Aug. 16, 2026

Exploring Moons with Atmospheres, Hot Jupiters, and the Mysteries of Black Holes

Exploring Moons with Atmospheres, Hot Jupiters, and the Mysteries of Black Holes

Sponsor Link: This Q&A episode of Space Nuts is brought to you with the support of https://www.nordvpn.com/spacenuts. When you decide to get serius about your security online, do what we did and get NordVPN. We have a special deal for you too,...

Sponsor Link:
This Q&A episode of Space Nuts is brought to you with the support of NordVPN. When you decide to get serius about your security online, do what we did and get NordVPN. We have a special deal for you too, chck out the details at www.nordvpn.com/spacenuts

In this episode of Space Nuts, hosts Andrew Dunkley and Professor Fred Watson delve into a captivating Q&A session, tackling a range of intriguing questions from listeners. From the possibility of moons having atmospheres to the mysteries surrounding hot Jupiters and the fascinating realm of black holes, this episode promises to ignite your curiosity about the cosmos.
Key topics include:
- Chris from Exmouth wonders if moons can have atmospheres and if they can share these with their parent planets, leading to a discussion on Titan and Pluto's unique characteristics.
- An anonymous listener poses a thought-provoking question about 'secret astronomy' and the potential for military satellite technology to advance our understanding of the universe.
- Fenton from Minnesota asks about the likelihood of rocky planets existing in solar systems with hot Jupiters, prompting a discussion on planetary migration and the diversity of solar systems.
- Ed raises a classic black hole question regarding the merger of black holes and the concept of mass escaping, leading to an exploration of gravitational waves and their implications.
Join Andrew and Fred Watson as they navigate these fascinating topics, providing insights and sparking further exploration into the wonders of space.
00:00 01:18 04:13 05:37 11:35 16:34 20:35 27:11 31:31

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WEBVTT

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Andrew Dunkley: Hello again and thank you for joining us on

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yet another episode of Space Nuts. I don't

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know what we're up to.652.

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Blimey. And we only started yesterday.

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Uh, coming up in this Q and A episode, we

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will be answering questions about, uh, moons

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with atmospheres, secret

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astronomy. This is a fascinating question.

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Uh, we've also got, uh, a question about hot

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Jupiters. We've talked about them before. And

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a very rare, never before

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asked black hole question that's

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coming up in this Q and A edition of space

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nuts. 15 seconds.

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Professor Fred Watson: Guidance is internal. 10,

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9, ignition sequence start. Uh,

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space nuts. 5, 4, 3, 2. 1, 2,

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3, 4, 5, 5, 4, 3, 2, 1.

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Andrew Dunkley: Space nuts.

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Professor Fred Watson: Astronauts report it feels good.

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Andrew Dunkley: Joining us again to resolve all of that is

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Professor Fred Watson Watson, astronomer at

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large. Hi, Fred Watson.

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Professor Fred Watson: Hello, Andrew. How are you? Good to see you

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again.

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Andrew Dunkley: I'm as well as I was the last time you saw

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me.

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Professor Fred Watson: Yes. All those years ago. That's right, yeah.

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Andrew Dunkley: Minutes or seconds, whichever comes first.

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Uh, we've got some good questions today and,

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uh, I thought we might just get straight into

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it if you're, uh, ready to.

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Oh, no, I've got an announcement.

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Professor Fred Watson: Oh, yes, Better do that then.

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Andrew Dunkley: It's a bit of shameless self promotion. I've

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finally released my science fiction trilogy.

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Yes, it's out there. Um, I'm just putting the

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final touches on a few bits and bobs. But the

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ebook is out. Uh, the paperback

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should be out by the time you hear this.

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Um, unless you're watching us live on

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YouTube.

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Professor Fred Watson: Hello.

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Andrew Dunkley: It's called the Human Epoch.

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M which I did look up to see if there are

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any other science fiction books with that

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name, and there are not. So the human

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epoch, parts 1, 2 and 3. I released them all

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at once.

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Andrew Dunkley: Oops.

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Andrew Dunkley: I, uh, nearly released the microphone. Yeah,

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all at once. I thought, I'm gonna write the

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whole thing and release it as a batch rather

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than write one book and then

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release it and then make people wait a year.

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Now the whole bang lot's out there already

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on its way.

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Professor Fred Watson: Seasons one, two and three.

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Andrew Dunkley: Yes, exactly. I hope people enjoy it. Can't

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wait to get the feedback. Good, bad or

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indifferent. So the Human Epoch.

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Professor Fred Watson: Look for it.

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Andrew Dunkley: Uh, and you should be able to order it from

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bookshops. I don't know. I don't know how it

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works. Um, but you know, looking

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at the cost of printing and the

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sharing of spoils, um, if you

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sell a book for 20 bucks these days, you

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might get two or three dollars out of that.

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It's a Tough industry.

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Professor Fred Watson: Very. Yeah.

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Andrew Dunkley: I mean, you've really got to sell

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m tens of thousands of books to even scratch

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the surface. Which I have not done.

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Professor Fred Watson: Yeah, neither have I.

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Andrew Dunkley: No, no. But anyway, I

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thought I'd give it a mention. I've mentioned

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that I was writing it times. I thought I

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might as well people. It's out there. So

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there. That's, um, done.

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Professor Fred Watson: So you're not emulating Douglas Adams with a

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trilogy in four parts?

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Andrew Dunkley: No, but, you know, I

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might. Yeah, I might continue the

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storey because I became very. Isn't.

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Andrew Dunkley: Uh.

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Andrew Dunkley: I don't know if this happens to other

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authors. I'm sure it does.

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Professor Fred Watson: Oh, there you are.

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Andrew Dunkley: It happens to Earth.

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Professor Fred Watson: Yes, it does. He's a bit late.

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Andrew Dunkley: We could have used him in the last episode.

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Professor Fred Watson: We could. That's right. With the dogs.

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Andrew Dunkley: Um, you get a bit attached to some of

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the characters you create.

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Professor Fred Watson: Yes. I believe that happens when you write

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fiction.

