Dwarf Planets, Peculiar Moons & the Mystery of Dark Matter

Dwarf Planets, Peculiar Moons & the Mystery of Dark Matter

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Exploring the Outer Solar System: New Dwarf Planets, Iapetus Mysteries, and Primordial Black Holes
In this captivating episode of Space Nuts, host Andrew Dunkley and the ever-knowledgeable Professor Fred Watson delve into the latest astronomical discoveries and theories that are reshaping our understanding of the cosmos. From the potential identification of a new dwarf planet to the intriguing features of Saturn's moon Iapetus and the enigmatic nature of primordial black holes, this episode is packed with cosmic insights.
Episode Highlights:
Potential New Dwarf Planet: Andrew and Fred Watson discuss the discovery of a new Trans-Neptunian object that could challenge the existence of Planet Nine. With its elongated orbit and significant distance from the Sun, this potential dwarf planet offers fresh perspectives on our solar system's architecture.
The Peculiar Moon Iapetus: The conversation shifts to Iapetus, a unique moon of Saturn known for its stark contrast in surface coloration and mysterious equatorial ridge. Andrew and Fred Watson explore the various theories regarding its formation and the renewed interest it has garnered in recent discussions.
Primordial Black Holes and Dark Matter: The episode wraps up with a deep dive into the theoretical research surrounding primordial black holes and their potential role in explaining dark matter. Fred shares insights from recent studies suggesting these ancient black holes might be more stable than previously thought, reigniting the debate on their contribution to the universe's missing mass.
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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.
(00:00) Welcome to Space Nuts with Andrew Dunkley and Fred Watson Watson
(01:20) Discussion on the potential new dwarf planet in the solar system
(15:00) Exploring the mysteries of Saturn's moon Iapetus
(25:30) Theoretical research on primordial black holes and dark matter
For commercial-free versions of Space Nuts, join us on Patreon, Supercast, Apple Podcasts, or become a supporter here: https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support.


00:00:00 --> 00:00:02 Andrew Dunkley: Hi there. Thanks for joining us. Andrew Dunkley here. Ah,

00:00:02 --> 00:00:05 this is Space Nuts, where we talk

00:00:05 --> 00:00:08 astronomy and space science. Thanks for

00:00:08 --> 00:00:11 joining us. Coming up on this episode, lots,

00:00:11 --> 00:00:14 to talk about and really interesting stuff for a change.

00:00:14 --> 00:00:16 No, as usual. and this one,

00:00:17 --> 00:00:20 I saw and thought, gee, we got to talk about this because we're

00:00:20 --> 00:00:23 always looking for something in the outer rim of

00:00:23 --> 00:00:26 the solar system and now we may have

00:00:26 --> 00:00:29 found something and it's not planet nine. In fact, it's

00:00:29 --> 00:00:31 possibly a new dwarf planet, which

00:00:31 --> 00:00:33 could mean there is no planet nine.

00:00:34 --> 00:00:37 Interesting. there's a peculiar moon,

00:00:37 --> 00:00:40 orbiting Saturn, known as Iapetus. And

00:00:40 --> 00:00:42 it's starting to get attention again.

00:00:42 --> 00:00:44 We'll tell you why. And

00:00:45 --> 00:00:48 primordial black holes. Yep. And

00:00:48 --> 00:00:51 the fact that they might be today's dark

00:00:51 --> 00:00:53 matter. Is that a matter we should discuss?

00:00:54 --> 00:00:56 Damn right it is. And we'll do m it.

00:00:57 --> 00:00:59 Do it right now on, Space nuts.

00:00:59 --> 00:01:02 Voice Over Guy: 15 seconds. Guidance is internal.

00:01:02 --> 00:01:05 10, 9. Ignition

00:01:05 --> 00:01:08 sequence start. Space nuts. 5, 4, 3,

00:01:08 --> 00:01:10 2. 1. 2, 3, 4, 5, 5, 4,

00:01:11 --> 00:01:14 3, 2, 1. Space nuts. Astronauts

00:01:14 --> 00:01:15 report it feels good.

00:01:15 --> 00:01:18 Andrew Dunkley: And despite his premature announcement,

00:01:19 --> 00:01:21 he officially welcome Professor Fred Watson Walton

00:01:22 --> 00:01:23 at large. Hello.

00:01:23 --> 00:01:26 Professor Fred Watson: Thank you for that. Yes, I do apologise for being there before. I'm,

00:01:26 --> 00:01:29 forgetting that I have to be formally introduced before I,

00:01:29 --> 00:01:30 Andrew Dunkley: More good.

00:01:30 --> 00:01:31 Professor Fred Watson: Yes, yes.

00:01:31 --> 00:01:34 Andrew Dunkley: Before, that's how I used to run my radio show. I didn't care

00:01:34 --> 00:01:37 what happened if some. If someone walked in. They were just part of the

00:01:37 --> 00:01:40 show. I didn't, you know, I

00:01:40 --> 00:01:42 never cared about standing on ceremony or,

00:01:42 --> 00:01:45 or, you know, sticking to the rules of radio.

00:01:46 --> 00:01:49 What rules? I mean, it's just people talking, isn't it? And

00:01:49 --> 00:01:52 playing music and enjoying themselves. I

00:01:52 --> 00:01:55 thought that's how I ran. Even when I

00:01:55 --> 00:01:57 worked for the nc, I was.

00:01:57 --> 00:01:58 Professor Fred Watson: I was like, that's right.

00:01:58 --> 00:02:01 Andrew Dunkley: I've been dropped for it a few times. But eventually

00:02:01 --> 00:02:04 they saw. They saw the light and started going, hang on a

00:02:04 --> 00:02:07 minute. Listening to this bloke. We

00:02:07 --> 00:02:09 might. We might be onto something.

00:02:09 --> 00:02:12 anyway, they eventually brought in an expert to teach us how

00:02:12 --> 00:02:14 to be human beings on the radio.

00:02:15 --> 00:02:16 Professor Fred Watson: Really give me dick.

00:02:18 --> 00:02:21 Andrew Dunkley: And when she, when she talked to me, she said, don't change

00:02:21 --> 00:02:24 a thing. Which I really. A great endorsement

00:02:24 --> 00:02:26 after being told shut up for several years.

00:02:27 --> 00:02:28 Professor Fred Watson: No. Well done. That's good.

00:02:29 --> 00:02:32 Andrew Dunkley: Now, before we get started, how's the weather down in

00:02:32 --> 00:02:35 Sydney? Because you've been copping us spanking with the

00:02:35 --> 00:02:35 rain.

