Interstellar Mysteries, Solar Celebrations, and the AI Propulsion Revolution
Movies First: Film Reviews & InsightsDecember 08, 202500:12:5411.82 MB

Interstellar Mysteries, Solar Celebrations, and the AI Propulsion Revolution

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

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

00:00:05 --> 00:00:07 across the cosmos. I'm Avery.

00:00:07 --> 00:00:10 >> And I'm Anna. We have a fascinating show

00:00:10 --> 00:00:13 for you today. We'll be looking at our

00:00:13 --> 00:00:15 mysterious interstellar object friend

00:00:15 --> 00:00:18 that's prompting secret space drills.

00:00:18 --> 00:00:20 >> We're also celebrating the 30th

00:00:20 --> 00:00:22 anniversary of a legendary solar

00:00:22 --> 00:00:26 observatory and diving into how AI is

00:00:26 --> 00:00:29 revolutionizing spacecraft propulsion.

00:00:29 --> 00:00:32 Plus, a hypersonic space gun, a preview

00:00:32 --> 00:00:35 of one of the best meteor showers of the

00:00:35 --> 00:00:37 year, and we'll solve a decad's old

00:00:37 --> 00:00:40 mystery from Voyager 2's journey to

00:00:40 --> 00:00:41 Uranus.

00:00:41 --> 00:00:43 >> Anna, let's start with something that

00:00:43 --> 00:00:46 has the astronomical community buzzing.

00:00:46 --> 00:00:49 The interstellar object known as threey

00:00:49 --> 00:00:51 Atlas is back in the spotlight.

00:00:51 --> 00:00:54 >> It certainly is, Avery. This object

00:00:54 --> 00:00:57 which came from outside our solar system

00:00:57 --> 00:00:59 is exhibiting some very strange

00:00:59 --> 00:01:01 behavior. Scientists have noted what

00:01:02 --> 00:01:04 they call non-gravitational

00:01:04 --> 00:01:05 acceleration.

00:01:05 --> 00:01:07 >> Meaning it's changing speed in a way

00:01:08 --> 00:01:10 that can't be explained by the pole of

00:01:10 --> 00:01:11 the sun or planets.

00:01:12 --> 00:01:14 >> Exactly. And it's not outgassing like a

00:01:14 --> 00:01:17 typical comet. Instead, it seems to have

00:01:17 --> 00:01:21 these strange focused jets pointing away

00:01:21 --> 00:01:25 from the sun, forming an anti-tail. It's

00:01:25 --> 00:01:26 a real puzzle.

00:01:26 --> 00:01:28 >> And this puzzle is getting some serious

00:01:28 --> 00:01:31 attention. There have been a series of

00:01:31 --> 00:01:34 coordinated but very quiet space defense

00:01:34 --> 00:01:38 drills involving the ESA, Japan, the US,

00:01:38 --> 00:01:41 Australia, and several other nations.

00:01:41 --> 00:01:43 >> That's right. The official line is that

00:01:43 --> 00:01:45 they are standard preparedness

00:01:45 --> 00:01:48 exercises, but the timing is

00:01:48 --> 00:01:50 conspicuous, especially with ThreeI

00:01:50 --> 00:01:53 Atlas's closest approach to Earth

00:01:53 --> 00:01:55 happening on December 19th.

00:01:55 --> 00:01:58 >> It adds a layer of intrigue, especially

00:01:58 --> 00:02:00 when you consider some of the more out

00:02:00 --> 00:02:01 there theories.

00:02:02 --> 00:02:04 >> You're thinking of Aviab's hypothesis.

00:02:04 --> 00:02:07 >> I am. He suggested that threeey atlas

00:02:08 --> 00:02:10 might not be a single object but a

00:02:10 --> 00:02:13 primary craft accompanied by a swarm of

00:02:13 --> 00:02:15 smaller probes. Now that is pure

00:02:16 --> 00:02:17 speculation of course.

00:02:17 --> 00:02:20 >> Pure speculation but it highlights just

00:02:20 --> 00:02:22 how little we understand about this

00:02:22 --> 00:02:25 visitor. Whatever its nature, its

00:02:25 --> 00:02:27 strange dynamics and the heightened

00:02:27 --> 00:02:30 military interest mean that countless

00:02:30 --> 00:02:33 telescopes will be tracking it very,

00:02:33 --> 00:02:35 very closely in the coming weeks.

