What Keeps a Galaxy Churning: Andromeda's Supernova Secrets Revealed
Astronomy Daily: Space News September 22, 2026x
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What Keeps a Galaxy Churning: Andromeda's Supernova Secrets Revealed

AnnaAnnaHost
Supernovae keep galaxies churning A new study led by Fan Yi Meng from Tsinghua University provides the first comprehensive census of superbubbles in the Andromeda Galaxy, revealing that clustered supernova feedback is sufficient to sustain galactic-scale turbulence. This finding helps to explain why galaxies remain active over billions of years, with turbulence playing a crucial role in regulating star formation rates. The research, published in Nature Astronomy, highlights the energy balance between supernovae and the turbulence they create.Neutrinos may dictate stellar explosions A paper from Mariam Gogilashvili and Irene Tambora at the Niels Bohr Institute explores the role of neutrinos in determining which massive stars explode as supernovae. Their findings suggest that neutrino oscillations could lead to a significant number of stars collapsing into black holes, particularly those in the 16 to 30 solar mass range, addressing the long-standing red supergiant problem.TOI 1355b: A planet with an expiry date Researchers from the University of Tokyo have discovered TOI 1355b, a hot Jupiter with a unique eccentric orbit around an A-type star. This planet will stop transiting its host star by 2033 due to nodal precession, providing a rare opportunity to study its characteristics before it disappears from view.SpaceX Crew Missions Update NASA has contracted SpaceX for three additional crew rotation missions to the International Space Station, extending their partnership and ensuring continued access to the station. Crew 13 is currently in quarantine, with a launch targeted for early October.The Sun goes blank For the first time since February, the Sun has gone completely spotless, marking a significant moment in the solar cycle. As solar activity declines, a coronal hole is set to rotate into position, potentially leading to minor geomagnetic storms and auroras.1. Supernovae keep galaxies churning2. Neutrinos may dictate stellar explosions3. TOI 1355b: A planet with an expiry date4. SpaceX Crew Missions Update5. The Sun goes blankBecome a supporter of this podcast: https://www.spreaker.com/podcast/astronomy-daily-latest-space-news--5648921/support.

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00:00:00 --> 00:00:02 Anna: A galaxy should be quiet. Stir

00:00:02 --> 00:00:05 a cloud of gas and the churning dies away in

00:00:05 --> 00:00:08 a few million years, like ripples going flat

00:00:08 --> 00:00:11 on a pond. And yet every spiral

00:00:11 --> 00:00:13 galaxy we look at is still churning.

00:00:13 --> 00:00:15 Something keeps stirring the pot.

00:00:16 --> 00:00:18 Avery: Today, a survey of the galaxy next door that

00:00:18 --> 00:00:21 catches a spoon in the act, plus the

00:00:21 --> 00:00:23 ghostly particles that may decide which stars

00:00:23 --> 00:00:26 explode at all. A planet with an expiry

00:00:26 --> 00:00:28 date and the sun goes blank for the first

00:00:28 --> 00:00:29 time since February.

00:00:30 --> 00:00:31 Anna: The I'm Anna.

00:00:31 --> 00:00:34 Avery: And I'm Avery. This is astronomy daily,

00:00:34 --> 00:00:36 episode 199.

00:00:36 --> 00:00:39 Anna: Start with a problem that has sat in the

00:00:39 --> 00:00:42 background of galaxy science for about 50

00:00:42 --> 00:00:45 years, and that has the useful quality of

00:00:45 --> 00:00:48 being easy to state and very hard to

00:00:48 --> 00:00:51 answer. The gas between the stars in a

00:00:51 --> 00:00:53 galaxy is turbulent. It is not sitting still

00:00:53 --> 00:00:56 and it is not flowing smoothly. It is

00:00:56 --> 00:00:59 churning on every scale from a few light

00:00:59 --> 00:01:02 years up to thousands, with gas moving at

00:01:02 --> 00:01:04 something like 10 kilometres a second

00:01:04 --> 00:01:06 relative to its neighbours. We have measured

00:01:06 --> 00:01:09 this in our own galaxy and in every nearby

00:01:09 --> 00:01:12 galaxy we can resolve it is simply how

00:01:12 --> 00:01:15 interstellar gas behaves. Here is the

00:01:15 --> 00:01:18 problem. Turbulence dies. That is

00:01:18 --> 00:01:20 the one thing turbulence reliably does.

00:01:21 --> 00:01:24 Energy cascades from big eddies down to

00:01:24 --> 00:01:26 small eddies, and at the bottom it turns into

00:01:26 --> 00:01:29 heat and it gone. In

00:01:29 --> 00:01:31 1999, an astrophysicist named

00:01:31 --> 00:01:34 Mordecai Mark Macklow put a number on

00:01:34 --> 00:01:36 how fast that happens in interstellar

00:01:36 --> 00:01:39 conditions. And the number was brutal.

00:01:40 --> 00:01:42 Turbulence in a galaxy's gas should decay

00:01:42 --> 00:01:45 away in roughly the time it takes the gas to

00:01:45 --> 00:01:48 cross itself once a few tens of

00:01:48 --> 00:01:50 millions of years on a galactic clock.

00:01:50 --> 00:01:53 That's an afternoon. So the churning

00:01:53 --> 00:01:56 we see should not be there unless

00:01:56 --> 00:01:58 something is putting the energy back

00:01:58 --> 00:02:01 continuously for billions of years.

00:02:01 --> 00:02:03 Avery: And there has never been a shortage of

00:02:03 --> 00:02:04 suspects.

00:02:04 --> 00:02:07 Anna: No shortage at all. Supernovae are

00:02:07 --> 00:02:10 the obvious one. But gravity itself can

00:02:10 --> 00:02:13 drive turbulence. As the disc shears and

00:02:13 --> 00:02:16 clumps, there is the magnetorotational

00:02:16 --> 00:02:18 instability, which wrings energy out of the

00:02:18 --> 00:02:21 galaxy's rotation through its magnetic field.

