Runaway Black Hole Confirmed, Mercury Still Active & 2032 Moon Impact Risk
Astronomy Daily: Space News January 29, 2026x
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00:20:1618.61 MB

Runaway Black Hole Confirmed, Mercury Still Active & 2032 Moon Impact Risk

AnnaAnnaHost
Join hosts Anna and Avery for an exciting journey through today's most compelling space stories. We explore Mercury's surprising geological activity, NASA's TESS satellite recovery, a frigid Earth-like exoplanet discovery, an accelerated ISS crew launch, runaway black holes tearing through space, and the scientific opportunities of a potential lunar asteroid impact in 2032.
### Episode Highlights
**Mercury's Hidden Activity**
New research reveals that Mercury, long considered geologically dead, is still actively losing volatile materials from its interior. Using AI analysis of 100,000 MESSENGER images, scientists have mapped 400 bright slope streaks that indicate ongoing geological processes. The BepiColombo mission will provide unprecedented new data when it arrives at Mercury.
**TESS Satellite Recovery**
NASA's planet-hunting TESS satellite recently entered safe mode after a command error caused solar panel misalignment. The spacecraft successfully recovered, demonstrating the importance of built-in safeguards. NASA is reviewing procedures to prevent future incidents.
**Ice-Cold Earth Twin**
Astronomers have discovered HD 137010 b, an Earth-like exoplanet 146 light-years away that could be as cold as minus 90°F. Despite frigid temperatures, it orbits within its star's habitable zone, offering insights into the diversity of potentially habitable worlds.
**Crew-12 Launch Advanced**
SpaceX and NASA have moved up the Crew-12 launch to February 11, four days earlier than planned, to provide relief for the three-person skeleton crew managing the ISS after the first-ever medical evacuation from the station.
**Runaway Black Holes Confirmed**
The James Webb Space Telescope has confirmed the first runaway supermassive black hole, ejected from its galaxy and leaving a 200,000 light-year trail of newborn stars. Traveling at 1,600 km/s, this discovery validates 50-year-old theoretical predictions.
**Moon Impact Opportunity**
Asteroid 2024 YR4 has a 4% chance of striking the Moon on December 22, 2032. While posing risks to satellites and Earth, such an impact would provide unprecedented scientific data on lunar geology, create spectacular meteor displays, and deliver free lunar samples to Earth.
### Featured Stories
1. **Mercury Still Geologically Active** - University of Bern researchers discover 400 bright streaks indicating ongoing volatile loss (Source: Space Daily)
2. **TESS Satellite Command Error** - NASA's exoplanet hunter recovers from safe mode after solar panel misalignment (Source: Daily Galaxy)
3. **Frigid Earth-Like Planet Discovery** - HD 137010 b joins the search for Earth's twin despite extreme cold (Source: Daily Galaxy)
4. **ISS Crew-12 Launch Moved Up** - February 11 launch provides relief after historic medical evacuation (Source: Space.com)
5. **First Confirmed Runaway Black Hole** - JWST observations validate theoretical predictions with stunning stellar trail (Source: Phys.org/Science Sources)
6. **Asteroid 2024 YR4 Lunar Impact** - 4% chance creates scientific opportunity and satellite risk in 2032 (Source: Universe Today)
### Hosts
Anna and Avery
### Links & Resources
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- Social Media: @AstroDailyPod (X, Facebook, Instagram, YouTube)
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This episode includes AI-generated content.


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

00:00:03 --> 00:00:05 source for the latest space and astronomy

00:00:05 --> 00:00:07 news. I'm Anna.

00:00:07 --> 00:00:09 Avery: And I'm Avery. Thanks for joining us on this

00:00:09 --> 00:00:12 Thursday, February 29, 2026.

00:00:12 --> 00:00:15 We've got a fascinating lineup today covering

00:00:15 --> 00:00:17 everything from Mercury's surprising

00:00:17 --> 00:00:19 geological activity to a possible

00:00:19 --> 00:00:21 asteroid impact on the M Moon.

00:00:21 --> 00:00:24 Anna: That's right. We're going to explore bright

00:00:24 --> 00:00:27 streaks on Mercury that suggest our

00:00:27 --> 00:00:29 smallest planet is still geologically

00:00:29 --> 00:00:32 active. Cheque in on NASA's TESS

00:00:32 --> 00:00:35 satellite after a command error temporarily

00:00:35 --> 00:00:38 sidelined it and discuss the discovery of an

00:00:38 --> 00:00:41 intriguing Earth like exoplanet that's

00:00:41 --> 00:00:42 much colder than you might expect.

