July 3, 2026
Solar Storms, Grounded Missions, and the Planet That Survived Its Star
Astronomy Daily S05E131 — Friday, July 3, 2026 1. Swift Rescue Mission — Grounded Mid-Flight • Katalyst Space Technologies' LINK spacecraft was set to launch aboard a Pegasus XL rocket, air-launched from Northrop Grumman's Stargazer aircraft over Kwajalein Atoll. • Thursday's attempt (July 2) got airborne after two prior weather scrubs, but was aborted mid-flight when engineers spotted an unexplained warning. • No new launch date has been set. Swift faces uncontrolled reentry by October 2026 without a successful reboost. 2. Solar Storm Watch — G2 Geomagnetic Storm Active Today • X1.1 flare (June 30) plus 10 M-class flares in 24 hours from sunspot region AR4479. • NOAA SWPC G2 (moderate) geomagnetic storm watch in effect for July 3, easing July 4. • Aurora borealis potential as far south as Idaho/New York (US); aurora australis potential for Tasmania and southern NZ/VIC under clear, dark skies. 3. TESS's First Microlensing Exoplanet — Gaia23bra b • Super-Jupiter (~1.63 Jupiter masses) orbiting an orange dwarf ~40,000 light-years away, discovered via gravitational microlensing — a first for TESS. • Originally flagged by ESA's Gaia mission in 2023; confirmed using archival TESS data. • Published July 1, 2026 in The Astrophysical Journal Letters, led by Mallory Harris (University of New Mexico). 4. GJ 3378b — Revised Habitable-Zone Super-Earth, 25 Light-Years Away • UC Irvine team revised the planet's mass down to 2.3 Earth masses (rocky super-Earth, not mini-Neptune) and orbital period to 21.45 days. • Receives ~90% of the stellar radiation Earth receives from the Sun — squarely in the habitable zone. • Atmosphere unknown; planet does not transit, so JWST transit spectroscopy isn't possible. Published in The Astrophysical Journal, led by Paul Robertson (UC Irvine). 5. ESO Study: 1.7 Million Planned Satellites 'Devastating' for Astronomy • Study led by ESO astronomer Olivier Hainaut, accepted for publication in Astronomy & Astrophysics. • Modelled impact of proposed constellations (SpaceX ~1M for space data centres, Reflect Orbital 50,000 mirror satellites) on ESO's VLT and the Vera Rubin Observatory. • Recommends a hard cap of 100,000 satellites, all fainter than naked-eye visibility. Decision pending from the US FCC. 6. JWST Solves the WD 1856b Mystery • Gas giant (4–11 Jupiter masses) orbits a white dwarf every 34 hours, blocking 56% of its star's light during transit. • New JWST atmospheric data shows the planet is ~240K hotter than expected — evidence it migrated inward 3–5.5 billion years after the star's death, rather than surviving the red giant phase in place. • Published July 1, 2026 in Nature, led by Ryan MacDonald with Northwestern's Christopher O'Connor.
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WEBVTT
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Anna: From the bytes.com podcast network. This is
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Astronomy Daily. I'm Anna.
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Avery: And I'm avery. It's Friday, July 3,
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2026, and we've got a proper Fourth of July
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weekend send off for you. A rescue mission
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that's still grounded, a solar storm that's
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actually arrived, and a planet that came back
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from the dead sort of.
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Anna: Today on the show, NASA's Swift Rescue
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mission hits another wall, this time mid
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flight. The sun is genuinely kicking
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off right now with a geomagnetic storm watch
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in effect for tonight. Hess accidentally
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discovers a planet it was never built to
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find. A red dwarf just 25 light years
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away might be hiding the most Earth like
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world we've found in ages.
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Astronomers sound the alarm on satellite
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mega constellations. And we close with a
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planet that shouldn't exist, orbiting the
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corpse of its own star.
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Avery: Six stories. One very busy week for the
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universe. Let's get into it.
