May 17, 2026
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.
For more Space Nuts, including our continuously updating newsfeed and to listen to all our episodes, visit our website. Follow us on social media at SpaceNutsPod on Facebook, Instagram, and more. We love engaging with our community, so be sure to drop us a message or comment on your favorite platform.
If you’d like to help support Space Nuts and join our growing family of insiders for commercial-free episodes and more, visit spacenutspodcast.com/about.
Stay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support.
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.
For more Space Nuts, including our continuously updating newsfeed and to listen to all our episodes, visit our website. Follow us on social media at SpaceNutsPod on Facebook, Instagram, and more. We love engaging with our community, so be sure to drop us a message or comment on your favorite platform.
If you’d like to help support Space Nuts and join our growing family of insiders for commercial-free episodes and more, visit spacenutspodcast.com/about.
Stay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support.
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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to the 24 kilos. So that is
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effectively, um, 2 times 10 to the minus
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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.
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It would decay in only 10 to the 49 years,
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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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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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is 28, 56,
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84. So that's 10 to the 84.
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So that means I would disintegrate in two
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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.
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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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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
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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
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formed at the Big Bang, Then maybe
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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,
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however, know what the distribution
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of masses for primordial black
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holes would be. It's possibly on this
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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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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
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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
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3,000 miles wide, um, with an
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incredibly shallow crater. Um, if you could
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explain for me why that occurs,
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that would be absolutely amazing. Thank you
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very much. Oh, and this is Andrea from
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Wanneroo and Andrew. Uh, Wanneroo is actually
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a noongar, or whadjuk? Noongar. Ah,
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people word. Um, that actually
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means the area of the
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digging stick. Unfortunately, not
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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,
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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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meaning, I want a pet kangaroo. So,
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yeah, I know I was being silly, but, um, no,
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it's, um, place of the digging stick. Didn't
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know that. So, um, of course, the digging
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stick was one of the implements, uh, that the
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ancient indigenous peoples of Australia used
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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
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that derive from the languages of the
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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
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language groups. And the origin of the
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names is not always that well known or
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understood because during the invasion of
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Australia and during the events that happened
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all the way through to the 1970s, there was a
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fairly aggressive attempt to, even if
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you weren't wiping out the people, to get rid
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of the culture and to get rid of the
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knowledge. I've just looked up Toowoomba
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where I am T o uh o uh w o uh o uh m b
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a I live about 20 ks west of there.
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Toowoomba is an indigenous name. It's a
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really interesting town because it's like the
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Florida of Queensland. All the old people
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come here to retire. It's a lovely place.
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It's a beautiful place because Queensland has
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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
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00:16:04.060 --> 00:16:06.620
700 meters above sea level. So it's not as
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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
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probably based on a word
406
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from likely the Gable or Jarawar
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00:16:19.380 --> 00:16:21.820
peoples. Not entirely sure. But if you look
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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
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00:16:27.040 --> 00:16:29.120
suggestion that it was a, ah, word for swamp
411
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because Toowoomba sits in this swampy area on
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top of the hills. According to the Toowoomba
413
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Regional Council, it may have been named
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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
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00:16:43.000 --> 00:16:45.680
will be the swamp thing or place of melon, or
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place where reeds grow or berries place or
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white man. There are other things saying
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meeting of the waters or. Or saying. The name
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00:16:53.050 --> 00:16:54.810
of Toowoomba may be an anglicized version of
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00:16:54.810 --> 00:16:57.770
the word bu wonga, which meant thunder in
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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
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00:17:02.770 --> 00:17:04.210
make me a little bit sad. We talk about
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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
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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
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00:17:12.130 --> 00:17:13.410
it does make me sad how much of this
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00:17:13.410 --> 00:17:15.010
knowledge is lost where you don't even know
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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
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00:17:19.439 --> 00:17:21.879
name comes from. We can talk to that. So when
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you're looking at the map of Australia and
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think a lot of the places are unusual from
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the perspective of someone from an Anglo
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background or from a European background,
439
00:17:29.799 --> 00:17:31.919
it's because even though it's a primarily
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English speaking country nowadays with a,
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00:17:35.159 --> 00:17:38.039
with that, you know, Anglo heritage, a lot of
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00:17:38.039 --> 00:17:39.519
the names are actually from the traditional
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00:17:39.519 --> 00:17:42.159
owners, even if the heritage of that name
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itself is lost.
