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

00:00:01 --> 00:00:04 Dunkley here. Ah, this is Space Nuts,

00:00:04 --> 00:00:07 where we talk astronomy and space science.

00:00:07 --> 00:00:10 Thanks for joining us. Coming up on this

00:00:10 --> 00:00:12 episode, lots, to talk about and really

00:00:12 --> 00:00:15 interesting stuff for a change. No, as usual.

00:00:15 --> 00:00:18 and this one, I saw and thought, gee,

00:00:18 --> 00:00:20 we got to talk about this because we're

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

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

00:00:26 --> 00:00:28 found something and it's not planet nine. In

00:00:28 --> 00:00:31 fact, it's possibly a new dwarf planet,

00:00:31 --> 00:00:33 which 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

00:01:21 --> 00:01:23 Walton at large. Hello.

00:01:23 --> 00:01:25 Professor Fred Watson: Thank you for that. Yes, I do apologise for

00:01:25 --> 00:01:27 being there before. I'm, forgetting that I

00:01:27 --> 00:01:29 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 --> 00:01:33 Andrew Dunkley: Before, that's how I used to run my radio

00:01:33 --> 00:01:35 show. I didn't care what happened if some. If

00:01:35 --> 00:01:37 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 --> 00:01:48 What rules? I mean, it's just people talking,

00:01:48 --> 00:01:50 isn't it? And playing music and enjoying

00:01:50 --> 00:01:52 themselves. I thought

00:01:53 --> 00:01:55 that's how I ran. Even when I worked for the

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

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

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

00:02:01 --> 00:02:03 eventually they saw. They saw the light and

00:02:03 --> 00:02:06 started going, hang on a minute. Listening

00:02:06 --> 00:02:08 to this bloke. We might. We might be onto

00:02:08 --> 00:02:11 something. anyway, they eventually brought in

00:02:11 --> 00:02:14 an expert to teach us how to be human beings

00:02:14 --> 00:02:14 on the radio.

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

00:02:18 --> 00:02:19 Andrew Dunkley: And when she, when she talked to me, she

00:02:19 --> 00:02:22 said, don't change a thing. Which I

00:02:22 --> 00:02:24 really. A great endorsement after being told

00:02:25 --> 00:02:26 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

00:02:32 --> 00:02:34 down in Sydney? Because you've been copping

00:02:34 --> 00:02:35 us spanking with the 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

00:02:44 --> 00:02:46 it in the measure? Yeah, that's right, four

00:02:46 --> 00:02:48 inches. that was just one night and all

00:02:48 --> 00:02:50 together we probably had something like 150

00:02:50 --> 00:02:52 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

00:02:58 --> 00:03:01 up. Our downstairs granny flat which

00:03:01 --> 00:03:03 used to flood when it rained but we had a lot

00:03:03 --> 00:03:05 of work done last year. That's was in good

00:03:05 --> 00:03:06 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 --> 00:03:22 Andrew Dunkley: It's easing off now. We had rain all day but

00:03:22 --> 00:03:23 I'm looking 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

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

00:03:29 --> 00:03:32 it's moving that way which is more

00:03:32 --> 00:03:32 due me.

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

00:03:36 --> 00:03:38 afternoon. It sort of started off quite

00:03:38 --> 00:03:39 bright this morning but it is definitely

00:03:40 --> 00:03:41 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

00:04:24 --> 00:04:26 latch perfectly, it doesn't hold tight so

00:04:26 --> 00:04:28 it's always a bit loose. So when the air

00:04:28 --> 00:04:30 conditioning comes on it usually goes thump.

00:04:31 --> 00:04:33 They said did more than thump on Saturday

00:04:33 --> 00:04:36 morning I went and I woke up,

00:04:36 --> 00:04:38 went oh, earthquake. And Judy went, you sure?

00:04:39 --> 00:04:41 Really? I said yeah, I reckon it was because

00:04:41 --> 00:04:42 nothing else happened. Didn't feel any

00:04:42 --> 00:04:43 vibration.

