March 8, 2026

Martian Meteorites, Gas Giants & The Search for Alien Life | Q&A

Martian Meteorites, Gas Giants & The Search for Alien Life | Q&A

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Mars Meteor Showers, Gas Giants, and the Search for Alien Civilizations
In this engaging Q&A episode of Space Nuts, hosts Andrew Dunkley and Professor Fred Watson respond to intriguing questions from listeners about our universe. From the risks of meteor showers on Mars to the gravitational effects of Jupiter on its moons, this episode is filled with cosmic curiosities and insightful discussions.
Episode Highlights:
Meteor Showers on Mars: David from the UK wonders about the potential hazards of meteor showers on Mars, given its thin atmosphere. Andrew and Fred discuss how the reduced atmospheric pressure could allow smaller meteorites to reach the Martian surface and the implications for future human habitation.
Exploring Gas Giants: Penny asks whether there are plans to fly spacecraft through the atmospheres of Saturn and Jupiter. The hosts explain the challenges of such missions and highlight ongoing projects focused on the fascinating moons of these gas giants instead.
The Gravitational Dance of Europa: Andy from London seeks clarity on how Jupiter's gravity affects its moon, Europa, without pulling it closer. Andrew and Fred elaborate on the tidal forces at play and how they create the intriguing geological activity observed on Europa.
The Search for Alien Civilizations: Duncan raises the thought-provoking question of whether we are truly alone in the universe. The hosts discuss the vast distances involved in the Milky Way and the implications for potential communication with extraterrestrial life.

For more Space Nuts, including our continuously updating newsfeed and to listen to all our episodes, visit our website. Follow us on social media at SpaceNutsPod on Facebook, Instagram, and more. We love engaging with our community, so be sure to drop us a message or comment on your favorite platform.
If you’d like to help support Space Nuts and join our growing family of insiders for commercial-free episodes and more, visit spacenutspodcast.com/about.
Stay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.

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WEBVTT

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Hello again, thanks for joining us. This is a Q

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and A episode of Space Nuts where we answer astronomy

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and space science questions from our audience. Today. David wants

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to know about Mars meteor showers. Penny is asking about

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fly through emissions for Satin and Jupiter that could be messy.

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Andy is asking about the gravitational effect of Jupiter on

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its moons, particularly Europa. And Duncan wants to talk about

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alien civilizations. We will deal with all of that and

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more on this episode of Space Nuts fifteen in Channal

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ten nine Ignition sequence Space Nuts NY or three two

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Space Nuts. As Can I reported, Bill's good. This is

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Fred Watson's favorite segment. He's back again for more. Professor

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Fred Watson, Astronomer at Large, Hello, Hello Andrew, you I

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am quite well. It's been a long time, like an

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anatu or three minutes.

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I hope nobody's guests that we record these impairs. But

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never mind, never mind.

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If they haven't figured it out by now, they probably

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never will.

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That's right.

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I'm pretty sure most people know how it works. I mean,

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they just have to look at the shirts we're wearing

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every week. That's if they do it on the YouTube channel. Well,

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I don't know if I don't know if they put

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the video on anymore, because it could be could be

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a bit of a turn off. So I don't know. Anyway,

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all is well with you, I trust it is. Thank you. Yes,

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I I already knew the answer, but we have to

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ask because you know, this is just to be that light. Yes,

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that's exactly. Why don't we try and answer some questions? Oh?

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Or if you must, well you do it. I'm just

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going to push them in there. Let's go to our

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first question that comes from David.

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Kind of a Compson here otly Spring in the UK,

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Back to Mars. As a child of the fifties and sixties,

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reading the comics at the time, there was always a

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risk of meet your showers. I'm just wondering, given that

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Mars atmosphere is not as dense as the IRBs, what

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are smaller meteorites would be able to hit the surface

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of Mars and be a real hazard to anybody put

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in the house there. Find the podcast absolutely amazing. Everybody,

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have a great day. Bye.

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Thank you David, Thanks for those kind words. I'm glad

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you're enjoying the podcast. Sorry, way back to Mars I

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didn't push him there. I didn't. Everyone knows a lot

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of Mars, but yeah, your shows it makes up. It

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brings up an interesting point. It's got a much less

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significant atmosphere than Earth. So does that mean smaller things

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can get through?

