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 just take a second and picture

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<v Speaker 2>volcanic magma.

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<v Speaker 3>Oh yeah, the classic mental image right.

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<v Speaker 2>Like you probably immediately think of this thick, glowing red,

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<v Speaker 2>slowly creeping lava.

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<v Speaker 3>Like something you'd see in Hawaii or Iceland exactly.

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<v Speaker 2>And that image, that whole process is totally driven by

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<v Speaker 2>the familiar elements we have right here on Earth, you know,

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<v Speaker 2>mainly oxygen and iron.

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<v Speaker 3>Yeah, those are the big players for us.

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<v Speaker 2>But we need to completely shatter that mental image right

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<v Speaker 2>out of the gate today. Oh, absolutely, throw it right

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<v Speaker 2>out the window, because we are heading to Mercury. It's

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<v Speaker 2>the smallest, innermost planet in our Solar system, but it

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<v Speaker 2>is hiding this massive, fundamentally alien secret.

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<v Speaker 3>It really is. It's just a totally different world.

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<v Speaker 2>Yeah, on Mercury, the familiar rules of geology, all that

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<v Speaker 2>oxygen and iron stuff, it's just it's gone. It's replaced

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<v Speaker 2>by a chemical reality that is so bizarre it forces

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<v Speaker 2>us to basically rethink how planets are even born.

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<v Speaker 3>It's wild. It completely flips our understanding of planetary evolution.

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<v Speaker 2>So that's our mission for you today. We are going

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<v Speaker 2>to journey far away from this comfortable Earth centric view

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<v Speaker 2>of planetary science, and we're dropping into a world where

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<v Speaker 2>a totally different element, sulfur just reigns supreme.

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<v Speaker 3>Lfer is the king on Mercury, right, and.

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<v Speaker 2>Our goal is to understand how this one single element

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<v Speaker 2>completely rewrites Mercury's history. It creates a crust and a

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<v Speaker 2>geologic timeline that looks honestly nothing like.

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<v Speaker 3>Our own, not even close to our own.

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<v Speaker 2>And it's so easy, right, It's so easy to just

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<v Speaker 2>assume all rocky planets are basically variations of Earth, like

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<v Speaker 2>Mars is a cold Earth, Venus is a hotter Earth.

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<v Speaker 3>Yeah, it's the single biggest trap in planetary science, honestly.

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<v Speaker 2>I mean, it makes sense why we do it, of

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<v Speaker 2>course it does.

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<v Speaker 3>We live here. We have naturally built our entire understanding

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<v Speaker 3>of you know, planetary accretion, mantle convection, crust formation, all

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<v Speaker 3>of it. The chemistry of Earth, Mars, and well Venus,

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<v Speaker 3>because that's what we can see and measure easily exactly.

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<v Speaker 3>And in those systems, the oxygen and fugacity, which is

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<v Speaker 3>basically just the availability and the chemical activity of oxygen.

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<v Speaker 3>When the planet was forming, that was relatively high.

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<v Speaker 2>So there's plenty of oxygen to go around.

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<v Speaker 3>Tons of it. Oxygen totally dominates the chemical structure on Earth.

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<v Speaker 3>It dictates which elements bond together, it decides at what

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<v Speaker 3>temperature rocks melt, and really importantly, how a planet loses

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<v Speaker 3>its internal heat over bions of years.

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<v Speaker 2>But mercury is playing a different game.

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<v Speaker 3>A completely different game. It formed under entirely different initial

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<v Speaker 3>conditions in the Solar nebula. The rules that govern how

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<v Speaker 3>magma evolves on Earth, they just fail, They literally fail

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<v Speaker 3>when you apply them to mercury.

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<v Speaker 2>Because oxygen isn't the boss there, right, We're.

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<v Speaker 3>Dealing with environment governed by a completely different primary driver,

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<v Speaker 3>which is, like you said, sulfur.

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<v Speaker 2>Okay, So let's look at the actual data that broke

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<v Speaker 2>this Earth centric model, because I think that's fascinating.

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<v Speaker 3>The NASA Messenger mission.

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<v Speaker 2>Yes, Messenger because before Messenger, our understanding of mercury surface

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<v Speaker 2>was pretty much just you know, educated guessing.

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<v Speaker 3>Yeah, we had some fly by data from Mariner ten

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<v Speaker 3>back in the seventies and some telescope observations from the ground,

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<v Speaker 3>but it was really speculative.

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<v Speaker 2>But then Messenger finally gets into orbit around Mercury and

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<v Speaker 2>it starts using this X ray spectrometer.

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<v Speaker 3>Which is such a cool instrument by the way it is.

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<v Speaker 2>It basically waits for solar flares from the Sun to

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<v Speaker 2>blast the planet's surface and then measures the secondary X

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<v Speaker 2>rays that bounce off the rocks.

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<v Speaker 3>Exactly. It uses the Sun as its own giant radiation

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<v Speaker 3>source to light up the planet's chemistry.

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<v Speaker 2>And the chemical signature at back was just shocking. It

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<v Speaker 2>was entirely incompatible with an.

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<v Speaker 3>Earth like mantle, totally incompatible. It threw everyone for a loop.

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<v Speaker 2>It showed that Mercury's crust was incredibly depleted in iron,

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<v Speaker 2>like missing so much iron, but it was extraordinarily enriched

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<v Speaker 2>in sulfur.

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<v Speaker 3>We are talking about sulfur levels on the surface that

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<v Speaker 3>are orders of magnitude higher than anything we ever see on.

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<v Speaker 2>Earth, which is crazy. And this immediately tells us there's

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<v Speaker 2>a huge difference in the planet's bulk chemistry. It points

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<v Speaker 2>to this thing called an extreme reducing environment, right.

