Theia’s True Origins, 40,000 Asteroids & Enceladus’ Organic Mystery | Space Nuts: Astronomy...
Space News TodayNovember 28, 202500:36:5833.86 MB

Theia’s True Origins, 40,000 Asteroids & Enceladus’ Organic Mystery | Space Nuts: Astronomy...

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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. (https://www.spacenutspodcast.com/) 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.

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Stay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.


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Episode link: https://play.headliner.app/episode/30340531?utm_source=youtube

Kind: captions Language: en
00:00:00 --> 00:00:02 Hi there. Thanks for joining us on Space

00:00:02 --> 00:00:04 Nuts, where we talk astronomy and space

00:00:04 --> 00:00:06 science. My name is Andrew Dunley. Great

00:00:06 --> 00:00:09 to have your company. Coming up on this

00:00:09 --> 00:00:11 episode, uh, a new study from the Max

00:00:11 --> 00:00:13 Plank Institute shedding some new light

00:00:13 --> 00:00:16 on the the Earth relationship, which

00:00:16 --> 00:00:18 might surprise you. And just when you

00:00:18 --> 00:00:21 thought it was safe to go back to sleep

00:00:21 --> 00:00:24 at night, 40 new uh near Earth

00:00:24 --> 00:00:26 asteroids have been discovered. Only

00:00:26 --> 00:00:29 40. And they're all coming our way.

00:00:29 --> 00:00:31 No, they're not. Uh, the Search for Life

00:00:31 --> 00:00:34 just got another um a bit closer uh

00:00:34 --> 00:00:37 thanks to some Cassini data and three

00:00:37 --> 00:00:40 Atlas still making the news. We'll talk

00:00:40 --> 00:00:42 about all of that on this episode of

00:00:42 --> 00:00:43 Space Nuts.

00:00:43 --> 00:00:48 >> 15 seconds. Guidance is internal. 10 9

00:00:48 --> 00:00:50 Ignition sequence start.

00:00:50 --> 00:00:51 >> Space Nuts.

00:00:51 --> 00:00:53 >> 5 4 3 2

00:00:53 --> 00:00:56 >> 1 2 3 4 5 5 4 3 2 1

00:00:56 --> 00:00:58 >> Space nuts. astronauts report. It feels

00:00:58 --> 00:00:59 good.

00:01:00 --> 00:01:02 >> And we rolled out the red carpet because

00:01:02 --> 00:01:04 he's back. It's Professor Fred, what's

00:01:04 --> 00:01:06 an astronomer at large? Hello, Fred.

00:01:06 --> 00:01:08 >> Hi, Andrew. I'm actually looking for the

00:01:08 --> 00:01:09 red carpet.

00:01:09 --> 00:01:11 >> Yeah, I rolled it back up again. It's

00:01:12 --> 00:01:14 had a few moth holes in it. [laughter]

00:01:14 --> 00:01:16 >> Yeah. But he's glad to hear it.

00:01:16 --> 00:01:17 >> Good.

00:01:17 --> 00:01:20 >> And you, too. And um Well, we've missed

00:01:20 --> 00:01:21 you. No, wait a minute. No, you've

00:01:21 --> 00:01:24 missed one or the other. Yes, we did

00:01:24 --> 00:01:26 have a few people starting to um I found

00:01:26 --> 00:01:28 in radio if you were away for more than

00:01:28 --> 00:01:30 about 3 or 4 weeks people started

00:01:30 --> 00:01:33 ringing the station and emailing to say

00:01:33 --> 00:01:36 where's Joe Blogs or where's you know

00:01:36 --> 00:01:38 this started happening with you Fred so

00:01:38 --> 00:01:39 >> oh seriously

00:01:39 --> 00:01:40 >> where's Fred where's Fred what's going

00:01:40 --> 00:01:42 on with Fred what happened to Fred

00:01:42 --> 00:01:45 >> uh and and funnily enough I I was able

00:01:45 --> 00:01:48 to say yeah I don't know

00:01:48 --> 00:01:48 [laughter]

00:01:48 --> 00:01:50 >> seen him for weeks

00:01:50 --> 00:01:53 >> he's just disappeared but no he's back.

00:01:53 --> 00:01:55 He's back. So, where did where did you

00:01:55 --> 00:01:57 go? What was the give us the give us the

00:01:57 --> 00:01:59 the the preed version of your seven

00:01:59 --> 00:02:01 weeks away.

00:02:01 --> 00:02:03 >> Three weeks um leading one of man's

00:02:04 --> 00:02:07 tours uh which uh is the third big one

00:02:07 --> 00:02:10 we've done this year actually um after

00:02:10 --> 00:02:12 the Arctic in in January and February

00:02:12 --> 00:02:14 and then it was uh Western Australia in

00:02:14 --> 00:02:16 the middle of the year and then this

00:02:16 --> 00:02:18 time we went to Japan. Uh, so we had a

00:02:18 --> 00:02:21 tour that took in uh interesting places

00:02:21 --> 00:02:25 like Osaka and Kyoto and Tokyo. And um

00:02:25 --> 00:02:27 Mani and I actually made a side trip

00:02:27 --> 00:02:29 down to Hiroshima, which is a place I've

00:02:29 --> 00:02:31 always wanted to visit and I'm very glad

00:02:31 --> 00:02:32 I did.

00:02:32 --> 00:02:35 >> Very sobering place to be. Uh but a

00:02:35 --> 00:02:37 welcoming city as well. It was um it was

00:02:38 --> 00:02:39 a pleasure to be there.

00:02:39 --> 00:02:41 >> Uh and then um we wound up actually in

00:02:41 --> 00:02:44 Hokkaido right in the north of of Japan

00:02:44 --> 00:02:46 where it was essentially coming on to

00:02:46 --> 00:02:48 winter. uh they they get lots and lots

00:02:48 --> 00:02:51 of snow up there. It's a lot similar to

00:02:51 --> 00:02:52 um to the Arctic, even though it's at a

00:02:52 --> 00:02:55 much lower latitude. Um yeah, that was

00:02:55 --> 00:02:56 all fun. So, we came back, we had four

00:02:56 --> 00:02:58 nights in Sydney at home [laughter] in

00:02:58 --> 00:03:00 our own bed, do the washing, and then

00:03:00 --> 00:03:02 off again to a conference on dark skies

00:03:02 --> 00:03:05 in County Mayo in Ireland. Uh we were in

00:03:05 --> 00:03:07 Ireland for about a week, a little bit

00:03:07 --> 00:03:08 more than a week. We did some touring

00:03:08 --> 00:03:11 down in the south. We blew a kiss to the

00:03:12 --> 00:03:14 Blanny Stone. I did.

00:03:14 --> 00:03:15 >> Yeah. [laughter]

00:03:15 --> 00:03:17 I wasn't game to kiss the Blney Stone

00:03:17 --> 00:03:18 because you have to be upside down.

00:03:18 --> 00:03:19 Yeah.

00:03:19 --> 00:03:20 >> Doesn't suit me at all.

00:03:20 --> 00:03:22 >> We didn't do that either.

00:03:22 --> 00:03:23 >> No. [snorts] So, we blew it a kiss,

00:03:23 --> 00:03:25 which is enough apparently to get the

00:03:25 --> 00:03:27 gift of the gab. And then, in fact,

00:03:27 --> 00:03:29 Blani was a delightful place. It was the

00:03:29 --> 00:03:31 one sunny afternoon we had in in um

00:03:31 --> 00:03:33 Ireland and it was lovely. Such an

00:03:33 --> 00:03:35 amazing castle and the crowds are

00:03:35 --> 00:03:37 picture perfect. Uh then we went over to

00:03:37 --> 00:03:40 Scotland, spent some time with my two

00:03:40 --> 00:03:42 daughters. Had a great time with them.