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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
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00:17:56.980 --> 00:17:58.800
everything turns red, uh,
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00:17:59.060 --> 00:18:01.700
Jonti Horner: when it gets wet and you're bringing it in
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00:18:01.700 --> 00:18:03.940
because the red soil marks horrible
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00:18:03.940 --> 00:18:06.340
everything up, you know. Yeah. Dog goes out
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00:18:06.340 --> 00:18:08.180
and gets their paws muddy and brings in red
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footprints.
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Andrew Dunkley: Red footprints on a light colored carpet. No,
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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
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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
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rocket range is where Australia's, uh,
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00:18:44.980 --> 00:18:47.740
early space efforts were, uh, were
470
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launched from in South Australia. So yeah,
471
00:18:49.660 --> 00:18:51.940
it's um, fascinating history really is.
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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
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being a thing that used for throwing space.
476
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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
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00:19:02.460 --> 00:19:04.660
word applatl apparently comes from Aztec.
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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.
0
00:00:01.120 --> 00:00:03.160
Andrew Dunkley: Hi there. Thanks for joining us on a Q and A
1
00:00:03.160 --> 00:00:05.640
edition of Space Nuts. Andrew Dunkley here,
2
00:00:05.640 --> 00:00:08.360
your host. Great to have your company. Coming
3
00:00:08.360 --> 00:00:10.520
up, we've got a few questions. Nick is going
4
00:00:10.520 --> 00:00:13.040
to ask about supercharged neutrinos.
5
00:00:13.120 --> 00:00:16.079
Andrea is making a return appearance.
6
00:00:16.079 --> 00:00:17.600
She's got a couple of questions about the
7
00:00:17.600 --> 00:00:19.720
dark side of the moon and shallow craters.
8
00:00:19.720 --> 00:00:22.560
And Eli is asking about elements
9
00:00:22.640 --> 00:00:25.440
and the speed of objects. And if we've got
10
00:00:25.440 --> 00:00:27.240
time, we'll chuck another question into the
11
00:00:27.240 --> 00:00:30.160
mix as well. All coming up on this edition of
12
00:00:30.240 --> 00:00:33.140
Space Nuts. Seconds. Guidance is
13
00:00:33.140 --> 00:00:35.580
internal. 10, 9.
14
00:00:36.140 --> 00:00:37.820
Ignition sequence start.
15
00:00:37.980 --> 00:00:38.664
Jonti Horner: Space nuts.
16
00:00:38.736 --> 00:00:41.544
Andrew Dunkley: 5, 4, 3, 2. 1. 2, 3, 4,
17
00:00:41.616 --> 00:00:44.220
5, 5, 4, 3, 2, 1. Space
18
00:00:44.380 --> 00:00:46.860
nuts. Astronauts report it feels good.
19
00:00:47.979 --> 00:00:50.380
And with Fred away, Jonti can play.
20
00:00:50.540 --> 00:00:52.860
It's professor, uh, Jonti
21
00:00:52.860 --> 00:00:55.460
Horner, professor of Astrophysics at the
22
00:00:55.460 --> 00:00:57.540
University of Southern Queensland. Jonti,
23
00:00:57.540 --> 00:00:58.820
hello again. Good afternoon.
24
00:00:58.820 --> 00:00:59.570
Jonti Horner: How are you going to.
25
00:00:59.720 --> 00:01:02.640
Andrew Dunkley: I am well. Great to see you. I think we
26
00:01:02.640 --> 00:01:05.540
should just go straight into it and, uh,
27
00:01:05.540 --> 00:01:07.000
hit you with our first question.
28
00:01:07.080 --> 00:01:10.080
It's a topic I'm not overly familiar
29
00:01:10.080 --> 00:01:12.280
with, but, uh, this one comes from Nick.
