WEBVTT - Special 200th episode!

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<v Speaker 1>Yeah, orgey, do you know what today is? Is it

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<v Speaker 1>a special day today? Oh my god, I can't believe

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<v Speaker 1>your forgot? Is it your birthday? Try again? Is it

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<v Speaker 1>the anniversary of the Higgs Boson closer? It's actually our anniversary.

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<v Speaker 1>Today is our two hundredth episode of Daniel and Jorge

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<v Speaker 1>Explain the Universe. Two hundred episodes. Oh my gosh, it's

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<v Speaker 1>a lot of physics and a lot of banana jots.

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<v Speaker 1>It's a whole universe of banana physics. Hi am orhand

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<v Speaker 1>my cartoonists and the creator of PhD comment. Hi. I'm Daniel.

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<v Speaker 1>I'm a particle physicist, and I know at least two

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<v Speaker 1>hundred things about physics, and I know at least two

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<v Speaker 1>hundred bad jokes about physics. I've made ten to the

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<v Speaker 1>two hundred bad jokes about physics, but our editor has

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<v Speaker 1>removed most. And Welcome to our podcast, Daniel and Jorge

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<v Speaker 1>Explained the Universe, a production of I Heart Radio, a

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<v Speaker 1>project we started to explain to you all the amazing

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<v Speaker 1>and crazy things out there in the universe, all the

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<v Speaker 1>things we do know, the facts we've learned about the universe,

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<v Speaker 1>the secret truth that we've revealed, and also the incredible questions,

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<v Speaker 1>the things that science still has to figure out, the

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<v Speaker 1>questions that scientists are asking, and the questions that you

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<v Speaker 1>are asking, the deep mysteries of the universe around us.

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<v Speaker 1>Because it turns out that there are more than two

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<v Speaker 1>hundred questions you can ask about the universe and more

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<v Speaker 1>than two hundred amazing facts to learn and to discover

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<v Speaker 1>about how this crazy cosmos works. At least that's what

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<v Speaker 1>we've discovered in doing this podcast. We had no idea

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<v Speaker 1>how long we could keep going on. Yeah, today is

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<v Speaker 1>a very special episode. It's our two hundred episode. What

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<v Speaker 1>does that make it anial? Is it like a birthday,

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<v Speaker 1>a broadcast day at pot day? I don't know, but

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<v Speaker 1>you know, if you look up anniversaries, like you know,

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<v Speaker 1>the fifth anniversaries paper, and the tenth anniversary is silver

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<v Speaker 1>or whatever, the fiftieth anniversary is diamond. There is no

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<v Speaker 1>culturally acceptable gift for two hundredth anniversary because he's ever

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<v Speaker 1>lasted that long. I think they give you a Nobel

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<v Speaker 1>price if you somehow managed to celebrate two hundredth anniversary,

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<v Speaker 1>Maybe you should be the fossil anniversary something, because you've

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<v Speaker 1>become fossilized. But congratulations Daniel, two hundred episodes. Did you

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<v Speaker 1>ever think we would get to two hundred episodes? No?

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<v Speaker 1>I thought you get sick of talking to me about

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<v Speaker 1>physics after about ten or twenty. No, congratulations to you. Also,

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<v Speaker 1>it's been a really fun ride. And thank you to

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<v Speaker 1>all of our listeners who have listened to us talking

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<v Speaker 1>about science and joking about bananas and shared your goofy

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<v Speaker 1>curiosity with us. That's really what's powered us forward. So

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<v Speaker 1>thanks for listening, and thanks for all the feedback and support. Well,

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<v Speaker 1>I have definitely not gotten tired of listening to amazing

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<v Speaker 1>physics and to listen to you explain rated. Um, I

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<v Speaker 1>feel like I could go another two hundred episodes. Let's

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<v Speaker 1>do it. Well. In honor of our two hundredth episode,

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<v Speaker 1>I put out a tweet asking folks what we should

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<v Speaker 1>do to celebrate our two hundredth episode, and as usual,

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<v Speaker 1>I put out some silly suggestions and we did a

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<v Speaker 1>little Twitter poll. Yeah, and so Daniel asked what should

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<v Speaker 1>we do for a two hundred episode? And the options

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<v Speaker 1>were one, eat two hundred bananas, to answer two hundred questions,

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<v Speaker 1>three to two hundred different accents, and number four just

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<v Speaker 1>shut up. And explain. That's right, and clearly I was

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<v Speaker 1>going to do the explaining, but I was hoping that

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<v Speaker 1>you would do the bananas in the accents seems a

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<v Speaker 1>little lopsided. Daniel, Well, you're the creative one, right. How

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<v Speaker 1>can I eat bananas and accents at the same time?

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<v Speaker 1>Those count as different accents, you know, like Scottish or

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<v Speaker 1>Scottish with the banana in your mouth sound very different.

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<v Speaker 1>It was a close pole. It was a close poll, yes,

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<v Speaker 1>exactly what it was. It dramatic like as you saw

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<v Speaker 1>the numbers come in. Um, well, bananas was racing to

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<v Speaker 1>the lead in the beginning, but eventually people voted for

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<v Speaker 1>Answer two hundred questions got about thirty five Eat two

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<v Speaker 1>hundred bananas in second place, and you know in last

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<v Speaker 1>place was due two hundred accidents, which I was sort

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<v Speaker 1>of hoping for. I think we have to trust the

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<v Speaker 1>wisdom of the crowd here and not offend two hundred

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<v Speaker 1>countries we can. There aren't two hundred countries to offend,

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<v Speaker 1>so that would be pretty impressive if we could offend

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<v Speaker 1>non existing countries. Yeah. So the top option was Answer

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<v Speaker 1>two hundred questions, which when Daniel told me, I said

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<v Speaker 1>it was a little impractical for a fifty minute podcast,

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<v Speaker 1>that's right. They have to be like true or false questions,

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<v Speaker 1>or you know, yes or no, or something which wouldn't

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<v Speaker 1>be too satisfied, right. I started to think, if we

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<v Speaker 1>take five minutes to answer each question, that's a thousand

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<v Speaker 1>minute episode. That's basically the next two hundred episodes. Basically,

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<v Speaker 1>we'd be done. We could celebrate our four hundred anniversary

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<v Speaker 1>next week. Then, well, this podcast is really accelerating the

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<v Speaker 1>logarithmic scales. We'll be doing our four thousand one in

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<v Speaker 1>a month, that's right. And I started looking through the

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<v Speaker 1>list of questions we've answered over email, because I answered

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<v Speaker 1>hundreds of questions a week from listeners, and there's a

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<v Speaker 1>lot of common things in there. But then or I

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<v Speaker 1>had a better idea something else we could do to

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<v Speaker 1>celebrate our two hundredth episode. Yeah, so it's be on

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<v Speaker 1>the podcast. We'll be asking two hundred questions, but not

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<v Speaker 1>two hundred number of questions, but a couple of questions

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<v Speaker 1>about the number two hundred. That's right, because while the

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<v Speaker 1>number ten and the number one hundred, and therefore the

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<v Speaker 1>number two hundred are really just artifacts of the number

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<v Speaker 1>of fingers we have in the way the human mind works.

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<v Speaker 1>It's also an interesting way to ask questions about the universe,

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<v Speaker 1>to think about like how far away are things or

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<v Speaker 1>what happened in certain moments of time in the universe.

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<v Speaker 1>It gives you like a fixed window to examine the universe.

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<v Speaker 1>We'll be asking coincidentally to two hundred questions here in

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<v Speaker 1>the podcast, and the first question has to do with

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<v Speaker 1>what happened at the beginning of the universe. So the

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<v Speaker 1>question is what happened in the first two hundred micro

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<v Speaker 1>seconds of the universe. And then later on we'll tackle

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<v Speaker 1>the another question about with the number two hundred, which

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<v Speaker 1>is what can we find within two hundred light years

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<v Speaker 1>of Earth? So a little bit of time and a

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<v Speaker 1>little bit of space, a little bit of space time, Daniel,

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<v Speaker 1>that's right. What can you find within two hundred light

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<v Speaker 1>years of Earth? Makes me think like, are you looking

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<v Speaker 1>for your keys? Are they somewhere out there in space?

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<v Speaker 1>I do lose my keys a lot, even even in

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<v Speaker 1>a pandemic where you don't go anywhere. Somehow I managed

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<v Speaker 1>to lose my keys like every day. Well, we'll see

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<v Speaker 1>if we can find them, all right, we'll tackle this

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<v Speaker 1>first question first, which is what happened in the first

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<v Speaker 1>two hundred micro seconds of the universe. Now, two hundred microseconds,

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<v Speaker 1>that's like, boy, that's like point to milliseconds. It's not

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<v Speaker 1>a lot of time. But it turns out a whole

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<v Speaker 1>lot of stuff happened in the first two hundred microseconds

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<v Speaker 1>to the universe. Basically everything's been boring ever since. Well,

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<v Speaker 1>two d micro seconds. That's that's shorter than a blink, right,

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<v Speaker 1>Like a blink is maybe a couple of microseconds, a

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<v Speaker 1>couple of milliseconds. It's a very small amount of time. Absolutely, Yeah,

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<v Speaker 1>So a lot happened in those first microseconds. A lot happened.

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<v Speaker 1>And one of the most interesting questions really is how

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<v Speaker 1>you even define like moment zero. If you're gonna say,

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<v Speaker 1>let's take a window of time from the very beginning

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<v Speaker 1>of the universe to two d microseconds afterwards, it's interesting

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<v Speaker 1>to think about, like how the universe expands and cools,

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<v Speaker 1>and we'll get into all of that. But then you

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<v Speaker 1>have to wonder, like where does T equal zero? How

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<v Speaker 1>do you define that moment? Do we even know that

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<v Speaker 1>there was a T equal zero? So already like anchoring

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<v Speaker 1>the left side, the early side of that window is very,

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<v Speaker 1>very difficult. It makes me think, like was there a

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<v Speaker 1>T minus one or like a countdown to the universe.

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<v Speaker 1>Nobody really knows, And the problem is that we don't

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<v Speaker 1>think about the history of the universe in that sort

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<v Speaker 1>of forward way because we don't really have anything to

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<v Speaker 1>build on. We don't know what was in the beginning

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<v Speaker 1>or when the beginning was. Usually we think about it

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<v Speaker 1>sort of in the reverse. We look at the universe now,

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<v Speaker 1>and we look backwards in time as we look further

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<v Speaker 1>further out into space, right, because remember the further out

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<v Speaker 1>in space, you look older the universe is. So we

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<v Speaker 1>can see how the universe looked a hundred years ago,

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<v Speaker 1>a thousand years ago, a million years ago, a billion

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<v Speaker 1>years ago, etcetera. And we can project backwards in time.

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<v Speaker 1>So we tend to think of the history of the

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<v Speaker 1>universe sort of from now and running the clock backwards,

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<v Speaker 1>and we can do it pretty well, you know, back

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<v Speaker 1>about thirteen billion years or so, But then it gets

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<v Speaker 1>pretty murky and we have trouble extrapolating back. We don't

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<v Speaker 1>know if there was a T equal zero, if there

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<v Speaker 1>was like a T equals question mark, or who knows

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<v Speaker 1>what was happening at the very beginning. That's interesting. Now,

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<v Speaker 1>why does the picture he get fuzzy beyond if you

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<v Speaker 1>rewind back to more than a few hundred thousand years

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<v Speaker 1>from what what might be the beginning of time? Like

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<v Speaker 1>what what? What actually marks up? Well, the reason is

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<v Speaker 1>that things change, Things get really hot and dense. Right,

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<v Speaker 1>the overall history of the universe is cooling and expanding,

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<v Speaker 1>and so if you run that backwards from now we

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<v Speaker 1>have a cold, large universe. You run that backwards, things

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<v Speaker 1>get hotter and denser. And of course you could just

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<v Speaker 1>do that naively, like assume that the laws of physics

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<v Speaker 1>we have learned today from our cold universe still work

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<v Speaker 1>back then, and just run the clock backwards and you

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<v Speaker 1>get infinite density and you call that T equal zero.

