Why Venus May Have Lost Its Moon Forever
Space Nuts: Astronomy Insights & Cosmic DiscoveriesSeptember 17, 2026
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00:33:4630.96 MB

Why Venus May Have Lost Its Moon Forever

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Space Nuts: Venus’s Missing Moon, Satellite Pollution, and Space Force Uniform Controversy
Space Nuts covers three very different space stories in this episode, ranging from planetary science to the consequences of satellite reentry and a controversial military uniform design. Andrew Dunkley and Professor Fred Watson also field listener questions on orbital mechanics, neutrinos, alien communication, and time dilation.
The discussion is broad, but the main thread is clear: how real-world physics shapes everything from Venus’s history to the future of spaceflight and even the look of space-age uniforms.
Key topics
Venus is Earth-like in size, mass, and gravity, but unlike Earth it has no moon, and the episode explores whether it may once have had one.
Fred explains a modeling study led by Stephen Kane suggesting a Venus moon could have spiraled inward, crossed the Roche limit, and been torn apart by tidal forces.
The team discusses what evidence might remain if Venus once consumed a moon, including possible chemical fingerprints in the atmosphere or surface.
Satellite pollution is examined through the lens of reentering spacecraft, especially the growing number of Starlink reentries and their impact on the upper atmosphere.
The European Space Agency’s jet-based chase of two reentering Cluster spacecraft, Tango and Samba, is described as an effort to measure reentry byproducts directly.
The conversation raises concerns about aluminium oxides, atmospheric chemistry, and whether repeated reentries could have broader consequences such as ozone depletion.
The final main story looks at proposed United States Space Force uniforms and why the design drew immediate comparisons to World War II-era fascist aesthetics and Starship Troopers.
Andrew and Fred note how uniform design can shape perception, and why the new concept feels divisive rather than inspiring.
Timestamps
00:00 - Intro and setup for the episode
00:41 - Venus, satellite pollution, and Space Force uniforms preview
04:40 - Venus as Earth’s twin and why it has no moon
08:21 - Modeling a missing Venusian moon
09:20 - Gravitational tug-of-war and moon migration toward Venus
11:44 - Conditions for a moon to survive around Venus
12:43 - Possible traces of an ancient moon impact
16:06 - Satellite pollution from reentering spacecraft
17:16 - Starlink reentries and atmospheric contamination
18:14 - ESA’s jet chase of reentering Cluster spacecraft
20:06 - Observing Tango and Samba during controlled reentry
21:45 - Why the atmospheric consequences could become controversial
23:12 - Wood as a potentially more benign spacecraft material
24:16 - Space Force uniforms and the first visual reaction
25:34 - Starship Troopers and deliberate fascist design cues
27:29 - Why the proposed uniforms feel unsettling


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00:00:00 --> 00:00:02 Andrew Dunkley: Hi there. Thanks for joining us. This is

00:00:02 --> 00:00:04 Space Nuts, where we talk astronomy and space

00:00:04 --> 00:00:07 science and dogs and cats living together and

00:00:08 --> 00:00:10 just about anything, really. There's no topic

00:00:10 --> 00:00:13 that is, uh, ever, um, ignored.

00:00:14 --> 00:00:16 Even when you don't want us to talk about it,

00:00:16 --> 00:00:17 we'll talk about it.

00:00:17 --> 00:00:19 Actually, we've got one of those storeys in

00:00:19 --> 00:00:21 this episode. Uh, not the first one, though,

00:00:21 --> 00:00:24 because we're going to discuss Venus. Now, in

00:00:24 --> 00:00:27 many ways, Venus is just like Earth, except

00:00:27 --> 00:00:30 for one striking difference. Aside from the

00:00:30 --> 00:00:33 weather, it doesn't have a moon. Why not?

00:00:33 --> 00:00:35 Well, um, yeah, there's probably a very

00:00:35 --> 00:00:38 dark reason for that. Uh, satellite

00:00:38 --> 00:00:40 pollution. Uh, we're not talking about

00:00:40 --> 00:00:43 satellites in orbit polluting, uh, our

00:00:43 --> 00:00:45 skies and making life for astronomers very

00:00:45 --> 00:00:47 difficult. We're talking about when they come

00:00:47 --> 00:00:49 back into the atmosphere and literally

00:00:50 --> 00:00:53 pollute our, uh, atmosphere. We'll see

00:00:53 --> 00:00:54 what's going on there.

00:00:54 --> 00:00:57 And the United States Space

00:00:57 --> 00:01:00 Force uniforms have been unveiled. At

00:01:00 --> 00:01:02 least one concept, and it's got some tongues

00:01:02 --> 00:01:05 wagging, some wiggling and some people

00:01:05 --> 00:01:07 scratching their heads. We'll talk about all

00:01:07 --> 00:01:09 of that on this episode of space nuts.

00:01:09 --> 00:01:12 Professor Fred Watson: 15 seconds. Guidance is internal.

00:01:12 --> 00:01:15 10, 9. Ignition

00:01:15 --> 00:01:16 sequence start.

00:01:16 --> 00:01:17 Professor Fred Watson: Space nuts.

00:01:17 --> 00:01:20 Professor Fred Watson: 5, 4, 3, 2. 1, 2, 3, 4,

00:01:20 --> 00:01:22 5, 5, 4, 3, 2, 1.

00:01:22 --> 00:01:23 Andrew Dunkley: Space nuts.

00:01:23 --> 00:01:25 Professor Fred Watson: Astronauts report it feels good.

00:01:26 --> 00:01:28 Andrew Dunkley: And he's back. Once again, it's Professor

00:01:28 --> 00:01:29 Fred Watson Watson, Astronomer at large.

00:01:29 --> 00:01:30 Hello, Fred Watson.

00:01:31 --> 00:01:34 Professor Fred Watson: Uh, hello, Andrew. You mean we're not going

00:01:34 --> 00:01:36 to cover migraines again this week or.

00:01:36 --> 00:01:39 Andrew Dunkley: Why not? We can do that if you like. We've

00:01:39 --> 00:01:40 talked about that before.

00:01:40 --> 00:01:41 Professor Fred Watson: Um, yeah, yeah, we did.

00:01:42 --> 00:01:44 Andrew Dunkley: I mean, we've reached that age where the

00:01:44 --> 00:01:47 first topic, because I'm the captain of

00:01:47 --> 00:01:50 the veteran golfers at our local

00:01:50 --> 00:01:52 club and, um,

00:01:53 --> 00:01:55 the first topic, whenever you sit down, is,

00:01:55 --> 00:01:58 um, your health. And what have you had done

00:01:58 --> 00:01:59 this week?

00:02:00 --> 00:02:02 Professor Fred Watson: Well, yes, I'm sure that's right,

00:02:03 --> 00:02:05 because I'm a little bit older than you, my

00:02:05 --> 00:02:07 topics are even more interesting. So I was at

00:02:07 --> 00:02:08 a presentation last night where they were

00:02:08 --> 00:02:11 talking about coffins, uh, made out of

00:02:11 --> 00:02:12 mushroom fibre.

