July 30, 2025
Interstellar Intrigue: 3I Atlas, Cosmic Probes & the Quest for Extraterrestrial Life
Interstellar Visitors and the Cosmic Connection: A Journey Through Space Mysteries In this captivating episode of Space Nuts, hosts Heidi Campo and Professor Fred Watson explore the latest cosmic curiosities and fascinating astronomical phenomena....
Interstellar Visitors and the Cosmic Connection: A Journey Through Space Mysteries
In this captivating episode of Space Nuts, hosts Heidi Campo and Professor Fred Watson explore the latest cosmic curiosities and fascinating astronomical phenomena. From the intriguing interstellar object 3I Atlas to the unexpected influences of space weather on ancient civilizations, this episode is filled with insights that will expand your understanding of the universe.
Episode Highlights:
- The Mystery of 3I Atlas: The episode kicks off with a discussion about the interstellar object 3I Atlas, which is hurtling through our solar system. Fred explains its origins, orbit, and the speculation surrounding its potential extraterrestrial origins, sparked by Harvard physicist Avi Loeb.
- Space Weather and Human History: The conversation then shifts to how space weather impacts life on Earth. Fred shares insights from a recent interdisciplinary study that connects changes in the Earth's magnetic field with increased use of ochre by ancient peoples, suggesting a fascinating link between cosmic events and human behavior.
- The Dramatic Fate of TOI 2108B: The hosts then discuss the dramatic fate of the exoplanet TOI 2108B, which is spiraling towards its parent star. Fred outlines the potential scenarios for its demise, including tidal disruption and atmospheric loss, highlighting the ongoing research surrounding this extreme world.
- Interdisciplinary Connections: Throughout the episode, Heidi and Fred emphasize the importance of interdisciplinary research in understanding the cosmos and our place within it, showcasing how different fields of study can illuminate one another.
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.
Got a question for our Q&A episode? https://spacenutspodcast.com/ama
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support.
In this captivating episode of Space Nuts, hosts Heidi Campo and Professor Fred Watson explore the latest cosmic curiosities and fascinating astronomical phenomena. From the intriguing interstellar object 3I Atlas to the unexpected influences of space weather on ancient civilizations, this episode is filled with insights that will expand your understanding of the universe.
Episode Highlights:
- The Mystery of 3I Atlas: The episode kicks off with a discussion about the interstellar object 3I Atlas, which is hurtling through our solar system. Fred explains its origins, orbit, and the speculation surrounding its potential extraterrestrial origins, sparked by Harvard physicist Avi Loeb.
- Space Weather and Human History: The conversation then shifts to how space weather impacts life on Earth. Fred shares insights from a recent interdisciplinary study that connects changes in the Earth's magnetic field with increased use of ochre by ancient peoples, suggesting a fascinating link between cosmic events and human behavior.
- The Dramatic Fate of TOI 2108B: The hosts then discuss the dramatic fate of the exoplanet TOI 2108B, which is spiraling towards its parent star. Fred outlines the potential scenarios for its demise, including tidal disruption and atmospheric loss, highlighting the ongoing research surrounding this extreme world.
- Interdisciplinary Connections: Throughout the episode, Heidi and Fred emphasize the importance of interdisciplinary research in understanding the cosmos and our place within it, showcasing how different fields of study can illuminate one another.
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.
Got a question for our Q&A episode? https://spacenutspodcast.com/ama
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-astronomy-insights-cosmic-discoveries--2631155/support.
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Heidi Campo: Welcome back to another fun and exciting episode
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of Space Nuts, the podcast
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that is out of this world.
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Generic: 15 seconds. Guidance is internal.
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10, 9. Ignition
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sequence start. Space nuts. 5, 4, 3,
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2. 1. 2, 3, 4, 5, 5, 4,
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3, 2, 1. Space nuts astronauts
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report it feels good.
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Heidi Campo: And I'm your host for this, uh, American
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summer and Australian winter. My
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name is Heidi Campo, filling in for Andrew
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Dunkley. And joining us is the wonderful
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Professor Fred Watson, astronomer at
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large. How are you doing, Fred?
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Professor Fred Watson: Very well, thank you, Heidi. I've been m
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traveling since we last spoke and have explored the
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great state of Western Australia, uh,
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in great detail. If I remember rightly, Western Australia
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would encompass Texas three times. I think that's the
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figure. Uh, it's very large. And
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so we spent a lot of time,
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uh, in coaches, but saw some incredible sites, including,
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um, the Carnarvon space ah,
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facility, which was, uh, one of the places where
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radio, um, signals were picked up and uh,
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beamed out to the world during the Apollo
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era. So lovely to visit some of the
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places where history was made at a time
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when I was, you know,
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um, a young budding astronomer and very
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excited by the whole thing. So it's great to see all that old technology
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again.
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Heidi Campo: Yeah, there's just something special about the old technology.
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The way it looked and felt and was packaged. And the
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new, sleek, modern stuff is cool and great, but it just
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doesn't feel the same.
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Professor Fred Watson: That's right. Well, when they get fashion designers to
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design their spacesuits, you know that things have moved on quite a long
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way since the Apollo era.
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Heidi Campo: It really has changed. But one thing
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that will never change until it does
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is our fascination with extraterrestrials.
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Which leads us into our first story
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today.
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So the three. I don't know if this is the
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three I or the three lowercase l. Atlas.
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Um, Harvard's thinking
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maybe alien probe. What's going on
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here, Fred? Give us some sanity.
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Professor Fred Watson: Yeah, so 3i.
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It is 3i because it's the third
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interstellar, um, visitor,
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uh, that has been recorded. There are probably many more
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that we haven't detected. Uh, but this is an
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object which is flying through the solar system. We have talked
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about it before. Uh, we're going to talk about it again
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just because of a couple of things that have come
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up. Um, so the
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bottom line, 3i. Atlas. Atlas was the facility that
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discovered it. Uh, it's, uh,
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an object which is whizzing through the solar system
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at about 60 km per second in an orbit
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that tells you immediately that it has come from outside
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the solar system. It's not, uh, in any
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sense gravitationally bound to the Sun. So it's not part
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of the Sun's family of planets. It's from somewhere else.
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We don't know where it came from. And, uh, is whizzing through
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the solar system. If I remember rightly, it passes
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closest to the Sun. I think it is
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October. Uh, it's, um,
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certainly, um, uh, down the track. Uh, yes,
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it's the closest approach in October. Um,
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so, uh, it's probably a comet.
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Um, a comet is an object made
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of ice, uh, with dust embedded in
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it. Uh, it's, uh, it's
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um. You know, the thing about comets is when they get
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near the sun, the ice turns into a gas. And
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we see the uh, result of that, um,
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often stretched in a tail across the sky,
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which makes them very bright occasionally and
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also occasionally quite, um, you know,
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quite, um, inspiring to people who don't know
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what they're looking at, which is why they were often regarded as portents
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of doom, uh, down, uh, uh, in
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historical times. So this one however,
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is probably not going to do that. It may be a comet.
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It's thought to be about 20 km across, which is actually
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quite large for the nucleus of a comet.
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But the reason why I wanted to bring it up again
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is it's the headline that I almost
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could have predicted. Uh, is
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Interstellar Object 3I Atlas an alien
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probe. Harvard Physicist sparks
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debate. Uh, and that Harvard physicist
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is a very eminent, uh, uh,
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astrophysicist. Uh, I think he's still the director
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of the Harvard Smithsonian Institute for
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Astronomy. His name is Avi Loeb, and
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he is famous for always
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putting, uh, a slant
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which could be
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interpreted as uh, suggesting
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I'm, um, going a long way around this because I want to be careful with
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my words, uh, that things like this
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could have an intelligent origin. Uh, we
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had the same when the first of these
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interstellar visitors came by back in
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2017. Um, an object called
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Oumuamua, named after, uh.
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Uh, it's a Hawaiian name meaning first
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visitor from afar, which is a lovely name. An
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interesting object, only 100 meters or so across. We
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didn't discover it until it was on its way out of the solar system.
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It's probably shaped a bit like a pancake from the light
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curve, the way the light was reflected off it. Uh,
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but I think Avi, um, very
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quickly, uh, found what he thought was evidence
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that this thing perhaps had an
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extraterrestrial intelligence origin.
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And exactly the same thing has happened, uh,
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with the uh, three I atlas his
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reasoning though I think is really
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interesting, uh, and that is,
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uh, the curious couple of
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curious coincidences, uh, in
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regard to the orbit of 3i
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ATLAS. And remember, this is an open orbit. It's just a
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pathway through the solar system. It's not like
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an ellipse or a circle. It's going almost in a
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straight line. In fact, it's going so fast. But
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uh, what Aviloeb has noted
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is that, uh,
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this object will actually pass close
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to Mars, Venus and
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Jupiter. Uh, and
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so, uh, what Avi has done is a
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statistical test on the likelihood of
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that. And he estimates that the chance of
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this path occurring naturally by chance
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is 0.005%.
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Uh, and another little feature of this,
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as uh, I mentioned, uh, the object
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actually passes closest to the sun in October. It's actually the
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29th of October. And it turns out that
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when that is the case, it will
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be, uh, on the other side of the sun from the
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Earth. It'll be hidden from the Earth. And so
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AVI goes as far as to suggest that that is
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perhaps so that it does not get detected
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to avoid detection. Now I think that one's
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stretching it a little bit too far. But I do think it's
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interesting, uh, that the
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interstellar comet, if that's what it is,
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passes close by, uh, those three planets that
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I just mentioned. Whether it is proof that it's
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an alien visitor is another story.
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Heidi Campo: Well, I guess we'll find out.
