WEBVTT - How do planets get rings?

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<v Speaker 1>Pee Katie, help me out with some research for an

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<v Speaker 1>upcoming episode. Alright, as long as you don't put me

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<v Speaker 1>in that collider of yours. Not this time, but you know,

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<v Speaker 1>in general, no promises, so just make sure you always

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<v Speaker 1>read the waiver very carefully. All right, I'll wear a helmet.

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<v Speaker 1>So what are we researching? Well, I'm trying to understand rings,

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<v Speaker 1>all right, and how can I help? Well, you got

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<v Speaker 1>engaged and married recently, didn't you. Yeah, during the pandemic.

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<v Speaker 1>I had a zoom wedding. It was It was really fun.

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<v Speaker 1>And did you get a real ring or a digital

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<v Speaker 1>zoom ring? I got a real ring, not just an

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<v Speaker 1>n f T pointing tour ring. Yes, I have a

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<v Speaker 1>real ring. And tell us a little bit about it.

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<v Speaker 1>Is it made out of icy particles or mostly dust

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<v Speaker 1>and rocks. It was actually grown in a lab lab

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<v Speaker 1>grown diamonds, which is pretty neat to me. Well, I

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<v Speaker 1>wonder if castor and planetary rings have anything in common. Yeah,

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<v Speaker 1>I wonder the same thing. You know. Actually, my husband

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<v Speaker 1>later told me that he had the choice to get

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<v Speaker 1>like a ring made out of a meteorite, So sometimes

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<v Speaker 1>they do converge. While it'd be awesome a little bit

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<v Speaker 1>of space on your finger. Well, we will have to

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<v Speaker 1>invite Saturn on the podcast to ask how it got

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<v Speaker 1>its rings and when it's fiance proposed to it. Saturn's

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<v Speaker 1>got the best bling in the Solar system. Hi, I'm Daniel.

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<v Speaker 1>I'm a physicist at UC Irvine and I do research

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<v Speaker 1>at the Large Hadron Collider. I am Katie Golden. I

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<v Speaker 1>host Creature Feature, a biology podcast, So I'm not actually

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<v Speaker 1>a physicist, but I have used a hula hoop before,

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<v Speaker 1>so I feel fairly confident I can talk about Saturn's

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<v Speaker 1>rings today. Oh. I think that makes you an engineer,

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<v Speaker 1>doesn't it. That's right, Just get me some tape and

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<v Speaker 1>a few paper clips, and boom, I'm an engineer. Well,

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<v Speaker 1>I actually don't wear a whole lot of rings. I

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<v Speaker 1>just have this one wedding ring, which my wife and

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<v Speaker 1>I picked up two days before our wedding on the

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<v Speaker 1>streets of Berkeley for about five bucks. And I think

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<v Speaker 1>at the time we were like, oh, this will work temporarily,

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<v Speaker 1>and here we are twenty years later, I'm still wearing

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<v Speaker 1>the same silver ring. No, that's so sweet. I love

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<v Speaker 1>that story. Yeah, it's a nice memory. It helps me

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<v Speaker 1>understand where I came from. And you know, in the

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<v Speaker 1>same way, we can look up at the night sky

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<v Speaker 1>and study the planets and use their rings to try

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<v Speaker 1>to get an idea of like where they came from,

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<v Speaker 1>what is the history of this planet? How did it

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<v Speaker 1>get that ring? Who gave it to it? And you know,

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<v Speaker 1>what is that wedding going to look like? So you're

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<v Speaker 1>saying because my ring was made in a lab, that

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<v Speaker 1>I two was made in a lab. Maybe your love

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<v Speaker 1>was grown in the lab, you know, which doesn't make

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<v Speaker 1>it any less authentic. I'm a big fan of labs

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<v Speaker 1>and research. It's very romantic test tube romance and welcome

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<v Speaker 1>to the podcast. Daniel and Jorge explain the universe in

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<v Speaker 1>which we try to grow your understanding of the nature

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<v Speaker 1>of this universe that we find ourselves and we cast

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<v Speaker 1>our minds out into the deepest darkness of space and

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<v Speaker 1>try to ring out understanding of everything that's out there

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<v Speaker 1>in the universe, and we zoom on into the tiniest

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<v Speaker 1>little things between our toes and under our fingernails, because

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<v Speaker 1>we want to understand the fundamental nature of the universe,

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<v Speaker 1>the nature of space and time itself, and matter and

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<v Speaker 1>energy and all those tiny little bits which, in their

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<v Speaker 1>two ing and frowing, come together to make the universe

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<v Speaker 1>that we know and love. My friend and co host

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<v Speaker 1>Jorge can't be with us today he is on vacation,

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<v Speaker 1>but we are very pleased to have the be Ringed,

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<v Speaker 1>be Jeweled, be Blinged Kiti two join this today. Well,

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<v Speaker 1>thank you for ringing me up for this episode. Yes,

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<v Speaker 1>I'm very excited. I love science, but that doesn't mean

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<v Speaker 1>I can't appreciate some good old fashioned cosmic jewelry. Well,

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<v Speaker 1>one thing I love about jewelry is that it really

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<v Speaker 1>does tell a story. You know, you talk to somebody

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<v Speaker 1>and you see them with ear rings or with a necklace,

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<v Speaker 1>you know that has a history. You know, maybe somebody

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<v Speaker 1>bought for them, or they got it for some big event,

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<v Speaker 1>or maybe they inherited it from their family, and it

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<v Speaker 1>tells like an even deeper story about where they came

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<v Speaker 1>from and their family history. So it's like everybody who's

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<v Speaker 1>wearing jewelry is walking around telling little stories about themselves. Yeah,

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<v Speaker 1>I love that. Or it bears an ancient curse? Are

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<v Speaker 1>we going to take a deep dark turn on this podcast?

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<v Speaker 1>I don't know. It is Saturn cursed? Is that where

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<v Speaker 1>we're going to discover maybe Aliens visited the Solar System

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<v Speaker 1>and had a war with the Octopi living under the

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<v Speaker 1>oceans of Insulatus, and the rings are just the left

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<v Speaker 1>over remnants that interstellar conflict. That's very spooky, and I

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<v Speaker 1>would love that story for a ring that I had,

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<v Speaker 1>that it was made by some kind of intergalactic war.

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<v Speaker 1>I think it is one of the things about the

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<v Speaker 1>Solar System that really adds a bit of magic to it,

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<v Speaker 1>adds a bit of artistry to it, because of course

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<v Speaker 1>I think all the planets are lovely, but they're all orbs,

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<v Speaker 1>you know, they're they're all these roughly of course, not

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<v Speaker 1>exact precise spears, but you know, roughly spherical. But then

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<v Speaker 1>you have these rings. And it always when I see

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<v Speaker 1>Saturn that gives me a feeling of awe about the

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<v Speaker 1>mystery and artistry of space that I don't necessarily get

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<v Speaker 1>with other planets, absolutely because it's so easy to grab onto,

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<v Speaker 1>you know, it's so visible out there. And it must

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<v Speaker 1>have been an amazing moment in sixteen ten when Galileo

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<v Speaker 1>looked through his telescope and saw the rings of Saturn,

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<v Speaker 1>and how shocking to discover that planets can have these

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<v Speaker 1>incredible dis you know, these things are like ten times

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<v Speaker 1>the size of Saturn. We'll talk later about how Saturday

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<v Speaker 1>might have rings that go out like two hundred times

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<v Speaker 1>the size of its radius. It's an incredible thing. Like

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<v Speaker 1>I have this little tiny ring on my finger. Imagine

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<v Speaker 1>if I was wearing a ring that was like two

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<v Speaker 1>hundred times the size of me. You know, some might

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<v Speaker 1>say that's a little overstated. It would be a statement piece,

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<v Speaker 1>for sure. You know. I was actually just in the

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<v Speaker 1>Galileo Museum in Florence, And when you think of Galileo

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<v Speaker 1>with his telescope, he's often depicted with this small, you know,

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<v Speaker 1>telescope he can hold in his hands. But you look

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<v Speaker 1>at the actual telescopes he used to observe Saturn and

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<v Speaker 1>they were huge. Yeah, he wasn't the inventor of the telescope,

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<v Speaker 1>but he was the first one to really perfect it

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<v Speaker 1>and then to turn it up on the skies, and

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<v Speaker 1>so he got like the biggest first scoop of all

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<v Speaker 1>these discoveries. You know, he saw the moons of Jupiter,

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<v Speaker 1>he saw the rings of Saturn. He's on mountains on

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<v Speaker 1>the Moon on a moment or like really look out

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<v Speaker 1>into the universe. And I think that one of the

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<v Speaker 1>most interesting things for me about it is that they

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<v Speaker 1>do reve yield the history of the Solar System. You know,

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<v Speaker 1>we look out unto the night sky and we want

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<v Speaker 1>to understand not just what's out there, but why it's

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<v Speaker 1>out there and why it looks the way that it does.

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<v Speaker 1>And so anything that's weird or strange or unusual that's

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<v Speaker 1>not just like a ball floating in the sky, Let's

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<v Speaker 1>just ask the question, how did that get there? How

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<v Speaker 1>long can that live? What does that tell us about

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<v Speaker 1>the history of the Solar System? Have those rings just

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<v Speaker 1>been there for the last million years? Have they been

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<v Speaker 1>there since the beginning of the Solar System? Why do

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<v Speaker 1>Saturn have rings and not other planets? Or do they right?

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<v Speaker 1>There's just so many immediate questions that you can ask

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<v Speaker 1>when you see these rings, and then those questions open

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<v Speaker 1>the door to try to understand the formation of the

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<v Speaker 1>Solar System. The other aspect, which is super fascinating for me,

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<v Speaker 1>is just thinking about what physics can do. You know,

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<v Speaker 1>you throw a whole bunch of stuff out into space

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<v Speaker 1>and it forms stars and it forms planets, But not

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<v Speaker 1>just that right, it can also do these other incredible things.

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<v Speaker 1>And it's all these fascinating little wrinkles, these little bits

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<v Speaker 1>of bling that really show us what gravity is capable

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<v Speaker 1>of and the interplay between gravity and all the other forces. So,

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<v Speaker 1>as we'll see on today's episode, these rings will teach

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<v Speaker 1>us a lot about the nature of the Solar System

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<v Speaker 1>and the universe that we live in. And so on

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<v Speaker 1>today's episode we'll be tackling exactly that question. How do

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<v Speaker 1>planets get rings? Okay, I'm gonna stop you right there,

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<v Speaker 1>because I think I have the answer. It is aliens,

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<v Speaker 1>giant aliens doing ring toss with our planets, or maybe

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<v Speaker 1>it's hula hoops from a leftover enormous alien birthday party.

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<v Speaker 1>We're basically their garbage bin. But it's an interesting question

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<v Speaker 1>not just why are there rings, but how do planets

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<v Speaker 1>get rings? Where do they come from? Why do some

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<v Speaker 1>planets have rings and others don't. Why do some planets

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<v Speaker 1>have more moons and fewer rings. What is the connection

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<v Speaker 1>between rings and moons? Can moons have rings? Can rings

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<v Speaker 1>exist on planets in other Solar systems? Is our Solar

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<v Speaker 1>System weird for having this incredible planet with these huge rings,

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<v Speaker 1>or are we weird for not having rings around every

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<v Speaker 1>single planet? These are the kinds of questions we can

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<v Speaker 1>now ask about our solar system because we have looked

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<v Speaker 1>out through our telescopes into even other solar systems around

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<v Speaker 1>other stars to try to get an answer to the

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<v Speaker 1>question of is our solar system strange or is our

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<v Speaker 1>solar system totally vanilla and typical. I find that an

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<v Speaker 1>interesting way to describe if our solar system is similar

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<v Speaker 1>to other solar systems, which is boring and vanilla. Well,

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<v Speaker 1>it's a deep question, right, like are we typical? Are

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<v Speaker 1>we boring? If alien scientists are studying the whole galaxy,

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<v Speaker 1>would they find us an interesting case study or would

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<v Speaker 1>they be like, oh, yeah, another one, just like all

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<v Speaker 1>the other sixty five million systems that I've already studied. Right,

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<v Speaker 1>we'd like to think that we are special in some sense.

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<v Speaker 1>We'd like to imagine that we are at the center

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<v Speaker 1>of the universe. We are unusual, we are sparkling, we

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<v Speaker 1>are exceptional. On the other hand, I'd like to believe

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<v Speaker 1>that we are vanilla, that we are boring, because that

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<v Speaker 1>means it's probably more of us, right, That means it's

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<v Speaker 1>probably life everywhere. One of my favorite things about this

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<v Speaker 1>kind of question, is our solar system typical or not?

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<v Speaker 1>Is that the answer is fascinating either way. Either we're

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<v Speaker 1>incredibly unusual and then we get to ask why, or

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<v Speaker 1>we're not, in which case we got lots of neighbors. Yeah,

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<v Speaker 1>so you would favor us being basic solar system with

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<v Speaker 1>our ugg boots and our Saturn's rings. That is kind

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<v Speaker 1>of an interesting personality quick personality tests, like would you

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<v Speaker 1>prefer our solar system to be unique and special in

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<v Speaker 1>us to be the only planet with life or would

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<v Speaker 1>you prefer us to be run of the mill lots

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<v Speaker 1>of solar systems like ours out there and not feel

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<v Speaker 1>so alone. I agree with you. I hope we're basic

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<v Speaker 1>so that we've got some friends out there. Exactly, We

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<v Speaker 1>can't answer that question directly today because our telescopes are

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<v Speaker 1>not powerful enough to look through the atmospheres of exo planets.

