From Rocket Ruins to Cosmic Discoveries: Blue Origin's Resilience and New Magnetic Insights
Astronomy Daily: Space News June 03, 2026x
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00:17:4916.37 MB

From Rocket Ruins to Cosmic Discoveries: Blue Origin's Resilience and New Magnetic Insights

AnnaAnnaHost
In today's Astronomy Daily, Anna and Avery cover six major stories: Blue Origin CEO Dave Limp pledges New Glenn will fly again before year's end despite last week's launchpad explosion; astronomers announce the first direct evidence of magnetic fields on exoplanets using Hot Jupiter wind data; NASA's Roman Space Telescope clears its final mirror inspection ahead of a September 2026 launch; SpaceX wins a $4.16 billion Space Force contract for an airborne threat-tracking satellite constellation; a reflection on the lasting scientific legacy of interstellar comet 3I/ATLAS; and Hungarian researchers publish the definitive mass boundary between neutron stars and black holes at 2.2–2.3 solar masses. Stories Covered • Blue Origin New Glenn explosion aftermath — CEO Dave Limp confirms damage is less severe than feared, pledges return to flight before end of 2026 • First direct evidence of exoplanet magnetic fields — Nature Astronomy, June 2, 2026 — ESO VLT and Gemini North study of seven Hot Jupiter wind speeds • NASA Roman Space Telescope primary mirror passes final Earth-side inspection — September 2026 launch target confirmed • SpaceX $4.16 billion US Space Force SB-AMTI contract — threat-tracking satellite constellation targeting 2028 operational capability • 3I/ATLAS scientific legacy — new analysis on what the interstellar comet reveals about solar system formation across the Milky Way • Neutron star mass limit defined at 2.2–2.3 solar masses — HUN-REN Wigner Research Centre for Physics, Hungary Key Terms Explained • Hot Jupiter: A gas giant exoplanet similar in size to Jupiter, orbiting very close to its host star, typically tidally locked • Magnetic field: An invisible force field generated by electrically conducting material moving inside a planet, critical for atmospheric protection • Lagrange point 2 (L2): A gravitationally stable point in space approximately 1.5 million kilometres from Earth, opposite the Sun — home to both JWST and (soon) Roman • SB-AMTI: Space-Based Airborne Moving Target Indicator — a satellite constellation for tracking airborne threats from orbit • Neutron star: The ultra-dense remnant of a collapsed massive star, composed almost entirely of neutrons • 3I/ATLAS: Third confirmed interstellar object, discovered July 2025; an active comet from outside our solar system • Deuterium: A heavy isotope of hydrogen containing one neutron; its abundance in 3I/ATLAS water suggests formation in an extremely cold environment

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00:00:00 --> 00:00:02 Anna: Last week, a rocket exploded on its launch

00:00:02 --> 00:00:05 pad in Cape Canaveral. The fireball could be

00:00:05 --> 00:00:08 seen from miles. This week, the CEO

00:00:08 --> 00:00:10 of Blue Origin looked at the wreckage and

00:00:10 --> 00:00:13 said, five, we will fly again

00:00:13 --> 00:00:16 this year. That story, plus magnetic

00:00:16 --> 00:00:19 fields discovered on distant worlds. A, uh,

00:00:19 --> 00:00:21 space telescope moments from launch, and

00:00:21 --> 00:00:24 the definitive answer to one of astronomy's

00:00:24 --> 00:00:26 oldest questions. This is

00:00:26 --> 00:00:28 Astronomy Daily.

00:00:28 --> 00:00:31 Avery: Hello and welcome to Astronomy Daily, your

00:00:31 --> 00:00:33 daily guide to the universe and everything in

00:00:33 --> 00:00:34 it. I'm Avery.

00:00:34 --> 00:00:37 Anna: And I'm Anna. It is Wednesday the 4th of

00:00:37 --> 00:00:40 June, 2026, and we have an

00:00:40 --> 00:00:41 exceptional episode lined up.

00:00:41 --> 00:00:44 Avery: Today we do six stories

00:00:44 --> 00:00:46 ranging from a dramatic comeback story in the

00:00:46 --> 00:00:48 world of commercial spaceflight to a

00:00:48 --> 00:00:51 scientific first that reshapes what we know

00:00:51 --> 00:00:53 about planets beyond our solar system.

