, we're back,

0:41:00.040 --> 0:41:03.120
<v Speaker 1>So Robert, take us into the mind of Karl schwartz Shield.

0:41:03.440 --> 0:41:06.880
<v Speaker 1>All right, So Karl schwartz Field was a German physicist

0:41:06.960 --> 0:41:12.000
<v Speaker 1>and astronomer. He lived only eighteen seventy three through nineteen sixteen.

0:41:12.400 --> 0:41:14.880
<v Speaker 1>He died in the war. Yeah, now he and I

0:41:14.920 --> 0:41:17.160
<v Speaker 1>should say they should point he did. He died of illness,

0:41:17.239 --> 0:41:20.319
<v Speaker 1>but he did still very much die during the First

0:41:20.360 --> 0:41:24.080
<v Speaker 1>World World War. Uh. And he calculated the possibility of

0:41:24.480 --> 0:41:28.960
<v Speaker 1>an Einsteiny and dark star. Um. He like did this

0:41:29.120 --> 0:41:32.560
<v Speaker 1>while he was in the in the service, I believe. Yeah. Yeah,

0:41:33.280 --> 0:41:35.600
<v Speaker 1>Often it's described as him like being in the trenches.

0:41:35.640 --> 0:41:38.359
<v Speaker 1>I think that, well, we like the room. The room.

0:41:38.440 --> 0:41:40.680
<v Speaker 1>It's a romantic idea, right, the idea that we have

0:41:40.880 --> 0:41:43.200
<v Speaker 1>someone that's in a literal pit and they're in a

0:41:43.600 --> 0:41:46.759
<v Speaker 1>it's a time in in world history that is that

0:41:46.960 --> 0:41:52.200
<v Speaker 1>feels like a pity and a time of just total war, uh,

0:41:52.520 --> 0:41:55.200
<v Speaker 1>encompassing the Earth, and it's seeming like we not, we

0:41:55.320 --> 0:41:56.960
<v Speaker 1>might not be able to climb back out of it.

0:41:57.200 --> 0:42:00.680
<v Speaker 1>And here this, uh, this gentleman is contemp lighting the

0:42:00.800 --> 0:42:03.680
<v Speaker 1>black hole. Yeah. As World War one is changing the

0:42:03.760 --> 0:42:07.520
<v Speaker 1>social fabric of Europe and much of the world, short

0:42:07.560 --> 0:42:10.840
<v Speaker 1>Shield here is changing the fabric of spacetime. Yeah. And

0:42:11.000 --> 0:42:15.279
<v Speaker 1>as a he shorts shorts Field was a very impressive dude,

0:42:15.320 --> 0:42:18.040
<v Speaker 1>though he was again he only lived to be forty

0:42:18.080 --> 0:42:20.919
<v Speaker 1>two years of age. Uh. But during his short life

0:42:20.960 --> 0:42:24.800
<v Speaker 1>he made practical and theoretical contributions to astronomy, and he

0:42:25.000 --> 0:42:29.560
<v Speaker 1>used general relativity equations to demonstrate celestial bodies within enough

0:42:29.680 --> 0:42:32.799
<v Speaker 1>mass would have an escape velocity beyond the speed of light.

0:42:33.239 --> 0:42:35.000
<v Speaker 1>I should also point out that again, even though he

0:42:35.400 --> 0:42:37.520
<v Speaker 1>died at the age of forty two, he had his

0:42:37.600 --> 0:42:41.239
<v Speaker 1>first theoretical physics paper published at the age of sixteen. Yeah.

0:42:41.360 --> 0:42:44.080
<v Speaker 1>He you get the impression that, like you're when you

0:42:44.160 --> 0:42:46.200
<v Speaker 1>read about him, you're sort of in the presence of

0:42:46.239 --> 0:42:49.719
<v Speaker 1>one of those brains. Uh so. Yeah. He he was

0:42:49.920 --> 0:42:54.000
<v Speaker 1>experimenting with different types of geometry for understanding the behavior

0:42:54.080 --> 0:42:56.640
<v Speaker 1>of massive objects like stars, and part of what he

0:42:56.760 --> 0:43:00.360
<v Speaker 1>was doing was trying to work out rigorous solution sans

0:43:00.440 --> 0:43:05.600
<v Speaker 1>to Einstein's equations. Einstein had sort of done the simplified

0:43:05.760 --> 0:43:08.680
<v Speaker 1>version of general relativity, and he's like, surely it'll be

0:43:08.760 --> 0:43:11.120
<v Speaker 1>really hard to work out all of the rigorous, you know,

0:43:11.480 --> 0:43:15.319
<v Speaker 1>precise solutions of my equations. But but swart Shield did,

0:43:15.719 --> 0:43:18.480
<v Speaker 1>and he did this by using a system of spherical coordinates.

