Mars Oceans Unveiled, Spinning Asteroids & Crew Evacuations
Space Nuts: Exploring the CosmosJanuary 16, 2026
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00:34:0331.23 MB

Mars Oceans Unveiled, Spinning Asteroids & Crew Evacuations

Exploring Mars Oceans, Fastest Asteroids, and ISS Evacuations
In this captivating episode of Space Nuts, hosts Andrew Dunkley and Professor Fred Watson delve into the latest astronomical discoveries and intriguing space news. Join them as they explore new evidence suggesting that Mars once boasted vast oceans, the astonishing characteristics of the fastest spinning asteroid ever recorded, and the unprecedented evacuation of the International Space Station due to a medical issue.
Episode Highlights:
Marsโ€™ Ancient Oceans: Andrew and Fred discuss groundbreaking research revealing that Mars may have once had oceans comparable in size to Earth's Arctic Ocean. They explore the implications of this discovery and what it means for the search for life on the Red Planet.
The Fastest Spinning Asteroid: The hosts introduce the asteroid 2025 MN45, which spins at an incredible rate of one rotation every 1 minute and 53 seconds. They discuss the significance of this finding and what it reveals about the asteroid's composition and history.
ISS Medical Evacuation: Andrew and Fred provide insights into the first-ever crew evacuation from the International Space Station, prompted by a medical issue. They discuss the implications of this event and the protocols in place for astronaut safety.

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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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00:00:00 --> 00:00:01 Andrew Dunkley: Hi there. Thanks for joining us on another

00:00:01 --> 00:00:04 episode of Space Nuts. Great to have your

00:00:04 --> 00:00:06 company. My name is Andrew Dunkley, your host

00:00:06 --> 00:00:08 and I uh, hope you can stick around because

00:00:08 --> 00:00:11 we've got a jam packed show. We're

00:00:11 --> 00:00:13 once again going to Mars because

00:00:13 --> 00:00:16 they've looked uh, at some new evidence that

00:00:17 --> 00:00:19 uh, does suggest Mars oceans may have

00:00:19 --> 00:00:22 been vast. That is really

00:00:22 --> 00:00:24 exciting news. We're also going to look at

00:00:24 --> 00:00:27 the fastest spinning asteroid yet discovered.

00:00:27 --> 00:00:29 This one's uh, really in a spin.

00:00:29 --> 00:00:32 It's uh, making everybody dizzy. And the

00:00:32 --> 00:00:35 evacuation of the International Space Station

00:00:35 --> 00:00:38 uh, due to ill health. We'll see if we can

00:00:38 --> 00:00:39 get uh, some news on that because that's

00:00:39 --> 00:00:42 actually happening as Fred and I are uh,

00:00:42 --> 00:00:44 recording today. That's all coming up

00:00:44 --> 00:00:47 on this edition of Space Nuts. 15

00:00:48 --> 00:00:49 seconds. Guidance is internal.

00:00:50 --> 00:00:52 Voice Over Guy: 10, 9. Ignition

00:00:52 --> 00:00:55 sequence start. Space Nuts. 5, 4,

00:00:55 --> 00:00:58 3. 2. 1, 2, 3, 4, 5, 5, 4,

00:00:58 --> 00:01:01 3, 2, 1. Space Nuts astronauts

00:01:01 --> 00:01:02 report it feels good.

00:01:03 --> 00:01:06 Andrew Dunkley: And he's back again to furnish us with his

00:01:06 --> 00:01:08 knowledge. He is Professor Fred Watson,

00:01:08 --> 00:01:09 Astronomer at large. Hello Fred.

00:01:10 --> 00:01:12 Professor Fred Watson: Hello Andrew. I was just doing a quick

00:01:12 --> 00:01:14 calculation there for a number that I want to

00:01:14 --> 00:01:17 use um, later in the chat.

00:01:19 --> 00:01:21 Andrew Dunkley: Now I need to apologise in advance because

00:01:21 --> 00:01:24 ah, they're working across the road and I

00:01:24 --> 00:01:26 think they're using uh, dynamite because

00:01:27 --> 00:01:30 it's pretty noisy um, but

00:01:30 --> 00:01:33 hopefully it won't mess me up too much. I can

00:01:33 --> 00:01:34 hear it but I don't know if it's coming

00:01:34 --> 00:01:36 through the system. It's got all sorts of

00:01:36 --> 00:01:39 filters but um, some things you can't stop.

00:01:40 --> 00:01:40 Professor Fred Watson: Um.

00:01:40 --> 00:01:42 Andrew Dunkley: Now Fred, I did want to actually mention a

00:01:42 --> 00:01:44 couple of things before we start on our

00:01:44 --> 00:01:47 topics because uh, I meant to do this last

00:01:47 --> 00:01:50 week for our first show back of the year just

00:01:50 --> 00:01:52 to highlight some of the things that are

00:01:52 --> 00:01:54 coming up in 2026 that we can look forward to

00:01:54 --> 00:01:56 and that you and I will probably talk about.

00:01:56 --> 00:01:59 The Artemis 2 launch is

00:01:59 --> 00:02:02 slated. Uh, whether or not it'll be delayed

00:02:02 --> 00:02:04 again remains to be seen. But um, that will

00:02:04 --> 00:02:07 see a crew doing a lap around the moon,

00:02:08 --> 00:02:10 uh, and that'll be the first time humans have

00:02:10 --> 00:02:13 been back uh, in orbit around the moon

00:02:13 --> 00:02:15 since the 70s which uh, is

00:02:15 --> 00:02:18 exciting and probably too long but um,

00:02:18 --> 00:02:20 that'll be good. Um, this one I know will

00:02:20 --> 00:02:23 excite you. The Grace Roman Space Telescope

00:02:23 --> 00:02:26 is going to be launched. That one um,

00:02:26 --> 00:02:29 is going to um, opened so many doors for

00:02:29 --> 00:02:31 us I suspect, um, the

00:02:31 --> 00:02:34 PLATO mission, uh, which will be searching

00:02:34 --> 00:02:36 for rocky planets. It'll uh, be doing a lot

00:02:36 --> 00:02:38 more than that. But that's one of the things

00:02:38 --> 00:02:41 that it's being set out to do. Uh,

00:02:41 --> 00:02:43 China is to launch its own space

00:02:43 --> 00:02:46 telescope as well, um, in the hunt

00:02:46 --> 00:02:48 for dark matter and dark energy.

00:02:49 --> 00:02:52 And there's another mission that's going to

00:02:52 --> 00:02:54 be studying uh, the moon and Mars. Well,

00:02:54 --> 00:02:56 several missions, not just one. Um, more

00:02:56 --> 00:02:58 Chinese and Japanese missions involved there.

00:02:59 --> 00:03:01 And I think this is one you and I have talked

00:03:01 --> 00:03:04 about before. The Smile mission, uh, which

00:03:04 --> 00:03:06 will be studying Earth's magnetic field and

00:03:06 --> 00:03:08 how the sun interacts with our uh,

00:03:08 --> 00:03:11 atmosphere, uh, is um, due to be launched

00:03:11 --> 00:03:12 this year as well. I'm sure there's a lot

00:03:12 --> 00:03:14 more going on than that, but there's some of

00:03:14 --> 00:03:17 the highlights of 2026 so

00:03:17 --> 00:03:19 uh, we'll have a lot to talk about.

00:03:19 --> 00:03:21 Professor Fred Watson: Fred, could I add a couple more as well?

00:03:21 --> 00:03:22 Andrew Dunkley: Oh, go for it.

