July 29, 2026

Betelgeuse Is Not Alone!

Betelgeuse Is Not Alone!
Astronomy Daily · S05E153 · Wednesday 29 July 2026. Four stories from the frontier of space and astronomy, plus a both-hemispheres look at the sky — and news of our brand-new website. In this episode • Betelgeuse is not alone. ESO’s VLT/SPHERE has captured the clearest direct image yet of Betelgeuse B, the long-suspected companion to the famous red supergiant — ending a roughly century-long search. Published 28 July 2026 in Astronomy & Astrophysics (Montargès, Boccaletti et al.). The companion is more massive than predicted (≈2–3 solar masses), likely paces Betelgeuse’s ~6-year brightness cycle, and may eventually spiral into the supergiant. • Swift catches a wandering black hole. TDE 2025abcr — the most off-centre tidal disruption event ever seen — reveals a ~1-million-solar-mass “wandering” black hole ~30,000 light-years from its galaxy’s core, ~750 million light-years away. First flagged by the Zwicky Transient Facility (Nov 2025) and pinned down with NASA’s Swift; an AI sifted ~500,000 nightly flashes to find it. Published 27 July 2026 in The Astrophysical Journal Letters (Stein et al.; Carney et al.). • Roman is fuelled for launch. NASA’s Nancy Grace Roman Space Telescope completed fuelling on 25 July (≈290 gallons of hydrazine) and holds its mission-preview briefing today — one month from a 30 August launch, roughly eight months ahead of schedule. Roman will survey ~50× as much sky as Hubble in five years, probe dark energy, and is expected to find 100,000+ exoplanets via microlensing. • Swift’s rescue mission is in trouble. Katalyst’s LINK servicing spacecraft — launched 3 July to boost the decaying Swift observatory — began spinning over the weekend; two of three reaction wheels are non-operable, with some cold-gas thruster degradation. LINK remains powered and in contact; the team is using its electric (xenon) thrusters to arrest the spin before deciding, with NASA, whether to proceed. Developing story — details accurate as of recording. • Skywatch. Full Buck Moon tonight (29 July); Jupiter at solar conjunction; Southern Delta Aquariids favour the Southern Hemisphere but are washed out by the Moon this year; Alpha Capricornid fireballs are the pick for both hemispheres; the Perseids peak on the moonless night of 12–13 August alongside a total solar eclipse (Greenland/Iceland/Spain; partial for parts of Europe and North America). Never view the partial phases without ISO 12312-2 eclipse glasses. Sources • ESO release eso2611 & Astronomy & Astrophysics, Montargès, Boccaletti et al., “VLT/SPHERE imaging of the candidate companion of Betelgeuse” (28 Jul 2026). • NASA Swift / The Astrophysical Journal Letters — TDE 2025abcr wandering-black-hole discovery (27 Jul 2026); UNC-Chapel Hill release. • NASA — Nancy Grace Roman Space Telescope fuelling & launch-preview updates (25–29 Jul 2026). • NASA Swift blog — “Commissioning Update for Spacecraft to Boost NASA’s Swift” (28 Jul 2026); Katalyst Space Technologies. • EarthSky, NASA, American Meteor Society, timeanddate — meteor showers, Buck Moon, Jupiter conjunction, 12 Aug eclipse. New — astronomydaily.io Our new website is live: full back catalogue, a continuously-updating space-news feed, listener reviews (read and leave your own), and a daily newsletter sign-up. Got a question or a story tip? Drop us a note — and tell us what you think of the new site.

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This episode includes AI-generated content.
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Avery: One of the most famous stars in the whole

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night sky has been keeping a secret for about

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100 years.

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Anna: And this week, a telescope in the Chilean

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desert finally caught it red handed.

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Betelgeuse, it turns out, is not alone.

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Avery: Also ahead, a black hole caught wandering the

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lonely outskirts of a galaxy dreading a

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star tens of thousands of light years from

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where any black hole has a right to be.

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Anna: NASA's next great observatory gets its tank

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filled and a date on the calendar.

