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 close your eyes for a second,

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<v Speaker 2>just for a moment. Forget about your to do list,

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<v Speaker 2>forget about the emails pinging in your inbox. Instead, I

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<v Speaker 2>want you to picture a heist.

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<v Speaker 3>Not your typical heist though, No ski masks, no getaway cars, no,

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<v Speaker 3>nothing like that.

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<v Speaker 2>This is a heist happening, oh about two hundred million

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<v Speaker 2>miles away from where you're sitting. Picture a robot, maybe

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<v Speaker 2>the size of a large van, and it's just floating

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<v Speaker 2>in the complete absolute silence of deep space.

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<v Speaker 3>And its target is this mountain of rubble that's just

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<v Speaker 3>tumbling through the dark.

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<v Speaker 2>Exactly it's trying to I don't know, high five. This

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<v Speaker 2>spinning pile of rocks and mountain.

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<v Speaker 3>Of rubble is actually, you know, not far from the

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<v Speaker 3>scientific term. We're talking about the asteroid Benu. It's what's

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<v Speaker 3>called a rubble pile asteroid, which means it's basically a

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<v Speaker 3>loose collection of rocks and dust all held together by well,

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<v Speaker 3>not much more than its own weak gravity.

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<v Speaker 2>It's it's fragile, right, And this Robi, which is Nanza's

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<v Speaker 2>Osyrius for Rex spacecraft, had one job, just one incredibly delicate,

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<v Speaker 2>high stakes job. Go to this asteroid, match its speed,

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<v Speaker 2>match it spin, then reach out an arm, touch the

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<v Speaker 2>surface for just a few seconds, grab a little souvenir,

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<v Speaker 2>and then fly all the way home.

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<v Speaker 3>It sounds so simple when you put it like that.

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<v Speaker 2>It sounds simple when you say it fast. But it

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<v Speaker 2>was anything but. I mean, the level precision is just

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<v Speaker 2>it's mind boggling.

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<v Speaker 3>And it was even harder than they planned when they

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<v Speaker 3>actually made contact. This was back in twenty twenty. The

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<v Speaker 3>surface was so much softer than their models predicted.

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<v Speaker 2>Softer.

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<v Speaker 3>Yeah, the collection arm it almost sank right into the astray.

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<v Speaker 3>It was like trying to punch a ball pit. The

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<v Speaker 3>surface just gave way.

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<v Speaker 2>I remember seeing the video from the spacecraft's camera. Yes,

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<v Speaker 2>it was terrifying to watch. Yeah, dust and pebbles flying everywhere.

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<v Speaker 2>You realize, if that arm gets stuck, or if the

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<v Speaker 2>thrusters fire at the wrong second, that's it. The whole

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<v Speaker 2>mission is lost.

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<v Speaker 3>Billions of dollars, decades of work just gone. But they

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<v Speaker 3>pulled it off. They fired the thrusters, they backed away,

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<v Speaker 3>and they had the goods. They sealed up the sample capsule.

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<v Speaker 2>And then came the long trip home and finally, in

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<v Speaker 2>twenty twenty three, that little capsule came blazing through our

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<v Speaker 2>atmosphere and parachuted down into the Utah Desert.

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<v Speaker 3>And that's another moment where you're holding your breath. I mean,

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<v Speaker 3>if that parachute doesn't deploy correctly, if the capsule cracks

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<v Speaker 3>open on impact.

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<v Speaker 2>All that effort, all that distance, and you just end

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<v Speaker 2>up with a very expensive crater in the sand exactly.

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<v Speaker 2>But it worked. It stuck the landing, and inside, once

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<v Speaker 2>they got it into a pristine, sterile clean room and

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<v Speaker 2>carefully opened it up, they found dust, just a little

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<v Speaker 2>cups worth of this very dark, very jagged dust.

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<v Speaker 3>And that dust, specifically about a teaspoon of it is

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<v Speaker 3>what we are here to talk about today, because this

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<v Speaker 3>isn't just a story about an amazing engineering feat. Yeah,

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<v Speaker 3>we were looking at a paper that was published literally yesterday,

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<v Speaker 3>February ninth, twenty twenty six, in the Proceedings of the

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<v Speaker 3>National Academy of Sciences. And it turns out that teaspoon

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<v Speaker 3>of Dust contains a story that well, it completely rewrites

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<v Speaker 3>what we thought we knew about the chemistry of life.