30
00:01:12.920 --> 00:01:15.679
Uh, I just read that a supercharged neutrino
31
00:01:15.679 --> 00:01:18.600
was detected by the Kilometer Cube
32
00:01:18.600 --> 00:01:21.560
Neutrino Telescope, and a theory was
33
00:01:21.560 --> 00:01:23.960
put forward that it came from an exploding
34
00:01:23.960 --> 00:01:26.680
black hole. Please explain how a black hole
35
00:01:26.680 --> 00:01:29.680
can explode. Love the show, Nick. Thank you,
36
00:01:29.680 --> 00:01:31.870
Nick, we love that you love the show.
37
00:01:32.750 --> 00:01:35.300
Thank you for sending in a question. Um,
38
00:01:35.300 --> 00:01:36.940
exploding black holes. Um,
39
00:01:38.350 --> 00:01:40.270
I seem to remember Fred might have written a
40
00:01:40.270 --> 00:01:42.990
book about something like that once. Um, but
41
00:01:42.990 --> 00:01:45.790
anyway, um, do they explode or do they
42
00:01:45.790 --> 00:01:48.110
merge or do they collapse? They eventually
43
00:01:48.110 --> 00:01:48.630
disappear.
44
00:01:48.630 --> 00:01:51.510
Jonti Horner: I know that now. You know straight up,
45
00:01:51.510 --> 00:01:53.830
I'm not a cosmologist or a cosmetologist,
46
00:01:53.830 --> 00:01:55.510
which I always used to joke about
47
00:01:55.510 --> 00:01:57.230
cosmologists being cosmetologists. And it
48
00:01:57.230 --> 00:01:59.470
turns out a cosmetologist is a real thing. So
49
00:01:59.630 --> 00:02:02.360
never mind. Um, that's, uh,
50
00:02:02.360 --> 00:02:04.670
further from my area of expertise. So any
51
00:02:04.670 --> 00:02:07.310
answer I give, take with a larger grain of
52
00:02:07.310 --> 00:02:09.310
salt, you know, as is always the way you
53
00:02:09.310 --> 00:02:10.910
know, you. The further you go from your
54
00:02:10.910 --> 00:02:12.310
expertise, the more out of date your
55
00:02:12.310 --> 00:02:14.670
knowledge is. My knowledge on
56
00:02:15.070 --> 00:02:17.750
exploding or rather evaporating black
57
00:02:17.750 --> 00:02:20.630
holes goes back to basically when I was an
58
00:02:20.630 --> 00:02:22.550
undergrad and I was doing lots of courses in
59
00:02:22.550 --> 00:02:25.230
lots of different things. And this goes back
60
00:02:25.310 --> 00:02:27.790
to some of the work that made Stephen
61
00:02:27.790 --> 00:02:30.350
Hawking so world renowned. Now, obviously,
62
00:02:30.350 --> 00:02:32.190
for a lot of people, Stephen Hawking became a
63
00:02:32.190 --> 00:02:34.430
global name with the publication of A Brief
64
00:02:34.430 --> 00:02:36.910
History of Time, which did a very good job of
65
00:02:36.910 --> 00:02:38.990
explaining very complicated things in A way
66
00:02:38.990 --> 00:02:41.150
that people could at least feel like they had
67
00:02:41.150 --> 00:02:43.430
a grasp of. Um, I remember reading it as a
68
00:02:43.430 --> 00:02:45.510
kid, and it made my head hurt. But it, in a
69
00:02:45.510 --> 00:02:47.310
good way, I could actually follow it. It was
70
00:02:47.310 --> 00:02:49.470
well explained. One of the things that
71
00:02:49.470 --> 00:02:51.150
Stephen Hawking did fairly early in his
72
00:02:51.150 --> 00:02:53.350
career, I think in, like, 1974 or something,
73
00:02:53.830 --> 00:02:56.560
was do some very theoretical work on, um,
74