0:43:18.680 --> 0:43:21.000
<v Speaker 1>Short Shield discovered that if you imagine the mass of

0:43:21.080 --> 0:43:24.800
<v Speaker 1>a star compressed down to a great density around it

0:43:24.880 --> 0:43:28.160
<v Speaker 1>in all directions reaching out to a specific radius later

0:43:28.239 --> 0:43:32.360
<v Speaker 1>known as the swart Shield radius, would form this gravitational

0:43:32.680 --> 0:43:36.479
<v Speaker 1>dead zone. Anything that went into the dead zone, whether

0:43:36.560 --> 0:43:40.440
<v Speaker 1>it was matter, light, whatever, would never come out again.

0:43:41.040 --> 0:43:43.640
<v Speaker 1>And this spherical dead zone came to be known at

0:43:43.680 --> 0:43:47.120
<v Speaker 1>the time as the schwart Shield sphere. Now we call

0:43:47.239 --> 0:43:51.200
<v Speaker 1>the boundary leading over into this zone today the event horizon,

0:43:51.440 --> 0:43:53.240
<v Speaker 1>and that's where you get the movie title. Of course,

0:43:53.760 --> 0:43:56.000
<v Speaker 1>that's sort of the outer boundary of the zone of

0:43:56.160 --> 0:43:59.960
<v Speaker 1>total influence of the black hole. Because inside this radius,

0:44:00.120 --> 0:44:04.360
<v Speaker 1>inside the event horizon, swart Shield concluded that all radiation

0:44:04.440 --> 0:44:07.480
<v Speaker 1>and matter passing into the sphere would become stuck. And

0:44:07.600 --> 0:44:10.399
<v Speaker 1>of course, under general relativity, if you were flying into

0:44:10.480 --> 0:44:15.080
<v Speaker 1>this sphere, outside, observers would notice your time slowing down

0:44:15.280 --> 0:44:18.560
<v Speaker 1>as you approached the sphere, and to those observers out there,

0:44:18.719 --> 0:44:21.680
<v Speaker 1>you would appear to sort of stop as you crossed over.

0:44:22.120 --> 0:44:24.640
<v Speaker 1>So do the people imagining this object, like, what would

0:44:24.640 --> 0:44:28.200
<v Speaker 1>they picture? Maybe according to this conception, anything entering the

0:44:28.280 --> 0:44:31.400
<v Speaker 1>sphere of the short Shield radius would seem to appear

0:44:31.560 --> 0:44:34.239
<v Speaker 1>frozen forever in time at the moment it was about

0:44:34.280 --> 0:44:38.000
<v Speaker 1>to cross over into the dead zone. Speaking, this made

0:44:38.040 --> 0:44:40.640
<v Speaker 1>me think about one of the videos we watched from

0:44:40.640 --> 0:44:42.640
<v Speaker 1>the World You were there at the event, but one

0:44:42.840 --> 0:44:44.799
<v Speaker 1>that I watched from the World Science Festival this year

0:44:44.880 --> 0:44:49.160
<v Speaker 1>had a astrophysicist Chep Doleman talking about black holes and

0:44:49.280 --> 0:44:52.160
<v Speaker 1>he said, quote, what happens in the black hole stays

0:44:52.200 --> 0:44:55.480
<v Speaker 1>in the black hole. Yeah. I like that. That that

0:44:55.640 --> 0:44:58.560
<v Speaker 1>that oftentimes you see the especially the more modern physicists

0:44:58.560 --> 0:45:01.239
<v Speaker 1>who who have written about black holes that they tend

0:45:01.320 --> 0:45:06.319
<v Speaker 1>to have a sense of humor regarding their nature. Yeah, yeah,

0:45:06.360 --> 0:45:09.680
<v Speaker 1>I think that's generally true, like they don't get all well.

0:45:09.719 --> 0:45:12.840
<v Speaker 1>I mean, so here's what you can contrast that lighthearted

0:45:12.880 --> 0:45:17.600
<v Speaker 1>approach with. Apparently some French speaking astrophysicists took to calling

0:45:17.640 --> 0:45:23.399
<v Speaker 1>the short shield sphere the sphere catastrophe, the sphere that's

0:45:23.400 --> 0:45:26.400
<v Speaker 1>a hard thing to say, sphere catastrophe. I like the

0:45:26.480 --> 0:45:28.920
<v Speaker 1>idea of this, of this is being the avant garde

0:45:29.040 --> 0:45:32.800
<v Speaker 1>French version of the event Arizon. Oh I'd pay to

0:45:32.840 --> 0:45:35.120
<v Speaker 1>see that. I hope it's still have sam Neil. Now

0:45:35.200 --> 0:45:39.239
<v Speaker 1>we go with the instead. Oh yeah, okay, it would be.