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<v Speaker 2>It really does. It's one of those moments in science

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<v Speaker 2>where you realize the recipe book you've been using might

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<v Speaker 2>have been missing a critical chapter, or maybe we were

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<v Speaker 2>just reading the wrong one entirely.

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

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<v Speaker 2>So let's set the stage here. The big headline is

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<v Speaker 2>that researchers from Penn State found amino acids in this

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<v Speaker 2>venue dust. But and I want to be really clear

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<v Speaker 2>on this, because it confused me at first finding amino

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<v Speaker 2>acids in space. That's not the new part, is it.

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<v Speaker 3>No, And you are absolutely right to flag that that's

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<v Speaker 3>the key nuance. If the headline was just scientists find

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<v Speaker 3>organics on asteroid, we'd say, ok, add it to the

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<v Speaker 3>growing list.

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<v Speaker 2>We've known for decades, really that space rocks can carry

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<v Speaker 2>these kinds of molecules.

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<v Speaker 3>So what's the big deal. Why is this particular discovery

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<v Speaker 3>causing such a stir.

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<v Speaker 2>It's because of the how. It's not that they found

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<v Speaker 2>amino acids. It's the story those amino acids have to tell.

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<v Speaker 2>It's about their history. It's like finding a person in

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<v Speaker 2>New York City. That's not a story, but finding out

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<v Speaker 2>they got there by walking from Antarctica, that's a story.

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<v Speaker 3>Okay, I like that. So we're looking at the molecule's journey.

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<v Speaker 3>It's origin story we are, And for the last fifty

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<v Speaker 3>years we had a pretty solid theory about that origin story.

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<v Speaker 3>We thought the answer was always you know, warmth and water.

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<v Speaker 2>The famous warm little pond that Darwin talked.

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<v Speaker 3>About, the very same, the classic idea. But the samples

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<v Speaker 3>from Benu they're telling us something completely different. They're saying

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<v Speaker 3>the ingredients for life don't just form in cozy, warm ponds.

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<v Speaker 2>They formed somewhere else.

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<v Speaker 3>They can form in the deep freeze, in the pitch dark,

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<v Speaker 3>in an environment that should be, by all accounts, completely

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<v Speaker 3>hostile to creating these delicate molecules.

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<v Speaker 2>We're talking about, what a radioactive environment.

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<v Speaker 3>We're talking about frozen eyes being blasted by gamma rays,

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<v Speaker 3>the harsh, unforgiving vacuum of the outer Solar system.

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<v Speaker 2>Wow, that's well, it sounds more like the origin story

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<v Speaker 2>for comic book Supervillain, not the origin story for life

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<v Speaker 2>on Earth.

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<v Speaker 3>And that's precisely why this is a revelation. The lead author,

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<v Speaker 3>Alison Bozinski says, it flips the script on where we

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<v Speaker 3>should be looking for life's ingredients and maybe even life itself.

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<v Speaker 2>So our mission today for this deep dive seems pretty clear.

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<v Speaker 2>We're going to unpack this brand new study. We're going

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<v Speaker 2>to look at the incredible technology this team, led by

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<v Speaker 2>Alison Bozinski and Elflee Macintosh used to basically read the

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<v Speaker 2>atomic history of these molecules, and we're going to try

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<v Speaker 2>to understand why a freezing radioactive void might actually be

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<v Speaker 2>a better kitchen for creating life's building blocks than a

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<v Speaker 2>warm bath.

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<v Speaker 3>And beyond that, we have to talk about what this

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<v Speaker 3>means for the rest of the universe, because if you

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<v Speaker 3>don't need a special Goldilocks planet with warm oceans to

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<v Speaker 3>make amino acids, if you can just make them in

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<v Speaker 3>the cold darkness of space.

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<v Speaker 2>Then the universe might be a lot more seeded with

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<v Speaker 2>potential than we ever thought.

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<v Speaker 3>Exactly the ingredients for the recipe it could be everywhere.

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<v Speaker 2>Okay, I love this let's start with the sample itself,

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<v Speaker 2>the Messenger from the Dawn of Time? Why this rock?

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<v Speaker 2>Why Benu? What made NASA spend over a billion dollars

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<v Speaker 2>to go to this specific pile of rubble.

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<v Speaker 3>To really appreciate the science, you have to appreciate the sample.

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<v Speaker 3>And as you mentioned, this material from Osiris Rex is

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<v Speaker 3>special for one big reason. The word is pristine.

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<v Speaker 2>Pristine meaning untouched.

