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Anna: Welcome, welcome, welcome to Astronomy

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Daily your go to source for everything

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happening beyond our blue planet. I'm

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Anna.

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Avery: And I'm Avery. We're so glad you could join

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us today for what promises to be a

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fascinating journey through the cosmos. We've

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got a packed show lined up delving into some

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truly mind bending discoveries and exciting

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news from across the solar system and beyond.

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Anna: That's right, we'll be unraveling the

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peculiar mysteries of Uranus and its moons,

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exploring a newly cosmic

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bubble surrounding our solar system and

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getting you up to speed on one of the busiest

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launch weeks we've seen this year.

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Avery: And um, stick around for what could be a

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groundbreaking discussion on how life might

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thrive in the most unexpected dark

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corners of the universe. It's a fresh

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perspective that challenges everything we

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thought we knew about habitability. So let's

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dive right in.

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Anna: Alright Avery, let's kick things off with a

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planet that truly lives up to its reputation

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for being a bit, well, weird.

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We're talking about Uranus, the seventh

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planet from the sun, which has always stood

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out from its solar system siblings.

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Avery: It really does. While most planets spin

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fairly upright and their moons orbit neatly,

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Uranus is just doing its own thing, tilted

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on its side at a whopping 98 degrees.

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Imagine Earth's north pole pointing towards

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say, the constellation Ophiuchus instead of

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Polaris the that's Uranus for you.

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Anna: And it's not just its tilt. Its

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magnetic field is also off kilter,

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differing by 59 degrees from its spin

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axis. That's like our magnetic poles being

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in Perth, Australia and northern Florida,

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which is quite the cosmic anomaly.

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Avery: This peculiar setup led astronomer Christian

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Soto and his team at the Space Telescope

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Science Institute to study how Uranus's

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magnetic field might interact with its four

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largest moons, Ariel, Umbriel,

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Titania and Oberon.

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Anna: You'd expect that because Uranus

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rotates faster than its moon's orbit, its

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magnetic field would catch the moons from

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behind and bombard their trailing sides with

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radiation. This process, called

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radiolysis, should create dark

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compounds, making those trailing sides appear

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darker in ultraviolet light.

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Avery: But here's where it gets truly puzzling. When

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the Hubble Space Telescope peered at these

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moons, it found the exact opposite. For

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Ariel and Umbriel, there was hardly any

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difference between their leading and training

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sides. And for the outer two moons, Titania

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and especially Oberon, it was their leading

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sides that were darker.

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Anna: This was completely startling to the

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researchers. It suggests that Uranus's

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magnetosphere might not be as active as

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previously thought. Or it's far more

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complex. But the Darkening on the leading

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sides points to another process entirely.

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Avery: And that process, Soto suggests, involves

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Uranus. Irregular moons. These are

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smaller, often captured asteroids with

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unusual, highly tilted orbits. The

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theory is that micrometeorites constantly hit

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these irregular moons, ejecting dust into

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their orbits.

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Anna: Over millions of years, this dust

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drifts inward, crossing the paths of the

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major moons. As the major moons orbit, they

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sweep up this dust primarily on their leading

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hemispheres. Soto likens it to driving

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fast on a highway and bugs hitting your

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windshield.

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Avery: And, um, the outer moons, Oberon and Titania,

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likely shield the inner ones, Ariel and

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Umbriel, from this dust. But even within the

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outer pair, they're still a mystery. Why is

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Oberon getting so much more dust than

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Titania? That's still one of the weird

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findings they're trying to figure out.

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Anna: This fascinating research highlights how

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much more there is to learn about our own

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solar system. So Soto hopes for a dedicated

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mission to Uranus in the future, perhaps in

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the early 2000 and 40s to truly unravel these

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mysteries. After all, as he put it, it

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is very weird.

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Avery: So why not from the mysteries of our own

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solar system? Let's zoom out a bit to our

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cosmic neighborhood. Our solar system isn't

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just floating in empty space. It resides

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within a massive million degree hot bubble

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of incredibly thin gas. And it's called the

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local hot bubble, or lhb.

