WEBVTT

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<v Speaker 1>Welcome to Bedtime Astronomy. Explore the wonders of the cosmos

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<v Speaker 1>with our soothing Bedtime Astronomie podcast. Each episode offers a

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<v Speaker 1>gentle journey through the stars, planets, and beyond, perfect for

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<v Speaker 1>unwinding after a long day. Let's travel through the mysteries

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<v Speaker 1>of the universe as you drift off into a peaceful

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<v Speaker 1>slumber under the night sky.

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<v Speaker 2>Okay, let's unpack this.

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<v Speaker 3>Imagine looking up at the night sky and pointing to

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<v Speaker 3>a tiny, distant speck forty light years away and asking,

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<v Speaker 3>could there be liquid water? There? Could there be an atmosphere?

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<v Speaker 3>That's exactly the cosmic adventure we're embarking on today. We're

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<v Speaker 3>diving deep into the mystery surrounding an Earth sized exoplanet

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<v Speaker 3>that's been captivating scientists and stargazers alike. Our star for

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<v Speaker 3>this deep dive is trappist One, a world that scientists

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<v Speaker 3>sometimes just call a planet e. Our mission today is

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<v Speaker 3>to explore the central enigma of this fascinating world, the

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<v Speaker 3>potential for liquid water and the absolutely creal role of

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<v Speaker 3>an atmosphere in making that possibility a reality and helping

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<v Speaker 3>us unravel this cosmic puzzle, of course, is the incredible

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<v Speaker 3>eye in the sky NASA's James Webb Space Telescope for you.

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<v Speaker 3>This deep dive is a shortcut to understanding cutting edge astrophysics,

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<v Speaker 3>revealing surprising facts, and hopefully giving you those aha moments

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<v Speaker 3>about world far far beyond our own.

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<v Speaker 4>And what's really fascinating here is that this isn't just

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<v Speaker 4>about you know, spotting a distant spec It's about meticulously

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<v Speaker 4>piecing together the precise conditions that could support liquid water,

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<v Speaker 4>that most fundamentally ingredient for life as we know it. So, yeah,

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<v Speaker 4>we're going to explore how scientists are using the most

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<v Speaker 4>powerful telescope ever built to try and detect these all

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<v Speaker 4>these faint whispers of an atmosphere and what those whispers

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<v Speaker 4>or maybe their absence might tell us about this really

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<v Speaker 4>intriguing world. This journey into Trappist One is it's a

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<v Speaker 4>prime example of how science actually works. You know, you

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<v Speaker 4>have initial theories, then groundbreaking observations and new data, constantly

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<v Speaker 4>refining our understanding. It moves closer to answers off in

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<v Speaker 4>a very collaborative way, and it really challenges us to

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<v Speaker 4>reconsider what we think we know about potentially habitable environments.

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<v Speaker 3>So what exactly is this enigmatic planet E that has

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<v Speaker 3>scientists so incredibly excited.

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<v Speaker 2>Let's start there.

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<v Speaker 4>You know, when we talk about exoplanets, often we're dealing

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<v Speaker 4>with worlds that are just just barely detectable, think blips

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<v Speaker 4>in the data. But trapp Is One, well, it's an

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<v Speaker 4>Earth size exoplanet orbiting a star forty light years away.

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<v Speaker 4>Now forty light years sounds enormous, and it is something

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<v Speaker 4>like two hundred and thirty five trillion miles, but in

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<v Speaker 4>cosmic terms, that's practically our next door neighbor. This relative

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<v Speaker 4>proximity is exactly what makes it such a prime candidate

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<v Speaker 4>for the kind of detailed observation we're going to talk about.

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<v Speaker 3>Right, it's close enough to get a good look, relatively speaking,

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<v Speaker 3>And it's not just its closeness, is it. The whole

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<v Speaker 3>system it's in is pretty special.

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<v Speaker 4>Absolutely, Planet E isn't alone out there. It's one of

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<v Speaker 4>seven Earth sized planets all packed quite tightly around a

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<v Speaker 4>star called trapp Is One. Now trapp Is One isn't

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<v Speaker 4>like our sun at all. What we call a red

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<v Speaker 4>dwarf star, much smaller, much cooler, and dimmer than our

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<v Speaker 4>familiar yellow dwarf sun. Think about a star that's maybe

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<v Speaker 4>only about eight percent the mass of our Sun, barely

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<v Speaker 4>larger than the planet Jupiter. Wow, that's yeah, really small

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<v Speaker 4>for a star. And this means its habitable zone. You

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<v Speaker 4>know that Goldilocks region where liquid water can theoretically exist

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<v Speaker 4>on a planet's surface. Yeah, it's much much closer to

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<v Speaker 4>the star than Earth's orbit is around our Sun.

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<v Speaker 3>So Planet EE must be orbiting incredibly close to Trappis

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<v Speaker 3>one to be in that zone. Does that mean it

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<v Speaker 3>gets baked.

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<v Speaker 4>Or that's the interesting part. It is incredibly close. Planet

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<v Speaker 4>E whips around its star in just six point one

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<v Speaker 4>earth days.

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<v Speaker 2>That's its year, six days, six days.

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<v Speaker 4>Compare that to our three sixty five. But because Trappis

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<v Speaker 4>one is so much cooler, so much dimmer than our sun,

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<v Speaker 4>Plant E actually receives a similar amount of stellar energy

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<v Speaker 4>to Earth. So this puts it squarely within that critical

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<v Speaker 4>habitable zone. Temperatures are theoretically just right for liquid water,

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<v Speaker 4>not so hot it boils away, and not so cold

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<v Speaker 4>it's permanently frozen solid.

