SpaceX's Starship 9: A Journey Through Triumph and Turmoil
SpaceTime: Astronomy & Science NewsJune 04, 2025x
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SpaceX's Starship 9: A Journey Through Triumph and Turmoil

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In this episode of SpaceTime, we explore the latest developments in space exploration, lunar geology, and solar phenomena.
SpaceX's Fiery Ninth Starship Test Flight
The latest test flight of SpaceX's Starship ended dramatically as both the orbiter and the booster were destroyed during reentry. Despite the fiery conclusion, SpaceX officials noted that the test was designed to push the limits of the spacecraft. The flight featured numerous milestones, including a successful hot staging and the first reflight of a booster. However, issues arose during the landing burn, resulting in a spectacular explosion. We discuss the implications of this test and what it means for future missions, including NASA's Artemis 3.
Lunar Rocks and Their Magnetic Mystery
A new study proposes that a significant asteroid impact may explain the presence of highly magnetic rocks on the Moon. Researchers suggest that a brief amplification of the Moon's weak magnetic field, caused by a large plasma-generated impact event, could account for the magnetism observed in some lunar samples. This hypothesis sheds light on the Moon's geological history and its magnetic properties, particularly in regions near the lunar south pole, where future missions are planned.
Revealing the Sun's Corona
Astronomers have captured unprecedented details of the Sun's corona using a new adaptive optics system. This groundbreaking technology has allowed scientists to produce the clearest images of the corona yet, enhancing our understanding of coronal heating and solar eruptions. The new observations reveal dynamic features and turbulent flows within the corona, providing insights into the mechanisms driving space weather and its effects on Earth.
www.spacetimewithstuartgary.com
✍️ Episode References
Nature Astronomy
https://www.nature.com/natureastronomy/
Science Advances
https://www.science.org/journal/sciadv
Become a supporter of this podcast: https://www.spreaker.com/podcast/spacetime-space-astronomy--2458531/support.
00:00 This is Space Time Series 28, Episode 67 for broadcast on 4 June 2025
01:00 SpaceX's ninth Starship test flight
12:15 Lunar rocks and their magnetic mystery
22:30 Revealing the Sun's corona
30:00 Science report: New methods for green hydrogen production


00:00:00 --> 00:00:02 Stuart Gary: This is space time series 28, episode

00:00:02 --> 00:00:05 67 for broadcast on 4 June

00:00:05 --> 00:00:07 2025. Coming up on space time,

00:00:08 --> 00:00:11 SpaceX's ninth Starship test flight comes to a

00:00:11 --> 00:00:14 fiery end. A possible solution as to why

00:00:14 --> 00:00:17 some rocks on the moon are highly magnetic and

00:00:17 --> 00:00:19 amazing. Never before seen details about the

00:00:19 --> 00:00:22 sun's atmosphere, the corona, all that and more coming

00:00:22 --> 00:00:24 up on Space Time.

00:00:25 --> 00:00:28 Voice Over Guy: Welcome to Space Time with Stuart

00:00:28 --> 00:00:28 Gary Gary.

00:00:44 --> 00:00:47 Stuart Gary: The ninth test flight of SpaceX's Starships reached a

00:00:47 --> 00:00:50 spectacular and fiery conclusion with the destruction of both

00:00:50 --> 00:00:53 the orbiter and the booster. The super heavy

00:00:53 --> 00:00:56 booster exploded during its landing engine burn, while the

00:00:56 --> 00:00:59 starship orbiter suddenly lost attitude control and began

00:00:59 --> 00:01:02 spinning wildly before ripping itself apart during

00:01:02 --> 00:01:05 re ent. However, mission managers at

00:01:05 --> 00:01:08 SpaceX said the outcome wasn't totally unexpected

00:01:08 --> 00:01:11 as the flight was always designed to test the limits of the

00:01:11 --> 00:01:14 spacecraft. The launch from SpaceX's Starbase

00:01:14 --> 00:01:16 in Boca Chica on the Texas Gulf coast went smoothly

00:01:16 --> 00:01:19 enough with all 33 Raptor 2 engines

00:01:19 --> 00:01:22 lighting up and sending the world's biggest and most powerful

00:01:22 --> 00:01:23 rocket into space.

00:01:36 --> 00:01:39 Stuart Gary: Sight from here we see it arcing right over top of us.

00:01:39 --> 00:01:42 We see 33 out of 33

00:01:42 --> 00:01:45 Raptor engines lit on super heavy as

00:01:45 --> 00:01:48 it starts to ascend skyward. Coming up on maximum

00:01:48 --> 00:01:51 aerodynamic pressure. Then only about a minute and a half

00:01:51 --> 00:01:52 until we get into hot staging.

00:01:52 --> 00:01:55 Commentator: We could feel the building shaking here,

00:01:55 --> 00:01:58 feel the vehicle's power and we're just about a

00:01:58 --> 00:02:01 minute away from shutting down those engines

00:02:01 --> 00:02:04 on the booster again. This booster is flying for

00:02:04 --> 00:02:05 its second time today.

00:02:05 --> 00:02:08 Stuart Gary: We're going to see all but the three center engines

00:02:08 --> 00:02:11 turn off on the booster. So our version of

00:02:11 --> 00:02:14 Miko, most engines cut off and then just a few seconds later,

00:02:14 --> 00:02:17 hoping to see six engines ignite on ship to

00:02:17 --> 00:02:17 push it away.

00:02:17 --> 00:02:20 Stuart Gary: The mission profile was supposed to see the spacecraft

00:02:20 --> 00:02:23 fly across the Atlantic Ocean in Africa before

00:02:23 --> 00:02:25 descending over the Indian Ocean and then finally

00:02:25 --> 00:02:28 splashing down off the western Australian coast.

00:02:29 --> 00:02:32 Hot staging of the 123 meter tall vehicle was

00:02:32 --> 00:02:34 nominal with Starship igniting all six Raptor engines

00:02:34 --> 00:02:37 for the climb to orbital altitude. While the super heavy booster

00:02:37 --> 00:02:40 performed a successful flip and boost back burn.

00:02:40 --> 00:02:43 Stuart Gary: Keep an eye on which way the booster flips. First ever

00:02:43 --> 00:02:46 directional flip we're going for today should flip straight

00:02:46 --> 00:02:48 up. See those engines powering down. Booster

00:02:48 --> 00:02:51 engine cutoff, Ship ignition, stage separation.

