Oct. 30, 2025
Jupiter's Cosmic Blueprint, White Dwarf Feasts & Chiron's Evolving Rings
Jupiter's Influence, Hungry White Dwarfs, and Chiron's Rings In this captivating episode of Space Nuts, hosts Andrew Dunkley and Professor Jonti Horner explore the dynamic forces shaping our solar system and beyond. From the pivotal role of Jupiter in...
Jupiter's Influence, Hungry White Dwarfs, and Chiron's Rings
In this captivating episode of Space Nuts, hosts Andrew Dunkley and Professor Jonti Horner explore the dynamic forces shaping our solar system and beyond. From the pivotal role of Jupiter in planetary formation to the intriguing behaviors of white dwarfs and the rapid evolution of Chiron's ring system, this episode is packed with cosmic revelations and scientific insights.
Episode Highlights:
- Jupiter's Role in the Solar System: Andrew and Jonti discuss a recent study that sheds light on how Jupiter's formation influenced the architecture of our solar system, potentially determining the locations and characteristics of the terrestrial planets. They delve into the gravitational effects Jupiter has on the inner solar system and how it may have created conditions favorable for planet formation.
- White Dwarf Devours Planetary Material: The hosts examine a fascinating case of a white dwarf star that has been observed consuming heavy elements from a planetesimal. They explain the implications of this discovery, including the potential for ongoing planetary activity around aging stars and what it suggests about the fate of planetary systems.
- Chiron's Evolving Ring System: The episode features a discussion about Chiron, the icy centaur that has recently been found to have a developing ring system. Andrew and Jonti explore the significance of this discovery, the potential origins of the rings, and what this tells us about the dynamic processes at play in the outer solar system.
- Exoplanet Life Candidates: The hosts wrap up with a critical look at claims surrounding a newly discovered exoplanet that is being touted as a potential candidate for life. They discuss the importance of scientific accuracy in media reporting and the implications of misrepresenting findings in the search for extraterrestrial life.
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, X, YouTube Music Music, Tumblr, Instagram, and TikTok. 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/po
In this captivating episode of Space Nuts, hosts Andrew Dunkley and Professor Jonti Horner explore the dynamic forces shaping our solar system and beyond. From the pivotal role of Jupiter in planetary formation to the intriguing behaviors of white dwarfs and the rapid evolution of Chiron's ring system, this episode is packed with cosmic revelations and scientific insights.
Episode Highlights:
- Jupiter's Role in the Solar System: Andrew and Jonti discuss a recent study that sheds light on how Jupiter's formation influenced the architecture of our solar system, potentially determining the locations and characteristics of the terrestrial planets. They delve into the gravitational effects Jupiter has on the inner solar system and how it may have created conditions favorable for planet formation.
- White Dwarf Devours Planetary Material: The hosts examine a fascinating case of a white dwarf star that has been observed consuming heavy elements from a planetesimal. They explain the implications of this discovery, including the potential for ongoing planetary activity around aging stars and what it suggests about the fate of planetary systems.
- Chiron's Evolving Ring System: The episode features a discussion about Chiron, the icy centaur that has recently been found to have a developing ring system. Andrew and Jonti explore the significance of this discovery, the potential origins of the rings, and what this tells us about the dynamic processes at play in the outer solar system.
- Exoplanet Life Candidates: The hosts wrap up with a critical look at claims surrounding a newly discovered exoplanet that is being touted as a potential candidate for life. They discuss the importance of scientific accuracy in media reporting and the implications of misrepresenting findings in the search for extraterrestrial life.
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, X, YouTube Music Music, Tumblr, Instagram, and TikTok. 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/po
WEBVTT
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Andrew Dunkley: Hello, thanks for joining us. This is Space
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Nuts. My name is Andrew Dunkley, and we're
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here to talk astronomy and space science. And
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on this episode, we are going to look at a
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study into Jupiter's role in shaping
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our solar system. What shape is that?
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It's rhomboid. No, we don't know. we're also
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going to look at a, white dwarf star that's
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chowing down on a planetesimal. Sounds
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appetizing. observing a rapidly
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developing ring system, and it's not far
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away. And if we've got time, an exoplanet
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that in inverted commas may
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be a life candidate. That's all coming up on
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space nuts. 15 seconds. Guidance is
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internal. 10, 9.
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Ignition sequence start. space nuts. 5, 4,
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3, 2. 1, 2, 3, 4, 5, 5,
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4, 3, 2, 1.
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Jonti Horner: Space nuts.
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Andrew Dunkley: Astronauts report it feels good. And it's
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good to have Jonti Horner back with us again.
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Professor of astrophysics at the University
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of Southern Queensland. Hi, Jonti.
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Jonti Horner: Good evening. How are you going?
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Andrew Dunkley: I am well. Good to see you.
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Jonti Horner: Oh, it's good to be back. Although I'm
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admittedly a bit of a zombie, so I warn
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everybody, I've had less sleep than I should
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have done in the last couple of days because
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of the weather. we had some weather happen on
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Sunday, which led to the power here being
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knocked out for 24 hours during a mini heat
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wave. So I didn't get much sleep then. And
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then this morning I've got a colleague from
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Japan visiting, so I had to pick him, his
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wife and their two lovely daughters up from
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Brisbane Airport. So I've had six hours of
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driving today off the back of two nights of
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not much sleep. So if I seem less coherent
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than normal, and I appreciate I'm normally
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not that coherent to begin with, you know
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why, of course.
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Andrew Dunkley: Yes, we've all been there. we've had dreadful
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weather here too. But it hasn't been the
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extreme heat, it's been the extreme wind.
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I got woken up, last night about
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1am by the Fly, screens rattling. It
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was so windy. Yes, they, they were just
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shuddering. And I thought, I can't live with
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this.
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Jonti Horner: So I went outside.
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Andrew Dunkley: It was freezing cold, supposed to be late
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spring here, and I
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just jammed some wood chips
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into the. I just went off to the
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garden and grabbed some mulch and shoved it
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in the wind in, in the fly screens to stop
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them rattling.
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Jonti Horner: It worked.
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Andrew Dunkley: I've done it better during the day, but,
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well, that's just Been ridiculous.
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Jonti Horner: I know your parents. I mean having said that
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we had heat wave conditions and couldn't
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sleep because of the heat, I'm happ confess
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that I've had the wood serve on today because
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having had 36, 38 degrees so
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that's around 100 for our American friends
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last few days. Today has been a toasty kind
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of 15 degrees. and we've got a rain event
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happening. so we've had everything in the
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last week we've had kind of almost tornadic
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storms, we've had hailstones the size of your
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fists, we've had under a kilometer an hour
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gusts and now we've got random cold that
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makes me feel like I'm back in the uk. So
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yeah, all happening. And this is why
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Australia is an interesting place to live
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even to the extent that with the
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thunderstorms. We had got an email through
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yesterday that our wonderful observatory,
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Queensland's only professional astronomical
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observatory in Mount Kent was closed
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yesterday. We weren't allowed to go there
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because there was a bushfire within 10km of
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it that had been sparked by the lightning
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from the storms and fanned by the heat wave
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in a place that got lightning but no rain. So
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ah, it's all happening here.
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Andrew Dunkley: Yes, dry storms are not uncommon where I am.
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We we do get quite a few storms every year
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with lightning and thunder and nothing else.
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and they, yeah, they're very well known for
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sparking bushfires.
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Jonti Horner: Yeah.
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So while we're on the diversion of the
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weather, actually I'll apologize for Maya the
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dog chirping in the background but my
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partner's just got home. But we're also
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sitting here with an incredibly heartbreaking
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record, record breaking storm in the
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Caribbean. Yes, I know she's just come
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home. Thank you for joining me with the
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podcast Happy Dog. but yeah, there's
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borderline record breaking storm in the
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Caribbean which is going to be a Category 5
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hurricane hitting Jamaica and doing a, ah,
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hell of a lot of damage. And it's one of
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these that from a scientist point of view,
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fascinating watching it looking at the radar
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footage and all the satellite footage and on
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one hand you've got this thing of incredible
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exceptional beauty and on the other hand the
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devastation it's going to cause. So the
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people in the, in the firing line for that.
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Andrew Dunkley: Yeah, I saw the satellite images this
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afternoon. It is enormous.
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Jonti Horner: Yeah, you look at the false color one
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with the color of the clouds which is an
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indication of the severity of the storm and
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the shape and it's the kind of thing that you
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only see with the strongest storms we've ever
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seen, typically in the Pacific. So for this
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thing to not only be happening in the
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Atlantic, which is less common, but
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to be, you know, crosshairs on Jamaica,
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which has had a bit of a charmed life with
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some sacks of the high mountains that tend to
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bounce and go around a bit. This one looks
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like it's not so much going to bounce a
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splat.
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Andrew Dunkley: So yeah, when we were in Panama earlier
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this year, we did the Panama Canal and
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they were saying that they never get
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hurricanes ever.
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Jonti Horner: Too equatorial is my understanding. You need
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to be far enough away from the equator to get
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enough spin so. So it's very rare that you
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get storms getting right up to the equator
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because coriolis force and things like that.
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Andrew Dunkley: Yeah, yeah, it's interesting, isn't it?
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Very interesting. Okay, we better get
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on with what we came here to get on with. And
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we're going to start with a study that's
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been released into Jupiter's role in shaping
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the solar system. Now I do recall Fred
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mentioning that Jupiter, if Jupiter
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didn't exist we wouldn't. And this study
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basically adds a lot of fuel to that claim.
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Jonti Horner: It does. Now where Fred said,
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Fred and other people talk about if Jupiter
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didn't exist then we probably wouldn't. Ties
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into something that's a pretty big
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myth in science communication, Ansel in
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science papers and stuff, which is the idea
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of Jupiter shielding us from impacts. And my
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most favorite piece of research I ever did in
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my career is proving that to be a lot of
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cobblers and it's actually a lot more
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complicated. Jupiter throws things at us as
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well as protecting us. So I've always got a
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bit of an eye on any study that says, hey
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guys, if Jupiter wasn't there, neither would
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we. But this is a really interesting one that
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looks an entirely different aspect of
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Jupiter, which is the role that Jupiter
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played on the formation and evolution of the
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early solar system, the formation of the
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planets. And I've actually been teaching
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planet formation this week to my undergrad
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students. I've just, prior to recording this,
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had a two hour tutorial with them where I've
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been talking about planet formation and
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brought this story up because it
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really highlights the fact that when we
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often see in documentaries and the stuff we
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get taught at school, we get the impression
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that everything's solved, that we know the
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answers, that we know full well how the
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planets formed in microscopic detail and
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we've got everything figured out and the
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Reality is that we haven't. We have a really
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good broad picture and we're getting better
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and better at understanding the processes
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that went on. But there's still a lot to
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learn. And part of that is that while we've
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known the solar system since the year dot,
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we've only known other planetary systems for
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the last 30 years. And in reality we're still
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learning an awful lot about the planetary
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systems we find elsewhere. And learning about
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them is cool and all, but it also gives us
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insights that help us better understand our
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planetary system and how it formed. And that
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ties into this because the more we
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study those other planetary systems, the more
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we're getting observations of really
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beautiful things like planetary systems that
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are in formation, where you've got a
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protoplanetary disk. And we're getting these
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gorgeous images from things like the
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ALMA array, the Ataccama Large Millimeter
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Array that shows disks of planet
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forming material around stars with gaps in
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them and ripples in them and bands in them,
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and all these beautiful structures. And some
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of these have been previous astronomy.
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Picture of the days where this ties into the
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solar system is if you imagine that kind of
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stereotypical image of a
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protoplanetary disk, a disk of gas and dust
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around a young star like the sun, where
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material is feeding in through that disk to
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the star. So while the gas and dust is
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orbiting the star, there is this kind of
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sense of inward motion where the stars kind
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of nominating at the inner edge of the disk,
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materials falling in, and more material from
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outside flowing in to replace it. Yeah, and
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some of the models of the formation of the
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solar system struggle to make the terrestrial
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planets as a result of that. Because the
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material in the inner solar system is
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destined to fall onto M the star. And how do
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you stop that happening to let that material
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hang around to actually form into planets?
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Now it's been pretty well established for a
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long time that the first planet that formed
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in the solar system and got to a good size
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was Jupiter. And there's good reasons for
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that. It formed far enough away from the sun
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that the temperature was cold enough that the
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disk was rich in ice, which at, the
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distance the Earth is from the sun, all that
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ice would be gas. when you're forming solid
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objects, you need solid objects to feed from.
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And so when you've got a lot of ice, you've
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got a lot more solids. So things grow
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quicker, there's a lot more to eat. And it's
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only when you get to about 10 or 12 times the
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Mass of the Earth that You're massive enough
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to effectively start gobbling up the gas as
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well. So Jupiter formed beyond this point
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called the snow line, where there's a lot
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more solid material. It got to grow really
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quickly. It grew quicker than things further
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out because the further out you go, the
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slower things happen. So Jupiter was very
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much in the sweet spot, grew really quickly
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and eventually got big enough that it started
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clearing the gas and the dust it could gather
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the gas as well. And it opened up a gap in
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the disk. And that's very analogous to what
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we're seeing with these beautiful images from
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ALMA places like this. So the team of
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researchers behind this work have run some
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really in depth computer modeling of the
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formation of the solar system formation of
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Jupiter, and showed that when Jupiter opens
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up the gap in the disk, its gravity will
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also have an impact on the inner solar
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system. It'll effectively create the
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gravitational equivalent of speed bumps,
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creating areas where the dust that's
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spiraling inwards can pile up and be
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stopped from traveling further in.
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Effectively. It also creates
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a gap between the in run out of solar system
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that nothing crosses because if anything gets
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in that gap, Jupiter noms on it. And that's
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really interesting because some studies that
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have looked at primordial material we've
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found from in the solar system suggests that
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there is a bit of a chemical difference
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between material that formed in the inner
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solar system and material that formed in the
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outer solar system. So this gap
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dividing the two gives a natural way for that
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to happen. But the really big exciting result
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from this is really that modeling of
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the structure that Jupiter would have imposed
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on the inner solar system. These kind of pile
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up regions where you get more m dust and
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debris than normal, the structures that, that
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would carve out ripples in the disk
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effectively and how that would then
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contribute to the formation of the
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terrestrial planets. and therefore suggesting
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that not only did Jupiter help the
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terrestrial planets form by creating sweet
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spots where material could pile up, but it
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may also have had a really strong influence
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on the architecture of the inner solar system
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by setting where the planets would form,
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which then would go through a bit of a
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randomization phase as everything collides
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with each other. But it kind of possibly set
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the blueprint for the inner solar system. And
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therefore, if Jupiter hadn't formed where it
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did and how it did, the Earth would look
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very, very different and we might not be
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here.
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Andrew Dunkley: Yeah, it's truly fascinating. And
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when you look at other systems that
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we've discovered, exoplanet solar systems,
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ours is starting to look a little bit more
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unusual than normal. and
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Jupiter may be the reason.
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Jonti Horner: It could well be. And it's one of those
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things, I'm reminded of the Monty Python
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thing. I think it's in Life of Brian, where
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you've got that thing of we're all
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individuals. Yes, we're. No, we're not. I'm
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not. Every
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planetary system is going to be unique
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because it is influenced by
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such a wide variety of things going on. Even
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the stars that form in the local
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neighborhood, whittling it away from the
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outside, it all starts going on. But what
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we're seeing is there's a commonality among a
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lot of the planetary systems that we find
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that look very different to ours.
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The thing that gives us a little bit of pause
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though, is that we have these observational
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biases that make us more likely to find
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systems that are different to ours than we
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are to find systems like ours. And so you've
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always got that question of do we look
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unusual because we are unusual,
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or do we look unusual because we're not yet
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very good at finding places that look like
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home? and that's where colleagues of mine,
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like professor, Rob Wittenmayer, my colleague
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at unisq, have done really interesting
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work where what they
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do is look at what we found, but work
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out what doesn't exist
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based on what we haven't found yet. So they
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can start getting an estimate of how common
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our, ah, planetary systems like ours based on
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the fact we haven't found them yet. And it's
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a really kind of weird type of science where
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the absence of finding thing places limits on
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how common that thing is. So if you said
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that every star had a planet exactly like the
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Earth, on an orbit that's one year long that
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is exactly the same size as us and all the
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rest of it, then we can work out
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statistically, based on how good our
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telescopes are and our techniques are, how
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many of those planets we would have found.
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And we wouldn't have found anywhere near all
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of them because it's really hard to do. But
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we'd have found X amount. And the fact that
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we've only found a very small number smaller
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than that places an upper limit on how common
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things can be. So you get this perverse
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science where you get the observations
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that tell us what we found and what we've
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seen, but you can also put inferences on
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what isn't there and what is there based on
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what we haven't found yet, which allows you
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to put limits on how common things are that
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you couldn't really find very easily. Which,
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if that makes your head hurt. it makes my
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head hurt a little bit as well. But it's a
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really kind of clever use of the data we get
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to extrapolate further and draw more
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conclusions. And the net result of that is
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that the solar system is not hugely rare, but
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it's not common either. It's usual.
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And, that's really cool. And that probably
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extends to everything. Like I say, we're all
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individuals. The Earth, even though it's
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peeing it down outside at the minute, the
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Earth's actually a very dry planet. If you
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took all the water off the Earth and made a
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little blob of it next to the Earth, that
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blob would be fairly tiny. And everybody
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views the Earth as being very wet, but I view
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it as being very dry because water is such a
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common compound in the universe. It's made of
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the first and third most common atom. You put
384
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them together. Yet water waters everywhere.
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So for the Earth to be as dry as it is is
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telling you a lot about the uniqueness of the
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solar system. And maybe that's partially
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because of Jupiter. Not, necessarily
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shielding us from impacts, but preventing
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that icy material spiraling in, preventing
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us from becoming an ocean world. It's also
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partly down to the moon forming impact. The
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moon forming impact would have stripped a lot
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of the primordial Earth's water away because
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it walked as light and sits near the surface.
396
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So a lot about our Earth and a lot about the
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solar system is down to the random nature of
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the events around us. When we formed the moon
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forming impact, a nearby star going
400
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supernova and lacing our solar system with
401
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radioactive aluminium. Things like this.
402
00:15:17.840 --> 00:15:19.400
There's all these oddities that made our
403
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solar system unique, but if those
404
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hadn't happened, other things would have
405
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happened and we'd have still ended up with
406
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something unique because of other random
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things happening.
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It's all fascinating and I just love this
409
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stuff.
410
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Andrew Dunkley: Yeah. And it adds more and more weight to the
411
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theory that we are just a freak accident.
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Jonti Horner: Yes.
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Andrew Dunkley: And probably a one off in the universe.
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That's one argument. So, yeah,
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who knows if, if we find a
416
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solar system just like ours, with a planet
417
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just like ours, orbiting a
418
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star just like ours. That would be
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the, you know, one of the greatest
420
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discoveries in astronomical history, I
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imagine. But no, we do that.
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Jonti Horner: We would have to get in touch with the planet
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builders at Magrathea and demand that money
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back. Because we thought we had a limited
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edition.
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Andrew Dunkley: Yes, yes. weren't they the white mice? Was
427
00:16:09.350 --> 00:16:10.270
that the white mice?
428
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Jonti Horner: Yes, it was.
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Andrew Dunkley: Yeah. All right, if you want to read all
430
00:16:13.320 --> 00:16:15.880
about it, you can find, the paper,
431
00:16:16.540 --> 00:16:19.240
which was published in the journal Science
432
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Advances.
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Jonti Horner: Roger, your labs are here. Also space nuts.
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Andrew Dunkley: now, Jonti, let's move on to our next story.
435
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And this one is about a planetismal,
436
00:16:32.190 --> 00:16:35.110
that appears doomed. According to the, paper
437
00:16:35.110 --> 00:16:37.190
I'm reading, it's a white dwarf that's
438
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chowing down very, very hungry, hungry
439
00:16:39.790 --> 00:16:40.990
individual is this one.
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00:16:41.790 --> 00:16:44.270
Jonti Horner: It is. So just to remind the audience, a
441
00:16:44.270 --> 00:16:47.030
white dwarf is the kind of little husk
442
00:16:47.030 --> 00:16:48.990
that's left after a cell like our sun comes
443
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to the end of its life, burns all its
444
00:16:51.430 --> 00:16:53.870
hydrogen, becomes a red giant, and then
445
00:16:53.870 --> 00:16:55.750
eventually blows off its outer layers. And it
446
00:16:55.750 --> 00:16:58.110
leaves a big chunk of the star's mass
447
00:16:58.510 --> 00:17:00.350
compressed into an object about the size of
448
00:17:00.350 --> 00:17:03.270
the Earth. That whole process will
449
00:17:03.270 --> 00:17:05.870
have a fairly hefty impact on the
450
00:17:05.870 --> 00:17:07.870
planetary system that star's got around it.
451
00:17:08.230 --> 00:17:09.710
And of course, as we just discussed, we now
452
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know that pretty much every star has planets.
453
00:17:12.150 --> 00:17:14.310
The expectation is that when the sun reaches
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this stage, unfortunately it's in about 7
455
00:17:16.350 --> 00:17:18.060
billion years, so nothing to worry about.
456
00:17:18.060 --> 00:17:20.700
Immediately it will swell up and it will
457
00:17:20.860 --> 00:17:23.020
chow down on Mercury and chow down on Venus.
458
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They'll just be swallowed up and gone. Yeah,
459
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There is some debate over whether the Earth
460
00:17:27.700 --> 00:17:30.300
will be swallowed up or will survive. Just
461
00:17:31.100 --> 00:17:33.230
all the models of star, evolution suggest
462
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that the sun will swell up to be about the
463
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radius of the Earth's orbit. But whether the
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00:17:37.510 --> 00:17:39.390
Earth is there to nominal or not is still
465
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open for debate. It may be that the loss of
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mass from the sun in the time before may just
467
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mean that the Earth nudges far enough away to
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survive as a burnt husk rather than be
469
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devoured. It still would be ideal
470
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to be around when that wouldn't be pleasant.
