WEBVTT - Are there comets in the asteroid belt?

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<v Speaker 4>Hey, Daniel, what's the difference between a physicist and an astronomer?

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<v Speaker 1>Oh? I feel like this is a trap.

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<v Speaker 4>I know it seems like a simple question.

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<v Speaker 1>It's a constant debate we have in faculty meetings in

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<v Speaker 1>the Department of Physics and Astronomy. Where do we draw

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<v Speaker 1>the arbitrary dotted line.

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<v Speaker 4>Like, are all astronomers physicists or are some physicists astronomers?

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<v Speaker 4>How does it work?

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<v Speaker 1>I feel like any answer I give here is can

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<v Speaker 1>generate a lot of angry.

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<v Speaker 4>Emails physicists or astronomers.

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<v Speaker 1>A lot of astronomers think of themselves as physicists first

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<v Speaker 1>applied to questions of astronomy, but also a lot of

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<v Speaker 1>astronomers think of themselves as a very different breed of

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<v Speaker 1>scientists who tackle problems differently and think about things differently

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<v Speaker 1>than physicists do.

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<v Speaker 4>All right, that wasn't so hard.

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<v Speaker 1>It was my best non answer.

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<v Speaker 4>All right, may actually just ask non questions in the future.

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<v Speaker 1>Welcome to our non podcast.

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<v Speaker 4>Jorge. I'm a cartoonist and the author of Oliver's Great

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<v Speaker 4>Big Universe.

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<v Speaker 1>Hi, I'm Daniel. I'm a particle physicist and a professor

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<v Speaker 1>at UC Irvine. Though I'm no longer sure what those

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<v Speaker 1>categories even mean.

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<v Speaker 4>You don't know what you are? Are you having like

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<v Speaker 4>an identity crisis?

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<v Speaker 1>Yes? Yes, and yes? I mean if everything's particles, then

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<v Speaker 1>isn't everybody a particle physicist?

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<v Speaker 5>Well?

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<v Speaker 4>Not everything's a particle?

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<v Speaker 1>Right, then we're all field physicists, I suppose.

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<v Speaker 4>Like what's dark energy? Dark energy is not necessarily a particle.

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<v Speaker 1>Yet nobody knows. Maybe dark energy is a particle we

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<v Speaker 1>don't know.

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<v Speaker 4>In fact, isn't particles in arbitrary name or a term like?

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<v Speaker 4>Isn't everything just energy? In the end, maybe you should

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<v Speaker 4>just all be energist.

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<v Speaker 1>Yeah, if you ask ten particle physicists what is a particle,

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<v Speaker 1>you'll get ten different answers.

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<v Speaker 4>Well, if you guys can't even agree, then you know

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<v Speaker 4>what's the point.

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<v Speaker 1>The point is that names and words are how we communicate,

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<v Speaker 1>though it's probably best if we do assign meaning to

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<v Speaker 1>them first.

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<v Speaker 4>Maybe should you just all do science with sign language

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<v Speaker 4>or like charades.

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<v Speaker 1>Let's just give up on language and use math. Right,

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<v Speaker 1>that's just so much more crisp.

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<v Speaker 4>I think charades is not just more fun, but also

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<v Speaker 4>maybe a little bit easier. You would have a whole

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<v Speaker 4>conferences where the presentations are just signists getting up there

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<v Speaker 4>and and miming their papers.

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<v Speaker 1>Is that supposed to increase clarity or just hilarity.

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<v Speaker 4>Well, hopefully it'll increase clarity and also hilarity. But anyways,

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<v Speaker 4>welcome to our podcast. Daniel and Jorge Explain the Universe

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<v Speaker 4>a production of iHeartRadio.

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<v Speaker 1>A podcast that does try to pump both clarity and

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<v Speaker 1>hilarity into your brain. We hope that the universe is

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<v Speaker 1>one that we can understand, that we could take it

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<v Speaker 1>apart into little bits that follow some fundamental rules, then

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<v Speaker 1>we can weave it back together into all the amazing

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<v Speaker 1>and beautiful emergent phenomena that we enjoy, from ourselves, to

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<v Speaker 1>our planets, to our solar system, to everything beyond, and

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<v Speaker 1>explain all of it to you with a little bit

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<v Speaker 1>of Dad Joe hilarity sprinkled on top.

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<v Speaker 4>Yeah, Because whether you're a physicist and astronomer, a cartoonists

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<v Speaker 4>and energiesst or a dad, we all live in this

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<v Speaker 4>universe and we all look out there and we wonder

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<v Speaker 4>how things work, why are things the way they are?

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<v Speaker 4>And can you cerde math?

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<v Speaker 1>Nobody wonders that, man, Nobody wonders that that's done. In

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<v Speaker 1>the top one thousand questions, humans.

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<v Speaker 4>Ask how do you know? Nobody wonders that, Daniel, do

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<v Speaker 4>you have scientific proof or data to back up your claim?

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<v Speaker 1>I do have some data. Yes, I cannot rule it

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<v Speaker 1>out entirely, but over the many tens of thousands of

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<v Speaker 1>questions I get from listeners, I've never gotten that one,

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<v Speaker 1>which means it's not in the top one thousand questions.

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<v Speaker 1>I can confidently say that.

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<v Speaker 4>I see, but you can't say that. Nobody wonders that.

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<v Speaker 1>No, you're right, that was too strong. You wonder that apparently,

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<v Speaker 1>and you're people. So the exception proves the rule.

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<v Speaker 4>I'm sure the situation has come up, like somewhere in

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<v Speaker 4>the history of math, at some point some people needed

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<v Speaker 4>to communicate some calculation or result and they couldn't talk

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<v Speaker 4>for some reason.

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<v Speaker 1>Maybe in Italian universities, you know, hand gestures are much

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<v Speaker 1>more important in communicating these abstract ideas.

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<v Speaker 4>Maybe that's why their equations have so much possessed.

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<v Speaker 1>Yes, exactly, whether we're Italian or not, or using charades

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<v Speaker 1>or symbols or language, we are trying to make sense

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<v Speaker 1>of the universe, and part of that involves categorizing it,

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<v Speaker 1>saying this is one kind of thing, this is another

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<v Speaker 1>kind of thing, whether that means distinguishing between particles and fields,

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<v Speaker 1>or between living things and not living things, or planets

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<v Speaker 1>and dwarf planets. Putting things in boxes is just one

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<v Speaker 1>way the humans make sense of the universe, defining kinds

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<v Speaker 1>of things and applying those labels willy nilly.

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<v Speaker 4>Yeah, and we are trying to make sense of the

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<v Speaker 4>whole universe, not just the little things that we're made

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<v Speaker 4>out of, then that things are made out of, but everything,

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<v Speaker 4>all the huge amazing phenomena that are happening out there,

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<v Speaker 4>the flying planets, the swirling galaxies, and the ginormous galaxy clusters.

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<v Speaker 1>And we'd love to study all that in great detail,

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<v Speaker 1>but most of it is very far away, and so

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<v Speaker 1>far our technological eyeballs aren't powerful enough to really resolve

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<v Speaker 1>all the details. So if we want to get down

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<v Speaker 1>to the astronomical nitty gritty, we're best off studying our

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<v Speaker 1>own backyard, looking in our solar system to understand how

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<v Speaker 1>did it form, what's in it, what kinds of stuff

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<v Speaker 1>are out there swirling around in our neighborhood. And over

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<v Speaker 1>the last few hundred years, we've come to a pretty

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<v Speaker 1>good understanding of what's there and where it's going.

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<v Speaker 4>Yeah, we live in a pretty busy neighborhood full of planets,

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<v Speaker 4>asteroid comets, raining satellites from failed rockets, and so there's

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<v Speaker 4>a lot for us to see in our very near vicinity.

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<v Speaker 1>And while the truth is that the Solar system is

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<v Speaker 1>filled with a huge spectrum of stuff, from tiny cosmic

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<v Speaker 1>dust to huge gas giants to the Sun itself, we

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<v Speaker 1>do like to impose categories on it. And as the

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<v Speaker 1>decades and centuries go by, we keep discovering things that

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<v Speaker 1>lie at the edge of those boundaries that challenge our

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<v Speaker 1>definitions for what is what, Pluto of course being a

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<v Speaker 1>famous example. But as our telescopes get more powerful, we

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<v Speaker 1>keep discovering things in the wrong places or at the

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<v Speaker 1>edge of these definitions that make us wonder, really, where

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<v Speaker 1>do we draw these dotted lines?

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<v Speaker 4>And so to be on the podcast will be tackling

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<v Speaker 4>the question are there comments in the asteroid belt? Now?

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<v Speaker 4>How many pop do you think wonder about this question?

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<v Speaker 5>Day?

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<v Speaker 4>Of your tens of thousands of emails, how many have

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<v Speaker 4>asked this particular question.

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<v Speaker 1>This particular question in this phrasing zero.

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<v Speaker 4>So you're saying the same amount of people that wonder

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<v Speaker 4>if there are comments in the asteroid belt? Also probably

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<v Speaker 4>perhaps wonder if you can cherate now.

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<v Speaker 1>If that was your metric, Yes, but there are a

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<v Speaker 1>lot of questions in the vicinity of this wondering about

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<v Speaker 1>like what's the difference between commets and asteroids? Or why

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<v Speaker 1>do we have comments out there and asteroids over here?

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<v Speaker 1>So I think people are curious about, like what's out

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<v Speaker 1>there in the Solar system? Why do we give them

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<v Speaker 1>these labels? And is it really so neat and crisp.

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<v Speaker 4>This is an interesting question, and so let's dig into it.

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<v Speaker 4>And as usually, we were wondering how many out there

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<v Speaker 4>had thought about this question of whether there are comets

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<v Speaker 4>in the asteroid belt.

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<v Speaker 1>Thanks very much to everybody who contributes their voice to

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<v Speaker 1>this segment of the podcast. Really appreciate your responses. If

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<v Speaker 1>you'd like to hear yourself on a future episode, please

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<v Speaker 1>don't be shy. Write to me too, questions at Danielandjorge

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<v Speaker 1>dot com.

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<v Speaker 4>So think about it for a second. Cast your mind

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<v Speaker 4>out there into the far reaches of our solar system

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<v Speaker 4>and wonder if there are comets in the asteroid belt.

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<v Speaker 4>Here's what people had to say.

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<v Speaker 6>I mean, sure, why not? Maybe they also pass through

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<v Speaker 6>the asteroid belt from time to time. And I always

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<v Speaker 6>thought astroid belt was what's mainly in that wage, not

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<v Speaker 6>what's the only thing in that region.

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<v Speaker 7>I don't have a very good idea the definition of

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<v Speaker 7>a comment versus an asteroid. But I think it has

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<v Speaker 7>to do with amount of ice in the structure. So

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<v Speaker 7>if that is the definition, I can imagine sure there

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<v Speaker 7>might be something that falls under that definition in the

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<v Speaker 7>asteroid belt.

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<v Speaker 1>No comment in the asteroid belt, just asteroids. Comments are

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<v Speaker 1>out a lot further.

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<v Speaker 5>I think another sort of way to distinguish comets from

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<v Speaker 5>asteroids is that asteroids are well in the asteroid belt

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<v Speaker 5>and comets can come from a couple different places. Long

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<v Speaker 5>period comets come from the Oort Cloud, but then there

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<v Speaker 5>are shorter period comets than that. Now, if we have

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<v Speaker 5>a dirty snowball in the asteroid belt, which I believe

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<v Speaker 5>there are, some of these bodies that have been discovered,

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<v Speaker 5>are they correctly labeled as comets?

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<v Speaker 1>Are not commets? I anser are made up ice. I

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<v Speaker 1>think if they were that close they probably melt.

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<v Speaker 8>I think comets coming in at a high rate of

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<v Speaker 8>speed from the Oort Cloud are unlikely to get caught

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<v Speaker 8>up in the asteroid belt.

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<v Speaker 4>Comet might be more about composition than trajectory. I mean

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<v Speaker 4>that if it has more ice than rock, it might

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<v Speaker 4>be a comet.

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<v Speaker 9>I can never remember the difference between asteroids and commets.

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<v Speaker 9>I mean, surely there's a good acronym or something else

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<v Speaker 9>there to remember the difference. But I have to say

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<v Speaker 9>that there's no comets in the asteroid belt because asteroids

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<v Speaker 9>become comets after they and through the atmosphere.