00:02:56.560 --> 00:02:58.950
black holes, where he postulated that black
75
00:02:58.950 --> 00:03:01.730
holes could lose we through a process called
76
00:03:01.730 --> 00:03:04.570
Hawking radiation. And the idea is
77
00:03:04.570 --> 00:03:07.530
that black holes can effectively be
78
00:03:07.530 --> 00:03:10.130
considered to have a temperature and to
79
00:03:10.130 --> 00:03:13.050
radiate energy and therefore mass away
80
00:03:13.050 --> 00:03:15.410
into space. And the smaller the black hole,
81
00:03:15.410 --> 00:03:17.050
the hotter it is, so the quicker it would
82
00:03:17.050 --> 00:03:18.770
radiate. And this is all backed up by
83
00:03:19.010 --> 00:03:21.290
ridiculously complex physics and mathematics
84
00:03:21.290 --> 00:03:23.250
that is way beyond my level of full
85
00:03:23.250 --> 00:03:25.970
understanding. But part of the idea behind it
86
00:03:25.970 --> 00:03:28.170
is what we think of as the empty vacuum of
87
00:03:28.170 --> 00:03:30.210
space is actually not a true vacuum, but is
88
00:03:30.210 --> 00:03:33.110
instead constantly populated by pairs
89
00:03:33.110 --> 00:03:35.350
of matter and antimatter particles that
90
00:03:35.350 --> 00:03:37.630
spontaneously create and then collide with
91
00:03:37.630 --> 00:03:40.110
each other and disappear again. And if these,
92
00:03:40.430 --> 00:03:42.350
if such an event happens near the event
93
00:03:42.350 --> 00:03:44.030
horizon of a black hole, one of the particles
94
00:03:44.030 --> 00:03:45.630
falls into the black hole, the other escapes,
95
00:03:45.630 --> 00:03:48.160
and it's seen to lose mass, lose energy, and,
96
00:03:48.160 --> 00:03:50.350
um, radiation going along with that. Now,
97
00:03:50.990 --> 00:03:53.270
the bigger the black hole, the colder it
98
00:03:53.270 --> 00:03:56.110
would be. So the slower it radiates anyway,
99
00:03:56.350 --> 00:03:58.310
but also the bigger it is, the more
100
00:03:58.310 --> 00:04:00.350
effectively it can feed from its environment.
101
00:04:00.990 --> 00:04:02.750
Even if that's little bits of dust falling
102
00:04:02.750 --> 00:04:05.050
in. Or if it's near a star, star, it can feed
103
00:04:05.050 --> 00:04:07.730
off that star, get an accretion disk. So the
104
00:04:07.730 --> 00:04:10.010
black holes that form in the modern universe
105
00:04:10.410 --> 00:04:12.690
are formed by stars reaching the end of their
106
00:04:12.690 --> 00:04:15.050
lives and are massive. They're more massive
107
00:04:15.050 --> 00:04:17.010
than the sun by L1, where they're formed from
108
00:04:17.010 --> 00:04:20.010
stars much more massive than the Sun. You get
109
00:04:20.249 --> 00:04:22.050
massive black holes, you get intermediate
110
00:04:22.050 --> 00:04:24.090
mass black holes, and you get supermassive
111
00:04:24.090 --> 00:04:25.650
black holes. And they're all the big whopping
112
00:04:25.650 --> 00:04:27.450
ones. And, um, the time scale, as I
113
00:04:27.450 --> 00:04:29.090
understand it, m for those black holes to
114
00:04:29.090 --> 00:04:32.020
decay through Hawking radiation is
115
00:04:32.260 --> 00:04:34.700
ridiculously, ridiculously, ridiculously
116
00:04:34.700 --> 00:04:36.780
longer than the edge of the universe. Yes.
