WEBVTT - Supervoids

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<v Speaker 1>When you look out into the night sky on a

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<v Speaker 1>camping trip, you're seeing the best view in the universe.

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<v Speaker 1>Much better than standing on a mountain top or on

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<v Speaker 1>the top floor of a building. Stretching over zillions of

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<v Speaker 1>light years of cosmic space, you're seeing entire stars and

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<v Speaker 1>galaxies across this black ocean. It's amazing. But there's something

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<v Speaker 1>else for you to see up there, for us to

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<v Speaker 1>learn about. The empty bits. Between the galaxies stretch huge

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<v Speaker 1>regions without all that flashy, glowy stuff. How is that

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<v Speaker 1>all arranged? What is the map of galaxies in the universe?

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<v Speaker 1>And what does that tell us about how the universe

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<v Speaker 1>forms and the forces that shape it? Today in the pod,

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<v Speaker 1>we're digging into the biggest maps we can make of

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<v Speaker 1>the biggest stuff and the biggest non-stuff in the universe.

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<v Speaker 1>Welcome to Daniel and Kelly's Extraordinary Mostly Empty Universe.

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<v Speaker 2>Hello, I'm Kelly Wienersmith.

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<v Speaker 3>I study parasites and space, and super void sounds like

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<v Speaker 3>a sort of gothy concept, so 16-year-old Kelly is totally

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<v Speaker 3>into it.

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<v Speaker 1>Hi, I'm Daniel. I'm a particle physicist who likes to

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<v Speaker 1>think about aliens, and I'm about 0% goth. So when

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<v Speaker 1>I hear super void, I don't think black lipstick. I

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<v Speaker 1>think Marvel characters.

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<v Speaker 2>Oh, all right.

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<v Speaker 3>Well, so Super Voids does make me think of gothy stuff,

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<v Speaker 3>which reminds me of some of my favorite gothy characters,

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<v Speaker 3>which are Frankenfurter from the Rocky.

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<v Speaker 2>Horror Picture Show.

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<v Speaker 1>Yes. R.I.P. Tim Curry.

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<v Speaker 2>Exactly. And the devil in Legend, which, yes.

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<v Speaker 3>So my question for you today is, what was Tim

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<v Speaker 3>Curry's best role and why is it the saddest thing

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<v Speaker 3>in the whole world that Tim Curry is gone?

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<v Speaker 1>Okay.

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<v Speaker 2>Because it's the saddest thing in the world that Tim

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<v Speaker 2>Curry is gone.

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<v Speaker 1>It is sad. He was wonderful. I loved him in Clue. Oh.

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<v Speaker 1>You know, the hilarious movie. Wonderful. And I love a mystery.

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<v Speaker 1>You know, for me, science is the biggest mystery in

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<v Speaker 1>the universe. How does this all work? Who caused the

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<v Speaker 1>ripples in the primordial plasma? You know, was it the

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<v Speaker 1>butler with the candlestick in the early universe? Who knows?

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<v Speaker 2>You are so good at keeping us on track.

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<v Speaker 1>I'm doing my best here. Oh, my gosh. This car

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<v Speaker 1>is going off into the weeds of Virginia.

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<v Speaker 3>I just needed a moment to like vent and feel

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<v Speaker 3>seen because I am just devastated about the loss of

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<v Speaker 3>Tim Curry.

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<v Speaker 1>Would you say that the loss of Tim Curry creates

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<v Speaker 1>a void in your heart?

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<v Speaker 2>A super void, Daniel. And so, and my heart is

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<v Speaker 2>now cold and empty.

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<v Speaker 3>And let's go ahead and change the subject before I

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<v Speaker 3>get too emotional here and dig into super voids.

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<v Speaker 2>Why are we talking about super voids today?

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<v Speaker 1>We're talking about supervoids because they're super awesome. They're fascinating.

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<v Speaker 1>They're one of the biggest things or non-things in the universe.

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<v Speaker 1>They tell us so much about its history, about its future,

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<v Speaker 1>about its formation, about how it works. And it's so

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<v Speaker 1>hard to get them in your mind because they give

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<v Speaker 1>you a sense of scale of the universe, you know?

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<v Speaker 1>how tiny, how small, how insignificant we are, and yet

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<v Speaker 1>how we can cast our minds to understanding the largest

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<v Speaker 1>scale structures in the universe, which stretch across billions and

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<v Speaker 1>zillions of light years. It's super awesome to think about

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<v Speaker 1>super voids. And I'm not the only one who thinks so.

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<v Speaker 1>We got a request from two listeners, Levi and Nathan,

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<v Speaker 1>who wrote and said, hey, would you tell us why

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<v Speaker 1>the universe has super voids. So that's why we're talking

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<v Speaker 1>about super voids specifically today.

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<v Speaker 3>Well, and I noted in that email that Levi also

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<v Speaker 3>says he enjoys my poop jokes. And so this is

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<v Speaker 3>a family that gets our podcast.

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<v Speaker 1>Exactly. And we'll try to make as many poo jokes

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<v Speaker 1>as we can in today's episode, just for you, Levi.

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<v Speaker 3>I am trying to connect super voids to poo jokes.

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<v Speaker 3>And the only thing I can think about is the

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<v Speaker 3>prep for a colonoscopy. You are super voided at that point.

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<v Speaker 3>But probably that joke's over Levi's head because Levi's a

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<v Speaker 3>little bit younger, isn't he?

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<v Speaker 2>Yeah.

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<v Speaker 1>Yes, exactly. But maybe Levi thinks about super voids every

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<v Speaker 1>time he's voiding himself.

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<v Speaker 2>Okay. Well, good.

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<v Speaker 1>Look it.

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<v Speaker 2>We did it. We did it. We got the poop

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<v Speaker 2>jokes in there.

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<v Speaker 3>Yes.

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<v Speaker 1>And, you know, a really important thing for understanding super

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<v Speaker 1>voids and the structure of the universe is, is dark matter,

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<v Speaker 1>which is its own poo joke right there.

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<v Speaker 3>Oh, man, I love the work we do together, Daniel.

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<v Speaker 2>It's the best.

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<v Speaker 1>We are out here doing hard-hitting science. No, really, we

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<v Speaker 1>are proving that it's possible to do deep dives into

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<v Speaker 1>science and also make poo jokes. That is our niche

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<v Speaker 1>in the SciComm community. That's right. But before we tell

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<v Speaker 1>you what we think about super voids and dig into

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<v Speaker 1>the cosmic history that created them and our confusion about them...

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<v Speaker 1>I wondered what the extraordinaries thought about why the universe

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<v Speaker 1>has super voids. So I reached out to our group

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<v Speaker 1>of volunteers, which you are very, very welcome to join.

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<v Speaker 1>Just write to us to questions at danielandkelly.org and you

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<v Speaker 1>can join this crew. In the meantime, think about it

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<v Speaker 1>for a minute. Why do you think the universe has

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<v Speaker 1>super voids?

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<v Speaker 2>The universe is expanding and the amount of stuff in

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<v Speaker 2>it is not increasing.

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<v Speaker 1>So we can fight all of those dastardly dark energy

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<v Speaker 1>and dark matter criminals. Initial randomness allowed some parts to

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<v Speaker 1>get denser and presumably some parts to get a lot sparser.

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<v Speaker 1>It's for the same reason that my gravy has lumps

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<v Speaker 1>in it. I don't know what that reason is, but

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<v Speaker 1>I think it's the same reason. Collects in some places,

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<v Speaker 1>then it has to clear out in others.

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<v Speaker 2>I think it has to do with the way matter

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<v Speaker 2>was created during the Big Bang.

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<v Speaker 1>I would guess some astronomers saw some very cold or

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<v Speaker 1>empty patch in space and could not avoid to give

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<v Speaker 1>it a super name.

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<v Speaker 2>Does not have to be uniform. I have no idea

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<v Speaker 2>what a super void is. Is it like a really,

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<v Speaker 2>really big void? Because of dark matter. A void is

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<v Speaker 2>just void.

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<v Speaker 1>Because of dark matter.

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<v Speaker 2>It's because of dark matter.

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<v Speaker 1>Yeah.

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<v Speaker 2>We're confused.

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<v Speaker 1>Help us.

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<v Speaker 2>Oh, my gosh. I love the answers.

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<v Speaker 3>Astronomers saw an empty patch and couldn't avoid giving it

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<v Speaker 3>a super name.

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<v Speaker 2>You are my new best friend.

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<v Speaker 1>That's got everything you love, right? It's got a pun.

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<v Speaker 1>It's got a dig against astronomers.

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<v Speaker 3>I feel like it implies that astronomers give things good names.

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<v Speaker 2>Oh, maybe they do. No, no, they don't, actually. What

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<v Speaker 2>is it?

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<v Speaker 3>The rings around Saturn or Jupiter or like A, B, C,

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<v Speaker 3>and D or.

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<v Speaker 1>Yeah, exactly. The solar system is a disaster. Even beyond

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<v Speaker 1>planets and dwarf planets, you've got like centaurs and meteors

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<v Speaker 1>and all sorts of stuff. It's a mess.

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<v Speaker 2>It's a mess.

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<v Speaker 3>But we are here to clear up confusion. And so

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<v Speaker 3>let's jump right in. Daniel, what the heck is the

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<v Speaker 3>super void?

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<v Speaker 1>So to understand super voids, we first have to understand

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<v Speaker 1>our cosmic context, like the structure of the universe around us.

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<v Speaker 1>So let's start here in California or Virginia. California, by

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<v Speaker 1>the way, feeling more like Virginia these days, you know,

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<v Speaker 1>because it's like stinky and humid and gross and like,

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<v Speaker 1>where do I even live anymore, man?

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<v Speaker 3>I see that your handle on Riverside today is humidity hater.

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<v Speaker 3>This is really living rent free in your brain. I'm

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<v Speaker 3>not a humidity fan either.

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<v Speaker 1>I mean, since we're putting ourselves in the cosmic context,

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<v Speaker 1>it's important to note that Los Angeles yesterday was the

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<v Speaker 1>most humid place in the country, which is breaking all

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<v Speaker 1>the rules, if you ask me.

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<v Speaker 2>That does not seem fair.

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<v Speaker 1>Anyway, zoom out from the sticky issues here on planet Earth.

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<v Speaker 1>And of course, we have our solar system. And the

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<v Speaker 1>sun is just one of hundreds of billions of stars

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<v Speaker 1>in the Milky Way swirling around in roughly a disk.

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<v Speaker 1>And then our galaxy is not just one of zillions

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<v Speaker 1>scattered through the universe. Galaxies themselves cluster. So we have

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<v Speaker 1>the local cluster of galaxies, a bunch of galaxies that

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<v Speaker 1>are gravitationally bound together, which doesn't mean that there's like

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<v Speaker 1>some big object in the center around which everything is

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<v Speaker 1>orbiting the way it is in the solar system. But

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<v Speaker 1>it does mean that there is a center of mass

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<v Speaker 1>of the local cluster and everything is swirling around that.

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<v Speaker 2>Okay, I'm with you.

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<v Speaker 1>All right, so we have clusters. And now clusters organize

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<v Speaker 1>into superclusters, right? Astronomers, great names. And superclusters are not

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<v Speaker 1>always gravitationally bound. They're like near each other in that

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<v Speaker 1>you can look at them and say, oh, these clusters

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<v Speaker 1>are near each other. But it's not clear whether gravity

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<v Speaker 1>is strong enough to hold them together. Because remember, the

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<v Speaker 1>universe is expanding. It's creating new space between everything. And

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<v Speaker 1>that includes new space between California and Virginia, new space

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<v Speaker 1>between Earth and the Sun, new space between the Sun

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<v Speaker 1>and the center of the Milky Way. But because there's

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<v Speaker 1>enough gravity to hold the Earth together and hold the

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<v Speaker 1>Sun to the Earth and hold the Sun to the

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<v Speaker 1>rest of the galaxy, those distances are not increasing. So

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<v Speaker 1>the expansion of the universe is losing to gravity. But

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<v Speaker 1>gravity gets weaker as distances get greater. So when you

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<v Speaker 1>get to super voids, dark energy is starting to get

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<v Speaker 1>powerful enough that it's going to overcome gravity. And that's

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<v Speaker 1>right about the cutoff. So we don't think that all

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<v Speaker 1>superclusters are technically objects in the sense that they're not

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<v Speaker 1>gravitationally bound. We think that as time goes on, they

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<v Speaker 1>probably will get pulled apart. But they're still sort of

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<v Speaker 1>objects in the sense that they're near each other. And

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<v Speaker 1>if you looked at them on a map, you'd probably

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<v Speaker 1>draw a circle around them.

