Hide and Seek - The Faintest Planet Ever Imaged, Pluto’s Landslides & Starlink’s 355,000 Dodges
Space News TodayJuly 16, 202600:19:2317.76 MB

Hide and Seek - The Faintest Planet Ever Imaged, Pluto’s Landslides & Starlink’s 355,000 Dodges

Anna and Avery kick off with a decade-long game of cosmic hide-and-seek that has finally ended: Beta Pictoris d, the faintest exoplanet ever directly imaged from Earth, found lurking in more than ten years of archival images — and orbiting a star in the southern constellation Pictor. Then it's the completion of VLASS, the sharpest radio map of the whole sky ever made, arriving just as the Rubin Observatory's optical survey switches on. The James Webb Space Telescope has caught a supermassive black hole feeding itself in the Centaurus Cluster — the missing link in a decades-old mystery. A Pluto system double bill follows: the first landslides ever identified on Pluto, and evidence written in Charon's mountains that the big moon once spun more than ten times faster than it does today — both delivered by New Horizons data from 2015. Finally, SpaceX's latest FCC filing reveals Starlink satellites made over 355,000 collision-avoidance manoeuvres in the past year — nearly one dodge per satellite per week — and experts are warning about where the trend leads. Plus dark-sky Southern Hemisphere stargazing and a Starship Flight 13 launch reminder. Chapters • 00:00 — Intro & billboard • 01:30 — Beta Pictoris d: the faintest exoplanet ever imaged from Earth • 05:30 — VLASS complete: the sharpest radio map of the sky • 08:45 — JWST reveals how supermassive black holes feed • 12:15 — Pluto has landslides (Pluto double, part 1) • 15:00 — Charon's slowing spin (Pluto double, part 2) • 17:45 — Starlink's 355,000 collision dodges in a year • 20:45 — Southern Hemisphere skywatch + Starship Flight 13 reminder • 22:30 — Outro Story sources • Beta Pictoris d: ESO release eso2609 (eso.org) · The Astrophysical Journal Letters · space.com · phys.org • VLASS completion: NRAO release (public.nrao.edu/news/vlass-observations-complete) · phys.org • JWST / NGC 4696: Université de Montréal · The Astrophysical Journal Letters · phys.org / EurekAlert • Pluto landslides: Icarus (Discenza et al. 2026) · phys.org · Discover Magazine · Science News • Charon despinning: Nature Communications (Chen et al. 2026, DOI 10.1038/s41467-026-75069-7) · phys.org · Gizmodo • Starlink manoeuvres: SpaceX semiannual FCC constellation status report, via space.com Boilerplate Astronomy Daily is part of the Bitesz.com Podcast Network. Show notes, links and the full back catalogue at astronomydaily.io. Follow @AstroDailyPod on X, Instagram, TikTok and Tumblr. New episodes every day.


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Kind: captions Language: en
00:00:00 --> 00:00:02 Welcome to Astronomy Daily, your daily

00:00:02 --> 00:00:05 dose of space and astronomy news. I'm

00:00:05 --> 00:00:06 Anna.

00:00:06 --> 00:00:09 >> And I'm Avery. It's Thursday, the 16th

00:00:09 --> 00:00:12 of July, 2026, and we have a genuinely

00:00:12 --> 00:00:15 lovely lineup for you today, including a

00:00:15 --> 00:00:17 story that's been 10 years in the

00:00:17 --> 00:00:19 making. Or more accurately, 10 years in

00:00:19 --> 00:00:20 the hiding.

00:00:20 --> 00:00:23 >> That's our lead. Astronomers have

00:00:23 --> 00:00:24 finally caught a planet that's been

00:00:24 --> 00:00:26 playing hideand seek with them for over

00:00:26 --> 00:00:29 a decade. And it turns out to be the

00:00:29 --> 00:00:31 faintest exoplanet ever imaged from

00:00:31 --> 00:00:33 Earth. And it lives in a southern

00:00:34 --> 00:00:36 constellation, which makes it feel just

00:00:36 --> 00:00:37 a little bit like ours.

00:00:37 --> 00:00:39 >> We've also got the completion of a

00:00:39 --> 00:00:42 9-year project to build the sharpest

00:00:42 --> 00:00:44 radio map of the entire sky and the

00:00:44 --> 00:00:47 James Web Space Telescope catching a

00:00:47 --> 00:00:49 super massive black hole in the act of

00:00:49 --> 00:00:52 feeding itself. Ben, it's a double bill

00:00:52 --> 00:00:54 from the outer solar system. Landslides

00:00:54 --> 00:00:57 on Pluto spotted for the first time and

00:00:57 --> 00:01:00 evidence that Pluto's big moon Cheron

00:01:00 --> 00:01:03 once spun more than 10 times faster than

00:01:03 --> 00:01:04 it does today.