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Avery: And the little spacecraft sent to rescue an

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aging telescope suddenly needs rescuing

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itself. G', day, and welcome to Astronomy

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Daily, your daily dose of space and astronomy

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news. I'm Avery.

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Anna: And I'm, um, anna. It's Wednesday, the 29th

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of July, four stories and a look at the sky

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from both hemispheres. Let's get into it.

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If you've ever looked up at Orion, and from

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Sydney or Seattle, just about everyone has,

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you've seen tonight's star Betelgeuse,

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that deep orange point marking the hunter's

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shoulder. It's a red supergiant, roughly

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650 light years away, and it is

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enormous. Drop it where our sun sits and it

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would swallow the orbit of Jupiter.

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Avery: And it's famous for misbehaving. It

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flickers.

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Anna: It does. Betelgeuse brightens and dims on

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a whole set of overlapping cycles. And people

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have been writing that down for more than a

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thousand years. But there's one rhythm, um,

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in particular, a slow beat about six years

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long that astronomers have never been able to

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fully explain. And for almost a century,

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one idea kept coming back. What if

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Betelgeuse has a companion, a second star,

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orbiting close, tugging on it?

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Avery: The famous Betel Buddy.

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Anna: That's the affectionate nickname, yes. The

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trouble is nobody had ever seen it. And you

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can see why. Imagine trying to spot a

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candle sitting right next to a lighthouse.

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Betelgeuse is so blindingly bright and so

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physically huge that any little companion

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tucked in beside it just drowns in the glare.

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For a hundred years, it stayed a hypothesis.

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Avery: So what changed?

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Anna: A team led by Miguel Montargis at the Paris

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Observatory in Chile, the vlt,

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and an instrument called Sphere that's built

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for exactly this job. Blocking out a bright

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star to hunt for faint things right beside

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it. And crucially, they picked their moment.

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They observed in December 2024, at the

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point in the orbit when the companion was

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predicted to swing out as far from Betelgeuse

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as it ever gets from seen from Earth. Best

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possible chance to split the two apart. And

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there it was. A faint little source right

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Where a companion should be. Their paper

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landed yesterday, 28th July in the journal

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Astronomy and Astrophysics. And Montargis

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called it the end of a century long quest.

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After a hundred years of arguing about it, we

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have a direct image of what is very likely

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Betelgeuse B.

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Avery: That gives me chills, honestly. A star that

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people have watched since antiquity and we're

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still learning brand new things about it.

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Anna: And here's the lovely twist. The reason they

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could see it at all is that it surprised

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them. The companion was predicted to be

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roughly the mass of our Sun. But the data

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say it's bigger than that, something like two

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to three times the Sun's mass. Montargis put

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it beautifully, because it's more massive

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than we expected, it's brighter than we

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expected, and that's the only reason it

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peeked out of the glare. If it had been as

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small as the textbook said, they might have

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missed it entirely.

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Avery: So the companion did us a favor by being

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chunkier than advertised. What is it though?

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Another supergiant?

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Anna: No, nothing like Betelgeuse. Think of it as

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a young, hot, fairly ordinary star,

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but locked in a very awkward orbit.

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It appears to circle so close that it's

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essentially skimming through the outer puffed

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up layers of the supergiant. And that has

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consequences. That orbit is almost

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certainly what paces that mysterious M6

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year brightness cycle. But it's also most

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likely a death sentence for the companion.

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Avery: Ooh, M. Go on.

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Anna: Plowing through a supergiant's outer

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atmosphere means constant drag. Every

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orbit, the little star loses a bit of energy.

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And models suggest it's slowly spiraling

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inward on astronomical timescales.

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Betelgeuse is very likely to swallow its

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own companion. Not tomorrow. We're talking

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thousands of years. But the relationship is,

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let's say, not built to last.

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Avery: The lighthouse eats the candle.

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Anna: Eventually, yes. And this matters for the big

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question everyone actually wants answered

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about Betelgeuse. When is it going to

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explode? Because it will. It's an old

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massive star, near the end of its life, and

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one day it will go supernova and briefly

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outshine everything in the night sky. Now,

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before anyone emails us, that's expected on a

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timescale of up to 100,000 years.

