Become a supporter of this podcast: https://www.spreaker.com/podcast/astronomy-daily-latest-space-news--5648921/support.
Sponsor Details:
Ensure your online privacy by using NordVPN. To get our special listener deal and save a lot of money, visit www.astronomydaily.io/nordvpn. You'll be glad you did!
Get the best secure and private email on the planet. Stop your Government, google and who knows who else spying on every email you write. Do what we did and use ProtonMail. They beleive in privacy and there are no ads in their business model...yet they still provide a free forever service. Check them out and get out special deal at www.astronomydaily.io/protonmail
Become a supporter of Astronomy Daily by joining our Supporters Club. Commercial free episodes daily are only a click way... Click Here
This episode includes AI-generated content.
00:00:00 --> 00:00:02 Anna: Welcome to Astronomy Daily, your daily dose
00:00:02 --> 00:00:05 of space and astronomy news. I'm Anna.
00:00:06 --> 00:00:08 Avery: And I'm, um, avery. It's Thursday, the 16th
00:00:08 --> 00:00:11 of July, 2026, and we have a
00:00:11 --> 00:00:14 genuinely lovely lineup for you today,
00:00:14 --> 00:00:17 including a story that's been 10 years in the
00:00:17 --> 00:00:19 making, or more accurately, 10 years in the
00:00:19 --> 00:00:20 hiding.
00:00:20 --> 00:00:23 Anna: That's Our lead astronomers have finally
00:00:23 --> 00:00:25 caught a planet that's been playing hide and
00:00:25 --> 00:00:28 seek with them for over a decade. And it
00:00:28 --> 00:00:31 turns out to be the faintest exoplanet ever
00:00:31 --> 00:00:33 imaged from Earth. And it lives in a southern
00:00:33 --> 00:00:36 constellation, which makes it feel just a
00:00:36 --> 00:00:37 little bit like ours.
00:00:37 --> 00:00:40 Avery: We've also got the completion of a nine year
00:00:40 --> 00:00:42 project to build the sharpest radio map of
00:00:42 --> 00:00:45 the entire sky. And the James Webb Space
00:00:45 --> 00:00:48 Telescope catching a supermassive black hole
00:00:48 --> 00:00:50 in the act of feeding itself.
00:00:50 --> 00:00:53 Anna: Then it's a double bill from the outer solar
00:00:53 --> 00:00:56 system. Landslides on Pluto spotted for
00:00:56 --> 00:00:59 the first time, and evidence that Pluto's big
00:00:59 --> 00:01:01 moon, Charon, once spun more than 10
00:01:01 --> 00:01:03 times faster than it does today.
00:01:04 --> 00:01:06 Avery: And we'll wrap the news with some sobering
00:01:06 --> 00:01:09 numbers. SpaceX's Starlink satellites had
00:01:09 --> 00:01:11 to dodge potential collisions more than
00:01:11 --> 00:01:14 355 times
00:01:14 --> 00:01:17 in the past year. We'll unpack what that
00:01:17 --> 00:01:18 means for everyone's
00:01:18 --> 00:01:21 Anna: orbit, plus your Southern hemisphere sky
00:01:21 --> 00:01:23 watching for tonight. Let's get into it.
00:01:23 --> 00:01:25 Avery, cast your mind.
00:01:25 --> 00:01:27 Back in 2008, astronomers
00:01:27 --> 00:01:30 directly imaged a planet around the young
00:01:30 --> 00:01:33 star Beta Pictoris, one of the very first
00:01:33 --> 00:01:36 exoplanets ever photographed. That was
00:01:36 --> 00:01:38 Beta Pictoris B. A second planet
00:01:38 --> 00:01:41 C followed. And ever since, there's been a,
00:01:41 --> 00:01:44 uh, nagging suspicion that the system was
00:01:44 --> 00:01:44 hiding
00:01:44 --> 00:01:46 Avery: something more because of the disk. Right.
00:01:47 --> 00:01:49 Beta Pictoris has this magnificent debris,
00:01:49 --> 00:01:51 uh, disk. It's the poster child for planet
00:01:51 --> 00:01:54 formation. And parts of it were warped and
00:01:54 --> 00:01:56 sculpted in ways that two known planets
00:01:56 --> 00:01:57 couldn't fully explain.
