WEBVTT - What is tidal locking?

0:00:08.520 --> 0:00:11.320
<v Speaker 1>Hey, Kelly, I have a controversial question for you.

0:00:11.760 --> 0:00:14.840
<v Speaker 2>Oh boy, coming from you that makes me particularly nervous.

0:00:15.280 --> 0:00:17.120
<v Speaker 2>Is this another episode I'm gonna have to make sure

0:00:17.160 --> 0:00:18.279
<v Speaker 2>my kids don't listen.

0:00:18.040 --> 0:00:21.520
<v Speaker 1>To no, but it might cause some other kind of

0:00:21.520 --> 0:00:22.320
<v Speaker 1>family drama.

0:00:22.560 --> 0:00:24.119
<v Speaker 2>Okay, now you have my attention.

0:00:25.120 --> 0:00:27.720
<v Speaker 1>Well, you know, since you're married to a cartoonist, I'm

0:00:27.760 --> 0:00:30.320
<v Speaker 1>wondering if I'm allowed to ask you whether you're a

0:00:30.360 --> 0:00:32.400
<v Speaker 1>fan of a different cartoon.

0:00:32.800 --> 0:00:36.040
<v Speaker 2>Well, that depends if it's a rival cartoon or not.

0:00:38.560 --> 0:00:42.080
<v Speaker 1>So I'm wondering if you have a favorite cartoon from

0:00:42.280 --> 0:00:43.080
<v Speaker 1>the Far Side.

0:00:43.440 --> 0:00:46.080
<v Speaker 2>Oh, I mean he hasn't updated for a while, right,

0:00:46.120 --> 0:00:48.440
<v Speaker 2>I mean, I suppose he's still competition. But anyway, all right,

0:00:48.479 --> 0:00:50.519
<v Speaker 2>let's see, let's see. Oh, so hard to pick so

0:00:50.560 --> 0:00:54.320
<v Speaker 2>many favorites. So there's one where there's a slide, you know,

0:00:54.440 --> 0:00:57.640
<v Speaker 2>like a kid's playground, and some spiders have built a

0:00:57.760 --> 0:01:02.840
<v Speaker 2>net or a web along the bottom, and one spider

0:01:02.920 --> 0:01:05.760
<v Speaker 2>is saying something like, if we can pull this off,

0:01:06.360 --> 0:01:10.080
<v Speaker 2>we'll never be hungry again, nor something like that, And I,

0:01:10.480 --> 0:01:13.240
<v Speaker 2>as an invert person, just thought that that was amazing.

0:01:13.240 --> 0:01:14.840
<v Speaker 2>And of course I liked the like School for the

0:01:14.880 --> 0:01:18.200
<v Speaker 2>Gifted the one that was on T shirts when I

0:01:18.280 --> 0:01:20.160
<v Speaker 2>was a kid. What about you, Well, I have.

0:01:20.040 --> 0:01:22.120
<v Speaker 1>To ask you. Do you see that Spider's eating a

0:01:22.160 --> 0:01:24.640
<v Speaker 1>baby cartoon differently now that you're a parent?

0:01:24.920 --> 0:01:26.280
<v Speaker 2>No, still hilarious.

0:01:28.040 --> 0:01:28.160
<v Speaker 3>Us.

0:01:28.200 --> 0:01:30.559
<v Speaker 1>I think your children should be terrified if they listen

0:01:30.680 --> 0:01:31.520
<v Speaker 1>to this episode.

0:01:31.959 --> 0:01:34.959
<v Speaker 2>Probably. Oh my gosh, poor kid won. The other day,

0:01:35.080 --> 0:01:37.959
<v Speaker 2>I told her to go get a bowl in my office,

0:01:38.360 --> 0:01:40.520
<v Speaker 2>and she thought it was going to have something like

0:01:40.600 --> 0:01:42.920
<v Speaker 2>candy in it, but she accidentally picked up the bowl

0:01:43.000 --> 0:01:46.440
<v Speaker 2>of dead insects that I found in the in the

0:01:46.480 --> 0:01:48.600
<v Speaker 2>barn that I was thinking of pinning at some point,

0:01:48.720 --> 0:01:51.320
<v Speaker 2>and they were all over my office, so she must

0:01:51.320 --> 0:01:53.160
<v Speaker 2>have seen it and thrown it up in the air

0:01:53.840 --> 0:01:56.320
<v Speaker 2>and they went all over. My kids are going to

0:01:56.400 --> 0:01:58.520
<v Speaker 2>have very high therapy bills at some point, but I

0:01:58.560 --> 0:01:59.440
<v Speaker 2>love them very much.

0:01:59.560 --> 0:02:01.800
<v Speaker 1>I think that living in your house must be even

0:02:01.840 --> 0:02:21.360
<v Speaker 1>weirder than the Far Side cartoon, almost certain. Hi. I'm Daniel.

0:02:21.400 --> 0:02:24.720
<v Speaker 1>I'm a particle physicist and a professor at UC Irvine,

0:02:25.000 --> 0:02:28.640
<v Speaker 1>and I don't think I've yet traumatized my children with insects.

0:02:28.840 --> 0:02:32.000
<v Speaker 2>Hi. I'm Kelly Wiener Smith, and I study creepy crawley

0:02:32.080 --> 0:02:35.840
<v Speaker 2>things at race university, and I'm traumatizing kids all the time.

0:02:36.080 --> 0:02:38.280
<v Speaker 1>Education through trauma is set your strategy.

0:02:38.400 --> 0:02:40.400
<v Speaker 2>That's a good way to make people remember stuff.

0:02:43.600 --> 0:02:45.400
<v Speaker 1>Where you live out on the farm, but there's lots

0:02:45.400 --> 0:02:48.240
<v Speaker 1>of access to creepy crawley weird things, and so I

0:02:48.280 --> 0:02:50.920
<v Speaker 1>hope your kids are become ver acclimatized.

0:02:50.280 --> 0:02:52.960
<v Speaker 2>To that I'm making them because it.

0:02:52.960 --> 0:02:56.359
<v Speaker 1>Takes a brave soul to explore the nature of the universe,

0:02:56.480 --> 0:02:59.919
<v Speaker 1>or even just your backyard, depending on what's slithering out there.

0:03:00.080 --> 0:03:02.280
<v Speaker 1>So whether or not you turn your eyes down to

0:03:02.320 --> 0:03:04.639
<v Speaker 1>the ground or up to the skies, there's a whole

0:03:04.680 --> 0:03:07.040
<v Speaker 1>lot of stuff to wonder about, and so welcome to

0:03:07.080 --> 0:03:10.000
<v Speaker 1>the podcast. Daniel and Jorge explain the universe in which

0:03:10.040 --> 0:03:12.720
<v Speaker 1>we do all of that wondering. We think about everything

0:03:12.760 --> 0:03:15.519
<v Speaker 1>that's between your toes and everything that your eyes can

0:03:15.560 --> 0:03:18.120
<v Speaker 1>gather as you look up into the night sky. We

0:03:18.160 --> 0:03:20.200
<v Speaker 1>think about what's on the moon, what's on the backside

0:03:20.240 --> 0:03:22.720
<v Speaker 1>of the moon, and what's in the deepest, darkest depths

0:03:22.760 --> 0:03:25.080
<v Speaker 1>of the universe. We chew all of it up and

0:03:25.120 --> 0:03:27.120
<v Speaker 1>try to digest it and explain.

0:03:26.800 --> 0:03:29.080
<v Speaker 2>It to you, and it's not always pretty.

0:03:31.240 --> 0:03:34.600
<v Speaker 1>Sometimes the truth is just gross. My typical co host

0:03:34.639 --> 0:03:36.680
<v Speaker 1>and friend, Jorge Champ can't be here today, so I'm

0:03:36.760 --> 0:03:39.360
<v Speaker 1>very glad to have one of our regular guest hosts, Kelly. Kelly,

0:03:39.360 --> 0:03:42.440
<v Speaker 1>thanks very much for joining us again and terrifying your children.

0:03:42.760 --> 0:03:45.320
<v Speaker 2>Yeah, well, I hope I could terrify some people today too.

0:03:45.400 --> 0:03:46.520
<v Speaker 2>Thanks for having me back.

0:03:47.560 --> 0:03:50.080
<v Speaker 1>But today we're not talking about the weird, creepy crawley

0:03:50.120 --> 0:03:54.320
<v Speaker 1>bits that are inside Kelly's pantry, strange as that might be.

0:03:55.680 --> 0:03:58.720
<v Speaker 1>We are turning our eyes to the sky tonight. We

0:03:58.760 --> 0:04:01.600
<v Speaker 1>are thinking about what's out there in the universe, and

0:04:01.640 --> 0:04:04.600
<v Speaker 1>what we can see and what we can't see, and

0:04:04.600 --> 0:04:07.520
<v Speaker 1>how the gravitational forces that have built the structure of

0:04:07.560 --> 0:04:10.720
<v Speaker 1>our universe also limit what we can see out there.

0:04:11.040 --> 0:04:12.560
<v Speaker 1>If you were a kid like me, then you spent

0:04:12.640 --> 0:04:14.280
<v Speaker 1>a lot of time looking up at the night sky,

0:04:14.480 --> 0:04:17.680
<v Speaker 1>not just absorbing the stars, but also gazing on the

0:04:17.839 --> 0:04:21.039
<v Speaker 1>closest object that's out there, the biggest, fattest thing in

0:04:21.080 --> 0:04:24.040
<v Speaker 1>the night sky, and that's, of course our moon. It

0:04:24.040 --> 0:04:26.720
<v Speaker 1>has so many fascinating features to it, but one of

0:04:26.760 --> 0:04:29.640
<v Speaker 1>the most interesting features is that you always see the

0:04:29.720 --> 0:04:33.400
<v Speaker 1>same features. Cally, do you remember understanding this as a kid,

0:04:33.520 --> 0:04:36.320
<v Speaker 1>or wondering about why you're always seeing the same bits

0:04:36.360 --> 0:04:36.880
<v Speaker 1>on the moon.

0:04:37.320 --> 0:04:40.040
<v Speaker 2>You know, I really wish you hadn't asked me that,

0:04:40.120 --> 0:04:43.479
<v Speaker 2>because the answer is, when I was a kid, I

0:04:43.560 --> 0:04:46.440
<v Speaker 2>didn't realize I was always seeing the same side of

0:04:46.440 --> 0:04:49.440
<v Speaker 2>the moon. That hadn't really hit me until I think, baby,

0:04:49.640 --> 0:04:51.640
<v Speaker 2>I was in college, and then I was like, wait

0:04:51.680 --> 0:04:53.960
<v Speaker 2>a minute, and I guess it just wasn't I was

0:04:53.960 --> 0:04:57.760
<v Speaker 2>looking down at the salamanders and not up at the sky.

0:04:58.080 --> 0:05:00.320
<v Speaker 2>But so, no, that is not a question I had

0:05:00.320 --> 0:05:03.039
<v Speaker 2>when I was a kid, but it should be. When

0:05:03.040 --> 0:05:03.760
<v Speaker 2>did you learn this?

0:05:04.080 --> 0:05:05.960
<v Speaker 1>I remember learning about it, I think when I was

0:05:06.000 --> 0:05:08.239
<v Speaker 1>seven or eight, But you know, my dad was pretty

0:05:08.240 --> 0:05:11.080
<v Speaker 1>into astronomy and into science, and so we talked about

0:05:11.080 --> 0:05:13.960
<v Speaker 1>this kind of stuff. Something I'm still curious about, though,

0:05:14.200 --> 0:05:17.440
<v Speaker 1>is when humanity understood that, or when humanity understood it

0:05:17.480 --> 0:05:22.080
<v Speaker 1>was an interesting question, like did ancient Chinese astronomers, who

0:05:22.160 --> 0:05:24.120
<v Speaker 1>spend a lot of time looking up at the moon

0:05:24.160 --> 0:05:27.520
<v Speaker 1>and predicting its eclipses, did they figure out that the

0:05:27.520 --> 0:05:29.600
<v Speaker 1>moon was a sphere and that it was rotating and

0:05:29.600 --> 0:05:31.920
<v Speaker 1>that it was weird that we always saw the same

0:05:32.000 --> 0:05:34.920
<v Speaker 1>side of it? Or is this just something they overlooked.

0:05:34.960 --> 0:05:36.359
<v Speaker 2>Do you know the answer to that question.