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It does, Yeah, it does. David's absolutely right. I'm delighted

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we've got a listener in hot and this spring. I

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used to drive past there very very frequently. It's between

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Durham and Sunderland in the north of England, and I

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was a very very regular user of the A one

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m which goes us taught and the spring. And it's

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lovely to hear your voice, David, and hear that lovely

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North Durham accent there. The answer is yes, so because

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the atmosphere, you know, the atmospheric pressure on Mars is

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I think it's point six percent of our atmospheric pressure,

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which means that meteorites coming in are going to have

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a lot less resistance. We know of meteorites on Mars,

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many have been identified by both Curious City and Perseverance, usually.

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By there but by their color.

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But both those rovers were equipped with lasers appas that

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could give us an idea of the content and some

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of those meteorites have been found to be metallic. So

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meteorites on Mars are something that happens. And yes, there's

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probably a higher risk of damage from an incoming meteorite

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on Mars than on Earth because the likelihood is but

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their terminal velocity, the sort of final velocity after they've

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passed through the atmosphere, will be much higher than it

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will be on Earth just because of a lot lower pressure.

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And so yes, meteorite protection might turn out to be

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quite an important aspect of putting humans on Mars. We

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haven't had any reports of you know, there's how many

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rovers have been on Mars now, I can think of

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long two, three, four, five, six, at least six, probably

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more like seven or eight. They are Andrew is googling

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it as we speak.

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Yeah, six six rovers. Sojournal, Spirit, opportunity, curiosity, perseverance, and Jurong,

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the Chinese mission.

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The Chinese one. That's right, Yeah, so I did get

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the right answer.

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Six.

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Yeah, yeah, it's so none of those, as to the

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best of our knowledge, has suffered any kind of meteoritic impact.

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So at least, so far, so good in terms of

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our understanding of the meteorite hazard on Mars. But a

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good question to raise, David, and it's always always gives

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us a chance to talk about Mars.

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He did ask about the danger to housing on Mars.

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They probably won't build houses on Mars like they do

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on Earth. And because of the radiation issues, they're probably

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going to have to go underground, which would pretend get

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them from anything like that. But there will be surface

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something or other there one day, infrastructure. Yeah, perhaps domes

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that they could be susceptible. Maybe.

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Yeah, it looks like I mean what we imagine is

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something like White Cliffs in western New South Wales where

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people live underground. They do, and that's just to get

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out of the heat.

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So that's radiation.

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Yes, it is silver radiation, that's right.

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Yeah, indeed, yeah, sort of another question. Yeah, here it is.

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We are constantly monitoring for big objects that could be

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threatening to Earth, things that could destroy these cities or

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regions or god forbid, the planet itself as we know it.

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What about Mars? Do we keep an eye on anything

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that might hit that?

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So yes, to some extent. If you you know, if

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you can identify near Earth objects look at their orbits,

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you would certainly find out from the analysis very quickly

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if there was any risk of one of those hitting

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the planet Mars. But there's probably many small objects in

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the vicinity of Mars because it's closer to the asteroid

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belt than we are, which are undetectable from the distance

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of Earth. You know, objects that might even be as

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big as Phoebost, Mars's biggest moon. We would be able

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to detect that from Earth quite easily, but as we

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obviously can. It was discovered in the eighteen hundreds. But

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you know, if you had something that was only a

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few tensimeters across, which could pose a hazard to houses

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on Mars, that would be hard to detect from the

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distance of Earth unless it unless it was also a

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near Earth object, so it was coming close to closer

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to our telescopes.

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Yeah, there'd be nothing much we could do about a

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beefing hitting Mars anyways, there or they'd be good experiment

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if we want to test our capabilities.

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Well, that's right, if there was you know, the bigger

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ones are the ones that we know more about because

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they're easier to see. If something like that was looking

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as though it might collide with Mars, yes, it might

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be a good time to test out the theories that

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were put into place with the Dart mission a few

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years ago. Yes, see, whether it'll actually work on something

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a bit bigger.

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Than that, one can only wonder, And hopefully we don't

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ever have to put it to the test for ourselves.

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But you just never know. There's always something going on

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out there. There's so much stuff bumping into it. There's

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something else out there. It's only a matter of time

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before one of them kareems into our sector and becomes

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a potential threat. Although we seem to be finding them

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more and more now, don't we.

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Frere with And that's the good news parts of this story.

