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 Astronomy 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>Welcome everyone. Today, we are doing a deep dive into well,

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<v Speaker 2>one of the biggest mysteries out there about our own

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<v Speaker 2>planet's history. It's a real cold case, it really is.

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<v Speaker 2>We're talking about the moment Earth fundamentally started to breathe,

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<v Speaker 2>the event that really set the stage for all complex life.

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<v Speaker 3>For us, the Great oxidation event. Yeah, the goe and Yeah.

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<v Speaker 3>The scale of this change is it's hard to overstate,

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<v Speaker 3>really billions of years where Earth was basically an oxygen

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<v Speaker 3>free zone, reducing.

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<v Speaker 2>World holding its breath as you put it, Yeah, exactly.

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<v Speaker 3>Then some are around two point one to two point

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<v Speaker 3>four billion years ago, things flipped dramatically. Suddenly there's this

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<v Speaker 3>massive release of oxygen into.

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<v Speaker 2>The atmosphere, changing everything forever.

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<v Speaker 3>Absolutely. But here's the kicker, The big puzzle scientists have

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<v Speaker 3>wrestled with. Right, the microbes responsible, these tiny little things

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<v Speaker 3>called cyanobacteria. They figured out how to make oxygen way

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<v Speaker 3>way before the goe actually.

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<v Speaker 2>Happened, hundreds of millions of years earlier. Right, that's the

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<v Speaker 2>baffling part.

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<v Speaker 3>Could be three hundred maybe even five hundred million years.

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<v Speaker 3>Think about that gap, it's enormous. You've got the oxygen factories,

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<v Speaker 3>they're built, they're running, technically capable of pumping out oxygen, but.

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<v Speaker 2>The atmosphere isn't changing. The lights are off globally speaking.

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<v Speaker 2>So the question's always been why why the huge delay?

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<v Speaker 3>Yeah, if the generators were online, what was stopping the

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<v Speaker 3>grid from powering up?

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<v Speaker 4>Mm hmm.

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<v Speaker 3>There have been theories, of course, good ones like volcanic

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<v Speaker 3>gases just sucking up all the oxygen or other microbes

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<v Speaker 3>eating it exactly.

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<v Speaker 2>Those are definitely part of the picture, but they they

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<v Speaker 2>never quite seemed to fully explain that incredibly long, stable

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<v Speaker 2>delay and then the sudden shift. It felt like something

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<v Speaker 2>was missing.

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<v Speaker 3>A bottleneck somewhere.

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<v Speaker 2>A bottleneck. Yeah, And that's where this new research comes in.

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<v Speaker 2>It's work out of Okayami University, led by doctor Dylan Retnayek,

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<v Speaker 2>published recently, they took a different angle. Instead of just

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<v Speaker 2>the big planetary sinks, they looked smaller exactly.

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<v Speaker 3>They zoomed right in on the microscopic level, the ecological factors.

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<v Speaker 3>What was actually controlling the growth of the cyanobacteria themselves?

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<v Speaker 3>Could they thrive or were they just sort of sputtering along?

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<v Speaker 2>Okay, So finding the precise control knob at the microbial level.

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<v Speaker 3>That's the idea, and their research points to two maybe

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<v Speaker 3>surprisingly simple compounds, nickel and urea.

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<v Speaker 2>Nickel and urea, Okay, that's not what usually comes to

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<v Speaker 2>mind with planet scale changes.

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<v Speaker 3>Right, but this study suggests they were the keys, first

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<v Speaker 3>locking the oxygen supply down and then eventually unlocking it.

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<v Speaker 2>So that's our mission for this deep dive. We're going

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<v Speaker 2>to unpack exactly how nickel and urea could have acted

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<v Speaker 2>as this biogeochemical bottleneck. We want to give you that

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<v Speaker 2>aha moment connecting the dots between tiny microbes and the

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<v Speaker 2>whole planet's atmosphere. Let's get into it, Okay, So let's

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<v Speaker 2>set the stage properly. Section one, the Great oxidation delay.

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<v Speaker 2>We need to appreciate just how big a deal the

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<v Speaker 2>GOE was.

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<v Speaker 3>It's truly a fundamental turning point. Before the goe. You've

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<v Speaker 3>got what's called a reducing atmosphere. I think lots of

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<v Speaker 3>compounds that readily react with oxygen, reduced iron, sulfur, methane,

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<v Speaker 3>things like that dominated.

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<v Speaker 2>So any free oxygen that popped up would just get

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<v Speaker 2>instantly consumed by the surrounding chemistry pretty much.

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<v Speaker 3>Yeah, the environment had a huge capacity to soak it up,

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<v Speaker 3>and when oxygen did start to build up significantly, it

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<v Speaker 3>was actually well toxic, a crisis for much of the

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<v Speaker 3>life that existed back then, which was anaerobic didn't use oxygen.

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<v Speaker 2>Right, Oxygen was poisonous to early life.

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<v Speaker 3>It's ironic, it is, But it was this very crisis,

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<v Speaker 3>this environmental shift, that ultimately paved the way for us

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<v Speaker 3>for complex multicellular life that needs oxygen. This transition marks

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<v Speaker 3>the boundary between the Rchean and Proterozoic eons roughly two

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<v Speaker 3>point four billion years ago.