0:05:36.640 --> 0:05:38.520
<v Speaker 1>I don't know the answer to that question. I've been

0:05:38.560 --> 0:05:41.760
<v Speaker 1>digging through the history of astronomy a little bit, and

0:05:41.839 --> 0:05:44.640
<v Speaker 1>I know that Newton understood it because of his ideas

0:05:44.680 --> 0:05:48.000
<v Speaker 1>of gravitation, But digging deeper into history, it's not really

0:05:48.000 --> 0:05:51.360
<v Speaker 1>discussed very much. And I sort of wonder if people

0:05:51.400 --> 0:05:54.800
<v Speaker 1>suspected that it was just a coincidence that the Moon

0:05:54.920 --> 0:05:57.360
<v Speaker 1>rotates at this perfect rate just so that we can

0:05:57.400 --> 0:05:59.360
<v Speaker 1>only see one side of it, because you know, there

0:05:59.400 --> 0:06:03.760
<v Speaker 1>are other fascinating coincidences about the moon. For example, the

0:06:03.760 --> 0:06:06.440
<v Speaker 1>moon and the Sun happen to be the same size

0:06:06.480 --> 0:06:09.560
<v Speaker 1>in our sky, right, the Sun is much much bigger,

0:06:09.680 --> 0:06:12.920
<v Speaker 1>but much much further away, and those two numbers line

0:06:13.000 --> 0:06:15.640
<v Speaker 1>up perfectly. So the Sun and the Moon appear to

0:06:15.680 --> 0:06:17.600
<v Speaker 1>be the same size, which is why we can get

0:06:17.640 --> 0:06:21.000
<v Speaker 1>so many fascinating eclipse effects. And that, of course, is

0:06:21.120 --> 0:06:23.599
<v Speaker 1>just a coincidence. There's no like deep reason for that.

0:06:24.000 --> 0:06:26.800
<v Speaker 1>It just happens to be. These two numbers just kind

0:06:26.800 --> 0:06:27.960
<v Speaker 1>of line up in our.

0:06:27.960 --> 0:06:33.160
<v Speaker 2>Universe, and humans are notoriously tripped up by coincidences.

0:06:32.640 --> 0:06:35.839
<v Speaker 1>Exactly, And so I think ancient astronomers must have wondered

0:06:35.880 --> 0:06:38.480
<v Speaker 1>about that size, and I wonder if they also wondered

0:06:38.640 --> 0:06:41.560
<v Speaker 1>about the rotation of the moon, if they understood that. Now,

0:06:41.600 --> 0:06:44.640
<v Speaker 1>I do know that ancient Chinese astronomers had a little

0:06:44.680 --> 0:06:47.920
<v Speaker 1>bit of a disadvantage compared to, for example, ancient Greek astronomers,

0:06:48.160 --> 0:06:51.320
<v Speaker 1>because they didn't have geometry. Right, we think about the

0:06:51.440 --> 0:06:54.719
<v Speaker 1>universe in terms of geometry. You imagine how clips has happened,

0:06:54.720 --> 0:06:56.320
<v Speaker 1>and you think, probably in your head, you have a

0:06:56.360 --> 0:06:59.960
<v Speaker 1>mental picture of all these things happening and to explain it.

0:07:00.240 --> 0:07:03.320
<v Speaker 1>But Chinese astronomers didn't develop geometry, so they didn't have

0:07:03.400 --> 0:07:06.760
<v Speaker 1>the same sort of geometrical thinking that we're all very

0:07:06.760 --> 0:07:09.680
<v Speaker 1>familiar with. Instead, they had like tables of numbers, and

0:07:09.680 --> 0:07:12.440
<v Speaker 1>they had arithmetic, and they could manipulate these numbers to

0:07:12.520 --> 0:07:14.680
<v Speaker 1>do their predictions. So I think they must have thought

0:07:14.680 --> 0:07:16.560
<v Speaker 1>about these things very differently than we did.

0:07:16.720 --> 0:07:18.640
<v Speaker 2>Interesting, it's nice to have our modern tools.

0:07:20.360 --> 0:07:22.840
<v Speaker 1>Thank you to those folks who invented geometry. It turns

0:07:22.840 --> 0:07:23.880
<v Speaker 1>out to be pretty.

0:07:23.680 --> 0:07:25.480
<v Speaker 2>Useful quote unquote modern.

0:07:25.760 --> 0:07:25.960
<v Speaker 3>Yeah.

0:07:26.040 --> 0:07:28.360
<v Speaker 1>Right, And so we have been looking up in the

0:07:28.400 --> 0:07:30.680
<v Speaker 1>night sky and looking at the moon and seeing the

0:07:30.680 --> 0:07:33.720
<v Speaker 1>same side of it for thousands and thousands of years,

0:07:34.120 --> 0:07:37.440
<v Speaker 1>and now, of course we understand why. And so today

0:07:37.440 --> 0:07:39.400
<v Speaker 1>on the podcast, we're going to be digging into the

0:07:39.440 --> 0:07:42.320
<v Speaker 1>physics of the far side of the Moon and many

0:07:42.440 --> 0:07:46.520
<v Speaker 1>other objects in our solar system that exhibit the same behavior.

0:07:46.880 --> 0:07:54.600
<v Speaker 1>On today's episode, well, I answer the question what is

0:07:54.920 --> 0:07:56.160
<v Speaker 1>tidal locking?

0:07:56.560 --> 0:07:59.040
<v Speaker 2>And this is another thing that connects us to the dinosaurs, right,

0:07:59.040 --> 0:08:01.040
<v Speaker 2>because they also would have seen the same side.

0:08:00.880 --> 0:08:05.480
<v Speaker 1>Of the moon. If dinosaur geometers had figured that out, boy,

0:08:06.000 --> 0:08:07.440
<v Speaker 1>they could have written a paper and got a lot

0:08:07.440 --> 0:08:08.160
<v Speaker 1>of citations.

0:08:08.400 --> 0:08:10.240
<v Speaker 2>They really could have, and then maybe they could have

0:08:10.280 --> 0:08:13.880
<v Speaker 2>started a you know, NASA and had an asteroid deflection program.

0:08:13.880 --> 0:08:14.960
<v Speaker 2>Everything could have been different.

0:08:15.840 --> 0:08:17.400
<v Speaker 1>You sound like you're kind of hoping for that, but

0:08:17.440 --> 0:08:19.960
<v Speaker 1>you know, in that scenario, we don't exist.

0:08:20.280 --> 0:08:21.280
<v Speaker 2>Oh, good point.

0:08:22.040 --> 0:08:24.040
<v Speaker 1>We're rooting for the asteroid on that one.

0:08:23.800 --> 0:08:24.800
<v Speaker 2>That's right, we sure are.

0:08:25.280 --> 0:08:28.120
<v Speaker 1>I'm sorry dinosaurs, which puts us on the anti math

0:08:28.280 --> 0:08:30.760
<v Speaker 1>Education for Dinosaurs committee as well.

0:08:30.920 --> 0:08:33.559
<v Speaker 2>It's an uncomfortable place to be, but no, it doesn't

0:08:33.559 --> 0:08:36.600
<v Speaker 2>feel very good, but I'm firmly in this position. Yeah.

0:08:36.640 --> 0:08:38.760
<v Speaker 1>So this is a topic that affects our Moon, and

0:08:38.880 --> 0:08:41.200
<v Speaker 1>affects our planet, and affects a lot of things in

0:08:41.240 --> 0:08:43.599
<v Speaker 1>the Solar system and in other Solar system. It's a

0:08:43.640 --> 0:08:46.440
<v Speaker 1>fascinating little bit of physics. So I was curious what

0:08:46.559 --> 0:08:50.400
<v Speaker 1>people knew about the topic of title locking and if

0:08:50.400 --> 0:08:52.480
<v Speaker 1>they understood the physics of it. So I went out

0:08:52.480 --> 0:08:55.640
<v Speaker 1>there into the internet to ask folks if they understood this.

0:08:55.800 --> 0:08:57.760
<v Speaker 1>Thanks very much to those of you who participate in

0:08:57.800 --> 0:09:00.240
<v Speaker 1>this segment of the podcast to let us know what

0:09:00.280 --> 0:09:02.880
<v Speaker 1>people think about the topic of the day. If you'd

0:09:02.880 --> 0:09:05.160
<v Speaker 1>like to hear your voice for a future episode, please

0:09:05.200 --> 0:09:08.760
<v Speaker 1>don't be shy. Write to me two questions at Danielandjorge

0:09:09.200 --> 0:09:11.240
<v Speaker 1>dot com. So think about it for a minute. Do

0:09:11.320 --> 0:09:14.600
<v Speaker 1>you understand the physics of title locking? Here's what some

0:09:14.640 --> 0:09:15.880
<v Speaker 1>listeners had to say.

0:09:16.120 --> 0:09:20.400
<v Speaker 4>So, I believe that title locking is when, say, a

0:09:20.440 --> 0:09:23.199
<v Speaker 4>planet has a moon that's locked in orbit at a

0:09:23.240 --> 0:09:26.320
<v Speaker 4>certain distance, so the tides are always the same. So

0:09:26.440 --> 0:09:29.000
<v Speaker 4>I guess you could say that we're in title locking

0:09:29.040 --> 0:09:32.520
<v Speaker 4>because day in and day out, our tides go the

0:09:32.600 --> 0:09:33.320
<v Speaker 4>same because.

0:09:33.080 --> 0:09:34.520
<v Speaker 1>The moon's in a fixed orbit.

0:09:34.880 --> 0:09:37.520
<v Speaker 2>Title locking is just like our moon. We see the

0:09:37.559 --> 0:09:40.000
<v Speaker 2>same face of it at all times.

0:09:40.080 --> 0:09:42.520
<v Speaker 4>It has no spin, and the dark side of the

0:09:42.520 --> 0:09:43.640
<v Speaker 4>moon is facing outward.

0:09:43.800 --> 0:09:47.760
<v Speaker 2>It is the deformation that a celestial body so first

0:09:47.800 --> 0:09:52.360
<v Speaker 2>when it's orbiting or is orbited by another massive celestial body.

0:09:52.600 --> 0:09:57.319
<v Speaker 3>Title locking is when a lower mass body is orbiting

0:09:57.480 --> 0:10:00.720
<v Speaker 3>a much higher mass body and the the same side

0:10:00.840 --> 0:10:03.640
<v Speaker 3>always faces it, so I know that we always see

0:10:03.679 --> 0:10:06.880
<v Speaker 3>the same side of the Moon means tidally locked to

0:10:06.920 --> 0:10:07.280
<v Speaker 3>the Earth.

0:10:07.679 --> 0:10:10.760
<v Speaker 2>I was impressed that none of the listeners seemed totally

0:10:10.760 --> 0:10:13.920
<v Speaker 2>stumped by this, because I feel like tidle locking is

0:10:13.960 --> 0:10:17.040
<v Speaker 2>not necessarily something that you hear, like that at least

0:10:17.040 --> 0:10:20.080
<v Speaker 2>there's a phrase I don't hear very often, and so like,

0:10:20.160 --> 0:10:22.959
<v Speaker 2>it seems like some people knew exactly what you were

0:10:23.000 --> 0:10:25.439
<v Speaker 2>asking about, and none of them were like me when

0:10:25.480 --> 0:10:27.880
<v Speaker 2>I was a kid, and we're just totally unaware that

0:10:27.920 --> 0:10:29.199
<v Speaker 2>this is a thing that was happening.

0:10:29.440 --> 0:10:33.040
<v Speaker 1>Yeah, we got some pretty well educated listeners. The word title,

0:10:33.200 --> 0:10:36.080
<v Speaker 1>I think makes some people think of tides, which is

0:10:36.120 --> 0:10:39.560
<v Speaker 1>connected of course to tidal forces, you know, like the

0:10:39.600 --> 0:10:43.040
<v Speaker 1>Moon pulls on the Earth and squishes its oceans and

0:10:43.360 --> 0:10:45.880
<v Speaker 1>makes us have higher tides in some places and lower

0:10:45.880 --> 0:10:48.160
<v Speaker 1>tides and other places. But that's not what we mean

0:10:48.200 --> 0:10:51.400
<v Speaker 1>by title locking. Tidle locking is actually a different phenomena

0:10:51.640 --> 0:10:54.440
<v Speaker 1>we're going to dig into today. But thank you very

0:10:54.520 --> 0:10:57.600
<v Speaker 1>much to all of our volunteers. We really cherish your thoughts.

0:10:57.800 --> 0:11:00.360
<v Speaker 2>Yeah, you have a smarter than average audience, I think,

0:11:00.440 --> 0:11:05.880
<v Speaker 2>or smarter than Kelly average. I'm always impressed by the answers.

0:11:06.280 --> 0:11:08.199
<v Speaker 1>They're smart and they're good looking too.

0:11:08.240 --> 0:11:11.920
<v Speaker 2>That's right. I think that's called the halo effect. You

0:11:12.040 --> 0:11:13.719
<v Speaker 2>know one good thing about them, and you assume you

0:11:13.760 --> 0:11:15.040
<v Speaker 2>know all the good things about them.

0:11:15.120 --> 0:11:18.080
<v Speaker 1>So let's dig into the physics of tidal locking. What

0:11:18.120 --> 0:11:20.120
<v Speaker 1>it is, what's going on and why I play such

0:11:20.120 --> 0:11:22.880
<v Speaker 1>a big role in what we see in our night sky.

