Spacewalks, Supernovas, and the Mysteries of Super Jupiters
Astronomy Daily: Space News December 10, 2025x
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Spacewalks, Supernovas, and the Mysteries of Super Jupiters

AnnaAnnaHost
### Episode Summary
A thrilling spacewalk at the Tiangong Space Station, the discovery of the oldest supernova witnessed by the James Webb Telescope, and new insights into the chaotic nature of Super Jupiters highlight today's episode. We also explore the powerful winds generated by a supermassive black hole, showcasing the dynamic interactions in our universe.
### Timestamps & Stories
01:05 – **Story 1: Marathon Spacewalk at Tiangong Space Station**
**Key Facts**
- Two astronauts from the Shenshou 21 mission conducted an 8-hour spacewalk to inspect damage on the Shenshou 20 return capsule, struck by space debris.
- Installation of new debris protection systems highlights the growing threat of space junk.
03:40 – **Story 2: Record Launches by China**
**Key Facts**
- China set a national record with three Long March rocket launches in under 19 hours.
- Missions included broadband satellite deployments and classified military satellites.
05:20 – **Story 3: Bold Recommendations for Mars Exploration**
**Key Facts**
- A new report emphasizes the search for life as the top priority for crewed Mars missions.
- Proposed campaigns focus on glacier ice and deep subsurface exploration for biosignatures.
07:00 – **Story 4: Oldest Supernova Detected by JWST**
**Key Facts**
- James Webb Telescope identifies a supernova from 13 billion years ago, just 730 million years post-Big Bang.
- This discovery provides insights into the early universe and the lifecycle of massive stars.
08:40 – **Story 5: Super Jupiters Challenge Our Understanding**
**Key Facts**
- Research on exoplanet VHS 1256 b reveals a chaotic atmosphere, differing significantly from Jupiter's stability.
- The study suggests massive gas giants may exhibit turbulent weather patterns instead of organized bands.
10:15 – **Story 6: Winds from a Supermassive Black Hole**
**Key Facts**
- A supermassive black hole in galaxy NGC 3783 emits powerful winds at 1/5 the speed of light, impacting galaxy evolution.
- Observations from XMM-Newton and XRISM telescopes reveal the connection between black holes and their host galaxies.

### Sources & Further Reading
1. NASA
2. European Space Agency
3. James Webb Space Telescope
4. Mars Exploration Program
5. NASA Black Hole Research

### Follow & Contact
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Instagram: @astrodailypod
Email: hello@astronomydaily.io
Website: astronomydaily.io
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This episode includes AI-generated content.


00:00:00 --> 00:00:03 Avery: Welcome to Astronomy Daily, the podcast that

00:00:03 --> 00:00:05 brings you the biggest news from across the

00:00:05 --> 00:00:06 cosmos. I'm Avery.

00:00:06 --> 00:00:08 Anna: And I'm Anna. It's great to be with you.

00:00:09 --> 00:00:11 Today we're talking about a dramatic

00:00:11 --> 00:00:14 spacewalk outside the Tiangong Space

00:00:14 --> 00:00:17 Station. Plus the James Webb Telescope spots

00:00:17 --> 00:00:20 the oldest supernova ever seen. And we'll

00:00:20 --> 00:00:22 find out why giant planets known as Super

00:00:22 --> 00:00:25 Jupiters might look nothing like our own

00:00:25 --> 00:00:25 Jupiter.

00:00:26 --> 00:00:28 Avery: And we'll finish with a black hole that's

00:00:28 --> 00:00:30 whipping up winds at a fraction of the speed

00:00:30 --> 00:00:30 of light.

00:00:30 --> 00:00:32 Let's get first up.

00:00:32 --> 00:00:35 Anna: Let's head to low Earth orbit. There's been

00:00:35 --> 00:00:37 some serious activity outside the Tiangong

00:00:37 --> 00:00:38 Space station.

00:00:38 --> 00:00:40 Avery: That's right. Two Chinese astronauts from the

00:00:40 --> 00:00:43 Shenshou 21 mission conducted a

00:00:43 --> 00:00:46 marathon eight hour spacewalk. The primary

00:00:46 --> 00:00:48 goal was to get a close look at the Shenshou

00:00:48 --> 00:00:49 20 return capsule.

00:00:50 --> 00:00:52 Anna: Mhm. And what they were looking for was

00:00:52 --> 00:00:53 damage, Right?

00:00:53 --> 00:00:56 Avery: Exactly. The capsule was likely struck by a

00:00:56 --> 00:00:58 piece of space junk, and the damage was

00:00:58 --> 00:01:01 serious enough that the Shenzhou 20 crew

00:01:01 --> 00:01:04 couldn't use it to return home. They had

00:01:04 --> 00:01:06 to come back to Earth on a different vehicle

00:01:06 --> 00:01:06 as a precaution.