00:02:51 --> 00:02:54 Commentator: Incredible flip by super heavy

00:02:54 --> 00:02:57 booster. Those six engines, those three engines on.

00:02:57 --> 00:03:00 Stuart Gary: The ship ignited six healthy Raptors

00:03:00 --> 00:03:03 running on ship on its way to space. Booster

00:03:03 --> 00:03:04 doing the boost.

00:03:04 --> 00:03:06 Commentator: Back chamber pressure's nominal. It Is looking absolutely

00:03:06 --> 00:03:09 incredible here in Hawthorne. As we said, six healthy

00:03:09 --> 00:03:12 engines on ship. We've got 13 out of 13 engines

00:03:12 --> 00:03:15 on the booster now down to those three, which is what we expect

00:03:15 --> 00:03:18 in the final moments of the boostback burn.

00:03:18 --> 00:03:21 Stuart Gary: This was the third flight for the V2 version

00:03:21 --> 00:03:24 of Starship and included numerous improvements over previous

00:03:24 --> 00:03:26 prototypes, including new heat shield tiles and additional

00:03:26 --> 00:03:29 venting. But the flight was even more significant as

00:03:29 --> 00:03:32 this marked the second launch for the same booster, the first

00:03:32 --> 00:03:35 time it had been tried on a Starship mission. That same

00:03:35 --> 00:03:38 booster had successfully flown previously on Flight 7

00:03:38 --> 00:03:41 back in January. And following that mission,

00:03:41 --> 00:03:44 only four of the 33 Raptor engines needed to be

00:03:44 --> 00:03:47 replaced, and one of those engines was now on its third

00:03:47 --> 00:03:49 launch. The booster's descent back to Earth

00:03:49 --> 00:03:52 included testing a new, steeper re entry angle of attack

00:03:52 --> 00:03:55 profile designed to send it to a watery splashdown

00:03:55 --> 00:03:58 landing in the Gulf rather than return to the launch pad.

00:03:58 --> 00:04:01 Commentator: Six healthy engines on ship. We've got 13 out of

00:04:01 --> 00:04:04 13 engines on the booster now down to those three, which

00:04:04 --> 00:04:07 is what we expect in the final moments of the boost back

00:04:07 --> 00:04:10 burn. Now, as a reminder, we are not recovering the

00:04:10 --> 00:04:12 super heavy booster today. We are instead going to do booster

00:04:12 --> 00:04:15 boostback shutdown. And there we had a good shutdown of

00:04:15 --> 00:04:18 the boost back burn. Next up will be the jettison

00:04:18 --> 00:04:19 of that hot stage.

00:04:20 --> 00:04:21 Stuart Gary: Avionics power and telemetry nominal.

00:04:21 --> 00:04:24 Commentator: Great call out there that everything looking nominal aboard

00:04:24 --> 00:04:27 the super heavy vehicle which is returning to Earth. And we're going

00:04:27 --> 00:04:30 to be doing some experiments with it, including, a higher

00:04:30 --> 00:04:33 angle of attack reentry, as well as

00:04:33 --> 00:04:36 some engine tests as it gets closer to

00:04:36 --> 00:04:38 the Gulf. We are again, because of these tests, not

00:04:38 --> 00:04:41 recovering it. We are sending it to the Gulf on purpose

00:04:41 --> 00:04:44 to do those test skip. With six healthy engines continuing

00:04:44 --> 00:04:47 its ascent to its planned suborbital trajectory.

00:04:47 --> 00:04:50 everything going very well so far for Starship's

00:04:50 --> 00:04:53 ninth flight. Now 4 minutes, 15 seconds in

00:04:53 --> 00:04:56 the booster doing its lox dump, that liquid

00:04:56 --> 00:04:59 oxygen dump. So because we don't need some of that liquid oxygen

00:04:59 --> 00:05:01 propellant, and in its tanks, we vent that propellant

00:05:01 --> 00:05:04 out to lessen the booster's mass as it comes in

00:05:05 --> 00:05:08 for its landing. Super heavy is descending

00:05:08 --> 00:05:10 rapidly. what can we expect here in the next few minutes as it

00:05:10 --> 00:05:12 does its atmospheric tests?

00:05:12 --> 00:05:15 Stuart Gary: Super heavy might not have a very smooth ride down. We're

00:05:15 --> 00:05:18 going to be putting it through this higher angle of attack.

00:05:18 --> 00:05:21 So we're kind of pitching it up a tiny bit, increasing drag.

00:05:22 --> 00:05:25 We've done this in wind tunnels. We've done this in

00:05:25 --> 00:05:27 computer modeling. It shows that sometimes

00:05:27 --> 00:05:30 the control isn't great, but only one way to

00:05:30 --> 00:05:33 really prove it out and that's to get real world data. So here

00:05:33 --> 00:05:35 comes super heavy. It should be

00:05:36 --> 00:05:38 igniting for its landing burn in

00:05:39 --> 00:05:41 just about 40 seconds from

00:05:41 --> 00:05:42 now.

00:05:42 --> 00:05:45 Commentator: And we are going to relight 13 engines, then

00:05:45 --> 00:05:47 bring that down to three engines. We will be

00:05:47 --> 00:05:50 intentionally shutting down. We will be shutting down

00:05:50 --> 00:05:53 one of those three center engines intentionally

00:05:53 --> 00:05:55 to push the limits of the super heavy booster.

00:05:55 --> 00:05:57 Commentator: Super raptor chamber pressure's nominal.

00:05:57 --> 00:06:00 Commentator: And continuing to see six healthy

00:06:00 --> 00:06:03 engines on the ship. Three sea

00:06:03 --> 00:06:06 level and three vacuum engines still ignited

00:06:06 --> 00:06:08 as the super heavy booster is making its way back down to Earth.

00:06:08 --> 00:06:11 Stuart Gary: Those grid fins doing some heavy work. Booster landing startup

00:06:11 --> 00:06:13 ignited for our landing burn.

00:06:13 --> 00:06:15 Stuart Gary: Everything appeared to be going smoothly until the landing

00:06:15 --> 00:06:18 burn. Thirteen Raptor engines were meant to restart for

00:06:18 --> 00:06:21 this, but only 12 did. And moments later, the

00:06:21 --> 00:06:24 booster suddenly exploded in a massive fireball.

