WEBVTT - Will our supercluster be torn apart?

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<v Speaker 1>Hey or hey, I have a physics version of would

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<v Speaker 1>you rather?

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<v Speaker 2>Well, oh, I'd rather not play?

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<v Speaker 1>Not an option today? So would you rather be blown

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<v Speaker 1>up in a supernova or crushed in a black hole?

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<v Speaker 2>Well, if I fell into a black hole, there would

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<v Speaker 2>be time dilation, so it sounds like it would take forever.

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<v Speaker 2>So maybe I'll go with a supernova, nice and quick.

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<v Speaker 1>All right? Next one, would you rather be eaten by

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<v Speaker 1>aliens or live your life never knowing if aliens exist?

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<v Speaker 2>I would pick live my life over and being eaten

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<v Speaker 2>by anything, aliens or otherwise.

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<v Speaker 1>Wrong answer, wrong answer. Next one, would you rather keep

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<v Speaker 1>playing this game or start the podcast?

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<v Speaker 2>I'll pick the supernova again. Please, I'm crushed just trying

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<v Speaker 2>to blow this up.

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<v Speaker 1>Hi.

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<v Speaker 2>I'm hoorhamy cartoonist and the creator of PhD comics.

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<v Speaker 1>Hi I'm Daniel. I'm a particle physicist and a professor

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<v Speaker 1>at UC Irvine, and I would rather be eaten by

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<v Speaker 1>aliens than never know if they exist for real.

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<v Speaker 2>Well, I guess if you get do you get to

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<v Speaker 2>choose when you get eaten by aliens? You know, if

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<v Speaker 2>you can choose to get it done right before you're

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<v Speaker 2>gonna die of natural causes. Maybe that's okay, but like

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<v Speaker 2>right now, you would make that choice right now.

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<v Speaker 1>I think this game is all about those loopholes, like

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<v Speaker 1>when people are planning for end of life, like do

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<v Speaker 1>you want to get buried or do you want to

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<v Speaker 1>get cremated. I'm going to fill out a box that

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<v Speaker 1>says I want to get eaten by aliens. But yeah,

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<v Speaker 1>it'd be nice if they waited till after I already

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<v Speaker 1>died of natural causes. Then you know, hey, barbecue me

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<v Speaker 1>for the alien pot luck. That's fine.

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<v Speaker 2>You gotta be careful, though, do you mean like extraterrestrial

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<v Speaker 2>aliens or people who are you know, alien alien to

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<v Speaker 2>your life or to your city?

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<v Speaker 1>You know what, I'm not gonna be around, so I

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<v Speaker 1>guess it doesn't really matter.

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<v Speaker 2>Oh you're gonna be around as you're getting in.

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<v Speaker 1>As long as I get to learn about the aliens

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<v Speaker 1>while I'm still alive, nothing else really matters.

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<v Speaker 2>Oh boy. Anyways, Welcome to our podcast Daniel and Jorge

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<v Speaker 2>Explain the Universe, a production of iHeartRadio in which.

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<v Speaker 1>We take great pains and great sacrifices to try to

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<v Speaker 1>explain the nature of the universe to you. We cast

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<v Speaker 1>our minds out into that dark cosmic mystery and wonder

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<v Speaker 1>what's out there, who's out there, what's going on out there,

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<v Speaker 1>how big is it? Is it still sloshing around, and

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<v Speaker 1>what will be its final fate. We want to understand

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<v Speaker 1>the cosmic context of our very existence because it drives

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<v Speaker 1>the choices we make every day about whether or not

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<v Speaker 1>we sign ourselves up to be part of an alien barbecue.

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<v Speaker 2>That's right. It is a humongous universe full of amazing

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<v Speaker 2>and awesome things out there that may kill you or

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<v Speaker 2>eat you, and or inspire you to learn more about

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<v Speaker 2>the universe and the cosmos and how everything works in it.

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<v Speaker 1>And it's part of this sort of incredible mental history,

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<v Speaker 1>the trajectory of our sort of mental map of the cosmos.

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<v Speaker 1>You know, it started out pretty small, your little village,

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<v Speaker 1>your neighborhood, eventually expanded to be a larger and larger region.

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<v Speaker 1>Finally people started incorporating the cosmos into it, this mental

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<v Speaker 1>picture of the whole universe that we were in. But

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<v Speaker 1>it just gets bigger and bigger as we understand where

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<v Speaker 1>our solar system sits and where our galaxy sits, and

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<v Speaker 1>as our telescopes get more and more powerful, we can

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<v Speaker 1>now understand even further the context of our cosmic neighborhood.

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<v Speaker 2>Yeah, it used to be there. Our context was pretty

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<v Speaker 2>much like the Earth, and people thought that the Sun

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<v Speaker 2>and the moon and the stars all revolved around the Earth.

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<v Speaker 2>People thought that the entire universe was just us.

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<v Speaker 1>Yeah. I was reading about ancient Chinese astronomy and they

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<v Speaker 1>even calculated like how far away the stars were. They

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<v Speaker 1>thought it was something like twenty seven thousand miles above

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<v Speaker 1>the Earth.

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<v Speaker 2>Oh, that's pretty close.

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<v Speaker 1>And the Greeks thought that everything moved in like literal

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<v Speaker 1>crystal spheres around the Earth. That was the original ether.

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<v Speaker 2>Interesting, now, Daniel, do we know for sure that's not true?

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<v Speaker 2>Do you know for sure that's not true.

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<v Speaker 1>I mean, we've sent probes out there to visit these things,

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<v Speaker 1>so we're pretty sure there are no crystal spheres out

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<v Speaker 1>there moving the planets.

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<v Speaker 2>By we mean the perverurial we but have you gone

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<v Speaker 2>up there and touched these that made sure there's no

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<v Speaker 2>crystal spheres.

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<v Speaker 1>I'm going to take NASA's word for it, you know,

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<v Speaker 1>for sure. I'm not part of the conspiracy community that

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<v Speaker 1>thinks NASA's been lying to us all these years.

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<v Speaker 2>You know, part of the crystal sphere conspiracy.

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<v Speaker 1>I'm sure there's a group of crystal truthists out there.

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<v Speaker 2>You know, part of the China was right theory.

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<v Speaker 1>No, but the Chinese did make a lot of really

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<v Speaker 1>amazing observations. You know, we have like records of eclipses

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<v Speaker 1>dating back foulands of years from China and observations is

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<v Speaker 1>like super nova from almost a thousand years ago. So

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<v Speaker 1>it's a really rich history of astronomical observations, some of

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<v Speaker 1>which are still relevant to our studies today. Is incredible.

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<v Speaker 2>Oh, it's pretty cool. Yeah, because, as you were saying,

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<v Speaker 2>our understanding of where or and how we fit in

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<v Speaker 2>this universe keeps growing and growing, and it seems like

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<v Speaker 2>each time we just get more and more insignificant with

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<v Speaker 2>each step.

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<v Speaker 1>But we become more and more aware of that significance,

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<v Speaker 1>which makes us sort of like philosophically more important. Right,

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<v Speaker 1>We're like incorporating more of the universe into our minds.

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<v Speaker 2>No, that makes no sense. We're insignificant specs in this

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<v Speaker 2>giant universe.

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<v Speaker 1>But it's better to know about your insignificance because then

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<v Speaker 1>you've gained some philosophical stature.

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<v Speaker 2>Like being know where you're being in by aliens doesn't help.

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<v Speaker 2>The fact that you're being eaten by.

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<v Speaker 1>Eight still makes it worth. It still makes it worth.

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<v Speaker 2>In fact, that makes it worse. But it does seem

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<v Speaker 2>like we are getting smaller and smaller in the sumer

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<v Speaker 2>And literally that's true, right because every year, every second

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<v Speaker 2>of the day, the universe, or our understanding of how

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<v Speaker 2>big it is, keeps getting bigger.

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<v Speaker 1>Right, it does. And even though we cannot explore the

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<v Speaker 1>far flung edges of the observable universe, we can build

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<v Speaker 1>this mental model, this sort of map of our neighborhood

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<v Speaker 1>that tells us where we are in this glittering cosmos.

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<v Speaker 1>And so even though no human will probably visit those

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<v Speaker 1>planets or visit those stars, we can still tell you

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<v Speaker 1>something about what's going on out there. And to me

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<v Speaker 1>that's incredible. Yes, we are probably trapped on this rock

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<v Speaker 1>or our neighboring rocks, but still we can build this

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<v Speaker 1>map of the cosmos, we can understand something about it.

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<v Speaker 1>And to me, that's a great achievement sort of intellectually

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<v Speaker 1>and scientifically, and what I'm pretty proud of.

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<v Speaker 2>Yeah, again, I think you're using the proverbial we there,

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<v Speaker 2>you're proud of the work of others. Let's be honest here.

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<v Speaker 1>No, I'm standing on the shoulders of many, many giants,

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<v Speaker 1>and I'm proud of their work. Absolutely, I'm not personally

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<v Speaker 1>taking credit for our understanding of the universe in case

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<v Speaker 1>anybody misunderstood, But.

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<v Speaker 2>At least we're helping, I guess talk about what they've

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<v Speaker 2>done and disseminate this information out to others. And it's

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<v Speaker 2>interesting when you say like that we might never reach

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<v Speaker 2>those places that we're seeing far far away. I'm wonder

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<v Speaker 2>if that's really true. I guess that's true because our

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<v Speaker 2>view of the universe expanding at the speed of light,

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<v Speaker 2>and there's no way that humans could outpacete that. Right.

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<v Speaker 1>Yeah, it's amazing we can see things that are moving

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<v Speaker 1>away from us faster than the speed of light. A

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<v Speaker 1>bunch of listeners wrote in and asked, like, how does

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<v Speaker 1>that work? We have a whole episode covering it, but briefly,

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<v Speaker 1>the thing to understand when you're looking at an object

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<v Speaker 1>and they tell you, oh, this thing is thirty billion

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<v Speaker 1>years away and it's moving away from us faster than

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<v Speaker 1>the speed of light, is that you're not seeing it

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<v Speaker 1>where it is now. They're telling you where it is now.

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<v Speaker 1>But you're seeing the light that was emitted from it

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<v Speaker 1>when it was much much closer. So it used to

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<v Speaker 1>be much closer, and it's sent a photon our way.

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<v Speaker 1>In the meantime, it's moved really really far away. When

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<v Speaker 1>they say here, we're looking at a galaxy that's really

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<v Speaker 1>really far away, we're not seeing light that came to

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<v Speaker 1>us from it when it was that far away. Were

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<v Speaker 1>seeing light that came to us when it was much

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<v Speaker 1>much closer. Light that leaves it now we will never see,

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<v Speaker 1>which means also we will never visit it.

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<v Speaker 2>Mmm. Yeah, Because the universe is expanding faster and faster

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<v Speaker 2>every time, every second of the day. Although we don't

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<v Speaker 2>know what's going to happen in the future right, it

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<v Speaker 2>could be that in the far distant future or maybe tomorrow,

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<v Speaker 2>the universe might decide, Hey, I think I'm going to

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<v Speaker 2>stop growing and I'm going to collapse back on myself,

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<v Speaker 2>and in which case, we're going to basically visit every

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<v Speaker 2>place in the universe at some point.

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<v Speaker 1>Yeah, or they're going to come visit us and they're

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<v Speaker 1>going to bring with them all their aliens, with all

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<v Speaker 1>their barbecue.

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<v Speaker 2>Tools, all their appetites. Well, maybe the big joke is

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<v Speaker 2>that in the end, the universe eats us.

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<v Speaker 3>All.

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<v Speaker 1>Well, we are the universe, so I guess the universe

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<v Speaker 1>eats itself. I'm not sure how that works.

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<v Speaker 2>Whoa dude.

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<v Speaker 1>And even though we are learning that we are a

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<v Speaker 1>tiny speck in a vast, vast cosmos, I think it

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<v Speaker 1>does make us sort of like philosophically or intellectually more

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<v Speaker 1>powerful to have grappled with that vast cosmos. It's better

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<v Speaker 1>at least than being ignorant of what's going on right right?

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<v Speaker 2>But don't they say ignorance is bliss Sometimes?

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<v Speaker 1>Who's looking for bliss? Man, I'm looking for knowledge.

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<v Speaker 2>Maybe that's the difference between you and me and Daniel.

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<v Speaker 2>I'll go for bliss any day.

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<v Speaker 1>Okay, Well, I'm glad we can split the tasks. But

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<v Speaker 1>it's also fun to think about that far future you

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<v Speaker 1>were talking about and wondering, like, what does the future hold?

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<v Speaker 1>Will our solar system survive for our billion years? Will

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<v Speaker 1>our galaxy survive for ten billion years? What exactly is

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<v Speaker 1>going to happen to our cosmic neighborhood over cosmic deep time? Yeah?

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<v Speaker 2>Because, as we mentioned, the universe is expanding faster and

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<v Speaker 2>faster and faster and that has some pretty dramatic consequences

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<v Speaker 2>for some of the bigger structures in the universe. And

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<v Speaker 2>so today on the podcast we'll be tackling the question

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<v Speaker 2>will our super cluster be torn apart? Sounds kind of sad.

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<v Speaker 1>Like a chunk of juicy barbecue.

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<v Speaker 2>Well, wow, who would eat a giant supercluster galaxies.

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<v Speaker 1>Some giant super space crab? I suppose, Oh boy?

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<v Speaker 2>And how big does the barbecue sauce bottle need to be? Well,

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<v Speaker 2>this is an interesting question and so we'll dig into

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<v Speaker 2>it of what a supercluster is, what does it mean

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<v Speaker 2>for it to be torn apart? And what could be

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<v Speaker 2>causing it to be torn apart? But as usual, we

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<v Speaker 2>were wondering how many people had considered these words together

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<v Speaker 2>as a question out there in the internet.

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<v Speaker 1>So thanks very much to everybody who participates in this

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<v Speaker 1>segment of our podcast. It's super fun for us to

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<v Speaker 1>hear what you're thinking about the topic of the day.

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<v Speaker 1>Please don't be shy. If you'd like to participate in

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<v Speaker 1>the future, just write to me to Questions at Danielandjorge

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<v Speaker 1>dot com.

