Launch Delays, Evolving Dark Matter, and Traces of a Catastrophic Solar Event
Astronomy Daily: Space News May 16, 2025x
117
00:18:0716.64 MB

Launch Delays, Evolving Dark Matter, and Traces of a Catastrophic Solar Event

Join Anna in this episode of Astronomy Daily as she navigates through a stellar array of updates from the cosmos, highlighting the latest breakthroughs and challenges in space exploration. Prepare for an informative journey that spans from the intricacies of SpaceX's Starship program to groundbreaking discoveries at the heart of our galaxy.
Highlights:
- SpaceX's Starship Flight 9 Update: Dive into the latest developments as the FAA gives a conditional green light for SpaceX's ninth Starship flight following the explosive mishap of Flight 8. Discover the implications for air travel and the ambitious plans for the future of space exploration.
- Gilmour Space Technologies' Launch Delay: Learn about the recent postponement of Australia's first sovereign orbital launch attempt due to a nose cone malfunction. Despite the setback, the team remains optimistic about the future of Australian aerospace engineering.
- Planet Formation in Galactic Center: Explore the astonishing discovery of protoplanetary disks forming in the extreme conditions of the Milky Way's center, challenging previous notions of planetary formation and expanding our understanding of the universe.
- Evolving Dark Matter Theory: Delve into a novel proposal suggesting that dark matter may evolve over time, offering fresh insights into the Hubble tension problem and opening new avenues for research in cosmology.
- Evidence of Ancient Solar Storm: Uncover the findings surrounding the most violent solar storm in recorded history, which struck Earth 14,300 years ago. Learn how this event could inform modern space weather preparedness in our technology-dependent world.
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 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 - SpaceX's Starship Flight 9 update
10:00 - Gilmour Space Technologies' launch delay
15:30 - Planet formation in the Milky Way's center
20:00 - Evolving dark matter theory
25:00 - Evidence of ancient solar storm
✍️ Episode References
SpaceX Starship Updates
[SpaceX](https://www.spacex.com/)
Gilmour Space Technologies
[Gilmour Space](https://gilmourspace.com/)
Protoplanetary Disks Research
[Peking University](https://www.pku.edu.cn/)
Dark Matter Theory
[University of Cologne](https://www.uni-koeln.de/en/)
Ancient Solar Storm Findings
[Climate Chemistry Model](https://www.sciencedirect.com/science/article/pii/S0921818121002175)
Astronomy Daily
[Astronomy Daily](http://www.astronomydaily.io/)

Become a supporter of this podcast: https://www.spreaker.com/podcast/astronomy-daily-exciting-space-discoveries-and-news--5648921/support.


00:00:00 --> 00:00:03 Anna: Welcome to Astronomy Daily, your cosmic companion

00:00:03 --> 00:00:06 for all things space. I'm Anna, and

00:00:06 --> 00:00:09 I'm thrilled to bring you today's celestial roundup of

00:00:09 --> 00:00:11 the most fascinating developments from across the universe.

00:00:12 --> 00:00:15 Today we're exploring a diverse constellation of

00:00:15 --> 00:00:18 space news that spans from our own backyard to the very

00:00:18 --> 00:00:21 heart of our galaxy. We'll start with the latest on

00:00:21 --> 00:00:24 SpaceX's Starship program, where the FAA

00:00:24 --> 00:00:27 has made some crucial decisions about Flight 9 following

00:00:27 --> 00:00:30 March's explosive setback. Then we'll jet off

00:00:30 --> 00:00:32 to Australia, where a Histor rocket second launch

00:00:32 --> 00:00:35 attempt was scrubbed at the last minute due to an

00:00:35 --> 00:00:38 unexpected glitch. With a most peculiar payload

00:00:38 --> 00:00:41 aboard, our journey takes us deeper into space

00:00:41 --> 00:00:43 as we discover something truly remarkable.

