WEBVTT - Why do stars twinkle?

0:00:08.880 --> 0:00:11.360
<v Speaker 1>Or Hey, do you know the song Twinkle Twinkle Little Star?

0:00:11.800 --> 0:00:14.240
<v Speaker 1>I do? Yeah? Are we taking song requests now on

0:00:14.280 --> 0:00:17.520
<v Speaker 1>the podcast? Now? I'm just trying to see something. How

0:00:17.520 --> 0:00:19.840
<v Speaker 1>about the alphabet song? Is that something you heard as

0:00:19.840 --> 0:00:22.960
<v Speaker 1>a kid. I've heard of the alphabet? Yeah? Do you

0:00:23.000 --> 0:00:25.760
<v Speaker 1>want me to get my guitar? Um? Do you also

0:00:25.800 --> 0:00:28.280
<v Speaker 1>know Bob Bob black Sheep? That one I'm not super

0:00:28.280 --> 0:00:32.040
<v Speaker 1>familiar with, but it's another kid song? Right? Well? Did

0:00:32.080 --> 0:00:36.479
<v Speaker 1>you ever realize these all have exactly the same music?

0:00:36.880 --> 0:00:40.280
<v Speaker 1>What you just blew my mind? Are they all called

0:00:40.320 --> 0:00:44.120
<v Speaker 1>the same like Twinkle Twinkle, Little Alphabet Black Sheep? Yeah?

0:00:44.240 --> 0:00:46.720
<v Speaker 1>They all end with three bags full of twinkling a

0:00:46.800 --> 0:00:51.760
<v Speaker 1>BCS and a bunch of lawsuits, maybe apparently for copyright infringement.

0:01:07.040 --> 0:01:10.280
<v Speaker 1>Hi am r Handy cartoonists and the creator of PhD comics. Hi.

0:01:10.400 --> 0:01:13.280
<v Speaker 1>I'm Daniel. I'm a particle physicist and a professor at

0:01:13.360 --> 0:01:16.440
<v Speaker 1>UC Irvine, And like every other professor, I also play

0:01:16.520 --> 0:01:21.440
<v Speaker 1>the guitar. Is that a requirement for professors? I don't know,

0:01:21.480 --> 0:01:23.240
<v Speaker 1>but I live in a neighborhood of professors, and I

0:01:23.280 --> 0:01:25.600
<v Speaker 1>feel like every single house I go into has a

0:01:25.600 --> 0:01:27.400
<v Speaker 1>guitar on the wall. I don't know if they play

0:01:27.440 --> 0:01:30.039
<v Speaker 1>it or if it's just like a demonstration object, but

0:01:30.080 --> 0:01:32.280
<v Speaker 1>there's lots of guitars in this neighborhood. It's like when

0:01:32.360 --> 0:01:35.040
<v Speaker 1>they were visiting some foreign country. They picked up a

0:01:35.040 --> 0:01:37.759
<v Speaker 1>guitar or something on a field trip or a conference,

0:01:38.040 --> 0:01:41.720
<v Speaker 1>or maybe it's just a conversation piece. Nobody actually plays.

0:01:42.640 --> 0:01:44.600
<v Speaker 1>Are you supposed to play guitar? You just have one

0:01:44.640 --> 0:01:47.360
<v Speaker 1>on your wall right to look cool? You could ask

0:01:47.440 --> 0:01:49.520
<v Speaker 1>something to look cool. I guess if you're a professor.

0:01:49.600 --> 0:01:51.960
<v Speaker 1>But you're quite an accomplished guitar player, aren't you. I

0:01:51.960 --> 0:01:54.040
<v Speaker 1>don't know if I would say accomplished. But I am

0:01:54.080 --> 0:01:56.600
<v Speaker 1>in a band now. Is there anyone else in your band?

0:01:57.440 --> 0:02:01.000
<v Speaker 1>Not a one man band. I'm in a rock band

0:02:01.040 --> 0:02:03.640
<v Speaker 1>with some friends. Oh wow, awesome. Yeah, a bunch of

0:02:03.680 --> 0:02:06.200
<v Speaker 1>middle aged men having a middle age crisis. I've never

0:02:06.240 --> 0:02:10.400
<v Speaker 1>heard of that happening before. That's amazing. We're called the

0:02:10.400 --> 0:02:13.440
<v Speaker 1>Grateful Dad's, so shout out to my band members. But

0:02:13.560 --> 0:02:15.520
<v Speaker 1>I don't think they listen to this podcast. But anyways,

0:02:15.520 --> 0:02:18.040
<v Speaker 1>welcome to our podcast. Daniel and Jorge explained the university

0:02:18.080 --> 0:02:21.160
<v Speaker 1>production of I Heart Radio, in which these two dads

0:02:21.200 --> 0:02:25.080
<v Speaker 1>are grateful for our ability to understand anything out there

0:02:25.160 --> 0:02:28.560
<v Speaker 1>in the universe and dive deep into all of the mysteries,

0:02:28.720 --> 0:02:32.959
<v Speaker 1>the crazy, bonkers weirdness of our universe, the amazing quantum

0:02:32.960 --> 0:02:37.280
<v Speaker 1>frothing foam, the incredible cosmic conundrums, all of the stuff

0:02:37.320 --> 0:02:39.400
<v Speaker 1>that you want to know, the answers to the things

0:02:39.400 --> 0:02:41.760
<v Speaker 1>that frame our existence, that tell us how we got

0:02:41.800 --> 0:02:44.720
<v Speaker 1>here and where the universe is going. We explore all

0:02:44.760 --> 0:02:47.320
<v Speaker 1>of these questions and more. Yeah, because it is a

0:02:47.360 --> 0:02:51.639
<v Speaker 1>pretty amazing and incredible universe, full of exciting and crazy

0:02:51.720 --> 0:02:53.720
<v Speaker 1>things happening, all at the same time as a lot

0:02:53.720 --> 0:02:56.680
<v Speaker 1>of sleepy things happening, a lot of interesting tunes to

0:02:56.760 --> 0:02:59.959
<v Speaker 1>putudiou sleep. I was wondering what you were talking about there,

0:03:00.240 --> 0:03:02.840
<v Speaker 1>sleepy things happening. It was like a rhel We're losing him.

0:03:02.880 --> 0:03:05.880
<v Speaker 1>Is he falling asleep over there? I don't think Twinkle Twinkle,

0:03:05.880 --> 0:03:07.840
<v Speaker 1>Little Star is supposed to put anybody to sleep? Is it?

0:03:07.840 --> 0:03:10.400
<v Speaker 1>It's in it a bedtime song? Oh maybe not. Maybe

0:03:10.440 --> 0:03:13.040
<v Speaker 1>I didn't grow up here, so these were not songs

0:03:13.040 --> 0:03:14.880
<v Speaker 1>that I was sunk to. I think it's more of

0:03:14.919 --> 0:03:17.520
<v Speaker 1>a campfire song. You're sitting there out in nature, looking

0:03:17.560 --> 0:03:20.120
<v Speaker 1>up at the stars and wondering, you know, what they are.

0:03:20.200 --> 0:03:23.280
<v Speaker 1>It's one of the oldest questions humans have been asking

0:03:23.320 --> 0:03:26.240
<v Speaker 1>about the nature of the cosmos. What is out there?

0:03:26.280 --> 0:03:28.840
<v Speaker 1>What is sending us those beams of light? Yeah, it's

0:03:28.880 --> 0:03:32.080
<v Speaker 1>pretty incredible to think that, you know, the earliest humans

0:03:32.160 --> 0:03:34.240
<v Speaker 1>were looking up at the same sky we were, and

0:03:34.280 --> 0:03:36.880
<v Speaker 1>they were probably asking themselves the same questions, like what

0:03:37.080 --> 0:03:39.480
<v Speaker 1>is that Chinese little dought there? And how far away

0:03:39.520 --> 0:03:42.040
<v Speaker 1>is it exactly? And how many quarks are inside the

0:03:42.080 --> 0:03:44.240
<v Speaker 1>heart of a neutron star. I think that's the question

0:03:44.280 --> 0:03:47.720
<v Speaker 1>people have been asking for thousands of years, right if

0:03:47.760 --> 0:03:50.280
<v Speaker 1>they were pretty smart. Cavement, I guess Warren Cavement the

0:03:50.280 --> 0:03:55.040
<v Speaker 1>original particle colliders getting rocks together exactly me makes smaller rocks.

0:03:55.320 --> 0:03:57.680
<v Speaker 1>But it's true, it's an age old question, and there's

0:03:57.680 --> 0:04:00.880
<v Speaker 1>a grand cosmic scale to these questions, because those photons

0:04:01.160 --> 0:04:05.400
<v Speaker 1>departed those stars millions of years or billions of years

0:04:05.440 --> 0:04:09.160
<v Speaker 1>before even cavemen evolved. Yeah, definitely, starts have been around

0:04:09.200 --> 0:04:13.000
<v Speaker 1>for billions, maybe trillions of years, way before people were

0:04:13.000 --> 0:04:15.080
<v Speaker 1>looking at them, and they've been sending their light to

0:04:15.280 --> 0:04:17.360
<v Speaker 1>us for all that time. And some of that light

0:04:17.440 --> 0:04:19.920
<v Speaker 1>is just now getting to us right now, And it's

0:04:19.960 --> 0:04:23.360
<v Speaker 1>incredible to think about how that light actually arrives here.

0:04:23.680 --> 0:04:26.880
<v Speaker 1>A tiny little photon emitted by a star billions and

0:04:26.960 --> 0:04:30.680
<v Speaker 1>billions of miles away, has to fly through an incredible

0:04:30.720 --> 0:04:34.000
<v Speaker 1>amount of universe, dodging all sorts of kinds of stuff

0:04:34.040 --> 0:04:37.880
<v Speaker 1>just to land in your eyeball. It's an incredible journey,

0:04:37.880 --> 0:04:39.720
<v Speaker 1>and frankly, it's amazing to me that any of the

0:04:39.760 --> 0:04:42.280
<v Speaker 1>photons survive it. Yeah, I mean, who knows what that

0:04:42.400 --> 0:04:44.719
<v Speaker 1>photon has been through, right Like it could have maybe

0:04:44.760 --> 0:04:48.040
<v Speaker 1>gone around a black hole or barely dodged an asteroid

0:04:48.120 --> 0:04:50.280
<v Speaker 1>or a comment, you know, made it through an atmosphere,

0:04:50.400 --> 0:04:53.479
<v Speaker 1>dodge all those bolly kills of air in our atmosphere,

0:04:53.600 --> 0:04:55.760
<v Speaker 1>and just to go into your eyeball, or just to

0:04:55.839 --> 0:04:58.159
<v Speaker 1>hit a rock, and nobody even observes it. That's the

0:04:58.200 --> 0:05:01.679
<v Speaker 1>thing that frustrates me. How many photons carrying tiny little

0:05:01.680 --> 0:05:05.400
<v Speaker 1>clues about the universe just go totally unobserved. They fade

0:05:05.400 --> 0:05:08.600
<v Speaker 1>away like an old rock star. They're like little presents

0:05:08.640 --> 0:05:11.400
<v Speaker 1>that nobody unwraps. You know, each one has a clue

0:05:11.400 --> 0:05:13.159
<v Speaker 1>about the kind of star that it came from, the

0:05:13.240 --> 0:05:15.400
<v Speaker 1>history of that star what was going on in that

0:05:15.440 --> 0:05:18.480
<v Speaker 1>star at that moment, and then just boom, nobody gathers

0:05:18.480 --> 0:05:21.080
<v Speaker 1>and it just goes like splat on the sidewalk. Yeah,

0:05:21.160 --> 0:05:23.840
<v Speaker 1>it's pretty cool to think that every star you see,

0:05:23.880 --> 0:05:26.280
<v Speaker 1>I mean it was generated by a whole sun, right,

0:05:26.400 --> 0:05:30.719
<v Speaker 1>basically a giant ball of of fusion powered fire that

0:05:30.880 --> 0:05:33.040
<v Speaker 1>was shooting photons in every direction, and some of them

0:05:33.120 --> 0:05:35.279
<v Speaker 1>make it out to here. It gives you a sense

0:05:35.279 --> 0:05:38.760
<v Speaker 1>for the incredible size and brightness of these stars that

0:05:38.839 --> 0:05:41.360
<v Speaker 1>you can see them from so far away. Imagine if

0:05:41.400 --> 0:05:44.680
<v Speaker 1>your friend in Los Angeles had a flashlight that you

0:05:44.720 --> 0:05:47.160
<v Speaker 1>could see in New York, you would think, oh my gosh,

0:05:47.160 --> 0:05:50.760
<v Speaker 1>that must be a crazy, crazy bright flashlight. Right. Well,

0:05:50.760 --> 0:05:53.920
<v Speaker 1>these stars are so much further away, and yet you

0:05:53.960 --> 0:05:57.159
<v Speaker 1>can see them with your naked eyes. It's incredible that

0:05:57.240 --> 0:05:59.760
<v Speaker 1>these photons make it over this distance. I feel like

0:05:59.800 --> 0:06:02.640
<v Speaker 1>something I realized only recently was the fact that the

0:06:02.680 --> 0:06:05.400
<v Speaker 1>reason why stars looked like little pin points in the sky.

0:06:05.560 --> 0:06:08.039
<v Speaker 1>It's not that they are pinpoints, or it's not that

0:06:08.080 --> 0:06:10.160
<v Speaker 1>the sun is so far away that the sun keeps

0:06:10.160 --> 0:06:12.599
<v Speaker 1>getting smaller as it goes away. It's it's it's literally

0:06:12.720 --> 0:06:16.480
<v Speaker 1>just like one photo receptor in my eyeball getting activated

0:06:16.640 --> 0:06:19.520
<v Speaker 1>by one photon. You're saying that stars are like single

0:06:19.640 --> 0:06:23.960
<v Speaker 1>eye pixels in your mind basically, right, Yeah, they're just well,

0:06:24.120 --> 0:06:25.599
<v Speaker 1>what I think of as a star, or what I

0:06:25.640 --> 0:06:27.799
<v Speaker 1>see as a star is really just one eye pixel,

0:06:27.960 --> 0:06:30.520
<v Speaker 1>right like, Like it doesn't really tell me anything about

0:06:30.560 --> 0:06:32.680
<v Speaker 1>its shape or size. Yeah, it's fascinating to think about

0:06:32.680 --> 0:06:35.320
<v Speaker 1>how photons spread out from that star and then sort

0:06:35.320 --> 0:06:37.880
<v Speaker 1>of get more and more distant from their neighbors. And

0:06:37.920 --> 0:06:39.880
<v Speaker 1>to see a star that's really far away, you only

0:06:39.920 --> 0:06:43.039
<v Speaker 1>really just need one photon, And even if that photon

0:06:43.160 --> 0:06:45.760
<v Speaker 1>was created with billions of other photons really near it,

0:06:45.960 --> 0:06:48.359
<v Speaker 1>they all shoot out at slightly different angles, and so

0:06:48.480 --> 0:06:51.479
<v Speaker 1>by the time they arrives on Earth, it's basically alone.

