Hide and Seek - The Faintest Planet Ever Imaged, Pluto’s Landslides & Starlink’s 355,000 Dodges
Movies First: Film Reviews & InsightsJuly 16, 202600:19:2317.76 MB

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

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.