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<v Speaker 10>So there are short period comets, and I think there

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<v Speaker 10>are some that operate closer to the Sun, kind of

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<v Speaker 10>in that asteroid belt range, but being within the ice

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<v Speaker 10>line like most of its quote unquote life, I don't

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<v Speaker 10>really see how they can be long lived.

0:11:20.640 --> 0:11:24.360
<v Speaker 11>I think comets are heavenly bodies which have eccentric orbits

0:11:24.400 --> 0:11:27.280
<v Speaker 11>around the Sun, so they don't fit in nicely with

0:11:27.360 --> 0:11:30.640
<v Speaker 11>the other better behaved inhabitants of the Solar System. So

0:11:30.920 --> 0:11:34.760
<v Speaker 11>although comets may pass through the asteroid belt, I don't

0:11:34.760 --> 0:11:36.600
<v Speaker 11>think they can remain there permanently.

0:11:37.040 --> 0:11:39.280
<v Speaker 12>I think that the asteroid belt is far enough out

0:11:39.480 --> 0:11:42.920
<v Speaker 12>so that comets could remain frozen, and I guess the

0:11:42.960 --> 0:11:45.120
<v Speaker 12>asteroid belt does have a lot of its own gravities,

0:11:45.120 --> 0:11:47.800
<v Speaker 12>so it could capture comets if it was lucky.

0:11:47.960 --> 0:11:50.960
<v Speaker 8>I think there might be a few transient comets in

0:11:51.000 --> 0:11:53.640
<v Speaker 8>the asteroid belt, but I don't think that there would

0:11:53.720 --> 0:11:58.000
<v Speaker 8>be much chance for comets to persist in that kind

0:11:58.040 --> 0:12:01.959
<v Speaker 8>of orbit because of exposure to the wind and the

0:12:02.000 --> 0:12:06.760
<v Speaker 8>interaction of the gravity of Jupiter disrupting either the orbit

0:12:06.880 --> 0:12:08.160
<v Speaker 8>or the structure of those comets.

0:12:08.320 --> 0:12:11.079
<v Speaker 13>Guess there could be comets, but yeah, usually commas have

0:12:11.120 --> 0:12:13.239
<v Speaker 13>a large orbit, a very large orbit in detail.

0:12:13.520 --> 0:12:15.079
<v Speaker 8>That wouldn't be the case if it was found in

0:12:15.120 --> 0:12:15.840
<v Speaker 8>the asteroid belt.

0:12:15.920 --> 0:12:19.480
<v Speaker 4>So yeah, pretty wide range of answers here. I guess

0:12:19.559 --> 0:12:20.959
<v Speaker 4>there's only two options, yes or.

0:12:20.920 --> 0:12:23.720
<v Speaker 1>No, or there could be this is a trick question,

0:12:24.320 --> 0:12:26.559
<v Speaker 1>or let's answer in charades, right.

0:12:29.040 --> 0:12:31.040
<v Speaker 4>What made you think of this question? Why are there

0:12:31.080 --> 0:12:33.840
<v Speaker 4>commets in the asteroid belt? Is this something that astronomers

0:12:33.880 --> 0:12:34.800
<v Speaker 4>have been wondering about.

0:12:34.960 --> 0:12:36.800
<v Speaker 1>I've been thinking about this kind of question for a

0:12:36.840 --> 0:12:40.360
<v Speaker 1>while because I find the whole labeling of stuff in

0:12:40.400 --> 0:12:43.880
<v Speaker 1>the Solar System to be kind of ridiculous and arbitrary.

0:12:43.960 --> 0:12:46.640
<v Speaker 1>You know, we're just humans putting dotted lines on a

0:12:46.640 --> 0:12:49.040
<v Speaker 1>smooth spectrum of different kind of stuff that's out there.

0:12:49.480 --> 0:12:52.680
<v Speaker 1>But also it is interesting because when you invent categories,

0:12:52.679 --> 0:12:54.680
<v Speaker 1>then you can wonder about things and the boundaries or

0:12:54.679 --> 0:12:57.160
<v Speaker 1>things across the boundaries. And then I read a paper

0:12:57.200 --> 0:13:00.000
<v Speaker 1>about people who were finding weird stuff in the asteroids

0:13:00.320 --> 0:13:01.640
<v Speaker 1>that didn't belong there.

0:13:02.520 --> 0:13:05.320
<v Speaker 4>All right, well, let's dig into it, Daniel, I guess

0:13:05.360 --> 0:13:08.280
<v Speaker 4>the question is, but comets and asteroids, what's the difference

0:13:08.320 --> 0:13:08.880
<v Speaker 4>between the two?

0:13:09.080 --> 0:13:13.000
<v Speaker 1>Yes, So these are two human constructed, arbitrary definitions that

0:13:13.120 --> 0:13:16.800
<v Speaker 1>are mostly historical and don't really represent like our best

0:13:16.880 --> 0:13:19.200
<v Speaker 1>understanding of what's out there in the Solar System. If

0:13:19.240 --> 0:13:21.120
<v Speaker 1>you were going to start today, you probably wouldn't come

0:13:21.200 --> 0:13:23.959
<v Speaker 1>up with the same definitions. But you know, science is

0:13:24.000 --> 0:13:26.120
<v Speaker 1>a human endeavor, which means we need to understand the

0:13:26.120 --> 0:13:28.679
<v Speaker 1>words scientists use when they talk to each other, even

0:13:28.720 --> 0:13:31.560
<v Speaker 1>if it's imprecise or historical or ridiculous. So what do

0:13:31.600 --> 0:13:33.720
<v Speaker 1>we mean by an asteroid and what do we mean

0:13:33.800 --> 0:13:37.160
<v Speaker 1>by a comet? So an asteroid is basically like a

0:13:37.200 --> 0:13:40.680
<v Speaker 1>mini planet. Right, there's this complicated definition of a planet

0:13:41.040 --> 0:13:44.360
<v Speaker 1>as an object in the Solar System that's orbiting the Sun,

0:13:45.000 --> 0:13:48.600
<v Speaker 1>is big enough to be mostly round and has cleared

0:13:48.600 --> 0:13:52.360
<v Speaker 1>its own path. An asteroid is like that, except that

0:13:52.440 --> 0:13:56.040
<v Speaker 1>it's not necessarily big enough to be round, and it

0:13:56.080 --> 0:13:59.840
<v Speaker 1>hasn't cleared its own path. So it's like a mini chunky,

0:14:00.040 --> 0:14:03.280
<v Speaker 1>funky shaped planet that doesn't have its own parking space.

0:14:03.360 --> 0:14:07.360
<v Speaker 4>But is there like a size range, like can you

0:14:07.400 --> 0:14:11.839
<v Speaker 4>have an asteroid the size of a marble or does

0:14:11.880 --> 0:14:12.880
<v Speaker 4>that count as something else?

0:14:13.160 --> 0:14:16.040
<v Speaker 1>Technically, there's no minimum size for an asteroid, so like

0:14:16.080 --> 0:14:20.040
<v Speaker 1>a dust grain technically is an asteroid. Practically that's very,

0:14:20.120 --> 0:14:22.280
<v Speaker 1>very difficult to see those things, you know, of course,

0:14:22.320 --> 0:14:24.160
<v Speaker 1>unless they land on Earth, in which case they're no

0:14:24.200 --> 0:14:27.160
<v Speaker 1>longer an asteroid. We can't really detect them in the

0:14:27.160 --> 0:14:30.240
<v Speaker 1>asteroid belt unless they're very shiny or large, or some

0:14:30.400 --> 0:14:33.760
<v Speaker 1>combination of them. So the range of asteroids that we've discovered,

0:14:33.840 --> 0:14:36.640
<v Speaker 1>like in the asteroid belt, goes from things like down

0:14:36.680 --> 0:14:39.480
<v Speaker 1>to one meter across all the way up to things

0:14:39.600 --> 0:14:44.640
<v Speaker 1>like five hundred kilometers across. So there's an incredible range

0:14:44.640 --> 0:14:47.080
<v Speaker 1>of stuff in the asteroid belt that we call asteroids.

0:14:47.160 --> 0:14:48.920
<v Speaker 1>We give them all the same name.

0:14:49.480 --> 0:14:51.840
<v Speaker 4>But I guess there's one common thread, which is that

0:14:51.880 --> 0:14:54.560
<v Speaker 4>it needs to be some kind of solid material, right,

0:14:55.040 --> 0:14:58.440
<v Speaker 4>Like a cloud of gas doesn't count as an asteroid, right.

0:14:58.600 --> 0:15:00.960
<v Speaker 1>Yeah, that's right, needs to hold itself together.

0:15:00.760 --> 0:15:02.560
<v Speaker 4>So it has to be solid, and it has to

0:15:02.560 --> 0:15:05.240
<v Speaker 4>be in space. Is that about the definition of an asteroid?

0:15:05.720 --> 0:15:08.600
<v Speaker 4>Something solid floating in space that's not round.

0:15:08.520 --> 0:15:10.160
<v Speaker 1>And it has to be orbiting the Sun. It's a

0:15:10.240 --> 0:15:13.440
<v Speaker 1>rocky object that orbits the Sun and doesn't qualify as

0:15:13.440 --> 0:15:15.800
<v Speaker 1>being a planet or a comet.

0:15:16.200 --> 0:15:18.000
<v Speaker 4>But I guess, why does it need to be orbiting

0:15:18.040 --> 0:15:20.480
<v Speaker 4>the Sun? Can't you have an asteroid other than space

0:15:20.560 --> 0:15:22.320
<v Speaker 4>by itself? Like what do you call those?

0:15:22.800 --> 0:15:25.120
<v Speaker 1>Well, if it's not orbiting the Sun and it's orbiting

0:15:25.200 --> 0:15:28.000
<v Speaker 1>like the Earth, then you'd call it a moon. If

0:15:28.040 --> 0:15:30.880
<v Speaker 1>it's not orbiting the Sun and it's not really orbiting anything,

0:15:30.960 --> 0:15:34.240
<v Speaker 1>it's just like floating in the galaxy, then it's not

0:15:34.240 --> 0:15:35.520
<v Speaker 1>an asteroid. It's just a rock.

0:15:36.800 --> 0:15:41.000
<v Speaker 4>Is that the official astronomy definition? It's just a space rock?

0:15:41.520 --> 0:15:45.320
<v Speaker 4>Are you sure we don't want to anger any astronomers.

0:15:44.840 --> 0:15:46.840
<v Speaker 1>Now, it's definitely don't. And you know, I'm in a

0:15:46.840 --> 0:15:50.360
<v Speaker 1>department of physics and astronomy, and that doesn't make me

0:15:50.480 --> 0:15:53.240
<v Speaker 1>an astronomer, even though I'm technically a professor of physics

0:15:53.240 --> 0:15:56.320
<v Speaker 1>and astronomy, and I don't want to speak for the astronomers,

0:15:56.920 --> 0:15:59.280
<v Speaker 1>but that is my understanding. If it's out there in

0:15:59.280 --> 0:16:02.440
<v Speaker 1>interstellar space, you could call it an interstellar asteroid. I

0:16:02.480 --> 0:16:05.680
<v Speaker 1>suppose the problem is we haven't like discovered or seen

0:16:05.720 --> 0:16:07.480
<v Speaker 1>many of those. You know, we have had a couple

0:16:07.520 --> 0:16:10.800
<v Speaker 1>of interstellar objects come, but those who think are interstellar

0:16:10.880 --> 0:16:15.720
<v Speaker 1>comets not interstellar asteroids. So yeah, that's a whole new frontier.

0:16:15.880 --> 0:16:18.200
<v Speaker 4>Yeah, like like in Star Wars when they run into

0:16:18.240 --> 0:16:21.600
<v Speaker 4>like an asteroid field, are they taken not calling it

0:16:21.640 --> 0:16:22.080
<v Speaker 4>the right thing?

0:16:22.400 --> 0:16:22.560
<v Speaker 5>Well?

0:16:22.600 --> 0:16:25.640
<v Speaker 1>I think those are usually near a stars. They're probably

0:16:25.640 --> 0:16:26.560
<v Speaker 1>are orbiting a star.

0:16:26.720 --> 0:16:28.080
<v Speaker 4>I don't know, they never show the star.

0:16:30.120 --> 0:16:32.400
<v Speaker 1>That's what I'm always thinking about when they're dodging asteroids.