0:11:23.160 --> 0:11:25.360
<v Speaker 1>And I think the first thing to understand is just

0:11:25.440 --> 0:11:28.480
<v Speaker 1>like the geometry of what's going on. Obviously, the Moon

0:11:28.800 --> 0:11:32.120
<v Speaker 1>is orbiting the Earth, and the Earth is spinning, and

0:11:32.200 --> 0:11:34.200
<v Speaker 1>the Moon is spinning around the Earth, and the Moon

0:11:34.280 --> 0:11:37.079
<v Speaker 1>is also spinning on its axis. So there's sort of

0:11:37.200 --> 0:11:39.480
<v Speaker 1>a lot of spinning going on. But you got to

0:11:39.520 --> 0:11:41.800
<v Speaker 1>get all that spinning in your head to understand, like

0:11:41.920 --> 0:11:44.640
<v Speaker 1>why we only see one side of the moon.

0:11:44.920 --> 0:11:48.640
<v Speaker 2>Yes, so I am staring directly ahead trying to picture everything,

0:11:48.760 --> 0:11:50.800
<v Speaker 2>So go ahead, what should I be imagining?

0:11:51.840 --> 0:11:54.439
<v Speaker 1>So first, just put yourself on the Earth and forget

0:11:54.440 --> 0:11:56.480
<v Speaker 1>the fact that the Earth is spinning, and just move

0:11:56.559 --> 0:11:59.480
<v Speaker 1>the Moon around the Earth in your mind and imagine

0:11:59.480 --> 0:12:01.320
<v Speaker 1>the Moon is like a shoe or something. If the

0:12:01.360 --> 0:12:03.960
<v Speaker 1>Moon is not spinning, it's just orbiting the Earth, then

0:12:04.040 --> 0:12:06.200
<v Speaker 1>the Earth is going to see different sides of the shoe.

0:12:06.240 --> 0:12:07.560
<v Speaker 1>It's going to see the back of the shoe, it's

0:12:07.600 --> 0:12:09.679
<v Speaker 1>going to see the front of the shoe, because as

0:12:09.720 --> 0:12:12.480
<v Speaker 1>the shoe moves around the Earth, different sides of it

0:12:12.559 --> 0:12:15.000
<v Speaker 1>are going to be closer to the Earth or closer

0:12:15.040 --> 0:12:15.880
<v Speaker 1>to outer space.

0:12:16.120 --> 0:12:17.640
<v Speaker 2>So the shoe is not rotating either.

0:12:17.800 --> 0:12:20.000
<v Speaker 1>That's right. So first the shoe is not rotating, and

0:12:20.040 --> 0:12:21.319
<v Speaker 1>so we see one side of it, and then we

0:12:21.360 --> 0:12:23.559
<v Speaker 1>see the other side of it. So if the shoe

0:12:23.720 --> 0:12:25.960
<v Speaker 1>or the moon or whatever is not spinning, then you

0:12:25.960 --> 0:12:28.440
<v Speaker 1>would see different sides of it. Right now, the moon,

0:12:28.440 --> 0:12:31.280
<v Speaker 1>of course, is spinning. It's spinning on its axis. But

0:12:31.360 --> 0:12:33.640
<v Speaker 1>if it was spinning at some random rate, like really

0:12:33.679 --> 0:12:36.360
<v Speaker 1>really fast or really really slow, you would still see

0:12:36.400 --> 0:12:38.599
<v Speaker 1>both sides of it, because eventually it would spin in

0:12:38.679 --> 0:12:41.520
<v Speaker 1>a way that revealed every part of the moon. The

0:12:41.559 --> 0:12:44.160
<v Speaker 1>only way for us to not be able to see

0:12:44.200 --> 0:12:46.760
<v Speaker 1>part of the moon is for its spin to be

0:12:46.880 --> 0:12:49.840
<v Speaker 1>perfectly syncd up with its orbit, so that as it

0:12:49.920 --> 0:12:52.480
<v Speaker 1>goes around the Earth, it turns just the right a

0:12:52.520 --> 0:12:55.560
<v Speaker 1>mount every second, so the same side of it is

0:12:55.640 --> 0:12:58.440
<v Speaker 1>always facing the Earth, like if the back side of

0:12:58.480 --> 0:13:01.320
<v Speaker 1>the shoe is always fa the Earth, because the shoe

0:13:01.360 --> 0:13:03.480
<v Speaker 1>itself is spinning at just the right rate as it

0:13:03.520 --> 0:13:04.880
<v Speaker 1>goes around the Earth.

0:13:04.760 --> 0:13:07.680
<v Speaker 2>And everyone on every part of the Earth is always

0:13:07.679 --> 0:13:09.760
<v Speaker 2>seeing the same side of the Moon. Right, It's not

0:13:09.840 --> 0:13:11.760
<v Speaker 2>like you know, in the US you see one side

0:13:11.760 --> 0:13:13.800
<v Speaker 2>and in China you see the other side, or right,

0:13:13.880 --> 0:13:15.079
<v Speaker 2>You're always seeing the same side.

0:13:15.160 --> 0:13:17.480
<v Speaker 1>That's right. The same side of the Moon is always

0:13:17.520 --> 0:13:19.760
<v Speaker 1>closer to the Earth, and the other side of the

0:13:19.760 --> 0:13:22.280
<v Speaker 1>Moon that we call the far side, which I assume

0:13:22.480 --> 0:13:24.480
<v Speaker 1>is the origin of the name of the far side

0:13:24.480 --> 0:13:28.520
<v Speaker 1>and comic, it is always facing outer space. And this

0:13:28.600 --> 0:13:31.600
<v Speaker 1>is the sort of coincidence we were talking about. Like these

0:13:31.640 --> 0:13:34.400
<v Speaker 1>two numbers, the rate at which the Moon goes around

0:13:34.400 --> 0:13:36.640
<v Speaker 1>the Earth and the rate at which the Moon spins

0:13:36.720 --> 0:13:40.320
<v Speaker 1>around its axis have to be perfectly synced up to

0:13:40.360 --> 0:13:41.160
<v Speaker 1>get this effect.

0:13:41.360 --> 0:13:44.040
<v Speaker 2>And why are they perfectly syncd up? Is this one

0:13:44.080 --> 0:13:46.720
<v Speaker 2>of the few instances in which we have something special

0:13:46.800 --> 0:13:49.640
<v Speaker 2>going on and they just happen to sync up. Or

0:13:49.840 --> 0:13:52.680
<v Speaker 2>are we just like every other moon because this happens

0:13:52.679 --> 0:13:53.240
<v Speaker 2>all the time.

0:13:54.559 --> 0:13:57.280
<v Speaker 1>So it's not that special and it's not a coincidence,

0:13:57.360 --> 0:14:00.439
<v Speaker 1>but it's not something that's always happened. Like, to get

0:14:00.440 --> 0:14:02.760
<v Speaker 1>into it, you have to understand the history of the

0:14:02.800 --> 0:14:05.040
<v Speaker 1>formation of the Moon, like how did it get made,

0:14:05.280 --> 0:14:08.440
<v Speaker 1>how was it spinning originally, and then how has that changed?

0:14:08.520 --> 0:14:10.840
<v Speaker 1>You know, our moon is not just like some object

0:14:10.920 --> 0:14:13.600
<v Speaker 1>that we captured as it was flying by. We think

0:14:13.600 --> 0:14:17.200
<v Speaker 1>that the Moon actually comes from a huge collision something

0:14:17.280 --> 0:14:20.320
<v Speaker 1>like one hundred million years after the Earth was formed,

0:14:20.320 --> 0:14:23.800
<v Speaker 1>so we're talking like four point four billion years ago.

0:14:24.080 --> 0:14:27.120
<v Speaker 1>You have some like very hot proto Earth. It got

0:14:27.160 --> 0:14:32.040
<v Speaker 1>slammed into by some giant Mars sized planet they called Fea,

0:14:32.520 --> 0:14:35.200
<v Speaker 1>And so you're talking about a huge collision like Earth

0:14:35.320 --> 0:14:40.000
<v Speaker 1>versus Mars in space and both objects are essentially vaporized.

0:14:40.280 --> 0:14:42.400
<v Speaker 2>But we still have thirst in the moon.

0:14:43.920 --> 0:14:47.320
<v Speaker 1>You're like, how do that to current reality? You know,

0:14:47.400 --> 0:14:51.000
<v Speaker 1>you're exactly right, it got vaporized, but then it coalesced. Right.

0:14:51.120 --> 0:14:54.320
<v Speaker 1>Gravity is very very patient, and so even though all

0:14:54.360 --> 0:14:56.160
<v Speaker 1>of its original work in the first one hundred million

0:14:56.200 --> 0:14:59.120
<v Speaker 1>years was ruined by this collision. It got back to

0:14:59.160 --> 0:15:01.800
<v Speaker 1>work and it pulled those blobs together and it made

0:15:02.000 --> 0:15:04.760
<v Speaker 1>two new blobs, one that formed the Earth, and then

0:15:04.800 --> 0:15:07.160
<v Speaker 1>a big ring around the Earth, like a ring of

0:15:07.200 --> 0:15:10.400
<v Speaker 1>debris that was spinning sort of too fast around the

0:15:10.400 --> 0:15:13.440
<v Speaker 1>Earth to fall into the central clump, which formed this

0:15:13.560 --> 0:15:15.480
<v Speaker 1>like huge spray of material.

0:15:15.800 --> 0:15:17.680
<v Speaker 2>All right, So, and that's why the Moon's made out

0:15:17.680 --> 0:15:19.160
<v Speaker 2>of the same stuff the Earth is made out of.

0:15:19.360 --> 0:15:22.160
<v Speaker 1>Exactly when we visited the Earth first and we sampled it,

0:15:22.360 --> 0:15:25.320
<v Speaker 1>people were surprised to discover that it's basically the same

0:15:25.400 --> 0:15:27.920
<v Speaker 1>mixture of stuff as the Earth. It's not like a

0:15:28.040 --> 0:15:31.120
<v Speaker 1>different Solar System body that was formed in another place,

0:15:31.160 --> 0:15:33.320
<v Speaker 1>and so it has a different mixture of like ices

0:15:33.400 --> 0:15:36.280
<v Speaker 1>and rocks and different isotopes and stuff. It's basically made

0:15:36.320 --> 0:15:38.120
<v Speaker 1>out of the same stuff as the Earth. And that's

0:15:38.120 --> 0:15:42.040
<v Speaker 1>because it comes from the same mixture of those two planets.

0:15:42.520 --> 0:15:44.960
<v Speaker 1>Like it was the same vaporized blob of stuff, and

0:15:45.080 --> 0:15:46.680
<v Speaker 1>some of it fell in towards the Earth, and the

0:15:46.680 --> 0:15:49.160
<v Speaker 1>stuff that was spinning around sort of too fast ended

0:15:49.240 --> 0:15:52.240
<v Speaker 1>up in this big debris ring. But then gravity pulled

0:15:52.280 --> 0:15:53.800
<v Speaker 1>that together into a moon.

0:15:54.160 --> 0:15:56.560
<v Speaker 2>Did we have this hypothesis before we went to the

0:15:56.560 --> 0:15:58.560
<v Speaker 2>Moon and found what it was made of, or did

0:15:58.640 --> 0:16:02.160
<v Speaker 2>going to the Moon and physically collecting samples give us

0:16:02.200 --> 0:16:04.960
<v Speaker 2>this hypothesis when we were like, whoa, it's the same stuff.

0:16:06.120 --> 0:16:08.400
<v Speaker 1>This hypothesis has been around for a while, but it

0:16:08.440 --> 0:16:10.840
<v Speaker 1>really became the favorite once we went to the Moon,

0:16:11.280 --> 0:16:14.400
<v Speaker 1>and also once we understood something about the Moon's inner core.

0:16:14.800 --> 0:16:17.640
<v Speaker 1>The Moon has sort of a small iron core, smaller

0:16:17.640 --> 0:16:20.480
<v Speaker 1>than you would expect, and the hypothesis is that a

0:16:20.520 --> 0:16:23.440
<v Speaker 1>lot of that iron was probably lost from when the

0:16:23.480 --> 0:16:26.000
<v Speaker 1>impactor hit the proto Earth, and some of that was

0:16:26.120 --> 0:16:28.320
<v Speaker 1>like melted and vaporized, and so it would have a

0:16:28.360 --> 0:16:31.440
<v Speaker 1>bigger iron core otherwise. This became a much more popular

0:16:31.560 --> 0:16:34.080
<v Speaker 1>hypothesis after we went to the Moon and visited and

0:16:34.160 --> 0:16:36.320
<v Speaker 1>understood what it was made out of. And there's a

0:16:36.320 --> 0:16:38.720
<v Speaker 1>lot of really interesting physics there that's relevant to it,

0:16:38.800 --> 0:16:41.760
<v Speaker 1>Like why doesn't it all just collapse into a planet, right,

0:16:41.920 --> 0:16:44.680
<v Speaker 1>Why doesn't it all just become one huge giant planet.

