WEBVTT - Does the Moon have an atmosphere?

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<v Speaker 1>A Kelly, how was your family trip? Oh? It was

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<v Speaker 1>so much fun. Did you guys get to break out

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<v Speaker 1>of your usual routines experience something different? Yeah, And something

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<v Speaker 1>that was unusual for our kids was eating at restaurants.

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<v Speaker 1>We don't do a lot of that when we're at home,

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<v Speaker 1>and you know, we didn't do a lot of it

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<v Speaker 1>because of COVID and stuff. So that was new. And though,

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<v Speaker 1>what is it that your kids like about eating out

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<v Speaker 1>at restaurants? Aren't you guys like super good cooks at home? Well,

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<v Speaker 1>we keep me out of the kitchen for everyone's sake,

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<v Speaker 1>but that is a really good cook, so that's good.

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<v Speaker 1>But I think for the kids, they mostly like the

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<v Speaker 1>novelty of it, you know, the atmosphere. M Well, that's exciting,

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<v Speaker 1>but it doesn't actually bode very well for them as

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<v Speaker 1>future space colonists. No, I'm not following. What do you mean, Well,

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<v Speaker 1>I hear that restaurants on the moon have no atmosphere. Oh. Hi,

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<v Speaker 1>I'm Daniel. I'm a particle physicist and a professor at

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<v Speaker 1>U C Irvine, and I'm always in the mood for

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<v Speaker 1>a good space pun. I'm Kelly Weener Smith. I'm an

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<v Speaker 1>adjunct assistant professor at Grace University, and I am also

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<v Speaker 1>a fan of the puns, especially the moon based ones.

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<v Speaker 1>There's a lot of inappropriate moon based puns that we

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<v Speaker 1>can make right now. Yeah, sure, no, you and I

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<v Speaker 1>are pretty good at that. But what we're going to

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<v Speaker 1>keep it clean. We are definitely gonna keep it clean

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<v Speaker 1>as we examine the deep dark mysteries of the universe.

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<v Speaker 1>And welcome to the podcast. Daniel and Jorge explain the

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<v Speaker 1>universe in which we do exactly that, ask the biggest, darkest,

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<v Speaker 1>deepest questions about everything that's out there in the universe.

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<v Speaker 1>We don't want to sweep anything under the rug. We

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<v Speaker 1>want to expose it all to the blinding glare of

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<v Speaker 1>sunlight and make it all makes sense to you. My

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<v Speaker 1>usual host, Orgy can't be here today, so we are

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<v Speaker 1>delighted to have one of our regular co hosts, Kelly. Kelly.

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<v Speaker 1>Thank you very much for joining us today. I'm delighted

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<v Speaker 1>to be back, Okelly. When you're on the podcast, we're

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<v Speaker 1>often talking about space and about the wonders of the

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<v Speaker 1>night sky, putting people out there mentally sort of at night,

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<v Speaker 1>staring up in the stars, being amazed at everything that

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<v Speaker 1>we are seeing that's right, and then you turn it

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<v Speaker 1>into something about how we're all going to die. But yes,

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<v Speaker 1>we are usually looking up at the night sky and

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<v Speaker 1>having a sense of all about it all because one

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<v Speaker 1>of the things that I love about science is that

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<v Speaker 1>it lifts us up away from our everyday lives. It

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<v Speaker 1>forces us to turn our eyes skywords and think about

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<v Speaker 1>what's out there in the universe. Usually that's something we

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<v Speaker 1>do at night because during the day the sun is

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<v Speaker 1>so bright it keeps us from seeing everything that's out there.

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<v Speaker 1>That makes us wonder, that makes us as deep questions

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<v Speaker 1>about the very nature of the universe. But you know,

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<v Speaker 1>everything that's out there is also out there during the daytime,

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<v Speaker 1>and I remember that blew my mind when I was

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<v Speaker 1>a kid and I first learned that. But yeah, it's

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<v Speaker 1>all still out there, and sometimes you can see the

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<v Speaker 1>moon during the day. It always feels sort of inappropriate, though.

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<v Speaker 1>When you see the moon during the day, it feels

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<v Speaker 1>like you know you've caught somebody, like they're not supposed

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<v Speaker 1>to be there, Like they're tiptoeing to the fridge in

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<v Speaker 1>the middle of the night and you spotted them, or

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<v Speaker 1>like they don't know their place you know, like moon,

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<v Speaker 1>your place is at night, you're stepping on the Sun's toes,

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<v Speaker 1>and you know, it's not only the nighttime sky. That's

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<v Speaker 1>really fascinating, that's really amazing. That has a lot of

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<v Speaker 1>physics in it is what we can learn about the

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<v Speaker 1>nature of the universe and what's out there just by

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<v Speaker 1>looking up at the daytime sky. Oh well, what can

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<v Speaker 1>we learn? Well, one common question from kids, of course,

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<v Speaker 1>is why is the sky blue? You know, if the

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<v Speaker 1>Sun is just shining through space at us, what is

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<v Speaker 1>it that makes the sky blue? And so we've talked

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<v Speaker 1>about on the podcast a few times. It's a fascinating

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<v Speaker 1>interaction between the Sun's gas and the atmospheric gases. The

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<v Speaker 1>light that comes directly from the Sun is white light.

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<v Speaker 1>If you were out in space looking at the Sun,

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<v Speaker 1>it would mostly look why it maybe a little bit yellow,

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<v Speaker 1>but not all of that light passes through our atmosphere

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<v Speaker 1>equally well, when light hits gases in the atmosphere tends

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<v Speaker 1>to scatter, and it scatters more for the very high

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<v Speaker 1>frequency light, the blue or light, and that might make

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<v Speaker 1>you think, oh, well, we should see everything, but the

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<v Speaker 1>blue light like the blue should get reflected back into space,

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<v Speaker 1>and it does get reflected back into space, but it

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<v Speaker 1>also gets reflected down to the ground. So when you're

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<v Speaker 1>standing on the surface of the Earth and you're looking

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<v Speaker 1>up at the sky, you're seeing light that doesn't come

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<v Speaker 1>directly from the sun and sort of hid an atom

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<v Speaker 1>and bounce down to your eyeballs. So the reason that

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<v Speaker 1>our daytime sky is blue is because those gases bounce

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<v Speaker 1>the blue light down to our eyeballs. And can we

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<v Speaker 1>use this to figure out what the atmospheres of other

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<v Speaker 1>planets are made up just by looking at the color

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<v Speaker 1>that we see when we shine a telescope about them.

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<v Speaker 1>We totally can and we do exactly that. When exo

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<v Speaker 1>planets pass in front of their stars, the light goes

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<v Speaker 1>through their atmosphere and some of it bounces off and

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<v Speaker 1>some of it passes through, and some of it is absorbed.

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<v Speaker 1>It's a great way to understand what's in those exo

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<v Speaker 1>planet atmospheres. And so it's sort of like X raying

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<v Speaker 1>the atmosphere. Passing light through it is a great way

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<v Speaker 1>to figure out like what's there as a glow, what

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<v Speaker 1>does it absorbed, what does it reflect? I love the

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<v Speaker 1>idea of seeing a sunrise on an exo planet and

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<v Speaker 1>using that to figure out what's in the sky. And

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<v Speaker 1>you know, sunrise is on different planets all look very

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<v Speaker 1>different because the different planets have different atmospheres. And so

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<v Speaker 1>when I am looking up in the night sky recently,

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<v Speaker 1>I've been seeing a big red dot. Is that Mars

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<v Speaker 1>or is it Venus? And also when I see those colors,

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<v Speaker 1>is that the atmosphere I'm seeing or is that something

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<v Speaker 1>else that I'm seeing entirely, So, if you look up

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<v Speaker 1>in the night sky and you're seeing a red dot,

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<v Speaker 1>that's probably Mars, and Mars is definitely red. If you

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<v Speaker 1>were in a satellite orbiting Mars looking down, it would

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<v Speaker 1>look red to your eyeballs. It's not just like a

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<v Speaker 1>false color thing from satellite imagery that we take and

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<v Speaker 1>then change the way like James web Space Telescope images

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<v Speaker 1>are all false color. If your eyeballs were there where

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<v Speaker 1>James Webb Space Telescope is, you wouldn't be seeing those

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<v Speaker 1>images because those images are all infrared. They're all too deep,

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<v Speaker 1>too long wavelengths for your eyeball to even register. But

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<v Speaker 1>if your eyeballs were orbiting Mars, hopefully with the rest

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<v Speaker 1>of your body, you would see it as red. And

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<v Speaker 1>the reason there is not actually the atmosphere, because Mars

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<v Speaker 1>has almost no atmosphere. It's very very thin atmosphere. It's

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<v Speaker 1>because the surface of Mars itself is mostly red due

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<v Speaker 1>to the iron and the oxidization of it, so it's

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<v Speaker 1>covered in this red dust. And it's sort of amazing

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<v Speaker 1>that you can see it from the Earth's surface, right,

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<v Speaker 1>that this thing is so red that you can see

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<v Speaker 1>it from your backyard. That's incredible. And then the fact

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<v Speaker 1>that you so you said that it has very little atmosphere,

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<v Speaker 1>that makes me I have a pop culture question to

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<v Speaker 1>ask you. Someone told me that one of the things

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<v Speaker 1>they didn't like about the Martian was that with a

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<v Speaker 1>low atmosphere, if you had a big dust storm, it

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<v Speaker 1>wouldn't be strong enough to like knock over a rocket,

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<v Speaker 1>because low atmosphere means like far fewer molecules pushing against

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<v Speaker 1>things even in a big windstorm. So is that not

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<v Speaker 1>accurate about the Martian? This is this is absolutely vital stuff. Yeah,

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<v Speaker 1>it's definitely true that the atmosphere on Mars is very

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<v Speaker 1>very low, like less than one percent of the Earth's atmosphere,

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<v Speaker 1>and that means that the wind don't apply as much pressure,

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<v Speaker 1>so whin did the same velocity. For example, there just

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<v Speaker 1>aren't as many molecules bouncing off of you. But the

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<v Speaker 1>velocity can get very high, and there's also a lot

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<v Speaker 1>of dust in the atmosphere on Mars. You definitely do

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<v Speaker 1>have to worry about storms. Very high velocity windstorm on

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<v Speaker 1>Mars can do a lot of damage because all the

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<v Speaker 1>dust particles you can basically sand blast you. Right, I

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<v Speaker 1>don't know if the velocity is actually get high enough

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<v Speaker 1>to knock things over. We'll have to get Andy Weir

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<v Speaker 1>on the podcast and ask him that question. Well, you know,

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<v Speaker 1>I loved that book in that movie, and you're making

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<v Speaker 1>me feel better knowing that maybe that opening scene was feasible,

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<v Speaker 1>because I would hate to think it wasn't. But okay,

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<v Speaker 1>all right, let's let's get back to the important stuff.

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<v Speaker 1>But it does bring us to a really fascinating fact

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<v Speaker 1>about Mars, which is, if you're standing on the surface

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<v Speaker 1>of Mars Mars and you look down, of course it

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<v Speaker 1>looks red. But also if you look up, it looks red.

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<v Speaker 1>That is, the sky on Mars doesn't look blue like

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<v Speaker 1>it does on Earth. That's because Earth has this atmosphere

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<v Speaker 1>which scatters the blue light down to your eyeballs. But

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<v Speaker 1>Mars doesn't. This atmosphere is so thin that it doesn't

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<v Speaker 1>effectively scatter that light. So then why is it red

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<v Speaker 1>instead of like white from the sun. It's because of

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<v Speaker 1>all of the dust. Right, Mars doesn't have much atmosphere,

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<v Speaker 1>but the dust is up there, and that dust tends

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<v Speaker 1>to absorb blue light. That's why it looks red. Remember,

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<v Speaker 1>things that look a certain color, they're reflecting that color

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<v Speaker 1>and they're absorbing everything else. So things that are yellow

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<v Speaker 1>are things that reflect yellow because the yellow makes it

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<v Speaker 1>to your eyeball and they absorb everything else. So it

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<v Speaker 1>sounds weird to say that red dust absorbs blue light.