00:03:23 --> 00:03:25 Professor Fred Watson: Um, we've just uh, heard that the Pandora

00:03:25 --> 00:03:28 spacecraft has entered orbit, uh, which I

00:03:28 --> 00:03:31 think is a spacecraft, uh, again looking

00:03:31 --> 00:03:34 um, looking at exoplanets to try

00:03:34 --> 00:03:36 and sort of tell us a bit more about how

00:03:36 --> 00:03:39 their atmospheres might reveal stuff. Um,

00:03:39 --> 00:03:42 China has just filed for 200

00:03:42 --> 00:03:44 satellites constellation with the

00:03:44 --> 00:03:47 International Telecommunications Union which

00:03:47 --> 00:03:50 is. Yeah, yeah, well it's not the biggest

00:03:50 --> 00:03:52 yet. The biggest was back in 2020 when the

00:03:52 --> 00:03:54 Rwandan government filed for over

00:03:54 --> 00:03:57 300. Um, uh, since then

00:03:57 --> 00:03:59 they've launched one cubesat, I think. So,

00:03:59 --> 00:04:02 um, that looked like a filing that

00:04:03 --> 00:04:05 getting your foot in the door. Uh, and just

00:04:05 --> 00:04:08 turning to nature. We've got some interesting

00:04:08 --> 00:04:11 events coming up. Uh, March 3rd, total

00:04:11 --> 00:04:13 eclipse of the Moon visible certainly from

00:04:13 --> 00:04:16 our hemisphere in Australia, not sure about

00:04:16 --> 00:04:18 North America and Europe. Um,

00:04:18 --> 00:04:21 there's uh, towards the end of the year and

00:04:21 --> 00:04:24 this will happen twice, uh, which is great

00:04:24 --> 00:04:26 cause you can see it on different sides of

00:04:26 --> 00:04:28 the Earth. I think it's October, sometime in

00:04:28 --> 00:04:31 October and sometime in November there will

00:04:31 --> 00:04:34 be an occultation of the planet Jupiter by

00:04:34 --> 00:04:35 the Moon. That means the moon will pass in

00:04:35 --> 00:04:38 front of Jupiter and certainly for us in

00:04:38 --> 00:04:40 November here in Australia it will be during

00:04:40 --> 00:04:42 the daytime. So get your binoculars out

00:04:42 --> 00:04:44 during the daytime, check out the moon and

00:04:44 --> 00:04:46 watch for Jupiter disappearing.

00:04:46 --> 00:04:49 Andrew Dunkley: Oh, that'll be good. Yeah,

00:04:49 --> 00:04:50 that'd be a good one for a backyard

00:04:50 --> 00:04:51 telescope, wouldn't it?

00:04:51 --> 00:04:53 Professor Fred Watson: Absolutely perfect, yes.

00:04:54 --> 00:04:57 Andrew Dunkley: Awesome. Um, I had my

00:04:57 --> 00:05:00 6 year old granddaughter here uh, the other

00:05:00 --> 00:05:02 day and uh, the moon was, was out in the

00:05:02 --> 00:05:05 east and um, it was still daytime but it was

00:05:05 --> 00:05:07 pretty prominent. So I grabbed the telescope

00:05:07 --> 00:05:10 and gave her a look and uh, I tried to

00:05:10 --> 00:05:12 explain to her what craters were and

00:05:13 --> 00:05:14 she struggled with the concept. But she

00:05:14 --> 00:05:17 eventually I think figured it out. But uh,

00:05:17 --> 00:05:19 yeah, took a couple of photos of her looking

00:05:19 --> 00:05:20 through the telescope. She was very excited

00:05:22 --> 00:05:23 which she sent to me.

00:05:23 --> 00:05:25 Professor Fred Watson: It was uh, lovely to see them, Andrew. Yeah,

00:05:25 --> 00:05:27 yeah, lovely, lovely shots. A youngster

00:05:27 --> 00:05:29 looking through a telescop with granddad in

00:05:29 --> 00:05:31 the background is great. Yeah, yeah.

00:05:31 --> 00:05:34 Andrew Dunkley: Uh, she's got blonde hair and blue eyes and

00:05:34 --> 00:05:36 her brothers and sisters are all brown haired

00:05:36 --> 00:05:38 and brown eyed. So. Okay,

00:05:39 --> 00:05:41 she, she seems to have picked up Judy's side

00:05:41 --> 00:05:44 of the family genes because Judy's blondie,

00:05:44 --> 00:05:47 blonde with blue eyes. But um, she's the only

00:05:47 --> 00:05:49 one in the, in the family that's, that's gone

00:05:49 --> 00:05:52 that, that way. It happens though, doesn't

00:05:52 --> 00:05:53 it? It's just the way it is.

00:05:53 --> 00:05:53 Professor Fred Watson: Yeah.

00:05:53 --> 00:05:54 Andrew Dunkley: That's DNA.

00:05:55 --> 00:05:58 Um, okay Fred, uh,

00:05:58 --> 00:06:00 let's get stuck into it because uh, we're

00:06:00 --> 00:06:03 heading off to Mars and we're

00:06:03 --> 00:06:06 doing this because of a study that's just

00:06:06 --> 00:06:08 been published. Uh, in fact in the

00:06:08 --> 00:06:11 last week, uh, or two about uh,

00:06:11 --> 00:06:14 observations of Mars that suggest

00:06:14 --> 00:06:17 that its oceans were once vast. Now

00:06:17 --> 00:06:19 we always knew there was probably surface

00:06:19 --> 00:06:22 water but we didn't really know whether they

00:06:22 --> 00:06:25 were, you know, pockets or separate

00:06:25 --> 00:06:28 oceans or what. But now they're thinking

00:06:28 --> 00:06:29 the oceans might have been

00:06:31 --> 00:06:31 enormous.

00:06:32 --> 00:06:35 Professor Fred Watson: Uh, yes, that's right. And I mean, you know,

00:06:36 --> 00:06:39 we revisit this story probably on average

00:06:39 --> 00:06:42 once every month or two. Uh, the

00:06:42 --> 00:06:44 last time we covered this, and I

00:06:45 --> 00:06:47 wrote it up actually in um, an Australian

00:06:47 --> 00:06:49 Geographic article, um, not that I did the

00:06:49 --> 00:06:51 research, but this is other people's research

00:06:51 --> 00:06:54 and that was pointing in the same direction.

00:06:54 --> 00:06:56 Andrew. It was um, a group that looked at the

00:06:56 --> 00:06:59 way um, rivers, ancient rivers on Mars, uh,

00:07:00 --> 00:07:02 meandered, uh, because you can learn

00:07:02 --> 00:07:05 something from the meandering about the

00:07:05 --> 00:07:07 size of the body of water that they're

00:07:07 --> 00:07:10 emptying into. And they came to the same

00:07:10 --> 00:07:13 conclusion. The river meanders tell you that

00:07:13 --> 00:07:15 there was a large body of water at the end of

00:07:15 --> 00:07:17 it at the mouth of these rivers, uh, rather

00:07:17 --> 00:07:20 than just a few puddles or a few lakes and

00:07:20 --> 00:07:22 things of that sort. Uh, and this new piece

00:07:22 --> 00:07:25 uh, of work, um, whilst it's a different,

00:07:25 --> 00:07:28 uh, you know, it's got a different emphasis,

00:07:28 --> 00:07:31 comes up with exactly the same answer. Uh,

00:07:31 --> 00:07:34 and it's scientists uh, who have looked uh,

00:07:34 --> 00:07:37 at the, I remember rightly there in

00:07:37 --> 00:07:40 uh, in Switzerland. Yeah, University of Bern,

00:07:40 --> 00:07:42 uh, it's scientists who've looked at the

00:07:42 --> 00:07:44 region around Valles, uh,

00:07:45 --> 00:07:48 Marineris, you know, that great huge

00:07:49 --> 00:07:51 chasm in the, uh, in the surface of

00:07:51 --> 00:07:54 Mars. Near Mars's equator. Uh, something that

00:07:54 --> 00:07:57 makes the Grand Canyon look like a bit of a

00:07:57 --> 00:07:59 scratch on the, on the surface of the Earth.