00:00:43 --> 00:00:45 Avery: Plus, we'll bring you updates on NASA and

00:00:45 --> 00:00:48 SpaceX. Moving up the Crew 12 launch to help

00:00:48 --> 00:00:49 out the Skeleton crew currently on the

00:00:49 --> 00:00:52 International Space Station. Then we'll dive

00:00:52 --> 00:00:54 into the wild world of runaway black holes

00:00:54 --> 00:00:57 tearing through space and wrap up with what

00:00:57 --> 00:00:59 could be a once in a lifetime scientific

00:00:59 --> 00:01:02 opportunity if an asteroid hits the moon in

00:01:02 --> 00:01:03 2020 32.

00:01:03 --> 00:01:04 Anna: It's quite a ride.

00:01:04 --> 00:01:07 Today, let's get started with some surprising

00:01:07 --> 00:01:10 news from the innermost planet in our solar

00:01:10 --> 00:01:10 system.

00:01:11 --> 00:01:13 Avery: Mercury has long been viewed as a small,

00:01:13 --> 00:01:16 geologically dead world, but new research

00:01:16 --> 00:01:19 is challenging that assumption in a big way.

00:01:19 --> 00:01:21 A team led by researchers at the University

00:01:21 --> 00:01:24 of Bern has uncovered hundreds of bright

00:01:24 --> 00:01:27 linear streaks on crater slopes that point to

00:01:27 --> 00:01:30 ongoing volcanic activity and and volatile

00:01:30 --> 00:01:31 laws from Mercury's interior.

00:01:32 --> 00:01:34 Anna: This is really fascinating work, Avery.

00:01:34 --> 00:01:37 The team applied deep learning techniques to

00:01:37 --> 00:01:40 analyse about 100 high

00:01:40 --> 00:01:42 resolution images taken by NASA's

00:01:42 --> 00:01:45 messenger spacecraft during its orbital

00:01:45 --> 00:01:47 mission from 2011 to 2015.

00:01:48 --> 00:01:51 Using this automated approach, they mapped

00:01:51 --> 00:01:53 the global distribution of roughly

00:01:53 --> 00:01:56 400 bright streaks that had previously

00:01:56 --> 00:01:58 escaped comprehensive cataloguing.

00:01:58 --> 00:02:01 Avery: And what they found was pretty telling. These

00:02:01 --> 00:02:04 features, known as slope lineae, occur

00:02:04 --> 00:02:06 preferentially on sun facing slopes inside

00:02:06 --> 00:02:09 relatively young impact craters that cut

00:02:09 --> 00:02:11 through thick volcanic deposits. The

00:02:11 --> 00:02:13 concentration of streaks in these thermally

00:02:13 --> 00:02:16 stressed environments indicates that solar

00:02:16 --> 00:02:18 heating is an important trigger for volatile

00:02:18 --> 00:02:20 escape from near surface layers.

00:02:20 --> 00:02:23 Anna: Much of these streaks originate in small

00:02:23 --> 00:02:26 bright depressions called hollows that dot

00:02:26 --> 00:02:29 crater floors and walls. These hollows have

00:02:29 --> 00:02:32 long been interpreted as products of volatile

00:02:32 --> 00:02:35 loss, and their close association with the

00:02:35 --> 00:02:38 lineae supports the view that both structures

00:02:38 --> 00:02:41 form when volatile components like sulphur

00:02:41 --> 00:02:43 or other light elements escape from the

00:02:43 --> 00:02:44 subsurface.

00:02:44 --> 00:02:47 Avery: According to the research team, fracture

00:02:47 --> 00:02:49 networks created by the original impact

00:02:49 --> 00:02:51 events likely provide pathways that allow

00:02:51 --> 00:02:54 volatile rich material from deeper levels to

00:02:54 --> 00:02:56 reach the surface. Uh, as solar radiation

00:02:56 --> 00:02:59 warms these exposed zones, volatiles can

00:02:59 --> 00:03:02 escape into space, driving the development or

00:03:02 --> 00:03:05 modification of the Bright streaks downslope.

00:03:05 --> 00:03:08 Anna: What's particularly exciting is the

00:03:08 --> 00:03:10 timing. This research arrives just as the

00:03:10 --> 00:03:13 joint ESA and JAXA uh, Becky Colombo

00:03:13 --> 00:03:16 mission is en route to Mercury. The mission

00:03:16 --> 00:03:19 carries an advanced payload that includes

00:03:19 --> 00:03:21 several key contributions from the University

00:03:21 --> 00:03:22 of Bernard.

00:03:22 --> 00:03:25 Avery: Absolutely. The Becky Colombo Laser Altimeter

00:03:25 --> 00:03:28 or bela, was designed and built in part

00:03:28 --> 00:03:31 at the University of Bern. It will use laser

00:03:31 --> 00:03:33 pulses from an orbit roughly a thousand

00:03:33 --> 00:03:35 kilometres above the surface to measure

00:03:35 --> 00:03:38 elevations with about 10 centimetre

00:03:38 --> 00:03:40 precision, enabling a uh, detailed

00:03:40 --> 00:03:42 reconstruction of Mercury's topography.

