WEBVTT - Listener Questions 36

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<v Speaker 1>Hey, or hey, do you ever wish you had more

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<v Speaker 1>than two arms? That would be weird, but sometimes it

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<v Speaker 1>would be useful. You know, if you're a parent, you're

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<v Speaker 1>carrying around a couple of kids, would be great to

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<v Speaker 1>have extra arms. Well, is it more arms do you

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<v Speaker 1>want or more hands? I think what I want is

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<v Speaker 1>maybe more brains. That would be handy. Then I can

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<v Speaker 1>have twice a number of thoughts, or one of them

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<v Speaker 1>could think while the other one naps, and then they

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<v Speaker 1>can take turns. I think I already have more ideas

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<v Speaker 1>than my arms and hands can handle. It. Sounds like

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<v Speaker 1>you need less brains then, or more arms, like a

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<v Speaker 1>whole army of arms. That would be pretty handy. It

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<v Speaker 1>would be quite a handful. I am hand with cartoonists

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<v Speaker 1>and the creator of PhD comics. Hi, I'm Daniel. I'm

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<v Speaker 1>a particle physicist and a professor at UC Irvine, and

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<v Speaker 1>I'm pretty sure I could make use of a third

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<v Speaker 1>arm if it had a hand attached to it. Where

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<v Speaker 1>would you put it? Though? In your body? Like at

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<v Speaker 1>the top of your head, that would be useful. I

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<v Speaker 1>was just gonna say it top of my head, yeah, exactly.

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<v Speaker 1>You could like scratch your nose or scratch your back.

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<v Speaker 1>Even that would be pretty handy. Yeah, but how would

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<v Speaker 1>you scratch your arm? I'd have two other arms for

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<v Speaker 1>that job, but would they reach I think the more

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<v Speaker 1>interesting question is how you would call them, Like is

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<v Speaker 1>it your right arm, your left arm, and your top arm,

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<v Speaker 1>or you're like your dominant arm, your subdominant arm, and

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<v Speaker 1>your sub subdominant arm. Maybe you could call it like

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<v Speaker 1>your color arm or your weak heart. What if it's

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<v Speaker 1>extra strong though, on the top of my head anyway,

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<v Speaker 1>lots of fun things to think about, Yeah, because it

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<v Speaker 1>is a fun universe with a lot to think about.

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<v Speaker 1>There are a lot of stars and galaxies and amazing

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<v Speaker 1>objects and invisible matter and will energy out there for

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<v Speaker 1>us to wonder about and to have questions about. No

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<v Speaker 1>matter which arm you'd like to use to scratch your head.

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<v Speaker 1>Welcome to our podcast Daniel and Jorge Explain the Universe,

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<v Speaker 1>a production of iHeartRadio in which we dig into all

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<v Speaker 1>of the heads scratching mysteries about the universe, Why it

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<v Speaker 1>looks the way it does, what color it is, if

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<v Speaker 1>we can even possibly understand it, Why everything out there

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<v Speaker 1>seems to be spinning, and why they spin in such beautiful,

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<v Speaker 1>worly patterns. We dig into all of the mysteries of

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<v Speaker 1>the universe, from the tiny quantum particle to the inside

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<v Speaker 1>of black holes, to the edge of the universe, to

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<v Speaker 1>its very beginning and its very end, because we love

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<v Speaker 1>these mysteries, and we love marinating in our understanding and

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<v Speaker 1>our ignorance. Yeah, because there are beautiful patterns out there

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<v Speaker 1>in the universe. Patterns in color, patterns, in shape patterns,

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<v Speaker 1>also in mysteries. It seems like the universe has sort

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<v Speaker 1>of a recurring pattern of always having things that are

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<v Speaker 1>difficult to explain or that don't reveal how they work

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<v Speaker 1>right away. It is interesting that the universe is mysterious,

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<v Speaker 1>but not so mysterious that we can't make progress. It's

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<v Speaker 1>like we are just smart enough to understand like the

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<v Speaker 1>next chunk of physics, but not so smart that we

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<v Speaker 1>figure it all out right away, but also not so

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<v Speaker 1>dumb that it's totally a mystery to us. We seem

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<v Speaker 1>to be sort of like fine tuned to be entertained

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<v Speaker 1>by the mysteries of this universe. You're saying, we're like

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<v Speaker 1>the goldilocks of all species in the universe, But how

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<v Speaker 1>do you know this, Daniel, how do you know we're

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<v Speaker 1>not behind? How do you know we're not actually like

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<v Speaker 1>at the back of the class roster. Yeah, we could be.

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<v Speaker 1>There might be aliens out there that I figured out

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<v Speaker 1>the physics of the universe and about ten seconds. But

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<v Speaker 1>what I'm saying is that maybe this is more fun.

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<v Speaker 1>Maybe it's more fun to be a little confused for

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<v Speaker 1>a while and then figure something out, rather than just

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<v Speaker 1>have the entire theory of everything come to you in

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<v Speaker 1>a single flash of insight. That sounds like something a

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<v Speaker 1>student who's not doing well in school might say, like, Hey,

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<v Speaker 1>I got an F because it's it's fun. It's more

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<v Speaker 1>like somebody who wants to keep the mysteries on because

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<v Speaker 1>it's part of my job. I mean, if we like

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<v Speaker 1>solved physics tomorrow, then what would I do the rest

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<v Speaker 1>of my life? Is that what you tell the funding

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<v Speaker 1>Agency's like, Hey, you paid me all this money and

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<v Speaker 1>I haven't figured anything out, but I'm having a lot

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<v Speaker 1>of fun. And really what's more important than that. It's

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<v Speaker 1>the friends you make along the way to figuring out

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<v Speaker 1>the universe. That's right, I got an F on my

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<v Speaker 1>research paper, but F stands for friends and fun. Not funding.

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<v Speaker 1>And it's not just people like me who are wondering

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<v Speaker 1>about the nature of the universe and enjoying thinking about it.

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<v Speaker 1>It's everybody sciences of the people, by the people, and

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<v Speaker 1>for the people, and that includes me and you. It

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<v Speaker 1>includes anybody who thinks about the universe, wonders why it

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<v Speaker 1>works the way that does, and tries to figure it out.

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<v Speaker 1>That's right. Everybody has questions, and sometimes we even answer

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<v Speaker 1>those questions on this podcast, although sometimes the answer is

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<v Speaker 1>we don't know. All too often the answer is we

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<v Speaker 1>don't know, so give us some money to figure it out.

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<v Speaker 1>Stay tuned. But we encourage everybody out there to engage

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<v Speaker 1>with their curiosity, to look out the universe and connect

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<v Speaker 1>with their personal questions. You know, something that I think

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<v Speaker 1>maybe people don't appreciate is how science is driven by

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<v Speaker 1>individual people's curiosity. The reason we study this and not that,

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<v Speaker 1>the reason people investigate the mating patterns of South American bats,

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<v Speaker 1>is because somebody has decided that that's the most important question,

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<v Speaker 1>the one to dedicate their life too. So I like

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<v Speaker 1>to encourage people to think about what is your most

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<v Speaker 1>important question? If you could ask a single question of

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<v Speaker 1>the universe and get an answer what would it be?

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<v Speaker 1>And so we encourage our listener to think about the

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<v Speaker 1>universe and to write to us with their questions. Yeah,

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<v Speaker 1>we get questions all the time, and sometimes we even

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<v Speaker 1>answer them on the podcast. We will pull up a

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<v Speaker 1>question that we get and we'll try to give you

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<v Speaker 1>our best answer on the air. Answer Right. We answer

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<v Speaker 1>all of our questions that listeners send us to questions

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<v Speaker 1>at Daniel and Jorge dot com. But sometimes there's one

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<v Speaker 1>that I think is especially intriguing or requires a little

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<v Speaker 1>bit of background research, so we answer it here on

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<v Speaker 1>the podcast. And so today on the program, we'll be

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<v Speaker 1>tackling listening our questions episode number thirty six of our

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<v Speaker 1>listener question series That's Right, which puts us well above

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<v Speaker 1>a hundred in terms of questions answered on air. And

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<v Speaker 1>do we have a theme for this set of questions?

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<v Speaker 1>This one's sort of like big questions about the big Universe.

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<v Speaker 1>I see the usual then everything exactly. Today we have

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<v Speaker 1>questions about questions exactly. Let's fall into the big questions category.

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<v Speaker 1>All right, big questions here today we have three awesome

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<v Speaker 1>questions about the shape of our galaxy, about the color

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<v Speaker 1>of the universe, and also about whether the universe is

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<v Speaker 1>maybe tearing itself apart. You mean emotionally or like physically.

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<v Speaker 1>I think first physically and then emotionally. If you tear

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<v Speaker 1>yourself apart physically, then if you want to really be

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<v Speaker 1>able to tear yourself a part emotionally, Yeah, that's true.

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<v Speaker 1>Depending on how the universe collapses, you might not have

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<v Speaker 1>time for an emotional response. Well, let's dig into these

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<v Speaker 1>questions because they're pretty interesting. The first one comes from

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<v Speaker 1>Matt from Indiana. Hey, Daniel and Horey. This is Matt

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<v Speaker 1>from Indiana. I was just reading an article which has

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<v Speaker 1>some of the most recent Hubble pictures now that it's

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<v Speaker 1>successfully returned to prime time. The question I have is

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<v Speaker 1>about the galaxy aarp m adri zero zero zero two

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<v Speaker 1>D five H three. NASA is saying it's noteworthy as

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<v Speaker 1>it only has three arms to it and most spiral

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<v Speaker 1>galaxies have even numbers. Why wouldn't we find an equal

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<v Speaker 1>amount of even an odd armed disc galaxies symmetry. I'm

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<v Speaker 1>perplexed on this. Thanks for your time, cheers, Matt. All right.

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<v Speaker 1>Awesome question from Matt. He's asking not about the milk Away,

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<v Speaker 1>but a different galaxy that the Hubble Telescope has found. Yeah,

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<v Speaker 1>we have imaged so many galaxies. You know, when you

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<v Speaker 1>look up in the night sky, you mostly see stars,

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<v Speaker 1>but behind those are tiny little smudges which are galaxies.

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<v Speaker 1>And as we saw from the recent James Webb Space

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<v Speaker 1>Telescope images, every tiny little dot of sky is filled

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<v Speaker 1>with galaxies, and they have lots of really interesting shapes

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<v Speaker 1>and characteristics. And so now we have lots and lots

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<v Speaker 1>of examples of what other galaxies look like. And Matt

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<v Speaker 1>is asking about one particular one that NASA said was

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<v Speaker 1>a little weird. Yeah, and he spelled out the name

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<v Speaker 1>of it. Maybe we should spill it out again in

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<v Speaker 1>case anyone wants to look it up. Yeah, that's galaxy

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<v Speaker 1>AARP DASH M A D O R E. Then the

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<v Speaker 1>number is two one one five dash two seven three

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<v Speaker 1>And we'll put a link to NASA's page about this

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<v Speaker 1>in the show notes. They just got a catchy name,

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<v Speaker 1>my daughter. It sounds like I love you or something. Well,

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<v Speaker 1>if you look up the image and the link on

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<v Speaker 1>our website, you'll see basically a picture of our galaxy.

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<v Speaker 1>But it looks kind of interesting because it's got two

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<v Speaker 1>short arms, but then a one long arm on the bottom. Yeah,

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<v Speaker 1>lots of these spiral galaxies have the same basic features

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<v Speaker 1>you have, like a central bar and then some arms

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<v Speaker 1>swirling around them. And this one is a little weird because,

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<v Speaker 1>as you say, it has two sort of shorter arms

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<v Speaker 1>and one longer arm. And that's the thing that Matt

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<v Speaker 1>picked up on that the fact that this has three arms,

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<v Speaker 1>according to this press release, having an odd number of arms,

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<v Speaker 1>like not two or four or six is a little weird.