00:03:42 --> 00:03:45 Took a weekend out. Uh we all beled off

00:03:45 --> 00:03:47 to St. Andrews where I was educated. Uh

00:03:47 --> 00:03:49 a town that's very close to my heart. We

00:03:49 --> 00:03:50 had a great time there. Didn't do any

00:03:50 --> 00:03:52 golf. I'm sorry, but we did walk past

00:03:52 --> 00:03:54 the old course and thought of you with

00:03:54 --> 00:03:57 your golf clubs and that they don't

00:03:57 --> 00:03:58 float and things like that.

00:03:58 --> 00:04:00 >> And and

00:04:00 --> 00:04:03 then after that we um took the train

00:04:03 --> 00:04:05 down to Birmingham from Edinburgh and

00:04:05 --> 00:04:07 that was pleasant. And at Birmingham, we

00:04:07 --> 00:04:09 got on a plane and went to Cyprus uh in

00:04:09 --> 00:04:11 the eastern end of the Mediterranean and

00:04:11 --> 00:04:13 had we actually had a holiday six

00:04:13 --> 00:04:15 >> nights. Found an observatory, a brand

00:04:15 --> 00:04:17 new one called Trudeau.

00:04:17 --> 00:04:19 >> Trudeau observatory. Yes, we did. We

00:04:19 --> 00:04:20 Manne checked it out as she does with

00:04:20 --> 00:04:22 these things. And so we made a

00:04:22 --> 00:04:24 pilgrimage up into the hills, not very

00:04:24 --> 00:04:26 far from the highest point in the island

00:04:26 --> 00:04:29 actually, Mount Olympus. Uh but um it's

00:04:29 --> 00:04:31 got its own little mountain has uh uh

00:04:31 --> 00:04:33 the Trudeau Observatory. Uh we went up

00:04:33 --> 00:04:35 there. We went completely unannounced.

00:04:35 --> 00:04:37 They just had a tour group through. So,

00:04:37 --> 00:04:39 there were two coaches which were just

00:04:39 --> 00:04:42 about to set off down this road that was

00:04:42 --> 00:04:44 slightly narrower than a coach. Uh, and

00:04:44 --> 00:04:48 an angle of 45 degrees. Uh, if we'd been

00:04:48 --> 00:04:49 um, you know, if we'd been half an hour

00:04:49 --> 00:04:51 later, we'd have probably not been able

00:04:51 --> 00:04:53 to get there because these damn coaches

00:04:53 --> 00:04:56 going by. But when we arrived, um, that,

00:04:56 --> 00:04:57 you know, they just got rid of all the

00:04:57 --> 00:04:59 coach party and we turned up and said,

00:04:59 --> 00:05:01 "We're astronomers. Uh, can we have a

00:05:01 --> 00:05:02 look?" And they said, "Oh, no, no,

00:05:02 --> 00:05:04 you'll have to wait till the next tour."

00:05:04 --> 00:05:06 Uh but we managed to get hold of the

00:05:06 --> 00:05:08 events manager who said, "Yeah, come in.

00:05:08 --> 00:05:09 Let's talk about what we do and all the

00:05:09 --> 00:05:11 rest of it." Had a great time. Awesome.

00:05:11 --> 00:05:12 So that was very very nice.

00:05:12 --> 00:05:13 >> Yeah.

00:05:13 --> 00:05:16 >> And if she's a Space Nuts listener, um

00:05:16 --> 00:05:18 nice to have met you. I think it was

00:05:18 --> 00:05:20 Arena was her name.

00:05:20 --> 00:05:20 >> Nice.

00:05:20 --> 00:05:22 >> Greek version of that. And then came

00:05:22 --> 00:05:24 home uh and we came home last week and

00:05:24 --> 00:05:25 we're now jetlagged.

00:05:26 --> 00:05:27 >> Yeah, it's it's hard to get over

00:05:27 --> 00:05:28 jetlagged. I think it's it's an age

00:05:28 --> 00:05:30 thing, Fred. We can't

00:05:30 --> 00:05:32 >> could be except um my other half is a

00:05:32 --> 00:05:34 lot younger than I am and she's jetlike

00:05:34 --> 00:05:36 too. [laughter]

00:05:36 --> 00:05:37 >> Just goes a bit territory.

00:05:38 --> 00:05:39 >> Yeah. Well, I I got a golf story for

00:05:39 --> 00:05:41 you. While you were away, I won a I won

00:05:41 --> 00:05:42 a championship.

00:05:42 --> 00:05:44 >> You You did? Yeah.

00:05:44 --> 00:05:46 >> Well done. So, it was um

00:05:46 --> 00:05:48 >> 17 years between

00:05:48 --> 00:05:51 >> uh uh Well, no, I came uh in the state

00:05:51 --> 00:05:55 championships. I came third on handicap

00:05:55 --> 00:05:57 and uh top 10. I finished ninth, I

00:05:57 --> 00:05:58 think.

00:05:58 --> 00:05:59 >> Fantastic. in the state championship,

00:05:59 --> 00:06:01 but then we had our own um championship

00:06:01 --> 00:06:03 at do golf club the other day and I I

00:06:04 --> 00:06:05 managed to win one of those. So

00:06:05 --> 00:06:06 >> that's very good.

00:06:06 --> 00:06:09 >> And then today just before this I played

00:06:09 --> 00:06:11 in the proam because we're hosting the

00:06:11 --> 00:06:14 New South Wales women's open qualifying

00:06:14 --> 00:06:15 event. So

00:06:15 --> 00:06:17 >> played with a young lass from Melbourne.

00:06:17 --> 00:06:21 Her name is Piper. Um Piper

00:06:21 --> 00:06:25 oh gone blank. Um anyway, come back to

00:06:25 --> 00:06:28 me. Uh lovely young lady, hits a really

00:06:28 --> 00:06:31 mean ball and wishing her well. Hope she

00:06:31 --> 00:06:33 makes it to the New South Wales Open and

00:06:33 --> 00:06:35 um I'll be watching her career closely.

00:06:35 --> 00:06:37 So very good.

00:06:37 --> 00:06:38 >> She beat you.

00:06:38 --> 00:06:41 >> Uh gosh, yes. Oh yes. Well, it was a

00:06:41 --> 00:06:42 team's event today, so we were

00:06:42 --> 00:06:43 technically playing together, but she

00:06:43 --> 00:06:47 out drove us miles. Yes. She could hit

00:06:47 --> 00:06:50 it a long way, but uh just a pleasure.

00:06:50 --> 00:06:53 Just a delight. We had a good day.

00:06:53 --> 00:06:55 >> We should get down to it, Fred.

00:06:55 --> 00:06:57 >> We should. Yes, we're not here to talk

00:06:57 --> 00:06:59 about golf, are we? Although it doesn't

00:06:59 --> 00:06:59 seem that way.

00:07:00 --> 00:07:03 >> Not for a change. Um, our first story

00:07:03 --> 00:07:05 takes us back 4 and a half billion years

00:07:05 --> 00:07:08 when our neighboring world known as Thea

00:07:08 --> 00:07:10 smashed into us and all hell broke

00:07:10 --> 00:07:13 loose, literally and figuratively. But,

00:07:13 --> 00:07:15 uh, a new study has just been released

00:07:15 --> 00:07:17 from the Max Plank Institute that's shed

00:07:17 --> 00:07:20 a bit of new light on the the earth

00:07:20 --> 00:07:22 relationship. Uh it it doesn't sound

00:07:22 --> 00:07:25 like this was a what we originally

00:07:25 --> 00:07:27 thought, just some random thing coming

00:07:27 --> 00:07:29 in and hitting us. There's there's more

00:07:29 --> 00:07:32 to the story now.

