WEBVTT - Where do comets come from?

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<v Speaker 1>Hey, Jorgey, what's your favorite Solar System object? I'm gonna

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<v Speaker 1>have to go with the Earth because you know, it's

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<v Speaker 1>the only one I've been to, so you're not a

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<v Speaker 1>gas giant kind of person. Depends how many tacas I

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<v Speaker 1>had for munch. But what if I do? You do

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<v Speaker 1>you have a favorite? I'm a big fan of the

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<v Speaker 1>Sun and everything it does for us here on Earth,

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<v Speaker 1>But my favorite thing in the Solar System is actually comets.

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<v Speaker 1>Comments what have commets done for us? Well, they're like

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<v Speaker 1>cosmic snowballs, and actually most of Earth's water turns out

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<v Speaker 1>to be melted comets. I guess water is pretty useful

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<v Speaker 1>to have. But wait, are you saying the Solar System

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<v Speaker 1>is having a snowball fight. Yeah, it's more like deadly

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<v Speaker 1>planetary dodgeball. Hi am more Hammon, cartoonists and the creator

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<v Speaker 1>of PhD Comics. Hi. I'm Daniel. I'm a particle physicist,

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<v Speaker 1>but I have strong opinions about various Solar System objects.

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<v Speaker 1>And Welcome to our podcast, Daniel and Jorge Explain the Universe,

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<v Speaker 1>a production of I Heart Radio in which we talk

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<v Speaker 1>about everything that we know about the universe and everything

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<v Speaker 1>that we don't know about the universe, everything that makes

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<v Speaker 1>us wonder and everything that makes us go huh. And

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<v Speaker 1>we explain all of it to you because we think

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<v Speaker 1>that your curiosity is as valuable as the curiosity of

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<v Speaker 1>scientists working on the front line. Yeah, and there's a

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<v Speaker 1>lot to be curious about. The universe is full of

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<v Speaker 1>amazing and incredible things and a lot of mysteries, a

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<v Speaker 1>lot of things that we don't know where they come from,

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<v Speaker 1>or what makes them what they are, or why they're there. Yeah,

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<v Speaker 1>And a lot of great scientific discoveries begin with pretty

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<v Speaker 1>simple questions, you know, like why is that thing there?

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<v Speaker 1>Or why are those common? It's flying through space and

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<v Speaker 1>where do they come from? Is one of them going

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<v Speaker 1>to hit us and wipe us out? Great scientific discoveries

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<v Speaker 1>come from really simple questions that everybody wants to know

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<v Speaker 1>the answers to. Yeah, because we have questions even about

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<v Speaker 1>our own backyard. Our solar system is still full of

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<v Speaker 1>things that we don't quite fully understand. People like to

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<v Speaker 1>talk about things in the distant universe that are still

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<v Speaker 1>a mystery. We don't know how big it is or

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<v Speaker 1>what's going on out there in the depths of the universe.

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<v Speaker 1>But you're absolutely right, there's still a lot to be

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<v Speaker 1>discovered right in our own neighborhood, big questions about what's

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<v Speaker 1>going on in our own household that we still don't

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<v Speaker 1>know the answers to. So they know you have a

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<v Speaker 1>strong opinions about things in our Solar System? Are they

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<v Speaker 1>all positive or are some of them negative? Is there

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<v Speaker 1>someone you don't like here in system? Now? They're all positive.

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<v Speaker 1>I love everything in the Solar System, from ice giants

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<v Speaker 1>to planetism als, to space centaurs, to deadly comments to

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<v Speaker 1>enormous burning balls of gas. I just think it's all

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<v Speaker 1>pretty awesome. I can't imagine having a negative opinion about anything.

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<v Speaker 1>Do you include in that all the people on Earth too? Yes?

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<v Speaker 1>I love everybody. No, it's incredible when you look out

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<v Speaker 1>there in space that you see so many beautiful, amazing things.

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<v Speaker 1>Like when was the last time you looked at something

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<v Speaker 1>out in space and you thought that's just kind of

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<v Speaker 1>you know, it's all just sort of like incredible and beautiful.

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<v Speaker 1>You know, whoever the universe's visual artist is, they're doing

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<v Speaker 1>a good job. Although you know, we live in California,

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<v Speaker 1>so right now, when I look up at the sky,

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<v Speaker 1>it's mostly smoke. Well, then take a journey through the

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<v Speaker 1>Solar System with your mind's eye. Yeah, there are a

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<v Speaker 1>lot of big questions about the Solar System and how

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<v Speaker 1>we got to where we are. And one of those

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<v Speaker 1>big questions about our Solar system is where do comets

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<v Speaker 1>come from? We don't know a comet factory here in

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<v Speaker 1>our Solar system, do we We don't know of a

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<v Speaker 1>comet factory. It could be that there are aliens out

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<v Speaker 1>there in the outskirts of the Solar System packing up

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<v Speaker 1>ice balls and shooting them at Earth. Or it could

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<v Speaker 1>be that they come from something else, something deep out

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<v Speaker 1>there in the Solar System. That's basically a huge reservoir

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<v Speaker 1>of comets ready to fall in, screaming towards the Sun

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<v Speaker 1>and boiling. And this is a big question because some

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<v Speaker 1>people think that most of the water on Earth came

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<v Speaker 1>from comets. That's right, Commets are mostly ice. You know,

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<v Speaker 1>something a lot of people don't understand about the universe

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<v Speaker 1>is that water is not rare. We talk about liquid

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<v Speaker 1>water being something we're looking for in the surface of

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<v Speaker 1>planets to see if there's alien life, but water as

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<v Speaker 1>a chemical, there's tons of it out there. There's like

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<v Speaker 1>planet size blobs of it. So most comets are icy

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<v Speaker 1>planetism alls. They're just big balls of ice, and some

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<v Speaker 1>of them fell towards the Earth in the early days

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<v Speaker 1>and landed and melted and formed our oceans. Thank goodness,

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<v Speaker 1>because that's where life came from. Right, we had them

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<v Speaker 1>in for those snowballs, and we wouldn't be here, that's right.

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<v Speaker 1>So next time you put your lips to a glass

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<v Speaker 1>of melted comet, remember you're drinking. The outer Solar System

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<v Speaker 1>are melted common Right, next time you go somewhere in

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<v Speaker 1>order a drink, order sparkling melted comment and see what

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<v Speaker 1>they do. Yeah, So a big question is where they

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<v Speaker 1>come from, and so scientists have a potential answer to

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<v Speaker 1>that question, right, Daniel, that's right. They don't know for sure.

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<v Speaker 1>Nobody's ever actually seen it, but we've given it a name.

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<v Speaker 1>So today on the podcast, we will be asking the question,

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<v Speaker 1>what is now Daniel? Is that pronounced or or or

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<v Speaker 1>because it's spelled O r T. It's a great question,

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<v Speaker 1>and it's a Dutch name. It comes from a Dutch

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<v Speaker 1>astronomer who first thought it up. And so I reached

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<v Speaker 1>out to my Dutch speaking brother to ask him for

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<v Speaker 1>his preferred pronunciation because I didn't know is it ort

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<v Speaker 1>ort ort or something like weird Dutch vowel that we

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<v Speaker 1>don't even have in English that can never be replicated?

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<v Speaker 1>Keep going, keep going? Well, you know there are vowels

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<v Speaker 1>in Danish that you know you can only replicate. You

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<v Speaker 1>get like punched in the gut in exactly the right way,

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<v Speaker 1>like you Dango speakers out there know what I'm talking about.

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<v Speaker 1>But it turns out that or its spelled o o

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<v Speaker 1>rt is pronounced like port. All right, So it's a

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<v Speaker 1>cloud apparently of some sort, and it's I'm guessing it's

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<v Speaker 1>out in space, and so the big question is how

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<v Speaker 1>many people out there know what it is and what

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<v Speaker 1>its significance is. That's right? So I pulled our listeners

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<v Speaker 1>who have volunteered to answer random questions over the Internet

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<v Speaker 1>from a businessist they've never met. If you'd like to

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<v Speaker 1>participate in such absurd commentary on our physical universe, please

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<v Speaker 1>write to me two questions at Daniel and Jorge dot com.

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<v Speaker 1>And thanks to everybody who shared your speculations. Think about

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<v Speaker 1>it for a second. If someone asked you what the

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<v Speaker 1>orc cloud is, what would you answer. Here's what people

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<v Speaker 1>had to say, The or Cloud is one of the

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<v Speaker 1>outermost regions of the Solar System, comprised of we think

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<v Speaker 1>a bunch of remnants of the early Solar system. The

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<v Speaker 1>Orc Cloud is a group of like dust and rocks

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<v Speaker 1>and asteroids and just material that's way outside are encircles

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<v Speaker 1>our whole Solar system. I think in a giant sphere,

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<v Speaker 1>or maybe just a circle. The art Cloud is a

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<v Speaker 1>vast array of comets and other such I see debris

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<v Speaker 1>forwarding around the Sun, very far away from the rest

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<v Speaker 1>of the planetary systems. I know that the Sun, it's

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<v Speaker 1>the middle of it, and it passes our solar systems,

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<v Speaker 1>so passes Pluto. Is it the big cloud of dust

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<v Speaker 1>that I'm spewing out the top and the bottom of

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<v Speaker 1>the Milky Way? I have anything to do with equippable?

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<v Speaker 1>Probably close to the Solar system. I think the art

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<v Speaker 1>Cloud is like an area outside the Solar system where

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<v Speaker 1>there are some icy objects. I'm not sure what, probably

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<v Speaker 1>comets and things like that. All right, some pretty good answers.

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<v Speaker 1>Most people seem to know it's something related to our

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<v Speaker 1>Solar system, and that it's a cloud, and that maybe

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<v Speaker 1>there's ice involved. Yeah, exactly, it's something big and fuzzy

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<v Speaker 1>and out there and cool. Cool. And my favorite thing

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<v Speaker 1>about the Orc cloud is at the acronym the O

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<v Speaker 1>C is the same as the place I live, Orange County,

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<v Speaker 1>except it's a little warmer, I think, a little warmer,

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<v Speaker 1>but it's also still very very cool. That's the first

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<v Speaker 1>time I've heard you give a compliment to the Orange

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<v Speaker 1>County there. I love Orange County. Best place in the

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<v Speaker 1>world to live. Seriously, what could you complain about? But

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<v Speaker 1>that's not the topic of today's podcast. We're talking about

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<v Speaker 1>the cosmic o C, the solar systems O C, not

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<v Speaker 1>calibornias o C and to uh, it's apparently something out

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<v Speaker 1>in space and so Daniel, let's step people through it.