00:01:07 --> 00:01:09 Anna: Wow. That really highlights the dangers of

00:01:09 --> 00:01:12 space debris. So this spacewalk was

00:01:12 --> 00:01:15 essentially a, ah, forensic investigation in

00:01:15 --> 00:01:15 orbit.

00:01:16 --> 00:01:18 Avery: It was. They were meticulously inspecting

00:01:18 --> 00:01:21 and photographing the damage to understand

00:01:21 --> 00:01:24 exactly what happened. But that wasn't all

00:01:24 --> 00:01:26 they did. They also took the opportunity to

00:01:26 --> 00:01:29 install new space debris protection systems

00:01:29 --> 00:01:30 on the station itself.

00:01:30 --> 00:01:33 Anna: Uh, a necessary upgrade, it seems. It's a

00:01:33 --> 00:01:36 growing problem that isn't going away. Every

00:01:36 --> 00:01:39 piece of junk, big or small, is a

00:01:39 --> 00:01:41 potential threat to current and future

00:01:41 --> 00:01:41 missions.

00:01:42 --> 00:01:44 Avery: And speaking of China's space program,

00:01:44 --> 00:01:46 they've been busy on the launch pad as well.

00:01:46 --> 00:01:48 Incredibly busy, in fact.

00:01:48 --> 00:01:51 Anna: You can say that again. They just set a new

00:01:51 --> 00:01:54 national record by launching three separate

00:01:54 --> 00:01:57 Long March rockets in less than 19

00:01:57 --> 00:01:57 hours.

00:01:58 --> 00:02:01 Avery: 19 hours, that's an astonishing pace.

00:02:01 --> 00:02:04 It brings their total for 20, 25 up to

00:02:04 --> 00:02:06 83 orbital launches already.

00:02:07 --> 00:02:09 Anna: So what were these missions carrying?

00:02:09 --> 00:02:11 Avery: A couple of different payloads. The launches

00:02:11 --> 00:02:14 deployed more broadband satellites for their

00:02:14 --> 00:02:17 Guang Mega Constellation, which is their

00:02:17 --> 00:02:19 competitor to systems like Starlink.

00:02:19 --> 00:02:19 Anna: Right.

00:02:20 --> 00:02:22 Avery: And they also sent up two classified military

00:02:22 --> 00:02:25 satellites. The details on those, as you'd

00:02:25 --> 00:02:26 expect, are pretty sparse.

00:02:27 --> 00:02:29 Anna: It just shows the sheer scale and speed of

00:02:29 --> 00:02:32 their operations. Right now they're not just

00:02:32 --> 00:02:34 launching frequently, they're launching with

00:02:34 --> 00:02:35 incredible efficiency.

00:02:36 --> 00:02:37 Avery: And, uh, they seem to be getting better at it

00:02:37 --> 00:02:38 with every launch.

00:02:39 --> 00:02:42 Anna: Okay, let's shift our focus from Earth orbit

00:02:42 --> 00:02:45 to the Red planet. A major new report from

00:02:45 --> 00:02:47 the U.S. national Academies of Sciences,

00:02:47 --> 00:02:50 Engineering and Medicine has just been

00:02:50 --> 00:02:52 released and it's making some bold

00:02:52 --> 00:02:54 recommendations for the future of Mars

00:02:54 --> 00:02:55 exploration.

00:02:56 --> 00:02:59 Avery: It really is. The headline recommendation is

00:02:59 --> 00:03:02 that the primary scientific objective for the

00:03:02 --> 00:03:04 first crewed missions to Mars should be the

00:03:04 --> 00:03:07 search for life, either past or present.

00:03:07 --> 00:03:10 Anna: That's a significant statement. For a long

00:03:10 --> 00:03:12 time, the focus has been on geology and

00:03:12 --> 00:03:15 paving the way for colonization. This report

00:03:15 --> 00:03:18 puts astrobiology front and center.

00:03:18 --> 00:03:21 Avery: Exactly. It outlines 11 specific

00:03:21 --> 00:03:23 science objectives and proposes two main

00:03:23 --> 00:03:26 science mission campaigns to achieve them.

00:03:26 --> 00:03:28 The the first campaign would target near.

00:03:28 --> 00:03:31 Anna: Surface glacier ice, which could preserve

00:03:31 --> 00:03:32 biosignatures.