00:03:42 --> 00:03:45 Anna: The Bern team also contributed the ion

00:03:45 --> 00:03:48 optical system for STROFEO, a NASA

00:03:48 --> 00:03:51 mass spectrometer on BepiColombo that will m

00:03:51 --> 00:03:53 measure the composition of Mercury's

00:03:53 --> 00:03:55 extremely thin atmosphere, connecting

00:03:55 --> 00:03:58 present day volatile escape at the surface to

00:03:58 --> 00:04:00 the surrounding exosphere.

00:04:00 --> 00:04:03 Avery: The research team plans to use the current

00:04:03 --> 00:04:05 inventory of slope streaks as a baseline for

00:04:05 --> 00:04:08 future comparisons once BepiColombo begins

00:04:08 --> 00:04:11 returning data by imaging key regions

00:04:11 --> 00:04:13 again, they aim to determine whether new

00:04:13 --> 00:04:16 streaks have formed or existing ones have

00:04:16 --> 00:04:18 changed since the MESSENGER era. Any such

00:04:18 --> 00:04:21 changes would provide strong evidence that

00:04:21 --> 00:04:23 volatile driven processes are still

00:04:23 --> 00:04:26 reshaping Mercury's surface on human time

00:04:26 --> 00:04:27 timescales.

00:04:27 --> 00:04:30 Anna: It's a great reminder that even our smallest

00:04:30 --> 00:04:32 closest planetary neighbour still has secrets

00:04:32 --> 00:04:35 to reveal. Mercury is far more dynamic than

00:04:35 --> 00:04:36 we thought.

00:04:36 --> 00:04:38 Avery: Shifting from Mercury to uh, our planet

00:04:38 --> 00:04:41 hunting efforts, NASA's Transiting Exoplanet

00:04:41 --> 00:04:44 Survey Satellite, or TESS, recently had a bit

00:04:44 --> 00:04:46 of a scare when a command error temporarily

00:04:46 --> 00:04:47 knocked it offline.

00:04:48 --> 00:04:50 Anna: Right. The spacecraft was forced into safe

00:04:50 --> 00:04:53 mode after an unexpected command error caused

00:04:53 --> 00:04:55 its solar panels to misalign with the sun.

00:04:56 --> 00:04:58 This misalignment had serious consequences

00:04:58 --> 00:05:00 because the panels were unable to charge

00:05:00 --> 00:05:03 tess's batteries, leading to a low power

00:05:03 --> 00:05:04 condition that triggered the automatic

00:05:04 --> 00:05:06 transition to safe mode.

00:05:06 --> 00:05:09 Avery: In safe mode, all non essential systems are

00:05:09 --> 00:05:11 turned off to conserve power and the

00:05:11 --> 00:05:13 spacecraft awaits further instructions from

00:05:13 --> 00:05:16 ground controllers. NASA engineers quickly

00:05:16 --> 00:05:18 worked to resolve the issue and fortunately

00:05:18 --> 00:05:20 tess's safe mode performed as intended,

00:05:21 --> 00:05:22 protecting the spacecraft from permanent

00:05:22 --> 00:05:23 damage.

00:05:24 --> 00:05:26 Anna: This incident is actually reminiscent of past

00:05:26 --> 00:05:29 missin failures. Remember Viking 1 back

00:05:29 --> 00:05:32 in 1982? A uh, faulty command caused the

00:05:32 --> 00:05:35 loss of communication and there was that

00:05:35 --> 00:05:37 catastrophic series of events that nearly

00:05:37 --> 00:05:39 destroyed the Soho probe in 1998.

00:05:40 --> 00:05:43 But unlike those cases, TESS was fortunate

00:05:43 --> 00:05:44 to have safeguards in place.

00:05:44 --> 00:05:47 Avery: Exactly. The spacecraft's automatic safe

00:05:47 --> 00:05:49 mode kicked in when the power situation

00:05:49 --> 00:05:52 became critical. The safe mode is designed to

00:05:52 --> 00:05:54 preserve the spacecraft's core functions such

00:05:54 --> 00:05:57 as attitude control and ensure it can be

00:05:57 --> 00:05:59 reactivated once engineers identify and

00:05:59 --> 00:06:00 address the issue.

00:06:00 --> 00:06:03 Anna: According to NASA, the mission team is now

00:06:03 --> 00:06:05 reviewing and updating procedures to prevent

00:06:05 --> 00:06:07 this command error from happening in the

00:06:07 --> 00:06:09 future. It's a good reminder that even with

00:06:09 --> 00:06:12 advanced technology, human error remains a

00:06:12 --> 00:06:14 significant challenge in space operations.