0:16:44.720 --> 0:16:46.760
<v Speaker 1>How come part of it ended up as a ring?

0:16:46.840 --> 0:16:48.960
<v Speaker 1>And that's just because you know, the whole thing is

0:16:49.000 --> 0:16:51.600
<v Speaker 1>spinning and a lot of it has angular momentum, and

0:16:51.680 --> 0:16:54.240
<v Speaker 1>so some stuff was just moving too fast to fall

0:16:54.240 --> 0:16:57.000
<v Speaker 1>in the way, like the moon now is moving too

0:16:57.040 --> 0:16:59.640
<v Speaker 1>fast to fall into the Earth. It's all about that.

0:17:00.520 --> 0:17:02.960
<v Speaker 1>And then when that stuff gathered together into a moon,

0:17:03.160 --> 0:17:07.720
<v Speaker 1>that stuff was spinning. So the moon had some original spin, right,

0:17:07.760 --> 0:17:10.239
<v Speaker 1>that came from the spinning motion of all of that

0:17:10.359 --> 0:17:14.000
<v Speaker 1>stuff after the vaporization. And we think that spin rate

0:17:14.080 --> 0:17:17.560
<v Speaker 1>originally was much much higher than it is today. So

0:17:17.600 --> 0:17:20.640
<v Speaker 1>the Moon used to be spinning faster than it is now.

0:17:20.800 --> 0:17:23.640
<v Speaker 2>Was there this is maybe an unfair question. Was there

0:17:23.680 --> 0:17:27.280
<v Speaker 2>anything alive on Earth when it was spinning fast enough

0:17:27.280 --> 0:17:29.560
<v Speaker 2>that sometimes you'd see what is now the far side

0:17:29.560 --> 0:17:32.439
<v Speaker 2>of the moon. So like dinosaurs probably never saw the

0:17:32.440 --> 0:17:34.600
<v Speaker 2>far side of the moon, but did like the first

0:17:34.640 --> 0:17:36.560
<v Speaker 2>bacteria see the far side of the Moon. I mean,

0:17:36.560 --> 0:17:39.080
<v Speaker 2>I'm sure they don't see anything that far away, but

0:17:39.160 --> 0:17:40.119
<v Speaker 2>you know, could they have.

0:17:40.640 --> 0:17:43.560
<v Speaker 1>Yeah, it's possible. We don't really know exactly how old

0:17:43.640 --> 0:17:46.760
<v Speaker 1>life is on Earth, but it stretches back billions of years, right,

0:17:47.240 --> 0:17:49.800
<v Speaker 1>And so it's possible that there are critters that have

0:17:49.880 --> 0:17:52.240
<v Speaker 1>lived on Earth that have seen other parts of the Moon.

0:17:52.280 --> 0:17:55.240
<v Speaker 1>That's a very cool thought. Because the Earth has been

0:17:55.359 --> 0:17:59.720
<v Speaker 1>gradually slowing down the Moon's spin little by a little

0:17:59.720 --> 0:18:03.679
<v Speaker 1>every year, and the opposite is also true. But you know,

0:18:03.840 --> 0:18:08.080
<v Speaker 1>until nineteen fifty nine, no human had ever seen the

0:18:08.119 --> 0:18:10.719
<v Speaker 1>backside of the Moon. It was this like dark spot

0:18:10.800 --> 0:18:13.040
<v Speaker 1>in our vision that we just couldn't see, no matter

0:18:13.280 --> 0:18:15.399
<v Speaker 1>how many thousands of years we've been staring up at

0:18:15.440 --> 0:18:18.040
<v Speaker 1>the Moon. Nobody had ever laid eyes on the backside

0:18:18.119 --> 0:18:21.920
<v Speaker 1>until nineteen fifty nine, which feels really recent.

0:18:21.880 --> 0:18:23.399
<v Speaker 2>Right, And the Soviets did.

0:18:23.280 --> 0:18:25.040
<v Speaker 1>It, right, Yeah, they certainly did.

0:18:25.440 --> 0:18:27.840
<v Speaker 2>Yeah, they beat us there with the lunar program. Their

0:18:27.880 --> 0:18:29.760
<v Speaker 2>third one made it there. I think the first two

0:18:30.000 --> 0:18:32.480
<v Speaker 2>maybe blew up. That was a thing that happened a

0:18:32.520 --> 0:18:36.600
<v Speaker 2>lot for the Soviets. But anyway, so.

0:18:36.640 --> 0:18:38.880
<v Speaker 1>Sorry, no, there's a really fun set of stories there.

0:18:39.040 --> 0:18:41.439
<v Speaker 1>Maybe you know about because of your book research, that

0:18:41.480 --> 0:18:43.320
<v Speaker 1>the Soviets were there first, and so they got to

0:18:43.440 --> 0:18:45.240
<v Speaker 1>name a lot of stuff on the far side of

0:18:45.280 --> 0:18:47.600
<v Speaker 1>the Moon first. So they have all these Russian names

0:18:48.080 --> 0:18:51.119
<v Speaker 1>and that like really annoyed the Americans at the time.

0:18:51.359 --> 0:18:54.800
<v Speaker 1>And then you know, later this International Astronomical Union took

0:18:54.840 --> 0:18:56.840
<v Speaker 1>over the naming, so it wasn't all just you know,

0:18:57.200 --> 0:18:59.159
<v Speaker 1>named after kinds of vodka or whatever.

0:18:59.480 --> 0:19:05.280
<v Speaker 2>All now that's an unfair stereotype. Did the IAU change

0:19:05.359 --> 0:19:07.920
<v Speaker 2>any of the names that the Soviet program had put

0:19:07.960 --> 0:19:10.640
<v Speaker 2>in place, or they just like stopped the Soviets from

0:19:10.680 --> 0:19:11.600
<v Speaker 2>doing any more naming.

0:19:11.960 --> 0:19:13.600
<v Speaker 1>I think they just stopped them. And there's a lot

0:19:13.640 --> 0:19:16.359
<v Speaker 1>of respect, I think for the people who discover something

0:19:16.440 --> 0:19:18.520
<v Speaker 1>to name it. But then I think that the Soviets

0:19:18.520 --> 0:19:20.520
<v Speaker 1>were so far ahead that they didn't want them to

0:19:20.560 --> 0:19:23.520
<v Speaker 1>just like name the whole thing after their favorite Soviet

0:19:23.560 --> 0:19:24.639
<v Speaker 1>flower or whatever.

0:19:24.880 --> 0:19:28.000
<v Speaker 2>Thank, yes, there we go. That's good. That's good. I

0:19:28.000 --> 0:19:30.440
<v Speaker 2>think there is like a Gagarian and seas or something

0:19:30.520 --> 0:19:33.000
<v Speaker 2>like them. All Right, so we're gonna take a quick

0:19:33.000 --> 0:19:34.919
<v Speaker 2>break and then we'll talk about what they found on

0:19:34.960 --> 0:19:49.399
<v Speaker 2>the far side of the moon. The first time we

0:19:49.440 --> 0:19:50.680
<v Speaker 2>got to see the far side of the moon was

0:19:50.760 --> 0:19:54.640
<v Speaker 2>nineteen fifty nine. Not too long after that, the Apollo

0:19:54.760 --> 0:19:57.400
<v Speaker 2>astronauts were flying around the Moon and got to see

0:19:57.440 --> 0:20:00.399
<v Speaker 2>the far side. What kinds of things were on the

0:20:00.400 --> 0:20:02.080
<v Speaker 2>far side to see, Daniel.

0:20:01.880 --> 0:20:04.920
<v Speaker 1>Well, you know, in research, it's always exciting to see

0:20:04.920 --> 0:20:07.320
<v Speaker 1>something nobody's ever seen before because you don't know what's

0:20:07.359 --> 0:20:09.119
<v Speaker 1>going to be there. Right, Maybe it's like a crashed

0:20:09.160 --> 0:20:13.160
<v Speaker 1>alien battleship or some weird new geological formation. Right, your

0:20:13.160 --> 0:20:16.160
<v Speaker 1>imagination goes crazy when you're first landing on a spot

0:20:16.200 --> 0:20:19.000
<v Speaker 1>and seeing something no human has ever seen before. But

0:20:19.200 --> 0:20:22.560
<v Speaker 1>you know, in research, discoveries never guaranteed. Just because you

0:20:22.720 --> 0:20:25.879
<v Speaker 1>land on new shores doesn't mean you find something fascinating.

0:20:25.960 --> 0:20:28.040
<v Speaker 1>And in this case, basically we found that the far

0:20:28.119 --> 0:20:30.400
<v Speaker 1>side of the Moon has more rocks and more dust,

0:20:30.600 --> 0:20:33.160
<v Speaker 1>and it's not even very different from the front side

0:20:33.160 --> 0:20:35.439
<v Speaker 1>of the Moon. I mean there are more craters, there

0:20:35.440 --> 0:20:38.800
<v Speaker 1>are fewer of these like seas, these lunar lava flows,

0:20:38.960 --> 0:20:40.880
<v Speaker 1>but all in all, it's not that exciting.

0:20:41.200 --> 0:20:45.520
<v Speaker 2>Yeah, that's the moon, good old, dependable Moon.

0:20:46.040 --> 0:20:49.680
<v Speaker 1>And the first time anybody actually landed there was twenty nineteen,

0:20:49.920 --> 0:20:52.240
<v Speaker 1>like just a few years ago the Chinese put a

0:20:52.320 --> 0:20:54.800
<v Speaker 1>lander down and started to do a bunch of experiments.

0:20:55.160 --> 0:20:57.680
<v Speaker 1>So it's only recently we started to explore it in detail.

0:20:57.720 --> 0:20:59.879
<v Speaker 1>So you know, there's still hope to find that crashed

0:21:00.040 --> 0:21:01.359
<v Speaker 1>alien battleship or.

0:21:01.280 --> 0:21:04.240
<v Speaker 2>The aliens might be living in a lavatude. We could

0:21:04.240 --> 0:21:06.680
<v Speaker 2>find something even more exciting than what you've imagined.

0:21:06.840 --> 0:21:09.679
<v Speaker 1>Yeah, maybe so, Or maybe we could build something that

0:21:09.760 --> 0:21:12.920
<v Speaker 1>future aliens could land and discover for themselves, like people

0:21:13.000 --> 0:21:17.320
<v Speaker 1>are proposing building radio telescopes on the far side of

0:21:17.359 --> 0:21:20.840
<v Speaker 1>the moon looking out into space, because then you'd have

0:21:20.880 --> 0:21:23.480
<v Speaker 1>the whole moon to shield you from the noise of

0:21:23.520 --> 0:21:24.000
<v Speaker 1>the Earth.

0:21:24.200 --> 0:21:28.119
<v Speaker 2>From my perspective, that's an interesting prospect geopolitically, because if

0:21:28.119 --> 0:21:30.399
<v Speaker 2>you built one of those radio telescopes, it wouldn't work

0:21:30.440 --> 0:21:32.800
<v Speaker 2>as well if people put other stuff on that side

0:21:32.800 --> 0:21:36.720
<v Speaker 2>of the moon. So now there's like competition for that space.

0:21:36.800 --> 0:21:38.919
<v Speaker 2>And can you tell someone they can't use the far

0:21:39.000 --> 0:21:41.800
<v Speaker 2>side of the moon because your radio telescope is there. Anyway,

0:21:41.840 --> 0:21:43.720
<v Speaker 2>These things are complicated, but yes, it would be a

0:21:43.720 --> 0:21:45.119
<v Speaker 2>good place for a radio telescope.

0:21:45.240 --> 0:21:46.919
<v Speaker 1>Sounds like the kind of things a bunch of lawyers

0:21:46.920 --> 0:21:48.720
<v Speaker 1>in a conference room are going to hash out one day.

0:21:48.960 --> 0:21:50.359
<v Speaker 1>So the far side of the Moon is not that

0:21:50.600 --> 0:21:53.440
<v Speaker 1>exciting on its own, but it is fascinating to understand

0:21:53.560 --> 0:21:56.000
<v Speaker 1>why there is a far side of the moon. Before

0:21:56.000 --> 0:21:57.920
<v Speaker 1>we dig into that, I just want to clarify something

0:21:57.960 --> 0:22:01.480
<v Speaker 1>that's a common misunderstanding, which the difference between the far

0:22:01.600 --> 0:22:03.920
<v Speaker 1>side of the Moon and the dark side of the moon.

0:22:04.320 --> 0:22:05.720
<v Speaker 1>Also the Pink Floyd album.

0:22:05.760 --> 0:22:08.320
<v Speaker 2>I don't think anyone needs clarification. We all know about that,

0:22:09.440 --> 0:22:11.760
<v Speaker 2>and we've all probably seen the light show if we're

0:22:11.800 --> 0:22:13.159
<v Speaker 2>around forty years old.