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<v Speaker 3>Completely untouched. See, most of the time when we study

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<v Speaker 3>space rocks, we're studying meteorites, and meteorites are well, they're compromised,

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<v Speaker 3>they've been through the Ringer, right.

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<v Speaker 2>They didn't have a nice, gentle parachute landing in Utah,

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<v Speaker 2>not at all.

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<v Speaker 3>Think about the journey of a typical meteorite. It spends

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<v Speaker 3>maybe millions, even billions of years floating through space, getting

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<v Speaker 3>bombarded by radiation. Then it hits Earth's atmosphere at what

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<v Speaker 3>thirty thousand miles an hour.

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<v Speaker 2>It's a fireball. It literally burns up.

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<v Speaker 3>It burns at thousands of degrees, the outer layers or vaporized.

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<v Speaker 3>It often breaks apart. It's a profoundly traumatic entry. And

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<v Speaker 3>then if a piece survives, it lands maybe in the

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<v Speaker 3>Antarctic ice. If we're lucky, or maybe it lands in

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<v Speaker 3>a field in Iowa.

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<v Speaker 2>Or jungle or the ocean.

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<v Speaker 3>Exactly, and it just sits there. It gets rained on.

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<v Speaker 3>Microbes and bacteria from Earth's soil start to crawl all

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<v Speaker 3>over it. It gets buried in mud. Humans eventually find it

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<v Speaker 3>and touch it with their oily, greasy fingers.

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<v Speaker 2>So it's contaminated from the second it enters our world.

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<v Speaker 2>It's being altered.

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<v Speaker 3>It is heavily, heavily contaminated. From a chemical analysis standpoint,

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<v Speaker 3>It's like trying to read an ancient scroll that's been

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<v Speaker 3>dropped in a puddle, then dried by a fire, and

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<v Speaker 3>then scribbled on by a toddler. You can still make

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<v Speaker 3>out some of the original text, but you're never one

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<v Speaker 3>hundred percent sure what's original and what's just dirt from

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<v Speaker 3>the journey.

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<v Speaker 2>But the Benu sample is different.

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<v Speaker 3>The Benu sample is a completely different ballgame. It was

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<v Speaker 3>a grab and go mission. We flew to the source,

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<v Speaker 3>We used a sterile robotic arm to grab the dust.

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<v Speaker 3>We sealed it in a hermetically sealed capsule right then

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<v Speaker 3>and there in space, and we brought it home.

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<v Speaker 2>It never touched Earth's atmosphere. It never saw rain. It

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<v Speaker 2>never encountered a single Earth bacterium.

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<v Speaker 3>Until the moment it was opened in that NASA clean room.

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<v Speaker 3>That dust was exactly as it had been for four

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<v Speaker 3>point six billion years, floating out there in the void.

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<v Speaker 2>So what this study is looking at is the real deal.

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<v Speaker 2>This is unfiltered history.

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<v Speaker 3>It is the closest thing we have to a perfect

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<v Speaker 3>time capsule from the birth of our solar system, back

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<v Speaker 3>before Earth even had oceans, before the first cell ever divided.

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<v Speaker 3>This is a snapshot of the raw material that built everything.

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<v Speaker 2>And what's just staggering to me is the amount of

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<v Speaker 2>material they're working with. You said a teaspoon. The breakthrough

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<v Speaker 2>came from a sample no bigger than a teaspoon of dust.

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<v Speaker 3>It really is a testament to the lane level of

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<v Speaker 3>technology we have now. The team at Penn State, the

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<v Speaker 3>lead researchers Alison Basinski and Offley Macintosh, along with Christopher House,

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<v Speaker 3>Catherine Freeman, and Mila Mattney, they weren't just putting this

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<v Speaker 3>dust under a normal microscope. They were using instruments that

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<v Speaker 3>tear molecules apart adam by adam and weigh them.

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<v Speaker 2>Zuski had a quote in the press release about this,

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<v Speaker 2>didn't she something like without these advances in technology.

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<v Speaker 3>She said, we would never have made this discovery. And

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<v Speaker 3>she's absolutely right, because they were looking for what she

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<v Speaker 3>called really low abundances. These aren't huge, visible chunks of

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<v Speaker 3>organic stuff. These are trace amounts parts per billion locked

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<v Speaker 3>inside the mineral structure of the dust. You need instruments

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<v Speaker 3>with incredible sensitivity to even see them, let alone analyze

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<v Speaker 3>their history.