00:02:12 --> 00:02:13 Andrew Dunkley: Oh, my goodness. Yeah,

00:02:15 --> 00:02:17 okay, that is different.

00:02:17 --> 00:02:19 Professor Fred Watson: It's different. Yeah, different. But

00:02:19 --> 00:02:20 apparently it works.

00:02:20 --> 00:02:22 Andrew Dunkley: Well, it'd be a lot cheaper, wouldn't it?

00:02:22 --> 00:02:24 Professor Fred Watson: Yeah, they don't last very long. Two days, I

00:02:24 --> 00:02:25 think, is the time it takes to decay.

00:02:26 --> 00:02:26 Andrew Dunkley: Wow.

00:02:26 --> 00:02:28 Professor Fred Watson: No, actually, I think it might be a bit

00:02:28 --> 00:02:29 longer than that.

00:02:29 --> 00:02:29 Professor Fred Watson: Very.

00:02:29 --> 00:02:32 Professor Fred Watson: Ah, interesting presentation, though, on, um,

00:02:33 --> 00:02:35 the. From the Symbioscene

00:02:36 --> 00:02:38 Institute, uh, which is looking

00:02:38 --> 00:02:41 at the ways that humankind can live

00:02:41 --> 00:02:44 more comfortably with its own planet

00:02:44 --> 00:02:47 rather than being the terrible Colonial

00:02:48 --> 00:02:50 um, species that we've been to date.

00:02:50 --> 00:02:52 Andrew Dunkley: Yeah. The problem with that is you've got to

00:02:52 --> 00:02:53 get everyone to agree.

00:02:54 --> 00:02:57 Professor Fred Watson: Uh, exactly. That was going to be my

00:02:57 --> 00:02:59 point which I never really got to raise.

00:03:01 --> 00:03:03 Andrew Dunkley: People come up with all these wonderful ideas

00:03:03 --> 00:03:06 about how we can do things right. But, and

00:03:06 --> 00:03:08 you know, some countries will go, well, you

00:03:08 --> 00:03:11 know, we don't want to do that. So we're not.

00:03:11 --> 00:03:14 Professor Fred Watson: So I think um, just as, as an idea though and

00:03:14 --> 00:03:16 as a concept, I think this has

00:03:17 --> 00:03:20 much to uh, um, approve

00:03:20 --> 00:03:23 of and it, and the reason what took me

00:03:23 --> 00:03:25 there was um. Marnie was part of a panel

00:03:25 --> 00:03:27 discussion yesterday.

00:03:28 --> 00:03:31 Excuse me, I'm sorry, sorry Marnie, I sneezed

00:03:31 --> 00:03:34 in the middle of your promo there. She was

00:03:34 --> 00:03:36 part of a panel discussion, uh, which one of

00:03:36 --> 00:03:38 the other guests was, was an

00:03:38 --> 00:03:40 advocate, in fact the founder of the

00:03:40 --> 00:03:42 Symbiosine Institute.

00:03:43 --> 00:03:46 Andrew Dunkley: Well I think if you go to um,

00:03:47 --> 00:03:49 try to make those kinds of changes in

00:03:50 --> 00:03:52 the psyche of humanity, it's going to be

00:03:52 --> 00:03:55 a multi generational approach.

00:03:55 --> 00:03:57 It's not going to be something we all just go

00:03:57 --> 00:04:00 to do the next day. Okay, we're

00:04:00 --> 00:04:03 now doing this. It just wouldn't

00:04:03 --> 00:04:04 happen.

00:04:04 --> 00:04:06 Professor Fred Watson: No, you're right, humans don't work that way.

00:04:06 --> 00:04:09 But uh, hopefully with

00:04:09 --> 00:04:12 enough panic from climate

00:04:12 --> 00:04:15 change, some things will change.

00:04:15 --> 00:04:18 Andrew Dunkley: Yes, certainly needs to happen that way.

00:04:18 --> 00:04:19 Professor Fred Watson: Indeed.

00:04:19 --> 00:04:20 Andrew Dunkley: Shall we get down to business?

00:04:21 --> 00:04:22 Professor Fred Watson: Well, why not?

00:04:22 --> 00:04:25 Andrew Dunkley: All right, our very first question uh,

00:04:25 --> 00:04:28 is focusing um, on our uh,

00:04:28 --> 00:04:31 twin planet. Um, when we say twin,

00:04:31 --> 00:04:33 we're the good twin, it's the evil twin.

00:04:33 --> 00:04:36 We're talking about Venus. Uh, I mean

00:04:36 --> 00:04:39 size wise it's similar to Earth. In fact

00:04:39 --> 00:04:41 everything about it is similar to Earth.

00:04:41 --> 00:04:43 Size, mass, gravity, that kind of thing.

00:04:43 --> 00:04:46 Except it's got a God awful

00:04:46 --> 00:04:49 weather pattern and it doesn't have a

00:04:49 --> 00:04:51 moon. And that's the subject of this

00:04:51 --> 00:04:53 particular storey because they're trying to

00:04:53 --> 00:04:54 figure out why.

00:04:55 --> 00:04:58 Professor Fred Watson: Indeed. That's right. Uh, yes. Often referred

00:04:58 --> 00:05:01 to as Earth's ugly sister because of all the

00:05:01 --> 00:05:02 things that you've mentioned, the

00:05:02 --> 00:05:05 similarities and um, as we're

00:05:05 --> 00:05:07 recording it's very prominent in our evening

00:05:07 --> 00:05:10 skies at the moment. Really can't fail to see

00:05:10 --> 00:05:13 the planet Venus as it uh, approaches its

00:05:13 --> 00:05:15 greatest distance from the sun. Greatest

00:05:15 --> 00:05:17 angular distance from the sun. In fact it may

00:05:17 --> 00:05:19 even have passed it. I've kind of lost track

00:05:19 --> 00:05:22 with my confinement to hospitals and things

00:05:22 --> 00:05:24 of that sort recently. Uh, but it is still

00:05:24 --> 00:05:26 very spectacular in the evening sky. Anyway,

00:05:26 --> 00:05:29 a planet about the size of ours, uh,

00:05:29 --> 00:05:32 of which we know a lot um, thanks

00:05:32 --> 00:05:34 to orbiting spacecraft which have Carried

00:05:34 --> 00:05:37 with them radar, uh, uh, equipment in

00:05:37 --> 00:05:39 order to be able to map m the surface.

00:05:39 --> 00:05:42 Because the atmosphere of course is largely

00:05:42 --> 00:05:44 opaque, uh you can penetrate the

00:05:44 --> 00:05:47 atmosphere down to surface in infrared. That

00:05:47 --> 00:05:49 was done actually by one of my former

00:05:49 --> 00:05:51 colleagues at the Anglo Australian Telescope,

00:05:51 --> 00:05:54 David Allen, back in the 1990s I

00:05:54 --> 00:05:57 think, or maybe 1980s using infrared

00:05:57 --> 00:05:59 uh radiation managed to see the surface of

00:05:59 --> 00:06:02 Venus which is quite a uh, spectacular

00:06:02 --> 00:06:05 outcome. Um, but the best way to do it

00:06:05 --> 00:06:06 is with radar and from that we can see the

00:06:06 --> 00:06:07 topography.

