SpaceX's Launch Delays, JUICE's Close Call, and the Brightest Cosmic Flash Yet
Astronomy Daily: Space News August 26, 2025x
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00:13:3512.49 MB

SpaceX's Launch Delays, JUICE's Close Call, and the Brightest Cosmic Flash Yet

AnnaAnnaHost
  • SpaceX's Starship Test Flight Delays: The highly anticipated 10th test flight of SpaceX's Starship has faced multiple delays due to ground systems issues and inclement weather. Learn about the challenges and what’s next for this revolutionary rocket designed for lunar and Martian exploration.
  • JUICE's Close Call: The European Space Agency's Jupiter Icy Moons Explorer (JUICE) experienced a nerve-wracking silence while on its way to Venus. Discover how the team successfully reestablished contact after a communication hiccup, ensuring the mission remains on track for its upcoming flyby.
  • Record-Breaking Fast Radio Burst: Astronomers have detected the brightest fast radio burst ever recorded, dubbed RB Float. This discovery not only showcases the burst's incredible brightness but also its close proximity, allowing for unprecedented study of its origins and potential links to nearby cosmic structures.
  • Ancient Raindrops from Jupiter's Formation: Researchers have pinpointed the origin of tiny molten droplets from the early solar system, providing insights into the formation of Jupiter. This fascinating study reveals how high-energy collisions in Jupiter's vicinity produced chondrules, offering a glimpse into the planet's birth.
  • For more cosmic updates, visit our website at astronomydaily.io. Join our community on social media by searching for #AstroDailyPod on Facebook, X, YouTube Music Music, 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 stay curious about the wonders of our universe.
✍️ Episode References
SpaceX Updates
[SpaceX](https://www.spacex.com/)
JUICE Mission Details
[ESA](https://www.esa.int/)
Fast Radio Burst Discoveries
[CHIME](https://chime.phas.ubc.ca/)
Jupiter's Chondrules Research
[Nagoya University](https://www.nagoya-u.ac.jp/en/)
Astronomy Daily
[Astronomy Daily](http://www.astronomydaily.io/)

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00:00:00 --> 00:00:03 Avery: Hello, space enthusiasts, and welcome back to

00:00:03 --> 00:00:05 Astronomy Daily. I'm Avery.

00:00:05 --> 00:00:07 Anna: And I'm Anna. We've got a packed show for you

00:00:07 --> 00:00:10 today, from lunch delays and spacecraft

00:00:10 --> 00:00:12 rescues to the brightest cosmic flash ever

00:00:12 --> 00:00:15 seen. And we'll finish by traveling back in

00:00:15 --> 00:00:17 time to the birth of Jupiter.

00:00:17 --> 00:00:20 Avery: It's a huge lineup. Let's get right into it,

00:00:20 --> 00:00:22 starting with the latest from SpaceX.

00:00:22 --> 00:00:24 Anna: That's right, it's been a classic hurry up

00:00:24 --> 00:00:27 and wait situation for SpaceX as they've had

00:00:27 --> 00:00:29 to postpone the 10th test flight of their

00:00:29 --> 00:00:32 massive Starship rocket again.

00:00:32 --> 00:00:35 Avery: Indeed. They first tried to launch from their

00:00:35 --> 00:00:37 Starbase site in South Texas on Sunday,

00:00:38 --> 00:00:40 but a ground systems issue got in the way.

00:00:40 --> 00:00:43 Then they tried again on Monday, but this

00:00:43 --> 00:00:45 time it was Mother Nature who said, not

00:00:45 --> 00:00:46 today.

00:00:46 --> 00:00:49 Anna: And it was a very specific kind of not

00:00:49 --> 00:00:52 today. Anvil shaped clouds were the culprit.

00:00:52 --> 00:00:54 Those pose a serious lightning risk and

00:00:54 --> 00:00:57 you do not want a lightning strike near a

00:00:57 --> 00:00:58 fully fueled rocket.

00:00:58 --> 00:01:01 Avery: SpaceX CEO Elon Musk, who was on site,

00:01:01 --> 00:01:03 confirmed the scrub on social media.