00:02:21 --> 00:02:23 There is gas falling in from outside, and

00:02:23 --> 00:02:26 massive stars blow winds long before they

00:02:26 --> 00:02:29 explode. All of these are real. The

00:02:29 --> 00:02:31 question was never whether supernovae

00:02:31 --> 00:02:34 contribute. It was whether they are enough

00:02:34 --> 00:02:37 on their own to pay the whole bill.

00:02:37 --> 00:02:39 Avery: Uh, and to answer that, you need to do

00:02:39 --> 00:02:41 something nobody had managed. You need to

00:02:41 --> 00:02:44 count the receipts. When massive stars in a

00:02:44 --> 00:02:46 cluster explode, and they do it in batches,

00:02:46 --> 00:02:49 because massive stars are born in groups and

00:02:49 --> 00:02:51 die within a few million years of one

00:02:51 --> 00:02:54 another, the blasts merge. Instead of

00:02:54 --> 00:02:56 a single expanding remnant you get a super

00:02:56 --> 00:02:59 bubble, an enormous cavity blown in the

00:02:59 --> 00:03:01 neutral hydrogen, its edge still pushing

00:03:01 --> 00:03:04 outwards. Superbubbles are the fingerprints

00:03:04 --> 00:03:07 each one carries in its size and its

00:03:07 --> 00:03:10 expansion speed, a record of how much energy

00:03:10 --> 00:03:11 went into it and roughly when.

00:03:12 --> 00:03:15 Anna: So a, uh, complete, dynamically resolved

00:03:15 --> 00:03:17 census of superbubbles across an entire

00:03:17 --> 00:03:20 galaxy would let you add up the energy

00:03:20 --> 00:03:23 supernovae have actually delivered and then

00:03:23 --> 00:03:25 compare it against how fast the turbine

00:03:25 --> 00:03:27 turbulence in that same galaxy is bleeding

00:03:27 --> 00:03:30 energy away. If the two numbers match,

00:03:30 --> 00:03:33 you have your answer. If supernovae falls

00:03:33 --> 00:03:35 short, something else is doing the work.

00:03:36 --> 00:03:38 Avery: Nobody had that senses for a reason. That's

00:03:38 --> 00:03:41 almost funny. We can't do it for the Milky

00:03:41 --> 00:03:43 Way because we live inside it. Mapping

00:03:43 --> 00:03:46 bubbles in our own galaxy is like surveying a

00:03:46 --> 00:03:48 forest from the base of one tree. And for

00:03:48 --> 00:03:51 other galaxies we have the sensitivity or the

00:03:51 --> 00:03:53 resolution, never both.

00:03:53 --> 00:03:56 Anna: Which is where two telescopes on opposite

00:03:56 --> 00:03:59 sides of the world come in. Exactly

00:03:59 --> 00:04:02 that. The paper is in Nature astronomy,

00:04:02 --> 00:04:05 published on 17 September. Led by

00:04:05 --> 00:04:07 Fan Yi Meng of Tsinghua University,

00:04:07 --> 00:04:10 with Zhao Wei Tsai and Jingwen Wu,

00:04:10 --> 00:04:13 and with D Li, Jinghua's head of

00:04:13 --> 00:04:15 astronomy and the former chief scientist of

00:04:15 --> 00:04:18 the FAST telescope as corresponding

00:04:18 --> 00:04:21 authority, they combined two instruments.

00:04:21 --> 00:04:24 FAST is the 500 metre aperture

00:04:24 --> 00:04:26 spherical telescope sitting in a natural

00:04:26 --> 00:04:29 limestone bowl in Guizhou Province in

00:04:29 --> 00:04:32 southern China, the most sensitive single

00:04:32 --> 00:04:34 dish on Earth. At these wavelengths, what it

00:04:34 --> 00:04:37 gives you is faint, diffuse, large

00:04:37 --> 00:04:40 scale structure, the outskirts of bubbles,

00:04:40 --> 00:04:43 the gas nobody else can see. What it

00:04:43 --> 00:04:46 cannot give you is fine detail. For

00:04:46 --> 00:04:48 that they used archival observations from the

00:04:48 --> 00:04:51 Jansky Very Large array in New Mexico,

00:04:52 --> 00:04:54 27 dishes spread across the desert.

00:04:54 --> 00:04:57 Working as one instrument, the array

00:04:57 --> 00:05:00 resolves the sharp edges fast,

00:05:00 --> 00:05:03 fills in everything. The array's spacing

00:05:03 --> 00:05:06 makes it blind to stitch them together, and

00:05:06 --> 00:05:08 you get a map that is both deep and sharp,

00:05:08 --> 00:05:11 which is exactly what this problem has always

00:05:11 --> 00:05:12 needed.

00:05:13 --> 00:05:15 Avery: They pointed that combination at Messier 31,

00:05:16 --> 00:05:18 the Andromeda Galaxy, the nearest big

00:05:18 --> 00:05:21 spiral, 2 1/2 million light years away

00:05:21 --> 00:05:23 and close enough that we can see the whole

00:05:23 --> 00:05:26 disc laid out from the outside. They mapped

00:05:26 --> 00:05:28 it in the 21 centimetre line of neutral

00:05:28 --> 00:05:31 hydrogen, the radio signal that traces

00:05:31 --> 00:05:33 cold atomic gas.

00:05:33 --> 00:05:35 Anna: From that map, they pulled

00:05:35 --> 00:05:38 365 candidate cavities

00:05:38 --> 00:05:40 and after classification, confirmed

00:05:40 --> 00:05:43 118 genuine super bubbles

00:05:43 --> 00:05:45 across the entire disc.

00:05:45 --> 00:05:46 Avery: And the result?

00:05:47 --> 00:05:49 Anna: The first thing worth noticing is the ages.

00:05:50 --> 00:05:52 Measured from their sizes and expansion

00:05:52 --> 00:05:55 speeds, the bubbles run up to 40 million

00:05:55 --> 00:05:58 years old. That is not an arbitrary number.

00:05:58 --> 00:06:01 It is almost exactly how long a star

00:06:01 --> 00:06:03 cluster keeps producing Supernovae from its

00:06:03 --> 00:06:06 first massive star dying to its last.