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Andrew Dunkley: Um, the main character in this trilogy,

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um, I've come to adore. I really. I love his

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attitude. That's all I say.

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Professor Fred Watson: Okay. All right.

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Andrew Dunkley: Okay. He's

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a different kind of character.

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Professor Fred Watson: Is he based on anybody real?

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Andrew Dunkley: No, I made him up. Um, and I made him

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Canadian. Uh, I don't know why. I just did.

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Professor Fred Watson: I just thought Canadian.

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Andrew Dunkley: Canadians never get much of a mention in

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science fiction novels. So I thought, I'll

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make my hero a Canadian.

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Professor Fred Watson: Good on you. Yeah.

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Andrew Dunkley: All right.

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Professor Fred Watson: Before we do that, I better just go and see

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what's, um. Because I'm home alone at the

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moment. Jordy, I won't be a sec.

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All right?

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Andrew Dunkley: Okay. This doesn't happen very often. He

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could have done that while I was spruiking

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the book, you know, because, um, that would

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have been a nice filler. But now he's

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just left me swinging in the breeze.

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Which, um, happens occasionally.

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This used to happen on radio. I remember

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once, uh, years ago, um, we were

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expecting some guests, so I played an

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appropriate song. I think they were circus

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performers. And I played

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circus by Britney Spears in the hope that

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they would actually arrive while the song was

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on. And, uh, I got lucky. They

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walked in the door just as it was finishing.

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So I got the interview on air in time. It's

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sometimes a bit scary like that. Anyway,

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welcome, uh, back, Fred Watson. Is Jordie

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okay?

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Professor Fred Watson: Yes. I don't know what was causing

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the howling. Uh, ruckus.

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Andrew Dunkley: A butterfly, probably.

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Professor Fred Watson: Could have been. Honestly, it's that level

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that sets him off. You know, a leaf

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moves two, uh, hundred metres away across

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the forest and off he goes. That's right.

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Andrew Dunkley: He could probably use a GPS collar.

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Professor Fred Watson: There were times when he could use a muzzle,

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I think to speak.

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Andrew Dunkley: Um, now let's get into some questions. I

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think that's why we're here.

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Professor Fred Watson: Oh, I suppose it is, yes. Yes.

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Andrew Dunkley: Um, so first question comes from Chris

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in Exmouth in the uk. Just

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wondering, could a moon ever have

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an atmosphere and is it possible for a moon

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to be close enough to a planet to share

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an atmosphere? Really enjoy the show. Thank,

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uh, you Chris for sending that in. Um,

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look, we already know in our solar system

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there are moons with atmospheres and I do

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believe they do share their stuff with their

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home planets, some of them.

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Professor Fred Watson: Uh, correct. That's right. Although

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it's sort of um, probably not quite

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what Chris has, his mind. So yes. Uh, I mean

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the classic example is Saturn's moon Titan,

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that has a very thick atmosphere,

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um, atmospheric pressure I think one and a

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half times that of the Earth. It's a dense

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atmosphere and um, also

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opaque because it's rich in um,

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ah, hydrocarbons. The same

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stuff that makes smog in a city. Uh, is why

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we can't see through Titan's atmosphere. So

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yes, a moon can have an atmosphere, um,

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but you can't have a situation where

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uh, you had a planet and a

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moon which were sort of embedded in a much

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larger dense atmosphere. Uh,

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and that's because the, you basically

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slow down the moon as it orbits the planet,

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uh, and it doesn't last very long. Uh, in

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fact that's what brings satellites down uh,

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from orbit. Low Earth orbit above the Earth.

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They are slowed down by the Earth's

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atmosphere, even though it's very tenuous up

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there. And uh, nevertheless it slows them

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down and they fall deeper into the atmosphere

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and the deceleration continues.

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But the example that you've mentioned is the

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one that came to mind when I read this

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question as well. Uh, which is

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the dwarf planet Pluto, uh,

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which has a large moon. It's uh,

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about half the size of Pluto actually. It's

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called Charon, uh, or Charon, not

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Charon. Some people call it Charon.

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Andrew Dunkley: They do.

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Professor Fred Watson: Charon, Shaz for short.

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Shaza. Yeah, um,

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it's uh, it's a large moon, as

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I said, half the size of Pluto.

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Uh, and so they are in a sense a

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binary dwarf planet system because

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they orbit around a point which

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is outside the body of Pluto, uh,

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which is the kind of definition of a binary

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system, something orbiting around a common

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centre of gravity. Uh, so you've

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got that ah, unusual situation to start

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with, but um,

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it Appears that because of that

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geometry,

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the atmosphere of

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Pluto, which is very, very thin, but it is

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there. I was once helping a project that

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measured the atmosphere of Pluto not from

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space, but by Pluto passing in front of a

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star as observed with the Anglo Australian

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telescope. We could see it dimmed gradually,

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the light of the star rather than just

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switching off as it would have been if

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there'd been no atmosphere. So, uh, that

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atmosphere is mostly nitroge gas,

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uh, or the part that's

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escaping. Uh, and

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apparently it is basically

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captured by Charon. There's

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this flow of the nitrogen

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from Pluto to its dwarf

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planet companion. Um,

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there's probably something similar happens

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with the Earth and Moon, but very, very much

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less intense. Uh, there's probably a

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bit of gas transfer, uh, from

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the Earth, uh, to the Moon. Given that

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the pressure of the Earth's atmosphere

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doesn't just stop suddenly, it falls away

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very gradually. And in fact there are some of

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the molecules of the Earth's atmosphere that

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are out at the distance of the Moon. Uh, so

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they probably do exchange, you

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know, some low levels of gas, but

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not very much. And it is, yes, it's

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a different situation from perhaps what Chris

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had in mind with an atmosphere, with a planet

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and its moon both orbiting within it.

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Andrew Dunkley: Yeah, I understand what he was saying. Uh,

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and as you suggested, um, it

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would be an impossible situation. Although

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we do see, I think around the gas giants,

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some of those planets, particularly the ice

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worlds, do shed some of their

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material, which is picked up by

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um, um, the gas giant, I think.