00:02:35 --> 00:02:38 >> Well, from a mysterious newcomer to a

00:02:38 --> 00:02:41 celebrated veteran, our next story is

00:02:41 --> 00:02:44 about a truly remarkable achievement.

00:02:44 --> 00:02:47 Happy 30th anniversary to the Solar and

00:02:47 --> 00:02:51 Heliospheric Observatory, or SOHO. An

00:02:51 --> 00:02:54 incredible milestone. When SOHO

00:02:54 --> 00:02:56 launched, its primary mission was

00:02:56 --> 00:02:58 scheduled to last just two years. 30

00:02:58 --> 00:03:01 years later, it's still providing

00:03:01 --> 00:03:03 invaluable data about our star.

00:03:03 --> 00:03:05 >> It really is the definition of

00:03:05 --> 00:03:07 resilience. It survived multiple

00:03:07 --> 00:03:10 technical crises that nearly ended the

00:03:10 --> 00:03:12 mission. Yet, the team on the ground

00:03:12 --> 00:03:14 always found a way to bring it back

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

00:03:15 --> 00:03:18 >> Right. And its contributions have been

00:03:18 --> 00:03:20 monumental. SOHO completely

00:03:20 --> 00:03:23 revolutionized solar science and our

00:03:23 --> 00:03:25 understanding of space weather. The

00:03:25 --> 00:03:28 images and data it provides are the

00:03:28 --> 00:03:31 foundation of modern solar forecasting,

00:03:31 --> 00:03:33 which is critical for protecting our

00:03:33 --> 00:03:35 satellites and power grids.

00:03:35 --> 00:03:37 >> Absolutely. But it has another

00:03:37 --> 00:03:40 completely unexpected legacy, doesn't

00:03:40 --> 00:03:42 it? For a satellite designed to look at

00:03:42 --> 00:03:45 the sun, it's found an incredible number

00:03:45 --> 00:03:48 of comets. It's the most prolific comet

00:03:48 --> 00:03:50 hunter in history, and it's not even

00:03:50 --> 00:03:51 close.

00:03:51 --> 00:03:53 >> Is it a case of being in the right place

00:03:53 --> 00:03:55 at the right time, or is there another

00:03:55 --> 00:03:57 reason why it's so prolific?

00:03:57 --> 00:03:59 >> It's because of its wide, uninterrupted

00:03:59 --> 00:04:02 view of the sun's corona. It spots

00:04:02 --> 00:04:05 so-called sungrazing comets that are

00:04:05 --> 00:04:07 otherwise invisible to us. As of this

00:04:08 --> 00:04:11 year, the official count is over 5

00:04:11 --> 00:04:13 comets discovered by SOHO.

00:04:13 --> 00:04:16 >> That's just amazing. 5 comments as a

00:04:16 --> 00:04:19 side project. SOHO is a true workhorse

00:04:19 --> 00:04:22 of space exploration and a testament to

00:04:22 --> 00:04:24 brilliant engineering.

00:04:24 --> 00:04:26 >> Speaking of brilliant engineering, our

00:04:26 --> 00:04:28 next story looks at the future of

00:04:28 --> 00:04:31 getting around the solar system. Avery,

00:04:31 --> 00:04:34 artificial intelligence is starting to

00:04:34 --> 00:04:36 fundamentally change how we design and

00:04:36 --> 00:04:39 operate spacecraft propulsion systems.

00:04:39 --> 00:04:41 >> This is fascinating stuff. It's not just

00:04:41 --> 00:04:44 about AI pilots like in the movies. This

00:04:44 --> 00:04:46 is about AI making the engines

00:04:46 --> 00:04:49 themselves smarter and more efficient.

00:04:49 --> 00:04:52 >> That's the core of it. Researchers are

00:04:52 --> 00:04:54 using a technique called reinforcement

00:04:54 --> 00:04:57 learning where an AI runs millions of

00:04:57 --> 00:04:59 simulations to discover the most

00:04:59 --> 00:05:01 efficient ways to operate an engine,

00:05:01 --> 00:05:03 often finding solutions that a human

00:05:04 --> 00:05:07 engineer might never think of.