00:02:35 --> 00:02:38 Professor Fred Watson: We did? Yes. one day last week, just

00:02:38 --> 00:02:40 overnight, we had 97 millimetres or

00:02:41 --> 00:02:44 getting on for five. Well four inches, isn't it in

00:02:44 --> 00:02:47 the measure? Yeah, that's right, four inches. that was

00:02:47 --> 00:02:50 just one night and all together we probably had something like

00:02:50 --> 00:02:52 150 of that wet period.

00:02:52 --> 00:02:53 Andrew Dunkley: Yeah.

00:02:53 --> 00:02:55 Professor Fred Watson: So it was very wet, very miserable, very

00:02:55 --> 00:02:58 soggy. fortunately everything seemed to hold up.

00:02:58 --> 00:03:01 Our downstairs granny flat which used to

00:03:01 --> 00:03:04 flood when it rained but we had a lot of work done last year.

00:03:04 --> 00:03:06 That's was in good shape.

00:03:08 --> 00:03:09 Everything seemed to be all right.

00:03:09 --> 00:03:12 Andrew Dunkley: Yeah, I shouldn't tell you that right now

00:03:12 --> 00:03:15 as we record there's a big

00:03:15 --> 00:03:17 rain band headed your way.

00:03:17 --> 00:03:19 Professor Fred Watson: Yes there is. That's right. We we already.

00:03:20 --> 00:03:23 Andrew Dunkley: It's easing off now. We had rain all day but I'm looking

00:03:23 --> 00:03:23 out now.

00:03:24 --> 00:03:24 Professor Fred Watson: Yeah.

00:03:24 --> 00:03:27 Andrew Dunkley: And it stopped raining. This the sky is actually

00:03:27 --> 00:03:29 thinning. It's still quite grey but it's moving

00:03:30 --> 00:03:32 that way which is more due me.

00:03:33 --> 00:03:36 Professor Fred Watson: It is. We're expecting that later this

00:03:36 --> 00:03:39 afternoon. It sort of started off quite bright this morning but it

00:03:39 --> 00:03:41 is definitely looking a bit grayer now.

00:03:41 --> 00:03:43 Andrew Dunkley: So yeah, I, I have some news.

00:03:44 --> 00:03:47 At 2:37am M.

00:03:47 --> 00:03:50 Saturday, oh, our

00:03:50 --> 00:03:51 bedroom door rattled.

00:03:52 --> 00:03:53 Professor Fred Watson: Okay.

00:03:53 --> 00:03:56 Andrew Dunkley: And I, my first thought was that was an earth

00:03:56 --> 00:03:59 tremor. And guess what it was.

00:03:59 --> 00:04:01 It was a five point. Well they keep

00:04:02 --> 00:04:05 varying it but at the time it was a 5.3

00:04:05 --> 00:04:08 earthquake, centred around north of

00:04:08 --> 00:04:11 Ningen which is Ningen's

00:04:11 --> 00:04:13 160 kilometres west of us. And the

00:04:13 --> 00:04:15 earthquake was north of them by about

00:04:15 --> 00:04:18 98Ks. So it was a bit further

00:04:18 --> 00:04:21 than 160 kilometres from us. And

00:04:21 --> 00:04:24 yeah it shook because our door doesn't quite latch

00:04:24 --> 00:04:27 perfectly, it doesn't hold tight so it's always a bit

00:04:27 --> 00:04:30 loose. So when the air conditioning comes on it usually goes thump.

00:04:31 --> 00:04:34 They said did more than thump on Saturday morning I went

00:04:35 --> 00:04:37 and I woke up, went oh, earthquake. And Judy went,

00:04:38 --> 00:04:41 you sure? Really? I said yeah, I reckon it was because

00:04:41 --> 00:04:43 nothing else happened. Didn't feel any vibration.

00:04:43 --> 00:04:46 Professor Fred Watson: Okay, that's interesting. Yeah. You didn't feel it, Just the door

00:04:46 --> 00:04:46 did.

00:04:47 --> 00:04:50 Andrew Dunkley: well we got a great bed. Just very.

00:04:50 --> 00:04:51 Professor Fred Watson: That's quite proof.

00:04:51 --> 00:04:53 Andrew Dunkley: I had a lot for it. But yeah, it worked. We didn't feel the

00:04:53 --> 00:04:56 earthquake but yeah, sure enough next morning I thought

00:04:56 --> 00:04:59 I'd check and Geosciences Australia confirmed

00:04:59 --> 00:05:02 it. So 5.3 which is 1 of the biggest

00:05:02 --> 00:05:03 ever recorded out here.

00:05:05 --> 00:05:07 Professor Fred Watson: Yes, that's right. Yeah it is. So one of my

00:05:07 --> 00:05:10 colleagues at ah, the Australian Astronomical Observatory or

00:05:10 --> 00:05:13 former Australian Astronomical Observatory on the Anglo

00:05:13 --> 00:05:15 Australian Telescope, he is One of the telescope,

00:05:16 --> 00:05:19 operators, Andre Phillips, he

00:05:19 --> 00:05:22 was sitting in the control chair for the

00:05:22 --> 00:05:25 telescope and he felt something as well.

00:05:25 --> 00:05:28 He felt the chair being sort of moved,

00:05:28 --> 00:05:30 as though somebody was shaking it from behind.

00:05:30 --> 00:05:33 Andrew Dunkley: Yeah, that's what it feels like. Yeah. Because I was in

00:05:33 --> 00:05:36 Newcastle earthquake and I'd done an overnight shift when it

00:05:36 --> 00:05:37 hit and it was 5.5.

00:05:38 --> 00:05:41 And it felt to me like somebody just got

00:05:41 --> 00:05:44 the end of the bed and was just bouncing,

00:05:44 --> 00:05:47 bouncing it up and down and. Yeah, it was much more violent

00:05:47 --> 00:05:48 than what we experienced.

00:05:48 --> 00:05:51 Professor Fred Watson: It would be. Yeah. yeah, actually, Andre,

00:05:51 --> 00:05:53 interestingly, this same gentleman I was just talking about, he

00:05:53 --> 00:05:56 also runs, a very sensitive seismograph at

00:05:56 --> 00:05:59 home because he's quite interested in seismometry.

00:06:00 --> 00:06:02 so, yes, I think he went home at the end of his night shift,

00:06:02 --> 00:06:05 had a look, and sure enough there was a 5.3 or

00:06:05 --> 00:06:07 5.2 earthquake, from

00:06:07 --> 00:06:08 Lingen.

00:06:08 --> 00:06:11 Andrew Dunkley: Yeah, he would have felt more of it in Coonabarabran than

00:06:11 --> 00:06:14 he calculation because,

00:06:14 --> 00:06:17 I looked at the clock immediately and it was 2:37.

00:06:18 --> 00:06:21 And I know that was the exact time because it was an

00:06:21 --> 00:06:24 apple watch. So it was synchronised.