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<v Speaker 1>But we can look in our own backyard and try

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<v Speaker 1>to understand how our solar system formed and if there's

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<v Speaker 1>anything in it that we cannot explained. And it's an

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<v Speaker 1>incredible piece of science to look around you and understand

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<v Speaker 1>how we came together to build a model for the

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<v Speaker 1>processes that could have formed such incredible structures, and to

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<v Speaker 1>think about how long they might have taken. You know,

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<v Speaker 1>we've done something similar here on Earth by looking under

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<v Speaker 1>our feet and asking questions like do we understand how

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<v Speaker 1>the Earth formed? And how the mountains have formed? And

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<v Speaker 1>all the ridges that we see in the layers of rock,

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<v Speaker 1>and those things are clues, the clues that led us

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<v Speaker 1>to understand something really shocking, that the Earth is billions

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<v Speaker 1>of years old, not thousands of years old. Right. We

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<v Speaker 1>have the evidence all around us to reveal the story

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<v Speaker 1>of the formation of the Solar System, but not just

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<v Speaker 1>here on Earth, out there in space, and one of

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<v Speaker 1>the funnest bits is to look at the rings around

0:11:45.360 --> 0:11:48.120
<v Speaker 1>those planets. So that's what we're focusing on today. And

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<v Speaker 1>I was curious whether people understood rings, whether rings were

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<v Speaker 1>still a big source of mystery, or people thought they

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<v Speaker 1>pretty much understood where they came from. So I went

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<v Speaker 1>out there to our cadre of Internet volunteers, who are

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<v Speaker 1>my random questions without a chance to prepare, which gives

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<v Speaker 1>us a sense for what people know, what they think about,

0:12:05.240 --> 0:12:07.440
<v Speaker 1>and what they want to hear about. If you'd like

0:12:07.520 --> 0:12:10.520
<v Speaker 1>to participate for future episodes. Please don't be shy, just

0:12:10.640 --> 0:12:14.120
<v Speaker 1>write to me two questions at Daniel and Jorge dot com.

0:12:14.160 --> 0:12:16.400
<v Speaker 1>Before you hear these answers, think to yourself, do you

0:12:16.520 --> 0:12:20.000
<v Speaker 1>have a good idea of where rings come from on planets?

0:12:20.440 --> 0:12:23.240
<v Speaker 1>Here's what our listeners had to say, UM, and I'm

0:12:23.240 --> 0:12:26.559
<v Speaker 1>pretty sure that I learned about this that UM like

0:12:26.640 --> 0:12:33.480
<v Speaker 1>it's asteroids colliding near the planet itself and the remnants

0:12:33.559 --> 0:12:37.520
<v Speaker 1>of those asteroids going into orbit and creating a sort

0:12:37.520 --> 0:12:41.160
<v Speaker 1>of disc. I think the two classical ways are by

0:12:41.200 --> 0:12:44.520
<v Speaker 1>planets capturing space debris um that's just floating through the

0:12:44.520 --> 0:12:48.320
<v Speaker 1>Solar System, or by recapturing debris caused by an impact.

0:12:48.720 --> 0:12:52.480
<v Speaker 1>But I've also heard of a moon orbiting Saturn. I

0:12:52.480 --> 0:12:55.320
<v Speaker 1>believe that has a geyser and when the guys are

0:12:55.480 --> 0:12:59.400
<v Speaker 1>spits out water um it forms into ice crystals, and

0:12:59.440 --> 0:13:02.880
<v Speaker 1>then that joins the rings of Saturn. So maybe that's

0:13:02.880 --> 0:13:09.559
<v Speaker 1>another option. Well, the rings are kind of like small satellites,

0:13:09.600 --> 0:13:12.040
<v Speaker 1>I would say, like small moons, Like we have the

0:13:12.080 --> 0:13:15.960
<v Speaker 1>most most really tiny moons that get around the planet.

0:13:16.440 --> 0:13:21.959
<v Speaker 1>Each planet has its own way of doing the rings. Well,

0:13:22.000 --> 0:13:24.360
<v Speaker 1>I wanted to say that planets can get rings if

0:13:24.400 --> 0:13:27.640
<v Speaker 1>they collide with big rocky bodies, but I don't know

0:13:27.679 --> 0:13:31.160
<v Speaker 1>how that would work with like gas giants and how

0:13:31.200 --> 0:13:33.560
<v Speaker 1>they got their rings. So I'm going to guess that

0:13:33.640 --> 0:13:37.280
<v Speaker 1>it's just stuff that is left over um from when

0:13:37.280 --> 0:13:39.920
<v Speaker 1>the planet was formed, and it was just stuff that

0:13:39.960 --> 0:13:41.720
<v Speaker 1>was so far away when it was being formed that

0:13:41.720 --> 0:13:43.599
<v Speaker 1>it didn't become part of the planet, but it was

0:13:43.600 --> 0:13:45.720
<v Speaker 1>still close enough to be influenced by the gravity of it.

0:13:45.840 --> 0:13:50.880
<v Speaker 1>I'm almost certain it's got to do with the acreation

0:13:51.960 --> 0:13:57.680
<v Speaker 1>process of when a planets formed and the attraction of

0:13:57.760 --> 0:14:02.840
<v Speaker 1>the stuff towards the planet. Apart from that, I'm not

0:14:02.880 --> 0:14:07.080
<v Speaker 1>really sure actually, because I think planets form when like

0:14:07.120 --> 0:14:11.200
<v Speaker 1>a heavy metal gets caught in orbit around the star,

0:14:11.440 --> 0:14:14.160
<v Speaker 1>so I think something similar happens around the planet. Debris

0:14:14.559 --> 0:14:18.800
<v Speaker 1>and maybe rocks or particles of ice or something um

0:14:19.040 --> 0:14:22.720
<v Speaker 1>gather around a planet in much the same way that

0:14:22.760 --> 0:14:28.360
<v Speaker 1>planets gather around stars. Does all seem like really intelligent answers,

0:14:28.480 --> 0:14:31.400
<v Speaker 1>but I still kind of like my giant alien ring

0:14:31.480 --> 0:14:35.280
<v Speaker 1>toss theory. We'll put it on the list as the

0:14:35.400 --> 0:14:37.520
<v Speaker 1>dark horse theory that might storm out at the end

0:14:37.560 --> 0:14:39.960
<v Speaker 1>if we can't explain it with any of the other theories.

0:14:40.200 --> 0:14:43.000
<v Speaker 1>So it seems like there are so many options for

0:14:43.120 --> 0:14:46.120
<v Speaker 1>what these rings could be made of. How on Earth

0:14:46.160 --> 0:14:48.520
<v Speaker 1>are we, or I should say, how in our Solar

0:14:48.560 --> 0:14:50.680
<v Speaker 1>system are we going to be able to figure out

0:14:50.800 --> 0:14:53.440
<v Speaker 1>what exactly they're made of? If there are so many

0:14:53.560 --> 0:14:56.600
<v Speaker 1>different theories, so many different options for what they could

0:14:56.640 --> 0:14:58.840
<v Speaker 1>be made of. Yeah, it's a great question. I listen

0:14:58.880 --> 0:15:01.120
<v Speaker 1>to these answers and seems to me like they form

0:15:01.200 --> 0:15:05.080
<v Speaker 1>in roughly two categories. There are some folks that say

0:15:05.120 --> 0:15:08.040
<v Speaker 1>that it's basically debris from other stuff that broke up,

0:15:08.160 --> 0:15:11.360
<v Speaker 1>like maybe you had comments or moons that smashed new

0:15:11.360 --> 0:15:14.160
<v Speaker 1>each other and basically just made a big mess, you know.

0:15:14.480 --> 0:15:16.320
<v Speaker 1>But then you have to wonder, like why don't those

0:15:16.360 --> 0:15:19.240
<v Speaker 1>things gather together to make a new moon or to

0:15:19.280 --> 0:15:22.040
<v Speaker 1>make a new comment or something. And the other category

0:15:22.240 --> 0:15:24.560
<v Speaker 1>is like, maybe it's just left over from when the

0:15:24.600 --> 0:15:27.360
<v Speaker 1>planet was formed, the same stuff that formed the planet,

0:15:27.360 --> 0:15:29.240
<v Speaker 1>but some of it didn't get into the planet. So

0:15:29.280 --> 0:15:31.960
<v Speaker 1>it seems like those are two different categories of ideas,

0:15:32.040 --> 0:15:34.520
<v Speaker 1>And you ask a great question, how could we possibly

0:15:34.640 --> 0:15:37.520
<v Speaker 1>ever figure this out? How could we know what the

0:15:37.640 --> 0:15:40.600
<v Speaker 1>history is of the Solar System? And the answer is that.

0:15:40.640 --> 0:15:42.600
<v Speaker 1>Of course, we can't just like watch a video of

0:15:42.640 --> 0:15:45.000
<v Speaker 1>its formation, though we'd love to, but we can just

0:15:45.040 --> 0:15:47.560
<v Speaker 1>look around us for clues. We can try to build

0:15:47.600 --> 0:15:50.640
<v Speaker 1>up models for how rings might form, and then compare

0:15:50.720 --> 0:15:53.520
<v Speaker 1>the details of those models to what we see. So

0:15:53.600 --> 0:15:55.600
<v Speaker 1>the short answer is we need more money and more

0:15:55.680 --> 0:15:58.960
<v Speaker 1>data to measure these rings, to look closely at them,

0:15:59.080 --> 0:16:01.200
<v Speaker 1>to see what they are made out of, how much

0:16:01.280 --> 0:16:04.560
<v Speaker 1>mass they have, what their distribution is. The more detail

0:16:04.600 --> 0:16:06.480
<v Speaker 1>we can get about what they look like and what

0:16:06.560 --> 0:16:08.840
<v Speaker 1>they're made out of, the better we can compare them

0:16:08.880 --> 0:16:12.200
<v Speaker 1>to predictions from our theories about how they were formed.

0:16:12.400 --> 0:16:16.800
<v Speaker 1>I mean, it sounds like a worthy use of funding. However,

0:16:16.960 --> 0:16:19.600
<v Speaker 1>might I suggest an n f T of a farting

0:16:19.640 --> 0:16:22.720
<v Speaker 1>panda instead? I'll put that on the proposed list and

0:16:22.760 --> 0:16:26.280
<v Speaker 1>see where it goes. So when we're talking about rings,

0:16:26.320 --> 0:16:29.000
<v Speaker 1>like what is it? Because you know my wedding ring

0:16:29.120 --> 0:16:34.359
<v Speaker 1>is this solid band that sits around my finger. Hula

0:16:34.440 --> 0:16:38.520
<v Speaker 1>hoop is this very thin tourists that you kind of

0:16:39.280 --> 0:16:43.040
<v Speaker 1>use the motion of your hips to keep moving around

0:16:43.280 --> 0:16:46.800
<v Speaker 1>with its momentum? So what are the rings that are

0:16:46.960 --> 0:16:50.600
<v Speaker 1>around Saturn? Are they spinning around like a hula hoop

0:16:50.720 --> 0:16:52.800
<v Speaker 1>or they just kind of sitting on it, like my

0:16:52.920 --> 0:16:55.360
<v Speaker 1>wedding ring. It's a great question, and when it comes

0:16:55.360 --> 0:16:58.120
<v Speaker 1>to astronomy, you always have to start with the definition,

0:16:58.240 --> 0:17:02.120
<v Speaker 1>which immediately puts you in to a swamp, because nothing

0:17:02.200 --> 0:17:05.719
<v Speaker 1>falls nicely into clean categories out there in space. You know,

0:17:05.760 --> 0:17:08.200
<v Speaker 1>what's a planet, what's a minor planet, what's a centaur.

0:17:08.480 --> 0:17:11.760
<v Speaker 1>A lot of these definitions come from history because we

0:17:11.760 --> 0:17:14.080
<v Speaker 1>didn't really understand what was going on, and we just

0:17:14.080 --> 0:17:16.080
<v Speaker 1>sort of named things randomly, and then we were sort

0:17:16.080 --> 0:17:19.200
<v Speaker 1>of stuck with different categories and so often they could

0:17:19.200 --> 0:17:21.080
<v Speaker 1>be a bit of a mess. Well, we're lucky in

0:17:21.160 --> 0:17:25.399
<v Speaker 1>biology because species is super simple and never has that

0:17:25.520 --> 0:17:29.600
<v Speaker 1>problem exactly. Nature doesn't confine itself to our categories. Was

0:17:29.720 --> 0:17:31.840
<v Speaker 1>out there in the universe is not things that fall

0:17:31.880 --> 0:17:36.080
<v Speaker 1>into crisply defined different boxes. It's a whole spectrum of stuff, right,

0:17:36.160 --> 0:17:38.719
<v Speaker 1>And so we just got to put these arbitrary definitions

0:17:38.720 --> 0:17:40.600
<v Speaker 1>out there so that we can talk to each other

0:17:40.680 --> 0:17:42.800
<v Speaker 1>about it. So one of the most common definitions of

0:17:42.840 --> 0:17:46.320
<v Speaker 1>a ring is a disc or ring composed of solid

0:17:46.400 --> 0:17:51.080
<v Speaker 1>materials such as dust or moonlits. Moonlits. That sounds really cute,

0:17:51.320 --> 0:17:54.240
<v Speaker 1>what's a moonlit moon is like a little moon, you know,

0:17:54.320 --> 0:17:59.560
<v Speaker 1>like a little Moonito, the old baby moon, exactly a

0:17:59.560 --> 0:18:02.320
<v Speaker 1>little my in your moon. Immediately understand, these rings are

0:18:02.359 --> 0:18:05.440
<v Speaker 1>not actually a solid object. It's not like a hulu, right,

0:18:05.560 --> 0:18:08.760
<v Speaker 1>or the rings around Saturn are not huge circles. They're

0:18:08.800 --> 0:18:12.119
<v Speaker 1>actually a bunch of tiny little particles, a bunch of

0:18:12.200 --> 0:18:14.639
<v Speaker 1>chunks that are moving in the same orbit. And so

0:18:14.720 --> 0:18:17.400
<v Speaker 1>from far away it looks like a ring. Of course,

0:18:17.440 --> 0:18:19.919
<v Speaker 1>it looks like a single hula hoop, for example, or

0:18:19.920 --> 0:18:22.080
<v Speaker 1>a wedding ring. But if you zoomed in closely, you

0:18:22.160 --> 0:18:24.640
<v Speaker 1>see it's actually a bunch of individual pieces that are

0:18:24.720 --> 0:18:27.679
<v Speaker 1>not touching each other. So cartoons have lied to me.