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<v Speaker 3>Yeah, a highly reduced environment. That's the absolute key to

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<v Speaker 3>interpreting all this messenger data.

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<v Speaker 2>Okay, So help us out here break down what it

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<v Speaker 2>actually means for a planetary body to be highly reduced

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<v Speaker 2>because that sounds like a very dense chemistry term.

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<v Speaker 3>Oh sure, So when planetary scientists talk about the redock

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<v Speaker 3>state of a planet, we're really just talking about the

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<v Speaker 3>balance between reduction and oxidation when the planet was first

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<v Speaker 3>clumping together.

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<v Speaker 2>Okay.

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<v Speaker 3>In an oxidized in environment like Earth, oxygen is superabundant,

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<v Speaker 3>and oxygen is highly electronegative.

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<v Speaker 2>Meaning it really wants electrons.

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<v Speaker 3>It loves electrons. It aggressively pulls electrons away from other

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<v Speaker 3>elements to form oxides. So iron, for example, easily oxidizes

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<v Speaker 3>to form silicate minerals, and those make up the bulk

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<v Speaker 3>of Earth's mantle and crust.

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<v Speaker 2>So an oxidized Earth is kind of like, well, it's

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<v Speaker 2>like a rusting piece of iron sitting out in the.

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<v Speaker 3>Brain right now that oxygen is grabbing onto everything.

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<v Speaker 2>That's a perfect analogy. Actually, Earth is basically fully rusted.

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<v Speaker 3>But mercury isn't rusting.

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<v Speaker 2>No, not at all. Mercury formed way closer to the

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<v Speaker 2>proto Sun in a part of the early Solar nebula

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<v Speaker 2>where the oxygen fugacity that the availability we talked about

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<v Speaker 2>was incredibly low.

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<v Speaker 3>So no free oxygen, almost none. It's the most chemically

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<v Speaker 3>reduced terrestrial planet we have in the Solar System. In

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<v Speaker 3>this kind of environment, elements don't lose their electrons to

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<v Speaker 3>oxygen to keep them right. The whole system favors retaining electrons.

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<v Speaker 3>So without enough oxygen around to bond with the iron

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<v Speaker 3>in this big molten protoplanet, the way the iron behaves

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<v Speaker 3>shifts dramatically.

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<v Speaker 2>Okay, but wait, let me push back on this a

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<v Speaker 2>little bit. We know as a planetary fact that Mercury

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<v Speaker 2>has a disproportionately massive iron core, right, Like, the core

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<v Speaker 2>is huge compared to the rest of the planet.

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<v Speaker 3>Oh, absolutely massive. It's essentially a giant iron cannonball with

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<v Speaker 3>a thin, little rocky shell.

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<v Speaker 2>Right. So if it has this giant iron core, how

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<v Speaker 2>can its crust be so incredibly poor and iron? Where

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<v Speaker 2>did it all go?

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<v Speaker 3>That is the magic of the reduced state, because the

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<v Speaker 3>iron wasn't bonding with oxygen to form light silicate rocks

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<v Speaker 3>in the mantle. It stayed as unbound heavy metallic iron.

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<v Speaker 3>Oh I see, and gravity just took over. In a

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<v Speaker 3>totally molten young planet, all that heavy unbound iron just

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<v Speaker 3>sank rapidly right to the center.

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<v Speaker 2>Wow, So it basically filtered itself out.

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<v Speaker 3>Exactly, the extreme reducing conditions caused super efficient planetary differentiation.

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<v Speaker 3>The iron partitioned almost completely into the core, and it

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<v Speaker 3>left behind a mantle that is just stripped bear of iron.

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<v Speaker 2>That makes so much sense, but that brings up a

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<v Speaker 2>really big chemical mystery, then the sulfur mystery. Exactly. If

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<v Speaker 2>the mantle has no iron but it has tons of sulfur,

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<v Speaker 2>what is the sulfur doing Because here on Earth, sulfur

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<v Speaker 2>is a home wrecker, but it specifically loves iron, right Yeah.

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<v Speaker 3>On Earth, sulfur is what we call a chalcophile element.

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<v Speaker 3>It has a super strong affinity for iron. It constantly

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<v Speaker 3>seeks out iron to form these dense sulfide melts.

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<v Speaker 2>But if all the iron on mercury already sank to

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<v Speaker 2>the center.

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<v Speaker 3>Then the sulfur in the outer layers the mantle is

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<v Speaker 3>basically stranded. It's stuck up there without its favorite bonding partner.

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<v Speaker 2>So it has to find someone else to dance with.

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<v Speaker 3>Exactly that total absence of iron forces a huge shift

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<v Speaker 3>in the mineral pathways. On Earth, sulfur and iron get

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<v Speaker 3>together in four minerals like pyrite, which you know as

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<v Speaker 3>fool's gold. But on mercury, the sulfur has to interact

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<v Speaker 3>with the next best things available, and in this highly

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<v Speaker 3>reduced iron poor molten rock, sulfur starts bonding aggressively with magnesium.

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<v Speaker 2>Calcium, magnesium and calcium.

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<v Speaker 3>Yeah, and that is a pathway that is almost entirely

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<v Speaker 3>shut down on Earth. We just don't see it much here,

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<v Speaker 3>But on mercury it becomes the dominant chemical mechanism.

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<v Speaker 2>Okay, so sulfur is suddenly best friends with magnesium and calcium.

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<v Speaker 2>But how does that atomic level chemistry actually change the

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<v Speaker 2>physical magma? Like, what is it doing to the rock itself?

