Sunlight Satellites, Near-Earth Asteroids & the 6,000th Exoplanet Revelation
Space Nuts: Exploring the CosmosOctober 17, 2025
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00:53:1748.84 MB

Sunlight Satellites, Near-Earth Asteroids & the 6,000th Exoplanet Revelation

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ontroversial Concepts: Sunlight Services, Near-Earth Asteroids, and the 6,000th Exoplanet
In this captivating episode of Space Nuts, hosts Andrew Dunkley and Professor Jonti Horner dive into a variety of cosmic topics that challenge our understanding of space and its implications for life on Earth. From a bold proposal for a satellite-based sunlight service to a near miss with an asteroid and the discovery of the 6,000th exoplanet, this episode is filled with intriguing discussions and scientific insights.
Episode Highlights:
Sunlight Services Proposal: Andrew and Jonti explore the controversial idea of launching satellites to reflect sunlight back to Earth, discussing the practical challenges and potential environmental impacts of such a scheme. They raise critical questions about the feasibility and safety of this ambitious project.
Asteroid Near Miss: The hosts analyze the recent close encounter with asteroid 2025 TF, emphasizing the importance of early detection in planetary defense and how light pollution from artificial satellites could hinder our ability to spot these potential threats in the future.
Milestone in Exoplanet Discovery: Celebrating the discovery of the 6,000th exoplanet, Andrew and Jonti reflect on the journey of exoplanet research over the past three decades and the implications of finding planets beyond our solar system. They discuss the criteria for confirming these distant worlds and what the future holds for exoplanet exploration.
Mimas and Subsurface Oceans: The episode concludes with a fascinating look at Saturn's moon Mimas, which may harbor a subsurface ocean. The discussion highlights the ongoing research into the moon's geological history and the potential for life beyond Earth in unexpected places.
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Stay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.

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00:00:00 --> 00:00:02 Andrew Dunkley: Hi there. Thanks for joining us on another

00:00:02 --> 00:00:04 edition of Space Nuts, where we talk

00:00:04 --> 00:00:06 astronomy and space science. My name is

00:00:06 --> 00:00:08 Andrew Dunkley, your host. It's good to have

00:00:08 --> 00:00:10 your company as always. Today,

00:00:11 --> 00:00:12 we're going to start off with something quite

00:00:12 --> 00:00:15 controversial. And in some

00:00:15 --> 00:00:17 parts of the world they probably call this

00:00:17 --> 00:00:20 dumb. But, a proposal to create

00:00:20 --> 00:00:23 a sunlight service. Yes. Using

00:00:23 --> 00:00:25 mirrors in orbit. It's a thing.

00:00:25 --> 00:00:28 also a near miss for Earth involving asteroid

00:00:28 --> 00:00:30 20, 2025 TF, the

00:00:30 --> 00:00:33 6th exoplanet has

00:00:33 --> 00:00:36 been discovered. And another potential

00:00:36 --> 00:00:38 subsurface ocean, this one

00:00:38 --> 00:00:41 involving the moon Mimas. That's all coming

00:00:41 --> 00:00:43 up on this edition of Space Nuts.

00:00:43 --> 00:00:46 Jonti Horner: 15 seconds. Guidance is internal.

00:00:46 --> 00:00:49 10, 9. Ignition

00:00:49 --> 00:00:51 sequence. Star. Space Nuts. 5, 4,

00:00:51 --> 00:00:54 3. 2. 1. 2, 3, 4, 5, 5, 4,

00:00:54 --> 00:00:57 3, 2, 1. Space Nuts astronauts,

00:00:57 --> 00:00:58 report.

00:00:58 --> 00:00:58 Andrew Dunkley: It feels good.

00:00:59 --> 00:01:02 And joining us, in the stead of Fred

00:01:02 --> 00:01:05 Watson, we are, joined by Jonti Horner,

00:01:05 --> 00:01:06 professor of astrophysics at the University

00:01:06 --> 00:01:08 of Southern Queensland. Hello again, Jonti.

00:01:09 --> 00:01:11 Jonti Horner: good morning. How are you going?

00:01:11 --> 00:01:13 Andrew Dunkley: I am well. And we should, just put a

00:01:13 --> 00:01:16 caveat to this episode. There might be noise

00:01:16 --> 00:01:17 because you're getting work done at the

00:01:17 --> 00:01:17 house.

00:01:18 --> 00:01:20 Jonti Horner: Yes. And of course we organized to record at

00:01:20 --> 00:01:22 this time prior to the trade is getting in

00:01:22 --> 00:01:23 touch and saying, you know what, we'll be

00:01:23 --> 00:01:25 there at 7am on Monday morning. It's like

00:01:25 --> 00:01:28 great, you know, want this done. Hopefully

00:01:28 --> 00:01:31 the wonders of the microphone will filter it

00:01:31 --> 00:01:33 all out. But given that some of the banging I

00:01:33 --> 00:01:35 can feel through my feet, I suspect the

00:01:35 --> 00:01:36 vibrations might go all the way through the

00:01:36 --> 00:01:38 desk and all the way up the microphone and

00:01:38 --> 00:01:40 we'll occasionally get bang, bang, bang,

00:01:40 --> 00:01:41 drill, drill, drill. So, yeah, I know.

00:01:42 --> 00:01:44 Consider it like we've got a craft work gig

00:01:44 --> 00:01:45 going on or something like that.

00:01:45 --> 00:01:47 Andrew Dunkley: Well, I can tell you we've, we've heard worse

00:01:47 --> 00:01:50 from Fred's house. So, yeah, it should, it

00:01:50 --> 00:01:52 shouldn't sound out of the ordinary, to be

00:01:52 --> 00:01:52 honest.

00:01:53 --> 00:01:55 All right, let's get, stuck into these

00:01:55 --> 00:01:57 stories because we've got a lot to talk

00:01:57 --> 00:02:00 about. This first one, I know you sent me

00:02:00 --> 00:02:02 the, information initially that came from, I

00:02:02 --> 00:02:05 believe, one of your students who's overseas.

00:02:05 --> 00:02:08 But this is, an idea of a Californian company

00:02:08 --> 00:02:10 who is applying to the federal,

00:02:11 --> 00:02:12 communications commission in the United

00:02:12 --> 00:02:15 States, the fcc, for permission to launch a

00:02:15 --> 00:02:17 satellite into space to reflect

00:02:18 --> 00:02:20 sunlight back down on Earth and

00:02:20 --> 00:02:22 charge people for the privilege.

00:02:24 --> 00:02:27 Jonti Horner: Yeah. Now I try very hard to be

00:02:27 --> 00:02:30 even handed and to not be too critical even

00:02:30 --> 00:02:32 when I'm talking About the people who shall

00:02:32 --> 00:02:33 not be named. You know, the ones who are

00:02:33 --> 00:02:36 putting up, Starlink satellites and abusing

00:02:36 --> 00:02:39 colleagues of mine, or people who are

00:02:39 --> 00:02:41 claiming that things that are not aliens are

00:02:41 --> 00:02:43 aliens in order to sell books. You know, I

00:02:43 --> 00:02:45 try and be even handed and it's very

00:02:45 --> 00:02:48 hard to talk about this one without getting a

00:02:48 --> 00:02:50 bit caustic. it reminds me

00:02:50 --> 00:02:53 of the late, great Terry Pratchett, who,

00:02:53 --> 00:02:55 in one of the books was talking about a

00:02:55 --> 00:02:58 certain subset of the landed gentry.

00:02:58 --> 00:03:00 You know, there's, political things going on

00:03:00 --> 00:03:02 and this is a time when the city's under

00:03:02 --> 00:03:05 siege and they're reforming the regiments and

00:03:05 --> 00:03:08 things like this. And it's talking about the

00:03:08 --> 00:03:09 boys who were dropped on their heads as

00:03:09 --> 00:03:12 babies, as this kind of subset of,

00:03:12 --> 00:03:15 you know, nice but dim gentry. Yeah, they're

00:03:15 --> 00:03:18 nice, but they're not all there. And this,

00:03:18 --> 00:03:20 to me, seems like an idea that was dropped on

00:03:20 --> 00:03:23 its head as a baby. It's so

00:03:23 --> 00:03:26 overwhelmingly dumb that you think it must be

00:03:26 --> 00:03:29 April 1st and it isn't. So the idea

00:03:29 --> 00:03:31 that this company called Reflector Orbital

00:03:31 --> 00:03:34 have. And it's an idea that has

00:03:34 --> 00:03:36 led to them getting tens of millions of

00:03:36 --> 00:03:38 dollars of funding. So it's not like,

00:03:39 --> 00:03:41 yeah, this is. It's

00:03:41 --> 00:03:43 not like these are people in the pub saying,

00:03:43 --> 00:03:45 we've had a few. You know what'd be funny?

00:03:45 --> 00:03:48 This is a company taking it seriously.

00:03:48 --> 00:03:50 They're getting interns in, they've got a

00:03:50 --> 00:03:52 very active social media presence and their

00:03:52 --> 00:03:55 whole business is. Isn't it sad that it's

00:03:55 --> 00:03:57 dark at nighttime? Wouldn't it be great if

00:03:57 --> 00:03:59 you could pay somebody and get sunshine

00:03:59 --> 00:04:02 delivered to you at night? And that could

00:04:02 --> 00:04:03 power your solar panels or it could help you

00:04:03 --> 00:04:06 grow your crops or, you know, help you

00:04:06 --> 00:04:08 illuminate your sporting event or your

00:04:08 --> 00:04:10 concert. And the idea that

00:04:10 --> 00:04:12 they've got is that they will launch

00:04:12 --> 00:04:14 satellites into low Earth orbit, maybe 400

00:04:14 --> 00:04:17 kilometers up, that will go around the Earth

00:04:17 --> 00:04:18 every 90 minutes. So they're going to be

00:04:18 --> 00:04:21 fleetingly above any given location, above

00:04:21 --> 00:04:23 the horizon for a few minutes. And if you

00:04:23 --> 00:04:26 send them a few of your dollary dues, they

00:04:26 --> 00:04:28 will make their satellite reflect light down

00:04:28 --> 00:04:31 to your location and deliver

00:04:31 --> 00:04:34 sunlight to you. Now, there's all sorts of

00:04:34 --> 00:04:35 problems with this. Firstly, you know, I

00:04:35 --> 00:04:38 live, in Toowoomba. I'm 27 degrees south and

00:04:38 --> 00:04:41 I can see satellites that are about 400 km up

00:04:41 --> 00:04:43 in about the first hour after sunset, the

00:04:43 --> 00:04:46 first hour before sunrise, the rest of the

00:04:46 --> 00:04:48 night, those satellites are in shadow too. So

00:04:48 --> 00:04:51 there isn't any sun to reflect. Oh.

00:04:51 --> 00:04:52 Andrew Dunkley: So, you know, fair point.

00:04:53 --> 00:04:55 Jonti Horner: Nobody seems to be really mentioning that in

00:04:55 --> 00:04:57 the narrative of how this will work. But even

00:04:57 --> 00:04:58 ignoring that, think about the International

00:04:59 --> 00:05:00 Space Station going overhead. And you can get

00:05:00 --> 00:05:02 predictions of this from wonderful websites

00:05:02 --> 00:05:05 like heavensabove.com and the space

00:05:05 --> 00:05:07 station becomes visible,

00:05:08 --> 00:05:10 passes over, and then goes into the shadow.