00:06:24 --> 00:06:24 Professor Fred Watson: Yeah.

00:06:24 --> 00:06:27 Andrew Dunkley: And I worked out that the vibration took

00:06:27 --> 00:06:28 40 seconds to reach us.

00:06:29 --> 00:06:30 Professor Fred Watson: Okay.

00:06:30 --> 00:06:32 Andrew Dunkley: At approximately 300 kilometres an hour.

00:06:32 --> 00:06:33 Professor Fred Watson: Yeah.

00:06:34 --> 00:06:34 Andrew Dunkley: Just round.

00:06:35 --> 00:06:37 Professor Fred Watson: Yes. Yeah, something like that.

00:06:38 --> 00:06:41 Andrew Dunkley: Yeah. Anyway, give, Or take, because I

00:06:41 --> 00:06:44 don't. It wasn't exactly 236, but you know

00:06:44 --> 00:06:47 what I'm saying. yeah. So

00:06:47 --> 00:06:49 exciting. Exciting. Haven't been any aftershocks that I'm aware

00:06:49 --> 00:06:52 of. But, there's a lot of tremors out here that you don't ever feel

00:06:52 --> 00:06:55 or notice because they're just so small. But,

00:06:55 --> 00:06:58 nothing that big. We better get

00:06:58 --> 00:06:59 on with it, Fred Watson.

00:06:59 --> 00:07:02 And our first story,

00:07:02 --> 00:07:05 from the cosmos or closer to home, is a possible

00:07:05 --> 00:07:08 new dwarf planet, in the extremities

00:07:08 --> 00:07:11 of our solar system. This is, really

00:07:11 --> 00:07:13 exciting, if it holds true and

00:07:13 --> 00:07:16 it's sort of stacking up that way.

00:07:16 --> 00:07:18 Professor Fred Watson: I think so, yes. this is

00:07:19 --> 00:07:20 relatively straightforward,

00:07:21 --> 00:07:24 astrometry, which is the measurement of

00:07:25 --> 00:07:28 celestial objects in space, their actual,

00:07:28 --> 00:07:31 direction. and it,

00:07:31 --> 00:07:34 comes from, information

00:07:34 --> 00:07:37 collected over quite a long period of time,

00:07:38 --> 00:07:40 with, telescopes around the world.

00:07:41 --> 00:07:44 so a lot of this discovery is due to archival data

00:07:45 --> 00:07:48 where you can look at images of particular bits of the sky

00:07:48 --> 00:07:50 and accurately work out the position of objects in

00:07:50 --> 00:07:53 those images. it's actually what you do,

00:07:53 --> 00:07:56 Andrew. Just as an aside here, when a near Earth

00:07:56 --> 00:07:59 asteroid is detected

00:08:00 --> 00:08:02 the first thing astronomers do is look back

00:08:02 --> 00:08:04 through archival, data. To see if there are any,

00:08:05 --> 00:08:08 images, photographic images or electronically

00:08:08 --> 00:08:11 detected images that will show it. Because the longer

00:08:11 --> 00:08:14 you can observe something for, the more accurately you can

00:08:14 --> 00:08:17 deduce its orbit. And that is true with

00:08:17 --> 00:08:19 this object, which turns out to be a

00:08:19 --> 00:08:22 tno, a Trans Neptunian object.

00:08:23 --> 00:08:24 it's been, studied by,

00:08:25 --> 00:08:28 astrophysicists at the Institute for Advanced Study in

00:08:28 --> 00:08:30 Princeton. Very, very distinguished,

00:08:31 --> 00:08:33 institution. and what they found,

00:08:34 --> 00:08:36 is an object with the very

00:08:36 --> 00:08:38 unmemorable name of 2017 of

00:08:39 --> 00:08:41 201. it is

00:08:41 --> 00:08:44 an. An object. A trans Neptunian object

00:08:44 --> 00:08:47 in a very, very elongated orbit.

00:08:48 --> 00:08:51 its nearest point to

00:08:51 --> 00:08:54 the solar system is. I think

00:08:54 --> 00:08:56 it's 42,

00:08:57 --> 00:08:59 thereabouts astronomical unit. Is that right?

00:08:59 --> 00:09:01 No. 44,

00:09:01 --> 00:09:04 44.5. That's its closest point to the

00:09:04 --> 00:09:07 Sun. What we call the perihelion. 44.5

00:09:08 --> 00:09:10 times that of the Earth's orbit. In other words,

00:09:10 --> 00:09:12 44.5 astronomical UN.

00:09:13 --> 00:09:16 But the staggering thing is that it's

00:09:16 --> 00:09:19 aphelion. the furthest point,

00:09:20 --> 00:09:23 is, Now let me find

00:09:23 --> 00:09:25 the number. It's much, much higher. You might have

00:09:25 --> 00:09:26 32.

00:09:29 --> 00:09:31 I think it's more than that. where are

00:09:31 --> 00:09:34 we? I think it's in the thousands. it's,

00:09:35 --> 00:09:38 very, very distant. So

00:09:38 --> 00:09:41 when it was found. I beg your

00:09:41 --> 00:09:44 par. Yeah, when it was found, it was about 90

00:09:45 --> 00:09:47 astronomical units away.

00:09:48 --> 00:09:50 and there are enough observations that it's

00:09:51 --> 00:09:53 sort of continuing its orbit.

00:09:53 --> 00:09:56 1600. Yeah, 1600

00:09:56 --> 00:09:59 astronomical units. That's its

00:09:59 --> 00:10:01 furthest. And, that means that,

00:10:02 --> 00:10:05 it's only going to be visible to Earth. based

00:10:05 --> 00:10:08 telescopes for a few percent of its orbit. When

00:10:08 --> 00:10:11 it's, when it's at its nearest, point

00:10:11 --> 00:10:12 to Earth.

00:10:12 --> 00:10:15 Andrew Dunkley: They're actually saying, Fred Watson, that it's going far

00:10:15 --> 00:10:18 enough out to be entering the Oort

00:10:18 --> 00:10:18 cloud.

00:10:18 --> 00:10:21 Professor Fred Watson: That's right. Part of the inner Oort cloud, which makes it a very

00:10:21 --> 00:10:24 interesting object indeed with

00:10:24 --> 00:10:27 an orbital period, if I remember rightly, of. What is it,

00:10:27 --> 00:10:30 25 light years or something ridiculous like

00:10:30 --> 00:10:30 that.

00:10:30 --> 00:10:32 Andrew Dunkley: 25 years to complete an orbit.

00:10:33 --> 00:10:36 Professor Fred Watson: Sorry, 25 years, not 25 light years.

00:10:36 --> 00:10:39 Yeah. So it's a very, very distant object.