00:00:54 --> 00:00:55 If you've been listening this week, you'll

00:00:55 --> 00:00:58 know Blue Origin had a very bad Thursday.

00:00:58 --> 00:01:00 We'll have a full update on what comes next,

00:01:00 --> 00:01:01 but let's get into it.

00:01:02 --> 00:01:04 Anna: Last Thursday night at Cape Canaveral, Blue

00:01:04 --> 00:01:07 Origin's New Glenn rocket exploded on its

00:01:07 --> 00:01:10 launch pad during a routine pre launch hot

00:01:10 --> 00:01:13 fire test. The fireball engulfed Launch

00:01:13 --> 00:01:15 Complex 36. Debris was found up

00:01:15 --> 00:01:18 to half a mile away. It was the biggest and

00:01:18 --> 00:01:20 most public failure in the company's history,

00:01:21 --> 00:01:24 and many observers feared the road back could

00:01:24 --> 00:01:24 take years.

00:01:25 --> 00:01:28 Avery: But as of this week, Blue Origin CEO

00:01:28 --> 00:01:30 Dave Limp is pushing back hard on that

00:01:30 --> 00:01:33 narrative. He's saying the damage is far less

00:01:33 --> 00:01:34 catastrophic than it looked.

00:01:35 --> 00:01:38 Anna: Limp posted a, uh, detailed update on X in

00:01:38 --> 00:01:40 which he said that now that teams have gained

00:01:40 --> 00:01:43 full access to the pad, there's actually some

00:01:43 --> 00:01:44 good news. The propellant storage

00:01:44 --> 00:01:47 infrastructure, the oxygen tanks, the liquid

00:01:47 --> 00:01:50 hydrogen storage, and the cryogenic methane

00:01:50 --> 00:01:52 tanks all came through the blast in good

00:01:52 --> 00:01:55 shape. He called that extremely fortunate

00:01:55 --> 00:01:58 because those are very long lead items to

00:01:58 --> 00:01:58 replace.

00:01:59 --> 00:02:01 Avery: The water tower also survived. The main

00:02:01 --> 00:02:04 support gantry is damaged, but crucially,

00:02:04 --> 00:02:07 Limp says it can be repaired in place. It

00:02:07 --> 00:02:09 doesn't need to be torn down and rebuilt from

00:02:09 --> 00:02:09 scratch.

00:02:10 --> 00:02:12 Anna: Perhaps most importantly, there are spare

00:02:12 --> 00:02:15 assets. The previously flown New Glenn

00:02:15 --> 00:02:18 Booster, nicknamed Never Tell Me the Odds,

00:02:18 --> 00:02:20 along with three upper stages stored in a

00:02:20 --> 00:02:23 neighboring integration facility, all appear

00:02:23 --> 00:02:24 undamaged.

00:02:24 --> 00:02:26 Avery: As for the cause of the explosion, there's

00:02:26 --> 00:02:29 still no official word. The test was not

00:02:29 --> 00:02:31 within the scope of FAA license activities,

00:02:31 --> 00:02:33 so the FAA won't be leading the

00:02:33 --> 00:02:36 investigation. Blue Origin is conducting its

00:02:36 --> 00:02:37 own assessment.

00:02:37 --> 00:02:39 Anna: Limp also used the moment to announce a

00:02:39 --> 00:02:42 strategic pivot the company had already been

00:02:42 --> 00:02:44 working on, eliminating the need for a

00:02:44 --> 00:02:47 transporter erector, the massive structure

00:02:47 --> 00:02:50 used to move and stand the rocket upright. He

00:02:50 --> 00:02:53 said Blue Origin will now skip straight to an

00:02:53 --> 00:02:55 alternative vertical launch concept, which

00:02:55 --> 00:02:57 means they don't need to build a replacement

00:02:57 --> 00:02:59 for the one destroyed during the explosion.

00:03:00 --> 00:03:02 Avery: And he closed his statement with Blue

00:03:02 --> 00:03:04 Origin's motto, gradatum ferociter,

00:03:05 --> 00:03:06 which means step by step,

00:03:07 --> 00:03:10 ferociously, and the declaration we

00:03:10 --> 00:03:12 will fly again before the end of this year.