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<v Speaker 1>You might think that makes it blue, right, but actually

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<v Speaker 1>that's what makes it red. So when you look up

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<v Speaker 1>in the sky during the daytime on Mars, you're seeing

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<v Speaker 1>the red light reflected from that dust. I didn't realize

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<v Speaker 1>that the dust never settled enough for the sky to

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<v Speaker 1>not be red. That's incredible. It is incredible, And if

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<v Speaker 1>you're lucky enough to observe a sunset on Mars, then

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<v Speaker 1>you'll see an amazing blue sunset. Right. It's like totally

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<v Speaker 1>reversed from Earth because this dust scatters the red light,

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<v Speaker 1>and so if you're looking directly at the sun sort of,

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<v Speaker 1>then most of the red light has been scattered away

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<v Speaker 1>by the dust, and so the blue light is all

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<v Speaker 1>that survives. So you see a blue sunset on Mars

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<v Speaker 1>on a red sky. Oh, that's incredible. I hope within

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<v Speaker 1>my lifetime we get photos of that taken by an

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<v Speaker 1>astronaut that landed on the Martian surface. Blue sunset. Selfie,

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<v Speaker 1>what an Instagram pick that will be in. And that

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<v Speaker 1>makes you wonder, like what it would be like to

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<v Speaker 1>be on other planets. Right, If the atmosphere of the

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<v Speaker 1>planet is what determines what it looks like to be

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<v Speaker 1>on the planet, the color of the daytime sky and

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<v Speaker 1>atmospheres can be like, you know, anything that opens the

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<v Speaker 1>door to like having all sorts of crazy daytime colors.

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<v Speaker 1>You know, can you have like a yellow sky or

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<v Speaker 1>a purple sky or something with crazy stripes from atmospheric bands? Right,

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<v Speaker 1>I haven't yet seen that in a science fiction movie.

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<v Speaker 1>You know, somebody living on Jupiter with the sky has

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<v Speaker 1>like stripes of color. That would be really awesome. And

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<v Speaker 1>there aren't many places in the solar system where we

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<v Speaker 1>have had people take pictures, right. One of those, of course,

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<v Speaker 1>is the moon. It's something that's striking about all of

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<v Speaker 1>the pictures from the moon, is that the sky the

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<v Speaker 1>backdrop or if you look above the moon, it's always black.

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<v Speaker 1>And why is that right? Because you associated black with

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<v Speaker 1>the color of the night sky, right, But even during

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<v Speaker 1>the moon sort of daytime, when the sun is shining

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<v Speaker 1>right at you, there's nothing there to scatter the light.

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<v Speaker 1>So from the point of view of somebody on the moon,

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<v Speaker 1>the sun is just another star. So it's sort of

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<v Speaker 1>like a perpetual night sky with one huge, very bright

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<v Speaker 1>star in it half the time. Also not very invited.

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<v Speaker 1>You wouldn't want to have a picnic under a black sky.

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<v Speaker 1>I feel like the regular would get in my sandwich

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<v Speaker 1>and was sort of mess up the overall feeling. So

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<v Speaker 1>the reason the night sky in the Moon is black

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<v Speaker 1>is because there isn't a strong enough atmosphere there on

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<v Speaker 1>the Moon to scatter it to make it blue or

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<v Speaker 1>purple or yellow at pink polka dots. But it does

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<v Speaker 1>raise an interesting question and the question of today's episode,

0:11:15.760 --> 0:11:24.640
<v Speaker 1>which is does the moon have an atmosphere? So this

0:11:24.720 --> 0:11:26.880
<v Speaker 1>is a fun question because it lets us dig into

0:11:26.960 --> 0:11:30.280
<v Speaker 1>definitions and quibble about what it means to have an

0:11:30.280 --> 0:11:35.080
<v Speaker 1>atmosphere for quibbling. Sometimes it feels to me like a

0:11:35.080 --> 0:11:37.280
<v Speaker 1>big part of science is just like arguing about what

0:11:37.320 --> 0:11:40.440
<v Speaker 1>a definition is, you know, like is this really a mammal?

0:11:40.520 --> 0:11:42.400
<v Speaker 1>I don't know what lays egg? What does that mean?

0:11:42.559 --> 0:11:45.839
<v Speaker 1>Whereas really that interesting questions are like the questions behind that,

0:11:45.920 --> 0:11:49.360
<v Speaker 1>you know, like why does something with hair lay eggs? Anyway, Yeah,

0:11:49.440 --> 0:11:51.120
<v Speaker 1>that was one of the most surprising things when I

0:11:51.120 --> 0:11:53.560
<v Speaker 1>started college, was like, wait a minute, we don't even

0:11:53.679 --> 0:11:57.280
<v Speaker 1>know how to define a species really and yeah, and

0:11:57.480 --> 0:12:00.680
<v Speaker 1>of course huge arguments over that, but know it's because

0:12:00.920 --> 0:12:03.360
<v Speaker 1>nature doesn't fit in the categories that humans would like

0:12:03.400 --> 0:12:06.280
<v Speaker 1>it to. Yeah, And sometimes those arguments are just a

0:12:06.320 --> 0:12:08.920
<v Speaker 1>waste of time, people splitting hairs where there's nothing really

0:12:08.920 --> 0:12:12.040
<v Speaker 1>to be learned. But sometimes it really is illuminating because

0:12:12.080 --> 0:12:15.319
<v Speaker 1>we do try to describe the universe in terms of categories.

0:12:15.480 --> 0:12:18.600
<v Speaker 1>These ways that we like to think about things are

0:12:18.640 --> 0:12:21.160
<v Speaker 1>sort of our familiar basis, and in the end, that's

0:12:21.160 --> 0:12:24.560
<v Speaker 1>what science is, is explaining everything we'd see in terms

0:12:24.600 --> 0:12:28.360
<v Speaker 1>of things we understand. Physics is describing the unfamiliar in

0:12:28.480 --> 0:12:31.079
<v Speaker 1>terms of the familiar. So the words we're using are

0:12:31.120 --> 0:12:33.160
<v Speaker 1>sort of important. If we're going to communicate with each

0:12:33.200 --> 0:12:35.400
<v Speaker 1>other about these ideas, we better at least know what

0:12:35.520 --> 0:12:37.719
<v Speaker 1>the words mean. And I guess, to be fair, I'm

0:12:37.720 --> 0:12:40.760
<v Speaker 1>thinking that I don't exactly know what an atmosphere starts

0:12:40.760 --> 0:12:42.840
<v Speaker 1>and stops, because it seems like sort of a gradient,

0:12:43.080 --> 0:12:45.319
<v Speaker 1>like is you know at what point do you call

0:12:45.360 --> 0:12:48.040
<v Speaker 1>it an atmosphere versus something else? And so I'm not

0:12:48.080 --> 0:12:50.120
<v Speaker 1>sure that I know the answer. So let's let's see

0:12:50.160 --> 0:12:53.400
<v Speaker 1>what your listeners think. Great idea, And so as usual,

0:12:53.440 --> 0:12:55.840
<v Speaker 1>I went out there into the internet to ask people

0:12:55.960 --> 0:12:59.040
<v Speaker 1>if they thought that the moon had an atmosphere. If

0:12:59.120 --> 0:13:02.319
<v Speaker 1>you like the artists made for future episodes of the podcast,

0:13:02.400 --> 0:13:05.080
<v Speaker 1>please don't be shy. Right to me two questions at

0:13:05.240 --> 0:13:07.880
<v Speaker 1>Daniel I and Jorge dot com, and I will set

0:13:07.920 --> 0:13:10.120
<v Speaker 1>you up. Is free. It's fun. Your friends can hear

0:13:10.160 --> 0:13:13.640
<v Speaker 1>your voice on the podcast. So before you hear these answers,

0:13:13.679 --> 0:13:17.280
<v Speaker 1>think to yourself, do you think the moon has an atmosphere?

0:13:18.400 --> 0:13:20.800
<v Speaker 1>Here's what people had to say. All right, so I

0:13:20.840 --> 0:13:23.200
<v Speaker 1>don't think that our moon has an atmosphere at least

0:13:23.240 --> 0:13:26.840
<v Speaker 1>anything substantial enough to call it an atmosphere. UM. I

0:13:26.840 --> 0:13:28.800
<v Speaker 1>did have a physics professor my first year of college

0:13:28.840 --> 0:13:31.000
<v Speaker 1>who claimed to have a plan to give the Moon

0:13:31.000 --> 0:13:34.360
<v Speaker 1>atmosphere for two hundred years by basically creating an orbital

0:13:34.480 --> 0:13:38.240
<v Speaker 1>cannon that could help a smaller Moon from either Jupiter Titan.

0:13:38.320 --> 0:13:40.160
<v Speaker 1>I have like an escape glossy of seventeen miles an

0:13:40.160 --> 0:13:44.160
<v Speaker 1>hour UH to slingshot that into ours vaporize and create

0:13:44.160 --> 0:13:46.880
<v Speaker 1>an atmosphere. But it wasn't only for two years, so

0:13:47.000 --> 0:13:50.080
<v Speaker 1>I can get implaced temporary and nothing substantial enough. I

0:13:50.120 --> 0:13:52.199
<v Speaker 1>don't think the Moon has an atmosphere. I mean there

0:13:52.320 --> 0:13:55.840
<v Speaker 1>might be some like low density hydrogen or something floating around,

0:13:55.960 --> 0:13:59.400
<v Speaker 1>but not enough to call it an atmosphere. I think

0:14:00.080 --> 0:14:07.160
<v Speaker 1>has some atmosphere UM only because I'm thinking that Moon

0:14:07.320 --> 0:14:11.560
<v Speaker 1>has a weak magnetic field that might be able to

0:14:11.840 --> 0:14:17.680
<v Speaker 1>contain some kind of atmosphere. There are so not what

0:14:17.960 --> 0:14:21.760
<v Speaker 1>Earth has, but still something. UM. I would guess it

0:14:21.800 --> 0:14:25.040
<v Speaker 1>probably does. I doubt it looks anything like ours does

0:14:25.080 --> 0:14:26.840
<v Speaker 1>on Earth, but I would guess that if you're a

0:14:27.600 --> 0:14:30.240
<v Speaker 1>body or an object in the sky, and you're large

0:14:30.320 --> 0:14:32.640
<v Speaker 1>enough or dense enough that you probably attract some kind

0:14:32.640 --> 0:14:36.360
<v Speaker 1>of atmosphere. The Moon doesn't have an atmosphere. I think

0:14:36.400 --> 0:14:42.440
<v Speaker 1>it's because it's gravitational attraction is too weak to um

0:14:43.640 --> 0:14:46.360
<v Speaker 1>sort of hold the guesses around it to form an atmosphere.

0:14:46.720 --> 0:14:48.360
<v Speaker 1>So what do you think of these answers? Kelly? A

0:14:48.360 --> 0:14:50.600
<v Speaker 1>lot of skepticism here, a lot of folks feeling like

0:14:50.640 --> 0:14:53.200
<v Speaker 1>the Moon can't really have much of an atmosphere. Yeah,

0:14:53.440 --> 0:14:55.280
<v Speaker 1>but a lot of critical thinking also, a lot of

0:14:55.280 --> 0:14:57.960
<v Speaker 1>folks trying to think through like, well, you know, I

0:14:58.000 --> 0:15:00.320
<v Speaker 1>think the moon has a weak magnetic field old, so

0:15:00.360 --> 0:15:04.000
<v Speaker 1>that wouldn't contain it. And yeah, so lots of good

0:15:04.040 --> 0:15:07.000
<v Speaker 1>thinking through the problem. Absolutely, And I love seeing people

0:15:07.000 --> 0:15:09.800
<v Speaker 1>apply their knowledge of physics to this question to come

0:15:09.880 --> 0:15:12.200
<v Speaker 1>up with an answer that they think makes sense, because

0:15:12.200 --> 0:15:14.240
<v Speaker 1>if the answer is not the one that you expect,

0:15:14.280 --> 0:15:17.000
<v Speaker 1>then there better to be an explanation for it. Right, That,

0:15:17.160 --> 0:15:20.280
<v Speaker 1>in the end, is what physics is all about. That's right.

0:15:20.640 --> 0:15:24.400
<v Speaker 1>So how about we start by talking about where atmosphere

0:15:24.400 --> 0:15:26.920
<v Speaker 1>has come from? How do you get an atmosphere? Well,

0:15:26.960 --> 0:15:29.360
<v Speaker 1>you go to Amazon dot com and you just type

0:15:29.360 --> 0:15:31.800
<v Speaker 1>in whatever you'd like, and you know, they deliver it.

