Rocket Lab’s Hungry Hippos Arrive!| NASA Enlists Global Volunteers for Artemis II
Space News TodayJanuary 25, 202600:17:3916.16 MB

Rocket Lab’s Hungry Hippos Arrive!| NASA Enlists Global Volunteers for Artemis II

Rocket Lab's "Hungry Hippos" arrive at Wallops Island despite tank test setback, NASA enlists global volunteers to track Artemis II, ancient lunar impact explains Moon's asymmetry, affordable space memorials launching in 2027, massive exomoon challenges definitions, and an 11th-century monk may have discovered Halley's Comet first.

EPISODE HIGHLIGHTS:

🚀 Rocket Lab's Neutron program reaches major milestone as innovative "Hungry Hippo" reusable fairings arrive at Wallops Island after month-long sea journey from New Zealand, though first-stage tank ruptures during qualification testing at Maryland facility

🌕 NASA selects 34 volunteers from 14 countries to track Artemis II mission around the Moon, expanding from 10 participants during Artemis I and representing government agencies, commercial companies, universities, and amateur radio enthusiasts

🌑 China's Chang'e 6 lunar samples reveal unusual potassium isotope ratios in South Pole-Aitken Basin rocks, providing evidence that the giant impact 4.2 billion years ago fundamentally altered the Moon's chemistry and explains why the far side has so few maria

⭐ Space Beyond startup plans to send 1,000 people's ashes to orbit for just $249 using CubeSat technology on SpaceX rideshare mission in October 2027, founded by former Blue Origin engineer Ryan Mitchell

🪐 Astronomers detect potential exomoon around HD 206893 B that may be 40% the mass of Jupiter, so massive it could force redefinition of what constitutes a moon versus binary companion system

☄️ New research reveals 11th-century English monk Eilmer of Malmesbury recognized Halley's Comet's periodicity centuries before Edmond Halley, calling into question the comet's namesake

LINKS & RESOURCES:

• Rocket Lab Neutron development: https://www.nasaspaceflight.com/2026/01/hungry-hippos-test-tanks-neutron/

• NASA Artemis II tracking participants: https://www.nasa.gov/technology/space-comms/nasa-selects-participants-to-track-artemis-ii-mission/

• Chang'e 6 lunar impact study: https://www.space.com/astronomy/moon/a-colossal-asteroid-may-have-warped-the-moon-from-the-inside-out

• Space Beyond memorial service: https://techcrunch.com/2026/01/23/this-startup-will-send-1000-peoples-ashes-to-space-affordably-in-2027/

• Massive exomoon discovery: https://dailygalaxy.com/2026/01/alien-moon-massive-redefine-what-a-moon-is/

• Halley's Comet historical research: https://phys.org/news/2026-01-halley-comet-wrongly-11th-century.html

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Kind: captions Language: en
00:00:00 --> 00:00:03 Welcome to Astronomy Daily, your source

00:00:03 --> 00:00:06 for the latest space and astronomy news.

00:00:06 --> 00:00:07 I'm Anna.

00:00:07 --> 00:00:09 >> And I'm Avery. Thanks for joining us on

00:00:09 --> 00:00:13 this Saturday, January 24th, 2026.

00:00:13 --> 00:00:16 We've got some fantastic stories lined

00:00:16 --> 00:00:17 up for you today.

00:00:17 --> 00:00:20 >> We certainly do. From rocket development

00:00:20 --> 00:00:22 milestones to prehistoric lunar

00:00:22 --> 00:00:25 discoveries, today's episode is packed

00:00:25 --> 00:00:28 with celestial intrigue. Let's dive

00:00:28 --> 00:00:31 right in with our top story. Rocket

00:00:31 --> 00:00:34 Lab's ambitious Neutron rocket has hit a

00:00:34 --> 00:00:36 significant milestone even though it

00:00:36 --> 00:00:38 came with a bit of a bump in the road.