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Anna: We start with an update to a story we've been
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tracking for weeks. And it's not the Update
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anyone wanted. NASA's mission to rescue
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the Swift Observatory attempted to launch on
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Thursday, July 2. And for the first
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time, it actually got off the ground.
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Avery: Right, quick recap for anyone just joining
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us. The Neil Garrels Swift Observatory is
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a 22 year old Gamma ray telescope that's
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losing altitude fast because heightened solar
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activity has puffed up Earth's upper
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atmosphere and increased drag on its orbit.
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Anna: Left alone, Swift reenters and burns up by
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October. So NASA hired a company
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called catalyst space technologies,
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$30 million, incredibly tight
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timeline to build a robotic spacecraft
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called Link 3 articulated arms.
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The plan is for Link to grapple Swift,
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a satellite that was never designed to be
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serviced, and shove it back up to a safer
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orbit.
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Avery: It launches piggyback. A Northrop Grumman
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Pegasus rocket tucked under the belly of the
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Stargazer aircraft takes off from Kwajalein
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Atoll in the Marshall Islands, climbs to
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about 39,000ft and then drops the
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rocket, which lights up five seconds later.
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This week alone, it had already been scrubbed
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twice for weather.
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Anna: So Thursday morning, Stargazer finally
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takes off. It's airborne, heading for the
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release point. And then mid flight, the team
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spots a, uh, warning in the data stream and
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makes the call not to release the rocket at
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all.
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Avery: Which is a genuinely different failure mode
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than what we told you earlier this week. This
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wasn't weather. This was an act of abort in
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the air on a live vehicle. It's not even
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clear yet whether the warning came from the
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rocket or from the carrier aircraft itself.
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Anna: No new Launch date has been set. NASA's been
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very upfront that this is a race against the
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clock. They've already suspended most of
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Swift's science operations since February
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just to buy time flying it in a low drag
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orientation to slow the decay.
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Avery: The stakes here go beyond one telescope. 2.
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If Link pulls this off, it's the first time a
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commercial spacecraft has docked with a
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government satellite that was never built for
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servicing. That's a template for saving
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Hubble one day or any number of aging
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observatories we'd otherwise just have to
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write off.
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Anna: So, still grounded, still no date, and the
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clock is still ticking towards October. We'll
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keep you posted the moment there's movement.
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Avery: Story 2 and if you were listening earlier
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this week, you'll remember we flagged the big
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X class flare and told you to watch the
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skies. Well, watch the skies.
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It's happening.
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Anna: The sun has been properly busy
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after that X1.1 flare from
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Sunspot Region
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AR4479 on June 30. It
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followed up with 10m M class flares
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in a single 24 hour stretch.
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Multiple coronal mass ejections, several of
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them Earth directed.
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Avery: NOAA Space Weather Prediction center has a G2
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that's a moderate geomagnetic stormwatch
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active for today July 3rd, with a chance of
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reaching G2 levels through the day as the CME
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arrives and interacts with Earth's magnetic
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field.
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Anna: The key thing forecasters are watching is the
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BZ component of the magnetic field,
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basically whether the storm's magnetic
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orientation points south, which is what lets
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solar wind energy pour into our
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magnetosphere efficiently. Get that right
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and the aurora show
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Avery: gets a lot more dramatic in the Northern
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Hemisphere. That means aurora potentially
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visible much farther south than usual.
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Forecasters are talking about spots like
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Idaho and New York if skies stay dark and
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clear over the coming nights.
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Anna: And for our Southern Hemisphere listeners,
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this is a genuine Aurora Australis
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opportunity too. D2 level storms can
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push the southern lights up into Tasmania
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and sometimes as far as southern Victoria and
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the Lower south island of New Zealand. If
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you've got clear, dark skies away from the
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coast tonight, it's worth a look.
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Avery: South conditions are expected to start
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easing back toward quieter levels tomorrow,
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July 4th as the CME's effects wane.
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So if you're chasing the lights tonight into
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the small hours is your best shot before the
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Northern Hemisphere's holiday fireworks take
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over as the main show.