00:01:04 --> 00:01:06 >> And we'll wrap the news with some

00:01:06 --> 00:01:09 sobering numbers. SpaceX's Starlink

00:01:09 --> 00:01:10 satellites had to dodge potential

00:01:10 --> 00:01:14 collisions more than 355

00:01:14 --> 00:01:16 times in the past year. We'll unpack

00:01:16 --> 00:01:19 what that means for everyone's orbit.

00:01:19 --> 00:01:21 plus your southern hemisphere sky

00:01:21 --> 00:01:23 watching for tonight. Let's get into it.

00:01:23 --> 00:01:27 Avery, cast your mind back. In 2008,

00:01:27 --> 00:01:29 astronomers directly imaged a planet

00:01:29 --> 00:01:32 around the young star Beta Ptorus, one

00:01:32 --> 00:01:34 of the very first exoplanets ever

00:01:34 --> 00:01:37 photographed. That was Beta Pictorius B.

00:01:38 --> 00:01:40 A second planet C followed and ever

00:01:40 --> 00:01:43 since there's been a nagging suspicion

00:01:43 --> 00:01:45 that the system was hiding something

00:01:45 --> 00:01:45 more

00:01:45 --> 00:01:48 >> because of the disc, right? Beta Pctorus

00:01:48 --> 00:01:50 has this magnificent debris disc. It's

00:01:50 --> 00:01:52 the poster child for planet formation.

00:01:52 --> 00:01:54 And parts of it were warped and sculpted

00:01:54 --> 00:01:57 in ways that two known planets couldn't

00:01:57 --> 00:01:58 fully explain.

00:01:58 --> 00:02:01 >> Exactly. And now we know why. In a study

00:02:01 --> 00:02:03 published Wednesday in the Astrophysical

00:02:03 --> 00:02:05 Journal Letters, a team using the

00:02:05 --> 00:02:08 European Southern Observatory's Very

00:02:08 --> 00:02:11 Large Telescope in Chile has confirmed a

00:02:11 --> 00:02:14 third planet, Beta Pictorius D. And

00:02:14 --> 00:02:16 here's the headline stat. It's roughly

00:02:16 --> 00:02:20 100 times fainter than Beta Pictorius B,

00:02:20 --> 00:02:22 which makes it the faintest exoplanet

00:02:22 --> 00:02:25 ever directly imaged from Earth. 100

00:02:25 --> 00:02:28 times fainter. To put that in context

00:02:28 --> 00:02:30 for everyone, direct imaging means

00:02:30 --> 00:02:32 actually capturing the planet's own

00:02:32 --> 00:02:34 light in a photograph next to a star

00:02:34 --> 00:02:36 that's overwhelmingly brighter. It's

00:02:36 --> 00:02:39 often compared to spotting a firefly

00:02:39 --> 00:02:42 next to a lighthouse. This is spotting a

00:02:42 --> 00:02:45 very dim firefly. And the discovery

00:02:45 --> 00:02:48 itself was serendipitous. Ben Sutliff at

00:02:48 --> 00:02:51 the University of Edinburgh, who co-led

00:02:51 --> 00:02:53 the study, said they were originally

00:02:53 --> 00:02:55 just going back to study the known

00:02:55 --> 00:02:57 planet Beta Pictorius B to see how it

00:02:57 --> 00:03:00 changed over time. But in their new

00:03:00 --> 00:03:03 images from the VLT's AIS instrument,

00:03:03 --> 00:03:05 there was something else, a faint point

00:03:05 --> 00:03:07 of light separated from planet B that

00:03:07 --> 00:03:10 sent them down an entirely new path.

00:03:10 --> 00:03:12 >> And this is where the hideand seek comes

00:03:12 --> 00:03:14 in. Once they knew what to look for,

00:03:14 --> 00:03:17 they trled back through the archives and

00:03:17 --> 00:03:19 there it was, lurking in more than a

00:03:19 --> 00:03:21 decade of old observations from the VT

00:03:22 --> 00:03:23 sphere instrument. And even in James

00:03:24 --> 00:03:26 Webb's space telescope data, the planet

00:03:26 --> 00:03:29 had been photographed for years. Nobody

00:03:29 --> 00:03:30 had noticed.