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<v Speaker 2>And the agents of this change, the little heroes or

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<v Speaker 2>villains depending on your perspective, back then, were the cyanobacteria.

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<v Speaker 3>These incredible microbes. They perform oxygenic photosynthesis. Basically, they take sunlight,

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<v Speaker 3>water CO two stuff that's everywhere and turn it into

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<v Speaker 3>energy for.

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<v Speaker 2>Themselves, and oxygen is the waste product.

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<v Speaker 3>Oxygen is the exhaust. Exactly a revolutionary invention.

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<v Speaker 2>But an invention that, based on genetic evidence, seems to

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<v Speaker 2>pre date the GOE by a massive margin.

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<v Speaker 4>Yeah.

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<v Speaker 3>The molecular clock studies looking at the genes of modern

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<v Speaker 3>cyanobacteria and tracing them back strongly suggests the evolution of

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<v Speaker 3>this process happened maybe three hundred maybe five hundred million

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<v Speaker 3>years before the atmosphere actually registered it. The tech was there,

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<v Speaker 3>the impact wasn't.

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<v Speaker 2>So let's revisit those earlier theories for the delay. You

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<v Speaker 2>mentioned the big sinks, right.

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<v Speaker 3>Traditionally the thinking focused on these massive planetary buffers. One

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<v Speaker 3>was geological vultvolcanic activity. Early Earth was much more volcanically active,

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<v Speaker 3>pumping out loads of producing gases hydrogen, sulfur, dioxide.

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<v Speaker 2>Methane, gasses that just react instantly with O two.

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<v Speaker 3>Instantly, So it's like a giant geological vacuum cleaner constantly

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<v Speaker 3>running sucking up any oxygen the cyanobacteria managed to produce

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<v Speaker 3>that kept levels incredibly low.

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<v Speaker 2>Okay, that makes sense. What was the other main idea?

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<v Speaker 3>The other focused more on chemical sinks. Within the oceans

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<v Speaker 3>themselves and maybe other microbes. The oceans were full of

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<v Speaker 3>dissolved iron, for example, which rusts oxidizes very readily, So.

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<v Speaker 2>The oceans themselves were acting like a giant rust bucket,

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<v Speaker 2>consuming oxygen effectively.

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<v Speaker 3>Yeah. Plus maybe other early microbes, non oxygen producing ones,

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<v Speaker 3>were super efficient at gobbling up any organic matter or

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<v Speaker 3>trace oxygen that appeared a biological sink working alongside the

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<v Speaker 3>chemical ones.

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<v Speaker 2>So you had this planetary tug of war cyanobacteria producing

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<v Speaker 2>oxygen on one size.

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<v Speaker 3>And volcanoes, ocean chemistry and maybe other microbes consuming it

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<v Speaker 3>on the other side.

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<v Speaker 2>And the argument was that these forces were just perfectly

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<v Speaker 2>balanced for half a billion years. That seems improbable.

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<v Speaker 3>That's the tricky part, isn't it. Maintaining such a perfect,

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<v Speaker 3>delicate balance for such an incredibly long time and then

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<v Speaker 3>having it suddenly fail. Yeah, it always felt a bit well,

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<v Speaker 3>unsatisfying plausible. Sure, those factors were important, but maybe not

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<v Speaker 3>the whole story.

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<v Speaker 2>It didn't explain why the producers the cyanobacteria didn't just

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<v Speaker 2>eventually overwhelm the sinks earlier exactly.

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<v Speaker 3>The older models focused heavily on oxygen consumption. They didn't

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<v Speaker 3>look as closely at factors that might have been limiting

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<v Speaker 3>oxygen production in the first place by suppressing the cyanobacteria themselves.

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<v Speaker 2>Which is where the okay, i'ma study pivots. They're looking

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<v Speaker 2>at these cyanobacteria's diet, essentially their immediate chemical environment.

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<v Speaker 3>That's the core idea. Looking for ecological constraints. Doctor Ratnac's

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<v Speaker 3>team focused on trace elements and simple organic compounds, things

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<v Speaker 3>that might be present in small amounts but could have

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<v Speaker 3>huge regulatory effects on life.

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<v Speaker 2>And they zeroed in on nickel and urea. Why those

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<v Speaker 2>two They.

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<v Speaker 3>Had a hunch based on biochemistry that these two might

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<v Speaker 3>have this interconnected, really crucial role in limiting cyanobacterial growth.

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<v Speaker 3>Specifically back in the rke and eon. They suspected an

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<v Speaker 3>ecological control mechanism was the real bottleneck, something that didn't

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<v Speaker 3>need a new evolution to overcome, just to change in

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<v Speaker 3>the environment to release the brakes.

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<v Speaker 2>Finding that microscopic switch in a giant planetary system, I'm hucked.

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<v Speaker 2>All right, let's dive into the evidence itself Section two.

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<v Speaker 2>How they actually tested this. This wasn't just computer modeling, right,

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<v Speaker 2>They did lab experiment.

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<v Speaker 3>Oh yeah, really, rigorous experimental work. It had to be

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<v Speaker 3>done in two parts. Really. First, they needed to establish

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<v Speaker 3>that their key players, Nickel and Urea, were actually plausible

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<v Speaker 3>components of the early Archean ocean around say four to

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<v Speaker 3>two point five billion years ago before the goe kicked off.