00:00:38 --> 00:00:40 Anna, what's the latest from Wallops

00:00:40 --> 00:00:43 Island? Well, Avery, it's a story of

00:00:43 --> 00:00:46 both triumph and setback. The good news

00:00:46 --> 00:00:49 first, Rocket Lab's innovative hungry

00:00:49 --> 00:00:52 hippo fairings have successfully arrived

00:00:52 --> 00:00:54 at Wallops Island, Virginia after a

00:00:54 --> 00:00:57 month-long sea journey from New Zealand.

00:00:57 --> 00:00:59 aboard the vessel Northstar Integrity.

00:01:00 --> 00:01:02 These aren't your typical payload

00:01:02 --> 00:01:04 fairings. They're part of Neutron's

00:01:04 --> 00:01:07 groundbreaking reusable system.

00:01:07 --> 00:01:09 >> Right. And what makes these hungry

00:01:09 --> 00:01:11 hippos so special?

00:01:11 --> 00:01:13 >> Great question. Unlike traditional

00:01:13 --> 00:01:15 fairings that are jettisoned and lost

00:01:15 --> 00:01:18 during flight, these clamshellike

00:01:18 --> 00:01:20 structures actually stay attached to the

00:01:20 --> 00:01:23 first stage as it returns home. They

00:01:23 --> 00:01:26 open to release the second stage and

00:01:26 --> 00:01:28 payload, then close back up for the ride

00:01:28 --> 00:01:31 home. It's a clever design that should

00:01:31 --> 00:01:33 help drive down launch costs through

00:01:33 --> 00:01:34 rapid reuse.

00:01:34 --> 00:01:37 >> That's fascinating engineering, but you

00:01:37 --> 00:01:38 mentioned a setback.

00:01:38 --> 00:01:41 >> Unfortunately, yes. While the fairings

00:01:41 --> 00:01:44 were making their journey, Rocket Lab

00:01:44 --> 00:01:46 experienced a tank rupture during

00:01:46 --> 00:01:48 qualification trials at their Middle

00:01:48 --> 00:01:51 River, Maryland facility. A first stage

00:01:51 --> 00:01:54 carbon composite tank failed during

00:01:54 --> 00:01:56 hydrostatic pressure testing. That's

00:01:56 --> 00:01:58 where they fill the structure with water

00:01:58 --> 00:02:01 and gradually increase pressure to

00:02:01 --> 00:02:04 verify it can handle operational loads.

00:02:04 --> 00:02:06 >> Ouch. How significant is that?

00:02:06 --> 00:02:09 >> Well, Rocket Lab was quick to emphasize

00:02:09 --> 00:02:11 that testing failures like this, while

00:02:12 --> 00:02:14 disappointing, are actually part of the

00:02:14 --> 00:02:16 rigorous development process for high

00:02:16 --> 00:02:19 performance rockets. They deliberately

00:02:19 --> 00:02:21 stress hardware to its limits and beyond

00:02:22 --> 00:02:24 to ensure reliability. The tank was

00:02:24 --> 00:02:27 found collapsed into a pile of debris.

00:02:27 --> 00:02:29 But the company maintains this is

00:02:29 --> 00:02:32 exactly why they test to find these

00:02:32 --> 00:02:34 issues on the ground rather than during

00:02:34 --> 00:02:35 flight.

00:02:35 --> 00:02:38 >> Silver lining thinking and the program

00:02:38 --> 00:02:39 moves forward.

00:02:39 --> 00:02:41 >> Absolutely. With the hungry hippo

00:02:41 --> 00:02:44 fairings now at Wallops, engineers can

00:02:44 --> 00:02:47 proceed with integration testing, fit

00:02:47 --> 00:02:49 checks, electrical interfaces, and

00:02:49 --> 00:02:52 eventually static fire preparations. The

00:02:52 --> 00:02:54 launch mount is already in place with

00:02:54 --> 00:02:57 the test stand ready for major testing

00:02:57 --> 00:02:59 with the rocket's second stage.

00:02:59 --> 00:03:01 >> Exciting times for commercial space

00:03:01 --> 00:03:04 flight. Now, speaking of major missions,

00:03:04 --> 00:03:06 NASA has some news about tracking the

00:03:06 --> 00:03:08 upcoming Artemis 2 mission, right?