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Anna: This LHB is essentially an

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invisible cocoon that glows in X ray

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light and stretches over a thousand light

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years across. And remarkably, despite

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its scorching temperature, its sparse

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atoms barely affect the surrounding matter.

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Some scientists even suggest this quiet

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warmth might have helped life flourish on

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Earth.

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Avery: For decades, the true shape and origin of

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this bubble remained a puzzle. But now,

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thanks to the sharp eyed Erocita X ray

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telescope and a team of scientists in

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Germany, the picture is finally coming

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into focus.

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Anna: The Max Planck Institute for

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Extraterrestrial Physics led the effort

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using Erocita to map the LHB in

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unprecedented detail. What made this

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telescope so crucial is its position

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far from Earth's atmosphere, allowing it to

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capture clear soft X rays ray emissions

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without interference from our own planet's

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solar wind interactions.

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Avery: And the findings? Well, the LHB is

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far from a smooth sphere. Lead researcher

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Michael Young described it as spikier and

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bumpier, with an irregular, jagged

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shape that bulges unevenly. It

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expands more freely towards the galactic

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poles, avoiding the denser midplane of the

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Milky Way, which makes sense as hot gas

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moves towards less resistance.

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Anna: This lumpiness likely reflects the chaotic

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forces that shaped it, such as Multiple

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overlapping supernova explosions and

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feedback from other stars. But perhaps the

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most surprising discovery was a previously

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unknown tunnel stretching towards the

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constellation Centaurus.

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Avery: This interstellar passage may connect the

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LHB with the neighboring superbubble, acting

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like a cosmic gateway. As co author

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Michael Freyberg explained, the existence of

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this tunnel carving a gap in the cooler

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interstellar medium was completely unknown

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until Erocita's sharper sensitivity

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revealed it.

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Anna: This new data from Erocita also helped

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settle a long standing debate. Scientists

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had proposed the LHB concept over

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50 years ago to explain faint X

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ray readings. But doubts arose in the

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90s when similar X rays were found to

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originate from solar wind interacting with

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Earth's atmosphere. Erocita's clear

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observations confirmed that much of that soft

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X ray background truly comes from the

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lhb.

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Avery: And the team also found a temperature

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difference across the bubble with the

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southern part being warmer than the northern

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side. This could point to recent heating

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events, perhaps new supernovas in the last

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few million years, suggesting the LHB

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isn't just a leftover but an active

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changing part of our uh, galactic landscape.

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Anna: And the idea of the Centaurus tunnel suggests

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it might be just one part of a larger system

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of tunnels like arteries running through the

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galaxy. These gaps between cold

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clouds could link the LHB to distant

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features like the Gum Nebula or other

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superbubbles, indicating the Milky Way is

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an interconnected structure and constantly

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shaped by explosive energy.

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Avery: It's truly mind boggling to think about.

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The team even mapped dense molecular clouds

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at the edges of the bubble, Some moving

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outward as if pushed by the original

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explosions that carved out the lhb.

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And fascinatingly, our sun is thought to have

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entered the LHB only a few million years ago.

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A ah, mere blank in its 4.6 billion year

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lifespan.

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Anna: The 3D model they built paints a

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vibrant layered picture of our solar

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system's galactic neighborhood, including

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supernova remains, molecular clouds,

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dust, and these newly discovered tunnels.

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Mapping this cosmic web could provide

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incredible insights into how stars

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die, galaxies evolve and how

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material moves between star systems.

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Avery: It's a major step in understanding not just

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our immediate bubble, but, but the dynamic,

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often explosive forces that shape the space

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between stars. It's like finding a secret

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highway system in space right outside our

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galactic door.

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Anna: Well from cosmic bubbles and

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planetary tilt, let's bring it back to

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Earth for a moment and look at the immediate

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future of space travel. We have a ah, packed

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week of launches ahead.

