WEBVTT - Listener Questions 4

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<v Speaker 1>Hey, Daniel, what's been in our inbox lately? Well, we

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<v Speaker 1>get the usual stuff, people with minor corrections, people with

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<v Speaker 1>you know, cosmic questions, people asking me for to send

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<v Speaker 1>them special stuff for Father's Day. So you said people

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<v Speaker 1>are asking about Father's Day. Yes, some people right in

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<v Speaker 1>I like this because they're not actually fans of our show,

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<v Speaker 1>but their dad or their mom is a fan of

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<v Speaker 1>the show, and they want us to send a special

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<v Speaker 1>Father's Day or Mother's Day message to their parents who listens.

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<v Speaker 1>So it's like young, cool, hip people saying, Hey, my

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<v Speaker 1>dad likes your show, and I have no ideas for

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<v Speaker 1>any Father's Day's gifts. So do we charge for these

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<v Speaker 1>or we don't charge for these because we're nice guys

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<v Speaker 1>and we like helping people, and we're also fathers, and

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<v Speaker 1>so I want to give a special shout out to

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<v Speaker 1>Paul truth Low, whose daughter Caitlin asked us to give

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<v Speaker 1>you a special Father's Day message. So happy Father's Day, Paul,

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<v Speaker 1>and uh roll Tide, I'm supposed to say. Also, Hi,

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<v Speaker 1>I'm Poor Hay, I'm a cartoonists and the creator of

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<v Speaker 1>PhD Comics. Hi I'm Daniel Whitson, I'm a particle physicist

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<v Speaker 1>by day and a podcaster by any other time I know.

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<v Speaker 1>Welcome to our podcast Daniel and Jorge Explain at Universe,

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<v Speaker 1>a production of I Heart Radio in which we really do,

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<v Speaker 1>honestly try to answer questions about physics, Questions that we have,

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<v Speaker 1>questions that you have, Questions that we just randomly float

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<v Speaker 1>into our minds some days. Yeah, and if you actually

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<v Speaker 1>send us a question, either at questions at Daniel and

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<v Speaker 1>Jorge dot com or any one of our social media

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<v Speaker 1>channels like Instagram or Twitter or Facebook, we will actually

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<v Speaker 1>get to your question and maybe even talk about it

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<v Speaker 1>on the podcast. That's right, because when you have a question,

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<v Speaker 1>probably other people have the same question. And that's the

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<v Speaker 1>wonderful thing about having people suggest questions, because sometimes there's

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<v Speaker 1>an angle to something that we haven't thought of because

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<v Speaker 1>we come at it from a scientific perspective, and seeing

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<v Speaker 1>it from the point of view of the audience helps

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<v Speaker 1>us really explain these things, really get down and untangle

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<v Speaker 1>all those mysteries that you have in your mind, because

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<v Speaker 1>our goal is at the end of this that you

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<v Speaker 1>have a crystal clear picture what's going on in this universe.

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<v Speaker 1>And if you send us a question that stumps Daniel,

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<v Speaker 1>you actually get a prize, right, Daniel, Yeah, banana cake.

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<v Speaker 1>I don't know. It's a podcast has to be audio,

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<v Speaker 1>So the sound of Jorgey eating a banana cake that

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<v Speaker 1>Daniel made. How about that? Some Rader shows give you

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<v Speaker 1>your phone message, they'll record your your voicemail message. We

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<v Speaker 1>will record one of the hosts eating bananas. What could

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<v Speaker 1>be better than that? Yeah? Well, hey, that could be

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<v Speaker 1>a good ring tone, right, that could be a good ringtowne. Hey,

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<v Speaker 1>I got a call coming and how do you know

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<v Speaker 1>it sounds like something's eating in your pocket. Yeah, that's right.

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<v Speaker 1>If you're really kind of personally doesn't like peop believing

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<v Speaker 1>your voicemails, this is this is the contest for you

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<v Speaker 1>right here. That's right, that's right. No, seriously, I would

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<v Speaker 1>love to get a question that stumps me. Um. I

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<v Speaker 1>do get questions A lot of times. I get questions

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<v Speaker 1>I've never heard before, and that's a wonderful experience because

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<v Speaker 1>you know, there's a standard as the questions people ask.

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<v Speaker 1>But then there's a question I'd never even thought to

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<v Speaker 1>ask before, and that's wonderful because it gives me a

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<v Speaker 1>little view into the mind of the question er. I

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<v Speaker 1>have to think what did they understand or what was

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<v Speaker 1>going on in their head that inspired this question, so

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<v Speaker 1>that I can then figure out how to guide them

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<v Speaker 1>from there to a clear picture of what's actually happening.

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<v Speaker 1>And that's the challenge of teaching, and that's what I

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<v Speaker 1>really love about that. So these are questions you hadn't

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<v Speaker 1>even thought anyone could ask or would ask. Yeah, I'll

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<v Speaker 1>give you an example. Um, I give demonstrations at elementary

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<v Speaker 1>school sometimes and we use like liquid nitrogen and all

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<v Speaker 1>sorts of stuff too, you know. Um, one time we

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<v Speaker 1>froze bananas and shattered it on the ground and the

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<v Speaker 1>kids thought that was cool, and afterwards were open for questions.

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<v Speaker 1>Wait wait, wait, you shattered bananas. That's right, some bananas

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<v Speaker 1>were harmed in the making of this pod cast. I

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<v Speaker 1>have to oh, man, my heart is bleeding, Daniel. But

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<v Speaker 1>afterwards we were open for questions, and some kid raised

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<v Speaker 1>his hand and he says, if lightsabers were real, would

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<v Speaker 1>they be made of liquid nitrogen? And I thought, I

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<v Speaker 1>have no idea how to answer that question, you know, like,

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<v Speaker 1>where do you even begin. You rolled your eye, You're like,

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<v Speaker 1>obviously they're made out of hyper crystal. Wikid do your research.

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<v Speaker 1>I had not done my research on fictional universes and

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<v Speaker 1>how science might work in that fictional universe. But I

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<v Speaker 1>love that he connected two things he found amazing liquid

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<v Speaker 1>nitrogen and lightsabers, and thought maybe these are the same things.

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<v Speaker 1>And actually we get a lot of emails like that.

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<v Speaker 1>They're like, hey, today you guys talked about the mystery

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<v Speaker 1>of you know, dark matter. Maybe that's the same thing

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<v Speaker 1>as this other mystery. Like after our time episode, a

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<v Speaker 1>lot of people wrote in and said, maybe dark energy

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<v Speaker 1>is just a mistake of how we observe time, and

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<v Speaker 1>time doesn't just move forward constantly. It's sort of stutter steps,

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<v Speaker 1>and that's dark energy. People love to connect to mysteries

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<v Speaker 1>and try to solve them at once. So you know

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<v Speaker 1>that little boy in the class, he really exemplified the

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<v Speaker 1>kinds of questions that that listeners ask. We're all just

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<v Speaker 1>little Star Wars fans inside. That's right, that's right. Yeah,

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<v Speaker 1>Well today we are answering your questions on the podcast.

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<v Speaker 1>Today's episode is about listener questions Part four, right or

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<v Speaker 1>are we up to part pie? Are we sort of

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<v Speaker 1>this version? Pie? I think our podcasts are integer numbered, Yeah,

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<v Speaker 1>so this would be number four. It would be awesome

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<v Speaker 1>to have a point one four of a podcast, but

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<v Speaker 1>I'm not sure how do you pull that off? All right,

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<v Speaker 1>So today we have three interesting questions from listeners from

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<v Speaker 1>all across the world, right or at least the United States. Oh,

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<v Speaker 1>I think some of them are international. They don't always

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<v Speaker 1>tell us where they come from, but based on the accent,

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<v Speaker 1>I don't think all of these come from the Southwest

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<v Speaker 1>the United States, which seems to be are a big

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<v Speaker 1>hotbed for fans over our show. No, it was just random.

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<v Speaker 1>Last time I happened to pick three questions which all

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<v Speaker 1>like came from the south I was totally just random.

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<v Speaker 1>But today we have three pretty cool questions from listeners.

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<v Speaker 1>One is about gravity, another one about dark matter, and

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<v Speaker 1>the other one is about the nuclei of Adam, Like

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<v Speaker 1>how do they stay together? And why don't we all

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<v Speaker 1>just explode into balls of nuclear explosions? Maybe we will.

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<v Speaker 1>You'll find out on today's episode. I think people um

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<v Speaker 1>might already know the answer. But teaser, you're you're okay

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<v Speaker 1>for the next couple of seconds. You'll survive long enough

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<v Speaker 1>to hear the end of this episode at the very least,

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<v Speaker 1>and then you can you can then explode view like

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<v Speaker 1>from knowledge? Do you think anybody has ever perished while

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<v Speaker 1>listening to our episode? That just dark thoughts just entered

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<v Speaker 1>my head. Oh my god, let's let's cut that out.

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<v Speaker 1>Can you imagine being the last thing anybody ever heard

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<v Speaker 1>in their life for making a joke about bananas? It

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<v Speaker 1>blew their minds, banded their idea of what a joke

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<v Speaker 1>could be, and it's just overwhelmed their neural network. Yeah.

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<v Speaker 1>I don't know if that means the joke was amazing

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<v Speaker 1>so good that they couldn't take it, or they're just like,

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<v Speaker 1>you know what, I'm done after that. I can't take

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<v Speaker 1>anymore people get paid to say those kinds of jokes.

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<v Speaker 1>Then I'm out of here. There's no amazing to go on.

