Twisting Waves on the Sun, the Brightest Radio Flash, and Europe's Solar Storm Simulation
Astronomy Daily: Space News October 27, 2025x
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00:09:208.6 MB

Twisting Waves on the Sun, the Brightest Radio Flash, and Europe's Solar Storm Simulation

  • Unlocking the Sun's Secrets: Astronomers have made a groundbreaking discovery regarding the Sun's corona, observing twisting magnetic waves that may explain why this outer atmosphere is millions of degrees hotter than the surface. This confirmation of decades-old theories could reshape our understanding of stellar dynamics.
  • Brightest Cosmic Flash: The brightest fast radio burst ever recorded, dubbed RB Float, has left astronomers perplexed as it has not repeated since its initial observation. This silence challenges existing theories about the origins of these enigmatic signals and suggests new possibilities for their formation.
  • Preparing for Solar Storms: The European Space Agency has conducted its most extreme solar storm simulation to date, highlighting the potential risks of such events on spacecraft and Earth’s infrastructure. This preparation underscores the importance of monitoring space weather as the Sentinel 1D mission approaches.
  • Japan's Successful Cargo Launch: JAXA has successfully launched its HTV X1 cargo spacecraft to the International Space Station. This mission not only supports ISS operations but also lays groundwork for future lunar missions as part of the Artemis program.
  • Spotting Legendary Spacecraft: Learn how to locate some of humanity's most iconic spacecraft in the night sky this October. From the James Webb Space Telescope to Voyager 1, discover where to look and appreciate the incredible journeys these machines have undertaken.
  • For more cosmic updates, visit our website at astronomydaily.io. Join our community on social media by searching for #AstroDailyPod on Facebook, X, YouTubeMusic, TikTok, and our new Instagram account! Don’t forget to subscribe to the podcast on Apple Podcasts, Spotify, iHeartRadio, or wherever you get your podcasts.
  • Thank you for tuning in. This is Anna and Avery signing off. Until next time, keep looking up and exploring the wonders of our universe.
✍️ Episode References
Sun's Corona Discovery
[NASA](https://www.nasa.gov/)
Fast Radio Bursts Research
[CHIME](https://chime.phas.ubc.ca/)
ESA Solar Storm Simulation
[ESA](https://www.esa.int/)
JAXA HTV X1 Launch
[JAXA](https://www.jaxa.jp/)
Night Sky Guide for Spacecraft
[Astronomy Daily](http://www.astronomydaily.io/)
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00:00:00 --> 00:00:03 Avery: Welcome to Astronomy Daily, the podcast that

00:00:03 --> 00:00:05 brings you the universe, one story at a time.

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

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

00:00:09 --> 00:00:12 today. We've got a fantastic lineup. We'll be

00:00:12 --> 00:00:14 looking at twisting magnetic waves on the sun

00:00:15 --> 00:00:17 that could finally solve a decades old

00:00:17 --> 00:00:18 mystery.

00:00:18 --> 00:00:21 Avery: We'll also dive into the brightest cosmic

00:00:21 --> 00:00:24 radio flash ever seen and why its silence

00:00:24 --> 00:00:26 is baffling astronomers. But plus, a sobering

00:00:26 --> 00:00:29 look at Europe's simulation of a catastrophic

00:00:29 --> 00:00:30 solar storm.

00:00:31 --> 00:00:33 Anna: And on a lighter note, a successful launch

00:00:33 --> 00:00:36 for Japan's new cargo ship. And we'll even

00:00:36 --> 00:00:38 tell you how you can spot some of humanity's

00:00:38 --> 00:00:41 most legendary spacecraft in the night sky.

00:00:41 --> 00:00:43 Avery: It's a packed show. Let's get started.

00:00:44 --> 00:00:46 Anna: Alright, Avery, let's start with our own

00:00:46 --> 00:00:49 star, the Sun. For more than 80

00:00:49 --> 00:00:52 years, scientists have puzzled over a

00:00:52 --> 00:00:55 major solar mystery. Why is the

00:00:55 --> 00:00:57 Sun's atmosphere the corona mill

00:00:58 --> 00:01:00 millions of degrees hotter than its surface?

00:01:00 --> 00:01:02 Avery: Right. It's completely counterintuitive.

00:01:02 --> 00:01:05 You'd expect it to get cooler the farther you

00:01:05 --> 00:01:06 move away from the heat source.

00:01:07 --> 00:01:09 Anna: Exactly. But now, for the first time,

00:01:09 --> 00:01:12 astronomers have direct evidence of a

00:01:12 --> 00:01:15 phenomenon that might be the key. They've

00:01:15 --> 00:01:17 observed twisting magnetic waves in the

00:01:17 --> 00:01:20 corona, something that was first proposed way

00:01:20 --> 00:01:21 back in the 1940s.