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Two good news sides of this story. One is that

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the big ones are the easiest to find, and the

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other is that we've been finding these things now for

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the last forty years and have a good idea of

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what this environment's like.

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Yep, great to hear from you, David. Great question and

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thanks for sending it in. Our next question comes from Penny.

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It's a short, quick one. I think I know where

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this one might go to in terms of an answer.

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As Satin and Jupiter are gas giants, are there any

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plans to fly a spacecraft through the Middle of one

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or both of them. Interesting question, Penny. I do recall,

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when you're talking about comet or asteroid impact, the impact

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with Jupiter many many years ago that we almost got

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footage of it was just quite not quite the right angle,

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but we did see the aftermath of it.

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That's Schumacher Levy.

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Yes.

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Second, the one Jupiter, Remember what year ninety four I

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think it might have been. So the issue is that

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the gas giant aspect of these planets is really just

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their outer envelope that's gassy, and we don't really know

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what's underneath that. The likelihood is there will be a

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solid core there. It may be rocky. Some have suggested

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that it will be made of metallic hydrogen, which is

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hydrogen in a very unusual form. So you've got a

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core of something called metallic hydrogen. So flying through is

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not anything that's planned because it will be impossible.

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But even if.

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These gas giants were sort of gaseous all the way through,

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it still would be a very hard thing to achieve

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because you're entering an atmosphere. You'd have to slow the

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rocket the spacecraft down enormously in order to prevent it

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from just melting by friction. With the atmosphere, which is

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what happened to Cassini. Cassini was plunged into Saturn's atmosphere

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at the end its mission in twenty seventeen. It didn't

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burn up because there's no oxygen in Saturn's atmosphere, but

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the friction made it melt. Basically, it just melted and

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felt pieces. In fact, NASA produced some real tear jerker

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footage of what that might have looked like, which we

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saw often at the end of the Cassini mission.

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You know, this thing which had.

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Performed valiantly for the previous thirteen years and done a

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marvelous job at revolutionizing our knowledge not just of Saturn

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and its rings and moons, but also the way planets

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form and things like that. This footage of Cassini hitting

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the top of Saturn's atmosphere and having its antennas ripped

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off and eventually just melting into becoming part of the

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atoms of the atmosphere of Saturn, and that is you know,

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any mission to try and penetrate down through the atmosphere

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would struggle because of the rapid increase in density, the

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fact that you've got to slow the spacecraft down in

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order to stop it just burning up my friction. I

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think one of the Jupiter missions, I can't remember which

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one might have been Galileo actually sensed as it hits

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Jupiter's atmosphere to burn up again or to melt. I

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think there were sensors on board that were giving us

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some readings of what the conditions were like.

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Yeah. I think the other big problem would be pressure,

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wouldn't it if you tried.

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To yeap, So the pressure just goes up, probably exponentially

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at some level.

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Yeah, and Penny might be interested to know that there

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are some missions slated for the near future, europea Clipper

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which will launch in it's already launched, I should recite

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it's quite yet twenty thirty. There's the Juice mission, which

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launched in twenty twenty three, which arrives in twenty thirty

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one and drag and fly with the helicopter off to Totem. Yeah,

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we'll launch in twenty twenty eight. So they're more interested

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in some of the moons around those gas giants. But yes,

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that they are fascinating, and of course we're most interested

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in Europa Clipper because we want enough anything's living in

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the ocean, and maybe there is, Maybe there isn't. Who knows,

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it could just be made of jelly. We don't really know,

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although the Juice mission is more likely to figure all

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that out. Boom boom, Thank you, Penny Lovely to hear

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from you. This is space Nuts Q and a edition

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with Andrew Dunkley and Professor Fred Watson. Let's take a

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00:13:50.320 --> 00:13:52.720
break from the show to tell you about our sponsor,

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246
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space nuts. Okay, we take your space nuts. And speaking

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of Europa and Jupiter, we've got a question now from Andy.

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This is Andy the train driver from London.

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I just got a question about Europa.

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I know Europa erupts because it's being sort of squeezed

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by the gravity of Jupiter. But what I don't understand

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is if Europa is being affected by Jupiter's gravity, why

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is it not just being pulled closer to Jupiter. I

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thought gravity pulls things down, like when you throw a

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ball in air, gravity pulls it back down. I don't

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understand how Europa is being squeezed. That suggests to me

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that it's being affected by gravity from all directions. Squeeze

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it like you could squeeze the tennis ball. Maybe you

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can shed some light on this or tell me that

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I'm blocking up the wrong tree.