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<v Speaker 1>That's right, goodbye, cool, unfunny world. Well help, neither of

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<v Speaker 1>these things happen to you, our dear listeners. But our

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<v Speaker 1>first question comes from Florence from Texas, and she has

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<v Speaker 1>a question about how gravity could um keep the Earth

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<v Speaker 1>in orbit. Here's what you had to say. I have

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<v Speaker 1>a question about gravity. You've described it before as the

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<v Speaker 1>weakest force, and you said in fact that it's so

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<v Speaker 1>weak that when you're picking up an object with a magnet,

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<v Speaker 1>you're overpowering the entire Earth's gravity, So that's pretty weak.

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<v Speaker 1>My problem is when I start thinking about the objects

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<v Speaker 1>and the Kuiper Belt, they're thirty two fifty astronomer gold

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<v Speaker 1>units away and that's billions and billions of miles, and

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<v Speaker 1>yet the Sun's gravity is still able to keep them

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<v Speaker 1>in orbit. And that just gives me the impression that

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<v Speaker 1>gravity is really strong, not weak. So those two thoughts

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<v Speaker 1>really don't go together. Um, would you help me with that?

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<v Speaker 1>All right? Thank you, Florence from Texas. So that's a

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<v Speaker 1>pretty interesting question, right, Daniel. Is that we often mentioned

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<v Speaker 1>on the show that gravity is the weakest force, and

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<v Speaker 1>it's actually super duper duper weak. But at the same time,

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<v Speaker 1>I think maybe a lot of listeners are thinking, but

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<v Speaker 1>weight of gravity is a weak how is it keeping

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<v Speaker 1>the Earth going around in orbit and other planets in Jupiter?

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<v Speaker 1>And how is it such an amazing, an incredible force

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<v Speaker 1>in the universe. It is an amazing, incredible force in

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<v Speaker 1>the universe, And you're right to wonder about that, because

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<v Speaker 1>as you look out into the night sky, you think about,

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<v Speaker 1>like all the structures in the universe, the Solar system

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<v Speaker 1>with the planets going around the Sun, and even the

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<v Speaker 1>galaxy and the structures of galaxies and the superclusters, all

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<v Speaker 1>of that is determined by gravity, right, So gravity seems

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<v Speaker 1>to have a huge role in organizing the way the

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<v Speaker 1>universe works, right, And and the way we discovered dark

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<v Speaker 1>matters through gravity. And so if you just looked at it,

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<v Speaker 1>you say, well, gravity is one of the most important

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<v Speaker 1>forces because it shapes the whole universe. So then to

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<v Speaker 1>hear somebody say actually, gravity is the weakest force in

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<v Speaker 1>the universe, it does seem like a strong contradiction, right,

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<v Speaker 1>it It doesn't make sense in your mind, because how

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<v Speaker 1>can it be the weakest force and also be the

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<v Speaker 1>thing that shapes everything else? Right, It's kind of like

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<v Speaker 1>the organizing force in the universe, right, It organizes planets

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<v Speaker 1>into solar systems, and solar systems into galaxies and galaxies

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<v Speaker 1>in two clusters. Like if we didn't have gravity, everything

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<v Speaker 1>which is a fly fly away and fly apart. Yeah,

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<v Speaker 1>that's right, we wouldn't have any of the good stuff

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<v Speaker 1>that we have without gravity. So we own a big

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<v Speaker 1>thanks to gravity. And I like the way you said

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<v Speaker 1>it's I sort of organized these things. I think that's

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<v Speaker 1>one of the big ideas to understand how gravity can

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<v Speaker 1>play such a big role and be so weak. It's

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<v Speaker 1>sort of like the way you make a big mess

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<v Speaker 1>in your house and then you come back home and

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<v Speaker 1>your mom is organized the living room or whatever. Right,

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<v Speaker 1>some mysterious forces organized it while while you were gone.

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<v Speaker 1>Your mom still cleans your house. That's pretty good. Know what,

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<v Speaker 1>your mom cleans my house where hey, she doesn't. She

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<v Speaker 1>doesn't clean yours. She flies from Panama every every week

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<v Speaker 1>and clean your house and she doesn't even call me.

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<v Speaker 1>Oh my god, Maybe because I didn't celebrate Mother's Day. Yeah, exactly,

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<v Speaker 1>Well you should have sent her banana cake. Um No.

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<v Speaker 1>But the point I wanted to make, the actual physics point,

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<v Speaker 1>not a joke, is that gravity is a force that's

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<v Speaker 1>sort of left over like all the other forces in

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<v Speaker 1>the universe. Electromagnetism, the strong force, the weak force. All

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<v Speaker 1>these forces are so powerful that they get kind of

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<v Speaker 1>naturally balanced. Like there's no electrostatic force or electromagnetic force

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<v Speaker 1>between the Earth and the Sun. Why because if there were,

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<v Speaker 1>it would be incredibly powerful and it would balance itself

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<v Speaker 1>the way like lightning is a balancing of the electrons

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<v Speaker 1>between the Earth and the sky. Right, anytime there's any

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<v Speaker 1>imbalance June, there's a huge bolt of lightning to balance

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<v Speaker 1>these things out. And so as a result, there is

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<v Speaker 1>no electromagnetic force between these huge celestial objects, and so

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<v Speaker 1>it's gravity. Gravity can't be balanced though. It's the one

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<v Speaker 1>force that cannot be neutralized because it only has mass.

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<v Speaker 1>There's no negative mass to balance it out. So after

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<v Speaker 1>all the other forces have made their big mess, gravity

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<v Speaker 1>sort of left to pick up the pieces. It's the

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<v Speaker 1>only thing left on the playing field, right. Well, I

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<v Speaker 1>think it's important to maybe mention that when we say

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<v Speaker 1>it's the weakest force, it's a relative assessment, right, Like

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<v Speaker 1>we're we're not saying gravity is weak, it's just weak

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<v Speaker 1>relative to the electromagnetic force. Well I'm saying it. No,

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<v Speaker 1>I'm saying gravity is super weak. It's embarrassing. It's puny's pathetic,

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<v Speaker 1>but only only because you know other forces that are stronger.

0:11:47.120 --> 0:11:48.839
<v Speaker 1>But if you didn't know the other forces, you'd be like,

0:11:48.920 --> 0:11:51.240
<v Speaker 1>oh my god. Gravity is what keeps the Earth from

0:11:51.240 --> 0:11:53.200
<v Speaker 1>going around the Sun, and the Earth is pretty big,

0:11:53.280 --> 0:11:55.880
<v Speaker 1>so it's like a huge force. You just know that

0:11:55.960 --> 0:11:58.560
<v Speaker 1>in comparison, it's kind of wimpy. I guess, so, I mean,

0:11:58.640 --> 0:12:00.840
<v Speaker 1>I think in comparison is really the only metric we have.

0:12:01.480 --> 0:12:05.000
<v Speaker 1>It's also important to recognize how much weaker it is.

0:12:05.520 --> 0:12:09.000
<v Speaker 1>Like if you took electrons, for example, and you asked, like,

0:12:09.120 --> 0:12:12.520
<v Speaker 1>what is the force of their electrostatic repulsion compared to

0:12:12.559 --> 0:12:17.800
<v Speaker 1>their gravitational um attraction, then the difference is like ten,

0:12:18.200 --> 0:12:23.839
<v Speaker 1>with thirty three zeros after it. So you know, millions, billions, trillions, quadrillions.

0:12:23.880 --> 0:12:26.920
<v Speaker 1>You run out of numbers really quick. It's a huge difference.

0:12:26.960 --> 0:12:30.040
<v Speaker 1>It's like a completely different scale, right, So you're saying,

0:12:30.040 --> 0:12:32.600
<v Speaker 1>if I have an electron and maybe a proton, they're

0:12:32.640 --> 0:12:38.080
<v Speaker 1>both being attracted by two forces, gravity and electromagnetism. But

0:12:38.120 --> 0:12:42.040
<v Speaker 1>you're saying the electromagnetism is thirty two orders of magnetudes

0:12:42.040 --> 0:12:45.880
<v Speaker 1>stronger than the gravitational force between them. Yeah, exactly, They're

0:12:46.000 --> 0:12:51.280
<v Speaker 1>totally different scales, exactly. Electromagnetism, I mean, it's jatillion. What

0:12:51.280 --> 0:12:56.280
<v Speaker 1>what's the word for thirty zeros? It's an alien you

0:12:56.320 --> 0:13:00.559
<v Speaker 1>go be a zillion um. It's so much bigger. If

0:13:00.640 --> 0:13:02.320
<v Speaker 1>you don't even really want to describe them in the

0:13:02.360 --> 0:13:05.040
<v Speaker 1>same level. It's like, you know, the mass of the

0:13:05.080 --> 0:13:07.679
<v Speaker 1>Earth versus the math of mass of a penny or something.

0:13:07.720 --> 0:13:10.040
<v Speaker 1>You know, you don't you don't call a penny a

0:13:10.120 --> 0:13:12.640
<v Speaker 1>celestial object because it isn't right so tiny, you just

0:13:12.720 --> 0:13:15.600
<v Speaker 1>sort of round it up into the earth um. Anyway,

0:13:15.880 --> 0:13:19.400
<v Speaker 1>the reason that gravity can still play on the field

0:13:19.440 --> 0:13:21.640
<v Speaker 1>at all is that these other forces are so strong

0:13:21.679 --> 0:13:24.240
<v Speaker 1>that they balance each other out, and gravity you can't

0:13:24.280 --> 0:13:27.200
<v Speaker 1>do that, right, Like we were talking about one electron

0:13:27.320 --> 0:13:30.079
<v Speaker 1>another electron, they repel each other, whereas an electron or

0:13:30.080 --> 0:13:33.560
<v Speaker 1>a proton they attract each other. Right, Gravity only makes

0:13:33.600 --> 0:13:37.679
<v Speaker 1>attractive forces. Everything with mass feels gravity and it attracts itself.