00:05:10 --> 00:05:12 And you might get five, six minutes of it

00:05:12 --> 00:05:15 going overhead, if you're lucky. Yeah. And

00:05:15 --> 00:05:18 then it's gone. So you have this idea that

00:05:18 --> 00:05:20 these mirrors, that they're going to launch

00:05:20 --> 00:05:22 at about that altitude, and

00:05:23 --> 00:05:25 if you want them to illuminate a single point

00:05:25 --> 00:05:26 on the ground, they've got to be turning. So

00:05:26 --> 00:05:29 they keep rotating the light to that point as

00:05:29 --> 00:05:31 they pass overhead. Mm. When they're

00:05:31 --> 00:05:33 passed overhead, what do they do? They can't

00:05:33 --> 00:05:36 just turn off the mirror. So is that

00:05:36 --> 00:05:39 suggesting that you're gonna have a beam of

00:05:39 --> 00:05:41 light sweeping across the countryside at

00:05:41 --> 00:05:44 orbital speed? Like when you're trying

00:05:44 --> 00:05:45 to entertain a cat and you're shining a laser

00:05:45 --> 00:05:47 pointer on the floor and the cat's chasing

00:05:47 --> 00:05:48 it, you've got a beam going across the Earth.

00:05:48 --> 00:05:51 yeah. Going across the skies of all these

00:05:51 --> 00:05:54 people who didn't pay for the service. Not

00:05:54 --> 00:05:56 just that, how do you get enough sunlight

00:05:56 --> 00:05:58 down to be functional? So

00:05:58 --> 00:06:00 these satellites are going to be small enough

00:06:00 --> 00:06:03 to launch. So you're talking about a mirror a

00:06:03 --> 00:06:06 few meters across, 400 kilometers away,

00:06:06 --> 00:06:08 trying to reflect sunlight down, and they,

00:06:08 --> 00:06:11 they talk about how the diameter of the

00:06:11 --> 00:06:13 beam will be about 5km across.

00:06:14 --> 00:06:17 So that means if I pay for them to deliver

00:06:17 --> 00:06:19 light to my backyard, anybody in a five

00:06:19 --> 00:06:22 kilometer diameter area around me also get

00:06:22 --> 00:06:24 illuminated as well, for free, whether they

00:06:24 --> 00:06:24 want to or not.

00:06:25 --> 00:06:26 Andrew Dunkley: Yeah, but not just that.

00:06:26 --> 00:06:27 Jonti Horner: The light's not going to be that bright,

00:06:27 --> 00:06:30 because if you've got a 1 meter sized mirror

00:06:30 --> 00:06:32 reflecting sunlight, and then you spread that

00:06:32 --> 00:06:35 light over an area that is 5km in diameter,

00:06:35 --> 00:06:37 you're spreading that light awfully thin. So

00:06:37 --> 00:06:40 any area on the ground there is not going to

00:06:40 --> 00:06:43 see broad daylight. They're going to see

00:06:43 --> 00:06:45 something that is comparable in brightness or

00:06:45 --> 00:06:46 a few times brighter than the full moon,

00:06:47 --> 00:06:50 which is. Okay, that's enough light for you

00:06:50 --> 00:06:52 to go out and do something in the backyard

00:06:52 --> 00:06:54 by. But it's not particularly enough light to

00:06:54 --> 00:06:56 get really effective solar power from. So if

00:06:56 --> 00:06:58 you want to make this effective, you're going

00:06:58 --> 00:07:01 to have to launch hundreds of thousands

00:07:01 --> 00:07:04 of these mirrors, all to work in

00:07:04 --> 00:07:06 concert to beam towards a given location,

00:07:07 --> 00:07:09 which doesn't sound that feasible. Add to

00:07:09 --> 00:07:11 that the fact that these are Big floating

00:07:11 --> 00:07:14 targets in space that space debris can hit

00:07:14 --> 00:07:17 and smash, which means that a, you could

00:07:17 --> 00:07:18 get all this debris scattered off in all

00:07:18 --> 00:07:21 sorts of different directions, but also that

00:07:21 --> 00:07:23 it's going to be hard for them to control the

00:07:23 --> 00:07:25 direction the mirror's pointing. So you've

00:07:25 --> 00:07:27 got all sorts of problems here. I mean, I

00:07:27 --> 00:07:29 think there's growing and

00:07:29 --> 00:07:32 demonstrated evidence, and Fred's talked

00:07:32 --> 00:07:34 about this to death, about all the negative

00:07:34 --> 00:07:36 effects artificial light at night has. We've

00:07:36 --> 00:07:38 got effects on people. You've got increased

00:07:38 --> 00:07:41 cancer rates, a very bizarre but

00:07:41 --> 00:07:44 very significant link between light at night

00:07:44 --> 00:07:45 and an increased risk of breast cancer for

00:07:45 --> 00:07:48 women. Believe it or not, just as one

00:07:48 --> 00:07:50 example, you've got the impact in our

00:07:50 --> 00:07:52 circadian rhythms, the fact that we need it

00:07:52 --> 00:07:55 to be dark to sleep, then you've got all the

00:07:55 --> 00:07:57 impact on flora and fauna. Now, I've visited

00:07:57 --> 00:07:59 some wonderful places on the coast of

00:07:59 --> 00:08:02 Queensland to do outreach sessions, you know,

00:08:02 --> 00:08:04 some kind of night sky observing. And a lot

00:08:04 --> 00:08:06 of these places are places where turtles

00:08:06 --> 00:08:09 nest. In fact, I'm going next weekend to the

00:08:09 --> 00:08:11 wonderful Lady Elliot island on the reef to

00:08:11 --> 00:08:13 do some outreach. And I go there several

00:08:13 --> 00:08:15 times a year. And all of their resort is

00:08:15 --> 00:08:18 designed to keep light down and pointed at

00:08:18 --> 00:08:19 the ground and have lights that get turned

00:08:19 --> 00:08:22 off because baby turtles, when they hatch,

00:08:23 --> 00:08:25 they navigate to the ocean by looking at the

00:08:25 --> 00:08:27 very faint light on the horizon, light

00:08:27 --> 00:08:29 reflecting off the ocean. And, that's what

00:08:29 --> 00:08:31 sets their internal compass as they start

00:08:31 --> 00:08:34 their lives. And if you have stray light,

00:08:34 --> 00:08:36 they go the wrong way and they end up under

00:08:36 --> 00:08:38 the buildings and on the road and things like

00:08:38 --> 00:08:41 this. Yeah, so there's huge impacts on life.

00:08:41 --> 00:08:44 But I think the biggest concern about this is

00:08:44 --> 00:08:46 the safety aspect. You know, you're driving

00:08:46 --> 00:08:48 around and I know here in regional Australia,

00:08:48 --> 00:08:50 most of our roads don't have street lights

00:08:50 --> 00:08:52 and that's perfectly fine. It's safer. As

00:08:52 --> 00:08:54 such, you drive along with your full beam on

00:08:54 --> 00:08:56 and any kangaroo that you see, you've got

00:08:56 --> 00:08:58 room to do something about it. So you're

00:08:58 --> 00:09:00 driving along on this pitch black road and,

00:09:00 --> 00:09:02 suddenly from nowhere, something brighter

00:09:02 --> 00:09:04 than the full moon shines full head on in

00:09:04 --> 00:09:06 your view. You're dazzled. That's

00:09:06 --> 00:09:09 hugely dangerous. Odd enough, if you're

00:09:09 --> 00:09:10 driving on the ground, if you're a pilot

00:09:10 --> 00:09:13 coming in to land, and suddenly somebody's

00:09:13 --> 00:09:15 trying to spotlight in your face, that's not

00:09:15 --> 00:09:18 going to be a particularly pleasant outcome

00:09:18 --> 00:09:21 for you and the passengers in your plane. And

00:09:21 --> 00:09:23 so there's all these issues there that

00:09:24 --> 00:09:26 any one of them will be enough for you to

00:09:26 --> 00:09:29 say, this is a really foolish idea. It

00:09:29 --> 00:09:31 is not something that is likely to work

00:09:31 --> 00:09:33 anyway, but it's a really foolish

00:09:33 --> 00:09:35 idea from the ground up. It's only going to

00:09:35 --> 00:09:37 work near twilight. You're going to have to

00:09:37 --> 00:09:39 launch thousands of satellites to make it

00:09:39 --> 00:09:42 work, but it isn't stopping people funding

00:09:42 --> 00:09:44 them. And, this company, like I say, has

00:09:44 --> 00:09:47 applied to the FCC in the US for

00:09:47 --> 00:09:48 permission to launch the first of these

00:09:48 --> 00:09:50 satellites, which they've named Earundel 1

00:09:50 --> 00:09:52 after the light from Lord of the Rings.

00:09:53 --> 00:09:56 Earundel 1. They're hoping to launch April,

00:09:56 --> 00:09:59 May time next year, 2026, to

00:09:59 --> 00:10:02 demonstrate that their wonderful great idea

00:10:02 --> 00:10:05 can work. And it's just yet another example

00:10:05 --> 00:10:07 of this kind of Wild west scenario we've got

00:10:07 --> 00:10:09 with the use of space around the Earth, where

00:10:09 --> 00:10:12 the use of space is really outstripping our

00:10:12 --> 00:10:14 ability to regulate and control that use.

00:10:14 --> 00:10:16 And, people are doing things because it

00:10:16 --> 00:10:17 seemed like a good idea at the time without

00:10:17 --> 00:10:20 any real thought about the practicality of

00:10:20 --> 00:10:22 it, whether it could work. And, normally you

00:10:22 --> 00:10:24 just think like, say you think this is an

00:10:24 --> 00:10:27 April Fool's Day kind of prank. But the

00:10:27 --> 00:10:29 fact that this company has raised tens of

00:10:29 --> 00:10:31 millions of dollars in kind of venture

00:10:31 --> 00:10:32 capital, it's supported by A M

00:10:32 --> 00:10:35 multibillionaire, is really, really

00:10:35 --> 00:10:37 concerning. And that's why a group of

00:10:37 --> 00:10:39 astronomers, including Jessica Heim, who's

00:10:39 --> 00:10:42 doing a PhD with me at UNISQ, have put

00:10:42 --> 00:10:45 out this fact sheet with lots of information,

00:10:45 --> 00:10:47 loads of links, number of astronomers in the

00:10:47 --> 00:10:49 US who people in the media can contact for

00:10:49 --> 00:10:52 more information and suggestions about what

00:10:52 --> 00:10:55 people can do to flag up how catastrophically

00:10:55 --> 00:10:57 dumb this is. And that includes submit

00:10:57 --> 00:10:59 comments on the application to the Federal

00:10:59 --> 00:11:02 Communications Commission in the US to demand

00:11:02 --> 00:11:04 an environmental review of reflected light

00:11:04 --> 00:11:06 from orbit. Contact government

00:11:06 --> 00:11:08 representatives, particularly in the US but

00:11:08 --> 00:11:10 also locally where you live, to try and raise

00:11:10 --> 00:11:13 noise about this, but also tell people about

00:11:13 --> 00:11:15 it and point out how dumb it is. Because I

00:11:15 --> 00:11:17 can understand that if you don't really think

00:11:17 --> 00:11:20 about this too much, you can think, yeah,

00:11:20 --> 00:11:21 there are times it'd be really nice to have a

00:11:21 --> 00:11:23 bit of extra light at night.

00:11:23 --> 00:11:24 I didn't get round to doing the gardening.

00:11:24 --> 00:11:26 It'd be good to mow the lawn tonight.

00:11:26 --> 00:11:27 Wouldn't it be great if I could just turn on

00:11:27 --> 00:11:29 the spotlight and have half an hour of my

00:11:29 --> 00:11:32 backyard being daily, at night for me to do

00:11:32 --> 00:11:35 that job? And you need to talk about it and

00:11:35 --> 00:11:37 you need to think about it to see why this is

00:11:37 --> 00:11:40 just so catastrophically dumb. In

00:11:40 --> 00:11:43 so, so many ways that you would have thought

00:11:43 --> 00:11:46 it'd be an unstarter, but yet they're getting

00:11:46 --> 00:11:46 money.