00:07:59 --> 00:08:01 Andrew Dunkley: Yeah. Is it right that the Grand Canyon would

00:08:01 --> 00:08:03 fit into one of its tributaries or something?

00:08:03 --> 00:08:05 Professor Fred Watson: That's right. I think that's correct, yeah.

00:08:05 --> 00:08:06 Andrew Dunkley: Amazing.

00:08:06 --> 00:08:08 Professor Fred Watson: Um, so they've been looking in that region

00:08:08 --> 00:08:10 and certainly on the northern side and the

00:08:10 --> 00:08:13 northern flanks there are valleys that

00:08:14 --> 00:08:17 um, sort of open out onto the plains of Mars.

00:08:17 --> 00:08:20 Because that uh, Valles Marineris is kind

00:08:20 --> 00:08:22 of right at the start of the highland areas

00:08:22 --> 00:08:24 of the southern hemisphere of Mars. Mars has

00:08:24 --> 00:08:26 got this dichotomy. The northern hemisphere

00:08:26 --> 00:08:29 is flat and low, southern hemisphere 3km

00:08:29 --> 00:08:31 higher on average, full of craters, mountains

00:08:31 --> 00:08:34 and all around rest of it. Uh, so um, uh,

00:08:34 --> 00:08:36 um, what they've done is they've looked at

00:08:37 --> 00:08:39 regions, uh, where, you know, where there's

00:08:39 --> 00:08:42 this transition from the mountainous

00:08:42 --> 00:08:44 highlands of the south to the

00:08:44 --> 00:08:47 lowlands of the north. And they've looked

00:08:47 --> 00:08:50 very carefully at uh, data from

00:08:50 --> 00:08:53 uh, several orbiting spacecraft, um, I

00:08:53 --> 00:08:56 guess Mars Reconnaissance Orbiter is one and

00:08:56 --> 00:08:58 some of the other ones, um, actually even um,

00:08:59 --> 00:09:01 uh, um, ESO's

00:09:01 --> 00:09:04 ExoMars Trace Gas Orbiter. So, uh,

00:09:04 --> 00:09:07 Mars Express, another ESA, sorry, not ESO,

00:09:07 --> 00:09:10 ESA, uh, European Space Agency, Another

00:09:10 --> 00:09:13 um, uh, uh, orbiting spacecraft. They've

00:09:13 --> 00:09:15 taken the data from these, looked

00:09:15 --> 00:09:18 at the height, the

00:09:18 --> 00:09:20 topography and looked at the

00:09:20 --> 00:09:22 geomorphology. Let me get it right.

00:09:22 --> 00:09:24 Geomorphological, um,

00:09:24 --> 00:09:27 um, features that they can find.

00:09:28 --> 00:09:30 What have they spotted? They've spotted,

00:09:30 --> 00:09:33 ah, a whole succession of

00:09:33 --> 00:09:36 ancient river deltas, um, this

00:09:36 --> 00:09:38 is to say regions where a river mouth

00:09:38 --> 00:09:41 opened into what they're calling now

00:09:41 --> 00:09:44 an ocean, uh, and deposited

00:09:45 --> 00:09:47 um, its sediments. The sediments out of the

00:09:47 --> 00:09:49 river fall down to the floor, uh, of the

00:09:49 --> 00:09:52 ocean and build up basically

00:09:52 --> 00:09:55 a rock form, uh, which is preserved today.

00:09:55 --> 00:09:57 It's a kind of fossilized river delta.

00:09:57 --> 00:10:00 There's something similar going on, uh, as

00:10:00 --> 00:10:01 you and I have spoken about many times at

00:10:01 --> 00:10:04 Jezero Crater, which is why, um,

00:10:04 --> 00:10:06 perseverance is there, because there's a

00:10:06 --> 00:10:08 river delta there. But I think these are on a

00:10:08 --> 00:10:11 much larger scale. And um, the

00:10:11 --> 00:10:14 great thing is that when you look at them,

00:10:15 --> 00:10:17 they sort of define a shoreline,

00:10:18 --> 00:10:21 um, because these are all occurring

00:10:21 --> 00:10:24 at the same topographical height in

00:10:24 --> 00:10:26 Mars's geography. And so they

00:10:26 --> 00:10:29 basically uh, define a shoreline. And that

00:10:29 --> 00:10:32 shoreline tells you that um, there would have

00:10:32 --> 00:10:35 been a lot of water in Mars's northern

00:10:35 --> 00:10:37 hemisphere for the water level to reach the

00:10:37 --> 00:10:39 height that we find those deltas at.

00:10:40 --> 00:10:43 Uh, so really? Yeah, really nice piece

00:10:43 --> 00:10:45 of Work, uh, done with characteristic

00:10:45 --> 00:10:48 Swiss precision, I think. Uh, that's been

00:10:48 --> 00:10:50 widely reported. Um, there's several

00:10:50 --> 00:10:53 articles, uh, on the science news feeds,

00:10:53 --> 00:10:56 um, which basically support this idea.

00:10:56 --> 00:10:58 Very nice piece of research indeed.

00:10:59 --> 00:11:02 Andrew Dunkley: And they think it was as big as

00:11:02 --> 00:11:05 the Arctic Ocean on Earth, just by

00:11:05 --> 00:11:07 comparison. And how big as the Arctic Ocean?

00:11:07 --> 00:11:09 It's 14 million square kilometers or

00:11:10 --> 00:11:12 five and a half million square miles

00:11:13 --> 00:11:16 big, uh, in size. So that's a lot of

00:11:16 --> 00:11:18 water on Mars and uh, a lot of it's still

00:11:18 --> 00:11:19 there, Fred.

00:11:19 --> 00:11:21 Professor Fred Watson: Yeah, that's right. We um, know from

00:11:21 --> 00:11:23 particularly, uh, the Phoenix mission that

00:11:23 --> 00:11:25 just scraped the surface in the Martian

00:11:25 --> 00:11:27 Arctic and sure enough there was permafrost

00:11:27 --> 00:11:29 underneath. So a lot of it's still there.

00:11:29 --> 00:11:32 There's still water locked up in the two ice

00:11:32 --> 00:11:34 caps of Mars. Um, but probably

00:11:34 --> 00:11:36 not. Well, I don't know. It's actually really

00:11:36 --> 00:11:38 interesting. I do remember reading quite some

00:11:38 --> 00:11:40 time ago that if you thawed out even just the

00:11:40 --> 00:11:43 Antarctic ice cap of Mars, you'd cover the

00:11:43 --> 00:11:45 whole planet to a depth of several meters.

00:11:46 --> 00:11:49 Um, now whether that still holds good with

00:11:49 --> 00:11:51 what we've discovered since then, that was

00:11:51 --> 00:11:52 quite an old, I think that was probably 20

00:11:52 --> 00:11:55 years, 15 years ago, so that that comment

00:11:55 --> 00:11:57 was made. It would be interesting to know how

00:11:57 --> 00:11:59 we evaluate that now. But I think it's still

00:11:59 --> 00:12:02 true, uh, that a lot of that water is still

00:12:02 --> 00:12:02 there.

00:12:02 --> 00:12:05 Andrew Dunkley: Ah, yeah, it is, uh, a

00:12:05 --> 00:12:06 fascinating story.

00:12:06 --> 00:12:07 Professor Fred Watson: Water means life.

00:12:08 --> 00:12:11 Andrew Dunkley: Well, yes, yes, we've said that many times.

00:12:11 --> 00:12:13 And you just don't know, do you?