00:03:30 --> 00:03:33 >> Co-author Jane Burkeby at Oxford put it

00:03:33 --> 00:03:35 beautifully. Planet D has been playing

00:03:35 --> 00:03:38 hideand seek with us for over a decade.

00:03:38 --> 00:03:41 And now we can say, "Found you." So,

00:03:41 --> 00:03:43 what do we know about the world itself?

00:03:43 --> 00:03:46 >> It's a gas giant about 2.4 times the

00:03:46 --> 00:03:49 mass of Jupiter, which sounds big, but

00:03:49 --> 00:03:50 is actually the lightweight of the

00:03:50 --> 00:03:53 family. Planets B and C are each 10

00:03:53 --> 00:03:56 Jupiter masses. Planet D sits much

00:03:56 --> 00:03:58 further out from the star on a wide

00:03:58 --> 00:04:00 orbit, so it's cooler and dimmer than

00:04:00 --> 00:04:03 its siblings, hence the difficulty. And

00:04:03 --> 00:04:05 satisfyingly, its presence helps explain

00:04:06 --> 00:04:08 that odd structure in the debris disc

00:04:08 --> 00:04:10 that's puzzled astronomers for years.

00:04:10 --> 00:04:13 >> There's also a nice milestone tucked in

00:04:13 --> 00:04:15 here. This makes Beta Ptorus only the

00:04:15 --> 00:04:19 second planetary system after HR8799

00:04:19 --> 00:04:21 where more than two planets have been

00:04:21 --> 00:04:24 directly imaged. We're building up

00:04:24 --> 00:04:26 actual family portraits of other solar

00:04:26 --> 00:04:27 systems. now

00:04:27 --> 00:04:29 >> and an independent team at the

00:04:29 --> 00:04:31 University of California spotted the

00:04:31 --> 00:04:33 same object in her own data at almost

00:04:33 --> 00:04:35 the same time which gives the detection

00:04:35 --> 00:04:38 real confidence. Now the bit our

00:04:38 --> 00:04:40 audience will love Beta Ptorus is a

00:04:40 --> 00:04:42 southern star. It sits in the

00:04:42 --> 00:04:45 constellation Pictor the painters easel

00:04:45 --> 00:04:48 just next to Brilliant Canopus and at 63

00:04:48 --> 00:04:50 lighty years away it's visible from

00:04:50 --> 00:04:52 Australia and New Zealand. Though right

00:04:52 --> 00:04:55 now in July, it's low in our evening sky

00:04:56 --> 00:04:57 and best hunted in the pre-dawn hours

00:04:58 --> 00:04:59 later in the year.

00:04:59 --> 00:05:01 >> A planetary system with three

00:05:01 --> 00:05:03 photographed worlds sitting in our

00:05:03 --> 00:05:06 southern sky. Not bad at all. Next, a n

00:05:06 --> 00:05:09 a project 9 years in the making has just

00:05:09 --> 00:05:12 crossed the finish line. The US National

00:05:12 --> 00:05:14 Science Foundation's National Radio

00:05:14 --> 00:05:17 Astronomy Observatory has announced that

00:05:17 --> 00:05:20 observations for the Very Large Array

00:05:20 --> 00:05:24 Sky Survey, VLAS, are complete. It's the

00:05:24 --> 00:05:27 most detailed radio survey of the sky

00:05:27 --> 00:05:28 ever conducted.

00:05:28 --> 00:05:31 >> This is the VA in New Mexico, the iconic

00:05:31 --> 00:05:34 Y-shaped array of 27 dishes from every

00:05:34 --> 00:05:37 space documentary ever made.

00:05:37 --> 00:05:40 >> That's the one. From September 2017

00:05:40 --> 00:05:42 through February this year, the array

00:05:42 --> 00:05:45 repeatedly swept about 34 square

00:05:46 --> 00:05:48 degrees. Essentially, the whole sky

00:05:48 --> 00:05:50 visible from New Mexico. Everything

00:05:50 --> 00:05:54 north of -40° declination. That's

00:05:54 --> 00:05:57 roughly 80% of the entire celestial

00:05:57 --> 00:06:00 sphere mapped at a resolution of about 2

00:06:00 --> 00:06:04 1/2 arcseconds in the 2 to 4 GHz band.

00:06:04 --> 00:06:05 >> And how does that compare to what came

00:06:05 --> 00:06:09 before? It's about 18 times sharper than

00:06:09 --> 00:06:11 the previous benchmark all sky radio

00:06:11 --> 00:06:14 survey from the 1990s. The numbers are

00:06:14 --> 00:06:18 staggering, roughly 6 1/2 observing

00:06:18 --> 00:06:21 hours, half a pabyte of raw data, and

00:06:21 --> 00:06:23 the processed data products are expected

00:06:23 --> 00:06:26 to reach around 2 pabytes, the largest

00:06:26 --> 00:06:29 data volume the VA has ever produced.

