May 17, 2026

Supercharged Neutrinos, Exploding Black Holes & Lunar Mysteries Uncovered | Q&A

Supercharged Neutrinos, Exploding Black Holes & Lunar Mysteries Uncovered | Q&A
Exploding Black Holes, Lunar Mysteries, and Cosmic Questions In this enlightening Q&A edition of Space Nuts, hosts Andrew Dunkley and Professor Jonti Horner tackle an array of fascinating questions from listeners. From the enigmatic nature of supercharged neutrinos linked to black holes to the mysteries of the Moon's surface, this episode is a deep dive into the cosmos.
Episode Highlights:
- Supercharged Neutrinos and Black Holes: Nick's intriguing question about the detection of a supercharged neutrino prompts a discussion on the theoretical concept of exploding black holes and Hawking radiation. Jonti explains the complexities of black hole evaporation and the potential implications for our understanding of the universe.
- The Dark Side of the Moon: Andrew returns with her questions about the far side of the Moon, exploring why it appears less damaged than the near side. Jonti provides insights into the Moon’s geological history and the differences in surface features that contribute to this phenomenon.
- Shallow Craters on the Moon: Continuing with Andrew's inquiries, the hosts discuss the nature of lunar craters and why many appear shallower than expected. Jonti elaborates on the processes that lead to complex craters and their unique characteristics compared to simpler ones.
- Planet Formation and Solar System Dynamics: Eli's two-part question leads to a discussion about the composition of planets in our solar system and how their formation relates to the elements present in the Sun. The hosts delve into the nuances of planetary formation and the role of distance from the Sun in determining a planet's composition.
- Speed of the Solar System: Eli's second question prompts an exploration of how fast our solar system could travel without causing noticeable effects on Earth. Jonti explains the implications of high speeds in a dense stellar environment and how it might alter our cosmic perspective.

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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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WEBVTT

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Andrew Dunkley: Hi there. Thanks for joining us on a Q and A

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edition of Space Nuts. Andrew Dunkley here,

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your host. Great to have your company. Coming

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up, we've got a few questions. Nick is going

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to ask about supercharged neutrinos.

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Andrea is making a return appearance.

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She's got a couple of questions about the

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dark side of the moon and shallow craters.

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And Eli is asking about elements

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and the speed of objects. And if we've got

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time, we'll chuck another question into the

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mix as well. All coming up on this edition of

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Space Nuts. Seconds. Guidance is

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internal. 10, 9.

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Ignition sequence start.

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Jonti Horner: Space nuts.

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Andrew Dunkley: 5, 4, 3, 2. 1. 2, 3, 4,

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5, 5, 4, 3, 2, 1. Space

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nuts. Astronauts report it feels good.

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And with Fred away, Jonti can play.

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It's professor, uh, Jonti

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Horner, professor of Astrophysics at the

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University of Southern Queensland. Jonti,

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hello again. Good afternoon.

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Jonti Horner: How are you going to.

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Andrew Dunkley: I am well. Great to see you. I think we

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should just go straight into it and, uh,

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hit you with our first question.

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It's a topic I'm not overly familiar

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with, but, uh, this one comes from Nick.

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Uh, I just read that a supercharged neutrino

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was detected by the Kilometer Cube

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Neutrino Telescope, and a theory was

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put forward that it came from an exploding

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black hole. Please explain how a black hole

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can explode. Love the show, Nick. Thank you,

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Nick, we love that you love the show.

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Thank you for sending in a question. Um,

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exploding black holes. Um,

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I seem to remember Fred might have written a

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book about something like that once. Um, but

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anyway, um, do they explode or do they

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merge or do they collapse? They eventually

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disappear.

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Jonti Horner: I know that now. You know straight up,

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I'm not a cosmologist or a cosmetologist,

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which I always used to joke about

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cosmologists being cosmetologists. And it

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turns out a cosmetologist is a real thing. So

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never mind. Um, that's, uh,

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further from my area of expertise. So any

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answer I give, take with a larger grain of

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salt, you know, as is always the way you

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know, you. The further you go from your

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expertise, the more out of date your

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knowledge is. My knowledge on

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exploding or rather evaporating black

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holes goes back to basically when I was an

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undergrad and I was doing lots of courses in

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lots of different things. And this goes back

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to some of the work that made Stephen

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Hawking so world renowned. Now, obviously,

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for a lot of people, Stephen Hawking became a

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global name with the publication of A Brief

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History of Time, which did a very good job of

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explaining very complicated things in A way

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that people could at least feel like they had

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a grasp of. Um, I remember reading it as a

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kid, and it made my head hurt. But it, in a

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good way, I could actually follow it. It was

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well explained. One of the things that

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Stephen Hawking did fairly early in his

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career, I think in, like, 1974 or something,

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was do some very theoretical work on, um,

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black holes, where he postulated that black

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holes could lose we through a process called

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Hawking radiation. And the idea is

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that black holes can effectively be

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considered to have a temperature and to

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radiate energy and therefore mass away

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into space. And the smaller the black hole,

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the hotter it is, so the quicker it would

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radiate. And this is all backed up by

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ridiculously complex physics and mathematics

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that is way beyond my level of full

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understanding. But part of the idea behind it

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is what we think of as the empty vacuum of

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space is actually not a true vacuum, but is

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instead constantly populated by pairs

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of matter and antimatter particles that

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spontaneously create and then collide with

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each other and disappear again. And if these,

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if such an event happens near the event

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horizon of a black hole, one of the particles

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falls into the black hole, the other escapes,

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and it's seen to lose mass, lose energy, and,

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um, radiation going along with that. Now,

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the bigger the black hole, the colder it

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would be. So the slower it radiates anyway,

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but also the bigger it is, the more

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effectively it can feed from its environment.

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Even if that's little bits of dust falling

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in. Or if it's near a star, star, it can feed

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off that star, get an accretion disk. So the

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black holes that form in the modern universe

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are formed by stars reaching the end of their

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lives and are massive. They're more massive

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than the sun by L1, where they're formed from

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stars much more massive than the Sun. You get

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massive black holes, you get intermediate

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mass black holes, and you get supermassive

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black holes. And they're all the big whopping

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ones. And, um, the time scale, as I

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understand it, m for those black holes to

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decay through Hawking radiation is

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ridiculously, ridiculously, ridiculously

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longer than the edge of the universe. Yes.

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And, um, they're probably not emitting

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Hawking radiation at a level that we could

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detect because they are very cold. In his

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quantification of it, however, at, uh,

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the birth of the universe, when the

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temperature and pressure was immense after

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the Big Bang, there were

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theoretically a class of black holes created

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called primordial black holes. So these were

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black holes that were not born from the fiery

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Death of a star, but were instead born

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out of the Big Bang and the pressures and the

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temperatures. And um, these could be black

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holes down to the mass of a thumbnail or down

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really, really tiny ones. Planet mass black

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holes.

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Andrew Dunkley: Yep.

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Jonti Horner: The smaller you are as a black hole, the more

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quickly you radiate things away, so the

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shorter your lifetime. And so you have this

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idea that these primordial black holes

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evaporated over time and effectively

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none of them will survive to the current day.

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Those evaporating black holes would

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evaporate over time and give off radiation

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that we have never yet detected. But a black

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hole coming to the end of its life will

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evaporate faster and m faster. There's a

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quote on an article I found recently which

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may be tied to this, um, article entitled

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An Exploding Black Hole Could Reveal the

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Foundations of the Universe, published from

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September last year, talking about

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the predictions that as our technology gets

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better in the coming years, we may be able to

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detect this Hawking radiation in an event

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where the black hole reaches its critical

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phase and evaporates entirely within the next

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few years. So not quite the neutrino

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discovery that we were talking about in the

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question, but a related thing. And there's a

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quote here from Andrea Tham, who

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Associate Professor Andrea Tham, I, I do hate

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it when articles don't give people's well

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earned titles until later in the sentence or

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don't give them at all. Um, which is another

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ont. I could go on, that's separate, but it

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particularly affects my, um,

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early career colleagues, um, affects

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colleagues from non traditional backgrounds

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and stuff. And it's a very

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diminutizing thing, diminishing thing. It

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lowers their expertise. Anyway, this is a

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quote from Associate Professor Andrea Tham

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from University of Massachusetts Amherst,

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says as primordial black holes evaporate,

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they become ever lighter, uh, so hotter.

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They therefore emit even more radiation. It's

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a runaway process until they explode.

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Um, it's that Hawking radiation that our

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telescopes can detect.

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Andrew Dunkley: Yeah.

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Jonti Horner: So what's happening is you've got these

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primordial black holes that are really itty

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bitty diddy ones that are therefore

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evaporating quicker than they can gain mass.

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They'll be on this critical threshold. And so

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you get this runaway death where the more

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massive ones live longer before they get

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small enough to finally evaporate and then

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explode. And so I would guess

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that the observation of this super

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neutrino that has been linked potentially to

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an exploding black hole is not two black

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holes colliding. It's not a modern Black hole

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formed from the death of sars, but rather is

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the death of a primordial black hole, as

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would be predicted by this research by

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Stephen hawking more than 50 years ago in the

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form of Hawking radiation. So that's my

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thinking on what's happening here. Now,

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obviously, I am, um, not an expert.

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Um, I've said previously on many places,

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uh, in a lot of disciplines, and when we're

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teaching our undergrads, we often say, avoid

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Wikipedia. Wikipedia is not a static

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resource. It's a fluid resource and it's

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often wrong. And I know for journalists, it's

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probably often something you caution, don't

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get your facts from Wikipedia. For

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astrophysics, and particularly the more

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technical and hardcore ends of astrophysics,

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Wikipedia is actually very reliable because

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very few people will be interested in

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maliciously editing a webpage because,

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frankly, they'll go off, uh, after other

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topics that are more triggering. But also,

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people who are interested in this stuff and

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have the knowledge tend to be very obsessive.

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And if they spot something wrong, they fix it

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very quickly. The result of that is if you

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Google Hawking radiation. The

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Wikipedia page is very lengthy, goes into a

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lot of detail, includes some of the maths.

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That makes my head hurt, huh? And makes me

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want to cry a little bit.

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I'm talking about black hole evaporation and

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things like this. Now,

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the equation for black hole evaporation

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that's on here, which is based on the Hawking

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work, gives a evaporation

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time for a black hole of

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2.14 times 10 to the 67

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years. So that's 2.14

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multiplied by 10 with 67 zeros

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multiplied by the mass of the black hole

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divided by the mass of the sun to the power

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three. So if you've got a black

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hole that is one solar mass, it will take

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2.14 times 10 to the 67 years to

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evaporate. And the M more massive it is, the

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larger that number gets to the power three.

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So the multiplier here is get the mass of the

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black hole as measured in units of the mass

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of the sun, cube that number, and

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then multiply it by 2.14 times 10 to the

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67, and you get a headache, but

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you get a number. Now, the mass of the sun

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is what, 2 times 10 to the 30

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kilos? Right? Mass of the

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Earth is 5.97 times 10

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00:09:44.010 --> 00:09:46.850
to the 24 kilos. So that is

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00:09:46.930 --> 00:09:49.930
effectively, um, 2 times 10 to the minus

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00:09:49.930 --> 00:09:52.050
6 solar masses, about a millionth of a solar

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mass. So we'll just say it's 1 millionth of a

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solar mass. 1 millionth

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cubed is 1 times 10 to the minus

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18. That means a, uh, black hole, the mass

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of the Earth, would decay much more quickly.

256
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It would decay in only 10 to the 49 years,

257
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which is still much, much, much, much longer

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than the edge of the universe. But you can

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play this game with everything. I. I'm

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too fat. You know, we talk about health and

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everything on the show before. I am a fair

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bit more than 100 kilos. But let's assume I

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was 100 kilos, um, just because that's an

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aspirational goal. And it would be nice if it

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were true one day. In fact, I'm 100 kilos and

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you make me a black hole. Um, I would be sad,

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but probably wouldn't have long to think

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about it. At 100 kilos,

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I will be 10 to the 28 times

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00:10:40.840 --> 00:10:43.400
less massive than the sun, roughly. The sun

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is 10 to the 30. I'm 10 to the 2. 10 to the

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28 is a difference. 10 to the 28 cubed

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00:10:49.000 --> 00:10:51.049
is 28, 56,

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00:10:51.231 --> 00:10:53.610
84. So that's 10 to the 84.

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So that means I would disintegrate in two

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00:10:57.290 --> 00:10:59.930
times 10 to the 67 times 10 to the minus

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84, which is about 10 to the minus 17

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years. So suddenly, a drum t mass black

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hole would disintegrate and evaporate in

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a tiny fraction of the millisecond.

281
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So these primordial mass black holes that

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evaporate are, uh, doing

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so because they're very small. You could, if

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you wanted to. And I'll leave this as an

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exercise to the reader, because me doing

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mental arithmetic is not the most exciting

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thing. You could work out what massive black

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hole would have to be to evaporate

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after 13.8 billion years,

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which is about how old the universe is. The

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reason that's an interesting one is if there

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were any primordial mass black holes of that

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mass and they were to evaporate,

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they will be evaporating in the very near

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universe. And that would make them much

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easier to detect because the intensity of

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radiation we detect is proportional to 1

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00:11:52.310 --> 00:11:54.350
over the square of the distance. So if

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something's twice as far away, it's four

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times fainter. If it's three times as far

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away, it's nine times fainter. So

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I don't know. I'm not a black hole expert by

303
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any means. I say that all the time.

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But if there were a black hole of that mass

305
00:12:08.670 --> 00:12:11.600
formed at the Big Bang, Then maybe

306
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they will be evaporating in the relatively

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local universe, and they're the ones that

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have been most likely to detect. I do not,

309
00:12:18.320 --> 00:12:20.880
however, know what the distribution

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00:12:21.360 --> 00:12:24.160
of masses for primordial black

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holes would be. It's possibly on this

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00:12:25.600 --> 00:12:28.600
Wikipedia page, but have a

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look and find out if it's your kind of thing.

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But hopefully that explains why there's a

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turnover point where things would decay in

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less than the edge of the universe or more

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than the edge of the universe. Uh, and that

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mass is somewhere between the mass of ajonti

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and the mass of the Earth.

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Andrew Dunkley: Okay, fascinating. Yeah. All right, thank

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you, Nick. Uh, and Nick, uh, you might have

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heard us talking a, uh, week or two or

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three or four back, uh, about, uh,

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what they think might be the discovery of a

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primordial black hole. So that's a story

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00:12:57.550 --> 00:12:58.870
worth looking up as well.

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Thanks for your question. This is Space Nuts,

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Q and A edition with Andrew Dunkley and John

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de Horner.

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Jonti Horner: 0G and I feel fine. Space Nuts.

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Andrew Dunkley: Uh, now, Jonti, we've got an audio question

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that comes from a repeat offender.

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Uh, her name's Andrea.