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<v Speaker 2>So think about it for a second. Do you think

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<v Speaker 2>our supercluster will be torn apart. Here's what people have

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<v Speaker 2>to say. I say no, I believe that dark matter

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<v Speaker 2>and dark energy will keep it together, just like it

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<v Speaker 2>build the supercluster that we see today.

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<v Speaker 4>Well, our supercluster, if I believe right, is a collection

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<v Speaker 4>of galaxy that we're in kind of grouped up. So

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<v Speaker 4>if anything, I feel like it would get larger just

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<v Speaker 4>by gravitationally attracting other galaxies that are just floating out there.

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<v Speaker 3>If I get it right, the galaxies of our supercluster

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<v Speaker 3>won't drift apart due to the expansion of the universe,

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<v Speaker 3>but they might dive into each other.

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<v Speaker 5>A supercluster is a group of galaxy dark energy. Obviously

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<v Speaker 5>he's moving things apart. But I think the galaxy would

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<v Speaker 5>stay together, but that galaxies would separate from each other.

0:11:36.880 --> 0:11:40.720
<v Speaker 5>So I reckon our supercluster will be torn apart.

0:11:40.920 --> 0:11:44.640
<v Speaker 2>All right, Some people are feeling optimistic about our supercluster.

0:11:44.800 --> 0:11:48.440
<v Speaker 1>It looks like three to one for our superclusters sticking together.

0:11:48.640 --> 0:11:50.040
<v Speaker 1>We got some optimists out there.

0:11:50.160 --> 0:11:53.400
<v Speaker 2>Yeah. Yeah, everyone wants to remain I guess in the cluster.

0:11:54.400 --> 0:11:56.360
<v Speaker 1>They want to stay cozy. No one wants to blow

0:11:56.440 --> 0:11:56.959
<v Speaker 1>up our spot.

0:11:57.080 --> 0:12:00.720
<v Speaker 2>Yeah, but I guess some people mentioned gravity us together

0:12:00.800 --> 0:12:03.840
<v Speaker 2>instead of letting the supercluster get torn apart, and some

0:12:03.880 --> 0:12:06.319
<v Speaker 2>people mention dark matter as a way to keep things together.

0:12:06.480 --> 0:12:09.320
<v Speaker 1>Yeah, and the overall theme here is pretty much spot

0:12:09.360 --> 0:12:11.840
<v Speaker 1>on that the universe is in a tug of war

0:12:12.320 --> 0:12:16.000
<v Speaker 1>between gravity and dark energy and those things play out

0:12:16.160 --> 0:12:19.840
<v Speaker 1>very differently on different distances and different scales. And so

0:12:19.920 --> 0:12:22.320
<v Speaker 1>the fascinating question is like, at what point does dark

0:12:22.400 --> 0:12:24.520
<v Speaker 1>energy win? And where will gravity win?

0:12:25.320 --> 0:12:28.240
<v Speaker 2>Who will eat who? Gravity versus dark energy.

0:12:29.360 --> 0:12:31.839
<v Speaker 1>That's like Godzilla versus King Kong.

0:12:32.160 --> 0:12:36.440
<v Speaker 2>That's like slow roasted ribs versus grilled chicken.

0:12:37.440 --> 0:12:38.400
<v Speaker 1>I'll just eat them both.

0:12:38.440 --> 0:12:46.760
<v Speaker 2>Mane sounds good. Well, let's dive into this tasty topic here,

0:12:46.880 --> 0:12:50.000
<v Speaker 2>step us through Daniel. What is a supercluster of galaxies?

0:12:50.040 --> 0:12:53.320
<v Speaker 1>So a supercluster is the biggest thing in the universe.

0:12:53.800 --> 0:12:58.280
<v Speaker 1>It's the largest structure we think can exist in the universe.

0:12:58.559 --> 0:13:01.000
<v Speaker 1>And this episode is going to hinge closely on what

0:13:01.080 --> 0:13:04.640
<v Speaker 1>we mean by a structure. What is a thing in

0:13:04.679 --> 0:13:07.240
<v Speaker 1>the universe? Because you could just look out in space

0:13:07.280 --> 0:13:09.240
<v Speaker 1>and say I'm going to group all this stuff together

0:13:09.280 --> 0:13:10.880
<v Speaker 1>and call it a thing and give it a name,

0:13:11.120 --> 0:13:13.640
<v Speaker 1>the way we sort of do for constellations, But astronomers

0:13:13.679 --> 0:13:16.360
<v Speaker 1>like to think about things in the universe structures as

0:13:16.440 --> 0:13:19.400
<v Speaker 1>things that sort of hold themselves together, that have enough

0:13:19.440 --> 0:13:23.200
<v Speaker 1>gravity to be tied together to be an equilibrium. So

0:13:23.240 --> 0:13:25.960
<v Speaker 1>in our immediate neighborhood, for example, we think of the

0:13:26.000 --> 0:13:28.680
<v Speaker 1>Solar System as a thing. The Earth is going around

0:13:28.720 --> 0:13:30.920
<v Speaker 1>the Sun and it's going to keep doing that. Gravity

0:13:31.000 --> 0:13:33.200
<v Speaker 1>is holding the Earth around the Sun and all the

0:13:33.240 --> 0:13:35.800
<v Speaker 1>other planets, So we think of the Solar System as

0:13:35.800 --> 0:13:39.360
<v Speaker 1>a structure, as this gravitationally bound kind of object.

0:13:39.520 --> 0:13:41.160
<v Speaker 2>Yeah, because I guess if you think about just the

0:13:41.200 --> 0:13:43.839
<v Speaker 2>word structure and what it means in our everyday lives,

0:13:43.920 --> 0:13:47.880
<v Speaker 2>it basically just means like things that are clumped together, right,

0:13:47.960 --> 0:13:50.360
<v Speaker 2>or that move together, or that can be separated from

0:13:50.400 --> 0:13:52.920
<v Speaker 2>each other. And you sort of drill down into it,

0:13:53.040 --> 0:13:55.520
<v Speaker 2>like even the house you're sitting on, or the building

0:13:55.559 --> 0:13:58.240
<v Speaker 2>you're sitting on, or maybe even the car you're sitting on,

0:13:58.400 --> 0:14:02.000
<v Speaker 2>it's just a collection of loose parts being held together

0:14:02.040 --> 0:14:04.480
<v Speaker 2>by a force in the universe. Like they're not part

0:14:04.480 --> 0:14:07.280
<v Speaker 2>of the same thing. They're individual particles, but there's just

0:14:07.320 --> 0:14:09.760
<v Speaker 2>some force that keeps them all moving together.

0:14:09.960 --> 0:14:11.840
<v Speaker 1>Yeah, and it feels like a really natural thing. Right

0:14:11.880 --> 0:14:14.800
<v Speaker 1>to say I'm held together, I'm a thing. You're held together,

0:14:14.920 --> 0:14:17.480
<v Speaker 1>you're another thing. Even if we're standing next to each other,

0:14:17.640 --> 0:14:19.560
<v Speaker 1>it's easy to draw the line between us and say,

0:14:19.600 --> 0:14:22.600
<v Speaker 1>like where I end and you begin. That's sort of philosophically,

0:14:22.680 --> 0:14:25.440
<v Speaker 1>very straightforward, and so we imagine maybe that's possible to

0:14:25.440 --> 0:14:27.560
<v Speaker 1>do for other stuff too, Right to say, well, here's

0:14:27.600 --> 0:14:30.120
<v Speaker 1>one planet and there's another planet, to draw these lines

0:14:30.160 --> 0:14:32.640
<v Speaker 1>and say this thing holds itself together, and that thing

0:14:32.640 --> 0:14:34.840
<v Speaker 1>holds itself together. So that's sort of the idea of

0:14:34.880 --> 0:14:37.200
<v Speaker 1>a structure, But it can also get kind of fuzzy,

0:14:37.320 --> 0:14:38.920
<v Speaker 1>Like when you look up at the sky and you

0:14:38.920 --> 0:14:42.640
<v Speaker 1>see a cloud. It's this big blob of vapor. It's

0:14:42.640 --> 0:14:44.920
<v Speaker 1>not really holding itself together. I mean, it looks like

0:14:44.960 --> 0:14:48.160
<v Speaker 1>a thing sort of localized and clumped, but it's definitely

0:14:48.200 --> 0:14:51.000
<v Speaker 1>not gravitationally holding itself together. It just sort of happens

0:14:51.040 --> 0:14:53.440
<v Speaker 1>to be all in the same place at the same time,

0:14:54.000 --> 0:14:56.080
<v Speaker 1>or like a crowd in a park at lunchtime. Right,

0:14:56.200 --> 0:14:58.200
<v Speaker 1>they all happen to be near each other. They're clumped,

0:14:58.240 --> 0:15:01.040
<v Speaker 1>but they're not holding themselves together. So there can be

0:15:01.120 --> 0:15:03.120
<v Speaker 1>sometimes things that are like near each other. There are

0:15:03.120 --> 0:15:04.560
<v Speaker 1>clumps but not structures.

0:15:05.440 --> 0:15:08.360
<v Speaker 2>Interesting, Yeah, crowd is a good example, right, because it

0:15:08.440 --> 0:15:10.960
<v Speaker 2>may look like a cluster, or like from a farm,

0:15:11.040 --> 0:15:13.160
<v Speaker 2>might look like a clump of things, but really there's

0:15:13.200 --> 0:15:16.680
<v Speaker 2>nothing keeping those individual people or structures together.

0:15:16.800 --> 0:15:16.960
<v Speaker 3>Right.

0:15:17.040 --> 0:15:19.320
<v Speaker 2>They could at any moment just leave the group.

0:15:19.400 --> 0:15:21.680
<v Speaker 1>Yeah. Every kindergarten teacher knows that when you try to

0:15:21.720 --> 0:15:23.560
<v Speaker 1>take them out on a field trip, right, they can

0:15:23.600 --> 0:15:26.080
<v Speaker 1>all just suddenly run in any random direction.

0:15:26.480 --> 0:15:29.640
<v Speaker 2>Yeah, Whereas maybe like for the planet Earth, all the

0:15:29.760 --> 0:15:33.160
<v Speaker 2>rocks on planet Earth are being kept from flying away

0:15:33.280 --> 0:15:34.520
<v Speaker 2>by gravity, by a force.

0:15:34.680 --> 0:15:36.640
<v Speaker 1>And it's really fascinating to think about the sort of

0:15:36.720 --> 0:15:39.080
<v Speaker 1>levels of structure, right, Like a rock is a structure,

0:15:39.080 --> 0:15:42.320
<v Speaker 1>but it's also part of a larger structure the Earth,

0:15:42.560 --> 0:15:44.880
<v Speaker 1>and the Earth of course is a structure, but again

0:15:44.920 --> 0:15:47.640
<v Speaker 1>it's part of a larger structure. So we have this

0:15:47.720 --> 0:15:52.600
<v Speaker 1>incredible nested hierarchy of structures, which is really fascinating to

0:15:52.640 --> 0:15:54.960
<v Speaker 1>think about, like the scale of those things, right, Like

0:15:55.000 --> 0:15:57.760
<v Speaker 1>an atom is a structure, You're made of so many

0:15:57.800 --> 0:16:00.960
<v Speaker 1>structures on so many levels. Incredible to think about, like

0:16:01.360 --> 0:16:04.320
<v Speaker 1>how organized the universe is, and as a whole group

0:16:04.320 --> 0:16:06.600
<v Speaker 1>of philosophers who study this kind of thing and wonder like,

0:16:06.960 --> 0:16:09.160
<v Speaker 1>why do we have structure of these distances and not

0:16:09.280 --> 0:16:11.920
<v Speaker 1>other distances? And does it bubble up from the fundamental

0:16:11.960 --> 0:16:14.800
<v Speaker 1>laws of the universe and all sorts of fascinating philosophical

0:16:14.880 --> 0:16:17.280
<v Speaker 1>rabbit holes. But it's also just kind of fun to

0:16:17.280 --> 0:16:19.600
<v Speaker 1>figure out, like what is the structure? What is our

0:16:19.680 --> 0:16:22.920
<v Speaker 1>cosmic neighborhood, and so we can like zoom out step

0:16:22.960 --> 0:16:26.000
<v Speaker 1>by step and understand how we fit in to this

0:16:26.080 --> 0:16:28.960
<v Speaker 1>sort of larger cosmic set of like Russian nesting dolls.

0:16:29.240 --> 0:16:31.280
<v Speaker 2>Yeah, because I guess you know, sort of like you

0:16:31.320 --> 0:16:34.840
<v Speaker 2>were saying, the atoms in my body make up my structure,

0:16:35.040 --> 0:16:38.560
<v Speaker 2>but they're all also kind of being pulled by the

0:16:38.600 --> 0:16:41.600
<v Speaker 2>gravity of the earth, right, so like is it more

0:16:41.800 --> 0:16:44.240
<v Speaker 2>part of my structure or are all the atoms in

0:16:44.280 --> 0:16:47.280
<v Speaker 2>my body more part of the earth structure? And even

0:16:47.320 --> 0:16:49.320
<v Speaker 2>like the atoms in my body are being pulled by

0:16:49.320 --> 0:16:51.640
<v Speaker 2>the gravity of the sun. But we wouldn't say, like, hey,

0:16:51.680 --> 0:16:54.320
<v Speaker 2>I'm just me and the sun are one, even though

0:16:54.400 --> 0:16:57.360
<v Speaker 2>if you sort of follow the chain of forces that

0:16:57.480 --> 0:16:59.640
<v Speaker 2>we are sort of in the same structure as the Sun.