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<v Speaker 2>Makes sense. You can't have them be the bottleneck if

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<v Speaker 2>they weren't even.

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<v Speaker 3>There precisely, So, Experiment Part one was all about abiotic

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<v Speaker 3>Urea formation. The question us could urea, which we know

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<v Speaker 3>is a vital nitrogen source for life, actually form without life,

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<v Speaker 3>making it through purely chemical.

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<v Speaker 2>Processes abiotic meaning non biological origin exactly.

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<v Speaker 3>And they needed to simulate the conditions of early Earth,

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<v Speaker 3>which were pretty brutal. Huw So well, the big thing

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<v Speaker 3>is the lack of an ozone layer. Back then, Earth's

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<v Speaker 3>early atmosphere didn't have much oxygen, so no ozone shield

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<v Speaker 3>like we have today. That meant intense high energy ultraviolet radiation,

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<v Speaker 3>specifically UVC was just blasting the surface, including the oceans.

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<v Speaker 2>And uvc's pretty nasty stuff.

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<v Speaker 1>Right.

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<v Speaker 2>We use it for sterilization, we do.

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<v Speaker 3>It's a highly energetic breaks down molecules, but that energy

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<v Speaker 3>can also drive chemical reactions that wouldn't normally happen, so

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<v Speaker 3>simulating that UVC exposure was crucial for accurately mimicking the

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<v Speaker 3>prebiotic environment. If a reaction needed UVC, it might have

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<v Speaker 3>happened then, but not now.

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<v Speaker 2>Okay, so intense UV light. What ingredients did they put

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<v Speaker 2>in their simulated primordial soup.

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<v Speaker 3>They used a mix of simple stuff thought to be

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<v Speaker 3>common back then, things like ammonium, cyanide and dissol iron compounds,

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<v Speaker 3>basic building blocks readily available from volcanic outgassing or hydrothermal vents.

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<v Speaker 2>And they zapped this mixture with UVC light.

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<v Speaker 3>Yep, they exposed these mixtures to UVC radiation and then

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<v Speaker 3>analyze the results to see if urea CONH two had formed,

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<v Speaker 3>and did it it did. They confirmed that urea could

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<v Speaker 3>indeed form abiotically under these plausible early Earth conditions.

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<v Speaker 2>Why is that single finding so important for their overall argument.

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<v Speaker 3>It's foundational because if urea could only be made by

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<v Speaker 3>complex biological processes, then its availability in the Archian Ocean

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<v Speaker 3>might have been really limited or patchy. Maybe that was

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<v Speaker 3>the bottleneck, just not enough nitrogen in a usable form.

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<v Speaker 2>But if it forms abiotically.

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<v Speaker 3>Then it was likely just there a constant background component

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<v Speaker 3>in the ancient oceans, produced by sunlight hitting common chemicals.

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<v Speaker 3>It wasn't a rare nutrient that life had to invent

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<v Speaker 3>ways to make. It was an environmental factor life had

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<v Speaker 3>to deal with, for better or worse.

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<v Speaker 2>So urea was likely present. Step one confirmed. What was

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<v Speaker 2>step two? Experiment Part two?

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<v Speaker 3>Right now? They needed to see how varying levels of

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<v Speaker 3>this urea along with nickel actually affected the growth of

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<v Speaker 3>the oxygen producers themselves. So testing cyanobacterial growth.

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<v Speaker 2>And they needed a stand in for ancient cyanobacteria.

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<v Speaker 3>Yeah, they used a well studied robust species called Cinachucoccus

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<v Speaker 3>SPPCC seven thousand and two. It's a modern cyanobacterium, but

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<v Speaker 3>it's often used as a model organism because it grows

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<v Speaker 3>relatively quickly and its basic photosynthetic machinery is thought to

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<v Speaker 3>be representative of those early forms.

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<v Speaker 2>Makes sense, So how do they set up the growth tests?

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<v Speaker 2>What were they controlling?

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<v Speaker 3>It was all about careful control. They grew the senachure

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<v Speaker 3>caucus under standard conditions, things like controlled like dark cycles

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<v Speaker 3>to mimic day and night. But the key manipulation was

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<v Speaker 3>the growth medium, the soup the sanobacteria lived in.

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<v Speaker 2>They tweaked the recipe exactly.

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<v Speaker 3>They created different patches with systematically varied concentrations of urea

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<v Speaker 3>and nickel. Some batches had low urea, some high, some

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<v Speaker 3>at low nickel, some high. And importantly, they tested various

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<v Speaker 3>combinations high er low nickel, low uryhine, nickel high, high,

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<v Speaker 3>lo low, all the possibilities, reflecting potential archeane conditions.

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<v Speaker 2>Covering all the bases. And how did they track if

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<v Speaker 2>the microups were actually growing well or not? How do

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<v Speaker 2>you measure that?

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<v Speaker 3>They use standard microbiology techniques. Two key metrics. First, they

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<v Speaker 3>measure the optical density of the liquid culture, basically how

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<v Speaker 3>cloudy it gets. As the cyanobacteria cells multiply, the culture

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<v Speaker 3>becomes more turbid, blocking more light passing through it. More

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<v Speaker 3>cloudiness equals more biomass.