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<v Speaker 1>You mean, it's a little odd you have an odd

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<v Speaker 1>number of arms, because I think we're kind of used

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<v Speaker 1>to arms coming in pairs, right, I certainly have two arms,

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<v Speaker 1>though i'd like a third. But if we're talking about galaxies,

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<v Speaker 1>then it sort of makes conceptual sense to imagine them

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<v Speaker 1>being even numbers, like or basically there's just two arms

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<v Speaker 1>because you have the central bar and then the arms

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<v Speaker 1>swirling off around it. But it turns out that galaxy

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<v Speaker 1>arms are a lot more complicated than you might imagine.

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<v Speaker 1>M Well, let's dig into it. First of all, why

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<v Speaker 1>do galaxies even have arms? And I guess maybe we

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<v Speaker 1>should define what we mean by arms. It's kind of

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<v Speaker 1>like a you look at a picture of a galaxy

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<v Speaker 1>you see a cluster of stars, but then you see

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<v Speaker 1>these kind of like tendrils, these rows of stars kind

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<v Speaker 1>of swirling from the center of it. That's what an

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<v Speaker 1>arm is. Yeah, and so we tend to call these

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<v Speaker 1>things spiral arms. And there's really two things going on there,

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<v Speaker 1>the spiral nature of them and the arms. Right, So

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<v Speaker 1>let's first talk about like why are these things spiraling

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<v Speaker 1>at all? Why is there a spiral pattern in the galaxy.

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<v Speaker 1>And that just comes from the fact that the galaxy

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<v Speaker 1>is spinning. So everything in space is spinning, and as

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<v Speaker 1>it collapses, it spins faster and faster. The things a

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<v Speaker 1>different distance from the center of the galaxy don't always

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<v Speaker 1>rotate at the same like number of angles per second. Instead,

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<v Speaker 1>they tend to move through space at the same linear speed.

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<v Speaker 1>So galaxies don't rotate like a DVD or a compact disc,

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<v Speaker 1>where like every point along some line rotates with the

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<v Speaker 1>same angular speed. It's more like they rotate like runners

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<v Speaker 1>going around a track, where people on the outside tend

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<v Speaker 1>to fall behind even if they're running at the same speed. Well,

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<v Speaker 1>maybe let's take it a step back. Because you mentioned

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<v Speaker 1>everything is always spinning. What does that mean? Wh are

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<v Speaker 1>things in space necessarily spinning or do you mean, like

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<v Speaker 1>everything's moving but relative to like the center of gravity

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<v Speaker 1>or the center of a cluster of stuff, you're sort

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<v Speaker 1>of spinning around that. So everything in space is sort

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<v Speaker 1>of whizzing around. And remember that spinning is relative to

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<v Speaker 1>an axis. You like, draw a line through space and say,

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<v Speaker 1>are things moving around this point? And so you can

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<v Speaker 1>pick any axis you like. You know, pick like the

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<v Speaker 1>center of the sun. That makes sense to think about

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<v Speaker 1>the motion of the Solar system, or you know, the

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<v Speaker 1>north south axis of the Earth. But you really could

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<v Speaker 1>pick anything, but it makes most sense to pick like

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<v Speaker 1>the center of mass of a big blob of stuff

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<v Speaker 1>and ask are things moving around this center of mass?

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<v Speaker 1>And because everything is sort of flying around through space,

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<v Speaker 1>it's not stationary with respect to like the center, then

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<v Speaker 1>all that stuff tends to add up to some spinning.

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<v Speaker 1>Like it's possible for a huge blob of stuff to

0:11:37.960 --> 0:11:41.080
<v Speaker 1>not be spinning, but that would require everything inside of

0:11:41.080 --> 0:11:44.360
<v Speaker 1>it to like exactly balance all of its motion. It's

0:11:44.360 --> 0:11:47.760
<v Speaker 1>sort of unlikely, like flipping a million coins and having

0:11:47.840 --> 0:11:51.520
<v Speaker 1>exactly fifty percent of them land up heads. So any

0:11:51.559 --> 0:11:54.840
<v Speaker 1>big blob of stuff tends to have some spin around

0:11:54.840 --> 0:11:57.200
<v Speaker 1>its center. Yeah, so I guess you know, things tend

0:11:57.240 --> 0:11:59.320
<v Speaker 1>to fly in a straight line in space. But once

0:11:59.320 --> 0:12:01.280
<v Speaker 1>you get a bunch of sort of in the same area,

0:12:01.440 --> 0:12:03.719
<v Speaker 1>it's going to have some gravity and it's going to

0:12:03.880 --> 0:12:07.880
<v Speaker 1>start pulling stuff inwards towards the center of massive that blob,

0:12:07.920 --> 0:12:10.280
<v Speaker 1>and that's where the kind of the spinning happens, right,

0:12:10.320 --> 0:12:12.920
<v Speaker 1>That's where the circular emotion happens. And so that's why

0:12:12.920 --> 0:12:16.800
<v Speaker 1>everything's kind of spinning around a galaxy cluster m exactly.

0:12:16.920 --> 0:12:19.400
<v Speaker 1>And as that's been happens, it very naturally forms a

0:12:19.480 --> 0:12:22.760
<v Speaker 1>spiral pattern, right, because things that the outside get left behind.

0:12:22.800 --> 0:12:26.360
<v Speaker 1>They're not spinning as fast as things closer in. Like

0:12:26.400 --> 0:12:28.640
<v Speaker 1>if you're really close to the center, it doesn't take

0:12:28.679 --> 0:12:30.720
<v Speaker 1>you as long to go all the way around the galaxy.

0:12:30.760 --> 0:12:33.280
<v Speaker 1>For example, if you're really far out and you're moving

0:12:33.280 --> 0:12:35.800
<v Speaker 1>at the same speed, takes you a lot longer to

0:12:35.840 --> 0:12:38.199
<v Speaker 1>go all the way around the galaxy. So things and

0:12:38.240 --> 0:12:40.559
<v Speaker 1>the outside tend to get left behind, and that's why

0:12:40.600 --> 0:12:43.440
<v Speaker 1>you end up with spiral patterns in the galaxy. But

0:12:43.520 --> 0:12:46.440
<v Speaker 1>that doesn't explain why you get arms, right, if you

0:12:46.520 --> 0:12:48.520
<v Speaker 1>just have like a big blob of stuff and it

0:12:48.559 --> 0:12:50.920
<v Speaker 1>was spinning and collapsing, it would tend to sort of

0:12:50.960 --> 0:12:54.680
<v Speaker 1>like wind itself up. You wouldn't necessarily get blobs like arms.

0:12:55.000 --> 0:12:58.640
<v Speaker 1>So the spinning explains the spiral nature, but not the arms. Right,

0:12:58.679 --> 0:13:00.840
<v Speaker 1>Like if you had a big blob of out there

0:13:00.840 --> 0:13:03.680
<v Speaker 1>in space and that was evenly distributed, like a hazy cloud,

0:13:03.800 --> 0:13:06.000
<v Speaker 1>and then you just got it going, you would think

0:13:06.000 --> 0:13:08.319
<v Speaker 1>it would just kind of like swirl towards the center,

0:13:08.480 --> 0:13:11.000
<v Speaker 1>kind of like a toilet, right, there'd be no clustering.

0:13:11.000 --> 0:13:13.400
<v Speaker 1>It's just like a like a tornado, like an even

0:13:13.559 --> 0:13:15.679
<v Speaker 1>swirl down to the center. Yeah, Like if you put

0:13:15.679 --> 0:13:18.160
<v Speaker 1>a fork in spaghetti and spin it, you're gonna end

0:13:18.200 --> 0:13:20.000
<v Speaker 1>up with lots and lots and lots of strands, not

0:13:20.120 --> 0:13:22.640
<v Speaker 1>like a few big clumps. But what we see in

0:13:22.760 --> 0:13:25.320
<v Speaker 1>galaxies is it we've got like really big chunks. We

0:13:25.400 --> 0:13:28.120
<v Speaker 1>got like two or four or three in this case,

0:13:28.480 --> 0:13:31.400
<v Speaker 1>chunks of stuff flying out in this spiral pattern, or

0:13:31.480 --> 0:13:34.480
<v Speaker 1>more like the three giant or three or four giant

0:13:34.760 --> 0:13:37.200
<v Speaker 1>spaghetti noodles, right, instead of like a bunch of little

0:13:37.200 --> 0:13:41.880
<v Speaker 1>spaghetti noodles. Somehow, the spaghetti's kind of clustering to giant

0:13:42.400 --> 0:13:48.080
<v Speaker 1>strands of spaghetti. Yeah, exactly like metapasta or something megapasta formations.

0:13:48.280 --> 0:13:50.360
<v Speaker 1>And so a lot of people think that when you're

0:13:50.400 --> 0:13:53.160
<v Speaker 1>looking at a galaxy and you're looking at these spiral arms,

0:13:53.200 --> 0:13:55.800
<v Speaker 1>that you're looking at structures of matter, that like, the

0:13:56.000 --> 0:13:59.560
<v Speaker 1>arms are a blob of stars like a blob of spaghetti,

0:13:59.600 --> 0:14:01.880
<v Speaker 1>and that whole arm is sort of rotating, that the

0:14:02.000 --> 0:14:05.280
<v Speaker 1>stars are moving with the arm. But that's actually not

0:14:05.480 --> 0:14:09.960
<v Speaker 1>the case. The arms are not structures of matter. They're

0:14:10.000 --> 0:14:14.120
<v Speaker 1>just density waves. They're more like traffic patterns in cars,

0:14:14.760 --> 0:14:18.120
<v Speaker 1>you know, like a traffic wave can move along the highway,

0:14:18.320 --> 0:14:20.760
<v Speaker 1>making some cars slow down and some cars speed up

0:14:20.840 --> 0:14:23.600
<v Speaker 1>or clump together, But the cars don't necessarily move with

0:14:23.640 --> 0:14:26.120
<v Speaker 1>those waves in the same way the arms in the

0:14:26.200 --> 0:14:30.760
<v Speaker 1>galaxy are rotating. But stars don't necessarily rotate with the arms.

0:14:31.000 --> 0:14:32.920
<v Speaker 1>They can be left behind by the arm, the arm

0:14:32.960 --> 0:14:36.080
<v Speaker 1>can catch up with them. The stars don't move with

0:14:36.240 --> 0:14:38.120
<v Speaker 1>the arms. Well, first of all, what do you mean,

0:14:38.160 --> 0:14:40.360
<v Speaker 1>because there aren't the arms made of stars? Like, if

0:14:40.360 --> 0:14:42.360
<v Speaker 1>we can see them in the night sky in space,

0:14:42.640 --> 0:14:44.960
<v Speaker 1>that means it's bright, and so that means we're seeing

0:14:45.280 --> 0:14:47.920
<v Speaker 1>the stars in them. Yeah, they are made of stars.

0:14:47.920 --> 0:14:49.920
<v Speaker 1>For sure, the same with the like traffic patterns are

0:14:49.960 --> 0:14:52.720
<v Speaker 1>made of cars. But the things that make the arm

0:14:52.760 --> 0:14:55.360
<v Speaker 1>the arm is that there's a denser spot of stars.

0:14:55.400 --> 0:14:59.040
<v Speaker 1>There's more stars there than somewhere else. But as the

0:14:59.280 --> 0:15:03.120
<v Speaker 1>arm moves, sort of moves through the stars the same

0:15:03.160 --> 0:15:06.600
<v Speaker 1>way that like waves move through water, but the individual

0:15:06.680 --> 0:15:10.200
<v Speaker 1>particles of water don't necessarily move with the wave. Right,

0:15:10.440 --> 0:15:12.760
<v Speaker 1>the wave is motion of the water. Oh, I see

0:15:12.760 --> 0:15:14.240
<v Speaker 1>what you're saying. You're saying, like if I looked at

0:15:14.320 --> 0:15:17.760
<v Speaker 1>a sped up or fast forwarded movie of a galaxy,

0:15:18.000 --> 0:15:20.400
<v Speaker 1>I would see it looking like it's a squirrel, like

0:15:20.400 --> 0:15:23.160
<v Speaker 1>it's spinning, But it's not actually spinning, you're saying. It

0:15:23.480 --> 0:15:26.760
<v Speaker 1>just has these waves running through it that go around.

