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>I want you to take a second and picture the

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<v Speaker 2>physics of just a regular, everyday morning fog.

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<v Speaker 3>Sure, just you know, a standard terrestrial weather thing.

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<v Speaker 2>Right, So you wake up, you look out the window,

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<v Speaker 2>and the ambient temperature overnight has dropped just enough to

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<v Speaker 2>push the local humidity past its dew point exactly.

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<v Speaker 3>The water vapor in the air condenses into this thick,

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<v Speaker 3>low lying cloud.

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<v Speaker 2>Yeah, and it's quiet, it's very localized. But then a

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<v Speaker 2>few hours later, the morning sun comes up, raises the temperature,

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<v Speaker 2>and the water sublimates right back into.

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<v Speaker 3>Gas, and the fog just vanishes. A really narrow thermal gradient.

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<v Speaker 3>We're talking what maybe a ten or fifteen degree difference

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<v Speaker 3>between the night and the day.

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<v Speaker 2>Right. It happens so easily here on Earth that we

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<v Speaker 2>barely even think about the mechanics of it, we just

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<v Speaker 2>call it weather exactly, but I want you to keep

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<v Speaker 2>that mechanism in mind and then scale it up to

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<v Speaker 2>an absolute planetary extreme.

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<v Speaker 3>Oh man, Yeah, this is where it gets wild.

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<v Speaker 2>Imagine that the suspended particles in that fog aren't liquid water.

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<v Speaker 2>They are vaporized.

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<v Speaker 3>Rock, specifically magnesium silicate, literally vaporized sand.

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<v Speaker 2>Right, And the temperature gradient that burns off this morning

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<v Speaker 2>fog isn't just a gentle sunrise. It is a one

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<v Speaker 2>thousand degree blast of extreme stellar.

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<v Speaker 3>Radiation, which is just I mean, the energy required to

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<v Speaker 3>vaporize a planetary wall of solidifying rock in a few

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<v Speaker 3>hours is staggering. It completely changes how we think about

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<v Speaker 3>atmospheric violence.

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<v Speaker 2>And that sheer atmospheric violence is exactly what we're focusing

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<v Speaker 2>on today because for decades as ronomers have been staring

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<v Speaker 2>at these distant worlds trying to figure out what they're

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<v Speaker 2>made of.

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<v Speaker 3>Yeah, relying on spectroscopy to read the chemical signatures, but.

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<v Speaker 2>They've been blocked by this incredibly mundane physical problem alien clouds.

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<v Speaker 3>Yeah, the fog in the way exactly.

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<v Speaker 2>It's been this massive thorn in the side of planetary scientists.

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<v Speaker 2>But recently there has been this monumental breakthrough.

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<v Speaker 3>We finally figured out how to wipe the fog off

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<v Speaker 3>the window.

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<v Speaker 2>Right, and the target that allowed us to do this

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<v Speaker 2>is a gas giant known as OBSP ninety four.

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<v Speaker 3>AB WSP ninety four AB. Yeah, it's located in the

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<v Speaker 3>Microscopium constellation, roughly seven hundred light years away from us, and.

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<v Speaker 2>It falls into that classic category we call a hot jupiter.

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<v Speaker 3>Which basically means it orbits incredibly close to its host star.

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<v Speaker 3>It's constantly getting blasted by radiation, and it's tidally locked.

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<v Speaker 2>Okay, so tidally locked, meaning one side of the planet

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<v Speaker 2>is always facing the star.

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<v Speaker 3>Right right, you have a permanent day side that is

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<v Speaker 3>just getting baked and a prominent night side that is

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<v Speaker 3>constantly radiating its heat out into the cold vacuum of space.

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<v Speaker 2>And that intense temperature difference is the engine for this

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<v Speaker 2>whole fog problem. But to really appreciate how big of

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<v Speaker 2>a deal this new discovery is, we have to look

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<v Speaker 2>back at the last twenty years.

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<v Speaker 3>The whole foggy window era of astronomy.

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<v Speaker 2>Right, because general cloudiness has basically stalled our ability to

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<v Speaker 2>study the atmospheres of these hot.

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<v Speaker 3>Jupiters, it really did. I mean the way we study

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<v Speaker 3>these exoplanets is through transmission spectroscopy.

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<v Speaker 2>Right, the telescope breeds the starlight.