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Professor Fred Watson: Well, we might not. Although, um,
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uh, so you know, what happens
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when something like this goes by is that all the world's
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telescopes concentrate uh, on it because it's
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something that you've only got a limited time frame to do.
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So there's a big, um,
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interest in bringing together lots of telescopes
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that can observe this object,
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uh, and uh, look at it in great detail,
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uh, with our uh, spectrographs and things of that
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sort, which analyze any gases that are coming
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from it, perhaps give us an idea of the sort of surface that
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it has. So those things will
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be, um, being looked at over the next
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month or so, couple of months. Um, but
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whether we will find enough evidence to
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demonstrate that it has an intelligent
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origin is a different story. Uh, because
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we could learn all sorts of things about it and still not
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have that answer. So, um, I think it's one that Space Nuts
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will keep an eye on over the next few months. Uh,
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and yes, if it turns out to have windows or
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spikes, ah, coming out of it or things like that,
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um, our uh, Space Nuts audience will be the first to know about
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it.
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Heidi Campo: Absolutely. You'll you. You'll always hear it
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here first.
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Generic: Okay, we checked all four systems and.
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Professor Fred Watson: Being with a go space nuts.
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Heidi Campo: Um, well, our next story is I guess
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a little bit less fringe alien
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stuff, but still odd and still
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so relevant to, you know, everything that we're looking at with
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space. But we're talking about how
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space weather,
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like, affects scientists here on Earth. So this
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is, uh, the article is saying, um,
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the weather has been influencing human behavior on
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Earth since years and years and years ago.
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But this one's a little bit
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interesting.
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Professor Fred Watson: It is. I think this is a lovely story.
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I always relish stories that bring
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together quite unrelated disciplines in science,
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which this one certainly does, uh, because it
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brings together, um, geophysicists, people who
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study space weather, um, uh,
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and uh, also archaeologists,
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people who study the uh, ancient history, uh,
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of our species. Uh, and
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it's um, actually a conversation article that sparked my
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interest on this, uh, which is written by three authors from,
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uh, um, the United States, two from the
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University of Michigan, uh, one from the
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Helmholtz center for
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Geosciences that might actually be not in the
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United States. But anyway, that's another story.
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Um, so we've got, uh, these, uh,
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scientists who have looked at,
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um, the evidence for the
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behavior of the Earth's magnetic field,
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uh, in geological time. Uh,
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now we know, uh, from quite
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reliable sources, namely,
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uh, basically the magnetic
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details of ancient rocks on the
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ocean bed. We know that the Earth's magnetic history
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has been very varied. And about three or four times every
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million years, the Earth's poles flip.
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And these are the magnetic poles, not the rotation
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poles. The Earth still rotates in the same axis,
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but the magnetic poles flip. And we think
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that's to do with the relationship
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between the, uh, solid core of the Earth and its
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liquid core. These two things mix together,
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uh, and they produce, uh, a magnetic field
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which, uh, occasionally basically
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declines. Uh, and then when it returns
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its pointing the other way, it's a different magnetic, uh,
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pole. And it's been known, uh, because
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of evidence like that from seabed rocks,
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uh, and things of that sort, uh, that there was a time
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about 41,000 years ago,
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uh, when the magnetism of the
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Earth basically dwindled
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away to something like 10% of its
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current, uh, intensity. Uh,
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and um, so, you know,
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we've got a magnetic field that is not offering
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the same protection, uh, from the solar wind
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as it does today. Uh, and that
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would lead to a number of things, one of
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which would be, um, the
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occurrence of aurorae,
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the northern and southern lights a long way from
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the poles. Because as the
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magnetic field dwindles, um, you can, you
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know, these subatomic particles are not funneled into the polar
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regions of the Earth as they are now, but they go
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to much lower latitudes. And so,
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uh, I think they've asked the question,
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what would that do to, uh, our
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distant forebears? Um, if they are watching the
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sky, um, they might
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well see, uh, aurorae, northern and southern
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lights, which, uh, had never been seen
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before, uh, at their latitudes.
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And so archaeologists have now looked at
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this, uh, and
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basically, uh,
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they imagine, uh, people seeing a green
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sky, a sky that's got really
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bright aurora. Now, uh, in
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archeology, um, a sort of response
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to something like that is really
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not easy to capture because there's nobody writing and
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saying, oh, we saw a green sky
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that we can still read today. It's not
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that sort of, you know, not at that sort of level.
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So you've got to look for, um,
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perhaps, uh, more
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circumstantial, uh, evidence for
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the fact that the space weather was causing a
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different sky from what they had before.
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And the paper that's been written on this,
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uh, is actually, um.
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It pinpoints something that perhaps
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otherwise would not be understood. And that
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is that, um, the use
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of ochre, uh, which is
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a sort of powdery rock, um, very, very
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well known in Australia. It's, uh, a reddish rock because,
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um, our first nations people used it and still
292
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do use ochre, uh, for body markings.
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It washes off, of course, but it's a way of decorating
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your body. Uh, and it turns out that that
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period, 41,000 years ago, coincides
296
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with an increased use of ochre,
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uh, by the people who lived at that time.
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And, um,
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the way they interpret this is that
300
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ochre actually is a kind
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of natural sunscreen. It's.
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I don't know what it's. You know, its SPF factor is,
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but if you put ochre on, you've got a
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sunscreen that will protect you a little bit
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from the increased ultraviolet
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radiation, which we would expect to find
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hitting the Earth at a time when the magnetic field was
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weak. Uh, so what they're suggesting
309
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is that, um,
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the risk of sunburnt, uh, eye
311
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damage and other health issues, uh,
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may have been mitigated by
313
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people discovering that if you rub more
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ochre on, you're actually more likely to be
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protected from these phenomena. And
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so it is interesting that at
317
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the time when we know the magnetic field was letting through much
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more radiation from the sun, we see
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people using more ochre on their Bodies
320
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perhaps for protection. A, uh, really
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interesting, you know, piece of research that
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brings together two apparently completely
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unrelated fields.
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Heidi Campo: Well, that's why, you know, a word that I throw around so
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often is interdisciplinary. And I think it's so,
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so, so important because,
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you know, nobody lives in a vacuum. Even,
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you know, even something as simple
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as mathematics touches everything.
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Well, I guess math wasn't a, ah, very good because it does touch
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everything. But any, any field is going to be related
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to every other field. And I was on a
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call, I joined a, um, bioastronautics journal club
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recently and we were talking about
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um, some research that had come out and it was
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brought up that um, extreme
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conditions has already been kind of
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defined and there's already protocols in place with submarine
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usage and people who summit high
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mountains and that there's already so much that we can
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learn from things that we already do here on Earth.
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So it's just, it is interesting and I think it is important for us
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to not live in our little bubbles and our little boxes, but we still have
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to go outside and talk to other people.
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Funny, uh, little, just anecdote, side tangent and then we'll move
346
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on is there was um, an
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ancient statue that people couldn't.
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Archeologists couldn't figure out what was going on with the
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hair. It was of a woman and they're like, well, was
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it artistic? Why does the hair look this way?
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You know, they couldn't figure it out. And then a modern
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day hairdresser was like, oh, it was, it was sewn
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in the, it was like, it was hair extensions that were
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sewn in. You're seeing a marble statue of
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somebody who had sewn hair extensions on.
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But the archaeologist couldn't figure it out. But the hairdresser
357
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looked at that immediately and was like, well, of course, that's what that
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is. So I just think that was kind of a funny little
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example.
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Professor Fred Watson: Um, that's a really interesting one
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actually. Makes you wonder, um,
362
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what, you know, what the person
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of whom the statue was made was. Uh, like
364
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whether they were somebody who was ah, vain about
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their hairstyle or um, whether it was something
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necessary because, uh, other, you know, other, um,
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reasons would make you keep your hair short. For example,
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if you were doing military things and stuff like
369
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that. Interesting stuff. Yeah, but again, you're quite right.
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Uh, interdisciplinary. It's a great word.
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Generic: 0G. And I feel fine.
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Heidi Campo: Space nuts. Well, speaking of. Well, I guess
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this last one's not really so interdisciplinary. It's
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dramatic and it is very in its own little
375
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niche field. But the title is A Cosmic
376
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Death Spiral. Astronomers
377
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catch planet in its final orbit before
378
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destruction. This is a very
379
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dramatic story. But Fred, I know that
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you always bring reason and
381
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logic and peace to all of
382
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these stories. So what's going on with this dramatic
383
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death spiral?
384
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Professor Fred Watson: Well, it's a death spiral. That's right.
385
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Um, and I like this story because it's, um,
386
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research that's been done by astronomers
387
00:18:34.360 --> 00:18:37.080
in the university that I'm associated with here in Australia,
388
00:18:37.160 --> 00:18:39.830
Macquarie University in Sydney. Uh,
389
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and so what they've done is looked at. It's actually a very
390
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well studied, uh, exoplanet, uh,
391
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with the marvelous name of Toi, uh,
392
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2108B. It's
393
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about 900 light years away.
394
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Uh, it's, uh, extreme in the
395
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sense that it is, um, an
396
00:18:59.830 --> 00:19:01.870
object that orbits its parent star,
397
00:19:02.830 --> 00:19:05.390
uh, closer than any other known
398
00:19:05.630 --> 00:19:08.350
planet. Um, its year.