00:03:12 --> 00:03:15 Anna: That's an aggressive timeline by any measure,

00:03:15 --> 00:03:17 but it's the kind of defiant pledge

00:03:17 --> 00:03:20 investors, customers and the broader space

00:03:20 --> 00:03:23 industry needed to hear. Patrick Space Force

00:03:23 --> 00:03:25 Base has cleared Blue Origin to begin its

00:03:25 --> 00:03:28 full damage assessment of Launch Complex 36,

00:03:28 --> 00:03:31 though the formal rebuilding process is now

00:03:31 --> 00:03:31 underway.

00:03:32 --> 00:03:34 Avery: We will of course, keep tracking this story

00:03:34 --> 00:03:35 as it develops.

00:03:35 --> 00:03:38 Anna: Now let's move from the dramatic to the

00:03:38 --> 00:03:41 extraordinary. Scientists have just published

00:03:41 --> 00:03:43 what they're calling the first direct

00:03:43 --> 00:03:45 evidence that planets beyond our solar system

00:03:46 --> 00:03:48 possess magnetic fields. And they found it

00:03:48 --> 00:03:50 by studying the wind.

00:03:50 --> 00:03:53 Avery: This is a remarkable piece of science. A team

00:03:53 --> 00:03:55 of astronomers used two of the world's most

00:03:55 --> 00:03:58 powerful ground based telescopes, the ESO's

00:03:58 --> 00:04:01 Very Large Telescope in Chile and the Gemini

00:04:01 --> 00:04:03 North Telescope in Hawaii, to measure wind

00:04:03 --> 00:04:05 speeds on seven so called hot Jupiter

00:04:05 --> 00:04:06 exoplanets.

00:04:07 --> 00:04:10 Anna: Hot Jupiters are gas giants roughly the

00:04:10 --> 00:04:13 size of Jupiter but orbiting extremely

00:04:13 --> 00:04:15 close to their host stars, far closer than

00:04:15 --> 00:04:18 Mercury is to our sun because they're

00:04:18 --> 00:04:21 tidally locked, always showing the same face

00:04:21 --> 00:04:24 to their star. One side is perpetually

00:04:24 --> 00:04:26 scorching hot and the other is freezing

00:04:26 --> 00:04:29 cold. That temperature difference creates

00:04:29 --> 00:04:32 powerful winds that howl from the day side to

00:04:32 --> 00:04:33 the night side.

00:04:33 --> 00:04:36 Avery: The researchers measured those wind speeds

00:04:36 --> 00:04:38 and found something totally counterintuitive.

00:04:39 --> 00:04:41 On the hotter planets, the winds were

00:04:41 --> 00:04:43 actually slower, and that is the opposite of

00:04:43 --> 00:04:45 what standard physics would predict.

00:04:45 --> 00:04:48 Anna: If you have more thermal energy, you'd expect

00:04:48 --> 00:04:51 stronger winds. But these planets are pumping

00:04:51 --> 00:04:54 the brakes. And the best explanation, the one

00:04:54 --> 00:04:57 that actually fits the data, is magnetic

00:04:57 --> 00:04:57 fields.

00:04:58 --> 00:05:00 Avery: A magnetic field can interact with the

00:05:00 --> 00:05:02 electrically charged gas in a planet's upper

00:05:02 --> 00:05:05 atmosphere and slow those winds down. The

00:05:05 --> 00:05:07 stronger the magnetic field, the greater the

00:05:07 --> 00:05:10 braking effect. The team inferred magnetic

00:05:10 --> 00:05:13 field strengths ranging up to four times that

00:05:13 --> 00:05:16 of Saturn and up to about half the strength

00:05:16 --> 00:05:17 of Jupiter's field.

00:05:17 --> 00:05:19 Anna: The wind speeds themselves were

00:05:19 --> 00:05:22 extraordinary. They ranged from around

00:05:22 --> 00:05:25 7 km per hour up to more

00:05:25 --> 00:05:27 than 25 km per hour.