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Andrea: Hi, guys. Got, um, a couple of questions I'm

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hoping you can help me with. Um, the first

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question I have is, um,

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why does the dark side of the Moon

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not have anywhere near as much damage as the

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face of the Moon? Um,

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my second question is,

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um, why are the

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craters so shallow on the moon? Considering

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the size of some of the impact

344
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zones and craters, um, they all seem to be

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the same depth, which is quite shallow, um,

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especially if you look at TAO, which is

347
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3,000 miles wide, um, with an

348
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incredibly shallow crater. Um, if you could

349
00:14:01.380 --> 00:14:04.340
explain for me why that occurs,

350
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that would be absolutely amazing. Thank you

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00:14:07.380 --> 00:14:09.500
very much. Oh, and this is Andrea from

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00:14:09.500 --> 00:14:12.180
Wanneroo and Andrew. Uh, Wanneroo is actually

353
00:14:12.660 --> 00:14:15.500
a noongar, or whadjuk? Noongar. Ah,

354
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people word. Um, that actually

355
00:14:19.460 --> 00:14:22.220
means the area of the

356
00:14:22.220 --> 00:14:25.060
digging stick. Unfortunately, not

357
00:14:25.060 --> 00:14:26.860
pet kangaroo, although I have had one of

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those as well. Thanks, guys. Take care.

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Jonti Horner: Bye.

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Andrew Dunkley: Thanks, Andrea. Lovely to hear from you. I'm

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glad she explained that. Um, you probably

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don't know what she's talking about, Jonti,

363
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but, um, when Andrea last sent us an audio

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question and she said she was from Wanneroo,

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I translated that to an indigenous word

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00:14:42.030 --> 00:14:45.029
meaning, I want a pet kangaroo. So,

367
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yeah, I know I was being silly, but, um, no,

368
00:14:47.630 --> 00:14:50.270
it's, um, place of the digging stick. Didn't

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know that. So, um, of course, the digging

370
00:14:52.510 --> 00:14:55.190
stick was one of the implements, uh, that the

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ancient indigenous peoples of Australia used

372
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to use to, to uh, dig up,

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um, grubs and other, other bush

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tucker as we call it these days.

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Jonti Horner: So it's probably worth mentioning for the

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listeners who are not in Australia that many

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of the Australian places have names

378
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that derive from the languages of the

379
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traditional owners of the land, the

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indigenous people of Australia, who had many

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different countries with many different

382
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language groups. And the origin of the

383
00:15:22.970 --> 00:15:24.970
names is not always that well known or

384
00:15:24.970 --> 00:15:27.950
understood because during the invasion of

385
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Australia and during the events that happened

386
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all the way through to the 1970s, there was a

387
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fairly aggressive attempt to, even if

388
00:15:34.710 --> 00:15:36.350
you weren't wiping out the people, to get rid

389
00:15:36.350 --> 00:15:37.710
of the culture and to get rid of the

390
00:15:37.710 --> 00:15:40.070
knowledge. I've just looked up Toowoomba

391
00:15:40.070 --> 00:15:42.949
where I am T o uh o uh w o uh o uh m b

392
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a I live about 20 ks west of there.

393
00:15:45.310 --> 00:15:47.510
Toowoomba is an indigenous name. It's a

394
00:15:47.510 --> 00:15:49.750
really interesting town because it's like the

395
00:15:49.750 --> 00:15:51.390
Florida of Queensland. All the old people

396
00:15:51.390 --> 00:15:53.820
come here to retire. It's a lovely place.

397
00:15:53.820 --> 00:15:56.660
It's a beautiful place because Queensland has

398
00:15:57.700 --> 00:16:00.620
a particular climate. But Toowoomba is

399
00:16:00.620 --> 00:16:02.300
a moderated version of that climate because

400
00:16:02.300 --> 00:16:04.060
it sits on the Great Dividing range at about

401
00:16:04.060 --> 00:16:06.620
700 meters above sea level. So it's not as

402
00:16:06.620 --> 00:16:08.460
humid as the coast. It doesn't get as hot as

403
00:16:08.460 --> 00:16:10.780
the coast. It has very lovely dry winters.

404
00:16:10.780 --> 00:16:13.380
Anyway, the name of Toowoomba is

405
00:16:13.700 --> 00:16:16.500
probably based on a word

406
00:16:16.500 --> 00:16:19.380
from likely the Gable or Jarawar

407
00:16:19.380 --> 00:16:21.820
peoples. Not entirely sure. But if you look

408
00:16:21.820 --> 00:16:24.730
around for the origin of Toowoomba as a word,

409
00:16:25.440 --> 00:16:27.040
there's lots of suggestions. There is a

410
00:16:27.040 --> 00:16:29.120
suggestion that it was a, ah, word for swamp

411
00:16:29.120 --> 00:16:31.000
because Toowoomba sits in this swampy area on

412
00:16:31.000 --> 00:16:33.200
top of the hills. According to the Toowoomba

413
00:16:33.200 --> 00:16:35.400
Regional Council, it may have been named

414
00:16:35.400 --> 00:16:38.000
after a property in the area in the 1850s,

415
00:16:38.560 --> 00:16:41.160
or it may have come from an Aboriginal word

416
00:16:41.160 --> 00:16:43.000
meaning either place where water sits, which

417
00:16:43.000 --> 00:16:45.680
will be the swamp thing or place of melon, or

418
00:16:45.680 --> 00:16:48.080
place where reeds grow or berries place or

419
00:16:48.080 --> 00:16:50.440
white man. There are other things saying

420
00:16:50.440 --> 00:16:53.050
meeting of the waters or. Or saying. The name

421
00:16:53.050 --> 00:16:54.810
of Toowoomba may be an anglicized version of

422
00:16:54.810 --> 00:16:57.770
the word bu wonga, which meant thunder in

423
00:16:57.770 --> 00:16:59.810
the dialect of the upper Burnett and Gaynda

424
00:16:59.810 --> 00:17:02.770
tribes. So we just don't know. And it does

425
00:17:02.770 --> 00:17:04.210
make me a little bit sad. We talk about

426
00:17:04.210 --> 00:17:06.170
indigenous astronomy a bit and the wonderful

427
00:17:06.170 --> 00:17:08.570
work that, um, Professor Duane Hamaker and

428
00:17:08.570 --> 00:17:10.250
his students have done over the years working

429
00:17:10.250 --> 00:17:12.130
with the indigenous people of Australia. But

430
00:17:12.130 --> 00:17:13.410
it does make me sad how much of this

431
00:17:13.410 --> 00:17:15.010
knowledge is lost where you don't even know

432
00:17:15.010 --> 00:17:16.930
the origin of the name. So it's wonderful

433
00:17:16.930 --> 00:17:19.439
that in this case we actually know where the

434
00:17:19.439 --> 00:17:21.879
name comes from. We can talk to that. So when

435
00:17:21.879 --> 00:17:23.119
you're looking at the map of Australia and

436
00:17:23.119 --> 00:17:25.439
think a lot of the places are unusual from

437
00:17:25.439 --> 00:17:27.639
the perspective of someone from an Anglo

438
00:17:27.639 --> 00:17:29.559
background or from a European background,

439
00:17:29.799 --> 00:17:31.919
it's because even though it's a primarily

440
00:17:31.919 --> 00:17:34.599
English speaking country nowadays with a,

441
00:17:35.159 --> 00:17:38.039
with that, you know, Anglo heritage, a lot of

442
00:17:38.039 --> 00:17:39.519
the names are actually from the traditional

443
00:17:39.519 --> 00:17:42.159
owners, even if the heritage of that name

444
00:17:42.159 --> 00:17:42.999
itself is lost.

445
00:17:43.479 --> 00:17:45.959
Andrew Dunkley: Yes. Uh, where I live, Dubbo is

446
00:17:45.959 --> 00:17:48.599
supposedly a Wiradjuri word for red

447
00:17:48.599 --> 00:17:50.900
earth, because the soil here is red,

448
00:17:51.740 --> 00:17:54.180
uh, which might sound horrifying to people.

449
00:17:54.460 --> 00:17:56.980
Uh, it is when you get a dust storm and

450
00:17:56.980 --> 00:17:58.800
everything turns red, uh,

451
00:17:59.060 --> 00:18:01.700
Jonti Horner: when it gets wet and you're bringing it in

452
00:18:01.700 --> 00:18:03.940
because the red soil marks horrible

453
00:18:03.940 --> 00:18:06.340
everything up, you know. Yeah. Dog goes out

454
00:18:06.340 --> 00:18:08.180
and gets their paws muddy and brings in red

455
00:18:08.180 --> 00:18:08.820
footprints.

456
00:18:09.140 --> 00:18:12.140
Andrew Dunkley: Red footprints on a light colored carpet. No,

457
00:18:12.140 --> 00:18:14.900
uh, terrible stuff. And of course one that

458
00:18:14.900 --> 00:18:17.540
relates to astronomy is warmera,

459
00:18:18.040 --> 00:18:20.680
which is an indigenous word for uh, the,

460
00:18:20.840 --> 00:18:23.800
the implement they used to launch a spear

461
00:18:24.120 --> 00:18:26.080
rather than just throw the spear. They used

462
00:18:26.080 --> 00:18:29.050
to have a specially made, um,

463
00:18:29.720 --> 00:18:32.040
I suppose you'd call it a, like a handheld

464
00:18:32.040 --> 00:18:33.850
catapult. And it, um,

465
00:18:35.240 --> 00:18:37.680
and, and it. Yeah, and it flung the spear at

466
00:18:37.680 --> 00:18:40.240
greater speed and distance. And that's uh, it

467
00:18:40.240 --> 00:18:42.040
was called a woomera. And of course woomera

468
00:18:42.040 --> 00:18:44.850
rocket range is where Australia's, uh,

469
00:18:44.980 --> 00:18:47.740
early space efforts were, uh, were

470
00:18:47.740 --> 00:18:49.660
launched from in South Australia. So yeah,

471
00:18:49.660 --> 00:18:51.940
it's um, fascinating history really is.

472
00:18:51.940 --> 00:18:54.100
Jonti Horner: And um, of course the aquilatl that I

473
00:18:54.100 --> 00:18:55.300
mentioned there, I just double checked

474
00:18:55.300 --> 00:18:57.780
because it's like I remember an aquilateral

475
00:18:57.780 --> 00:18:59.020
being a thing that used for throwing space.

476
00:18:59.020 --> 00:19:00.860
It turns out that that was an Aztec implement

477
00:19:00.860 --> 00:19:02.460
that served the same kind of process. So the

478
00:19:02.460 --> 00:19:04.660
word applatl apparently comes from Aztec.

479
00:19:05.060 --> 00:19:08.060
Andrew Dunkley: Oh, wow. Didn't know that. Back

480
00:19:08.060 --> 00:19:08.940
to you, Andrea.

481
00:19:08.940 --> 00:19:09.380
Jonti Horner: Yes.

482
00:19:10.660 --> 00:19:12.900
Andrew Dunkley: Okay, two questions. Dark side of the moon?

483
00:19:13.370 --> 00:19:16.270
Uh, smoother. Now I've always been aware that

484
00:19:16.430 --> 00:19:18.990
the side we can see is so rugged and

485
00:19:19.230 --> 00:19:20.830
pockmarked and mountainous.

486
00:19:20.910 --> 00:19:21.390
Jonti Horner: Yes.

487
00:19:21.710 --> 00:19:24.090
Andrew Dunkley: But the side that we cannot see that, uh,

488
00:19:24.090 --> 00:19:26.790
Artemis 2 recently had a look at, uh, and

489
00:19:26.790 --> 00:19:28.750
where the Chinese have been running around on

490
00:19:28.750 --> 00:19:31.490
their little scooters. Um,

491
00:19:31.490 --> 00:19:32.830
it's smoother. Why?

492
00:19:33.470 --> 00:19:35.630
Jonti Horner: Well, this is a weird one. So

493
00:19:36.350 --> 00:19:39.350
it looks more uniform when

494
00:19:39.350 --> 00:19:40.950
you look at it. And I'm saying that very

495
00:19:40.950 --> 00:19:42.630
carefully rather than smoother, because

496
00:19:42.630 --> 00:19:45.380
smoother invokes polished or smooth.

497
00:19:45.380 --> 00:19:47.340
Like your skin when you're a kid is a lot

498
00:19:47.340 --> 00:19:48.700
smoother than your skin when you get to my

499
00:19:48.700 --> 00:19:50.100
edge and you've got all the wrinkles right.

500
00:19:50.420 --> 00:19:52.220
Yeah. Um, or the scars.

501
00:19:52.220 --> 00:19:52.820
Andrew Dunkley: See this one?

502
00:19:52.820 --> 00:19:53.220
Jonti Horner: Yeah.

503
00:19:53.540 --> 00:19:56.060
Andrew Dunkley: Uh, that's from a golf club. My neighbor hit

504
00:19:56.060 --> 00:19:58.460
me in the face with a seven iron. Yeah. It

505
00:19:58.460 --> 00:20:00.380
wasn't malicious. It was the backswing. I was

506
00:20:00.380 --> 00:20:01.140
standing too close.

507
00:20:01.140 --> 00:20:02.340
Jonti Horner: I was going to say it sounds like the

508
00:20:02.340 --> 00:20:03.860
adventures you have in double. You know,

509
00:20:04.100 --> 00:20:06.620
something to pass the time. The reason that

510
00:20:06.620 --> 00:20:08.300
I'm being careful in my wording here and

511
00:20:08.300 --> 00:20:10.140
saying it looks more uniform rather than it's

512
00:20:10.140 --> 00:20:12.440
smoother is actually, I don't think it is

513
00:20:12.440 --> 00:20:14.120
smoother, but I think it definitely does look

514
00:20:14.120 --> 00:20:17.000
more uniform on the near side of the

515
00:20:17.000 --> 00:20:18.360
Moon. It should be said that we're talking

516
00:20:18.360 --> 00:20:20.320
near side and far side. The dark side of the

517
00:20:20.320 --> 00:20:21.880
Moon is simply the side of the Moon pointed

518
00:20:21.880 --> 00:20:24.120
away from the Sun. And, um, that rotates

519
00:20:24.120 --> 00:20:25.960
around as the Moon goes around the Earth,

520
00:20:25.960 --> 00:20:27.360
which is why we get the faces right. If

521
00:20:27.360 --> 00:20:29.200
you're stood on the Moon, you'll get at a

522
00:20:29.200 --> 00:20:31.240
given location two weeks of daytime and two

523
00:20:31.240 --> 00:20:33.200
weeks of nighttime. And when it's nighttime

524
00:20:33.200 --> 00:20:34.720
for you, you'd be on the dark side of the

525
00:20:34.720 --> 00:20:36.880
Moon. But when the Moon's new, the dark side

526
00:20:36.880 --> 00:20:38.750
points towards us. The far side of the Moon

527
00:20:39.140 --> 00:20:41.340
always points away from the Earth. Now, on

528
00:20:41.340 --> 00:20:42.900
the near side of the Moon, which is a side

529
00:20:42.900 --> 00:20:45.620
we're familiar with, the view we get is

530
00:20:45.700 --> 00:20:48.660
very non uniform because we've got the

531
00:20:48.660 --> 00:20:51.500
mare and the non mare regions. So the mare

532
00:20:51.500 --> 00:20:53.300
are the seas which make up the man in the

533
00:20:53.300 --> 00:20:55.380
Moon or whatever picture you have, which are

534
00:20:55.380 --> 00:20:57.820
these flood basalt areas. And, um, then

535
00:20:57.820 --> 00:21:00.500
you've got the non mari areas, which are more

536
00:21:00.500 --> 00:21:02.260
traditionally rocky object looking.

