Nov. 27, 2025

Theia's True Origins, 40,000 Asteroids & Enceladus’ Organic Mystery

Theia's True Origins, 40,000 Asteroids & Enceladus’ Organic Mystery

Sponsor Details: This episode of Space Nuts is brought to you with the support of NordVPN. To get our special Space Nuts listener discounts and four months free bonus, all with a 30-day money-back guarantee, simply...

Sponsor Details:
This episode of Space Nuts is brought to you with the support of NordVPN. To get our special Space Nuts listener discounts and four months free bonus, all with a 30-day money-back guarantee, simply visit www.nordvpn.com/spacenuts or use the coupon code SPACENUTS at checkout.

Exploring Theia, Near-Earth Asteroids, and Enceladus
In this exciting episode of Space Nuts, hosts Andrew Dunkley and Professor Fred Watson dive into a wealth of astronomical discoveries and insights. From new revelations about the ancient collision between Earth and Theia to the astounding discovery of 40,000 near-Earth asteroids, this episode is packed with cosmic revelations that will spark your curiosity about the universe.
Episode Highlights:
Theia and Earth's Relationship: Andrew and Fred discuss groundbreaking research from the Max Planck Institute that redefines our understanding of Theia, the protoplanet that collided with Earth. They explore how isotopic similarities suggest Theia was not just a random object, but likely a companion planet in the early solar system.
40,000 Near-Earth Asteroids: The hosts celebrate the milestone of 40,000 discovered near-Earth asteroids, discussing the implications for planetary defense and the importance of monitoring potentially hazardous objects that could pose a threat to Earth.
Life on Enceladus: A thrilling discussion emerges around the latest findings from the Cassini mission, revealing new organic compounds in the icy plumes of Enceladus. Andrew and Fred ponder the exciting possibility of life existing in the subsurface ocean of this intriguing moon of Saturn.
Updates on Comet 3I Atlas: The episode wraps up with an update on the interstellar comet 3I Atlas, including stunning new images captured from Mars. The hosts discuss the significance of these observations and what they might reveal about the comet's characteristics as it continues its journey through our solar system.
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.

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WEBVTT

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Andrew Dunkley: Hi there. Thanks for joining us on Space

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Nuts, where we talk astronomy and space

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science. My name is Andrew Dunkley. Great to

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have your company. Coming up on this episode,

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uh, a new study from the Max Planck Institute

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shedding some new light on the theia, uh,

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Earth relationship, which might surprise you.

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And just when you thought it was safe to go

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back, uh, to sleep at night. 40,000

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new near earth asteroids have been

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discovered. Only 40,000? And they're all

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coming our way. No, they're not. Uh, the

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search for life just got another, um,

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a bit closer. Thanks uh, to some Cassini

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data. And 3i atlas still

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making the news. We'll talk about all of that

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on this episode of space nuts. 15

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seconds.

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Professor Fred Watson: Guidance is internal. 10, 9,

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uh, ignition sequence start.

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Space nuts.

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5, 4, 3, 2, 1, 2, 3, 4,

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5, 5, 4, 3, 2,.

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Andrew Dunkley: Space nuts.

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Professor Fred Watson: Astronauts report it feels.

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Andrew Dunkley: And we rolled out the red carpet because.

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He's back. It's Professor Fred Watson,

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astronomer at large. Hello, Fred.

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Professor Fred Watson: Hi, Andrew. I'm actually looking for the red

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carpet.

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Andrew Dunkley: Yeah, I rolled it back up again. It's had

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a few moth holes in it.

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Professor Fred Watson: Yeah, but, yeah, it's glad to hear it. Good.

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And you too. And, um, well, we've missed you.

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No, wait a minute. No, you've missed one or

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the other.

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Andrew Dunkley: Yes, we did have a few people starting to,

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um. I found in radio, if you're away for

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more than about three or four weeks, people

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started ringing the station and emailing to

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say, where's Joe Bloggs? Or where's. You

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know, this started happening with you, Fred?

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So.

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Professor Fred Watson: Oh, seriously, where's Fred?

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Andrew Dunkley: Where's Fred? What's going on with Fred? What

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happened to Fred? Uh, and funnily enough,

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I was able to say, yeah, I don't know.

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Professor Fred Watson: We haven't seen him for weeks. He's just

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disappeared.

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Andrew Dunkley: But no, he's back. He's back.

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So where did you go? What was the. Give us

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the. Give us the precede version of your

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seven weeks away.

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Professor Fred Watson: Three weeks, um, leading one of Marnie's

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tours, uh, which, uh, is the third

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big one we've done this year, actually. Um,

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after the Arctic in January and

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February. And then it was, uh, Western

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Australia in the middle of the year. And then

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this time we went to Japan. Uh, so we had a

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tour that took in interesting, uh, places

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like Osaka and Kyoto and

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Tokyo. And, um, Marnie and I actually made

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a side trip down to Hiroshima, which is a

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place I've always wanted to visit and I'm

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very glad I did. Very sobering place to

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be. Uh, But a welcoming city as well.

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Um, it was a pleasure to be there. Uh, and

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then, um, we wound up actually in Hokkaido,

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right in the north of Japan, where it was

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essentially coming onto winter. Uh, they get

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lots and lots of snow up there. It's a lot

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similar to, um, the Arctic, even though it's

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at a much lower latitude. Um, yeah, that was

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all fun. So we came back, we had four nights

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in Sydney, at home in our own bed, do the

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washing, and then off again to a conference.

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Conference on dark skies in County Mayo in

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Ireland. Uh, we were in Ireland for about a

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week, a little bit more than a week. We did

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some touring down in the South. We blew

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a kiss to the Blarney Stone.

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Andrew Dunkley: I did.

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Professor Fred Watson: Uh. Yeah, I wasn't game to

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kiss the Blarney Stone because you have to be

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upside down.

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Andrew Dunkley: Yeah.

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Professor Fred Watson: Doesn't suit me at all.

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Andrew Dunkley: We didn't do that either.

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Professor Fred Watson: No. So we blew it a kiss, which is, uh,

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enough, apparently, to get the gift of the

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gab. And then, uh, in fact, Blarney was a

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delightful place. It was the one sunny

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afternoon we had in, um. And it was

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lovely. Such an amazing castle. And the

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grounds are picture perfect. Uh, then we went

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over to Scotland, spent some time with my two

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daughters, had a great time with them. Took a

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weekend out. Uh, we all beetled off to St.

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Andrews, where I was educated. A, uh, town

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that's very close to my heart. We had a great

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time there. Uh, didn't do any golf. I'm

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sorry. But we did walk past the old course

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and thought of you with your golf clubs and

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that they don't float and things like that.

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And then after that, we, um, took the

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train down to Birmingham from Edinburgh, and

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that was pleasant. And at Birmingham, we got

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on a plane and went to Cyprus, uh, in the

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eastern end of the Mediterranean. And we

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actually had a holiday, six nights.

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Andrew Dunkley: And you found an observatory, a brand new one

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called Troodos.

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Professor Fred Watson: Troodos Observatory. Yes, we did. Marnie had

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checked it out, as she does with these

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things. And so we made a pilgrimage up into

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the hills. Not very far from the highest

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point in the island, actually, Mount Olympus.