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Is it Enceladus?

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Professor Fred Watson: Uh, yeah, that forms, um, that's correct.

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So that's solid matter. Actually it's the

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ice crystals that come from Enceladus

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Ocean. They form, uh, Saturn's E

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ring, uh, which is a very, um,

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non dense, very, uh, rarefied ring.

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One. I think it's the outermost ring of

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Saturn. Um, and it's basically,

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uh, the orbit of uh, Enceladus is embedded in

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that. So, yes, that's a sort of similar sort

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of situation. Yeah, that's right.

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Andrew Dunkley: It's not sharing atmosphere, but it's sharing

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material in a way.

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So, uh, the answer to both of your points,

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Chris, is definite. Yes, um,

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but no, in terms of them both sharing the

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same atmosphere. Hold us,

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Bolus. As we say so. Yeah, but great

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question, uh, Christian Exmouth. Where's

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Exmouth, Fred Watson?

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Professor Fred Watson: Uh, down in Devon. It's a lovely part of the

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country. Uh, and um, it's

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uh, not far from Exeter. The River X

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runs through both of them, as you'd expect.

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Andrew Dunkley: Uh, and the River X owned by Elon

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Musk.

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Professor Fred Watson: Probably, yes. It's spelled

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slightly differently from Elon Musk's X, but

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yes, probably still the same thing.

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Andrew Dunkley: Thanks for the question, Chris.

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Next question comes from, uh, somebody

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who's keeping their name a secret. And it's,

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uh, it's about secret astronomy. Oh, hang

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on, That's. I've got to change pages. Here we

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go. Here we go.

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Professor Fred Watson: I have a question about secret

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astronomy. We know that gamma

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ray bursts were first detected by spy

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satellites looking for nuclear testing. We

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know that satellites use star tracking and

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star catalogues for calculating their

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position. And we, uh, know that the Nancy

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Grace Roman launching, hopefully in August,

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uses, um, is built out of a,

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um, spy satellite the National Reconnaissance

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Office, the US Uh spy satellite agency,

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donated to NASA because they weren't going to

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launch it. They donated two and only one is

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being used yet. And we know that the Space

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Force released, um, a bunch of observational

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data around bolides to, um, help with

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planetary defence and asteroid detection

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and understanding. So by their nature, spy

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satellites tend to point at the Earth. Um,

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but obviously they push into a lot of

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astronomy and astronomy adjacent, um, things.

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I just wondered if you could speculate, given

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their budgets and um,

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constantly improving capabilities, where they

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might be ahead of public astronomy or running

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into things that, um. Uh,

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yeah, it might be pretty interesting in a few

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years. Thank you so much.

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Andrew Dunkley: Thank you for the question.

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Professor Fred Watson: Um,

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Andrew Dunkley: yeah, I don't know who that was, but, um.

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That's okay. Happens from time to time. But

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interesting, uh, question, Fred Watson.

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Professor Fred Watson: Really, it's, uh, not just an interesting

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question, but a very well posed one as well.

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Because everything our anonymous questioner

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said is true. Uh, and so we are being

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invited to speculate on what, what else

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might be up and running. Uh, we didn't know

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for a long time that there were two more

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Hubble telescopes, uh, because,

329
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you know, the company kept their. Built

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it. I think it might have been perkinelmer.

331
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I'm, um, not sure. But they kept their cards

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very close to their chest, uh, in terms

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of, uh, the existence of the Hubble

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telescope. But it turned out subsequently we

335
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found out there were two more built for

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surveillance. Um, something else

337
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that did find its way into astronomy

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that was originally secret was, um,

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President Reagan's Star wars technology,

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uh, which, um, required

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adaptive optics. And those are optical

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surfaces that change in response to, um,

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basically things like, um,

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uh, scintillation in the atmosphere or

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twinkling for a star. So that adaptive

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optics technology is now used very commonly

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in astronomy. Uh, it's not Used

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here in Australia we don't have a

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site that is naturally good enough um,

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to be able to compensate for um,

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this um, atmospheric turbulence. Whereas some

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of the better sites in the world like Mauna

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Kea in Hawaii and Ceropa

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Paranal, uh, in Chile, they do. And

355
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so they use um, adaptive optics

356
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very, very uh, commonly for their work.

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Basically allows you to take out the

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twinkling of a star which is something that

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ruins the images as you see them through

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telescopes. Uh and um,

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as I said, came from Star wars technology.

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Uh, that technology by the way, this is uh.

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Not really along the lines of the question

364
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but uh. It's leapfrogged as well from

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astronomy into um,

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ophthalmology. So uh, people are now using

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adaptive optics to compensate for

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the turbulence inside your eye

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when they're doing sort of retinoscopy and

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things like that. Uh, so that adaptive optics

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technology is now uh, gone from

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defence through astronomy and is

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now um, being developed for uh,

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health reasons, which is very, very good.

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Andrew Dunkley: Don't know if it's quite the same thing but

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my optometrist was telling me they've

377
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invented a new um, kind of

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um, lens that replaces human

379
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lens that can now

380
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do the same thing as a human lens. Like okay,

381
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when you have a cataract operation they

382
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replace the human lens. That's all fogged up

383
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with generally a plastic lens of some

384
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kind. But it was a fixed lens. It could only

385
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do one thing. They've now advanced the

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technology to the point where they can put a

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lens in that will be able to

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be controlled by your brain and give you

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various focal lengths.

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Professor Fred Watson: Yeah.

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Andrew Dunkley: Which I think is amazing.

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Professor Fred Watson: It's what you. What your eye naturally does.

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It's called accommodation you that the eye

394
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accommodates to different distances by

395
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changing the shape of the lens. Yeah, yeah.

396
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So um, that's pretty. Yes. Quite remarkable

397
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and um. Would be a real breakthrough for

398
00:16:31.730 --> 00:16:34.450
um. You know, for vision, uh, for poor

399
00:16:34.450 --> 00:16:34.810
vision.