0:16:59.760 --> 0:17:01.920
<v Speaker 1>Yeah, And so you're part of many structures or you

0:17:01.920 --> 0:17:04.200
<v Speaker 1>could say that there's substructure, right, You could just look

0:17:04.200 --> 0:17:06.240
<v Speaker 1>at the whole galaxy and say the galaxy is a blob,

0:17:06.320 --> 0:17:09.600
<v Speaker 1>but obviously it has substructure. It's not just a smooth

0:17:09.680 --> 0:17:13.520
<v Speaker 1>distribution of atoms. There are stars and solar systems and

0:17:13.560 --> 0:17:16.760
<v Speaker 1>even clumps to those stars. They are like these groups

0:17:16.800 --> 0:17:19.959
<v Speaker 1>of stars are all formed together that are still moving together,

0:17:20.119 --> 0:17:22.240
<v Speaker 1>like that Kindergarten group. So there's sort of lots of

0:17:22.359 --> 0:17:26.160
<v Speaker 1>layers of structure, and it's fascinating to ask, like how

0:17:26.160 --> 0:17:29.520
<v Speaker 1>many layers are there? How many layers can we zoom

0:17:29.560 --> 0:17:32.560
<v Speaker 1>out and still see things that seem to be holding

0:17:32.640 --> 0:17:35.879
<v Speaker 1>themselves together. So we start with ourselves, and then of

0:17:35.920 --> 0:17:38.840
<v Speaker 1>course we have the Earth, and then there's the solar system,

0:17:39.520 --> 0:17:41.560
<v Speaker 1>and then we zoom out. The next sort of big

0:17:41.640 --> 0:17:44.639
<v Speaker 1>layer of structure would either be like a group of

0:17:44.760 --> 0:17:47.640
<v Speaker 1>stars that we all form together with or you would

0:17:47.680 --> 0:17:50.000
<v Speaker 1>zoom all the way out to the galaxy. Because those

0:17:50.040 --> 0:17:52.400
<v Speaker 1>groups of stars that form together, they don't really hold

0:17:52.440 --> 0:17:55.800
<v Speaker 1>themselves together for very long. They tend to disperse into

0:17:55.840 --> 0:17:56.480
<v Speaker 1>the galaxy.

0:17:56.800 --> 0:17:59.399
<v Speaker 2>M do we know that's for sure? Or I mean, like,

0:17:59.440 --> 0:18:02.120
<v Speaker 2>do we know which stars are near us? And would

0:18:02.119 --> 0:18:04.639
<v Speaker 2>you say maybe they're too far away for their gravity

0:18:04.680 --> 0:18:05.679
<v Speaker 2>to really affect us.

0:18:05.880 --> 0:18:08.040
<v Speaker 1>Yeah, other stars are too far away for the gravity

0:18:08.040 --> 0:18:10.320
<v Speaker 1>to really affect us. And we all have velocity through

0:18:10.320 --> 0:18:12.560
<v Speaker 1>the galaxy, and so we know a lot about actually

0:18:12.600 --> 0:18:16.160
<v Speaker 1>how stars dissipate from their original cluster. It can take

0:18:16.240 --> 0:18:18.719
<v Speaker 1>tens or hundreds of millions of years, but we definitely

0:18:18.720 --> 0:18:20.679
<v Speaker 1>see evidence of that when we look out at the

0:18:20.720 --> 0:18:24.200
<v Speaker 1>pattern of the stars in our galaxy. It also helps

0:18:24.280 --> 0:18:27.439
<v Speaker 1>us understand how the stars are moving. For example, like

0:18:27.480 --> 0:18:30.000
<v Speaker 1>the Big Dipper is a group of stars that were

0:18:30.040 --> 0:18:33.000
<v Speaker 1>all formed together, and they're moving together, but they're also

0:18:33.080 --> 0:18:35.680
<v Speaker 1>moving really fast and they're kind of close by, which

0:18:35.720 --> 0:18:38.080
<v Speaker 1>means that the Big Dipper is changing. You don't think

0:18:38.080 --> 0:18:40.639
<v Speaker 1>about the constellations as changing very much, but they actually

0:18:40.720 --> 0:18:42.720
<v Speaker 1>are all moving. We're not all moving at the same

0:18:42.840 --> 0:18:45.760
<v Speaker 1>relative velocity. So like the galaxy is a big, slashing

0:18:45.840 --> 0:18:48.680
<v Speaker 1>bathtub of stars. So the Big Dipper changes, and over

0:18:48.760 --> 0:18:51.399
<v Speaker 1>like one hundred thousand years or a few hundred thousand years,

0:18:51.600 --> 0:18:54.080
<v Speaker 1>the Big Dipper will no longer look like the Big Dipper.

0:18:54.200 --> 0:18:56.480
<v Speaker 2>Now are they would you say they're a structure or

0:18:56.520 --> 0:18:59.480
<v Speaker 2>are they just moving together like a crowd, or like

0:18:59.520 --> 0:19:00.760
<v Speaker 2>a wisp of clouds.

0:19:00.840 --> 0:19:02.520
<v Speaker 1>They are not a structure because they're not going to

0:19:02.560 --> 0:19:05.720
<v Speaker 1>hold themselves together. They're not like tight enough to be

0:19:05.800 --> 0:19:08.399
<v Speaker 1>a structure. They're definitely going to dissolve into the larger

0:19:08.440 --> 0:19:13.040
<v Speaker 1>sort of bathtub of the galaxy. There are sometimes substructures

0:19:13.040 --> 0:19:14.920
<v Speaker 1>to the galaxy, but those tend to be like little

0:19:15.000 --> 0:19:18.560
<v Speaker 1>dwarf galaxies that orbit the Milky Way and that have

0:19:18.640 --> 0:19:22.280
<v Speaker 1>their own gravitational hold on themselves that haven't gotten pulled

0:19:22.320 --> 0:19:24.720
<v Speaker 1>apart by the Milky Way. But within the Milky Way,

0:19:24.720 --> 0:19:26.440
<v Speaker 1>there aren't really those kinds of structures.

0:19:26.600 --> 0:19:29.400
<v Speaker 2>So you would say, like after our solar system, the

0:19:29.440 --> 0:19:32.639
<v Speaker 2>next structure is a galaxy. You wouldn't maybe call the

0:19:32.800 --> 0:19:34.280
<v Speaker 2>arms of a galaxy a structure.

0:19:34.400 --> 0:19:37.119
<v Speaker 1>Well, those are density waves, right. Even the arms of

0:19:37.160 --> 0:19:40.199
<v Speaker 1>the galaxy are not physical structures. It's not like the

0:19:40.280 --> 0:19:44.119
<v Speaker 1>same stars are moving through those arms. The arms are

0:19:44.160 --> 0:19:47.000
<v Speaker 1>a wave through the stars. Like when you go to

0:19:47.040 --> 0:19:50.040
<v Speaker 1>a football game and people do the wave. That wave

0:19:50.080 --> 0:19:52.320
<v Speaker 1>itself is not a structure. It's just an arrangement of

0:19:52.320 --> 0:19:54.880
<v Speaker 1>the people as they move up and down. Galaxy arms

0:19:54.880 --> 0:19:57.639
<v Speaker 1>are the same way. They're not physical structures. They're just

0:19:57.760 --> 0:20:01.199
<v Speaker 1>density waves. So they're not actually whole themselves together, just

0:20:01.240 --> 0:20:03.399
<v Speaker 1>like waves in the ocean are not really structures that

0:20:03.440 --> 0:20:04.359
<v Speaker 1>I'm bound together.

0:20:05.359 --> 0:20:07.920
<v Speaker 2>And so our solar system, our star is not part

0:20:07.960 --> 0:20:10.440
<v Speaker 2>of a like a mini dwarf galaxy. We're just out

0:20:10.480 --> 0:20:12.400
<v Speaker 2>in the larger Milky Way galaxy.

0:20:12.520 --> 0:20:15.200
<v Speaker 1>Yep, we're just floating in the bathtub of the Milky Way,

0:20:15.560 --> 0:20:18.359
<v Speaker 1>along with hundreds of billions of other stars.

0:20:18.119 --> 0:20:22.239
<v Speaker 2>And potentially aliens that might eat us one of us. Right,

0:20:22.280 --> 0:20:25.120
<v Speaker 2>it sounds like a dangerous hot tub. Well, let's dig

0:20:25.160 --> 0:20:28.119
<v Speaker 2>into the next level of structure in the universe, and

0:20:28.240 --> 0:20:31.240
<v Speaker 2>let's see how big we can go. How far can

0:20:31.280 --> 0:20:34.440
<v Speaker 2>we add or recognize structure in the universe, and what's

0:20:34.480 --> 0:20:36.480
<v Speaker 2>going to happen to all that structure at the end

0:20:36.560 --> 0:20:39.560
<v Speaker 2>of time. So let's dig into that. But first let's

0:20:39.600 --> 0:20:54.600
<v Speaker 2>take a quick break. All right, we're asking the question

0:20:54.680 --> 0:20:58.320
<v Speaker 2>will our supercluster be torn apart? Which kind of sounds

0:20:58.359 --> 0:21:02.200
<v Speaker 2>like an oxymoron question or a contradictory question. Well, something

0:21:02.240 --> 0:21:04.320
<v Speaker 2>that's clustered together and not be clustered together.

0:21:05.240 --> 0:21:07.159
<v Speaker 1>Yeah, in the end, we're going to learn that astronomers

0:21:07.200 --> 0:21:11.000
<v Speaker 1>are arguing about how to define a supercluster, and some

0:21:11.160 --> 0:21:14.119
<v Speaker 1>definitions make the answer obvious, and some definitions make the

0:21:14.119 --> 0:21:16.280
<v Speaker 1>answer to this question very fuzzy.

0:21:16.440 --> 0:21:19.040
<v Speaker 2>But we were talking about how you know things, how

0:21:19.040 --> 0:21:22.199
<v Speaker 2>do you define structures? And it seems like sometimes, like

0:21:22.200 --> 0:21:23.960
<v Speaker 2>in a cloud or in a crowd, things might look

0:21:24.000 --> 0:21:26.399
<v Speaker 2>like they're together, but really they can fall apart at

0:21:26.400 --> 0:21:28.399
<v Speaker 2>any point, so you wouldn't call that a structure. But

0:21:28.560 --> 0:21:31.080
<v Speaker 2>like the atoms in your body or the atoms in

0:21:31.119 --> 0:21:33.359
<v Speaker 2>the building or car you're sitting on, they're held together

0:21:33.400 --> 0:21:37.640
<v Speaker 2>pretty tightly by forces, and they basically sort of ignore

0:21:37.760 --> 0:21:40.080
<v Speaker 2>other forces in favor of the forces that are holding

0:21:40.119 --> 0:21:42.280
<v Speaker 2>them together. And so maybe that's why we call them

0:21:42.400 --> 0:21:43.000
<v Speaker 2>a structure.

0:21:43.080 --> 0:21:45.320
<v Speaker 1>That's right, And it can be gravitational, or it can

0:21:45.359 --> 0:21:48.840
<v Speaker 1>be electromagnetic, or can be the strong force that forms

0:21:48.880 --> 0:21:51.720
<v Speaker 1>these structures, like the proton is a structure of the

0:21:51.760 --> 0:21:54.840
<v Speaker 1>strong force, and the atom is a structure of electromagnetism.

0:21:54.920 --> 0:21:58.920
<v Speaker 1>But at larger distances, basically anything bigger than a few meters,

0:21:59.200 --> 0:22:02.760
<v Speaker 1>it's mostly gravity that takes over because the other forces

0:22:02.760 --> 0:22:05.959
<v Speaker 1>are so powerful that they tend to neutralize themselves. Anything

0:22:06.000 --> 0:22:08.639
<v Speaker 1>that has a large positive or negative charge is going

0:22:08.680 --> 0:22:11.520
<v Speaker 1>to attract the opposite charge and end up neutralizing itself,

0:22:11.560 --> 0:22:15.200
<v Speaker 1>but over the large distances, it's gravity that forms structure

0:22:15.200 --> 0:22:19.480
<v Speaker 1>because gravity cannot be neutralized. Essentially, it's only attractive. There

0:22:19.480 --> 0:22:21.720
<v Speaker 1>are a few scenarios we can talk about with like

0:22:21.800 --> 0:22:25.320
<v Speaker 1>repulsive gravity, and dark energy might be an example of that,

0:22:25.359 --> 0:22:27.800
<v Speaker 1>but on the whole, gravity is attractive, and so it's

0:22:27.920 --> 0:22:30.399
<v Speaker 1>the force that's responsible for most of the structure we

0:22:30.440 --> 0:22:31.560
<v Speaker 1>think about in the universe.

0:22:31.840 --> 0:22:32.080
<v Speaker 5>Mmm.

0:22:32.400 --> 0:22:34.600
<v Speaker 2>Yeah, Like after about the size of a planet, there's

0:22:34.600 --> 0:22:37.320
<v Speaker 2>no other forces really at play in the universe that

0:22:37.400 --> 0:22:39.520
<v Speaker 2>we know of. Maybe there's something hitting out there. Could

0:22:39.600 --> 0:22:41.200
<v Speaker 2>dark matter be some kind of new force?

0:22:42.280 --> 0:22:44.440
<v Speaker 1>It could in dark energy is definitely in that category.

0:22:44.480 --> 0:22:47.600
<v Speaker 1>We don't know if it's a manifestation of gravity due

0:22:47.600 --> 0:22:50.960
<v Speaker 1>to the quantum energy of space or something totally else

0:22:51.040 --> 0:22:51.560
<v Speaker 1>and weird.

0:22:51.800 --> 0:22:54.240
<v Speaker 2>All right, Well, we talked about how we're part of

0:22:54.280 --> 0:22:57.080
<v Speaker 2>a solar system, and the Solar system is part of

0:22:57.680 --> 0:23:00.000
<v Speaker 2>a bigger structure called the Milky Way galaxy.

0:23:00.200 --> 0:23:02.720
<v Speaker 1>After that, so the galaxies aren't just like floating out

0:23:02.760 --> 0:23:06.240
<v Speaker 1>in space sprinkled evenly through the universe. They tend to

0:23:06.359 --> 0:23:08.800
<v Speaker 1>clump together, and they can clump together into something that

0:23:08.840 --> 0:23:12.280
<v Speaker 1>we call a galactic group or a group of galaxies

0:23:12.400 --> 0:23:14.440
<v Speaker 1>in our galaxy, the Milky Way is part of a

0:23:14.480 --> 0:23:17.639
<v Speaker 1>group we call the Local Group very cleverly, and it

0:23:17.680 --> 0:23:21.240
<v Speaker 1>has about fifty ish galaxies in it. The biggest one

0:23:21.400 --> 0:23:24.200
<v Speaker 1>is Andromeda, which is also the nearest one to us.