471
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I mean, that said, the Earth is going to
472
00:17:54.630 --> 00:17:56.870
become uninhabitable a lot sooner than that
473
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because the Sun's getting brighter and the
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Earth's oceans will boil and it'll all go
475
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downhill. But after all that process
476
00:18:04.460 --> 00:18:06.700
happens when the sun sheds its outer layers,
477
00:18:07.020 --> 00:18:09.380
that'll have a pretty cataclysmic event on
478
00:18:09.380 --> 00:18:12.060
the planets and the debris that are left. So
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suddenly the sun goes on the ultimate kind of
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weight loss kick loses mass. And that
481
00:18:16.860 --> 00:18:18.860
will mean that all of the objects going
482
00:18:18.860 --> 00:18:21.300
around the sun will be held less strongly.
483
00:18:21.300 --> 00:18:23.020
And so therefore their orbits will move
484
00:18:23.020 --> 00:18:25.700
outwards because the gravity pulling them in
485
00:18:25.700 --> 00:18:28.580
gets weaker. Now, if you suddenly Press the
486
00:18:28.580 --> 00:18:30.960
button and vanished half of the mass of the
487
00:18:30.960 --> 00:18:33.560
Sun. What had happened is that the speed that
488
00:18:33.560 --> 00:18:35.720
any of the objects are going in their orbit
489
00:18:35.880 --> 00:18:37.680
will be too quick for that orbit to be
490
00:18:37.680 --> 00:18:40.520
circular. So at that instant, at that
491
00:18:40.520 --> 00:18:43.040
point, they'd now be at their new perihelion,
492
00:18:43.040 --> 00:18:44.560
they'd be at their closest point to the sun,
493
00:18:44.560 --> 00:18:45.960
and they'd all move out onto much more
494
00:18:45.960 --> 00:18:48.520
elongated orbits with a longer orbital
495
00:18:48.520 --> 00:18:51.200
period, but orbits that would then cross one
496
00:18:51.200 --> 00:18:53.640
another. So if you imagine you lose half of
497
00:18:53.640 --> 00:18:56.320
the Sun's mass, Jupiter moves onto an orbit
498
00:18:56.320 --> 00:18:58.480
where its perihelion is 5 au from the sun,
499
00:18:58.480 --> 00:19:00.840
but its aphelion could be 15 au from the Sun.
500
00:19:01.400 --> 00:19:03.760
Saturn at the same time would have perihelion
501
00:19:03.760 --> 00:19:06.120
at 10 au and aphelion at say 20 au. And I'm
502
00:19:06.120 --> 00:19:08.440
making the numbers up a bit here. So suddenly
503
00:19:08.440 --> 00:19:11.199
Jupiter and Saturn are on orbits that
504
00:19:11.199 --> 00:19:14.120
cross one another. Their orbits
505
00:19:14.120 --> 00:19:16.520
will probably still have the same ratio of
506
00:19:16.520 --> 00:19:19.400
orbital periods, so 12 years to 29 years. But
507
00:19:19.400 --> 00:19:21.290
they'd scale up to be something like, I don't
508
00:19:21.290 --> 00:19:23.650
know, 30 to 70 or something like that,
509
00:19:23.970 --> 00:19:25.570
because they've both moved out by the same
510
00:19:25.570 --> 00:19:27.650
amount. But suddenly you've got these planets
511
00:19:27.650 --> 00:19:29.450
that are on orbits that cross each other and
512
00:19:29.450 --> 00:19:32.130
therefore can really strongly interact. They
513
00:19:32.130 --> 00:19:33.890
can stir everything else up because all of
514
00:19:33.890 --> 00:19:35.570
the objects in the asteroid belt, all of the
515
00:19:35.570 --> 00:19:37.330
objects beyond Neptune, this happens to
516
00:19:37.330 --> 00:19:39.770
everything. Now the mass loss is a bit more
517
00:19:39.770 --> 00:19:42.330
gradual than that in actuality. So what
518
00:19:42.330 --> 00:19:44.370
happens is you get the orbit spiraling out,
519
00:19:44.370 --> 00:19:46.170
but getting perturbed, being made more
520
00:19:46.170 --> 00:19:48.640
eccentric. You've also got these objects
521
00:19:48.640 --> 00:19:51.240
moving through the headwind of possibly half
522
00:19:51.240 --> 00:19:53.200
a solar mass of material being blown
523
00:19:53.200 --> 00:19:55.560
outwards. That provides friction and so
524
00:19:55.560 --> 00:19:57.720
causes them possibly to spiral inwards a bit.
525
00:19:58.520 --> 00:20:00.760
Causes Jupiter potentially to gather mass as
526
00:20:00.760 --> 00:20:03.400
it numbs on all that gas that's going out. At
527
00:20:03.400 --> 00:20:04.960
the same time, its atmosphere is probably
528
00:20:04.960 --> 00:20:07.360
being blasted away by all this wind blowing
529
00:20:07.360 --> 00:20:10.280
past. All of this complexity means
530
00:20:10.280 --> 00:20:12.200
that you couldn't predict with absolute
531
00:20:12.200 --> 00:20:14.080
certainty what the solar system would look
532
00:20:14.080 --> 00:20:16.920
like at the end of this, but certainly
533
00:20:16.920 --> 00:20:19.320
there'd be a period of chaos. A lot of stuff
534
00:20:19.320 --> 00:20:21.800
would survive, but it would survive on orbits
535
00:20:21.800 --> 00:20:24.520
that are now much more unstable. So you get a
536
00:20:24.520 --> 00:20:26.570
lot of material flung inwards and, some of
537
00:20:26.570 --> 00:20:29.170
that will be flung inwards far enough for it
538
00:20:29.170 --> 00:20:31.370
to impact on the Earth sized object in the
539
00:20:31.370 --> 00:20:33.700
middle and, for the white dwarf to get a
540
00:20:33.700 --> 00:20:36.300
snack. Now all that's expected to happen
541
00:20:36.300 --> 00:20:38.860
really early on. And over time everything
542
00:20:38.860 --> 00:20:41.530
stabilizes out, things get flung around and
543
00:20:41.530 --> 00:20:44.250
clean up happens a bit like the
544
00:20:44.250 --> 00:20:45.730
solar system. You know, we were talking early
545
00:20:45.730 --> 00:20:47.170
on about the early stages of planet
546
00:20:47.170 --> 00:20:49.090
formation. Everything gets flung around and
547
00:20:49.090 --> 00:20:51.210
by the time you get to now, four and a half
548
00:20:51.210 --> 00:20:52.770
billion years down the road, it's fairly
549
00:20:52.770 --> 00:20:55.210
quiet. There's a bit going on, but most of
550
00:20:55.210 --> 00:20:57.730
the drama's finished. So the
551
00:20:57.730 --> 00:20:59.730
expectation is you'd see white dwarfs that
552
00:20:59.730 --> 00:21:02.450
are very young occasionally eating things
553
00:21:02.450 --> 00:21:04.650
because things get flung in and they get a
554
00:21:04.650 --> 00:21:06.780
bit of a snack. And the material from that
555
00:21:06.780 --> 00:21:08.820
snack will be spattered over the surface of
556
00:21:08.820 --> 00:21:10.980
the white dwarf and be visible in its
557
00:21:10.980 --> 00:21:13.620
spectrum as anomalous added
558
00:21:14.100 --> 00:21:16.420
solid material, heavy elements.
559
00:21:17.140 --> 00:21:19.300
But that signal would only last a short time
560
00:21:19.300 --> 00:21:21.220
because the outer layer of the white dwarf is
561
00:21:21.220 --> 00:21:24.220
kind of a hydrogen soup and heavier elements
562
00:21:24.220 --> 00:21:27.140
would sink down. So any given time you'd eat
563
00:21:27.140 --> 00:21:29.660
something. The evidence for that meal would
564
00:21:29.660 --> 00:21:31.740
only remain for a few tens of thousands of
565
00:21:31.740 --> 00:21:34.650
years, SOPs before it goes away. Okay, so
566
00:21:34.650 --> 00:21:36.530
the fact is we've seen some white dwarfs
567
00:21:36.530 --> 00:21:38.810
which have these anomalous heavy element
568
00:21:38.810 --> 00:21:41.010
readings in their atmospheres. We can tell
569
00:21:41.010 --> 00:21:42.690
they're eating stuff, but typically they're
570
00:21:42.690 --> 00:21:45.450
young. So you'd expect that.
571
00:21:45.930 --> 00:21:48.010
The quirky thing here is that this white
572
00:21:48.010 --> 00:21:49.850
dwarf, which goes by the name of
573
00:21:49.850 --> 00:21:52.820
lspm, which I think is a survey name,
574
00:21:52.820 --> 00:21:54.010
m followed by
575
00:21:54.010 --> 00:21:57.770
J020733331.
576
00:21:58.330 --> 00:22:00.210
So that's a coordinate on the sky. So that's
577
00:22:00.210 --> 00:22:01.690
telling you where in the sky this is. It's
578
00:22:01.690 --> 00:22:04.390
catalog number. Yeah, this thing is an old
579
00:22:04.390 --> 00:22:06.310
white dwarf. It's thought to be about 3
580
00:22:06.310 --> 00:22:08.350
billion years old. So in other words, the
581
00:22:08.350 --> 00:22:11.230
star that formed it died 3
582
00:22:11.230 --> 00:22:13.510
billion years ago and it's been sitting there
583
00:22:13.510 --> 00:22:16.390
minding its own business. That's old enough
584
00:22:16.390 --> 00:22:18.070
that you'd expect everything to have calmed
585
00:22:18.070 --> 00:22:20.910
down around it. But what the new
586
00:22:20.910 --> 00:22:23.870
observations have shown is evidence of
587
00:22:23.870 --> 00:22:25.870
13 different heavy elements,
588
00:22:26.670 --> 00:22:28.750
including carbon, chromium,
589
00:22:29.980 --> 00:22:32.220
strontium, titanium, a lot of these different
590
00:22:32.220 --> 00:22:35.100
elements, roughly in the kind of abundance as
591
00:22:35.100 --> 00:22:37.630
you'd see on the Earth, added, to this white
592
00:22:37.630 --> 00:22:40.230
dwarf's atmosphere. So it's
593
00:22:40.230 --> 00:22:42.350
obviously just had a meal and we know it's a
594
00:22:42.350 --> 00:22:44.470
case of just had a meal rather than it's been
595
00:22:44.470 --> 00:22:47.190
a leftover from a long time ago, because this
596
00:22:47.190 --> 00:22:49.150
stuff will sink and disappear over the next
597
00:22:49.150 --> 00:22:52.110
few tens of thousands of years. So what
598
00:22:52.110 --> 00:22:54.190
that means is that this white dwarf
599
00:22:55.020 --> 00:22:57.380
has just had a snack. Now it might have had
600
00:22:57.380 --> 00:23:00.220
that snack 30,000 years ago, or it
601
00:23:00.220 --> 00:23:03.020
may still be in the process of eating as
602
00:23:03.020 --> 00:23:05.820
we speak. Now what the team have been able to
603
00:23:05.820 --> 00:23:08.340
do is look at the amount of material you'd
604
00:23:08.340 --> 00:23:10.140
need to give the strength of signal you've
605
00:23:10.140 --> 00:23:12.080
got in the spectrum of the star. And, what
606
00:23:12.080 --> 00:23:14.320
they've calculated is that to get this amount
607
00:23:14.320 --> 00:23:17.080
of material you'd need to eat an asteroid
608
00:23:17.800 --> 00:23:19.960
about 200 kilometers in diameter.
609
00:23:20.760 --> 00:23:22.520
So that's comparable to some of the larger
610
00:23:22.520 --> 00:23:24.200
asteroids in the asteroid belt, but not the
611
00:23:24.200 --> 00:23:26.920
largest by any means. It's within the bounds
612
00:23:26.920 --> 00:23:28.680
of possibility of what we see here at home.
613
00:23:29.080 --> 00:23:31.160
But the real question is why is it eating it
614
00:23:31.160 --> 00:23:33.520
now? Why is this happening now when you'd
615
00:23:33.520 --> 00:23:35.200
expect the system to have had plenty of time
616
00:23:35.200 --> 00:23:37.560
to calm down? What
617
00:23:37.960 --> 00:23:40.760
it suggests to me, and it suggests in the
618
00:23:40.760 --> 00:23:42.960
paper, it suggests in the articles about this
619
00:23:42.960 --> 00:23:45.240
as well, is that the only way you can get
620
00:23:45.240 --> 00:23:48.070
something eating this late, after 3 billion
621
00:23:48.070 --> 00:23:50.830
years have passed, is if you've still got a
622
00:23:50.830 --> 00:23:53.310
number of planet mass objects in the system
623
00:23:53.310 --> 00:23:56.230
serving things up, which is what we've got
624
00:23:56.230 --> 00:23:57.910
in the solar system. If we look at the inner
625
00:23:57.910 --> 00:24:00.270
solar system, fragments of comets and
626
00:24:00.270 --> 00:24:02.070
asteroids are falling onto the sun all the
627
00:24:02.070 --> 00:24:04.350
time. We've got near Earth asteroids, short
628
00:24:04.350 --> 00:24:06.390
period comets and long period comets whizzing
629
00:24:06.390 --> 00:24:08.760
around. And, they're being bounced around by
630
00:24:08.760 --> 00:24:10.480
the planets. Jupiter's throwing a lot of
631
00:24:10.480 --> 00:24:12.920
stuff away. Their orbits are constantly
632
00:24:12.920 --> 00:24:15.800
getting tweaked. And so therefore the sun
633
00:24:15.800 --> 00:24:18.640
is still getting this rain of solid material
634
00:24:18.640 --> 00:24:20.880
falling on it as a result of the planets
635
00:24:20.880 --> 00:24:23.560
stirring things up. Even though the solar
636
00:24:23.560 --> 00:24:25.760
system mostly quietened down, the planets are
637
00:24:25.760 --> 00:24:28.320
still injecting material to the inner solar
638
00:24:28.320 --> 00:24:30.760
system, which is why we're getting meteorites
639
00:24:30.760 --> 00:24:32.400
and it's why the sun occasionally gets to
640
00:24:32.400 --> 00:24:35.120
numb some stuff. The idea here is
641
00:24:35.120 --> 00:24:37.400
that this star reached the end of its life.
642
00:24:37.400 --> 00:24:40.260
Puff dots with its outer layers. You have
643
00:24:40.260 --> 00:24:42.260
this really chaotic period where everything
644
00:24:42.260 --> 00:24:44.820
had got stirred up, then it settled down. But
645
00:24:44.820 --> 00:24:46.660
because you still got planet mass objects
646
00:24:46.660 --> 00:24:49.020
there, they're still bouncing around what
647
00:24:49.020 --> 00:24:51.620
debris is left. And we're just catching this
648
00:24:51.620 --> 00:24:54.460
white dwarf just at the right time, when
649
00:24:54.460 --> 00:24:56.740
another asteroid has been flung inwards close
650
00:24:56.740 --> 00:24:59.100
enough to be torn apart by the star's gravity
651
00:24:59.260 --> 00:25:01.900
and to give it a snack. So in other words,
652
00:25:02.220 --> 00:25:04.460
seeing this snack happening this late in the
653
00:25:04.460 --> 00:25:07.060
life of this white dwarf is fairly strong
654
00:25:07.060 --> 00:25:09.500
evidence that planets survived the death of
655
00:25:09.500 --> 00:25:12.140
its star, have lived there for 3 billion
656
00:25:12.140 --> 00:25:14.460
years, which a is really cool in of itself.
657
00:25:14.460 --> 00:25:17.380
But it also means that here is a star that we
658
00:25:17.380 --> 00:25:19.860
should look at when the Gaia data release
659
00:25:19.940 --> 00:25:22.500
comes next year. Gaia Dr. AH4,
660
00:25:22.980 --> 00:25:24.780
which will have been measuring this star's
661
00:25:24.780 --> 00:25:26.460
position on the sky. And if there Are planets
662
00:25:26.460 --> 00:25:28.220
there, we'll be able to detect the wobble and
663
00:25:28.220 --> 00:25:31.100
confirm them. So it's also holding up a flag
664
00:25:31.100 --> 00:25:33.760
to exoplanet people saying,
665
00:25:33.920 --> 00:25:36.520
hey, folks, here's a target for you to look
666
00:25:36.520 --> 00:25:38.320
at when the data release comes out where you
667
00:25:38.320 --> 00:25:39.840
might be able to find some planets, because
668
00:25:39.840 --> 00:25:42.240
we think there's a smoking gun here that the
669
00:25:42.240 --> 00:25:44.600
planets are feeding the white dwarf, giving
670
00:25:44.600 --> 00:25:46.160
it little snacks every now and again.
671
00:25:47.120 --> 00:25:49.040
Andrew Dunkley: Okay, wow. All right.
672
00:25:49.040 --> 00:25:51.950
so are there many white dwarf
673
00:25:52.030 --> 00:25:54.830
stars out there? What, do they, sort of,
674
00:25:55.870 --> 00:25:58.560
percentage wise, inhabit the star field?
675
00:25:58.720 --> 00:26:01.480
Jonti Horner: There would be a fair few of them. So the
676
00:26:01.480 --> 00:26:03.600
more massive a star is, the shorter its life
677
00:26:03.600 --> 00:26:05.850
is. And, that's a really rapid function.
678
00:26:06.330 --> 00:26:08.860
Where that works is, if your star's more
679
00:26:08.860 --> 00:26:11.420
massive, its gravitational pull is stronger,
680
00:26:11.980 --> 00:26:14.940
so its ability to pull material into
681
00:26:14.940 --> 00:26:17.900
the middle of the star is higher, which means
682
00:26:17.900 --> 00:26:19.780
that that star's got to give off a lot more
683
00:26:19.780 --> 00:26:21.900
energy to balance that gravitational pull.
684
00:26:21.900 --> 00:26:24.140
And so stars in the main sequence part of
685
00:26:24.140 --> 00:26:26.690
their life are in equilibrium. The radiation
686
00:26:26.690 --> 00:26:28.330
coming out from the nuclear fusion in the
687
00:26:28.330 --> 00:26:31.250
middle balances gravity pulling in. The
688
00:26:31.250 --> 00:26:33.730
more massive you are, the hotter and denser
689
00:26:33.730 --> 00:26:35.490
you get in the middle, so the more energy you
690
00:26:35.490 --> 00:26:38.250
give off. And the result of that is that it
691
00:26:38.650 --> 00:26:40.809
roughly, it varies a little bit by star's
692
00:26:40.809 --> 00:26:42.850
mass, but roughly the brightness of a star,
693
00:26:42.850 --> 00:26:45.570
the luminosity of a star is proportional to
694
00:26:45.570 --> 00:26:47.050
the mass of the star to the power
695
00:26:47.050 --> 00:26:49.890
4.3.54. Which means if you
696
00:26:49.890 --> 00:26:52.480
double the mass of a star, it'll get between
697
00:26:52.480 --> 00:26:54.560
10 and 16 times brighter.
698
00:26:55.440 --> 00:26:58.240
So twice the mass, Call it a factor of 10
699
00:26:58.240 --> 00:26:59.960
just to keep it easy. If it's 10 times
700
00:26:59.960 --> 00:27:02.600
brighter, that means it's burning its fuel 10
701
00:27:02.600 --> 00:27:04.880
times quicker to produce 10 times as much
702
00:27:04.880 --> 00:27:07.120
energy. But it's only twice the mass, so it's
703
00:27:07.120 --> 00:27:09.920
only got twice as much fuel, so its
704
00:27:09.920 --> 00:27:11.920
life will be a factor of five times shorter.
705
00:27:12.080 --> 00:27:13.800
And the more massive you get, the shorter the
706
00:27:13.800 --> 00:27:16.640
life gets. Now, stars of different masses
707
00:27:16.720 --> 00:27:19.330
have different. A star like Proxima
708
00:27:19.330 --> 00:27:21.770
Centauri will never swell up to become a red
709
00:27:21.770 --> 00:27:23.490
giant. It'll just be a dull, glowing ember
710
00:27:23.490 --> 00:27:26.090
and eventually go out. But even the
711
00:27:26.090 --> 00:27:28.570
oldest stars like Proxima Centauri are still
712
00:27:28.730 --> 00:27:30.370
really in their youth because they're burning
713
00:27:30.370 --> 00:27:33.170
their fuel so slowly. Stars that are more
714
00:27:33.170 --> 00:27:35.050
massive eventually get stars like the sun,
715
00:27:35.050 --> 00:27:37.520
which are what form like dwarfs. And, they
716
00:27:37.680 --> 00:27:39.600
eventually swell up to become a red giant,
717
00:27:39.600 --> 00:27:41.680
puff off their outer layers. And for a star
718
00:27:42.000 --> 00:27:44.930
of the Sun's mass, that process from
719
00:27:44.930 --> 00:27:46.770
forming to the end of its life is thought to
720
00:27:46.770 --> 00:27:49.010
be about 12 billion years. It used to be 10
721
00:27:49.010 --> 00:27:51.130
billion models seem to have refined. So
722
00:27:51.130 --> 00:27:52.730
people nowadays seem to say it's about 12
723
00:27:52.730 --> 00:27:55.690
billion years. So a star of
724
00:27:55.690 --> 00:27:58.180
the mass of the sun that formed when our,
725
00:27:58.180 --> 00:28:00.740
Milky Way was very young will have lived and
726
00:28:00.740 --> 00:28:02.900
died and become a white dwarf more than a
727
00:28:02.900 --> 00:28:05.860
billion years ago. But stars more massive
728
00:28:05.860 --> 00:28:08.180
than the sun can form white dwarfs as well,
729
00:28:08.180 --> 00:28:10.750
up to maybe two or even three times the mass
730
00:28:10.750 --> 00:28:12.590
of the sun, depending how effective it is at
731
00:28:12.590 --> 00:28:14.870
shedding mass at the end. Yeah, the maximum
732
00:28:14.870 --> 00:28:17.070
mass for white dwarf, you can get about 1.4
733
00:28:17.070 --> 00:28:19.390
times the mass of the Sun. If stars lose half
734
00:28:19.390 --> 00:28:20.750
their mass, that gives you something about
735
00:28:20.750 --> 00:28:22.710
three times the mass of the sun before you
736
00:28:22.710 --> 00:28:25.430
start it. Three times the mass of the sun.