399
00:19:09.090 --> 00:19:12.030
Uh, that is the time it takes to go around its star
400
00:19:12.510 --> 00:19:15.390
is 16 hours. So it
401
00:19:15.390 --> 00:19:18.230
whizzes around its parent star. It's very close to
402
00:19:18.230 --> 00:19:21.190
it. So, um, it's bathed in
403
00:19:21.190 --> 00:19:24.190
radiation, uh, from the star. It's what we call a
404
00:19:24.190 --> 00:19:26.940
hot Jupiter. It's, it's, um, actually
405
00:19:26.940 --> 00:19:29.420
bigger than Jupiter, uh, and is,
406
00:19:29.870 --> 00:19:32.620
um, essentially, um, you
407
00:19:32.620 --> 00:19:35.460
know, as I said, bathed in the radiation of its parent
408
00:19:35.460 --> 00:19:38.270
star. It's very, very hot. Um,
409
00:19:38.380 --> 00:19:39.900
so, um, that
410
00:19:41.580 --> 00:19:44.460
situation that you've got this object going around
411
00:19:44.460 --> 00:19:46.540
its parent star once every 16 hours,
412
00:19:47.270 --> 00:19:49.260
uh, is telling you
413
00:19:49.900 --> 00:19:52.900
that that orbit is untenable in the
414
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long term. Uh, the orbit is going to
415
00:19:55.490 --> 00:19:58.010
decay. Uh, and what the
416
00:19:58.010 --> 00:19:59.690
scientists have studied is
417
00:20:00.650 --> 00:20:03.410
basically the mechanics of that. How will the orbit
418
00:20:03.410 --> 00:20:04.660
decay? Uh,
419
00:20:06.170 --> 00:20:08.970
will this planet just get gobbled up by its star?
420
00:20:08.970 --> 00:20:11.770
Will it get flung away in a random
421
00:20:11.770 --> 00:20:14.490
direction? Uh, how's it going to work?
422
00:20:15.060 --> 00:20:18.050
Uh, and so, um, what they've done is they've looked
423
00:20:18.050 --> 00:20:20.890
at, uh, data that goes back to 2010,
424
00:20:21.520 --> 00:20:24.310
um, to look for changes in the orbit
425
00:20:24.310 --> 00:20:26.630
of this planet. Uh, and
426
00:20:27.030 --> 00:20:29.670
there's um, details that
427
00:20:29.830 --> 00:20:32.790
they've found that can suggest
428
00:20:32.870 --> 00:20:35.510
that there might be three different ways that it could,
429
00:20:36.040 --> 00:20:38.870
uh, reach the end of its life. Uh, either,
430
00:20:39.350 --> 00:20:42.150
number one, uh, it gets torn apart,
431
00:20:42.480 --> 00:20:44.630
uh, as it gets closer to the star. Because,
432
00:20:45.540 --> 00:20:48.260
um, what you have is this phenomenon called, um,
433
00:20:48.310 --> 00:20:50.270
tidal disruption. It's where
434
00:20:51.710 --> 00:20:54.470
part of the planet that's nearer to the star feels a much bigger
435
00:20:54.470 --> 00:20:57.350
gravitational force on the other side. And that tends
436
00:20:57.350 --> 00:21:00.110
to pull the planet to pieces. So that's one
437
00:21:00.110 --> 00:21:02.990
scenario. Uh, the other one is that it
438
00:21:02.990 --> 00:21:05.869
might just disappear into the star.
439
00:21:06.510 --> 00:21:09.510
In other words, just get sucked into the star. And we know
440
00:21:09.510 --> 00:21:12.340
that happens because we've seen evidence of it, uh,
441
00:21:13.120 --> 00:21:15.310
uh, in other solar systems. We've seen
442
00:21:15.930 --> 00:21:18.490
brightening of a star that seems to be caused by
443
00:21:19.050 --> 00:21:22.050
a planet basically impacting on
444
00:21:22.050 --> 00:21:24.970
it. And we can also find evidence in the atmospheres
445
00:21:24.970 --> 00:21:27.650
of stars, uh, for the sorts of
446
00:21:27.650 --> 00:21:30.530
chemicals that you would only find in a planet, but not in the star
447
00:21:30.530 --> 00:21:33.490
itself. So we know that happens. Uh, but
448
00:21:33.490 --> 00:21:36.250
the other one is perhaps the most interesting one. The third of their,
449
00:21:36.650 --> 00:21:39.330
um, uh, possible end games for
450
00:21:39.330 --> 00:21:42.170
Toi, uh, 2109B,
451
00:21:42.810 --> 00:21:45.690
that it's a gas giant like Jupiter and Saturn
452
00:21:45.690 --> 00:21:47.530
are. Uh, and what they're
453
00:21:48.170 --> 00:21:50.410
suggesting is that perhaps its
454
00:21:50.490 --> 00:21:52.810
gaseous envelope, its atmosphere
455
00:21:53.210 --> 00:21:55.810
might just be blown away by the
456
00:21:55.810 --> 00:21:58.409
radiation coming from the star and just
457
00:21:58.409 --> 00:22:01.210
essentially leave a planet that's still going around that parent
458
00:22:01.210 --> 00:22:04.090
star, but is now just a rocky remnant.
459
00:22:04.970 --> 00:22:07.730
Um, it's not, uh, a gas giant
460
00:22:07.730 --> 00:22:10.450
anymore. So what, um,
461
00:22:10.760 --> 00:22:13.480
people are going to look for, uh,
462
00:22:13.560 --> 00:22:16.520
is to see exactly how this
463
00:22:16.520 --> 00:22:19.440
behavior continues. The prediction
464
00:22:19.440 --> 00:22:22.360
is that, um, the orbit of this
465
00:22:22.360 --> 00:22:25.240
planet is shortening by, I think it's 10
466
00:22:25.240 --> 00:22:28.120
seconds per year, the amount of orbital
467
00:22:28.120 --> 00:22:31.080
shortening that's going on at the moment. As time goes on,
468
00:22:31.080 --> 00:22:33.960
we will see the planet pass some kind
469
00:22:33.960 --> 00:22:36.630
of, um, some kind of trigger point,
470
00:22:36.670 --> 00:22:39.550
uh, you know, a tipping point, uh, where
471
00:22:39.550 --> 00:22:42.470
one of these three scenarios might become more obvious
472
00:22:42.470 --> 00:22:45.390
as to what's going to happen to it. Once again, we'll
473
00:22:45.390 --> 00:22:47.800
keep an eye on that with the space nuts. Eagle, uh,
474
00:22:48.190 --> 00:22:50.790
eye on astrophysics and what's going on in the
475
00:22:50.790 --> 00:22:51.270
universe.
476
00:22:51.990 --> 00:22:54.870
Heidi Campo: That planet sounds like your average grad student just
477
00:22:55.030 --> 00:22:57.710
circling in chaos and they're either going to get
478
00:22:57.710 --> 00:23:00.710
flung out, never to enter that field again, or they're just going to
479
00:23:00.710 --> 00:23:03.610
get absorbed by it and become whatever
480
00:23:03.610 --> 00:23:05.010
it is that they're studying.
481
00:23:05.410 --> 00:23:07.810
Professor Fred Watson: Yep, that's right. That's what you do. You become
482
00:23:08.450 --> 00:23:09.170
what you study.
483
00:23:10.210 --> 00:23:13.010
Heidi Campo: Yeah. So I am, um, nicknaming this
484
00:23:13.010 --> 00:23:15.170
planet the grad student.
485
00:23:16.050 --> 00:23:18.690
Professor Fred Watson: I think it's a better name than toi, whatever it was.
486
00:23:21.250 --> 00:23:24.130
Toi, by the way, stands for, um, tess,
487
00:23:24.130 --> 00:23:26.890
Object of Interest. TESS was a planet finding
488
00:23:26.890 --> 00:23:29.480
satellite that was active a few years.
489
00:23:29.960 --> 00:23:32.840
Heidi Campo: And if it gets flung out into the universe, this could be our next
490
00:23:33.560 --> 00:23:34.720
alien, uh, spaceship.
491
00:23:34.720 --> 00:23:36.400
Professor Fred Watson: Yes, that's right. Who knows?
492
00:23:36.400 --> 00:23:39.400
Heidi Campo: What is this thing? It's just a planet that got
493
00:23:39.400 --> 00:23:41.080
flung out of its orbit.
494
00:23:42.360 --> 00:23:45.240
Well Fred, that uh, that uh, wraps up this episode.
495
00:23:45.240 --> 00:23:48.240
That was kind of a fun, eclectic group of articles. Thank you
496
00:23:48.240 --> 00:23:51.000
so much for finding those and disseminating all of that information
497
00:23:51.160 --> 00:23:53.480
for us. We definitely
498
00:23:53.480 --> 00:23:56.250
appreciate you and thank you. This is,
499
00:23:56.250 --> 00:23:59.160
uh, I guess that's uh, that's the end of
500
00:23:59.160 --> 00:23:59.960
our tale today.
501
00:24:00.760 --> 00:24:03.760
Professor Fred Watson: It's uh, a tale that's never ending really, because there'll be
502
00:24:03.760 --> 00:24:06.720
other things to talk about. But yes, I look forward to next
503
00:24:06.720 --> 00:24:08.200
time. Heidi, thanks very much.
504
00:24:08.520 --> 00:24:11.000
Heidi Campo: All right, catch you next time on our Q and A
505
00:24:11.000 --> 00:24:12.840
episode. That's all for now.
506
00:24:12.920 --> 00:24:15.560
Andrew Dunkley: Hi Fred. Hi Heidi. Hi Huw. In the studio.
507
00:24:15.560 --> 00:24:18.440
Andrew again with another update on our world tour.