00:01:04 --> 00:01:06 Anna: The team is now looking for the next best

00:01:06 --> 00:01:08 launch opportunity. A, uh, SpaceX

00:01:08 --> 00:01:10 spokesperson mentioned that since they didn't

00:01:10 --> 00:01:13 fire the water deluge system, reloading

00:01:13 --> 00:01:15 propellant should be a relatively quick

00:01:15 --> 00:01:17 process. So hopefully we'll see flight 10

00:01:17 --> 00:01:18 take the sky soon.

00:01:18 --> 00:01:21 Avery: And what a sight it'll be. For anyone new to

00:01:21 --> 00:01:23 the program, Starship is the biggest and most

00:01:23 --> 00:01:25 powerful rocket ever built.

00:01:26 --> 00:01:29 SpaceX's grand vision is to use it to help

00:01:29 --> 00:01:31 humanity settle the the moon and

00:01:31 --> 00:01:32 Mars.

00:01:32 --> 00:01:34 Anna: It's an incredible piece of engineering. The

00:01:34 --> 00:01:37 vehicle consists of two fully reusable

00:01:37 --> 00:01:39 stainless steel stages, a massive booster

00:01:39 --> 00:01:42 called Super Heavy, and the upper stage,

00:01:42 --> 00:01:45 which is also called Starship. The goal is

00:01:45 --> 00:01:47 rapid reusability, but getting.

00:01:47 --> 00:01:49 Avery: There has been a real process of trial and

00:01:49 --> 00:01:52 error. Starship has flown nine times so far,

00:01:52 --> 00:01:55 with the first flight back in April of 2023.

00:01:55 --> 00:01:58 The last three flights this year have all,

00:01:58 --> 00:02:00 been, well, learning experiences.

00:02:00 --> 00:02:03 Anna: That's a polite way of putting it. On Flight

00:02:03 --> 00:02:06 7 and 8, the upper stage exploded less than

00:02:06 --> 00:02:08 10 minutes after launch. And on Flight 9, it

00:02:08 --> 00:02:11 lost attitude control during re entry and

00:02:11 --> 00:02:13 broke apart in the atmosphere. We even saw

00:02:13 --> 00:02:16 reports of debris spotted over the Bahamas.

00:02:16 --> 00:02:18 Avery: It's all part of the rapid iterative

00:02:18 --> 00:02:21 development process, I suppose. SpaceX

00:02:21 --> 00:02:24 traced the Flight 7 anomaly to a

00:02:24 --> 00:02:26 harmonic response that caused propellant

00:02:26 --> 00:02:29 leaks and fires. They've since made hardware

00:02:29 --> 00:02:31 changes and adjustments to prevent it from

00:02:31 --> 00:02:32 happening again.

00:02:32 --> 00:02:34 Anna: So the plan for Flight 10 whenever it

00:02:34 --> 00:02:37 launches, is ambitious. The super heavy

00:02:37 --> 00:02:39 boosters will perform some experiments before

00:02:40 --> 00:02:42 Attempting a controlled splashdown in the

00:02:42 --> 00:02:45 Gulf of Mexico, The Starship Upper Stage will

00:02:45 --> 00:02:47 aim to deploy eight dummy Starlink

00:02:47 --> 00:02:50 satellites, relight an engine in space, and

00:02:50 --> 00:02:52 then come down in the Indian Ocean about

00:02:52 --> 00:02:54 66 minutes after launch.

00:02:55 --> 00:02:57 Avery: It's a huge step and it's clear they're

00:02:57 --> 00:02:59 looking to pick up the pace. Despite the

00:02:59 --> 00:03:02 setbacks, SpaceX has requested approval for

00:03:02 --> 00:03:04 an incredible 25 Starship

00:03:04 --> 00:03:07 launches from Starbase in 2025.

00:03:08 --> 00:03:10 They are not slowing down, Definitely not.

00:03:10 --> 00:03:12 Anna: We'll be watching closely and will bring you

00:03:12 --> 00:03:14 updates as uh, soon as Flight 10 gets off the

00:03:14 --> 00:03:15 ground.