0:22:13.920 --> 0:22:16.119
<v Speaker 1>So some people imagine that the far side of the

0:22:16.119 --> 0:22:18.240
<v Speaker 1>moon is also the dark side of the moon, that like,

0:22:18.480 --> 0:22:21.119
<v Speaker 1>this part of the moon never sees sunlight, which is

0:22:21.119 --> 0:22:23.639
<v Speaker 1>definitely not true. The dark side of the moon is

0:22:23.680 --> 0:22:25.960
<v Speaker 1>the side of the moon facing away from the Sun.

0:22:26.200 --> 0:22:28.080
<v Speaker 1>The far side of the moon is the side facing

0:22:28.119 --> 0:22:31.320
<v Speaker 1>away from the Earth, and those two often don't agree.

0:22:31.560 --> 0:22:33.119
<v Speaker 1>So when we have a full moon, the sun is

0:22:33.119 --> 0:22:36.240
<v Speaker 1>illuminating the entire side of the Moon that we are

0:22:36.280 --> 0:22:39.960
<v Speaker 1>seeing because the Sun is sort of behind us in space.

0:22:40.200 --> 0:22:42.040
<v Speaker 1>Then the back side of the moon, the far side

0:22:42.040 --> 0:22:44.960
<v Speaker 1>that we don't see, is also dark. But the opposite

0:22:44.960 --> 0:22:47.680
<v Speaker 1>scenario when the moon is totally dark when we see

0:22:47.720 --> 0:22:50.240
<v Speaker 1>a new moon, and that's because the far side of

0:22:50.240 --> 0:22:52.440
<v Speaker 1>the moon is totally lit up by the sun. Right

0:22:52.640 --> 0:22:55.359
<v Speaker 1>half of the moon is always lit up, it's just

0:22:55.400 --> 0:22:58.200
<v Speaker 1>sometimes not the side that we're seeing, So the far

0:22:58.280 --> 0:23:00.520
<v Speaker 1>side and the dark side are different. It would be

0:23:00.600 --> 0:23:03.320
<v Speaker 1>like a Gary Larsen Pink Floyd crossover event when they meet.

0:23:03.480 --> 0:23:05.320
<v Speaker 2>I'm pretty sure if you play Dark Side of the

0:23:05.320 --> 0:23:09.640
<v Speaker 2>Moon backwards it explains that.

0:23:09.640 --> 0:23:12.199
<v Speaker 1>That's how you understand the far side cartoons, right, you

0:23:12.240 --> 0:23:14.240
<v Speaker 1>have to listen to the dark side of the moon backwards.

0:23:14.320 --> 0:23:17.040
<v Speaker 2>Yeah, there was a lot of cross talk between the

0:23:17.240 --> 0:23:22.080
<v Speaker 2>arts back then. Okay, so how is this happening. The

0:23:22.080 --> 0:23:25.000
<v Speaker 2>moon was going faster, you said, and it's been slowing down.

0:23:25.960 --> 0:23:29.040
<v Speaker 2>Why has it slowed down to be exactly the same

0:23:29.240 --> 0:23:31.359
<v Speaker 2>rotation rate and stuff? What's going on?

0:23:31.520 --> 0:23:34.480
<v Speaker 1>So it's not a coincidence, right. Physics seems to like

0:23:34.560 --> 0:23:38.480
<v Speaker 1>this scenario, and it's called tidal locking because it's connected

0:23:38.520 --> 0:23:41.520
<v Speaker 1>to the concept of tidal forces, which are in effect

0:23:41.560 --> 0:23:44.040
<v Speaker 1>we see all the time in gravity. And it sounds complicated,

0:23:44.040 --> 0:23:46.080
<v Speaker 1>but it's really pretty simple. The only thing you really

0:23:46.160 --> 0:23:50.119
<v Speaker 1>have to understand is that gravity gets weaker as distances

0:23:50.200 --> 0:23:52.120
<v Speaker 1>get longer. So if you're further away from the Sun,

0:23:52.160 --> 0:23:54.439
<v Speaker 1>it's gravity is less powerful. As you get closer to

0:23:54.480 --> 0:23:57.200
<v Speaker 1>the Sun, it's gravity is more powerful. That makes sense.

0:23:57.560 --> 0:24:00.479
<v Speaker 1>But now imagine you're a pretty big object. Part of

0:24:00.480 --> 0:24:03.280
<v Speaker 1>you is closer to the Sun than another part, then

0:24:03.400 --> 0:24:06.159
<v Speaker 1>part of you is going to feel stronger gravity than

0:24:06.200 --> 0:24:08.240
<v Speaker 1>the other part. And this happens all the time, Like

0:24:08.280 --> 0:24:10.359
<v Speaker 1>if you are standing on the surface of the Earth,

0:24:10.680 --> 0:24:13.520
<v Speaker 1>then the Earth is pulling on your legs harder than

0:24:13.560 --> 0:24:16.159
<v Speaker 1>it's pulling on your head, right, and so that's a

0:24:16.200 --> 0:24:19.800
<v Speaker 1>tidal force because there's a difference there. You can actually

0:24:19.840 --> 0:24:21.600
<v Speaker 1>think about the Earth is sort of like trying to

0:24:21.640 --> 0:24:23.440
<v Speaker 1>pull your head off of your body.

0:24:23.680 --> 0:24:26.000
<v Speaker 2>Is this like many spaghetification?

0:24:26.359 --> 0:24:30.040
<v Speaker 1>Yes, exactly, when it's very powerful. When it's more powerful,

0:24:30.280 --> 0:24:33.520
<v Speaker 1>then the force is holding an object together, that's spaghetification.

0:24:33.640 --> 0:24:36.240
<v Speaker 1>And so when you get near a black hole, for example,

0:24:36.240 --> 0:24:39.600
<v Speaker 1>gravity is super powerful, and the difference between the gravity

0:24:39.640 --> 0:24:42.639
<v Speaker 1>at your feet and your head is much more dramatic

0:24:42.840 --> 0:24:45.080
<v Speaker 1>and much more powerful than the force is holding your

0:24:45.119 --> 0:24:47.920
<v Speaker 1>head on your body, and so it's effectively natural decapitation

0:24:48.320 --> 0:24:49.280
<v Speaker 1>or spaghetification.

0:24:49.640 --> 0:24:53.040
<v Speaker 2>But lucky for us, instead of death, we get.

0:24:52.800 --> 0:24:56.479
<v Speaker 1>The tie exactly, so you don't have to worry about that,

0:24:56.560 --> 0:24:58.760
<v Speaker 1>because the difference of the force of gravity on your

0:24:58.760 --> 0:25:01.160
<v Speaker 1>feet and on your head is very gentle, and your

0:25:01.200 --> 0:25:04.479
<v Speaker 1>neck is very powerful in comparison. But the moon is

0:25:04.560 --> 0:25:07.640
<v Speaker 1>pretty big, and so the difference between the gravitational force

0:25:07.680 --> 0:25:09.560
<v Speaker 1>on one side of the moon and on the other

0:25:10.240 --> 0:25:12.679
<v Speaker 1>is much stronger. And so what happens is that the

0:25:12.720 --> 0:25:16.000
<v Speaker 1>Earth basically turns the Moon a little bit into a football.

0:25:16.480 --> 0:25:18.760
<v Speaker 1>It like makes it a little bit all blong, because

0:25:18.800 --> 0:25:20.960
<v Speaker 1>it pulls on the closer bits more powerfully, and it

0:25:21.000 --> 0:25:23.320
<v Speaker 1>pulls on the further bits more gently, and has the

0:25:23.320 --> 0:25:25.919
<v Speaker 1>effect of sort of like stretching it out, making it

0:25:26.040 --> 0:25:28.479
<v Speaker 1>longer like a football instead of like a sphere.

0:25:28.760 --> 0:25:30.399
<v Speaker 2>This is another one of those things I'm surprised we

0:25:30.400 --> 0:25:32.080
<v Speaker 2>ever figured out, because when I look at the Moon,

0:25:32.119 --> 0:25:33.919
<v Speaker 2>I would not think football.

0:25:34.160 --> 0:25:36.320
<v Speaker 1>It's a subtle effect, right, It looks like a sphere,

0:25:36.320 --> 0:25:38.920
<v Speaker 1>but is slightly distorted by the gravity of the Earth,

0:25:39.080 --> 0:25:41.400
<v Speaker 1>and that has a big impact on how it spins,

0:25:41.480 --> 0:25:44.560
<v Speaker 1>because now it has a gravitational preference to be aligned

0:25:44.560 --> 0:25:47.080
<v Speaker 1>a certain way with the Earth. If it was a

0:25:47.080 --> 0:25:49.920
<v Speaker 1>perfect sphere, then the gravity on the object wouldn't change

0:25:49.960 --> 0:25:52.800
<v Speaker 1>as it spins. But if it has a bulge, then

0:25:52.840 --> 0:25:56.560
<v Speaker 1>gravity prefers that bulge to be aligned with the object,

0:25:56.640 --> 0:25:59.000
<v Speaker 1>sort of like gravity has a handle now on the

0:25:59.040 --> 0:26:02.760
<v Speaker 1>Moon to pull that bulge, so one point is towards

0:26:02.760 --> 0:26:04.720
<v Speaker 1>the Earth and one point is away from the Earth.

0:26:04.800 --> 0:26:08.879
<v Speaker 1>That's like gravitationally less energetic a configuration than having the

0:26:08.920 --> 0:26:09.680
<v Speaker 1>whole thing spin.

0:26:10.359 --> 0:26:12.000
<v Speaker 2>All right, Okay, so I'm trying to wrap my head

0:26:12.040 --> 0:26:15.439
<v Speaker 2>around this, and picturing things in my head is not

0:26:15.560 --> 0:26:17.480
<v Speaker 2>one of my stronger suits. But here we go. Okay,

0:26:17.480 --> 0:26:19.280
<v Speaker 2>so we prefer to have a grip on the handle.

0:26:19.640 --> 0:26:23.920
<v Speaker 2>Does the moon spin at a not constant speed where

0:26:23.960 --> 0:26:26.080
<v Speaker 2>like we hold on to the handle for a little longer.

0:26:26.280 --> 0:26:28.320
<v Speaker 2>I don't think that's what you're saying, And so what

0:26:28.359 --> 0:26:29.000
<v Speaker 2>am I missing?

0:26:29.200 --> 0:26:31.679
<v Speaker 1>So what happened initially is that the Earth started to

0:26:31.720 --> 0:26:34.680
<v Speaker 1>form these bulges on the Moon, and then the Moon

0:26:34.760 --> 0:26:37.480
<v Speaker 1>was spinning, and so these bulges were like ripples through

0:26:37.520 --> 0:26:40.400
<v Speaker 1>the surface of the Moon. There were like these waves

0:26:40.440 --> 0:26:43.320
<v Speaker 1>that pass through the Moon. But Earth is also pulling

0:26:43.359 --> 0:26:46.359
<v Speaker 1>on those bulges, right Like, if the Moon has a bulge,

0:26:46.400 --> 0:26:48.440
<v Speaker 1>it's like a football, and then it starts to spin

0:26:48.480 --> 0:26:51.000
<v Speaker 1>away from the Earth. The Earth is going to pull

0:26:51.240 --> 0:26:53.639
<v Speaker 1>on that nearest point a little bit and try to

0:26:53.680 --> 0:26:56.400
<v Speaker 1>pull it back, and that effectively moves the bulge through

0:26:56.440 --> 0:26:58.320
<v Speaker 1>the surface of the Moon a little bit, and so

0:26:58.400 --> 0:27:01.239
<v Speaker 1>that slows down the rotation of the Moon a little bit,

0:27:01.240 --> 0:27:03.320
<v Speaker 1>because the Earth is like tugging trying to pull that

0:27:03.359 --> 0:27:06.440
<v Speaker 1>point back towards it, and so that slows the moon

0:27:06.480 --> 0:27:09.720
<v Speaker 1>down a little bit. And eventually the Moon settles into

0:27:09.800 --> 0:27:13.320
<v Speaker 1>a pattern where these waves the bulge doesn't travel over

0:27:13.359 --> 0:27:17.200
<v Speaker 1>its surface anymore, like settles into one location. And that's

0:27:17.240 --> 0:27:18.520
<v Speaker 1>what the Earth prefers.

0:27:18.160 --> 0:27:20.199
<v Speaker 2>Gravitationally, Okay, I'm with you.

0:27:20.359 --> 0:27:23.160
<v Speaker 1>And so that's how gravity makes the Moon a little

0:27:23.200 --> 0:27:26.760
<v Speaker 1>bit pointy and also slows down its spin. It's like

0:27:26.880 --> 0:27:29.879
<v Speaker 1>stealing some of its energy a little bit to slow

0:27:29.960 --> 0:27:30.920
<v Speaker 1>down its spin.

0:27:31.200 --> 0:27:34.800
<v Speaker 2>But why does its spin get slowed down to exactly

0:27:35.000 --> 0:27:37.679
<v Speaker 2>the right amount, Like it seems like that should just

0:27:37.680 --> 0:27:39.040
<v Speaker 2>slow things down in general.