508
00:24:19.160 --> 00:24:21.720
And we've uh, done a heck of a lot since I
509
00:24:21.880 --> 00:24:24.800
spoke to you last year. Uh, we went to
510
00:24:25.390 --> 00:24:28.280
uh, this was an amazing place, but then again it
511
00:24:28.280 --> 00:24:31.040
wasn't and I'll tell you why. But we were back in Morocco
512
00:24:31.760 --> 00:24:34.640
and we docked in Tangier and then we did
513
00:24:34.640 --> 00:24:37.400
a couple of hours drive to a place called the Blue
514
00:24:37.400 --> 00:24:40.200
City where all the buildings are blue and there's all
515
00:24:40.200 --> 00:24:43.080
sorts of reasons why they're blue that come up when you do a Google
516
00:24:43.080 --> 00:24:45.920
search. But the main reason that we were told was that
517
00:24:45.920 --> 00:24:48.720
one day somebody painted his house blue and everyone went,
518
00:24:49.020 --> 00:24:51.980
well, that's a good idea. And so everyone else did. So that's
519
00:24:51.980 --> 00:24:54.980
why it's a blue city and everything's blue. Blue doors, blue buildings,
520
00:24:54.980 --> 00:24:57.880
blue fences, blue lights, blue everything. Um,
521
00:24:58.060 --> 00:25:00.460
not those kinds of blue lights, but uh, yeah,
522
00:25:00.540 --> 00:25:02.620
interesting place. Downside
523
00:25:03.180 --> 00:25:05.820
over saturated with hawkers and
524
00:25:05.820 --> 00:25:08.060
salespeople and high pressure tactics.
525
00:25:08.670 --> 00:25:11.540
Uh, and, and it's a pretty smelly place.
526
00:25:11.540 --> 00:25:14.300
Lots of mangy cats and dog poo everywhere.
527
00:25:15.180 --> 00:25:18.020
Yeah, um, nice place to visit. Wouldn't want to live
528
00:25:18.020 --> 00:25:20.700
there. But uh, and then we got caught up in a
529
00:25:20.860 --> 00:25:23.780
Palestinian protest that they were having. So that was
530
00:25:23.780 --> 00:25:26.750
a bit um, intimidating, I must say. Uh,
531
00:25:26.750 --> 00:25:29.420
then we moved on to our next stop which
532
00:25:29.580 --> 00:25:31.870
was, um, Seville. Uh,
533
00:25:33.100 --> 00:25:35.980
Seville, uh, was really fantastic. We actually got
534
00:25:35.980 --> 00:25:37.750
to walk on a, um, ah,
535
00:25:38.780 --> 00:25:41.350
a bullring where they still have bull
536
00:25:41.350 --> 00:25:44.270
fighting today. Mixed, um, opinions about
537
00:25:44.270 --> 00:25:47.150
the ethics of that. But uh, getting to actually see
538
00:25:47.150 --> 00:25:50.150
it and stand on the ground where they do that was, was
539
00:25:50.150 --> 00:25:53.070
incredible. And uh, yeah, quite
540
00:25:53.070 --> 00:25:55.750
a beautiful city. Really, uh, really
541
00:25:55.750 --> 00:25:58.310
loved Seville. Uh, most enjoyable.
542
00:25:58.550 --> 00:26:00.790
Our next stop took us to
543
00:26:01.070 --> 00:26:03.890
um, a really amazing place, uh,
544
00:26:03.890 --> 00:26:06.560
Lisbon in Portugal, where we
545
00:26:06.640 --> 00:26:09.560
saw the monument to the explorers, uh, the great
546
00:26:09.560 --> 00:26:12.240
names like Magellan and so on,
547
00:26:12.590 --> 00:26:14.560
uh, and Henry the Explorer.
548
00:26:15.360 --> 00:26:18.320
And uh, of course, uh, they've got a
549
00:26:18.320 --> 00:26:21.000
bridge there that looks uncannily like the
550
00:26:21.000 --> 00:26:23.720
Golden Gate Bridge in San Francisco. And
551
00:26:23.720 --> 00:26:26.480
going under that on the ship as we left was quite awe
552
00:26:26.480 --> 00:26:29.330
inspiring because you look like you're going to hit it. Uh,
553
00:26:29.330 --> 00:26:32.050
not much clearance between the Top of the ship. Ship and the bottom of the
554
00:26:32.050 --> 00:26:34.890
bridge. Uh, they've got a, um, a giant
555
00:26:35.610 --> 00:26:38.370
statue, uh, of Jesus Christ there as well. Like the one
556
00:26:38.370 --> 00:26:41.250
in, uh, Brazil. So we went up and
557
00:26:41.250 --> 00:26:43.790
had a look at that and went around the city and uh,
558
00:26:43.790 --> 00:26:46.670
enjoyed Portuguese tarts, which are, uh,
559
00:26:46.850 --> 00:26:49.770
just so delectable. But we went to the original place
560
00:26:49.770 --> 00:26:52.050
where they were first made by the monks in
561
00:26:52.050 --> 00:26:55.050
1837 or something. Oh
562
00:26:55.050 --> 00:26:57.640
my gosh. And, and it's like KFC.
563
00:26:57.640 --> 00:27:00.410
There's. They don't tell you what's in them. Uh,
564
00:27:00.530 --> 00:27:03.400
uh, and uh, our next stop, I mean we've
565
00:27:03.640 --> 00:27:05.640
done a lot of stops, was uh, um,
566
00:27:06.630 --> 00:27:09.320
uh, the place, uh, where
567
00:27:09.480 --> 00:27:12.000
they um, found the
568
00:27:12.000 --> 00:27:14.680
location for uh, one of the. One of the great
569
00:27:14.680 --> 00:27:17.480
scenes in Game, um, of Thrones.
570
00:27:17.880 --> 00:27:20.680
Remember the castle Dragonstone? Well,
571
00:27:21.080 --> 00:27:23.990
we, we saw it, but there's no castle on top of the
572
00:27:23.990 --> 00:27:26.990
island. It's just a church. But that windy little passage,
573
00:27:27.530 --> 00:27:30.110
uh, up the stairs to the top, uh, is real.
574
00:27:30.830 --> 00:27:33.790
And uh, I can't remember where,
575
00:27:34.270 --> 00:27:37.270
where it was now that we've been to so many places. Um,
576
00:27:38.429 --> 00:27:40.430
Jude, can you remember where that was?
577
00:27:43.070 --> 00:27:43.790
Professor Fred Watson: Bilbao.
578
00:27:43.790 --> 00:27:46.440
Andrew Dunkley: Bilbao in Spain. That's right, yeah. Um,
579
00:27:46.830 --> 00:27:49.630
lovely place as well. Really great city. And
580
00:27:50.030 --> 00:27:52.990
they have the Guggenheim museum there as well, which we visited.
581
00:27:53.230 --> 00:27:56.070
That's right. And since then we've been to
582
00:27:56.070 --> 00:27:58.890
France and we did a day trip in a Volkswagen, uh,
583
00:27:58.890 --> 00:28:01.760
Combi to a vineyard. And uh,
584
00:28:01.870 --> 00:28:04.190
that was our last stop.
585
00:28:04.670 --> 00:28:07.230
Uh, and just now, as I speak, we've
586
00:28:07.390 --> 00:28:10.310
parked the boat, uh, in Cork
587
00:28:10.310 --> 00:28:13.230
in Ireland. So we're going to spend the day there. We're going to
588
00:28:13.230 --> 00:28:16.210
do the Titanic museum and have a look around town. We're
589
00:28:16.440 --> 00:28:19.160
here till 10 o' clock tonight, so we're going to probably do a bit of a,
590
00:28:19.570 --> 00:28:22.520
uh, visit to some Irish pubs and just sort of
591
00:28:22.520 --> 00:28:25.440
get into the, uh, atmosphere of the Irish.
592
00:28:25.440 --> 00:28:28.320
So we're looking forward to that. Should be great fun. Hope all
593
00:28:28.320 --> 00:28:31.080
is well back home. Uh, we've still got one
594
00:28:31.080 --> 00:28:33.960
third of our trip to go. Uh, looking forward
595
00:28:33.960 --> 00:28:36.600
to getting home, but, uh, having such a great time.
596
00:28:36.600 --> 00:28:39.440
We're not in a hurry. All right, catch you
597
00:28:39.440 --> 00:28:40.840
soon. Take care. Bye. Bye.
598
00:28:42.210 --> 00:28:44.850
Generic: You've been listening to the Space Nuts podcast,
599
00:28:46.450 --> 00:28:49.170
available at Apple Podcasts, Spotify,
600
00:28:49.330 --> 00:28:52.130
iHeartRadio or your favorite podcast
601
00:28:52.130 --> 00:28:54.490
player. You can also stream on Demand at
602
00:28:54.490 --> 00:28:56.880
bitesz.com This has been another quality
603
00:28:56.880 --> 00:28:59.600
podcast production from Bytes. Com.
0
00:00:00.640 --> 00:00:03.600
Heidi Campo: Welcome back to another fun and exciting episode
1
00:00:03.600 --> 00:00:06.480
of Space Nuts, the podcast
2
00:00:06.480 --> 00:00:07.920
that is out of this world.
3
00:00:08.320 --> 00:00:10.720
Generic: 15 seconds. Guidance is internal.
4
00:00:11.040 --> 00:00:13.680
10, 9. Ignition
5
00:00:13.680 --> 00:00:16.644
sequence start. Space nuts. 5, 4, 3,
6
00:00:16.716 --> 00:00:19.524
2. 1. 2, 3, 4, 5, 5, 4,
7
00:00:19.596 --> 00:00:22.560
3, 2, 1. Space nuts astronauts
8
00:00:22.560 --> 00:00:23.760
report it feels good.
9
00:00:24.240 --> 00:00:26.640
Heidi Campo: And I'm your host for this, uh, American
10
00:00:26.800 --> 00:00:29.750
summer and Australian winter. My
11
00:00:29.750 --> 00:00:32.630
name is Heidi Campo, filling in for Andrew
12
00:00:32.630 --> 00:00:35.470
Dunkley. And joining us is the wonderful
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00:00:35.710 --> 00:00:38.430
Professor Fred Watson, astronomer at
14
00:00:38.430 --> 00:00:40.030
large. How are you doing, Fred?