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<v Speaker 2>Okay, a measure of overall growth yep.

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<v Speaker 3>And Second, they measure the concentration of chlorophyll. That's the

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<v Speaker 3>main pigment cyanobacteria use for photosynthesis, So tracking chlorophyll gives

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<v Speaker 3>you a direct measure of the photosynthetic capacity of the culture.

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<v Speaker 3>How much oxygen making machinery is present.

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<v Speaker 2>Got it?

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<v Speaker 4>Two?

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<v Speaker 2>Different ways to measure success. And what did they find?

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<v Speaker 2>Was it just more urea, more growth?

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<v Speaker 3>Not at all. It was much more complex. It wasn't

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<v Speaker 3>a simple case of urea being just food. They found

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<v Speaker 3>this intricate relationship, this dual role where the combination of

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<v Speaker 3>nickel and urea concentrations was the critical factor.

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<v Speaker 2>Doctor Rutnaya called it complex yet fascinating.

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<v Speaker 3>Right, that's the quote. The key finding wasn't about the

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<v Speaker 3>absolute amount of urea, but the ratio of nickel to urea.

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<v Speaker 3>That ratio scene to dictate whether the cyanobacteria could actually

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<v Speaker 3>flourish or if their growth was actively suppressed, even if

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<v Speaker 3>there was plenty of nitrogen theoretically available in the form

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<v Speaker 3>of urea.

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<v Speaker 2>So it wasn't simple starvation. It was something more like interference.

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<v Speaker 3>Exactly, pointing towards more subtle chemical control mechanism rather than

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<v Speaker 3>just basic nutrient limitation.

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<v Speaker 2>Okay, this is where it gets really interesting. Section three.

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<v Speaker 2>Unpacking the biogeochemical bottleneck model itself. How did high nickel

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<v Speaker 2>and urea actually work together to suppress life and delay

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<v Speaker 2>the GOE?

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<v Speaker 3>Right, this is the core of their proposed mechanism. To

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<v Speaker 3>understand the bottleneck, you need to picture the rkey in

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<v Speaker 3>ocean chemistry. The model suggests that back then concentrations of

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<v Speaker 3>both nickel and urea were significantly higher than they are today,

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<v Speaker 3>and crucially, it was this combination of high levels that

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<v Speaker 3>acted as the suppressor.

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<v Speaker 2>Okay, hang on, I'm still slightly stuck on why hy

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<v Speaker 2>urea would be bad. We established it's a nitrogen source,

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<v Speaker 2>and nitrogen is essential, right for proteins, DNA, everything, it

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<v Speaker 2>is essential absolutely, and nickel isn't that also a trace

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<v Speaker 2>nutrient needed for some enzymes? So why would having more

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<v Speaker 2>of these essential things be bad? It feels counterintuitive, it does.

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<v Speaker 3>Seem paradoxical, but the devil's in the biochemical details. It

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<v Speaker 3>goes down to a specific enzyme called.

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<v Speaker 2>Urese eurese Okay, what does that do?

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<v Speaker 3>Cyanobacteria, like many organisms, can't use urea directly as is.

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<v Speaker 3>They need to break it down first into simpler, more

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<v Speaker 3>biologically available forms of nitrogen like ammonia. Use is the

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<v Speaker 3>enzyme that does this job. It catalyzes the breakdown of urea.

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<v Speaker 2>Okay, so use is the tool they use to process

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<v Speaker 2>the urea food exactly.

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<v Speaker 3>And here's the crucial link to nickel therese enzyme absolutely

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<v Speaker 3>requires a tiny amount of nickel to function. Nickel acts

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<v Speaker 3>as a cofactor, fitting into the enzyme's active site and

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<v Speaker 3>helping it do its chemical work.

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<v Speaker 2>So they do need nickel.

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<v Speaker 3>They do, but only in trace amounts. Here's the problem.

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<v Speaker 3>The Archean oceans were apparently swimming in nickel compared to today.

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<v Speaker 2>Why so much nickel back then?

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<v Speaker 3>It's linked to the Earth's geology. At the time, there

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<v Speaker 3>was much higher geothermal activity, lots of deep sea hydroluminal

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<v Speaker 3>events spewing out dissolved metals, and also a specific type

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<v Speaker 3>of magnesium rich volcanic rock called comati eate was much

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<v Speaker 3>more common than These rocks are very rich in nickel,

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<v Speaker 3>and as they weathered or interacted with sea water, they

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<v Speaker 3>released a lot of nickel.

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<v Speaker 2>So nickel concentrations were way higher.

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<v Speaker 3>Potentially orders of magnitude higher, maybe four hundred times the

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<v Speaker 3>concentration we see in modern oceans based on geological evidence,

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<v Speaker 3>way way above trace nutrient levels.

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<v Speaker 2>Okay, so too much of a good thing. What happens

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<v Speaker 2>when the ures enzyme encounters these super high nickel levels

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<v Speaker 2>along with high urea.

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<v Speaker 3>That's where the inhibition comes in. When nickel concentrations get

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<v Speaker 3>that high, it stops being just a helpful cofactor and

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<v Speaker 3>starts coming up the works. The excess nickel ions essentially

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<v Speaker 3>compete for or interfere with the active site of the

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<v Speaker 3>ures enzyme. They block it. They interfere, Yeah, especially when

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<v Speaker 3>the enzyme is already trying to bind and process lots

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<v Speaker 3>of UREA molecules. Because the UREA concentration is also high.