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<v Speaker 3>It completely changes the structural integrity of the magma. Think

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<v Speaker 3>about how molden rock where silicon melt is built in

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<v Speaker 3>a normal Earth magma, the structure is this really complex

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<v Speaker 3>network of silicon, oxygen tetrahedrol.

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<v Speaker 2>Okay, silicon and oxygen linking up right.

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<v Speaker 3>Oxygen acts as the glue or the bridging ion. It

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<v Speaker 3>links these structures together into a really robust three dimensional web.

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<v Speaker 3>So it's strong, very strong, and that interconnected web dictates everything.

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<v Speaker 3>It controls how thick and viscous the magma is, its density,

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<v Speaker 3>and crucially its liquidst temperature.

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<v Speaker 2>The liquidst temperature meaning the exact point where it stops

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<v Speaker 2>being liquid and starts forming solid crystals exactly.

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<v Speaker 3>So if you have all this sulfur for forming complexes

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<v Speaker 3>with magnesium and calcium on mercury, it isn't just floating

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<v Speaker 3>around doing nothing. It actively attacks that silicon oxygen framework.

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<v Speaker 2>It's actively breaking it. Like Okay, think about Earth's magma

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<v Speaker 2>as a building. The oxygen atoms are these strong steel

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<v Speaker 2>bolts holding the steel beams together. I like that, But

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<v Speaker 2>on molcury, because of all this weird chemistry, those steel

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<v Speaker 2>bolts get replaced by a softer metal, yes, exactly, like

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<v Speaker 2>lead or something. So it fundamentally compromises the rigidity of

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<v Speaker 2>the whole building. It's way easier to collapse.

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<v Speaker 3>That's spot on. The sulfur actively substitutes for oxygen in

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<v Speaker 3>the network because sulfur is in the same group as

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<v Speaker 3>oxygen on the periodic table, it can technically fit into

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<v Speaker 3>those same spots. It's like an impostor a very clumsy imposter.

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<v Speaker 3>Sulfur is a much larger ion than oxygen, and it

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<v Speaker 3>doesn't hold onto electrons as tightly, So when sulfur forces

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<v Speaker 3>its way in and replaces a bridging oxygen atom, it

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<v Speaker 3>bends the bond.

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<v Speaker 2>Angles, it warps the structure, It.

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<v Speaker 3>Totally warps it. The bond between sulfur and silic is

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<v Speaker 3>just much weaker and way easier to break than the

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<v Speaker 3>normal oxygen silicon bond, so the milt to polymizes.

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<v Speaker 2>To polymerizes, meaning it just falls apart.

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<v Speaker 3>It breaks up those long, strong chains. Now, a strong

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<v Speaker 3>oxidized magma on Earth needs a huge amount of heat

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<v Speaker 3>just to stay liquid. But if you introduce sulfur and

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<v Speaker 3>break all those bonds, you're lowering the amount of energy.

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<v Speaker 2>Needed, which means it stays liquid at much cooler temperatures.

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<v Speaker 3>Exactly the thermal energy required to prevent it from freezing

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<v Speaker 3>into solid rock drops significantly.

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<v Speaker 2>Okay, so that's the theory, But how do we actually

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<v Speaker 2>know this Because we haven't brought any rocks back from Mercury.

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<v Speaker 3>No, we haven't. And that's where the lab work comes.

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<v Speaker 2>In, right, because you can't just run a computer simulation

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<v Speaker 2>and call it a day. You have to prove it.

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<v Speaker 2>You have to physically cook a rock and see what happens.

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<v Speaker 3>Yeah, you have to subject the exact chemical recipe of

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<v Speaker 3>mercury's mantle to the massive pressures and temperatures deep inside

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<v Speaker 3>the planet.

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<v Speaker 2>Which brings us to this mind blowing research from twenty

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<v Speaker 2>twenty six. This was done at Rice University.

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<v Speaker 3>Yes, pecifically by a postdoctoral researcher named Yushen Zang working

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<v Speaker 3>in roj Deep Dusk Gupta's lab. They wanted to physically replicate.

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<v Speaker 2>Early mercury, but again, no rocks for mercury. So they

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<v Speaker 2>needed a stand in proxy and.

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<v Speaker 3>They found the perfect proxy, the in Darsch meteorite.

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<v Speaker 2>Okay, we have to talk up the backstory of this

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<v Speaker 2>meteorite because it is just incredible to me that this

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<v Speaker 2>rock fell out of the sky in Azerbaijan in eighteen

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<v Speaker 2>ninety one.

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<v Speaker 3>Eighteen ninety one, way before we even knew what mercury

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<v Speaker 3>really was.

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<v Speaker 2>Yeah, it's just astounding. A rock falls from space in

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<v Speaker 2>the nineteenth century sits in a drawer somewhere for one

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<v Speaker 2>hundred and thirty years, and now we're using it to

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<v Speaker 2>simulate an unreachable planet. Why this specific rock though, What

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<v Speaker 2>makes in dark so special.

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<v Speaker 3>In darts is a very rare type of rock called

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<v Speaker 3>an ensteatite chondrite. They make up only about two percent

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<v Speaker 3>of all meteorites that hit Earth.

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<v Speaker 2>Wow, so very rare, extremely.

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<v Speaker 3>Rare, and their chemistry is key. When we look at

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<v Speaker 3>their isotopes like oxygen, titanium, and calcium, they look a

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<v Speaker 3>lot like the rocks in the Earth Moon system, which

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<v Speaker 3>tells us they formed in inner solar nebula.

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<v Speaker 2>Toast of the Sun.