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<v Speaker 1>You could do that, but we don't think that's right.

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<v Speaker 1>We don't think the laws we have work anymore as

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<v Speaker 1>things get that hot and dense, just like you know,

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<v Speaker 1>the physics of gases is different from the physics of

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<v Speaker 1>liquids and the physics of solids, and so things change

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<v Speaker 1>as you get hotter and denser, and then it becomes

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<v Speaker 1>difficult to extrapolate because we're reaching into regions that we

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<v Speaker 1>can't see anymore and we have no experience of because

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<v Speaker 1>there's a moment in the early universe when the universe cooled.

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<v Speaker 1>It was a hot, dense, nastiness, will talk about it,

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<v Speaker 1>and it cooled to a place where light could fly through.

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<v Speaker 1>It became transparent, And that's the last moment in the

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<v Speaker 1>early universe that we can actually see. Beyond that, we're

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<v Speaker 1>just really sort of guessing and extrapolating and using models,

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<v Speaker 1>but those models are very uncertain. We really don't know

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<v Speaker 1>what we're talking about. So a lot of the details

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<v Speaker 1>we'll talk through today in this episode are really speculative.

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<v Speaker 1>They're like, maybe it was this, and maybe it was that,

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<v Speaker 1>and under various assumptions which seemed reasonable but could be

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<v Speaker 1>totally wrong. You know, maybe this happened, But it's really guesswork.

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<v Speaker 1>Is it guesswork because we don't know, like our simulations

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<v Speaker 1>don't aren't very definitive, or like the physics of the

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<v Speaker 1>universe might actually change it in those kind of conditions.

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<v Speaker 1>We don't know how the physics of the universe operates

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<v Speaker 1>in those very hot and dense environments. You know, we've

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<v Speaker 1>only experienced it when it's pretty cold and separated, and

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<v Speaker 1>so we're extrapolating back. We think we have ideas or

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<v Speaker 1>how it might work, and we can simulate various ones

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<v Speaker 1>of them, but we can't necessarily like tell the difference

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<v Speaker 1>between if it's like this or if it's like that,

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<v Speaker 1>and so we just we're extrapolating into the unknown, and

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<v Speaker 1>and that's always very dangerous and delicate. Now, even the

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<v Speaker 1>concept of time equals zero is weird, right, because I've

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<v Speaker 1>heard people say that, you know, like it's it's almost

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<v Speaker 1>like asking what is more north than the north Pole?

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<v Speaker 1>Because once you get to the north pole, there's no

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<v Speaker 1>more north? And is it the same? Also that you know,

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<v Speaker 1>maybe time started at T equal zero and there was

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<v Speaker 1>no time before that. It sounds bonkers to say that, right,

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<v Speaker 1>like there was no time before that, because it's before

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<v Speaker 1>mean if there was no time, right, It's it's confusing.

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<v Speaker 1>It's hard to really get these ideas into your head.

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<v Speaker 1>But it's true that some theories of the universe say

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<v Speaker 1>that space and time were created at some moment and

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<v Speaker 1>things have expanded and cooled since then, and before that point,

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<v Speaker 1>there was no time, There was no space, there was

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<v Speaker 1>no before that point. That's really hard to grasp your

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<v Speaker 1>mind around because your mind lives in that space in

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<v Speaker 1>that time. It's all you've experienced, and so it's all

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<v Speaker 1>you can really imagine how you organize your thinking. It's

0:12:03.240 --> 0:12:06.440
<v Speaker 1>how we think about causality and logic, and a it happens,

0:12:06.480 --> 0:12:09.160
<v Speaker 1>then be happens, then see happens. But it doesn't mean

0:12:09.200 --> 0:12:12.000
<v Speaker 1>it's the only way the universe can be. And so

0:12:12.080 --> 0:12:15.320
<v Speaker 1>it's extraordinarily difficult to sort of extrapolate your brain and

0:12:15.320 --> 0:12:19.280
<v Speaker 1>you're thinking into something completely unfamiliar, right, And so what

0:12:19.320 --> 0:12:21.959
<v Speaker 1>we do is we have these frameworks like general relativity

0:12:22.000 --> 0:12:24.559
<v Speaker 1>and quantum mechanics that try to tell us about what

0:12:24.720 --> 0:12:28.160
<v Speaker 1>might have happened, But those aren't very conclusive either. I

0:12:28.160 --> 0:12:30.760
<v Speaker 1>guess the North Pole analogy kind of works also in that,

0:12:30.960 --> 0:12:33.240
<v Speaker 1>you know, like here where we are. You know, if

0:12:33.280 --> 0:12:36.280
<v Speaker 1>you have like a compass, it's pretty clear how to

0:12:36.360 --> 0:12:38.560
<v Speaker 1>use it, Like, you know, it tells you north and

0:12:38.640 --> 0:12:40.559
<v Speaker 1>right and south and east and west, and you can

0:12:40.559 --> 0:12:42.320
<v Speaker 1>walk around pretty easy blue. But if you are like

0:12:42.400 --> 0:12:44.920
<v Speaker 1>near the North Pole, it might be a little tricky

0:12:45.000 --> 0:12:48.280
<v Speaker 1>to use a compass, right, Yeah, if you're at the

0:12:48.320 --> 0:12:50.559
<v Speaker 1>North Pole, you'd be a little disoriented. Yeah, if you're

0:12:50.559 --> 0:12:53.040
<v Speaker 1>at the north pole. There is no more north to go, right,

0:12:53.120 --> 0:12:55.719
<v Speaker 1>you can't go any north eier than that. But we

0:12:55.760 --> 0:12:58.200
<v Speaker 1>don't know if time works that way. It could be

0:12:58.559 --> 0:13:02.120
<v Speaker 1>that there was stuff for you know, these early moments,

0:13:02.160 --> 0:13:05.120
<v Speaker 1>these singularities. There was a whole other universe perhaps which

0:13:05.200 --> 0:13:09.120
<v Speaker 1>came down into a big crunch or something else totally different,

0:13:09.320 --> 0:13:11.839
<v Speaker 1>some sort of other weird kind of thing which gave

0:13:11.880 --> 0:13:15.679
<v Speaker 1>birth two hours space and time. You know, our entire universe,

0:13:15.679 --> 0:13:18.360
<v Speaker 1>Our space and time could be a bubble of that

0:13:18.440 --> 0:13:22.240
<v Speaker 1>other pre universe stuff like decaying into a universe. There

0:13:22.280 --> 0:13:24.640
<v Speaker 1>could be a whole spectrum of other universes also that

0:13:24.679 --> 0:13:27.079
<v Speaker 1>were created in the same moment, or the could that

0:13:27.120 --> 0:13:29.640
<v Speaker 1>are still being created now. There could be like you know,

0:13:29.720 --> 0:13:32.360
<v Speaker 1>moments of creation happening right now, really far away in

0:13:32.360 --> 0:13:36.360
<v Speaker 1>this other meta space. It sounds like bonker speculation because

0:13:36.480 --> 0:13:39.480
<v Speaker 1>it is mostly because we're so clueless. You mean, like now,

0:13:39.520 --> 0:13:41.680
<v Speaker 1>like as we speak, there could be some time equal

0:13:41.800 --> 0:13:45.520
<v Speaker 1>zero moments right now for other universes in this universe. Yeah.

0:13:45.720 --> 0:13:49.280
<v Speaker 1>One idea of how our universe got started is that

0:13:49.320 --> 0:13:53.080
<v Speaker 1>there was some sort of like pre universe stuff some

0:13:53.360 --> 0:13:58.320
<v Speaker 1>Inflaton fields, and that our universe is essentially some random

0:13:58.360 --> 0:14:02.120
<v Speaker 1>spontaneous decay of at and that's when our universe began,

0:14:02.600 --> 0:14:04.920
<v Speaker 1>and that influence on Field is just like expanding and

0:14:05.000 --> 0:14:09.480
<v Speaker 1>creating and eternally inflating. But all the time it's parts

0:14:09.480 --> 0:14:12.160
<v Speaker 1>of it are decaying and starting whole new universes, their

0:14:12.240 --> 0:14:14.720
<v Speaker 1>universes that haven't even gotten started yet, in universes that

0:14:14.760 --> 0:14:16.840
<v Speaker 1>are trillions of years old. And none of this is

0:14:16.920 --> 0:14:19.840
<v Speaker 1>anything we know. It's just like it's a crazy idea,

0:14:20.360 --> 0:14:22.800
<v Speaker 1>and in a thousand years people will read about these

0:14:22.800 --> 0:14:25.240
<v Speaker 1>ideas the way we think about, you know, the Greek's

0:14:25.320 --> 0:14:28.360
<v Speaker 1>ideas about air, water, fire, and earth. We're like, well,

0:14:28.520 --> 0:14:31.280
<v Speaker 1>that's cute, you know, and it could have been true.

0:14:31.360 --> 0:14:36.160
<v Speaker 1>I suppose, yeah, it's it's well meaning, carefully thought out,

0:14:36.360 --> 0:14:39.320
<v Speaker 1>totally wrong, And that could be the way we describe

0:14:39.400 --> 0:14:41.800
<v Speaker 1>all of our current ideas about what happened to T

0:14:41.880 --> 0:14:44.200
<v Speaker 1>equal zero and whether T equal zero even makes sense.

0:14:44.200 --> 0:14:48.400
<v Speaker 1>It could be like cute to future busicists, exactly lessly

0:14:48.480 --> 0:14:50.960
<v Speaker 1>cute to a future five year olds. Man, five year olds,

0:14:50.960 --> 0:14:53.960
<v Speaker 1>and a thousand years will laugh at our ideas that

0:14:54.080 --> 0:14:58.280
<v Speaker 1>were like, oh, you're ridiculous, that's silly, oh man, well,

0:14:58.440 --> 0:15:01.160
<v Speaker 1>five year olds already laugh at me, Daniel, so that

0:15:01.320 --> 0:15:03.480
<v Speaker 1>that's going to be We'll pretend that's on purpose though,

0:15:03.480 --> 0:15:05.880
<v Speaker 1>all right, so it seems like, okay, so we can't

0:15:05.920 --> 0:15:10.200
<v Speaker 1>see that well beyond a few hundred thousand years into

0:15:10.240 --> 0:15:12.840
<v Speaker 1>the universe. So really asking like what happened in the

0:15:12.840 --> 0:15:17.080
<v Speaker 1>first twohundred microseconds is really speculative, then that's right. All

0:15:17.120 --> 0:15:20.360
<v Speaker 1>you can do is say, like, you know, extrapolate backwards

0:15:20.400 --> 0:15:23.040
<v Speaker 1>from where we are it gets hotter and denser, hotter

0:15:23.080 --> 0:15:26.000
<v Speaker 1>and denser, and pretend that you know how to extrapolate

0:15:26.200 --> 0:15:29.320
<v Speaker 1>back to some point like general relativity says you can

0:15:29.320 --> 0:15:31.760
<v Speaker 1>extrapolate all the way back to a point of infinite

0:15:31.800 --> 0:15:34.360
<v Speaker 1>density and temperature. But you know, we know that general

0:15:34.400 --> 0:15:37.920
<v Speaker 1>relativity is probably wrong when it talks about singularities and

0:15:37.960 --> 0:15:41.800
<v Speaker 1>stuff like that, because it ignores important things like quantum mechanics,

0:15:42.040 --> 0:15:45.040
<v Speaker 1>which tells us that you can't have an infinite amount

0:15:45.040 --> 0:15:47.760
<v Speaker 1>of stuff in a tiny zero volume point and know

0:15:47.920 --> 0:15:51.640
<v Speaker 1>all about it. So definitely something wonky happens. But you know,

0:15:51.960 --> 0:15:55.000
<v Speaker 1>you can extrapolate sort of naively and say we'll call

0:15:55.080 --> 0:15:57.920
<v Speaker 1>this t equal zero and we'll move forward from there.