00:06:07 --> 00:06:09 The ages line up with the clock you would

00:06:09 --> 00:06:12 predict if clusters are uh, what makes them B

00:06:12 --> 00:06:14 Lee put the scale plainly. Those

00:06:14 --> 00:06:17 118 bubbles correspond to

00:06:17 --> 00:06:19 thousands of supernova explosions over the

00:06:19 --> 00:06:22 past 40 million years. Then the actual

00:06:22 --> 00:06:25 test from the bubbles they calculated the

00:06:25 --> 00:06:28 rate at which supernovae are injecting

00:06:28 --> 00:06:30 kinetic energy between 10 to the

00:06:30 --> 00:06:33 49th to 10 to the 51.5

00:06:33 --> 00:06:36 ergs per cubic kiloparsec per

00:06:36 --> 00:06:39 million years. Separately and this is the

00:06:39 --> 00:06:42 part that makes the paper work. They derived

00:06:42 --> 00:06:44 the rate at which turbulence is dissipating

00:06:44 --> 00:06:47 energy from the same data using the

00:06:47 --> 00:06:49 observed motions of the gastwo

00:06:49 --> 00:06:52 independent numbers. They match match

00:06:52 --> 00:06:55 how closely in magnitude. And

00:06:55 --> 00:06:58 this is the stronger claim in spatial

00:06:58 --> 00:06:58 distribution.

00:06:59 --> 00:07:01 It's not just that the galaxy wide totals

00:07:01 --> 00:07:04 happen to agree, which could be coincidence

00:07:04 --> 00:07:06 between two quantities that both scale with

00:07:06 --> 00:07:09 how many stars a ah galaxy has. It's that

00:07:09 --> 00:07:12 where the supernovae energy goes in is

00:07:12 --> 00:07:14 where the turbulent energy comes out

00:07:15 --> 00:07:17 region by region across the disc. The

00:07:17 --> 00:07:20 supply map matches the demand map.

00:07:20 --> 00:07:23 That's much harder to get by accent. The

00:07:23 --> 00:07:25 conclusion the authors draw is carefully

00:07:25 --> 00:07:27 worded and I want to keep their wording.

00:07:27 --> 00:07:30 Clustered supernova feedback is

00:07:30 --> 00:07:32 sufficient to sustain galactic scale

00:07:32 --> 00:07:35 turbulence. Why this matters beyond

00:07:35 --> 00:07:37 bookkeeping is turbulence is not a detail

00:07:37 --> 00:07:40 of galaxies, it's one of the controls.

00:07:40 --> 00:07:43 Turbulent pressure helps hold a ah gas disc

00:07:43 --> 00:07:46 up against its own gravity. And turbulence is

00:07:46 --> 00:07:49 what stops molecular clouds collapsing all at

00:07:49 --> 00:07:51 once. A large part of why galaxies

00:07:51 --> 00:07:54 convert gas into stars. So slowly

00:07:54 --> 00:07:57 change the turbulence and you change the star

00:07:57 --> 00:08:00 formation rate. So this closes a loop.

00:08:00 --> 00:08:03 Gas collapses and forms stars. The biggest

00:08:03 --> 00:08:06 of those stars explode. The explosions

00:08:06 --> 00:08:08 stir the remaining gas. The stirring

00:08:08 --> 00:08:11 regulates how readily the next generation

00:08:11 --> 00:08:13 forms. Galaxies are partly self

00:08:13 --> 00:08:16 governing and this is the first time both

00:08:16 --> 00:08:18 ends of that loop have been measured in the

00:08:18 --> 00:08:21 same galaxy from the same data and found

00:08:21 --> 00:08:22 to balance.

00:08:22 --> 00:08:25 Avery: And um, the caveat now the honest

00:08:25 --> 00:08:27 Anna: limits and there are three first,

00:08:27 --> 00:08:30 sufficient is not the same as sole

00:08:30 --> 00:08:32 showing supernovae can pay the whole bill

00:08:32 --> 00:08:35 does not prove nothing else. Chips in

00:08:35 --> 00:08:37 gravity and the magneto rotational

00:08:37 --> 00:08:40 instability have not been eliminated. They

00:08:40 --> 00:08:43 have been made unnecessary, which is a weaker

00:08:43 --> 00:08:46 and more interesting result. Second, this

00:08:46 --> 00:08:49 is neutral atomic hydrogen. It does not

00:08:49 --> 00:08:51 directly trace the molecular gas where

00:08:51 --> 00:08:54 stars actually form or the hot

00:08:54 --> 00:08:56 ionised gas and the energy budget in those

00:08:56 --> 00:08:59 phases could behave differently. And third,

00:08:59 --> 00:09:02 this is one galaxy, a large,

00:09:02 --> 00:09:05 fairly quiet spiral that has not formed stars

00:09:05 --> 00:09:08 vigorously in a long while. Whether the books

00:09:08 --> 00:09:11 balance the same way in a starburst or in a

00:09:11 --> 00:09:13 small, irregular, uh, galaxy where bubbles

00:09:13 --> 00:09:14 can blow straight out.

00:09:14 --> 00:09:17 The top is exactly the next question.

00:09:17 --> 00:09:20 Two footnotes I enjoyed Bordechai Mark

00:09:20 --> 00:09:23 McClo, the man whose 1999

00:09:23 --> 00:09:26 paper showed this turbulence should have died

00:09:26 --> 00:09:29 long ago, is a co author here. His own

00:09:29 --> 00:09:31 result is referenced too, in the paper that

00:09:31 --> 00:09:34 answers it. And because Nature Astronomy

00:09:34 --> 00:09:37 publishes its referee reports, we know one

00:09:37 --> 00:09:39 of the two reviewers was Christoph Federath

00:09:40 --> 00:09:42 at the Australian National University, who

00:09:42 --> 00:09:45 has spent a career on this exact question.