0:16:32.480 --> 0:16:34.680
<v Speaker 1>Where's the star that makes us an asteroid and not

0:16:34.760 --> 0:16:35.160
<v Speaker 1>a rock?

0:16:36.080 --> 0:16:40.080
<v Speaker 4>Excuse me? Excuse me, I don't see the sun actually,

0:16:42.160 --> 0:16:45.920
<v Speaker 4>all right, So an asteroid is by definition a rock

0:16:46.320 --> 0:16:50.000
<v Speaker 4>that's orbiting the sun. Basically, Yeah, it has to be solid, right,

0:16:50.280 --> 0:16:52.920
<v Speaker 4>or like a solid object that's orbiting the sun.

0:16:53.000 --> 0:16:55.200
<v Speaker 1>Yeah, And your point there about it being solid is crucial.

0:16:55.520 --> 0:16:59.000
<v Speaker 1>Asteroids are rocky objects, meaning they're made of rock and

0:16:59.080 --> 0:17:01.360
<v Speaker 1>metal in this kind kind of stuff, and that's going

0:17:01.400 --> 0:17:04.720
<v Speaker 1>to help us distinguish them from their cousin the comet.

0:17:05.200 --> 0:17:07.000
<v Speaker 4>Gosh, well, how do you define a rock?

0:17:07.480 --> 0:17:09.600
<v Speaker 1>A rock is something made it mostly out of silica.

0:17:09.720 --> 0:17:12.159
<v Speaker 1>You know, the chemical composition of these things tells you

0:17:12.200 --> 0:17:14.280
<v Speaker 1>what it is. If it's a blob of iron, then

0:17:14.280 --> 0:17:17.720
<v Speaker 1>it's metal. You know, if it's a this is all chemistry. Man,

0:17:17.760 --> 0:17:20.600
<v Speaker 1>it's well beyond me. Don't ask me to do chemistry.

0:17:20.680 --> 0:17:22.760
<v Speaker 4>Joined the Department of Physics, Astronomy and chemistry.

0:17:22.840 --> 0:17:27.240
<v Speaker 1>No, never, never, My son is into chemistry.

0:17:27.320 --> 0:17:29.560
<v Speaker 4>Yeah, I guess, I guess all those professors just don't

0:17:29.600 --> 0:17:30.280
<v Speaker 4>have the chemistry.

0:17:30.880 --> 0:17:33.960
<v Speaker 1>I don't have chemistry with those professors, that's for sure. No.

0:17:34.119 --> 0:17:37.240
<v Speaker 1>I respect chemistry, I respect chemists, but I'm not that

0:17:37.359 --> 0:17:40.879
<v Speaker 1>in the history of asteroids is kind of fascinating because,

0:17:40.880 --> 0:17:43.639
<v Speaker 1>you know, we use these words, but for a long time,

0:17:43.720 --> 0:17:47.480
<v Speaker 1>people didn't really distinguish between planets and asteroids, and the

0:17:47.480 --> 0:17:50.119
<v Speaker 1>word planet was used very broadly, like the moon was

0:17:50.160 --> 0:17:52.680
<v Speaker 1>a planet for a while before we invented the concept

0:17:52.720 --> 0:17:55.240
<v Speaker 1>of a moon. So these things change with time. It's

0:17:55.280 --> 0:17:58.160
<v Speaker 1>possible to redefine what is a planet or an asteroid.

0:17:58.200 --> 0:18:01.200
<v Speaker 1>Maybe in five hundred years, honors will have totally different

0:18:01.240 --> 0:18:03.119
<v Speaker 1>words for these things, or use the same words in

0:18:03.160 --> 0:18:03.840
<v Speaker 1>a different way.

0:18:04.280 --> 0:18:06.600
<v Speaker 4>Who knows, yeah, or maybe they'll use the same like

0:18:06.680 --> 0:18:07.480
<v Speaker 4>charade gesture.

0:18:08.960 --> 0:18:13.480
<v Speaker 1>That's exactly when we transition fully to charade science, then.

0:18:13.880 --> 0:18:15.600
<v Speaker 4>We're I wonder if in the future we transition to

0:18:15.680 --> 0:18:19.119
<v Speaker 4>like telepathy, you know, then you don't need words, you

0:18:19.160 --> 0:18:20.280
<v Speaker 4>can just transfer thoughts.

0:18:20.320 --> 0:18:23.480
<v Speaker 1>All right, Well, if we're playing charades and your clue

0:18:23.600 --> 0:18:26.919
<v Speaker 1>was asteroid, what motions would you use to describe it?

0:18:27.040 --> 0:18:31.840
<v Speaker 4>Oh, that's totally easy, Dan, I would do this, so

0:18:31.960 --> 0:18:33.880
<v Speaker 4>he totally conveys what asteroid means.

0:18:34.040 --> 0:18:36.440
<v Speaker 1>Okay, that's a funny way to duck the question. But seriously,

0:18:37.080 --> 0:18:39.440
<v Speaker 1>can you describe what an asteroid gesture would be?

0:18:40.119 --> 0:18:45.200
<v Speaker 4>I just did, all right, but I feel like we're

0:18:45.200 --> 0:18:46.920
<v Speaker 4>getting a little bit uh delled.

0:18:48.400 --> 0:18:50.760
<v Speaker 1>Well, then let's go back to the history of asteroids,

0:18:50.760 --> 0:18:53.800
<v Speaker 1>because I also think it's fascinating when we knew there

0:18:53.800 --> 0:18:57.320
<v Speaker 1>were lots of asteroids, Like, as our technology developed to

0:18:57.320 --> 0:18:59.959
<v Speaker 1>be able to see these things, right, we can see smaller,

0:19:00.160 --> 0:19:03.000
<v Speaker 1>smaller ones. Then we discovered more, and it's this incredible

0:19:03.000 --> 0:19:05.120
<v Speaker 1>sort of explosion of discovery.

0:19:05.680 --> 0:19:07.359
<v Speaker 4>But how do we see them? Like you sort of

0:19:07.400 --> 0:19:10.280
<v Speaker 4>can't see asteroids with the naked eye, can you? Or

0:19:10.320 --> 0:19:12.160
<v Speaker 4>sometimes if they like catch the sun.

0:19:12.480 --> 0:19:15.480
<v Speaker 1>Technically, I don't see why you couldn't have photons hit

0:19:15.520 --> 0:19:18.320
<v Speaker 1>an asteroid and then hit your eye, but enough of

0:19:18.359 --> 0:19:21.200
<v Speaker 1>them for you to spot it and identify it seems

0:19:21.320 --> 0:19:24.960
<v Speaker 1>very challenging. So asteroids are usually seen through telescopes just

0:19:24.960 --> 0:19:27.720
<v Speaker 1>because you know, the aperture is larger and you're gathering

0:19:27.760 --> 0:19:30.600
<v Speaker 1>more light and so it's basically a bigger eyeball.

0:19:31.240 --> 0:19:32.959
<v Speaker 4>So is that how they discover them? Like they were

0:19:33.000 --> 0:19:35.320
<v Speaker 4>looking through a telescope and they saw a bunch of

0:19:35.320 --> 0:19:38.720
<v Speaker 4>these They probably looked like pinpoint stars, but they were

0:19:38.760 --> 0:19:41.520
<v Speaker 4>probably moving faster than the regular stars.

0:19:41.359 --> 0:19:44.439
<v Speaker 1>Exactly the same way that planets move across the field

0:19:44.560 --> 0:19:47.520
<v Speaker 1>of the stars, which is how you know that they're closer, right,

0:19:47.560 --> 0:19:49.760
<v Speaker 1>And that's why sort of planets and asteroids were called

0:19:49.760 --> 0:19:52.200
<v Speaker 1>the same thing for a long time before we distinguished

0:19:52.400 --> 0:19:55.880
<v Speaker 1>between them somewhat arbitrarily. And you know, until one hundred

0:19:55.880 --> 0:19:58.320
<v Speaker 1>and fifty years ago, we thought there were six ish planets,

0:19:58.400 --> 0:20:01.479
<v Speaker 1>and we thought there were about ten astraids. Like eighteen

0:20:01.600 --> 0:20:04.840
<v Speaker 1>forty nine, we knew about ten different asteroids, and then

0:20:04.880 --> 0:20:08.160
<v Speaker 1>as technology improved, that number grew to be one hundred

0:20:08.200 --> 0:20:12.760
<v Speaker 1>twenty years later, to a thousand about one hundred years ago,

0:20:12.800 --> 0:20:16.240
<v Speaker 1>And now we know about more than a million individual

0:20:16.359 --> 0:20:19.720
<v Speaker 1>asteroids that can be tracked, and we have these telescopes

0:20:19.760 --> 0:20:21.920
<v Speaker 1>that look at these things, of course, because we're concerned

0:20:21.960 --> 0:20:24.840
<v Speaker 1>about whether one of them might eventually hit the Earth,

0:20:25.280 --> 0:20:27.840
<v Speaker 1>and NASA is tracking all of these things. And as

0:20:27.840 --> 0:20:30.160
<v Speaker 1>you say it, they don't glow, but they do reflect

0:20:30.200 --> 0:20:33.040
<v Speaker 1>the Sun, and so when the conditions line up for

0:20:33.119 --> 0:20:35.560
<v Speaker 1>like photons from the Sun to hit the asteroid and

0:20:35.560 --> 0:20:39.080
<v Speaker 1>then reflect back into the telescope aperture, that's when we

0:20:39.119 --> 0:20:41.439
<v Speaker 1>see it. But a lot of these things are invisible

0:20:41.520 --> 0:20:44.440
<v Speaker 1>for long fractions of their flight around the Sun.

0:20:44.720 --> 0:20:47.960
<v Speaker 4>Now, what was the technological advance that it allows us

0:20:47.960 --> 0:20:50.639
<v Speaker 4>to see so many? Like you, we just got bigger

0:20:50.680 --> 0:20:53.719
<v Speaker 4>telescopes and we're more sensitive. They could see dimmer things,

0:20:53.960 --> 0:20:57.800
<v Speaker 4>or we could maybe zoom with more presition into certain

0:20:57.800 --> 0:20:59.879
<v Speaker 4>parts of the sky.

0:21:00.040 --> 0:21:03.480
<v Speaker 1>Yea. It's a combination of more telescopes and bigger telescopes.

0:21:03.760 --> 0:21:07.360
<v Speaker 1>So a lot of this is limited by glass technology.

0:21:07.880 --> 0:21:10.439
<v Speaker 1>Can you make lenses that are big and smooth and

0:21:10.560 --> 0:21:14.479
<v Speaker 1>free of aberrations and so like Galileo's original telescopes are

0:21:14.480 --> 0:21:17.280
<v Speaker 1>pretty bad, right, and limited by the size of the

0:21:17.320 --> 0:21:20.240
<v Speaker 1>telescope you could make because the glass you could grind

0:21:20.280 --> 0:21:23.040
<v Speaker 1>and have it to be smooth and not create distortions

0:21:23.119 --> 0:21:25.600
<v Speaker 1>was pretty small. But then people got a lot better

0:21:25.720 --> 0:21:28.439
<v Speaker 1>at that about one hundred and fifty years ago, and

0:21:28.560 --> 0:21:30.879
<v Speaker 1>things exploded from there, and then we also just built

0:21:30.920 --> 0:21:33.920
<v Speaker 1>more of them. And now, of course we have dedicated

0:21:34.040 --> 0:21:36.280
<v Speaker 1>space telescopes just out there looking for.

0:21:36.200 --> 0:21:39.960
<v Speaker 4>These things millionnasteras. That's pretty wild. I mean, if you

0:21:40.000 --> 0:21:42.440
<v Speaker 4>could see the way these telescopes could see, you would

0:21:42.480 --> 0:21:48.120
<v Speaker 4>see the night sky basically like shifting all the time, right, moving, swirling, spinning.

