WEBVTT - Listener Questions 5

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<v Speaker 1>Hey, Daniel, do you get tired of answering questions? Oh? Never,

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<v Speaker 1>I love our listener questions. I just mean questions in general,

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<v Speaker 1>like about the universe, about your personal life, poor like

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<v Speaker 1>this question you're asking me now from your podcast host partner. No,

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<v Speaker 1>people ask me questions all the time, but it's fun

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<v Speaker 1>to answer them. You know, sometimes I wish I got

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<v Speaker 1>asked more science questions, you know, sometimes with questions are

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<v Speaker 1>more prosaic. But about your kids? And your kids constantly

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<v Speaker 1>pester you with science questions too, I wish they asked more.

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<v Speaker 1>You know. It's the occasional like what does the black

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<v Speaker 1>hole look like? But more often it's like can I

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<v Speaker 1>have more dessert? Or how could my sister just to

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<v Speaker 1>use the iPad more than I do? And the answer

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<v Speaker 1>is always the same. Nobody knows that we have no idea.

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<v Speaker 1>They're kind of six questions too, aren't they? Like? Um,

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<v Speaker 1>they're about time? Who gets more time on the iPad?

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<v Speaker 1>Or matter who gets more desserted? Exactly? And what about you?

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<v Speaker 1>Your kids ask you science questions? Uh? They do, yeah,

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<v Speaker 1>pretty pretty often. I think my kids, um like to

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<v Speaker 1>read and sometimes they kind of make connections in their

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<v Speaker 1>head and they ask me questions. And what do you

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<v Speaker 1>do when they ask you questions if you don't know

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<v Speaker 1>the answer. What do you mean you assume that I

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<v Speaker 1>don't know the answers. I often don't know the answer,

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<v Speaker 1>so I assume not everybody has all the answers. Sure, no,

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<v Speaker 1>Well I do my best. I guess um and maybe baby. Mainly,

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<v Speaker 1>I just tell them to send their questions into our

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<v Speaker 1>podcast so that you can answer them. That sounds good.

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<v Speaker 1>I'm glad to be your backup science parent. I mean,

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<v Speaker 1>what's the whole point of befriending as physicists if not

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<v Speaker 1>to get these questions answered? I knew, just would you

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<v Speaker 1>want to be friends with the physicists? I knew? I

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<v Speaker 1>felt used. Now I know why. Hi am Jorge. I'm

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<v Speaker 1>a cartoonist and the creator of PhD Comics. Hi I'm Daniel.

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<v Speaker 1>I'm a particle physicist and a backup science parent for

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<v Speaker 1>many people out there. And welcome to our podcast, Daniel

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<v Speaker 1>and Jorge Explain the Universe, a production of I Heart

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<v Speaker 1>Radio in which we take funny, weird, amazing, crazy things

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<v Speaker 1>about the universe and explain them to you so that

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<v Speaker 1>you can explain them to your kids or your parents

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<v Speaker 1>or just sit them down with with our podcast as

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<v Speaker 1>free babysitting. That's right. Yeah, so we we love answering questions,

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<v Speaker 1>right Daniel. Oh yeah, it's really fun because we can

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<v Speaker 1>think about the universe and we can talk about what's

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<v Speaker 1>exciting for us. But the most is interesting is answering

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<v Speaker 1>questions from listeners because it reveals what they understand and

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<v Speaker 1>what they own't and what they're wondering about, what all

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<v Speaker 1>those collective brains out there are cognating on. Yeah, so

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<v Speaker 1>if you don't know this already, we actually answer people's questions.

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<v Speaker 1>If we have an Instagram account, on Twitter account, on

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<v Speaker 1>Facebook account, and if you post a question, well, first

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<v Speaker 1>of all, follow us there, but if you post a question,

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<v Speaker 1>most likely Daniel will answer the question, right Daniel, or

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<v Speaker 1>at least maybe one of your regrets, that's right. No,

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<v Speaker 1>I'll answer questions via email or Twitter or Facebook. I'll

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<v Speaker 1>be honest, though, I don't use Instagram, so all those

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<v Speaker 1>people asking physics questions on Instagram are just questioning into

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<v Speaker 1>the void. Sorry, folks. The question is does anyone use

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<v Speaker 1>Instagram anymore? Now that I don't, I think the question

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<v Speaker 1>is who doesn't use Instagram these days? Just me, I guess,

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<v Speaker 1>I guess just physicists, you know. But it's wonderful. We

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<v Speaker 1>hear questions from all over the world, and sometimes there

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<v Speaker 1>are questions people just had in their minds they wanted

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<v Speaker 1>to know the answers to, and those are wonderful. But

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<v Speaker 1>also sometimes the questions are in reaction to something we

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<v Speaker 1>talked about on the show. You know, on the show,

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<v Speaker 1>we do our best to think, what's confusing about this?

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<v Speaker 1>How do we explain this? How do we make something clear?

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<v Speaker 1>But we never can completely succeed. So it's really nice

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<v Speaker 1>to have feedback when people say you said X, but

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<v Speaker 1>then I that made me wonder why, and that helps

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<v Speaker 1>us be more clear in the future. So please send

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<v Speaker 1>us feedback, send us questions, send us presents, send us gags,

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<v Speaker 1>send us whatever you have at Mostly you send us

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<v Speaker 1>money please, I mean, how much do you think podcasting? Me? Podcaster?

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<v Speaker 1>That's right? And sometimes people send us serious questions about

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<v Speaker 1>the universe. And then sometimes people send us silly questions. Yeah,

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<v Speaker 1>like what's been a silly question? All right, here's a

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<v Speaker 1>question we got on Twitter from Patrick Nouman. He says,

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<v Speaker 1>Dear Daniel and Jorge, I've got a question that really

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<v Speaker 1>want to get answered. How heavy would a blob or

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<v Speaker 1>banana bee of all of the photons in sun? And

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<v Speaker 1>how big would it be? Oh? Interesting, So you took

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<v Speaker 1>all the photons in the sun and somehow, what do

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<v Speaker 1>you think, transformed them into a banana or put them

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<v Speaker 1>in the space shaped them into a banana? What do

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<v Speaker 1>you think I actually started trying to work on this question.

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<v Speaker 1>At first, I thought, well, how many photons are in

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<v Speaker 1>the sun, right, like, is that a number? Um? You know,

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<v Speaker 1>and it's pretty tough. But it turns out you can

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<v Speaker 1>do a rough calculation and the sun creates ten to

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<v Speaker 1>the forty five photons per second. That's ten with that's

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<v Speaker 1>a lot of photons, a lot of like trillion, billy

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<v Speaker 1>busily but gillions, yes, exactly, billions and yeah, exactly. But

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<v Speaker 1>not all those photons escape the sun. You know, the

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<v Speaker 1>sun is a huge ball of plas and most of

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<v Speaker 1>the stuff that's made by the Sun is then just

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<v Speaker 1>reabsorbed by the Sun, and so only things that actually

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<v Speaker 1>penetrate leave the Sun and hate your eyeballs arrive here

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<v Speaker 1>on Earth. That's a tiny fraction what comes out of

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<v Speaker 1>the Sun. But anyway, let's say you had ten to

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<v Speaker 1>the forty five photons. Okay, that's a huge amount of

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<v Speaker 1>energy um. And then this question is interesting. He said,

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<v Speaker 1>how big would that be? Right? Like if you had

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<v Speaker 1>a pile of tending the forty five photons, right? How well?

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<v Speaker 1>How how how close together can you cram them in? Maybe? Yeah,

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<v Speaker 1>And that's really interesting because there's no limit on how

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<v Speaker 1>close you can cram photons together. That's not true ordinary

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<v Speaker 1>matter like electrons and other particles. These things are fermions,

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<v Speaker 1>and fermions are different from photons and other kind of

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<v Speaker 1>particles that we call bosons because fermions have to have

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<v Speaker 1>different quantum states. No two of them can be in

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<v Speaker 1>the same quantum state. They can literally be on top

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<v Speaker 1>of each other. That's impossible, that's right. They have to

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<v Speaker 1>have some difference, like you can have two electrons in

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<v Speaker 1>the same level of energy in a in an atom,

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<v Speaker 1>but then they have different have to have different spins

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<v Speaker 1>or something different about them, and so fer meons have

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<v Speaker 1>to be distinguishable, whereas bosons, these are particles with integer

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<v Speaker 1>spin like a photon. They can be right on top

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<v Speaker 1>of each other. They can be exactly the same place,

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<v Speaker 1>have the same momentum, had the same everything. I feel

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<v Speaker 1>like the silly question is is gotten a little seriously Yeah,

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<v Speaker 1>serious physics, yea, even silly questions reveals something interesting about

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<v Speaker 1>the universe. And so you can have ten to the

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<v Speaker 1>forty five photons on the head of a pin, basically

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<v Speaker 1>right or on top of each other. You're saying, yes, exactly,

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<v Speaker 1>all on top of each other in a tiny, tiny space.

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<v Speaker 1>So thank you Patrick for sending in that hilarious question.

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<v Speaker 1>It really made us think, and there really is some

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<v Speaker 1>physics in that question, even in silly questions. Well, we

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<v Speaker 1>do have three questions today from listeners, and so that

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<v Speaker 1>is the topic of today's podcast. To be on the podcast,

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<v Speaker 1>we'll be talking about listener questions five point five point

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<v Speaker 1>one five point one because we because we just answered

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<v Speaker 1>Patrick's questions, so we got to add a little that's right.

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<v Speaker 1>We're part way through this episode already. Um, that's right.

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<v Speaker 1>We'll be answering questions about electrons, about space, about stars,

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<v Speaker 1>about black holes, questions from far away, and questions from

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<v Speaker 1>surprisingly nearby. Yeah, and we might even know the answer

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<v Speaker 1>to some of these questions this time, and if we don't,

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<v Speaker 1>will speculate hilariously. All right, let's jump right into it. Daniel, there,

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<v Speaker 1>Our first question today is from this really pretty cool guy,

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<v Speaker 1>fun guy, one of maybe one of my favorite people,

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<v Speaker 1>has a great dad. Yeah, so this is a question

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<v Speaker 1>from Oliver from southern California. What if for whole solar

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<v Speaker 1>system is in a black hole and we don't notice? Wow,

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<v Speaker 1>that's a deep question. His voice sounds a little familiar

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<v Speaker 1>to me. Yeah. What a what a smart sounding little kid.