00:01:58 --> 00:02:01 Anna: Exactly. And now we know why. In a
00:02:01 --> 00:02:02 study published Wednesday in the
00:02:02 --> 00:02:05 Astrophysical Journal Letters, a team using
00:02:05 --> 00:02:08 the European Southern Observatory's Very
00:02:08 --> 00:02:11 Large Telescope in Chile has confirmed a
00:02:11 --> 00:02:13 third planet, Beta Pictoris D.
00:02:13 --> 00:02:16 And here's the headline. It's roughly
00:02:16 --> 00:02:19 100 times fainter than Beta Pictoris
00:02:19 --> 00:02:22 B, which makes it the faintest exoplanet
00:02:22 --> 00:02:24 ever directly imaged from Earth.
00:02:25 --> 00:02:27 Avery: A hundred times fainter. To put that in
00:02:27 --> 00:02:30 context for everyone, direct imaging means
00:02:30 --> 00:02:32 actually capturing the planet's own light in
00:02:32 --> 00:02:34 a photograph next to a star that's
00:02:34 --> 00:02:37 overwhelmingly brighter. It's often compared
00:02:37 --> 00:02:40 to spotting a firefly next to a lighthouse.
00:02:40 --> 00:02:43 This is spotting a very Dim
00:02:43 --> 00:02:43 firefly.
00:02:44 --> 00:02:47 Anna: And the discovery itself was serendipitous.
00:02:47 --> 00:02:50 Ben Sutliff at the University of Edinburgh
00:02:50 --> 00:02:52 who co led the study, said they were
00:02:52 --> 00:02:55 originally just going back to study the known
00:02:55 --> 00:02:57 planet Beta Pictoris B to see how it
00:02:57 --> 00:03:00 changed over time. But in their new images
00:03:00 --> 00:03:03 from the VLT's Eris instrument, there was
00:03:03 --> 00:03:05 something else. A faint point of light
00:03:05 --> 00:03:08 separated from Planet B that sent them down
00:03:08 --> 00:03:10 an entirely new path.
00:03:10 --> 00:03:12 Avery: And this is where the hide and seek comes in.
00:03:13 --> 00:03:15 Once they knew what to look for, they trawled
00:03:15 --> 00:03:17 back through the archives. And there it was,
00:03:17 --> 00:03:20 lurking. In more than a decade of old
00:03:20 --> 00:03:22 observations from the VLT SPEAR instrument
00:03:23 --> 00:03:25 and even in James Webb Space Telescope data,
00:03:25 --> 00:03:28 the planet had been photographed for years.
00:03:28 --> 00:03:30 Nobody had noticed.
00:03:30 --> 00:03:33 Anna: Co author Jane Burkeby at Oxford put it
00:03:33 --> 00:03:36 beautifully. Planet D has been playing hide
00:03:36 --> 00:03:38 and seek with us for over a decade and now
00:03:38 --> 00:03:40 we can say found you.
00:03:40 --> 00:03:42 Avery: So what do we know about the world itself?
00:03:43 --> 00:03:46 Anna: It's a gas giant about 2.4 times
00:03:46 --> 00:03:48 the mass of Jupiter, which sounds big, but
00:03:48 --> 00:03:50 is actually the lightweight of the family.
00:03:51 --> 00:03:54 Planets B and c are each 10 Jupiter
00:03:54 --> 00:03:57 masses. Planet D sits, um, much further out
00:03:57 --> 00:03:59 from the star on a wide orbit, so it's cooler
00:03:59 --> 00:04:02 and dimmer than its siblings, hence the
00:04:02 --> 00:04:04 difficulty. And satisfyingly, its
00:04:04 --> 00:04:07 presence helps explain that odd structure in
00:04:07 --> 00:04:09 the debris disk that's puzzled astronomers
00:04:09 --> 00:04:10 for years.
00:04:10 --> 00:04:13 Avery: There's also a nice milestone tucked in here.