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<v Speaker 2>Okay, so let's get into what they actually found. We

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<v Speaker 2>keep using the term amino acids, and I feel like

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<v Speaker 2>most of us have heard that term, maybe on a

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<v Speaker 2>nutritional labels or in a biology class. But let's really

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<v Speaker 2>define it for our context here. What exactly are we

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<v Speaker 2>looking at.

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<v Speaker 3>The best analogy, and it's one we use a lot

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<v Speaker 3>in science communication is lego bricks.

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<v Speaker 2>Legos. I can do legos. Everyone gets legos.

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<v Speaker 3>Imagine you have a giant bin of mixed lego bricks.

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<v Speaker 3>An individual brick, say a single red two by four piece,

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<v Speaker 3>is just a piece of plastic. It doesn't do much

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<v Speaker 3>on its own, but if you start snapping them together

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<v Speaker 3>in a specific sequence, you can build anything. A house,

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<v Speaker 3>a spaceship, a working model of a car engine. The

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<v Speaker 3>complexity emerges from how you connect the simple pieces.

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<v Speaker 2>So the power isn't in the brick, it's in the

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<v Speaker 2>structure you build with it.

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<v Speaker 3>Precisely, in the world of biology, amino acids are those

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<v Speaker 3>lego bricks. You snap them together in long chains to

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<v Speaker 3>build proteins, and proteins proteins are the machines that run

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<v Speaker 3>the city of life. They do all the work, They

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<v Speaker 3>do everything. They form the physical structure of your cells,

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<v Speaker 3>like the steel beams and a skyscraper. They act as

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<v Speaker 3>enzymes to catalyze chemical reactions like digesting your food. They

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<v Speaker 3>carry oxygen in your blood. They fight off diseases as antibodies.

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<v Speaker 3>Without protein, you can't replicate DNA, you can't have a metabolism.

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<v Speaker 3>There is no life as we know it without them.

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<v Speaker 2>So finding these fundamental lego bricks on an asteroid is

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<v Speaker 2>a huge deal because it suggests the raw materials for

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<v Speaker 2>life weren't invented here on Earth. Yeah, we didn't have

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<v Speaker 2>to manufacture the plastic for the bricks ourselves. They were

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<v Speaker 2>delivered to us pre made in the box.

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<v Speaker 3>That is a perfect way to phrase it. And in

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<v Speaker 3>this particular study from Penn State, they were focused on

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<v Speaker 3>one specific very important amino acid glycine.

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<v Speaker 2>Glycine, Why that one is it special?

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<v Speaker 3>It's special because it's the simplest. If we're sticking with

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<v Speaker 3>the Lego analogy, glycine is the most basic brick. It's

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<v Speaker 3>the little two by two square. It's the smallest possible

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<v Speaker 3>amino acid, just a tiny two carbon molecule. But because

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<v Speaker 3>it's so simple and fundamental, it's found everywhere in biology.

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<v Speaker 2>Okay, so they found glycine in the binu dust. But

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<v Speaker 2>as we established earlier, we found glycine in space before

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<v Speaker 2>we have Yes, So this is where we get to

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<v Speaker 2>the script slip. You mentioned Lit's dig into the old

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<v Speaker 2>theory before this paper dropped yesterday. If I were to

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<v Speaker 2>ask you, how does glycine form in space? What would

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<v Speaker 2>the textbook answer have been?

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<v Speaker 3>The textbook answer for about half a century would have

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<v Speaker 3>been a process called Strucker synthesis.

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<v Speaker 2>Treker synthesis sounds like a villain's evil plan in a

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<v Speaker 2>spy movie. We must initiate Operation Strecker.

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<v Speaker 3>It does have that ring to it, doesn't it. But

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<v Speaker 3>it's actually some pretty classic old school chemistry. It's named

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<v Speaker 3>after Adolph Strecker, who figured this out all the way

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<v Speaker 3>back in the eighteen fifties.

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<v Speaker 2>The eighteen fifties, So this is really foundational chemistry.

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<v Speaker 3>Very foundational, And for Streker synthesis, you need a few

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<v Speaker 3>key ingredients. First, you need some kind of aldehyde or ketne.

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<v Speaker 3>You can just think of that as your basic carbon

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<v Speaker 3>containing molecule. Then you need ammonia. That's your source of nitrogen.

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<v Speaker 3>And you need hydrogen cyanide.

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<v Speaker 2>Hydrogen cyanide. Wait a second, isn't that Isn't that a

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<v Speaker 2>lethal poison to us?