00:03:08 --> 00:03:12 >> They do indeed. NASA has selected 34

00:03:12 --> 00:03:15 global volunteers from 14 different

00:03:15 --> 00:03:17 countries to track the Orion spacecraft

00:03:18 --> 00:03:20 during its journey around the moon. This

00:03:20 --> 00:03:22 is a significant expansion from the

00:03:22 --> 00:03:25 Aremis 1 mission which had only 10

00:03:25 --> 00:03:26 volunteers.

00:03:26 --> 00:03:28 >> So what exactly will these volunteers be

00:03:28 --> 00:03:29 doing?

00:03:29 --> 00:03:31 >> They'll be using their own equipment.

00:03:31 --> 00:03:33 Everything from established commercial

00:03:33 --> 00:03:36 service providers to university research

00:03:36 --> 00:03:39 facilities to individual amateur radio

00:03:39 --> 00:03:42 enthusiasts to passively track radio

00:03:42 --> 00:03:45 waves transmitted by Orion during its

00:03:45 --> 00:03:47 approximately 10day mission. We're

00:03:47 --> 00:03:50 talking about 47 ground assets spanning

00:03:50 --> 00:03:51 the globe.

00:03:51 --> 00:03:53 >> That's impressive international

00:03:53 --> 00:03:55 cooperation. Who made the cut?

00:03:55 --> 00:03:58 >> The list is quite diverse. Government

00:03:58 --> 00:04:00 agencies like the Canadian Space Agency

00:04:00 --> 00:04:04 and Germany's DLR are participating.

00:04:04 --> 00:04:06 Commercial companies include Goonhilly

00:04:06 --> 00:04:09 Earth Station in the UK, Kongsburg

00:04:09 --> 00:04:11 Satellite Services in Norway, and

00:04:11 --> 00:04:13 Intuitive Machines in Houston.

00:04:14 --> 00:04:16 Universities like UC Berkeley, the

00:04:16 --> 00:04:18 University of Pittsburgh, and even

00:04:18 --> 00:04:20 Morehead State University in Kentucky

00:04:20 --> 00:04:22 are involved.

00:04:22 --> 00:04:24 >> What about amateur radio operators?

00:04:24 --> 00:04:27 >> Oh, yes, they're well represented. We've

00:04:27 --> 00:04:29 got individuals like Chris Swire from

00:04:29 --> 00:04:32 South Dakota and Dan Slater from

00:04:32 --> 00:04:35 California. Amateur radio organizations

00:04:35 --> 00:04:37 from Argentina, Germany, the

00:04:37 --> 00:04:39 Netherlands, and France are also

00:04:39 --> 00:04:42 participating. It's truly a global

00:04:42 --> 00:04:43 effort.

00:04:43 --> 00:04:45 >> And this data they collect, what's NASA

00:04:45 --> 00:04:46 doing with it?

00:04:46 --> 00:04:48 >> The volunteers will submit their

00:04:48 --> 00:04:51 tracking data to NASA for analysis. This

00:04:51 --> 00:04:53 helps the agency assess the broader

00:04:53 --> 00:04:55 aerospace community's tracking

00:04:55 --> 00:04:57 capabilities and identify ways to

00:04:57 --> 00:04:59 augment future moon and Mars mission

00:04:59 --> 00:05:03 support. Kevin Coggins, NASA's deputy

00:05:03 --> 00:05:04 associate administrator for space

00:05:04 --> 00:05:07 communications and navigation, called it

00:05:07 --> 00:05:10 a real step toward SCAN's commercial

00:05:10 --> 00:05:11 first vision.

00:05:11 --> 00:05:13 >> Building that public private ecosystem

00:05:13 --> 00:05:15 for deep space exploration.

00:05:15 --> 00:05:19 >> Exactly. Now, let's shift gears to some

00:05:19 --> 00:05:21 groundbreaking lunar research.

00:05:21 --> 00:05:24 Scientists analyzing samples from

00:05:24 --> 00:05:26 China's Chonga 6 mission have made a

00:05:26 --> 00:05:29 discovery that helps explain one of the

00:05:29 --> 00:05:31 moon's most puzzling features,

00:05:31 --> 00:05:33 >> the asymmetry between the near and far

00:05:33 --> 00:05:34 sides.

