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Anna: Welcome to Astronomy Daily, your daily dose

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of space and astronomy news. I'm Anna.

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Avery: And I'm, um, avery. It's Thursday, the 16th

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of July, 2026, and we have a

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genuinely lovely lineup for you today,

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including a story that's been 10 years in the

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making, or more accurately, 10 years in the

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hiding.

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Anna: That's Our lead astronomers have finally

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caught a planet that's been playing hide and

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seek with them for over a decade. And it

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turns out to be the faintest exoplanet ever

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imaged from Earth. And it lives in a southern

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constellation, which makes it feel just a

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little bit like ours.

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Avery: We've also got the completion of a nine year

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project to build the sharpest radio map of

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the entire sky. And the James Webb Space

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Telescope catching a supermassive black hole

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in the act of feeding itself.

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Anna: Then it's a double bill from the outer solar

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system. Landslides on Pluto spotted for

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the first time, and evidence that Pluto's big

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moon, Charon, once spun more than 10

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times faster than it does today.

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Avery: And we'll wrap the news with some sobering

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numbers. SpaceX's Starlink satellites had

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to dodge potential collisions more than

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355,000 times

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in the past year. We'll unpack what that

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means for everyone's

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Anna: orbit, plus your Southern hemisphere sky

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watching for tonight. Let's get into it.

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Avery, cast your mind.

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Back in 2008, astronomers

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directly imaged a planet around the young

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star Beta Pictoris, one of the very first

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exoplanets ever photographed. That was

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Beta Pictoris B. A second planet

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C followed. And ever since, there's been a,

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uh, nagging suspicion that the system was

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hiding

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Avery: something more because of the disk. Right.

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Beta Pictoris has this magnificent debris,

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uh, disk. It's the poster child for planet

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formation. And parts of it were warped and

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sculpted in ways that two known planets

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couldn't fully explain.

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Anna: Exactly. And now we know why. In a

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study published Wednesday in the

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Astrophysical Journal Letters, a team using

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the European Southern Observatory's Very

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Large Telescope in Chile has confirmed a

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third planet, Beta Pictoris D.

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And here's the headline. It's roughly

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100 times fainter than Beta Pictoris

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B, which makes it the faintest exoplanet

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ever directly imaged from Earth.

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Avery: A hundred times fainter. To put that in

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context for everyone, direct imaging means

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actually capturing the planet's own light in

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a photograph next to a star that's

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overwhelmingly brighter. It's often compared

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to spotting a firefly next to a lighthouse.

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This is spotting a very Dim

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firefly.

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Anna: And the discovery itself was serendipitous.

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Ben Sutliff at the University of Edinburgh

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who co led the study, said they were

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originally just going back to study the known

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planet Beta Pictoris B to see how it

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changed over time. But in their new images

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from the VLT's Eris instrument, there was

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something else. A faint point of light

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separated from Planet B that sent them down

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an entirely new path.

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Avery: And this is where the hide and seek comes in.

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Once they knew what to look for, they trawled

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back through the archives. And there it was,

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lurking. In more than a decade of old

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observations from the VLT SPEAR instrument

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and even in James Webb Space Telescope data,

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the planet had been photographed for years.

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Nobody had noticed.

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Anna: Co author Jane Burkeby at Oxford put it

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beautifully. Planet D has been playing hide

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and seek with us for over a decade and now

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we can say found you.

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Avery: So what do we know about the world itself?

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Anna: It's a gas giant about 2.4 times

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the mass of Jupiter, which sounds big, but

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is actually the lightweight of the family.

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Planets B and c are each 10 Jupiter

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masses. Planet D sits, um, much further out

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from the star on a wide orbit, so it's cooler

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and dimmer than its siblings, hence the

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difficulty. And satisfyingly, its

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presence helps explain that odd structure in

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the debris disk that's puzzled astronomers

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for years.

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Avery: There's also a nice milestone tucked in here.

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This makes Beta Pictoris only the second

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planetary system after HR

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8799, where more than two

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planets have been directly. We're building

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up actual family portraits of other solar

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systems now.

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Anna: And an independent team at the University of

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California spotted the same object in their

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own data at almost the same time, which gives

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the detection real confidence. Now the

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bit our audience will love. Beta Pictoris is

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a southern star. It sits in the constellation

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Pictor, the Painter's Easel, just next to

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brilliant canopus. And at 63 light

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years away, it's visible from Australia and

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New Zealand. Though right now in July

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it's low in our evening sky and best hunted

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in the pre dawn hours later in

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Avery: the year, a planetary system with three

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photographed worlds sitting in our southern

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sky. Not bad at all.