0:18:27.800 --> 0:18:31.800
<v Speaker 1>I cannot drive a race car or a skateboard around

0:18:32.000 --> 0:18:34.600
<v Speaker 1>the rings of Saturn. That's right. You can't do Mario

0:18:34.720 --> 0:18:37.040
<v Speaker 1>Kart on the rings of Saturn and you would fall

0:18:37.160 --> 0:18:40.560
<v Speaker 1>right through. It's very disappointing. Cartoons play it real fast

0:18:40.600 --> 0:18:44.919
<v Speaker 1>and loose with physics I'm discovering. And so basically a

0:18:45.040 --> 0:18:47.679
<v Speaker 1>ring is just like a disc of material in a

0:18:47.680 --> 0:18:49.800
<v Speaker 1>single orbit, moving all around. And that makes it a

0:18:49.800 --> 0:18:52.960
<v Speaker 1>little bit unusual because orbits are usually for one object

0:18:53.160 --> 0:18:55.040
<v Speaker 1>you know, like the Moon orbits the Earth and there's

0:18:55.040 --> 0:18:57.600
<v Speaker 1>nothing else in the Moon's orbit. It's not like there's

0:18:57.600 --> 0:19:00.560
<v Speaker 1>something else on the other side, or the Earth disorbiting

0:19:00.600 --> 0:19:03.680
<v Speaker 1>the Sun and there's nothing else in Earth's orbit, right,

0:19:03.720 --> 0:19:06.800
<v Speaker 1>it clears its own path. So it's a bunch of

0:19:07.119 --> 0:19:11.879
<v Speaker 1>individual things sharing a single orbit, kind of like a

0:19:11.960 --> 0:19:15.720
<v Speaker 1>lazy river at a water park exactly so to like

0:19:15.760 --> 0:19:18.200
<v Speaker 1>a lazy river. And once you define it that way,

0:19:18.240 --> 0:19:20.840
<v Speaker 1>you can ask questions like, well, what counts as a ring?

0:19:21.000 --> 0:19:23.280
<v Speaker 1>You know, does it have to be natural? For example,

0:19:23.440 --> 0:19:26.479
<v Speaker 1>like Earth has a bunch of stuff out there in space,

0:19:26.560 --> 0:19:29.440
<v Speaker 1>things we have launched out there, a bunch of satellites

0:19:29.600 --> 0:19:32.520
<v Speaker 1>in the same orbit, you know, zooming all around. Does

0:19:32.560 --> 0:19:35.080
<v Speaker 1>that count as a ring? Have we built our own

0:19:35.200 --> 0:19:37.920
<v Speaker 1>ring system around the Earth because all of the junk

0:19:38.000 --> 0:19:40.399
<v Speaker 1>that we put out there in space. Nobody talks about

0:19:40.440 --> 0:19:43.399
<v Speaker 1>Earth's rings, but technically, you know, it seems like that

0:19:43.480 --> 0:19:47.159
<v Speaker 1>might qualify. There's no like minimum mass requirement for the

0:19:47.280 --> 0:19:49.520
<v Speaker 1>rings as far as I can tell, so we're one

0:19:49.560 --> 0:19:53.480
<v Speaker 1>step closer to Halo am I right, high fibes everyone

0:19:53.560 --> 0:19:57.760
<v Speaker 1>who plays computer games. Another requirement for rings usually is

0:19:57.760 --> 0:19:59.960
<v Speaker 1>that they are pretty flat right, if you have just

0:20:00.119 --> 0:20:03.000
<v Speaker 1>like a swarm of spherical swarm of objects, then your

0:20:03.000 --> 0:20:05.640
<v Speaker 1>planet is just surrounded by junk. A ring is typically

0:20:05.680 --> 0:20:07.920
<v Speaker 1>something which is flattened, right, it's more like a disc.

0:20:08.280 --> 0:20:11.359
<v Speaker 1>And this already shows off what's going on with gravity.

0:20:11.640 --> 0:20:14.720
<v Speaker 1>You know, gravity has pulled the planet together and it's spinning,

0:20:14.760 --> 0:20:17.399
<v Speaker 1>and it's also pulled the ring together. And the reason

0:20:17.440 --> 0:20:20.000
<v Speaker 1>that rings form in disks is the same reason that

0:20:20.040 --> 0:20:22.919
<v Speaker 1>the Solar system is a disc. Right. That most of

0:20:22.920 --> 0:20:25.320
<v Speaker 1>the stuff is spinning in the same direction, along the

0:20:25.359 --> 0:20:29.159
<v Speaker 1>same plane, and that's because of conservation of angular momentum.

0:20:29.520 --> 0:20:33.719
<v Speaker 1>Stuff that spinning keeps spinning, and if gravity pulls it together,

0:20:33.760 --> 0:20:36.480
<v Speaker 1>it keeps spinning. It's harder for gravity to pull together

0:20:36.760 --> 0:20:40.439
<v Speaker 1>towards the spin axis than along the spin axis the

0:20:40.480 --> 0:20:44.000
<v Speaker 1>same way. For example, that like Earth resists falling into

0:20:44.040 --> 0:20:47.520
<v Speaker 1>the Sun because of its speed because of its angular momentum, right,

0:20:47.560 --> 0:20:50.640
<v Speaker 1>But the Earth didn't resist falling into the Sun's plane.

0:20:50.920 --> 0:20:53.639
<v Speaker 1>So gravity is free to compress things down into a

0:20:53.680 --> 0:20:56.880
<v Speaker 1>flat disc. But angular momentum keeps things spinning and keep

0:20:56.920 --> 0:20:59.560
<v Speaker 1>things from falling in That's what gives rings these sort

0:20:59.600 --> 0:21:02.640
<v Speaker 1>of flat structure. So that's another typical thing we expect

0:21:02.720 --> 0:21:06.080
<v Speaker 1>of rings that they're not spherical distributions of stuff. They're

0:21:06.080 --> 0:21:08.800
<v Speaker 1>like these flat disks. Because that's sort of like if

0:21:08.840 --> 0:21:11.960
<v Speaker 1>you pile a bunch of peas on a plate and

0:21:11.960 --> 0:21:14.119
<v Speaker 1>then spin the plate, all the p's are going to

0:21:14.280 --> 0:21:17.080
<v Speaker 1>scatter outwards and get everywhere, but in sort of a

0:21:17.119 --> 0:21:20.919
<v Speaker 1>flat circle. I've never done that experiment, but yes, in

0:21:20.960 --> 0:21:24.400
<v Speaker 1>my mind that that's exactly what you don't do that.

0:21:24.720 --> 0:21:27.760
<v Speaker 1>We call it pea spinning in this household. But in

0:21:27.800 --> 0:21:30.320
<v Speaker 1>our Solar system, of course, there's gravity, and gravity would

0:21:30.320 --> 0:21:33.040
<v Speaker 1>hold those p's in right, so those p's would end

0:21:33.119 --> 0:21:35.560
<v Speaker 1>up in like a circular orbit exactly instead of like

0:21:35.800 --> 0:21:38.320
<v Speaker 1>a bunch of different orbits. And so that's why the

0:21:38.320 --> 0:21:41.560
<v Speaker 1>planets are all roughly in the same plane, because they

0:21:41.600 --> 0:21:44.600
<v Speaker 1>have the same spin from the original blob of gas

0:21:44.640 --> 0:21:47.080
<v Speaker 1>and dust that formed our Solar system. And so that's

0:21:47.119 --> 0:21:50.640
<v Speaker 1>already a clue that tells you something about the origins

0:21:50.680 --> 0:21:53.760
<v Speaker 1>of these rings, because if we're if rings were formed

0:21:53.840 --> 0:21:56.040
<v Speaker 1>with the planet, then you would expect them to have

0:21:56.200 --> 0:21:58.800
<v Speaker 1>roughly the same alignment, the same spin as the planet.

0:21:58.800 --> 0:22:01.080
<v Speaker 1>And if they were not, then they necessarily have to

0:22:01.119 --> 0:22:03.120
<v Speaker 1>have that same spin that came in from like a

0:22:03.119 --> 0:22:06.120
<v Speaker 1>comet that smashed into the planet or broke up a moon,

0:22:06.520 --> 0:22:08.760
<v Speaker 1>it might give you a different kind of distribution. So

0:22:08.800 --> 0:22:11.480
<v Speaker 1>already that's a clue that tells you something about where

0:22:11.560 --> 0:22:14.320
<v Speaker 1>rings might have come from. Oh, that's really interesting. So

0:22:14.680 --> 0:22:19.680
<v Speaker 1>when you have debris from a planet's formation, everything's spinning

0:22:20.200 --> 0:22:23.320
<v Speaker 1>at the same rate, sort of going with the same flow.

0:22:23.440 --> 0:22:26.200
<v Speaker 1>But then if you have something smash into a planet,

0:22:26.240 --> 0:22:30.720
<v Speaker 1>release all these all this debris and it starts orbiting

0:22:30.720 --> 0:22:34.440
<v Speaker 1>the planet, it doesn't need to spin at the same

0:22:34.760 --> 0:22:38.520
<v Speaker 1>rate as the planet spins. Just like our moon. Our

0:22:38.560 --> 0:22:41.160
<v Speaker 1>moon doesn't spin at the same rate as Earth. Right,

0:22:41.320 --> 0:22:43.560
<v Speaker 1>that's right now, it does not, right, So that would

0:22:43.600 --> 0:22:47.080
<v Speaker 1>suggest that the moon was not necessarily formed when the

0:22:47.119 --> 0:22:49.919
<v Speaker 1>Earth was formed, right exactly. And we think that the

0:22:49.960 --> 0:22:52.960
<v Speaker 1>moon is the result of a huge collision, that something

0:22:53.000 --> 0:22:55.840
<v Speaker 1>came and smashed into the Earth and released an enormous

0:22:55.880 --> 0:23:00.240
<v Speaker 1>amount of debris which then coalesced into a moon. Right,

0:23:00.280 --> 0:23:02.920
<v Speaker 1>So that after that collision, Earth may have had a

0:23:03.040 --> 0:23:07.240
<v Speaker 1>very large cloud of debris which then probably coalesced into

0:23:07.280 --> 0:23:11.080
<v Speaker 1>a ring system, which then further gathered into a moon.

0:23:11.560 --> 0:23:14.439
<v Speaker 1>So our moon may have once been a ring. So

0:23:14.480 --> 0:23:17.800
<v Speaker 1>do we know with the rings of Saturn if they

0:23:17.840 --> 0:23:20.119
<v Speaker 1>are moving at the same rate of Saturn where to

0:23:20.160 --> 0:23:23.600
<v Speaker 1>differ rate The rings of Saturn are especially complicated because

0:23:23.640 --> 0:23:25.919
<v Speaker 1>there are so many rings, and some of them are

0:23:25.960 --> 0:23:27.800
<v Speaker 1>moving with Saturn, and some of them may actually be

0:23:27.920 --> 0:23:32.439
<v Speaker 1>rotating the other direction. It's really tricky and complicated, and

0:23:32.440 --> 0:23:34.240
<v Speaker 1>we'll dig into it in a moment when we talk

0:23:34.359 --> 0:23:38.000
<v Speaker 1>about how the rings of planets are formed, the various

0:23:38.040 --> 0:23:41.520
<v Speaker 1>theories and the pieces of evidence for and against the

0:23:41.640 --> 0:23:45.160
<v Speaker 1>first Let's take a quick break. All right, I'm gonna

0:23:45.440 --> 0:23:49.280
<v Speaker 1>try to imagine those rings moving in different directions without

0:23:49.400 --> 0:24:05.639
<v Speaker 1>getting sea sick during the break. All right, we are back.

0:24:05.960 --> 0:24:09.679
<v Speaker 1>I got a little dizzy trying to think about Saturn's rings,

0:24:09.720 --> 0:24:12.720
<v Speaker 1>some moving in one direction, others moving in another. It's

0:24:12.800 --> 0:24:15.359
<v Speaker 1>pretty trippy. But yeah, I still have a lot of

0:24:15.480 --> 0:24:20.199
<v Speaker 1>questions about these rings we're talking about, like how maybe

0:24:20.240 --> 0:24:23.960
<v Speaker 1>they're formed, whether they're formed when the planet forms out

0:24:24.000 --> 0:24:27.959
<v Speaker 1>of basically the same stuff that the planet is formed

0:24:28.000 --> 0:24:31.000
<v Speaker 1>out of, or if it is made out of kind

0:24:31.000 --> 0:24:33.879
<v Speaker 1>of some outside stuff, stuff that wasn't around when the

0:24:33.880 --> 0:24:36.880
<v Speaker 1>planet was formed, like by a collision, Like how maybe

0:24:36.920 --> 0:24:40.879
<v Speaker 1>our moon was formed do we know like what stuff

0:24:41.040 --> 0:24:43.880
<v Speaker 1>is inside of these rings? And how do we know

0:24:44.119 --> 0:24:47.320
<v Speaker 1>what is inside a ring without actually going up there

0:24:47.440 --> 0:24:50.040
<v Speaker 1>and taking a scoop of it. Yeah, that's a good question.

0:24:50.160 --> 0:24:51.639
<v Speaker 1>One thing we can do is we can look at

0:24:51.640 --> 0:24:53.720
<v Speaker 1>it through a telescope and see what kind of light

0:24:53.800 --> 0:24:56.880
<v Speaker 1>it reflects. Is it opaque, is it transparent? Is transparent

0:24:56.920 --> 0:24:59.680
<v Speaker 1>to different kinds of light? Each planet reflects sunlight, but

0:24:59.760 --> 0:25:02.320
<v Speaker 1>or all so emits particles, And so we can see

0:25:02.320 --> 0:25:05.280
<v Speaker 1>whether the rings create shadows in some sort of the

0:25:05.320 --> 0:25:08.439
<v Speaker 1>wind of Jupiter or the wind of Saturn. And we

0:25:08.520 --> 0:25:11.120
<v Speaker 1>have also sent probes out there, and these probes will

0:25:11.119 --> 0:25:13.080
<v Speaker 1>talk about them in a minute have made some really

0:25:13.080 --> 0:25:17.000
<v Speaker 1>startling discoveries by getting very close up to these rings.