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<v Speaker 1>So what is the orc Cloud? The orc cloud is

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<v Speaker 1>super awesome. It is a theoretical cloud of icy planetisml's

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<v Speaker 1>or many planets planetismal. Did you just make that up

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<v Speaker 1>or is that the actual science terms? Oh? Man, I

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<v Speaker 1>wish I could have made that word of there's something

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<v Speaker 1>wonderful about just saying that word planetismal. Right, but no,

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<v Speaker 1>planetismal is a mini planet and it's smaller than a

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<v Speaker 1>dwarf planet. Right, You've got planet dwarf planet, and then

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<v Speaker 1>planet Tismal. They couldn't just say mini planet. Well it's

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<v Speaker 1>sort of like Planetino, you know, that's what you do

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<v Speaker 1>with English planet Tito. And so it's a bunch of

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<v Speaker 1>these and they're really really far out there. Like if

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<v Speaker 1>you have the Solar system, you know, the Earth is

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<v Speaker 1>at one AU call an astronomical unit, and you go

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<v Speaker 1>really far out you get out to like Neptune and Pluto.

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<v Speaker 1>You have to go much, much, much further before you

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<v Speaker 1>get to the arch cloud. Is it even considered our

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<v Speaker 1>Solar system or is it technically outside of our Solar system? Yeah,

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<v Speaker 1>it's a great question. Most people consider the end of

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<v Speaker 1>our Solar system to be just under about a hundred

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<v Speaker 1>a U, where the sun radiation becomes dominated by the

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<v Speaker 1>galactic radiation. How you think of space is sort of

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<v Speaker 1>like empty, right, but actually it's filled with streaming particles.

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<v Speaker 1>The Sun is pumping out particles, not just photons, but

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<v Speaker 1>protons and electrons and all sorts of crazy stuff, and

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<v Speaker 1>it dominates the region around it with all of its

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<v Speaker 1>pulsating radiation. But the rest of the galaxy also has

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<v Speaker 1>a wind that's coming from all the other stars in

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<v Speaker 1>the central black hole. And all that crazy stuff. So

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<v Speaker 1>we define the edge of the Solar system it's called

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<v Speaker 1>the helio pause, as the place where the Sun's radiation

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<v Speaker 1>stops dominating the local environment and you're taken over by

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<v Speaker 1>the galactic wind. And that's like a hundred or so A.

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<v Speaker 1>It's like when our Sun becomes just another star kind

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<v Speaker 1>of yeah, exactly, and the wind from the rest of

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<v Speaker 1>the galaxy takes over the Sun's wind. And here again

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<v Speaker 1>wind we don't mean air, We just mean the particles

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<v Speaker 1>that it's shooting out. But the rac cloud starts like

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<v Speaker 1>ten times further out than that, like at a thousand

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<v Speaker 1>a U. Now it's just still sort of like bound

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<v Speaker 1>by the gravity of the Sun, or is it pretty

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<v Speaker 1>much like an independent thing from our solar system. It's

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<v Speaker 1>definitely bound by the gravity of the Sun. So if

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<v Speaker 1>you define the edge of the Solar system by the radiation,

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<v Speaker 1>it's like a hundred a U. But stuff that's further

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<v Speaker 1>out is still gravitationally bound to the Sun, but it's

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<v Speaker 1>a little bit loose. It's like a little fuzzy. It's

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<v Speaker 1>so far out from the Sun that it's not that

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<v Speaker 1>hard to knock something off and have an escape into

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<v Speaker 1>interstellar space, so it's not orbiting around us. It's sort

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<v Speaker 1>of like we're tugging them and it's tugging us. It's

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<v Speaker 1>definitely orbiting around us. Think of it like a huge

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<v Speaker 1>shell surrounding the Solar System. The other fascinating thing about

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<v Speaker 1>it is that it's not a disk, right, Most of

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<v Speaker 1>the stuff in the Solar System is a big disc,

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<v Speaker 1>it's flat. But the Orc Cloud, we think, is a sphere.

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<v Speaker 1>It's like totally surrounding the Solar System, and it goes

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<v Speaker 1>out really really far out to like a light year

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<v Speaker 1>maybe two light years of just this like cloud of

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<v Speaker 1>little frozen objects, and there could be like trillions of

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<v Speaker 1>the planetismal, trillions of planetism many planets I'm sorry, yeah,

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<v Speaker 1>planet titos. And it's sort of like calculus. You know,

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<v Speaker 1>in calculus, you sum over infinitismals and you get like

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<v Speaker 1>an actual quantity. In the same way, if you sum

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<v Speaker 1>over all the planetism als in the ord cloud, you

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<v Speaker 1>get a combined mass of stuff that's like five times

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<v Speaker 1>the mass of the Earth, but then again spread out

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<v Speaker 1>into like trillions of objects. It spread out not just

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<v Speaker 1>like wide but tall to like it's it's pretty diffuse

0:12:31.280 --> 0:12:34.360
<v Speaker 1>it's very diffuse, Like it's not like flying the millennium

0:12:34.400 --> 0:12:36.840
<v Speaker 1>falcon through an asteroid field. You gonna like dodge and

0:12:36.880 --> 0:12:39.880
<v Speaker 1>weave right, it's like, could we see something, like is

0:12:39.920 --> 0:12:43.720
<v Speaker 1>there one there? It's so far out there, it's mostly empty.

0:12:43.920 --> 0:12:46.600
<v Speaker 1>But again, they are gravitationally bound to the Sun and

0:12:46.640 --> 0:12:48.640
<v Speaker 1>they are orbiting the Sun. That's why they are in

0:12:48.679 --> 0:12:51.480
<v Speaker 1>a cloud around the Sun. It's not like just the

0:12:51.520 --> 0:12:54.160
<v Speaker 1>whole interstellar medium is filled with these objects. It's a

0:12:54.200 --> 0:12:56.680
<v Speaker 1>cloud of them. We think. Again, we think we don't

0:12:56.679 --> 0:12:58.840
<v Speaker 1>know for sure. We haven't seen them because they're so

0:12:58.880 --> 0:13:01.960
<v Speaker 1>small and far away, but we think that they're there

0:13:02.200 --> 0:13:04.319
<v Speaker 1>in this big blob around the size see, and it's

0:13:04.360 --> 0:13:07.520
<v Speaker 1>made up of like giant literally like giant balls of ice,

0:13:07.800 --> 0:13:11.280
<v Speaker 1>basically snowballs. How big, Well, each one could be like

0:13:11.360 --> 0:13:14.120
<v Speaker 1>bigger than a kilometer in size, So we think that

0:13:14.200 --> 0:13:16.200
<v Speaker 1>they're like trillions of them that are more than a

0:13:16.240 --> 0:13:20.080
<v Speaker 1>kilometer and maybe only billions that are twenty kilometers are larger.

0:13:20.480 --> 0:13:23.040
<v Speaker 1>But if you wanted to have a cosmic snowball fight,

0:13:23.120 --> 0:13:25.640
<v Speaker 1>that's like where your arsenal is, that's the best place

0:13:25.679 --> 0:13:28.200
<v Speaker 1>to go for the stockpile. Wow, So that's like, let

0:13:28.200 --> 0:13:30.679
<v Speaker 1>me see, that's like a snowball about the size of

0:13:30.920 --> 0:13:35.520
<v Speaker 1>Los Angeles right kilometers. Yeah, there are billions of frozen

0:13:35.559 --> 0:13:39.640
<v Speaker 1>Los Angeles is out there in the o C because

0:13:39.679 --> 0:13:42.959
<v Speaker 1>they are pretty cool, icy cool. They are pretty cool,

0:13:43.320 --> 0:13:45.800
<v Speaker 1>and if they weren't gravitationally bound to the Sun, they

0:13:45.800 --> 0:13:49.120
<v Speaker 1>would just sort of float away into space. But they

0:13:49.160 --> 0:13:51.800
<v Speaker 1>are bound there. They're floating around, but you know, it's

0:13:51.840 --> 0:13:55.720
<v Speaker 1>sort of loose, and so sometimes the thought is sometimes

0:13:55.800 --> 0:13:58.839
<v Speaker 1>something perturbs them and then they can get knocked out

0:13:58.840 --> 0:14:01.520
<v Speaker 1>of their very loose orbit and plummet towards the inner

0:14:01.520 --> 0:14:04.120
<v Speaker 1>Solar System because they're in a stable orbit. Is that

0:14:04.160 --> 0:14:07.160
<v Speaker 1>the idea is that they're like happily going around our

0:14:07.200 --> 0:14:11.640
<v Speaker 1>Sun in this huge, wide orbit, but sometimes they can

0:14:11.720 --> 0:14:14.160
<v Speaker 1>fall in. Yeah, we think it's probably stable and if

0:14:14.200 --> 0:14:17.040
<v Speaker 1>nothing perturbed them, they would just happily hang out there

0:14:17.080 --> 0:14:21.040
<v Speaker 1>really far away, staying frozen. But you know, we are

0:14:21.160 --> 0:14:24.320
<v Speaker 1>in a little neighborhood, and since it's sort of loosely

0:14:24.400 --> 0:14:27.240
<v Speaker 1>held by the Sun, it's not that hard to perturb them.

0:14:27.440 --> 0:14:31.280
<v Speaker 1>And you can have things like galactic tides that squeeze

0:14:31.320 --> 0:14:33.440
<v Speaker 1>the orac cloud and knock some of them out of orbit.

0:14:33.960 --> 0:14:35.880
<v Speaker 1>You mean from the center of the galaxy. Yeah, just

0:14:35.920 --> 0:14:38.760
<v Speaker 1>the way the Moon has a gravitational effect on the

0:14:38.800 --> 0:14:41.040
<v Speaker 1>water of the Earth. So as the Moon goes around

0:14:41.080 --> 0:14:43.640
<v Speaker 1>the Earth, it tugs on the oceans and causes tides.