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Avery: It's truly bustling. Anna. This week's

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launch manifest is one of the busiest of

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2025. So far we've. With 10

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launches scheduled from around the world,

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we're talking everything from crewed missions

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to secret government payloads.

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Anna: Kicking things off on July 29,

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ispace's Shuangquusian 1 rocket

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is set for its eighth flight from China after

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a year long hiatus following a failure on its

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seventh mission. The payload for this one is

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currently unknown, but ISPACE is clearly

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hoping this launch will restore some

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reliability to their rocket.

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Avery: Then later that day, SpaceX is launching

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its first batch of Starlink satellites. This

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week, Group 1029 from

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Cape Canaveral Falcon Booster

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B1069 will be making its

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impressive 26th flight after

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a quick 37 day refurbishment.

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That's a true workhorse.

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Anna: China's CASC has a launch on July

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30th with their Changxing 8A

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carrying an undisclosed number of Guawang

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communications satellites. These are part of

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China's planned mega constellation of

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Internet satellites, aiming to rival SpaceX's

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Starlink, at least within China.

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Avery: Also on July 30, we have a significant

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international mission, the joint NASA

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ISRO Synthetic Aperture Radar, or

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NISAR satellite. This satellite is

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set to map Earth's elevation multiple times

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a month, focusing on ecosystem

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disturbances like earthquakes, tsunamis,

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volcanoes and ice sheet collapses.

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Anna: NASA is contributing the L band radar and

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a high rate telecommunications system, while

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ISRO is providing the satellite bus, the S

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band radar and the launch services from

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India. It's a great example of global

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collaboration in space science.

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Avery: Later that same day, SpaceX is back at

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it with another Starlink launch, Group

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134 from Vandenberg.

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This flight will mark Falcon's 500th

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recovery attempt, really underscoring

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SpaceX's commitment to reusability.

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Anna: And speaking of secretive payloads, Rocket

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Lab is launching a suborbital mission called

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Jake 4 on their haste testbed.

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This is a highly secretive government payload

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believed to be a hypersonic reentry missile.

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Rocket Lab has completed three HASTE missions

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so far, showing a growing demand for

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launching payloads to suborbital space at

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hypersonic speeds.

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Avery: Another unknown payload is scheduled to

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launch from China on July 31, with

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X Pace's Kuaizhou 1A rocket

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making its 30th mission.

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Anna: But perhaps the biggest highlight of the week

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is SpaceX and NASA's Crew 11

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mission to the International Space Station.

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On July 31, four astronauts,

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including NASA's Zena Cardman and Mike

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Finke, JAXA's Kamiya Yui and

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Russian cosmonaut Oleg Platanov, will head to

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the ISS for a six month mission of Science

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and research.

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Avery: And of course, in true SpaceX fashion, the

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Booster B1094 will

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attempt a return to launch site landing. And

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the crew Dragon capsule Endeavor will be

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flying to the ISS for the sixth time as

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after 515 days of refurbishment.

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Anna: Wrapping up the week, SpaceX has a third

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Starlink mission on August 2nd. And then on

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August 4th, another Chinese Changzang 12

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rocket will launch from Winchinchuang

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carrying more Guawang satellites. Given

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that this is the second launch of Guawang

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satellites this week, it looks like China is

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pushing hard to expand its constellation

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rapidly, aiming to fulfill its goal of

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13,000 satellites and provide

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reliable Internet for its people. It's

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certainly going to be a busy week for space

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watchers.

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From the incredible pace of launches, let's

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shift our focus to something even more

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fundamentalthe very definition of where life

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can exist. A groundbreaking new study

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is challenging our traditional views on

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habitability, proposing that life doesn't

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always need sunlight to thrive.

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Avery: That's right, Anna. Uh, this study, led by

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Demetra Attri at NYU Abu Dhabi,

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suggests that high energy radiation from deep

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space, specifically galactic cosmic

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rays, could actually support life in

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dark underground environments on planets like

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Mars and moons such as Europa and

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Enceladus. It really flips the script on

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what makes a planet or moon livable.