0:25:17.119 --> 0:25:18.679
<v Speaker 1>But first I want to talk about sort of the

0:25:18.760 --> 0:25:21.359
<v Speaker 1>general question like talked a minute ago about the Earth's

0:25:21.400 --> 0:25:23.080
<v Speaker 1>moon and how it used to be a ring. And

0:25:23.119 --> 0:25:24.720
<v Speaker 1>you know, in my mind, one of the first question

0:25:24.760 --> 0:25:27.920
<v Speaker 1>is is like why do sometimes things form together into

0:25:28.000 --> 0:25:30.439
<v Speaker 1>a moon and sometimes they don't and they stay as

0:25:30.560 --> 0:25:33.080
<v Speaker 1>rings or is there like a process there where every

0:25:33.160 --> 0:25:37.080
<v Speaker 1>ring eventually turns into a moon. It's really fascinating question,

0:25:37.280 --> 0:25:39.320
<v Speaker 1>and it turns out to be totally dominated by the

0:25:39.400 --> 0:25:42.600
<v Speaker 1>gravity of the planet and how far you are away

0:25:42.680 --> 0:25:48.320
<v Speaker 1>from that planet. So Saturn's rings could conceivably have turned

0:25:48.320 --> 0:25:52.480
<v Speaker 1>into moons if they had been in a different situation. Conceivably. Yeah,

0:25:52.480 --> 0:25:55.200
<v Speaker 1>And it actually turns out the Saturn's rings have little

0:25:55.280 --> 0:25:58.639
<v Speaker 1>moonlits inside them that move around and shepherd them and

0:25:58.720 --> 0:26:01.199
<v Speaker 1>keep them apart. Though really fun. But the crucial thing

0:26:01.240 --> 0:26:03.880
<v Speaker 1>that determines whether something is a moon or a ring,

0:26:03.920 --> 0:26:06.200
<v Speaker 1>whether it gets torn up into little bits, or whether

0:26:06.200 --> 0:26:09.199
<v Speaker 1>it gets clumped together by gravity, is the gravity of

0:26:09.240 --> 0:26:11.200
<v Speaker 1>the host planet. You know, you have a bunch of

0:26:11.240 --> 0:26:13.760
<v Speaker 1>stuff out in the middle of space, gravity will eventually

0:26:13.800 --> 0:26:16.359
<v Speaker 1>gather it together. Gravity is very, very weak, it's the

0:26:16.400 --> 0:26:19.639
<v Speaker 1>weakest force we know. But it's also very patient and

0:26:19.680 --> 0:26:22.399
<v Speaker 1>eventually will pull things together to make a clump. So

0:26:22.440 --> 0:26:25.679
<v Speaker 1>you might expect that all rings would be transient, that

0:26:25.720 --> 0:26:28.480
<v Speaker 1>they would be eventually just gathered together into a moon,

0:26:28.760 --> 0:26:31.680
<v Speaker 1>but that's not necessarily the case because of the gravity

0:26:31.720 --> 0:26:34.240
<v Speaker 1>of the planet. This gravity does more than just pull

0:26:34.359 --> 0:26:36.879
<v Speaker 1>the moon into orbit or keep the rings in orbit.

0:26:37.080 --> 0:26:39.879
<v Speaker 1>You can also pull them apart. This is the concept

0:26:39.880 --> 0:26:42.840
<v Speaker 1>we've talked about on the podcast before, called tidal forces.

0:26:43.280 --> 0:26:45.800
<v Speaker 1>The ideas they have a very strong source of gravity

0:26:45.840 --> 0:26:48.800
<v Speaker 1>like Jupiter or a black hole, or the Sun or

0:26:48.880 --> 0:26:51.720
<v Speaker 1>even the Earth, and it's pulling on you right But

0:26:51.800 --> 0:26:54.439
<v Speaker 1>the strength of its force on you depends on how

0:26:54.480 --> 0:26:57.320
<v Speaker 1>close you are to that object. So if your feet

0:26:57.480 --> 0:27:00.399
<v Speaker 1>are closer to the Sun than your head, then the

0:27:00.440 --> 0:27:03.280
<v Speaker 1>Sun is pulling on your feet harder than it's pulling

0:27:03.280 --> 0:27:05.720
<v Speaker 1>on your head, and effectively it means it's trying to

0:27:05.720 --> 0:27:11.040
<v Speaker 1>pull your head off of your body. Nobody ever said

0:27:11.080 --> 0:27:14.560
<v Speaker 1>the Sun was a nice guy. Okay, oh, I know what.

0:27:14.720 --> 0:27:17.439
<v Speaker 1>I know that right now in July, and that's happening

0:27:17.520 --> 0:27:19.520
<v Speaker 1>right now. If you stand on the surface of the Earth,

0:27:19.600 --> 0:27:22.120
<v Speaker 1>then the Earth is literally trying to pull your head

0:27:22.200 --> 0:27:25.080
<v Speaker 1>off of your body. Now we've evolved with strong enough

0:27:25.080 --> 0:27:27.159
<v Speaker 1>next or is this this and the title forces here

0:27:27.200 --> 0:27:30.879
<v Speaker 1>are not that strong? Yeah, take that Earth. But if

0:27:30.920 --> 0:27:34.159
<v Speaker 1>you're in a situation where the gravitational forces get strong

0:27:34.400 --> 0:27:37.000
<v Speaker 1>very quickly, so the force on your feet is much

0:27:37.040 --> 0:27:39.080
<v Speaker 1>stronger than the force on your head, you can be

0:27:39.160 --> 0:27:42.040
<v Speaker 1>torn apart. And if you're near a black hole for example,

0:27:42.040 --> 0:27:44.880
<v Speaker 1>where this is very dramatic, this is what we call spaghettification,

0:27:45.240 --> 0:27:47.919
<v Speaker 1>you can get pulled apart into tiny little pieces, the

0:27:47.960 --> 0:27:52.359
<v Speaker 1>most delicious way to describe a horrific that exactly. And

0:27:52.359 --> 0:27:55.359
<v Speaker 1>we've seen this happen when comet shoemaker Levy came into

0:27:55.359 --> 0:27:57.800
<v Speaker 1>the Solar System in the nineties. It was headed for

0:27:57.840 --> 0:28:00.560
<v Speaker 1>an impact with Jupiter, but before it hit Jupiter, it

0:28:00.600 --> 0:28:03.840
<v Speaker 1>made a near miss and Jupiter pulled it apart into

0:28:03.880 --> 0:28:07.000
<v Speaker 1>twenty six pieces. So you have this comment coming into

0:28:07.000 --> 0:28:10.360
<v Speaker 1>the Solar System, which got shredded by jupiter gravity. Then

0:28:10.359 --> 0:28:13.000
<v Speaker 1>it went around the Sun and it hit Jupiter twenty

0:28:13.040 --> 0:28:16.520
<v Speaker 1>six different times, which is pretty awesome for everybody to

0:28:16.560 --> 0:28:19.480
<v Speaker 1>look at these huge fireballs the size of the Earth.

0:28:19.560 --> 0:28:22.040
<v Speaker 1>But for our six today, this is just a demonstration

0:28:22.119 --> 0:28:25.439
<v Speaker 1>of tidal forces. So a planet doesn't just pull stuff

0:28:25.520 --> 0:28:27.880
<v Speaker 1>in and keep it in orbit. It can also tear

0:28:27.920 --> 0:28:30.600
<v Speaker 1>it apart if you are close enough, I see so

0:28:30.640 --> 0:28:35.280
<v Speaker 1>because gravity gets weaker the further away you are from something,

0:28:35.359 --> 0:28:39.000
<v Speaker 1>but stronger the closer you are to something. If part

0:28:39.040 --> 0:28:41.720
<v Speaker 1>of you is far enough away that it's pretty weak

0:28:41.720 --> 0:28:43.760
<v Speaker 1>and it's not pulling on you, but the other part

0:28:43.760 --> 0:28:46.880
<v Speaker 1>of you is closer and it's tugging on you more strongly,

0:28:47.520 --> 0:28:49.280
<v Speaker 1>that part of you is going to get kind of

0:28:49.360 --> 0:28:51.800
<v Speaker 1>ripped off of the other part of you. Is that

0:28:51.880 --> 0:28:56.120
<v Speaker 1>what's happening to these poor baby little moonlits, That's what's

0:28:56.120 --> 0:28:58.720
<v Speaker 1>happening to those rings. So if you're a big blob

0:28:58.800 --> 0:29:01.520
<v Speaker 1>of material and you're too close to a planet, you

0:29:01.560 --> 0:29:04.200
<v Speaker 1>cannot form a moon because the planet will just keep

0:29:04.240 --> 0:29:07.440
<v Speaker 1>tearing you apart. If you're far enough away, then you

0:29:07.480 --> 0:29:09.880
<v Speaker 1>can form a moon. So there's a limit there. It's

0:29:09.880 --> 0:29:12.680
<v Speaker 1>called the Roche limit r O. C h E, after

0:29:12.720 --> 0:29:15.120
<v Speaker 1>a scientist who came up with this idea. If you

0:29:15.160 --> 0:29:17.960
<v Speaker 1>are closer than the Roche limit, then you cannot form

0:29:18.040 --> 0:29:21.080
<v Speaker 1>a gravitationally bound object because the gravity of the planet

0:29:21.120 --> 0:29:24.680
<v Speaker 1>is stronger than you're inherent gravity to hold yourself together.

0:29:24.760 --> 0:29:26.640
<v Speaker 1>If you're out past it, then the tidal forces are

0:29:26.640 --> 0:29:29.640
<v Speaker 1>so weak that you can clump the ring together into

0:29:29.640 --> 0:29:32.760
<v Speaker 1>a moon. So past the Roche limit you get moons.

0:29:32.800 --> 0:29:36.000
<v Speaker 1>Closer in than the Roche limit, you get rings. So

0:29:36.640 --> 0:29:41.800
<v Speaker 1>Saturn's rings are too close to Saturn itself to form

0:29:41.920 --> 0:29:46.400
<v Speaker 1>the moon, whereas our moon, which maybe started as a ring,

0:29:46.720 --> 0:29:49.320
<v Speaker 1>was far enough away that it could do its own

0:29:49.360 --> 0:29:53.640
<v Speaker 1>thing without Earth overbearing and deciding its fate for it.

0:29:53.880 --> 0:29:56.160
<v Speaker 1>That's exactly right, and it depends a little bit on

0:29:56.320 --> 0:29:58.560
<v Speaker 1>like what you're made out of. The roche limit itself

0:29:58.800 --> 0:30:01.760
<v Speaker 1>is technically just as me your hell together gravitationally, but

0:30:01.800 --> 0:30:04.120
<v Speaker 1>things can also be held together in different ways. You know,

0:30:04.160 --> 0:30:06.640
<v Speaker 1>if you have a blob of diamond, for example, as

0:30:06.640 --> 0:30:09.560
<v Speaker 1>opposed to a loose bag of golf balls, then the

0:30:09.640 --> 0:30:11.560
<v Speaker 1>diamond is going to be able to hold itself together

0:30:11.680 --> 0:30:14.040
<v Speaker 1>closer to a planet than your bag of golf balls.

0:30:14.200 --> 0:30:17.240
<v Speaker 1>I wish my wedding ring was a bag of golf balls. Now,

0:30:17.680 --> 0:30:19.760
<v Speaker 1>that would be fun. I hope your husband listens to

0:30:19.760 --> 0:30:22.640
<v Speaker 1>this podcast to hear you complaining about his gift to you.

0:30:24.080 --> 0:30:26.640
<v Speaker 1>There's a beautiful gift of love. I wish it was

0:30:26.680 --> 0:30:30.320
<v Speaker 1>a bag of golf balls. Well, in the case of

0:30:30.360 --> 0:30:33.320
<v Speaker 1>our system, for example, you know, the moon holds itself together,

0:30:33.520 --> 0:30:35.640
<v Speaker 1>but if it was closer to the Earth, the Earth

0:30:35.680 --> 0:30:39.280
<v Speaker 1>would shred it. Our moon is about three five thousand

0:30:39.400 --> 0:30:42.400
<v Speaker 1>kilometers away, and the roche limit for the Earth and

0:30:42.800 --> 0:30:45.200
<v Speaker 1>an object the size of the moon is about ten

0:30:45.320 --> 0:30:48.080
<v Speaker 1>thousand kilometers, so the Moon would have to be much

0:30:48.280 --> 0:30:51.240
<v Speaker 1>much closer to the Earth in order for the Earth

0:30:51.280 --> 0:30:53.680
<v Speaker 1>to pull it apart um and make it into a

0:30:53.760 --> 0:30:56.200
<v Speaker 1>ring system. And so that's why the moon is a moon.

0:30:56.360 --> 0:30:58.640
<v Speaker 1>In a similar way. You know, the Sun has a

0:30:58.680 --> 0:31:01.320
<v Speaker 1>tidal force on the Earth, pulling on the part of

0:31:01.320 --> 0:31:03.920
<v Speaker 1>the Earth that's closer to its stronger than it's pulling

0:31:03.960 --> 0:31:05.560
<v Speaker 1>on part of the Earth that's further from it. So

0:31:05.600 --> 0:31:08.160
<v Speaker 1>the Sun is trying to rip the Earth apart, but

0:31:08.200 --> 0:31:10.800
<v Speaker 1>the Earth is too far away, it's too strong. It

0:31:10.800 --> 0:31:14.080
<v Speaker 1>has structural integrity that keeps the Sun from destroying us

0:31:14.240 --> 0:31:17.080
<v Speaker 1>or about a hundred and fifty million kilometers from the Sun.

0:31:17.440 --> 0:31:20.040
<v Speaker 1>If we were just less than a million kilometers, then

0:31:20.040 --> 0:31:22.320
<v Speaker 1>the Earth would get pulled apart and we get torn

0:31:22.400 --> 0:31:25.760
<v Speaker 1>into a ring system around the Sun. Seems like planetary

0:31:25.800 --> 0:31:29.120
<v Speaker 1>bodies are like complicated friendships. You've got to set strong

0:31:29.280 --> 0:31:33.479
<v Speaker 1>boundaries or else you're going to get destroyed exactly. So

0:31:33.520 --> 0:31:34.920
<v Speaker 1>you just you gotta know where you are. You know,

0:31:34.920 --> 0:31:38.520
<v Speaker 1>you've got to have the conversation sometimes to figure this out. Listen, son,

0:31:38.600 --> 0:31:41.400
<v Speaker 1>we love you. You provide us with energy that gives

0:31:41.440 --> 0:31:44.120
<v Speaker 1>us food. But you know, if we're too close to you,

0:31:44.200 --> 0:31:46.400
<v Speaker 1>we all die. So you know how it is. And

0:31:46.400 --> 0:31:48.120
<v Speaker 1>so this is the basic physics of it, right, You

0:31:48.160 --> 0:31:50.440
<v Speaker 1>get too close, you turn into a ring. You stay

0:31:50.480 --> 0:31:52.880
<v Speaker 1>far away, you can be a moon. But that doesn't

0:31:52.920 --> 0:31:55.440
<v Speaker 1>answer the question of like where these things come from,

0:31:55.520 --> 0:31:59.400
<v Speaker 1>because there's still two basic ideas there. One is that

0:31:59.640 --> 0:32:02.520
<v Speaker 1>some of this stuff is from the original formation of

0:32:02.560 --> 0:32:05.000
<v Speaker 1>the Solar System. You know, you have this huge cloud

0:32:05.040 --> 0:32:07.720
<v Speaker 1>of gas and dust. A lot of it formed the Sun.