00:04:43 --> 00:04:45 Professor Fred Watson: Okay, that's interesting. Yeah. You didn't

00:04:45 --> 00:04:46 feel it, Just the door 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

00:04:53 --> 00:04:55 didn't feel the earthquake but yeah, sure

00:04:55 --> 00:04:57 enough next morning I thought I'd check and

00:04:57 --> 00:05:00 Geosciences Australia confirmed it. So

00:05:00 --> 00:05:03 5.3 which is 1 of the biggest ever recorded

00:05:03 --> 00:05:03 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

00:05:10 --> 00:05:12 Observatory or former Australian Astronomical

00:05:12 --> 00:05:14 Observatory on the Anglo Australian

00:05:14 --> 00:05:15 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

00:05:30 --> 00:05:30 behind.

00:05:30 --> 00:05:32 Andrew Dunkley: Yeah, that's what it feels like. Yeah.

00:05:32 --> 00:05:34 Because I was in Newcastle earthquake and I'd

00:05:34 --> 00:05:36 done an overnight shift when it hit and it

00:05:36 --> 00:05:39 was 5.5. And

00:05:39 --> 00:05:42 it felt to me like somebody just got the end

00:05:42 --> 00:05:45 of the bed and was just bouncing, bouncing it

00:05:45 --> 00:05:47 up and down and. Yeah, it was much more

00:05:47 --> 00:05:48 violent 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

00:05:53 --> 00:05:55 talking about, he also runs, a very sensitive

00:05:55 --> 00:05:58 seismograph at home because he's quite

00:05:58 --> 00:06:00 interested in seismometry. so, yes, I think

00:06:00 --> 00:06:02 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

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

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

00:06:08 --> 00:06:10 Andrew Dunkley: Yeah, he would have felt more of it in

00:06:10 --> 00:06:12 Coonabarabran than he

00:06:13 --> 00:06:15 calculation because, I looked at the clock

00:06:15 --> 00:06:17 immediately and it was 2:37.

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

00:06:21 --> 00:06:24 was an 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 --> 00:06:48 exciting. Exciting. Haven't been any

00:06:48 --> 00:06:50 aftershocks that I'm aware of. But, there's a

00:06:50 --> 00:06:52 lot of tremors out here that you don't ever

00:06:52 --> 00:06:54 feel or notice because they're just so small.

00:06:54 --> 00:06:56 But, nothing that big.

00:06:57 --> 00:06:59 We better get 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

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

00:07:07 --> 00:07:10 extremities of our solar system. This is,

00:07:11 --> 00:07:13 really 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

00:07:44 --> 00:07:46 data where you can look at images of

00:07:46 --> 00:07:48 particular bits of the sky and accurately

00:07:48 --> 00:07:51 work out the position of objects in those

00:07:51 --> 00:07:54 images. it's actually what you do, Andrew.

00:07:54 --> 00:07:56 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

00:08:04 --> 00:08:07 any, images, photographic images

00:08:07 --> 00:08:10 or electronically detected images that will

00:08:10 --> 00:08:12 show it. Because the longer you can observe

00:08:12 --> 00:08:14 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 --> 00:08:27 astrophysicists at the Institute for Advanced

00:08:27 --> 00:08:30 Study in Princeton. Very, very

00:08:30 --> 00:08:32 distinguished, institution. and what

00:08:32 --> 00:08:35 they found, is an object with the

00:08:35 --> 00:08:38 very 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

00:09:10 --> 00:09:12 words, 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

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

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

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

00:10:12 --> 00:10:14 Andrew Dunkley: They're actually saying, Fred Watson, that

00:10:14 --> 00:10:16 it's going far enough out to be

00:10:17 --> 00:10:18 entering the Oort cloud.

00:10:18 --> 00:10:20 Professor Fred Watson: That's right. Part of the inner Oort cloud,

00:10:20 --> 00:10:22 which makes it a very interesting object

00:10:22 --> 00:10:25 indeed with an orbital period,

00:10:25 --> 00:10:28 if I remember rightly, of. What is it, 25

00:10:28 --> 00:10:30 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 --> 00:10:52 distance from the sun as Pluto is. But it's