0:15:26.960 --> 0:15:29.120
<v Speaker 1>The waves are spinning, But if you tracked a wave

0:15:29.280 --> 0:15:31.680
<v Speaker 1>and you also tracked an individual star, you would not

0:15:31.800 --> 0:15:35.560
<v Speaker 1>necessarily see them move together, like a star can be

0:15:35.680 --> 0:15:37.920
<v Speaker 1>part of an arm and then later not part of

0:15:37.920 --> 0:15:41.040
<v Speaker 1>an arm, and then part of another arm. Whoa, and

0:15:41.400 --> 0:15:43.040
<v Speaker 1>so how do we know this because we haven't been

0:15:43.120 --> 0:15:45.440
<v Speaker 1>looking long enough for us to see that. Yeah, it's

0:15:45.440 --> 0:15:48.040
<v Speaker 1>a really interesting idea. It's only been around for a

0:15:48.080 --> 0:15:51.680
<v Speaker 1>few decades, and it's not one hundred percent certain, though

0:15:51.680 --> 0:15:53.920
<v Speaker 1>in the last few years we've got some evidence that

0:15:53.960 --> 0:15:56.640
<v Speaker 1>this is true because we've looked at the color of

0:15:56.760 --> 0:15:59.600
<v Speaker 1>light in these stars. Because the galactic arms tend to

0:15:59.600 --> 0:16:03.040
<v Speaker 1>be aligned with star formation, these galactic arms are places

0:16:03.080 --> 0:16:06.160
<v Speaker 1>of greater density, which means you get more stars being

0:16:06.200 --> 0:16:08.960
<v Speaker 1>made because you're compressing the gas. So you tend to

0:16:08.960 --> 0:16:11.760
<v Speaker 1>have younger stars in the arms as they are forming,

0:16:12.040 --> 0:16:15.040
<v Speaker 1>and younger stars tend to be bluer because bluer stars

0:16:15.080 --> 0:16:17.680
<v Speaker 1>don't live as long. So anyway, the long story short,

0:16:17.720 --> 0:16:19.960
<v Speaker 1>you can look at the pattern of color in these

0:16:20.080 --> 0:16:22.680
<v Speaker 1>arms and you can see how sort of how old

0:16:22.680 --> 0:16:25.200
<v Speaker 1>they are and the age of stars within the arms,

0:16:25.480 --> 0:16:28.200
<v Speaker 1>and so you can sort of confirm this hypothesis, though

0:16:28.400 --> 0:16:31.320
<v Speaker 1>I should say it's not a one hundred percent totally established.

0:16:31.760 --> 0:16:34.200
<v Speaker 1>So you're saying the arms of a galaxy are actually

0:16:34.400 --> 0:16:38.200
<v Speaker 1>kind of like waves that are going through the huge

0:16:38.240 --> 0:16:42.480
<v Speaker 1>cloud of stars in the galaxy. But what's causing these waves?

0:16:42.760 --> 0:16:45.440
<v Speaker 1>So these are density waves, So they're just caused by

0:16:45.440 --> 0:16:48.440
<v Speaker 1>things not being totally smooth, the same way like all

0:16:48.520 --> 0:16:52.000
<v Speaker 1>gravitational effects are. If you have a little perburbation, things

0:16:52.000 --> 0:16:54.600
<v Speaker 1>aren't totally smooth. Then gravity tends to pull on that

0:16:54.640 --> 0:16:58.240
<v Speaker 1>and exaggerated, so gravity will take a little perburbation in

0:16:58.320 --> 0:17:01.360
<v Speaker 1>like a totally smooth clump and turn it into larger

0:17:01.400 --> 0:17:05.160
<v Speaker 1>and larger perturbations. So it's not again totally understood where

0:17:05.200 --> 0:17:08.320
<v Speaker 1>these come from and why they last so long. But

0:17:08.400 --> 0:17:11.480
<v Speaker 1>they think they come from original density perturbations and like

0:17:11.560 --> 0:17:15.080
<v Speaker 1>the central clump of the galaxy. So they are structures.

0:17:15.080 --> 0:17:17.960
<v Speaker 1>Then you said earlier that they weren't structures. So it

0:17:18.119 --> 0:17:20.560
<v Speaker 1>is there because the stuff in it is kind of

0:17:20.560 --> 0:17:23.840
<v Speaker 1>holding together gravitationally. Yeah, but it's a density structure. It's

0:17:23.840 --> 0:17:26.280
<v Speaker 1>not like a matter structure. It's not like the same

0:17:26.359 --> 0:17:29.840
<v Speaker 1>stars are sweeping around and staying in the arm. There

0:17:29.920 --> 0:17:32.680
<v Speaker 1>is a structure there at the density structure, right, and

0:17:32.720 --> 0:17:35.080
<v Speaker 1>that you're saying the density is caused by the gravity

0:17:35.119 --> 0:17:39.199
<v Speaker 1>between them. So let's see, I'm a planet or I'm

0:17:39.240 --> 0:17:42.359
<v Speaker 1>a star around a galaxy. What's going to make me

0:17:42.400 --> 0:17:44.320
<v Speaker 1>want to join one of these waves. Well, it's sort

0:17:44.320 --> 0:17:47.040
<v Speaker 1>of sweeping through the galaxy and it creates regions with

0:17:47.200 --> 0:17:49.760
<v Speaker 1>higher gravity and regions with lesser gravity, and so some

0:17:49.800 --> 0:17:52.720
<v Speaker 1>stars are like getting pulled towards these things, and some

0:17:52.720 --> 0:17:55.959
<v Speaker 1>stars are getting left behind right, And so that's how

0:17:56.000 --> 0:17:59.920
<v Speaker 1>a density wave propagates. Right, it creates regions of great

0:18:00.160 --> 0:18:04.000
<v Speaker 1>and lesser force, which tends to apply differential forces on

0:18:04.040 --> 0:18:07.719
<v Speaker 1>the stars. Right. But unlike a wave and water, you

0:18:07.720 --> 0:18:12.240
<v Speaker 1>have forces that pull and push, right, like something behind

0:18:12.280 --> 0:18:14.359
<v Speaker 1>you pushes you forward, but then some in front of

0:18:14.400 --> 0:18:16.320
<v Speaker 1>you pushes you back, and that's kind of how the

0:18:16.400 --> 0:18:19.639
<v Speaker 1>wave occurs. But in gravity, gravity only attracts. So what

0:18:20.040 --> 0:18:22.679
<v Speaker 1>moves the wave forward? Well, what's moving the wave forward,

0:18:22.960 --> 0:18:25.760
<v Speaker 1>Like at the forefront of the wave, it's density, So

0:18:25.800 --> 0:18:29.560
<v Speaker 1>it's pulling those stars towards it. Right, So the density

0:18:29.600 --> 0:18:32.399
<v Speaker 1>of the arm creates a denser region in front of it.

0:18:32.640 --> 0:18:34.720
<v Speaker 1>Oh I see, So the wave in front of it

0:18:34.760 --> 0:18:38.359
<v Speaker 1>eats up more stars, which moves the center of gravity

0:18:38.440 --> 0:18:42.280
<v Speaker 1>of the arm forward, which then leaves behind the stars

0:18:42.320 --> 0:18:46.240
<v Speaker 1>behind it exactly. And so that's how a density wave propagates.

0:18:46.320 --> 0:18:48.560
<v Speaker 1>And what's really interesting to me is that you know,

0:18:48.600 --> 0:18:51.000
<v Speaker 1>the velocity of the arms is not the same as

0:18:51.000 --> 0:18:53.880
<v Speaker 1>the velocity of the stars. That means where your star

0:18:54.080 --> 0:18:57.040
<v Speaker 1>is in the galaxy determines whether these density waves are

0:18:57.080 --> 0:19:00.960
<v Speaker 1>passing you or whether you're passing them, like for example,

0:19:01.040 --> 0:19:03.359
<v Speaker 1>our sun moves around the center of the galaxy at

0:19:03.359 --> 0:19:05.760
<v Speaker 1>a certain speed, which is basically determined by where it

0:19:06.000 --> 0:19:08.719
<v Speaker 1>is a distance from the center, And so it's actually

0:19:08.720 --> 0:19:12.160
<v Speaker 1>moving around the galaxy about twice as fast as the arms.

0:19:12.200 --> 0:19:14.960
<v Speaker 1>So we are catching up to arms and passing them by.

0:19:15.119 --> 0:19:17.399
<v Speaker 1>But if we were further out, then the density waves

0:19:17.400 --> 0:19:20.000
<v Speaker 1>would be passing us by, and so that's where arms

0:19:20.040 --> 0:19:23.800
<v Speaker 1>come from. Now. Matt's question was, why is it weird

0:19:23.920 --> 0:19:26.720
<v Speaker 1>that this one galaxy that we saw has three arms?

0:19:26.760 --> 0:19:28.800
<v Speaker 1>Why is it weird to have an odd number of arms?

0:19:28.840 --> 0:19:31.680
<v Speaker 1>So they make this comment on the page describing this galaxy.

0:19:31.800 --> 0:19:35.080
<v Speaker 1>So I chatted with a couple of experts about galaxy formation,

0:19:35.240 --> 0:19:37.439
<v Speaker 1>and they quibbled a little bit with this claim that

0:19:37.480 --> 0:19:40.040
<v Speaker 1>it is unusual. First of all, they say, it's not

0:19:40.080 --> 0:19:43.119
<v Speaker 1>even really easy to define, like how many arms a

0:19:43.160 --> 0:19:47.120
<v Speaker 1>galaxy has, you know, because it's basically just visual inspection.

0:19:47.160 --> 0:19:49.720
<v Speaker 1>You're just sort of like looking at it and seeing sorrels.

0:19:50.280 --> 0:19:52.959
<v Speaker 1>But you know, galaxies have more complex structure than just

0:19:53.000 --> 0:19:55.240
<v Speaker 1>like here's an arm. There's an arm. Like if you

0:19:55.240 --> 0:19:58.080
<v Speaker 1>look at the Milky Way our galaxy, it has sort

0:19:58.119 --> 0:20:01.200
<v Speaker 1>of two major arms, but lots of like little spurs

0:20:01.359 --> 0:20:05.119
<v Speaker 1>off of it. For example, we live in the Orion spur,

0:20:05.440 --> 0:20:09.960
<v Speaker 1>which is like a little offshoot from the major Sagittarius arm.

0:20:10.480 --> 0:20:13.359
<v Speaker 1>So is that really another arm or not. It's not

0:20:13.440 --> 0:20:15.960
<v Speaker 1>like a well defined way to count these arms. It's

0:20:15.960 --> 0:20:18.520
<v Speaker 1>just sort of like by looking at it, M I

0:20:18.600 --> 0:20:21.920
<v Speaker 1>see so's it's it's hard to define what makes an arm.

0:20:21.960 --> 0:20:25.280
<v Speaker 1>It's hard to define what makes an arm exactly. And

0:20:25.359 --> 0:20:28.080
<v Speaker 1>so you look at this particular galaxy and you're like, yeah,

0:20:28.080 --> 0:20:29.840
<v Speaker 1>I could call that three or I could call that

0:20:30.000 --> 0:20:33.320
<v Speaker 1>four maybe. And so the short answer is that I

0:20:33.359 --> 0:20:36.879
<v Speaker 1>don't think there's broad agreement on how to define arms

0:20:37.200 --> 0:20:41.320
<v Speaker 1>or how many arms it makes sense for galaxies to have. M.