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So don't cancel your weekend. But whether a

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star has a close binary companion

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changes the whole picture. How it sheds mass,

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the shape of the gas around it, even the

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choreography of the explosion when it finally

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comes. Knowing Betelgeuse is a pear

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rewrites part of that story.

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Avery: And this was direct imaging. An actual

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Picture not just an inference from wobbles in

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the light.

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Anna: That's what makes it land. There had been

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circumstantial hints for years, but this is a

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direct detection light caught from the

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companion itself in the right place at the

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right time. It's the difference between the

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data suggest a second star and here

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it is.

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Avery: So if you want to go and look at the star at

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the center of all this, Betelgeuse itself.

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Where are we? Both hemispheres right now?

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Anna: Orion is a pre dawn act. It's climbing

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back into the morning sky after being lost in

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the sun's glare. For our Southern hemisphere

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listeners, Orion rides high in the northern

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part of the early morning sky. And it's

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upside down compared to the northern view.

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Look for Betelgeuse as the bright orange star

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from North America and mid northern

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latitudes. It's lower in the east southeast

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before dawn, climbing higher each week. As we

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head towards the northern winter, we'll come

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back to it properly in the sky watch. But

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next time you find it, just remember it's not

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one star. It never was.

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Avery: Now from a star that's hiding a companion to

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a black hole that was hiding full stop.

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Anna, picture, uh, a supermassive black hole.

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Where is it?

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Anna: Dead center of a galaxy. That's the rule. The

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big ones sit in the core.

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Avery: That's the rule. And this week, NASA's Swift

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observatory helped break it. Astronomers

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announced a tidal disruption event. That's

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the technical name for a black hole tearing a

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star apart and eating it. And the flare it

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produced was blazing briefly outshining its

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entire host galaxy in ultraviolet. Like

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10 billion suns switched on at once. But

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here's the thing. It didn't happen in the

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middle of the galaxy. It went off about

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30,000 light years out from the core.

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Anna: 30,000. That's not a rounding error.

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That's further from the center than the sun

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is from the middle of the Milky Way. That

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black hole is out in the suburbs.

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Avery: Way out in the suburbs. The event's called

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TDE 2025 ABCR

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in a Galaxy about 750 million light

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years away. And the teams one led out of

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NASA and the University of Maryland, another

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from UNC Chapel Hill, published it on

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27 July in the Astrophysical Journal

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Letters. It's the most off center tidal

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disruption ever seen. And what it reveals is

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a wandering black hole, a around a million

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times the mass of the sun, just roaming

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through its galaxy, nowhere near the core.

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Anna: How does a black hole end up out there? They

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don't exactly stroll.

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Avery: Best guess is a, uh, galaxy merger. When two

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galaxies collide and their central black

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holes get thrown together, one can get kicked

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out of the middle and left drifting.

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Theorists have predicted these wanderers for

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years. The problem is they're invisible. A

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black hole sitting quietly in the dark emits

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no light. You only ever attach one if it does

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something dramatic.

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Anna: Like grabbing a passing star and lighting up.

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Avery: Exactly. The star is the flashbulb. It

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wanders too close, gets shredded, and for a

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few weeks, the wreckage glows and gives the

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whole thing away. That's the only reason we

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know this black hole is there at all.

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Anna: And there's a lovely modern wrinkle to how

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they found it isn't there. This wasn't a

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human squinting at plates.

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Avery: Not a chance. The sky is too big for that

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now. The initial flare was picked up back in

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November 2025 by a survey at Palo are

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in California that scans the whole northern

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sky every couple of nights. It throws up

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something like half a million flashes every

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single night. So the team trained an AI to

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sift that fire hose and flag the ones that

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look like a tidal disruption. And it caught

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this one precisely because it was in a weird

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place off in the outskirts where nobody would

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have thought to look. Swift followed up to

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nail down the details.

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Anna: And that's the taste of what's coming, right?

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Once the big new survey telescopes are

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running.