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<v Speaker 3>Right. But unlike Earth rocks, their mineral makeup is aggressively reduced.

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<v Speaker 2>There's that word again, reduced, Right.

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<v Speaker 3>They're packed with minerals that simply cannot exist if there's

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<v Speaker 3>any free oxygen around. Minerals like oldamite, which is calcium sulfide,

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<v Speaker 3>and nineiningerite, which is a magnesium iron sulfide.

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<v Speaker 2>So this meteorite basically has the exact same weird low

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<v Speaker 2>iron high sulfur recipe as mercury's crust.

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<v Speaker 3>It's practically a perfect match for the messenger data. It

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<v Speaker 3>is a surviving piece of the exact type of material

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<v Speaker 3>that clump together to build mercury.

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<v Speaker 2>Okay, so Zang and the team at Rice University have

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<v Speaker 2>this piece of the in darch meteorite. But you can't

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<v Speaker 2>just stick it in a microwave. How do you simulate

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<v Speaker 2>the inside of a planet? How do you cook this

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<v Speaker 2>rock at those kinds of pressures without destroying the laboratory?

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<v Speaker 1>Oh?

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<v Speaker 3>It requires some serious heavy duty engineering. They use what's

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<v Speaker 3>called a multianvil press.

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<v Speaker 2>Multi anvil sounds heavy, it's massive. These machines generate gigab

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<v Speaker 2>has scals of pressure.

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<v Speaker 3>You get pascals. What does that feel life? It's basically

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<v Speaker 3>equivalent to the crushing weight of hundreds of kilometers of

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<v Speaker 3>solid planetary rock pressing down on you all at once.

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<v Speaker 2>Oh wow, Okay, So how does the machine do that?

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<v Speaker 3>They take the rock, sample, powder it, and put it

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<v Speaker 3>inside this tiny capsule, usually made a graphite or a

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<v Speaker 3>special metal alloy. Then they put that tiny capsule inside

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<v Speaker 3>an octaegal pressure medium, basically an eight sided block. Then

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<v Speaker 3>massive hydraulic rams drive heavy tungsten carbide andles together from

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<v Speaker 3>all sides at the exact same time from all side. Yeah,

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<v Speaker 3>so the pressure's perfectly even, simulating depth, and while it's

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<v Speaker 3>being crushed, a tiny internal heater like a rhanium furnace

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<v Speaker 3>cranks the heat up to thousands of degrees celsius.

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<v Speaker 2>That is insane. Maintaining that kind of heat and pressure

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<v Speaker 2>without the whole thing just exploding.

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<v Speaker 3>The precision is unbelievable, but they have to do it

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<v Speaker 3>to track exactly when the rock melts and when it freezes.

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<v Speaker 3>They map the liquidus and the solidus.

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<v Speaker 2>It's the solidus being the point where it's totally hundred

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<v Speaker 2>percent solid rock.

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<v Speaker 3>Right, So they get the rock to the exact pressure

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<v Speaker 3>and temperature they want, wait for the chemistry to balance out,

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<v Speaker 3>and then they do a rabid quench, a.

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<v Speaker 2>Quench like plunging a hot sword into water.

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<v Speaker 3>Essentially, Yes, they instantly drop the temperature while keeping the

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<v Speaker 3>crushing pressure on. It freezes the molten rock into glass

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<v Speaker 3>in a split second.

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<v Speaker 2>So it basically takes a chemical snapshot of what the

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<v Speaker 2>magma look like at that exact depth and temperature exactly.

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<v Speaker 3>And then they slice it open and look at it

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<v Speaker 3>under an electron microprobe.

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<v Speaker 2>And so the big reveal when they finally looked at

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<v Speaker 2>these cooked, quenched samples of this mercury like rock. What

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<v Speaker 2>did they actually see? Did the sulfur do what they

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<v Speaker 2>thought it would?

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<v Speaker 3>It did exactly what they predicted. The data was crystal clear.

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<v Speaker 3>The sulfur aggressively substituted into the silicate network, weakened it

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<v Speaker 3>and actively suppressed crystallization.

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<v Speaker 2>So the anti freeze theory worked.

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<v Speaker 3>It worked perfectly. These reduced sulfur rich melts stayed liquid

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<v Speaker 3>at significantly lower temperatures than an equivalent Earth rock would have.

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<v Speaker 2>Which brings up that great quote from Rajdeep Dascupta, the

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<v Speaker 2>head of the lab.

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<v Speaker 3>Oh I love this quote. He said, what water or

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<v Speaker 3>carbon does to magmatic evolution on Earth, sulfur does on mercury.

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<v Speaker 2>It's such a perfect summary because on Earth, if you

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<v Speaker 2>add water to hot rock deep underground, like at a

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<v Speaker 2>subduction zone, it acts as a flux. It lowers the

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<v Speaker 2>melting point and triggers volcanoes.

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<v Speaker 3>Right The water physically gets into the rock structure and

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<v Speaker 3>breaks up the.

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<v Speaker 2>Polymers, like pouring salt on an icy road exactly.

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<v Speaker 3>It forces the ice to melt even though it's freezing outside.

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<v Speaker 3>On mercury, sulfur is the salt. It's the planetary anti freeze.

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<v Speaker 2>But the difference is water on Earth is kind of localized.

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<v Speaker 2>It happens at specific tectonic plates. On Mercury, this sulfur

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<v Speaker 2>is everywhere. It's built into the whole planet.

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<v Speaker 3>Yes, it operates globally. It depressed the melting point across

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<v Speaker 3>the entire mantle of the planet.

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<v Speaker 2>Okay, so let's zoom out. Now we've got the lab data.