00:06:15 --> 00:06:17 Avery: Absolutely. While tess's recovery was

00:06:17 --> 00:06:20 successful and demonstrates how far space

00:06:20 --> 00:06:22 mission technology has come, this incident

00:06:22 --> 00:06:25 emphasises the need for continued vigilance

00:06:25 --> 00:06:28 in mission planning. The risk of human error

00:06:28 --> 00:06:30 is always there, and the consequences can be

00:06:30 --> 00:06:33 costly in terms of both time and resources.

00:06:33 --> 00:06:36 Anna: The good news is that TESS is back online and

00:06:36 --> 00:06:38 continuing its important work of hunting for

00:06:38 --> 00:06:41 exoplanets. Which brings us nicely to our

00:06:41 --> 00:06:43 next storey about a newly discovered Earth

00:06:43 --> 00:06:44 like world.

00:06:45 --> 00:06:47 Avery: Speaking of exoplanets, astronomers have just

00:06:47 --> 00:06:49 discovered what might be one of the closest

00:06:49 --> 00:06:52 things we have to Earth's twin. Though it's

00:06:52 --> 00:06:54 considerably colder than our home.

00:06:54 --> 00:06:56 Anna: Planet, the Exoplanet is called

00:06:56 --> 00:06:59 HD13710B

00:06:59 --> 00:07:02 and it's located 146 light years

00:07:02 --> 00:07:05 away. It's slightly larger than Earth and

00:07:05 --> 00:07:07 orbits a star that resembles our Sun.

00:07:07 --> 00:07:10 However, despite its similarities to Earth in

00:07:10 --> 00:07:13 terms of size and orbital period, its surface

00:07:13 --> 00:07:15 could be far colder than even Mars,

00:07:15 --> 00:07:18 potentially reaching a frigid minus 90

00:07:18 --> 00:07:21 degrees Fahrenheit or minus 68 degrees

00:07:21 --> 00:07:21 Celsius.

00:07:21 --> 00:07:23 Avery: This discovery was published in the

00:07:23 --> 00:07:26 Astrophysical Journal Letters and was made by

00:07:26 --> 00:07:29 an international team led by Alexander

00:07:29 --> 00:07:32 Venner. The search for Earth, like

00:07:32 --> 00:07:35 exoplanets, has been a central focus of

00:07:35 --> 00:07:38 astronomical research for over three decades

00:07:38 --> 00:07:38 now.

00:07:38 --> 00:07:41 Anna: Dr. Huang, a key member of the research team,

00:07:41 --> 00:07:43 explained it well when he said, since the

00:07:43 --> 00:07:45 discovery of the first exoplanet 30 years

00:07:45 --> 00:07:48 ago, we've always tried to find Earth's

00:07:48 --> 00:07:51 Trinity. HD13007 010

00:07:51 --> 00:07:53 b could bring us closer to that goal.

00:07:53 --> 00:07:56 Although it's not an exact match, the.

00:07:56 --> 00:07:58 Avery: Planet is positioned in what astronomers call

00:07:58 --> 00:08:01 the habitable zone of its star, which is the

00:08:01 --> 00:08:03 area where water could potentially exist in

00:08:03 --> 00:08:06 liquid form, which is crucial for life as we

00:08:06 --> 00:08:08 know it. However, there's a major obstacle

00:08:09 --> 00:08:10 right the.

00:08:10 --> 00:08:11 Anna: Star HD

00:08:11 --> 00:08:14 137010B

00:08:14 --> 00:08:16 orbits is cooler and dimmer than our sun,

00:08:17 --> 00:08:20 meaning the planet receives only a fraction

00:08:20 --> 00:08:22 of the energy Earth does. This could result

00:08:22 --> 00:08:24 in surface temperatures as low as

00:08:24 --> 00:08:27 -90 degrees Fahrenheit, making it one

00:08:27 --> 00:08:30 of the coldest exoplanets discovered in

00:08:30 --> 00:08:30 recent years.

00:08:31 --> 00:08:34 Avery: But scientists remain hopeful. Dr.

00:08:34 --> 00:08:36 Venner pointed out that while the planet's

00:08:36 --> 00:08:38 surface might be frozen, it could still fall

00:08:38 --> 00:08:41 within the broader optimistic habitable zone

00:08:41 --> 00:08:43 of its star. With the right atmospheric

00:08:43 --> 00:08:44 conditions,

00:08:44 --> 00:08:47 HD137010B

00:08:47 --> 00:08:49 might not be as inhospitable as its

00:08:49 --> 00:08:50 temperature suggests.

00:08:51 --> 00:08:53 Anna: One of the challenges of studying this planet

00:08:53 --> 00:08:56 is its orbital distance from its star, which

00:08:56 --> 00:08:58 is similar to Earth's but much farther than

00:08:58 --> 00:09:01 the typical exoplanets that are easier to

00:09:01 --> 00:09:04 observe. Transits when the planet crosses

00:09:04 --> 00:09:06 in front of its star happen less frequently,

00:09:07 --> 00:09:09 making it harder to confirm the planet's

00:09:09 --> 00:09:09 existence.