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Uh, but, uh, it's got its own little

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mountain, has, uh. Uh, the Troodos

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Observatory. Uh, we went up there. We went

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completely unannounced. They just had a tour

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group through. So there were two coaches

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which were just about to set off down this

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road that was slightly narrower than a coach.

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Ah, and an angle of 45 degrees. Uh, if

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we'd been, um, you know, if we'd Been half an

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hour later, we'd have probably not been able

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to get there because these damn, um, coaches

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going by. But when we arrived, um,

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you know, they just got rid of all the coach

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party, and we turned up and said, we're

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astronomers. Can, uh, we have a look? And

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they said, oh, no, no, you'll have to wait

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till the next tour. Uh, but we managed to get

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hold of the events manager who said, yeah,

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come in, let's talk about what we do. And all

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the rest of it. Had a great time. So that was

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very, very nice. Uh, and if she's a Space

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Nuts listener, um,

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nice to have met you, I think it was. Irena

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was her name. Greek version of that. And then

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came home, uh, and we came home last week and

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we're now jet lagged.

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Andrew Dunkley: Yeah, it's hard to get over jet lag. I think

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it's. It's an age thing, Fred. We take you.

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Professor Fred Watson: Could be. Except, um, my other half is a lot

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younger than I am and she's jet lagged too.

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Andrew Dunkley: Just goes a bit territory. Yeah.

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Well, I've got a golf story for you while

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you're away. I won it. I won a championship.

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Professor Fred Watson: You did? Yes. Well done. So it

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was, um, 17 years between.

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Andrew Dunkley: M. Ah, uh, well, no, I came, uh,

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in the state championship, So I came third

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on handicaps and top, uh,

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10. I finished ninth, I think, in the state

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championship. But then we had our own, um,

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championship at Dubbo Golf Club the other

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day, and I managed to win one of those. So,

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uh, that's very good. And then today, just

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before this, I played in the Pro Am because

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we're hosting the New South Wales Women's

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Open qualifying event. So. Played with

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a young lass from Melbourne. Her name is

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Piper. Um, Piper.

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Oh, I've gone blank. Um,

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anyway, come back to me, lovely, uh, young

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lady hits a really mean ball and wishing

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her well, hope she makes it to the New South

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Wales Open. And, um, I'll be watching her

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career closely, so. Very good.

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Professor Fred Watson: She beat you.

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Andrew Dunkley: Oh, uh, gosh, yes. Oh, uh, yes, well, it was

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a teams event today, so we were technically

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playing together, but she out drove Smoke

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Miles. Yes, Chicken Head is interesting. It

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is a long way, but, uh, just a pleasure. Just

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a delight. We had a good day. We

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should get down to it, Fred.

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Professor Fred Watson: Yeah, we should. Yes. We're not here to talk

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about golf, are we? Although, no, it doesn't

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seem that way.

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Andrew Dunkley: Not for a change.

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Um, our first story takes us back four

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and a half billion years when our neighboring

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world, known as Thea, smashed into

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Us and all hell broke loose, literally and

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figuratively. But, uh, a new study has

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just, uh, been released from the Max Planck

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Institute Institute that's uh, shed a bit of

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new light on the thea Earth relationship. Uh,

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it doesn't sound like this was what

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we originally thought. Just some m. Random

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thing coming in and hitting us.

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There's more to the story now.

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Professor Fred Watson: There is, yes. Um, sorry Andrew, you broke up

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there, but I think I know what you said. Uh,

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um, the story of Theia, of course, this has

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been the principal theory, uh, for the

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origin of the Moon for at least the last 60

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years. Uh, when the Apollo astronauts brought

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back, what was it, 380 kg of lunar

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rock and soil, which is still being analyzed.

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Um, so, uh, Theia is the

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hypothesized planet, uh,

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perhaps protoplanet is a better word because

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this was at a time when the solar system was

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still in its infancy 4 1/2 billion years ago.

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And this object, uh, basically clouted the

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Earth. Uh, and uh, we think that what

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happened in the aftermath of that collision

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was a cloud of debris raised from the surface

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of the Earth, went into orbit around the

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Earth and eventually coalesced to form the

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Moon. And so we've um,

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had puzzles which you and I have spoken about

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a number of times as to why it is.

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Well, let me step back a bit. The first

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theory was that because this is

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a smaller object hitting a bigger object, so

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theories thought to have been half the size

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of the Earth to get the dynamics right, um,

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the Earth's the bigger planet. Uh, what you

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would expect is that the debris cloud

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raised from the Earth when the collision

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happened would be mostly made of Theia

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material. Um, and

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that's been a puzzle for a long time because

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most of the lunar rocks and soil

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have the same isotopic signature

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which we've talked about before as well, the

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same isotopic signature as the Earth. They're

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identical, uh, to the Earth's rocks. And so

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that was seen as a puzzle about probably five

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years ago or so. We did cover it on space

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notes. Some Japanese researchers, um,

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figured out that if the Earth were still

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effectively molten at that time, if it was

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still a magma world when the collision

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happened, then you'd get, um, a moon that

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was formed largely of Earth

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compounds. So, um, what has

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now happened is that, um, a close

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examination has been made and as you write

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it, the Max Planck Institute for Solar System

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Research, along with the University of

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Chicago, um, they've really honed

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in on um,

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the exact, uh, details of

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the isotopes in rocks from the, uh, Earth,

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the Moon and meteorites, because they're part

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of the story too. And it's not just

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the sort of isotopes that have been looked at

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before. These are, uh, iron, chromium,

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molybdenum, molybdenum, ah,

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zirconium, all these,

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um, chemical elements. Their isotope

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data have been analyzed to

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look again at, uh, what we find, because,

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yes, we still find that the Earth and the

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Moon have very similar isotopic mixes.

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Uh, but then you can identify

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some slight differences that are

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attributed to be isotopes that have come

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from Theia itself. So they can tease out

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what was Theia and what was Earth. And it

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turns out that when you do that, you still

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get a similar picture, that the

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isotope ratios, uh, on

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Theia were probably very similar to what

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they are on Earth. Um, and

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that is

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symptomatic, if I can put it that way, of

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the Earth and Theia being born

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close together. And the reason why we think

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that is that when you look at the solar

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system, you find that these isotope ratios

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change depending on how far out you are from

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the Sun. So if you've got two planets

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with very similar isotope ratios, then

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what you can deduce from that is

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that they were orbiting the sun close

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together. And that makes complete sense

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because eventually they run into one another.

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Um, but what the outcome of this research

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is is that, uh, Theia was not just

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a random object that ran into the Earth in

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the early solar system. It was actually, if

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not a companion of Earth, but something in a

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very similar orbit. So, you know, maybe we

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had Mercury, Venus, Theia, uh, Earth, Mars as

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the rocky planets. Um, although that order,

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you know, I've made that up, but that's the

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kind of thing it's bringing, bringing

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Theia into the picture as something that

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would have been maybe, had it not collided

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with the Earth, it would have, uh, the ninth

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planet, uh, in the inner part of the solar

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system. So, uh, a very nice piece of work,

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some very, very careful studies there that I

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think has raised a lot of, um, interest in

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the planetary, uh, science

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community.