00:09:45 --> 00:09:48 The Australian fingerprint is on the scrutiny

00:09:48 --> 00:09:51 rather than the data. Regular listeners will

00:09:51 --> 00:09:54 hear an echo here. Two weeks ago we ran

00:09:54 --> 00:09:56 the finding that black hole outflows can

00:09:56 --> 00:09:59 trigger star formation as well as shut it

00:09:59 --> 00:10:02 down. Feedback that builds as well as

00:10:02 --> 00:10:05 breaks. This is the same lesson one

00:10:05 --> 00:10:07 rung down the letter. At stellar scale,

00:10:07 --> 00:10:10 feedback is not simply destructive, it is

00:10:10 --> 00:10:12 a galaxy's thermostat.

00:10:13 --> 00:10:15 Avery: Anna's Storey takes supernovae as given and

00:10:15 --> 00:10:18 asks what they do to a galaxy. This one

00:10:18 --> 00:10:21 asks a question one step which

00:10:21 --> 00:10:24 stars actually managed to explode? You would

00:10:24 --> 00:10:27 think that was settled. It is not. We

00:10:27 --> 00:10:29 see fewer supernovae than our models say we

00:10:29 --> 00:10:32 should. And there's a related puzzle, the red

00:10:32 --> 00:10:35 supergiant problem. When astronomers go back

00:10:35 --> 00:10:38 through archival images to identify the star

00:10:38 --> 00:10:40 that blew up, they never find 1 above about

00:10:40 --> 00:10:43 16 to 18 solar masses. Even

00:10:43 --> 00:10:46 though plenty of stars are heavier, something

00:10:46 --> 00:10:48 is quietly removing the most massive stars

00:10:48 --> 00:10:51 from the exploding population. A new paper in

00:10:51 --> 00:10:54 Physical Review D from Mariam Gogilashvili

00:10:54 --> 00:10:56 and Irene Tambora at the Niels Bohr Institute

00:10:56 --> 00:10:59 in Copenhagen Contorm points at an

00:10:59 --> 00:11:02 unlikely culprit. Neutrinos changing

00:11:02 --> 00:11:04 identity Quick refresher When a

00:11:04 --> 00:11:07 Anna: massive star's core collapses, about

00:11:07 --> 00:11:10 99% of the energy released leaves

00:11:10 --> 00:11:13 as neutrinos. And the explosion depends on

00:11:13 --> 00:11:15 a small fraction of that flood being

00:11:15 --> 00:11:18 reabsorbed by the gas just outside the

00:11:18 --> 00:11:20 core, heating it enough to revive the

00:11:20 --> 00:11:23 stalled shock wave. It's a narrow margin.

00:11:24 --> 00:11:26 Neutrinos also come in three flavours

00:11:26 --> 00:11:29 electron, muon and tau and

00:11:29 --> 00:11:31 oscillate between them, which is Nobel

00:11:31 --> 00:11:33 winning physics from 1998.

00:11:34 --> 00:11:37 Avery: Here's the catch. Only the electron flavour

00:11:37 --> 00:11:39 deposits heat efficiently. Muon and tau

00:11:39 --> 00:11:42 neutrinos mostly sail straight out. So

00:11:42 --> 00:11:45 if flavour conversion happens deep inside a

00:11:45 --> 00:11:47 collapsing core, it takes energy earmarked

00:11:47 --> 00:11:50 for the explosion and redistributes it into

00:11:50 --> 00:11:52 flavours that simply leave. Most state of the

00:11:52 --> 00:11:55 art simulations leave this out on the old

00:11:55 --> 00:11:57 assumption that conversion happens too far

00:11:57 --> 00:11:59 out to matter. Recent work says

00:11:59 --> 00:12:02 otherwise, so Maryam Gogilashvili and

00:12:02 --> 00:12:05 Irene Tambora put it in schematically and

00:12:05 --> 00:12:08 ran the collapse of 195 stars

00:12:08 --> 00:12:11 from 9 to 120 solar masses

00:12:12 --> 00:12:14 without flavour conversion. About 27%

00:12:14 --> 00:12:17 of their stars fail to explode and collapse

00:12:17 --> 00:12:20 straight to black holes. That matches both

00:12:20 --> 00:12:22 the literature and observations. Switch

00:12:22 --> 00:12:25 flavour conversion on and the failure rate

00:12:25 --> 00:12:28 climbs to somewhere between 48 and

00:12:28 --> 00:12:30 88% depending on how deep in the

00:12:30 --> 00:12:33 core you let it happen. And the stars most

00:12:33 --> 00:12:36 affected sit between 16 and 30

00:12:36 --> 00:12:37 solar masses, which is

00:12:37 --> 00:12:40 Anna: precisely the missing mass range. In the red

00:12:40 --> 00:12:41 supergiant problem.

00:12:42 --> 00:12:44 Avery: There is a second quieter result I like more.

00:12:45 --> 00:12:47 And the stars that do still explode. Flavour

00:12:47 --> 00:12:50 conversion revives the shock earlier so less

00:12:50 --> 00:12:52 material rains back onto the newborn neutron

00:12:52 --> 00:12:55 star. The neutron stars come out lighter,

00:12:55 --> 00:12:58 closer to the 1.2 to 1.4 solar

00:12:58 --> 00:13:00 masses we actually measure in pulsars.

00:13:00 --> 00:13:03 A model that was running heavy now matches

00:13:03 --> 00:13:06 the honest handling. Here is the range. 48

00:13:06 --> 00:13:09 to 88% is not a measurement. It is a span

00:13:09 --> 00:13:11 across assumptions. And the authors say

00:13:11 --> 00:13:13 plainly that their upper valleys look to be

00:13:13 --> 00:13:16 in tension with observations. This is one

00:13:16 --> 00:13:18 dimensional modelling with a deliberately

00:13:18 --> 00:13:20 simplified switch for the neutrino physics.