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Anyway.

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Thanks for the podcast, guys, really interesting and see you

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in the next one.

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It's Jordie's job to bark up the wrong tree.

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But nicely done, Andrew.

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Your point is well taken. Andy. It's not just Europer though.

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There are several moons orbiting the gas giants that do

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get that squeeze effect tightened. I think is one of them,

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and I look probably all of them to some degree.

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But Europe, yeah, it's it's it's in a difficult position.

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It's a good question though, why don't they just get

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sucked in? Doesn't? But we're not a gas giant.

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No, the same thing happens to our moon though, so

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it's actually probably I think the moon that and is

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thinking of his Eo, which is the innermost of the

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of the moons that the big moon, big four moons

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of Jupiter, and it is the one that gets the

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most squeezing and squashing because of its proximity to Jupiter.

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Europa probably also has the same phenomenon, and there may

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be eruptions of it on Europa that possibly a bit

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like Enceladus, where you've got stuff streaming out through the

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cracks in the in the ice. But the genuine volcanic eruptions,

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which they really are, it's hot lava, is what takes

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place on Eo, the innermost of those moons. So the

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way to understand this is to realize recognize that if

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you've got an object in a very strong gravitational field.

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First of all, let me just clarify the reason why

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objects in orbit around other objects don't just get pulled in.

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They are getting pulled in, but they've got a forward

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motion that compensates for the for the pull. So basically

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the motion of the object through space is what balances

292
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out the gravity of a giant like Jupiter. And so

293
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that you know, the greater the gravity of a of

294
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a planet, the faster its satellites have to orbit in

295
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order not to not to fall in. And so that's

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that's the mechanism that stops these things just immediately being

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sucked in to Jupiter. They're already moving. And that comes

298
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about why are they moving because they were formed that

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way with the way the you know, the planets and

300
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their satellites evolve the way they formed, they're basically swirling

301
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around right from the start and that swirling motion is

302
00:18:52.799 --> 00:18:56.240
what stops which is fossilized in the in the planets

303
00:18:56.279 --> 00:18:59.480
themselves and the moons of the planets, and stops them

304
00:18:59.519 --> 00:19:04.319
falling into their parent object. But the squeezing and squashing

305
00:19:04.400 --> 00:19:07.279
comes from what we call the tidal effect, and it

306
00:19:07.359 --> 00:19:09.759
is actually exactly the same thing that gives rise to

307
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tides on the Earth. But let's concentrate for a minute

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on EO. Here's this little world right next to gas

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giant Jupiter. One side of EO is feeling the gravitational

310
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pull of Jupiter. The other side is as well, but

311
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it's feeling slightly less because it's further away, because the

312
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gravitational pull falls off as the distant squared one of

313
00:19:34.440 --> 00:19:38.759
the distant squared, So further on the further side of

314
00:19:38.839 --> 00:19:42.400
EO from Jupiter, it's going to feel less force. And

315
00:19:42.440 --> 00:19:46.000
that is what contributes to this tension that there is

316
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and basically elongates the planets slightly in the direction of Jupiter.

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Now why we talk about squashing and squeezing is that

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00:19:56.440 --> 00:19:59.519
throughout the orbit of EO, she's not a planet, it's

319
00:19:59.519 --> 00:20:02.400
a subtleite. But around the orbit of EO as it

320
00:20:02.440 --> 00:20:06.160
goes around is not circular. So sometimes that force is

321
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greater than others. That tension that's trying to pull it apart,

322
00:20:10.319 --> 00:20:14.039
it's greater than at other times. And basically it's that

323
00:20:15.039 --> 00:20:18.559
squashing stretching really is the best word for it. As

324
00:20:18.599 --> 00:20:22.640
it goes round, as it goes around Jupiter. That change

325
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in the stretch force that's being applied is what generates

326
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the heat that causes these eruptions to continually take place.

327
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And that's called the tidal effect. The fact that one

328
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side of a body feels a different gravitational force from

329
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the other. It's what makes us susceptible if we fall

330
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into a black hole to spaghettification. Spaghettification is just a

331
00:20:43.799 --> 00:20:45.759
nicer word than tidal effects.