0:13:37.760 --> 0:13:40.640
<v Speaker 1>There's no way to have repulsive gravity. And we did

0:13:40.679 --> 0:13:42.960
<v Speaker 1>a whole podcast episode about anti gravity. As far as

0:13:42.960 --> 0:13:45.480
<v Speaker 1>we know, it's not possible. So there's no way to

0:13:45.480 --> 0:13:48.600
<v Speaker 1>balance gravity out. After everybody else has done their stuff

0:13:48.640 --> 0:13:51.320
<v Speaker 1>and and been neutralized, gravity is left over, and so

0:13:51.360 --> 0:13:54.240
<v Speaker 1>then it gets to organize the universe. Yeah, I was thinking,

0:13:54.280 --> 0:13:57.439
<v Speaker 1>like maybe an interesting picture is to imagine a proton

0:13:58.440 --> 0:14:01.800
<v Speaker 1>in the Sun and then imagine a proton and an

0:14:01.840 --> 0:14:06.199
<v Speaker 1>electron on Earth. It's not that there's no electromagnetic force

0:14:06.280 --> 0:14:10.320
<v Speaker 1>between that proton and this proton and electron. It's just

0:14:10.400 --> 0:14:12.960
<v Speaker 1>that that the proton in the sun's pulling the electron

0:14:12.960 --> 0:14:15.320
<v Speaker 1>towards the Sun, but it's also pushing the proton away

0:14:15.320 --> 0:14:19.040
<v Speaker 1>from the Sun with the exact same force. So our

0:14:19.080 --> 0:14:21.720
<v Speaker 1>pair of proton and electron here on Earth just doesn't

0:14:21.760 --> 0:14:25.480
<v Speaker 1>feel any electro metnetic force with that proton in the Sun,

0:14:25.760 --> 0:14:28.880
<v Speaker 1>but it does feel gravity, yeah, exactly. And you know,

0:14:28.920 --> 0:14:31.240
<v Speaker 1>there's lots of protons and electrons in the Sun, and

0:14:31.280 --> 0:14:33.680
<v Speaker 1>so they all work, they all arrange themselves in such

0:14:33.680 --> 0:14:36.440
<v Speaker 1>a way that there's effectively no net force, and there's

0:14:36.480 --> 0:14:39.400
<v Speaker 1>no way to arrange the protons electrons to get no

0:14:39.560 --> 0:14:42.400
<v Speaker 1>net gravitational force. There's just no way to do that.

0:14:42.480 --> 0:14:44.200
<v Speaker 1>But I think it's interesting to think about. It's not

0:14:44.240 --> 0:14:47.640
<v Speaker 1>that there's no force, it's just that there's no net force,

0:14:47.720 --> 0:14:51.400
<v Speaker 1>you know, like it is pushing and pulling as electromagnetically

0:14:51.480 --> 0:14:54.560
<v Speaker 1>the Sun, it all just sort of cancels out. Yeah, yeah,

0:14:54.720 --> 0:14:56.800
<v Speaker 1>like it's pushing on a proton and it's pushing on

0:14:56.840 --> 0:14:59.680
<v Speaker 1>an electron the opposite direction, right, But because our proton

0:14:59.760 --> 0:15:02.280
<v Speaker 1>and the electron are holding on together, they're they're not

0:15:02.320 --> 0:15:04.560
<v Speaker 1>going anywhere. Yeah, that's that's a fine way to think

0:15:04.560 --> 0:15:07.080
<v Speaker 1>about it. Um. And I think the other thing to

0:15:07.120 --> 0:15:10.920
<v Speaker 1>recognize is that gravity is really really weak, but the

0:15:10.960 --> 0:15:14.720
<v Speaker 1>Sun is really really big, like really really really really big,

0:15:15.160 --> 0:15:18.200
<v Speaker 1>so it can have a pretty strong gravitational effect on

0:15:18.200 --> 0:15:20.520
<v Speaker 1>the Earth even though gravity is weak, because it just

0:15:20.600 --> 0:15:24.240
<v Speaker 1>has so much mass, right, And so yeah, gravity is weak,

0:15:24.280 --> 0:15:27.120
<v Speaker 1>but the Sun is so big that those two factors

0:15:27.240 --> 0:15:29.080
<v Speaker 1>kind of cancel each other out and it becomes an

0:15:29.080 --> 0:15:33.400
<v Speaker 1>important force. Yeah, the weakness accumulates exactly. You have like

0:15:33.680 --> 0:15:36.600
<v Speaker 1>a billion people all whispering your name, it's going to

0:15:36.680 --> 0:15:39.400
<v Speaker 1>add up to a huge scream, right, And that's the

0:15:39.440 --> 0:15:41.840
<v Speaker 1>way it is with gravity. All those protons in the

0:15:41.880 --> 0:15:45.200
<v Speaker 1>Sun are giving a tiny little tug on the protons

0:15:45.200 --> 0:15:48.920
<v Speaker 1>and electrons on Earth gravitationally. But there's so many protons

0:15:48.920 --> 0:15:50.760
<v Speaker 1>in the Sun that it's enough to pull a whole

0:15:50.840 --> 0:15:53.360
<v Speaker 1>planet around in a circle. Right. It's not a small

0:15:53.360 --> 0:15:55.960
<v Speaker 1>amount of force to keep the Earth in orbit, right,

0:15:56.000 --> 0:15:58.240
<v Speaker 1>It's a huge force that keeps the Earth in orbit.

0:15:58.600 --> 0:16:00.800
<v Speaker 1>Oh man, you just gave me a new nightmare. To

0:16:00.840 --> 0:16:08.480
<v Speaker 1>imagine a billion people whispering my name. That is so bizarre.

0:16:08.240 --> 0:16:12.280
<v Speaker 1>That is kind of creepy. Actually, yes, that doesn't where

0:16:12.320 --> 0:16:15.920
<v Speaker 1>that came from. Hey, let's all whisper Paul's name for

0:16:15.920 --> 0:16:20.720
<v Speaker 1>for father's sake, for father's days, didn't heal sense of

0:16:20.800 --> 0:16:24.080
<v Speaker 1>disturbance in the force when that happens. Everybody listened to

0:16:24.080 --> 0:16:29.280
<v Speaker 1>me to this right now, go Paul, Paul, Happy Father's Day, Paul,

0:16:32.320 --> 0:16:40.040
<v Speaker 1>your daughter is awesome. Cool. All right, that's um Florence's

0:16:40.120 --> 0:16:43.760
<v Speaker 1>question about gravity, and so the answer Florence is that

0:16:44.080 --> 0:16:48.520
<v Speaker 1>gravity is weak, but it's also happening on such a

0:16:48.600 --> 0:16:52.840
<v Speaker 1>large scale that it does. It is enough to pool

0:16:52.880 --> 0:16:56.120
<v Speaker 1>planets and keep galaxies together, that's right. And after all

0:16:56.160 --> 0:16:58.960
<v Speaker 1>the other forces have done their business, gravity is left

0:16:58.960 --> 0:17:02.400
<v Speaker 1>over to organize the universe because it can't be balanced out.

0:17:02.640 --> 0:17:04.879
<v Speaker 1>All right, Well, that's one question, and we'll get to

0:17:05.200 --> 0:17:07.680
<v Speaker 1>the two other questions we have today about dark matter

0:17:08.040 --> 0:17:12.119
<v Speaker 1>and atomic nuclei. But first let's take a quick break.

0:17:25.200 --> 0:17:27.639
<v Speaker 1>Our second question of the day comes from Margie, who

0:17:27.680 --> 0:17:31.040
<v Speaker 1>has a question about dark matter. Hey, Daniel and Jorge,

0:17:31.200 --> 0:17:34.440
<v Speaker 1>this is Marchie. My question is how does dark matter

0:17:34.480 --> 0:17:36.879
<v Speaker 1>influence the movement of the planets in the Solar System?

0:17:37.000 --> 0:17:38.959
<v Speaker 1>Does it make them all orbit at the same speed

0:17:39.320 --> 0:17:42.920
<v Speaker 1>and if so, all right, that's a pretty interesting question. Um,

0:17:43.280 --> 0:17:45.600
<v Speaker 1>we talked, we've talked a lot about dark matter in

0:17:45.640 --> 0:17:49.359
<v Speaker 1>this podcast and how it's there. It's all around us,

0:17:49.480 --> 0:17:53.760
<v Speaker 1>it's in the center of galaxies, right all over the galaxy,

0:17:53.800 --> 0:17:58.879
<v Speaker 1>and it's constantly pulling on everything and helping galaxy stay together. Yeah,

0:17:58.920 --> 0:18:01.240
<v Speaker 1>this is a wonderful question. And because this is a

0:18:01.320 --> 0:18:03.360
<v Speaker 1>kind of question that shows me that people are doing

0:18:03.359 --> 0:18:06.560
<v Speaker 1>physics in their mind, right, they says, you've learned how

0:18:06.640 --> 0:18:10.440
<v Speaker 1>dark matter influences how galaxies rotate, Like we discovered dark

0:18:10.440 --> 0:18:13.600
<v Speaker 1>matter because we saw the galaxies were spinning too fast

0:18:13.640 --> 0:18:16.159
<v Speaker 1>and they need more gravity to hold them together. So

0:18:16.200 --> 0:18:19.000
<v Speaker 1>that means that dark matter makes enough gravity to be

0:18:19.040 --> 0:18:22.040
<v Speaker 1>like noticeable about how things spin. Right, So that the

0:18:22.160 --> 0:18:24.480
<v Speaker 1>natural physics thing to do is to say, okay, I

0:18:24.480 --> 0:18:27.560
<v Speaker 1>have my new understanding, let me apply it to something else.