0:21:48.359 --> 0:21:51.119
<v Speaker 1>Yeah, it's much more dynamic than you imagine. There's a

0:21:51.160 --> 0:21:54.720
<v Speaker 1>lot of stuff out there. There's also an inflection point

0:21:54.760 --> 0:21:57.080
<v Speaker 1>in sort of the history of astronomy in the mid

0:21:57.200 --> 0:22:00.920
<v Speaker 1>nineties when Jupiter was hit by a comet. Comet Shoemaker

0:22:01.000 --> 0:22:03.959
<v Speaker 1>Levee broke up as it entered the inner Solar System,

0:22:04.119 --> 0:22:06.400
<v Speaker 1>whipped around the Sun, and then each of the twenty

0:22:06.480 --> 0:22:10.560
<v Speaker 1>six or so pieces slammed into Jupiter, creating huge fireballs

0:22:10.600 --> 0:22:13.120
<v Speaker 1>the size of the Earth. And that's made people wake

0:22:13.200 --> 0:22:15.400
<v Speaker 1>up to the idea that like, wow, you know, asteroids

0:22:15.400 --> 0:22:18.200
<v Speaker 1>of comets really could hit the Earth. This is potentially

0:22:18.200 --> 0:22:21.479
<v Speaker 1>an existential threat. And NASA has really been investing in

0:22:21.600 --> 0:22:26.080
<v Speaker 1>tracking near Earth objects ever since that moment. Comet Shoemaker Levee.

0:22:26.320 --> 0:22:28.639
<v Speaker 1>That's one reason why we went from like seeing some

0:22:28.760 --> 0:22:30.960
<v Speaker 1>of the asteroids to like, let's be serious about this,

0:22:31.119 --> 0:22:34.200
<v Speaker 1>folks and make a solid catalog of all the biggest ones.

0:22:35.920 --> 0:22:39.000
<v Speaker 4>Okay, so that's asteroids, and most asteroids are in the

0:22:39.040 --> 0:22:41.480
<v Speaker 4>asteroid belt, right, or there's a couple of belts around

0:22:41.480 --> 0:22:42.240
<v Speaker 4>the Solar System.

0:22:42.680 --> 0:22:45.760
<v Speaker 1>Yeah, asteroids are mostly in the asteroid belt, which is

0:22:45.760 --> 0:22:48.880
<v Speaker 1>between Mars and Jupiter. And that's not an accident, right.

0:22:48.920 --> 0:22:52.400
<v Speaker 1>The reason we have asteroids is basically because of Jupiter.

0:22:52.960 --> 0:22:55.679
<v Speaker 1>Jupiter has a huge fraction of the mass of the

0:22:55.680 --> 0:22:58.480
<v Speaker 1>Solar System that's not in the Sun. Like the Sun

0:22:58.720 --> 0:23:01.240
<v Speaker 1>is ninety nine percent of the mass Solar System, and

0:23:01.440 --> 0:23:04.440
<v Speaker 1>Jupiter is almost three times the mass of everything else

0:23:04.480 --> 0:23:07.960
<v Speaker 1>in the Solar System combined, including like Saturn and Neptune

0:23:07.960 --> 0:23:11.960
<v Speaker 1>and Urinous. So it's a big massive thing and it's gravity.

0:23:12.040 --> 0:23:16.159
<v Speaker 4>Wait what so like seventy percent of the non Sun

0:23:16.200 --> 0:23:17.800
<v Speaker 4>mass in the Solar System is Jupiter.

0:23:18.160 --> 0:23:20.040
<v Speaker 1>Yeah, Jupiter is a big hog.

0:23:20.320 --> 0:23:23.200
<v Speaker 4>You know, I'm not sure we should be shaming Jupiter, Daniel.

0:23:25.240 --> 0:23:27.440
<v Speaker 1>You're taking big hog to be pejorative. I meant that

0:23:27.480 --> 0:23:31.480
<v Speaker 1>as a compliment, like, hey, good job, Jupiter, congrats.

0:23:32.520 --> 0:23:33.920
<v Speaker 4>I don't know, I guess it was your tone.

0:23:34.119 --> 0:23:38.879
<v Speaker 1>Okay, Hey, Jupiter is a big hog has that. But

0:23:38.960 --> 0:23:41.600
<v Speaker 1>you know, this is a gravitational runaway effect at work.

0:23:41.920 --> 0:23:43.840
<v Speaker 1>You have a huge cloud of gas and dust that

0:23:43.920 --> 0:23:47.280
<v Speaker 1>forms the Solar System. Somewhere in there is an initial

0:23:47.320 --> 0:23:50.080
<v Speaker 1>density that causes the collapse that's going to turn into

0:23:50.080 --> 0:23:53.359
<v Speaker 1>the Sun. But if somewhere else in that nearby cloud

0:23:53.440 --> 0:23:56.600
<v Speaker 1>also has a little spot of density, then it can

0:23:56.680 --> 0:23:59.600
<v Speaker 1>form its own little runaway effect to gobble up some

0:23:59.720 --> 0:24:02.200
<v Speaker 1>of that gas and dust before it falls into the Sun.

0:24:02.680 --> 0:24:03.880
<v Speaker 1>And that's what Jupiter did.

0:24:04.920 --> 0:24:07.159
<v Speaker 4>Now, Jupiter is mostly made out of gas, So I

0:24:07.240 --> 0:24:09.199
<v Speaker 4>wonder why got so much of the gas in the

0:24:09.200 --> 0:24:12.080
<v Speaker 4>Solar system? Like, did it some of it just blow

0:24:12.160 --> 0:24:14.760
<v Speaker 4>away when the Sun ignited or what and it just

0:24:14.760 --> 0:24:16.199
<v Speaker 4>happened to gather around Jupiter.

0:24:16.560 --> 0:24:19.280
<v Speaker 1>Yeah, there's a lot of controversy about that. Where gas

0:24:19.320 --> 0:24:21.680
<v Speaker 1>giants form. Do they mostly form in the outer Solar

0:24:21.720 --> 0:24:24.000
<v Speaker 1>System and then transition inward? Do they form in the

0:24:24.000 --> 0:24:27.000
<v Speaker 1>inner Solar System? We see a lot of gas giants

0:24:27.040 --> 0:24:30.240
<v Speaker 1>in exoplanet systems that are near their Sun, but we

0:24:30.280 --> 0:24:34.640
<v Speaker 1>think probably these gas giants form farther away because further

0:24:34.680 --> 0:24:37.520
<v Speaker 1>away from the Sun. Number one, the gas isn't being

0:24:37.560 --> 0:24:40.600
<v Speaker 1>blown away by the radiation of the Sun. And number two,

0:24:40.880 --> 0:24:44.200
<v Speaker 1>there's ice there, which helps these planets accrete more quickly.

0:24:44.240 --> 0:24:47.000
<v Speaker 1>There's like more stuff to gather. So we think that

0:24:47.119 --> 0:24:50.320
<v Speaker 1>Jupiter became so big because it's so close to that

0:24:50.480 --> 0:24:53.280
<v Speaker 1>snow line, you know, where ice and frozen vapor can

0:24:53.320 --> 0:24:56.600
<v Speaker 1>still exist. It helps these planets a creek quickly. And

0:24:56.600 --> 0:24:58.919
<v Speaker 1>then we think it's probably a complicated history of Jupiter

0:24:59.000 --> 0:25:02.160
<v Speaker 1>moving in towards the Sun and then getting pulled back

0:25:02.200 --> 0:25:05.639
<v Speaker 1>out by a now missing gas giant which was ejected

0:25:05.880 --> 0:25:09.040
<v Speaker 1>in that interaction. So the whole formation of Jupiter is

0:25:09.040 --> 0:25:11.159
<v Speaker 1>a really fascinating and complex topic.

0:25:12.520 --> 0:25:14.720
<v Speaker 4>All right, Well, let's dig into where else in the

0:25:14.760 --> 0:25:17.320
<v Speaker 4>Solar System you might find asteroids, and then we'll dig

0:25:17.359 --> 0:25:21.119
<v Speaker 4>into comments and whether there are any in the asteroid belt.

0:25:21.480 --> 0:25:23.439
<v Speaker 4>So we'll get to that, but first let's take a

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<v Speaker 4>Where we're talking about asteroids, commets and belts and the

0:29:53.200 --> 0:29:56.880
<v Speaker 4>fact that Jupiter needs a really big built And the

0:29:56.960 --> 0:30:00.080
<v Speaker 4>question is are there commets in the asteroid belt. So

0:30:00.080 --> 0:30:02.360
<v Speaker 4>we've been talking about asteroids what they are, and you

0:30:02.400 --> 0:30:04.840
<v Speaker 4>said they're mostly in the asteroid built but can you

0:30:04.880 --> 0:30:06.960
<v Speaker 4>find them anywhere else in the Solar System.

0:30:07.400 --> 0:30:10.840
<v Speaker 1>You can find them also in Jupiter's orbit. So there's

0:30:10.880 --> 0:30:14.560
<v Speaker 1>a big blob of asteroids ahead of Jupiter in its

0:30:14.640 --> 0:30:17.680
<v Speaker 1>orbit and another one behind Jupiter in its orbit. They're

0:30:17.720 --> 0:30:21.080
<v Speaker 1>like leading and trailing Jupiter. These are called the Greeks

0:30:21.120 --> 0:30:24.280
<v Speaker 1>and the Trojans, and these are just like big clumps

0:30:24.280 --> 0:30:27.760
<v Speaker 1>of rock that are in Jupiter's orbit. So you know, technically,

0:30:27.920 --> 0:30:32.600
<v Speaker 1>did Jupiter really clear its orbit? Is Jupiter even a planet? Well?

0:30:32.640 --> 0:30:34.640
<v Speaker 4>I mean is if these things are orbiting Jupiter, then

0:30:34.640 --> 0:30:36.280
<v Speaker 4>they're not asteroids, right, No.

0:30:36.360 --> 0:30:39.200
<v Speaker 1>These things are orbiting the Sun in the same orbit

0:30:39.320 --> 0:30:43.240
<v Speaker 1>as Jupiter. Oh yeah, And all of this is just

0:30:43.320 --> 0:30:46.480
<v Speaker 1>dominated by Jupiter's gravity. Like, why don't the rocks in

0:30:46.520 --> 0:30:49.720
<v Speaker 1>the asteroid belt come together to make another planet the

0:30:49.760 --> 0:30:52.560
<v Speaker 1>way they did for Earth or for Mercury, or even

0:30:52.640 --> 0:30:56.400
<v Speaker 1>for Mars. The answer is Jupiter's gravity distorts it, It

0:30:56.480 --> 0:30:59.800
<v Speaker 1>pulls it apart, it shreds things. These are all tidal

0:30:59.800 --> 0:31:02.040
<v Speaker 1>for do you put in gravity so strongly if you

0:31:02.120 --> 0:31:04.960
<v Speaker 1>try to pull these things together, It's gravity would tug

0:31:05.000 --> 0:31:07.480
<v Speaker 1>on one side harder than the tug's on another side

0:31:07.760 --> 0:31:10.320
<v Speaker 1>and pull it apart. So it sort of like mixes

0:31:10.360 --> 0:31:11.920
<v Speaker 1>it up. It's I got a big spoon, and it

0:31:12.000 --> 0:31:14.880
<v Speaker 1>keeps stirring up the asteroid belt and keeping it from

0:31:14.920 --> 0:31:17.160
<v Speaker 1>coalescing into something WOA.

0:31:17.200 --> 0:31:20.560
<v Speaker 4>It just disrupts the formation of any planets in that

0:31:20.640 --> 0:31:24.440
<v Speaker 4>sort of neighborhood exactly. Do we have any asteroids out

0:31:24.480 --> 0:31:27.160
<v Speaker 4>there beyond the gas giants?

0:31:27.320 --> 0:31:29.960
<v Speaker 1>There are definitely rocks further out in the Solar System,

0:31:30.600 --> 0:31:33.520
<v Speaker 1>because remember any big rocky object that's not a planet

0:31:33.640 --> 0:31:37.000
<v Speaker 1>or a dwarf planet is technically an asteroid. There's some

0:31:37.040 --> 0:31:41.080
<v Speaker 1>fuzziness there because past Neptune there's a huge number of

0:31:41.120 --> 0:31:44.640
<v Speaker 1>these objects we called dwarf planets, which are like sort

0:31:44.680 --> 0:31:47.520
<v Speaker 1>of larger enough to be called a planet, maybe by

0:31:47.520 --> 0:31:51.000
<v Speaker 1>havn't cleared their own path right, like Pluto and Sharon,

0:31:51.160 --> 0:31:54.640
<v Speaker 1>for example. And so the distinction between dwarf planet and

0:31:54.640 --> 0:31:57.160
<v Speaker 1>asteroid out there and the edges of the Solar System

0:31:57.200 --> 0:31:58.120
<v Speaker 1>is pretty fuzzy.