0:20:41.800 --> 0:20:43.640
<v Speaker 1>I guess my question would be, if you look at

0:20:43.680 --> 0:20:46.280
<v Speaker 1>all the galaxies that we can see out they're in space,

0:20:47.280 --> 0:20:49.560
<v Speaker 1>what is more common? Is it more common to have

0:20:49.720 --> 0:20:52.920
<v Speaker 1>an even ish number of arms or an odd ish

0:20:53.040 --> 0:20:55.640
<v Speaker 1>number of arms. Yeah, it's a great question, and it's

0:20:55.640 --> 0:20:58.840
<v Speaker 1>a hard question to answer without like a systematic way

0:20:58.880 --> 0:21:01.360
<v Speaker 1>to analyze these things. Basically, a human has to look

0:21:01.400 --> 0:21:03.520
<v Speaker 1>at it and say, I think it has three, But

0:21:03.640 --> 0:21:05.960
<v Speaker 1>another human might look at the same galaxy and say, no,

0:21:06.040 --> 0:21:08.560
<v Speaker 1>I think this one has four. So to get like

0:21:08.840 --> 0:21:12.400
<v Speaker 1>enough statistics to do some analysis of that, you need

0:21:12.520 --> 0:21:15.800
<v Speaker 1>some like really rigorous way to analyze these things. And

0:21:15.840 --> 0:21:18.119
<v Speaker 1>people have done like for any analysis or the distribution

0:21:18.200 --> 0:21:21.199
<v Speaker 1>of density waves through galaxies, But that's really just a

0:21:21.200 --> 0:21:23.920
<v Speaker 1>way of counting like the strength of these things. Again,

0:21:23.960 --> 0:21:26.119
<v Speaker 1>you have the problem of deciding when to call it

0:21:26.200 --> 0:21:29.520
<v Speaker 1>another arm. So right now is really just mostly anecdotal.

0:21:29.800 --> 0:21:32.000
<v Speaker 1>People have seen a bunch of galaxies and they haven't

0:21:32.000 --> 0:21:34.560
<v Speaker 1>seen ones that look like this to them, And there

0:21:34.600 --> 0:21:36.159
<v Speaker 1>are ways to explain it. Like if you look at

0:21:36.160 --> 0:21:37.879
<v Speaker 1>a galaxy like this and you say, how did this

0:21:37.960 --> 0:21:41.720
<v Speaker 1>galaxy get this way? Well, one possible explanation is that

0:21:41.800 --> 0:21:45.280
<v Speaker 1>it recently had a strong gravitational interaction with another galaxy

0:21:45.440 --> 0:21:47.600
<v Speaker 1>that sort of messed it up. Because this one also

0:21:47.600 --> 0:21:50.800
<v Speaker 1>seems sort of asymmetric, right It's got like one long

0:21:50.960 --> 0:21:52.879
<v Speaker 1>arm on one side and two shorter arms on the

0:21:52.920 --> 0:21:55.159
<v Speaker 1>other side. So it may just be that like a

0:21:55.200 --> 0:21:58.000
<v Speaker 1>passing galaxy sort of pulled on it in a way

0:21:58.000 --> 0:22:01.840
<v Speaker 1>it separated those density waves. M But I mean, I

0:22:01.880 --> 0:22:05.160
<v Speaker 1>guess is it easy to pull up pictures of galaxies

0:22:05.200 --> 0:22:07.800
<v Speaker 1>that look like they have three arms? Is it maybe

0:22:07.840 --> 0:22:10.919
<v Speaker 1>harder or easier or the same as pulling up pictures

0:22:10.920 --> 0:22:13.520
<v Speaker 1>that looked like they have four arms or two. I

0:22:13.560 --> 0:22:16.280
<v Speaker 1>think it's probably true that most of the galaxies you

0:22:16.400 --> 0:22:18.720
<v Speaker 1>look at, if you've just counted them, you would probably

0:22:18.760 --> 0:22:20.560
<v Speaker 1>get an even number of arms. A lot of them

0:22:20.640 --> 0:22:22.639
<v Speaker 1>just look like they have two, though they're sort of

0:22:22.680 --> 0:22:25.240
<v Speaker 1>like tightly wrapped around. But look at the Milky Way,

0:22:25.240 --> 0:22:27.600
<v Speaker 1>for example, it's not easy to say, like how many

0:22:27.680 --> 0:22:30.520
<v Speaker 1>are there? Like I count one, two big ones and

0:22:30.600 --> 0:22:33.840
<v Speaker 1>at least two maybe four little ones. Although we don't

0:22:33.840 --> 0:22:35.440
<v Speaker 1>really have a picture of the Milky Way, do we.

0:22:35.880 --> 0:22:38.399
<v Speaker 1>We certainly don't have an actual image of the Milky

0:22:38.400 --> 0:22:41.960
<v Speaker 1>Way from the outside, though we can reconstruct the density

0:22:42.000 --> 0:22:44.240
<v Speaker 1>of stars in the Milky Way using a lot of

0:22:44.240 --> 0:22:47.920
<v Speaker 1>our observations. Right, well, could there be maybe some effects

0:22:48.000 --> 0:22:50.480
<v Speaker 1>we are talking about waves right around sort of a

0:22:50.560 --> 0:22:54.160
<v Speaker 1>fixed medium. Is it possible that, you know, given the

0:22:54.160 --> 0:22:57.800
<v Speaker 1>typical size of a galaxy with the typical number of stars,

0:22:57.840 --> 0:23:02.120
<v Speaker 1>maybe like a standing way of four arms is more

0:23:02.200 --> 0:23:04.800
<v Speaker 1>likely than a standing wave of three arms, you know,

0:23:05.000 --> 0:23:08.800
<v Speaker 1>like waves around the spiral of the galaxy. I read

0:23:08.840 --> 0:23:11.879
<v Speaker 1>some papers about these things, and there's are some arguments

0:23:12.000 --> 0:23:15.200
<v Speaker 1>for why you might get two or four if these

0:23:15.240 --> 0:23:18.199
<v Speaker 1>things really do come from like density perturbations in the

0:23:18.200 --> 0:23:20.399
<v Speaker 1>center of the galaxy, because you would expect that to

0:23:20.440 --> 0:23:24.119
<v Speaker 1>be somewhat symmetric, right, that it would cause similar effects

0:23:24.119 --> 0:23:26.600
<v Speaker 1>in one direction and in the other. And so it

0:23:26.640 --> 0:23:28.840
<v Speaker 1>makes some sort of sense for this thing that collapse

0:23:28.880 --> 0:23:31.800
<v Speaker 1>into a bar that then generates two arms, and that

0:23:31.880 --> 0:23:35.040
<v Speaker 1>those might split, but that splitting would always give you

0:23:35.080 --> 0:23:38.760
<v Speaker 1>an even number. So there are some papers suggesting that

0:23:38.800 --> 0:23:41.439
<v Speaker 1>you would expect, on average to get an even number

0:23:41.440 --> 0:23:43.800
<v Speaker 1>of arms, and I think that makes some sense, but

0:23:43.880 --> 0:23:47.200
<v Speaker 1>it's not very well established. Well, so then the picture

0:23:47.240 --> 0:23:49.119
<v Speaker 1>that Matt saw, he saw I did an article that

0:23:49.160 --> 0:23:52.000
<v Speaker 1>said that NASA think is weird to have an odd

0:23:52.080 --> 0:23:55.119
<v Speaker 1>number of arms? What was NASA saying there? So the

0:23:55.200 --> 0:23:58.000
<v Speaker 1>quote the article says, while most disc galaxies have an

0:23:58.040 --> 0:24:01.440
<v Speaker 1>even number of spiral arms, this one has three. But

0:24:01.480 --> 0:24:03.680
<v Speaker 1>you know, the astronomers I talked too, quibbled with that

0:24:03.800 --> 0:24:05.639
<v Speaker 1>a little bit. They didn't think it was so weird.

0:24:05.920 --> 0:24:09.440
<v Speaker 1>They've seen galaxies with three arms before. M I guess

0:24:09.480 --> 0:24:11.679
<v Speaker 1>we'll have to ask NASA. I mean, what do they know.

0:24:12.560 --> 0:24:14.600
<v Speaker 1>Let's have them on the podcast. All right, Well, I

0:24:14.640 --> 0:24:17.400
<v Speaker 1>think that answers Matt's question, which is like, maybe it's

0:24:17.600 --> 0:24:20.040
<v Speaker 1>maybe it's not that weird, right, It seems like some

0:24:20.160 --> 0:24:22.800
<v Speaker 1>astronomers don't think it's as weird to have three arms.

0:24:23.119 --> 0:24:25.320
<v Speaker 1>It seems like it's kind of a fuzzy thing. Anyways,

0:24:25.520 --> 0:24:28.000
<v Speaker 1>it is. But what is weird is that arms exist

0:24:28.119 --> 0:24:31.359
<v Speaker 1>at all. It's really fascinating in the dynamics of galaxies.

0:24:31.760 --> 0:24:34.480
<v Speaker 1>They have these things slashing and swirling around, and it

0:24:34.560 --> 0:24:38.399
<v Speaker 1>just reminds you that galaxies are dynamical objects. They're not

0:24:38.520 --> 0:24:41.120
<v Speaker 1>fixed things that have been formed millions of years ago

0:24:41.200 --> 0:24:45.080
<v Speaker 1>and unchanged. Right, they are swirling, they're crashing into each other,

0:24:45.400 --> 0:24:49.800
<v Speaker 1>they're constantly changing, just on these vast, vast time scales

0:24:49.840 --> 0:24:52.199
<v Speaker 1>that we can hardly even imagine. Yeah, and they're not

0:24:52.240 --> 0:24:54.960
<v Speaker 1>just dynamic, they're like wavy, right, They're rippling. That's what

0:24:55.000 --> 0:24:57.919
<v Speaker 1>these arms are. They're ripples in their structure. All right, Well,

0:24:58.000 --> 0:25:00.800
<v Speaker 1>let's get into some of our other questions. One is

0:25:00.840 --> 0:25:03.359
<v Speaker 1>about the color of the universe and the other is

0:25:03.400 --> 0:25:07.160
<v Speaker 1>about the fate of the universe. So let's get into those.

0:25:07.200 --> 0:25:21.760
<v Speaker 1>But first let's take a quick break. All right. We're

0:25:21.760 --> 0:25:26.160
<v Speaker 1>answering listener questions here about everything is usual, the whole

0:25:26.160 --> 0:25:29.879
<v Speaker 1>she bang, the whole universe. And our second question comes

0:25:29.920 --> 0:25:33.120
<v Speaker 1>from Genie, Hi, Daniel and Hagee. The question I would

0:25:33.119 --> 0:25:35.639
<v Speaker 1>really like to ask is did the universe have a

0:25:35.680 --> 0:25:38.679
<v Speaker 1>color after the Big Bang? If there was no color,

0:25:39.200 --> 0:25:41.600
<v Speaker 1>when was there first a color? And what was it?

0:25:42.119 --> 0:25:45.720
<v Speaker 1>Thank you have all the questions we've gotten, this is

0:25:45.720 --> 0:25:48.000
<v Speaker 1>the one that really threw me for a loop, Like, Wow,

0:25:48.040 --> 0:25:50.920
<v Speaker 1>a question I've never even thought of before, never heard

0:25:50.920 --> 0:25:54.080
<v Speaker 1>of before. What a super fun question. Yeah, it's a

0:25:54.160 --> 0:25:57.240
<v Speaker 1>very colorful question. Jennie asked, did the universe have a

0:25:57.359 --> 0:26:00.320
<v Speaker 1>color after the Big Bang? So I guess a big

0:26:00.359 --> 0:26:03.800
<v Speaker 1>bang happened, and I guess her maybe her question is like,

0:26:03.840 --> 0:26:06.879
<v Speaker 1>if there was a human present there, what would it

0:26:06.920 --> 0:26:10.800
<v Speaker 1>look like? Would it look red, purple, green, polka? Or

0:26:10.800 --> 0:26:13.320
<v Speaker 1>would it just fry your eyes? Yeah? It really is

0:26:13.320 --> 0:26:16.080
<v Speaker 1>one question what would you see if you were there? Right?

0:26:16.280 --> 0:26:18.840
<v Speaker 1>Really love this question and I think it's really fun

0:26:18.880 --> 0:26:21.720
<v Speaker 1>because it makes us think about like what is color? Anyway? Yeah,

0:26:21.840 --> 0:26:24.600
<v Speaker 1>let's dig into that. What is color? How would you

0:26:24.640 --> 0:26:27.080
<v Speaker 1>define it? I know it's related to the wavelength of

0:26:27.119 --> 0:26:29.920
<v Speaker 1>the light. It is related to the wavelength of light,

0:26:30.240 --> 0:26:33.600
<v Speaker 1>But I think it's important to distinguish, right, Like, photons

0:26:33.720 --> 0:26:36.240
<v Speaker 1>have a wavelength, which means like how long it takes

0:26:36.280 --> 0:26:38.200
<v Speaker 1>for them to go up and down. It's related to

0:26:38.200 --> 0:26:40.919
<v Speaker 1>their frequency, right, how many times they wiggle per second.