0:23:24.400 --> 0:23:27.160
<v Speaker 2>And so these are galaxies that are not just neros

0:23:27.240 --> 0:23:30.560
<v Speaker 2>out of convenience. We're actually sort of locked together with

0:23:30.720 --> 0:23:33.680
<v Speaker 2>them in some sort of gravitational dance. Right.

0:23:33.760 --> 0:23:36.639
<v Speaker 1>Yeah. We think that these galaxies are holding themselves together.

0:23:36.680 --> 0:23:40.520
<v Speaker 1>They're like a single gravitational object. They are orbiting the

0:23:40.520 --> 0:23:43.879
<v Speaker 1>center of mass of all of these galaxies. And people

0:23:43.920 --> 0:23:47.159
<v Speaker 1>hear a lot that the universe is expanding and everything

0:23:47.200 --> 0:23:49.360
<v Speaker 1>is getting farther and farther away. And that's true sort

0:23:49.359 --> 0:23:51.679
<v Speaker 1>of on the whole when you look at vast distances,

0:23:52.160 --> 0:23:55.440
<v Speaker 1>but nearby gravity is powerful enough to hold us together,

0:23:55.880 --> 0:23:59.360
<v Speaker 1>and that's happening also with these galaxies. That's why, for example,

0:23:59.560 --> 0:24:02.960
<v Speaker 1>we are towards the Andromeda galaxy and in a few

0:24:02.960 --> 0:24:06.520
<v Speaker 1>billion years our galaxy and Andromeda will collide and will

0:24:06.560 --> 0:24:09.679
<v Speaker 1>merge because gravity is winning the battle over the expansion

0:24:09.760 --> 0:24:12.560
<v Speaker 1>of space. So this local group, we think, is a thing.

0:24:12.640 --> 0:24:16.159
<v Speaker 1>It's a structure that gravity is powerful enough to hold together.

0:24:16.320 --> 0:24:18.760
<v Speaker 2>And now what kind of shape does this local group have?

0:24:19.000 --> 0:24:21.000
<v Speaker 2>Is it like a disk like our solar system or

0:24:21.080 --> 0:24:22.919
<v Speaker 2>the galaxy, or is it still kind of like a

0:24:22.960 --> 0:24:26.200
<v Speaker 2>fuzzy cloud of things moving in all directions.

0:24:26.320 --> 0:24:28.960
<v Speaker 1>It doesn't really have a great shape because it's sort

0:24:29.000 --> 0:24:32.440
<v Speaker 1>of weirdly distributed, like there's Andromeda, then there's the Milky Way,

0:24:32.560 --> 0:24:36.000
<v Speaker 1>there's another galaxy called the Triangular Galaxy, and the rest

0:24:36.040 --> 0:24:38.879
<v Speaker 1>of it is like a sprinkle of little tiny galaxies.

0:24:39.240 --> 0:24:41.800
<v Speaker 1>So they're not like nicely organized into a flat disc

0:24:42.240 --> 0:24:44.840
<v Speaker 1>or anything like that. It's just sort of like a blob.

0:24:45.160 --> 0:24:47.000
<v Speaker 2>Or at least not yet. Right, Like, maybe if you

0:24:47.080 --> 0:24:49.640
<v Speaker 2>fast forward a few billion years, things will even out

0:24:49.640 --> 0:24:51.560
<v Speaker 2>into a disk, because that's what things do in space,

0:24:51.640 --> 0:24:54.640
<v Speaker 2>they organize themselves into discs, right.

0:24:54.720 --> 0:24:56.280
<v Speaker 1>They do tend to do that if you give them

0:24:56.359 --> 0:24:59.960
<v Speaker 1>enough time, because they're spinning and gravity will collapse everything

0:25:00.119 --> 0:25:02.439
<v Speaker 1>down eventually, except along the plane of their spin they

0:25:02.440 --> 0:25:05.000
<v Speaker 1>can resist gravity a little bit, which is why they

0:25:05.080 --> 0:25:07.439
<v Speaker 1>end up as disks. So in sort of one direction

0:25:07.520 --> 0:25:09.720
<v Speaker 1>they can collapse, and along the other two dimensions on

0:25:09.760 --> 0:25:12.359
<v Speaker 1>that plane they end up sort of spinning around, which

0:25:12.359 --> 0:25:14.119
<v Speaker 1>is how you get a flat solar system and a

0:25:14.119 --> 0:25:17.920
<v Speaker 1>flat galaxy. Eventually, though, we think that gravity will win,

0:25:18.119 --> 0:25:20.080
<v Speaker 1>that those things will bump against each other and lose

0:25:20.119 --> 0:25:24.040
<v Speaker 1>angular momentum, or they will radiate gravitational waves and lose

0:25:24.080 --> 0:25:27.600
<v Speaker 1>that energy. And eventually we think that gravitationally bound objects

0:25:27.680 --> 0:25:30.840
<v Speaker 1>will all collapse together, first into one big galaxy and

0:25:30.880 --> 0:25:33.040
<v Speaker 1>then eventually just into one big black hole.

0:25:33.359 --> 0:25:33.600
<v Speaker 3>Yit.

0:25:33.880 --> 0:25:37.000
<v Speaker 2>But before that happens, we can see other kinds of structures, right,

0:25:37.040 --> 0:25:40.119
<v Speaker 2>bigger structures, So like a group of galaxies can be

0:25:40.160 --> 0:25:42.840
<v Speaker 2>part of a larger kind of thing.

0:25:43.119 --> 0:25:45.080
<v Speaker 1>Yeah, so we call this either a group or a

0:25:45.119 --> 0:25:48.240
<v Speaker 1>cluster of galaxies. And depending on the size, like if

0:25:48.280 --> 0:25:50.919
<v Speaker 1>there aren't that many galaxies in it, like in hours,

0:25:50.920 --> 0:25:53.560
<v Speaker 1>we call it a group. If there are more galaxies

0:25:53.560 --> 0:25:56.040
<v Speaker 1>in it, you can call it a cluster. And so nearby,

0:25:56.160 --> 0:25:59.159
<v Speaker 1>for example, is the Virgo cluster. It has more than

0:25:59.240 --> 0:26:01.919
<v Speaker 1>a thousand galaxies that are like the Milky Way, so

0:26:01.960 --> 0:26:05.119
<v Speaker 1>it's much much bigger than the local group, and we

0:26:05.119 --> 0:26:07.520
<v Speaker 1>think that is also like an object that has structure,

0:26:07.720 --> 0:26:09.800
<v Speaker 1>we think it's going to hold itself together, that there's

0:26:09.920 --> 0:26:12.119
<v Speaker 1>enough gravity to keep itself together.

0:26:12.359 --> 0:26:15.400
<v Speaker 2>Yeah, isn't it pretty amazing to think even at these numbers,

0:26:15.440 --> 0:26:17.320
<v Speaker 2>like a thousand. A thousand doesn't sound like a lot,

0:26:17.480 --> 0:26:21.160
<v Speaker 2>But if you imagine a thousand galaxies like the Milky Way,

0:26:21.400 --> 0:26:23.880
<v Speaker 2>that is sort of mind blowing. Right, Like, we think

0:26:23.920 --> 0:26:27.040
<v Speaker 2>our galaxy is pretty huge and we'll probably never get

0:26:27.080 --> 0:26:29.520
<v Speaker 2>to the other side of it, and has billions of stars.

0:26:29.960 --> 0:26:32.119
<v Speaker 2>Now imagine there are thousands of these things out there

0:26:32.119 --> 0:26:32.560
<v Speaker 2>in space.

0:26:32.680 --> 0:26:34.800
<v Speaker 1>And the thing that blows my mind is the planets. Right,

0:26:34.880 --> 0:26:37.199
<v Speaker 1>even in our galaxy, we know there are hundreds of

0:26:37.280 --> 0:26:40.840
<v Speaker 1>billions of stars, and a significant fraction of those have

0:26:41.000 --> 0:26:44.000
<v Speaker 1>Earth like planets. You know, planets about the same size

0:26:44.040 --> 0:26:47.000
<v Speaker 1>with about the same surface temperature. We don't really know

0:26:47.119 --> 0:26:49.639
<v Speaker 1>that much more about them, but like, that's a lot

0:26:49.720 --> 0:26:53.200
<v Speaker 1>of Earth like planets. We're talking about tens of billions

0:26:53.280 --> 0:26:56.040
<v Speaker 1>just in our galaxy, and now multiply that by a

0:26:56.119 --> 0:27:00.240
<v Speaker 1>thousand for all the galaxies in the Virgo clusters hard

0:27:00.240 --> 0:27:02.640
<v Speaker 1>to keep track of, like all the places aliens could

0:27:02.640 --> 0:27:04.280
<v Speaker 1>be sharpening their barbecue tools.

0:27:04.560 --> 0:27:08.000
<v Speaker 2>Yeah, so let's not think about that. Yeah, I agree with.

0:27:08.000 --> 0:27:13.080
<v Speaker 1>You, But the Virgo cluster is like the biggest thing around.

0:27:13.119 --> 0:27:16.320
<v Speaker 1>There are other little galaxy groups nearby, Like there's the

0:27:16.440 --> 0:27:19.520
<v Speaker 1>M eighty one group, and the Sculptor group other little

0:27:19.600 --> 0:27:22.120
<v Speaker 1>groups of galaxies that are sort of in this sort

0:27:22.160 --> 0:27:24.639
<v Speaker 1>of the same size as our group. But the Virgo

0:27:24.680 --> 0:27:28.000
<v Speaker 1>cluster is like the big Papa and Mama galaxy cluster nearby.

0:27:28.040 --> 0:27:30.760
<v Speaker 1>It's like the most massive thing in the nearby universe.

0:27:31.000 --> 0:27:33.920
<v Speaker 2>Well, it's interesting with gravity, I feel, because gravity doesn't

0:27:33.920 --> 0:27:37.240
<v Speaker 2>have a limit, right, Like there's no distance limit for gravity,

0:27:37.480 --> 0:27:40.120
<v Speaker 2>Like this Virgo cluster is super dup or duper far

0:27:40.160 --> 0:27:43.359
<v Speaker 2>away from us. But technically speaking, like the atoms in

0:27:43.400 --> 0:27:46.040
<v Speaker 2>my body and in your body and everybody's bodies is

0:27:46.080 --> 0:27:50.680
<v Speaker 2>being tugged pulled by the gravity of that cluster super

0:27:50.720 --> 0:27:51.120
<v Speaker 2>far away.

0:27:51.200 --> 0:27:54.479
<v Speaker 1>That's right, Everything in the universe technically is pulling on

0:27:54.520 --> 0:27:57.280
<v Speaker 1>you gravitationally. Gravity does have this weakness though, which is

0:27:57.560 --> 0:28:01.520
<v Speaker 1>that its power drops as the dist is squared. So

0:28:01.560 --> 0:28:04.360
<v Speaker 1>if you're twice as far away from something, it's gravity

0:28:04.400 --> 0:28:06.880
<v Speaker 1>goes down by a factor of four. If you're ten

0:28:06.960 --> 0:28:09.560
<v Speaker 1>times further away, then the gravity goes down by a

0:28:09.600 --> 0:28:11.520
<v Speaker 1>factor of one hundred. And this gets to be a

0:28:11.600 --> 0:28:15.880
<v Speaker 1>very powerful obstacle to gravity as distances grow large, and

0:28:15.960 --> 0:28:18.360
<v Speaker 1>so the Virgo cluster, even though it's the most massive

0:28:18.359 --> 0:28:21.360
<v Speaker 1>thing in the nearby universe. It's like fifty or sixty

0:28:21.640 --> 0:28:26.760
<v Speaker 1>million light years away. That's a big distance to square, right,

0:28:27.080 --> 0:28:29.840
<v Speaker 1>So its gravity is really tiny, which is why it's

0:28:29.840 --> 0:28:32.720
<v Speaker 1>not obvious whether our little group, the local group, and

0:28:32.800 --> 0:28:35.439
<v Speaker 1>the Virgo cluster should be considered as part of some

0:28:35.600 --> 0:28:36.440
<v Speaker 1>larger object.

0:28:36.680 --> 0:28:36.840
<v Speaker 3>Right.

0:28:36.880 --> 0:28:39.680
<v Speaker 2>It gets attenuated a lot, it weakened a lot by distance,

0:28:39.720 --> 0:28:42.000
<v Speaker 2>but it's still there, right, Like I feel like like

0:28:42.040 --> 0:28:46.040
<v Speaker 2>I'm sensing I have this feeling of like a small

0:28:46.200 --> 0:28:49.240
<v Speaker 2>tendril of force that pulls me from the atoms in

0:28:49.320 --> 0:28:52.800
<v Speaker 2>my body to the Virgo cluster, right, And it also

0:28:52.880 --> 0:28:54.920
<v Speaker 2>kind of depends like what if the Virgo cluster was

0:28:55.560 --> 0:28:59.960
<v Speaker 2>super duper massive, right, we would eventually feel their gravity.

0:29:00.120 --> 0:29:02.520
<v Speaker 1>Yeah, that's true, and we do feel it's gravity. You're

0:29:02.520 --> 0:29:05.120
<v Speaker 1>absolutely right. I feel like you're just sort of preparing

0:29:05.160 --> 0:29:07.040
<v Speaker 1>an argument for when the aliens come and you're like,

0:29:07.080 --> 0:29:09.240
<v Speaker 1>hey man, we're all part of the same thing, and

0:29:09.320 --> 0:29:11.400
<v Speaker 1>we can feel your gravity, and we do, and we

0:29:11.480 --> 0:29:14.360
<v Speaker 1>can feel that gravity. And there's another way in which

0:29:14.400 --> 0:29:17.040
<v Speaker 1>we are connected to those objects. Right now, we're just

0:29:17.120 --> 0:29:20.480
<v Speaker 1>thinking mostly about the stars, the things that shine brightly,

0:29:20.600 --> 0:29:23.600
<v Speaker 1>but there are these filaments that connect us to the

0:29:23.680 --> 0:29:27.640
<v Speaker 1>other galaxies. Like between US and ANDRAMA is not empty space.