00:12:13 --> 00:12:15 Professor Fred Watson: You don't. Yeah.

00:12:15 --> 00:12:17 Andrew Dunkley: Although the, uh, the mission to retrieve

00:12:17 --> 00:12:20 those um, cylinders that contain

00:12:21 --> 00:12:22 potential evidence of that.

00:12:22 --> 00:12:23 Professor Fred Watson: Yeah.

00:12:23 --> 00:12:26 Andrew Dunkley: Has been scotched. So it's just going to sit

00:12:26 --> 00:12:28 in abeyance for um, an

00:12:28 --> 00:12:29 indefinite period.

00:12:30 --> 00:12:32 Professor Fred Watson: So, yeah, I think, um,

00:12:33 --> 00:12:35 so this is news that, um, the Senate have

00:12:35 --> 00:12:38 um, basically agreed with the White House in

00:12:38 --> 00:12:41 saying that um, the Mars Sample Return

00:12:41 --> 00:12:44 Mission, uh, should be canceled. Uh,

00:12:44 --> 00:12:46 and so that will probably go through. It's

00:12:46 --> 00:12:48 not been voted on yet, I don't think. Um,

00:12:49 --> 00:12:51 and so that means, yes, we've got these

00:12:51 --> 00:12:53 canisters on Mars, uh, carefully dropped by

00:12:53 --> 00:12:56 perseverance, uh, but

00:12:56 --> 00:12:59 with a joint European Space Agency NASA

00:12:59 --> 00:13:02 mission to retrieve them, uh, which, whose

00:13:02 --> 00:13:05 cost has blown out. Uh, we've talked about

00:13:05 --> 00:13:07 this before, uh, and not perhaps

00:13:07 --> 00:13:10 surprising that it's now had a line drawn

00:13:10 --> 00:13:12 under it. Now that's bad

00:13:12 --> 00:13:15 news because we really would like to get hold

00:13:15 --> 00:13:16 of these samples. There's one in particular

00:13:16 --> 00:13:18 that may contain actually fossilized

00:13:18 --> 00:13:21 microbes. Uh, you know, um,

00:13:21 --> 00:13:24 so it's um, there's uh, every keenness to do

00:13:24 --> 00:13:27 that. Um, um, and I think it

00:13:27 --> 00:13:30 will. There'll certainly be a revisiting

00:13:30 --> 00:13:33 of this idea. Esa, I think, is still going

00:13:33 --> 00:13:34 ahead with their half of the bargain. Which

00:13:34 --> 00:13:36 was, I think, to build the orbiter which

00:13:36 --> 00:13:38 would actually bring the samples back to

00:13:38 --> 00:13:41 Mars. NASA's part was gathering them up on

00:13:41 --> 00:13:43 the surface and sending them up to orbit

00:13:43 --> 00:13:45 around Mars. Uh, so, you know,

00:13:46 --> 00:13:49 uh, it's bad news. There's a bright side to

00:13:49 --> 00:13:51 it though, in that the money that's being

00:13:51 --> 00:13:52 saved will probably go to some of the other

00:13:52 --> 00:13:54 missions that are being planned.

00:13:55 --> 00:13:57 Name your favorite planet. You might get some

00:13:57 --> 00:13:59 good news out of this. I know your favorite

00:13:59 --> 00:14:02 and probably mine too, is Mars. Uh, but,

00:14:02 --> 00:14:05 um, anyway, we'll see what happens. I

00:14:05 --> 00:14:07 wouldn't write, uh, the Mars sample return

00:14:08 --> 00:14:10 off altogether in my flights of

00:14:10 --> 00:14:12 fantasy. Last night, while my,

00:14:12 --> 00:14:15 uh, respiratory tract infection was

00:14:15 --> 00:14:18 making me cough all night, I was thinking

00:14:18 --> 00:14:20 maybe the Chinese could bring them back

00:14:21 --> 00:14:23 because I think they're planning a sample

00:14:23 --> 00:14:26 return mission as well. So maybe we do a deal

00:14:26 --> 00:14:28 there. Which would be fabulous international

00:14:28 --> 00:14:29 cooperation.

00:14:29 --> 00:14:31 Andrew Dunkley: It would. It would indeed. Of course, we

00:14:31 --> 00:14:33 could always start the conspiracy and say,

00:14:33 --> 00:14:35 what does NASA and the US Government know

00:14:35 --> 00:14:36 that they're not telling us?

00:14:38 --> 00:14:39 Hence no return. Yeah, yeah.

00:14:39 --> 00:14:42 Professor Fred Watson: Be careful what you, what you say, Andrew.

00:14:42 --> 00:14:45 Andrew Dunkley: No, look, I'm just kidding around, but, uh,

00:14:46 --> 00:14:48 it's just money, isn't it? That's, that's the

00:14:48 --> 00:14:48 thing.

00:14:48 --> 00:14:50 Professor Fred Watson: It's all about money. That's right. It's not

00:14:50 --> 00:14:52 about finding something with legs that you

00:14:52 --> 00:14:54 don't want anybody to know about.

00:14:55 --> 00:14:57 Andrew Dunkley: Yes, that's been done in a lot of science

00:14:57 --> 00:14:57 fiction films.

00:14:57 --> 00:14:59 Professor Fred Watson: Yeah, it has. And um.

00:14:59 --> 00:15:02 Andrew Dunkley: Yes, all right. Great story about

00:15:02 --> 00:15:04 the oceans of Mars though. If you'd like to

00:15:04 --> 00:15:06 check it out, it's on the Phys p h y

00:15:06 --> 00:15:09 s.org website. Or you can read the

00:15:09 --> 00:15:11 paper that's been published in the journal

00:15:11 --> 00:15:13 NPJ Space Exploration.

00:15:14 --> 00:15:16 This is Space Nuts with Andrew Dunkley and

00:15:16 --> 00:15:17 Professor Fred Watson.

00:15:20 --> 00:15:21 Roger, in your labs right here.

00:15:21 --> 00:15:24 Also Space Nuts to our

00:15:24 --> 00:15:27 next story, Fred. And this

00:15:27 --> 00:15:29 is, uh, a really good one for a couple of

00:15:29 --> 00:15:31 reasons. It's something we haven't seen

00:15:31 --> 00:15:34 before, but it also involves the, uh,

00:15:34 --> 00:15:36 Rubin Observatory, which, um,

00:15:37 --> 00:15:40 has already, uh, done things that,

00:15:40 --> 00:15:43 uh, other observatories have not been able

00:15:43 --> 00:15:45 to do and promises to do so much more.

00:15:46 --> 00:15:48 This is the fastest spinning asteroid yet

00:15:48 --> 00:15:50 discovered. And a couple of headlines I've

00:15:50 --> 00:15:53 read suggested why hasn't it thrown itself

00:15:54 --> 00:15:56 to pieces because of the speed at which it's

00:15:56 --> 00:15:59 rotating and

00:15:59 --> 00:16:02 the rate is rather high when you look at what

00:16:02 --> 00:16:04 the average asteroid does.

00:16:04 --> 00:16:07 Professor Fred Watson: Yeah, so it is a record breaker.

00:16:07 --> 00:16:10 It's the fastest spinning asteroid

00:16:10 --> 00:16:13 for its size. Uh, because I think

00:16:13 --> 00:16:16 smaller things can spin faster than this.

