WEBVTT - Black Holes, Part 3: The Future

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<v Speaker 1>Welcome to Stuff to Blow Your Mind from how Stuff

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<v Speaker 1>Works dot com. Hey, welcome to Stuff to Blow your Mind.

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<v Speaker 1>My name is Robert Lamb and I'm Joe McCormick, and

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<v Speaker 1>you are here. We're here. It's part three of our

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<v Speaker 1>exploration of black holes. Now. I think this all came about, Robert,

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<v Speaker 1>because you went to the World Science Festival and saw

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<v Speaker 1>a great presentation on black holes. In't that right? Yes,

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<v Speaker 1>it was called Darkness Visible, Shedding New Light on black Holes.

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<v Speaker 1>It's a tremendous presentation. It's available on YouTube for your viewing,

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<v Speaker 1>and I'll make sure that there is a link to

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<v Speaker 1>it on the landing page for this episode. It's Stuff

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<v Speaker 1>to Blow your Mind dot com. Now, it's funny. This

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<v Speaker 1>is gonna be our third episode in a row on

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<v Speaker 1>black holes, and this will be the last one for now.

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<v Speaker 1>We will probably revisit the subject again in the future,

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<v Speaker 1>because even in three whole episodes, there's no way to

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<v Speaker 1>even come close to exploring all of the interesting stuff

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<v Speaker 1>about black holes. But we're here for part three. In

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<v Speaker 1>the first part, we explored the sort of the idea

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<v Speaker 1>history of black holes, like where they came from conceptually

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<v Speaker 1>before anybody had ever looked up and seen one. And

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<v Speaker 1>then in the second episode we tried to talk about

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<v Speaker 1>ways of inferring the physical existence of black holes, not

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<v Speaker 1>just the theoretical framework underlying them, but how we can

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<v Speaker 1>detect them out there in the universe. And then in

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<v Speaker 1>today's episode, we wanted to sort of like, uh, just

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<v Speaker 1>do a grab bag of interesting outstanding questions about black

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<v Speaker 1>holes or thought experiments involving what we know about black

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<v Speaker 1>holes today. Yeah, then we'll get into some sort of

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<v Speaker 1>sci fi ideas here as well for sure, which, of course,

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<v Speaker 1>uh brings us back to the topic of cinematic betrayals

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<v Speaker 1>of black holes. We talked a little bit about the

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<v Speaker 1>Disney movie The Black Hole. In the previous episodes we

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<v Speaker 1>talked about Interstellar and how Interstellar is is actually a

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<v Speaker 1>pretty good um scientific model to look at as far

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<v Speaker 1>as depictions of black holes in cinema. But then of

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<v Speaker 1>course there's Event Horizon, Oh is there? This was the

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<v Speaker 1>Paul W. S Anderson film, arguably in my mind, the

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<v Speaker 1>best um Paul W. S Anderson film. What would be

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<v Speaker 1>the other candidate for the best Paul W. S Anderson

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<v Speaker 1>film one of the Resident Evils, I guess one of

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<v Speaker 1>the seven or Eight Resident Evils or Mortal Kombat. You

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<v Speaker 1>know you can go with that. That was his film

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<v Speaker 1>prior to Event Horizon. No, I don't want to be mean,

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<v Speaker 1>but to be generous, we could say not this generation's

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<v Speaker 1>most highbrow filmmaker. Not to say that that that you

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<v Speaker 1>and I are purely highbrow of Cinnema enthusiasts. No, we

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<v Speaker 1>love some trash, and boy's Event Horizon some delectable nineties trash.

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<v Speaker 1>It's it's got funny c g I. It's got get

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<v Speaker 1>to the Chopper kind of stuff. It's got a great cast. Actually,

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<v Speaker 1>it's got hilariously bad writing. It's uh yeah, it's solid

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<v Speaker 1>B movie territory. It certainly is in that it has

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<v Speaker 1>uh well, I mean for starters. It's it's certainly not

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<v Speaker 1>a beam of you if when it comes to the

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<v Speaker 1>amount of money that's enter this thing. But in terms

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<v Speaker 1>of of of of looking when you look at it

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<v Speaker 1>as a whole, there are a lot of problems when

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<v Speaker 1>you but when you look at some of the of

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<v Speaker 1>the elements that go into making the film, there are

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<v Speaker 1>a lot of things I like about it. I think

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<v Speaker 1>the ship looks really cool, this ideal leather punk spaceship, yeah,

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<v Speaker 1>I mean it looks like a cathedral. They I like

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<v Speaker 1>how it incorporates some of these, um these these very

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<v Speaker 1>obvious elements from films like the Shining uh you know,

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<v Speaker 1>two thousand and one of Space Odyssey Solaris and brings

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<v Speaker 1>them all to together. I bet you like the soundtrack,

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<v Speaker 1>don't you. Well. I thought I was gonna like the

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<v Speaker 1>soundtrack because it's been a long time since I've seen this,

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<v Speaker 1>like possibly since high school, and I rewatched rewatched it

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<v Speaker 1>before we went into to to record this episode. The

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<v Speaker 1>main thing I was remembering here was that, oh yeah,

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<v Speaker 1>Orbital worked on the soundtrack Orbital of course, or Legends

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<v Speaker 1>of the electronic genre that for instance there the Orbital

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<v Speaker 1>too is a classic, and I recommend everyone who's into

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<v Speaker 1>electronic and ambience you should check it out. They were

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<v Speaker 1>also on the soundtrack of the Paul ws Anderson film

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<v Speaker 1>Mortal Kombat. Yeah, so that that soundtrack was pretty awesome

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<v Speaker 1>back in the day. But you know me, I love

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<v Speaker 1>a good electronic score. So I went back to View

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<v Speaker 1>of the Horizon expecting there to be a lot more Orbital,

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<v Speaker 1>a lot more electronic uh nuance. But the thing is,

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<v Speaker 1>it's not just an orbital score. It's orbital and Michael Common,

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<v Speaker 1>and Michael Common brings the the orchestral stuff into this equation,

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<v Speaker 1>and it really felt like there was far It was

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<v Speaker 1>a far more traditional film score than I really wanted

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<v Speaker 1>to hear. It's one of those beat you over the

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<v Speaker 1>head horror scores, you know, I hope you want some

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<v Speaker 1>was Yeah. Yeah, so it did not really Uh it

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<v Speaker 1>did did not really please me on that level. Um,

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<v Speaker 1>but I you know, I like this. I like the ship,

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<v Speaker 1>I like some of the horror elements, and the cast

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<v Speaker 1>is so good that you can forgive a lot of things,

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<v Speaker 1>like when Sam neil Is is your lead actor, it

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<v Speaker 1>forgives a lot of sins. And he, arguably, I would argue,

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<v Speaker 1>plays the best possible pinhead in this true he essentially

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<v Speaker 1>becomes a cinebyte in this film, and in doing so,

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<v Speaker 1>he's like he's a cut above any other cinematic cinebyte. Yeah.

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<v Speaker 1>You could argue that Event Horizon is a very bad movie,

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<v Speaker 1>but that it might be in a way the best

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<v Speaker 1>Hell raisor sequel. Yeah, yeah, I would agree with that. Now,

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<v Speaker 1>of course, that the harder Why are we talking about

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<v Speaker 1>Event Horizon? As we touched we've discussed already in There's

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<v Speaker 1>a black Hole episodes. The event horizon is the point

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<v Speaker 1>at which light cannot escape the gravity of the singularity.

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<v Speaker 1>It's the point of no return, right, So you've got

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<v Speaker 1>this incredibly dense core at the middle of a black hole. Say,

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<v Speaker 1>if your black hole is the remnant of a collapse star.

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<v Speaker 1>You know, your star goes supernova, blasts a lot of

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<v Speaker 1>its material out into space, and then it's got this

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<v Speaker 1>remnant leftover that's very din It's within what's known as

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<v Speaker 1>short shield radius, and if it's within that radius, it

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<v Speaker 1>will collapse upon itself in this weird process that even

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<v Speaker 1>now we're still trying to understand most fully. It will

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<v Speaker 1>collapse it this way that it looks like it collapses

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<v Speaker 1>towards infinite density, and it creates this sphere around it

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<v Speaker 1>where anything that goes inside the sphere never comes out again.

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<v Speaker 1>It cannot overcome the force of gravity. It just becomes

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<v Speaker 1>part of the black hole. Right. And in the film

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<v Speaker 1>Event Arizon, the essential science the argument that is made

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<v Speaker 1>uh when when Sam Neil's character Like is forced to

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<v Speaker 1>explain this to the crew of a spaceship who apparently

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<v Speaker 1>have no idea how space works. Uh. Apparently the Event

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<v Speaker 1>Horizon spaceship creates an artificial singularity which is then used

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<v Speaker 1>to open a wormhole of some sort. And that's that's

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<v Speaker 1>his about is is? Uh? Is detailed as the explanation

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<v Speaker 1>gets so also they go to Hell? Well, yes, but

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<v Speaker 1>that's that's how they get there through the wormhole, or

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<v Speaker 1>the wormhole goes through Hell. I've done a little vague here.

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<v Speaker 1>So why have we spent so much time talking about

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<v Speaker 1>Event Horizon. Here's why, because I'm going to argue that

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<v Speaker 1>I think a scientifically accurate movie about going to a

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<v Speaker 1>black hole could be scarier than a movie where you

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<v Speaker 1>need to put hell and demons in there. All right, Well,

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<v Speaker 1>that that can be the argument we make during the

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<v Speaker 1>course of this episode for sure. Okay, well, I think

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<v Speaker 1>we should talk about what would be like if you

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<v Speaker 1>want to fall into a black hole. Let's say you

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<v Speaker 1>get a hanker and you're saying, I want to approach

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<v Speaker 1>infinite density. Hey it's two thousand eighteen. Yeah, you know,

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<v Speaker 1>I totally understand that desire. I feel flabby, I feel

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<v Speaker 1>kind of bloated. I'm going for infinite density now, So

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<v Speaker 1>you say I'm going to fall into a black hole.

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<v Speaker 1>You've decided to hop into a spaceship, travel out into

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<v Speaker 1>the universe, and intentionally fly straight into a very big

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<v Speaker 1>black hole. Now, there are a lot of people who

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<v Speaker 1>have written about this subject, trying to imagine what it

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<v Speaker 1>would be like, the subjective experience of approaching a black hole,

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<v Speaker 1>crossing the event her Eisen, and then falling in. Uh there.

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<v Speaker 1>I think Neil de grass Tyson actually has a book

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<v Speaker 1>about it. I haven't read that book, but I've read

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<v Speaker 1>a bunch of stuff about this. Probably the best explanation

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<v Speaker 1>I've read, and one of my main sources here is

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<v Speaker 1>going to be an explanation from the astrophysicist Ethan Siegel,

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<v Speaker 1>who is astrophysicist and a science blogger. He runs the

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<v Speaker 1>Starts with a Bang blog. Do you ever read that, Robert?

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<v Speaker 1>He writes good stuff about astrophysics. Um so, so he's

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<v Speaker 1>got an exploration here that I think is pretty good.

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<v Speaker 1>So he says, Okay, you imagine you're approaching a black hole,

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<v Speaker 1>and if the black hole were the mass of Earth,

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<v Speaker 1>the sphere that you do you'd be approaching would only

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<v Speaker 1>be about one centimeter in radius or about two centimeters wide.