00:10:52 --> 00:10:55 furthest, as you've said. It's skimming the

00:10:55 --> 00:10:57 inner edge of the Oort Cloud, that cloud of,

00:10:57 --> 00:11:00 icy debris that we recognise as being the

00:11:00 --> 00:11:03 source of comets, comets that drifting

00:11:03 --> 00:11:06 towards the inner solar system. So a,

00:11:06 --> 00:11:08 really, remarkable,

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

00:11:11 --> 00:11:13 times, so it's got a very high certainty

00:11:14 --> 00:11:16 in its orbit. but the

00:11:16 --> 00:11:18 quirky part of this, which you've already

00:11:18 --> 00:11:21 alluded to, is that,

00:11:21 --> 00:11:24 when the team, the research team who've

00:11:24 --> 00:11:27 done this work, actually looked at the

00:11:27 --> 00:11:30 simulations of, the way the

00:11:30 --> 00:11:31 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

00:11:52 --> 00:11:55 time 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 --> 00:12:06 Professor Fred Watson: That is what they are saying, yes. That it's.

00:12:06 --> 00:12:09 This is, a quote from the media.

00:12:09 --> 00:12:12 It's one of the strongest pieces of evidence

00:12:12 --> 00:12:14 yet against the 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

00:12:22 --> 00:12:24 same kind. We haven't found them yet. but

00:12:24 --> 00:12:27 yes, the figure I was looking for earlier, it

00:12:27 --> 00:12:29 spends only 1% of its time in

00:12:29 --> 00:12:32 orbit, near enough to be able to be

00:12:32 --> 00:12:34 detected from Earth because

00:12:35 --> 00:12:37 it's such a. It's a relatively small object

00:12:37 --> 00:12:39 thought to be around 700 kilometres, which

00:12:39 --> 00:12:42 probably makes it a dwarf planet rather than

00:12:42 --> 00:12:45 a large asteroid. and, the,

00:12:45 --> 00:12:47 that's imagining that something that size

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

00:12:51 --> 00:12:53 orbital period because the rest just takes it

00:12:53 --> 00:12:56 too far away. It gives you a good idea of

00:12:56 --> 00:12:58 just how elongated its orbit is.

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

00:13:00 --> 00:13:01 timeframe.

00:13:01 --> 00:13:03 Professor Fred Watson: Well, that's right, yes. because it'll drift

00:13:03 --> 00:13:06 away and will very soon be, invisible

00:13:06 --> 00:13:07 to our planet.

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

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

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

00:13:16 --> 00:13:18 I think there's a whole bunch of stuff out

00:13:18 --> 00:13:21 there that's causing the same effect.

00:13:21 --> 00:13:24 And this sounds like one of those things.

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

00:13:27 --> 00:13:29 was a similar argument around the same time

00:13:29 --> 00:13:31 by another group of scientists, one of whom I

00:13:31 --> 00:13:34 actually spoke to in Canada a couple of years

00:13:34 --> 00:13:36 ago, who said effectively that

00:13:37 --> 00:13:39 the evidence for Planet Nine is based on.

00:13:39 --> 00:13:42 I don't know it's probably a dozen or so

00:13:42 --> 00:13:45 of these icy asteroids all of whose

00:13:45 --> 00:13:48 elongated orbits sort of line up in the same

00:13:48 --> 00:13:51 way. And the suggestion that was being

00:13:51 --> 00:13:53 made by these other scientists is that

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

00:13:56 --> 00:13:58 that it's a selection effect. We just haven't

00:13:58 --> 00:14:00 found all the other ones that aren't aligned

00:14:00 --> 00:14:02 in the same way. that would

00:14:03 --> 00:14:05 contradict the idea of Planet nine. So

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

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

00:14:11 --> 00:14:14 does seem to suggest that it does not

00:14:14 --> 00:14:17 Planet nine does not exist. And just to

00:14:18 --> 00:14:21 underline what we're saying earlier, it has

00:14:21 --> 00:14:23 actually been officially confirmed

00:14:23 --> 00:14:26 as an asteroid by the International

00:14:26 --> 00:14:29 Astronomical Union. So it will no doubt

00:14:29 --> 00:14:31 get a name because once it's confirmed by the

00:14:31 --> 00:14:34 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

00:14:49 --> 00:14:51 700 kilometres. I don't think the IAU

00:14:51 --> 00:14:54 makes a distinction when they, when they

00:14:54 --> 00:14:57 actually confirm its orbit. They don't

00:14:57 --> 00:14:58 say anything about its size

00:14:59 --> 00:15:02 because that's dependent on, but that, that

00:15:02 --> 00:15:03 depends on measurements that are a lot more

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

00:15:06 --> 00:15:08 confirmed then it becomes an official object

00:15:09 --> 00:15:10 which could be either a dwarf planet or an

00:15:10 --> 00:15:11 asteroid.