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<v Speaker 3>Exactly when the planet transits or you know, passes in

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<v Speaker 3>front of its star. The starlight filters through the very

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<v Speaker 3>edge of the planet's atmosphere like a halo. Yeah, exactly,

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<v Speaker 3>an annulus of gas. And as the light passes through

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<v Speaker 3>different chemicals like sodium or water or carbon monoxide, they

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<v Speaker 3>absorb specific wavelengths of that light.

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<v Speaker 2>And then we catch that light in our telescopes and

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<v Speaker 2>basically look at what's missing to figure out the recipe

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<v Speaker 2>of the atmosphere.

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<v Speaker 3>Which works flawlessly, assuming of course, that the atmosphere is

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<v Speaker 3>made of transparent gases.

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<v Speaker 2>Which brings us back to the fog. So think of

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<v Speaker 2>it like this. Imagine you're standing across the street.

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<v Speaker 3>From a diner, okay, a diner, Yeah, and.

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<v Speaker 2>You're trying to appreciate the super fine details of a

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<v Speaker 2>masterpiece painting hanging on the back wall inside that diner.

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<v Speaker 2>You know, the painting is there, you can get the

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<v Speaker 2>general shapes, but the diner window is completely steamed up

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<v Speaker 2>with condensation.

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<v Speaker 3>Oh that's a great way to put it.

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<v Speaker 2>The crucial details are totally hidden because the light from

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<v Speaker 2>the diner gets scrambled before it reaches you.

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<v Speaker 3>In physics we call that me scattering the droplets of condensation,

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<v Speaker 3>or in the case of these planets, the high altitude clouds,

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<v Speaker 3>they literally scatter the photons.

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<v Speaker 2>So the telescope doesn't see the painting.

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<v Speaker 3>No, it just reads the chemical signature of the steamed

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<v Speaker 3>up window. It just reads the cloud layer.

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<v Speaker 2>And for a long time, the best tool we had

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<v Speaker 2>for this was the Hubble Space Telescope, which you know

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<v Speaker 2>is an absolute marvel of engineer.

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<v Speaker 3>Oh absolutely, But Hubble had a very specific limitation when

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<v Speaker 3>it came to this cloudy window problem.

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<v Speaker 2>Right the wide field camera three.

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<v Speaker 3>Yeah, when researchers pointed Hubble at these hot jupiters, they

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<v Speaker 3>expected to see these nice deep absorption lines for things

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<v Speaker 3>like water vapor.

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<v Speaker 2>But instead the data just came back completely.

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<v Speaker 3>Flat muted because it was just hitting that opaque, gray

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<v Speaker 3>wall of high altitude clouds. Hubble was basically just skimming

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<v Speaker 3>the tops of the cloud decks.

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<v Speaker 2>And the real issue wasn't just that Hubble couldn't see

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<v Speaker 2>through the clouds, it was how it collected the data right,

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<v Speaker 2>it provided this averaged view, yes.

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<v Speaker 3>The spatial integration. That's the technical term for the squish,

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<v Speaker 3>the squishing right.

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<v Speaker 2>Hubble lacked the precision to slice up the data over time,

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<v Speaker 2>so when it looked at the planet passing in front

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<v Speaker 2>of the star, it just took all the light from

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<v Speaker 2>the entire atmosphere mashed it together into one single data point.

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<v Speaker 3>It convolved it so if one side of the planet

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<v Speaker 3>was completely blocked by clouds, that opacity basically watered down

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<v Speaker 3>the data for the entire planet.

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<v Speaker 2>It's like taking a really comple like symphony audio track.

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<v Speaker 2>You've got this delicate string section and then a super

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<v Speaker 2>loud brass section, right, and you just compress the whole

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<v Speaker 2>thing down to a single mono channel with heavy distortion.

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<v Speaker 2>You totally lose the violins because the brass just overrides everything.

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<v Speaker 3>And that's exactly what was happening to our atmospheric models.

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<v Speaker 3>We were building our understanding of these planets based on

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<v Speaker 3>this muddy, compressed data.

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<v Speaker 2>Which was incredibly frustrating. I mean, we were staring at

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<v Speaker 2>a steamed up window for two decades. We needed a

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<v Speaker 2>better tool to isolate the different parts of the atmosphere.

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<v Speaker 3>Enter the James Web Space Telescope JWST.

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<v Speaker 2>Yes, the James Web. This is where everything changes because

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<v Speaker 2>JWST didn't just give us a bigger mirror.