00:00:44 --> 00:00:46 Planets forming in the extreme environment at the center of our

00:00:46 --> 00:00:49 Milky Way, challenging what scientists thought possible

00:00:49 --> 00:00:52 about planetary formation. We'll

00:00:52 --> 00:00:55 also delve into theoretical physics with a fascinating new

00:00:55 --> 00:00:58 proposal about dark matter. Could this

00:00:58 --> 00:01:01 mysterious substance actually be evolving over time?

00:01:01 --> 00:01:04 The answer might solve one of cosmology most

00:01:04 --> 00:01:07 persistent puzzles. And finally, we'll travel

00:01:07 --> 00:01:10 back in time to discover evidence of what may be the most

00:01:10 --> 00:01:12 violent solar storm ever to hit Earth. A

00:01:12 --> 00:01:15 cosmic event so powerful it left traces we can still

00:01:15 --> 00:01:18 detect 14 years later.

00:01:19 --> 00:01:21 So buckle up for a journey across space and time as we

00:01:21 --> 00:01:24 explore today's biggest astronomical breakthroughs.

00:01:25 --> 00:01:28 Let's m start with some SpaceX news. The

00:01:28 --> 00:01:31 Federal Aviation Administration has given SpaceX a

00:01:31 --> 00:01:34 conditional green light for its ninth Starship flight,

00:01:34 --> 00:01:37 approving license modifications but stopping short of

00:01:37 --> 00:01:39 authorizing an immediate launch. This decision

00:01:39 --> 00:01:42 comes in the wake of Flight 8's explosion in March,

00:01:43 --> 00:01:45 which created significant disruptions in our skies.

00:01:46 --> 00:01:49 Before Elon Musk's massive rocket can take to the

00:01:49 --> 00:01:52 launch pad again, SpaceX must wait for the

00:01:52 --> 00:01:55 FAA to either close its investigation into the

00:01:55 --> 00:01:57 Flight 8 mishap or make a specific return to

00:01:57 --> 00:02:00 flight determination. As you might recall,

00:02:00 --> 00:02:03 the previous test ended dramatically when the spacecraft

00:02:03 --> 00:02:06 began spinning uncontrollably with its engines cut off

00:02:06 --> 00:02:09 before exploding in space. That incident

00:02:09 --> 00:02:11 wasn't just a setback for SpaceX. It

00:02:11 --> 00:02:14 disrupted approximately 240 flights with

00:02:14 --> 00:02:17 space debris concerns forcing more than 24 aircraft

00:02:17 --> 00:02:20 into diversions. It's a stark reminder that even

00:02:20 --> 00:02:23 events happening in space can have very real consequences

00:02:23 --> 00:02:26 for air travel here on Earth. The

00:02:26 --> 00:02:29 FAA is currently reviewing SpaceX's mishap

00:02:29 --> 00:02:31 report, which was only submitted on May

00:02:31 --> 00:02:34 14. When Flight 9 does eventually launch,

00:02:34 --> 00:02:37 we'll see expanded safety measures, including larger

00:02:37 --> 00:02:40 aircraft and maritime hazard areas, both in the United States

00:02:40 --> 00:02:43 and other countries. This expansion stems

00:02:43 --> 00:02:46 directly from the March explosion and reflects Another

00:02:46 --> 00:02:49 notable first, SpaceX plans to

00:02:49 --> 00:02:51 reuse a UH previously launched super heavy booster

00:02:51 --> 00:02:54 rocket, marking an important milestone in the company's

00:02:54 --> 00:02:57 reusability goals. The impact on air travel will

00:02:57 --> 00:03:00 be substantial when the launch eventually proceeds.

00:03:01 --> 00:03:03 The flight path will affect air routes extending

00:03:03 --> 00:03:06 1 nautical miles eastward from

00:03:06 --> 00:03:08 Texas through the Straits of Florida.