00:06:24 --> 00:06:27 Stuart Gary: It may have ended with that, landing burn. Does look like we

00:06:27 --> 00:06:29 lost telemetry from the booster once we started

00:06:29 --> 00:06:32 into that landing burn. Did you see a confirmation

00:06:32 --> 00:06:35 that the booster did demise? So the booster's

00:06:35 --> 00:06:38 flight ending before it was able to get through landing burn.

00:06:38 --> 00:06:41 But again, we were not bringing that back. We were expecting it

00:06:41 --> 00:06:44 to make a hard splashdown in the Gulf. We

00:06:44 --> 00:06:47 were getting live data back the entire time through that

00:06:47 --> 00:06:50 high angle of attack flight. So that was something that

00:06:50 --> 00:06:52 was really vital for us to get during this

00:06:52 --> 00:06:53 reuse.

00:06:53 --> 00:06:55 First reflighted booster in the books.

00:06:55 --> 00:06:58 Stuart Gary: Meanwhile, starship continued its ascent into space.

00:06:58 --> 00:07:01 But then a jet of fluid was seen venting from the

00:07:01 --> 00:07:04 engine bay between the sea level and vacuum Raptor

00:07:04 --> 00:07:07 engines. Now it's thought this was probably just the new

00:07:07 --> 00:07:10 nitrogen purge system installed in the attic space between

00:07:10 --> 00:07:13 the top of the engine heat shield and the bottom of the oxygen tank.

00:07:13 --> 00:07:16 See, that's where fire broke out during Flight 7. So

00:07:16 --> 00:07:18 SpaceX installed the new purge system to vent out

00:07:18 --> 00:07:21 built up gases. Then about nine minutes into the

00:07:21 --> 00:07:24 flight, hotspots began to develop quite noticeably

00:07:24 --> 00:07:27 at two separate locations in the engine bay.

00:07:27 --> 00:07:29 Commentator: In about two minutes, we expect all six

00:07:30 --> 00:07:32 Raptor engines to shut down. That will

00:07:32 --> 00:07:35 be seco. Basically second engine or

00:07:35 --> 00:07:37 second stage engine shut off.

00:07:37 --> 00:07:40 Stuart Gary: All eyes definitely on ship. As we get through the final

00:07:40 --> 00:07:43 stages into its ascent, we're expecting

00:07:43 --> 00:07:45 it to start to cut those engines off.

00:07:45 --> 00:07:48 Terminal guidance. We're in terminal guidance. The final

00:07:48 --> 00:07:51 stages of this ascent burn. we did see shutdown of

00:07:51 --> 00:07:54 the Raptor engines. We do stagger these. So we do

00:07:54 --> 00:07:57 the Raptors first. Those three have shut down

00:07:57 --> 00:08:00 successfully. Sea levels still running. Ship

00:08:00 --> 00:08:02 engine cut off. Ship engine. The three

00:08:02 --> 00:08:05 most beautiful words in the English language.

00:08:05 --> 00:08:08 Commentator: And great call out that we had. Nominal

00:08:08 --> 00:08:10 insertion. An incredible

00:08:11 --> 00:08:12 flight test so far.

00:08:12 --> 00:08:15 Today we reflew a super

00:08:15 --> 00:08:18 heavy booster. For the very first time in nine

00:08:18 --> 00:08:21 test flights. Ship is in its

00:08:21 --> 00:08:24 orbital trajectory again. It's going to remain

00:08:24 --> 00:08:27 suborbital for its mission today. But it

00:08:27 --> 00:08:30 ignited, it ignited all six

00:08:30 --> 00:08:32 of its engines and made it all the way through

00:08:32 --> 00:08:34 SECO just now.

00:08:34 --> 00:08:37 Stuart Gary: Main engine cutout happened as planned. But it was at about

00:08:37 --> 00:08:40 this time that Starship began tumbling end over

00:08:40 --> 00:08:43 end out of control, possibly from venting fuel

00:08:43 --> 00:08:45 leaks acting as a sort of jet and causing an asymmetric

00:08:45 --> 00:08:48 rotation of the spacecraft. Now this should have been countered

00:08:48 --> 00:08:51 by Starship's attitude control system. It

00:08:51 --> 00:08:54 uses some of the gas normally used to pressurise the fuel system

00:08:54 --> 00:08:57 to act as a propellant. But because the

00:08:57 --> 00:08:59 fuel system was leaking, there simply wasn't enough gas

00:08:59 --> 00:09:02 left to charge the attitude control system.

00:09:02 --> 00:09:05 And so gradually the end over end tumble got

00:09:05 --> 00:09:08 worse and eventually a horizontal spin began

00:09:08 --> 00:09:09 developing as well.

00:09:09 --> 00:09:12 Stuart Gary: And so at this point we've essentially

00:09:12 --> 00:09:14 lost our attitude control with Starship. We are

00:09:14 --> 00:09:17 still on a path toward reentry. We are suborbital.

00:09:17 --> 00:09:20 So no matter what we are going to enter, however,

00:09:20 --> 00:09:23 this lowers the chances for it to be a controlled

00:09:23 --> 00:09:26 reentry. So if you think back to

00:09:26 --> 00:09:29 Flight 3 when we had something similar

00:09:29 --> 00:09:32 happen, just the end symptom

00:09:32 --> 00:09:35 of a loss of attitude control. We were in a roll by the time we

00:09:35 --> 00:09:37 hit reentry. So we are going to re enter.

00:09:37 --> 00:09:40 We should hopefully still have views. the

00:09:40 --> 00:09:43 Starlink satellites are pretty robust to still

00:09:43 --> 00:09:46 maintaining contact. We've got four of those terminals on

00:09:46 --> 00:09:49 the vehicle and they're pretty robust to maintaining contact

00:09:49 --> 00:09:51 even when we are in a spin.

00:09:51 --> 00:09:54 Essentially, we're coming up on Africa, I

00:09:54 --> 00:09:56 believe we do swing just to the south of that

00:09:56 --> 00:09:59 continent. and by the time we start heading out

00:09:59 --> 00:10:02 over the Indian Ocean, we'll start heading into a sunrise.