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Anna: Our third story is a lovely bit of science
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serendipity. NASA's Tess, the
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transiting exoplanet Survey satellite has
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notched ah, a genuine first. Its first
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planet found by gravitational
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microlensing,
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Avery: which is a big deal because TESS wasn't
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designed for that at all. Its entire job is
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watching for the tiny dip in starlight when a
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planet crosses in front of its star.
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Microlensing is a completely different trick.
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It happens when a foreground star drifts
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almost exactly in front of a background star
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and its gravity bends and briefly magnifies
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that background star's light, like a natural
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lens.
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Anna: If that foreground star happens to have its
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own planet, the planet adds its own little
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flicker to that magnification event. And
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that's exactly what happened here. The
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planet's called Gaia 23 Bra, a
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super Jupiter, about 1.63
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times Jupiter's mass, orbiting an orange
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dwarf star roughly 40,000 light years away
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out near the galactic center.
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Avery: It was actually the European Space Agency's
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Gaia mission that first flagged the
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brightening event back in 2023. But
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Gaia's observations were too sparse to
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confirm a planet was involved. It was only
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when researchers went back and combed through
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tess's archival data that they realized
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TESS had caught the same event with enough
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detail to nail it down.
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Anna: Lead author Mallory Harris, a UH doctoral
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candidate at the University of New Mexico,
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published The findings on July 1st in the
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Astrophysical Journal Letters. And the
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tantalizing bit is what it implies. TESS
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has been quietly recording eight years of
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data and nobody was looking for this kind of
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signal. There could be plenty more of these
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hiding in the archive.
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Avery: It's also a nice bit of foreshadowing.
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NASA's Roman Space Telescope, on track to
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launch August 30 this year, is being
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purpose built for exactly this kind of
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survey. It's expected to find around
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1,000 microlensing planets. By staring
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into the crowded center of The Galaxy
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Gaia, uh, 23B is basically a
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preview of what's coming.
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Story four takes us a lot closer to home,
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just 25 light years away, which in galactic
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terms is basically next door.
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Anna: This is
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GJ3378B,
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a rocky world orbiting a faint red dwarf
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star in the constellation Camilo partillaris,
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the giraffe. It was actually first picked up
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back in 2024 by French astronomers,
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but the original numbers pegged it as a puffy
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mini Neptune, five times Earth's mass,
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orbiting on a 25 day period, sitting
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right at the edge of the habitable zone.
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Avery: A team at UC Irvine led by Paul
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Robertson went back with two instruments. The
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Habitable Zone Planet Finder on the Hobby
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Eberly Telescope in Texas and the NED
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Spectrometer on the YIYN Telescope
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at Kitt Peak in Arizona and revised those
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numbers substantially. Robertson put it
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nicely this super Earth gets about 90%
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of the radiation Earth gets from the sun
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right in the sweet spot for liquid water, at
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least in principle.
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Anna: The catch, and there's always a catch with
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red dwarfs, is that these stars can be
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vicious with stellar wind and radiation,
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which tends to strip atmospheres clean
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off nearby planets. And because
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GJ3378B doesn't
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transit its star from our point of view, we
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can't use transit spectroscopy to check
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whether it's actually kept in atmosphere, the
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trick JWST has been using on planets
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like the Trappist 1 system.
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Avery: So the honest answer is nobody knows yet.
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We'll likely have to wait for NASA's
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Habitable Worlds Observatory, which isn't due
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to launch until sometime in the 2000-40s, to
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get a direct look. But for a planet this
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close and this promising, that's a long wait
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worth marking on the calendar.
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Anna: Dory 5 is one that hits close to home
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for us, quite literally given our own dark
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skies down here in the Southern Hemisphere.
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Avery: The European Southern Observatory has
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published the first study to actually
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calculate what happens to ground based
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astronomy if current satellite mega
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constellation proposals go ahead and um, the
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word ESO used was devastating.