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<v Speaker 1>He sounds like he might grow up to be a cartoonist.

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<v Speaker 1>Well not if he's that smart, hopefully. So yeah, that's

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<v Speaker 1>my son who just asked that question in and he

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<v Speaker 1>just turned to me one day, Well, what happened? What?

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<v Speaker 1>He was reading our book? So we, Daniel and I

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<v Speaker 1>wrote a book called We Have No Idea, A Guide

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<v Speaker 1>to the Unknown Universe, available now in Amazon dot com.

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<v Speaker 1>And and you can verify it's been read by at

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<v Speaker 1>least one person since your son is reading it. That's right,

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<v Speaker 1>that's right. He's under age, but he still counts as

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<v Speaker 1>a person. He's nine years old, and so he's been

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<v Speaker 1>reading our book and I always kind of wonder how

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<v Speaker 1>much of it he's getting. You know, he's nine, he's

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<v Speaker 1>in third grade. Um, but he seems to be enjoying it,

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<v Speaker 1>and he keeps reading it, and so one day he

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<v Speaker 1>just turned to me and he asked me this question, right,

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<v Speaker 1>and what do you think is behind the question? What

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<v Speaker 1>do you think he's wondering? Explain the question to me?

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<v Speaker 1>Even explain my son do a deep dive. If I

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<v Speaker 1>knew that answer, Daniel, if I could explain my son,

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<v Speaker 1>my parenting experience would be so much. You know, I

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<v Speaker 1>thought it was really interesting. One part of his question says,

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<v Speaker 1>what if our whole solar system is in a black hole? Cool? Fascinating, Yeah,

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<v Speaker 1>But then he says, and we don't don't even notice?

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<v Speaker 1>Like I think that taps into you know, is the

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<v Speaker 1>universe different from how we expected? Is it possible that

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<v Speaker 1>we think we're living in universe X, but we're actually

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<v Speaker 1>living in universe? Why? You know? I think he was

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<v Speaker 1>probably kind of reading about black holes and he just

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<v Speaker 1>kind of wondered, like, what what if? What if we're

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<v Speaker 1>inside of a black hole? Is that possible? Like could

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<v Speaker 1>the universe? Or or like could could a solar system

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<v Speaker 1>exists inside of a black hole? And you know we

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<v Speaker 1>don't even know it? Yeah, And I think there's something

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<v Speaker 1>wonderful there about the feeling that maybe, you know, the

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<v Speaker 1>universe could be revealed to be totally different from what

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<v Speaker 1>you expected, because that's precisely happened a lot of times

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<v Speaker 1>in history, right, we thought, oh, the universe works this way. Nope,

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<v Speaker 1>it's totally different from what you imagined. And those are

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<v Speaker 1>the best moments in physics. So to hear your son

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<v Speaker 1>like sort of wondering if he's coming to that realization

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<v Speaker 1>him self, or wondering if this kind of realization is

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<v Speaker 1>around the corner, that's fantastic. He's been bitten by the

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<v Speaker 1>physics bug, so be careful. Oh no, he's gonna be

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<v Speaker 1>like Spider Man. Well that's only if he's bitten by

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<v Speaker 1>a radioactive physicist. Okay, radioactive. Well I grew up in

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<v Speaker 1>Los Alamos, so maybe I'm especially radioactive. But I'll do

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<v Speaker 1>my best not to not to about your son. Yeah,

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<v Speaker 1>but let's break it down. Um, it's interesting question. And

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<v Speaker 1>you know, something that's important to think about is sort

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<v Speaker 1>of the size of a black hole, like, could our

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<v Speaker 1>entire solar system fit into a black hole? Well? Right,

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<v Speaker 1>the size of a black hole is really we can

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<v Speaker 1>usually consider that to be the size of the event

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<v Speaker 1>horizon that's the point, right, the black style. Yeah, like

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<v Speaker 1>the point return. Look at a black hole, it would

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<v Speaker 1>look like a black sort of sphere, and so the

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<v Speaker 1>size of that sphere, that's the size of the black yeah. Yeah,

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<v Speaker 1>And if you go past that point, you can't escape, right.

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<v Speaker 1>And nobody knows what's inside of a black hole, but

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<v Speaker 1>we know how to calculate the size of the horizon.

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<v Speaker 1>It's determined just by the amount of stuff in the

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<v Speaker 1>black hole. So the more mass in the black hole,

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<v Speaker 1>the stronger the gravitational pull. The farther away it can

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<v Speaker 1>grab stuff and never let go, right, So the size

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<v Speaker 1>of the black hole is determined by its mass. So

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<v Speaker 1>how much stuff is in our solar system? Well, basically

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<v Speaker 1>the first approximation our solar system is just a soun.

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<v Speaker 1>Like the rest of the stuff in the solar system Jupiter, Mars,

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<v Speaker 1>me you hamsters, all that stuff is negligible. It's a

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<v Speaker 1>tiny fraction of the mass of the solar system. So

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<v Speaker 1>basically you can ask, like, if you had a black

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<v Speaker 1>hole with the mass of our Sun, how far away

0:12:38.160 --> 0:12:40.800
<v Speaker 1>would the event horizon B would it be out past

0:12:40.920 --> 0:12:43.000
<v Speaker 1>the edge of the black of the solar system? Is

0:12:43.040 --> 0:12:45.800
<v Speaker 1>it possible to fit a solar system in a black

0:12:45.840 --> 0:12:48.560
<v Speaker 1>hole that has the mass of our Sun. It's sort

0:12:48.559 --> 0:12:51.160
<v Speaker 1>of the way I interpret the question. So you're interpreting

0:12:51.200 --> 0:12:56.120
<v Speaker 1>the question as could our solar system be a black hole? Yeah? Exactly?

0:12:56.200 --> 0:12:58.720
<v Speaker 1>Could we be inside a black hole right now? Is

0:12:58.720 --> 0:13:01.280
<v Speaker 1>there enough room in a black hole with the mass

0:13:01.320 --> 0:13:05.240
<v Speaker 1>of the Sun to fit the entire solar system? So

0:13:05.360 --> 0:13:08.400
<v Speaker 1>could we be in a hole where the only thing

0:13:08.400 --> 0:13:11.800
<v Speaker 1>inside of it is our solar system? Yeah? Exactly exactly

0:13:11.880 --> 0:13:13.719
<v Speaker 1>is how you're interrupting the question. And the answer to

0:13:13.760 --> 0:13:17.800
<v Speaker 1>that is no, Because a black hole that has only

0:13:17.840 --> 0:13:20.679
<v Speaker 1>the mass of our sun, the event horizon would only

0:13:20.760 --> 0:13:24.240
<v Speaker 1>be three kilometers from the center of the Sun, and

0:13:24.320 --> 0:13:27.040
<v Speaker 1>so that definitely wouldn't be big enough to have the

0:13:27.080 --> 0:13:29.240
<v Speaker 1>whole solar system in it, because the solar system is

0:13:29.280 --> 0:13:33.360
<v Speaker 1>a lot more than three kilometers. It's one billion kilometers wide.

0:13:33.400 --> 0:13:35.000
<v Speaker 1>So we couldn't be in a black hole where the

0:13:35.040 --> 0:13:38.480
<v Speaker 1>only thing in it was our solar system. But is

0:13:38.520 --> 0:13:42.000
<v Speaker 1>it possible that we are that our solar system is

0:13:42.120 --> 0:13:44.880
<v Speaker 1>inside of somebody else's black hole? You know what I mean? Like,

0:13:45.880 --> 0:13:48.199
<v Speaker 1>maybe there's a black hole out there with a lot

0:13:48.200 --> 0:13:51.439
<v Speaker 1>of mass inside of it and we are just inside

0:13:51.440 --> 0:13:54.439
<v Speaker 1>of the event horizon of that black hole floating around. Yeah,

0:13:54.520 --> 0:13:57.959
<v Speaker 1>that's possible. Right, Let's let's consider that for a moment. So,

0:13:58.040 --> 0:14:01.960
<v Speaker 1>what if there's a really ends blobs somewhere else sort

0:14:02.000 --> 0:14:05.120
<v Speaker 1>of nearby, and that makes a black hole that's big

0:14:05.240 --> 0:14:08.440
<v Speaker 1>enough to encompass us, and we're inside that black hole

0:14:08.640 --> 0:14:13.080
<v Speaker 1>right right right, Well that's possible, but it's difficult to

0:14:13.120 --> 0:14:16.400
<v Speaker 1>imagine because such a huge mass would have a big

0:14:16.440 --> 0:14:19.200
<v Speaker 1>effect on us. You know, if there was a like

0:14:19.360 --> 0:14:21.960
<v Speaker 1>if there's a really big mass somewhere else inside our

0:14:21.960 --> 0:14:25.000
<v Speaker 1>Solar system next to the Sun, like an invisible huge

0:14:25.040 --> 0:14:28.240
<v Speaker 1>blob of dark matter, that that made their enough mass

0:14:28.240 --> 0:14:30.440
<v Speaker 1>so that the black hole was big enough, we would

0:14:30.480 --> 0:14:33.280
<v Speaker 1>definitely notice that that would affect the orbit of the planets.

0:14:33.800 --> 0:14:35.800
<v Speaker 1>What if there was another big mass kind of far

0:14:35.880 --> 0:14:39.000
<v Speaker 1>away but close enough that we were still inside the

0:14:39.040 --> 0:14:43.120
<v Speaker 1>event horizon, Well, you're talking about still really strong gravity.