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Andrew Dunkley: Yeah, I suppose that sort of, uh,

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confirms that it was part of the solar system

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and not just some random thing passing

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through, knocking us over in the process.

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Professor Fred Watson: That's right, yeah. And, um, I should just

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explain how the Theia remnants have

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been. The Theia isotopes have been

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determined, and it's by looking at things

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that we find in the crust of the, uh, Earth,

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because we know that the heavy elements would

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have already sunk to the. To the center of

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the Earth when that collision happened. So

316
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when we think fine things like these

317
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molybdenum, iron, zirconium, things

318
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of that sort, um, we can infer

319
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that some of that actually came from Thee

320
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itself. And that's how the similarity

321
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has been deduced, along with looking at

322
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meteorite samples too. So you're right. Um,

323
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it is not something that's come from

324
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another solar system like our current visitor

325
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3i atlas. Uh, it's

326
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definitely a homegrown planet that, uh, we

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collided with.

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Andrew Dunkley: Okay. And now it's sort of a. Well, it's not

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a part of us. There's bits and pieces of it,

330
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but most, um, of it, it's sort of vanquished

331
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into the never never, didn't it?

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Professor Fred Watson: Yeah, a lot of it would have done. But, um,

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some of it's in the moon, some of it's on the

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Earth as well.

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Andrew Dunkley: Yeah.

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Professor Fred Watson: All right.

337
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Andrew Dunkley: So, yes, some new information from the

338
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Max Planck Institute about, uh, theia

339
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being a part of the inner solar system. If

340
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you'd like to read about that, uh, there's a

341
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really great

342
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article@scienceblog.com

343
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this is space Nuts with Andrew Dunkley and

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Professor Fred.

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Space Nuts.

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Uh, now to some really good news, Fred.

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40,000 near Earth asteroids have been

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discovered. Is that all? Is that all I could

349
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find?

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Professor Fred Watson: Well, yeah, I mean, for a long time

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we've known 39,999.

352
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Um, maybe not for very long because we're

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discovering asteroids at a very prolific rate

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at the moment. And that comes about because

355
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we've got such good technology discovering

356
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them. Um, and so, yes, this is a

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milestone that's been celebrated by esa, the

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European Space Agency.

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Andrew Dunkley: Uh.

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Professor Fred Watson: So they've put out a press release saying

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40,000 near Earth asteroids discovered. Uh,

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what do we mean by a near Earth asteroid?

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It's one that approaches within about

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45 million kilometers of

365
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the Earth. Uh, and that's nearly a third

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of the distance to the sun. So when you

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say near, it's a fairly

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relative term. It's one, uh, with objects

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that can get within that distance of Earth.

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Then there's another subset of those, though,

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that we tend to call PHAs,

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potentially hazardous asteroids.

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Uh, and, um, there are something like. I

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think if I remember rightly, it's about two

375
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and a half thousand of those. And they're the

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ones whose orbits cross the orbit of the

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Earth. Um, and so they are potentially

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hazardous. And they're the ones that we keep

379
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an eye on all the time, uh,

380
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monitoring where they are, uh, and

381
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checking forward, uh, in computers.

382
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Once we know their orbits, checking forward

383
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as to whether there's any likelihood of

384
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collision. The good news is is that there's

385
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not. Uh, over the next hundred years or so

386
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we've got a fairly clean sweep of things.

387
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At least things bigger than about 140

388
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meters across and they can be very dangerous.

389
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They could be city destroyers or even state

390
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destroyers. So um, keeping an eye on

391
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those is important. Uh, and I think the

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reason why ESA has highlighted this is

393
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because it does highlight the whole regime

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of planetary defense. Uh, that's a very

395
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active area in astronomy and um,

396
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m actually almost civil defense as well. It's

397
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not just astronomy that is concerned with

398
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that. I think I probably mentioned before

399
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when I was at the IAU a couple of years ago,

400
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I actually got myself into a meeting uh,

401
00:16:16.330 --> 00:16:18.870
which was the Planetary Defense Agency,

402
00:16:19.830 --> 00:16:22.590
uh talking about uh, their next activities

403
00:16:22.590 --> 00:16:25.160
which included uh, um,

404
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a mock threatened uh, planetary asteroid

405
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impact and how all the services would deal

406
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with that. And from the astronomers

407
00:16:33.510 --> 00:16:36.160
right to the, the people who get the fire

408
00:16:36.160 --> 00:16:38.200
engines out to put out the fires and things

409
00:16:38.200 --> 00:16:40.240
of that sort. It's a very interesting thing

410
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to watch. So uh, what it did was

411
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reassured me that we're in quite good hands.

412
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Uh but yeah, the bottom line, 40 uh, thousand

413
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near Earth asteroids known. Uh, the

414
00:16:51.360 --> 00:16:53.450
good news is always that the big ones which

415
00:16:53.450 --> 00:16:55.240
uh, are the most dangerous ones, they're the

416
00:16:55.240 --> 00:16:58.200
easiest to find. And we think we know pretty

417
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well all of the asteroids bigger

418
00:17:01.120 --> 00:17:03.280
than a uh, kilometer which would be

419
00:17:03.750 --> 00:17:06.700
um, dinosaur killers, they would wipe out,

420
00:17:06.700 --> 00:17:09.020
you know, there'd be mass extinction objects.

421
00:17:09.350 --> 00:17:12.300
Uh, we think one of those hits the earth

422
00:17:12.460 --> 00:17:15.350
roughly every 200 million years. It's uh,

423
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66 million years ago since the last one did,

424
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which was, was the one that wiped out we, the

425
00:17:20.740 --> 00:17:23.460
dinosaurs. Um, since then though we've

426
00:17:23.460 --> 00:17:25.860
learned a lot about, not only about asteroids

427
00:17:25.860 --> 00:17:28.860
but about how we might deflect uh an

428
00:17:28.860 --> 00:17:31.660
asteroid if uh, if there was

429
00:17:31.660 --> 00:17:33.340
one that could be shown to be on a collision

430
00:17:33.340 --> 00:17:35.940
course with Earth. And you and I have talked

431
00:17:35.940 --> 00:17:38.660
at length and with great enthusiasm about the

432
00:17:38.660 --> 00:17:41.420
dart mission back in 2022 and the double

433
00:17:41.420 --> 00:17:44.370
asteroid redirection test, a uh,

434
00:17:44.460 --> 00:17:47.180
really well put together experiment by NASA

435
00:17:47.420 --> 00:17:50.420
which succeeded uh, in changing the

436
00:17:50.420 --> 00:17:52.860
orbit of a little world called Dimorphos.

437
00:17:53.220 --> 00:17:56.060
Uh, and that's great news because we know

438
00:17:56.060 --> 00:17:58.500
that it's now possible to do that. And just

439
00:17:58.500 --> 00:18:01.370
as a postscript to this story, um, ESA

440
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currently has a spacecraft called Hera H E R

441
00:18:04.520 --> 00:18:07.280
A on um, its way to Dimorphos

442
00:18:07.520 --> 00:18:10.240
to check out what the result of that impact

443
00:18:10.320 --> 00:18:12.240
was. It's going to study that little world,

444
00:18:12.640 --> 00:18:15.640
look at the debris that was raised by the

445
00:18:15.640 --> 00:18:18.480
impact, get uh, a much better idea of whether

446
00:18:19.120 --> 00:18:21.160
it really is just a rubble pile, which we

447
00:18:21.160 --> 00:18:24.080
think it probably is, and just uh, learn more

448
00:18:24.080 --> 00:18:26.940
about what an impact by uh,

449
00:18:27.120 --> 00:18:29.800
a spacecraft does to an asteroid. Because

450
00:18:29.800 --> 00:18:31.880
that's the key thing. If we're going to have

451
00:18:31.880 --> 00:18:34.060
to save ourselves one day by, by doing this.