00:05:34 --> 00:05:36 >> Precisely. You know how the near side of

00:05:36 --> 00:05:39 the moon has all those dark maria, those

00:05:39 --> 00:05:42 vast volcanic planes that formed the man

00:05:42 --> 00:05:44 in the moon pattern we're all familiar

00:05:44 --> 00:05:47 with? The far side has barely any.

00:05:47 --> 00:05:49 >> I've always found that fascinating. What

00:05:49 --> 00:05:50 did they discover?

00:05:50 --> 00:05:53 >> Tong A6 brought back samples from the

00:05:53 --> 00:05:55 south pole atkin basin, which is one of

00:05:55 --> 00:05:57 the largest impact features in the

00:05:57 --> 00:06:01 entire solar system, about 1 miles

00:06:01 --> 00:06:05 wide and between 4.2 2 and 4.3 billion

00:06:05 --> 00:06:07 years old. Much older than the lunar

00:06:07 --> 00:06:10 maria which are around 3.6 billion years

00:06:10 --> 00:06:11 old.

00:06:11 --> 00:06:12 >> And what did these ancient samples

00:06:12 --> 00:06:13 reveal?

00:06:13 --> 00:06:16 >> The research team led by Hang Ton from

00:06:16 --> 00:06:19 the Chinese Academy of Sciences found

00:06:19 --> 00:06:21 something unusual in the basaltic rock

00:06:21 --> 00:06:25 samples, an abnormal ratio of potassium

00:06:25 --> 00:06:27 isotopes. Specifically, they found more

00:06:27 --> 00:06:31 of the heavier potassium 41 relative to

00:06:31 --> 00:06:33 potassium 39 compared to samples from

00:06:33 --> 00:06:35 the near side.

00:06:35 --> 00:06:36 >> What would cause that?

00:06:36 --> 00:06:39 >> After exploring several possibilities,

00:06:39 --> 00:06:42 cosmic ray irradiation, magma processes,

00:06:42 --> 00:06:45 meteoritic contamination, they concluded

00:06:45 --> 00:06:48 that this isotopic signature is a relic

00:06:48 --> 00:06:50 of the giant impact that formed the

00:06:50 --> 00:06:53 south pole atkin basin itself. So the

00:06:54 --> 00:06:55 impact actually changed the moon's

00:06:55 --> 00:06:56 chemistry.

00:06:56 --> 00:06:59 >> Not just changed it, it fundamentally

00:06:59 --> 00:07:02 altered it. The impact was so violent

00:07:02 --> 00:07:04 that it heated the moon's crust and

00:07:04 --> 00:07:07 mantle intensely, causing many volatile

00:07:07 --> 00:07:09 elements, including potassium, to

00:07:09 --> 00:07:11 evaporate and escape into space. The

00:07:11 --> 00:07:15 lighter potassium 39 isotope evaporated

00:07:15 --> 00:07:17 more easily than the heavier one,

00:07:17 --> 00:07:20 leaving behind this unusual ratio.

00:07:20 --> 00:07:22 >> That's incredible detective work. And

00:07:22 --> 00:07:24 this explains the lack of maria on the

00:07:24 --> 00:07:25 far side.

00:07:25 --> 00:07:27 >> Exactly. The reduction in volatiles

00:07:27 --> 00:07:30 would have suppressed magma formation,

00:07:30 --> 00:07:32 limiting volcanism on the far side. It

00:07:32 --> 00:07:35 shows how deeply that ancient impact

00:07:35 --> 00:07:37 affected the moon's interior and why

00:07:37 --> 00:07:40 isotopic analysis can provide windows

00:07:40 --> 00:07:42 into the conditions of such catastrophic

00:07:42 --> 00:07:45 events. This research was published in

00:07:45 --> 00:07:47 the proceedings of the National Academy

00:07:47 --> 00:07:48 of Sciences.

00:07:48 --> 00:07:50 >> Fascinating stuff. Now, here's something

00:07:50 --> 00:07:52 a bit more down to earth, even if it's

00:07:52 --> 00:07:55 going to space. Anna, tell us about the

00:07:55 --> 00:07:57 startup that's making space memorials

00:07:57 --> 00:07:57 affordable.