00:09:10 --> 00:09:13 Avery: The discovery was made from a single Transit

00:09:13 --> 00:09:15 captured by NASA's Kepler Space Telescope.

00:09:16 --> 00:09:17 Further confirmation of the planet's

00:09:17 --> 00:09:20 existence and detailed analysis of its mass

00:09:20 --> 00:09:23 and atmosphere will require more data, which

00:09:23 --> 00:09:25 might not be possible until the next

00:09:25 --> 00:09:27 generation of telescopes become operational.

00:09:27 --> 00:09:30 Anna: It's an exciting discovery that adds to our

00:09:30 --> 00:09:32 understanding of the types of environments

00:09:32 --> 00:09:35 where life could potentially exist beyond our

00:09:35 --> 00:09:37 solar system. Even if

00:09:37 --> 00:09:40 HD137010B

00:09:40 --> 00:09:43 is too cold for life as we know it, it

00:09:43 --> 00:09:46 teaches us valuable lessons about planetary

00:09:46 --> 00:09:46 habitability.

00:09:47 --> 00:09:49 Avery: Now let's turn our attention back to Earth

00:09:49 --> 00:09:52 orbit and the International Space Station.

00:09:52 --> 00:09:55 NASA has announced an earlier than expected

00:09:55 --> 00:09:57 target date to launch the next astronauts to

00:09:57 --> 00:09:58 the ISS.

00:09:59 --> 00:10:01 Anna: That's right, the agency is now targeting

00:10:01 --> 00:10:04 February 11 for liftoff of SpaceX

00:10:04 --> 00:10:07 Crew 12 mission, which will fly four

00:10:07 --> 00:10:09 astronauts to join the skeleton crew

00:10:09 --> 00:10:11 presently operating the orbital.

00:10:12 --> 00:10:15 That's four days earlier than originally

00:10:15 --> 00:10:15 planned.

00:10:15 --> 00:10:18 Avery: Just to give everyone context, currently only

00:10:18 --> 00:10:20 three crew members are covering the

00:10:20 --> 00:10:22 maintenance and science investigations aboard

00:10:22 --> 00:10:25 the ISS. They were left behind on January

00:10:25 --> 00:10:28 14th by the early departure of Crew 11

00:10:28 --> 00:10:30 on the station's first ever medical

00:10:30 --> 00:10:31 evacuation.

00:10:32 --> 00:10:35 Anna: The M Crew 12 astronauts were already in line

00:10:35 --> 00:10:38 to take the Crew 11's quartet's place, but

00:10:38 --> 00:10:40 they had originally been scheduled to overlap

00:10:40 --> 00:10:42 with them before their return to Earth.

00:10:42 --> 00:10:45 SpaceX and NASA had originally targeted

00:10:45 --> 00:10:48 February 15 for Crew 12's launch, but

00:10:48 --> 00:10:50 managed to get the mission's crew Dragon

00:10:50 --> 00:10:53 spacecraft and Falcon 9 rocket ready ahead

00:10:53 --> 00:10:54 of schedule.

00:10:54 --> 00:10:57 Avery: The Crew 12 team includes NASA

00:10:57 --> 00:10:59 astronauts Jessica Meir, who's the mission

00:10:59 --> 00:11:02 commander, and Jack Hathaway as pilot.

00:11:02 --> 00:11:05 The mission specialists are Sophie Adenot of

00:11:05 --> 00:11:07 the European Space Agency and

00:11:07 --> 00:11:10 Roscosmos cosmonaut Andrei

00:11:10 --> 00:11:11 Fedyayev.

00:11:11 --> 00:11:14 Anna: Interestingly, Fedyav was a relatively late

00:11:14 --> 00:11:17 replacement for cosmonaut Oleg Artemiev, who

00:11:17 --> 00:11:20 was pulled off Crew 12 in early December,

00:11:20 --> 00:11:23 possibly for violating US national security

00:11:23 --> 00:11:24 regulations.

00:11:24 --> 00:11:27 Avery: This quartet will fly the crew Dragon capsule

00:11:27 --> 00:11:30 named Grace to the ISS for a longer than

00:11:30 --> 00:11:32 normal assignment lasting nine months instead

00:11:32 --> 00:11:35 of the typical six months. It'll be the

00:11:35 --> 00:11:37 second spaceflight for both Mayur and Fedyav,

00:11:37 --> 00:11:40 while Hathaway and Adino uh are both

00:11:40 --> 00:11:42 spaceflight rookies headed to orbit for the

00:11:42 --> 00:11:43 first time.