0:15:58.280 --> 0:16:00.000
<v Speaker 1>I see, I see so we're gonna plant the flow.

0:16:00.080 --> 0:16:02.280
<v Speaker 1>I can say this is tequals zero, and then we're

0:16:02.280 --> 0:16:04.560
<v Speaker 1>going to see what can the universe do to get

0:16:04.600 --> 0:16:07.600
<v Speaker 1>us to where we are today? Kind of yeah, exactly.

0:16:07.680 --> 0:16:09.680
<v Speaker 1>All right, well let's get into that and to the

0:16:09.760 --> 0:16:11.920
<v Speaker 1>question of what is within two hundred light years of Earth?

0:16:12.000 --> 0:16:28.360
<v Speaker 1>But first let's take a quick break. All right, Daniel,

0:16:28.560 --> 0:16:31.880
<v Speaker 1>we're celebrating our two birthday. Does that mean that I'm

0:16:31.880 --> 0:16:34.120
<v Speaker 1>two years old and you're two hundred years old, or

0:16:34.120 --> 0:16:36.960
<v Speaker 1>we're each a hundred years old? It means we should

0:16:36.960 --> 0:16:40.640
<v Speaker 1>have retired a hundred and thirty years ago. I feel

0:16:40.680 --> 0:16:43.040
<v Speaker 1>like this podcast has aged me two years. I feel

0:16:43.080 --> 0:16:45.360
<v Speaker 1>like I'm two hundred light years from where I started. There,

0:16:45.360 --> 0:16:47.840
<v Speaker 1>you go, all right, well, so we're talking about the

0:16:47.840 --> 0:16:51.160
<v Speaker 1>first two hundred microseconds of the universe, and so we'll

0:16:51.160 --> 0:16:54.200
<v Speaker 1>start with time equals zero. What what happened at times zero? Daniel?

0:16:54.280 --> 0:16:56.640
<v Speaker 1>We don't know, but one idea is that there was

0:16:56.680 --> 0:16:59.520
<v Speaker 1>a singularity that you know, the universe was super hot

0:16:59.560 --> 0:17:01.640
<v Speaker 1>and super dense. And I think a lot of people

0:17:01.720 --> 0:17:05.560
<v Speaker 1>imagine this as a single point. They hear singularity to

0:17:05.640 --> 0:17:09.080
<v Speaker 1>think a single point. They think one hot, dense spot

0:17:09.440 --> 0:17:12.239
<v Speaker 1>like the entire energy and all the matter of the

0:17:12.320 --> 0:17:17.080
<v Speaker 1>universe was in a really tiny dot. But it's better

0:17:17.119 --> 0:17:19.360
<v Speaker 1>not to think about it as one place, but more

0:17:19.400 --> 0:17:21.960
<v Speaker 1>to think about it as the density. Because we don't

0:17:22.000 --> 0:17:26.560
<v Speaker 1>know if the universe is finite or infinite. Possible that

0:17:26.600 --> 0:17:30.000
<v Speaker 1>when the universe started it was already infinite, and that

0:17:30.080 --> 0:17:36.440
<v Speaker 1>this singularity we're talking about was everywhere like multiple singularity, yes, yes, precisely,

0:17:36.560 --> 0:17:39.960
<v Speaker 1>like a non singular singularity. Yes. Like the singularity refers

0:17:40.160 --> 0:17:42.919
<v Speaker 1>not to how many of them there were, but the

0:17:42.960 --> 0:17:46.320
<v Speaker 1>fact that the density becomes infinite singularity refers to what

0:17:46.359 --> 0:17:50.000
<v Speaker 1>happens to the equations, that the equations get infinities in them,

0:17:50.240 --> 0:17:53.360
<v Speaker 1>because the density becomes infinite, not the size of it.

0:17:53.600 --> 0:17:56.080
<v Speaker 1>And there's a i think a very common misconception that

0:17:56.080 --> 0:17:58.720
<v Speaker 1>the Big Bang or pre Big Bang starts with a dot,

0:17:59.080 --> 0:18:02.040
<v Speaker 1>and a dots small than an adam becomes the entire universe.

0:18:02.400 --> 0:18:04.480
<v Speaker 1>And because we don't know how big the universe is,

0:18:04.480 --> 0:18:06.359
<v Speaker 1>it could have been a little blob, it could have

0:18:06.359 --> 0:18:08.760
<v Speaker 1>been an infinite extent. It's better to think about it

0:18:08.800 --> 0:18:12.399
<v Speaker 1>in terms of infinite density, or like an infinite number

0:18:12.440 --> 0:18:15.200
<v Speaker 1>of dots, an infinite number of dots. Yeah, The thing

0:18:15.240 --> 0:18:18.280
<v Speaker 1>we do know is that the universe was denser and

0:18:18.359 --> 0:18:20.520
<v Speaker 1>harder back then. We don't know how much of it

0:18:20.560 --> 0:18:23.119
<v Speaker 1>there was, could have been infinite, could be finite, and

0:18:23.160 --> 0:18:26.040
<v Speaker 1>loop all around on itself. That's a whole other episode

0:18:26.080 --> 0:18:28.639
<v Speaker 1>about the size and shape of the universe, which is fascinating.

0:18:28.960 --> 0:18:30.679
<v Speaker 1>But to think through the history of the universe is

0:18:30.720 --> 0:18:33.679
<v Speaker 1>mostly to think about the density changing da days that

0:18:34.080 --> 0:18:37.159
<v Speaker 1>you know, there's no real reason for this to exist,

0:18:37.359 --> 0:18:41.000
<v Speaker 1>just somehow the universe what we know was really dance,

0:18:41.400 --> 0:18:43.600
<v Speaker 1>almost like infinitely dance. Yeah, there must have been a

0:18:43.640 --> 0:18:45.879
<v Speaker 1>reason for it to exist, because it does. And we

0:18:45.920 --> 0:18:48.760
<v Speaker 1>think the universe follows reasons and laws. We just don't

0:18:48.800 --> 0:18:50.600
<v Speaker 1>know what they are and we can't argue for it.

0:18:50.600 --> 0:18:53.160
<v Speaker 1>We don't know why there was something instead of nothing,

0:18:53.200 --> 0:18:54.919
<v Speaker 1>and why there was this, and could there have been

0:18:55.000 --> 0:18:58.320
<v Speaker 1>other things, and you know, just really shockingly basic questions

0:18:58.560 --> 0:19:00.720
<v Speaker 1>that we have really no clue about. Okay, so we

0:19:00.760 --> 0:19:04.440
<v Speaker 1>had to super dance state almost infinitely dense, maybe everywhere,

0:19:04.520 --> 0:19:07.199
<v Speaker 1>maybe just one dot, and then what's next thing that

0:19:07.320 --> 0:19:09.320
<v Speaker 1>happened and what happened in the first tend to the

0:19:09.440 --> 0:19:11.879
<v Speaker 1>minus you know, forty three seconds, so The picture you

0:19:11.880 --> 0:19:14.320
<v Speaker 1>should have in your mind is that we have space,

0:19:14.840 --> 0:19:17.520
<v Speaker 1>and space is really really hot, like there's a huge

0:19:17.520 --> 0:19:20.440
<v Speaker 1>amount of energy. Right. The density we're really talking about

0:19:20.480 --> 0:19:24.160
<v Speaker 1>there is energy density. And if you've been following the podcast,

0:19:24.200 --> 0:19:25.760
<v Speaker 1>you know that we like to think about space in

0:19:25.840 --> 0:19:29.400
<v Speaker 1>terms of quantum fields. Every point in space has fields

0:19:29.400 --> 0:19:33.440
<v Speaker 1>in it, the electron fields of cork fields, the photon fields, etcetera.

0:19:33.800 --> 0:19:36.640
<v Speaker 1>And particles that we think about today are little blobs

0:19:36.640 --> 0:19:40.000
<v Speaker 1>of excitations of those fields. Today, most of those fields

0:19:40.000 --> 0:19:42.879
<v Speaker 1>are very very low energy. Most of space is empty

0:19:42.880 --> 0:19:46.400
<v Speaker 1>in those fields are zero. But back then, infinite density

0:19:46.440 --> 0:19:49.479
<v Speaker 1>really means all those fields are going nuts. They're going crazy,

0:19:49.520 --> 0:19:53.000
<v Speaker 1>they're oscillating, they're just full of energy. And so instead

0:19:53.000 --> 0:19:56.600
<v Speaker 1>of thinking about individual particles, it's like having an ocean, right,

0:19:56.640 --> 0:19:59.080
<v Speaker 1>you don't think about a drop of water. When you

0:19:59.119 --> 0:20:01.520
<v Speaker 1>have an ocean. You can just think about the entire crazy,

0:20:01.520 --> 0:20:04.520
<v Speaker 1>turbulent blob and it's doing all sorts of stuff. So

0:20:04.560 --> 0:20:07.439
<v Speaker 1>the first ten to the minus forty three seconds of

0:20:07.480 --> 0:20:10.720
<v Speaker 1>the universe we called this the plant epoch. Everything was

0:20:10.760 --> 0:20:12.959
<v Speaker 1>hot and dense in these fields were just going crazy.

0:20:13.480 --> 0:20:16.040
<v Speaker 1>Now I have a question, though, somebody's talk about that.

0:20:16.160 --> 0:20:19.640
<v Speaker 1>It's not just like stuff that was crammed in together

0:20:19.720 --> 0:20:25.000
<v Speaker 1>really tightly. It's also that space itself was smaller, much smaller.

0:20:26.000 --> 0:20:28.600
<v Speaker 1>So it's like it's both those things. It's like everything

0:20:28.680 --> 0:20:31.959
<v Speaker 1>was crowned in together and also space was smaller. That's right.

0:20:32.000 --> 0:20:34.680
<v Speaker 1>There's two kinds of expansion we're gonna talk about later.

0:20:34.880 --> 0:20:38.360
<v Speaker 1>One is the expansion of stuff through space as things

0:20:38.440 --> 0:20:41.520
<v Speaker 1>spread out into existing space. The other is the expansion

0:20:41.880 --> 0:20:45.600
<v Speaker 1>of space that you create more space, and new space

0:20:45.600 --> 0:20:48.879
<v Speaker 1>itself is created. Because remember that space is not just

0:20:48.960 --> 0:20:52.600
<v Speaker 1>like a backdrop on which things happen. There's a dynamical

0:20:52.640 --> 0:20:56.760
<v Speaker 1>connection between space and energy. Space curves and bends and

0:20:56.800 --> 0:21:00.320
<v Speaker 1>expands in response to the mass and energy that's in it,

0:21:00.720 --> 0:21:03.600
<v Speaker 1>and then it shapes the motion of that mass and energy.