00:03:09 --> 00:03:12 Both the Bahamas and Turks and Caicos are expected

00:03:12 --> 00:03:14 to close their airspace up to 6ft,

00:03:15 --> 00:03:17 while the FAA will close airspace above that level.

00:03:18 --> 00:03:20 All told, the agency estimates about

00:03:20 --> 00:03:22 175 flights will be affected.

00:03:23 --> 00:03:26 In a separate but related decision, the FAA

00:03:26 --> 00:03:29 has also approved increasing the number of launches at

00:03:29 --> 00:03:32 SpaceX's Boca Chica, Texas

00:03:32 --> 00:03:34 facility from five to as many as 25,

00:03:35 --> 00:03:38 a significant expansion of operations that

00:03:38 --> 00:03:41 had actually been announced back in March. While these

00:03:41 --> 00:03:43 setbacks may seem disappointing, it's worth

00:03:43 --> 00:03:46 remembering the ambitious nature of what SpaceX is

00:03:46 --> 00:03:49 attempting to the Starship system stands at a

00:03:49 --> 00:03:51 towering 403ft and represents the

00:03:51 --> 00:03:54 centerpiece of Musk's vision to eventually send

00:03:54 --> 00:03:57 humans to Mars, potentially as soon as the turn of the decade.

00:03:58 --> 00:04:01 The March explosion marked the second consecutive failure

00:04:01 --> 00:04:03 in SpaceX's test launch program, following

00:04:03 --> 00:04:06 another explosion in the seventh test flight.

00:04:06 --> 00:04:09 Both incidents occurred during early mission phases that

00:04:09 --> 00:04:12 SpaceX had previously navigated successfully,

00:04:12 --> 00:04:15 highlighting the ongoing challenges in developing such

00:04:15 --> 00:04:16 revolutionary technology.

00:04:18 --> 00:04:21 Next, an update from Australia in what

00:04:21 --> 00:04:23 would have been a historic moment for Australia's space industry,

00:04:24 --> 00:04:27 Gilmour Space Technologies has been forced to postpone

00:04:27 --> 00:04:29 its eagerly anticipated rocket launch after

00:04:29 --> 00:04:32 discovering a glitch in the nose cone mechanism.

00:04:33 --> 00:04:36 This would have marked the first time an Australian made rocket

00:04:36 --> 00:04:39 reached orbit from Australian soil. M

00:04:39 --> 00:04:42 the company reported Friday that an electrical fault erroneously

00:04:42 --> 00:04:44 triggered the opening mechanism of the carbon fiber nose

00:04:44 --> 00:04:47 cone during pre flight testing. In short,

00:04:47 --> 00:04:50 the nose cone fell off. This

00:04:50 --> 00:04:53 critical component is designed to shield the payload,

00:04:53 --> 00:04:55 in this case, quite charmingly, a jar of

00:04:55 --> 00:04:58 vegemite as the rocket ascends through Earth's

00:04:58 --> 00:05:01 atmosphere. Fortunately, the mishap

00:05:01 --> 00:05:04 occurred before fueling began at the company's spaceport near

00:05:04 --> 00:05:06 Bowen, a coastal township situated about

00:05:06 --> 00:05:09 1000km north of Brisbane in Queensland.

00:05:09 --> 00:05:12 Both the rocket and ground crew were unharmed in the incident.

00:05:13 --> 00:05:16 CEO Adam Gilmour maintained an optimistic

00:05:16 --> 00:05:19 outlook despite the setback, stating, while we're

00:05:19 --> 00:05:21 disappointed by the delay, we're already working through a

00:05:21 --> 00:05:24 resolution and expect to be back on the pad soon.

00:05:24 --> 00:05:27 He emphasized that safety remains their highest

00:05:27 --> 00:05:30 priority, a sentiment echoed by communications

00:05:30 --> 00:05:33 chief Michelle Gilmour, who noted that the team

00:05:33 --> 00:05:35 is accustomed to such challenges. We do

00:05:35 --> 00:05:37 rockets, they are used to setbacks.