0:45:39.360 --> 0:45:41.680
<v Speaker 1>It would be a great version of event Horizon where

0:45:41.880 --> 0:45:45.080
<v Speaker 1>every scene they have fresh baked bread. Now, one thing

0:45:45.120 --> 0:45:47.760
<v Speaker 1>that's worth noting about the sphere of doom, the schwart

0:45:47.800 --> 0:45:51.400
<v Speaker 1>shield sphere or the sphere catastrophe, it's not actually the

0:45:51.600 --> 0:45:56.120
<v Speaker 1>same as the central object, the black hole itself. An

0:45:56.160 --> 0:46:00.360
<v Speaker 1>example given in Marcia Bartosik's black Hole, our son is

0:46:00.360 --> 0:46:04.040
<v Speaker 1>about one point four million kilometers wide. If a star

0:46:04.400 --> 0:46:07.920
<v Speaker 1>the mass of our Sun were compressed down to a point,

0:46:08.400 --> 0:46:11.759
<v Speaker 1>the sphere catastropheke surrounding it would be less than six

0:46:11.880 --> 0:46:15.760
<v Speaker 1>kilometers across. If the mass of ten sons were reduced

0:46:15.800 --> 0:46:19.239
<v Speaker 1>to a point like volume, its sphere catastrophe would be

0:46:19.280 --> 0:46:22.680
<v Speaker 1>about sixty kilometers wide. And as we mentioned earlier, if

0:46:22.719 --> 0:46:24.920
<v Speaker 1>our son were to suddenly shrink down to that size,

0:46:24.960 --> 0:46:28.360
<v Speaker 1>objects far outside the sphere would not suddenly be like

0:46:28.560 --> 0:46:32.400
<v Speaker 1>sucked in or torn apart. The planets would continue orbiting

0:46:32.480 --> 0:46:35.200
<v Speaker 1>just like they orbit the Sun, only it's only much

0:46:35.280 --> 0:46:38.239
<v Speaker 1>closer that things would really go crazy. But here's a

0:46:38.320 --> 0:46:41.040
<v Speaker 1>really important point that we need to drive home. At

0:46:41.120 --> 0:46:45.160
<v Speaker 1>this stage, even after short Shield had done these these calculations,

0:46:45.320 --> 0:46:48.640
<v Speaker 1>most physicists and astronomers did not believe a black hole

0:46:48.719 --> 0:46:52.080
<v Speaker 1>could exist in nature. Uh. Einstein just thought that short

0:46:52.120 --> 0:46:55.160
<v Speaker 1>Shield sphere sphere of doom thing was a sign there

0:46:55.200 --> 0:46:57.040
<v Speaker 1>was still some things to work out in the theory,

0:46:57.080 --> 0:46:59.880
<v Speaker 1>and Einstein did not think that black holes would be

0:47:00.040 --> 0:47:03.400
<v Speaker 1>found in the actual universe. So at the time, the

0:47:03.520 --> 0:47:05.360
<v Speaker 1>idea that it might have just been a mirror ghost

0:47:05.480 --> 0:47:08.440
<v Speaker 1>in the math kind of a remainder that had to

0:47:08.480 --> 0:47:10.680
<v Speaker 1>be figured out later on. Yeah, so you do the

0:47:10.800 --> 0:47:13.120
<v Speaker 1>math and you say, oh, this is a strange finding.

0:47:13.320 --> 0:47:16.960
<v Speaker 1>But people, I think, just assumed, Well, so we'll find

0:47:17.040 --> 0:47:19.000
<v Speaker 1>out something in the future that will make sense of

0:47:19.040 --> 0:47:22.000
<v Speaker 1>all this, you know, we will have some kind of observation,

0:47:22.160 --> 0:47:25.279
<v Speaker 1>some update to the theory, something that will eventually let

0:47:25.400 --> 0:47:27.960
<v Speaker 1>us know, oh, okay, there's not actually such a thing

0:47:28.000 --> 0:47:29.960
<v Speaker 1>as a black hole. They weren't calling it a black

0:47:30.000 --> 0:47:32.160
<v Speaker 1>hole at the time, but there's not actually one of

0:47:32.239 --> 0:47:35.000
<v Speaker 1>these to be found in nature. Something prevents this from happening.