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<v Speaker 1>If the black hole were about the mass of the Sun,

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<v Speaker 1>the sphere would only be about three kilometers in radius

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<v Speaker 1>or about six kilometers wide. So the actual spheres of

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<v Speaker 1>the event horizon that you would see are are much

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<v Speaker 1>smaller than a lot of the other things you'd encounter

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<v Speaker 1>out in the universe. That is, unless you're coming up

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<v Speaker 1>against one of the biggest ones, like say, a super

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<v Speaker 1>massive black hole. The kinds of that are at the

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<v Speaker 1>center of galaxies, So as you approach the black hole

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<v Speaker 1>from a kind of normal orbital distance. One of the

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<v Speaker 1>funny things is that, first of all, you might not

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<v Speaker 1>immediately notice anything strange about the gravity. The gravitational influence

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<v Speaker 1>you would feel would be a lot like approaching or

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<v Speaker 1>orbiting a star of the same mass. And to reiterate,

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<v Speaker 1>if a star the size of our Sun were suddenly

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<v Speaker 1>magically turned into a black hole. Uh and by the way,

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<v Speaker 1>this would not ever happen in point of fact, because

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<v Speaker 1>our son is not massive enough to naturally become a

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<v Speaker 1>black hole. But if you were to buy magic turn

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<v Speaker 1>it into a black hole of the same mass, Earth

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<v Speaker 1>would simply continue orbiting. It wouldn't be immediately sucked in

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<v Speaker 1>or anything. Things would get very weird on Earth but

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<v Speaker 1>but yeah, we would not be sucked into the black hole. Right.

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<v Speaker 1>But once you got closer, then things really do start

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<v Speaker 1>to get weirder, especially when you get very close. So

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<v Speaker 1>as you approach the black hole, first of all, you

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<v Speaker 1>would notice that as you get closer, the black back

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<v Speaker 1>hole gets bigger faster than any normal object would as

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<v Speaker 1>you approached it. So you might have a normal sense

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<v Speaker 1>of Okay, I'm flying towards a planet, or I'm flying

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<v Speaker 1>towards a star. At a certain speed, you can have

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<v Speaker 1>a pretty predictable rate of its expansion to take up

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<v Speaker 1>more and more degrees of your field of view. Right

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<v Speaker 1>as you near a black hole, the black hole actually

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<v Speaker 1>gets bigger faster than any normal object would because rays

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<v Speaker 1>of light beaming towards you passing all around the black

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<v Speaker 1>hole are bent dramatically inward. Now, remember what we'd actually

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<v Speaker 1>be seeing out there is you'd see sort of a

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<v Speaker 1>black disc with light warped around it. Remember the short

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<v Speaker 1>shield radius, the distance from the center of the black

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<v Speaker 1>hole to the event horizon. Uh. The the event horizon,

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<v Speaker 1>of course, is the sphere catastrophe, the point beyond which nothing,

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<v Speaker 1>not even light can escape. And as you approach that sphere.

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<v Speaker 1>More closely, the apparent short shield radius from your point

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<v Speaker 1>of view will grow dramatically. A seagull rights that by

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<v Speaker 1>the time you're about ten schwart shield radii away from

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<v Speaker 1>the black holes, about ten of the radius of the

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<v Speaker 1>black hole away from it, it will appear so big

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<v Speaker 1>that it will blot out your entire forward forward facing

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<v Speaker 1>view right, so if you're looking toward it, it will

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<v Speaker 1>be your entire field of view. A normal object of

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<v Speaker 1>the same size at that distance would only appear to

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<v Speaker 1>be about the size of your fist at an arm's length.

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<v Speaker 1>Then you go deeper and you can reach There are

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<v Speaker 1>several sort of stops along the way. One of the

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<v Speaker 1>stops you would reach along the way is what's known

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<v Speaker 1>as the innermost stable circular orbit, or the I s

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<v Speaker 1>c O. This is sort of the last filling station

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<v Speaker 1>before you head down to the border. The I s

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<v Speaker 1>c O is about one point five times the radius

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<v Speaker 1>of the event horizon, and it's what it sounds like

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<v Speaker 1>based on the name. It's the closest that particles can

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<v Speaker 1>orbit the black hole in a stable circle. Go any

0:11:54.640 --> 0:11:58.600
<v Speaker 1>closer and it's all downhill, pretty much literally. By the

0:11:58.640 --> 0:12:00.520
<v Speaker 1>time you reach the I s c O. If you

0:12:00.559 --> 0:12:03.320
<v Speaker 1>face a black hole, you will see nothing but black

0:12:03.360 --> 0:12:05.559
<v Speaker 1>in the direction of the black hole, and the event

0:12:05.640 --> 0:12:08.160
<v Speaker 1>horizon will appear to take up your your whole field

0:12:08.160 --> 0:12:11.080
<v Speaker 1>of view. But here's the crazy part. You keep going

0:12:11.160 --> 0:12:14.240
<v Speaker 1>down past the I s c OH and of course

0:12:14.280 --> 0:12:16.760
<v Speaker 1>total blackness will still take up your entire field of

0:12:16.800 --> 0:12:19.840
<v Speaker 1>view if you look toward the black hole. But here's

0:12:19.880 --> 0:12:22.960
<v Speaker 1>what happens if you turn around and look away. And

0:12:23.000 --> 0:12:25.240
<v Speaker 1>I'll explore this in a couple of different ways. First,

0:12:25.320 --> 0:12:28.200
<v Speaker 1>a scenario one. This is where you imagine it's only

0:12:28.360 --> 0:12:31.920
<v Speaker 1>you falling in. It's not light or other stuff falling

0:12:31.920 --> 0:12:33.560
<v Speaker 1>in with you. And this is not how it would

0:12:33.559 --> 0:12:37.600
<v Speaker 1>probably really be, just to illustrate the gravitational influences involved.

0:12:37.840 --> 0:12:40.520
<v Speaker 1>If you keep going toward the black hole and you

0:12:40.640 --> 0:12:43.400
<v Speaker 1>turn back and look away from it as you're falling in,

0:12:43.920 --> 0:12:47.000
<v Speaker 1>you will see total darkness begin to creep in from

0:12:47.040 --> 0:12:51.520
<v Speaker 1>every direction as well in the direction you came from.

0:12:51.559 --> 0:12:53.640
<v Speaker 1>So you're looking backward, and you will see what looks

0:12:53.679 --> 0:12:57.800
<v Speaker 1>like a membrane of total darkness closing in all around,

0:12:58.480 --> 0:13:01.439
<v Speaker 1>and your view of the stars the universe will shrink

0:13:01.600 --> 0:13:05.000
<v Speaker 1>down to a circle in the direction opposite of the

0:13:05.000 --> 0:13:07.640
<v Speaker 1>black hole. Just try to imagine that your whole view

0:13:08.160 --> 0:13:11.600
<v Speaker 1>of the universe being bent and crushed down into a

0:13:11.679 --> 0:13:16.080
<v Speaker 1>shrinking circle that's receding behind you rapidly. Well again it

0:13:16.120 --> 0:13:20.800
<v Speaker 1>is so I can't imagine that to a certain extent. Yeah,

0:13:20.880 --> 0:13:24.560
<v Speaker 1>all starlight dies in a shrinking circle. That that's that's

0:13:24.559 --> 0:13:27.640
<v Speaker 1>in your past like that. But at this point it's

0:13:27.640 --> 0:13:30.480
<v Speaker 1>important to remember you have not crossed the event horizon yet,

0:13:30.520 --> 0:13:33.200
<v Speaker 1>you're just approaching it. So at this point, if you

0:13:33.200 --> 0:13:35.079
<v Speaker 1>were to change your mind and say, hey, I want

0:13:35.080 --> 0:13:37.680
<v Speaker 1>to get out of here, uh, there is in principle

0:13:37.760 --> 0:13:40.560
<v Speaker 1>still hope if you have a powerful enough spaceship you

0:13:40.600 --> 0:13:42.800
<v Speaker 1>could turn around. You could pile it back towards that

0:13:42.880 --> 0:13:45.960
<v Speaker 1>shrinking circle of starlight and escape the black hole, at

0:13:46.000 --> 0:13:48.440
<v Speaker 1>least in theory. But it is at this point going

0:13:48.480 --> 0:13:51.000
<v Speaker 1>to be a really powerful uphill climb against the gravity

0:13:51.000 --> 0:13:52.959
<v Speaker 1>of the black hole. But let's say, you know, I

0:13:53.000 --> 0:13:55.079
<v Speaker 1>don't want to escape, I just want to keep falling.

0:13:55.160 --> 0:13:58.600
<v Speaker 1>So that's what you do. Assuming you keep looking towards

0:13:58.640 --> 0:14:01.280
<v Speaker 1>that shrinking circle of are light behind you where you

0:14:01.320 --> 0:14:04.560
<v Speaker 1>came from, it will eventually shrink down to a point

0:14:04.679 --> 0:14:07.840
<v Speaker 1>like light source as you near the boundary, as you

0:14:07.880 --> 0:14:10.559
<v Speaker 1>near the event horizon, and right before you cross the

0:14:10.600 --> 0:14:13.840
<v Speaker 1>event horizon, the light from that point will cycle through

0:14:13.840 --> 0:14:17.479
<v Speaker 1>an array of colors due to what's known as gravitational

0:14:17.559 --> 0:14:20.520
<v Speaker 1>blue shifting, so you'll see red than white, than blue.

0:14:21.080 --> 0:14:23.960
<v Speaker 1>And at this point, all the low frequency radiation in

0:14:23.960 --> 0:14:28.520
<v Speaker 1>the universe, stuff like the cosmic microwave background, which stuff

0:14:28.520 --> 0:14:31.000
<v Speaker 1>which is like microwaves and radio waves, not stuff that's

0:14:31.040 --> 0:14:35.040
<v Speaker 1>normally visible, will shift up because of the blue shift

0:14:35.120 --> 0:14:40.239
<v Speaker 1>of the electromagnetic spectrum. It'll shift up into the visible spectrum,

0:14:40.440 --> 0:14:43.200
<v Speaker 1>and you'll actually be able to see the cosmic microwave

0:14:43.240 --> 0:14:47.520
<v Speaker 1>background as a visible blue with your eyes. Then finally

0:14:48.000 --> 0:14:51.120
<v Speaker 1>you hit the border. Okay, so you crossed the event horizon.

0:14:51.160 --> 0:14:54.200
<v Speaker 1>What do you see in this toy scenario where light

0:14:54.360 --> 0:14:57.080
<v Speaker 1>is not falling in with you, you will see nothing

0:14:57.120 --> 0:15:00.440
<v Speaker 1>at all. You have entered ultimate darkness and this point

0:15:00.480 --> 0:15:04.040
<v Speaker 1>there is no escape, no matter what. So let's say

0:15:04.040 --> 0:15:07.040
<v Speaker 1>you say, no, I changed my mind after I crossed

0:15:07.080 --> 0:15:09.720
<v Speaker 1>the event horizon. I want to pilot my spaceship back

0:15:09.760 --> 0:15:12.400
<v Speaker 1>in the direction I came from. So that should be easy, right,

0:15:12.680 --> 0:15:15.240
<v Speaker 1>You just turn around and you come back in exactly

0:15:15.240 --> 0:15:19.720
<v Speaker 1>the opposite direction. You've been traveling. Too bad, you can't

0:15:19.840 --> 0:15:22.880
<v Speaker 1>do it. If you try, you will discover to your

0:15:22.920 --> 0:15:25.720
<v Speaker 1>great surprise that the direction that used to be the

0:15:25.760 --> 0:15:28.760
<v Speaker 1>direction you came from is now downhill into the center

0:15:28.760 --> 0:15:31.560
<v Speaker 1>of the black hole. And in fact, every direction you

0:15:31.640 --> 0:15:34.000
<v Speaker 1>try to go in is downhill into the center of

0:15:34.000 --> 0:15:37.240
<v Speaker 1>the black hole. It is the perfect pit. It is

0:15:37.280 --> 0:15:40.600
<v Speaker 1>a pit in which the only direction is down. You're

0:15:40.640 --> 0:15:43.760
<v Speaker 1>going into that thing no matter what in any travel

0:15:43.840 --> 0:15:47.240
<v Speaker 1>you do would only speed your travel towards the center

0:15:47.280 --> 0:15:49.760
<v Speaker 1>of the thing. That's kind of mind bending to to

0:15:49.760 --> 0:15:52.800
<v Speaker 1>to think about. But yeah, essentially all all roads lead

0:15:52.800 --> 0:15:55.200
<v Speaker 1>to Rome at this point. The remaining question is how

0:15:55.240 --> 0:15:57.600
<v Speaker 1>long does it take you to get to Rome? Right,

0:15:57.640 --> 0:16:00.320
<v Speaker 1>so you've crossed, you can't go back, how long do

0:16:00.360 --> 0:16:02.960
<v Speaker 1>you fall before you sort of reach the center of

0:16:03.000 --> 0:16:06.240
<v Speaker 1>this thing? Seagull rights that quote as you crossed the

0:16:06.280 --> 0:16:09.840
<v Speaker 1>horizon at the super massive four million solar mass black

0:16:09.880 --> 0:16:13.160
<v Speaker 1>hole at the galactic center, believe it or not. Despite

0:16:13.200 --> 0:16:15.400
<v Speaker 1>the fact that we're talking about an event horizon that

0:16:15.480 --> 0:16:18.960
<v Speaker 1>might be around a light hour in diameter in our

0:16:19.000 --> 0:16:22.840
<v Speaker 1>reference frame, it would only take around twenty seconds to

0:16:22.880 --> 0:16:26.200
<v Speaker 1>reach the singularity once you cross the event horizon. Now,

0:16:26.240 --> 0:16:28.760
<v Speaker 1>remember that first scenario was kind of a toy scenario

0:16:28.800 --> 0:16:31.320
<v Speaker 1>where light is falling is not falling in with you.