00:11:47 --> 00:11:49 Andrew Dunkley: I can't see or understand

00:11:50 --> 00:11:53 any logic in this. And,

00:11:54 --> 00:11:56 the way in low Earth orbit, as you said,

00:11:56 --> 00:11:58 there's only going to be a few minutes of

00:11:58 --> 00:12:00 light. It's not like they can light a stadium

00:12:00 --> 00:12:03 for four hours straight. Not yet, any. But,

00:12:03 --> 00:12:05 even if they could, that's going to take a

00:12:05 --> 00:12:07 lot of hardware up in space. And there's more

00:12:07 --> 00:12:09 light pollution on Earth.

00:12:09 --> 00:12:10 Jonti Horner: Which is a big problem.

00:12:10 --> 00:12:12 Andrew Dunkley: Fred and Marnie are so heavily involved in

00:12:12 --> 00:12:15 the Dark Skies project. This would just blow

00:12:15 --> 00:12:16 that out of the water.

00:12:16 --> 00:12:18 Jonti Horner: Well, it would. And I mean, to light that

00:12:18 --> 00:12:20 stadium for four hours, you would need

00:12:20 --> 00:12:23 mirrors going overhead continuously in a

00:12:23 --> 00:12:26 parade. You'd need that stadium to be near

00:12:26 --> 00:12:28 enough to the pole on it to be summertime

00:12:28 --> 00:12:31 that those satellites were always in sunlight

00:12:31 --> 00:12:33 or you'd need to put them further from the

00:12:33 --> 00:12:35 Earth. The further you move them from the

00:12:35 --> 00:12:37 Earth, the more spread out the light will be,

00:12:37 --> 00:12:39 and so therefore the more satellites you'll

00:12:39 --> 00:12:42 need, you know. And if you get

00:12:42 --> 00:12:44 to that stage, if you've got that many

00:12:44 --> 00:12:46 satellites in orbit around the Earth, you may

00:12:46 --> 00:12:48 as well build a mirror that

00:12:48 --> 00:12:51 is held in geostationary orbit that covers

00:12:51 --> 00:12:54 half of the size of the Earth, and bears the

00:12:54 --> 00:12:55 entirety of that side of the Earth in

00:12:55 --> 00:12:58 sunlight. And, you know, while you're at it,

00:12:58 --> 00:12:59 you're increasing the amount of heat coming

00:12:59 --> 00:13:00 to the Earth and we'll just speed up global

00:13:00 --> 00:13:01 warming and kill everybody.

00:13:03 --> 00:13:05 Andrew Dunkley: Yeah, there is a groundswell of discontent,

00:13:05 --> 00:13:08 as you mentioned. So people are starting to

00:13:08 --> 00:13:10 make some noise about this. I hope the fcc,

00:13:13 --> 00:13:15 you know, looks at both sides of the story.

00:13:15 --> 00:13:18 how, just quickly, how likely are they

00:13:18 --> 00:13:21 to get their license and start testing

00:13:21 --> 00:13:21 this?

00:13:22 --> 00:13:24 Jonti Horner: I mean, a pessimist would say it's almost

00:13:24 --> 00:13:26 certain to happen because, you know, the FCC

00:13:26 --> 00:13:28 are quite happy for sailing to be putting up

00:13:28 --> 00:13:30 the number of satellites. They are looking at

00:13:30 --> 00:13:33 42 long term. So it

00:13:33 --> 00:13:35 doesn't seem like there's much thought of

00:13:35 --> 00:13:37 that. And there's the added concern. I think

00:13:37 --> 00:13:39 one of the things that is hindering

00:13:39 --> 00:13:41 legislation is the fact that you can launch

00:13:41 --> 00:13:44 the space from many, many countries. And so

00:13:44 --> 00:13:46 companies can quite rightly say to, a given

00:13:46 --> 00:13:48 legislating body, if you don't give us this,

00:13:48 --> 00:13:50 we'll just take our business elsewhere and

00:13:50 --> 00:13:53 someone else will. And, you know, once you're

00:13:53 --> 00:13:55 launched from a given country, you're above

00:13:56 --> 00:13:58 all of the countries of the world as you move

00:13:58 --> 00:14:00 over them in your orbit. So it isn't like

00:14:00 --> 00:14:02 this thing is just going to affect people in

00:14:02 --> 00:14:03 the U.S. because it's been launched from the

00:14:03 --> 00:14:05 U.S. it's going to be going around the Earth,

00:14:05 --> 00:14:08 like say, running a five kilometer size beam

00:14:08 --> 00:14:10 of light across the surface of the earth,

00:14:11 --> 00:14:13 every 90 minutes as it goes round and round

00:14:13 --> 00:14:14 and round and round.

00:14:14 --> 00:14:17 Andrew Dunkley: It just doesn't, doesn't make much sense

00:14:17 --> 00:14:19 really. It sounds like pie in the sky. But,

00:14:20 --> 00:14:22 yeah, they're actually seriously considering

00:14:22 --> 00:14:25 doing this. And yeah, hopefully

00:14:25 --> 00:14:28 common sense will prevail, but, time will

00:14:28 --> 00:14:30 tell, I suppose we'll know next year whether

00:14:30 --> 00:14:32 or not they start testing these things.

00:14:33 --> 00:14:35 I know they did do this some years ago

00:14:36 --> 00:14:38 with a mirror array up in space and they,

00:14:38 --> 00:14:41 they lit up a spot on Siberia or something.

00:14:43 --> 00:14:45 yeah, I don't know why they did that then. I

00:14:45 --> 00:14:47 can't remember. But, it was, somewhat

00:14:47 --> 00:14:49 successful, although quite dim. But, This,

00:14:49 --> 00:14:52 this just. Yeah, I mean, I don't know where

00:14:52 --> 00:14:55 it stops. there seems to be this,

00:14:55 --> 00:14:58 this constant tug of war between what

00:14:58 --> 00:15:01 we need up there and what we don't need up

00:15:01 --> 00:15:03 there. And the. Yeah,

00:15:04 --> 00:15:06 it's swinging the wrong way at the moment, I

00:15:06 --> 00:15:08 suppose, would be the way to describe it.

00:15:08 --> 00:15:10 But, I dare say this will get a lot more

00:15:10 --> 00:15:13 press and a lot more pushback and maybe the

00:15:13 --> 00:15:16 fcc, will look at the

00:15:16 --> 00:15:17 problems associated with this.

00:15:18 --> 00:15:20 Jonti Horner: Really hope so. I mean, it reminds me, and

00:15:20 --> 00:15:22 I'm probably paraphrasing terribly, but

00:15:22 --> 00:15:23 there's a famous science fiction quote,

00:15:23 --> 00:15:25 something along the lines of, you know, they

00:15:25 --> 00:15:27 spent so much time and effort trying to show

00:15:27 --> 00:15:28 that they could, that they never put any

00:15:28 --> 00:15:31 thought into whether they should. It feels

00:15:31 --> 00:15:31 like all of those.

00:15:32 --> 00:15:35 Andrew Dunkley: Yes, yes, indeed. All right. yeah, it's

00:15:35 --> 00:15:37 a project, you might find online. It's only

00:15:37 --> 00:15:39 just sort of starting to emerge. I don't know

00:15:39 --> 00:15:41 how much press it's got yet, but, it will

00:15:41 --> 00:15:44 grow. Because it's one of those stories that,

00:15:45 --> 00:15:47 is also fascinating and they're the ones that

00:15:47 --> 00:15:49 generally get a lot of attention.

00:15:49 --> 00:15:51 Jonti Horner: Looking at the website, the company seems to

00:15:51 --> 00:15:52 have been around for quite a while and I

00:15:52 --> 00:15:54 think it's probably getting attention now

00:15:54 --> 00:15:57 because previously everybody thought, well,

00:15:57 --> 00:16:00 no, this will never fly. This is clearly not

00:16:00 --> 00:16:02 something we should be worried about. And now

00:16:02 --> 00:16:04 it's very clear that actually it is, because

00:16:04 --> 00:16:07 they're in for licenses and they've got a lot

00:16:07 --> 00:16:08 of money invested.

00:16:08 --> 00:16:09 Andrew Dunkley: Yeah.

00:16:09 --> 00:16:09 Jonti Horner: Yeah.

00:16:09 --> 00:16:11 Andrew Dunkley: And one wonders who's really going to pay

00:16:11 --> 00:16:14 them to shed a little light on their

00:16:14 --> 00:16:16 whatever. I mean, what would you use it for?

00:16:16 --> 00:16:18 Solar panels. You said they won't work.

00:16:19 --> 00:16:21 Football, matches. Well, we've got lights for

00:16:21 --> 00:16:23 that. I don't know. I don't know.

00:16:23 --> 00:16:25 Jonti Horner: We can do a bit of quick mental arithmetic to

00:16:25 --> 00:16:27 cheer everybody up. I mean, the brightness of

00:16:27 --> 00:16:30 the full moon to first order very roughly, is

00:16:30 --> 00:16:32 about magnitude -12 in the wonderful

00:16:32 --> 00:16:35 complex magnitude system astronomers are so

00:16:35 --> 00:16:37 fond of. The brightness of the noonday sun's

00:16:37 --> 00:16:40 about magnitude -27. So that's a 15

00:16:40 --> 00:16:43 magnitude difference. Now, that magnitude

00:16:43 --> 00:16:45 system is a logarithmic scale.

00:16:45 --> 00:16:47 So every five magnitudes you're brighter off

00:16:47 --> 00:16:50 enter than something is equivalent to a

00:16:50 --> 00:16:52 factor of 100 influx. So if you're

00:16:52 --> 00:16:55 15 magnitudes, that's three lots of 100. So

00:16:55 --> 00:16:58 100 times 100 times 100, that's 100

00:16:58 --> 00:17:01 becomes 10 becomes a million.

00:17:02 --> 00:17:04 So if the light from this thing is about the

00:17:04 --> 00:17:06 brightness of the full moon, it's a million

00:17:06 --> 00:17:08 times fainter than the sun is.

00:17:09 --> 00:17:12 So if you've got your solar panels that are

00:17:12 --> 00:17:15 generating in full sunlight, you know, a few

00:17:15 --> 00:17:17 hundred watts of power, right. they're

00:17:17 --> 00:17:20 generating a few hundred watts. Divide that

00:17:20 --> 00:17:23 by a million and you're not

00:17:23 --> 00:17:25 generating enough to register. Yeah,

00:17:25 --> 00:17:26 yeah.

00:17:26 --> 00:17:28 Andrew Dunkley: It would be like putting up a solar panel to

00:17:28 --> 00:17:31 power a light and using that light to

00:17:31 --> 00:17:33 generate the power to power that light.

00:17:33 --> 00:17:36 Jonti Horner: It's just absolutely. Or just holding a

00:17:36 --> 00:17:38 match, a lit match near your solar panels and

00:17:38 --> 00:17:41 expecting it to run your entire house. Yeah,

00:17:41 --> 00:17:41 yeah.

00:17:41 --> 00:17:43 Andrew Dunkley: Ah, it's crazy stuff. All right, yeah, keep

00:17:43 --> 00:17:45 an eye out for that story and if you feel

00:17:45 --> 00:17:47 strongly enough about it, maybe, get

00:17:47 --> 00:17:48 involved.

00:17:49 --> 00:17:50 let's move on to our next story. this

00:17:50 --> 00:17:53 involves a near miss for Earth with asteroid,

00:17:54 --> 00:17:56 2025 TF just skimming us,

00:17:56 --> 00:17:59 and we didn't see it till it was too late,

00:18:00 --> 00:18:02 technically speaking. And, it kind of

00:18:02 --> 00:18:05 dovetails into the previous story because if

00:18:05 --> 00:18:07 there's going to be more light up there, it's

00:18:07 --> 00:18:09 going to make us harder, make things harder

00:18:09 --> 00:18:11 for us in terms of, you know, getting these

00:18:11 --> 00:18:14 ready alerts for potential objects that could

00:18:14 --> 00:18:17 strike Earth. this one wasn't huge,

00:18:17 --> 00:18:20 but, yeah, it was, it was there and

00:18:20 --> 00:18:22 it was a detectable object and we didn't see

00:18:22 --> 00:18:22 it.