0:14:44.040 --> 0:14:46.880
<v Speaker 1>We have a gravitational pull towards the center of the galaxy,

0:14:47.240 --> 0:14:49.240
<v Speaker 1>and that tends to tug on one part of the

0:14:49.320 --> 0:14:52.040
<v Speaker 1>Orc Cloud that's closer to it more than the rest

0:14:52.040 --> 0:14:54.360
<v Speaker 1>of the Orc clouds, so sort of extends it. And

0:14:54.360 --> 0:14:57.240
<v Speaker 1>then as we move around the center of the galaxy

0:14:57.360 --> 0:15:00.520
<v Speaker 1>very slowly, you know, hundreds of millions of years, the

0:15:00.560 --> 0:15:04.160
<v Speaker 1>direction of that tug changes, so it's a dynamic. So

0:15:04.200 --> 0:15:06.160
<v Speaker 1>as we move around the center of the galaxy, the

0:15:06.200 --> 0:15:09.280
<v Speaker 1>tides change, the galactic tides change. So are we right

0:15:09.320 --> 0:15:17.800
<v Speaker 1>now and high tide or lord tide. Well, we're at

0:15:17.840 --> 0:15:20.080
<v Speaker 1>the center of it right so we wouldn't feel it

0:15:20.080 --> 0:15:22.160
<v Speaker 1>at all. But there's a blob of the Orc cloud

0:15:22.200 --> 0:15:25.320
<v Speaker 1>that's always pointed towards the center of the galaxy that

0:15:25.360 --> 0:15:27.720
<v Speaker 1>would be at high tide. There's more objects in that

0:15:27.880 --> 0:15:30.240
<v Speaker 1>part of it, so we're sort of at the very

0:15:30.240 --> 0:15:33.040
<v Speaker 1>center of it, so we can't tell, but it can

0:15:33.120 --> 0:15:36.320
<v Speaker 1>be galactic tides. It can also be like nearby stars.

0:15:36.760 --> 0:15:39.720
<v Speaker 1>If a nearby star happens to come somewhere close to

0:15:39.840 --> 0:15:42.440
<v Speaker 1>us as we all swish around the Milky Way, it

0:15:42.480 --> 0:15:45.640
<v Speaker 1>can perturb the orc cloud and send comets falling in

0:15:45.680 --> 0:15:47.960
<v Speaker 1>towards the center of the Solar system, right or steal them,

0:15:48.400 --> 0:15:51.960
<v Speaker 1>possibly steal them, or steal them absolutely, and we'll talk

0:15:51.960 --> 0:15:53.960
<v Speaker 1>about where these came from. It's not clear that all

0:15:53.960 --> 0:15:57.720
<v Speaker 1>of them actually came from our Solar system. And I

0:15:57.720 --> 0:16:00.880
<v Speaker 1>guess the thing is that we've never actually seen the cloud, right, Like,

0:16:00.920 --> 0:16:03.320
<v Speaker 1>we don't have pictures of it or even like radar

0:16:03.360 --> 0:16:05.960
<v Speaker 1>of it or evidence of it. That's right. It's so

0:16:06.080 --> 0:16:08.880
<v Speaker 1>far out there that it's still theoretical. There have been

0:16:08.960 --> 0:16:11.720
<v Speaker 1>some glimpses of one or two objects that people debate

0:16:12.040 --> 0:16:15.520
<v Speaker 1>might be like part of the Inner Inner Inner or cloud.

0:16:15.840 --> 0:16:19.280
<v Speaker 1>But these things are really small and really really far away,

0:16:19.320 --> 0:16:22.560
<v Speaker 1>Like it's hard to see Pluto, right, and Pluto is

0:16:22.640 --> 0:16:26.240
<v Speaker 1>really close compared to these things, and nothing that we

0:16:26.360 --> 0:16:29.120
<v Speaker 1>have out there in the Solar System has gotten anywhere

0:16:29.160 --> 0:16:31.400
<v Speaker 1>close to them, Like the thing that we have sent

0:16:31.600 --> 0:16:34.760
<v Speaker 1>out into space, that's the furthest object the humans have

0:16:34.920 --> 0:16:39.680
<v Speaker 1>ever built, that's Voyager one. The fastest human spaceship ever. Right,

0:16:40.200 --> 0:16:42.160
<v Speaker 1>that thing won't get to the beginning of the Orc

0:16:42.200 --> 0:16:46.160
<v Speaker 1>Cloud for another three hundred years. Well, Daniel, I don't

0:16:46.160 --> 0:16:49.280
<v Speaker 1>know if I believe in this thing or not, but

0:16:49.360 --> 0:16:51.800
<v Speaker 1>let's get into how we know it's actually there and

0:16:52.080 --> 0:16:55.760
<v Speaker 1>why we think it's important for our origin as a

0:16:55.960 --> 0:16:59.000
<v Speaker 1>planet and as a human species. But first, let's take

0:16:59.000 --> 0:17:14.440
<v Speaker 1>a quick break. All right, we're talking about the or Cloud,

0:17:14.880 --> 0:17:17.720
<v Speaker 1>which is uh. I guess Daniel, you would describe it

0:17:17.760 --> 0:17:22.879
<v Speaker 1>as like a giant shell of city size snowballs floating

0:17:22.920 --> 0:17:26.800
<v Speaker 1>out hundreds of light years away from the Sun. That's right,

0:17:27.000 --> 0:17:30.359
<v Speaker 1>And snowballs makes it sound quaint and fun and like

0:17:30.520 --> 0:17:32.199
<v Speaker 1>if you get hit by one, you can just go

0:17:32.320 --> 0:17:34.800
<v Speaker 1>inside and warm up with a cup of hot cocoa. Right,

0:17:35.119 --> 0:17:38.160
<v Speaker 1>But these things are massive ice balls, and if one

0:17:38.160 --> 0:17:40.920
<v Speaker 1>of them hit the Earth, we might be toasted. So

0:17:40.960 --> 0:17:43.320
<v Speaker 1>we'll talk about the danger these things later on, but

0:17:43.480 --> 0:17:45.440
<v Speaker 1>I want to make sure people are aware that these

0:17:45.440 --> 0:17:48.920
<v Speaker 1>are basically massive space bullets waiting to hit the Earth.

0:17:48.960 --> 0:17:50.800
<v Speaker 1>It's like a real snowball. If they pack enough ice

0:17:50.840 --> 0:17:53.160
<v Speaker 1>into that slush ball, it can really hurt. Yeah, alright,

0:17:53.200 --> 0:17:55.240
<v Speaker 1>so how do we know that it's actually there. Then

0:17:55.280 --> 0:17:57.560
<v Speaker 1>what makes us think that there is this giant cloud

0:17:57.600 --> 0:18:00.520
<v Speaker 1>of snowballs in space? Well, it comes um sort of

0:18:00.520 --> 0:18:03.320
<v Speaker 1>a paradox. In the last hundred years, we've established that

0:18:03.359 --> 0:18:06.240
<v Speaker 1>there are lots of comets, but the Solar system is

0:18:06.280 --> 0:18:08.840
<v Speaker 1>not very young, and so people have been wondering, like,

0:18:08.960 --> 0:18:12.000
<v Speaker 1>where do all these comets come from? Because comets are

0:18:12.000 --> 0:18:15.120
<v Speaker 1>not stable. Like, once a comet starts falling in towards

0:18:15.119 --> 0:18:17.760
<v Speaker 1>the Sun, it loses a lot of its mass as

0:18:17.760 --> 0:18:20.719
<v Speaker 1>the Sun boils it away. So a comet can't like

0:18:21.080 --> 0:18:24.000
<v Speaker 1>zip around the Sun for billions of years. It only

0:18:24.040 --> 0:18:26.880
<v Speaker 1>gets like, you know, fifty or a hundred, maybe two

0:18:27.000 --> 0:18:30.320
<v Speaker 1>hundred times around before it gets boiled away. Right, So

0:18:30.720 --> 0:18:33.040
<v Speaker 1>if that's the case, if comets don't last very long,

0:18:33.280 --> 0:18:36.399
<v Speaker 1>why are we still seeing commets? Like you lived in Arizona,

0:18:36.480 --> 0:18:38.360
<v Speaker 1>and every once in a while somebody throws a snowball

0:18:38.400 --> 0:18:41.040
<v Speaker 1>at your house, You're like, this is recent, Like somebody

0:18:41.119 --> 0:18:44.080
<v Speaker 1>just made this. Yeah, Or you know, if you're walking

0:18:44.080 --> 0:18:46.399
<v Speaker 1>around your neighborhood and everybody's eating ice cream, you're like,

0:18:46.520 --> 0:18:48.600
<v Speaker 1>where's the ice cream? Chuck? It must have just come by.