0:26:41.200 --> 0:26:44.560
<v Speaker 1>But the color is not a property of the photon,

0:26:44.760 --> 0:26:48.560
<v Speaker 1>like photons themselves don't have color. Color is something inside

0:26:48.560 --> 0:26:51.960
<v Speaker 1>your head. It's like how your brain responds to a

0:26:52.080 --> 0:26:56.040
<v Speaker 1>signal of a photon of a specific color, So it's

0:26:56.080 --> 0:26:58.959
<v Speaker 1>not part of the photon itself. It's like the taste

0:26:58.960 --> 0:27:01.840
<v Speaker 1>of salt itself. Doesn't have a taste your tongue as

0:27:01.880 --> 0:27:05.040
<v Speaker 1>a response to sensing salt. Right, I guess you're sort

0:27:05.040 --> 0:27:07.320
<v Speaker 1>of quivaling about the definition of things. But I mean

0:27:07.440 --> 0:27:10.600
<v Speaker 1>light does have different wavelengths, right, it does. But there

0:27:10.600 --> 0:27:13.280
<v Speaker 1>are lots of wavelengths of light that we can't see

0:27:13.400 --> 0:27:16.440
<v Speaker 1>and our brain doesn't respond to. So photons above the

0:27:16.520 --> 0:27:20.640
<v Speaker 1>visible spectrum like have no color to them. Early, they

0:27:20.680 --> 0:27:24.480
<v Speaker 1>have no color. So far, we could panically start naming

0:27:24.480 --> 0:27:29.320
<v Speaker 1>other colors, right, Yeah, absolutely, you could even imagine creating

0:27:29.440 --> 0:27:33.040
<v Speaker 1>a new internal response that's a different color than anybody

0:27:33.080 --> 0:27:35.840
<v Speaker 1>has ever imagined before. Right, If colors are really just

0:27:36.000 --> 0:27:39.000
<v Speaker 1>part of your mind, If there are a response to

0:27:39.600 --> 0:27:42.680
<v Speaker 1>signals from your optic nerve that in principle there's no

0:27:42.760 --> 0:27:47.159
<v Speaker 1>limitation on experiencing new colors, not just combinations of existing colors,

0:27:47.160 --> 0:27:50.959
<v Speaker 1>but like brand new colors, and so in principle that's possible,

0:27:51.040 --> 0:27:53.720
<v Speaker 1>and you could assign those to very high frequency light.

0:27:53.760 --> 0:27:57.240
<v Speaker 1>You could imagine like building a technological eyeball that sends

0:27:57.280 --> 0:27:59.960
<v Speaker 1>messages to your brain. Your brain would learn to interpret

0:28:00.080 --> 0:28:02.880
<v Speaker 1>those responses by giving you some new experience that would

0:28:02.880 --> 0:28:05.000
<v Speaker 1>be like a new color. Yeah. I think what you're

0:28:05.040 --> 0:28:06.920
<v Speaker 1>talking about is that you know, light has a certain

0:28:06.960 --> 0:28:09.640
<v Speaker 1>frequency that can come in certain frequencies, and let's say

0:28:09.720 --> 0:28:13.040
<v Speaker 1>like seven gig gigga hurts or something, or like seven

0:28:13.480 --> 0:28:18.040
<v Speaker 1>hurts might be a frequency. And when I see that

0:28:18.119 --> 0:28:20.920
<v Speaker 1>frequency of light, I think the color green, for example,

0:28:22.000 --> 0:28:24.400
<v Speaker 1>And you and I agree that if we see light

0:28:24.440 --> 0:28:26.200
<v Speaker 1>at this frequency, if we're going to call it green.

0:28:26.280 --> 0:28:27.760
<v Speaker 1>But I think what you're saying is like, maybe what

0:28:27.880 --> 0:28:30.199
<v Speaker 1>I experienced this green is different with them what you

0:28:30.280 --> 0:28:33.040
<v Speaker 1>experience is green. That's certainly true. And there's only also

0:28:33.119 --> 0:28:36.199
<v Speaker 1>a narrow band of photon frequencies that we even have

0:28:36.359 --> 0:28:39.400
<v Speaker 1>colors assigned to, and sort of the long history of

0:28:39.400 --> 0:28:42.320
<v Speaker 1>the universe is that it started out really really hot

0:28:42.360 --> 0:28:45.560
<v Speaker 1>and dense, and photons created in the very very beginning

0:28:45.640 --> 0:28:47.960
<v Speaker 1>of the universe after the Big Bang had very very

0:28:48.080 --> 0:28:51.840
<v Speaker 1>high energies, very high frequencies. Then the universe is cooling down,

0:28:51.920 --> 0:28:55.600
<v Speaker 1>and so the photons created get longer and longer, right,

0:28:55.800 --> 0:28:58.480
<v Speaker 1>lower frequencies, and so the universe sort of starts out

0:28:58.520 --> 0:29:02.000
<v Speaker 1>invisible and then passes through the visible spectrum. And so

0:29:02.080 --> 0:29:05.840
<v Speaker 1>like Genie's asking, what color was the universe when it started? Right,

0:29:05.880 --> 0:29:07.880
<v Speaker 1>And the problem is that the energy of the photons

0:29:07.880 --> 0:29:10.120
<v Speaker 1>at the very beginning of the universe don't really have

0:29:10.160 --> 0:29:13.640
<v Speaker 1>a color. They're too high frequency for us to fc right,

0:29:13.680 --> 0:29:16.959
<v Speaker 1>because the energy of a photon is related directly related

0:29:17.000 --> 0:29:20.120
<v Speaker 1>to its frequency, right, Like the higher the energy, the

0:29:20.200 --> 0:29:24.200
<v Speaker 1>higher the exactly, and hot stuff tends to make higher

0:29:24.280 --> 0:29:26.600
<v Speaker 1>energy photons. We've talked about this on the podcast a

0:29:26.600 --> 0:29:30.720
<v Speaker 1>few times. Everything generates photons. Everything that has charged particles

0:29:30.720 --> 0:29:34.040
<v Speaker 1>inside of it generates photons, and it generates photons based

0:29:34.080 --> 0:29:37.240
<v Speaker 1>on its temperature. So the Sun generates photons as some

0:29:37.360 --> 0:29:40.880
<v Speaker 1>temperature because of its thousands of degrees kelvin, the Earth

0:29:40.920 --> 0:29:44.600
<v Speaker 1>glows and generates photons at some temperature because it's much cooler,

0:29:44.640 --> 0:29:47.440
<v Speaker 1>and you generates photons at some wavelength. Your eyes can't

0:29:47.520 --> 0:29:50.520
<v Speaker 1>see the photons generated by yourself or by the Earth.

0:29:50.720 --> 0:29:53.160
<v Speaker 1>They can see the ones from the sun. So some

0:29:53.200 --> 0:29:55.760
<v Speaker 1>of these photons are visible and some of them are invisible.

0:29:55.960 --> 0:29:58.360
<v Speaker 1>But the hot or something is the higher energy the

0:29:58.400 --> 0:30:01.320
<v Speaker 1>photons it generates. Right. So are you're saying maybe at

0:30:01.360 --> 0:30:04.880
<v Speaker 1>the Big Bang everything all the photons that were there

0:30:05.400 --> 0:30:09.080
<v Speaker 1>were super high frequency or low wavelength. What are you

0:30:09.080 --> 0:30:11.840
<v Speaker 1>saying that? Initially at the Big Bank things were so crazy.

0:30:12.360 --> 0:30:15.800
<v Speaker 1>All the photons were super duper high energy. They were

0:30:15.840 --> 0:30:19.280
<v Speaker 1>super high energy, which means very short wavelength, which means

0:30:19.360 --> 0:30:22.800
<v Speaker 1>very high frequency, right, And so these photons were zipping

0:30:22.800 --> 0:30:24.960
<v Speaker 1>around the universe. And if your eyeball was there just

0:30:25.000 --> 0:30:27.120
<v Speaker 1>after this moment, when the universe was like at the

0:30:27.160 --> 0:30:30.040
<v Speaker 1>Plank temperature, then not only would it be cooked instantly,

0:30:30.240 --> 0:30:32.080
<v Speaker 1>but the photons that hit it it wouldn't know how

0:30:32.080 --> 0:30:35.080
<v Speaker 1>to interpret. Your eye wouldn't see them, So the universe

0:30:35.120 --> 0:30:37.680
<v Speaker 1>would just be black, even though it'd be super duper

0:30:37.720 --> 0:30:40.360
<v Speaker 1>hot and filled with photons. Yeah, Like, if your eye

0:30:40.360 --> 0:30:42.760
<v Speaker 1>could somehow survive being in a Big Bang, it wouldn't

0:30:42.800 --> 0:30:45.120
<v Speaker 1>you would see total darkness, right, because all the light

0:30:45.160 --> 0:30:47.000
<v Speaker 1>would be sort of like X rays, they just passed

0:30:47.040 --> 0:30:49.320
<v Speaker 1>through your eyeball. One question is would they interact with

0:30:49.360 --> 0:30:52.320
<v Speaker 1>your eyeball or they passed through like X rays, right.

0:30:52.480 --> 0:30:54.480
<v Speaker 1>X rays do interact with some parts of your body,

0:30:54.520 --> 0:30:57.120
<v Speaker 1>but not others. And as a frequency of photons change,

0:30:57.160 --> 0:30:59.840
<v Speaker 1>there are chances of interacting with you changes. But you're right,

0:30:59.840 --> 0:31:02.160
<v Speaker 1>a lot of these photons might just fly right through you,

0:31:02.400 --> 0:31:05.320
<v Speaker 1>like X rays, which are higher energy photons than our

0:31:05.360 --> 0:31:08.760
<v Speaker 1>eyeballs can see. But then the universe temperature changes. But

0:31:08.840 --> 0:31:12.360
<v Speaker 1>then eventually, after the Big Bang, the universe started cooling down, right,

0:31:12.400 --> 0:31:16.920
<v Speaker 1>and so you started seeing photons with a lower energy, yes, exactly.

0:31:16.960 --> 0:31:19.400
<v Speaker 1>So as the universe cools and it's really dense, plasma

0:31:19.440 --> 0:31:22.000
<v Speaker 1>gets more and more dilute, it cools down, and so

0:31:22.040 --> 0:31:26.160
<v Speaker 1>it starts generating photons with longer wavelengths. So as time

0:31:26.200 --> 0:31:29.680
<v Speaker 1>goes on, the temperature of the universe is dropping and

0:31:29.720 --> 0:31:32.560
<v Speaker 1>the energy those photons is dropping, and so the wavelength

0:31:32.680 --> 0:31:36.440
<v Speaker 1>is increasing. So they're like the general light of the

0:31:36.520 --> 0:31:39.560
<v Speaker 1>universe started off way too high for our eyes, but

0:31:39.640 --> 0:31:42.720
<v Speaker 1>then it gradually as it cools starts to approach the

0:31:42.840 --> 0:31:46.400
<v Speaker 1>visible spectrum. Yeah, and there's a really fascinating moment around

0:31:46.440 --> 0:31:49.280
<v Speaker 1>three hundred and eighty thousand years after the Big Bang

0:31:49.840 --> 0:31:53.800
<v Speaker 1>when the universe cooled so much that atoms could now form.

0:31:54.160 --> 0:31:56.800
<v Speaker 1>So you have protons and electrons whizzing around with so

0:31:56.880 --> 0:31:59.440
<v Speaker 1>much energy that they couldn't be bothered to bond together.