0:21:03.960 --> 0:21:06.639
<v Speaker 1>So space and mass and energy are two things that

0:21:06.640 --> 0:21:10.280
<v Speaker 1>are very tightly coupled and respond to each other. Okay,

0:21:10.440 --> 0:21:13.120
<v Speaker 1>so in the first you know point zero zero zero

0:21:13.200 --> 0:21:17.840
<v Speaker 1>zero down to forty zeros one seconds, you said, that's

0:21:17.880 --> 0:21:20.040
<v Speaker 1>called the planet. Yeah, and back there we had a

0:21:20.040 --> 0:21:22.560
<v Speaker 1>bunch of really hot fields. And the thing to think

0:21:22.560 --> 0:21:25.280
<v Speaker 1>about here is that there are no particles. What it's

0:21:25.359 --> 0:21:28.160
<v Speaker 1>it's like too hot for particles like particles just kind

0:21:28.200 --> 0:21:30.399
<v Speaker 1>of everything is just crazy. That's right. There are no

0:21:30.520 --> 0:21:33.800
<v Speaker 1>isolated particles because everything is just too hot and too intense.

0:21:34.119 --> 0:21:36.959
<v Speaker 1>It's all just energy in these fields. It's slashing around.

0:21:37.320 --> 0:21:39.480
<v Speaker 1>You know, later on things will cool down enough for

0:21:39.720 --> 0:21:42.520
<v Speaker 1>particles to form. But particles are like you know, when

0:21:42.520 --> 0:21:45.159
<v Speaker 1>you have a few little isolated blobs of energy in

0:21:45.200 --> 0:21:48.240
<v Speaker 1>the field. Here we have like an incredible turbulent ocean.

0:21:48.520 --> 0:21:50.280
<v Speaker 1>So it makes no sense to think about in terms

0:21:50.280 --> 0:21:52.880
<v Speaker 1>of particles. I mean, technically you could, you could say

0:21:53.200 --> 0:21:55.960
<v Speaker 1>this field is ten ca jillion particles in it, but

0:21:56.000 --> 0:21:58.600
<v Speaker 1>it doesn't really make any sense. It's really just energies,

0:21:58.640 --> 0:22:01.639
<v Speaker 1>not discrete packets being around through space. It's just a

0:22:01.720 --> 0:22:04.520
<v Speaker 1>huge blob of energy slashing around in the field. I see.

0:22:04.560 --> 0:22:06.720
<v Speaker 1>There's no moment where you're like, oh, there's an electron.

0:22:06.960 --> 0:22:10.200
<v Speaker 1>It's just that the whole field is just sit on fire. Yeah, precisely.

0:22:10.600 --> 0:22:13.000
<v Speaker 1>You can't follow a drop of water in the ocean, right.

0:22:13.480 --> 0:22:15.159
<v Speaker 1>And the other thing to think about is that the

0:22:15.200 --> 0:22:18.719
<v Speaker 1>fields here behave differently, just like the way materials on

0:22:18.800 --> 0:22:22.520
<v Speaker 1>Earth have phases as you cool them or or heat

0:22:22.560 --> 0:22:25.480
<v Speaker 1>them up. The physics of them changes completely, right, The

0:22:25.520 --> 0:22:27.879
<v Speaker 1>same thing happens for fields. They tend to act in

0:22:27.960 --> 0:22:32.000
<v Speaker 1>different ways at different temperatures and different energy densities. And

0:22:32.000 --> 0:22:34.440
<v Speaker 1>this is not like the laws of physics changing. It's

0:22:34.480 --> 0:22:36.560
<v Speaker 1>just like how you can think about it, how you

0:22:36.560 --> 0:22:40.000
<v Speaker 1>can describe it. The effective the emergent results of it

0:22:40.160 --> 0:22:42.960
<v Speaker 1>are very different at different temperatures, just the same way

0:22:43.000 --> 0:22:45.000
<v Speaker 1>they are for solid But can we still use the

0:22:45.000 --> 0:22:47.840
<v Speaker 1>same equations we have, Like do our equations still work?

0:22:48.000 --> 0:22:50.480
<v Speaker 1>We don't think they do. We think the equations that

0:22:50.520 --> 0:22:54.480
<v Speaker 1>we have now only describe physics sort of at lower temperatures,

0:22:54.760 --> 0:22:57.240
<v Speaker 1>that they're sort of like the falling at the effective

0:22:57.280 --> 0:23:00.720
<v Speaker 1>equations for what happens when things are old. We don't

0:23:00.760 --> 0:23:04.200
<v Speaker 1>think we have like the fundamental equations. Our equations should

0:23:04.280 --> 0:23:07.919
<v Speaker 1>be like the low temperature limit of the true equations,

0:23:07.920 --> 0:23:10.760
<v Speaker 1>which we haven't found yet. But for example, and we

0:23:10.800 --> 0:23:13.040
<v Speaker 1>think that a very hot temperature is the early moments,

0:23:13.359 --> 0:23:18.439
<v Speaker 1>all of the forces acted like one gravity, electromagnetism, the

0:23:18.480 --> 0:23:20.919
<v Speaker 1>weak force, and the strong force. We think they're probably

0:23:20.960 --> 0:23:23.679
<v Speaker 1>all just one force that acted together. What do you

0:23:23.680 --> 0:23:26.439
<v Speaker 1>mean of force? Don't forces depend on particles to no?

0:23:26.600 --> 0:23:29.520
<v Speaker 1>Forces are also just fields? Right, But we think that

0:23:29.560 --> 0:23:33.120
<v Speaker 1>there was a single field that represents all those forces

0:23:33.119 --> 0:23:35.399
<v Speaker 1>but combined into one. And we think when it was

0:23:35.440 --> 0:23:38.040
<v Speaker 1>really hot and dense, that they acted together. They all

0:23:38.080 --> 0:23:40.399
<v Speaker 1>had the same strength, and there were all just different

0:23:40.440 --> 0:23:44.520
<v Speaker 1>components of one mega force which exists in the universe. Well,

0:23:44.520 --> 0:23:46.840
<v Speaker 1>I think you just coined the term right there at

0:23:46.840 --> 0:23:50.320
<v Speaker 1>the megaphorce. This is like to call it the grand

0:23:50.440 --> 0:23:55.160
<v Speaker 1>unified theory. I like megaphorce better megaforce. It is, then,

0:23:56.359 --> 0:23:58.439
<v Speaker 1>all right, so those are the first ten to the

0:23:58.480 --> 0:24:01.120
<v Speaker 1>minus forty three second. Is then what happened? And things

0:24:01.160 --> 0:24:03.920
<v Speaker 1>start to cool, things start to expand a little bit,

0:24:04.200 --> 0:24:08.200
<v Speaker 1>and the first breaking happens. Here the force splits into two.

0:24:08.520 --> 0:24:11.199
<v Speaker 1>You have gravity on one side, and then all the

0:24:11.320 --> 0:24:14.920
<v Speaker 1>other forces electromagnetism, the weak force, and the strong force

0:24:15.119 --> 0:24:18.719
<v Speaker 1>combined still into one single force, which we call electro strong.

0:24:19.560 --> 0:24:22.080
<v Speaker 1>And so here the temperature has dropped enough that the

0:24:22.080 --> 0:24:25.080
<v Speaker 1>force has split. It's like cracked. You know how. Sometimes

0:24:25.080 --> 0:24:28.439
<v Speaker 1>when you cool something, you can freeze, or it can crack,

0:24:28.560 --> 0:24:31.160
<v Speaker 1>or it can end them as some weird configuration. As

0:24:31.200 --> 0:24:33.879
<v Speaker 1>the universe cooled, gravity sort of like froze and split

0:24:33.960 --> 0:24:37.600
<v Speaker 1>off from the other forces. Interesting like inevitably or is

0:24:37.600 --> 0:24:39.640
<v Speaker 1>it like a random you know, like an ice when

0:24:39.640 --> 0:24:42.320
<v Speaker 1>you freeze eyes, you you sometimes get crystals here or

0:24:42.359 --> 0:24:44.320
<v Speaker 1>crystals there. Is it random like that or is it

0:24:44.359 --> 0:24:47.000
<v Speaker 1>like inevitable? Do you think that the equations were like

0:24:47.160 --> 0:24:49.080
<v Speaker 1>we were always going to get gravity and these other

0:24:49.119 --> 0:24:52.879
<v Speaker 1>forces we don't know. We call it spontaneous symmetry breaking

0:24:52.880 --> 0:24:55.680
<v Speaker 1>because we think there's a random element in it and

0:24:55.720 --> 0:24:57.920
<v Speaker 1>all the forces you'll see as we go through time,

0:24:57.960 --> 0:25:00.119
<v Speaker 1>all the forces split off, and we think that those

0:25:00.119 --> 0:25:04.040
<v Speaker 1>splittings are spontaneous, that they're essentially the result of one

0:25:04.080 --> 0:25:07.480
<v Speaker 1>little quantum fluctuation which then gets propagated through the universe.

0:25:07.800 --> 0:25:10.560
<v Speaker 1>You know, like when everybody sits down at a dinner table,

0:25:10.840 --> 0:25:12.560
<v Speaker 1>do you drink from the glass to your left to

0:25:12.600 --> 0:25:15.480
<v Speaker 1>your right? Well, if one person chooses left, then you know,

0:25:15.560 --> 0:25:17.879
<v Speaker 1>everybody around them starts to choose left and it spreads

0:25:17.880 --> 0:25:20.760
<v Speaker 1>across the whole dinner table. Right, they could have chosen

0:25:20.800 --> 0:25:22.320
<v Speaker 1>to drink from the one to their right and then

0:25:22.359 --> 0:25:25.600
<v Speaker 1>everyone would use that one. So one little fluctuation like

0:25:25.640 --> 0:25:29.000
<v Speaker 1>that can propagate itself through the whole universe. And we

0:25:29.040 --> 0:25:33.320
<v Speaker 1>don't know if gravity splitting off was inevitable or at

0:25:33.359 --> 0:25:36.080
<v Speaker 1>what temperature it should have split off? We just don't know.

0:25:36.160 --> 0:25:39.480
<v Speaker 1>We think gravity split off first because it's the weakest force,

0:25:39.880 --> 0:25:42.159
<v Speaker 1>and so we think it would take the hottest temperature

0:25:42.400 --> 0:25:45.720
<v Speaker 1>to combine all the forces. And then fourteen billion years later,

0:25:45.760 --> 0:25:49.800
<v Speaker 1>everyone's like, is this my glasses? Is your glass? Did

0:25:49.800 --> 0:25:51.440
<v Speaker 1>you drink from mine? Because I thought I had more

0:25:51.440 --> 0:25:55.720
<v Speaker 1>wine left over? And then people are spitting up what

0:25:57.560 --> 0:25:59.720
<v Speaker 1>And then it's it's like back to the big bank,

0:26:00.119 --> 0:26:02.720
<v Speaker 1>all right, So things start to split off and cool down,

0:26:02.760 --> 0:26:06.520
<v Speaker 1>and then we start to get more forces defined. Uh,

0:26:06.640 --> 0:26:08.880
<v Speaker 1>and then what happens next? And then the next thing

0:26:08.920 --> 0:26:12.359
<v Speaker 1>to split off is the strong force. So gravity split off,

0:26:12.440 --> 0:26:14.560
<v Speaker 1>and then the strong force splits off. So now we

0:26:14.600 --> 0:26:16.720
<v Speaker 1>have gravity, we have the strong force, and we have

0:26:16.800 --> 0:26:20.000
<v Speaker 1>the electro weak force electro week being the combination of

0:26:20.000 --> 0:26:24.080
<v Speaker 1>electromagnetism and the weak force. Remember still we have no particles,

0:26:24.080 --> 0:26:26.479
<v Speaker 1>so these things aren't like forces that we think of

0:26:26.520 --> 0:26:29.560
<v Speaker 1>today that are balancing particles around. It's just the fields

0:26:29.640 --> 0:26:34.000
<v Speaker 1>now have different properties. They operate differently, they contain energy differently,

0:26:34.240 --> 0:26:36.960
<v Speaker 1>they have different strengths. As the universe is coolest, so

0:26:37.000 --> 0:26:39.679
<v Speaker 1>gravity split off, but it's not like bringing anything together

0:26:39.720 --> 0:26:42.000
<v Speaker 1>because there is no thing. Well, gravity is doing what

0:26:42.080 --> 0:26:44.520
<v Speaker 1>gravity does. It's you know, the bending of space. But

0:26:44.960 --> 0:26:48.040
<v Speaker 1>you know, even talking about merging gravity with these other

0:26:48.080 --> 0:26:51.200
<v Speaker 1>forces requires a conceptual leap that we haven't made yet,

0:26:51.359 --> 0:26:54.440
<v Speaker 1>which is thinking about gravity as a quantum field, which

0:26:54.480 --> 0:26:57.400
<v Speaker 1>we don't know how to do, especially in the early universe.