00:06:07 --> 00:06:10 This jury I think is still out on whether

00:06:10 --> 00:06:13 uh Venus has plate tectonics because we see

00:06:13 --> 00:06:16 conflicting results. Uh, but

00:06:16 --> 00:06:18 the one thing that we do know for absolute

00:06:18 --> 00:06:21 certain uh, is that it doesn't have a moon.

00:06:21 --> 00:06:24 Um, uh, Mercury and Venus, the only two

00:06:24 --> 00:06:26 planets in the solar system that do not

00:06:26 --> 00:06:29 have satellites, at least do not have

00:06:29 --> 00:06:32 natural satellites. Um

00:06:33 --> 00:06:36 so the question that you would ask as a

00:06:36 --> 00:06:39 scientist is that significant is

00:06:39 --> 00:06:41 that um, you know, is

00:06:41 --> 00:06:44 it just happen, just the fact that

00:06:44 --> 00:06:47 the planet happens not to have a moon

00:06:47 --> 00:06:50 or whether it is a uh,

00:06:50 --> 00:06:53 situation where Venus once did have a

00:06:53 --> 00:06:56 moon. Um, given that moons are pretty common

00:06:56 --> 00:06:58 throughout the solar system, perhaps uh,

00:06:58 --> 00:07:00 there was a similar formation event to the

00:07:00 --> 00:07:03 event that formed our moon when uh, Theia,

00:07:03 --> 00:07:06 the object size of Mars clouted the Earth in

00:07:06 --> 00:07:09 the early history of the solar system and

00:07:09 --> 00:07:11 eventually that coalesced to form the moon

00:07:11 --> 00:07:14 which uh, both way. I read a headline not

00:07:14 --> 00:07:16 very long ago that looks as though that

00:07:16 --> 00:07:18 formation of the moon from that debris cloud

00:07:18 --> 00:07:20 might have happened very very quickly. And I

00:07:20 --> 00:07:22 can't remember how quickly it was but it was

00:07:22 --> 00:07:25 surprisingly quickly. You might have seen

00:07:25 --> 00:07:26 that too I

00:07:26 --> 00:07:28 Andrew Dunkley: think uh, Jonty and I did actually do that

00:07:28 --> 00:07:28 Storey.

00:07:28 --> 00:07:29 Professor Fred Watson: Okay, great.

00:07:30 --> 00:07:32 Andrew Dunkley: Yeah, um, so uh,

00:07:33 --> 00:07:35 yeah I was trying to find it actually through

00:07:35 --> 00:07:37 my notes. M seen my notes.

00:07:38 --> 00:07:40 These are all past episodes, all my notes.

00:07:41 --> 00:07:43 Professor Fred Watson: But I could have nicely filed Ye

00:07:44 --> 00:07:46 Andrew Dunkley: it's just a neat pile. It's not file

00:07:48 --> 00:07:50 uh, but um, I couldn't find it. But yeah, I

00:07:50 --> 00:07:52 was trying to remember what we did about

00:07:52 --> 00:07:54 Venus previously and that was it.

00:07:54 --> 00:07:57 Professor Fred Watson: Yes, okay. Anyway,

00:07:57 --> 00:07:59 um, yes, so Venus may have had the same

00:08:00 --> 00:08:02 experience. Uh what uh,

00:08:03 --> 00:08:05 would have happened though if uh, Venus had

00:08:05 --> 00:08:08 had a moon? Why isn't it there now? And

00:08:08 --> 00:08:10 so this is the uh

00:08:11 --> 00:08:14 thesis of ah, a group of scientists

00:08:14 --> 00:08:17 um led by um, Stephen Cain who's at

00:08:17 --> 00:08:20 the University of California Riverside. Uh

00:08:20 --> 00:08:22 he uh and his colleagues

00:08:22 --> 00:08:25 have looked to see you know

00:08:26 --> 00:08:29 what might have happened had Venus had

00:08:29 --> 00:08:31 a moon. So it's all done by modelling of

00:08:31 --> 00:08:33 course, um,

00:08:34 --> 00:08:37 their Comments more or less, as we've just

00:08:37 --> 00:08:39 related, uh, this is a comment from Stephen.

00:08:40 --> 00:08:42 Venus undoubtedly experienced large impacts

00:08:42 --> 00:08:45 just as as Earth has and so has had

00:08:45 --> 00:08:48 m as much if not more opportunity to form

00:08:48 --> 00:08:50 a moon similar to what we see in our own

00:08:50 --> 00:08:50 skies.

00:08:51 --> 00:08:54 So, all right, put a moon there in your

00:08:54 --> 00:08:57 modelling um, and see

00:08:57 --> 00:09:00 what happens. And this is the

00:09:00 --> 00:09:02 interesting bit because um,

00:09:02 --> 00:09:05 there is a really very neat

00:09:05 --> 00:09:07 explanation for why Venus doesn't have a

00:09:07 --> 00:09:10 moon. That comes almost straight

00:09:10 --> 00:09:13 out of the modelling. Uh, and it's all about

00:09:14 --> 00:09:16 what the they describe as the gravitational

00:09:16 --> 00:09:18 tug of war between Venus, a

00:09:18 --> 00:09:21 hypothetical moon and the sun. And

00:09:21 --> 00:09:24 if you track this over billions of years,

00:09:25 --> 00:09:27 what you get is a situation

00:09:29 --> 00:09:32 opposite to what we've got on um,

00:09:32 --> 00:09:34 planet Earth. And that is that

00:09:34 --> 00:09:37 the laws of physics dictate uh, that

00:09:37 --> 00:09:39 because um, there is

00:09:40 --> 00:09:42 basically an impulse given to the moon

00:09:43 --> 00:09:45 from the Earth's rotation slowing down,

00:09:46 --> 00:09:48 uh, it means the moon is drifting away from

00:09:48 --> 00:09:51 Earth. And that's um, something we've

00:09:51 --> 00:09:53 talked about, it's well known, well

00:09:53 --> 00:09:56 established, one of those phenomena that

00:09:56 --> 00:09:59 we recognise as being scientific facts.

00:09:59 --> 00:10:02 But uh, what they

00:10:02 --> 00:10:04 found, what these researchers found when they

00:10:04 --> 00:10:07 put the same sort of analysis into Venus and

00:10:07 --> 00:10:10 a moon, uh, the moon would go the other way.