0:14:43.400 --> 0:14:47.600
<v Speaker 1>So it's hard to imagine having some enormously powerful gravitational

0:14:47.640 --> 0:14:51.320
<v Speaker 1>attractor nearby and not having it disturbed like the orbits

0:14:51.360 --> 0:14:54.560
<v Speaker 1>of the planets or even just tossing of baseballs and

0:14:54.560 --> 0:14:56.880
<v Speaker 1>all sorts of stuff. So I think if you were

0:14:56.880 --> 0:14:59.640
<v Speaker 1>inside a black hole that was big enough to hold

0:14:59.640 --> 0:15:02.160
<v Speaker 1>a solar system, it would have to have a huge mass,

0:15:02.520 --> 0:15:05.360
<v Speaker 1>and that mass would definitely be noticeable. It would affect

0:15:05.400 --> 0:15:07.480
<v Speaker 1>the way things move on Earth, would it, though, Because

0:15:07.520 --> 0:15:10.920
<v Speaker 1>you know, like um so so our our solar system

0:15:11.200 --> 0:15:14.040
<v Speaker 1>is moving around a galaxy, right, Like, a galaxy has

0:15:14.040 --> 0:15:17.760
<v Speaker 1>a lot of mass and um and it's huge, and

0:15:17.840 --> 0:15:19.400
<v Speaker 1>there's a lot there's a huge black hole in the

0:15:19.440 --> 0:15:22.920
<v Speaker 1>center of the galaxy, but it's not really affecting us

0:15:23.440 --> 0:15:27.240
<v Speaker 1>in a local level, right, Like that gravity is kind

0:15:27.280 --> 0:15:30.160
<v Speaker 1>of spinning us around the galaxy, but it's not really

0:15:30.400 --> 0:15:33.600
<v Speaker 1>changing the orbits of the planets around the Sun, that's right. Yeah,

0:15:33.640 --> 0:15:35.400
<v Speaker 1>And that black hole in the center of the galaxy

0:15:35.640 --> 0:15:38.560
<v Speaker 1>is really massive and it's pretty big, but it's also

0:15:38.680 --> 0:15:42.480
<v Speaker 1>super duper duper duper far away. Right. Any black hole

0:15:42.480 --> 0:15:45.800
<v Speaker 1>that's either near enough to include us or far away

0:15:45.840 --> 0:15:49.760
<v Speaker 1>but huge enough to include us still would definitely affect

0:15:49.880 --> 0:15:52.479
<v Speaker 1>the gravitational poll But you know, I haven't done the calculation.

0:15:53.080 --> 0:15:57.240
<v Speaker 1>There is one configuration I imagine though. Imagine our entire

0:15:57.280 --> 0:16:01.800
<v Speaker 1>solar system and then it's surrounded by some enormously dense

0:16:01.840 --> 0:16:06.520
<v Speaker 1>sphere of material. Okay, if you're inside a sphere of material,

0:16:06.800 --> 0:16:09.760
<v Speaker 1>then the gravitational pull of that stuff doesn't affect you

0:16:09.840 --> 0:16:13.000
<v Speaker 1>at all, right, because it all balances out. Is enough

0:16:13.040 --> 0:16:15.520
<v Speaker 1>stuff on the left to balance the stuff on the right.

0:16:16.000 --> 0:16:17.840
<v Speaker 1>Just like that episode we talked about where you jump

0:16:17.920 --> 0:16:20.480
<v Speaker 1>inside the Earth. Once you get to the center of

0:16:20.480 --> 0:16:24.920
<v Speaker 1>the Earth, is no gravitational force from the stuff around you. Right, Well,

0:16:25.040 --> 0:16:28.160
<v Speaker 1>if you have to spear a super dense material surrounding

0:16:28.200 --> 0:16:32.360
<v Speaker 1>the Solar System, right, then that might be enough to

0:16:32.400 --> 0:16:35.600
<v Speaker 1>create a black hole, right that we would be inside of.

0:16:36.000 --> 0:16:39.080
<v Speaker 1>We wouldn't feel the gravitational force because we would be

0:16:39.200 --> 0:16:42.400
<v Speaker 1>inside all the stuff. It would be all around us. Yeah,

0:16:42.560 --> 0:16:44.640
<v Speaker 1>that's what I mean. Yeah, yeah, but they have to

0:16:44.680 --> 0:16:48.520
<v Speaker 1>be perfectly distributed, right. And the only reason that there's

0:16:48.600 --> 0:16:51.400
<v Speaker 1>one reason to think that's not the case, and that's

0:16:51.440 --> 0:16:54.080
<v Speaker 1>that we have sent stuff outside the Solar System, Like

0:16:54.160 --> 0:16:57.240
<v Speaker 1>we launched probes and they're floating off into space and

0:16:57.280 --> 0:17:00.040
<v Speaker 1>we're watching them and they haven't like banged up and

0:17:00.280 --> 0:17:03.600
<v Speaker 1>the wall of some hugely massive blob of stuff. But

0:17:03.640 --> 0:17:06.560
<v Speaker 1>what have you expand that idea even further to encompass

0:17:06.760 --> 0:17:11.520
<v Speaker 1>the whole observable universe. It is possible then that we

0:17:11.600 --> 0:17:14.400
<v Speaker 1>could be inside of a black hole. Yeah, yeah, it's

0:17:14.440 --> 0:17:18.640
<v Speaker 1>possible the entire observable universe is inside a black hole. Yes,

0:17:19.760 --> 0:17:21.520
<v Speaker 1>you can't rule that out. How do you feel about

0:17:21.520 --> 0:17:25.080
<v Speaker 1>saying that on a public record, Um, I wonder if

0:17:25.080 --> 0:17:29.080
<v Speaker 1>any of my colleagues are listening. No, I think it's awesome.

0:17:29.400 --> 0:17:32.080
<v Speaker 1>You would be surprised. I think it's awesome, And I

0:17:32.119 --> 0:17:35.359
<v Speaker 1>think sometimes these awesome questions come from the minds of children,

0:17:35.400 --> 0:17:38.040
<v Speaker 1>And that's why I hope that people are listening to

0:17:38.040 --> 0:17:41.040
<v Speaker 1>the podcast with their kids, because kids ask amazing questions

0:17:41.200 --> 0:17:43.119
<v Speaker 1>that make us think about things we otherwise would have

0:17:43.119 --> 0:17:47.320
<v Speaker 1>totally discarded that might actually be reality. Well, so that's

0:17:47.320 --> 0:17:49.320
<v Speaker 1>so that's the answer. The answer is that it is

0:17:49.359 --> 0:17:52.160
<v Speaker 1>totally possible that we are inside of a black hole

0:17:52.240 --> 0:17:54.639
<v Speaker 1>and not knowing. Yeah, but I think our whole universe

0:17:54.640 --> 0:17:56.239
<v Speaker 1>would have to be inside the black hole, not just

0:17:56.280 --> 0:17:58.760
<v Speaker 1>the solar system. But yeah, that's a pretty small conviat

0:17:58.800 --> 0:18:00.920
<v Speaker 1>for it for a yes answer to that question, isn't

0:18:00.920 --> 0:18:03.280
<v Speaker 1>that sort of a theory out there that were like

0:18:03.359 --> 0:18:06.399
<v Speaker 1>the whole universe are are inside the whole universe inside

0:18:06.440 --> 0:18:08.280
<v Speaker 1>of a black hole, and there are other black holes

0:18:08.320 --> 0:18:10.720
<v Speaker 1>and stuff. Like that or is that pretty fringe? I

0:18:10.720 --> 0:18:13.080
<v Speaker 1>think it is the theory out there, and it's pretty fringe,

0:18:13.119 --> 0:18:16.760
<v Speaker 1>But it's also totally possible, you know, like we really

0:18:16.800 --> 0:18:19.119
<v Speaker 1>just we don't know what's going on inside black holes?

0:18:19.160 --> 0:18:22.080
<v Speaker 1>Are there little universes in there? You know? The inside

0:18:22.080 --> 0:18:26.000
<v Speaker 1>of a black hole is totally disconnected from the space

0:18:26.000 --> 0:18:27.920
<v Speaker 1>that we live in, right, Like there's no way to

0:18:28.000 --> 0:18:30.919
<v Speaker 1>get from here to there, right, That's why that's how

0:18:30.960 --> 0:18:33.240
<v Speaker 1>a black hole works, even like can't escape it, not

0:18:33.320 --> 0:18:35.520
<v Speaker 1>because it's like slowing down the light as it tries

0:18:35.560 --> 0:18:38.119
<v Speaker 1>to leave, but because it's bent space in such a

0:18:38.160 --> 0:18:40.760
<v Speaker 1>way that there's just no path out, like just zooming

0:18:40.760 --> 0:18:43.639
<v Speaker 1>around inside the black hole. So in some ways you

0:18:43.640 --> 0:18:45.119
<v Speaker 1>can think of it as sort of like a different

0:18:45.240 --> 0:18:49.080
<v Speaker 1>universe disconnected from our our space, and so you can

0:18:49.119 --> 0:18:51.600
<v Speaker 1>imagine then anything that goes on in there. And uh,

0:18:52.000 --> 0:18:56.399
<v Speaker 1>when experiments can't constrain things, theorists minds tend to go wild,

0:18:56.560 --> 0:18:58.639
<v Speaker 1>and so they think about all sorts of crazy stuff

0:18:58.680 --> 0:19:01.879
<v Speaker 1>that could be inside there, insing bears or entire universes.

0:19:02.240 --> 0:19:05.440
<v Speaker 1>Crazy scientists and nine year old boys whom I grew

0:19:05.520 --> 0:19:08.159
<v Speaker 1>up to be crazy scientists. All right, Well, that's the

0:19:08.200 --> 0:19:12.240
<v Speaker 1>answered for Oliver's son of Jorge, and I'll let him

0:19:12.240 --> 0:19:17.440
<v Speaker 1>know if he has a good sum he stumped the physicists. Yeah,

0:19:17.480 --> 0:19:20.200
<v Speaker 1>it's a great question. If he was Icelandic, his last

0:19:20.240 --> 0:19:26.439
<v Speaker 1>name would be or Hasten exactly. All right, Well, we

0:19:26.520 --> 0:19:28.960
<v Speaker 1>have two other awesome questions that we are going to

0:19:29.000 --> 0:19:33.640
<v Speaker 1>answer about electron identity. I guess is that is that

0:19:33.920 --> 0:19:36.520
<v Speaker 1>we would be the right topic and also about dark

0:19:36.600 --> 0:19:42.200
<v Speaker 1>Matter stars, which sounds like a heavy battle band last

0:19:42.320 --> 0:19:45.200
<v Speaker 1>science fiction movie. So stay tuned, will be right back.