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

00:15:14 --> 00:15:16 out for a bit but yes, it's there and

00:15:16 --> 00:15:19 it 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

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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

00:18:26 --> 00:18:29 one reason. This is going to sound

00:18:29 --> 00:18:30 strange. I've 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 --> 00:18:40 heard of it. When I saw the picture I went,

00:18:40 --> 00:18:42 oh, yeah, I know I've seen that picture

00:18:42 --> 00:18:45 before. Yes, because it's

00:18:45 --> 00:18:48 unique. That's why, this moon is

00:18:48 --> 00:18:50 so very interesting. Because

00:18:50 --> 00:18:52 questions are still being asked as to how it

00:18:52 --> 00:18:55 looks the way it does. It's a strange place

00:18:55 --> 00:18:58 and it's getting, a fair bit of attention

00:18:58 --> 00:19:00 in social media at the moment,

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

00:19:04 --> 00:19:04 the news.

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

00:19:07 --> 00:19:09 as you say, I think it really is social media

00:19:09 --> 00:19:11 that stirred this up. we. So,

00:19:12 --> 00:19:14 you know, until 2017, when the

00:19:14 --> 00:19:17 spacecraft plunged into the atmosphere of

00:19:18 --> 00:19:20 Saturn, 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

00:19:29 --> 00:19:31 Saturn than we could ever have guessed that

00:19:31 --> 00:19:34 we'd learn. and I think,

00:19:34 --> 00:19:37 So Iapetus was certainly very much in the

00:19:37 --> 00:19:39 headlines then because it is such a peculiar

00:19:39 --> 00:19:42 world. but it sort of. Because

00:19:42 --> 00:19:44 so many of the questions don't really have

00:19:44 --> 00:19:46 proper answers, that's

00:19:46 --> 00:19:49 allowed it to sort of fade from, from

00:19:49 --> 00:19:52 the 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

00:20:07 --> 00:20:09 some of the planetary, scientists who've

00:20:09 --> 00:20:12 certainly had an interest in Iapetus, to go

00:20:12 --> 00:20:14 back to some of the Cassini data, maybe

00:20:14 --> 00:20:17 using, you know, more modern AI

00:20:17 --> 00:20:20 methods to analyse it and actually check out

00:20:20 --> 00:20:21 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 --> 00:20:38 discovered the Cassini Division since the

00:20:38 --> 00:20:41 name, made

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

00:20:44 --> 00:20:47 world orbiting Saturn, is

00:20:47 --> 00:20:50 peculiar because one side of it was very

00:20:50 --> 00:20:52 much darker than the other. I remember

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

00:20:55 --> 00:20:58 the, early 1970s when I was working at

00:20:58 --> 00:21:00 the Nautical Almanack Office of the Royal

00:21:00 --> 00:21:02 Greenwich Observatory with one of my

00:21:02 --> 00:21:04 colleagues there, Andy Sinclair was a

00:21:04 --> 00:21:06 specialist on Iapetus and he kept telling me

00:21:06 --> 00:21:09 it was a very peculiar world. but it was only

00:21:09 --> 00:21:12 when Cassini flew by a few decades later that

00:21:12 --> 00:21:15 we realised just how peculiar it is. So

00:21:15 --> 00:21:16 it is covered in craters,

00:21:18 --> 00:21:20 but it's got this dark side which

00:21:20 --> 00:21:23 just looks as though it's been spattered with

00:21:23 --> 00:21:26 soot. Looks as though, you know, somebody's

00:21:26 --> 00:21:28 put a pile of soot out there and Iapetus,

00:21:29 --> 00:21:31 has run into it. and you've. So

00:21:31 --> 00:21:33 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 --> 00:21:44 it's only on one side and that's the forward

00:21:44 --> 00:21:47 facing side. Iapetus goes around Saturn

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

00:21:50 --> 00:21:52 same face to Saturn. That means there's

00:21:52 --> 00:21:54 always a forward side and a backward side.