00:05:07 --> 00:05:09 >> So, what kind of advanced systems are

00:05:09 --> 00:05:11 benefiting from this?

00:05:11 --> 00:05:13 We're seeing it applied to next

00:05:13 --> 00:05:16 generation concepts like nuclear thermal

00:05:16 --> 00:05:18 propulsion, both fision and the more

00:05:18 --> 00:05:21 complex fusionbased designs. These

00:05:21 --> 00:05:24 engines are incredibly powerful, but

00:05:24 --> 00:05:27 also incredibly complex to manage.

00:05:28 --> 00:05:30 >> So just what can AI help with? A lot, I

00:05:30 --> 00:05:31 would imagine.

00:05:31 --> 00:05:34 >> AI can optimize the fuel flow,

00:05:34 --> 00:05:37 temperature, and thrust in real time.

00:05:37 --> 00:05:39 It's also being used to tackle one of

00:05:39 --> 00:05:41 the biggest challenges in fusion

00:05:41 --> 00:05:44 research, managing the superheated

00:05:44 --> 00:05:47 plasma. In concepts like the poly well,

00:05:47 --> 00:05:50 a compact fusion device, AI is learning

00:05:50 --> 00:05:52 how to best configure the magnetic

00:05:52 --> 00:05:55 fields to confine the plasma, which is a

00:05:55 --> 00:05:57 massive step forward.

00:05:57 --> 00:06:00 >> So AI is becoming a design partner. It's

00:06:00 --> 00:06:02 not just running the machine, it's

00:06:02 --> 00:06:04 helping to perfect the machine's very

00:06:04 --> 00:06:06 operation. This could be the key to

00:06:06 --> 00:06:08 unlocking faster, more efficient travel

00:06:08 --> 00:06:10 across the solar system.

00:06:10 --> 00:06:12 >> We'll keep an eye on this and report

00:06:12 --> 00:06:15 back on any developments, but it sounds

00:06:15 --> 00:06:16 exciting.

00:06:16 --> 00:06:19 >> From the digital frontier of AI, we go

00:06:19 --> 00:06:22 to something that sounds decidedly more

00:06:22 --> 00:06:26 analog. Anna, what is a hypersonic space

00:06:26 --> 00:06:27 gun?

00:06:27 --> 00:06:29 >> It sounds like something out of Jules

00:06:29 --> 00:06:31 Vern novel, doesn't it? But it's a very

00:06:32 --> 00:06:34 real concept being developed by a

00:06:34 --> 00:06:35 company called Longshot Space

00:06:35 --> 00:06:38 Technologies. They are building a

00:06:38 --> 00:06:41 kinetic space launch system. In simple

00:06:41 --> 00:06:44 terms, it's a massive gun designed to

00:06:44 --> 00:06:47 fire payloads directly into orbit.

00:06:47 --> 00:06:50 >> You're kidding. How does that even work?

00:06:50 --> 00:06:53 >> The system uses a huge piston driven by

00:06:53 --> 00:06:56 compressed gas to launch a projectile at

00:06:56 --> 00:07:00 incredible speeds. We're talking Mach 23

00:07:00 --> 00:07:03 or about 28

00:07:03 --> 00:07:07 km hour. The projectile would carry a

00:07:07 --> 00:07:10 small hardened satellite or other cargo.

00:07:10 --> 00:07:13 >> I can't even imagine the forces

00:07:13 --> 00:07:15 involved. The heat and the acceleration

00:07:15 --> 00:07:17 must be astronomical.

00:07:17 --> 00:07:20 >> They are. That's the biggest challenge.

00:07:20 --> 00:07:22 The payload would experience about

00:07:22 --> 00:07:26 10 gs of acceleration and intense

00:07:26 --> 00:07:29 atmospheric heating. So this isn't for

00:07:29 --> 00:07:31 launching astronauts or delicate

00:07:31 --> 00:07:33 telescopes.

00:07:33 --> 00:07:35 >> Definitely not. So it's for hardened

00:07:36 --> 00:07:37 cargo only.

00:07:37 --> 00:07:40 >> Exactly. Things like fuel, water,

00:07:40 --> 00:07:42 building materials, or ruggedized

00:07:42 --> 00:07:44 military satellites. But here's the

00:07:44 --> 00:07:47 payoff. Longot believes they can get the

00:07:47 --> 00:07:50 cost of launching a kilogram of cargo to

00:07:50 --> 00:07:52 just $10.