00:10:02 --> 00:10:05 So not looking great with a lot of our on orbit objectives

00:10:05 --> 00:10:07 for today. Relight an engine and then really

00:10:07 --> 00:10:10 importantly, get into that controlled entry to really

00:10:10 --> 00:10:13 put the heat shield through the ringer. Nonetheless,

00:10:13 --> 00:10:16 Starship marching forward towards that re entry over the

00:10:16 --> 00:10:19 Indian Ocean. So we'll continue to hang with it.

00:10:19 --> 00:10:22 Stuart Gary: Now, while all this was going on, an attempt was being made to deploy a

00:10:22 --> 00:10:25 series of eight Starlink satellite simulators as part of an

00:10:25 --> 00:10:28 in flight test. But that also failed when the

00:10:28 --> 00:10:31 payload bay door failed to open. But the

00:10:31 --> 00:10:34 bigger problem, Starship now spinning out of control, was

00:10:34 --> 00:10:36 doomed to fall back into the atmosphere at crazy

00:10:36 --> 00:10:37 angles.

00:10:37 --> 00:10:39 Stuart Gary: So we are expecting it break up

00:10:39 --> 00:10:42 essentially on its reentry over the Indian Ocean.

00:10:42 --> 00:10:45 So not able to do a lot of our on

00:10:45 --> 00:10:47 orbit objectives today. Again, we are

00:10:48 --> 00:10:51 in essentially a tumble. We had lost that attitude control.

00:10:51 --> 00:10:53 Stuart Gary: 41 minutes into the flight, Starship began to break

00:10:53 --> 00:10:56 apart and melt as it was ripped into pieces by its

00:10:56 --> 00:10:58 atmosphere vehicle.

00:10:58 --> 00:11:00 Commentator: To see about 1400 degrees Celsius,

00:11:00 --> 00:11:03 feeling that temperature there melting away.

00:11:03 --> 00:11:06 But as we expected, with the spinning of the

00:11:06 --> 00:11:09 vehicle, we are no longer controlling it,

00:11:09 --> 00:11:12 is expected to see, see it begin to

00:11:12 --> 00:11:14 demise a little bit on its way back down to Earth.

00:11:14 --> 00:11:17 Stuart Gary: It's re entering actively right now. and again, we did

00:11:17 --> 00:11:20 do what's called passivation. So you essentially vent all

00:11:20 --> 00:11:22 of your excess propellant overboard before you hit the

00:11:22 --> 00:11:25 atmosphere. That's a safety measure we can take on the ship

00:11:25 --> 00:11:28 while you still have contact with it. So that was done.

00:11:28 --> 00:11:31 It's now coming down m in the predetermined hazard area

00:11:31 --> 00:11:34 that was cleared ahead of flight, not controlled. So we're not going to

00:11:34 --> 00:11:37 get all of that reentry data that we're still really looking

00:11:37 --> 00:11:39 forward to. This is kind of a new generation

00:11:40 --> 00:11:42 of ship. It has different flaps,

00:11:42 --> 00:11:45 improved heat shield, a whole lot of things that we're really trying

00:11:45 --> 00:11:48 to really put through the wringer. There's a whole lot we still

00:11:48 --> 00:11:51 need to learn before we get to kind of the next step that we're

00:11:51 --> 00:11:54 hoping for, which is going to be that ship going orbital and

00:11:54 --> 00:11:57 eventually coming back here for a catch. So getting

00:11:57 --> 00:12:00 through one of these fully is going to be really

00:12:00 --> 00:12:03 important. it's not going to be today, but we are just

00:12:03 --> 00:12:05 going to stick with the ship, see what else we can learn

00:12:06 --> 00:12:09 as it makes its way through the atmosphere and

00:12:09 --> 00:12:12 brings an end to the ninth flight test. so we'll stick with it.

00:12:12 --> 00:12:14 Stuart Gary: The mission was over. a full investigation to determine what

00:12:14 --> 00:12:17 happened is now underway. SpaceX boss

00:12:17 --> 00:12:20 Elon Musk says launch cadence for the next three flights will be

00:12:20 --> 00:12:23 faster at approximately one every three to four weeks.

00:12:23 --> 00:12:26 The company need to get on top of the problem because no V2

00:12:26 --> 00:12:29 version of Starship has successfully achieved its flight

00:12:29 --> 00:12:32 parameters. See, a key part of the starship

00:12:32 --> 00:12:34 program will be assisting NASA's plans to return

00:12:34 --> 00:12:37 humans to the moon in 2027 aboard the Artemis

00:12:37 --> 00:12:40 3 mission. A version of starship will act as a

00:12:40 --> 00:12:43 shuttle, transporting crew and supplies from the Orion

00:12:43 --> 00:12:45 capsule down to the lunar surface.

00:12:46 --> 00:12:48 Meanwhile, Major design changes for Starship and Super

00:12:48 --> 00:12:51 heavy are also on the horizon. These include

00:12:51 --> 00:12:54 a nine engine variant of Starship. There are currently six

00:12:54 --> 00:12:57 engines on the Starship orbiter, and the use of just three rather

00:12:57 --> 00:13:00 than the current four grid fins on the super heavy booster.

00:13:01 --> 00:13:04 Also future versions of the Starship super heavy booster

00:13:04 --> 00:13:06 stack will get taller, eventually reaching a height of

00:13:06 --> 00:13:09 142 meters. These ongoing

00:13:09 --> 00:13:12 evolutionary changes are all part of Musk's plan

00:13:12 --> 00:13:14 to develop Starship as a true interplanetary

00:13:14 --> 00:13:17 colonial transport vehicle one capable of taking

00:13:17 --> 00:13:20 100 people or 150 tons of equipment and supplies

00:13:20 --> 00:13:23 on journeys not just to the moon, but eventually

00:13:23 --> 00:13:26 Mars and beyond. In the process turning the

00:13:26 --> 00:13:28 human race into a two planet civilization.

00:13:29 --> 00:13:32 This is space time still to come.

00:13:33 --> 00:13:35 Why are some rocks on the moon so heavily magnetized?

00:13:36 --> 00:13:39 And astronomers scope never before seen details in

00:13:39 --> 00:13:41 the Sun's atmosphere, the corona, all that and more

00:13:41 --> 00:13:43 still to come on space time.