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<v Speaker 3>It's like the enzyme gets overwhelmed and effectively poisoned or

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<v Speaker 3>jammed by the sheer abundance of nickel ions hitting it

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<v Speaker 3>while it's trying to work on the urea.

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<v Speaker 2>Wow. So the cyanobacteria are floating in this ocean full

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<v Speaker 2>of potential nitrogen fuel urea, but the tool they need

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<v Speaker 2>to use that fuel, ureas, is constantly being sabotaged by

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<v Speaker 2>the massive overdose of nickel.

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<v Speaker 3>That's the bottleneck mechanism. In a nutshell, They're effectively starving

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<v Speaker 3>for usable nitrogen right in the middle of the urea

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<v Speaker 3>feast because their metabolic machinery to access it is chemically

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<v Speaker 3>inhibited by the nickel overload.

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<v Speaker 2>So they can't grow efficiently, they can't divide rapidly and

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<v Speaker 2>form massive blooms.

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<v Speaker 3>Exactly. Their proliferation is suppressed, you might get small, localized,

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<v Speaker 3>short lived blooms perhaps, but not the sustained planet wide

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<v Speaker 3>explosion of cyanobacteria needed to overwhelm the oxygen sinks and

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<v Speaker 3>fundamentally change the atmosphere. The nickel urea combination acted like

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<v Speaker 3>a powerful break on the whole system.

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<v Speaker 2>That explains the lights off period, the great delay. The

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<v Speaker 2>factory was built, the fuel urea was there, but a

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<v Speaker 2>key piece of machinery UYS was jammed by nickel.

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<v Speaker 3>Okay, so what released the break? What caused the tipping

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<v Speaker 3>point for the goe?

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<v Speaker 2>According to this model, the trigger wasn't some new biological

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<v Speaker 2>invention or mutation in the cyanobacteria. It was a gradual,

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<v Speaker 2>large scale change in Earth's geochemistry that naturally lowered the

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<v Speaker 2>nickel concentration in the oceans.

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<v Speaker 3>The planet itself changed the conditions. How why would nickel

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<v Speaker 3>levels drop?

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<v Speaker 2>This links back to major geological shifts happening around that time,

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<v Speaker 2>roughly two point five billion years ago, the Earth's mantle

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<v Speaker 2>was slowly cooling down less internal heat, less internal heat,

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<v Speaker 2>which meant overall volcanic activity likely decreased. Somewhat Crucially, the

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<v Speaker 2>formation of those super nickel rich comatite rocks largely ceased.

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<v Speaker 2>The source of excessive nickel started to dwindle.

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<v Speaker 3>Okay less input from volcanoes and at the same time

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<v Speaker 3>large stable continental land mass as Cretans were forming and growing.

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<v Speaker 3>The emergence of continents changed global weathering patterns. More land

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<v Speaker 3>surface means different types of chemical weathering, potentially locking up

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<v Speaker 3>nickel and minerals on land rather than letting it wash

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<v Speaker 3>into the sea.

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<v Speaker 2>So less nickel coming in from volcanic sources and maybe

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<v Speaker 2>more getting trapped on land or in sediments. The overall supply.

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<v Speaker 3>Dropped exactly the input decreased, the sinks might have changed,

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<v Speaker 3>and gradually, over millions of years, the concentration of dissolved

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<v Speaker 3>nickel in the oceans fell. It dropped from those incredibly

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<v Speaker 3>high inhibitory archaean levels down to something much closer to

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<v Speaker 3>the trace nutrient levels we see today.

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<v Speaker 2>It crossed a threshold below the level where it poisoned

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<v Speaker 2>the urresenz that's.

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<v Speaker 3>The critical idea. Once nickel dropped below that toxic threshold,

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<v Speaker 3>the urease enzyme was finally free to work efficiently again.

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<v Speaker 3>Cyanobacteria could now effectively utilize the urea that was still present.

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<v Speaker 2>The metabolic break was released.

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<v Speaker 3>The break was off with non inhibitory nickel levels, candobacteria

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<v Speaker 3>could access the nitrogen they needed, and they began to

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<v Speaker 3>proliferate massively globally, sustained large scale growth.

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<v Speaker 2>And that sustained massive growth finally produced oxygen faster than

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<v Speaker 2>the geological and chemical sinks could keep up.

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<v Speaker 3>That is the Great oxidation event, triggered by the geologically

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<v Speaker 3>driven decline in oceanic nickel.

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<v Speaker 2>Wow. That really reframes the whole story. It wasn't about

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<v Speaker 2>waiting for life to figure out oxygen production. It was

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<v Speaker 2>about waiting for the planet's chemistry to allow the oxygen

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<v Speaker 2>producers to truly take over.

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<v Speaker 3>It puts the timing squarely in the core of planetary geochemistry,

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<v Speaker 3>controlling microbioly ecology. The moderation of nickel, and by extension,

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<v Speaker 3>the effective usability of us Rhea pave the way for

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<v Speaker 3>the oxygenated world.