00:11:43 --> 00:11:46 Anna: The launch window opens on February 11th at

00:11:46 --> 00:11:49 6:00am Eastern Time from Launch Complex 40

00:11:49 --> 00:11:52 at Cape Canaveral Space Force Station in

00:11:52 --> 00:11:54 Florida. If they don't manage to launch that

00:11:54 --> 00:11:56 day, there are backup opportunities. On

00:11:56 --> 00:11:59 February 12th and 13th, the Crew.

00:11:59 --> 00:12:02 Avery: 12 astronauts will join NASA, Chris Williams

00:12:02 --> 00:12:05 and cosmonauts Sergey Kud Sverskov and

00:12:05 --> 00:12:07 Sergei Mikayev as part of ISS

00:12:07 --> 00:12:10 Expedition 74, which will eventually

00:12:10 --> 00:12:13 transition to Expedition 75 before

00:12:13 --> 00:12:16 the end of Crew 12's rotation station. It's

00:12:16 --> 00:12:17 great to see the relief crew heading up

00:12:17 --> 00:12:19 sooner to help out the skeleton crew

00:12:19 --> 00:12:21 currently managing the station.

00:12:21 --> 00:12:24 Anna: Now for something truly mind bending.

00:12:24 --> 00:12:27 Astronomers have confirmed the first runaway

00:12:27 --> 00:12:30 supermassive black hole and it's leaving

00:12:30 --> 00:12:31 quite a trail behind it.

00:12:31 --> 00:12:34 Avery: This is wild stuff, Anna. Uh, the black

00:12:34 --> 00:12:37 hole was identified by a 200 light

00:12:37 --> 00:12:40 year tail and a supersonic bow shock in the

00:12:40 --> 00:12:43 Cosmic Owl galaxy, which is actually a

00:12:43 --> 00:12:45 pair of ring galaxies about 8.8 billion

00:12:46 --> 00:12:48 light years away. The rings appear as

00:12:48 --> 00:12:50 owlized as they get closer and closer to

00:12:50 --> 00:12:51 merging.

00:12:51 --> 00:12:54 Anna: The research led by Peter von Dockam, um,

00:12:54 --> 00:12:56 from Yale's Astronomy Department, was

00:12:56 --> 00:12:59 confirmed using observations from the James

00:12:59 --> 00:13:01 Webb Space Telescope. The central

00:13:01 --> 00:13:04 proposal is that this linear feature is the

00:13:04 --> 00:13:07 wake behind a runaway supermassive black

00:13:07 --> 00:13:10 hole. And this is strongly supported by their

00:13:10 --> 00:13:10 analysis.

00:13:10 --> 00:13:13 Avery: But how does something weighing potentially

00:13:13 --> 00:13:15 millions or even billions of times the mass

00:13:15 --> 00:13:18 of our sun get kicked out of a galaxy? The

00:13:18 --> 00:13:21 answer lies in galaxy mergers. When big

00:13:21 --> 00:13:23 galaxies collide and merge, they force the

00:13:23 --> 00:13:25 black holes at their respective centres into

00:13:25 --> 00:13:26 close proximity.

00:13:27 --> 00:13:29 Anna: Right. If two black holes become locked in a

00:13:29 --> 00:13:32 gravitational dance and then a third crashes

00:13:32 --> 00:13:35 in from another merging galaxy, the resulting

00:13:35 --> 00:13:38 instability can hurl one of the trio away at

00:13:38 --> 00:13:41 sufficient speed to exit the host galaxy

00:13:41 --> 00:13:43 entirely. This can happen through two main

00:13:43 --> 00:13:44 mechanisms.

00:13:44 --> 00:13:47 Avery: The first is gravitational wave recoil.

00:13:47 --> 00:13:49 When black holes merge, they emit uh,

00:13:49 --> 00:13:51 gravitational waves that can give the

00:13:51 --> 00:13:54 resulting black hole a velocity boost of up

00:13:54 --> 00:13:56 to several thousand kilometres per second,

00:13:56 --> 00:13:58 propelling it away from the galactic centre.

00:13:59 --> 00:14:01 Anna: The second mechanism is the classical

00:14:01 --> 00:14:04 slingshot scenario. In this case, a long

00:14:04 --> 00:14:06 lived binary black hole forms through a

00:14:06 --> 00:14:09 merger of two galaxies when a third

00:14:09 --> 00:14:11 supermassive black hole is introduced. In a

00:14:11 --> 00:14:14 second merger, the three body interaction can

00:14:14 --> 00:14:16 eject one of the black holes, usually the

00:14:16 --> 00:14:17 lightest one.

00:14:17 --> 00:14:19 Avery: What's particularly striking about this

00:14:19 --> 00:14:22 confirmed runaway black hole is the trail it

00:14:22 --> 00:14:25 leaves behind. As the black hole ploughs

00:14:25 --> 00:14:27 through intergalactic space, it compresses

00:14:27 --> 00:14:29 tenuous gas in front of it, which

00:14:29 --> 00:14:32 precipitates the birth of hot blue stars.