00:07:32 --> 00:07:34 >> There is. Yes. Um sorry, Andrew, you

00:07:34 --> 00:07:35 broke up there, but I think I know what

00:07:35 --> 00:07:37 you said. Uh

00:07:37 --> 00:07:40 um the the story of the of course this

00:07:40 --> 00:07:43 has been the the principal theory uh for

00:07:43 --> 00:07:44 the origin of the moon for at least the

00:07:44 --> 00:07:47 last 60 years. uh when the Apollo

00:07:47 --> 00:07:49 astronauts brought back what was it 380

00:07:49 --> 00:07:52 kg of lunar rock and soil which is still

00:07:52 --> 00:07:56 being analyzed. Um so uh thea is the

00:07:56 --> 00:08:00 hypothesized planet uh perhaps

00:08:00 --> 00:08:02 protolanet is a better word because this

00:08:02 --> 00:08:04 was at a time when the solar system was

00:08:04 --> 00:08:05 still in its infancy 4 and a half

00:08:05 --> 00:08:09 billion years ago. Um and this object uh

00:08:09 --> 00:08:12 basically clouded the earth. Uh and uh

00:08:12 --> 00:08:14 we think that what happened in the

00:08:14 --> 00:08:16 aftermath of the that collision was a

00:08:16 --> 00:08:19 cloud of debris raised from the surface

00:08:19 --> 00:08:21 of the earth went into orbit around the

00:08:21 --> 00:08:22 earth and eventually coalesed to form

00:08:22 --> 00:08:26 the moon. And so we've we've um had

00:08:26 --> 00:08:28 puzzles which you and I have spoken

00:08:28 --> 00:08:32 about a number of times as to why it is.

00:08:32 --> 00:08:34 Well, let me let me step back a bit. The

00:08:34 --> 00:08:37 the first theory was that because this

00:08:37 --> 00:08:39 is a smaller object hitting a bigger

00:08:39 --> 00:08:41 object. So theor is thought to have been

00:08:41 --> 00:08:43 half the size of the earth to get the

00:08:43 --> 00:08:46 dynamics right. Um the earth's a bigger

00:08:46 --> 00:08:49 planet. Uh what you would expect is that

00:08:49 --> 00:08:52 the the debris cloud raised from the

00:08:52 --> 00:08:54 earth when the collision happened would

00:08:54 --> 00:08:58 be mostly made of the material. Um, and

00:08:58 --> 00:09:00 that's been a puzzle for a long time

00:09:00 --> 00:09:04 because most of the lunar rocks and soil

00:09:04 --> 00:09:07 have the same isotopic signature, which

00:09:07 --> 00:09:09 we've talked about before as well, the

00:09:10 --> 00:09:11 same isotopic signature as the Earth.

00:09:11 --> 00:09:14 They're identical uh to the Earth's

00:09:14 --> 00:09:16 rocks. And so that was seen as a puzzle.

00:09:16 --> 00:09:18 And then about probably five years ago

00:09:18 --> 00:09:20 or so, we did cover it on Space Note.

00:09:20 --> 00:09:22 some Japanese researchers um figured out

00:09:22 --> 00:09:24 that if the Earth was still effectively

00:09:24 --> 00:09:27 molten at that time, if it was still a

00:09:27 --> 00:09:29 magnum magma world when the collision

00:09:29 --> 00:09:32 happened, then you'd get um a moon that

00:09:32 --> 00:09:34 was formed largely of of Earth

00:09:34 --> 00:09:36 compounds.

00:09:36 --> 00:09:39 So, um what has now happened is that um

00:09:39 --> 00:09:42 a close examination has been made and as

00:09:42 --> 00:09:44 you're right, it's the Maxplank

00:09:44 --> 00:09:46 Institute for Solar System Research

00:09:46 --> 00:09:48 along with the University of Chicago. um

00:09:48 --> 00:09:52 they've they've really honed in on the

00:09:52 --> 00:09:56 uh the the exact uh details of the

00:09:56 --> 00:09:59 isotopes in rocks from the earth, the

00:09:59 --> 00:10:01 moon and meteorites because they're part

00:10:02 --> 00:10:05 of the story too. And and it's not just

00:10:05 --> 00:10:06 the sort of isotopes that have been

00:10:06 --> 00:10:08 looked at before. These are iron,

00:10:08 --> 00:10:11 chromium, malibdum, malibdinum,

00:10:11 --> 00:10:15 zirconium. All these iso that these um

00:10:15 --> 00:10:17 chemical elements their isotope data

00:10:18 --> 00:10:22 have been analyzed to look again at what

00:10:22 --> 00:10:25 we find because yes we we still find

00:10:25 --> 00:10:27 that the the earth and the moon have

00:10:27 --> 00:10:31 very similar isotopic mixes. Uh but then

00:10:31 --> 00:10:34 you can identify some slight differences

00:10:34 --> 00:10:37 that are attributed to be isotopes that

00:10:37 --> 00:10:40 have come from thea itself. So they can

00:10:40 --> 00:10:43 tease out what was Thea and what was

00:10:43 --> 00:10:46 Earth. And it turns out that when you do

00:10:46 --> 00:10:49 that, you still get a similar picture

00:10:49 --> 00:10:53 that the isotope ratios on Thea were

00:10:53 --> 00:10:55 probably very similar to what they are

00:10:56 --> 00:11:01 on Earth. Um, and that is

00:11:01 --> 00:11:03 symptomatic, if I can put it that way,

00:11:03 --> 00:11:08 of the Earth and Thea being born close

00:11:08 --> 00:11:10 together. And the reason why we think

00:11:10 --> 00:11:12 that is that when you look at the solar

00:11:12 --> 00:11:15 system, you find that these isotope

00:11:15 --> 00:11:18 ratios change depending on how far out

00:11:18 --> 00:11:20 you are from the sun. So if you've got

00:11:20 --> 00:11:23 two planets with very similar isotope

00:11:23 --> 00:11:26 ratios, then what you can deduce from

00:11:26 --> 00:11:29 that is that they were orbiting the sun

00:11:29 --> 00:11:32 close together. And that makes complete

00:11:32 --> 00:11:33 sense because eventually they run into

00:11:33 --> 00:11:37 one another. Um but what the outcome of

00:11:37 --> 00:11:40 this research is is that uh thea was not

00:11:40 --> 00:11:42 just a random object that ran into the

00:11:42 --> 00:11:44 earth in the early solar system. It was

00:11:44 --> 00:11:47 actually if not a companion of earth but

00:11:47 --> 00:11:49 something in a very similar orbit. So

00:11:50 --> 00:11:51 you know maybe we had Mercury, Venus,

00:11:51 --> 00:11:55 the Earth, Mars as the rocky planets. Um

00:11:55 --> 00:11:57 although that order, you know, I've made

00:11:57 --> 00:11:59 that up, but that's the kind of thing

00:11:59 --> 00:12:01 it's it's bringing bringing Thea into

00:12:02 --> 00:12:03 the picture as something that would have

00:12:03 --> 00:12:06 been maybe had it not collided with the

00:12:06 --> 00:12:08 Earth, it would have been uh the ninth

00:12:08 --> 00:12:10 planet uh in the inner part of the solar

00:12:10 --> 00:12:13 system. So uh a very nice piece of work,

00:12:13 --> 00:12:15 some very very careful studies there

00:12:15 --> 00:12:16 that I think has raised a lot of um

00:12:16 --> 00:12:19 interest in the uh uh the planetary

00:12:20 --> 00:12:22 science community. Yeah, I suppose that

00:12:22 --> 00:12:25 sort of uh confirms that it was part of

00:12:25 --> 00:12:26 the solar system and not just some

00:12:26 --> 00:12:29 random thing passing through knocking us

00:12:29 --> 00:12:31 over in the process.