0:31:59.680 --> 0:32:02.520
<v Speaker 1>But after a certain time things cool down those electrons

0:32:02.520 --> 0:32:05.240
<v Speaker 1>that it no longer had enough energy to escape the

0:32:05.280 --> 0:32:08.000
<v Speaker 1>pull of those protons which have a positive charge and

0:32:08.360 --> 0:32:12.280
<v Speaker 1>pull on the electrons, and so you get neutral hydrogen forms.

0:32:12.600 --> 0:32:15.280
<v Speaker 1>And in this moment, the universe goes from being opaque

0:32:15.560 --> 0:32:17.800
<v Speaker 1>like a really hot plasma like the center of the Sun,

0:32:18.120 --> 0:32:21.560
<v Speaker 1>to being transparent, just like clouds of gas in space

0:32:21.800 --> 0:32:24.760
<v Speaker 1>that light could mostly pass through. So all the light

0:32:24.840 --> 0:32:28.280
<v Speaker 1>generated before this moment was just reabsorbed by the hot plasma.

0:32:28.440 --> 0:32:32.000
<v Speaker 1>Light generated after this moment can fly through the universe,

0:32:32.040 --> 0:32:34.760
<v Speaker 1>and like hit your eyeball, and this light is still

0:32:34.840 --> 0:32:37.920
<v Speaker 1>flying through the universe. It's the cosmic microwave background light.

0:32:38.240 --> 0:32:40.640
<v Speaker 1>We can see it with our telescopes. When it was

0:32:40.720 --> 0:32:43.880
<v Speaker 1>generated at that moment in time, the universe was still

0:32:43.880 --> 0:32:46.200
<v Speaker 1>filled with a pretty hot plasma. It was like several

0:32:46.280 --> 0:32:48.840
<v Speaker 1>thousand degrees So that was the moment when the universe

0:32:48.920 --> 0:32:52.520
<v Speaker 1>first became transparent and the light that were created sort

0:32:52.520 --> 0:32:56.160
<v Speaker 1>of becomes persistent. Right, But still that light is too

0:32:56.560 --> 0:32:59.040
<v Speaker 1>high energy for eyeballs to capture. Right, Like when I

0:32:59.040 --> 0:33:01.280
<v Speaker 1>look up at the night sky, I can't see the

0:33:01.320 --> 0:33:04.120
<v Speaker 1>cosmic microwave background with my eyes, can I You cannot

0:33:04.160 --> 0:33:07.800
<v Speaker 1>see the cosmic microwave background with your eyes currently. But

0:33:07.840 --> 0:33:10.880
<v Speaker 1>when it was created, it actually was in the visible

0:33:10.920 --> 0:33:13.920
<v Speaker 1>spectrum because remember that the wavelength depends on the energy,

0:33:13.920 --> 0:33:17.040
<v Speaker 1>on the temperature, and when that light was created, the

0:33:17.160 --> 0:33:20.760
<v Speaker 1>universe was still pretty hot. It was several thousand degrees kelvin,

0:33:21.040 --> 0:33:23.600
<v Speaker 1>which is about the same temperature as the surface of

0:33:23.640 --> 0:33:27.680
<v Speaker 1>the Sun, which produces visible light. So when the CMB

0:33:27.800 --> 0:33:30.600
<v Speaker 1>light was created, it was in the visible spectrum. You

0:33:30.640 --> 0:33:33.040
<v Speaker 1>could have seen it if Jeanie had her eyeballs back

0:33:33.080 --> 0:33:35.720
<v Speaker 1>in the early universe. Back then, she could have seen

0:33:35.800 --> 0:33:38.120
<v Speaker 1>the CMB with her eyeballs. Now, you're right, when you

0:33:38.160 --> 0:33:39.800
<v Speaker 1>look up in the night sky, you don't see it.

0:33:40.080 --> 0:33:43.080
<v Speaker 1>That's because it's no longer at that frequency. It's been

0:33:43.120 --> 0:33:46.600
<v Speaker 1>stretched by the expansion of the universe. Down to much

0:33:46.680 --> 0:33:50.000
<v Speaker 1>much longer wavelengths, right, and that's why you need like

0:33:50.560 --> 0:33:55.040
<v Speaker 1>infrared telescopes, right exactly. But it's too low frequency for

0:33:55.120 --> 0:33:56.840
<v Speaker 1>us to see, right. It started out in the visible

0:33:56.880 --> 0:34:00.360
<v Speaker 1>spectrum and got stretched out below the visible spectrum very

0:34:00.440 --> 0:34:03.920
<v Speaker 1>very long wavelengths infrared, and so that's why we need

0:34:03.960 --> 0:34:06.440
<v Speaker 1>really sensitive telescopes in order to see it, because it's

0:34:06.440 --> 0:34:09.440
<v Speaker 1>now super duper infrared. And people say the temperature of

0:34:09.480 --> 0:34:12.680
<v Speaker 1>the universe is two point seven three degrees kelvin. What

0:34:12.760 --> 0:34:16.520
<v Speaker 1>they're talking about is the temperature a plasma would have

0:34:16.560 --> 0:34:19.920
<v Speaker 1>to be to generate the photons that we see in

0:34:19.960 --> 0:34:23.960
<v Speaker 1>the CMB. The plasma that actually generated those photons much

0:34:24.040 --> 0:34:27.040
<v Speaker 1>much earlier, was much hotter, but then it's light got

0:34:27.160 --> 0:34:30.200
<v Speaker 1>stretched out, so now it looks like a plasma that's

0:34:30.280 --> 0:34:34.280
<v Speaker 1>much cooler generated this light. Right. So that's a cosmic

0:34:34.320 --> 0:34:37.440
<v Speaker 1>microwave background radiation which comes from the moment when the

0:34:37.520 --> 0:34:41.480
<v Speaker 1>universe became transparent and not hazy. But that's I wonder

0:34:41.520 --> 0:34:44.760
<v Speaker 1>if that's really what would fit into her definition of

0:34:45.080 --> 0:34:47.959
<v Speaker 1>the first light, Like, you know that the light still

0:34:47.960 --> 0:34:51.200
<v Speaker 1>existed when the universe was hazy and opaque, right, yeah, exactly,

0:34:51.239 --> 0:34:54.720
<v Speaker 1>So backing up again, the universe started out really really hot,

0:34:54.760 --> 0:34:58.120
<v Speaker 1>and then as it cools, it passes into the visible spectrum.

0:34:58.320 --> 0:35:02.040
<v Speaker 1>That happened before this moment when the universe became transparent,

0:35:02.080 --> 0:35:04.600
<v Speaker 1>but just about the same time. It's like an interesting

0:35:04.640 --> 0:35:08.120
<v Speaker 1>overlap here that the universe became transparent around the same

0:35:08.160 --> 0:35:12.200
<v Speaker 1>time as it became visible. The temperature for hydrogen become

0:35:12.320 --> 0:35:15.000
<v Speaker 1>neutral is about the same as the temperature of the

0:35:15.000 --> 0:35:19.080
<v Speaker 1>surface of the sun where visible light is generated. Right, So,

0:35:19.120 --> 0:35:22.279
<v Speaker 1>then as the universe moved into the visible spectrum, what

0:35:22.400 --> 0:35:24.799
<v Speaker 1>would have been the first color that you would have

0:35:24.800 --> 0:35:27.560
<v Speaker 1>seen if you were there and was able to survive, Like,

0:35:27.680 --> 0:35:30.840
<v Speaker 1>what's the highest frequency color that we can see with

0:35:30.880 --> 0:35:34.480
<v Speaker 1>our eyes? Yeah, it'd be like the most violet violet, right,

0:35:34.480 --> 0:35:37.320
<v Speaker 1>it'd be like super duper purply blue is the highest

0:35:37.360 --> 0:35:40.480
<v Speaker 1>frequency light that we can seem. So then the first

0:35:40.520 --> 0:35:46.480
<v Speaker 1>color was blue, That was right. I don't know if

0:35:46.520 --> 0:35:48.239
<v Speaker 1>purple and blue are the same, but yeah, it was

0:35:48.320 --> 0:35:52.440
<v Speaker 1>definitely very very bluey, very purply blue, ultra violet, he said,

0:35:52.560 --> 0:35:55.640
<v Speaker 1>violet blue. All right, we'll go with purple. The first

0:35:55.640 --> 0:35:59.279
<v Speaker 1>color in the universe was purple, basically, Yeah, I think

0:35:59.320 --> 0:36:01.879
<v Speaker 1>that's true. It was purple. All right, Well, Genie, thank

0:36:01.880 --> 0:36:04.280
<v Speaker 1>you for that question. I hope purple is your favorite

0:36:04.280 --> 0:36:08.400
<v Speaker 1>color as well, because it is apparently the universe first color.

0:36:08.640 --> 0:36:10.400
<v Speaker 1>But you know, if there are aliens out there and

0:36:10.440 --> 0:36:13.839
<v Speaker 1>they have eyeballs and their brains interpret things differently, if

0:36:13.840 --> 0:36:16.120
<v Speaker 1>they brains give them like a red experience for that

0:36:16.160 --> 0:36:19.239
<v Speaker 1>same frequency and a purple experience for very low frequencies,

0:36:19.520 --> 0:36:23.000
<v Speaker 1>then aliens would say a different color was the first color.

0:36:23.200 --> 0:36:25.120
<v Speaker 1>And that's just because again, color is not part of

0:36:25.120 --> 0:36:27.719
<v Speaker 1>the universe, it's part of our brains. So it's a

0:36:27.800 --> 0:36:30.439
<v Speaker 1>very human thing to say that violet was the first

0:36:30.440 --> 0:36:32.760
<v Speaker 1>color in the universe. It was the first human color

0:36:32.800 --> 0:36:35.319
<v Speaker 1>in the universe, I suppose. Well, it's the first name

0:36:35.360 --> 0:36:37.440
<v Speaker 1>that the human would give it. But the frequency was

0:36:37.480 --> 0:36:39.680
<v Speaker 1>still the same, so we would all agree. I mean,

0:36:39.880 --> 0:36:41.640
<v Speaker 1>the experience I have a violet might not be the

0:36:41.640 --> 0:36:44.000
<v Speaker 1>same experience you have a violet, but we can all

0:36:44.000 --> 0:36:48.280
<v Speaker 1>agree that about that frequency. That's true. Yeah, though aliens

0:36:48.360 --> 0:36:50.719
<v Speaker 1>might be able to see much higher frequencies, and they

0:36:50.840 --> 0:36:54.840
<v Speaker 1>might say an even higher frequency was visible before our violet.

0:36:55.520 --> 0:36:58.239
<v Speaker 1>M I see, they might have a different first color,

0:36:58.520 --> 0:37:01.279
<v Speaker 1>assuming they call it color. Maybe they spell over the

0:37:01.360 --> 0:37:05.480
<v Speaker 1>K or something, but they put a U after the second. Oh,

0:37:08.560 --> 0:37:10.879
<v Speaker 1>I think you went too far there, Yeah, who would

0:37:10.920 --> 0:37:13.680
<v Speaker 1>do that? All right, well, I think then answers Jeannie's question.

0:37:13.960 --> 0:37:16.320
<v Speaker 1>Thank you, Jeanie. And so we'll get to our last question.

0:37:16.440 --> 0:37:20.160
<v Speaker 1>This one is about the universe tearing itself apart. So

0:37:20.239 --> 0:37:23.560
<v Speaker 1>let's take that apart. But first let's take another quick break.

0:37:36.120 --> 0:37:38.839
<v Speaker 1>All right, we're answering questions about the universe and our

0:37:38.920 --> 0:37:43.520
<v Speaker 1>last question. It's a bit dramatic, a bit drastic, it

0:37:43.640 --> 0:37:45.760
<v Speaker 1>certainly is, which is why we saved it from last.

