Nov. 8, 2025
Cosmic Auroras, Planetary Demise, and Martian Mysteries
- Stunning Aurora Display: Mark your calendars for November 5th to 8th, 2025, as a powerful geomagnetic storm is set to light up the night sky with breathtaking auroras. Classified as a G3 storm, this display will be triggered by a significant coronal mass ejection from the Sun, resulting in vibrant colors visible farther south than usual.
- The Fate of Earth: NASA's Transiting Exoplanet Survey Satellite (TESS) reveals alarming insights into the fate of planets orbiting sun-like stars. As these stars enter their red giant phase, they often engulf their inner planets. New data suggests that Earth's future may be more precarious than previously thought, as the Sun's expansion could ultimately consume our planet.
- Interstellar Object Risks: Recent research sheds light on the potential impact risks from interstellar objects (ISOs). As our solar system travels through the galaxy, it encounters a stream of these cosmic nomads. While the chances of a significant impact remain low, understanding their trajectories is crucial for planetary defense.
- Enceladus: A Hotbed for Life: Exciting new findings from the Cassini mission suggest that Saturn's moon Enceladus could be more promising for extraterrestrial life than previously thought. A newly discovered heat signature at the North Pole indicates a sustained global ocean, providing a stable environment for potential life.
- Blue Origin's Mars Mission: On November 9, 2025, Blue Origin will launch its first interplanetary mission, Escapade, using its new Glenn rocket. This NASA-funded mission aims to explore how Mars lost its atmosphere, providing critical insights into planetary habitability.
- For more cosmic updates, visit our website at astronomydaily.io. Join our community on social media by searching for #AstroDailyPod on Facebook, X, YouTubeMusic, TikTok, and our new Instagram account! Don’t forget to subscribe to the podcast on Apple Podcasts, Spotify, iHeartRadio, or wherever you get your podcasts.
- Thank you for tuning in. This is Anna and Avery signing off. Until next time, keep looking up and exploring the wonders of our universe.
Aurora Forecast
[NOAA](https://www.noaa.gov/)
TESS Findings on Planetary Fates
[NASA](https://www.nasa.gov/)
Interstellar Objects Research
[arXiv](https://arxiv.org/)
Enceladus Heat Signature Study
[NASA](https://www.nasa.gov/)
Blue Origin Escapade Mission
[Blue Origin](https://www.blueorigin.com/)
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This episode includes AI-generated content.
WEBVTT
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Avery: Welcome to Astronomy Daily, the podcast that
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brings you the universe one story at a time.
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I'm your host, Avery.
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Anna: And I'm your co host, Anna. It's great
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to be with you all again, Avery.
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Here in the northern hemisphere, it feels
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like the nights are really drawing in.
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Getting colder, darker.
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Avery: They certainly are. But that darkness
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isn't always a bad thing, especially when it
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becomes a canvas for some of the universe's
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most incredible art. And we're starting
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today's show with just that.
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Anna: That's right. We have a packed episode
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from spectacular atmospheric light shows
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right here at home to the ultimate
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fate of Earth itself.
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Avery: And we'll also look at potential threats from
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outside our solar system, find a beacon of
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hope on an icy moon, and preview an exciting
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new mission to Mars. So let's get right to
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it.
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Anna: I'm ready if you are.
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Avery: Alrighty. Our first story is a visual
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feast for anyone lucky enough to be in the
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right place at the right time. Between
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November 5th and 8th, 2025, the night
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sky put on a show for the ages. A
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powerful geomagnetic storm triggered stunning
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auroras.
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Anna: It really was something special. This was
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classified as a G3 class storm on the
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five point scale, which is considered strong.
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It was all thanks to a significant coronal
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mass ejection, or cme, that
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erupted from the Sun a few days prior.
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Avery: Right. A, uh, cme. Um, so basically the sun
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threw a massive blob of plasma and
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magnetic field our way.
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Anna: Exactly. When that wave of charged
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particles hits our magnetosphere, it
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channels them towards the poles. They rain
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down into our upper atmosphere, collide with
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air molecules, and energize them, causing
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them to glow. The. The beautiful greens are
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from oxygen, while rarer pinks and
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reds come from nitrogen.
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Avery: And this storm was powerful enough that the
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lights were seen much farther south than
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usual. We saw incredible photos and time
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lapses from the northern United States, the
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UK, and all across Scandinavia. It must
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have been just breathtaking to see in person.
