July 29, 2026
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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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
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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
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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
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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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is to use Link's electric thrusters, its
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xenon propulsion, to stop the spin over the
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next few days, then re establish stable
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pointing, update the spacecraft's guidance
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and navigation to work around the dead
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hardware, and only then sit, uh, down with
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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
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still do the job.
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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
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we're recording. By the time you hear this,
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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
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back and look at the shape of it. The same
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little observatory that just helped us find
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an invisible black hole halfway across the
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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
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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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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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Anna: The full buck moon. Full tonight, the
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29th, and near enough to 100%
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lit for a couple of nights either side.
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Gorgeous to look at as it climbs the eastern
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sky after sunset. But it is a
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floodlight and that shapes everything else we
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can and can't
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Avery: do this week, starting with the meteors,
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because there are three showers on the go at
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once.
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Anna: There are. And this is where our two
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hemispheres genuinely differ. The headline
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shower right now is the Southern Delta
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Aquarius, peaking over the next couple of
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nights. And the clue is in the name of. For
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our Southern Hemisphere listeners, this one's
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yours. The radiant over near the bright star
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Fomalhaut rides high almost
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overhead in the pre dawn hours. So from
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Australia, New Zealand and southern Africa,
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you're in the best seats on Earth for it.
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And for the north, from North America,
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it's lower and stingier, though observers
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in the southern United States still get a
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fair look. Best window everywhere is
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the couple of hours before dawn. But
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big caveat, this year, that brilliant
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00:16:39.760 --> 00:16:42.400
moon is going to wash out most of the faint
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Delta Aquarids. So temper expectations.
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Avery: If the faint ones are drowned out, what's
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worth staying up for?
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Anna: The fireballs. The Alpha Capricornids
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are active at the same time. They're sparse,
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only a handful an hour. But they specialize
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in slow, brilliant fireballs bright enough
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00:17:00.600 --> 00:17:03.250
to punch through moonlight. And unlike the
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Delta Aquarids, the Capricornids play
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fair. They're just as good from either
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hemisphere. So the tip for everyone this
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week, don't chase quantity. Get
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comfortable, be patient and wait for
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one big slow fireball to make your
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night.
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Avery: And the shower, everyone's really waiting for
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the Perseids.
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Anna: And here's the good news to hold onto.
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They're building now, but they peak on the
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night of the 12th into the 13th of August.
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And this year the timing is close to perfect.
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The peak lands right on the New Moon.
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Dark skies, no moonlight.
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Potentially the best Perseids in years.
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They favor the northern Hemisphere, but mid
427
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southern latitudes will catch some too. Mark
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00:17:48.770 --> 00:17:51.570
it. The night of 12 August is the one to
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00:17:51.570 --> 00:17:52.210
keep clear.
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Avery: And that same date is a big one for another
431
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reason.
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Anna: It is a, uh, total solar eclipse on
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12 August, with the path of totality
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crossing Greenland, Iceland and slice of
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Spain, and a partial eclipse visible across
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much of Europe and parts of North America.
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We'll have full timings closer to the day.
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And the one rule that never changes
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wherever you are, never look at the
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partial phases of a solar eclipse. Without
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certified eclipse glasses, ISO
442
00:18:23.390 --> 00:18:26.030
123122
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or a properly filtered telescope.
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Ordinary sunglasses will not protect your
445
00:18:31.430 --> 00:18:34.170
eyes. That safety line stays in.
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No exceptions.
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Avery: One quick planet note before we wrap the sky.
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Anna: Yes, say goodbye to Jupiter for a
449
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little while. Today the 29th
450
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Jupiter reaches solar conjunction. It's
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passing almost directly behind the sun from
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our point of view, so it's lost in the glare
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and out of action for the next few weeks.
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It'll creep back as a pre dawn object
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later in August. And for early risers,
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Mercury is putting on its best morning
457
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showing of the season, low in the pre dawn
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east,
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Avery: and we have to close the loop on our lead
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00:19:08.520 --> 00:19:08.920
story.
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Anna: We do. If you're up before dawn chasing
462
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those meteors, look for Orion climbing in
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00:19:15.200 --> 00:19:18.160
the east and find Betelgeuse, that bright
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00:19:18.160 --> 00:19:20.800
orange shoulder from the southern hemisphere.
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It's high in the northern sky and flipped
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over from the north. It's lower in the east
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before sunrise. Either way, give it a nod.
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You now know something about that star that
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00:19:31.860 --> 00:19:33.900
nobody knew for a hundred years.
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It's got a companion before we go,
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Avery: a bit of proper news from our end. We've just
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launched the brand new home for the show
473
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astronomydaily.
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Anna: Uh, IO same
475
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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
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can keep up with the latest space and
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astronomy headlines between episodes. You can
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read listener reviews and leave one of your
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own. And you can sign up for uh, our daily
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Space News newsletter to get it all straight
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to your inbox.
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Avery: And there's a spot to drop us a line,
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00:20:10.880 --> 00:20:13.240
questions, suggestions, a story you think
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00:20:13.240 --> 00:20:15.640
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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00:20:26.650 --> 00:20:27.570
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.