00:03:15 --> 00:03:17 Now, from a mission waiting to start, let's

00:03:17 --> 00:03:20 turn to one that just survived a major scare

00:03:21 --> 00:03:23 millions of kilometers from home. This is a

00:03:23 --> 00:03:25 fantastic story of teamwork from the European

00:03:25 --> 00:03:28 Space Agency. Their Jupiter Icy Moons

00:03:28 --> 00:03:30 Explorer, or juice, is currently on its way

00:03:30 --> 00:03:33 to Venus for a gravity assist flyby. But for

00:03:33 --> 00:03:36 a little while, the team on the ground had no

00:03:36 --> 00:03:37 idea if it was okay.

00:03:37 --> 00:03:40 Avery: Talk about a nerve wracking situation. On

00:03:40 --> 00:03:42 July 16, during a routine check in,

00:03:43 --> 00:03:45 JUICE just fell silent. The

00:03:45 --> 00:03:48 Deep Space Antenna in Spain couldn't

00:03:48 --> 00:03:50 establish contact. No signal, no

00:03:50 --> 00:03:53 telemetry about its health or stat, nothing.

00:03:53 --> 00:03:55 Anna: The control team at ESOC in Germany

00:03:55 --> 00:03:57 immediately began troubleshooting. The

00:03:57 --> 00:03:59 biggest fear was that JUICE had entered

00:03:59 --> 00:04:02 survival mode, a last resort state triggered

00:04:02 --> 00:04:05 by multiple system failures. But they weren't

00:04:05 --> 00:04:07 detecting the intermittent signal you'd

00:04:07 --> 00:04:08 expect in that scenario.

00:04:09 --> 00:04:11 Avery: So with no data coming in, they had to start

00:04:11 --> 00:04:14 making some educated guesses. The

00:04:14 --> 00:04:16 team suspected an issue with the

00:04:16 --> 00:04:19 communication subsystem. They faced a tough

00:04:20 --> 00:04:22 wait, 14 days for an automatic

00:04:22 --> 00:04:25 spacecraft reset or send

00:04:25 --> 00:04:28 commands blind into space and hope

00:04:28 --> 00:04:29 the spacecraft heard them.

00:04:30 --> 00:04:32 Anna: Waiting wasn't really an option, as uh,

00:04:32 --> 00:04:34 spacecraft Operations Manager Angela

00:04:34 --> 00:04:37 Dietz explained, that would have delayed

00:04:37 --> 00:04:39 crucial preparations for the Venus flyby.

00:04:40 --> 00:04:42 So they went with the blind commanding

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

00:04:44 --> 00:04:46 Avery: Um, and that is not easy. Juice was

00:04:46 --> 00:04:49 200 million kilometers away on

00:04:49 --> 00:04:52 the other side of the sun. Each command

00:04:52 --> 00:04:54 took 11 minutes to get there, and then they

00:04:54 --> 00:04:57 had to wait another 11 minutes to see if it

00:04:57 --> 00:05:00 worked. After nearly 20 hours of

00:05:00 --> 00:05:02 troubleshooting, a command finally got

00:05:02 --> 00:05:03 through.

00:05:03 --> 00:05:06 Anna: The successful command manually activated the

00:05:06 --> 00:05:08 signal amplifier, which boosts the strength

00:05:08 --> 00:05:11 of the signal Juice sends to Earth. Suddenly,

00:05:11 --> 00:05:14 they had contact again, and the spacecraft

00:05:14 --> 00:05:16 was in perfect health. It turns out the

00:05:16 --> 00:05:19 culprit was a very subtle software bug,

00:05:20 --> 00:05:21 A, uh, timing.

00:05:21 --> 00:05:24 Avery: Bug of all things. The software

00:05:24 --> 00:05:26 function that controls the amplifier uses an

00:05:26 --> 00:05:29 internal timer that resets every 16

00:05:29 --> 00:05:32 months. It just so happened that the function

00:05:32 --> 00:05:34 was running at the exact moment the timer

00:05:34 --> 00:05:37 restarted, which left the Amplifier switched

00:05:37 --> 00:05:39 off. What are the odds?

00:05:40 --> 00:05:43 Anna: Incredibly small. But as we know, in

00:05:43 --> 00:05:45 space, you have to plan for everything.