00:18:22 --> 00:18:25 Jonti Horner: Yes. And that's the issue. Now, this

00:18:25 --> 00:18:28 thing, you know, quite happy to say, straight

00:18:28 --> 00:18:30 up the size of this thing is such that it

00:18:30 --> 00:18:32 would have put on a nice light show as it,

00:18:32 --> 00:18:35 you know, was quite harmlessly destroyed in

00:18:35 --> 00:18:37 the atmosphere. It was probably about 1 to 3

00:18:37 --> 00:18:37 meters across.

00:18:38 --> 00:18:38 Andrew Dunkley: Yeah.

00:18:38 --> 00:18:40 Jonti Horner: But of the things that have not entered the

00:18:40 --> 00:18:43 Earth's atmosphere, but have come close, this

00:18:43 --> 00:18:45 is the second closest on record. Now,

00:18:46 --> 00:18:48 back in. I'm trying to remember exactly when

00:18:48 --> 00:18:50 the great daylight fireball was. But in the

00:18:50 --> 00:18:53 early 1970s, there was a fireball

00:18:54 --> 00:18:56 observed widely over, North America, which

00:18:56 --> 00:18:59 was what we call an earth grazing object, and

00:18:59 --> 00:19:00 it actually hit the atmosphere and skimmed

00:19:00 --> 00:19:03 back out. That is not counted when people

00:19:03 --> 00:19:05 talk about these two closest encounters that

00:19:05 --> 00:19:07 didn't hit Earth because technically that did

00:19:07 --> 00:19:09 hit the atmosphere. The fact that it skipped

00:19:09 --> 00:19:12 back out again is beside the point.

00:19:12 --> 00:19:14 And that was a daylight fireball. It created

00:19:14 --> 00:19:16 sonic booms over a couple of the US States

00:19:16 --> 00:19:18 and was really the first kind of fireball

00:19:18 --> 00:19:20 event that was widely captured because it was

00:19:20 --> 00:19:23 early in the era of modern holiday

00:19:23 --> 00:19:25 snaps. And this was a time when people were

00:19:25 --> 00:19:27 taking photos on holiday, then boring their

00:19:27 --> 00:19:28 friends when they came home.

00:19:28 --> 00:19:30 Andrew Dunkley: Yeah, yeah, 1972 it was.

00:19:30 --> 00:19:32 Jonti Horner: That's the one. Yeah, I thought it was. It

00:19:32 --> 00:19:35 was, probably something smaller than a house

00:19:35 --> 00:19:37 that came within about 57 km

00:19:37 --> 00:19:40 of the surface of the Earth. And put that in

00:19:40 --> 00:19:42 perspective, that's like, you know, the old

00:19:42 --> 00:19:43 William Tell thing of shooting an apple off

00:19:43 --> 00:19:45 somebody's head. That's like shooting the

00:19:45 --> 00:19:47 arrow at the apple and touching the skin of

00:19:47 --> 00:19:50 the apple without breaking it. It's coming

00:19:50 --> 00:19:52 within less than 1% of the diameter of the

00:19:52 --> 00:19:54 Earth of actually hitting our planet. This

00:19:54 --> 00:19:57 one wasn't quite that close. But it's an

00:19:57 --> 00:19:59 object that was discovered by the Catalina

00:19:59 --> 00:20:02 Sky Survey a few hours after

00:20:02 --> 00:20:04 its closest approach to the Earth,

00:20:05 --> 00:20:08 basically whizzed over Antarctica. So I think

00:20:08 --> 00:20:10 it's one of those that even if it had hit the

00:20:10 --> 00:20:11 atmosphere and burned up, very few people

00:20:11 --> 00:20:13 would have seen it, but a lot of penguins

00:20:13 --> 00:20:16 would have been impressed. at

00:20:16 --> 00:20:19 its closest, it was 428km above the

00:20:19 --> 00:20:21 Earth's surface. So that's slightly closer

00:20:21 --> 00:20:23 than reflector orbital. Want to put their

00:20:23 --> 00:20:25 mirrors. so if it had come through a few

00:20:25 --> 00:20:27 years later, we could have hoped it would

00:20:27 --> 00:20:28 have knocked a few of them out of the way.

00:20:28 --> 00:20:31 But it's a really close approach.

00:20:31 --> 00:20:33 And, yes, it's an object that in this case

00:20:33 --> 00:20:35 wouldn't have been big enough to cause any

00:20:35 --> 00:20:38 damage, wouldn't have had any impacts felt at

00:20:38 --> 00:20:41 ground level. It may have, if it was made of

00:20:41 --> 00:20:42 the right stuff, dropped a few little bits of

00:20:42 --> 00:20:45 meteorite on the surface, but that's about

00:20:45 --> 00:20:47 it. But it's a reminder,

00:20:48 --> 00:20:50 of the fact that as we're looking for things

00:20:50 --> 00:20:52 that come close enough to the Earth, to pose

00:20:52 --> 00:20:54 a threat. We haven't found them all yet.

00:20:54 --> 00:20:57 Now probably about 75% of the threat

00:20:57 --> 00:20:59 to the Earth, from impacts comes from the

00:20:59 --> 00:21:01 near Earth asteroids. And they're objects at

00:21:01 --> 00:21:04 the bottom of the asteroid belt, typically

00:21:04 --> 00:21:06 rocky or metallic objects moving on orbits at

00:21:06 --> 00:21:08 a relatively short period in the inner solar

00:21:08 --> 00:21:10 system. And they're short lived. You know, if

00:21:10 --> 00:21:12 you come back in a million years, most of the

00:21:12 --> 00:21:14 ones we currently know will have been

00:21:14 --> 00:21:15 removed. They'll have been ejected from the

00:21:15 --> 00:21:17 solar system or collided with a planet or

00:21:17 --> 00:21:20 fallen apart or fallen into the sun. But

00:21:20 --> 00:21:21 they're continually being repopulated from

00:21:21 --> 00:21:24 the asteroid belt. Some of them hide

00:21:24 --> 00:21:26 closer to the sun than we are and then pop

00:21:26 --> 00:21:28 out to say hello. We were talking about that

00:21:28 --> 00:21:30 last week with the objects near Venus.

00:21:31 --> 00:21:33 But there's this effort to try and find all

00:21:33 --> 00:21:36 of them. And the earlier you can find them,

00:21:36 --> 00:21:38 and the earlier you can figure out if there's

00:21:38 --> 00:21:40 going to be an encounter with the Earth that

00:21:40 --> 00:21:43 poses a threat, the better the odds of you

00:21:43 --> 00:21:45 doing something about it. And we saw this

00:21:46 --> 00:21:48 kind of a bright light shone on this back at

00:21:48 --> 00:21:50 the start of 2025 with the object

00:21:50 --> 00:21:53 2024 yr 4. I think the name M was

00:21:53 --> 00:21:55 that for a while we thought had a

00:21:56 --> 00:21:58 substantial possibility of hitting the Earth

00:21:58 --> 00:22:01 in 2032 that we now know is not going to

00:22:01 --> 00:22:02 hit the Earth, but might hit the moon in

00:22:02 --> 00:22:04 2032. And that was a big success because we

00:22:04 --> 00:22:06 found it early enough to get a lot of data.

00:22:06 --> 00:22:07 and over the course of about a month

00:22:07 --> 00:22:10 astronomers observed it repeatedly until

00:22:10 --> 00:22:12 eventually we showed that it definitely

00:22:12 --> 00:22:13 wasn't going to hit the Earth in eight year

00:22:13 --> 00:22:15 time. And everybody kind of basically jumped

00:22:15 --> 00:22:17 up and down and said hooray. And there was

00:22:17 --> 00:22:19 much rejoicing. So that's like the ideal

00:22:19 --> 00:22:22 scenario. We find something when it passes

00:22:22 --> 00:22:25 relatively nearby on one apparition a

00:22:25 --> 00:22:27 few years before it would realistically pose

00:22:27 --> 00:22:30 a threat. And that's what we want to achieve.

00:22:30 --> 00:22:32 And the stated goal of a lot of the agencies

00:22:32 --> 00:22:34 looking for these things is to find all the

00:22:34 --> 00:22:36 objects bigger than about 100 meters across

00:22:37 --> 00:22:38 that could pose a threat to the Earth, and

00:22:38 --> 00:22:41 catalog them. And we haven't managed

00:22:41 --> 00:22:44 that yet. We even more haven't managed that

00:22:44 --> 00:22:45 when you take into account things like

00:22:45 --> 00:22:47 comets. You know we were talking about, about

00:22:47 --> 00:22:50 Comet Swan last week, which appeared from

00:22:50 --> 00:22:52 hiding behind the sun and came and was

00:22:52 --> 00:22:54 suddenly the brightest comet in the sky.

00:22:54 --> 00:22:56 Comets are coming in on orbits that take

00:22:56 --> 00:22:59 hundreds, thousands, sometimes even tens of

00:22:59 --> 00:23:00 thousands or millions of years to complete.

00:23:01 --> 00:23:02 So even if we find all the near Earth

00:23:02 --> 00:23:05 asteroids, we're still going to have comets

00:23:05 --> 00:23:06 coming in. So we'll have to stay vigilant and

00:23:06 --> 00:23:09 keep watching forevermore. But this

00:23:09 --> 00:23:12 is a really good reminder that despite how

00:23:12 --> 00:23:15 you feel, we're not there yet. We are still

00:23:15 --> 00:23:17 in a position where these things are

00:23:17 --> 00:23:20 catching us by surprise. And the worst case

00:23:20 --> 00:23:22 scenario is what happened in 2013 with the

00:23:22 --> 00:23:24 Chelyabinsk impactor to a similar

00:23:24 --> 00:23:27 level of what happened with comets 1 earlier

00:23:27 --> 00:23:28 this year in that as, ah, the object

00:23:28 --> 00:23:30 approaches the Earth and eventually gets

00:23:30 --> 00:23:32 close enough that it was visible in the

00:23:32 --> 00:23:34 nighttime sky, would be able to detect it.

00:23:34 --> 00:23:36 It's coming from the sunward side of the

00:23:36 --> 00:23:37 Earth, so it's hidden in the glare of

00:23:37 --> 00:23:40 daylight. And so that's why you

00:23:40 --> 00:23:42 don't want to try and detect something the

00:23:42 --> 00:23:44 moment it's on an approach to hit you. You

00:23:44 --> 00:23:47 want to find it well in advance. And with

00:23:47 --> 00:23:48 Charlie Abinsky, it demonstrated something

00:23:48 --> 00:23:51 big enough to injure people, damage a city

00:23:51 --> 00:23:53 we didn't find until it was in the

00:23:53 --> 00:23:55 atmosphere. And it was kind of too late. It

00:23:55 --> 00:23:56 was seconds from disaster.

00:23:57 --> 00:23:57 Andrew Dunkley: Indeed.

00:23:58 --> 00:24:00 Jonti Horner: Now there's hope. We've got Vera Rubin

00:24:00 --> 00:24:02 coming online. We saw a beautiful picture

00:24:02 --> 00:24:05 from that earlier this year. Vera Rubin's

00:24:05 --> 00:24:06 going to start getting data regularly,

00:24:07 --> 00:24:09 continuously later this year, early next

00:24:09 --> 00:24:11 year, that's when the Mayan mission starts.