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<v Speaker 2>A much clearer, more mechanistic explanation for that huge delay.

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<v Speaker 2>This is fascinating just for understanding Earth history. But you

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<v Speaker 2>mentioned earlier this has implications beyond our own planet. Let's

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<v Speaker 2>get into that in section four. So what for searching

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<v Speaker 2>for life elsewhere.

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<v Speaker 3>Absolutely, this is where the research really connects to astrobiology.

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<v Speaker 3>Doctor Ratniak explicitly points this out. If we want to

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<v Speaker 3>find life on other planets, understanding the mechanisms that allowed

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<v Speaker 3>life here to fundamentally reshape its environment is critical.

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<v Speaker 2>It's not just about finding life, but finding life that's

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<v Speaker 2>had a planetary impact.

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<v Speaker 3>Or understanding why it hasn't even if it exists. We

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<v Speaker 3>often assume that if life evolves, it will inevitably boom

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<v Speaker 3>and change its planet, maybe producing biosignatures like oxygen that

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<v Speaker 3>we can detect. But this study is a powerful reminder

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<v Speaker 3>that life can exist for vast periods while being ecologically

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<v Speaker 3>suppressed stuck.

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00:19:54.839 --> 00:19:58.400
<v Speaker 2>So when doctor Ratnek says this sheds light on biosignature detection,

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<v Speaker 2>it's not just about looking for oxygen.

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<v Speaker 3>It's about looking for oxygen in context or perhaps explaining

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00:20:03.759 --> 00:20:06.759
<v Speaker 3>its absence. Imagine we find an exoplanet that looks potentially

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<v Speaker 3>habitable with the right temperature, maybe signs of water. We

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00:20:09.640 --> 00:20:12.519
<v Speaker 3>analyze its atmosphere, maybe we don't see much oxygen.

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00:20:12.559 --> 00:20:15.319
<v Speaker 2>We might assume life isn't there or isn't photosynthetic.

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<v Speaker 3>Right, But this research gives us another possibility. Maybe life

398
00:20:19.319 --> 00:20:23.119
<v Speaker 3>is there, Maybe it even invented oxygenic photosynthesis, but it's

399
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<v Speaker 3>stuck in its own great oxidation delay because of a

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00:20:26.240 --> 00:20:30.359
<v Speaker 3>chemical bottleneck. Maybe its star system or planetary geology keeps

401
00:20:30.440 --> 00:20:33.400
<v Speaker 3>baiting the planet in high levels of nickel or some

402
00:20:33.519 --> 00:20:35.079
<v Speaker 3>other inhibitory trace element.

403
00:20:35.200 --> 00:20:38.319
<v Speaker 2>So we need to consider the planet's geochemistry, its likely

404
00:20:38.400 --> 00:20:42.039
<v Speaker 2>trace element environment, alongside the atmospheric gases.

405
00:20:42.200 --> 00:20:46.240
<v Speaker 3>Exactly the star's composition can give clues about the elements

406
00:20:46.400 --> 00:20:50.000
<v Speaker 3>likely abundant in its planets, The planet's age and infer

407
00:20:50.119 --> 00:20:53.359
<v Speaker 3>geological activity matter. It adds a whole new layer to

408
00:20:53.440 --> 00:20:57.920
<v Speaker 3>interpreting potential biosignatures. We shouldn't just look for the smoke oxygen,

409
00:20:58.000 --> 00:21:00.799
<v Speaker 3>but also for the damp wood, the chemical inhibitors that

410
00:21:00.920 --> 00:21:02.559
<v Speaker 3>might be preventing the fire from starting.

411
00:21:02.759 --> 00:21:05.599
<v Speaker 2>And this has direct relevance for missions we're planning now,

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<v Speaker 2>like Mars sample return.

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00:21:07.519 --> 00:21:10.960
<v Speaker 3>Very direct. The paper mentions this provides a new framework

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<v Speaker 3>for the sample analysis strategies. When those precious Martian rock

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00:21:14.240 --> 00:21:16.440
<v Speaker 3>and soil samples eventually get back to Earth labs.

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00:21:16.519 --> 00:21:19.799
<v Speaker 2>We'll be hunting for fossils organic molecules.

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00:21:19.519 --> 00:21:22.720
<v Speaker 3>Yes, but we also need to be meticulously analyzing the

418
00:21:22.839 --> 00:21:26.759
<v Speaker 3>trace element chemistry of those ancient Martian environments. If we

419
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<v Speaker 3>find sediments from a time when Mars might have had

420
00:21:29.559 --> 00:21:33.720
<v Speaker 3>liquid water, maybe even signs of ancient microbial mats or textures,

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00:21:34.440 --> 00:21:37.640
<v Speaker 3>we absolutely need to measure that the nickel concentration in

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00:21:37.720 --> 00:21:41.000
<v Speaker 3>those same layers and look for evidence of nitrogen compounds

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<v Speaker 3>like urea or its.

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00:21:42.400 --> 00:21:45.480
<v Speaker 2>Precursors, because if we find signs of past life but

425
00:21:45.559 --> 00:21:49.839
<v Speaker 2>also evidence of super high nickel levels from that same era, it.