0:29:27.720 --> 0:29:32.160
<v Speaker 1>There's this filament, this string of both matter like hydrogen atoms,

0:29:32.160 --> 0:29:35.520
<v Speaker 1>et cetera, and also dark matter. So it's not like

0:29:35.600 --> 0:29:38.640
<v Speaker 1>a bunch of dots out in space. These galaxies they're

0:29:38.680 --> 0:29:42.080
<v Speaker 1>connected to each other. It's part of some huge cosmic

0:29:42.200 --> 0:29:45.040
<v Speaker 1>web where the other parts are more invisible because they're

0:29:45.080 --> 0:29:45.720
<v Speaker 1>not glowing.

0:29:46.400 --> 0:29:48.640
<v Speaker 2>Yeah, it's sort of like a spider's web right the universe.

0:29:48.720 --> 0:29:50.360
<v Speaker 2>Like if you look at a picture of the universe

0:29:50.520 --> 0:29:52.640
<v Speaker 2>and all the stars in it, the stars, even though

0:29:52.680 --> 0:29:55.440
<v Speaker 2>they're pinpoints, they sort of don't look like a random

0:29:55.480 --> 0:29:58.600
<v Speaker 2>white noise. They sort of look like a spider's web kind.

0:29:58.520 --> 0:30:02.640
<v Speaker 1>Of mm hmm. Between those dots there really is stuff.

0:30:03.040 --> 0:30:06.320
<v Speaker 1>You know, galaxies form in certain locations because that happens

0:30:06.360 --> 0:30:08.640
<v Speaker 1>to me where there was a little bit more dark matter.

0:30:09.120 --> 0:30:11.200
<v Speaker 1>So there's like a blob of dark matter there that's

0:30:11.240 --> 0:30:16.000
<v Speaker 1>gathered together enough light to start fusion going in those stars.

0:30:16.080 --> 0:30:18.640
<v Speaker 1>But between them there are these filaments of gas and

0:30:18.760 --> 0:30:22.240
<v Speaker 1>dark matter still flowing into those halos. So you could

0:30:22.240 --> 0:30:24.760
<v Speaker 1>think about it like a network of lakes with rivers

0:30:24.800 --> 0:30:27.800
<v Speaker 1>flowing into them, still filling them up, So galaxies are

0:30:27.840 --> 0:30:32.160
<v Speaker 1>still gathering dark matter and gas from these filaments. Structure

0:30:32.160 --> 0:30:35.840
<v Speaker 1>there is still sort of forming. Even though fourteen billion

0:30:35.920 --> 0:30:38.640
<v Speaker 1>years have gone by, things are still happening out there

0:30:38.640 --> 0:30:39.280
<v Speaker 1>in the universe.

0:30:40.080 --> 0:30:42.000
<v Speaker 2>I guess if there's a big cloud of something like

0:30:42.080 --> 0:30:44.560
<v Speaker 2>hydrogen out there in the middle of empty space, gravity

0:30:44.600 --> 0:30:47.680
<v Speaker 2>would be pulling it together, that cloud together into a

0:30:47.720 --> 0:30:50.600
<v Speaker 2>smaller cloud, and then our gravity would be and the

0:30:50.640 --> 0:30:52.840
<v Speaker 2>gravity of other clusters would be trying to stuck that

0:30:52.960 --> 0:30:55.560
<v Speaker 2>gas towards them. And so that's why maybe you get

0:30:55.600 --> 0:30:58.680
<v Speaker 2>these tendrils, these sort of like tentacles of gas out

0:30:58.680 --> 0:31:00.880
<v Speaker 2>there in space because they're being straight out and sucked

0:31:00.880 --> 0:31:03.000
<v Speaker 2>and do the different galaxies.

0:31:02.520 --> 0:31:05.480
<v Speaker 1>Exactly, And mostly it's the dark matter doing that. Remember,

0:31:05.520 --> 0:31:09.040
<v Speaker 1>we only see the visible matter, but that's twenty percent

0:31:09.240 --> 0:31:11.680
<v Speaker 1>of the matter that's out there, most of the gravity

0:31:11.680 --> 0:31:14.520
<v Speaker 1>in the universe. Most of those tendrils you feel from

0:31:14.520 --> 0:31:17.440
<v Speaker 1>the other cluster are actually from the dark matter in

0:31:17.480 --> 0:31:19.960
<v Speaker 1>that cluster, because that's most of the matter, and so

0:31:20.120 --> 0:31:22.680
<v Speaker 1>most of the gravity in the universe. Like, the reason

0:31:22.680 --> 0:31:25.000
<v Speaker 1>we have a galaxy here and not somewhere else is

0:31:25.040 --> 0:31:28.040
<v Speaker 1>because there was dark matter to form this structure. It

0:31:28.080 --> 0:31:30.920
<v Speaker 1>created this like gravitational well, the sort of lake to

0:31:31.040 --> 0:31:33.720
<v Speaker 1>pull all the other rivers of matter into it.

0:31:34.000 --> 0:31:37.680
<v Speaker 2>Cool. Well, after a cluster of galaxies, what's next?

0:31:37.920 --> 0:31:40.560
<v Speaker 1>So what's next is a little bit controversial, and in

0:31:40.600 --> 0:31:42.200
<v Speaker 1>the last ten years or so there's been a lot

0:31:42.240 --> 0:31:44.960
<v Speaker 1>of arguments about it. But there's a group of astronomers

0:31:45.000 --> 0:31:47.520
<v Speaker 1>out there that say that all these clusters, in these

0:31:47.560 --> 0:31:51.160
<v Speaker 1>little groups can be gathered together into something bigger called

0:31:51.200 --> 0:31:54.960
<v Speaker 1>a supercluster. The supercluster would take like the Virgo cluster

0:31:55.440 --> 0:31:57.840
<v Speaker 1>and our little group, and a bunch of other things,

0:31:57.880 --> 0:32:01.000
<v Speaker 1>including like the Great Attractor and them a cluster, and

0:32:01.040 --> 0:32:04.960
<v Speaker 1>the Centauris cluster and many others, into some huge object

0:32:05.000 --> 0:32:07.600
<v Speaker 1>that has like one hundred thousand galaxies in it.

0:32:07.760 --> 0:32:11.920
<v Speaker 2>Right, And this supercluster is called the Lenni Kiak supercluster. Right.

0:32:12.080 --> 0:32:15.000
<v Speaker 1>Yeah, it's a Hawaiian word that means immense heaven, and

0:32:14.960 --> 0:32:17.840
<v Speaker 1>it were defined in like twenty fourteen when a bunch

0:32:17.880 --> 0:32:20.560
<v Speaker 1>of astronomers looked at the velocity of all these things

0:32:20.560 --> 0:32:22.640
<v Speaker 1>and said, you know what, all these things are sort

0:32:22.680 --> 0:32:26.520
<v Speaker 1>of like falling towards themselves, and there's another blob of

0:32:26.560 --> 0:32:30.080
<v Speaker 1>stuff over there that's falling towards themselves, and so they

0:32:30.200 --> 0:32:32.080
<v Speaker 1>figure out how to sort of like draw a line

0:32:32.120 --> 0:32:35.160
<v Speaker 1>between one set of blobs and another set of blobs,

0:32:35.200 --> 0:32:37.680
<v Speaker 1>and they said, we're in this blob over here.

0:32:38.040 --> 0:32:41.360
<v Speaker 2>M I see. But can you make the mathematical calculation,

0:32:41.520 --> 0:32:45.080
<v Speaker 2>like if you compute the gravity that we're feeling between

0:32:45.120 --> 0:32:48.520
<v Speaker 2>these clusters, and does it really work out that you

0:32:48.640 --> 0:32:53.280
<v Speaker 2>can group these superclusters as one or is it more

0:32:53.320 --> 0:32:55.800
<v Speaker 2>like an illusion like a wisp of cloud or a

0:32:55.880 --> 0:32:57.040
<v Speaker 2>crowd of people in a park.

0:32:57.240 --> 0:32:59.680
<v Speaker 1>Yeah, that's exactly the question, and that's really what we're

0:32:59.720 --> 0:33:03.680
<v Speaker 1>in entering today is what is the future of this supercluster?

0:33:03.880 --> 0:33:06.240
<v Speaker 1>Is it going to hold itself together or is it

0:33:06.240 --> 0:33:08.720
<v Speaker 1>going to get torn apart? Because we've been talking about

0:33:08.760 --> 0:33:12.120
<v Speaker 1>gravity so far, but there's another force at play here,

0:33:12.200 --> 0:33:15.200
<v Speaker 1>and that's dark energy. If it was only gravity, then

0:33:15.240 --> 0:33:18.480
<v Speaker 1>this thing would collapse. Landi Ko would definitely fall into

0:33:18.600 --> 0:33:21.640
<v Speaker 1>one big object and maybe form one super galaxy and

0:33:21.680 --> 0:33:25.280
<v Speaker 1>one super black hole. There is enough gravity if the

0:33:25.360 --> 0:33:28.600
<v Speaker 1>universe wasn't expanding to pull this thing together, like it's

0:33:28.640 --> 0:33:32.480
<v Speaker 1>already right now falling inwards. Everything in the Lanti Kia

0:33:32.560 --> 0:33:36.840
<v Speaker 1>supercluster has an overall in falling velocity. But there's another

0:33:36.840 --> 0:33:39.160
<v Speaker 1>player on this stage, right, which is the expansion of

0:33:39.240 --> 0:33:42.360
<v Speaker 1>the universe, and this has a very different behavior as

0:33:42.400 --> 0:33:45.600
<v Speaker 1>distances grow large, like gravity gets weaker and weaker as

0:33:45.640 --> 0:33:49.160
<v Speaker 1>distances grow large, but dark energy, this accelerating expansion of

0:33:49.160 --> 0:33:52.760
<v Speaker 1>the universe, gets more powerful as distances grow large. So

0:33:52.800 --> 0:33:55.480
<v Speaker 1>at some point it takes over. There's like a crossover

0:33:55.560 --> 0:33:57.560
<v Speaker 1>point where dark energy starts to win.

0:33:57.880 --> 0:33:59.880
<v Speaker 2>Well, let's stick into that to gives that is the

0:34:00.240 --> 0:34:02.360
<v Speaker 2>question of the episode. Now we are in the Lenni

0:34:02.400 --> 0:34:05.600
<v Speaker 2>Kia supercluster, and so the question is is something tearing

0:34:05.720 --> 0:34:09.120
<v Speaker 2>it apart. It's the biggest structure in the universe, and

0:34:09.200 --> 0:34:12.880
<v Speaker 2>so Danny, you're saying that maybe dark energy is tearing

0:34:12.920 --> 0:34:15.800
<v Speaker 2>it apart, or maybe at least fraying it at the edges.

0:34:16.040 --> 0:34:18.600
<v Speaker 1>Yeah, dark energy is definitely working to tear it apart.

0:34:18.719 --> 0:34:20.839
<v Speaker 1>And listeners right in all the time and ask about

0:34:20.920 --> 0:34:24.040
<v Speaker 1>dark energy and have this idea sometimes that dark energy

0:34:24.080 --> 0:34:26.880
<v Speaker 1>is something happening at the edges of the universe, that

0:34:26.920 --> 0:34:29.520
<v Speaker 1>there's something pulling on us from the outside, or that

0:34:29.560 --> 0:34:33.239
<v Speaker 1>maybe the expansion is only happening out there between galaxies,

0:34:33.280 --> 0:34:36.160
<v Speaker 1>but the expansion is happening everywhere. Every chunk of space

0:34:36.320 --> 0:34:39.560
<v Speaker 1>is expanding. Like the Hubble constant is a measure of

0:34:39.600 --> 0:34:43.840
<v Speaker 1>how fast things are expanding, and it's like seventy kilometers

0:34:43.880 --> 0:34:47.040
<v Speaker 1>per second per megaparsek, which is sort of a hard

0:34:47.040 --> 0:34:48.680
<v Speaker 1>thing to get your mind around, but really it just

0:34:48.760 --> 0:34:51.720
<v Speaker 1>means that, like every megaparsec, which is like three light years,

0:34:52.160 --> 0:34:56.280
<v Speaker 1>grows by about seventy kilometers every second, and that happens

0:34:56.280 --> 0:34:59.239
<v Speaker 1>everywhere in space. If you have a smaller distance, like

0:34:59.239 --> 0:35:01.520
<v Speaker 1>the distance between Earth in the Sun, which is only

0:35:01.600 --> 0:35:04.640
<v Speaker 1>a few tens of millions of miles, it would grow

0:35:04.760 --> 0:35:08.520
<v Speaker 1>by a much smaller amount than seventy kilometers every second.

0:35:08.920 --> 0:35:11.040
<v Speaker 1>So that expansion is happening everywhere, but it's sort of

0:35:11.080 --> 0:35:14.800
<v Speaker 1>faint and weak. It's not very strong over short distances,

0:35:14.840 --> 0:35:17.600
<v Speaker 1>and gravity is strong enough to hold us together against

0:35:17.600 --> 0:35:21.080
<v Speaker 1>this like very weak breeze of dark energy. But then

0:35:21.120 --> 0:35:24.360
<v Speaker 1>at large distances, when gravity is weak, dark energy is

0:35:24.400 --> 0:35:26.920
<v Speaker 1>more powerful. It sort of adds up as you get

0:35:26.920 --> 0:35:30.200
<v Speaker 1>to these bigger distances, and so for the supercluster, it

0:35:30.320 --> 0:35:33.839
<v Speaker 1>really is an interesting question of whether that's the crossover point.