00:24:11 --> 00:24:13 And Vera Rubin is going to be an exceptional

00:24:13 --> 00:24:16 thing finding tool no matter what. The thing

00:24:16 --> 00:24:18 is, it will find more of them than anybody's

00:24:18 --> 00:24:20 found before. From a solar system point of

00:24:20 --> 00:24:22 view. We're really excited because it will

00:24:22 --> 00:24:24 increase the number of objects we know by a

00:24:24 --> 00:24:27 factor of several to an order of magnitude

00:24:27 --> 00:24:29 within a year or two. And it'll be great at

00:24:29 --> 00:24:32 finding these things, but it'll be less

00:24:32 --> 00:24:34 great than it would have been thanks to all

00:24:34 --> 00:24:35 the stuff we keep watching.

00:24:35 --> 00:24:36 Then this is where it ties into the previous

00:24:37 --> 00:24:40 story. Also ties in again to the wonderful

00:24:40 --> 00:24:42 student who sent me the information about the

00:24:42 --> 00:24:44 reflector orbital stuff. Jessica Heim

00:24:45 --> 00:24:47 is finishing up her PhD with us at UNESCO.

00:24:47 --> 00:24:50 She's based in North America and she's

00:24:50 --> 00:24:53 done a lot of her work about light pollution

00:24:53 --> 00:24:55 and artificial, light at night and things

00:24:55 --> 00:24:57 like this. And one of her papers early in a

00:24:57 --> 00:25:00 PhD that she was a co author on was in

00:25:00 --> 00:25:02 Nature Astronomy. And they actually did a

00:25:02 --> 00:25:05 study looking at just the starlink satellites

00:25:05 --> 00:25:07 that were in orbit at that time, so not the

00:25:07 --> 00:25:10 predicted number in the future, and tried to

00:25:10 --> 00:25:13 quantify how much harder they would make

00:25:13 --> 00:25:14 life for Vera Rubin, and particularly how

00:25:14 --> 00:25:16 much harder they make it for Vera Rubin to

00:25:16 --> 00:25:18 find objects like the one we're just talking

00:25:18 --> 00:25:20 about that was over Antarctica.

00:25:21 --> 00:25:23 And what they found was the Starlink

00:25:23 --> 00:25:25 satellites that were in orbit at the time. So

00:25:25 --> 00:25:27 not the constellation we have now, which is

00:25:27 --> 00:25:30 big and not the final constellation would

00:25:30 --> 00:25:32 make it 10% harder for Vera Rubin to do its

00:25:32 --> 00:25:33 job. So in other words, it would have to

00:25:33 --> 00:25:36 observe for 10% longer. Roughly. I think the

00:25:36 --> 00:25:37 number was actually slightly higher than that

00:25:38 --> 00:25:40 in order to achieve the same results. Now

00:25:40 --> 00:25:42 when you're talking about a facility that's a

00:25:42 --> 00:25:45 billion dollar level facility, hundreds of

00:25:45 --> 00:25:47 millions of dollars to build, having to take

00:25:47 --> 00:25:50 10% longer to do something is a cost measured

00:25:50 --> 00:25:52 in tens of millions of dollars. Yeah, that's

00:25:52 --> 00:25:54 real impact in this. And what it means is

00:25:54 --> 00:25:56 that things like this are going to be harder

00:25:56 --> 00:25:58 to find. And our ability to

00:25:59 --> 00:26:02 detect potential threats is really

00:26:02 --> 00:26:05 kind of confused and obfuscated by the

00:26:05 --> 00:26:07 stuff we're putting to hang around in the

00:26:07 --> 00:26:09 foreground. It's like, I guess it's really

00:26:09 --> 00:26:11 easy to see a road sign on a clear day, but

00:26:11 --> 00:26:13 when it's foggy, it's a lot harder to spot it

00:26:13 --> 00:26:14 until you're right on that side.

00:26:15 --> 00:26:18 Andrew Dunkley: Yeah, yeah, indeed. And

00:26:18 --> 00:26:20 if you want to read up on that story, about

00:26:20 --> 00:26:23 the near miss, you can do so@space

00:26:23 --> 00:26:25 space.com. this is Space Nuts with Andrew

00:26:25 --> 00:26:27 Dunkley and John T. Horner.

00:26:28 --> 00:26:30 Jonti Horner: Three, two, one.

00:26:31 --> 00:26:32 Andrew Dunkley: Space nuts.

00:26:33 --> 00:26:35 Now, Johnny, we have found the

00:26:35 --> 00:26:38 6th exoplanet.

00:26:38 --> 00:26:40 It took us 30 years, which is,

00:26:41 --> 00:26:43 you know, if you, if you look back at when we

00:26:43 --> 00:26:46 found the first one, it was quite a surprise

00:26:46 --> 00:26:49 for a bunch of reasons. mostly because

00:26:49 --> 00:26:51 we didn't even know they could have existed

00:26:51 --> 00:26:53 beyond our solar system. Logic suggests, you

00:26:53 --> 00:26:56 know, if it's. We've got planets around our

00:26:56 --> 00:26:59 sun, other stars must have planets too.

00:26:59 --> 00:27:02 And 30 years ago, that was proven. Well, now

00:27:02 --> 00:27:04 we're up to number 6. When are we going

00:27:04 --> 00:27:06 to stop counting? Because it's going to reach

00:27:06 --> 00:27:08 a point where we're going to find millions

00:27:08 --> 00:27:10 upon millions of these things, isn't it?

00:27:10 --> 00:27:12 Jonti Horner: It is. And even the counting's a little bit

00:27:12 --> 00:27:15 confused because the resource I

00:27:15 --> 00:27:18 trust as kind of being the authoritative word

00:27:18 --> 00:27:20 on this is the NASA exoplanet archive, which

00:27:20 --> 00:27:22 is a wonderful resource. And they've got a

00:27:22 --> 00:27:25 certain threshold for what they consider a

00:27:25 --> 00:27:27 confirmed planet. And we've got all these

00:27:27 --> 00:27:29 candidate planets as well, of which there are

00:27:29 --> 00:27:31 thousands more where we're fairly Confident

00:27:31 --> 00:27:33 there's a planet there, but it doesn't meet

00:27:33 --> 00:27:36 that rigorous criterion. There is a

00:27:36 --> 00:27:38 different exoplanet catalog run out of Europe

00:27:38 --> 00:27:40 that has a number higher because they are

00:27:40 --> 00:27:42 less strict on their criterion for

00:27:43 --> 00:27:45 confirmation. part of the reason I'm more

00:27:45 --> 00:27:47 skeptical about that catalog is that there's

00:27:47 --> 00:27:49 a number of planetary systems I've helped to

00:27:49 --> 00:27:52 kill and they've left them in their catalog.

00:27:52 --> 00:27:53 So we know for a fact those planets aren't

00:27:53 --> 00:27:55 there. I did some of that work and they still

00:27:55 --> 00:27:57 include them in their catalog, which puts

00:27:57 --> 00:27:59 them m on my naughty list. So I prefer the

00:27:59 --> 00:28:02 NASA one and the NASA one is the more

00:28:02 --> 00:28:04 cautious of them. It's really

00:28:04 --> 00:28:06 interesting how this has come though. You

00:28:06 --> 00:28:08 know, I'm, I'm 47 now. I don't feel it, but

00:28:08 --> 00:28:11 I'm getting on a little bit. I was a kid who

00:28:11 --> 00:28:13 was mad about astronomy. You know, like some

00:28:13 --> 00:28:14 of the people who send in their questions,

00:28:14 --> 00:28:16 some of the youngsters who send in questions.

00:28:16 --> 00:28:18 And when I was growing up, one of the

00:28:18 --> 00:28:19 questions I'd have been asking is do you

00:28:19 --> 00:28:21 think there are planets around other stars?

00:28:22 --> 00:28:24 We'd had observations from satellites like

00:28:24 --> 00:28:27 IRAS in the 1980s that indicated there was

00:28:27 --> 00:28:30 dust and debris around some stars. But at

00:28:30 --> 00:28:33 the time our models of planet formation fell

00:28:33 --> 00:28:35 into kind of two camps. So whereas what's now

00:28:35 --> 00:28:37 become kind of the standard baseline with

00:28:37 --> 00:28:39 some tweaks, which was that you get a disc of

00:28:39 --> 00:28:42 material around every young star and planets

00:28:42 --> 00:28:44 forming it. So most stars will have planets.

00:28:44 --> 00:28:47 But there was a competing theory that said

00:28:47 --> 00:28:49 that the planets were formed by a very close

00:28:49 --> 00:28:51 encounter between the sun and a passing star

00:28:51 --> 00:28:54 that pulled material out of the sun like a

00:28:54 --> 00:28:56 tongue of material, and the planets formed

00:28:56 --> 00:28:59 from that. and there are people who were

00:28:59 --> 00:29:02 very strong advocates of that. Now

00:29:02 --> 00:29:04 the test of those theories

00:29:05 --> 00:29:07 it would have been, are, ah, there planets

00:29:07 --> 00:29:09 around other stars, Are they common? Because

00:29:09 --> 00:29:10 the idea that two stars get close enough

00:29:10 --> 00:29:13 together to have this tidal interaction pull

00:29:13 --> 00:29:15 out a ton of material and planets form from

00:29:15 --> 00:29:17 that would suggest that planets would be

00:29:17 --> 00:29:20 overwhelmingly rare in the cosmos. So

00:29:20 --> 00:29:21 likelihood of 2 stars getting that close

00:29:21 --> 00:29:23 together and having exactly the right

00:29:23 --> 00:29:25 conditions would mean that planets were

00:29:25 --> 00:29:28 pretty much non existent, that they were a

00:29:28 --> 00:29:31 fluke of nature. The other model

00:29:31 --> 00:29:33 suggested that planets are common. And so one

00:29:33 --> 00:29:36 of the goals in the early 1990s with the

00:29:36 --> 00:29:39 search for planets elsewhere was to see

00:29:39 --> 00:29:40 whether there were any at all. And we just

00:29:40 --> 00:29:43 didn't know. The discovery of

00:29:43 --> 00:29:45 three planets around a pulsar in the early

00:29:45 --> 00:29:48 1990s broke everybody's heads. Those

00:29:48 --> 00:29:50 planets have now, incidentally, been called

00:29:50 --> 00:29:53 drow, Phoebeta and poltergeist, which are

00:29:53 --> 00:29:54 names of different types of undead from

00:29:54 --> 00:29:56 different cultures around the world. And I

00:29:56 --> 00:29:57 think that's kind of cute because you've got

00:29:57 --> 00:30:00 zombie planets around a dead star. That's all

00:30:00 --> 00:30:03 good. But 30 years ago, and actually 30 years

00:30:03 --> 00:30:05 ago last week on the 6th of October

00:30:05 --> 00:30:08 1995, we saw the announcement

00:30:08 --> 00:30:10 of the first confirmed planet around a star

00:30:10 --> 00:30:13 like the sun. And that planet was 51 Pegasi

00:30:13 --> 00:30:16 b. So it's a planet going around the south 51

00:30:16 --> 00:30:19 Pegasi. And it immediately broke

00:30:19 --> 00:30:20 everybody's heads because it was not what we

00:30:20 --> 00:30:23 expected. So both our models of planet

00:30:23 --> 00:30:26 formation that were based on a grand total of

00:30:26 --> 00:30:28 one planetary system, our own, predicted

00:30:28 --> 00:30:30 you'd have rocky planets close to the star

00:30:30 --> 00:30:33 and big gas giants a long way from the star,

00:30:33 --> 00:30:34 because that's what we see at home. And that

00:30:34 --> 00:30:37 makes sense. So to find a planet

00:30:37 --> 00:30:39 similar to Jupiter, but going around its star

00:30:39 --> 00:30:41 every four days with a surface temperature in

00:30:41 --> 00:30:44 excess of a thousand degrees C was not

00:30:44 --> 00:30:46 what was expected, I think would be the

00:30:46 --> 00:30:48 polite way to put it. Now, that forced people

00:30:48 --> 00:30:51 to immediately go back and start revisiting

00:30:51 --> 00:30:53 and improving that disk model of planet

00:30:53 --> 00:30:55 formation, which has kind of led us to where

00:30:55 --> 00:30:57 we are now. But that was kind of

00:30:57 --> 00:31:00 fundamental and foundational. For the first

00:31:01 --> 00:31:03 decade or so after that

00:31:03 --> 00:31:06 discovery, new planets were found in dribs

00:31:06 --> 00:31:08 and drabs, and the rate at which they were

00:31:08 --> 00:31:10 discovered gradually increased. And in that

00:31:10 --> 00:31:12 first decade, the best technique for finding

00:31:12 --> 00:31:14 planets, the one that was most successful,

00:31:14 --> 00:31:16 was what we call the radial velocity method,

00:31:17 --> 00:31:19 which Australia really played a leading role

00:31:19 --> 00:31:21 in with the Anglo Australian Planet Search.