00:13:20 --> 00:13:23 What it establishes is not a number. It is

00:13:23 --> 00:13:25 that this effect is too big to keep leaving

00:13:25 --> 00:13:28 out. The preprint went up in mid

00:13:28 --> 00:13:30 May, so the work has been circulating about

00:13:30 --> 00:13:32 four months. It is the journal version that

00:13:32 --> 00:13:32 is

00:13:32 --> 00:13:34 Anna: new and a southern footnote that is not a

00:13:34 --> 00:13:36 stretch. We have caught neutrinos from

00:13:36 --> 00:13:39 exactly one supernova SN

00:13:39 --> 00:13:42 1987A in the Southern Magellanic

00:13:42 --> 00:13:45 Cloud cloud 20 dozen particles over about 13

00:13:45 --> 00:13:47 seconds in February 1987.

00:13:48 --> 00:13:50 Every word of this debate traces back to that

00:13:50 --> 00:13:53 1 handful of detections from a galaxy only

00:13:53 --> 00:13:56 southern observers see properly. The next

00:13:56 --> 00:13:58 galactic supernova settles a great deal of

00:13:58 --> 00:13:58 it.

00:13:59 --> 00:14:00 Avery: Okay, moving on to storey 3.

00:14:01 --> 00:14:03 Most exoplanet discoveries come with an open

00:14:03 --> 00:14:06 ended invitation. Go and study it whenever

00:14:06 --> 00:14:08 you like. This one comes with a deadline.

00:14:09 --> 00:14:11 Published on 18 September in the publications

00:14:11 --> 00:14:14 of the Astronomical Society of Japan from

00:14:14 --> 00:14:16 Noriharu Watanabe and Norio

00:14:16 --> 00:14:18 Narita at the University of Tokyo with a

00:14:18 --> 00:14:21 large international team. The discovery of

00:14:21 --> 00:14:24 TOI 1355b, a

00:14:24 --> 00:14:27 hot Jupiter and a strange one on three counts

00:14:27 --> 00:14:30 count one is the star. TOI

00:14:30 --> 00:14:33 1355 is an A type star about twice

00:14:33 --> 00:14:36 the Sun's mass with a surface near 8

00:14:36 --> 00:14:39 Kelvin, um, some 3 degrees hotter than

00:14:39 --> 00:14:41 the Sun. It's around 800 light years away

00:14:41 --> 00:14:44 and it spins fast better than 80

00:14:44 --> 00:14:46 kilometres a second against our Sun's

00:14:46 --> 00:14:49 leisurely two count two is the

00:14:49 --> 00:14:52 planet. Nearly six Jupiter masses. About

00:14:52 --> 00:14:55 1.4 Jupiter radii whipping around

00:14:55 --> 00:14:57 that star every 2.17 days.

00:14:57 --> 00:15:00 But its orbit is not a circle. The

00:15:00 --> 00:15:03 eccentricity is about 0.22 a

00:15:03 --> 00:15:04 properly lopsided orbit.

00:15:04 --> 00:15:07 Anna: Why is that surprising for a hot Jupiter?

00:15:07 --> 00:15:09 Avery: Because they're almost never lopsided sitting

00:15:09 --> 00:15:12 that close in tides should round off an orbit

00:15:12 --> 00:15:15 quickly. Of the roughly 20 hot Jupiters known

00:15:15 --> 00:15:17 around hot stars, the measured eccentricities

00:15:17 --> 00:15:20 are essentially zero, some to four decimal

00:15:20 --> 00:15:22 places. And there's exactly one other

00:15:22 --> 00:15:24 eccentric case on record. These worlds are

00:15:24 --> 00:15:27 thought to be flung inward on wild elliptical

00:15:27 --> 00:15:29 orbits by gravitational bullying from other

00:15:29 --> 00:15:32 planets. Then have those orbits ground down

00:15:32 --> 00:15:34 to circles by tides. TOI

00:15:34 --> 00:15:37 1355B is partway through the grinding,

00:15:37 --> 00:15:40 which we rarely gets. Watch count three

00:15:40 --> 00:15:42 is the deadline. Comparing transits across

00:15:42 --> 00:15:45 TESS observations from 2019, 2020,

00:15:46 --> 00:15:48 2022 and 2024. The team

00:15:48 --> 00:15:50 found the planet crossing the star at a

00:15:50 --> 00:15:53 steadily different height each time. The

00:15:53 --> 00:15:55 orbit's plane is swinging nodal precession

00:15:55 --> 00:15:58 driven by the bulge of that rapidly spinning

00:15:58 --> 00:16:01 star. Wind it forward and the planet stops

00:16:01 --> 00:16:03 crossing the star's face from our point of

00:16:03 --> 00:16:05 view around the middle of 2033.

00:16:05 --> 00:16:08 Anna: After that, no transits for centuries. The

00:16:08 --> 00:16:09 planet is fine.

00:16:09 --> 00:16:12 Our line of sight is what runs out. There is

00:16:12 --> 00:16:15 a lovely methodological wrinkle too.

00:16:15 --> 00:16:17 You normally weigh a planet by watching the

00:16:17 --> 00:16:20 star wobble. But this star spins

00:16:20 --> 00:16:23 so fast its spectral lines are smeared

00:16:23 --> 00:16:26 and that does not work. So they weighed it

00:16:26 --> 00:16:28 from the light curve instead from M. The way

00:16:28 --> 00:16:31 the planet's gravity distorts the star into

00:16:31 --> 00:16:33 a faint rugby ball shape. And from the

00:16:33 --> 00:16:36 subtle brightening as the star is tugged

00:16:36 --> 00:16:39 towards us. The mass came out of the shape of

00:16:39 --> 00:16:41 the light, not the shift of the lines. And

00:16:41 --> 00:16:43 the supporting cast is worth naming.