332
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Yeah. So you've got a real combination of effected. Yeah,

333
00:20:49.759 --> 00:20:52.920
that's right. You've got the gravitational effect, You've got all

334
00:20:53.000 --> 00:20:57.720
little dynamics, yeah, or sort of coinciding to keep these

335
00:20:57.720 --> 00:21:00.319
things from falling into the planet that there's attack war

336
00:21:00.440 --> 00:21:05.720
going on. I saw a really good demonstration online or

337
00:21:05.759 --> 00:21:09.279
probably three or four weeks ago on how the tides

338
00:21:09.839 --> 00:21:13.119
work on Earth and of because most people, and I

339
00:21:13.200 --> 00:21:17.519
must confess guilt here, assume that the Moon causes the

340
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water to rise and then fall. But it's not. It's

341
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the fact that the Earth is rotating, the Moon is orbiting,

342
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and there's always a wave. It's just always there, and

343
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it's just that when it when the moon reaches your vicinity,

344
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that that lump of water comes up and goes down again.

345
00:21:37.720 --> 00:21:40.240
It's it's not the water so much rising, it's just

346
00:21:40.279 --> 00:21:44.000
it's always risen in proximity to the moon. Am I right?

347
00:21:44.920 --> 00:21:45.279
You are?

348
00:21:46.079 --> 00:21:48.680
You're partly right, because it's a bit more you I

349
00:21:48.720 --> 00:21:49.319
missed something.

350
00:21:49.799 --> 00:21:54.039
Yeah, that doesn't explain the bulge on the other side, because,

351
00:21:54.079 --> 00:21:58.039
as you will, you get a high tide every toye

352
00:21:58.880 --> 00:22:03.359
and that's because again it's the tidal effect. So the

353
00:22:03.359 --> 00:22:06.559
moon's pulling on the ocean on the near side, it's

354
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also pulling on the earth itself and that leaves behind

355
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the water on the other side, so you get a

356
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bulge on each side.

357
00:22:15.759 --> 00:22:21.599
That works. Fascinating. It's worth looking up that demo. I

358
00:22:21.599 --> 00:22:24.640
didn't really fine print obviously, but yeah, that makes sense.

359
00:22:24.680 --> 00:22:28.599
So the water's being poured earth sort of dragging with it,

360
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and then the water's been left behind on the other side.

361
00:22:31.119 --> 00:22:35.680
So you've got two bulges, two bulges exactly, so fascinating. So,

362
00:22:36.359 --> 00:22:38.319
and that's kind of ague. What's happening to all these

363
00:22:38.480 --> 00:22:41.799
these moons in various ways. If I have not water,

364
00:22:41.920 --> 00:22:42.920
something else has been.

365
00:22:43.200 --> 00:22:45.559
Well, that's right, it's the rock, does it as well?

366
00:22:45.559 --> 00:22:48.279
The same is true on Earth. The rock goes up

367
00:22:48.279 --> 00:22:50.680
and down as well. I've got a question for Andy though,

368
00:22:51.680 --> 00:22:54.680
if he's for getting back to us, I'd like to

369
00:22:54.720 --> 00:22:58.519
know what sort of trains he drives, because yeah, I'm

370
00:22:58.519 --> 00:23:02.200
a bit of a train myself. Of train drivers are

371
00:23:02.200 --> 00:23:02.920
my heroes.

372
00:23:03.759 --> 00:23:06.559
Yeah, I live next door to a retired train driver.

373
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So yeah. But when we flew into Dubbo the other day,

374
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I looked down at the rail maintenance facility. It's a

375
00:23:15.920 --> 00:23:19.200
brand new system facility that's just been built in Dubbo

376
00:23:19.599 --> 00:23:22.359
and they're fitting out all the new regional trains and

377
00:23:22.400 --> 00:23:25.079
you can see them all lined up, bright red, all

378
00:23:25.880 --> 00:23:28.400
getting ready to go. They're putting all the furniture in

379
00:23:28.440 --> 00:23:33.039
them and the Wi Fi systems, and yeah, they'll be

380
00:23:33.119 --> 00:23:37.039
rolled out pretty soon, not exactly sure when, but the

381
00:23:37.079 --> 00:23:39.720
plan is soon. That's the answer to the question.