00:16:16 --> 00:16:19 It's uh, 710 meters long, nearly

00:16:19 --> 00:16:22 three quarters of a kilometer. Uh, so

00:16:22 --> 00:16:24 it's not a small asteroid at all. This

00:16:24 --> 00:16:27 is quite a large one. Uh, and

00:16:27 --> 00:16:30 it spins at the rate of one rotation

00:16:30 --> 00:16:33 every one minute 53

00:16:33 --> 00:16:36 seconds. So that

00:16:36 --> 00:16:38 is one heck of a spin. So that's its day

00:16:38 --> 00:16:41 length, Andrew. If you were standing on it,

00:16:41 --> 00:16:43 your day will be 1 minute 53 seconds. Seconds

00:16:43 --> 00:16:46 night and day, not 24 hours. Um,

00:16:47 --> 00:16:49 but uh, you're absolutely right. I think it's

00:16:49 --> 00:16:52 interesting for two reasons. One is exactly

00:16:52 --> 00:16:55 as you've said. It underlines, uh, just

00:16:55 --> 00:16:57 how powerful the Rubin Observatory is going

00:16:57 --> 00:17:00 to be. The observations of

00:17:00 --> 00:17:03 this object were made during the

00:17:03 --> 00:17:05 sort of commissioning period for the

00:17:05 --> 00:17:07 telescope's instruments, which was earlier

00:17:07 --> 00:17:10 last year, April and May 2025. Uh,

00:17:10 --> 00:17:13 and um, that you know, that um,

00:17:13 --> 00:17:15 as you probably remember, I think they

00:17:15 --> 00:17:18 released uh, uh, information saying they got.

00:17:18 --> 00:17:19 They discovered more than a thousand

00:17:19 --> 00:17:22 asteroids in 10 hours of observing, which is

00:17:22 --> 00:17:25 pretty fantastic. Uh, the telescope's

00:17:25 --> 00:17:27 capabilities will allow it to survey the

00:17:27 --> 00:17:29 entire southern sky every three

00:17:29 --> 00:17:32 nights, uh, with an eight meter class

00:17:32 --> 00:17:34 telescope. That is an astonishing achievement

00:17:34 --> 00:17:37 and we.

00:17:37 --> 00:17:39 Andrew Dunkley: Must find something incredible.

00:17:40 --> 00:17:42 Professor Fred Watson: Yeah, we will. Yeah, there's going to be all

00:17:42 --> 00:17:44 kinds of things that come out of the

00:17:44 --> 00:17:46 woodwork. Uh, it's what we call, um,

00:17:47 --> 00:17:50 uh, sort of time sensitive astronomy or

00:17:50 --> 00:17:51 transient astronomy. You're looking for

00:17:51 --> 00:17:54 things that either move or change in the sky

00:17:54 --> 00:17:56 and it's going to be so good at finding them.

00:17:56 --> 00:17:59 And um. Yeah. So the real

00:17:59 --> 00:18:01 observing, uh, campaign, the Large

00:18:01 --> 00:18:04 Synoptic Survey, uh, will start

00:18:04 --> 00:18:07 uh, sometime this year, uh, sort of when

00:18:07 --> 00:18:10 they're ready to hit the go button. Uh, but I

00:18:10 --> 00:18:12 think everybody at the Rubin is pretty happy

00:18:12 --> 00:18:14 with the way things are going. Um, and just

00:18:14 --> 00:18:17 to sort of highlight that, you know,

00:18:18 --> 00:18:21 it's a telescope with this kind of capability

00:18:21 --> 00:18:24 to make many observations over a short period

00:18:24 --> 00:18:26 of time of the same area of sky. That has

00:18:26 --> 00:18:29 allowed uh, the scientists to

00:18:29 --> 00:18:32 discover the very rapid rotation

00:18:32 --> 00:18:34 of this asteroid. Because what you have to

00:18:34 --> 00:18:37 produce, uh, to look at the way an asteroid

00:18:37 --> 00:18:39 rotates is what's called a light curve. You

00:18:39 --> 00:18:41 look at the way its brightness changes. Uh,

00:18:41 --> 00:18:44 because most asteroids, asteroids are quite

00:18:44 --> 00:18:46 asymmetric. They're either shaped like a

00:18:46 --> 00:18:48 potato or a dumbbell. Very, uh, few are

00:18:48 --> 00:18:51 anything remotely spherical. Um, uh,

00:18:51 --> 00:18:53 this particular one is I think Quite

00:18:53 --> 00:18:56 elongated. And so as it rotates,

00:18:56 --> 00:18:59 uh, different sides of it catch the

00:18:59 --> 00:19:01 sunlight and you get a variation in the light

00:19:01 --> 00:19:04 that we see from it. Uh, and so that uh,

00:19:04 --> 00:19:06 has allowed, because it's, you know, it's

00:19:06 --> 00:19:08 only 1 minute 53 seconds for one

00:19:09 --> 00:19:11 complete revolution that has allowed the

00:19:11 --> 00:19:14 scientists to determine that fact,

00:19:14 --> 00:19:17 um, to the asteroid itself. You're right,

00:19:17 --> 00:19:19 it's interesting. It rejoices in the name of

00:19:19 --> 00:19:22 2025 MN45, a

00:19:22 --> 00:19:25 classic asteroid name. Um, and

00:19:25 --> 00:19:27 it's in the main asteroid belt. That's

00:19:28 --> 00:19:31 a good place for it to be between uh, Jupiter

00:19:31 --> 00:19:33 and Mars, where most of the asteroids are.

00:19:33 --> 00:19:36 Uh, but um, its rotation

00:19:36 --> 00:19:39 is what highlights um,

00:19:39 --> 00:19:42 the unusual nature of it. Because as you and

00:19:42 --> 00:19:44 I have spoken about before, many asteroids

00:19:44 --> 00:19:46 are uh, basically what we call rubble piles.

00:19:46 --> 00:19:49 They're just piles of debris which stick

00:19:49 --> 00:19:52 together loosely under their own,

00:19:52 --> 00:19:55 uh, gravity. Um, little

00:19:55 --> 00:19:57 uh, Dimorphos and Didymos, the

00:19:57 --> 00:20:00 two, uh, objects that NASA did the

00:20:00 --> 00:20:02 DART test on a few years ago, they are

00:20:02 --> 00:20:04 probably rubber piles. They've got the

00:20:04 --> 00:20:06 characteristic rubber pile shape, which is

00:20:06 --> 00:20:09 like two cones, um, uh, back to

00:20:09 --> 00:20:11 back. Uh, if it was a rubber

00:20:11 --> 00:20:13 pile, it would have flown apart

00:20:14 --> 00:20:17 gazillions of years ago, uh, with

00:20:17 --> 00:20:19 that short period of rotation, 1 minute

00:20:20 --> 00:20:23 53 seconds. So, um, uh, and when

00:20:23 --> 00:20:25 you look at the size of it and

00:20:25 --> 00:20:28 uh, interpret what the rotation means, it

00:20:28 --> 00:20:30 tells you it's probably made of absolutely

00:20:30 --> 00:20:32 solid rock. This is something that is

00:20:33 --> 00:20:35 um, going to be hard to pull apart, to

00:20:35 --> 00:20:38 rotate. For it to be that big rotate at that

00:20:38 --> 00:20:41 speed, it's got to be solid rock, um,

00:20:41 --> 00:20:43 um, making it uh, you know, in some ways even

00:20:43 --> 00:20:45 more interesting because we think the rubber

00:20:45 --> 00:20:47 piles are perhaps the more common uh,

00:20:47 --> 00:20:48 asteroids that we see.

00:20:49 --> 00:20:51 Andrew Dunkley: Do we, do we have any idea what would make it

00:20:51 --> 00:20:53 different, why it would be different? Is it a

00:20:53 --> 00:20:56 piece of a destroyed planet Theia?

00:20:57 --> 00:20:59 Professor Fred Watson: Well, yeah, could be, uh, might be part of

00:20:59 --> 00:21:02 Theia, the one that created the moon, uh,

00:21:03 --> 00:21:05 after, after it collided with the ah, Earth.