0:35:34.200 --> 0:35:37.319
<v Speaker 2>Yeah, it's interesting to think about. Like even here in

0:35:37.360 --> 0:35:40.120
<v Speaker 2>the room where I'm at, and the room where you are,

0:35:40.200 --> 0:35:42.520
<v Speaker 2>and where our listeners are. If you just stare at

0:35:42.560 --> 0:35:45.560
<v Speaker 2>your hand, like the space that your hand is occupying

0:35:45.760 --> 0:35:49.839
<v Speaker 2>is expanding, it's getting trying to like pull your hand

0:35:49.880 --> 0:35:51.680
<v Speaker 2>apart in a way, except that your hand is being

0:35:51.719 --> 0:35:54.360
<v Speaker 2>held together by the bonds of the atoms in it.

0:35:54.400 --> 0:35:56.160
<v Speaker 2>But if it wasn't your hand, which is kind of

0:35:56.160 --> 0:35:57.440
<v Speaker 2>dissipate eventually.

0:35:57.120 --> 0:35:59.759
<v Speaker 1>Right, Yeah, exactly, if there wasn't gravity and there weren't

0:35:59.760 --> 0:36:03.080
<v Speaker 1>those forces, than dark energy would pull your hand apart,

0:36:03.160 --> 0:36:05.200
<v Speaker 1>and it would pull the Earth from the Sun. So

0:36:05.239 --> 0:36:07.520
<v Speaker 1>there's a bunch of really interesting things all happening at

0:36:07.520 --> 0:36:11.520
<v Speaker 1>the same time. Like gravity needs time to form structure.

0:36:12.000 --> 0:36:14.560
<v Speaker 1>You start from like a fuzzy universe, and it gradually

0:36:14.600 --> 0:36:18.080
<v Speaker 1>pulls things together, and so as time goes on, gravity

0:36:18.120 --> 0:36:21.400
<v Speaker 1>makes bigger and bigger and bigger structures. So one reason

0:36:21.440 --> 0:36:24.960
<v Speaker 1>we don't have bigger structures than superclusters, or even if

0:36:25.000 --> 0:36:28.479
<v Speaker 1>superclusters counter structure is just time. Like without dark energy,

0:36:28.480 --> 0:36:31.160
<v Speaker 1>if you ran the universe forward, it would form larger

0:36:31.200 --> 0:36:34.160
<v Speaker 1>and larger and larger structures. But dark energy turned on

0:36:34.239 --> 0:36:37.080
<v Speaker 1>a few billion years ago and it started accelerating the

0:36:37.120 --> 0:36:39.920
<v Speaker 1>expansion of the universe. So gravity is sort of running

0:36:39.960 --> 0:36:43.000
<v Speaker 1>out of time, which means something kind of fascinating. It

0:36:43.040 --> 0:36:45.520
<v Speaker 1>means that we are living maybe at the moment of

0:36:45.560 --> 0:36:48.040
<v Speaker 1>the largest structures in the universe.

0:36:48.360 --> 0:36:50.360
<v Speaker 2>Well, I think that's kind of the point of discussion,

0:36:50.440 --> 0:36:53.600
<v Speaker 2>is like, is dark energy eventually going to tear our

0:36:53.680 --> 0:36:56.719
<v Speaker 2>supercluster apart? Or is maybe that expansion not strong enough

0:36:56.719 --> 0:36:59.520
<v Speaker 2>to really tear apart and keep things the way they

0:36:59.520 --> 0:37:02.640
<v Speaker 2>are forever, Right, that's kind of the question we're asking today.

0:37:02.719 --> 0:37:05.839
<v Speaker 1>Yeah, that's right. But whether or not our supercluster survives,

0:37:05.880 --> 0:37:09.440
<v Speaker 1>there will never be anything bigger in the universe because

0:37:09.520 --> 0:37:12.759
<v Speaker 1>dark energy is getting more and more powerful, and so

0:37:12.880 --> 0:37:16.359
<v Speaker 1>gravity will never have time to make anything bigger. Like

0:37:16.440 --> 0:37:19.480
<v Speaker 1>if a structure hasn't formed by now in the universe,

0:37:19.760 --> 0:37:23.440
<v Speaker 1>it will not because dark energy is just growing in power.

0:37:23.600 --> 0:37:27.399
<v Speaker 1>So whether or not our supercluster survives, nothing bigger than

0:37:27.440 --> 0:37:29.960
<v Speaker 1>anything that's been made already will ever be made.

0:37:30.080 --> 0:37:32.919
<v Speaker 2>Well, let's dig into that and what it might mean

0:37:33.000 --> 0:37:36.880
<v Speaker 2>for our local structure or superstructure of galaxies. Does that

0:37:36.920 --> 0:37:40.040
<v Speaker 2>reduce our chances of getting eaten by aliens? We'll see. First,

0:37:40.120 --> 0:37:55.360
<v Speaker 2>let's take another quick break all right, we're talking about

0:37:55.600 --> 0:37:58.840
<v Speaker 2>getting eaten by aliens. Now, Daniel, are you sort of prepared?

0:37:59.040 --> 0:38:00.759
<v Speaker 2>It sounds like you look forward to it. Now are

0:38:00.800 --> 0:38:02.839
<v Speaker 2>you preparing yourself? Are you staying in shape? Or are

0:38:02.840 --> 0:38:07.160
<v Speaker 2>you trying to fan yourself like like your goose so

0:38:07.160 --> 0:38:09.800
<v Speaker 2>that you're tastier to the aliens? You know, tag on

0:38:09.840 --> 0:38:10.480
<v Speaker 2>those calories.

0:38:11.360 --> 0:38:13.520
<v Speaker 1>I just don't even know, Like what do aliens like?

0:38:13.560 --> 0:38:16.880
<v Speaker 1>How am I supposed to anticipate what they're gonna find? Yummy? Like?

0:38:17.280 --> 0:38:19.440
<v Speaker 1>So I'm just living my life, you know, and hoping

0:38:19.800 --> 0:38:20.839
<v Speaker 1>and hoping that they.

0:38:20.760 --> 0:38:26.279
<v Speaker 2>Put I'm hoping they pick you two over me.

0:38:26.680 --> 0:38:28.640
<v Speaker 1>Hey, something we can agree on. Awesome.

0:38:28.840 --> 0:38:31.879
<v Speaker 2>Well, we're talking about whether we're actually talking about whether

0:38:32.200 --> 0:38:35.640
<v Speaker 2>our supercluster, which is called lanny Kia, which is a

0:38:35.719 --> 0:38:39.120
<v Speaker 2>cluster of galaxy clusters, will one day be torn apart

0:38:39.440 --> 0:38:42.839
<v Speaker 2>because of dark energy. Now, dark energy is expanding all

0:38:42.960 --> 0:38:46.280
<v Speaker 2>space as far as we know, and the question is

0:38:46.280 --> 0:38:49.399
<v Speaker 2>is it expanding space faster than lanny Kiya can hold

0:38:49.440 --> 0:38:52.000
<v Speaker 2>itself together? And it sounds like you have the answer

0:38:52.040 --> 0:38:52.200
<v Speaker 2>to that.

0:38:52.480 --> 0:38:52.799
<v Speaker 3>I do.

0:38:52.960 --> 0:38:57.200
<v Speaker 1>Yeah. So originally they defined a supercluster to be this

0:38:57.400 --> 0:39:00.120
<v Speaker 1>object because everything was sort of falling in towards it.

0:39:00.400 --> 0:39:03.480
<v Speaker 1>That like delineated a blob of stuff that was moving

0:39:03.520 --> 0:39:05.879
<v Speaker 1>towards itself, and the next supercluster is a blob that's

0:39:05.880 --> 0:39:09.080
<v Speaker 1>moving towards itself. But then astronomers thought, hm, that's not

0:39:09.160 --> 0:39:12.240
<v Speaker 1>really enough. Like what we want is something that's gonna survive.

0:39:12.480 --> 0:39:14.680
<v Speaker 1>We wanted to find a supercluster to be something that

0:39:14.880 --> 0:39:18.200
<v Speaker 1>is going to manage to hold itself together against dark energy.

0:39:18.280 --> 0:39:20.720
<v Speaker 1>So they did a bunch of calculations and it looks

0:39:20.840 --> 0:39:23.680
<v Speaker 1>like it's probably not gonna make it. It looks like

0:39:23.760 --> 0:39:27.319
<v Speaker 1>the supercluster is very loosely organized. It's just more like

0:39:27.360 --> 0:39:30.200
<v Speaker 1>a cloud or like a crowd. You know, it happens

0:39:30.200 --> 0:39:33.400
<v Speaker 1>to be nearby, but it's not really like in equilibrium.

0:39:33.480 --> 0:39:35.239
<v Speaker 1>You know, like the Earth and the Sun had a

0:39:35.280 --> 0:39:37.520
<v Speaker 1>lot of time to sort of get in balance and

0:39:37.600 --> 0:39:39.680
<v Speaker 1>find a place where they're happy together, and the Earth

0:39:39.680 --> 0:39:42.960
<v Speaker 1>can orbit forever and be here. But the supercluster, like

0:39:43.000 --> 0:39:45.280
<v Speaker 1>we said earlier, hasn't really had a lot of time

0:39:45.360 --> 0:39:48.840
<v Speaker 1>to gather together and to form something solid. It's just

0:39:48.880 --> 0:39:51.280
<v Speaker 1>sort of like a big blob of stuff that happened

0:39:51.280 --> 0:39:53.600
<v Speaker 1>to be near each other and are starting to fall

0:39:53.640 --> 0:39:56.840
<v Speaker 1>in a little bit but dark energy is powerful enough

0:39:57.040 --> 0:39:59.000
<v Speaker 1>that they're pretty sure it's going to tear it apart.

0:39:59.239 --> 0:40:00.880
<v Speaker 2>Now you mentioned one one of the reasons is that

0:40:00.960 --> 0:40:04.680
<v Speaker 2>dark energy is getting stronger. Now, is it getting stronger

0:40:05.000 --> 0:40:07.719
<v Speaker 2>at the local level or is it just or you're

0:40:07.719 --> 0:40:10.560
<v Speaker 2>saying it's getting stronger because the universe is getting bigger

0:40:10.600 --> 0:40:13.040
<v Speaker 2>and so therefore there's more dark energy. Is it getting

0:40:13.040 --> 0:40:15.600
<v Speaker 2>stronger measureably like inside of my hand, Is this dark

0:40:15.719 --> 0:40:17.440
<v Speaker 2>energy that I would feel over the course of my

0:40:17.480 --> 0:40:20.680
<v Speaker 2>life getting stronger or is it going to be constant?

0:40:21.000 --> 0:40:24.040
<v Speaker 1>Dark energy is everywhere at the same level, so it's

0:40:24.080 --> 0:40:28.640
<v Speaker 1>a constant in space here and there and in other galaxies.

0:40:29.000 --> 0:40:32.760
<v Speaker 1>Every chunk of space has the same amount of dark energy.

0:40:33.160 --> 0:40:36.959
<v Speaker 1>So when the universe expands, it's making more space, which

0:40:37.040 --> 0:40:40.799
<v Speaker 1>means more dark energy doesn't get diluted. It's a constant

0:40:40.920 --> 0:40:44.920
<v Speaker 1>in space. That's not true for other stuff like matter

0:40:45.040 --> 0:40:49.040
<v Speaker 1>or radiation. As the universe expands, matter gets more dilute

0:40:49.120 --> 0:40:52.640
<v Speaker 1>because more space doesn't mean more matter. So as time

0:40:52.719 --> 0:40:55.640
<v Speaker 1>goes on, the expansion of the universe means dark energy

0:40:55.760 --> 0:40:59.319
<v Speaker 1>is constant, But then it's an increasing fraction of the

0:40:59.440 --> 0:41:02.680
<v Speaker 1>energy of the universe because it doesn't get diluted, and

0:41:02.719 --> 0:41:06.280
<v Speaker 1>other stuff does. And when dark energy is an increasing fraction,

0:41:06.400 --> 0:41:10.320
<v Speaker 1>that triggers more expansion, which only tells the balance further

0:41:10.520 --> 0:41:14.120
<v Speaker 1>towards dark energy. So it's like a runaway effect. Once

0:41:14.200 --> 0:41:17.440
<v Speaker 1>dark energy starts to win, which happened about six billion

0:41:17.560 --> 0:41:20.600
<v Speaker 1>years ago, it will zoom ahead and be impossible to

0:41:20.640 --> 0:41:23.600
<v Speaker 1>catch up to. But about seeing it change, we live

0:41:23.760 --> 0:41:26.560
<v Speaker 1>such short lives that we can't really notice it changing

0:41:26.680 --> 0:41:29.799
<v Speaker 1>on our time scales, but we can look back into

0:41:29.840 --> 0:41:32.680
<v Speaker 1>the past by looking out into deep space and seeing

0:41:32.719 --> 0:41:35.120
<v Speaker 1>how things used to be. And of course there's a

0:41:35.200 --> 0:41:38.759
<v Speaker 1>huge asterisk to all of this because we don't really

0:41:38.840 --> 0:41:41.600
<v Speaker 1>understand dark energy and what's going on and what's making

0:41:41.600 --> 0:41:44.320
<v Speaker 1>this happen, and so the rules could be very different

0:41:44.320 --> 0:41:47.239
<v Speaker 1>from this very simple model that honestly we're pretty sure

0:41:47.400 --> 0:41:47.840
<v Speaker 1>is wrong.

0:41:48.160 --> 0:41:50.080
<v Speaker 2>Right, Well, I guess what I mean is that, you know,

0:41:50.160 --> 0:41:52.680
<v Speaker 2>we've always talked about dark energy as being kind of

0:41:52.719 --> 0:41:56.400
<v Speaker 2>the force that's expanding the Universe's expanding space, and I

0:41:56.440 --> 0:41:58.640
<v Speaker 2>always think of it as sort of like the foot

0:41:58.719 --> 0:42:01.920
<v Speaker 2>in the accelerator. Like when I'm driving, I press the

0:42:01.960 --> 0:42:05.000
<v Speaker 2>accelerator and I usually leave it at a certain level

0:42:05.160 --> 0:42:07.840
<v Speaker 2>to keep going at a certain speed, and if I

0:42:07.840 --> 0:42:10.360
<v Speaker 2>want to accelerate go faster, I press it harder, and

0:42:10.400 --> 0:42:12.239
<v Speaker 2>if I want to go slower, I let go of

0:42:12.280 --> 0:42:14.919
<v Speaker 2>the pedal. Now, it sort of seems from what we've

0:42:14.920 --> 0:42:18.400
<v Speaker 2>talked about before that is that, you know, the pedal

0:42:18.440 --> 0:42:21.800
<v Speaker 2>of dark energy is sort of pretty constant. And for example,

0:42:21.840 --> 0:42:23.960
<v Speaker 2>our Solar system is never going to be torn apart

0:42:24.040 --> 0:42:27.160
<v Speaker 2>by dark energy because the gravitational bonds between us and

0:42:27.200 --> 0:42:29.400
<v Speaker 2>the Sun is strong enough that even if the space

0:42:29.480 --> 0:42:32.080
<v Speaker 2>between us gets bigger and bigger and bigger, we're always

0:42:32.120 --> 0:42:33.479
<v Speaker 2>going to hang on to the Sun.