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<v Speaker 2>We know the atomic bonds are weaker. We know the

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<v Speaker 2>magma stays liquid at cooler temperatures. How does it's that

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<v Speaker 2>atomic level chemistry translate to the huge planet wide features

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<v Speaker 2>we see on Mercury today.

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<v Speaker 3>Well, if the magma stays liquid longer at cooler temperatures,

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<v Speaker 3>it drastically extends the life span of Mercury's early magma oceans.

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<v Speaker 2>So instead of freezing solid quickly, the planet just sloshed

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<v Speaker 2>around as a giant ball of liquid rock for millions

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<v Speaker 2>of years, longer than we thought exactly.

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<v Speaker 3>And because the magma had a weaker structureless polymerized, it

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<v Speaker 3>was also runnier, less.

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<v Speaker 2>Viscous like water instead of honey.

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<v Speaker 3>Right, and a running mantle moves heat really efficiently. It

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<v Speaker 3>convects faster, pulling heat from the core to the surface.

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<v Speaker 2>Wait, if it's moving heat to the surface faster, wouldn't

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<v Speaker 2>the planet cool down faster. That seems like a contradiction.

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00:16:42.840 --> 00:16:45.000
<v Speaker 3>It does seem like one. Yeah, but remember the anti

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<v Speaker 3>freeze effect. Even though the planet is losing heat rapidly,

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<v Speaker 3>the sulfur ensures the rock simply refuses to solidify until

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<v Speaker 3>the temperature drops incredibly low.

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<v Speaker 2>Oh man, So it's cooling off, but it's trapped in

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<v Speaker 2>a liquid.

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00:16:58.120 --> 00:17:01.200
<v Speaker 3>State precisely, and this extended period of cooling as a

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<v Speaker 3>liquid completely changes what kind of rocks eventually form. As

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<v Speaker 3>the temperature slowly drops toward that new super low freezing point.

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<v Speaker 3>The very first minerals to pop out of the liquid

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<v Speaker 3>and crystallize are those sulfur compounds.

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<v Speaker 2>The calcium and magnesium sulfides we talked about earlier oldamite

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<v Speaker 2>and nininjurite.

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00:17:18.799 --> 00:17:23.400
<v Speaker 3>Yes, because they crystallized early while the mantle was still fluid,

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<v Speaker 3>they were able to concentrate in the upper.

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<v Speaker 2>Crust, which perfectly explains why messengers saw all that calcium

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<v Speaker 2>and magnesium on the surface exactly.

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00:17:31.319 --> 00:17:34.680
<v Speaker 3>The entire surface composition is a direct result of this

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<v Speaker 3>prolonged low temperature crystallization that is.

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<v Speaker 2>So incredibly elegant. It just ties everything together.

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00:17:41.279 --> 00:17:45.039
<v Speaker 3>It really does. It also explains Mercury's volcanic history, oh.

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<v Speaker 2>Right, because Mercury has these huge, smooth volcanic planes.

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<v Speaker 3>Right, vast plains of cured lava that sit on top

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<v Speaker 3>of older, cratered terrain, which means these massive volcanic eruptions

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<v Speaker 3>happened relatively late in the planet's youth.

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<v Speaker 2>But if Mercury was an Earth like rock, it's so

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<v Speaker 2>small it should have cooled and formed a thick, solid

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<v Speaker 2>crust really early. The volcano should have choked off and

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<v Speaker 2>died exactly.

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00:18:07.960 --> 00:18:11.720
<v Speaker 3>The thermal models for a normal rocky planet of Mercury

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00:18:11.839 --> 00:18:15.279
<v Speaker 3>size say the volcano should have shut down quickly, but

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<v Speaker 3>the sulfur kept the engine running. It kept the mantle

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<v Speaker 3>partially melted and fluid enough to erupt onto the surface

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<v Speaker 3>long after it should have frozen solid.

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00:18:23.519 --> 00:18:26.079
<v Speaker 2>Okay, but this leads me to another question, a pushback.

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00:18:26.119 --> 00:18:27.240
<v Speaker 3>Actually, let's hear it.

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00:18:27.400 --> 00:18:30.440
<v Speaker 2>If the sulfur kept the magma hot and fluid for

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00:18:30.480 --> 00:18:32.839
<v Speaker 2>such a long time, how does that fit with the

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00:18:32.880 --> 00:18:33.400
<v Speaker 2>low bait.

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00:18:33.319 --> 00:18:34.880
<v Speaker 3>Scarps us the scarps?

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00:18:35.000 --> 00:18:37.319
<v Speaker 2>Yeah, for people who don't know mercury is covered in

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00:18:37.359 --> 00:18:40.920
<v Speaker 2>these massive cliffs and ridges called scarps. They look like wrinkles.

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00:18:41.279 --> 00:18:44.559
<v Speaker 2>The planet literally contracted and shrank like a raisin.

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00:18:44.400 --> 00:18:46.160
<v Speaker 3>A giant iron filled raisin.

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00:18:46.319 --> 00:18:48.640
<v Speaker 2>Right, But you can't wrinkle a liquid. If the mantle

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00:18:48.680 --> 00:18:51.720
<v Speaker 2>was fluid for so long, a shrinking core wouldn't cause

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00:18:51.720 --> 00:18:54.359
<v Speaker 2>the surface to snap and form cliffs. The liquid would

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00:18:54.400 --> 00:18:57.400
<v Speaker 2>just adjust. So how did the scarps form?