00:10:10 --> 00:10:13 Uh, it would basically eventually,

00:10:14 --> 00:10:17 um, it would start to drift

00:10:17 --> 00:10:19 inwards towards Venus

00:10:20 --> 00:10:22 and spiral towards the

00:10:22 --> 00:10:25 planet, eventually passing within the

00:10:25 --> 00:10:28 Roche limit, which is where you can't have

00:10:28 --> 00:10:31 something uh, staying together because of the

00:10:31 --> 00:10:33 competing gravitational pull on one side and

00:10:33 --> 00:10:36 the other what we call the tidal effect.

00:10:37 --> 00:10:39 So it would break up, um, and

00:10:40 --> 00:10:43 uh, even a

00:10:43 --> 00:10:46 big moon, uh, would not

00:10:46 --> 00:10:47 necessarily survive.

00:10:47 --> 00:10:50 Uh, in fact one of the comments that Stephen

00:10:50 --> 00:10:53 Kane makes is an interesting aspect is that a

00:10:53 --> 00:10:56 heavier moon is destroyed faster since

00:10:56 --> 00:10:58 a massive moon would drain Venus's spin so

00:10:58 --> 00:11:01 efficiently that it hastens its destruction.

00:11:02 --> 00:11:05 Uh, and so um, that

00:11:05 --> 00:11:08 is the basic outcome of

00:11:08 --> 00:11:10 this work. I um, think

00:11:12 --> 00:11:14 in uh, fact I'm sure that they looked

00:11:14 --> 00:11:17 at a whole variety these

00:11:17 --> 00:11:20 researchers of different scenarios. Uh,

00:11:20 --> 00:11:22 and one of the questions they addressed was

00:11:23 --> 00:11:25 are there any circumstances under which a

00:11:25 --> 00:11:28 Venusian m moon could actually survive?

00:11:29 --> 00:11:32 And the comments that Stephen, uh, Kane made

00:11:32 --> 00:11:34 on this are uh, survival came down to two

00:11:34 --> 00:11:37 main things. Venus had to be

00:11:37 --> 00:11:39 spinning fast when the moon formed

00:11:40 --> 00:11:43 with a day shorter than about 12 hours. And

00:11:43 --> 00:11:45 the moon couldn't be too massive up to

00:11:45 --> 00:11:48 roughly the mass of our own moon. In that

00:11:48 --> 00:11:50 narrow window, the moon migrates outwards and

00:11:50 --> 00:11:53 stabilises much as the Earth did. Outside

00:11:53 --> 00:11:56 that range, the moon is unfortunately

00:11:56 --> 00:11:58 doomed to be consumed by Venus.

00:11:59 --> 00:12:01 So a Surviving moon would have to be

00:12:02 --> 00:12:05 modest in size, orbiting a rapidly spinning

00:12:05 --> 00:12:07 early Venus, which are conditions that don't

00:12:07 --> 00:12:09 match what we think the early Venus was

00:12:09 --> 00:12:10 actually like.

00:12:11 --> 00:12:13 Uh, and so, you know, the

00:12:14 --> 00:12:15 upshot of this is,

00:12:16 --> 00:12:19 um, maybe indeed Venus did

00:12:19 --> 00:12:22 have a moon, which eventually was

00:12:22 --> 00:12:24 essentially gobbled up by Venus. It was

00:12:25 --> 00:12:27 drifted inwards, uh, was torn apart and the

00:12:27 --> 00:12:30 debris essentially rained down on the planet.

00:12:31 --> 00:12:34 Um, the

00:12:34 --> 00:12:37 next step would be essentially

00:12:38 --> 00:12:41 to look for any, what you might

00:12:41 --> 00:12:42 call geological evidence,

00:12:44 --> 00:12:46 uh, on Venus that would

00:12:47 --> 00:12:49 give you some

00:12:49 --> 00:12:52 hints that this is what happened. Uh,

00:12:52 --> 00:12:54 forgive me, Andrew, because I think I'm about

00:12:54 --> 00:12:54 to sneeze.

00:12:55 --> 00:12:57 Andrew Dunkley: Yeah, I've been fighting one for the last few

00:12:57 --> 00:12:57 minutes too.

00:12:58 --> 00:13:01 Professor Fred Watson: Why are we both sneezing? It's the time of

00:13:01 --> 00:13:04 year. That's right. Uh, let me, um, quote

00:13:04 --> 00:13:06 again, uh, Stephen Cain. Uh,

00:13:06 --> 00:13:09 finding direct observational evidence is

00:13:09 --> 00:13:12 pretty tough. A moon lost billions

00:13:12 --> 00:13:14 of years ago would leave little to no direct

00:13:14 --> 00:13:16 trace we can point a telescope at today

00:13:17 --> 00:13:19 so we can't observe the event itself.

00:13:20 --> 00:13:22 However, there are indirect avenues. For

00:13:22 --> 00:13:25 example, if a moon was destroyed

00:13:25 --> 00:13:28 and its debris rained down on Venus, it could

00:13:28 --> 00:13:30 have left a chemical fingerprint in the

00:13:30 --> 00:13:33 planet's surface or atmosphere. And upcoming

00:13:33 --> 00:13:35 missions to Venus, including NASA's da

00:13:35 --> 00:13:38 Vinci, uh, will measure the

00:13:38 --> 00:13:41 atmospheric composition in detail. So it is

00:13:41 --> 00:13:44 possible, uh, that we might eventually, um,

00:13:45 --> 00:13:47 find something. Uh, one other comment from

00:13:47 --> 00:13:50 Stephen Cain is there's a broader test beyond

00:13:50 --> 00:13:52 our solar system because our results predict

00:13:52 --> 00:13:55 that slowly rotating Venus, like planets

00:13:55 --> 00:13:58 around other stars, should generically

00:13:58 --> 00:14:00 lack large moons. So as astronomers

00:14:00 --> 00:14:03 begin searching for moons around exoplanets,

00:14:03 --> 00:14:06 that's a prediction that can eventually be

00:14:06 --> 00:14:09 checked against real data. Uh, so, yeah, it's

00:14:09 --> 00:14:11 very, very nice piece of work. Uh, I think a

00:14:11 --> 00:14:13 very interesting outcome as well.

00:14:13 --> 00:14:16 Andrew Dunkley: Yeah, and it sort of harps back to a storey

00:14:16 --> 00:14:19 from a few weeks ago about, uh, how they

00:14:19 --> 00:14:22 do think they have found continental size

00:14:24 --> 00:14:26 anomalies, um, deep in our

00:14:26 --> 00:14:29 crust that suggests parts of Theia

00:14:29 --> 00:14:30 exist.

00:14:30 --> 00:14:32 Professor Fred Watson: Might be parts of Theia. That's right, yes,

00:14:32 --> 00:14:33 indeed. Yeah.

00:14:33 --> 00:14:35 Andrew Dunkley: So, yeah, then you can draw a similarity

00:14:35 --> 00:14:37 there. And so, yeah, there probably is

00:14:37 --> 00:14:40 evidence if that's indeed what happened. But,

00:14:40 --> 00:14:41 yeah. Ah, how do you find it?