117
00:04:36.780 --> 00:04:38.460
And, um, they're probably not emitting
118
00:04:38.460 --> 00:04:40.300
Hawking radiation at a level that we could
119
00:04:40.300 --> 00:04:42.580
detect because they are very cold. In his
120
00:04:42.660 --> 00:04:45.350
quantification of it, however, at, uh,
121
00:04:45.380 --> 00:04:47.180
the birth of the universe, when the
122
00:04:47.180 --> 00:04:48.740
temperature and pressure was immense after
123
00:04:48.740 --> 00:04:51.060
the Big Bang, there were
124
00:04:51.460 --> 00:04:54.020
theoretically a class of black holes created
125
00:04:54.020 --> 00:04:56.860
called primordial black holes. So these were
126
00:04:56.860 --> 00:04:59.220
black holes that were not born from the fiery
127
00:04:59.220 --> 00:05:02.090
Death of a star, but were instead born
128
00:05:02.330 --> 00:05:04.930
out of the Big Bang and the pressures and the
129
00:05:04.930 --> 00:05:06.810
temperatures. And um, these could be black
130
00:05:06.810 --> 00:05:09.450
holes down to the mass of a thumbnail or down
131
00:05:09.530 --> 00:05:11.410
really, really tiny ones. Planet mass black
132
00:05:11.410 --> 00:05:11.850
holes.
133
00:05:12.010 --> 00:05:12.490
Andrew Dunkley: Yep.
134
00:05:12.490 --> 00:05:14.450
Jonti Horner: The smaller you are as a black hole, the more
135
00:05:14.450 --> 00:05:16.290
quickly you radiate things away, so the
136
00:05:16.290 --> 00:05:19.290
shorter your lifetime. And so you have this
137
00:05:19.290 --> 00:05:21.210
idea that these primordial black holes
138
00:05:21.850 --> 00:05:24.650
evaporated over time and effectively
139
00:05:24.650 --> 00:05:26.570
none of them will survive to the current day.
140
00:05:27.370 --> 00:05:30.350
Those evaporating black holes would
141
00:05:30.350 --> 00:05:32.190
evaporate over time and give off radiation
142
00:05:32.190 --> 00:05:35.030
that we have never yet detected. But a black
143
00:05:35.030 --> 00:05:36.590
hole coming to the end of its life will
144
00:05:36.590 --> 00:05:38.870
evaporate faster and m faster. There's a
145
00:05:38.870 --> 00:05:40.750
quote on an article I found recently which
146
00:05:40.750 --> 00:05:43.670
may be tied to this, um, article entitled
147
00:05:43.670 --> 00:05:45.470
An Exploding Black Hole Could Reveal the
148
00:05:45.470 --> 00:05:47.750
Foundations of the Universe, published from
149
00:05:47.750 --> 00:05:50.310
September last year, talking about
150
00:05:50.550 --> 00:05:52.870
the predictions that as our technology gets
151
00:05:52.870 --> 00:05:55.230
better in the coming years, we may be able to
152
00:05:55.230 --> 00:05:57.940
detect this Hawking radiation in an event
153
00:05:57.940 --> 00:05:59.700
where the black hole reaches its critical
154
00:05:59.700 --> 00:06:02.220
phase and evaporates entirely within the next
155
00:06:02.220 --> 00:06:04.260
few years. So not quite the neutrino
156
00:06:04.260 --> 00:06:05.620
discovery that we were talking about in the
157
00:06:05.620 --> 00:06:08.180
question, but a related thing. And there's a
158
00:06:08.180 --> 00:06:10.700
quote here from Andrea Tham, who
159
00:06:10.780 --> 00:06:13.660
Associate Professor Andrea Tham, I, I do hate
160
00:06:13.660 --> 00:06:15.900
it when articles don't give people's well
161
00:06:15.900 --> 00:06:17.940
earned titles until later in the sentence or
162
00:06:17.940 --> 00:06:20.340
don't give them at all. Um, which is another
163
00:06:20.340 --> 00:06:22.180
ont. I could go on, that's separate, but it
164
00:06:22.180 --> 00:06:24.650
particularly affects my, um,
165
00:06:25.550 --> 00:06:27.990
early career colleagues, um, affects
166
00:06:27.990 --> 00:06:29.590
colleagues from non traditional backgrounds
167
00:06:29.590 --> 00:06:30.750
and stuff. And it's a very
168
00:06:32.350 --> 00:06:34.750
diminutizing thing, diminishing thing. It
169
00:06:35.070 --> 00:06:37.150
lowers their expertise. Anyway, this is a
170
00:06:37.150 --> 00:06:39.150
quote from Associate Professor Andrea Tham
171
00:06:39.150 --> 00:06:41.630
from University of Massachusetts Amherst,
172
00:06:41.950 --> 00:06:44.390
says as primordial black holes evaporate,
173
00:06:44.390 --> 00:06:46.910
they become ever lighter, uh, so hotter.