0:16:31.440 --> 0:16:33.840
<v Speaker 1>That's just to like see what the gravitational effects are.

0:16:34.640 --> 0:16:38.120
<v Speaker 1>The physics of the effects are on display, But we

0:16:38.200 --> 0:16:41.680
<v Speaker 1>created a kind of unrealistic scenario. So in reality, you

0:16:41.680 --> 0:16:44.760
<v Speaker 1>would probably not be approaching and entering a black hole alone,

0:16:44.800 --> 0:16:47.520
<v Speaker 1>but you'd be approaching and entering along with a huge

0:16:47.640 --> 0:16:50.640
<v Speaker 1>tide of light and radiation. And this would mean that

0:16:50.680 --> 0:16:53.400
<v Speaker 1>in reality, your picture of the universe would not shrink

0:16:53.440 --> 0:16:56.000
<v Speaker 1>to a point behind you as you approached the black hole,

0:16:56.280 --> 0:16:59.040
<v Speaker 1>but would remain a kind of warped division of the

0:16:59.080 --> 0:17:02.920
<v Speaker 1>sky following you down through the darkness after you crossed

0:17:02.960 --> 0:17:05.440
<v Speaker 1>the event horizon, and that light that you would see

0:17:05.440 --> 0:17:08.120
<v Speaker 1>would be the light that's been sucked toward and into

0:17:08.160 --> 0:17:11.880
<v Speaker 1>the event horizon with you. But as as we've been

0:17:11.880 --> 0:17:16.239
<v Speaker 1>talking about before, unless you just assume some kind of

0:17:16.240 --> 0:17:21.119
<v Speaker 1>technological or magical form of invincibility, it's highly possible given

0:17:21.240 --> 0:17:23.240
<v Speaker 1>various factors. There are a lot of different ways that

0:17:23.320 --> 0:17:25.720
<v Speaker 1>a black hole could be but it's highly possible that

0:17:25.760 --> 0:17:27.840
<v Speaker 1>you would die at pretty much every stage of the

0:17:27.880 --> 0:17:31.639
<v Speaker 1>scenario would be describing um for several reasons, one of

0:17:31.720 --> 0:17:36.119
<v Speaker 1>which is what's been classically known as spaghettification. I've certainly

0:17:36.359 --> 0:17:38.719
<v Speaker 1>heard Neil de grass Tyson speak about this. It's one

0:17:38.760 --> 0:17:42.800
<v Speaker 1>of the astrophysicists favorite concepts. Uh So, as you approach

0:17:42.960 --> 0:17:46.879
<v Speaker 1>the center of gravity of smaller classes of black holes,

0:17:47.440 --> 0:17:51.360
<v Speaker 1>title forces would work you up good and title forces

0:17:51.400 --> 0:17:55.119
<v Speaker 1>occur when an object is stretched and deformed because of

0:17:55.160 --> 0:17:59.320
<v Speaker 1>an imbalance of gravitational forces at different parts of the object.

0:17:59.480 --> 0:18:02.639
<v Speaker 1>We've talked before about Jupiter's moon Io. You know, Io

0:18:02.840 --> 0:18:04.760
<v Speaker 1>is one of the most I think it might be

0:18:04.840 --> 0:18:07.640
<v Speaker 1>the most volcanically active object in the Solar System. If

0:18:07.640 --> 0:18:09.440
<v Speaker 1>it's not the most, it's one of the most. It's

0:18:09.440 --> 0:18:12.639
<v Speaker 1>got these volcanoes erupting. What's causing all of this heat

0:18:12.760 --> 0:18:16.359
<v Speaker 1>and and geologic activity inside Io It's believed to be

0:18:16.440 --> 0:18:20.120
<v Speaker 1>tidal forces of Jupiter acting on the planet that you know, Jupiter.

0:18:20.840 --> 0:18:23.239
<v Speaker 1>It's close enough to Jupiter that Jupiter is kind of

0:18:23.280 --> 0:18:26.480
<v Speaker 1>working the planet with its gravity, and so as you're

0:18:26.520 --> 0:18:28.840
<v Speaker 1>falling into a black hole, a similar kind of working

0:18:28.880 --> 0:18:32.639
<v Speaker 1>would happen on you. Basically, imagine you're falling feet first

0:18:32.840 --> 0:18:36.520
<v Speaker 1>into a relatively small black hole. At a certain radius

0:18:36.520 --> 0:18:38.760
<v Speaker 1>from the black holes center, you would start to notice

0:18:38.840 --> 0:18:42.040
<v Speaker 1>that the force of gravity pulling your feet is a

0:18:42.040 --> 0:18:45.080
<v Speaker 1>lot stronger than the force of gravity pulling your head.

0:18:45.720 --> 0:18:48.400
<v Speaker 1>And since Einstein, we know that the experience of gravity

0:18:48.480 --> 0:18:53.240
<v Speaker 1>is subjectively equivalent to the experience of acceleration through space. Right.

0:18:53.560 --> 0:18:56.760
<v Speaker 1>Gravity is just like being in an accelerating room. So

0:18:56.840 --> 0:19:00.280
<v Speaker 1>imagine you're falling feet first and you discover that your

0:19:00.359 --> 0:19:04.800
<v Speaker 1>feet are accelerating faster than your head is. If you

0:19:04.840 --> 0:19:07.439
<v Speaker 1>were otherwise still alive, when this started to happen to you,

0:19:07.720 --> 0:19:11.080
<v Speaker 1>it would stretch your body out until it ripped into pieces,

0:19:11.280 --> 0:19:13.960
<v Speaker 1>and then those pieces would get stretched and ripped into

0:19:14.000 --> 0:19:16.760
<v Speaker 1>smaller and smaller pieces, until you're just kind of a

0:19:16.800 --> 0:19:20.719
<v Speaker 1>wet carbon particle jelly streaming through toward a point of

0:19:20.720 --> 0:19:24.040
<v Speaker 1>infinite density. Also worth noting, if you did a cannonball

0:19:24.119 --> 0:19:27.080
<v Speaker 1>into the singularity, Uh, then all of this would happen.

0:19:27.160 --> 0:19:30.920
<v Speaker 1>But first, I'm not sure that has any impact in

0:19:31.000 --> 0:19:34.560
<v Speaker 1>anybody's decision making. Oh, it has a lot of impact.

0:19:34.960 --> 0:19:38.720
<v Speaker 1>Somebody should work that up that that should be a paper. Yeah,

0:19:38.720 --> 0:19:42.160
<v Speaker 1>how would the body react? Uh? As a side note,

0:19:42.440 --> 0:19:45.040
<v Speaker 1>you might have heard me mention smaller black holes here.

0:19:45.119 --> 0:19:47.440
<v Speaker 1>Why Why did I mention smaller black holes? It's kind

0:19:47.440 --> 0:19:51.600
<v Speaker 1>of counterintuitive, but actually smaller black holes will tend to

0:19:51.800 --> 0:19:55.680
<v Speaker 1>kill you faster through tidal forces than larger black holes will.

0:19:55.880 --> 0:19:58.960
<v Speaker 1>A much larger black hole actually has a more gentle

0:19:59.000 --> 0:20:04.320
<v Speaker 1>gradient of gravity acceleration. But so we've been imagining one

0:20:04.480 --> 0:20:07.840
<v Speaker 1>type of way of picturing this awesome event, the what

0:20:07.840 --> 0:20:11.240
<v Speaker 1>what it's like to pass into a black hole? One

0:20:11.240 --> 0:20:13.040
<v Speaker 1>of the things that I want to think about is,

0:20:13.080 --> 0:20:15.480
<v Speaker 1>once you're within the event horizon of a black hole,

0:20:16.040 --> 0:20:19.600
<v Speaker 1>does it even make sense to talk about you falling

0:20:19.600 --> 0:20:22.119
<v Speaker 1>into the black hole? To talk about you and the

0:20:22.160 --> 0:20:26.400
<v Speaker 1>black hole as separate objects if you can literally never

0:20:26.560 --> 0:20:30.480
<v Speaker 1>leave no matter what, you are no longer an entity

0:20:30.560 --> 0:20:33.159
<v Speaker 1>separate from the black hole itself. You are part of

0:20:33.200 --> 0:20:36.440
<v Speaker 1>the black hole, and the black hole is you. That's true.

0:20:36.600 --> 0:20:39.399
<v Speaker 1>Like you're no longer a denizen of the larger universe.

0:20:39.400 --> 0:20:42.320
<v Speaker 1>You're denizen of that particular black hole. H and yeah,

0:20:42.320 --> 0:20:45.560
<v Speaker 1>and arguably a part of its substance. Yeah. So maybe

0:20:45.800 --> 0:20:48.200
<v Speaker 1>maybe a more transcendent way of thinking about it would

0:20:48.240 --> 0:20:50.280
<v Speaker 1>be to say, okay, when you fall into a black hole,

0:20:50.560 --> 0:20:54.120
<v Speaker 1>it doesn't just kill you. You get to become it

0:20:54.880 --> 0:20:57.440
<v Speaker 1>consolation price. Yeah, alright, On that note, we're going to

0:20:57.520 --> 0:21:00.240
<v Speaker 1>take a break and when we come back, we will

0:21:00.280 --> 0:21:03.720
<v Speaker 1>discuss more of the mysteries and wonders within the black hole.

0:21:04.520 --> 0:21:08.520
<v Speaker 1>Thank alright, we're back now. One of the things I

0:21:08.560 --> 0:21:10.720
<v Speaker 1>know they talked about in the Darkness Visible event you

0:21:10.760 --> 0:21:13.920
<v Speaker 1>saw in New York was the relationship between black holes

0:21:13.920 --> 0:21:17.560
<v Speaker 1>and entropy? What what was the deal here? Alright, I'm

0:21:17.600 --> 0:21:20.160
<v Speaker 1>gonna I'm gonna attempt to explain all of this and

0:21:20.280 --> 0:21:23.480
<v Speaker 1>uh and I do just want to advise listeners more

0:21:23.520 --> 0:21:26.480
<v Speaker 1>than usual that if if this doesn't completely make sense,

0:21:27.080 --> 0:21:30.240
<v Speaker 1>do check out the talk, because I get to hear

0:21:30.560 --> 0:21:33.520
<v Speaker 1>a pair of experts discuss it, uh in with more

0:21:33.600 --> 0:21:37.440
<v Speaker 1>time and with with greater expertise. But but I will

0:21:37.440 --> 0:21:40.560
<v Speaker 1>attempt to to summarize here. It is astrophysics. It is

0:21:40.640 --> 0:21:43.280
<v Speaker 1>it is astrophysics, and we are talking about black holes.

0:21:43.680 --> 0:21:45.320
<v Speaker 1>So one of the more interesting points brought up in

0:21:45.359 --> 0:21:48.840
<v Speaker 1>the talk was that string theory actually helps us make

0:21:48.960 --> 0:21:53.040
<v Speaker 1>sense of what's known as the intropy problem with black holes.