0:18:49.240 --> 0:18:51.600
<v Speaker 1>And so exactly, they thought there must be some sort

0:18:51.600 --> 0:18:55.120
<v Speaker 1>of source of these things. The other clue was that

0:18:55.160 --> 0:18:58.480
<v Speaker 1>there's sort of two types of comets. There are short

0:18:58.520 --> 0:19:01.240
<v Speaker 1>period comets. Com is to have an orbit around the

0:19:01.240 --> 0:19:04.200
<v Speaker 1>Sun that's like less than ten a U, and these

0:19:04.200 --> 0:19:06.439
<v Speaker 1>are mostly aligned with the Solar System. It seems like

0:19:06.440 --> 0:19:09.600
<v Speaker 1>they're like basically Solar System objects, just blobs of ice

0:19:09.960 --> 0:19:12.399
<v Speaker 1>somewhere in the outer reaches of the Solar System. But

0:19:12.480 --> 0:19:14.920
<v Speaker 1>then there's a second group of commets. They're called long

0:19:15.119 --> 0:19:18.040
<v Speaker 1>period comets. These are ones that have an orbit that's

0:19:18.080 --> 0:19:21.000
<v Speaker 1>like a thousand a U or more, and they take

0:19:21.040 --> 0:19:23.480
<v Speaker 1>a long time to go around the Sun, and they

0:19:23.600 --> 0:19:26.800
<v Speaker 1>don't follow the plane of the Solar system. So these

0:19:26.840 --> 0:19:28.960
<v Speaker 1>were really the mystery. They're like, where are these long

0:19:29.080 --> 0:19:32.520
<v Speaker 1>period comets coming from? They couldn't explain it. They shouldn't

0:19:32.560 --> 0:19:36.120
<v Speaker 1>stick around. And so to explain where the new ones

0:19:36.200 --> 0:19:38.919
<v Speaker 1>were coming from, they said, maybe there's a huge blob

0:19:38.960 --> 0:19:41.760
<v Speaker 1>of them somewhere out there beyond where we can see. Oh,

0:19:41.800 --> 0:19:44.600
<v Speaker 1>I see, you're saying these long period comments. They're sort

0:19:44.600 --> 0:19:46.960
<v Speaker 1>of coming out of left field. Doesn't look like they're

0:19:46.960 --> 0:19:48.879
<v Speaker 1>hanging out with us, or have been hanging out with

0:19:48.920 --> 0:19:52.000
<v Speaker 1>us for a long time. It's like they're coming from

0:19:52.080 --> 0:19:55.280
<v Speaker 1>somewhere else. Yeah, because they can't last for very long. Like,

0:19:55.359 --> 0:19:57.760
<v Speaker 1>once you see a comet, you're seeing it in the

0:19:57.880 --> 0:20:00.360
<v Speaker 1>end of its life cycle. It could have been out

0:20:00.400 --> 0:20:02.760
<v Speaker 1>happily for billions of years deep out there in the

0:20:02.760 --> 0:20:05.080
<v Speaker 1>Solar System. But once you see it, that means it's

0:20:05.119 --> 0:20:07.800
<v Speaker 1>falling towards the Sun and it's going to get boiled

0:20:07.840 --> 0:20:10.160
<v Speaker 1>away as it goes around the Sun, and it can't

0:20:10.160 --> 0:20:13.240
<v Speaker 1>survive for very long. And even if it does make

0:20:13.280 --> 0:20:15.560
<v Speaker 1>it a hundred or two hundred orbits, it's got a

0:20:15.640 --> 0:20:18.399
<v Speaker 1>high chance of getting kicked out of the Solar System

0:20:18.440 --> 0:20:21.560
<v Speaker 1>being perturbed by the gravity of one of the outer planets.

0:20:21.600 --> 0:20:24.040
<v Speaker 1>So once you see a comet, it means it's in

0:20:24.119 --> 0:20:26.639
<v Speaker 1>its last chapter of its life in the Solar System.

0:20:26.760 --> 0:20:29.320
<v Speaker 1>So we're still seeing comets four and a half billion

0:20:29.440 --> 0:20:31.679
<v Speaker 1>years into the story of the Solar System. There has

0:20:31.760 --> 0:20:34.320
<v Speaker 1>to be some fresh resupply every once in a while.

0:20:34.520 --> 0:20:36.440
<v Speaker 1>I guess if you're seeing a comment, that means it's

0:20:36.440 --> 0:20:38.920
<v Speaker 1>getting hit by the rays of the Sun, which is

0:20:38.960 --> 0:20:42.440
<v Speaker 1>probably melting it. It's definitely melting it, and that's where

0:20:42.440 --> 0:20:44.720
<v Speaker 1>the comets tail is. Right. People like to imagine the

0:20:44.720 --> 0:20:47.920
<v Speaker 1>commets tails like little action lines in a cartoon that

0:20:48.000 --> 0:20:50.680
<v Speaker 1>show you where it's moving. But the commets tail is

0:20:50.720 --> 0:20:54.080
<v Speaker 1>not actually pointed away from the direction of the comets motion.

0:20:54.560 --> 0:20:57.480
<v Speaker 1>It's pointed away from the sun because the tail comes

0:20:57.520 --> 0:21:01.840
<v Speaker 1>from the sun boiling away all the stuff on the comet. Yeah,

0:21:02.000 --> 0:21:04.720
<v Speaker 1>that's the signature tale of of comets. That's what it is.

0:21:04.880 --> 0:21:07.320
<v Speaker 1>It's not really a tail. It's more like a haircut.

0:21:07.480 --> 0:21:12.159
<v Speaker 1>Is that what you're saying, Yeah, precisely. And comets can

0:21:12.160 --> 0:21:15.080
<v Speaker 1>actually have multiple tales. They can have tales going in

0:21:15.119 --> 0:21:18.080
<v Speaker 1>different directions based on like the stuff that's in there

0:21:18.119 --> 0:21:21.160
<v Speaker 1>that's good and getting boiled away different compositions. So it's

0:21:21.160 --> 0:21:24.399
<v Speaker 1>pretty fascinating look at the tales of comets. It's pretty awesome. Okay.

0:21:24.400 --> 0:21:28.000
<v Speaker 1>So then someone named Yon Ord in the fifties said, hey,

0:21:28.000 --> 0:21:31.760
<v Speaker 1>maybe all of these weird long period comets are coming

0:21:32.000 --> 0:21:35.080
<v Speaker 1>from a very specific place. And so he came up

0:21:35.119 --> 0:21:37.320
<v Speaker 1>with this idea of the Ord cloud. Yeah, and he

0:21:37.359 --> 0:21:39.520
<v Speaker 1>looked at the orbits of these comets and he said,

0:21:39.520 --> 0:21:42.160
<v Speaker 1>how far out does it have to be to generate

0:21:42.240 --> 0:21:45.720
<v Speaker 1>comets with this length or but these long period comets,

0:21:46.240 --> 0:21:48.080
<v Speaker 1>And so that's how he estimated. He made a very

0:21:48.200 --> 0:21:50.800
<v Speaker 1>rough estimate for you know, how far away should be.

0:21:51.040 --> 0:21:54.160
<v Speaker 1>And since then we have much better data, better telescopes.

0:21:54.280 --> 0:21:57.320
<v Speaker 1>We can see the orbit of these comets much more clearly.

0:21:57.400 --> 0:21:59.920
<v Speaker 1>We have more telescopes, we have hubble and so be

0:22:00.040 --> 0:22:02.119
<v Speaker 1>can track all this stuff, and we have better estimates

0:22:02.119 --> 0:22:05.280
<v Speaker 1>for what's out there and how big it is. But

0:22:05.400 --> 0:22:08.199
<v Speaker 1>the basic idea came from this guy, yawned Ort in

0:22:08.320 --> 0:22:10.800
<v Speaker 1>nineteen fifty. And you know, it's pretty awesome to get

0:22:10.840 --> 0:22:13.280
<v Speaker 1>to put your name on the biggest thing in the

0:22:13.320 --> 0:22:16.080
<v Speaker 1>Solar system, Like this thing just dwarfs the rest of

0:22:16.080 --> 0:22:18.320
<v Speaker 1>the Solar system. Did he call it that the the

0:22:18.480 --> 0:22:20.840
<v Speaker 1>ord cloud or was it named after him? That's a

0:22:20.880 --> 0:22:23.800
<v Speaker 1>great question. I should read his original paper to see

0:22:23.840 --> 0:22:25.399
<v Speaker 1>if he put his own name on it or if

0:22:25.440 --> 0:22:27.639
<v Speaker 1>he was humble. Yeah, when he called the cloud of

0:22:27.720 --> 0:22:31.920
<v Speaker 1>Testimal and let somebody said that's a ridiculous name. We'll

0:22:31.960 --> 0:22:34.320
<v Speaker 1>go with orc. Yeah. And it's fascinating and it's cool

0:22:34.400 --> 0:22:36.720
<v Speaker 1>because it answers a question, right, It tells you, oh,

0:22:36.800 --> 0:22:39.159
<v Speaker 1>that must be where these comets are coming from. But

0:22:39.280 --> 0:22:41.639
<v Speaker 1>like everything in science, when you answer a question, it

0:22:41.840 --> 0:22:44.760
<v Speaker 1>opens up more questions, like all right, Well, where did

0:22:44.800 --> 0:22:47.200
<v Speaker 1>this ort cloud come from? Why is it there? Why

0:22:47.240 --> 0:22:50.240
<v Speaker 1>aren't they just closer into the rest of the Solar System.

0:22:50.280 --> 0:22:52.840
<v Speaker 1>And that's an active area of research right now. So

0:22:52.880 --> 0:22:55.760
<v Speaker 1>we actually haven't seen this cloud. We're just sort of

0:22:55.800 --> 0:22:59.640
<v Speaker 1>tracking where comets come from, and we think they come

0:22:59.680 --> 0:23:02.439
<v Speaker 1>from the cloud. Yeah, we have not seen this. We

0:23:02.520 --> 0:23:04.760
<v Speaker 1>don't have telescopes that are powerful enough to spot it,

0:23:05.040 --> 0:23:08.200
<v Speaker 1>none of our probes are anywhere near it. But it's

0:23:08.200 --> 0:23:10.919
<v Speaker 1>sort of the best explanation and we have for the

0:23:11.000 --> 0:23:14.359
<v Speaker 1>source of comets. So it's pretty well accepted in the

0:23:14.400 --> 0:23:18.520
<v Speaker 1>astronomical community that it exists. Like we always like to

0:23:18.560 --> 0:23:22.040
<v Speaker 1>see direct evidence of something before we conclude that it exists,

0:23:22.080 --> 0:23:25.159
<v Speaker 1>like there was evidence for Pluto before we spotted it

0:23:25.200 --> 0:23:28.080
<v Speaker 1>in a telescope. But you don't really claim discovery of

0:23:28.119 --> 0:23:31.240
<v Speaker 1>it until you actually see it, right, It's like finding

0:23:31.240 --> 0:23:33.960
<v Speaker 1>the body in a murder mystery. But sometimes it's the

0:23:34.000 --> 0:23:36.000
<v Speaker 1>best you can do for a while, so we can

0:23:36.000 --> 0:23:39.159
<v Speaker 1>talk later about like plans people have for how to

0:23:39.280 --> 0:23:41.560
<v Speaker 1>spot the Orc cloud and to study it, but for

0:23:41.680 --> 0:23:43.920
<v Speaker 1>now we have no direct evidence of it. I guess

0:23:43.960 --> 0:23:45.880
<v Speaker 1>it's not a thick enough cloud that it like makes