00:05:28 --> 00:05:30 For context, the fastest winds measured on

00:05:30 --> 00:05:33 Jupiter reach about 1

00:05:33 --> 00:05:36 kilometers per hour. These are winds on a

00:05:36 --> 00:05:38 scale we simply don't see in our own solar

00:05:38 --> 00:05:38 system.

00:05:39 --> 00:05:41 Avery: The results were published in the journal

00:05:41 --> 00:05:44 nature astronomy on June 2, and the

00:05:44 --> 00:05:46 implications go well beyond just knowing that

00:05:46 --> 00:05:49 Other planets have magnetic fields. Magnetic

00:05:49 --> 00:05:51 fields are thought to play a critical role in

00:05:51 --> 00:05:53 protecting planetary atmospheres from being

00:05:53 --> 00:05:56 stripped away by stellar radiation, which is

00:05:56 --> 00:05:58 one of the key factors in whether a planet

00:05:58 --> 00:06:01 could over billions of years, be potentially

00:06:01 --> 00:06:02 remain habitable.

00:06:03 --> 00:06:05 Anna: As the lead researcher put it, this is a key

00:06:05 --> 00:06:08 step toward ultimately understanding which

00:06:08 --> 00:06:11 planets can stay alive, keep their water,

00:06:11 --> 00:06:14 and perhaps even one day host life

00:06:14 --> 00:06:15 as we know it.

00:06:15 --> 00:06:17 Avery: A genuinely landmark result.

00:06:18 --> 00:06:21 Anna: Our next story takes us to NASA's Goddard

00:06:21 --> 00:06:23 Space Flight center in Greenbelt, Maryland,

00:06:23 --> 00:06:25 where engineers have completed what they

00:06:25 --> 00:06:28 describe as the last look humanity

00:06:28 --> 00:06:31 will ever take on a critical piece of

00:06:31 --> 00:06:33 hardware before it becomes the eyes of

00:06:33 --> 00:06:35 humanity on the universe.

00:06:35 --> 00:06:38 Avery: We're talking about the Nancy Grace Roman

00:06:38 --> 00:06:41 Space Telescope and specifically its primary

00:06:41 --> 00:06:43 mirror, a 2.4 meter

00:06:45 --> 00:06:47 reflector that will be the heart of the

00:06:47 --> 00:06:49 instrument once it launches into space.

00:06:49 --> 00:06:51 Anna: On May 20th and 21st,

00:06:52 --> 00:06:54 engineers performed a meticulous final

00:06:54 --> 00:06:57 inspection. They tilted the entire

00:06:57 --> 00:07:00 observatory onto its side, deployed the

00:07:00 --> 00:07:02 protective hood that will be stowed during

00:07:02 --> 00:07:05 launch, and used a high resolution camera

00:07:05 --> 00:07:08 with a powerful zoom lens to do a thorough

00:07:08 --> 00:07:10 multipurpose check, looking for any particles

00:07:10 --> 00:07:13 that may have settled on the mirror surface

00:07:13 --> 00:07:15 during testing and confirming that the

00:07:15 --> 00:07:16 optical alignment hadn't

00:07:16 --> 00:07:19 Avery: shifted it pass with flying colors.

00:07:20 --> 00:07:22 No specs, no misalignment. The

00:07:22 --> 00:07:24 mirror's silver coating, which is just

00:07:24 --> 00:07:27 400nm thick, hundreds

00:07:27 --> 00:07:29 of times thinner than a human hair, is

00:07:29 --> 00:07:30 perfect.

00:07:31 --> 00:07:34 Anna: The Roman telescope manager at Goddard, J.

00:07:34 --> 00:07:36 Scott Smith, marked the moment beautifully.

00:07:37 --> 00:07:39 He said the Roman engineering team laid

00:07:39 --> 00:07:42 eyes on the telescope for the final time

00:07:42 --> 00:07:45 before it in turn becomes the eyes of

00:07:45 --> 00:07:47 humanity, revealing the wonders of the

00:07:47 --> 00:07:50 cosmos. That's a sentence worth sitting with.

00:07:51 --> 00:07:53 Avery: With this milestone complete, Roman will now

00:07:53 --> 00:07:56 be shipped to Kennedy Space center in Florida

00:07:56 --> 00:07:57 in preparation for its planned launch,

00:07:58 --> 00:08:00 currently scheduled for as early as, ah,

00:08:00 --> 00:08:01 September 2026.