00:01:21 --> 00:01:23 Avery: And these aren't just any waves. They're

00:01:23 --> 00:01:26 called small scale torsional alfven waves.

00:01:26 --> 00:01:29 Essentially, imagine the Sun's magnetic field

00:01:29 --> 00:01:32 lines as guitar strings. These waves are like

00:01:32 --> 00:01:34 a, twisting or plucking motion traveling

00:01:34 --> 00:01:37 along those strings carrying enormous amounts

00:01:37 --> 00:01:39 of energy from the sun's surface up into the

00:01:39 --> 00:01:40 corona.

00:01:40 --> 00:01:43 Anna: That's a great analogy. This energy heats the

00:01:43 --> 00:01:45 corona to its incredible temperatures.

00:01:46 --> 00:01:47 According to one of the lead researchers,

00:01:48 --> 00:01:50 this discovery provides essential validation

00:01:50 --> 00:01:52 for the models describing how this process

00:01:52 --> 00:01:55 works. He said having direct

00:01:55 --> 00:01:57 observations for finally allows us to test

00:01:57 --> 00:01:59 these models against reality.

00:01:59 --> 00:02:02 Avery: It's a huge deal. This isn't just confirming

00:02:02 --> 00:02:04 a theory. It's a fundamental piece of the

00:02:04 --> 00:02:06 puzzle of how our star works. And by

00:02:06 --> 00:02:09 extension, how other stars work too. A

00:02:09 --> 00:02:12 mystery 80 years in the making might finally

00:02:12 --> 00:02:14 be getting solved. Next, from a mystery

00:02:14 --> 00:02:17 solved to one that just got deeper, let's

00:02:17 --> 00:02:19 talk about fast radio bursts, or FRBs.

00:02:20 --> 00:02:22 These are intense, millisecond long bursts of

00:02:22 --> 00:02:24 radio waves from deep space.

00:02:24 --> 00:02:27 Anna: And recently, astronomers spotted the

00:02:27 --> 00:02:28 brightest one ever.

00:02:28 --> 00:02:30 Avery: Right. This new Signal is designated

00:02:30 --> 00:02:32 FRB2025

00:02:32 --> 00:02:35 16A, but it has a much

00:02:35 --> 00:02:38 better nickname, RB Float, which stands for

00:02:38 --> 00:02:40 radio brightest flash of all time.

00:02:40 --> 00:02:42 Anna: I love when scientists have fun with the

00:02:42 --> 00:02:45 names. So they traced this incredibly

00:02:45 --> 00:02:48 bright flash to a nearby galaxy, giving them

00:02:48 --> 00:02:51 a fantastic view. But here's the

00:02:51 --> 00:02:51 twist.

00:02:51 --> 00:02:54 Avery: The twist is that it's gone completely

00:02:54 --> 00:02:54 silent.

00:02:54 --> 00:02:57 Anna: Exactly. Many known FRBs are

00:02:57 --> 00:02:59 repeaters. They flash over and over again

00:02:59 --> 00:03:01 from the same spot, which helps astronomers

00:03:01 --> 00:03:04 study them. But RB Float, despite being the

00:03:04 --> 00:03:06 brightest ever detected by the CHIME

00:03:06 --> 00:03:09 telescope, hasn't sent out a single repeat

00:03:09 --> 00:03:09 burst.

00:03:09 --> 00:03:11 Avery: And that challenges a major theory in the

00:03:11 --> 00:03:14 field, which is that, all FRBs might

00:03:14 --> 00:03:16 eventually repeat if we just watch them for

00:03:16 --> 00:03:16 long enough.

00:03:17 --> 00:03:20 Anna: Mm. This non repeater, especially one

00:03:20 --> 00:03:23 so powerful, opens the door to reconsidering

00:03:23 --> 00:03:26 other origins. It suggests that at least

00:03:26 --> 00:03:28 some of these events might be caused by a

00:03:28 --> 00:03:31 single cataclysmic explosion, like the

00:03:31 --> 00:03:33 collapse of a massive star, rather than a

00:03:33 --> 00:03:35 repeating source like a magnetar.

00:03:35 --> 00:03:38 Avery: So the brightest flash ever seen has left us

00:03:38 --> 00:03:40 with more questions than answers. Classic

00:03:40 --> 00:03:41 astronomy.

00:03:41 --> 00:03:44 Anna: Well, from distant cosmic explosions

00:03:44 --> 00:03:47 to a potential threat much closer to home,

00:03:47 --> 00:03:50 the European Space Agency recently ran its

00:03:50 --> 00:03:53 most extreme space weather simulation ever.