00:21:05 --> 00:21:08 It's more likely you're right. It's

00:21:08 --> 00:21:11 probably, um, you know, maybe part of the

00:21:11 --> 00:21:14 outer mantle of what would have been

00:21:14 --> 00:21:17 a protoplanet. In the early solar

00:21:17 --> 00:21:19 system, these things were the building blocks

00:21:19 --> 00:21:21 of planets. They collided and sometimes they

00:21:21 --> 00:21:23 blasted each other apart, sometimes

00:21:24 --> 00:21:26 they stuck together to form what we see

00:21:26 --> 00:21:29 in the solar system today. Um,

00:21:29 --> 00:21:31 and I, uh, think some of the collisions that

00:21:31 --> 00:21:33 would have happened in the early solar

00:21:33 --> 00:21:36 system, uh, may well have set an

00:21:36 --> 00:21:38 object like this spinning very rapidly. In

00:21:38 --> 00:21:41 fact, it might have initially been

00:21:41 --> 00:21:43 spinning even more rapidly. Than it is now.

00:21:43 --> 00:21:45 Because we're looking at probably several

00:21:45 --> 00:21:47 billion years ago. When whatever

00:21:47 --> 00:21:50 happened to it happened. So, uh, an

00:21:50 --> 00:21:53 object of some interest. And, um, one

00:21:53 --> 00:21:56 that I'm sure will be studied, uh, in

00:21:56 --> 00:21:58 greater detail. We might want to know things

00:21:58 --> 00:22:01 like, um, the infrared signature of its

00:22:01 --> 00:22:03 surface. Which gives you an idea of what the

00:22:03 --> 00:22:05 surface is like, how rough it is, whether

00:22:05 --> 00:22:08 it's a. Whether it's a smooth

00:22:08 --> 00:22:10 surface. What materials are likely to be,

00:22:11 --> 00:22:12 uh, found on its surface. That can all come

00:22:12 --> 00:22:15 from spectroscopy and also the science of

00:22:15 --> 00:22:17 polarimetry, which is what you look at to

00:22:17 --> 00:22:19 know whether something's highly reflective.

00:22:19 --> 00:22:22 Or rather rough and diffuse. So,

00:22:22 --> 00:22:24 yeah, m. I think there's lots to learn about,

00:22:24 --> 00:22:26 uh, 2025 MN45.

00:22:27 --> 00:22:30 Andrew Dunkley: Indeed. So it's in the asteroid

00:22:30 --> 00:22:32 belt between Mars and Jupiter.

00:22:32 --> 00:22:35 Um, people probably imagine

00:22:35 --> 00:22:38 that to be just a wall of roc.

00:22:38 --> 00:22:40 How do we get through it? But it's quite

00:22:40 --> 00:22:41 sparse, isn't it?

00:22:41 --> 00:22:44 Professor Fred Watson: It is, yeah. Yeah. Uh, it's

00:22:44 --> 00:22:46 sparse enough that, um, uh, several

00:22:46 --> 00:22:48 spacecraft have actually gone through it

00:22:48 --> 00:22:51 unscathed. Um, so,

00:22:51 --> 00:22:52 yes, it's.

00:22:52 --> 00:22:53 Andrew Dunkley: Well, I've never heard of a spacecraft

00:22:53 --> 00:22:55 actually running into anything out there.

00:22:56 --> 00:22:58 Not that there have been that many that have

00:22:58 --> 00:22:59 gone through, but.

00:22:59 --> 00:23:01 Professor Fred Watson: That's right. But, you know, as, um.

00:23:02 --> 00:23:05 Uh. Was it Douglas Adams. Space

00:23:05 --> 00:23:05 is big. Yes.

00:23:06 --> 00:23:06 Andrew Dunkley: Yes.

00:23:06 --> 00:23:08 Professor Fred Watson: You might think it's a long way down to the

00:23:08 --> 00:23:10 chemist at the corner of the street. But

00:23:10 --> 00:23:13 that's nothing compared with space. I think

00:23:13 --> 00:23:14 that was what he said.

00:23:16 --> 00:23:18 Andrew Dunkley: Yes, indeed. Uh, so if you would like to

00:23:18 --> 00:23:21 learn more about what the Vera C. Rubin

00:23:21 --> 00:23:23 Observatory has discovered, you can do

00:23:23 --> 00:23:26 that@the universitytoday.com website.

00:23:26 --> 00:23:28 Or you can read the paper in the

00:23:28 --> 00:23:31 Astrophysical Journal Letters. Which was,

00:23:31 --> 00:23:34 uh, only published on January 7th. So they're

00:23:34 --> 00:23:35 getting down to business early this year,

00:23:35 --> 00:23:36 aren't they?

00:23:36 --> 00:23:39 Professor Fred Watson: This is space nuts. Sorry. I was

00:23:39 --> 00:23:41 going to say, um, we always get a really

00:23:42 --> 00:23:44 good, um, crop of news stories at this time

00:23:44 --> 00:23:46 of year. Because it's right at the beginning

00:23:46 --> 00:23:48 of January that the American Astronomical

00:23:48 --> 00:23:51 Society has its annual meeting.

00:23:52 --> 00:23:55 And, um, so there's always some great

00:23:55 --> 00:23:58 stories. So, you know, that's why it was,

00:23:58 --> 00:23:59 uh. You know, it was published last week. I'm

00:23:59 --> 00:24:00 sure that's actually.

00:24:00 --> 00:24:02 Andrew Dunkley: It's actually very clever because as someone

00:24:02 --> 00:24:05 who worked in the media for 40 years. And

00:24:07 --> 00:24:09 had, um, to work a lot of Christmases and New

00:24:09 --> 00:24:12 Years, you quite often find you're

00:24:12 --> 00:24:14 struggling for stories because

00:24:14 --> 00:24:16 everything's shut down. So you're not getting

00:24:16 --> 00:24:19 the information that you normally get. So

00:24:19 --> 00:24:22 to actually be in a position to do stories

00:24:22 --> 00:24:25 like this at this time of year is

00:24:25 --> 00:24:28 um. Yeah, it's well

00:24:28 --> 00:24:30 positioned, as we would say. M. Uh,

00:24:30 --> 00:24:33 you can read all about it, of course. And uh,

00:24:33 --> 00:24:36 we uh, will certainly be keeping a very close

00:24:36 --> 00:24:38 eye on what the Vera C. Rubin Observatory is

00:24:38 --> 00:24:39 going to be doing

00:24:40 --> 00:24:43 um, from now on because it's uh,

00:24:43 --> 00:24:46 it's, it's, it's all up and running and uh,

00:24:46 --> 00:24:49 already doing some remarkable things. This

00:24:49 --> 00:24:51 is Space Nuts with Andrew Dunkley and Fred

00:24:51 --> 00:24:51 Watson.

00:24:55 --> 00:24:58 Space Nuts. Now Fred, uh, by the time

00:24:58 --> 00:25:00 people hear us talking about this story,

00:25:00 --> 00:25:03 things will have uh, changed a bit. But

00:25:03 --> 00:25:06 as we speak, uh, we understand that

00:25:06 --> 00:25:08 the Crew Dragon spacecraft

00:25:09 --> 00:25:12 is docking at the International Space Station

00:25:12 --> 00:25:15 to do the first ever crew

00:25:15 --> 00:25:17 evacuation. Now, after 25 years,

00:25:18 --> 00:25:20 I'm surprised this is the first time this has

00:25:20 --> 00:25:22 happened. But uh, there's been a medical

00:25:22 --> 00:25:24 issue. They won't elaborate on who or what,

00:25:25 --> 00:25:27 uh, but it's gotta be serious if somebody's

00:25:27 --> 00:25:29 um, if they're bringing the whole crew back.