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Avery: That's the real headline. Under the headline,

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with observatories like the Vera Rubin

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Observatory and UNC's Argus array coming

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online, we go from finding a handful of these

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a year to potentially hundreds or thousands.

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And suddenly all those invisible wandering

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black holes become findable. We're about to

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start taking a census of the galaxy's hidden

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monsters. And keep swip in mind, by the

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Anna: way, because it's going to come back to bite

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us later in the show.

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Avery: It is. Hold that thought.

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Anna: Speaking of survey telescopes about to change

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the game, let's talk about one that's now

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genuinely nearly on the

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NASA's Nancy Grace Roman Space

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Telescope, because as of this week, it is

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fueled and counting down.

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Avery: Fueled. That's a real milestone. That's not a

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slide in a presentation. That's propellant in

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the tank.

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Anna: Precisely. On the 25th of July,

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teams at, uh, Kennedy loaded around

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290 gallons of hydrazine into

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the observatory. That's the fuel it'll use to

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hold its position and point with real

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precision once it's out there. And NASA is

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holding its big mission preview briefing

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today, exactly one month out from launch.

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The date to circle is the 30th of August

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and remarkably, that's about eight months

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ahead of the original schedule.

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Avery: A NASA flagship running early and as

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I understand it, on budget. Let the record

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show it can be done.

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Anna: It can. And here's why Roman is worth

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the excitement. Think of it as a telescope

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with Hubble quality sharpness, but a jaw

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droppingly wide field of view. Something like

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a hundred times the patch of sky Hubble sees

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in a single shot. Bass estimate is that in

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its first five years, it could image more

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than 50 times as much sky as Hubble has

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in 30. It's built to survey fast and

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wide.

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Avery: And what's that actually hunting?

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Anna: Two headline jobs. One, dark Energy,

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the mystery. Pushing the universe apart

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faster and faster. Roman will map how

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cosmic structure has grown over billions of

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years to pin down what Dark Energy is

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actually doing. And two, this is the one

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I love. It's an exoplanet machine.

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Using a trick called microlensing, Roman

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is expected to find more than 100,000

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new planets and to catch hundreds of others

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in the very act of finding forming around

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young stars.

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Avery: 100,000. We do a story

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most weeks about one interesting new planet

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and Roman's going to hand us 100,000.

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Anna: It really might reset the whole field.

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And this is genuinely for everyone listening

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wherever you are. It's a space telescope,

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though there's no hemisphere that misses out.

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The whole planet shares this one. One

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month to go.

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Avery: Fingers crossed for the 30th of August.

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Right? I told you Swift would come back

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around. In story two, Swift was the hero,

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the observatory that helped us catch that

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wandering black hole. Well, here's the

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thing in the tale, Swift itself is in

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trouble and the spacecraft sent to save it

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is now in trouble too.

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Anna: Set it up. Why does Swift need saving in

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the first place?

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Avery: Because Swift is falling. It's a fantastic

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gamma ray and X ray observatory that's been

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working since 2004. But it has no

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engine of its own, no way to boost its own

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orbit, and its orbit has been decaying faster

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than expected, partly because heightened

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solar activity puffs up the upper atmosphere

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and increases the drag. Left alone,

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Swift is looking at an uncontrolled re entry

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by around the end of this year.

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Anna: So it burns up unless someone

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goes up and gives it a push.

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Avery: Which is exactly the plan. A company called

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Catalyst Space Technologies built a

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robotics servicing spacecraft named Link.

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And NASA hired them for what its own mission

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director called a fast, high risk, high

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reward rescue. Link launched on 3

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July, and the goal is genuinely a first

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to fly up, grab hold of Swift, a

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satellite that was never designed to be

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docked with or serviced and physically

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boosted into a higher, safer orbit.

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Nobody has ever commercially docked with a

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government spacecraft that wasn't built for

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it.

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Anna: That's ambitious. So what's gone wrong?

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Avery: Over the weekend, Link ran into an attitude

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control problem and started spinning with its

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communications dropping in and out. According

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to NASA's update, and I want to be precise

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here because this is developing, the

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preliminary finding is that two of Link's

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three reaction wheels are no longer working

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and, and there's some loss of function in its

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cold gas thruster system as well.