00:10:39 --> 00:10:41 In fact, it's probably, Apart from

00:10:41 --> 00:10:44 comets, it's probably one of the most distant

00:10:44 --> 00:10:46 objects ever discovered.

00:10:47 --> 00:10:50 because at its nearest, it's roughly the same

00:10:50 --> 00:10:53 distance from the sun as Pluto is. But it's furthest,

00:10:53 --> 00:10:56 as you've said. It's skimming the inner edge of the

00:10:56 --> 00:10:58 Oort Cloud, that cloud of, icy debris

00:10:58 --> 00:11:01 that we recognise as being the source of comets,

00:11:01 --> 00:11:04 comets that drifting towards the inner solar system.

00:11:05 --> 00:11:08 So a, really, remarkable,

00:11:08 --> 00:11:11 set of observations. It's been observed 19 times, so

00:11:11 --> 00:11:14 it's got a very high certainty in its

00:11:14 --> 00:11:17 orbit. but the quirky part

00:11:17 --> 00:11:20 of this, which you've already alluded to, is

00:11:20 --> 00:11:23 that, when the team, the

00:11:23 --> 00:11:26 research team who've done this work, actually

00:11:26 --> 00:11:29 looked at the simulations of,

00:11:29 --> 00:11:31 the way the orbit of 2017, of

00:11:31 --> 00:11:34 201, behaves,

00:11:34 --> 00:11:37 they found that, its

00:11:37 --> 00:11:40 orbit is only stable and long

00:11:40 --> 00:11:43 term without Planet Nine.

00:11:44 --> 00:11:46 so if you have Planet Nine in the

00:11:46 --> 00:11:49 equation, then it gets thrown out within

00:11:49 --> 00:11:52 100 million years, which means that's a short time

00:11:52 --> 00:11:55 in astronomical terms. So,

00:11:55 --> 00:11:57 yeah, it's it's that if.

00:11:57 --> 00:11:59 Andrew Dunkley: Its existence is confirmed,

00:12:00 --> 00:12:03 then Planet nine can't exist.

00:12:03 --> 00:12:04 That's what they're saying.

00:12:04 --> 00:12:07 Professor Fred Watson: That is what they are saying, yes. That it's. This is,

00:12:07 --> 00:12:10 a quote from the media. It's one of the

00:12:10 --> 00:12:13 strongest pieces of evidence yet against the

00:12:13 --> 00:12:14 existence of Planet Nine.

00:12:16 --> 00:12:19 yeah, that's right. it, it, it does

00:12:19 --> 00:12:22 suggests that there are more objects of the same

00:12:22 --> 00:12:25 kind. We haven't found them yet. but yes, the

00:12:25 --> 00:12:27 figure I was looking for earlier, it spends

00:12:28 --> 00:12:30 only 1% of its time in orbit, near

00:12:30 --> 00:12:33 enough to be able to be detected from Earth

00:12:34 --> 00:12:37 because it's such a. It's a relatively small

00:12:37 --> 00:12:40 object thought to be around 700 kilometres, which probably

00:12:40 --> 00:12:42 makes it a dwarf planet rather than a large

00:12:43 --> 00:12:45 asteroid. and, the, that's

00:12:46 --> 00:12:48 imagining that something that size can

00:12:48 --> 00:12:51 only be visible for 1% of its orbital

00:12:51 --> 00:12:54 period because the rest just takes it too far away.

00:12:54 --> 00:12:57 It gives you a good idea of just how elongated its

00:12:57 --> 00:12:58 orbit is.

00:12:58 --> 00:13:01 Andrew Dunkley: Gee, we're lucky to have spotted it given the timeframe.

00:13:01 --> 00:13:04 Professor Fred Watson: Well, that's right, yes. because it'll drift away and will

00:13:04 --> 00:13:06 very soon be, invisible to our

00:13:07 --> 00:13:07 planet.

00:13:07 --> 00:13:10 Andrew Dunkley: And it's a lot of weight to a theory we talked about

00:13:10 --> 00:13:13 some time ago from one

00:13:13 --> 00:13:16 scientist who said there is no Planet Nine.

00:13:16 --> 00:13:19 I think there's a whole bunch of stuff out there

00:13:19 --> 00:13:22 that's causing the same effect. And this

00:13:22 --> 00:13:24 sounds like one of those things.

00:13:24 --> 00:13:27 Professor Fred Watson: Yes, that's right. And it's similar. There was

00:13:27 --> 00:13:30 a similar argument around the same time by another group of

00:13:30 --> 00:13:33 scientists, one of whom I actually spoke to in

00:13:33 --> 00:13:35 Canada a couple of years ago, who said

00:13:35 --> 00:13:38 effectively that the evidence for Planet Nine is

00:13:38 --> 00:13:41 based on. I don't know it's probably a dozen or

00:13:41 --> 00:13:44 so of these icy asteroids all

00:13:44 --> 00:13:47 of whose elongated orbits sort of line up

00:13:47 --> 00:13:50 in the same way. And the suggestion

00:13:50 --> 00:13:53 that was being made by these other scientists is that

00:13:53 --> 00:13:56 actually it's not so much

00:13:56 --> 00:13:59 that it's a selection effect. We just haven't found all the other

00:13:59 --> 00:14:02 ones that aren't aligned in the same way. that

00:14:02 --> 00:14:04 would contradict the idea of Planet nine.

00:14:05 --> 00:14:08 So yes, this object might be the poster child

00:14:08 --> 00:14:11 of the anti Planet nine lobby.

00:14:11 --> 00:14:14 but it does seem to suggest that it does

00:14:14 --> 00:14:16 not Planet nine does not exist. And just

00:14:16 --> 00:14:19 to underline what

00:14:19 --> 00:14:22 we're saying earlier, it has actually been officially

00:14:22 --> 00:14:25 confirmed as an asteroid

00:14:25 --> 00:14:28 by the International Astronomical Union. So it

00:14:28 --> 00:14:31 will no doubt get a name because once it's confirmed

00:14:31 --> 00:14:34 by the IAU then you can give it a name.

00:14:34 --> 00:14:36 Andrew Dunkley: Asteroid or dwarf planet.

00:14:38 --> 00:14:41 Professor Fred Watson: I mean a, ah, name like you know, Pluto

00:14:41 --> 00:14:44 or Makemake or one of

00:14:44 --> 00:14:44 those names.

00:14:45 --> 00:14:46 Andrew Dunkley: But we're calling it a dwarf planet.