00:05:38 --> 00:05:41 The 23 meter 3 stage ARIS rocket

00:05:41 --> 00:05:44 represents a significant achievement in Australian

00:05:44 --> 00:05:47 aerospace engineering. Weighing 30 tons when

00:05:47 --> 00:05:49 fully fueled, it employs a hybrid propulsion

00:05:49 --> 00:05:52 system combining solid inert fuel with a

00:05:52 --> 00:05:55 liquid oxidizer. The team expects the delay

00:05:55 --> 00:05:58 to last at least a few weeks as they transport a

00:05:58 --> 00:06:01 replacement nose cone to the launch site. This

00:06:01 --> 00:06:04 postponement follows another delay just the previous day

00:06:04 --> 00:06:07 caused by a bug in the external power system used for

00:06:07 --> 00:06:10 system checks. These consecutive

00:06:10 --> 00:06:13 setbacks highlight the inherent challenges in rocket

00:06:13 --> 00:06:15 development, even for a company with a decade of

00:06:15 --> 00:06:18 experience in the field. The choice of

00:06:18 --> 00:06:21 Vegemite as payload speaks to the Australian

00:06:21 --> 00:06:24 character of the mission, with Michelle Gilmour describing the

00:06:24 --> 00:06:26 iconic spread as hardy, resilient, like

00:06:26 --> 00:06:29 Ozzies. The payload reportedly remained

00:06:29 --> 00:06:31 intact despite the nosecone malfunction.

00:06:32 --> 00:06:35 With 230 employees and backing from venture

00:06:35 --> 00:06:38 capital group Blackbird and pension fund Hesta,

00:06:38 --> 00:06:41 Gilmour, Space Technologies has ambitious plans.

00:06:41 --> 00:06:44 While this test flight has been delayed, the company

00:06:44 --> 00:06:47 remains focused on beginning commercial launches by

00:06:47 --> 00:06:49 late 2026 or early 2027,

00:06:50 --> 00:06:53 potentially establishing Australia as a significant player

00:06:53 --> 00:06:56 in in the increasingly competitive commercial space launch

00:06:56 --> 00:06:56 industry.

00:06:58 --> 00:07:00 Let's move on out to some space news. In a uh,

00:07:00 --> 00:07:03 groundbreaking discovery that challenges our understanding of

00:07:03 --> 00:07:06 planetary formation, astronomers have found

00:07:06 --> 00:07:08 evidence of protoplanetary disks forming in the most

00:07:08 --> 00:07:11 extreme environment of our galaxy, its very

00:07:11 --> 00:07:14 center. An international team from Peking

00:07:14 --> 00:07:17 University, the Shanghai Astronomical Observatory,

00:07:17 --> 00:07:20 and the University of Cologne conducted the most

00:07:20 --> 00:07:22 detailed survey yet of the Milky Way's central

00:07:22 --> 00:07:25 molecular zone, or cmz,

00:07:25 --> 00:07:28 revealing that planets may be forming in places we never

00:07:28 --> 00:07:31 expected. Protoplanetary disks

00:07:31 --> 00:07:33 are essentially cosmic nurseries, swirling

00:07:33 --> 00:07:36 rings of gas and dust surrounding young stars where

00:07:36 --> 00:07:39 planets are born. Within these structures,

00:07:39 --> 00:07:42 tiny dust particles collide and stick together,

00:07:42 --> 00:07:45 gradually building into pebbles, boulders, and eventually

00:07:45 --> 00:07:48 planetary embryos through a process called core

00:07:48 --> 00:07:51 accretion. As these embryonic planets

00:07:51 --> 00:07:53 grow, they leave behind distinctive patterns that

00:07:53 --> 00:07:56 astronomers can detect with advanced telescopes.

00:07:56 --> 00:07:59 What makes this discovery so remarkable is the location.