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00:18:57.480 --> 00:19:00.000
<v Speaker 3>That is a brilliant point. The mechanics have scarp formed

391
00:19:00.680 --> 00:19:05.440
<v Speaker 3>absolutely require a rigid, solid, thick outer shell lithosphere. So

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00:19:05.480 --> 00:19:09.000
<v Speaker 3>the timeline is everything here. The global contraction, the shrinking

393
00:19:09.039 --> 00:19:12.039
<v Speaker 3>that made those cliffs. It had to happen primarily after

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00:19:12.079 --> 00:19:16.119
<v Speaker 3>the sulfur rich magma ocean finally cooled past its super

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00:19:16.160 --> 00:19:17.960
<v Speaker 3>low freezing point and locked up.

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00:19:18.119 --> 00:19:20.319
<v Speaker 2>Oh I see, So it stayed liquid for a long time,

397
00:19:20.400 --> 00:19:23.839
<v Speaker 2>letting the volcanoes erupt but eventually even the anti freeze

398
00:19:23.839 --> 00:19:25.759
<v Speaker 2>couldn't stop it from freezing exactly.

399
00:19:26.079 --> 00:19:28.960
<v Speaker 3>The temperature eventually dropped low enough that even those weakened

400
00:19:29.039 --> 00:19:31.640
<v Speaker 3>sulfur silicate networks froze solid.

401
00:19:31.359 --> 00:19:34.000
<v Speaker 2>And once it formed that thick, hard shell.

402
00:19:34.160 --> 00:19:37.640
<v Speaker 3>Once that rigid lithosphere was in place, the massive iron

403
00:19:37.680 --> 00:19:41.960
<v Speaker 3>core underneath continued to slowly cool and shrink over billions.

404
00:19:41.599 --> 00:19:44.720
<v Speaker 2>Of years, and the crust had nowhere to go right, it.

405
00:19:44.720 --> 00:19:47.880
<v Speaker 3>Induced immense compressive stress on the solid rock above it.

406
00:19:48.359 --> 00:19:51.519
<v Speaker 3>The crust had no choice but to snap, fail catastrophically,

407
00:19:51.759 --> 00:19:54.279
<v Speaker 3>and thrust up over itself to create those huge cliffs.

408
00:19:54.519 --> 00:19:57.519
<v Speaker 2>So the timing of the whole tectonic history is dictated

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00:19:57.519 --> 00:19:59.440
<v Speaker 2>by the atomic behavior of sulfur.

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00:19:59.640 --> 00:20:03.079
<v Speaker 3>Yes, down to the very atoms, and it goes even deeper.

411
00:20:03.119 --> 00:20:04.519
<v Speaker 3>It affects the magnetic field too.

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00:20:04.599 --> 00:20:07.200
<v Speaker 2>Wait, really, the sulfur on the rocks affects the magnetic

413
00:20:07.200 --> 00:20:08.000
<v Speaker 2>field of the core.

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00:20:08.240 --> 00:20:12.920
<v Speaker 3>Oh. Absolutely, Mercury has a global magnetic field generated by

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00:20:13.000 --> 00:20:17.720
<v Speaker 3>a churning, convecting liquid iron core, a geodynamo.

416
00:20:17.240 --> 00:20:17.880
<v Speaker 2>Just like Earth.

417
00:20:18.160 --> 00:20:21.279
<v Speaker 3>Just like Earth, But for a geodynamo to work, you

418
00:20:21.359 --> 00:20:24.000
<v Speaker 3>need a very specific rate of heat escaping from the

419
00:20:24.000 --> 00:20:27.160
<v Speaker 3>core into the mantle. If the mantle acts like a

420
00:20:27.160 --> 00:20:30.519
<v Speaker 3>thick thermal blanket, the core stops churning and the magnetic

421
00:20:30.599 --> 00:20:31.200
<v Speaker 3>field dies.

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00:20:31.480 --> 00:20:33.920
<v Speaker 2>But we just said the sulfur made the mantle runnier

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00:20:33.960 --> 00:20:35.559
<v Speaker 2>and more efficient at moving heat.

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00:20:35.799 --> 00:20:39.640
<v Speaker 3>Exactly by proving that the sulfur rich mantle stayed fluid

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00:20:39.680 --> 00:20:43.119
<v Speaker 3>and less viscous for longer. The researchers basically re rode

426
00:20:43.160 --> 00:20:46.160
<v Speaker 3>the equations for how heat moves across that boundary. The

427
00:20:46.240 --> 00:20:48.920
<v Speaker 3>chemistry of the rock directly controlled the cooling rate of

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00:20:48.960 --> 00:20:50.039
<v Speaker 3>the iron core.

429
00:20:49.960 --> 00:20:53.039
<v Speaker 2>Which means the sulfur literally dictated the strength and the

430
00:20:53.079 --> 00:20:55.559
<v Speaker 2>longevity of the magnetic field we still measure today.

431
00:20:55.680 --> 00:20:58.640
<v Speaker 3>It's all connected. The microscopic chemistry of the rock is

432
00:20:58.720 --> 00:21:02.359
<v Speaker 3>inextricably linked to the massive geophysical engine inside the planet.

433
00:21:02.559 --> 00:21:05.759
<v Speaker 2>That is just phenomenal. It's a cohesive start to finish

434
00:21:05.799 --> 00:21:09.519
<v Speaker 2>explanation for every weird thing about mercury, the surface chemistry,

435
00:21:09.599 --> 00:21:12.960
<v Speaker 2>the extended volcanoes, the cliffs, the magnetic field, it all

436
00:21:13.000 --> 00:21:14.000
<v Speaker 2>tracks back to sulfur.

437
00:21:14.279 --> 00:21:17.720
<v Speaker 3>It's a total paradigm shift, and it really validates the

438
00:21:17.759 --> 00:21:21.000
<v Speaker 3>incredible work done by the Rice University team.