00:04:13 --> 00:04:15 This makes Beta Pictoris only the second
00:04:15 --> 00:04:18 planetary system after HR
00:04:18 --> 00:04:20 8799, where more than two
00:04:20 --> 00:04:23 planets have been directly. We're building
00:04:23 --> 00:04:26 up actual family portraits of other solar
00:04:26 --> 00:04:26 systems now.
00:04:27 --> 00:04:29 Anna: And an independent team at the University of
00:04:29 --> 00:04:32 California spotted the same object in their
00:04:32 --> 00:04:34 own data at almost the same time, which gives
00:04:34 --> 00:04:37 the detection real confidence. Now the
00:04:37 --> 00:04:40 bit our audience will love. Beta Pictoris is
00:04:40 --> 00:04:43 a southern star. It sits in the constellation
00:04:43 --> 00:04:46 Pictor, the Painter's Easel, just next to
00:04:46 --> 00:04:48 brilliant canopus. And at 63 light
00:04:48 --> 00:04:51 years away, it's visible from Australia and
00:04:51 --> 00:04:53 New Zealand. Though right now in July
00:04:53 --> 00:04:56 it's low in our evening sky and best hunted
00:04:56 --> 00:04:58 in the pre dawn hours later in
00:04:58 --> 00:05:01 Avery: the year, a planetary system with three
00:05:01 --> 00:05:03 photographed worlds sitting in our southern
00:05:03 --> 00:05:05 sky. Not bad at all.
00:05:05 --> 00:05:08 Next, A, uh, project nine years in the
00:05:08 --> 00:05:11 making has just crossed the finish line. The
00:05:11 --> 00:05:14 U.S. national Science Foundation's National
00:05:14 --> 00:05:17 Radio Astronomy Observatory has announced
00:05:17 --> 00:05:20 that observations for the Very Large Array
00:05:20 --> 00:05:22 Sky Survey VLAS are
00:05:22 --> 00:05:25 complete. It's the most detailed radio
00:05:25 --> 00:05:27 survey of the sky ever conducted.
00:05:28 --> 00:05:31 Anna: This is the VLA in New Mexico. The
00:05:31 --> 00:05:34 iconic Y shaped array of 27 dishes
00:05:34 --> 00:05:36 from every space documentary ever made.
00:05:36 --> 00:05:39 Avery: That's the one. From September 2017
00:05:39 --> 00:05:42 through February this year, the array
00:05:42 --> 00:05:45 repeatedly swept about 34
00:05:45 --> 00:05:48 square degrees. Essentially the whole sky
00:05:48 --> 00:05:51 visible from New Mexico and everything north
00:05:51 --> 00:05:53 of minus 40 degrees declination.
00:05:53 --> 00:05:56 That's roughly 80% of the entire
00:05:56 --> 00:05:59 celestial sphere. Mapped at a resolution
00:05:59 --> 00:06:02 of about 2 and a half arcseconds in the 2
00:06:02 --> 00:06:03 to 4 GHz band.
00:06:03 --> 00:06:05 Anna: And how does that compare to what came
00:06:05 --> 00:06:06 before?
00:06:06 --> 00:06:09 Avery: It's about 18 times sharper than the
00:06:09 --> 00:06:12 previous benchmark all sky radio survey from
00:06:12 --> 00:06:14 the 1990s. The numbers are
00:06:14 --> 00:06:16 staggering. Roughly six and a half thousand
00:06:17 --> 00:06:20 thousand observing hours. Half a petabyte of
00:06:20 --> 00:06:22 raw data. And the processed data products are
00:06:22 --> 00:06:25 expected to reach around 2 petabytes, the
00:06:25 --> 00:06:28 largest data volume the VLA has ever
00:06:28 --> 00:06:31 produced. They use a clever on the fly
00:06:31 --> 00:06:34 mosaicing 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 each
00:06:39 --> 00:06:39 field.
00:06:39 --> 00:06:42 Anna: And crucially, they surveyed the sky multiple
00:06:42 --> 00:06:45 times over those nine years. Which means VLAS
00:06:45 --> 00:06:48 isn't just a map, it's a movie. Comparing
00:06:48 --> 00:06:51 epochs revealed a dynamic radio sky.