0:27:39.359 --> 0:27:41.720
<v Speaker 1>It does. It slows things down in general, but at

0:27:41.720 --> 0:27:44.080
<v Speaker 1>some point it starts spinning at just the right speed

0:27:44.160 --> 0:27:47.040
<v Speaker 1>so that the pointy bit is always pointing towards the Earth.

0:27:47.400 --> 0:27:49.600
<v Speaker 1>And then the Earth is happy, and the gravity of

0:27:49.640 --> 0:27:52.080
<v Speaker 1>the Earth no longer wants to slow down the spin

0:27:52.240 --> 0:27:54.119
<v Speaker 1>of the Moon because the point to bit is always

0:27:54.160 --> 0:27:56.639
<v Speaker 1>facing the Earth, and so gravity is happy, because it's

0:27:56.680 --> 0:27:59.000
<v Speaker 1>sort of like a ball rolling to the bottom of

0:27:59.040 --> 0:28:02.000
<v Speaker 1>a valley, happy when it's settled in the bottom of

0:28:02.040 --> 0:28:03.760
<v Speaker 1>the valley. So this is sort of like, you know,

0:28:03.800 --> 0:28:05.359
<v Speaker 1>you let a marble go at the top of a

0:28:05.440 --> 0:28:08.000
<v Speaker 1>hill and it's gonna roll down. It's gonna awesantly pass

0:28:08.080 --> 0:28:10.960
<v Speaker 1>the minimum, but eventually friction and everything it's gonna settle

0:28:11.000 --> 0:28:13.400
<v Speaker 1>down in the minimum, and the same thing happens. There's

0:28:13.440 --> 0:28:16.520
<v Speaker 1>like friction inside the Moon, and the Moon gets heated

0:28:16.600 --> 0:28:18.800
<v Speaker 1>up a little bit by this, and the Moon also

0:28:18.920 --> 0:28:21.879
<v Speaker 1>speeds up in its orbit because there's like conservation of

0:28:21.920 --> 0:28:24.720
<v Speaker 1>angular momentum. So you've slowed down the Moon's spin a

0:28:24.760 --> 0:28:27.160
<v Speaker 1>little bit, and you've sped up its orbit a little bit,

0:28:27.200 --> 0:28:29.760
<v Speaker 1>which is why the Moon's orbital radius is increasing a

0:28:29.840 --> 0:28:30.240
<v Speaker 1>little bit.

0:28:30.640 --> 0:28:33.840
<v Speaker 2>And so how rare is this? Like if Earth were

0:28:33.840 --> 0:28:37.520
<v Speaker 2>a little bit smaller, would this not happen? If there was,

0:28:37.640 --> 0:28:40.880
<v Speaker 2>like if Mars was a little closer, would this not happen?

0:28:41.000 --> 0:28:41.080
<v Speaker 1>Like?

0:28:41.240 --> 0:28:43.640
<v Speaker 2>How lucky are we that it worked out this way?

0:28:43.720 --> 0:28:45.800
<v Speaker 1>We're not that lucky. It's sort of the eventual fate

0:28:45.880 --> 0:28:49.120
<v Speaker 1>of almost every pair of bodies that orbit each other

0:28:49.160 --> 0:28:51.400
<v Speaker 1>for long enough. And in fact, we've done it to

0:28:51.440 --> 0:28:54.600
<v Speaker 1>the Moon, and eventually the Moon will do it to

0:28:54.680 --> 0:28:56.960
<v Speaker 1>the Earth. It's just a slower process.

0:28:57.280 --> 0:29:00.959
<v Speaker 2>Whoa like, how slow? Like are we gonna swallowed up

0:29:00.960 --> 0:29:04.080
<v Speaker 2>by the Sun before it happens? Or is my you know,

0:29:04.200 --> 0:29:07.160
<v Speaker 2>kid gonna see it before they turn eighty.

0:29:07.200 --> 0:29:11.080
<v Speaker 1>Yeah, so the Earth's rotation has already been significantly slowed

0:29:11.120 --> 0:29:14.080
<v Speaker 1>by this effect from the Moon. Over the four billion

0:29:14.200 --> 0:29:16.280
<v Speaker 1>years since the Earth and the Moon were formed, the

0:29:16.400 --> 0:29:19.840
<v Speaker 1>length of an Earth day has lengthened from six hours

0:29:20.040 --> 0:29:22.880
<v Speaker 1>to twenty four hours. So the Moon has made our

0:29:23.000 --> 0:29:25.960
<v Speaker 1>days four times longer. It's slowed down the Earth spin

0:29:26.080 --> 0:29:29.720
<v Speaker 1>by a big factor. And eventually, because the Moon keeps

0:29:29.760 --> 0:29:31.640
<v Speaker 1>tugging on the Earth and making it a little bit

0:29:31.680 --> 0:29:34.880
<v Speaker 1>longer than tugging on that handle as it passes, eventually

0:29:34.920 --> 0:29:38.600
<v Speaker 1>it's gonna make the Earth take forty seven days to spin.

0:29:39.080 --> 0:29:41.040
<v Speaker 1>And at that point, the Earth and the Moon will

0:29:41.080 --> 0:29:44.360
<v Speaker 1>both be tidally locked to each other, and the Moon

0:29:44.400 --> 0:29:47.200
<v Speaker 1>will only ever see the same face of the Earth.

0:29:47.520 --> 0:29:50.800
<v Speaker 2>I don't think that's very nice of the bit. I

0:29:51.000 --> 0:29:54.360
<v Speaker 2>like having days. Ah, so I'm glad that's not gonna

0:29:54.360 --> 0:29:55.440
<v Speaker 2>happen in my lifetime.

0:29:55.640 --> 0:29:57.760
<v Speaker 1>That would be fascinating, right because it would mean that

0:29:57.920 --> 0:29:59.640
<v Speaker 1>half of the Earth would see the Moon and the

0:29:59.680 --> 0:30:02.800
<v Speaker 1>other would never see it. If life evolved in that planet,

0:30:02.800 --> 0:30:04.880
<v Speaker 1>then like half of life wouldn't even know there was

0:30:04.920 --> 0:30:05.320
<v Speaker 1>a moon.

0:30:05.800 --> 0:30:07.880
<v Speaker 2>WHOA, I bet we'd have all sorts of different like

0:30:07.960 --> 0:30:10.760
<v Speaker 2>creation stories. If some of us had moons and some

0:30:10.800 --> 0:30:13.680
<v Speaker 2>of us didn't. That would be that would be fascinating.

0:30:13.840 --> 0:30:16.160
<v Speaker 1>Or imagine being an explorer and like settling around the

0:30:16.200 --> 0:30:18.880
<v Speaker 1>world and then discovering this huge thing floating in your sky.

0:30:19.000 --> 0:30:24.400
<v Speaker 1>You're like, what, that would be crazy, that would be

0:30:24.480 --> 0:30:26.640
<v Speaker 1>super amazing. But you're right, it's going to take a

0:30:26.640 --> 0:30:30.040
<v Speaker 1>long time. And well, before that happens, the Earth is

0:30:30.080 --> 0:30:32.360
<v Speaker 1>going to be eaten by the Sun, which is going

0:30:32.440 --> 0:30:34.840
<v Speaker 1>to end its life cycle in about five billion years,

0:30:35.120 --> 0:30:38.120
<v Speaker 1>turn into a red giant and absorb the Earth. So

0:30:38.320 --> 0:30:41.000
<v Speaker 1>the Moon is not powerful enough to make that happen

0:30:41.040 --> 0:30:41.800
<v Speaker 1>anytime soon.

0:30:42.160 --> 0:30:45.440
<v Speaker 2>Well, on the upbeat topic of the end of our planets,

0:30:45.920 --> 0:30:48.240
<v Speaker 2>let's take a break, and when we come back, you

0:30:48.280 --> 0:30:50.640
<v Speaker 2>can tell us if the other moons on the other

0:30:50.720 --> 0:30:53.080
<v Speaker 2>planets are doing this as well. If I live on Mars,

0:30:53.120 --> 0:31:08.960
<v Speaker 2>am i gonna see all of Phobos or not? Okay,

0:31:09.040 --> 0:31:12.640
<v Speaker 2>we're back. So, Daniel, the question that everybody wants to

0:31:12.680 --> 0:31:15.920
<v Speaker 2>know when we move to Mars, are we going to

0:31:16.000 --> 0:31:18.720
<v Speaker 2>see the far side of Phobos and Demos or what?

0:31:19.080 --> 0:31:21.040
<v Speaker 1>So this is a process that happens all over the

0:31:21.080 --> 0:31:24.840
<v Speaker 1>Solar System and all over the universe. Eventually, gravity will

0:31:24.880 --> 0:31:27.880
<v Speaker 1>do its bit and distort objects from spheres into like

0:31:27.960 --> 0:31:31.000
<v Speaker 1>gentle little footballs. It'll grab on those handles and it

0:31:31.000 --> 0:31:33.720
<v Speaker 1>will hidly lock stuff. And so as we look around

0:31:33.760 --> 0:31:36.640
<v Speaker 1>the Solar System, we notice that all of the big moons,

0:31:36.680 --> 0:31:40.680
<v Speaker 1>all of the twenty round moons that exist around planets,

0:31:40.920 --> 0:31:43.680
<v Speaker 1>are all tidally locked to their planet.

0:31:44.080 --> 0:31:47.080
<v Speaker 2>Only the round moons. And what causes the Moon to

0:31:47.120 --> 0:31:50.160
<v Speaker 2>be round, It's that it needs to be a certain size,

0:31:50.400 --> 0:31:50.960
<v Speaker 2>Is that right?

0:31:51.200 --> 0:31:53.240
<v Speaker 1>Yeah, If you're big enough, then gravity is going to

0:31:53.240 --> 0:31:56.320
<v Speaker 1>be powerful enough to pull down any big features, which

0:31:56.320 --> 0:31:59.400
<v Speaker 1>is why, for example, like neutron stars have no features

0:31:59.400 --> 0:32:01.720
<v Speaker 1>on them that are highiher than one millimeter. And the

0:32:01.800 --> 0:32:04.280
<v Speaker 1>larger the gravity, the harder it is to keep a

0:32:04.320 --> 0:32:07.200
<v Speaker 1>stack of stuff from falling down. And so if you're

0:32:07.200 --> 0:32:09.120
<v Speaker 1>a pretty small object, you don't have to be very

0:32:09.160 --> 0:32:11.720
<v Speaker 1>spherical because your gravity's pretty weak. If you're a big

0:32:11.800 --> 0:32:14.160
<v Speaker 1>object like the Moon or the Earth, then you're going

0:32:14.240 --> 0:32:17.440
<v Speaker 1>to end up as a sphere because stuff falls down basically,

0:32:17.720 --> 0:32:20.320
<v Speaker 1>and stuff falls down more when you have more gravity.

0:32:20.600 --> 0:32:23.680
<v Speaker 1>And so these round moons are technically not actually round, right,

0:32:23.680 --> 0:32:26.800
<v Speaker 1>They're a little bit footballish and they're all tidally locked

0:32:27.080 --> 0:32:30.000
<v Speaker 1>to their planet. Most of these also orbit pretty closely

0:32:30.040 --> 0:32:32.640
<v Speaker 1>and so their gravity is pretty powerful. And then example,

0:32:32.680 --> 0:32:35.360
<v Speaker 1>you raise like Phobos and Demos on Mars. These are

0:32:35.520 --> 0:32:39.240
<v Speaker 1>little moons and they're not very large, they're not very round,

0:32:39.400 --> 0:32:41.480
<v Speaker 1>and they're actually spending really really fast. And so while

0:32:41.520 --> 0:32:45.280
<v Speaker 1>Mars is doing its job to try to tidly lock them, Phobos,

0:32:45.320 --> 0:32:48.360
<v Speaker 1>for example, is not yet tidally locked, but it will be.

0:32:48.680 --> 0:32:51.200
<v Speaker 1>It will be eventually. It's going to happen to everybody.

0:32:51.520 --> 0:32:54.240
<v Speaker 2>So we've been talking about moon planets. Has it happened

0:32:54.280 --> 0:32:57.920
<v Speaker 2>to any sun and planets or planets yet?

0:32:58.200 --> 0:33:01.040
<v Speaker 1>Absolutely? It has absolutely will Right, the Sun is the

0:33:01.040 --> 0:33:03.400
<v Speaker 1>most powerful source of gravity in the Solar System, and

0:33:03.480 --> 0:33:05.720
<v Speaker 1>so it's not going to be left out of this party.