0:06:51.520 --> 0:06:54.520
<v Speaker 1>It's the only photon that came from that star. Of course,

0:06:54.680 --> 0:06:56.680
<v Speaker 1>there are more coming behind it, but that's why the

0:06:56.720 --> 0:06:59.560
<v Speaker 1>stars seem much dimmer, of course, the further way they are,

0:06:59.600 --> 0:07:01.839
<v Speaker 1>because the photons are now spread out over a much

0:07:02.040 --> 0:07:05.039
<v Speaker 1>larger area, and so only a single cone in your

0:07:05.040 --> 0:07:07.840
<v Speaker 1>eye might register a photon from that star. Yeah, it

0:07:07.880 --> 0:07:09.679
<v Speaker 1>kind of makes you wonder like if we had bigger

0:07:09.720 --> 0:07:12.080
<v Speaker 1>photo receptors in our eyeballs, you know, like if our

0:07:12.080 --> 0:07:15.120
<v Speaker 1>pixels were bigger, the stars would look bigger, right, And

0:07:15.160 --> 0:07:17.560
<v Speaker 1>if they were smaller they would look like smaller pinpoints.

0:07:17.680 --> 0:07:19.960
<v Speaker 1>I suppose if they were smaller, eventually we could even

0:07:20.000 --> 0:07:23.480
<v Speaker 1>resolve the size and the shape of the stars. You think,

0:07:23.520 --> 0:07:26.480
<v Speaker 1>so eventually eventually, right, because there is that information there.

0:07:26.520 --> 0:07:28.160
<v Speaker 1>I mean, if you have a large enough telescope for

0:07:28.200 --> 0:07:31.360
<v Speaker 1>close enough stars, you can definitely resolve the size of

0:07:31.400 --> 0:07:33.520
<v Speaker 1>the star. You think, maybe like a hawk can see

0:07:33.560 --> 0:07:36.960
<v Speaker 1>the somehow, the contours of Alpha Centauri or something, or

0:07:36.960 --> 0:07:40.480
<v Speaker 1>the Sagittarius. We shouldn't be inviting eagles to astronomy conferences

0:07:40.520 --> 0:07:42.920
<v Speaker 1>for sure, Yeah, or at least on the podcast. I

0:07:42.960 --> 0:07:44.880
<v Speaker 1>have questions for them. I want to interview the first

0:07:44.920 --> 0:07:46.760
<v Speaker 1>hawks astronomer. Now I hear they're just a bunch of

0:07:48.200 --> 0:07:50.080
<v Speaker 1>ye astronomy is for the birds. But I hear that

0:07:50.120 --> 0:07:53.680
<v Speaker 1>have a lot of feathers in their publishing caps. But anyways,

0:07:53.760 --> 0:07:55.680
<v Speaker 1>it's just it is interesting to look at a star

0:07:55.760 --> 0:07:58.000
<v Speaker 1>in the night sky and see it twinkle, right. It

0:07:58.080 --> 0:08:00.600
<v Speaker 1>kind of makes you wonder, like, why is it twink

0:08:01.000 --> 0:08:03.320
<v Speaker 1>wiz it actually twinkling? Or is it does it just

0:08:03.360 --> 0:08:05.600
<v Speaker 1>look like it's twinkling. Yeah, And this is a question

0:08:05.640 --> 0:08:07.920
<v Speaker 1>that people have been asking for a long long time,

0:08:08.200 --> 0:08:10.360
<v Speaker 1>not just what are the stars, but what is the

0:08:10.400 --> 0:08:13.160
<v Speaker 1>fact that they're twinkling? Tell us about them? Why do

0:08:13.240 --> 0:08:16.080
<v Speaker 1>different stars seem to twinkle different amounts? And it's a

0:08:16.160 --> 0:08:19.200
<v Speaker 1>question with lots of different layers of answers, because it

0:08:19.200 --> 0:08:22.640
<v Speaker 1>turns out there's lots of different reasons that stars can twinkle. Yeah,

0:08:22.720 --> 0:08:24.840
<v Speaker 1>And it's a question that apparently inspired a song a

0:08:24.880 --> 0:08:28.240
<v Speaker 1>long time ago. Three different songs. M have you dug

0:08:28.240 --> 0:08:30.600
<v Speaker 1>into it? Which one came first, Twinkle Twinkle, Little Star

0:08:30.760 --> 0:08:33.360
<v Speaker 1>or the ABC song. Yeah. Actually, turns out the song

0:08:33.480 --> 0:08:37.920
<v Speaker 1>for Twinkle Twinkle is derived from something composed by Mozart,

0:08:38.120 --> 0:08:41.720
<v Speaker 1>which is inspired by something even earlier, And then later

0:08:42.080 --> 0:08:45.040
<v Speaker 1>an American music publisher adapted the tune to fit the

0:08:45.080 --> 0:08:47.560
<v Speaker 1>alphabet song. So Twinkle Twinkle came first, and then the

0:08:47.600 --> 0:08:50.840
<v Speaker 1>alphabet Interesting, but even Twinkle Twinkle was based on something else.

0:08:50.960 --> 0:08:53.680
<v Speaker 1>All music, of course, is inspired by previous music. Right,

0:08:53.720 --> 0:08:56.120
<v Speaker 1>It's all derivative, right, right, We're all made out of

0:08:56.120 --> 0:08:58.520
<v Speaker 1>start us, even the songs about stars. Does your band

0:08:58.520 --> 0:09:02.280
<v Speaker 1>play original music or only cover? So far we're only covers.

0:09:02.320 --> 0:09:05.000
<v Speaker 1>Yet I say, you got twinkle twinkle, you've got Bob Bob,

0:09:05.000 --> 0:09:08.120
<v Speaker 1>black Sheep, you've got the alphabet song. A huge variety,

0:09:08.720 --> 0:09:11.960
<v Speaker 1>that's right. We cover everything from back to Pink Floyd.

0:09:12.160 --> 0:09:14.439
<v Speaker 1>But anyways, this is an interesting question, and so today

0:09:14.440 --> 0:09:24.280
<v Speaker 1>on the podcast, we'll be asking what makes a star twinkle? Twinkle? Right,

0:09:24.280 --> 0:09:27.400
<v Speaker 1>not tinkle. It's not that kind of podcast. We don't

0:09:27.400 --> 0:09:32.280
<v Speaker 1>ask stars about their personal habits, about their bodily functions.

0:09:32.559 --> 0:09:35.360
<v Speaker 1>We do sort of ask a lot about how the

0:09:35.440 --> 0:09:38.240
<v Speaker 1>insights of stars all right, and and the gases that

0:09:38.400 --> 0:09:40.240
<v Speaker 1>erupt from it. And that's true when you talk about

0:09:40.280 --> 0:09:42.880
<v Speaker 1>the waste products of stars and how they can be

0:09:43.000 --> 0:09:46.760
<v Speaker 1>the compost that nourishes the formation of a future solar system.

0:09:46.760 --> 0:09:48.840
<v Speaker 1>They're all part of the life cycle. Yeah, yeah, it's

0:09:48.880 --> 0:09:51.040
<v Speaker 1>all physics. And so maybe next time we should ask

0:09:51.080 --> 0:09:56.319
<v Speaker 1>what makes its start tinkle? Welcome to our spinoff podcast,

0:09:56.520 --> 0:09:59.360
<v Speaker 1>Inappropriate Physics. But it's a fascinating question. I think a

0:09:59.360 --> 0:10:02.040
<v Speaker 1>lot of people i'd have some sense of the common

0:10:02.080 --> 0:10:04.440
<v Speaker 1>answer to this question, but if you dig deeper, it

0:10:04.440 --> 0:10:07.680
<v Speaker 1>turns out there's lots of different fascinating physics that might

0:10:07.760 --> 0:10:10.120
<v Speaker 1>make stars twinkle. Yeah, it turns out. There's not just

0:10:10.200 --> 0:10:14.280
<v Speaker 1>one reason stars twinkle. There are several reasons. But the

0:10:14.320 --> 0:10:15.880
<v Speaker 1>basic effect is that when you look at the star

0:10:15.920 --> 0:10:18.480
<v Speaker 1>in the night sky, it's sort of doesn't look like

0:10:18.520 --> 0:10:22.800
<v Speaker 1>a constant dot, right, or a constant dots shining. It

0:10:22.840 --> 0:10:24.720
<v Speaker 1>looks sort of like it's blinking on and off a

0:10:24.720 --> 0:10:27.079
<v Speaker 1>little bit. Yeah, exactly, stars look a little bit like

0:10:27.120 --> 0:10:30.320
<v Speaker 1>they blink like they're not just like a laser focused

0:10:30.400 --> 0:10:33.160
<v Speaker 1>at your eyeball. Yeah, it's it's it's almost like something

0:10:33.320 --> 0:10:35.679
<v Speaker 1>is turning it on and off a little bit, or

0:10:35.800 --> 0:10:38.280
<v Speaker 1>something is interfering with it, something is getting between you

0:10:38.480 --> 0:10:41.440
<v Speaker 1>and the star. All right, So we'll dig into this

0:10:41.520 --> 0:10:44.000
<v Speaker 1>question what makes its start twinkle? But first we were

0:10:44.000 --> 0:10:45.720
<v Speaker 1>wondering how many people either there have thought about this

0:10:45.840 --> 0:10:49.560
<v Speaker 1>question when they were singing the song or otherwise, And

0:10:49.600 --> 0:10:51.880
<v Speaker 1>so Daniel went out there into the did you go

0:10:51.880 --> 0:10:53.960
<v Speaker 1>into the internet or to the u c I campus

0:10:54.000 --> 0:10:56.439
<v Speaker 1>this time? These are answers from the internet. So thank

0:10:56.520 --> 0:10:59.280
<v Speaker 1>you to everybody who participated. And if you like to

0:10:59.480 --> 0:11:02.240
<v Speaker 1>put your mind to the test for future episodes and

0:11:02.320 --> 0:11:05.360
<v Speaker 1>let people hear what you think about hard physics problems,

0:11:05.440 --> 0:11:08.320
<v Speaker 1>please don't be shy right to us, do questions, add

0:11:08.400 --> 0:11:10.800
<v Speaker 1>Daniel and Jorge dot com. That's right, and you can

0:11:10.800 --> 0:11:14.360
<v Speaker 1>also go visit Daniel. Do you see Irvine right and

0:11:14.480 --> 0:11:16.280
<v Speaker 1>hope to run into him in the middle of campus.

0:11:16.760 --> 0:11:19.160
<v Speaker 1>That's right. I'm on canvas at Easy Irvine. I have

0:11:19.240 --> 0:11:21.720
<v Speaker 1>office hours, so come on stop by to think about

0:11:21.720 --> 0:11:24.120
<v Speaker 1>it for a second. Why do you think stars twinkle?

0:11:24.920 --> 0:11:27.559
<v Speaker 1>Here's what people had say. I don't think stars twinkle.

0:11:28.200 --> 0:11:31.240
<v Speaker 1>I think their photons are disrupted by temperature and pressure

0:11:31.360 --> 0:11:35.199
<v Speaker 1>differentials in our atmosphere, giving us the appearance of twinkling.

0:11:35.280 --> 0:11:38.120
<v Speaker 1>I imagine it's the same phenomenon that one witnesses looking

0:11:38.120 --> 0:11:40.719
<v Speaker 1>over hot asphalt and seeing the horizon winkle. And I

0:11:40.840 --> 0:11:43.320
<v Speaker 1>venture to guess that they don't twinkle when observed from

0:11:43.360 --> 0:11:46.920
<v Speaker 1>the International Space Station. Well, I guess it depends what

0:11:46.960 --> 0:11:49.840
<v Speaker 1>we mean by blink. The first thing that comes to

0:11:49.880 --> 0:11:54.840
<v Speaker 1>mind is if we're observing a star and something moves

0:11:54.880 --> 0:11:58.040
<v Speaker 1>between us and the star, like a planet, it's gonna

0:11:58.240 --> 0:12:01.679
<v Speaker 1>appear to have blink, I guess. But the star itself

0:12:01.760 --> 0:12:04.760
<v Speaker 1>isn't actually doing anything. It's just something's moved in front

0:12:04.800 --> 0:12:07.000
<v Speaker 1>of it, so it looks like something's happened to it.

0:12:07.600 --> 0:12:11.440
<v Speaker 1>I think that might be what the blink is. In general,

0:12:11.600 --> 0:12:17.800
<v Speaker 1>I don't think stars actually blink, but I can envision

0:12:18.920 --> 0:12:24.360
<v Speaker 1>dust clouds were particularly large planets moving between us and

0:12:24.480 --> 0:12:31.320
<v Speaker 1>that star, making them appear to blink or dim significantly.

0:12:32.000 --> 0:12:35.359
<v Speaker 1>It makes us star blink when the stars about to explode,

0:12:35.840 --> 0:12:39.920
<v Speaker 1>that is one. That is one reason the atmosphere makes

0:12:39.920 --> 0:12:44.080
<v Speaker 1>the start blank to right h And then a lot

0:12:44.120 --> 0:12:47.920
<v Speaker 1>of stars are binary pairs actually, and some of them

0:12:47.960 --> 0:12:52.000
<v Speaker 1>I think can be uh rotating around really quick, and

0:12:52.200 --> 0:12:55.199
<v Speaker 1>that would make the star appear like it's blinking. Well,

0:12:55.200 --> 0:12:57.480
<v Speaker 1>I know, the blinking that we see from here on Earth,

0:12:57.880 --> 0:13:00.960
<v Speaker 1>like the twinkling star, that's more to do with our

0:13:01.000 --> 0:13:04.200
<v Speaker 1>atmosphere than the star itself. But I do know that

0:13:04.240 --> 0:13:08.400
<v Speaker 1>stars also blink over the course of weeks and months.