737
00:28:26.150 --> 00:28:28.230
Three to the power four is three times three
738
00:28:28.230 --> 00:28:30.430
times three times three. That's 81 if my
739
00:28:30.430 --> 00:28:33.030
mental arithmetic is correct. So three times
740
00:28:33.030 --> 00:28:35.270
the mass of the sun burns its fuel 81 times
741
00:28:35.270 --> 00:28:38.050
as quickly, which means it would live a 27th
742
00:28:38.050 --> 00:28:40.930
as long. Which means instead of 12 billion
743
00:28:40.930 --> 00:28:43.400
years, you get down to, 1.2 billion years,
744
00:28:43.400 --> 00:28:45.360
you get down to or like, 600 million years,
745
00:28:45.440 --> 00:28:48.200
500 million years. So there will have been a
746
00:28:48.200 --> 00:28:50.520
lot of stars that were more m massive than
747
00:28:50.520 --> 00:28:52.560
the sun that have lived and died and created
748
00:28:52.560 --> 00:28:54.960
white dwarfs. And so there's going to be a
749
00:28:54.960 --> 00:28:57.880
lot of white dwarfs out there. I saw
750
00:28:57.880 --> 00:29:00.120
someone talking a while back about how old
751
00:29:00.120 --> 00:29:02.760
the oldest white dwarf will be in how dim it
752
00:29:02.760 --> 00:29:04.680
will be, because white dwarfs just cool and
753
00:29:04.680 --> 00:29:07.240
gradually go from being blue to white to
754
00:29:07.240 --> 00:29:09.360
yellow to red. You know, gradually dim down.
755
00:29:09.680 --> 00:29:11.910
Yeah. but what that all means is that there
756
00:29:11.910 --> 00:29:14.350
are probably a really large population of
757
00:29:14.350 --> 00:29:16.190
white dwarfs out there. We know quite a large
758
00:29:16.190 --> 00:29:19.030
number, but we won't know anywhere near
759
00:29:19.030 --> 00:29:21.230
as many of them as we do stars that are
760
00:29:21.230 --> 00:29:22.630
actually the mass of the sun, that are in the
761
00:29:22.630 --> 00:29:24.990
prime of their life because they're much
762
00:29:24.990 --> 00:29:27.110
fainter and harder to spot because they've
763
00:29:27.110 --> 00:29:28.670
got a much smaller surface area. So even
764
00:29:28.670 --> 00:29:30.130
though they're hot, they're tiny and,
765
00:29:30.080 --> 00:29:31.940
therefore they're faint. and the best example
766
00:29:31.940 --> 00:29:33.860
of that, of course, is a white dwarf that is
767
00:29:33.860 --> 00:29:36.220
a companion to Sirius. Sirius is the
768
00:29:36.220 --> 00:29:38.020
brightest star in the night sky. It's more
769
00:29:38.020 --> 00:29:40.860
massive than the Sun. It's also nearby. Its
770
00:29:41.100 --> 00:29:44.060
white dwarf companion is something
771
00:29:44.060 --> 00:29:46.940
like a factor of a million times fainter than
772
00:29:46.940 --> 00:29:49.500
Sirius is. So even though the white dwarf is
773
00:29:49.500 --> 00:29:51.660
comparable in Master Sirius A,
774
00:29:52.300 --> 00:29:55.060
it is like a million times dimmer because
775
00:29:55.060 --> 00:29:57.220
it's so tiny. And that's why they're Hard to
776
00:29:57.220 --> 00:29:57.500
find.
777
00:29:58.270 --> 00:30:00.070
Andrew Dunkley: Yeah, even though there's probably a hell of
778
00:30:00.070 --> 00:30:02.980
a lot of them out there. Okay, if you would
779
00:30:02.980 --> 00:30:05.180
like to read more about this particular white
780
00:30:05.180 --> 00:30:08.050
dwarf star that is, you know, got a case of
781
00:30:08.050 --> 00:30:10.610
the munchies, probably spent too much time
782
00:30:10.770 --> 00:30:13.360
smoking the juju. you can read all about it
783
00:30:14.240 --> 00:30:17.200
in the Astronomical Journal. This is Space
784
00:30:17.200 --> 00:30:20.080
Nuts with Andrew Dunkley and Jonti Horner.
785
00:30:20.240 --> 00:30:22.680
Jonti Horner: Okay, we checked all four systems and being
786
00:30:22.680 --> 00:30:24.170
with the jerk space nets,
787
00:30:25.140 --> 00:30:26.600
Andrew Dunkley: Don'T know why we went down that road.
788
00:30:26.600 --> 00:30:29.280
Let's go to our next story. And this
789
00:30:29.280 --> 00:30:32.050
one is, this one's close to home.
790
00:30:32.080 --> 00:30:35.030
a, an object that is rapidly developing
791
00:30:35.030 --> 00:30:37.840
a ring system and it's it's in
792
00:30:37.840 --> 00:30:40.080
the outer solar system.
793
00:30:40.480 --> 00:30:43.120
Jonti Horner: It is, this is an object called Chiron,
794
00:30:43.920 --> 00:30:45.920
which was the first of the centaurs to be
795
00:30:45.920 --> 00:30:47.240
discovered. And I always like to talk about
796
00:30:47.240 --> 00:30:48.920
the centaurs because they're what I studied
797
00:30:48.920 --> 00:30:51.660
for my PhD, so, so I was at one
798
00:30:51.660 --> 00:30:54.220
point, 20 odd years ago, one of the world's
799
00:30:54.220 --> 00:30:56.140
experts in how these things move around the
800
00:30:56.140 --> 00:30:57.740
solar system. And then science has moved on
801
00:30:57.740 --> 00:31:00.060
and I haven't, so I probably can no longer
802
00:31:00.060 --> 00:31:02.740
claim that. But Chiron is
803
00:31:02.820 --> 00:31:04.980
an interesting object. It's an icy object,
804
00:31:05.220 --> 00:31:08.220
bit more than 200km across. It was
805
00:31:08.220 --> 00:31:10.900
one of, if not the first object to get both a
806
00:31:10.900 --> 00:31:12.980
classification as an asteroid and as a comet.
807
00:31:13.540 --> 00:31:15.940
So it was initially discovered as a tiny
808
00:31:15.940 --> 00:31:17.460
speck of light moving around. It's discovered
809
00:31:17.460 --> 00:31:19.300
by Cowell I think in 1970,
810
00:31:20.340 --> 00:31:22.380
moving on an orbit that spends nearly all its
811
00:31:22.380 --> 00:31:24.220
time between the orbits of Saturn and Uranus.
812
00:31:24.220 --> 00:31:25.980
At the minute. Long term it's an unstable
813
00:31:25.980 --> 00:31:28.500
orbit. There's about a, ah, one in three
814
00:31:28.500 --> 00:31:29.940
chance that this will eventually end up in
815
00:31:29.940 --> 00:31:31.540
the inner solar system at some point in the
816
00:31:31.540 --> 00:31:33.780
next few million years. And that's part of
817
00:31:33.780 --> 00:31:36.060
the work I did during my PhD was running
818
00:31:36.060 --> 00:31:37.540
simulations of where this thing's going to
819
00:31:37.540 --> 00:31:40.100
go. That in itself is interesting because
820
00:31:40.100 --> 00:31:42.580
it's about a bit more than 200km across.
821
00:31:43.300 --> 00:31:44.900
So if this thing got trapped in the inner
822
00:31:44.900 --> 00:31:46.540
solar system, it will be, be a comet like
823
00:31:46.540 --> 00:31:48.780
nothing we've seen in recorded history. Hale
824
00:31:48.780 --> 00:31:51.660
Bopp, which was ridiculous, had a 50
825
00:31:51.660 --> 00:31:54.660
kilometer nucleus. If this thing's 250
826
00:31:54.660 --> 00:31:56.420
kilometers across, that's five times the
827
00:31:56.420 --> 00:31:59.220
radius, which means it's something like 25
828
00:31:59.220 --> 00:32:01.899
times the surface area, which means it will
829
00:32:01.899 --> 00:32:04.450
be a lot more impressive. So it's obviously
830
00:32:04.450 --> 00:32:07.130
an interesting object. Back in
831
00:32:07.130 --> 00:32:10.010
2011, team of scientists
832
00:32:10.410 --> 00:32:13.200
traveled across the world to gather to
833
00:32:13.200 --> 00:32:15.560
watch Chiron block out the light from a
834
00:32:15.640 --> 00:32:18.000
background star. So as this thing's moving
835
00:32:18.000 --> 00:32:20.560
through space, it just happened to pass in
836
00:32:20.560 --> 00:32:23.080
front of a star, from a subset of locations
837
00:32:23.080 --> 00:32:25.680
across the Earth. Now the distant stars are
838
00:32:25.680 --> 00:32:27.839
effectively so far away, we can consider the
839
00:32:27.839 --> 00:32:30.640
light coming in perfectly parallel. And
840
00:32:30.640 --> 00:32:32.200
so a 200 kilometer
841
00:32:33.000 --> 00:32:35.240
centaur will cast a shadow on the earth
842
00:32:35.240 --> 00:32:37.280
that's 200 kilometers across. And that shadow
843
00:32:37.280 --> 00:32:39.730
will whip across our planet. As the object
844
00:32:39.730 --> 00:32:41.570
and the Earth move around the sun, the shadow
845
00:32:41.570 --> 00:32:43.850
moves, the Earth moves through it. And so you
846
00:32:43.850 --> 00:32:46.850
get a 200 kilometer roughly scale band on the
847
00:32:46.850 --> 00:32:48.970
Earth where that star will disappear, then
848
00:32:48.970 --> 00:32:51.810
reappear. We know how fast everything's
849
00:32:51.810 --> 00:32:53.690
moving. So if you can get in that location,
850
00:32:54.010 --> 00:32:56.210
have a lot of telescopes spread out in a
851
00:32:56.210 --> 00:32:58.730
line, you can observe that
852
00:32:58.730 --> 00:33:01.330
occultation event and, by how long the star
853
00:33:01.330 --> 00:33:03.250
vanishes from different locations, you can
854
00:33:03.250 --> 00:33:05.640
actually figure out the shape and the size of
855
00:33:05.640 --> 00:33:08.320
the centaur because you can essentially map
856
00:33:08.560 --> 00:33:11.320
that shadow. And if you're near the edge, the
857
00:33:11.320 --> 00:33:12.880
star will disappear and reappear really
858
00:33:12.880 --> 00:33:14.520
quickly. If you're near the middle, you'll
859
00:33:14.520 --> 00:33:17.080
get a longer period where it vanishes. So
860
00:33:17.080 --> 00:33:18.720
these kind of, ah, occultation observations
861
00:33:18.800 --> 00:33:21.520
are really valuable to scientists. What
862
00:33:21.520 --> 00:33:23.560
happened in 2011 was they set their
863
00:33:23.560 --> 00:33:25.280
telescopes up and started watching a bit
864
00:33:25.280 --> 00:33:26.760
early to make sure they were looking at the
865
00:33:26.760 --> 00:33:29.320
star. And they noticed the star flickered on
866
00:33:29.320 --> 00:33:31.400
and off a couple of times before it properly
867
00:33:31.400 --> 00:33:33.540
disappeared for the main occultation. Then
868
00:33:33.540 --> 00:33:35.380
after it reappeared, it flickered on and off
869
00:33:35.380 --> 00:33:37.580
again a couple of times. And that's really
870
00:33:37.580 --> 00:33:40.420
weird. Now there was a kind of
871
00:33:40.420 --> 00:33:42.260
precedent for this with observations that
872
00:33:42.260 --> 00:33:44.780
were made in 1977, I believe,
873
00:33:45.100 --> 00:33:47.820
of Uranus, which was being observed from, I
874
00:33:47.820 --> 00:33:49.540
think it was the Kuiper Airborne Observatory
875
00:33:49.540 --> 00:33:52.100
doing one of these occultations. And they'd
876
00:33:52.100 --> 00:33:54.660
observed Uranus for this occultation because
877
00:33:54.660 --> 00:33:57.180
they wanted to understand the atmosphere of
878
00:33:57.180 --> 00:33:59.500
Uranus. And they figured as a stalwart behind
879
00:33:59.500 --> 00:34:02.109
Uranus, you'd see it not just disappear, but
880
00:34:02.109 --> 00:34:03.989
actually fade out as the light passed through
881
00:34:03.989 --> 00:34:06.149
the atmosphere. So you could measure the
882
00:34:06.149 --> 00:34:08.549
atmosphere and with that occultation of
883
00:34:08.549 --> 00:34:11.549
Uranus, occultation by Uranus, sorry, they
884
00:34:11.549 --> 00:34:12.949
got this flickering on and off thing. And
885
00:34:12.949 --> 00:34:14.749
that was the discovery of Uranus, of ring
886
00:34:14.749 --> 00:34:17.749
system. So basically the star vanished behind
887
00:34:17.749 --> 00:34:19.149
the rings, then reappeared, then vanished
888
00:34:19.149 --> 00:34:20.749
again, then reappeared, then went behind the
889
00:34:20.749 --> 00:34:23.629
planet. Right. So with this
890
00:34:23.629 --> 00:34:26.589
2011 event, the same kind of thing applied.
891
00:34:27.179 --> 00:34:29.139
It was the discovery of a ring system around
892
00:34:29.139 --> 00:34:31.259
this icy object. So this is a tiny thing,
893
00:34:31.899 --> 00:34:34.539
smaller than even Mimas, that we talked about
894
00:34:34.539 --> 00:34:36.299
last week with the subsurface ocean,
895
00:34:36.539 --> 00:34:38.419
something so small that its gravity is
896
00:34:38.419 --> 00:34:39.659
probably not strong enough to make it
897
00:34:39.659 --> 00:34:42.360
spherical. It's probably peanut shaped or
898
00:34:42.349 --> 00:34:44.028
rugby ball shaped or something like this.
899
00:34:44.028 --> 00:34:46.508
It's probably not spherical. Around this
900
00:34:46.508 --> 00:34:48.628
object, it seems that there is a system of
901
00:34:48.628 --> 00:34:50.268
rings where there are three or four narrow
902
00:34:50.268 --> 00:34:52.548
rings at various distances. I think the
903
00:34:52.548 --> 00:34:55.419
distances are something like 273, 325, 438
904
00:34:55.419 --> 00:34:58.379
and 1400 kilometers from the
905
00:34:58.379 --> 00:35:01.259
center of Chiron. Got this ring
906
00:35:01.259 --> 00:35:03.819
system and it's been observed again since
907
00:35:03.819 --> 00:35:06.739
they did observations in 2018, 2022 and
908
00:35:06.739 --> 00:35:09.579
2023, where they again figured
909
00:35:09.579 --> 00:35:11.579
out that the shadow of Chiron was going to
910
00:35:11.579 --> 00:35:13.939
scan across the planet, got a load of
911
00:35:13.939 --> 00:35:16.299
telescopes, went on a road trip and observed
912
00:35:16.299 --> 00:35:18.739
it happen to get more information about the
913
00:35:18.739 --> 00:35:21.059
rings. Because having a ring system around an
914
00:35:21.059 --> 00:35:23.139
object that isn't a planet is really cool.
915
00:35:23.649 --> 00:35:23.969
Andrew Dunkley: Yeah.
916
00:35:24.049 --> 00:35:26.489
Jonti Horner: And how did it form? How long has it been
917
00:35:26.489 --> 00:35:28.329
there? What's going on? How common are ring
918
00:35:28.329 --> 00:35:31.249
systems like this? Incidentally, a former PhD
919
00:35:31.249 --> 00:35:33.649
student of mine, Jeremy Wood, did some really
920
00:35:33.649 --> 00:35:36.089
cool dynamical studies that basically showed
921
00:35:36.089 --> 00:35:38.289
that the ring system could be
922
00:35:38.449 --> 00:35:40.809
primordial. It could be as old as the solar
923
00:35:40.809 --> 00:35:43.129
system. From the point of view of Chiron has
924
00:35:43.129 --> 00:35:45.009
never been close enough to one of the planets
925
00:35:45.009 --> 00:35:48.009
to disrupt the rings. So that
926
00:35:48.009 --> 00:35:49.529
doesn't put an edge limit on it, but it was
927
00:35:49.529 --> 00:35:52.169
still quite cool. What the new observations
928
00:35:52.169 --> 00:35:53.749
have shown though, is that, the ring system
929
00:35:53.829 --> 00:35:56.309
now seems to be different to how it was in
930
00:35:56.309 --> 00:35:59.269
2011. In other words, the ring
931
00:35:59.269 --> 00:36:01.949
system is evolving before our very
932
00:36:01.949 --> 00:36:04.069
eyes and it actually seems to be a denser,
933
00:36:04.069 --> 00:36:06.829
stronger ring system now than it was 10 or 15
934
00:36:06.829 --> 00:36:09.109
years ago. So it's possible that we're
935
00:36:09.109 --> 00:36:11.389
actually witnessing this ring system as it is
936
00:36:11.389 --> 00:36:14.069
forming or as it's changing over time.
937
00:36:14.069 --> 00:36:16.869
Now I know Chiron has been quite active,
938
00:36:17.309 --> 00:36:19.469
it's been outgassing because it's been closer
939
00:36:19.469 --> 00:36:21.629
to the sun, hence the cometary type
940
00:36:21.629 --> 00:36:24.629
classification it got. Maybe some
941
00:36:24.629 --> 00:36:26.309
of the material it's ejecting in that
942
00:36:26.309 --> 00:36:28.389
outgassing is being ejected gently enough
943
00:36:28.389 --> 00:36:31.009
that it doesn't escape from Chiron and,
944
00:36:30.959 --> 00:36:33.799
that's repopulating the rings. We just don't
945
00:36:33.799 --> 00:36:36.719
know. But the only way we'll find
946
00:36:36.719 --> 00:36:38.399
out is by doing more of these observations.
947
00:36:38.399 --> 00:36:41.279
But I think it's just really exciting and
948
00:36:41.279 --> 00:36:44.229
it's a really good reminder again that we
949
00:36:44.229 --> 00:36:46.069
always kind of imagine the solar system as a
950
00:36:46.069 --> 00:36:48.429
very sad and boring, placid place where not
951
00:36:48.429 --> 00:36:50.709
much changing anymore because it's four and a
952
00:36:50.709 --> 00:36:52.389
half billion years old. And as you get older,
953
00:36:52.389 --> 00:36:53.949
you Get a bit more sedentary and not much
954
00:36:53.949 --> 00:36:56.829
happens. But in fact it's a reminder that
955
00:36:56.829 --> 00:36:59.269
the solar system's a really dynamic place and
956
00:36:59.349 --> 00:37:01.269
things are constantly influenced, constantly
957
00:37:01.269 --> 00:37:03.429
changing. We talked about it last week. The
958
00:37:03.429 --> 00:37:05.829
ocean on Mimas that is possibly
959
00:37:06.149 --> 00:37:08.469
only 15 million years old. Now, 50 million
960
00:37:08.469 --> 00:37:11.029
years sounds like a really long time, but in
961
00:37:11.029 --> 00:37:12.749
a system that's four and a half thousand
962
00:37:12.749 --> 00:37:15.709
million years old, that's like something
963
00:37:15.709 --> 00:37:17.829
that has happened to me in the last couple of
964
00:37:17.829 --> 00:37:20.389
weeks. That's a new feature, not something
965
00:37:20.389 --> 00:37:22.389
I've had since birth. And this is yet another
966
00:37:22.389 --> 00:37:24.069
example of the fact that the solar system
967
00:37:24.069 --> 00:37:26.709
just seems to be continually rapidly changing
968
00:37:26.709 --> 00:37:27.309
and evolving.
969
00:37:27.789 --> 00:37:29.629
Andrew Dunkley: Yeah, yeah, it's a really interesting
970
00:37:29.789 --> 00:37:32.769
situation. how far out is chiron?
971
00:37:33.809 --> 00:37:36.089
Jonti Horner: It varies. So it's closest to the sun, It's a
972
00:37:36.089 --> 00:37:37.729
little bit closer to the sun than the orbit
973
00:37:37.729 --> 00:37:39.719
of Saturn. at its furthest, it's a bit
974
00:37:39.719 --> 00:37:41.279
further away than the orbit of Uranus. And
975
00:37:41.279 --> 00:37:42.959
that's an unstable orbit. So it bounces
976
00:37:42.959 --> 00:37:45.479
around over time, it will have encounters
977
00:37:45.479 --> 00:37:47.839
with them that fling it around. But at the
978
00:37:47.839 --> 00:37:50.399
minute it's in the outer solar system
979
00:37:50.479 --> 00:37:53.159
between the orbits of Saturn and Uranus most
980
00:37:53.159 --> 00:37:55.679
of the time. Unstable solution. It probably
981
00:37:55.679 --> 00:37:57.719
originated out beyond the orbit of Neptune.