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<v Speaker 5>And it's this initial draw the potential for liquid water,

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<v Speaker 5>combined with its Earth like size, that immediately made Trappis

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<v Speaker 5>one a top tier target for well for astrobiology research.

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<v Speaker 3>Okay, so it ticks the big boxes, Earth sized in

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<v Speaker 3>the habitable zone. That sounds like the perfect recipe. But

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<v Speaker 3>you keep saying theoretical viability. What's the catch, what's the

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<v Speaker 3>big uncertainty?

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<v Speaker 5>You've nailed it.

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<v Speaker 4>That's the absolutely critical point and a common misconception when

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<v Speaker 4>people hear habitable zone. While Trappist one m really does

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<v Speaker 4>stand out its size, its position, the presence of liquid

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<v Speaker 4>water isn't guaranteed at all, not by a long shot.

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<v Speaker 4>It hinges entirely on one huge, still unanswered question, does

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<v Speaker 4>planet actually have an atmosphere?

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<v Speaker 3>Ah?

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<v Speaker 2>Right, the at.

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<v Speaker 5>Without an atmosphere, even in that sweet spot orbit, a

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<v Speaker 5>planet's surface conditions could be completely hostile. You'd get wild

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<v Speaker 5>temperature swings between the side facing the star and the

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<v Speaker 5>side facing away. Any surface water could just boil off

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<v Speaker 5>or freeze, or even subtle meate turns straight from mice

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<v Speaker 5>to gas and just get lost to space over time.

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<v Speaker 5>And this brings us right to the big mystery that

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<v Speaker 5>the astrophysicists at the University of Bristol and a large

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<v Speaker 5>international team are working so hard to solve. What this

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<v Speaker 5>really highlights for you the listener is that finding a

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<v Speaker 5>truly habitable world isn't just about location, location, location, It's

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<v Speaker 5>not just the orbital address. It's about understanding the atmosphere,

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<v Speaker 5>the planet's climate system. Really does it have one, what's

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<v Speaker 5>it made of? How does it act as a thermostat

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<v Speaker 5>and maybe a shield? That's what dictates if liquid water

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<v Speaker 5>can actually stick around. It's a delicate balance, and Planet

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<v Speaker 5>E is this fascinating test case that's really pushing our understanding.

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<v Speaker 3>It's truly astonishing that we can even try to detect

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<v Speaker 3>an atmosphere on a planet forty light years away. I mean,

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<v Speaker 3>how on Earth, or rather how off Earth does a

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<v Speaker 3>telescope like JWSTEAM manage that sifting through all that starlight?

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<v Speaker 2>What's the biggest challenge there?

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<v Speaker 5>It is an incredible feed, and you're right, the challenges

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<v Speaker 5>are immense. Think about it.

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<v Speaker 4>We're essentially trying to find the tiny chemical signature of

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<v Speaker 4>a planet's air, a world completely dwarfed by its star

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<v Speaker 4>from trillions of miles away. This is where NASA's James

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<v Speaker 4>Webspace Telescope, the JWST comes in. It's not just another telescope.

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<v Speaker 4>It's genuinely changing the game in exoplanet research. It's part

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<v Speaker 4>of a major international collaboration too. You can think of

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<v Speaker 4>it as humanity's most sensitive eye, specifically tuned to see

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<v Speaker 4>in the infrared to see what was previously hidden from us.

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<v Speaker 3>And it uses a specific instrument for this job, doesn't

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<v Speaker 3>it the ni RESPEC exactly.

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<v Speaker 4>Scientists are using one of JWST's workhorse instruments, ni I RESPEC,

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<v Speaker 4>the Near Infrared spectrographs NOW in I respect, isn't just

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<v Speaker 4>splitting light like a simple prism. It's incredibly sensitive and

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<v Speaker 4>specifically designed for the near infrared part of the spectrum,

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<v Speaker 4>and that's crucial because that's the wavelength range where molecules

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<v Speaker 4>we care about, like water, vapor, carbon dioxide, methane, leave

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<v Speaker 4>their most distinct chemical fingerprints.

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<v Speaker 2>Oh okay, and it's especially.

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<v Speaker 4>Vital for looking at planets around cool red dwarf stars

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<v Speaker 4>like trap Is to one, because these stars emit most

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<v Speaker 4>of their life in the infrared, so it means any

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<v Speaker 4>faint atmospheric signals are relatively speaking easier for JAST to

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<v Speaker 4>read against the star's background infrared light compared to trying

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<v Speaker 4>to see them invisible light, where a star like our

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<v Speaker 4>sun shines brightest. It's like having special glasses that filter

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<v Speaker 4>out everything except the exact chemical signatures you're looking for

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<v Speaker 4>cuts through the noise.

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<v Speaker 3>So how do they actually use enerspect to do this?

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<v Speaker 3>They can't just point it at the planet and see clouds,

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<v Speaker 3>can they?

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<v Speaker 4>No, not directly like that. It relies on a really

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<v Speaker 4>clever technique called the transit method. Picture this from our

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<v Speaker 4>viewpoint here on Earth, or rather from JWST's viewpoint in space.

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<v Speaker 4>Planet E occasionally passes directly in front of its host star,

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<v Speaker 4>Trappist One. This is called a transit. As it does,

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<v Speaker 4>it blocks a tiny, tiny fraction of the star's light,

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<v Speaker 4>causing a very slight dip in the star's overall brightness.

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<v Speaker 4>That's actually how we often find these exoplanets in.

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<v Speaker 5>The first place.

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<v Speaker 2>Okay, I've heard of that, the dip in's starlight, right.