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<v Speaker 2>Okay. That doesn't sound void-y.

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<v Speaker 1>No, we're not at the voids yet. Okay. But now

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<v Speaker 1>we've already zoomed out incredibly, right? Like from the Earth

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<v Speaker 1>to the Sun to the galaxy to like clusters of

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<v Speaker 1>galaxies to now super clusters of galaxies. It might feel

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<v Speaker 1>like this is the biggest thing you could ever have

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<v Speaker 1>in your head. Okay, now collapse all those super clusters

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<v Speaker 1>down to a point because now we're going to zoom

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<v Speaker 1>out so far that structure inside a super cluster is irrelevant.

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<v Speaker 1>We're just going to treat each super cluster like a

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<v Speaker 1>dot and we're going to ask, How are the superclusters

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<v Speaker 1>organized across the universe? And they're not organized evenly. It's

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<v Speaker 1>not like somebody sprinkled sand across the universe, each one

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<v Speaker 1>being a supercluster. Instead, they form filaments. They form walls.

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<v Speaker 1>They form bubbles. So there are sheets and filaments of superclusters.

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<v Speaker 1>And inside those bubbles are the voids. That's where there

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<v Speaker 1>are fewer galaxies and fewer superclusters. And so imagine like

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<v Speaker 1>a foam, right? Where super clusters lie on the edges

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<v Speaker 1>of the bubbles and inside the bubbles, there's comparatively less.

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<v Speaker 3>All right, so my brain is now wondering why you

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<v Speaker 3>can't get super voids on the outsides of the bubbles too.

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<v Speaker 3>Am I just letting this analogy get stuck in my

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<v Speaker 3>head too much?

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<v Speaker 1>There is no outside to the bubbles. The universe is

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<v Speaker 1>filled with these bubbles.

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<v Speaker 3>Oh.

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<v Speaker 1>Yes, the bubbles are everywhere. The universe is just bubbles.

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<v Speaker 1>And it's the foam fills the whole universe. And everywhere

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<v Speaker 1>you have a bubble edge where the bubbles meet, that's

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<v Speaker 1>where you have superclusters, walls, sheets of superclusters. And inside,

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<v Speaker 1>those are the voids.

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<v Speaker 2>Whoa, okay.

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<v Speaker 1>Yeah.

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<v Speaker 3>Are they totally empty or just less empty than the

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<v Speaker 3>outside of the bubble?

0:11:33.559 --> 0:11:36.319
<v Speaker 1>Yeah, great question. They're not completely empty, right? It's a

0:11:36.440 --> 0:11:39.319
<v Speaker 1>relative density. So we measure the density of stuff in

0:11:39.340 --> 0:11:42.820
<v Speaker 1>the universe and we say anything less than like 10%

0:11:42.820 --> 0:11:46.200
<v Speaker 1>of the mean density, we call that a void. And

0:11:46.240 --> 0:11:49.959
<v Speaker 1>these things are pretty big. They have diameters like 10

0:11:49.960 --> 0:11:55.700
<v Speaker 1>to 100 megaparsecs, which is like 300 million light years across.

0:11:56.040 --> 0:11:58.370
<v Speaker 1>Oh my gosh. These are vast structures. And these are

0:11:58.410 --> 0:12:02.349
<v Speaker 1>not super voids. These are just voids. These are just normal, everyday,

0:12:02.390 --> 0:12:06.810
<v Speaker 1>run-of-the-mill voids. Already, these things are much, much bigger than

0:12:07.030 --> 0:12:10.620
<v Speaker 1>one individual supercluster relative to To a void, a supercluster

0:12:10.750 --> 0:12:12.589
<v Speaker 1>is so tiny you just think of it as a dot.

0:12:12.870 --> 0:12:16.030
<v Speaker 1>And remember, inside that supercluster is a bunch of clusters

0:12:16.070 --> 0:12:19.209
<v Speaker 1>of galaxies, and inside each cluster of galaxies is a

0:12:19.230 --> 0:12:22.410
<v Speaker 1>bunch of galaxies, each of which is unfathomably huge to

0:12:22.429 --> 0:12:25.370
<v Speaker 1>the human mind. So this is like a real brain

0:12:25.410 --> 0:12:28.150
<v Speaker 1>stretcher to even get this in your head, what a

0:12:28.210 --> 0:12:29.800
<v Speaker 1>supervoid is and how big it is.

0:12:30.250 --> 0:12:31.070
<v Speaker 2>Yeah, I was.

0:12:31.210 --> 0:12:34.610
<v Speaker 3>So you said 30 to 300 million light years. And

0:12:34.630 --> 0:12:36.429
<v Speaker 3>I was still having a little trouble wrapping my head

0:12:36.450 --> 0:12:37.790
<v Speaker 3>around that number.

0:12:38.090 --> 0:12:38.850
<v Speaker 2>So I just looked it up.

0:12:38.870 --> 0:12:43.830
<v Speaker 3>The distance between our galaxy and Andromeda is 2.5 million

0:12:43.870 --> 0:12:46.910
<v Speaker 3>light years away. So we are talking about voids that

0:12:46.970 --> 0:12:50.620
<v Speaker 3>are like, I don't know, 15 times bigger than that minimum.

0:12:51.540 --> 0:12:52.920
<v Speaker 2>That is huge.

0:12:53.020 --> 0:12:55.020
<v Speaker 1>Yeah. And, you know, the size of our galaxy is

0:12:55.040 --> 0:12:58.939
<v Speaker 1>like 100,000 light years across. And so if you can

0:12:59.059 --> 0:13:02.949
<v Speaker 1>somehow get the Milky Way into your brain, then we're

0:13:02.990 --> 0:13:06.309
<v Speaker 1>talking about distances that are thousands of times bigger than

0:13:06.350 --> 0:13:07.030
<v Speaker 1>the Milky Way.

0:13:07.130 --> 0:13:07.709
<v Speaker 2>Oh, my gosh.

0:13:07.770 --> 0:13:11.850
<v Speaker 1>And so, yeah, these are big, empty regions of space. Wow.

0:13:12.010 --> 0:13:13.319
<v Speaker 2>We should put something in there.

0:13:17.500 --> 0:13:19.420
<v Speaker 1>I mean, I know your house is filled to the

0:13:19.480 --> 0:13:23.059
<v Speaker 1>brim with all kinds of Interesting stuff. And so you're

0:13:23.100 --> 0:13:24.819
<v Speaker 1>always looking for more storage space.

0:13:25.040 --> 0:13:26.599
<v Speaker 3>I was thinking we could put all the stuff in

0:13:26.640 --> 0:13:29.100
<v Speaker 3>my house into the super void so that I don't have,

0:13:29.160 --> 0:13:31.719
<v Speaker 3>but I think Zach might fill the super void pretty quick.

0:13:34.059 --> 0:13:35.100
<v Speaker 2>With Dorito bags.

0:13:37.200 --> 0:13:39.000
<v Speaker 1>Not just Dorito bags, but you know, you've got all

0:13:39.040 --> 0:13:42.170
<v Speaker 1>these projects. They're always half done. You're like, I'm storing

0:13:42.190 --> 0:13:44.150
<v Speaker 1>all these cabinets in this room because I can't put

0:13:44.190 --> 0:13:46.349
<v Speaker 1>them on the wall yet. They're on the wall now.

0:13:46.370 --> 0:13:46.970
<v Speaker 2>Do you imagine?

0:13:48.400 --> 0:13:50.540
<v Speaker 1>Do you imagine someday in the future you will be

0:13:50.559 --> 0:13:52.439
<v Speaker 1>done with projects and the house will just be like

0:13:52.880 --> 0:13:54.040
<v Speaker 1>actually totally functional?

0:13:54.520 --> 0:13:54.870
<v Speaker 2>No.

0:13:55.370 --> 0:13:58.170
<v Speaker 1>No? No. She says with resignation.

0:13:58.490 --> 0:14:00.670
<v Speaker 2>I don't know when I'll have time to finish everything.

0:14:01.770 --> 0:14:02.770
<v Speaker 2>Maybe when I die.

0:14:03.610 --> 0:14:05.650
<v Speaker 1>All right. Well, maybe your house never will have voids.

0:14:05.730 --> 0:14:08.170
<v Speaker 1>It's always going to be filled with stuff. But the

0:14:08.250 --> 0:14:11.460
<v Speaker 1>universe has voids and they're fascinating. And they were kind

0:14:11.480 --> 0:14:14.460
<v Speaker 1>of a surprise when we learned that the universe had

0:14:14.500 --> 0:14:15.059
<v Speaker 1>this structure.

0:14:15.480 --> 0:14:16.100
<v Speaker 2>So why?

0:14:16.120 --> 0:14:20.760
<v Speaker 3>OK, so if I'm like imagining a giant space, I

0:14:20.800 --> 0:14:24.350
<v Speaker 3>would imagine that if you like distributed stuff around that space,

0:14:24.370 --> 0:14:26.670
<v Speaker 3>you would expect there to be some empty areas for

0:14:26.750 --> 0:14:30.230
<v Speaker 3>random reasons. But you've I think you've already explained to

0:14:30.310 --> 0:14:32.810
<v Speaker 3>us that these voids aren't random because they tend to

0:14:32.830 --> 0:14:35.050
<v Speaker 3>be on the inside of like bubbles. Does that tell

0:14:35.110 --> 0:14:36.330
<v Speaker 3>us something about how they're formed?

0:14:37.050 --> 0:14:39.080
<v Speaker 1>It does tell us something about how they're formed. And

0:14:39.100 --> 0:14:41.620
<v Speaker 1>you put your finger on exactly what the discovery was.

0:14:42.250 --> 0:14:45.770
<v Speaker 1>Until around the 70s, we thought that galaxies were distributed

0:14:45.850 --> 0:14:49.050
<v Speaker 1>roughly equally. That, you know, any galaxy had an equal

0:14:49.090 --> 0:14:51.190
<v Speaker 1>chance to be here or there. And if you took

0:14:51.330 --> 0:14:53.910
<v Speaker 1>any chunk of space, you would find roughly the same

0:14:53.980 --> 0:14:57.600
<v Speaker 1>number of galaxies. You know, that the density was pretty smooth.

0:14:58.140 --> 0:15:00.320
<v Speaker 1>And it wasn't until the 70s that they went out

0:15:00.340 --> 0:15:02.440
<v Speaker 1>and they started measuring these things and trying to map

0:15:02.660 --> 0:15:05.300
<v Speaker 1>out the structure of the universe. You know, I love

0:15:05.320 --> 0:15:07.200
<v Speaker 1>when we have an idea about how the universe works.

0:15:07.540 --> 0:15:09.880
<v Speaker 1>And then we develop the technology, the capacity to actually

0:15:09.940 --> 0:15:12.930
<v Speaker 1>measure it. And the universe is like, no, what you

0:15:12.950 --> 0:15:15.570
<v Speaker 1>thought was natural, what you thought was intuitive, what you

0:15:15.590 --> 0:15:18.770
<v Speaker 1>thought made sense. That's not how things work. Because those

0:15:18.790 --> 0:15:20.340
<v Speaker 1>are the best moments. Those are the moments when the

0:15:20.390 --> 0:15:24.280
<v Speaker 1>universe is confronting your intuition and teaching you something about

0:15:24.320 --> 0:15:26.840
<v Speaker 1>how things work. I mean, not like the universe is

0:15:26.880 --> 0:15:29.160
<v Speaker 1>a teacher, you know, that cares what we understand. But

0:15:29.440 --> 0:15:32.240
<v Speaker 1>those are the best moments of discovery. And it was

0:15:32.280 --> 0:15:35.620
<v Speaker 1>in the 70s that people first started measuring red shifts

0:15:35.750 --> 0:15:38.390
<v Speaker 1>of these galaxies and trying to assemble them into sort

0:15:38.410 --> 0:15:40.890
<v Speaker 1>of a 3D map. What you need to understand the

0:15:40.930 --> 0:15:43.620
<v Speaker 1>structure of the universe is to know where is a galaxy?