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Anna: Reaction wheels, Those are the spinning

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wheels inside a spacecraft that let it turn

335
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and hold steady without using fuel.

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Lose those and you lose fine control of which

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way you're pointing.

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Avery: That's the one. And losing two of three is

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serious, especially because there was already

340
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a wobble with one Wheel earlier in

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commissioning that they patched in software.

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The good news, Link is not lost. It's still

343
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powered, still in contact, and its other

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major systems are behaving. The team's plan

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00:14:20.000 --> 00:14:22.360
is to use Link's electric thrusters, its

346
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xenon propulsion, to stop the spin over the

347
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next few days, then re establish stable

348
00:14:27.880 --> 00:14:30.200
pointing, update the spacecraft's guidance

349
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and navigation to work around the dead

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hardware, and only then sit, uh, down with

351
00:14:34.920 --> 00:14:37.080
NASA and decide whether it's still safe to

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attempt the approach and capture of Swift.

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Anna: So the rescue isn't canceled, it's on

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hold while they figure out if the rescuer can

355
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still do the job.

356
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Avery: That's exactly it. And I'll flag for

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everyone. This is a life situation as of when

358
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we're recording. By the time you hear this,

359
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the team may already have stopped a spin or

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the picture may have changed again. But step

361
00:14:59.470 --> 00:15:01.750
back and look at the shape of it. The same

362
00:15:01.750 --> 00:15:03.990
little observatory that just helped us find

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an invisible black hole halfway across the

364
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universe is now clinging on in low Earth

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orbit, waiting to see if its own lifeboat can

366
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limp over and give it a shovel. Space is

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hard. Even the rescue missions need rescuing.

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Anna: We'll keep you posted as that one develops.

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And that brings us to the sky over the next

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few nights. And there's one thing you cannot

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00:15:24.900 --> 00:15:27.420
miss, because it's going to be lighting up

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the whole night. The moon.

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Avery: The full buck moon.

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00:15:31.340 --> 00:15:34.180
Anna: The full buck moon. Full tonight, the

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00:15:34.180 --> 00:15:37.060
29th, and near enough to 100%

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lit for a couple of nights either side.

377
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Gorgeous to look at as it climbs the eastern

378
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sky after sunset. But it is a

379
00:15:45.060 --> 00:15:48.060
floodlight and that shapes everything else we

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00:15:48.060 --> 00:15:49.180
can and can't

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Avery: do this week, starting with the meteors,

382
00:15:51.380 --> 00:15:53.500
because there are three showers on the go at

383
00:15:53.500 --> 00:15:53.780
once.

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00:15:54.180 --> 00:15:56.340
Anna: There are. And this is where our two

385
00:15:56.340 --> 00:15:59.260
hemispheres genuinely differ. The headline

386
00:15:59.260 --> 00:16:01.740
shower right now is the Southern Delta

387
00:16:01.740 --> 00:16:04.140
Aquarius, peaking over the next couple of

388
00:16:04.140 --> 00:16:06.870
nights. And the clue is in the name of. For

389
00:16:06.870 --> 00:16:09.470
our Southern Hemisphere listeners, this one's

390
00:16:09.470 --> 00:16:12.350
yours. The radiant over near the bright star

391
00:16:12.350 --> 00:16:14.830
Fomalhaut rides high almost

392
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overhead in the pre dawn hours. So from

393
00:16:17.710 --> 00:16:20.230
Australia, New Zealand and southern Africa,

394
00:16:20.630 --> 00:16:23.190
you're in the best seats on Earth for it.

395
00:16:23.510 --> 00:16:26.230
And for the north, from North America,

396
00:16:26.230 --> 00:16:29.150
it's lower and stingier, though observers

397
00:16:29.150 --> 00:16:31.230
in the southern United States still get a

398
00:16:31.230 --> 00:16:34.040
fair look. Best window everywhere is

399
00:16:34.040 --> 00:16:36.800
the couple of hours before dawn. But

400
00:16:37.040 --> 00:16:39.760
big caveat, this year, that brilliant

401
00:16:39.760 --> 00:16:42.400
moon is going to wash out most of the faint

402
00:16:42.400 --> 00:16:45.360
Delta Aquarids. So temper expectations.