00:08:00 --> 00:08:02 The galactic center presents incredibly harsh

00:08:02 --> 00:08:05 conditions with intense radiation, strong

00:08:05 --> 00:08:08 magnetic fields, and turbulent gas clouds,

00:08:08 --> 00:08:11 environments previously thought hostile to planet

00:08:11 --> 00:08:14 formation. Yet the research team identified

00:08:14 --> 00:08:16 over 500 dense cores where stars are

00:08:16 --> 00:08:19 forming under these remarkably different conditions.

00:08:20 --> 00:08:23 Detecting these systems was no small feat. The central

00:08:23 --> 00:08:25 molecular zone is approximately 17 billion

00:08:25 --> 00:08:28 astronomical units away and heavily obscured by dust.

00:08:28 --> 00:08:31 To overcome these challenges, the team employed the

00:08:31 --> 00:08:34 Atacama Large Millimeter Array, or alma,

00:08:34 --> 00:08:37 in Chile. This powerful radio telescope

00:08:37 --> 00:08:39 combines signals from widely spaced antennas to achieve

00:08:39 --> 00:08:42 extraordinary resolution, allowing researchers to observe

00:08:42 --> 00:08:45 structures as small as 1 astronomical

00:08:45 --> 00:08:48 units. Despite the immense distance, the team

00:08:48 --> 00:08:50 used a clever approach called dual band imaging

00:08:51 --> 00:08:53 Capturing two wavelengths at the same resolution to gather

00:08:53 --> 00:08:56 critical data on temperature, dust composition

00:08:56 --> 00:08:59 and structure. What particularly

00:08:59 --> 00:09:02 surprised researchers was that over 70% of

00:09:02 --> 00:09:05 the dense cores Appeared redder than expected,

00:09:05 --> 00:09:08 suggesting the presence of protoplanetary disks.

00:09:09 --> 00:09:12 As Feng Weishu from the University of Cologne's

00:09:12 --> 00:09:14 Institute of Astrophysics described it, we were

00:09:14 --> 00:09:17 astonished to see these little red dots across the

00:09:17 --> 00:09:20 whole molecular clouds. They are telling us the hidden

00:09:20 --> 00:09:23 nature of dense star forming cores.

00:09:23 --> 00:09:26 The findings suggest there may be over 300 potential

00:09:26 --> 00:09:29 disk forming systems in just three CMZ clouds,

00:09:29 --> 00:09:32 opening a new window into how planetary systems might form

00:09:32 --> 00:09:35 under radically different conditions Than those near our

00:09:35 --> 00:09:38 Sun. This diversity in planet forming

00:09:38 --> 00:09:40 environments could have profound implications for our

00:09:40 --> 00:09:43 understanding of exoplanet populations such as throughout

00:09:43 --> 00:09:46 the Galaxy. If planets can form in the

00:09:46 --> 00:09:49 turbulent high pressure environment at the galactic center,

00:09:49 --> 00:09:52 it suggests the building blocks of planetary systems

00:09:52 --> 00:09:55 Are far more resilient and adaptable than

00:09:55 --> 00:09:58 previously thought. As astronomers continue to

00:09:58 --> 00:10:00 study these distant protoplanetary disks, we

00:10:00 --> 00:10:03 may soon discover whether these early formations can

00:10:03 --> 00:10:06 indeed evolve into full planetary systems and

00:10:06 --> 00:10:09 how such processes might differ across the vast

00:10:09 --> 00:10:11 expanse of the Milky Way.

00:10:12 --> 00:10:15 Next up, everybody's favorite subject, dark matter.

00:10:15 --> 00:10:18 For a while now, cosmologists have been wrestling with a

00:10:18 --> 00:10:21 perplexing mystery known as the Hubble tension problem.

00:10:21 --> 00:10:24 While observations consistently support the expanding

00:10:24 --> 00:10:27 universe model, There's a troubling discrepancy.