00:14:46 --> 00:14:49 Professor Fred Watson: That's, that's right, that's right, yeah. At 700

00:14:49 --> 00:14:52 kilometres. I don't think the IAU makes a

00:14:52 --> 00:14:54 distinction when they, when they actually

00:14:55 --> 00:14:58 confirm its orbit. They don't say anything about its

00:14:58 --> 00:15:00 size because that's

00:15:00 --> 00:15:03 dependent on, but that, that depends on measurements that are a

00:15:03 --> 00:15:06 lot more difficult to do. But once its orbit's been confirmed

00:15:06 --> 00:15:09 then it becomes an official object which could be

00:15:09 --> 00:15:11 either a dwarf planet or an asteroid.

00:15:11 --> 00:15:14 Andrew Dunkley: Okay, all right, so the jury might still be out

00:15:14 --> 00:15:17 for a bit but yes, it's there and it

00:15:17 --> 00:15:19 looks like that's put the kibosh on

00:15:19 --> 00:15:22 Planet Nine. More to come on

00:15:22 --> 00:15:25 that one I'm sure. Yes. Now

00:15:25 --> 00:15:27 if you'd like to read all about it you can do

00:15:27 --> 00:15:29 that@sciencealert.com

00:15:30 --> 00:15:32 this is space Nuts, Andrew Dunkley here with

00:15:32 --> 00:15:34 Professor Fred Watson Watson.

00:15:35 --> 00:15:38 Now let's take a quick break from the show to tell you

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00:18:16 --> 00:18:18 Now back to Space Nuts.

00:18:20 --> 00:18:23 Space Nuts. Let's move on to our, next story.

00:18:23 --> 00:18:26 Fred Watson, I find this one fascinating for one

00:18:26 --> 00:18:29 reason. This is going to sound strange. I've

00:18:29 --> 00:18:30 never heard of this place.

00:18:31 --> 00:18:33 Professor Fred Watson: Oh really? I think I heard of it.

00:18:33 --> 00:18:35 Andrew Dunkley: it's a moon of Saturn known as

00:18:35 --> 00:18:38 Iapetus now. And I say I've never

00:18:38 --> 00:18:41 heard of it. When I saw the picture I went, oh, yeah, I know I've

00:18:41 --> 00:18:43 seen that picture before. Yes,

00:18:44 --> 00:18:47 because it's unique. That's why,

00:18:47 --> 00:18:49 this moon is so very interesting.

00:18:50 --> 00:18:53 Because questions are still being asked as to how it looks

00:18:53 --> 00:18:56 the way it does. It's a strange place and

00:18:56 --> 00:18:59 it's getting, a fair bit of attention in

00:18:59 --> 00:19:00 social media at the moment,

00:19:02 --> 00:19:04 amongst other things. But, yes, it's back in the news.

00:19:04 --> 00:19:07 Professor Fred Watson: It is back in the news. I think it is really, as you say, I think

00:19:07 --> 00:19:10 it really is social media that stirred this up.

00:19:11 --> 00:19:13 we. So, you know, until 2017,

00:19:13 --> 00:19:16 when the spacecraft plunged into the

00:19:16 --> 00:19:18 atmosphere of Saturn,

00:19:19 --> 00:19:20 we were absolutely,

00:19:21 --> 00:19:24 swamped by marvellous photographs of

00:19:24 --> 00:19:27 the moons of Saturn from the Cassini

00:19:27 --> 00:19:29 spacecraft. told us more about the moons of Saturn than we

00:19:29 --> 00:19:32 could ever have guessed that we'd learn.

00:19:33 --> 00:19:35 and I think, So Iapetus was

00:19:36 --> 00:19:38 certainly very much in the headlines then because it is such a

00:19:38 --> 00:19:41 peculiar world. but it sort of.

00:19:41 --> 00:19:44 Because so many of the questions don't really have proper

00:19:44 --> 00:19:47 answers, that's allowed

00:19:47 --> 00:19:50 it to sort of fade from, from the

00:19:50 --> 00:19:52 attention of planetary scientists. But

00:19:53 --> 00:19:55 it's been spotted by, I mean

00:19:55 --> 00:19:58 spotted in the media by social, Social

00:19:58 --> 00:20:01 media people who have really raised it

00:20:01 --> 00:20:04 once again, you know, as a place of

00:20:04 --> 00:20:07 great interest. And maybe that will encourage some of

00:20:07 --> 00:20:10 the planetary, scientists who've certainly had an interest

00:20:10 --> 00:20:13 in Iapetus, to go back to some of the

00:20:13 --> 00:20:15 Cassini data, maybe using, you know, more

00:20:15 --> 00:20:18 modern AI methods to analyse it and

00:20:18 --> 00:20:21 actually check out what is going on there.

00:20:22 --> 00:20:25 so it's the first thing you'd find

00:20:25 --> 00:20:28 out about Yapetus. And it

00:20:28 --> 00:20:31 was when it was discovered back in

00:20:31 --> 00:20:34 the 17th century, Giovanni

00:20:34 --> 00:20:36 Cassini, that great, observer who

00:20:36 --> 00:20:39 discovered the Cassini Division since the name,

00:20:41 --> 00:20:44 made the discovery that this, this

00:20:44 --> 00:20:46 little world orbiting Saturn,

00:20:47 --> 00:20:49 is peculiar because one side of it

00:20:49 --> 00:20:52 was very much darker than the other. I remember

00:20:52 --> 00:20:55 actually at the start of my career, back in the,

00:20:56 --> 00:20:58 early 1970s when I was working at the Nautical

00:20:58 --> 00:21:01 Almanack Office of the Royal Greenwich Observatory with one

00:21:01 --> 00:21:04 of my colleagues there, Andy Sinclair was a specialist on

00:21:04 --> 00:21:07 Iapetus and he kept telling me it was a very peculiar

00:21:07 --> 00:21:10 world. but it was only when Cassini flew

00:21:10 --> 00:21:13 by a few decades later that we realised just how peculiar

00:21:13 --> 00:21:16 it is. So it is covered in

00:21:16 --> 00:21:19 craters, but it's got

00:21:19 --> 00:21:21 this dark side which just looks as though

00:21:21 --> 00:21:24 it's been spattered with soot. Looks as though,

00:21:24 --> 00:21:27 you know, somebody's put a pile of soot out there

00:21:28 --> 00:21:29 and Iapetus, has run into it.

00:21:31 --> 00:21:33 and you've. So you've got this very dark face to it,

00:21:34 --> 00:21:36 contrasting with a very highly reflective

00:21:36 --> 00:21:39 surface. now

00:21:39 --> 00:21:42 that's peculiar in itself because

00:21:42 --> 00:21:45 it's only on one side and that's the forward facing

00:21:45 --> 00:21:47 side. Iapetus goes around Saturn

00:21:47 --> 00:21:50 tidally locked, so that it always keeps the same face

00:21:50 --> 00:21:53 to Saturn. That means there's always a forward side and

00:21:53 --> 00:21:56 a backward side. This stuff's on the forward side.