0:21:53.480 --> 0:21:56.359
<v Speaker 1>The basic problem being is that is that how can

0:21:56.400 --> 0:21:59.639
<v Speaker 1>a black hole be in a high entropy state if

0:21:59.680 --> 0:22:03.320
<v Speaker 1>everything inside it is super condensed to a state of

0:22:03.520 --> 0:22:08.000
<v Speaker 1>less entropy than normal matter, whereas the missing entropy and

0:22:08.280 --> 0:22:11.280
<v Speaker 1>the thing is. According to string theory, you can say, well,

0:22:11.320 --> 0:22:13.479
<v Speaker 1>the missing the missing intropy can be found in the

0:22:13.560 --> 0:22:17.439
<v Speaker 1>six microscopic spatial dimensions that exist in addition to the

0:22:17.440 --> 0:22:20.359
<v Speaker 1>three spatial dimensions that we can observe. And yes, I

0:22:20.400 --> 0:22:22.520
<v Speaker 1>realize all that kind of may have sounded to some

0:22:22.600 --> 0:22:27.000
<v Speaker 1>of you, like, uh, like a monologue from Ghostbusters. But

0:22:27.000 --> 0:22:29.520
<v Speaker 1>but but it does it does make sense. Okay, So

0:22:29.840 --> 0:22:34.640
<v Speaker 1>basics on string theory. String theory is an unproven hypothetical

0:22:34.680 --> 0:22:38.159
<v Speaker 1>framework in physics that explain that goes toward explaining the

0:22:38.200 --> 0:22:41.280
<v Speaker 1>more ultimate nature of our universe. We've got the Standard model,

0:22:41.680 --> 0:22:44.479
<v Speaker 1>and you've got particles, and you've got energy and all that,

0:22:44.520 --> 0:22:47.760
<v Speaker 1>and you're like, does something lie underneath all this? What

0:22:47.960 --> 0:22:51.879
<v Speaker 1>generates its string theory? That the very basic version is

0:22:51.920 --> 0:22:54.560
<v Speaker 1>that it posits that underneath all of our model of

0:22:54.560 --> 0:22:58.840
<v Speaker 1>particle physics and everything are these vibrating strings. And these

0:22:58.880 --> 0:23:01.639
<v Speaker 1>strings make up space, time and particles, and they can

0:23:01.760 --> 0:23:05.760
<v Speaker 1>vibrate in different ways that create different kinds of phenomena

0:23:05.800 --> 0:23:08.360
<v Speaker 1>and objects in our universe. Is that is that kind

0:23:08.359 --> 0:23:12.000
<v Speaker 1>of close approximation. Uh, And so under string theory, it's

0:23:12.040 --> 0:23:14.600
<v Speaker 1>this sort of mathematical framework we haven't been able to

0:23:14.640 --> 0:23:18.960
<v Speaker 1>fully test yet, but under this mathematical framework, it is

0:23:19.000 --> 0:23:22.320
<v Speaker 1>believed that there are more dimensions than just the three

0:23:22.359 --> 0:23:25.640
<v Speaker 1>space dimensions and the one time dimension that we observe, right,

0:23:25.680 --> 0:23:29.240
<v Speaker 1>and they're necessary for string theory to work. Um like this,

0:23:29.359 --> 0:23:31.359
<v Speaker 1>this basically emerges from the math. And one of the

0:23:31.400 --> 0:23:34.080
<v Speaker 1>things that that that Brian Green pointed out in the

0:23:34.080 --> 0:23:36.760
<v Speaker 1>World Science Festival talk is that for for a long

0:23:36.800 --> 0:23:38.760
<v Speaker 1>time this was kind of not really a dirty secret

0:23:38.760 --> 0:23:40.600
<v Speaker 1>of string theory, but it was one of those things

0:23:40.600 --> 0:23:42.760
<v Speaker 1>that was necessary by the math. But it wasn't something

0:23:42.760 --> 0:23:45.760
<v Speaker 1>that necessarily they were putting out there first like saying, uh,

0:23:45.840 --> 0:23:50.280
<v Speaker 1>you know, headline six dimensions, additional spatial dimensions. It was

0:23:50.320 --> 0:23:53.240
<v Speaker 1>more like, we have this this this attempt to understand

0:23:53.280 --> 0:23:56.840
<v Speaker 1>the universe and oh, by the way, six dimensional spatial dimensions.

0:23:56.920 --> 0:23:58.880
<v Speaker 1>And we should mention that Brian Green is a big

0:23:58.920 --> 0:24:01.720
<v Speaker 1>fan of string theory, been working on string three for years,

0:24:01.760 --> 0:24:05.359
<v Speaker 1>but not everybody in the physics community is uh. String

0:24:05.400 --> 0:24:07.520
<v Speaker 1>theory has plenty of critics, people who say, you know,

0:24:07.600 --> 0:24:10.119
<v Speaker 1>this is an even science. It's not testable yet, so

0:24:10.160 --> 0:24:12.920
<v Speaker 1>how could you you know? But the people who work

0:24:12.920 --> 0:24:15.119
<v Speaker 1>on it say, well, we're trying to create a theoretical

0:24:15.119 --> 0:24:17.479
<v Speaker 1>framework and maybe sometime in the future we could do

0:24:17.560 --> 0:24:20.320
<v Speaker 1>tests to try to confirm it or disconfirm it. Yes.

0:24:20.760 --> 0:24:22.439
<v Speaker 1>Now the other side of this, of course, is the

0:24:22.560 --> 0:24:26.920
<v Speaker 1>entropy we're talking about. So the second law of thermot

0:24:26.960 --> 0:24:31.080
<v Speaker 1>thermodynamic states that in a natural thermodynamic process, the sum

0:24:31.240 --> 0:24:36.320
<v Speaker 1>of the entropies of the interacting thermodynamic dynamic systems increases,

0:24:36.680 --> 0:24:39.720
<v Speaker 1>So things are going from low intropy to higher entropy. Um.

0:24:40.080 --> 0:24:41.959
<v Speaker 1>The example that Brian Green throws out is that if

0:24:41.960 --> 0:24:43.560
<v Speaker 1>you have a book's worth of page is stacked on

0:24:43.600 --> 0:24:47.280
<v Speaker 1>top of each other in order, uh, that is low entropy,

0:24:47.400 --> 0:24:48.879
<v Speaker 1>and then you throw it into the air and all

0:24:48.880 --> 0:24:50.719
<v Speaker 1>the pages fall on the ground. Well, now it's gone

0:24:50.760 --> 0:24:53.280
<v Speaker 1>to a high entroview state. In the former the low

0:24:53.359 --> 0:24:56.600
<v Speaker 1>entropy state, less information was required to describe it. But

0:24:56.680 --> 0:24:59.480
<v Speaker 1>in the because you just say, oh, well the information

0:24:59.520 --> 0:25:02.160
<v Speaker 1>on page X is on the sixth page, etcetera, you'll

0:25:02.200 --> 0:25:05.320
<v Speaker 1>find them in order in this stack. But now everything

0:25:05.760 --> 0:25:08.359
<v Speaker 1>is in a high entropy state. You need more information

0:25:08.400 --> 0:25:11.439
<v Speaker 1>to tell you where where everything is. You say, okay,

0:25:11.480 --> 0:25:15.800
<v Speaker 1>page six is, well, it's it's over here, um in

0:25:15.800 --> 0:25:19.080
<v Speaker 1>the middle of the field near pages you know, eight

0:25:19.119 --> 0:25:22.679
<v Speaker 1>hundred and page seventy two, that sort of thing with

0:25:22.720 --> 0:25:26.560
<v Speaker 1>a weasel chewin on it. Right, So when we looked

0:25:26.600 --> 0:25:29.320
<v Speaker 1>back to black holes, yeah, you have to account the

0:25:29.320 --> 0:25:31.120
<v Speaker 1>wee but in the weasels moving around, you gotta track

0:25:31.160 --> 0:25:33.560
<v Speaker 1>the weasel. See, it's so much easier to keep track

0:25:33.560 --> 0:25:35.960
<v Speaker 1>of everything when it's just in a stack. This is

0:25:36.000 --> 0:25:41.800
<v Speaker 1>why good housekeeping is essential. So back to black holes. Though,

0:25:41.840 --> 0:25:46.119
<v Speaker 1>when black holes merge, the area of the event horizon

0:25:46.480 --> 0:25:51.000
<v Speaker 1>holds onto the entropy. But there's this lost information. Uh,

0:25:51.160 --> 0:25:53.119
<v Speaker 1>and this is probably it's probably a terrible way of

0:25:53.119 --> 0:25:55.760
<v Speaker 1>thinking about it. So please, you know, don't like really

0:25:55.840 --> 0:25:57.840
<v Speaker 1>hold onto this or make a T shirt out of it.

0:25:57.920 --> 0:26:01.439
<v Speaker 1>But if two circus clowns were to into a single clown,

0:26:02.080 --> 0:26:04.800
<v Speaker 1>you might expect to have a circus clown with twice

0:26:04.840 --> 0:26:08.119
<v Speaker 1>as many articles of clown clothing, twice as many buzzers,

0:26:08.560 --> 0:26:11.959
<v Speaker 1>twice as many flowers and other like clown gimmicks. Right, uh,

0:26:12.119 --> 0:26:15.080
<v Speaker 1>twice as much face paint. But no, there's something missing.

0:26:15.160 --> 0:26:17.439
<v Speaker 1>Where did the missing clown gimmicks go? Where did the

0:26:17.440 --> 0:26:21.439
<v Speaker 1>missing entropy go? Where the missing information go? Or it

0:26:21.520 --> 0:26:24.520
<v Speaker 1>seems to be missing? Uh, seems to be there, seems

0:26:24.560 --> 0:26:27.600
<v Speaker 1>to be a loss of information. Uh. Intropy is supposed

0:26:27.600 --> 0:26:29.720
<v Speaker 1>to increase, but this would seem to be a decrease

0:26:29.760 --> 0:26:33.520
<v Speaker 1>in entropy, which violates that second loft thermo dynamics. And

0:26:33.520 --> 0:26:37.639
<v Speaker 1>then scientists also found an area increase in merging black holes,

0:26:37.880 --> 0:26:40.600
<v Speaker 1>seeming to line up with the increase in entropy. UH.

0:26:40.680 --> 0:26:43.919
<v Speaker 1>The area of the event horizon is somehow holding onto

0:26:43.960 --> 0:26:47.240
<v Speaker 1>the information that's inside the black hole, and Stephen Hawking

0:26:47.320 --> 0:26:51.080
<v Speaker 1>argued that there was a connection between the black hole

0:26:51.119 --> 0:26:54.679
<v Speaker 1>area in intropy. There must be information, but the horizon

0:26:54.880 --> 0:26:58.840
<v Speaker 1>is is featureless. There's no room for information there to

0:26:58.880 --> 0:27:01.760
<v Speaker 1>be deciphered. So if you solve all of this with

0:27:01.760 --> 0:27:05.600
<v Speaker 1>Einstein's equations, the black hole would seem to have zero entropy.

0:27:05.720 --> 0:27:07.720
<v Speaker 1>It would seem to be a perfectly ordered state. But

0:27:07.840 --> 0:27:11.680
<v Speaker 1>that can't be right now. Basically, as Brian Green described

0:27:11.680 --> 0:27:14.359
<v Speaker 1>at the World Science Festival, you have these extra dimensions

0:27:14.359 --> 0:27:16.760
<v Speaker 1>and string theory that emerges kind of a remainder, a

0:27:16.840 --> 0:27:20.399
<v Speaker 1>kind of a problem, and with black holes you have

0:27:20.560 --> 0:27:23.879
<v Speaker 1>this problem of missing introview, and when you combine the two,

0:27:24.359 --> 0:27:27.000
<v Speaker 1>the problems would seem to kind of cancel each other out.