0:31:58.280 --> 0:32:01.240
<v Speaker 4>You have to ask an astronomer Okay, So then the

0:32:01.320 --> 0:32:03.920
<v Speaker 4>question was are there comets in the astory belt? And

0:32:03.960 --> 0:32:05.959
<v Speaker 4>now how do you define what a comet is?

0:32:06.840 --> 0:32:10.400
<v Speaker 1>Yeah? So your comment earlier about asteroids that they have

0:32:10.480 --> 0:32:13.600
<v Speaker 1>to be solid was really on point because one of

0:32:13.640 --> 0:32:17.120
<v Speaker 1>the crucial ways we define a comet is very similar

0:32:17.160 --> 0:32:19.960
<v Speaker 1>to the way we define an asteroid. An asteroid is

0:32:20.000 --> 0:32:23.640
<v Speaker 1>a rocky object that orbits the sun. A comet is

0:32:23.680 --> 0:32:26.800
<v Speaker 1>an icy and dusty object that orbits the sun.

0:32:27.560 --> 0:32:27.640
<v Speaker 13>Icy.

0:32:27.760 --> 0:32:31.000
<v Speaker 4>So it's made out of ice. But isn't ice technically

0:32:31.120 --> 0:32:34.640
<v Speaker 4>a mineral, which means it's a rock? Right?

0:32:34.880 --> 0:32:37.520
<v Speaker 1>Yeah, there's a distinction here. Ice is not like a silicate, right,

0:32:37.840 --> 0:32:41.160
<v Speaker 1>It doesn't have the same chemical composition as these things

0:32:41.200 --> 0:32:41.920
<v Speaker 1>we call it rocks.

0:32:42.120 --> 0:32:46.000
<v Speaker 4>Excuse me, Daniel, excuse me. I believe. I believe that

0:32:46.440 --> 0:32:50.920
<v Speaker 4>the definition of a rock is like a composite of minerals, right,

0:32:51.320 --> 0:32:54.920
<v Speaker 4>and ice is a mineral. So wouldn't ice be a rock?

0:32:55.440 --> 0:32:57.040
<v Speaker 4>Or is this something that would be have to be

0:32:57.160 --> 0:33:00.440
<v Speaker 4>decided in a death match between geologists and astronomer.

0:33:00.240 --> 0:33:02.240
<v Speaker 1>Yeah, and I think some chemists need to be involved

0:33:02.280 --> 0:33:05.880
<v Speaker 1>in that conversation. But in terms of the Solar system,

0:33:06.040 --> 0:33:09.920
<v Speaker 1>we distinguish between ice and other kinds of rock or rocks,

0:33:09.960 --> 0:33:12.000
<v Speaker 1>depending on whether you're gonna call ice.

0:33:12.040 --> 0:33:14.280
<v Speaker 4>A rock and so ice. How do you define ice?

0:33:14.360 --> 0:33:16.000
<v Speaker 4>Does it need to be water or can it be

0:33:16.080 --> 0:33:16.800
<v Speaker 4>other liquids?

0:33:16.840 --> 0:33:20.200
<v Speaker 1>There's several categories there. First of all, water ice has

0:33:20.280 --> 0:33:22.600
<v Speaker 1>lots of different chemical forms, so it's not just the

0:33:22.680 --> 0:33:24.959
<v Speaker 1>kind of ice that we see on Earth. There's like

0:33:25.040 --> 0:33:27.360
<v Speaker 1>ice and ice three, and ice seven and ice nine,

0:33:27.880 --> 0:33:31.440
<v Speaker 1>all sorts of complicated water chemistry to give you solid

0:33:31.480 --> 0:33:33.400
<v Speaker 1>forms of ice that we don't often see on Earth

0:33:33.400 --> 0:33:36.080
<v Speaker 1>because it's a very different pressure environment out there in

0:33:36.120 --> 0:33:39.880
<v Speaker 1>the outer Solar System. But also you know, things like methane.

0:33:40.280 --> 0:33:42.720
<v Speaker 1>If that's frozen, they call that ice. A lot of

0:33:42.720 --> 0:33:44.280
<v Speaker 1>the ice that's out there is water ice, but there

0:33:44.280 --> 0:33:45.840
<v Speaker 1>are also other kinds of ices.

0:33:46.080 --> 0:33:51.160
<v Speaker 4>Gosh, I have so many netpicky questions, Daniel. I mean, like,

0:33:51.200 --> 0:33:53.840
<v Speaker 4>if you heat up a rock, it'll melt, so it's liquid.

0:33:53.960 --> 0:33:56.520
<v Speaker 4>So really a rock is just frozen liquid rock.

0:33:56.720 --> 0:33:59.760
<v Speaker 1>Yes, a rock is frozen liquid rock. But lots of

0:33:59.760 --> 0:34:01.400
<v Speaker 1>sot our frozen liquids.

0:34:01.480 --> 0:34:03.560
<v Speaker 4>Right, how do you define what an ice is?

0:34:03.800 --> 0:34:06.280
<v Speaker 1>There's an arbitrary dotted line, you know, it's just historical.

0:34:06.760 --> 0:34:09.600
<v Speaker 1>Some crystals we call ices. Some crystals we call rocks.

0:34:09.920 --> 0:34:13.000
<v Speaker 1>And that's, frankly, is my whole problem with chemistry. All

0:34:13.040 --> 0:34:15.759
<v Speaker 1>of chemistry is like this, just like draw dotted lines

0:34:15.800 --> 0:34:18.040
<v Speaker 1>between stuff because some dude one hundred and fifty years

0:34:18.080 --> 0:34:20.359
<v Speaker 1>ago thought that made sense. We're sticking to it.

0:34:20.760 --> 0:34:23.200
<v Speaker 4>Well, it sounds like it's not just chemistry, it's physics, astronomy.

0:34:23.440 --> 0:34:25.320
<v Speaker 4>Why are you tying chemist under the bus.

0:34:25.440 --> 0:34:28.480
<v Speaker 1>We're definitely guilty of that in physics and in astronomy,

0:34:28.520 --> 0:34:32.160
<v Speaker 1>and especially in this situation naming things in the solar system.

0:34:32.320 --> 0:34:34.360
<v Speaker 1>But and I'm really going to catch a lot of

0:34:34.360 --> 0:34:36.359
<v Speaker 1>flak from the chemists out there. I feel like all

0:34:36.400 --> 0:34:38.239
<v Speaker 1>of chemistry is just built on that. Like, if you

0:34:38.239 --> 0:34:40.560
<v Speaker 1>took that away from chemistry, what do you have left?

0:34:40.640 --> 0:34:40.879
<v Speaker 12>Man?

0:34:41.440 --> 0:34:42.719
<v Speaker 1>It's all just exceptions.

0:34:43.040 --> 0:34:46.719
<v Speaker 4>Oh man, he just lost is a bunch of chemists listeners?

0:34:47.080 --> 0:34:48.320
<v Speaker 1>No, man, they're all going to right to me, and

0:34:48.320 --> 0:34:50.799
<v Speaker 1>they're gonna listen carefully through all the next episodes to

0:34:50.800 --> 0:34:52.040
<v Speaker 1>see if I slight chemistry.

0:34:52.320 --> 0:34:55.319
<v Speaker 4>I see they're gonna hate listening. That's the kind of

0:34:55.360 --> 0:34:58.399
<v Speaker 4>fan that we want. Look, as long as they sit

0:34:58.440 --> 0:35:00.359
<v Speaker 4>through the ads, then we don't care or why.

0:35:00.280 --> 0:35:02.359
<v Speaker 1>They're Lovelessen or hate listen, we love you.

0:35:05.360 --> 0:35:07.440
<v Speaker 4>All right, So then what does that leaves about the

0:35:07.440 --> 0:35:08.480
<v Speaker 4>definition of a comet.

0:35:08.960 --> 0:35:12.640
<v Speaker 1>So, according to the arbitrary distinction between ices and rocks,

0:35:13.000 --> 0:35:16.319
<v Speaker 1>comets are made out of ice and asteroids are made

0:35:16.360 --> 0:35:19.440
<v Speaker 1>out of rocks. And one important difference is that if

0:35:19.520 --> 0:35:21.719
<v Speaker 1>you bring something made out of ice into the Inner

0:35:21.760 --> 0:35:25.000
<v Speaker 1>Solar System, it tends to vaporize, Like the Sun is

0:35:25.080 --> 0:35:28.319
<v Speaker 1>capable of turning those ices into vapor and it's not

0:35:28.400 --> 0:35:31.080
<v Speaker 1>capable of doing that with rock. So probably there's some

0:35:31.120 --> 0:35:33.800
<v Speaker 1>distinction there about like the melting point or the vapor

0:35:33.840 --> 0:35:35.200
<v Speaker 1>point of these substances.

0:35:35.840 --> 0:35:38.560
<v Speaker 4>Oh, I see, all right, So now we're getting somewhere.

0:35:38.560 --> 0:35:40.960
<v Speaker 4>It's the sort of scientific If it melts under the

0:35:41.040 --> 0:35:43.880
<v Speaker 4>light of the Sun, then you might call it a comet.

0:35:44.000 --> 0:35:45.839
<v Speaker 4>That's basically the only distinction that sea.

0:35:45.920 --> 0:35:48.120
<v Speaker 1>Yeah, And when you bring these things into the inner

0:35:48.200 --> 0:35:52.880
<v Speaker 1>Solar System, like comets traditionally originate in the Kuiper Belt

0:35:52.960 --> 0:35:55.200
<v Speaker 1>or in the Ort cloud, which you're kind of like

0:35:55.360 --> 0:35:57.759
<v Speaker 1>bands of rocks in the more distant parts of the

0:35:57.760 --> 0:36:01.279
<v Speaker 1>Solar System, much further out than the asteroid belt. When

0:36:01.280 --> 0:36:04.000
<v Speaker 1>you bring them into the inner Solar System, they develop

0:36:04.080 --> 0:36:07.399
<v Speaker 1>tails because the Sun is beginning to vaporize them, they

0:36:07.400 --> 0:36:09.560
<v Speaker 1>get a coma, they have like a little envelope of

0:36:09.600 --> 0:36:12.440
<v Speaker 1>gas around them, and then as they move in towards

0:36:12.440 --> 0:36:15.120
<v Speaker 1>the Solar System, they get tails. And so that's really

0:36:15.200 --> 0:36:19.080
<v Speaker 1>what distinguishes comets from asteroids. Asteroids are just rocks, and

0:36:19.120 --> 0:36:22.040
<v Speaker 1>comets have these little gas clouds and tails because they're

0:36:22.080 --> 0:36:22.480
<v Speaker 1>made out of.

0:36:22.520 --> 0:36:27.279
<v Speaker 4>Ices, all right, and they mostly hang out on the

0:36:27.280 --> 0:36:28.600
<v Speaker 4>outside of the Solar System.

0:36:28.440 --> 0:36:31.120
<v Speaker 1>Right, Yeah, they originate in the Kuiper Belt, which is

0:36:31.160 --> 0:36:35.919
<v Speaker 1>this big collection of rocks, billions and billions of snowballs

0:36:35.960 --> 0:36:38.520
<v Speaker 1>in the distant Solar System, and this is probably the

0:36:38.560 --> 0:36:41.200
<v Speaker 1>origin of short period comets, like you know, years up

0:36:41.200 --> 0:36:43.719
<v Speaker 1>to tens of years. And then we think there's a

0:36:43.760 --> 0:36:46.560
<v Speaker 1>collection of them also much much further out in the

0:36:46.719 --> 0:36:49.799
<v Speaker 1>Ort Cloud, which is like very far out there, much

0:36:49.840 --> 0:36:54.040
<v Speaker 1>further than Pluto. And it's also technically theoretical because we've

0:36:54.080 --> 0:36:57.240
<v Speaker 1>never actually seen the Ork Cloud. We've just like deduced

0:36:57.280 --> 0:37:02.160
<v Speaker 1>its existence from various gravitational calculations and models. And we

0:37:02.280 --> 0:37:05.120
<v Speaker 1>also think that it's the source of long period comets,

0:37:05.120 --> 0:37:08.000
<v Speaker 1>comets with periods you know, again longer than tens or

0:37:08.080 --> 0:37:10.719
<v Speaker 1>hundreds of years, and they could take a very long

0:37:10.760 --> 0:37:13.200
<v Speaker 1>time to fall into the inner Solar System, and out

0:37:13.200 --> 0:37:15.600
<v Speaker 1>there there could be trillions of these.