00:14:32 --> 00:14:35 This creates a 200 light year long

00:14:35 --> 00:14:36 contrail of young stars.

00:14:37 --> 00:14:39 Anna: The black hole also generates a bow shock at

00:14:39 --> 00:14:41 the head of this week, something the

00:14:41 --> 00:14:44 researchers predicted based on shock models

00:14:44 --> 00:14:46 from the ages of the stars in the trail. They

00:14:46 --> 00:14:49 deduce that the black hole escaped about 40

00:14:49 --> 00:14:51 million years ago and is barreling through

00:14:51 --> 00:14:54 space at roughly 1600 kilometres per

00:14:54 --> 00:14:54 second.

00:14:55 --> 00:14:57 Avery: To put that in perspective, that's fast

00:14:57 --> 00:14:59 enough to travel from Earth to the moon in

00:14:59 --> 00:15:02 about 14 minutes. It's an incredible

00:15:02 --> 00:15:04 speed for something so massive.

00:15:04 --> 00:15:06 Anna: Recent papers have shown images of

00:15:06 --> 00:15:09 surprisingly straight streaks of stars within

00:15:09 --> 00:15:12 galaxies that seem to be convincing evidence

00:15:12 --> 00:15:15 for runaway black holes. One paper describes

00:15:15 --> 00:15:17 a very distant galaxy imaged by James Webb

00:15:17 --> 00:15:20 with a bright contrail, suggesting a black

00:15:20 --> 00:15:23 hole with a mass 10 million times the mass

00:15:23 --> 00:15:23 of the sun.

00:15:23 --> 00:15:26 Avery: It's a reminder that the universe is even

00:15:26 --> 00:15:28 more dynamic and violent than we often

00:15:28 --> 00:15:31 imagine. These behemoths aren't just sitting

00:15:31 --> 00:15:33 quietly at the centres of galaxies. Some of

00:15:33 --> 00:15:35 them are literally tearing through space,

00:15:35 --> 00:15:37 creating new stars in their wake.

00:15:37 --> 00:15:40 Anna: And finally, let's talk about an upcoming

00:15:40 --> 00:15:42 event that has both exciting scientific

00:15:42 --> 00:15:45 potential and some concerning risks.

00:15:45 --> 00:15:48 On 12-22-2032,

00:15:48 --> 00:15:51 asteroid 2024 yr 4

00:15:51 --> 00:15:54 has a 4% chance of actually striking

00:15:54 --> 00:15:55 the Moon.

00:15:55 --> 00:15:58 Avery: A 4% chance might not sound like much, but

00:15:58 --> 00:16:01 it's definitely non negligible. If this

00:16:01 --> 00:16:03 collision does happen, it will release enough

00:16:03 --> 00:16:06 energy to be the equivalent of smacking our

00:16:06 --> 00:16:08 nearest neighbour with a medium sized

00:16:08 --> 00:16:11 thermonuclear weapon. It would be six

00:16:11 --> 00:16:13 orders of magnitude more powerful than the

00:16:13 --> 00:16:15 last major impact on the moon, which happened

00:16:15 --> 00:16:16 back in 2013.

00:16:17 --> 00:16:20 Anna: A uh, new paper from Yifan he of Tsinghua

00:16:20 --> 00:16:22 University looks at the potential scientific

00:16:22 --> 00:16:25 opportunities if this collision occurs. And

00:16:25 --> 00:16:27 while they can simulate models of how the

00:16:27 --> 00:16:30 impact will go, monitoring it as it happens

00:16:30 --> 00:16:32 will provide never before collected actual

00:16:32 --> 00:16:35 data that's infeasible to get any other way.

00:16:35 --> 00:16:38 Avery: The impact would vaporise rock and plasma and

00:16:38 --> 00:16:40 would be clearly visible from the Pacific

00:16:40 --> 00:16:42 region where it will be nighttime during the

00:16:42 --> 00:16:45 impact. Even days after the impact, the

00:16:45 --> 00:16:48 melt pool of the impacted material will still

00:16:48 --> 00:16:50 be cooling, allowing infrared observers like

00:16:50 --> 00:16:53 the James Webb Space Telescope to capture

00:16:53 --> 00:16:53 plenty of data.

00:16:54 --> 00:16:57 Anna: The impact should form a crater roughly one

00:16:57 --> 00:16:59 kilometre wide and 150 to

00:16:59 --> 00:17:02 260 metres deep, with a 100

00:17:02 --> 00:17:05 metre pool of molten rock at the centre.

00:17:05 --> 00:17:07 Comparing it in size to other craters

00:17:07 --> 00:17:09 scattered around the moon will help us

00:17:09 --> 00:17:11 understand its bombardment history.