0:13:09.160 --> 0:13:12.120
<v Speaker 1>I know Bill just did recently. I'm not sure what

0:13:12.120 --> 0:13:14.000
<v Speaker 1>the cause was, though, so if I had to guess,

0:13:14.000 --> 0:13:17.080
<v Speaker 1>I would think it would be maybe gas clouds, um

0:13:17.240 --> 0:13:21.040
<v Speaker 1>or even transitting planets. I don't know. I think that

0:13:21.440 --> 0:13:26.320
<v Speaker 1>what makes us start blink maybe some kind of intern

0:13:26.720 --> 0:13:32.400
<v Speaker 1>interference with any object objects that may cross in the

0:13:32.559 --> 0:13:38.440
<v Speaker 1>path between the star and the person who observes the blinking.

0:13:38.880 --> 0:13:41.679
<v Speaker 1>I would say that What makes us star blink is

0:13:41.760 --> 0:13:47.600
<v Speaker 1>the disturbances in the atmosphere, similar to what we see

0:13:47.800 --> 0:13:52.160
<v Speaker 1>when looking at distant street lights. There are um, you know,

0:13:52.280 --> 0:13:56.000
<v Speaker 1>small air currents, pockets of warm and cold air that

0:13:56.040 --> 0:14:00.839
<v Speaker 1>are constantly moving that through refraction, cause distant, tiny light

0:14:00.880 --> 0:14:04.240
<v Speaker 1>sources such as stars to blink when viewed. Although that

0:14:04.320 --> 0:14:08.600
<v Speaker 1>just might be my view as an amateur astronomer. All right,

0:14:08.720 --> 0:14:11.160
<v Speaker 1>people seem to have pretty strong opinions here. I mean

0:14:11.200 --> 0:14:13.280
<v Speaker 1>a few people didn't know, but a lot of people

0:14:13.320 --> 0:14:15.280
<v Speaker 1>seem to think what was going on. Yeah, there's a

0:14:15.280 --> 0:14:18.400
<v Speaker 1>strong vein here of people thinking that stars are interfered

0:14:18.440 --> 0:14:21.000
<v Speaker 1>with by our atmosphere. Yeah. A lot of people said

0:14:21.000 --> 0:14:23.840
<v Speaker 1>that it's not that the stars actually blinked, like at

0:14:23.840 --> 0:14:26.240
<v Speaker 1>the source, like the star itself. It's just that it

0:14:26.360 --> 0:14:28.880
<v Speaker 1>just looks like it's blinking. And that's a fascinating answer

0:14:28.920 --> 0:14:32.240
<v Speaker 1>because it suggests that the photons are like uninterrupted for

0:14:32.440 --> 0:14:36.040
<v Speaker 1>billions and billions of years and then just like micro

0:14:36.240 --> 0:14:39.880
<v Speaker 1>seconds before they hit your eyeball, that's when they get twinkled. Yeah,

0:14:39.920 --> 0:14:41.680
<v Speaker 1>that's what we tell people who come listen to our band.

0:14:41.760 --> 0:14:44.240
<v Speaker 1>That's thought that we sound bad. It's just said you

0:14:44.280 --> 0:14:46.640
<v Speaker 1>know our perfect sounds. Somebody guests distorted it on the

0:14:46.680 --> 0:14:48.200
<v Speaker 1>way to your ear. That's right. That's why you have

0:14:48.280 --> 0:14:50.880
<v Speaker 1>forced them to plug indirectly to your instruments, right, so

0:14:50.920 --> 0:14:54.320
<v Speaker 1>they can hear the adulterated intended version of your music.

0:14:54.480 --> 0:14:58.200
<v Speaker 1>That's right. Yes, the direct neural download. That's the next step. Actually,

0:14:58.200 --> 0:15:00.480
<v Speaker 1>I know somebody with hearing loss and have a new

0:15:00.600 --> 0:15:03.680
<v Speaker 1>kind of hearing aid that allows for a Bluetooth connection

0:15:04.120 --> 0:15:06.520
<v Speaker 1>so that the sound doesn't have to go through the air.

0:15:06.680 --> 0:15:10.440
<v Speaker 1>They can just hear the original unadulterated sound. Wow, that's

0:15:10.520 --> 0:15:13.240
<v Speaker 1>really interesting. I wonder if it sounds better or different. Oh,

0:15:13.280 --> 0:15:15.680
<v Speaker 1>it's much clearer. They can go to presentations, they can

0:15:15.720 --> 0:15:18.560
<v Speaker 1>hear in church. Now, it's much better than just amplifying

0:15:18.560 --> 0:15:20.720
<v Speaker 1>the sound through the air. Sounds great, And that means

0:15:20.760 --> 0:15:23.520
<v Speaker 1>you can also hit the mute button, I imagine at

0:15:23.600 --> 0:15:26.400
<v Speaker 1>church or at a professor lecture, that's right. It probably

0:15:26.440 --> 0:15:28.680
<v Speaker 1>also means that you can hack them and you can

0:15:28.720 --> 0:15:31.200
<v Speaker 1>like pipe in the Grateful Dads or something else. Yeah,

0:15:31.320 --> 0:15:33.880
<v Speaker 1>much better than a professor lecture for sure, especially if

0:15:33.880 --> 0:15:36.760
<v Speaker 1>you're getting it at the source. But anyways, it's there's

0:15:36.840 --> 0:15:38.760
<v Speaker 1>some interesting ideas here. A lot of people say, it's

0:15:38.800 --> 0:15:41.360
<v Speaker 1>not the stars that are actually blinking, it's somehow like

0:15:41.440 --> 0:15:44.480
<v Speaker 1>the atmosphere that's making them blink or somehow making them

0:15:44.480 --> 0:15:46.880
<v Speaker 1>look like they're blinking. So Daniel, maybe step us through.

0:15:47.080 --> 0:15:50.200
<v Speaker 1>What are some of the actual reasons why stars sprinkle? Well,

0:15:50.200 --> 0:15:52.920
<v Speaker 1>our atmosphere is the number one reason. And this is

0:15:52.960 --> 0:15:56.480
<v Speaker 1>basically why we have space telescopes, because it's not a

0:15:56.600 --> 0:15:59.960
<v Speaker 1>very nice to look at distant stars through the atmosphere

0:16:00.160 --> 0:16:03.320
<v Speaker 1>because while the air seems clear to you, it actually

0:16:03.320 --> 0:16:06.640
<v Speaker 1>can make light zig and zag a little bit because

0:16:06.680 --> 0:16:09.960
<v Speaker 1>it's a slightly different temperatures and slightly different densities. And

0:16:09.960 --> 0:16:13.440
<v Speaker 1>that's sort of like looking through glass with impurities in it.

0:16:13.560 --> 0:16:15.920
<v Speaker 1>That's interesting. But I guess like if I look at

0:16:15.960 --> 0:16:19.600
<v Speaker 1>something through a glass or like a hazy glass, it

0:16:19.640 --> 0:16:21.920
<v Speaker 1>doesn't make the light source twinkle, It just makes it

0:16:21.920 --> 0:16:24.440
<v Speaker 1>look dimmer. Well, what a glass does It bends the light, right,

0:16:24.480 --> 0:16:26.320
<v Speaker 1>That's how a lens works. And so if you have

0:16:26.440 --> 0:16:30.080
<v Speaker 1>glass that has like varying densities and varying temperatures in it,

0:16:30.120 --> 0:16:32.560
<v Speaker 1>for example, then it will change the path of that light.

0:16:32.680 --> 0:16:34.440
<v Speaker 1>And so what happens to the photons is they hit

0:16:34.480 --> 0:16:37.360
<v Speaker 1>the atmosphere. Is not that they're like destroyed, is that

0:16:37.400 --> 0:16:40.000
<v Speaker 1>they're just change direction. And so for you to see

0:16:40.000 --> 0:16:42.000
<v Speaker 1>a star, you need like a direct line of sight

0:16:42.080 --> 0:16:44.920
<v Speaker 1>between you and the star. But if some photons are deflected,

0:16:45.160 --> 0:16:47.320
<v Speaker 1>then you don't see them. Those photons might land to

0:16:47.400 --> 0:16:49.880
<v Speaker 1>your left or to your right or somewhere else. They

0:16:49.920 --> 0:16:52.560
<v Speaker 1>still hit the earth, but they're not hitting your eye anymore.

0:16:52.600 --> 0:16:55.080
<v Speaker 1>So to your eye it looks like the star is

0:16:55.120 --> 0:16:58.160
<v Speaker 1>twinkling because the stream of photons is interrupted. Right. But

0:16:58.160 --> 0:16:59.640
<v Speaker 1>but I guess what I mean is that the difference

0:16:59.640 --> 0:17:02.280
<v Speaker 1>between like a glass and the atmosphere is that the

0:17:02.320 --> 0:17:05.760
<v Speaker 1>atmosphere is sort of like always changing. Right, there's wind,

0:17:06.000 --> 0:17:09.280
<v Speaker 1>and there's you know, variations and clouds, and so it's

0:17:09.320 --> 0:17:12.000
<v Speaker 1>it makes the starts twinkle because the air is sort

0:17:12.000 --> 0:17:14.639
<v Speaker 1>of like moving and waving around in front of you,

0:17:15.080 --> 0:17:17.080
<v Speaker 1>whereas it like a glass doesn't. Right, Like a glass

0:17:17.080 --> 0:17:19.280
<v Speaker 1>doesn't make a start twinkle. That's right, a glass wouldn't

0:17:19.280 --> 0:17:21.359
<v Speaker 1>make a start twinkle. It might deflect the path, but

0:17:21.400 --> 0:17:23.199
<v Speaker 1>if you find the right location, you could see a

0:17:23.240 --> 0:17:26.440
<v Speaker 1>constant stream of light flowing through the glass. But as

0:17:26.480 --> 0:17:29.439
<v Speaker 1>you say, air is constantly changing, right, The wind. The

0:17:29.440 --> 0:17:32.760
<v Speaker 1>atmospheric conditions are constantly changing, and so the path of

0:17:32.760 --> 0:17:35.359
<v Speaker 1>a photon through the air is not constant. So if

0:17:35.359 --> 0:17:37.680
<v Speaker 1>you're just standing there with your eyeball in one location,

0:17:37.960 --> 0:17:40.160
<v Speaker 1>you're not going to get all the photons that come

0:17:40.240 --> 0:17:42.560
<v Speaker 1>from that star. Well, it's kind of interesting because the

0:17:42.600 --> 0:17:45.760
<v Speaker 1>atmosphere makes the stars twinkle like it makes the photons

0:17:45.800 --> 0:17:48.200
<v Speaker 1>sometimes reach your eyeball and sometimes not. But you're saying

0:17:48.240 --> 0:17:50.560
<v Speaker 1>that it can also bend the photons, But it doesn't

0:17:50.560 --> 0:17:53.600
<v Speaker 1>make the stars kind of wavy? Does it? Right? In principle,

0:17:53.680 --> 0:17:56.120
<v Speaker 1>it does if you could capture all of those photons,

0:17:56.160 --> 0:17:58.639
<v Speaker 1>like if you had a huge collection device, then you

0:17:58.680 --> 0:18:01.160
<v Speaker 1>would still see the star because as the deflected photons

0:18:01.200 --> 0:18:03.440
<v Speaker 1>would land in your collection device, and then you would

0:18:03.440 --> 0:18:05.920
<v Speaker 1>think the star came from a different place. And so

0:18:06.040 --> 0:18:08.560
<v Speaker 1>because you have a small collection device, just your eyeball,

0:18:08.640 --> 0:18:10.919
<v Speaker 1>you're missing some of those photons, so it looks like

0:18:10.960 --> 0:18:14.200
<v Speaker 1>the star twinkles rather than dances. There's actually another really

0:18:14.240 --> 0:18:17.560
<v Speaker 1>interesting effect called stellar aberration, which means that the stars

0:18:17.560 --> 0:18:20.320
<v Speaker 1>are not actually where they look like they are because

0:18:20.359 --> 0:18:22.800
<v Speaker 1>they have relative velocity to the Earth. So by the

0:18:22.840 --> 0:18:25.399
<v Speaker 1>time the light gets here, the stars have sort of

0:18:25.600 --> 0:18:28.120
<v Speaker 1>moved away from where they appear to be. But that's

0:18:28.119 --> 0:18:29.919
<v Speaker 1>a different thing. It doesn't cause the stars to twinkle,

0:18:30.080 --> 0:18:32.399
<v Speaker 1>just causes them to be somewhere other than where they

0:18:32.440 --> 0:18:35.880
<v Speaker 1>appear to be. I see, that's a different song altogether.

0:18:36.200 --> 0:18:39.880
<v Speaker 1>That's more like a Baba Black stellar aberration. Yeah. Historically

0:18:39.880 --> 0:18:41.960
<v Speaker 1>it is actually really important because it's one clue that

0:18:41.960 --> 0:18:44.520
<v Speaker 1>we use against the either hypothesis. People are trying to

0:18:44.600 --> 0:18:47.320
<v Speaker 1>understand how light propagated through the universe, and they thought

0:18:47.359 --> 0:18:50.040
<v Speaker 1>maybe there's ether, but then Michaelson and Morley showed that

0:18:50.040 --> 0:18:52.280
<v Speaker 1>there couldn't be either. Some people thought, oh, well, maybe

0:18:52.320 --> 0:18:54.880
<v Speaker 1>we are stuck in a blob of ether that travels

0:18:54.880 --> 0:18:57.359
<v Speaker 1>with the Earth, but then we wouldn't have stellar aberration.

0:18:57.600 --> 0:19:00.200
<v Speaker 1>But anyway, back to twinkling stars. Yeah, I think you're

0:19:00.200 --> 0:19:02.159
<v Speaker 1>saying is that the Start is shooting this train of

0:19:02.200 --> 0:19:04.439
<v Speaker 1>photons add us and they're all coming sort of in

0:19:04.480 --> 0:19:07.639
<v Speaker 1>a street line to our eyeballs. But some of them,

0:19:07.680 --> 0:19:09.960
<v Speaker 1>like hit a pocket of hot air and get deflected,

0:19:10.040 --> 0:19:13.119
<v Speaker 1>or they happen to hit a molecule of nitrogen in

0:19:13.160 --> 0:19:15.359
<v Speaker 1>the atmosphere and it doesn't make it out to us.