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Anna: It truly is an experience that connects you
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to the cosmos. It's a vivid, dynamic
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reminder that we live inside the atmosphere
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of a star.
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Avery: It's.
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Anna: And that our sun is an active, powerful
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force. We're currently in an active period
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of the solar cycle, so we might get a few
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more shows like this in the coming years.
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Avery: I certainly hope so. A, uh, beautiful event
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and a great way to start our cosmic journey
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today.
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Anna: From the beautiful effects of our star's
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activity to a more sobering look at its
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eventual demise.
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Our next story comes from NASA's Transiting
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Exoplanet Survey Satellite, which or TESS.
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And it paints a stark picture of the fate of
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planets orbiting sun like stars.
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Avery: Ah, uh, tess. Its main job is hunting for
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exoplanets. But it's great at just watching
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stars. What did it see this time?
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Anna: It was watching older stars, those beginning
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to enter their red giant phase. And the new
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study confirms that these swelling stars are
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engulfing their inner planets far more often
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than some models predicted. They the evidence
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is in the starlight itself. They can detect
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the chemical signatures of planetary material
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being consumed by the star.
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Avery: Consumed? That's a gentle word for it.
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It's more like being vaporized and
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eaten.
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Anna: A very accurate description. As a star
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like our sun exhausts hydrogen fuel in its
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core, it starts burning it in a shell, which
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causes its outer layers to expand enormously
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and it can swell to hundreds of times its
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original size.
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Avery: And um, any planets in the way.
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Anna: Any planets in the way are first subjected to
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immense tidal forces that can tear them
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apart. And then they are swallowed by the
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star's expanding atmosphere, the
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photosphere.
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Avery: Which brings us to the big scary.
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What does this mean for Mercury, Venus and
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us, uh, here on Earth?
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Anna: Well, Mercury and Venus are almost
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certainly doomed. As for Earth, the
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picture is now looking grimmer. While some
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models suggested Earth's orbit might widen
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and save us, this new data suggests
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the Sun's expansion will be too aggressive to
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overcome that shift.
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Avery: It does. But let's not forget this is about
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5 billion years in the future. So there's no
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need to sell your stocks just yet.
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Anna: Exactly. But it's a profound look into the
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celestial mechanics that govern the birth and
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death of worlds. It gives us a real sense of
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cosmic perspective. Our planet has an
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expiration date written in the stars.
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Avery: Okay. From a threat 5 billion years
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away to one that is, well, less
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predictable. A fascinating new piece of
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research is helping us understand the risk of
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impacts from interstellar objects
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or ISOs.
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Anna: These are the cosmic nomads. Objects like
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asteroids and comets that have been ejected
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from their own star systems and are now
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wandering the Milky Way.
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Avery: That's them. Um, we've had three famous
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visitors so far that we know of. The strange
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cigar shaped Oumuamua in 2017
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and the more comet like Borisov in
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2019. Then there's the current one
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everyone's talking about. 3i
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Atlas those three flybys prove that these
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objects are out there.
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Anna: Right. And now we want to know how many more
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there are and what the chances are that one
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might hit us.
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Avery: Precisely. This new study tells us where
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we're most likely to see them coming from the
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solar apex. That's the direction our
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solar system is traveling as we orbit the
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galaxy. It's what's in front of our cosmic
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windshield, so to speak.
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Anna: So we're essentially running into a stream of
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these objects as we travel through the
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galaxy.
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Avery: It does. The study also pointed to the
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galactic plane as another likely source.
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Now, to be clear, the researchers stress that
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the probability of an impact on from a large
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ISO remains extremely low.
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There's just a lot of empty space out there.
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But for planetary defense experts, this is
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crucial information. It tells them where to
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prioritize their search efforts. It's about
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being smart and looking in the right
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direction for these very faint, very fast
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moving objects.
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Anna: So it's another step towards creating a
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comprehensive map of potential hazards both
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from within and without our solar system.
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Fascinating stuff.
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Avery: Alright, let's leave the threats behind and
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travel to Saturn's icy moon
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Enceladus. It's getting more promising in the
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search for extraterrestrial life, thanks to
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a fresh look at old data from the
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Cassini mission.