00:10:27 --> 00:10:30 Measurements from the early cosmos show a lower

00:10:30 --> 00:10:32 acceleration rate Than what we observe locally.

00:10:33 --> 00:10:36 This inconsistency has led scientists to propose

00:10:36 --> 00:10:39 numerous potential solutions, from questioning

00:10:39 --> 00:10:41 general relativity to rethinking dark matter

00:10:41 --> 00:10:44 entirely. Now a fascinating new

00:10:44 --> 00:10:47 theory has emerged that puts a fresh spin on

00:10:47 --> 00:10:50 dark matter. What if it evolves over time?

00:10:50 --> 00:10:53 This concept is particularly novel because, while evolving

00:10:53 --> 00:10:56 dark energy has been proposed before, the idea of dark

00:10:56 --> 00:10:59 matter changing over time hasn't received much attention from

00:10:59 --> 00:11:01 researchers. There are good reasons for this

00:11:01 --> 00:11:04 oversight. First, we have excellent observational

00:11:04 --> 00:11:07 evidence for dark matter. It appears to be some kind

00:11:07 --> 00:11:10 of material that doesn't interact strongly with light,

00:11:10 --> 00:11:13 perfectly explaining galaxy rotation curves and

00:11:13 --> 00:11:16 gravitational lensing. The only major gap is

00:11:16 --> 00:11:18 our inability to directly detect dark matter

00:11:18 --> 00:11:21 particles. Second, most critics of

00:11:21 --> 00:11:24 dark matter theory Focus on eliminating it entirely through

00:11:24 --> 00:11:27 alternative M models like modified gravity, rather

00:11:27 --> 00:11:30 than refining the concept. What makes this

00:11:30 --> 00:11:32 new approach interesting is how it flips. Uh, our thinking.

00:11:33 --> 00:11:36 Researchers have found that models with evolving dark

00:11:36 --> 00:11:38 matter and constant dark energy can produce

00:11:38 --> 00:11:41 results similar to those with constant dark matter and

00:11:41 --> 00:11:44 evolving dark energy. To match observations,

00:11:45 --> 00:11:48 they propose that dark matter must have a changeable

00:11:48 --> 00:11:50 equation of state that oscillates over time.

00:11:51 --> 00:11:53 This isn't actually as strange as it might sound.

00:11:54 --> 00:11:56 Consider neutrinos. They have mass,

00:11:57 --> 00:12:00 don't interact strongly with light, and are effectively

00:12:00 --> 00:12:03 a form of hot dark matter, Though they can't account

00:12:03 --> 00:12:04 for all the dark matter in the universe.

00:12:06 --> 00:12:08 Importantly, neutrinos undergo mass oscillation.

00:12:09 --> 00:12:12 Perhaps cold dark matter particles experience something similar.

00:12:13 --> 00:12:16 The researcher's model suggests that roughly

00:12:16 --> 00:12:18 15% of cold dark matter might be

00:12:18 --> 00:12:21 oscillatory, with the remaining 85%

00:12:21 --> 00:12:23 being standard dark matter. This combination

00:12:23 --> 00:12:26 would address the Hubble tension while remaining consistent

00:12:26 --> 00:12:28 with our other dark matter observations.

00:12:29 --> 00:12:32 It's worth emphasizing that this remains a conceptual um,

00:12:32 --> 00:12:34 model without specific constraints for dark matter

00:12:34 --> 00:12:37 particles. The researchers themselves

00:12:37 --> 00:12:40 describe it as a toy model, a simplified

00:12:40 --> 00:12:43 framework that captures essential features while omitting

00:12:43 --> 00:12:45 details. Nevertheless, it opens an

00:12:45 --> 00:12:48 intriguing new avenue for dark matter research that

00:12:48 --> 00:12:51 broadens our thinking beyond conventional models

00:12:51 --> 00:12:54 as we continue to gather data and refine our understanding of

00:12:54 --> 00:12:57 the cosmos. Evolving dark matter might prove

00:12:57 --> 00:13:00 to be a valuable piece in solving one of astrophysics most

00:13:00 --> 00:13:03 persistent puzzles. At the very least, it

00:13:03 --> 00:13:06 demonstrates how creative thinking can help us tackle even the

00:13:06 --> 00:13:08 most fundamental questions about our universe.