0:19:15.400 --> 0:19:18.919
<v Speaker 1>And so this train of photons is interrupted, and that

0:19:19.200 --> 0:19:21.040
<v Speaker 1>is making it look like it's turning on and off

0:19:21.080 --> 0:19:23.320
<v Speaker 1>to our eyeballs. That's exactly right. And then if you

0:19:23.359 --> 0:19:26.959
<v Speaker 1>look at something slightly bigger, like a planet, which is closer,

0:19:27.040 --> 0:19:30.160
<v Speaker 1>you're getting multiple streams of photons from that planet. It's

0:19:30.200 --> 0:19:31.840
<v Speaker 1>not so far away that it just looks like a

0:19:31.880 --> 0:19:34.200
<v Speaker 1>point source. It's like a little disc in the sky.

0:19:34.400 --> 0:19:37.200
<v Speaker 1>And so while some of those photons may get scattered

0:19:37.240 --> 0:19:39.560
<v Speaker 1>from one stream, you're pretty much always getting them from

0:19:39.560 --> 0:19:42.200
<v Speaker 1>another stream. And so a planet looks like a little

0:19:42.240 --> 0:19:45.080
<v Speaker 1>hazy because the atmosphere or its edges might wiggle a

0:19:45.119 --> 0:19:47.680
<v Speaker 1>little bit. But a planet doesn't twinkle because it doesn't

0:19:47.680 --> 0:19:51.320
<v Speaker 1>get like all of its streams interrupted at once, unless

0:19:51.320 --> 0:19:54.920
<v Speaker 1>it's maybe like a super cloudy day, right or you know,

0:19:55.080 --> 0:19:57.520
<v Speaker 1>particularly kind of hazy night. Yeah, it could be, you know,

0:19:57.560 --> 0:20:00.320
<v Speaker 1>if something passes between you and the planet, like an

0:20:00.359 --> 0:20:02.520
<v Speaker 1>eagle or something, it can block the view, or if

0:20:02.560 --> 0:20:05.399
<v Speaker 1>it's like a huge blob of gas hot gas somewhere

0:20:05.400 --> 0:20:07.720
<v Speaker 1>in the atmosphere, it could distort it. But twinkling is

0:20:07.760 --> 0:20:09.919
<v Speaker 1>not something you're going to see regularly from a planet

0:20:09.960 --> 0:20:12.320
<v Speaker 1>because it appears larger in the sky, and so it's

0:20:12.359 --> 0:20:14.840
<v Speaker 1>not as often actually interrupted. All right, Well, that's one

0:20:14.840 --> 0:20:17.800
<v Speaker 1>source of twinkling of the stars, and there are others,

0:20:17.920 --> 0:20:20.200
<v Speaker 1>and there's are things we can do to correct that twinkling,

0:20:20.240 --> 0:20:23.480
<v Speaker 1>so we can actually study stars. But let's get into

0:20:23.520 --> 0:20:38.080
<v Speaker 1>that after we take a quick break. All right, we're

0:20:38.119 --> 0:20:41.720
<v Speaker 1>talking about twinkle twinkle, little stars or big stars. I

0:20:41.720 --> 0:20:46.359
<v Speaker 1>guess yeah, technically stars are not little. Some stars are little,

0:20:46.400 --> 0:20:49.360
<v Speaker 1>you know, Neutron stars are only like ten kilometers across.

0:20:49.960 --> 0:20:52.840
<v Speaker 1>That's pretty little by star standards, and some of them

0:20:52.840 --> 0:20:55.919
<v Speaker 1>are enormous. We have an episode about the biggest stars

0:20:55.960 --> 0:20:58.160
<v Speaker 1>in the universe, and some of them are bigger than

0:20:58.200 --> 0:21:00.479
<v Speaker 1>our solar systems. So maybe should be more like twinkle

0:21:00.520 --> 0:21:04.159
<v Speaker 1>twinkle gigantic star. You say it that way, it sounds flattering, like, wow,

0:21:04.200 --> 0:21:09.240
<v Speaker 1>you're swoll star. You've been working out Twinkle twinkle rip star.

0:21:10.920 --> 0:21:13.960
<v Speaker 1>Stars always skip leg day. So we were talking about

0:21:13.960 --> 0:21:16.239
<v Speaker 1>how the twinkling, most of the twinkling, or a lot

0:21:16.240 --> 0:21:17.880
<v Speaker 1>of the twinkling we see of the stars is due

0:21:17.920 --> 0:21:20.600
<v Speaker 1>to our atmosphere, Like we have this kind of hazy

0:21:21.440 --> 0:21:23.840
<v Speaker 1>layer of air and gas around the Earth which is

0:21:23.880 --> 0:21:27.240
<v Speaker 1>constantly moving, maybe has pockets of hot air cold air,

0:21:27.520 --> 0:21:29.719
<v Speaker 1>different you know, clouds and things like that, and so

0:21:29.800 --> 0:21:32.159
<v Speaker 1>that is what a lot of what makes stars twinkle

0:21:32.280 --> 0:21:35.760
<v Speaker 1>because they kind of obscure or interrupt the train of

0:21:35.800 --> 0:21:39.000
<v Speaker 1>photons coming to our eyes from the stars. Yeah, and

0:21:39.040 --> 0:21:42.199
<v Speaker 1>that's a big challenge for ground based astronomy because we

0:21:42.240 --> 0:21:43.680
<v Speaker 1>want to study the star and we want to get

0:21:43.720 --> 0:21:46.320
<v Speaker 1>great resolution. You know, this fuzzes out one star that

0:21:46.400 --> 0:21:48.960
<v Speaker 1>might be next to another one. It makes it harder

0:21:48.960 --> 0:21:53.400
<v Speaker 1>to observe things in space and get really really crisp images. Yeah,

0:21:53.480 --> 0:21:55.800
<v Speaker 1>I guess you know, the way astronomy started is that

0:21:55.840 --> 0:21:58.000
<v Speaker 1>it was pretty good for like basic stuff of of

0:21:58.119 --> 0:22:00.640
<v Speaker 1>star observing. But then as we want to get more

0:22:00.680 --> 0:22:03.480
<v Speaker 1>detailed or you know, look further out than the atmosphere,

0:22:03.520 --> 0:22:06.000
<v Speaker 1>and the twinkling became a problem. Yeah. Well, until recently,

0:22:06.040 --> 0:22:09.000
<v Speaker 1>we couldn't do anything about it. We couldn't avoid the atmosphere. Now,

0:22:09.040 --> 0:22:12.120
<v Speaker 1>of course we have things like space based telescopes, which

0:22:12.119 --> 0:22:15.280
<v Speaker 1>are awesome and it can avoid atmospheric effects. But there

0:22:15.320 --> 0:22:18.800
<v Speaker 1>are limitations on space telescopes, right, They're expensive, they're hard

0:22:18.840 --> 0:22:21.800
<v Speaker 1>to fix, they have to fit within a rocket. Sometimes

0:22:21.840 --> 0:22:23.920
<v Speaker 1>they blow up, and so there's sort of two very

0:22:24.000 --> 0:22:27.879
<v Speaker 1>complementary paths for astronomy, one space based where you get crisp,

0:22:27.920 --> 0:22:31.200
<v Speaker 1>clear pictures, and the other ground based astronomy, where they've

0:22:31.240 --> 0:22:34.040
<v Speaker 1>come up with some really really clever techniques to try

0:22:34.040 --> 0:22:37.280
<v Speaker 1>to overcome some of the atmospheric limitations. Yeah, this is

0:22:37.400 --> 0:22:41.320
<v Speaker 1>called adaptive optics. Like they actually constantly move the mirrors

0:22:41.320 --> 0:22:43.879
<v Speaker 1>to correct for the twinkling. It's totally bonkers and it

0:22:43.960 --> 0:22:46.080
<v Speaker 1>sounds like it would never work, but you're right. They

0:22:46.119 --> 0:22:49.560
<v Speaker 1>have these mirrors that are deformable, meaning you can change

0:22:49.640 --> 0:22:51.960
<v Speaker 1>the shape of the mirror so when the light hits it,

0:22:51.960 --> 0:22:54.000
<v Speaker 1>it bounces off at a different angle. And if you

0:22:54.080 --> 0:22:57.760
<v Speaker 1>know the effect of the atmosphere on your light source,

0:22:58.160 --> 0:23:01.320
<v Speaker 1>then you can calculate in real time how to deform

0:23:01.400 --> 0:23:05.560
<v Speaker 1>your mirror, to undo it, to like enhance, to defog it,

0:23:05.640 --> 0:23:07.720
<v Speaker 1>to de fuzz it. And so they do these on

0:23:07.800 --> 0:23:11.480
<v Speaker 1>really fancy telescopes on like the millisecond time scale. It's

0:23:11.560 --> 0:23:15.680
<v Speaker 1>like constantly varying in small amounts the shape of the mirrors.

0:23:16.119 --> 0:23:18.320
<v Speaker 1>But I guess I'm a little confused now because earlier

0:23:18.359 --> 0:23:20.720
<v Speaker 1>we said that, you know, the twinkling is sort of

0:23:20.760 --> 0:23:24.680
<v Speaker 1>not it's not making the star wavy or fuzzy. It's

0:23:24.720 --> 0:23:28.000
<v Speaker 1>actually just kind of interrupting the stream of photons. So

0:23:28.040 --> 0:23:31.639
<v Speaker 1>how can moving the mirrors correct for photons that didn't

0:23:31.680 --> 0:23:33.159
<v Speaker 1>get to me? Well, it doesn't get to you if

0:23:33.160 --> 0:23:35.440
<v Speaker 1>you have a tiny little collection device like an eyeball.

0:23:35.520 --> 0:23:38.480
<v Speaker 1>But if you have, you know, like a thirty meter telescope,

0:23:38.520 --> 0:23:40.400
<v Speaker 1>then it's more likely that you are going to get

0:23:40.400 --> 0:23:42.480
<v Speaker 1>that photon. And the photon has just been deflected a

0:23:42.520 --> 0:23:44.560
<v Speaker 1>little bit in one direction. And now if you have

0:23:44.680 --> 0:23:48.240
<v Speaker 1>a few objects near each other, then when the atmosphere changes,

0:23:48.280 --> 0:23:50.639
<v Speaker 1>it's changing the path of all those photons, and those

0:23:50.640 --> 0:23:53.959
<v Speaker 1>objects get fussed together instead of getting a clear crisp image.

0:23:54.000 --> 0:23:56.119
<v Speaker 1>So if you change in the shape of your mirror,

0:23:56.160 --> 0:23:58.560
<v Speaker 1>you can sort of undo that and send the photons

0:23:58.600 --> 0:24:01.359
<v Speaker 1>back as if the atmosphere had happened. Oh, I see

0:24:01.400 --> 0:24:03.679
<v Speaker 1>this is for a different song. I guess right, this

0:24:03.720 --> 0:24:08.560
<v Speaker 1>would be for like fuzzy fuzzy Little Star. Yeah, exactly.

0:24:08.560 --> 0:24:10.600
<v Speaker 1>But it's a hard problem to solve, Like, to do this,

0:24:10.680 --> 0:24:13.000
<v Speaker 1>you have to know what the atmosphere has done to

0:24:13.080 --> 0:24:15.280
<v Speaker 1>your photons, and you might wonder like, well, how could

0:24:15.280 --> 0:24:17.960
<v Speaker 1>you possibly know? You're trying to get a crisp image?

0:24:18.000 --> 0:24:20.160
<v Speaker 1>You don't know what the true image should look like,

0:24:20.400 --> 0:24:23.240
<v Speaker 1>so how can you like invert the atmosphere. It's a

0:24:23.280 --> 0:24:26.400
<v Speaker 1>really hard problem. Yeah, and I hear they use lasers

0:24:26.440 --> 0:24:29.000
<v Speaker 1>for that, right, Sometimes they use lasers. What you need,

0:24:29.040 --> 0:24:32.560
<v Speaker 1>ideally is some point source near the thing you're looking

0:24:32.560 --> 0:24:34.879
<v Speaker 1>at where you know what it should look like, like

0:24:34.960 --> 0:24:38.080
<v Speaker 1>something else nearby in the sky, where you know exactly

0:24:38.080 --> 0:24:40.240
<v Speaker 1>how it should look, and that lets you calculate what

0:24:40.280 --> 0:24:42.719
<v Speaker 1>the atmosphere has done to it. You don't always have that,

0:24:42.800 --> 0:24:45.000
<v Speaker 1>because you don't have like something we have a hubble

0:24:45.080 --> 0:24:48.439
<v Speaker 1>image of it nearby your star. So sometimes they use

0:24:48.520 --> 0:24:52.119
<v Speaker 1>lasers and they create these artificial guide stars, Like we

0:24:52.200 --> 0:24:53.879
<v Speaker 1>know what it should look like when you shoot a

0:24:53.960 --> 0:24:56.760
<v Speaker 1>laser into the upper atmosphere to like excite the gases

0:24:57.080 --> 0:24:59.840
<v Speaker 1>and create some emission. We know what that should look like,

0:25:00.040 --> 0:25:02.040
<v Speaker 1>so we can sort of calculate what the atmosphere has

0:25:02.080 --> 0:25:04.720
<v Speaker 1>done to that light and then undo that to the

0:25:04.800 --> 0:25:08.000
<v Speaker 1>light from the stars. I see used the laser or

0:25:08.040 --> 0:25:10.399
<v Speaker 1>the reference like a control and it actually sort of

0:25:10.440 --> 0:25:13.600
<v Speaker 1>tells you what the atmosphere is doing. Out's distorting your image, Yeah,

0:25:13.600 --> 0:25:16.159
<v Speaker 1>it's probing the atmosphere. That's why sometimes you see these

0:25:16.200 --> 0:25:18.879
<v Speaker 1>telescopes with these lasers shooting out at it. It's not

0:25:18.920 --> 0:25:22.080
<v Speaker 1>like we're defending the Earth from aliens or sending messages

0:25:22.200 --> 0:25:25.240
<v Speaker 1>or zapping eagles or anything like that. We're just creating

0:25:25.280 --> 0:25:27.760
<v Speaker 1>a reference image. So we know what the atmosphere has

0:25:27.800 --> 0:25:29.920
<v Speaker 1>done to our star light. All right, Well, that's kind

0:25:29.960 --> 0:25:32.000
<v Speaker 1>of the what the atmosphere is doing. It's doing a

0:25:32.000 --> 0:25:34.359
<v Speaker 1>lot of the twinkling So does that mean that like

0:25:34.400 --> 0:25:37.080
<v Speaker 1>a space telescope like the Hubble or the New James

0:25:37.160 --> 0:25:40.280
<v Speaker 1>Web that's out there in space doesn't get twinkling stars.