0:27:27.600 --> 0:27:31.320
<v Speaker 1>Uh and in a way but possibly reveal what could

0:27:31.359 --> 0:27:33.960
<v Speaker 1>be going on inside a black hole. It's still a puzzle.

0:27:34.000 --> 0:27:35.919
<v Speaker 1>It's still a big mystery. You know, where does the

0:27:35.920 --> 0:27:39.159
<v Speaker 1>intropy go when the black hole evaporates and uh, it

0:27:39.720 --> 0:27:44.240
<v Speaker 1>radiates particles and this hawking radiation when it vanishes, what

0:27:44.280 --> 0:27:47.359
<v Speaker 1>happens to the information? Uh? All and all of this

0:27:47.440 --> 0:27:50.280
<v Speaker 1>is based on the math, by the way. Um, but

0:27:50.440 --> 0:27:53.520
<v Speaker 1>it's yeah, it's it's it's fascinating. This is another one

0:27:53.520 --> 0:27:56.440
<v Speaker 1>of those areas where where we were chasing the math

0:27:56.760 --> 0:28:00.119
<v Speaker 1>to find the black hole, and we're still chasing the

0:28:00.160 --> 0:28:04.520
<v Speaker 1>math to understand exactly how it's functioning. Yeah, this is

0:28:04.560 --> 0:28:07.480
<v Speaker 1>one of the frontiers of science. I mean, it's an

0:28:07.480 --> 0:28:11.280
<v Speaker 1>exciting realm because it's a place where you've got to

0:28:11.320 --> 0:28:16.480
<v Speaker 1>have this, uh, this sort of clever cooperation between indirect

0:28:16.600 --> 0:28:21.440
<v Speaker 1>kinds of observations from the experimentalists and clever innovations by

0:28:21.600 --> 0:28:25.440
<v Speaker 1>the theorists, the people coming up with the mathematical framework

0:28:25.440 --> 0:28:27.800
<v Speaker 1>in the theory. I mean, you can't like sample a

0:28:27.840 --> 0:28:31.160
<v Speaker 1>black hole and just say, Okay, let's see what's going on. Right,

0:28:31.920 --> 0:28:34.600
<v Speaker 1>So I realized a lot of that is is very

0:28:34.600 --> 0:28:38.320
<v Speaker 1>difficult to relate to the human experience. So I think

0:28:38.320 --> 0:28:41.120
<v Speaker 1>it's time to move on and talk about black holes

0:28:41.240 --> 0:28:44.080
<v Speaker 1>and time. We've talked about like the sort of the

0:28:44.240 --> 0:28:48.240
<v Speaker 1>visual experience and the the spatial experience of approaching and

0:28:48.240 --> 0:28:50.520
<v Speaker 1>then injuring a black hole crossing its event arise, and

0:28:51.080 --> 0:28:53.280
<v Speaker 1>but then there's this whole question about what happens with

0:28:53.360 --> 0:28:56.720
<v Speaker 1>time because we're talking about space time. We're talking about

0:28:56.720 --> 0:29:00.600
<v Speaker 1>an object that warps space time with its incredible math. Yeah. Now,

0:29:00.640 --> 0:29:03.200
<v Speaker 1>one thing that's absolutely true that we know is that

0:29:03.280 --> 0:29:08.760
<v Speaker 1>time is relative. So the outside observers version of what

0:29:08.840 --> 0:29:11.200
<v Speaker 1>happens to you when you enter a black hole might

0:29:11.240 --> 0:29:14.640
<v Speaker 1>be very different than your subjective experience of what happens

0:29:14.680 --> 0:29:16.760
<v Speaker 1>to you when you enter a black hole, because you're

0:29:16.760 --> 0:29:19.560
<v Speaker 1>not experiencing time in the same way. Yeah. Like, one

0:29:19.560 --> 0:29:21.360
<v Speaker 1>of the key things that will touch on again here

0:29:21.480 --> 0:29:24.040
<v Speaker 1>is you talk about these scenarios where one person enters

0:29:24.080 --> 0:29:26.760
<v Speaker 1>the black hole and one person watches from behind the

0:29:26.800 --> 0:29:28.240
<v Speaker 1>one in the front looks back at the one in

0:29:28.280 --> 0:29:31.000
<v Speaker 1>the back. But then you cannot have a third observer

0:29:31.600 --> 0:29:34.440
<v Speaker 1>who can see both inside a black hole and outside

0:29:34.440 --> 0:29:37.280
<v Speaker 1>of the black hole like that. There that once you

0:29:37.360 --> 0:29:39.960
<v Speaker 1>cross the event arise and that's it. Yeah, okay, well

0:29:39.960 --> 0:29:41.480
<v Speaker 1>I think we've got to take a quick break and

0:29:41.520 --> 0:29:43.920
<v Speaker 1>then after that we will come back and explore black

0:29:43.920 --> 0:29:49.520
<v Speaker 1>holes in time than all right, we're back, so key

0:29:49.560 --> 0:29:52.920
<v Speaker 1>and all of this is a phenomenon called time dilation,

0:29:53.160 --> 0:29:55.720
<v Speaker 1>which we've discussed in the show before. This is the

0:29:55.760 --> 0:29:58.520
<v Speaker 1>idea that time passes more slowly the closer you approach

0:29:58.600 --> 0:30:01.360
<v Speaker 1>the speed of light, which of course is an unbreakable

0:30:01.360 --> 0:30:04.520
<v Speaker 1>cosmic speed limit. Now, one thing we need to say there, though,

0:30:04.600 --> 0:30:07.520
<v Speaker 1>is that the What what that means when you say is,

0:30:07.600 --> 0:30:09.280
<v Speaker 1>let's say you get in a spaceship and you approach

0:30:09.360 --> 0:30:12.480
<v Speaker 1>the speed of light, is that time passes more slowly

0:30:12.520 --> 0:30:16.800
<v Speaker 1>relative to other observers for you, Uh, it doesn't necessarily

0:30:16.840 --> 0:30:20.160
<v Speaker 1>mean that you would feel like you're living in slow motion.

0:30:20.240 --> 0:30:22.960
<v Speaker 1>In fact, what it means is that you are living

0:30:23.200 --> 0:30:26.240
<v Speaker 1>in normal time. But say if you get in a spaceship,

0:30:26.280 --> 0:30:27.960
<v Speaker 1>travel at the speed of light or not at the

0:30:27.960 --> 0:30:30.040
<v Speaker 1>speed of light, close to the speed of light, and

0:30:30.120 --> 0:30:32.760
<v Speaker 1>come back even though it felt like time was passing

0:30:32.800 --> 0:30:35.440
<v Speaker 1>normally for you. You might get back to Earth and

0:30:35.480 --> 0:30:38.200
<v Speaker 1>then realize a lot of time has passed on Earth,

0:30:38.240 --> 0:30:41.800
<v Speaker 1>where it seemed like much less time had passed for you. Right,

0:30:41.880 --> 0:30:43.480
<v Speaker 1>And this is one of those things you could say

0:30:43.640 --> 0:30:46.280
<v Speaker 1>is true on Earth as it is in heaven, because

0:30:46.320 --> 0:30:49.120
<v Speaker 1>the the hands of a clock in a speeding train

0:30:49.520 --> 0:30:52.480
<v Speaker 1>are going to move ever so slightly slower than those

0:30:52.480 --> 0:30:56.600
<v Speaker 1>in a stationary On a stationary clock, the difference would

0:30:56.760 --> 0:30:59.280
<v Speaker 1>not be humanly noticeable, but when the train pulled back

0:30:59.280 --> 0:31:01.200
<v Speaker 1>around to the station and the two clocks would be

0:31:01.240 --> 0:31:05.040
<v Speaker 1>off by billions of a second um. If such a

0:31:05.120 --> 0:31:10.200
<v Speaker 1>train could attain nine point nine nine nine percent light speed,

0:31:10.600 --> 0:31:13.240
<v Speaker 1>only one year would pass on board for every two

0:31:13.320 --> 0:31:16.000
<v Speaker 1>hundred and twenty three years back at the train station,

0:31:16.240 --> 0:31:18.960
<v Speaker 1>even though for the passengers it would feel like time

0:31:19.040 --> 0:31:20.960
<v Speaker 1>was moving normally. Right, This would all be a matter

0:31:21.000 --> 0:31:23.560
<v Speaker 1>of like comparing notes and uh and like looking at

0:31:23.640 --> 0:31:27.160
<v Speaker 1>stop watches when you return. That's the thing. But speed

0:31:27.240 --> 0:31:29.880
<v Speaker 1>isn't the only factor that affects time. On a much

0:31:29.920 --> 0:31:34.960
<v Speaker 1>smaller scale, mass also influences time, so time slows down

0:31:35.000 --> 0:31:37.840
<v Speaker 1>the closer you are to the center of a massive object.

0:31:37.960 --> 0:31:40.040
<v Speaker 1>This is something that was explored to great effect in

0:31:40.040 --> 0:31:42.680
<v Speaker 1>the movie Interstellar, which we mentioned earlier. You get really

0:31:42.720 --> 0:31:45.760
<v Speaker 1>close to the supermassive black hole and and you're gonna

0:31:45.800 --> 0:31:49.240
<v Speaker 1>have some real problems sinking up with your person way

0:31:49.280 --> 0:31:52.600
<v Speaker 1>back in the space station. Yeah, indeed. Uh. And and

0:31:52.640 --> 0:31:54.160
<v Speaker 1>you know, based on this, we know that there are

0:31:54.200 --> 0:31:56.560
<v Speaker 1>places in the universe where time speeds up in places

0:31:56.600 --> 0:32:00.840
<v Speaker 1>where it slows down. Uh. Time, as it's often pointed out,

0:32:00.960 --> 0:32:03.080
<v Speaker 1>runs a little bit faster in space than it does

0:32:03.160 --> 0:32:06.719
<v Speaker 1>down on Earth. A clock aboard and orbiting satellite experiences

0:32:06.800 --> 0:32:09.640
<v Speaker 1>time dilation due to both the speed of its orbit

0:32:09.840 --> 0:32:13.000
<v Speaker 1>and it's greater distance from the center of Earth's gravity.

0:32:13.080 --> 0:32:15.560
<v Speaker 1>And we actually do have to make adjustments for this,

0:32:15.760 --> 0:32:19.920
<v Speaker 1>like for GPS satellites, Uh, they need occasional we we

0:32:19.960 --> 0:32:24.440
<v Speaker 1>need to occasionally adjust timekeeping between GPS satellites and what's

0:32:24.440 --> 0:32:28.960
<v Speaker 1>going on on Earth. So so that's the real world

0:32:29.560 --> 0:32:32.720
<v Speaker 1>version of this, like the accessible version of this that

0:32:32.800 --> 0:32:35.840
<v Speaker 1>actually impacts life on Earth. But then there's the Then

0:32:35.920 --> 0:32:38.280
<v Speaker 1>then we return to black holes though, because the closer

0:32:39.040 --> 0:32:42.280
<v Speaker 1>one gets to a black hole, the stronger the gravity

0:32:42.280 --> 0:32:44.800
<v Speaker 1>would be. And this is gonna have a dramatic effect

0:32:44.800 --> 0:32:49.040
<v Speaker 1>on time making a supermassive black hole, in Hawkings words,

0:32:49.760 --> 0:32:53.080
<v Speaker 1>a sort of natural time machine. The trick would be

0:32:53.120 --> 0:32:56.040
<v Speaker 1>to avoid falling in, hitting just the right trajectory and

0:32:56.080 --> 0:32:59.240
<v Speaker 1>your your spaceship or even your time ship. I guess

0:32:59.240 --> 0:33:01.480
<v Speaker 1>it would be at this point it to orbit around

0:33:01.560 --> 0:33:06.280
<v Speaker 1>the event horizon. High speed would keep you stable, but

0:33:06.480 --> 0:33:09.360
<v Speaker 1>time would slow down by half. So you could take

0:33:09.440 --> 0:33:13.600
<v Speaker 1>say a five year journey to travel ten years into

0:33:13.640 --> 0:33:16.000
<v Speaker 1>the future. That might not seem like a lot, but