00:21:54 --> 00:21:57 This stuff's on the forward side. If I'm

00:21:57 --> 00:21:59 actually remembering from my, talks on

00:22:00 --> 00:22:02 Cassini, ah, back in the day, I haven't done

00:22:02 --> 00:22:04 one of 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 --> 00:22:32 Professor Fred Watson: It is. That's right. I used to think it

00:22:32 --> 00:22:34 looked like a walnut. Exactly that. and

00:22:34 --> 00:22:37 so, I mean, there's various

00:22:37 --> 00:22:39 theories as to how it got there. And the one

00:22:39 --> 00:22:42 that I thought was the most common

00:22:42 --> 00:22:45 one, was that,

00:22:45 --> 00:22:48 it was caused by the contraction of the crust

00:22:48 --> 00:22:49 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 --> 00:23:46 because of, the fact that they're what we

00:23:46 --> 00:23:49 call ice worlds with a, with a central rocky

00:23:49 --> 00:23:52 core, a, liquid ocean above it, which

00:23:52 --> 00:23:55 may be quite slushy. and then a crust of

00:23:55 --> 00:23:57 solid ice on top of that. That could be the

00:23:57 --> 00:23:59 construction. Once again, if you've got stuff

00:23:59 --> 00:24:01 coming up from beneath the surface and the

00:24:01 --> 00:24:04 object is spinning fast enough, then you

00:24:04 --> 00:24:07 will get, perhaps a ring of mountains

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

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

00:24:13 --> 00:24:15 which was contraction. So I'm very

00:24:15 --> 00:24:18 interested to know where the scientific,

00:24:18 --> 00:24:21 you know, the scientific, consensus

00:24:21 --> 00:24:23 is going on this little world. And, it's

00:24:23 --> 00:24:25 great that it's, it's cropped up again, it's

00:24:25 --> 00:24:27 welled up again into the public

00:24:27 --> 00:24:27 consciousness.

00:24:28 --> 00:24:30 Andrew Dunkley: It has, yeah. Another theory I read was just

00:24:30 --> 00:24:32 a 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 --> 00:24:37 than a mountain range. I would, I would

00:24:37 --> 00:24:38 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 --> 00:24:50 shape is that ah, what we call an oblate

00:24:50 --> 00:24:53 spheroid. Saturn itself actually is the

00:24:53 --> 00:24:55 most extreme example in the solar system

00:24:55 --> 00:24:58 because it's the diameter

00:24:58 --> 00:25:01 between the poles is significantly less than

00:25:01 --> 00:25:03 the diameter across the equator. and it's

00:25:03 --> 00:25:06 this kind of oval shape in cross section.

00:25:07 --> 00:25:09 so that's what you'd expect from something

00:25:10 --> 00:25:12 rotating quickly not as a

00:25:12 --> 00:25:15 well defined ridge of mountains like

00:25:15 --> 00:25:17 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

00:25:24 --> 00:25:24 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 --> 00:25:40 Andrew Dunkley: Could the dark face be some sort of reaction

00:25:40 --> 00:25:43 with 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

00:25:48 --> 00:25:51 similar is that it consists of organic

00:25:51 --> 00:25:54 chemicals that form this kind of

00:25:54 --> 00:25:56 soot. I think solens might have

00:25:56 --> 00:25:59 been in invoked as well. These are

00:25:59 --> 00:26:02 particular organic chemicals that we

00:26:02 --> 00:26:04 know coat a lot of the outer worlds because

00:26:05 --> 00:26:07 they're generated by I think the impact of

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

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

00:26:13 --> 00:26:15 it's ah, only on one side. It looks as though

00:26:15 --> 00:26:17 it's just kind of run into something that's

00:26:17 --> 00:26:19 splattered all over the front of it.

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

00:26:21 --> 00:26:21 spilled the paint.