00:03:53 --> 00:03:56 And the scenario was so severe that in the

00:03:56 --> 00:03:59 exercise, no spacecraft was left

00:03:59 --> 00:04:00 unscathed.

00:04:00 --> 00:04:02 Avery: Wow, that sounds intense. So what was the

00:04:02 --> 00:04:04 purpose of this cosmic fire drill?

00:04:04 --> 00:04:06 Anna: It was designed to test how spacecraft

00:04:06 --> 00:04:09 operations teams and space weather experts

00:04:09 --> 00:04:12 would handle a truly catastrophic solar

00:04:12 --> 00:04:14 storm. This is all in preparation for the

00:04:14 --> 00:04:17 upcoming Sentinel 1D mission, which is

00:04:17 --> 00:04:20 set to launch in November. They want to be

00:04:20 --> 00:04:21 ready for the worst.

00:04:21 --> 00:04:23 Avery: And these storms are no joke. A major one

00:04:23 --> 00:04:26 could knock out satellites, disrupt gps,

00:04:26 --> 00:04:29 and even take down power grids here on Earth.

00:04:29 --> 00:04:32 Anna: Precisely. The lead simulation officer,

00:04:32 --> 00:04:34 Gustavo Baldo Carvalho, put it bluntly.

00:04:35 --> 00:04:37 He said the key takeaway is that it's not a

00:04:37 --> 00:04:40 question of if this will happen, but when.

00:04:40 --> 00:04:43 Avery: Sobering words. So what are they doing? To

00:04:43 --> 00:04:45 prepare for the inevitable, ESA is.

00:04:45 --> 00:04:47 Anna: Expanding its network of space weather

00:04:47 --> 00:04:49 monitors. They're placing sensors on more

00:04:49 --> 00:04:52 satellites, and even developing a dedicated

00:04:52 --> 00:04:54 mission called Vigil, which is planned for

00:04:54 --> 00:04:57 2031. It will be positioned at a stable

00:04:57 --> 00:05:00 point in space to give us an early warning of

00:05:00 --> 00:05:03 any dangerous solar activity heading our way.

00:05:03 --> 00:05:05 Avery: That's good to hear. It's a reminder that

00:05:05 --> 00:05:08 space isn't just about discovery. It's also

00:05:08 --> 00:05:10 about understanding and mitigating the risks

00:05:10 --> 00:05:12 that come with living next to an active star.

00:05:13 --> 00:05:16 On a much more positive note, let's talk

00:05:16 --> 00:05:18 about a successful mission launch. The Japan

00:05:18 --> 00:05:21 Aerospace Exploration Agency, or JAXA,

00:05:21 --> 00:05:23 has successfully launched its new advanced

00:05:23 --> 00:05:26 cargo spacecraft, the HTV

00:05:26 --> 00:05:28 X1, aboard an H3 rocket.

00:05:28 --> 00:05:31 Anna: Yes, it lifted off from the Tanegashima

00:05:31 --> 00:05:33 Space center and is now on its way to the

00:05:33 --> 00:05:36 International Space Station. This is a big

00:05:36 --> 00:05:38 deal for JAXA and for the station's crew.

00:05:39 --> 00:05:41 Avery: So what makes this spacecraft special?

00:05:41 --> 00:05:44 Anna: The HTV X1 is an uncrewed

00:05:44 --> 00:05:46 expendable ship designed to resupply the ISS

00:05:47 --> 00:05:50 with essentials like food, water and science

00:05:50 --> 00:05:52 experiments. But it's also a platform for

00:05:52 --> 00:05:54 technical demonstrations, testing new

00:05:54 --> 00:05:57 technologies in space. It's a real workhorse.

00:05:58 --> 00:06:00 Avery: And it seems JAXA has its sights set much

00:06:00 --> 00:06:01 further than the iss.

00:06:02 --> 00:06:04 Anna: They absolutely do. With the International

00:06:04 --> 00:06:07 Space Station scheduled for deorbit in 2030,

00:06:07 --> 00:06:09 space agencies are planning for what comes

00:06:09 --> 00:06:12 next. The HTVX platform is

00:06:12 --> 00:06:15 designed to be versatile in the future. It's

00:06:15 --> 00:06:17 intended to deliver cargo to Gateway, the

00:06:17 --> 00:06:20 planned lunar orbiting space station that

00:06:20 --> 00:06:21 will support the Artemis missions to the

00:06:21 --> 00:06:22 moon.

00:06:22 --> 00:06:24 Avery: So this launch isn't just about keeping the

00:06:24 --> 00:06:27 lights on at the iss. It's a critical step

00:06:27 --> 00:06:30 in building the infrastructure for humanity's

00:06:30 --> 00:06:32 return to the moon and missions beyond low

00:06:32 --> 00:06:35 Earth orbit. A very exciting development from

00:06:35 --> 00:06:35 Japan.