00:07:58 --> 00:07:59 >> This is a really interesting story,

00:08:00 --> 00:08:03 Avery. A startup called Space Beyond,

00:08:03 --> 00:08:05 founded by Ryan Mitchell, is planning to

00:08:05 --> 00:08:08 send up to 1 people's ashes to space

00:08:08 --> 00:08:13 in October 2027 for as little as $249,

00:08:13 --> 00:08:15 dramatically cheaper than traditional

00:08:15 --> 00:08:17 space memorial services that typically

00:08:18 --> 00:08:20 cost thousands of dollars.

00:08:20 --> 00:08:21 >> That's quite a price difference. How are

00:08:21 --> 00:08:23 they pulling this off?

00:08:23 --> 00:08:25 >> It's all about smart use of existing

00:08:25 --> 00:08:28 infrastructure. They're using a Cubsat,

00:08:28 --> 00:08:30 one of those miniature cube- shaped

00:08:30 --> 00:08:32 satellites that will launch as a ride

00:08:32 --> 00:08:34 share payload on a SpaceX Falcon 9

00:08:34 --> 00:08:37 rocket. The ride share model has really

00:08:37 --> 00:08:39 democratized access to space.

00:08:39 --> 00:08:42 >> And Ryan Mitchell, he's got some serious

00:08:42 --> 00:08:43 space credentials. Right.

00:08:44 --> 00:08:46 >> Absolutely. He worked on NASA's space

00:08:46 --> 00:08:48 shuttle program and spent nearly a

00:08:48 --> 00:08:51 decade at Blue Origin. The idea actually

00:08:51 --> 00:08:53 came to him while attending a family

00:08:53 --> 00:08:55 member's ash spreading ceremony. He

00:08:55 --> 00:08:57 thought, "How could I do this better?"

00:08:57 --> 00:09:00 And thus, Space Beyond was born.

00:09:00 --> 00:09:02 >> But there must be some limitations with

00:09:02 --> 00:09:04 such an affordable service.

00:09:04 --> 00:09:07 >> There are customers can only send about

00:09:07 --> 00:09:10 1 g of ashes, a practical limit due to

00:09:10 --> 00:09:12 weight considerations and the need to

00:09:12 --> 00:09:15 fit many customers remains in the Cubat.

00:09:15 --> 00:09:17 The satellite will only orbit for about

00:09:17 --> 00:09:19 5 years before burning up in Earth's

00:09:19 --> 00:09:22 atmosphere. So, it's not forever. Though

00:09:22 --> 00:09:25 that fiery ending has a certain poetic

00:09:25 --> 00:09:26 quality to it.

00:09:26 --> 00:09:28 >> Mitchell certainly thinks so. Plus, the

00:09:28 --> 00:09:30 Cubat will be in a suns synchronous

00:09:30 --> 00:09:34 orbit at about 550 km altitude, meaning

00:09:34 --> 00:09:37 it'll fly over the entire globe. With

00:09:37 --> 00:09:39 modern spacecraft tracking services,

00:09:39 --> 00:09:41 families should be able to locate it and

00:09:41 --> 00:09:43 know when it's passing overhead.

00:09:44 --> 00:09:46 >> That's actually really touching. And

00:09:46 --> 00:09:48 importantly, they're not spreading the

00:09:48 --> 00:09:50 ashes in space. Right.

00:09:50 --> 00:09:52 >> Correct. Mitchell called that an almost

00:09:52 --> 00:09:54 nightmare scenario because the particles

00:09:54 --> 00:09:56 could create a debris cloud that could

00:09:56 --> 00:09:59 endanger other spacecraft. Since

00:09:59 --> 00:10:01 customers only send about a gram, they

00:10:01 --> 00:10:03 can do what they wish with the rest.

00:10:03 --> 00:10:05 >> Thoughtful approach to a sensitive

00:10:05 --> 00:10:07 service. Now, let's talk about something

00:10:07 --> 00:10:10 that might literally redefine astronomy.

00:10:10 --> 00:10:12 Anna, tell us about this massive

00:10:12 --> 00:10:14 potential exomoon.