0:26:57.640 --> 0:27:00.119
<v Speaker 1>So we are really out on very thin ice, or

0:27:00.160 --> 0:27:04.199
<v Speaker 1>conceptually would like maybe if gravity can be unified with

0:27:04.200 --> 0:27:06.720
<v Speaker 1>the other forces, then it was the first thing to

0:27:06.720 --> 0:27:09.200
<v Speaker 1>split off of some mega force which might exist. And

0:27:09.359 --> 0:27:14.200
<v Speaker 1>I can't emphasize enough how much respeculating cluelessly here, Okay, right, right,

0:27:14.280 --> 0:27:16.639
<v Speaker 1>if gravity is a quantum field, this is kind of

0:27:16.640 --> 0:27:19.840
<v Speaker 1>what we might expect. Yeah, yeah, exactly. But it's not

0:27:19.880 --> 0:27:21.760
<v Speaker 1>like we have a firm prediction that we can like

0:27:21.960 --> 0:27:25.760
<v Speaker 1>interrogate and explore. It's just like, hopefully somebody clever comes

0:27:25.760 --> 0:27:28.119
<v Speaker 1>along and figures out how to make gravity quantum field

0:27:28.240 --> 0:27:30.159
<v Speaker 1>and maybe it would work like this. All right, So

0:27:30.200 --> 0:27:32.399
<v Speaker 1>now that and we split off the strong force, now

0:27:32.440 --> 0:27:35.880
<v Speaker 1>we have more forces, and then something dramatic happens at

0:27:35.880 --> 0:27:39.160
<v Speaker 1>around ten to the minus thirty two seconds. Right, Yeah,

0:27:39.359 --> 0:27:42.240
<v Speaker 1>here's where the excitement really happens, and we don't know why,

0:27:42.560 --> 0:27:45.240
<v Speaker 1>but we think at this point, for some reason, the

0:27:45.359 --> 0:27:50.640
<v Speaker 1>universe started to expand extraordinarily rapidly, like space itself expanded,

0:27:50.720 --> 0:27:54.040
<v Speaker 1>not just stuff flying through space slashing around, but space

0:27:54.080 --> 0:27:58.320
<v Speaker 1>itself got stretched. Remember that space can expand based on

0:27:58.359 --> 0:28:00.720
<v Speaker 1>the mass that's in it, Like we know the space

0:28:00.800 --> 0:28:03.840
<v Speaker 1>is expanding right now. In their current universe is something

0:28:03.880 --> 0:28:06.919
<v Speaker 1>called dark energy, which is creating new space, not just

0:28:07.280 --> 0:28:10.840
<v Speaker 1>pulling on space, not pushing things further apart through space,

0:28:10.840 --> 0:28:14.400
<v Speaker 1>but actually like adding new bits of space between galaxies.

0:28:15.000 --> 0:28:17.680
<v Speaker 1>So that can definitely happen, and we know that it

0:28:17.720 --> 0:28:20.639
<v Speaker 1>did happen in the very early which were created more space.

0:28:21.040 --> 0:28:24.040
<v Speaker 1>The universe just started just creating at a crazy rate. Right.

0:28:24.240 --> 0:28:25.960
<v Speaker 1>It's the kind of this kind of the bang in

0:28:26.000 --> 0:28:27.800
<v Speaker 1>the Big Bang theory. Yeah, this is sort of the

0:28:28.200 --> 0:28:30.359
<v Speaker 1>bang and the Big Bang theory. I mean, originally people

0:28:30.400 --> 0:28:32.359
<v Speaker 1>thought of the Big Bang is like a dot and

0:28:32.400 --> 0:28:35.800
<v Speaker 1>things explode through space. These days, we have this period

0:28:36.000 --> 0:28:38.520
<v Speaker 1>we're talking about now, which we call inflation, and then

0:28:38.560 --> 0:28:40.720
<v Speaker 1>we think of the hot Big Bang is basically at

0:28:40.720 --> 0:28:43.320
<v Speaker 1>the very end of inflation. But you know, the terms

0:28:43.360 --> 0:28:46.160
<v Speaker 1>are a little fuzzy, but essentially here you have the

0:28:46.160 --> 0:28:50.440
<v Speaker 1>biggest bang. I mean, the universe expands by a ridiculous amount.

0:28:50.440 --> 0:28:55.840
<v Speaker 1>It's ten to the seventy eight ten ten to zero.

0:28:55.960 --> 0:28:58.320
<v Speaker 1>So you take a piece of space that's like a

0:28:58.440 --> 0:29:02.160
<v Speaker 1>nanometer across, very very quickly, in like ten to the

0:29:02.160 --> 0:29:07.280
<v Speaker 1>minus thirty two seconds, you expanded to a hundred trillion kilometers. Crazy.

0:29:07.520 --> 0:29:10.560
<v Speaker 1>So in ten to the minus thirty two point zero

0:29:10.640 --> 0:29:16.080
<v Speaker 1>zero zeros one seconds, the universe for some reason just

0:29:16.600 --> 0:29:19.760
<v Speaker 1>was like come out of here. Yeah, exactly, And and

0:29:19.800 --> 0:29:22.600
<v Speaker 1>we don't know why. We we have, like you know,

0:29:22.800 --> 0:29:25.480
<v Speaker 1>given fancy names to this theory to make it sound

0:29:25.520 --> 0:29:27.360
<v Speaker 1>like it's a thing we know how to deal with.

0:29:27.760 --> 0:29:30.000
<v Speaker 1>We call the inflation theory. We think maybe it was

0:29:30.040 --> 0:29:34.080
<v Speaker 1>generated by the inflaton field, but that's really just like saying, oh,

0:29:34.160 --> 0:29:38.160
<v Speaker 1>you know, the answer is a fluctuation in my cluelessness field,

0:29:38.240 --> 0:29:41.120
<v Speaker 1>like I really just don't know. For this into the

0:29:41.160 --> 0:29:45.960
<v Speaker 1>framework of ideas, so it sounds clever, so they're like, oh,

0:29:46.240 --> 0:29:49.760
<v Speaker 1>they blew up. And it could be, you know, that

0:29:49.800 --> 0:29:53.680
<v Speaker 1>it's triggered by the electroweak breaking that like maybe breaking

0:29:53.680 --> 0:29:56.760
<v Speaker 1>off the strong force from the electroweak force created the

0:29:56.800 --> 0:29:59.920
<v Speaker 1>infloton field or settled the infloton field into a way

0:30:00.040 --> 0:30:03.040
<v Speaker 1>that made it do this crazy expansion. But this is

0:30:03.080 --> 0:30:07.440
<v Speaker 1>guessing upon guess. We are very confident that inflation happened.

0:30:07.720 --> 0:30:10.160
<v Speaker 1>I mean the things that it predicts are very specific

0:30:10.480 --> 0:30:14.880
<v Speaker 1>and very concrete. You know, like before inflation, the universe

0:30:14.960 --> 0:30:18.080
<v Speaker 1>is very hot and dense, but not totally uniform because

0:30:18.080 --> 0:30:20.840
<v Speaker 1>it's quantum mechanical, and so you get subspots that have

0:30:20.960 --> 0:30:23.840
<v Speaker 1>like little quantum fluctuations of a little bit more density

0:30:23.880 --> 0:30:26.400
<v Speaker 1>and quantum fluctuation is a little bit less density, really

0:30:26.400 --> 0:30:30.920
<v Speaker 1>really tiny variations. But then this inflation is stretching, turns

0:30:31.000 --> 0:30:35.200
<v Speaker 1>those little seeds of over densities into big structures which

0:30:35.240 --> 0:30:37.280
<v Speaker 1>then form the structure of the universe. And we can

0:30:37.600 --> 0:30:40.520
<v Speaker 1>do all those simulations and it describes very well what

0:30:40.560 --> 0:30:43.400
<v Speaker 1>we see today is thing. And I guess one question

0:30:43.480 --> 0:30:45.880
<v Speaker 1>is where did all the space come from? Like when

0:30:45.920 --> 0:30:48.800
<v Speaker 1>you make space, does it require energy? Yeah, we don't

0:30:48.800 --> 0:30:51.200
<v Speaker 1>really know. I mean, we know that the universe is

0:30:51.200 --> 0:30:55.000
<v Speaker 1>not closed, and so an energy conservation is not required

0:30:55.080 --> 0:30:59.000
<v Speaker 1>by general relativity to make space, you don't need energy. Maybe, well,

0:30:59.040 --> 0:31:02.080
<v Speaker 1>you know space is energy, like space has energy in it.

0:31:02.200 --> 0:31:04.480
<v Speaker 1>When you create space, it has all these fields, and

0:31:04.520 --> 0:31:07.120
<v Speaker 1>those fields have energy in them, and so when you

0:31:07.200 --> 0:31:10.200
<v Speaker 1>create space, it's like creating energy. So it's not something

0:31:10.240 --> 0:31:12.640
<v Speaker 1>that we understand. It's not something we know how to do,

0:31:13.160 --> 0:31:15.600
<v Speaker 1>or that we understand the rules about. We see it

0:31:15.680 --> 0:31:18.680
<v Speaker 1>happening in our current universe. We don't understand the mechanism

0:31:18.680 --> 0:31:20.960
<v Speaker 1>behind it. We call it dark energy because we're clueless.

0:31:21.320 --> 0:31:23.440
<v Speaker 1>We know that it happened in the very early universe.

0:31:23.840 --> 0:31:27.320
<v Speaker 1>Maybe it's the same mechanism, maybe it's something totally different.

0:31:27.440 --> 0:31:29.320
<v Speaker 1>We really just don't know, all right, So now we're

0:31:29.320 --> 0:31:33.080
<v Speaker 1>getting almost to the two microsecond mark, So let's finish

0:31:33.080 --> 0:31:35.880
<v Speaker 1>off what happens in the first two microseconds, and then

0:31:35.920 --> 0:31:38.520
<v Speaker 1>we'll go on to our next question. But first let's

0:31:38.560 --> 0:31:53.560
<v Speaker 1>to get quick break, all right, Daniel, we just exploded

0:31:53.600 --> 0:31:57.440
<v Speaker 1>the universe. We just went through inflation. In the first

0:31:57.480 --> 0:32:01.160
<v Speaker 1>tent of the minus thirty two seconds, one ter became

0:32:01.280 --> 0:32:06.440
<v Speaker 1>a hundred trillion kilometers. Now things are expanding like crazy.