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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
15
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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
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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
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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
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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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is to use Link's electric thrusters, its
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xenon propulsion, to stop the spin over the
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next few days, then re establish stable
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pointing, update the spacecraft's guidance
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and navigation to work around the dead
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hardware, and only then sit, uh, down with
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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
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still do the job.
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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
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we're recording. By the time you hear this,
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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
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back and look at the shape of it. The same
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little observatory that just helped us find
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an invisible black hole halfway across the
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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
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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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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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Anna: The full buck moon. Full tonight, the
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29th, and near enough to 100%
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lit for a couple of nights either side.
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Gorgeous to look at as it climbs the eastern
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sky after sunset. But it is a
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floodlight and that shapes everything else we
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can and can't
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Avery: do this week, starting with the meteors,
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because there are three showers on the go at
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once.
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Anna: There are. And this is where our two
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hemispheres genuinely differ. The headline
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shower right now is the Southern Delta
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Aquarius, peaking over the next couple of
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nights. And the clue is in the name of. For
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our Southern Hemisphere listeners, this one's
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yours. The radiant over near the bright star
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Fomalhaut rides high almost
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overhead in the pre dawn hours. So from
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Australia, New Zealand and southern Africa,
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you're in the best seats on Earth for it.
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And for the north, from North America,
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it's lower and stingier, though observers
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in the southern United States still get a
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fair look. Best window everywhere is
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the couple of hours before dawn. But
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big caveat, this year, that brilliant
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moon is going to wash out most of the faint
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Delta Aquarids. So temper expectations.
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Avery: If the faint ones are drowned out, what's
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worth staying up for?
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Anna: The fireballs. The Alpha Capricornids
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are active at the same time. They're sparse,
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only a handful an hour. But they specialize
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in slow, brilliant fireballs bright enough
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to punch through moonlight. And unlike the
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Delta Aquarids, the Capricornids play
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fair. They're just as good from either
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hemisphere. So the tip for everyone this
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week, don't chase quantity. Get
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comfortable, be patient and wait for
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one big slow fireball to make your
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night.
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Avery: And the shower, everyone's really waiting for
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the Perseids.
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Anna: And here's the good news to hold onto.
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They're building now, but they peak on the
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night of the 12th into the 13th of August.
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And this year the timing is close to perfect.
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The peak lands right on the New Moon.
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Dark skies, no moonlight.
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Potentially the best Perseids in years.
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They favor the northern Hemisphere, but mid
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southern latitudes will catch some too. Mark
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it. The night of 12 August is the one to
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keep clear.
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Avery: And that same date is a big one for another
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reason.
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Anna: It is a, uh, total solar eclipse on
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12 August, with the path of totality
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crossing Greenland, Iceland and slice of
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Spain, and a partial eclipse visible across
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much of Europe and parts of North America.
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We'll have full timings closer to the day.
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And the one rule that never changes
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wherever you are, never look at the
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partial phases of a solar eclipse. Without
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certified eclipse glasses, ISO
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123122
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or a properly filtered telescope.
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Ordinary sunglasses will not protect your
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eyes. That safety line stays in.
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No exceptions.
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Avery: One quick planet note before we wrap the sky.
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Anna: Yes, say goodbye to Jupiter for a
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little while. Today the 29th
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Jupiter reaches solar conjunction. It's
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passing almost directly behind the sun from
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our point of view, so it's lost in the glare
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and out of action for the next few weeks.
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It'll creep back as a pre dawn object
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later in August. And for early risers,
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Mercury is putting on its best morning
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showing of the season, low in the pre dawn
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east,
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Avery: and we have to close the loop on our lead
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story.
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Anna: We do. If you're up before dawn chasing
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those meteors, look for Orion climbing in
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the east and find Betelgeuse, that bright
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orange shoulder from the southern hemisphere.
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It's high in the northern sky and flipped
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over from the north. It's lower in the east
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before sunrise. Either way, give it a nod.
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You now know something about that star that
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nobody knew for a hundred years.
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It's got a companion before we go,
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Avery: a bit of proper news from our end. We've just
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launched the brand new home for the show
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astronomydaily.
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Anna: Uh, IO same
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address you already know, but it's had a
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complete makeover and there's a lot there.
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Now you can stream the entire back catalog
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every episode. There's a news feed that
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updates continuously through the day so you
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can keep up with the latest space and
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astronomy headlines between episodes. You can
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read listener reviews and leave one of your
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00:20:03.080 --> 00:20:05.280
own. And you can sign up for uh, our daily
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Space News newsletter to get it all straight
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00:20:07.880 --> 00:20:08.720
to your inbox.
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Avery: And there's a spot to drop us a line,
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questions, suggestions, a story you think
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00:20:13.240 --> 00:20:15.640
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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00:20:18.840 --> 00:20:21.170
feedback on it. Head to astronomydaily
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00:20:21.330 --> 00:20:24.090
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.
500
00:20:39.970 --> 00:20:41.970
Anna: Thanks for spending part of your day with us.
501
00:20:41.970 --> 00:20:44.050
Look after each other and whichever
502
00:20:44.050 --> 00:20:45.170
hemisphere you're in.
503
00:20:45.670 --> 00:20:46.310
Avery: Clear skies.