00:13:47 --> 00:13:50 Okay, let's take a break from M. Our show for a word from our sponsor

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00:15:25 --> 00:15:25 back to our show.

00:15:33 --> 00:15:36 A new study claims a large asteroid impact on the

00:15:36 --> 00:15:39 Moon could explain why some lunar rocks are highly

00:15:39 --> 00:15:42 magnetic. The findings, reported in the journal

00:15:42 --> 00:15:45 Science Advances, suggest the impact could have briefly

00:15:45 --> 00:15:47 amplified the Moon's weak magnetic field, creating a

00:15:47 --> 00:15:50 momentary spike that was recorded in some lunar

00:15:50 --> 00:15:53 rocks. Scientists have puzzled over the fate of the

00:15:53 --> 00:15:56 Moon's magnetic field for decades, ever since orbiting

00:15:56 --> 00:15:59 spacecraft first picked up signs of a highly magnetic field

00:15:59 --> 00:16:02 in some lunar surface rocks. The problem is

00:16:02 --> 00:16:04 the Moon itself has no inherent magnetism. Today,

00:16:05 --> 00:16:08 this new hypothesis suggests that a combination of

00:16:08 --> 00:16:10 an ancient weak magnetic field and a large

00:16:10 --> 00:16:13 plasma generated impact event may have

00:16:13 --> 00:16:15 temporarily created a strong magnetic field

00:16:15 --> 00:16:18 concentrated on the far side of the Moon. The

00:16:18 --> 00:16:21 study's authors undertook detailed simulations showing

00:16:21 --> 00:16:24 how an impact such as from a large asteroid could have generated

00:16:24 --> 00:16:27 a cloud of ionized particles that briefly enveloped the

00:16:27 --> 00:16:30 entire Moon. This plasma would have streamed around the

00:16:30 --> 00:16:33 Moon and concentrated at the opposite location from the

00:16:33 --> 00:16:35 initial point of impact. There, the plasma would have

00:16:35 --> 00:16:38 interacted with and momentarily amplified the Moon's own

00:16:38 --> 00:16:41 weak magnetic field, and any rocks in that region

00:16:41 --> 00:16:44 could have recorded signs of heightened magnetism before the

00:16:44 --> 00:16:47 field died away. This combination of

00:16:47 --> 00:16:50 events could explain the presence of highly magnetic rocks

00:16:50 --> 00:16:53 detected in a region near the lunar south pole on the

00:16:53 --> 00:16:56 Moon's far side. And as it happens, one of

00:16:56 --> 00:16:58 the largest impact basins on the Moon, the Ibrium

00:16:58 --> 00:17:01 basin, is located in the exact opposite spot on the

00:17:01 --> 00:17:04 near side of the Moon. The study's lead author,

00:17:04 --> 00:17:07 Isaac Nurett from mit, says whatever made the impact

00:17:07 --> 00:17:10 likely released a cloud of plasma that kicked off the

00:17:10 --> 00:17:12 magnetic scenario seen in their simulations.

00:17:12 --> 00:17:15 He says there are large parts of lunar magnetism that are simply

00:17:15 --> 00:17:18 unexplained. But the majority of the strong

00:17:18 --> 00:17:21 magnetic fields that are being measured by orbiting spacecraft could

00:17:21 --> 00:17:24 be explained by this impact process, especially on the

00:17:24 --> 00:17:27 lunar far side. Scientists have known

00:17:27 --> 00:17:30 for decades that the Moon does hold remnants of a strong

00:17:30 --> 00:17:33 magnetic field. Samples from the surface of the Moon

00:17:33 --> 00:17:36 returned by astronauts on NASA's Apollo missions in the 60s

00:17:36 --> 00:17:38 and 70s, as well as global measurements of the Moon taken from

00:17:39 --> 00:17:41 orbiting spacecraft, show signs of remnant magnetism in

00:17:41 --> 00:17:44 surface rocks, especially on the far side of the Moon.

00:17:44 --> 00:17:47 Now, the typical explanation for surface magnetism is

00:17:47 --> 00:17:50 a global magnetic field generated by an internal

00:17:50 --> 00:17:53 geodynamo, a core of molten, churning

00:17:53 --> 00:17:55 metallic material. In fact, the Earth today

00:17:55 --> 00:17:58 generates just such a magnetic field through its Own

00:17:58 --> 00:18:01 geodynamo process. And it's thought that the Moon May

00:18:01 --> 00:18:03 well once have done the same. Although being a m much smaller

00:18:03 --> 00:18:06 core, it would have produced A much weaker magnetic field.

00:18:07 --> 00:18:09 But that wouldn't explain the highly magnetized rocks

00:18:09 --> 00:18:12 observed, Particularly those on the Moon's far side.

00:18:12 --> 00:18:15 And that's where this alternative hypothesis Involving a giant

00:18:15 --> 00:18:18 impact comes in. In 2020,

00:18:18 --> 00:18:21 scientists tested this hypothesis with simulations of a

00:18:21 --> 00:18:24 giant impact on the Moon in combination with the solar

00:18:24 --> 00:18:27 generated magnetic field, which is weak as it stretches

00:18:27 --> 00:18:30 out to the Earth and Moon. In the simulations,

00:18:30 --> 00:18:32 they tested whether an impact on the Moon could amplify such a

00:18:32 --> 00:18:35 solar field enough to explain the highly magnetic measurements

00:18:35 --> 00:18:38 they found on the surface rocks. It turns out

00:18:38 --> 00:18:41 it wasn't enough. So the results seemed to rule out a

00:18:41 --> 00:18:44 plasma induced impact as playing any sort of role in the

00:18:44 --> 00:18:46 Moon's missing magnetism. But in this new

00:18:46 --> 00:18:49 hypothesis, the authors took a different tack. Instead

00:18:49 --> 00:18:52 of accounting for the Sun's magnetic field, they assumed the

00:18:52 --> 00:18:54 Moon once hosted Its own geodynamo produced

00:18:54 --> 00:18:57 magnetic field, although a reasonably weak one.

00:18:57 --> 00:19:00 Now, given the size of the lunar core, they estimate that such

00:19:00 --> 00:19:03 a field Would have been about one micro Tesla, 50

00:19:03 --> 00:19:05 times weaker than the Earth's magnetic field today.