452
00:18:34.220 --> 00:18:36.300
We want to know as much about it as possible.

453
00:18:36.540 --> 00:18:38.940
And if I remember rightly, Hera will reach

454
00:18:39.020 --> 00:18:41.300
Dimorphous. I think it's late next year. I

455
00:18:41.300 --> 00:18:42.700
think it's towards the end of next year.

456
00:18:43.340 --> 00:18:46.220
Andrew Dunkley: Very exciting. Yeah, nice to get a follow up

457
00:18:46.220 --> 00:18:49.020
on that story too. Yeah. Um, and of course

458
00:18:49.020 --> 00:18:51.860
this is not the end of finding these kinds of

459
00:18:51.860 --> 00:18:54.420
things because, uh, the Vera C. Rubin

460
00:18:54.420 --> 00:18:55.500
Observatory in Chile,

461
00:18:57.100 --> 00:18:59.340
it's not its primary role, but it will be

462
00:19:00.000 --> 00:19:02.840
looking for other, um, Near Earth

463
00:19:02.840 --> 00:19:05.520
objects. And they expect it to find

464
00:19:05.520 --> 00:19:06.880
tens of thousands of them.

465
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Professor Fred Watson: Absolutely, that's right. By this time next

466
00:19:09.280 --> 00:19:11.600
year we might be Talking about, uh, 80,000 or

467
00:19:11.600 --> 00:19:14.200
100,000 near Earth asteroids

468
00:19:14.200 --> 00:19:16.560
discovered. And of course again that's a good

469
00:19:16.560 --> 00:19:18.400
news story because as soon as you discover

470
00:19:18.400 --> 00:19:20.360
one of these things, first thing you do is

471
00:19:20.360 --> 00:19:23.240
put its orbital elements into the computer

472
00:19:23.240 --> 00:19:26.000
grind away, look at its trajectory in the

473
00:19:26.000 --> 00:19:28.720
future. And that is all done automatically.

474
00:19:28.720 --> 00:19:31.610
And if there is a need, uh, the system will

475
00:19:31.610 --> 00:19:33.690
raise alerts that there could be a collision,

476
00:19:34.130 --> 00:19:36.810
uh, in a certain window in the future. So

477
00:19:37.070 --> 00:19:39.890
um, that whole process is really part of

478
00:19:39.890 --> 00:19:41.650
planetary defense. It's what's safeguarding

479
00:19:41.650 --> 00:19:43.050
us from the asteroid hazard.

480
00:19:43.370 --> 00:19:46.250
Andrew Dunkley: Yeah, yeah. Um, I read a

481
00:19:46.250 --> 00:19:48.570
story the other day, I think Vera C. Rubin,

482
00:19:48.630 --> 00:19:51.370
um, had had it took its first

483
00:19:51.370 --> 00:19:53.610
picture, first light. I think they refer to

484
00:19:53.610 --> 00:19:55.690
it as in, was it June or July this year?

485
00:19:56.010 --> 00:19:57.330
Professor Fred Watson: Yeah, I think it's about then.

486
00:19:57.330 --> 00:20:00.190
Andrew Dunkley: Yeah, yeah. Uh, so we're almost at

487
00:20:00.190 --> 00:20:02.950
the pointy end of that, um, observatory

488
00:20:02.950 --> 00:20:03.910
kicking into action.

489
00:20:04.310 --> 00:20:06.110
Professor Fred Watson: That's right. If I remember rightly, I might

490
00:20:06.110 --> 00:20:07.630
have these figures slightly wrong, but it was

491
00:20:07.630 --> 00:20:10.110
something like. Was it a 10 hour set of

492
00:20:10.110 --> 00:20:11.790
observations they took and they discovered

493
00:20:11.790 --> 00:20:13.989
more than a thousand asteroids in that

494
00:20:13.990 --> 00:20:16.070
period. So imagine what it's going to be

495
00:20:16.070 --> 00:20:18.870
like. This thing looks at the entire southern

496
00:20:18.870 --> 00:20:21.310
sky every three nights. That's incredibly

497
00:20:21.310 --> 00:20:23.270
remarkable. Yeah, it's quite, yeah.

498
00:20:23.310 --> 00:20:26.290
Andrew Dunkley: Um, like we, we were so blessed to be able to

499
00:20:26.290 --> 00:20:28.920
get so much information out of, um.

500
00:20:30.850 --> 00:20:33.770
My brain's not working today. Um, the

501
00:20:33.770 --> 00:20:35.890
other observatory, the one that's out on in

502
00:20:35.890 --> 00:20:37.210
the L2.

503
00:20:37.210 --> 00:20:39.210
Professor Fred Watson: Oh yeah, you mean the James Webb Telescope.

504
00:20:39.210 --> 00:20:40.930
Andrew Dunkley: James Webb. Gosh, why Couldn't I think of

505
00:20:40.930 --> 00:20:43.810
that? But, um, working side by

506
00:20:43.810 --> 00:20:45.930
side with VC Rubin, this is just going to

507
00:20:45.930 --> 00:20:47.250
open up a whole new.

508
00:20:47.970 --> 00:20:50.930
Professor Fred Watson: Yep, that's right. At least a new registry of

509
00:20:50.930 --> 00:20:52.670
new discoveries. Yeah, yeah. Very, very

510
00:20:52.670 --> 00:20:53.110
exciting.

511
00:20:54.230 --> 00:20:56.550
Andrew Dunkley: If you would like to read about those 40,000

512
00:20:56.630 --> 00:20:59.350
Near Earth Objects, if you

513
00:20:59.350 --> 00:21:01.310
really, you know, you can go to a horror

514
00:21:01.310 --> 00:21:03.660
movie instead, probably much more fun. But,

515
00:21:03.660 --> 00:21:06.110
um, 40,000 near earth objects, you can do

516
00:21:06.110 --> 00:21:08.550
that through the European Space Agency

517
00:21:08.550 --> 00:21:08.870
website.

518
00:21:11.590 --> 00:21:13.990
Professor Fred Watson: Okay. We checked all four systems and being

519
00:21:13.990 --> 00:21:15.430
with a girl space nats.