0:15:32.000 --> 0:15:34.960
<v Speaker 1>I know so many space space element advocates who are

0:15:34.960 --> 0:15:36.480
<v Speaker 1>going to be so excited to know it's going to

0:15:36.560 --> 0:15:39.880
<v Speaker 1>be so easy on the Moon or Mars. It's surprising, Bezos,

0:15:39.920 --> 0:15:42.520
<v Speaker 1>isn't saying more about this on Mars. Isn't the plans

0:15:42.640 --> 0:15:44.920
<v Speaker 1>just like nuke the polar ice caps? Isn't that like

0:15:45.000 --> 0:15:47.640
<v Speaker 1>step one in getting a Martian atmosphere? You know that

0:15:47.640 --> 0:15:50.800
<v Speaker 1>that has been proposed, but I'm fairly certain the international

0:15:50.840 --> 0:15:53.760
<v Speaker 1>community has mixed feelings about that proposal, so I'm not

0:15:53.840 --> 0:15:55.760
<v Speaker 1>holding my breath. And also I think it makes it

0:15:55.840 --> 0:15:58.520
<v Speaker 1>uninhabitable for quite a while. But you know, if we've

0:15:58.520 --> 0:16:00.840
<v Speaker 1>got our great grandkids in mind, maybe it's maybe it's

0:16:00.840 --> 0:16:02.880
<v Speaker 1>a good plan. Yeah, we have a whole episode on

0:16:03.120 --> 0:16:06.360
<v Speaker 1>terra forming Mars and why that plan will not work.

0:16:06.520 --> 0:16:09.280
<v Speaker 1>So we're lucky we have such a nice atmosphere here

0:16:09.320 --> 0:16:10.720
<v Speaker 1>on Earth. And I think you're right. It's a good

0:16:10.720 --> 0:16:13.200
<v Speaker 1>idea to think about why Earth has an atmosphere and

0:16:13.240 --> 0:16:16.480
<v Speaker 1>why the Moon doesn't have at least the same atmosphere

0:16:16.560 --> 0:16:19.000
<v Speaker 1>as we do. And the interesting thing is that the

0:16:19.040 --> 0:16:22.200
<v Speaker 1>Earth sort of has had a few different atmospheres. The

0:16:22.240 --> 0:16:24.840
<v Speaker 1>Earth got its first atmosphere when it was just forming.

0:16:24.880 --> 0:16:27.000
<v Speaker 1>Remember that the whole Solar system just comes from a

0:16:27.040 --> 0:16:30.360
<v Speaker 1>big cloud of gas and dust and rock and little

0:16:30.360 --> 0:16:33.440
<v Speaker 1>bits from other solar systems and stars that died. Most

0:16:33.480 --> 0:16:36.200
<v Speaker 1>of it's just hydrogen left over from the Big Bang.

0:16:36.360 --> 0:16:38.120
<v Speaker 1>But you have this big cloud of gas and dust

0:16:38.200 --> 0:16:40.520
<v Speaker 1>in space, you have some blobs in it that are

0:16:40.520 --> 0:16:43.280
<v Speaker 1>a little denser than others, so they have stronger gravity.

0:16:43.480 --> 0:16:46.520
<v Speaker 1>They are pulling everything together, and that's the formation of

0:16:46.560 --> 0:16:49.040
<v Speaker 1>the Solar system. Of course, in the very center is

0:16:49.080 --> 0:16:51.520
<v Speaker 1>the Sun, which gathers in most of the gas and

0:16:51.560 --> 0:16:54.400
<v Speaker 1>the dust. But you also have other little blobs which

0:16:54.400 --> 0:16:57.320
<v Speaker 1>eventually formed planets, and they try to gather as much

0:16:57.320 --> 0:16:59.880
<v Speaker 1>stuff as they can before the Sun gobbles it all up.

0:17:00.000 --> 0:17:02.920
<v Speaker 1>You know. It's funny my intuition, and this is why

0:17:02.920 --> 0:17:05.679
<v Speaker 1>I didn't become a physicist. My intuition, Like, it feels

0:17:05.680 --> 0:17:09.240
<v Speaker 1>to me like gases shouldn't get pulled in by gravity,

0:17:09.280 --> 0:17:12.280
<v Speaker 1>but of course they are, and they should. But the

0:17:12.320 --> 0:17:15.919
<v Speaker 1>idea that gravity is holding our atmosphere on, I don't know.

0:17:15.960 --> 0:17:17.760
<v Speaker 1>It feels like the little molecule should be able to

0:17:17.800 --> 0:17:20.200
<v Speaker 1>just pop out in escape. But I'm glad that I'm

0:17:20.200 --> 0:17:22.280
<v Speaker 1>wrong about it. You're not actually wrong A lot of

0:17:22.320 --> 0:17:25.200
<v Speaker 1>them do escape, and the Earth is constantly boiling off

0:17:25.280 --> 0:17:28.840
<v Speaker 1>its atmosphere into space. It's a tenuous balance, right, The

0:17:28.880 --> 0:17:30.760
<v Speaker 1>Earth is pulling on those little guys, but they are

0:17:30.800 --> 0:17:33.879
<v Speaker 1>moving quickly, and the ones that have higher velocity and

0:17:34.040 --> 0:17:37.639
<v Speaker 1>higher altitudes definitely do escape. And in the very early

0:17:37.720 --> 0:17:40.160
<v Speaker 1>days of the Solar System, the Earth had an atmosphere

0:17:40.200 --> 0:17:43.560
<v Speaker 1>which came from these primordial gases, the hydrogen helium that

0:17:43.640 --> 0:17:46.080
<v Speaker 1>was just sort of like around, but it didn't last

0:17:46.119 --> 0:17:48.159
<v Speaker 1>for very long. It's not a very good atmosphere for

0:17:48.200 --> 0:17:51.000
<v Speaker 1>having an atmosphere, I guess you could say, because first

0:17:51.000 --> 0:17:52.800
<v Speaker 1>of all, the Sun was gobbling up most of the

0:17:52.880 --> 0:17:55.560
<v Speaker 1>hydrogen and the helium, and then once the Sun formed,

0:17:55.640 --> 0:17:58.639
<v Speaker 1>it was producing a lot of radiation which stripped the

0:17:58.640 --> 0:18:02.119
<v Speaker 1>inner planets of theirmosphere. So like solar wind and heat

0:18:02.400 --> 0:18:06.239
<v Speaker 1>from the Sun basically blasted the Earth's atmosphere away. So

0:18:06.240 --> 0:18:09.160
<v Speaker 1>it started off having a scoop of hygen and helium

0:18:09.160 --> 0:18:11.160
<v Speaker 1>and stuff that could have made an atmosphere, but then

0:18:11.160 --> 0:18:14.439
<v Speaker 1>it got blasted dry basically by the early Sun. So

0:18:14.680 --> 0:18:18.639
<v Speaker 1>is solar wind well named? Is it like the sun

0:18:18.920 --> 0:18:22.320
<v Speaker 1>is like and the stuff just sort of blows away?

0:18:22.480 --> 0:18:25.240
<v Speaker 1>Or is it more like the photons that come out

0:18:25.280 --> 0:18:27.679
<v Speaker 1>from the Sun. It's like a billiard table, and it

0:18:27.800 --> 0:18:30.159
<v Speaker 1>like knocks the hydrogen in the helium out of our

0:18:30.200 --> 0:18:32.800
<v Speaker 1>atmosphere when they like bounce into each other. I think

0:18:32.800 --> 0:18:36.960
<v Speaker 1>it's pretty well named because it's not just photons. It's protons,

0:18:37.040 --> 0:18:40.000
<v Speaker 1>it's electrons, it's actual particles. So if you think about

0:18:40.000 --> 0:18:43.480
<v Speaker 1>wind on Earth, it's like high moving particles that carry

0:18:43.520 --> 0:18:46.000
<v Speaker 1>momentum and it can push stuff over, and the solar

0:18:46.040 --> 0:18:49.000
<v Speaker 1>wind is really the same thing. It's stuff, it's matter

0:18:49.080 --> 0:18:52.119
<v Speaker 1>particles carrying momentum, and it could like push a solar sail,

0:18:52.480 --> 0:18:55.399
<v Speaker 1>and it definitely blasts things off of the Moon and

0:18:55.560 --> 0:18:58.240
<v Speaker 1>Mars and early Earth. Way to go, phus. This good

0:18:58.280 --> 0:19:01.000
<v Speaker 1>job name in that thing. And that's one reason why

0:19:01.040 --> 0:19:03.679
<v Speaker 1>you have, for example, rocky planets in the interior of

0:19:03.680 --> 0:19:06.000
<v Speaker 1>the Solar system, because that's the kind of stuff the

0:19:06.040 --> 0:19:09.800
<v Speaker 1>Sun couldn't blast off and like formed dense or blobs.

0:19:10.080 --> 0:19:11.919
<v Speaker 1>And in the outer part of the Solar system you

0:19:11.960 --> 0:19:14.520
<v Speaker 1>have the gas giants because they were far enough away

0:19:14.520 --> 0:19:16.560
<v Speaker 1>from the Sun to get to gobble up some of

0:19:16.560 --> 0:19:19.120
<v Speaker 1>their own gas and to hold onto it out there

0:19:19.119 --> 0:19:22.040
<v Speaker 1>where the solar radiation is weaker, So we got amosphere

0:19:22.119 --> 0:19:24.480
<v Speaker 1>very early on, and so did the Moon. As the

0:19:24.520 --> 0:19:28.119
<v Speaker 1>moon form from whatever primordial blobs made it. It also

0:19:28.200 --> 0:19:31.280
<v Speaker 1>must have had some helium and some hydrogen, but that

0:19:31.359 --> 0:19:34.240
<v Speaker 1>also was blasted clean by the Sun. So we both

0:19:34.280 --> 0:19:37.520
<v Speaker 1>started with an atmosphere and both lost our atmosphere very quickly,

0:19:37.640 --> 0:19:40.119
<v Speaker 1>and we both both of them lost it entirely or

0:19:40.119 --> 0:19:42.840
<v Speaker 1>did Earth retain some of it almost entirely, I mean

0:19:43.119 --> 0:19:45.880
<v Speaker 1>never completely dry. There must have been a little bit

0:19:45.880 --> 0:19:48.399
<v Speaker 1>of hydrogen floating around, but compared to the densities we

0:19:48.400 --> 0:19:51.800
<v Speaker 1>have today basically zero. Okay, Well, before we get into

0:19:51.840 --> 0:20:08.080
<v Speaker 1>what our second atmosphere was, like, let's take a break. Okay,

0:20:08.119 --> 0:20:12.639
<v Speaker 1>So the first atmosphere we had and we lost, but

0:20:12.760 --> 0:20:15.240
<v Speaker 1>we know that we get to hold onto one atmosphere eventually,

0:20:15.560 --> 0:20:18.080
<v Speaker 1>So what happens to the next atmosphere? This is like

0:20:18.119 --> 0:20:20.359
<v Speaker 1>a Disney movie. You know, there's a happy ending, right,

0:20:20.400 --> 0:20:22.760
<v Speaker 1>So even when there's ups and downs, you can sort

0:20:22.760 --> 0:20:26.000
<v Speaker 1>of hold on, just like life. Right. But we're telling

0:20:26.040 --> 0:20:29.280
<v Speaker 1>two stories simultaneously here. We're interested in whether the Moon

0:20:29.400 --> 0:20:31.439
<v Speaker 1>has an atmosphere, and we're telling the story of the

0:20:31.480 --> 0:20:34.359
<v Speaker 1>Earth and the Moon's atmosphere. Is in parallel to see

0:20:34.400 --> 0:20:37.199
<v Speaker 1>why they have different fates. So the Earth's got its

0:20:37.240 --> 0:20:40.160
<v Speaker 1>atmosphere is sort of rebooted from its interior. You had

0:20:40.160 --> 0:20:42.919
<v Speaker 1>like volcanoes and all sorts of crazy stuff happening on

0:20:42.960 --> 0:20:46.080
<v Speaker 1>the surface of the Earth which outgased like water and

0:20:46.200 --> 0:20:50.000
<v Speaker 1>CEO two and sulfur dioxide and nitrogen. So this is

0:20:50.040 --> 0:20:53.280
<v Speaker 1>like the Earth burping and giving itself an atmosphere just

0:20:53.440 --> 0:20:58.240
<v Speaker 1>from those burps. That makes it like substantially less beautiful

0:20:58.280 --> 0:21:01.760
<v Speaker 1>to watch the sunset. All those are Earth burps making

0:21:01.760 --> 0:21:04.240
<v Speaker 1>those colors. Yeah, and you know, let's go with burps

0:21:04.280 --> 0:21:06.800
<v Speaker 1>rather than any sort of other gaseous emission. But it's

0:21:06.840 --> 0:21:09.960
<v Speaker 1>incredible that there must have been so many volcanoes, so

0:21:10.040 --> 0:21:12.560
<v Speaker 1>much sort of tectonic action in the early Earth, that

0:21:12.640 --> 0:21:16.159
<v Speaker 1>you could release vast quantities of gas. Right. Did this

0:21:16.200 --> 0:21:18.439
<v Speaker 1>happen on Mars too? Or am I getting too far

0:21:18.480 --> 0:21:21.560
<v Speaker 1>afield by asking that because Morris has volcanoes too, Right, Yeah,

0:21:21.640 --> 0:21:23.520
<v Speaker 1>we think it happened on a lot of these planets.