0:25:40.320 --> 0:25:42.800
<v Speaker 1>It doesn't get twinkling stars for that reason, right, there's

0:25:42.800 --> 0:25:45.720
<v Speaker 1>no atmosphere up there in space to interfere with the Hubble,

0:25:45.800 --> 0:25:47.960
<v Speaker 1>and that's one reason why it's pictures can be so

0:25:48.040 --> 0:25:51.159
<v Speaker 1>awesome and crisp and clear. So it's definitely an advantage

0:25:51.160 --> 0:25:53.679
<v Speaker 1>of space based telescopes. But when the Hubble looks out

0:25:53.720 --> 0:25:58.080
<v Speaker 1>of stars, it's still sometimes sees their life getting interrupted interesting.

0:25:58.240 --> 0:26:02.200
<v Speaker 1>It still sees twinkling stars, still sees twinkling stars. And

0:26:02.240 --> 0:26:05.479
<v Speaker 1>because we can remove the atmosphere from the explanation, that

0:26:05.520 --> 0:26:08.479
<v Speaker 1>means there must be something else interfering with these stars

0:26:08.640 --> 0:26:12.479
<v Speaker 1>or something else going on at the actual star itself. WHOA,

0:26:13.359 --> 0:26:16.320
<v Speaker 1>So there are other sources of twinkling for a star,

0:26:16.520 --> 0:26:18.399
<v Speaker 1>like even if you get out of the atmosphere, you

0:26:18.480 --> 0:26:21.240
<v Speaker 1>might still see some twinkling. Yeah, and it's totally fascinating.

0:26:21.280 --> 0:26:22.960
<v Speaker 1>There were a lot of articles a few years ago

0:26:23.000 --> 0:26:26.240
<v Speaker 1>about this star called Tabby Star wearing two thousand fifteen.

0:26:26.280 --> 0:26:29.600
<v Speaker 1>Some citizen scientists saw this dimming of this star that

0:26:29.640 --> 0:26:31.800
<v Speaker 1>nobody could explain. And you might remember there were a

0:26:31.800 --> 0:26:33.719
<v Speaker 1>lot of articles written about how like it might be

0:26:33.760 --> 0:26:37.680
<v Speaker 1>an alien dicen sphere, some huge megastructure built to gather

0:26:37.800 --> 0:26:39.800
<v Speaker 1>all of the energy from the star that might be

0:26:39.840 --> 0:26:42.920
<v Speaker 1>explaining why it seemed to be eclipsed. Who did you say?

0:26:42.960 --> 0:26:48.000
<v Speaker 1>A Tabby star like a cat. It's called Tabby's Star.

0:26:48.240 --> 0:26:50.000
<v Speaker 1>I'm not sure if it's named after a person named

0:26:50.040 --> 0:26:53.640
<v Speaker 1>Tabby or a person's cat named Tabby. It's called Tabby Star.

0:26:53.960 --> 0:26:55.520
<v Speaker 1>I feel like if you had the whole zoo here

0:26:56.080 --> 0:27:00.200
<v Speaker 1>talked about black sheep and hawks and now cats. It's

0:27:00.200 --> 0:27:03.680
<v Speaker 1>also sometimes called w t F star, though I won't

0:27:03.720 --> 0:27:09.440
<v Speaker 1>speculate on what that stands for White toroid formation. Yes,

0:27:09.520 --> 0:27:14.720
<v Speaker 1>I'm sure that's what they meant or what the physics

0:27:14.840 --> 0:27:17.159
<v Speaker 1>in Spanish. But it turns out, of course, that it's

0:27:17.200 --> 0:27:20.720
<v Speaker 1>likely not a Dicens swarm. A dicenswarm would block light

0:27:20.760 --> 0:27:23.679
<v Speaker 1>at all wavelengths because it would basically be opaque. But

0:27:23.720 --> 0:27:26.120
<v Speaker 1>the light that's coming from Tabby Star has been interfered

0:27:26.160 --> 0:27:30.200
<v Speaker 1>with in some way that's not consistent across the spectrum,

0:27:30.240 --> 0:27:33.560
<v Speaker 1>like some frequencies of light can penetrate still from Tabby

0:27:33.560 --> 0:27:36.199
<v Speaker 1>Star and other frequencies can't. But we don't have a

0:27:36.240 --> 0:27:39.280
<v Speaker 1>great idea for what it is that's interfering with the light.

0:27:39.520 --> 0:27:41.720
<v Speaker 1>People thought maybe it's a planet that blew up and

0:27:41.760 --> 0:27:44.520
<v Speaker 1>created a big ring of dust, but that's also not

0:27:44.560 --> 0:27:47.160
<v Speaker 1>creating the amount of infrared glowing people would see. It's

0:27:47.160 --> 0:27:50.120
<v Speaker 1>so it's really fascinating when a star twinkles when it dims,

0:27:50.440 --> 0:27:52.840
<v Speaker 1>because it lets us understand what might be going on

0:27:53.080 --> 0:27:55.680
<v Speaker 1>in that star's system. Right. It tells us a little

0:27:55.720 --> 0:28:00.639
<v Speaker 1>bit about its internal body bound movements. Breath. I like

0:28:00.680 --> 0:28:03.400
<v Speaker 1>to think about it. It's like telling us about its neighborhood. Hey,

0:28:03.440 --> 0:28:06.040
<v Speaker 1>what's going on over there, Tabby Star? Who are your friends?

0:28:06.040 --> 0:28:07.800
<v Speaker 1>Who are you hanging out with? Did you blow up

0:28:07.800 --> 0:28:11.240
<v Speaker 1>a planet? All? Right? So you're saying, that's kind of

0:28:11.280 --> 0:28:14.399
<v Speaker 1>one example of of us seeing a star out in

0:28:14.520 --> 0:28:17.720
<v Speaker 1>space sort of changing its brightness, but not due to

0:28:17.760 --> 0:28:20.560
<v Speaker 1>the atmosphere. And people who are interested in exo planets,

0:28:20.560 --> 0:28:22.880
<v Speaker 1>of course, know that seeing the stars light dim by

0:28:22.880 --> 0:28:25.880
<v Speaker 1>a tiny little bit is an excellent way to observe

0:28:25.960 --> 0:28:28.199
<v Speaker 1>exo planets in that star. Right When we get like

0:28:28.240 --> 0:28:31.200
<v Speaker 1>eclipsed by planet that passes in front of the star,

0:28:31.560 --> 0:28:34.040
<v Speaker 1>it can cause a very slight dimming, and if you

0:28:34.080 --> 0:28:37.359
<v Speaker 1>observe that carefully, you can deduce the presence of that

0:28:37.520 --> 0:28:40.520
<v Speaker 1>exo planet. I wouldn't call that exactly twinkling, but it's

0:28:40.520 --> 0:28:43.440
<v Speaker 1>an example of a star getting a small eclipse from

0:28:43.480 --> 0:28:46.840
<v Speaker 1>an exo planet, right, Because these planets, they don't come

0:28:46.880 --> 0:28:49.120
<v Speaker 1>in front of the sun that often, right, like maybe

0:28:49.160 --> 0:28:51.560
<v Speaker 1>every couple of most like a couple of hours, right,

0:28:51.800 --> 0:28:55.440
<v Speaker 1>it could be a slow twinkle, slow twinkle like a twinkle,

0:28:56.080 --> 0:28:58.520
<v Speaker 1>And of course it depends on the exo planet and

0:28:58.560 --> 0:29:00.880
<v Speaker 1>what its orbit is. Sometimes it's once in a hundred

0:29:01.000 --> 0:29:03.800
<v Speaker 1>years it passes around, or maybe it's every few hours.

0:29:03.840 --> 0:29:06.160
<v Speaker 1>If it's zooming around really close to the star, really

0:29:06.200 --> 0:29:08.640
<v Speaker 1>limits our ability to discover this kind of thing. But

0:29:08.760 --> 0:29:12.720
<v Speaker 1>sometimes we see stars with much more dramatic dimming than

0:29:12.720 --> 0:29:16.680
<v Speaker 1>we could ever explain with exoplanets or even dust swarms. Interesting.

0:29:16.720 --> 0:29:19.080
<v Speaker 1>I guess my question is like, how common are these

0:29:19.120 --> 0:29:21.680
<v Speaker 1>other phenomenon? Like if I was out in space in

0:29:21.680 --> 0:29:23.680
<v Speaker 1>my space suit and I looked at the stars, would

0:29:23.720 --> 0:29:25.920
<v Speaker 1>I see the stars twinkling? Or they would they look

0:29:26.000 --> 0:29:29.720
<v Speaker 1>pretty overall, pretty constant to my eyeball, this is pretty unusual.

0:29:29.840 --> 0:29:32.800
<v Speaker 1>Most of the stars are pretty constant. Sometimes there are

0:29:32.840 --> 0:29:35.160
<v Speaker 1>things that interfere with the star light, and that's fascinating

0:29:35.160 --> 0:29:37.960
<v Speaker 1>for astronomers, and there's like a short list of these objects.

0:29:38.160 --> 0:29:40.280
<v Speaker 1>But most of the stars would look pretty bright and

0:29:40.320 --> 0:29:42.400
<v Speaker 1>pretty even if I was out in space. If you're

0:29:42.440 --> 0:29:44.280
<v Speaker 1>out in space, yeah, so if you're observing from the

0:29:44.280 --> 0:29:46.520
<v Speaker 1>I S S or you're living on the Moon, if

0:29:46.520 --> 0:29:49.520
<v Speaker 1>you're flying in Elon Musk's roadster, for example, then the

0:29:49.560 --> 0:29:52.280
<v Speaker 1>stars are going to look pretty clear. Interesting. So the

0:29:52.400 --> 0:29:56.480
<v Speaker 1>song Twinkle Twinkle Little Star kind of doesn't apply in space. Yeah,

0:29:56.520 --> 0:29:58.880
<v Speaker 1>nobody's gonna be selling the galactic rights to that song.

0:29:58.960 --> 0:30:02.320
<v Speaker 1>It's really just the Earth territories or any planet with

0:30:02.480 --> 0:30:06.120
<v Speaker 1>an atmosphere, right, or maybe like if you're in the

0:30:06.160 --> 0:30:09.520
<v Speaker 1>middle of a nebula maybe like a space cloud maybe.

0:30:09.720 --> 0:30:12.240
<v Speaker 1>But there is one star that's really interesting that astronomer

0:30:12.240 --> 0:30:15.040
<v Speaker 1>has been struggling to understand for like ten years. Now.

0:30:15.920 --> 0:30:18.880
<v Speaker 1>What is it. It's a star called vvv w I

0:30:19.080 --> 0:30:23.120
<v Speaker 1>T zero eight and it's in the Sagittarius constellation about

0:30:23.120 --> 0:30:26.720
<v Speaker 1>twenty five thousand light years away. This is a giant star.

0:30:26.880 --> 0:30:29.880
<v Speaker 1>It's like a hundred times the size of the Sun.

0:30:30.680 --> 0:30:33.840
<v Speaker 1>And about ten years ago it seemed to be eclipsed

0:30:34.040 --> 0:30:36.600
<v Speaker 1>and not just slightly dimmed. Its light was reduced by

0:30:36.760 --> 0:30:41.120
<v Speaker 1>nine seven percent. Whoa it like it almost turned off completely.

0:30:41.200 --> 0:30:44.240
<v Speaker 1>It almost turned off exactly. And they've been observing this

0:30:44.280 --> 0:30:46.800
<v Speaker 1>star for like seventeen years since it is the only

0:30:46.840 --> 0:30:50.040
<v Speaker 1>time it ever happened. And it dimmed by nine percent

0:30:50.200 --> 0:30:52.560
<v Speaker 1>for a few hundred days and then came back up

0:30:52.600 --> 0:30:55.480
<v Speaker 1>to full brightness. Wait what in like the space of

0:30:55.800 --> 0:30:58.320
<v Speaker 1>like a few months. Yeah, they watched this star for

0:30:58.480 --> 0:31:01.600
<v Speaker 1>years and nothing happens, and then all of a sudden, boom,

0:31:01.640 --> 0:31:04.200
<v Speaker 1>it's knocked down by a factor of thirty and then

0:31:04.240 --> 0:31:06.960
<v Speaker 1>it stays pretty dark for a few months, and then

0:31:06.960 --> 0:31:10.640
<v Speaker 1>it goes back up to full brightness like all of

0:31:10.720 --> 0:31:13.440
<v Speaker 1>a sudden or was this a gradual thing? It happened

0:31:13.520 --> 0:31:16.000
<v Speaker 1>very quickly once it began, and then it stayed dark

0:31:16.080 --> 0:31:19.080
<v Speaker 1>for months. Right, And so this is fascinating because this

0:31:19.160 --> 0:31:21.520
<v Speaker 1>is a huge star, right, this is not an eclipse

0:31:21.520 --> 0:31:24.760
<v Speaker 1>from a small object. No planet passing in front of

0:31:24.800 --> 0:31:29.680
<v Speaker 1>this giant star could reduce its light by Yeah, that's

0:31:29.680 --> 0:31:33.400
<v Speaker 1>a big twinkle. I guess it's one big twink. Really,

0:31:33.440 --> 0:31:38.160
<v Speaker 1>you know, it made all this torontomer twinkle observing it.

0:31:38.640 --> 0:31:41.320
<v Speaker 1>They were so excited, exactly. And so people are wondering

0:31:41.320 --> 0:31:43.840
<v Speaker 1>what could this thing be and they've done some calculations.