0:42:33.800 --> 0:42:37.000
<v Speaker 1>Dark energy is expanding the space in our Solar system,

0:42:37.080 --> 0:42:39.800
<v Speaker 1>but it doesn't have much effect over those short distances.

0:42:39.840 --> 0:42:43.200
<v Speaker 1>And short distances is when gravity is the most powerful.

0:42:43.560 --> 0:42:46.279
<v Speaker 1>So gravity is always going to be powerful enough to

0:42:46.400 --> 0:42:49.480
<v Speaker 1>hold the Solar system together if dark energy is a

0:42:49.600 --> 0:42:53.319
<v Speaker 1>constant in space. Remember, a constant in space can still

0:42:53.360 --> 0:42:57.560
<v Speaker 1>be an increasing fraction of the universe's energy budget, which

0:42:57.640 --> 0:43:01.680
<v Speaker 1>leads to accelerating expansion even if the dark energy in

0:43:01.760 --> 0:43:04.840
<v Speaker 1>any given chunk of space isn't changing. Except for the

0:43:04.880 --> 0:43:07.880
<v Speaker 1>scenario of the Big Rip, where dark energy gets more

0:43:07.960 --> 0:43:10.600
<v Speaker 1>powerful and even tears our solar system apart and even

0:43:10.600 --> 0:43:13.279
<v Speaker 1>our atoms. But you're right, in our current projection of

0:43:13.360 --> 0:43:16.120
<v Speaker 1>dark energy, it will not tear apart our solar system.

0:43:16.200 --> 0:43:19.919
<v Speaker 2>Right, and so it's because it's not being accelerated enough.

0:43:20.000 --> 0:43:23.040
<v Speaker 2>Now at the level of a galaxy, do we currently

0:43:23.040 --> 0:43:24.920
<v Speaker 2>think that our galaxy is going to be torn apart

0:43:25.320 --> 0:43:25.520
<v Speaker 2>or not?

0:43:25.760 --> 0:43:28.279
<v Speaker 1>We think our galaxy is going to survive, and we

0:43:28.320 --> 0:43:31.760
<v Speaker 1>think our group is going to survive. So everything below

0:43:31.840 --> 0:43:35.200
<v Speaker 1>a supercluster, we're pretty sure gravity is already won and

0:43:35.239 --> 0:43:38.240
<v Speaker 1>it's going to continue to win again, assuming this naive

0:43:38.360 --> 0:43:42.359
<v Speaker 1>projection of dark energy continuing at the same rate that

0:43:42.400 --> 0:43:44.440
<v Speaker 1>it's been continuing, that it's not going to ramp up

0:43:44.480 --> 0:43:47.200
<v Speaker 1>into the big rip or turn around into the big crunch.

0:43:47.680 --> 0:43:50.400
<v Speaker 1>So our solar system will survive, Our galaxy will survive,

0:43:50.480 --> 0:43:54.280
<v Speaker 1>our local group will survive, The Virgo cluster nearby will survive.

0:43:54.480 --> 0:43:58.399
<v Speaker 1>But the question is will our supercluster survive? And that's

0:43:58.480 --> 0:44:01.359
<v Speaker 1>where dark energy starts to win, and dark energy will

0:44:01.400 --> 0:44:05.719
<v Speaker 1>tear these groups of galaxies apart and basically pull apart leni.

0:44:05.520 --> 0:44:08.799
<v Speaker 2>Ka because the things that make up Lenikia, you know,

0:44:09.080 --> 0:44:12.799
<v Speaker 2>our cluster, the Virgo cluster, the Great Attractor, they are

0:44:13.040 --> 0:44:16.839
<v Speaker 2>being attracted to each other, but not more than the

0:44:17.040 --> 0:44:19.759
<v Speaker 2>expansion of the huge amount of space in between them.

0:44:19.800 --> 0:44:20.720
<v Speaker 2>That's kind of what you're saying.

0:44:20.840 --> 0:44:24.120
<v Speaker 1>Yeah, it's just too big, right. Gravity gets weak over

0:44:24.160 --> 0:44:27.040
<v Speaker 1>those huge distances. It does not have the strength to

0:44:27.080 --> 0:44:30.399
<v Speaker 1>overcome dark energy, and as the distances get bigger, dark

0:44:30.520 --> 0:44:33.720
<v Speaker 1>energy becomes harder and harder to surmount. Like, it doesn't

0:44:33.719 --> 0:44:36.680
<v Speaker 1>take that much mass and that much gravity to overcome

0:44:36.760 --> 0:44:39.440
<v Speaker 1>dark energy in our solar system. It takes more mass

0:44:39.440 --> 0:44:42.000
<v Speaker 1>to overcome the dark energy in the galaxy, and even

0:44:42.080 --> 0:44:44.600
<v Speaker 1>more to overcome the dark energy of the group. But

0:44:44.680 --> 0:44:47.640
<v Speaker 1>to overcome the dark energy of the supercluster, we need

0:44:47.640 --> 0:44:51.040
<v Speaker 1>an incredible amount of mass because of the vast distances involved.

0:44:51.600 --> 0:44:54.400
<v Speaker 2>So you're saying that lani Ka, the supercluster of galaxies,

0:44:54.719 --> 0:44:57.719
<v Speaker 2>it's really more like a visual cluster, right, It's more

0:44:57.760 --> 0:45:00.720
<v Speaker 2>of a visual structure. It looks like it's holding together.

0:45:00.760 --> 0:45:02.920
<v Speaker 2>It looks like a wisp of cloud or a crowd

0:45:02.960 --> 0:45:05.920
<v Speaker 2>of people in the park, But really there's nothing that

0:45:06.040 --> 0:45:09.920
<v Speaker 2>much holding it together, or at least proportionally to the

0:45:10.040 --> 0:45:11.280
<v Speaker 2>dark energy in the universe.

0:45:11.400 --> 0:45:14.520
<v Speaker 1>Yeah, our supercluster seems to be right about that turnover

0:45:14.560 --> 0:45:17.600
<v Speaker 1>point where things that are smaller or more massive either

0:45:17.640 --> 0:45:20.960
<v Speaker 1>one would survive, and things that are bigger definitely would not.

0:45:21.640 --> 0:45:23.840
<v Speaker 1>So sort of fascinating. It's like the biggest kind of

0:45:23.840 --> 0:45:26.719
<v Speaker 1>blog we can identify, but it's not really technically a structure.

0:45:26.760 --> 0:45:28.800
<v Speaker 1>So there were some papers a few years ago suggesting

0:45:29.000 --> 0:45:32.160
<v Speaker 1>we shouldn't be calling Lenika a supercluster because it's not

0:45:32.239 --> 0:45:35.319
<v Speaker 1>a structure, And they said, maybe we should redefine what

0:45:35.400 --> 0:45:40.399
<v Speaker 1>a structure is as something that will survive in the future, right,

0:45:40.520 --> 0:45:43.800
<v Speaker 1>things that will hold themselves together in the long term

0:45:44.120 --> 0:45:47.759
<v Speaker 1>after dark energy has played itself out. So by that definition,

0:45:48.000 --> 0:45:51.560
<v Speaker 1>the lani Kaya supercluster is not actually a structure and

0:45:51.560 --> 0:45:53.520
<v Speaker 1>we shouldn't even be calling it a supercluster.

0:45:53.840 --> 0:45:56.239
<v Speaker 2>Well, I mean, as long as you're playing with definitions,

0:45:56.280 --> 0:45:58.719
<v Speaker 2>you can get either way. I feel like, right like

0:45:58.760 --> 0:46:02.000
<v Speaker 2>you could just read a find what a super cluster means.

0:46:02.040 --> 0:46:04.680
<v Speaker 2>A supercluster could just mean like a cloud or a

0:46:04.719 --> 0:46:07.320
<v Speaker 2>crowd in a park. Right, Maybe you can just define

0:46:07.320 --> 0:46:11.680
<v Speaker 2>a supercluster as not necessarily a structure, but you can

0:46:11.680 --> 0:46:14.320
<v Speaker 2>still call it a super cluster, right because a cluster,

0:46:14.560 --> 0:46:16.799
<v Speaker 2>the word cluster just means like, hey, hanging out together.

0:46:16.960 --> 0:46:17.319
<v Speaker 2>M hmm.

0:46:17.400 --> 0:46:20.440
<v Speaker 1>I suppose you could call it a banana if you wanted. Yeah,

0:46:20.560 --> 0:46:22.759
<v Speaker 1>we want these words to have some meaning to them,

0:46:23.320 --> 0:46:25.520
<v Speaker 1>and so these papers suggest that we shouldn't, and they

0:46:25.560 --> 0:46:29.400
<v Speaker 1>actually suggest another name because there are some other superclusters

0:46:29.640 --> 0:46:32.640
<v Speaker 1>that they do think will hold themselves together. So some

0:46:32.719 --> 0:46:36.000
<v Speaker 1>superclusters are more massive or a little bit closer together,

0:46:36.320 --> 0:46:39.239
<v Speaker 1>and they think they will overcome dark energy, and they

0:46:39.280 --> 0:46:43.960
<v Speaker 1>suggest calling these things supersties clusters. Super So what it's

0:46:43.960 --> 0:46:47.320
<v Speaker 1>a word in Latin that means survivor probably not pronouncing

0:46:47.320 --> 0:46:50.000
<v Speaker 1>it correctly, but I think it's superstese clusters. It's the

0:46:50.080 --> 0:46:55.960
<v Speaker 1>new name for superclusters that will survive dark energy.

0:46:57.239 --> 0:47:00.640
<v Speaker 2>It sounds like we're really rather about way for what

0:47:00.719 --> 0:47:02.719
<v Speaker 2>did you say? What did you just call them structures

0:47:02.719 --> 0:47:05.760
<v Speaker 2>like superstructures? Why do we have to go Laddin?

0:47:06.200 --> 0:47:08.960
<v Speaker 1>Well, because you know, not all superclusters are structures. They

0:47:08.960 --> 0:47:11.360
<v Speaker 1>don't hold themselves together. And you're right, we could just

0:47:11.360 --> 0:47:13.960
<v Speaker 1>put a name on things. But we like this hierarchy

0:47:14.000 --> 0:47:16.200
<v Speaker 1>of structures. We like thinking about the universe in terms

0:47:16.200 --> 0:47:18.640
<v Speaker 1>of the structures all the way down from the proton

0:47:18.840 --> 0:47:21.960
<v Speaker 1>zooming out to the biggest structures in the universe. And

0:47:21.960 --> 0:47:24.960
<v Speaker 1>we want a consistency there. We want it to mean something,

0:47:25.000 --> 0:47:27.040
<v Speaker 1>for there to be a structure you don't want just

0:47:27.080 --> 0:47:29.200
<v Speaker 1>like an arbitrary definition at every level.

0:47:29.320 --> 0:47:32.160
<v Speaker 2>Well, I feel like maybe you're only having to adjust

0:47:32.200 --> 0:47:35.719
<v Speaker 2>this definition because of dark energy, right, Like, if it

0:47:35.800 --> 0:47:38.480
<v Speaker 2>wasn't for dark energy, yeah, lenning Care would be a

0:47:38.480 --> 0:47:40.839
<v Speaker 2>structure and it would be gravitational bound and it would

0:47:40.920 --> 0:47:43.360
<v Speaker 2>last until the end of time. But you have dark energy,

0:47:43.440 --> 0:47:47.080
<v Speaker 2>which will make it fuzzy up in the future, except

0:47:47.120 --> 0:47:49.800
<v Speaker 2>that you don't know what dark energy is going to do, right,

0:47:49.960 --> 0:47:53.120
<v Speaker 2>So it seems a little bit like you're rushing ahead

0:47:53.160 --> 0:47:55.520
<v Speaker 2>to redefine everything based on something you don't know what's

0:47:55.560 --> 0:47:56.040
<v Speaker 2>going to happen.

0:47:56.680 --> 0:47:59.880
<v Speaker 1>Well, you know, astronomers love fights over names and definition

0:48:00.120 --> 0:48:02.520
<v Speaker 1>and who gets to name something, so this is one

0:48:02.520 --> 0:48:04.319
<v Speaker 1>of the hot topics these days. But you're right that

0:48:04.360 --> 0:48:06.840
<v Speaker 1>the definition of depends a little bit on what happens

0:48:06.840 --> 0:48:09.440
<v Speaker 1>in the future. In that sense, it's sort of like

0:48:09.520 --> 0:48:11.480
<v Speaker 1>the way you think about an event horizon for a

0:48:11.520 --> 0:48:14.800
<v Speaker 1>black hole, Like the event horizon isn't a physical structure,

0:48:14.960 --> 0:48:18.040
<v Speaker 1>it's just like a delineation that says anything passed here

0:48:18.239 --> 0:48:21.359
<v Speaker 1>in the infinite future will never escape. To really know that,

0:48:21.400 --> 0:48:24.000
<v Speaker 1>you have to see the infinite future. We just sort

0:48:24.040 --> 0:48:26.400
<v Speaker 1>of project it and in the same way, we like

0:48:26.640 --> 0:48:28.520
<v Speaker 1>group this stuff together and say, hey, is this going

0:48:28.600 --> 0:48:30.840
<v Speaker 1>to survive if so that we can call it a

0:48:30.880 --> 0:48:34.280
<v Speaker 1>cluster or a structure or a supercluster or a superstes

0:48:34.440 --> 0:48:38.319
<v Speaker 1>cluster or whatever the astronomers finally settle on. But the

0:48:38.360 --> 0:48:41.799
<v Speaker 1>basic story is that if dark energy continues the way

0:48:41.840 --> 0:48:45.560
<v Speaker 1>it has been, probably Lanikea will just dissolve into a

0:48:45.560 --> 0:48:47.200
<v Speaker 1>bunch of islands of mass.