0:33:16.040 --> 0:33:19.000
<v Speaker 1>it's ultimately the best the universe offers as far as

0:33:19.240 --> 0:33:23.080
<v Speaker 1>time travel goes without getting into the paradox producing feedback

0:33:23.160 --> 0:33:26.680
<v Speaker 1>loop destroying aspects of wormholes. Right now, this would only

0:33:26.720 --> 0:33:30.040
<v Speaker 1>be travel into the future. I think, as we've discussed before,

0:33:30.880 --> 0:33:34.960
<v Speaker 1>when people ask is time travel possible the questions the

0:33:35.000 --> 0:33:37.760
<v Speaker 1>answer to the question seems to me travel into the

0:33:37.760 --> 0:33:41.520
<v Speaker 1>past absolutely not. Travel into the future is not only possible,

0:33:41.560 --> 0:33:44.400
<v Speaker 1>it is known to be real. Yeah, And it gets

0:33:44.440 --> 0:33:46.800
<v Speaker 1>in this weird scenario where someone could say, Hey, you

0:33:46.800 --> 0:33:49.480
<v Speaker 1>wanna you wanna get to let's say it's eighteen now,

0:33:49.640 --> 0:33:52.960
<v Speaker 1>you want to get to the year Yes, all right, Well,

0:33:53.200 --> 0:33:55.480
<v Speaker 1>how how many years do you want to take to

0:33:55.520 --> 0:33:57.360
<v Speaker 1>get there? You want to take the standard ten. Do

0:33:57.360 --> 0:33:59.720
<v Speaker 1>you want to take five? Well, if you want it

0:33:59.760 --> 0:34:02.520
<v Speaker 1>to want to get there in five years, uh, you know,

0:34:03.000 --> 0:34:07.880
<v Speaker 1>uh relativistically, then you're gonna have to jump on this spaceship.

0:34:07.960 --> 0:34:10.040
<v Speaker 1>And all of our physics tells us this would work.

0:34:10.640 --> 0:34:15.720
<v Speaker 1>But that's outside the event horizon. What what's time like? Uh?

0:34:15.760 --> 0:34:18.760
<v Speaker 1>Within the event horizon? Yeah? Does it even make sense

0:34:18.840 --> 0:34:23.440
<v Speaker 1>to say from an outside observer's perspective that anything happens

0:34:23.480 --> 0:34:27.000
<v Speaker 1>inside a black hole? Is that even a meaningful concept?

0:34:27.400 --> 0:34:30.360
<v Speaker 1>I mean, we're it certainly gets into an area where

0:34:30.400 --> 0:34:33.359
<v Speaker 1>these are all decent questions, you know, because you sort

0:34:33.360 --> 0:34:35.400
<v Speaker 1>of you can do this with a sort of physics breakdown.

0:34:35.440 --> 0:34:38.200
<v Speaker 1>But then ultimately, yeah, what does it mean to be

0:34:38.239 --> 0:34:40.719
<v Speaker 1>within the event horizon? Yeah? By the way, I meant

0:34:40.760 --> 0:34:42.719
<v Speaker 1>that not to say that nothing happens. It was just

0:34:42.880 --> 0:34:44.879
<v Speaker 1>I don't actually know the answer to that question. Well,

0:34:44.880 --> 0:34:48.000
<v Speaker 1>I looked into this, and I was reading an article

0:34:48.120 --> 0:34:53.000
<v Speaker 1>on Ask an Astronomer by Harvard physics graduate students Sarah

0:34:53.040 --> 0:34:57.000
<v Speaker 1>Slater and uh and and she had this fascinating nugget.

0:34:57.080 --> 0:35:00.080
<v Speaker 1>She's she's shared that quote. Everyone inside the event to

0:35:00.160 --> 0:35:03.640
<v Speaker 1>horizon is a psychic whoa explain that okay. So she

0:35:03.760 --> 0:35:07.680
<v Speaker 1>points out that outside of the event horizon, there are

0:35:07.719 --> 0:35:12.080
<v Speaker 1>two criteria for remembering something. One it has to have

0:35:12.120 --> 0:35:15.200
<v Speaker 1>been in the past, and two, it has to have

0:35:15.320 --> 0:35:18.759
<v Speaker 1>happened at a distance no more than what light could

0:35:18.760 --> 0:35:22.160
<v Speaker 1>have traveled since it happened. Okay. So that sort of

0:35:22.200 --> 0:35:26.960
<v Speaker 1>means like, we can't remember events that took place farther

0:35:27.040 --> 0:35:30.920
<v Speaker 1>away than the observable universe because it would have taken

0:35:31.080 --> 0:35:33.920
<v Speaker 1>light longer than the history of the universe to cross

0:35:34.000 --> 0:35:36.520
<v Speaker 1>that distance to reach us. There's no way we could

0:35:36.520 --> 0:35:39.480
<v Speaker 1>have that information, right, I mean, this is like basically

0:35:39.719 --> 0:35:41.359
<v Speaker 1>I'm gonna put that on the shelf and say that's

0:35:41.360 --> 0:35:45.120
<v Speaker 1>space and time as it relates to our our ability

0:35:45.120 --> 0:35:49.399
<v Speaker 1>to remember something. But inside the event horizon, things get

0:35:49.400 --> 0:35:53.280
<v Speaker 1>flipped around space and time you could say, become switched.

0:35:53.640 --> 0:35:55.200
<v Speaker 1>So now these are the two These are the two

0:35:55.200 --> 0:35:59.200
<v Speaker 1>criteria within the event horizon for remembering something. One it

0:35:59.320 --> 0:36:01.960
<v Speaker 1>has to have happened farther from the center of the

0:36:02.000 --> 0:36:06.319
<v Speaker 1>black hole, uh than where you are right now. And

0:36:06.560 --> 0:36:10.080
<v Speaker 1>number two, if T is in the letter T is

0:36:10.120 --> 0:36:12.680
<v Speaker 1>the time that it would take light to travel to

0:36:12.760 --> 0:36:16.000
<v Speaker 1>you from the location of the event, then it happened

0:36:16.000 --> 0:36:20.080
<v Speaker 1>either no more than tea hours ago or tea hours

0:36:20.160 --> 0:36:23.720
<v Speaker 1>into the future. So I'm gonna just read this direct

0:36:23.840 --> 0:36:27.760
<v Speaker 1>quote from her quote if you look away from the center.

0:36:27.840 --> 0:36:30.920
<v Speaker 1>And again this goes back to our earlier ideas of

0:36:31.080 --> 0:36:34.120
<v Speaker 1>crossing the event horizon and looking back or trying to

0:36:34.160 --> 0:36:36.640
<v Speaker 1>look back. She says, quote, if you look away from

0:36:36.640 --> 0:36:39.840
<v Speaker 1>the center, though, you can see two images of everything,

0:36:40.480 --> 0:36:43.080
<v Speaker 1>one from tea hours in the past and one from

0:36:43.160 --> 0:36:46.439
<v Speaker 1>tea hours in the future. For nearby objects, these two

0:36:46.440 --> 0:36:49.560
<v Speaker 1>images will look just the same, since t will be

0:36:49.680 --> 0:36:52.560
<v Speaker 1>very small due the due to the large speed of light.

0:36:53.040 --> 0:36:56.320
<v Speaker 1>For far away objects, though, they could be completely different.

0:36:56.560 --> 0:36:59.520
<v Speaker 1>So you could see the past beginning of something and

0:36:59.600 --> 0:37:03.520
<v Speaker 1>it's few your end. At the same time, spacetime is twisted.

0:37:04.360 --> 0:37:05.759
<v Speaker 1>And then there's this. If you were to enter a

0:37:05.800 --> 0:37:09.840
<v Speaker 1>black hole, theoretically speaking, an outside observer might watch you

0:37:09.920 --> 0:37:12.279
<v Speaker 1>crash and burn on the event arise and destroyed by

0:37:12.280 --> 0:37:15.480
<v Speaker 1>all that hawking radiation, all of your information spread out

0:37:15.480 --> 0:37:19.560
<v Speaker 1>across the face of the dark sphere. Uh because again

0:37:19.560 --> 0:37:22.520
<v Speaker 1>the information can't be lost, but your experience would be

0:37:22.560 --> 0:37:25.320
<v Speaker 1>one of free fall for the rest of your life.

0:37:25.920 --> 0:37:28.960
<v Speaker 1>And in short, this is the firewall paradox. Uh, there's

0:37:29.000 --> 0:37:32.120
<v Speaker 1>no third witness who can see both within and without

0:37:32.320 --> 0:37:35.560
<v Speaker 1>the event Arizona. And to me, that's all just mind

0:37:35.600 --> 0:37:38.839
<v Speaker 1>going to try and and uh and and contemplate. Yeah,

0:37:38.840 --> 0:37:41.520
<v Speaker 1>I feel like I'm still trying to understand it. Um.

0:37:41.560 --> 0:37:44.520
<v Speaker 1>I mean it drives home the way that black holes

0:37:44.560 --> 0:37:50.040
<v Speaker 1>are kind of They're great because they are a reality

0:37:50.120 --> 0:37:53.880
<v Speaker 1>that brings to life all of these impossible relativity experiments

0:37:53.920 --> 0:37:57.520
<v Speaker 1>that people try to use to explain how weird spacetime

0:37:57.560 --> 0:37:59.719
<v Speaker 1>really is. One of the things we talked about in

0:37:59.719 --> 0:38:01.440
<v Speaker 1>the last episode is you know, if you were to

0:38:01.480 --> 0:38:04.000
<v Speaker 1>just go based on your intuitions, you'd probably think, well,

0:38:04.400 --> 0:38:08.200
<v Speaker 1>space and time are are fixed, and the speed of

0:38:08.320 --> 0:38:11.279
<v Speaker 1>light is can be moved all around. But in fact

0:38:11.320 --> 0:38:14.200
<v Speaker 1>it's exactly the opposite. Speed of light is fixed speed

0:38:14.200 --> 0:38:16.560
<v Speaker 1>of light and a vacuum is fixed and space and

0:38:16.600 --> 0:38:20.239
<v Speaker 1>time can be stretched all around. And you can't really

0:38:20.280 --> 0:38:22.560
<v Speaker 1>internalize that. But people try to come up with all

0:38:22.600 --> 0:38:27.680
<v Speaker 1>these impossible scenarios to illustrate the principle. At the black hole,

0:38:28.239 --> 0:38:30.000
<v Speaker 1>you don't have to come up with scenarios. This just

0:38:30.040 --> 0:38:32.959
<v Speaker 1>apparently is what black holes do. Now. At this point

0:38:32.960 --> 0:38:35.040
<v Speaker 1>in the podcast, is we're beginning to wind down here,

0:38:35.440 --> 0:38:37.520
<v Speaker 1>I thought it might be fun to just talk about

0:38:37.560 --> 0:38:41.160
<v Speaker 1>a couple of questions that that frequently come up. Either

0:38:41.680 --> 0:38:43.840
<v Speaker 1>some of these we have received as emails from people,

0:38:44.040 --> 0:38:45.799
<v Speaker 1>and then others are just sort of general questions that

0:38:45.840 --> 0:38:50.480
<v Speaker 1>arise from sci fi treatments of black holes, including event Horizon. Okay,

0:38:50.480 --> 0:38:52.640
<v Speaker 1>so the first one is if and I know we've

0:38:52.640 --> 0:38:55.560
<v Speaker 1>received this from listeners, if I'm pulled into a black hole,

0:38:55.680 --> 0:38:57.960
<v Speaker 1>will I then come back out of a white hole?

0:38:58.160 --> 0:39:00.080
<v Speaker 1>And I think sometimes this is an area where we

0:39:00.080 --> 0:39:02.080
<v Speaker 1>we fall into the trap of thinking of black holes

0:39:02.120 --> 0:39:06.120
<v Speaker 1>more as wormholes. But the white hole concept is in

0:39:06.200 --> 0:39:09.759
<v Speaker 1>fact a byproduct of general relativity. But it's even more

0:39:09.800 --> 0:39:13.400
<v Speaker 1>of a mathematical phantom. In many respects, it is the

0:39:13.440 --> 0:39:15.640
<v Speaker 1>reverse of a black hole. It's not a place where

0:39:15.719 --> 0:39:18.880
<v Speaker 1>matter is lost, but rather a place where matter is born.