00:16:44 --> 00:16:47 Alongside TESS and the 3.8 metre

00:16:47 --> 00:16:49 SEMI telescope in Okayama, this

00:16:49 --> 00:16:52 paper leans on a 91 centimetre

00:16:52 --> 00:16:55 telescope on the slopes of Matt Etna,

00:16:55 --> 00:16:58 a 40 centimetre in Switzerland and a

00:16:58 --> 00:17:00 28 centimetre at a private observatory in

00:17:00 --> 00:17:03 Germany. Backyard scale instruments on the

00:17:03 --> 00:17:06 Discovery paper for a six Jupiter mass

00:17:06 --> 00:17:09 world. The preprint went up in August, so

00:17:09 --> 00:17:12 about a month ahead of the journal. And for

00:17:12 --> 00:17:14 our southern listeners the star sits at Ah,

00:17:14 --> 00:17:17 Declination 67, which means

00:17:17 --> 00:17:20 it never rises from Sydney. Northern

00:17:20 --> 00:17:22 listeners can find the field in Cepheus. The

00:17:22 --> 00:17:25 team is already preparing a follow up on how

00:17:25 --> 00:17:27 tilted the orbit is and wants

00:17:27 --> 00:17:30 JWST time to low

00:17:30 --> 00:17:31 ETH

00:17:31 --> 00:17:32 Avery: orbit now and the business end of

00:17:32 --> 00:17:33 spaceflight.

00:17:33 --> 00:17:36 On 18 September, NASA exercised a UH

00:17:36 --> 00:17:39 contract modification with SpaceX for three

00:17:39 --> 00:17:41 additional crew rotation missions to the

00:17:41 --> 00:17:44 International Space Crew 1 5, Crew

00:17:44 --> 00:17:47 16 and Crew 1 7. The value

00:17:47 --> 00:17:50 is $946 million for all

00:17:50 --> 00:17:52 three covering ground launch in

00:17:52 --> 00:17:54 orbit and return and recovery operations,

00:17:55 --> 00:17:58 cargo on each mission and lifeboat capability

00:17:58 --> 00:18:00 while docked. That takes SpaceX to

00:18:00 --> 00:18:03 17 crew missions under the commercial crew

00:18:03 --> 00:18:06 transportation contract and that contract's

00:18:06 --> 00:18:08 running total to $5.92

00:18:08 --> 00:18:11 billion. Period of performance runs through

00:18:11 --> 00:18:13 2030 with mission readiness dates in

00:18:13 --> 00:18:16 2027 and 2028. NASA

00:18:16 --> 00:18:18 flagged its intent to buy back in May and

00:18:18 --> 00:18:21 calls this a sole source modification that

00:18:21 --> 00:18:23 does not pre further purchases later.

00:18:24 --> 00:18:26 Anna: One line in that release is worth reading

00:18:26 --> 00:18:29 carefully. NASA says the change helps

00:18:29 --> 00:18:32 it maintain access to the station with quote,

00:18:32 --> 00:18:34 two unique commercial crew industry

00:18:34 --> 00:18:37 partners. The award itself goes to one

00:18:37 --> 00:18:40 of them. The original 2014

00:18:40 --> 00:18:42 contracts went to both Boeing and SpaceX

00:18:43 --> 00:18:46 and Boeing appears in this release exactly

00:18:46 --> 00:18:48 once in that history. NASA does

00:18:48 --> 00:18:51 not say anything here about when its second

00:18:51 --> 00:18:53 provider next flies people.

00:18:53 --> 00:18:55 We'll report that when they do say.

00:18:55 --> 00:18:57 Avery: Meanwhile, the near term mission is moving.

00:18:58 --> 00:19:00 The four astronauts of Crew 13 entered

00:19:00 --> 00:19:02 quarantine late on Thursday at UH Johnson

00:19:02 --> 00:19:05 Space Centre in Houston. NASA's Jessica

00:19:05 --> 00:19:08 Watkins and Luke Delaney, the Canadian Space

00:19:08 --> 00:19:10 Agency's Yoshua Kutryk and

00:19:10 --> 00:19:12 Roscosmos cosmonaut Sergey

00:19:12 --> 00:19:15 tatariotnikov. NASA and SpaceX

00:19:15 --> 00:19:18 are still targeting early October. Before

00:19:18 --> 00:19:20 quarantine. They finished training at SpaceX

00:19:20 --> 00:19:22 in Hawthorne and ran a crew equipment

00:19:22 --> 00:19:25 interface test at Cape Canaveral. Suits on

00:19:25 --> 00:19:28 into the Dragon leak cheques, seat fit

00:19:28 --> 00:19:31 comms cheques, my favourite detail. They sit

00:19:31 --> 00:19:33 in the capsule and listen to its fans and

00:19:33 --> 00:19:35 pumps so that none of the sounds are

00:19:35 --> 00:19:37 unfamiliar on launch day.

00:19:37 --> 00:19:40 Anna: The quarantine itself is an Apollo era

00:19:40 --> 00:19:43 invention still doing its job. Keeping a head

00:19:43 --> 00:19:45 cold on the ground where it belongs. That

00:19:45 --> 00:19:47 closes out an arc we tracked since the

00:19:47 --> 00:19:50 oxidizer leak stood. Crew 13 down

00:19:50 --> 00:19:53 valve replaced. Crew in quarantine early

00:19:53 --> 00:19:55 October. We still want a date.

00:19:55 --> 00:19:57 Quick hit, closing a thread. We opened on

00:19:57 --> 00:20:00 Friday. It happened on the 18th of

00:20:00 --> 00:20:02 September. The earth facing sun went

00:20:02 --> 00:20:05 completely spotless. No numbered active

00:20:05 --> 00:20:08 regions at all. It's the first spotless day

00:20:08 --> 00:20:11 since the 24th of February and the

00:20:11 --> 00:20:13 19th was spotless too, making it two in a

00:20:13 --> 00:20:16 row. By the 20th, a small new region

00:20:16 --> 00:20:19 had rotated up and the run ended. Which is

00:20:19 --> 00:20:21 exactly how the descent from a solar maximum

00:20:21 --> 00:20:24 goes. Not a switch, but a flicker that

00:20:24 --> 00:20:27 Avery: lengthens for scale on how far we have come

00:20:27 --> 00:20:27 down.

00:20:27 --> 00:20:30 The busiest single day of the Solar cycle

00:20:30 --> 00:20:33 was 8 August 2024, with

00:20:33 --> 00:20:35 an estimated 337

00:20:35 --> 00:20:38 sunspots. That was the highest daily count

00:20:38 --> 00:20:41 since March 2001. Cycle

00:20:41 --> 00:20:44 25 peaked in late 2024

00:20:44 --> 00:20:46 and minimum is not expected before about

00:20:46 --> 00:20:47 2030.