00:19:06 --> 00:19:09 From this starting point, the authors simulated a large impact

00:19:09 --> 00:19:12 on the Moon's surface, similar to what would have created the Imbrium

00:19:12 --> 00:19:15 crater On the Moon's near side. Using impact

00:19:15 --> 00:19:18 simulations, the authors then simulated the cloud of

00:19:18 --> 00:19:21 plasma that such an impact would have generated. As the force of the

00:19:21 --> 00:19:23 impact vaporized the surface material,

00:19:24 --> 00:19:26 they simulated how the resulting plasma would flow and

00:19:26 --> 00:19:29 interact with the Moon's weak magnetic field. And

00:19:29 --> 00:19:32 these simulations showed that as a plasma cloud arose from the

00:19:32 --> 00:19:35 impact, Some of it would have expanded into space, While the rest

00:19:35 --> 00:19:38 would have streamed around the Moon and concentrated on the

00:19:38 --> 00:19:41 opposite side. There, the plasma would

00:19:41 --> 00:19:44 have compressed and briefly amplified the Moon's own weak

00:19:44 --> 00:19:46 magnetic field. The entire process, from

00:19:46 --> 00:19:49 the moment the magnetic field is amplified to the time it decays

00:19:49 --> 00:19:52 back to the baseline, Would have been fairly quick, no more than

00:19:52 --> 00:19:55 around 40 minutes. But they also found that an

00:19:55 --> 00:19:58 Imbrium scale impact Would have produced a pressure wave which

00:19:58 --> 00:20:01 traveled through the Moon, similar to a seismic shock. And these

00:20:01 --> 00:20:04 waves would have converged on the opposite side from the impact, where the shock

00:20:04 --> 00:20:07 front Would have jittered the surrounding rocks, briefly unsettling

00:20:07 --> 00:20:09 the rock's electrons. They're the subatomic particles that

00:20:09 --> 00:20:12 naturally orient their spins to any external magnetic

00:20:12 --> 00:20:15 field. The authors suspect that the rocks were being

00:20:15 --> 00:20:18 shocked Just as the impact plasma was amplifying the

00:20:18 --> 00:20:20 Moon's magnetic field. So as the rock's

00:20:20 --> 00:20:23 electrons settled back, they assumed a new

00:20:23 --> 00:20:25 orientation in line with the momentarily high

00:20:25 --> 00:20:28 magnetic field. This combination of a

00:20:28 --> 00:20:31 dynamo plus a large impact coupled with the impact

00:20:31 --> 00:20:34 shock wave would be enough to explain the Moon's highly

00:20:34 --> 00:20:36 magnetic surface rocks, especially on the far side.

00:20:37 --> 00:20:40 Of course, one way to know for sure is to directly sample these

00:20:40 --> 00:20:43 rocks for signs of shock and high magnetism. And

00:20:43 --> 00:20:46 that could well be possible relatively soon, as the rocks on

00:20:46 --> 00:20:48 the far side are near the lunar south pole, where

00:20:48 --> 00:20:51 NASA's Artemis manned lunar missions are, programmed to land

00:20:51 --> 00:20:54 and explore. Needless to say, we'll

00:20:54 --> 00:20:57 keep you informed. This is space time

00:20:58 --> 00:21:01 still to come. Never before seen details about the

00:21:01 --> 00:21:04 Sun's corona. And later in the science report, a

00:21:04 --> 00:21:07 new study shows that urine rather than water will

00:21:07 --> 00:21:09 be the most efficient method of production if you wanted to make

00:21:09 --> 00:21:12 green hydrogen. All that and more coming up on

00:21:12 --> 00:21:13 space time.

00:21:28 --> 00:21:31 Astronomers have employed a new adaptive optics system,

00:21:31 --> 00:21:34 allowing them to uncover stunning, never before seen

00:21:34 --> 00:21:37 details about the Sun's atmosphere. The corona.

00:21:37 --> 00:21:40 The groundbreaking results reported in the journal Nature Astronomy

00:21:40 --> 00:21:43 are paving the way for deeper insights into coronal heating,

00:21:43 --> 00:21:46 solar eruptions and space weather events.

00:21:47 --> 00:21:50 Research by scientists from the United States National Science

00:21:50 --> 00:21:53 Foundation's National Solar Observatory and the New Jersey

00:21:53 --> 00:21:55 Institute of Technology have produced the clearest high

00:21:55 --> 00:21:58 resolution images of the Sun's corona ever undertaken.

00:21:59 --> 00:22:02 The key is this new coronal adaptive optics

00:22:02 --> 00:22:04 system that removes the blur from images caused by

00:22:04 --> 00:22:07 Earth's atmosphere. Funded by the National

00:22:07 --> 00:22:10 Science foundation and installed on the 1.6 meter

00:22:10 --> 00:22:13 Goode Solar Telescope at Big Bear Solar Observatory in

00:22:13 --> 00:22:16 California, Kona. The name of the adaptive optics system

00:22:16 --> 00:22:19 responsible for these new images compensates for the blur

00:22:19 --> 00:22:21 caused by air turbulence in the atmosphere.

00:22:21 --> 00:22:24 Dirk Schmidt, who helped develop the system, says the turbulence

00:22:24 --> 00:22:27 in the air severely degrades images of objects in space

00:22:27 --> 00:22:29 seen by telescopes, and that includes the Sun.

00:22:30 --> 00:22:33 The Sun's corona, the outermost layer of the Sun's

00:22:33 --> 00:22:35 atmosphere, is visible only during a total solar

00:22:35 --> 00:22:38 eclipse. And its long intrigued science scientists due to its

00:22:38 --> 00:22:41 extreme temperatures, violent eruptions and large

00:22:41 --> 00:22:44 prominences. Among the remarkable observations

00:22:44 --> 00:22:47 seen in these new images are quickly restructuring

00:22:47 --> 00:22:49 solar prominences. Unveiling fine turbulent

00:22:49 --> 00:22:52 internal flows. These look like raindrops

00:22:52 --> 00:22:55 in the Sun's atmosphere. Solar prominences

00:22:55 --> 00:22:58 are large bright features often appearing as arches or

00:22:58 --> 00:23:01 loops and extending out from the Sun's surface.

00:23:01 --> 00:23:04 The corona is heated to millions of degrees, much

00:23:04 --> 00:23:07 hotter than the Sun's surface, which is about 6 degrees.