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Anna: There are currently somewhere around 14
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to 17,500 satellites in
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orbit. But between SpaceX, which wants
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roughly a million more for space based data
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centers, and companies like
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Reflectorbital, which is proposing three
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50,000 mirror satellites designed to beam
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sunlight down to Earth at night, the combined
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proposals on the table add up to over
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1.7 million satellites.
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Avery: The study, led by ESO astronomer
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Olivier Hainau and accepted for publication
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in Astronomy and Astrophysics, modeled the
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actual imaging impact for a SpaceX
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scale constellation. Even if every satellite
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stayed just below naked eye brightness, the
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study found it would produce dozens of trails
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per image on ESO's Very Large Telescope,
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cutting usable field of view by up to
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28%.
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Anna: It gets worse for the Vera Rubin
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Observatory's new legacy survey of Space and
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Time, which just began full science
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operations. If those satellites were even a
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little brighter than assumed, most of Rubin's
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images each night could be rendered
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essentially unusable.
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Avery: And reflect orbital's mirrors are their own
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special problem. Even when they're not
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pointed directly at an observer, the
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scattered light alone could brighten the
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entire night sky three to four times over.
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I now describe the single one of those
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mirrors as being as Bright as, uh, Venus, the
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so called Morning Star.
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Anna: ESO's recommendation is a hard
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ceiling, no more than 100,000
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satellites total, all kept fainter than
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naked eye visibility. Worth noting, this
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study also directly informs the
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observatories closest to us here in the
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southern hemisphere, since ESO's Very
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Large Telescope and the Extremely Large
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Telescope currently under construction. Both
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sit in the Chilean Atacama Desert.
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Avery: SpaceX and reflect orbital are both still
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waiting for a decision from the U.S. federal
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Communications Commission about whether their
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proposed constellations get approved. And
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this study is now very much part of that
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conversation.
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And for our, uh, final story today, one
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that's been bugging astronomers since 2020,
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and JWST just cracked it.
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Anna: Meet WD 1856
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b. It's a gas giant,
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somewhere between 4 and 11 times
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Jupiter's mass. And it orbits its star
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every 34 hours, less than 3
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million kilometers out, 50 times
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closer than Earth is to the Sun. When it
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transits, it blocks 56% of
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the star's light, one of the deepest transits
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ever recorded.
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Avery: Here's the problem. The star it's orbiting is
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a white dwarf, the collapsed Earth
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sized corpse of a star that has already gone
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through its red giant phase, where it swells
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up hundreds of times its original size and
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incinerates anything nearby. A, uh,
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planet orbiting this close should have been
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vaporized billions of years ago when the star
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was still ballooning outward.
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Anna: So how is it still there? Using
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JWST, an international team
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including Northwestern's Christopher O'
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Connor and lead author Ryan McDonald measured
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the planet's atmosphere directly for the
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first time. Gas temperature and chemical
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composition, including methane and
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hydrocarbon haze, which would give it a color
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similar to Saturn's moon.
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Avery: Titanium and the temperature was the
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giveaway. The planet's running at around
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400 kelvin, roughly
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240 degrees hotter than
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it should be if it were only being warmed by
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the faint light of its dead star. That extra
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heat had to come from somewhere.
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Anna: By modeling how giant planets cool over time,
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the team worked backward and found the planet
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was heated somewhere between 3 and 5.5
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billion years after the white dwarf formed.
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In other words, it wasn't sitting in this
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tight, dangerous orbit during the red giant
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phase at all. It was out at a safe distance
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the whole time and only migrated inward
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billions of years later through gravitational
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interactions with other bodies in the system,
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eating up as it went.
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Avery: It didn't survive the apocalypse. It arrived
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after the funeral.
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Anna: Which makes this more than just a curiosity,
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because our own sun is going to do exactly
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this in about 5 billion years swell
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into a red giant, almost certainly consume
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Mercury and Venus, with Earth sitting right
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on the edge of that danger zone. Jupiter and
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Saturn will very likely survive that phase
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out at a safe distance, just like
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WD1856B's planet originally
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did.