00:20:47 --> 00:20:50 Anna: But do not put the aurora gear away. A

00:20:50 --> 00:20:53 coronal hole is rotating into position and

00:20:53 --> 00:20:55 its fast solar wind stream should reach us

00:20:55 --> 00:20:58 around the 23rd, with forecasters flagging a

00:20:58 --> 00:21:01 chance of minor geomagnetic storming. If

00:21:01 --> 00:21:03 it lands, best chances are the far north,

00:21:03 --> 00:21:06 northern Scotland and the far south, southern

00:21:06 --> 00:21:09 New Zealand. It arrives right on the equinox,

00:21:09 --> 00:21:11 which is the most aurora friendly moment of

00:21:11 --> 00:21:14 the year. For reasons of geometry and the

00:21:14 --> 00:21:16 standing point we keep making. A, uh, quiet

00:21:16 --> 00:21:19 sun means fewer auroras, but it also means

00:21:19 --> 00:21:22 a weaker shield against galactic cosmic rays.

00:21:22 --> 00:21:25 So that background quietly rises same

00:21:25 --> 00:21:27 dial opposite end to the sky.

00:21:27 --> 00:21:30 Avery: And this week the calendar does something

00:21:30 --> 00:21:32 that only makes sense if you remember. The

00:21:32 --> 00:21:35 Earth is tilted first to equinox,

00:21:35 --> 00:21:37 five minutes past midnight universal time on

00:21:37 --> 00:21:40 the 23rd. An equinox is an instant,

00:21:40 --> 00:21:43 not a day. So where you stand decides the

00:21:43 --> 00:21:45 date. That is Tuesday evening in the

00:21:45 --> 00:21:48 Americas, just after five in Los Angeles,

00:21:48 --> 00:21:50 just after eight in New York, one in the

00:21:50 --> 00:21:53 morning in London and five past ten on

00:21:53 --> 00:21:56 Wednesday morning in Sydney. Spring here,

00:21:56 --> 00:21:58 autumn there, same instant.

00:21:58 --> 00:22:01 Anna: Then on Saturday the 26th, the full

00:22:01 --> 00:22:04 moon, the harvest moon. The full moon falling

00:22:04 --> 00:22:07 closest to the September equinox. And here's

00:22:07 --> 00:22:09 where it gets interesting. Because the

00:22:09 --> 00:22:11 harvest moon's entire reputation is a

00:22:11 --> 00:22:13 northern hemisphere phenomenon.

00:22:13 --> 00:22:15 Avery: Explain that, because I think most people

00:22:15 --> 00:22:16 assume it's just a name.

00:22:17 --> 00:22:19 Anna: It's not just a name. The moon Normally

00:22:19 --> 00:22:22 rises about 50 minutes later each night.

00:22:22 --> 00:22:24 Around the northern autumn equinox. The

00:22:24 --> 00:22:26 Moon's path meets the eastern horizon at a

00:22:26 --> 00:22:29 shallow angle. So successive moon rises,

00:22:29 --> 00:22:32 bunch up and you get several evenings running

00:22:32 --> 00:22:34 with bright moonlight arriving just after

00:22:34 --> 00:22:37 sunset, which was the whole point. Extra

00:22:37 --> 00:22:38 light to finish the harvest.

00:22:39 --> 00:22:41 Avery: We ran the numbers for this week. On the

00:22:41 --> 00:22:44 nights around full moon, moonrise comes later

00:22:44 --> 00:22:46 by about 12 minutes a night. In London,

00:22:46 --> 00:22:49 22 minutes in New York, 27 in Los

00:22:49 --> 00:22:51 Angeles and in Sydney,

00:22:51 --> 00:22:53 62 minutes.

00:22:53 --> 00:22:56 Anna: So we get the opposite of a harvest moon.

00:22:56 --> 00:22:59 Avery: We get the anti harvest moon. The effect the

00:22:59 --> 00:23:01 thing is named for is more than five times

00:23:01 --> 00:23:04 weaker here than in London. Same moon,

00:23:04 --> 00:23:07 same week, geometry simply reversed. In

00:23:07 --> 00:23:10 spring it's the same ecliptic angle that

00:23:10 --> 00:23:13 gives us a brilliant high Venus and one

00:23:13 --> 00:23:14 hugging the horizon.

00:23:14 --> 00:23:17 One wrinkle for Australian listeners The full

00:23:17 --> 00:23:20 moon Instant lands at 2:48 on Sunday

00:23:20 --> 00:23:22 morning our time, so our calendars say

00:23:22 --> 00:23:25 27th and northern ones say

00:23:25 --> 00:23:27 26th. It looks full on both nights.

00:23:27 --> 00:23:28 Anna: And the planets?

00:23:28 --> 00:23:30 Avery: Venus is still the show in the west after

00:23:30 --> 00:23:33 sunset. At uh magnitude -4.5

00:23:34 --> 00:23:37 from Sydney it stands 37 degrees high as

00:23:37 --> 00:23:40 the sun sets and hangs on for more than three

00:23:40 --> 00:23:42 hours. From New York, 13 degrees

00:23:42 --> 00:23:45 from London, 2 1/2 degrees about

00:23:45 --> 00:23:48 25 minutes with a dead flat western horizon

00:23:48 --> 00:23:51 in the north. Look early and low through a

00:23:51 --> 00:23:54 telescope. It's a big thin crescent, a

00:23:54 --> 00:23:57 quarter lit but 42 arcseconds across.

00:23:57 --> 00:24:00 Larger than Jupiter's disc. Below it

00:24:00 --> 00:24:03 Mercury is having a genuinely good Southern

00:24:03 --> 00:24:05 apparition. Magnitude

00:24:05 --> 00:24:08 0.2, 18 degrees up from Sydney

00:24:08 --> 00:24:11 at sunset and setting an hour and a half

00:24:11 --> 00:24:14 after the Sun. From London it's 3 degrees

00:24:14 --> 00:24:16 up and effectively out of reach for the

00:24:16 --> 00:24:17 north.