00:08:02 --> 00:08:04 Anna: Once in space, Roman will travel to the sun,

00:08:04 --> 00:08:07 earth, Lagrange point 2, known as

00:08:07 --> 00:08:10 L2, the same orbital neighborhood where the

00:08:10 --> 00:08:13 James Webb Space Telescope operates. It will

00:08:13 --> 00:08:15 join the most exclusive telescope real estate

00:08:15 --> 00:08:16 in the solar system.

00:08:17 --> 00:08:19 Avery: And Roman's scientific ambitions are

00:08:19 --> 00:08:22 extraordinary. It will have a field of view

00:08:22 --> 00:08:24 at least 100 times larger than the Hubble

00:08:24 --> 00:08:27 Space Telescope, potentially measuring light

00:08:27 --> 00:08:29 from a billion galaxies over its lifetime.

00:08:30 --> 00:08:32 It will also be capable of directly imaging

00:08:32 --> 00:08:35 exoplanets by blocking out starlight

00:08:35 --> 00:08:37 and conducting a comprehensive statistical

00:08:37 --> 00:08:40 census of planetary systems across our

00:08:40 --> 00:08:40 galaxy.

00:08:41 --> 00:08:43 Anna: We are getting very close to launch.

00:08:43 --> 00:08:45 September can't come soon enough.

00:08:45 --> 00:08:47 Avery: We'll be right back after this short break

00:08:47 --> 00:08:48 for a word from our sponsors.

00:08:48 --> 00:08:51 Anna: Stay with us and we're back three more

00:08:51 --> 00:08:54 stories to go and they are all fascinating.

00:08:54 --> 00:08:57 Avery: Space Force Has Made a Very large Investment

00:08:57 --> 00:09:00 in SpaceX On May 29, the US

00:09:00 --> 00:09:02 Space Force announced it had awarded Elon

00:09:02 --> 00:09:05 Musk's company a $4.16

00:09:05 --> 00:09:08 billion contract for a program called the

00:09:08 --> 00:09:10 Space Based Airborne Moving Target

00:09:10 --> 00:09:12 Indicator, or SBAMTI M.

00:09:13 --> 00:09:15 Anna: In plain language, the goal is to build a

00:09:15 --> 00:09:17 constellation of satellites that can track

00:09:17 --> 00:09:20 and target airborne threats from orbit,

00:09:20 --> 00:09:22 things like aircraft, cruise missiles and

00:09:22 --> 00:09:25 other fast moving threats anywhere on Earth

00:09:25 --> 00:09:26 at any time.

00:09:26 --> 00:09:28 Avery: The satellites are designed to fill a gap

00:09:28 --> 00:09:30 that currently exists in military

00:09:30 --> 00:09:32 surveillance. Traditionally, the US

00:09:32 --> 00:09:35 Military uses aircraft, particularly AWOKS

00:09:35 --> 00:09:38 planes, to track airborne targets. But

00:09:38 --> 00:09:40 satellites can reach areas where it's too

00:09:40 --> 00:09:42 dangerous to fly and they can maintain

00:09:42 --> 00:09:45 persistent coverage that aircraft simply

00:09:45 --> 00:09:45 can't match.

00:09:46 --> 00:09:47 Anna: The contract is part of the Trump

00:09:47 --> 00:09:50 administration's broader Golden Dome Missile

00:09:50 --> 00:09:52 Defense Initiative, which aims to build a

00:09:52 --> 00:09:54 layered national defense system including

00:09:54 --> 00:09:57 ground based interceptors, enhanced radar

00:09:57 --> 00:10:00 networks, and now this space based tracking

00:10:00 --> 00:10:00 layer.

00:10:00 --> 00:10:03 Avery: SpaceX isn't the only company involved. Space

00:10:03 --> 00:10:05 Force confirmed there are nine companies in

00:10:05 --> 00:10:08 the SBA MTI vendor pool, though the

00:10:08 --> 00:10:10 identities of the other eight have not been

00:10:10 --> 00:10:12 made public for national security reasons.

00:10:13 --> 00:10:15 More contracts are expected to be issued over

00:10:15 --> 00:10:16 the coming year.