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Anna: It absolutely is. Cassini orbited
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Saturn from 2004 to 2017,
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and scientists are still making incredible
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discoveries from its data archives. The big
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news we've known for years is the South Pole
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with its Deimos tiger stripe fissures that
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blast plumes of water from a subsurface ocean
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into space.
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Avery: Yeah, an underground ocean of
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liquid water. That m alone is amazing.
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Anna: It is. But the North Pole was always
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considered the boring one. Frozen,
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ancient and inactive. Well, by
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reanalyzing thermal data from Cassini's
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flybys, scientists have now discovered a
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significant heat signature coming from the
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North Pole as well. The ice is much thicker
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there, so it was trapping the heat, but it's
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definitely there.
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Avery: Wow. So the moon's internal engine is
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heating it at both poles. What does that
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imply for the ocean?
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Anna: It implies the ocean is truly global
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and that the geological activity isn't just a
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recent or temporary phenomenon. At one pole,
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a sustained global heat source means this
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ocean has likely been stable and warm from
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for billions of years.
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Avery: And that is the magic ingredient, a stable
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environment. It gives life, if it were to
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start, a real chance to take hold and evolve.
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Anna: Precisely. We're talking about a world with
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liquid water, organic molecules, which
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Cassini also found, and now a long
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lasting source of energy. That's a perfect
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trifecta for habitability. It makes
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Enceladus arguably the most compelling target
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for future astrobiology missions.
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Avery: We just have to go back, we have to sample
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those plumes and see what's really in that
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water.
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And while a mission to Enceladus is still on
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the drawing board, our final story is about a
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mission that is very much on the launchpad.
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On November 9, 2025, which is
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this Sunday, Blue Origin is set to launch
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its first ever interplanetary mission
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using its heavy lift new Glenn rocket.
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Anna: This is a big step for the commercial space
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industry and it's a NASA funded mission
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they're carrying. Right. A great example of
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public private partnership it is.
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Avery: The payload is a mission called Escapade,
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which consists of two identical probes
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destined for Mars.
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Anna: Escapade. I like the name. What's their
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purpose?
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Avery: They are designed to solve one of Mars
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biggest how it lost its
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atmosphere. We know Mars was once
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warmer and wetter with a thicker atmosphere,
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but over billions of years it was stripped
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away by the solar wind.
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Anna: Right. And that happened because Mars lost
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its global magnetic field, which acts as a
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protective shield for a planet's atmosphere.
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Earth's magnetic field protects us from the
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same fate.
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Avery: Exactly. Mars now only has
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these localized remnant pockets of magnetism
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in its crust. The two Escapade spacecraft
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will orbit in formation, allowing one
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to measure the incoming solar wind while the
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other measures the atmospheric effects at
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that exact moment.
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Anna: This will give us the first ever 3D picture
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of how the solar wind is siphoning off what's
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left of the Martian air. It's fundamental
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science for understanding how a habitable
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planet can become an inhospitable one.
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A cautionary tale, perhaps a very important
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one.
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Avery: It's a fantastic mission and a huge milestone
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for Blue Origin. We'll be watching that
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launch closely.
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Anna: And with that, we're out of time for today's
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episode. What a journey across the cosmos.
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Avery: The universe never fails to deliver. A
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huge thank you to all of you for listening to
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Astronomy Daily. Join us next time for
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another journey through the cosmos. Until
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then, stay curious and keep looking up.
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Astronomy Daily
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stories we told
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Love
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story HM Soul.
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Avery: Welcome to Astronomy Daily, the podcast that
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brings you the universe one story at a time.
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I'm your host, Avery.
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Anna: And I'm your co host, Anna. It's great
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to be with you all again, Avery.
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Here in the northern hemisphere, it feels
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like the nights are really drawing in.
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Getting colder, darker.
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Avery: They certainly are. But that darkness
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isn't always a bad thing, especially when it
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becomes a canvas for some of the universe's
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most incredible art. And we're starting
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today's show with just that.
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Anna: That's right. We have a packed episode
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from spectacular atmospheric light shows
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right here at home to the ultimate
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fate of Earth itself.
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Avery: And we'll also look at potential threats from
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outside our solar system, find a beacon of
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hope on an icy moon, and preview an exciting
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new mission to Mars. So let's get right to
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it.
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Anna: I'm ready if you are.