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Next, A, uh, project nine years in the

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making has just crossed the finish line. The

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U.S. national Science Foundation's National

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Radio Astronomy Observatory has announced

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that observations for the Very Large Array

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Sky Survey VLAS are

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complete. It's the most detailed radio

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survey of the sky ever conducted.

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Anna: This is the VLA in New Mexico. The

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iconic Y shaped array of 27 dishes

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from every space documentary ever made.

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Avery: That's the one. From September 2017

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through February this year, the array

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repeatedly swept about 34,000

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square degrees. Essentially the whole sky

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visible from New Mexico and everything north

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of minus 40 degrees declination.

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That's roughly 80% of the entire

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celestial sphere. Mapped at a resolution

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of about 2 and a half arcseconds in the 2

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to 4 GHz band.

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Anna: And how does that compare to what came

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before?

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Avery: It's about 18 times sharper than the

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previous benchmark all sky radio survey from

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the 1990s. The numbers are

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staggering. Roughly six and a half thousand

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thousand observing hours. Half a petabyte of

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raw data. And the processed data products are

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expected to reach around 2 petabytes, the

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largest data volume the VLA has ever

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produced. They use a clever on the fly

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mosaicing technique where the antennas sweep

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continuously across the sky in a raster

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pattern rather than stopping to point at each

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field.

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Anna: And crucially, they surveyed the sky multiple

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times over those nine years. Which means VLAS

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isn't just a map, it's a movie. Comparing

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epochs revealed a dynamic radio sky.

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Sources that flare, fade or appear from

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nowhere. Exploding stars, feeding black

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holes, colliding neutron stars.

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Avery: Which brings us to the timing. And honestly,

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the timing is the best part of the story.

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Just over two weeks ago on June 30, the

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Vera C. Rubin Observatory in Chile began

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its decade long legacy survey of space and

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time, sweeping the southern optical sky

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every few nights. So for the first time in

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history, we have a complete high resolution

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radio map and a real time optical

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transient stream operating simultaneously.

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Anna: Though when Rubin flags something going bang

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in the optical, astronomers can immediately

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check what that patch of sky looks like and

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looked like in the radio. The whole multi

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wavelength discovery machine the community

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has spent two decades building is now

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switched on and the data's public.

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Avery: Radio astronomers, multi wavelength folks,

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citizen scientists. The radio sky now

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belongs to everyone.

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Anna: Now to a decades old mystery that may

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finally have its answer. Avery, how do

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supermassive black holes keep feeding?

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Nearly every large galaxy hosts one of these

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monsters. Millions or billions of times the

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mass of the Sun. When they feed, they blast

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out enormous energy, powerful jets that heat

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the gas around them. And that's the paradox.

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That heating should cut off the black hole's

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own fuel supply. So why don't they starve?

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Avery: The leading idea has been a kind of cosmic

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recycling loop. The heated gas eventually

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cools back down, condenses into long thin

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streamers called filaments and rains back

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towards the center. Self regulating

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but Actually seeing the connection filament

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to black hole has eluded astronomers for

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decades.

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Anna: Until now. An international team led by Julie

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Hvlasic Lorando at the University of Montreal

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pointed the James Webb Space telescope at

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NGC 4696, the giant

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elliptical galaxy at the heart of the

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Centaurus cluster, about 145

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million light years away. Their results were

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published this week in the Astrophysical

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Journal Letters.

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Avery: And Centaurus, we should note, is a southern

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constellation. This galaxy cluster rides high

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in our winter sky right now, though you'll

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need a decent telescope for the galaxy

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itself.

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Anna: White. Now, Hubble had previously

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photographed a curious S shaped swirl of gas

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near this galaxy's central black hole. But

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Hubble could only show where the gas sat, not

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how it moved. So the team gave Webb's

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NIRSP instrument nearly eight hours on the

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target and mapped the motion of the gas deep

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inside the black hole's sphere of influence,

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resolving features just 30 light years across

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in a galaxy hundreds of thousands of light

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years wide.

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Avery: And the swirl turned out to be

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Anna: a spinning disk of gas wrapped around

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the black hole, nearly 800 light

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years across, with material whipping around

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at, uh, up to 600 kilometers per second.