00:05:46 --> 00:05:48 The team has already identified ways to

00:05:48 --> 00:05:50 prevent this from happening again. It's a

00:05:50 --> 00:05:53 textbook example of calm, methodical problem

00:05:53 --> 00:05:56 solving under extreme pressure.

00:05:56 --> 00:05:59 Avery: Absolutely. A huge congratulations to

00:05:59 --> 00:06:02 the ESA mission operations team. With

00:06:02 --> 00:06:04 that drama behind them, JUICE is now back on

00:06:04 --> 00:06:07 track for its Venus flyby at the end of

00:06:07 --> 00:06:07 August.

00:06:08 --> 00:06:11 From a close call to a cosmic bullseye,

00:06:11 --> 00:06:14 our next story is about a truly record

00:06:14 --> 00:06:17 breaking discovery. This one is genuinely

00:06:17 --> 00:06:19 exciting. Astronomers have just detected the

00:06:19 --> 00:06:22 brightest fast radio burst ever recorded.

00:06:23 --> 00:06:25 It's so powerful, they've nicknamed it

00:06:25 --> 00:06:28 RB Float, which stands for radio

00:06:28 --> 00:06:30 brightest flash of all time.

00:06:31 --> 00:06:34 Anna: A very fitting name. The burst, officially

00:06:34 --> 00:06:36 cataloged as FRB2025

00:06:37 --> 00:06:40 0316A, was spotted spotted

00:06:40 --> 00:06:42 back in March by the CHIME telescope in

00:06:42 --> 00:06:44 British Columbia. CHIME has found

00:06:44 --> 00:06:47 thousands of these fast radio bursts, or

00:06:47 --> 00:06:49 FRBs, but this one is special.

00:06:50 --> 00:06:52 Avery: It's not just about the brightness. Right.

00:06:52 --> 00:06:54 It's about where they found it.

00:06:54 --> 00:06:57 Usually tracing an FRB is like trying to

00:06:57 --> 00:07:00 find which tree a firefly is in from a

00:07:00 --> 00:07:02 mile away. But this time they

00:07:02 --> 00:07:05 pinpointed its origin to a region just

00:07:05 --> 00:07:07 45 light years across.

00:07:08 --> 00:07:11 Anna: Exactly that incredible precision is

00:07:11 --> 00:07:13 thanks to a new upgrade to the CHIME system.

00:07:13 --> 00:07:15 They've added three smaller outrigger

00:07:15 --> 00:07:18 stations across North America, which

00:07:18 --> 00:07:20 effectively turns them into a single

00:07:20 --> 00:07:23 continent wide telescope. This allows them to

00:07:23 --> 00:07:26 trace these millisecond long flashes back to

00:07:26 --> 00:07:29 their home galaxies with stunning accuracy.

00:07:29 --> 00:07:32 Avery: And the home galaxy in this case NGC

00:07:32 --> 00:07:35 4141, is practically in

00:07:35 --> 00:07:38 our backyard. Cosmically speaking, it's about

00:07:38 --> 00:07:41 130 million light years away, which is

00:07:41 --> 00:07:43 incredibly close for an frb. Most of

00:07:43 --> 00:07:46 them come from billions of light years away.

00:07:46 --> 00:07:49 Anna: That proximity, combined with its brightness

00:07:49 --> 00:07:51 gives scientists a, uh, unique chance to

00:07:51 --> 00:07:54 study the source in detail. The team found

00:07:54 --> 00:07:56 the burst originated near the edge of a star

00:07:56 --> 00:07:59 forming region in the galaxy. This hints that

00:07:59 --> 00:08:02 the source could be a magnetar, an ultra

00:08:02 --> 00:08:05 magnetized neutron star that's perhaps

00:08:05 --> 00:08:07 a bit older than the very youngest stars at

00:08:07 --> 00:08:08 the galaxy's core.

00:08:09 --> 00:08:11 Avery: And the story gets even better. Because they

00:08:11 --> 00:08:14 located it so quickly, they were able to

00:08:14 --> 00:08:16 point the James Webb Telescope at the

00:08:16 --> 00:08:19 location. Webb's infrared cameras spotted

00:08:19 --> 00:08:22 a faint point of light nearby, which they've

00:08:22 --> 00:08:23 dubbed Nir1.

