In this episode
Highlights:- Giant Planet Discovery: Dive into the astonishing discovery of TOI 6894 b, a gas giant orbiting the diminutive red dwarf star TOI 6894. This finding challenges our understanding of planet formation, as such small stars were not thought to possess enough material to form giant planets. With deep transits blocking 17% of the star's light, astronomers are eager to study its atmosphere using the James Webb Space Telescope.
- The Mystery of Heavy Elements: Explore the peculiar star Limos J 0804 5740, found within the remnants of a dwarf galaxy known as the Gaia Sausage. This actinide boost star holds clues to the origins of the universe's heaviest elements, such as uranium and thorium, which are produced through rapid neutron capture processes. Studying this star may help unravel the cosmic puzzle of how these elements are formed.
- China's Reusable Rocket: Learn about Space Epic's recent test launch of their reusable rocket booster, the Yangxing Zhi one, which successfully performed a soft landing in the ocean. Although it sank post-landing, the test demonstrated crucial capabilities for future missions, showcasing China's growing ambitions in space exploration alongside its emerging private sector.
- Galaxy Clusters on a Collision Course: Get the latest on NASA's Chandra X-ray Observatory findings, revealing two galaxy clusters that have already collided and are now on a trajectory for a second encounter. These clusters, located 2.8 billion light years away, exhibit unique shock fronts and provide valuable insights into the dynamics of massive cosmic structures.
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, 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 signing off. Until next time, keep looking up and stay curious about the wonders of our universe.
Chapters:
00:00 - Welcome to Astronomy Daily
01:10 - Discovery of giant planet TOI 6894 b
10:00 - The mystery of heavy elements and Limos J 0804 5740
15:30 - China's reusable rocket Yangxing Zhi one
20:00 - Galaxy clusters on a collision course
✍️ Episode References
TOI 6894 b Discovery Details
[NASA Exoplanet Archive](https://exoplanetarchive.ipac.caltech.edu/)
Heavy Elements and R Process Research
[Nature Astronomy](https://www.nature.com)
Space Epic's Yangxing Zhi one Launch
[Space Epic](https://www.spaceepic.com/)
Chandra X-ray Observatory Findings
[NASA Chandra](https://www.nasa.gov/mission_pages/chandra/main/index.html)
Astronomy Daily
[Astronomy Daily](http://www.astronomydaily.io/)
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Anna: Hello and welcome to Astronomy Daily. I'm your host, Anna, and I'm really excited to bring you your daily dose of cosmic happenings. Today we've got some really cool stuff to talk about. From a giant planet orbiting a tiny star to a weird star that might just solve one of astronomy's biggest mysteries. We will also cover China's reusable rocket and two galaxy clusters about to crash into each other again. So buckle up space fans. It's going to be an awesome ride. First up, we're diving into the head scratching discovery of a giant planet, TOI 6894 b, orbiting a red dwarf star called TOI 6894.
Now, this star is tiny. I mean, we're talking about one fifth the size of our sun, which makes the discovery of this planet like a huge surprise. See, these small stars weren't thought to have enough material to even form giant planets. But there it is, TOI 6894B, a gas giant roughly the size of Saturn. It's kinda like finding a fully grown elephant living in a mousehole, you know, this discovery kinda turns our understanding of planet formation on its head. The current theory suggests that the amount of material in the disc around a star which eventually forms planets is proportional to the star's mass.
So a tiny star shouldn't have enough stuff to make a giant planet. But apparently nature loves to throw curveballs. Now, because TOI6894B has such deep transits, I mean, when it passes in front of its star, it blocks a whopping 17% of the light. It's a perfect candidate for atmosphere study. A team of astronomers has already applied for time with the James Webb Space Telescope to do just that. They are hoping to find a lot of methane in the exoplanet's atmosphere. That'll give us a better idea of how this planet formed and maybe help us refine our planet formation theories.
Pretty cool, huh? Huh? Next up, let's talk about a really odd star, limos J 0804 5740, residing in what's known as the Gaia Sausage. And no, it's not a galactic deli item. The Gaia Sausage is actually the remains of a dwarf galaxy that merged with our Milky Way billions of years ago. Now, this star, it may just help us solve one of astronomy's big mysteries. Where did the universe's heaviest elements come from? These elements, like uranium and thorium, are created through something called the R process.
That's a rapid neutron capture process, essentially Atomic nuclei rapidly grab neutrons in extreme environments like neutron star mergers or supernovas, creating heavier elements. But here's the thing. We haven't quite figured out all the sources of the R process, and that's where Lemost J 08045740 comes in. This star is what they call an actinide boost star, meaning it has a high abundance of radioactive elements, actinides. So the star's unusual composition provides new clues about the different types of R process events that can occur in the universe.
By studying it, astronomers, hope to better understand where these heavy elements come from and how they're created. It's like piecing together a cosmic puzzle, you know? You okay? So shifting gears a little, let's head over to China where a rocket startup called Space Epic, or Sepok if you like it short, recently showed off its reusable rocket booster, the Yangxing Zhi one. They had a test launch and get this, it did a soft landing right in the ocean. I mean, sadly it sank afterwards, but hey, the launch and the test were still a success.
Apparently the whole point was to test things like the engine's thrust control, shutdown and restart capabilities. Plus they tested free descent, gliding and hovering before splashdown. Pretty cool right? Now this Yangxing Zhe booster is kinda interesting. It's made from lightweight, thin walled aluminium, stainless steel and runs on liquid oxygen and methane. It's about 4.2 metres in diameter and almost 27 metres tall. Now I know what you're thinking, how does this stack up against SpaceX? Well, SpaceX's Falcon 9 booster is a bit narrower, but it's taller.
And speaking of SpaceX, it's kind of wild how they've turned landing and reusing boosters into like a near daily thing. Meanwhile, China is catching up with a bunch of space startups popping up recently. And you know, with China working on its own mega satellite constellation and planning some seriously ambitious missions, including their own version of the Hubble telescope, it's clear they are becoming a major player in space exploration. Space Epoch is hoping to reach orbit later this year. So yeah, it's definitely going to be interesting to see what these China based startups do in the coming years.
Alright. Ah, next up in our cosmic headlines, NASA's Chandra X Ray Observatory has spotted something pretty wild. We're talking about two galaxy clusters known as PSZ2 G1, 81.06 plus 48.47 that have already collided once and are now heading back for a second smash up. Now, galaxy clusters just so, you know, are like the biggest structures in the universe held together by gravity. They're basically massive collections of galaxies, superheated gas, and dark matter. These two clusters are about 2.8 billion light years away.
And after their first collision, they created these huge parentheses shaped shock fronts, kind of like sonic booms, but on a cosmic scale. These shock fronts are now separated by about 11 million light years, which is apparently the largest separation astronomers have ever seen. But get this. Chandra and XMM Newton data show that these clusters are now slowing down and turning around for another collision. Astronomers have spotted three new shock fronts that seem to be early signs of this second crash.
What's really interesting is that the total mass of this system is less than other colliding galaxy clusters, making it a pretty unusual case. This event is giving scientists a, peek into the dynamics of these massive structures and how they evolve over time. So that's your Astronomy Daily News summary for today. From a tiny star with a giant planet to colliding galaxy clusters, I've been your host, Anna, and I hope you enjoyed our little tour of the cosmos. For all the latest space and astronomy news, don't forget to visit our website at astronomydaily IO where you can catch up on our constantly updating news feed.
Until tomorrow, thanks for tuning in and keep looking up
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