0:33:06.040 --> 0:33:09.400
<v Speaker 1>And it has mercury tidly locked in its grasp. But

0:33:09.440 --> 0:33:13.320
<v Speaker 1>it's actually fascinating. It's not quite the same way as

0:33:13.360 --> 0:33:16.200
<v Speaker 1>with the Earth and the Moon because mercury doesn't have

0:33:16.280 --> 0:33:19.880
<v Speaker 1>as circular an orbit. It's much more elliptical. The mercury

0:33:19.920 --> 0:33:23.080
<v Speaker 1>is tightly locked in this weird way. Instead of spinning

0:33:23.200 --> 0:33:25.880
<v Speaker 1>once every time it goes around the Sun, it spins

0:33:25.920 --> 0:33:29.280
<v Speaker 1>three times for every two revolutions around the Sun. And

0:33:29.320 --> 0:33:32.040
<v Speaker 1>this is not something we understood for a while because

0:33:32.120 --> 0:33:34.400
<v Speaker 1>we can't always see Mercury because it's so close to

0:33:34.440 --> 0:33:37.240
<v Speaker 1>the Sun. There's a few spots in its orbit when

0:33:37.240 --> 0:33:39.520
<v Speaker 1>it's like easy to see mercury, and so when people

0:33:39.560 --> 0:33:42.520
<v Speaker 1>were observing Mercury, they were always seeing the same side

0:33:42.520 --> 0:33:43.959
<v Speaker 1>of it, so they thought, oh, it must have been

0:33:43.960 --> 0:33:46.360
<v Speaker 1>a one to one tide locking. And it's only later

0:33:46.440 --> 0:33:49.160
<v Speaker 1>when we got more observations in Mercury did we notice, Oh, no,

0:33:49.200 --> 0:33:52.160
<v Speaker 1>it's doing this even weirder thing. That's because the orbit

0:33:52.240 --> 0:33:54.680
<v Speaker 1>is not circular, and so it can do another little

0:33:54.680 --> 0:33:56.920
<v Speaker 1>bit of spin as it gets further away, and then

0:33:56.960 --> 0:33:59.840
<v Speaker 1>it comes back around, but still it settles into this

0:34:00.080 --> 0:34:03.000
<v Speaker 1>really cool pattern, this three two tidal locking.

0:34:03.160 --> 0:34:05.719
<v Speaker 2>All right, So let's see, my very elderly mother. We're

0:34:05.800 --> 0:34:09.760
<v Speaker 2>on v I'm guessing Mercury is tidally locked in part

0:34:09.800 --> 0:34:12.920
<v Speaker 2>because it's so close to the Sun. So is Venus

0:34:13.080 --> 0:34:16.080
<v Speaker 2>the next closest to being tidally locked or is is

0:34:16.160 --> 0:34:17.160
<v Speaker 2>it tidally locked?

0:34:17.239 --> 0:34:20.920
<v Speaker 1>Also, Venus is next on the list to getting tidly locked.

0:34:21.080 --> 0:34:23.839
<v Speaker 1>It's not yet tidly locked. In fact, Venus has a

0:34:23.880 --> 0:34:27.440
<v Speaker 1>really weird orbit and spin. It takes five hundred and

0:34:27.480 --> 0:34:30.359
<v Speaker 1>eighty three days to go around the Sun, but it

0:34:30.400 --> 0:34:33.680
<v Speaker 1>takes two hundred and twenty four Earth days to rotate.

0:34:34.280 --> 0:34:38.080
<v Speaker 1>So like a Venus year only has one point nine

0:34:38.200 --> 0:34:42.319
<v Speaker 1>Venus days. Like you only see two sunrises and two

0:34:42.400 --> 0:34:43.919
<v Speaker 1>sunsets in a Venus year.

0:34:44.280 --> 0:34:46.640
<v Speaker 2>Huh, But that wouldn't bother you, because Venus would have

0:34:46.719 --> 0:34:50.200
<v Speaker 2>killed you in four or five different ways long before

0:34:50.239 --> 0:34:52.120
<v Speaker 2>you cared about whether the sunrise was coming.

0:34:53.160 --> 0:34:55.319
<v Speaker 1>That's right. But Venus is sot again there right, Like

0:34:55.360 --> 0:34:59.160
<v Speaker 1>it's spin is similar to its orbital period. We actually

0:34:59.160 --> 0:35:01.719
<v Speaker 1>think that's because of a collision that Venus was like

0:35:01.840 --> 0:35:05.160
<v Speaker 1>smacked into by something which really changed its spin. We

0:35:05.160 --> 0:35:06.799
<v Speaker 1>don't think there's been enough time for it to be

0:35:06.880 --> 0:35:09.360
<v Speaker 1>like almost tighly locked by the Sun. It takes a

0:35:09.400 --> 0:35:11.799
<v Speaker 1>much longer time because Venus is so far away from

0:35:11.800 --> 0:35:14.479
<v Speaker 1>the Sun and so small relative to the Sun.

0:35:14.760 --> 0:35:20.200
<v Speaker 2>All right, So we've done moon and planets. We've done

0:35:20.280 --> 0:35:26.080
<v Speaker 2>comparisons between the Sun and the planets. Is there any

0:35:26.120 --> 0:35:29.759
<v Speaker 2>other combination of tidally locked things for us to think about?

0:35:29.840 --> 0:35:32.360
<v Speaker 2>Can asteroids get tidly locked? For example?

0:35:32.680 --> 0:35:35.239
<v Speaker 1>They could, but it's much harder because their gravity is

0:35:35.239 --> 0:35:38.160
<v Speaker 1>so weak. Another really fascinating thing to look at are

0:35:38.320 --> 0:35:43.120
<v Speaker 1>things that have similar masses, like dwarf planets and their moons. So,

0:35:43.200 --> 0:35:46.319
<v Speaker 1>for example, Pluto no longer a planet, but it's still

0:35:46.360 --> 0:35:50.360
<v Speaker 1>a dwarf planet. It's got a pretty big moon, Sharon,

0:35:50.960 --> 0:35:54.600
<v Speaker 1>and these two things are mutually tightly locked already. So

0:35:54.640 --> 0:35:56.560
<v Speaker 1>if you're like on Pluto and you look up, you

0:35:56.680 --> 0:35:59.520
<v Speaker 1>always see the same side of the Moon. And if

0:35:59.560 --> 0:36:02.239
<v Speaker 1>you're on Moon and you look up, you always see

0:36:02.280 --> 0:36:03.760
<v Speaker 1>the same side of Pluto.

0:36:04.000 --> 0:36:04.239
<v Speaker 4>Oh.

0:36:04.320 --> 0:36:06.040
<v Speaker 2>Interesting to how many moons does Pluto have.

0:36:06.320 --> 0:36:08.360
<v Speaker 1>Oh, Pluto's got a bunch of moons, but most of

0:36:08.360 --> 0:36:11.680
<v Speaker 1>them rotate chaotically. They're too small to have been tidly

0:36:11.719 --> 0:36:14.279
<v Speaker 1>locked so far. But it's sort of beautiful to see

0:36:14.280 --> 0:36:16.840
<v Speaker 1>these things like orbiting their center of mass and facing

0:36:16.880 --> 0:36:18.280
<v Speaker 1>each other. It's kind of like a dance.

0:36:18.640 --> 0:36:20.799
<v Speaker 2>Yeah, that's awesome. It's beautiful.

0:36:20.880 --> 0:36:23.040
<v Speaker 1>And that's not the only example of a dwarf planet.

0:36:23.080 --> 0:36:26.600
<v Speaker 1>There's another one out there, a trans Neptunian object called Eris,

0:36:26.600 --> 0:36:28.880
<v Speaker 1>which is also a dwarf planet, and it's got a

0:36:28.880 --> 0:36:32.160
<v Speaker 1>pretty big moon called Dyspnomia, which happens to be the

0:36:32.280 --> 0:36:36.759
<v Speaker 1>second largest dwarf planet moon after Pluto's moon, and these

0:36:36.760 --> 0:36:38.799
<v Speaker 1>two are also tidly locked with each other.

0:36:39.080 --> 0:36:42.000
<v Speaker 2>That sounds like it's a pretty common thing for dwarf

0:36:42.040 --> 0:36:44.239
<v Speaker 2>planets to have moons, that know, because how many dwarf

0:36:44.239 --> 0:36:45.000
<v Speaker 2>planets are there.

0:36:45.120 --> 0:36:47.040
<v Speaker 1>There's a lot of dwarf planets out there. That's one

0:36:47.120 --> 0:36:49.759
<v Speaker 1>reason why Pluto isn't really a planet anymore, because we

0:36:49.840 --> 0:36:52.120
<v Speaker 1>discovered there's kind of a lot of them out there.

0:36:52.160 --> 0:36:53.800
<v Speaker 1>And if we call Pluto a planet, we've got to

0:36:53.840 --> 0:36:56.000
<v Speaker 1>call them all planets, and then we're going to have

0:36:56.040 --> 0:36:58.120
<v Speaker 1>a lot of planet and so you know, astronomers have

0:36:58.200 --> 0:37:00.759
<v Speaker 1>big arguments about where to draw the line, but there's

0:37:00.760 --> 0:37:02.200
<v Speaker 1>a lot of dwarf planets.

0:37:01.800 --> 0:37:03.560
<v Speaker 2>Out there, right, and like, how are we going to

0:37:03.640 --> 0:37:05.920
<v Speaker 2>have naemonic if there's twenty of one or something like?

0:37:05.960 --> 0:37:08.279
<v Speaker 2>We just no way, no way, all right. So that's

0:37:08.360 --> 0:37:12.160
<v Speaker 2>our solar system. This sounds like a fundamental physics thing.

0:37:12.280 --> 0:37:14.760
<v Speaker 2>So I'm guessing that when we look at other solar systems,

0:37:14.800 --> 0:37:16.040
<v Speaker 2>they've got the same thing going on.

0:37:16.239 --> 0:37:19.360
<v Speaker 1>Yes, exactly. We expect that the same thing will happen

0:37:19.400 --> 0:37:23.239
<v Speaker 1>to planets around other stars and to moons around those planets,

0:37:23.840 --> 0:37:25.920
<v Speaker 1>and because of sort of the way that we can

0:37:25.960 --> 0:37:29.520
<v Speaker 1>discover those exoplanets. We expect a lot of the ones

0:37:29.560 --> 0:37:33.040
<v Speaker 1>we've seen so far have been tidly locked. Like the

0:37:33.040 --> 0:37:36.000
<v Speaker 1>way that we discover these planets is by seeing their

0:37:36.040 --> 0:37:39.040
<v Speaker 1>impact on their star. Either they pass in front of

0:37:39.080 --> 0:37:41.719
<v Speaker 1>their stars, so they give like a little mini planetary

0:37:41.760 --> 0:37:45.000
<v Speaker 1>eclipse which dims the star a little bit, or they

0:37:45.040 --> 0:37:47.760
<v Speaker 1>wiggle the star because of the gravity of the planet

0:37:47.800 --> 0:37:50.640
<v Speaker 1>pulling on the star. So in both cases they have

0:37:50.719 --> 0:37:52.920
<v Speaker 1>to be pretty close to the star for us to

0:37:52.960 --> 0:37:55.120
<v Speaker 1>see it, which means that of all the planets out

0:37:55.160 --> 0:37:57.960
<v Speaker 1>there in the galaxy orbiting their stars, we're best at

0:37:57.960 --> 0:38:00.520
<v Speaker 1>seeing the ones that are closest to their stars, which

0:38:00.600 --> 0:38:03.200
<v Speaker 1>also means we're best at seeing the ones that are

0:38:03.239 --> 0:38:07.120
<v Speaker 1>probably tidally locked. And so astronomers have done a bunch

0:38:07.120 --> 0:38:09.480
<v Speaker 1>of calculations to understand the orbits of these things and

0:38:09.520 --> 0:38:12.800
<v Speaker 1>the masses and predict their tidle locking, and they expect

0:38:12.840 --> 0:38:15.920
<v Speaker 1>that a lot of these planets are tidly locked, maybe

0:38:16.000 --> 0:38:18.560
<v Speaker 1>one to one, maybe like three to two the way

0:38:18.560 --> 0:38:21.720
<v Speaker 1>Mercury is, or maybe like five to two. It depends

0:38:21.760 --> 0:38:24.080
<v Speaker 1>a lot on the eccentricity of the orbit. Wh's the

0:38:24.080 --> 0:38:27.000
<v Speaker 1>sort of gravitationally most preferred arrangement.

0:38:27.200 --> 0:38:29.640
<v Speaker 2>Would it be fair to say that it's too far

0:38:29.800 --> 0:38:32.440
<v Speaker 2>away for us to have been able outside of our

0:38:32.480 --> 0:38:36.360
<v Speaker 2>solar system to see planets and their moons being tidally locked,

0:38:36.360 --> 0:38:37.719
<v Speaker 2>and so the only thing we've been able to look

0:38:37.719 --> 0:38:40.680
<v Speaker 2>at so far is tidal locking with suns and planets.