0:15:43.960 --> 0:15:46.380
<v Speaker 1>How far away is it? If you know those two things,

0:15:46.440 --> 0:15:48.740
<v Speaker 1>you can start to build a 3D map of where

0:15:48.760 --> 0:15:51.000
<v Speaker 1>all the galaxies are and you can start to see structure.

0:15:51.620 --> 0:15:54.380
<v Speaker 1>And so people started doing this seriously in the 70s.

0:15:54.990 --> 0:15:57.730
<v Speaker 1>The Center for Astrophysics at Harvard and the Smithsonian started

0:15:57.770 --> 0:16:01.450
<v Speaker 1>to do this with the Tillinghast Telescope. And they were surprised.

0:16:01.930 --> 0:16:05.460
<v Speaker 1>They surveyed like 2,200 galaxies. And they saw that things

0:16:05.500 --> 0:16:07.980
<v Speaker 1>were not smooth, right? It didn't look like galaxies were

0:16:08.020 --> 0:16:12.220
<v Speaker 1>distributed randomly across the universe. They were clustered together into

0:16:12.280 --> 0:16:15.020
<v Speaker 1>these bubbles. Imagine a sheet of paper and you throw

0:16:15.060 --> 0:16:17.380
<v Speaker 1>sand over it and you expect there, as you said,

0:16:17.420 --> 0:16:19.500
<v Speaker 1>to be some places where there are galaxies and some

0:16:19.520 --> 0:16:20.930
<v Speaker 1>places where there are not. It's not going to be

0:16:21.330 --> 0:16:23.730
<v Speaker 1>perfectly smooth. You don't expect the galaxies to be like

0:16:24.110 --> 0:16:27.730
<v Speaker 1>in a grid, you know, perfectly arranged. There'd be some

0:16:27.790 --> 0:16:31.610
<v Speaker 1>clustering accidentally. But what they saw was definite structure, not

0:16:31.670 --> 0:16:34.980
<v Speaker 1>just random distributions. they saw like a bubble bath of

0:16:35.060 --> 0:16:37.860
<v Speaker 1>cosmic voids and filaments. And they discovered what they call

0:16:38.100 --> 0:16:42.740
<v Speaker 1>the Great Wall, a superstructure over 500 million light years wide.

0:16:43.320 --> 0:16:45.200
<v Speaker 1>And what a moment, you know, to be the first

0:16:45.260 --> 0:16:50.340
<v Speaker 1>person to map the universe, right? Like I always imagined...

0:16:50.340 --> 0:16:52.680
<v Speaker 1>The joy of being like a first person to land

0:16:52.820 --> 0:16:55.530
<v Speaker 1>on a new shore or to cross a land bridge or,

0:16:55.550 --> 0:16:57.830
<v Speaker 1>you know, get in a boat 10,000 years ago and

0:16:57.870 --> 0:17:01.010
<v Speaker 1>cross the Pacific to the South Pacific islands or whatever, right?

0:17:01.350 --> 0:17:03.550
<v Speaker 1>What a moment of discovery. But this is just on

0:17:03.610 --> 0:17:06.850
<v Speaker 1>another scale, you know? This is like, oh my gosh,

0:17:06.890 --> 0:17:09.929
<v Speaker 1>the universe has patterns and we're part of this and

0:17:09.950 --> 0:17:12.380
<v Speaker 1>there's a huge wall over there. And like, oh my God,

0:17:12.760 --> 0:17:15.000
<v Speaker 1>what a moment. And, you know, I think that's sort

0:17:15.020 --> 0:17:17.320
<v Speaker 1>of natural for us to think about now because we've

0:17:17.359 --> 0:17:19.859
<v Speaker 1>known about it for 50 years. But at the time,

0:17:19.940 --> 0:17:22.200
<v Speaker 1>this was a real revolution in the way people thought

0:17:22.300 --> 0:17:26.660
<v Speaker 1>about our entire cosmic context. So that was very cool,

0:17:26.680 --> 0:17:29.260
<v Speaker 1>and that was in the 70s. And again, the primary

0:17:29.320 --> 0:17:30.879
<v Speaker 1>way we figured this out is that we look at

0:17:30.920 --> 0:17:34.700
<v Speaker 1>galaxies and we measure their redshift, meaning that the light

0:17:34.740 --> 0:17:37.719
<v Speaker 1>that comes from them has been shifted to lower frequencies.

0:17:38.500 --> 0:17:40.879
<v Speaker 1>And we measure their redshift, which tells us how the

0:17:40.920 --> 0:17:43.140
<v Speaker 1>light has been shifted, which tells us how fast they're

0:17:43.160 --> 0:17:45.939
<v Speaker 1>moving away from us. Because remember, the things that are

0:17:45.980 --> 0:17:48.970
<v Speaker 1>moving away from us have their light shifted into the red.

0:17:49.880 --> 0:17:51.919
<v Speaker 1>And if we know how fast they're moving away from us,

0:17:51.960 --> 0:17:54.300
<v Speaker 1>then we can tell how far away they are because

0:17:54.320 --> 0:17:56.500
<v Speaker 1>that's the Hubble relationship. It tells us that things that

0:17:56.540 --> 0:17:59.540
<v Speaker 1>are further away are moving away faster. So if you

0:17:59.580 --> 0:18:01.879
<v Speaker 1>just measure the light from one of these galaxies, you

0:18:01.900 --> 0:18:05.060
<v Speaker 1>measure the redshift, you say, I know where hydrogen should be.

0:18:05.180 --> 0:18:07.659
<v Speaker 1>I know where helium should be on my spectrum. And

0:18:07.700 --> 0:18:10.260
<v Speaker 1>I see it shifted. You measure that shift. You can

0:18:10.320 --> 0:18:13.500
<v Speaker 1>translate that to the distance to the galaxies. And now

0:18:13.560 --> 0:18:15.399
<v Speaker 1>you know the angle in the sky, right? You know,

0:18:15.420 --> 0:18:17.320
<v Speaker 1>I saw this galaxy at this angle. I saw that

0:18:17.359 --> 0:18:19.879
<v Speaker 1>galaxy at the other angle. You put those together and

0:18:19.920 --> 0:18:22.290
<v Speaker 1>you start to make your 3D map of the universe.

0:18:22.869 --> 0:18:23.350
<v Speaker 3>Amazing.

0:18:23.400 --> 0:18:27.030
<v Speaker 2>Okay, so now we know what the pattern is. Let's

0:18:27.070 --> 0:18:27.629
<v Speaker 2>take a break.

0:18:27.670 --> 0:18:29.310
<v Speaker 3>And when we come back, we'll talk about now that

0:18:29.350 --> 0:18:31.510
<v Speaker 3>we know what the pattern is, what does that imply

0:18:31.609 --> 0:18:34.429
<v Speaker 3>about how everything ended up where it finally ended up?

0:18:54.369 --> 0:18:57.310
<v Speaker 2>And we're back. We've been talking about how.

0:18:57.050 --> 0:19:01.580
<v Speaker 3>Like the universe is like this foamy wash full of

0:19:01.700 --> 0:19:04.280
<v Speaker 3>clusters that are like on the edges of the bubbles.

0:19:04.660 --> 0:19:07.080
<v Speaker 3>And then inside of the bubbles, we have super voids.

0:19:07.800 --> 0:19:11.350
<v Speaker 3>What does that tell us about how the universe formed?

0:19:11.790 --> 0:19:13.270
<v Speaker 3>And like, have we figured that out yet? Because that's

0:19:13.290 --> 0:19:14.050
<v Speaker 3>not what we expected.

0:19:14.470 --> 0:19:18.250
<v Speaker 1>Right, yeah. So first, slight clarification. Inside the bubbles are voids.

0:19:18.450 --> 0:19:18.790
<v Speaker 2>Oh, okay.

0:19:18.830 --> 0:19:21.680
<v Speaker 1>Super voids we haven't really talked about exactly yet. Super

0:19:21.700 --> 0:19:25.379
<v Speaker 1>voids are essentially like really, really big voids. In many cases,

0:19:25.500 --> 0:19:27.980
<v Speaker 1>bigger than we expect. And so that's why we have

0:19:28.000 --> 0:19:29.720
<v Speaker 1>to dive into the history of the universe to think

0:19:29.740 --> 0:19:31.879
<v Speaker 1>about like, do we expect to see voids? Do we

0:19:31.940 --> 0:19:34.620
<v Speaker 1>expect to see super voids? Does what we see line

0:19:34.660 --> 0:19:36.659
<v Speaker 1>up with what we expect? And to do that, we

0:19:36.680 --> 0:19:38.699
<v Speaker 1>have to go all the way back to the earliest

0:19:38.740 --> 0:19:39.880
<v Speaker 1>known thing in the universe.

0:19:40.270 --> 0:19:40.850
<v Speaker 2>Which is?

0:19:41.310 --> 0:19:44.100
<v Speaker 1>The cosmic microwave background, of course, which, you know, physics

0:19:44.150 --> 0:19:46.239
<v Speaker 1>is always going back to. You might be like, oh,

0:19:46.260 --> 0:19:48.610
<v Speaker 1>my gosh, these guys lean on the CMB so much.

0:19:48.710 --> 0:19:52.670
<v Speaker 1>It's just such a. rich and incredible source of information.

0:19:52.730 --> 0:19:55.190
<v Speaker 1>You know, if you were trying to understand somebody's life

0:19:55.609 --> 0:19:57.930
<v Speaker 1>and you had like a picture of them in kindergarten,

0:19:58.390 --> 0:20:00.430
<v Speaker 1>it would tell you so much about where they grew

0:20:00.570 --> 0:20:02.730
<v Speaker 1>up and what they were like. And that's basically what

0:20:02.770 --> 0:20:07.440
<v Speaker 1>we have. We And so when we want to understand

0:20:07.500 --> 0:20:09.179
<v Speaker 1>how the universe got to be the way it is,

0:20:09.220 --> 0:20:11.100
<v Speaker 1>we look back at that baby picture. We're like, huh,

0:20:11.320 --> 0:20:13.399
<v Speaker 1>did it have seven toes when it was born? Or

0:20:13.440 --> 0:20:16.680
<v Speaker 1>was that surgery that came later? You know, what features

0:20:16.720 --> 0:20:18.980
<v Speaker 1>of the universe can you trace back to the origin?

0:20:19.040 --> 0:20:21.080
<v Speaker 1>And if they're not there, what does that tell you?

0:20:21.180 --> 0:20:24.050
<v Speaker 1>So it's incredibly valuable. And that's why we look back.

0:20:24.590 --> 0:20:26.290
<v Speaker 1>And for those of you who don't remember, the cosmic

0:20:26.330 --> 0:20:29.690
<v Speaker 1>microwave background light is light that came from the universe

0:20:29.730 --> 0:20:32.659
<v Speaker 1>the first moment that it was transparent. So we don't

0:20:32.680 --> 0:20:34.699
<v Speaker 1>know how the universe began or when it began, but

0:20:34.720 --> 0:20:36.960
<v Speaker 1>we do know that it was filled with a hot,

0:20:37.160 --> 0:20:40.100
<v Speaker 1>dense plasma and that plasma was glowing and it was opaque.