00:21:56 --> 00:21:59 If I'm actually remembering from my, talks

00:21:59 --> 00:22:02 on Cassini, ah, back in the day, I haven't done one of

00:22:02 --> 00:22:04 those for nearly a decade. But anyway,

00:22:05 --> 00:22:08 that's the one peculiar thing about it, but

00:22:08 --> 00:22:11 the other one is even weirder. And this is

00:22:11 --> 00:22:14 this equatorial ridge, a ridge that goes

00:22:14 --> 00:22:16 all the way around it. It's something like 10

00:22:16 --> 00:22:19 kilometres, or thereabouts.

00:22:19 --> 00:22:22 It's a line of mountains, effectively, but

00:22:22 --> 00:22:25 it's right along the equator

00:22:25 --> 00:22:26 of Iapetus.

00:22:27 --> 00:22:29 Andrew Dunkley: It reminds me of a walnut.

00:22:30 --> 00:22:33 Professor Fred Watson: It is. That's right. I used to think it looked like a walnut.

00:22:33 --> 00:22:35 Exactly that. and so,

00:22:36 --> 00:22:38 I mean, there's various theories as to how it got

00:22:38 --> 00:22:41 there. And the one that I thought was the most

00:22:41 --> 00:22:44 common one, was

00:22:44 --> 00:22:47 that, it was caused by the contraction of

00:22:47 --> 00:22:49 the crust of Iapetus.

00:22:49 --> 00:22:50 Andrew Dunkley: That makes sense.

00:22:50 --> 00:22:51 Professor Fred Watson: the, you know,

00:22:53 --> 00:22:55 Iapetus cooled after its creation.

00:22:55 --> 00:22:58 it's rotating on its axis. the

00:22:58 --> 00:23:01 crust contracts until you get a

00:23:01 --> 00:23:04 bulge which naturally forms around the

00:23:04 --> 00:23:07 equator of rotation, right angles to the axis

00:23:07 --> 00:23:09 of rotation. But, I think other

00:23:09 --> 00:23:12 hypotheses have, have

00:23:12 --> 00:23:15 been put forward. One is

00:23:15 --> 00:23:18 that perhaps there was a ring system

00:23:18 --> 00:23:21 around Iapetus that actually

00:23:21 --> 00:23:23 collapsed and fell onto the surface and

00:23:23 --> 00:23:26 generated the ring of mountains.

00:23:26 --> 00:23:29 another one is possibly icy material

00:23:29 --> 00:23:32 coming out from beneath the surface of

00:23:32 --> 00:23:34 Iapetus. We know that, many of the

00:23:34 --> 00:23:37 moons of the, of those outer planets,

00:23:38 --> 00:23:41 got ice or perhaps icy

00:23:41 --> 00:23:44 slush underneath the surface.

00:23:44 --> 00:23:47 because of, the fact that they're what we call ice

00:23:47 --> 00:23:50 worlds with a, with a central rocky core, a,

00:23:50 --> 00:23:53 liquid ocean above it, which may be quite

00:23:53 --> 00:23:56 slushy. and then a crust of solid ice on top of

00:23:56 --> 00:23:59 that. That could be the construction. Once again, if you've

00:23:59 --> 00:24:02 got stuff coming up from beneath the surface and the object

00:24:02 --> 00:24:05 is spinning fast enough, then you will get,

00:24:05 --> 00:24:07 perhaps a ring of mountains like we

00:24:07 --> 00:24:09 see on the apertus,

00:24:10 --> 00:24:13 none of which come from the original idea, which was

00:24:13 --> 00:24:16 contraction. So I'm very interested

00:24:16 --> 00:24:19 to know where the scientific, you know, the scientific,

00:24:20 --> 00:24:23 consensus is going on this little world. And, it's

00:24:23 --> 00:24:26 great that it's, it's cropped up again, it's welled up again

00:24:26 --> 00:24:27 into the public consciousness.

00:24:28 --> 00:24:31 Andrew Dunkley: It has, yeah. Another theory I read was just a

00:24:31 --> 00:24:32 high spin rate at some stage.

00:24:32 --> 00:24:33 Professor Fred Watson: Yes.

00:24:33 --> 00:24:36 Andrew Dunkley: Yeah, that would Cause a bulge rather

00:24:36 --> 00:24:38 than a mountain range. I would, I would expect that.

00:24:39 --> 00:24:42 Professor Fred Watson: Well you'd normally that causes a

00:24:42 --> 00:24:45 planet to flatten slightly so that it's

00:24:46 --> 00:24:48 it's. Yes it's a bulge. It's the ah, Earth's

00:24:48 --> 00:24:51 shape is that ah, what we call an oblate spheroid.

00:24:52 --> 00:24:55 Saturn itself actually is the most extreme example in the

00:24:55 --> 00:24:57 solar system because it's the

00:24:57 --> 00:25:00 diameter between the poles is

00:25:00 --> 00:25:02 significantly less than the diameter across the equator.

00:25:03 --> 00:25:06 and it's this kind of oval shape in cross

00:25:06 --> 00:25:09 section. so that's what you'd

00:25:09 --> 00:25:12 expect from something rotating quickly not as

00:25:12 --> 00:25:14 a well defined ridge of

00:25:14 --> 00:25:17 mountains like we see on Iapetus.

00:25:17 --> 00:25:19 Quite an amazing world.

00:25:19 --> 00:25:22 Andrew Dunkley: Another weird factor I suppose is its

00:25:22 --> 00:25:24 proximity to Saturn. It's actually a long way away.

00:25:25 --> 00:25:27 Professor Fred Watson: Very far. Yes, that's right. So what is it?

00:25:27 --> 00:25:30 3.2 million millimetres or

00:25:30 --> 00:25:33 thereabouts? It's a long, long way,

00:25:33 --> 00:25:35 3.22 million kilometres from Saturn.

00:25:38 --> 00:25:41 Andrew Dunkley: Could the dark face be some sort of reaction with

00:25:41 --> 00:25:43 Saturn radiation or something like that?

00:25:43 --> 00:25:46 Professor Fred Watson: It's the thinking back in the

00:25:46 --> 00:25:48 Cassini era and I suspect it's probably similar

00:25:49 --> 00:25:51 is that it consists of organic chemicals

00:25:52 --> 00:25:55 that form this kind of soot. I think

00:25:55 --> 00:25:58 solens might have been in invoked

00:25:58 --> 00:26:01 as well. These are particular organic chemicals

00:26:01 --> 00:26:04 that we know coat a lot of the outer

00:26:04 --> 00:26:07 worlds because they're generated by I think the

00:26:07 --> 00:26:09 impact of cosmic rays on material.