00:06:51 --> 00:06:53 Sources that flare, fade or appear from
00:06:53 --> 00:06:56 nowhere. Exploding stars, feeding black
00:06:56 --> 00:06:58 holes, colliding neutron stars.
00:06:59 --> 00:07:01 Avery: Which brings us to the timing. And honestly,
00:07:01 --> 00:07:03 the timing is the best part of the story.
00:07:04 --> 00:07:07 Just over two weeks ago on June 30, the
00:07:07 --> 00:07:10 Vera C. Rubin Observatory in Chile began
00:07:10 --> 00:07:13 its decade long legacy survey of space and
00:07:13 --> 00:07:15 time, sweeping the southern optical sky
00:07:16 --> 00:07:18 every few nights. So for the first time in
00:07:18 --> 00:07:21 history, we have a complete high resolution
00:07:21 --> 00:07:24 radio map and a real time optical
00:07:24 --> 00:07:27 transient stream operating simultaneously.
00:07:27 --> 00:07:29 Anna: Though when Rubin flags something going bang
00:07:29 --> 00:07:32 in the optical, astronomers can immediately
00:07:32 --> 00:07:34 check what that patch of sky looks like and
00:07:34 --> 00:07:37 looked like in the radio. The whole multi
00:07:37 --> 00:07:39 wavelength discovery machine the community
00:07:39 --> 00:07:42 has spent two decades building is now
00:07:42 --> 00:07:44 switched on and the data's public.
00:07:44 --> 00:07:47 Avery: Radio 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 Anna: Now to a decades old mystery that may
00:07:55 --> 00:07:57 finally have its answer. Avery, how do
00:07:57 --> 00:08:00 supermassive black holes keep feeding?
00:08:00 --> 00:08:03 Nearly every large galaxy hosts one of these
00:08:03 --> 00:08:06 monsters. Millions or billions of times the
00:08:06 --> 00:08:09 mass of the Sun. When they feed, they blast
00:08:09 --> 00:08:11 out enormous energy, powerful jets that heat
00:08:11 --> 00:08:14 the gas around them. And that's the paradox.
00:08:14 --> 00:08:17 That heating should cut off the black hole's
00:08:17 --> 00:08:19 own fuel supply. So why don't they starve?
00:08:20 --> 00:08:23 Avery: The leading idea has been a kind of cosmic
00:08:23 --> 00:08:25 recycling loop. The heated gas eventually
00:08:25 --> 00:08:28 cools back down, condenses into long thin
00:08:28 --> 00:08:31 streamers called filaments and rains back
00:08:31 --> 00:08:33 towards the center. Self regulating
00:08:34 --> 00:08:36 but Actually seeing the connection filament
00:08:36 --> 00:08:39 to black hole has eluded astronomers for
00:08:39 --> 00:08:40 decades.
00:08:40 --> 00:08:43 Anna: Until now. An international team led by Julie
00:08:43 --> 00:08:46 Hvlasic Lorando at the University of Montreal
00:08:46 --> 00:08:48 pointed the James Webb Space telescope at
00:08:48 --> 00:08:51 NGC 4696, the giant
00:08:51 --> 00:08:53 elliptical galaxy at the heart of the
00:08:53 --> 00:08:56 Centaurus cluster, about 145
00:08:56 --> 00:08:58 million light years away. Their results were
00:08:58 --> 00:09:00 published this week in the Astrophysical
00:09:00 --> 00:09:01 Journal Letters.
00:09:01 --> 00:09:04 Avery: And Centaurus, we should note, is a southern
00:09:04 --> 00:09:07 constellation. This galaxy cluster rides high
00:09:07 --> 00:09:09 in our winter sky right now, though you'll
00:09:09 --> 00:09:11 need a decent telescope for the galaxy
00:09:11 --> 00:09:11 itself.