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Avery: And what this research suggests is that the
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story doesn't necessarily end there. Over
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billions more years afterward, gravitational
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nudges could send one of our own surviving
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gas giants migrating inward, closer
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to whatever's left of the sun, just like this
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planet did around its white dwarf.
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Anna: As the researchers put it, stellar death
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isn't necessarily the end. Some planets
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get a whole second act afterwards. A
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nice thought to leave you with heading into
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the weekend.
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Avery: And that's a wrap on Astronomy daily for
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Friday, July 3. A grounded rescue
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mission, A solar storm right over our heads.
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A planet Tess wasn't even looking for. A
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promising new neighbor 25 light years out,
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a warning about our crowding skies, and a
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planet that outlived its own star's death.
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Anna: If you're in the US have a safe and happy 4th
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of July weekend. And if the skies stay dark
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and clear, maybe let the aurora provide a few
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fireworks of its own tonight.
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Avery: If you enjoyed today's episode, please hit
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subscribe wherever you're listening and, uh,
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leave us a review. If you can spare 30
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seconds, it really does help new listeners
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find the show.
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Anna: You can find full show notes, sources and
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links at astronomydaily IO and
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follow us on socials@astrodaily pod.
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We're back tomorrow with more from across the
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universe and of course, the weekend wrap.
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Avery: I'm Avery.
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Anna: I'm Anna. Clear skies, everyone.
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Astronomy Day
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stories. Mhm. Be told.
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Anna: From the bytes.com podcast network. This is
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Astronomy Daily. I'm Anna.
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Avery: And I'm avery. It's Friday, July 3,
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2026, and we've got a proper Fourth of July
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weekend send off for you. A rescue mission
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that's still grounded, a solar storm that's
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actually arrived, and a planet that came back
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from the dead sort of.
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Anna: Today on the show, NASA's Swift Rescue
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mission hits another wall, this time mid
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flight. The sun is genuinely kicking
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off right now with a geomagnetic storm watch
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00:00:31.180 --> 00:00:34.140
in effect for tonight. Hess accidentally
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discovers a planet it was never built to
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find. A red dwarf just 25 light years
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away might be hiding the most Earth like
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world we've found in ages.
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Astronomers sound the alarm on satellite
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mega constellations. And we close with a
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planet that shouldn't exist, orbiting the
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corpse of its own star.
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Avery: Six stories. One very busy week for the
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universe. Let's get into it.
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Anna: We start with an update to a story we've been
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tracking for weeks. And it's not the Update
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anyone wanted. NASA's mission to rescue
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the Swift Observatory attempted to launch on
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Thursday, July 2. And for the first
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time, it actually got off the ground.
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Avery: Right, quick recap for anyone just joining
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us. The Neil Garrels Swift Observatory is
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a 22 year old Gamma ray telescope that's
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losing altitude fast because heightened solar
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activity has puffed up Earth's upper
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atmosphere and increased drag on its orbit.
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Anna: Left alone, Swift reenters and burns up by
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October. So NASA hired a company
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called catalyst space technologies,
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$30 million, incredibly tight
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timeline to build a robotic spacecraft
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called Link 3 articulated arms.
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The plan is for Link to grapple Swift,
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a satellite that was never designed to be
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serviced, and shove it back up to a safer
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orbit.
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Avery: It launches piggyback. A Northrop Grumman
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Pegasus rocket tucked under the belly of the
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Stargazer aircraft takes off from Kwajalein
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Atoll in the Marshall Islands, climbs to
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about 39,000ft and then drops the
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rocket, which lights up five seconds later.
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This week alone, it had already been scrubbed
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twice for weather.
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Anna: So Thursday morning, Stargazer finally
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takes off. It's airborne, heading for the
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release point. And then mid flight, the team
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spots a, uh, warning in the data stream and
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makes the call not to release the rocket at
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all.