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<v Speaker 4>But here's a really ingenious part for studying atmospheres. Just

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<v Speaker 4>as the planet starts to cross or finishes crossing, some

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<v Speaker 4>of the starlight grazes the edge of the planet. If

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<v Speaker 4>the planet has an atmosphere, that starlight passes through the

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<v Speaker 4>upper layers of that atmosphere on its way to us.

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<v Speaker 3>Ah.

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<v Speaker 2>Okay, the starlight gets.

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<v Speaker 5>Filtered, exactly filtered. The chemicals present in.

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<v Speaker 4>That atmosphere, if one exists, will absorb very specific wavelengths,

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<v Speaker 4>specific colors of that starlight. Every molecule like water or

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<v Speaker 4>CO two, has a unique absorption pattern, like a fingerprint

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<v Speaker 4>or barcode in the infrared spectrum. So by carefully analyzing

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<v Speaker 4>the starlight during these transits, using narspect to spread the

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<v Speaker 4>light into its full spectrum, astronomers can look for these

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<v Speaker 4>characteristic dips missing wavelengths within the starlight. Those dips tell

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<v Speaker 4>them precisely what chemicals are present in the planet's atmosphere.

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<v Speaker 4>It's incredibly precise. Work needs super stable instruments and long

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<v Speaker 4>observation times, and with each additional transit they observe. Each

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<v Speaker 4>time Planet E passes in front of the star and

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<v Speaker 4>JWST gathers more light, the signal gets stronger. The atmosphere

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<v Speaker 4>of contents, or indeed the lack of them, become clearer

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<v Speaker 4>and clearer. It's like building up a picture transit by transit,

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<v Speaker 4>adding more data points to map out what might be

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<v Speaker 4>a truly alien sky.

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<v Speaker 2>That's absolutely incredible.

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<v Speaker 3>It really sounds like the JAWST specific infrared capabilities are

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<v Speaker 3>the game changer here.

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<v Speaker 5>They truly are.

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<v Speaker 4>Doctor Hannah Wakeford, who is an associate professor in astrophysics

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<v Speaker 4>at the University of Bristol and a key member of

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<v Speaker 4>this JWST Transitting exoplanet team. She was instrumental in designing

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<v Speaker 4>the actual observational setup for the telescope. That kind of

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<v Speaker 4>meticulous planning is vital to make sure they get the

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<v Speaker 4>best possible data for these extremely delicate measurements. As doctor

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<v Speaker 4>Wayford herself put it, JWST's infrared instruments are providing unprecedented detail,

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<v Speaker 4>helping us understand much more about what determines the planet's

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<v Speaker 4>atmosphere and surface environment and what they're composed of.

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<v Speaker 2>You can really feel the excitement.

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<v Speaker 5>Oh absolutely.

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<v Speaker 4>She also said, it's incredibly exciting to be peeling back

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<v Speaker 4>the curtain on these fascinating other worlds, measuring the details

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<v Speaker 4>of starlight around Earth sized planets to ascertain what it

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<v Speaker 4>might be like if life could be possible.

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<v Speaker 3>Right.

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<v Speaker 4>As she mentioned, it's this careful process of elimination and

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<v Speaker 4>comparison that's leading to these great new insights really shifting

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<v Speaker 4>our understanding of planetary science. It's just a stunning testament

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<v Speaker 4>to human ingenuity, isn't it our drive to explore? Lets

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<v Speaker 4>us ask and now start to answer questions that we're

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<v Speaker 4>pure science fiction, just a generation to go, this technological

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<v Speaker 4>leap with JWST. It just pushes our cosmic reach further

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<v Speaker 4>than ever before, giving us these tantalizing glimpses into previously

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<v Speaker 4>inaccessible worlds.

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<v Speaker 3>So, after all that incredible BEATA collection, all that painstaking analysis,

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<v Speaker 3>what does it actually mean for planetes potential atmosphere? What

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<v Speaker 3>are the headlines coming out of these first observations the

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<v Speaker 3>big reveals.

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<v Speaker 4>Well, the initial results are now published actually across two

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<v Speaker 4>fevored papers in the Astrophysical Journal Letters. Yeah, well they're fascinating,

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<v Speaker 4>but also, as science often is quite nuanced and cautiously presented,

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<v Speaker 4>they're definitely what they call hints of an atmosphere. That's

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<v Speaker 4>a key.

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<v Speaker 2>Phrase, and it's okay, not a slam dunk yet.

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<v Speaker 4>Not a slam dunk now, to be really precise here,

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<v Speaker 4>as doctor Wakeford explained, the possibility that there's simply nothing there,

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<v Speaker 4>no significant atmosphere at all can't be completely ruled out

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<v Speaker 4>just yet based on this initial data. It's very much

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<v Speaker 4>a careful process of elimination like cosmic detective work unfolding

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<v Speaker 4>as we speak, comparing the data to different models. So

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<v Speaker 4>it's not a definitive yes or no right now, but

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<v Speaker 4>the picture is getting clearer, and crucially, we're starting to

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<v Speaker 4>understand what Planet EA's atmosphere isn't which is often just

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<v Speaker 4>as important in science.

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<v Speaker 2>Okay, so what isn't it?

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<v Speaker 3>What have they managed to definitively rule out with these

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<v Speaker 3>first JWST looks.

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<v Speaker 4>This is actually one of the most definitive findings so far,

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<v Speaker 4>real revelation. The researchers are pretty confident that planet E

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<v Speaker 4>does not have its original primordial atmosphere.

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<v Speaker 2>It's original atmosphere.

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<v Speaker 4>Yeah, this is a really crucial piece of the puzzle.