00:09:12 --> 00:09:14 Anna: White. Now, Hubble had previously
00:09:14 --> 00:09:17 photographed a curious S shaped swirl of gas
00:09:17 --> 00:09:19 near this galaxy's central black hole. But
00:09:19 --> 00:09:22 Hubble could only show where the gas sat, not
00:09:22 --> 00:09:24 how it moved. So the team gave Webb's
00:09:24 --> 00:09:27 NIRSP instrument nearly eight hours on the
00:09:27 --> 00:09:29 target and mapped the motion of the gas deep
00:09:29 --> 00:09:32 inside the black hole's sphere of influence,
00:09:32 --> 00:09:35 resolving features just 30 light years across
00:09:35 --> 00:09:37 in a galaxy hundreds of thousands of light
00:09:37 --> 00:09:38 years wide.
00:09:38 --> 00:09:40 Avery: And the swirl turned out to be
00:09:41 --> 00:09:44 Anna: a spinning disk of gas wrapped around
00:09:44 --> 00:09:46 the black hole, nearly 800 light
00:09:46 --> 00:09:49 years across, with material whipping around
00:09:49 --> 00:09:52 at, uh, up to 600 kilometers per second.
00:09:52 --> 00:09:55 And here's the money shot. That disk is
00:09:55 --> 00:09:58 physically connected to one of the huge
00:09:58 --> 00:10:00 infalling 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 disk, and from
00:10:06 --> 00:10:08 the disk falling onto the black hole.
00:10:09 --> 00:10:12 Avery: The missing link caught on camera heat the
00:10:12 --> 00:10:14 gas. The gas cools into filaments. The
00:10:14 --> 00:10:16 filaments feed the disk. The disk feeds the
00:10:16 --> 00:10:18 black hole. The black hole heats the gas.
00:10:19 --> 00:10:20 Round and round it goes.
00:10:20 --> 00:10:22 Anna: Havlasic Lorando said Webb is revealing that
00:10:22 --> 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
00:10:29 --> 00:10:32 stars, understanding it is really
00:10:32 --> 00:10:35 understanding how galaxies, including ours,
00:10:35 --> 00:10:35 grow up.
00:10:35 --> 00:10:38 Avery: Anna, uh, time for a double bill from the
00:10:38 --> 00:10:41 outer solar system. Two stories,
00:10:41 --> 00:10:43 one spacecraft, and a dwarf planet that
00:10:43 --> 00:10:46 keeps on giving. First,
00:10:46 --> 00:10:49 scientists have detected landslides on Pluto
00:10:49 --> 00:10:50 for the very first time.
00:10:50 --> 00:10:53 Anna: This is New Horizons data, isn't it? That
00:10:53 --> 00:10:55 Flyby was 11 years ago this week.
00:10:55 --> 00:10:58 Avery: It is, and that's the delightful part. A
00:10:58 --> 00:11:00 paper in the journal Icarus, which has been
00:11:00 --> 00:11:03 making headlines this week, reports that an
00:11:03 --> 00:11:05 international team went back through the high
00:11:05 --> 00:11:08 resolution images from New Horizons lorry
00:11:08 --> 00:11:10 camera pictures showing Pluto's surface at
00:11:10 --> 00:11:13 about 300 meters per pixel and found
00:11:13 --> 00:11:16 six large landslides inside three impact
00:11:16 --> 00:11:19 craters near Sputnik Planita. That famous
00:11:19 --> 00:11:20 heart shaped nitrogen ice plane.
00:11:21 --> 00:11:23 Anna: How do you recognize a landslide on a world
00:11:23 --> 00:11:24 made of ice?
00:11:25 --> 00:11:27 Avery: Same fingerprints as Earth. Crescent shaped
00:11:27 --> 00:11:30 collapse scars near the crater rims. Huge
00:11:30 --> 00:11:32 displaced blocks of ice and debris fanning
00:11:32 --> 00:11:35 out across the crater floors. The team
00:11:35 --> 00:11:37 measured them. These slides descend one and a
00:11:37 --> 00:11:40 half to over two kilometers, run out as far
00:11:40 --> 00:11:42 as 14 and a half kilometers and the largest
00:11:42 --> 00:11:45 covers around 130 square kilometers.