403
00:16:45.760 --> 00:16:47.720
Avery: If the faint ones are drowned out, what's

404
00:16:47.720 --> 00:16:48.720
worth staying up for?

405
00:16:49.040 --> 00:16:51.960
Anna: The fireballs. The Alpha Capricornids

406
00:16:51.960 --> 00:16:54.880
are active at the same time. They're sparse,

407
00:16:54.880 --> 00:16:57.640
only a handful an hour. But they specialize

408
00:16:57.640 --> 00:17:00.600
in slow, brilliant fireballs bright enough

409
00:17:00.600 --> 00:17:03.250
to punch through moonlight. And unlike the

410
00:17:03.250 --> 00:17:05.930
Delta Aquarids, the Capricornids play

411
00:17:05.930 --> 00:17:08.210
fair. They're just as good from either

412
00:17:08.210 --> 00:17:10.930
hemisphere. So the tip for everyone this

413
00:17:10.930 --> 00:17:13.570
week, don't chase quantity. Get

414
00:17:13.570 --> 00:17:16.210
comfortable, be patient and wait for

415
00:17:16.210 --> 00:17:19.170
one big slow fireball to make your

416
00:17:19.170 --> 00:17:19.490
night.

417
00:17:19.810 --> 00:17:22.210
Avery: And the shower, everyone's really waiting for

418
00:17:22.530 --> 00:17:23.570
the Perseids.

419
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Anna: And here's the good news to hold onto.

420
00:17:26.210 --> 00:17:28.810
They're building now, but they peak on the

421
00:17:28.810 --> 00:17:31.570
night of the 12th into the 13th of August.

422
00:17:31.970 --> 00:17:34.770
And this year the timing is close to perfect.

423
00:17:35.010 --> 00:17:37.570
The peak lands right on the New Moon.

424
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Dark skies, no moonlight.

425
00:17:40.290 --> 00:17:42.770
Potentially the best Perseids in years.

426
00:17:43.170 --> 00:17:45.890
They favor the northern Hemisphere, but mid

427
00:17:45.890 --> 00:17:48.770
southern latitudes will catch some too. Mark

428
00:17:48.770 --> 00:17:51.570
it. The night of 12 August is the one to

429
00:17:51.570 --> 00:17:52.210
keep clear.

430
00:17:52.610 --> 00:17:54.890
Avery: And that same date is a big one for another

431
00:17:54.890 --> 00:17:55.250
reason.

432
00:17:55.730 --> 00:17:58.490
Anna: It is a, uh, total solar eclipse on

433
00:17:58.490 --> 00:18:01.370
12 August, with the path of totality

434
00:18:01.370 --> 00:18:04.310
crossing Greenland, Iceland and slice of

435
00:18:04.310 --> 00:18:07.070
Spain, and a partial eclipse visible across

436
00:18:07.230 --> 00:18:09.630
much of Europe and parts of North America.

437
00:18:09.870 --> 00:18:12.190
We'll have full timings closer to the day.

438
00:18:12.430 --> 00:18:14.830
And the one rule that never changes

439
00:18:14.830 --> 00:18:17.510
wherever you are, never look at the

440
00:18:17.510 --> 00:18:20.110
partial phases of a solar eclipse. Without

441
00:18:20.350 --> 00:18:23.310
certified eclipse glasses, ISO

442
00:18:23.390 --> 00:18:26.030
123122

443
00:18:26.190 --> 00:18:28.590
or a properly filtered telescope.

444
00:18:28.830 --> 00:18:31.430
Ordinary sunglasses will not protect your

445
00:18:31.430 --> 00:18:34.170
eyes. That safety line stays in.

446
00:18:34.410 --> 00:18:35.530
No exceptions.

447
00:18:36.090 --> 00:18:38.650
Avery: One quick planet note before we wrap the sky.