00:06:29 --> 00:06:32 They use a clever on the-fly mosaicing

00:06:32 --> 00:06:34 technique where the antennas sweep

00:06:34 --> 00:06:36 continuously across the sky in a raster

00:06:36 --> 00:06:39 pattern rather than stopping to point at

00:06:39 --> 00:06:40 each field.

00:06:40 --> 00:06:42 >> And crucially, they surveyed the sky

00:06:42 --> 00:06:44 multiple times over those nine years,

00:06:44 --> 00:06:47 which means Vlass isn't just a map, it's

00:06:47 --> 00:06:49 a movie. Comparing epochs revealed a

00:06:49 --> 00:06:52 dynamic radio sky sources that flare,

00:06:52 --> 00:06:55 fade, or appear from nowhere. exploding

00:06:55 --> 00:06:58 stars, feeding black holes, colliding

00:06:58 --> 00:06:59 neutron stars.

00:06:59 --> 00:07:01 >> Which brings us to the timing. And

00:07:01 --> 00:07:03 honestly, the timing is the best part of

00:07:03 --> 00:07:06 the story. Just over 2 weeks ago, on

00:07:06 --> 00:07:09 June 30th, the Vera C. Rubin Observatory

00:07:09 --> 00:07:12 in Chile began its decadel long legacy

00:07:12 --> 00:07:14 survey of space and time, sweeping the

00:07:14 --> 00:07:17 southern optical sky every few nights.

00:07:17 --> 00:07:19 So for the first time in history, we

00:07:20 --> 00:07:22 have a complete highresolution radio map

00:07:22 --> 00:07:25 and a real-time optical transient stream

00:07:25 --> 00:07:27 operating simultaneously.

00:07:27 --> 00:07:29 >> Though when Reuben flags something going

00:07:29 --> 00:07:31 bang in the optical, astronomers can

00:07:31 --> 00:07:33 immediately check what that patch of sky

00:07:33 --> 00:07:36 looks like and looked like in the radio.

00:07:36 --> 00:07:38 The whole multi-wavelength discovery

00:07:38 --> 00:07:40 machine the community has spent two

00:07:40 --> 00:07:43 decades building is now switched on

00:07:43 --> 00:07:45 >> and the data is public. Radio

00:07:45 --> 00:07:47 astronomers, multi-wavelength folks,

00:07:47 --> 00:07:50 citizen scientists, the radio sky now

00:07:50 --> 00:07:52 belongs to everyone.

00:07:52 --> 00:07:55 >> Now to a decades old mystery that may

00:07:55 --> 00:07:58 finally have its answer, Avery. How do

00:07:58 --> 00:08:00 super massive black holes keep feeding?

00:08:00 --> 00:08:03 Nearly every large galaxy hosts one of

00:08:03 --> 00:08:05 these monsters. Millions or billions of

00:08:05 --> 00:08:07 times the mass of the sun. When they

00:08:07 --> 00:08:10 feed, they blast out enormous energy,

00:08:10 --> 00:08:12 powerful jets that heat the gas around

00:08:12 --> 00:08:15 them. And that's the paradox. That

00:08:15 --> 00:08:17 heating should cut off the black hole's

00:08:17 --> 00:08:19 own fuel supply. So why don't they

00:08:19 --> 00:08:20 starve?

00:08:20 --> 00:08:22 >> The leading idea has been a kind of

00:08:22 --> 00:08:25 cosmic recycling loop. The heated gas

00:08:25 --> 00:08:27 eventually cools back down, condenses

00:08:27 --> 00:08:29 into long, thin streamers called

00:08:29 --> 00:08:32 filaments and rains back towards the

00:08:32 --> 00:08:35 center, self-regulating. But actually

00:08:35 --> 00:08:37 seeing the connection filament to black

00:08:37 --> 00:08:40 hole has eluded astronomers for decades

00:08:40 --> 00:08:43 >> until now. An international team led by

00:08:43 --> 00:08:45 Julia Havlassa Laurando at the

00:08:45 --> 00:08:47 University of Montreal pointed the James

00:08:47 --> 00:08:51 Webb Space Telescope at NGC 4696,

00:08:51 --> 00:08:53 the giant elliptical galaxy at the heart

00:08:53 --> 00:08:56 of the Centurus cluster about 145

00:08:56 --> 00:08:58 million lighty years away. Their results

00:08:58 --> 00:09:00 were published this week in the

00:09:00 --> 00:09:02 astrophysical journal Letters.