982
00:37:57.719 --> 00:38:00.199
And it's one of this population called the
983
00:38:00.199 --> 00:38:03.059
Centaurs that are, the future parents of the
984
00:38:03.059 --> 00:38:04.699
next generation of short period comets.
985
00:38:04.699 --> 00:38:06.139
Effectively in the same way that the near
986
00:38:06.139 --> 00:38:08.379
Earth asteroids have their origin in the
987
00:38:08.379 --> 00:38:10.939
asteroid belt, short period comets have their
988
00:38:10.939 --> 00:38:13.579
origin in the Transeptunian region. But to
989
00:38:13.579 --> 00:38:15.059
get here from there, they've got to pass
990
00:38:15.059 --> 00:38:16.419
through the outer solar system. And that's
991
00:38:16.419 --> 00:38:17.459
what the Centaurs are.
992
00:38:18.019 --> 00:38:20.299
Andrew Dunkley: Okay. Fascinating. Yeah, it's really
993
00:38:20.299 --> 00:38:22.659
interesting and probably not one that,
994
00:38:23.048 --> 00:38:25.529
too many people would be aware of. I remember
995
00:38:25.529 --> 00:38:28.529
when it was making the news some
996
00:38:28.529 --> 00:38:30.969
years ago, and that's why the name stuck when
997
00:38:30.969 --> 00:38:33.499
you, when you sent the story to me. But, you
998
00:38:33.499 --> 00:38:35.459
don't really hear much about it. But now
999
00:38:35.929 --> 00:38:37.769
we've got a very good reason to look at it.
1000
00:38:38.209 --> 00:38:40.129
if you would like to look into that
1001
00:38:40.129 --> 00:38:43.009
particular paper, it's been published in
1002
00:38:43.009 --> 00:38:45.809
the Astrophysical Journal Letters.
1003
00:38:51.809 --> 00:38:53.729
Our final story, Jonti, is,
1004
00:38:54.689 --> 00:38:57.449
an exoplanet that the popular press are going
1005
00:38:57.449 --> 00:38:59.909
to say has got, some kind of life on it. it's
1006
00:38:59.909 --> 00:39:02.759
a, it's a maybe life candidate, story,
1007
00:39:02.759 --> 00:39:05.749
this one. And Yeah, but they're still
1008
00:39:05.749 --> 00:39:07.309
using the term super Earth.
1009
00:39:07.469 --> 00:39:09.869
Jonti Horner: Yeah, I'll keep this one a little bit short
1010
00:39:09.869 --> 00:39:12.709
and try not to get too grumpy. But one of my
1011
00:39:12.709 --> 00:39:15.549
big bug bears all the way through my career
1012
00:39:15.629 --> 00:39:18.479
is a good way for people to get media
1013
00:39:18.479 --> 00:39:20.679
coverage of their new planet discovery is say
1014
00:39:20.679 --> 00:39:23.119
it could be habitable. It's in the Goldilocks
1015
00:39:23.119 --> 00:39:23.759
zone. Hooray.
1016
00:39:24.079 --> 00:39:25.279
Andrew Dunkley: Using the L word.
1017
00:39:25.599 --> 00:39:27.119
Jonti Horner: Rumble, rumble, grumble, grumble.
1018
00:39:27.199 --> 00:39:28.879
Andrew Dunkley: It's a four letter word too, that one.
1019
00:39:28.879 --> 00:39:30.829
Jonti Horner: It is, and it's one of the terrible four
1020
00:39:30.829 --> 00:39:33.669
letter words. Part of the problem here is
1021
00:39:33.659 --> 00:39:35.499
there's this concept of the Goldilocks zone,
1022
00:39:35.499 --> 00:39:37.019
of the habitable zone, which has become
1023
00:39:37.019 --> 00:39:38.939
really entrenched in the popular
1024
00:39:38.939 --> 00:39:41.139
consciousness. And it's always viewed as
1025
00:39:41.139 --> 00:39:43.539
being this sweet spot for life. And the idea
1026
00:39:43.539 --> 00:39:45.219
is that if you have a planet in the habitable
1027
00:39:45.219 --> 00:39:46.659
zone, it will have liquid water on its
1028
00:39:46.659 --> 00:39:48.739
surface and all sorts of happy life things
1029
00:39:48.739 --> 00:39:51.179
will happen and everything will be good.
1030
00:39:52.169 --> 00:39:54.649
What it actually means is that if you took
1031
00:39:54.649 --> 00:39:56.829
the Earth, as it is today and put it where
1032
00:39:56.829 --> 00:39:59.149
that planet is, the Earth would still
1033
00:39:59.149 --> 00:40:01.869
maintain its liquid water because planets are
1034
00:40:01.869 --> 00:40:04.669
really diverse. If you took Venus and put
1035
00:40:04.669 --> 00:40:06.349
Venus where the Earth is, With Venus's
1036
00:40:06.349 --> 00:40:08.109
current atmosphere, Venus will be too hot to
1037
00:40:08.109 --> 00:40:10.469
have liquid water. But if you observe the
1038
00:40:10.469 --> 00:40:12.589
solar system from a long long way away and
1039
00:40:12.589 --> 00:40:15.079
you discovered Venus on the Earth's
1040
00:40:15.079 --> 00:40:17.729
orbit, it wouldn't look any different to the
1041
00:40:17.729 --> 00:40:19.059
Earth. it's a planet about the size of the
1042
00:40:19.059 --> 00:40:21.069
Earth, sat in the habitable sun. We, it's
1043
00:40:21.069 --> 00:40:23.709
habitable. Hooray. Whereas Venus is actually
1044
00:40:23.709 --> 00:40:25.749
so hot that on the surface it had melt lead.
1045
00:40:25.749 --> 00:40:27.629
And I certainly wouldn't want to visit there.
1046
00:40:27.629 --> 00:40:30.389
It's even hotter than my room was the other
1047
00:40:30.389 --> 00:40:32.869
night when the power cut had happened. And
1048
00:40:32.869 --> 00:40:35.849
that was bad enough and brutal enough. so
1049
00:40:35.849 --> 00:40:38.329
what this means is that ah, people
1050
00:40:38.649 --> 00:40:40.729
have become very fond of
1051
00:40:41.809 --> 00:40:44.609
find a planet around a star, you can work out
1052
00:40:44.849 --> 00:40:46.649
where the boundaries of the habitable zone
1053
00:40:46.649 --> 00:40:48.649
will be based on a few assumptions. And this
1054
00:40:48.649 --> 00:40:51.409
is work going back about a decade of the
1055
00:40:51.409 --> 00:40:53.129
definitions we use now. And you've got the
1056
00:40:53.129 --> 00:40:55.249
conservative and the optimistic habitable
1057
00:40:55.249 --> 00:40:57.399
zone, which are basically loosely based
1058
00:40:57.399 --> 00:40:59.839
around the fact that if you're as close to
1059
00:40:59.839 --> 00:41:02.279
the star that you get an amount of radiation
1060
00:41:02.279 --> 00:41:04.119
coming in comparable to Venus, you'll be too
1061
00:41:04.119 --> 00:41:05.959
hot. If you're about where Mars is, you'll be
1062
00:41:05.959 --> 00:41:07.359
too cold, but in the middle you'll be just
1063
00:41:07.359 --> 00:41:09.899
right m. and that's about it.
1064
00:41:10.059 --> 00:41:12.659
Now that definition doesn't really take any
1065
00:41:12.659 --> 00:41:14.339
account of the mass of the planet or its
1066
00:41:14.339 --> 00:41:17.339
atmosphere. What that
1067
00:41:17.339 --> 00:41:20.099
means is that ah, when you find a planet that
1068
00:41:20.099 --> 00:41:22.139
is a super Earth that Is four times the mass
1069
00:41:22.139 --> 00:41:24.539
of the Earth. That is almost certainly
1070
00:41:24.859 --> 00:41:27.019
nothing like our planet at all.
1071
00:41:27.899 --> 00:41:30.059
You'll do a calculation and say it sits in
1072
00:41:30.059 --> 00:41:32.779
the optimistic habitable zone. So there is a
1073
00:41:32.779 --> 00:41:34.419
potential it could have liquid water on its
1074
00:41:34.419 --> 00:41:37.369
surface. That's full of a whole heap
1075
00:41:37.369 --> 00:41:39.409
of assumptions. But to me it's a really long
1076
00:41:39.409 --> 00:41:41.009
stretch from saying it could have life.
1077
00:41:41.649 --> 00:41:41.969
Andrew Dunkley: A.
1078
00:41:41.969 --> 00:41:43.409
Jonti Horner: You're assuming it's got the right kind of
1079
00:41:43.409 --> 00:41:45.529
atmosphere to have liquid water where it's
1080
00:41:45.529 --> 00:41:46.889
four times the mass of the Earth. So its
1081
00:41:46.889 --> 00:41:48.589
atmosphere is almost certainly much, much m
1082
00:41:48.609 --> 00:41:50.689
thicker, Therefore
1083
00:41:51.329 --> 00:41:53.649
likely has a much stronger greenhouse effect,
1084
00:41:54.049 --> 00:41:55.969
Therefore probably runaway greenhouse. Not
1085
00:41:55.969 --> 00:41:56.289
good.
1086
00:41:56.849 --> 00:41:58.729
The other thing with this particular planet,
1087
00:41:58.729 --> 00:42:01.499
GJ 251C is it's a super
1088
00:42:01.499 --> 00:42:03.639
Earth orbiting a red dwarf star, ah,
1089
00:42:04.259 --> 00:42:06.749
nearby, less than 20 light years away. And
1090
00:42:06.749 --> 00:42:08.389
that's part of why people are excited. It's
1091
00:42:08.389 --> 00:42:09.869
near enough that we'll learn a lot more about
1092
00:42:09.869 --> 00:42:11.909
it in the future. However,
1093
00:42:12.629 --> 00:42:15.069
planet orbiting a red dwarf star means that
1094
00:42:15.069 --> 00:42:16.609
to be in the habitable zone, it's got to be
1095
00:42:16.609 --> 00:42:18.889
close in. This thing goes around its star
1096
00:42:18.889 --> 00:42:21.689
every 54 days, which means that it is
1097
00:42:21.689 --> 00:42:23.729
closer to its star than Mercury is to the
1098
00:42:23.729 --> 00:42:25.769
sun. And given the difference in the masses,
1099
00:42:25.769 --> 00:42:28.239
it's actually much closer in than that. That
1100
00:42:28.239 --> 00:42:30.439
means it's up close and personal with a red
1101
00:42:30.439 --> 00:42:32.759
dwarf star, which are notorious for being
1102
00:42:32.999 --> 00:42:35.479
active and flary and noisy, Particularly when
1103
00:42:35.479 --> 00:42:37.279
they're young. They're tempestuous teenagers
1104
00:42:37.279 --> 00:42:40.239
in their early days with mega stellar flares
1105
00:42:40.239 --> 00:42:43.039
and stuff like this. So it seems to be
1106
00:42:43.039 --> 00:42:44.999
fairly widely accepted that planets around
1107
00:42:44.999 --> 00:42:47.679
red dwarf stars that are close enough to be
1108
00:42:47.679 --> 00:42:50.119
warm enough to have liquid water will have a
1109
00:42:50.119 --> 00:42:51.879
hard time holding onto their atmospheres,
1110
00:42:51.959 --> 00:42:53.119
Particularly when the stars are young,
1111
00:42:53.119 --> 00:42:55.769
because it'll be having all sorts of
1112
00:42:55.769 --> 00:42:57.819
bonkers fun. And that's kind of borne out
1113
00:42:57.899 --> 00:43:00.699
with the planets around Trappist 1, which for
1114
00:43:00.699 --> 00:43:02.939
years have been people saying these are the
1115
00:43:02.939 --> 00:43:04.499
most Earth like planets ever and we'll find
1116
00:43:04.499 --> 00:43:06.899
life on them and hooray. And then when they
1117
00:43:06.899 --> 00:43:08.539
finally got to use the James Webb space
1118
00:43:08.539 --> 00:43:10.739
telescope and look at those planets, none of
1119
00:43:10.739 --> 00:43:13.179
them have an atmosphere. Now I don't know
1120
00:43:13.179 --> 00:43:15.499
about you, but I kind of like to breathe.
1121
00:43:15.659 --> 00:43:17.949
It's a fairly important part of living. And a
1122
00:43:17.949 --> 00:43:19.949
planet without an atmosphere is not going to
1123
00:43:19.949 --> 00:43:21.629
have liquid water on the surface because if
1124
00:43:21.629 --> 00:43:23.029
you take the atmosphere away, there's no
1125
00:43:23.029 --> 00:43:25.769
pressure, the oceans boil and then are blown
1126
00:43:25.769 --> 00:43:28.129
away by the red dwarfs, which makes that
1127
00:43:28.129 --> 00:43:30.249
planet a desiccated husk, which not
1128
00:43:30.249 --> 00:43:32.929
particularly habitable. The reason I Get
1129
00:43:33.169 --> 00:43:35.969
energized and activated about this. It's a
1130
00:43:35.969 --> 00:43:37.729
lovely discovery. It's a really interesting
1131
00:43:37.729 --> 00:43:39.439
planet. We'll, learn a lot more about planets
1132
00:43:39.439 --> 00:43:41.999
elsewhere. If there is an atmosphere, it's
1133
00:43:41.999 --> 00:43:43.639
around us now that's near enough to us that
1134
00:43:43.639 --> 00:43:45.119
with James Webb, we'll be able to study it,
1135
00:43:45.119 --> 00:43:46.599
learn more about the atmosphere. We'll learn
1136
00:43:46.599 --> 00:43:48.759
a whole heap from it. But I get really
1137
00:43:48.759 --> 00:43:50.479
energized about this because there's only so
1138
00:43:50.479 --> 00:43:52.399
many times that people can hear a story that
1139
00:43:52.399 --> 00:43:54.519
says we found the most Earth like planet ever
1140
00:43:55.239 --> 00:43:57.639
before they think we found the Earth before
1141
00:43:57.639 --> 00:44:00.279
they think we found life elsewhere. And that
1142
00:44:00.279 --> 00:44:02.359
then really devalues it. When we finally do
1143
00:44:02.359 --> 00:44:04.799
find planets that are, ah, properly like the
1144
00:44:04.799 --> 00:44:07.439
Earth, when we do find signs of life
1145
00:44:07.439 --> 00:44:09.759
elsewhere, scientists will be getting really
1146
00:44:09.759 --> 00:44:11.279
excited because we've finally done it. And
1147
00:44:11.279 --> 00:44:13.079
everybody will be like, well, why bother?
1148
00:44:13.079 --> 00:44:15.439
You've done this a million times before. The
1149
00:44:15.439 --> 00:44:16.999
whole boy who cried wolf thing
1150
00:44:18.519 --> 00:44:21.199
again, a big bugbear. And something that's
1151
00:44:21.199 --> 00:44:22.759
really critically important these days is
1152
00:44:22.759 --> 00:44:25.629
trust in science and trust in scientists. We,
1153
00:44:25.779 --> 00:44:27.819
we've got all the controversies about topics
1154
00:44:27.819 --> 00:44:29.249
that, are much more controversial than we're
1155
00:44:29.249 --> 00:44:31.369
talking about with astronomy, with vaccine
1156
00:44:31.369 --> 00:44:34.169
denial, with climate change denial, with
1157
00:44:34.169 --> 00:44:36.449
people refusing to evacuate in the path of a
1158
00:44:36.449 --> 00:44:38.409
hurricane that's coming because they don't
1159
00:44:38.409 --> 00:44:41.289
believe the scientists. Anything that
1160
00:44:41.528 --> 00:44:44.009
makes people less trusting of scientists
1161
00:44:44.009 --> 00:44:46.809
because they're overblowing stories is
1162
00:44:46.809 --> 00:44:49.809
damaging now far more than it has been in
1163
00:44:49.809 --> 00:44:51.569
decades past. It's part of why I get so
1164
00:44:51.569 --> 00:44:54.209
frustrated with Avi Loeb and Three Eye Atlas.
1165
00:44:54.209 --> 00:44:56.739
It's why get frustrated with the media
1166
00:44:56.739 --> 00:44:58.259
coverage of stories like this and the
1167
00:44:58.259 --> 00:45:00.819
scientists pushing, I think, somewhat
1168
00:45:00.819 --> 00:45:03.299
unethically an argument that this could be a
1169
00:45:03.299 --> 00:45:06.259
habitable planet because it makes
1170
00:45:06.259 --> 00:45:07.819
the rest of us look like fools. And it makes
1171
00:45:07.819 --> 00:45:10.259
people, it gives them ammunition to say,
1172
00:45:10.259 --> 00:45:12.819
well, scientists lie to us when they're not.
1173
00:45:13.379 --> 00:45:15.339
They're saying that this meets the criteria
1174
00:45:15.339 --> 00:45:16.819
for the Habitable Zone paper that was
1175
00:45:16.819 --> 00:45:19.219
published 10 years ago. But
1176
00:45:19.539 --> 00:45:21.899
it weakens that trust in science, which is so
1177
00:45:21.899 --> 00:45:23.739
important now more than it ever has done. And
1178
00:45:23.739 --> 00:45:25.369
I said I wouldn't go on a run and I'm now
1179
00:45:25.839 --> 00:45:27.719
waving the flag and banging the table and all
1180
00:45:27.719 --> 00:45:30.359
the rest of it. But it's a frustration that's
1181
00:45:30.359 --> 00:45:32.159
wider than this story. And this story is
1182
00:45:32.159 --> 00:45:34.799
lovely. It's an awesome discovery. They found
1183
00:45:34.799 --> 00:45:36.519
a planet going around a star. That's very
1184
00:45:36.519 --> 00:45:38.399
cool. We'll learn a lot more about it. It's a
1185
00:45:38.399 --> 00:45:41.159
brilliant result. You don't need to tag every
1186
00:45:41.159 --> 00:45:43.079
result like this and say that this planet
1187
00:45:43.079 --> 00:45:43.759
could have life.
1188
00:45:45.519 --> 00:45:47.759
Andrew Dunkley: And yet that's what, that's what happens.
1189
00:45:47.719 --> 00:45:49.419
it's sort of like, what artificial
1190
00:45:49.419 --> 00:45:51.619
intelligence is doing to social media. You
1191
00:45:51.619 --> 00:45:53.999
don't know. You don't know what you're
1192
00:45:53.999 --> 00:45:56.719
looking at anymore. And my
1193
00:45:56.719 --> 00:45:59.559
trust levels have dropped significantly in
1194
00:45:59.559 --> 00:46:00.199
recent months.
1195
00:46:02.119 --> 00:46:04.729
Jonti Horner: My dad is, 80, and
1196
00:46:04.729 --> 00:46:06.529
he's still on Facebook. And he doesn't like
1197
00:46:06.529 --> 00:46:08.329
it, but he's on it because it's a way to
1198
00:46:08.329 --> 00:46:10.089
communicate with people back in the uk. Moved
1199
00:46:10.089 --> 00:46:12.609
over here a few years ago and he's constantly
1200
00:46:12.609 --> 00:46:14.529
saying to me, he's getting so frustrated with
1201
00:46:14.529 --> 00:46:16.929
these AI stories and fake news things that he
1202
00:46:16.929 --> 00:46:18.569
doesn't know what to trust on there anymore
1203
00:46:18.649 --> 00:46:21.059
because he'll see a story that some famous
1204
00:46:21.059 --> 00:46:23.659
actors died and then he'll look up on
1205
00:46:23.659 --> 00:46:25.459
Wikipedia and they're still alive and kicking
1206
00:46:25.459 --> 00:46:26.779
and they've got a film coming out. But
1207
00:46:26.779 --> 00:46:28.099
there's this thing of, you'd never believe
1208
00:46:28.099 --> 00:46:31.059
the tragic photos. And it's
1209
00:46:31.059 --> 00:46:33.699
bizarre. And at a time when we need fidelity
1210
00:46:33.699 --> 00:46:36.019
and trust in our news and trust in our
1211
00:46:36.019 --> 00:46:38.979
science, we've got to be careful about how
1212
00:46:38.979 --> 00:46:41.099
much hyperbole we put into stories. I think.
1213
00:46:41.419 --> 00:46:43.979
Andrew Dunkley: I totally agree. Yes. If you'd like to read
1214
00:46:43.979 --> 00:46:46.809
about that, particular exoplanet, you can,
1215
00:46:47.159 --> 00:46:49.619
pick up that yarn through the Astronomical
1216
00:46:49.619 --> 00:46:51.419
Journal where they publish the paper. Or you
1217
00:46:51.419 --> 00:46:53.519
can read up on all the stories we've talked
1218
00:46:53.519 --> 00:46:53.719
about
1219
00:46:53.719 --> 00:46:56.639
today@space.com
1220
00:46:57.199 --> 00:46:59.569
and I'm sure a few other, platforms have
1221
00:46:59.569 --> 00:47:00.569
published them as well.
1222
00:47:01.019 --> 00:47:03.169
and that brings us to the end of, this
1223
00:47:03.409 --> 00:47:05.329
program. Jonti, thank you so much.
1224
00:47:05.969 --> 00:47:07.729
Jonti Horner: It's a pleasure. It's lovely to chat. Thanks
1225
00:47:07.729 --> 00:47:09.609
for bearing with me, being a bit flighty and
1226
00:47:09.609 --> 00:47:11.329
flirty thanks to the power cuts and the
1227
00:47:11.329 --> 00:47:11.649
weather.