00:12:31 --> 00:12:33 >> That's right. Yeah. And um and I should

00:12:33 --> 00:12:36 just explain how how the the remnants

00:12:36 --> 00:12:39 have been the the isotopes have been

00:12:39 --> 00:12:41 determined and it's by looking at things

00:12:41 --> 00:12:43 that we find in the crust of the earth.

00:12:43 --> 00:12:45 Uh because we know that the heavy

00:12:45 --> 00:12:47 elements would have already sunk to the

00:12:47 --> 00:12:49 to the center of the earth when that

00:12:49 --> 00:12:51 collision happened. So when we think

00:12:51 --> 00:12:53 find things like these malib malibdinum

00:12:54 --> 00:12:57 iron zirconium things of that sort we

00:12:58 --> 00:12:59 can infer that some of that actually

00:12:59 --> 00:13:02 came from theory itself and that's how

00:13:02 --> 00:13:05 the similarity has been deduced along

00:13:05 --> 00:13:07 with looking at meteorite samples too.

00:13:07 --> 00:13:11 So you're right um it it is not

00:13:11 --> 00:13:13 something that's come from another solar

00:13:13 --> 00:13:15 system like our current visitor Threei

00:13:15 --> 00:13:18 Atlas. Uh it's it's definitely a

00:13:18 --> 00:13:21 homegrown planet that we collided with.

00:13:21 --> 00:13:23 >> Okay. And now it's sort of a well it's

00:13:23 --> 00:13:25 not a part of us. There's bits and

00:13:25 --> 00:13:27 pieces of it but um most of it sort of

00:13:27 --> 00:13:29 vanquished into into the never never

00:13:29 --> 00:13:30 didn't it?

00:13:30 --> 00:13:32 >> Yeah. A lot of it would have done but um

00:13:32 --> 00:13:33 some of it's in the moon. Some of it's

00:13:33 --> 00:13:35 on the earth as well.

00:13:35 --> 00:13:37 >> Yeah. All right. Uh so I guess some new

00:13:38 --> 00:13:40 information from the Max Planck

00:13:40 --> 00:13:43 Institute about uh Thea being a part of

00:13:43 --> 00:13:44 the inner solar system. If you'd like to

00:13:44 --> 00:13:46 read about that, there's a really great

00:13:46 --> 00:13:49 article at scienceblog.com.

00:13:49 --> 00:13:51 This is Space Nuts with Andrew Dunley

00:13:51 --> 00:13:53 and Professor Fred.

00:13:53 --> 00:13:55 Let's take a break from the show and

00:13:55 --> 00:13:58 talk about our sponsor, NordVPN. Now, if

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00:15:10 --> 00:15:12 Don't forget the code word spacen nuts

00:15:12 --> 00:15:17 and their 30-day money back guarantee.

00:15:17 --> 00:15:18 >> And I feel

00:15:18 --> 00:15:20 >> space nuts. Uh, now to some really good

00:15:20 --> 00:15:24 news, Fred. 40 near-earth asteroids

00:15:24 --> 00:15:26 have been discovered. Is that all? Is

00:15:26 --> 00:15:28 that all they could find?

00:15:28 --> 00:15:30 >> Well, it's Yeah, I mean, we've for a you

00:15:30 --> 00:15:32 know, for a long time we've known of

00:15:32 --> 00:15:34 39.

00:15:34 --> 00:15:36 [laughter]

00:15:36 --> 00:15:37 Maybe not for very long because because

00:15:37 --> 00:15:39 we're discovering asteroids at a very

00:15:39 --> 00:15:41 prolific rate at the moment and that

00:15:41 --> 00:15:42 comes about because we've got such good

00:15:42 --> 00:15:45 technology discovering them. Um, and so

00:15:46 --> 00:15:47 yes, this is a milestone that's been

00:15:47 --> 00:15:49 celebrated by ISSa, the European Space

00:15:49 --> 00:15:52 Agency. Uh, and you know, so they've

00:15:52 --> 00:15:55 they've put out a a press release saying

00:15:55 --> 00:15:57 40 near-ear asteroids discovered.

00:15:57 --> 00:15:59 Uh, what do we mean by a near-earth

00:15:59 --> 00:16:01 asteroid? It's one that approaches

00:16:01 --> 00:16:05 within about 45 million kilometers of

00:16:05 --> 00:16:08 the Earth. And that's nearly a third of

00:16:08 --> 00:16:11 the distance to the sun. So it's when

00:16:11 --> 00:16:13 you say near, it's it's a fairly

00:16:13 --> 00:16:16 relative term. It's one uh with objects

00:16:16 --> 00:16:18 that that can get within that distance

00:16:18 --> 00:16:21 of Earth. Then there's another subset of

00:16:21 --> 00:16:24 those though that we tend to call PHAS,

00:16:24 --> 00:16:28 potentially hazardous asteroids. Uh and

00:16:28 --> 00:16:30 um there are something like I think if I

00:16:30 --> 00:16:31 remember right, it's about two and a

00:16:31 --> 00:16:33 half thousand of those. And they're the

00:16:33 --> 00:16:35 ones whose orbits cross the orbit of the

00:16:35 --> 00:16:36 Earth.