0:21:23.720 --> 0:21:26.160
<v Speaker 1>And remember the scale though of the atmosphere. Even though

0:21:26.200 --> 0:21:28.840
<v Speaker 1>it seems vast to us and it seems dense, it's

0:21:28.840 --> 0:21:31.440
<v Speaker 1>really a very very thin layer on top of an

0:21:31.640 --> 0:21:35.439
<v Speaker 1>enormous sphere. Atmosphere goes up like a few hundred kilometers

0:21:35.480 --> 0:21:38.040
<v Speaker 1>depending on how you define it. But the Earth's radius

0:21:38.119 --> 0:21:42.080
<v Speaker 1>is six thousand kilometers, and so it's not that surprising

0:21:42.119 --> 0:21:45.479
<v Speaker 1>that all of that stuff could bubble up enough gas

0:21:45.520 --> 0:21:48.000
<v Speaker 1>to cover it with a very thin shell. It happened

0:21:48.040 --> 0:21:50.000
<v Speaker 1>on Earth, and it happened on Mars, and we also

0:21:50.040 --> 0:21:52.840
<v Speaker 1>think it might have happened on the Moon. The Moon

0:21:53.080 --> 0:21:56.000
<v Speaker 1>is not just like a lifeless, inert, frozen rock. It

0:21:56.160 --> 0:21:58.840
<v Speaker 1>had volcanoes. We can see this on the surface of

0:21:58.880 --> 0:22:01.960
<v Speaker 1>the Moon. There are all lava planes underneath the Moon.

0:22:02.000 --> 0:22:05.240
<v Speaker 1>There are these lava tubes, all sorts of crazy volcanic

0:22:05.280 --> 0:22:07.680
<v Speaker 1>stuff that happened on the Moon. How long ago did

0:22:07.720 --> 0:22:10.920
<v Speaker 1>the volcanic activity end, We don't know, and we don't

0:22:10.920 --> 0:22:13.480
<v Speaker 1>think that there are any active volcanoes right now. But

0:22:13.560 --> 0:22:16.960
<v Speaker 1>we have measured moon quakes, like you put these sensors

0:22:17.000 --> 0:22:19.720
<v Speaker 1>on the surface of the Moon and there are moon quakes,

0:22:19.840 --> 0:22:23.000
<v Speaker 1>right and that suggests, yeah, that there's stuff going on

0:22:23.160 --> 0:22:25.919
<v Speaker 1>inside the Moon, that there's internal magma, this stuff like

0:22:25.960 --> 0:22:28.679
<v Speaker 1>splashing around in there, which might mean you know, a

0:22:28.720 --> 0:22:31.920
<v Speaker 1>future volcanic action. Probably not, though across is probably now

0:22:32.000 --> 0:22:34.440
<v Speaker 1>cooled and sealed, and all that stuff is sunk too

0:22:34.440 --> 0:22:37.440
<v Speaker 1>far towards the center to ever crop up again. Will

0:22:37.480 --> 0:22:41.720
<v Speaker 1>it cool and stop moonquaking at some point? Eventually? Probably will. Yeah,

0:22:41.760 --> 0:22:44.359
<v Speaker 1>the same sort of thing is happening on Mars. Mars

0:22:44.400 --> 0:22:46.960
<v Speaker 1>and the Moon of course much much smaller than the Earth,

0:22:47.000 --> 0:22:49.320
<v Speaker 1>and so they cool faster. And we think, for example,

0:22:49.359 --> 0:22:52.280
<v Speaker 1>Mars still has some sort of liquid or at least

0:22:52.359 --> 0:22:54.960
<v Speaker 1>fluid core, and there's stuff going on inside there, because

0:22:54.960 --> 0:22:57.720
<v Speaker 1>we have measured Mars quakes as well. But there isn't

0:22:57.760 --> 0:23:01.439
<v Speaker 1>active volcanism on the Moon or on Mars, okay. And

0:23:01.520 --> 0:23:05.479
<v Speaker 1>so did the Moon lose its second atmosphere for the

0:23:05.520 --> 0:23:07.680
<v Speaker 1>same reason that it lost its first, or did the

0:23:07.720 --> 0:23:11.080
<v Speaker 1>volcanoes never give it an atmosphere to begin with? Yeah,

0:23:11.080 --> 0:23:13.400
<v Speaker 1>it's a great question. And so we have to understand

0:23:13.440 --> 0:23:15.840
<v Speaker 1>not just how you get an atmosphere, but how you

0:23:15.920 --> 0:23:18.840
<v Speaker 1>hold onto it right. It's not enough to just produce

0:23:18.880 --> 0:23:21.679
<v Speaker 1>the gases either from the first scoop of Solar system

0:23:21.760 --> 0:23:25.480
<v Speaker 1>stuff or remaking it again from volcanoes. You gotta hold

0:23:25.600 --> 0:23:28.440
<v Speaker 1>onto it right, because, as you say, there are things

0:23:28.480 --> 0:23:30.199
<v Speaker 1>out there in the Solar System that are trying to

0:23:30.240 --> 0:23:33.200
<v Speaker 1>get rid of your atmosphere, and so the solar wind

0:23:33.240 --> 0:23:35.840
<v Speaker 1>didn't stop, right. The solar wind was around in the

0:23:35.880 --> 0:23:38.720
<v Speaker 1>early days when things were forming, and it's still going

0:23:38.840 --> 0:23:42.639
<v Speaker 1>on today. And so their processes out there which remove atmospheres,

0:23:42.640 --> 0:23:46.600
<v Speaker 1>which work against having an atmosphere on the Earth and

0:23:46.880 --> 0:23:50.160
<v Speaker 1>on the Moon and on Mars. So this second atmosphere

0:23:50.200 --> 0:23:53.960
<v Speaker 1>that the Moon did have, unfortunately did get blown away. Sorry. Moon.

0:23:54.240 --> 0:23:58.280
<v Speaker 1>The story always seems so sad for the Moon. But

0:23:58.359 --> 0:24:00.840
<v Speaker 1>I think it's really interesting to understand sort of the

0:24:00.880 --> 0:24:04.119
<v Speaker 1>balance between those effects. I like thinking about it microscopically

0:24:04.160 --> 0:24:06.639
<v Speaker 1>the way you were. I think about the atmosphere and

0:24:06.760 --> 0:24:10.320
<v Speaker 1>individual particles of that gas, right, because in the end,

0:24:10.320 --> 0:24:13.440
<v Speaker 1>the atmosphere is not just like a huge blob of gas.

0:24:13.560 --> 0:24:16.760
<v Speaker 1>It really is made of individual particles. And the fate

0:24:16.800 --> 0:24:19.560
<v Speaker 1>of those individual particles is what determines the fade of

0:24:19.600 --> 0:24:21.720
<v Speaker 1>the atmosphere. And it's sort of weird to think about,

0:24:21.720 --> 0:24:26.560
<v Speaker 1>but gravity does operate on like individual atoms of gas, right,

0:24:26.600 --> 0:24:30.320
<v Speaker 1>Like the Earth pulls on each of those nitrogen atoms

0:24:30.320 --> 0:24:33.600
<v Speaker 1>and each of those oxygen atoms. It really is yanking

0:24:33.600 --> 0:24:36.000
<v Speaker 1>and keeping a lot of them on the surface. Of

0:24:36.040 --> 0:24:38.719
<v Speaker 1>the Earth, and that's of course, the biggest difference between

0:24:38.720 --> 0:24:41.719
<v Speaker 1>the Earth and the Moon is that the Earth is bigger,

0:24:41.800 --> 0:24:44.200
<v Speaker 1>it has more gravity, and it's a lot of our

0:24:44.200 --> 0:24:47.159
<v Speaker 1>listeners said, the Moon just doesn't have the gravity to

0:24:47.280 --> 0:24:50.840
<v Speaker 1>hold onto its atmosphere. Does the magnetosphere player roll too

0:24:50.920 --> 0:24:53.119
<v Speaker 1>or is it mostly about gravity. That's a really interesting

0:24:53.119 --> 0:24:56.760
<v Speaker 1>topic because the Earth's magnetic field does protect us from

0:24:56.800 --> 0:24:59.959
<v Speaker 1>the solar wind. Right, the solar wind are charged particle,

0:25:00.119 --> 0:25:03.280
<v Speaker 1>These are protons, these are electrons. What happens when a

0:25:03.359 --> 0:25:05.880
<v Speaker 1>charge particle hits a magnetic field is that it tends

0:25:05.920 --> 0:25:08.320
<v Speaker 1>to bend. And so when charge particles from the Sun

0:25:08.480 --> 0:25:11.680
<v Speaker 1>hit our magnetic field, they don't immediately just like slam

0:25:11.720 --> 0:25:15.320
<v Speaker 1>into our atmosphere. They spiral around these magnetic field lines,

0:25:15.359 --> 0:25:17.520
<v Speaker 1>and they go up to the north pole or down

0:25:17.560 --> 0:25:20.160
<v Speaker 1>to the south pole, and you finally see them as

0:25:20.200 --> 0:25:22.760
<v Speaker 1>like the Northern lights or the Southern lights. That's what

0:25:22.880 --> 0:25:26.440
<v Speaker 1>causes them, this magnetic field, and so initially you think, oh, well,

0:25:26.480 --> 0:25:29.320
<v Speaker 1>this must protect us. It's like a shield keeping our

0:25:29.359 --> 0:25:32.800
<v Speaker 1>atmosphere in place. That's sort of the prevailing view that

0:25:32.880 --> 0:25:36.320
<v Speaker 1>a big magnetic field will protect you like a shield.

0:25:36.400 --> 0:25:38.960
<v Speaker 1>But other people feel like, actually, a magnetic field is

0:25:39.000 --> 0:25:41.359
<v Speaker 1>sort of like a sale. It's going to capture a

0:25:41.400 --> 0:25:44.120
<v Speaker 1>lot of solar wind and funnel it into the planet,

0:25:44.160 --> 0:25:47.080
<v Speaker 1>helping strip the atmosphere, and so, like most things that

0:25:47.080 --> 0:25:50.680
<v Speaker 1>involved like more than one particle, the story is complicated

0:25:50.720 --> 0:25:53.000
<v Speaker 1>and people have differing opinions about it. But in the

0:25:53.040 --> 0:25:56.080
<v Speaker 1>case of the Moon, this very very little magnetic field there.