00:07:52 --> 00:07:54 >> $10. That's compared to thousands of

00:07:54 --> 00:07:56 dollars per kilogram on a traditional

00:07:56 --> 00:07:59 rocket. That's a complete gamecher for

00:07:59 --> 00:08:00 space logistics.

00:08:00 --> 00:08:03 >> It is. And that's why it's attracting

00:08:03 --> 00:08:05 serious interest from both venture

00:08:05 --> 00:08:08 capital and military agencies. If they

00:08:08 --> 00:08:10 can solve the engineering challenges,

00:08:10 --> 00:08:13 this space gun could revolutionize how

00:08:13 --> 00:08:16 we supply future operations in orbit and

00:08:16 --> 00:08:17 beyond.

00:08:17 --> 00:08:19 >> All right, let's bring our focus back to

00:08:19 --> 00:08:21 our own night sky. For all our

00:08:21 --> 00:08:23 stargazing listeners out there, one of

00:08:23 --> 00:08:25 the best celestial shows of the year is

00:08:25 --> 00:08:27 just around the corner.

00:08:27 --> 00:08:30 >> That's right. The Gemini meteor shower

00:08:30 --> 00:08:32 is set to peak on the night of December

00:08:32 --> 00:08:35 13th into the morning of the 14th. And

00:08:35 --> 00:08:37 this year, the conditions are just about

00:08:37 --> 00:08:39 perfect.

00:08:39 --> 00:08:41 >> What makes this year so good?

00:08:41 --> 00:08:44 >> The moon. It will be a waning crescent,

00:08:44 --> 00:08:46 which means it won't rise until the

00:08:46 --> 00:08:48 early hours of the morning, and its

00:08:48 --> 00:08:50 light won't wash out the fainter

00:08:50 --> 00:08:52 meteors. We'll have beautifully dark

00:08:52 --> 00:08:54 skies for most of the night.

00:08:54 --> 00:08:57 >> Fantastic. So, what can people expect to

00:08:57 --> 00:08:59 see?

00:08:59 --> 00:09:01 >> Under ideal conditions, you could see

00:09:01 --> 00:09:05 between 120 and 150 meteors per hour at

00:09:05 --> 00:09:08 the peak. The radiant, the point they

00:09:08 --> 00:09:10 appear to come from, is near the star

00:09:10 --> 00:09:14 castor in the constellation Gemini.

00:09:14 --> 00:09:16 >> And Geminites are known for being a bit

00:09:16 --> 00:09:18 slower, right? It makes them easier to

00:09:18 --> 00:09:19 spot.

00:09:19 --> 00:09:22 >> Yes, they enter the atmosphere at about

00:09:22 --> 00:09:25 22 m per second. That sounds fast, but

00:09:25 --> 00:09:27 it's slower than many other showers,

00:09:27 --> 00:09:30 which can lead to longer, more graceful

00:09:30 --> 00:09:33 streaks across the sky. They are also

00:09:33 --> 00:09:34 often brightly colored

00:09:34 --> 00:09:36 >> and they have a really interesting

00:09:36 --> 00:09:37 origin.

00:09:37 --> 00:09:39 >> They do. Unlike most meteor showers

00:09:40 --> 00:09:42 which come from the debris trail of a

00:09:42 --> 00:09:44 comet, the Geminids originate from an

00:09:44 --> 00:09:48 asteroid called 3200 Faithon. It's a bit

00:09:48 --> 00:09:50 of a mystery how this rocky body

00:09:50 --> 00:09:52 produces so much debris.

00:09:52 --> 00:09:54 >> So what are your tips for viewers?

00:09:54 --> 00:09:57 >> Find a location away from city lights.

00:09:57 --> 00:10:00 Dress warmly, lie back on a blanket or a

00:10:00 --> 00:10:03 chair, and just look up. You don't need

00:10:03 --> 00:10:06 a telescope or binoculars. Just give

00:10:06 --> 00:10:08 your eyes about 20 minutes to fully

00:10:08 --> 00:10:11 adapt to the dark and enjoy the show.