0:47:35.640 --> 0:47:38.799
<v Speaker 1>So remember Arthur Eddington, the English astro physicist who did

0:47:38.840 --> 0:47:43.160
<v Speaker 1>the eclipse experiment about general relativity. In his nineteen book

0:47:43.239 --> 0:47:46.279
<v Speaker 1>The Internal Constitution of the Stars, he wrote, I think,

0:47:46.719 --> 0:47:50.320
<v Speaker 1>kind of dryly, invoking some awesome imagery, I might add quote,

0:47:51.520 --> 0:47:54.440
<v Speaker 1>a star of two d and fifty million kilometers radius

0:47:54.760 --> 0:47:58.440
<v Speaker 1>could not possibly have so high a density as the Sun. Firstly,

0:47:58.560 --> 0:48:01.319
<v Speaker 1>the force of gravitation would so great that light would

0:48:01.320 --> 0:48:04.400
<v Speaker 1>be unable to escape it, the rays falling back to

0:48:04.480 --> 0:48:07.279
<v Speaker 1>the star like a stone to the Earth. Secondly, the

0:48:07.400 --> 0:48:10.040
<v Speaker 1>red shift of the spectral lines would be so great

0:48:10.120 --> 0:48:13.440
<v Speaker 1>that the spectrum would be shifted out of existence. Thirdly,

0:48:13.800 --> 0:48:17.320
<v Speaker 1>the mass would produce so much curvature of the space

0:48:17.440 --> 0:48:21.640
<v Speaker 1>time metric that space would close up around the star,

0:48:22.239 --> 0:48:27.160
<v Speaker 1>leaving us outside i e. Nowhere. So the idea is

0:48:27.239 --> 0:48:30.600
<v Speaker 1>that it would can suddenly contain all of space, and

0:48:30.640 --> 0:48:32.960
<v Speaker 1>then we couldn't be in space anymore. Well, when you

0:48:33.000 --> 0:48:34.800
<v Speaker 1>put it like that, it does sound like a like

0:48:34.880 --> 0:48:37.719
<v Speaker 1>a mathematical problem that has to be worked out later on.

0:48:38.360 --> 0:48:41.040
<v Speaker 1>But of course Eddington was wrong about that, and even

0:48:41.120 --> 0:48:44.440
<v Speaker 1>Schwartzfield himself didn't think you would find these mathematical objects

0:48:44.480 --> 0:48:46.880
<v Speaker 1>in nature. He thought that sort of the outward pressure

0:48:46.920 --> 0:48:49.640
<v Speaker 1>of stars would prevent them from collapsing down to a

0:48:50.120 --> 0:48:54.120
<v Speaker 1>volume smaller than that sphere catastrophe. And remember he was

0:48:54.200 --> 0:48:57.160
<v Speaker 1>not setting out to posit the existence of black holes.

0:48:57.239 --> 0:49:00.279
<v Speaker 1>That wasn't his goal. That they just simply pop up

0:49:00.400 --> 0:49:04.040
<v Speaker 1>as this weird byproduct of him using general relativity to

0:49:04.160 --> 0:49:07.760
<v Speaker 1>calculate the gravitational fields generated by different kinds of massive

0:49:07.800 --> 0:49:11.480
<v Speaker 1>bodies in space. Now we have to stress here that

0:49:11.640 --> 0:49:14.439
<v Speaker 1>sword Shield didn't call it a black hole. He called

0:49:14.440 --> 0:49:17.719
<v Speaker 1>it a discontinuity. Yeah, what did Eddington call it? Oh?

0:49:17.800 --> 0:49:20.839
<v Speaker 1>He called it a magic circle. Oh that's really good.

0:49:21.360 --> 0:49:23.759
<v Speaker 1>I kind of wish we'd stuck with that. Yeah, though

0:49:23.800 --> 0:49:26.160
<v Speaker 1>that of course has its own baggage. You expect like

0:49:26.320 --> 0:49:28.759
<v Speaker 1>elves to come flying out of it, right. Uh No,

0:49:28.920 --> 0:49:32.600
<v Speaker 1>But the term black hole was coined later still by

0:49:32.760 --> 0:49:37.240
<v Speaker 1>American theoretical physicist John Archibald Wheeler, who lived nineteen eleven

0:49:37.280 --> 0:49:39.600
<v Speaker 1>through two thousand and eight. Did he coin it or

0:49:39.719 --> 0:49:42.080
<v Speaker 1>was he just the first one to start using it? Well?