00:10:16 --> 00:10:18 Anna: The goal is to have an initial operational

00:10:18 --> 00:10:21 constellation of these satellites in place by

00:10:21 --> 00:10:24 2028. This contract was also

00:10:24 --> 00:10:26 accompanied by a separate $2.29

00:10:26 --> 00:10:29 billion Space Force award to SpaceX

00:10:29 --> 00:10:32 earlier in the week for a Space Data Network

00:10:32 --> 00:10:35 backbone, a secure high speed military

00:10:35 --> 00:10:36 communication system.

00:10:36 --> 00:10:39 Avery: In total, SpaceX received over six and a half

00:10:39 --> 00:10:42 billion dollars in Space Force contracts in a

00:10:42 --> 00:10:44 single week. For a company that is also

00:10:44 --> 00:10:46 preparing for what could be the largest IPO

00:10:46 --> 00:10:49 in stock market history, it's been quite a

00:10:49 --> 00:10:50 week in Hawthorne, California.

00:10:51 --> 00:10:53 Anna: Now an update about a visitor that has

00:10:53 --> 00:10:55 already left, but whose influence is still

00:10:55 --> 00:10:58 being felt across the astronomy community.

00:10:58 --> 00:11:00 Avery: 3i ATLAS, the third

00:11:00 --> 00:11:03 interstellar object ever confirmed to pass

00:11:03 --> 00:11:06 through our solar system. Discovered on July

00:11:06 --> 00:11:09 1, 2025 by the Atlas Telescope Network in

00:11:09 --> 00:11:11 Chile, it is now heading back out into the

00:11:11 --> 00:11:13 deep Galaxy, never to return.

00:11:13 --> 00:11:16 Anna: But the scientific conversation it sparked is

00:11:16 --> 00:11:19 very much alive. A new analysis published

00:11:19 --> 00:11:21 this week explores the way that 3i

00:11:21 --> 00:11:24 atlas has prompted astronomers to

00:11:24 --> 00:11:26 fundamentally update what they understand

00:11:26 --> 00:11:29 not just about foreign solar systems, but

00:11:29 --> 00:11:29 about our own.

00:11:30 --> 00:11:32 Avery: Let's do a quick recap for listeners who may

00:11:32 --> 00:11:35 have joined us since the main 3i Atlas

00:11:35 --> 00:11:38 coverage last year. This was an extraordinary

00:11:38 --> 00:11:40 object. It was only the third interstellar

00:11:40 --> 00:11:43 visitor ever confirmed after 1i

00:11:43 --> 00:11:46 Oumuamua, um, in 2017 and

00:11:46 --> 00:11:48 2i Borisov in 2019.

00:11:49 --> 00:11:51 But unlike those, 2 3i Atlas

00:11:51 --> 00:11:54 was clearly an active comet, releasing dust

00:11:54 --> 00:11:57 and gas with multiple tails and a nucleus

00:11:57 --> 00:11:59 estimated at somewhere between a few hundred

00:11:59 --> 00:12:02 meters and several kilometers across.

00:12:02 --> 00:12:05 Anna: It passed closest to the sun in late October

00:12:05 --> 00:12:08 2025, then flew by Mars, then

00:12:08 --> 00:12:10 Jupiter, in March 2026, and is now

00:12:10 --> 00:12:13 departing. But even as it fades, the data it

00:12:13 --> 00:12:15 generated continues to be analyzed.

00:12:16 --> 00:12:18 Avery: One of the most striking findings came from a

00:12:18 --> 00:12:20 University of Michigan study that examined

00:12:20 --> 00:12:23 the water ice in 3i atlas

00:12:23 --> 00:12:26 and found it contained an extraordinarily

00:12:26 --> 00:12:28 high concentration of deuterium heavy

00:12:28 --> 00:12:31 isotope of hydrogen that is far less common

00:12:31 --> 00:12:33 in comets from our own solar system.