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<v Speaker 4>It immediately crosses off a major possibility and tells us

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<v Speaker 4>something fundamental about the planet's history and its environment. To

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<v Speaker 4>unpack that a bit, we're talking about what's called a

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<v Speaker 4>primordial hideen based atmosphere. This is basically the initial gas

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<v Speaker 4>envelope mostly hydrogen and helium that a planet gathers from

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<v Speaker 4>the disc it forms in. Think of it as the

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<v Speaker 4>leftover gas from the planet's birth cloud. These are thought

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<v Speaker 4>to be pretty common for young planets both gas giants

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<v Speaker 4>and rocky ones like Earth way back in the early

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<v Speaker 4>Solar System.

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<v Speaker 3>So like baby Earth might have had one of these

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<v Speaker 3>fluffy hydrogen atmospheres.

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<v Speaker 4>That's the idea, yes, But for Planet E, the JWST

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<v Speaker 4>data strongly suggests this isn't the case anywhere it's gone.

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<v Speaker 4>Doctor David Grant, who was a senior research associated Bristol

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<v Speaker 4>and a co author, explained why. He pointed out that

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<v Speaker 4>trappist One, the parent star, is a very active star

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<v Speaker 4>with frequent flares. Ah the star itself is the culprit.

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<v Speaker 4>It seems very likely these aren't just gentle flickers. They

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<v Speaker 4>are intense bursts of radiation, powerful stellar winds, high energy

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<v Speaker 4>particles blasting out from the star over billions of years.

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<v Speaker 4>This constant barrage, especially when the planet was young, would

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<v Speaker 4>have acted like a cosmic sand blaster.

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<v Speaker 5>It would have just.

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<v Speaker 4>Stripped off by stellar radiation. Any light easily removed gases

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<v Speaker 4>like hydrogen and helium, so that initial primordial atmosphere, if

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<v Speaker 4>it ever had one, would likely have been blown away

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<v Speaker 4>into space relatively early in the planet's history. It's a

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<v Speaker 4>harsh place to grow up orbardly.

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<v Speaker 3>Speaking, right, that makes sense A very active star would

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<v Speaker 3>make it hard to hold onto light gases. So if

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<v Speaker 3>it doesn't have its primordial atmosphere, does that just mean

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<v Speaker 3>it's a barren rock now or is there another possibility?

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<v Speaker 4>And this is where it gets really interesting and hopeful.

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<v Speaker 4>This leads us directly to the concept of a secondary atmosphere.

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<v Speaker 4>Doctor Wakeford pointed this out specifically. She noted many planets,

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<v Speaker 4>including Earth, build up a heavier secondary atmosphere after losing

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<v Speaker 4>their primary atmosphere.

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<v Speaker 2>Like Earth did.

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<v Speaker 4>Exactly like Earth did, our early hydrogen helium atmosphere was

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<v Speaker 4>lost too, but then over millions billions of years, processes

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<v Speaker 4>like volcanic outgasing released heavier gases from the planet's interior,

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<v Speaker 4>things like carbon dioxide, water, vapor, nitrogen, and then, of

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<v Speaker 4>course life eventually reshaped or atmosphere dramatically by adding oxygen.

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<v Speaker 4>The point is planets can generate a new atmosphere from within,

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<v Speaker 4>So this is the current frontier for Planet E. As

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<v Speaker 4>doctor Wakefort put it, it is possible Planet E was

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<v Speaker 4>never able to do this and doesn't have a secondary atmosphere,

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<v Speaker 4>but there's an equal chance one does exist. Ah, so

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<v Speaker 4>the jury is still out, but the possibility is definitely

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<v Speaker 4>there precisely while that initial hydrogen cloak is gone. The

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<v Speaker 4>chance that it generated a new heavier atmosphere, maybe rich

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<v Speaker 4>in CO two, maybe nitrogen, maybe even water vapor released

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<v Speaker 4>from its rocks and magma over time, that remains very

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<v Speaker 4>much an open question. The data doesn't rule it out.

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<v Speaker 4>It really is like that detective analogy, figuring out what's

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<v Speaker 4>not there. The primordial atmosphere is just as important for

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<v Speaker 4>narrowing down the possibilities as finding clues about what might

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<v Speaker 4>be there. And it also really underscores how dynamic these

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<v Speaker 4>stellar environments are, especially around these active red dwarfs. They

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<v Speaker 4>can completely reshape a planet's atmospheric destiny. It's not a

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<v Speaker 4>static picture. It's an ongoing cosmic drama of atmospheric survival.

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<v Speaker 3>Okay, So if Planet E does manage to have that

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<v Speaker 3>secondary atmosphere, that heavier one, what's the next domino to

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<v Speaker 3>fall in this whole cosmic puzzle. Does that automatically mean

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<v Speaker 3>liquid water because that seems to be the holy grail here.

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<v Speaker 4>That's exactly right. The potential for liquid water is the

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<v Speaker 4>next crucial link in the chain. And yes, if a

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<v Speaker 4>secondary atmosphere exists, then liquid water could certainly persist on

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<v Speaker 4>the surface, and if that's the case, researchers are pretty

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<v Speaker 4>confident it would almost certainly require and be accompanied by

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<v Speaker 4>a greenhouse effect, something basically similar in principle to what

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<v Speaker 4>happens here on Earth.

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<v Speaker 2>The greenhouse effect keeping it warm enough.

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<v Speaker 4>Exactly certain gases in that atmosphere. Carbon dioxide is a

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<v Speaker 4>prime candidate, but maybe methane or water vapor too, would

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<v Speaker 4>trap some of the heat radiating for the planet's surface,

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<v Speaker 4>heat that originally came from the star. This trapped heat

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<v Speaker 4>keeps the planet warmer than it would be otherwise, and

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<v Speaker 4>critically it helps stabilize the temperature, ending all the water

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<v Speaker 4>from just freezing solid or boiling away instantly. Without a

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<v Speaker 4>reasonably significant greenhouse effect, even with an atmosphere, the average

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<v Speaker 4>surface temperature might just be too low for liquid water,

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<v Speaker 4>or you'd get such extreme temperature swings between the day

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<v Speaker 4>and night sides that water couldn't remain liquid reliably.