00:16:36 --> 00:16:38 >> Um and so they are potentially

00:16:38 --> 00:16:39 hazardous. So they're the ones that we

00:16:40 --> 00:16:42 keep an eye on all the time uh

00:16:42 --> 00:16:45 monitoring where they are uh and

00:16:45 --> 00:16:48 checking forward uh in computers once we

00:16:48 --> 00:16:50 know their orbits checking forward as to

00:16:50 --> 00:16:52 whether there's any likelihood of

00:16:52 --> 00:16:54 collision. The good news is is that

00:16:54 --> 00:16:56 there's not uh over the next 100 years

00:16:56 --> 00:16:59 or so we've got a fairly clean sweep of

00:16:59 --> 00:17:01 things at least things bigger than about

00:17:01 --> 00:17:04 140 mters across and they can be very

00:17:04 --> 00:17:06 dangerous. they can be they could be

00:17:06 --> 00:17:08 city destroyers or even state

00:17:08 --> 00:17:11 destroyers. So um so keeping an eye on

00:17:11 --> 00:17:13 those is important. Uh and I think you

00:17:13 --> 00:17:15 know the reason why um issa has

00:17:16 --> 00:17:17 highlighted this is because it does

00:17:17 --> 00:17:20 highlight the whole um regime of

00:17:20 --> 00:17:22 planetary defense. Uh that's a very

00:17:22 --> 00:17:26 active area in astronomy and um actually

00:17:26 --> 00:17:28 almost civil defense as well. It's not

00:17:28 --> 00:17:30 just astronomy that is concerned with

00:17:30 --> 00:17:32 that. I I think I probably mentioned

00:17:32 --> 00:17:34 before when I was at the IAU a couple of

00:17:34 --> 00:17:36 years ago um I actually got myself into

00:17:36 --> 00:17:38 a meeting uh which was the planetary

00:17:38 --> 00:17:41 defense agency

00:17:41 --> 00:17:43 uh talking about uh their next

00:17:43 --> 00:17:47 activities which included a a mock um a

00:17:47 --> 00:17:49 mock threatened planetary asteroid

00:17:49 --> 00:17:51 impact and how all the services would

00:17:52 --> 00:17:53 deal with that and you know the astron

00:17:53 --> 00:17:56 from the astronomers right to the people

00:17:56 --> 00:17:58 who get the fire engines out to put out

00:17:58 --> 00:18:00 the fires and things of that. thought it

00:18:00 --> 00:18:02 was very interesting thing to watch. So,

00:18:02 --> 00:18:04 um what it did was reure reassured me

00:18:04 --> 00:18:07 that were in quite good hands. Uh but

00:18:07 --> 00:18:09 yeah, the bottom line, uh 40

00:18:09 --> 00:18:12 near-earth asteroids known. Uh the good

00:18:12 --> 00:18:14 news is always that the big ones, uh

00:18:14 --> 00:18:16 which are the most dangerous ones,

00:18:16 --> 00:18:18 they're the easiest to find. And we

00:18:18 --> 00:18:21 think we know pretty well all of the

00:18:21 --> 00:18:24 asteroids bigger than a kilometer, which

00:18:24 --> 00:18:27 would be um dinosaur killers. they would

00:18:27 --> 00:18:28 wipe out, you know, there'd be mass

00:18:28 --> 00:18:31 extinction objects. Uh we think one of

00:18:31 --> 00:18:35 those hits the earth roughly every 200

00:18:35 --> 00:18:37 million years. Uh it's 66 million years

00:18:37 --> 00:18:40 ago since the last one did, which was

00:18:40 --> 00:18:42 was the one that wiped out the the

00:18:42 --> 00:18:44 dinosaurs. Um since then though, we've

00:18:44 --> 00:18:46 learned a lot about not only about

00:18:46 --> 00:18:48 asteroids, but about how we might

00:18:48 --> 00:18:52 deflect uh an asteroid if uh if there

00:18:52 --> 00:18:54 was one that could be shown to be on a

00:18:54 --> 00:18:55 collision course with Earth. And you

00:18:56 --> 00:18:58 have I you and I have talked at length

00:18:58 --> 00:19:00 and with great enthusiasm about the Dart

00:19:00 --> 00:19:02 mission back in 2022 in the double

00:19:02 --> 00:19:06 asteroid redirection test uh a really

00:19:06 --> 00:19:08 well put together experiment by NASA

00:19:08 --> 00:19:12 which uh succeeded in changing the orbit

00:19:12 --> 00:19:15 of a little world called Dorphos uh and

00:19:15 --> 00:19:17 that's great news because we know that

00:19:17 --> 00:19:19 it's now possible to do that. And just

00:19:19 --> 00:19:22 as a postcript to this story, um, ISSA

00:19:22 --> 00:19:25 currently has a spacecraft called HIA, H

00:19:25 --> 00:19:29 E R A on its way to Dorphos to check out

00:19:29 --> 00:19:32 what the result of that impact was. It's

00:19:32 --> 00:19:34 going to study that little world, look

00:19:34 --> 00:19:37 at the debris that was raised by the

00:19:37 --> 00:19:39 impact, uh, get a much better idea of

00:19:39 --> 00:19:41 whether it's a it really is just a

00:19:41 --> 00:19:43 rubble pile, which we think it probably

00:19:43 --> 00:19:46 is, and just, uh, learn more about what

00:19:46 --> 00:19:50 an impact by uh, a spacecraft does to an

00:19:50 --> 00:19:52 asteroid because that's the key thing.

00:19:52 --> 00:19:54 If we're going to have to save ourselves

00:19:54 --> 00:19:56 one day by doing this, we want to know

00:19:56 --> 00:19:58 as much about it as possible. And if I

00:19:58 --> 00:20:00 remember rightly, here will reach

00:20:00 --> 00:20:02 Dimorphus. I think it's late next year.

00:20:02 --> 00:20:03 I think it's towards the end of next

00:20:03 --> 00:20:04 year.

00:20:04 --> 00:20:07 >> Very exciting. Yeah. Nice to get a

00:20:07 --> 00:20:09 follow-up on that story, too. Yeah. Um

00:20:09 --> 00:20:12 and of course this is not the end of

00:20:12 --> 00:20:14 finding these kinds of things cuz uh the

00:20:14 --> 00:20:18 Vera C Rubin Observatory in Chile is

00:20:18 --> 00:20:20 it's it's not its primary role but it

00:20:20 --> 00:20:24 will be looking for other um near-Earth

00:20:24 --> 00:20:27 objects and they expect it to find tens

00:20:27 --> 00:20:28 of thousands of them.

00:20:28 --> 00:20:30 >> Absolutely. That's right. By this time

00:20:30 --> 00:20:32 next year we might be talking about

00:20:32 --> 00:20:35 80 or 100 nearear asteroids

00:20:35 --> 00:20:37 discovered. And of course again that's a

00:20:37 --> 00:20:39 good news story because as soon as you

00:20:39 --> 00:20:41 discover one of these things first thing

00:20:41 --> 00:20:43 you do is put its orbital elements into

00:20:43 --> 00:20:46 the computer grind away uh look at its

00:20:46 --> 00:20:49 trajectory in the future and that is all

00:20:49 --> 00:20:51 done automatically and if there is a

00:20:51 --> 00:20:53 need uh the system will raise alerts

00:20:53 --> 00:20:56 that there could be a collision uh in a

00:20:56 --> 00:20:58 certain window in the future. So um that

00:20:58 --> 00:21:01 whole process is really part of

00:21:01 --> 00:21:02 planetary defense. It's what's

00:21:02 --> 00:21:03 safeguarding us from the asteroid

00:21:03 --> 00:21:04 hazard.

00:21:04 --> 00:21:08 >> Yeah. Yeah. Um I I read a story the

00:21:08 --> 00:21:11 other day. I think Vera C. Rubin um had

00:21:11 --> 00:21:13 had it took its first picture, first

00:21:13 --> 00:21:15 light or I think they refer to it as in

00:21:15 --> 00:21:17 was it June or July this year?

00:21:17 --> 00:21:19 >> It was Yeah, I think it's about Yeah.

00:21:19 --> 00:21:22 >> Yeah. Uh so we almost at the pointy end

00:21:22 --> 00:21:25 of that um that observatory kicking into

00:21:25 --> 00:21:25 action.

00:21:25 --> 00:21:27 >> That's right. If I remember rightly, I

00:21:27 --> 00:21:28 might have these figures slightly wrong,

00:21:28 --> 00:21:29 but it was something like was it a

00:21:30 --> 00:21:32 10-hour set of observations they took

00:21:32 --> 00:21:33 and they discovered more than a thousand

00:21:34 --> 00:21:36 asteroids. Yeah. Period. So, you know,

00:21:36 --> 00:21:37 imagine what it's going to be like. This

00:21:37 --> 00:21:40 thing looks at the entire southern sky

00:21:40 --> 00:21:41 every three nights.

00:21:42 --> 00:21:43 >> That's incredibly remarkable.

00:21:43 --> 00:21:44 >> Yeah. It's quite

00:21:44 --> 00:21:47 >> Yeah. Um like we we were so blessed to

00:21:47 --> 00:21:49 be able to get so much information out

00:21:49 --> 00:21:53 of um um Oh gosh, my brain's not working

00:21:53 --> 00:21:56 today. Um the other observatory, the one

00:21:56 --> 00:21:58 that's out on in the L2.

00:21:58 --> 00:22:00 >> Oh yeah, you you mean the James Webb

00:22:00 --> 00:22:00 telescope?

00:22:00 --> 00:22:02 >> James Webb. Gosh, why couldn't I think

00:22:02 --> 00:22:05 of that? But um working side by side

00:22:05 --> 00:22:07 with Ver Rubin, this is just going to

00:22:07 --> 00:22:09 open up a whole new

00:22:09 --> 00:22:12 >> Yep, that's right. List of new

00:22:12 --> 00:22:15 discoveries. Yeah. Yeah. Very exciting.