00:26:10 --> 00:26:13 but it's the peculiar thing is that

00:26:13 --> 00:26:16 it's ah, only on one side. It looks as though it's just

00:26:16 --> 00:26:19 kind of run into something that's splattered all over the front of

00:26:19 --> 00:26:19 it.

00:26:19 --> 00:26:21 Andrew Dunkley: It's got that impression. Yeah. Somebody spilled the paint.

00:26:23 --> 00:26:24 Professor Fred Watson: Just what it looks like. That's why.

00:26:24 --> 00:26:27 Andrew Dunkley: Really odd. Yeah. If you'd like to take a look at it. Yapetis

00:26:28 --> 00:26:31 is all over the Internet, lots of social media. But there's a great

00:26:31 --> 00:26:34 article@dailygalaxy.com worth

00:26:34 --> 00:26:37 reading on Yapetis. It starts with an I. It's

00:26:37 --> 00:26:40 spelled I A P E T U S

00:26:40 --> 00:26:43 Yapetus. This is Space Nuts with Andrew

00:26:43 --> 00:26:44 Dunkley and Fred Watson Watson.

00:26:47 --> 00:26:49 Roger, you're last Nuts.

00:26:50 --> 00:26:53 Our final story today Fred Watson ah,

00:26:53 --> 00:26:55 takes us to the very rare

00:26:56 --> 00:26:58 area of black hole discussion.

00:26:59 --> 00:27:02 we get so many questions on this. I mean

00:27:02 --> 00:27:05 it's, it's unbelievable. In fact I think there was

00:27:05 --> 00:27:07 a question popping up about black holes

00:27:08 --> 00:27:11 in our next episode as a matter of fact. But and,

00:27:11 --> 00:27:14 and I think the reason is quite simple. People

00:27:14 --> 00:27:16 just want to understand Them and

00:27:16 --> 00:27:18 there's so much we don't know.

00:27:20 --> 00:27:23 this particular story focuses on

00:27:23 --> 00:27:26 primordial black holes and the possibility that

00:27:26 --> 00:27:29 they may well be responsible for today's

00:27:29 --> 00:27:31 dark matter. Please

00:27:31 --> 00:27:32 explain.

00:27:34 --> 00:27:37 Professor Fred Watson: Well, yeah, this is a piece of theoretical

00:27:37 --> 00:27:40 research which is good

00:27:40 --> 00:27:42 because you need it. it's ah,

00:27:43 --> 00:27:45 this is research by Japanese scientists

00:27:46 --> 00:27:48 in Tokyo and elsewhere. and

00:27:49 --> 00:27:52 what you have got here is

00:27:52 --> 00:27:54 people who are ah, looking

00:27:55 --> 00:27:58 sort of almost with new eyes if I can put it that way, at

00:27:58 --> 00:28:00 the dark matter problem because

00:28:01 --> 00:28:04 dark matter is a big problem. We've got this stuff

00:28:04 --> 00:28:07 that seems to have a gravitational hold on galaxies

00:28:07 --> 00:28:10 so that they don't fly ap. and a ah,

00:28:10 --> 00:28:13 gravitational hold on galaxy clusters so

00:28:13 --> 00:28:15 they don't fly apart as well. and yet we can't

00:28:15 --> 00:28:18 detect it. We cannot detect it in any way

00:28:18 --> 00:28:21 other than by its gravitational pull.

00:28:21 --> 00:28:23 Andrew Dunkley: Yeah, we've never captured any of it or

00:28:24 --> 00:28:25 anything like that.

00:28:25 --> 00:28:28 Professor Fred Watson: No, that's right. So this, the, the you know,

00:28:28 --> 00:28:30 what, what, what have we got to go on?

00:28:31 --> 00:28:34 Not very much, ah, in terms of

00:28:35 --> 00:28:38 our understanding. however

00:28:39 --> 00:28:42 there was quite early on in the black, in

00:28:42 --> 00:28:44 the dark matter story, a number

00:28:44 --> 00:28:47 of experiments carried out on on

00:28:47 --> 00:28:50 big telescopes. One of which was actually here

00:28:50 --> 00:28:53 in Australia a very historic telescope

00:28:53 --> 00:28:56 called the 50 inch at Matt Strongloe, previously

00:28:56 --> 00:28:59 known as the Great Melbourne Telescope because it's very old but

00:28:59 --> 00:29:02 it had been modernised with new equipment.

00:29:02 --> 00:29:05 And they did an experiment which was called macho.

00:29:05 --> 00:29:08 And it was designed to look

00:29:08 --> 00:29:11 for the gravitational lensing effect

00:29:11 --> 00:29:14 of large objects in

00:29:14 --> 00:29:17 the, in the universe, basically in the

00:29:17 --> 00:29:20 vicinity of our galaxy. And by large objects I mean things

00:29:20 --> 00:29:23 that aren't subatomic particles. So I mean

00:29:23 --> 00:29:25 things like orphaned planets,

00:29:26 --> 00:29:29 dead stars or black holes.

00:29:29 --> 00:29:32 MACHO was actually an acronym for Massive Compact Halo

00:29:32 --> 00:29:35 Objects. Now they didn't

00:29:35 --> 00:29:38 see as many of these

00:29:38 --> 00:29:40 gravitational lensing phenomena,

00:29:42 --> 00:29:45 in other words the space around one of these objects being bent

00:29:45 --> 00:29:48 so it magnifies an object behind it. They didn't see

00:29:48 --> 00:29:51 any in numbers that were sufficient to

00:29:51 --> 00:29:53 make machos the

00:29:54 --> 00:29:57 missing dark matter. And so

00:29:57 --> 00:30:00 that was in the 90s that

00:30:00 --> 00:30:03 really ruled out things like black holes

00:30:03 --> 00:30:06 as being the culprits for dark matter.

00:30:06 --> 00:30:09 And so that's when we were you know, our attention

00:30:09 --> 00:30:12 was shifted to the idea that dark matter is

00:30:12 --> 00:30:15 actually some species of subatomic particles, perhaps

00:30:15 --> 00:30:18 many species, but ones that don't interact in any way

00:30:18 --> 00:30:20 with normal matter. And that's where things remain today.

00:30:21 --> 00:30:24 So it's interesting to find a paper which kind

00:30:24 --> 00:30:26 of goes back to an older idea that

00:30:27 --> 00:30:29 maybe black holes actually do

00:30:29 --> 00:30:32 contribute to the dark matter. and the

00:30:32 --> 00:30:35 reason why I think this paper has been published. Is that there

00:30:35 --> 00:30:38 is a slightly new twist to it. Because

00:30:38 --> 00:30:40 these are, The

00:30:40 --> 00:30:43 postulate is that these are primordial black holes.