537
00:21:03.540 --> 00:21:05.920
Andrew Dunkley: He's the drunk man in the Moon,

538
00:21:06.310 --> 00:21:08.000
uh, here because he's upside down.

539
00:21:08.000 --> 00:21:11.000
Jonti Horner: Absolutely, yeah. Those areas

540
00:21:11.000 --> 00:21:13.420
that make the drunk man are, uh,

541
00:21:13.600 --> 00:21:16.480
flood basalt outpourings on the near side of

542
00:21:16.480 --> 00:21:18.320
the Moon that were formed early in the Moon's

543
00:21:18.320 --> 00:21:20.719
formation. If you ascribe to the idea that

544
00:21:20.719 --> 00:21:22.720
there was a Late Heavy Bombardment when the

545
00:21:22.720 --> 00:21:25.400
impact rate spiked, then they are thought to

546
00:21:25.400 --> 00:21:27.600
have formed there. But in actuality, evidence

547
00:21:27.600 --> 00:21:29.200
for the Late Heavy Bombardment has pretty

548
00:21:29.200 --> 00:21:31.520
much dissipated. So the closer you are to

549
00:21:32.250 --> 00:21:34.410
impact studies and studies of the Moon, the

550
00:21:34.410 --> 00:21:36.330
less strongly you hold to the idea that heavy

551
00:21:36.330 --> 00:21:38.170
bombardment was a thing. But as with all

552
00:21:38.170 --> 00:21:40.170
science, the further you get from a certain

553
00:21:40.170 --> 00:21:41.570
expertise, the more out of date your

554
00:21:41.570 --> 00:21:44.050
knowledge is. So the heavy bombardment is

555
00:21:44.050 --> 00:21:45.970
quite often still viewed as canon in a Lot of

556
00:21:45.970 --> 00:21:47.969
areas, whereas those who are closest to the

557
00:21:47.969 --> 00:21:49.890
topic have a lot more doubt that it ever

558
00:21:49.890 --> 00:21:52.010
happened. But anyway, on the near side of the

559
00:21:52.010 --> 00:21:54.970
Moon, you've got areas

560
00:21:54.970 --> 00:21:57.450
of the Moon that didn't have

561
00:21:57.920 --> 00:22:00.040
Amare, didn't have a flood basalt

562
00:22:00.040 --> 00:22:02.880
outpouring. And, um, you've got areas that

563
00:22:02.880 --> 00:22:04.680
did. And then overlaid on that, you've got

564
00:22:04.680 --> 00:22:06.800
some more recent impacts, which are the rare

565
00:22:06.800 --> 00:22:09.560
craters where you've got weathered material

566
00:22:09.560 --> 00:22:11.320
on the surface that looks darker and an

567
00:22:11.320 --> 00:22:13.160
impact comes along, digs through the darker

568
00:22:13.160 --> 00:22:14.760
material to the unweathered material below

569
00:22:14.760 --> 00:22:17.000
and splashes it across the surface. So the

570
00:22:17.000 --> 00:22:18.920
near side of the Moon looks very non uniform

571
00:22:18.920 --> 00:22:20.960
because you've got that disparity between the

572
00:22:21.120 --> 00:22:24.050
flood basalts and the non flood basalts. And

573
00:22:24.050 --> 00:22:26.210
the non flood basalt is an older surface

574
00:22:26.210 --> 00:22:28.090
because the flood basalt erases the evidence

575
00:22:28.090 --> 00:22:30.570
of what happened before. So there are

576
00:22:30.650 --> 00:22:32.970
slightly fewer impacts on the mare than there

577
00:22:32.970 --> 00:22:35.650
are on the non mare because it's younger

578
00:22:35.650 --> 00:22:38.170
surface. Prior to any

579
00:22:38.170 --> 00:22:39.850
spacecraft going to the Moon, the assumption

580
00:22:39.850 --> 00:22:41.330
was the far side of the Moon would look like

581
00:22:41.330 --> 00:22:43.810
the near side. But when we sent spacecraft

582
00:22:43.810 --> 00:22:45.490
there, we realized it doesn't. And that was a

583
00:22:45.490 --> 00:22:47.250
big puzzle for astronomers for a very long

584
00:22:47.250 --> 00:22:50.050
time in that there were effectively no mare

585
00:22:50.050 --> 00:22:51.970
on the far side. There's little bits, but not

586
00:22:51.970 --> 00:22:54.890
very much. Now, the idea here is

587
00:22:54.890 --> 00:22:57.850
that, uh, when the Moon formed, it formed as

588
00:22:57.850 --> 00:23:00.170
a result of a giant impact on the Earth. The

589
00:23:00.170 --> 00:23:02.170
Moon accreted, uh, and initially was fully

590
00:23:02.170 --> 00:23:03.570
molten and then it cooled from the outside

591
00:23:03.570 --> 00:23:06.530
in. So at a certain time in the Moon's youth,

592
00:23:07.010 --> 00:23:09.650
the surface was very thin above a magma

593
00:23:09.650 --> 00:23:12.170
ocean, above a molten ocean. And at that

594
00:23:12.170 --> 00:23:14.810
time, small impacts wouldn't penetrate that

595
00:23:14.810 --> 00:23:17.130
crust. And you get normal craters, you get

596
00:23:17.130 --> 00:23:18.610
mountain ranges and all the rest of it

597
00:23:18.610 --> 00:23:20.370
forming. But when you got a really big impact

598
00:23:21.010 --> 00:23:23.130
that would break through the crust, create a

599
00:23:23.130 --> 00:23:25.450
big impact basin that would then be flooded

600
00:23:25.450 --> 00:23:27.330
with flood basalt, which gave you this

601
00:23:27.330 --> 00:23:29.810
incredibly flat, smooth floor and

602
00:23:29.810 --> 00:23:31.890
erased all the evidence of the impacts before

603
00:23:32.930 --> 00:23:35.810
eventually the Moon cooled enough that any

604
00:23:35.810 --> 00:23:37.810
molten material was sufficiently deep that

605
00:23:37.810 --> 00:23:40.410
even the biggest impacts would not cause

606
00:23:40.410 --> 00:23:43.210
these flood basalt outpourings. Coupled with

607
00:23:43.210 --> 00:23:46.090
the fact that as the solar system aged,

608
00:23:46.090 --> 00:23:47.850
it cleaned up very effectively and the big

609
00:23:47.850 --> 00:23:49.530
impactors were effectively gone. So the big

610
00:23:49.530 --> 00:23:52.020
impacts were early on. So the idea was that

611
00:23:52.020 --> 00:23:55.020
the mare are caused by the very biggest

612
00:23:55.020 --> 00:23:57.900
impacts that will create impact basins

613
00:23:57.900 --> 00:23:59.620
that are, uh, hundreds or thousands of

614
00:23:59.620 --> 00:24:02.620
kilometres across, that are broadly

615
00:24:02.780 --> 00:24:05.180
circular in shape before other things happen,

616
00:24:05.500 --> 00:24:07.500
and that they're filled with molten material.

617
00:24:08.060 --> 00:24:10.220
And the areas on the near side that are not

618
00:24:10.220 --> 00:24:12.300
in the mare are the areas that were not

619
00:24:12.860 --> 00:24:15.140
induced into one of these flood basalt outpat

620
00:24:15.140 --> 00:24:16.860
rings. Effectively they escaped being in one

621
00:24:16.860 --> 00:24:19.090
of the craters from the very biggest impact

622
00:24:19.090 --> 00:24:22.010
us. We thought that prior

623
00:24:22.010 --> 00:24:23.650
to going to the far side of the Moon, you

624
00:24:23.650 --> 00:24:25.170
would have assumed that the far side would be

625
00:24:25.170 --> 00:24:26.850
the same, but it turns out that it's not.

626
00:24:27.410 --> 00:24:29.490
That was a real problem because this idea

627
00:24:29.490 --> 00:24:31.250
that the impacts were big enough to punch

628
00:24:31.250 --> 00:24:34.210
through and flood to the surface

629
00:24:35.410 --> 00:24:38.210
should work all across the Moon. So why

630
00:24:38.210 --> 00:24:39.650
then do you not get the flood basalt

631
00:24:39.650 --> 00:24:41.330
outpourings on the far side of the Moon?

632
00:24:41.330 --> 00:24:43.850
There are kind of three explanations that

633
00:24:43.850 --> 00:24:46.350
have been put forward for this, the first of

634
00:24:46.350 --> 00:24:49.190
which is, frankly, bunkham. The idea that the

635
00:24:49.190 --> 00:24:50.650
near side of the Moon faced the Earth, uh,

636
00:24:50.790 --> 00:24:52.910
and the Earth, uh, shielded it and so

637
00:24:52.910 --> 00:24:54.990
therefore there'd be more impacts on the far

638
00:24:54.990 --> 00:24:56.470
side. Well, that just kind of

639
00:24:57.830 --> 00:25:00.310
runs counterintuitive. You'd say the far side

640
00:25:00.310 --> 00:25:02.310
experience more hits, it gets more cratering.

641
00:25:02.390 --> 00:25:03.830
Well, I don't believe that from a minute

642
00:25:03.830 --> 00:25:05.270
because the Earth is so small from the Moon's

643
00:25:05.270 --> 00:25:06.870
point of view, it's barely a shield at all.

644
00:25:07.590 --> 00:25:09.790
But if that were the case, surely you'd

645
00:25:09.790 --> 00:25:11.870
expect more mare on the far side because you

646
00:25:11.870 --> 00:25:14.020
get more of these big impacts. So that, to

647
00:25:14.020 --> 00:25:15.620
me, doesn't work. So we can rule that out.

648
00:25:16.420 --> 00:25:19.380
The other answers are, uh, kind of tied

649
00:25:19.380 --> 00:25:22.180
together. But the idea is

650
00:25:22.980 --> 00:25:25.700
that the Moon had a thicker

651
00:25:25.700 --> 00:25:28.300
layer above the molten layer on the far side

652
00:25:28.300 --> 00:25:31.180
of the Moon to the near side. Two

653
00:25:31.180 --> 00:25:33.140
ways you can make that happen. One idea is

654
00:25:33.140 --> 00:25:36.140
that the heat from the young Earth, which

655
00:25:36.140 --> 00:25:37.860
would also have been molten at this time, and

656
00:25:37.860 --> 00:25:39.620
being bigger will keep its heat longer, so

657
00:25:39.620 --> 00:25:42.150
will be molten for longer. The Earth will be

658
00:25:42.150 --> 00:25:44.230
irradiating the Moon. The Moon will be close

659
00:25:44.230 --> 00:25:45.790
to the Earth, uh, when they formed because

660
00:25:45.790 --> 00:25:47.870
it's moved away. Since that

661
00:25:48.110 --> 00:25:50.390
radiative heat would have kept the near side

662
00:25:50.390 --> 00:25:53.110
of the Moon hot for longer, which the molten

663
00:25:53.110 --> 00:25:54.630
material on the surface would have stayed for

664
00:25:54.630 --> 00:25:57.390
longer, but also it would have taken longer

665
00:25:57.390 --> 00:26:00.110
for the crust to thicken on that side. So

666
00:26:00.110 --> 00:26:01.790
therefore the crust on the far side of the

667
00:26:01.790 --> 00:26:03.440
Moon would have formed quicker and, um,

668
00:26:03.440 --> 00:26:06.310
thicker. The other idea is that, ah, you

669
00:26:06.310 --> 00:26:08.350
get the same kind of effect from tidal forces

670
00:26:08.860 --> 00:26:10.620
that the tidal influence of the Earth on the

671
00:26:10.620 --> 00:26:11.980
Moon is stronger on the near side than the

672
00:26:11.980 --> 00:26:14.540
far side because the strength of tides falls

673
00:26:14.540 --> 00:26:16.460
off as distance to the power four. So that's

674
00:26:16.460 --> 00:26:19.100
a very strong, very rapid effect. Yeah,

675
00:26:19.260 --> 00:26:21.580
possibly both of those things combine

676
00:26:22.220 --> 00:26:24.260
give you a crust around the Moon that is

677
00:26:24.260 --> 00:26:26.460
thinner on the near side than the far side at

678
00:26:26.460 --> 00:26:28.300
all times as, ah, the Moon cools on the

679
00:26:28.300 --> 00:26:30.540
interior. Which means that

680
00:26:31.100 --> 00:26:33.700
the far side of the moon, the molten

681
00:26:33.700 --> 00:26:36.140
material was deeply enough buried quickly

682
00:26:36.140 --> 00:26:38.970
enough that no Maori forming impact happened.

683
00:26:38.970 --> 00:26:40.730
You've got the South Pole Ait Kin basin,

684
00:26:40.730 --> 00:26:42.690
which is the biggest impact scar on the Moon,

685
00:26:43.010 --> 00:26:44.930
doesn't really have much flood basalt in it,

686
00:26:44.930 --> 00:26:47.690
which either means that it is younger and

687
00:26:47.690 --> 00:26:50.130
therefore, uh, the interior had cooled enough

688
00:26:50.130 --> 00:26:53.009
that it didn't crack that egg or

689
00:26:53.570 --> 00:26:56.370
that it was an area where the crust

690
00:26:56.370 --> 00:26:59.130
was thicker anyway, you know, so the idea is

691
00:26:59.130 --> 00:27:00.850
that the difference between the near side and

692
00:27:00.850 --> 00:27:02.290
the far side of the Moon is down to the

693
00:27:02.290 --> 00:27:03.840
thickness of the crust when the biggest

694
00:27:03.840 --> 00:27:06.440
impacts were happening. And the idea that

695
00:27:06.440 --> 00:27:08.320
probably due to a combination of tidal

696
00:27:08.320 --> 00:27:10.560
effects and radiative heating from the

697
00:27:10.560 --> 00:27:13.240
incredibly luminous molten Earth, the

698
00:27:13.320 --> 00:27:15.560
near side of the Moon stayed a thicker shell

699
00:27:15.800 --> 00:27:17.960
and therefore was more effectively punctured.