00:22:15 --> 00:22:17 >> Uh if you would like to read about those

00:22:17 --> 00:22:20 40 near-earth objects,

00:22:20 --> 00:22:22 if you really, you know, you can go to a

00:22:22 --> 00:22:24 horror movie instead. It probably much

00:22:24 --> 00:22:26 more fun. But um 40 near-earth

00:22:26 --> 00:22:28 objects, you can do that through the

00:22:28 --> 00:22:33 European Space Agency website.

00:22:33 --> 00:22:35 Okay, we checked all four systems and

00:22:36 --> 00:22:37 >> space nets.

00:22:37 --> 00:22:38 >> Now, this this is a story that really

00:22:38 --> 00:22:41 excites me because um we've talked about

00:22:41 --> 00:22:45 this so many times, but um this this

00:22:45 --> 00:22:48 story I saw pop up last weekend and we

00:22:48 --> 00:22:51 we have been talking so much about the

00:22:51 --> 00:22:54 potential for life elsewhere. haven't

00:22:54 --> 00:22:56 found it yet, but the signs are starting

00:22:56 --> 00:22:59 to build, particularly within our own

00:22:59 --> 00:23:03 solar system. And this particular story

00:23:03 --> 00:23:07 is is one again where we have taken a

00:23:07 --> 00:23:10 bit of old data and reanalyzed it. And

00:23:10 --> 00:23:13 this involves the Cassini uh mission uh

00:23:14 --> 00:23:17 which has been taking samples of the

00:23:17 --> 00:23:21 eruptions from Enceladus. And what

00:23:21 --> 00:23:24 they've discovered is very very uh

00:23:24 --> 00:23:25 exciting.

00:23:25 --> 00:23:28 >> It is. Uh that's right. And uh yes,

00:23:28 --> 00:23:30 Cassini, you know, uh it was active if

00:23:30 --> 00:23:33 if I remember rightly between

00:23:33 --> 00:23:35


00:23:35 --> 00:23:39 I think was it 2004? Yes. And 2017. So

00:23:39 --> 00:23:41 that was the period when Cassini was

00:23:41 --> 00:23:43 collecting its data. And as you've just

00:23:43 --> 00:23:46 said, we're still learning things from

00:23:46 --> 00:23:49 those data. Uh, and in particular, what

00:23:49 --> 00:23:52 has been identified is some previously

00:23:52 --> 00:23:56 unknown organic chemicals in the ice

00:23:56 --> 00:23:59 grains that Cassini flew through, which

00:23:59 --> 00:24:02 are erupting, as you said, from the ice

00:24:02 --> 00:24:05 geysers in near the southern uh pole,

00:24:05 --> 00:24:07 the south pole of Enteladus, that little

00:24:08 --> 00:24:11 500 kilometer diameter world, which is

00:24:11 --> 00:24:13 one of Saturn's moons with the structure

00:24:13 --> 00:24:15 that we think is fairly common out in

00:24:15 --> 00:24:18 that part of the solar system, a rocky

00:24:18 --> 00:24:21 body overlay with a liquid ocean with

00:24:21 --> 00:24:23 ice on top of that. And the pressure of

00:24:23 --> 00:24:24 the ice is what's keeping that ocean

00:24:24 --> 00:24:27 liquid along with the the squeezing and

00:24:27 --> 00:24:29 squashing of the of the rocky part of

00:24:29 --> 00:24:32 the the body by the tidal forces exerted

00:24:32 --> 00:24:35 by the giant planet Saturn uh next door.

00:24:35 --> 00:24:37 And Saturn, by the way, um we've just

00:24:37 --> 00:24:39 gone through its ring plane. So Saturn,

00:24:39 --> 00:24:40 if you looked at Saturn through a

00:24:40 --> 00:24:43 telescope tonight or anytime within the

00:24:43 --> 00:24:44 next couple of weeks, you won't see any

00:24:44 --> 00:24:45 sign of the rings because we're they're

00:24:46 --> 00:24:46 edge onto us.

00:24:46 --> 00:24:47 >> Oh, okay.

00:24:47 --> 00:24:51 >> Y just a little aside there. Um so what

00:24:51 --> 00:24:55 uh what has happened is that uh we've

00:24:55 --> 00:24:58 we've known about these organic

00:24:58 --> 00:25:02 chemicals in ice grains which we we know

00:25:02 --> 00:25:04 come from Enceladus because they

00:25:04 --> 00:25:07 actually feed into the outer ring of

00:25:07 --> 00:25:09 Saturn something called the E-ring which

00:25:09 --> 00:25:12 is a very diffuse ring and we know that

00:25:12 --> 00:25:14 the material in that ring the ice

00:25:14 --> 00:25:16 crystals in that E-ring actually come

00:25:16 --> 00:25:19 from the south pole of of Enceladus.

00:25:19 --> 00:25:22 And those have been well analyzed um by

00:25:22 --> 00:25:26 Cassini and also by other observations.

00:25:26 --> 00:25:27 And so it was known that there were

00:25:27 --> 00:25:31 organics in there. But the question was

00:25:31 --> 00:25:34 these ice crystals may have been in

00:25:34 --> 00:25:35 orbit. They may have been in space for

00:25:35 --> 00:25:39 centuries. And so their chemical

00:25:39 --> 00:25:43 structure might well have been modified

00:25:43 --> 00:25:44 first of all by the the sun's

00:25:44 --> 00:25:47 ultraviolet radiation which tends to

00:25:47 --> 00:25:50 change chemistry. uh and the the solar

00:25:50 --> 00:25:51 wind, the wind of subatomic particles

00:25:52 --> 00:25:54 that comes from the sun that too can

00:25:54 --> 00:25:57 change the chemistry of particles uh

00:25:57 --> 00:26:00 grains of you know of of of ice with

00:26:00 --> 00:26:03 their with their organics uh on them the

00:26:03 --> 00:26:05 organic chemicals uh it can change their

00:26:05 --> 00:26:07 chemistry and so there was always a

00:26:07 --> 00:26:10 question whether these quite complex

00:26:10 --> 00:26:13 organic chemicals that were identified

00:26:13 --> 00:26:17 uh in the E-ring uh whether they are

00:26:17 --> 00:26:19 telling knew that that's how

00:26:19 --> 00:26:21 [clears throat] the ice crystals were

00:26:21 --> 00:26:23 when they came when they were spat out

00:26:23 --> 00:26:26 from Cassini's south pole. Um, it puts

00:26:26 --> 00:26:29 doubt on it. And so what this new

00:26:29 --> 00:26:32 analysis does is looks back to one of

00:26:32 --> 00:26:36 the flythroughs of uh Cassini through

00:26:36 --> 00:26:40 the ice plumes back in 2008.