00:09:02 --> 00:09:04 >> And Centurus, we should note, is a

00:09:04 --> 00:09:06 southern constellation. This galaxy

00:09:06 --> 00:09:08 cluster rides high in our winter sky

00:09:08 --> 00:09:10 right now, though you'll need a decent

00:09:10 --> 00:09:12 telescope for the galaxy itself.

00:09:12 --> 00:09:14 >> Right. Now, Hubble had previously

00:09:14 --> 00:09:17 photographed a curious S-shaped swirl of

00:09:17 --> 00:09:19 gas near this galaxy's central black

00:09:19 --> 00:09:20 hole. But Hubble could only show where

00:09:20 --> 00:09:23 the gas sat, not how it moved. So the

00:09:23 --> 00:09:26 team gave Web's NISP instrument nearly 8

00:09:26 --> 00:09:28 hours on the target and mapped the

00:09:28 --> 00:09:30 motion of the gas deep inside the black

00:09:30 --> 00:09:33 hole sphere of influence, resolving

00:09:33 --> 00:09:35 features just 30 light years across in a

00:09:35 --> 00:09:37 galaxy hundreds of thousands of

00:09:37 --> 00:09:40 light-years wide. And the swirl turned

00:09:40 --> 00:09:41 out to be

00:09:41 --> 00:09:44 >> a spinning disc of gas wrapped around

00:09:44 --> 00:09:47 the black hole nearly 800 lightyears

00:09:47 --> 00:09:50 across with material whipping around at

00:09:50 --> 00:09:53 up to 600 km per second. And here's the

00:09:53 --> 00:09:56 money shot. That disc is physically

00:09:56 --> 00:09:58 connected to one of the huge infalling

00:09:58 --> 00:10:00 filaments stretching out into the

00:10:00 --> 00:10:03 galaxy. They watched gas flowing along

00:10:03 --> 00:10:06 the filament pouring into the disc and

00:10:06 --> 00:10:08 from the disc falling onto the black

00:10:08 --> 00:10:09 hole.

00:10:09 --> 00:10:12 >> The missing link caught on camera. Heat

00:10:12 --> 00:10:14 the gas. The gas cools into filaments.

00:10:14 --> 00:10:16 The filaments feed the disc. The disc

00:10:16 --> 00:10:18 feeds the black hole. The black hole

00:10:18 --> 00:10:20 heats the gas. Round and round it goes.

00:10:20 --> 00:10:23 >> Pavlocondo said web is revealing that

00:10:23 --> 00:10:25 black holes might be the ultimate cosmic

00:10:25 --> 00:10:27 recyclers. And because this feeding loop

00:10:27 --> 00:10:29 shapes when galaxies can and can't form

00:10:30 --> 00:10:32 stars, understanding it is really

00:10:32 --> 00:10:34 understanding how galaxies, including

00:10:34 --> 00:10:35 ours, grow up.

00:10:36 --> 00:10:38 >> Anna, time for a double bill from the

00:10:38 --> 00:10:41 outer solar system. Two stories, one

00:10:41 --> 00:10:44 spacecraft, and a dwarf planet that

00:10:44 --> 00:10:47 keeps on giving. First, scientists have

00:10:47 --> 00:10:49 detected landslides on Pluto for the

00:10:49 --> 00:10:51 very first time.

00:10:51 --> 00:10:53 >> This is New Horizon's data, isn't it?

00:10:53 --> 00:10:56 That flyby was 11 years ago this week.

00:10:56 --> 00:10:58 >> It is. And that's the delightful part. A

00:10:58 --> 00:11:00 paper in the journal Icorus, which has

00:11:00 --> 00:11:02 been making headlines this week, reports

00:11:02 --> 00:11:04 that an international team went back

00:11:04 --> 00:11:06 through the highresolution images from

00:11:06 --> 00:11:09 New Horizon's Lori camera. Pictures

00:11:09 --> 00:11:11 showing Pluto's surface at about 300 m

00:11:11 --> 00:11:15 per pixel and found six large landslides

00:11:15 --> 00:11:17 inside three impact craters near Sputnik

00:11:17 --> 00:11:19 Planita, that famous heart-shaped

00:11:19 --> 00:11:22 nitrogen ice plane. How do you recognize

00:11:22 --> 00:11:25 a landslide on a world made of ice?