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<v Speaker 3>Now, when we hear a greenhouse effect, a lot of

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<v Speaker 3>us immediately picture Venus right with that incredibly thick runaway

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<v Speaker 3>carbon dioxide atmosphere and surface temperatures hot enough to melt lead.

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<v Speaker 2>Is that the kind of scenario we might be looking

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<v Speaker 2>at for Planet E.

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<v Speaker 4>That's a really important question, and it's vital we add

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<v Speaker 4>some nuance there. The lead author on the theoretical interpretation paper,

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<v Speaker 4>doctor Anna Glidden from MIT, specifically addressed this. She explained

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<v Speaker 4>that based on their modeling and the current data, it

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<v Speaker 4>is unlikely the atmosphere of planet E is dominated by

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<v Speaker 4>carbon dioxide like the thick atmosphere of Venus and the

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<v Speaker 4>thin atmosphere of Mars.

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<v Speaker 2>Okay, so not like Venus, whew, and not like Mars either.

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<v Speaker 4>Apparently not dominated by CO two in the way either

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<v Speaker 4>of those are, which suggests something potentially different. Doctor Glidden

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<v Speaker 4>also emphasized, but it's also important to note there are

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<v Speaker 4>no direct parallels with our solar system. Trappist One is

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<v Speaker 4>a very different star from our Sun, and the planetary

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<v Speaker 4>system around it is also distinct. That's a really key takeaway.

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<v Speaker 4>We're dealing with an alien solar system, an alien star.

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<v Speaker 4>We shouldn't expect things to look exactly like Earth, Venus

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<v Speaker 4>or Mars. The conditions, the history, the chemistry could all

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<v Speaker 4>be unique.

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<v Speaker 3>Okay, so maybe not Venus like, maybe not Mars like,

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<v Speaker 3>but some CO two could still be really important, couldn't

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<v Speaker 3>it for that warming effect?

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<v Speaker 4>Precisely, even if CO two isn't the main component, it

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<v Speaker 4>could still play that crucial greenhouse role. And doctor Wakeford

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<v Speaker 4>added a very encouraging detail on this point. She said,

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<v Speaker 4>a little greenhouse effect can go a long way. And

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<v Speaker 4>the new measurements do not rule out sufficient carbon dioxide

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<v Speaker 4>to sustain some liquid water on the surface.

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<v Speaker 2>Ah not ruled out. That sounds significant.

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<v Speaker 4>It is significant in scientific terms. It means the observations

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<v Speaker 4>we have so far are still perfectly consistent, whether it

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<v Speaker 4>being enough CO two or perhaps other greenhouse gases to

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<v Speaker 4>keep the surface temperature above freezing at least in some places.

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<v Speaker 4>It means the possibility of liquid water enabled by a

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<v Speaker 4>modest greenhouse effect remains firmly on the table based on

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<v Speaker 4>this initial JWST data. That's a major step forward. Now,

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<v Speaker 4>let's just imagine for a second what that liquid water

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<v Speaker 4>might actually look like on such a well, such a

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<v Speaker 4>unique world. Because it might not be a global ocean

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<v Speaker 4>like Earth's, the water could potentially take one of two

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<v Speaker 4>main forms. Maybe it is a global ocean covering most

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<v Speaker 4>of the planet, a true water world, or and this

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<v Speaker 4>is where the unique environment that the system really comes

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<v Speaker 4>into play, the water might only cover a smaller specific area,

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<v Speaker 4>perhaps a region where the star is at perpetual noon

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<v Speaker 4>surrounded by ice.

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<v Speaker 2>Perpetual noon surrounded by ice.

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<v Speaker 3>That sounds incredibly bizarre, like an eyeball staring at the star.

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<v Speaker 2>I think I've heard that term eyeball planet.

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<v Speaker 4>That's exactly the concept the eyeball, or sometimes lava lamp

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<v Speaker 4>ocean configuration, and as a direct consequence of something called

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<v Speaker 4>tidal locking.

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<v Speaker 2>Tidal locking like our moon.

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<v Speaker 4>Decisely like our moon because the trapis one planets are

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<v Speaker 4>relatively large compared to their small star, and because the

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<v Speaker 4>orbits so incredibly close, the star's gravity has locked their rotation.

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<v Speaker 4>What this means is that one side of Planet E

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<v Speaker 4>always faces the star, experiencing perpetual daylight, while the other

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<v Speaker 4>side is permanently turned away, plunged into perpetual darkness and cold.

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<v Speaker 3>Wow, a permanent day side and a permanent night side.

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<v Speaker 4>Exactly Unlike Earth, which rotates, distributing heat more evenly, Planet

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<v Speaker 4>E would have this stark contrast. So if liquid water exists,

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<v Speaker 4>the most likely place for it to pool and persist

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<v Speaker 4>would be on that permanently warm day side. Maybe concentrated

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<v Speaker 4>near the point directly facing the star, the substellar point.

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<v Speaker 4>This could form that eyeball ocean, a large patch of

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<v Speaker 4>liquid water facing the star, potentially surrounded by glaciers, or

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<v Speaker 4>a vast frozen ice sheet covering the twilight zones and

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<v Speaker 4>the entire dark side.

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<v Speaker 3>That paints such a drastically alien picture, not Earth two

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<v Speaker 3>point zero, but something entirely different. What would the conditions

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<v Speaker 3>even be like near that ocean?