400
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Anyway, we've strayed off the topic here. We

401
00:16:36.490 --> 00:16:38.340
have a bit and uh.

402
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Andrew Dunkley: I do, I'm sure never happens usually.

403
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Professor Fred Watson: I'm sure that um. Uh. Our uh.

404
00:16:45.750 --> 00:16:47.930
Listener is on the money suggesting that

405
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there are technologies that are being used

406
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in secrets, um.

407
00:16:53.650 --> 00:16:53.870
Professor Fred Watson: Ah.

408
00:16:53.870 --> 00:16:56.290
Professor Fred Watson: Or restricted environments.

409
00:16:56.770 --> 00:16:59.730
Uh, that would be of great

410
00:16:59.730 --> 00:17:02.670
value for astronomy. I uh.

411
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Guess the kind of thing that comes to mind is

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quantum detectors and. And things of that

413
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sort. Um, there is no. I don't think there's

414
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any equivalent uh, for example in the

415
00:17:14.210 --> 00:17:16.690
field of gravitational wave astronomy. I

416
00:17:16.690 --> 00:17:18.050
don't think there's anything that the

417
00:17:18.050 --> 00:17:19.850
military are doing that could feed into that.

418
00:17:19.850 --> 00:17:21.730
Although quantum optics are being used in

419
00:17:21.730 --> 00:17:24.690
that now. So, um, I

420
00:17:24.690 --> 00:17:26.930
suspect it's in, you know, in relation to the

421
00:17:26.930 --> 00:17:29.440
tools that are developed for, uh,

422
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our observations. Um,

423
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we owe infrared detectors,

424
00:17:35.650 --> 00:17:37.770
the things that see redder than red light or

425
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heat radiation. We owe them to the military.

426
00:17:40.210 --> 00:17:43.110
That's a spin off from military work. Um,

427
00:17:43.110 --> 00:17:46.050
I do remember, uh, one of the first

428
00:17:46.050 --> 00:17:48.250
infrared instruments on the Anglo Australian

429
00:17:48.250 --> 00:17:51.010
telescope. When it was being delivered.

430
00:17:51.310 --> 00:17:53.730
Uh, I think,

431
00:17:54.030 --> 00:17:56.450
um, the detector came under armed guard

432
00:17:56.450 --> 00:17:58.810
almost. It wasn't quite like that. But there

433
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was a lot of hoops to jump through when this

434
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detector was delivered. Because it had to be

435
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certain not to stray into the hands

436
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of certain foreign nations who the

437
00:18:09.370 --> 00:18:12.250
Americans who developed this detector didn't

438
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want, uh, them to get hold of.

439
00:18:15.370 --> 00:18:17.930
So those technologies do eventually

440
00:18:19.050 --> 00:18:21.250
kind of sprinkle down to astronomy where the

441
00:18:21.250 --> 00:18:24.010
poor relations in that regard, uh, although

442
00:18:24.010 --> 00:18:25.930
we do push the limits perhaps more than

443
00:18:25.930 --> 00:18:28.250
anybody else, uh, in technology.

444
00:18:29.210 --> 00:18:31.210
So, um, yes,

445
00:18:31.850 --> 00:18:34.020
I, I don't have any

446
00:18:35.300 --> 00:18:38.030
definite, um, speculations, uh,

447
00:18:38.030 --> 00:18:40.540
except to say that nothing would

448
00:18:40.540 --> 00:18:42.580
surprise me in that regard

449
00:18:43.380 --> 00:18:44.180
when it comes.

450
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Andrew Dunkley: I'm not a conspiracy theorist, but I do

451
00:18:47.940 --> 00:18:50.340
believe there's a heck of a lot going on up

452
00:18:50.340 --> 00:18:53.260
there that we do not and probably will

453
00:18:53.260 --> 00:18:56.260
not know about. Um, and

454
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I truly believe that the technology

455
00:18:59.930 --> 00:19:02.810
available today in space and on

456
00:19:02.810 --> 00:19:05.450
the planet, um, in those

457
00:19:05.530 --> 00:19:08.410
dark corners of government buildings

458
00:19:08.490 --> 00:19:10.730
is far, far more advanced than we

459
00:19:11.450 --> 00:19:14.049
could possibly imagine. I think given what

460
00:19:14.049 --> 00:19:16.730
we've got access to in a domestic sense in

461
00:19:16.730 --> 00:19:18.570
the public arena today,

462
00:19:19.650 --> 00:19:22.290
uh, what's been developed already behind

463
00:19:22.290 --> 00:19:25.170
closed doors that we're unaware of. And

464
00:19:25.170 --> 00:19:27.560
it's probably up. They're circling the planet

465
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as we speak.

466
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Professor Fred Watson: Yeah, I think it works both ways though,

467
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because I think, um, we're now

468
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seeing, uh, the military adopting

469
00:19:37.880 --> 00:19:39.880
what would have been thought of as commercial

470
00:19:39.880 --> 00:19:41.940
products before. Uh,

471
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and that's happened certainly in Ukraine.

472
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There's been an adaptation of

473
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all sorts of commercial products for

474
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military purposes. Um, so

475
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what I guess I'm saying is that the

476
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technology that we use every day is not

477
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as far removed from what the military use

478
00:20:01.700 --> 00:20:04.420
as it would have been 20 or 30 years ago.

479
00:20:05.150 --> 00:20:08.140
Uh, I think that's probably fair to say, but

480
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that's me going out on a limb. And who can

481
00:20:09.940 --> 00:20:10.820
prove me wrong?

482
00:20:11.620 --> 00:20:14.550
Andrew Dunkley: Well, that's a good point too. Yeah, it's a,

483
00:20:14.550 --> 00:20:16.060
uh, really interesting question. Thank you

484
00:20:16.060 --> 00:20:18.700
for sending it in. This is Space Nuts Andrew

485
00:20:18.700 --> 00:20:20.420
Dunkley here with Professor Fred Watson

486
00:20:20.420 --> 00:20:20.980
Watson.