1228
00:47:12.529 --> 00:47:15.129
Andrew Dunkley: You've done well. You've done well. We'll,
1229
00:47:15.129 --> 00:47:17.129
catch you on the next program, a Q and A
1230
00:47:17.129 --> 00:47:19.099
program. Johnty, Horn, a professor of
1231
00:47:19.099 --> 00:47:21.419
astrophysics at the University University of
1232
00:47:21.419 --> 00:47:24.079
Southern Queens. And thanks to Huw in the
1233
00:47:24.079 --> 00:47:26.399
studio, who couldn't be with us today
1234
00:47:27.119 --> 00:47:30.119
because he never tells me. I
1235
00:47:30.119 --> 00:47:32.639
have no idea. I just make up the reasons he's
1236
00:47:32.639 --> 00:47:34.839
not here. I honestly don't know why he didn't
1237
00:47:34.839 --> 00:47:36.719
turn up this week. Probably because we didn't
1238
00:47:36.719 --> 00:47:37.839
tell him when we were recording.
1239
00:47:38.319 --> 00:47:39.359
Jonti Horner: That might have been it.
1240
00:47:39.569 --> 00:47:41.769
Andrew Dunkley: and from me, Andrew Dunkley, thanks for your
1241
00:47:41.769 --> 00:47:44.409
company. Catch you on the very next episode
1242
00:47:44.409 --> 00:47:46.049
of Space Nuts. Bye.
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Jonti Horner: Bye.
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You've been listening to the Space Nuts
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00:47:49.689 --> 00:47:52.609
podcast, available at
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00:47:52.609 --> 00:47:54.569
Apple Podcasts, Spotify,
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00:47:54.729 --> 00:47:57.529
iHeartRadio or your favorite podcast
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player. You can also stream on demand at
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bytes. Com.
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Andrew Dunkley: This has been another quality podcast
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production from Bytes. Com.
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Andrew Dunkley: Hello, thanks for joining us. This is Space
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Nuts. My name is Andrew Dunkley, and we're
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here to talk astronomy and space science. And
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on this episode, we are going to look at a
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study into Jupiter's role in shaping
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our solar system. What shape is that?
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It's rhomboid. No, we don't know. we're also
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going to look at a, white dwarf star that's
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chowing down on a planetesimal. Sounds
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appetizing. observing a rapidly
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developing ring system, and it's not far
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away. And if we've got time, an exoplanet
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that in inverted commas may
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be a life candidate. That's all coming up on
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space nuts. 15 seconds. Guidance is
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internal. 10, 9.
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Ignition sequence start. space nuts. 5, 4,
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3, 2. 1, 2, 3, 4, 5, 5,
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4, 3, 2, 1.
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Jonti Horner: Space nuts.
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Andrew Dunkley: Astronauts report it feels good. And it's
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good to have Jonti Horner back with us again.
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Professor of astrophysics at the University
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of Southern Queensland. Hi, Jonti.
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Jonti Horner: Good evening. How are you going?
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Andrew Dunkley: I am well. Good to see you.
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Jonti Horner: Oh, it's good to be back. Although I'm
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admittedly a bit of a zombie, so I warn
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everybody, I've had less sleep than I should
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have done in the last couple of days because
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of the weather. we had some weather happen on
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Sunday, which led to the power here being
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knocked out for 24 hours during a mini heat
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wave. So I didn't get much sleep then. And
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then this morning I've got a colleague from
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Japan visiting, so I had to pick him, his
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wife and their two lovely daughters up from
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Brisbane Airport. So I've had six hours of
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driving today off the back of two nights of
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not much sleep. So if I seem less coherent
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than normal, and I appreciate I'm normally
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not that coherent to begin with, you know
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why, of course.
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Andrew Dunkley: Yes, we've all been there. we've had dreadful
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weather here too. But it hasn't been the
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extreme heat, it's been the extreme wind.
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I got woken up, last night about
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1am by the Fly, screens rattling. It
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was so windy. Yes, they, they were just
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shuddering. And I thought, I can't live with
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this.
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Jonti Horner: So I went outside.
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Andrew Dunkley: It was freezing cold, supposed to be late
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spring here, and I
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just jammed some wood chips
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into the. I just went off to the
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garden and grabbed some mulch and shoved it
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in the wind in, in the fly screens to stop
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them rattling.
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Jonti Horner: It worked.
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Andrew Dunkley: I've done it better during the day, but,
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well, that's just Been ridiculous.
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Jonti Horner: I know your parents. I mean having said that
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we had heat wave conditions and couldn't
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sleep because of the heat, I'm happ confess
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that I've had the wood serve on today because
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having had 36, 38 degrees so
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that's around 100 for our American friends
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last few days. Today has been a toasty kind
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of 15 degrees. and we've got a rain event
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happening. so we've had everything in the
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last week we've had kind of almost tornadic
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storms, we've had hailstones the size of your
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fists, we've had under a kilometer an hour
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gusts and now we've got random cold that
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makes me feel like I'm back in the uk. So
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yeah, all happening. And this is why
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Australia is an interesting place to live
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even to the extent that with the
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thunderstorms. We had got an email through
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yesterday that our wonderful observatory,
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Queensland's only professional astronomical
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observatory in Mount Kent was closed
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yesterday. We weren't allowed to go there
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because there was a bushfire within 10km of
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it that had been sparked by the lightning
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from the storms and fanned by the heat wave
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in a place that got lightning but no rain. So
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ah, it's all happening here.
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Andrew Dunkley: Yes, dry storms are not uncommon where I am.
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We we do get quite a few storms every year
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with lightning and thunder and nothing else.
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and they, yeah, they're very well known for
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sparking bushfires.
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Jonti Horner: Yeah.
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So while we're on the diversion of the
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weather, actually I'll apologize for Maya the
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dog chirping in the background but my
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partner's just got home. But we're also
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sitting here with an incredibly heartbreaking
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record, record breaking storm in the
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Caribbean. Yes, I know she's just come
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home. Thank you for joining me with the
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podcast Happy Dog. but yeah, there's
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borderline record breaking storm in the
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Caribbean which is going to be a Category 5
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hurricane hitting Jamaica and doing a, ah,
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hell of a lot of damage. And it's one of
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these that from a scientist point of view,
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fascinating watching it looking at the radar
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footage and all the satellite footage and on
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one hand you've got this thing of incredible
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exceptional beauty and on the other hand the
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devastation it's going to cause. So the
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people in the, in the firing line for that.
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Andrew Dunkley: Yeah, I saw the satellite images this
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afternoon. It is enormous.
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Jonti Horner: Yeah, you look at the false color one
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with the color of the clouds which is an
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indication of the severity of the storm and
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the shape and it's the kind of thing that you
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only see with the strongest storms we've ever
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seen, typically in the Pacific. So for this
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thing to not only be happening in the
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Atlantic, which is less common, but
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to be, you know, crosshairs on Jamaica,
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which has had a bit of a charmed life with
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some sacks of the high mountains that tend to
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bounce and go around a bit. This one looks
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like it's not so much going to bounce a
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splat.
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Andrew Dunkley: So yeah, when we were in Panama earlier
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this year, we did the Panama Canal and
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they were saying that they never get
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hurricanes ever.
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Jonti Horner: Too equatorial is my understanding. You need
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to be far enough away from the equator to get
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enough spin so. So it's very rare that you
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get storms getting right up to the equator
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because coriolis force and things like that.
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Andrew Dunkley: Yeah, yeah, it's interesting, isn't it?
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Very interesting. Okay, we better get
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on with what we came here to get on with. And
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we're going to start with a study that's
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been released into Jupiter's role in shaping
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the solar system. Now I do recall Fred
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mentioning that Jupiter, if Jupiter
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didn't exist we wouldn't. And this study
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basically adds a lot of fuel to that claim.
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Jonti Horner: It does. Now where Fred said,
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Fred and other people talk about if Jupiter
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didn't exist then we probably wouldn't. Ties
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into something that's a pretty big
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myth in science communication, Ansel in
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science papers and stuff, which is the idea
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of Jupiter shielding us from impacts. And my
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most favorite piece of research I ever did in
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my career is proving that to be a lot of
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cobblers and it's actually a lot more
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complicated. Jupiter throws things at us as
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well as protecting us. So I've always got a
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bit of an eye on any study that says, hey
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guys, if Jupiter wasn't there, neither would
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we. But this is a really interesting one that
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looks an entirely different aspect of
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Jupiter, which is the role that Jupiter
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played on the formation and evolution of the
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early solar system, the formation of the
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planets. And I've actually been teaching
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planet formation this week to my undergrad
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students. I've just, prior to recording this,
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had a two hour tutorial with them where I've
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been talking about planet formation and
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brought this story up because it
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really highlights the fact that when we
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often see in documentaries and the stuff we
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get taught at school, we get the impression
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that everything's solved, that we know the
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answers, that we know full well how the
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planets formed in microscopic detail and
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we've got everything figured out and the
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Reality is that we haven't. We have a really
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good broad picture and we're getting better
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and better at understanding the processes
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that went on. But there's still a lot to
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learn. And part of that is that while we've
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known the solar system since the year dot,
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we've only known other planetary systems for
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the last 30 years. And in reality we're still
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learning an awful lot about the planetary
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systems we find elsewhere. And learning about
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them is cool and all, but it also gives us
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insights that help us better understand our
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planetary system and how it formed. And that
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ties into this because the more we
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study those other planetary systems, the more
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we're getting observations of really
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beautiful things like planetary systems that
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are in formation, where you've got a
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protoplanetary disk. And we're getting these
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gorgeous images from things like the
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ALMA array, the Ataccama Large Millimeter
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Array that shows disks of planet
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forming material around stars with gaps in
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them and ripples in them and bands in them,
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and all these beautiful structures. And some
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of these have been previous astronomy.
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Picture of the days where this ties into the
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solar system is if you imagine that kind of
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stereotypical image of a
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protoplanetary disk, a disk of gas and dust
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around a young star like the sun, where
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material is feeding in through that disk to
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the star. So while the gas and dust is
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orbiting the star, there is this kind of
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sense of inward motion where the stars kind
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of nominating at the inner edge of the disk,
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materials falling in, and more material from
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outside flowing in to replace it. Yeah, and
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some of the models of the formation of the
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solar system struggle to make the terrestrial
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planets as a result of that. Because the
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material in the inner solar system is
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destined to fall onto M the star. And how do
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you stop that happening to let that material
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hang around to actually form into planets?
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Now it's been pretty well established for a
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long time that the first planet that formed
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in the solar system and got to a good size
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was Jupiter. And there's good reasons for
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that. It formed far enough away from the sun
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that the temperature was cold enough that the
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disk was rich in ice, which at, the
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distance the Earth is from the sun, all that
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ice would be gas. when you're forming solid
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objects, you need solid objects to feed from.
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And so when you've got a lot of ice, you've
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got a lot more solids. So things grow
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quicker, there's a lot more to eat. And it's
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only when you get to about 10 or 12 times the
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Mass of the Earth that You're massive enough
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to effectively start gobbling up the gas as
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well. So Jupiter formed beyond this point
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called the snow line, where there's a lot
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more solid material. It got to grow really
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quickly. It grew quicker than things further
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out because the further out you go, the
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slower things happen. So Jupiter was very
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much in the sweet spot, grew really quickly
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and eventually got big enough that it started
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clearing the gas and the dust it could gather
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the gas as well. And it opened up a gap in
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the disk. And that's very analogous to what
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we're seeing with these beautiful images from
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ALMA places like this. So the team of
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researchers behind this work have run some
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really in depth computer modeling of the
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formation of the solar system formation of
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Jupiter, and showed that when Jupiter opens
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up the gap in the disk, its gravity will
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also have an impact on the inner solar
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system. It'll effectively create the
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gravitational equivalent of speed bumps,
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creating areas where the dust that's
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spiraling inwards can pile up and be
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stopped from traveling further in.
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Effectively. It also creates
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a gap between the in run out of solar system
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that nothing crosses because if anything gets
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in that gap, Jupiter noms on it. And that's
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really interesting because some studies that
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have looked at primordial material we've
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found from in the solar system suggests that
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there is a bit of a chemical difference
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between material that formed in the inner
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solar system and material that formed in the
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outer solar system. So this gap
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dividing the two gives a natural way for that
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to happen. But the really big exciting result
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from this is really that modeling of
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the structure that Jupiter would have imposed
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on the inner solar system. These kind of pile
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up regions where you get more m dust and
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debris than normal, the structures that, that
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would carve out ripples in the disk
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effectively and how that would then
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contribute to the formation of the
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terrestrial planets. and therefore suggesting
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that not only did Jupiter help the
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terrestrial planets form by creating sweet
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spots where material could pile up, but it
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may also have had a really strong influence
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on the architecture of the inner solar system
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by setting where the planets would form,
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which then would go through a bit of a
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randomization phase as everything collides
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with each other. But it kind of possibly set
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the blueprint for the inner solar system. And
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therefore, if Jupiter hadn't formed where it
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did and how it did, the Earth would look
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very, very different and we might not be
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here.
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Andrew Dunkley: Yeah, it's truly fascinating. And
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when you look at other systems that
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we've discovered, exoplanet solar systems,
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ours is starting to look a little bit more
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unusual than normal. and
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Jupiter may be the reason.
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Jonti Horner: It could well be. And it's one of those
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things, I'm reminded of the Monty Python
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thing. I think it's in Life of Brian, where
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you've got that thing of we're all
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individuals. Yes, we're. No, we're not. I'm
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not. Every
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planetary system is going to be unique
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because it is influenced by
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such a wide variety of things going on. Even
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the stars that form in the local
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neighborhood, whittling it away from the
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outside, it all starts going on. But what
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we're seeing is there's a commonality among a
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lot of the planetary systems that we find
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that look very different to ours.
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The thing that gives us a little bit of pause
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though, is that we have these observational
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biases that make us more likely to find
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systems that are different to ours than we
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are to find systems like ours. And so you've
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always got that question of do we look
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unusual because we are unusual,
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or do we look unusual because we're not yet
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very good at finding places that look like
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home? and that's where colleagues of mine,
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like professor, Rob Wittenmayer, my colleague
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at unisq, have done really interesting
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work where what they
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do is look at what we found, but work
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out what doesn't exist
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based on what we haven't found yet. So they
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can start getting an estimate of how common
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our, ah, planetary systems like ours based on
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the fact we haven't found them yet. And it's
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a really kind of weird type of science where
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the absence of finding thing places limits on
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how common that thing is. So if you said
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that every star had a planet exactly like the
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Earth, on an orbit that's one year long that
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is exactly the same size as us and all the
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rest of it, then we can work out
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statistically, based on how good our
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telescopes are and our techniques are, how
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many of those planets we would have found.
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And we wouldn't have found anywhere near all
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of them because it's really hard to do. But
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we'd have found X amount. And the fact that
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we've only found a very small number smaller
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than that places an upper limit on how common
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things can be. So you get this perverse
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science where you get the observations
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that tell us what we found and what we've
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seen, but you can also put inferences on
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what isn't there and what is there based on
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what we haven't found yet, which allows you
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to put limits on how common things are that
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you couldn't really find very easily. Which,
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if that makes your head hurt. it makes my
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head hurt a little bit as well. But it's a
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really kind of clever use of the data we get
368
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to extrapolate further and draw more
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conclusions. And the net result of that is
370
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that the solar system is not hugely rare, but
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it's not common either. It's usual.
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And, that's really cool. And that probably
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extends to everything. Like I say, we're all
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individuals. The Earth, even though it's
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peeing it down outside at the minute, the
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Earth's actually a very dry planet. If you
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took all the water off the Earth and made a
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little blob of it next to the Earth, that
379
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blob would be fairly tiny. And everybody
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views the Earth as being very wet, but I view
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it as being very dry because water is such a
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common compound in the universe. It's made of
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the first and third most common atom. You put
384
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them together. Yet water waters everywhere.
385
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So for the Earth to be as dry as it is is
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telling you a lot about the uniqueness of the
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solar system. And maybe that's partially
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because of Jupiter. Not, necessarily
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shielding us from impacts, but preventing
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that icy material spiraling in, preventing
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us from becoming an ocean world. It's also
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partly down to the moon forming impact. The
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moon forming impact would have stripped a lot
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of the primordial Earth's water away because
395
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it walked as light and sits near the surface.
396
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So a lot about our Earth and a lot about the
397
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solar system is down to the random nature of
398
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the events around us. When we formed the moon
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forming impact, a nearby star going
400
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supernova and lacing our solar system with
401
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radioactive aluminium. Things like this.
402
00:15:17.840 --> 00:15:19.400
There's all these oddities that made our
403
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solar system unique, but if those
404
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hadn't happened, other things would have
405
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happened and we'd have still ended up with
406
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something unique because of other random
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things happening.
408
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It's all fascinating and I just love this
409
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stuff.
410
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Andrew Dunkley: Yeah. And it adds more and more weight to the
411
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theory that we are just a freak accident.
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Jonti Horner: Yes.
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Andrew Dunkley: And probably a one off in the universe.
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That's one argument. So, yeah,
415
00:15:42.560 --> 00:15:45.410
who knows if, if we find a
416
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solar system just like ours, with a planet
417
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just like ours, orbiting a
418
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star just like ours. That would be
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the, you know, one of the greatest
420
00:15:56.680 --> 00:15:58.560
discoveries in astronomical history, I
421
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imagine. But no, we do that.
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Jonti Horner: We would have to get in touch with the planet
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builders at Magrathea and demand that money
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back. Because we thought we had a limited
425
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edition.
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Andrew Dunkley: Yes, yes. weren't they the white mice? Was
427
00:16:09.350 --> 00:16:10.270
that the white mice?
428
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Jonti Horner: Yes, it was.
429
00:16:11.600 --> 00:16:13.320
Andrew Dunkley: Yeah. All right, if you want to read all
430
00:16:13.320 --> 00:16:15.880
about it, you can find, the paper,
431
00:16:16.540 --> 00:16:19.240
which was published in the journal Science
432
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Advances.
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Jonti Horner: Roger, your labs are here. Also space nuts.
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Andrew Dunkley: now, Jonti, let's move on to our next story.
435
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And this one is about a planetismal,
436
00:16:32.190 --> 00:16:35.110
that appears doomed. According to the, paper
437
00:16:35.110 --> 00:16:37.190
I'm reading, it's a white dwarf that's
438
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chowing down very, very hungry, hungry
439
00:16:39.790 --> 00:16:40.990
individual is this one.
440
00:16:41.790 --> 00:16:44.270
Jonti Horner: It is. So just to remind the audience, a
441
00:16:44.270 --> 00:16:47.030
white dwarf is the kind of little husk
442
00:16:47.030 --> 00:16:48.990
that's left after a cell like our sun comes
443
00:16:48.990 --> 00:16:51.430
to the end of its life, burns all its
444
00:16:51.430 --> 00:16:53.870
hydrogen, becomes a red giant, and then
445
00:16:53.870 --> 00:16:55.750
eventually blows off its outer layers. And it
446
00:16:55.750 --> 00:16:58.110
leaves a big chunk of the star's mass
447
00:16:58.510 --> 00:17:00.350
compressed into an object about the size of
448
00:17:00.350 --> 00:17:03.270
the Earth. That whole process will
449
00:17:03.270 --> 00:17:05.870
have a fairly hefty impact on the
450
00:17:05.870 --> 00:17:07.870
planetary system that star's got around it.
451
00:17:08.230 --> 00:17:09.710
And of course, as we just discussed, we now
452
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know that pretty much every star has planets.
453
00:17:12.150 --> 00:17:14.310
The expectation is that when the sun reaches
454
00:17:14.310 --> 00:17:16.350
this stage, unfortunately it's in about 7
455
00:17:16.350 --> 00:17:18.060
billion years, so nothing to worry about.
456
00:17:18.060 --> 00:17:20.700
Immediately it will swell up and it will
457
00:17:20.860 --> 00:17:23.020
chow down on Mercury and chow down on Venus.
458
00:17:23.020 --> 00:17:25.820
They'll just be swallowed up and gone. Yeah,
459
00:17:25.820 --> 00:17:27.700
There is some debate over whether the Earth
460
00:17:27.700 --> 00:17:30.300
will be swallowed up or will survive. Just
461
00:17:31.100 --> 00:17:33.230
all the models of star, evolution suggest
462
00:17:33.230 --> 00:17:35.190
that the sun will swell up to be about the
463
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radius of the Earth's orbit. But whether the
464
00:17:37.510 --> 00:17:39.390
Earth is there to nominal or not is still
465
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open for debate. It may be that the loss of
466
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mass from the sun in the time before may just
467
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mean that the Earth nudges far enough away to
468
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survive as a burnt husk rather than be
469
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devoured. It still would be ideal
470
00:17:51.430 --> 00:17:53.270
to be around when that wouldn't be pleasant.
471
00:17:53.270 --> 00:17:54.630
I mean, that said, the Earth is going to
472
00:17:54.630 --> 00:17:56.870
become uninhabitable a lot sooner than that
473
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because the Sun's getting brighter and the
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Earth's oceans will boil and it'll all go
475
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downhill. But after all that process
476
00:18:04.460 --> 00:18:06.700
happens when the sun sheds its outer layers,
477
00:18:07.020 --> 00:18:09.380
that'll have a pretty cataclysmic event on
478
00:18:09.380 --> 00:18:12.060
the planets and the debris that are left. So
479
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suddenly the sun goes on the ultimate kind of
480
00:18:14.020 --> 00:18:16.860
weight loss kick loses mass. And that
481
00:18:16.860 --> 00:18:18.860
will mean that all of the objects going
482
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around the sun will be held less strongly.