0:32:07.920 --> 0:32:10.160
<v Speaker 1>Some of the clumps together to form planets. You can

0:32:10.200 --> 0:32:12.720
<v Speaker 1>imagine that some of the stuff is close enough to

0:32:12.760 --> 0:32:15.440
<v Speaker 1>the planet that it gets trapped by the planet's gravity,

0:32:15.440 --> 0:32:17.600
<v Speaker 1>but not so close that it actually gets sucked in.

0:32:17.680 --> 0:32:20.640
<v Speaker 1>It has like too much angular momentum to actually fall

0:32:20.760 --> 0:32:23.239
<v Speaker 1>to the Earth, you know, the same way, like the

0:32:23.280 --> 0:32:26.160
<v Speaker 1>Earth right now has particles that are trapped by its

0:32:26.160 --> 0:32:29.400
<v Speaker 1>gravity and also particles that are not. The Earth's atmosphere

0:32:29.480 --> 0:32:32.920
<v Speaker 1>is boiling away into space. So you can imagine that

0:32:33.000 --> 0:32:35.400
<v Speaker 1>at the edge of the planetary formation, there might have

0:32:35.400 --> 0:32:39.000
<v Speaker 1>been particles there that didn't quite get captured by the gravity,

0:32:39.240 --> 0:32:42.080
<v Speaker 1>but they're too close to clump together into their own moon.

0:32:42.480 --> 0:32:45.360
<v Speaker 1>So that's one theory of how these rings get formed.

0:32:45.560 --> 0:32:48.520
<v Speaker 1>They're like the fastest moving bits of the planet didn't

0:32:48.560 --> 0:32:51.080
<v Speaker 1>quite get captured, but they're not fast enough moving to

0:32:51.120 --> 0:32:53.560
<v Speaker 1>be like out on a further orbit, far enough away

0:32:53.600 --> 0:32:56.360
<v Speaker 1>where they could make their own moon. So the other

0:32:56.480 --> 0:33:00.000
<v Speaker 1>theory has to do with something that wasn't there during

0:33:00.040 --> 0:33:03.640
<v Speaker 1>in the origin of the Solar System coming in and

0:33:04.520 --> 0:33:08.760
<v Speaker 1>creating some debris around Saturn or whatever planet decides to

0:33:08.960 --> 0:33:11.520
<v Speaker 1>make a ring. Yeah, so the first theory that they

0:33:11.640 --> 0:33:14.840
<v Speaker 1>are made with the planet that suggests the rings are old, right,

0:33:14.920 --> 0:33:17.000
<v Speaker 1>that they're as old as the Solar System, like four

0:33:17.000 --> 0:33:19.280
<v Speaker 1>and a half billion years old. The other theories you

0:33:19.320 --> 0:33:21.600
<v Speaker 1>say is that rings could be fairly new. Maybe they're

0:33:21.640 --> 0:33:25.040
<v Speaker 1>sort of transient. Maybe they come from a cataclysmic event,

0:33:25.200 --> 0:33:27.800
<v Speaker 1>like something comes in and smashes into a moon or

0:33:27.880 --> 0:33:31.720
<v Speaker 1>breaks up a moon, and that moon gets shredded into pieces,

0:33:31.960 --> 0:33:35.120
<v Speaker 1>and maybe it will eventually get gathered back together into

0:33:35.160 --> 0:33:38.400
<v Speaker 1>a new moon. Right, So these rings might be short

0:33:38.480 --> 0:33:41.640
<v Speaker 1>lived events in that scenario, like a comet or an

0:33:41.640 --> 0:33:45.080
<v Speaker 1>asteroid or something else might have created this huge mess.

0:33:45.120 --> 0:33:47.640
<v Speaker 1>But the Solar System will eventually clean itself up. But

0:33:47.720 --> 0:33:51.560
<v Speaker 1>if it's in that sweet spot where it's still getting

0:33:51.600 --> 0:33:56.520
<v Speaker 1>shredded by the planet's gravitational force, but it's not so

0:33:56.600 --> 0:33:58.880
<v Speaker 1>close that doesn't get sucked into the planet's going to

0:33:59.000 --> 0:34:01.320
<v Speaker 1>stay a ring, right, it could right, It depends a

0:34:01.360 --> 0:34:03.400
<v Speaker 1>lot on the details. Like you could have a moon

0:34:03.640 --> 0:34:06.240
<v Speaker 1>that was past the roche limit, but then an impact

0:34:06.320 --> 0:34:08.600
<v Speaker 1>creates a huge amount of debris, some of which falls

0:34:08.640 --> 0:34:10.759
<v Speaker 1>into the sort of the ring zone, some of it

0:34:10.800 --> 0:34:12.439
<v Speaker 1>could fall into the planet, or some of it could

0:34:12.440 --> 0:34:14.760
<v Speaker 1>stay out in the sort of moon area and form

0:34:14.800 --> 0:34:17.400
<v Speaker 1>a new moon. So you're right that you could also

0:34:17.480 --> 0:34:20.279
<v Speaker 1>form rings, which then can be fairly stable. If you

0:34:20.280 --> 0:34:22.480
<v Speaker 1>have a collision which creates a lot of mess, and

0:34:22.560 --> 0:34:24.560
<v Speaker 1>some of that mess is stable in the sort of

0:34:24.640 --> 0:34:27.040
<v Speaker 1>ring zone, then you could have a long, living ring.

0:34:27.320 --> 0:34:30.480
<v Speaker 1>That's how I like to describe myself, a stable mess.

0:34:30.520 --> 0:34:34.200
<v Speaker 1>So that seems really difficult to kind of parse out

0:34:34.320 --> 0:34:37.640
<v Speaker 1>those theories, I guess without taking a closer look, because

0:34:38.080 --> 0:34:43.120
<v Speaker 1>stuff that comes crashing into Saturn and stuff that was

0:34:43.200 --> 0:34:47.280
<v Speaker 1>originally there when Saturn was formed may from a distance

0:34:47.400 --> 0:34:51.719
<v Speaker 1>look pretty similar unless we keep investigating right exactly, And

0:34:51.760 --> 0:34:55.400
<v Speaker 1>so to understand where its specific ring comes from, we

0:34:55.440 --> 0:34:57.319
<v Speaker 1>need to look at that ring in detail, and we

0:34:57.360 --> 0:34:59.080
<v Speaker 1>need to think about isn't made out of the same

0:34:59.160 --> 0:35:01.439
<v Speaker 1>stuff as the plan in it or something weird and new?

0:35:01.600 --> 0:35:04.040
<v Speaker 1>Does it look like it's aged a lot, and does

0:35:04.080 --> 0:35:06.400
<v Speaker 1>it look like it's a fairly fresh result of a

0:35:06.400 --> 0:35:08.959
<v Speaker 1>collision or does it look like really weathered from lots

0:35:08.960 --> 0:35:12.600
<v Speaker 1>of Solar system radiation and collisions. We can also understand

0:35:12.680 --> 0:35:15.120
<v Speaker 1>the distribution of the rings, like where the mass is

0:35:15.239 --> 0:35:17.759
<v Speaker 1>in the ring, and build models to see like is

0:35:17.800 --> 0:35:20.600
<v Speaker 1>it stable, could it hold itself together? Could have developed

0:35:20.640 --> 0:35:23.720
<v Speaker 1>into this over time? So for each ring, the crucial

0:35:23.719 --> 0:35:26.080
<v Speaker 1>thing is to get as much information as possible and

0:35:26.080 --> 0:35:28.600
<v Speaker 1>then to build these models to try to explain what

0:35:28.640 --> 0:35:32.040
<v Speaker 1>we see, and that will help us discriminate between various scenarios.

0:35:32.440 --> 0:35:34.200
<v Speaker 1>And a key thing to understand is that it might

0:35:34.239 --> 0:35:37.279
<v Speaker 1>not be one answer for every ring. It might be

0:35:37.320 --> 0:35:39.960
<v Speaker 1>there are some rings that are ancient and other rings

0:35:40.000 --> 0:35:42.759
<v Speaker 1>that are very fresh. What is the difference between what

0:35:42.800 --> 0:35:45.840
<v Speaker 1>we can tell with like a telescope here on Earth

0:35:46.160 --> 0:35:49.479
<v Speaker 1>versus something we send out to get a closer look.

0:35:49.719 --> 0:35:52.240
<v Speaker 1>There's no fundamental difference, right. We can do the same

0:35:52.280 --> 0:35:54.840
<v Speaker 1>things here as we can do getting close. But of

0:35:54.880 --> 0:35:57.360
<v Speaker 1>course the closer you get, the better your data. You

0:35:57.360 --> 0:35:59.560
<v Speaker 1>can resolve these things better just because you're closer up,

0:35:59.560 --> 0:36:01.560
<v Speaker 1>so you don't need like as big a lens. You

0:36:01.600 --> 0:36:04.400
<v Speaker 1>can also bring instruments closer up, you know, things like

0:36:04.440 --> 0:36:07.560
<v Speaker 1>spectrometers to measure these things. There's one thing that you

0:36:07.600 --> 0:36:10.560
<v Speaker 1>can do by sending a satellite that you can't do

0:36:10.680 --> 0:36:13.120
<v Speaker 1>from Earth, which is to try to measure the mass

0:36:13.239 --> 0:36:15.719
<v Speaker 1>of the rings. We'll talk about it when we get

0:36:15.760 --> 0:36:18.759
<v Speaker 1>into Saturn, when we send Cassini out to Saturn and

0:36:18.800 --> 0:36:22.239
<v Speaker 1>actually dove in between the rings and the planets and

0:36:22.360 --> 0:36:26.800
<v Speaker 1>measure the effect of the rings gravity on Cassini itself

0:36:27.080 --> 0:36:29.560
<v Speaker 1>as a way to measure the mass of the rings.

0:36:29.880 --> 0:36:31.879
<v Speaker 1>And that's just not something you can do from Earth.

0:36:31.920 --> 0:36:36.040
<v Speaker 1>That's something that requires perturbing, a gravitationally throwing something out

0:36:36.120 --> 0:36:38.880
<v Speaker 1>there which is going to actually interact with the mass

0:36:38.960 --> 0:36:41.440
<v Speaker 1>of the ring itself to see how much stuff there

0:36:41.520 --> 0:36:43.960
<v Speaker 1>is in there. Is it dangerous for the satellite to

0:36:44.000 --> 0:36:45.480
<v Speaker 1>be in the rings? Like, is it going to get

0:36:45.560 --> 0:36:50.000
<v Speaker 1>hit by a bunch of little little space baby? It

0:36:50.120 --> 0:36:52.440
<v Speaker 1>can be dangerous, But a dove in between in one

0:36:52.440 --> 0:36:54.840
<v Speaker 1>of the gaps to avoid collisions. Yeah, And you know

0:36:54.920 --> 0:36:57.840
<v Speaker 1>these things seem smooth, they seem like, oh, it's a

0:36:57.840 --> 0:37:01.080
<v Speaker 1>continuous blob, but actually there's lots of gaps in between them,

0:37:01.120 --> 0:37:03.720
<v Speaker 1>so you could fly through the rings and survive, though,

0:37:03.880 --> 0:37:05.719
<v Speaker 1>you know, it would be a little bit harrowing. I

0:37:05.840 --> 0:37:08.759
<v Speaker 1>see it, well, brave little satellite, But we don't have

0:37:08.800 --> 0:37:12.400
<v Speaker 1>any satellites that have like a little extendable ice cream

0:37:12.480 --> 0:37:16.160
<v Speaker 1>scoop that scoops up some of the stuff in the rings.

0:37:16.200 --> 0:37:18.920
<v Speaker 1>So how do we know what they're made of? And

0:37:19.280 --> 0:37:20.920
<v Speaker 1>do we know what they're made of? So we can

0:37:21.160 --> 0:37:22.759
<v Speaker 1>so we know a little bit about what they're made

0:37:22.760 --> 0:37:25.000
<v Speaker 1>out of based on our models, you know what's in

0:37:25.040 --> 0:37:28.279
<v Speaker 1>the Solar system, and also based on our studies of

0:37:28.320 --> 0:37:31.200
<v Speaker 1>what light reflects off of them. That's really our best

0:37:31.239 --> 0:37:34.160
<v Speaker 1>way to understand what's in them. Mostly we think that

0:37:34.239 --> 0:37:36.960
<v Speaker 1>the rings are made out of ice and dust, and

0:37:37.000 --> 0:37:39.000
<v Speaker 1>that's also you know what the planets are made out of.

0:37:39.080 --> 0:37:41.000
<v Speaker 1>The Planets when they were forming, were made out of

0:37:41.000 --> 0:37:43.880
<v Speaker 1>the basic ingredients of the Solar system, which was dust

0:37:44.160 --> 0:37:47.799
<v Speaker 1>and ice and gas. Now, most of the gas got

0:37:47.880 --> 0:37:51.040
<v Speaker 1>slurped up by the Sun or by the gas giants themselves,

0:37:51.320 --> 0:37:53.839
<v Speaker 1>and so you're left over with ice and dust. Now,

0:37:53.880 --> 0:37:55.759
<v Speaker 1>in the inner Solar system, a lot of that ice

0:37:55.880 --> 0:37:58.640
<v Speaker 1>is vaporized. But in the outer Solar system, past what

0:37:58.680 --> 0:38:01.120
<v Speaker 1>we call the frost line, it was cold enough for

0:38:01.160 --> 0:38:03.919
<v Speaker 1>that ice to stay solid, and so it helped form

0:38:04.000 --> 0:38:06.239
<v Speaker 1>some of these ice giants, And so the rings are

0:38:06.280 --> 0:38:09.000
<v Speaker 1>made out of that same stuff, mostly ice and dust.