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Anna: It's fascinating because we usually associate

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ionizing radiation with harm damage to

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cells, DNA and proteins. Space

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agencies even consider cosmic rays a major

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threat to astronauts. But this research

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highlights another side. In certain

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environments, radiation doesn't just destroy,

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it creates.

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Avery: Exactly. When these energetic charged

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particles hit ice or rock, they can break

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apart water molecules in a process called

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radiolysis. This reaction releases

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electrons and other useful products. On

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Earth, we found bacteria in deep South

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African gold mines that use these electrons

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as an energy source, much like plants use

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sunlight for photosynthesis, thriving

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kilometers below the surface without any

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light at all.

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Anna: So Autry's team used a, uh, physics

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simulation tool to calculate how much energy

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cosmic rays could deposit beneath the

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surfaces of Mars, Europa and

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Enceladus. They then estimated how much

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of that energy could support life, leading to

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a new concept they call the rhz,

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or Radiolytic Habitable Zone.

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Avery: This RHZ shifts the focus away from

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the traditional Goldilocks zone, that sweet

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spot around a star where temperatures allow

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for liquid water. Instead, the

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RHZ looks underground at places where

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water, ice and cosmic radiation

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combine to create energy rich environments.

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It depends on how much radiation penetrates,

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uh, a planet's thin atmosphere or icy shell,

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and how deep it can reach.

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Anna: Their simulations showed that Saturn's moon

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Enceladus actually had the greatest potential

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to support life through radiolysis. With

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Mars following closely and Jupiter's moon

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Europa coming in third. These icy

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bodies, often thought of as lifeless because

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of their cold, sunless surfaces, could

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harbor dense underground ecosystems

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fueled by this radiation.

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Avery: And the key here, as with so many discussions

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about extraterrestrial life, is water.

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Even small pockets of liquid water

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underground would allow these chemical

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reactions to happen more easily, providing a

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medium for complex molecules to form and

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react. It means those suspected oceans

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beneath the ice of Europa or Enceladus

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could be prime locations for alien life.

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Powered by cosmic rays hitting the surface

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ice.

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Anna: This study truly broadens our definition of

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habitability. Life might not need warmth from

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a star or even geothermal heat from a

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planet's core. Cosmic rays, long

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feared, could actually be a life giving

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energy source.

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Avery: In the right conditions, it completely

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redefines where we might look next. Instead

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of just focusing on warm, sunlit worlds, we

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can now consider cold, dark places. As long

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as they have some water beneath the surface

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and are exposed to cosmic rays, it

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offers hope that the universe may be teeming

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with life, quietly thriving in hidden

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oceans, powered by the stars themselves.

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Anna: What an episode. Avery. We've journeyed from

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the puzzling mysteries of Uranus and its

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strangely dark moons, which are still

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baffling scientists, to the incredibly

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dynamic local hot bubbles surrounding our

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solar system.

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Avery: It's been a whirlwind. And let's not forget

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the sheer excitement of this week's launch

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roundup. With so many missions heading into

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space, including crewed flights and

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groundbreaking Earth observation satellites.

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Anna: Absolutely. But perhaps the most mind bending

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discussion was about the radiolytic habitable

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zone, pushing the boundaries of where life

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could exist beyond our traditional sun

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drenched views. It really makes you rethink

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what's possible out there.

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Avery: It certainly does. It's been a privilege to

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share all this incredible space and astronomy

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news with our listeners today. Don't forget,

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if you want more news and commentary from us,

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simply visit astronomydaily.IO.

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Anna: We hope you enjoyed exploring the cosmos with

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us on Astronomy Daily. Thank you for tuning

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in, and we look forward to sharing more

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cosmic insights with you in our next episode,

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which will be tomorrow, of course. Until

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then, keep looking up.