0:19:58.080 --> 0:20:01.000
<v Speaker 1>Al Right, we are back answering list are questions, and

0:20:01.080 --> 0:20:04.679
<v Speaker 1>so our next question comes from Yugi from the Netherlands,

0:20:04.920 --> 0:20:10.520
<v Speaker 1>and he is wondering if electrons have identity crises. That's right,

0:20:10.640 --> 0:20:13.240
<v Speaker 1>And this particular listener is something of a super fan,

0:20:13.440 --> 0:20:16.639
<v Speaker 1>writing to us on Twitter fairly often with insightful questions,

0:20:16.760 --> 0:20:18.320
<v Speaker 1>and he sent me this one and I thought, well

0:20:18.400 --> 0:20:22.360
<v Speaker 1>that's a good question, let's take it online, and so

0:20:22.520 --> 0:20:25.760
<v Speaker 1>here he is, Hi, Danielle and Jorge. My name is

0:20:25.800 --> 0:20:29.960
<v Speaker 1>Eugene Raudemake and I live in the Netherlands, hence the actions.

0:20:30.720 --> 0:20:33.240
<v Speaker 1>I'm a big fan of your morphous poticast cities, for

0:20:33.400 --> 0:20:36.920
<v Speaker 1>it makes me understand more of physics, and it makes

0:20:36.960 --> 0:20:41.439
<v Speaker 1>me think a lot about the universe in general. After

0:20:41.480 --> 0:20:45.399
<v Speaker 1>listening to your episode about quantum tunneling, the following question

0:20:45.440 --> 0:20:50.080
<v Speaker 1>came to my mind. If an electron tapt well say A,

0:20:50.560 --> 0:20:54.640
<v Speaker 1>suddenly appears in well B, how can physically still it's

0:20:54.680 --> 0:20:59.400
<v Speaker 1>actually this very same electron. I realized that I had

0:20:59.600 --> 0:21:02.679
<v Speaker 1>the both bowl empty swimming pool and the analogy in

0:21:02.760 --> 0:21:06.520
<v Speaker 1>my mind when the Christians sue appearance in my will.

0:21:07.359 --> 0:21:12.080
<v Speaker 1>Thanks for spending time answering my questions, all right, thank

0:21:12.080 --> 0:21:14.760
<v Speaker 1>you for saying this question, and also for being a

0:21:14.800 --> 0:21:18.600
<v Speaker 1>fan of the show. We really appreciate everyone listening out there. Yeah, exactly,

0:21:19.240 --> 0:21:21.919
<v Speaker 1>And uh, it's really a wonderful question, you know. To me,

0:21:21.960 --> 0:21:24.760
<v Speaker 1>it goes to the heart of like what are these particles?

0:21:24.760 --> 0:21:27.919
<v Speaker 1>What are we talking about? Um? But the way I

0:21:27.960 --> 0:21:30.920
<v Speaker 1>interpret his question is like, you haven't quite an electron

0:21:31.000 --> 0:21:34.000
<v Speaker 1>over here, and physics tells us the electron can then

0:21:34.080 --> 0:21:36.679
<v Speaker 1>later be over there. But his question is, how do

0:21:36.760 --> 0:21:40.360
<v Speaker 1>you know it's the same electron? Right, because we don't

0:21:40.359 --> 0:21:43.040
<v Speaker 1>have this sort of notion anymore of a classical path

0:21:43.080 --> 0:21:45.240
<v Speaker 1>that you can like watch a baseball fly through the

0:21:45.280 --> 0:21:48.200
<v Speaker 1>air and when a baseball, you know, when somebody hits

0:21:48.400 --> 0:21:50.919
<v Speaker 1>a home run, you watch it fly. You don't ask like,

0:21:51.080 --> 0:21:53.520
<v Speaker 1>is that the same baseball or is it suddenly swapped out?

0:21:54.080 --> 0:21:57.320
<v Speaker 1>But with quantum mechanical particles, because you can't observe them

0:21:57.359 --> 0:22:00.000
<v Speaker 1>all the way along the path, you just get these snapshots.

0:22:00.240 --> 0:22:02.000
<v Speaker 1>You can sort of wonder like, how do you know

0:22:02.080 --> 0:22:04.800
<v Speaker 1>that's the same electron? Maybe it's from another electron down

0:22:04.840 --> 0:22:06.920
<v Speaker 1>the street, right, it's just Tom or Harry or Mary

0:22:07.000 --> 0:22:09.800
<v Speaker 1>or Sally. I feel like the question is there such

0:22:09.840 --> 0:22:13.240
<v Speaker 1>a thing as an electron? Is there an electron? You

0:22:13.240 --> 0:22:16.280
<v Speaker 1>can say and follow it around and it has a

0:22:16.440 --> 0:22:19.800
<v Speaker 1>birth in a you know, journey, and then it maybe

0:22:19.840 --> 0:22:22.719
<v Speaker 1>answer at some point we can you follow an electron?

0:22:22.800 --> 0:22:25.760
<v Speaker 1>Or are we getting into identity politics now? So there's

0:22:25.800 --> 0:22:30.920
<v Speaker 1>electrons go back to where they came from physics. Yeah,

0:22:31.359 --> 0:22:36.119
<v Speaker 1>obviously we're not qualified to dive into those topics. You know,

0:22:36.160 --> 0:22:38.359
<v Speaker 1>well that's a it's a famous topic in physics, and

0:22:38.400 --> 0:22:43.399
<v Speaker 1>it's something that real physicists wonder and uh. In this

0:22:43.480 --> 0:22:46.399
<v Speaker 1>famous physicist, John Wheeler, he had this sort of moment

0:22:46.400 --> 0:22:48.159
<v Speaker 1>of insight and I don't know if he was smoking

0:22:48.160 --> 0:22:51.560
<v Speaker 1>banana peels or what. But he was wondering, like, why

0:22:51.600 --> 0:22:55.000
<v Speaker 1>do all electrons behave the same way? Like you drop

0:22:55.000 --> 0:22:57.720
<v Speaker 1>an electron in the in the circumstance, it's always going

0:22:57.800 --> 0:22:59.440
<v Speaker 1>to get repulsed in the same way. It's not like

0:22:59.800 --> 0:23:01.639
<v Speaker 1>this one's got a little bit more charge and that

0:23:01.680 --> 0:23:04.320
<v Speaker 1>one's got a little bit more mass. They're all identical.

0:23:04.320 --> 0:23:06.440
<v Speaker 1>They're not like scoops of ice cream, right, they all

0:23:06.440 --> 0:23:09.520
<v Speaker 1>have exactly the same properties. And he had this moment

0:23:09.520 --> 0:23:12.200
<v Speaker 1>of in said he thought, wait a second, maybe there

0:23:12.320 --> 0:23:16.280
<v Speaker 1>is just one electron. These are all the same electron.

0:23:18.160 --> 0:23:21.520
<v Speaker 1>What what do you mean, like the electrons in my

0:23:21.600 --> 0:23:24.800
<v Speaker 1>body and the ones in your body, they're all the same. Yes, yes,

0:23:24.960 --> 0:23:28.399
<v Speaker 1>sort of um, And I think I think that's actually

0:23:28.400 --> 0:23:32.080
<v Speaker 1>sort of the answer is that the electron is not

0:23:32.240 --> 0:23:36.200
<v Speaker 1>really um a particle that has an identity. It's sort

0:23:36.240 --> 0:23:40.000
<v Speaker 1>of like a state of mind or a state of matter, right,

0:23:40.119 --> 0:23:44.240
<v Speaker 1>because these days we don't think quantum mechanically about particles

0:23:44.359 --> 0:23:47.240
<v Speaker 1>as the fundamental basis of the universe. Instead we think

0:23:47.280 --> 0:23:51.200
<v Speaker 1>of fields, right, and particles are just excited states of

0:23:51.240 --> 0:23:53.560
<v Speaker 1>the field. It's sort of like when you look at

0:23:53.560 --> 0:23:56.440
<v Speaker 1>the ocean, you know, and you've tried to follow a wave. Right,

0:23:56.800 --> 0:23:59.080
<v Speaker 1>A wave is not the basic unit of the ocean.

0:23:59.119 --> 0:24:01.879
<v Speaker 1>It's the water. Right. The wave is just like, you know,

0:24:01.960 --> 0:24:04.160
<v Speaker 1>the ocean has got excited a little bit by the wind,

0:24:04.200 --> 0:24:06.200
<v Speaker 1>and it comes and it goes, and there's more waves

0:24:06.200 --> 0:24:09.280
<v Speaker 1>behind it. It's just it's just the motion of the ocean.

0:24:09.400 --> 0:24:12.360
<v Speaker 1>And that's right exactly. And so in that same way,

0:24:12.400 --> 0:24:14.960
<v Speaker 1>you can think of electrons. Not a's like, here's a

0:24:14.960 --> 0:24:17.520
<v Speaker 1>little chunk of matter, a little like piece of the

0:24:17.600 --> 0:24:20.399
<v Speaker 1>universe we're gonna follow around. But it's just like a

0:24:20.440 --> 0:24:24.159
<v Speaker 1>momentary excitation of this sort of hard to think about

0:24:24.240 --> 0:24:28.040
<v Speaker 1>thing called the electron field which fills the universe. And

0:24:28.040 --> 0:24:30.080
<v Speaker 1>when it gets a little bit of energy somewhere, you

0:24:30.160 --> 0:24:33.239
<v Speaker 1>call that an electron. It's not an object. It's kind

0:24:33.280 --> 0:24:36.320
<v Speaker 1>of a wiggle of an object. Yes, exactly, it's a

0:24:36.320 --> 0:24:39.400
<v Speaker 1>wiggle of an object. And you know, this goes back

0:24:39.400 --> 0:24:42.040
<v Speaker 1>to that other question we tried to answer. It's a photon,

0:24:42.160 --> 0:24:44.800
<v Speaker 1>a particle, or a wave, for example, And I think

0:24:44.800 --> 0:24:46.879
<v Speaker 1>I said on that podcast that it's sort of neither

0:24:47.040 --> 0:24:49.280
<v Speaker 1>and sort of both, and really it's something else weird

0:24:49.320 --> 0:24:53.600
<v Speaker 1>and fundamental that we just cannot understand by making analogies, right,

0:24:54.000 --> 0:24:57.240
<v Speaker 1>analogies from our macroscopic experience. Things that we're familiar with

0:24:57.640 --> 0:25:01.199
<v Speaker 1>just don't work because we've never seen anything like that before. Well,

0:25:01.160 --> 0:25:03.120
<v Speaker 1>it turns out you can apply the same idea as

0:25:03.119 --> 0:25:05.919
<v Speaker 1>to an electron also, right, an electron is both a