0:38:09.200 --> 0:38:11.560
<v Speaker 1>Beyond the frost line, there's a lot of ice in them.

0:38:11.680 --> 0:38:15.400
<v Speaker 1>Saturn's rings, for example, are mostly icy particles in closes ring.

0:38:15.480 --> 0:38:18.000
<v Speaker 1>You expect more rock and dust in rings. So when

0:38:18.000 --> 0:38:20.640
<v Speaker 1>we're talking about ice, you know, I think of I

0:38:20.640 --> 0:38:22.919
<v Speaker 1>mean especially today because it's so hot, but I think

0:38:22.920 --> 0:38:25.640
<v Speaker 1>of a big chunk of ice that I would put

0:38:25.680 --> 0:38:27.839
<v Speaker 1>in my drink, like in my glass. But is that

0:38:28.000 --> 0:38:31.480
<v Speaker 1>what this ice is? Are they big chunks? Is it

0:38:31.680 --> 0:38:34.399
<v Speaker 1>sort of like ice crystals and a bunch of them?

0:38:34.520 --> 0:38:37.680
<v Speaker 1>What form does this ice take? So when we're talking

0:38:37.719 --> 0:38:40.200
<v Speaker 1>about ice, we do mean water ice. This is like

0:38:40.440 --> 0:38:42.880
<v Speaker 1>h duo. But there's also other kinds of ice, you know,

0:38:42.920 --> 0:38:45.800
<v Speaker 1>ammonia ice and other kinds of things. So when chemists

0:38:45.880 --> 0:38:48.839
<v Speaker 1>say ice, they mean a wide range of stuff, not

0:38:49.000 --> 0:38:51.160
<v Speaker 1>just the stuff you put in your summer cocktails. But

0:38:51.239 --> 0:38:54.960
<v Speaker 1>it does include you know, drinkable water ice, like if

0:38:55.000 --> 0:38:58.640
<v Speaker 1>you are building a colony around Saturn and you need water,

0:38:58.960 --> 0:39:01.520
<v Speaker 1>like the rings are a great source of water the

0:39:01.640 --> 0:39:04.719
<v Speaker 1>humans could actually drink and it comes in chunks. You know.

0:39:04.800 --> 0:39:06.800
<v Speaker 1>Some of these things are as small as a centimeter,

0:39:06.960 --> 0:39:10.000
<v Speaker 1>like cute little ice cubes that would fit in your glass.

0:39:10.040 --> 0:39:11.520
<v Speaker 1>And some of them are like are as big as

0:39:11.600 --> 0:39:15.280
<v Speaker 1>ten meters, so you know, like really pretty big chunks.

0:39:15.320 --> 0:39:17.080
<v Speaker 1>You'd have to be a giant to enjoy that in

0:39:17.120 --> 0:39:21.000
<v Speaker 1>your limited So I couldn't theory right that satellite hold

0:39:21.080 --> 0:39:23.719
<v Speaker 1>out a glass eliminated and get some ice in there.

0:39:23.800 --> 0:39:26.480
<v Speaker 1>As long as I don't get pulverized by a giant

0:39:26.520 --> 0:39:30.239
<v Speaker 1>ice chunk, that's great news. What's the dust made out of?

0:39:30.480 --> 0:39:32.919
<v Speaker 1>So the dust is just you know, silicates, it's like rock,

0:39:33.200 --> 0:39:34.960
<v Speaker 1>the same kind of stuff that the Earth is made

0:39:35.000 --> 0:39:37.800
<v Speaker 1>out of. Like it's just basically dirt, you know, huge

0:39:37.880 --> 0:39:40.280
<v Speaker 1>chunks of rock and dirt. And some of these things

0:39:40.360 --> 0:39:43.760
<v Speaker 1>have organic compounds in them, you know. We wonder about

0:39:43.760 --> 0:39:46.560
<v Speaker 1>like the formation of life whatever. The interesting area of

0:39:46.560 --> 0:39:49.759
<v Speaker 1>research is like where do organic molecules come from the

0:39:49.760 --> 0:39:52.520
<v Speaker 1>basic building blocks of life? Are they only found on

0:39:52.600 --> 0:39:55.040
<v Speaker 1>Earth or are they found all over the universe? So

0:39:55.120 --> 0:39:57.279
<v Speaker 1>looking at the rings helps us understand that kind of thing.

0:39:57.320 --> 0:40:00.799
<v Speaker 1>We also study asteroids and comets and we find is

0:40:00.800 --> 0:40:04.080
<v Speaker 1>that there are organic compounds all over the Solar system.

0:40:04.360 --> 0:40:08.000
<v Speaker 1>These basic building blocks are not rare, They're everywhere. So

0:40:08.080 --> 0:40:11.719
<v Speaker 1>you've got ice, which is, you know, the solid form

0:40:11.760 --> 0:40:14.880
<v Speaker 1>of water, and you've got organic compounds. Is there a

0:40:14.960 --> 0:40:18.840
<v Speaker 1>reason why we wouldn't expect there to be life on Saturn?

0:40:18.960 --> 0:40:21.200
<v Speaker 1>Is it because the ice would be solid? Or is

0:40:21.239 --> 0:40:25.640
<v Speaker 1>it because Saturn's surface is not hospitable to the formation

0:40:25.680 --> 0:40:27.560
<v Speaker 1>of life. I don't know if there's life on Satura.

0:40:27.600 --> 0:40:30.000
<v Speaker 1>And of course, if there is, life on Saturday would

0:40:30.040 --> 0:40:32.920
<v Speaker 1>have to be quite different from life on Earth because

0:40:33.200 --> 0:40:36.400
<v Speaker 1>the environment on Saturday is very different. Right Saturday is

0:40:36.440 --> 0:40:39.439
<v Speaker 1>a gas giant and so it's very high pressure. There's

0:40:39.480 --> 0:40:42.239
<v Speaker 1>a lot of radiation on Saturn, so it would have

0:40:42.280 --> 0:40:45.600
<v Speaker 1>to be quite different. But one of the moons of Saturn, Insulatus,

0:40:45.680 --> 0:40:49.480
<v Speaker 1>which we've talked about, has an icy shell, and underneath

0:40:49.719 --> 0:40:53.400
<v Speaker 1>is a liquid ocean, and that liquid ocean is partially

0:40:53.480 --> 0:40:57.520
<v Speaker 1>kept liquid by those tidal forces. Saturny is squeezing that moon,

0:40:57.600 --> 0:41:00.480
<v Speaker 1>which keeps it from freezing. It's imparting energy to it,

0:41:00.719 --> 0:41:03.680
<v Speaker 1>sort of like by massaging it with its gravity. So

0:41:03.800 --> 0:41:07.920
<v Speaker 1>in the water under the surface of Ensilatus might be

0:41:08.200 --> 0:41:10.879
<v Speaker 1>some life. We just don't know, but the rings are

0:41:11.000 --> 0:41:14.279
<v Speaker 1>mostly frozen. They're mostly just big chunks of ice. And

0:41:14.320 --> 0:41:17.440
<v Speaker 1>you know, there's a fascinating sort of geometrical structure here

0:41:17.480 --> 0:41:21.120
<v Speaker 1>because they are very, very wide. You know, these things

0:41:21.160 --> 0:41:25.399
<v Speaker 1>are like seventy two hundred thousand kilometers wide. We're talking

0:41:25.400 --> 0:41:28.640
<v Speaker 1>about Saturn's rings, but in terms of thickness, they're like

0:41:28.800 --> 0:41:32.080
<v Speaker 1>twenty meters thick. So there are tens of thousands of

0:41:32.160 --> 0:41:35.719
<v Speaker 1>kilometers wide and only tens of meters thick. If you

0:41:35.800 --> 0:41:38.319
<v Speaker 1>had a sheet of paper of this thickness, they would

0:41:38.320 --> 0:41:41.080
<v Speaker 1>have to be like a kilometer wide sheet of paper

0:41:41.360 --> 0:41:44.239
<v Speaker 1>to have the same proportions as Saturn's rings. That's an

0:41:44.280 --> 0:41:48.960
<v Speaker 1>idea for your science project, elementary schoolers, a model of

0:41:49.040 --> 0:41:52.080
<v Speaker 1>Saturn's rings. And you know, you can see Saturn's rings

0:41:52.160 --> 0:41:55.239
<v Speaker 1>from Earth, which is incredible without a really powerful telescope.

0:41:55.440 --> 0:41:57.520
<v Speaker 1>But there's a lot more rings to Saturn than you

0:41:57.520 --> 0:42:00.920
<v Speaker 1>can just see. There's three really bright ring which astronomers

0:42:00.920 --> 0:42:04.799
<v Speaker 1>have cleverly named A, B, and C, of course, but

0:42:04.880 --> 0:42:07.200
<v Speaker 1>there are other rings that go out even further out

0:42:07.239 --> 0:42:09.680
<v Speaker 1>to the G ring and the E ring, and these

0:42:09.760 --> 0:42:13.600
<v Speaker 1>go out like past three to nine times the radius

0:42:13.640 --> 0:42:16.920
<v Speaker 1>of Saturn itself, So like the volume of Saturn is

0:42:17.000 --> 0:42:20.400
<v Speaker 1>dominated by these rings. It's like the biggest thing in

0:42:20.440 --> 0:42:24.479
<v Speaker 1>the Saturn system. That's really interesting. So how many rings

0:42:24.480 --> 0:42:27.000
<v Speaker 1>are there total? Denal, Well, there are rings out to

0:42:27.160 --> 0:42:29.480
<v Speaker 1>G rings and the rings right and so there are

0:42:29.600 --> 0:42:31.719
<v Speaker 1>like dozens of these rings. And it depends a little

0:42:31.719 --> 0:42:33.840
<v Speaker 1>bit on how you count, because each of the rings

0:42:33.960 --> 0:42:37.160
<v Speaker 1>can be subdivided into like sub rings. And some of

0:42:37.160 --> 0:42:39.560
<v Speaker 1>these rings that have there are these gaps between them

0:42:39.640 --> 0:42:43.200
<v Speaker 1>which are maintained by these little shepherd moons. So you

0:42:43.239 --> 0:42:46.239
<v Speaker 1>have these little moonlits which are strong enough to survive

0:42:46.440 --> 0:42:48.719
<v Speaker 1>inside the roche limit. Remember the rocial limit not a

0:42:48.760 --> 0:42:50.960
<v Speaker 1>hard and fast rule, depending on what you're made out of.

0:42:51.320 --> 0:42:53.239
<v Speaker 1>So if you're a small enough moon and you made

0:42:53.239 --> 0:42:55.799
<v Speaker 1>have a really tough stuff and you can survive in

0:42:55.880 --> 0:42:58.520
<v Speaker 1>the ring system and you sort of perturb the rings,

0:42:58.640 --> 0:43:01.239
<v Speaker 1>you can like keep the rings from mixing with each other.

0:43:01.560 --> 0:43:03.880
<v Speaker 1>So a lot of these gaps are because there's a moon.

0:43:04.000 --> 0:43:06.800
<v Speaker 1>They are a little moonlit that's keeping them apart, a

0:43:06.920 --> 0:43:10.799
<v Speaker 1>little hall monitor moon that's adorable exactly, and it keeps

0:43:10.880 --> 0:43:14.279
<v Speaker 1>them having the like really crisply sharply defined edges. It

0:43:14.320 --> 0:43:17.440
<v Speaker 1>seems like there's a bunch of mass and these rings,

0:43:17.680 --> 0:43:22.040
<v Speaker 1>how do we know that, like Saturn's gravity is strong

0:43:22.160 --> 0:43:25.920
<v Speaker 1>enough to keep them in that sort of sweet spot

0:43:26.040 --> 0:43:30.160
<v Speaker 1>of staying rings and not drifting out or forming moons.

0:43:30.400 --> 0:43:32.919
<v Speaker 1>So we didn't know until pretty recently how much mass

0:43:32.960 --> 0:43:34.759
<v Speaker 1>there was. You knew we could see it, but we

0:43:34.760 --> 0:43:36.840
<v Speaker 1>didn't really know like how much stuff is there is

0:43:37.000 --> 0:43:39.840
<v Speaker 1>equivalent to a moon? Is it like thousand times and moons?

0:43:39.840 --> 0:43:41.799
<v Speaker 1>It much less than a moon of Saturn. And so

0:43:41.880 --> 0:43:43.880
<v Speaker 1>it was when Cassini went up there and it passed

0:43:43.920 --> 0:43:46.799
<v Speaker 1>between these rings that it gave us a measurement for

0:43:46.840 --> 0:43:49.239
<v Speaker 1>how much mass there is. And what we discovered was

0:43:49.280 --> 0:43:52.560
<v Speaker 1>that the rings had sort of surprisingly low mass. We

0:43:52.600 --> 0:43:54.840
<v Speaker 1>expected them to have some more mass, to be like

0:43:54.880 --> 0:43:58.200
<v Speaker 1>more substantial, but they're really sort of like light and fluffy.

0:43:58.280 --> 0:44:00.719
<v Speaker 1>The other thing that's really interesting for Cassini is that

0:44:00.760 --> 0:44:03.040
<v Speaker 1>we got these very close up pictures of what these

0:44:03.120 --> 0:44:05.640
<v Speaker 1>rings were made out of, and scientists were surprised to

0:44:05.680 --> 0:44:08.160
<v Speaker 1>see that the components of the rings were still sort

0:44:08.200 --> 0:44:10.960
<v Speaker 1>of sharp, you know, they have like crisp edges to them.