00:10:14 --> 00:10:17 >> This one's mindbending, Avery.

00:10:17 --> 00:10:19 Astronomers using the gravity instrument

00:10:19 --> 00:10:21 on the Very Large Telescope in Chile

00:10:21 --> 00:10:24 have detected what might be an exomoon

00:10:24 --> 00:10:29 orbiting the gas giant HD206893b

00:10:29 --> 00:10:32 located 133 light years from Earth. But

00:10:32 --> 00:10:35 here's the kicker. This moon is so

00:10:35 --> 00:10:37 massive that it might force us to

00:10:37 --> 00:10:40 rethink the word moon even means.

00:10:40 --> 00:10:42 >> How massive are we talking?

00:10:42 --> 00:10:44 >> Get this. They estimate it could be as

00:10:44 --> 00:10:48 much as 40% the mass of Jupiter or about

00:10:48 --> 00:10:50 nine times the mass of Neptune. To put

00:10:50 --> 00:10:52 that in perspective, it's thousands of

00:10:52 --> 00:10:55 times heavier than any moon in our solar

00:10:55 --> 00:10:58 system. Anamine, Jupiter's largest moon

00:10:58 --> 00:11:00 and the biggest in our solar system, is

00:11:00 --> 00:11:02 thousands of times less massive than

00:11:02 --> 00:11:03 Neptune.

00:11:03 --> 00:11:05 >> Wow. So, how did they even detect

00:11:05 --> 00:11:07 something like this? Through a technique

00:11:08 --> 00:11:10 called astrometry, which precisely

00:11:10 --> 00:11:12 tracks the position of celestial bodies

00:11:12 --> 00:11:15 over time, the team led by Quentyn Crawl

00:11:15 --> 00:11:17 from the University of Cambridge

00:11:17 --> 00:11:20 observed a measurable wobble in HD

00:11:20 --> 00:11:22 206893b's

00:11:22 --> 00:11:25 motion, a back and forth movement with a

00:11:25 --> 00:11:27 period of about 9 months.

00:11:27 --> 00:11:29 >> And that wobble is the moon's

00:11:29 --> 00:11:30 gravitational tug.

00:11:30 --> 00:11:33 >> Exactly. PL explained that the wobble

00:11:33 --> 00:11:35 has a size comparable to the Earth moon

00:11:35 --> 00:11:38 distance, which is the exact signature

00:11:38 --> 00:11:40 you'd expect from an unseen companion.

00:11:40 --> 00:11:42 The potential moon's orbit is also

00:11:42 --> 00:11:46 tilted by roughly 60°, suggesting a

00:11:46 --> 00:11:48 turbulent history of gravitational

00:11:48 --> 00:11:49 interactions.

00:11:49 --> 00:11:51 >> So, at what point does something stop

00:11:51 --> 00:11:53 being a moon and become a binary

00:11:53 --> 00:11:54 companion?

00:11:54 --> 00:11:57 >> That's the milliondoll question. Crawl

00:11:57 --> 00:11:59 noted that at these masses, the

00:11:59 --> 00:12:01 distinction between a massive moon and a

00:12:01 --> 00:12:03 low mass companion becomes blurred.

00:12:03 --> 00:12:05 There's currently no official definition

00:12:06 --> 00:12:08 of an exomoon. So, astronomers generally

00:12:08 --> 00:12:11 refer to any object orbiting a planet as

00:12:11 --> 00:12:12 a moon.

00:12:12 --> 00:12:14 >> This could force a redefin

00:12:14 --> 00:12:17 >> potentially. Crawl suggested that as

00:12:17 --> 00:12:19 observational techniques improve, our

00:12:19 --> 00:12:21 definitions and understanding of what

00:12:21 --> 00:12:24 constitutes a moon will almost certainly

00:12:24 --> 00:12:26 evolve. He also pointed out that we're

00:12:26 --> 00:12:28 likely only seeing the tip of the

00:12:28 --> 00:12:31 iceberg. Just as the first exoplanets

00:12:31 --> 00:12:33 discovered were massive ones close to

00:12:33 --> 00:12:35 their stars because they were easiest to

00:12:35 --> 00:12:37 detect, the first exomoons we identify

00:12:37 --> 00:12:40 will be the most massive and extreme

00:12:40 --> 00:12:41 examples.