382
00:23:39.799 --> 00:23:45.160
Officially, have you ridden on a new metro trains here

383
00:23:45.200 --> 00:23:47.880
in Sydney, Yes, I have, yes, so you'll know that

384
00:23:47.960 --> 00:23:50.480
they drive one hundred kilometers an hour. With new driver.

385
00:23:50.599 --> 00:23:52.319
You can stand at the front, look out the front

386
00:23:52.319 --> 00:23:54.279
window and pretend you're driving it.

387
00:23:54.960 --> 00:23:57.319
And I've done that in a taxi in San Francisco.

388
00:23:57.559 --> 00:24:01.680
Oh yes, yehs for rival as taxi. That's next level.

389
00:24:01.839 --> 00:24:06.440
That's just amazing. But yeah, yeah, pretty incredible stuff. Thanks. Andy,

390
00:24:07.160 --> 00:24:10.039
really enjoyed that question. And yeah, if you want to

391
00:24:10.079 --> 00:24:11.880
tell us what sort of train you drive, send us

392
00:24:11.920 --> 00:24:17.799
another message. We'd love to find out how their barlow.

393
00:24:20.640 --> 00:24:23.000
If I'm Provan.

394
00:24:28.799 --> 00:24:34.559
Spiece notutes. Our final question today, Fred comes from Duncan.

395
00:24:34.720 --> 00:24:37.559
He said, I've heard that a group of astrophysicists have

396
00:24:37.720 --> 00:24:42.480
calculated that there are an estimated one thousand alien civilizations

397
00:24:42.480 --> 00:24:45.440
spread across the Milky Way. But the Milky Way is

398
00:24:45.440 --> 00:24:48.920
one hundred thousand light years across. How far away would

399
00:24:48.920 --> 00:24:52.640
an advanced civilization have to be in practical terms to

400
00:24:52.720 --> 00:24:58.359
be uncontactable? In other words, are we realistically given the

401
00:24:58.559 --> 00:25:01.079
distances involved actively alone?

402
00:25:03.200 --> 00:25:08.200
Yes, is the answer. And it's not just about the distance.

403
00:25:08.240 --> 00:25:13.880
It's also about the time. Because a thousand civilizations with

404
00:25:14.160 --> 00:25:18.279
in a galaxy that's twelve billion years old, they might

405
00:25:18.319 --> 00:25:21.039
well have turned up and gone long ago or still

406
00:25:21.039 --> 00:25:22.119
be in the future.

407
00:25:22.319 --> 00:25:25.880
Because assume that we all coexist.

408
00:25:25.119 --> 00:25:28.839
That's right, and we probably don't. There's actually a really

409
00:25:28.920 --> 00:25:31.559
nice piece. Now let me see if I can find

410
00:25:31.559 --> 00:25:37.440
it to direct Duncan to it. It's on one of

411
00:25:37.440 --> 00:25:41.640
the space the science media came he today is actually.

412
00:25:41.319 --> 00:25:45.599
I think is Oh where is it? Sorry, I've lost it.

413
00:25:46.799 --> 00:25:51.359
Yeah, it's basically a summary of thinking by the likes

414
00:25:51.480 --> 00:25:57.200
of Richard Feynman and other great minds. And the bottom

415
00:25:57.240 --> 00:25:59.839
line is, it's exactly what I've been saying. It's not

416
00:25:59.880 --> 00:26:05.200
just the distances, it's the time that you're the era

417
00:26:05.319 --> 00:26:09.559
in which you live, and it's very unlikely that we'd

418
00:26:09.559 --> 00:26:16.240
find communicable civilizations within the same time zone that we're

419
00:26:16.279 --> 00:26:18.279
living in, if I can put it that way. It's

420
00:26:18.319 --> 00:26:21.440
actually on. It is on again on the brighter side

421
00:26:21.440 --> 00:26:25.759
of news, and the headline is a really very very

422
00:26:25.799 --> 00:26:29.720
thoughtful article, well worth a read. Interstellar travel is impossible

423
00:26:29.759 --> 00:26:32.960
and aliens haven't visited the Earth, physicists say, and it's

424
00:26:32.960 --> 00:26:36.359
because the laws of physics basically make any kind of

425
00:26:36.400 --> 00:26:41.079
travel or even communication extremely difficult. The laws of physics

426
00:26:41.119 --> 00:26:43.400
are very rigid, worth having.

