Aug. 16, 2026
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
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support.
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
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support.
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,
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you know, the company kept their. Built
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it. I think it might have been perkinelmer.
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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
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found out there were two more built for
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surveillance. Um, something else
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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
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so they use um, adaptive optics
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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
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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
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invented a new um, kind of
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um, lens that replaces human
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lens that can now
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do the same thing as a human lens. Like okay,
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when you have a cataract operation they
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replace the human lens. That's all fogged up
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with generally a plastic lens of some
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kind. But it was a fixed lens. It could only
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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
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accommodates to different distances by
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changing the shape of the lens. Yeah, yeah.
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So um, that's pretty. Yes. Quite remarkable
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and um. Would be a real breakthrough for
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um. You know, for vision, uh, for poor
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vision.
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Anyway, we've strayed off the topic here. We
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have a bit and uh.
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Andrew Dunkley: I do, I'm sure never happens usually.
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Professor Fred Watson: I'm sure that um. Uh. Our uh.
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Listener is on the money suggesting that
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there are technologies that are being used
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in secrets, um.
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Professor Fred Watson: Ah.
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Professor Fred Watson: Or restricted environments.
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Uh, that would be of great
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value for astronomy. I uh.
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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
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sort. Um, there is no. I don't think there's
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any equivalent uh, for example in the
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field of gravitational wave astronomy. I
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don't think there's anything that the
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military are doing that could feed into that.
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Although quantum optics are being used in
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that now. So, um, I
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suspect it's in, you know, in relation to the
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tools that are developed for, uh,
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our observations. Um,
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we owe infrared detectors,
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the things that see redder than red light or
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heat radiation. We owe them to the military.
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That's a spin off from military work. Um,
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I do remember, uh, one of the first
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infrared instruments on the Anglo Australian
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telescope. When it was being delivered.
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Uh, I think,
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um, the detector came under armed guard
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almost. It wasn't quite like that. But there
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was a lot of hoops to jump through when this
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detector was delivered. Because it had to be
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certain not to stray into the hands
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of certain foreign nations who the
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Americans who developed this detector didn't
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want, uh, them to get hold of.
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So those technologies do eventually
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kind of sprinkle down to astronomy where the
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poor relations in that regard, uh, although
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we do push the limits perhaps more than
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anybody else, uh, in technology.
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So, um, yes,
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I, I don't have any
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definite, um, speculations, uh,
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except to say that nothing would
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surprise me in that regard
449
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when it comes.
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Andrew Dunkley: I'm not a conspiracy theorist, but I do
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believe there's a heck of a lot going on up
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there that we do not and probably will
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not know about. Um, and
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I truly believe that the technology
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available today in space and on
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the planet, um, in those
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dark corners of government buildings
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is far, far more advanced than we
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could possibly imagine. I think given what
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we've got access to in a domestic sense in
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the public arena today,
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uh, what's been developed already behind
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closed doors that we're unaware of. And
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it's probably up. They're circling the planet
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as we speak.
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Professor Fred Watson: Yeah, I think it works both ways though,
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because I think, um, we're now
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seeing, uh, the military adopting
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what would have been thought of as commercial
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products before. Uh,
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and that's happened certainly in Ukraine.
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There's been an adaptation of
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all sorts of commercial products for
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military purposes. Um, so
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what I guess I'm saying is that the
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technology that we use every day is not
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as far removed from what the military use
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as it would have been 20 or 30 years ago.
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Uh, I think that's probably fair to say, but
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that's me going out on a limb. And who can
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prove me wrong?
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Andrew Dunkley: Well, that's a good point too. Yeah, it's a,
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uh, really interesting question. Thank you
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for sending it in. This is Space Nuts Andrew
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Dunkley here with Professor Fred Watson
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Watson.
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Professor Fred Watson: I believe that this nation should commit
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itself to achieving the goal
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before this decade is out of landing A man
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on the moon and returning him safely
491
00:20:33.020 --> 00:20:34.540
Andrew Dunkley: to the Earth face nuts.
492
00:20:35.660 --> 00:20:38.540
Another audio question from Fred.
493
00:20:39.260 --> 00:20:41.780
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
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astronomer at large, thanks to Huw in the
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studio, um, who couldn't be with
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00:31:42.640 --> 00:31:45.440
us today because, uh, he's got a black
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00:31:45.440 --> 00:31:48.120
hole problem. He called a plumber and neither
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00:31:48.120 --> 00:31:50.500
of them can get out. And from me, Andrew
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Dunkley. Thanks for your company. I'll catch
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00:31:52.780 --> 00:31:55.380
you on the next episode of Space Nuts. Until
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00:31:55.380 --> 00:31:58.220
then, bye bye. You've been
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00:31:58.220 --> 00:32:00.460
listening to the Space Nuts podcast
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00:32:01.980 --> 00:32:04.700
available at Apple Podcasts, Spotify,
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00:32:05.020 --> 00:32:07.700
iHeartRadio or your favourite podcast
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00:32:07.700 --> 00:32:09.460
player. You can also stream on
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00:32:09.460 --> 00:32:11.310
demand@bytes.com um,
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00:32:11.500 --> 00:32:13.540
Professor Fred Watson: this has been another quality podcast
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00:32:13.540 --> 00:32:15.660
production from bytes.um com.