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<v Speaker 3>Could provide a powerful explanation for why Martian life, if

427
00:21:53.200 --> 00:21:56.319
<v Speaker 3>it ever arose, might never have reached the scale needed

428
00:21:56.359 --> 00:21:59.079
<v Speaker 3>to oxygenate the planet like earthlife did. It might have

429
00:21:59.119 --> 00:22:01.599
<v Speaker 3>been stuck in its own biogeochemical bottleneck.

430
00:22:01.839 --> 00:22:04.920
<v Speaker 2>It shifts the question from just was their life to

431
00:22:05.799 --> 00:22:08.720
<v Speaker 2>were the conditions right for life to thrive and reshape

432
00:22:08.720 --> 00:22:09.599
<v Speaker 2>the planet.

433
00:22:09.400 --> 00:22:13.640
<v Speaker 3>Precisely, It's a more nuanced, ecologically informed approach to the search.

434
00:22:13.559 --> 00:22:17.839
<v Speaker 2>And broadening out beyond Mars to exoplanets orbiting distant stars.

435
00:22:18.119 --> 00:22:21.160
<v Speaker 2>We can't get rock samples there obviously, not yet anyway.

436
00:22:21.000 --> 00:22:23.599
<v Speaker 3>But we can analyze the light passing through their atmospheres

437
00:22:23.720 --> 00:22:25.200
<v Speaker 3>looking for chemical fingerprints.

438
00:22:25.400 --> 00:22:28.720
<v Speaker 2>So the interplay between inorganic stuff like nickel and organic

439
00:22:28.759 --> 00:22:31.680
<v Speaker 2>stuff like urea was key on Earth. We should expect

440
00:22:31.720 --> 00:22:34.640
<v Speaker 2>similar complex chemical controls on other worlds.

441
00:22:34.920 --> 00:22:38.200
<v Speaker 3>It seems highly likely biology doesn't happen in a vacuum.

442
00:22:38.279 --> 00:22:42.559
<v Speaker 3>It's constantly interacting with its chemical environment. Different star systems

443
00:22:42.599 --> 00:22:46.119
<v Speaker 3>will have different elemental abundances, Different planets will have different

444
00:22:46.200 --> 00:22:51.720
<v Speaker 3>geological histories, different levels of vulcanism, different atmosphere compositions. It's

445
00:22:51.759 --> 00:22:56.079
<v Speaker 3>almost certain that other bottomeeck elements or compounds exist out there,

446
00:22:56.279 --> 00:22:58.559
<v Speaker 3>controlling the fate of potential biospheres.

447
00:22:58.799 --> 00:23:01.599
<v Speaker 2>So the big lesson for alien hunters is don't just

448
00:23:01.680 --> 00:23:03.000
<v Speaker 2>look for the oxygen.

449
00:23:02.799 --> 00:23:06.720
<v Speaker 3>Or rather understand that oxygen's presence or absence might depend

450
00:23:06.839 --> 00:23:10.519
<v Speaker 3>heavily on these subtle chemical constraints. Look for the conditions

451
00:23:10.519 --> 00:23:13.880
<v Speaker 3>that allow oxygen producing life to dominate. Is the environment

452
00:23:13.960 --> 00:23:17.359
<v Speaker 3>chemically permissive or is there some trace element like nickel

453
00:23:17.559 --> 00:23:20.119
<v Speaker 3>was on early Earth acting as a planetary handbrake.

454
00:23:20.519 --> 00:23:23.039
<v Speaker 2>It really adds layers of complexity, but also makes the

455
00:23:23.039 --> 00:23:26.359
<v Speaker 2>search potentially more revealing Thinking about these chemical governors.

456
00:23:26.599 --> 00:23:29.279
<v Speaker 3>Yeah, it tells us that planetary habitability isn't just about

457
00:23:29.319 --> 00:23:32.000
<v Speaker 3>having the right temperature and water It's also about having

458
00:23:32.079 --> 00:23:35.480
<v Speaker 3>the right trace chemistry. Too much of even a necessary

459
00:23:35.559 --> 00:23:39.000
<v Speaker 3>nutrient can stall life's ability to transform a world for

460
00:23:39.079 --> 00:23:40.079
<v Speaker 3>billions of years.

461
00:23:40.319 --> 00:23:44.119
<v Speaker 2>Incredible that for maybe half a billion years, the entire

462
00:23:44.160 --> 00:23:47.920
<v Speaker 2>trajectory of complex life on Earth hinged on the concentration

463
00:23:48.039 --> 00:23:51.039
<v Speaker 2>of nickel jamming up one specific enzyme.

464
00:23:51.240 --> 00:23:54.160
<v Speaker 3>It really puts things in perspective, doesn't it The intricate

465
00:23:54.279 --> 00:23:58.799
<v Speaker 3>dance between geology and biology. So let's wrap this up.

466
00:23:58.920 --> 00:24:01.359
<v Speaker 3>We've covered a lot of ground, from twenty microbes to

467
00:24:01.400 --> 00:24:02.880
<v Speaker 3>planetary atmospheres we.

468
00:24:02.920 --> 00:24:05.480
<v Speaker 2>Have and the core takeaway from this deep dive from

469
00:24:05.480 --> 00:24:09.680
<v Speaker 2>the Okayama University research is pretty revolutionary. I think that

470
00:24:09.920 --> 00:24:13.799
<v Speaker 2>huge baffling delay in the Great Oxidation Event wasn't primarily

471
00:24:13.839 --> 00:24:16.759
<v Speaker 2>about waiting for evolution to invent something new.