0:32:06.760 --> 0:32:10.320
<v Speaker 1>Quantum fluctuations make a huge difference. Now what happens now

0:32:10.360 --> 0:32:14.200
<v Speaker 1>we finally get particles. Things have cooled down enough that

0:32:14.320 --> 0:32:17.880
<v Speaker 1>the energy that's in the field is distinct and discretized,

0:32:17.920 --> 0:32:20.000
<v Speaker 1>and you can follow it around. You can say, oh,

0:32:20.160 --> 0:32:23.080
<v Speaker 1>this little blob of energy in the electron field is

0:32:23.160 --> 0:32:26.080
<v Speaker 1>moving through space in a coherent way. You can call

0:32:26.160 --> 0:32:29.040
<v Speaker 1>this an electron and the same for the other fields.

0:32:29.240 --> 0:32:32.200
<v Speaker 1>And so you start to get particles made, and you

0:32:32.240 --> 0:32:34.720
<v Speaker 1>get the last moment of breaking that we're aware of

0:32:35.120 --> 0:32:37.800
<v Speaker 1>the electro weak force, which at the time was just

0:32:37.960 --> 0:32:40.840
<v Speaker 1>one force. You know, there wasn't like a separate photon

0:32:41.000 --> 0:32:44.040
<v Speaker 1>and W n z bosons acting separately. It was a

0:32:44.080 --> 0:32:47.760
<v Speaker 1>single force with four of its own bosons. This field

0:32:47.760 --> 0:32:51.840
<v Speaker 1>now breaks, and it breaks into electromagnetism and the weak force.

0:32:51.920 --> 0:32:54.479
<v Speaker 1>It becomes two forces. It becomes two forces that are

0:32:54.480 --> 0:32:57.600
<v Speaker 1>still closely connected. I mean, they're two broken pieces of

0:32:57.600 --> 0:32:59.600
<v Speaker 1>a larger force. You can sort of like fit them

0:32:59.600 --> 0:33:02.560
<v Speaker 1>together roughly the way you can fit continents together, you know,

0:33:02.600 --> 0:33:05.040
<v Speaker 1>like you can think of the mega continent breaks into

0:33:05.080 --> 0:33:07.360
<v Speaker 1>little continents and now they're a little different, but the

0:33:07.400 --> 0:33:09.800
<v Speaker 1>contours sort of match, and so you can think about

0:33:09.840 --> 0:33:13.760
<v Speaker 1>their history. Right, And this is another example spontaneous symmetry.

0:33:13.760 --> 0:33:17.440
<v Speaker 1>Breaking the Higgs field gives the photon no mass, and

0:33:17.480 --> 0:33:19.720
<v Speaker 1>it gives the ws and z s a lot of mass,

0:33:20.040 --> 0:33:23.160
<v Speaker 1>So all of a sudden, the weak force becomes really

0:33:23.160 --> 0:33:26.640
<v Speaker 1>really weak. Interesting, and so then that's what kind of

0:33:26.800 --> 0:33:29.320
<v Speaker 1>gives rise to the Higgs field, which is the one

0:33:29.360 --> 0:33:32.080
<v Speaker 1>that gives mass to everything. Yeah, so the Higgs field,

0:33:32.160 --> 0:33:34.719
<v Speaker 1>like all the other field started out really hot. It

0:33:34.800 --> 0:33:37.280
<v Speaker 1>was cooling down and cooling down, and most of the

0:33:37.280 --> 0:33:39.640
<v Speaker 1>other fields they like settled down to zero, but the

0:33:39.720 --> 0:33:42.680
<v Speaker 1>Higgs field got stuck, got stuck at a certain point

0:33:42.680 --> 0:33:44.680
<v Speaker 1>where it couldn't go any lower because it has a

0:33:44.720 --> 0:33:46.560
<v Speaker 1>really weird shape to It's like you know, on the

0:33:46.680 --> 0:33:49.040
<v Speaker 1>edge of a canyon wall. It's got a little like

0:33:49.400 --> 0:33:51.240
<v Speaker 1>dip in it, so you can get stuck in a

0:33:51.240 --> 0:33:54.240
<v Speaker 1>little like on the precipice, like a little buzz right,

0:33:54.720 --> 0:33:57.120
<v Speaker 1>And it got stuck there. And because it got stuck

0:33:57.160 --> 0:34:00.040
<v Speaker 1>there and not somewhere else, it gave mass to the

0:34:00.240 --> 0:34:02.680
<v Speaker 1>ws and disease, but not the photon and also to

0:34:02.760 --> 0:34:05.360
<v Speaker 1>the other part of it. So all the other particles

0:34:05.520 --> 0:34:08.160
<v Speaker 1>their mass then gets fixed because the Higgs field got

0:34:08.160 --> 0:34:10.719
<v Speaker 1>stuck at this value. And before so before that we

0:34:10.760 --> 0:34:13.640
<v Speaker 1>didn't have mass, or we just didn't have like consistent mass,

0:34:13.760 --> 0:34:16.080
<v Speaker 1>or you can't even talk about mass. It's harder to

0:34:16.120 --> 0:34:18.880
<v Speaker 1>talk about mass before. The particles really are like separate,

0:34:18.920 --> 0:34:22.120
<v Speaker 1>identifiable spots. But the mass of the particles depends on

0:34:22.160 --> 0:34:24.520
<v Speaker 1>the energy of the Higgs field. So as the universe

0:34:24.600 --> 0:34:26.600
<v Speaker 1>is cooling down and the Higgs field is cooling down,

0:34:26.680 --> 0:34:28.719
<v Speaker 1>you can think of it as like the masses of

0:34:28.719 --> 0:34:31.800
<v Speaker 1>the particles are decreasing because the Higgs field is cooling down.

0:34:32.880 --> 0:34:35.760
<v Speaker 1>All right, So now all of our forces are in motion.

0:34:35.800 --> 0:34:39.719
<v Speaker 1>Now they're in play, and particles now exist, which is

0:34:39.760 --> 0:34:43.680
<v Speaker 1>crazy to think about that. We didn't have particles before. Yeah,

0:34:43.800 --> 0:34:45.880
<v Speaker 1>and now they have mass or they interact with the

0:34:45.920 --> 0:34:49.120
<v Speaker 1>Higgs field, and and so is that then? Kind of

0:34:49.360 --> 0:34:51.640
<v Speaker 1>is that it like is it a straight line from

0:34:51.680 --> 0:34:54.040
<v Speaker 1>there to here? Or are there there still things we

0:34:54.080 --> 0:34:55.960
<v Speaker 1>don't know. There's a lot of things we don't know,

0:34:56.040 --> 0:34:57.840
<v Speaker 1>but it's basically a straight line. I mean, now you

0:34:57.840 --> 0:35:00.440
<v Speaker 1>have particles, and the interactions in play are the ones

0:35:00.480 --> 0:35:03.880
<v Speaker 1>we're familiar with. There's electromagnetic fields, the weak force, the

0:35:03.960 --> 0:35:06.720
<v Speaker 1>strong force, there's gravity. But you know, it's still pretty

0:35:06.760 --> 0:35:09.719
<v Speaker 1>hard to understand, Like it's a hot, dense and nasty mess.

0:35:09.719 --> 0:35:13.000
<v Speaker 1>Like it's mostly quarks and leftons, but they are too

0:35:13.040 --> 0:35:15.160
<v Speaker 1>hot to form any larger particles, Like you don't have

0:35:15.400 --> 0:35:18.400
<v Speaker 1>protons and neutrons and stuff like that, which are bound

0:35:18.440 --> 0:35:23.799
<v Speaker 1>states books just quarks quarks and flying around annihilating each other,

0:35:23.840 --> 0:35:27.479
<v Speaker 1>constantly turning into photons, turning back into particles. It's still

0:35:27.600 --> 0:35:30.359
<v Speaker 1>hot and dense, and then things are cooling off, so

0:35:30.480 --> 0:35:33.839
<v Speaker 1>like you know about after one micro second you get

0:35:33.840 --> 0:35:36.560
<v Speaker 1>this cork glue on plasma. Things start to cool off,

0:35:36.600 --> 0:35:39.240
<v Speaker 1>and then you get things like protons and neutrons and whatever.

0:35:39.640 --> 0:35:42.400
<v Speaker 1>And there's a really interesting mystery there about like what

0:35:42.600 --> 0:35:46.360
<v Speaker 1>happened to all the anti matter. If everything was symmetric,

0:35:46.400 --> 0:35:48.399
<v Speaker 1>you would expect the fields to create like as much

0:35:48.440 --> 0:35:51.640
<v Speaker 1>matter and antimatter should all annihilate into a universe filled

0:35:51.680 --> 0:35:54.719
<v Speaker 1>with light. But instead there was some asymmetry there. We

0:35:54.800 --> 0:35:57.719
<v Speaker 1>ended up with like a little bit more matter than antimatter.

0:35:57.840 --> 0:35:59.759
<v Speaker 1>Most of it is gone, but a little bit of

0:35:59.760 --> 0:36:01.960
<v Speaker 1>matter or was left, and that's what led in a

0:36:02.000 --> 0:36:04.560
<v Speaker 1>straight line to where we are today. I think the

0:36:04.640 --> 0:36:06.560
<v Speaker 1>lesson here is a lot happened in the first two

0:36:06.600 --> 0:36:10.959
<v Speaker 1>hundred microseconds. We missed the big party. I just feel

0:36:11.000 --> 0:36:14.200
<v Speaker 1>like we went through an hour of just to cover

0:36:14.200 --> 0:36:17.440
<v Speaker 1>a two d microseconds. That's amazing, So a lot happened, right,

0:36:17.520 --> 0:36:19.920
<v Speaker 1>and a lot could have happened. Yeah, the history of

0:36:19.920 --> 0:36:23.080
<v Speaker 1>the universe has been pretty boring ever since. You know,

0:36:23.160 --> 0:36:25.440
<v Speaker 1>like most of the excitement was in the first few

0:36:25.560 --> 0:36:29.440
<v Speaker 1>tiny slices of time, and ever since then it's been

0:36:29.440 --> 0:36:32.120
<v Speaker 1>pretty slow. But you know, think about it, like on

0:36:32.200 --> 0:36:36.160
<v Speaker 1>the cosmic time scale, like trillions and quadrillions of years,

0:36:36.640 --> 0:36:41.280
<v Speaker 1>it could be that, you know, intelligent species in septillion years.

0:36:41.560 --> 0:36:44.040
<v Speaker 1>Think about the first few billion years of the universe

0:36:44.120 --> 0:36:47.360
<v Speaker 1>as like, you know, the first moments, because you know,

0:36:47.440 --> 0:36:49.600
<v Speaker 1>it could be that the universe is very different in

0:36:49.600 --> 0:36:52.480
<v Speaker 1>a trillion years, that it's all just black holes separated

0:36:52.520 --> 0:36:55.759
<v Speaker 1>by vast distances or something else forms. You know, there's

0:36:55.760 --> 0:37:00.000
<v Speaker 1>so many fascinating emergent phenomena they're really hard to anticipate,

0:37:00.600 --> 0:37:03.719
<v Speaker 1>and so you know, maybe this will seem exciting to

0:37:03.760 --> 0:37:06.560
<v Speaker 1>people who come much much later. Yeah, I'm sure they'll say, like,

0:37:06.640 --> 0:37:08.680
<v Speaker 1>you know, that day where they post the two hundred

0:37:08.719 --> 0:37:11.320
<v Speaker 1>episode of Daniel and Horge Explained the Universe, that's the

0:37:11.480 --> 0:37:15.400
<v Speaker 1>equal zero to us. That's when that's when the party

0:37:15.440 --> 0:37:19.440
<v Speaker 1>really started. Before then, it's not even really worth there,

0:37:21.320 --> 0:37:23.560
<v Speaker 1>all right, Well, I think the answer is a lot

0:37:23.600 --> 0:37:26.680
<v Speaker 1>happened in the first two hundred microseconds of the universe,

0:37:26.920 --> 0:37:29.680
<v Speaker 1>which is amazing. All right, we have one more question here.