0:25:56.359 --> 0:25:59.440
<v Speaker 1>Like the Moon, we don't think has enough internal motion

0:25:59.640 --> 0:26:02.200
<v Speaker 1>in its core to generate a strong magnetic field. There

0:26:02.240 --> 0:26:04.480
<v Speaker 1>are magnetic rocks on the surface of the Moon, but

0:26:04.560 --> 0:26:07.760
<v Speaker 1>has no like big overall magnetic field to shield it

0:26:07.840 --> 0:26:10.240
<v Speaker 1>or to act like a sale. Are those magnetic rocks

0:26:10.320 --> 0:26:13.040
<v Speaker 1>big enough that you could try to address the question

0:26:13.080 --> 0:26:16.280
<v Speaker 1>about whether magnetic fields help or hurt atmospheres or no,

0:26:16.320 --> 0:26:18.359
<v Speaker 1>because there's just no atmosphere on the Moon, so you

0:26:18.400 --> 0:26:21.840
<v Speaker 1>can't compare like the area around magnetic rocks versus the

0:26:21.880 --> 0:26:24.760
<v Speaker 1>area around non magnetic rocks. Yeah, in order to operate

0:26:24.800 --> 0:26:26.359
<v Speaker 1>like a shield, I think you really do need to

0:26:26.359 --> 0:26:29.879
<v Speaker 1>have a planet sized magnetic field, um, and there just

0:26:30.040 --> 0:26:31.840
<v Speaker 1>isn't a coherent one on the Moon. I mean, if

0:26:31.840 --> 0:26:35.160
<v Speaker 1>you map the Moon's surface for magnetism, and they've done

0:26:35.200 --> 0:26:37.760
<v Speaker 1>that you do identify some spots with more magnetic field

0:26:37.800 --> 0:26:40.199
<v Speaker 1>or less. That's more probe of like what kind of

0:26:40.240 --> 0:26:43.200
<v Speaker 1>metals are there just under the surface, rather than telling

0:26:43.240 --> 0:26:45.840
<v Speaker 1>you anything about the planet's atmosphere. Arts was that the

0:26:46.000 --> 0:26:49.479
<v Speaker 1>end of our atmosphere story? Or is there a third phase?

0:26:49.800 --> 0:26:52.680
<v Speaker 1>So the Earth's atmosphere did keep evolving. Of course, now

0:26:52.680 --> 0:26:55.480
<v Speaker 1>we have oxygen in the Earth's atmosphere, which didn't come

0:26:55.520 --> 0:26:58.840
<v Speaker 1>from those volcanoes, right, That actually mostly came from life

0:26:58.840 --> 0:27:02.600
<v Speaker 1>when little cells begin into drink sunlight and do photosynthesis.

0:27:02.760 --> 0:27:05.880
<v Speaker 1>They turned a lot of the atmosphere into oxygen, though

0:27:05.920 --> 0:27:08.520
<v Speaker 1>surprisingly it took a long time. Right, You can't just

0:27:08.600 --> 0:27:11.440
<v Speaker 1>pump oxygen into the atmosphere and have it to stay

0:27:11.440 --> 0:27:14.840
<v Speaker 1>there because oxygen is so reactive. Most of the oxygen

0:27:14.880 --> 0:27:17.720
<v Speaker 1>that was produced by life actually got gobbled up by

0:27:17.880 --> 0:27:21.080
<v Speaker 1>rocks because rocks like to get oxydized. So if you

0:27:21.119 --> 0:27:24.760
<v Speaker 1>put oxygen in your atmosphere, it will weather. The rocks

0:27:25.080 --> 0:27:27.919
<v Speaker 1>are the surface of your planet will get like rusty,

0:27:28.000 --> 0:27:30.840
<v Speaker 1>for example, and that gobbles up a lot of the oxygen.

0:27:31.000 --> 0:27:33.440
<v Speaker 1>So it took hundreds of millions of years of pumping

0:27:33.480 --> 0:27:35.760
<v Speaker 1>oxygen into the atmosphere of the Earth before it had

0:27:35.800 --> 0:27:39.720
<v Speaker 1>like a measurable impact on what actually was in the atmosphere.

0:27:39.800 --> 0:27:45.440
<v Speaker 1>And today the Earth's atmosphere is mostly nitrogen. It's like oxygen,

0:27:45.720 --> 0:27:48.639
<v Speaker 1>and then like one percent argon point oh three percent

0:27:48.800 --> 0:27:51.199
<v Speaker 1>c O two and rising, and then a bunch of

0:27:51.200 --> 0:27:53.840
<v Speaker 1>other stuff. But the Moon, of course doesn't have life

0:27:53.880 --> 0:27:55.720
<v Speaker 1>on it, and it didn't have and it wasn't able

0:27:55.760 --> 0:27:58.240
<v Speaker 1>to keep that atmosphere around, and so it didn't get

0:27:58.240 --> 0:28:00.840
<v Speaker 1>to have the third act of its atmosphere. And is

0:28:00.880 --> 0:28:05.800
<v Speaker 1>there like a physics definition for when your atmosphere ends?

0:28:06.119 --> 0:28:10.119
<v Speaker 1>Is it like, you know, all what exactly kilometers the

0:28:10.200 --> 0:28:12.760
<v Speaker 1>atmosphere ends, or is it like a gradient where you

0:28:12.840 --> 0:28:14.520
<v Speaker 1>just have a little bit less and less as you

0:28:14.520 --> 0:28:17.120
<v Speaker 1>go and there's no clear cut off point. It's totally

0:28:17.160 --> 0:28:20.520
<v Speaker 1>a gradient. And there are definitions and they all disagree

0:28:20.520 --> 0:28:22.440
<v Speaker 1>with each other. You know. Some people say, oh, a

0:28:22.520 --> 0:28:25.440
<v Speaker 1>hundred kilometers, some people say no, the threshold should be

0:28:25.480 --> 0:28:28.359
<v Speaker 1>sixty five kilometers, and people argue endlessly about it, and

0:28:28.400 --> 0:28:31.360
<v Speaker 1>I'm not sure that we're really learning anything through that argument.

0:28:31.400 --> 0:28:34.040
<v Speaker 1>There are some interesting distinctions, like the Earth's atmosphere is

0:28:34.080 --> 0:28:38.000
<v Speaker 1>mostly within thirty kilometers of the surface, it's like of

0:28:38.000 --> 0:28:39.800
<v Speaker 1>the mass of the atmosphere. But you know, you could

0:28:39.840 --> 0:28:42.880
<v Speaker 1>draw that threshold anywhere, you could say nine or ninety

0:28:42.960 --> 0:28:44.840
<v Speaker 1>nine nine percent. In order to get all of it,

0:28:44.880 --> 0:28:47.720
<v Speaker 1>you have to go out like ridiculously far, you know,

0:28:47.800 --> 0:28:50.400
<v Speaker 1>hundreds of thousands of kilometers to say this is the

0:28:50.480 --> 0:28:53.040
<v Speaker 1>full envelope of the Earth. But there is an interesting

0:28:53.040 --> 0:28:56.880
<v Speaker 1>transition above a certain distance, the density is so low

0:28:57.200 --> 0:28:59.800
<v Speaker 1>that the atoms don't really bump into each other, and

0:28:59.800 --> 0:29:03.600
<v Speaker 1>so above what we call the atmosphere something called the exosphere,

0:29:03.760 --> 0:29:05.840
<v Speaker 1>where the density is so low that adams can travel

0:29:05.880 --> 0:29:09.320
<v Speaker 1>for like hundreds of kilometers without bouncing into each other.

0:29:09.360 --> 0:29:11.320
<v Speaker 1>So the dynamics of it are a little bit different.

0:29:11.320 --> 0:29:14.840
<v Speaker 1>It's collision lists. So usually where we get to by

0:29:14.840 --> 0:29:18.400
<v Speaker 1>the end of the episode, is you telling me something awful?

0:29:18.960 --> 0:29:22.160
<v Speaker 1>So now you've got me wondering is Earth going to

0:29:22.240 --> 0:29:26.560
<v Speaker 1>lose its atmosphere? So can you tell me about the ways,

0:29:26.560 --> 0:29:29.760
<v Speaker 1>like summarized for me, the ways that atmosphere gets lost,

0:29:30.320 --> 0:29:33.400
<v Speaker 1>and then is Earth gonna lose the atmosphere? Because probably

0:29:33.440 --> 0:29:37.840
<v Speaker 1>that's where this conversation is going. Right, your kids are

0:29:37.840 --> 0:29:40.680
<v Speaker 1>going to be fine, Kelly. Now, their kids and their

0:29:40.800 --> 0:29:42.600
<v Speaker 1>kids kids. You know, they're gonna have to listen to

0:29:42.640 --> 0:29:45.800
<v Speaker 1>the next generation of the podcast to find out. But

0:29:45.880 --> 0:29:48.360
<v Speaker 1>I think it's really fascinating to think about the dynamic

0:29:48.440 --> 0:29:51.400
<v Speaker 1>processes here and the things that are changing. The solar system.

0:29:51.720 --> 0:29:53.920
<v Speaker 1>We usually think of the solar system is so static.

0:29:53.960 --> 0:29:56.120
<v Speaker 1>It's just like this is the way it's been. It's

0:29:56.120 --> 0:29:59.040
<v Speaker 1>been this way for thousands or millions or maybe billions

0:29:59.080 --> 0:30:01.840
<v Speaker 1>of years, and so probably has always been this way,

0:30:02.280 --> 0:30:04.560
<v Speaker 1>and so there's always a little bit shocking and surprising

0:30:04.600 --> 0:30:07.800
<v Speaker 1>to discover that things are dynamic, that things are changing.

0:30:07.920 --> 0:30:10.200
<v Speaker 1>And the atmosphere is definitely in that category because it

0:30:10.320 --> 0:30:12.840
<v Speaker 1>is pretty tenuous. You know, it's not easy to hold

0:30:12.880 --> 0:30:15.200
<v Speaker 1>onto these gases, and there are a lot of factors

0:30:15.240 --> 0:30:17.120
<v Speaker 1>that are helped blowing it away. So we talked about

0:30:17.120 --> 0:30:19.640
<v Speaker 1>the solar wind. You know, something that people don't really appreciate,

0:30:19.720 --> 0:30:22.040
<v Speaker 1>I think is that the solar wind comes in like

0:30:22.120 --> 0:30:26.640
<v Speaker 1>a million miles per hour, these particles coming from the Sun. Yeah,

0:30:26.720 --> 0:30:29.880
<v Speaker 1>there's a bit along, right, and so like point one

0:30:30.040 --> 0:30:33.000
<v Speaker 1>five percent of the speed of light. It sounds like

0:30:33.040 --> 0:30:35.600
<v Speaker 1>a low value, but it's really really high. And nobody

0:30:35.640 --> 0:30:37.560
<v Speaker 1>wants to get shot at in the face with a

0:30:37.560 --> 0:30:41.040
<v Speaker 1>proton at a million miles per hour, I'll pass. And

0:30:41.080 --> 0:30:43.440
<v Speaker 1>even if we didn't have the Sun trying to strip

0:30:43.520 --> 0:30:46.600
<v Speaker 1>us of our atmosphere, right, it does just boil away.

0:30:46.680 --> 0:30:49.080
<v Speaker 1>There's gravity is powerful, but at the upper edges of

0:30:49.120 --> 0:30:51.840
<v Speaker 1>the atmosphere there are fast moving particles and they can

0:30:51.920 --> 0:30:54.440
<v Speaker 1>just achieve escape velocity. You know, you have a particle

0:30:54.560 --> 0:30:57.680
<v Speaker 1>going fast enough, pointed in the right direction, it's just gone.

0:30:58.080 --> 0:30:59.920
<v Speaker 1>You know, you don't have to launch it into out

0:31:00.000 --> 0:31:02.840
<v Speaker 1>of space. It's just hot and fast moving and it's

0:31:02.880 --> 0:31:07.040
<v Speaker 1>just taken off. And so this definitely happens for every planet,

0:31:07.040 --> 0:31:09.760
<v Speaker 1>and it happens also for Earth. No heavier planets is

0:31:09.800 --> 0:31:12.640
<v Speaker 1>gonna lose less because the escape velocity is higher. But

0:31:12.680 --> 0:31:16.280
<v Speaker 1>if you have lower mass gases like hydrogen and helium,

0:31:16.640 --> 0:31:19.800
<v Speaker 1>then they just boil off. Does it get replenished. It

0:31:19.840 --> 0:31:23.400
<v Speaker 1>doesn't really get replenished by new hydrogen or helium or oxygen.

0:31:23.680 --> 0:31:26.040
<v Speaker 1>That we do get a lot of space dust every year,

0:31:26.320 --> 0:31:28.960
<v Speaker 1>and so we get like tons of space dust, just

0:31:29.040 --> 0:31:32.920
<v Speaker 1>like debris falling to Earth, and we're also losing our atmosphere.

0:31:33.040 --> 0:31:37.560
<v Speaker 1>We lose three kilograms per second of hydrogen. That sounds

0:31:37.640 --> 0:31:41.560
<v Speaker 1>kind of scary, Okay, but we'll probably be fine. We're

0:31:41.560 --> 0:31:45.120
<v Speaker 1>gonna be fine for about a billion years until the Sun,

0:31:45.440 --> 0:31:48.120
<v Speaker 1>when it's gonna be like ten brighter than it is now,

0:31:48.360 --> 0:31:49.960
<v Speaker 1>is going to make it hot enough on Earth for

0:31:50.000 --> 0:31:52.720
<v Speaker 1>the oceans to boil, for water to break down into

0:31:52.800 --> 0:31:55.560
<v Speaker 1>hydrogen oxygen, and the Earth will probably lose a lot

0:31:55.600 --> 0:31:59.640
<v Speaker 1>of that hydrogen. Time to invest in interstellar travel, all right.