00:11:25 --> 00:11:26 >> Same fingerprints as Earth.

00:11:26 --> 00:11:28 Crescent-shaped collapse scars near the

00:11:28 --> 00:11:31 crater rims, huge displaced blocks of

00:11:31 --> 00:11:33 ice, and debris fanning out across the

00:11:33 --> 00:11:35 crater floors. The team measured them.

00:11:35 --> 00:11:39 These slides descend 1 12 to over 2 km

00:11:39 --> 00:11:42 run out as far as 14 1/2 km, and the

00:11:42 --> 00:11:46 largest covers around the 130 km.

00:11:46 --> 00:11:47 >> And landslides are everywhere else,

00:11:47 --> 00:11:50 aren't they? Earth, Mars, series,

00:11:50 --> 00:11:53 asteroids. Even Pluto's moon, Sharon,

00:11:53 --> 00:11:55 showed evidence years ago. Pluto itself

00:11:55 --> 00:11:57 was the odd one out,

00:11:57 --> 00:11:59 >> which was genuinely puzzling because

00:11:59 --> 00:12:01 Pluto has steep crater walls and rugged

00:12:01 --> 00:12:04 icy terrain. All the right ingredients.

00:12:04 --> 00:12:06 Now, the gap is filled, and it tells us

00:12:06 --> 00:12:08 gravity-driven slope processes are

00:12:08 --> 00:12:10 actively reshaping Pluto's frozen

00:12:10 --> 00:12:13 surface, even under gravity a fraction

00:12:13 --> 00:12:15 of ours. What triggered them is still

00:12:15 --> 00:12:17 open. Possibilities range from tectonic

00:12:17 --> 00:12:19 activity to meteoroid impacts.

00:12:20 --> 00:12:22 >> A world we visited for a few hours in

00:12:22 --> 00:12:25 2015 still handing us firsts a decade

00:12:25 --> 00:12:26 later.

00:12:26 --> 00:12:29 >> And it's not done because part two of

00:12:29 --> 00:12:31 our Pluto double is about the other half

00:12:31 --> 00:12:33 of that famous pair.

00:12:33 --> 00:12:36 >> Jiren Pluto's enormous moon so big

00:12:36 --> 00:12:38 relative to Pluto that the two really

00:12:38 --> 00:12:40 form a double world. And a study

00:12:40 --> 00:12:42 published Tuesday in Nature

00:12:42 --> 00:12:44 Communications says Sharon's mountains

00:12:44 --> 00:12:47 have preserved a memory of a wilder

00:12:47 --> 00:12:47 youth.

00:12:47 --> 00:12:49 >> What kind of memory?

00:12:49 --> 00:12:52 >> A record of despinning across the solar

00:12:52 --> 00:12:54 system. Tidal forces gradually slow a

00:12:54 --> 00:12:57 body's rotation. And as the spin slows,

00:12:57 --> 00:13:00 the body's shape relaxes, stressing and

00:13:00 --> 00:13:02 cracking the surface. It's long been

00:13:02 --> 00:13:05 theorized for Sharon, but clear

00:13:05 --> 00:13:07 geological evidence was missing. So

00:13:07 --> 00:13:10 Hanzang Chin and colleagues at ETH Zoric

00:13:10 --> 00:13:13 and UCLA examined the orientations and

00:13:13 --> 00:13:16 types of tectonic features, mountain

00:13:16 --> 00:13:19 ranges and faults in Oz Terra, Sharon's

00:13:19 --> 00:13:22 northern rugged highlands. Again, using

00:13:22 --> 00:13:24 New Horizon's flyby data,

00:13:24 --> 00:13:26 >> and the tectonic pattern fits the

00:13:26 --> 00:13:27 despinning story

00:13:27 --> 00:13:29 >> beautifully. Their modeling suggests

00:13:29 --> 00:13:32 Sharon's rotation period was once around

00:13:32 --> 00:13:35 14.3 hours and it has since slowed to

00:13:35 --> 00:13:38 today's roughly 153 hours, locked in

00:13:38 --> 00:13:41 step with its orbit around Pluto. That's

00:13:41 --> 00:13:43 more than a 10-fold slowdown, and the

00:13:43 --> 00:13:45 stresses from that transformation are

00:13:45 --> 00:13:47 etched into the mountains we

00:13:47 --> 00:13:48 photographed in 2015.

00:13:48 --> 00:13:51 >> Chen said the study drastically changed

00:13:51 --> 00:13:53 her understanding of Cheron's geological

00:13:53 --> 00:13:55 history. And there's a bonus finding,

00:13:55 --> 00:13:57 isn't there, about how Cheron was born.