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Avery: Which is a genuinely different failure mode
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than what we told you earlier this week. This
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wasn't weather. This was an act of abort in
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the air on a live vehicle. It's not even
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clear yet whether the warning came from the
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rocket or from the carrier aircraft itself.
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Anna: No new Launch date has been set. NASA's been
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very upfront that this is a race against the
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clock. They've already suspended most of
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Swift's science operations since February
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just to buy time flying it in a low drag
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orientation to slow the decay.
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Avery: The stakes here go beyond one telescope. 2.
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If Link pulls this off, it's the first time a
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commercial spacecraft has docked with a
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government satellite that was never built for
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servicing. That's a template for saving
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Hubble one day or any number of aging
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observatories we'd otherwise just have to
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write off.
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Anna: So, still grounded, still no date, and the
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clock is still ticking towards October. We'll
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keep you posted the moment there's movement.
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Avery: Story 2 and if you were listening earlier
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this week, you'll remember we flagged the big
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X class flare and told you to watch the
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skies. Well, watch the skies.
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It's happening.
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Anna: The sun has been properly busy
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after that X1.1 flare from
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Sunspot Region
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AR4479 on June 30. It
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followed up with 10m M class flares
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in a single 24 hour stretch.
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Multiple coronal mass ejections, several of
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them Earth directed.
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Avery: NOAA Space Weather Prediction center has a G2
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that's a moderate geomagnetic stormwatch
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active for today July 3rd, with a chance of
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reaching G2 levels through the day as the CME
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arrives and interacts with Earth's magnetic
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field.
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Anna: The key thing forecasters are watching is the
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BZ component of the magnetic field,
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basically whether the storm's magnetic
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orientation points south, which is what lets
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solar wind energy pour into our
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magnetosphere efficiently. Get that right
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and the aurora show
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Avery: gets a lot more dramatic in the Northern
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Hemisphere. That means aurora potentially
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visible much farther south than usual.
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Forecasters are talking about spots like
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Idaho and New York if skies stay dark and
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clear over the coming nights.
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Anna: And for our Southern Hemisphere listeners,
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this is a genuine Aurora Australis
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opportunity too. D2 level storms can
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push the southern lights up into Tasmania
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and sometimes as far as southern Victoria and
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the Lower south island of New Zealand. If
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you've got clear, dark skies away from the
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coast tonight, it's worth a look.
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Avery: South conditions are expected to start
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easing back toward quieter levels tomorrow,
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July 4th as the CME's effects wane.
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So if you're chasing the lights tonight into
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the small hours is your best shot before the
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Northern Hemisphere's holiday fireworks take
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over as the main show.
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Anna: Our third story is a lovely bit of science
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serendipity. NASA's Tess, the
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transiting exoplanet Survey satellite has
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notched ah, a genuine first. Its first
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planet found by gravitational
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microlensing,
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Avery: which is a big deal because TESS wasn't
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designed for that at all. Its entire job is
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watching for the tiny dip in starlight when a
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planet crosses in front of its star.
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Microlensing is a completely different trick.
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It happens when a foreground star drifts
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almost exactly in front of a background star
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and its gravity bends and briefly magnifies
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that background star's light, like a natural
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lens.
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Anna: If that foreground star happens to have its
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own planet, the planet adds its own little
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flicker to that magnification event. And
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that's exactly what happened here. The
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planet's called Gaia 23 Bra, a
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super Jupiter, about 1.63
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times Jupiter's mass, orbiting an orange
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dwarf star roughly 40,000 light years away
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out near the galactic center.
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Avery: It was actually the European Space Agency's
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Gaia mission that first flagged the
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brightening event back in 2023. But
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Gaia's observations were too sparse to
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confirm a planet was involved. It was only
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when researchers went back and combed through
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tess's archival data that they realized
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TESS had caught the same event with enough
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detail to nail it down.
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Anna: Lead author Mallory Harris, a UH doctoral
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candidate at the University of New Mexico,
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published The findings on July 1st in the
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Astrophysical Journal Letters. And the
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tantalizing bit is what it implies. TESS
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has been quietly recording eight years of
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data and nobody was looking for this kind of
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signal. There could be plenty more of these
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hiding in the archive.