487
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Professor Fred Watson: I believe that this nation should commit

488
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itself to achieving the goal

489
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before this decade is out of landing A man

490
00:20:30.940 --> 00:20:33.020
on the moon and returning him safely

491
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Andrew Dunkley: to the Earth face nuts.

492
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Another audio question from Fred.

493
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Andrew Dunkley: Hi, this is Fred calling you from St. Paul,

494
00:20:41.780 --> 00:20:44.540
Minnesota in the US I have a question for

495
00:20:44.540 --> 00:20:47.420
you regarding the solar systems that contain

496
00:20:48.050 --> 00:20:50.620
uh, so called hot Jupiter planets, those

497
00:20:50.620 --> 00:20:53.180
which are very close, ah, around their

498
00:20:53.180 --> 00:20:55.930
suns. Is it reasonable at all to

499
00:20:55.930 --> 00:20:58.010
expect that they will have

500
00:20:58.570 --> 00:21:00.890
smaller planets, rocky planets,

501
00:21:01.370 --> 00:21:04.370
or are there good reasons that

502
00:21:04.370 --> 00:21:06.130
come to mind where that should not be the

503
00:21:06.130 --> 00:21:08.970
case? Um, I'd uh, appreciate hearing

504
00:21:09.130 --> 00:21:12.130
your theories on this, uh, what the variables

505
00:21:12.130 --> 00:21:14.730
would be in this and I of course enjoy

506
00:21:15.050 --> 00:21:17.930
listening to your show. Thank you very much.

507
00:21:18.330 --> 00:21:19.050
Goodbye.

508
00:21:19.450 --> 00:21:22.010
Andrew Dunkley: Thank you Fred. Uh, Fred's one of our semi

509
00:21:22.010 --> 00:21:24.430
regular sender inners and um,

510
00:21:24.890 --> 00:21:27.350
he's always got a very interesting question

511
00:21:27.350 --> 00:21:30.030
in mind. Um, so uh, yeah, I'm

512
00:21:30.030 --> 00:21:32.390
guessing that what he is asking is if you've

513
00:21:32.390 --> 00:21:35.220
got a solar system with hot Jupiters, uh,

514
00:21:35.220 --> 00:21:38.070
that are orbiting their parent star in

515
00:21:38.070 --> 00:21:41.030
close proximity, could those systems

516
00:21:41.030 --> 00:21:43.550
have rocky planets further out? Now, uh, the

517
00:21:43.550 --> 00:21:45.950
downside of exoplanet detection is rocky

518
00:21:45.950 --> 00:21:47.990
planets are very hard to find at a distance.

519
00:21:47.990 --> 00:21:50.670
You generally find the gas giants

520
00:21:50.670 --> 00:21:53.600
fast or first. Um,

521
00:21:53.910 --> 00:21:55.830
we do know there are a lot of hot Jupiters

522
00:21:55.830 --> 00:21:57.430
out there because we've talked about them.

523
00:21:58.150 --> 00:22:00.130
Um, but uh, yeah,

524
00:22:01.170 --> 00:22:04.010
uh, what's the likelihood that that's a

525
00:22:04.010 --> 00:22:06.970
common thing? Um, not that there's

526
00:22:06.970 --> 00:22:09.930
anything absolutely common about anything you

527
00:22:09.930 --> 00:22:12.210
find when you start looking around at other

528
00:22:12.210 --> 00:22:13.090
solar systems?

529
00:22:13.409 --> 00:22:16.330
Professor Fred Watson: Yeah, that's exactly right. Our solar

530
00:22:16.330 --> 00:22:18.250
system is very neat and tidy compared with

531
00:22:18.250 --> 00:22:20.930
most of the other ones that we've detected.

532
00:22:20.930 --> 00:22:23.530
But you're absolutely right Andrew. Um, the

533
00:22:23.530 --> 00:22:25.830
rocky planets are the, the tricky ones to

534
00:22:25.830 --> 00:22:28.190
observe. And so it might well be that

535
00:22:28.990 --> 00:22:31.030
what we're seeing is effectively a selection

536
00:22:31.030 --> 00:22:33.630
effect. We're selecting the easiest ones,

537
00:22:34.190 --> 00:22:37.070
uh, to discover. Uh, and that's why we see a

538
00:22:37.070 --> 00:22:40.030
lot of hot Jupiters without any evidence

539
00:22:40.030 --> 00:22:42.910
of rocky planets in the same solar systems,

540
00:22:43.870 --> 00:22:46.710
I think, and I haven't looked at this for

541
00:22:46.710 --> 00:22:49.550
some time but um, one of the ideas

542
00:22:49.710 --> 00:22:52.250
for why we've got this

543
00:22:52.250 --> 00:22:55.250
situation with hot Jupiters is basically

544
00:22:56.210 --> 00:22:59.170
a planetary migration. This is where planets

545
00:22:59.170 --> 00:23:01.970
change their positions in the solar system.