0:18:27.880 --> 0:18:30.880
<v Speaker 1>Does that make sense? And this listener obviously thought, well,

0:18:30.920 --> 0:18:34.320
<v Speaker 1>if there's dark matter enough to affect the galaxy spinning,

0:18:34.560 --> 0:18:36.520
<v Speaker 1>why can't we notice it here on Earth? Like, why

0:18:36.520 --> 0:18:39.200
<v Speaker 1>can't we do that same measurement and see like, hey,

0:18:39.240 --> 0:18:42.119
<v Speaker 1>the Earth is going around the Sun too fast? Can't

0:18:42.119 --> 0:18:44.920
<v Speaker 1>we detect the dark matter in our Solar system by

0:18:44.960 --> 0:18:47.800
<v Speaker 1>looking at how the Earth orbits the Sun the same

0:18:47.840 --> 0:18:49.720
<v Speaker 1>way we look at how the Sun orbits the center

0:18:49.720 --> 0:18:52.440
<v Speaker 1>of the galaxy. So it's really a genius question. Oh,

0:18:52.480 --> 0:18:55.600
<v Speaker 1>I see. The question is is the Earth going around

0:18:55.640 --> 0:18:58.600
<v Speaker 1>the Sun faster than it should be if dark matter

0:18:58.840 --> 0:19:02.520
<v Speaker 1>didn't exist? Because imagine, for example, that there wasn't just

0:19:02.600 --> 0:19:04.720
<v Speaker 1>the Sun in the center of the Solar system. Imagine

0:19:04.720 --> 0:19:06.720
<v Speaker 1>there were five sons, but you can only see the

0:19:06.760 --> 0:19:08.640
<v Speaker 1>one of them, right, and the other ones were made

0:19:08.640 --> 0:19:11.439
<v Speaker 1>of dark matter. What would happen in that case. In

0:19:11.480 --> 0:19:14.919
<v Speaker 1>that case, there'd be a much stronger gravitational force than

0:19:14.960 --> 0:19:17.360
<v Speaker 1>you would expect from one Sun, and for the Earth

0:19:17.440 --> 0:19:18.800
<v Speaker 1>to stay in its orbit, it would have to go

0:19:18.920 --> 0:19:22.520
<v Speaker 1>much much faster, and so you would see a discrepancy.

0:19:22.560 --> 0:19:24.919
<v Speaker 1>You'd measure the speed at which the Earth was orbiting

0:19:25.160 --> 0:19:28.040
<v Speaker 1>the Sun, and you'd say, huh, it's going way too fast.

0:19:28.720 --> 0:19:32.240
<v Speaker 1>What's what's um, what's keeping it together, what's keeping it

0:19:32.280 --> 0:19:34.320
<v Speaker 1>in the Solar system? Why isn't it just flying off?

0:19:34.440 --> 0:19:36.280
<v Speaker 1>And then you would deduce the presence of all those

0:19:36.359 --> 0:19:39.640
<v Speaker 1>dark suns. Right, So this listener is like, well, can

0:19:39.720 --> 0:19:41.320
<v Speaker 1>we see the dark matter? Because We've said on this

0:19:41.320 --> 0:19:43.679
<v Speaker 1>podcast several times, a dark matter is everywhere. It's not

0:19:43.760 --> 0:19:45.720
<v Speaker 1>just out there, it's here, It's in this room, it's

0:19:45.720 --> 0:19:47.320
<v Speaker 1>on your planet, it's hanging out in that bunch of

0:19:47.359 --> 0:19:49.679
<v Speaker 1>bananas you just ate. It's everywhere. So why can't we

0:19:49.680 --> 0:19:51.640
<v Speaker 1>see it in our solar system? Right? Well, I guess

0:19:51.720 --> 0:19:54.160
<v Speaker 1>question number one is is there dark matter in our

0:19:54.160 --> 0:19:56.960
<v Speaker 1>solar system? And then question number two is is does

0:19:57.000 --> 0:20:00.840
<v Speaker 1>it influence the orbit of planets? So that Daniels, is

0:20:00.840 --> 0:20:03.280
<v Speaker 1>there a dark matter here in our solar system? We

0:20:03.359 --> 0:20:06.359
<v Speaker 1>think so. Now we don't know for sure, and the

0:20:06.400 --> 0:20:08.800
<v Speaker 1>reason is that gravity is pretty weak, right, as we

0:20:08.880 --> 0:20:11.639
<v Speaker 1>talked about recently, and so it's hard to get a

0:20:11.680 --> 0:20:14.080
<v Speaker 1>sense for exactly where dark matter is because the only

0:20:14.080 --> 0:20:16.040
<v Speaker 1>way that we can see it is is through its

0:20:16.040 --> 0:20:18.600
<v Speaker 1>gravitational effects, and so we can see its effects sort

0:20:18.600 --> 0:20:21.160
<v Speaker 1>of like on a galaxy sized scale, but it's really

0:20:21.160 --> 0:20:23.119
<v Speaker 1>hard to get a very clear map of where the

0:20:23.200 --> 0:20:26.560
<v Speaker 1>dark matter is. But we think it probably is. We

0:20:26.600 --> 0:20:29.480
<v Speaker 1>think it's probably distributed pretty evenly through the galaxy. There's

0:20:29.480 --> 0:20:31.639
<v Speaker 1>a blob in the very center and it sort of

0:20:31.720 --> 0:20:35.200
<v Speaker 1>just falls off gradually. So we suspect, like we would

0:20:35.200 --> 0:20:38.720
<v Speaker 1>see it as a haze just permeating everything exactly. And

0:20:38.720 --> 0:20:40.720
<v Speaker 1>you know what a deep question about dark matter is,

0:20:40.760 --> 0:20:43.359
<v Speaker 1>like is it just a smooth haze or are there structures?

0:20:43.359 --> 0:20:45.480
<v Speaker 1>It's a stuff happening. Is there like life forms in

0:20:45.560 --> 0:20:48.000
<v Speaker 1>dark matter? We really don't know because we haven't been

0:20:48.000 --> 0:20:50.200
<v Speaker 1>able to see it with enough resolution, because the only

0:20:50.200 --> 0:20:53.240
<v Speaker 1>way we've ever been able to probe it is through gravity.

0:20:53.280 --> 0:20:56.040
<v Speaker 1>And that's a it's you know, real frustration for us

0:20:56.080 --> 0:20:58.520
<v Speaker 1>as scientists. It's like most of the matter in the

0:20:58.600 --> 0:21:01.560
<v Speaker 1>universe is there, it's in front of us. We can't

0:21:01.600 --> 0:21:03.920
<v Speaker 1>see it. We can't tell if it's doing anything interesting

0:21:04.040 --> 0:21:06.639
<v Speaker 1>or just sort of a smooth haze. Right, And so

0:21:06.680 --> 0:21:08.359
<v Speaker 1>the question is if we are kind of in a

0:21:08.440 --> 0:21:11.119
<v Speaker 1>bath of dark matter right now, which we could be

0:21:11.240 --> 0:21:13.280
<v Speaker 1>or could not be. Maybe we're like in a bubble

0:21:13.480 --> 0:21:16.000
<v Speaker 1>of non dark matter. Is that possible? We might be

0:21:16.000 --> 0:21:18.240
<v Speaker 1>in a little gap, It's possible, right, But I think

0:21:18.280 --> 0:21:21.119
<v Speaker 1>the most sensible and the simplest assumption is just that

0:21:21.240 --> 0:21:23.280
<v Speaker 1>dark matter is smooth, and as you say, we're in

0:21:23.280 --> 0:21:24.840
<v Speaker 1>a bath of dark matter. I think that makes the

0:21:24.880 --> 0:21:27.840
<v Speaker 1>most sense. It's it's the most likely explanation. Okay, So

0:21:27.880 --> 0:21:30.200
<v Speaker 1>in that case, if we are bathing in dark matter,

0:21:30.760 --> 0:21:33.320
<v Speaker 1>would it affect the orbit of the planets. So the

0:21:33.640 --> 0:21:37.520
<v Speaker 1>short answer is yes, but not in a noticeable way.

0:21:37.680 --> 0:21:40.320
<v Speaker 1>And the reason is that the Solar System is not

0:21:40.440 --> 0:21:43.560
<v Speaker 1>big enough, right Like, if you take the density of

0:21:43.640 --> 0:21:47.400
<v Speaker 1>dark matter, and we expected, it's about like one protons

0:21:47.480 --> 0:21:51.240
<v Speaker 1>worth of dark matter about every three cubic centimeters, So

0:21:51.359 --> 0:21:54.160
<v Speaker 1>there's not actually that much dark matter spread out over

0:21:54.200 --> 0:21:56.159
<v Speaker 1>the universe, right Like, if you sort of look at

0:21:56.160 --> 0:22:00.000
<v Speaker 1>your thumb, there's probably only one proton's worth of dark

0:22:00.160 --> 0:22:02.040
<v Speaker 1>matter in it. Yeah. If you take all the dark

0:22:02.080 --> 0:22:04.880
<v Speaker 1>matter and you spread it out evenly through space, then

0:22:04.920 --> 0:22:07.760
<v Speaker 1>you end up with about one proton per per thumb.