483
00:18:21.300 --> 00:18:23.020
And so therefore their orbits will move
484
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outwards because the gravity pulling them in
485
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gets weaker. Now, if you suddenly Press the
486
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button and vanished half of the mass of the
487
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Sun. What had happened is that the speed that
488
00:18:33.560 --> 00:18:35.720
any of the objects are going in their orbit
489
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will be too quick for that orbit to be
490
00:18:37.680 --> 00:18:40.520
circular. So at that instant, at that
491
00:18:40.520 --> 00:18:43.040
point, they'd now be at their new perihelion,
492
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they'd be at their closest point to the sun,
493
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and they'd all move out onto much more
494
00:18:45.960 --> 00:18:48.520
elongated orbits with a longer orbital
495
00:18:48.520 --> 00:18:51.200
period, but orbits that would then cross one
496
00:18:51.200 --> 00:18:53.640
another. So if you imagine you lose half of
497
00:18:53.640 --> 00:18:56.320
the Sun's mass, Jupiter moves onto an orbit
498
00:18:56.320 --> 00:18:58.480
where its perihelion is 5 au from the sun,
499
00:18:58.480 --> 00:19:00.840
but its aphelion could be 15 au from the Sun.
500
00:19:01.400 --> 00:19:03.760
Saturn at the same time would have perihelion
501
00:19:03.760 --> 00:19:06.120
at 10 au and aphelion at say 20 au. And I'm
502
00:19:06.120 --> 00:19:08.440
making the numbers up a bit here. So suddenly
503
00:19:08.440 --> 00:19:11.199
Jupiter and Saturn are on orbits that
504
00:19:11.199 --> 00:19:14.120
cross one another. Their orbits
505
00:19:14.120 --> 00:19:16.520
will probably still have the same ratio of
506
00:19:16.520 --> 00:19:19.400
orbital periods, so 12 years to 29 years. But
507
00:19:19.400 --> 00:19:21.290
they'd scale up to be something like, I don't
508
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know, 30 to 70 or something like that,
509
00:19:23.970 --> 00:19:25.570
because they've both moved out by the same
510
00:19:25.570 --> 00:19:27.650
amount. But suddenly you've got these planets
511
00:19:27.650 --> 00:19:29.450
that are on orbits that cross each other and
512
00:19:29.450 --> 00:19:32.130
therefore can really strongly interact. They
513
00:19:32.130 --> 00:19:33.890
can stir everything else up because all of
514
00:19:33.890 --> 00:19:35.570
the objects in the asteroid belt, all of the
515
00:19:35.570 --> 00:19:37.330
objects beyond Neptune, this happens to
516
00:19:37.330 --> 00:19:39.770
everything. Now the mass loss is a bit more
517
00:19:39.770 --> 00:19:42.330
gradual than that in actuality. So what
518
00:19:42.330 --> 00:19:44.370
happens is you get the orbit spiraling out,
519
00:19:44.370 --> 00:19:46.170
but getting perturbed, being made more
520
00:19:46.170 --> 00:19:48.640
eccentric. You've also got these objects
521
00:19:48.640 --> 00:19:51.240
moving through the headwind of possibly half
522
00:19:51.240 --> 00:19:53.200
a solar mass of material being blown
523
00:19:53.200 --> 00:19:55.560
outwards. That provides friction and so
524
00:19:55.560 --> 00:19:57.720
causes them possibly to spiral inwards a bit.
525
00:19:58.520 --> 00:20:00.760
Causes Jupiter potentially to gather mass as
526
00:20:00.760 --> 00:20:03.400
it numbs on all that gas that's going out. At
527
00:20:03.400 --> 00:20:04.960
the same time, its atmosphere is probably
528
00:20:04.960 --> 00:20:07.360
being blasted away by all this wind blowing
529
00:20:07.360 --> 00:20:10.280
past. All of this complexity means
530
00:20:10.280 --> 00:20:12.200
that you couldn't predict with absolute
531
00:20:12.200 --> 00:20:14.080
certainty what the solar system would look
532
00:20:14.080 --> 00:20:16.920
like at the end of this, but certainly
533
00:20:16.920 --> 00:20:19.320
there'd be a period of chaos. A lot of stuff
534
00:20:19.320 --> 00:20:21.800
would survive, but it would survive on orbits
535
00:20:21.800 --> 00:20:24.520
that are now much more unstable. So you get a
536
00:20:24.520 --> 00:20:26.570
lot of material flung inwards and, some of
537
00:20:26.570 --> 00:20:29.170
that will be flung inwards far enough for it
538
00:20:29.170 --> 00:20:31.370
to impact on the Earth sized object in the
539
00:20:31.370 --> 00:20:33.700
middle and, for the white dwarf to get a
540
00:20:33.700 --> 00:20:36.300
snack. Now all that's expected to happen
541
00:20:36.300 --> 00:20:38.860
really early on. And over time everything
542
00:20:38.860 --> 00:20:41.530
stabilizes out, things get flung around and
543
00:20:41.530 --> 00:20:44.250
clean up happens a bit like the
544
00:20:44.250 --> 00:20:45.730
solar system. You know, we were talking early
545
00:20:45.730 --> 00:20:47.170
on about the early stages of planet
546
00:20:47.170 --> 00:20:49.090
formation. Everything gets flung around and
547
00:20:49.090 --> 00:20:51.210
by the time you get to now, four and a half
548
00:20:51.210 --> 00:20:52.770
billion years down the road, it's fairly
549
00:20:52.770 --> 00:20:55.210
quiet. There's a bit going on, but most of
550
00:20:55.210 --> 00:20:57.730
the drama's finished. So the
551
00:20:57.730 --> 00:20:59.730
expectation is you'd see white dwarfs that
552
00:20:59.730 --> 00:21:02.450
are very young occasionally eating things
553
00:21:02.450 --> 00:21:04.650
because things get flung in and they get a
554
00:21:04.650 --> 00:21:06.780
bit of a snack. And the material from that
555
00:21:06.780 --> 00:21:08.820
snack will be spattered over the surface of
556
00:21:08.820 --> 00:21:10.980
the white dwarf and be visible in its
557
00:21:10.980 --> 00:21:13.620
spectrum as anomalous added
558
00:21:14.100 --> 00:21:16.420
solid material, heavy elements.
559
00:21:17.140 --> 00:21:19.300
But that signal would only last a short time
560
00:21:19.300 --> 00:21:21.220
because the outer layer of the white dwarf is
561
00:21:21.220 --> 00:21:24.220
kind of a hydrogen soup and heavier elements
562
00:21:24.220 --> 00:21:27.140
would sink down. So any given time you'd eat
563
00:21:27.140 --> 00:21:29.660
something. The evidence for that meal would
564
00:21:29.660 --> 00:21:31.740
only remain for a few tens of thousands of
565
00:21:31.740 --> 00:21:34.650
years, SOPs before it goes away. Okay, so
566
00:21:34.650 --> 00:21:36.530
the fact is we've seen some white dwarfs
567
00:21:36.530 --> 00:21:38.810
which have these anomalous heavy element
568
00:21:38.810 --> 00:21:41.010
readings in their atmospheres. We can tell
569
00:21:41.010 --> 00:21:42.690
they're eating stuff, but typically they're
570
00:21:42.690 --> 00:21:45.450
young. So you'd expect that.
571
00:21:45.930 --> 00:21:48.010
The quirky thing here is that this white
572
00:21:48.010 --> 00:21:49.850
dwarf, which goes by the name of
573
00:21:49.850 --> 00:21:52.820
lspm, which I think is a survey name,
574
00:21:52.820 --> 00:21:54.010
m followed by
575
00:21:54.010 --> 00:21:57.770
J020733331.
576
00:21:58.330 --> 00:22:00.210
So that's a coordinate on the sky. So that's
577
00:22:00.210 --> 00:22:01.690
telling you where in the sky this is. It's
578
00:22:01.690 --> 00:22:04.390
catalog number. Yeah, this thing is an old
579
00:22:04.390 --> 00:22:06.310
white dwarf. It's thought to be about 3
580
00:22:06.310 --> 00:22:08.350
billion years old. So in other words, the
581
00:22:08.350 --> 00:22:11.230
star that formed it died 3
582
00:22:11.230 --> 00:22:13.510
billion years ago and it's been sitting there
583
00:22:13.510 --> 00:22:16.390
minding its own business. That's old enough
584
00:22:16.390 --> 00:22:18.070
that you'd expect everything to have calmed
585
00:22:18.070 --> 00:22:20.910
down around it. But what the new
586
00:22:20.910 --> 00:22:23.870
observations have shown is evidence of
587
00:22:23.870 --> 00:22:25.870
13 different heavy elements,
588
00:22:26.670 --> 00:22:28.750
including carbon, chromium,
589
00:22:29.980 --> 00:22:32.220
strontium, titanium, a lot of these different
590
00:22:32.220 --> 00:22:35.100
elements, roughly in the kind of abundance as
591
00:22:35.100 --> 00:22:37.630
you'd see on the Earth, added, to this white
592
00:22:37.630 --> 00:22:40.230
dwarf's atmosphere. So it's
593
00:22:40.230 --> 00:22:42.350
obviously just had a meal and we know it's a
594
00:22:42.350 --> 00:22:44.470
case of just had a meal rather than it's been
595
00:22:44.470 --> 00:22:47.190
a leftover from a long time ago, because this
596
00:22:47.190 --> 00:22:49.150
stuff will sink and disappear over the next
597
00:22:49.150 --> 00:22:52.110
few tens of thousands of years. So what
598
00:22:52.110 --> 00:22:54.190
that means is that this white dwarf
599
00:22:55.020 --> 00:22:57.380
has just had a snack. Now it might have had
600
00:22:57.380 --> 00:23:00.220
that snack 30,000 years ago, or it
601
00:23:00.220 --> 00:23:03.020
may still be in the process of eating as
602
00:23:03.020 --> 00:23:05.820
we speak. Now what the team have been able to
603
00:23:05.820 --> 00:23:08.340
do is look at the amount of material you'd
604
00:23:08.340 --> 00:23:10.140
need to give the strength of signal you've
605
00:23:10.140 --> 00:23:12.080
got in the spectrum of the star. And, what
606
00:23:12.080 --> 00:23:14.320
they've calculated is that to get this amount
607
00:23:14.320 --> 00:23:17.080
of material you'd need to eat an asteroid
608
00:23:17.800 --> 00:23:19.960
about 200 kilometers in diameter.
609
00:23:20.760 --> 00:23:22.520
So that's comparable to some of the larger
610
00:23:22.520 --> 00:23:24.200
asteroids in the asteroid belt, but not the
611
00:23:24.200 --> 00:23:26.920
largest by any means. It's within the bounds
612
00:23:26.920 --> 00:23:28.680
of possibility of what we see here at home.
613
00:23:29.080 --> 00:23:31.160
But the real question is why is it eating it
614
00:23:31.160 --> 00:23:33.520
now? Why is this happening now when you'd
615
00:23:33.520 --> 00:23:35.200
expect the system to have had plenty of time
616
00:23:35.200 --> 00:23:37.560
to calm down? What
617
00:23:37.960 --> 00:23:40.760
it suggests to me, and it suggests in the
618
00:23:40.760 --> 00:23:42.960
paper, it suggests in the articles about this
619
00:23:42.960 --> 00:23:45.240
as well, is that the only way you can get
620
00:23:45.240 --> 00:23:48.070
something eating this late, after 3 billion
621
00:23:48.070 --> 00:23:50.830
years have passed, is if you've still got a
622
00:23:50.830 --> 00:23:53.310
number of planet mass objects in the system
623
00:23:53.310 --> 00:23:56.230
serving things up, which is what we've got
624
00:23:56.230 --> 00:23:57.910
in the solar system. If we look at the inner
625
00:23:57.910 --> 00:24:00.270
solar system, fragments of comets and
626
00:24:00.270 --> 00:24:02.070
asteroids are falling onto the sun all the
627
00:24:02.070 --> 00:24:04.350
time. We've got near Earth asteroids, short
628
00:24:04.350 --> 00:24:06.390
period comets and long period comets whizzing
629
00:24:06.390 --> 00:24:08.760
around. And, they're being bounced around by
630
00:24:08.760 --> 00:24:10.480
the planets. Jupiter's throwing a lot of
631
00:24:10.480 --> 00:24:12.920
stuff away. Their orbits are constantly
632
00:24:12.920 --> 00:24:15.800
getting tweaked. And so therefore the sun
633
00:24:15.800 --> 00:24:18.640
is still getting this rain of solid material
634
00:24:18.640 --> 00:24:20.880
falling on it as a result of the planets
635
00:24:20.880 --> 00:24:23.560
stirring things up. Even though the solar
636
00:24:23.560 --> 00:24:25.760
system mostly quietened down, the planets are
637
00:24:25.760 --> 00:24:28.320
still injecting material to the inner solar
638
00:24:28.320 --> 00:24:30.760
system, which is why we're getting meteorites
639
00:24:30.760 --> 00:24:32.400
and it's why the sun occasionally gets to
640
00:24:32.400 --> 00:24:35.120
numb some stuff. The idea here is
641
00:24:35.120 --> 00:24:37.400
that this star reached the end of its life.
642
00:24:37.400 --> 00:24:40.260
Puff dots with its outer layers. You have
643
00:24:40.260 --> 00:24:42.260
this really chaotic period where everything
644
00:24:42.260 --> 00:24:44.820
had got stirred up, then it settled down. But
645
00:24:44.820 --> 00:24:46.660
because you still got planet mass objects
646
00:24:46.660 --> 00:24:49.020
there, they're still bouncing around what
647
00:24:49.020 --> 00:24:51.620
debris is left. And we're just catching this
648
00:24:51.620 --> 00:24:54.460
white dwarf just at the right time, when
649
00:24:54.460 --> 00:24:56.740
another asteroid has been flung inwards close
650
00:24:56.740 --> 00:24:59.100
enough to be torn apart by the star's gravity
651
00:24:59.260 --> 00:25:01.900
and to give it a snack. So in other words,
652
00:25:02.220 --> 00:25:04.460
seeing this snack happening this late in the
653
00:25:04.460 --> 00:25:07.060
life of this white dwarf is fairly strong
654
00:25:07.060 --> 00:25:09.500
evidence that planets survived the death of
655
00:25:09.500 --> 00:25:12.140
its star, have lived there for 3 billion
656
00:25:12.140 --> 00:25:14.460
years, which a is really cool in of itself.
657
00:25:14.460 --> 00:25:17.380
But it also means that here is a star that we
658
00:25:17.380 --> 00:25:19.860
should look at when the Gaia data release
659
00:25:19.940 --> 00:25:22.500
comes next year. Gaia Dr. AH4,
660
00:25:22.980 --> 00:25:24.780
which will have been measuring this star's
661
00:25:24.780 --> 00:25:26.460
position on the sky. And if there Are planets
662
00:25:26.460 --> 00:25:28.220
there, we'll be able to detect the wobble and
663
00:25:28.220 --> 00:25:31.100
confirm them. So it's also holding up a flag
664
00:25:31.100 --> 00:25:33.760
to exoplanet people saying,
665
00:25:33.920 --> 00:25:36.520
hey, folks, here's a target for you to look
666
00:25:36.520 --> 00:25:38.320
at when the data release comes out where you
667
00:25:38.320 --> 00:25:39.840
might be able to find some planets, because
668
00:25:39.840 --> 00:25:42.240
we think there's a smoking gun here that the
669
00:25:42.240 --> 00:25:44.600
planets are feeding the white dwarf, giving
670
00:25:44.600 --> 00:25:46.160
it little snacks every now and again.
671
00:25:47.120 --> 00:25:49.040
Andrew Dunkley: Okay, wow. All right.
672
00:25:49.040 --> 00:25:51.950
so are there many white dwarf
673
00:25:52.030 --> 00:25:54.830
stars out there? What, do they, sort of,
674
00:25:55.870 --> 00:25:58.560
percentage wise, inhabit the star field?
675
00:25:58.720 --> 00:26:01.480
Jonti Horner: There would be a fair few of them. So the
676
00:26:01.480 --> 00:26:03.600
more massive a star is, the shorter its life
677
00:26:03.600 --> 00:26:05.850
is. And, that's a really rapid function.
678
00:26:06.330 --> 00:26:08.860
Where that works is, if your star's more
679
00:26:08.860 --> 00:26:11.420
massive, its gravitational pull is stronger,
680
00:26:11.980 --> 00:26:14.940
so its ability to pull material into
681
00:26:14.940 --> 00:26:17.900
the middle of the star is higher, which means
682
00:26:17.900 --> 00:26:19.780
that that star's got to give off a lot more
683
00:26:19.780 --> 00:26:21.900
energy to balance that gravitational pull.
684
00:26:21.900 --> 00:26:24.140
And so stars in the main sequence part of
685
00:26:24.140 --> 00:26:26.690
their life are in equilibrium. The radiation
686
00:26:26.690 --> 00:26:28.330
coming out from the nuclear fusion in the
687
00:26:28.330 --> 00:26:31.250
middle balances gravity pulling in. The
688
00:26:31.250 --> 00:26:33.730
more massive you are, the hotter and denser
689
00:26:33.730 --> 00:26:35.490
you get in the middle, so the more energy you
690
00:26:35.490 --> 00:26:38.250
give off. And the result of that is that it
691
00:26:38.650 --> 00:26:40.809
roughly, it varies a little bit by star's
692
00:26:40.809 --> 00:26:42.850
mass, but roughly the brightness of a star,
693
00:26:42.850 --> 00:26:45.570
the luminosity of a star is proportional to
694
00:26:45.570 --> 00:26:47.050
the mass of the star to the power
695
00:26:47.050 --> 00:26:49.890
4.3.54. Which means if you
696
00:26:49.890 --> 00:26:52.480
double the mass of a star, it'll get between
697
00:26:52.480 --> 00:26:54.560
10 and 16 times brighter.
698
00:26:55.440 --> 00:26:58.240
So twice the mass, Call it a factor of 10
699
00:26:58.240 --> 00:26:59.960
just to keep it easy. If it's 10 times
700
00:26:59.960 --> 00:27:02.600
brighter, that means it's burning its fuel 10
701
00:27:02.600 --> 00:27:04.880
times quicker to produce 10 times as much
702
00:27:04.880 --> 00:27:07.120
energy. But it's only twice the mass, so it's
703
00:27:07.120 --> 00:27:09.920
only got twice as much fuel, so its
704
00:27:09.920 --> 00:27:11.920
life will be a factor of five times shorter.
705
00:27:12.080 --> 00:27:13.800
And the more massive you get, the shorter the
706
00:27:13.800 --> 00:27:16.640
life gets. Now, stars of different masses
707
00:27:16.720 --> 00:27:19.330
have different. A star like Proxima
708
00:27:19.330 --> 00:27:21.770
Centauri will never swell up to become a red
709
00:27:21.770 --> 00:27:23.490
giant. It'll just be a dull, glowing ember
710
00:27:23.490 --> 00:27:26.090
and eventually go out. But even the
711
00:27:26.090 --> 00:27:28.570
oldest stars like Proxima Centauri are still
712
00:27:28.730 --> 00:27:30.370
really in their youth because they're burning
713
00:27:30.370 --> 00:27:33.170
their fuel so slowly. Stars that are more
714
00:27:33.170 --> 00:27:35.050
massive eventually get stars like the sun,
715
00:27:35.050 --> 00:27:37.520
which are what form like dwarfs. And, they
716
00:27:37.680 --> 00:27:39.600
eventually swell up to become a red giant,
717
00:27:39.600 --> 00:27:41.680
puff off their outer layers. And for a star
718
00:27:42.000 --> 00:27:44.930
of the Sun's mass, that process from
719
00:27:44.930 --> 00:27:46.770
forming to the end of its life is thought to
720
00:27:46.770 --> 00:27:49.010
be about 12 billion years. It used to be 10
721
00:27:49.010 --> 00:27:51.130
billion models seem to have refined. So
722
00:27:51.130 --> 00:27:52.730
people nowadays seem to say it's about 12
723
00:27:52.730 --> 00:27:55.690
billion years. So a star of
724
00:27:55.690 --> 00:27:58.180
the mass of the sun that formed when our,
725
00:27:58.180 --> 00:28:00.740
Milky Way was very young will have lived and
726
00:28:00.740 --> 00:28:02.900
died and become a white dwarf more than a
727
00:28:02.900 --> 00:28:05.860
billion years ago. But stars more massive
728
00:28:05.860 --> 00:28:08.180
than the sun can form white dwarfs as well,
729
00:28:08.180 --> 00:28:10.750
up to maybe two or even three times the mass
730
00:28:10.750 --> 00:28:12.590
of the sun, depending how effective it is at
731
00:28:12.590 --> 00:28:14.870
shedding mass at the end. Yeah, the maximum
732
00:28:14.870 --> 00:28:17.070
mass for white dwarf, you can get about 1.4
733
00:28:17.070 --> 00:28:19.390
times the mass of the Sun. If stars lose half
734
00:28:19.390 --> 00:28:20.750
their mass, that gives you something about
735
00:28:20.750 --> 00:28:22.710
three times the mass of the sun before you
736
00:28:22.710 --> 00:28:25.430
start it. Three times the mass of the sun.
737
00:28:26.150 --> 00:28:28.230
Three to the power four is three times three
738
00:28:28.230 --> 00:28:30.430
times three times three. That's 81 if my
739
00:28:30.430 --> 00:28:33.030
mental arithmetic is correct. So three times
740
00:28:33.030 --> 00:28:35.270
the mass of the sun burns its fuel 81 times
741
00:28:35.270 --> 00:28:38.050
as quickly, which means it would live a 27th
742
00:28:38.050 --> 00:28:40.930
as long. Which means instead of 12 billion
743
00:28:40.930 --> 00:28:43.400
years, you get down to, 1.2 billion years,
744
00:28:43.400 --> 00:28:45.360
you get down to or like, 600 million years,
745
00:28:45.440 --> 00:28:48.200
500 million years. So there will have been a
746
00:28:48.200 --> 00:28:50.520
lot of stars that were more m massive than
747
00:28:50.520 --> 00:28:52.560
the sun that have lived and died and created
748
00:28:52.560 --> 00:28:54.960
white dwarfs. And so there's going to be a
749
00:28:54.960 --> 00:28:57.880
lot of white dwarfs out there. I saw
750
00:28:57.880 --> 00:29:00.120
someone talking a while back about how old
751
00:29:00.120 --> 00:29:02.760
the oldest white dwarf will be in how dim it
752
00:29:02.760 --> 00:29:04.680
will be, because white dwarfs just cool and
753
00:29:04.680 --> 00:29:07.240
gradually go from being blue to white to
754
00:29:07.240 --> 00:29:09.360
yellow to red. You know, gradually dim down.