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

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

00:26:26 --> 00:26:29 look at it. Yapetis is all over the Internet,

00:26:29 --> 00:26:31 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

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

00:27:07 --> 00:27:10 holes in our next episode as

00:27:10 --> 00:27:12 a matter of fact. But and, and I think the

00:27:12 --> 00:27:15 reason is quite simple. People just want to

00:27:15 --> 00:27:18 understand Them and there's so much we don't

00:27:18 --> 00:27:18 know.

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

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

00:27:26 --> 00:27:29 that 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 --> 00:27:57 sort of almost with new eyes if I can put it

00:27:57 --> 00:28:00 that way, at the dark matter problem because

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

00:28:04 --> 00:28:06 stuff that seems to have a gravitational hold

00:28:06 --> 00:28:08 on galaxies so that they don't fly ap.

00:28:09 --> 00:28:12 and a ah, gravitational hold on galaxy

00:28:12 --> 00:28:15 clusters so they don't fly apart as well. and

00:28:15 --> 00:28:17 yet we can't detect it. We cannot detect it

00:28:17 --> 00:28:20 in any way other than by its gravitational

00:28:20 --> 00:28:21 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 --> 00:28:49 big telescopes. One of which was actually

00:28:49 --> 00:28:52 here in Australia a very historic

00:28:52 --> 00:28:55 telescope called the 50 inch at Matt

00:28:55 --> 00:28:57 Strongloe, previously known as the Great

00:28:57 --> 00:28:59 Melbourne Telescope because it's very old but

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

00:29:02 --> 00:29:04 And they did an experiment which was called

00:29:04 --> 00:29:06 macho. And it was

00:29:07 --> 00:29:10 designed to look for the gravitational

00:29:10 --> 00:29:13 lensing effect of large objects

00:29:13 --> 00:29:16 in the, in the

00:29:16 --> 00:29:18 universe, basically in the vicinity of our

00:29:18 --> 00:29:20 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 --> 00:29:31 MACHO was actually an acronym for Massive

00:29:31 --> 00:29:34 Compact Halo Objects. Now they

00:29:34 --> 00:29:37 didn't see as many

00:29:37 --> 00:29:40 of these gravitational lensing

00:29:40 --> 00:29:40 phenomena,

00:29:42 --> 00:29:44 in other words the space around one of these

00:29:44 --> 00:29:47 objects being bent so it magnifies an object

00:29:47 --> 00:29:49 behind it. They didn't see any in

00:29:49 --> 00:29:52 numbers that were sufficient to make

00:29:52 --> 00:29:55 machos the missing

00:29:55 --> 00:29:58 dark matter. And so that was in

00:29:58 --> 00:30:01 the 90s that really ruled

00:30:01 --> 00:30:03 out things like black holes as being

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

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

00:30:09 --> 00:30:11 attention was shifted to the idea that dark

00:30:11 --> 00:30:14 matter is actually some species of subatomic

00:30:14 --> 00:30:16 particles, perhaps many species, but ones

00:30:16 --> 00:30:18 that don't interact in any way with normal

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

00:30:21 --> 00:30:23 So it's interesting to find a paper which

00:30:23 --> 00:30:26 kind 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 --> 00:30:34 reason why I think this paper has been

00:30:34 --> 00:30:36 published. Is that there is a slightly new

00:30:36 --> 00:30:39 twist to it. Because these are,

00:30:40 --> 00:30:42 The postulate is that these are primordial

00:30:42 --> 00:30:45 black holes. Black holes which were created

00:30:45 --> 00:30:47 at the same time as the universe was. In

00:30:47 --> 00:30:50 other words, during or immediately after the

00:30:50 --> 00:30:53 Big Bang. so that

00:30:53 --> 00:30:54 you, you basically,

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

00:30:59 --> 00:31:01 we've never observed a primordial black hole.

00:31:01 --> 00:31:03 People just kind of guess that they are

00:31:03 --> 00:31:06 there. And we do see black

00:31:06 --> 00:31:08 holes that, that, that

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

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

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

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

00:31:19 --> 00:31:21 clear here. What has actually

00:31:22 --> 00:31:25 led, to this research is that the lifetime of

00:31:25 --> 00:31:28 a black hole is possibly much,

00:31:28 --> 00:31:31 much longer than Hawking predicted

00:31:31 --> 00:31:33 that these primordial black holes would last.