0:20:40.440 --> 0:20:42.060
<v Speaker 1>Just like plasma at the center of the sun, it

0:20:42.359 --> 0:20:45.520
<v Speaker 1>gives off light and then is immediately reabsorbed. Which, you know,

0:20:45.580 --> 0:20:49.300
<v Speaker 1>you hear maybe on pop-sci channels like a photon takes

0:20:49.300 --> 0:20:50.720
<v Speaker 1>50,000 years to get from the center of the sun

0:20:50.780 --> 0:20:52.700
<v Speaker 1>to the surface of the sun. And that's like mostly

0:20:52.720 --> 0:20:56.300
<v Speaker 1>pop-sci nonsense. because a photon is emitted at the center

0:20:56.320 --> 0:20:58.220
<v Speaker 1>of the sun and then immediately absorbed. It never gets

0:20:58.260 --> 0:21:01.440
<v Speaker 1>to the surface. Like, you know, maybe you could say

0:21:01.480 --> 0:21:03.880
<v Speaker 1>that heat waves travel through the sun at some velocity

0:21:03.900 --> 0:21:07.640
<v Speaker 1>or whatever, but you're not tracing a photon. Anyway, photons

0:21:07.660 --> 0:21:10.179
<v Speaker 1>that were created in the very early universe, no longer around,

0:21:10.400 --> 0:21:14.119
<v Speaker 1>immediately absorbed because the universe they were born into was opaque.

0:21:14.609 --> 0:21:17.130
<v Speaker 1>But the universe is expanding and the universe is cooling.

0:21:17.470 --> 0:21:19.970
<v Speaker 1>And at some point, the universe expanded and cooled enough

0:21:20.310 --> 0:21:23.909
<v Speaker 1>that protons and electrons found each other and became neutral.

0:21:24.330 --> 0:21:28.669
<v Speaker 1>And then the universe became suddenly transparent. So photons that

0:21:28.690 --> 0:21:31.930
<v Speaker 1>were born after that moment are still around. And they

0:21:31.970 --> 0:21:34.210
<v Speaker 1>are still here for us to measure and for us

0:21:34.230 --> 0:21:36.970
<v Speaker 1>to learn about the early universe. And what we see

0:21:37.030 --> 0:21:41.690
<v Speaker 1>in those photons is not a smooth plasma. Not like

0:21:41.880 --> 0:21:44.660
<v Speaker 1>everything was filled with stuff equally. We see some places

0:21:44.700 --> 0:21:47.200
<v Speaker 1>with more density and some places with less density.

0:21:47.730 --> 0:21:51.480
<v Speaker 3>And that is not what we expected initially. And why

0:21:51.580 --> 0:21:53.720
<v Speaker 3>is that not what we expected initially?

0:21:54.060 --> 0:21:56.820
<v Speaker 1>Yeah, good question. Here we have like two threads we

0:21:56.859 --> 0:22:01.139
<v Speaker 1>have to follow. One is the density of galaxies as

0:22:01.180 --> 0:22:04.190
<v Speaker 1>we're seeing them like today. And that started in the 70s.

0:22:05.170 --> 0:22:08.090
<v Speaker 1>And by the 70s, we had seen the cosmic microwave

0:22:08.130 --> 0:22:09.990
<v Speaker 1>background light. That happened in the 60s. It was a

0:22:10.320 --> 0:22:13.500
<v Speaker 1>huge confirmation that the universe had an early hot, dense state.

0:22:13.780 --> 0:22:16.420
<v Speaker 1>But we had not yet seen its wiggles. It wasn't

0:22:16.480 --> 0:22:18.879
<v Speaker 1>until like the 80s and the 90s that we measured

0:22:18.920 --> 0:22:22.219
<v Speaker 1>the CMB light with enough precision to see, oh, there

0:22:22.260 --> 0:22:24.100
<v Speaker 1>are some little hot spots and there are some little

0:22:24.160 --> 0:22:27.690
<v Speaker 1>cold spots. It just seemed sort of smooth. And so

0:22:27.750 --> 0:22:29.710
<v Speaker 1>it wasn't until later that we saw wiggles in the

0:22:29.750 --> 0:22:33.420
<v Speaker 1>CMB and we saw structure in the universe. And you're

0:22:33.460 --> 0:22:35.280
<v Speaker 1>right to ask about that because those two things are

0:22:35.300 --> 0:22:37.970
<v Speaker 1>definitely connected. And the listener who made that connection is

0:22:38.010 --> 0:22:41.609
<v Speaker 1>totally right. We think that all the structure in the

0:22:41.670 --> 0:22:44.890
<v Speaker 1>current universe comes from that structure in the early universe.

0:22:45.390 --> 0:22:47.830
<v Speaker 1>That you had places with more density and that had

0:22:47.869 --> 0:22:50.690
<v Speaker 1>more gravity and that pulled in more stuff. And that

0:22:50.880 --> 0:22:53.480
<v Speaker 1>in those regions, you now have more galaxies and more

0:22:53.540 --> 0:22:56.500
<v Speaker 1>dark matter than in places where you didn't. And so

0:22:56.520 --> 0:22:58.700
<v Speaker 1>you should be able to line up a place in

0:22:58.720 --> 0:23:01.520
<v Speaker 1>the early universe where there was less dense stuff with

0:23:01.640 --> 0:23:02.500
<v Speaker 1>voids today.

0:23:02.869 --> 0:23:03.720
<v Speaker 2>Okay, got it.

0:23:03.950 --> 0:23:06.090
<v Speaker 1>And you might be tempted to say, oh, well, can

0:23:06.130 --> 0:23:09.850
<v Speaker 1>we trace an individual like hotspot or cold spot in

0:23:09.869 --> 0:23:14.359
<v Speaker 1>the CMB to something in the universe today? And you

0:23:14.380 --> 0:23:17.000
<v Speaker 1>might be preparing yourself for disappointment because usually the answer

0:23:17.020 --> 0:23:19.460
<v Speaker 1>to that is no. We can just do it statistically.

0:23:19.500 --> 0:23:22.480
<v Speaker 1>We can say, oh, we expect this kind of distribution

0:23:22.520 --> 0:23:25.959
<v Speaker 1>of galaxies in the late universe based on this kind

0:23:26.000 --> 0:23:28.310
<v Speaker 1>of density in the early universe. But we can't say

0:23:28.350 --> 0:23:32.040
<v Speaker 1>like this photon caused that galaxy or whatever, right? But

0:23:32.200 --> 0:23:34.720
<v Speaker 1>there is one feature that seems to correlate.

0:23:34.740 --> 0:23:35.300
<v Speaker 2>What?

0:23:35.320 --> 0:23:38.100
<v Speaker 1>So there's a feature in the early universe, the cosmic

0:23:38.140 --> 0:23:41.240
<v Speaker 1>microwave background, that seems to line up with a super

0:23:41.280 --> 0:23:44.760
<v Speaker 1>void in the universe. Yeah. So the feature in the

0:23:44.780 --> 0:23:48.720
<v Speaker 1>cosmic microwave background is called the CMB cold spot. This

0:23:48.790 --> 0:23:52.429
<v Speaker 1>is a region where it's redder than everywhere else. So

0:23:52.470 --> 0:23:55.190
<v Speaker 1>we expect there to be some variations in the cosmic

0:23:55.230 --> 0:23:59.510
<v Speaker 1>microwave background. They vary by like microkelvin. And we talk

0:23:59.550 --> 0:24:01.950
<v Speaker 1>about the CMB in terms of temperature, which is equivalent

0:24:01.970 --> 0:24:05.750
<v Speaker 1>to thinking about wavelength, because blackbody radiation rules tell us

0:24:05.869 --> 0:24:07.990
<v Speaker 1>that something at a certain temperature will radiate at a

0:24:08.010 --> 0:24:11.020
<v Speaker 1>certain wavelength. So when we measure light at a certain wavelength,

0:24:11.040 --> 0:24:13.100
<v Speaker 1>we say, oh, that came from an object at a

0:24:13.119 --> 0:24:16.540
<v Speaker 1>certain temperature. So for example, the CMB light came from

0:24:16.580 --> 0:24:19.420
<v Speaker 1>a really hot plasma, thousands and thousands of degrees, I

0:24:19.500 --> 0:24:22.720
<v Speaker 1>think 3,000 K. But that light has been redshifted by

0:24:22.770 --> 0:24:25.050
<v Speaker 1>the expansion of the universe down to about 2.7 K.

0:24:25.090 --> 0:24:27.950
<v Speaker 1>So if you read that like oh, the CMB light

0:24:28.210 --> 0:24:30.129
<v Speaker 1>is 2.7K, that's what it means. It means that it's

0:24:30.170 --> 0:24:33.450
<v Speaker 1>the wavelength that an object at 2.7 Kelvin would emit.

0:24:33.730 --> 0:24:37.540
<v Speaker 1>So very, very cold light. And we see variations like

0:24:37.540 --> 0:24:41.760
<v Speaker 1>20 microkelvin in the CMB. That's like typical expected hot

0:24:41.800 --> 0:24:44.260
<v Speaker 1>spots and cold spots. But there is one spot in

0:24:44.300 --> 0:24:46.360
<v Speaker 1>the CMB, one spot in the sky when we look

0:24:46.420 --> 0:24:50.860
<v Speaker 1>at it, that it's like 70 microkelvin colder. So some

0:24:50.900 --> 0:24:55.340
<v Speaker 1>places like 150 microK colder. It's in the southern hemisphere

0:24:55.700 --> 0:24:59.400
<v Speaker 1>in the direction of the constellation Eridanus, which is maybe

0:24:59.480 --> 0:25:01.320
<v Speaker 1>the source of a poop joke for those of you

0:25:01.780 --> 0:25:04.180
<v Speaker 1>who are interested in the southern hemisphere.

0:25:04.480 --> 0:25:07.450
<v Speaker 3>If you could see how it's spelled, you would get

0:25:07.490 --> 0:25:08.730
<v Speaker 3>why this could be a poop joke.

0:25:09.850 --> 0:25:13.290
<v Speaker 1>Maybe all constellations in the southern hemisphere should have anus

0:25:13.330 --> 0:25:14.970
<v Speaker 1>in them, you know? Absolutely.

0:25:14.990 --> 0:25:15.410
<v Speaker 2>Yes.

0:25:16.150 --> 0:25:17.430
<v Speaker 1>Astronomers, get on that.

0:25:17.590 --> 0:25:20.659
<v Speaker 2>Or synonyms of anus. Yes. Because you need some options.

0:25:21.000 --> 0:25:23.940
<v Speaker 1>Yeah. So this is really interesting. You know, it could

0:25:24.000 --> 0:25:27.060
<v Speaker 1>just be random. It could just be like a fluctuation.

0:25:27.240 --> 0:25:29.650
<v Speaker 1>And they've done a calculation to suggest it's like, there's

0:25:29.690 --> 0:25:33.409
<v Speaker 1>like a 1.5% chance of this happening randomly. So it's

0:25:33.470 --> 0:25:37.450
<v Speaker 1>like weird. It sticks out, but it's not insane. But

0:25:37.510 --> 0:25:41.609
<v Speaker 1>it does also correspond with a place in the late

0:25:41.750 --> 0:25:45.010
<v Speaker 1>universe that there seems to be a super void.

0:25:45.490 --> 0:25:48.150
<v Speaker 3>And you said at one point, well, we haven't really

0:25:48.190 --> 0:25:49.370
<v Speaker 3>talked about super voids yet.

0:25:49.470 --> 0:25:52.540
<v Speaker 2>And super voids are just like Really big voids, right?

0:25:52.900 --> 0:25:55.880
<v Speaker 1>Yes, exactly. Okay. And so if you look in the

0:25:55.960 --> 0:25:59.730
<v Speaker 1>structure of the universe today, in the same direction, you

0:25:59.830 --> 0:26:03.630
<v Speaker 1>do see a really, really big void there. It's like

0:26:03.650 --> 0:26:07.250
<v Speaker 1>a thousand times the size of a typical void. Wow.

0:26:07.290 --> 0:26:09.649
<v Speaker 1>So it's like you have bubbles in your sink and

0:26:09.670 --> 0:26:11.730
<v Speaker 1>they're all roughly the same size. And then there's one

0:26:11.770 --> 0:26:14.270
<v Speaker 1>that's just like a thousand times bigger than all the

0:26:14.390 --> 0:26:18.070
<v Speaker 1>other bubbles. This one's a billion light years across. It's

0:26:18.090 --> 0:26:20.130
<v Speaker 1>like five to 10 billion light years away.