439
00:21:20.880 --> 00:21:24.400
<v Speaker 2>Supported by NASA grants and the Rice Space Institute Center

440
00:21:24.440 --> 00:21:28.119
<v Speaker 2>for Planetary Origins to Habitability, which you know is a

441
00:21:28.160 --> 00:21:30.359
<v Speaker 2>long name, but they are doing vital work.

442
00:21:30.440 --> 00:21:33.799
<v Speaker 3>Vital work because honestly, this goes way beyond mercury.

443
00:21:34.000 --> 00:21:36.359
<v Speaker 2>Yes, this is what I really want to get into.

444
00:21:36.720 --> 00:21:40.119
<v Speaker 2>Why does this single case study matter for the rest

445
00:21:40.119 --> 00:21:41.359
<v Speaker 2>of the universe.

446
00:21:41.039 --> 00:21:45.119
<v Speaker 3>Because it exposes our severe terrestrial bias, our Earth centric

447
00:21:45.200 --> 00:21:49.039
<v Speaker 3>trap exactly because we live here. All our instruments are math,

448
00:21:49.079 --> 00:21:53.440
<v Speaker 3>our thermodynamic assumptions. They are all grounded in the oxidized,

449
00:21:53.640 --> 00:21:55.359
<v Speaker 3>iron rich chemistry of Earth.

450
00:21:55.599 --> 00:21:57.880
<v Speaker 2>So when we look at other planets, we just assume

451
00:21:57.920 --> 00:21:59.079
<v Speaker 2>they're built the same way.

452
00:21:59.279 --> 00:22:02.119
<v Speaker 3>We project our local rules onto the rest of the galaxy.

453
00:22:02.319 --> 00:22:05.119
<v Speaker 3>And Mercury just proved that if you apply an oxidized

454
00:22:05.119 --> 00:22:08.559
<v Speaker 3>model to a highly reduced planet, you get totally wrong answers.

455
00:22:08.680 --> 00:22:11.480
<v Speaker 3>You predict the wrong thermal history, the wrong structure, everything.

456
00:22:11.519 --> 00:22:14.039
<v Speaker 2>And we are discovering so many planets right now.

457
00:22:14.079 --> 00:22:17.519
<v Speaker 3>Thousands of them with advanced telescopes like James Web. We

458
00:22:17.640 --> 00:22:21.920
<v Speaker 3>aren't just finding rocky exoplanets, super earths and sub neptunes.

459
00:22:22.000 --> 00:22:24.559
<v Speaker 3>We're actually starting to look at their atmospheres and figure

460
00:22:24.559 --> 00:22:25.400
<v Speaker 3>out what they're made of.

461
00:22:25.559 --> 00:22:27.920
<v Speaker 2>And they aren't all like Earth, not at all.

462
00:22:28.759 --> 00:22:32.039
<v Speaker 3>Many of them orbit stars with totally different chemistry in

463
00:22:32.079 --> 00:22:35.960
<v Speaker 3>primordial discs that are vastly different from our own. Statistically,

464
00:22:36.079 --> 00:22:39.480
<v Speaker 3>a huge number of these rocky exoplanets formed under highly

465
00:22:39.519 --> 00:22:41.119
<v Speaker 3>reduced conditions.

466
00:22:40.759 --> 00:22:44.880
<v Speaker 2>Meaning the universe is likely just teeming with these sulfur dominated,

467
00:22:44.960 --> 00:22:48.079
<v Speaker 2>iron poor worlds absolutely teeming with them, which is kind

468
00:22:48.079 --> 00:22:51.160
<v Speaker 2>of ironic. Right. By turning our focus inward to the

469
00:22:51.279 --> 00:22:55.599
<v Speaker 2>absolute smallest closest planet to our Sun, we've basically built

470
00:22:55.640 --> 00:22:59.759
<v Speaker 2>a decoder ring to understand the farthest most alien exoplanets

471
00:22:59.759 --> 00:23:00.519
<v Speaker 2>in the galaxy.

472
00:23:00.599 --> 00:23:02.039
<v Speaker 3>That's a great way to put it, because if we

473
00:23:02.079 --> 00:23:04.960
<v Speaker 3>look at a distant super Earth through a telescope and

474
00:23:05.000 --> 00:23:08.519
<v Speaker 3>try to model its interior using Earth math, we will fail.

475
00:23:08.640 --> 00:23:12.640
<v Speaker 2>We'd calculate the wrong melting points, the wrong crust thickness.

476
00:23:12.359 --> 00:23:15.519
<v Speaker 3>The wrong timeline for when it might release gases into

477
00:23:15.559 --> 00:23:19.359
<v Speaker 3>an atmosphere. We would completely misunderstand its capacity to be

478
00:23:19.799 --> 00:23:22.000
<v Speaker 3>a stable, maybe even habitable environment.

479
00:23:22.160 --> 00:23:25.640
<v Speaker 2>But thanks to the data from crushing that little in

480
00:23:25.720 --> 00:23:26.720
<v Speaker 2>darch media.

481
00:23:26.480 --> 00:23:29.759
<v Speaker 3>Right, we now have the actual thermodynamic framework. We have

482
00:23:29.880 --> 00:23:33.519
<v Speaker 3>the correct phase boundaries to model the geology of reduced

483
00:23:33.559 --> 00:23:34.920
<v Speaker 3>exoplanets accurately.