472
00:24:16.920 --> 00:24:17.079
<v Speaker 1>Right.

473
00:24:17.119 --> 00:24:20.960
<v Speaker 3>The machinery the cyanobacteria capable of making oxygen was likely

474
00:24:20.960 --> 00:24:23.920
<v Speaker 3>there for a long long time. The delay was fundamentally

475
00:24:23.960 --> 00:24:24.880
<v Speaker 3>about chemistry and.

476
00:24:24.799 --> 00:24:28.519
<v Speaker 2>Ecology, specifically, the high levels of nickel in the Archaean oceans,

477
00:24:28.599 --> 00:24:31.960
<v Speaker 2>acting in concert with high levels of urea. The nickel

478
00:24:32.000 --> 00:24:35.279
<v Speaker 2>effectively poisoned a key enzyme urease.

479
00:24:35.240 --> 00:24:39.720
<v Speaker 3>Preventing the cyanobacteria from efficiently using the available nitrogen, which

480
00:24:39.759 --> 00:24:42.880
<v Speaker 3>suppressed their growth on a massive scale. It created a

481
00:24:42.880 --> 00:24:45.640
<v Speaker 3>powerful biogeochemical.

482
00:24:44.559 --> 00:24:47.920
<v Speaker 2>Bottleneck, and the planet only started breathing, kicking off the

483
00:24:47.960 --> 00:24:53.480
<v Speaker 2>goe when long term geological changes cooling, mantle changing, volcanism,

484
00:24:53.640 --> 00:24:57.720
<v Speaker 2>continent formation caused the nickel concentration in the oceans to

485
00:24:57.839 --> 00:25:00.200
<v Speaker 2>drop below that critical inhibitory.

486
00:24:59.759 --> 00:25:04.759
<v Speaker 3>Threat, releasing the break, allowing santobacteria to finally bloom globally

487
00:25:04.799 --> 00:25:07.400
<v Speaker 3>and pump out enough oxygen to permanently change the.

488
00:25:07.359 --> 00:25:10.920
<v Speaker 2>Atmosphere, and the ripple effects go way beyond Earth history.

489
00:25:11.039 --> 00:25:13.079
<v Speaker 2>This gives us a whole new framework for looking for

490
00:25:13.160 --> 00:25:13.880
<v Speaker 2>life elsewhere.

491
00:25:13.920 --> 00:25:16.279
<v Speaker 3>Definitely, it tells us to look beyond just the presence

492
00:25:16.279 --> 00:25:20.000
<v Speaker 3>of potential biosignatures like oxygen and consider the enabling or

493
00:25:20.039 --> 00:25:24.039
<v Speaker 3>inhibiting chemical context. Are there trace elements acting as bottlenecks

494
00:25:24.039 --> 00:25:26.720
<v Speaker 3>on other worlds. It adds crucial nuance to how we

495
00:25:26.799 --> 00:25:29.319
<v Speaker 3>interpret data from Mars or distant exoplanets.

496
00:25:29.599 --> 00:25:34.599
<v Speaker 2>It makes this incredibly complex billion years story suddenly click

497
00:25:34.640 --> 00:25:38.240
<v Speaker 2>into place, connecting microscopic enzymes to the fate of the

498
00:25:38.400 --> 00:25:42.039
<v Speaker 2>entire planet. Hopefully, you the listener, feel like you've got

499
00:25:42.079 --> 00:25:45.440
<v Speaker 2>that aha moment now understanding the nuts and bolts of

500
00:25:45.480 --> 00:25:47.599
<v Speaker 2>this ancient bottleneck.

501
00:25:47.240 --> 00:25:49.039
<v Speaker 3>So we'll leave you with a final thought to mull

502
00:25:49.079 --> 00:25:52.680
<v Speaker 3>over building on this idea, if a chemical bottleneck high

503
00:25:52.720 --> 00:25:56.359
<v Speaker 3>nickel levels held back Earth's oxygenation for maybe half a

504
00:25:56.400 --> 00:26:01.319
<v Speaker 3>billion years, what subtle chemical factor, what unseen trace element

505
00:26:01.640 --> 00:26:03.640
<v Speaker 3>might be playing a similar role right now on an

506
00:26:03.640 --> 00:26:06.440
<v Speaker 3>exoplanet that otherwise looks perfectly right for life.

507
00:26:06.480 --> 00:26:10.000
<v Speaker 2>Could there be countless worlds out there teeming with microbial life,

508
00:26:10.039 --> 00:26:13.440
<v Speaker 2>just patiently waiting for their own planet's nickel concentration or

509
00:26:13.480 --> 00:26:16.319
<v Speaker 2>something equivalent to finally drop so they can kick off

510
00:26:16.319 --> 00:26:17.880
<v Speaker 2>their own great oxidation event.

511
00:26:18.319 --> 00:26:20.039
<v Speaker 3>Makes you wonder what the universe might look like in

512
00:26:20.079 --> 00:26:21.680
<v Speaker 3>another billion years, doesn't.

513
00:26:21.400 --> 00:28:03.079
<v Speaker 4>It, said us used