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<v Speaker 3>Absolutely, it's incredibly toxic, But in the world of prebiotic chemistry,

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<v Speaker 3>it's an essential ingredient. It's a very simple molecule containing

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<v Speaker 3>carbon and nitrogen, and it's very very reactive.

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<v Speaker 2>It's just so ironic that a key ingredient for life

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<v Speaker 2>is something that's so deadly to life.

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<v Speaker 3>Chemistry is full of these little ironies. But here's the

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<v Speaker 3>crucial part of the recipe. If you just take those

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<v Speaker 3>three ingredients, the aldehyde, the ammonia, the cyanide, and you

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<v Speaker 3>put them in a jar and shake them up as gases,

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<v Speaker 3>basically nothing happens. They just bounce off each other. They

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<v Speaker 3>need a catalyst, a match.

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<v Speaker 2>Maker, if you will, and the match maker is water.

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<v Speaker 3>Liquid water. Absolutely, water acts as a solvent. It allows

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<v Speaker 3>these molecules to dissolve, to move around freely, to exchange protons,

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<v Speaker 3>and to actually interact and react with each other. But

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<v Speaker 3>you need one more thing. You need energy. You need heat. Well,

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<v Speaker 3>the heat, because molecules are fundamentally lazy, they're stable in

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<v Speaker 3>the current forms. To get them to break their existing

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<v Speaker 3>bonds and form new, more complex ones, to get them

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<v Speaker 3>to rearrange themselves into an amino acid, you need to

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<v Speaker 3>give them an energetic shove. Heat provides that shove. It's

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<v Speaker 3>kinetic energy. It makes the molecules vibrate and smash into

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<v Speaker 3>each other with enough force to trigger the reaction.

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<v Speaker 2>So the warm little pond concept isn't just a nice

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<v Speaker 2>poetic image. It's a literal chemical requirement. You need a

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<v Speaker 2>liquid medium for the ingredients to mix, and you need

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<v Speaker 2>warmth to make the reaction go precisely.

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<v Speaker 3>So, for fifty years, whenever we found amino acids and meteorites,

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<v Speaker 3>the assumption was always Okay, this rock must have, at

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<v Speaker 3>some point in its history been part of a larger

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<v Speaker 3>parent body that had liquid water and some source of

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<v Speaker 3>internal heat.

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<v Speaker 2>We just assumed it was cooked in some kind of

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<v Speaker 2>cosmic crock pot, maybe inside a big asteroid with hydrothermal vents,

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<v Speaker 2>or some surface ocean warmed by radioactive decay.

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<v Speaker 3>Exactly. We were, in a way projecting our own planet

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<v Speaker 3>story onto the rest of the Solar System. We see

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<v Speaker 3>life thriving in water here, so we assumed life's ingredients

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<v Speaker 3>must also need water there.

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<v Speaker 2>But Benu is here to tell us that's not the

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<v Speaker 2>only way.

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<v Speaker 3>Benu is telling us something radically different. And this is

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<v Speaker 3>where the real detective work gets incredibly cool. This is

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<v Speaker 3>where we have to talk about isotopes.

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<v Speaker 2>Lisotopes. Okay, I remember the term from high school chemistry,

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<v Speaker 2>but let's do a quick refresher. How does weighing an

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<v Speaker 2>atom tell you anything about its past.

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<v Speaker 3>Think of atoms of a particular element like carbon, as

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<v Speaker 3>all being part of the same family. They all have

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<v Speaker 3>six protons. That's what makes them carbon. But some family

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<v Speaker 3>members might weigh a little more than others. They might

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<v Speaker 3>have an extra neutron or two in their nucleus.

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<v Speaker 2>So it's the same element chemically, it just has a

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<v Speaker 2>bit more mass. It's the chubby cousin of the family.

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<v Speaker 3>That's a perfect analogy. It's a chubby atom had a

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<v Speaker 3>little extra baggage. It's still carbon. It behaves light carbon.

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<v Speaker 3>It forms bonds like carbon, but it's heavier. We call

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<v Speaker 3>these heavier versions isotopes. Carbon twelve is the common one.

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<v Speaker 3>Carbon thirteen is the heavier one. Now Here is the

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<v Speaker 3>magic trick of this whole science. The ratio of the

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<v Speaker 3>heavy atoms to the light atoms in a molecule acts

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<v Speaker 3>like a passport stamp. It tells you where that molecule

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<v Speaker 3>was born.