0:37:15.480 --> 0:37:18.480
<v Speaker 4>Snowballs, and that's in the or cloud. So what's the

0:37:18.560 --> 0:37:20.640
<v Speaker 4>Kuiper belt? Is it asteroids or comets?

0:37:20.920 --> 0:37:23.319
<v Speaker 1>The Kuiper Belt is snowballs, and when they fall into

0:37:23.320 --> 0:37:25.920
<v Speaker 1>the Inner Solar System you call them comets. I think

0:37:25.920 --> 0:37:27.800
<v Speaker 1>you still call them commets when they're in the Kuiper

0:37:27.800 --> 0:37:31.319
<v Speaker 1>Belt before they've fallen in, because technically they are icy

0:37:31.360 --> 0:37:34.160
<v Speaker 1>objects out in the Solar System orbiting the Sun.

0:37:34.200 --> 0:37:36.919
<v Speaker 4>Because they would melt if they got closer to the Sun.

0:37:37.080 --> 0:37:39.279
<v Speaker 4>But doesn't everything melt if you get close enough to

0:37:39.280 --> 0:37:39.520
<v Speaker 4>the Sun?

0:37:39.640 --> 0:37:42.440
<v Speaker 1>Yeah, exactly, And so this distinction between asteroids and comets

0:37:42.480 --> 0:37:44.920
<v Speaker 1>is also a little bit fuzzy. I found a comet

0:37:44.920 --> 0:37:48.200
<v Speaker 1>from an astronomer or the University of Arizona who said, quote,

0:37:48.280 --> 0:37:50.919
<v Speaker 1>everything is a comet. If you brought my couch close

0:37:51.040 --> 0:37:53.080
<v Speaker 1>enough to the Sun, it would start melting and have

0:37:53.160 --> 0:37:55.879
<v Speaker 1>a coma. So like it's just a question of how

0:37:55.880 --> 0:37:57.759
<v Speaker 1>close you get to the Sun. Because you bring an

0:37:57.840 --> 0:38:00.840
<v Speaker 1>asteroid close enough to the Sun, it's to get vaporized.

0:38:00.880 --> 0:38:02.520
<v Speaker 1>Even if it's like a hunk of iron.

0:38:02.920 --> 0:38:04.840
<v Speaker 4>What if it's a hunk of like diamond.

0:38:05.440 --> 0:38:07.800
<v Speaker 1>If you dropped a huge diamond into the sun, it

0:38:07.840 --> 0:38:09.319
<v Speaker 1>would definitely get vaporized.

0:38:09.880 --> 0:38:10.799
<v Speaker 4>Yeah, into the sun.

0:38:11.120 --> 0:38:12.880
<v Speaker 1>If you had a huge diamond and you dropped it

0:38:12.880 --> 0:38:15.040
<v Speaker 1>from the outer solar system and it fell in towards

0:38:15.080 --> 0:38:17.160
<v Speaker 1>the Sun at some point at which it would reach

0:38:17.200 --> 0:38:19.080
<v Speaker 1>its melting point, and you would melt.

0:38:18.840 --> 0:38:21.400
<v Speaker 4>That diamond and become a diamond commet.

0:38:22.680 --> 0:38:25.040
<v Speaker 1>A diamond commet with a cloud of carbon.

0:38:24.760 --> 0:38:27.160
<v Speaker 4>And leave a trail of sparkly melted diamonds.

0:38:28.160 --> 0:38:31.200
<v Speaker 1>Yeah. I think melted diamond is just carbon though, because

0:38:31.239 --> 0:38:34.160
<v Speaker 1>it's only diamond because of the arrangement of those carbon atoms,

0:38:34.400 --> 0:38:36.040
<v Speaker 1>and so once you melted it could it's the same

0:38:36.040 --> 0:38:37.600
<v Speaker 1>as like melted coal. I guess.

0:38:38.200 --> 0:38:40.800
<v Speaker 4>Oh man, now we're getting really confusing.

0:38:40.880 --> 0:38:43.240
<v Speaker 1>Turn chemistry is a mess.

0:38:43.400 --> 0:38:44.880
<v Speaker 4>Is melted chocolate just carbon?

0:38:44.920 --> 0:38:45.120
<v Speaker 12>Then?

0:38:45.560 --> 0:38:49.719
<v Speaker 4>Oh no, are just eating coal when I when I'm

0:38:49.800 --> 0:38:50.760
<v Speaker 4>drinking my hot cocoa.

0:38:52.840 --> 0:38:54.960
<v Speaker 1>That's why putting these names on things is such a mess,

0:38:54.960 --> 0:38:56.840
<v Speaker 1>and we should just use math or charades.

0:38:57.560 --> 0:39:01.759
<v Speaker 4>That's why would you just use charades or speed up

0:39:01.760 --> 0:39:03.879
<v Speaker 4>the telepathy idea?

0:39:03.960 --> 0:39:06.520
<v Speaker 1>And then to make things even more confusing, there's another

0:39:06.640 --> 0:39:10.399
<v Speaker 1>category of stuff that's sort of like a hybrid, these

0:39:10.400 --> 0:39:14.719
<v Speaker 1>things that are actually brilliantly named. They call them centaurs.

0:39:14.800 --> 0:39:17.680
<v Speaker 1>You know. Centaurs are like half horse, half human. These

0:39:17.719 --> 0:39:23.000
<v Speaker 1>things have characteristics of asteroids and characteristics of comets. So

0:39:23.040 --> 0:39:25.880
<v Speaker 1>they're sort of like a comet because they have long

0:39:25.960 --> 0:39:29.279
<v Speaker 1>elliptical orbits the way comets do, and some of them

0:39:29.320 --> 0:39:33.160
<v Speaker 1>have dust comas. But they're kind of like asteroids in

0:39:33.200 --> 0:39:36.640
<v Speaker 1>that they're really large and they're mostly metallic. But they're

0:39:36.680 --> 0:39:39.640
<v Speaker 1>not like asteroids because they leave the asteroid belts and

0:39:39.640 --> 0:39:42.680
<v Speaker 1>they sort of traverse the Solar system the way comets do.

0:39:43.640 --> 0:39:46.000
<v Speaker 1>So these centaurs are sort of like a weird thing

0:39:46.040 --> 0:39:49.479
<v Speaker 1>in the Solar system that blurs the line between asteroid and.

0:39:49.719 --> 0:39:53.120
<v Speaker 4>Comet, meaning like it's a mix of rocks and ice.

0:39:53.080 --> 0:39:55.760
<v Speaker 1>Yeah, exactly, And it sort of moves like a comet,

0:39:56.040 --> 0:39:58.279
<v Speaker 1>and it's the size of an asteroid. These things tend

0:39:58.280 --> 0:39:59.240
<v Speaker 1>to be typically bigger.

0:40:00.000 --> 0:40:02.000
<v Speaker 4>I mean, it moves like a common You never said

0:40:02.719 --> 0:40:04.480
<v Speaker 4>motion was part of the definition.

0:40:04.719 --> 0:40:07.400
<v Speaker 1>Yeah, it's not technically part of the definition, right, But

0:40:07.520 --> 0:40:10.279
<v Speaker 1>comets tend to have these longer elliptical orbits just because

0:40:10.320 --> 0:40:12.399
<v Speaker 1>of where they come from in the Solar System. They

0:40:12.400 --> 0:40:15.280
<v Speaker 1>come from further out, and so they have these longer

0:40:15.360 --> 0:40:18.240
<v Speaker 1>orbits that traverse the path of the giant planets, whereas

0:40:18.320 --> 0:40:21.280
<v Speaker 1>asteroids typically hanging out in the asteroid belt and sometimes

0:40:21.280 --> 0:40:24.360
<v Speaker 1>fall in and so they don't traverse the giant planets.

0:40:25.120 --> 0:40:27.560
<v Speaker 1>So if you have like an asteroid like rock that

0:40:27.719 --> 0:40:30.319
<v Speaker 1>also has a long elliptical orbit, you're like, hmm, it's

0:40:30.320 --> 0:40:33.160
<v Speaker 1>a little comedy. It's a little asteroidy. You know. It's

0:40:33.160 --> 0:40:35.880
<v Speaker 1>sort of like chocolate and peanut butter, which.

0:40:35.840 --> 0:40:38.200
<v Speaker 4>We all know. If you melt it just becomes carbon.

0:40:38.200 --> 0:40:40.160
<v Speaker 1>And if you squeeze it hard enough, it becomes a diamond.

0:40:41.120 --> 0:40:44.840
<v Speaker 4>Yeah, technically a chunky diamond or a smooth diamond.

0:40:44.960 --> 0:40:46.680
<v Speaker 1>Yeah, maybe a creamy diamond.

0:40:46.400 --> 0:40:47.680
<v Speaker 4>Yeah, or me a carrot diamond.

0:40:47.760 --> 0:40:49.320
<v Speaker 1>I like my diamonds nicely salted.

0:40:49.440 --> 0:40:52.439
<v Speaker 4>So these centers are pretty interesting. How big can they get?

0:40:52.520 --> 0:40:54.680
<v Speaker 1>Some of them are pretty big, Like the largest one

0:40:54.840 --> 0:40:59.359
<v Speaker 1>is two hundred and seventy kilometers across, and actually it's

0:40:59.360 --> 0:41:02.040
<v Speaker 1>so big that it has its own rings, like a

0:41:02.080 --> 0:41:05.680
<v Speaker 1>little group of dust and tiny rocks orbiting this centaur.

0:41:06.160 --> 0:41:07.239
<v Speaker 4>Well, and where is that one?

0:41:07.360 --> 0:41:09.960
<v Speaker 1>It orbits in the Solar system out there between Saturn

0:41:10.080 --> 0:41:13.719
<v Speaker 1>and Urinus. So it's a big blob out there, and

0:41:13.760 --> 0:41:16.439
<v Speaker 1>it's sort of weird to be that far out. Why

0:41:16.480 --> 0:41:18.200
<v Speaker 1>isn't it in the asteroid belts? Or if it's that

0:41:18.280 --> 0:41:20.240
<v Speaker 1>far out, why doesn't that have more ice?

0:41:20.760 --> 0:41:20.920
<v Speaker 5>You know?

0:41:21.040 --> 0:41:23.840
<v Speaker 1>You might ask also, well, why do all the objects

0:41:23.880 --> 0:41:26.000
<v Speaker 1>and what we call the asteroid belt, why are they

0:41:26.040 --> 0:41:29.080
<v Speaker 1>mostly rocks and metal and the stuff out there in

0:41:29.120 --> 0:41:30.800
<v Speaker 1>what we call the Kuyper belt in the or cloud,

0:41:31.040 --> 0:41:33.320
<v Speaker 1>why do they have more ices? And that's just distance

0:41:33.360 --> 0:41:35.759
<v Speaker 1>from the sun. If you're further from the Sun, then

0:41:35.800 --> 0:41:38.160
<v Speaker 1>the sun is not bright enough, not hot enough to

0:41:38.280 --> 0:41:40.799
<v Speaker 1>vaporize all that stuff, so you get these ices. And

0:41:40.800 --> 0:41:44.160
<v Speaker 1>that's why comets when they form out there, are icy

0:41:44.200 --> 0:41:46.480
<v Speaker 1>and asteroids are not. The way the Earth is not

0:41:46.680 --> 0:41:49.759
<v Speaker 1>mostly icy, right, And so it's weird to have an

0:41:49.840 --> 0:41:53.000
<v Speaker 1>object that's out there beyond the snow line that doesn't

0:41:53.040 --> 0:41:56.040
<v Speaker 1>have as much snow or ice as everything else.

0:41:57.400 --> 0:41:59.560
<v Speaker 4>And how do we know it's a centaur? Does it

0:41:59.600 --> 0:41:59.960
<v Speaker 4>have a take?

0:42:00.600 --> 0:42:02.279
<v Speaker 1>This one is big enough that it might have its

0:42:02.320 --> 0:42:05.640
<v Speaker 1>own like little atmosphere, right, things that are boiling off

0:42:05.640 --> 0:42:07.560
<v Speaker 1>of it, But we don't know the composition of it

0:42:07.640 --> 0:42:09.600
<v Speaker 1>that well, it's sort of far enough away that it's

0:42:09.880 --> 0:42:12.279
<v Speaker 1>difficult to study, but we do see that it has

0:42:12.280 --> 0:42:15.040
<v Speaker 1>its own ring systems, so we have some information about it.