0:26:20.770 --> 0:26:23.650
<v Speaker 3>So is this like most mornings you eat Special K,

0:26:24.070 --> 0:26:26.250
<v Speaker 3>but one morning you eat Poops Like a Champion?

0:26:26.270 --> 0:26:29.429
<v Speaker 2>And that's the difference between void and super void?

0:26:29.450 --> 0:26:36.780
<v Speaker 1>Yes, exactly. You feel it about 24 hours later, exactly,

0:26:36.820 --> 0:26:39.700
<v Speaker 1>when you have a super void. And here the universe

0:26:39.920 --> 0:26:41.500
<v Speaker 1>has formed a void like a champion.

0:26:41.520 --> 0:26:44.649
<v Speaker 3>And just to be clear, Poops Like a Champion... Is

0:26:44.670 --> 0:26:46.700
<v Speaker 3>an actual cereal you told me about the other day.

0:26:48.080 --> 0:26:50.000
<v Speaker 1>It is an actual cereal and we have boxes of

0:26:50.040 --> 0:26:53.550
<v Speaker 1>it at home. Because some company out there that makes

0:26:53.630 --> 0:26:56.899
<v Speaker 1>it heard about Katrina and her fiber journey and her,

0:26:57.750 --> 0:27:00.229
<v Speaker 1>you know, her effort to make everybody poop better by

0:27:00.320 --> 0:27:03.360
<v Speaker 1>eating fiber and improve their gut microbiome. So they sent

0:27:03.380 --> 0:27:05.619
<v Speaker 1>her a bunch of free boxes of poop like a champion.

0:27:06.260 --> 0:27:08.500
<v Speaker 1>And I am not on their payroll, so I can

0:27:08.540 --> 0:27:10.220
<v Speaker 1>tell you that it tastes like cardboard.

0:27:11.480 --> 0:27:13.440
<v Speaker 3>But still, you know, I think Katrina is one of

0:27:13.500 --> 0:27:14.740
<v Speaker 3>the better people on this planet.

0:27:16.050 --> 0:27:17.350
<v Speaker 2>That's what that story tells me.

0:27:18.170 --> 0:27:21.350
<v Speaker 1>She's out there. She really does want to improve your pooping. Yeah.

0:27:21.390 --> 0:27:23.260
<v Speaker 1>Even though she has nothing to do with super voids.

0:27:23.710 --> 0:27:26.420
<v Speaker 3>I tried really hard to derail this conversation.

0:27:26.480 --> 0:27:29.600
<v Speaker 2>Let's go back to super voids of the universe.

0:27:30.020 --> 0:27:33.280
<v Speaker 1>Yeah. So this is really interesting because when you run

0:27:33.300 --> 0:27:36.220
<v Speaker 1>the simulations in the universe, you don't get these kinds

0:27:36.260 --> 0:27:39.679
<v Speaker 1>of super voids. Like it's really unusual. And so it

0:27:39.720 --> 0:27:42.380
<v Speaker 1>helps us try to understand, like, you know, we talked

0:27:42.400 --> 0:27:46.000
<v Speaker 1>about in our simulating the universe episode recently that, How

0:27:46.020 --> 0:27:48.379
<v Speaker 1>when you see something different in your simulation and in

0:27:48.420 --> 0:27:50.720
<v Speaker 1>your data, it tells you that there's a gap. There's

0:27:50.740 --> 0:27:54.000
<v Speaker 1>something in your simulation that isn't describing the universe correctly,

0:27:54.060 --> 0:27:56.389
<v Speaker 1>or there's an element of the universe that you're not

0:27:56.430 --> 0:28:00.190
<v Speaker 1>describing correctly. And these are super fascinating, especially because they're

0:28:00.230 --> 0:28:04.130
<v Speaker 1>very sensitive to the expansion of the universe. How we

0:28:04.170 --> 0:28:06.490
<v Speaker 1>see these cold spots and these hot spots in the

0:28:06.590 --> 0:28:09.530
<v Speaker 1>CMB tells us a lot about the expansion of the

0:28:09.609 --> 0:28:13.480
<v Speaker 1>universe because photons fly through the universe as they get

0:28:13.540 --> 0:28:16.730
<v Speaker 1>to us. And there's two different effects here to disentangle.

0:28:16.750 --> 0:28:18.790
<v Speaker 1>When we're looking at the CMB and we see some

0:28:18.830 --> 0:28:22.410
<v Speaker 1>places are hotter, some places are colder, there's two different

0:28:22.430 --> 0:28:25.300
<v Speaker 1>reasons why. One is, well, we could just be looking

0:28:25.359 --> 0:28:28.140
<v Speaker 1>at a place that was denser or it was less dense.

0:28:28.520 --> 0:28:31.899
<v Speaker 1>And so there's like initial over-density or initial under-density. That's

0:28:31.920 --> 0:28:34.780
<v Speaker 1>what we typically think about. But remember that the photons

0:28:34.859 --> 0:28:37.679
<v Speaker 1>also have to fly through the universe to get to us.

0:28:38.340 --> 0:28:43.390
<v Speaker 1>And those photons are red-shifted by the expansion of the universe. And...

0:28:43.580 --> 0:28:46.060
<v Speaker 1>they fly through the universe, which means that they're sensitive

0:28:46.440 --> 0:28:49.940
<v Speaker 1>to gravitational density. Because if you fly through a region

0:28:49.960 --> 0:28:53.070
<v Speaker 1>with a lot of mass, you get redshifted, right? Like

0:28:53.150 --> 0:28:57.350
<v Speaker 1>black holes produce gravitational redshifts. And so a photon that's

0:28:57.430 --> 0:29:01.230
<v Speaker 1>flown through the universe, in some senses, measures the density

0:29:01.250 --> 0:29:04.690
<v Speaker 1>of the universe along its path. which is super duper cool.

0:29:04.910 --> 0:29:07.890
<v Speaker 3>That is super duper cool. That photo from our childhood

0:29:08.010 --> 0:29:10.290
<v Speaker 3>is telling us a lot. Although is it more like,

0:29:10.310 --> 0:29:12.330
<v Speaker 3>I mean, you should never really dig into an analogy,

0:29:12.350 --> 0:29:15.270
<v Speaker 3>but it's more like a video from your childhood, isn't it,

0:29:15.350 --> 0:29:15.990
<v Speaker 3>than a photo?

0:29:16.880 --> 0:29:19.060
<v Speaker 1>It is like a video because if you keep watching it,

0:29:19.140 --> 0:29:21.520
<v Speaker 1>you see different things, right? We are looking at the

0:29:21.560 --> 0:29:24.220
<v Speaker 1>cosmic microwave background radiation and we can't see it for

0:29:24.240 --> 0:29:27.080
<v Speaker 1>the whole universe. We see the light that's arriving right now,

0:29:27.700 --> 0:29:30.370
<v Speaker 1>which left, of course, many, many, many billions of years ago.

0:29:31.000 --> 0:29:33.700
<v Speaker 1>And it's arriving to us from a shell of that

0:29:33.790 --> 0:29:37.150
<v Speaker 1>original plasma that's very far away and around the Earth.

0:29:37.450 --> 0:29:39.470
<v Speaker 1>And as time goes on, we get light from a

0:29:39.530 --> 0:29:42.230
<v Speaker 1>different shell. So it's not like we're watching the same

0:29:42.310 --> 0:29:46.150
<v Speaker 1>place over time. Over time, we're scanning more and more

0:29:46.260 --> 0:29:49.920
<v Speaker 1>distant shells of that original CMB. Got it. Cool. So

0:29:49.940 --> 0:29:52.320
<v Speaker 1>let's trace the trajectory of a photon as it's moving

0:29:52.340 --> 0:29:56.200
<v Speaker 1>through the universe. And let's think first about overdensities, places

0:29:56.240 --> 0:29:59.020
<v Speaker 1>where there's a lot of mass. So say a photon

0:29:59.060 --> 0:30:01.300
<v Speaker 1>is on its way to us, but it's passing by

0:30:01.500 --> 0:30:05.420
<v Speaker 1>a black hole, right? And so as it falls in

0:30:05.480 --> 0:30:08.160
<v Speaker 1>towards the black hole, it gains energy, right? So it's

0:30:08.180 --> 0:30:11.090
<v Speaker 1>getting blue shifted. And then if it doesn't get eaten

0:30:11.130 --> 0:30:12.790
<v Speaker 1>by the black hole, it makes it out and it

0:30:12.830 --> 0:30:15.330
<v Speaker 1>comes towards us. And as it's leaving the black hole,

0:30:15.390 --> 0:30:17.550
<v Speaker 1>it's losing energy. It's having to climb out of that

0:30:17.590 --> 0:30:20.490
<v Speaker 1>gravitational well. So it gets red shifted. And so you

0:30:20.510 --> 0:30:24.120
<v Speaker 1>might think, okay, blue shifted more energy, red shifted less energy.

0:30:24.400 --> 0:30:27.150
<v Speaker 1>It all balances out. So how could a photon that's

0:30:27.210 --> 0:30:30.790
<v Speaker 1>coming to us tell us anything about that dense region

0:30:31.150 --> 0:30:34.130
<v Speaker 1>if it's all got canceled out, if it's basically unchanged, right?

0:30:34.750 --> 0:30:37.190
<v Speaker 3>So you can't watch it as it changes? You just

0:30:37.210 --> 0:30:39.530
<v Speaker 3>see like the average of what happened to it over

0:30:39.570 --> 0:30:40.010
<v Speaker 3>a distance?

0:30:40.470 --> 0:30:42.320
<v Speaker 1>Yeah, you can't watch a photon go through the universe.

0:30:42.340 --> 0:30:44.700
<v Speaker 1>You just see one here on Earth. And you're like, oh,

0:30:44.760 --> 0:30:46.459
<v Speaker 1>is it hotter than I expected or colder?

0:30:46.480 --> 0:30:47.760
<v Speaker 2>Okay, got it.

0:30:48.080 --> 0:30:51.000
<v Speaker 1>And so the opposite is true for voids, right? If

0:30:51.020 --> 0:30:53.590
<v Speaker 1>you go near a black hole, then you get blue

0:30:53.650 --> 0:30:55.790
<v Speaker 1>shifted as you fall in and red shifted as you

0:30:55.830 --> 0:30:57.770
<v Speaker 1>fall out. And the opposite is true for a void.

0:30:58.110 --> 0:31:01.130
<v Speaker 1>You get red shifted as you fall in and blue

0:31:01.200 --> 0:31:02.810
<v Speaker 1>shifted as you fall out. Okay.

0:31:02.830 --> 0:31:05.510
<v Speaker 3>And so if we only see the average of what

0:31:05.530 --> 0:31:08.270
<v Speaker 3>happened to a photon when it gets here, how do

0:31:08.310 --> 0:31:08.850
<v Speaker 3>we know that?

0:31:09.210 --> 0:31:12.710
<v Speaker 1>So that's our theoretical calculation, but it's missing something really important,

0:31:13.250 --> 0:31:16.080
<v Speaker 1>which is as time goes on, when the photon is

0:31:16.230 --> 0:31:18.980
<v Speaker 1>in that void or near that black hole, the universe

0:31:19.040 --> 0:31:23.200
<v Speaker 1>is not static. The universe is expanding. And so the

0:31:23.240 --> 0:31:25.800
<v Speaker 1>amount of energy the photon loses or gains when it

0:31:25.840 --> 0:31:28.370
<v Speaker 1>goes in or out of that void changes because the

0:31:28.450 --> 0:31:31.380
<v Speaker 1>void is changing or the black hole is changing as

0:31:31.450 --> 0:31:35.160
<v Speaker 1>time goes on. So it doesn't perfectly cancel out. And

0:31:35.200 --> 0:31:38.680
<v Speaker 1>so it does leave an overall effect on these photons.