00:12:33 --> 00:12:36 Anna: That suggests three I ATLAS

00:12:36 --> 00:12:38 formed in an environment that was

00:12:38 --> 00:12:40 dramatically colder and more isolated than

00:12:40 --> 00:12:43 the conditions that shaped our solar system's

00:12:43 --> 00:12:46 comets. Researchers have since traced its

00:12:46 --> 00:12:49 likely origin to a cold, dark corner of the

00:12:49 --> 00:12:51 Milky Way that had not yet fully assembled

00:12:51 --> 00:12:54 into a planetary system when this object

00:12:54 --> 00:12:57 formed, potentially making it up to 11

00:12:57 --> 00:13:00 billion years old, more than twice the age of

00:13:00 --> 00:13:00 our Sun.

00:13:01 --> 00:13:03 Avery: What does all of this teach us? Quite a lot,

00:13:03 --> 00:13:05 as it turns out. It tells us that the

00:13:05 --> 00:13:07 chemical signatures of comets vary

00:13:07 --> 00:13:10 dramatically across the galaxy, meaning the

00:13:10 --> 00:13:12 building blocks of planetary systems,

00:13:12 --> 00:13:15 including the water and organics that may

00:13:15 --> 00:13:17 seed life differ significantly from one

00:13:17 --> 00:13:19 stellar neighborhood to another.

00:13:19 --> 00:13:22 Anna: It also demonstrates how much we can learn

00:13:22 --> 00:13:24 from fleeting cosmic visitors, and if we have

00:13:24 --> 00:13:27 the tools to observe them quickly. The

00:13:27 --> 00:13:30 Veracruz Rubin Observatory in Chile, which

00:13:30 --> 00:13:32 released its first images in June, is

00:13:32 --> 00:13:35 expected to dramatically increase the rate at

00:13:35 --> 00:13:37 which we detect future interstellar objects,

00:13:37 --> 00:13:40 which could let astronomers determine whether

00:13:40 --> 00:13:42 three I Atlas unusual

00:13:42 --> 00:13:45 properties are rare or commonplace.

00:13:45 --> 00:13:47 Avery: A visitor that has left the building but

00:13:47 --> 00:13:50 whose lessons will be with us for years to

00:13:50 --> 00:13:50 come.

00:13:50 --> 00:13:53 Anna: Our final story today answers a question that

00:13:53 --> 00:13:55 astrophysicists have been wrestling with for

00:13:56 --> 00:13:59 at what exact mass does a neutron star

00:13:59 --> 00:14:00 collapse into a black hole?

00:14:01 --> 00:14:03 Avery: This is one of those wonderfully fundamental

00:14:03 --> 00:14:05 questions in physics. We know that when a

00:14:05 --> 00:14:08 massive star dies, it can leave behind either

00:14:08 --> 00:14:11 a neutron star or a black hole, depending on

00:14:11 --> 00:14:13 how massive the original star was. But the

00:14:13 --> 00:14:16 precise boundary between those two fates has

00:14:16 --> 00:14:19 never been defeated definitively pinned down

00:14:19 --> 00:14:20 until now.

00:14:20 --> 00:14:23 Anna: Researchers at the Hun Ren Wigner Research

00:14:23 --> 00:14:25 center for Physics in Hungary have published

00:14:25 --> 00:14:28 what they describe as a definitive answer.

00:14:28 --> 00:14:31 The boundary falls between 2.2 and

00:14:31 --> 00:14:32 2.3 solar masses.

00:14:33 --> 00:14:36 Avery: To unpack that a neutron star is one of

00:14:36 --> 00:14:38 the most extreme objects in the universe,

00:14:38 --> 00:14:41 imagine taking the mass of two suns and

00:14:41 --> 00:14:44 compressing it into a sphere about the size

00:14:44 --> 00:14:47 of a city. A teaspoon of its material would

00:14:47 --> 00:14:49 weigh billions of tons. These are

00:14:49 --> 00:14:52 objects so dense that the neutrons themselves

00:14:52 --> 00:14:55 are packed together like one giant atomic

00:14:55 --> 00:14:55 nucleus.