755
00:29:09.680 --> 00:29:11.910
Yeah. but what that all means is that there
756
00:29:11.910 --> 00:29:14.350
are probably a really large population of
757
00:29:14.350 --> 00:29:16.190
white dwarfs out there. We know quite a large
758
00:29:16.190 --> 00:29:19.030
number, but we won't know anywhere near
759
00:29:19.030 --> 00:29:21.230
as many of them as we do stars that are
760
00:29:21.230 --> 00:29:22.630
actually the mass of the sun, that are in the
761
00:29:22.630 --> 00:29:24.990
prime of their life because they're much
762
00:29:24.990 --> 00:29:27.110
fainter and harder to spot because they've
763
00:29:27.110 --> 00:29:28.670
got a much smaller surface area. So even
764
00:29:28.670 --> 00:29:30.130
though they're hot, they're tiny and,
765
00:29:30.080 --> 00:29:31.940
therefore they're faint. and the best example
766
00:29:31.940 --> 00:29:33.860
of that, of course, is a white dwarf that is
767
00:29:33.860 --> 00:29:36.220
a companion to Sirius. Sirius is the
768
00:29:36.220 --> 00:29:38.020
brightest star in the night sky. It's more
769
00:29:38.020 --> 00:29:40.860
massive than the Sun. It's also nearby. Its
770
00:29:41.100 --> 00:29:44.060
white dwarf companion is something
771
00:29:44.060 --> 00:29:46.940
like a factor of a million times fainter than
772
00:29:46.940 --> 00:29:49.500
Sirius is. So even though the white dwarf is
773
00:29:49.500 --> 00:29:51.660
comparable in Master Sirius A,
774
00:29:52.300 --> 00:29:55.060
it is like a million times dimmer because
775
00:29:55.060 --> 00:29:57.220
it's so tiny. And that's why they're Hard to
776
00:29:57.220 --> 00:29:57.500
find.
777
00:29:58.270 --> 00:30:00.070
Andrew Dunkley: Yeah, even though there's probably a hell of
778
00:30:00.070 --> 00:30:02.980
a lot of them out there. Okay, if you would
779
00:30:02.980 --> 00:30:05.180
like to read more about this particular white
780
00:30:05.180 --> 00:30:08.050
dwarf star that is, you know, got a case of
781
00:30:08.050 --> 00:30:10.610
the munchies, probably spent too much time
782
00:30:10.770 --> 00:30:13.360
smoking the juju. you can read all about it
783
00:30:14.240 --> 00:30:17.200
in the Astronomical Journal. This is Space
784
00:30:17.200 --> 00:30:20.080
Nuts with Andrew Dunkley and Jonti Horner.
785
00:30:20.240 --> 00:30:22.680
Jonti Horner: Okay, we checked all four systems and being
786
00:30:22.680 --> 00:30:24.170
with the jerk space nets,
787
00:30:25.140 --> 00:30:26.600
Andrew Dunkley: Don'T know why we went down that road.
788
00:30:26.600 --> 00:30:29.280
Let's go to our next story. And this
789
00:30:29.280 --> 00:30:32.050
one is, this one's close to home.
790
00:30:32.080 --> 00:30:35.030
a, an object that is rapidly developing
791
00:30:35.030 --> 00:30:37.840
a ring system and it's it's in
792
00:30:37.840 --> 00:30:40.080
the outer solar system.
793
00:30:40.480 --> 00:30:43.120
Jonti Horner: It is, this is an object called Chiron,
794
00:30:43.920 --> 00:30:45.920
which was the first of the centaurs to be
795
00:30:45.920 --> 00:30:47.240
discovered. And I always like to talk about
796
00:30:47.240 --> 00:30:48.920
the centaurs because they're what I studied
797
00:30:48.920 --> 00:30:51.660
for my PhD, so, so I was at one
798
00:30:51.660 --> 00:30:54.220
point, 20 odd years ago, one of the world's
799
00:30:54.220 --> 00:30:56.140
experts in how these things move around the
800
00:30:56.140 --> 00:30:57.740
solar system. And then science has moved on
801
00:30:57.740 --> 00:31:00.060
and I haven't, so I probably can no longer
802
00:31:00.060 --> 00:31:02.740
claim that. But Chiron is
803
00:31:02.820 --> 00:31:04.980
an interesting object. It's an icy object,
804
00:31:05.220 --> 00:31:08.220
bit more than 200km across. It was
805
00:31:08.220 --> 00:31:10.900
one of, if not the first object to get both a
806
00:31:10.900 --> 00:31:12.980
classification as an asteroid and as a comet.
807
00:31:13.540 --> 00:31:15.940
So it was initially discovered as a tiny
808
00:31:15.940 --> 00:31:17.460
speck of light moving around. It's discovered
809
00:31:17.460 --> 00:31:19.300
by Cowell I think in 1970,
810
00:31:20.340 --> 00:31:22.380
moving on an orbit that spends nearly all its
811
00:31:22.380 --> 00:31:24.220
time between the orbits of Saturn and Uranus.
812
00:31:24.220 --> 00:31:25.980
At the minute. Long term it's an unstable
813
00:31:25.980 --> 00:31:28.500
orbit. There's about a, ah, one in three
814
00:31:28.500 --> 00:31:29.940
chance that this will eventually end up in
815
00:31:29.940 --> 00:31:31.540
the inner solar system at some point in the
816
00:31:31.540 --> 00:31:33.780
next few million years. And that's part of
817
00:31:33.780 --> 00:31:36.060
the work I did during my PhD was running
818
00:31:36.060 --> 00:31:37.540
simulations of where this thing's going to
819
00:31:37.540 --> 00:31:40.100
go. That in itself is interesting because
820
00:31:40.100 --> 00:31:42.580
it's about a bit more than 200km across.
821
00:31:43.300 --> 00:31:44.900
So if this thing got trapped in the inner
822
00:31:44.900 --> 00:31:46.540
solar system, it will be, be a comet like
823
00:31:46.540 --> 00:31:48.780
nothing we've seen in recorded history. Hale
824
00:31:48.780 --> 00:31:51.660
Bopp, which was ridiculous, had a 50
825
00:31:51.660 --> 00:31:54.660
kilometer nucleus. If this thing's 250
826
00:31:54.660 --> 00:31:56.420
kilometers across, that's five times the
827
00:31:56.420 --> 00:31:59.220
radius, which means it's something like 25
828
00:31:59.220 --> 00:32:01.899
times the surface area, which means it will
829
00:32:01.899 --> 00:32:04.450
be a lot more impressive. So it's obviously
830
00:32:04.450 --> 00:32:07.130
an interesting object. Back in
831
00:32:07.130 --> 00:32:10.010
2011, team of scientists
832
00:32:10.410 --> 00:32:13.200
traveled across the world to gather to
833
00:32:13.200 --> 00:32:15.560
watch Chiron block out the light from a
834
00:32:15.640 --> 00:32:18.000
background star. So as this thing's moving
835
00:32:18.000 --> 00:32:20.560
through space, it just happened to pass in
836
00:32:20.560 --> 00:32:23.080
front of a star, from a subset of locations
837
00:32:23.080 --> 00:32:25.680
across the Earth. Now the distant stars are
838
00:32:25.680 --> 00:32:27.839
effectively so far away, we can consider the
839
00:32:27.839 --> 00:32:30.640
light coming in perfectly parallel. And
840
00:32:30.640 --> 00:32:32.200
so a 200 kilometer
841
00:32:33.000 --> 00:32:35.240
centaur will cast a shadow on the earth
842
00:32:35.240 --> 00:32:37.280
that's 200 kilometers across. And that shadow
843
00:32:37.280 --> 00:32:39.730
will whip across our planet. As the object
844
00:32:39.730 --> 00:32:41.570
and the Earth move around the sun, the shadow
845
00:32:41.570 --> 00:32:43.850
moves, the Earth moves through it. And so you
846
00:32:43.850 --> 00:32:46.850
get a 200 kilometer roughly scale band on the
847
00:32:46.850 --> 00:32:48.970
Earth where that star will disappear, then
848
00:32:48.970 --> 00:32:51.810
reappear. We know how fast everything's
849
00:32:51.810 --> 00:32:53.690
moving. So if you can get in that location,
850
00:32:54.010 --> 00:32:56.210
have a lot of telescopes spread out in a
851
00:32:56.210 --> 00:32:58.730
line, you can observe that
852
00:32:58.730 --> 00:33:01.330
occultation event and, by how long the star
853
00:33:01.330 --> 00:33:03.250
vanishes from different locations, you can
854
00:33:03.250 --> 00:33:05.640
actually figure out the shape and the size of
855
00:33:05.640 --> 00:33:08.320
the centaur because you can essentially map
856
00:33:08.560 --> 00:33:11.320
that shadow. And if you're near the edge, the
857
00:33:11.320 --> 00:33:12.880
star will disappear and reappear really
858
00:33:12.880 --> 00:33:14.520
quickly. If you're near the middle, you'll
859
00:33:14.520 --> 00:33:17.080
get a longer period where it vanishes. So
860
00:33:17.080 --> 00:33:18.720
these kind of, ah, occultation observations
861
00:33:18.800 --> 00:33:21.520
are really valuable to scientists. What
862
00:33:21.520 --> 00:33:23.560
happened in 2011 was they set their
863
00:33:23.560 --> 00:33:25.280
telescopes up and started watching a bit
864
00:33:25.280 --> 00:33:26.760
early to make sure they were looking at the
865
00:33:26.760 --> 00:33:29.320
star. And they noticed the star flickered on
866
00:33:29.320 --> 00:33:31.400
and off a couple of times before it properly
867
00:33:31.400 --> 00:33:33.540
disappeared for the main occultation. Then
868
00:33:33.540 --> 00:33:35.380
after it reappeared, it flickered on and off
869
00:33:35.380 --> 00:33:37.580
again a couple of times. And that's really
870
00:33:37.580 --> 00:33:40.420
weird. Now there was a kind of
871
00:33:40.420 --> 00:33:42.260
precedent for this with observations that
872
00:33:42.260 --> 00:33:44.780
were made in 1977, I believe,
873
00:33:45.100 --> 00:33:47.820
of Uranus, which was being observed from, I
874
00:33:47.820 --> 00:33:49.540
think it was the Kuiper Airborne Observatory
875
00:33:49.540 --> 00:33:52.100
doing one of these occultations. And they'd
876
00:33:52.100 --> 00:33:54.660
observed Uranus for this occultation because
877
00:33:54.660 --> 00:33:57.180
they wanted to understand the atmosphere of
878
00:33:57.180 --> 00:33:59.500
Uranus. And they figured as a stalwart behind
879
00:33:59.500 --> 00:34:02.109
Uranus, you'd see it not just disappear, but
880
00:34:02.109 --> 00:34:03.989
actually fade out as the light passed through
881
00:34:03.989 --> 00:34:06.149
the atmosphere. So you could measure the
882
00:34:06.149 --> 00:34:08.549
atmosphere and with that occultation of
883
00:34:08.549 --> 00:34:11.549
Uranus, occultation by Uranus, sorry, they
884
00:34:11.549 --> 00:34:12.949
got this flickering on and off thing. And
885
00:34:12.949 --> 00:34:14.749
that was the discovery of Uranus, of ring
886
00:34:14.749 --> 00:34:17.749
system. So basically the star vanished behind
887
00:34:17.749 --> 00:34:19.149
the rings, then reappeared, then vanished
888
00:34:19.149 --> 00:34:20.749
again, then reappeared, then went behind the
889
00:34:20.749 --> 00:34:23.629
planet. Right. So with this
890
00:34:23.629 --> 00:34:26.589
2011 event, the same kind of thing applied.
891
00:34:27.179 --> 00:34:29.139
It was the discovery of a ring system around
892
00:34:29.139 --> 00:34:31.259
this icy object. So this is a tiny thing,
893
00:34:31.899 --> 00:34:34.539
smaller than even Mimas, that we talked about
894
00:34:34.539 --> 00:34:36.299
last week with the subsurface ocean,
895
00:34:36.539 --> 00:34:38.419
something so small that its gravity is
896
00:34:38.419 --> 00:34:39.659
probably not strong enough to make it
897
00:34:39.659 --> 00:34:42.360
spherical. It's probably peanut shaped or
898
00:34:42.349 --> 00:34:44.028
rugby ball shaped or something like this.
899
00:34:44.028 --> 00:34:46.508
It's probably not spherical. Around this
900
00:34:46.508 --> 00:34:48.628
object, it seems that there is a system of
901
00:34:48.628 --> 00:34:50.268
rings where there are three or four narrow
902
00:34:50.268 --> 00:34:52.548
rings at various distances. I think the
903
00:34:52.548 --> 00:34:55.419
distances are something like 273, 325, 438
904
00:34:55.419 --> 00:34:58.379
and 1400 kilometers from the
905
00:34:58.379 --> 00:35:01.259
center of Chiron. Got this ring
906
00:35:01.259 --> 00:35:03.819
system and it's been observed again since
907
00:35:03.819 --> 00:35:06.739
they did observations in 2018, 2022 and
908
00:35:06.739 --> 00:35:09.579
2023, where they again figured
909
00:35:09.579 --> 00:35:11.579
out that the shadow of Chiron was going to
910
00:35:11.579 --> 00:35:13.939
scan across the planet, got a load of
911
00:35:13.939 --> 00:35:16.299
telescopes, went on a road trip and observed
912
00:35:16.299 --> 00:35:18.739
it happen to get more information about the
913
00:35:18.739 --> 00:35:21.059
rings. Because having a ring system around an
914
00:35:21.059 --> 00:35:23.139
object that isn't a planet is really cool.
915
00:35:23.649 --> 00:35:23.969
Andrew Dunkley: Yeah.
916
00:35:24.049 --> 00:35:26.489
Jonti Horner: And how did it form? How long has it been
917
00:35:26.489 --> 00:35:28.329
there? What's going on? How common are ring
918
00:35:28.329 --> 00:35:31.249
systems like this? Incidentally, a former PhD
919
00:35:31.249 --> 00:35:33.649
student of mine, Jeremy Wood, did some really
920
00:35:33.649 --> 00:35:36.089
cool dynamical studies that basically showed
921
00:35:36.089 --> 00:35:38.289
that the ring system could be
922
00:35:38.449 --> 00:35:40.809
primordial. It could be as old as the solar
923
00:35:40.809 --> 00:35:43.129
system. From the point of view of Chiron has
924
00:35:43.129 --> 00:35:45.009
never been close enough to one of the planets
925
00:35:45.009 --> 00:35:48.009
to disrupt the rings. So that
926
00:35:48.009 --> 00:35:49.529
doesn't put an edge limit on it, but it was
927
00:35:49.529 --> 00:35:52.169
still quite cool. What the new observations
928
00:35:52.169 --> 00:35:53.749
have shown though, is that, the ring system
929
00:35:53.829 --> 00:35:56.309
now seems to be different to how it was in
930
00:35:56.309 --> 00:35:59.269
2011. In other words, the ring
931
00:35:59.269 --> 00:36:01.949
system is evolving before our very
932
00:36:01.949 --> 00:36:04.069
eyes and it actually seems to be a denser,
933
00:36:04.069 --> 00:36:06.829
stronger ring system now than it was 10 or 15
934
00:36:06.829 --> 00:36:09.109
years ago. So it's possible that we're
935
00:36:09.109 --> 00:36:11.389
actually witnessing this ring system as it is
936
00:36:11.389 --> 00:36:14.069
forming or as it's changing over time.
937
00:36:14.069 --> 00:36:16.869
Now I know Chiron has been quite active,
938
00:36:17.309 --> 00:36:19.469
it's been outgassing because it's been closer
939
00:36:19.469 --> 00:36:21.629
to the sun, hence the cometary type
940
00:36:21.629 --> 00:36:24.629
classification it got. Maybe some
941
00:36:24.629 --> 00:36:26.309
of the material it's ejecting in that
942
00:36:26.309 --> 00:36:28.389
outgassing is being ejected gently enough
943
00:36:28.389 --> 00:36:31.009
that it doesn't escape from Chiron and,
944
00:36:30.959 --> 00:36:33.799
that's repopulating the rings. We just don't
945
00:36:33.799 --> 00:36:36.719
know. But the only way we'll find
946
00:36:36.719 --> 00:36:38.399
out is by doing more of these observations.
947
00:36:38.399 --> 00:36:41.279
But I think it's just really exciting and
948
00:36:41.279 --> 00:36:44.229
it's a really good reminder again that we
949
00:36:44.229 --> 00:36:46.069
always kind of imagine the solar system as a
950
00:36:46.069 --> 00:36:48.429
very sad and boring, placid place where not
951
00:36:48.429 --> 00:36:50.709
much changing anymore because it's four and a
952
00:36:50.709 --> 00:36:52.389
half billion years old. And as you get older,
953
00:36:52.389 --> 00:36:53.949
you Get a bit more sedentary and not much
954
00:36:53.949 --> 00:36:56.829
happens. But in fact it's a reminder that
955
00:36:56.829 --> 00:36:59.269
the solar system's a really dynamic place and
956
00:36:59.349 --> 00:37:01.269
things are constantly influenced, constantly
957
00:37:01.269 --> 00:37:03.429
changing. We talked about it last week. The
958
00:37:03.429 --> 00:37:05.829
ocean on Mimas that is possibly
959
00:37:06.149 --> 00:37:08.469
only 15 million years old. Now, 50 million
960
00:37:08.469 --> 00:37:11.029
years sounds like a really long time, but in
961
00:37:11.029 --> 00:37:12.749
a system that's four and a half thousand
962
00:37:12.749 --> 00:37:15.709
million years old, that's like something
963
00:37:15.709 --> 00:37:17.829
that has happened to me in the last couple of
964
00:37:17.829 --> 00:37:20.389
weeks. That's a new feature, not something
965
00:37:20.389 --> 00:37:22.389
I've had since birth. And this is yet another
966
00:37:22.389 --> 00:37:24.069
example of the fact that the solar system
967
00:37:24.069 --> 00:37:26.709
just seems to be continually rapidly changing
968
00:37:26.709 --> 00:37:27.309
and evolving.
969
00:37:27.789 --> 00:37:29.629
Andrew Dunkley: Yeah, yeah, it's a really interesting
970
00:37:29.789 --> 00:37:32.769
situation. how far out is chiron?
971
00:37:33.809 --> 00:37:36.089
Jonti Horner: It varies. So it's closest to the sun, It's a
972
00:37:36.089 --> 00:37:37.729
little bit closer to the sun than the orbit
973
00:37:37.729 --> 00:37:39.719
of Saturn. at its furthest, it's a bit
974
00:37:39.719 --> 00:37:41.279
further away than the orbit of Uranus. And
975
00:37:41.279 --> 00:37:42.959
that's an unstable orbit. So it bounces
976
00:37:42.959 --> 00:37:45.479
around over time, it will have encounters
977
00:37:45.479 --> 00:37:47.839
with them that fling it around. But at the
978
00:37:47.839 --> 00:37:50.399
minute it's in the outer solar system
979
00:37:50.479 --> 00:37:53.159
between the orbits of Saturn and Uranus most
980
00:37:53.159 --> 00:37:55.679
of the time. Unstable solution. It probably
981
00:37:55.679 --> 00:37:57.719
originated out beyond the orbit of Neptune.
982
00:37:57.719 --> 00:38:00.199
And it's one of this population called the
983
00:38:00.199 --> 00:38:03.059
Centaurs that are, the future parents of the
984
00:38:03.059 --> 00:38:04.699
next generation of short period comets.
985
00:38:04.699 --> 00:38:06.139
Effectively in the same way that the near
986
00:38:06.139 --> 00:38:08.379
Earth asteroids have their origin in the
987
00:38:08.379 --> 00:38:10.939
asteroid belt, short period comets have their
988
00:38:10.939 --> 00:38:13.579
origin in the Transeptunian region. But to
989
00:38:13.579 --> 00:38:15.059
get here from there, they've got to pass
990
00:38:15.059 --> 00:38:16.419
through the outer solar system. And that's
991
00:38:16.419 --> 00:38:17.459
what the Centaurs are.
992
00:38:18.019 --> 00:38:20.299
Andrew Dunkley: Okay. Fascinating. Yeah, it's really
993
00:38:20.299 --> 00:38:22.659
interesting and probably not one that,
994
00:38:23.048 --> 00:38:25.529
too many people would be aware of. I remember
995
00:38:25.529 --> 00:38:28.529
when it was making the news some
996
00:38:28.529 --> 00:38:30.969
years ago, and that's why the name stuck when
997
00:38:30.969 --> 00:38:33.499
you, when you sent the story to me. But, you
998
00:38:33.499 --> 00:38:35.459
don't really hear much about it. But now
999
00:38:35.929 --> 00:38:37.769
we've got a very good reason to look at it.
1000
00:38:38.209 --> 00:38:40.129
if you would like to look into that
1001
00:38:40.129 --> 00:38:43.009
particular paper, it's been published in
1002
00:38:43.009 --> 00:38:45.809
the Astrophysical Journal Letters.