0:22:07.800 --> 0:22:09.760
<v Speaker 1>I Like, the thumb is a unit of volume. Yeah,

0:22:10.359 --> 0:22:13.320
<v Speaker 1>one dark matter proton per thumb thumbs up. Yeah, And

0:22:13.320 --> 0:22:15.320
<v Speaker 1>you might and you might be thinking, hold on, isn't

0:22:15.359 --> 0:22:17.680
<v Speaker 1>there supposed to be more dark matter than normal matter?

0:22:17.960 --> 0:22:20.040
<v Speaker 1>And there is, but there's five times as much. But

0:22:20.080 --> 0:22:22.520
<v Speaker 1>here we're sort of spreading it evenly through space, so

0:22:22.600 --> 0:22:25.159
<v Speaker 1>we can imagine how it might affect the Solar System,

0:22:25.240 --> 0:22:28.040
<v Speaker 1>but we we actually don't sort of know that, right Like,

0:22:28.080 --> 0:22:30.359
<v Speaker 1>it could be all concentrated in my thumb, or it

0:22:30.359 --> 0:22:33.280
<v Speaker 1>could just be kind of this haze that's covering everything. Yes,

0:22:33.359 --> 0:22:36.600
<v Speaker 1>it could all be concentrated in your thumb. Now there's

0:22:36.600 --> 0:22:38.880
<v Speaker 1>some limits. I mean, if dark matter was really really

0:22:38.880 --> 0:22:41.080
<v Speaker 1>clumpy and it was all concentrated in your thumb, that

0:22:41.119 --> 0:22:43.160
<v Speaker 1>would be a huge amount of mass and we would

0:22:43.200 --> 0:22:45.879
<v Speaker 1>definitely notice that, Like your thumb would be attracting stuff

0:22:45.920 --> 0:22:47.800
<v Speaker 1>to it all the time, like a crazy weird magnet.

0:22:49.359 --> 0:22:52.600
<v Speaker 1>My thumb is pretty attractive. Well do you hitch high

0:22:52.600 --> 0:22:56.800
<v Speaker 1>a lot? Did your thumb stop a lot of cars? Uh? Yeah, No,

0:22:56.920 --> 0:22:58.800
<v Speaker 1>I get I get compliments from about my thumb all

0:22:58.840 --> 0:23:02.440
<v Speaker 1>the time. I'm gonna believe that for a second. I

0:23:02.480 --> 0:23:04.400
<v Speaker 1>don't believe that for a second. You're like, I've seen

0:23:04.440 --> 0:23:07.600
<v Speaker 1>your thumb. It's nothing special. Next time we're in a

0:23:07.680 --> 0:23:09.760
<v Speaker 1>random situation, I'm gonna ask somebody to come in on

0:23:09.760 --> 0:23:11.679
<v Speaker 1>your thumb and we'll just see what they say. All right,

0:23:11.760 --> 0:23:17.480
<v Speaker 1>let's do it. If you take one protons worth of

0:23:17.640 --> 0:23:20.399
<v Speaker 1>dark matter per thumb and you add that all up

0:23:20.440 --> 0:23:23.160
<v Speaker 1>inside the Solar system, it adds up to a lot.

0:23:23.240 --> 0:23:26.080
<v Speaker 1>It's like ten to the ten kms of dark matter

0:23:26.119 --> 0:23:28.080
<v Speaker 1>in the Solar system, and that might seem like, oh

0:23:28.119 --> 0:23:29.960
<v Speaker 1>my gosh, that's a huge amount, ten to the ten,

0:23:30.480 --> 0:23:33.000
<v Speaker 1>but it's small compared to the Sun, which is like

0:23:33.040 --> 0:23:36.920
<v Speaker 1>ten to the thirty. So dark matter, if you spread

0:23:36.960 --> 0:23:39.160
<v Speaker 1>it out evenly, there's not enough of it in our

0:23:39.160 --> 0:23:42.119
<v Speaker 1>solar system to influence the gravity on top of what

0:23:42.160 --> 0:23:44.280
<v Speaker 1>the Sun is already doing. So you're saying, like, our

0:23:44.280 --> 0:23:47.760
<v Speaker 1>solar system is a it's kind of a concentrated part

0:23:47.760 --> 0:23:49.680
<v Speaker 1>of the universe where there's a lot of mass here

0:23:50.440 --> 0:23:53.720
<v Speaker 1>as opposed to like in the empty gas between solar systems,

0:23:53.760 --> 0:23:56.680
<v Speaker 1>And so you're saying, like, here in our neighborhood, there

0:23:56.800 --> 0:23:59.240
<v Speaker 1>is just a lot more of the regular stuff than

0:23:59.280 --> 0:24:01.240
<v Speaker 1>there is dark matter. So dark matter is kind of

0:24:01.280 --> 0:24:05.240
<v Speaker 1>negligible right here where we are, exactly. Dark matter is

0:24:05.280 --> 0:24:08.000
<v Speaker 1>negligible for the for the gravitational effects of the Earth

0:24:08.040 --> 0:24:10.680
<v Speaker 1>and the Sun, exactly right, because mostly the Sun is

0:24:10.720 --> 0:24:13.480
<v Speaker 1>a concentrated blob of normal matter, and we don't think

0:24:13.480 --> 0:24:15.920
<v Speaker 1>the dark matter has been concentrated in that same way.

0:24:16.119 --> 0:24:18.119
<v Speaker 1>Not only is it negligible, but it's also going to

0:24:18.200 --> 0:24:20.840
<v Speaker 1>spread out evenly all around us, right, So it wouldn't

0:24:21.000 --> 0:24:23.200
<v Speaker 1>it would be sort of maybe tugging us in all

0:24:23.280 --> 0:24:25.720
<v Speaker 1>directions at the same time and maybe not really affecting

0:24:25.760 --> 0:24:28.359
<v Speaker 1>the orbit. It would be tugging us in all directions.

0:24:28.440 --> 0:24:32.159
<v Speaker 1>But um physics says that if you're moving in an orbit,

0:24:32.440 --> 0:24:34.920
<v Speaker 1>you're affected by the mass of all the stuff that's

0:24:34.920 --> 0:24:37.359
<v Speaker 1>the smaller radius than your orbit, and you actually it

0:24:37.400 --> 0:24:41.520
<v Speaker 1>doesn't matter how that's distributed inside that radius. If it's

0:24:41.560 --> 0:24:43.600
<v Speaker 1>like you know, like if the Sun was a point particle,

0:24:43.880 --> 0:24:46.440
<v Speaker 1>or the Sun was its normal size or twice its size,

0:24:46.480 --> 0:24:48.919
<v Speaker 1>if it doesn't change its mass, the physics says that

0:24:48.960 --> 0:24:51.360
<v Speaker 1>it doesn't affect how you're how the force of gravity

0:24:51.400 --> 0:24:53.480
<v Speaker 1>acts on that body. It all integrates out to be

0:24:53.480 --> 0:24:55.879
<v Speaker 1>the same thing. So the dark matter outside of our

0:24:56.000 --> 0:24:59.400
<v Speaker 1>orbit is just cannot affect our orbit. That's right. It's

0:24:59.440 --> 0:25:01.119
<v Speaker 1>sort of like that episode we talked about where you

0:25:01.160 --> 0:25:03.919
<v Speaker 1>jump into the center of the Earth. You're only affected

0:25:03.960 --> 0:25:06.879
<v Speaker 1>by the mass of the Earth has a smaller radius

0:25:06.880 --> 0:25:09.640
<v Speaker 1>than you do. Everything else outside of you cancels out

0:25:09.680 --> 0:25:12.200
<v Speaker 1>because there's always one bit tugging you here and another

0:25:12.200 --> 0:25:15.119
<v Speaker 1>bit tugging you the other direction, and the stuff with

0:25:15.160 --> 0:25:18.240
<v Speaker 1>a smaller orbit adds up to give you an overall tug.

0:25:18.400 --> 0:25:20.920
<v Speaker 1>That's the same as if you just put a particle

0:25:21.240 --> 0:25:23.240
<v Speaker 1>with the mass of that stuff at the center of

0:25:23.280 --> 0:25:24.960
<v Speaker 1>mass of it, which would be the center of the Earth.

0:25:25.520 --> 0:25:27.679
<v Speaker 1>So in this case you would still be affected by

0:25:27.760 --> 0:25:29.639
<v Speaker 1>dark matter, and we are, like the orbit of the

0:25:29.680 --> 0:25:32.359
<v Speaker 1>Earth is affected by the dark matter in the Solar system,

0:25:32.680 --> 0:25:35.000
<v Speaker 1>but it's you know, one part in tend of the twenty,

0:25:35.200 --> 0:25:37.359
<v Speaker 1>so it's not measurable. So you're saying that we do

0:25:37.480 --> 0:25:39.520
<v Speaker 1>sort of have like an equivalent of a dark Sun

0:25:39.720 --> 0:25:42.440
<v Speaker 1>in the middle of our Solar system affecting our orbit.