00:14:56 --> 00:14:58 Anna: But there's a limit to how much mass a

00:14:58 --> 00:15:01 neutron star can hold before gravity wins

00:15:01 --> 00:15:03 and the whole thing collapses inward to form

00:15:03 --> 00:15:06 a black hole. That limit, the Tolman,

00:15:06 --> 00:15:09 Oppenheimer, Volkov limit, has previously

00:15:09 --> 00:15:11 been estimated to be somewhere between two

00:15:11 --> 00:15:14 and three solar masses. Depending on the

00:15:14 --> 00:15:16 assumptions used, this new

00:15:16 --> 00:15:18 Avery: work narrows that window considerably,

00:15:18 --> 00:15:21 placing the critical threshold between 2.2

00:15:21 --> 00:15:23 and 2.3 solar masses.

00:15:24 --> 00:15:27 Beyond that, a neutron star simply cannot

00:15:27 --> 00:15:29 support itself against gravity, and the black

00:15:29 --> 00:15:30 hole is born.

00:15:30 --> 00:15:32 Anna: Why does this matter? Because it gives

00:15:32 --> 00:15:35 astronomers a clearer tool to classify

00:15:35 --> 00:15:38 compact objects they observe. When we detect

00:15:38 --> 00:15:40 something via, uh, gravitational waves or X

00:15:40 --> 00:15:43 ray observations, knowing the precise mass

00:15:43 --> 00:15:45 boundary between neutron stars and black

00:15:45 --> 00:15:48 holes helps us identify what we're actually

00:15:48 --> 00:15:49 looking at.

00:15:49 --> 00:15:51 Avery: It also feeds into our understanding of what

00:15:51 --> 00:15:54 happens in neutron star m mergers, the

00:15:54 --> 00:15:56 cataclysmic collisions that produce

00:15:56 --> 00:15:58 gravitational wave signals, and some of the

00:15:58 --> 00:16:00 most energetic explosions in the universe.

00:16:01 --> 00:16:03 Anna: A beautifully precise answer to one of the

00:16:03 --> 00:16:06 universe's most extreme questions.

00:16:06 --> 00:16:09 Avery: Before we go, a quick look at the June sky

00:16:09 --> 00:16:11 for our listeners in Australia, New Zealand,

00:16:11 --> 00:16:13 and across the Southern hemisphere.

00:16:13 --> 00:16:15 Anna: June is a wonderful month for southern

00:16:15 --> 00:16:17 observers. We're heading toward the winter

00:16:17 --> 00:16:20 solstice on June 21, which means longer

00:16:20 --> 00:16:23 nights, prime time for stargazing.

00:16:23 --> 00:16:26 Jupiter and Venus are currently visible in

00:16:26 --> 00:16:29 the western sky after sunset, and on June

00:16:29 --> 00:16:31 9, they'll appear at their closest to each

00:16:31 --> 00:16:34 other, a spectacular conjunction worth

00:16:34 --> 00:16:35 getting outside for.

00:16:35 --> 00:16:38 Avery: The Milky Way core is also rising in the

00:16:38 --> 00:16:40 evening sky from the Southern hemisphere

00:16:40 --> 00:16:42 right now, beautifully positioned for

00:16:42 --> 00:16:44 photography and naked eye observation in dark

00:16:44 --> 00:16:47 sky locations away from city lights.

00:16:47 --> 00:16:50 Anna: That is all from us for today. Six stories,

00:16:50 --> 00:16:52 and every one of them a reminder that the

00:16:52 --> 00:16:54 universe is never standing still.

00:16:55 --> 00:16:58 Avery: From blue origin's defiant pledge to rise

00:16:58 --> 00:17:00 from the ashes to magnetic fields discovered

00:17:00 --> 00:17:03 on distant worlds, it has been a remarkable

00:17:03 --> 00:17:04 day to cover space.

00:17:05 --> 00:17:07 Anna: If you enjoyed today's episode, please

00:17:07 --> 00:17:10 subscribe, leave us a review, and tell a

00:17:10 --> 00:17:13 fellow space lover about the show. Find us on

00:17:13 --> 00:17:15 Instagram, Facebook, and x@, uh,

00:17:15 --> 00:17:17 astrodaily pod

00:17:17 --> 00:17:18 and@astronomydaily.IO.

00:17:19 --> 00:17:20 Avery: i'm Avery.

00:17:20 --> 00:17:22 Anna: And, uh, I'm Anna. We'll see you tomorrow.

00:17:22 --> 00:17:24 And until then, keep looking up.

00:17:37 --> 00:17:48 Avery: Sam.