00:06:35 --> 00:06:38 Anna: And for our final story today, we're bringing

00:06:38 --> 00:06:41 things back to Earth, or at least back to our

00:06:41 --> 00:06:43 own backyards. We all know the names of

00:06:43 --> 00:06:46 legendary spacecraft like the James Webb

00:06:46 --> 00:06:49 Space telescope and Voyager 1. But do you

00:06:49 --> 00:06:51 know where to find them in the night sky?

00:06:51 --> 00:06:53 Avery: That is a great question. I think most people

00:06:53 --> 00:06:55 assume they're just up there somewhere,

00:06:55 --> 00:06:58 completely invisible. But with a bit of

00:06:58 --> 00:07:00 guidance, you can actually point to the patch

00:07:00 --> 00:07:01 of sky where they are.

00:07:01 --> 00:07:04 Anna: Exactly. And a recent guide has laid out

00:07:04 --> 00:07:06 where to look for five of these incredible

00:07:06 --> 00:07:09 explorers during October of 2025.

00:07:09 --> 00:07:12 It's a great way to feel to these missions.

00:07:12 --> 00:07:14 Avery: Okay, so let's run through them. For the

00:07:14 --> 00:07:17 James Webb Space Telescope or jwst.

00:07:17 --> 00:07:19 You'll need to find the famous red star

00:07:19 --> 00:07:22 Aldebaran and the constellation Taurus.

00:07:22 --> 00:07:25 JWST will be in that same area of the sky.

00:07:25 --> 00:07:28 Anna: And what about the Parker solar probe, the

00:07:28 --> 00:07:29 craft that's touching the Sun?

00:07:30 --> 00:07:32 Avery: That one can be found low in the southwestern

00:07:32 --> 00:07:35 sky right around sunset. Next up is

00:07:35 --> 00:07:37 NASA's Juno spacecraft which is orbiting

00:07:37 --> 00:07:40 Jupiter. It can be found high overhead

00:07:40 --> 00:07:43 in the eastern sky during the pre dawn hours.

00:07:43 --> 00:07:46 Anna: Two more to go. The New Horizons probe, which

00:07:46 --> 00:07:47 flew past Pluto.

00:07:47 --> 00:07:49 Avery: For New Horizons, you'll need to locate the

00:07:49 --> 00:07:52 famous Teapot Asterism in the constellation

00:07:52 --> 00:07:55 Sagittarius. The probe is cruising through

00:07:55 --> 00:07:57 that region of space. And finally, the

00:07:57 --> 00:08:00 legend itself, Voyager 1, humanity's most

00:08:00 --> 00:08:01 distant object.

00:08:02 --> 00:08:04 Anna: Where can we wave hello to Voyager?

00:08:04 --> 00:08:07 Avery: To find Voyager 1, you'll first need to

00:08:07 --> 00:08:09 locate the stars of the constellation

00:08:09 --> 00:08:11 Ophiuchus. It's out there

00:08:12 --> 00:08:15 over 15 billion miles away in

00:08:15 --> 00:08:18 that direction. Of course, you can't see the

00:08:18 --> 00:08:20 spacecraft themselves, but just knowing

00:08:20 --> 00:08:22 you're looking at their exact location in the

00:08:22 --> 00:08:25 cosmos is pretty amazing. And that's a

00:08:25 --> 00:08:28 wrap for today's episode of Astronomy Daily.

00:08:28 --> 00:08:31 From solving the sun's mysteries to spotting

00:08:31 --> 00:08:33 our most distant explorers in the night.

00:08:33 --> 00:08:36 Anna: Sky, thanks for listening. I'm Anna

00:08:36 --> 00:08:38 reminding you to keep looking up.

00:08:38 --> 00:08:40 Avery: And I'm Avery Clear Skies.

00:08:40 --> 00:08:43 Anna: It's a constant reminder of how much is

00:08:43 --> 00:08:46 happening out there and how much we are a

00:08:46 --> 00:08:48 part of it. We hope you enjoyed the journey

00:08:48 --> 00:08:49 with us today.

00:08:49 --> 00:08:51 Avery: Be sure to subscribe to Astronomy Daily

00:08:51 --> 00:08:53 wherever you get your podcasts so you don't

00:08:53 --> 00:08:54 miss an episode.

00:08:58 --> 00:08:59 Hm.

00:09:01 --> 00:09:02 The.

00:09:07 --> 00:09:07 Anna: Story.

00:09:15 --> 00:09:16 Avery: For Soul.