0:25:42.520 --> 0:25:45.359
<v Speaker 1>It's just very small, that's right. Dark matter is changing

0:25:45.400 --> 0:25:48.440
<v Speaker 1>our lives. It makes our years shorter by one part

0:25:48.480 --> 0:25:51.199
<v Speaker 1>and tend to the twenty because it speeds up the

0:25:51.200 --> 0:25:53.919
<v Speaker 1>Earth because of its additional gravity. But it's you know,

0:25:53.960 --> 0:25:56.639
<v Speaker 1>it's not something we can measure on the galaxy scale,

0:25:56.640 --> 0:25:59.080
<v Speaker 1>though you can. And the reason it affects things on

0:25:59.119 --> 0:26:01.480
<v Speaker 1>the galaxy scale, the reason that you can detect it

0:26:01.480 --> 0:26:04.080
<v Speaker 1>at all, is that galaxies are just so much bigger

0:26:04.119 --> 0:26:06.000
<v Speaker 1>than solar systems, and so they add up to a

0:26:06.160 --> 0:26:10.320
<v Speaker 1>huge amount of dark matter um compared to the mass

0:26:10.359 --> 0:26:12.719
<v Speaker 1>of the Sun. Like the stuff in between solar systems

0:26:12.720 --> 0:26:15.280
<v Speaker 1>adds up. But maybe the stuff within a Solar System

0:26:15.320 --> 0:26:17.960
<v Speaker 1>doesn't add up to much exactly. So when you're calculating

0:26:18.200 --> 0:26:21.479
<v Speaker 1>the force of gravity on the Sun as it rotates

0:26:21.520 --> 0:26:24.840
<v Speaker 1>around the center of the galaxy, it's influenced by everything

0:26:25.200 --> 0:26:27.720
<v Speaker 1>that has a radius smaller than it's compared to the

0:26:27.720 --> 0:26:30.159
<v Speaker 1>center of the galaxy, and that's a huge amount of

0:26:30.240 --> 0:26:32.399
<v Speaker 1>dark matter. Well, I think that's probably why I was

0:26:32.480 --> 0:26:34.760
<v Speaker 1>late to the recording of this podcast. It's it was,

0:26:34.840 --> 0:26:38.920
<v Speaker 1>you know, dark matter shortening my ear. That's right, Well,

0:26:38.960 --> 0:26:42.359
<v Speaker 1>you used up your one you know, one ten, one

0:26:42.359 --> 0:26:44.080
<v Speaker 1>in ten of the twenty a year, so you need

0:26:44.080 --> 0:26:48.880
<v Speaker 1>another excuse next, no build over my entire life and

0:26:48.960 --> 0:26:51.200
<v Speaker 1>leading up to me being late to this podcast, it's

0:26:51.200 --> 0:26:52.920
<v Speaker 1>not that you were finishing that one last piece of

0:26:52.960 --> 0:26:57.399
<v Speaker 1>banana cream cake. No, no, I finished that, Yester. Al Right.

0:26:57.440 --> 0:27:01.199
<v Speaker 1>So that's Marki's question about whether dark matter affects the

0:27:01.280 --> 0:27:03.800
<v Speaker 1>orbits of the planets in our Solar system, and the

0:27:03.840 --> 0:27:07.480
<v Speaker 1>answer is yes, we kind of do have a dark

0:27:08.000 --> 0:27:11.960
<v Speaker 1>matter sun in our dark dark matter mass in our

0:27:12.480 --> 0:27:16.679
<v Speaker 1>Solar system, making everything just a little bit faster, go

0:27:16.800 --> 0:27:19.879
<v Speaker 1>faster around the Solar System, but it's really not measurable,

0:27:19.960 --> 0:27:22.520
<v Speaker 1>and without seeing how galaxy spin, I don't think we

0:27:22.560 --> 0:27:25.040
<v Speaker 1>ever would have discovered dark matter just by looking at

0:27:25.040 --> 0:27:27.280
<v Speaker 1>the orbit of the Earth. All right, thank you, Margie,

0:27:27.400 --> 0:27:29.919
<v Speaker 1>And so we'll get to our last question from Prita

0:27:30.359 --> 0:27:45.920
<v Speaker 1>when we get back from a quick break. Alright, our

0:27:46.000 --> 0:27:49.240
<v Speaker 1>last question of this episode comes from Preda, and she

0:27:49.359 --> 0:27:54.439
<v Speaker 1>has a question about why the nucleus is stable. I

0:27:54.440 --> 0:27:56.840
<v Speaker 1>imagine the nucleus of an atom, right, what else could

0:27:56.840 --> 0:27:58.680
<v Speaker 1>it be about the nucleus of what the cell, the

0:27:58.800 --> 0:28:03.160
<v Speaker 1>nucleus of a banana? At This is a physics podcast, man,

0:28:03.280 --> 0:28:07.000
<v Speaker 1>So here's a Prettius question. My name is Pritto, and

0:28:07.240 --> 0:28:10.679
<v Speaker 1>my question is why is the nucleus of an atom

0:28:10.800 --> 0:28:14.880
<v Speaker 1>even stable? The nucleus of atom has protons which are

0:28:14.920 --> 0:28:19.680
<v Speaker 1>positively charged. They're supposed to reple each other and they're

0:28:19.680 --> 0:28:23.239
<v Speaker 1>not supposed to stay to Please explain why does this happen? Right?

0:28:23.280 --> 0:28:26.119
<v Speaker 1>So Preta wants to know how a nucleus can be

0:28:26.200 --> 0:28:29.880
<v Speaker 1>stable like because then the nuclei of atoms are made

0:28:29.920 --> 0:28:35.199
<v Speaker 1>up of protons mostly right, and nucle and neutrons but

0:28:35.280 --> 0:28:37.919
<v Speaker 1>mostly but a lot of protons, and all the protons

0:28:37.960 --> 0:28:42.400
<v Speaker 1>are positively charged, so they should be repelling each other

0:28:43.000 --> 0:28:46.000
<v Speaker 1>with the electro magnetic force. Yeah, So how how do

0:28:46.320 --> 0:28:48.800
<v Speaker 1>how can they all stay together? How? How is it

0:28:48.880 --> 0:28:50.880
<v Speaker 1>that you and I are here? Daniel? Yeah, I love

0:28:50.920 --> 0:28:53.680
<v Speaker 1>that we're talking about forces and force, bouncing and all

0:28:53.720 --> 0:28:56.280
<v Speaker 1>these questions today. This is a great question, right, And

0:28:56.280 --> 0:28:58.360
<v Speaker 1>they all are positive and they are pushing away from

0:28:58.400 --> 0:29:00.840
<v Speaker 1>from each other. So what holds it together? There? Um?

0:29:01.000 --> 0:29:03.400
<v Speaker 1>I don't know, that's a really positive thing, I think, yeah,

0:29:03.880 --> 0:29:07.480
<v Speaker 1>and kind of negative to well. I'm kind of neutral

0:29:07.480 --> 0:29:11.000
<v Speaker 1>on the topic. But I was wondering whether people knew

0:29:11.000 --> 0:29:13.000
<v Speaker 1>about this, like is this a common question? Do people

0:29:13.040 --> 0:29:16.640
<v Speaker 1>have an idea? So actually, yesterday when my kids were

0:29:16.640 --> 0:29:19.160
<v Speaker 1>watching a movie, I walked around the mall here in

0:29:19.200 --> 0:29:22.200
<v Speaker 1>Irvine and I asked people, um if they knew what

0:29:22.360 --> 0:29:25.720
<v Speaker 1>kept the nucleus together? And I got some interesting answers. Cool.

0:29:25.800 --> 0:29:27.680
<v Speaker 1>So here's what people had to say. Do you know

0:29:27.720 --> 0:29:30.160
<v Speaker 1>why the nucleus stays together? Like what keeps it together

0:29:30.160 --> 0:29:33.880
<v Speaker 1>if it's all positive charges opposite course on the outside,

0:29:34.120 --> 0:29:39.440
<v Speaker 1>or what holds an atom together? Huh? Right, I'm sure

0:29:39.480 --> 0:29:42.080
<v Speaker 1>I learned that in physics long ago, but I can't remember.

0:29:42.480 --> 0:29:45.480
<v Speaker 1>I don't know about that one. I don't know more

0:29:45.480 --> 0:29:51.200
<v Speaker 1>electrons they stay together because the more protons there are,

0:29:51.240 --> 0:29:53.239
<v Speaker 1>the heavier the atomic weight. So what do you think

0:29:53.320 --> 0:29:56.080
<v Speaker 1>Now we're getting random people on the street to answer

0:29:56.160 --> 0:29:58.040
<v Speaker 1>listen to questions. Eventually we don't even need to be

0:29:58.080 --> 0:30:02.200
<v Speaker 1>here anymore, right, Yeah, I wish you just crowdsource this podcast,

0:30:03.720 --> 0:30:05.880
<v Speaker 1>just going the mom and be like, hey, here's the question.