0:38:40.840 --> 0:38:44.200
<v Speaker 1>Yeah, that's exactly right. Exo moons is a brand new

0:38:44.320 --> 0:38:47.520
<v Speaker 1>area of study. People looking for these moons around exo

0:38:47.600 --> 0:38:50.719
<v Speaker 1>planets super exciting and in the next few years, as

0:38:50.760 --> 0:38:53.080
<v Speaker 1>we turn on more and more space telescopes, we're going

0:38:53.120 --> 0:38:56.760
<v Speaker 1>to get more information about these planets and their moons

0:38:56.920 --> 0:38:58.680
<v Speaker 1>and we can start to measure their spin and to

0:38:58.760 --> 0:39:01.480
<v Speaker 1>understand this and to figure out like whether these planets

0:39:01.520 --> 0:39:04.040
<v Speaker 1>out there a lot more of them are tidly locked

0:39:04.120 --> 0:39:06.440
<v Speaker 1>or a lot less. You know, a question we always

0:39:06.520 --> 0:39:10.680
<v Speaker 1>have is is our solar system weird or is it typical?

0:39:11.160 --> 0:39:13.600
<v Speaker 1>Like in most cases, is it just the first couple

0:39:13.640 --> 0:39:15.960
<v Speaker 1>of planets closest to the Sun that are tidally locked,

0:39:16.000 --> 0:39:18.239
<v Speaker 1>which would align with our understanding and tell us that

0:39:18.280 --> 0:39:21.240
<v Speaker 1>our solar systems not that weird, or maybe would be surprised,

0:39:21.280 --> 0:39:23.720
<v Speaker 1>and we'll discover Oh my gosh, all those solar systems

0:39:23.719 --> 0:39:26.240
<v Speaker 1>out there, they're all tidly locked. What's going on. Something

0:39:26.400 --> 0:39:29.319
<v Speaker 1>is different from what we expect. You never know when

0:39:29.360 --> 0:39:31.480
<v Speaker 1>you go out in the universe and ask these questions

0:39:31.480 --> 0:39:33.400
<v Speaker 1>and look for the first time, if you're just going

0:39:33.440 --> 0:39:36.000
<v Speaker 1>to see like more dust and rubbel or something really

0:39:36.000 --> 0:39:36.760
<v Speaker 1>really exciting.

0:39:36.960 --> 0:39:39.520
<v Speaker 2>The universe is good at providing job security in the

0:39:39.560 --> 0:39:40.719
<v Speaker 2>form of new questions.

0:39:40.800 --> 0:39:43.120
<v Speaker 1>And it's not just stars and planets we can study.

0:39:43.120 --> 0:39:47.120
<v Speaker 1>We can also look at pairs of stars. We're used

0:39:47.120 --> 0:39:50.040
<v Speaker 1>to thinking about stars as like individual and you have

0:39:50.080 --> 0:39:52.520
<v Speaker 1>a solar system with one star at its core and

0:39:52.560 --> 0:39:55.719
<v Speaker 1>a bunch of planets, But actually there's lots of binary

0:39:55.800 --> 0:39:58.680
<v Speaker 1>star systems out there. And the reason is that stars,

0:39:58.719 --> 0:40:01.000
<v Speaker 1>when they're formed, it's a big cloud of gas and

0:40:01.080 --> 0:40:04.480
<v Speaker 1>dust which collapses, and typically you get multiple stars from

0:40:04.520 --> 0:40:06.680
<v Speaker 1>a big cloud of gas and dust. You have like

0:40:06.760 --> 0:40:11.160
<v Speaker 1>little gravitational seeds that start this runaway gravitational effect, and

0:40:11.200 --> 0:40:12.799
<v Speaker 1>you don't just have one seed, you have a bunch

0:40:12.800 --> 0:40:15.319
<v Speaker 1>of them, so you get like an stellar nursery makes

0:40:15.520 --> 0:40:17.959
<v Speaker 1>lots and lots of stars. So we have a whole

0:40:17.960 --> 0:40:21.400
<v Speaker 1>podcast episode about binary star systems and even like trinary

0:40:21.480 --> 0:40:23.960
<v Speaker 1>star systems. But the point is that lots of stars

0:40:24.000 --> 0:40:27.239
<v Speaker 1>out there have brothers and sisters they were born with

0:40:27.360 --> 0:40:30.680
<v Speaker 1>like twins, and so they're pretty close to another star,

0:40:30.960 --> 0:40:33.440
<v Speaker 1>which means that you can have pairs of stars that

0:40:33.480 --> 0:40:35.359
<v Speaker 1>are tidly locked to each other.

0:40:35.680 --> 0:40:36.760
<v Speaker 2>That's awesome.

0:40:36.960 --> 0:40:39.160
<v Speaker 1>Or if you have a really big planet, you could

0:40:39.200 --> 0:40:41.479
<v Speaker 1>have a planet and a star that are tidly locked

0:40:41.520 --> 0:40:44.000
<v Speaker 1>to each other, so the planet is always seeing the

0:40:44.040 --> 0:40:47.280
<v Speaker 1>same side of the star. Right, that could be weird.

0:40:47.719 --> 0:40:49.720
<v Speaker 2>Yeah, but we haven't seen that yet, Right.

0:40:49.719 --> 0:40:51.680
<v Speaker 1>We have not seen that yet. There's a star out

0:40:51.680 --> 0:40:55.319
<v Speaker 1>there Tao Buddhists, which we suspect is tidly locked to

0:40:55.520 --> 0:40:58.040
<v Speaker 1>its planet, but we're not one hundred percent sure of that.

0:40:58.120 --> 0:40:59.960
<v Speaker 1>But you know, this kind of stuff makes a difference

0:41:00.120 --> 0:41:03.040
<v Speaker 1>because it really changes the experience of being on a planet.

0:41:03.320 --> 0:41:05.919
<v Speaker 1>Like if Earth was tidly locked to the sun, we'd

0:41:06.000 --> 0:41:08.160
<v Speaker 1>have half of the Earth at sunshine all day, and

0:41:08.280 --> 0:41:10.680
<v Speaker 1>half of the Earth would be the dark side of

0:41:10.680 --> 0:41:12.600
<v Speaker 1>the Earth. The far side of the Earth would be

0:41:12.640 --> 0:41:15.240
<v Speaker 1>the dark side, you know where Pink Floyd plays concerts

0:41:15.280 --> 0:41:18.400
<v Speaker 1>and Gary Larson draws his cartoons, And that would be

0:41:18.440 --> 0:41:22.000
<v Speaker 1>the very very cold side of the Earth, right dead side,

0:41:22.040 --> 0:41:24.520
<v Speaker 1>the oh, the dead side exactly. And then you'd have

0:41:24.640 --> 0:41:26.880
<v Speaker 1>this ring around the middle of the Earth that was

0:41:26.920 --> 0:41:29.359
<v Speaker 1>like right on the edge, you'd be like permanent sunrise,

0:41:30.040 --> 0:41:32.360
<v Speaker 1>and that might be the only place on the planet

0:41:32.440 --> 0:41:34.439
<v Speaker 1>you could live because one side would be too hot

0:41:34.480 --> 0:41:36.160
<v Speaker 1>and one side would be too cold. And then you'd

0:41:36.160 --> 0:41:39.520
<v Speaker 1>have this like goldilocks ring around the planet that might

0:41:39.600 --> 0:41:40.400
<v Speaker 1>be hospitable.

0:41:40.560 --> 0:41:42.560
<v Speaker 2>Location, location, location.

0:41:44.480 --> 0:41:46.759
<v Speaker 1>Exactly. And so if that's the case on some of

0:41:46.760 --> 0:41:49.799
<v Speaker 1>these exoplanets, that means it'd be a lot harder for

0:41:49.960 --> 0:41:52.560
<v Speaker 1>life to form. Either they'd have to evolve to survive

0:41:52.719 --> 0:41:56.239
<v Speaker 1>very hot conditions or very cold conditions, or there'd only

0:41:56.280 --> 0:41:58.600
<v Speaker 1>be a thin strip of their planet that they could

0:41:58.600 --> 0:42:00.560
<v Speaker 1>live on, and you know, then there wouldn't be seasons.

0:42:00.560 --> 0:42:02.239
<v Speaker 1>In the same way, it would make for a very

0:42:02.280 --> 0:42:03.759
<v Speaker 1>different kind of biology.

0:42:04.040 --> 0:42:07.120
<v Speaker 2>It would make it easy to study extremophiles, though, because

0:42:07.160 --> 0:42:10.080
<v Speaker 2>you know exactly where you needed to go, just you know,

0:42:10.120 --> 0:42:11.879
<v Speaker 2>the cold ones are over there and the hot ones

0:42:11.920 --> 0:42:13.600
<v Speaker 2>are over there. But there probably wouldn't be a lot

0:42:13.600 --> 0:42:15.120
<v Speaker 2>of funding for science in a world like that.

0:42:16.280 --> 0:42:18.800
<v Speaker 1>You never know, right, and we have all these expectations

0:42:18.800 --> 0:42:21.160
<v Speaker 1>for what life would be like on these planets, because

0:42:21.200 --> 0:42:23.840
<v Speaker 1>we imagine what our life would be like on those planets.

0:42:23.880 --> 0:42:26.160
<v Speaker 1>But of course, if you evolve on those planets, you'd

0:42:26.160 --> 0:42:28.080
<v Speaker 1>think that's the normal way to live, and they would

0:42:28.239 --> 0:42:31.279
<v Speaker 1>think it's super duper weird for like your planet to

0:42:31.320 --> 0:42:34.880
<v Speaker 1>spin and get constantly bathed in sunlight, or for you

0:42:34.920 --> 0:42:37.560
<v Speaker 1>to have no control over whether you're seeing the sun

0:42:37.680 --> 0:42:40.239
<v Speaker 1>or not. Because on tidly locked planets, right, you don't

0:42:40.239 --> 0:42:42.960
<v Speaker 1>want sun, you just move to the backside. You want sun,

0:42:43.000 --> 0:42:44.920
<v Speaker 1>you move to the front side, totally up to you,

0:42:45.160 --> 0:42:48.320
<v Speaker 1>whereas here we're like at the mercy of celestial objects,

0:42:48.520 --> 0:42:51.120
<v Speaker 1>spin rates to determine when we see sun and when

0:42:51.120 --> 0:42:51.520
<v Speaker 1>we don't.

0:42:51.719 --> 0:42:53.480
<v Speaker 2>Yeah, I guess you get used to what you grew

0:42:53.560 --> 0:42:56.440
<v Speaker 2>up with. It sure seems like it's nice to have

0:42:56.480 --> 0:42:58.000
<v Speaker 2>a more moderate in between.

0:42:58.360 --> 0:43:01.560
<v Speaker 1>It certainly does. But in the end, the universe prefers

0:43:01.680 --> 0:43:04.279
<v Speaker 1>tidal luck, and given enough time gravity, it's going to

0:43:04.360 --> 0:43:06.880
<v Speaker 1>do its business, make everything round and then make it

0:43:06.920 --> 0:43:09.520
<v Speaker 1>a little bit footballish, and it's going to tug on

0:43:09.600 --> 0:43:14.160
<v Speaker 1>those gravitational handles until everything is tidly locked, unless, of course,

0:43:14.239 --> 0:43:17.440
<v Speaker 1>your son explodes and eats you before it can even happen,

0:43:17.520 --> 0:43:20.120
<v Speaker 1>but it's sort of the gravitational destiny of every other

0:43:20.239 --> 0:43:20.920
<v Speaker 1>kind of object.

0:43:21.200 --> 0:43:24.640
<v Speaker 2>And there's the ending that'll keep from listening.

0:43:26.400 --> 0:43:30.799
<v Speaker 1>And hopefully inspire a lot of crazy music and silly cartoons. Yes,

0:43:31.560 --> 0:43:34.200
<v Speaker 1>all right, Thanks very much everybody for exploring the physics

0:43:34.239 --> 0:43:36.680
<v Speaker 1>of tidal locking with us. It turns out to play

0:43:36.680 --> 0:43:38.759
<v Speaker 1>a big role in what it's like to live on

0:43:38.760 --> 0:43:40.800
<v Speaker 1>our planet, what it's like to look up at disguise

0:43:40.920 --> 0:43:44.880
<v Speaker 1>and understand the universe or wonder at its mysteries, and

0:43:44.920 --> 0:43:47.280
<v Speaker 1>it will continue to play a big role in life

0:43:47.320 --> 0:43:47.880
<v Speaker 1>on Earth.

0:43:47.960 --> 0:43:48.280
<v Speaker 2>Huzza.

0:43:48.480 --> 0:43:58.880
<v Speaker 1>Thanks for listening. Tune in next time. Thanks for listening,

0:43:58.920 --> 0:44:01.600
<v Speaker 1>and remember that Daniel and Jorge Explain the Universe is

0:44:01.640 --> 0:44:06.239
<v Speaker 1>a production of iHeartRadio. For more podcasts from iHeartRadio, visit

0:44:06.320 --> 0:44:10.360
<v Speaker 1>the iHeartRadio app, Apple Podcasts, or wherever you listen to

0:44:10.440 --> 0:44:11.440
<v Speaker 1>your favorite shows.