00:14:43 --> 00:14:45 Professor Fred Watson: Well, um, we're very, uh, resourceful, uh,

00:14:46 --> 00:14:47 in that regard, I think. I think, um,

00:14:48 --> 00:14:50 scientists, particularly astronomers, because

00:14:50 --> 00:14:51 they, you know, they've got.

00:14:52 --> 00:14:55 All they've got is what comes in, usually on

00:14:55 --> 00:14:57 electromagnetic radiation, apart from a few

00:14:57 --> 00:15:00 satellites going here and there. Uh, but,

00:15:00 --> 00:15:02 yes, um, uh,

00:15:03 --> 00:15:06 uh, I think we might well

00:15:06 --> 00:15:08 get some hints as to whether this has

00:15:08 --> 00:15:09 happened in the past or not.

00:15:09 --> 00:15:12 Andrew Dunkley: Yeah. Okay. Uh if you'd like to read up

00:15:12 --> 00:15:15 on that storey uh great article@spare.com or

00:15:15 --> 00:15:18 you can uh see the pre peer

00:15:18 --> 00:15:21 reviewed paper on the repository site

00:15:21 --> 00:15:23 arXiv. This is space Nuts with Andrew

00:15:23 --> 00:15:25 Dunkley and Professor Fred Watson Watson.

00:15:28 --> 00:15:31 Professor Fred Watson: Roger, you're lots Space Nuts.

00:15:31 --> 00:15:34 Andrew Dunkley: Okay, let's uh get close to

00:15:34 --> 00:15:37 home. In fact uh, we're getting right down

00:15:37 --> 00:15:39 and dirty into our own atmosphere with this

00:15:39 --> 00:15:41 storey and it's got to do with satellite

00:15:41 --> 00:15:44 pollution. Now the number of satellites that

00:15:44 --> 00:15:46 are starting to appear in our sky is

00:15:47 --> 00:15:49 somewhat um, disturbing when it comes to

00:15:50 --> 00:15:52 um optical astronomy. In fact I

00:15:52 --> 00:15:55 saw a photo the other day where this problem

00:15:55 --> 00:15:58 was exhibited. Uh where they'd done a little

00:15:58 --> 00:16:01 bit of time lapse and the

00:16:01 --> 00:16:04 satellite that image were

00:16:04 --> 00:16:07 horrifying. Uh if you're an astronomer they

00:16:07 --> 00:16:08 were probably really interesting for

00:16:09 --> 00:16:12 other people. But uh, it looked the same as

00:16:12 --> 00:16:15 um the contrails that you see

00:16:15 --> 00:16:18 airliners leaving the sky. Um

00:16:19 --> 00:16:21 but it was actually the light reflection

00:16:21 --> 00:16:24 images of the uh satellites. But the

00:16:24 --> 00:16:26 other problem with them is when they come

00:16:26 --> 00:16:29 back down uh, they burn up and

00:16:29 --> 00:16:31 what happens to all that stuff? And that's

00:16:31 --> 00:16:33 the nuts and bolts of this storey.

00:16:34 --> 00:16:36 They've chased a couple down to try and

00:16:36 --> 00:16:39 figure out what happens to you know

00:16:39 --> 00:16:41 everything that burns off them.

00:16:42 --> 00:16:44 Professor Fred Watson: Exactly. So and um, it is a

00:16:45 --> 00:16:47 um. This uh essentially

00:16:47 --> 00:16:49 experiment is very well timed because at the

00:16:49 --> 00:16:52 moment we're with the Starlink

00:16:52 --> 00:16:54 constellation which I think is kind of

00:16:54 --> 00:16:56 already past 12 spacecraft. Uh

00:16:58 --> 00:17:00 not all of them functioning. Um

00:17:01 --> 00:17:03 those are re entering at about one a day.

00:17:04 --> 00:17:06 That's the current rate. And every time one

00:17:06 --> 00:17:09 of those re uh enters the atmosphere it burns

00:17:09 --> 00:17:12 up at about 90 kilometres or thereabouts

00:17:12 --> 00:17:15 above the Earth's surface and its

00:17:15 --> 00:17:18 contents, its metallic contents become part

00:17:18 --> 00:17:21 of the upper atmosphere. Uh and we

00:17:21 --> 00:17:24 already are seeing um, higher levels of

00:17:24 --> 00:17:26 certain oxides of aluminium and things of

00:17:26 --> 00:17:26 that sort.

00:17:26 --> 00:17:29 Uh uh that are probably the result of

00:17:29 --> 00:17:32 these uh reentering satellites. So

00:17:33 --> 00:17:35 uh, the European Space

00:17:36 --> 00:17:38 Agency uh has

00:17:39 --> 00:17:41 I uh think uh in

00:17:41 --> 00:17:44 collaboration with a number of other

00:17:44 --> 00:17:46 organisations. Uh what they've done

00:17:46 --> 00:17:49 is they have decided that they're going to

00:17:49 --> 00:17:52 cheque this out directly. And the way they've

00:17:52 --> 00:17:55 done that is by hiring a private jet as

00:17:55 --> 00:17:58 you do. Um and it's

00:17:59 --> 00:18:01 using uh, that uh private jet. They've

00:18:01 --> 00:18:04 basically chased a pair of reentering

00:18:04 --> 00:18:07 satellites. Um both were due to re

00:18:07 --> 00:18:10 enter uh at about the same um

00:18:10 --> 00:18:13 place I think a day apart. Um and so

00:18:13 --> 00:18:15 what they've done is um, actually

00:18:16 --> 00:18:18 basically followed these In a jet which

00:18:18 --> 00:18:21 is festooned with uh

00:18:21 --> 00:18:23 spectrometers, images, uh and

00:18:23 --> 00:18:26 all of the equipment that we use to try

00:18:26 --> 00:18:29 and learn about what's happening when

00:18:29 --> 00:18:32 things burn up in space. Uh and

00:18:32 --> 00:18:35 so uh, um essentially

00:18:35 --> 00:18:38 uh the satellites tracked

00:18:38 --> 00:18:41 uh in detail uh I like

00:18:41 --> 00:18:44 um the spacecraft that

00:18:44 --> 00:18:47 they chose because there was a constellation

00:18:47 --> 00:18:49 called Cluster which I think we might have

00:18:49 --> 00:18:51 talked about many years ago. A European Space

00:18:51 --> 00:18:54 Agency constellation which had four

00:18:54 --> 00:18:57 individual spacecraft uh which

00:18:57 --> 00:18:59 were named after well known

00:18:59 --> 00:19:02 dances, Tango, samba, rumba and

00:19:02 --> 00:19:03 Salsa.

00:19:03 --> 00:19:06 Uh were the quartet of uh the Cluster

00:19:06 --> 00:19:09 spacecraft and they actually were studying

00:19:09 --> 00:19:12 the way the Earth's magnetic field uh

00:19:12 --> 00:19:15 interacts with the solar wind. And they were

00:19:15 --> 00:19:17 launched back in I think back in the 90s.