0:42:15.520 --> 0:42:18.480
<v Speaker 1>But these things are really fascinating because they paint sort

0:42:18.480 --> 0:42:20.560
<v Speaker 1>of a picture of the history of the solar system.

0:42:20.800 --> 0:42:22.640
<v Speaker 1>A lot of this stuff is interesting in the context

0:42:22.640 --> 0:42:24.600
<v Speaker 1>of like, hey, how did we get here? How did

0:42:24.600 --> 0:42:26.920
<v Speaker 1>our solar system end up the way that it is.

0:42:27.360 --> 0:42:29.760
<v Speaker 1>All these things are clues that let us like back

0:42:29.800 --> 0:42:32.319
<v Speaker 1>out that story and figure out how it all got

0:42:32.360 --> 0:42:33.600
<v Speaker 1>arranged to be this way.

0:42:35.360 --> 0:42:37.400
<v Speaker 4>Sok Can we tell what it's made out of with

0:42:37.480 --> 0:42:38.839
<v Speaker 4>our telescopes.

0:42:38.320 --> 0:42:40.400
<v Speaker 1>We can tell a little bit because of the color,

0:42:40.800 --> 0:42:42.759
<v Speaker 1>Like some of these things are a little bluer and

0:42:42.800 --> 0:42:44.959
<v Speaker 1>some of these things are a little redder. That gives

0:42:45.040 --> 0:42:47.880
<v Speaker 1>us a clue as to what they are, because what

0:42:47.960 --> 0:42:50.239
<v Speaker 1>they are determines, you know, what they're reflecting and what

0:42:50.280 --> 0:42:53.799
<v Speaker 1>they're absorbing. So we have some clues about their chemical composition.

0:42:54.200 --> 0:42:56.160
<v Speaker 1>But that's also sort of a mystery. Like some of

0:42:56.200 --> 0:42:58.440
<v Speaker 1>these centaurs are bluer and some of these are redder.

0:42:58.719 --> 0:43:00.920
<v Speaker 1>Some of them look more like asteroids, of them look

0:43:01.000 --> 0:43:03.440
<v Speaker 1>less like asteroids. That's sort of one of the central

0:43:03.480 --> 0:43:06.560
<v Speaker 1>mysteries of centaurs. But none of these things have been

0:43:06.560 --> 0:43:09.719
<v Speaker 1>like photographed up close. A lot of Solar System objects

0:43:09.840 --> 0:43:12.960
<v Speaker 1>have been visited by probes, like we recently had up

0:43:13.040 --> 0:43:15.680
<v Speaker 1>close pictures of Pluto, which is awesome, and most of

0:43:15.719 --> 0:43:18.920
<v Speaker 1>the moons of Saturn and Jupiter have been visited, but

0:43:19.000 --> 0:43:22.320
<v Speaker 1>nobody's ever done a close flyby of a centaur to

0:43:22.320 --> 0:43:25.440
<v Speaker 1>take like crisp photos of its surface and see what

0:43:25.440 --> 0:43:27.440
<v Speaker 1>it's made out of and what that surface looks like.

0:43:27.880 --> 0:43:29.040
<v Speaker 1>It'd be really fascinating.

0:43:29.440 --> 0:43:31.040
<v Speaker 4>But wait, how do we know what they're made out of?

0:43:31.080 --> 0:43:33.480
<v Speaker 1>Ben We don't know for sure. It's just really guesses

0:43:33.520 --> 0:43:36.600
<v Speaker 1>based on the spectrometry looking at the wavelength of light

0:43:36.640 --> 0:43:39.160
<v Speaker 1>that bounces off of it. So we have ideas.

0:43:39.360 --> 0:43:40.920
<v Speaker 4>How do you assume that it has ion it?

0:43:41.000 --> 0:43:43.680
<v Speaker 1>Because they look different from the asteroids, right, They have

0:43:43.880 --> 0:43:47.839
<v Speaker 1>different reflections than asteroids do m All.

0:43:47.800 --> 0:43:49.760
<v Speaker 4>Right, Well, let's get to the question of the episode,

0:43:49.800 --> 0:43:53.120
<v Speaker 4>which is are there comments in the asteroid belt? So

0:43:53.200 --> 0:43:56.000
<v Speaker 4>let's tackle that. But first let's take another quick break.

0:44:00.080 --> 0:44:03.680
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<v Speaker 4>All right, we're talking about comments, asteroids, and centaurs and

0:47:29.280 --> 0:47:30.160
<v Speaker 4>also charades.

0:47:31.719 --> 0:47:34.440
<v Speaker 1>So in your house, who typically wins the games of charades?

0:47:34.640 --> 0:47:36.000
<v Speaker 4>We never play charades.

0:47:36.120 --> 0:47:38.600
<v Speaker 1>What you're such a big proponent on the podcast, but

0:47:38.640 --> 0:47:39.839
<v Speaker 1>you don't practice that at home.

0:47:40.360 --> 0:47:42.319
<v Speaker 4>That's what I'm trying to do, see, Daniel, is bring

0:47:42.320 --> 0:47:45.520
<v Speaker 4>more charates into everyone's homes. So we're tackling today the

0:47:45.600 --> 0:47:48.880
<v Speaker 4>question are there comments in the asteroid belt? Now, Daniel?

0:47:48.960 --> 0:47:50.120
<v Speaker 4>Is the answer yes or no?

0:47:50.600 --> 0:47:53.480
<v Speaker 1>The answer is that there's some weird stuff in the

0:47:53.520 --> 0:47:58.160
<v Speaker 1>asteroid belt that we don't understand. In nineteen ninety six,

0:47:58.320 --> 0:48:02.360
<v Speaker 1>people saw something any asteroid belt that had a coma

0:48:02.880 --> 0:48:05.400
<v Speaker 1>like it has this gas and envelope in it, so

0:48:05.440 --> 0:48:07.799
<v Speaker 1>it looks like it's melting in the presence of the sun.

0:48:08.080 --> 0:48:08.279
<v Speaker 3>Wait.

0:48:08.280 --> 0:48:09.960
<v Speaker 4>Wait, so that the tail of a comet, you call

0:48:10.000 --> 0:48:10.640
<v Speaker 4>it a coma.

0:48:10.840 --> 0:48:13.000
<v Speaker 1>The tail is when it's moving. A coma is like

0:48:13.040 --> 0:48:15.799
<v Speaker 1>the envelope that surrounds It's sort of like a little atmosphere.

0:48:15.880 --> 0:48:17.920
<v Speaker 1>But it's not really an atmosphere because it's not holding

0:48:17.920 --> 0:48:20.840
<v Speaker 1>onto it gravitationally. It's just sort of like off gasing.

0:48:21.239 --> 0:48:23.680
<v Speaker 1>It's like melting. It's the vapor that's coming off as

0:48:23.719 --> 0:48:24.759
<v Speaker 1>the sun is melting it.

0:48:24.920 --> 0:48:27.960
<v Speaker 4>That's the coma, like an aura or like a cloud

0:48:28.040 --> 0:48:29.120
<v Speaker 4>of a vapor around it.

0:48:29.200 --> 0:48:31.880
<v Speaker 1>Yeah, exactly. And then if it's in motion, it's going

0:48:31.960 --> 0:48:34.839
<v Speaker 1>to leave that behind because it's not gravitationally holding onto

0:48:34.840 --> 0:48:37.640
<v Speaker 1>it and generate a tail. So a coma and a

0:48:37.719 --> 0:48:41.680
<v Speaker 1>tail are characteristic signatures of a comet rather than an asteroid.

0:48:42.400 --> 0:48:45.520
<v Speaker 1>And in nineteen ninety six people were looking at stuff

0:48:45.520 --> 0:48:47.480
<v Speaker 1>in the asteroid belt and it's like, what's out there,

0:48:47.640 --> 0:48:49.960
<v Speaker 1>what's weird? And they found this one that had a

0:48:50.000 --> 0:48:52.960
<v Speaker 1>coma and a tail, And people were like, well, that's weird.

0:48:53.000 --> 0:48:56.040
<v Speaker 1>But you know, one example is never anything, because you

0:48:56.040 --> 0:48:59.800
<v Speaker 1>can always find one weird thing just necessarily tell you anything.

0:49:01.160 --> 0:49:03.520
<v Speaker 1>But then a few years later they did a systematic

0:49:03.560 --> 0:49:07.359
<v Speaker 1>study this Isaac Newton telescope in the Canary Islands. They

0:49:07.360 --> 0:49:11.440
<v Speaker 1>were watching five hundred and thirty four asteroids specifically looking

0:49:11.800 --> 0:49:14.040
<v Speaker 1>for like a gassy shell around them or whether they

0:49:14.040 --> 0:49:16.960
<v Speaker 1>had a tail, and they found like twenty more of

0:49:17.000 --> 0:49:21.480
<v Speaker 1>these things in the asteroid belt that have comas and tails, Well.

0:49:21.440 --> 0:49:23.560
<v Speaker 4>So does that mean their comments or centaurs.

0:49:23.680 --> 0:49:25.680
<v Speaker 1>That means we don't know what to name these things,

0:49:26.040 --> 0:49:29.600
<v Speaker 1>and maybe we're all wrong about these definitions. After all.

0:49:30.080 --> 0:49:32.319
<v Speaker 1>It means that we don't really understand like how they

0:49:32.360 --> 0:49:34.400
<v Speaker 1>got there, you know. I think question number one is

0:49:34.480 --> 0:49:37.839
<v Speaker 1>like why is there something in the asteroid belt that's

0:49:37.840 --> 0:49:40.560
<v Speaker 1>still melting? You put something there and it's melting, it's

0:49:40.560 --> 0:49:43.480
<v Speaker 1>gonna shrink, so it can't last for very long. But

0:49:43.520 --> 0:49:45.399
<v Speaker 1>we think a lot of these asteroids have been there

0:49:45.440 --> 0:49:49.000
<v Speaker 1>for like billions of years, and so how long have

0:49:49.080 --> 0:49:51.520
<v Speaker 1>these things been in the asteroid belt? And if it's

0:49:51.719 --> 0:49:54.080
<v Speaker 1>only and if it's a recent event, then where did

0:49:54.080 --> 0:49:56.879
<v Speaker 1>they come from? And if it's not a recent event,

0:49:56.920 --> 0:49:59.400
<v Speaker 1>then how they lasted so long? So it's weird to

0:49:59.400 --> 0:50:01.600
<v Speaker 1>see something that you know has got to be short lived.

0:50:02.400 --> 0:50:04.279
<v Speaker 1>So it's weird to see so many things that you

0:50:04.320 --> 0:50:06.360
<v Speaker 1>know have to be short lived, because there's got to

0:50:06.400 --> 0:50:07.640
<v Speaker 1>be some explanation there.

0:50:08.680 --> 0:50:11.920
<v Speaker 4>You're saying they saw a coma or a shell or

0:50:11.920 --> 0:50:14.239
<v Speaker 4>a cloud or a tail, because you can see it

0:50:14.239 --> 0:50:15.799
<v Speaker 4>with the telescope.

0:50:15.400 --> 0:50:17.240
<v Speaker 1>As it passes in front of the Sun. For example,

0:50:17.560 --> 0:50:20.480
<v Speaker 1>you could see the gas around it affecting the light

0:50:20.560 --> 0:50:22.759
<v Speaker 1>as it transits, or you can see the way it

0:50:22.800 --> 0:50:23.800
<v Speaker 1>reflects light differently.

0:50:24.040 --> 0:50:26.359
<v Speaker 4>These are pretty firmly in the asteroid belt or are

0:50:26.360 --> 0:50:28.919
<v Speaker 4>they maybe just cruising through the asteroid belt?