0:25:05.920 --> 0:25:09.720
<v Speaker 1>particle and a wave and both and neither and something

0:25:09.760 --> 0:25:13.040
<v Speaker 1>else totally weird. It's really just the excitation of a

0:25:13.119 --> 0:25:16.679
<v Speaker 1>quantum field. And and the reason, the reason actually that

0:25:16.720 --> 0:25:19.080
<v Speaker 1>we came up with quantum fields, the reason that this

0:25:19.119 --> 0:25:23.679
<v Speaker 1>whole development is progress, right and not just confusion, is

0:25:23.680 --> 0:25:26.080
<v Speaker 1>that it helps us think about the way particles are

0:25:26.119 --> 0:25:29.960
<v Speaker 1>created and destroyed. Because when electron is flying through um

0:25:30.080 --> 0:25:33.960
<v Speaker 1>the universe, it doesn't just sit around happily. It generates photons,

0:25:34.000 --> 0:25:37.000
<v Speaker 1>and those photons turned into electrons and positrons which turned

0:25:37.000 --> 0:25:40.520
<v Speaker 1>back into photons. Every electron is actually surrounded by like

0:25:40.600 --> 0:25:43.960
<v Speaker 1>a fuzz ball of virtual particles, photons and electrons and

0:25:43.960 --> 0:25:46.280
<v Speaker 1>things popping in out of the vacuum. What do you mean,

0:25:46.320 --> 0:25:51.159
<v Speaker 1>like an electron is not always an electron. It's constantly

0:25:51.320 --> 0:25:55.240
<v Speaker 1>kind of fuzzy and morphing and changing. Yes, exactly, it's

0:25:55.280 --> 0:25:59.080
<v Speaker 1>constantly morphing and changing and it's surrounded by a ball

0:25:59.160 --> 0:26:03.720
<v Speaker 1>of like almost an infinite number of low energy particles

0:26:03.720 --> 0:26:06.679
<v Speaker 1>that are being created and destroyed around it. Right, And

0:26:06.720 --> 0:26:10.080
<v Speaker 1>so we came up with this alternative mathematical formulation quantum

0:26:10.119 --> 0:26:13.520
<v Speaker 1>field theory, because it's really hard to follow the path

0:26:13.560 --> 0:26:17.479
<v Speaker 1>of an individual particle through this sort of probabilistic storm

0:26:17.560 --> 0:26:20.119
<v Speaker 1>of things that's happening, and it's much easier to just

0:26:20.119 --> 0:26:23.000
<v Speaker 1>think about the field that's generating all these particles. And

0:26:23.040 --> 0:26:25.920
<v Speaker 1>then a particle creation and destruction is much more natural

0:26:26.359 --> 0:26:29.120
<v Speaker 1>in quantum field theory than an old quantum mechanics where

0:26:29.119 --> 0:26:32.239
<v Speaker 1>we try to track follow an individual particle as if

0:26:32.280 --> 0:26:34.159
<v Speaker 1>it was a baseball. So we have to sort of

0:26:34.359 --> 0:26:38.040
<v Speaker 1>let go of this whole idea of particles having identities,

0:26:38.280 --> 0:26:41.719
<v Speaker 1>particles having paths, um and just think of them as

0:26:41.960 --> 0:26:45.280
<v Speaker 1>momentary oscillations in this field. Well, I think there's several

0:26:45.359 --> 0:26:50.080
<v Speaker 1>questions here, like, you know, maybe maybe you he was

0:26:50.240 --> 0:26:53.639
<v Speaker 1>also thinking of the wave analogy maybe, and so maybe

0:26:53.680 --> 0:26:56.520
<v Speaker 1>his question was, you know, just like you can follow

0:26:56.600 --> 0:26:59.080
<v Speaker 1>a wave in the ocean, you know, if you if

0:26:59.080 --> 0:27:01.840
<v Speaker 1>I make a ripple in the in the lake or something,

0:27:01.960 --> 0:27:04.920
<v Speaker 1>or you've even wave is made out into the ocean.

0:27:04.960 --> 0:27:07.760
<v Speaker 1>You can you can kind of follow that wave, right, like,

0:27:07.840 --> 0:27:12.119
<v Speaker 1>that's wave A. I'm gonna call it Sally, and you

0:27:12.119 --> 0:27:15.919
<v Speaker 1>can follow Sally as it moves across the Pacific, right,

0:27:16.000 --> 0:27:18.880
<v Speaker 1>you sort of can. But what if Sally looks exactly

0:27:18.920 --> 0:27:22.240
<v Speaker 1>like all the other waves, and there's billions of them,

0:27:22.320 --> 0:27:25.280
<v Speaker 1>and you look away, and then you look back and

0:27:25.320 --> 0:27:30.480
<v Speaker 1>you wonder which of those waves is Sally. That's the

0:27:30.520 --> 0:27:33.440
<v Speaker 1>situation where the one that um like, if I see

0:27:33.480 --> 0:27:35.280
<v Speaker 1>it at point A and I see at point B

0:27:35.600 --> 0:27:39.240
<v Speaker 1>one second later, well that's his question, right, the one

0:27:39.280 --> 0:27:42.600
<v Speaker 1>that's a point C another second later, basically right, could

0:27:42.600 --> 0:27:44.400
<v Speaker 1>be or could be there along the way got turned

0:27:44.400 --> 0:27:46.879
<v Speaker 1>into something else and then got turned back into a wave,

0:27:46.960 --> 0:27:49.919
<v Speaker 1>And is it the same wave then? But it almost

0:27:49.960 --> 0:27:54.400
<v Speaker 1>always is, isn't it? Like? Do electrons really just transformed

0:27:54.400 --> 0:27:58.280
<v Speaker 1>to something else constantly when we're not looking, constantly, even

0:27:58.280 --> 0:28:02.520
<v Speaker 1>while we're looking, electrons are constantly influx Yes, exactly. You

0:28:02.520 --> 0:28:04.520
<v Speaker 1>know there's that even the ones that in my body,

0:28:04.680 --> 0:28:06.920
<v Speaker 1>even the ones in your body, they're not special, sorry

0:28:06.920 --> 0:28:10.959
<v Speaker 1>to inform you. Um, you know, there's that ancient philosophical question, right,

0:28:11.000 --> 0:28:14.080
<v Speaker 1>there's some some ancient Greek ship, and every time it

0:28:14.119 --> 0:28:16.840
<v Speaker 1>comes into harbor that it's lost a piece and they

0:28:16.920 --> 0:28:19.240
<v Speaker 1>repair it, and then after five years there are no

0:28:19.400 --> 0:28:21.760
<v Speaker 1>pieces of the original ship, and they wonder, like, is

0:28:21.800 --> 0:28:24.160
<v Speaker 1>it still that same ship? You know, if it's made

0:28:24.160 --> 0:28:26.840
<v Speaker 1>out of all new pieces? Um, And it's sort of

0:28:26.880 --> 0:28:30.800
<v Speaker 1>that question, but it's the particle version of that question.

0:28:31.480 --> 0:28:33.640
<v Speaker 1>And uh, wait, what if it rides the same wave

0:28:33.720 --> 0:28:42.280
<v Speaker 1>though that the Greeks mine? Yeah, exactly, And so I'd

0:28:42.280 --> 0:28:43.960
<v Speaker 1>say in this in the same way, there there is

0:28:44.000 --> 0:28:46.960
<v Speaker 1>really no particle identity. Um, I don't I don't know

0:28:47.000 --> 0:28:48.800
<v Speaker 1>that I've smoked enough. But An appeals to say they're

0:28:48.800 --> 0:28:51.600
<v Speaker 1>all the same electron But I think sort of what

0:28:51.640 --> 0:28:54.959
<v Speaker 1>he's saying is that they're all manifestations of the same field. Right,

0:28:55.000 --> 0:28:59.160
<v Speaker 1>there's really just one electron field and it appears and

0:28:59.200 --> 0:29:01.360
<v Speaker 1>lots of different places is in the universe. But then

0:29:01.480 --> 0:29:04.960
<v Speaker 1>what's really going on? Because you know, I feel pretty consistent,

0:29:05.360 --> 0:29:08.840
<v Speaker 1>you know, like I am this way sort of now

0:29:08.920 --> 0:29:12.720
<v Speaker 1>and and I'm sort of the same way a second ago.

0:29:12.800 --> 0:29:16.240
<v Speaker 1>I think that's my perception. Are you saying that, you

0:29:16.280 --> 0:29:18.920
<v Speaker 1>know I could have changed into something totally different between

0:29:18.960 --> 0:29:22.280
<v Speaker 1>now and the next second, that I am conscious about, yes,

0:29:22.480 --> 0:29:25.760
<v Speaker 1>But the jorhan nous is not about the stuff that

0:29:25.800 --> 0:29:28.959
<v Speaker 1>you're made up of, but the arrangement of those particles. Right,

0:29:29.080 --> 0:29:32.040
<v Speaker 1>just like that ship is not about the pieces of

0:29:32.040 --> 0:29:34.080
<v Speaker 1>wood that went into it, but how they're put together

0:29:34.200 --> 0:29:36.400
<v Speaker 1>and what it's doing, and you know how it spends

0:29:36.400 --> 0:29:39.080
<v Speaker 1>its time. And so in the same way, you are

0:29:39.120 --> 0:29:42.920
<v Speaker 1>a constantly frothing mass of quantum mechanical particles. But that's

0:29:42.920 --> 0:29:45.400
<v Speaker 1>not what makes you you. What makes you use the

0:29:45.440 --> 0:29:47.840
<v Speaker 1>way they're arranged and the way they live their life. Well,

0:29:47.880 --> 0:29:52.880
<v Speaker 1>I am a constant frothing mass of something. Sure, it's

0:29:52.920 --> 0:29:55.480
<v Speaker 1>a really hard question. And you know, this is a

0:29:55.560 --> 0:29:59.560
<v Speaker 1>question which is definitely on the philosophy side of the threshold.