00:31:33 --> 00:31:36 He gave them because they were smaller. He

00:31:36 --> 00:31:39 gave them a relatively short lifetime. Black

00:31:39 --> 00:31:41 holes, we know, do evaporate because they

00:31:41 --> 00:31:43 release Hawking radiation. This quantum,

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

00:31:48 --> 00:31:50 the idea, even though that is a very, very

00:31:50 --> 00:31:52 slow process. If you've got these sort of

00:31:52 --> 00:31:55 mini black holes that were formed in the,

00:31:55 --> 00:31:58 origin of the universe, our thinking was that

00:31:58 --> 00:32:00 they might all have evaporated by now. And

00:32:00 --> 00:32:02 that's where this new research comes in.

00:32:02 --> 00:32:05 Because they're proposing a new mechanism,

00:32:05 --> 00:32:08 which has got an interesting name. It is,

00:32:09 --> 00:32:12 something called. I've lost

00:32:12 --> 00:32:14 the name of it. M It's basically,

00:32:15 --> 00:32:17 yes, the memory burden effect. Work that one

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

00:32:20 --> 00:32:23 burden effect, suggests that,

00:32:24 --> 00:32:27 the information stored, if I can put it that

00:32:27 --> 00:32:30 way, in the black hole. Actually stabilises

00:32:30 --> 00:32:33 it and keeps it, from decaying. So

00:32:33 --> 00:32:35 that the. To cut to the quick, the

00:32:36 --> 00:32:38 idea is that these primordial black holes.

00:32:38 --> 00:32:40 Might last a lot longer than Hawking

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

00:32:43 --> 00:32:45 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.

00:32:51 --> 00:32:53 During the Macho experiment. And similar

00:32:53 --> 00:32:55 experiments carried out elsewhere in the

00:32:55 --> 00:32:58 world. But it is an interesting possibility.

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

00:33:01 --> 00:33:03 it's probably the best theory we've got, I

00:33:03 --> 00:33:05 suppose, at 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 --> 00:33:16 we don't even know whether primordial black

00:33:16 --> 00:33:19 holes actually exist. we don't know that

00:33:19 --> 00:33:22 these 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 --> 00:33:38 Andrew Dunkley: Well, they won't be letting you do a peer

00:33:38 --> 00:33:39 review, will they?

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

00:33:41 --> 00:33:43 mind up already, you see, but we don't know

00:33:43 --> 00:33:45 what they are. What? You know, are they

00:33:45 --> 00:33:47 neutralinos? Are they WIMPs?

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

00:33:50 --> 00:33:52 Sterile neutrinos? There's all kinds of

00:33:52 --> 00:33:54 things that have been proposed for these,

00:33:54 --> 00:33:57 subatomic particles, but none have yet been

00:33:57 --> 00:33:57 detected.

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

00:34:00 --> 00:34:02 that'll spawn no questions whatsoever from

00:34:02 --> 00:34:03 our audience.

00:34:04 --> 00:34:06 Professor Fred Watson: Heidi will have to deal with them next time.

00:34:06 --> 00:34:07 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

00:34:12 --> 00:34:14 great article, on fizz

00:34:16 --> 00:34:18 detecting the primordial black holes that

00:34:18 --> 00:34:20 could be today's dark matter. Fred Watson

00:34:20 --> 00:34:23 thinks not. But, that's what science

00:34:23 --> 00:34:26 is about, tossing these ideas around. And

00:34:26 --> 00:34:28 that brings us to the end of yet another

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

00:34:31 --> 00:34:33 Professor Fred Watson: It's a pleasure, Andrew. Always good to talk.

00:34:33 --> 00:34:34 And, I look forward to our next time.

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

00:34:38 --> 00:34:40 studio who couldn't be with us today. He

00:34:40 --> 00:34:42 found himself a primordial black hole and.

00:34:42 --> 00:34:45 And we've not seen him since him since

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

00:34:49 --> 00:34:50 Andrew Dunkley. Thanks for your company.

00:34:51 --> 00:34:53 Catch you on the next episode of Space Nuts.

00:34:53 --> 00:34:54 Bye. Bye.

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