00:25:29 --> 00:25:32 It's uh, a crew of four. There's seven on

00:25:32 --> 00:25:33 board at the moment. But they're bringing

00:25:33 --> 00:25:35 four back, correct?

00:25:35 --> 00:25:37 Professor Fred Watson: That's right. So, uh, there is a crew of

00:25:37 --> 00:25:40 three uh, now. So as we speak, um, I

00:25:40 --> 00:25:43 think they've probably undocked the crew

00:25:43 --> 00:25:45 Dragon spacecraft from the International

00:25:45 --> 00:25:46 Space Station. I think that happened an hour

00:25:46 --> 00:25:49 ago. And um, they

00:25:49 --> 00:25:52 will then re. Enter and bring the crew

00:25:52 --> 00:25:55 back in a pretty routine fashion,

00:25:55 --> 00:25:58 uh, landing in a few hours from now. Um, so

00:25:58 --> 00:26:01 you're right, it's Crew 11, uh,

00:26:01 --> 00:26:03 the SpaceX, um,

00:26:04 --> 00:26:06 what's called the SpaceX Crew 11 because

00:26:06 --> 00:26:07 they're the ones that go up and down in the

00:26:07 --> 00:26:10 crew Dragon, uh, rather than the Soyuts,

00:26:10 --> 00:26:12 which is the space vehicle that will bring

00:26:12 --> 00:26:14 the other uh, the remaining three astronauts

00:26:14 --> 00:26:17 down when their time comes to an end. Uh,

00:26:17 --> 00:26:19 you're right. It's a medical evacuation that

00:26:19 --> 00:26:22 Crew, Crew 11 consists of, um, if I

00:26:22 --> 00:26:25 remember rightly, two NASA, uh, uh,

00:26:25 --> 00:26:27 astronauts, one Russian

00:26:27 --> 00:26:30 cosmonaut and uh, a Japanese

00:26:31 --> 00:26:33 uh, astronaut as well. Uh, so they're coming

00:26:33 --> 00:26:36 home, uh, they're coming home something like

00:26:36 --> 00:26:39 a month early. And we are told as

00:26:39 --> 00:26:41 exactly as you've said that this is because

00:26:41 --> 00:26:43 of a medical issue which apparently is not

00:26:43 --> 00:26:46 uh, an emergency. It's not urgent, but it's

00:26:46 --> 00:26:48 thought to be something that is going to be

00:26:48 --> 00:26:51 much better dealt with on Earth. Uh, we don't

00:26:51 --> 00:26:54 know which of the astronauts has the issue.

00:26:54 --> 00:26:57 Um, I saw a picture of them posed just before

00:26:57 --> 00:26:58 they evacuated the spacecraft,

00:26:59 --> 00:27:02 uh, um, last night and they all looked

00:27:02 --> 00:27:05 fairly cheerful, uh, but um, so

00:27:05 --> 00:27:07 you know, uh, you can't really read

00:27:09 --> 00:27:11 from people's faces how they're feeling. Um,

00:27:12 --> 00:27:13 which is just as well because I feel pretty

00:27:13 --> 00:27:16 crook at the moment. So

00:27:16 --> 00:27:19 that's uh, because of my uh, uh, upper

00:27:19 --> 00:27:21 respiratory tract infection. Sorry to keep

00:27:21 --> 00:27:23 harping on about it. Anyway, going back to

00:27:23 --> 00:27:26 the more important story, Andrew. Well it's

00:27:26 --> 00:27:27 a good thing you're not.

00:27:27 --> 00:27:29 Andrew Dunkley: In the International Space Station feeling

00:27:29 --> 00:27:29 like that.

00:27:29 --> 00:27:31 Professor Fred Watson: Well, that's right, I, you'd have the same

00:27:31 --> 00:27:33 thing too. Uh, so, yeah, so,

00:27:33 --> 00:27:36 um, interesting. Uh, but your comment's well

00:27:36 --> 00:27:38 made. You know the fact that it's the first

00:27:38 --> 00:27:40 time in the 25 year history

00:27:41 --> 00:27:44 of the ISS, of the

00:27:44 --> 00:27:46 ISS being permanently occupied,

00:27:47 --> 00:27:49 um, the first time this has happened. And I

00:27:49 --> 00:27:52 think it was Jared Isaacman, the newly

00:27:52 --> 00:27:55 appointed NASA administrator, the boss of

00:27:55 --> 00:27:58 NASA, who made the comment. It might

00:27:58 --> 00:28:01 be somebody else but it is one of the

00:28:01 --> 00:28:04 high ups in NASA made the comment that

00:28:04 --> 00:28:06 when they planned the ISS and they were

00:28:06 --> 00:28:09 working towards it, they expected that there

00:28:09 --> 00:28:10 would be something like this happening every

00:28:10 --> 00:28:13 three years. So they've done pretty well

00:28:13 --> 00:28:16 to get through 2015, five years without um,

00:28:16 --> 00:28:17 needing to bring people home because of a

00:28:17 --> 00:28:19 medical issue. Yeah.

00:28:20 --> 00:28:22 Andrew Dunkley: While you've been talking Fred, I've just

00:28:22 --> 00:28:24 been looking online to see where things are

00:28:24 --> 00:28:27 up to and I've found a um, they did a live

00:28:27 --> 00:28:30 stream of the crew uh, Dragon docking at the

00:28:30 --> 00:28:32 International Space Station through

00:28:32 --> 00:28:35 uh, I think it's NASA's YouTube Music

00:28:35 --> 00:28:38 channel and you can, you can

00:28:38 --> 00:28:40 actually log on and, and watch what happens

00:28:40 --> 00:28:43 and see the whole process. It's quite

00:28:43 --> 00:28:45 incredible what we can do now isn't it with

00:28:45 --> 00:28:48 um, live coverage from space as ah, things

00:28:48 --> 00:28:51 unfold. It's uh, a far cry

00:28:51 --> 00:28:54 from those times back in the 60s and 70s when

00:28:54 --> 00:28:55 we were looking at those really fuzzy black

00:28:55 --> 00:28:57 and white pictures off the moon.

00:28:59 --> 00:29:00 Professor Fred Watson: Which was miraculous in its day.

00:29:00 --> 00:29:02 Andrew Dunkley: Oh it was in itself, yes. Yes.

00:29:03 --> 00:29:03 Professor Fred Watson: Yeah.

00:29:04 --> 00:29:07 Andrew Dunkley: Actually I am watching Crew Dragon detach as

00:29:07 --> 00:29:07 we speak.

00:29:07 --> 00:29:08 Professor Fred Watson: Yes, that's right.

00:29:08 --> 00:29:10 Andrew Dunkley: So that happened probably 30 minutes ago,

00:29:10 --> 00:29:13 give or take our time. Yeah,

00:29:13 --> 00:29:16 um, it's, it's like a slow motion ballet

00:29:16 --> 00:29:18 isn't it? When they uh, things in

00:29:18 --> 00:29:19 spacecraft.

00:29:19 --> 00:29:22 Professor Fred Watson: Ah, yeah, well you don't want to bang into

00:29:22 --> 00:29:22 anything.

00:29:23 --> 00:29:25 Andrew Dunkley: Yeah. Anyway, I hope all is well with

00:29:25 --> 00:29:27 the uh, individual involved. I'm uh,

00:29:28 --> 00:29:30 I'm not sure we'll ever find out what exactly

00:29:31 --> 00:29:33 the issue is. That's, that's subject to

00:29:33 --> 00:29:35 privacy from what I understand. But the fact

00:29:35 --> 00:29:38 that they've been able to go

00:29:38 --> 00:29:40 up there, get them, bring them back and deal

00:29:40 --> 00:29:43 with the problem is extraordinary

00:29:43 --> 00:29:46 because go back to the 70s when

00:29:46 --> 00:29:49 Skylab was in orbit. If someone got sick

00:29:49 --> 00:29:52 or injured in that situation,

00:29:52 --> 00:29:55 I don't know if we would have been able to do

00:29:55 --> 00:29:56 much in a hurry.