520
00:21:15.910 --> 00:21:17.990
Andrew Dunkley: Now this, this is a story that really excites

521
00:21:17.990 --> 00:21:20.400
me because, because, um, we've talked about

522
00:21:20.400 --> 00:21:23.150
this so many times, but, um,

523
00:21:23.320 --> 00:21:26.200
this story I saw pop up last weekend

524
00:21:26.440 --> 00:21:29.240
and we have been talking so much

525
00:21:29.240 --> 00:21:30.840
about the potential for life

526
00:21:31.640 --> 00:21:34.479
elsewhere. Haven't found it yet, but the

527
00:21:34.479 --> 00:21:37.040
signs are starting to build, particularly

528
00:21:37.040 --> 00:21:39.720
within our own solar system. And

529
00:21:40.040 --> 00:21:41.480
this particular story

530
00:21:42.920 --> 00:21:45.920
is one again where we have taken a bit of

531
00:21:45.920 --> 00:21:48.330
old data and reanalyzed it.

532
00:21:49.040 --> 00:21:51.040
And this involves the Cassini

533
00:21:51.520 --> 00:21:53.920
mission, uh, which has been taking

534
00:21:54.160 --> 00:21:56.960
samples of the eruptions

535
00:21:57.360 --> 00:22:00.120
from Enceladus. And what they've

536
00:22:00.120 --> 00:22:02.540
discovered is very, very, uh,

537
00:22:02.640 --> 00:22:03.200
exciting.

538
00:22:04.399 --> 00:22:06.960
Professor Fred Watson: It is, uh, that's right. And uh, yes,

539
00:22:06.960 --> 00:22:09.840
Cassini, you know, uh, was active, if I

540
00:22:09.840 --> 00:22:12.640
remember rightly, between 2000

541
00:22:13.040 --> 00:22:15.960
and I think. Was it 2004? Yes,

542
00:22:15.960 --> 00:22:18.960
and 2017. So that was the period when

543
00:22:19.200 --> 00:22:22.180
Cassini collecting its data. And as you've

544
00:22:22.180 --> 00:22:24.860
just said, we're still learning things from

545
00:22:24.860 --> 00:22:27.260
those data. Uh, and in particular

546
00:22:27.900 --> 00:22:30.780
what has been identified is some

547
00:22:30.780 --> 00:22:33.260
previously unknown organic

548
00:22:33.340 --> 00:22:35.940
chemicals in the ice grains that

549
00:22:35.940 --> 00:22:38.540
Cassini flew through, which are

550
00:22:38.540 --> 00:22:40.860
erupting, as you said, from the ice

551
00:22:40.940 --> 00:22:43.670
geysers near the southern, uh,

552
00:22:43.670 --> 00:22:46.300
pole, the south pole of enceladus, that

553
00:22:46.300 --> 00:22:49.180
little 500 kilometer diameter world which

554
00:22:49.180 --> 00:22:51.800
is, uh, one of Saturn's moons with the

555
00:22:51.800 --> 00:22:53.840
structure that we think is fairly common out

556
00:22:53.840 --> 00:22:56.720
in that part of the solar system. Ah, a rocky

557
00:22:56.720 --> 00:22:59.200
body overlaying with a liquid ocean

558
00:22:59.360 --> 00:23:01.760
with ice on top of that. And the pressure of

559
00:23:01.760 --> 00:23:03.920
the ice is what's keeping that ocean liquid,

560
00:23:03.920 --> 00:23:06.840
along with the squeezing and squashing of the

561
00:23:06.840 --> 00:23:09.600
rocky part of the body by the,

562
00:23:09.890 --> 00:23:12.280
uh, tidal forces exerted by the giant planet

563
00:23:12.280 --> 00:23:14.960
Saturn, uh, next door. And Saturn, by the

564
00:23:14.960 --> 00:23:17.320
way, um, we've just gone through its ring

565
00:23:17.320 --> 00:23:19.230
plane. So Saturn. If you looked at Saturn

566
00:23:19.230 --> 00:23:21.510
through a telescope tonight or anytime within

567
00:23:21.510 --> 00:23:23.070
the next couple of weeks, you won't see any

568
00:23:23.070 --> 00:23:25.230
sign of the rings because we're the edge onto

569
00:23:25.230 --> 00:23:25.470
us.

570
00:23:25.470 --> 00:23:26.430
Andrew Dunkley: Oh, okay.

571
00:23:26.430 --> 00:23:29.190
Professor Fred Watson: Yep. Just a little aside there. Um, so,

572
00:23:29.730 --> 00:23:31.830
uh, what has happened is

573
00:23:32.390 --> 00:23:35.350
that, uh, we've known about

574
00:23:35.430 --> 00:23:38.390
these organic chemicals in

575
00:23:38.390 --> 00:23:41.390
Ice grains, which we know come

576
00:23:41.390 --> 00:23:43.910
from Enceladus because they actually

577
00:23:43.990 --> 00:23:46.810
feed into the outer ring of Saturn,

578
00:23:46.810 --> 00:23:48.410
something called the E ring, which is a very

579
00:23:48.410 --> 00:23:51.130
diffuse ring. And we know that the

580
00:23:51.210 --> 00:23:53.250
material in that ring, the ice crystals in

581
00:23:53.250 --> 00:23:56.010
that E ring, actually come from the south

582
00:23:56.010 --> 00:23:59.010
pole of Enceladus. And those

583
00:23:59.010 --> 00:24:02.010
have been well analyzed, um, by Cassini

584
00:24:02.010 --> 00:24:05.010
and also by other observations. And

585
00:24:05.010 --> 00:24:07.410
so it was known that there were organics in

586
00:24:07.410 --> 00:24:09.770
there. But the question was

587
00:24:10.170 --> 00:24:12.720
these ice crystals may have been in

588
00:24:12.720 --> 00:24:14.520
orbit, they may have been in space for

589
00:24:14.520 --> 00:24:16.760
centuries. And so their

590
00:24:17.480 --> 00:24:19.960
chemical structure might well have been

591
00:24:20.440 --> 00:24:23.280
modified first of all by the sun's

592
00:24:23.280 --> 00:24:25.960
ultraviolet radiation, which tends to change

593
00:24:25.960 --> 00:24:28.800
chemistry. Uh, and the solar

594
00:24:28.800 --> 00:24:30.880
wind, the wind of subatomic particles that

595
00:24:30.880 --> 00:24:33.680
comes from the sun, that too can change the

596
00:24:33.680 --> 00:24:35.620
chemistry of particles, uh,

597
00:24:36.440 --> 00:24:39.000
grains of, um, ice

598
00:24:39.720 --> 00:24:42.480
with their organics on them, the organic

599
00:24:42.480 --> 00:24:44.460
chemicals, uh, it can, can change their

600
00:24:44.460 --> 00:24:46.820
chemistry. And so there was always a question

601
00:24:47.300 --> 00:24:50.060
whether these quite complex organic

602
00:24:50.060 --> 00:24:52.940
chemicals that were identified, uh, in

603
00:24:52.940 --> 00:24:55.940
the E ring, uh, whether they are

604
00:24:55.940 --> 00:24:58.740
telling you that that's how the

605
00:24:58.740 --> 00:25:00.820
ice crystals were when they came, when they

606
00:25:00.820 --> 00:25:03.300
were spat out from M. Cassini's south

607
00:25:03.300 --> 00:25:06.100
pole, um, it puts doubt on it.