0:31:44.160 --> 0:31:46.200
<v Speaker 1>You know, if this thing is going to eclipse such

0:31:46.240 --> 0:31:48.360
<v Speaker 1>a big star, it has to be huge. It has

0:31:48.400 --> 0:31:51.240
<v Speaker 1>to be. The minimum size of this thing would be

0:31:51.360 --> 0:31:54.720
<v Speaker 1>point to five a U, like a quarter of the

0:31:54.800 --> 0:31:57.760
<v Speaker 1>distance between the Earth and the Sun. We're talking about

0:31:57.800 --> 0:32:01.400
<v Speaker 1>a single object that size with the thing that blocked

0:32:01.400 --> 0:32:04.120
<v Speaker 1>the star. Because you're saying the star is so big,

0:32:04.160 --> 0:32:06.240
<v Speaker 1>it would have to be that something really big to

0:32:06.280 --> 0:32:08.160
<v Speaker 1>block it. But that's only if we assume that the

0:32:08.160 --> 0:32:10.000
<v Speaker 1>thing that blocked it is close to the star, Like

0:32:10.000 --> 0:32:13.200
<v Speaker 1>it could have maybe been something closer that blocked it. Yeah,

0:32:13.200 --> 0:32:15.800
<v Speaker 1>it could have been something in between us and the star, right,

0:32:15.840 --> 0:32:17.840
<v Speaker 1>because you can block an entire star with the tip

0:32:17.880 --> 0:32:19.960
<v Speaker 1>of your finger, which is not a quarter a U

0:32:20.080 --> 0:32:22.520
<v Speaker 1>wide if your finger is really close. But that would

0:32:22.520 --> 0:32:25.200
<v Speaker 1>require like a bunch of just dark objects floating through

0:32:25.240 --> 0:32:27.960
<v Speaker 1>the universe passing between us and these stars. And they

0:32:27.960 --> 0:32:30.160
<v Speaker 1>did a calculation to see, like how many of those

0:32:30.240 --> 0:32:32.640
<v Speaker 1>dark objects would have to be randomly floating around the

0:32:32.680 --> 0:32:34.800
<v Speaker 1>galaxy in order to block stars like this, and it

0:32:34.800 --> 0:32:38.000
<v Speaker 1>would be a huge number. So that's an explanation, but

0:32:38.040 --> 0:32:41.320
<v Speaker 1>it's less likely than some huge object closer to the star,

0:32:41.440 --> 0:32:45.640
<v Speaker 1>some remnant of the stellar formation. But this doesn't happen

0:32:45.680 --> 0:32:48.200
<v Speaker 1>that often, right, does it? This does not happen that often,

0:32:48.280 --> 0:32:51.200
<v Speaker 1>But for it to ever happen, space would basically have

0:32:51.280 --> 0:32:54.560
<v Speaker 1>to be filled with these big dark objects because it's

0:32:54.720 --> 0:32:57.000
<v Speaker 1>very hard to cross the line of side between a

0:32:57.080 --> 0:32:59.760
<v Speaker 1>star and us unless you have a lot of stuff

0:32:59.760 --> 0:33:04.640
<v Speaker 1>out there in space, because space is really, really really big. Interesting,

0:33:04.760 --> 0:33:06.840
<v Speaker 1>So they think it's maybe something in the orbit of

0:33:06.840 --> 0:33:09.160
<v Speaker 1>the star and it's something huge, yeah, but they don't

0:33:09.160 --> 0:33:11.760
<v Speaker 1>really understand it because we don't have models for solar

0:33:11.760 --> 0:33:14.920
<v Speaker 1>system formation that include stuff like this, Like what could

0:33:14.920 --> 0:33:17.680
<v Speaker 1>it be? We have ideas of planets and maybe even

0:33:17.800 --> 0:33:20.680
<v Speaker 1>rings around stars. People have this theory that maybe it's

0:33:20.720 --> 0:33:23.200
<v Speaker 1>like a huge ring with a big blob in it

0:33:23.280 --> 0:33:26.440
<v Speaker 1>that got exploded or torn apart by tidal forces, something

0:33:26.520 --> 0:33:29.720
<v Speaker 1>like a circumstellar disc with a huge object in it,

0:33:29.760 --> 0:33:32.680
<v Speaker 1>but it's much bigger than any model can predict. Interesting,

0:33:32.760 --> 0:33:35.040
<v Speaker 1>Could it be like a giant cloud of something like

0:33:35.040 --> 0:33:37.680
<v Speaker 1>an asteroid cloud? Maybe you certainly could be. And perhaps

0:33:37.760 --> 0:33:41.240
<v Speaker 1>for example, another solar system passed by and lost some

0:33:41.360 --> 0:33:43.440
<v Speaker 1>of its stuff to this solar system, So it could

0:33:43.440 --> 0:33:46.760
<v Speaker 1>be something that happened fairly recently, because these things wouldn't

0:33:46.840 --> 0:33:49.160
<v Speaker 1>last for very long. If you have like a huge

0:33:49.200 --> 0:33:52.200
<v Speaker 1>cloud of stuff in your solar system, eventually gravity is

0:33:52.200 --> 0:33:54.440
<v Speaker 1>going to pull it together after a few million years

0:33:54.520 --> 0:33:57.600
<v Speaker 1>and form it into like a planet or into something else.

0:33:58.080 --> 0:34:00.560
<v Speaker 1>And so like huge clouds of gas and dust around

0:34:00.600 --> 0:34:03.680
<v Speaker 1>the star and to be short lived objects on astronomical

0:34:03.680 --> 0:34:08.160
<v Speaker 1>time scales. WHOA, alright, so that's one, I guess twinkling

0:34:08.280 --> 0:34:12.399
<v Speaker 1>That puzzled scientist. It's it's like a big twinkle that

0:34:12.800 --> 0:34:15.080
<v Speaker 1>caused this one start to twinkle. What are some other

0:34:15.480 --> 0:34:17.920
<v Speaker 1>famous examples of twinkling stars? Yeah, so we have a

0:34:17.920 --> 0:34:20.960
<v Speaker 1>short list of them. There's another one called Epsilon R

0:34:21.040 --> 0:34:25.360
<v Speaker 1>e J, and this one is eclipped every twenty seven

0:34:25.480 --> 0:34:29.040
<v Speaker 1>years by some giant dust cloud which orbits it, and

0:34:29.040 --> 0:34:32.919
<v Speaker 1>it's eclipsed by fifty percent whoa meaning like we see

0:34:32.920 --> 0:34:35.760
<v Speaker 1>the star called Epsilon R J, and it it dims

0:34:35.800 --> 0:34:37.920
<v Speaker 1>every twenty seven years. We've been looking at it that

0:34:38.000 --> 0:34:40.120
<v Speaker 1>long to note to notice this pattern. Yeah, it was

0:34:40.160 --> 0:34:43.879
<v Speaker 1>first observed in eighteen twenty one, so we've been looking

0:34:43.880 --> 0:34:46.000
<v Speaker 1>at this thing for like hundreds of years, which is

0:34:46.000 --> 0:34:48.120
<v Speaker 1>why we have a handle on like a twenty seven

0:34:48.160 --> 0:34:51.760
<v Speaker 1>year cycle. So it's like a twinkle, but in atar

0:34:51.800 --> 0:34:55.240
<v Speaker 1>scale kind of exactly if you fast forward at the universe,

0:34:55.280 --> 0:34:57.960
<v Speaker 1>this one would seem to twinkle. It's like a very

0:34:58.160 --> 0:35:02.319
<v Speaker 1>slow motion tween. You have to play the song one

0:35:02.360 --> 0:35:05.680
<v Speaker 1>note per year exactly, and the dimming here lasts for

0:35:05.760 --> 0:35:09.479
<v Speaker 1>like two years and then it happens every twenty seven years.

0:35:09.480 --> 0:35:12.160
<v Speaker 1>So it's like a giant, slow moving dust cloud. And

0:35:12.239 --> 0:35:14.160
<v Speaker 1>this one we do know what causes. How do we

0:35:14.200 --> 0:35:16.680
<v Speaker 1>know what causes this eclipse? Mostly we can study these

0:35:16.719 --> 0:35:19.160
<v Speaker 1>things by looking at the spectrum, Like we can study

0:35:19.200 --> 0:35:22.120
<v Speaker 1>the kind of light that can penetrate, and that tells

0:35:22.239 --> 0:35:24.799
<v Speaker 1>us why this thing is transparent and why this thing

0:35:24.840 --> 0:35:28.279
<v Speaker 1>is opaque, because remember every object is either transparent or

0:35:28.280 --> 0:35:31.520
<v Speaker 1>opaque to light at different frequencies depending on what it is,

0:35:31.920 --> 0:35:34.880
<v Speaker 1>because the atoms that make things up can only absorb

0:35:35.000 --> 0:35:38.360
<v Speaker 1>photons as specific frequencies. And so by looking at the

0:35:38.440 --> 0:35:41.040
<v Speaker 1>light that passes through, for example, a cloud of gas,

0:35:41.080 --> 0:35:43.920
<v Speaker 1>you can tell, oh, there hydrogen, or there's helium, or

0:35:43.920 --> 0:35:46.680
<v Speaker 1>there's sodium, or it's gas or its dust or whatever.

0:35:46.840 --> 0:35:49.799
<v Speaker 1>You can tell by seeing which frequencies of light are

0:35:49.880 --> 0:35:53.319
<v Speaker 1>filtered out by that object. And so by studying it

0:35:53.320 --> 0:35:55.320
<v Speaker 1>we can tell, oh, this is probably a big cloud

0:35:55.360 --> 0:35:57.840
<v Speaker 1>of dust, and I see like the shade of the

0:35:57.960 --> 0:36:00.279
<v Speaker 1>light that comes through tells you kind of what it

0:36:00.440 --> 0:36:02.800
<v Speaker 1>went through exactly, just like you know, you can throw

0:36:02.880 --> 0:36:05.479
<v Speaker 1>things into flames and they make different colors. That's because

0:36:05.520 --> 0:36:09.520
<v Speaker 1>different elements emit at different frequencies. They also absorb at

0:36:09.560 --> 0:36:12.719
<v Speaker 1>those same frequencies. And so if you shine white light

0:36:12.760 --> 0:36:15.440
<v Speaker 1>through a cloud of random gas, and astronomer can tell

0:36:15.480 --> 0:36:18.720
<v Speaker 1>you what was in that gas based on whether green

0:36:18.880 --> 0:36:21.640
<v Speaker 1>was removed or red was removed, or the infrared was

0:36:21.680 --> 0:36:24.279
<v Speaker 1>removed or something. It's like a fingerprint. All right, that's

0:36:24.280 --> 0:36:28.360
<v Speaker 1>another twinkling star in space. What are some other examples,

0:36:28.560 --> 0:36:30.879
<v Speaker 1>So this is a short list of them. V four

0:36:31.280 --> 0:36:34.759
<v Speaker 1>hundred Centauri, which is also called Mama Jets object is

0:36:34.800 --> 0:36:38.120
<v Speaker 1>also eclipsed by something we don't really understand, but astronomers

0:36:38.160 --> 0:36:41.400
<v Speaker 1>suspect that it's something that's point for a U wide,

0:36:41.520 --> 0:36:44.680
<v Speaker 1>it's an object that's like forty million miles wide. Well,

0:36:44.680 --> 0:36:47.200
<v Speaker 1>it's it's not maybe one objecting it's at that scale.

0:36:47.200 --> 0:36:49.760
<v Speaker 1>It's probably like a cloud of something or a cluster

0:36:49.840 --> 0:36:52.080
<v Speaker 1>of something. Right, Yeah, it's probably like a big cloud

0:36:52.120 --> 0:36:54.880
<v Speaker 1>of gas or dust or a huge rain of rocks. Right,

0:36:54.920 --> 0:36:57.239
<v Speaker 1>it's probably not a single solid object that would big

0:36:57.280 --> 0:36:59.959
<v Speaker 1>because it's like a huge block of iron that big

0:37:00.360 --> 0:37:03.480
<v Speaker 1>and gravitationally will probably collapse into a black hole. All right. Well,

0:37:03.520 --> 0:37:05.920
<v Speaker 1>those are different things that can make a star twinkle

0:37:06.320 --> 0:37:08.920
<v Speaker 1>out in space that is not our atmosphere. But it

0:37:08.920 --> 0:37:11.520
<v Speaker 1>turns out there are other reasons why a star might twinkle,

0:37:11.560 --> 0:37:14.200
<v Speaker 1>and it might have to do with their inner bowel movement.

0:37:14.360 --> 0:37:16.440
<v Speaker 1>So let's get into that. But first let's take another

0:37:16.560 --> 0:37:32.880
<v Speaker 1>quick break. All right, we're talking about twinkling and twinkling stars.

0:37:32.880 --> 0:37:36.800
<v Speaker 1>Both big and little and also bad bla black cheeps

0:37:36.880 --> 0:37:40.120
<v Speaker 1>that might be eclipsing stars out there in space. So

0:37:40.160 --> 0:37:42.040
<v Speaker 1>then we talked about how, like most of the stars

0:37:42.040 --> 0:37:44.080
<v Speaker 1>we see twinkle here on Earth, it's it's because of

0:37:44.080 --> 0:37:47.000
<v Speaker 1>the atmosphere. It's the air around us is making the

0:37:47.120 --> 0:37:49.440
<v Speaker 1>light kind of dim on and off. But you can

0:37:49.440 --> 0:37:51.960
<v Speaker 1>also see a about twinkling in space because there are

0:37:52.000 --> 0:37:54.319
<v Speaker 1>other things in space that might be blocking our view.

0:37:54.440 --> 0:37:55.960
<v Speaker 1>But it turns out that even if you are sort

0:37:55.960 --> 0:37:59.080
<v Speaker 1>of standing next to the star, you might even then

0:37:59.160 --> 0:38:01.560
<v Speaker 1>see a twinkle. This is one of my favorite explanations

0:38:01.560 --> 0:38:04.200
<v Speaker 1>for twinkling stars because it really goes to the heart

0:38:04.280 --> 0:38:07.120
<v Speaker 1>of like your original idea. When you're looking up at

0:38:07.120 --> 0:38:09.120
<v Speaker 1>the night sky and you're looking at the star and

0:38:09.160 --> 0:38:12.360
<v Speaker 1>it's twinkling, you're wondering, like, is it getting brighter and

0:38:12.400 --> 0:38:14.920
<v Speaker 1>dimmer or is the light getting blocked. Well, it turns

0:38:14.920 --> 0:38:18.000
<v Speaker 1>out that stars can actually get brighter and dimmer. That's

0:38:18.040 --> 0:38:20.840
<v Speaker 1>something that a bunch of stars can do. And I

0:38:20.920 --> 0:38:23.600
<v Speaker 1>was surprised to learn that the Sun does this as well.

0:38:23.880 --> 0:38:26.560
<v Speaker 1>The Sun varies its brightness. It's not just like a

0:38:26.600 --> 0:38:30.640
<v Speaker 1>constant stream of photons every year. Wait, what like our sun,

0:38:30.719 --> 0:38:33.520
<v Speaker 1>that the one that provides are daylight is not constant.