0:50:28.960 --> 0:50:30.920
<v Speaker 1>Oh yeah, great question. Now these are things that are

0:50:30.960 --> 0:50:32.759
<v Speaker 1>part of the asteroid belt, and as they watch them,

0:50:32.760 --> 0:50:35.200
<v Speaker 1>they have stable orbits that can make them be part

0:50:35.239 --> 0:50:37.640
<v Speaker 1>of the asteroid belt. They're not just like happened to

0:50:37.680 --> 0:50:40.040
<v Speaker 1>be comets that were captured on their way into the

0:50:40.080 --> 0:50:42.960
<v Speaker 1>inner Solar System. These things are not transients. They're there

0:50:42.960 --> 0:50:46.120
<v Speaker 1>in the asteroid belt basically to stay. But we don't

0:50:46.200 --> 0:50:49.120
<v Speaker 1>understand where they came from. And these are deep and

0:50:49.160 --> 0:50:52.640
<v Speaker 1>important questions because we want to understand, like where is

0:50:52.680 --> 0:50:55.000
<v Speaker 1>the water in the Solar System? How did it get

0:50:55.000 --> 0:50:58.160
<v Speaker 1>spread out the way that it did? For example, where

0:50:58.239 --> 0:51:01.200
<v Speaker 1>did Earth's water come from? We know that all the

0:51:01.280 --> 0:51:04.279
<v Speaker 1>ice and all the water that originally was involved in

0:51:04.360 --> 0:51:07.359
<v Speaker 1>the formation of our planet got boiled off by the

0:51:07.400 --> 0:51:10.400
<v Speaker 1>Sun in the early history of the Solar System, and

0:51:10.480 --> 0:51:12.759
<v Speaker 1>so it's still an open question of like where did

0:51:12.760 --> 0:51:14.520
<v Speaker 1>the water that's on the surface of the Earth now,

0:51:14.719 --> 0:51:17.359
<v Speaker 1>like where did our oceans come from? Did it come

0:51:17.440 --> 0:51:19.840
<v Speaker 1>from comets hitting the Earth? Did it come from the

0:51:19.840 --> 0:51:23.840
<v Speaker 1>water that's still trapped inside the Earth. These are important

0:51:23.880 --> 0:51:25.360
<v Speaker 1>questions and to answer them, we're going to have to

0:51:25.400 --> 0:51:27.520
<v Speaker 1>understand like where's the water now and what is it?

0:51:27.560 --> 0:51:30.200
<v Speaker 1>All of its history. It's a deep question about our

0:51:30.280 --> 0:51:33.040
<v Speaker 1>origins and the whole history of the Solar System. And

0:51:33.120 --> 0:51:34.960
<v Speaker 1>so whenever you see something weird.

0:51:34.800 --> 0:51:36.440
<v Speaker 4>Like wait, are you saying that maybe, like some of

0:51:36.440 --> 0:51:40.560
<v Speaker 4>these weird objects in the asteroid belt, they came from

0:51:40.719 --> 0:51:43.720
<v Speaker 4>the outer Solar System and then maybe they crashed into

0:51:44.200 --> 0:51:45.040
<v Speaker 4>the asteroid belt.

0:51:45.120 --> 0:51:47.080
<v Speaker 1>It could be absolutely it could be that they were

0:51:47.160 --> 0:51:49.920
<v Speaker 1>comets and they were coming into the asteroid belt and

0:51:49.960 --> 0:51:52.880
<v Speaker 1>they like interfered with something. And people think of the

0:51:52.880 --> 0:51:55.640
<v Speaker 1>asteroid belt the way you described like Star Wars earlier,

0:51:55.840 --> 0:51:58.400
<v Speaker 1>like oh it's heart you got to dodge the asteroids.

0:51:58.400 --> 0:52:01.680
<v Speaker 1>It's very dense. In reality, the asteroid belt is very dilute,

0:52:01.760 --> 0:52:03.799
<v Speaker 1>Like if you flew through the asteroid belt, it'd be

0:52:03.840 --> 0:52:06.640
<v Speaker 1>hard to hit an asteroid. So a random commet flying

0:52:06.640 --> 0:52:08.560
<v Speaker 1>through the asteroid belt is not gonna have a problem

0:52:08.560 --> 0:52:11.440
<v Speaker 1>making it through. But you know, maybe occasionally these things

0:52:11.760 --> 0:52:14.480
<v Speaker 1>do get disturbed, or they get deflected by Jupiter or

0:52:14.520 --> 0:52:18.080
<v Speaker 1>captured effectively somehow, And so it could be that these

0:52:18.080 --> 0:52:20.880
<v Speaker 1>are comets that got waylaid and ended up in the

0:52:20.920 --> 0:52:24.120
<v Speaker 1>asteroid belt. But then you'd need a continuous stream of

0:52:24.160 --> 0:52:26.719
<v Speaker 1>them to keep it populated because they're not gonna last

0:52:26.800 --> 0:52:28.640
<v Speaker 1>very long in the asteroid belt, like the Sun is.

0:52:28.640 --> 0:52:30.680
<v Speaker 4>Gonna fry them even with that far away.

0:52:31.040 --> 0:52:33.560
<v Speaker 1>Yeah, I mean, the fact that they have a gassy

0:52:33.560 --> 0:52:36.959
<v Speaker 1>shell means that they are actively outgassing because they can't

0:52:36.960 --> 0:52:40.279
<v Speaker 1>hold onto that gas. And if you're actively outgassing, you're

0:52:40.360 --> 0:52:43.600
<v Speaker 1>literally melting, you're shrinking. That's not gonna last very long.

0:52:43.800 --> 0:52:46.319
<v Speaker 1>They might have like a rocky core, and that might

0:52:46.360 --> 0:52:48.920
<v Speaker 1>be left over when the Sun is done frying all

0:52:48.960 --> 0:52:51.440
<v Speaker 1>of their ices, but they're definitely not gonna look like

0:52:51.520 --> 0:52:54.880
<v Speaker 1>this for that long. We're talking, you know, millions of years,

0:52:54.920 --> 0:52:57.239
<v Speaker 1>but in the history of the Solar System, that's just

0:52:57.239 --> 0:52:58.200
<v Speaker 1>a blink of an eye.

0:52:59.400 --> 0:53:01.120
<v Speaker 4>I wonder if it could be just like the Earth,

0:53:01.200 --> 0:53:04.040
<v Speaker 4>when the Earth got formed, they had water trapped inside

0:53:04.040 --> 0:53:06.840
<v Speaker 4>of it in the rock. Could these asteroids also have

0:53:06.920 --> 0:53:09.080
<v Speaker 4>water inside of them that's maybe sweating out.

0:53:09.200 --> 0:53:11.839
<v Speaker 1>They certainly might have water inside of them the way

0:53:11.880 --> 0:53:13.760
<v Speaker 1>the Earth does. And you know, if you think about

0:53:13.760 --> 0:53:16.200
<v Speaker 1>water inside the Earth, it's not like there's literally an

0:53:16.200 --> 0:53:18.960
<v Speaker 1>ocean you can go swimming in. It's like the chemical

0:53:18.960 --> 0:53:22.560
<v Speaker 1>composition of the rock includes a lot of water. And

0:53:22.640 --> 0:53:25.120
<v Speaker 1>so in a similar way, you might have water infused

0:53:25.160 --> 0:53:27.000
<v Speaker 1>into the metals and the rocks at the heart of

0:53:27.040 --> 0:53:29.880
<v Speaker 1>these asteroids. But any water ice that the sun is

0:53:29.960 --> 0:53:32.520
<v Speaker 1>capable of frying off got fried off a long time ago,

0:53:32.600 --> 0:53:35.520
<v Speaker 1>because these asteroids have been there for billions of years,

0:53:36.400 --> 0:53:38.279
<v Speaker 1>and so these guys would have to be new, right,

0:53:38.320 --> 0:53:41.160
<v Speaker 1>These new, weird things they spotted in the asteroid belt

0:53:41.440 --> 0:53:44.240
<v Speaker 1>should have arrived fairly recently, if that makes any.

0:53:44.080 --> 0:53:46.719
<v Speaker 4>Sense, all right, Well, so I guess the answer is,

0:53:47.280 --> 0:53:50.279
<v Speaker 4>maybe are there comets in the asteroid There could be.

0:53:50.360 --> 0:53:53.680
<v Speaker 4>There are definitely things that are comedy, right, or that

0:53:53.760 --> 0:53:54.719
<v Speaker 4>have ice in them.

0:53:54.840 --> 0:53:57.399
<v Speaker 1>There's definitely something in the asteroid belt that has ice

0:53:57.480 --> 0:54:00.080
<v Speaker 1>because it's melting. We don't understand what they are or

0:54:00.080 --> 0:54:02.280
<v Speaker 1>where they came from, or what it means about where

0:54:02.320 --> 0:54:03.719
<v Speaker 1>our drinking water came from.

0:54:03.960 --> 0:54:06.800
<v Speaker 4>Or would you say maybe the answer is that some

0:54:06.920 --> 0:54:10.320
<v Speaker 4>of the things in the asteroid belt are comments or

0:54:10.360 --> 0:54:12.240
<v Speaker 4>could be classified as sort of comments.

0:54:12.320 --> 0:54:14.680
<v Speaker 1>Yeah, by our definition, where commets are things that have

0:54:14.760 --> 0:54:17.120
<v Speaker 1>ice in them, they're icy and dusty, then yeah, there

0:54:17.120 --> 0:54:19.959
<v Speaker 1>are definitely some icy, dusty things in the asteroid belt.

0:54:20.120 --> 0:54:22.800
<v Speaker 1>The asteroid belt is not just asteroids anymore.

0:54:23.000 --> 0:54:24.680
<v Speaker 4>Or I guess if you go by your definition of

0:54:24.719 --> 0:54:28.280
<v Speaker 4>a comet, then everything is a comet.

0:54:28.719 --> 0:54:31.600
<v Speaker 1>That's right, You're a comet. Right, we tossed you into

0:54:31.640 --> 0:54:33.719
<v Speaker 1>the sun, you would melt and vaporize as well.

0:54:33.800 --> 0:54:36.600
<v Speaker 4>So yeah, yeah, yeah, of course i'd be you know,

0:54:36.640 --> 0:54:40.440
<v Speaker 4>trying to communicate with charades all the way down hoping

0:54:40.480 --> 0:54:41.839
<v Speaker 4>someone picks me up.

0:54:43.440 --> 0:54:45.000
<v Speaker 1>Good luck with that, all right.

0:54:45.080 --> 0:54:50.000
<v Speaker 4>Well, another interesting exploration into our solar system. It's history

0:54:50.160 --> 0:54:52.920
<v Speaker 4>and the mysteries that are still out there waiting to

0:54:52.960 --> 0:54:53.680
<v Speaker 4>be discovered.

0:54:53.760 --> 0:54:56.120
<v Speaker 1>There's so many missing chapters to the history of our

0:54:56.120 --> 0:54:58.920
<v Speaker 1>solar system, so many things about our own backyard we

0:54:59.000 --> 0:55:02.200
<v Speaker 1>still don't understand. And every time we look more carefully

0:55:02.280 --> 0:55:04.960
<v Speaker 1>the things we thought we understood, we find weird things

0:55:05.000 --> 0:55:07.840
<v Speaker 1>that defy our explanation, that tell us that it's a

0:55:07.840 --> 0:55:09.840
<v Speaker 1>lot more to this story to be revealed.

0:55:10.239 --> 0:55:14.800
<v Speaker 4>Yeah, to be revealed by astronomers or physicists or both,

0:55:15.040 --> 0:55:17.440
<v Speaker 4>or perhaps chemists.

0:55:18.440 --> 0:55:19.520
<v Speaker 1>We're all just people.

0:55:19.719 --> 0:55:20.960
<v Speaker 4>No, we're all just comments.

0:55:21.239 --> 0:55:22.960
<v Speaker 1>That's right, everybody's a comment.

0:55:23.239 --> 0:55:26.839
<v Speaker 4>Yeah, we all have tales in komas. All right. Well,

0:55:26.840 --> 0:55:29.959
<v Speaker 4>we hope you enjoyed that. Thanks for joining us, See

0:55:29.960 --> 0:55:30.520
<v Speaker 4>you next time.

0:55:35.160 --> 0:55:38.040
<v Speaker 1>For more science and curiosity, come find us on social

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<v Speaker 1>media where we answer questions and post videos. We're on Twitter, Discord, Insta,

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<v Speaker 1>and now TikTok. Thanks for listening, and remember that Daniel

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<v Speaker 1>and Jorge Explain the Universe is a production of iHeartRadio.

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<v Speaker 1>For more podcasts from iHeart Radio, visit the iHeartRadio app,

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