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And here's the money shot. That disk is

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physically connected to one of the huge

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infalling filaments stretching out into the

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galaxy. They watched gas flowing along

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the filament, pouring into the disk, and from

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the disk falling onto the black hole.

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Avery: The missing link caught on camera heat the

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gas. The gas cools into filaments. The

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filaments feed the disk. The disk feeds the

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black hole. The black hole heats the gas.

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Round and round it goes.

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Anna: Havlasic Lorando said Webb is revealing that

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black holes might be the ultimate cosmic

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recyclers. And because this feeding loop

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shapes when galaxies can and can't form

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stars, understanding it is really

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understanding how galaxies, including ours,

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grow up.

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Avery: Anna, uh, time for a double bill from the

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outer solar system. Two stories,

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one spacecraft, and a dwarf planet that

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keeps on giving. First,

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scientists have detected landslides on Pluto

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for the very first time.

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Anna: This is New Horizons data, isn't it? That

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Flyby was 11 years ago this week.

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Avery: It is, and that's the delightful part. A

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paper in the journal Icarus, which has been

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making headlines this week, reports that an

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international team went back through the high

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resolution images from New Horizons lorry

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camera pictures showing Pluto's surface at

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about 300 meters per pixel and found

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six large landslides inside three impact

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craters near Sputnik Planita. That famous

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heart shaped nitrogen ice plane.

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Anna: How do you recognize a landslide on a world

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made of ice?

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Avery: Same fingerprints as Earth. Crescent shaped

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collapse scars near the crater rims. Huge

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displaced blocks of ice and debris fanning

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out across the crater floors. The team

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measured them. These slides descend one and a

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half to over two kilometers, run out as far

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as 14 and a half kilometers and the largest

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covers around 130 square kilometers.

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Anna: And landslides are everywhere else, aren't

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they? Earth, Mars, Ceres,

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asteroids, even Pluto's moon Charon showed

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evidence years ago Pluto itself was the odd

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one out which was

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Avery: genuinely puzzling because Pluto has steep

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crater walls and rugged icy terrain. All the

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right ingredients. Now the gap is filled and

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it tells us gravity driven slope processes

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are actively reshaping Pluto's frozen

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surface. Even under gravity, a fraction of

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ours. What triggered them is still open.

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Possibilities range from tectonic activity to

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meteoroid impacts.

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Anna: A world we visited for a few hours in 2015,

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still handing us firsts a decade later.

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Avery: And um, it's not done because part two of

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our Pluto double is about

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Avery: the other half of that famous pair

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Anna: of Charon, Pluto's enormous moon. So

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big relative to Pluto that the two really

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form a double world. And a study published

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Tuesday in Nature Communications says

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Charon's mountains have preserved a memory of

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a wilder youth.

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Avery: What kind of memory?

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Anna: A record of despinning across the solar

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system. Tidal forces gradually slow a body's

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rotation and as ah, the spin slows the

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body's shape relaxes stressing and

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cracking the surface. The it's long been

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theorized for Charon but clear geological

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evidence was missing. So Han, Zeng Chin

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and colleagues at ETH Zurich and

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UCLA examined the orientations

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and types of tectonic features, mountain

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ranges and faults in Aus Terra

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Sharon's northern rugged highlands. Again

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using New Horizons flyby data.

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Avery: And um, the tectonic pattern fits the de

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spinning story beautifully.

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Anna: Their modeling suggests Charon's rotation

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period was once around 14.3 hours

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and it has since slowed to today's roughly

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153 hours locked in step with

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its orbit around Pluto. That's more than a

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tenfold slowdown and the stresses from that

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transformation are etched into the mountains

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we photographed in 2015.

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Avery: Chen said the study drastically changed her

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understanding of Charon's geologic history.

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And there's a bonus finding, isn't there

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about how Charon was born?

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Anna: Yes, the way despinning and global

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contraction evolved together favors

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what's called a cold start for Charon, which

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is a real clue to the early thermal history

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of icy moons across the Outer solar system.

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So between Pluto's landslides and charon's

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slowing spin, one 11 year old dataset

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gave us two papers in a week. Not a bad

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return on a flyby.

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Avery: Our final story today, Anna, uh, comes with

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some genuinely eye widening numbers.

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SpaceX has filed its latest semi annual

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constellation status report with the U.S.