00:30:43 --> 00:30:46 Black holes which were created at the same

00:30:46 --> 00:30:49 time as the universe was. In other words, during

00:30:49 --> 00:30:51 or immediately after the Big Bang.

00:30:52 --> 00:30:54 so that you, you basically,

00:30:56 --> 00:30:59 find these objects potentially. We,

00:30:59 --> 00:31:02 we've never observed a primordial black hole. People just kind

00:31:02 --> 00:31:04 of guess that they are there. And we do

00:31:05 --> 00:31:08 see black holes that, that, that

00:31:08 --> 00:31:11 maybe fall within the mass range of a primordial

00:31:11 --> 00:31:14 black hole. But, we don't actually know

00:31:14 --> 00:31:16 that they exist. But,

00:31:17 --> 00:31:19 to come to the point, I'm not being very clear here.

00:31:20 --> 00:31:23 What has actually led, to this research

00:31:23 --> 00:31:26 is that the lifetime of a black hole

00:31:26 --> 00:31:29 is possibly much, much longer

00:31:29 --> 00:31:32 than Hawking predicted that these primordial

00:31:32 --> 00:31:35 black holes would last. He gave them because

00:31:35 --> 00:31:37 they were smaller. He gave them a relatively short

00:31:37 --> 00:31:40 lifetime. Black holes, we know, do

00:31:40 --> 00:31:43 evaporate because they release Hawking radiation. This

00:31:43 --> 00:31:45 quantum, mechanics phenomena. and,

00:31:48 --> 00:31:51 the idea, even though that is a very, very slow

00:31:51 --> 00:31:53 process. If you've got these sort of mini black holes that

00:31:53 --> 00:31:56 were formed in the, origin of the

00:31:56 --> 00:31:59 universe, our thinking was that they might all have evaporated

00:31:59 --> 00:32:02 by now. And that's where this new research

00:32:02 --> 00:32:04 comes in. Because they're proposing a new

00:32:04 --> 00:32:07 mechanism, which has got an interesting name.

00:32:07 --> 00:32:10 It is, something called.

00:32:11 --> 00:32:14 I've lost the name of it. M It's

00:32:14 --> 00:32:17 basically, yes, the memory burden effect. Work

00:32:17 --> 00:32:20 that one out. Yeah, the

00:32:20 --> 00:32:22 memory burden effect, suggests

00:32:22 --> 00:32:25 that, the information

00:32:26 --> 00:32:28 stored, if I can put it that way, in the black hole.

00:32:28 --> 00:32:31 Actually stabilises it and keeps it,

00:32:31 --> 00:32:34 from decaying. So that the. To cut to the

00:32:34 --> 00:32:37 quick, the idea is that these

00:32:37 --> 00:32:40 primordial black holes. Might last a lot longer than

00:32:40 --> 00:32:43 Hawking predicted they would. And perhaps they

00:32:43 --> 00:32:45 are, after all, the missing dark matter.

00:32:46 --> 00:32:49 Now, that still has to account for why we

00:32:49 --> 00:32:51 didn't detect them by gravitational lensing. During the

00:32:51 --> 00:32:54 Macho experiment. And similar experiments carried

00:32:54 --> 00:32:57 out elsewhere in the world. But it is an interesting

00:32:57 --> 00:32:58 possibility.

00:32:58 --> 00:32:59 Andrew Dunkley: Yes, yes.

00:33:01 --> 00:33:04 it's probably the best theory we've got, I suppose, at

00:33:04 --> 00:33:05 the moment.

00:33:06 --> 00:33:08 Professor Fred Watson: yeah. I'm not sure that it is. Oh,

00:33:08 --> 00:33:11 okay. I, think, You

00:33:11 --> 00:33:14 know, I, I Because

00:33:14 --> 00:33:17 we don't even know whether primordial black holes

00:33:17 --> 00:33:19 actually exist. we don't know that these

00:33:19 --> 00:33:22 subatomic particles exist either. but

00:33:22 --> 00:33:25 it seems to me that the bill is better

00:33:25 --> 00:33:28 fitted by what black holes might be.

00:33:28 --> 00:33:31 sorry, by what dark matter might be. by

00:33:31 --> 00:33:34 the subatomic particles rather than

00:33:34 --> 00:33:36 primordial black holes.

00:33:36 --> 00:33:39 Andrew Dunkley: Well, they won't be letting you do a peer review, will they?

00:33:39 --> 00:33:41 Professor Fred Watson: They won't. No, that's about me. I've made my mind up

00:33:41 --> 00:33:44 already, you see, but we don't know what they are. What? You know, are

00:33:44 --> 00:33:47 they neutralinos? Are they WIMPs?

00:33:47 --> 00:33:49 Weakly interacting massive particles?

00:33:50 --> 00:33:53 Sterile neutrinos? There's all kinds of things that have been

00:33:53 --> 00:33:56 proposed for these, subatomic particles, but

00:33:56 --> 00:33:57 none have yet been detected.

00:33:57 --> 00:34:00 Andrew Dunkley: Yeah, all right, interesting. I'm sure that'll

00:34:00 --> 00:34:03 spawn no questions whatsoever from our audience.

00:34:04 --> 00:34:07 Professor Fred Watson: Heidi will have to deal with them next time. Yes, he will.

00:34:07 --> 00:34:09 Andrew Dunkley: Yes, she will indeed.

00:34:10 --> 00:34:12 so if you'd like to chase that up, there's a great article,

00:34:13 --> 00:34:14 on fizz

00:34:16 --> 00:34:19 detecting the primordial black holes that could be today's

00:34:19 --> 00:34:21 dark matter. Fred Watson thinks not.

00:34:22 --> 00:34:25 But, that's what science is about, tossing these ideas

00:34:25 --> 00:34:28 around. And that brings us to the end of

00:34:28 --> 00:34:30 yet another episode of Space Nuts. Thanks, Fred Watson.

00:34:31 --> 00:34:34 Professor Fred Watson: It's a pleasure, Andrew. Always good to talk. And, I look forward to

00:34:34 --> 00:34:34 our next time.

00:34:35 --> 00:34:38 Andrew Dunkley: Indeed. And thanks, to Huw in the

00:34:38 --> 00:34:41 studio who couldn't be with us today. He found himself a

00:34:41 --> 00:34:44 primordial black hole and. And we've

00:34:44 --> 00:34:46 not seen him since him since Baron

00:34:46 --> 00:34:49 Feed Love Spaghetti. with me, Andrew

00:34:49 --> 00:34:52 Dunkley. Thanks for your company. Catch you on the next episode of

00:34:52 --> 00:34:54 Space Nuts. Bye. Bye.

00:34:55 --> 00:34:58 Voice Over Guy: You've been listening to the Space Nuts Podcast,

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