427
00:26:43.200 --> 00:26:46.759
A look at. Yeah, indeed, although there's this new book

428
00:26:46.799 --> 00:26:49.759
that I know that's been written that kind of is

429
00:26:49.839 --> 00:26:52.640
counted all that. But you can do that in science fiction.

430
00:26:54.799 --> 00:26:58.920
Quite so that's why it's called science fiction.

431
00:26:59.400 --> 00:27:03.200
Yes, that's what it is. By way of example, though,

432
00:27:03.279 --> 00:27:07.920
if I may duncan, if you were to be aware

433
00:27:08.119 --> 00:27:14.160
of an advanced communicative civilization on a rocky planet orbiting

434
00:27:14.240 --> 00:27:20.640
Alpha centaury A, for example, and you sent them a message,

435
00:27:20.799 --> 00:27:24.599
it would take I'm just trying to remember four point

436
00:27:24.960 --> 00:27:28.599
three seven years to get there, and that means a

437
00:27:28.640 --> 00:27:33.000
return message. If they answered you immediately, would mean that

438
00:27:33.079 --> 00:27:35.240
you would not get a reply for eight point seven

439
00:27:35.359 --> 00:27:39.599
four years, give or take. But let's round that out

440
00:27:39.599 --> 00:27:41.680
though a decade, because you know what the bureaucracy is

441
00:27:41.799 --> 00:27:44.039
like around Alpha Tory. They're not going to you know,

442
00:27:44.839 --> 00:27:46.480
they're going to take a couple of years to figure

443
00:27:46.480 --> 00:27:51.200
out what they want to say. But that's the reality

444
00:27:51.200 --> 00:27:55.440
of it, isn't And that's our nearest potential, ye neighbor,

445
00:27:57.640 --> 00:27:58.240
It's true.

446
00:27:58.359 --> 00:28:02.599
And I mean the point that this article makes is,

447
00:28:03.640 --> 00:28:07.000
you know, we live in a bubble of radio radio radiation,

448
00:28:07.079 --> 00:28:11.359
which are all the transmissions from Earth that's now basically

449
00:28:11.359 --> 00:28:16.359
one hundred light years in radius because we've been sending

450
00:28:16.519 --> 00:28:20.279
radio transmissions for about a hundred years and all right,

451
00:28:20.400 --> 00:28:23.119
what's that one hundred divided? But it's a thousandth of

452
00:28:23.160 --> 00:28:26.440
the diameter of the galaxy, and so you know, it's

453
00:28:26.559 --> 00:28:33.920
hardly any distance at all. So yeah, it's in a

454
00:28:33.920 --> 00:28:38.880
way and uncomfortable reality. To all intents and purposes. We're alone,

455
00:28:38.880 --> 00:28:42.559
We're uncontactable. We are alone. It's good side because we're

456
00:28:42.640 --> 00:28:46.559
unlikely to be picked on by any voracious aliens.

457
00:28:47.440 --> 00:28:51.440
But yep, yeah, yeah, I think we've got to be

458
00:28:51.480 --> 00:28:54.559
realistic about it. Even if there are a thousand alien

459
00:28:55.000 --> 00:29:02.240
civilizations with advanced technology in our gal see, we are

460
00:29:02.279 --> 00:29:04.599
probably never going to be in a position to communicate

461
00:29:04.640 --> 00:29:07.759
with them more and certainly not be able to travel

462
00:29:07.759 --> 00:29:13.160
to them in any meaningful way. And so even if

463
00:29:13.160 --> 00:29:14.799
we're not alone, we are alone.

464
00:29:15.839 --> 00:29:22.079
Yes, that's right exactly. You know that of that thousand civilizations,

465
00:29:22.079 --> 00:29:23.920
maybe five hundred of them have been and gone and

466
00:29:23.960 --> 00:29:26.559
five hundred of them are yet to evolve.

467
00:29:28.200 --> 00:29:32.240
Do you concur with that estimation or you don't think.

468
00:29:32.160 --> 00:29:36.720
It's I look, I have seen similar figures being quoted.

469
00:29:37.759 --> 00:29:40.559
Not that there's that number of civilizations, but that there

470
00:29:40.599 --> 00:29:43.400
might be that sort of number of habitable planets that

471
00:29:43.480 --> 00:29:48.079
might be earth like. We don't know whether being earth

472
00:29:48.240 --> 00:29:53.039
like necessarily means you evolve an intelligent species because it's

473
00:29:53.079 --> 00:29:53.720
done it once.