0:23:45.880 --> 0:23:48.760
<v Speaker 1>your view hazy, or you can see some of the

0:23:48.880 --> 0:23:52.280
<v Speaker 1>like the light getting filtered through it. It's not that thick, No,

0:23:52.480 --> 0:23:54.719
<v Speaker 1>it's not that thick. These things are very small and

0:23:54.840 --> 0:23:57.359
<v Speaker 1>very far away, so thick is definitely not how you

0:23:57.440 --> 0:24:02.600
<v Speaker 1>describe it. There's enormous that empty spaces between every object

0:24:02.680 --> 0:24:05.320
<v Speaker 1>in the orc cloud. Even though there are trillions and

0:24:05.400 --> 0:24:09.760
<v Speaker 1>trillions of objects. The space we're talking about is incredibly vast, Right,

0:24:10.040 --> 0:24:13.200
<v Speaker 1>We're talking about a sphere that's basically a light year

0:24:13.280 --> 0:24:16.159
<v Speaker 1>in radius, and so there's a lot of space in

0:24:16.200 --> 0:24:20.000
<v Speaker 1>there to distribute the trillion objects and still have lots

0:24:20.040 --> 0:24:21.960
<v Speaker 1>of room in between them. All Right, Well, I guess,

0:24:21.960 --> 0:24:23.600
<v Speaker 1>like you said, a big question is where did this

0:24:23.800 --> 0:24:26.280
<v Speaker 1>orc cloud come from? Like why is there all this

0:24:26.400 --> 0:24:29.639
<v Speaker 1>water deposited in one spot out there in the Solar system?

0:24:29.800 --> 0:24:32.040
<v Speaker 1>Beyond the Solar system. Well, as usual, we have a

0:24:32.040 --> 0:24:34.640
<v Speaker 1>few theories. We have sort of like the most boring

0:24:34.720 --> 0:24:37.960
<v Speaker 1>theory and then the most exciting theory, and the most

0:24:37.960 --> 0:24:40.320
<v Speaker 1>boring theory is sort of a story of the formation

0:24:40.400 --> 0:24:43.280
<v Speaker 1>of our Solar system. Like we start from a big

0:24:43.320 --> 0:24:46.719
<v Speaker 1>cloud of molecular gas and dust and stuff that collapses

0:24:47.080 --> 0:24:49.200
<v Speaker 1>and you get the Sun and you have a disc

0:24:49.240 --> 0:24:51.960
<v Speaker 1>of stuff that has too much angular momentum to collapse

0:24:52.000 --> 0:24:54.840
<v Speaker 1>into the Sun, so it spins around the Sun without

0:24:54.880 --> 0:24:59.040
<v Speaker 1>forming part of the star. And that's the protoplanetary disc, right.

0:24:59.280 --> 0:25:01.520
<v Speaker 1>And there you have of ice and gas and dust

0:25:01.760 --> 0:25:04.960
<v Speaker 1>and all kinds of stuff that starts to form planets

0:25:04.960 --> 0:25:07.679
<v Speaker 1>and clump together and form all sorts of stuff. The

0:25:07.720 --> 0:25:11.320
<v Speaker 1>idea is that not everything clumps together to form a planet,

0:25:11.359 --> 0:25:14.680
<v Speaker 1>like you have asteroids for example, of smaller things. Gravity

0:25:14.720 --> 0:25:18.880
<v Speaker 1>doesn't succeed in clumping everything together. But you do get

0:25:19.000 --> 0:25:22.480
<v Speaker 1>big gas giants out there, like Neptune and Urineus and

0:25:22.560 --> 0:25:25.359
<v Speaker 1>Saturn and Jupiter. They start to be sort of like

0:25:25.520 --> 0:25:29.320
<v Speaker 1>heavyweights of their own gravitationally, and they can perturb the

0:25:29.359 --> 0:25:31.760
<v Speaker 1>other stuff. And so there was a bit of a

0:25:31.880 --> 0:25:35.520
<v Speaker 1>dance in the early Solar System as these big planets

0:25:35.520 --> 0:25:38.399
<v Speaker 1>we're finding their place, and as they move around, they

0:25:38.440 --> 0:25:41.399
<v Speaker 1>affected everything else. So the short version of the story

0:25:41.440 --> 0:25:43.640
<v Speaker 1>is that we think that they were essentially tossed out

0:25:43.680 --> 0:25:46.560
<v Speaker 1>of the Solar System by some of these gas giants

0:25:46.600 --> 0:25:48.959
<v Speaker 1>as they were being born. These planets sort of like

0:25:49.200 --> 0:25:52.200
<v Speaker 1>muscled their way around the craziness of the Solar System. Yeah,

0:25:52.200 --> 0:25:54.480
<v Speaker 1>and one of the definitions of planets, if you believe

0:25:54.520 --> 0:25:58.080
<v Speaker 1>in you know, silly astronomical categories, is that it's cleared

0:25:58.119 --> 0:26:00.679
<v Speaker 1>its own path around the Sun. And so that's just

0:26:00.720 --> 0:26:02.879
<v Speaker 1>sort of like the job of growing up and being

0:26:02.960 --> 0:26:04.920
<v Speaker 1>a modern planet is that you have to like toss

0:26:05.000 --> 0:26:07.359
<v Speaker 1>the little bits out of the way, or you know,

0:26:07.440 --> 0:26:09.840
<v Speaker 1>slave them and make them into your moons. But in

0:26:09.880 --> 0:26:12.560
<v Speaker 1>this case, most of the stuff we think was tossed

0:26:12.560 --> 0:26:15.320
<v Speaker 1>out sort of in the early days of the Solar

0:26:15.320 --> 0:26:18.200
<v Speaker 1>System formation. And it also it had a reverse effect.

0:26:18.280 --> 0:26:21.199
<v Speaker 1>Remember gravity is always two directions. So we think that

0:26:21.280 --> 0:26:23.760
<v Speaker 1>one of the reasons that Neptune is as far out

0:26:23.840 --> 0:26:26.640
<v Speaker 1>as it is is that it got tugged out by

0:26:26.720 --> 0:26:29.880
<v Speaker 1>these objects as they were leaving the Solar System. I guess.

0:26:29.920 --> 0:26:32.320
<v Speaker 1>One question is if a planet is kind of plowing

0:26:32.359 --> 0:26:35.280
<v Speaker 1>through and sending things out into space, wouldn't it send

0:26:35.280 --> 0:26:38.520
<v Speaker 1>all kinds of things like asteroids and rocks and gas.

0:26:38.600 --> 0:26:43.560
<v Speaker 1>How did all this ice come together so purely, I guess,

0:26:43.560 --> 0:26:45.280
<v Speaker 1>And like, you know, why isn't it a mix of

0:26:45.280 --> 0:26:47.800
<v Speaker 1>all other things? Yeah, that's a great question. It is

0:26:47.880 --> 0:26:50.679
<v Speaker 1>mostly a mix, right, These things are not pure water.

0:26:50.880 --> 0:26:52.639
<v Speaker 1>It's like you go out there and you find these

0:26:52.680 --> 0:26:55.880
<v Speaker 1>pristine cubes of ice that you're ready to chisel out

0:26:55.920 --> 0:26:59.199
<v Speaker 1>and put onto your space cocktails. These things are dirty.

0:26:59.320 --> 0:27:02.040
<v Speaker 1>It's definitely still rocks in there. But remember that a

0:27:02.200 --> 0:27:04.919
<v Speaker 1>large fraction of the stuff in the outer Solar system

0:27:05.280 --> 0:27:08.040
<v Speaker 1>is ice, like you call uranus and neptune. They are

0:27:08.080 --> 0:27:11.119
<v Speaker 1>called ice giants, and so it's something of a matter

0:27:11.200 --> 0:27:14.359
<v Speaker 1>of how these chemicals are distributed through the solar system,

0:27:14.440 --> 0:27:17.480
<v Speaker 1>like where water ends up and ends up freezing and

0:27:17.520 --> 0:27:20.119
<v Speaker 1>gathering together. But a lot of the stuff in the

0:27:20.160 --> 0:27:23.080
<v Speaker 1>outer Solar system, and non significant fraction of all the

0:27:23.119 --> 0:27:26.800
<v Speaker 1>mass in the outer Solar system is water. I guess

0:27:26.840 --> 0:27:29.720
<v Speaker 1>out there most of it is ice and liquid, because

0:27:29.760 --> 0:27:32.120
<v Speaker 1>if it was closer, it would evaporate and maybe blow

0:27:32.119 --> 0:27:35.679
<v Speaker 1>out exactly. Some complicated arguments about where stuff in the

0:27:35.760 --> 0:27:38.959
<v Speaker 1>solar system collapses and what falls in and what doesn't.

0:27:39.119 --> 0:27:40.720
<v Speaker 1>But you end up with a lot of ice in

0:27:40.760 --> 0:27:44.120
<v Speaker 1>the outer Solar system. But these things are not pure water. Again,

0:27:44.160 --> 0:27:47.720
<v Speaker 1>they're definitely bits of rock. I would not recommend drinking

0:27:47.840 --> 0:27:51.000
<v Speaker 1>an or object if you found one, unless you like rocks,

0:27:52.040 --> 0:27:54.600
<v Speaker 1>unless they like your cocktails dirty. I guess they're dirty

0:27:54.600 --> 0:27:57.959
<v Speaker 1>snowballs all right, So that's one theory about how it forms,

0:27:58.000 --> 0:28:00.679
<v Speaker 1>just like you know, byproduct of the dynamics of the

0:28:00.720 --> 0:28:03.400
<v Speaker 1>solar system. What are the more interesting theories? The more

0:28:03.440 --> 0:28:07.159
<v Speaker 1>interesting theories are the interstellar theories. One idea is that

0:28:07.200 --> 0:28:10.480
<v Speaker 1>our son, when it formed, wasn't on its own. But

0:28:10.760 --> 0:28:13.639
<v Speaker 1>you know, we've discovered barely recently that a lot of

0:28:13.680 --> 0:28:16.359
<v Speaker 1>stars it was a twin. Yes, we're born as twins.

0:28:16.400 --> 0:28:20.160
<v Speaker 1>That binary star systems are much more common than we imagined.