00:19:17 --> 00:19:20 It's a long, long time ago. But their

00:19:20 --> 00:19:22 orbits um were

00:19:23 --> 00:19:26 decaying and in fact uh, Rumba and Salsa

00:19:26 --> 00:19:29 I think decayed quite some time ago. So what

00:19:29 --> 00:19:32 was uh in question here was since

00:19:32 --> 00:19:34 they you know these spacecraft are still

00:19:34 --> 00:19:36 sending telemetry back so you know what their

00:19:36 --> 00:19:39 velocity is, you when and where these things

00:19:39 --> 00:19:41 are going to re. Enter the atmosphere. Uh and

00:19:41 --> 00:19:44 it was Tango and Samba which

00:19:44 --> 00:19:47 were basically uh,

00:19:47 --> 00:19:50 um they had controlled RE entry and

00:19:50 --> 00:19:53 it was basically that re entry that was uh

00:19:53 --> 00:19:56 observed by this mission using ah

00:19:56 --> 00:19:59 a chaser jet, if I can put it that way

00:19:59 --> 00:20:02 uh over the South Pacific Ocean. So

00:20:02 --> 00:20:05 uh, what we've seen I think is that this was

00:20:05 --> 00:20:07 successful. There's been um

00:20:09 --> 00:20:11 a bit of a report saying that um

00:20:12 --> 00:20:14 the outcome of the experiment was successful

00:20:14 --> 00:20:16 and that they got the data that they wanted.

00:20:16 --> 00:20:19 I'm uh not sure whether we yet have the

00:20:19 --> 00:20:21 details of what that

00:20:21 --> 00:20:24 analysis was, you know in terms of

00:20:24 --> 00:20:27 what the exact uh effects on the

00:20:27 --> 00:20:30 atmosphere and the byproducts that

00:20:30 --> 00:20:32 came from uh the reentry of these two

00:20:32 --> 00:20:33 spacecraft.

00:20:33 --> 00:20:35 So I think those results are still yet

00:20:36 --> 00:20:38 uh to be described but at least the

00:20:38 --> 00:20:40 experiments are worked. Uh apparently there

00:20:40 --> 00:20:43 were eight scientists on board this aircraft

00:20:43 --> 00:20:46 and they um observed

00:20:46 --> 00:20:49 the satellites from about 90 kilometres

00:20:49 --> 00:20:52 down to something like 65 to

00:20:52 --> 00:20:54 70 kilometres when they stopped, basically

00:20:54 --> 00:20:57 stopped burning up. Uh so

00:20:58 --> 00:21:00 they were then completely vaporised. Uh so

00:21:00 --> 00:21:03 these details uh as I said we hope we will

00:21:03 --> 00:21:06 find a little bit more uh as the results

00:21:06 --> 00:21:09 come from that group of

00:21:09 --> 00:21:11 scient, they've

00:21:11 --> 00:21:13 Andrew Dunkley: finished analysing the data and

00:21:14 --> 00:21:16 start uh publishing uh it could

00:21:16 --> 00:21:18 turn into something quite controversial

00:21:18 --> 00:21:21 because if they reveal that there's some

00:21:21 --> 00:21:24 really nasty stuff coming out of all of this,

00:21:24 --> 00:21:26 you know a handful of satellites doing this

00:21:26 --> 00:21:29 probably no big deal but we're going to be

00:21:29 --> 00:21:31 talking over decades to come

00:21:32 --> 00:21:35 tens of thousands burning up,

00:21:35 --> 00:21:36 probably more.

00:21:36 --> 00:21:39 Professor Fred Watson: Yeah. When it's one a day, uh, which it is

00:21:39 --> 00:21:41 now, then, uh, you're potentially in trouble.

00:21:41 --> 00:21:43 And you're absolutely right, Andrew, because

00:21:44 --> 00:21:46 one of the possibilities is something

00:21:47 --> 00:21:50 we thought we'd licked back in the 1980s, and

00:21:50 --> 00:21:53 that's ozone depletion. Um, that's one

00:21:53 --> 00:21:56 of the possible outcomes of this. And that

00:21:56 --> 00:21:58 would then become a really hot political

00:22:00 --> 00:22:02 hot potato politically. Uh, given

00:22:02 --> 00:22:04 that you've now got people saying, well,

00:22:04 --> 00:22:06 we've got all these pollutants that are

00:22:06 --> 00:22:08 actually starting to affect the behaviour of

00:22:08 --> 00:22:10 the upper atmosphere. And on the other side

00:22:10 --> 00:22:11 of the coin, you've got people saying, well,

00:22:11 --> 00:22:13 we need Starlink because it's actually a

00:22:13 --> 00:22:15 vital, uh, service, it's vital

00:22:15 --> 00:22:18 infrastructure now on so many fronts. You've

00:22:18 --> 00:22:20 got a really quite interesting situation

00:22:20 --> 00:22:21 emerging, I think.

00:22:21 --> 00:22:22 Andrew Dunkley: Sure have.

00:22:22 --> 00:22:23 Professor Fred Watson: And,

00:22:24 --> 00:22:25 Andrew Dunkley: yeah,

00:22:28 --> 00:22:30 where do you point the finger, if you want to

00:22:30 --> 00:22:33 put it that way? Uh, how do you, um,

00:22:33 --> 00:22:35 curtail these effects and whose

00:22:35 --> 00:22:36 responsibility does it become?

00:22:38 --> 00:22:40 Professor Fred Watson: Yeah, you start looking, I think, at, um,

00:22:40 --> 00:22:42 what you make your spacecraft out of. The

00:22:42 --> 00:22:44 Japanese have demonstrated that you can make

00:22:44 --> 00:22:46 wooden spacecraft and operate them

00:22:46 --> 00:22:48 successfully. Uh, and I think wood

00:22:48 --> 00:22:51 is one of the more benign, uh,

00:22:51 --> 00:22:54 materials, um, that would burn up. Of

00:22:54 --> 00:22:56 course, you still got soot and carbon coming

00:22:56 --> 00:22:58 off that. But, um, it might not be the

00:22:59 --> 00:23:01 aluminium that, um, is

00:23:01 --> 00:23:04 certainly the biggest constituent of, of what

00:23:04 --> 00:23:06 is coming from present satellite reentries.

00:23:07 --> 00:23:10 Andrew Dunkley: Yes, indeed. M. So, yeah, it's a case of,

00:23:10 --> 00:23:11 watch this. Space.

00:23:11 --> 00:23:14 Uh, we will probably learn more about this

00:23:14 --> 00:23:17 and, uh, we'll tell you all about it when

00:23:17 --> 00:23:19 that day comes. Um, but they'll be analysing

00:23:19 --> 00:23:21 the data at the moment and,

00:23:22 --> 00:23:24 uh, we hope it's good news, but I've got a

00:23:24 --> 00:23:25 feeling it won't be, Fred Watson.

00:23:26 --> 00:23:28 Professor Fred Watson: M. Yeah, I think you're right.