15
00:00:41.470 --> 00:00:43.960
Professor Fred Watson: Very well, thank you, Heidi. I've been m
16
00:00:44.109 --> 00:00:46.870
traveling since we last spoke and have explored the
17
00:00:46.870 --> 00:00:49.220
great state of Western Australia, uh,
18
00:00:49.550 --> 00:00:52.270
in great detail. If I remember rightly, Western Australia
19
00:00:52.350 --> 00:00:55.350
would encompass Texas three times. I think that's the
20
00:00:55.350 --> 00:00:58.110
figure. Uh, it's very large. And
21
00:00:58.510 --> 00:01:01.210
so we spent a lot of time,
22
00:01:01.480 --> 00:01:04.330
uh, in coaches, but saw some incredible sites, including,
23
00:01:04.820 --> 00:01:07.700
um, the Carnarvon space ah,
24
00:01:07.700 --> 00:01:10.570
facility, which was, uh, one of the places where
25
00:01:11.290 --> 00:01:13.940
radio, um, signals were picked up and uh,
26
00:01:13.940 --> 00:01:16.770
beamed out to the world during the Apollo
27
00:01:16.770 --> 00:01:19.570
era. So lovely to visit some of the
28
00:01:19.570 --> 00:01:22.090
places where history was made at a time
29
00:01:22.650 --> 00:01:24.330
when I was, you know,
30
00:01:25.500 --> 00:01:28.090
um, a young budding astronomer and very
31
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excited by the whole thing. So it's great to see all that old technology
32
00:01:30.890 --> 00:01:31.290
again.
33
00:01:32.320 --> 00:01:35.040
Heidi Campo: Yeah, there's just something special about the old technology.
34
00:01:35.360 --> 00:01:38.160
The way it looked and felt and was packaged. And the
35
00:01:38.160 --> 00:01:41.000
new, sleek, modern stuff is cool and great, but it just
36
00:01:41.000 --> 00:01:42.000
doesn't feel the same.
37
00:01:43.200 --> 00:01:46.120
Professor Fred Watson: That's right. Well, when they get fashion designers to
38
00:01:46.120 --> 00:01:48.960
design their spacesuits, you know that things have moved on quite a long
39
00:01:48.960 --> 00:01:50.440
way since the Apollo era.
40
00:01:50.440 --> 00:01:53.240
Heidi Campo: It really has changed. But one thing
41
00:01:53.240 --> 00:01:56.160
that will never change until it does
42
00:01:56.320 --> 00:01:59.200
is our fascination with extraterrestrials.
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Which leads us into our first story
44
00:02:03.070 --> 00:02:03.470
today.
45
00:02:04.270 --> 00:02:07.030
So the three. I don't know if this is the
46
00:02:07.030 --> 00:02:09.950
three I or the three lowercase l. Atlas.
47
00:02:10.720 --> 00:02:13.470
Um, Harvard's thinking
48
00:02:13.790 --> 00:02:16.670
maybe alien probe. What's going on
49
00:02:16.670 --> 00:02:18.430
here, Fred? Give us some sanity.
50
00:02:19.230 --> 00:02:21.710
Professor Fred Watson: Yeah, so 3i.
51
00:02:22.030 --> 00:02:23.950
It is 3i because it's the third
52
00:02:24.110 --> 00:02:26.570
interstellar, um, visitor,
53
00:02:27.000 --> 00:02:29.690
uh, that has been recorded. There are probably many more
54
00:02:29.770 --> 00:02:32.450
that we haven't detected. Uh, but this is an
55
00:02:32.450 --> 00:02:35.410
object which is flying through the solar system. We have talked
56
00:02:35.410 --> 00:02:38.250
about it before. Uh, we're going to talk about it again
57
00:02:38.330 --> 00:02:41.090
just because of a couple of things that have come
58
00:02:41.090 --> 00:02:44.050
up. Um, so the
59
00:02:44.050 --> 00:02:46.850
bottom line, 3i. Atlas. Atlas was the facility that
60
00:02:46.850 --> 00:02:49.280
discovered it. Uh, it's, uh,
61
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an object which is whizzing through the solar system
62
00:02:52.570 --> 00:02:55.530
at about 60 km per second in an orbit
63
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that tells you immediately that it has come from outside
64
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the solar system. It's not, uh, in any
65
00:03:01.630 --> 00:03:04.510
sense gravitationally bound to the Sun. So it's not part
66
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of the Sun's family of planets. It's from somewhere else.
67
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We don't know where it came from. And, uh, is whizzing through
68
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the solar system. If I remember rightly, it passes
69
00:03:13.510 --> 00:03:15.950
closest to the Sun. I think it is
70
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October. Uh, it's, um,
71
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certainly, um, uh, down the track. Uh, yes,
72
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it's the closest approach in October. Um,
73
00:03:24.350 --> 00:03:27.300
so, uh, it's probably a comet.
74
00:03:27.500 --> 00:03:30.260
Um, a comet is an object made
75
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of ice, uh, with dust embedded in
76
00:03:33.020 --> 00:03:35.580
it. Uh, it's, uh, it's
77
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um. You know, the thing about comets is when they get
78
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near the sun, the ice turns into a gas. And
79
00:03:41.780 --> 00:03:44.520
we see the uh, result of that, um,
80
00:03:44.660 --> 00:03:47.580
often stretched in a tail across the sky,
81
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which makes them very bright occasionally and
82
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also occasionally quite, um, you know,
83
00:03:53.160 --> 00:03:56.160
quite, um, inspiring to people who don't know
84
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what they're looking at, which is why they were often regarded as portents
85
00:03:59.040 --> 00:04:01.760
of doom, uh, down, uh, uh, in
86
00:04:01.760 --> 00:04:04.480
historical times. So this one however,
87
00:04:04.480 --> 00:04:07.400
is probably not going to do that. It may be a comet.
88
00:04:07.400 --> 00:04:10.280
It's thought to be about 20 km across, which is actually
89
00:04:10.280 --> 00:04:12.960
quite large for the nucleus of a comet.
90
00:04:13.200 --> 00:04:15.920
But the reason why I wanted to bring it up again
91
00:04:16.560 --> 00:04:19.360
is it's the headline that I almost
92
00:04:19.360 --> 00:04:21.950
could have predicted. Uh, is
93
00:04:21.950 --> 00:04:24.710
Interstellar Object 3I Atlas an alien
94
00:04:24.710 --> 00:04:27.310
probe. Harvard Physicist sparks
95
00:04:27.310 --> 00:04:30.110
debate. Uh, and that Harvard physicist
96
00:04:30.110 --> 00:04:32.390
is a very eminent, uh, uh,
97
00:04:32.390 --> 00:04:35.150
astrophysicist. Uh, I think he's still the director
98
00:04:35.150 --> 00:04:37.510
of the Harvard Smithsonian Institute for
99
00:04:37.510 --> 00:04:40.430
Astronomy. His name is Avi Loeb, and
100
00:04:40.670 --> 00:04:42.910
he is famous for always
101
00:04:43.070 --> 00:04:45.790
putting, uh, a slant
102
00:04:46.190 --> 00:04:48.840
which could be
103
00:04:48.840 --> 00:04:51.800
interpreted as uh, suggesting
104
00:04:51.960 --> 00:04:54.760
I'm, um, going a long way around this because I want to be careful with
105
00:04:54.760 --> 00:04:57.320
my words, uh, that things like this
106
00:04:57.960 --> 00:05:00.840
could have an intelligent origin. Uh, we
107
00:05:00.840 --> 00:05:03.200
had the same when the first of these
108
00:05:03.200 --> 00:05:05.840
interstellar visitors came by back in
109
00:05:05.840 --> 00:05:08.600
2017. Um, an object called
110
00:05:08.600 --> 00:05:11.550
Oumuamua, named after, uh.
111
00:05:11.590 --> 00:05:14.120
Uh, it's a Hawaiian name meaning first
112
00:05:14.120 --> 00:05:16.760
visitor from afar, which is a lovely name. An
113
00:05:16.760 --> 00:05:19.740
interesting object, only 100 meters or so across. We
114
00:05:19.740 --> 00:05:22.500
didn't discover it until it was on its way out of the solar system.
115
00:05:23.060 --> 00:05:25.980
It's probably shaped a bit like a pancake from the light
116
00:05:25.980 --> 00:05:28.830
curve, the way the light was reflected off it. Uh,
117
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but I think Avi, um, very
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quickly, uh, found what he thought was evidence
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that this thing perhaps had an
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extraterrestrial intelligence origin.
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And exactly the same thing has happened, uh,
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with the uh, three I atlas his
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reasoning though I think is really
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interesting, uh, and that is,
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uh, the curious couple of
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curious coincidences, uh, in
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regard to the orbit of 3i
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ATLAS. And remember, this is an open orbit. It's just a
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pathway through the solar system. It's not like
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an ellipse or a circle. It's going almost in a
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straight line. In fact, it's going so fast. But
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uh, what Aviloeb has noted
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is that, uh,
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this object will actually pass close
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to Mars, Venus and
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Jupiter. Uh, and
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so, uh, what Avi has done is a
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statistical test on the likelihood of
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that. And he estimates that the chance of
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this path occurring naturally by chance
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is 0.005%.