1003
00:38:51.809 --> 00:38:53.729
Our final story, Jonti, is,
1004
00:38:54.689 --> 00:38:57.449
an exoplanet that the popular press are going
1005
00:38:57.449 --> 00:38:59.909
to say has got, some kind of life on it. it's
1006
00:38:59.909 --> 00:39:02.759
a, it's a maybe life candidate, story,
1007
00:39:02.759 --> 00:39:05.749
this one. And Yeah, but they're still
1008
00:39:05.749 --> 00:39:07.309
using the term super Earth.
1009
00:39:07.469 --> 00:39:09.869
Jonti Horner: Yeah, I'll keep this one a little bit short
1010
00:39:09.869 --> 00:39:12.709
and try not to get too grumpy. But one of my
1011
00:39:12.709 --> 00:39:15.549
big bug bears all the way through my career
1012
00:39:15.629 --> 00:39:18.479
is a good way for people to get media
1013
00:39:18.479 --> 00:39:20.679
coverage of their new planet discovery is say
1014
00:39:20.679 --> 00:39:23.119
it could be habitable. It's in the Goldilocks
1015
00:39:23.119 --> 00:39:23.759
zone. Hooray.
1016
00:39:24.079 --> 00:39:25.279
Andrew Dunkley: Using the L word.
1017
00:39:25.599 --> 00:39:27.119
Jonti Horner: Rumble, rumble, grumble, grumble.
1018
00:39:27.199 --> 00:39:28.879
Andrew Dunkley: It's a four letter word too, that one.
1019
00:39:28.879 --> 00:39:30.829
Jonti Horner: It is, and it's one of the terrible four
1020
00:39:30.829 --> 00:39:33.669
letter words. Part of the problem here is
1021
00:39:33.659 --> 00:39:35.499
there's this concept of the Goldilocks zone,
1022
00:39:35.499 --> 00:39:37.019
of the habitable zone, which has become
1023
00:39:37.019 --> 00:39:38.939
really entrenched in the popular
1024
00:39:38.939 --> 00:39:41.139
consciousness. And it's always viewed as
1025
00:39:41.139 --> 00:39:43.539
being this sweet spot for life. And the idea
1026
00:39:43.539 --> 00:39:45.219
is that if you have a planet in the habitable
1027
00:39:45.219 --> 00:39:46.659
zone, it will have liquid water on its
1028
00:39:46.659 --> 00:39:48.739
surface and all sorts of happy life things
1029
00:39:48.739 --> 00:39:51.179
will happen and everything will be good.
1030
00:39:52.169 --> 00:39:54.649
What it actually means is that if you took
1031
00:39:54.649 --> 00:39:56.829
the Earth, as it is today and put it where
1032
00:39:56.829 --> 00:39:59.149
that planet is, the Earth would still
1033
00:39:59.149 --> 00:40:01.869
maintain its liquid water because planets are
1034
00:40:01.869 --> 00:40:04.669
really diverse. If you took Venus and put
1035
00:40:04.669 --> 00:40:06.349
Venus where the Earth is, With Venus's
1036
00:40:06.349 --> 00:40:08.109
current atmosphere, Venus will be too hot to
1037
00:40:08.109 --> 00:40:10.469
have liquid water. But if you observe the
1038
00:40:10.469 --> 00:40:12.589
solar system from a long long way away and
1039
00:40:12.589 --> 00:40:15.079
you discovered Venus on the Earth's
1040
00:40:15.079 --> 00:40:17.729
orbit, it wouldn't look any different to the
1041
00:40:17.729 --> 00:40:19.059
Earth. it's a planet about the size of the
1042
00:40:19.059 --> 00:40:21.069
Earth, sat in the habitable sun. We, it's
1043
00:40:21.069 --> 00:40:23.709
habitable. Hooray. Whereas Venus is actually
1044
00:40:23.709 --> 00:40:25.749
so hot that on the surface it had melt lead.
1045
00:40:25.749 --> 00:40:27.629
And I certainly wouldn't want to visit there.
1046
00:40:27.629 --> 00:40:30.389
It's even hotter than my room was the other
1047
00:40:30.389 --> 00:40:32.869
night when the power cut had happened. And
1048
00:40:32.869 --> 00:40:35.849
that was bad enough and brutal enough. so
1049
00:40:35.849 --> 00:40:38.329
what this means is that ah, people
1050
00:40:38.649 --> 00:40:40.729
have become very fond of
1051
00:40:41.809 --> 00:40:44.609
find a planet around a star, you can work out
1052
00:40:44.849 --> 00:40:46.649
where the boundaries of the habitable zone
1053
00:40:46.649 --> 00:40:48.649
will be based on a few assumptions. And this
1054
00:40:48.649 --> 00:40:51.409
is work going back about a decade of the
1055
00:40:51.409 --> 00:40:53.129
definitions we use now. And you've got the
1056
00:40:53.129 --> 00:40:55.249
conservative and the optimistic habitable
1057
00:40:55.249 --> 00:40:57.399
zone, which are basically loosely based
1058
00:40:57.399 --> 00:40:59.839
around the fact that if you're as close to
1059
00:40:59.839 --> 00:41:02.279
the star that you get an amount of radiation
1060
00:41:02.279 --> 00:41:04.119
coming in comparable to Venus, you'll be too
1061
00:41:04.119 --> 00:41:05.959
hot. If you're about where Mars is, you'll be
1062
00:41:05.959 --> 00:41:07.359
too cold, but in the middle you'll be just
1063
00:41:07.359 --> 00:41:09.899
right m. and that's about it.
1064
00:41:10.059 --> 00:41:12.659
Now that definition doesn't really take any
1065
00:41:12.659 --> 00:41:14.339
account of the mass of the planet or its
1066
00:41:14.339 --> 00:41:17.339
atmosphere. What that
1067
00:41:17.339 --> 00:41:20.099
means is that ah, when you find a planet that
1068
00:41:20.099 --> 00:41:22.139
is a super Earth that Is four times the mass
1069
00:41:22.139 --> 00:41:24.539
of the Earth. That is almost certainly
1070
00:41:24.859 --> 00:41:27.019
nothing like our planet at all.
1071
00:41:27.899 --> 00:41:30.059
You'll do a calculation and say it sits in
1072
00:41:30.059 --> 00:41:32.779
the optimistic habitable zone. So there is a
1073
00:41:32.779 --> 00:41:34.419
potential it could have liquid water on its
1074
00:41:34.419 --> 00:41:37.369
surface. That's full of a whole heap
1075
00:41:37.369 --> 00:41:39.409
of assumptions. But to me it's a really long
1076
00:41:39.409 --> 00:41:41.009
stretch from saying it could have life.
1077
00:41:41.649 --> 00:41:41.969
Andrew Dunkley: A.
1078
00:41:41.969 --> 00:41:43.409
Jonti Horner: You're assuming it's got the right kind of
1079
00:41:43.409 --> 00:41:45.529
atmosphere to have liquid water where it's
1080
00:41:45.529 --> 00:41:46.889
four times the mass of the Earth. So its
1081
00:41:46.889 --> 00:41:48.589
atmosphere is almost certainly much, much m
1082
00:41:48.609 --> 00:41:50.689
thicker, Therefore
1083
00:41:51.329 --> 00:41:53.649
likely has a much stronger greenhouse effect,
1084
00:41:54.049 --> 00:41:55.969
Therefore probably runaway greenhouse. Not
1085
00:41:55.969 --> 00:41:56.289
good.
1086
00:41:56.849 --> 00:41:58.729
The other thing with this particular planet,
1087
00:41:58.729 --> 00:42:01.499
GJ 251C is it's a super
1088
00:42:01.499 --> 00:42:03.639
Earth orbiting a red dwarf star, ah,
1089
00:42:04.259 --> 00:42:06.749
nearby, less than 20 light years away. And
1090
00:42:06.749 --> 00:42:08.389
that's part of why people are excited. It's
1091
00:42:08.389 --> 00:42:09.869
near enough that we'll learn a lot more about
1092
00:42:09.869 --> 00:42:11.909
it in the future. However,
1093
00:42:12.629 --> 00:42:15.069
planet orbiting a red dwarf star means that
1094
00:42:15.069 --> 00:42:16.609
to be in the habitable zone, it's got to be
1095
00:42:16.609 --> 00:42:18.889
close in. This thing goes around its star
1096
00:42:18.889 --> 00:42:21.689
every 54 days, which means that it is
1097
00:42:21.689 --> 00:42:23.729
closer to its star than Mercury is to the
1098
00:42:23.729 --> 00:42:25.769
sun. And given the difference in the masses,
1099
00:42:25.769 --> 00:42:28.239
it's actually much closer in than that. That
1100
00:42:28.239 --> 00:42:30.439
means it's up close and personal with a red
1101
00:42:30.439 --> 00:42:32.759
dwarf star, which are notorious for being
1102
00:42:32.999 --> 00:42:35.479
active and flary and noisy, Particularly when
1103
00:42:35.479 --> 00:42:37.279
they're young. They're tempestuous teenagers
1104
00:42:37.279 --> 00:42:40.239
in their early days with mega stellar flares
1105
00:42:40.239 --> 00:42:43.039
and stuff like this. So it seems to be
1106
00:42:43.039 --> 00:42:44.999
fairly widely accepted that planets around
1107
00:42:44.999 --> 00:42:47.679
red dwarf stars that are close enough to be
1108
00:42:47.679 --> 00:42:50.119
warm enough to have liquid water will have a
1109
00:42:50.119 --> 00:42:51.879
hard time holding onto their atmospheres,
1110
00:42:51.959 --> 00:42:53.119
Particularly when the stars are young,
1111
00:42:53.119 --> 00:42:55.769
because it'll be having all sorts of
1112
00:42:55.769 --> 00:42:57.819
bonkers fun. And that's kind of borne out
1113
00:42:57.899 --> 00:43:00.699
with the planets around Trappist 1, which for
1114
00:43:00.699 --> 00:43:02.939
years have been people saying these are the
1115
00:43:02.939 --> 00:43:04.499
most Earth like planets ever and we'll find
1116
00:43:04.499 --> 00:43:06.899
life on them and hooray. And then when they
1117
00:43:06.899 --> 00:43:08.539
finally got to use the James Webb space
1118
00:43:08.539 --> 00:43:10.739
telescope and look at those planets, none of
1119
00:43:10.739 --> 00:43:13.179
them have an atmosphere. Now I don't know
1120
00:43:13.179 --> 00:43:15.499
about you, but I kind of like to breathe.
1121
00:43:15.659 --> 00:43:17.949
It's a fairly important part of living. And a
1122
00:43:17.949 --> 00:43:19.949
planet without an atmosphere is not going to
1123
00:43:19.949 --> 00:43:21.629
have liquid water on the surface because if
1124
00:43:21.629 --> 00:43:23.029
you take the atmosphere away, there's no
1125
00:43:23.029 --> 00:43:25.769
pressure, the oceans boil and then are blown
1126
00:43:25.769 --> 00:43:28.129
away by the red dwarfs, which makes that
1127
00:43:28.129 --> 00:43:30.249
planet a desiccated husk, which not
1128
00:43:30.249 --> 00:43:32.929
particularly habitable. The reason I Get
1129
00:43:33.169 --> 00:43:35.969
energized and activated about this. It's a
1130
00:43:35.969 --> 00:43:37.729
lovely discovery. It's a really interesting
1131
00:43:37.729 --> 00:43:39.439
planet. We'll, learn a lot more about planets
1132
00:43:39.439 --> 00:43:41.999
elsewhere. If there is an atmosphere, it's
1133
00:43:41.999 --> 00:43:43.639
around us now that's near enough to us that
1134
00:43:43.639 --> 00:43:45.119
with James Webb, we'll be able to study it,
1135
00:43:45.119 --> 00:43:46.599
learn more about the atmosphere. We'll learn
1136
00:43:46.599 --> 00:43:48.759
a whole heap from it. But I get really
1137
00:43:48.759 --> 00:43:50.479
energized about this because there's only so
1138
00:43:50.479 --> 00:43:52.399
many times that people can hear a story that
1139
00:43:52.399 --> 00:43:54.519
says we found the most Earth like planet ever
1140
00:43:55.239 --> 00:43:57.639
before they think we found the Earth before
1141
00:43:57.639 --> 00:44:00.279
they think we found life elsewhere. And that
1142
00:44:00.279 --> 00:44:02.359
then really devalues it. When we finally do
1143
00:44:02.359 --> 00:44:04.799
find planets that are, ah, properly like the
1144
00:44:04.799 --> 00:44:07.439
Earth, when we do find signs of life
1145
00:44:07.439 --> 00:44:09.759
elsewhere, scientists will be getting really
1146
00:44:09.759 --> 00:44:11.279
excited because we've finally done it. And
1147
00:44:11.279 --> 00:44:13.079
everybody will be like, well, why bother?
1148
00:44:13.079 --> 00:44:15.439
You've done this a million times before. The
1149
00:44:15.439 --> 00:44:16.999
whole boy who cried wolf thing
1150
00:44:18.519 --> 00:44:21.199
again, a big bugbear. And something that's
1151
00:44:21.199 --> 00:44:22.759
really critically important these days is
1152
00:44:22.759 --> 00:44:25.629
trust in science and trust in scientists. We,
1153
00:44:25.779 --> 00:44:27.819
we've got all the controversies about topics
1154
00:44:27.819 --> 00:44:29.249
that, are much more controversial than we're
1155
00:44:29.249 --> 00:44:31.369
talking about with astronomy, with vaccine
1156
00:44:31.369 --> 00:44:34.169
denial, with climate change denial, with
1157
00:44:34.169 --> 00:44:36.449
people refusing to evacuate in the path of a
1158
00:44:36.449 --> 00:44:38.409
hurricane that's coming because they don't
1159
00:44:38.409 --> 00:44:41.289
believe the scientists. Anything that
1160
00:44:41.528 --> 00:44:44.009
makes people less trusting of scientists
1161
00:44:44.009 --> 00:44:46.809
because they're overblowing stories is
1162
00:44:46.809 --> 00:44:49.809
damaging now far more than it has been in
1163
00:44:49.809 --> 00:44:51.569
decades past. It's part of why I get so
1164
00:44:51.569 --> 00:44:54.209
frustrated with Avi Loeb and Three Eye Atlas.
1165
00:44:54.209 --> 00:44:56.739
It's why get frustrated with the media
1166
00:44:56.739 --> 00:44:58.259
coverage of stories like this and the
1167
00:44:58.259 --> 00:45:00.819
scientists pushing, I think, somewhat
1168
00:45:00.819 --> 00:45:03.299
unethically an argument that this could be a
1169
00:45:03.299 --> 00:45:06.259
habitable planet because it makes
1170
00:45:06.259 --> 00:45:07.819
the rest of us look like fools. And it makes
1171
00:45:07.819 --> 00:45:10.259
people, it gives them ammunition to say,
1172
00:45:10.259 --> 00:45:12.819
well, scientists lie to us when they're not.
1173
00:45:13.379 --> 00:45:15.339
They're saying that this meets the criteria
1174
00:45:15.339 --> 00:45:16.819
for the Habitable Zone paper that was
1175
00:45:16.819 --> 00:45:19.219
published 10 years ago. But
1176
00:45:19.539 --> 00:45:21.899
it weakens that trust in science, which is so
1177
00:45:21.899 --> 00:45:23.739
important now more than it ever has done. And
1178
00:45:23.739 --> 00:45:25.369
I said I wouldn't go on a run and I'm now
1179
00:45:25.839 --> 00:45:27.719
waving the flag and banging the table and all
1180
00:45:27.719 --> 00:45:30.359
the rest of it. But it's a frustration that's
1181
00:45:30.359 --> 00:45:32.159
wider than this story. And this story is
1182
00:45:32.159 --> 00:45:34.799
lovely. It's an awesome discovery. They found
1183
00:45:34.799 --> 00:45:36.519
a planet going around a star. That's very
1184
00:45:36.519 --> 00:45:38.399
cool. We'll learn a lot more about it. It's a
1185
00:45:38.399 --> 00:45:41.159
brilliant result. You don't need to tag every
1186
00:45:41.159 --> 00:45:43.079
result like this and say that this planet
1187
00:45:43.079 --> 00:45:43.759
could have life.
1188
00:45:45.519 --> 00:45:47.759
Andrew Dunkley: And yet that's what, that's what happens.
1189
00:45:47.719 --> 00:45:49.419
it's sort of like, what artificial
1190
00:45:49.419 --> 00:45:51.619
intelligence is doing to social media. You
1191
00:45:51.619 --> 00:45:53.999
don't know. You don't know what you're
1192
00:45:53.999 --> 00:45:56.719
looking at anymore. And my
1193
00:45:56.719 --> 00:45:59.559
trust levels have dropped significantly in
1194
00:45:59.559 --> 00:46:00.199
recent months.
1195
00:46:02.119 --> 00:46:04.729
Jonti Horner: My dad is, 80, and
1196
00:46:04.729 --> 00:46:06.529
he's still on Facebook. And he doesn't like
1197
00:46:06.529 --> 00:46:08.329
it, but he's on it because it's a way to
1198
00:46:08.329 --> 00:46:10.089
communicate with people back in the uk. Moved
1199
00:46:10.089 --> 00:46:12.609
over here a few years ago and he's constantly
1200
00:46:12.609 --> 00:46:14.529
saying to me, he's getting so frustrated with
1201
00:46:14.529 --> 00:46:16.929
these AI stories and fake news things that he
1202
00:46:16.929 --> 00:46:18.569
doesn't know what to trust on there anymore
1203
00:46:18.649 --> 00:46:21.059
because he'll see a story that some famous
1204
00:46:21.059 --> 00:46:23.659
actors died and then he'll look up on
1205
00:46:23.659 --> 00:46:25.459
Wikipedia and they're still alive and kicking
1206
00:46:25.459 --> 00:46:26.779
and they've got a film coming out. But
1207
00:46:26.779 --> 00:46:28.099
there's this thing of, you'd never believe
1208
00:46:28.099 --> 00:46:31.059
the tragic photos. And it's
1209
00:46:31.059 --> 00:46:33.699
bizarre. And at a time when we need fidelity
1210
00:46:33.699 --> 00:46:36.019
and trust in our news and trust in our
1211
00:46:36.019 --> 00:46:38.979
science, we've got to be careful about how
1212
00:46:38.979 --> 00:46:41.099
much hyperbole we put into stories. I think.
1213
00:46:41.419 --> 00:46:43.979
Andrew Dunkley: I totally agree. Yes. If you'd like to read
1214
00:46:43.979 --> 00:46:46.809
about that, particular exoplanet, you can,
1215
00:46:47.159 --> 00:46:49.619
pick up that yarn through the Astronomical
1216
00:46:49.619 --> 00:46:51.419
Journal where they publish the paper. Or you
1217
00:46:51.419 --> 00:46:53.519
can read up on all the stories we've talked
1218
00:46:53.519 --> 00:46:53.719
about
1219
00:46:53.719 --> 00:46:56.639
today@space.com
1220
00:46:57.199 --> 00:46:59.569
and I'm sure a few other, platforms have
1221
00:46:59.569 --> 00:47:00.569
published them as well.
1222
00:47:01.019 --> 00:47:03.169
and that brings us to the end of, this
1223
00:47:03.409 --> 00:47:05.329
program. Jonti, thank you so much.
1224
00:47:05.969 --> 00:47:07.729
Jonti Horner: It's a pleasure. It's lovely to chat. Thanks
1225
00:47:07.729 --> 00:47:09.609
for bearing with me, being a bit flighty and
1226
00:47:09.609 --> 00:47:11.329
flirty thanks to the power cuts and the
1227
00:47:11.329 --> 00:47:11.649
weather.
1228
00:47:12.529 --> 00:47:15.129
Andrew Dunkley: You've done well. You've done well. We'll,
1229
00:47:15.129 --> 00:47:17.129
catch you on the next program, a Q and A
1230
00:47:17.129 --> 00:47:19.099
program. Johnty, Horn, a professor of
1231
00:47:19.099 --> 00:47:21.419
astrophysics at the University University of
1232
00:47:21.419 --> 00:47:24.079
Southern Queens. And thanks to Huw in the
1233
00:47:24.079 --> 00:47:26.399
studio, who couldn't be with us today
1234
00:47:27.119 --> 00:47:30.119
because he never tells me. I
1235
00:47:30.119 --> 00:47:32.639
have no idea. I just make up the reasons he's
1236
00:47:32.639 --> 00:47:34.839
not here. I honestly don't know why he didn't
1237
00:47:34.839 --> 00:47:36.719
turn up this week. Probably because we didn't
1238
00:47:36.719 --> 00:47:37.839
tell him when we were recording.
1239
00:47:38.319 --> 00:47:39.359
Jonti Horner: That might have been it.
1240
00:47:39.569 --> 00:47:41.769
Andrew Dunkley: and from me, Andrew Dunkley, thanks for your
1241
00:47:41.769 --> 00:47:44.409
company. Catch you on the very next episode
1242
00:47:44.409 --> 00:47:46.049
of Space Nuts. Bye.
1243
00:47:46.049 --> 00:47:46.369
Jonti Horner: Bye.
1244
00:47:47.409 --> 00:47:49.689
You've been listening to the Space Nuts
1245
00:47:49.689 --> 00:47:52.609
podcast, available at
1246
00:47:52.609 --> 00:47:54.569
Apple Podcasts, Spotify,
1247
00:47:54.729 --> 00:47:57.529
iHeartRadio or your favorite podcast
1248
00:47:57.529 --> 00:47:59.889
player. You can also stream on demand at
1249
00:47:59.889 --> 00:48:00.969
bytes. Com.
1250
00:48:01.289 --> 00:48:03.369
Andrew Dunkley: This has been another quality podcast
1251
00:48:03.369 --> 00:48:05.099
production from Bytes. Com.