0:32:00.440 --> 0:32:02.560
<v Speaker 1>You know that news isn't as bad as some of

0:32:02.600 --> 0:32:04.760
<v Speaker 1>the news that you've delivered to me, But I still

0:32:04.800 --> 0:32:06.160
<v Speaker 1>think that we should take a break so that I

0:32:06.160 --> 0:32:21.479
<v Speaker 1>can recover for a moment. We'll be back soon. Okay,

0:32:21.520 --> 0:32:24.720
<v Speaker 1>we're back. Recap for me what we know about the

0:32:24.720 --> 0:32:27.880
<v Speaker 1>Moon's atmosphere. So we think that the Moon probably did

0:32:28.040 --> 0:32:31.520
<v Speaker 1>get a delivery of gas early on, right from the

0:32:31.560 --> 0:32:34.800
<v Speaker 1>primordial soup, and then it may have also gotten the

0:32:34.880 --> 0:32:38.720
<v Speaker 1>refreshing of its gas from volcanism. But we don't think

0:32:38.720 --> 0:32:41.880
<v Speaker 1>that there's much atmosphere there today, and the reason is

0:32:41.920 --> 0:32:44.920
<v Speaker 1>that it just doesn't have the mass to hold onto.

0:32:44.920 --> 0:32:47.560
<v Speaker 1>The stuff doesn't have the magnetic feel. So if you

0:32:47.800 --> 0:32:50.400
<v Speaker 1>ordered a new atmosphere for the Moon, if you like

0:32:50.440 --> 0:32:53.200
<v Speaker 1>went up there and pumped a bunch of oxygen and

0:32:53.320 --> 0:32:55.840
<v Speaker 1>nitrogen and c O two onto the Moon. Most of

0:32:55.880 --> 0:32:57.960
<v Speaker 1>it would get stripped away by the Sun or it

0:32:57.960 --> 0:33:00.600
<v Speaker 1>would just drift away because remember remember that the Moon

0:33:00.720 --> 0:33:03.440
<v Speaker 1>is really pretty tiny. I mean, it looks impressive in

0:33:03.480 --> 0:33:06.440
<v Speaker 1>the sky, but it's got like one percent of the

0:33:06.480 --> 0:33:09.360
<v Speaker 1>mass of the Earth, and its surface gravity is very,

0:33:09.440 --> 0:33:11.600
<v Speaker 1>very low, and so the escape velossity of the Moon

0:33:11.720 --> 0:33:13.560
<v Speaker 1>is just much lower than it is here on Earth,

0:33:13.600 --> 0:33:16.440
<v Speaker 1>which makes it easier for the stuff to boil away.

0:33:16.640 --> 0:33:18.479
<v Speaker 1>So I feel like I would have, you know, as

0:33:18.520 --> 0:33:21.120
<v Speaker 1>someone who thinks about terror forming a little, I would

0:33:21.120 --> 0:33:24.360
<v Speaker 1>have thought, well, maybe we can, at great, great, great, great, great,

0:33:24.400 --> 0:33:27.560
<v Speaker 1>great great great expense, give the Moon a magnetic field

0:33:28.280 --> 0:33:30.880
<v Speaker 1>to hold onto an atmosphere. But now what you've told

0:33:30.920 --> 0:33:33.200
<v Speaker 1>me is that physics doesn't have that figured out yet,

0:33:33.280 --> 0:33:35.560
<v Speaker 1>and a magnetic field may or may not help, So

0:33:35.600 --> 0:33:37.560
<v Speaker 1>there's maybe nothing we can do about the Moon not

0:33:37.640 --> 0:33:40.200
<v Speaker 1>having an atmosphere. Giving the Moon an atmosphere is definitely

0:33:40.240 --> 0:33:42.800
<v Speaker 1>a hopeless engineering project. I mean, you need to build

0:33:42.840 --> 0:33:45.080
<v Speaker 1>like a containment vessel, right, You need to like put

0:33:45.120 --> 0:33:48.280
<v Speaker 1>the whole Moon inside a glass bulb or something crazy.

0:33:48.360 --> 0:33:51.360
<v Speaker 1>Because it's not just that it doesn't have the gravity

0:33:51.400 --> 0:33:54.040
<v Speaker 1>to hold onto that gas envelope on its own. It's

0:33:54.040 --> 0:33:56.320
<v Speaker 1>a pretty harsh environment. I mean, the surface of the

0:33:56.320 --> 0:33:58.920
<v Speaker 1>Moon gets to like two hundred and fifty fahrenheit a

0:33:59.000 --> 0:34:01.760
<v Speaker 1>hundred and twenty cell see us during the day, which

0:34:01.800 --> 0:34:04.760
<v Speaker 1>makes it pretty easy to boil this stuff off, because remember,

0:34:04.800 --> 0:34:07.240
<v Speaker 1>it's a trade off between the temperature of the gas,

0:34:07.280 --> 0:34:10.680
<v Speaker 1>which means fast moving particles, and the gravity of the object.

0:34:10.719 --> 0:34:13.120
<v Speaker 1>If you have a small object, it's only hope for

0:34:13.239 --> 0:34:16.480
<v Speaker 1>holding onto its gas is if that gas is very cold,

0:34:16.600 --> 0:34:19.520
<v Speaker 1>meaning it's slow moving. But if the gas is hot

0:34:19.560 --> 0:34:22.200
<v Speaker 1>and the object is small, then that stuff is just

0:34:22.200 --> 0:34:24.400
<v Speaker 1>going to boil off into space. All right. I'm not

0:34:24.440 --> 0:34:26.919
<v Speaker 1>investing in that project. And people have been wondering about

0:34:26.960 --> 0:34:29.040
<v Speaker 1>the Moon's atmosphere for a long time. It's not for

0:34:29.040 --> 0:34:31.840
<v Speaker 1>a very long time that we've understood the source of

0:34:31.840 --> 0:34:34.279
<v Speaker 1>the Earth's atmosphere. This is a very complex story. It

0:34:34.320 --> 0:34:36.120
<v Speaker 1>took us a long time to piece together, and so

0:34:36.160 --> 0:34:38.560
<v Speaker 1>it wasn't until like the seventeen hundreds of people were

0:34:38.560 --> 0:34:41.600
<v Speaker 1>speculating about whether the Moon had an atmosphere, and people considered,

0:34:41.800 --> 0:34:44.480
<v Speaker 1>oh my gosh, maybe the Moon doesn't have any air

0:34:44.560 --> 0:34:46.520
<v Speaker 1>on it. They just for a long time assumed that

0:34:46.560 --> 0:34:48.880
<v Speaker 1>it would because the Earth did right, But it's not

0:34:48.920 --> 0:34:51.440
<v Speaker 1>actually that hard to tell even from the Earth that

0:34:51.480 --> 0:34:54.200
<v Speaker 1>the Moon must not have any atmosphere, and it's using

0:34:54.239 --> 0:34:56.440
<v Speaker 1>the same technique we talked about earlier. Remember, if we

0:34:56.480 --> 0:34:59.000
<v Speaker 1>are studying exoplanet, one thing we can do is look

0:34:59.040 --> 0:35:02.239
<v Speaker 1>at the light that passes through the atmosphere of those

0:35:02.239 --> 0:35:05.160
<v Speaker 1>exoplanets to see that there is an atmosphere and what's

0:35:05.200 --> 0:35:06.839
<v Speaker 1>in it. But you can do the same thing when

0:35:06.920 --> 0:35:09.040
<v Speaker 1>you look at the Moon. You can look at sunlight

0:35:09.080 --> 0:35:11.520
<v Speaker 1>that passes very very close to the Moon and see

0:35:11.880 --> 0:35:15.080
<v Speaker 1>is it absorbed, is it getting reflected, is it getting scattered.

0:35:15.239 --> 0:35:17.920
<v Speaker 1>You can basically use the sun as a probe of

0:35:18.000 --> 0:35:20.920
<v Speaker 1>what's right around the Moon. But we've been there, so

0:35:20.960 --> 0:35:23.680
<v Speaker 1>we don't have to rely on far off things. Didn't

0:35:23.680 --> 0:35:25.839
<v Speaker 1>they try to measure an atmosphere when they got there,

0:35:26.080 --> 0:35:28.000
<v Speaker 1>You're right, we have been there, and the Apollo missians

0:35:28.040 --> 0:35:31.480
<v Speaker 1>have a long series of experiments trying to measure things

0:35:31.520 --> 0:35:34.800
<v Speaker 1>on the Moon, looking for trace atmosphere and really finding

0:35:34.840 --> 0:35:38.719
<v Speaker 1>almost nothing. A Poulost seventeen saw a little bit of

0:35:38.760 --> 0:35:42.799
<v Speaker 1>evidence for UV emitting gases, but there's another big clue

0:35:42.840 --> 0:35:44.960
<v Speaker 1>about the Moon's atmosphere from the fact that we did

0:35:45.040 --> 0:35:47.920
<v Speaker 1>go there. You know, those footprints that people left on

0:35:47.960 --> 0:35:51.479
<v Speaker 1>the moon, they're still there. You like, write your name

0:35:51.520 --> 0:35:54.160
<v Speaker 1>in the sand on the Moon, and you could look

0:35:54.200 --> 0:35:56.239
<v Speaker 1>at it twenty years later from the surface of the

0:35:56.239 --> 0:35:59.239
<v Speaker 1>Earth and read your own handwriting, because there's basically no

0:35:59.480 --> 0:36:01.879
<v Speaker 1>whether on the moon, right, there's no wind of their

0:36:01.960 --> 0:36:04.720
<v Speaker 1>like blow things around, and so it's sort of amazing

0:36:04.760 --> 0:36:07.360
<v Speaker 1>that the rover tracks and the footprints they're all still

0:36:07.480 --> 0:36:09.800
<v Speaker 1>up there. You know, I've read that pizza hut was

0:36:09.840 --> 0:36:13.640
<v Speaker 1>looking into the cost estimate for like lasering its name

0:36:13.719 --> 0:36:19.279
<v Speaker 1>onto the moon. Yeah, it sounds like it would have

0:36:19.320 --> 0:36:21.759
<v Speaker 1>been a good long term investment because once it's up there,

0:36:21.880 --> 0:36:24.000
<v Speaker 1>it's not going away, right, But I think they did

0:36:24.080 --> 0:36:29.160
<v Speaker 1>determine it was probably not cost effective and actually might

0:36:29.239 --> 0:36:33.120
<v Speaker 1>make people angry, And in a million years archaeologists are

0:36:33.120 --> 0:36:35.719
<v Speaker 1>gonna be like, what is a pizza and why did

0:36:35.800 --> 0:36:39.400
<v Speaker 1>humans think to write about it on the moon? Right?

0:36:39.440 --> 0:36:41.640
<v Speaker 1>And why are they keeping it in a hut? Yeah?