0:28:20.600 --> 0:28:22.240
<v Speaker 1>So it could have been that our son had a

0:28:22.280 --> 0:28:26.040
<v Speaker 1>twin and that this collapsing cloud of stuff formed two

0:28:26.080 --> 0:28:28.639
<v Speaker 1>stars instead of one. But then these two sort of

0:28:28.720 --> 0:28:33.000
<v Speaker 1>drifted apart, as you know siblings sometimes do, and there's

0:28:33.000 --> 0:28:35.359
<v Speaker 1>a lot of material exchanged, and that gives you an

0:28:35.400 --> 0:28:39.360
<v Speaker 1>opportunity to sort of pull material further away from the

0:28:39.400 --> 0:28:42.360
<v Speaker 1>Sun because you have this big, heavy object, the other star,

0:28:42.760 --> 0:28:46.120
<v Speaker 1>tugging on your solar system. What so, what happened to

0:28:46.160 --> 0:28:49.000
<v Speaker 1>this other star, sister star. It's the subject of a

0:28:49.040 --> 0:28:51.320
<v Speaker 1>Netflix documentary, you know, where they're going to reunite the

0:28:51.360 --> 0:28:54.040
<v Speaker 1>stars for a dramatic conclusion at the end of the universe,

0:28:54.600 --> 0:28:59.800
<v Speaker 1>or a hit podcast mini series. That's right, not true crime,

0:28:59.840 --> 0:29:02.920
<v Speaker 1>but true physics. No, we don't know. It's just hypothetical.

0:29:02.960 --> 0:29:05.720
<v Speaker 1>We don't know that the Sun had a twin star

0:29:05.840 --> 0:29:08.640
<v Speaker 1>at its birth. It's just an idea. But if it did,

0:29:08.960 --> 0:29:11.200
<v Speaker 1>it could have been pulled off and gone in any direction.

0:29:11.360 --> 0:29:13.680
<v Speaker 1>It's been a long time, it's been billions of years,

0:29:13.960 --> 0:29:16.120
<v Speaker 1>and so it's hard to trace. It's not like the

0:29:16.160 --> 0:29:19.920
<v Speaker 1>nearest star is necessarily a category for our lost twin.

0:29:20.280 --> 0:29:22.480
<v Speaker 1>This thing would have been moving for a long time.

0:29:22.520 --> 0:29:24.520
<v Speaker 1>It could be anywhere at this point. And so the

0:29:24.560 --> 0:29:27.720
<v Speaker 1>idea is that the sister star pulled some things from

0:29:27.760 --> 0:29:30.080
<v Speaker 1>the Sun and then left it out there and where

0:29:30.120 --> 0:29:32.320
<v Speaker 1>the orc tod would be. Yeah, just like we were

0:29:32.360 --> 0:29:35.160
<v Speaker 1>talking about the gas giants tossing stuff out of the

0:29:35.160 --> 0:29:38.080
<v Speaker 1>Solar system, Now you have a much bigger object, a

0:29:38.120 --> 0:29:41.760
<v Speaker 1>heavier object, another star even further out. It's going to

0:29:41.840 --> 0:29:44.160
<v Speaker 1>tug out some of these stuff in our solar system

0:29:44.400 --> 0:29:46.920
<v Speaker 1>to have a very large radius. And then as the

0:29:46.960 --> 0:29:49.720
<v Speaker 1>to sort of separate. I'm imagining, like you know, sell

0:29:49.840 --> 0:29:52.720
<v Speaker 1>mitoses here two stars are pulling apart from each other

0:29:52.920 --> 0:29:55.040
<v Speaker 1>and it's sort of like threads in between them, and

0:29:55.080 --> 0:29:57.560
<v Speaker 1>then as they get far enough away, they stop affecting

0:29:57.560 --> 0:30:01.200
<v Speaker 1>each other gravitationally and things settle into place. But you

0:30:01.240 --> 0:30:03.960
<v Speaker 1>have stuff out at a pretty far radius because the

0:30:04.000 --> 0:30:07.160
<v Speaker 1>gravitational pull of the other star interesting. So it was

0:30:07.200 --> 0:30:10.320
<v Speaker 1>like the leftover from the divorce or something I just

0:30:10.360 --> 0:30:13.240
<v Speaker 1>got dropped there in the middle of space. That's right,

0:30:13.560 --> 0:30:17.200
<v Speaker 1>the poor abandoned objects in the stellar o c so

0:30:17.280 --> 0:30:22.960
<v Speaker 1>many seems appropriate. All right, let's get into our last

0:30:23.040 --> 0:30:26.440
<v Speaker 1>theory about where this orc cloud came from and what

0:30:26.600 --> 0:30:29.320
<v Speaker 1>it all means. The first let's take another quick break.

0:30:41.800 --> 0:30:45.920
<v Speaker 1>All right, Daniel, there's a giant cloud of snowballs out

0:30:46.000 --> 0:30:49.280
<v Speaker 1>in space about three light years away from the Sun,

0:30:50.000 --> 0:30:51.800
<v Speaker 1>and we think that's where comments come from. But the

0:30:51.880 --> 0:30:54.400
<v Speaker 1>question is where did this cloud come from? And so

0:30:54.480 --> 0:30:57.400
<v Speaker 1>you have one more theory for us about that, and

0:30:57.560 --> 0:31:01.720
<v Speaker 1>I'm going to guess it involves eight It involves alien stars,

0:31:02.080 --> 0:31:04.360
<v Speaker 1>though we don't know if there are aliens enough living

0:31:04.400 --> 0:31:06.880
<v Speaker 1>around those stars. The problem is that if you do

0:31:06.920 --> 0:31:09.880
<v Speaker 1>the calculations, and you have your theory of the Solar

0:31:09.920 --> 0:31:12.880
<v Speaker 1>system and you predict how many things there should be

0:31:12.960 --> 0:31:15.160
<v Speaker 1>in the or cloud, you get a number that's way

0:31:15.160 --> 0:31:18.320
<v Speaker 1>too small. You get a number like six billion objects.

0:31:18.600 --> 0:31:21.040
<v Speaker 1>But we know the number is much much bigger than that.

0:31:21.560 --> 0:31:23.480
<v Speaker 1>So the idea is like, well, where do these things

0:31:23.560 --> 0:31:26.080
<v Speaker 1>come from? So wait, how do we know how big

0:31:26.120 --> 0:31:28.000
<v Speaker 1>it should be? If we don't, we've never seen it

0:31:28.040 --> 0:31:30.160
<v Speaker 1>and it's all theoretical. Is it just from like the

0:31:30.240 --> 0:31:33.640
<v Speaker 1>frequency of comments that we get exactly to explain the

0:31:33.720 --> 0:31:36.440
<v Speaker 1>number of comments that we see, and they're radius and stuff,

0:31:36.600 --> 0:31:38.960
<v Speaker 1>there should be a certain number of objects in the

0:31:39.120 --> 0:31:42.240
<v Speaker 1>Orc cloud, otherwise we would see fewer and fewer comments.

0:31:42.280 --> 0:31:44.320
<v Speaker 1>But if we try to predict how many things are

0:31:44.360 --> 0:31:47.000
<v Speaker 1>in the Orc cloud from sort of first principles formation,

0:31:47.040 --> 0:31:49.200
<v Speaker 1>like how many things should have been tossed out there

0:31:49.200 --> 0:31:52.160
<v Speaker 1>by Neptune and Saturn Uranus, then we get a much

0:31:52.200 --> 0:31:55.120
<v Speaker 1>smaller number. So there's a discrepancy there. We know there

0:31:55.160 --> 0:31:57.880
<v Speaker 1>are objects out there, we can't explain how they got there.

0:31:58.560 --> 0:32:01.640
<v Speaker 1>So one idea is as well, when our star was forming,

0:32:01.960 --> 0:32:04.840
<v Speaker 1>what was going on nearby? We talked about how maybe

0:32:04.840 --> 0:32:07.320
<v Speaker 1>there was a sister star formed with us. But another

0:32:07.440 --> 0:32:11.760
<v Speaker 1>idea is that maybe our stellar cloud that collapsed was

0:32:11.920 --> 0:32:15.760
<v Speaker 1>near some other objects and it stole some material from

0:32:15.800 --> 0:32:19.000
<v Speaker 1>those objects. That basically the Orc cloud is like a

0:32:19.040 --> 0:32:22.280
<v Speaker 1>lot of stuff from other solar systems that was stolen

0:32:22.320 --> 0:32:28.160
<v Speaker 1>by our sun when it formed. What it could be stolen? Good? Yeah,

0:32:28.320 --> 0:32:31.120
<v Speaker 1>the water we're drinking could have been stolen from another

0:32:31.160 --> 0:32:33.200
<v Speaker 1>solar system. Is that what you're saying? You should feel

0:32:33.200 --> 0:32:36.120
<v Speaker 1>guilty every time you have a drink. It's elicit. But

0:32:36.160 --> 0:32:39.600
<v Speaker 1>it could basically be all a muamua, right, Remember Mumua

0:32:39.760 --> 0:32:43.560
<v Speaker 1>was this interstellar comment, this frozen object that passed through

0:32:43.560 --> 0:32:47.800
<v Speaker 1>our solar system coming from some other solar system. And

0:32:47.880 --> 0:32:50.480
<v Speaker 1>it could be that the Orc Cloud is basically just

0:32:50.560 --> 0:32:52.200
<v Speaker 1>a bunch of these. Oh I see, is that a

0:32:52.280 --> 0:32:55.080
<v Speaker 1>theory that Oma came from the Orc Cloud? No, mum

0:32:55.280 --> 0:32:57.560
<v Speaker 1>It definitely did not come from the Orc Cloud. Its

0:32:57.560 --> 0:33:00.080
<v Speaker 1>trajectory is totally inconsistent with that. We know that it

0:33:00.200 --> 0:33:03.080
<v Speaker 1>came from another solar system. But it could be think

0:33:03.080 --> 0:33:06.040
<v Speaker 1>the Orc Cloud is the product of stealing a bunch

0:33:06.040 --> 0:33:10.320
<v Speaker 1>of Omumua like objects much much earlier, a long time ago,

0:33:10.600 --> 0:33:13.920
<v Speaker 1>as our solar systems forming. So you know, possession is

0:33:14.000 --> 0:33:16.400
<v Speaker 1>nine tenths of the law. Then you know we've had

0:33:16.400 --> 0:33:19.480
<v Speaker 1>these for billions of years. They're basically ours now, but

0:33:19.680 --> 0:33:22.240
<v Speaker 1>there's a bit of original sin there and having stolen

0:33:22.240 --> 0:33:24.880
<v Speaker 1>them from another solar system a long time ago. Well, yeah,

0:33:24.920 --> 0:33:27.360
<v Speaker 1>I guess, because you know, I think the closest stars

0:33:27.360 --> 0:33:30.800
<v Speaker 1>to us our solar system are about what is it

0:33:30.880 --> 0:33:33.800
<v Speaker 1>like five light years away, right, yeah, three and a

0:33:33.840 --> 0:33:36.479
<v Speaker 1>half light years away to proximates Centauri. Yeah, so this

0:33:36.600 --> 0:33:39.320
<v Speaker 1>orc cloud is about where those other stars are. Yeah,

0:33:39.360 --> 0:33:41.800
<v Speaker 1>it's the right order of magnitude, right, it's that big.