0:38:33.520 --> 0:38:37.000
<v Speaker 1>It's twinkling. Also, Yeah, it turns out all stars are variable.

0:38:37.040 --> 0:38:39.160
<v Speaker 1>Some of them are much more variable than others, and

0:38:39.200 --> 0:38:41.719
<v Speaker 1>we'll talk about those, but every single star has some

0:38:42.000 --> 0:38:44.160
<v Speaker 1>variability to it. You know, our sun has like an

0:38:44.160 --> 0:38:47.680
<v Speaker 1>eleven year cycle where something mysterious is going on at

0:38:47.719 --> 0:38:52.080
<v Speaker 1>the heart of this swirling, crazy plasmas with these enormous

0:38:52.120 --> 0:38:55.319
<v Speaker 1>tubes and magnetic fields that flip every eleven years, and

0:38:55.400 --> 0:38:57.880
<v Speaker 1>so the brightness of our sun varies, but only a

0:38:57.880 --> 0:39:01.360
<v Speaker 1>small amount. It's like zero point one percent over the

0:39:01.400 --> 0:39:04.239
<v Speaker 1>eleven year cycle. Well, I meaning like if you took

0:39:04.239 --> 0:39:06.560
<v Speaker 1>a film of the Sun and you fast forward at it,

0:39:07.080 --> 0:39:09.200
<v Speaker 1>you would see it kind of like twinkle, right, you'd

0:39:09.239 --> 0:39:11.640
<v Speaker 1>see it kind of blinking on and off about point

0:39:11.680 --> 0:39:14.080
<v Speaker 1>one percent, but still you might notice it. Yeah, you

0:39:14.120 --> 0:39:16.000
<v Speaker 1>have a good camera, you could definitely detect that, and

0:39:16.040 --> 0:39:18.200
<v Speaker 1>people have and people who study the sun see this

0:39:18.280 --> 0:39:21.040
<v Speaker 1>kind of cycle. You know, there's another longer term trend,

0:39:21.080 --> 0:39:23.760
<v Speaker 1>which is the sun is overall getting brighter and brighter

0:39:24.000 --> 0:39:26.600
<v Speaker 1>as it gets older, and over like a billion years,

0:39:26.640 --> 0:39:29.080
<v Speaker 1>it's going to get maybe ten percent brighter. That's not

0:39:29.160 --> 0:39:31.839
<v Speaker 1>something we can observe with our telescope today. But this

0:39:31.960 --> 0:39:35.200
<v Speaker 1>kind of gentle twinkling is something that the Sun does.

0:39:36.360 --> 0:39:38.640
<v Speaker 1>And then I guess that's because the Sun. I mean,

0:39:38.680 --> 0:39:41.120
<v Speaker 1>it's not like a machine, right, It's like a process.

0:39:41.640 --> 0:39:44.719
<v Speaker 1>It's like a giant nuclear chemical reaction, right, Like there's

0:39:44.719 --> 0:39:47.400
<v Speaker 1>stuff going on inside of it that maybe causes it

0:39:47.400 --> 0:39:51.000
<v Speaker 1>to kind of grow brighter or dimmer. Sometimes you're suggesting

0:39:51.040 --> 0:39:52.759
<v Speaker 1>that if it was a machine, like designed by a

0:39:52.800 --> 0:39:56.440
<v Speaker 1>stellar engineer or something, it would be more reliable. Well,

0:39:56.480 --> 0:40:00.520
<v Speaker 1>all engineers are stars, Daniel. All engineers are stellar. We're

0:40:00.520 --> 0:40:02.960
<v Speaker 1>all stellar engineers. I mean, the Sun has been burning

0:40:03.000 --> 0:40:06.200
<v Speaker 1>for five billion years without a breakdown, so you know,

0:40:06.440 --> 0:40:08.719
<v Speaker 1>I think it's pretty effective. Well, I guess what I

0:40:08.719 --> 0:40:10.359
<v Speaker 1>mean is it's it's a it's kind of like it's

0:40:10.360 --> 0:40:14.240
<v Speaker 1>an organic process, right, Like, it's not perfectly imbalanced. Maybe

0:40:14.320 --> 0:40:16.759
<v Speaker 1>sometimes it gets a little over excited and sometimes a

0:40:16.800 --> 0:40:19.920
<v Speaker 1>little under excited. Yeah, it's a different process than combustion.

0:40:20.000 --> 0:40:21.520
<v Speaker 1>But it's sort of like a fire. You know, it

0:40:21.560 --> 0:40:25.360
<v Speaker 1>has fuel, it keeps burning and that flame fluctuates and

0:40:25.400 --> 0:40:27.960
<v Speaker 1>so it's not like designed or orchestrated in order to

0:40:27.960 --> 0:40:29.799
<v Speaker 1>provide a certain amount of light. It's just a thing

0:40:29.880 --> 0:40:32.319
<v Speaker 1>that is there and does what it's doing, and that

0:40:32.400 --> 0:40:35.480
<v Speaker 1>means that it has cycles because of the internal workings

0:40:35.520 --> 0:40:38.480
<v Speaker 1>of the sun very and it's incredible that it's so

0:40:38.600 --> 0:40:41.600
<v Speaker 1>regular too. It's not something that we understand the source

0:40:41.640 --> 0:40:44.440
<v Speaker 1>of this eleven year cycle for the sun. Well, so

0:40:44.480 --> 0:40:46.960
<v Speaker 1>I wonder, like, if we're a different species of animal

0:40:47.040 --> 0:40:49.040
<v Speaker 1>and we had like a thought process that was a

0:40:49.080 --> 0:40:51.839
<v Speaker 1>lot slower like to us, maybe the sun would look

0:40:51.880 --> 0:40:54.600
<v Speaker 1>like a stroke light almost if we thought about things

0:40:54.640 --> 0:40:56.719
<v Speaker 1>in the scale of like centuries, it would look like

0:40:56.920 --> 0:40:58.799
<v Speaker 1>it was blinking on and off kind of. Yeah, that's

0:40:58.800 --> 0:41:01.759
<v Speaker 1>fun to think about. Or another idea is what if

0:41:01.760 --> 0:41:04.760
<v Speaker 1>we were species that was extraordinarily sensitive is the abount

0:41:04.760 --> 0:41:07.560
<v Speaker 1>of sunlight, so that we could like observe and notice

0:41:07.880 --> 0:41:10.880
<v Speaker 1>this eleven year cycle and it affected our evolution the

0:41:10.920 --> 0:41:13.040
<v Speaker 1>way like the day night cycle and the winters have

0:41:13.080 --> 0:41:15.600
<v Speaker 1>affected the evolution of light on Earth. I'd be interesting

0:41:15.600 --> 0:41:17.720
<v Speaker 1>if you had species that were sensitive to these eleven

0:41:17.800 --> 0:41:21.799
<v Speaker 1>year cycles. Whoa, like, maybe you're sleepier for eleven years

0:41:21.880 --> 0:41:25.040
<v Speaker 1>and then you're less sleepy. Maybe that's why I've been

0:41:25.080 --> 0:41:28.160
<v Speaker 1>late this past eleven years. Yeah, all right, well, then

0:41:28.160 --> 0:41:31.520
<v Speaker 1>how do you explained the previous eleven years? I was

0:41:31.560 --> 0:41:33.560
<v Speaker 1>a lot more on time eleven years ago. Man, I

0:41:33.600 --> 0:41:35.799
<v Speaker 1>believe that I've known you for more than eleven years,

0:41:35.840 --> 0:41:38.759
<v Speaker 1>so I can contest that data. Well, you just don't

0:41:38.800 --> 0:41:41.279
<v Speaker 1>have enough data points. Then you need at least what's

0:41:41.320 --> 0:41:44.000
<v Speaker 1>the mic was frequency that you need at least twice

0:41:44.040 --> 0:41:48.520
<v Speaker 1>the periosity. All right, I'll get back to you intend Yeah, wait,

0:41:48.680 --> 0:41:51.120
<v Speaker 1>wait or other thirty years and then we'll talk about

0:41:51.120 --> 0:41:52.920
<v Speaker 1>my peakers. All right, I'm putting it on my calendar

0:41:53.160 --> 0:41:58.480
<v Speaker 1>series schedule appointment for thirty years from today. But anyways,

0:41:58.520 --> 0:42:00.200
<v Speaker 1>I think what you're saying is that, like, maybe I

0:42:00.239 --> 0:42:02.560
<v Speaker 1>wonder if there are things on Earth that are sensitive

0:42:02.600 --> 0:42:05.120
<v Speaker 1>to that cycle, right, Like, maybe it might affect our

0:42:05.160 --> 0:42:07.680
<v Speaker 1>atmosphere too, Right, every eleven years, maybe things get a

0:42:07.719 --> 0:42:10.200
<v Speaker 1>little bit warmer or colder. Yeah, well, the brightness of

0:42:10.239 --> 0:42:12.839
<v Speaker 1>the sun definitely affects the atmosphere and the climate here

0:42:12.880 --> 0:42:15.479
<v Speaker 1>on Earth, but there are larger effects. The Earth goes

0:42:15.480 --> 0:42:17.880
<v Speaker 1>through these cycles that affect like the ice ages and

0:42:17.960 --> 0:42:21.120
<v Speaker 1>glaciation because the Earth's orbit changes a little bit, and

0:42:21.160 --> 0:42:23.319
<v Speaker 1>the tilt changes a little bit. Is it's tweaked by

0:42:23.360 --> 0:42:26.080
<v Speaker 1>like Jupiter. So I think those effects are larger than

0:42:26.120 --> 0:42:28.520
<v Speaker 1>the variability of the Sun itself. So the Sun is

0:42:28.560 --> 0:42:31.600
<v Speaker 1>a twinkling star. It's pretty interesting. But then and then

0:42:31.600 --> 0:42:34.719
<v Speaker 1>there are other ways in which a star can change to. Yeah,

0:42:34.800 --> 0:42:37.760
<v Speaker 1>so all stars vary, and some of them vary a lot.

0:42:38.040 --> 0:42:41.000
<v Speaker 1>They are these stars that are called pulsating stars, and

0:42:41.040 --> 0:42:44.040
<v Speaker 1>they get brighter and dimmer and brighter and dimmer, sometimes

0:42:44.120 --> 0:42:47.520
<v Speaker 1>by huge amount. A classic example of these are the sefids.

0:42:47.680 --> 0:42:49.560
<v Speaker 1>These are the ones that Hubble used to discover that

0:42:49.560 --> 0:42:52.640
<v Speaker 1>the universe is expanding. These aren't like pulsars, which shoot

0:42:52.640 --> 0:42:54.920
<v Speaker 1>out a beam of light which spins around and sweeps

0:42:54.920 --> 0:42:58.520
<v Speaker 1>over the Earth. These are like radially shrinking and growing.

0:42:58.560 --> 0:43:02.560
<v Speaker 1>They get bigger and bright, eater, and then smaller and dimmer. Whoa,

0:43:02.640 --> 0:43:05.080
<v Speaker 1>they're They're like a beating heart, almost like the star

0:43:05.200 --> 0:43:08.520
<v Speaker 1>is growing and shrinking. Yeah, they pulse with a regular frequency.

0:43:08.600 --> 0:43:10.600
<v Speaker 1>Well what kind of frequency we're talking about. There's a

0:43:10.640 --> 0:43:13.040
<v Speaker 1>big range in the periods, but it's on the order

0:43:13.080 --> 0:43:15.440
<v Speaker 1>of days. Some of these things have a period of

0:43:15.480 --> 0:43:19.160
<v Speaker 1>like ten days or eighty days or ninety days. So

0:43:19.200 --> 0:43:21.960
<v Speaker 1>this is not like a pulsar that can be spinning

0:43:22.000 --> 0:43:24.880
<v Speaker 1>at like millisecond frequencies or something that's more like on

0:43:24.920 --> 0:43:28.560
<v Speaker 1>the order of days. But sometimes they have like multiple frequencies.

0:43:28.680 --> 0:43:30.640
<v Speaker 1>They can have like a major frequency, and then they

0:43:30.640 --> 0:43:33.360
<v Speaker 1>have like another cycle that's going on inside of that

0:43:33.360 --> 0:43:37.840
<v Speaker 1>that I can constructively or destructively interfere. But even a

0:43:37.880 --> 0:43:40.600
<v Speaker 1>period of days seems a lot, right, Like can you

0:43:40.640 --> 0:43:43.839
<v Speaker 1>imagine the start changing that quickly, like a start size

0:43:43.880 --> 0:43:46.160
<v Speaker 1>of our sun changing that quickly every couple of days,

0:43:46.160 --> 0:43:48.400
<v Speaker 1>that that would be pretty dramatic. It would be crazy

0:43:48.520 --> 0:43:50.399
<v Speaker 1>to be in a system like that where things got

0:43:50.400 --> 0:43:52.600
<v Speaker 1>a lot brighter and then a lot dimmer, and also

0:43:52.680 --> 0:43:55.200
<v Speaker 1>the star itself is getting bigger, right, This is like

0:43:55.239 --> 0:43:58.160
<v Speaker 1>an astrophysical thing you can observe, like the star is

0:43:58.200 --> 0:44:00.920
<v Speaker 1>expanding and now it's shrinking. It has to do with

0:44:00.960 --> 0:44:03.840
<v Speaker 1>what's going on inside the star, you know, like is

0:44:03.880 --> 0:44:07.120
<v Speaker 1>the star opaque to its own energy, so that there's

0:44:07.120 --> 0:44:10.239
<v Speaker 1>all this pressure from the radiation being generated the core

0:44:10.320 --> 0:44:12.799
<v Speaker 1>that's pushing out the outer layers or it is a

0:44:12.840 --> 0:44:15.600
<v Speaker 1>cool down and then become like transparent to that energy

0:44:15.640 --> 0:44:17.600
<v Speaker 1>and it can collapse a little bit. So this this

0:44:17.680 --> 0:44:20.120
<v Speaker 1>cycle that's going on inside every star, but in some

0:44:20.200 --> 0:44:23.080
<v Speaker 1>stars it's very dramatic, right, because stars, as we talked

0:44:23.120 --> 0:44:26.760
<v Speaker 1>about it, are kind of a balance between gravity squishing

0:44:26.800 --> 0:44:30.200
<v Speaker 1>everything in and effusion exploding everything out. And like our

0:44:30.239 --> 0:44:32.319
<v Speaker 1>star is pretty steady, Like it's pretty well balanced, but

0:44:32.360 --> 0:44:34.480
<v Speaker 1>maybe there are stars out there that are not as

0:44:34.480 --> 0:44:36.440
<v Speaker 1>well balanced, and so they kind of swing back and

0:44:36.480 --> 0:44:39.960
<v Speaker 1>forth more wildly between squishing and exploding, you know. And

0:44:39.960 --> 0:44:42.680
<v Speaker 1>it's something we're still trying to understand in detail. People

0:44:42.719 --> 0:44:45.120
<v Speaker 1>are building models to try to explain this kind of thing,

0:44:45.480 --> 0:44:47.839
<v Speaker 1>and it's a great way to probe what's going on

0:44:47.960 --> 0:44:51.319
<v Speaker 1>inside the star. Also because the sefids, at least, there's

0:44:51.360 --> 0:44:55.000
<v Speaker 1>this close connection between the period, how long it takes

0:44:55.000 --> 0:44:57.160
<v Speaker 1>to go from bright to dim and bright to dim,

0:44:57.320 --> 0:45:00.560
<v Speaker 1>and how bright it is at its brightest point, which

0:45:00.560 --> 0:45:02.720
<v Speaker 1>of course is super helpful if you want to understand

0:45:02.719 --> 0:45:05.120
<v Speaker 1>how far away the star is, but also helpful if

0:45:05.120 --> 0:45:07.600
<v Speaker 1>you want to understand what's going on inside the star,

0:45:08.040 --> 0:45:12.359
<v Speaker 1>what crazy processes are driving these things. Uh, it's got

0:45:12.440 --> 0:45:15.280
<v Speaker 1>like a lot of turmoil inside of it, but predictable

0:45:15.320 --> 0:45:19.040
<v Speaker 1>turmoil on this yeah, precisely, okay, cool. And then there

0:45:19.080 --> 0:45:22.359
<v Speaker 1>are also erupting stars or farting stars. There are some

0:45:22.400 --> 0:45:25.640
<v Speaker 1>stars that are even more dramatic than these pulsating stars.