00:26:40 --> 00:26:42 uh Cassini flew through the plume at

00:26:42 --> 00:26:45 about um 18 kilometers/s

00:26:45 --> 00:26:47 at a height of about 20 kilometers above

00:26:47 --> 00:26:51 the surface of Cassini. And so the the

00:26:51 --> 00:26:54 ice crystals that it passed through um

00:26:54 --> 00:26:57 only a few minutes earlier were actually

00:26:57 --> 00:27:01 water in the ocean of Enceladus. So

00:27:01 --> 00:27:04 these are fresh crystals of ice straight

00:27:04 --> 00:27:06 from the ocean. In other words, they,

00:27:06 --> 00:27:07 you know, they're effectively samples of

00:27:07 --> 00:27:10 the ocean water. And what they've

00:27:10 --> 00:27:12 succeeded in showing, uh, what the

00:27:12 --> 00:27:13 scientists who have done this succeeded

00:27:13 --> 00:27:16 in showing is that the chemistry is

00:27:16 --> 00:27:18 still there. The the organic, the

00:27:18 --> 00:27:22 complex organics are there in this fresh

00:27:22 --> 00:27:24 ocean spray, as they call it. I love

00:27:24 --> 00:27:26 that idea. It's an ocean spray, but it's

00:27:26 --> 00:27:30 ice crystals. And there's a whole you

00:27:30 --> 00:27:33 know a whole list of um things like

00:27:33 --> 00:27:36 esters, aromatics, hetereroatombearing

00:27:36 --> 00:27:39 organics. These are chemical terms that

00:27:39 --> 00:27:41 um I'm not that familiar with because

00:27:41 --> 00:27:44 chemistry was not my strong point. Uh

00:27:44 --> 00:27:47 but these chemicals are yes they are

00:27:47 --> 00:27:50 there in the ocean of Enceladus. Uh and

00:27:50 --> 00:27:53 what that has done is raised again the

00:27:53 --> 00:27:55 possibility that living organisms might

00:27:55 --> 00:27:58 exist in that ocean. uh and that because

00:27:58 --> 00:28:00 these chemicals are as we keep on saying

00:28:00 --> 00:28:03 the building blocks of life. Uh so just

00:28:04 --> 00:28:05 maybe there's something swimming around

00:28:05 --> 00:28:07 in the ocean of Enceladus that we are

00:28:07 --> 00:28:09 yet to discover.

00:28:09 --> 00:28:11 >> Yes. And wouldn't it be exciting? And uh

00:28:11 --> 00:28:13 hopefully in the not too distant future

00:28:13 --> 00:28:17 we'll be able to confirm it. Um I think

00:28:17 --> 00:28:18 people are starting to get very

00:28:18 --> 00:28:20 confident about the possibility though.

00:28:20 --> 00:28:20 >> Yeah. Yep.

00:28:20 --> 00:28:21 >> Yeah, that's right.

00:28:21 --> 00:28:24 >> So um fingers crossed. But uh yeah, the

00:28:24 --> 00:28:25 signs are starting to really build and I

00:28:25 --> 00:28:28 I even though it'll be probably one of

00:28:28 --> 00:28:31 the most exciting things ever discovered

00:28:31 --> 00:28:33 should we succeed in finding evidence of

00:28:33 --> 00:28:36 life elsewhere, we also probably

00:28:36 --> 00:28:40 shouldn't be surprised because water we

00:28:40 --> 00:28:42 now is know prolific throughout the

00:28:42 --> 00:28:43 universe.

00:28:43 --> 00:28:47 >> We know there are probably exoplanets

00:28:47 --> 00:28:49 orbiting almost every star in the

00:28:49 --> 00:28:51 universe. stands to reason that

00:28:51 --> 00:28:54 somewhere somewhere out there there's

00:28:54 --> 00:28:56 there's got to be some form of life.

00:28:56 --> 00:28:59 Even if it's only microbial, but

00:28:59 --> 00:29:01 >> or krill.

00:29:01 --> 00:29:04 >> Krill would be exciting. Green slime is

00:29:04 --> 00:29:06 what we're likely to find. I think

00:29:06 --> 00:29:08 >> green slime. Green slime will do.

00:29:08 --> 00:29:10 >> Green. Green slime would do it. That's

00:29:10 --> 00:29:11 right. It would indeed.

00:29:11 --> 00:29:13 >> Indeed. If you'd like to read up on that

00:29:13 --> 00:29:16 story about the latest from Enceladus,

00:29:16 --> 00:29:18 you can find it in the journal Nature

00:29:18 --> 00:29:22 Astronomy

00:29:22 --> 00:29:25 Space Nuts. One last story in this

00:29:25 --> 00:29:27 episode, Fred, and it's a bit of an

00:29:27 --> 00:29:30 update on three Atlas, the exo comet

00:29:30 --> 00:29:34 that is currently uh doing its thing.

00:29:34 --> 00:29:36 It's doing whatever it wants really. Uh

00:29:36 --> 00:29:39 but um it it's uh it's it's sort of

00:29:39 --> 00:29:41 reappeared and they're getting some

00:29:41 --> 00:29:42 great pictures of it, not only from

00:29:42 --> 00:29:47 Earth, but from Mars. And um some of

00:29:47 --> 00:29:49 these photos are extraordinary.

00:29:49 --> 00:29:51 Yes, they are. They're when you look at

00:29:51 --> 00:29:53 them, they're a little bit underwhelming

00:29:53 --> 00:29:54 until you realize that they've they've

00:29:54 --> 00:29:57 been taken by telescopes, not on Earth,

00:29:57 --> 00:29:59 but um in one case on the surface of

00:29:59 --> 00:30:04 Mars, but but also from Mars orbit. Uh

00:30:04 --> 00:30:06 and there's a little bit of a story to

00:30:06 --> 00:30:09 this because these images were taken um

00:30:09 --> 00:30:13 when uh the interstellar comet Three

00:30:13 --> 00:30:18 Atlas uh made its closest passage next

00:30:18 --> 00:30:20 close closest flyby of Mars basically uh

00:30:20 --> 00:30:23 30 million kilometers of Mars. That's

00:30:23 --> 00:30:25 quite a close approach compared with the

00:30:25 --> 00:30:28 distances that we we are from from it on

00:30:28 --> 00:30:31 Earth. Uh and that took place actually

00:30:31 --> 00:30:34 nearly two months ago. uh in early

00:30:34 --> 00:30:36 October. Um but what's held up the

00:30:36 --> 00:30:40 release of the uh of the images is the

00:30:40 --> 00:30:43 um US government shutdown which

00:30:43 --> 00:30:47 prevented these images being the world.

00:30:47 --> 00:30:49 >> Spoke about that at length

00:30:49 --> 00:30:51 previous episode. So yeah, I think

00:30:51 --> 00:30:53 pretty we're pretty well squared away on

00:30:53 --> 00:30:56 the issue. Um but he had colleagues that

00:30:56 --> 00:30:59 were so badly affected by that because

00:30:59 --> 00:31:02 >> the um you know well basically no income

00:31:02 --> 00:31:04 for as long as the shutdown existed.

00:31:04 --> 00:31:07 It's very very difficult situation but

00:31:07 --> 00:31:09 >> yes so we we we know why NASA couldn't

00:31:09 --> 00:31:11 do anything at the time.

00:31:11 --> 00:31:15 >> Yeah. So so that's right. So um but we

00:31:15 --> 00:31:17 now have these images revealed now that

00:31:17 --> 00:31:19 things are up and running again. And it

00:31:19 --> 00:31:22 perhaps the the best one has come from

00:31:22 --> 00:31:26 the um high-rise camera on board Mars

00:31:26 --> 00:31:28 Reconnaissance Orbiter. Uh and that's

00:31:28 --> 00:31:32 quite a detailed image of comet 3i Atlas

00:31:32 --> 00:31:35 with its a short tail and its coma.

00:31:35 --> 00:31:37 That's the region around the nucleus

00:31:37 --> 00:31:41 where material is outgassing and and

00:31:41 --> 00:31:44 shining because of exitation by the sun.