00:03:32 --> 00:03:34 Avery: Precisely. The second, even more ambitious

00:03:34 --> 00:03:37 campaign would involve exploring the deep

00:03:37 --> 00:03:39 subsurface of Mars. They're talking about

00:03:39 --> 00:03:41 drilling deep down to where liquid water

00:03:41 --> 00:03:44 might still exist, Protected from the harsh

00:03:44 --> 00:03:44 surface radiation.

00:03:46 --> 00:03:48 Anna: That would be an incredible undertaking.

00:03:48 --> 00:03:51 The technical challenges alone are immense.

00:03:52 --> 00:03:54 But the potential payoff for finding evidence

00:03:54 --> 00:03:57 of life on another planet is arguably

00:03:57 --> 00:03:59 the greatest prize in science.

00:03:59 --> 00:04:02 Avery: It completely reframes the why of sending

00:04:02 --> 00:04:05 humans to Mars. It's not just about planting

00:04:05 --> 00:04:07 a flag. It's about answering one of

00:04:07 --> 00:04:08 humanity's biggest questions.

00:04:09 --> 00:04:11 Anna: It would be nice if we could get a definitive

00:04:11 --> 00:04:12 answer one day.

00:04:12 --> 00:04:15 Avery: Well, from the search for life to the death

00:04:15 --> 00:04:18 of stars, the James Webb Space Telescope has

00:04:18 --> 00:04:21 done it again. It's given us a glimpse into

00:04:21 --> 00:04:23 the cosmic dawn by finding the oldest

00:04:23 --> 00:04:24 supernova ever seen.

00:04:25 --> 00:04:27 Anna: This story is just mind boggling.

00:04:28 --> 00:04:30 JWST detected light from a star

00:04:30 --> 00:04:33 that exploded 13 billion years ago.

00:04:34 --> 00:04:36 Avery: Let that sink in. The universe itself is

00:04:36 --> 00:04:39 about 13.7 billion years old.

00:04:39 --> 00:04:42 So this event happened just 730

00:04:42 --> 00:04:44 million years after the Big Bang.

00:04:45 --> 00:04:47 Anna: Incredible. So what do we know about this

00:04:47 --> 00:04:47 event?

00:04:48 --> 00:04:50 Avery: It's been designated GRB

00:04:51 --> 00:04:54 250314A.

00:04:54 --> 00:04:57 The GRB stands for Gamma ray

00:04:57 --> 00:04:59 burst, which was detected first.

00:05:00 --> 00:05:03 That burst is the telltale sign of a

00:05:03 --> 00:05:05 massive star collapsing into a black hole

00:05:05 --> 00:05:08 or neutron star. The

00:05:08 --> 00:05:10 supernova is the explosion that follows.

00:05:11 --> 00:05:14 Anna: So this breaks the previous record for the

00:05:14 --> 00:05:16 most distant supernova by a long

00:05:16 --> 00:05:17 shot.

00:05:17 --> 00:05:19 Avery: Observing an event like this from the very

00:05:19 --> 00:05:22 early universe gives astronomers a direct

00:05:22 --> 00:05:24 look at at the life cycle of the first

00:05:24 --> 00:05:27 generations of stars, which were much more

00:05:27 --> 00:05:29 massive and short lived than stars like our

00:05:29 --> 00:05:32 Sun. It's a crucial piece of the puzzle for

00:05:32 --> 00:05:35 understanding how the universe evolved from.

00:05:35 --> 00:05:38 Anna: The most distant to some of the most massive.

00:05:38 --> 00:05:41 Let's talk about exoplanets. A new study

00:05:41 --> 00:05:44 is challenging. What we thought we knew about

00:05:44 --> 00:05:46 super Jupiters, right?

00:05:46 --> 00:05:48 Avery: These are gas giants that are significantly

00:05:48 --> 00:05:51 more massive than our own Jupiter. This

00:05:51 --> 00:05:54 new research focused on an exoplanet called

00:05:54 --> 00:05:57 VHS 1256 b,

00:05:57 --> 00:06:00 it has a mass of about 20 jupiters,

00:06:00 --> 00:06:01 20 times.

00:06:01 --> 00:06:04 Anna: The mass of Jupiter. That's almost in the

00:06:04 --> 00:06:07 territory of a brown dwarf, a failed

00:06:07 --> 00:06:07 star.

00:06:07 --> 00:06:10 Avery: It's right on that line. And the study

00:06:10 --> 00:06:12 suggests that planets this massive might not

00:06:12 --> 00:06:15 look like Jupiter at all. We picture Jupiter

00:06:15 --> 00:06:18 with its beautiful stable, banded cloud

00:06:18 --> 00:06:18 patterns.

00:06:19 --> 00:06:22 Anna: Mhm. Mm. The Great Red Spot. The distinct

00:06:22 --> 00:06:23 zones and belts.