0:44:11.120 --> 0:44:14.600
<v Speaker 1>They're really quite reflective compared to what we expected if

0:44:14.640 --> 0:44:17.120
<v Speaker 1>these rings were ancient. If they've been there for a

0:44:17.160 --> 0:44:19.960
<v Speaker 1>long long time, you would expect them to bump into

0:44:20.000 --> 0:44:23.160
<v Speaker 1>each other. Things eventually get rounded. All the radiation from

0:44:23.200 --> 0:44:25.319
<v Speaker 1>Saturn would have weathered them a little bit. That gives

0:44:25.400 --> 0:44:29.200
<v Speaker 1>people the impression that maybe these things are quite new. Right,

0:44:29.239 --> 0:44:31.200
<v Speaker 1>If you add up all the mass of these rings,

0:44:31.280 --> 0:44:34.160
<v Speaker 1>it's just about the mass of a typical moon of Saturn,

0:44:34.320 --> 0:44:37.760
<v Speaker 1>which is very suggestive. It says maybe this was once

0:44:37.840 --> 0:44:40.120
<v Speaker 1>a moon of Saturn. Maybe one of the moons of

0:44:40.160 --> 0:44:43.239
<v Speaker 1>Saturn got smashed up in a collision, they bounced into

0:44:43.239 --> 0:44:45.880
<v Speaker 1>each other, or something came into the Solar system and

0:44:45.920 --> 0:44:49.080
<v Speaker 1>destroyed a moon of Saturn and created this big mess

0:44:49.239 --> 0:44:52.000
<v Speaker 1>which then fell into the Roche limit and became the

0:44:52.080 --> 0:44:54.719
<v Speaker 1>rings of Saturn. It's a theory. We just don't know,

0:44:55.040 --> 0:44:58.120
<v Speaker 1>but it's one speculation. So if when you're saying these

0:44:58.160 --> 0:45:01.000
<v Speaker 1>are relatively new, what do you mean by that? Because

0:45:01.160 --> 0:45:04.160
<v Speaker 1>I've learned that when you say new in terms of

0:45:04.520 --> 0:45:09.120
<v Speaker 1>the Solar System or the universe, it means very old exactly.

0:45:09.400 --> 0:45:12.279
<v Speaker 1>It means new on a universe time scale. So we're

0:45:12.280 --> 0:45:16.240
<v Speaker 1>talking like maybe in the last hundred million years, whereas

0:45:16.280 --> 0:45:18.960
<v Speaker 1>the Solar system is four and a half billion years

0:45:19.040 --> 0:45:22.239
<v Speaker 1>old if you're forty five, for example, saying you had

0:45:22.280 --> 0:45:24.480
<v Speaker 1>a ring in the last year or so makes it

0:45:24.520 --> 0:45:27.319
<v Speaker 1>feel sort of new, right, Yeah, I mean my ring

0:45:27.560 --> 0:45:31.560
<v Speaker 1>feels still pretty new even though it's about a year old.

0:45:31.600 --> 0:45:36.680
<v Speaker 1>But yes, so that is really interesting. Do you think

0:45:36.719 --> 0:45:39.719
<v Speaker 1>these rings around Saturn are permanent? Well, we don't know

0:45:39.960 --> 0:45:42.400
<v Speaker 1>how long they are going to last. If they're fairly new,

0:45:42.800 --> 0:45:44.799
<v Speaker 1>it suggests that they might not. They might be like

0:45:44.920 --> 0:45:48.319
<v Speaker 1>falling into Saturn. Saturn might be losing its moods as

0:45:48.360 --> 0:45:51.440
<v Speaker 1>its gravity pulls these little bits into it. Or they

0:45:51.480 --> 0:45:54.000
<v Speaker 1>could also be quite stable, right, even if they are new,

0:45:54.040 --> 0:45:55.920
<v Speaker 1>they could still be stable if they ended up in

0:45:55.960 --> 0:45:58.360
<v Speaker 1>the right spot, if they're within the roche limit. So

0:45:58.400 --> 0:46:00.400
<v Speaker 1>in order to understand that whether it's and it's going

0:46:00.440 --> 0:46:02.480
<v Speaker 1>to keep its rings, we need to understand some of

0:46:02.480 --> 0:46:05.240
<v Speaker 1>the process is going on there, like is Saturn gathering

0:46:05.239 --> 0:46:08.040
<v Speaker 1>these things up? Are things falling into Saturn or not.

0:46:08.239 --> 0:46:10.719
<v Speaker 1>We also need to understand like whether there are new

0:46:10.840 --> 0:46:14.160
<v Speaker 1>sources for these rings. That same moon we talked about

0:46:14.160 --> 0:46:17.720
<v Speaker 1>insult Us also has geysers on it, so like cracks

0:46:17.800 --> 0:46:22.239
<v Speaker 1>in those oceans shoot water out into space, constantly, and

0:46:22.280 --> 0:46:25.240
<v Speaker 1>this is new material for rings, as those newly formed

0:46:25.280 --> 0:46:28.759
<v Speaker 1>crystals in space gets sucked in by Saturn's gravity. So

0:46:28.800 --> 0:46:31.560
<v Speaker 1>there's a really far out ring called the E ring,

0:46:31.800 --> 0:46:36.120
<v Speaker 1>which probably is being constantly replenished by geysers from one

0:46:36.120 --> 0:46:39.560
<v Speaker 1>of Saturn's moons. Well, that's interesting. So you've got like

0:46:39.600 --> 0:46:44.160
<v Speaker 1>a sprinkler system that is keeping these rings alive. Well,

0:46:44.160 --> 0:46:47.440
<v Speaker 1>I hope Saturn has a sense of commitment so keeps

0:46:47.440 --> 0:46:50.280
<v Speaker 1>that ring for our benefit because it is so pretty

0:46:50.320 --> 0:46:55.120
<v Speaker 1>to look at. But I'm also curious why Saturn is

0:46:55.200 --> 0:46:58.160
<v Speaker 1>so unique in its rings in the Solar System, or

0:46:58.200 --> 0:47:01.680
<v Speaker 1>whether it is unique. But first I need to take

0:47:01.680 --> 0:47:05.080
<v Speaker 1>a break, and I'm gonna do a little hula hooping

0:47:05.200 --> 0:47:08.920
<v Speaker 1>so I can feel more like I am saturned, so

0:47:09.000 --> 0:47:25.200
<v Speaker 1>I can visualize what it's like to be saturned. And

0:47:25.360 --> 0:47:29.880
<v Speaker 1>we're back after an exhausting five minutes of me hula hooping.

0:47:29.960 --> 0:47:32.440
<v Speaker 1>Remind me never to do that again. But I was

0:47:32.480 --> 0:47:36.960
<v Speaker 1>asking before the break, is Saturn unique in the Solar

0:47:37.000 --> 0:47:39.960
<v Speaker 1>System in terms of its rings and why is it unique?

0:47:39.960 --> 0:47:43.000
<v Speaker 1>Because it seems like it at least has the most

0:47:43.040 --> 0:47:46.480
<v Speaker 1>spectacular rings in the Solar System. It definitely has the

0:47:46.480 --> 0:47:49.520
<v Speaker 1>most spectacular rings and the most obvious from Earth, but

0:47:49.560 --> 0:47:51.839
<v Speaker 1>it turns out it's actually not unique, and that there

0:47:51.880 --> 0:47:54.680
<v Speaker 1>are rings all over the Solar System, and there are

0:47:54.760 --> 0:47:57.480
<v Speaker 1>rings that might be right in our backyard and in

0:47:57.560 --> 0:48:00.600
<v Speaker 1>our future. When you look up at more Cars, which

0:48:00.640 --> 0:48:03.000
<v Speaker 1>is one of our neighboring planets, you don't see rings

0:48:03.040 --> 0:48:05.720
<v Speaker 1>on it. But that might be different in about thirty

0:48:05.760 --> 0:48:09.320
<v Speaker 1>two fifty million years, because Mars is in the process

0:48:09.320 --> 0:48:12.799
<v Speaker 1>of pulling apart its moons and shredding them, so they

0:48:12.840 --> 0:48:16.440
<v Speaker 1>eventually might turn into rings. So physicists out there, I

0:48:16.440 --> 0:48:18.400
<v Speaker 1>want to give you some advice. If you are in

0:48:18.400 --> 0:48:22.319
<v Speaker 1>a relationship and you tell your partner, I see a

0:48:22.400 --> 0:48:25.919
<v Speaker 1>ring in our future, just before warned that they may

0:48:25.960 --> 0:48:30.600
<v Speaker 1>not know you're talking about Mars, and that you've got

0:48:30.680 --> 0:48:33.040
<v Speaker 1>to wait quite a while. You know, we're talking about

0:48:33.080 --> 0:48:36.120
<v Speaker 1>tens of millions of years, and Mars is a really

0:48:36.120 --> 0:48:40.000
<v Speaker 1>fascinating case because it might sort of up end this clear,

0:48:40.080 --> 0:48:42.759
<v Speaker 1>crisp difference between rings and moons a little bit. I

0:48:42.840 --> 0:48:45.279
<v Speaker 1>read a recent paper that suggests that it might be

0:48:45.320 --> 0:48:48.800
<v Speaker 1>in the middle of a ring moon cycle. Then it

0:48:48.880 --> 0:48:51.760
<v Speaker 1>might be forming moons which then get shredded into rings.

0:48:51.840 --> 0:48:54.479
<v Speaker 1>Which then get formed back into moons. So it could

0:48:54.480 --> 0:48:57.760
<v Speaker 1>be like slashing back and forth between ringed and mooned

0:48:57.760 --> 0:49:00.239
<v Speaker 1>and ringed and mooned. That's interesting, I do you know

0:49:00.360 --> 0:49:04.200
<v Speaker 1>some people like that. But so how does it If

0:49:04.239 --> 0:49:06.959
<v Speaker 1>it keeps shifting back and forth, that must mean that

0:49:07.000 --> 0:49:11.319
<v Speaker 1>this roche limit is not always stable. What makes it unstable? Well,

0:49:11.360 --> 0:49:14.680
<v Speaker 1>it depends again on how strong this thing is, the

0:49:14.719 --> 0:49:18.120
<v Speaker 1>structural integrity of the object, and exactly where it is.

0:49:18.280 --> 0:49:20.840
<v Speaker 1>The idea here is you have a giant impact, and

0:49:20.880 --> 0:49:23.759
<v Speaker 1>this giant impact doesn't just create a big spray of

0:49:23.800 --> 0:49:26.400
<v Speaker 1>debris which can form into rings and moons, but it

0:49:26.400 --> 0:49:30.400
<v Speaker 1>can also actually change the gravitational field of the planet itself,

0:49:30.440 --> 0:49:33.560
<v Speaker 1>so like exactly where the roche limit is can change.

0:49:33.760 --> 0:49:36.120
<v Speaker 1>So you can have, for example, the formation of a moon,

0:49:36.719 --> 0:49:39.120
<v Speaker 1>which can last for a little while, but then as

0:49:39.200 --> 0:49:41.880
<v Speaker 1>the planet itself settles back down, you know, part of

0:49:41.880 --> 0:49:44.399
<v Speaker 1>this debris then falls back onto the planet, it can

0:49:44.480 --> 0:49:47.680
<v Speaker 1>change where the roche limit is. So the moon forms

0:49:47.680 --> 0:49:49.960
<v Speaker 1>when the rocial limits in one place, but then as

0:49:50.040 --> 0:49:52.200
<v Speaker 1>the stuff settles in and some of it falls onto

0:49:52.239 --> 0:49:55.360
<v Speaker 1>the planet, the rochial limit shifts, and so the moons

0:49:55.360 --> 0:49:57.759
<v Speaker 1>can then be torn apart. Some of that stuff might

0:49:57.800 --> 0:50:00.239
<v Speaker 1>fall down to the planet, some of it might former ring,

0:50:00.520 --> 0:50:02.479
<v Speaker 1>some of it might like form like a half moon

0:50:02.719 --> 0:50:06.360
<v Speaker 1>which gets pushed out even further. So we're talking about Mars'

0:50:06.560 --> 0:50:10.240
<v Speaker 1>potential future here and potential past. But you also mentioned

0:50:10.239 --> 0:50:12.800
<v Speaker 1>that there are a lot of rings in the Solar

0:50:12.840 --> 0:50:15.799
<v Speaker 1>system currently, right, There are a lot of rings in

0:50:15.800 --> 0:50:19.040
<v Speaker 1>the Solar System exactly. So Jupiter, for example, also has rings.

0:50:19.120 --> 0:50:20.959
<v Speaker 1>These are interesting because they're one of the first ones

0:50:21.040 --> 0:50:24.359
<v Speaker 1>discovered by a satellite. Like it's very hard to see

0:50:24.440 --> 0:50:29.239
<v Speaker 1>Jupiter's rings from Earth, even with a very very powerful telescope,

0:50:29.560 --> 0:50:32.160
<v Speaker 1>and so these were discovered in seventy nine by voyage

0:50:32.160 --> 0:50:33.960
<v Speaker 1>of one And the reason that they're hard to see

0:50:34.000 --> 0:50:36.680
<v Speaker 1>is that they're very faint and it consists mostly of dust,

0:50:37.120 --> 0:50:41.279
<v Speaker 1>and people think that they're probably just constantly created by

0:50:41.360 --> 0:50:45.319
<v Speaker 1>micro meteorites hitting the planets moons. Remember, Jupiter is very

0:50:45.440 --> 0:50:48.479
<v Speaker 1>very massive and it's very strong gravity, so it's likely

0:50:48.600 --> 0:50:50.120
<v Speaker 1>just like suck a lot of this stuff up. But

0:50:50.120 --> 0:50:53.120
<v Speaker 1>they think that there's like a constant replenishment of this

0:50:53.200 --> 0:50:56.480
<v Speaker 1>stuff as things hit the Moon create this like debris

0:50:56.840 --> 0:50:59.600
<v Speaker 1>which forms sort of a temporary ring around Jupiter, which

0:50:59.640 --> 0:51:03.080
<v Speaker 1>eventually falls back into Jupiter. So Jupiter's gravity is so

0:51:03.120 --> 0:51:05.560
<v Speaker 1>strong that doesn't really have a chance to accumulate a

0:51:05.680 --> 0:51:08.840
<v Speaker 1>ring that lasts very long. You mentioned that it's harder

0:51:08.880 --> 0:51:11.200
<v Speaker 1>to see it because it's mainly made out of dust.

0:51:11.320 --> 0:51:14.600
<v Speaker 1>What makes ice more visible? Ice is just shiny or like,

0:51:14.640 --> 0:51:16.800
<v Speaker 1>it's just basic chemistry. You shine a light on a

0:51:16.800 --> 0:51:18.640
<v Speaker 1>piece of ice, it's going to reflect more than a

0:51:18.760 --> 0:51:21.920
<v Speaker 1>rock will. Right, So ice is just brighter and wider.

0:51:22.120 --> 0:51:25.080
<v Speaker 1>I guess that's why we call diamonds ice. That makes fun.