608
00:25:06.180 --> 00:25:08.980
And so what this new analysis

609
00:25:08.980 --> 00:25:11.770
does is looks back to one of the

610
00:25:11.770 --> 00:25:14.650
fly throughs of, uh, Cassini

611
00:25:14.650 --> 00:25:16.810
through the ice plumes back in

612
00:25:16.810 --> 00:25:19.570
2008. Uh, Cassini

613
00:25:19.570 --> 00:25:21.930
flew through the plume at about, um, 18

614
00:25:21.930 --> 00:25:24.690
kilometers per second at Ah, a height of

615
00:25:24.690 --> 00:25:27.410
about 20 kilometers above the surface of

616
00:25:27.410 --> 00:25:29.770
Cassini. And so the

617
00:25:30.170 --> 00:25:32.410
ice crystals that it passed through,

618
00:25:33.280 --> 00:25:36.010
um, only a few minutes earlier were actually

619
00:25:36.010 --> 00:25:38.330
water in the ocean of

620
00:25:38.490 --> 00:25:41.130
Enceladus. So these are fresh

621
00:25:41.450 --> 00:25:44.250
crystals of ice straight from the ocean. In

622
00:25:44.250 --> 00:25:45.250
other words, they're, you know, they're

623
00:25:45.250 --> 00:25:48.050
effectively samples of the ocean water. And

624
00:25:48.050 --> 00:25:50.850
what they've succeeded in showing, uh, what

625
00:25:50.850 --> 00:25:52.690
the scientists who've done this succeeded in

626
00:25:52.690 --> 00:25:55.330
showing is that the chemistry is still there.

627
00:25:55.330 --> 00:25:58.010
The, the organic, the complex organics

628
00:25:58.330 --> 00:26:00.490
are uh, there in this fresh

629
00:26:01.080 --> 00:26:03.120
ocean spray, as they call it. I love that

630
00:26:03.120 --> 00:26:05.880
idea. It's an ocean spray, uh, but it's ice

631
00:26:05.880 --> 00:26:08.840
crystals and there's a whole, you

632
00:26:08.840 --> 00:26:11.560
know, a whole list of um, things

633
00:26:11.640 --> 00:26:14.600
like esters, aromatics, heteroatom

634
00:26:14.600 --> 00:26:17.040
bearing organics. These are chemical terms

635
00:26:17.040 --> 00:26:19.840
that, um, I'm not that familiar with

636
00:26:19.840 --> 00:26:22.360
because chemistry was not my strong point.

637
00:26:22.940 --> 00:26:25.520
Uh, but these chemicals are, ah, yes, they

638
00:26:25.520 --> 00:26:27.800
are there in the ocean of Enceladus.

639
00:26:28.280 --> 00:26:31.040
And what that has done is raised

640
00:26:31.200 --> 00:26:33.520
again the possibility that living organisms

641
00:26:33.520 --> 00:26:36.480
might exist in that ocean. Uh, and that

642
00:26:36.640 --> 00:26:39.080
because these chemicals are, as we keep on

643
00:26:39.080 --> 00:26:42.080
saying, the building blocks of life uh, so

644
00:26:42.160 --> 00:26:44.160
just maybe there's something swimming around

645
00:26:44.160 --> 00:26:46.520
in the ocean of Enceladus that we are yet to

646
00:26:46.520 --> 00:26:46.960
discover.

647
00:26:47.600 --> 00:26:49.720
Andrew Dunkley: Yes. And wouldn't it be exciting? And, uh,

648
00:26:49.840 --> 00:26:52.360
hopefully in the not too distant future we'll

649
00:26:52.360 --> 00:26:54.690
be able to confirm it. Um,

650
00:26:55.280 --> 00:26:56.920
I think people are starting to get very

651
00:26:56.920 --> 00:26:58.720
confident about the possibility, though.

652
00:26:59.210 --> 00:26:59.490
Professor Fred Watson: Yep.

653
00:26:59.490 --> 00:27:02.450
Andrew Dunkley: Yeah, that's right. Fingers crossed. But, uh,

654
00:27:02.450 --> 00:27:04.170
yeah, the signs are starting to really build.

655
00:27:04.170 --> 00:27:06.730
And even though it'll be

656
00:27:06.890 --> 00:27:09.050
probably one of the most exciting things ever

657
00:27:09.050 --> 00:27:11.850
discovered, should we succeed in finding

658
00:27:11.850 --> 00:27:14.410
evidence of life elsewhere, we

659
00:27:14.650 --> 00:27:17.050
also probably shouldn't be surprised because

660
00:27:17.770 --> 00:27:20.770
water, we now know is prolific

661
00:27:20.770 --> 00:27:23.510
throughout the universe. We know there are,

662
00:27:23.510 --> 00:27:26.490
uh, probably exoplanets orbiting almost

663
00:27:26.490 --> 00:27:29.430
every star in the universe. Stands to

664
00:27:29.430 --> 00:27:32.230
reason that somewhere, somewhere out there,

665
00:27:32.390 --> 00:27:34.950
there's. There's got to be some form of life,

666
00:27:34.950 --> 00:27:37.510
even if it's only microbial, but.

667
00:27:38.150 --> 00:27:41.150
Professor Fred Watson: Or krill. Krill would be

668
00:27:41.150 --> 00:27:43.670
exciting. Green slime is what we're likely to

669
00:27:43.670 --> 00:27:46.150
find. I think green slime. Green slime will

670
00:27:46.150 --> 00:27:49.150
do. Green slime would do it. That's right. It

671
00:27:49.150 --> 00:27:49.710
would indeed.

672
00:27:49.710 --> 00:27:51.990
Andrew Dunkley: Indeed. If you'd like to read up on that

673
00:27:51.990 --> 00:27:54.710
story about the latest from Enceladus,

674
00:27:55.030 --> 00:27:57.350
you can find it in the journal Nature

675
00:27:57.430 --> 00:27:58.310
Astronomy.

676
00:28:01.190 --> 00:28:02.230
Space Butts.

677
00:28:02.790 --> 00:28:05.150
One last story in this episode, Fred, and

678
00:28:05.150 --> 00:28:07.990
it's a bit of an update on 3i Atlas the

679
00:28:07.990 --> 00:28:10.630
XO comet that is currently,

680
00:28:11.030 --> 00:28:13.790
um, doing its thing. It's doing whatever it

681
00:28:13.790 --> 00:28:16.200
wants, really. Um, but, um,

682
00:28:16.550 --> 00:28:19.190
it's, uh. It's. It's sort of reappeared. And

683
00:28:19.190 --> 00:28:21.030
they're getting some great pictures of it,

684
00:28:21.030 --> 00:28:23.840
not only from Earth, but from Mars. And,

685
00:28:24.670 --> 00:28:27.600
um. Some of these photos are extraordinary.