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Uh, and another little feature of this,
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as uh, I mentioned, uh, the object
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actually passes closest to the sun in October. It's actually the
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29th of October. And it turns out that
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when that is the case, it will
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be, uh, on the other side of the sun from the
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Earth. It'll be hidden from the Earth. And so
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AVI goes as far as to suggest that that is
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perhaps so that it does not get detected
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to avoid detection. Now I think that one's
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stretching it a little bit too far. But I do think it's
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interesting, uh, that the
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interstellar comet, if that's what it is,
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passes close by, uh, those three planets that
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I just mentioned. Whether it is proof that it's
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an alien visitor is another story.
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Heidi Campo: Well, I guess we'll find out.
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Professor Fred Watson: Well, we might not. Although, um,
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uh, so you know, what happens
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when something like this goes by is that all the world's
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telescopes concentrate uh, on it because it's
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something that you've only got a limited time frame to do.
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So there's a big, um,
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interest in bringing together lots of telescopes
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that can observe this object,
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uh, and uh, look at it in great detail,
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uh, with our uh, spectrographs and things of that
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sort, which analyze any gases that are coming
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from it, perhaps give us an idea of the sort of surface that
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it has. So those things will
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be, um, being looked at over the next
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month or so, couple of months. Um, but
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whether we will find enough evidence to
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demonstrate that it has an intelligent
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origin is a different story. Uh, because
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we could learn all sorts of things about it and still not
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have that answer. So, um, I think it's one that Space Nuts
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will keep an eye on over the next few months. Uh,
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and yes, if it turns out to have windows or
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spikes, ah, coming out of it or things like that,
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um, our uh, Space Nuts audience will be the first to know about
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it.
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Heidi Campo: Absolutely. You'll you. You'll always hear it
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here first.
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Generic: Okay, we checked all four systems and.
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Professor Fred Watson: Being with a go space nuts.
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Heidi Campo: Um, well, our next story is I guess
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a little bit less fringe alien
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stuff, but still odd and still
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so relevant to, you know, everything that we're looking at with
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space. But we're talking about how
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space weather,
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like, affects scientists here on Earth. So this
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is, uh, the article is saying, um,
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the weather has been influencing human behavior on
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Earth since years and years and years ago.
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But this one's a little bit
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interesting.
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Professor Fred Watson: It is. I think this is a lovely story.
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I always relish stories that bring
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together quite unrelated disciplines in science,
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which this one certainly does, uh, because it
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brings together, um, geophysicists, people who
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study space weather, um, uh,
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and uh, also archaeologists,
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people who study the uh, ancient history, uh,
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of our species. Uh, and
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it's um, actually a conversation article that sparked my
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interest on this, uh, which is written by three authors from,
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uh, um, the United States, two from the
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University of Michigan, uh, one from the
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Helmholtz center for
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Geosciences that might actually be not in the
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United States. But anyway, that's another story.
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Um, so we've got, uh, these, uh,
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scientists who have looked at,
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um, the evidence for the
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behavior of the Earth's magnetic field,
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uh, in geological time. Uh,
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now we know, uh, from quite
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reliable sources, namely,
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uh, basically the magnetic
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details of ancient rocks on the
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ocean bed. We know that the Earth's magnetic history
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has been very varied. And about three or four times every
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million years, the Earth's poles flip.
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And these are the magnetic poles, not the rotation
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poles. The Earth still rotates in the same axis,
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but the magnetic poles flip. And we think
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that's to do with the relationship
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between the, uh, solid core of the Earth and its
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liquid core. These two things mix together,
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uh, and they produce, uh, a magnetic field
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which, uh, occasionally basically
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declines. Uh, and then when it returns
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its pointing the other way, it's a different magnetic, uh,
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pole. And it's been known, uh, because
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of evidence like that from seabed rocks,
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uh, and things of that sort, uh, that there was a time
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about 41,000 years ago,
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uh, when the magnetism of the
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Earth basically dwindled
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away to something like 10% of its
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current, uh, intensity. Uh,
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and um, so, you know,
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we've got a magnetic field that is not offering
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the same protection, uh, from the solar wind
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as it does today. Uh, and that
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would lead to a number of things, one of
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which would be, um, the
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occurrence of aurorae,
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the northern and southern lights a long way from
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the poles. Because as the
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magnetic field dwindles, um, you can, you
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know, these subatomic particles are not funneled into the polar
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regions of the Earth as they are now, but they go
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to much lower latitudes. And so,
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uh, I think they've asked the question,
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what would that do to, uh, our
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distant forebears? Um, if they are watching the
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sky, um, they might
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well see, uh, aurorae, northern and southern
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lights, which, uh, had never been seen
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before, uh, at their latitudes.
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And so archaeologists have now looked at
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this, uh, and
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basically, uh,
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they imagine, uh, people seeing a green
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sky, a sky that's got really
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bright aurora. Now, uh, in
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archeology, um, a sort of response
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to something like that is really
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not easy to capture because there's nobody writing and
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saying, oh, we saw a green sky
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that we can still read today. It's not
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that sort of, you know, not at that sort of level.
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So you've got to look for, um,
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perhaps, uh, more
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circumstantial, uh, evidence for
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the fact that the space weather was causing a
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different sky from what they had before.
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And the paper that's been written on this,
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uh, is actually, um.
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It pinpoints something that perhaps
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otherwise would not be understood. And that
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is that, um, the use
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of ochre, uh, which is
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a sort of powdery rock, um, very, very
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well known in Australia. It's, uh, a reddish rock because,
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um, our first nations people used it and still
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do use ochre, uh, for body markings.
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It washes off, of course, but it's a way of decorating
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your body. Uh, and it turns out that that
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period, 41,000 years ago, coincides
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with an increased use of ochre,
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uh, by the people who lived at that time.
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And, um,
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the way they interpret this is that
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ochre actually is a kind
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of natural sunscreen. It's.
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I don't know what it's. You know, its SPF factor is,
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but if you put ochre on, you've got a
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sunscreen that will protect you a little bit
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from the increased ultraviolet
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radiation, which we would expect to find
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hitting the Earth at a time when the magnetic field was
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weak. Uh, so what they're suggesting
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is that, um,
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the risk of sunburnt, uh, eye
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damage and other health issues, uh,
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may have been mitigated by
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people discovering that if you rub more
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ochre on, you're actually more likely to be
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protected from these phenomena. And
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so it is interesting that at
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the time when we know the magnetic field was letting through much
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more radiation from the sun, we see
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people using more ochre on their Bodies
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perhaps for protection. A, uh, really
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interesting, you know, piece of research that
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brings together two apparently completely
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unrelated fields.
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Heidi Campo: Well, that's why, you know, a word that I throw around so
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often is interdisciplinary. And I think it's so,
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so, so important because,
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you know, nobody lives in a vacuum. Even,
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you know, even something as simple
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as mathematics touches everything.
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Well, I guess math wasn't a, ah, very good because it does touch
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everything. But any, any field is going to be related
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to every other field. And I was on a
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call, I joined a, um, bioastronautics journal club
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recently and we were talking about
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um, some research that had come out and it was
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brought up that um, extreme
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conditions has already been kind of
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defined and there's already protocols in place with submarine
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usage and people who summit high
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mountains and that there's already so much that we can
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learn from things that we already do here on Earth.
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So it's just, it is interesting and I think it is important for us
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to not live in our little bubbles and our little boxes, but we still have
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to go outside and talk to other people.
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Funny, uh, little, just anecdote, side tangent and then we'll move
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on is there was um, an
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ancient statue that people couldn't.
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Archeologists couldn't figure out what was going on with the
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hair. It was of a woman and they're like, well, was
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it artistic? Why does the hair look this way?
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You know, they couldn't figure it out. And then a modern
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day hairdresser was like, oh, it was, it was sewn
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in the, it was like, it was hair extensions that were
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sewn in. You're seeing a marble statue of
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somebody who had sewn hair extensions on.
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But the archaeologist couldn't figure it out. But the hairdresser
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looked at that immediately and was like, well, of course, that's what that
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is. So I just think that was kind of a funny little
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example.
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Professor Fred Watson: Um, that's a really interesting one
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actually. Makes you wonder, um,
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what, you know, what the person
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of whom the statue was made was. Uh, like
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whether they were somebody who was ah, vain about
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their hairstyle or um, whether it was something
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necessary because, uh, other, you know, other, um,
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reasons would make you keep your hair short. For example,
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if you were doing military things and stuff like
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that. Interesting stuff. Yeah, but again, you're quite right.
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Uh, interdisciplinary. It's a great word.
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Generic: 0G. And I feel fine.
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Heidi Campo: Space nuts. Well, speaking of. Well, I guess
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this last one's not really so interdisciplinary. It's
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dramatic and it is very in its own little
375
00:18:02.110 --> 00:18:04.870
niche field. But the title is A Cosmic
376
00:18:04.870 --> 00:18:07.490
Death Spiral. Astronomers
377
00:18:07.490 --> 00:18:09.970
catch planet in its final orbit before
378
00:18:09.970 --> 00:18:12.290
destruction. This is a very
379
00:18:12.290 --> 00:18:15.210
dramatic story. But Fred, I know that
380
00:18:15.210 --> 00:18:17.970
you always bring reason and
381
00:18:18.130 --> 00:18:21.130
logic and peace to all of
382
00:18:21.130 --> 00:18:23.890
these stories. So what's going on with this dramatic
383
00:18:24.130 --> 00:18:25.250
death spiral?
384
00:18:25.730 --> 00:18:27.490
Professor Fred Watson: Well, it's a death spiral. That's right.