00:11:45 --> 00:11:48 Anna: And landslides are everywhere else, aren't
00:11:48 --> 00:11:50 they? Earth, Mars, Ceres,
00:11:50 --> 00:11:53 asteroids, even Pluto's moon Charon showed
00:11:53 --> 00:11:56 evidence years ago Pluto itself was the odd
00:11:56 --> 00:11:57 one out which was
00:11:57 --> 00:12:00 Avery: genuinely puzzling because Pluto has steep
00:12:00 --> 00:12:02 crater walls and rugged icy terrain. All the
00:12:02 --> 00:12:05 right ingredients. Now the gap is filled and
00:12:05 --> 00:12:08 it tells us gravity driven slope processes
00:12:08 --> 00:12:10 are actively reshaping Pluto's frozen
00:12:10 --> 00:12:13 surface. Even under gravity, a fraction of
00:12:13 --> 00:12:15 ours. What triggered them is still open.
00:12:15 --> 00:12:18 Possibilities range from tectonic activity to
00:12:18 --> 00:12:19 meteoroid impacts.
00:12:19 --> 00:12:22 Anna: A world we visited for a few hours in 2015,
00:12:23 --> 00:12:25 still handing us firsts a decade later.
00:12:26 --> 00:12:28 Avery: And um, it's not done because part two of
00:12:28 --> 00:12:30 our Pluto double is about
00:12:30 --> 00:12:32 Avery: the other half of that famous pair
00:12:32 --> 00:12:35 Anna: of Charon, Pluto's enormous moon. So
00:12:35 --> 00:12:38 big relative to Pluto that the two really
00:12:38 --> 00:12:40 form a double world. And a study published
00:12:41 --> 00:12:43 Tuesday in Nature Communications says
00:12:43 --> 00:12:46 Charon's mountains have preserved a memory of
00:12:46 --> 00:12:47 a wilder youth.
00:12:47 --> 00:12:48 Avery: What kind of memory?
00:12:49 --> 00:12:52 Anna: A record of despinning across the solar
00:12:52 --> 00:12:54 system. Tidal forces gradually slow a body's
00:12:54 --> 00:12:57 rotation and as ah, the spin slows the
00:12:57 --> 00:13:00 body's shape relaxes stressing and
00:13:00 --> 00:13:02 cracking the surface. The it's long been
00:13:02 --> 00:13:05 theorized for Charon but clear geological
00:13:05 --> 00:13:08 evidence was missing. So Han, Zeng Chin
00:13:08 --> 00:13:10 and colleagues at ETH Zurich and
00:13:10 --> 00:13:13 UCLA examined the orientations
00:13:13 --> 00:13:16 and types of tectonic features, mountain
00:13:16 --> 00:13:18 ranges and faults in Aus Terra
00:13:18 --> 00:13:21 Sharon's northern rugged highlands. Again
00:13:21 --> 00:13:23 using New Horizons flyby data.
00:13:24 --> 00:13:26 Avery: And um, the tectonic pattern fits the de
00:13:26 --> 00:13:27 spinning story beautifully.
00:13:28 --> 00:13:30 Anna: Their modeling suggests Charon's rotation
00:13:30 --> 00:13:33 period was once around 14.3 hours
00:13:33 --> 00:13:36 and it has since slowed to today's roughly
00:13:36 --> 00:13:39 153 hours locked in step with
00:13:39 --> 00:13:41 its orbit around Pluto. That's more than a
00:13:41 --> 00:13:44 tenfold slowdown and the stresses from that
00:13:44 --> 00:13:46 transformation are etched into the mountains
00:13:46 --> 00:13:48 we photographed in 2015.
00:13:48 --> 00:13:51 Avery: Chen said the study drastically changed her
00:13:51 --> 00:13:53 understanding of Charon's geologic history.
00:13:53 --> 00:13:55 And there's a bonus finding, isn't there
00:13:55 --> 00:13:57 about how Charon was born?
00:13:57 --> 00:14:00 Anna: Yes, the way despinning and global
00:14:00 --> 00:14:02 contraction evolved together favors
00:14:02 --> 00:14:05 what's called a cold start for Charon, which
00:14:05 --> 00:14:08 is a real clue to the early thermal history
00:14:08 --> 00:14:11 of icy moons across the Outer solar system.