0:36:43.000 --> 0:36:45.880
<v Speaker 1>Bad idea, bad idea. So it seems like when you

0:36:45.920 --> 0:36:49.120
<v Speaker 1>and I talk about something, the answer is never yes

0:36:49.719 --> 0:36:53.040
<v Speaker 1>or no. The answer is always something like yes but

0:36:54.600 --> 0:36:57.960
<v Speaker 1>or yes, well, so is is there a will? Is

0:36:58.000 --> 0:37:01.440
<v Speaker 1>there something sort of like an atmosphere? Sometimes where's the

0:37:01.480 --> 0:37:05.520
<v Speaker 1>well actually parked to this this episode? Yeah, there's definitely

0:37:05.520 --> 0:37:08.319
<v Speaker 1>a well actually varked to this episode, otherwise it would

0:37:08.320 --> 0:37:10.160
<v Speaker 1>have been very short. And the answer is that the

0:37:10.200 --> 0:37:13.840
<v Speaker 1>Moon technically doesn't have an atmosphere, but it does have

0:37:14.040 --> 0:37:17.360
<v Speaker 1>an exosphere. Remember earlier we were talking about the Earth

0:37:17.400 --> 0:37:20.680
<v Speaker 1>having an exosphere. Up above the atmosphere, there's this point

0:37:20.719 --> 0:37:23.200
<v Speaker 1>where there are gases, but they're very diffuse and very

0:37:23.239 --> 0:37:25.560
<v Speaker 1>low density, so they're not bumping into each other. The

0:37:25.600 --> 0:37:28.960
<v Speaker 1>Moon does have some gas particles and some other stuff

0:37:29.000 --> 0:37:32.160
<v Speaker 1>floating around near it in this envelope that don't bump

0:37:32.200 --> 0:37:34.359
<v Speaker 1>into each other. And so we can say the Moon

0:37:34.440 --> 0:37:36.920
<v Speaker 1>has an exosphere, and you might wonder, like, well, how

0:37:37.000 --> 0:37:39.480
<v Speaker 1>is it possible for it to hold onto its exosphere

0:37:39.520 --> 0:37:42.080
<v Speaker 1>if it can't hold onto an atmosphere, and it's part

0:37:42.080 --> 0:37:45.719
<v Speaker 1>of this fascinating dynamic story. Basically, it can't hold onto it,

0:37:45.760 --> 0:37:48.520
<v Speaker 1>but it has sources of new material at the same

0:37:48.600 --> 0:37:51.319
<v Speaker 1>time as it has sinks ways to get rid of it,

0:37:51.719 --> 0:37:55.839
<v Speaker 1>so it's constantly losing its exosphere and getting it replenished

0:37:56.239 --> 0:37:57.839
<v Speaker 1>tell me more about where it comes from. So it's

0:37:57.840 --> 0:38:02.480
<v Speaker 1>really a fun story. The Moon's exosphere actually comes from itself, right,

0:38:02.520 --> 0:38:05.040
<v Speaker 1>So things are constantly hitting the Moon, like you have

0:38:05.160 --> 0:38:08.279
<v Speaker 1>meteorites and then includes like really tiny little rocks that

0:38:08.280 --> 0:38:10.440
<v Speaker 1>are hitting the surface of the Moon. And we know

0:38:10.560 --> 0:38:12.080
<v Speaker 1>this is happening because you look up at the Moon

0:38:12.120 --> 0:38:14.680
<v Speaker 1>and it's covered with craters, right, which means that things

0:38:14.680 --> 0:38:17.000
<v Speaker 1>are constantly impacting it. Well, what happens if you don't

0:38:17.000 --> 0:38:19.320
<v Speaker 1>have very strong gravity and you get impacted with the

0:38:19.360 --> 0:38:21.879
<v Speaker 1>meteorite is that it sprays a bunch of stuff up

0:38:21.920 --> 0:38:25.600
<v Speaker 1>above the surface, and that stuff doesn't all immediately float

0:38:25.600 --> 0:38:27.799
<v Speaker 1>back down. Some of it's pretty light, and it's sort

0:38:27.800 --> 0:38:30.200
<v Speaker 1>of like hangs out there a little bit, like this

0:38:30.600 --> 0:38:34.000
<v Speaker 1>cloud of dust particles. So when when you say a

0:38:34.000 --> 0:38:39.040
<v Speaker 1>little bit, do you mean like decades or like that's

0:38:39.040 --> 0:38:41.480
<v Speaker 1>a great question. I think that for an individual particle,

0:38:41.520 --> 0:38:43.400
<v Speaker 1>it can vary a lot. Some of them might just

0:38:43.440 --> 0:38:45.640
<v Speaker 1>stay in the moon for minutes, some of them might

0:38:45.640 --> 0:38:49.520
<v Speaker 1>float around for days or years or decades. I don't

0:38:49.520 --> 0:38:51.080
<v Speaker 1>think that any of those things are going to last

0:38:51.120 --> 0:38:53.560
<v Speaker 1>for more than decades though, Okay, so it must be

0:38:53.560 --> 0:38:56.600
<v Speaker 1>getting pounded pretty often then, or does it have an

0:38:56.600 --> 0:38:59.840
<v Speaker 1>exosphere sometimes but not all the time. It has a

0:39:00.000 --> 0:39:02.880
<v Speaker 1>constant exosphere. But I have to emphasize that this is

0:39:03.080 --> 0:39:06.480
<v Speaker 1>very very low density. We're talking about like a few

0:39:06.560 --> 0:39:10.400
<v Speaker 1>hundred atoms per cubic centimeter. The Earth's atmosphere is like

0:39:10.480 --> 0:39:14.799
<v Speaker 1>ten to the nineteen particles per cubic centimeter, so we're

0:39:14.800 --> 0:39:18.440
<v Speaker 1>talking about something very very very very thin. You know,

0:39:18.560 --> 0:39:21.760
<v Speaker 1>the I S S the International Space Station, it flies

0:39:21.840 --> 0:39:25.200
<v Speaker 1>through the Earth's exosphere, which is about as dense. So

0:39:25.239 --> 0:39:27.960
<v Speaker 1>we're talking about the Moon having an exosphere which is

0:39:28.000 --> 0:39:30.120
<v Speaker 1>similar to like what you would feel if you stuck

0:39:30.160 --> 0:39:32.239
<v Speaker 1>your head out of the window and on the I.

0:39:32.520 --> 0:39:37.400
<v Speaker 1>S S, which I do not recommend remend you. So

0:39:37.440 --> 0:39:39.560
<v Speaker 1>if you have like a dog on the Moon in

0:39:39.600 --> 0:39:42.360
<v Speaker 1>your rover, and maybe you've called your dog rover, don't

0:39:42.440 --> 0:39:45.040
<v Speaker 1>encourage it to stick its head out because there's not

0:39:45.080 --> 0:39:47.719
<v Speaker 1>really a lot there. But it is really fascinating sort

0:39:47.760 --> 0:39:51.080
<v Speaker 1>of physics because it's not just like common fragments and meteorites.

0:39:51.320 --> 0:39:53.919
<v Speaker 1>It's other processes as well. We talked about the sun

0:39:54.320 --> 0:39:57.240
<v Speaker 1>blasting is free of an atmosphere, Well, that solar wind

0:39:57.320 --> 0:40:01.560
<v Speaker 1>also helps generate new atmosphere because each of those particles

0:40:01.640 --> 0:40:05.080
<v Speaker 1>hitting the surface of the Moon kicks up stuff from

0:40:05.120 --> 0:40:08.520
<v Speaker 1>the Moon's surface, right like knock stuff off the surface,

0:40:08.600 --> 0:40:10.920
<v Speaker 1>which then becomes part of the exosphere. Some of that

0:40:10.960 --> 0:40:13.640
<v Speaker 1>again settles back down, but some of it doesn't. Some

0:40:13.719 --> 0:40:16.320
<v Speaker 1>of it floats around for a while before then getting

0:40:16.320 --> 0:40:19.240
<v Speaker 1>like ionized by the Sun and then floating off into space.

0:40:19.560 --> 0:40:24.000
<v Speaker 1>Does it get like pushed in a certain direction by

0:40:24.120 --> 0:40:26.960
<v Speaker 1>the wind or is it just sort of like floating

0:40:26.960 --> 0:40:30.160
<v Speaker 1>off in all directions. So there's an envelope surrounding the

0:40:30.200 --> 0:40:32.400
<v Speaker 1>Moon of all of this stuff, and it's constantly getting

0:40:32.440 --> 0:40:35.000
<v Speaker 1>blown away. You know how commets have a tail, right,

0:40:35.040 --> 0:40:37.640
<v Speaker 1>They have a tail because the solar wind is pushing

0:40:37.640 --> 0:40:39.799
<v Speaker 1>them away. You imagine a comet has a tail because

0:40:39.840 --> 0:40:41.799
<v Speaker 1>it's like streaking through the sky and it's sort of

0:40:41.800 --> 0:40:43.680
<v Speaker 1>like comic book wiggles or motion behind it. With the

0:40:43.719 --> 0:40:46.800
<v Speaker 1>largest contribution for a comet's tail is actually the solar wind,

0:40:46.960 --> 0:40:49.000
<v Speaker 1>and so the tail points away from the Sun, not

0:40:49.120 --> 0:40:52.080
<v Speaker 1>always away from the direction of its motion. And the

0:40:52.160 --> 0:40:54.400
<v Speaker 1>same thing is true of the Moon. It has this

0:40:54.520 --> 0:40:58.200
<v Speaker 1>sort of short lived envelope that's constantly being refreshed, and

0:40:58.239 --> 0:41:00.920
<v Speaker 1>it also has a tail. We can now see it

0:41:01.040 --> 0:41:03.680
<v Speaker 1>from Earth using special telescopes that we have to like

0:41:03.920 --> 0:41:06.480
<v Speaker 1>block the light from the actual part of the Moon's surface,

0:41:06.520 --> 0:41:08.640
<v Speaker 1>so we can see just around it, like the corona

0:41:08.680 --> 0:41:11.400
<v Speaker 1>of the Moon. And they can see this envelope of

0:41:11.480 --> 0:41:14.279
<v Speaker 1>sodium around the Moon, and it has this tail that's

0:41:14.280 --> 0:41:17.439
<v Speaker 1>getting blown by the Sun away from the Moon. That's

0:41:17.480 --> 0:41:19.480
<v Speaker 1>so cool. I wish I could see that in real life.

0:41:20.360 --> 0:41:22.240
<v Speaker 1>If you google for it, there are these really cool

0:41:22.320 --> 0:41:24.520
<v Speaker 1>videos where you can see the Moon going around the

0:41:24.560 --> 0:41:27.040
<v Speaker 1>Earth and when the Moon is between the Earth and

0:41:27.080 --> 0:41:30.120
<v Speaker 1>the Sun, the Earth is in the Moon's tail. Right,

0:41:30.120 --> 0:41:35.600
<v Speaker 1>we're like eating the Moon's sodium dust is do we

0:41:35.640 --> 0:41:37.719
<v Speaker 1>retain any of it or does it just pass through?

0:41:38.040 --> 0:41:39.760
<v Speaker 1>We can retain it, you know, it just gets gathered

0:41:39.760 --> 0:41:42.320
<v Speaker 1>by the Earth. But again these are very very small amounts.

0:41:42.400 --> 0:41:44.120
<v Speaker 1>Is the reason it took us a long time to

0:41:44.280 --> 0:41:47.240
<v Speaker 1>even spot it. It was like that we first saw

0:41:47.280 --> 0:41:50.719
<v Speaker 1>the Moon's like sodium envelope and this tail. It takes

0:41:50.760 --> 0:41:53.640
<v Speaker 1>a long time. And one reason that they actually spotted

0:41:53.680 --> 0:41:56.480
<v Speaker 1>it is really cool is because of the landed meteor shower.

0:41:56.600 --> 0:41:58.640
<v Speaker 1>You know, when there's a meteor shower. It means like

0:41:58.680 --> 0:42:02.600
<v Speaker 1>spectacular things happening in our atmosphere. It also means more

0:42:02.760 --> 0:42:06.080
<v Speaker 1>things hitting the Moon's surface, which kicks up more stuff,

0:42:06.239 --> 0:42:09.919
<v Speaker 1>which enhances the Moon's exosphere and its tail. So during

0:42:09.960 --> 0:42:15.200
<v Speaker 1>the Leanded meteor shower, the Moon's exosphere was tripled in density,

0:42:15.440 --> 0:42:18.880
<v Speaker 1>heavy stuff, heavy stuff exactly. So there's a lot of

0:42:18.880 --> 0:42:21.600
<v Speaker 1>these processes going on, you know, like not just the

0:42:21.600 --> 0:42:25.799
<v Speaker 1>solar wind and commentary impact, also just photons. This is

0:42:25.840 --> 0:42:29.560
<v Speaker 1>fun process called desorption. You know, we're used to the

0:42:29.560 --> 0:42:32.680
<v Speaker 1>process of absorption where you can like gobble something up,

0:42:33.040 --> 0:42:35.920
<v Speaker 1>but desorption is when a photon hits something and it

0:42:36.040 --> 0:42:38.080
<v Speaker 1>kicks something off, just like when a meteor hits the

0:42:38.120 --> 0:42:40.000
<v Speaker 1>surface and kicks off a rock. Now we're talking about

0:42:40.000 --> 0:42:42.160
<v Speaker 1>a photon hitting an atom and giving it the energy

0:42:42.200 --> 0:42:44.719
<v Speaker 1>to like escape whatever bonds it was in and it

0:42:44.800 --> 0:42:47.399
<v Speaker 1>comes off the surface. And so the Moon has all

0:42:47.440 --> 0:42:51.640
<v Speaker 1>these various ways to replenish its exosphere and all these

0:42:51.640 --> 0:42:54.680
<v Speaker 1>ways to lose it. So it's like more like a flow, right,

0:42:54.680 --> 0:42:57.080
<v Speaker 1>It's not just like a gaseous pool. It's like the

0:42:57.160 --> 0:43:00.040
<v Speaker 1>stuff flowing off the Moon and getting a braid and

0:43:00.280 --> 0:43:02.840
<v Speaker 1>by everything that's around it. Does this mean that that

0:43:02.960 --> 0:43:07.240
<v Speaker 1>the other moons in the Solar System might also have tails?