0:39:19.360 --> 0:39:21.759
<v Speaker 1>I've seen it explained as sort of like the Big

0:39:21.800 --> 0:39:25.719
<v Speaker 1>Bang singularity but not but not quite the same. But

0:39:25.840 --> 0:39:29.880
<v Speaker 1>it also can't actually exist in our universe. Yeah, so

0:39:30.120 --> 0:39:32.000
<v Speaker 1>I hadn't heard this. I've heard the white holes were

0:39:32.040 --> 0:39:36.319
<v Speaker 1>still kind of a speculative possibility. Well, this is, well,

0:39:36.920 --> 0:39:39.560
<v Speaker 1>my understanding of it and again this could be that

0:39:39.719 --> 0:39:41.719
<v Speaker 1>this could be incorrect, and I may have to be

0:39:41.840 --> 0:39:47.200
<v Speaker 1>corrected on this later. But my understand my my understanding

0:39:47.200 --> 0:39:49.760
<v Speaker 1>of it that it is that it emerges from the math.

0:39:50.200 --> 0:39:51.680
<v Speaker 1>But it's one of these things that emerges from the

0:39:51.719 --> 0:39:53.720
<v Speaker 1>math that that we're like, well, that doesn't really square

0:39:53.800 --> 0:39:56.799
<v Speaker 1>up with what we we actually expect to see in

0:39:56.840 --> 0:40:02.040
<v Speaker 1>the universe. Astrophysicist Karen master Is once described it this way, quote,

0:40:02.120 --> 0:40:04.719
<v Speaker 1>there is only such a thing as a white hole

0:40:05.120 --> 0:40:07.879
<v Speaker 1>in the theory of black holes, and no such thing

0:40:08.200 --> 0:40:12.239
<v Speaker 1>is possible, is possible physically. Well, I'm sure she knows

0:40:12.239 --> 0:40:14.239
<v Speaker 1>a million times more about this than I do, but

0:40:14.280 --> 0:40:16.880
<v Speaker 1>I would just point out that that used to be

0:40:16.960 --> 0:40:21.040
<v Speaker 1>what the astronomers said about black holes. Yeah, but I'm

0:40:21.080 --> 0:40:23.040
<v Speaker 1>not using that to say white holes exist. I mean,

0:40:23.040 --> 0:40:25.280
<v Speaker 1>I'm sure she's probably drawing on a lot of facts

0:40:25.320 --> 0:40:28.040
<v Speaker 1>that that I'm not aware of my But basically, my

0:40:28.040 --> 0:40:31.080
<v Speaker 1>my read from this information is that the answer to

0:40:31.200 --> 0:40:32.839
<v Speaker 1>if if I go into a black hole, I come

0:40:32.840 --> 0:40:36.279
<v Speaker 1>out a white hole, the answer is is probably no.

0:40:36.920 --> 0:40:40.600
<v Speaker 1>And probably you're thinking more about a wormhole here, You're

0:40:40.600 --> 0:40:43.520
<v Speaker 1>not really you're not really picturing what a black hole

0:40:43.640 --> 0:40:47.279
<v Speaker 1>and indeed, a white hole would actually be well, I'm

0:40:47.440 --> 0:40:50.040
<v Speaker 1>more I'm inclined to take the astrophysicists word on it,

0:40:50.160 --> 0:40:53.160
<v Speaker 1>so so I'll go with that. No, no white holes. Okay.

0:40:53.280 --> 0:40:56.920
<v Speaker 1>So another frequently asked question, and this one's a lot

0:40:56.920 --> 0:40:59.279
<v Speaker 1>more fun I have to have to say, is could

0:40:59.280 --> 0:41:01.600
<v Speaker 1>we one day harness the power of a black hole?

0:41:02.120 --> 0:41:05.040
<v Speaker 1>Perhaps like what we see an event horizon, it's a

0:41:05.080 --> 0:41:08.160
<v Speaker 1>black hole. Drive tell me event horizon as possible. Kay,

0:41:08.360 --> 0:41:11.279
<v Speaker 1>let's hear it. Okay, So, first of all, this is

0:41:11.280 --> 0:41:13.640
<v Speaker 1>probably a good time to refresh everyone on the Kardashian scale,

0:41:13.719 --> 0:41:17.160
<v Speaker 1>which we referenced earlier. This is the idea that this

0:41:17.200 --> 0:41:19.520
<v Speaker 1>is just like a very rough way of understanding like

0:41:19.520 --> 0:41:25.239
<v Speaker 1>what would be the technological levels of possible um civilizations

0:41:25.360 --> 0:41:28.040
<v Speaker 1>in the universe. And it's judge based on how much

0:41:28.160 --> 0:41:31.120
<v Speaker 1>energy you can take control of, right and like truly

0:41:31.160 --> 0:41:34.200
<v Speaker 1>take control of. So, for instance, Type one civilizations are

0:41:34.239 --> 0:41:37.160
<v Speaker 1>masters of planetary energy, meaning they can harness this some

0:41:37.440 --> 0:41:40.719
<v Speaker 1>energy of an entire world. We're not there yet, no,

0:41:40.880 --> 0:41:43.759
<v Speaker 1>we would still be a type zero civilization. Type to

0:41:43.920 --> 0:41:47.560
<v Speaker 1>civilizations can summon the power of an entire star system,

0:41:47.600 --> 0:41:49.880
<v Speaker 1>and those would be I mean these would be godlike

0:41:50.000 --> 0:41:52.360
<v Speaker 1>entities if we were to encounter them, if I remember correctly,

0:41:52.440 --> 0:41:55.799
<v Speaker 1>like the the the aliens we encounter in two thousand

0:41:55.840 --> 0:41:59.319
<v Speaker 1>and one Space Odyssey are probably Type two. Yeah, so

0:41:59.360 --> 0:42:02.520
<v Speaker 1>they know you. Dyson's fears would be an example. So

0:42:02.560 --> 0:42:05.600
<v Speaker 1>if you you create a structure that can harness and

0:42:05.640 --> 0:42:08.720
<v Speaker 1>make usable all of the radiation coming off of a star,

0:42:10.160 --> 0:42:13.760
<v Speaker 1>and then Type three civilizations command energy on a galactic scale,

0:42:14.080 --> 0:42:17.160
<v Speaker 1>and that we can't even picture that that's god like

0:42:17.360 --> 0:42:19.480
<v Speaker 1>to a level that it's yeah, I think it's difficult

0:42:19.520 --> 0:42:23.279
<v Speaker 1>for us to even summon. Yeah, it's difficult for me

0:42:23.320 --> 0:42:26.000
<v Speaker 1>to even imagine that as well, it would do because

0:42:26.080 --> 0:42:30.120
<v Speaker 1>Type two civilizations would appear as God's Type three. We

0:42:30.600 --> 0:42:32.440
<v Speaker 1>I don't know, we don't even know they're there. If

0:42:32.440 --> 0:42:34.040
<v Speaker 1>we could, they could be all in the room with us.

0:42:34.080 --> 0:42:37.480
<v Speaker 1>And who are we? Who are we to to to

0:42:37.480 --> 0:42:41.080
<v Speaker 1>to even notice them? So anyway, harvesting the power of

0:42:41.120 --> 0:42:43.719
<v Speaker 1>a black hole sounds exactly like the type of thing

0:42:43.840 --> 0:42:48.240
<v Speaker 1>a Type to civilization would be into um and in fact,

0:42:48.320 --> 0:42:51.120
<v Speaker 1>even a Type zero civilization like our own can think

0:42:51.120 --> 0:42:53.960
<v Speaker 1>of a few ways one might go about it. So

0:42:54.120 --> 0:42:57.880
<v Speaker 1>remember that hawking radiation that we've mentioned already that's emitted

0:42:57.880 --> 0:43:01.000
<v Speaker 1>by a black hole. Well one to harvest that, yeah,

0:43:01.120 --> 0:43:06.120
<v Speaker 1>just turned into a nuclear reactor. Well in, physicist George

0:43:06.239 --> 0:43:10.320
<v Speaker 1>unrou and Robert Wald suggested that one could essentially lower

0:43:10.360 --> 0:43:14.160
<v Speaker 1>a bucket toward the event horizon, collect this radiation, and

0:43:14.200 --> 0:43:16.880
<v Speaker 1>then drawl it back out. Now, if you let the

0:43:17.040 --> 0:43:19.480
<v Speaker 1>bucket go through the event horizon, you would not be

0:43:19.480 --> 0:43:21.759
<v Speaker 1>able to get it back right, Yeah, there's no that

0:43:22.719 --> 0:43:25.920
<v Speaker 1>the light cannot escape, and certainly a type two Kardashian

0:43:26.040 --> 0:43:28.080
<v Speaker 1>bucket would not be able to escape. Right. That would

0:43:28.080 --> 0:43:30.640
<v Speaker 1>be like the black holes. Like the neighbor who you know,

0:43:30.680 --> 0:43:35.080
<v Speaker 1>your frisbee goes in their yard and that's my bucket. Now. Now,

0:43:35.480 --> 0:43:38.000
<v Speaker 1>there's some problems with this though, because the tension of

0:43:38.040 --> 0:43:41.000
<v Speaker 1>the rope here is an issue. Adam Brown of the

0:43:41.239 --> 0:43:46.120
<v Speaker 1>Princeton Center of for the Theoretical Science countered that the

0:43:46.239 --> 0:43:49.319
<v Speaker 1>rope descending towards such high gravity would only be able

0:43:49.360 --> 0:43:52.600
<v Speaker 1>to support its own mass, not the additional mass of

0:43:52.680 --> 0:43:56.160
<v Speaker 1>this mind hawking radiation. Plus, as you know, it also

0:43:56.200 --> 0:43:58.399
<v Speaker 1>needs to be able to withstand the crazy hey heat

0:43:58.480 --> 0:44:04.320
<v Speaker 1>of hawking radiation, as with the bucket. Now in albion

0:44:04.400 --> 0:44:08.080
<v Speaker 1>Lawrence and A. Mill Martinique of the University of Chicago

0:44:08.520 --> 0:44:12.640
<v Speaker 1>proposed that we could instead dip strings into the black

0:44:12.680 --> 0:44:17.200
<v Speaker 1>hole and hawking radiation would climb up out on its own.

0:44:17.680 --> 0:44:19.960
<v Speaker 1>So this would be like I've seen it compared to

0:44:20.239 --> 0:44:22.799
<v Speaker 1>U like the like an oil wick in a in

0:44:22.840 --> 0:44:26.839
<v Speaker 1>an oil lantern. So you're not getting anything back from

0:44:26.840 --> 0:44:30.920
<v Speaker 1>beyond the event horizon, but you're harvesting the hawking radiation

0:44:30.960 --> 0:44:33.879
<v Speaker 1>around it. Yeah, kind of almost like luring it out.

0:44:34.840 --> 0:44:36.640
<v Speaker 1>So you know, this is this is an interesting think

0:44:36.640 --> 0:44:38.600
<v Speaker 1>about and you would be able to to to mind

0:44:38.680 --> 0:44:41.520
<v Speaker 1>just a colossal amount of energy this way. But what

0:44:41.640 --> 0:44:45.200
<v Speaker 1>about doing more of this event horizon model Event Horizon

0:44:45.239 --> 0:44:48.800
<v Speaker 1>the movie? What about actually, you say, capturing a small

0:44:48.800 --> 0:44:52.319
<v Speaker 1>black hole, maybe a primordial black hole, using that to

0:44:52.320 --> 0:44:56.120
<v Speaker 1>power your space or making your own singularity. Well, on

0:44:56.120 --> 0:44:58.080
<v Speaker 1>one hand, that sounds kind of impossible, But on the

0:44:58.080 --> 0:45:00.680
<v Speaker 1>other hand, we should be clear that a black hole

0:45:00.920 --> 0:45:03.839
<v Speaker 1>doesn't have to come from a star in principle at least,

0:45:03.920 --> 0:45:06.839
<v Speaker 1>I mean, we we don't have any technology for like

0:45:07.120 --> 0:45:11.080
<v Speaker 1>making big old black holes. But in order to create

0:45:11.120 --> 0:45:12.839
<v Speaker 1>a black hole, all you have to do is get

0:45:12.920 --> 0:45:16.360
<v Speaker 1>an amount of mass within Swart shield radius. Right. And

0:45:16.400 --> 0:45:18.520
<v Speaker 1>if you can do that, you've made a black hole.