546
00:23:02.760 --> 00:23:04.330
Uh, and that might have happened to some

547
00:23:04.330 --> 00:23:07.250
extent in our solar system, but not

548
00:23:07.810 --> 00:23:10.690
in um, a really sort

549
00:23:10.690 --> 00:23:13.570
of existential way. Not in a way that will

550
00:23:13.650 --> 00:23:15.890
totally alter the shape of the solar system

551
00:23:16.130 --> 00:23:17.930
because we've got four rocky planets which

552
00:23:17.930 --> 00:23:20.810
are the innermost ones and they exist within

553
00:23:20.810 --> 00:23:23.320
a zone where um,

554
00:23:23.540 --> 00:23:26.300
water exists as a

555
00:23:26.300 --> 00:23:29.140
gas, whereas beyond the orbit of Mars,

556
00:23:29.220 --> 00:23:31.500
and we sometimes call that the frost line or

557
00:23:31.500 --> 00:23:34.100
the ice line water exists

558
00:23:34.780 --> 00:23:37.619
uh, as ice and that ice is what

559
00:23:37.619 --> 00:23:40.260
has allowed the gas giants to grow

560
00:23:40.820 --> 00:23:43.700
to the size that they have because the ice

561
00:23:43.700 --> 00:23:46.580
basically collects and uh, the

562
00:23:46.660 --> 00:23:48.680
planets absorb it. So you've got ah,

563
00:23:50.100 --> 00:23:52.580
not just a massive rock being formed but ice

564
00:23:52.580 --> 00:23:55.540
as well. And then you end up with a gas

565
00:23:55.540 --> 00:23:58.340
giant planet. Uh so the four gas giants

566
00:23:58.340 --> 00:24:00.300
we think are ah, like that because they're

567
00:24:00.300 --> 00:24:03.220
outside the frost line. Now if you've got

568
00:24:03.220 --> 00:24:05.940
planetary migration taking place then

569
00:24:06.180 --> 00:24:08.620
some of those planets could wander in to the

570
00:24:08.620 --> 00:24:10.740
inner solar system. Uh and

571
00:24:11.700 --> 00:24:14.700
it may essentially leave your solar

572
00:24:14.700 --> 00:24:16.940
system looking like some of the ones that we

573
00:24:16.940 --> 00:24:19.820
see with a hot Jupiter orbiting very close

574
00:24:19.820 --> 00:24:22.160
to Paris star. But also

575
00:24:22.480 --> 00:24:24.720
perhaps with some rocky planets lingering

576
00:24:25.160 --> 00:24:27.760
uh, moaning around or moping around

577
00:24:28.280 --> 00:24:31.200
uh, where they've been uh, projected

578
00:24:31.200 --> 00:24:33.280
to by the rearrangement of the planets

579
00:24:33.600 --> 00:24:35.760
because some of them could be ejected by

580
00:24:35.840 --> 00:24:38.400
planetary migration. If you've got your gas

581
00:24:38.400 --> 00:24:40.680
giant wanders too near your little rocky

582
00:24:40.680 --> 00:24:42.520
planet, it's going to boot it out the solar

583
00:24:42.520 --> 00:24:45.360
system altogether. Uh but um, I

584
00:24:45.360 --> 00:24:47.850
suspect that there will be solar systems uh,

585
00:24:48.340 --> 00:24:50.840
ah that will turn out to have both hot

586
00:24:50.840 --> 00:24:53.020
Jupiters and rocky planets. And as our

587
00:24:54.060 --> 00:24:56.300
um, technology improves and allows us to

588
00:24:56.300 --> 00:24:59.220
detect these things uh, at lower masses, I

589
00:24:59.220 --> 00:25:01.420
think we'll be finding them as well. So um,

590
00:25:01.420 --> 00:25:03.300
watch this space phantom. That's the bottom

591
00:25:03.300 --> 00:25:03.740
line there.

592
00:25:04.220 --> 00:25:06.060
Andrew Dunkley: Theo was a wandering planet.

593
00:25:06.540 --> 00:25:08.540
Professor Fred Watson: Yes, that's right. Theo wandered into the

594
00:25:08.540 --> 00:25:11.420
Earth back in the uh, literally

595
00:25:11.500 --> 00:25:14.380
late 4,000 B.C. yeah,

596
00:25:15.260 --> 00:25:17.540
4,000 million BCS. I beg your pardon. Four

597
00:25:17.540 --> 00:25:18.780
billion. Yeah.

598
00:25:19.570 --> 00:25:22.290
Andrew Dunkley: I think um, the train of thought these days

599
00:25:22.290 --> 00:25:25.170
is that uh, in terms of solar systems,

600
00:25:25.370 --> 00:25:28.370
um, just about every star has at least got

601
00:25:28.370 --> 00:25:31.250
one planet. Um, that's based

602
00:25:31.250 --> 00:25:33.890
on an average assumption. But um,

603
00:25:34.530 --> 00:25:36.790
it also stands to reason that uh,

604
00:25:37.250 --> 00:25:40.250
solar systems are as many and as varied as

605
00:25:40.250 --> 00:25:43.170
there are stars in the sky. Ours

606
00:25:43.490 --> 00:25:45.290
which has the four rocky planets, then the

607
00:25:45.290 --> 00:25:47.890
gas giants as you move out and then the dwarf

608
00:25:47.890 --> 00:25:50.610
planets beyond that um, ours

609
00:25:50.610 --> 00:25:53.330
seems to be quite different

610
00:25:53.330 --> 00:25:54.050
from most.

611
00:25:54.690 --> 00:25:56.930
Professor Fred Watson: It does, that's what I meant. It's very neat

612
00:25:56.930 --> 00:25:59.250
and tidy compared with uh, what we see

613
00:25:59.250 --> 00:26:02.210
elsewhere. Um, certainly

614
00:26:02.610 --> 00:26:05.530
if you were on uh, the planet of

615
00:26:05.530 --> 00:26:08.410
a star 100 light years away, our rocky

616
00:26:08.410 --> 00:26:10.250
planets would be very difficult to detect.

617
00:26:10.250 --> 00:26:12.410
And you just think, you'd probably think all

618
00:26:12.410 --> 00:26:15.410
it had was Jupiter, uh because you'd be

619
00:26:15.410 --> 00:26:17.850
able to detect Jupiter relatively easily. If

620
00:26:17.850 --> 00:26:19.630
it passed in front of the sun it would, would

621
00:26:19.630 --> 00:26:22.470
produce a 1% drop in the um, light

622
00:26:22.470 --> 00:26:25.310
of the sun. And that's easy to

623
00:26:25.310 --> 00:26:28.110
measure. So yes. So um,

624
00:26:28.170 --> 00:26:30.790
uh is the future

625
00:26:31.270 --> 00:26:33.510
of our solar system, one that does involve

626
00:26:33.510 --> 00:26:36.430
planetary migration. Um, it doesn't seem

627
00:26:36.430 --> 00:26:38.310
to be. The planets seem to be in very, very

628
00:26:38.310 --> 00:26:40.870
stable orbits. And maybe that's just

629
00:26:40.870 --> 00:26:42.470
something to do with the geometry of the

630
00:26:42.470 --> 00:26:44.830
solar system itself. But maybe it's something

631
00:26:44.830 --> 00:26:47.630
to do also with why intelligent

632
00:26:47.630 --> 00:26:49.390
life has evolved on one of those planets.