00:13:57 --> 00:14:00 Yes, the way despinning and global

00:14:00 --> 00:14:03 contraction evolved together favors

00:14:03 --> 00:14:05 what's called a cold start for Sharon,

00:14:05 --> 00:14:07 which is a real clue to the early

00:14:07 --> 00:14:10 thermal history of icy moons across the

00:14:10 --> 00:14:12 outer solar system. So, between Pluto's

00:14:12 --> 00:14:15 landslides and Sharon's slowing spin,

00:14:15 --> 00:14:18 one 11-year-old data set gave us two

00:14:18 --> 00:14:20 papers in a week. Not a bad return on a

00:14:20 --> 00:14:21 flyby.

00:14:21 --> 00:14:23 >> Our final story today, Anna, comes with

00:14:23 --> 00:14:26 some genuinely eyewidening numbers.

00:14:26 --> 00:14:29 SpaceX has filed its latest semiannual

00:14:29 --> 00:14:32 constellation status report with the US

00:14:32 --> 00:14:34 Federal Communications Commission. And

00:14:34 --> 00:14:36 according to coverage of the filing,

00:14:36 --> 00:14:42 Starling satellites performed 27

00:14:42 --> 00:14:44 collision avoidance maneuvers between

00:14:44 --> 00:14:48 December 2025 and May 2026.

00:14:48 --> 00:14:50 >> 207

00:14:50 --> 00:14:51 in 6 months.

00:14:52 --> 00:14:54 >> Up nearly 60 on the previous half

00:14:54 --> 00:14:57 year. Put the two periods together and

00:14:57 --> 00:15:01 the constellation made over 355

00:15:01 --> 00:15:04 dodges in 12 months, more than triple

00:15:04 --> 00:15:07 what it performed in all of 2024. At on

00:15:07 --> 00:15:10 average, each Starling satellite now

00:15:10 --> 00:15:13 swerves more than 40 times a year.

00:15:13 --> 00:15:15 That's nearly a dodge a week per

00:15:15 --> 00:15:16 satellite.

00:15:16 --> 00:15:18 >> Let's be fair to SpaceX for a moment,

00:15:18 --> 00:15:20 though. These maneuvers are the system

00:15:20 --> 00:15:22 working as designed, aren't they?

00:15:22 --> 00:15:24 >> They are. The satellites dodge

00:15:24 --> 00:15:27 autonomously whenever the predicted

00:15:27 --> 00:15:29 collision probability exceeds 3 in 10

00:15:30 --> 00:15:32 million, an extremely conservative

00:15:32 --> 00:15:34 threshold, far tighter than the industry

00:15:34 --> 00:15:37 standard. Experts consistently credit

00:15:37 --> 00:15:40 SpaceX with managing its traffic well

00:15:40 --> 00:15:42 and being transparent with the data. The

00:15:42 --> 00:15:44 concern is the trend line, not the

00:15:44 --> 00:15:46 competence. because the numbers

00:15:46 --> 00:15:49 compound. More satellites means more

00:15:49 --> 00:15:51 close approaches means more maneuvers

00:15:51 --> 00:15:54 means more residual risk that never

00:15:54 --> 00:15:55 quite goes to zero.

00:15:55 --> 00:15:58 >> Exactly the point Hugh Lewis makes. He's

00:15:58 --> 00:15:59 the University of Birmingham

00:15:59 --> 00:16:01 astronautics professor who's tracked

00:16:02 --> 00:16:04 these reports for years. Each maneuver

00:16:04 --> 00:16:07 cuts the collision odds to about 1 in a

00:16:07 --> 00:16:09 million, which sounds negligible, but as

00:16:09 --> 00:16:11 he puts it, if you make a million

00:16:11 --> 00:16:13 maneuvers with a 1 in a million

00:16:13 --> 00:16:16 residual, you end up with an aggregate

00:16:16 --> 00:16:18 risk across the constellation that you

00:16:18 --> 00:16:20 simply can't get rid of. His blunt

00:16:20 --> 00:16:22 assessment, he thinks we're heading

00:16:22 --> 00:16:24 towards a situation where there will be

00:16:24 --> 00:16:27 a collision involving an operational

00:16:27 --> 00:16:29 satellite in the constellation. And the

00:16:29 --> 00:16:31 projections

00:16:31 --> 00:16:33 >> on current growth, Starlink passes a

00:16:33 --> 00:16:36 million total avoidance maneuvers by mid

00:16:36 --> 00:16:39 2027. And by 2030, the constellation

00:16:39 --> 00:16:41 could be making more than a million

00:16:41 --> 00:16:44 maneuvers every single year. Remember

00:16:44 --> 00:16:47 too, and regular listeners will, SpaceX

00:16:47 --> 00:16:49 has applied to the FCC to grow Starlink

00:16:49 --> 00:16:52 toward a 100 satellites, a story we

00:16:52 --> 00:16:54 covered a couple of weeks back. And it's

00:16:54 --> 00:16:56 not alone up there. Amazon's

00:16:56 --> 00:16:59 constellation and China's Ken Fan are

00:16:59 --> 00:17:00 actively deploying as well.