448
00:18:38.890 --> 00:18:41.730
Anna: Yes, say goodbye to Jupiter for a

449
00:18:41.730 --> 00:18:44.010
little while. Today the 29th

450
00:18:44.170 --> 00:18:47.170
Jupiter reaches solar conjunction. It's

451
00:18:47.170 --> 00:18:49.930
passing almost directly behind the sun from

452
00:18:49.930 --> 00:18:52.450
our point of view, so it's lost in the glare

453
00:18:52.450 --> 00:18:54.650
and out of action for the next few weeks.

454
00:18:54.810 --> 00:18:57.450
It'll creep back as a pre dawn object

455
00:18:57.530 --> 00:19:00.280
later in August. And for early risers,

456
00:19:00.440 --> 00:19:02.840
Mercury is putting on its best morning

457
00:19:02.840 --> 00:19:05.640
showing of the season, low in the pre dawn

458
00:19:05.640 --> 00:19:06.040
east,

459
00:19:06.520 --> 00:19:08.520
Avery: and we have to close the loop on our lead

460
00:19:08.520 --> 00:19:08.920
story.

461
00:19:09.320 --> 00:19:12.240
Anna: We do. If you're up before dawn chasing

462
00:19:12.240 --> 00:19:15.200
those meteors, look for Orion climbing in

463
00:19:15.200 --> 00:19:18.160
the east and find Betelgeuse, that bright

464
00:19:18.160 --> 00:19:20.800
orange shoulder from the southern hemisphere.

465
00:19:20.800 --> 00:19:23.280
It's high in the northern sky and flipped

466
00:19:23.280 --> 00:19:25.880
over from the north. It's lower in the east

467
00:19:25.880 --> 00:19:28.860
before sunrise. Either way, give it a nod.

468
00:19:29.180 --> 00:19:31.860
You now know something about that star that

469
00:19:31.860 --> 00:19:33.900
nobody knew for a hundred years.

470
00:19:34.140 --> 00:19:36.780
It's got a companion before we go,

471
00:19:36.780 --> 00:19:39.260
Avery: a bit of proper news from our end. We've just

472
00:19:39.260 --> 00:19:41.100
launched the brand new home for the show

473
00:19:41.260 --> 00:19:41.340
astronomydaily.

474
00:19:41.340 --> 00:19:44.300
Anna: Uh, IO same

475
00:19:44.300 --> 00:19:46.900
address you already know, but it's had a

476
00:19:46.900 --> 00:19:49.020
complete makeover and there's a lot there.

477
00:19:49.020 --> 00:19:51.980
Now you can stream the entire back catalog

478
00:19:52.060 --> 00:19:54.320
every episode. There's a news feed that

479
00:19:54.320 --> 00:19:56.600
updates continuously through the day so you

480
00:19:56.600 --> 00:19:58.360
can keep up with the latest space and

481
00:19:58.360 --> 00:20:01.160
astronomy headlines between episodes. You can

482
00:20:01.160 --> 00:20:03.080
read listener reviews and leave one of your

483
00:20:03.080 --> 00:20:05.280
own. And you can sign up for uh, our daily

484
00:20:05.280 --> 00:20:07.880
Space News newsletter to get it all straight

485
00:20:07.880 --> 00:20:08.720
to your inbox.

486
00:20:09.040 --> 00:20:10.720
Avery: And there's a spot to drop us a line,

487
00:20:10.880 --> 00:20:13.240
questions, suggestions, a story you think

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we've missed, or just to say good day, we

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read them.

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Anna: It's brand new, so we genuinely love your

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feedback on it. Head to astronomydaily

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IO have a wander around and tell us what you

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think, what you love, what you change. Help

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us make it yours.

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Avery: That's astronomy daily for Wednesday, 29th of

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July. Betelgeuse's Hundred Year Secret

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A black hole in the wrong part of town, Roman

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on the clock and a rescue mission holding its

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breath.

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Anna: Thanks for spending part of your day with us.

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Look after each other and whichever

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hemisphere you're in.

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Avery: Clear skies.