700
00:27:18.200 --> 00:27:20.480
And so the near side got the mare and the far

701
00:27:20.480 --> 00:27:22.360
side looks more like your typical rocky

702
00:27:22.360 --> 00:27:25.280
objects like Mercury, like a lot of the rocky

703
00:27:25.280 --> 00:27:26.840
moons and stuff like that in the outer solar

704
00:27:26.840 --> 00:27:29.800
system. That's the thinking there. But it is

705
00:27:29.800 --> 00:27:32.120
really strikingly obvious when you see photos

706
00:27:32.120 --> 00:27:34.230
of the far side side of the Moon and you're

707
00:27:34.230 --> 00:27:35.750
not told it's the far side of the Moon, you

708
00:27:35.750 --> 00:27:37.510
assume you're looking at an object that is

709
00:27:37.510 --> 00:27:39.590
not the Moon because it's not different to

710
00:27:39.590 --> 00:27:40.750
our experience of the Moon.

711
00:27:41.150 --> 00:27:41.710
Andrew Dunkley: Indeed.

712
00:27:41.870 --> 00:27:44.030
So, so part two of your question, you

713
00:27:44.030 --> 00:27:46.150
basically covered because of the deep

714
00:27:46.150 --> 00:27:49.030
Jonti Horner: impact a little bit. Part two is a bit

715
00:27:49.030 --> 00:27:50.070
more complex.

716
00:27:50.070 --> 00:27:51.910
Andrew Dunkley: This is about, this is the one about shallow

717
00:27:51.910 --> 00:27:52.430
craters.

718
00:27:53.550 --> 00:27:56.190
Jonti Horner: And craters are uh, shallow, not just on the

719
00:27:56.190 --> 00:27:58.070
Moon, but everywhere. There is a boundary

720
00:27:58.070 --> 00:28:00.070
between what, what researchers describe as a

721
00:28:00.070 --> 00:28:02.870
simple creator and a complex crater. The

722
00:28:02.870 --> 00:28:05.550
size at which you get that boundary varies

723
00:28:05.550 --> 00:28:07.630
dependent on the strength of material that's

724
00:28:07.630 --> 00:28:10.550
impacted and also the mass of the planet and

725
00:28:10.550 --> 00:28:12.390
therefore the strength of gravity. So I

726
00:28:12.390 --> 00:28:14.709
believe on the Earth it's about 8 or 9

727
00:28:14.709 --> 00:28:16.590
kilometers. For the moon it's about 18

728
00:28:16.590 --> 00:28:19.590
kilometers smaller than that. You get

729
00:28:19.590 --> 00:28:21.470
a simple crater that forms, which looks very

730
00:28:21.470 --> 00:28:23.310
similar to what you'd get if you almost just

731
00:28:23.390 --> 00:28:26.350
threw a rock really hard into sand or

732
00:28:26.350 --> 00:28:28.070
something. You get the typical bowl shaped

733
00:28:28.070 --> 00:28:30.310
crater like Meteor Crater in Arizona. Really

734
00:28:30.310 --> 00:28:33.110
nice example. Yeah, ah, a

735
00:28:33.110 --> 00:28:36.030
size above about like say 8 or 9 kilometers

736
00:28:36.030 --> 00:28:38.670
on Earth or above about 20 kilometers on the

737
00:28:38.670 --> 00:28:40.830
moon. You get to the domain where you get a

738
00:28:40.830 --> 00:28:42.790
complex crater. And complex craters are

739
00:28:42.790 --> 00:28:45.590
characterized by having quite often central

740
00:28:45.750 --> 00:28:48.670
impact peaks, but also having

741
00:28:48.670 --> 00:28:51.550
these much shallower depths compared to

742
00:28:51.550 --> 00:28:54.260
their width, you know, and it's particularly

743
00:28:54.260 --> 00:28:55.620
true for the mare, where they're flood

744
00:28:55.620 --> 00:28:58.540
basalts, where you have a very shallow crater

745
00:28:58.540 --> 00:29:00.860
for the width of the crater. But it's true

746
00:29:00.860 --> 00:29:02.860
even if you look at 20 kilometer craters on

747
00:29:02.860 --> 00:29:04.820
the moon and there's a beautiful photo,

748
00:29:04.820 --> 00:29:06.500
incidentally, if you look on some of the NASA

749
00:29:06.500 --> 00:29:08.139
images, there's a beautiful photo of the

750
00:29:08.139 --> 00:29:10.700
crater Aristarchus taken by the Lunar

751
00:29:10.700 --> 00:29:12.860
Reconnaissance Orbiter, and that shows this

752
00:29:12.860 --> 00:29:15.180
kind of terracing around the walls, the

753
00:29:15.180 --> 00:29:16.980
central peaks. And so there's a few things

754
00:29:16.980 --> 00:29:19.800
going on here that contribute to why what

755
00:29:19.800 --> 00:29:21.480
we describe as being,

756
00:29:22.560 --> 00:29:25.440
um, what I say, complex craters are

757
00:29:25.440 --> 00:29:25.800
actually,

758
00:29:26.960 --> 00:29:29.840
um, shallower compared to

759
00:29:29.840 --> 00:29:31.840
their width than the simple ones. And, uh,

760
00:29:31.840 --> 00:29:33.280
there's a few things that have been suggested

761
00:29:33.280 --> 00:29:36.080
to this. So complex craters have depths that

762
00:29:36.080 --> 00:29:38.520
can be a 15th, a 25th or even less

763
00:29:38.920 --> 00:29:41.400
of the crater width, which looks very, very

764
00:29:41.400 --> 00:29:44.120
shallow. Now, there's a few things proposed

765
00:29:44.120 --> 00:29:47.080
in for this. Firstly, when you form a bigger

766
00:29:47.080 --> 00:29:49.640
crater, uh, the walls can slump in, so

767
00:29:49.640 --> 00:29:52.560
material slides and gradually you get this

768
00:29:53.040 --> 00:29:54.800
material from the edges sliding into the

769
00:29:54.800 --> 00:29:56.040
middle. And if you look at that photo of

770
00:29:56.040 --> 00:29:58.240
Arisarcus, it looks very much like that's

771
00:29:58.240 --> 00:30:01.240
happened. You see evidence of landslides that

772
00:30:01.240 --> 00:30:02.880
have filled in the crater and made it

773
00:30:02.880 --> 00:30:05.880
shallower. The other thing is craters

774
00:30:05.880 --> 00:30:08.600
that big are, ah, large enough to render the

775
00:30:08.600 --> 00:30:11.420
material, where the impact happens, molten.

776
00:30:12.290 --> 00:30:14.050
And in other words, the material can flow

777
00:30:14.050 --> 00:30:16.010
like a liquid rather than behaving like a

778
00:30:16.010 --> 00:30:17.490
solid material of your desk.

779
00:30:17.650 --> 00:30:20.090
Andrew Dunkley: Well, you can still see a rebound point in

780
00:30:20.090 --> 00:30:21.250
the middle of the crater too.

781
00:30:21.250 --> 00:30:23.610
Jonti Horner: That's it. So the stuff at the middle, the

782
00:30:23.610 --> 00:30:25.250
central peaks, are thought to be rebound of

783
00:30:25.250 --> 00:30:28.010
this fluid material springing back before it

784
00:30:28.010 --> 00:30:30.390
freezes solid again effectively. And, um,

785
00:30:30.410 --> 00:30:32.570
then the flat base of these craters that

786
00:30:32.570 --> 00:30:34.690
makes them shallower is because you make a

787
00:30:34.690 --> 00:30:37.250
pool of liquid that spreads out and settles.

788
00:30:38.550 --> 00:30:40.230
And so therefore you get these shower things,

789
00:30:40.230 --> 00:30:43.110
whereas with smaller craters you don't get to

790
00:30:43.110 --> 00:30:45.670
that point. So you get much more material

791
00:30:45.670 --> 00:30:47.670
behaving more as a solid than a liquid,

792
00:30:47.750 --> 00:30:49.990
effectively. So the thinking is for these

793
00:30:49.990 --> 00:30:51.510
complex craters, and like I said for the

794
00:30:51.510 --> 00:30:53.789
moon, I think the size scale is what, 18 to

795
00:30:53.789 --> 00:30:56.350
20 kilometers, something like that. It's a

796
00:30:56.350 --> 00:30:58.030
point at which you transition from simply

797
00:30:58.030 --> 00:31:00.590
behaving as a solid to the surface behaving

798
00:31:00.590 --> 00:31:03.270
in more of a liquid fashion, you get

799
00:31:03.580 --> 00:31:05.620
complex craters having central peaks, they

800
00:31:05.620 --> 00:31:08.500
have terraces, they've got flat floors. The

801
00:31:08.500 --> 00:31:10.860
more massive the object, the smaller the

802
00:31:10.860 --> 00:31:13.820
boundary is, because gravity has a

803
00:31:13.820 --> 00:31:14.540
role in this.

804
00:31:15.020 --> 00:31:15.580
Andrew Dunkley: Yeah.

805
00:31:15.690 --> 00:31:18.300
Jonti Horner: Um, and then you get the basins which are

806
00:31:18.300 --> 00:31:19.940
even bigger and there where you get the

807
00:31:19.940 --> 00:31:22.100
flooding from basalts, which makes them even

808
00:31:22.100 --> 00:31:24.660
shallower compared to their width. So there

809
00:31:24.660 --> 00:31:27.340
is some beautiful complexity of this

810
00:31:28.060 --> 00:31:30.220
where it's all to do with the physical

811
00:31:30.540 --> 00:31:33.260
behavior of material and how that

812
00:31:33.260 --> 00:31:35.260
changes as an impact gets larger and larger

813
00:31:35.260 --> 00:31:37.620
and therefore more and more damaging and

814
00:31:37.620 --> 00:31:40.620
energetic. Now, NASA have a Mars Ed

815
00:31:40.620 --> 00:31:43.020
website, um, where they actually

816
00:31:43.020 --> 00:31:45.460
explicitly say, if you Google for this, it's

817
00:31:45.460 --> 00:31:48.379
marsed Asu. Edu and then

818
00:31:48.379 --> 00:31:50.460
a really long string afterwards. It's a Mars

819
00:31:50.460 --> 00:31:52.340
education thing at Arizona State University.

820
00:31:52.820 --> 00:31:54.580
And I'll just quote here.

821
00:31:55.540 --> 00:31:58.380
Compared to simple craters, complex craters

822
00:31:58.380 --> 00:32:01.040
also generate a lot more impact. Melted

823
00:32:01.040 --> 00:32:03.640
rock, this typically flows and pools like

824
00:32:03.640 --> 00:32:05.880
lava to form a sheet that covers a shattered

825
00:32:05.880 --> 00:32:08.360
rock known as breccia. On the crater floor,

826
00:32:08.760 --> 00:32:11.160
the crater's inner walls may slump downwards,

827
00:32:11.240 --> 00:32:13.600
rotating backwards in blocks, which can widen

828
00:32:13.600 --> 00:32:15.640
the crater's rim and line the inner walls

829
00:32:15.640 --> 00:32:18.040
with terraces. But as a result, complex

830
00:32:18.040 --> 00:32:19.680
craters look shallow. Uh, they have rim

831
00:32:19.680 --> 00:32:21.760
diameters about 30 times greater than their

832
00:32:21.760 --> 00:32:24.240
depths. By comparison, simple craters are

833
00:32:24.240 --> 00:32:26.120
about five times wider than they are deep.

834
00:32:26.910 --> 00:32:28.470
Um, earlier on it said the more energy and

835
00:32:28.470 --> 00:32:30.310
impact delivers, the bigger the cavity on the

836
00:32:30.310 --> 00:32:32.470
ground. But immediately after the blast, the

837
00:32:32.470 --> 00:32:34.590
center of the cavity begins to rise as rocks

838
00:32:34.590 --> 00:32:36.150
rebound from the shock. That's what gives you

839
00:32:36.150 --> 00:32:38.190
the mountains. This uplift gives you a

840
00:32:38.190 --> 00:32:40.670
central peak or cluster of peaks. So that's a

841
00:32:40.670 --> 00:32:42.630
really nice way of condensing my lengthy,

842
00:32:42.630 --> 00:32:45.350
waffly answer into something a bit more

843
00:32:45.350 --> 00:32:46.270
simple and straightforward.

844
00:32:47.150 --> 00:32:49.790
Andrew Dunkley: Fair enough. Okay, uh, now, Andrea, you can

845
00:32:49.790 --> 00:32:51.870
believe all of that, or you can go with my

846
00:32:51.870 --> 00:32:53.930
theory that the lunar city council were on

847
00:32:54.240 --> 00:32:56.080
strike and they didn't finish filling the

848
00:32:56.080 --> 00:32:56.720
potholes.

849
00:32:58.720 --> 00:33:01.530
I go with option two. Um,

850
00:33:01.530 --> 00:33:03.080
Andrea, thanks for your question. Great to

851
00:33:03.080 --> 00:33:04.400
hear from you. Thanks for explaining

852
00:33:04.400 --> 00:33:05.200
Wanneroo.

853
00:33:05.440 --> 00:33:07.800
This is Space Nuts, a Q and A edition with

854
00:33:07.800 --> 00:33:10.800
Professor Jonti Horner and Andrew Dunkley.

855
00:33:13.280 --> 00:33:15.320
Okay, Houston, we've had a problem here. This

856
00:33:15.320 --> 00:33:17.680
is Houston. Say again, please. Houston, we've

857
00:33:17.680 --> 00:33:19.240
had a problem. Is that a main B plus

858
00:33:19.240 --> 00:33:21.320
undervolt? Roger, main B undervolt. Okay,

859
00:33:21.320 --> 00:33:22.880
standby 13. We're looking at it.

860
00:33:23.130 --> 00:33:23.850
Jonti Horner: These butts.

861
00:33:25.210 --> 00:33:27.450
Andrew Dunkley: Our, uh, last question comes, uh, in two

862
00:33:27.450 --> 00:33:30.280
parts, and it comes, uh, from Eli. Uh,

863
00:33:30.280 --> 00:33:32.770
hello from Coachella Valley in

864
00:33:32.770 --> 00:33:34.970
California. Was Coachella in the news

865
00:33:34.970 --> 00:33:37.970
recently for some big soiree that happened

866
00:33:37.970 --> 00:33:40.970
there? Yeah, uh, big event. Uh, anyway, he

867
00:33:40.970 --> 00:33:43.090
says the grasshoppers have decided to invade.

868
00:33:43.090 --> 00:33:45.570
Believe it or not, Eli, exactly the same

869
00:33:45.570 --> 00:33:48.090
thing is happening where I am. We have

870
00:33:48.410 --> 00:33:50.490
locust, uh, plagues. Once in a blue moon. And

871
00:33:50.490 --> 00:33:53.130
we Had a little one recently. Wasn't, uh, too

872
00:33:53.130 --> 00:33:55.750
significant. But I have discovered with

873
00:33:55.910 --> 00:33:57.950
locusts, or grasshoppers or whatever you call

874
00:33:57.950 --> 00:34:00.630
them wherever you are, that if you drive

875
00:34:00.870 --> 00:34:03.510
over 50 kilometers an hour, they splatter.