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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,
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you know, the company kept their. Built
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it. I think it might have been perkinelmer.
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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
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found out there were two more built for
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surveillance. Um, something else
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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
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so they use um, adaptive optics
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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
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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
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invented a new um, kind of
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um, lens that replaces human
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lens that can now
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do the same thing as a human lens. Like okay,
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when you have a cataract operation they
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replace the human lens. That's all fogged up
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with generally a plastic lens of some
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kind. But it was a fixed lens. It could only
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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
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accommodates to different distances by
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changing the shape of the lens. Yeah, yeah.
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So um, that's pretty. Yes. Quite remarkable
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and um. Would be a real breakthrough for
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um. You know, for vision, uh, for poor
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vision.
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Anyway, we've strayed off the topic here. We
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have a bit and uh.
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Andrew Dunkley: I do, I'm sure never happens usually.
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Professor Fred Watson: I'm sure that um. Uh. Our uh.
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Listener is on the money suggesting that
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there are technologies that are being used
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in secrets, um.
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Professor Fred Watson: Ah.
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Professor Fred Watson: Or restricted environments.
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Uh, that would be of great
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value for astronomy. I uh.
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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
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sort. Um, there is no. I don't think there's
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any equivalent uh, for example in the
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field of gravitational wave astronomy. I
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don't think there's anything that the
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military are doing that could feed into that.
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Although quantum optics are being used in
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that now. So, um, I
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suspect it's in, you know, in relation to the
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tools that are developed for, uh,
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our observations. Um,
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we owe infrared detectors,
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the things that see redder than red light or
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heat radiation. We owe them to the military.
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That's a spin off from military work. Um,
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I do remember, uh, one of the first
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infrared instruments on the Anglo Australian
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telescope. When it was being delivered.
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Uh, I think,
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um, the detector came under armed guard
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almost. It wasn't quite like that. But there
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was a lot of hoops to jump through when this
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detector was delivered. Because it had to be
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certain not to stray into the hands
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of certain foreign nations who the
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Americans who developed this detector didn't
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want, uh, them to get hold of.
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So those technologies do eventually
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kind of sprinkle down to astronomy where the
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poor relations in that regard, uh, although
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we do push the limits perhaps more than
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anybody else, uh, in technology.
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So, um, yes,
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I, I don't have any
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definite, um, speculations, uh,
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except to say that nothing would
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surprise me in that regard
449
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when it comes.
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Andrew Dunkley: I'm not a conspiracy theorist, but I do
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believe there's a heck of a lot going on up
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there that we do not and probably will
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not know about. Um, and
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I truly believe that the technology
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available today in space and on
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the planet, um, in those
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dark corners of government buildings
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is far, far more advanced than we
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could possibly imagine. I think given what
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we've got access to in a domestic sense in
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the public arena today,
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uh, what's been developed already behind
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closed doors that we're unaware of. And
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it's probably up. They're circling the planet
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as we speak.
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Professor Fred Watson: Yeah, I think it works both ways though,
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because I think, um, we're now
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seeing, uh, the military adopting
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what would have been thought of as commercial
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products before. Uh,
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and that's happened certainly in Ukraine.
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There's been an adaptation of
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all sorts of commercial products for
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military purposes. Um, so
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what I guess I'm saying is that the
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technology that we use every day is not
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as far removed from what the military use
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as it would have been 20 or 30 years ago.
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Uh, I think that's probably fair to say, but
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that's me going out on a limb. And who can
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prove me wrong?
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Andrew Dunkley: Well, that's a good point too. Yeah, it's a,
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uh, really interesting question. Thank you
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for sending it in. This is Space Nuts Andrew
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Dunkley here with Professor Fred Watson
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Watson.
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Professor Fred Watson: I believe that this nation should commit
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itself to achieving the goal
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before this decade is out of landing A man
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on the moon and returning him safely
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Andrew Dunkley: to the Earth face nuts.
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Another audio question from Fred.
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Andrew Dunkley: Hi, this is Fred calling you from St. Paul,
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Minnesota in the US I have a question for
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you regarding the solar systems that contain
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uh, so called hot Jupiter planets, those
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which are very close, ah, around their
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suns. Is it reasonable at all to
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expect that they will have
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smaller planets, rocky planets,
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or are there good reasons that
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come to mind where that should not be the
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case? Um, I'd uh, appreciate hearing
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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
00:32:09.460 --> 00:32:11.310
demand@bytes.com um,
764
00:32:11.500 --> 00:32:13.540
Professor Fred Watson: this has been another quality podcast
765
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