00:23:07 --> 00:23:10 But the exact methods doing this are still not fully

00:23:10 --> 00:23:13 understood. After all, the Further you get away from a heat source, the

00:23:13 --> 00:23:15 cooler it's supposed to get. The corona is also home

00:23:15 --> 00:23:18 to dynamic phenomena, such as cooler solar plasma

00:23:18 --> 00:23:21 that appears reddish pink during eclipses.

00:23:21 --> 00:23:24 Astronomers believe that resolving the structure and

00:23:24 --> 00:23:27 dynamics of the cooler plasma at smaller scales

00:23:27 --> 00:23:29 holds the key to answering the coronal heating mystery,

00:23:29 --> 00:23:32 thereby improving our understanding of the eruptions ejecting

00:23:32 --> 00:23:35 plasma deep into space, driving space weather the

00:23:35 --> 00:23:37 conditions which in near Earth space are primarily

00:23:37 --> 00:23:40 influenced by the sun's activity, such as solar flares,

00:23:40 --> 00:23:43 coronal mass ejections, and the solar wind.

00:23:44 --> 00:23:46 These effects can impact technology and systems

00:23:46 --> 00:23:49 on the Earth and near Earth space. They can damage or

00:23:49 --> 00:23:52 destroy satellites, cause the Earth's atmosphere to suddenly

00:23:52 --> 00:23:55 expand and contract unexpectedly inducing atmospheric

00:23:55 --> 00:23:58 drag and orbital decay on spacecraft, thereby causing them to

00:23:58 --> 00:24:01 use more fuel. They can also increase radioactive

00:24:01 --> 00:24:04 exposure for astronauts and other crew in space.

00:24:04 --> 00:24:07 They can affect communications and navigation systems.

00:24:07 --> 00:24:09 And they can severely disrupt terrestrial power

00:24:09 --> 00:24:12 grids by overloading power lines, causing

00:24:12 --> 00:24:15 blackouts. Adaptive optics systems like

00:24:15 --> 00:24:17 that used on Kona use a mirror that continually

00:24:17 --> 00:24:20 reshapes itself 2 times every second

00:24:20 --> 00:24:23 in order to counteract the image degradation caused by

00:24:23 --> 00:24:26 turbulent air. I guess you can describe adaptive

00:24:26 --> 00:24:29 optics as sort of being like pumped up autofocus and

00:24:29 --> 00:24:31 optical image stabilization in your smartphone camera,

00:24:31 --> 00:24:34 but correcting the errors for the atmosphere rather than the

00:24:34 --> 00:24:37 user's shaky hands. Since the early

00:24:37 --> 00:24:39 2000s, adaptive optics have been used by large

00:24:39 --> 00:24:42 telescopes, including solar observatories, to study the

00:24:42 --> 00:24:45 Sun's surface, enabling scientists to reach their

00:24:45 --> 00:24:48 theoretical diffraction limits, I.e. the theoretical

00:24:48 --> 00:24:50 maximum resolution of an optical system.

00:24:50 --> 00:24:53 These systems have since revolutionized observing the Sun's

00:24:53 --> 00:24:56 surface, But until now, they have not been used for observing the

00:24:56 --> 00:24:59 corona. And the resolution features beyond the solar

00:24:59 --> 00:25:01 limb stagnated at an order of

00:25:01 --> 00:25:04 1000km or worse. Same levels were

00:25:04 --> 00:25:07 achieved 80 years ago. And that's where this new coronal

00:25:07 --> 00:25:10 adaptive optics system comes in. It closes that

00:25:10 --> 00:25:13 decades old gap, delivering images of coronal features

00:25:13 --> 00:25:16 at 63 kilometer resolution, which is the theoretical

00:25:16 --> 00:25:18 limit of a 1.6 meter telescope.

00:25:18 --> 00:25:20 This is space time.

00:25:22 --> 00:25:24 This episode of space time is brought to you by

00:25:24 --> 00:25:27 Insta360. The trailblazers in

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00:25:44 --> 00:25:47 Dust drops, debris. It's built to survive it all.

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00:26:43 --> 00:26:45 you've got to be one of the first 30 standard package

00:26:45 --> 00:26:48 purchases. For more information, be sure to check out

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00:26:54 --> 00:26:56 use the promo code SpaceTime.

00:26:56 --> 00:26:58 And now it's back to our show

00:27:09 --> 00:27:12 and time. Now to take another brief look at some of the other stories making

00:27:12 --> 00:27:15 use in Science this week with the Science Report,

00:27:16 --> 00:27:19 scientists say they've created a new device that can detect atrial

00:27:19 --> 00:27:21 fibrillation without needing to touch a patient.

00:27:22 --> 00:27:25 Atrial fibrillation, or afib, is an irregular and

00:27:25 --> 00:27:27 often rapid heartbeat, which can be fatal.

00:27:27 --> 00:27:30 Usually, this kind of heart issue is diagnosed with the help of an

00:27:30 --> 00:27:33 electrocardiogram, a device that's connected to the body

00:27:33 --> 00:27:36 and M measures the heart's electrical signals. But a report

00:27:36 --> 00:27:39 in the journal Nature Communications claims researchers say they can

00:27:39 --> 00:27:42 now perform the same monitoring with radar sensing.

00:27:42 --> 00:27:45 The authors evaluated the system using data from over

00:27:45 --> 00:27:48 6 patients that included 229

00:27:48 --> 00:27:50 with afib, and they say it showed comparable

00:27:50 --> 00:27:52 results to a standard ecg.

00:27:54 --> 00:27:57 A new study claims that people who value personal

00:27:57 --> 00:28:00 success, excitement and the challenges of life, as

00:28:00 --> 00:28:03 well as control over other people and resources, are also

00:28:03 --> 00:28:06 more likely to be vegetarians. The

00:28:06 --> 00:28:08 findings, reported in the journal PLOS One, also suggest

00:28:08 --> 00:28:11 that these differences indicate that people who adopt a vegetarian

00:28:11 --> 00:28:14 diet tend to be independent thinkers who aren't

00:28:14 --> 00:28:17 afraid to march to the beat of a different drum.