686
00:28:28.400 --> 00:28:30.640
Professor Fred Watson: Yes, they are. When you look at them, they're

687
00:28:30.880 --> 00:28:32.800
a little bit underwhelming until you realize

688
00:28:32.800 --> 00:28:35.640
that they've been taken by telescopes not on

689
00:28:35.640 --> 00:28:38.440
Earth, but, um, in one case on the surface of

690
00:28:38.440 --> 00:28:41.200
Mars. But, um. Uh, also, uh, from

691
00:28:41.200 --> 00:28:44.160
Mars orbit. Uh, and there's a little bit of

692
00:28:44.160 --> 00:28:46.400
a story to this because these images were

693
00:28:46.400 --> 00:28:49.210
taken, um, when, um,

694
00:28:50.160 --> 00:28:52.990
the interstellar comet 3I Atlas uh,

695
00:28:53.120 --> 00:28:56.060
made its closest passage, uh,

696
00:28:56.960 --> 00:28:59.840
closest flyby of Mars, basically, uh, 30

697
00:28:59.840 --> 00:29:02.120
million kilometers of Mars. That's quite a

698
00:29:02.120 --> 00:29:04.560
close approach compared with, um, the

699
00:29:04.560 --> 00:29:07.280
distances that we are from it on

700
00:29:07.280 --> 00:29:09.680
Earth. Uh, and that took place

701
00:29:10.080 --> 00:29:12.640
actually nearly two months ago, uh, in early

702
00:29:12.640 --> 00:29:15.480
October. Um, but what's held up the

703
00:29:15.480 --> 00:29:18.460
release of the, uh, of the images, uh,

704
00:29:18.460 --> 00:29:21.240
is the US Um government shutdown, which,

705
00:29:21.240 --> 00:29:24.040
yeah, prevented these images being

706
00:29:24.280 --> 00:29:25.000
situated.

707
00:29:25.320 --> 00:29:27.960
Andrew Dunkley: He spoke about that at length. Oh, getting

708
00:29:27.960 --> 00:29:29.040
back previous episode.

709
00:29:29.040 --> 00:29:31.320
Professor Fred Watson: So, yeah, I think, yes, we're pretty.

710
00:29:31.320 --> 00:29:34.200
Andrew Dunkley: Well squared away on the issue um, but he

711
00:29:34.200 --> 00:29:36.800
had colleagues that was so badly affected by

712
00:29:36.800 --> 00:29:39.800
that because, yes, the, um, you know, well,

713
00:29:39.800 --> 00:29:42.160
basically no income for as long as the

714
00:29:42.160 --> 00:29:43.040
shutdown existed.

715
00:29:43.040 --> 00:29:44.760
Professor Fred Watson: It's very, very difficult situation.

716
00:29:44.760 --> 00:29:47.710
Andrew Dunkley: But, yeah, so we, we know why

717
00:29:47.710 --> 00:29:49.710
NASA couldn't do anything at the time.

718
00:29:50.110 --> 00:29:52.190
Professor Fred Watson: Yeah, so that's right.

719
00:29:52.800 --> 00:29:55.670
Um, but we now have these images revealed now

720
00:29:55.670 --> 00:29:57.630
that things are up and running again. And

721
00:29:57.710 --> 00:30:00.190
perhaps the best one has come

722
00:30:00.350 --> 00:30:02.830
from the, um, HiRise

723
00:30:03.470 --> 00:30:06.110
camera on board Mars Reconnaissance Orbiter.

724
00:30:06.590 --> 00:30:09.590
And that's quite a detailed image of Comet

725
00:30:09.590 --> 00:30:12.550
3I Atlas with its short

726
00:30:12.550 --> 00:30:15.550
tail and its coma. That's the region around

727
00:30:15.550 --> 00:30:18.310
the nucleus where, uh, material is outgassing

728
00:30:18.310 --> 00:30:21.260
and, and um, shining because of, um,

729
00:30:21.260 --> 00:30:22.570
excitation by the sun.

730
00:30:24.650 --> 00:30:27.130
There's some interesting images from,

731
00:30:27.650 --> 00:30:30.490
uh, the Maven, uh, spacecraft

732
00:30:30.490 --> 00:30:33.370
as well, which, uh, has cameras on looking

733
00:30:33.370 --> 00:30:35.610
in the ultraviolet. And in fact it's got a

734
00:30:35.610 --> 00:30:38.450
spectrometer on that allows you to, uh, split

735
00:30:38.450 --> 00:30:41.200
the light up into its component colors. Uh,

736
00:30:41.610 --> 00:30:44.250
so we see the glow of hydrogen actually from,

737
00:30:44.790 --> 00:30:47.720
uh, from 3i Atlas, uh, photographed by the

738
00:30:47.720 --> 00:30:50.200
Maven spacecraft

739
00:30:50.200 --> 00:30:52.930
cameras and the Mastcam camera, uh,

740
00:30:53.520 --> 00:30:56.520
on the, uh, it's Mastcam

741
00:30:56.520 --> 00:30:59.240
Z, it's called on Perseverance on the

742
00:30:59.240 --> 00:31:01.600
surface of Mars, actually managed to capture

743
00:31:01.920 --> 00:31:04.720
a very, very faint image, uh, of

744
00:31:04.870 --> 00:31:07.720
uh, three Eye Atlas against a background of

745
00:31:07.720 --> 00:31:10.090
stars. It's faint because that's. That

746
00:31:10.330 --> 00:31:13.090
mastcam was never designed to do

747
00:31:13.090 --> 00:31:15.890
astronomy. It's all designed to navigate on

748
00:31:15.890 --> 00:31:18.010
the surface of Mars. But yet it's managed to

749
00:31:18.010 --> 00:31:20.450
catch a picture, uh, by being pointed

750
00:31:20.450 --> 00:31:23.090
upwards, obviously, uh, at this

751
00:31:23.090 --> 00:31:25.929
celestial visitor. So the hope is that as

752
00:31:25.929 --> 00:31:28.490
these images are analyzed, Andrew, we'll find

753
00:31:28.490 --> 00:31:31.330
out more about 3i Atlas, maybe even to

754
00:31:31.330 --> 00:31:34.050
get a good measurement of how big its nucleus

755
00:31:34.050 --> 00:31:36.970
is, the icy component that gives rise to

756
00:31:37.690 --> 00:31:40.460
all this luminosity. Um, the last

757
00:31:40.460 --> 00:31:42.580
I heard was that the thinking was it was in

758
00:31:42.580 --> 00:31:45.340
the region of 20 km across, which is large

759
00:31:45.340 --> 00:31:47.780
for a comet nucleus. Uh, but I think the jury

760
00:31:47.780 --> 00:31:50.300
is probably still out on that. Um, might find

761
00:31:50.300 --> 00:31:51.580
more from these measurements.

762
00:31:52.060 --> 00:31:54.700
Andrew Dunkley: So how much longer will 3i Atlas be

763
00:31:54.780 --> 00:31:55.980
in our vicinity?

764
00:31:58.460 --> 00:32:00.620
Professor Fred Watson: Quite a while. Uh, it's not. You know,

765
00:32:02.300 --> 00:32:04.860
I, um, think it passes closest to Earth

766
00:32:05.350 --> 00:32:07.790
this month, if I remember rightly. Um, and

767
00:32:07.790 --> 00:32:10.670
then we'll be receding. Uh, it has passed

768
00:32:10.670 --> 00:32:12.910
its closest to the sun, and so it certainly

769
00:32:12.910 --> 00:32:14.510
brightened up when it did that, which is what

770
00:32:14.510 --> 00:32:17.230
you expect as it leaves the

771
00:32:17.230 --> 00:32:19.910
solar system. We'll continue to track it with

772
00:32:20.150 --> 00:32:22.030
the world's big telescopes. Probably the

773
00:32:22.030 --> 00:32:23.990
James Webb will have a few more looks at it.