633
00:26:49.390 --> 00:26:51.280
Because we've had this idea long term

634
00:26:51.280 --> 00:26:53.640
stability over many millions of years,

635
00:26:54.520 --> 00:26:54.800
which

636
00:26:54.800 --> 00:26:56.640
Andrew Dunkley: is why it's going to be near impossible to

637
00:26:56.640 --> 00:26:59.240
find another intelligent, communicative

638
00:26:59.400 --> 00:27:02.160
civilization. Because, um, the circumstances

639
00:27:02.160 --> 00:27:03.000
are unique.

640
00:27:03.240 --> 00:27:05.360
Professor Fred Watson: Could be, probably, yeah, could be almost

641
00:27:05.360 --> 00:27:06.800
unique. Yes.

642
00:27:06.800 --> 00:27:07.720
Andrew Dunkley: Thank you, Fred.

643
00:27:10.280 --> 00:27:11.720
Professor Fred Watson: Roger, you're allowed to clear here.

644
00:27:11.720 --> 00:27:14.280
Andrew Dunkley: Also space nuts. Our final question

645
00:27:14.520 --> 00:27:17.040
comes from Ed. Now this is not dissimilar to

646
00:27:17.040 --> 00:27:19.400
a question we had recently, but it's not

647
00:27:19.400 --> 00:27:21.960
quite the same either. Uh, we believe

648
00:27:22.580 --> 00:27:25.060
that nothing can escape from a black hole.

649
00:27:25.060 --> 00:27:27.900
And yet when two black holes merge, the mass

650
00:27:27.900 --> 00:27:30.260
of the surviving black hole is significantly

651
00:27:30.260 --> 00:27:31.980
less than the combined mass of the two

652
00:27:31.980 --> 00:27:34.740
merging black holes. It would appear this

653
00:27:34.740 --> 00:27:36.780
missing mass, which I understand is converted

654
00:27:36.780 --> 00:27:39.580
to gravitational waves, has to come from the

655
00:27:39.580 --> 00:27:42.300
black holes, hence energy. Matter does

656
00:27:42.300 --> 00:27:44.820
escape from black holes. Is this

657
00:27:44.980 --> 00:27:47.740
wrong? Ed asks. Hello, Ed, thanks for the

658
00:27:47.740 --> 00:27:50.140
question. Uh, black hole questions,

659
00:27:50.140 --> 00:27:52.860
Fred Watson. It's not. A week goes by we

660
00:27:52.860 --> 00:27:54.090
don't get a black hole.

661
00:27:54.240 --> 00:27:56.200
Professor Fred Watson: A great one, though. It's a good question

662
00:27:56.200 --> 00:27:59.200
that Ed's raised. Um, so it's.

663
00:27:59.440 --> 00:28:02.400
Yes, the uh, gravitational radiation

664
00:28:03.200 --> 00:28:03.600
is

665
00:28:06.640 --> 00:28:07.760
quite different from

666
00:28:09.540 --> 00:28:11.920
uh, the electromagnetic radiation that's

667
00:28:12.160 --> 00:28:14.280
coming from a black hole which does get

668
00:28:14.280 --> 00:28:16.480
trapped. It can't pass the event horizon.

669
00:28:16.480 --> 00:28:18.000
That's what the event horizon is all about.

670
00:28:18.800 --> 00:28:21.770
Because gravitation is a property

671
00:28:22.250 --> 00:28:25.250
not of the black hole, but of

672
00:28:25.250 --> 00:28:28.210
the universe itself. Ah. It's

673
00:28:28.210 --> 00:28:30.970
the underlying sort of fabric of space that

674
00:28:30.970 --> 00:28:33.770
is what carries gravity. Um,

675
00:28:33.930 --> 00:28:36.890
and so if you've got these colliding

676
00:28:36.890 --> 00:28:39.130
black holes, they shake the space

677
00:28:39.930 --> 00:28:42.570
itself rather than emit

678
00:28:43.130 --> 00:28:45.730
something. So that's the

679
00:28:45.730 --> 00:28:48.440
difference. The gravitational waves. Uh,

680
00:28:48.570 --> 00:28:51.450
yes, indeed. They're caused by, uh, the,

681
00:28:51.750 --> 00:28:54.270
by a loss of mass from the black holes. But

682
00:28:54.270 --> 00:28:56.790
they're not a property of the black holes. If

683
00:28:56.790 --> 00:28:59.790
I can put it that way. Yes, it's an

684
00:28:59.790 --> 00:29:02.070
effect rather than something being emitted.

685
00:29:02.390 --> 00:29:05.350
So, um, um, Ed's quite right that

686
00:29:05.350 --> 00:29:07.709
nothing can escape a black hole, but

687
00:29:07.709 --> 00:29:10.590
gravitational waves apparently do. But

688
00:29:10.590 --> 00:29:13.030
they're not. Basically what you're seeing is,

689
00:29:13.670 --> 00:29:15.870
uh, something to do with the universe, not

690
00:29:15.870 --> 00:29:16.630
the black hole.

691
00:29:17.910 --> 00:29:20.110
Andrew Dunkley: Okay, yeah, I get it. It's the old pebble in

692
00:29:20.110 --> 00:29:21.150
the pond trick.

693
00:29:21.150 --> 00:29:23.350
Professor Fred Watson: Yeah, that's right. Yes it is, yeah.

694
00:29:24.390 --> 00:29:27.230
The ripples in the pond, uh, don't come

695
00:29:27.230 --> 00:29:30.230
from the pebble. They come from the fact that

696
00:29:30.230 --> 00:29:32.710
the pebble has disturbed the underlying

697
00:29:33.269 --> 00:29:35.390
fabric. Uh, of the water, in fact. Put it

698
00:29:35.390 --> 00:29:37.750
that way. Yeah, it's a really good analogy.

699
00:29:39.750 --> 00:29:41.030
Andrew Dunkley: I come up with all sorts.