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00:20:02.960 --> 00:20:08.400
<v Speaker 4>Oh, incredibly dramatic. Most likely imagine constant, perhaps hurricane force

402
00:20:08.480 --> 00:20:11.640
<v Speaker 4>winds blowing from the hottest point under the star towards

403
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<v Speaker 4>the colder twilight regions and the night side. Driven by

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00:20:14.799 --> 00:20:18.599
<v Speaker 4>that massive temperature difference. These winds would likely drive strong

405
00:20:18.680 --> 00:20:22.440
<v Speaker 4>ocean currents. Within that eyeball sea. You might have intensive

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<v Speaker 4>operation under the star, leading to thick clouds, maybe perpetual

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<v Speaker 4>rain or snow in the transition zones. The terminator line,

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<v Speaker 4>that ring of perpetual twilight between the day and night

409
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<v Speaker 4>sides could be a really interesting zone. Maybe temperatures there

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<v Speaker 4>are more stable, more clement.

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<v Speaker 3>It really forces you to think outside the box about

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<v Speaker 3>what habitable even means, doesn't it.

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<v Speaker 4>It absolutely does? How would life adapt could something live

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<v Speaker 4>in the boiling center or the freezing edges, or find

415
00:20:46.359 --> 00:20:49.759
<v Speaker 4>a niche in that twilight zone. Maybe life exists under

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<v Speaker 4>the ice on the dark side, warmed by geothermal heat.

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<v Speaker 4>The fact that these initial Jawst findings are still consistent

418
00:20:57.119 --> 00:21:00.000
<v Speaker 4>with enough greenhouse gases to make any surface liquid water

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<v Speaker 4>are possible even in this strange eyeball configuration is what

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<v Speaker 4>keeps scientists so incredibly engaged. It challenges all our earth

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<v Speaker 4>centric biases about what a habitable world must look like.

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<v Speaker 4>It really broadens our perspective on the sheer variety of

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<v Speaker 4>potentially life bearing environments the universe might offer.

424
00:21:17.680 --> 00:21:19.839
<v Speaker 3>This really does feel like just the beginning, doesn't it.

425
00:21:19.880 --> 00:21:22.519
<v Speaker 3>This deep dive into Trappis one m is clearly far

426
00:21:22.599 --> 00:21:25.640
<v Speaker 3>from over. These initial findings, these hints are just paving

427
00:21:25.640 --> 00:21:27.200
<v Speaker 3>the way for more. It feels like we found the

428
00:21:27.240 --> 00:21:31.359
<v Speaker 3>first few pieces of this incredibly complex and captivating cosmic puzzle.

429
00:21:31.759 --> 00:21:34.359
<v Speaker 3>But maybe those pieces just raise even more questions. So

430
00:21:34.599 --> 00:21:37.160
<v Speaker 3>what's next? What's on the cosmic research agenda for Planet E?

431
00:21:37.440 --> 00:21:40.359
<v Speaker 4>You're absolutely right, this is very much just the first chapter.

432
00:21:40.759 --> 00:21:44.319
<v Speaker 4>The quest to understand Planet E is an ongoing process.

433
00:21:44.680 --> 00:21:49.440
<v Speaker 4>The immediate next steps involved well more data, more observations

434
00:21:49.519 --> 00:21:52.440
<v Speaker 4>they need to build on these initial four transit observations.

435
00:21:52.680 --> 00:21:55.039
<v Speaker 4>The more times they can watch planet ePass in front

436
00:21:55.039 --> 00:21:57.720
<v Speaker 4>of trap this one, the more starlight they collect passing

437
00:21:57.799 --> 00:22:00.720
<v Speaker 4>through its potential atmosphere. This will strain than the signal

438
00:22:00.920 --> 00:22:03.720
<v Speaker 4>or perhaps show its absence more clearly. It will allow

439
00:22:03.759 --> 00:22:06.720
<v Speaker 4>scientists to confirm or deny the presence of that secondary

440
00:22:06.720 --> 00:22:10.319
<v Speaker 4>atmosphere with much greater confidence and hopefully start to really

441
00:22:10.319 --> 00:22:13.519
<v Speaker 4>pin down its composition what is it made of? But crucially,

442
00:22:13.839 --> 00:22:15.680
<v Speaker 4>it's not just about staring at Planet E.

443
00:22:15.839 --> 00:22:16.519
<v Speaker 5>They will also.

444
00:22:16.359 --> 00:22:19.279
<v Speaker 4>Compare its data very closely with data from another planet

445
00:22:19.279 --> 00:22:20.759
<v Speaker 4>in the same system, Trappist one B.

446
00:22:21.039 --> 00:22:23.440
<v Speaker 2>Planet B, the one even closer to the star.

447
00:22:23.720 --> 00:22:26.440
<v Speaker 4>That's the one Planet B orbits closest to the star,

448
00:22:26.799 --> 00:22:30.079
<v Speaker 4>so it gets blasted with even more intense radiation. It's

449
00:22:30.160 --> 00:22:32.359
<v Speaker 4>likely lost any atmosphere it might have had, even more

450
00:22:32.400 --> 00:22:36.400
<v Speaker 4>readily than Planet E. By comparing the atmospheric signals or

451
00:22:36.480 --> 00:22:39.440
<v Speaker 4>lack thereof, from both planet B and Planet E, scientists

452
00:22:39.440 --> 00:22:41.839
<v Speaker 4>can get a much better handle on the processes of

453
00:22:41.880 --> 00:22:45.240
<v Speaker 4>atmospheric loss and retention across the whole system. How does

454
00:22:45.240 --> 00:22:48.920
<v Speaker 4>this star's activity affect planets at different distances. This kind

455
00:22:48.960 --> 00:22:52.920
<v Speaker 4>of comparative exoplanetology, studying multiple planets in the same system

456
00:22:53.079 --> 00:22:56.599
<v Speaker 4>is incredibly powerful. It gives context. It will provide really

457
00:22:56.720 --> 00:23:00.400
<v Speaker 4>nuanced insights, not just a planet E's potential habitability, but

458
00:23:00.480 --> 00:23:03.920
<v Speaker 4>about how these common red dwarf stars shape the world's

459
00:23:04.039 --> 00:23:06.880
<v Speaker 4>orbiting them. It's like having multiple experiments running in the

460
00:23:06.880 --> 00:23:07.799
<v Speaker 4>same cosmic lab.