0:45:25.840 --> 0:45:30.600
<v Speaker 1>They are called erupting stars. These stars like blowout material.

0:45:31.040 --> 0:45:33.880
<v Speaker 1>They're like puff away material and then they lose it.

0:45:34.040 --> 0:45:36.879
<v Speaker 1>You know, it's like gone out into space. These are

0:45:36.880 --> 0:45:39.320
<v Speaker 1>not like explosive events. It's not like, you know, the

0:45:39.360 --> 0:45:42.239
<v Speaker 1>star has exploded. It's not like a supernova. It's more

0:45:42.320 --> 0:45:45.040
<v Speaker 1>just like the star has very rapidly grown and then

0:45:45.160 --> 0:45:48.200
<v Speaker 1>loses some of its material. It's not like a gas pocket.

0:45:48.280 --> 0:45:50.439
<v Speaker 1>It's more like it has one of these flow ups

0:45:50.560 --> 0:45:53.520
<v Speaker 1>and in the process that shoots out a big bunch

0:45:53.560 --> 0:45:55.240
<v Speaker 1>of stuff. It shoots out a big bunch of stuff,

0:45:55.360 --> 0:45:57.280
<v Speaker 1>and it can also a creed a big bunch of stuff.

0:45:57.520 --> 0:46:00.520
<v Speaker 1>Like sometimes they're near a source and so they're gathering

0:46:00.719 --> 0:46:03.440
<v Speaker 1>more fuel and that can make the star brighter. In

0:46:03.520 --> 0:46:06.560
<v Speaker 1>extreme cases, it can be really dramatic. One example is

0:46:06.600 --> 0:46:09.640
<v Speaker 1>called a flare star. These kind of stars can grow

0:46:09.680 --> 0:46:12.480
<v Speaker 1>in brightness by a factor of six and then fade

0:46:12.480 --> 0:46:15.000
<v Speaker 1>back down. And this whole thing happens in like half

0:46:15.000 --> 0:46:18.000
<v Speaker 1>an hour. That's huge, but it's not is it constant

0:46:18.040 --> 0:46:19.919
<v Speaker 1>or is it just happens every once in a while.

0:46:20.160 --> 0:46:23.400
<v Speaker 1>These things are not regular the way like pulsating stars are,

0:46:23.680 --> 0:46:26.480
<v Speaker 1>and it's not something that we understand, you know, we

0:46:26.520 --> 0:46:28.960
<v Speaker 1>don't even understand it as well as we understand like

0:46:29.000 --> 0:46:31.680
<v Speaker 1>solar flares on the surface of our sun, which have

0:46:31.800 --> 0:46:34.600
<v Speaker 1>to do with like magnetic field lines snapping and reconnecting.

0:46:34.680 --> 0:46:36.759
<v Speaker 1>So it's something we observe by, something we still don't

0:46:36.840 --> 0:46:39.520
<v Speaker 1>understand the process of. Oh, I see, it's more like

0:46:39.560 --> 0:46:42.960
<v Speaker 1>one twinkle like it twinkles ones sometimes you know, it's

0:46:43.040 --> 0:46:46.120
<v Speaker 1>regular and it's unpredictable. Um, but it does seem to

0:46:46.120 --> 0:46:49.640
<v Speaker 1>happen much more often to red dwarfs, like these dim

0:46:49.719 --> 0:46:52.239
<v Speaker 1>red dwarfs that are all over the galaxy one of

0:46:52.239 --> 0:46:54.520
<v Speaker 1>the most common types of star. These are the ones

0:46:54.560 --> 0:46:59.000
<v Speaker 1>that turn into flare stars. Interesting, regular and unpredictable. I

0:46:59.040 --> 0:47:02.839
<v Speaker 1>feel like it's a good description of myself as well.

0:47:03.760 --> 0:47:07.319
<v Speaker 1>Maybe I should have said not uncommon and unpredictable. It's

0:47:07.360 --> 0:47:10.239
<v Speaker 1>sort of cool because the galaxy is filled with these unassuming,

0:47:10.280 --> 0:47:13.080
<v Speaker 1>sort of generic dim red dwarfs. But occasionally one of

0:47:13.120 --> 0:47:16.040
<v Speaker 1>them becomes like ridiculously bright for just like a half

0:47:16.080 --> 0:47:18.560
<v Speaker 1>an hour and then goes back to being a boring star.

0:47:18.760 --> 0:47:22.880
<v Speaker 1>So these are examples of stars kind of twinkling by themselves.

0:47:23.000 --> 0:47:25.359
<v Speaker 1>Like you said, like, it's not something that's blocking it.

0:47:25.360 --> 0:47:27.319
<v Speaker 1>It's not the atmosphere that's the story. It's like the

0:47:27.360 --> 0:47:29.680
<v Speaker 1>star it self kind of twinkles, even if it's on

0:47:29.760 --> 0:47:32.279
<v Speaker 1>a pretty big time scale exactly, and it's sort of

0:47:32.320 --> 0:47:35.680
<v Speaker 1>across the whole spectrum, you know, the whole star lights

0:47:35.760 --> 0:47:38.560
<v Speaker 1>up in many different frequencies, and so it's pretty cool

0:47:38.560 --> 0:47:40.480
<v Speaker 1>because that means that the twinkling you're seeing is not

0:47:40.560 --> 0:47:43.520
<v Speaker 1>just something local, not just your atmosphere, but it's actually

0:47:43.640 --> 0:47:47.040
<v Speaker 1>information about what's going on inside the star. So it's

0:47:47.080 --> 0:47:50.800
<v Speaker 1>like there's science there. It's like it's sending you a message. Interesting,

0:47:50.920 --> 0:47:54.000
<v Speaker 1>it's like there's yeah, there's a there's hidden mechanics going

0:47:54.040 --> 0:47:55.759
<v Speaker 1>on that you can maybe figure out if you could

0:47:55.800 --> 0:47:58.120
<v Speaker 1>study this, this twinkling. Yeah, and I think about this

0:47:58.200 --> 0:48:00.760
<v Speaker 1>kind of thing every time I'm out in nature enjoying

0:48:00.800 --> 0:48:02.840
<v Speaker 1>a dark sky night, which you know is harder and

0:48:02.840 --> 0:48:05.640
<v Speaker 1>harder to get these days. Right, But you go camping

0:48:05.640 --> 0:48:08.200
<v Speaker 1>a lot, right, is that when you look at stars mostly, Yeah,

0:48:08.200 --> 0:48:10.200
<v Speaker 1>when you go camping is when you're far away from

0:48:10.239 --> 0:48:12.759
<v Speaker 1>the city and all the light pollution, and hopefully you

0:48:12.760 --> 0:48:14.799
<v Speaker 1>don't see too many clouds. That's when you break out

0:48:14.840 --> 0:48:18.840
<v Speaker 1>the guitar and you start lecturing. Do your kids about

0:48:18.880 --> 0:48:22.600
<v Speaker 1>the stars in music? I try not to force them

0:48:22.640 --> 0:48:24.080
<v Speaker 1>to listen to it, but you know, by the way,

0:48:24.080 --> 0:48:26.680
<v Speaker 1>we got a comment from a listener about something you

0:48:26.719 --> 0:48:30.360
<v Speaker 1>said about the weather in Spokane, Washington and how likely

0:48:30.440 --> 0:48:32.800
<v Speaker 1>they are to have clear skies. Wait, what what happened?

0:48:32.800 --> 0:48:34.480
<v Speaker 1>What did I say? And what did they say? Apparently

0:48:34.520 --> 0:48:38.240
<v Speaker 1>you said that it rains eleven months per year in Spokane, Washington,

0:48:38.440 --> 0:48:40.920
<v Speaker 1>and this listener, Jeremy wrote in and said, I just

0:48:40.960 --> 0:48:43.440
<v Speaker 1>want you to know that Spokane is basically a desert

0:48:43.520 --> 0:48:47.640
<v Speaker 1>and it's pronounced Spokane. So thanks Jeremy for the fact checking.

0:48:47.800 --> 0:48:50.040
<v Speaker 1>So I was wrong and many many counts. Yeah, and

0:48:50.120 --> 0:48:52.960
<v Speaker 1>actually I looked it up and it rains seventeen inches

0:48:52.960 --> 0:48:55.600
<v Speaker 1>a year in Spokane and twenty inches a year in

0:48:55.640 --> 0:48:59.080
<v Speaker 1>your hometown of Pasadena. So it's even drier and Spokane

0:48:59.080 --> 0:49:01.920
<v Speaker 1>than it is where you live. Interesting. Wow, Well I

0:49:02.000 --> 0:49:04.200
<v Speaker 1>was wrong, but it means that observing the night sky

0:49:04.239 --> 0:49:07.160
<v Speaker 1>in Pasadena and in Spokane, you won't get blocked by

0:49:07.160 --> 0:49:10.520
<v Speaker 1>a lot of clouds. I am wrong. Every eleven years

0:49:10.520 --> 0:49:13.600
<v Speaker 1>it does happen due to the sun variations. You know,

0:49:13.640 --> 0:49:15.680
<v Speaker 1>it's not something I can help. That's right. Every star

0:49:15.760 --> 0:49:19.560
<v Speaker 1>has their variability, and this is yours. That's right. Every

0:49:19.560 --> 0:49:23.879
<v Speaker 1>stellar engineer has a cycle. All right. Well, it's interesting that,

0:49:23.960 --> 0:49:25.799
<v Speaker 1>you know, something as simple as a kids song like

0:49:25.880 --> 0:49:28.799
<v Speaker 1>Twinkle Twinkle Little Star has so much science behind it.

0:49:28.880 --> 0:49:32.040
<v Speaker 1>You know, it tells us it's inspired by, you know,

0:49:32.200 --> 0:49:34.560
<v Speaker 1>the effects of our atmosphere that we have, how it

0:49:34.560 --> 0:49:37.040
<v Speaker 1>blocks our view of the universe. And it also maybe

0:49:37.120 --> 0:49:40.160
<v Speaker 1>has something to do with the mechanics of stellar you know,

0:49:40.280 --> 0:49:45.439
<v Speaker 1>fusion and processes inside of these incredible exploding machines. Yeah,

0:49:45.480 --> 0:49:47.960
<v Speaker 1>it's really an outstanding way to think about the universe

0:49:48.040 --> 0:49:50.960
<v Speaker 1>and the journey that these lotons make across it, from

0:49:51.000 --> 0:49:53.760
<v Speaker 1>when they're born in this hot ball of plasma billions

0:49:53.760 --> 0:49:57.160
<v Speaker 1>and billions of miles away to finally landing on your eyeball.

0:49:57.360 --> 0:49:59.640
<v Speaker 1>The fact that they get there tells you something about

0:49:59.640 --> 0:50:02.120
<v Speaker 1>the union verse between here and there, and the fact

0:50:02.120 --> 0:50:04.600
<v Speaker 1>that some of their brothers and sisters didn't get there

0:50:04.640 --> 0:50:08.919
<v Speaker 1>also tells you something about what's between us and that star. Yeah.

0:50:09.000 --> 0:50:13.720
<v Speaker 1>Only the lucky ones make it too spoken. The unlucky

0:50:13.760 --> 0:50:17.239
<v Speaker 1>ones make it to Pasadena or Irvine is the lucky

0:50:17.280 --> 0:50:18.880
<v Speaker 1>ones get here and they have to listen to my

0:50:18.920 --> 0:50:24.600
<v Speaker 1>band plan. I'm gonna file a noise complain the universe

0:50:24.640 --> 0:50:27.400
<v Speaker 1>already did it all right? Well, the next time you

0:50:27.600 --> 0:50:29.920
<v Speaker 1>listen to this song, think about the stars and think

0:50:29.960 --> 0:50:33.919
<v Speaker 1>about how our view of the universe still not completely clear.

0:50:34.200 --> 0:50:36.480
<v Speaker 1>We hope you enjoyed that. Thanks for joining us, See

0:50:36.480 --> 0:50:46.760
<v Speaker 1>you next time. Thanks for listening, and remember that Daniel

0:50:46.800 --> 0:50:49.319
<v Speaker 1>and Jorge Explain the Universe is a production of I

0:50:49.560 --> 0:50:53.000
<v Speaker 1>Heart Radio. For more podcast for my heart Radio, visit

0:50:53.000 --> 0:50:56.520
<v Speaker 1>the i heart Radio app, Apple Podcasts, or wherever you

0:50:56.600 --> 0:51:03.680
<v Speaker 1>listen to your favorite shows. No