700
00:29:41.190 --> 00:29:43.310
Professor Fred Watson: You do, but that's a cracking good one,

701
00:29:43.310 --> 00:29:44.550
Andrew. Well done. I like that.

702
00:29:45.030 --> 00:29:46.870
Andrew Dunkley: I think you told it to me once before.

703
00:29:48.960 --> 00:29:49.280
Maybe.

704
00:29:49.440 --> 00:29:49.930
Professor Fred Watson: Maybe.

705
00:29:49.930 --> 00:29:52.160
Andrew Dunkley: Um, so that's the simplicity of it, really.

706
00:29:52.160 --> 00:29:53.680
There's not much more to tell.

707
00:29:53.680 --> 00:29:55.520
Professor Fred Watson: No, no, that's right. It's not. You know, it

708
00:29:55.520 --> 00:29:58.040
doesn't defy the logic of nothing being able

709
00:29:58.040 --> 00:30:01.030
to escape a black hole. Uh, it's, um,

710
00:30:01.440 --> 00:30:04.200
because you, um. Yes, Ed's right. Nothing

711
00:30:04.200 --> 00:30:06.480
can. Nothing solid or,

712
00:30:07.030 --> 00:30:09.840
um, electromagnetic or particles

713
00:30:09.840 --> 00:30:12.560
can't either. Uh, but the

714
00:30:12.560 --> 00:30:15.080
gravitational field is different. It's

715
00:30:15.080 --> 00:30:17.360
something to do with the underlying universe.

716
00:30:18.410 --> 00:30:20.570
Andrew Dunkley: Indeed it is. Uh, thanks, Ed. Great question.

717
00:30:21.210 --> 00:30:24.170
And, um, yeah, answered

718
00:30:24.250 --> 00:30:26.810
very simply in the end. Which

719
00:30:27.050 --> 00:30:28.570
doesn't happen often, does it, really?

720
00:30:29.130 --> 00:30:30.970
Professor Fred Watson: No, usually they're not answered at all.

721
00:30:32.410 --> 00:30:33.690
Andrew Dunkley: Or just adequately.

722
00:30:33.690 --> 00:30:36.010
Professor Fred Watson: Yes, adequately. That's right.

723
00:30:36.090 --> 00:30:38.010
Andrew Dunkley: Thanks, Ed. Uh, thanks to everyone who's sent

724
00:30:38.010 --> 00:30:39.810
in questions. And if you would like to send a

725
00:30:39.810 --> 00:30:41.970
question to us, please do go to our website,

726
00:30:41.970 --> 00:30:44.730
spacenutspodcast.com or spacenuts

727
00:30:44.810 --> 00:30:47.170
IO and there's a little button, uh, up the

728
00:30:47.170 --> 00:30:49.930
top top. Uh, or a tab or a link or whatever.

729
00:30:49.930 --> 00:30:52.650
It's a link. Uh, AMA stands for Ask me

730
00:30:52.650 --> 00:30:54.570
Anything. And you can send your questions in

731
00:30:54.570 --> 00:30:56.850
through that particular interface,

732
00:30:57.570 --> 00:31:00.210
text or audio. Don't forget to tell us who

733
00:31:00.210 --> 00:31:01.570
you are or where you're from. Although

734
00:31:01.570 --> 00:31:03.650
sometimes people forget. And you're not going

735
00:31:03.650 --> 00:31:06.090
to get into trouble for that. We're not that

736
00:31:06.090 --> 00:31:07.840
kind of people. M

737
00:31:08.290 --> 00:31:10.650
Nobody there. Have a look around. Visit the

738
00:31:10.650 --> 00:31:13.090
shop, become a supporter. And don't forget to

739
00:31:13.330 --> 00:31:15.490
leave, uh, reviews wherever you listen to us.

740
00:31:15.730 --> 00:31:18.680
Maybe the people listening live right now

741
00:31:18.680 --> 00:31:20.760
via YouTube could leave reviews. That'd be

742
00:31:20.760 --> 00:31:23.120
nice. Unless they hated us. Just don't do

743
00:31:23.120 --> 00:31:26.000
anything. No, I'm just kidding. They've stuck

744
00:31:26.000 --> 00:31:27.680
around, so we must be doing something right.

745
00:31:28.160 --> 00:31:28.720
Professor Fred Watson: Yeah.

746
00:31:28.880 --> 00:31:30.360
Andrew Dunkley: And we're all done, Fred Watson. Thank you

747
00:31:30.360 --> 00:31:30.880
very much.

748
00:31:31.440 --> 00:31:34.280
Professor Fred Watson: Thank you, Andrew. Um, we'll talk again soon.

749
00:31:34.280 --> 00:31:35.520
I, uh, look forward to it.

750
00:31:35.840 --> 00:31:37.880
Andrew Dunkley: I hope so. Uh, Professor Fred Watson Watson,

751
00:31:37.880 --> 00:31:39.640
astronomer at large, thanks to Huw in the

752
00:31:39.640 --> 00:31:42.640
studio, um, who couldn't be with

753
00:31:42.640 --> 00:31:45.440
us today because, uh, he's got a black

754
00:31:45.440 --> 00:31:48.120
hole problem. He called a plumber and neither

755
00:31:48.120 --> 00:31:50.500
of them can get out. And from me, Andrew

756
00:31:50.500 --> 00:31:52.780
Dunkley. Thanks for your company. I'll catch

757
00:31:52.780 --> 00:31:55.380
you on the next episode of Space Nuts. Until

758
00:31:55.380 --> 00:31:58.220
then, bye bye. You've been

759
00:31:58.220 --> 00:32:00.460
listening to the Space Nuts podcast

760
00:32:01.980 --> 00:32:04.700
available at Apple Podcasts, Spotify,

761
00:32:05.020 --> 00:32:07.700
iHeartRadio or your favourite podcast

762
00:32:07.700 --> 00:32:09.460
player. You can also stream on

763
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demand@bytes.com um,

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Professor Fred Watson: this has been another quality podcast

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production from bytes.um com.
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