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Avery: It's also a nice bit of foreshadowing.
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NASA's Roman Space Telescope, on track to
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launch August 30 this year, is being
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purpose built for exactly this kind of
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survey. It's expected to find around
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1,000 microlensing planets. By staring
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into the crowded center of The Galaxy
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Gaia, uh, 23B is basically a
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preview of what's coming.
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Story four takes us a lot closer to home,
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just 25 light years away, which in galactic
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terms is basically next door.
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Anna: This is
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GJ3378B,
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a rocky world orbiting a faint red dwarf
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star in the constellation Camilo partillaris,
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the giraffe. It was actually first picked up
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back in 2024 by French astronomers,
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but the original numbers pegged it as a puffy
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mini Neptune, five times Earth's mass,
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orbiting on a 25 day period, sitting
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right at the edge of the habitable zone.
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Avery: A team at UC Irvine led by Paul
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Robertson went back with two instruments. The
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Habitable Zone Planet Finder on the Hobby
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Eberly Telescope in Texas and the NED
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Spectrometer on the YIYN Telescope
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at Kitt Peak in Arizona and revised those
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numbers substantially. Robertson put it
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nicely this super Earth gets about 90%
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of the radiation Earth gets from the sun
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right in the sweet spot for liquid water, at
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least in principle.
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Anna: The catch, and there's always a catch with
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red dwarfs, is that these stars can be
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vicious with stellar wind and radiation,
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which tends to strip atmospheres clean
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off nearby planets. And because
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GJ3378B doesn't
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transit its star from our point of view, we
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can't use transit spectroscopy to check
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whether it's actually kept in atmosphere, the
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trick JWST has been using on planets
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like the Trappist 1 system.
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Avery: So the honest answer is nobody knows yet.
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We'll likely have to wait for NASA's
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Habitable Worlds Observatory, which isn't due
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to launch until sometime in the 2000-40s, to
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get a direct look. But for a planet this
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close and this promising, that's a long wait
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worth marking on the calendar.
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Anna: Dory 5 is one that hits close to home
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for us, quite literally given our own dark
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skies down here in the Southern Hemisphere.
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Avery: The European Southern Observatory has
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published the first study to actually
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calculate what happens to ground based
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astronomy if current satellite mega
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constellation proposals go ahead and um, the
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word ESO used was devastating.
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Anna: There are currently somewhere around 14
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to 17,500 satellites in
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orbit. But between SpaceX, which wants
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roughly a million more for space based data
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centers, and companies like
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Reflectorbital, which is proposing three
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50,000 mirror satellites designed to beam
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sunlight down to Earth at night, the combined
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proposals on the table add up to over
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1.7 million satellites.
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Avery: The study, led by ESO astronomer
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Olivier Hainau and accepted for publication
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in Astronomy and Astrophysics, modeled the
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actual imaging impact for a SpaceX
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scale constellation. Even if every satellite
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stayed just below naked eye brightness, the
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study found it would produce dozens of trails
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per image on ESO's Very Large Telescope,
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cutting usable field of view by up to
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28%.
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Anna: It gets worse for the Vera Rubin
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Observatory's new legacy survey of Space and
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Time, which just began full science
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operations. If those satellites were even a
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little brighter than assumed, most of Rubin's
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images each night could be rendered
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essentially unusable.
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Avery: And reflect orbital's mirrors are their own
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special problem. Even when they're not
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pointed directly at an observer, the
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scattered light alone could brighten the
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entire night sky three to four times over.
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I now describe the single one of those
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mirrors as being as Bright as, uh, Venus, the
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so called Morning Star.
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Anna: ESO's recommendation is a hard
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ceiling, no more than 100,000
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satellites total, all kept fainter than
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naked eye visibility. Worth noting, this
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study also directly informs the
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observatories closest to us here in the
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southern hemisphere, since ESO's Very
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Large Telescope and the Extremely Large
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Telescope currently under construction. Both
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sit in the Chilean Atacama Desert.