876
00:34:04.320 --> 00:34:06.910
Uh, if you drive under 50 kilometers an hour,

877
00:34:06.910 --> 00:34:09.430
they bounce off. Important safety tip.

878
00:34:09.430 --> 00:34:12.150
Especially because when they splatter, they

879
00:34:12.150 --> 00:34:14.590
stink and it's very hard to get off when

880
00:34:14.590 --> 00:34:15.110
they're dry.

881
00:34:15.110 --> 00:34:17.550
Jonti Horner: I'd love to have a swapsy where we've had an

882
00:34:17.550 --> 00:34:19.670
incredibly dry last few months here. It's

883
00:34:19.670 --> 00:34:21.590
been our wet season. We've had 40 mil of rain

884
00:34:21.590 --> 00:34:24.450
in four months. Months, wow. Which is hooray,

885
00:34:24.450 --> 00:34:25.930
you know, that's really what you want in your

886
00:34:25.930 --> 00:34:27.530
wet season when the dry season is about to

887
00:34:27.530 --> 00:34:29.410
start. But what that means is that we're

888
00:34:29.410 --> 00:34:31.090
probably going to see yet another mouse

889
00:34:31.090 --> 00:34:33.170
plague. And mouse plagues are sad because in

890
00:34:33.170 --> 00:34:34.930
the times that are good, mice reproduce like

891
00:34:34.930 --> 00:34:37.450
crazy. But then you get the boom busting and

892
00:34:37.450 --> 00:34:39.130
so you start getting lots of them coming to

893
00:34:39.130 --> 00:34:41.250
your house. And I'm soft hearted. I don't

894
00:34:41.250 --> 00:34:43.010
want to hurt them or do anything, but at the

895
00:34:43.010 --> 00:34:44.370
same time, I don't want them pooing on

896
00:34:44.370 --> 00:34:46.370
everything in my kitchen. Yeah. So we're

897
00:34:46.370 --> 00:34:49.070
getting mouth plague times. Uh, I, I, I

898
00:34:49.070 --> 00:34:51.350
suspect that locust plagues are horrible, but

899
00:34:51.350 --> 00:34:53.350
mouse plague is an entirely different horror.

900
00:34:53.350 --> 00:34:54.710
Andrew Dunkley: And mouse plagues are worse.

901
00:34:54.870 --> 00:34:55.270
Jonti Horner: Yeah.

902
00:34:55.270 --> 00:34:57.830
Andrew Dunkley: Because the mice try to find somewhere to

903
00:34:57.830 --> 00:35:00.710
hide inside. Locusts only get in if they've

904
00:35:00.870 --> 00:35:03.310
got an open avenue, otherwise they just stay

905
00:35:03.310 --> 00:35:06.230
outside. And you, you know. And they also are

906
00:35:06.230 --> 00:35:08.790
very disturbing when you're trying to putt on

907
00:35:08.790 --> 00:35:09.350
a golf cart.

908
00:35:09.350 --> 00:35:10.310
Jonti Horner: Oh, absolutely.

909
00:35:10.550 --> 00:35:11.670
Andrew Dunkley: It's getting away.

910
00:35:11.910 --> 00:35:12.710
Jonti Horner: They must see.

911
00:35:12.950 --> 00:35:13.430
Andrew Dunkley: Sorry.

912
00:35:13.780 --> 00:35:15.340
Jonti Horner: You walk into the kitchen at night or you

913
00:35:15.340 --> 00:35:16.500
walk somewhere and you just see something

914
00:35:16.500 --> 00:35:18.660
move in the periphery, and that's always a

915
00:35:18.660 --> 00:35:21.500
little disturbing. Yeah, well, uh, we, yeah,

916
00:35:21.500 --> 00:35:21.980
we talk,

917
00:35:21.980 --> 00:35:24.060
Andrew Dunkley: we're talking mouse plague here as well. So

918
00:35:24.060 --> 00:35:26.700
we could have, we could have both. But our

919
00:35:26.700 --> 00:35:29.500
last big locust plague, it was so

920
00:35:29.500 --> 00:35:31.260
big, the birds just got fed up with eating

921
00:35:31.260 --> 00:35:33.220
them, so they gave up as well.

922
00:35:33.220 --> 00:35:34.260
Jonti Horner: It's very weird.

923
00:35:35.040 --> 00:35:37.500
Andrew Dunkley: Um, Eli, what are you asking us? Uh, since

924
00:35:37.500 --> 00:35:40.420
you mentioned a paucity of questions,

925
00:35:40.420 --> 00:35:43.300
I hope you don't mind, um, a

926
00:35:43.300 --> 00:35:43.780
twofer.

927
00:35:43.780 --> 00:35:46.380
Okay, well, we've got two questions then. Uh,

928
00:35:46.380 --> 00:35:48.420
when the solar system formed, I always

929
00:35:48.420 --> 00:35:51.420
imagined the inner rockier planets as having

930
00:35:51.420 --> 00:35:53.380
more heavier elements due to their greater

931
00:35:53.380 --> 00:35:55.820
mass and gravity, and with lighter elements

932
00:35:56.220 --> 00:35:59.100
collecting more in the outer gas giants.

933
00:35:59.100 --> 00:36:01.860
But then I realized, isn't the sun mostly

934
00:36:01.860 --> 00:36:04.700
hydrogen the lightest element? Now I'm

935
00:36:04.700 --> 00:36:06.700
Confused. That's his first question.

936
00:36:06.780 --> 00:36:07.260
Jonti Horner: Yeah.

937
00:36:08.140 --> 00:36:10.850
Andrew Dunkley: This is your bullpen, isn't it? This is your

938
00:36:10.850 --> 00:36:11.850
area of expertise.

939
00:36:11.850 --> 00:36:14.050
Jonti Horner: This is much more my comfort zone. So this is

940
00:36:14.770 --> 00:36:15.130
really.

941
00:36:15.130 --> 00:36:16.930
Andrew Dunkley: I hope you realize I did try to find

942
00:36:16.930 --> 00:36:18.370
questions that worked for you.

943
00:36:18.370 --> 00:36:20.650
Jonti Horner: No, no, that's all good. And it means you can

944
00:36:20.650 --> 00:36:22.450
leave the cosmology ones for when Fred gets

945
00:36:22.450 --> 00:36:23.410
back as well, which is great.

946
00:36:24.210 --> 00:36:26.610
This is a lovely question. And it speaks to

947
00:36:26.930 --> 00:36:29.050
how our understanding of how planets form has

948
00:36:29.050 --> 00:36:31.530
changed over time. And we've now got quite a

949
00:36:31.530 --> 00:36:34.490
high level of complexity in the ideas we have

950
00:36:34.490 --> 00:36:36.170
behind planet formation. But a really

951
00:36:36.170 --> 00:36:39.000
fundamental part of it is that everything

952
00:36:39.320 --> 00:36:41.880
in the solar system to first order

953
00:36:42.280 --> 00:36:45.000
has the same composition as the sun, because

954
00:36:45.000 --> 00:36:46.400
we're all formed from the same material,

955
00:36:46.400 --> 00:36:48.240
formed from an enormous cloud of gas and dust

956
00:36:48.240 --> 00:36:50.720
called a giant molecular cloud that collapsed

957
00:36:50.720 --> 00:36:53.040
under its own gravity. You got effectively

958
00:36:53.040 --> 00:36:55.040
the protostarsome forming in the middle with

959
00:36:55.040 --> 00:36:56.760
a disk of material around it we call a

960
00:36:56.760 --> 00:36:59.640
protoplanetary disk. And in that disk you

961
00:36:59.640 --> 00:37:02.040
have solid material and gaseous

962
00:37:02.040 --> 00:37:04.880
material going around the sun, orbiting the

963
00:37:04.880 --> 00:37:06.740
sun, collapsing to a disk because of the

964
00:37:06.740 --> 00:37:08.580
conservation of angular momentum. So kind of

965
00:37:08.580 --> 00:37:10.740
where the Earth is, material was whizzing

966
00:37:10.740 --> 00:37:13.660
around at about 30 kilometers a second. But

967
00:37:13.660 --> 00:37:15.580
individual dust grains that were next to each

968
00:37:15.580 --> 00:37:17.700
other were both moving at about the same

969
00:37:17.700 --> 00:37:20.580
speed. So very little difference in speed

970
00:37:20.580 --> 00:37:22.020
between the particles, even though they're

971
00:37:22.020 --> 00:37:24.740
going really quickly. Now, the further you

972
00:37:24.740 --> 00:37:26.820
are from the sun, the colder the temperature

973
00:37:26.820 --> 00:37:29.780
is in that disk. And every single material

974
00:37:29.780 --> 00:37:31.960
you can think of has a

975
00:37:32.120 --> 00:37:34.920
sublimation temperature. Below that

976
00:37:34.920 --> 00:37:37.120
temperature it will be solid, and above that

977
00:37:37.120 --> 00:37:39.480
temperature it will be gas. Reason I'm not

978
00:37:39.480 --> 00:37:41.080
talking about liquid is in order to have

979
00:37:41.080 --> 00:37:43.240
liquid you need pressure. And in this case

980
00:37:43.240 --> 00:37:45.000
you don't have any or you don't have enough

981
00:37:45.160 --> 00:37:46.680
to either have solid or gas.

982
00:37:47.079 --> 00:37:47.559
Andrew Dunkley: Yep.

983
00:37:47.880 --> 00:37:50.800
Jonti Horner: If you are gas, then you

984
00:37:50.800 --> 00:37:52.720
don't form planets initially. If you're

985
00:37:52.720 --> 00:37:55.280
solid, you can do. So what happens all

986
00:37:55.280 --> 00:37:57.680
through this disk? For a variety of different

987
00:37:57.680 --> 00:38:00.000
bits of physics going on, you get whatever

988
00:38:00.000 --> 00:38:01.880
solid material you have at that distance

989
00:38:02.540 --> 00:38:05.340
colliding, sticking together, forming

990
00:38:05.340 --> 00:38:07.980
bigger bits. And so you get from millimeter

991
00:38:07.980 --> 00:38:10.620
to meter to kilometer to planet sized

992
00:38:10.700 --> 00:38:13.340
bits of debris. As you get bigger,

993
00:38:13.340 --> 00:38:16.220
gravity can start taking on a role and start

994
00:38:16.220 --> 00:38:17.620
pulling in a bit of extra stuff so you can

995
00:38:17.620 --> 00:38:19.500
feed quicker. Plus if you're bigger, you've

996
00:38:19.500 --> 00:38:21.220
got a bigger cross section, so you hit more

997
00:38:21.220 --> 00:38:23.260
things to devour them. So you get this

998
00:38:23.260 --> 00:38:25.060
process where you get lots of small things,

999
00:38:25.060 --> 00:38:26.820
making a few bigger things, and the big ones

1000
00:38:26.820 --> 00:38:29.720
tend to dominate um, so a thing called

1001
00:38:29.720 --> 00:38:32.360
oligarchic growth is the idea. And you form

1002
00:38:32.360 --> 00:38:34.290
planetesimals, and then oligarchs, which are,

1003
00:38:34.290 --> 00:38:37.160
uh, protoplanets, and a few of them collide

1004
00:38:37.240 --> 00:38:40.040
all the rest of it. If you are far

1005
00:38:40.040 --> 00:38:42.560
enough from the sun, you're beyond what's

1006
00:38:42.560 --> 00:38:45.200
known as the water ice line. Now, that's the

1007
00:38:45.200 --> 00:38:47.600
point at which the temperature is below the

1008
00:38:47.600 --> 00:38:49.800
sublimation point of water. So instead of

1009
00:38:49.800 --> 00:38:52.200
water being a gas or vapor, it's a solid.

1010
00:38:52.840 --> 00:38:54.600
Now, we always imagine water being quite

1011
00:38:54.600 --> 00:38:56.000
scarce. And I just said we've had 40

1012
00:38:56.000 --> 00:38:57.750
millimeters of rain in the last four months.

1013
00:38:58.090 --> 00:39:00.860
Uh, water is very scarce here. But in terms

1014
00:39:00.860 --> 00:39:03.020
of compounds in the universe, water is one of

1015
00:39:03.020 --> 00:39:05.420
the most abundant things there is because

1016
00:39:05.420 --> 00:39:07.300
it's a combination of hydrogen, which is the

1017
00:39:07.300 --> 00:39:09.940
most common atom with 74, 75% of all

1018
00:39:09.940 --> 00:39:12.300
atoms, and oxygen, which is the second most

1019
00:39:12.300 --> 00:39:15.260
common atom with about 1% of all atoms. Put

1020
00:39:15.260 --> 00:39:17.100
hydrogen, oxygen together, and you get water.

1021
00:39:17.660 --> 00:39:19.980
So in the protoplanetary disk around the sun,

1022
00:39:20.220 --> 00:39:23.180
water was probably about the most

1023
00:39:23.180 --> 00:39:25.180
common species other than molecular hydrogen,

1024
00:39:25.180 --> 00:39:27.330
molecular and helium atoms.

1025
00:39:27.970 --> 00:39:29.890
Lots and lots of water. Now, where the Earth

1026
00:39:29.890 --> 00:39:32.810
formed, it was too hot. So you don't

1027
00:39:32.810 --> 00:39:35.170
have water as a solid, so you form the Earth

1028
00:39:35.170 --> 00:39:38.090
dry. There's no solid water to accrete. You

1029
00:39:38.090 --> 00:39:40.490
might get a little bit of water as a gas that

1030
00:39:40.490 --> 00:39:43.450
is trapped in the solid material, which is

1031
00:39:43.450 --> 00:39:45.170
why people think most of the Earth's water

1032
00:39:45.170 --> 00:39:46.770
was delivered from further out. Because if

1033
00:39:46.770 --> 00:39:49.770
far enough out, you form from primarily water

1034
00:39:49.770 --> 00:39:52.570
with everything else added in. So the inner

1035
00:39:52.570 --> 00:39:55.160
solar system, you don't have that water to

1036
00:39:55.160 --> 00:39:57.080
accrete. So you're limited to the things that

1037
00:39:57.080 --> 00:39:59.920
are solid at, uh, higher temperatures. So

1038
00:39:59.920 --> 00:40:01.920
you're limited to accreting from rock and

1039
00:40:01.920 --> 00:40:04.800
metal. So you get telluric planets, or

1040
00:40:04.800 --> 00:40:06.440
is the archaic way of saying it, or

1041
00:40:06.440 --> 00:40:09.120
terrestrial planets beyond the ice line.