484
00:23:35.079 --> 00:23:37.799
<v Speaker 2>It's incredible. It lets us predict when a sulfur rich

485
00:23:37.880 --> 00:23:42.039
<v Speaker 2>planet light years away will solidify, when its volcanoes will stop,

486
00:23:42.119 --> 00:23:43.680
<v Speaker 2>and how its crust will deform.

487
00:23:44.000 --> 00:23:46.240
<v Speaker 3>We can anticipate that its surface might be covered in

488
00:23:46.319 --> 00:23:49.160
<v Speaker 3>old mite instead of basalt. We can adjust our models

489
00:23:49.160 --> 00:23:51.880
<v Speaker 3>for its magnetic field. We are learning how to read

490
00:23:51.920 --> 00:23:55.240
<v Speaker 3>the geological history of worlds we can't even see clearly yet.

491
00:23:55.359 --> 00:23:58.359
<v Speaker 2>It's just a remarkable progression of knowledge. To summarize this

492
00:23:58.400 --> 00:24:02.640
<v Speaker 2>whole journey, we started with one anomalous, weirdly reduced rock

493
00:24:02.720 --> 00:24:05.359
<v Speaker 2>that fell in Azerbaijan in eighteen ninety one.

494
00:24:05.279 --> 00:24:07.640
<v Speaker 3>The indarge and statype chondrite.

495
00:24:07.160 --> 00:24:10.279
<v Speaker 2>Right, and by recognizing that its chemistry matched the weird

496
00:24:10.359 --> 00:24:13.240
<v Speaker 2>data from mercury, researchers in twenty twenty six used it

497
00:24:13.279 --> 00:24:16.720
<v Speaker 2>as a proxy. They subjected it to gigapascals of pressure

498
00:24:16.799 --> 00:24:18.240
<v Speaker 2>and thousands of degrees of heat.

499
00:24:18.519 --> 00:24:21.559
<v Speaker 3>They mapped the phase boundaries of a sulfur rich.

500
00:24:21.480 --> 00:24:25.000
<v Speaker 2>Mantle and prove that sulfur acts as a planetary anti freeze.

501
00:24:25.319 --> 00:24:28.519
<v Speaker 2>It depalmerizes the melt, lowers the energy needed to stay liquid,

502
00:24:28.799 --> 00:24:30.839
<v Speaker 2>and pushes the freezing point way down.

503
00:24:31.079 --> 00:24:35.200
<v Speaker 3>Which subsequently rewrites the entire geological timeline of mercury. It

504
00:24:35.240 --> 00:24:39.119
<v Speaker 3>explains the sulfide crust, the long lasting magma oceans, the

505
00:24:39.200 --> 00:24:41.839
<v Speaker 3>late forming scarps, and the magnetic dynamo.

506
00:24:42.119 --> 00:24:44.839
<v Speaker 2>And more importantly, it proves how much our understanding of

507
00:24:44.880 --> 00:24:48.559
<v Speaker 2>the universe is biased by our own backyard. Sometimes just

508
00:24:48.599 --> 00:24:52.519
<v Speaker 2>swapping out one single element, oxygen for sulfur, can rewrite

509
00:24:52.559 --> 00:24:54.240
<v Speaker 2>an entire planet's history.

510
00:24:54.319 --> 00:24:56.880
<v Speaker 3>It changes the architecture from the atomic scale all the

511
00:24:56.880 --> 00:24:58.720
<v Speaker 3>way up to the global features.

512
00:24:58.519 --> 00:25:00.480
<v Speaker 2>Which leaves us with a really provoked could have thought

513
00:25:00.519 --> 00:25:03.680
<v Speaker 2>to end on today? We now know the profound consequences

514
00:25:03.680 --> 00:25:07.240
<v Speaker 2>of swapping oxygen for sulfur. But sulfur is just one variable,

515
00:25:07.400 --> 00:25:09.720
<v Speaker 2>just one of many. Right as we keep looking at

516
00:25:09.759 --> 00:25:13.000
<v Speaker 2>distant star systems, we are going to find protoplanetary discs

517
00:25:13.079 --> 00:25:17.480
<v Speaker 2>with entirely alien elemental recipes. If a relatively simple swap

518
00:25:17.599 --> 00:25:20.079
<v Speaker 2>like sulfur can create a world as bizarre as mercury,

519
00:25:20.359 --> 00:25:21.200
<v Speaker 2>what else is out there?

520
00:25:21.240 --> 00:25:22.519
<v Speaker 3>The possibilities are endless.

521
00:25:22.640 --> 00:25:25.480
<v Speaker 2>What happens to a planet's mantle if it's heavily enriched

522
00:25:25.480 --> 00:25:28.319
<v Speaker 2>with carbon? How does a planet dissipate heat if it's

523
00:25:28.319 --> 00:25:33.119
<v Speaker 2>dominated by exotic refractory metals. What kind of wild, unpredicted

524
00:25:33.200 --> 00:25:36.519
<v Speaker 2>rocks are currently shaping worlds where the initial chemistry forces

525
00:25:36.559 --> 00:25:39.720
<v Speaker 2>elements into configurations we haven't even thought to synthesize in

526
00:25:39.759 --> 00:25:40.119
<v Speaker 2>a lab.

527
00:25:40.240 --> 00:25:41.039
<v Speaker 3>It's mind boggling.

528
00:25:41.119 --> 00:25:43.799
<v Speaker 2>Mercury is proof that our familiar Earth chemistry is just

529
00:25:43.960 --> 00:25:47.079
<v Speaker 2>one specific lucky outcome in a universe that is capable

530
00:25:47.119 --> 00:25:50.079
<v Speaker 2>of building planets through an almost infinite number of distinct

531
00:25:50.240 --> 00:25:51.279
<v Speaker 2>alien pathways.