00:23:28 --> 00:23:31 Andrew Dunkley: Okay. Uh, that is a storey you can Also

00:23:31 --> 00:23:34 read@spare.com this is Space

00:23:34 --> 00:23:36 Nuts. Andrew Dunc, frankly, here with

00:23:36 --> 00:23:37 Fred Watson Watson,

00:23:41 --> 00:23:44 Professor Fred Watson: Tranquilly Base here. The Eagle has landed.

00:23:44 --> 00:23:45 Space Nuts.

00:23:46 --> 00:23:48 Andrew Dunkley: Our final storey. Uh, Fred Watson,

00:23:48 --> 00:23:51 takes us into the realm of science fiction,

00:23:51 --> 00:23:54 at least in part. Uh, they have just

00:23:54 --> 00:23:56 unveiled what might be

00:23:56 --> 00:23:59 the new United, uh, States

00:23:59 --> 00:24:01 Space Force uniforms.

00:24:02 --> 00:24:05 And they've got tongues wagging

00:24:05 --> 00:24:07 because they've drawn some similarities

00:24:07 --> 00:24:10 between the uniforms. And when I first saw

00:24:10 --> 00:24:12 them, my mind immediately went to,

00:24:13 --> 00:24:15 um, SS uniforms of World War II.

00:24:15 --> 00:24:16 Professor Fred Watson: Exactly.

00:24:17 --> 00:24:19 Andrew Dunkley: And, uh, that is the controversy because they

00:24:19 --> 00:24:22 do not sort of. I mean, it's the first

00:24:22 --> 00:24:24 thing that comes to mind when you look at

00:24:24 --> 00:24:27 these designs which have just been unveiled.

00:24:28 --> 00:24:30 Professor Fred Watson: Um, and Just to clarify where this has come

00:24:30 --> 00:24:33 from. It's come from Truth Social. Uh, it's

00:24:33 --> 00:24:35 one of uh, President Trump's

00:24:37 --> 00:24:39 basically, uh, uh, one of his posts on Truth

00:24:39 --> 00:24:42 Social. The um, as yet

00:24:42 --> 00:24:44 unconfirmed design is how it's being

00:24:44 --> 00:24:44 described.

00:24:45 --> 00:24:47 But yes, um, that was my thought too

00:24:48 --> 00:24:49 when I looked at this. I thought, wait a

00:24:49 --> 00:24:51 minute, I've seen that sort of thing before.

00:24:52 --> 00:24:55 Um, but you are ah, probably aware as well of

00:24:55 --> 00:24:58 the sort of science fiction links that there

00:24:58 --> 00:25:00 are with uh, with this, where this

00:25:00 --> 00:25:02 uniform is said to have come from.

00:25:02 --> 00:25:05 Andrew Dunkley: Yes, this, uh, back in the

00:25:05 --> 00:25:08 90s, the late 90s, uh, 1997, there was a

00:25:08 --> 00:25:10 movie released based on a book called

00:25:10 --> 00:25:13 Starship Troopers. And

00:25:13 --> 00:25:14 anybody who's watched that film, and I've

00:25:14 --> 00:25:17 watched it multiple times, it's a bit

00:25:17 --> 00:25:20 tongue in cheek. Um, there's a lot of,

00:25:20 --> 00:25:23 um, to use the Australian vernacular,

00:25:23 --> 00:25:26 Jingo is a m. Minute. Um, but it

00:25:26 --> 00:25:29 portrays a, ah, human society that is

00:25:29 --> 00:25:32 very, very authoritari, very,

00:25:33 --> 00:25:35 very super aggressive, very um,

00:25:36 --> 00:25:38 competitive. Uh, lots of.

00:25:39 --> 00:25:41 It would be a very tense place to live

00:25:42 --> 00:25:44 if Earth as we know it,

00:25:45 --> 00:25:48 um, was the way Starship Troopers

00:25:48 --> 00:25:51 portrays human life. And they're at war

00:25:51 --> 00:25:54 against the bugs, um, who live

00:25:54 --> 00:25:57 on a planet called Clandathu. You know what's

00:25:57 --> 00:25:58 sad about this, Fred Watson? I'm doing it all

00:25:58 --> 00:26:01 from memory. And they have been shooting

00:26:01 --> 00:26:04 asteroids at ear. And um, in the

00:26:04 --> 00:26:06 movie they destroy the city of Buenos Aires.

00:26:06 --> 00:26:09 And that sort of causes um,

00:26:09 --> 00:26:12 the humans to up the ante in terms of

00:26:12 --> 00:26:15 trying to eliminate the bugs. Uh, and

00:26:15 --> 00:26:18 so it goes on. But what's striking about it,

00:26:18 --> 00:26:20 not only the authoritarian,

00:26:21 --> 00:26:24 um, nature of the military in

00:26:25 --> 00:26:27 this film, is the uniforms.

00:26:28 --> 00:26:31 They are dead set. Um, just

00:26:31 --> 00:26:33 like the uniforms that have been

00:26:33 --> 00:26:36 suggested as the new U.S. space Force

00:26:36 --> 00:26:38 uniforms. I did a bit of research on this,

00:26:38 --> 00:26:39 Fred Watson.

00:26:39 --> 00:26:42 Um, uh, the uniforms in

00:26:42 --> 00:26:45 um, the 1997 film

00:26:45 --> 00:26:48 Starship Troopers were deliberately designed

00:26:48 --> 00:26:50 by a costume designer, Ellen

00:26:50 --> 00:26:53 mirojink, uh, to evoke

00:26:53 --> 00:26:55 fascist aesthetics.

00:26:55 --> 00:26:56 Professor Fred Watson: Yeah, so.

00:26:56 --> 00:26:59 Andrew Dunkley: So they're basically designed

00:26:59 --> 00:27:01 around the Nazi military uniform.

00:27:02 --> 00:27:04 That was deliberate. That was done on

00:27:04 --> 00:27:06 purpose. And now we're seeing These new

00:27:06 --> 00:27:09 uniforms, 2026,

00:27:09 --> 00:27:12 um, being unveiled, um, based

00:27:12 --> 00:27:15 on the uniforms from Starship Troopers

00:27:15 --> 00:27:16 and um,

00:27:18 --> 00:27:21 Star Wars. If you remember, um, the Empire

00:27:21 --> 00:27:24 uniforms were of a similar ilk. They

00:27:24 --> 00:27:26 are, look, don't get me wrong, they're quite

00:27:26 --> 00:27:29 striking, quite striking. But

00:27:30 --> 00:27:33 they immediately put you in um,

00:27:33 --> 00:27:35 a mindset of going, whoa.

00:27:36 --> 00:27:36 Professor Fred Watson: What?

00:27:39 --> 00:27:42 Andrew Dunkley: You're not impressed? You're just going,

00:27:43 --> 00:27:46 hello. What are we thinking here? Why are we

00:27:46 --> 00:27:49 doing it this way. That's kind of the

00:27:49 --> 00:27:50 reaction I had head.