00:08:24 --> 00:08:26 Anna: The nature of Nir1 is still a

00:08:26 --> 00:08:29 mystery. It could be a red giant star or

00:08:29 --> 00:08:32 maybe a massive star in its midlife. It

00:08:32 --> 00:08:34 Neither of these are typically associated

00:08:34 --> 00:08:36 with FRBs, which has led to a

00:08:36 --> 00:08:38 fascinating theory. Perhaps

00:08:38 --> 00:08:41 NIR1 is part of a binary system

00:08:42 --> 00:08:44 with its gravitational partner being the

00:08:44 --> 00:08:47 compact objects like a neutron star that

00:08:47 --> 00:08:48 produce the burst.

00:08:48 --> 00:08:51 Avery: It's a fantastic cosmic puzzle. Another idea

00:08:51 --> 00:08:54 is that NIR1 isn't a star at all, but the

00:08:54 --> 00:08:55 fading afterglow of the burst itself,

00:08:56 --> 00:08:58 whatever it is. As Ito Berger from the

00:08:58 --> 00:09:00 Harvard Smithsonian center for Astrophysics

00:09:00 --> 00:09:02 said the this could be the first step on a

00:09:02 --> 00:09:04 new path to solving the FRB mystery.

00:09:04 --> 00:09:07 Anna: It also adds to the debate over whether FRBs

00:09:07 --> 00:09:10 are one time events or repeaters. So

00:09:10 --> 00:09:12 far, RB float seems to be a one

00:09:12 --> 00:09:15 off. Being able to study the environment of

00:09:15 --> 00:09:18 a non repeating FRB this closely is a huge

00:09:18 --> 00:09:21 deal. And it shows just how diverse their

00:09:21 --> 00:09:22 origins might be.

00:09:22 --> 00:09:25 Avery: Absolutely. It's a perfect illustration of

00:09:25 --> 00:09:26 how collaboration between different

00:09:26 --> 00:09:28 observatories can unlock new discoveries.

00:09:29 --> 00:09:31 Now for our final story, we're coming a bit

00:09:31 --> 00:09:34 closer to home to look at ancient raindrops

00:09:34 --> 00:09:36 from the formation of our own solar system.

00:09:37 --> 00:09:40 Anna: That's right. Avery researchers

00:09:40 --> 00:09:42 have for the first time managed to determine

00:09:42 --> 00:09:45 the date and origin of tiny ancient

00:09:45 --> 00:09:48 molten droplets that came from the

00:09:48 --> 00:09:50 neighborhood of a young Jupiter. These

00:09:50 --> 00:09:53 droplets were found inside meteorites here

00:09:53 --> 00:09:54 on Earth.

00:09:55 --> 00:09:57 Avery: Molten rock raindrops from Jupiter?

00:09:58 --> 00:10:00 That sounds incredible. How does that even

00:10:00 --> 00:10:01 happen?

00:10:02 --> 00:10:04 Anna: Well, about 4.5 billion years

00:10:04 --> 00:10:07 ago, as Jupiter was forming, its

00:10:07 --> 00:10:10 immense gravitational pull started flinging

00:10:10 --> 00:10:12 nearby small rocky and icy

00:10:12 --> 00:10:15 bodies called planetesimals into

00:10:15 --> 00:10:18 each other at incredibly high speeds.

00:10:19 --> 00:10:21 Avery: So these were seriously high energy

00:10:21 --> 00:10:23 collisions. What happened to the rock?

00:10:24 --> 00:10:27 Anna: The impacts were so forceful that the rock

00:10:27 --> 00:10:30 and dust on these planetesimals melted

00:10:30 --> 00:10:33 instantly, creating tiny molten

00:10:33 --> 00:10:35 rock droplets known as chondrules.

00:10:35 --> 00:10:38 These spheres, only about a millimeter wide,

00:10:39 --> 00:10:41 eventually got incorporated into asteroids,

00:10:41 --> 00:10:43 some of which later fell to Earth as

00:10:43 --> 00:10:44 meteorites.