0:33:42.080 --> 0:33:44.320
<v Speaker 1>It's so big that it gets you part way to

0:33:44.600 --> 0:33:48.480
<v Speaker 1>other stars. And those other stars probably have their own clouds,

0:33:48.520 --> 0:33:50.440
<v Speaker 1>and these stars tugging each other, and one of the

0:33:50.440 --> 0:33:53.720
<v Speaker 1>ways to perturb our or cloud is to have other

0:33:53.720 --> 0:33:56.640
<v Speaker 1>stars come nearby and give it like a little gravitational tug,

0:33:56.920 --> 0:34:00.200
<v Speaker 1>which results in comets falling towards the Earth. Also, an

0:34:00.200 --> 0:34:02.760
<v Speaker 1>orac cloud is not necessarily like a good thing. We

0:34:02.800 --> 0:34:05.200
<v Speaker 1>talked about stealing this, but like it's a bunch of

0:34:05.240 --> 0:34:08.279
<v Speaker 1>bullets hanging over our head where at the bottom of

0:34:08.320 --> 0:34:11.080
<v Speaker 1>this gravity, well, any of them roll down, they could

0:34:11.120 --> 0:34:13.840
<v Speaker 1>totally wipe us out, like deadly hail or something. You

0:34:13.840 --> 0:34:16.120
<v Speaker 1>don't You don't necessarily want that, it won't create a

0:34:16.160 --> 0:34:18.840
<v Speaker 1>winter wonder lamp. You want it early on, so we

0:34:18.880 --> 0:34:21.120
<v Speaker 1>can give you oceans, but then you basically want to

0:34:21.200 --> 0:34:23.239
<v Speaker 1>give them away. To your neighbor, so you don't have

0:34:23.280 --> 0:34:25.799
<v Speaker 1>them anymore. Wow. Alright, so it is kind of like

0:34:25.800 --> 0:34:30.800
<v Speaker 1>a giant interplanetary snowball fight almost or tug of war. Yeah,

0:34:31.040 --> 0:34:33.839
<v Speaker 1>and that's where we think most commets come from. And

0:34:33.920 --> 0:34:35.759
<v Speaker 1>you know, every time you see a comet that's come

0:34:35.800 --> 0:34:38.080
<v Speaker 1>from the outer Solar System, it's been out there for

0:34:38.200 --> 0:34:42.120
<v Speaker 1>billions of years, happily orbiting, not being close to anybody,

0:34:42.280 --> 0:34:45.480
<v Speaker 1>being an introvert. And now it's screaming towards the center

0:34:45.480 --> 0:34:48.439
<v Speaker 1>of the Solar System, maybe hitting a planet, maybe hitting

0:34:48.480 --> 0:34:51.680
<v Speaker 1>the Sun, maybe just whipping around and going back out right.

0:34:51.880 --> 0:34:54.440
<v Speaker 1>It's kind of dangerous. It's actually quite dangerous. You know.

0:34:54.480 --> 0:34:58.200
<v Speaker 1>People talk about asteroids hitting the Earth and worrying about

0:34:58.239 --> 0:35:00.800
<v Speaker 1>big rocks and planet killers and all kinds of stuff,

0:35:01.040 --> 0:35:04.080
<v Speaker 1>But the truth is NASA has most of those figured out.

0:35:04.120 --> 0:35:07.120
<v Speaker 1>Like most of the asteroids, the things in our Solar System,

0:35:07.400 --> 0:35:10.400
<v Speaker 1>we could see them because they're pretty close, certainly anything

0:35:10.440 --> 0:35:13.160
<v Speaker 1>that's big enough to cause us any danger. And NASA

0:35:13.160 --> 0:35:17.000
<v Speaker 1>has a great team of planetary protectors tracking these things

0:35:17.000 --> 0:35:19.120
<v Speaker 1>and predicting where they're gonna be and letting us know

0:35:19.160 --> 0:35:22.040
<v Speaker 1>if they're gonna be anywhere nearby, and often one of

0:35:22.080 --> 0:35:23.920
<v Speaker 1>them slips through and we don't see it until it

0:35:23.960 --> 0:35:26.920
<v Speaker 1>hits us. But that's because it's small. So a really

0:35:27.080 --> 0:35:30.319
<v Speaker 1>big object that would actually cause any damage. NASA is

0:35:30.360 --> 0:35:32.680
<v Speaker 1>pretty sure we're safe from those for a couple hundred

0:35:32.760 --> 0:35:34.880
<v Speaker 1>years because they're hanging out in the Solar System, so

0:35:34.880 --> 0:35:36.919
<v Speaker 1>we can kind of see them, but we can see them.

0:35:36.920 --> 0:35:39.120
<v Speaker 1>But if it's coming from outside the Solar System, then

0:35:39.120 --> 0:35:42.040
<v Speaker 1>it can surprise us. Yeah, if it comes from left field,

0:35:42.360 --> 0:35:44.799
<v Speaker 1>it could be a real surprise. These things could have

0:35:44.920 --> 0:35:48.239
<v Speaker 1>orbits that are hundreds or thousands of years, and so

0:35:48.480 --> 0:35:51.400
<v Speaker 1>the first time we see one might be the last

0:35:51.440 --> 0:35:54.560
<v Speaker 1>time we see one because it could be headed for Earth.

0:35:55.000 --> 0:35:57.360
<v Speaker 1>And so these things could fall into the Solar System

0:35:57.719 --> 0:36:00.760
<v Speaker 1>and smack right into a planet and you know, cause

0:36:00.800 --> 0:36:03.640
<v Speaker 1>a lot of destruction. Because they also they move really

0:36:03.719 --> 0:36:07.520
<v Speaker 1>really fast. They've been accelerating for a long time falling

0:36:07.520 --> 0:36:09.520
<v Speaker 1>in towards the Sun, and so they have a huge

0:36:09.520 --> 0:36:13.200
<v Speaker 1>amount of kinetic energy. This is not a gently tossed snowball.

0:36:13.480 --> 0:36:16.200
<v Speaker 1>This is like a rocket. It's like a rocket propelled

0:36:16.360 --> 0:36:19.200
<v Speaker 1>missile launched snowball. Yeah, you give like a really hard

0:36:19.200 --> 0:36:22.239
<v Speaker 1>block of ice to a major League pitcher and stand

0:36:22.320 --> 0:36:23.680
<v Speaker 1>right in front of the mess. He throws it at

0:36:23.680 --> 0:36:26.040
<v Speaker 1>your face. That's about how terrifying this is. Just like

0:36:26.120 --> 0:36:29.600
<v Speaker 1>when they threw those frozen turkeys at airplane to see

0:36:29.640 --> 0:36:32.400
<v Speaker 1>if the airplanes would break. Is that a real experiment

0:36:32.520 --> 0:36:35.399
<v Speaker 1>used to make that up? That's a real thing. They

0:36:35.480 --> 0:36:38.360
<v Speaker 1>shot frozen turkeys at an airplanes to see what would happen.

0:36:39.080 --> 0:36:41.440
<v Speaker 1>And it's happened before, right, Like our Solar system has

0:36:41.480 --> 0:36:44.680
<v Speaker 1>gone pelted by giant snowballs, and some of them even

0:36:44.800 --> 0:36:47.240
<v Speaker 1>hit some planets. Yeah, exactly. If you think, oh, that's

0:36:47.280 --> 0:36:49.880
<v Speaker 1>not likely to happen, or it might only happen every

0:36:49.920 --> 0:36:53.480
<v Speaker 1>thousand or million years, we don't know how often it happens,

0:36:53.480 --> 0:36:56.440
<v Speaker 1>but we do know that it happened recently. It was

0:36:56.480 --> 0:36:59.680
<v Speaker 1>in the nineties that a big comet hit Jupiter commt

0:37:00.160 --> 0:37:02.600
<v Speaker 1>Maker Levy. It broke up into a bunch of pieces

0:37:02.760 --> 0:37:06.240
<v Speaker 1>and each one pelted Jupiter, and even after it broke

0:37:06.320 --> 0:37:09.960
<v Speaker 1>up and made fireballs that were larger than Earth when

0:37:10.000 --> 0:37:13.240
<v Speaker 1>each one hit. So these are very dramatic planetary events,

0:37:13.320 --> 0:37:15.080
<v Speaker 1>not the kind of thing we want to have happened

0:37:15.080 --> 0:37:18.239
<v Speaker 1>to Earth. Yeah, that would be bad, It would be bad.

0:37:18.280 --> 0:37:20.600
<v Speaker 1>And now, Daniel, I have a note here in the

0:37:20.640 --> 0:37:22.920
<v Speaker 1>document you send me here, and I'm trying to figure

0:37:22.920 --> 0:37:29.560
<v Speaker 1>out it says also space centaurs, And that's it. What

0:37:29.640 --> 0:37:32.840
<v Speaker 1>does that even mean? Space centers are so much fun.

0:37:33.120 --> 0:37:35.440
<v Speaker 1>I decided to make it a whole other episode for

0:37:35.480 --> 0:37:37.719
<v Speaker 1>a few weeks from now. But there is this thing

0:37:37.880 --> 0:37:42.399
<v Speaker 1>in the Solar System called a space center. Seriously, it's

0:37:42.440 --> 0:37:46.280
<v Speaker 1>a thing. Scientists found the thing and called them space centers.