00:10:11 --> 00:10:13 And for our final story today, we are

00:10:13 --> 00:10:15 revisiting a cold case from the outer

00:10:15 --> 00:10:18 solar system and solving a mystery

00:10:18 --> 00:10:20 that's nearly four decades old.

00:10:20 --> 00:10:23 >> This has to be about Voyager 2's flyby

00:10:23 --> 00:10:26 of Uranus in 1986. I remember reading

00:10:26 --> 00:10:29 that it found something unexpected in

00:10:29 --> 00:10:31 the planet's radiation belts.

00:10:31 --> 00:10:33 >> That's the one. Voyager 2 detected an

00:10:34 --> 00:10:36 incredibly intense belt of high energy

00:10:36 --> 00:10:39 electron radiation, far more powerful

00:10:39 --> 00:10:42 than models had predicted. For decades,

00:10:42 --> 00:10:44 scientists couldn't quite explain why it

00:10:44 --> 00:10:45 was so strong.

00:10:45 --> 00:10:48 >> And after all this time, there's a new

00:10:48 --> 00:10:48 explanation.

00:10:48 --> 00:10:51 >> There is. A team at the Southwest

00:10:51 --> 00:10:53 Research Institute revisited the old

00:10:54 --> 00:10:56 Voyager data. They proposed the intense

00:10:56 --> 00:10:59 radiation wasn't caused by Uranus alone.

00:10:59 --> 00:11:02 Instead, it was a case of being in the

00:11:02 --> 00:11:04 right place at the right time.

00:11:04 --> 00:11:05 >> So, what was happening?

00:11:06 --> 00:11:08 >> The team believes a huge structure in

00:11:08 --> 00:11:10 the solar wind called a co-rotating

00:11:10 --> 00:11:13 interaction region was passing through

00:11:13 --> 00:11:16 the Uranian system just as Voyager 2

00:11:16 --> 00:11:17 flew by.

00:11:17 --> 00:11:19 >> A co-rotating what? Now,

00:11:19 --> 00:11:21 >> think of it as a massive shock wave in

00:11:21 --> 00:11:23 the solar wind where fast moving solar

00:11:23 --> 00:11:26 particles overtake slower ones. This

00:11:26 --> 00:11:28 interaction creates powerful

00:11:28 --> 00:11:30 highfrequency plasma waves like Whistler

00:11:30 --> 00:11:33 waves. These waves were the perfect

00:11:33 --> 00:11:35 frequency to grab electrons already

00:11:35 --> 00:11:37 trapped in Uranus's magnetic field and

00:11:38 --> 00:11:40 accelerate them to incredible speeds,

00:11:40 --> 00:11:42 creating that intense radiation belt

00:11:42 --> 00:11:45 Voyager saw. We see similar events

00:11:45 --> 00:11:48 happen near Earth, but this is the first

00:11:48 --> 00:11:50 time we've confirmed it happening so far

00:11:50 --> 00:11:51 out in the solar system.

00:11:51 --> 00:11:54 >> So, it was a temporary storm caused by

00:11:54 --> 00:11:56 the sun that Voyager just happened to

00:11:56 --> 00:11:59 fly through. That is a brilliant piece

00:11:59 --> 00:12:01 of cosmic detective work.

00:12:01 --> 00:12:01 >> You betcha.

00:12:01 --> 00:12:04 >> And that's a wrap. From mysterious

00:12:04 --> 00:12:06 interstellar visitors and hypersonic

00:12:06 --> 00:12:08 cannons to celebrating a 30-year-old

00:12:08 --> 00:12:12 hero of astronomy and finally solving a

00:12:12 --> 00:12:14 cold case from Uranus. What an episode.

00:12:14 --> 00:12:17 >> It really was. That's all the time we

00:12:17 --> 00:12:19 have for today on Astronomy Daily. We'd

00:12:19 --> 00:12:21 like to thank you all for tuning in.

00:12:21 --> 00:12:23 >> Join us next time as we continue to

00:12:23 --> 00:12:25 explore the wonders of the universe.

00:12:25 --> 00:12:28 Until then, clear skies everyone and

00:12:28 --> 00:12:31 remember to get out there and look up.

00:12:31 --> 00:12:34 Every day

00:12:34 --> 00:12:42 stories we told

00:12:42 --> 00:12:50 stories told

00:12:50 --> 00:12:52 stories