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<v Speaker 3>No, it gave us than your infrared spectrograph, the NIRSpec

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<v Speaker 3>and crucially the temporal resolution.

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<v Speaker 2>The ability to track the light perfectly over time, which

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<v Speaker 2>allowed astronomers to do something basically magical. They watched mcguoy's

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<v Speaker 2>pay ninety four AB pass directly in front of.

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<v Speaker 3>Its star, and instead of mashing all the light together

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<v Speaker 3>like Hubble did, they sliced it.

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<v Speaker 2>Okay, but I have to stop you here. I want

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<v Speaker 2>to play Devil's advocate for the listener for a second.

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<v Speaker 3>Go for it.

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<v Speaker 2>This planet is seven hundred light years away from us. Yep.

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<v Speaker 2>From our perspective, it is a sub microscopic speck. It

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<v Speaker 2>doesn't even look like a disk in the telescope, righty.

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<v Speaker 3>It's essentially just a single pixel of light dipping slightly

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<v Speaker 3>in brightness.

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<v Speaker 2>So how on earth is it physically possible to isolate

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<v Speaker 2>the morning weather from the evening weather on a literal.

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<v Speaker 3>Spec It sounds impossible, right, But it all comes down

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<v Speaker 3>to the ingenious geometry of a transit. Let's break down

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<v Speaker 3>how JWST actually reads the leading edge and the trailing edge.

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<v Speaker 2>Okay, the anatomy of the transit walks through it.

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<v Speaker 3>So when Wastpai ninety for ab first begins to cross

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<v Speaker 3>in front of the star, the very first part of

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<v Speaker 3>the planet's atmosphere to get back lit by the starlight

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<v Speaker 3>is the leading edge.

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<v Speaker 2>The front of the planet, essentially.

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<v Speaker 3>Exactly, And because the planet is tidally locked, that leading

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<v Speaker 3>edge represents a very specific atmospheric zone. It's the region

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<v Speaker 3>where the winds are blowing from the dark, freezing night

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<v Speaker 3>side across the terminator into the blazing heat of the

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<v Speaker 3>day side.

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<v Speaker 2>Okay, so the air is moving from night to day.

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<v Speaker 2>That's a sunrise.

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<v Speaker 3>That's the alien morning.

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<v Speaker 2>Yes.

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<v Speaker 3>So JWST takes its first slices of data right then

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<v Speaker 3>at the morning terminator. Right then the planet continues its

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<v Speaker 3>journey across the face of the star, and as it's

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<v Speaker 3>exiting the transit, the very last sliver of atmosphere to

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<v Speaker 3>be backlit is the trailing edge, the back of the planet.

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<v Speaker 3>Right and here the atmosphere flow is going in the

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<v Speaker 3>exact opposite direction. The superheated air from the day side

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<v Speaker 3>is rotating across the terminator back into the dark night side.

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<v Speaker 2>Which makes it the alien sunset the.

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<v Speaker 3>Evening precisely the evening terminator. So by looking at the

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<v Speaker 3>exact timing of the transit, the very beginning versus the

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<v Speaker 3>very end, JWST can completely separate the chemical signature of

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<v Speaker 3>the morning from the chemical signature of the evening.

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<v Speaker 2>Which is just a staggering technological leap To be able

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<v Speaker 2>to not just see the specs seven hundred light years away,

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<v Speaker 2>but to pinpoint incredibly specific localized slivers of its atmosphere

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<v Speaker 2>at exact moments in its rotation.

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<v Speaker 3>It's mind blowing signal processing. They basically take the overlapping data,

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<v Speaker 3>do some intense math and subtract the pieces to reveal

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<v Speaker 3>the distinct morning and evening profiles.

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<v Speaker 2>When they finally did that math on WT ninety four AB,

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<v Speaker 2>the dichotomy they found was bizarre. It totally shattered the

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<v Speaker 2>old Hubble models complete paradigm shift because when they isolated

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<v Speaker 2>the morning edge, the data showed it was entirely clouded over,

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<v Speaker 2>densely cloudy, just a flat wall of opacity.

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<v Speaker 3>But then they looked at the evening edge, the trailing

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<v Speaker 3>limb and the skies were perfectly clear, massive distinct chemical

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<v Speaker 3>absorption features zero clouds.

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<v Speaker 2>A completely cloudy morning and a perfectly clear evening, which

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<v Speaker 2>you know, on its face doesn't sound that crazy to right.