0:43:07.280 --> 0:43:10.239
<v Speaker 1>Almost certainly every object in the Solar System has an

0:43:10.280 --> 0:43:13.279
<v Speaker 1>exo sphere because they're not just alone, right, They're all

0:43:13.360 --> 0:43:16.359
<v Speaker 1>in the Solar wind. They're all getting constantly bombarded by

0:43:16.400 --> 0:43:19.720
<v Speaker 1>little meteor fragments or big objects. So the Solar System

0:43:19.760 --> 0:43:22.080
<v Speaker 1>is a very dynamic place. And because of it, all

0:43:22.120 --> 0:43:25.960
<v Speaker 1>these things are constantly providing sources for their own exosphere

0:43:26.000 --> 0:43:28.560
<v Speaker 1>and then also losing them constantly. So we think that

0:43:28.600 --> 0:43:32.239
<v Speaker 1>for example, and slate Us in Europa, and Callisto and

0:43:32.320 --> 0:43:36.440
<v Speaker 1>Ganymede and even dwarf planets like Ceres in the Asteroid

0:43:36.480 --> 0:43:41.000
<v Speaker 1>Belt probably have their own little exosphere. Not quite an atmosphere, right,

0:43:41.280 --> 0:43:44.200
<v Speaker 1>but a little exosphere of their own. Interesting. And then,

0:43:44.200 --> 0:43:46.279
<v Speaker 1>and you know, as somebod who thinks about settlements, these

0:43:46.280 --> 0:43:49.200
<v Speaker 1>exo spheres will probably never be useful for anything, because

0:43:49.200 --> 0:43:51.000
<v Speaker 1>even if they were made out of useful stuff, it's

0:43:51.080 --> 0:43:53.640
<v Speaker 1>so it would be so hard to extract it. Yeah,

0:43:53.640 --> 0:43:56.480
<v Speaker 1>exactly right. There's probably no economic benefit there, But there

0:43:56.560 --> 0:43:59.120
<v Speaker 1>is a lot of physics that you can learn because

0:43:59.160 --> 0:44:02.480
<v Speaker 1>their collision list they're not interacting with each other, mostly

0:44:02.480 --> 0:44:04.920
<v Speaker 1>just flying along and doing their own dance. Each one

0:44:04.960 --> 0:44:07.759
<v Speaker 1>tells you something different about a physics process that's going on.

0:44:08.080 --> 0:44:10.080
<v Speaker 1>It helps to sort of like isolate the things and

0:44:10.120 --> 0:44:12.640
<v Speaker 1>study them in detail. So we think that each of

0:44:12.640 --> 0:44:17.279
<v Speaker 1>these Solar System bodies probably have different sinks and different sources. Right.

0:44:17.400 --> 0:44:20.080
<v Speaker 1>Some of them, for example, are really cold on the surface,

0:44:20.080 --> 0:44:21.960
<v Speaker 1>and that can be a sink. It can be like

0:44:22.000 --> 0:44:24.320
<v Speaker 1>that there's so it's so cold that it's like sticking

0:44:24.320 --> 0:44:27.360
<v Speaker 1>your tongue to a flagpole, that when those little molecules

0:44:27.400 --> 0:44:30.000
<v Speaker 1>touch the surface they stick on. So the exospheres are

0:44:30.040 --> 0:44:31.920
<v Speaker 1>a really cool way to learn a lot about the

0:44:31.960 --> 0:44:34.839
<v Speaker 1>surface of these planets without even landing on them. Right,

0:44:34.840 --> 0:44:37.280
<v Speaker 1>You can pass your satellite near one of these objects

0:44:37.320 --> 0:44:39.680
<v Speaker 1>and sample them and learn a lot about what's going

0:44:39.719 --> 0:44:42.800
<v Speaker 1>on in the surface without actually having to land. It's incredible.

0:44:42.880 --> 0:44:46.560
<v Speaker 1>We can collect enough data from these very thin exospheres

0:44:46.600 --> 0:44:48.319
<v Speaker 1>to learn this kind of stuff. Yeah, which you need

0:44:48.440 --> 0:44:50.879
<v Speaker 1>is a mass spectrometer. One of these devices that tells

0:44:50.920 --> 0:44:53.960
<v Speaker 1>you like, oh, you have seventy two atoms of hydrogen

0:44:54.120 --> 0:44:56.960
<v Speaker 1>or sixteen atoms of sodium. Can tell you exactly what

0:44:57.040 --> 0:44:59.440
<v Speaker 1>the composition is, and that gives you a lot of

0:44:59.440 --> 0:45:02.080
<v Speaker 1>clues to how these things formed and also what's going

0:45:02.160 --> 0:45:04.560
<v Speaker 1>on on their surface right now. I spoke to one

0:45:04.600 --> 0:45:06.600
<v Speaker 1>of my old friends from grad school who's now an

0:45:06.600 --> 0:45:09.920
<v Speaker 1>expert in this. He's a he's a space geoscientist, and

0:45:09.920 --> 0:45:13.239
<v Speaker 1>he said, any rocky object in space gets bombarded by

0:45:13.280 --> 0:45:16.040
<v Speaker 1>all sorts of crap that can liberate materials from the

0:45:16.080 --> 0:45:20.759
<v Speaker 1>surface and form an exo sphere is crap a technical term.

0:45:20.800 --> 0:45:23.080
<v Speaker 1>I mean he's speaking as a scientist, he's a professor,

0:45:23.160 --> 0:45:26.319
<v Speaker 1>So now it is a technical term. Fantastic. I didn't

0:45:26.320 --> 0:45:28.600
<v Speaker 1>realize it was that easy, And I guess that means that,

0:45:28.640 --> 0:45:31.120
<v Speaker 1>you know, even objects like the I s s, which

0:45:31.160 --> 0:45:33.359
<v Speaker 1>are getting hit by the solar wind and getting hit

0:45:33.360 --> 0:45:36.480
<v Speaker 1>by all sorts of stuff, are also like liberating little bits, right,

0:45:36.600 --> 0:45:40.239
<v Speaker 1>Spellation and abration are giving off little particles. And so

0:45:40.600 --> 0:45:45.160
<v Speaker 1>even like an individual astronaut out there in space on

0:45:45.200 --> 0:45:50.040
<v Speaker 1>an e v A must have their own little exo sphere. Somehow,

0:45:50.080 --> 0:45:51.839
<v Speaker 1>I feel like that would make me feel even more

0:45:51.880 --> 0:45:55.360
<v Speaker 1>important to know I had my own little exo sphere exactly,

0:45:55.400 --> 0:45:58.359
<v Speaker 1>and you don't even have to burp it out. That's right.

0:45:58.400 --> 0:46:01.359
<v Speaker 1>It's one thing we have advantage we have over Earth,

0:46:01.640 --> 0:46:04.480
<v Speaker 1>and so recent studies of the Moon suggests that, of

0:46:04.520 --> 0:46:07.480
<v Speaker 1>course there's sodium there. We can see sodium pretty clearly

0:46:07.560 --> 0:46:10.080
<v Speaker 1>because it's very responsive in the UV, which is what

0:46:10.200 --> 0:46:12.560
<v Speaker 1>these telescopes are good at looking at. But there's also

0:46:12.640 --> 0:46:16.120
<v Speaker 1>helium there, there's neon, there's argon. There might even be

0:46:16.160 --> 0:46:20.120
<v Speaker 1>like carbon burying species up there in the Moon's exosphere.

0:46:21.280 --> 0:46:23.560
<v Speaker 1>But there's not a lot of carbon on the Moon.

0:46:24.280 --> 0:46:26.960
<v Speaker 1>Where's the carbon coming from. There's definitely not a lot,

0:46:27.000 --> 0:46:29.839
<v Speaker 1>but some of it could be coming from the asteroid impacts, right.

0:46:29.920 --> 0:46:32.360
<v Speaker 1>Asteroids sometimes are have silica in them, sometimes they have

0:46:32.400 --> 0:46:37.080
<v Speaker 1>carbon in them. They sometimes even have complex organic molecules. Interesting.

0:46:37.360 --> 0:46:39.920
<v Speaker 1>So when you look up at the daytime sky, you're

0:46:39.920 --> 0:46:43.000
<v Speaker 1>seeing mostly the blue from our atmosphere, but beyond that

0:46:43.120 --> 0:46:46.319
<v Speaker 1>there's also the Earth's exosphere, which is so dilute that

0:46:46.360 --> 0:46:50.200
<v Speaker 1>you cannot see it. It's black, it's invisible, but it's there.

0:46:50.360 --> 0:46:53.239
<v Speaker 1>It's doing something. And everything else out there in the

0:46:53.239 --> 0:46:57.040
<v Speaker 1>Solar system, the Moon, mercury, all the other objects which

0:46:57.040 --> 0:47:00.200
<v Speaker 1>are quote bombarded by all sorts of crap, they also

0:47:00.320 --> 0:47:02.960
<v Speaker 1>generate an exo sphere, and that tells you that the

0:47:03.000 --> 0:47:06.520
<v Speaker 1>Solar System is not a static thing. It's a dance.

0:47:06.719 --> 0:47:10.719
<v Speaker 1>Everybody is giving off gas and accepting photons and interacting

0:47:10.800 --> 0:47:14.040
<v Speaker 1>with each other. So the Solar system has an exciting future.

0:47:14.239 --> 0:47:16.040
<v Speaker 1>You know, I usually think dances are better when they

0:47:16.040 --> 0:47:19.840
<v Speaker 1>don't involve gas, but but but this one is beautiful.

0:47:20.200 --> 0:47:22.440
<v Speaker 1>This is sort of how objects in the Solar System

0:47:22.520 --> 0:47:25.680
<v Speaker 1>talk to each other and evolve. All right, Thanks very

0:47:25.719 --> 0:47:28.360
<v Speaker 1>much for joining us on this exploration of whether or

0:47:28.400 --> 0:47:31.120
<v Speaker 1>not the Moon has an atmosphere. To put a pin

0:47:31.200 --> 0:47:33.239
<v Speaker 1>in it, I would say the Moon does not have

0:47:33.360 --> 0:47:36.720
<v Speaker 1>an atmosphere, but it definitely does have an exo sphere.

0:47:36.800 --> 0:47:38.920
<v Speaker 1>And thanks very much to our exo host Kelly for

0:47:39.000 --> 0:47:42.239
<v Speaker 1>joining us today. Thanks. I had a great time. I

0:47:42.320 --> 0:47:45.279
<v Speaker 1>was gonna say I had gas e time, but that

0:47:45.360 --> 0:47:47.120
<v Speaker 1>just doesn't sound what. It's good. I hope you didn't

0:47:47.120 --> 0:47:50.760
<v Speaker 1>have gas, but I thought it was a pretty nice atmosphere. Agreed,

0:47:51.239 --> 0:47:53.839
<v Speaker 1>that was a good punt. All right, Thanks for joining us.

0:47:53.840 --> 0:47:56.440
<v Speaker 1>Everyone tune in next time. All right, that was fun.

0:48:04.480 --> 0:48:07.280
<v Speaker 1>Thanks for listening, and remember that Daniel and Jorge Explain

0:48:07.360 --> 0:48:10.200
<v Speaker 1>the Universe is a production of I Heart Radio. For

0:48:10.360 --> 0:48:14.040
<v Speaker 1>more podcast from My Heart Radio, visit the I heart radio, app,

0:48:14.320 --> 0:48:17.760
<v Speaker 1>Apple podcasts, or wherever you listen to your favorite shows.

0:48:19.640 --> 0:48:19.680
<v Speaker 1>H