00:14:11 --> 00:14:14 So between Pluto's landslides and charon's
00:14:14 --> 00:14:17 slowing spin, one 11 year old dataset
00:14:17 --> 00:14:19 gave us two papers in a week. Not a bad
00:14:19 --> 00:14:21 return on a flyby.
00:14:21 --> 00:14:23 Avery: Our final story today, Anna, uh, comes with
00:14:23 --> 00:14:26 some genuinely eye widening numbers.
00:14:26 --> 00:14:29 SpaceX has filed its latest semi annual
00:14:29 --> 00:14:32 constellation status report with the U.S.
00:14:32 --> 00:14:34 federal Communications Commission. And
00:14:34 --> 00:14:37 according to coverage of the filing, StarLink
00:14:37 --> 00:14:38 satellites performed
00:14:38 --> 00:14:42 207
00:14:42 --> 00:14:44 collision avoidance maneuvers between
00:14:44 --> 00:14:46 December 2025 and
00:14:46 --> 00:14:48 May 2026.
00:14:48 --> 00:14:51 Anna: 207 in six months,
00:14:51 --> 00:14:53 up nearly 60
00:14:53 --> 00:14:55 Avery: on the previous half year. Put the two
00:14:55 --> 00:14:58 periods together and the constellation made
00:14:58 --> 00:15:00 over 355
00:15:00 --> 00:15:03 dodges in 12 months. More
00:15:03 --> 00:15:05 than triple what it performed in all of
00:15:05 --> 00:15:08 2024. At uh, on average,
00:15:08 --> 00:15:11 each Starlink satellite now swerves more
00:15:11 --> 00:15:14 than 40 times a year. That's nearly a
00:15:14 --> 00:15:16 dodge a week per satellite.
00:15:16 --> 00:15:18 Anna: Let's be fair to SpaceX for a moment though.
00:15:19 --> 00:15:21 These maneuvers are the system working as
00:15:21 --> 00:15:22 designed, aren't they?
00:15:22 --> 00:15:24 Avery: They are. The satellites dodge
00:15:24 --> 00:15:27 autonomously whenever the predicted collision
00:15:27 --> 00:15:30 probability exceeds 3 in 10 million,
00:15:30 --> 00:15:33 an extremely conservative threshold, far
00:15:33 --> 00:15:36 tighter than the industry standard. Experts
00:15:36 --> 00:15:38 consistently credit SpaceX with managing its
00:15:38 --> 00:15:41 traffic well and being transparent with the
00:15:41 --> 00:15:44 data. The concern is the trendline,
00:15:44 --> 00:15:45 not the competence.
00:15:45 --> 00:15:47 Anna: Because the numbers compound. More
00:15:47 --> 00:15:50 satellites means more close approaches means
00:15:50 --> 00:15:53 more maneuvers means more residual risk
00:15:53 --> 00:15:55 that never quite goes to zero.
00:15:55 --> 00:15:58 Avery: Exactly the point Huw Lewis makes. He's the
00:15:58 --> 00:16:00 University of Birmingham um, astronautics
00:16:00 --> 00:16:02 professor who's tracked these reports for
00:16:02 --> 00:16:05 years. Each maneuver cuts the collision odds
00:16:05 --> 00:16:08 to about one in a million, which sounds
00:16:08 --> 00:16:11 negligible, but as he puts it, if you make
00:16:11 --> 00:16:13 a million maneuvers with a one in a million
00:16:13 --> 00:16:16 residual, you end up with an aggregate risk
00:16:16 --> 00:16:18 across the Constellation that you simply
00:16:18 --> 00:16:21 can't get rid of. His blunt assessment,
00:16:21 --> 00:16:23 he thinks we're heading towards a situation
00:16:23 --> 00:16:26 where there will be a collision involving an
00:16:26 --> 00:16:28 operational satellite in the Constellation.
00:16:29 --> 00:16:32 Avery: And the projections on current growth
00:16:32 --> 00:16:35 Starlink passes. A million total avoidance
00:16:35 --> 00:16:37 maneuvers by mid2027. And by
00:16:37 --> 00:16:40 2030 the constellation could be making more
00:16:40 --> 00:16:42 than a million maneuvers every single year.
00:16:43 --> 00:16:46 Remember too, and regular listeners will.