0:31:38.740 --> 0:31:42.350
<v Speaker 1>And so you can get cold spots in the CMB

0:31:42.870 --> 0:31:46.770
<v Speaker 1>if photons have moved through a super void on their

0:31:46.810 --> 0:31:50.270
<v Speaker 1>way here, if the universe is expanding. And so not

0:31:50.410 --> 0:31:52.910
<v Speaker 1>only do super voids tell us about like, hey, what

0:31:52.970 --> 0:31:54.870
<v Speaker 1>is the evolution of the universe? How do you get

0:31:54.910 --> 0:31:58.990
<v Speaker 1>these bubbles? Do they come from initial overdensities? Also, the

0:31:59.030 --> 0:32:02.180
<v Speaker 1>CMB tells us about photons moving through the universe and

0:32:02.360 --> 0:32:06.260
<v Speaker 1>measuring existing voids, not from the early universe, but today.

0:32:06.880 --> 0:32:10.880
<v Speaker 1>So there's like so many dimensions of information in the CMB.

0:32:10.930 --> 0:32:13.570
<v Speaker 1>It's not just a baby picture. It's a baby picture

0:32:13.590 --> 0:32:17.000
<v Speaker 1>that was then like dragged through your life and distorted

0:32:17.060 --> 0:32:19.540
<v Speaker 1>by the way your life turned out. And then here

0:32:19.560 --> 0:32:22.320
<v Speaker 1>we are, like we can disentangle those two things in

0:32:22.340 --> 0:32:24.520
<v Speaker 1>the single picture from the CMB and be like, oh,

0:32:24.880 --> 0:32:27.650
<v Speaker 1>this is a primordial hotspot. Or this is one that

0:32:27.690 --> 0:32:31.250
<v Speaker 1>appeared because of how the photons moved through the universe. Wow.

0:32:31.370 --> 0:32:34.600
<v Speaker 1>So all these incredibly clever little effects. We can use

0:32:34.640 --> 0:32:37.760
<v Speaker 1>to try to disentangle the history of the universe. And

0:32:37.780 --> 0:32:40.239
<v Speaker 1>this is why, like, people seem like they're in love

0:32:40.270 --> 0:32:43.810
<v Speaker 1>with the CMB. It's just such a gift. It's such

0:32:43.870 --> 0:32:45.050
<v Speaker 1>a gift. Oh, my gosh.

0:32:45.630 --> 0:32:48.650
<v Speaker 3>So what if a photon went through a black or

0:32:48.710 --> 0:32:51.170
<v Speaker 3>past a black hole and then through a super void? Like,

0:32:51.490 --> 0:32:54.370
<v Speaker 3>how do you how can you know what a photon

0:32:54.470 --> 0:32:56.730
<v Speaker 3>saw when it could have seen a bunch of things

0:32:56.770 --> 0:32:57.500
<v Speaker 3>before it gets to us?

0:32:57.510 --> 0:33:01.320
<v Speaker 1>Wow. You get it in that interview room. Okay. You

0:33:01.400 --> 0:33:04.380
<v Speaker 1>shine the lights in its face. Oh, boy. No, you're right.

0:33:04.420 --> 0:33:07.080
<v Speaker 1>You can't. And all you can do is look for patterns.

0:33:07.620 --> 0:33:10.500
<v Speaker 1>And we see in the universe, we see a big

0:33:10.680 --> 0:33:13.620
<v Speaker 1>cold spot, right, in the sky. Okay. And that's in

0:33:13.660 --> 0:33:16.300
<v Speaker 1>the same direction as a super void. And so that

0:33:16.340 --> 0:33:19.790
<v Speaker 1>means either there was like an initial underdensity there, which

0:33:19.870 --> 0:33:23.830
<v Speaker 1>created a colder region, or the photons getting here from

0:33:23.930 --> 0:33:28.070
<v Speaker 1>there have passed through a super void on the way. Okay.

0:33:28.270 --> 0:33:30.540
<v Speaker 1>And so it's just like, It's fascinating to see that

0:33:30.660 --> 0:33:33.380
<v Speaker 1>in the CMB and also then to look at our

0:33:33.420 --> 0:33:37.170
<v Speaker 1>late-time measurements of galactic structure and see, oh, there's also

0:33:37.210 --> 0:33:39.930
<v Speaker 1>a super void over there. So, like, things are lining up.

0:33:39.970 --> 0:33:42.490
<v Speaker 1>They're clicking together. You know, that's exciting when you're doing

0:33:42.510 --> 0:33:45.810
<v Speaker 1>science and you see two completely separate measurements that are

0:33:45.850 --> 0:33:48.590
<v Speaker 1>sensitive to the same thing lining up and telling you

0:33:48.630 --> 0:33:50.650
<v Speaker 1>the same story. That's when you feel like, ooh, we're

0:33:50.670 --> 0:33:51.620
<v Speaker 1>going to crack this case.

0:33:52.130 --> 0:33:52.360
<v Speaker 2>All right.

0:33:52.380 --> 0:33:54.580
<v Speaker 3>We're getting super excited over here, but we have to

0:33:54.620 --> 0:33:57.450
<v Speaker 3>take a break. Super Void if you must, but come

0:33:57.490 --> 0:34:01.890
<v Speaker 3>back in just a moment. But when we get back,

0:34:02.280 --> 0:34:04.760
<v Speaker 3>we're going to talk about how Super Voids get made.

0:34:06.060 --> 0:34:08.319
<v Speaker 3>The space ones, not the one you just made.

0:34:08.340 --> 0:34:16.799
<v Speaker 2>Super Voids.

0:34:28.410 --> 0:34:28.630
<v Speaker 3>All right.

0:34:28.790 --> 0:34:31.950
<v Speaker 2>And we're back. So, all right, Daniel, how do super

0:34:31.969 --> 0:34:32.629
<v Speaker 2>voids get made?

0:34:33.070 --> 0:34:34.710
<v Speaker 1>So this is really fun to think about how you

0:34:34.730 --> 0:34:37.930
<v Speaker 1>get super voids. One is that you can just have

0:34:38.010 --> 0:34:41.350
<v Speaker 1>an underdense region initially and, you know, you could just

0:34:41.370 --> 0:34:44.890
<v Speaker 1>have a fluctuation. Like these things we think are seeded

0:34:44.969 --> 0:34:49.560
<v Speaker 1>originally by quantum fluctuations. Why anyway are there regions that

0:34:49.600 --> 0:34:52.160
<v Speaker 1>are higher or lower density? You know, one theory is

0:34:52.200 --> 0:34:55.259
<v Speaker 1>you have quantum fluctuations in the very early universe and

0:34:55.300 --> 0:34:59.470
<v Speaker 1>then inflation is this pre-Big Bang theory we talked about recently,

0:34:59.800 --> 0:35:05.050
<v Speaker 1>stretch those out into macroscopic actual fluctuations that matter to gravity.

0:35:05.969 --> 0:35:08.010
<v Speaker 1>That's just a speculative theory. We don't know for sure.

0:35:08.570 --> 0:35:11.350
<v Speaker 1>But that would suggest that the fluctuations themselves, the reason

0:35:11.390 --> 0:35:14.250
<v Speaker 1>we have more stuff here and less stuff there, comes

0:35:14.450 --> 0:35:17.450
<v Speaker 1>initially randomly, which means that lots of stuff could happen.

0:35:18.090 --> 0:35:20.550
<v Speaker 1>For example, you're flipping coins. You don't expect to get

0:35:20.930 --> 0:35:22.420
<v Speaker 1>heads in the tails and then heads in the tails.

0:35:22.440 --> 0:35:25.379
<v Speaker 1>You'll have runs of heads and runs of tails. And so,

0:35:26.020 --> 0:35:28.580
<v Speaker 1>If somebody's flipping coins for the early universe, it's like,

0:35:28.620 --> 0:35:30.500
<v Speaker 1>are we getting stuff here or not? They could have

0:35:30.540 --> 0:35:32.739
<v Speaker 1>just come up with no stuff in this part of

0:35:32.780 --> 0:35:35.750
<v Speaker 1>the universe a lot of times, occasionally, right? So that

0:35:35.790 --> 0:35:38.670
<v Speaker 1>kind of thing can happen, but it's unlikely, right? The

0:35:38.730 --> 0:35:40.910
<v Speaker 1>bigger the void, the less likely it is that can happen.

0:35:41.210 --> 0:35:43.070
<v Speaker 1>The same way like having a run of 10 heads

0:35:43.170 --> 0:35:45.190
<v Speaker 1>is less likely than a run of five heads and

0:35:45.210 --> 0:35:47.730
<v Speaker 1>a run of like 50 heads in rows, essentially unheard of,

0:35:48.830 --> 0:35:51.450
<v Speaker 1>though there is a probability. And so, you know, we

0:35:51.590 --> 0:35:54.820
<v Speaker 1>only have this one universe. And so we can't tell like, hey,

0:35:54.960 --> 0:35:58.070
<v Speaker 1>did we just get lucky or slash unlucky? We don't know.

0:35:58.510 --> 0:36:00.569
<v Speaker 1>But there are also other ways people have come up

0:36:00.630 --> 0:36:04.230
<v Speaker 1>with in watching these simulations to see supervoids form, which

0:36:04.270 --> 0:36:07.270
<v Speaker 1>is that you can get voids merging. So these bubbles

0:36:07.330 --> 0:36:11.960
<v Speaker 1>can pop because you get gravitational disturbances between these things

0:36:12.219 --> 0:36:15.420
<v Speaker 1>and the walls can fall apart, essentially. And so you

0:36:15.440 --> 0:36:19.239
<v Speaker 1>can get these cells merging. Basically, if you have an

0:36:19.340 --> 0:36:21.930
<v Speaker 1>over density in some walls, they can attract those filaments

0:36:22.010 --> 0:36:24.890
<v Speaker 1>and It's not like these super voids are totally empty.

0:36:25.330 --> 0:36:28.330
<v Speaker 1>And so you still have some galaxies remaining inside of them.

0:36:29.030 --> 0:36:32.730
<v Speaker 1>And so you can get mergers of these voids to

0:36:32.770 --> 0:36:35.130
<v Speaker 1>form super voids. And this is the kind of example

0:36:35.150 --> 0:36:37.529
<v Speaker 1>of something you can learn about in simulation. You can

0:36:37.590 --> 0:36:39.250
<v Speaker 1>run a simulation in the universe. You can watch it.

0:36:39.250 --> 0:36:41.730
<v Speaker 1>You'd be like, look at that. I didn't expect that

0:36:41.770 --> 0:36:44.969
<v Speaker 1>to happen. But you see it in simulation. You learn that.

0:36:45.500 --> 0:36:49.620
<v Speaker 1>about emergent phenomena in simulation that you didn't predict. Super

0:36:49.640 --> 0:36:50.260
<v Speaker 1>duper cool.

0:36:50.520 --> 0:36:51.820
<v Speaker 2>Yay, theoretical physicists.