0:51:26.000 --> 0:51:29.080
<v Speaker 1>And Jupiter also, remember, is not just gravitationally powerful. It

0:51:29.080 --> 0:51:32.239
<v Speaker 1>has very strong magnetic fields and radiation, and so the

0:51:32.239 --> 0:51:36.680
<v Speaker 1>electromagnetic forces interact with these dust particles moving around Jupiter,

0:51:37.000 --> 0:51:38.920
<v Speaker 1>and it means that it's hard for these things to

0:51:39.200 --> 0:51:41.279
<v Speaker 1>orbit Jupiter for more than like a hundred or a

0:51:41.360 --> 0:51:44.680
<v Speaker 1>thousand years. And so for Jupiter to have a ring

0:51:44.719 --> 0:51:46.960
<v Speaker 1>system at any point that lasts more than you know,

0:51:47.000 --> 0:51:49.040
<v Speaker 1>a hundred or a thousand years, means it needs a

0:51:49.080 --> 0:51:52.680
<v Speaker 1>constant source of replenishment. That's why this theory that micro

0:51:52.719 --> 0:51:56.880
<v Speaker 1>meteorites are creating dust constantly to sort of feed Jupiter's

0:51:56.960 --> 0:52:00.000
<v Speaker 1>ring system. I see, so Jupiter is just too hungry

0:52:00.360 --> 0:52:05.360
<v Speaker 1>to maintain that ring without having some of those micro

0:52:05.480 --> 0:52:09.759
<v Speaker 1>collisions spewing out more debris. Is Jupiter the only other

0:52:09.800 --> 0:52:13.160
<v Speaker 1>planet that has rings. No Neptune also has rings. These

0:52:13.160 --> 0:52:16.040
<v Speaker 1>are really fascinating, the Air five rings, but they're sort

0:52:16.040 --> 0:52:18.680
<v Speaker 1>of the reverse of Saturn. Instead of being mostly ice,

0:52:18.760 --> 0:52:22.000
<v Speaker 1>they're actually mostly dark particles and they're confined to a

0:52:22.040 --> 0:52:25.600
<v Speaker 1>few little narrow rings, and they're really interesting because they're

0:52:25.640 --> 0:52:27.960
<v Speaker 1>not the same all the way around. It's not like

0:52:28.040 --> 0:52:30.760
<v Speaker 1>Saturn that has this symmetry to have these like bright

0:52:30.920 --> 0:52:33.719
<v Speaker 1>arcs and then these empty gaps between them, so it's

0:52:33.800 --> 0:52:39.239
<v Speaker 1>really kind of weird. So these like broken rings around Saturn, yeah, exactly.

0:52:39.280 --> 0:52:41.880
<v Speaker 1>And people think that maybe there are moons. They're like

0:52:41.960 --> 0:52:44.440
<v Speaker 1>little shepherd moons that are interfering with these rings and

0:52:44.520 --> 0:52:46.640
<v Speaker 1>causing this structure, but we haven't been able to see

0:52:46.640 --> 0:52:49.600
<v Speaker 1>them because our telescopes aren't powerful enough yet. And Urine

0:52:49.680 --> 0:52:52.920
<v Speaker 1>is also has rings. These rings are really strange because

0:52:52.920 --> 0:52:57.319
<v Speaker 1>they're almost totally black. They're like lumps of coal, so

0:52:57.360 --> 0:53:00.239
<v Speaker 1>they think they might be like carbon and hydrocarbon, but

0:53:00.280 --> 0:53:02.640
<v Speaker 1>they're just not sure. So we really need are like

0:53:02.880 --> 0:53:06.120
<v Speaker 1>more exploration of the outer Solar system to understand these

0:53:06.239 --> 0:53:08.400
<v Speaker 1>rings and the role they play in the history of

0:53:08.440 --> 0:53:11.880
<v Speaker 1>these planets. I like that Urineus is going for a

0:53:11.920 --> 0:53:14.799
<v Speaker 1>golf look that is bringing Goth back. I don't know

0:53:14.840 --> 0:53:18.719
<v Speaker 1>if it ever left. So our solar system has a

0:53:18.760 --> 0:53:21.239
<v Speaker 1>good number of rings. But we talked about at the

0:53:21.280 --> 0:53:25.320
<v Speaker 1>beginning whether we are unique as a solar system, whether

0:53:25.600 --> 0:53:29.600
<v Speaker 1>we can find rings outside of our solar system. Is

0:53:29.600 --> 0:53:33.480
<v Speaker 1>there any evidence of rings uh far and wide. So

0:53:33.560 --> 0:53:37.120
<v Speaker 1>scientists think that it's very plausible that other planets might

0:53:37.160 --> 0:53:39.960
<v Speaker 1>have rings, just because they're not that unusual in our

0:53:39.960 --> 0:53:42.880
<v Speaker 1>solar system. As you can hear, they're like basically everywhere

0:53:42.920 --> 0:53:46.760
<v Speaker 1>you know, Saturn, Jupiter, Urinous, Neptune, even Mars might eventually

0:53:46.760 --> 0:53:50.360
<v Speaker 1>have rings. So we suspect that just from that data,

0:53:50.440 --> 0:53:52.640
<v Speaker 1>they should be in other solar systems. But of course

0:53:52.640 --> 0:53:54.400
<v Speaker 1>we want to see it and to know. We don't

0:53:54.600 --> 0:53:56.800
<v Speaker 1>just want to speculate about the nature of the universe.

0:53:56.880 --> 0:53:59.520
<v Speaker 1>And so what we can do is look for rings

0:53:59.560 --> 0:54:01.719
<v Speaker 1>around planet's in much the same way that we look

0:54:01.719 --> 0:54:05.279
<v Speaker 1>for the planets themselves. The way we detect planets around

0:54:05.280 --> 0:54:08.440
<v Speaker 1>other stars, or one way at least, is the transit method.

0:54:08.560 --> 0:54:10.880
<v Speaker 1>The planet passes in front of its star like a

0:54:10.880 --> 0:54:13.959
<v Speaker 1>little mini eclipse and dims the light of that star

0:54:14.160 --> 0:54:16.799
<v Speaker 1>a little bit. That's how we know the planet is there.

0:54:16.960 --> 0:54:19.040
<v Speaker 1>How can we see rings around it? Well? From the

0:54:19.080 --> 0:54:20.880
<v Speaker 1>transit method, we can also get a sense of the

0:54:21.000 --> 0:54:24.440
<v Speaker 1>size of the planet and its mass. So we get

0:54:24.440 --> 0:54:26.759
<v Speaker 1>a sense of the size because of how much light

0:54:27.000 --> 0:54:29.279
<v Speaker 1>is blocked from the star. We get a sense of

0:54:29.280 --> 0:54:31.719
<v Speaker 1>its mass because we can measure its orbit. And so

0:54:31.760 --> 0:54:35.000
<v Speaker 1>if the planet seems to be really really large, there's

0:54:35.040 --> 0:54:37.439
<v Speaker 1>like this extra reduction in the light of the star

0:54:37.560 --> 0:54:41.040
<v Speaker 1>because it has like big fluffy things around it, that

0:54:41.120 --> 0:54:44.160
<v Speaker 1>might be evidence for rings around the planet. If it

0:54:44.200 --> 0:54:47.640
<v Speaker 1>seems like bigger than we would otherwise understand it to be.

0:54:47.880 --> 0:54:50.279
<v Speaker 1>It seems like bigger than we would otherwise expect it

0:54:50.320 --> 0:54:52.879
<v Speaker 1>to be from its mass and from its orbit. I see.

0:54:52.920 --> 0:54:56.520
<v Speaker 1>So if the orbit doesn't match how fluffy it looks,

0:54:56.520 --> 0:54:59.680
<v Speaker 1>how much light it blocks, that may be a sign

0:54:59.680 --> 0:55:02.400
<v Speaker 1>of a ring. Could it be something else instead of

0:55:02.400 --> 0:55:05.359
<v Speaker 1>a ring, like we mentioned, just having a bunch of

0:55:05.600 --> 0:55:09.320
<v Speaker 1>junk kind of floating around the planet in not ring form.

0:55:09.360 --> 0:55:11.240
<v Speaker 1>I mean, it could be like a lot of moons.

0:55:11.360 --> 0:55:14.480
<v Speaker 1>I suppose one candidate is this planet h I p

0:55:15.880 --> 0:55:19.200
<v Speaker 1>S eight F, which looks like it has a really

0:55:19.280 --> 0:55:22.359
<v Speaker 1>really huge radius, like nine times the radius of the Earth.

0:55:22.360 --> 0:55:25.360
<v Speaker 1>So either it's like a big styrofoam planet hardly filled

0:55:25.400 --> 0:55:28.520
<v Speaker 1>with anything, or it's a planet with an extensive ring

0:55:28.600 --> 0:55:31.399
<v Speaker 1>system that's blocking all of that light. And that's really

0:55:31.440 --> 0:55:33.840
<v Speaker 1>the only thing we can really think of. Is another planet,

0:55:33.880 --> 0:55:37.440
<v Speaker 1>Proxima Centauri C, which is a planet orbiting our immediate

0:55:37.480 --> 0:55:40.440
<v Speaker 1>neighbor Proximus Centauri. It has seven times the mass of

0:55:40.480 --> 0:55:43.640
<v Speaker 1>the Earth, but it's sort of weirdly bright and reflective,

0:55:44.000 --> 0:55:47.800
<v Speaker 1>which makes people think like perhaps it's surrounded by icy rings.

0:55:48.000 --> 0:55:49.839
<v Speaker 1>But as you can maybe get a sense for this

0:55:49.880 --> 0:55:53.439
<v Speaker 1>is very uncertain stuff. We're only just recently been able

0:55:53.480 --> 0:55:56.160
<v Speaker 1>to detect exo planets. We're getting better and better at it,

0:55:56.239 --> 0:55:58.879
<v Speaker 1>and soon we'll be doing things like studying the atmosphere

0:55:58.960 --> 0:56:01.160
<v Speaker 1>of exo planets, and this is sort of on that

0:56:01.200 --> 0:56:03.680
<v Speaker 1>list of things we're just beginning to be able to do.

0:56:03.920 --> 0:56:07.760
<v Speaker 1>It's kind of like physicists need to start to catch

0:56:07.840 --> 0:56:11.439
<v Speaker 1>up with jewelers, who can look at rings by using

0:56:11.440 --> 0:56:15.000
<v Speaker 1>a magnifying glass to see things really really tiny, but

0:56:15.120 --> 0:56:19.880
<v Speaker 1>physicists have to investigate their rings by looking at things

0:56:20.080 --> 0:56:22.799
<v Speaker 1>really really far away and blowing them up as much

0:56:22.840 --> 0:56:25.920
<v Speaker 1>as they can. Absolutely, and I expect that some of

0:56:25.920 --> 0:56:29.600
<v Speaker 1>those solar systems may have spectacular ring systems. I suspect

0:56:29.600 --> 0:56:31.920
<v Speaker 1>that when we get really nice images of them, you know,

0:56:31.920 --> 0:56:34.560
<v Speaker 1>if maybe from James Web or from the next generation

0:56:34.680 --> 0:56:37.320
<v Speaker 1>of space telescopes, we'll see things that blow our minds,

0:56:37.360 --> 0:56:40.480
<v Speaker 1>that make scientists say, what, that's impossible. You can't have

0:56:40.640 --> 0:56:43.319
<v Speaker 1>rings like that. That breaks all of our understandings. And

0:56:43.360 --> 0:56:46.439
<v Speaker 1>breaking our understanding is exactly the moment to learn about

0:56:46.480 --> 0:56:49.040
<v Speaker 1>the universe, to say, oh, well, it turns out we

0:56:49.040 --> 0:56:51.200
<v Speaker 1>didn't understand this as well as we thought we did.

0:56:51.239 --> 0:56:53.680
<v Speaker 1>We got to change our models. We have to add

0:56:53.719 --> 0:56:56.640
<v Speaker 1>something new to it, or develop some new idea for

0:56:56.719 --> 0:56:59.279
<v Speaker 1>how these things can form. And that's the exciting thing.

0:56:59.320 --> 0:57:02.319
<v Speaker 1>It's like opening a new book and being surprised by

0:57:02.360 --> 0:57:04.920
<v Speaker 1>what you find in Every one of these solar systems

0:57:05.200 --> 0:57:08.319
<v Speaker 1>will have surprises for us, things that we probably can't

0:57:08.320 --> 0:57:11.560
<v Speaker 1>imagine today. And isn't that the dream of every planetary

0:57:11.719 --> 0:57:16.920
<v Speaker 1>fashionista to wear rings so spectacular it makes scientists scratch

0:57:17.000 --> 0:57:21.800
<v Speaker 1>their heads and throw away all their textbooks. Exactly so

0:57:21.920 --> 0:57:25.160
<v Speaker 1>from Rings down here on Earth, wowing all of your friends,

0:57:25.360 --> 0:57:28.960
<v Speaker 1>two rings around the planets themselves, telling us something about

0:57:28.960 --> 0:57:31.640
<v Speaker 1>how those planets formed, and something about their history and

0:57:31.800 --> 0:57:34.800
<v Speaker 1>something about their future. Rings have a lot to tell

0:57:34.880 --> 0:57:37.440
<v Speaker 1>us about the nature of our lives, all right, Thanks

0:57:37.560 --> 0:57:41.000
<v Speaker 1>very much Katie for joining us on today's episode about Rings.

0:57:41.120 --> 0:57:43.400
<v Speaker 1>Was a lot of fun and we hope you all

0:57:43.520 --> 0:57:46.320
<v Speaker 1>ring in a wonderful day. Thank you very much for

0:57:46.440 --> 0:57:49.320
<v Speaker 1>listening and tune in next time. Hi, thanks for having me,

0:57:57.200 --> 0:57:59.960
<v Speaker 1>Thanks for listening, and remember that Daniel and Jorge Explain

0:58:00.000 --> 0:58:02.600
<v Speaker 1>in the Universe is a production of I Heart Radio

0:58:02.960 --> 0:58:05.600
<v Speaker 1>or more podcast from my Heart Radio. Visit the I

0:58:05.760 --> 0:58:09.440
<v Speaker 1>Heart Radio app, Apple Podcasts, or wherever you listen to

0:58:09.520 --> 0:58:12.240
<v Speaker 1>your favorite shows. Ye