0:29:59.760 --> 0:30:02.760
<v Speaker 1>And something I love about physics is that it bumps

0:30:02.840 --> 0:30:07.080
<v Speaker 1>up against philosophy so often because they're deep consequences to

0:30:07.120 --> 0:30:10.239
<v Speaker 1>the answers of physics questions. And so I've always been

0:30:10.280 --> 0:30:15.320
<v Speaker 1>really interested in in the philosophical implications of particle physics. Um,

0:30:15.400 --> 0:30:17.640
<v Speaker 1>but I have to say it's not something that most

0:30:17.680 --> 0:30:20.959
<v Speaker 1>of us, most of us particle physicists, are actually qualified

0:30:21.000 --> 0:30:24.160
<v Speaker 1>to talk about, even though we do pontificate long windedly

0:30:24.200 --> 0:30:26.280
<v Speaker 1>on it. Oh, I see. It's it's one of these

0:30:26.360 --> 0:30:29.520
<v Speaker 1>questions that the answer is kind of like it depends

0:30:29.520 --> 0:30:34.400
<v Speaker 1>on what the definition of is isuly I have to

0:30:34.400 --> 0:30:38.160
<v Speaker 1>go there, but I think it applies in this case.

0:30:38.760 --> 0:30:41.240
<v Speaker 1>Yeah right, It's sort of like it depends on what

0:30:41.320 --> 0:30:43.680
<v Speaker 1>you mean by having an identity or being the same

0:30:43.720 --> 0:30:47.040
<v Speaker 1>electron exactly, you can dig into that forever and smoke

0:30:47.120 --> 0:30:50.920
<v Speaker 1>manin appeals and not necessarily make any progress exactly. Yeah,

0:30:51.040 --> 0:30:54.120
<v Speaker 1>or cigars. But it's a really fun question, So thank

0:30:54.160 --> 0:30:56.280
<v Speaker 1>you for asking it. Yeah, well, what's the What would

0:30:56.280 --> 0:30:59.200
<v Speaker 1>you say is the answer? Then? Do electrons have an

0:30:59.240 --> 0:31:02.240
<v Speaker 1>identity or can you have the same electro on? The

0:31:02.240 --> 0:31:04.480
<v Speaker 1>answer seems to be I would say no. I would

0:31:04.480 --> 0:31:08.239
<v Speaker 1>say identity is a macroscopic quality that we like to

0:31:08.280 --> 0:31:10.440
<v Speaker 1>attribute to things because we're used to it, because we're

0:31:10.520 --> 0:31:14.880
<v Speaker 1>familiar with it. We expected to tom. We expect also

0:31:14.960 --> 0:31:17.680
<v Speaker 1>tiny particles to have it, but they don't and and

0:31:17.720 --> 0:31:20.160
<v Speaker 1>so I think it's odd and uh, and it's it

0:31:20.680 --> 0:31:22.920
<v Speaker 1>tells us more about how we think than about how

0:31:22.960 --> 0:31:26.280
<v Speaker 1>the universe works. So you're saying, at the microscopic level,

0:31:26.320 --> 0:31:30.120
<v Speaker 1>at the individual electron level, these things we can apply

0:31:30.280 --> 0:31:35.560
<v Speaker 1>because things are just constantly changing and frothing, and yeah, exactly,

0:31:35.600 --> 0:31:37.720
<v Speaker 1>I don't think it has any meaning at the microscopic level.

0:31:37.840 --> 0:31:40.560
<v Speaker 1>All right, well, thank you hear you from the Netherlands

0:31:40.840 --> 0:31:43.200
<v Speaker 1>for that question. Please keep listening. I hope he answered

0:31:43.240 --> 0:31:47.560
<v Speaker 1>your question. Answer your question to your satisfaction. Uh So

0:31:47.680 --> 0:31:50.080
<v Speaker 1>we have one more question, and this one comes from

0:31:50.160 --> 0:31:54.720
<v Speaker 1>Mexico or Mexico about dark matter stars. But first let's

0:31:54.800 --> 0:32:10.160
<v Speaker 1>take a quick break. Al right. Our last question of

0:32:10.240 --> 0:32:14.440
<v Speaker 1>today comes from ben who is sending his question from Mexico,

0:32:15.480 --> 0:32:18.720
<v Speaker 1>and he has a question about dark matter stars. Hi,

0:32:18.800 --> 0:32:22.479
<v Speaker 1>Daniel lane J. This is Benjamin from Mexico, and I

0:32:22.600 --> 0:32:26.200
<v Speaker 1>was wondering, if the dark matter has all these gravitational

0:32:26.280 --> 0:32:30.960
<v Speaker 1>properties as the regular matter, why have an astrophysicists discovered

0:32:31.040 --> 0:32:35.040
<v Speaker 1>yet a big celestial body made of dark matter, like

0:32:35.120 --> 0:32:38.840
<v Speaker 1>a dark matter star or something big that we can

0:32:38.960 --> 0:32:42.760
<v Speaker 1>indirectly now it's there. Thank you. All right, that's a

0:32:42.800 --> 0:32:48.400
<v Speaker 1>pretty cool question. Where aren't there dark stars besides a

0:32:49.280 --> 0:32:52.960
<v Speaker 1>in comic books? I think that's a comic book villain.

0:32:53.680 --> 0:32:56.800
<v Speaker 1>Exactly it should be, yeah, exactly. Um No, it's an

0:32:56.840 --> 0:32:59.840
<v Speaker 1>awesome question, and the way I interpret it is that

0:33:00.000 --> 0:33:03.200
<v Speaker 1>he's wondering why can't we tell that dark matter is there?

0:33:03.360 --> 0:33:06.320
<v Speaker 1>Why it hasn't dark matter coalesced into some sort of

0:33:06.400 --> 0:33:09.520
<v Speaker 1>object that we could then pinpoint, Because I think he

0:33:09.880 --> 0:33:13.520
<v Speaker 1>maybe is frustrated at the sort of diffusiveness of dark matter.

0:33:13.880 --> 0:33:16.000
<v Speaker 1>We know it's there, we know it's sort of everywhere,

0:33:16.040 --> 0:33:18.120
<v Speaker 1>but we can't seem to say exactly where it is

0:33:18.160 --> 0:33:20.520
<v Speaker 1>and why not? Is that how you interpret the question?

0:33:20.560 --> 0:33:24.640
<v Speaker 1>Why does it stay so fuzzy? Yeah? Yeah, exactly. And

0:33:25.280 --> 0:33:27.200
<v Speaker 1>I think that the key thing to understand here is

0:33:27.240 --> 0:33:30.240
<v Speaker 1>remember that gravity is really really weak, and it's the

0:33:30.280 --> 0:33:32.880
<v Speaker 1>only way we can see dark matter so far. The

0:33:32.920 --> 0:33:35.760
<v Speaker 1>only way we can feel it is through its gravity,

0:33:35.840 --> 0:33:38.360
<v Speaker 1>and and so it takes a huge amount of stuff

0:33:38.560 --> 0:33:41.240
<v Speaker 1>to notice something just from gravity. Remember, the gravity is

0:33:41.240 --> 0:33:44.240
<v Speaker 1>so weak that you can feel the Earth's gravity, but

0:33:44.360 --> 0:33:47.440
<v Speaker 1>you can't feel the gravity of your car or your house,

0:33:47.520 --> 0:33:50.120
<v Speaker 1>even though there is a gravitational pull there, it takes

0:33:50.120 --> 0:33:53.120
<v Speaker 1>some huge body to even feel it. Right, Well, maybe

0:33:53.120 --> 0:33:56.280
<v Speaker 1>we should recap and a little bit about dark matter. Right,

0:33:57.240 --> 0:34:00.960
<v Speaker 1>So we know that dark matter feels gravity, right, that's

0:34:01.000 --> 0:34:03.440
<v Speaker 1>how we sort of know it's there because it's pulling

0:34:03.480 --> 0:34:07.440
<v Speaker 1>us around the galaxy. But it doesn't feel electromagnetic forces,

0:34:07.480 --> 0:34:10.160
<v Speaker 1>which means we can't see it or touch it. Right,

0:34:10.200 --> 0:34:13.000
<v Speaker 1>that's right exactly. It doesn't give off light, it doesn't

0:34:13.040 --> 0:34:15.879
<v Speaker 1>reflect light. We can't see it using any of those

0:34:15.920 --> 0:34:19.279
<v Speaker 1>normal methods that we usually used to see stuff, right,

0:34:19.360 --> 0:34:22.120
<v Speaker 1>But it does feel gravity, and so I think maybe

0:34:22.239 --> 0:34:26.200
<v Speaker 1>Ben's question is, if dark matter feels gravity, why hasn't

0:34:26.200 --> 0:34:30.960
<v Speaker 1>it clumped together out in space because it's attracted to itself, right,

0:34:31.080 --> 0:34:33.600
<v Speaker 1>isn't it attracted to itself? Dark matter is attracted to

0:34:33.600 --> 0:34:38.520
<v Speaker 1>itself by gravity, absolutely yes, and it has clumped together. Right,

0:34:38.840 --> 0:34:42.160
<v Speaker 1>dark matter is not evenly spread throughout the universe. Dark

0:34:42.200 --> 0:34:45.520
<v Speaker 1>matter has clumped together thanks to gravity, and it's formed

0:34:45.520 --> 0:34:49.560
<v Speaker 1>these big blobs. And it's, in fact only because dark

0:34:49.640 --> 0:34:53.120
<v Speaker 1>matter has clumped together to make these blobs that we

0:34:53.239 --> 0:34:56.960
<v Speaker 1>have galaxies and we are alive, because without dark matters

0:34:57.000 --> 0:35:00.320
<v Speaker 1>gravitational pull, there wouldn't be enough gravity to hold the

0:35:00.440 --> 0:35:04.000
<v Speaker 1>galaxies together. And we've done simulations and seeing that in

0:35:04.160 --> 0:35:07.440
<v Speaker 1>universities without dark matter, it takes a lot longer for

0:35:07.480 --> 0:35:11.239
<v Speaker 1>gravity to pull all this luminous stuff together to make

0:35:11.280 --> 0:35:15.000
<v Speaker 1>stars and planets and galaxies. So dark matter does make

0:35:15.239 --> 0:35:18.480
<v Speaker 1>um structure, It does make objects. But those objects are

0:35:18.600 --> 0:35:21.640
<v Speaker 1>sort of big and diffuse, and and they're sort of

0:35:21.680 --> 0:35:24.680
<v Speaker 1>the size of the galaxy. And and you might ask, well,

0:35:24.719 --> 0:35:27.480
<v Speaker 1>how do we know that the dark matter inside the