385
00:18:28.590 --> 00:18:31.430
Um, and I like this story because it's, um,
386
00:18:31.490 --> 00:18:34.360
research that's been done by astronomers
387
00:18:34.360 --> 00:18:37.080
in the university that I'm associated with here in Australia,
388
00:18:37.160 --> 00:18:39.830
Macquarie University in Sydney. Uh,
389
00:18:39.880 --> 00:18:42.800
and so what they've done is looked at. It's actually a very
390
00:18:42.800 --> 00:18:45.710
well studied, uh, exoplanet, uh,
391
00:18:45.710 --> 00:18:48.550
with the marvelous name of Toi, uh,
392
00:18:48.600 --> 00:18:51.360
2108B. It's
393
00:18:51.360 --> 00:18:53.800
about 900 light years away.
394
00:18:54.150 --> 00:18:57.000
Uh, it's, uh, extreme in the
395
00:18:57.000 --> 00:18:59.830
sense that it is, um, an
396
00:18:59.830 --> 00:19:01.870
object that orbits its parent star,
397
00:19:02.830 --> 00:19:05.390
uh, closer than any other known
398
00:19:05.630 --> 00:19:08.350
planet. Um, its year.
399
00:19:09.090 --> 00:19:12.030
Uh, that is the time it takes to go around its star
400
00:19:12.510 --> 00:19:15.390
is 16 hours. So it
401
00:19:15.390 --> 00:19:18.230
whizzes around its parent star. It's very close to
402
00:19:18.230 --> 00:19:21.190
it. So, um, it's bathed in
403
00:19:21.190 --> 00:19:24.190
radiation, uh, from the star. It's what we call a
404
00:19:24.190 --> 00:19:26.940
hot Jupiter. It's, it's, um, actually
405
00:19:26.940 --> 00:19:29.420
bigger than Jupiter, uh, and is,
406
00:19:29.870 --> 00:19:32.620
um, essentially, um, you
407
00:19:32.620 --> 00:19:35.460
know, as I said, bathed in the radiation of its parent
408
00:19:35.460 --> 00:19:38.270
star. It's very, very hot. Um,
409
00:19:38.380 --> 00:19:39.900
so, um, that
410
00:19:41.580 --> 00:19:44.460
situation that you've got this object going around
411
00:19:44.460 --> 00:19:46.540
its parent star once every 16 hours,
412
00:19:47.270 --> 00:19:49.260
uh, is telling you
413
00:19:49.900 --> 00:19:52.900
that that orbit is untenable in the
414
00:19:52.900 --> 00:19:55.490
long term. Uh, the orbit is going to
415
00:19:55.490 --> 00:19:58.010
decay. Uh, and what the
416
00:19:58.010 --> 00:19:59.690
scientists have studied is
417
00:20:00.650 --> 00:20:03.410
basically the mechanics of that. How will the orbit
418
00:20:03.410 --> 00:20:04.660
decay? Uh,
419
00:20:06.170 --> 00:20:08.970
will this planet just get gobbled up by its star?
420
00:20:08.970 --> 00:20:11.770
Will it get flung away in a random
421
00:20:11.770 --> 00:20:14.490
direction? Uh, how's it going to work?
422
00:20:15.060 --> 00:20:18.050
Uh, and so, um, what they've done is they've looked
423
00:20:18.050 --> 00:20:20.890
at, uh, data that goes back to 2010,
424
00:20:21.520 --> 00:20:24.310
um, to look for changes in the orbit
425
00:20:24.310 --> 00:20:26.630
of this planet. Uh, and
426
00:20:27.030 --> 00:20:29.670
there's um, details that
427
00:20:29.830 --> 00:20:32.790
they've found that can suggest
428
00:20:32.870 --> 00:20:35.510
that there might be three different ways that it could,
429
00:20:36.040 --> 00:20:38.870
uh, reach the end of its life. Uh, either,
430
00:20:39.350 --> 00:20:42.150
number one, uh, it gets torn apart,
431
00:20:42.480 --> 00:20:44.630
uh, as it gets closer to the star. Because,
432
00:20:45.540 --> 00:20:48.260
um, what you have is this phenomenon called, um,
433
00:20:48.310 --> 00:20:50.270
tidal disruption. It's where
434
00:20:51.710 --> 00:20:54.470
part of the planet that's nearer to the star feels a much bigger
435
00:20:54.470 --> 00:20:57.350
gravitational force on the other side. And that tends
436
00:20:57.350 --> 00:21:00.110
to pull the planet to pieces. So that's one
437
00:21:00.110 --> 00:21:02.990
scenario. Uh, the other one is that it
438
00:21:02.990 --> 00:21:05.869
might just disappear into the star.
439
00:21:06.510 --> 00:21:09.510
In other words, just get sucked into the star. And we know
440
00:21:09.510 --> 00:21:12.340
that happens because we've seen evidence of it, uh,
441
00:21:13.120 --> 00:21:15.310
uh, in other solar systems. We've seen
442
00:21:15.930 --> 00:21:18.490
brightening of a star that seems to be caused by
443
00:21:19.050 --> 00:21:22.050
a planet basically impacting on
444
00:21:22.050 --> 00:21:24.970
it. And we can also find evidence in the atmospheres
445
00:21:24.970 --> 00:21:27.650
of stars, uh, for the sorts of
446
00:21:27.650 --> 00:21:30.530
chemicals that you would only find in a planet, but not in the star
447
00:21:30.530 --> 00:21:33.490
itself. So we know that happens. Uh, but
448
00:21:33.490 --> 00:21:36.250
the other one is perhaps the most interesting one. The third of their,
449
00:21:36.650 --> 00:21:39.330
um, uh, possible end games for
450
00:21:39.330 --> 00:21:42.170
Toi, uh, 2109B,
451
00:21:42.810 --> 00:21:45.690
that it's a gas giant like Jupiter and Saturn
452
00:21:45.690 --> 00:21:47.530
are. Uh, and what they're
453
00:21:48.170 --> 00:21:50.410
suggesting is that perhaps its
454
00:21:50.490 --> 00:21:52.810
gaseous envelope, its atmosphere
455
00:21:53.210 --> 00:21:55.810
might just be blown away by the
456
00:21:55.810 --> 00:21:58.409
radiation coming from the star and just
457
00:21:58.409 --> 00:22:01.210
essentially leave a planet that's still going around that parent
458
00:22:01.210 --> 00:22:04.090
star, but is now just a rocky remnant.
459
00:22:04.970 --> 00:22:07.730
Um, it's not, uh, a gas giant
460
00:22:07.730 --> 00:22:10.450
anymore. So what, um,
461
00:22:10.760 --> 00:22:13.480
people are going to look for, uh,
462
00:22:13.560 --> 00:22:16.520
is to see exactly how this
463
00:22:16.520 --> 00:22:19.440
behavior continues. The prediction
464
00:22:19.440 --> 00:22:22.360
is that, um, the orbit of this
465
00:22:22.360 --> 00:22:25.240
planet is shortening by, I think it's 10
466
00:22:25.240 --> 00:22:28.120
seconds per year, the amount of orbital
467
00:22:28.120 --> 00:22:31.080
shortening that's going on at the moment. As time goes on,
468
00:22:31.080 --> 00:22:33.960
we will see the planet pass some kind
469
00:22:33.960 --> 00:22:36.630
of, um, some kind of trigger point,
470
00:22:36.670 --> 00:22:39.550
uh, you know, a tipping point, uh, where
471
00:22:39.550 --> 00:22:42.470
one of these three scenarios might become more obvious
472
00:22:42.470 --> 00:22:45.390
as to what's going to happen to it. Once again, we'll
473
00:22:45.390 --> 00:22:47.800
keep an eye on that with the space nuts. Eagle, uh,
474
00:22:48.190 --> 00:22:50.790
eye on astrophysics and what's going on in the
475
00:22:50.790 --> 00:22:51.270
universe.
476
00:22:51.990 --> 00:22:54.870
Heidi Campo: That planet sounds like your average grad student just
477
00:22:55.030 --> 00:22:57.710
circling in chaos and they're either going to get
478
00:22:57.710 --> 00:23:00.710
flung out, never to enter that field again, or they're just going to
479
00:23:00.710 --> 00:23:03.610
get absorbed by it and become whatever
480
00:23:03.610 --> 00:23:05.010
it is that they're studying.
481
00:23:05.410 --> 00:23:07.810
Professor Fred Watson: Yep, that's right. That's what you do. You become
482
00:23:08.450 --> 00:23:09.170
what you study.
483
00:23:10.210 --> 00:23:13.010
Heidi Campo: Yeah. So I am, um, nicknaming this
484
00:23:13.010 --> 00:23:15.170
planet the grad student.
485
00:23:16.050 --> 00:23:18.690
Professor Fred Watson: I think it's a better name than toi, whatever it was.
486
00:23:21.250 --> 00:23:24.130
Toi, by the way, stands for, um, tess,
487
00:23:24.130 --> 00:23:26.890
Object of Interest. TESS was a planet finding
488
00:23:26.890 --> 00:23:29.480
satellite that was active a few years.
489
00:23:29.960 --> 00:23:32.840
Heidi Campo: And if it gets flung out into the universe, this could be our next
490
00:23:33.560 --> 00:23:34.720
alien, uh, spaceship.
491
00:23:34.720 --> 00:23:36.400
Professor Fred Watson: Yes, that's right. Who knows?
492
00:23:36.400 --> 00:23:39.400
Heidi Campo: What is this thing? It's just a planet that got
493
00:23:39.400 --> 00:23:41.080
flung out of its orbit.
494
00:23:42.360 --> 00:23:45.240
Well Fred, that uh, that uh, wraps up this episode.
495
00:23:45.240 --> 00:23:48.240
That was kind of a fun, eclectic group of articles. Thank you
496
00:23:48.240 --> 00:23:51.000
so much for finding those and disseminating all of that information
497
00:23:51.160 --> 00:23:53.480
for us. We definitely
498
00:23:53.480 --> 00:23:56.250
appreciate you and thank you. This is,
499
00:23:56.250 --> 00:23:59.160
uh, I guess that's uh, that's the end of
500
00:23:59.160 --> 00:23:59.960
our tale today.