00:29:58 --> 00:30:00 Professor Fred Watson: Um, yeah, maybe not. I mean, there would have

00:30:00 --> 00:30:03 been contingency plans in place.

00:30:04 --> 00:30:07 It's, um. I think

00:30:07 --> 00:30:09 some of the things that might have brought

00:30:09 --> 00:30:11 somebody home from Skylab might be things

00:30:11 --> 00:30:12 that could have been fixed on the

00:30:12 --> 00:30:14 International Space Station because there is

00:30:14 --> 00:30:17 quite a, you know, a fair, Fair amount of

00:30:17 --> 00:30:19 medical expertise up there and some of the

00:30:19 --> 00:30:21 kit. But you don't want people taking

00:30:21 --> 00:30:23 appendices out and things like that in space.

00:30:23 --> 00:30:25 Andrew Dunkley: No, not really. You just have to wipe down

00:30:25 --> 00:30:27 the walls afterwards, and that's not fun.

00:30:28 --> 00:30:31 Although I should, um, counter it by saying

00:30:31 --> 00:30:33 we did recently have a situation where. Where

00:30:34 --> 00:30:36 a crew got stuck on the International Space

00:30:36 --> 00:30:39 Station for very unusual reasons due to,

00:30:39 --> 00:30:41 uh, incompatible spacesuits because of a

00:30:41 --> 00:30:43 failure in the Boeing Starliner.

00:30:44 --> 00:30:47 So, you know, that wasn't a quick

00:30:47 --> 00:30:49 rescue, that one, but it didn't involve

00:30:49 --> 00:30:51 illness or injury, so it wasn't as urgent.

00:30:51 --> 00:30:54 But, uh, sometimes it. It can be a

00:30:54 --> 00:30:57 slow process, but, um. Uh, yeah, but

00:30:57 --> 00:30:59 NASA's been very quick to point out that this

00:30:59 --> 00:31:01 has got nothing to do with an operational

00:31:01 --> 00:31:03 issue. It's, um. It's a personal issue.

00:31:03 --> 00:31:06 Nothing to do with an injury or accident on

00:31:06 --> 00:31:08 board. They want to make that pretty clear.

00:31:09 --> 00:31:11 Um, so, uh, yeah, we wish them well. They're

00:31:11 --> 00:31:13 on their way back as we speak. And by the

00:31:13 --> 00:31:16 time you hear this podcast, they will have

00:31:16 --> 00:31:17 returned, no doubt.

00:31:18 --> 00:31:21 Um, that's it, Fred. Gosh, we got through

00:31:21 --> 00:31:22 that in a mighty hurry, didn't we?

00:31:23 --> 00:31:26 Professor Fred Watson: Um, yes, I think

00:31:26 --> 00:31:29 we. We gave it due, due

00:31:29 --> 00:31:32 recognition. We've been talking for well over

00:31:32 --> 00:31:33 an hour, Andrew.

00:31:35 --> 00:31:35 Andrew Dunkley: Oh, have we?

00:31:37 --> 00:31:40 Doesn't feel like it, but no. Um.

00:31:42 --> 00:31:45 Professor Fred Watson: 38 minutes. I'm sorry. I'm misreading my

00:31:45 --> 00:31:46 clock. You're right.

00:31:46 --> 00:31:46 Andrew Dunkley: That's okay.

00:31:47 --> 00:31:48 Professor Fred Watson: Well, we got through that in a hurry.

00:31:49 --> 00:31:51 Andrew Dunkley: You're probably reading a Mars clock because

00:31:51 --> 00:31:53 we talked about it. It's going a bit

00:31:53 --> 00:31:56 faster. Um, now

00:31:56 --> 00:31:59 if you were to follow, uh, up those stories,

00:31:59 --> 00:32:00 I've told you where to go and look for them.

00:32:00 --> 00:32:03 But you, uh, can also read the show notes on

00:32:03 --> 00:32:06 our website, spacenutspodcast.more space

00:32:06 --> 00:32:09 nuts IO and while you're

00:32:09 --> 00:32:12 there, uh, you might like to, um, check out

00:32:12 --> 00:32:14 all the. All the tabs and,

00:32:15 --> 00:32:17 uh, links on our. On our website, the, uh,

00:32:17 --> 00:32:19 Astronomy Daily feed. You can subscribe for

00:32:19 --> 00:32:21 your daily dose of astronomy and space

00:32:21 --> 00:32:24 Science news. Uh, don't forget reviews.

00:32:24 --> 00:32:26 We really do appreciate your reviews. The

00:32:26 --> 00:32:29 more reviews, the more we get noticed. And

00:32:29 --> 00:32:31 the more we get noticed, the more people

00:32:31 --> 00:32:33 listen. And then, you know, we can buy

00:32:33 --> 00:32:35 ourselves an ice cream at the end of the day.

00:32:35 --> 00:32:38 Um, you can also send questions

00:32:38 --> 00:32:41 or comments in through the AMA link and

00:32:41 --> 00:32:43 so on and so forth. And don't forget to visit

00:32:43 --> 00:32:45 the Space Nuts shop. Uh, that's one thing

00:32:45 --> 00:32:48 that Huw, um, did some years ago

00:32:48 --> 00:32:51 and it's been very popular. All the, uh,

00:32:51 --> 00:32:53 Space Nuts memorabilia, if you, if you want

00:32:53 --> 00:32:54 to get hold of it. I've got, I've got my

00:32:54 --> 00:32:56 Space Nuts cup here somewhere.

00:32:56 --> 00:32:58 Professor Fred Watson: Here it is. Look. Look at this.

00:32:59 --> 00:32:59 Andrew Dunkley: There it is.

00:32:59 --> 00:33:01 Professor Fred Watson: I never got, I never got one of those.

00:33:02 --> 00:33:03 Andrew Dunkley: I, I'd buy.

00:33:03 --> 00:33:06 It's

00:33:06 --> 00:33:07 good. That's good.

00:33:07 --> 00:33:08 Professor Fred Watson: I'm too stingy.

00:33:09 --> 00:33:12 Andrew Dunkley: Got shirts. We've got hoodies, we've got, uh,

00:33:12 --> 00:33:15 all sorts of bits and bobs at the Space Nuts

00:33:15 --> 00:33:17 Shop, uh, at our website. Thank, uh,

00:33:18 --> 00:33:19 you, Fred. We'll leave it there. We'll catch

00:33:19 --> 00:33:20 you on the next episode.

00:33:21 --> 00:33:22 Professor Fred Watson: Look forward to it, Andrew. See you soon.

00:33:23 --> 00:33:25 Andrew Dunkley: Professor Fred Watson, astronomer at large.

00:33:25 --> 00:33:28 And thanks to Huw in the studio, who couldn't

00:33:28 --> 00:33:30 be with us today, had to be evacuated

00:33:30 --> 00:33:33 after attempting, uh, a Michael Jackson

00:33:33 --> 00:33:35 moonwalk. Not good at his age.

00:33:35 --> 00:33:35 Professor Fred Watson: No.

00:33:35 --> 00:33:37 Andrew Dunkley: And from me, Andrew Dunkley, thanks for your

00:33:37 --> 00:33:39 company. We'll catch you on the next episode

00:33:39 --> 00:33:41 of Space Nuts.

00:33:41 --> 00:33:41 Professor Fred Watson: Bye.

00:33:41 --> 00:33:44 Voice Over Guy: Bye. You've been listening to the

00:33:44 --> 00:33:45 Space Nuts podcast,

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