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<v Speaker 2>Wait, how why would the environment affect how many chubby

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<v Speaker 2>atoms get included in the molecule.

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<v Speaker 3>It comes down to a principle called the kinetic isotope effect.

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<v Speaker 2>Okay, but that sounds complicated, but break it down for us.

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<v Speaker 3>It's actually just about that molecular laziness we talked about again.

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<v Speaker 3>It turns out that chemical bonds involving the heavier isotope

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<v Speaker 3>carbon thirteen are just a tiny bit stronger and more stable.

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<v Speaker 3>They take a little more energy to break. So if

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<v Speaker 3>you have a chemical reaction happening in that warm pond,

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<v Speaker 3>a reaction that requires breaking bonds, it's slightly easier. It

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<v Speaker 3>takes less energy to break the bond with the lighter

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<v Speaker 3>carbon twelve atom, so.

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<v Speaker 2>Nature takes the path of least resistance. The reaction prefers

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<v Speaker 2>the lighter easier to work with atoms. You got it.

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<v Speaker 3>So, generally speaking, chemical reactions driven by heat and happening

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<v Speaker 3>in water will end up with a product that is

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<v Speaker 3>depleted in the heavy isotope. They discriminate against the heavy stuff.

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<v Speaker 2>So if I analyze the molecule made in a warm environment,

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<v Speaker 2>it's isotopic fingerprint should show it's full of the light stuff.

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<v Speaker 2>Relatively speaking, yes, it.

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<v Speaker 3>Will have a very specific, predictable ratio of light versus

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<v Speaker 3>heavy atoms. But here's the amazing part. At extremely cold

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<v Speaker 3>temperatures we're talking deep space cold hundreds of degrees below zero,

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<v Speaker 3>the rules of chemistry change. When you're not using heat

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<v Speaker 3>to drive reactions, but you're using high energy radiation instead,

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<v Speaker 3>that discrimination goes away.

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<v Speaker 2>Radiation doesn't care if an atom is chevy or not.

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<v Speaker 3>Radiation is like a sledgehammer. Heat is like a gentle push.

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<v Speaker 3>The sledgehammer doesn't care if the one bond is slightly

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<v Speaker 3>stronger than another. It just smashes everything. So reactions that

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<v Speaker 3>are driven by radiation and frozen ice tend to incorporate

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<v Speaker 3>the heavy and light isotopes in a different, more random

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<v Speaker 3>seeming ratio. They don't show the same preference for the

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<v Speaker 3>light stuff.

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<v Speaker 2>I think I'm getting it. So the Penn State team,

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<v Speaker 2>kachen Ski, Macintosh and the others, they take the glycine

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<v Speaker 2>from the Beni sample. They put it in their super

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<v Speaker 2>sensitive machine.

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<v Speaker 3>A set of custom instruments, a mass spectrometer.

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<v Speaker 2>And they literally just count the number of heavy carbon

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<v Speaker 2>atoms versus light carbon atoms than nitrogen atoms too.

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<v Speaker 3>That's essentially it. They measure that ratio with incredible precision,

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<v Speaker 3>and the ratio they found it sacreamed coald. It screamed ice.

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<v Speaker 2>It didn't look like the ratio from the Streker synthesis,

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<v Speaker 2>the warm pond dress.

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<v Speaker 3>It wasn't even in the same ballpark. The isotopic signature

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<v Speaker 3>was completely inconsistent with formation in liquid water, but it

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<v Speaker 3>perfectly matched the signature you'd expect from formation in solid

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<v Speaker 3>frozen ice. Ice frozen solid, and not just ice sitting

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<v Speaker 3>there peacefully, but ice being actively zapped by high energy

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<v Speaker 3>cosmic rays and gamma rays.

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<v Speaker 2>Okay, so let me see if I can picture this.

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<v Speaker 2>The ingredients we talked about before, the ammonia, the cyani

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<v Speaker 2>the simple carbon molecules. They're not dissolved in water. They're

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<v Speaker 2>just trapped frozen solid inside.

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<v Speaker 3>A block of ice exactly. They are suspended in the

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<v Speaker 3>ice matrix like fruit in a jello mole and.

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<v Speaker 2>Then over millions of years, radiation from space comes along

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<v Speaker 2>and just zaps them, and that forces them to become

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<v Speaker 2>amino acids.