174
00:06:47.310 --> 00:06:49.470
They therefore emit even more radiation. It's
175
00:06:49.470 --> 00:06:51.470
a runaway process until they explode.
176
00:06:52.520 --> 00:06:54.460
Um, it's that Hawking radiation that our
177
00:06:54.460 --> 00:06:55.620
telescopes can detect.
178
00:06:55.940 --> 00:06:56.420
Andrew Dunkley: Yeah.
179
00:06:56.420 --> 00:06:57.660
Jonti Horner: So what's happening is you've got these
180
00:06:57.660 --> 00:06:59.740
primordial black holes that are really itty
181
00:06:59.740 --> 00:07:02.100
bitty diddy ones that are therefore
182
00:07:02.100 --> 00:07:04.420
evaporating quicker than they can gain mass.
183
00:07:04.820 --> 00:07:06.500
They'll be on this critical threshold. And so
184
00:07:06.500 --> 00:07:08.820
you get this runaway death where the more
185
00:07:08.820 --> 00:07:11.260
massive ones live longer before they get
186
00:07:11.260 --> 00:07:13.860
small enough to finally evaporate and then
187
00:07:13.860 --> 00:07:16.500
explode. And so I would guess
188
00:07:17.220 --> 00:07:19.940
that the observation of this super
189
00:07:19.940 --> 00:07:22.500
neutrino that has been linked potentially to
190
00:07:22.500 --> 00:07:24.740
an exploding black hole is not two black
191
00:07:24.740 --> 00:07:27.180
holes colliding. It's not a modern Black hole
192
00:07:27.180 --> 00:07:30.100
formed from the death of sars, but rather is
193
00:07:30.100 --> 00:07:32.700
the death of a primordial black hole, as
194
00:07:32.700 --> 00:07:34.740
would be predicted by this research by
195
00:07:34.740 --> 00:07:37.340
Stephen hawking more than 50 years ago in the
196
00:07:37.340 --> 00:07:40.300
form of Hawking radiation. So that's my
197
00:07:40.380 --> 00:07:42.140
thinking on what's happening here. Now,
198
00:07:42.140 --> 00:07:44.940
obviously, I am, um, not an expert.
199
00:07:45.370 --> 00:07:47.660
Um, I've said previously on many places,
200
00:07:47.750 --> 00:07:49.820
uh, in a lot of disciplines, and when we're
201
00:07:49.820 --> 00:07:51.500
teaching our undergrads, we often say, avoid
202
00:07:51.500 --> 00:07:53.540
Wikipedia. Wikipedia is not a static
203
00:07:53.540 --> 00:07:55.300
resource. It's a fluid resource and it's
204
00:07:55.300 --> 00:07:57.700
often wrong. And I know for journalists, it's
205
00:07:57.700 --> 00:07:59.420
probably often something you caution, don't
206
00:07:59.420 --> 00:08:01.460
get your facts from Wikipedia. For
207
00:08:01.460 --> 00:08:03.500
astrophysics, and particularly the more
208
00:08:03.660 --> 00:08:06.620
technical and hardcore ends of astrophysics,
209
00:08:07.020 --> 00:08:09.380
Wikipedia is actually very reliable because
210
00:08:09.380 --> 00:08:11.340
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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to the 24 kilos. So that is
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effectively, um, 2 times 10 to the minus
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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.
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It would decay in only 10 to the 49 years,
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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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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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is 28, 56,
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84. So that's 10 to the 84.
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So that means I would disintegrate in two
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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.