00:28:17 --> 00:28:20 Fascinatingly, the same study also found that non

00:28:20 --> 00:28:22 vegetarians are more likely to value other people's

00:28:22 --> 00:28:25 welfare, other people's safety and the harmony of

00:28:25 --> 00:28:28 society and social cohesion. The authors

00:28:28 --> 00:28:31 reached their conclusions by analyzing data from three studies in

00:28:31 --> 00:28:34 the United States and Poland in which people were surveyed on their

00:28:34 --> 00:28:37 dietary habits and answered a series of questions on the basic

00:28:37 --> 00:28:40 human values which are important to them. They found

00:28:40 --> 00:28:42 that vegetarians prized basic human values of

00:28:42 --> 00:28:45 stimulation, achievement and power to be more important

00:28:45 --> 00:28:48 than non vegetarians, while non vegetarians

00:28:48 --> 00:28:51 found benevolence, security and conformity

00:28:51 --> 00:28:54 to be more important. The authors admit that these new

00:28:54 --> 00:28:57 results are somewhat at odds with how vegetarianism

00:28:57 --> 00:28:58 is often discussed.

00:29:00 --> 00:29:03 A new study has found that urine, not water, is the

00:29:03 --> 00:29:05 most efficient production method to generate green

00:29:05 --> 00:29:08 hydrogen. The researchers have now developed two

00:29:08 --> 00:29:11 unique energy efficient and cost effective systems that

00:29:11 --> 00:29:14 use urea found in urine and wastewater to

00:29:14 --> 00:29:16 generate hydrogen. A report in the journal Nature

00:29:16 --> 00:29:19 Communications claims the findings show a new pathway to

00:29:19 --> 00:29:22 economically generate green hydrogen, a sustainable and

00:29:22 --> 00:29:25 renewable energy source, and the potential to remediate

00:29:25 --> 00:29:27 nitrogen waste in aquatic systems.

00:29:28 --> 00:29:31 Samsung have just released their latest smartphone, the new

00:29:31 --> 00:29:34 lightweight S25 Edge. With the

00:29:34 --> 00:29:37 details, we're joined by Technology editor Alex Saharov. Roy

00:29:37 --> 00:29:39 from Tech Advice Start Life there's.

00:29:39 --> 00:29:42 Alex Zaharov-Reutt: Been a lot of talk that Apple was going to launch the iPhone 17

00:29:42 --> 00:29:44 Air in 2025 and that was going to be a

00:29:44 --> 00:29:47 5.5 millimeter phone, very thin and it would be

00:29:47 --> 00:29:50 replacing the iPhone 17 plus,

00:29:50 --> 00:29:53 although they might still have that. So knowing this was, you

00:29:53 --> 00:29:56 know, heavily rumored, Samsung decided to gazump

00:29:56 --> 00:29:59 Apple and when they showcased their S25 range

00:29:59 --> 00:30:02 in January this year, the very last thing they showed was the

00:30:02 --> 00:30:05 Samsung S25 Edge. Now this has now come on to

00:30:05 --> 00:30:07 pre sale. I managed to get one in my little

00:30:07 --> 00:30:10 hands today and it is 5.8

00:30:10 --> 00:30:13 millimeters thick. So it's very thin. It's much thinner

00:30:13 --> 00:30:16 than the Samsung S25 Ultra and

00:30:16 --> 00:30:18 thinner than the Samsung A56 mid range

00:30:18 --> 00:30:21 phone. It's about 50 grams lighter than the S25

00:30:21 --> 00:30:24 Ultra, so it's noticeably lighter than the most premium phone. You do

00:30:24 --> 00:30:27 only get two cameras on the back as opposed to the five on the

00:30:27 --> 00:30:30 S25 Ultra. There's obviously no stylus and

00:30:30 --> 00:30:33 you have a 3 milliamp

00:30:33 --> 00:30:35 hour battery as opposed to the 5 milliamp hour

00:30:35 --> 00:30:38 batteries you find on mini of the premium phones today, even the mid

00:30:38 --> 00:30:41 range phone. So you will have to charge it a bit more often

00:30:41 --> 00:30:44 if you're a heavy user of it. We're yet to see the full

00:30:44 --> 00:30:47 ramifications of this in terms of battery life, but

00:30:47 --> 00:30:50 I'm not terribly worried that People are going to be too concerned. And

00:30:50 --> 00:30:52 Apple's battery is meant to be 2

00:30:53 --> 00:30:55 milliamp hours, according to the rumors, although they

00:30:55 --> 00:30:58 are supposed to be using a different battery chemistry that

00:30:58 --> 00:31:00 will give it more capacity than what

00:31:00 --> 00:31:03 2 milliamp hours would normally give you. So

00:31:03 --> 00:31:06 again, we're yet to see in that regard. But holding the phone,

00:31:06 --> 00:31:09 it's delightful. I mean, it's light. They haven't tried betting it, but

00:31:09 --> 00:31:11 people on the Internet say they haven't.

00:31:11 --> 00:31:13 Stuart Gary: They said it's very robust, back pocket and sit down.

00:31:13 --> 00:31:14 That's the test.

00:31:14 --> 00:31:17 Alex Zaharov-Reutt: Well, yes, yes, but I mean, look, they would have done all sorts of stress tests

00:31:17 --> 00:31:20 because there was a huge kerfuffle over the iPhone 6, which was

00:31:20 --> 00:31:23 supposedly bending in people's back pockets when they were doing this. And look,

00:31:23 --> 00:31:26 you're going to buy a case for it, going to be careful with it. I mean, you know, you

00:31:26 --> 00:31:29 don't want to be, manhandling a phone that at The Moment

00:31:29 --> 00:31:32 costs $1 in Australia for

00:31:32 --> 00:31:35 the 512 gig version. There is also a 256

00:31:35 --> 00:31:37 gig version, which is the one that I have though. The age of thin

00:31:37 --> 00:31:38 phones is upon us.

00:31:38 --> 00:31:41 Stuart Gary: That's Alex Zaharov-Reutt from Teg Advice, dot Life.

00:31:56 --> 00:31:59 And that's the show for now. Space Time

00:31:59 --> 00:32:02 is available every Monday, Wednesday and Friday through

00:32:02 --> 00:32:05 Apple Podcasts, itunes, Stitcher, Google

00:32:05 --> 00:32:07 Podcast, Pocketcasts, Spotify,

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00:32:09 --> 00:32:12 bitesz.com, soundcloud, YouTube Music,

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