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Avery: Alrighty. Our first story is a visual
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feast for anyone lucky enough to be in the
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right place at the right time. Between
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November 5th and 8th, 2025, the night
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sky put on a show for the ages. A
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powerful geomagnetic storm triggered stunning
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auroras.
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Anna: It really was something special. This was
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classified as a G3 class storm on the
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five point scale, which is considered strong.
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It was all thanks to a significant coronal
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mass ejection, or cme, that
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erupted from the Sun a few days prior.
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Avery: Right. A, uh, cme. Um, so basically the sun
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threw a massive blob of plasma and
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magnetic field our way.
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Anna: Exactly. When that wave of charged
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particles hits our magnetosphere, it
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channels them towards the poles. They rain
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down into our upper atmosphere, collide with
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air molecules, and energize them, causing
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them to glow. The. The beautiful greens are
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from oxygen, while rarer pinks and
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reds come from nitrogen.
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Avery: And this storm was powerful enough that the
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lights were seen much farther south than
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usual. We saw incredible photos and time
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lapses from the northern United States, the
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UK, and all across Scandinavia. It must
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have been just breathtaking to see in person.
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Anna: It truly is an experience that connects you
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to the cosmos. It's a vivid, dynamic
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reminder that we live inside the atmosphere
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of a star.
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Avery: It's.
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Anna: And that our sun is an active, powerful
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force. We're currently in an active period
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of the solar cycle, so we might get a few
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more shows like this in the coming years.
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Avery: I certainly hope so. A, uh, beautiful event
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and a great way to start our cosmic journey
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today.
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Anna: From the beautiful effects of our star's
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activity to a more sobering look at its
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eventual demise.
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Our next story comes from NASA's Transiting
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Exoplanet Survey Satellite, which or TESS.
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And it paints a stark picture of the fate of
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planets orbiting sun like stars.
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Avery: Ah, uh, tess. Its main job is hunting for
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exoplanets. But it's great at just watching
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stars. What did it see this time?
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Anna: It was watching older stars, those beginning
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to enter their red giant phase. And the new
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study confirms that these swelling stars are
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engulfing their inner planets far more often
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than some models predicted. They the evidence
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is in the starlight itself. They can detect
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the chemical signatures of planetary material
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being consumed by the star.
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Avery: Consumed? That's a gentle word for it.
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It's more like being vaporized and
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eaten.
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Anna: A very accurate description. As a star
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like our sun exhausts hydrogen fuel in its
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core, it starts burning it in a shell, which
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causes its outer layers to expand enormously
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and it can swell to hundreds of times its
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original size.
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Avery: And um, any planets in the way.
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Anna: Any planets in the way are first subjected to
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immense tidal forces that can tear them
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apart. And then they are swallowed by the
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star's expanding atmosphere, the
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photosphere.
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Avery: Which brings us to the big scary.
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What does this mean for Mercury, Venus and
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us, uh, here on Earth?
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Anna: Well, Mercury and Venus are almost
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certainly doomed. As for Earth, the
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picture is now looking grimmer. While some
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models suggested Earth's orbit might widen
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and save us, this new data suggests
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the Sun's expansion will be too aggressive to
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overcome that shift.
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Avery: It does. But let's not forget this is about
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5 billion years in the future. So there's no
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need to sell your stocks just yet.
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Anna: Exactly. But it's a profound look into the
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celestial mechanics that govern the birth and
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death of worlds. It gives us a real sense of
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cosmic perspective. Our planet has an
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expiration date written in the stars.
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Avery: Okay. From a threat 5 billion years
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away to one that is, well, less
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predictable. A fascinating new piece of
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research is helping us understand the risk of
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impacts from interstellar objects
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or ISOs.
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Anna: These are the cosmic nomads. Objects like
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asteroids and comets that have been ejected
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from their own star systems and are now
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wandering the Milky Way.
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Avery: That's them. Um, we've had three famous
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visitors so far that we know of. The strange
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cigar shaped Oumuamua in 2017
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and the more comet like Borisov in
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2019. Then there's the current one
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everyone's talking about. 3i
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Atlas those three flybys prove that these
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objects are out there.
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Anna: Right. And now we want to know how many more
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there are and what the chances are that one
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might hit us.
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Avery: Precisely. This new study tells us where
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we're most likely to see them coming from the
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solar apex. That's the direction our
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solar system is traveling as we orbit the
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galaxy. It's what's in front of our cosmic
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windshield, so to speak.