00:10:45 --> 00:10:47 Avery: So scientists have had these chondrules for a

00:10:47 --> 00:10:50 while, but they weren't sure exactly how they

00:10:50 --> 00:10:52 formed. What's the new theory?

00:10:52 --> 00:10:55 Anna: A team from Nagoya University in Japan

00:10:55 --> 00:10:58 and the INAF Turin Astrophysical

00:10:58 --> 00:11:01 Observatory in Italy developed a new

00:11:01 --> 00:11:04 model. They realized that when these water

00:11:04 --> 00:11:07 rich planetesimals collided, the water would

00:11:07 --> 00:11:09 have instantly vaporized into steam.

00:11:10 --> 00:11:12 This expanding steam acted like a series

00:11:12 --> 00:11:15 of tiny explosions, breaking apart the

00:11:15 --> 00:11:18 molten rock into the exact kind of droplets

00:11:18 --> 00:11:20 we see in meteorites.

00:11:21 --> 00:11:23 Avery: That makes so much sense. So they tested this

00:11:23 --> 00:11:24 with a computer simulation.

00:11:25 --> 00:11:28 Anna: They did. They programmed a simulation of

00:11:28 --> 00:11:30 Jupiter's formation, tracking how its gravity

00:11:30 --> 00:11:33 would cause these collisions. Co lead

00:11:33 --> 00:11:36 author Dr. Diego Turini said the

00:11:36 --> 00:11:39 model spontaneously generated realistic

00:11:39 --> 00:11:42 looking chondrules. And importantly, it

00:11:42 --> 00:11:44 showed that the peak of this chondrule

00:11:44 --> 00:11:47 production happened right as Jupiter was

00:11:47 --> 00:11:49 accumulating gas to become the giant it is

00:11:49 --> 00:11:50 today.

00:11:51 --> 00:11:52 Avery: And, um, the evidence from actual meteorites

00:11:52 --> 00:11:54 backs this up perfectly.

00:11:55 --> 00:11:58 Anna: The meteorite data shows that peak chondrul

00:11:58 --> 00:12:01 Production occurred about 1.8 million years

00:12:01 --> 00:12:03 after the solar system began, which is

00:12:03 --> 00:12:06 exactly when they believed Jupiter was going

00:12:06 --> 00:12:08 through its main growth spurt.

00:12:09 --> 00:12:11 Avery: Wow. So these tiny droplets are like

00:12:11 --> 00:12:13 fossilized evidence of Jupiter's birth.

00:12:14 --> 00:12:17 That's amazing. Does this solve all the

00:12:17 --> 00:12:17 mysteries?

00:12:18 --> 00:12:21 Anna: Not quite. The model doesn't fully

00:12:21 --> 00:12:23 explain why we find chondrules of different

00:12:23 --> 00:12:26 ages in meteorites. The researchers suggest

00:12:26 --> 00:12:29 that the formation of other gas giants like

00:12:29 --> 00:12:32 Saturn could have triggered similar events

00:12:32 --> 00:12:34 later on, creating more chondrules.

00:12:35 --> 00:12:38 Avery: It's a fantastic piece of detective work. It

00:12:38 --> 00:12:40 m gives us a clearer picture of how our solar

00:12:40 --> 00:12:42 system formed and provides insights that

00:12:42 --> 00:12:45 could apply to other systems as well. A huge

00:12:45 --> 00:12:47 story contained in a tiny, ancient raindrop.

00:12:48 --> 00:12:49 And that's all the time we have for this

00:12:49 --> 00:12:52 episode of Astronomy Daily. From cosmic

00:12:52 --> 00:12:54 flashes to planetary raindrops, it's been

00:12:54 --> 00:12:56 another incredible week in space.

00:12:56 --> 00:12:59 Anna: It certainly has. Thank you so much for

00:12:59 --> 00:13:02 joining us. If you enjoyed the show, please

00:13:02 --> 00:13:04 subscribe wherever you get your podcasts, and

00:13:04 --> 00:13:06 you can follow us on social media for daily

00:13:06 --> 00:13:07 updates.

00:13:07 --> 00:13:09 Avery: Until next time, keep looking up.

00:13:10 --> 00:13:10 Anna: Goodbye, everyone.