0:48:47.360 --> 0:48:49.920
<v Speaker 2>It sounds more like you're saying that we shouldn't call

0:48:50.000 --> 0:48:51.560
<v Speaker 2>anything anything until the end of time.

0:48:52.200 --> 0:48:54.719
<v Speaker 1>You go, that's exactly right. We want to be totally

0:48:54.760 --> 0:48:56.680
<v Speaker 1>accurate about everything. We've got to wait to the end

0:48:56.719 --> 0:48:59.440
<v Speaker 1>of the universe. Then we'll know what was going on.

0:49:00.000 --> 0:49:01.799
<v Speaker 2>Well, let's spend the minute here because if we still

0:49:01.800 --> 0:49:04.319
<v Speaker 2>have like a few minutes left here talking about the

0:49:04.440 --> 0:49:06.320
<v Speaker 2>dark energy, right, because it seems like it all depends

0:49:06.320 --> 0:49:08.759
<v Speaker 2>on what dark energy is going to do, whether the

0:49:08.880 --> 0:49:11.440
<v Speaker 2>universe is going to press harder on the accelerator or

0:49:11.480 --> 0:49:14.480
<v Speaker 2>press lower on the accelerator. What's been the history of that,

0:49:14.600 --> 0:49:17.200
<v Speaker 2>Like since the beginning of the universe, there was a

0:49:17.280 --> 0:49:19.719
<v Speaker 2>huge expansion, and then it slowed down and now it's

0:49:19.760 --> 0:49:20.560
<v Speaker 2>picking back up again.

0:49:20.640 --> 0:49:22.480
<v Speaker 1>Right, Yeah, that's true. And there's sort of a bunch

0:49:22.520 --> 0:49:25.120
<v Speaker 1>of different time periods to talk about there, Like there

0:49:25.160 --> 0:49:28.560
<v Speaker 1>was inflation very very early on, huge expansion and very

0:49:28.600 --> 0:49:31.759
<v Speaker 1>short time scales. We don't understand what caused that at all.

0:49:31.800 --> 0:49:34.480
<v Speaker 1>There's a few theories, the insuloton field, whatever, but it's

0:49:34.520 --> 0:49:37.120
<v Speaker 1>a big question mark. And then after that, you know

0:49:37.120 --> 0:49:38.839
<v Speaker 1>what we call the Big Bang, the sort of like

0:49:38.960 --> 0:49:43.160
<v Speaker 1>more gradual expansion of the universe as it cools. We

0:49:43.280 --> 0:49:46.640
<v Speaker 1>have pretty good models of that. We have gravity, and

0:49:46.680 --> 0:49:49.000
<v Speaker 1>we have dark energy, we have all the other forces

0:49:49.040 --> 0:49:51.719
<v Speaker 1>that come into play, and in that period we can

0:49:51.760 --> 0:49:54.799
<v Speaker 1>model dark energy as constant, saying like a chunk of

0:49:54.840 --> 0:49:57.400
<v Speaker 1>space has the same amount of potential energy, and that

0:49:57.480 --> 0:50:01.360
<v Speaker 1>creates this repulsive field in general relative which drives the

0:50:01.400 --> 0:50:04.600
<v Speaker 1>expansion of the universe. Remember that dark energy can be

0:50:04.640 --> 0:50:07.680
<v Speaker 1>a constant in space, every chunk has the same amount,

0:50:07.880 --> 0:50:11.520
<v Speaker 1>but still be a growing fraction of the universe's energy

0:50:11.680 --> 0:50:15.200
<v Speaker 1>because other stuff is getting diluted as things expand, So

0:50:15.320 --> 0:50:19.200
<v Speaker 1>dark energy is both constant and taking over as other

0:50:19.280 --> 0:50:23.279
<v Speaker 1>things get more dilute. It's not exactly true, because we

0:50:23.320 --> 0:50:26.320
<v Speaker 1>make these measurements over time we get slightly different answers,

0:50:26.719 --> 0:50:29.080
<v Speaker 1>so nobody really knows if that's true or it needs

0:50:29.080 --> 0:50:31.040
<v Speaker 1>a little bit of adjusting. We had a whole episode

0:50:31.080 --> 0:50:34.400
<v Speaker 1>about early dark energy, whether dark energy was more powerful

0:50:34.440 --> 0:50:37.200
<v Speaker 1>early on, this kind of stuff. But mostly we can

0:50:37.239 --> 0:50:41.040
<v Speaker 1>explain the history of the universe after that first inflationary period.

0:50:41.200 --> 0:50:44.440
<v Speaker 1>We can explain it assuming dark energy is constant, So

0:50:44.480 --> 0:50:46.800
<v Speaker 1>that seems to be a reasonable assumption.

0:50:46.520 --> 0:50:49.160
<v Speaker 2>Meaning that the universe is not pressing the accelerator faster,

0:50:49.520 --> 0:50:50.759
<v Speaker 2>it's just kind of leaving it on.

0:50:51.160 --> 0:50:53.880
<v Speaker 1>That's right. It's pressing the accelerator at the same level,

0:50:54.160 --> 0:50:56.480
<v Speaker 1>meaning every part of space has the same amount of

0:50:56.560 --> 0:51:00.400
<v Speaker 1>dark energy. But eventually that does take over. When you

0:51:00.440 --> 0:51:03.200
<v Speaker 1>press the accelerator on your car. There are other things

0:51:03.280 --> 0:51:06.040
<v Speaker 1>keeping you from going faster and faster, right, there's friction

0:51:06.200 --> 0:51:08.840
<v Speaker 1>and this AerR, resistance whatever. That doesn't quite apply to

0:51:08.880 --> 0:51:10.920
<v Speaker 1>this model because in this model, the level that the

0:51:10.960 --> 0:51:13.640
<v Speaker 1>accelerator is at ends up speeding us up. It's like

0:51:13.760 --> 0:51:17.640
<v Speaker 1>winning against the other forces. So it really is accelerating

0:51:17.680 --> 0:51:20.320
<v Speaker 1>the expansion of the universe. So sort of two different

0:51:20.320 --> 0:51:22.719
<v Speaker 1>ideas there. One is the amount of dark energy in

0:51:22.760 --> 0:51:26.960
<v Speaker 1>space is constant, but because it overcomes the other things,

0:51:27.200 --> 0:51:30.719
<v Speaker 1>it ends up accelerating the expansion of the universe.

0:51:30.680 --> 0:51:34.799
<v Speaker 2>Meaning that the space is growing at an accelerated rate.

0:51:34.920 --> 0:51:38.680
<v Speaker 2>But is that acceleration getting faster or is it slowing down?

0:51:38.880 --> 0:51:40.160
<v Speaker 2>Or is it pretty constant.

0:51:40.320 --> 0:51:43.640
<v Speaker 1>We think that acceleration itself is pretty constant, yes, and

0:51:43.680 --> 0:51:45.600
<v Speaker 1>we can track that back through the history of the

0:51:45.680 --> 0:51:47.960
<v Speaker 1>universe and see if that explains our history, and it

0:51:48.040 --> 0:51:51.000
<v Speaker 1>mostly does. Again, there's some questions there about their early

0:51:51.040 --> 0:51:53.840
<v Speaker 1>first few bits you might have read about, like different

0:51:53.880 --> 0:51:57.080
<v Speaker 1>measurements of the Hubble constant that we can't quite reconcile.

0:51:57.160 --> 0:51:59.200
<v Speaker 1>And that's what that's about. Is that level of acceleration

0:51:59.320 --> 0:52:01.600
<v Speaker 1>the same all the way through time or.

0:52:01.520 --> 0:52:02.799
<v Speaker 2>Not it is it or not?

0:52:02.960 --> 0:52:05.120
<v Speaker 1>We think that it is, but we don't quite know

0:52:05.239 --> 0:52:07.320
<v Speaker 1>that these measurements that we can't quite reconcile.

0:52:08.000 --> 0:52:09.919
<v Speaker 2>I guess it's kind of the difference of whether dark

0:52:10.040 --> 0:52:13.240
<v Speaker 2>energy is a constant, like a number in your equations

0:52:13.239 --> 0:52:15.640
<v Speaker 2>of the universe, or is it a variable that somehow

0:52:15.719 --> 0:52:18.680
<v Speaker 2>feeds in it itself or that maybe has a little

0:52:18.680 --> 0:52:21.480
<v Speaker 2>button that you know, the makers of the universe are

0:52:22.640 --> 0:52:23.840
<v Speaker 2>increasing exactly.

0:52:23.960 --> 0:52:26.400
<v Speaker 1>Yeah, right, now, we can describe it just using a number.

0:52:26.640 --> 0:52:29.560
<v Speaker 1>It's a cosmological constant. We don't know where that number

0:52:29.600 --> 0:52:31.440
<v Speaker 1>comes from or why it is what it is. We

0:52:31.480 --> 0:52:33.800
<v Speaker 1>have really no explanation for it. But we can mostly

0:52:33.840 --> 0:52:36.400
<v Speaker 1>describe the history of the universe using just a number

0:52:36.640 --> 0:52:37.520
<v Speaker 1>for dark energy.

0:52:37.760 --> 0:52:39.600
<v Speaker 2>All right, Well, it sounds like the answer to the

0:52:39.680 --> 0:52:43.040
<v Speaker 2>question of the episode is yes. It sounds like, as

0:52:43.080 --> 0:52:45.160
<v Speaker 2>far as we know, if things stay the same with

0:52:45.280 --> 0:52:49.040
<v Speaker 2>dark energy, are super cluster of galaxies that we live

0:52:49.040 --> 0:52:52.360
<v Speaker 2>in will be torn apart sometime in the future.

0:52:52.640 --> 0:52:56.120
<v Speaker 1>That's right. So our more immedia cosmic neighborhood is safe

0:52:56.160 --> 0:52:59.560
<v Speaker 1>and probably will eventually collapse into a black hole, but

0:52:59.680 --> 0:53:03.560
<v Speaker 1>the cluster will not be in our neighborhood forever. Dark

0:53:03.640 --> 0:53:06.240
<v Speaker 1>energy will take over and pull us apart from it.

0:53:06.239 --> 0:53:09.360
<v Speaker 2>It's going to be declustered, but we won't know, I

0:53:09.360 --> 0:53:10.560
<v Speaker 2>guess until the end of time.

0:53:10.760 --> 0:53:13.480
<v Speaker 1>That's right. So we'll do our five millionth episode at

0:53:13.480 --> 0:53:15.920
<v Speaker 1>the end of time, and we'll answer this question definitively.

0:53:16.440 --> 0:53:19.560
<v Speaker 2>So maybe I shouldn't call you a person, Daniel, because eventually,

0:53:19.560 --> 0:53:21.840
<v Speaker 2>who knows, maybe aliens will come and tear you apart.

0:53:22.360 --> 0:53:24.040
<v Speaker 2>We just have to wait and see before we call

0:53:24.080 --> 0:53:24.600
<v Speaker 2>you a person.

0:53:24.760 --> 0:53:26.440
<v Speaker 1>That's true. From that point of view, none of us

0:53:26.440 --> 0:53:27.040
<v Speaker 1>are structured.

0:53:27.920 --> 0:53:31.120
<v Speaker 2>We could all be lunch in our future, hey, fellow,

0:53:31.200 --> 0:53:32.759
<v Speaker 2>lunch meat.

0:53:32.840 --> 0:53:35.120
<v Speaker 1>Ashes to ashes, dust to lunch.

0:53:35.120 --> 0:53:38.799
<v Speaker 2>And lunch to something else once the aliens digest us.

0:53:39.760 --> 0:53:44.480
<v Speaker 2>All right, well, pretty interesting lesson to think about, not

0:53:44.640 --> 0:53:47.160
<v Speaker 2>just like our place in the universe and how small

0:53:47.160 --> 0:53:50.600
<v Speaker 2>we are compared to these enormous clusters of galaxies, but

0:53:50.640 --> 0:53:53.880
<v Speaker 2>also about the permanence of the universe. Like even something

0:53:54.040 --> 0:53:57.080
<v Speaker 2>as huge as a super cluster Lenni Kia, it may

0:53:57.120 --> 0:53:59.320
<v Speaker 2>not be around for the entire life of the universe.

0:53:59.400 --> 0:54:03.760
<v Speaker 1>That's right. Think about these incredibly powerful, vast forces at play,

0:54:03.840 --> 0:54:08.360
<v Speaker 1>tugging on these galaxies with millions and billions of stars,

0:54:08.760 --> 0:54:11.400
<v Speaker 1>all in a battle against dark energy. It's really a

0:54:11.480 --> 0:54:13.960
<v Speaker 1>very dynamical place. If you think about the universe and

0:54:14.000 --> 0:54:17.719
<v Speaker 1>sort of fast forward, it's slashing, it's frothen it's doing

0:54:17.840 --> 0:54:18.200
<v Speaker 1>a lot.

0:54:18.520 --> 0:54:20.960
<v Speaker 2>All right. We hope you enjoyed that. Thanks for joining us,

0:54:22.000 --> 0:54:22.719
<v Speaker 2>See you next time.

0:54:30.600 --> 0:54:33.400
<v Speaker 1>Thanks for listening, and remember that Daniel and Jorge Explain

0:54:33.480 --> 0:54:36.719
<v Speaker 1>the Universe is a production of iHeart Radio. For more

0:54:36.800 --> 0:54:41.640
<v Speaker 1>podcasts from iHeartRadio, visit the iHeartRadio, ap Apple podcasts, or

0:54:41.680 --> 0:54:43.920
<v Speaker 1>wherever you listen to your favorite shows.