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<v Speaker 3>It happens in Seattle all the time, exactly.

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<v Speaker 2>A foggy morning that clears up by dinner time is

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<v Speaker 2>totally normal on Earth. But this discovery absolutely shocked the

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<v Speaker 2>astronomical community. Why was it such a big deal Because.

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<v Speaker 3>Of what the clouds are made of and the extreme

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<v Speaker 3>physics required to make them disappear. We have to remember

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<v Speaker 3>these aren't fluffy water vapor clouds, right.

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<v Speaker 2>We mentioned this at the start.

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<v Speaker 3>Magnesium silicate, yes, and stay tight and forced to write.

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<v Speaker 3>If you look at the Earth's mantle, these minerals make

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<v Speaker 3>up the vast majority of it.

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<v Speaker 2>We are literally talking about rock sand.

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<v Speaker 3>Yes, So on this planet it is cloudy with a

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<v Speaker 3>high chance of literal sandstorms.

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<v Speaker 2>That's horrifying it is.

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<v Speaker 3>And the reason the morning is so cloudy is because

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<v Speaker 3>of the night side temperature. The dark side of this

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<v Speaker 3>planet is cold enough that gaseous magnesium and silicon actually condense,

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<v Speaker 3>They nucleate and form this massive global cloud deck of

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<v Speaker 3>suspended sand in the dark.

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<v Speaker 2>So you have this solid wall of rock particles, and

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<v Speaker 2>the plant's rotation carries that dark, sandy atmospheric mass right

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<v Speaker 2>across the morning terminator exactly.

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<v Speaker 3>It passes in front of the star as a literal

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<v Speaker 3>physical wall of sand, which perfectly explains why the morning

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<v Speaker 3>data was flat.

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<v Speaker 2>The starlight couldn't punch through the rock.

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<v Speaker 1>Right.

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<v Speaker 3>By the time that exact same patch of atmosphere reaches

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<v Speaker 3>the evening terminator, the sand is completely gone. The skies

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<v Speaker 3>are crystal clear.

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<v Speaker 2>And that is the massive physical question, right. Yeah, on

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<v Speaker 2>a planet that's bigger than Jupiter, where do thousands of

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<v Speaker 2>miles of suspended, vaporized rock go in just a few hours.

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<v Speaker 3>It's a huge mystery. You have this massive thermal gradient.

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<v Speaker 3>The day side is getting blasted by a thousand degree heat.

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<v Speaker 3>You can't just maintain a static wall of sand under

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<v Speaker 3>those conditions.

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<v Speaker 2>The atmosphere has to react violently.

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<v Speaker 3>Very violently. And researchers basically have two working theories for

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<v Speaker 3>what is causing this great disappearance by nightfall.

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<v Speaker 2>Theory one and theory two. Let's break them down.

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<v Speaker 3>Ray Theory one is the burial mechanism.

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<v Speaker 2>Burial, meaning the clouds are getting shoved underground.

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<v Speaker 3>Basically, yes, So you have this extreme temperature difference between

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<v Speaker 3>the day and the night right that creates an immense

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<v Speaker 3>pressure gradient, and because the planet is rotating, it spins

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<v Speaker 3>up this massive, superfast jet stream right around the equator.

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<v Speaker 2>In the equatorial jet just blast the eastward exactly.

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<v Speaker 3>And as this jet stream carries those heavy sand clouds

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<v Speaker 3>from the cold morning into the blazing hot day side,

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<v Speaker 3>the sudden heat causes complex vertical wind share, meaning.

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<v Speaker 2>The wind doesn't just blow left to right, it blows

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<v Speaker 2>up and down.

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<v Speaker 3>Yes, massive planetary down drafts. The theory is that these

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<v Speaker 3>powerful winds violently plunge downward, dragging millions of tons of

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<v Speaker 3>silicate clouds deep into the planet's interior wow yeah, pulling

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<v Speaker 3>them completely out of sight. So by the time that

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<v Speaker 3>air mass reaches the evening, the upper atmosphere has been

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<v Speaker 3>essentially vacuum to clean the clouds are buried.

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<v Speaker 2>That is intense just to localized vertical wind dragging an

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<v Speaker 2>entire ocean of sand straight down. What kind of immense

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<v Speaker 2>planetary circulation would be required to sustain that.