0:49:42.560 --> 0:49:45.120
<v Speaker 1>He has. So the story that I read is that

0:49:45.320 --> 0:49:47.200
<v Speaker 1>he was in a conference in New York City in

0:49:47.280 --> 0:49:51.000
<v Speaker 1>nineteen sixty seven and he apparently seized on a suggestion

0:49:51.320 --> 0:49:54.520
<v Speaker 1>shouted from the audience. I'm a I'm as I could.

0:49:54.560 --> 0:49:57.120
<v Speaker 1>I couldn't find out what the exact shout was, but

0:49:57.160 --> 0:49:59.839
<v Speaker 1>I'm assuming it was something like call it a black hole, John,

0:50:00.120 --> 0:50:02.920
<v Speaker 1>or that's a black hole, something of that effect, or

0:50:03.000 --> 0:50:05.600
<v Speaker 1>just maybe a chant black hole black hole. So he

0:50:05.719 --> 0:50:07.680
<v Speaker 1>was like trying to work the audience. He's like, throw

0:50:07.719 --> 0:50:09.600
<v Speaker 1>out some names, come on, give me some ideas, and

0:50:09.680 --> 0:50:13.080
<v Speaker 1>people are like magic circle and he's like, nah, no,

0:50:13.239 --> 0:50:16.200
<v Speaker 1>no magic circles here. Yeah, it's like improv alright, somebody

0:50:16.280 --> 0:50:19.239
<v Speaker 1>give me a theme and we'll we'll construct some sort

0:50:19.280 --> 0:50:23.640
<v Speaker 1>of theoretical physics structure out of it. How about dark Star?

0:50:25.520 --> 0:50:31.200
<v Speaker 1>So in his autobiography Sphere Catastrophe, I would like to

0:50:31.200 --> 0:50:34.400
<v Speaker 1>see an improv sketch around the sphere catastrophe. Uh So.

0:50:34.800 --> 0:50:38.640
<v Speaker 1>In his autobiography, Wheeler wrote that the black hole quote

0:50:38.840 --> 0:50:41.919
<v Speaker 1>teaches us that space can be crumpled like a piece

0:50:41.960 --> 0:50:45.719
<v Speaker 1>of paper into an infanticible dot, that time can be

0:50:45.840 --> 0:50:48.800
<v Speaker 1>extinguished like a blown out flame, and that the laws

0:50:48.840 --> 0:50:52.800
<v Speaker 1>of physics that we regard as sacred, as immutable or anything,

0:50:52.920 --> 0:50:55.439
<v Speaker 1>but which I think sums it up rather nicely. Yeah,

0:50:56.000 --> 0:50:59.520
<v Speaker 1>I like that. Well, I mean it also Wheeler, there

0:50:59.600 --> 0:51:03.160
<v Speaker 1>he speaking, Einstein is ms right, Like the whole idea

0:51:03.200 --> 0:51:05.640
<v Speaker 1>of general relativity is that we used to think, oh,

0:51:05.719 --> 0:51:08.160
<v Speaker 1>space and time, those are the things that are constant

0:51:08.200 --> 0:51:10.960
<v Speaker 1>and immutable, and other stuff can can get moved around,

0:51:11.080 --> 0:51:13.759
<v Speaker 1>and we found out through relativity. No, well, the speed

0:51:13.800 --> 0:51:15.879
<v Speaker 1>of light and a vacuum might be constant, but space

0:51:15.960 --> 0:51:18.000
<v Speaker 1>and time you mess all. You mess with them a

0:51:18.120 --> 0:51:23.239
<v Speaker 1>lot and Wheeler Wheeler is carrying that torch. So maybe

0:51:23.320 --> 0:51:25.280
<v Speaker 1>that's going to be where we have to wrap up today.

0:51:25.480 --> 0:51:28.280
<v Speaker 1>But the big question left lingering for us to explore

0:51:28.360 --> 0:51:31.640
<v Speaker 1>next time is how did this mathematical curiosity this sort

0:51:31.680 --> 0:51:34.440
<v Speaker 1>of like weird artifact of people trying to solve problems

0:51:34.520 --> 0:51:38.719
<v Speaker 1>on paper become a feature that scientists actually think exists

0:51:38.880 --> 0:51:42.080
<v Speaker 1>out in the physical world, and how do we detect

0:51:42.200 --> 0:51:44.919
<v Speaker 1>them if they do exist? You will find out next time.

0:51:45.480 --> 0:51:48.120
<v Speaker 1>In the meantime, however, be sure to head on over

0:51:48.239 --> 0:51:50.120
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0:51:55.280 --> 0:51:57.680
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