501
00:24:00.760 --> 00:24:03.760
Professor Fred Watson: It's uh, a tale that's never ending really, because there'll be
502
00:24:03.760 --> 00:24:06.720
other things to talk about. But yes, I look forward to next
503
00:24:06.720 --> 00:24:08.200
time. Heidi, thanks very much.
504
00:24:08.520 --> 00:24:11.000
Heidi Campo: All right, catch you next time on our Q and A
505
00:24:11.000 --> 00:24:12.840
episode. That's all for now.
506
00:24:12.920 --> 00:24:15.560
Andrew Dunkley: Hi Fred. Hi Heidi. Hi Huw. In the studio.
507
00:24:15.560 --> 00:24:18.440
Andrew again with another update on our world tour.
508
00:24:19.160 --> 00:24:21.720
And we've uh, done a heck of a lot since I
509
00:24:21.880 --> 00:24:24.800
spoke to you last year. Uh, we went to
510
00:24:25.390 --> 00:24:28.280
uh, this was an amazing place, but then again it
511
00:24:28.280 --> 00:24:31.040
wasn't and I'll tell you why. But we were back in Morocco
512
00:24:31.760 --> 00:24:34.640
and we docked in Tangier and then we did
513
00:24:34.640 --> 00:24:37.400
a couple of hours drive to a place called the Blue
514
00:24:37.400 --> 00:24:40.200
City where all the buildings are blue and there's all
515
00:24:40.200 --> 00:24:43.080
sorts of reasons why they're blue that come up when you do a Google
516
00:24:43.080 --> 00:24:45.920
search. But the main reason that we were told was that
517
00:24:45.920 --> 00:24:48.720
one day somebody painted his house blue and everyone went,
518
00:24:49.020 --> 00:24:51.980
well, that's a good idea. And so everyone else did. So that's
519
00:24:51.980 --> 00:24:54.980
why it's a blue city and everything's blue. Blue doors, blue buildings,
520
00:24:54.980 --> 00:24:57.880
blue fences, blue lights, blue everything. Um,
521
00:24:58.060 --> 00:25:00.460
not those kinds of blue lights, but uh, yeah,
522
00:25:00.540 --> 00:25:02.620
interesting place. Downside
523
00:25:03.180 --> 00:25:05.820
over saturated with hawkers and
524
00:25:05.820 --> 00:25:08.060
salespeople and high pressure tactics.
525
00:25:08.670 --> 00:25:11.540
Uh, and, and it's a pretty smelly place.
526
00:25:11.540 --> 00:25:14.300
Lots of mangy cats and dog poo everywhere.
527
00:25:15.180 --> 00:25:18.020
Yeah, um, nice place to visit. Wouldn't want to live
528
00:25:18.020 --> 00:25:20.700
there. But uh, and then we got caught up in a
529
00:25:20.860 --> 00:25:23.780
Palestinian protest that they were having. So that was
530
00:25:23.780 --> 00:25:26.750
a bit um, intimidating, I must say. Uh,
531
00:25:26.750 --> 00:25:29.420
then we moved on to our next stop which
532
00:25:29.580 --> 00:25:31.870
was, um, Seville. Uh,
533
00:25:33.100 --> 00:25:35.980
Seville, uh, was really fantastic. We actually got
534
00:25:35.980 --> 00:25:37.750
to walk on a, um, ah,
535
00:25:38.780 --> 00:25:41.350
a bullring where they still have bull
536
00:25:41.350 --> 00:25:44.270
fighting today. Mixed, um, opinions about
537
00:25:44.270 --> 00:25:47.150
the ethics of that. But uh, getting to actually see
538
00:25:47.150 --> 00:25:50.150
it and stand on the ground where they do that was, was
539
00:25:50.150 --> 00:25:53.070
incredible. And uh, yeah, quite
540
00:25:53.070 --> 00:25:55.750
a beautiful city. Really, uh, really
541
00:25:55.750 --> 00:25:58.310
loved Seville. Uh, most enjoyable.
542
00:25:58.550 --> 00:26:00.790
Our next stop took us to
543
00:26:01.070 --> 00:26:03.890
um, a really amazing place, uh,
544
00:26:03.890 --> 00:26:06.560
Lisbon in Portugal, where we
545
00:26:06.640 --> 00:26:09.560
saw the monument to the explorers, uh, the great
546
00:26:09.560 --> 00:26:12.240
names like Magellan and so on,
547
00:26:12.590 --> 00:26:14.560
uh, and Henry the Explorer.
548
00:26:15.360 --> 00:26:18.320
And uh, of course, uh, they've got a
549
00:26:18.320 --> 00:26:21.000
bridge there that looks uncannily like the
550
00:26:21.000 --> 00:26:23.720
Golden Gate Bridge in San Francisco. And
551
00:26:23.720 --> 00:26:26.480
going under that on the ship as we left was quite awe
552
00:26:26.480 --> 00:26:29.330
inspiring because you look like you're going to hit it. Uh,
553
00:26:29.330 --> 00:26:32.050
not much clearance between the Top of the ship. Ship and the bottom of the
554
00:26:32.050 --> 00:26:34.890
bridge. Uh, they've got a, um, a giant
555
00:26:35.610 --> 00:26:38.370
statue, uh, of Jesus Christ there as well. Like the one
556
00:26:38.370 --> 00:26:41.250
in, uh, Brazil. So we went up and
557
00:26:41.250 --> 00:26:43.790
had a look at that and went around the city and uh,
558
00:26:43.790 --> 00:26:46.670
enjoyed Portuguese tarts, which are, uh,
559
00:26:46.850 --> 00:26:49.770
just so delectable. But we went to the original place
560
00:26:49.770 --> 00:26:52.050
where they were first made by the monks in
561
00:26:52.050 --> 00:26:55.050
1837 or something. Oh
562
00:26:55.050 --> 00:26:57.640
my gosh. And, and it's like KFC.
563
00:26:57.640 --> 00:27:00.410
There's. They don't tell you what's in them. Uh,
564
00:27:00.530 --> 00:27:03.400
uh, and uh, our next stop, I mean we've
565
00:27:03.640 --> 00:27:05.640
done a lot of stops, was uh, um,
566
00:27:06.630 --> 00:27:09.320
uh, the place, uh, where
567
00:27:09.480 --> 00:27:12.000
they um, found the
568
00:27:12.000 --> 00:27:14.680
location for uh, one of the. One of the great
569
00:27:14.680 --> 00:27:17.480
scenes in Game, um, of Thrones.
570
00:27:17.880 --> 00:27:20.680
Remember the castle Dragonstone? Well,
571
00:27:21.080 --> 00:27:23.990
we, we saw it, but there's no castle on top of the
572
00:27:23.990 --> 00:27:26.990
island. It's just a church. But that windy little passage,
573
00:27:27.530 --> 00:27:30.110
uh, up the stairs to the top, uh, is real.
574
00:27:30.830 --> 00:27:33.790
And uh, I can't remember where,
575
00:27:34.270 --> 00:27:37.270
where it was now that we've been to so many places. Um,
576
00:27:38.429 --> 00:27:40.430
Jude, can you remember where that was?
577
00:27:43.070 --> 00:27:43.790
Professor Fred Watson: Bilbao.
578
00:27:43.790 --> 00:27:46.440
Andrew Dunkley: Bilbao in Spain. That's right, yeah. Um,
579
00:27:46.830 --> 00:27:49.630
lovely place as well. Really great city. And
580
00:27:50.030 --> 00:27:52.990
they have the Guggenheim museum there as well, which we visited.
581
00:27:53.230 --> 00:27:56.070
That's right. And since then we've been to
582
00:27:56.070 --> 00:27:58.890
France and we did a day trip in a Volkswagen, uh,
583
00:27:58.890 --> 00:28:01.760
Combi to a vineyard. And uh,
584
00:28:01.870 --> 00:28:04.190
that was our last stop.
585
00:28:04.670 --> 00:28:07.230
Uh, and just now, as I speak, we've
586
00:28:07.390 --> 00:28:10.310
parked the boat, uh, in Cork
587
00:28:10.310 --> 00:28:13.230
in Ireland. So we're going to spend the day there. We're going to
588
00:28:13.230 --> 00:28:16.210
do the Titanic museum and have a look around town. We're
589
00:28:16.440 --> 00:28:19.160
here till 10 o' clock tonight, so we're going to probably do a bit of a,
590
00:28:19.570 --> 00:28:22.520
uh, visit to some Irish pubs and just sort of
591
00:28:22.520 --> 00:28:25.440
get into the, uh, atmosphere of the Irish.
592
00:28:25.440 --> 00:28:28.320
So we're looking forward to that. Should be great fun. Hope all
593
00:28:28.320 --> 00:28:31.080
is well back home. Uh, we've still got one
594
00:28:31.080 --> 00:28:33.960
third of our trip to go. Uh, looking forward
595
00:28:33.960 --> 00:28:36.600
to getting home, but, uh, having such a great time.
596
00:28:36.600 --> 00:28:39.440
We're not in a hurry. All right, catch you
597
00:28:39.440 --> 00:28:40.840
soon. Take care. Bye. Bye.
598
00:28:42.210 --> 00:28:44.850
Generic: You've been listening to the Space Nuts podcast,
599
00:28:46.450 --> 00:28:49.170
available at Apple Podcasts, Spotify,
600
00:28:49.330 --> 00:28:52.130
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601
00:28:52.130 --> 00:28:54.490
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602
00:28:54.490 --> 00:28:56.880
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