474
00:29:53.839 --> 00:29:57.039
But but yeah, the only time could be because the

475
00:29:57.039 --> 00:30:00.279
circumstances have to be perfectly right. Although you know, we're

476
00:30:00.319 --> 00:30:04.200
assuming humanoid type, carbon based life forms, but there could

477
00:30:04.200 --> 00:30:08.279
be others out there that were created a completely different way. Yeah.

478
00:30:08.359 --> 00:30:12.720
So yeah, that's the stuff of imagination at the moment.

479
00:30:12.759 --> 00:30:15.920
But it's a possibility, I suppose. And of course we'll

480
00:30:15.960 --> 00:30:20.440
look like Dill's next week when a massive alien mothership

481
00:30:20.559 --> 00:30:23.079
sets itself down on top of the White House and.

482
00:30:24.599 --> 00:30:25.599
To rescue us all.

483
00:30:26.920 --> 00:30:32.440
Maybe maybe. Gosh, thanks Duncan. Thanks to everybody who's said

484
00:30:32.480 --> 00:30:35.200
in questions, please send them in to us. I do

485
00:30:35.279 --> 00:30:37.359
have a bit of homework, sort of. We got a

486
00:30:37.440 --> 00:30:42.440
question twice now I've received it from Mike in New York. Mike,

487
00:30:42.480 --> 00:30:45.359
you sent us a question in about black holes, an

488
00:30:45.400 --> 00:30:48.960
audio question. The whole guts of the question got cut

489
00:30:49.000 --> 00:30:52.079
off somehow, and so we got the first We got

490
00:30:52.079 --> 00:30:54.799
your pre amble, then you started asking the question. Then

491
00:30:54.839 --> 00:30:59.000
there was about five hours of nothing, probably about twenty

492
00:30:59.000 --> 00:31:01.799
seconds and then we heard you say goodbye. So we

493
00:31:01.839 --> 00:31:04.839
don't actually have the question, so if you'd like to

494
00:31:04.880 --> 00:31:08.200
send it again, please do. I don't know what happened there,

495
00:31:08.240 --> 00:31:12.079
but yeah, it's the internet, so that's what happened there.

496
00:31:12.880 --> 00:31:15.880
But yeah, Mike would love to get that question so

497
00:31:15.920 --> 00:31:18.079
we can run with it and any questions you want

498
00:31:18.119 --> 00:31:20.559
to send in via the Ask Me Anything tab at

499
00:31:20.599 --> 00:31:23.480
the top of our website Spacenuts podcast dot com, Space

500
00:31:23.599 --> 00:31:27.000
Nuts dot io, and don't forget to tell us who

501
00:31:27.079 --> 00:31:29.680
you are and we're from. Thank you. Fred has always

502
00:31:29.720 --> 00:31:30.480
been a lot of fun.

503
00:31:31.160 --> 00:31:34.440
Absolutely, it's great questions. Good to hear everybody's voice and

504
00:31:34.880 --> 00:31:36.039
nice to see those questions.

505
00:31:36.079 --> 00:31:39.519
Thank you. Indeed, that's Professor Fred Wat's an astronomer at

506
00:31:39.599 --> 00:31:43.359
large and thanks to heu in the studio. Couldn't be

507
00:31:43.400 --> 00:31:46.319
with us today. He got stopped by border security and

508
00:31:46.480 --> 00:31:49.599
they realized he was an alien. It comes from New Zealand,

509
00:31:49.599 --> 00:31:52.319
that made sense, So he's been arrested. He might be

510
00:31:52.400 --> 00:31:54.400
back next week and from me Andrew Uncley, thanks for

511
00:31:54.440 --> 00:31:56.839
your company. We'll catch you on the next episode of

512
00:31:57.160 --> 00:32:01.440
Space Nuts. Bye bye, SUTs. Been listening to the Space

513
00:32:01.559 --> 00:32:08.720
Nights podcast, available at Apple Podcasts, Spotify, iHeartRadio, or your

514
00:32:08.799 --> 00:32:12.160
favorite podcast player. You can also stream on demand at

515
00:32:12.200 --> 00:32:16.039
fights dot com. This has been another quality podcast production

516
00:32:16.319 --> 00:32:19.359
from nights dot com.