1042
00:40:09.439 --> 00:40:12.240
Water ice dominates the solid material. So

1043
00:40:12.240 --> 00:40:14.040
you've got a lot more to feed from, so you

1044
00:40:14.040 --> 00:40:16.440
grow more quickly, and you can get more

1045
00:40:16.440 --> 00:40:17.960
massive planets more quickly, which is where

1046
00:40:17.960 --> 00:40:20.240
Jupiter and Saturn come in. Now, there's a

1047
00:40:20.240 --> 00:40:21.960
lot of discussion about how they may have

1048
00:40:21.960 --> 00:40:23.960
migrated through the nebula, all the rest of

1049
00:40:23.960 --> 00:40:26.200
it, and the subtleties of the formation in

1050
00:40:26.200 --> 00:40:28.360
other planetary systems. We have planets like

1051
00:40:28.360 --> 00:40:30.120
Jupiter orbiting their stars every four or

1052
00:40:30.120 --> 00:40:32.120
five hours even, but we don't think they

1053
00:40:32.120 --> 00:40:34.480
formed there. We think they migrated in. So

1054
00:40:34.480 --> 00:40:37.120
you form beyond the ice line

1055
00:40:37.200 --> 00:40:39.760
more quickly because you've got more food,

1056
00:40:39.760 --> 00:40:42.240
and you can grow to masses like 10 or 12.

1057
00:40:42.240 --> 00:40:44.760
Earth matters while there is still an

1058
00:40:44.760 --> 00:40:47.710
Abundance of gas around. That gas doesn't

1059
00:40:47.710 --> 00:40:49.550
hang around long because once the sun fully

1060
00:40:49.550 --> 00:40:51.870
turns on after a few million years, it blows

1061
00:40:51.870 --> 00:40:53.950
the dust and the gas away and you're left

1062
00:40:53.950 --> 00:40:56.630
with what, whatever's left over. But if you

1063
00:40:56.630 --> 00:40:59.030
form to be 10 or 12 earth masses

1064
00:40:59.750 --> 00:41:01.910
before the gas is blown away, suddenly your

1065
00:41:01.990 --> 00:41:04.510
gravitational ah, pull is strong enough to

1066
00:41:04.510 --> 00:41:06.830
hold on to hydrogen and helium. If you're

1067
00:41:06.830 --> 00:41:09.190
less massive than that, then the escape

1068
00:41:09.190 --> 00:41:11.430
velocity of a hydrogen or helium atom will be

1069
00:41:11.510 --> 00:41:14.430
higher. Sorry, the escape velocity of

1070
00:41:14.430 --> 00:41:17.270
your object with that mass will be lower than

1071
00:41:17.270 --> 00:41:19.470
the speed at which hydrogen and helium atoms

1072
00:41:19.470 --> 00:41:21.710
move at that temperature. So you can't hold

1073
00:41:21.710 --> 00:41:23.590
on to them, they just escape because of their

1074
00:41:23.830 --> 00:41:25.550
motion, because of the temperature they're

1075
00:41:25.550 --> 00:41:27.750
at. When you get to 10 or 12 earth masses,

1076
00:41:27.830 --> 00:41:30.070
the escape velocity from your core

1077
00:41:30.550 --> 00:41:32.510
is higher than the speed at which hydrogen

1078
00:41:32.510 --> 00:41:34.110
and helium is moving. So you can start to

1079
00:41:34.110 --> 00:41:36.990
capture that. And like I said, 75% of all

1080
00:41:36.990 --> 00:41:39.150
atoms are hydrogen, 24% of all atoms are

1081
00:41:39.150 --> 00:41:41.920
helium. 99% of the mass of the

1082
00:41:41.920 --> 00:41:44.480
protoplanetary disk, or 98%

1083
00:41:44.480 --> 00:41:46.800
maybe is unaccessible till you get to that

1084
00:41:46.800 --> 00:41:48.360
mass and suddenly you've got this whole new

1085
00:41:48.680 --> 00:41:51.280
food source. So you quickly devour all the

1086
00:41:51.280 --> 00:41:53.040
gas around you until you open a gap in the

1087
00:41:53.040 --> 00:41:55.520
disk. And that's how you get the gas giant

1088
00:41:55.520 --> 00:41:57.880
planet shoot from Saturn with Uranus and

1089
00:41:57.880 --> 00:41:59.560
Neptune they formed further out, they had a

1090
00:41:59.560 --> 00:42:02.280
lot of abundant volatile material, but they

1091
00:42:02.280 --> 00:42:04.440
didn't really get massive enough to devour

1092
00:42:04.440 --> 00:42:07.380
the gas before the gas was blown away.

1093
00:42:07.380 --> 00:42:09.980
So that's why you get the ice giants. Uh, and

1094
00:42:10.140 --> 00:42:11.660
that is partially because they're further

1095
00:42:11.660 --> 00:42:13.780
away, they form slower. There are some

1096
00:42:13.780 --> 00:42:15.500
arguments that Uranus and Neptune may have

1097
00:42:15.500 --> 00:42:17.060
formed between Jupiter and Saturn and been

1098
00:42:17.060 --> 00:42:19.580
scattered out. But on a broad

1099
00:42:19.580 --> 00:42:22.580
brushstrokes sense, in our solar

1100
00:42:22.580 --> 00:42:24.420
system we don't think a huge amount of

1101
00:42:24.420 --> 00:42:26.220
migration happened, which is probably down to

1102
00:42:26.220 --> 00:42:28.660
the mass of the protoplanetary disk, not

1103
00:42:28.660 --> 00:42:31.620
compared to the hot Jupiter systems we

1104
00:42:31.620 --> 00:42:34.210
find elsewhere. So the planets we see today

1105
00:42:34.530 --> 00:42:37.490
are within a factor of two or three times

1106
00:42:37.570 --> 00:42:39.490
the same distance they were when they formed.

1107
00:42:39.570 --> 00:42:41.730
Jupiter might have migrated in and back out.

1108
00:42:41.890 --> 00:42:43.610
Uranus and Neptune probably formed

1109
00:42:43.610 --> 00:42:45.370
significantly closer to the sun and migrated

1110
00:42:45.370 --> 00:42:48.330
outwards. But you've got Jupiter and

1111
00:42:48.330 --> 00:42:50.770
outwards forming in the ice dominated area,

1112
00:42:51.410 --> 00:42:53.770
the terrestrial planets forming in the, in

1113
00:42:53.770 --> 00:42:56.450
the area without ice and therefore they're

1114
00:42:56.450 --> 00:42:57.970
dominated by the rock and the metal. So

1115
00:42:57.970 --> 00:43:00.260
you've like got this filter. So if you look

1116
00:43:00.260 --> 00:43:03.180
at the fraction of iron compared to carbon

1117
00:43:03.500 --> 00:43:06.380
in the Earth, or pick any Two things that

1118
00:43:06.380 --> 00:43:08.780
would have been solid silicon versus iron,

1119
00:43:09.020 --> 00:43:11.220
phosphorus for whatever, you know, things

1120
00:43:11.220 --> 00:43:13.660
that were solid. The abundances of those

1121
00:43:13.660 --> 00:43:16.540
things in all of the planets relative

1122
00:43:16.540 --> 00:43:18.580
to one another will be effectively the same

1123
00:43:18.580 --> 00:43:20.740
as the abundance in the Sun. But the

1124
00:43:20.740 --> 00:43:22.740
terrestrial planets weren't able to capture

1125
00:43:22.740 --> 00:43:24.380
the things that would have been gas at their

1126
00:43:24.380 --> 00:43:26.640
distances. Other than that, what was

1127
00:43:26.640 --> 00:43:29.000
delivered later on and weren't able to hold

1128
00:43:29.000 --> 00:43:30.800
on to hydrogen and helium. So you get that

1129
00:43:30.800 --> 00:43:33.720
chemical differentiation as a

1130
00:43:33.720 --> 00:43:35.360
result of the location of the solar system,

1131
00:43:35.360 --> 00:43:37.000
There's a bit of added complexity because

1132
00:43:37.000 --> 00:43:39.840
chemistry happens, and you'll get isotopic

1133
00:43:39.840 --> 00:43:41.439
variations and stuff. But in broad brush

1134
00:43:41.439 --> 00:43:43.920
strokes, the reason the terrestrial planets

1135
00:43:43.920 --> 00:43:46.040
are dominated by rocky and metallic material

1136
00:43:46.120 --> 00:43:47.840
is they never got massive enough to capture

1137
00:43:47.840 --> 00:43:50.680
the gas, and they formed close in where ice

1138
00:43:50.680 --> 00:43:53.430
wasn't around. That's effectively how it

1139
00:43:53.430 --> 00:43:55.870
happens. So what this question from Eli is

1140
00:43:55.870 --> 00:43:58.870
doing is actually effectively describing

1141
00:43:59.110 --> 00:44:02.110
the logic process that went into how

1142
00:44:02.110 --> 00:44:04.110
we first began to understand planet

1143
00:44:04.110 --> 00:44:07.030
formation. Because I said before, I think,

1144
00:44:07.380 --> 00:44:09.270
um, on a previous episode, astronomy is not

1145
00:44:09.270 --> 00:44:11.190
an experimental science in the way that every

1146
00:44:11.190 --> 00:44:12.950
other science is. You know, biology,

1147
00:44:12.950 --> 00:44:15.110
chemistry, physics. You want to figure out

1148
00:44:15.110 --> 00:44:16.790
how something works, you can do experiments.

1149
00:44:17.110 --> 00:44:18.790
Astronomy is an observational science.

1150
00:44:18.790 --> 00:44:20.790
Everything's so big and so far away, we can't

1151
00:44:20.790 --> 00:44:23.160
put it in a lab and smash it it. We instead

1152
00:44:23.160 --> 00:44:24.960
play detective. We look out at the universe

1153
00:44:24.960 --> 00:44:26.640
and we gather clues and we ask questions,

1154
00:44:26.640 --> 00:44:28.600
exactly like the question Eli has asked here,

1155
00:44:28.840 --> 00:44:30.760
which in its fundamental sense is, why do we

1156
00:44:30.760 --> 00:44:33.040
have rocky planets close in and gaseous ones

1157
00:44:33.040 --> 00:44:34.720
further out? Why are there different

1158
00:44:34.720 --> 00:44:36.280
compositions when we should be the same

1159
00:44:36.280 --> 00:44:38.600
composition of the sun? We then come up with

1160
00:44:38.600 --> 00:44:41.000
explanations for that that are our theories.

1161
00:44:41.320 --> 00:44:43.320
And to be a good theory, you can't just say,

1162
00:44:43.320 --> 00:44:45.560
I explain everything we see. You've got to

1163
00:44:45.560 --> 00:44:48.560
make predictions. As we find more things, we

1164
00:44:48.560 --> 00:44:50.600
will observe this. And that's how we test

1165
00:44:50.600 --> 00:44:52.560
that theory. And we test it by this interplay

1166
00:44:52.560 --> 00:44:55.060
between observation on the one theory on the

1167
00:44:55.060 --> 00:44:57.300
other. And what Eli's asked here is

1168
00:44:57.300 --> 00:44:59.580
essentially the questions that people are

1169
00:44:59.580 --> 00:45:01.220
asking that led to our current understanding

1170
00:45:01.220 --> 00:45:02.100
of planet formation.

1171
00:45:03.620 --> 00:45:06.580
Andrew Dunkley: And yet, uh, we

1172
00:45:06.580 --> 00:45:09.540
see other solar systems with exoplanets that

1173
00:45:09.540 --> 00:45:12.540
defy what we think is normal. Uh, you

1174
00:45:12.540 --> 00:45:15.100
have gas giants close to the parent star and

1175
00:45:15.100 --> 00:45:16.580
rocky planets further out.

1176
00:45:17.510 --> 00:45:19.900
Jonti Horner: Um, and that's how we develop.

1177
00:45:19.900 --> 00:45:21.580
Andrew Dunkley: Is that because they've just drifted that

1178
00:45:21.580 --> 00:45:21.860
way.

1179
00:45:22.370 --> 00:45:25.330
Jonti Horner: It's complicated. So our

1180
00:45:25.490 --> 00:45:28.490
ideas planet formation happened

1181
00:45:28.490 --> 00:45:30.370
have undergone quite a few major revolutions

1182
00:45:30.370 --> 00:45:32.530
as we found planets around other stars. So

1183
00:45:33.090 --> 00:45:35.250
in the early 1990s,

1184
00:45:36.370 --> 00:45:38.329
had a couple of talks at my local astronomy

1185
00:45:38.329 --> 00:45:41.170
society in the UK from um, Professor Wolfson

1186
00:45:41.250 --> 00:45:44.130
of York University. And Professor Wolfson

1187
00:45:44.130 --> 00:45:45.810
was an advocate of an entirely different

1188
00:45:45.810 --> 00:45:48.690
formation scenario for the solar system. I

1189
00:45:48.690 --> 00:45:50.440
think he was someone who argued that, that

1190
00:45:50.440 --> 00:45:52.920
the solar system formed through an encounter

1191
00:45:52.920 --> 00:45:54.680
between the sun and a young proto star where

1192
00:45:54.680 --> 00:45:56.320
materials pulled out of the sun into a

1193
00:45:56.320 --> 00:45:58.640
massive tongue and that tongue condensed into

1194
00:45:58.640 --> 00:45:59.200
planets.

1195
00:46:01.520 --> 00:46:04.140
Back then, um,

1196
00:46:04.640 --> 00:46:06.439
that idea was going out of fashion because

1197
00:46:06.439 --> 00:46:08.320
we'd found a few debris disks around stars

1198
00:46:08.320 --> 00:46:10.160
like Vega formal heartbeat pictoris but it

1199
00:46:10.160 --> 00:46:12.520
was still considered possible. Yeah, such an

1200
00:46:12.520 --> 00:46:15.160
event would be incredibly vanishingly

1201
00:46:15.160 --> 00:46:17.520
rare because stars getting that close

1202
00:46:17.520 --> 00:46:20.360
together within one another's hills sphere

1203
00:46:20.840 --> 00:46:23.640
is incredibly unusual. Very, very rare.