00:24:17 --> 00:24:19 Anna: The compensation is the morning at the start

00:24:19 --> 00:24:22 of nautical Twilight. Mars stands 49

00:24:22 --> 00:24:25 degrees high from Los Angeles, 47 from

00:24:25 --> 00:24:28 New York, 42 from London and just

00:24:28 --> 00:24:30 21 from Sydney. Jupiter is

00:24:30 --> 00:24:33 28 degrees up from Los Angeles against 10

00:24:33 --> 00:24:34 from here.

00:24:34 --> 00:24:37 The pre dawn sky belongs to the north right

00:24:37 --> 00:24:39 now and it is worth getting up for.

00:24:39 --> 00:24:42 Saturn rises mid evening and is highest

00:24:42 --> 00:24:45 just after midnight, better than 50 degrees

00:24:45 --> 00:24:47 up from Sydney at magnitude plus

00:24:47 --> 00:24:50 0.3. It is heading for opposition

00:24:50 --> 00:24:53 in early October and you will see listings

00:24:53 --> 00:24:55 disagree about the date. Some um, say the

00:24:55 --> 00:24:57 fourth, some the fifth. Both are right.

00:24:58 --> 00:25:00 Opposition measured by ecliptic longitude

00:25:00 --> 00:25:03 falls on the 4th, measured by right ascension

00:25:03 --> 00:25:06 the 5th. Saturn's brightness and size are

00:25:06 --> 00:25:08 identical across that whole week so you

00:25:08 --> 00:25:11 cannot pick the wrong night and our lead

00:25:11 --> 00:25:13 storey. Can anyone actually see

00:25:13 --> 00:25:14 Andromeda?

00:25:15 --> 00:25:17 Avery: Depends entirely where you are. From New

00:25:17 --> 00:25:19 York, Andromeda passes almost overhead,

00:25:20 --> 00:25:23 89 degrees up around half past one in the

00:25:23 --> 00:25:25 morning from Los Angeles, 83 from

00:25:25 --> 00:25:28 London, 80 from Sydney. It scrapes to

00:25:28 --> 00:25:31 under 15 degrees low in the north through the

00:25:31 --> 00:25:34 thickest part of our atmosphere. Binocular is

00:25:34 --> 00:25:36 in a clear northern horizon after midnight

00:25:36 --> 00:25:39 we'll find it but it is a smudge rather than

00:25:39 --> 00:25:41 the showpiece. It is up north which is the

00:25:41 --> 00:25:44 storey of tonight really. The north gets the

00:25:44 --> 00:25:46 deep sky, the predawn planets and the lunar

00:25:46 --> 00:25:49 occultation of Jupiter on 6 October

00:25:49 --> 00:25:51 that sits below our horizon entirely.

00:25:52 --> 00:25:55 We get Venus, Mercury and the better half of

00:25:55 --> 00:25:56 the geometry.

00:25:56 --> 00:25:57 Some weeks it runs the other way

00:25:58 --> 00:26:00 Anna: and the standing reminder because we are

00:26:00 --> 00:26:03 talking about a sun with almost nothing on it

00:26:03 --> 00:26:05 and people will be tempted to look. Never

00:26:05 --> 00:26:07 look at the sun without proper protection.

00:26:08 --> 00:26:10 Solar viewers and eclipse glasses must meet

00:26:10 --> 00:26:11 the ISO

00:26:12 --> 00:26:14


00:26:14 --> 00:26:17 international safety standard, and that is

00:26:17 --> 00:26:20 not the same as ordinary sunglasses, no

00:26:20 --> 00:26:22 matter how dark they are. And stacking

00:26:22 --> 00:26:24 sunglasses does not help.

00:26:24 --> 00:26:26 Cheque your filters for damage before use,

00:26:26 --> 00:26:29 and discard any that are scratched, punctured

00:26:29 --> 00:26:32 or peeling. If you're using a telescope or

00:26:32 --> 00:26:34 binoculars, the filter goes on the front of

00:26:34 --> 00:26:37 the instrument, never on the eyepiece, where

00:26:37 --> 00:26:39 focused sunlight can crack it without

00:26:39 --> 00:26:42 warning. There is no safe way to improvise

00:26:42 --> 00:26:42 this.

00:26:43 --> 00:26:45 Avery: That's astronomy daily for today.

00:26:45 --> 00:26:48 118 Bubbles in Andromeda that bounce a

00:26:48 --> 00:26:51 galaxy's energy books neutrinos that may

00:26:51 --> 00:26:53 quietly decide which stars are allowed to

00:26:53 --> 00:26:56 explode a planet. We have until

00:26:56 --> 00:26:58 2033 to study three more

00:26:58 --> 00:27:00 dragonflights on the books and a crew in

00:27:00 --> 00:27:03 quarantine and a sun with nothing on its face

00:27:03 --> 00:27:05 for the first time since February.

00:27:05 --> 00:27:08 Anna: A note for tomorrow this was episode

00:27:08 --> 00:27:10 199, which makes the next one

00:27:10 --> 00:27:13 200, and we would like to mark it

00:27:13 --> 00:27:15 properly. If there's a storey from this

00:27:15 --> 00:27:17 series you want revisited or a question

00:27:17 --> 00:27:20 you've been sitting on the contact form at

00:27:20 --> 00:27:22 astronomydaily IO is the place.

00:27:23 --> 00:27:25 We do read them, and listener questions have

00:27:25 --> 00:27:27 set our running order more than once.

00:27:27 --> 00:27:29 Avery: All our sources are linked in the show notes,

00:27:29 --> 00:27:32 as always, along with the full references for

00:27:32 --> 00:27:33 today's papers.

00:27:33 --> 00:27:36 You'll find us at astronomydaily IO until

00:27:36 --> 00:27:36 tomorrow.

00:27:36 --> 00:27:37 Anna: Clear skies.

00:27:49 --> 00:27:50 The storeys.

00:27:57 --> 00:27:58 Avery: Were told.