0:30:06.280 --> 0:30:08.440
<v Speaker 1>We'll give you twenty bucks to talk about it for

0:30:08.440 --> 0:30:11.840
<v Speaker 1>forty minutes. Exactly. That's our retirement plan. Uh No, this

0:30:11.840 --> 0:30:13.880
<v Speaker 1>one was interesting enough, and I really was curious about

0:30:13.880 --> 0:30:15.719
<v Speaker 1>what people knew. So I thought, we don't often do

0:30:15.760 --> 0:30:17.440
<v Speaker 1>this for listening to questions, but I did the man

0:30:17.480 --> 0:30:19.720
<v Speaker 1>of the street interviews for this one. Well, I'm surprised

0:30:19.760 --> 0:30:24.040
<v Speaker 1>that people kind of I knew a little bit of

0:30:24.160 --> 0:30:26.320
<v Speaker 1>what you were talking about, right, because they they were like, oh,

0:30:26.480 --> 0:30:28.760
<v Speaker 1>you mean like the O an Adam, and they sort

0:30:28.760 --> 0:30:31.120
<v Speaker 1>of understood the question because it's not an easy question

0:30:31.200 --> 0:30:33.440
<v Speaker 1>to get your head around, right. No, it's not an

0:30:33.440 --> 0:30:36.239
<v Speaker 1>easy question. It's not a simple answer. But you're right,

0:30:36.240 --> 0:30:38.720
<v Speaker 1>people understood the question and that was cool. Um, so

0:30:38.760 --> 0:30:40.520
<v Speaker 1>I think it is a common question. And all these

0:30:40.560 --> 0:30:42.360
<v Speaker 1>people after I asked them, they're like, we tell me

0:30:42.400 --> 0:30:44.440
<v Speaker 1>what is the answer? You can't just walk away after

0:30:44.520 --> 0:30:46.680
<v Speaker 1>asking me that question. I have to know now it's

0:30:46.720 --> 0:30:50.320
<v Speaker 1>like inspire this burning desire and them to understand why

0:30:50.360 --> 0:30:52.520
<v Speaker 1>their nuclei were not flying apart. Do you try to

0:30:52.560 --> 0:30:54.880
<v Speaker 1>when you're roaming the malls looking for people? Do you

0:30:54.920 --> 0:30:57.320
<v Speaker 1>try to always hit like the you know, the dad

0:30:57.600 --> 0:30:59.840
<v Speaker 1>or the mom just waiting for their kids or their

0:31:00.240 --> 0:31:02.920
<v Speaker 1>spouse who's dropping. I try to ask people who are

0:31:02.920 --> 0:31:05.360
<v Speaker 1>on their phone board. Yeah. I don't interrupt people in

0:31:05.360 --> 0:31:07.800
<v Speaker 1>conversation or people who look like they're going somewhere. I

0:31:07.840 --> 0:31:09.600
<v Speaker 1>look for somebody who's like sitting there on their phone

0:31:09.640 --> 0:31:12.520
<v Speaker 1>obviously waiting for somebody to like try on pants or something,

0:31:13.120 --> 0:31:16.040
<v Speaker 1>so they don't they don't. I don't want to interrupt

0:31:16.040 --> 0:31:18.520
<v Speaker 1>somebody's day. You're going to the dressing room, You're like, hey,

0:31:19.320 --> 0:31:24.560
<v Speaker 1>I have a physics question for you, friendly neighborhood physicist.

0:31:24.720 --> 0:31:27.920
<v Speaker 1>Physicists arrested at local mall and then I ask people

0:31:27.920 --> 0:31:30.040
<v Speaker 1>in the next cell when I get arrested. All right,

0:31:30.120 --> 0:31:32.240
<v Speaker 1>so let's ask you the question. So how is it

0:31:32.320 --> 0:31:37.320
<v Speaker 1>that protons stick together inside the nuclei of atoms? Yeah, Well,

0:31:37.400 --> 0:31:39.720
<v Speaker 1>to answer this question, you need to understand a little

0:31:39.760 --> 0:31:43.200
<v Speaker 1>bit about how protons and neutrons are held together because

0:31:43.200 --> 0:31:46.520
<v Speaker 1>protons and neutrons, remember, are not fundamental particles, but they're

0:31:46.560 --> 0:31:49.800
<v Speaker 1>made of quarks. So there's up corks and down corks,

0:31:49.880 --> 0:31:53.000
<v Speaker 1>and those particles are held together by a different force

0:31:53.080 --> 0:31:55.960
<v Speaker 1>called the strong nuclear force, and it's called the strong

0:31:56.080 --> 0:31:59.440
<v Speaker 1>nuclear force because it's super duper strong. It's much much

0:31:59.440 --> 0:32:02.720
<v Speaker 1>stronger an electromagnetism, which of course puts gravity to shame.

0:32:03.080 --> 0:32:05.920
<v Speaker 1>So the strong nuclear force is the strongest, most powerful

0:32:05.960 --> 0:32:10.040
<v Speaker 1>force we've ever discovered, and that's what holds the protons together. Yeah,

0:32:10.080 --> 0:32:13.479
<v Speaker 1>it's the reason the protons and the neutrons their bound

0:32:13.520 --> 0:32:16.720
<v Speaker 1>states of this force, so that there's quarks inside the

0:32:16.720 --> 0:32:20.240
<v Speaker 1>proton and quirks inside the neutron, and they're exchanging gluons

0:32:20.320 --> 0:32:22.280
<v Speaker 1>all the time. There is this particle called a gluon

0:32:22.760 --> 0:32:26.280
<v Speaker 1>which holds the corks together into a proton and into

0:32:26.320 --> 0:32:30.200
<v Speaker 1>a neutron. So that's what holds the protons and neutrons together.

0:32:30.320 --> 0:32:33.840
<v Speaker 1>But what what keeps the protons from repelling each other? Yeah,

0:32:33.920 --> 0:32:36.480
<v Speaker 1>so the strong nuclear force which holds them together. It's

0:32:36.600 --> 0:32:39.280
<v Speaker 1>very short range, like it's super powerful, but it doesn't

0:32:39.360 --> 0:32:42.920
<v Speaker 1>go very far, but it extends a little bit of

0:32:42.920 --> 0:32:45.680
<v Speaker 1>ways past the edge of the proton, and so what

0:32:45.760 --> 0:32:47.480
<v Speaker 1>happens is that there's a little bit of the strong

0:32:47.600 --> 0:32:50.760
<v Speaker 1>nuclear force left over between the corks inside the proton

0:32:50.800 --> 0:32:53.880
<v Speaker 1>and neutron to attract the protons and neutrons to each other.

0:32:54.160 --> 0:32:56.920
<v Speaker 1>So even this little extra bit of the strong nuclear

0:32:56.960 --> 0:33:01.000
<v Speaker 1>force is enough to overcome the pulsion of the protons

0:33:01.040 --> 0:33:04.400
<v Speaker 1>because they have the same charge. Oh really, I never

0:33:04.440 --> 0:33:07.120
<v Speaker 1>thought about that? Is that? Is that? How you explain it?

0:33:07.160 --> 0:33:11.280
<v Speaker 1>Is that the force that's keeping the protons together is

0:33:11.320 --> 0:33:14.320
<v Speaker 1>also the force that keeps a proton stuck to another proton,

0:33:14.360 --> 0:33:17.560
<v Speaker 1>because it's sort of leaks outside of the proton. Yeah. Essentially,

0:33:17.600 --> 0:33:20.040
<v Speaker 1>it's like the quarks in one proton are talking a

0:33:20.080 --> 0:33:22.480
<v Speaker 1>little bit with the quirks in the neighboring proton or

0:33:22.480 --> 0:33:25.080
<v Speaker 1>the neighboring neutron, and to them, the fact that there's

0:33:25.120 --> 0:33:27.800
<v Speaker 1>like an overall positive charge in protons and um and

0:33:27.840 --> 0:33:30.760
<v Speaker 1>not a neutrons is irrelevant because those forces are so

0:33:30.880 --> 0:33:34.200
<v Speaker 1>weak compared to the strong nuclear force. The strong nuclear

0:33:34.240 --> 0:33:38.360
<v Speaker 1>force doesn't care about your electro magnetic charge, right, Yeah, exactly,

0:33:38.400 --> 0:33:40.920
<v Speaker 1>doesn't care at all. And the corks do have electromagnetic

0:33:41.000 --> 0:33:44.040
<v Speaker 1>charges and Actually they're really weird that like two thirds

0:33:44.120 --> 0:33:47.720
<v Speaker 1>charges and minus one thirds charge. They're pretty strange, but

0:33:47.880 --> 0:33:51.080
<v Speaker 1>they're the forces are much weaker than the strong nuclear force.

0:33:51.440 --> 0:33:53.719
<v Speaker 1>So the strong nuclear force sort of leaks out of

0:33:53.760 --> 0:33:56.360
<v Speaker 1>the proton and into the next neutron and into that

0:33:56.440 --> 0:33:59.280
<v Speaker 1>next neutron, and that's how they tie themselves together. There's

0:33:59.360 --> 0:34:01.800
<v Speaker 1>enough lefto or after you make the proton or the

0:34:01.840 --> 0:34:04.320
<v Speaker 1>neutron to tie it to the next one. How can

0:34:04.360 --> 0:34:07.720
<v Speaker 1>there be any leftover? I mean, if if the proton

0:34:08.440 --> 0:34:12.600
<v Speaker 1>is stable right like it likes being held together, how

0:34:12.640 --> 0:34:16.560
<v Speaker 1>can it have any leftover? You know, attraction, doesn't it

0:34:16.600 --> 0:34:19.040
<v Speaker 1>all just cancel out within the proton? How can you

0:34:19.040 --> 0:34:22.319
<v Speaker 1>have some left over to attract more protons? Now, you're right,

0:34:22.400 --> 0:34:24.840
<v Speaker 1>and it would if all the corks inside the proton

0:34:24.960 --> 0:34:27.000
<v Speaker 1>were like right on top of each other, but they're not.