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<v Speaker 3>That's the idea. The process is called radiolysis. The high

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<v Speaker 3>energy radiation particle smashes into a water molecule in the ice,

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<v Speaker 3>shattering it and creating these incredibly reactive fragments called radicals.

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<v Speaker 3>These radicals are like like chemical grenades. They are desperate

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<v Speaker 3>to react with anything nearby, so they attack the frozen cyanide,

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00:19:10.759 --> 00:19:13.559
<v Speaker 3>they attack the ammonia, and they force them to combine

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<v Speaker 3>in new ways.

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<v Speaker 2>So the radiation is providing the energy that the heat

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<v Speaker 2>would have provided in the warm pond.

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<v Speaker 3>Precisely, but it's doing it without ever melting the ice.

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00:19:21.759 --> 00:19:24.799
<v Speaker 3>It's a cold forging process, and it's a process that

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<v Speaker 3>happens in what the paper calls the outer reaches of

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<v Speaker 3>the early Solar System.

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<v Speaker 2>The outer reaches, so we're talking way out there beyond Mars,

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<v Speaker 2>beyond the asteroid belt, maybe upast Jupiter, way out.

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<v Speaker 3>In the cold, dark vacuum, in a region we typically

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<v Speaker 3>think of as a chemical wasteland, a place we considered

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<v Speaker 3>hostile to the formation of complex organic molecules.

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<v Speaker 2>This is that script flip that Bazinski mentioned.

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<v Speaker 3>It is her direct quote was our results flip, the

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<v Speaker 3>script on how we have typically thought amino acids formed.

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<v Speaker 2>It's just it's incredible. It suggests that the potential for

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<v Speaker 2>life is so much more rugged and persistent than we

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<v Speaker 2>gave it credit for. It doesn't need to wait around

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<v Speaker 2>for a perfect little planet with a nice ocean to

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<v Speaker 2>get started. The chemistry can begin in the harshest parts

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<v Speaker 2>of the void.

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<v Speaker 3>That's the profound implication. It means these fundamental molecules aren't

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<v Speaker 3>rare flukes restricted to these little goldilock zones where the

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<v Speaker 3>temperature is just right for liquid water. Bazinski put it perfectly,

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<v Speaker 3>It now looks like there are many conditions where these

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<v Speaker 3>building blocks of life can form.

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<v Speaker 2>It's all about diversity.

424
00:20:26.160 --> 00:20:29.839
<v Speaker 3>Diversity in the pathways to life. Can you make glycine

425
00:20:29.839 --> 00:20:33.559
<v Speaker 3>in a warm watery asteroid, Yes, absolutely, that method works,

426
00:20:33.920 --> 00:20:35.680
<v Speaker 3>But this shows you can also make it in a

427
00:20:35.759 --> 00:20:37.839
<v Speaker 3>radioactive ice cube floating in the dark.

428
00:20:38.039 --> 00:20:41.519
<v Speaker 2>That just feels huge. It makes the universe feel less

429
00:20:41.559 --> 00:20:43.960
<v Speaker 2>like this vast empty place where life is a one

430
00:20:44.000 --> 00:20:47.279
<v Speaker 2>and a trillion miracle, and more like a giant factory

431
00:20:47.319 --> 00:20:51.279
<v Speaker 2>that's constantly in different departments churning out the necessary parts

432
00:20:51.319 --> 00:20:53.079
<v Speaker 2>for life, no matter the local conditions.

433
00:20:53.319 --> 00:20:56.519
<v Speaker 3>A factory is a fantastic analogy. And this brings us

434
00:20:56.559 --> 00:21:00.880
<v Speaker 3>to a really fascinating comparison. The study made really nailed

435
00:21:00.880 --> 00:21:03.720
<v Speaker 3>down their case. They didn't just look at Benu by itself.

436
00:21:04.160 --> 00:21:07.440
<v Speaker 3>They put it head to head with the undisputed celebrity

437
00:21:07.480 --> 00:21:08.559
<v Speaker 3>of the metiorrite world.

438
00:21:08.680 --> 00:21:13.359
<v Speaker 2>Ah. Yes, you're talking about the Murchison metiaorite, the heavyweight champion.

439
00:21:13.039 --> 00:21:16.200
<v Speaker 3>The one and only Murchison. It fell in a shower

440
00:21:16.279 --> 00:21:19.160
<v Speaker 3>over the town of Murchison, Australia, back in nineteen sixty nine.