0:37:46.040 --> 0:37:48.640
<v Speaker 1>All right, our last question comes from Courtney, and she

0:37:48.680 --> 0:37:52.800
<v Speaker 1>has a question about the universe. Hey, Daniel and Jorge,

0:37:53.000 --> 0:37:55.520
<v Speaker 1>I have a question for y'all. Is our universe tearing

0:37:55.560 --> 0:37:58.400
<v Speaker 1>itself apart? Is physics as we know and measure it

0:37:58.719 --> 0:38:01.400
<v Speaker 1>stable enough to be really light upon? If so, for

0:38:01.520 --> 0:38:04.200
<v Speaker 1>how long? If at the beginning of the universe the

0:38:04.239 --> 0:38:08.280
<v Speaker 1>electro week force broke in one moment, everything was whizzing

0:38:08.360 --> 0:38:12.040
<v Speaker 1>around at the speed of light, then suddenly the next

0:38:12.160 --> 0:38:17.960
<v Speaker 1>some particles experienced mass, fundamentally altering the trajectory of our universe.

0:38:18.320 --> 0:38:20.920
<v Speaker 1>Could we be looking forward to another dramatic change in

0:38:21.000 --> 0:38:24.440
<v Speaker 1>how our physical forces manifest themselves? Could we measure that

0:38:25.760 --> 0:38:29.240
<v Speaker 1>looking forward to hearing back? Thanks? All right, awesome question

0:38:29.280 --> 0:38:31.440
<v Speaker 1>for Corney. I think really what she's asking is does

0:38:31.480 --> 0:38:34.200
<v Speaker 1>she have to do her homework for tomorrow or do

0:38:34.280 --> 0:38:36.640
<v Speaker 1>that errente she needs to do? Or if the universe

0:38:36.719 --> 0:38:40.239
<v Speaker 1>just totally going to flip on itself or maybe she

0:38:40.640 --> 0:38:42.879
<v Speaker 1>could be doing other things today. Yeah. I did get

0:38:42.880 --> 0:38:44.840
<v Speaker 1>the sense that she was trying to make plans and

0:38:44.920 --> 0:38:47.279
<v Speaker 1>she wanted to know how far in the future she

0:38:47.400 --> 0:38:49.759
<v Speaker 1>needed to think, Like, if I buy this house, is

0:38:49.800 --> 0:38:51.520
<v Speaker 1>it going to be for sale in twenty years or

0:38:51.600 --> 0:38:54.520
<v Speaker 1>is the whole universe going to get shredded before that? Yeah?

0:38:54.600 --> 0:38:56.520
<v Speaker 1>Do I still have to pay my mortgage? Or can

0:38:56.600 --> 0:39:00.239
<v Speaker 1>I just buy the biggest mansion I can now because

0:39:00.239 --> 0:39:02.479
<v Speaker 1>the universe is going to end? That's right, real estate

0:39:02.480 --> 0:39:05.120
<v Speaker 1>investment advice from people you shouldn't be listening to about

0:39:05.160 --> 0:39:07.680
<v Speaker 1>real estate. Well, she's going to ask a multipart question.

0:39:07.760 --> 0:39:10.839
<v Speaker 1>She asked whether the universe is tearing itself apart, which

0:39:10.880 --> 0:39:12.959
<v Speaker 1>I guess maybe is related to her second question, which

0:39:13.000 --> 0:39:15.680
<v Speaker 1>is like how stable do we think the universe is? Like?

0:39:15.840 --> 0:39:18.000
<v Speaker 1>Is it going to stay like this? Forever. Can we

0:39:18.320 --> 0:39:21.680
<v Speaker 1>invest in real estate? Or is it possible for the

0:39:21.760 --> 0:39:25.479
<v Speaker 1>universe to suddenly change tomorrow or today or right now

0:39:25.600 --> 0:39:28.160
<v Speaker 1>and make it a whole different universe, And it maybe

0:39:28.160 --> 0:39:31.160
<v Speaker 1>that happened, we would we notice even I really love

0:39:31.239 --> 0:39:32.920
<v Speaker 1>this question because the touch is on one of the

0:39:32.960 --> 0:39:36.000
<v Speaker 1>most interesting ideas in physics that I think is not

0:39:36.239 --> 0:39:40.160
<v Speaker 1>very widely appreciated, And it's actually connected to Genie's question

0:39:40.200 --> 0:39:42.920
<v Speaker 1>about like the temperature of the universe. You know, we

0:39:43.000 --> 0:39:46.080
<v Speaker 1>think about the universe and how it works, but we're

0:39:46.080 --> 0:39:49.759
<v Speaker 1>really just describing the universe in one phase. When I

0:39:49.800 --> 0:39:51.680
<v Speaker 1>say phase, I don't mean like, you know, a toddler

0:39:51.719 --> 0:39:54.120
<v Speaker 1>throwing a tantrum. More like a phase is in the

0:39:54.160 --> 0:39:56.560
<v Speaker 1>state of matter. Like if you're a scientist and you're

0:39:56.560 --> 0:39:59.759
<v Speaker 1>trying to understand water, then you might have one understanding

0:39:59.760 --> 0:40:02.360
<v Speaker 1>of how works when it's a vapor, and another understanding

0:40:02.360 --> 0:40:04.400
<v Speaker 1>of how it works when it's a liquid, and another

0:40:04.480 --> 0:40:06.799
<v Speaker 1>understanding of how it works when it's a solid. Right,

0:40:06.840 --> 0:40:10.800
<v Speaker 1>we notice these phase transitions when water changes its behavior

0:40:10.880 --> 0:40:13.919
<v Speaker 1>pretty dramatically as it heats up or as it cools down,

0:40:14.200 --> 0:40:16.600
<v Speaker 1>and we can have a law that describes each of

0:40:16.600 --> 0:40:19.600
<v Speaker 1>those phases and in principle, if you had like the

0:40:19.719 --> 0:40:22.560
<v Speaker 1>ultimate theory of physics, you could have a single law

0:40:22.600 --> 0:40:24.920
<v Speaker 1>that describes all of them. But typically what we do

0:40:25.000 --> 0:40:27.839
<v Speaker 1>is we have effective laws to describe one phase at

0:40:27.880 --> 0:40:31.960
<v Speaker 1>a time. And so the universe, the whole universe is

0:40:32.000 --> 0:40:34.440
<v Speaker 1>cooling down, as we talked about a minute ago, and

0:40:34.480 --> 0:40:38.080
<v Speaker 1>so we think it's passing through different phases, and so

0:40:38.160 --> 0:40:41.440
<v Speaker 1>our current understanding of physics, a standard model of quarks,

0:40:41.440 --> 0:40:43.799
<v Speaker 1>the photons, the weak force, the Higgs boson, all that

0:40:43.840 --> 0:40:48.239
<v Speaker 1>stuff just describes the current phase of the universe in

0:40:48.280 --> 0:40:51.160
<v Speaker 1>the sense of like having an effective theory that describes

0:40:51.200 --> 0:40:54.680
<v Speaker 1>how things work right now, right because as we kind

0:40:54.680 --> 0:40:57.440
<v Speaker 1>of talked about a minute ago with Genie's question, the

0:40:57.560 --> 0:41:00.760
<v Speaker 1>universe kind of went through a pretty significant a change

0:41:00.960 --> 0:41:05.000
<v Speaker 1>early soon after the Big Bang, Like before this event,

0:41:05.600 --> 0:41:07.880
<v Speaker 1>everything all the matter, what's had so much energy, so

0:41:08.000 --> 0:41:11.640
<v Speaker 1>much velocity, so much going on that like not even

0:41:11.760 --> 0:41:14.880
<v Speaker 1>protons and electrons could hold together or come together and

0:41:14.960 --> 0:41:17.920
<v Speaker 1>stick into atoms and matter things that are just kind

0:41:17.920 --> 0:41:20.120
<v Speaker 1>of like a giant plasma. And then when things cooled,

0:41:20.200 --> 0:41:24.400
<v Speaker 1>when space expanded, things cool suddenly, like things clicked into

0:41:24.560 --> 0:41:26.920
<v Speaker 1>atoms and the stuff we see today, which is I

0:41:27.239 --> 0:41:28.799
<v Speaker 1>think what you're trying to say is similar to like

0:41:28.920 --> 0:41:32.560
<v Speaker 1>what happens to vapor or ice. It's like the molecules

0:41:32.600 --> 0:41:34.440
<v Speaker 1>are flying around, but at some point they lose so

0:41:34.520 --> 0:41:36.600
<v Speaker 1>much energy that some of the other forces in plate

0:41:36.800 --> 0:41:39.680
<v Speaker 1>start to click them together or to bring them together

0:41:39.719 --> 0:41:42.919
<v Speaker 1>as a liquid exactly. And what Cordy is bringing up

0:41:43.040 --> 0:41:46.400
<v Speaker 1>is another kind of phase transition, even deeper phase transition

0:41:46.440 --> 0:41:49.800
<v Speaker 1>than just like how do protons and electrons click together?

0:41:50.320 --> 0:41:53.160
<v Speaker 1>She was talking about the moment when things got mass.

0:41:53.560 --> 0:41:55.800
<v Speaker 1>All right, we've described the nature of the universes. We

0:41:55.880 --> 0:41:58.319
<v Speaker 1>understand it in terms of all these quantum fields that

0:41:58.360 --> 0:42:00.800
<v Speaker 1>are slashing around, and we talk about how the Higgs

0:42:00.800 --> 0:42:04.239
<v Speaker 1>field is there and it's giving mass to particles by

0:42:04.360 --> 0:42:06.880
<v Speaker 1>interacting with them and changing how they moved through the

0:42:07.000 --> 0:42:08.759
<v Speaker 1>universe and all of this stuff. But if you go

0:42:08.800 --> 0:42:10.480
<v Speaker 1>back to one of our podcasts where we talk about

0:42:10.520 --> 0:42:13.319
<v Speaker 1>the very early history of the universe, you know that

0:42:13.360 --> 0:42:16.080
<v Speaker 1>there was a moment before this happened, before the Higgs

0:42:16.080 --> 0:42:18.960
<v Speaker 1>field was giving mass to particles, when we still had

0:42:19.000 --> 0:42:21.680
<v Speaker 1>this description of everything in terms of quantum fields, but

0:42:21.719 --> 0:42:25.320
<v Speaker 1>effectively the universe was very different. Everything was basically mass

0:42:25.480 --> 0:42:28.360
<v Speaker 1>less electrons and quarks and all this stuff. We're flying

0:42:28.360 --> 0:42:30.760
<v Speaker 1>to the universe all at the speed of light before

0:42:30.800 --> 0:42:34.400
<v Speaker 1>the Higgs boson sort of kicked in and gave everything mass.

0:42:34.640 --> 0:42:37.760
<v Speaker 1>So that was another big phase transition in our universe.

0:42:38.280 --> 0:42:41.359
<v Speaker 1>Now that one's pretty fundamental, like the universe went from

0:42:41.400 --> 0:42:45.400
<v Speaker 1>not having mass to having mass. Things having mass, and

0:42:45.440 --> 0:42:49.440
<v Speaker 1>you said, something clicked, but like the laws of physics change,

0:42:49.640 --> 0:42:53.479
<v Speaker 1>or within our laws just some sort of potential change,

0:42:53.600 --> 0:42:56.800
<v Speaker 1>or we reached the threshold where suddenly the laws preferred

0:42:56.840 --> 0:42:59.680
<v Speaker 1>to be this way rather than having no mass, so

0:43:00.120 --> 0:43:02.960
<v Speaker 1>that the laws we have now describe the universe now.