461
00:23:07.880 --> 00:23:10.759
<v Speaker 3>That sounds like a truly monumental undertaking. It must involve

462
00:23:10.799 --> 00:23:13.119
<v Speaker 3>a huge team. Who are the people behind this kind

463
00:23:13.200 --> 00:23:15.200
<v Speaker 3>of groundbreaking research.

464
00:23:15.799 --> 00:23:19.319
<v Speaker 4>It really does highlight the scale and the collaborative nature

465
00:23:19.440 --> 00:23:23.960
<v Speaker 4>of modern astrophysics. Doctor Nestor Espinoza, who's an associate astronomer

466
00:23:23.960 --> 00:23:27.079
<v Speaker 4>at the Space Telescope Science Institute, the place that operates

467
00:23:27.200 --> 00:23:30.720
<v Speaker 4>JWST and one of the principal investigators focusing on trappis

468
00:23:30.799 --> 00:23:35.319
<v Speaker 4>one he emphasized this. He said, web's infrared instruments are

469
00:23:35.359 --> 00:23:38.519
<v Speaker 4>giving us more detail than we've ever had access to before,

470
00:23:38.680 --> 00:23:41.240
<v Speaker 4>and the initial four observations we've been able to make

471
00:23:41.240 --> 00:23:43.680
<v Speaker 4>of planet E are showing us what we will have

472
00:23:43.720 --> 00:23:46.160
<v Speaker 4>to work with when the rest of the information comes in.

473
00:23:47.880 --> 00:23:50.960
<v Speaker 4>That clearly indicates this is a planned, long term campaign.

474
00:23:51.240 --> 00:23:54.119
<v Speaker 4>They knew the first look would be suggestive, maybe not definitive,

475
00:23:54.400 --> 00:23:55.759
<v Speaker 4>and they're ready to gather the rest of.

476
00:23:55.759 --> 00:23:56.480
<v Speaker 5>The data needed.

477
00:23:56.599 --> 00:23:58.200
<v Speaker 2>It's part of a bigger program.

478
00:23:57.839 --> 00:23:58.200
<v Speaker 3>Isn't it?

479
00:23:58.319 --> 00:24:01.200
<v Speaker 5>Yes, exactly, The whole problem is part of a larger

480
00:24:01.279 --> 00:24:05.839
<v Speaker 5>JWST initiative called the Dreams program that stands for trappis

481
00:24:05.880 --> 00:24:10.119
<v Speaker 5>one m survey team detailed research for exoplanetary atmospheres and

482
00:24:10.160 --> 00:24:11.240
<v Speaker 5>mass loss studies.

483
00:24:11.559 --> 00:24:14.759
<v Speaker 4>Quite a mouthful. It's a massive collaborative effort led by

484
00:24:14.759 --> 00:24:18.279
<v Speaker 4>doctor Nicole Lewis, who's an associate professor over at Cornell University,

485
00:24:18.559 --> 00:24:21.960
<v Speaker 4>and it's truly international. We're talking more than thirty scientists

486
00:24:22.000 --> 00:24:25.680
<v Speaker 4>involved from the UK, the US and India, including, as

487
00:24:25.680 --> 00:24:28.519
<v Speaker 4>you might expect, several current and former members of doctor

488
00:24:28.519 --> 00:24:31.920
<v Speaker 4>Wakeford's team at Bristol. It really showcases that global effort

489
00:24:32.000 --> 00:24:33.440
<v Speaker 4>needed to tackle these big questions.

490
00:24:33.599 --> 00:24:35.839
<v Speaker 3>And this team they have a pretty strong track record

491
00:24:35.880 --> 00:24:38.119
<v Speaker 3>already with JWST, don't they. I think I remember hearing

492
00:24:38.119 --> 00:24:39.839
<v Speaker 3>about another big discovery they made.

493
00:24:39.960 --> 00:24:42.400
<v Speaker 5>You're absolutely right. This group has already made headlines. They

494
00:24:42.440 --> 00:24:45.839
<v Speaker 5>had that breakthrough detection of quartz clouds made of tiny

495
00:24:46.039 --> 00:24:48.880
<v Speaker 5>sand like particles in the atmosphere of a different, very

496
00:24:48.920 --> 00:24:51.960
<v Speaker 5>hot exoplanet that was published back in twenty twenty three

497
00:24:52.440 --> 00:24:54.920
<v Speaker 5>study led by doctor Grant, the same research we mentioned

498
00:24:54.960 --> 00:24:58.160
<v Speaker 5>earlier and co authored by doctor Wakeford. So yes, this

499
00:24:58.319 --> 00:25:01.680
<v Speaker 5>prior success really underscore the caliber of the team and

500
00:25:01.839 --> 00:25:06.279
<v Speaker 5>again the incredible transformative power of JWST itself. It shows

501
00:25:06.519 --> 00:25:09.000
<v Speaker 5>they know how to use this instrument to tease out

502
00:25:09.039 --> 00:25:12.319
<v Speaker 5>really difficult signals. It reinforces that we're not just passively