00:17:12 --> 00:17:14 Avery: The impact will also set off a global

00:17:14 --> 00:17:17 moonquake of magnitude 5.0 that

00:17:17 --> 00:17:19 would be the strongest moonquake yet detected

00:17:19 --> 00:17:22 by any seismometer on the Moon. Watching the

00:17:22 --> 00:17:24 propagation of the moonquake will shine a

00:17:24 --> 00:17:26 light on the Moon's interior and help

00:17:26 --> 00:17:28 researchers understand its composition.

00:17:28 --> 00:17:31 Anna: And here's where it gets really spectacular.

00:17:31 --> 00:17:33 A final piece of the scientific puzzle will

00:17:33 --> 00:17:36 be the debris field created by the blast. Up

00:17:36 --> 00:17:39 to 400 kilogrammes of lunar material

00:17:39 --> 00:17:42 is expected to survive re entry to Earth,

00:17:42 --> 00:17:45 creating essentially a free large scale

00:17:45 --> 00:17:46 lunar sample return mission.

00:17:46 --> 00:17:49 Avery: At its peak right around Christmas of 2032,

00:17:50 --> 00:17:52 simulations expect up to 20 million meteors

00:17:52 --> 00:17:55 per hour to hit our atmosphere, at least on

00:17:55 --> 00:17:57 the leading edge of the planet. Most of them

00:17:57 --> 00:17:59 would have naked eye visibility, including

00:17:59 --> 00:18:02 some 100 to 400 fireballs per hour.

00:18:03 --> 00:18:05 Anna: But there is a downside to all of this that

00:18:05 --> 00:18:08 400 kilogrammes of meteors has to land

00:18:08 --> 00:18:10 somewhere, and it looks like the crosshairs

00:18:10 --> 00:18:13 fall squarely on South America, North Africa

00:18:13 --> 00:18:16 and the Arabian Peninsula. A few kilogrammes

00:18:16 --> 00:18:18 of space rock falling on Dubai could

00:18:18 --> 00:18:20 certainly cause some damage.

00:18:20 --> 00:18:22 Avery: Perhaps more dangerous is the risk of

00:18:22 --> 00:18:24 satellite mega constellations that play such

00:18:24 --> 00:18:26 an important role in our modern day

00:18:26 --> 00:18:29 navigation and Internet systems. Such an

00:18:29 --> 00:18:31 event could trigger Kessler Syndrome and

00:18:31 --> 00:18:34 bring the entire network down over the span

00:18:34 --> 00:18:36 of a few short years, while also locking us

00:18:36 --> 00:18:38 out from being able to get anything else

00:18:38 --> 00:18:40 safely into orbit for much longer.

00:18:41 --> 00:18:43 Anna: Due to the risks, some space agencies are

00:18:43 --> 00:18:46 already considering a deflection mission that

00:18:46 --> 00:18:49 would bump asteroid 2024 yr 4

00:18:49 --> 00:18:51 out of the way of a potential lunar

00:18:51 --> 00:18:53 collision. But that hasn't been set in stone

00:18:53 --> 00:18:56 yet. Neither has the actual impact itself,

00:18:56 --> 00:18:58 with only a 4% chance of happening.

00:18:59 --> 00:19:01 Avery: If the odds increase over the coming years,

00:19:01 --> 00:19:03 we as a species will have to decide whether

00:19:03 --> 00:19:06 it's worth it to deflect it or not. If we

00:19:06 --> 00:19:08 do, we might miss out on a whole bunch of

00:19:08 --> 00:19:11 cool science, but we also might save our

00:19:11 --> 00:19:13 entire orbital infrastructure and the few

00:19:13 --> 00:19:14 lives directly to boot.

00:19:14 --> 00:19:16 Anna: And that wraps up today's episode of

00:19:16 --> 00:19:19 Astronomy Daily. From Mercury's surprising

00:19:19 --> 00:19:22 activity to a possible lunar impact in our

00:19:22 --> 00:19:25 future, space continues to surprise and

00:19:25 --> 00:19:25 amaze us.

00:19:26 --> 00:19:28 Avery: Thanks for joining us today. For more space

00:19:28 --> 00:19:30 news and to explore our archive of episodes,

00:19:30 --> 00:19:33 visit our website@astronomydaily.IO.

00:19:33 --> 00:19:35 you can also find us on social media,

00:19:35 --> 00:19:38 AstroDaily Pod on X, Facebook,

00:19:38 --> 00:19:40 Instagram and YouTube.

00:19:40 --> 00:19:42 Anna: If you enjoyed today's show, please subscribe

00:19:42 --> 00:19:44 on your favourite podcast platform and leave

00:19:44 --> 00:19:46 us a review. It really helps other space

00:19:46 --> 00:19:49 enthusiasts find us. Until next time, keep

00:19:49 --> 00:19:51 looking up clear skies everyone.

00:20:00 --> 00:20:01 Astronomy Day

00:20:03 --> 00:20:04 storeys

00:20:06 --> 00:20:06 love.