0:36:53.810 --> 0:36:56.129
<v Speaker 1>But this allows us to ask the question like, well,

0:36:56.210 --> 0:36:58.810
<v Speaker 1>why are there super voids? Do they make sense in

0:36:58.850 --> 0:37:01.990
<v Speaker 1>the universe? And, you know, we have this cold spot,

0:37:02.090 --> 0:37:05.900
<v Speaker 1>which we can partially explain using this like photons come in,

0:37:05.940 --> 0:37:08.340
<v Speaker 1>photons go out, but it's not a full explanation. It

0:37:08.400 --> 0:37:10.799
<v Speaker 1>explains like part of the cold spot, but not all

0:37:10.820 --> 0:37:14.390
<v Speaker 1>of it. It's really very unusual. Though it's hard to say, like,

0:37:14.630 --> 0:37:17.149
<v Speaker 1>how unusual is a 1% effect? You know, you see

0:37:17.170 --> 0:37:19.529
<v Speaker 1>it in one out of 100 universes. And so are

0:37:19.550 --> 0:37:21.890
<v Speaker 1>we just unlucky or is this a hint that there's

0:37:21.910 --> 0:37:25.009
<v Speaker 1>something else going on? Because remember that these things are

0:37:25.050 --> 0:37:27.850
<v Speaker 1>very sensitive to the parameters of the universe. How much

0:37:27.910 --> 0:37:31.290
<v Speaker 1>dark matter was there, dark matter forming that structure, how

0:37:31.310 --> 0:37:34.330
<v Speaker 1>much dark energy was there to create this acceleration and

0:37:34.370 --> 0:37:37.910
<v Speaker 1>this expansion, which is what's causing this effect, this cold

0:37:37.930 --> 0:37:40.430
<v Speaker 1>spot effect. Because remember, it's only if the voids are

0:37:40.510 --> 0:37:43.410
<v Speaker 1>changing as the photons are going through them that you

0:37:43.430 --> 0:37:46.560
<v Speaker 1>even see an effect from the voids. And so there's

0:37:46.580 --> 0:37:49.420
<v Speaker 1>a lot of questions about whether the super voids are

0:37:49.460 --> 0:37:51.759
<v Speaker 1>something we expect or whether they indicate that we need

0:37:51.820 --> 0:37:55.299
<v Speaker 1>something new in our theory of the universe, which of

0:37:55.360 --> 0:37:57.560
<v Speaker 1>course is where the fun begins because then we get

0:37:57.580 --> 0:38:00.150
<v Speaker 1>to speculate about all the crazy ideas.

0:38:00.350 --> 0:38:02.130
<v Speaker 2>Daniel has a sparkle in his eye.

0:38:04.230 --> 0:38:06.630
<v Speaker 3>So at the beginning of the episode, you said super

0:38:06.650 --> 0:38:09.989
<v Speaker 3>voids remind you of like the Marvel Universe. So if

0:38:10.030 --> 0:38:12.670
<v Speaker 3>you had like parallel universes like you do in the

0:38:12.710 --> 0:38:15.989
<v Speaker 3>Marvel Universe, would you expect super voids to be distributed

0:38:16.070 --> 0:38:18.850
<v Speaker 3>about the same way or like have about the same number?

0:38:18.969 --> 0:38:22.009
<v Speaker 2>Like what? I'm trying to get to parallel universes for you.

0:38:24.270 --> 0:38:27.530
<v Speaker 1>Well, there's an even cooler way that parallel universes connect

0:38:27.550 --> 0:38:30.390
<v Speaker 1>to super voids, which is that maybe you had a

0:38:30.410 --> 0:38:33.160
<v Speaker 1>bunch of initial universes early on. And remember, we talked

0:38:33.180 --> 0:38:37.380
<v Speaker 1>about inflation. how our universe maybe is like a tiny

0:38:37.500 --> 0:38:42.299
<v Speaker 1>dot in a vast landscape of inflationary matter. And in

0:38:42.340 --> 0:38:44.779
<v Speaker 1>that dot, it just like went from inflationary matter to

0:38:44.840 --> 0:38:47.180
<v Speaker 1>normal matter. And then our universe is there and expanded.

0:38:47.580 --> 0:38:50.260
<v Speaker 1>And there could be other dots out there. And usually

0:38:50.340 --> 0:38:52.200
<v Speaker 1>those other dots are really far away. And there's a

0:38:52.200 --> 0:38:54.360
<v Speaker 1>bunch of inflationary matter between us and them, which is

0:38:54.420 --> 0:38:57.000
<v Speaker 1>expanding at some insane rates. So we'll never see those

0:38:57.040 --> 0:39:01.020
<v Speaker 1>other universes. But what if that's not true? What if

0:39:01.060 --> 0:39:04.190
<v Speaker 1>there are other universes out there And our universe has collided.

0:39:04.710 --> 0:39:08.700
<v Speaker 1>If early on our bubble bounced into another bubble, it

0:39:08.800 --> 0:39:12.640
<v Speaker 1>might leave an imprint on the early universe. And according

0:39:12.680 --> 0:39:16.020
<v Speaker 1>to some theories and according to some simulations, that can

0:39:16.080 --> 0:39:19.160
<v Speaker 1>cause like a bruise in the density, which would be

0:39:19.200 --> 0:39:22.009
<v Speaker 1>like a cold spot, which would lead to a super void.

0:39:22.590 --> 0:39:24.989
<v Speaker 1>And so there are some really fun speculative theories of

0:39:25.010 --> 0:39:27.830
<v Speaker 1>the early universe out there that suggest that if there

0:39:28.070 --> 0:39:33.000
<v Speaker 1>are these parallel bubble universes, created in this inflationary landscape,

0:39:33.340 --> 0:39:35.760
<v Speaker 1>that sometimes they'll bump into each other and they'll leave

0:39:35.800 --> 0:39:38.509
<v Speaker 1>a mark, and that mark is super voids.

0:39:39.210 --> 0:39:45.759
<v Speaker 2>Well, I think I'm still having one. Awesome, too. I'm

0:39:45.780 --> 0:39:48.020
<v Speaker 2>having a little trouble imagining. So you get two bubbles.

0:39:48.500 --> 0:39:49.660
<v Speaker 2>They like merge.

0:39:50.080 --> 0:39:52.600
<v Speaker 3>And then is it like whatever was making the outside

0:39:52.640 --> 0:39:54.540
<v Speaker 3>wall of the bubble where they touch just sort of

0:39:54.580 --> 0:39:57.430
<v Speaker 3>like gets blown to somewhere else. And now you get

0:39:57.469 --> 0:40:00.770
<v Speaker 3>a big center as those two bubbles merge. Is that

0:40:01.250 --> 0:40:02.489
<v Speaker 3>how does that result in.

0:40:02.469 --> 0:40:03.109
<v Speaker 2>A super void?

0:40:03.450 --> 0:40:06.029
<v Speaker 1>Yeah, great question. And I realize that now we're using

0:40:06.070 --> 0:40:09.029
<v Speaker 1>the word bubble to mean two different things. Shame on us.

0:40:09.050 --> 0:40:09.629
<v Speaker 1>Shame on me.

0:40:09.650 --> 0:40:16.089
<v Speaker 2>Yeah, I'm not taking any blame for that. Fair.

0:40:16.560 --> 0:40:18.700
<v Speaker 1>No, when we talked earlier about bubbles, we were talking

0:40:18.719 --> 0:40:22.060
<v Speaker 1>about the structure of our universe. And there's densities of

0:40:22.200 --> 0:40:26.020
<v Speaker 1>superclusters of galaxies and under densities. And we talked about

0:40:26.080 --> 0:40:29.779
<v Speaker 1>those organizing into bubbles. And those are bubbles. Now we're

0:40:29.800 --> 0:40:32.760
<v Speaker 1>talking about bubbles as the whole universe is one bubble.

0:40:33.610 --> 0:40:37.969
<v Speaker 1>in a vaster inflationary landscape. So let's not call them

0:40:38.010 --> 0:40:40.880
<v Speaker 1>a bubble. Let's just say if our universe bumps into

0:40:40.930 --> 0:40:44.740
<v Speaker 1>another universe, because remember in this theory, universes are finite.

0:40:44.760 --> 0:40:48.820
<v Speaker 1>They're little regions of this inflationary landscape that have decayed

0:40:48.860 --> 0:40:52.070
<v Speaker 1>into normal matter. So if our universe bumps into another

0:40:52.150 --> 0:40:55.190
<v Speaker 1>universe and then bounces off, they don't merge. They bounce

0:40:55.270 --> 0:40:57.140
<v Speaker 1>off each other, but they leave a mark. You know,

0:40:57.160 --> 0:40:58.850
<v Speaker 1>the way like if you take two apples and you

0:40:58.870 --> 0:41:00.870
<v Speaker 1>smash them together, they don't become one apple, but you

0:41:00.890 --> 0:41:03.029
<v Speaker 1>get a bruise on each one. Yeah. What would that

0:41:03.070 --> 0:41:06.089
<v Speaker 1>bruise look like on our universe if another universe had

0:41:06.150 --> 0:41:09.109
<v Speaker 1>bumped into us and like not even left a note, just,

0:41:09.150 --> 0:41:11.880
<v Speaker 1>you know, just like hit and run universe style?

0:41:11.900 --> 0:41:12.520
<v Speaker 2>Not cool.

0:41:12.540 --> 0:41:14.680
<v Speaker 1>Well, we would get a bruise and it would change

0:41:14.739 --> 0:41:18.700
<v Speaker 1>the initial density of matter in the early universe. And

0:41:18.800 --> 0:41:22.380
<v Speaker 1>simulations and calculations suggest that that would leave a cold

0:41:22.440 --> 0:41:25.130
<v Speaker 1>spot and under density in that part of the universe,

0:41:25.170 --> 0:41:27.890
<v Speaker 1>which would If you ran the simulations forward, leave to

0:41:27.930 --> 0:41:29.050
<v Speaker 1>a super void today.

0:41:29.489 --> 0:41:31.210
<v Speaker 2>Wow. Okay. All right. I'm with you.

0:41:31.370 --> 0:41:34.860
<v Speaker 1>Yeah. So that's one fun theory. And, you know, there's

0:41:34.900 --> 0:41:37.359
<v Speaker 1>a lot of debate about that. People say, you know,

0:41:37.400 --> 0:41:40.680
<v Speaker 1>you're cherry picking, you're crafting an explanation to match something

0:41:40.719 --> 0:41:43.600
<v Speaker 1>you see. It would be much more compelling if you

0:41:43.620 --> 0:41:45.580
<v Speaker 1>had a prediction for this before you saw the super

0:41:45.600 --> 0:41:47.480
<v Speaker 1>voids and you say, I predict a super void. And

0:41:47.500 --> 0:41:49.339
<v Speaker 1>then you went out and saw it. That'd be much

0:41:49.360 --> 0:41:52.560
<v Speaker 1>more compelling. This is more like a post addiction. It's like, oh,

0:41:52.580 --> 0:41:54.779
<v Speaker 1>we see this thing in the universe. What could explain it?

0:41:55.310 --> 0:41:57.250
<v Speaker 1>Not as a criticism, but just saying it would be

0:41:57.290 --> 0:41:59.969
<v Speaker 1>more powerful, more compelling if it was a prediction and

0:42:00.010 --> 0:42:01.410
<v Speaker 1>not a postdiction. Okay.

0:42:01.450 --> 0:42:04.359
<v Speaker 3>I mean, I totally see that. But on the other hand, like, okay,

0:42:04.380 --> 0:42:06.010
<v Speaker 3>but you've seen the thing and you can't unsee it.

0:42:06.040 --> 0:42:07.839
<v Speaker 3>And now you have to try to explain it. And so,

0:42:07.900 --> 0:42:10.500
<v Speaker 3>but I agree. It would have been more powerful if

0:42:10.560 --> 0:42:12.160
<v Speaker 3>it had met expectations.

0:42:12.200 --> 0:42:14.540
<v Speaker 2>But the universe doesn't care about our expectations.

0:42:15.040 --> 0:42:19.470
<v Speaker 1>Yeah. So another potential explanation for this is a favorite

0:42:19.530 --> 0:42:23.190
<v Speaker 1>alternative for dark matter. You remember that we talked about

0:42:23.250 --> 0:42:25.970
<v Speaker 1>dark matter being out there. We have lots of independent

0:42:25.989 --> 0:42:28.630
<v Speaker 1>lines of evidence for it. But there are alternatives, and

0:42:28.670 --> 0:42:31.899
<v Speaker 1>it's healthy that people are thinking about other things and

0:42:32.040 --> 0:42:35.100
<v Speaker 1>trying to understand if those other explanations are coherent, if

0:42:35.140 --> 0:42:38.540
<v Speaker 1>they can explain multiple things and not just galactic rotation curves.

0:42:39.180 --> 0:42:42.440
<v Speaker 1>One of those is modified gravity. To say maybe gravity

0:42:42.480 --> 0:42:45.700
<v Speaker 1>doesn't work the way we expect. Maybe it's not that

0:42:45.760 --> 0:42:49.000
<v Speaker 1>there is more invisible stuff out there causing gravity, but

0:42:49.020 --> 0:42:52.020
<v Speaker 1>that gravity behaves differently and there isn't any dark matter.