00:17:00 --> 00:17:03 >> The number of operational spacecraft in

00:17:03 --> 00:17:05 orbit has gone from about 10 to

00:17:05 --> 00:17:08 about 16 in just a year. Other

00:17:08 --> 00:17:10 experts are calling for operators to

00:17:10 --> 00:17:12 disclose predicted maneuver counts

00:17:12 --> 00:17:15 before constellations are even approved.

00:17:15 --> 00:17:16 Though regulators know whether the

00:17:16 --> 00:17:18 satellites can actually keep up.

00:17:18 --> 00:17:21 >> Low Earth orbit is a shared resource.

00:17:21 --> 00:17:23 And this is the traffic report. We'll

00:17:23 --> 00:17:24 keep watching the numbers because

00:17:24 --> 00:17:27 everyone from astronomers to airlines to

00:17:27 --> 00:17:29 your GPS depends on that neighborhood

00:17:29 --> 00:17:31 staying safe.

00:17:31 --> 00:17:33 >> Time now for tonight's sky watching. And

00:17:33 --> 00:17:35 for our southern hemisphere friends, the

00:17:35 --> 00:17:37 news is good. The moon is a waning

00:17:37 --> 00:17:39 crescent rising in the small hours. So

00:17:40 --> 00:17:41 evenings this week are dark and

00:17:41 --> 00:17:42 glorious.

00:17:42 --> 00:17:45 >> Which means the winter Milky Way at its

00:17:45 --> 00:17:47 absolute best. Face south after dinner

00:17:48 --> 00:17:50 and the galactic core in Sagittarius and

00:17:50 --> 00:17:52 Scorpius is almost directly overhead

00:17:52 --> 00:17:55 from most of Australia and New Zealand.

00:17:55 --> 00:17:58 Dust lanes, star clouds, the lot. If you

00:17:58 --> 00:18:00 can get away from city lights this week,

00:18:00 --> 00:18:01 do it.

00:18:01 --> 00:18:03 >> While you're there, sweep up Omega

00:18:03 --> 00:18:05 Centauri and the Southern Cross riding

00:18:05 --> 00:18:07 high. And if you've got binoculars, the

00:18:07 --> 00:18:09 starfields between Scorpius's tail and

00:18:09 --> 00:18:12 the teapot of Sagittarius will keep you

00:18:12 --> 00:18:14 busy all evening. Saturn is climbing in

00:18:14 --> 00:18:16 the east by mid evening for a late night

00:18:16 --> 00:18:19 treat. And dazzling Venus still rules

00:18:19 --> 00:18:21 the early evening western sky.

00:18:21 --> 00:18:23 >> And one for the launch watchers.

00:18:23 --> 00:18:26 SpaceX's Starship Flight 13 window opens

00:18:26 --> 00:18:29 tonight, US time. That's tomorrow

00:18:29 --> 00:18:33 morning for us from about 8:45 AEST. So

00:18:33 --> 00:18:35 pour a coffee and watch this space.

00:18:35 --> 00:18:37 We'll have the full story in Saturday's

00:18:37 --> 00:18:38 weekend rap.

00:18:38 --> 00:18:40 >> That's it for today's episode. Thanks

00:18:40 --> 00:18:42 for joining us. You can find show notes,

00:18:42 --> 00:18:44 links to every story, and our back

00:18:44 --> 00:18:47 catalog at astronomydaily.io.

00:18:47 --> 00:18:50 And we're astronomyaily pod on all the

00:18:50 --> 00:18:51 socials.

00:18:51 --> 00:18:53 >> Astronomy Daily is part of the byes.com

00:18:54 --> 00:18:56 podcast network. I'm Avery

00:18:56 --> 00:18:58 >> and I'm Anna. We'll see you tomorrow.

00:18:58 --> 00:18:59 Until then,

00:18:59 --> 00:19:11 >> clear skies.

00:19:11 --> 00:19:15 Stories told.