00:13:09 --> 00:13:12 Finally, today, a little history lesson. Imagine

00:13:12 --> 00:13:15 discovering that 14 years

00:13:15 --> 00:13:18 ago, our planet was struck by a cosmic event

00:13:18 --> 00:13:21 so powerful it left physical evidence that

00:13:21 --> 00:13:24 scientists can still detect today. That's

00:13:24 --> 00:13:26 exactly what researchers have uncovered. The most

00:13:26 --> 00:13:28 violent solar storm in recorded history,

00:13:29 --> 00:13:32 dwarfing anything we've experienced in modern times.

00:13:32 --> 00:13:35 By examining partially fossilized tree trunks and ancient

00:13:35 --> 00:13:38 ice cores, scientists found unmistakable

00:13:38 --> 00:13:41 signatures of an extraordinary event that occurred around

00:13:41 --> 00:13:43 12 BCE.

00:13:44 --> 00:13:46 Using a specially developed climate chemistry model called

00:13:46 --> 00:13:47 SOCOL,

00:13:49 --> 00:13:52 researchers have now confirmed this was a massive solar storm, the

00:13:52 --> 00:13:55 biggest we've ever found evidence for. To put this

00:13:55 --> 00:13:57 in perspective, the ancient storm was more than

00:13:57 --> 00:14:00 500 times more intense than the largest event of the

00:14:00 --> 00:14:03 modern satellite era, which occurred in 2005. That's

00:14:03 --> 00:14:06 simply staggering when you consider the potential impacts.

00:14:07 --> 00:14:10 For those wondering how scientists can possibly know about something

00:14:10 --> 00:14:13 that happened so long ago, the answer lies in

00:14:13 --> 00:14:16 radioactive carbon 14. When the sun

00:14:16 --> 00:14:19 unleashes a, uh, powerful coronal mass ejection,

00:14:19 --> 00:14:22 essentially billions of tons of plasma with embedded

00:14:22 --> 00:14:24 magnetic fields, the particles interact with our

00:14:24 --> 00:14:27 atmosphere to temporarily increase carbon 14

00:14:27 --> 00:14:30 production. This carbon 14 gets

00:14:30 --> 00:14:32 incorporated into living organisms like trees,

00:14:32 --> 00:14:35 creating a distinctive spike in tree rings from that period.

00:14:36 --> 00:14:38 Since carbon 14 decays at a known rate,

00:14:39 --> 00:14:41 scientists can precisely date these events and even determine their

00:14:41 --> 00:14:44 relative strength. What makes the

00:14:44 --> 00:14:47 12 before Common Era event

00:14:47 --> 00:14:49 particularly significant is that it's the only

00:14:50 --> 00:14:53 known extreme solar particle event outside

00:14:53 --> 00:14:56 the Holocene epoch, the relatively stable

00:14:56 --> 00:14:58 warm climate period of the past 12 years.

00:14:59 --> 00:15:02 This required the researchers to develop new modeling

00:15:02 --> 00:15:05 approaches that could analyze radiocarbon data

00:15:05 --> 00:15:07 under different climate conditions. The

00:15:07 --> 00:15:10 implications for our modern world are sobering.

00:15:10 --> 00:15:13 We've already seen how smaller solar storms can

00:15:13 --> 00:15:16 disrupt technology like the carrington event

00:15:16 --> 00:15:19 of 1859, which set telegraph

00:15:19 --> 00:15:22 systems ablaze worldwide, or the 1989

00:15:22 --> 00:15:24 storm that caused multiple power grid failures.

