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Anna: Welcome to Astronomy Daily, the podcast

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where we chat about the coolest space and

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astronomy news we can source. I'm Anna,

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um, and with me is my co host, Avery.

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Hey Avery, it's January 8,

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2026. How's your week going?

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Avery: Hey Anna. And hello to all our listeners.

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It's been fantastic. Clear nights for

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some stargazing. We've got a stellar lineup

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today. Mysteries solved on a famous star.

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A decades long supernova video,

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a cens nearby stars for life,

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lunar events to watch, a dramatic but

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low risk orbital scenario, and fresh

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insights on asteroid mining. Plenty to

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unpack. Let's get started.

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Anna: Leading off with big news from Orion,

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astronomers have finally cracked Betelgeuse's

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biggest mystery. The cause of its weird

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brightness swings and that dramatic great

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dimming back in 2020.

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Avery: Yeah, this red supergiant, one of the

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brightest stars in the sky and about 650

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light years, has been puzzling folks

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forever. With its pulsations, it has a short

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400 day cycle from internal throbbing.

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But there's this longer 2100 day

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variation that stumped everyone. Theories

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range from giant convection cells to dust

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clouds or even a companion star.

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Anna: Turns out it is a hidden companion.

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Researchers from the Centre for Astrophysics

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at Harvard and Smithsonian, led by Andrea

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Dupre, used nearly eight years of Hubble

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data plus ground telescopes to

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direct evidence. The companion, playfully

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called Siwarha, orbits every six years or

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so, ploughing through Betelgeuse's massive

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extended atmosphere. Like a boat cutting

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through water, leaving a dense wake of gas.

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Avery: That wake disrupts the star's light and

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spectrum, causing the dimming and patterns we

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see. Dupree described it perfectly. It's a

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bit like a boat moving through water. The

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companion star creates a ripple effect in

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Betelgeuse's atmosphere that we can actually

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see. In the data they caught the wake form

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forming right after the companion passes in

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front.

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Anna: This explains the 2020 sneeze too.

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Dust and gas from that interaction. Huge

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implications. It shows how companions can

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reshape massive stars. Evolution, mass

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loss and eventual supernovae.

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Betelgeuse is eclipsing Siwarha right now,

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but they'll watch for it emerging in 2027.

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Avery: Front row. See to a star's dramatic life.

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Love it.

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Anna: Next, NASA dropped an incredible video

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that's literally decades in the making. A

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time lapse of Kepler's supernova remnant

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from Chandra Xway Observatory data.

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Avery: This is the remnant from the supernova

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spotted by Johannes Kepler in 1604.

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A, uh, type 1A explosion from a white dwarf

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that blew up after Gaining too much mass,

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maybe from a companion or merger. It's about

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17,000 light years away and

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Chandra's been watching since 2000.

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Anna: The video combines observations from

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2000-2004-2006-2014

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and even in 2025 over

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25 years. It shows this neon

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blue X ray ring expanding like a balloon

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overlaid on optical light. The bottom side

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blasts out faster at 13.8

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million miles per hour while the top lags

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at 4 million miles per hour because it hits

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denser gas, Chandra.

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Avery: Glows in blue from million degree material

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and the rim measurements tell us about the

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explosion's power and surroundings. It's the

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longest spanning Chandra video ever showing

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remnant crashes into space stuff hurling

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elements for new stars and planets.

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Anna: Mind blowing to see cosmic history unfold.

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Avery: Frame by frame Shifting closer to

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home, a uh new all sky census of over

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2100 K dwarfs within about

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130 light years reveals some prime real

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estate for potential life bearing planets.

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Anna: K dwarfs are cooler, fainter orange

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stars twice as common as sun like G

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dwarfs nearby and they live way longer,

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giving planets stable rates radiation for

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billions more years Perfect for life to

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evolve slowly.

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Avery: The team use high res spectrometers on

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telescopes in Chile and Arizona for full sky

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coverage. They measured temperatures,

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ages, spin rates, magnetic activity

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all key for habitability since flaring

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stars can strip atmospheres.

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Anna: This spectroscopic recon is a goldmine

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data set for future exoplanet hunts and even

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interstellar travel planning Presented just

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this week at the AAS meeting.

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Foundational for decades makes you wonder

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how.

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Avery: Many Earth likes are chilling around these

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steady stars.

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Anna: For sky watchers, especially down south,

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2026 has some lunar a red

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moon from a total eclipse, a blue moon and

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a Christmas Eve supermoon.

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Avery: The total lunar eclipse on March 3 evening

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will turn the moon coppery red as Earth's

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atmosphere bends sunset light onto it.

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Totality's best from the Southern hemisphere

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Australia, New Zealand lasting about an hour

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visible even in cities Naked eye Then a.

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Anna: Blue moon on May 31 the second full

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moon in a month. A calendar quirk every

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couple years and December 24

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supermoon full moon at perigee

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looking bigger and brighter. Perfect illusion

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at moonrise.

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Avery: No equipment needed. Safe to watch. Mark

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those calendars for some magical nights.

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Anna: Now Headline grabber Could a passing

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star fling Earth into deep space,

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destabilising our orbit faster than thought?

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Avery: This comes from simulations by Nathan Kaib

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and Sean Raymond factoring in galactic

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flybys stars passing within 100

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AU at slow speeds. Normally

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solar system models assume isolation, but

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Reality includes these encounters.

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Anna: Mercury's the weak link. A flyby could make

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its orbit more eccentric, leading to crashes

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or tugs that cascade outward. Maybe

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Venus or Mars Nudging Earth toward

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Jupiter for a slingshot ejection.

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Avery: Probability about 0.2%

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chance over the next 5 billion years for

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Earth ejection or collision Tiny,

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but higher than old estimates. Pluto's risk

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is 4 to 5%, based on Gaia

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data and AARXIVE paper Real science. But

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the article amps up the drama with hidden

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threat vibes.

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Anna: Comforting to know it's super rare. Are

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orbits stable for aeons?

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Avery: Last up Is asteroid mining actually

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feasible? New chemistry data from meteorites

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offers sobering but insightful answers.

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Anna: Researchers analysed Carbonius chondrites

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proxies for C type asteroids. Measuring

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46 elements, these primitive rocks

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mix metals, silicates, water

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bearing stuff. But impacts create

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breccias and regolith, making separation

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tough in low gravity.

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Avery: Some groups show enriched titanium or rare

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Earths, but overall depleted in easy metals

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like copper. Water alteration oxidises

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things, complicating extraction. Led by

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Joseph Tirigo Rodriguez and team, it suggests

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mining's hard for bulk profit, better for

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targeted water or in space manufacturing.

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Anna: Focus on sample returns like Osiris Rex

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to pick winners. Feasible eventually with

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tech advances, but not a quick space gold

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rush.

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Avery: Realistic view Space resources for

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exploration, not Earth riches.

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Anna: Whew.

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Uh, from stellar companions to lunar lights

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in cosmic risks, what a ride Today.

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Avery: The universe never runs out of storeys.

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Thanks for joining us on Astronomy Daily.

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Anna: We appreciate every listen, subscribe, share

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and we'll catch you tomorrow with more. Keep

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looking up Clear skive.