0:37:30.080 --> 0:37:32.320
<v Speaker 1>I think we might have to talk about it in

0:37:32.360 --> 0:37:36.360
<v Speaker 1>two hundred microseconds, Daniel. But the question is pretty interesting.

0:37:36.640 --> 0:37:39.680
<v Speaker 1>It's something I thought about as we try to brainstorm

0:37:39.719 --> 0:37:42.520
<v Speaker 1>ideas for this episode. But the question is what can

0:37:42.600 --> 0:37:46.319
<v Speaker 1>we find within two hundred light years of Earth? So

0:37:47.239 --> 0:37:48.960
<v Speaker 1>I guess, first of all, how much is two hundred

0:37:49.000 --> 0:37:52.359
<v Speaker 1>light years? Like a few Brazilian kilometers? Yeah, a light

0:37:52.440 --> 0:37:55.160
<v Speaker 1>year is really far. So a light year is like

0:37:55.440 --> 0:37:59.919
<v Speaker 1>nine point five times ten to the twelve kilometers. That's

0:38:00.000 --> 0:38:02.400
<v Speaker 1>why we use light years, because the distances in the

0:38:02.480 --> 0:38:05.920
<v Speaker 1>universe are so vast the kilometers become an absurd unity.

0:38:06.000 --> 0:38:09.040
<v Speaker 1>So it's like two hundred million million kilometers. So if

0:38:09.040 --> 0:38:11.120
<v Speaker 1>you could hop in a spaceship and go two hundred

0:38:11.160 --> 0:38:14.920
<v Speaker 1>million million kilometers, where could we go visit? Yeah? So

0:38:15.360 --> 0:38:17.560
<v Speaker 1>mostly the universe is empty. You know, you pick our

0:38:17.640 --> 0:38:21.200
<v Speaker 1>random spot outside the Solar system and you go in

0:38:21.280 --> 0:38:24.360
<v Speaker 1>a straight line, you'll see nothing for two hundred light years. Like,

0:38:24.560 --> 0:38:27.040
<v Speaker 1>it's just not much there. The universe is not very

0:38:27.120 --> 0:38:30.359
<v Speaker 1>dense anymore. And you know, I read these science fiction

0:38:30.400 --> 0:38:33.319
<v Speaker 1>novels about people flying through space and like hitting asteroid

0:38:33.360 --> 0:38:36.120
<v Speaker 1>fields and bumping into stars, and I'm like, it's just

0:38:36.160 --> 0:38:39.120
<v Speaker 1>not that much stuff out there. Likely, No, It's like

0:38:39.160 --> 0:38:42.000
<v Speaker 1>swimming in the ocean. How often do you really encounter

0:38:42.120 --> 0:38:45.399
<v Speaker 1>a desert island? Like? Really not that often? Oh, I see,

0:38:45.400 --> 0:38:47.080
<v Speaker 1>that's a good analogy. Like if you were in the

0:38:47.080 --> 0:38:50.640
<v Speaker 1>middle of the ocean and you went a few hundred kilometers,

0:38:51.040 --> 0:38:53.040
<v Speaker 1>you know, what are the chances that you'll hit another island?

0:38:53.040 --> 0:38:56.239
<v Speaker 1>Pretty small? Yeah, pretty small. It's mostly just ocean out there.

0:38:56.719 --> 0:38:58.960
<v Speaker 1>But there are things out there, and mostly within two

0:38:59.040 --> 0:39:01.240
<v Speaker 1>hundred light years of Earth. There are a bunch of stars,

0:39:01.560 --> 0:39:04.400
<v Speaker 1>but you know, not that close. Like the closest star really,

0:39:04.520 --> 0:39:07.239
<v Speaker 1>once you leave our Solar system, the closest thing that

0:39:07.320 --> 0:39:09.879
<v Speaker 1>you can find to our Solar system is a star

0:39:09.960 --> 0:39:13.560
<v Speaker 1>called Proximus Centauri. It's about four point two light years away.

0:39:13.840 --> 0:39:16.799
<v Speaker 1>It's done the name of an Avengers villain. I feel

0:39:16.840 --> 0:39:19.279
<v Speaker 1>like I've heard that name before. Are you auditioning to

0:39:19.360 --> 0:39:21.239
<v Speaker 1>be in the next Marvel movie? That's what happening here?

0:39:22.239 --> 0:39:24.920
<v Speaker 1>To be the voiceover? I think Proximate can Centauri, the

0:39:24.960 --> 0:39:27.319
<v Speaker 1>Marvel villain can do two hundred accents. So if you

0:39:27.360 --> 0:39:30.879
<v Speaker 1>really want to audition, then we've got to hear some accents. Yeah,

0:39:30.920 --> 0:39:33.080
<v Speaker 1>all right, so that's the nearest star. I guess how

0:39:33.120 --> 0:39:35.359
<v Speaker 1>how many stars can we find within two hundred light years?

0:39:35.440 --> 0:39:38.200
<v Speaker 1>You know, surprisingly, you can find a lot of stars. Now,

0:39:38.400 --> 0:39:41.080
<v Speaker 1>on one hand, stars are not very dense. I mean,

0:39:41.320 --> 0:39:44.920
<v Speaker 1>in our galactic neighborhood, there's about one star per two

0:39:45.080 --> 0:39:49.880
<v Speaker 1>hundred and fifty cubic light years. But as the radius

0:39:49.920 --> 0:39:52.640
<v Speaker 1>of your sphere grows, the volume of it goes up

0:39:52.719 --> 0:39:56.000
<v Speaker 1>very quickly, goes up with radius cubed. So a sphere

0:39:56.080 --> 0:39:59.400
<v Speaker 1>with radius two hundred light years has a lot of

0:39:59.520 --> 0:40:03.080
<v Speaker 1>cubic light years, like thirty million. If you go at

0:40:03.080 --> 0:40:05.319
<v Speaker 1>about two hundred light years, there's something like, you know,

0:40:05.480 --> 0:40:08.960
<v Speaker 1>tens of thousands or maybe a hundred thousand stars in

0:40:09.040 --> 0:40:12.440
<v Speaker 1>that volume. Really, yeah, I could visit a hundred thousand

0:40:12.520 --> 0:40:15.239
<v Speaker 1>stars within two hundred light years. Yes, But you know,

0:40:15.280 --> 0:40:17.719
<v Speaker 1>if you travel in a straight line two hundred years,

0:40:17.760 --> 0:40:20.200
<v Speaker 1>you would probably find very small number of stars. If

0:40:20.239 --> 0:40:25.120
<v Speaker 1>you completely visited a spear with radius two hundred light years,

0:40:25.280 --> 0:40:27.120
<v Speaker 1>would be a hundred thousand stars there. But you know,

0:40:27.200 --> 0:40:30.520
<v Speaker 1>like the list of destinations I can go. Is it's

0:40:30.600 --> 0:40:33.360
<v Speaker 1>like a hundred thousand stars. Yeah, there's a lot of options.

0:40:33.360 --> 0:40:35.760
<v Speaker 1>I mean, if you like decisions and you like choices,

0:40:36.000 --> 0:40:37.840
<v Speaker 1>then there's a lot of options. Most of them are

0:40:37.840 --> 0:40:40.200
<v Speaker 1>pretty far away. I mean, the vast majority of those

0:40:40.280 --> 0:40:43.800
<v Speaker 1>hundred thousand are on a thin shell on the outside

0:40:43.840 --> 0:40:46.040
<v Speaker 1>of that sphere, mostly because that's where most of the

0:40:46.120 --> 0:40:48.799
<v Speaker 1>volume is. But they say that, you know, about one

0:40:48.800 --> 0:40:51.640
<v Speaker 1>in five star has an Earth like planet, So we're

0:40:51.680 --> 0:40:55.480
<v Speaker 1>talking about like there's twenty thousand earthlike planets I could visit. Yeah,

0:40:55.480 --> 0:40:57.319
<v Speaker 1>there are definitely a lot of Earth like planets, and

0:40:57.320 --> 0:41:00.520
<v Speaker 1>we think that most of those solar systems have planets

0:41:00.520 --> 0:41:03.400
<v Speaker 1>like multiple planets, which is fascinating. We don't know a

0:41:03.400 --> 0:41:05.880
<v Speaker 1>lot about like what those solar systems look like, and

0:41:05.880 --> 0:41:08.360
<v Speaker 1>how often do you get big gas giants and rocky

0:41:08.400 --> 0:41:11.680
<v Speaker 1>inner worlds, And is our solar system unusual or totally typical.

0:41:12.120 --> 0:41:14.640
<v Speaker 1>Something that is unusual about our solar system that you'll

0:41:14.680 --> 0:41:18.000
<v Speaker 1>discover as you look around in the solar system is

0:41:18.000 --> 0:41:21.720
<v Speaker 1>how many solar systems have multiple stars. Like in the

0:41:21.760 --> 0:41:25.800
<v Speaker 1>closest fifteen light years is like fifty something stars, and

0:41:25.840 --> 0:41:28.080
<v Speaker 1>about half of them are single stars, just like a

0:41:28.120 --> 0:41:30.880
<v Speaker 1>star with planets around it. But there's like ten of

0:41:30.920 --> 0:41:34.200
<v Speaker 1>them that are binary systems, like two stars orbiting each

0:41:34.200 --> 0:41:37.800
<v Speaker 1>other and then planets around the wo that's common. That's common.

0:41:37.880 --> 0:41:41.640
<v Speaker 1>And even within fifteen light years there are four systems

0:41:41.640 --> 0:41:45.439
<v Speaker 1>that are trinary systems that have three stars in orbit

0:41:45.560 --> 0:41:48.280
<v Speaker 1>around each other. That's pretty cool. So in Star Wars

0:41:48.280 --> 0:41:50.160
<v Speaker 1>when Luke is looking out at the two suns on

0:41:50.239 --> 0:41:53.600
<v Speaker 1>the horizon, that's like maybe more common than you think.

0:41:53.800 --> 0:41:55.960
<v Speaker 1>That's not rare. It's a lot more common than you think.

0:41:56.000 --> 0:41:58.359
<v Speaker 1>And if you think about how things form, you start

0:41:58.400 --> 0:42:00.799
<v Speaker 1>from a big cloud and things cold less, and so

0:42:00.880 --> 0:42:04.120
<v Speaker 1>it's not necessary for its all coalesceent to one really

0:42:04.239 --> 0:42:06.799
<v Speaker 1>big blob in the center of a solar system. If

0:42:06.800 --> 0:42:08.360
<v Speaker 1>you have like a little bit of density here, in

0:42:08.360 --> 0:42:10.600
<v Speaker 1>a little bit of density there, it can form two.

0:42:10.960 --> 0:42:13.200
<v Speaker 1>Or if two stars form close enough to each other,

0:42:13.480 --> 0:42:16.480
<v Speaker 1>they'll pull on each other and form one of these systems.