00:15:25 --> 00:15:28 Now imagine something hundreds of times more powerful

00:15:28 --> 00:15:30 hitting our satellite dependent, electronically

00:15:30 --> 00:15:33 interconnected civilization. This discovery

00:15:33 --> 00:15:36 establishes a new worst case scenario for space

00:15:36 --> 00:15:39 weather preparedness. Understanding the potential

00:15:39 --> 00:15:42 scale of these events is crucial for evaluating risks

00:15:42 --> 00:15:45 to modern infrastructure, from power grids and

00:15:45 --> 00:15:48 communication systems to the satellites that enable everything

00:15:48 --> 00:15:51 from GPS navigation to weather forecasting.

00:15:52 --> 00:15:54 While such extreme events appear to be rare on human

00:15:54 --> 00:15:57 timescales, this research reminds us that the

00:15:57 --> 00:16:00 sun is capable of far more violent outbursts than anything

00:16:00 --> 00:16:03 we've witnessed in recent centuries. As we

00:16:03 --> 00:16:05 become increasingly dependent on vulnerable technologies,

00:16:06 --> 00:16:08 the importance of space weather monitoring and developing

00:16:08 --> 00:16:11 resilient systems becomes even more critical.

00:16:12 --> 00:16:15 This ancient solar tantrum, preserved in the rings of

00:16:15 --> 00:16:17 trees that stood witness to its fury, serves as

00:16:17 --> 00:16:20 both a scientific treasure and a warning from the distant past.

00:16:22 --> 00:16:25 And on that somber note, that wraps up another fascinating

00:16:25 --> 00:16:28 journey through our cosmos. From the earthbound

00:16:28 --> 00:16:31 challenges facing SpaceX's Starship and Australia's

00:16:31 --> 00:16:34 budding rocket program, to the mind bending

00:16:34 --> 00:16:36 discoveries of planets forming in our galaxy's heart

00:16:37 --> 00:16:40 and the possibility of evolving dark matter, we've

00:16:40 --> 00:16:42 covered quite the astronomical landscape today.

00:16:43 --> 00:16:46 And that ancient solar storm revelation really puts

00:16:46 --> 00:16:48 things in perspective, doesn't it? A cosmic

00:16:48 --> 00:16:51 event 500 times more powerful than anything we've

00:16:51 --> 00:16:54 experienced in modern times reminds us just how

00:16:54 --> 00:16:57 dynamic and sometimes temperamental our stellar

00:16:57 --> 00:17:00 companion can be. I'm Anna and I've been

00:17:00 --> 00:17:03 your guide through today's cosmic headlines on Astronomy

00:17:03 --> 00:17:06 Daily. If you enjoyed this episode and want to keep

00:17:06 --> 00:17:08 up with all the latest developments in space science and

00:17:08 --> 00:17:11 exploration, I invite you to visit our

00:17:11 --> 00:17:13 website@astronomydaily.IO

00:17:14 --> 00:17:16 where you can sign up for our free daily newsletter.

00:17:17 --> 00:17:19 There you'll also find our complete archive

00:17:19 --> 00:17:22 of past episodes ready for you to

00:17:22 --> 00:17:25 explore at your leisure. Don't forget to

00:17:25 --> 00:17:28 subscribe to Astronomy Daily on Apple Podcasts, Spotify,

00:17:28 --> 00:17:31 YouTubeMusic, or wherever you get your podcasts. To ensure you

00:17:31 --> 00:17:34 never miss an episode, Each day brings new

00:17:34 --> 00:17:36 discoveries and insights into our fascinating universe,

00:17:36 --> 00:17:39 and I'd love to share them with you. Until

00:17:39 --> 00:17:42 tomorrow, keep looking up the cosmos never ceases

00:17:42 --> 00:17:43 to amaze.