0:45:18.520 --> 0:45:21.480
<v Speaker 1>It doesn't have to be a collapse stellar remnant, right,

0:45:21.600 --> 0:45:24.880
<v Speaker 1>And then arguably you could make one out of energy

0:45:24.960 --> 0:45:28.359
<v Speaker 1>instead of just pure mass. So this is what's known

0:45:28.360 --> 0:45:32.759
<v Speaker 1>as a swart shield. Google blitz, Google blitz, google blitz. Yes,

0:45:32.840 --> 0:45:35.600
<v Speaker 1>sounds like a brand of blender or something, yeah, or

0:45:35.719 --> 0:45:38.800
<v Speaker 1>a delicious breakfast cereal or part of your your complete breakfast.

0:45:39.400 --> 0:45:44.200
<v Speaker 1>So this is the brainchild of theoretical physicist John Archibald

0:45:44.200 --> 0:45:48.760
<v Speaker 1>Wheeler Wheeler and uh, it's the google blitz is German

0:45:48.800 --> 0:45:51.399
<v Speaker 1>for ball lightning. Uh. And the idea is that these

0:45:51.400 --> 0:45:54.880
<v Speaker 1>are These would be concentrations of energy so intense that

0:45:54.960 --> 0:45:58.120
<v Speaker 1>they form their own event horizons and collapse on themselves.

0:45:58.719 --> 0:46:01.319
<v Speaker 1>And it would need for this to work to be

0:46:01.520 --> 0:46:05.160
<v Speaker 1>for this to be something you could actually utilize, it

0:46:05.160 --> 0:46:07.719
<v Speaker 1>would need to be smaller than a proton. It would

0:46:07.719 --> 0:46:10.399
<v Speaker 1>be incredibly hot, but if you could contain it, you'd

0:46:10.440 --> 0:46:13.480
<v Speaker 1>have just immense energy at your disposal. Now, I'm not

0:46:13.520 --> 0:46:16.040
<v Speaker 1>the biggest star Trek the next generation buff I like

0:46:16.120 --> 0:46:18.959
<v Speaker 1>watched all these episodes, I think every evening at nine

0:46:19.000 --> 0:46:22.600
<v Speaker 1>pm back in um in middle school, watched them on syndication,

0:46:22.640 --> 0:46:24.799
<v Speaker 1>But it's been a long time since I've viewed them.

0:46:24.920 --> 0:46:27.880
<v Speaker 1>You went down to the planets, to the pottered plants. Oh, yeah,

0:46:27.920 --> 0:46:29.920
<v Speaker 1>I I think I watched them them all back in

0:46:29.960 --> 0:46:31.920
<v Speaker 1>the day. But there was an episode that I do

0:46:31.960 --> 0:46:35.920
<v Speaker 1>not directly remember, titled Timescape, and it reveals that a

0:46:36.000 --> 0:46:39.560
<v Speaker 1>Romulan warbird is powered by one of these uh sword

0:46:39.640 --> 0:46:42.080
<v Speaker 1>shield google blitz uh and it didn't, but it ends

0:46:42.160 --> 0:46:45.160
<v Speaker 1>up resulting in all these temporal anomalies. Uh. And that's

0:46:45.239 --> 0:46:47.359
<v Speaker 1>you know, the plot of the show is like, what's

0:46:47.360 --> 0:46:50.480
<v Speaker 1>happening to time? Oh, it's something that Romulans did. Um.

0:46:50.520 --> 0:46:53.840
<v Speaker 1>I don't remember it myself, but I've seen it cited

0:46:54.000 --> 0:46:57.759
<v Speaker 1>as a as as an episode that utilizes this concept. Yeah,

0:46:57.760 --> 0:46:59.759
<v Speaker 1>if Wheeler wants to try it out, I'd say let's

0:46:59.800 --> 0:47:02.759
<v Speaker 1>go with Wheeler's I D idea. But I like thinking

0:47:02.800 --> 0:47:05.520
<v Speaker 1>of it. This. What if you create this uh this

0:47:05.520 --> 0:47:09.000
<v Speaker 1>this artificial black hole or this uh this this little

0:47:09.040 --> 0:47:11.640
<v Speaker 1>lightning ball and then you drop it on the floor.

0:47:12.160 --> 0:47:13.920
<v Speaker 1>That's got to be the worst. It's you know, it's

0:47:13.960 --> 0:47:17.360
<v Speaker 1>bad enough when you say, drop a hummingbird feeder onto

0:47:17.400 --> 0:47:19.600
<v Speaker 1>the kitchen floor and you get sugar water everywhere. What

0:47:19.640 --> 0:47:22.560
<v Speaker 1>happens when you drop a black hole that's hard to

0:47:22.560 --> 0:47:26.279
<v Speaker 1>clean up? Here's a hint. It's sticky, And I think

0:47:26.320 --> 0:47:30.120
<v Speaker 1>that sums up the whole episode right there. Well, you know,

0:47:30.200 --> 0:47:32.080
<v Speaker 1>I would say that there's all kinds of other black

0:47:32.080 --> 0:47:34.360
<v Speaker 1>hole stuff we didn't even get to. So maybe we

0:47:34.360 --> 0:47:36.320
<v Speaker 1>can come back again in the future. I just figured

0:47:36.320 --> 0:47:38.320
<v Speaker 1>three episodes in a row, that's a lot. We probably

0:47:38.320 --> 0:47:41.160
<v Speaker 1>shouldn't push it to four this week, I I think,

0:47:41.200 --> 0:47:42.759
<v Speaker 1>so we have to move on to other topics and

0:47:42.760 --> 0:47:45.560
<v Speaker 1>then we can return later because, as we've already touched

0:47:45.600 --> 0:47:49.560
<v Speaker 1>on the the exploration of black holes is ongoing. It

0:47:49.680 --> 0:47:52.319
<v Speaker 1>is far from a closed book. Yeah, we're learning. We're

0:47:52.440 --> 0:47:55.520
<v Speaker 1>learning new stuff about black holes this year, especially with say,

0:47:55.520 --> 0:47:58.440
<v Speaker 1>the research into Sagittarys, a star in the middle of

0:47:58.440 --> 0:48:01.440
<v Speaker 1>our galaxy going on just this year. Yeah. So hey,

0:48:01.520 --> 0:48:04.120
<v Speaker 1>maybe at the end of we can come back and

0:48:04.120 --> 0:48:07.080
<v Speaker 1>we just we can discuss what we know now about

0:48:07.800 --> 0:48:11.600
<v Speaker 1>about singularities that we did not know just a year earlier.

0:48:11.640 --> 0:48:13.959
<v Speaker 1>One of the most interesting things mentioned in that World

0:48:13.960 --> 0:48:17.000
<v Speaker 1>Science Festival event that we keep referring to is the

0:48:17.040 --> 0:48:19.879
<v Speaker 1>idea that observations of black holes that are just now

0:48:19.920 --> 0:48:23.600
<v Speaker 1>coming online, Like what we're finally learning about sagittarys a

0:48:23.719 --> 0:48:27.279
<v Speaker 1>star in fact, seems to be though this could this

0:48:27.320 --> 0:48:30.560
<v Speaker 1>could change, but at least seems in initial observations to

0:48:30.640 --> 0:48:34.520
<v Speaker 1>be challenging some of the findings of general relativity. Yeah,

0:48:34.920 --> 0:48:37.000
<v Speaker 1>so what do you what do you do with that?

0:48:37.040 --> 0:48:39.239
<v Speaker 1>What happens when you do an experiment you think it's

0:48:39.239 --> 0:48:42.839
<v Speaker 1>a well designed experiment, but then it disagrees with Einstein?

0:48:43.400 --> 0:48:46.120
<v Speaker 1>Well it's it's yeah, I mean, if they discussed in

0:48:46.160 --> 0:48:48.279
<v Speaker 1>that of that talk, it's like you you, first of all,

0:48:48.320 --> 0:48:51.200
<v Speaker 1>you might question, well, one of my results actually saying,

0:48:51.239 --> 0:48:53.520
<v Speaker 1>but then you may be reaching the point where you're

0:48:53.520 --> 0:48:57.799
<v Speaker 1>having to move beyond, uh, these theories and work with

0:48:57.880 --> 0:49:01.000
<v Speaker 1>new theories. So as we learn more about black holes,

0:49:01.040 --> 0:49:04.759
<v Speaker 1>we're not just learning more about this arguably kind of

0:49:04.800 --> 0:49:08.120
<v Speaker 1>abstract seeming thing that has no direct influence over our

0:49:08.160 --> 0:49:10.080
<v Speaker 1>lives here on Earth. But it changed. But they have

0:49:10.120 --> 0:49:12.960
<v Speaker 1>the ability to change our understanding of the cosmos itself.

0:49:13.000 --> 0:49:15.680
<v Speaker 1>I mean, wouldn't it be a fascinating thing if we

0:49:15.680 --> 0:49:19.800
<v Speaker 1>were alive to see a new better theory of gravity emerge?

0:49:20.520 --> 0:49:23.160
<v Speaker 1>It would? It would? It would it would change everything.

0:49:23.200 --> 0:49:25.239
<v Speaker 1>It's like it's like them. It's it's kind of like

0:49:25.280 --> 0:49:28.680
<v Speaker 1>when they made another Blade Runner movie, except except even

0:49:28.760 --> 0:49:31.839
<v Speaker 1>more ground shaking. You know, like you grow up thinking

0:49:31.840 --> 0:49:33.520
<v Speaker 1>you're only going to ever have that one, and then

0:49:33.560 --> 0:49:36.040
<v Speaker 1>they go and make another one, and then likewise you

0:49:36.280 --> 0:49:38.239
<v Speaker 1>we would be living in a in a world in

0:49:38.280 --> 0:49:42.719
<v Speaker 1>which we had our third gravitational theory, So third major one. Yeah,

0:49:42.840 --> 0:49:46.520
<v Speaker 1>that would be really cool. Yeah. So yeah, astrophysicists, please

0:49:46.560 --> 0:49:50.600
<v Speaker 1>go out there and break Einstein kick his butt. Alright, Well,

0:49:50.600 --> 0:49:53.920
<v Speaker 1>on that note, we're going to uh, we're going to

0:49:54.040 --> 0:49:56.319
<v Speaker 1>rock it away from the event horizon. Now, we are

0:49:56.400 --> 0:49:59.799
<v Speaker 1>going to close this episode out. As always, we urge

0:49:59.800 --> 0:50:01.520
<v Speaker 1>you to check out Stuff to Blow your Mind dot com.

0:50:01.520 --> 0:50:04.600
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0:50:04.920 --> 0:50:07.640
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0:50:07.719 --> 0:50:10.160
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0:50:10.160 --> 0:50:11.600
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0:50:11.600 --> 0:50:14.320
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0:50:14.360 --> 0:50:17.839
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0:50:18.000 --> 0:50:20.120
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0:50:20.120 --> 0:50:23.720
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0:50:23.760 --> 0:50:26.960
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0:50:26.960 --> 0:50:28.880
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0:50:28.960 --> 0:50:30.839
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0:50:30.880 --> 0:50:34.239
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0:50:34.280 --> 0:50:36.400
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0:50:38.640 --> 0:50:41.800
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0:50:41.840 --> 0:50:53.320
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0:50:53.480 --> 0:50:56.000
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0:50:56.000 --> 0:51:12.760
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