0:35:27.480 --> 0:35:30.960
<v Speaker 1>galaxy hasn't also clumped together to make you know, star

0:35:31.000 --> 0:35:34.560
<v Speaker 1>size stuff or planet sized stuff the way normal matter has, right,

0:35:35.800 --> 0:35:38.120
<v Speaker 1>And And we don't know the answer to that, right,

0:35:38.239 --> 0:35:40.440
<v Speaker 1>And the reason we don't know is because we can't

0:35:40.520 --> 0:35:43.360
<v Speaker 1>see dark matter and enough to tail Like, it's totally

0:35:43.480 --> 0:35:47.359
<v Speaker 1>possible that the distribution of dark matter in the galaxy

0:35:47.000 --> 0:35:52.560
<v Speaker 1>is either a totally smoothly spread out right, be sort

0:35:52.560 --> 0:35:55.760
<v Speaker 1>of like a cloud. Now we know it's denser towards

0:35:55.760 --> 0:35:58.960
<v Speaker 1>the center and less dense towards the outside, but it

0:35:59.000 --> 0:36:01.080
<v Speaker 1>could still be like a like a big cloud, right,

0:36:01.719 --> 0:36:04.880
<v Speaker 1>Or it could be that their structure that it's clumped

0:36:04.920 --> 0:36:07.880
<v Speaker 1>together to make, you know, a bunch of dense points,

0:36:07.920 --> 0:36:10.080
<v Speaker 1>just the way normal matter has. So there could be

0:36:10.160 --> 0:36:14.960
<v Speaker 1>dark matter stars or dark matter planets exactly, but the

0:36:15.000 --> 0:36:17.400
<v Speaker 1>only way to see them would be through gravity. And

0:36:17.480 --> 0:36:20.520
<v Speaker 1>it's really hard to see a gravity from like one

0:36:20.560 --> 0:36:23.960
<v Speaker 1>planet or the gravity from one star, right unless it's

0:36:24.000 --> 0:36:27.120
<v Speaker 1>really close by. Like if there were dark matter stars

0:36:27.600 --> 0:36:31.440
<v Speaker 1>and a dark matter star passed near our solar system,

0:36:31.800 --> 0:36:34.080
<v Speaker 1>then we could detect it the way we detect black

0:36:34.080 --> 0:36:37.680
<v Speaker 1>holes right there. Black holes are invisible. We detect them

0:36:37.680 --> 0:36:40.239
<v Speaker 1>from their gravity. Sometimes we detect black holes because of

0:36:40.280 --> 0:36:43.520
<v Speaker 1>the X rays that are produced from compressed gas nearby.

0:36:43.560 --> 0:36:46.680
<v Speaker 1>But a lot of black holes we see through their gravity.

0:36:46.719 --> 0:36:48.399
<v Speaker 1>But you need to be a pretty big black hole

0:36:48.440 --> 0:36:51.160
<v Speaker 1>to detect its gravity from far away or to see

0:36:51.280 --> 0:36:55.480
<v Speaker 1>its gravitational effect. Are nearby stuff, right, And in fact,

0:36:55.640 --> 0:36:57.960
<v Speaker 1>there are a few of these things we found, and

0:36:58.000 --> 0:36:59.960
<v Speaker 1>they have a pretty silly name. You ready for it

0:37:00.680 --> 0:37:05.040
<v Speaker 1>always physics really names. Yeah, they're back a long time

0:37:05.080 --> 0:37:07.239
<v Speaker 1>ago before we knew whether dark matter was the thing.

0:37:07.280 --> 0:37:09.799
<v Speaker 1>People were wondering if they were just big clumps of

0:37:09.880 --> 0:37:12.200
<v Speaker 1>normal matter there was sort of hidden out there, and

0:37:12.280 --> 0:37:17.000
<v Speaker 1>they gave them this name, massive compact halo objects, and

0:37:17.040 --> 0:37:20.279
<v Speaker 1>the acronym for that is m A C h O. Right,

0:37:20.360 --> 0:37:23.799
<v Speaker 1>so mach of these not nachos. Nachos are a totally

0:37:23.840 --> 0:37:27.840
<v Speaker 1>different thing. These are MACHOs. And so that's not physicists

0:37:28.520 --> 0:37:31.920
<v Speaker 1>over compensating for anything, not at all. No, And so

0:37:31.960 --> 0:37:33.520
<v Speaker 1>people went out there and looking for these things, like

0:37:33.600 --> 0:37:38.240
<v Speaker 1>can we find dark blobs out there, dark condensed blobs

0:37:38.239 --> 0:37:42.000
<v Speaker 1>out there that might be responsible for all the missing mass, right,

0:37:42.440 --> 0:37:44.799
<v Speaker 1>And they did find a bunch of not nearly enough

0:37:44.880 --> 0:37:46.879
<v Speaker 1>to account for all the dark matter, but they found

0:37:46.920 --> 0:37:49.200
<v Speaker 1>a bunch of them. They would find them like eclipsing

0:37:49.239 --> 0:37:53.080
<v Speaker 1>stars or bending the path of other objects. Um. And

0:37:53.120 --> 0:37:55.439
<v Speaker 1>so we know that there are dark objects out there.

0:37:55.680 --> 0:37:58.799
<v Speaker 1>Some of them could be dark matter, right, Some of

0:37:58.800 --> 0:38:02.160
<v Speaker 1>them could be so totally possible that dark matter has

0:38:02.160 --> 0:38:05.480
<v Speaker 1>clumped these objects together. We just don't have the gravitational

0:38:05.520 --> 0:38:09.640
<v Speaker 1>sensitivity to see them because they're too small. Essentially, in

0:38:09.719 --> 0:38:14.239
<v Speaker 1>gravity is so weak, Like our ability to notice or

0:38:14.640 --> 0:38:18.240
<v Speaker 1>feel or see dark matter is not at the planet

0:38:18.360 --> 0:38:20.640
<v Speaker 1>or at the star level. It's only at sort of

0:38:20.680 --> 0:38:23.600
<v Speaker 1>the galaxy level, yeah, exactly a little bit less than

0:38:23.600 --> 0:38:25.759
<v Speaker 1>the galaxy. We can we can get some sense of

0:38:25.760 --> 0:38:28.880
<v Speaker 1>where they are based on how rotations vary as a

0:38:29.040 --> 0:38:31.120
<v Speaker 1>function of the radius from the center of the galaxy.

0:38:31.360 --> 0:38:33.799
<v Speaker 1>But roughly yet much more the galaxy level than the

0:38:33.840 --> 0:38:36.560
<v Speaker 1>star level. But but it's fun to think about, like

0:38:37.000 --> 0:38:39.480
<v Speaker 1>imagine what would happen. What would happen if you had

0:38:39.480 --> 0:38:42.200
<v Speaker 1>a huge blob of dark matter and it coalesced into

0:38:42.280 --> 0:38:44.480
<v Speaker 1>sort of a tight blob, like would it make a

0:38:44.600 --> 0:38:47.120
<v Speaker 1>star like planet? You know? And we when we say

0:38:47.120 --> 0:38:49.719
<v Speaker 1>a star, we sort of mean something that's big enough,

0:38:49.880 --> 0:38:52.960
<v Speaker 1>has enough gravity that it's pushed the stuff together that

0:38:53.000 --> 0:38:56.840
<v Speaker 1>begins to fuse and release energy, right, And so another

0:38:56.880 --> 0:38:59.360
<v Speaker 1>interesting question is like, what would happen if you squeeze

0:38:59.360 --> 0:39:04.480
<v Speaker 1>that much dark matter together? What interesting things happen, like, um,

0:39:04.520 --> 0:39:08.279
<v Speaker 1>you know, elements fusing and releasing photons and things like that. Well,

0:39:08.280 --> 0:39:10.360
<v Speaker 1>we don't know, but we know it's not made of elements, right,

0:39:10.400 --> 0:39:12.080
<v Speaker 1>It's not made of atoms. It's made of some some

0:39:12.200 --> 0:39:15.120
<v Speaker 1>other kind of matter. And the only interaction we know

0:39:15.200 --> 0:39:18.160
<v Speaker 1>it has is gravity. So as far as we know,

0:39:18.239 --> 0:39:20.920
<v Speaker 1>it would just squeeze and squeeze and squeeze and squeeze,

0:39:21.000 --> 0:39:23.920
<v Speaker 1>and there's no repulsion. Right. The thing that keeps a

0:39:24.000 --> 0:39:26.719
<v Speaker 1>star or a planet from immediately becoming a black hole

0:39:27.040 --> 0:39:31.480
<v Speaker 1>are the other forces. It feels like electromagnetism, which and

0:39:31.719 --> 0:39:34.759
<v Speaker 1>the strong force which fuel fusion, right, which keeps a

0:39:34.800 --> 0:39:38.839
<v Speaker 1>star exploding. It keeps it from collapsing immediately. So if

0:39:38.920 --> 0:39:41.920
<v Speaker 1>dark matter has no other forces, then every time it

0:39:41.960 --> 0:39:43.719
<v Speaker 1>gets to be a pretty dense clump is just going

0:39:43.760 --> 0:39:46.480
<v Speaker 1>to turn into a dark matter black hole, because that's

0:39:46.560 --> 0:39:50.160
<v Speaker 1>it's just gravity. But if dark matter does feel some

0:39:50.239 --> 0:39:53.120
<v Speaker 1>other force, maybe some new force we've never seen before

0:39:53.320 --> 0:39:56.720
<v Speaker 1>that only affects dark matter on dark matter interactions, then maybe,

0:39:57.000 --> 0:39:59.080
<v Speaker 1>you know, clumping a bunch of the dark matter together

0:39:59.360 --> 0:40:02.600
<v Speaker 1>could sp some sort of dark matter interaction which could

0:40:02.640 --> 0:40:07.280
<v Speaker 1>release like dark photons. We're just wildly speculating here because

0:40:07.280 --> 0:40:09.839
<v Speaker 1>we just really don't know what happens when dark matter

0:40:09.840 --> 0:40:14.080
<v Speaker 1>bumps into dark matter, dark photons, and dark light. Yes, exactly,

0:40:14.080 --> 0:40:19.239
<v Speaker 1>sounds like all good comic book characters. That's right. Today

0:40:19.280 --> 0:40:22.120
<v Speaker 1>we've been exploring the connection between physics, philosophy and physics

0:40:22.120 --> 0:40:25.560
<v Speaker 1>and comics books. Is it trifecta um? I think? You know,

0:40:25.600 --> 0:40:28.799
<v Speaker 1>maybe that's where Ben's question came from. You know, like,

0:40:29.200 --> 0:40:31.839
<v Speaker 1>you know, we know dark matter feels gravity, so why

0:40:32.000 --> 0:40:36.120
<v Speaker 1>hasn't it clumped into dark matter black holes? You know,

0:40:36.200 --> 0:40:39.480
<v Speaker 1>why is it still kind of diffused and and not

0:40:39.800 --> 0:40:44.400
<v Speaker 1>um not more noticeable? You know? Does that mean that

0:40:44.760 --> 0:40:49.600
<v Speaker 1>you know he's a alternative you mentioned are maybe probably true?