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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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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
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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
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formed at the Big Bang, Then maybe
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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,
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however, know what the distribution
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of masses for primordial black
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holes would be. It's possibly on this
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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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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
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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
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3,000 miles wide, um, with an
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incredibly shallow crater. Um, if you could
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explain for me why that occurs,
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that would be absolutely amazing. Thank you
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very much. Oh, and this is Andrea from
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Wanneroo and Andrew. Uh, Wanneroo is actually
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a noongar, or whadjuk? Noongar. Ah,
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people word. Um, that actually
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means the area of the
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digging stick. Unfortunately, not
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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,
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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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meaning, I want a pet kangaroo. So,
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yeah, I know I was being silly, but, um, no,
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it's, um, place of the digging stick. Didn't
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know that. So, um, of course, the digging
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stick was one of the implements, uh, that the
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ancient indigenous peoples of Australia used
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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
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that derive from the languages of the
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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
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language groups. And the origin of the
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names is not always that well known or
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understood because during the invasion of
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Australia and during the events that happened
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all the way through to the 1970s, there was a
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fairly aggressive attempt to, even if
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you weren't wiping out the people, to get rid
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of the culture and to get rid of the
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knowledge. I've just looked up Toowoomba
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where I am T o uh o uh w o uh o uh m b
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a I live about 20 ks west of there.
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Toowoomba is an indigenous name. It's a
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really interesting town because it's like the
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Florida of Queensland. All the old people
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come here to retire. It's a lovely place.
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It's a beautiful place because Queensland has
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a particular climate. But Toowoomba is
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a moderated version of that climate because
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it sits on the Great Dividing range at about
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700 meters above sea level. So it's not as
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humid as the coast. It doesn't get as hot as
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the coast. It has very lovely dry winters.
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Anyway, the name of Toowoomba is
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probably based on a word
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from likely the Gable or Jarawar
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peoples. Not entirely sure. But if you look
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around for the origin of Toowoomba as a word,
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there's lots of suggestions. There is a
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suggestion that it was a, ah, word for swamp
411
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because Toowoomba sits in this swampy area on
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top of the hills. According to the Toowoomba
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Regional Council, it may have been named
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after a property in the area in the 1850s,
415
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or it may have come from an Aboriginal word
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00:16:41.160 --> 00:16:43.000
meaning either place where water sits, which
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will be the swamp thing or place of melon, or
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place where reeds grow or berries place or
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white man. There are other things saying
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meeting of the waters or. Or saying. The name
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of Toowoomba may be an anglicized version of
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00:16:54.810 --> 00:16:57.770
the word bu wonga, which meant thunder in
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the dialect of the upper Burnett and Gaynda
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tribes. So we just don't know. And it does
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make me a little bit sad. We talk about
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indigenous astronomy a bit and the wonderful
427
00:17:06.170 --> 00:17:08.570
work that, um, Professor Duane Hamaker and
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his students have done over the years working
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00:17:10.250 --> 00:17:12.130
with the indigenous people of Australia. But
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it does make me sad how much of this
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knowledge is lost where you don't even know
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the origin of the name. So it's wonderful
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00:17:16.930 --> 00:17:19.439
that in this case we actually know where the
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name comes from. We can talk to that. So when
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you're looking at the map of Australia and
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think a lot of the places are unusual from
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the perspective of someone from an Anglo
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background or from a European background,
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00:17:29.799 --> 00:17:31.919
it's because even though it's a primarily
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English speaking country nowadays with a,
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with that, you know, Anglo heritage, a lot of
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the names are actually from the traditional
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owners, even if the heritage of that name
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itself is lost.
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Andrew Dunkley: Yes. Uh, where I live, Dubbo is
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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.
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00:17:54.460 --> 00:17:56.980
Uh, it is when you get a dust storm and
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everything turns red, uh,
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Jonti Horner: when it gets wet and you're bringing it in
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because the red soil marks horrible
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everything up, you know. Yeah. Dog goes out
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and gets their paws muddy and brings in red
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footprints.
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Andrew Dunkley: Red footprints on a light colored carpet. No,
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uh, terrible stuff. And of course one that
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relates to astronomy is warmera,
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which is an indigenous word for uh, the,
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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
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to have a specially made, um,
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I suppose you'd call it a, like a handheld
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catapult. And it, um,
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and, and it. Yeah, and it flung the spear at
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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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