00:16:46 --> 00:16:49 SpaceX has applied to the FCC to grow
00:16:49 --> 00:16:51 Starlink toward 100 satellites,
00:16:51 --> 00:16:53 a story we covered a couple of weeks back.
00:16:54 --> 00:16:56 And it's not alone up there. Amazon's
00:16:56 --> 00:16:58 Constellation and China's Qian Fan are
00:16:58 --> 00:17:00 actively deploying as well.
00:17:00 --> 00:17:03 Anna: The number of operational spacecraft in orbit
00:17:03 --> 00:17:05 has gone from about 10 to about
00:17:05 --> 00:17:08 16 in just a year. Other
00:17:08 --> 00:17:10 experts are calling for operators to disclose
00:17:10 --> 00:17:12 predicted maneuver counts before
00:17:12 --> 00:17:15 Constellations are even approved. Though
00:17:15 --> 00:17:17 regulators know whether the satellites can
00:17:17 --> 00:17:19 Avery: actually keep up, low Earth orbit is a
00:17:19 --> 00:17:22 shared resource. And this is the traffic
00:17:22 --> 00:17:24 report. We'll keep watching the numbers
00:17:24 --> 00:17:27 because everyone from astronomers to airlines
00:17:27 --> 00:17:29 to your GPs depends on that neighborhood
00:17:29 --> 00:17:30 staying safe.
00:17:30 --> 00:17:33 Anna: Time now for tonight's skywatching. And for
00:17:33 --> 00:17:35 our Southern Hemisphere friends, the news is
00:17:35 --> 00:17:38 good. The Moon is a waning crescent rising in
00:17:38 --> 00:17:40 the small hours, so evenings this week are
00:17:40 --> 00:17:43 dark and glorious, which means
00:17:43 --> 00:17:46 Avery: the winter Milky Way at its absolute best
00:17:46 --> 00:17:48 face south after dinner. And the galactic
00:17:48 --> 00:17:51 core in Sagittarius and Scorpius is almost
00:17:51 --> 00:17:54 directly overhead from most of Australia and
00:17:54 --> 00:17:57 New Zealand dust lanes. Star clouds, the
00:17:57 --> 00:17:59 lot. If you can get away from city lights
00:17:59 --> 00:18:01 this week, do it while you're there.
00:18:01 --> 00:18:04 Anna: Sweep up Omega, uh, Centauri and the Southern
00:18:04 --> 00:18:06 Cross riding high. And if you've got
00:18:06 --> 00:18:08 binoculars, the star fields between
00:18:08 --> 00:18:11 Scorpius's tail and the teapot of Sagittarius
00:18:11 --> 00:18:14 will keep you busy all evening. Saturn
00:18:14 --> 00:18:16 is climbing in the east by mid evening for a
00:18:16 --> 00:18:18 late night treat. And dazzling Venus still
00:18:18 --> 00:18:21 rules the early evening western sky.
00:18:21 --> 00:18:24 Avery: And one for the launch watchers. SpaceX's
00:18:24 --> 00:18:27 Starship Flight 13 window opens tonight,
00:18:27 --> 00:18:29 US time. That's tomorrow morning for us
00:18:30 --> 00:18:32 from about 8:45 aesthetic.
00:18:33 --> 00:18:35 So pour a coffee and watch this space. We'll
00:18:35 --> 00:18:37 have the full story in Saturday's weekend
00:18:37 --> 00:18:38 wrap.
00:18:38 --> 00:18:40 Anna: That's it for today's episode. Thanks for
00:18:40 --> 00:18:43 joining us. You can find show notes, links to
00:18:43 --> 00:18:45 every story and our back catalog@ah,
00:18:46 --> 00:18:48 astronomydaily.IO and we're astronomy
00:18:48 --> 00:18:50 Daily Pod on all the socials.
00:18:51 --> 00:18:53 Avery: Astronomy Daily is part of the bytes.com
00:18:53 --> 00:18:55 podcast network. I'm um, Avery.
00:18:55 --> 00:18:58 Anna: And I'm Anna. We'll see you tomorrow. Until
00:18:58 --> 00:19:00 then, clear skies.