0:40:49.840 --> 0:40:52.879
<v Speaker 1>You know that there are other forces or there are

0:40:52.920 --> 0:40:56.799
<v Speaker 1>maybe other mechanisms going on inside of a dark matter Absolutely,

0:40:57.239 --> 0:40:59.520
<v Speaker 1>I think a lot of physicists believe that there must

0:40:59.560 --> 0:41:02.160
<v Speaker 1>be some other kind of force that dark matter feels,

0:41:02.239 --> 0:41:05.279
<v Speaker 1>not just gravity, and the sort of complicated arguments for

0:41:05.320 --> 0:41:07.719
<v Speaker 1>that based on what happened in the early universe and

0:41:07.719 --> 0:41:10.239
<v Speaker 1>how some matter and dark matter turned back and forth

0:41:10.280 --> 0:41:13.640
<v Speaker 1>into itself. We have indirect evidence of that happening, which

0:41:13.680 --> 0:41:16.600
<v Speaker 1>suggests there must be some other force that dark matter feels,

0:41:16.640 --> 0:41:18.879
<v Speaker 1>but we haven't figured that out yet at all. It's

0:41:18.920 --> 0:41:22.600
<v Speaker 1>really it's very indirect arguments. But there is one thing

0:41:22.640 --> 0:41:26.080
<v Speaker 1>that keeps dark matter from collapsing sort of quickly into

0:41:26.120 --> 0:41:29.440
<v Speaker 1>a black hole, and that's our old friend rotation. Like,

0:41:29.840 --> 0:41:32.200
<v Speaker 1>one thing that keeps the galaxy from collapsing into a

0:41:32.360 --> 0:41:35.320
<v Speaker 1>black hole is that it's spinning, and so that keeps

0:41:35.360 --> 0:41:38.160
<v Speaker 1>the stars from falling in just the way spinning the

0:41:38.200 --> 0:41:40.640
<v Speaker 1>Earth spinning around the Sun keeps it from falling into

0:41:40.680 --> 0:41:43.040
<v Speaker 1>the Sun. Right, it's an orbit. If you have a

0:41:43.120 --> 0:41:46.239
<v Speaker 1>huge blob of dark matter and it's rotating, that rotation

0:41:46.520 --> 0:41:50.120
<v Speaker 1>keeps it from collapsing gravitationally into a black hole. And

0:41:50.160 --> 0:41:53.239
<v Speaker 1>so that's something that dark matter can do, even if

0:41:53.400 --> 0:41:56.600
<v Speaker 1>even if it has no other interactions. But yeah, I

0:41:56.640 --> 0:41:59.520
<v Speaker 1>think that it's totally possible that dark matter has formed

0:41:59.760 --> 0:42:03.400
<v Speaker 1>really dense blobs inside our galaxy, and it's possible that

0:42:03.440 --> 0:42:06.879
<v Speaker 1>there's new interactions doing weird stuff inside those dark matter

0:42:06.960 --> 0:42:09.640
<v Speaker 1>objects that we have no idea about. But I think

0:42:09.640 --> 0:42:11.680
<v Speaker 1>what you're saying maybe is that we we sort of

0:42:11.719 --> 0:42:14.279
<v Speaker 1>haven't seen that yet, right, Like, if if we are

0:42:14.520 --> 0:42:18.400
<v Speaker 1>surrounded by dark matter stars or dark matter you know,

0:42:18.480 --> 0:42:21.439
<v Speaker 1>giant asteroids, you know, and one of them came through

0:42:21.480 --> 0:42:24.120
<v Speaker 1>our Solar system, would we would notice it? Right, like

0:42:24.120 --> 0:42:29.040
<v Speaker 1>we would notice all the other planets going whoa gravitation, Yes, exactly,

0:42:29.160 --> 0:42:30.799
<v Speaker 1>that's the kind of thing we would notice for sure.

0:42:31.160 --> 0:42:33.960
<v Speaker 1>I mean we noticed Omuamua, right, this tiny little rock

0:42:34.040 --> 0:42:36.759
<v Speaker 1>coming through from from deep space and passing through our

0:42:36.800 --> 0:42:40.040
<v Speaker 1>soul system with no gravitational interaction at all. That was

0:42:40.320 --> 0:42:43.880
<v Speaker 1>but it was reflective. But imagine some really dense, heavy

0:42:43.920 --> 0:42:46.799
<v Speaker 1>object that perturbed the path of the planets that we

0:42:46.800 --> 0:42:48.800
<v Speaker 1>would definitely notice. Yeah, it would have to be pretty

0:42:48.800 --> 0:42:51.879
<v Speaker 1>big though, because gravity is pretty weak, So like some

0:42:52.000 --> 0:42:54.840
<v Speaker 1>random rock flying through the universe we wouldn't notice and

0:42:55.000 --> 0:42:57.600
<v Speaker 1>have to be you know, like, it had to be

0:42:57.640 --> 0:42:59.960
<v Speaker 1>a pretty significant objects. I'm not sure exactly how man,

0:43:00.560 --> 0:43:02.839
<v Speaker 1>but some significant fraction in the mass of the Sun

0:43:02.920 --> 0:43:05.080
<v Speaker 1>at the very least. Yeah, we would notice it, right,

0:43:05.120 --> 0:43:09.560
<v Speaker 1>It would totally disrupt our solar system. Yeah, absolutely. But

0:43:09.960 --> 0:43:12.360
<v Speaker 1>there could be a lot of these dark matter blobs

0:43:12.400 --> 0:43:14.000
<v Speaker 1>out there and just none of them have passed through

0:43:14.000 --> 0:43:17.839
<v Speaker 1>the Solar system because the galaxy is huge, right, and

0:43:18.040 --> 0:43:20.400
<v Speaker 1>there's lots of blobs out there that that made a

0:43:20.480 --> 0:43:23.200
<v Speaker 1>normal matter that don't pass through our solar system. Doesn't

0:43:23.200 --> 0:43:25.560
<v Speaker 1>mean they're not out there. I mean, there could be

0:43:25.719 --> 0:43:31.400
<v Speaker 1>a giant banana shaped massive dark matter out there that's

0:43:31.440 --> 0:43:33.399
<v Speaker 1>waiting for us to slip on. That's right. You're gonna

0:43:33.400 --> 0:43:36.160
<v Speaker 1>tie all the questions together. What if there's a banana

0:43:36.239 --> 0:43:39.920
<v Speaker 1>shaped massive dark matter creating a Solar system sized black

0:43:40.000 --> 0:43:43.000
<v Speaker 1>hole and we're in it, could we tell if there

0:43:43.040 --> 0:43:46.120
<v Speaker 1>was another one that was identical? All right? Well, I

0:43:46.160 --> 0:43:49.839
<v Speaker 1>guess that band's answer is that there could be dark

0:43:49.880 --> 0:43:52.640
<v Speaker 1>matter stars and planets or things out there. We just

0:43:52.800 --> 0:43:55.400
<v Speaker 1>we just can't see them yet. That's just don't have

0:43:55.480 --> 0:43:59.560
<v Speaker 1>the the right glasses to see it more sharply, right,

0:44:00.080 --> 0:44:02.920
<v Speaker 1>that's right. Yeah, um, And it's not clear that we

0:44:03.000 --> 0:44:05.799
<v Speaker 1>ever will because we don't know what glasses to put on,

0:44:05.880 --> 0:44:09.000
<v Speaker 1>or if there are glasses that you could even potentially

0:44:09.040 --> 0:44:11.640
<v Speaker 1>theoretically put on to see this stuff. Well, obviously we

0:44:11.719 --> 0:44:15.920
<v Speaker 1>just need dark glasses. I wear my sunglasses at night.

0:44:15.960 --> 0:44:18.040
<v Speaker 1>I don't know about you. All right, Well, once again,

0:44:18.080 --> 0:44:20.920
<v Speaker 1>thank you listeners for sending you as your questions. We

0:44:21.480 --> 0:44:24.280
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0:44:24.400 --> 0:44:27.560
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0:44:27.600 --> 0:44:29.600
<v Speaker 1>And if you're listening to us talk about something in

0:44:29.640 --> 0:44:32.400
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0:44:32.520 --> 0:44:35.200
<v Speaker 1>please share it with us. The reason we're doing this

0:44:35.280 --> 0:44:38.200
<v Speaker 1>podcast is to clarify these things and explain them to you.

0:44:38.560 --> 0:44:40.960
<v Speaker 1>And so there's something we've missed, we want to get

0:44:40.960 --> 0:44:43.360
<v Speaker 1>on it. Yeah, and we'll answer it even if you

0:44:43.360 --> 0:44:47.360
<v Speaker 1>are not our sons, unless you're on Instagram. In that case, sorry,

0:44:47.920 --> 0:44:51.319
<v Speaker 1>in that case, you're out of luck. Do you have

0:44:51.320 --> 0:44:53.720
<v Speaker 1>any sons on Instagram? You not aware of your trendy

0:44:53.760 --> 0:44:56.000
<v Speaker 1>and like the rest of the universe, then maybe you

0:44:56.000 --> 0:45:00.279
<v Speaker 1>should ask the question on Twitter. That's solid advice. Thanks

0:45:00.320 --> 0:45:02.640
<v Speaker 1>for listening, hope you enjoyed it, Thanks for tuning in.

0:45:13.719 --> 0:45:16.040
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0:45:16.080 --> 0:45:19.279
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0:45:19.320 --> 0:45:21.680
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0:45:29.560 --> 0:45:32.360
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