00:31:21 --> 00:31:23 There was this beautiful spectrograph

00:31:23 --> 00:31:25 attached to the 3.9 meter telescope at Siding

00:31:25 --> 00:31:28 Spring, which I know Fred loves daily. It's a

00:31:28 --> 00:31:31 real icon of Australian astronomy. And, that

00:31:31 --> 00:31:33 telescope was used to point at one star,

00:31:33 --> 00:31:35 measure that star speed, then point at

00:31:35 --> 00:31:38 another, and gradually survey this collection

00:31:38 --> 00:31:40 of stars and then keep coming back to them

00:31:40 --> 00:31:41 every now and again and measure their speed

00:31:41 --> 00:31:43 again. And, by measuring the speed of these

00:31:43 --> 00:31:46 stars to the level that you can see them

00:31:46 --> 00:31:49 wobbling with changes of

00:31:49 --> 00:31:51 speed measured in a few meters per second. So

00:31:51 --> 00:31:53 comparable to speed, people walk or jog

00:31:53 --> 00:31:56 around stars that are trillions or

00:31:56 --> 00:31:57 quadrillions of kilometers away, measuring

00:31:57 --> 00:31:59 their wobbles to a precision of meters per

00:31:59 --> 00:32:02 second. That just makes my head hurt. But by

00:32:02 --> 00:32:04 doing that, you can spot the telltale wobble

00:32:04 --> 00:32:07 of a star rocking back and forward in space

00:32:07 --> 00:32:09 and infer the presence of a planet. But it's

00:32:09 --> 00:32:12 a really time consuming, challenging

00:32:12 --> 00:32:14 method where you can only observe a few stars

00:32:14 --> 00:32:15 at once, because you've got to gather light

00:32:15 --> 00:32:18 for an hour or more to get enough

00:32:18 --> 00:32:20 light, to get an accurate enough spectrum to

00:32:20 --> 00:32:22 get a single measurement. And you can only

00:32:22 --> 00:32:24 point at one star at once. By

00:32:25 --> 00:32:27 the late part of the first decade of the

00:32:27 --> 00:32:30 21st century, the transit method started to

00:32:30 --> 00:32:32 take over. And this is where we look at a lot

00:32:32 --> 00:32:35 of stars all at once and look for the

00:32:35 --> 00:32:37 few of them that are winking at us. So

00:32:37 --> 00:32:39 they've got a planet going around them that's

00:32:39 --> 00:32:40 lined, up just right that every time it goes

00:32:40 --> 00:32:42 around that star, it will block a bit of that

00:32:42 --> 00:32:44 star's light and the star will dim and then

00:32:44 --> 00:32:47 brighten again. And that started to

00:32:47 --> 00:32:49 take over from the radial velocity method

00:32:49 --> 00:32:51 purely because of the numbers. Again, because

00:32:51 --> 00:32:53 you can look at a large number of stars at

00:32:53 --> 00:32:56 the same time. And even if only

00:32:56 --> 00:32:58 1% of those stars have a planet oriented in

00:32:58 --> 00:33:00 the right direction for you to have it line

00:33:00 --> 00:33:03 up and give us a dip by looking at 100

00:33:03 --> 00:33:05 stars at once, you'll have plenty of

00:33:05 --> 00:33:07 candidates. The Kepler spacecraft

00:33:07 --> 00:33:10 launched in about 2008 and became

00:33:10 --> 00:33:13 this first census of the night sky. And

00:33:13 --> 00:33:15 it discovered on its own more than 3

00:33:15 --> 00:33:17 planets around other stars using this transit

00:33:17 --> 00:33:20 method. So we've got better and better at

00:33:20 --> 00:33:22 doing it. And over time what's happened is

00:33:22 --> 00:33:24 we've not only found the low hanging fruit,

00:33:24 --> 00:33:26 the really big planets close to their stars

00:33:26 --> 00:33:28 that give a whopping great signal that you

00:33:28 --> 00:33:30 can find, but with each generation of new

00:33:30 --> 00:33:31 instrument that's gone up there, we've got

00:33:31 --> 00:33:33 better at finding planets that are further

00:33:33 --> 00:33:35 from their stars, better at finding planets

00:33:35 --> 00:33:37 that are ever smaller, finding planets that

00:33:37 --> 00:33:40 are weird, or other techniques are coming

00:33:40 --> 00:33:41 online that allow us to do things another

00:33:41 --> 00:33:43 way. And I still think one of the greatest

00:33:43 --> 00:33:45 movies that never won an Oscar are, ah, the

00:33:45 --> 00:33:48 wonderful Images of the SAHR 8799 that

00:33:48 --> 00:33:51 shows four planets going around it. And we've

00:33:51 --> 00:33:53 got kind of a live movie of those planets

00:33:53 --> 00:33:56 orbiting that star that runs back more than a

00:33:56 --> 00:33:57 decade now. It's just breathtaking.

00:33:57 --> 00:33:59 Andrew Dunkley: Yeah, I saw it.

00:33:59 --> 00:34:02 Jonti Horner: Yeah, it's awesome. And we've basically lived

00:34:02 --> 00:34:04 through this awesome scientific

00:34:04 --> 00:34:07 revolution without really realizing it. You

00:34:07 --> 00:34:09 know, we've gone from a world where nobody

00:34:09 --> 00:34:10 knew if there were planets around other stars

00:34:11 --> 00:34:13 to a fact that there is nobody younger than

00:34:13 --> 00:34:15 the age of 30 now who grew up in that world

00:34:15 --> 00:34:18 that you and I grew up in, where we wondered

00:34:18 --> 00:34:19 if there were planets around other stars.

00:34:19 --> 00:34:22 It's absolutely breathtaking. We've had

00:34:22 --> 00:34:24 real big involvement with this here in

00:34:24 --> 00:34:26 Australia. The Anglo Australian Planet Search

00:34:26 --> 00:34:29 was one of the leaders for the first 10 or 15

00:34:29 --> 00:34:31 years of this exoplanet era. We've got a

00:34:31 --> 00:34:33 facility here in Queensland that is now

00:34:33 --> 00:34:34 leading the way, one of the leading

00:34:34 --> 00:34:37 facilities in the entire planet. You

00:34:37 --> 00:34:40 know, the only dedicated exoplanet search

00:34:40 --> 00:34:41 facility in the Southern hemisphere. And we

00:34:41 --> 00:34:44 work with NASA to do this. We've been

00:34:44 --> 00:34:47 directly involved with 41 planet discoveries

00:34:47 --> 00:34:49 in the last couple of years, using NASA's

00:34:49 --> 00:34:52 test mission and working with them. But it's

00:34:52 --> 00:34:54 this kind of ongoing exploration, this

00:34:54 --> 00:34:57 ongoing search. And, you know, what will the

00:34:57 --> 00:34:59 next 30 years bring? That's kind of what I

00:34:59 --> 00:35:02 wonder. Where will we go with it? And

00:35:02 --> 00:35:05 it's not so much when will we stop counting,

00:35:05 --> 00:35:07 but when will we start to get things that

00:35:08 --> 00:35:10 really potentially could be like the Earth?

00:35:10 --> 00:35:12 And I've said this before, I don't think

00:35:12 --> 00:35:13 we've found an Earth like planet yet. We

00:35:13 --> 00:35:15 found things about as big as the Earth that

00:35:15 --> 00:35:18 are very different. Like saying, I went

00:35:18 --> 00:35:19 swimming last week and I saw the most human

00:35:19 --> 00:35:21 like creature I've ever seen. And it was a

00:35:21 --> 00:35:23 dolphin. It was about the same size and

00:35:23 --> 00:35:25 weight as a human, but it's fundamentally not

00:35:25 --> 00:35:27 a human being. Yeah, but we're going to be

00:35:27 --> 00:35:29 moving forward and we're going to be moving

00:35:29 --> 00:35:30 from just finding these things to learning

00:35:30 --> 00:35:32 more about them. We're moving into this era

00:35:32 --> 00:35:35 of characterization and I think the number's

00:35:35 --> 00:35:36 going to gradually lose importance.

00:35:36 --> 00:35:39 You know, when we find 10 or 100,

00:35:40 --> 00:35:42 the difference will be a lot less significant

00:35:42 --> 00:35:44 than the difference between 0 and 1. But

00:35:44 --> 00:35:46 it'll start being which of the planets we

00:35:46 --> 00:35:49 know the most about. What are they like? What

00:35:49 --> 00:35:52 can we learn about them? And that's, I think,

00:35:52 --> 00:35:53 the journey for the next 30 years.

00:35:53 --> 00:35:56 Andrew Dunkley: Yes. And finding, and as you said, finding

00:35:56 --> 00:35:59 that, one planet that is so

00:35:59 --> 00:36:01 like ours in size and proximity,

00:36:02 --> 00:36:04 orbiting a sun like ours,

00:36:05 --> 00:36:08 maybe with liquid water, et cetera, et

00:36:08 --> 00:36:08 cetera.

00:36:08 --> 00:36:08 Jonti Horner: Yeah.

00:36:09 --> 00:36:11 Andrew Dunkley: that's the golden goose, isn't it, really?

00:36:11 --> 00:36:12 Jonti Horner: Absolutely.

00:36:12 --> 00:36:14 And we've got this really interesting

00:36:14 --> 00:36:17 question about how long has the

00:36:17 --> 00:36:20 Earth being in a condition that if we looked

00:36:20 --> 00:36:22 at it, it would look like the Earth. So in

00:36:22 --> 00:36:24 other words, how long has the Earth been an

00:36:24 --> 00:36:26 Earth like planet? Because when we're talking

00:36:26 --> 00:36:29 about a planet like the Earth, when it's

00:36:29 --> 00:36:30 something like the Earth is today, with, you

00:36:30 --> 00:36:32 know, beautiful blue sparkling oceans and A

00:36:32 --> 00:36:35 thin oxygen rich atmosphere and life

00:36:35 --> 00:36:37 teeming in abundant continents that are

00:36:37 --> 00:36:39 mottled brown and green and icy polar

00:36:39 --> 00:36:41 caps. But for the vast majority of the

00:36:41 --> 00:36:44 Earth's history it has looked nothing like it

00:36:44 --> 00:36:45 does now. It's had an entirely different

00:36:45 --> 00:36:48 atmosphere. It's not had free

00:36:48 --> 00:36:50 oxygen in the atmosphere. It's had periods

00:36:50 --> 00:36:52 when it was an enormous snowball, you know,

00:36:52 --> 00:36:55 snowball Earth episodes. So it's quite likely

00:36:55 --> 00:36:57 that for the majority of the Earth's history

00:36:58 --> 00:37:00 we wouldn't recognize it as an Earth like

00:37:00 --> 00:37:02 planet because it would look totally, totally

00:37:02 --> 00:37:03 different.