0:37:46.320 --> 0:37:49.480
<v Speaker 1>But they're not like you might imagine, maybe like you know,

0:37:49.960 --> 0:37:52.919
<v Speaker 1>asteroids that happened to look like the fusion between man

0:37:52.960 --> 0:37:56.120
<v Speaker 1>and horse. No, they're just the name that you give

0:37:56.320 --> 0:38:00.360
<v Speaker 1>small objects between Jupiter and Neptune that sort of cross

0:38:00.440 --> 0:38:03.320
<v Speaker 1>back and forth between the orbits of these gas giants,

0:38:03.320 --> 0:38:05.879
<v Speaker 1>sort of like transitional objects. So they're like we could

0:38:05.880 --> 0:38:09.560
<v Speaker 1>call them space unicorns or space griffins. That would be

0:38:09.560 --> 0:38:12.719
<v Speaker 1>too crazy, but we'll go with space centers. I don't

0:38:12.719 --> 0:38:14.520
<v Speaker 1>know what kind of bananas they were smoking the day

0:38:14.640 --> 0:38:16.839
<v Speaker 1>they came up with that name, but it did tickle

0:38:16.920 --> 0:38:19.680
<v Speaker 1>my sense of humor. But they think that maybe space

0:38:19.719 --> 0:38:23.200
<v Speaker 1>centers also have come from the orc cloud. They've essentially

0:38:23.239 --> 0:38:27.240
<v Speaker 1>fallen in and then into these more stable orbits somewhere

0:38:27.239 --> 0:38:29.839
<v Speaker 1>in the outer solar systems thing. Well, then I vote

0:38:29.880 --> 0:38:34.480
<v Speaker 1>we rename comments to space unicorns. I second your motion,

0:38:34.640 --> 0:38:39.160
<v Speaker 1>but I don't think we have any jurisdiction here. All right, Well,

0:38:39.200 --> 0:38:41.680
<v Speaker 1>it sounds like comments are pretty cool. They might be

0:38:41.680 --> 0:38:45.200
<v Speaker 1>coming from the Orc cloud, this theoretical cloud out there

0:38:45.200 --> 0:38:47.680
<v Speaker 1>in space which gave us water, which is a good thing,

0:38:47.719 --> 0:38:50.400
<v Speaker 1>but which may kill us in the future. And so

0:38:50.520 --> 0:38:52.920
<v Speaker 1>we're we're studying this cloud. Now we're studying comments more.

0:38:53.000 --> 0:38:54.960
<v Speaker 1>What are we doing about it? Well, we're doing everything

0:38:55.000 --> 0:38:58.160
<v Speaker 1>we can. It's pretty hard to spot these things right there,

0:38:58.200 --> 0:39:01.520
<v Speaker 1>so small, they're so far away. People have one really

0:39:01.560 --> 0:39:05.000
<v Speaker 1>fun idea for how to visualize these things, and essentially

0:39:05.000 --> 0:39:09.080
<v Speaker 1>it's to look for star eclipses. Like if we are

0:39:09.160 --> 0:39:12.839
<v Speaker 1>surrounded by this huge cloud of these little objects there

0:39:12.880 --> 0:39:15.760
<v Speaker 1>essentially black, they're so far away they don't reflect enough sunlight,

0:39:16.160 --> 0:39:20.680
<v Speaker 1>but occasionally they should pass in front of stars, causing

0:39:20.680 --> 0:39:24.320
<v Speaker 1>these little transitions where the star basically blinks out momentarily.

0:39:25.040 --> 0:39:27.760
<v Speaker 1>So you can look at all the stars and watch

0:39:27.800 --> 0:39:30.480
<v Speaker 1>them and wait to see if you see one of

0:39:30.480 --> 0:39:33.560
<v Speaker 1>these eclipses, and if you do, then you can use

0:39:33.560 --> 0:39:36.520
<v Speaker 1>that to measure like how many things there are out there,

0:39:36.560 --> 0:39:38.920
<v Speaker 1>but based on the rate at which you see these things,

0:39:38.960 --> 0:39:40.959
<v Speaker 1>And if you don't, then you can set a limit

0:39:41.000 --> 0:39:43.080
<v Speaker 1>and say, well, there can't be that many, otherwise I

0:39:43.080 --> 0:39:45.960
<v Speaker 1>would have seen them. You're looking at Like how the

0:39:46.080 --> 0:39:49.080
<v Speaker 1>stars are twinkling, Yeah, because they might be twinkling because

0:39:49.080 --> 0:39:52.200
<v Speaker 1>of a giant comment heading towards us, Yeah, or just

0:39:52.320 --> 0:39:56.640
<v Speaker 1>a giant, silent, frozen comment passing between us and that star.

0:39:57.239 --> 0:39:58.960
<v Speaker 1>And you know it has to line up just right.

0:39:59.000 --> 0:40:01.120
<v Speaker 1>You have to draw a line between the Earth and

0:40:01.160 --> 0:40:04.760
<v Speaker 1>that star super far away, and then the orc cloud

0:40:04.800 --> 0:40:07.960
<v Speaker 1>object has to basically break that line in order for

0:40:08.040 --> 0:40:11.120
<v Speaker 1>there to be this eclipse. So it's not that likely,

0:40:11.320 --> 0:40:13.120
<v Speaker 1>but there are a lot of stars out there and

0:40:13.160 --> 0:40:15.600
<v Speaker 1>maybe a lot of orc cloud objects, so if you

0:40:15.600 --> 0:40:18.080
<v Speaker 1>get enough telescope time, you might be able to spot it.

0:40:18.160 --> 0:40:20.360
<v Speaker 1>And unicorns are pretty magical, so you never know what

0:40:20.360 --> 0:40:23.440
<v Speaker 1>they're gonna do. What if they're all turned out to

0:40:23.440 --> 0:40:27.200
<v Speaker 1>be rainbow colored, that would be amazing. And it could

0:40:27.280 --> 0:40:30.759
<v Speaker 1>also be that if we pass nearby another star, that

0:40:30.760 --> 0:40:34.080
<v Speaker 1>that star could like pass through our or cloud, causing

0:40:34.160 --> 0:40:37.040
<v Speaker 1>like a new bombardment of comets, and that would be

0:40:37.080 --> 0:40:39.120
<v Speaker 1>sort of a confirmation because we'd see a lot of

0:40:39.160 --> 0:40:42.160
<v Speaker 1>these things rushing towards the inner Solar system. Well, clearly

0:40:42.160 --> 0:40:45.000
<v Speaker 1>we need to build like an ice Ford Daniel around

0:40:45.040 --> 0:40:48.759
<v Speaker 1>the Earth. That um, yeah, I think it's called Neptune.

0:40:49.840 --> 0:40:53.040
<v Speaker 1>That's an ice giant, and hopefully it captures these things

0:40:53.160 --> 0:40:55.680
<v Speaker 1>as they come into the inner Solar system. You know,

0:40:55.719 --> 0:40:58.640
<v Speaker 1>we actually do have the gas giants to thank for

0:40:58.719 --> 0:41:01.120
<v Speaker 1>protecting us from a lot of these things. They tend

0:41:01.120 --> 0:41:02.759
<v Speaker 1>to pull them in and they also tend to clean

0:41:02.800 --> 0:41:06.120
<v Speaker 1>them up. So without those big planets out there protecting

0:41:06.239 --> 0:41:10.200
<v Speaker 1>us from the o C bullies throwing snowballs, we would

0:41:10.200 --> 0:41:11.560
<v Speaker 1>have had a rougher time of it. And then, to

0:41:11.640 --> 0:41:14.080
<v Speaker 1>be ironic, if there was a like a giant comment

0:41:14.120 --> 0:41:16.480
<v Speaker 1>heading towards us, but then at the last minute Pluto

0:41:16.560 --> 0:41:20.040
<v Speaker 1>gets in the way and blocks it. That sounds like

0:41:20.080 --> 0:41:22.200
<v Speaker 1>the plot of our movie. That sounds like a good

0:41:22.239 --> 0:41:28.360
<v Speaker 1>slow motion scene at the end and flat and everyone's like, oh, Pluto,

0:41:29.280 --> 0:41:31.160
<v Speaker 1>we took you for granted, but now you see it

0:41:31.320 --> 0:41:35.040
<v Speaker 1>is all it's too late, but now we value your contribution,

0:41:35.640 --> 0:41:38.000
<v Speaker 1>all right. Well, the next time you look out into

0:41:38.040 --> 0:41:40.759
<v Speaker 1>the night, Skuy, we hope you think about what's out

0:41:40.800 --> 0:41:44.320
<v Speaker 1>there and what could possibly be out there, and also

0:41:44.360 --> 0:41:46.960
<v Speaker 1>think of ice unicorns floating out there in space. And

0:41:47.000 --> 0:41:49.399
<v Speaker 1>remember that there's a lot of things out there that

0:41:49.440 --> 0:41:52.800
<v Speaker 1>we still don't understand, sources of mystery, sources of wonder,

0:41:52.880 --> 0:41:56.000
<v Speaker 1>and sources of danger. So we better get on it

0:41:56.040 --> 0:41:58.759
<v Speaker 1>and figure this stuff out before it wipes us out,

0:41:59.000 --> 0:42:01.600
<v Speaker 1>or it might be too late. We're ready or not.

0:42:01.840 --> 0:42:03.480
<v Speaker 1>All right, Well, we hope you enjoyed that. Thanks for

0:42:03.560 --> 0:42:14.600
<v Speaker 1>joining us, See you next time. Thanks for listening, and

0:42:14.640 --> 0:42:17.360
<v Speaker 1>remember that Daniel and Jorge Explain the Universe is a

0:42:17.400 --> 0:42:20.840
<v Speaker 1>production of I Heart Radio or more podcast For my

0:42:20.960 --> 0:42:24.560
<v Speaker 1>heart Radio, visit the I heart Radio app, Apple Podcasts,

0:42:24.680 --> 0:42:27.000
<v Speaker 1>or wherever you listen to your favorite shows.