0:42:52.680 --> 0:42:56.590
<v Speaker 1>This is called MOND, Modified Newtonian Dynamics. I remember how

0:42:56.610 --> 0:42:58.799
<v Speaker 1>we talked about some of these cold spots are due

0:42:58.860 --> 0:43:02.029
<v Speaker 1>to the expansion of the universe as photons fall in

0:43:02.150 --> 0:43:04.670
<v Speaker 1>and out of these voids or in and out of

0:43:04.710 --> 0:43:07.490
<v Speaker 1>the neighborhood of a black hole. Well, that could also

0:43:07.570 --> 0:43:11.980
<v Speaker 1>be explained in some models of modified gravity. Okay. Because

0:43:12.020 --> 0:43:14.780
<v Speaker 1>you're changing how gravity works, so it's going to change

0:43:14.820 --> 0:43:18.319
<v Speaker 1>how these photons experience the universe. And even some theories

0:43:18.360 --> 0:43:21.379
<v Speaker 1>of the universe isn't expanding, and these things are just

0:43:21.480 --> 0:43:24.190
<v Speaker 1>due to evidence that gravity doesn't work the way that

0:43:24.210 --> 0:43:27.730
<v Speaker 1>we expect. And it's true that we can't fully explain

0:43:27.770 --> 0:43:30.430
<v Speaker 1>these supervoids. We don't know where they come from. Our

0:43:30.489 --> 0:43:33.710
<v Speaker 1>current theories do definitely need something. Do you need to

0:43:33.750 --> 0:43:37.150
<v Speaker 1>go all the way to modified gravity to explain supervoids?

0:43:37.600 --> 0:43:39.460
<v Speaker 1>I don't think so. But, you know, maybe I'm just

0:43:39.500 --> 0:43:41.569
<v Speaker 1>not a fan of the modified gravity theory, and so

0:43:41.610 --> 0:43:44.630
<v Speaker 1>I'm blind to it. I do respect that they're trying

0:43:44.650 --> 0:43:47.810
<v Speaker 1>to find other ways to support this theory, other places

0:43:48.450 --> 0:43:50.870
<v Speaker 1>to look for evidence that might indicate that it's the

0:43:50.950 --> 0:43:54.160
<v Speaker 1>real explanation for the universe and not just a single

0:43:54.200 --> 0:43:57.020
<v Speaker 1>fudge factor they're using to fix galactic rotation curves.

0:43:57.400 --> 0:44:00.460
<v Speaker 3>Now, when we finish getting through all of the explanations,

0:44:00.500 --> 0:44:02.920
<v Speaker 3>are you going to tell us which explanation is your favorite?

0:44:05.680 --> 0:44:07.400
<v Speaker 2>Or are you just going to super void on this one?

0:44:10.060 --> 0:44:12.100
<v Speaker 1>No, instead, I'm going to tell you about how we

0:44:12.140 --> 0:44:14.880
<v Speaker 1>might learn more about the universe rather than betting on

0:44:14.960 --> 0:44:18.760
<v Speaker 1>any individual one. Because we talked about how in the 70s,

0:44:18.800 --> 0:44:21.520
<v Speaker 1>they started putting this together when they were measuring the

0:44:21.560 --> 0:44:24.580
<v Speaker 1>cosmic structure. And they've continued to do that. There was

0:44:24.620 --> 0:44:27.660
<v Speaker 1>a big survey in the 2000s called the Sloan Digital

0:44:27.680 --> 0:44:30.830
<v Speaker 1>Sky Survey, mapped out a huge number of these big

0:44:30.910 --> 0:44:35.100
<v Speaker 1>walls and bubbles and and really giving us a broader

0:44:35.200 --> 0:44:38.540
<v Speaker 1>sense of where we are in the universe. And that's continuing.

0:44:38.600 --> 0:44:42.359
<v Speaker 1>We now have this telescope called DESI, D-E-S-I, the Dark

0:44:42.440 --> 0:44:46.219
<v Speaker 1>Energy Survey Instrument, which is the most powerful telescope we've

0:44:46.280 --> 0:44:49.780
<v Speaker 1>ever had for understanding where things are in the universe

0:44:50.219 --> 0:44:52.840
<v Speaker 1>in terms of measuring the redshift of a huge number

0:44:52.860 --> 0:44:56.950
<v Speaker 1>of distant galaxies. And so like, what's more important? What's

0:44:56.989 --> 0:44:59.930
<v Speaker 1>more exciting than like mapping out the universe? And that's

0:44:59.950 --> 0:45:02.190
<v Speaker 1>what we're doing. And just yesterday we saw the launch

0:45:02.710 --> 0:45:05.270
<v Speaker 1>of the Nancy Grace Roman telescope, which is also going

0:45:05.290 --> 0:45:07.270
<v Speaker 1>to tell us about the expansion of the universe and

0:45:07.350 --> 0:45:11.569
<v Speaker 1>red shifts and the structure of the universe. So we

0:45:11.630 --> 0:45:14.969
<v Speaker 1>are learning so much more. It reminds me of like,

0:45:15.210 --> 0:45:17.310
<v Speaker 1>have you seen early maps? I love looking at like

0:45:17.610 --> 0:45:21.339
<v Speaker 1>maps people drew of the world in like 1200, you know,

0:45:21.360 --> 0:45:23.469
<v Speaker 1>when like they didn't know about this whole continent and

0:45:23.489 --> 0:45:26.060
<v Speaker 1>they misunderstood this whole piece, but you see truth in there.

0:45:26.520 --> 0:45:28.540
<v Speaker 1>You see like the shape of Portugal or you see

0:45:28.580 --> 0:45:31.910
<v Speaker 1>like the coast of Madagascar or whatever. And that's what

0:45:31.969 --> 0:45:33.930
<v Speaker 1>our maps are like today. And I think in a

0:45:33.969 --> 0:45:37.350
<v Speaker 1>thousand years, people will look back at our primitive, basic

0:45:37.450 --> 0:45:40.790
<v Speaker 1>maps of our neighborhood and be like, wow, they knew nothing.

0:45:41.710 --> 0:45:44.280
<v Speaker 1>But the information is coming. We are building those maps.

0:45:44.320 --> 0:45:47.800
<v Speaker 1>We are exploring the universe. We're figuring out. And along

0:45:47.820 --> 0:45:50.580
<v Speaker 1>the way, we're discovering mysteries and puzzles, which are going

0:45:50.600 --> 0:45:52.900
<v Speaker 1>to clue us into how the universe works. There are

0:45:53.610 --> 0:45:57.109
<v Speaker 1>answers out there to questions we haven't thought to ask

0:45:57.210 --> 0:46:00.250
<v Speaker 1>because we haven't even mapped out what the universe looks like,

0:46:00.570 --> 0:46:03.549
<v Speaker 1>you know? And so we can't, we don't even know

0:46:03.590 --> 0:46:04.420
<v Speaker 1>what to ask yet.

0:46:04.719 --> 0:46:04.859
<v Speaker 2>Yep.

0:46:05.040 --> 0:46:08.120
<v Speaker 3>We are constantly pushing the boundaries of our ignorance back

0:46:08.180 --> 0:46:08.980
<v Speaker 3>farther and farther.

0:46:09.040 --> 0:46:09.420
<v Speaker 2>I love it.

0:46:09.520 --> 0:46:12.580
<v Speaker 1>Yeah. And super voids are really fascinating hole in our

0:46:12.600 --> 0:46:16.450
<v Speaker 1>understanding because, you know, we don't fully understand how they form.

0:46:16.550 --> 0:46:19.509
<v Speaker 1>Are we just lucky slash unlucky? Is there something else

0:46:19.550 --> 0:46:22.310
<v Speaker 1>going on in the universe that makes these incredibly under

0:46:22.370 --> 0:46:24.890
<v Speaker 1>dense regions? Is this a clue or is it a

0:46:24.930 --> 0:46:27.549
<v Speaker 1>red herring? We don't know. And really, the only way

0:46:27.590 --> 0:46:30.840
<v Speaker 1>to know is to get more data, more mapping, more structure,

0:46:31.020 --> 0:46:33.940
<v Speaker 1>more images, more understanding of where we are in the universe.

0:46:34.000 --> 0:46:38.410
<v Speaker 1>I'm definitely for that. And also, it's cheap. Compared to

0:46:38.430 --> 0:46:40.830
<v Speaker 1>the kind of stuff we spend money on, it costs pennies.

0:46:42.050 --> 0:46:46.010
<v Speaker 3>Usually physics doesn't feel super cheap, but this one's cheap,

0:46:46.050 --> 0:46:46.530
<v Speaker 3>you're saying?

0:46:47.870 --> 0:46:50.190
<v Speaker 1>I mean, it's a lot more expensive than, say, a

0:46:50.250 --> 0:46:53.030
<v Speaker 1>week in the archives in New York City reading somebody's

0:46:53.110 --> 0:46:55.009
<v Speaker 1>blood-covered notes, hypothetically.

0:46:55.090 --> 0:46:55.669
<v Speaker 2>That was fun.

0:46:55.710 --> 0:46:57.430
<v Speaker 1>It's a lot more expensive than a lot of stuff.

0:46:57.950 --> 0:47:01.489
<v Speaker 1>But compared to aircraft carriers, you know, or wars in

0:47:01.510 --> 0:47:02.890
<v Speaker 1>the Middle East, it's definitely cheap.

0:47:03.430 --> 0:47:05.770
<v Speaker 3>And then you get to enjoy that knowledge forever.

0:47:06.050 --> 0:47:08.890
<v Speaker 1>Yes, you do. And you create the opportunities for a

0:47:08.969 --> 0:47:11.969
<v Speaker 1>new generation of scientists to study new puzzles and come

0:47:12.030 --> 0:47:15.390
<v Speaker 1>up with new answers. So thanks very much to Nathan

0:47:15.489 --> 0:47:18.110
<v Speaker 1>and Levi for asking about superboards and giving us an

0:47:18.150 --> 0:47:21.489
<v Speaker 1>opportunity to talk about this incredible cosmic history, all the

0:47:21.530 --> 0:47:24.729
<v Speaker 1>detective stories we've cracked along the way, and so many

0:47:24.850 --> 0:47:26.710
<v Speaker 1>open questions we have yet to even ask.

0:47:27.210 --> 0:47:28.210
<v Speaker 2>Fun science, please.

0:47:37.070 --> 0:47:39.440
<v Speaker 1>Thanks everybody for listening. Please go and do us a

0:47:39.460 --> 0:47:42.760
<v Speaker 1>favor and rate the show on whatever podcast app you're using.

0:47:42.820 --> 0:47:44.299
<v Speaker 1>It really helps people find us.

0:47:44.940 --> 0:47:48.870
<v Speaker 3>Daniel and Kelly's Extraordinary Universe is edited by the amazing

0:47:48.930 --> 0:47:49.590
<v Speaker 3>Matt Kesselman.

0:47:49.850 --> 0:47:53.040
<v Speaker 1>He really is a wizard. You can also find us

0:47:53.280 --> 0:47:58.220
<v Speaker 1>online on Blue Sky, Instagram, and X, D &amp; K Universe.

0:47:58.300 --> 0:47:59.420
<v Speaker 1>Come engage with us.

0:47:59.800 --> 0:48:03.800
<v Speaker 3>You can email us at questions at danielandkelly.org. We really

0:48:03.860 --> 0:48:04.980
<v Speaker 3>do want to hear from you.

0:48:05.180 --> 0:48:10.480
<v Speaker 1>And you can find our website, www.danielandkelly.org, where you'll also

0:48:10.540 --> 0:48:13.930
<v Speaker 1>find an invitation to join our Discord, where everybody comes

0:48:14.010 --> 0:48:16.110
<v Speaker 1>and talks about the amazing universe.

0:48:16.450 --> 0:48:20.370
<v Speaker 3>And we also have the most amazing moderators. This is

0:48:20.410 --> 0:48:22.790
<v Speaker 3>an iHeart podcast. Thanks for joining us.