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<v Speaker 3>Our three D fluid dynamics model suggests it's entirely possible,

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<v Speaker 3>especially near the equator where these forces converge.

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<v Speaker 2>Okay, so that's theory one, the burial. The Theory two

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<v Speaker 2>is even more extreme, isn't it.

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<v Speaker 3>Oh, Theory two is the extreme burnoff flash vaporization.

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<v Speaker 2>This is the Earth analogy, but just dialed up to

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<v Speaker 2>a terrifying extreme.

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<v Speaker 3>Precisely, this theory says we don't even need complex downward winds,

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<v Speaker 3>it's just brute force thermodynamics. As the planet rotates and

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<v Speaker 3>that thick wall of solidifying sand drifts out of the

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<v Speaker 3>dark morning and hits the one thousand plus degree heat

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<v Speaker 3>of the day side.

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<v Speaker 2>It just boils the actual chemical bonds of the rock.

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<v Speaker 3>The solid particles literally flash vaporize. They absorb the stellar

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<v Speaker 3>radiation so fast that they sublimate right back into a transparent.

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<v Speaker 2>Gas vaporized into nothingness. Yeah, just completely annihilated by the

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<v Speaker 2>heat of the star.

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<v Speaker 3>Yep. And because gash of silicon doesn't block the infrared

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<v Speaker 3>telescope plight the way solid sand does, the opacity just

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<v Speaker 3>drops to zero.

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<v Speaker 2>So by the time the wind carries that air to

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<v Speaker 2>the evening terminator, it's perfectly transparent. The clouds only form

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<v Speaker 2>again once they cross back into the cold night. Ah.

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<v Speaker 2>A daily planetary scale sand boil. The sheer violence of

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<v Speaker 2>that imagery is amazing. A wall of solid sand flying

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<v Speaker 2>out of the dark and instantly vaporizing in blind and heat.

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<v Speaker 3>It really is incredible to picture. But as fascinating as

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<v Speaker 3>that violent meteorological event is, the absence of those clouds

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<v Speaker 3>in the evening actually provided an even bigger scientific price.

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<v Speaker 2>Right because the evening was finally clear, astronomers could just

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<v Speaker 2>look at the trailing edge and see the actual true atmosphere.

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<v Speaker 3>Of the planet without any fog in the way.

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<v Speaker 2>And this brings us back to that baffling error from

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<v Speaker 2>the old Hubble data. When Hubble was squishing the cloudy

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<v Speaker 2>morning and the clear evening together, the data it spit

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00:14:28.600 --> 00:14:31.200
<v Speaker 2>out was deeply, deeply problematic.

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00:14:31.399 --> 00:14:34.320
<v Speaker 3>It was a nightmare for theorists because when you convolve

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00:14:34.360 --> 00:14:37.559
<v Speaker 3>that data, the massive cloud deck hid all the water

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00:14:37.639 --> 00:14:40.879
<v Speaker 3>absorption lines, so the planet looked like it was completely

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<v Speaker 3>depleted of oxygen, but the.

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<v Speaker 2>Carbon lines were still somewhat visible.

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00:14:44.159 --> 00:14:48.000
<v Speaker 3>Right, So the old data suggested that WSP ninety four

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00:14:48.159 --> 00:14:51.639
<v Speaker 3>AB had a carbon to oxygen ratio of almost one

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<v Speaker 3>point zero.

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00:14:52.320 --> 00:14:54.759
<v Speaker 2>Meaning there was basically just as much carbon as oxygen,

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<v Speaker 2>which doesn't sound like a big deal to a layman,

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00:14:57.720 --> 00:14:59.960
<v Speaker 2>but in planetary science that's impossible.

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<v Speaker 3>It completely broke existing theories of how planets form. You

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<v Speaker 3>cannot easily explain how a gas giant could form with

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00:15:07.080 --> 00:15:10.960
<v Speaker 3>that absurdly high ratio of carbon to oxygen. It also

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<v Speaker 3>implied the planet was hundreds of times more metal rich

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<v Speaker 3>than our own Jupiter.

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00:15:15.000 --> 00:15:17.559
<v Speaker 2>So it's like it's like looking at a person who

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00:15:17.600 --> 00:15:22.039
<v Speaker 2>is wearing a massive, puffy, leadlined winter coat. Huh exactly,

319
00:15:22.120 --> 00:15:24.879
<v Speaker 2>and from across the street you look at them in

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00:15:24.919 --> 00:15:28.320
<v Speaker 2>this giant coat and you conclude, Wow, that person must

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<v Speaker 2>weigh six hundred pounds. They are medically inexplicable.