00:27:51 --> 00:27:54 Professor Fred Watson: And me too. Um, when, when I saw

00:27:54 --> 00:27:56 it was the boots, I noticed first I thought,

00:27:56 --> 00:27:57 wait a minute, I've seen that sort of thing

00:27:57 --> 00:27:58 before.

00:27:58 --> 00:27:59 Andrew Dunkley: Yeah, Jack Boots.

00:27:59 --> 00:28:00 Professor Fred Watson: Yeah, exactly.

00:28:00 --> 00:28:02 Andrew Dunkley: More or less. Yeah, yeah, they're quite,

00:28:02 --> 00:28:05 um, I mean, I, I think

00:28:05 --> 00:28:08 uniforms are an amazing thing. Uh, I, I don't

00:28:08 --> 00:28:10 know where they originated. I, I did look it

00:28:10 --> 00:28:13 up once and I, I, I think it was the British

00:28:13 --> 00:28:16 or no, the Romans. The Romans, um, that

00:28:16 --> 00:28:18 invented uniforms. But, um,

00:28:19 --> 00:28:21 everybody has them now and, and some of them

00:28:21 --> 00:28:23 are incredible. I mean, uniforms for some

00:28:23 --> 00:28:26 reason make human beings look better

00:28:27 --> 00:28:29 somehow. Um, and

00:28:31 --> 00:28:33 these ones, I don't know if you're going to

00:28:33 --> 00:28:36 get the right kind of psychological

00:28:36 --> 00:28:39 reaction when, if they

00:28:39 --> 00:28:41 go down this road. And that's a, that's a big

00:28:41 --> 00:28:41 if, I guess.

00:28:43 --> 00:28:46 Professor Fred Watson: I don't know where this storey's going

00:28:46 --> 00:28:49 really, Andrew. And, um, you know, what

00:28:49 --> 00:28:52 we are likely to see coming out of the Space

00:28:52 --> 00:28:54 Force itself rather than just coming from the

00:28:54 --> 00:28:57 President's fertile, uh, mind.

00:28:58 --> 00:29:00 But, um, yes, I didn't find it

00:29:00 --> 00:29:03 something that cheered me up particularly.

00:29:03 --> 00:29:06 Uh, I thought it was very much along

00:29:06 --> 00:29:08 the lines that you've described something

00:29:08 --> 00:29:10 that we could probably well do with that.

00:29:10 --> 00:29:11 Uniformly so.

00:29:11 --> 00:29:14 Andrew Dunkley: Yeah. But what I would say to, uh, Space

00:29:14 --> 00:29:16 Nuts listeners is have a look for yourself

00:29:17 --> 00:29:19 and be your own judge. Don't, you don't have

00:29:19 --> 00:29:22 to believe what we think. Um, we're just.

00:29:23 --> 00:29:25 As soon as I opened the storey that

00:29:25 --> 00:29:27 Fred Watson sent me, I went, what is this?

00:29:29 --> 00:29:31 Before I read a thing, I saw the picture and

00:29:31 --> 00:29:34 went, what are we looking at here? And then I

00:29:34 --> 00:29:36 read the caption and went, no,

00:29:38 --> 00:29:41 seriously. Ah, anyway, have a look.

00:29:41 --> 00:29:43 Uh, you can see it@, uh,

00:29:43 --> 00:29:45 spaceconnectonline.com

00:29:46 --> 00:29:48 it's um. Yeah, or just do

00:29:49 --> 00:29:51 a search through your favourite search engine

00:29:51 --> 00:29:54 of United States Space Force Service

00:29:54 --> 00:29:57 dress uniform, I think is what it's called.

00:29:57 --> 00:30:00 Um, and. Yeah, well,

00:30:01 --> 00:30:03 we'll leave it to you to decide what you

00:30:03 --> 00:30:06 think. Uh, ah, it's a

00:30:06 --> 00:30:08 difficult one because, uh, it's so divisive.

00:30:09 --> 00:30:11 Just that look in

00:30:11 --> 00:30:14 itself without saying anything, um, would

00:30:14 --> 00:30:17 be instantly divisive, I venture to

00:30:17 --> 00:30:17 say.

00:30:18 --> 00:30:19 Professor Fred Watson: Yeah, you're probably right.

00:30:21 --> 00:30:24 Um, yeah, to me

00:30:24 --> 00:30:26 it just portrays arrogance of a kind that,

00:30:26 --> 00:30:28 um, we could do without.

00:30:28 --> 00:30:30 Andrew Dunkley: Yeah, possibly so.

00:30:30 --> 00:30:30 Professor Fred Watson: All right.

00:30:31 --> 00:30:34 Andrew Dunkley: Uh, yeah, As I said, spaceconnectonline.com

00:30:34 --> 00:30:36 if you want to cheque that out. And I think

00:30:36 --> 00:30:38 we are just about done.

00:30:38 --> 00:30:39 Fred Watson, thank you so much.

00:30:39 --> 00:30:41 Professor Fred Watson: It's a pleasure, Andrew. Always interesting

00:30:41 --> 00:30:43 to chew the fat over these issues, no matter

00:30:43 --> 00:30:46 what they are. We did get away from our

00:30:46 --> 00:30:48 normal stocking trade there, uh, with the

00:30:48 --> 00:30:51 uniforms. It's not often we talk about, uh,

00:30:51 --> 00:30:53 fashion in terms of, um, you know, space

00:30:53 --> 00:30:55 fashion, if I can put it that way.

00:30:55 --> 00:30:57 Andrew Dunkley: Well, that's what it is, isn't it, really?

00:30:57 --> 00:30:58 Space fashion.

00:30:58 --> 00:30:58 Professor Fred Watson: Yeah.

00:30:58 --> 00:31:01 Andrew Dunkley: Well, we've talked about the flight

00:31:01 --> 00:31:02 suits, certainly.

00:31:02 --> 00:31:03 Professor Fred Watson: Yes, we have.

00:31:03 --> 00:31:05 Andrew Dunkley: When they've done major upgrades on those and

00:31:05 --> 00:31:08 their incompatibility between space agencies,

00:31:08 --> 00:31:08 so.

00:31:08 --> 00:31:09 Professor Fred Watson: That's right.

00:31:09 --> 00:31:12 Andrew Dunkley: There's always controversy somewhere, even in

00:31:12 --> 00:31:14 fashion. Uh, thanks, Fred Watson. We'll catch

00:31:14 --> 00:31:15 you on the next episode.

00:31:15 --> 00:31:16 Professor Fred Watson: Sounds great.

00:31:16 --> 00:31:18 Andrew Dunkley: Thank you, Professor Fred Watson Watson,

00:31:18 --> 00:31:20 astronomer at large. And don't forget to

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00:31:49 --> 00:31:51 Uh, and thanks to Huw in the studio, uh, who

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00:31:53 --> 00:31:56 uh, to be the first in line for a Space Force

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00:31:59 --> 00:32:01 And from me, Andrew Dunkley, we'll catch you

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