00:12:41 --> 00:12:44 >> Finding exomoons is challenging. I

00:12:44 --> 00:12:45 imagine

00:12:45 --> 00:12:47 >> extremely the signals they produce are

00:12:47 --> 00:12:50 minute, often lost in the noise of their

00:12:50 --> 00:12:53 parent planet's data. The transit method

00:12:53 --> 00:12:55 that's revolutionized exoplanet

00:12:55 --> 00:12:58 discovery is less effective for moons

00:12:58 --> 00:13:00 because they produce light dips too

00:13:00 --> 00:13:03 faint to distinguish. But astrometry

00:13:03 --> 00:13:05 offers a new path forward, especially

00:13:05 --> 00:13:08 for detecting companions in far orbits

00:13:08 --> 00:13:11 where large stable moons are more likely

00:13:11 --> 00:13:12 to exist.

00:13:12 --> 00:13:15 >> This research was published in astronomy

00:13:15 --> 00:13:17 and astrophysics. It's been accepted for

00:13:18 --> 00:13:19 publication there and it's currently

00:13:19 --> 00:13:21 available as a pre- peer-reviewed paper

00:13:22 --> 00:13:24 on archive. If confirmed, this would not

00:13:24 --> 00:13:27 only expand our catalog of celestial

00:13:27 --> 00:13:30 bodies, but force astronomers to rethink

00:13:30 --> 00:13:32 one of the oldest definitions in

00:13:32 --> 00:13:33 planetary science.

00:13:34 --> 00:13:36 >> Incredible. And finally, Anna, we have a

00:13:36 --> 00:13:39 story that might rewrite history or at

00:13:39 --> 00:13:41 least rename a famous comet.

00:13:41 --> 00:13:44 >> That's right. New research suggests that

00:13:44 --> 00:13:47 Haley's comet might be wrongly named.

00:13:47 --> 00:13:49 Turns out an 11th century English monk

00:13:49 --> 00:13:52 named Elmer of Malmsbury understood the

00:13:52 --> 00:13:55 comet's periodic nature centuries before

00:13:55 --> 00:13:58 the British astronomer Edmund Haley.

00:13:58 --> 00:14:00 >> Wait, so Halley wasn't the first to

00:14:00 --> 00:14:02 figure this out? According to research

00:14:02 --> 00:14:05 by professor Simon Portiges wart and

00:14:05 --> 00:14:07 colleagues published in the book

00:14:07 --> 00:14:10 Doristad and everything after Ilmer

00:14:10 --> 00:14:13 witnessed Haley's comet twice in 989 CE

00:14:14 --> 00:14:17 and again in 1066 CE and realized it was

00:14:17 --> 00:14:20 the same comet returning.

00:14:20 --> 00:14:21 >> How do we know this?

00:14:21 --> 00:14:23 >> The events are described by the 12th

00:14:23 --> 00:14:26 century chronicler William of Malssbury.

00:14:26 --> 00:14:28 But this connection had gone unnoticed

00:14:28 --> 00:14:31 by scholars until now. The 1066

00:14:32 --> 00:14:34 appearance is actually depicted on the

00:14:34 --> 00:14:36 famous Bayou tapestry which illustrates

00:14:36 --> 00:14:39 the events of that year including the

00:14:39 --> 00:14:41 Norman conquest of England.

00:14:41 --> 00:14:43 >> So Ilmer must have been quite elderly to

00:14:43 --> 00:14:45 see it twice.

00:14:45 --> 00:14:47 >> Exactly. Given that the comet appears

00:14:47 --> 00:14:50 roughly 76 years, he would have been

00:14:50 --> 00:14:52 advanced in age when he witnessed it for

00:14:52 --> 00:14:55 the second time. And here's a

00:14:55 --> 00:14:57 fascinating detail. As was customary at

00:14:58 --> 00:15:01 the time when he saw it in 1066, the

00:15:01 --> 00:15:04 king was warned of impending disaster.