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00:15:31.480 --> 00:15:32.879
<v Speaker 3>Right, they defy biology.

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00:15:33.000 --> 00:15:36.399
<v Speaker 2>But really it's just the coat. And JWST basically just

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00:15:36.440 --> 00:15:38.200
<v Speaker 2>waited for the planet to take the coat off in

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00:15:38.200 --> 00:15:39.799
<v Speaker 2>the evening so we could finally put it on a

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00:15:39.840 --> 00:15:40.559
<v Speaker 2>real scale.

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00:15:40.639 --> 00:15:43.799
<v Speaker 3>That is a perfect analogy. The anomaly was a total

328
00:15:43.840 --> 00:15:45.639
<v Speaker 3>illusion caused by the clouds.

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00:15:45.679 --> 00:15:49.200
<v Speaker 2>So what happened when JWST actually weighed the planet so

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00:15:49.279 --> 00:15:50.919
<v Speaker 2>to speak, in the clear evening.

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<v Speaker 3>Sky, the unfogged spectrum revealed these massive, beautiful absorption bands

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00:15:55.840 --> 00:15:59.120
<v Speaker 3>for water vapor. The oxygen was there all along. It

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<v Speaker 3>was just hiding behind in the morning sandstorm, So the.

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00:16:01.360 --> 00:16:03.960
<v Speaker 2>Carbon oxygen ratio wasn't one point zero.

335
00:16:03.679 --> 00:16:06.240
<v Speaker 3>No, it plummeted right back down to a totally normal

336
00:16:06.279 --> 00:16:09.799
<v Speaker 3>baseline about point five. And the overall metallicity was only

337
00:16:09.799 --> 00:16:13.159
<v Speaker 3>about five times that of Jupiter, not hundreds of times,

338
00:16:13.159 --> 00:16:13.720
<v Speaker 3>so it's.

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00:16:13.559 --> 00:16:18.000
<v Speaker 2>Actually incredibly Jupiter like. It completely solved the formation theory crisis.

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00:16:18.200 --> 00:16:22.120
<v Speaker 3>Yep, the theorists all breathed a massive sigh of relief.

341
00:16:22.440 --> 00:16:25.720
<v Speaker 3>The core accretion models didn't need to be rewritten. The

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00:16:25.759 --> 00:16:29.159
<v Speaker 3>planet formed exactly how we expect gas giants to form

343
00:16:29.440 --> 00:16:32.200
<v Speaker 3>out beyond the water snow line in its stellar nursery,

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00:16:32.679 --> 00:16:34.080
<v Speaker 3>and then migrated inward.

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00:16:34.440 --> 00:16:37.559
<v Speaker 2>The error was entirely observational. We just couldn't see through

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00:16:37.559 --> 00:16:40.799
<v Speaker 2>the fog exactly. Fixing our understanding of this one specific

347
00:16:40.919 --> 00:16:44.679
<v Speaker 2>planet is incredible. But this new technique, this ability to

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00:16:44.879 --> 00:16:48.080
<v Speaker 2>isolate the morning and evening to find clear skies on

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00:16:48.120 --> 00:16:51.519
<v Speaker 2>a cloudy planet, that has implications for the entire galaxy,

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00:16:51.559 --> 00:16:51.879
<v Speaker 2>doesn't it?

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00:16:51.919 --> 00:16:55.159
<v Speaker 3>Oh? Absolutely, this is just the beginning. These hot Jupiters

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<v Speaker 3>like WSP ninety four AB, because of their extreme environments,

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00:16:59.720 --> 00:17:02.480
<v Speaker 3>they serve as these perfect cosmic laboratory.

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00:17:02.759 --> 00:17:04.960
<v Speaker 2>Because the forces are so exaggerated, it makes the physics

355
00:17:05.000 --> 00:17:06.319
<v Speaker 2>easier to see exactly.

356
00:17:06.359 --> 00:17:09.079
<v Speaker 3>It's a stress test for our atmospheric models. We can

357
00:17:09.119 --> 00:17:12.279
<v Speaker 3>study the intense chemistry and the physics of cloud dynamics

358
00:17:12.359 --> 00:17:13.039
<v Speaker 3>in real time.