503
00:25:12.319 --> 00:25:14.960
<v Speaker 5>looking anymore. We're actively pushing the boundaries of what we

504
00:25:15.000 --> 00:25:18.559
<v Speaker 5>can detect and understand about these alien atmospheres. And it's

505
00:25:18.599 --> 00:25:21.759
<v Speaker 5>always worth remembering the bigger picture of JWST itself. It's

506
00:25:21.759 --> 00:25:25.119
<v Speaker 5>the world's premiere space science observatory right now. Its mission

507
00:25:25.160 --> 00:25:29.319
<v Speaker 5>is broad distant galaxies star formation probing the universe's mysteries,

508
00:25:29.799 --> 00:25:32.119
<v Speaker 5>but studying exoplanets is a huge part of that, and

509
00:25:32.200 --> 00:25:35.240
<v Speaker 5>it's an international program, NASA, the European Space Agency, the

510
00:25:35.240 --> 00:25:38.440
<v Speaker 5>Canadian Space Agency all working together. The whole Trappist one

511
00:25:38.559 --> 00:25:41.720
<v Speaker 5>M story is just a fantastic example of this global

512
00:25:41.759 --> 00:25:45.720
<v Speaker 5>scientific cooperation, constantly pushing the frontiers of discovery and revealing

513
00:25:45.759 --> 00:25:48.440
<v Speaker 5>bit by bit just how much richer and more complex

514
00:25:48.480 --> 00:25:51.319
<v Speaker 5>the universe is than we ever imagined. Each new piece

515
00:25:51.359 --> 00:25:53.440
<v Speaker 5>of data really does bring us a little closer to

516
00:25:53.519 --> 00:25:55.160
<v Speaker 5>understanding our own place within it all.

517
00:25:55.359 --> 00:25:58.839
<v Speaker 3>So we've journeyed forty light years in our minds today,

518
00:25:58.920 --> 00:26:02.640
<v Speaker 3>peered through starlight using the most advanced telescope humanity has

519
00:26:02.680 --> 00:26:06.359
<v Speaker 3>ever built, and we found these compelling hints, this tantalizing clues,

520
00:26:06.400 --> 00:26:10.319
<v Speaker 3>clues that an Earth's size exoplanet Trapeze T one might

521
00:26:10.400 --> 00:26:12.920
<v Speaker 3>just hold on to a secondary atmosphere, and if it

522
00:26:12.960 --> 00:26:15.680
<v Speaker 3>does well, then the potential for liquid water follows, maybe

523
00:26:15.680 --> 00:26:19.559
<v Speaker 3>a global ocean, maybe that strange sunkissed eyeballpool on a

524
00:26:19.599 --> 00:26:22.559
<v Speaker 3>tidally locked world. This isn't just a story about a

525
00:26:22.559 --> 00:26:25.720
<v Speaker 3>distant planet, is. It feels like a testament to human curiosity,

526
00:26:25.759 --> 00:26:28.000
<v Speaker 3>to our ingeneviity. It really reminds us that we are

527
00:26:28.039 --> 00:26:32.000
<v Speaker 3>living in a golden age of cosmic exploration, constantly redefining

528
00:26:32.000 --> 00:26:34.759
<v Speaker 3>what's possible to find out there. Science fiction is literally

529
00:26:34.799 --> 00:26:36.640
<v Speaker 3>becoming science fact before our eyes.

530
00:26:36.880 --> 00:26:39.839
<v Speaker 4>And what's truly fascinating here, I think, is how these discoveries,

531
00:26:40.000 --> 00:26:43.799
<v Speaker 4>even these tentative hints from worlds like Trappist one, they

532
00:26:43.839 --> 00:26:46.720
<v Speaker 4>really compel us to rethink our most basic assumptions about

533
00:26:46.720 --> 00:26:49.559
<v Speaker 4>where life could emerge in what forms it might take.

534
00:26:50.480 --> 00:26:53.880
<v Speaker 4>If a tidally locked planet orbiting a volatile red dwarf

535
00:26:53.960 --> 00:26:58.039
<v Speaker 4>star can potentially sustain liquid water, perhaps in a configuration

536
00:26:58.160 --> 00:27:03.559
<v Speaker 4>totally unlike Earth, well, what other completely unexpected possibilities will

537
00:27:03.640 --> 00:27:08.799
<v Speaker 4>JWST uncover next out there in the vastness, And ultimately,

538
00:27:08.880 --> 00:27:10.920
<v Speaker 4>what does that tell us about our own unique or

539
00:27:10.960 --> 00:27:13.920
<v Speaker 4>perhaps not so unique place in the cosmos. It forces

540
00:27:14.000 --> 00:27:16.720
<v Speaker 4>us to broaden that definition of habitable in ways we

541
00:27:16.759 --> 00:27:19.440
<v Speaker 4>probably haven't even conceived of yet. It's a profound question

542
00:27:19.480 --> 00:27:20.400
<v Speaker 4>to ponder.

543
00:27:20.119 --> 00:27:22.720
<v Speaker 3>Absolutely our really powerful thought to end on. Thank you

544
00:27:22.799 --> 00:27:25.279
<v Speaker 3>so much for sharing your expertise on this deep dive today,

545
00:27:25.319 --> 00:27:27.480
<v Speaker 3>and thank you our listener for joining us. Keep looking up,

546
00:27:27.559 --> 00:27:29.359
<v Speaker 3>keen asking those big questions, and we'll see you on

547
00:27:29.400 --> 00:28:36.960
<v Speaker 3>the next cosmic Adventuress.

548
00:28:06.559 --> 00:28:35.519
<v Speaker 6>Says said

549
00:36:00.039 --> 00:36:10.039
<v Speaker 2>Yousssssss