1204
00:46:24.280 --> 00:46:27.200
And so what that would predict is

1205
00:46:27.200 --> 00:46:29.680
if that theory were correct, we would be

1206
00:46:29.680 --> 00:46:32.520
almost unique. There will be vanishingly

1207
00:46:32.520 --> 00:46:34.640
few planets round of the stars because the

1208
00:46:34.640 --> 00:46:36.960
scenario you need to form planets would only

1209
00:46:36.960 --> 00:46:39.440
happen very rarely. On the other hand, there

1210
00:46:39.440 --> 00:46:41.430
was the idea which dated back to uh,

1211
00:46:41.430 --> 00:46:44.240
initially the 1700s and beyond the

1212
00:46:44.240 --> 00:46:47.220
Laplacian model, the circum solar disk

1213
00:46:47.220 --> 00:46:48.860
model, which has evolved into what we have

1214
00:46:48.860 --> 00:46:51.580
now, which suggested that as part of star

1215
00:46:51.580 --> 00:46:53.300
formation you get a disk of material around a

1216
00:46:53.300 --> 00:46:55.700
star and planets form from that disk. Disks

1217
00:46:55.700 --> 00:46:57.540
are a natural byproduct of the formation of

1218
00:46:57.540 --> 00:46:59.620
stars. Therefore planetary systems should be

1219
00:46:59.620 --> 00:47:02.380
common. Both scenarios, with a bit of

1220
00:47:02.380 --> 00:47:04.260
fudging and fiddling, could perfectly explain

1221
00:47:04.260 --> 00:47:05.700
how the solar system looked and have been

1222
00:47:05.700 --> 00:47:08.500
finessed to reproduce the solar system. But

1223
00:47:08.500 --> 00:47:10.140
the test was always going to be which of

1224
00:47:10.140 --> 00:47:12.700
these series is correct will depend on how

1225
00:47:12.700 --> 00:47:15.140
many planets we found on other stars. If

1226
00:47:15.140 --> 00:47:17.460
planets are rare, then maybe the solar system

1227
00:47:17.460 --> 00:47:19.140
is the result of a tongue being pulled out on

1228
00:47:19.140 --> 00:47:22.140
the sun. If planetary systems are common,

1229
00:47:22.140 --> 00:47:24.740
that cannot be the case. So that was a test

1230
00:47:24.740 --> 00:47:27.100
that was done there. So when we found the

1231
00:47:27.100 --> 00:47:28.780
first planetary systems around other stars

1232
00:47:28.780 --> 00:47:30.500
and we found that planets are ubiquitous,

1233
00:47:30.820 --> 00:47:32.580
that was kind of the death knell for the

1234
00:47:32.580 --> 00:47:35.300
Wolfson type model of a tongue being sucked

1235
00:47:35.300 --> 00:47:38.290
out of the sun and forming planets. But

1236
00:47:38.290 --> 00:47:40.570
it kind of confirmed the Laplace model. But

1237
00:47:40.570 --> 00:47:42.410
it also threw a spanner into the work in that

1238
00:47:42.410 --> 00:47:45.130
the variation of planet formation of that

1239
00:47:45.130 --> 00:47:47.530
disk model suggested that you would always

1240
00:47:47.530 --> 00:47:49.370
form planetary systems with rocky planets in

1241
00:47:49.370 --> 00:47:50.690
the middle and gas planets on the outside.

1242
00:47:50.690 --> 00:47:52.850
Because it had been developed to explain the

1243
00:47:52.850 --> 00:47:55.690
solar system. When you found planets

1244
00:47:55.690 --> 00:47:57.410
that were hot Jupiters, they don't fit. Their

1245
00:47:57.410 --> 00:47:59.290
planets are massive Jupiter close to their

1246
00:47:59.290 --> 00:48:02.290
star, which brought in the concept of inward

1247
00:48:02.290 --> 00:48:04.050
migration. Now it's an interesting time

1248
00:48:04.050 --> 00:48:06.320
because in the same few years

1249
00:48:06.880 --> 00:48:08.600
people had started to realize that in the

1250
00:48:08.600 --> 00:48:10.320
Solar system, there was clear evidence of

1251
00:48:10.320 --> 00:48:12.400
planetary migration for the giant planets,

1252
00:48:12.640 --> 00:48:15.360
primarily that Neptune had migrated outwards,

1253
00:48:15.360 --> 00:48:18.000
carrying Pluto with it from the Plutinos.

1254
00:48:18.480 --> 00:48:20.599
So you've got these seminal papers by Renu

1255
00:48:20.599 --> 00:48:23.120
Malhotra talking about the outward migration

1256
00:48:23.120 --> 00:48:26.040
of Neptune being evidenced in Pluto and the

1257
00:48:26.040 --> 00:48:28.400
Plutinos, predating the discovery of the

1258
00:48:28.400 --> 00:48:30.760
first exoplanet. And one of my gripes through

1259
00:48:30.760 --> 00:48:32.890
my career has been that the exoplanet

1260
00:48:32.890 --> 00:48:35.530
community primarily came from binary star

1261
00:48:35.530 --> 00:48:37.010
astronomers, not from solar system

1262
00:48:37.010 --> 00:48:39.610
astronomers. So reinvented migration to some

1263
00:48:39.610 --> 00:48:41.810
degree and assumed that we had no evidence

1264
00:48:41.810 --> 00:48:43.570
for it in the solar system. And in parallel,

1265
00:48:43.570 --> 00:48:45.290
the solar system community was working on

1266
00:48:45.290 --> 00:48:47.890
migration separately. But the

1267
00:48:48.210 --> 00:48:50.610
discoveries of planet stars over the last

1268
00:48:51.010 --> 00:48:54.010
30 years and more, which is a great

1269
00:48:54.010 --> 00:48:55.610
scientific revolution we've lived through.

1270
00:48:55.610 --> 00:48:57.050
You know, you and I grew up in a world where

1271
00:48:57.050 --> 00:48:58.650
the only planetary system we knew was our

1272
00:48:58.650 --> 00:49:00.960
own. And kids today grew up in a world where

1273
00:49:00.960 --> 00:49:02.760
we know planets are ubiquitous. That's a

1274
00:49:02.760 --> 00:49:04.600
cataclysmic shift to have lived through.

1275
00:49:05.080 --> 00:49:07.720
Yeah, living through that has proven

1276
00:49:07.800 --> 00:49:09.880
an incredibly fertile testing ground for our

1277
00:49:09.880 --> 00:49:12.560
theories of planet formation. Turns out that

1278
00:49:12.560 --> 00:49:15.400
that Laplace theory, the disk theory, was

1279
00:49:15.640 --> 00:49:18.200
a good way of the way there. So it hasn't

1280
00:49:18.200 --> 00:49:20.000
been totally discarded, but it's been refined

1281
00:49:20.000 --> 00:49:21.360
and we've learned more about it, and that

1282
00:49:21.360 --> 00:49:23.480
continues to the current day. The refinements

1283
00:49:23.800 --> 00:49:25.830
are leading to all sorts of complexities,

1284
00:49:25.830 --> 00:49:28.110
like invoking streaming instabilities to

1285
00:49:28.110 --> 00:49:30.470
concentrate pebbles at certain distances and

1286
00:49:30.630 --> 00:49:33.350
all sorts of subtleties to try and address

1287
00:49:33.350 --> 00:49:35.510
some of the pitfalls of how on Earth do you

1288
00:49:35.510 --> 00:49:37.630
get from millimeter size to meter sized

1289
00:49:37.630 --> 00:49:38.950
objects when collisions should become

1290
00:49:38.950 --> 00:49:41.790
disruptive? All sorts of things like

1291
00:49:41.790 --> 00:49:43.590
this. And it's through those observations

1292
00:49:44.230 --> 00:49:46.470
that we get to improve and refine our models.

1293
00:49:47.510 --> 00:49:49.190
We're not going to end up throwing out the

1294
00:49:49.190 --> 00:49:51.190
disk model now because we can see the disks

1295
00:49:51.190 --> 00:49:52.870
that form planets around other stars. Because

1296
00:49:52.870 --> 00:49:55.220
our telescopes have got that good. Yep. Um,

1297
00:49:55.220 --> 00:49:56.700
and one of the predictions would have been

1298
00:49:57.260 --> 00:49:59.300
prior to them getting that good, if the disk

1299
00:49:59.300 --> 00:50:00.700
model is right. When we look at places like

1300
00:50:00.700 --> 00:50:02.500
the Orion Nebula with a sufficiently good

1301
00:50:02.500 --> 00:50:04.900
telescope, we should see protoplanetary

1302
00:50:04.900 --> 00:50:07.300
disks, propolids. Then the telescope's got

1303
00:50:07.300 --> 00:50:09.380
good enough and we can see them now. We've

1304
00:50:09.380 --> 00:50:11.860
even got to the point now where we can

1305
00:50:11.860 --> 00:50:14.020
actually even observe fine structure within

1306
00:50:14.020 --> 00:50:16.580
them to see the gaps that giant planets open

1307
00:50:16.580 --> 00:50:18.900
up, to see the spiral waves that are

1308
00:50:18.900 --> 00:50:20.500
sometimes induced by a massive planet being

1309
00:50:20.500 --> 00:50:22.350
born. So we're now not only

1310
00:50:22.750 --> 00:50:25.750
inferring planet formation from the plethora

1311
00:50:25.750 --> 00:50:27.070
of planets that we're discovering around

1312
00:50:27.070 --> 00:50:29.670
other stars and from the fine details of what

1313
00:50:29.670 --> 00:50:30.990
we know about the solar system. But we're

1314
00:50:30.990 --> 00:50:32.430
actually also getting observations of the

1315
00:50:32.430 --> 00:50:34.430
disks in which it's happening that are

1316
00:50:34.430 --> 00:50:36.270
providing extra information to improve those

1317
00:50:36.270 --> 00:50:36.750
models.

1318
00:50:37.310 --> 00:50:40.270
Andrew Dunkley: It's fascinating. So you can simply

1319
00:50:40.270 --> 00:50:42.350
say there's no one size fits all

1320
00:50:43.150 --> 00:50:44.750
way of this happening.

1321
00:50:44.990 --> 00:50:46.910
Jonti Horner: Well, it's circumstantial. It's a broad

1322
00:50:46.910 --> 00:50:49.710
thing, rather a narrow thing. So in a broad

1323
00:50:49.710 --> 00:50:51.910
sense, planets form in a disc around a star.

1324
00:50:52.070 --> 00:50:54.990
Natural product of star formation. There may

1325
00:50:54.990 --> 00:50:57.750
be occasional ways of the planet formation

1326
00:50:57.750 --> 00:50:59.430
mechanisms happen like the planets around.

1327
00:51:00.040 --> 00:51:02.870
Um, neutron stars are thought

1328
00:51:02.870 --> 00:51:04.950
to probably be second generation planets.

1329
00:51:05.110 --> 00:51:06.830
Probably material formed from a disk that

1330
00:51:06.830 --> 00:51:08.350
formed around the neutron star after the

1331
00:51:08.350 --> 00:51:10.470
supernova and formed a new generation of

1332
00:51:10.470 --> 00:51:13.310
planets. You might eventually one

1333
00:51:13.310 --> 00:51:15.920
day possibly find planets formed from

1334
00:51:16.480 --> 00:51:18.800
material pulled off a star. The very most

1335
00:51:18.800 --> 00:51:20.400
massive planets, some of them will probably

1336
00:51:20.400 --> 00:51:23.160
have been formed more like binary stars

1337
00:51:23.160 --> 00:51:25.360
than actual planets which we talked in the

1338
00:51:25.360 --> 00:51:28.200
past about. When is a brown dwarf not a brown

1339
00:51:28.200 --> 00:51:30.720
dwarf? Yes, but the broad brushstroke thing

1340
00:51:30.720 --> 00:51:33.360
is fairly well established. But n every

1341
00:51:33.360 --> 00:51:36.200
single planetary system is unique. Everyone

1342
00:51:36.200 --> 00:51:38.800
has unique circumstances. Some disks around

1343
00:51:38.800 --> 00:51:40.680
stars are more massive than others. Not every

1344
00:51:40.680 --> 00:51:43.530
cell will have an identical disc. Some disks

1345
00:51:43.530 --> 00:51:45.610
get truncated because passing starship's

1346
00:51:45.610 --> 00:51:48.330
material away. Some disks get ablated away

1347
00:51:48.330 --> 00:51:50.010
because it's a massive star nearby whose

1348
00:51:50.010 --> 00:51:52.890
radiation pushes material away. You then even

1349
00:51:52.890 --> 00:51:54.570
get impacts on the chemistry. So there's

1350
00:51:54.570 --> 00:51:56.970
really fascinating studies looking at the

1351
00:51:56.970 --> 00:51:59.490
solar system that suggests there was a nearby

1352
00:51:59.810 --> 00:52:02.210
supernova when the planets were forming that

1353
00:52:02.210 --> 00:52:04.330
injected highly radioactive short lived

1354
00:52:04.330 --> 00:52:07.290
aluminium 23 I think it is that gave an

1355
00:52:07.290 --> 00:52:10.050
extra spike to the melting of planetesimals

1356
00:52:10.810 --> 00:52:13.170
that led to some of the subtleties of how the

1357
00:52:13.170 --> 00:52:15.410
solar system looks. There are indications

1358
00:52:15.410 --> 00:52:17.290
even I think that the amount of gold in the

1359
00:52:17.290 --> 00:52:19.890
solar system is unusually high compared to

1360
00:52:19.890 --> 00:52:21.810
the standard metallicity. The amounts of

1361
00:52:21.810 --> 00:52:24.330
everything else with indication of pollution

1362
00:52:24.330 --> 00:52:26.930
from two neutron stars colliding within

1363
00:52:26.930 --> 00:52:29.090
10,000 light years of where the solar system

1364
00:52:29.090 --> 00:52:31.850
would form about 100 million years before we

1365
00:52:31.850 --> 00:52:34.810
formed. So even that level of injection

1366
00:52:34.810 --> 00:52:37.770
of material is unique from one system to the

1367
00:52:37.770 --> 00:52:39.770
next. And that's why every planetary system,

1368
00:52:39.770 --> 00:52:41.130
like every person is unique.

1369
00:52:41.850 --> 00:52:42.650
Andrew Dunkley: Fascinating.

1370
00:52:42.730 --> 00:52:43.290
Jonti Horner: Fascinating.

1371
00:52:43.290 --> 00:52:45.970
Andrew Dunkley: Aren't you glad you asked Eli and Eli's

1372
00:52:45.970 --> 00:52:46.610
second question?

1373
00:52:46.610 --> 00:52:49.410
I recently read that some star systems

1374
00:52:49.410 --> 00:52:51.849
are zipping through their galaxy orbits at

1375
00:52:51.849 --> 00:52:54.650
incredible speeds of 1200. I'm

1376
00:52:54.650 --> 00:52:57.340
assuming that is kilometers per second. Uh,

1377
00:52:57.450 --> 00:53:00.290
that's 0.4% the speed of

1378
00:53:00.290 --> 00:53:03.010
light. That got me wondering how fast could

1379
00:53:03.010 --> 00:53:05.520
our solar system get going before

1380
00:53:05.680 --> 00:53:08.520
we started noticing Things going wrong, you

1381
00:53:08.520 --> 00:53:10.320
know, the windows rattling and such.