359
00:17:13.160 --> 00:17:16.400
<v Speaker 2>In WSP ninety four AB wasn't just a one off fluke, right,

360
00:17:16.559 --> 00:17:18.440
<v Speaker 2>The researchers actually expanded their roster.

361
00:17:18.680 --> 00:17:22.319
<v Speaker 3>Yeah. They took the same asymmetric limb analysis, the morning

362
00:17:22.400 --> 00:17:25.640
<v Speaker 3>versus evening technique, and applied it to eight other hot

363
00:17:25.680 --> 00:17:26.400
<v Speaker 3>gas giants.

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00:17:26.640 --> 00:17:27.440
<v Speaker 2>And what did they find.

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00:17:27.599 --> 00:17:31.279
<v Speaker 3>They found this exact same distinctive cloud cycle on at

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<v Speaker 3>least two other worlds right away, WASP thirty nine B

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00:17:35.200 --> 00:17:36.720
<v Speaker 3>and WASP P seventeen B.

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00:17:37.279 --> 00:17:40.759
<v Speaker 2>Wow. So it's a fundamental feature of these tidally locked giants,

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00:17:41.240 --> 00:17:43.200
<v Speaker 2>a cloudy morning and a clear evening.

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00:17:43.400 --> 00:17:47.240
<v Speaker 3>It seems to be ubiquitous, which gives the JWST teams

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00:17:47.319 --> 00:17:51.759
<v Speaker 3>incredible confidence as they plan their upcoming large scale observing programs.

372
00:17:51.799 --> 00:17:53.359
<v Speaker 2>They're scaling up big time.

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00:17:53.559 --> 00:17:56.720
<v Speaker 3>Astronomers are moving way beyond just the hot jupiters. Now

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00:17:57.039 --> 00:17:59.599
<v Speaker 3>they are preparing to study cloud cycles across a huge

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00:17:59.680 --> 00:18:03.720
<v Speaker 3>variet of exoplanets. They're even looking at eccentric gas giants

376
00:18:03.799 --> 00:18:06.920
<v Speaker 3>that have highly variable heating as they swing close to

377
00:18:07.160 --> 00:18:08.640
<v Speaker 3>and far away from their stars.

378
00:18:08.839 --> 00:18:11.559
<v Speaker 2>Okay, so they're perfecting these tools. They're learning exactly how

379
00:18:11.559 --> 00:18:14.119
<v Speaker 2>to read the weather, how to mathematically strip away the

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00:18:14.119 --> 00:18:16.960
<v Speaker 2>clouds on a molten gas chanel. Right, and this is

381
00:18:17.000 --> 00:18:20.359
<v Speaker 2>the ultimate forward looking question. Is this the necessary stepping.

382
00:18:19.960 --> 00:18:21.680
<v Speaker 3>Stone to earth like planets?

383
00:18:21.759 --> 00:18:25.480
<v Speaker 2>Yes? Are we building the exact tools we need to

384
00:18:25.559 --> 00:18:28.359
<v Speaker 2>eventually look through the clouds of a terrestrial rock planet

385
00:18:28.799 --> 00:18:32.400
<v Speaker 2>in the habitable zone to find the exact chemicals signatures

386
00:18:32.440 --> 00:18:33.079
<v Speaker 2>of life.

387
00:18:33.400 --> 00:18:38.440
<v Speaker 3>Yes, categorically yes. Understanding cloud physics is the mandatory gateway

388
00:18:38.480 --> 00:18:41.440
<v Speaker 3>to finding true biosignatures.

389
00:18:40.720 --> 00:18:43.759
<v Speaker 2>Because if an earth like planet has a dense water

390
00:18:43.839 --> 00:18:46.400
<v Speaker 2>cloud layer and we try to read it the way

391
00:18:46.480 --> 00:18:48.319
<v Speaker 2>Hubble read the hot jupiters.

392
00:18:47.960 --> 00:18:50.720
<v Speaker 3>We'd get a completely false reading. A thick cloud layer

393
00:18:50.720 --> 00:18:53.400
<v Speaker 3>on a rocky world could easily mask the upsten or

394
00:18:53.440 --> 00:18:56.720
<v Speaker 3>methane we're looking for, or worse, the light scattering off

395
00:18:56.759 --> 00:18:58.960
<v Speaker 3>the clouds could mimic a gas that isn't even there,

396
00:18:59.400 --> 00:19:01.400
<v Speaker 3>giving us a false positive for life.