0:42:16.960 --> 0:42:19.719
<v Speaker 1>Some listeners send me an awesome question recently. He said,

0:42:19.760 --> 0:42:22.239
<v Speaker 1>are there any stars out there that have sort of

0:42:22.320 --> 0:42:26.600
<v Speaker 1>two planetary disks, Like one planetary disc aligned in one

0:42:26.600 --> 0:42:28.560
<v Speaker 1>way and then the second one aligned you know, at

0:42:28.600 --> 0:42:31.880
<v Speaker 1>an angle to it like two hula hoops. Yeah, like

0:42:31.920 --> 0:42:34.600
<v Speaker 1>two hula hoops. And I don't know if one, but

0:42:34.680 --> 0:42:36.960
<v Speaker 1>there's no reason to think there couldn't be. Like if

0:42:37.000 --> 0:42:39.520
<v Speaker 1>you had two solar systems that sort of merged and

0:42:39.600 --> 0:42:41.800
<v Speaker 1>the stars combined in the center, or you get a

0:42:41.800 --> 0:42:44.600
<v Speaker 1>binary star system in the center, they could keep each

0:42:44.600 --> 0:42:47.799
<v Speaker 1>of their planetary disks and it would be at different angles,

0:42:47.880 --> 0:42:49.960
<v Speaker 1>and so that could totally happen. I think that would

0:42:50.000 --> 0:42:52.279
<v Speaker 1>be an awesome setting for a science fiction right, but

0:42:52.480 --> 0:42:54.160
<v Speaker 1>every year you go around the Sun, you'll be like,

0:42:54.280 --> 0:42:56.560
<v Speaker 1>watch out for those other this other planet is would

0:42:56.560 --> 0:43:00.160
<v Speaker 1>be a drama every year. It would have to work

0:43:00.239 --> 0:43:02.839
<v Speaker 1>like clockwork, but it might make for some pretty cool

0:43:02.960 --> 0:43:05.840
<v Speaker 1>nighttime observations. All right, cool, So there's about a hundred

0:43:05.880 --> 0:43:08.239
<v Speaker 1>thousand stars within two hundred light years. What else can

0:43:08.239 --> 0:43:11.719
<v Speaker 1>we find in this bubble? Well, it's mostly it. I

0:43:11.760 --> 0:43:14.799
<v Speaker 1>mean in the galaxy we have stars. Of course, we

0:43:14.880 --> 0:43:18.520
<v Speaker 1>have gas clouds, which are the birthplace of stars, but

0:43:18.560 --> 0:43:20.800
<v Speaker 1>there aren't any of those within two hundred light years.

0:43:20.800 --> 0:43:23.320
<v Speaker 1>Like the closest one is about four hundred and something

0:43:23.400 --> 0:43:26.800
<v Speaker 1>light years away. It's called Taurus, and it's where stars

0:43:26.840 --> 0:43:28.680
<v Speaker 1>are being born. There are stars in there. They're like

0:43:28.800 --> 0:43:31.560
<v Speaker 1>one or two million years old, But we don't have

0:43:31.600 --> 0:43:34.680
<v Speaker 1>any of those big blobs inside our like two hundred

0:43:34.760 --> 0:43:39.680
<v Speaker 1>light year windows, because like a cluster itself is pretty big.

0:43:39.840 --> 0:43:42.000
<v Speaker 1>It's almost as big as two hundred light years. Yeah,

0:43:42.080 --> 0:43:44.200
<v Speaker 1>some of these gas clouds are are hundreds of light

0:43:44.280 --> 0:43:47.760
<v Speaker 1>years across. They're really vast. There's like the birthing regions

0:43:47.760 --> 0:43:51.080
<v Speaker 1>of stars. But there is a cluster of stars. Like

0:43:51.080 --> 0:43:53.320
<v Speaker 1>there's a big major cluster of stars. It's called the

0:43:53.360 --> 0:43:56.759
<v Speaker 1>Hyades cluster, and it's about a hundred and fifty light

0:43:56.800 --> 0:43:59.640
<v Speaker 1>years away. It's like six hundred something million years old,

0:44:00.080 --> 0:44:02.279
<v Speaker 1>and it's just like a big blob of stars that

0:44:02.280 --> 0:44:05.320
<v Speaker 1>are all together. It's probably comes from a really dense

0:44:05.360 --> 0:44:09.160
<v Speaker 1>region of of gas and molecules that got formed early on,

0:44:09.680 --> 0:44:11.920
<v Speaker 1>and so that's like a big blob of stars. So

0:44:12.040 --> 0:44:14.400
<v Speaker 1>I see, oh wow, that must be pretty amazing to

0:44:14.480 --> 0:44:16.800
<v Speaker 1>go near or to visit there. Yeah, And you know,

0:44:16.840 --> 0:44:18.279
<v Speaker 1>if you're looking to visit a lot of stars and a

0:44:18.239 --> 0:44:20.759
<v Speaker 1>a lot of planets at once, it's probably a good destination.

0:44:20.960 --> 0:44:22.880
<v Speaker 1>On the other hand, it's a hundred and fifty light

0:44:22.960 --> 0:44:25.160
<v Speaker 1>years away, so it's to take you a while to

0:44:25.239 --> 0:44:27.200
<v Speaker 1>get there. Well, I think this kind of tells you

0:44:27.239 --> 0:44:30.000
<v Speaker 1>how big the universe is, you know, two hundred light years,

0:44:30.040 --> 0:44:34.239
<v Speaker 1>Like that's even like if we prolong human life and

0:44:34.360 --> 0:44:36.600
<v Speaker 1>double it and was able to go at the speed

0:44:36.640 --> 0:44:38.720
<v Speaker 1>of light, that's as far as like any one person

0:44:38.760 --> 0:44:42.759
<v Speaker 1>could probably go without any kind of special awards beat

0:44:42.840 --> 0:44:45.680
<v Speaker 1>or wormhole, right. Yeah, And you know the thing that's

0:44:45.760 --> 0:44:48.640
<v Speaker 1>furthest away, the human device that's furthest away from the

0:44:48.719 --> 0:44:52.400
<v Speaker 1>Solar system right now is voyage or one. It's traveling

0:44:52.400 --> 0:44:56.080
<v Speaker 1>at sixty one thousand kilometers per hour, and if it

0:44:56.160 --> 0:44:59.520
<v Speaker 1>kept going, it would take another seventy thousand years to

0:44:59.600 --> 0:45:04.200
<v Speaker 1>reach the nearest star. Like, these distances are just incredible,

0:45:05.360 --> 0:45:09.279
<v Speaker 1>and it's already eighteen billion kilometers away from us, but

0:45:09.400 --> 0:45:12.000
<v Speaker 1>that's just like a tiny fraction of the distance to

0:45:12.000 --> 0:45:16.120
<v Speaker 1>approximates centauri. I see, seventy thousand years, that's like what

0:45:16.360 --> 0:45:21.600
<v Speaker 1>three thousand more episodes, Daniel, I got all those ideas. Yeah,

0:45:21.719 --> 0:45:24.840
<v Speaker 1>I've sketched them out already. You would really like to

0:45:24.840 --> 0:45:28.040
<v Speaker 1>work ahead. Yeah, And you know, if you think about

0:45:28.040 --> 0:45:31.520
<v Speaker 1>the larger context you know of our galaxy. Our galaxy

0:45:31.560 --> 0:45:33.760
<v Speaker 1>is a hundred thousand light years across. So a bubble

0:45:33.880 --> 0:45:37.360
<v Speaker 1>two hundred light years is really a tiny neighborhood. You know,

0:45:37.400 --> 0:45:40.640
<v Speaker 1>the Sun itself is just like is twenty something thousand

0:45:40.760 --> 0:45:43.800
<v Speaker 1>light years from the center of the galaxy. So even

0:45:43.840 --> 0:45:46.760
<v Speaker 1>like the most we might right now could imagine traveling

0:45:46.800 --> 0:45:49.719
<v Speaker 1>to for a single human is is a drop in

0:45:49.719 --> 0:45:52.279
<v Speaker 1>the bucket of the size of our galaxy. Yeah, if

0:45:52.320 --> 0:45:54.080
<v Speaker 1>you were looking at a map of the galaxy, you

0:45:54.080 --> 0:45:58.560
<v Speaker 1>wouldn't even notice that distance, right, Wow, alright, Well, I

0:45:58.560 --> 0:46:00.719
<v Speaker 1>feel like we covered a lot in the first two

0:46:01.440 --> 0:46:05.920
<v Speaker 1>seconds this podcast. And uh, we also got this kind

0:46:05.960 --> 0:46:09.440
<v Speaker 1>of amazing view of how big the galaxy is and

0:46:09.600 --> 0:46:12.320
<v Speaker 1>spaces and how empty it is. It's incredible how dense

0:46:12.320 --> 0:46:14.800
<v Speaker 1>and hot the universe used to be and how big

0:46:14.840 --> 0:46:17.800
<v Speaker 1>and cold it is today, and yet it's still filled

0:46:17.840 --> 0:46:20.839
<v Speaker 1>with mystery and our whole concept of the universe, where

0:46:20.880 --> 0:46:23.680
<v Speaker 1>it came from, how it began, what it looks like now,

0:46:23.760 --> 0:46:27.080
<v Speaker 1>what's out there could be totally rocked by discoveries that

0:46:27.120 --> 0:46:30.600
<v Speaker 1>are coming, discoveries made by scientists working today, over by

0:46:30.640 --> 0:46:34.320
<v Speaker 1>somebody out there listening to this podcast right now that's thinking, Hey,

0:46:34.320 --> 0:46:37.160
<v Speaker 1>maybe I could crack one of the biggest questions in

0:46:37.200 --> 0:46:39.799
<v Speaker 1>the universe because you know you could. Yeah, yeah, and

0:46:39.840 --> 0:46:44.440
<v Speaker 1>then we'll cover it here in our episode. That's right,

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<v Speaker 1>And so I want to say a personal thank you

0:46:46.400 --> 0:46:48.920
<v Speaker 1>to all the fans and listeners for tuning into all

0:46:48.920 --> 0:46:51.880
<v Speaker 1>these episodes, for sending us supportive messages, for letting us

0:46:51.920 --> 0:46:54.680
<v Speaker 1>know that you're enjoying what you're hearing, and for sharing

0:46:54.680 --> 0:46:57.440
<v Speaker 1>with us all of your wonder and your curiosity, and

0:46:57.480 --> 0:47:00.319
<v Speaker 1>for going on this crazy journey with us. Absolutely believe

0:47:00.360 --> 0:47:03.120
<v Speaker 1>we wouldn't be doing this without you. And thanks also

0:47:03.239 --> 0:47:05.440
<v Speaker 1>for letting all your friends know and all your context

0:47:05.520 --> 0:47:08.040
<v Speaker 1>note because the more people that are listening, the more

0:47:08.080 --> 0:47:11.719
<v Speaker 1>episodes we can make. All right, well, thanks again for

0:47:11.760 --> 0:47:14.680
<v Speaker 1>helping us celebrate our two hundred episode. We hope you

0:47:14.760 --> 0:47:25.279
<v Speaker 1>enjoyed that. See you next time. Thanks for listening, and

0:47:25.320 --> 0:47:28.040
<v Speaker 1>remember that Daniel and Jorge Explain the Universe is a

0:47:28.120 --> 0:47:31.560
<v Speaker 1>production of I Heart Radio. For more podcast For my

0:47:31.640 --> 0:47:35.239
<v Speaker 1>Heart Radio, visit the I Heart Radio app, Apple Podcasts,

0:47:35.360 --> 0:47:37.720
<v Speaker 1>or wherever you listen to your favorite shows