00:37:03 --> 00:37:05 Andrew Dunkley: Yeah, that's an interesting point. And that

00:37:05 --> 00:37:08 could exist elsewhere in the

00:37:08 --> 00:37:10 universe. And we may have seen a planet

00:37:10 --> 00:37:13 already that could one day be like

00:37:13 --> 00:37:15 ours, but it might be tens of thousands or

00:37:15 --> 00:37:17 hundreds of thousands of years before it

00:37:17 --> 00:37:19 reaches that point. So

00:37:20 --> 00:37:23 that's a really interesting factor to bring

00:37:23 --> 00:37:24 into the equation.

00:37:24 --> 00:37:27 you said some odd planets. I thought I'd do a

00:37:27 --> 00:37:29 bit of a search. these exoplanets that we've

00:37:29 --> 00:37:31 discovered in the last 30 years. Wasp

00:37:31 --> 00:37:34 76B. It's a hot

00:37:34 --> 00:37:37 Jupiter which rains molten iron. I think Fred

00:37:37 --> 00:37:38 and I talked about that one. Wasp,

00:37:39 --> 00:37:42 107B. A gas giant, with

00:37:42 --> 00:37:44 a density so low it's been described as a

00:37:44 --> 00:37:45 marshmallow planet.

00:37:47 --> 00:37:47 HD,

00:37:48 --> 00:37:51 189773B. It's a planet

00:37:51 --> 00:37:53 with an atmosphere that contains clouds of

00:37:53 --> 00:37:54 molten glass.

00:37:54 --> 00:37:57 Jonti Horner: Yeah, that's often described as a blue marble

00:37:57 --> 00:37:58 planet, I think.

00:37:58 --> 00:38:01 Andrew Dunkley: Yeah, yeah. Hat P7B is an ultra

00:38:01 --> 00:38:03 hot Jupiter that's so dark it's nearly

00:38:03 --> 00:38:05 charcoal and 5,

00:38:06 --> 00:38:08 5 Cancri E I think it's

00:38:08 --> 00:38:11 pronounced a, super Earth with a lava world,

00:38:11 --> 00:38:14 and sparkling skies. And there's probably

00:38:14 --> 00:38:17 more weird ones out there. We yet defined

00:38:17 --> 00:38:19 that, defy explanation. It's a really

00:38:19 --> 00:38:21 fascinating part of astronomy.

00:38:21 --> 00:38:23 Jonti Horner: it is. And it's that realization that the

00:38:23 --> 00:38:25 diversity of things that are out there is far

00:38:25 --> 00:38:26 greater than we could have possibly imagined.

00:38:26 --> 00:38:29 And it really forces us to revisit

00:38:29 --> 00:38:31 and refine our definitions of what a planet

00:38:31 --> 00:38:34 is. So we historically people have this

00:38:34 --> 00:38:37 idealized boundary at 13 Jupiter masses where

00:38:38 --> 00:38:39 if you're more massive than that, you're a

00:38:39 --> 00:38:41 brown dwarf and you're a fail star. And if

00:38:41 --> 00:38:42 you're less massive than that, you're a

00:38:42 --> 00:38:43 planet.

00:38:43 --> 00:38:43 Andrew Dunkley: Yeah.

00:38:43 --> 00:38:45 Jonti Horner: And we're now finding things that people are

00:38:45 --> 00:38:47 claiming a brown dwarfs that are only twice

00:38:47 --> 00:38:49 the mass of Jupiter and things people are

00:38:49 --> 00:38:50 claiming are planets that are 20 Jupiter

00:38:50 --> 00:38:53 masses. You know, there's a real blurring of

00:38:53 --> 00:38:56 that Boundary. You've then got one weird

00:38:56 --> 00:38:58 object. If you look at what the most dense

00:38:58 --> 00:39:00 planet we found is, there's one planet that

00:39:00 --> 00:39:03 has a density that is something like

00:39:03 --> 00:39:06 150 times the density of water or something

00:39:06 --> 00:39:09 like this. And it's a few Jupiter

00:39:09 --> 00:39:11 masses. And we know the density, we know the

00:39:11 --> 00:39:13 size because of transits and we know the mass

00:39:13 --> 00:39:15 because of radial velocity. And if you've got

00:39:15 --> 00:39:16 the size and the mass, you get the density.

00:39:18 --> 00:39:20 This thing is so dense so that it doesn't

00:39:20 --> 00:39:22 confirm with any known material.

00:39:23 --> 00:39:25 You know, it's many times denser than the

00:39:25 --> 00:39:27 densest metal. Gravity pulling things in

00:39:27 --> 00:39:30 can't explain it. And so

00:39:30 --> 00:39:32 is it really a planet? There is some

00:39:32 --> 00:39:34 speculation that it's actually something that

00:39:34 --> 00:39:36 was probably a white dwarf that has somehow

00:39:36 --> 00:39:39 been bombarded and fractured. So there's only

00:39:39 --> 00:39:41 a few Jupiter masses left.

00:39:42 --> 00:39:45 So it's not a planet. You know,

00:39:46 --> 00:39:47 if it was a white.

00:39:47 --> 00:39:49 Andrew Dunkley: Dwarf that's been culver, I would say no, but

00:39:49 --> 00:39:51 gosh, yeah, there's.

00:39:51 --> 00:39:53 Jonti Horner: All these other things. Planets that are less

00:39:53 --> 00:39:56 dense than cotton candy and yeah, it's

00:39:56 --> 00:39:58 awesome from a speculation point of view. And

00:39:58 --> 00:40:00 it's a, a lot of the planets we've found are

00:40:00 --> 00:40:02 things that if you saw them in an episode of

00:40:02 --> 00:40:05 Star Trek or you know, any of these sci fi

00:40:05 --> 00:40:08 series, you'd think that they jumped the

00:40:08 --> 00:40:09 shark, that that kind of thing just wasn't

00:40:09 --> 00:40:12 possible anymore. They'd obviously been

00:40:12 --> 00:40:14 enjoying themselves a little bit too much in

00:40:14 --> 00:40:17 the pre writing session. And yet we're

00:40:17 --> 00:40:19 finding these objects are just so diverse

00:40:19 --> 00:40:21 and bonkers. It's untrue. That's part of the

00:40:21 --> 00:40:23 fun of it. You never know what we're going to

00:40:23 --> 00:40:23 find next.

00:40:23 --> 00:40:24 Andrew Dunkley: Absolutely not.

00:40:25 --> 00:40:27 and that sort of takes us into our final

00:40:27 --> 00:40:30 story because this is an object that

00:40:30 --> 00:40:32 a little bit weird in our solar system.

00:40:33 --> 00:40:35 It's the moon Mimas. But it's also been

00:40:35 --> 00:40:38 called the Death Star because it does have

00:40:38 --> 00:40:40 that Death Star look about it. It's got a

00:40:40 --> 00:40:43 dish like depression, in it where it

00:40:43 --> 00:40:46 must have got hit at some stage. But the

00:40:46 --> 00:40:49 reason it's in the news now is because it

00:40:49 --> 00:40:51 is yet another object in our solar system

00:40:52 --> 00:40:54 that may contain a subsurface

00:40:54 --> 00:40:55 ocean.

00:40:56 --> 00:40:58 Jonti Horner: Yes. And it's probably of all the moons where

00:40:58 --> 00:41:01 subsurface oceans have been suspected or

00:41:01 --> 00:41:03 detected, it is the smallest of them and

00:41:03 --> 00:41:06 it's probably the most surprising of the lot.

00:41:07 --> 00:41:10 The evidence for this has built up over

00:41:10 --> 00:41:12 a bit more than a decade and comes from the

00:41:12 --> 00:41:14 Cassini mission that Spent all that time

00:41:14 --> 00:41:16 orbiting Saturn making wonderful discoveries,

00:41:16 --> 00:41:19 most famously, of course, being the geysers

00:41:19 --> 00:41:21 of liquid water erupting from the south pole

00:41:21 --> 00:41:23 of another of the small icy moons, Enceladus,

00:41:24 --> 00:41:26 which was a shock because Enceladus is so

00:41:26 --> 00:41:28 small that it should be frozen to the core.

00:41:28 --> 00:41:29 So it's a bit of a surprise there's liquid

00:41:29 --> 00:41:32 water there. Mimas is even smaller.

00:41:32 --> 00:41:35 It's the smallest object in the solar system

00:41:36 --> 00:41:39 that is spherical because its gravity has

00:41:39 --> 00:41:40 overcome the strength of the material it's

00:41:40 --> 00:41:43 made from. And when you look at the

00:41:43 --> 00:41:45 calculations people have made at what the

00:41:45 --> 00:41:48 minimum size something would have to be to be

00:41:48 --> 00:41:51 in hydrostatic equilibrium to be an object

00:41:51 --> 00:41:53 where gravity overcomes the strength. Mimas

00:41:53 --> 00:41:55 is actually a little bit smaller than that,

00:41:55 --> 00:41:58 which is interesting. It's a real edge case.

00:41:59 --> 00:42:01 And, you know, the fact that it is spherical

00:42:01 --> 00:42:03 like it is would suggest that at some point

00:42:03 --> 00:42:05 it has not been that strong in the past. So

00:42:05 --> 00:42:07 it was probably fairly liquid early on in its

00:42:07 --> 00:42:10 formation. But any ocean it had when it was

00:42:10 --> 00:42:13 born should have frozen out

00:42:13 --> 00:42:16 long, long, long, long, long ago. And, that's

00:42:16 --> 00:42:18 kind of borne out when you see the photos

00:42:18 --> 00:42:20 that are taken of Mimas. It doesn't look like

00:42:20 --> 00:42:22 Enceladus. It doesn't look like AR were

00:42:22 --> 00:42:24 talking about last week. It doesn't look like

00:42:24 --> 00:42:26 Europa. They're all places that have

00:42:26 --> 00:42:29 obviously been resurfaced, that have flat

00:42:29 --> 00:42:31 areas with cracks that look like ice that has

00:42:31 --> 00:42:33 been broken by plate tectonics. Because it's

00:42:33 --> 00:42:36 floating on an ocean, Mimas just looks like

00:42:36 --> 00:42:37 another cratered ice ball.

00:42:37 --> 00:42:38 Andrew Dunkley: Yes.

00:42:38 --> 00:42:40 Jonti Horner: So there's a few oddities that have built up.

00:42:40 --> 00:42:41 One of them is that, enormous crater,

00:42:41 --> 00:42:44 Herschel. Now, Herschel, as a crater, is

00:42:44 --> 00:42:46 almost big enough that the impactor could

00:42:46 --> 00:42:48 have shattered me. And if it had been only

00:42:48 --> 00:42:50 slightly larger, Mimas would have been

00:42:50 --> 00:42:53 destroyed. So it's right at the limit of

00:42:53 --> 00:42:56 how big a crater can be before things get

00:42:56 --> 00:42:58 seriously bad. But a lot of calculations

00:42:58 --> 00:43:01 have shown that if the Herschel crater had

00:43:01 --> 00:43:04 formed when the Moon was frozen solid to its

00:43:04 --> 00:43:07 core, it shouldn't have a central peak.

00:43:07 --> 00:43:10 But it has a central peak. Now, that suggests

00:43:10 --> 00:43:13 that Mimas was a bit slushy. But if you do

00:43:13 --> 00:43:15 the calculations and assume Mimas had a very,

00:43:15 --> 00:43:18 very well developed ocean, that

00:43:18 --> 00:43:19 crater wouldn't look like it did either,

00:43:19 --> 00:43:21 because it would have dug down into the ocean

00:43:21 --> 00:43:24 and splashed liquid water everywhere. So

00:43:24 --> 00:43:25 there are suggestions that the Herschel

00:43:25 --> 00:43:28 crater formed when Mimas was slushy rather

00:43:28 --> 00:43:30 than ocean, when it was fluid enough to get

00:43:30 --> 00:43:33 this central peak form, but not so fluid that

00:43:33 --> 00:43:35 an ocean was breached. And with the size of

00:43:35 --> 00:43:36 that M impact, it would have breached one if

00:43:36 --> 00:43:39 one was there. Now I've seen some suggestions

00:43:39 --> 00:43:41 from that saying that Herschel must therefore

00:43:41 --> 00:43:44 be a young crater because it's tied

00:43:44 --> 00:43:45 to this young ocean that is thought to be

00:43:45 --> 00:43:48 there on Mimas. Now that's one of the

00:43:48 --> 00:43:50 suggestions. I'm not necessarily sure that's

00:43:50 --> 00:43:51 the case. It may be that Herschel may be

00:43:51 --> 00:43:53 older than there was an ocean in the past.