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Avery: SpaceX and reflect orbital are both still
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waiting for a decision from the U.S. federal
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Communications Commission about whether their
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proposed constellations get approved. And
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this study is now very much part of that
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conversation.
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And for our, uh, final story today, one
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that's been bugging astronomers since 2020,
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and JWST just cracked it.
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Anna: Meet WD 1856
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b. It's a gas giant,
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somewhere between 4 and 11 times
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Jupiter's mass. And it orbits its star
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every 34 hours, less than 3
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million kilometers out, 50 times
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closer than Earth is to the Sun. When it
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transits, it blocks 56% of
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the star's light, one of the deepest transits
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ever recorded.
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Avery: Here's the problem. The star it's orbiting is
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a white dwarf, the collapsed Earth
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sized corpse of a star that has already gone
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through its red giant phase, where it swells
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up hundreds of times its original size and
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incinerates anything nearby. A, uh,
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planet orbiting this close should have been
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vaporized billions of years ago when the star
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was still ballooning outward.
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Anna: So how is it still there? Using
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JWST, an international team
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including Northwestern's Christopher O'
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Connor and lead author Ryan McDonald measured
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the planet's atmosphere directly for the
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first time. Gas temperature and chemical
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composition, including methane and
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hydrocarbon haze, which would give it a color
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similar to Saturn's moon.
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Avery: Titanium and the temperature was the
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giveaway. The planet's running at around
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400 kelvin, roughly
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240 degrees hotter than
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it should be if it were only being warmed by
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the faint light of its dead star. That extra
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heat had to come from somewhere.
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Anna: By modeling how giant planets cool over time,
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the team worked backward and found the planet
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was heated somewhere between 3 and 5.5
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billion years after the white dwarf formed.
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In other words, it wasn't sitting in this
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tight, dangerous orbit during the red giant
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phase at all. It was out at a safe distance
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the whole time and only migrated inward
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billions of years later through gravitational
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interactions with other bodies in the system,
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eating up as it went.
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Avery: It didn't survive the apocalypse. It arrived
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after the funeral.
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Anna: Which makes this more than just a curiosity,
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because our own sun is going to do exactly
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this in about 5 billion years swell
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into a red giant, almost certainly consume
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Mercury and Venus, with Earth sitting right
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on the edge of that danger zone. Jupiter and
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Saturn will very likely survive that phase
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out at a safe distance, just like
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WD1856B's planet originally
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did.
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Avery: And what this research suggests is that the
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story doesn't necessarily end there. Over
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billions more years afterward, gravitational
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nudges could send one of our own surviving
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gas giants migrating inward, closer
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to whatever's left of the sun, just like this
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planet did around its white dwarf.
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Anna: As the researchers put it, stellar death
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isn't necessarily the end. Some planets
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get a whole second act afterwards. A
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nice thought to leave you with heading into
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the weekend.
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Avery: And that's a wrap on Astronomy daily for
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Friday, July 3. A grounded rescue
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mission, A solar storm right over our heads.
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A planet Tess wasn't even looking for. A
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promising new neighbor 25 light years out,
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a warning about our crowding skies, and a
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planet that outlived its own star's death.
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Anna: If you're in the US have a safe and happy 4th
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of July weekend. And if the skies stay dark
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and clear, maybe let the aurora provide a few
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fireworks of its own tonight.
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Avery: If you enjoyed today's episode, please hit
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subscribe wherever you're listening and, uh,
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leave us a review. If you can spare 30
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seconds, it really does help new listeners
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find the show.
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Anna: You can find full show notes, sources and
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links at astronomydaily IO and
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follow us on socials@astrodaily pod.
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We're back tomorrow with more from across the
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universe and of course, the weekend wrap.
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Avery: I'm Avery.
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Anna: I'm Anna. Clear skies, everyone.
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Astronomy Day
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stories. Mhm. Be told.