397
00:19:01.680 --> 00:19:04.480
<v Speaker 2>So if you can't subtract the clouds mathematically, you can't

398
00:19:04.519 --> 00:19:06.079
<v Speaker 2>trust the biological signature.

399
00:19:06.200 --> 00:19:08.799
<v Speaker 3>Exactly the work we're doing right now in these violent

400
00:19:08.839 --> 00:19:12.920
<v Speaker 3>extreme gas giants is building the robust mathematical architecture we

401
00:19:12.960 --> 00:19:14.400
<v Speaker 3>absolutely need for the future.

402
00:19:14.480 --> 00:19:16.680
<v Speaker 2>We are learning how to see through the fog so

403
00:19:16.759 --> 00:19:19.000
<v Speaker 2>that when we finally stare at an Earth twin, we

404
00:19:19.119 --> 00:19:20.559
<v Speaker 2>actually know what we're looking at.

405
00:19:20.640 --> 00:19:21.720
<v Speaker 3>That's the ultimate goal.

406
00:19:21.799 --> 00:19:24.920
<v Speaker 2>It's incredible journey just to recap where we've been today.

407
00:19:25.240 --> 00:19:30.079
<v Speaker 2>We started with a frustrating twenty year astronomical roadblock, this

408
00:19:30.240 --> 00:19:34.039
<v Speaker 2>foggy diner window that forced us into using corrupted, squished

409
00:19:34.160 --> 00:19:38.000
<v Speaker 2>data that threatened to break our entire understanding of planet formation.

410
00:19:38.039 --> 00:19:40.200
<v Speaker 3>All because of high altitude aerosols right.

411
00:19:41.000 --> 00:19:43.799
<v Speaker 2>But then through the sheer ingenuity of astronomers using the

412
00:19:43.880 --> 00:19:47.240
<v Speaker 2>Jans Web space telescope, we figured out how to slice

413
00:19:47.240 --> 00:19:48.160
<v Speaker 2>the transit into.

414
00:19:47.960 --> 00:19:50.880
<v Speaker 3>Pieces, isolating the morning from the evening.

415
00:19:50.680 --> 00:19:55.920
<v Speaker 2>Finding completely localized vaporizing sandstorms, realizing that the violent weather

416
00:19:56.119 --> 00:19:58.240
<v Speaker 2>was leaving the evening sky clear.

417
00:19:58.160 --> 00:20:01.079
<v Speaker 3>And then using that clear sky to finally put the

418
00:20:01.079 --> 00:20:02.839
<v Speaker 3>carbon ratio mystery to rest.

419
00:20:03.079 --> 00:20:06.759
<v Speaker 2>It's an absolute triumph of observational physics. So as we

420
00:20:06.799 --> 00:20:08.480
<v Speaker 2>wrap up today, I want to leave you with a

421
00:20:08.720 --> 00:20:10.319
<v Speaker 2>final thought to Maul over.

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00:20:10.480 --> 00:20:11.400
<v Speaker 3>Oh, I love these.

423
00:20:11.839 --> 00:20:14.079
<v Speaker 2>Next time you walk outside at night and you look

424
00:20:14.119 --> 00:20:16.400
<v Speaker 2>up at a star in the sky, to your eye,

425
00:20:16.440 --> 00:20:19.480
<v Speaker 2>it just looks like a seemingly static, twinkling point of light.

426
00:20:20.240 --> 00:20:24.039
<v Speaker 2>It's peaceful, it's quiet, but it's not. No realize that

427
00:20:24.039 --> 00:20:27.039
<v Speaker 2>that point of light is just a canvas. Around it

428
00:20:27.079 --> 00:20:30.279
<v Speaker 2>are worlds with their own millions of localized morning sunrises

429
00:20:30.279 --> 00:20:33.920
<v Speaker 2>and evening sunsets. Worlds being swept by towering storms of

430
00:20:34.000 --> 00:20:36.200
<v Speaker 2>vaporized rock and violent plunging winds.

431
00:20:36.319 --> 00:20:38.880
<v Speaker 3>A dynamic, churning universe of extreme weather

432
00:20:38.960 --> 00:20:41.680
<v Speaker 2>Systems, exactly a universe of weather that we are only

433
00:20:41.759 --> 00:20:43.000
<v Speaker 2>just beginning to comprehend.