0:34:27.080 --> 0:34:29.680
<v Speaker 1>They're like all slashing around. So if you're like on

0:34:29.680 --> 0:34:32.160
<v Speaker 1>one side of the proton, you're a little bit closer

0:34:32.200 --> 0:34:34.440
<v Speaker 1>to one of the corks than the other two, and

0:34:34.520 --> 0:34:37.160
<v Speaker 1>so the force from that one little cork is enough

0:34:37.320 --> 0:34:39.520
<v Speaker 1>to have like a little bit of leftover charge. So

0:34:39.560 --> 0:34:46.560
<v Speaker 1>actually maybe two protons being stuck together makes them weaker inside, right,

0:34:47.080 --> 0:34:49.400
<v Speaker 1>each one is maybe just a little bit weaker because

0:34:49.400 --> 0:34:50.960
<v Speaker 1>they're stuck to each other. You can think of it

0:34:51.080 --> 0:34:53.520
<v Speaker 1>sort of the way you know atoms for molecules, right,

0:34:53.680 --> 0:34:58.160
<v Speaker 1>and atom is electrically neutral, right, because the protons and

0:34:58.200 --> 0:35:01.719
<v Speaker 1>the electrons right are balanced. But how do atoms form

0:35:01.800 --> 0:35:05.040
<v Speaker 1>molecules their bonds between the electrons because the electrons, you know,

0:35:05.080 --> 0:35:06.799
<v Speaker 1>they talk to each other and one like jumps from

0:35:06.840 --> 0:35:10.239
<v Speaker 1>here to there, and they exchange photons and stuff and

0:35:10.320 --> 0:35:13.759
<v Speaker 1>so um, this is like protons getting stuck together by

0:35:13.760 --> 0:35:16.560
<v Speaker 1>those extra little bits of leftover forces. So it's a

0:35:16.600 --> 0:35:20.480
<v Speaker 1>strong nuclear force that's so much more powerful than electromagnetism

0:35:20.520 --> 0:35:23.759
<v Speaker 1>that even the little extra leftover bits can overpower the

0:35:23.800 --> 0:35:26.440
<v Speaker 1>protons pushing away from each other. This strikes me as

0:35:26.400 --> 0:35:30.759
<v Speaker 1>a little bit as a nuclear infidelity. You know, like

0:35:30.960 --> 0:35:33.920
<v Speaker 1>you've got three quarts being perfectly happy in a bond

0:35:34.320 --> 0:35:36.439
<v Speaker 1>to make a proton, but then one of them is like, hey,

0:35:36.600 --> 0:35:38.960
<v Speaker 1>look at that. There's some other quartz over there, and

0:35:39.000 --> 0:35:45.160
<v Speaker 1>that other trio mana protons um a little bit attracted

0:35:45.200 --> 0:35:47.440
<v Speaker 1>to them too, and so that's what brings the two

0:35:47.480 --> 0:35:50.279
<v Speaker 1>things together. Right. Yeah, quarks feel a lot of love, right,

0:35:50.719 --> 0:35:53.640
<v Speaker 1>They they're happy to to share their love with quarks

0:35:53.719 --> 0:35:57.799
<v Speaker 1>even inside other protons and neutrons, and and and you know,

0:35:57.880 --> 0:35:59.640
<v Speaker 1>the sort of a limit how much you can do

0:35:59.680 --> 0:36:02.719
<v Speaker 1>this because these forces are very short range, and so

0:36:02.840 --> 0:36:06.719
<v Speaker 1>the bigger the nucleus gets, then the weaker the sort

0:36:06.760 --> 0:36:09.080
<v Speaker 1>of the stability of the nucleus. If you try to

0:36:09.080 --> 0:36:11.680
<v Speaker 1>make a nucleus that's too big, then like the protons

0:36:11.800 --> 0:36:14.560
<v Speaker 1>on the opposite sides of the nucleus, they'll feel the

0:36:14.600 --> 0:36:17.680
<v Speaker 1>electrostatic repulsion, but they won't be close enough to feel

0:36:17.680 --> 0:36:20.880
<v Speaker 1>the strong nuclear force anymore. And that's why like heavier

0:36:20.920 --> 0:36:24.239
<v Speaker 1>elements are less stable and more likely like decay radioactively.

0:36:24.440 --> 0:36:27.080
<v Speaker 1>That's why we use uranium and like uranium two thirty

0:36:27.120 --> 0:36:31.280
<v Speaker 1>five to do radioactive fission, and not like helium or lithium.

0:36:31.560 --> 0:36:34.440
<v Speaker 1>Put enough protons together, they bunch up, and at some

0:36:34.560 --> 0:36:38.319
<v Speaker 1>point the nuclear force, the strong force, isn't enough. They

0:36:38.320 --> 0:36:41.040
<v Speaker 1>start to repel each other exactly because the strong force

0:36:41.320 --> 0:36:44.279
<v Speaker 1>drops very quickly with distance, right, And so if you're

0:36:44.280 --> 0:36:46.560
<v Speaker 1>far enough away from the proton, then you don't feel

0:36:46.560 --> 0:36:48.160
<v Speaker 1>it then all. Then it's like all the corks are

0:36:48.200 --> 0:36:50.279
<v Speaker 1>on top of each other, and so that's why there's

0:36:50.320 --> 0:36:52.840
<v Speaker 1>like a maximum size you can make to a nucleus

0:36:52.920 --> 0:36:55.279
<v Speaker 1>because the strong force which holds it together it's a

0:36:55.400 --> 0:36:57.759
<v Speaker 1>very short range. And when the nucleus gets sort of

0:36:57.800 --> 0:37:00.720
<v Speaker 1>bigger than that range, then it can't do the job anymore.

0:37:00.840 --> 0:37:02.520
<v Speaker 1>It's like, you know, you trying to hold a bunch

0:37:02.520 --> 0:37:05.000
<v Speaker 1>of balloons, right, Imagine trying to hold a huge pile

0:37:05.000 --> 0:37:07.920
<v Speaker 1>of balloons. Is a maximum number you can hold until

0:37:08.000 --> 0:37:10.120
<v Speaker 1>somebody You need somebody else to come over and grab

0:37:10.160 --> 0:37:12.520
<v Speaker 1>a bunch of them. So then the nucleus splits into two.

0:37:13.040 --> 0:37:18.920
<v Speaker 1>And that's what happens in a radioactive decay. Alright, So

0:37:18.960 --> 0:37:21.439
<v Speaker 1>then that's the answer to the question. The nucleus stays

0:37:21.520 --> 0:37:25.040
<v Speaker 1>together even though the protons are are repelling each other,

0:37:25.080 --> 0:37:27.600
<v Speaker 1>they're trying to push each other apart. There is another

0:37:27.640 --> 0:37:31.480
<v Speaker 1>force that leaks out from inside of each proton that

0:37:31.560 --> 0:37:34.480
<v Speaker 1>then sort of links up the two protons together, and

0:37:34.520 --> 0:37:38.600
<v Speaker 1>that force is stronger than the electric magnetic repulsion exactly.

0:37:38.680 --> 0:37:41.000
<v Speaker 1>That's what holds them together, and that's what holds us

0:37:41.040 --> 0:37:44.520
<v Speaker 1>together with you, listeners, the force of these questions. You guys,

0:37:44.600 --> 0:37:47.239
<v Speaker 1>have all these questions bouncing around your head, and you

0:37:47.280 --> 0:37:49.319
<v Speaker 1>send them to us, and we love thinking about them,

0:37:49.320 --> 0:37:50.920
<v Speaker 1>we love talking about them, and we love trying to

0:37:50.920 --> 0:37:53.160
<v Speaker 1>explain them to you. And really it's this love of

0:37:53.200 --> 0:37:55.759
<v Speaker 1>the universe and this desire to ask questions and this

0:37:56.160 --> 0:37:58.800
<v Speaker 1>hunger to get the answers that brings us all together.

0:37:59.040 --> 0:38:02.120
<v Speaker 1>All right, Well, thank you so much to Florence, Margie

0:38:02.160 --> 0:38:05.200
<v Speaker 1>and Pritta for sending in their questions, and thanks to

0:38:05.360 --> 0:38:07.399
<v Speaker 1>all of you who are sending us questions as well.

0:38:07.440 --> 0:38:10.600
<v Speaker 1>We enjoy reading them and it kind of makes our

0:38:10.680 --> 0:38:13.239
<v Speaker 1>day to hear from you. Guys. Absolutely, please don't stop

0:38:13.280 --> 0:38:17.360
<v Speaker 1>sending questions questions at Daniel and Jorge dot com. All right,

0:38:17.400 --> 0:38:20.040
<v Speaker 1>and that's our podcast. We hope you enjoyed those questions,

0:38:20.160 --> 0:38:24.480
<v Speaker 1>and stay tuned for more amazing facts and questions and

0:38:24.719 --> 0:38:28.480
<v Speaker 1>interesting perspectives about the universe. And stay tuned for the

0:38:28.520 --> 0:38:31.480
<v Speaker 1>sound of Jorge enjoying a banana cake. That's right, one

0:38:31.520 --> 0:38:35.640
<v Speaker 1>of you lucky people will win this prize. Lucky unlucky.

0:38:35.719 --> 0:38:38.800
<v Speaker 1>We're not sure, but somebody's gonna win it. Positive and negative.

0:38:39.120 --> 0:38:49.280
<v Speaker 1>See you next time. If you still have a question

0:38:49.320 --> 0:38:52.759
<v Speaker 1>after listening to all these explanations, please drop us a line.

0:38:52.800 --> 0:38:54.920
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0:38:54.960 --> 0:38:58.759
<v Speaker 1>at Facebook, Twitter, and Instagram at Daniel and Jorge That's

0:38:58.760 --> 0:39:02.040
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0:39:02.080 --> 0:39:05.200
<v Speaker 1>and Jorge dot com. Thanks for listening and remember that

0:39:05.320 --> 0:39:08.080
<v Speaker 1>Daniel and Jorge Explain the Universe is a production of

0:39:08.200 --> 0:39:11.560
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