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Anna: So we're essentially running into a stream of
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these objects as we travel through the
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galaxy.
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Avery: It does. The study also pointed to the
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galactic plane as another likely source.
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Now, to be clear, the researchers stress that
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the probability of an impact on from a large
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ISO remains extremely low.
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There's just a lot of empty space out there.
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But for planetary defense experts, this is
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crucial information. It tells them where to
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prioritize their search efforts. It's about
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being smart and looking in the right
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direction for these very faint, very fast
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moving objects.
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Anna: So it's another step towards creating a
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comprehensive map of potential hazards both
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from within and without our solar system.
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Fascinating stuff.
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Avery: Alright, let's leave the threats behind and
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travel to Saturn's icy moon
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Enceladus. It's getting more promising in the
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search for extraterrestrial life, thanks to
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a fresh look at old data from the
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Cassini mission.
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Anna: It absolutely is. Cassini orbited
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Saturn from 2004 to 2017,
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and scientists are still making incredible
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discoveries from its data archives. The big
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news we've known for years is the South Pole
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with its Deimos tiger stripe fissures that
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blast plumes of water from a subsurface ocean
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into space.
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Avery: Yeah, an underground ocean of
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liquid water. That m alone is amazing.
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Anna: It is. But the North Pole was always
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considered the boring one. Frozen,
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ancient and inactive. Well, by
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reanalyzing thermal data from Cassini's
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flybys, scientists have now discovered a
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significant heat signature coming from the
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North Pole as well. The ice is much thicker
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there, so it was trapping the heat, but it's
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definitely there.
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Avery: Wow. So the moon's internal engine is
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heating it at both poles. What does that
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imply for the ocean?
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Anna: It implies the ocean is truly global
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and that the geological activity isn't just a
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recent or temporary phenomenon. At one pole,
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a sustained global heat source means this
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ocean has likely been stable and warm from
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for billions of years.
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Avery: And that is the magic ingredient, a stable
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environment. It gives life, if it were to
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start, a real chance to take hold and evolve.
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Anna: Precisely. We're talking about a world with
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liquid water, organic molecules, which
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Cassini also found, and now a long
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lasting source of energy. That's a perfect
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trifecta for habitability. It makes
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Enceladus arguably the most compelling target
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for future astrobiology missions.
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Avery: We just have to go back, we have to sample
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those plumes and see what's really in that
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water.
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And while a mission to Enceladus is still on
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the drawing board, our final story is about a
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mission that is very much on the launchpad.
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On November 9, 2025, which is
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this Sunday, Blue Origin is set to launch
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its first ever interplanetary mission
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using its heavy lift new Glenn rocket.
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Anna: This is a big step for the commercial space
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industry and it's a NASA funded mission
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they're carrying. Right. A great example of
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public private partnership it is.
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Avery: The payload is a mission called Escapade,
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which consists of two identical probes
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destined for Mars.
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Anna: Escapade. I like the name. What's their
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purpose?
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Avery: They are designed to solve one of Mars
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biggest how it lost its
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atmosphere. We know Mars was once
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warmer and wetter with a thicker atmosphere,
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but over billions of years it was stripped
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away by the solar wind.
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Anna: Right. And that happened because Mars lost
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its global magnetic field, which acts as a
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protective shield for a planet's atmosphere.
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Earth's magnetic field protects us from the
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same fate.
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Avery: Exactly. Mars now only has
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these localized remnant pockets of magnetism
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in its crust. The two Escapade spacecraft
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will orbit in formation, allowing one
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to measure the incoming solar wind while the
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other measures the atmospheric effects at
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that exact moment.
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Anna: This will give us the first ever 3D picture
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of how the solar wind is siphoning off what's
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left of the Martian air. It's fundamental
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science for understanding how a habitable
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planet can become an inhospitable one.
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A cautionary tale, perhaps a very important
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one.
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Avery: It's a fantastic mission and a huge milestone
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for Blue Origin. We'll be watching that
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launch closely.
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Anna: And with that, we're out of time for today's
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episode. What a journey across the cosmos.
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Avery: The universe never fails to deliver. A
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huge thank you to all of you for listening to
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Astronomy Daily. Join us next time for
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another journey through the cosmos. Until
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then, stay curious and keep looking up.
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Astronomy Daily
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stories we told
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Love
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story HM Soul.