1382
00:53:11.580 --> 00:53:14.480
Um, yeah, I, I

1383
00:53:14.480 --> 00:53:17.320
think we've had questions similar to this. I

1384
00:53:17.320 --> 00:53:19.280
think we did one recently where we talked

1385
00:53:19.280 --> 00:53:21.080
about how fast the Earth would spin before

1386
00:53:21.080 --> 00:53:23.920
things started to go horribly wrong. Um,

1387
00:53:24.320 --> 00:53:26.960
this is a question of similar ilk. I

1388
00:53:27.040 --> 00:53:29.200
hadn't heard about those sorts of speeds

1389
00:53:29.200 --> 00:53:31.760
being detected by, um.

1390
00:53:31.820 --> 00:53:34.300
Jonti Horner: Uh, there'd be stars very near the

1391
00:53:34.300 --> 00:53:35.820
supermassive black holes at sense of

1392
00:53:35.820 --> 00:53:37.900
galaxies. And that kind of speed surprised

1393
00:53:37.900 --> 00:53:40.600
me. Now, my immediate take on this is that,

1394
00:53:40.600 --> 00:53:43.260
uh, we wouldn't notice

1395
00:53:43.260 --> 00:53:46.140
effectively. So the reason that I'm saying

1396
00:53:46.140 --> 00:53:48.340
that and I, I stand to be proved wrong when

1397
00:53:48.340 --> 00:53:50.740
you get up to relativistic speeds, because my

1398
00:53:50.740 --> 00:53:52.740
knowledge of relativity is not sufficiently

1399
00:53:52.740 --> 00:53:55.300
good to be absolutely certain on this. If you

1400
00:53:55.300 --> 00:53:58.270
are moving at a substantial fraction

1401
00:53:58.270 --> 00:54:00.510
of the speed of light, I don't think we'd

1402
00:54:00.510 --> 00:54:02.110
notice anything wrong in terms of the Earth

1403
00:54:02.110 --> 00:54:03.350
moving around the sun, because we'd still be

1404
00:54:03.350 --> 00:54:04.910
going around the sun at 30 kilometers per

1405
00:54:04.910 --> 00:54:07.030
second while we're both moving around the

1406
00:54:07.030 --> 00:54:08.510
galaxy at relativistic speed and

1407
00:54:08.510 --> 00:54:11.110
accelerating. What we might notice then is

1408
00:54:11.430 --> 00:54:14.270
time dilation in the fact that the external

1409
00:54:14.270 --> 00:54:17.150
universe appears to be moving quicker than it

1410
00:54:17.150 --> 00:54:19.230
should do. So we might see the effect of the

1411
00:54:19.230 --> 00:54:22.200
fact that our time is slowed down if we

1412
00:54:22.200 --> 00:54:23.600
were going around just the same. As, you

1413
00:54:23.600 --> 00:54:24.880
know, you see this stuff about people

1414
00:54:24.880 --> 00:54:26.360
orbiting a black hole at high speed or

1415
00:54:26.360 --> 00:54:28.680
whatever, or falling into a black hole. But

1416
00:54:28.680 --> 00:54:31.680
in terms of us noticing, in terms

1417
00:54:31.680 --> 00:54:34.680
of physical phenomena on Earth that

1418
00:54:34.680 --> 00:54:36.600
we're traveling at a certain speed around the

1419
00:54:36.600 --> 00:54:39.160
galaxy, I don't see a way that that would

1420
00:54:39.160 --> 00:54:41.760
work. And the reason for that is that there's

1421
00:54:41.760 --> 00:54:43.640
no resistive medium. We think about this

1422
00:54:43.640 --> 00:54:45.000
thing happening because when you're driving

1423
00:54:45.000 --> 00:54:46.560
in your car, the quick you get, the more

1424
00:54:46.560 --> 00:54:48.320
obvious your speed is because of the rattling

1425
00:54:48.320 --> 00:54:49.640
and the wind, really resistance and the

1426
00:54:49.640 --> 00:54:51.600
noise. But that's all down to your

1427
00:54:51.600 --> 00:54:53.560
interaction with something that isn't moving

1428
00:54:53.560 --> 00:54:56.160
at the same speed you are. If you're in the

1429
00:54:56.160 --> 00:54:57.480
International Space Station and you're

1430
00:54:57.480 --> 00:54:59.280
orbiting the, uh, Earth at several kilometers

1431
00:54:59.280 --> 00:55:01.640
a second, you don't feel the space station

1432
00:55:01.640 --> 00:55:03.160
rattling because it's going really quick

1433
00:55:03.640 --> 00:55:05.240
because it's moving through the vacuum of

1434
00:55:05.240 --> 00:55:07.320
space, so it's not interacting with anything.

1435
00:55:07.480 --> 00:55:09.080
If you're coming back into the atmosphere,

1436
00:55:09.080 --> 00:55:10.760
you rattle and rumble and all the rest of it.

1437
00:55:10.760 --> 00:55:13.080
We saw this with Artemis 2, because you're

1438
00:55:13.080 --> 00:55:14.160
slowing down, you're experiencing

1439
00:55:14.160 --> 00:55:16.270
acceleration, you're experiencing buffeting.

1440
00:55:17.220 --> 00:55:20.140
So to me, if we are moving as a

1441
00:55:20.140 --> 00:55:22.340
planetary system around the middle of the

1442
00:55:22.340 --> 00:55:25.260
galaxy at very high speed. Our planets would

1443
00:55:25.260 --> 00:55:27.860
still be orbiting the sun in the same way and

1444
00:55:27.860 --> 00:55:30.340
we wouldn't notice any difference. What would

1445
00:55:30.340 --> 00:55:31.880
happen though, is we'd be moving through a m.

1446
00:55:31.900 --> 00:55:34.460
Much, much denser stellar neighborhood. The

1447
00:55:34.460 --> 00:55:37.020
sky would be immeasurably beautiful, but

1448
00:55:37.020 --> 00:55:39.300
challenge. But also close encounters between

1449
00:55:39.300 --> 00:55:42.190
stars will be very common. And so

1450
00:55:42.190 --> 00:55:43.910
it may well be that the stars will be so

1451
00:55:43.910 --> 00:55:45.590
densely packed that eventually we'd have a

1452
00:55:45.590 --> 00:55:47.750
stellar approach that will be so close to

1453
00:55:47.750 --> 00:55:49.830
solar system will be disrupted. And we'd

1454
00:55:49.830 --> 00:55:51.790
certainly notice that also

1455
00:55:52.750 --> 00:55:54.990
if we were injected to there from where we

1456
00:55:54.990 --> 00:55:57.590
are now, There will be a period of adjustment

1457
00:55:57.590 --> 00:55:59.110
where the Oort cloud will be heavily

1458
00:55:59.110 --> 00:56:01.030
destabilized and we'd have catastrophic

1459
00:56:01.030 --> 00:56:02.630
levels of impacts from the comets being

1460
00:56:02.630 --> 00:56:04.830
scattered. But eventually they'd all be gone,

1461
00:56:04.830 --> 00:56:07.750
so it wouldn't be a problem. So we'd notice

1462
00:56:07.750 --> 00:56:08.390
it from the point

1463
00:56:08.390 --> 00:56:10.070
Andrew Dunkley: of view until led to the dinosaurs.

1464
00:56:10.070 --> 00:56:12.870
Jonti Horner: Oh, absolutely. Um, Long may they rest.

1465
00:56:13.110 --> 00:56:15.910
But it's one of those things where

1466
00:56:15.910 --> 00:56:17.950
if we were there and we were transported

1467
00:56:17.950 --> 00:56:20.070
there from now, what we'd notice is that the

1468
00:56:20.230 --> 00:56:22.190
sky looked very different. If we were moving

1469
00:56:22.190 --> 00:56:25.150
at that kind of speed in that denser

1470
00:56:25.150 --> 00:56:26.870
stellar neighborhood, the proper motion of

1471
00:56:26.870 --> 00:56:29.470
stars would be apparent to the naked eye over

1472
00:56:29.470 --> 00:56:31.430
human timescales, which it's not for us.

1473
00:56:31.750 --> 00:56:33.830
Barnard Star, which is the fastest moving

1474
00:56:33.830 --> 00:56:36.030
star across the night sky, will cross the

1475
00:56:36.030 --> 00:56:38.560
diameter of the full Moon in a century. Very

1476
00:56:38.560 --> 00:56:41.480
roughly, that means if Barnard's star was

1477
00:56:41.480 --> 00:56:43.920
bright enough to see with the naked eye, we'd

1478
00:56:43.920 --> 00:56:45.280
have known about proper motion earlier

1479
00:56:45.520 --> 00:56:48.040
because it would be obvious, but it wouldn't

1480
00:56:48.040 --> 00:56:49.320
be the kind of thing you'd notice from one

1481
00:56:49.320 --> 00:56:50.960
year to the next. Whereas if we were in the

1482
00:56:50.960 --> 00:56:52.280
middle of the galaxy Going around the

1483
00:56:52.280 --> 00:56:54.160
supermassive black hole, at that ridiculous

1484
00:56:54.160 --> 00:56:57.120
speed, stars will be closer together, which

1485
00:56:57.280 --> 00:56:59.600
magnifies the effect of motion

1486
00:57:00.720 --> 00:57:03.320
from our perspective. Also, they'd be moving

1487
00:57:03.320 --> 00:57:04.930
quicker, which means that the motion is

1488
00:57:04.930 --> 00:57:06.850
quicker from our perspective. And you

1489
00:57:06.850 --> 00:57:09.210
probably have proper motion being visible on

1490
00:57:09.210 --> 00:57:10.930
human timescales to the point that the

1491
00:57:10.930 --> 00:57:13.050
constellations would move. Rather than being

1492
00:57:13.130 --> 00:57:15.770
fixed patterns that you'd notice,

1493
00:57:16.810 --> 00:57:18.970
you wouldn't feel the acceleration, you

1494
00:57:18.970 --> 00:57:21.250
wouldn't notice anything's wrong. But we

1495
00:57:21.250 --> 00:57:22.770
probably wouldn't be there if the sun had

1496
00:57:22.770 --> 00:57:24.210
been there for a long time. Because it's a

1497
00:57:24.210 --> 00:57:26.890
very intermissal environment for life.

1498
00:57:26.890 --> 00:57:28.290
Because there's a lot of stars close

1499
00:57:28.290 --> 00:57:30.010
together, a lot of massive stars, a lot of

1500
00:57:30.010 --> 00:57:32.270
supernovae. It's probably a bit of a dead

1501
00:57:32.270 --> 00:57:32.670
zone.

1502
00:57:33.790 --> 00:57:33.940
Andrew Dunkley: Aha.

1503
00:57:33.940 --> 00:57:34.760
Jonti Horner: Uh-huh.

1504
00:57:34.760 --> 00:57:37.630
Andrew Dunkley: Okay. All right. Um, thanks

1505
00:57:37.630 --> 00:57:40.430
for your questions, Eli. And, uh, yeah, I

1506
00:57:40.430 --> 00:57:42.390
love that second one. I love what if

1507
00:57:42.390 --> 00:57:44.950
questions. Uh, so, uh, yeah, we've been

1508
00:57:44.950 --> 00:57:47.110
getting a few of those lately. It's. They're

1509
00:57:47.110 --> 00:57:49.630
just such great fun. Thanks, uh, to Nick and

1510
00:57:49.630 --> 00:57:51.750
Andrea as well, for contributing. And if you

1511
00:57:51.750 --> 00:57:53.950
would like to send us a question, please do

1512
00:57:53.950 --> 00:57:56.510
on our website, space nutspodcast.com

1513
00:57:56.510 --> 00:57:59.310
spacenut Click on the AMA

1514
00:57:59.310 --> 00:58:01.230
button at the top. Ask me anything is what

1515
00:58:01.230 --> 00:58:03.830
that stands for. And you can send text and

1516
00:58:03.830 --> 00:58:05.790
audio questions. Don't forget to tell us who

1517
00:58:05.790 --> 00:58:07.550
you are and where you're from. And while

1518
00:58:07.550 --> 00:58:08.830
you're there, have a look around. Check out

1519
00:58:08.830 --> 00:58:10.950
the Space Nuts shop. Maybe you'd like to

1520
00:58:10.950 --> 00:58:13.029
become a supporter. Sign up for the Astronomy

1521
00:58:13.029 --> 00:58:15.150
Daily newsletter, all sorts of things to see

1522
00:58:15.150 --> 00:58:17.510
and do on our website. And please leave

1523
00:58:17.510 --> 00:58:19.910
reviews wherever you listen to

1524
00:58:20.390 --> 00:58:22.940
Space Nuts. We appreciate that as well. Well,

1525
00:58:22.940 --> 00:58:25.100
and we appreciate you, Jonti. Thanks so much

1526
00:58:25.100 --> 00:58:27.340
for, uh, your input today. Fantastic.

1527
00:58:27.340 --> 00:58:28.900
Jonti Horner: Oh, it's always a pleasure. And yeah,

1528
00:58:28.900 --> 00:58:30.540
fabulous questions. Really enjoy them.

1529
00:58:31.500 --> 00:58:33.740
Andrew Dunkley: Me too. And we'll catch up, uh, with you

1530
00:58:33.740 --> 00:58:34.420
very, very soon.

1531
00:58:34.420 --> 00:58:35.980
Jonti Horner: Yeah, I look forward to it. Thank you.

1532
00:58:36.540 --> 00:58:38.779
Andrew Dunkley: Professor Jonti Horner from, uh, the

1533
00:58:38.779 --> 00:58:40.740
University of Southern Queensland, where he

1534
00:58:40.740 --> 00:58:43.460
is a professor of astrophysics. And thanks to

1535
00:58:43.460 --> 00:58:45.220
Huw in the studio, who couldn't be with us

1536
00:58:45.220 --> 00:58:47.640
today because time moves slower for Huw. So,

1537
00:58:47.640 --> 00:58:50.340
uh, he'll be joining us in a couple of

1538
00:58:50.340 --> 00:58:52.780
thousand years. And from me, Andrew Dunkley.

1539
00:58:52.780 --> 00:58:54.180
Thanks for your company. We'll see you on the

1540
00:58:54.180 --> 00:58:55.700
next episode of Space Nuts.

1541
00:58:55.700 --> 00:58:56.020
Jonti Horner: Bye.

1542
00:58:56.020 --> 00:58:58.940
Andrew Dunkley: Bye. Uh, you'll be listening to the

1543
00:58:58.940 --> 00:58:59.220
Space

1544
00:58:59.220 --> 00:59:00.340
Jonti Horner: Nuts podcast,

1545
00:59:01.860 --> 00:59:04.660
available at Apple Podcasts, Spotify,

1546
00:59:04.900 --> 00:59:07.580
iHeartRadio or your favorite podcast

1547
00:59:07.580 --> 00:59:09.300
player. You can also stream on

1548
00:59:09.300 --> 00:59:10.980
demand@bytes.com.

1549
00:59:11.300 --> 00:59:13.380
Andrew Dunkley: this has been another quality podcast

1550
00:59:13.380 --> 00:59:15.540
production from bytes.com.
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