00:31:44 --> 00:31:47 Um the there there's some interesting

00:31:47 --> 00:31:51 images from uh from the Maven uh

00:31:51 --> 00:31:54 spacecraft as well which uh has cameras

00:31:54 --> 00:31:56 on looking in the ultraviolet and in

00:31:56 --> 00:31:57 fact it's got a spectrometer on that

00:31:57 --> 00:32:00 allows you to uh split the light up into

00:32:00 --> 00:32:03 its component colors. Uh so we see the

00:32:03 --> 00:32:06 glow of hydrogen actually from uh from

00:32:06 --> 00:32:09 three Atlas uh photographed by the Maven

00:32:09 --> 00:32:12 spectra uh spec spacecraft cameras and

00:32:12 --> 00:32:17 the mast cam uh camera on the uh it's

00:32:17 --> 00:32:20 mass cam zed it's called on perseverance

00:32:20 --> 00:32:22 on the surface of Mars actually managed

00:32:22 --> 00:32:26 to capture a very very faint image uh of

00:32:26 --> 00:32:28 uh of three eye atlas against a

00:32:28 --> 00:32:30 background of stars. It's faint because

00:32:30 --> 00:32:33 that cam, mass cam, was never designed

00:32:33 --> 00:32:36 to do astronomy. It's all designed to

00:32:36 --> 00:32:38 navigate on the surface of Mars, but yet

00:32:38 --> 00:32:41 it's managed to catch a picture uh by

00:32:41 --> 00:32:43 being pointed upwards obviously uh at um

00:32:43 --> 00:32:46 at this celestial visitor. So the the

00:32:46 --> 00:32:47 hope is that as these images are

00:32:48 --> 00:32:50 analyzed, Andrew, we'll find out more

00:32:50 --> 00:32:53 about threei Atlas, maybe even to get a

00:32:53 --> 00:32:55 good measurement of how big its nucleus

00:32:55 --> 00:32:57 is, the the icy component that gives

00:32:57 --> 00:33:01 rise to all this all this luminosity. Um

00:33:01 --> 00:33:03 the last I heard was that the thinking

00:33:03 --> 00:33:05 was it was in the region of 20

00:33:05 --> 00:33:06 kilometers across, which is large for a

00:33:06 --> 00:33:09 comet nucleus. Uh but I think the jury

00:33:09 --> 00:33:11 is probably still out on that. Um might

00:33:11 --> 00:33:13 find more from these measurements. So,

00:33:13 --> 00:33:16 how much longer will ThreeI Atlas be in

00:33:16 --> 00:33:18 our vicinity?

00:33:18 --> 00:33:21 >> Uh, no, no, quite a while. Uh, it's not,

00:33:21 --> 00:33:24 you know, it's it's it's um I think it

00:33:24 --> 00:33:27 passes closest to Earth this month if I

00:33:27 --> 00:33:29 remember rightly. Um, and then we'll be

00:33:29 --> 00:33:32 receding. Uh, it has passed its closest

00:33:32 --> 00:33:34 to the sun and so it it certainly

00:33:34 --> 00:33:35 brightened up when it did that, which is

00:33:35 --> 00:33:38 what you expect. uh as it as it leaves

00:33:38 --> 00:33:40 the solar system, we'll continue to

00:33:40 --> 00:33:42 track it with the world's big

00:33:42 --> 00:33:44 telescopes. Probably the James Web will

00:33:44 --> 00:33:46 have a few more looks at it. Uh and so

00:33:46 --> 00:33:48 um I think we're we're going to be

00:33:48 --> 00:33:51 observing it for several months yet.

00:33:51 --> 00:33:52 >> Very good. All right. Yeah, it keeps

00:33:52 --> 00:33:55 making the news and uh I mean it's it's

00:33:55 --> 00:33:58 one of those things like this it's only

00:33:58 --> 00:34:00 one of a handful of these things that

00:34:00 --> 00:34:03 we've we've found, but it's starting to

00:34:03 --> 00:34:04 look like this is not an uncommon

00:34:04 --> 00:34:05 thread.

00:34:06 --> 00:34:08 That's right. And I think once again

00:34:08 --> 00:34:10 harking back to the Ver Rubin telescope,

00:34:10 --> 00:34:12 we're going to find more of these uh

00:34:12 --> 00:34:14 when that telescope comes online. We're

00:34:14 --> 00:34:15 probably going to have, you know, we've

00:34:15 --> 00:34:17 got three known interstellar objects

00:34:18 --> 00:34:20 now. It'll probably be 20 by middle of

00:34:20 --> 00:34:23 next year. Who knows? It'll be quite

00:34:23 --> 00:34:24 extraordinary

00:34:24 --> 00:34:26 >> indeed. All right. Uh you can read more

00:34:26 --> 00:34:29 about the uh the images that have been

00:34:29 --> 00:34:30 taken of three Atlas and you can see

00:34:30 --> 00:34:34 them too at the univertoday.com

00:34:34 --> 00:34:37 website. Uh Fred, that brings us to the

00:34:37 --> 00:34:39 end. Thank you so much.

00:34:39 --> 00:34:42 >> It's been a pleasure, Andrew. I amum uh

00:34:42 --> 00:34:44 I've forgotten how much I miss uh my

00:34:44 --> 00:34:46 weekly dose of space knots. So it's good

00:34:46 --> 00:34:48 to be talking again.

00:34:48 --> 00:34:49 >> It's good to have you back. Thank you

00:34:49 --> 00:34:52 for Thank you for deciding to return.

00:34:52 --> 00:34:53 >> [laughter]

00:34:53 --> 00:34:53 >> Yes,

00:34:53 --> 00:34:56 >> even without the red carpet. Oh, and by

00:34:56 --> 00:34:57 the way, that golfer I played with

00:34:57 --> 00:34:59 today, Piper Stubs from Melbourne, Piper

00:35:00 --> 00:35:01 Stubs. Look up her name.

00:35:01 --> 00:35:05 >> She uh she studied um at college in the

00:35:05 --> 00:35:06 United States and played collegiate golf

00:35:06 --> 00:35:07 over there.

00:35:07 --> 00:35:08 >> Very good.

00:35:08 --> 00:35:10 >> Uh she's finished now and she um

00:35:10 --> 00:35:14 qualified as a in political science. So,

00:35:14 --> 00:35:18 >> yeah. Uh quite a bright young lady. Uh,

00:35:18 --> 00:35:20 and um, thanks to Hugh in the studio,

00:35:20 --> 00:35:21 although he couldn't be with us today

00:35:21 --> 00:35:23 because he heard there were 40 near

00:35:23 --> 00:35:25 Earth asteroids discovered, so he built

00:35:25 --> 00:35:29 himself a bunker. He won't come out. And

00:35:29 --> 00:35:30 um,

00:35:30 --> 00:35:33 and by the way, uh, if you would like to

00:35:33 --> 00:35:35 become a patron, uh, by all means, jump

00:35:35 --> 00:35:38 on our website and and, uh, find out all

00:35:38 --> 00:35:40 about it. Uh, I know it's there are

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00:35:42 --> 00:35:45 expect you to, um, to to spend money to

00:35:45 --> 00:35:47 listen to us. It's a it's a free

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00:36:12 --> 00:36:14 not, just forget everything I just said.

00:36:14 --> 00:36:16 Uh and don't forget to visit us online

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00:36:22 --> 00:36:24 talk to each other about anything you

00:36:24 --> 00:36:27 like to do with space and astronomy.

00:36:27 --> 00:36:28 That's it for this episode. Join us

00:36:28 --> 00:36:31 again soon when we do a Q&A episode. Um

00:36:32 --> 00:36:34 and and looking forward to having you

00:36:34 --> 00:36:36 join us then from me, Andrew Dunley.

00:36:36 --> 00:36:38 Until next time, bye-bye.

00:36:38 --> 00:36:41 >> Space. You'll be listening to the Space

00:36:41 --> 00:36:43 Nuts podcast

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