00:15:04 --> 00:15:06 The comet appeared during the brief

00:15:06 --> 00:15:09 reign of King Harold Godwinson, who died

00:15:09 --> 00:15:12 at the Battle of Hastings that October.

00:15:12 --> 00:15:14 >> Medieval people really did see comets as

00:15:14 --> 00:15:16 omens, didn't they?

00:15:16 --> 00:15:18 >> They did indeed. The research shows that

00:15:18 --> 00:15:21 comet appearances around this time were

00:15:21 --> 00:15:23 consistently associated with the deaths

00:15:23 --> 00:15:26 of kings, war, or famine in the British

00:15:26 --> 00:15:28 Isles. The researchers even found what

00:15:28 --> 00:15:31 might be historical fake news. A comment

00:15:31 --> 00:15:33 supposedly seen before the death of

00:15:33 --> 00:15:36 Archbishop Cydrich of Canterbury in 995,

00:15:36 --> 00:15:38 which wasn't actually recorded in the

00:15:38 --> 00:15:41 Chronicles, possibly an exaggeration to

00:15:41 --> 00:15:42 frighten people.

00:15:42 --> 00:15:44 >> So, what are the researchers calling

00:15:44 --> 00:15:47 for? They're arguing that Haley's comet

00:15:47 --> 00:15:48 should be given a different name since

00:15:48 --> 00:15:50 it had been observed twice and its

00:15:50 --> 00:15:53 periodicity understood centuries before

00:15:53 --> 00:15:55 Haley's work. Portuge's wart mentioned

00:15:56 --> 00:15:58 that while the research was fun to do,

00:15:58 --> 00:16:00 it was challenging working in such an

00:16:00 --> 00:16:02 interdisciplinary project alongside a

00:16:02 --> 00:16:05 historian. Nevertheless, they plan to

00:16:05 --> 00:16:07 carry out further research into periodic

00:16:07 --> 00:16:08 comet.

00:16:08 --> 00:16:10 >> It's amazing how interdisciplinary

00:16:10 --> 00:16:12 research can uncover these historical

00:16:12 --> 00:16:15 oversightes. It really is. And it shows

00:16:15 --> 00:16:18 that scientific discovery isn't always

00:16:18 --> 00:16:20 about new observations. Sometimes it's

00:16:20 --> 00:16:23 about looking at old records with fresh

00:16:23 --> 00:16:25 eyes. Well, that's all the time we have

00:16:25 --> 00:16:27 for today's episode. What a journey

00:16:27 --> 00:16:29 we've been on. From rocket fairings to

00:16:29 --> 00:16:32 ancient lunar impacts, affordable space

00:16:32 --> 00:16:34 memorials to massive exomoons, and

00:16:34 --> 00:16:37 historical comet discoveries.

00:16:37 --> 00:16:39 >> It never ceases to amaze me how much is

00:16:39 --> 00:16:42 happening in space and astronomy every

00:16:42 --> 00:16:43 single day. From cutting edge

00:16:44 --> 00:16:45 engineering to billion-year-old

00:16:45 --> 00:16:47 mysteries, there's always something new

00:16:47 --> 00:16:48 to learn.

00:16:48 --> 00:16:50 >> Thanks so much for tuning in to

00:16:50 --> 00:16:52 Astronomy Daily. Be sure to visit our

00:16:52 --> 00:16:54 website at astronomydaily.io

00:16:54 --> 00:16:56 for detailed show notes, transcripts,

00:16:56 --> 00:16:58 and links to all the stories we

00:16:58 --> 00:16:59 discussed today.

00:16:59 --> 00:17:01 >> And don't forget to follow us on social

00:17:01 --> 00:17:04 media. We're @ astroailyaily pod on X,

00:17:04 --> 00:17:07 Facebook, Instagram, Tik Tok, YouTube,

00:17:07 --> 00:17:10 and Tumblr. Until next time, keep

00:17:10 --> 00:17:12 looking up and keep exploring the

00:17:12 --> 00:17:14 wonders of our universe.

00:17:14 --> 00:17:16 >> Clear skies everyone.

00:17:16 --> 00:17:19 >> Day

00:17:19 --> 00:17:22 stories told.