774
00:32:24.330 --> 00:32:27.190
Uh, and so, um, I Think we're going to

775
00:32:27.190 --> 00:32:28.950
be observing it for several months yet.

776
00:32:29.670 --> 00:32:31.990
Andrew Dunkley: Very good. All right. Keeps making the news.

777
00:32:31.990 --> 00:32:34.790
And uh, I mean it's one of those

778
00:32:34.790 --> 00:32:37.460
things like, like this is only one of a

779
00:32:37.460 --> 00:32:40.140
handful of these things that we've

780
00:32:40.140 --> 00:32:42.380
found, but it's starting to look like this is

781
00:32:42.380 --> 00:32:43.780
not an uncommon thread.

782
00:32:44.580 --> 00:32:47.180
Professor Fred Watson: That's right. And I think once again harking

783
00:32:47.180 --> 00:32:49.620
back to the Vera C. Rubin telescope, we're

784
00:32:49.620 --> 00:32:51.499
going to find more of these. Uh, when that

785
00:32:51.499 --> 00:32:53.060
telescope comes online we're probably going

786
00:32:53.060 --> 00:32:55.500
to have, you know, we've got three known

787
00:32:55.500 --> 00:32:57.820
interstellar objects now. It'll probably be

788
00:32:57.820 --> 00:33:00.580
20 by middle of next year. Who

789
00:33:00.580 --> 00:33:03.200
knows, it'll be quite extraordinary indeed.

790
00:33:03.280 --> 00:33:05.760
Andrew Dunkley: All right, uh, you can read more about the

791
00:33:05.870 --> 00:33:08.498
uh, images that have been taken of 3i

792
00:33:08.582 --> 00:33:10.920
Atlas and you can see them too at the

793
00:33:10.920 --> 00:33:13.440
universetoday.com website.

794
00:33:14.560 --> 00:33:17.080
Fred, that brings us to the end. Thank you so

795
00:33:17.080 --> 00:33:17.360
much.

796
00:33:17.920 --> 00:33:20.690
Professor Fred Watson: It's been a pleasure. Andrew. Um, uh, uh,

797
00:33:20.800 --> 00:33:23.520
I've forgotten how much I miss uh, my

798
00:33:23.520 --> 00:33:25.720
weekly dose of spacenauts. So it's good to be

799
00:33:25.720 --> 00:33:26.560
talking again.

800
00:33:26.720 --> 00:33:29.560
Andrew Dunkley: It's good to have you back. Um, thank you for

801
00:33:29.560 --> 00:33:30.320
deciding to return

802
00:33:32.650 --> 00:33:34.810
even without the red carpet. Oh and by the

803
00:33:34.810 --> 00:33:36.530
way, that golfer uh, I played with today,

804
00:33:36.530 --> 00:33:39.010
Piper Stubbs from Melbourne. Oh good, Stubbs.

805
00:33:39.010 --> 00:33:39.930
Professor Fred Watson: Look up the name.

806
00:33:40.010 --> 00:33:42.810
Andrew Dunkley: She uh, she studied um, at

807
00:33:43.050 --> 00:33:44.770
college uh, in the United States and played

808
00:33:44.770 --> 00:33:47.610
collegiate golf over there. Ah, she's

809
00:33:47.610 --> 00:33:50.410
finished now and she qualified um, as a,

810
00:33:50.650 --> 00:33:52.610
in political science. So.

811
00:33:52.610 --> 00:33:53.210
Professor Fred Watson: Very good.

812
00:33:53.450 --> 00:33:56.250
Andrew Dunkley: Yeah, uh, quite a bright young lady.

813
00:33:56.560 --> 00:33:59.010
Uh, and um, thanks to Huw in the studio.

814
00:33:59.010 --> 00:34:00.570
Although he couldn't be with us today because

815
00:34:00.570 --> 00:34:03.070
he heard there were 40,000 near of asteroids

816
00:34:03.070 --> 00:34:05.350
discovered. So he built himself a bunker.

817
00:34:05.830 --> 00:34:08.300
He won't come out. And um,

818
00:34:09.350 --> 00:34:11.830
and uh, by the way, if you would like to

819
00:34:11.830 --> 00:34:14.270
become a patron, um, by all means, jump on

820
00:34:14.270 --> 00:34:17.150
our website and, and find uh, out uh, all

821
00:34:17.150 --> 00:34:19.150
about it. I uh, know it's uh, there are

822
00:34:19.150 --> 00:34:21.590
difficult times and we would never expect you

823
00:34:22.150 --> 00:34:24.950
to um, to, to spend money to listen to us.

824
00:34:24.950 --> 00:34:27.630
It's a, it's a free podcast but people choose

825
00:34:27.630 --> 00:34:30.590
to and there are multiple options these

826
00:34:30.590 --> 00:34:32.960
days. So if you want to become a patron, uh,

827
00:34:33.110 --> 00:34:36.050
you'll get commercial free edition of the

828
00:34:36.050 --> 00:34:38.770
podcast. So um, uh, if you'd prefer to be

829
00:34:38.770 --> 00:34:40.330
commercial free, this is the way to do it.

830
00:34:40.330 --> 00:34:42.690
You can do it through Patreon, Supercast,

831
00:34:42.930 --> 00:34:45.930
Spreaker and Apple podcasts. They

832
00:34:45.930 --> 00:34:48.930
all do um, various uh, uh, payment

833
00:34:48.930 --> 00:34:51.090
options if that's your thing. If it's not,

834
00:34:51.330 --> 00:34:54.010
just forget everything I just said and don't

835
00:34:54.010 --> 00:34:55.650
forget to visit us online while you're there.

836
00:34:55.650 --> 00:34:58.090
Or the, uh, or the Facebook group. Uh, the

837
00:34:58.090 --> 00:35:00.370
podcast group on Facebook. Uh, very active.

838
00:35:00.370 --> 00:35:02.100
And you can talk to each other about. About

839
00:35:02.100 --> 00:35:04.260
anything you like to do with space and

840
00:35:04.340 --> 00:35:07.140
astronomy. That's it for this episode.

841
00:35:07.140 --> 00:35:09.780
Join us again soon when we do a Q A episode.

842
00:35:09.940 --> 00:35:12.700
Um, and, and looking forward to having you

843
00:35:12.700 --> 00:35:15.140
join us then from me, Andrew Dunkley. Until

844
00:35:15.140 --> 00:35:15.700
next time.

845
00:35:16.100 --> 00:35:16.460
Professor Fred Watson: Bye.

846
00:35:16.460 --> 00:35:19.420
Andrew Dunkley: Bye. You'll be listening to the

847
00:35:19.420 --> 00:35:20.820
Space Nuts podcast,

848
00:35:22.340 --> 00:35:25.140
available at Apple Podcasts, Spotify,

849
00:35:25.300 --> 00:35:27.630
iHeartRadio, or your favorite favorite

850
00:35:27.630 --> 00:35:29.790
podcast player. You can also stream on

851
00:35:29.790 --> 00:35:32.790
demand@bytes.com. um, this has been another

852
00:35:32.790 --> 00:35:35.470
quality podcast production from bytes.

853
00:35:35.630 --> 00:35:35.910
Professor Fred Watson: Com. Um.