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federal Communications Commission. And

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according to coverage of the filing, StarLink

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satellites performed

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207,152

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collision avoidance maneuvers between

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December 2025 and

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May 2026.

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Anna: 207,000 in six months,

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up nearly 60,000

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Avery: on the previous half year. Put the two

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periods together and the constellation made

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over 355,000

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dodges in 12 months. More

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than triple what it performed in all of

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2024. At uh, on average,

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each Starlink satellite now swerves more

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than 40 times a year. That's nearly a

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dodge a week per satellite.

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Anna: Let's be fair to SpaceX for a moment though.

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These maneuvers are the system working as

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designed, aren't they?

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Avery: They are. The satellites dodge

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autonomously whenever the predicted collision

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probability exceeds 3 in 10 million,

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an extremely conservative threshold, far

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tighter than the industry standard. Experts

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consistently credit SpaceX with managing its

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traffic well and being transparent with the

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data. The concern is the trendline,

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not the competence.

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Anna: Because the numbers compound. More

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satellites means more close approaches means

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more maneuvers means more residual risk

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that never quite goes to zero.

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Avery: Exactly the point Huw Lewis makes. He's the

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University of Birmingham um, astronautics

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professor who's tracked these reports for

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years. Each maneuver cuts the collision odds

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to about one in a million, which sounds

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negligible, but as he puts it, if you make

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a million maneuvers with a one in a million

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residual, you end up with an aggregate risk

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across the Constellation that you simply

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can't get rid of. His blunt assessment,

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he thinks we're heading towards a situation

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where there will be a collision involving an

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operational satellite in the Constellation.

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Avery: And the projections on current growth

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Starlink passes. A million total avoidance

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maneuvers by mid2027. And by

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2030 the constellation could be making more

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than a million maneuvers every single year.

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Remember too, and regular listeners will.

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SpaceX has applied to the FCC to grow

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Starlink toward 100,000 satellites,

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a story we covered a couple of weeks back.

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And it's not alone up there. Amazon's

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Constellation and China's Qian Fan are

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actively deploying as well.

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Anna: The number of operational spacecraft in orbit

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has gone from about 10,000 to about

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16,000 in just a year. Other

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experts are calling for operators to disclose

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predicted maneuver counts before

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Constellations are even approved. Though

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regulators know whether the satellites can

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Avery: actually keep up, low Earth orbit is a

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shared resource. And this is the traffic

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report. We'll keep watching the numbers

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because everyone from astronomers to airlines

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to your GPs depends on that neighborhood

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staying safe.

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Anna: Time now for tonight's skywatching. And for

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our Southern Hemisphere friends, the news is

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good. The Moon is a waning crescent rising in

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the small hours, so evenings this week are

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dark and glorious, which means

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Avery: the winter Milky Way at its absolute best

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face south after dinner. And the galactic

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core in Sagittarius and Scorpius is almost

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directly overhead from most of Australia and

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New Zealand dust lanes. Star clouds, the

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lot. If you can get away from city lights

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this week, do it while you're there.

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Anna: Sweep up Omega, uh, Centauri and the Southern

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Cross riding high. And if you've got

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00:18:06.300 --> 00:18:08.340
binoculars, the star fields between

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Scorpius's tail and the teapot of Sagittarius

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will keep you busy all evening. Saturn

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is climbing in the east by mid evening for a

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late night treat. And dazzling Venus still

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rules the early evening western sky.

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Avery: And one for the launch watchers. SpaceX's

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Starship Flight 13 window opens tonight,

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US time. That's tomorrow morning for us

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from about 8:45 aesthetic.

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So pour a coffee and watch this space. We'll

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have the full story in Saturday's weekend

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wrap.

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Anna: That's it for today's episode. Thanks for

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00:18:40.460 --> 00:18:43.140
joining us. You can find show notes, links to

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00:18:43.140 --> 00:18:45.818
every story and our back catalog@ah,

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00:18:46.102 --> 00:18:48.939
astronomydaily.IO and we're astronomy

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00:18:48.939 --> 00:18:50.740
Daily Pod on all the socials.

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00:18:51.140 --> 00:18:53.780
Avery: Astronomy Daily is part of the bytes.com

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00:18:53.860 --> 00:18:55.780
podcast network. I'm um, Avery.

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Anna: And I'm Anna. We'll see you tomorrow. Until

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then, clear skies.