0:43:03.040 --> 0:43:06.400
<v Speaker 1>And also before this transition, so same laws of physics,

0:43:06.560 --> 0:43:09.120
<v Speaker 1>but you have different temperature. And so as the Higgs

0:43:09.160 --> 0:43:12.160
<v Speaker 1>field was cooling down, it got stuck in sort of

0:43:12.160 --> 0:43:14.680
<v Speaker 1>a local minimum, and that's what she referred to as

0:43:14.719 --> 0:43:18.360
<v Speaker 1>electroweak symmetry breaking. It's got stuck in this sort of

0:43:18.400 --> 0:43:21.839
<v Speaker 1>weird spot where it treats w's and z's differently from

0:43:21.840 --> 0:43:24.720
<v Speaker 1>how it treats photons, and it gave those particles mass,

0:43:24.840 --> 0:43:26.920
<v Speaker 1>and it gives mass to the other particles sort of

0:43:26.920 --> 0:43:29.880
<v Speaker 1>because where it got stuck as the universe was cooling,

0:43:30.040 --> 0:43:32.560
<v Speaker 1>So it's the same basic laws of physics, but as

0:43:32.560 --> 0:43:35.480
<v Speaker 1>the universe cools down, the effect of those laws changes,

0:43:35.760 --> 0:43:37.720
<v Speaker 1>and one of the effects is that the Higgs field

0:43:37.719 --> 0:43:40.040
<v Speaker 1>got stuck in this weird spot and that's why these

0:43:40.080 --> 0:43:42.920
<v Speaker 1>particles have mass. And so really, I think her question

0:43:43.040 --> 0:43:46.400
<v Speaker 1>is like, do we expect further similar phase transitions in

0:43:46.440 --> 0:43:49.680
<v Speaker 1>the future or the universe that could fundamentally change what

0:43:49.800 --> 0:43:53.080
<v Speaker 1>we experience. Yeah, I guess she's not asking like can

0:43:53.120 --> 0:43:56.320
<v Speaker 1>the laws change? He's more asking like, is the universe,

0:43:56.360 --> 0:43:58.719
<v Speaker 1>like you said, is the universe stable? Are we like

0:43:58.880 --> 0:44:01.360
<v Speaker 1>in a spot where the basic configuration of the universe

0:44:01.440 --> 0:44:03.160
<v Speaker 1>is going to be the same, or can it change

0:44:03.200 --> 0:44:05.759
<v Speaker 1>like it did once before? Though, you know, it is

0:44:05.800 --> 0:44:09.040
<v Speaker 1>possible that the laws could change, because even though we

0:44:09.080 --> 0:44:12.200
<v Speaker 1>can describe the history of the universe pretty far back

0:44:12.320 --> 0:44:15.240
<v Speaker 1>using our laws and quantum fields, there's a moment beyond

0:44:15.239 --> 0:44:17.799
<v Speaker 1>which we can't right at the very very beginning of

0:44:17.840 --> 0:44:20.080
<v Speaker 1>the universe, just after inflation with things where at the

0:44:20.080 --> 0:44:23.080
<v Speaker 1>plank temperature. We think our laws break down there, and

0:44:23.120 --> 0:44:25.920
<v Speaker 1>before that we need something else, some theory of quantum

0:44:25.960 --> 0:44:29.719
<v Speaker 1>gravity that's deeper. We think that even our laws of

0:44:29.760 --> 0:44:32.280
<v Speaker 1>physics that do a great job of describing the universe

0:44:32.320 --> 0:44:34.799
<v Speaker 1>today and very very far back in time. They are

0:44:34.920 --> 0:44:37.840
<v Speaker 1>just effective laws. They're like understanding water when it's a

0:44:37.840 --> 0:44:40.960
<v Speaker 1>liquid and how it flows, but not deeply understanding the

0:44:40.960 --> 0:44:44.240
<v Speaker 1>true theory of water that would explain all of its phases.

0:44:44.719 --> 0:44:47.160
<v Speaker 1>So there is a sense in which the actual effective

0:44:47.200 --> 0:44:50.520
<v Speaker 1>laws of physics do change over time, though we don't

0:44:50.520 --> 0:44:52.000
<v Speaker 1>know what's going to happen in the future. We think

0:44:52.000 --> 0:44:54.520
<v Speaker 1>the universe is just going to keep cooling and probably

0:44:54.840 --> 0:44:57.920
<v Speaker 1>this current effective set of laws are going to hold fast.

0:44:58.120 --> 0:45:00.600
<v Speaker 1>But even if these laws hold fast, there might be

0:45:00.640 --> 0:45:03.759
<v Speaker 1>phase transition still in our future. Right. We talked on

0:45:03.800 --> 0:45:06.000
<v Speaker 1>the podcast once about how the Higgs field is sort

0:45:06.000 --> 0:45:08.640
<v Speaker 1>of stuck in this one spot, but it's not that stable.

0:45:08.920 --> 0:45:11.080
<v Speaker 1>We don't know if it's going to stay stuck in

0:45:11.080 --> 0:45:14.600
<v Speaker 1>that spot or if it's going to collapse and change

0:45:14.640 --> 0:45:17.200
<v Speaker 1>the masses of everything, and that would be like another

0:45:17.239 --> 0:45:20.840
<v Speaker 1>effective phase transition. So it might be that sometime in

0:45:20.880 --> 0:45:24.200
<v Speaker 1>the future, you know, maybe spurred on by particle collisions,

0:45:24.239 --> 0:45:26.719
<v Speaker 1>that some super collider could spark a change in the

0:45:26.800 --> 0:45:29.719
<v Speaker 1>Higgs field which creates an effective phase transition in the

0:45:29.760 --> 0:45:32.279
<v Speaker 1>basic laws of physics. Yeah, I think we talked about

0:45:32.320 --> 0:45:34.680
<v Speaker 1>this in our book. Frequently ask questions about the universe,

0:45:34.760 --> 0:45:36.920
<v Speaker 1>But you know, is the universe is going to end

0:45:36.960 --> 0:45:38.680
<v Speaker 1>at some point? Or how is the universe going to end?

0:45:38.680 --> 0:45:42.400
<v Speaker 1>And one possibility is for this Higgs field to collapse,

0:45:42.560 --> 0:45:45.120
<v Speaker 1>because it can collapse right like, it's sitting at a

0:45:45.160 --> 0:45:49.680
<v Speaker 1>place where it can still fall down in terms of energy. Yeah,

0:45:49.719 --> 0:45:51.920
<v Speaker 1>the reason the Higgs field does what it does is

0:45:51.920 --> 0:45:54.600
<v Speaker 1>because it has a lot of energy still stored in it.

0:45:54.600 --> 0:45:56.759
<v Speaker 1>It's like the whole universe is cooling down, but the

0:45:56.840 --> 0:45:59.400
<v Speaker 1>Higgs field got stuck and sort of staying hot. But

0:45:59.400 --> 0:46:01.560
<v Speaker 1>it's kind of like ball that's stuck on a shelf

0:46:01.600 --> 0:46:04.000
<v Speaker 1>and it could roll off that shelf and fall further

0:46:04.160 --> 0:46:07.640
<v Speaker 1>down in temperature. We don't really understand very well how

0:46:07.800 --> 0:46:11.040
<v Speaker 1>stable the spot it's stuck in is and what it

0:46:11.040 --> 0:46:13.000
<v Speaker 1>would take to sort of nudge it out of that,

0:46:13.280 --> 0:46:16.320
<v Speaker 1>and so there's a possibility that it could collapse even further,

0:46:16.719 --> 0:46:18.400
<v Speaker 1>and that would mean a change in the masses of

0:46:18.400 --> 0:46:21.680
<v Speaker 1>all the particles, which would mean like chemistry out the window,

0:46:21.960 --> 0:46:24.760
<v Speaker 1>need totally new chemistry, and you know, everything that relies

0:46:24.800 --> 0:46:28.480
<v Speaker 1>on chemistry, like life and podcasts also out the window,

0:46:28.840 --> 0:46:31.480
<v Speaker 1>and I guess buying a house also along with that.

0:46:32.040 --> 0:46:34.520
<v Speaker 1>But I think you describe it as sort of like

0:46:34.520 --> 0:46:37.440
<v Speaker 1>a spark and a spark propagating. I know we've covered

0:46:37.440 --> 0:46:39.919
<v Speaker 1>this in the book, but it's almost like if something

0:46:40.000 --> 0:46:42.480
<v Speaker 1>happens and does cause a Higgs boson to kind of

0:46:42.520 --> 0:46:45.000
<v Speaker 1>fall over or give up its energy in one spot,

0:46:45.280 --> 0:46:48.239
<v Speaker 1>it would basically cause the entire universe to do the same,

0:46:48.280 --> 0:46:51.640
<v Speaker 1>Like it would spread out like a wave. Right, if

0:46:51.640 --> 0:46:54.120
<v Speaker 1>it happened anywhere, it would spread out like a wave

0:46:54.200 --> 0:46:56.600
<v Speaker 1>propagating at the speed of light. So it may have

0:46:56.719 --> 0:47:00.719
<v Speaker 1>already happened somewhere else in the universe, and that wavefront

0:47:00.760 --> 0:47:04.200
<v Speaker 1>of phase transitions is heading for us or maybe not,

0:47:04.280 --> 0:47:06.879
<v Speaker 1>and maybe it'll be stable forever, right, And you're saying

0:47:06.880 --> 0:47:09.160
<v Speaker 1>that one thing that could trigger it maybe is building

0:47:09.200 --> 0:47:13.600
<v Speaker 1>a large particle collider, maybe under Geneva or something, yeah,

0:47:13.719 --> 0:47:16.160
<v Speaker 1>or around the surface of the Moon or around the

0:47:16.239 --> 0:47:18.080
<v Speaker 1>edge of the galaxy. It sounds like we need to

0:47:18.120 --> 0:47:20.719
<v Speaker 1>shut those things down right away. It sounds like we

0:47:20.760 --> 0:47:25.920
<v Speaker 1>need to build one and find out. That sounds like

0:47:26.000 --> 0:47:28.400
<v Speaker 1>exactly the opposite thing. You want to find out if

0:47:28.400 --> 0:47:30.880
<v Speaker 1>you can destroy the universe. I don't know. I'm pro curiosity.

0:47:30.880 --> 0:47:32.640
<v Speaker 1>I don't know how you feel. I am pro not

0:47:32.760 --> 0:47:35.719
<v Speaker 1>destroying the universe, because once you find out that you

0:47:35.719 --> 0:47:39.960
<v Speaker 1>can destroy the universe, you've destroyed the universe, Daniel, but

0:47:40.080 --> 0:47:43.919
<v Speaker 1>you've learned something along the way. No, because you won't

0:47:43.960 --> 0:47:46.520
<v Speaker 1>be here. Look what I'm saying, is nobody ever regretted

0:47:46.560 --> 0:47:50.560
<v Speaker 1>destroying the universe. Well, I think the answer here for

0:47:50.680 --> 0:47:53.879
<v Speaker 1>Corney is that go ahead and buy that house you're

0:47:53.960 --> 0:47:55.880
<v Speaker 1>thinking of buying. And maybe you should write to Daniel

0:47:55.880 --> 0:48:00.840
<v Speaker 1>tell him not to destroy the universe. Send your questions,

0:48:00.840 --> 0:48:04.680
<v Speaker 1>your ideas, your requests to not destroy the universe. Two

0:48:04.760 --> 0:48:07.680
<v Speaker 1>questions at Daniel and Jorge dot com. All right, thank

0:48:07.719 --> 0:48:10.279
<v Speaker 1>you everyone for sending us their question. A lot of

0:48:10.280 --> 0:48:12.560
<v Speaker 1>interesting things we've learned about here. I think we can

0:48:12.600 --> 0:48:14.640
<v Speaker 1>give ourselves a pat on the back, Daniel, maybe with

0:48:14.680 --> 0:48:17.000
<v Speaker 1>a third army out at the top of your head. Yeah, exactly,

0:48:17.040 --> 0:48:18.960
<v Speaker 1>it's busy scratching my head right now. You can give

0:48:19.000 --> 0:48:21.320
<v Speaker 1>yourself three handshakes. Triple high five. It would be the

0:48:21.400 --> 0:48:24.840
<v Speaker 1>highest of fives. M it would be a triple five. Yeah,

0:48:25.200 --> 0:48:28.320
<v Speaker 1>it would be a fifteen. All right, Well, thanks for

0:48:28.400 --> 0:48:31.160
<v Speaker 1>joining us. We hope you enjoyed that. See you next time.

0:48:39.000 --> 0:48:41.800
<v Speaker 1>Thanks for listening, and remember that Daniel and Jorge Explain

0:48:41.880 --> 0:48:45.759
<v Speaker 1>the Universe is a production of iHeartRadio. For more podcast

0:48:45.920 --> 0:48:49.799
<v Speaker 1>from my heart Radio, visit the iHeartRadio app, Apple Podcasts,

0:48:49.920 --> 0:48:52.320
<v Speaker 1>or wherever you listen to your favorite shows.