00:43:53 --> 00:43:56 That's still to be sorted. But aside from

00:43:56 --> 00:43:58 that, there's been a lot of the data from

00:43:58 --> 00:44:01 Cassini linked to how Mimas is

00:44:01 --> 00:44:04 rotating and wobbling, suggested that

00:44:04 --> 00:44:07 it couldn't be solid to the core unless the

00:44:07 --> 00:44:09 core was not in her static equilibrium. The

00:44:09 --> 00:44:11 core was elongated and pancake shaped. and

00:44:11 --> 00:44:13 that just doesn't make sense. And as they got

00:44:13 --> 00:44:14 more and more data, more and more

00:44:14 --> 00:44:17 observations, that just doesn't work. And

00:44:17 --> 00:44:19 so from the rotation and the wobble of this

00:44:19 --> 00:44:22 moon, it suggests that as much as

00:44:22 --> 00:44:24 50% of its volume is liquid water.

00:44:25 --> 00:44:27 Wow. Which is an enormous subsurface ocean.

00:44:27 --> 00:44:30 That's an absolutely incredible ocean. But

00:44:30 --> 00:44:32 because of the thermodynamics of it, that

00:44:32 --> 00:44:34 ocean can't be old because if it was old, it

00:44:34 --> 00:44:37 would have frozen out already. Now, part of

00:44:37 --> 00:44:39 the supporting evidence for this is that the

00:44:39 --> 00:44:42 orbit of Mimas around Saturn is not perfectly

00:44:42 --> 00:44:44 circular. It's actually a little bit more

00:44:44 --> 00:44:46 eccentric than the orbit of the Earth around

00:44:46 --> 00:44:49 the Sun. That is not a

00:44:49 --> 00:44:51 situation that's tenable long term. The orbit

00:44:51 --> 00:44:53 should be circularized by tidal

00:44:53 --> 00:44:56 effects with Saturn. And so the suggestion

00:44:56 --> 00:44:58 seems to be that at some point, probably in

00:44:58 --> 00:45:01 the last 15 million years, something

00:45:01 --> 00:45:04 happened to stir, Mimas's orbit upper Mechi

00:45:04 --> 00:45:06 more eccentric, to actually make it a bit

00:45:06 --> 00:45:09 more elongated. That increased

00:45:09 --> 00:45:11 eccentricity means that Mimas now experience

00:45:11 --> 00:45:13 a significant tidal heating

00:45:14 --> 00:45:16 from being squashed and squeezed effectively

00:45:18 --> 00:45:20 by the gravity of Saturn and also by the

00:45:20 --> 00:45:21 other moons. It's in mean motion resonance

00:45:21 --> 00:45:23 with a couple of the other saturnian moons.

00:45:24 --> 00:45:25 And all of that means that you're going to

00:45:25 --> 00:45:27 get a significant amount of heat dumped into

00:45:27 --> 00:45:30 the interior of Mimas, melting that interior

00:45:30 --> 00:45:33 and creating this ocean. And the argument

00:45:33 --> 00:45:35 for the fact that the surface is not yet

00:45:35 --> 00:45:38 smooth and resurfaced is that a, that

00:45:38 --> 00:45:41 ocean is young and it's a still developing

00:45:41 --> 00:45:44 situation. But also that the crust of

00:45:44 --> 00:45:46 Mimas is 20 or 30 kilometers thick and

00:45:46 --> 00:45:48 that's thick enough that it hasn't yet

00:45:48 --> 00:45:51 responded to the liquid underneath

00:45:51 --> 00:45:53 and so you've almost got this hidden ocean in

00:45:53 --> 00:45:56 a place you wouldn't expect, but where all

00:45:56 --> 00:45:59 our observations, all our data is suggesting

00:45:59 --> 00:46:01 that the only explanation that works for all

00:46:01 --> 00:46:03 of the different things we've observed for it

00:46:03 --> 00:46:05 is that this is yet another of this growing

00:46:05 --> 00:46:08 catalog of places where there's a huge volume

00:46:08 --> 00:46:10 of liquid water buried beneath an icy

00:46:10 --> 00:46:12 surface. It's absolutely breathtaking work

00:46:12 --> 00:46:14 and it's a really good example of the

00:46:14 --> 00:46:17 iterative nature of science because it's not

00:46:17 --> 00:46:19 like this is a new discovery this week.

00:46:20 --> 00:46:21 There've been whispers about this for years

00:46:21 --> 00:46:23 and papers published about it for years and

00:46:24 --> 00:46:26 alternative hypotheses proposed and

00:46:26 --> 00:46:29 disproved and all the rest of it. And all

00:46:29 --> 00:46:31 the way through we're getting more and more

00:46:31 --> 00:46:33 certain that this ocean's there. We're

00:46:33 --> 00:46:36 learning more about the history. And I guess

00:46:36 --> 00:46:38 again, not only are we learning that liquid

00:46:38 --> 00:46:39 water is more common than the solar system,

00:46:39 --> 00:46:41 but we're getting reminded once again that

00:46:42 --> 00:46:44 the solar system's a very dynamic place. And

00:46:44 --> 00:46:47 it's not like everything of interest happened

00:46:47 --> 00:46:48 four and a half thousand million years ago.

00:46:48 --> 00:46:50 And now we're in the kind of mop up phase

00:46:50 --> 00:46:52 where nothing interesting happens. There's

00:46:52 --> 00:46:55 still a lot going on. And the solar system's

00:46:55 --> 00:46:57 dynamic in a way that if we were around when

00:46:57 --> 00:47:00 the dinosaurs walked the Earth, it would have

00:47:00 --> 00:47:01 looked like a very different place than the

00:47:01 --> 00:47:03 place we see today. It's that changeable.

00:47:03 --> 00:47:05 Andrew Dunkley: Yeah, absolutely. Yeah. And

00:47:06 --> 00:47:07 Mimas is also,

00:47:09 --> 00:47:11 if indeed it is another,

00:47:13 --> 00:47:15 water moon, let's say ice moon, whatever you

00:47:15 --> 00:47:17 want to call it, it's starting to show that

00:47:17 --> 00:47:20 it's probably more normal than we ever

00:47:20 --> 00:47:23 thought. You've got so many others that are

00:47:23 --> 00:47:26 starting to be found. obviously

00:47:26 --> 00:47:28 Europa Enceladus would be the top two, but

00:47:28 --> 00:47:30 Ganymede's now in there.

00:47:32 --> 00:47:35 Andrew Dunkley: Most of the dwarf moons,

00:47:35 --> 00:47:37 or dwarf planets in the outer solar system

00:47:37 --> 00:47:40 are starting to show these signs. So

00:47:40 --> 00:47:43 it could be quite normal here. And

00:47:43 --> 00:47:46 as we've already discussed, you know, there

00:47:46 --> 00:47:47 was a time where we weren't sure whether or

00:47:47 --> 00:47:50 not there were other planets in other solar

00:47:50 --> 00:47:53 systems in the universe. Well, it's

00:47:53 --> 00:47:55 probably going to be discovered that there

00:47:55 --> 00:47:58 are probably a lot more ice moons out there

00:47:58 --> 00:48:00 than we could possibly imagine. So.

00:48:00 --> 00:48:02 Jonti Horner: Absolutely. And the other interesting thing

00:48:02 --> 00:48:04 about this to me is it's not just suggesting

00:48:04 --> 00:48:06 that you get oceans and the oceans go away.

00:48:06 --> 00:48:09 It's suggesting you can get episodic oceans

00:48:10 --> 00:48:12 because m. If this Ocean is only 10 or 15

00:48:12 --> 00:48:15 million years old. We've had a lot of 10 and

00:48:15 --> 00:48:17 15 million year old windows

00:48:17 --> 00:48:20 in four and a half thousand million years of

00:48:20 --> 00:48:23 time. And, what is the likelihood that we

00:48:23 --> 00:48:24 just happen to be in the only one of those

00:48:24 --> 00:48:26 windows where you've got two temporary oceans

00:48:26 --> 00:48:29 at the same time, Where Enceladus and

00:48:29 --> 00:48:32 Mimas have temporary transient oceans that

00:48:32 --> 00:48:35 have only formed in recent times. And for

00:48:35 --> 00:48:37 both of them, the logic is the same. They're

00:48:37 --> 00:48:38 too small to have had this ocean since

00:48:38 --> 00:48:39 they're formed. It's got to be a recent

00:48:40 --> 00:48:42 thing. What is the likelihood that we catch

00:48:42 --> 00:48:44 two of them going off at once, just by

00:48:44 --> 00:48:46 random, when there have never been any

00:48:46 --> 00:48:48 others? So that's suggesting that these

00:48:48 --> 00:48:50 subsurface oceans on the smaller moons come

00:48:50 --> 00:48:52 and go and come again, which means

00:48:52 --> 00:48:55 that again, from the point of view of life

00:48:55 --> 00:48:57 elsewhere, life that can

00:48:57 --> 00:49:00 survive the long freeze is ready to take over

00:49:00 --> 00:49:03 during the short summer. And we see that on

00:49:03 --> 00:49:05 Earth. It's a really interesting thing that

00:49:06 --> 00:49:08 if this is a temporary transient ocean now,

00:49:09 --> 00:49:11 it's possibly been there multiple times in

00:49:11 --> 00:49:13 the past. And that's why I

00:49:13 --> 00:49:15 suspect that the Herschel Crater may not have

00:49:15 --> 00:49:18 formed with the latest recent ocean. But

00:49:18 --> 00:49:20 maybe it's a previous episode of it. We will

00:49:20 --> 00:49:22 only know when we get more studies. And of

00:49:22 --> 00:49:24 course, it's a really good reason to go back

00:49:24 --> 00:49:25 to Saturn to find out.

00:49:25 --> 00:49:28 Andrew Dunkley: Absolutely true. Yes, indeed. All right, if

00:49:28 --> 00:49:30 you want to read about that story and the,

00:49:30 --> 00:49:33 previous story, about exoplanets, you

00:49:33 --> 00:49:35 can go to space.com

00:49:36 --> 00:49:38 and we are done. Jonti, thank you so much.

00:49:39 --> 00:49:41 Jonti Horner: It's a pleasure. It's a lot to talk about.

00:49:41 --> 00:49:42 It's always good fun.

00:49:42 --> 00:49:44 Andrew Dunkley: It is great fun. Good, to see you. that's

00:49:44 --> 00:49:46 Jonti Horner, professor of Astrophysics at

00:49:46 --> 00:49:48 the University of Southern Queensland. And

00:49:48 --> 00:49:50 don't forget to visit our website while

00:49:50 --> 00:49:53 you're online and check us out. you can do

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00:50:22 --> 00:50:24 check it all out on our, space,

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00:50:28 --> 00:50:30 and I would say thanks to Huw in the studio.

00:50:30 --> 00:50:33 But he's out counting, exoplanets. And he got

00:50:33 --> 00:50:36 to 10, and you can't count any higher.

00:50:36 --> 00:50:38 And from me, Andrew Dunkley, thanks for your

00:50:38 --> 00:50:39 company. We'll see you on the next episode of

00:50:39 --> 00:50:41 Space Nuts real soon. Bye. Bye.