00:06:23 --> 00:06:26 Avery: Exactly. But on a world like VHS

00:06:26 --> 00:06:29 1256 B, the internal heat and

00:06:29 --> 00:06:32 higher temperatures could drive a much more

00:06:32 --> 00:06:34 turbulent and chaotic atmosphere. The

00:06:34 --> 00:06:37 model suggests that instead of stable bands,

00:06:37 --> 00:06:40 you'd see large, dusty silicate

00:06:40 --> 00:06:41 storms swirling chaotically.

00:06:42 --> 00:06:45 Anna: So less organized beauty, more

00:06:45 --> 00:06:46 violent chaos.

00:06:47 --> 00:06:49 Avery: That's a good way to put it. It reminds us

00:06:49 --> 00:06:51 that our own solar system is just one

00:06:51 --> 00:06:53 example. And the diversity of planets out

00:06:53 --> 00:06:55 there is far greater than we can imagine.

00:06:56 --> 00:06:57 Anna: Well said.

00:06:57 --> 00:07:00 And from voyages within our solar system,

00:07:00 --> 00:07:03 let's take a leap to the truly cosmic scale.

00:07:03 --> 00:07:05 For our final story, we're heading to the

00:07:05 --> 00:07:08 center of galaxy NGC 378

00:07:08 --> 00:07:11 3, where a supermassive black hole

00:07:11 --> 00:07:13 is putting on a spectacle spectacular and

00:07:13 --> 00:07:15 very windy show.

00:07:15 --> 00:07:17 Avery: And this was a coordinated effort between two

00:07:17 --> 00:07:20 powerful space telescopes, the XMM M Newton M

00:07:21 --> 00:07:23 and the new Xrism M Observatory.

00:07:24 --> 00:07:27 Anna: That's right. They observed the black hole's

00:07:27 --> 00:07:30 active galactic nucleus, or agn,

00:07:30 --> 00:07:32 as it let out a massive X ray flare.

00:07:33 --> 00:07:35 Avery: So similar to a solar flare from our sun,

00:07:35 --> 00:07:37 but on an unimaginable scale.

00:07:38 --> 00:07:41 Anna: Precisely. And this flare had a dramatic

00:07:41 --> 00:07:43 effect. It triggered powerful winds of

00:07:43 --> 00:07:46 superheated gas being blasted away from the

00:07:46 --> 00:07:49 black hole at an incredible 1/5

00:07:49 --> 00:07:49 the speed of.

00:07:49 --> 00:07:52 Avery: Light, 20% of the speed of

00:07:52 --> 00:07:54 light. That's just phenomenal speed.

00:07:55 --> 00:07:58 Anna: It really is. And observing this process

00:07:58 --> 00:08:00 helps astronomers understand how these

00:08:00 --> 00:08:03 central black holes influence their entire

00:08:03 --> 00:08:06 host galaxies. These winds are so

00:08:06 --> 00:08:09 powerful that they can clear out gas from the

00:08:09 --> 00:08:11 galaxy's center, which can shut down star

00:08:11 --> 00:08:14 formation and fundamentally shape how a, uh,

00:08:14 --> 00:08:16 galaxy evolves over billions of years.

00:08:17 --> 00:08:20 Avery: It's a direct link between the very

00:08:20 --> 00:08:22 small, the accretion disk of a black

00:08:22 --> 00:08:25 hole, and the very large, the

00:08:25 --> 00:08:28 entire galaxy. A

00:08:28 --> 00:08:30 fantastic discovery to end on.

00:08:30 --> 00:08:33 Anna: And that's all the time we have for today on

00:08:33 --> 00:08:36 Astronomy Daily. We covered everything from

00:08:36 --> 00:08:38 spacewalks and launch records to the hunt for

00:08:38 --> 00:08:39 life on Mars.

00:08:40 --> 00:08:43 Avery: And we peered back to the dawn of time

00:08:43 --> 00:08:46 with the oldest supernova and questioned

00:08:46 --> 00:08:48 what a super Jupiter really looks like.

00:08:49 --> 00:08:50 Thanks so much for joining us.

00:08:51 --> 00:08:53 Anna: You can find us wherever you get your

00:08:53 --> 00:08:55 podcasts or our website, which can be found

00:08:55 --> 00:08:58 at astronomydaily.io we'll be back tomorrow

00:08:58 --> 00:09:01 with another roundup of the latest news from

00:09:01 --> 00:09:02 the final frontier.

00:09:03 --> 00:09:06 Avery: Until then, keep looking up. This is

00:09:06 --> 00:09:08 Avery and Anna signing off.