441
00:21:19.240 --> 00:21:21.599
<v Speaker 2>Nineteen sixty nine, what a year for space. We go

442
00:21:21.680 --> 00:21:23.720
<v Speaker 2>to the Moon and a piece of the early Solar

443
00:21:23.720 --> 00:21:24.640
<v Speaker 2>System comes to us.

444
00:21:24.759 --> 00:21:28.480
<v Speaker 3>A huge year, and Murchison is this carbon rich meteorite

445
00:21:28.519 --> 00:21:32.400
<v Speaker 3>that became the absolute gold standard for astrobiology for fifty years.

446
00:21:32.759 --> 00:21:34.920
<v Speaker 3>If you were a scientist in the eighties nineties, even

447
00:21:34.920 --> 00:21:37.440
<v Speaker 3>the two thousands, and you wanted to study amino acids

448
00:21:37.440 --> 00:21:40.440
<v Speaker 3>from space. You begged, borrowed, and stole for a tiny

449
00:21:40.480 --> 00:21:41.359
<v Speaker 3>crumb of Murchison.

450
00:21:41.480 --> 00:21:43.200
<v Speaker 2>And what did Murchison's story tell us?

451
00:21:43.359 --> 00:21:46.799
<v Speaker 3>Well, for all those decades, Murchison consistently confirmed the old theory.

452
00:21:47.079 --> 00:21:50.720
<v Speaker 3>When scientists analyzed the isotopes of the amino acids inside Murchison,

453
00:21:50.839 --> 00:21:53.319
<v Speaker 3>the fingerprint was clear. It said I was made in

454
00:21:53.480 --> 00:21:54.640
<v Speaker 3>warm liquid water.

455
00:21:54.880 --> 00:21:57.640
<v Speaker 2>So Murchison fits the classic warm pond theory to a

456
00:21:57.680 --> 00:21:58.759
<v Speaker 2>t perfectly.

457
00:21:59.160 --> 00:22:02.759
<v Speaker 3>The evidence from murch strongly suggests its parent body, the

458
00:22:02.880 --> 00:22:05.279
<v Speaker 3>larger asteroid it broke off from, was a place that

459
00:22:05.319 --> 00:22:09.359
<v Speaker 3>had liquid water flowing and relatively mild temperatures, conditions that

460
00:22:09.559 --> 00:22:12.559
<v Speaker 3>ironically look a lot like what we think early Earth

461
00:22:12.680 --> 00:22:12.960
<v Speaker 3>was like.

462
00:22:13.279 --> 00:22:15.960
<v Speaker 2>So for half a century we built our entire model

463
00:22:16.000 --> 00:22:19.480
<v Speaker 2>of prebiotic chemistry in the Solar System based on Murchison.

464
00:22:20.000 --> 00:22:24.240
<v Speaker 2>We pictured these big, warm, wet asteroids breaking apart and

465
00:22:24.279 --> 00:22:26.880
<v Speaker 2>delivering their life giving cargo to the early planets.

466
00:22:27.000 --> 00:22:30.119
<v Speaker 3>That was the dominant model. But now Benu walks into

467
00:22:30.160 --> 00:22:30.759
<v Speaker 3>the room.

468
00:22:30.640 --> 00:22:32.960
<v Speaker 2>And Benu is the rebel, the nonconformist.

469
00:22:33.039 --> 00:22:36.279
<v Speaker 3>Benu stands up and says, hey, I've got amino acids too,

470
00:22:36.400 --> 00:22:38.400
<v Speaker 3>loads of them. But I've never been warm a day

471
00:22:38.440 --> 00:22:41.119
<v Speaker 3>in my four point six billion year life. I've been

472
00:22:41.200 --> 00:22:43.000
<v Speaker 3>floating in the deep freeze.

473
00:22:43.119 --> 00:22:45.920
<v Speaker 2>The steady shows Binez amino acids have a much different

474
00:22:45.920 --> 00:22:47.759
<v Speaker 2>isotopic pattern than Murchison's.

475
00:22:47.799 --> 00:22:50.599
<v Speaker 3>So you have two ancient rocks, both from our solar system,

476
00:22:50.640 --> 00:22:53.079
<v Speaker 3>both the same age. One says I was cooked in

477
00:22:53.119 --> 00:22:55.440
<v Speaker 3>water and the other says I was forged in ice

478
00:22:55.480 --> 00:22:58.720
<v Speaker 3>and radiation. And Ofully Macintosh, the other lead author on

479
00:22:58.759 --> 00:23:01.799
<v Speaker 3>the paper, spelled out exactly what this means. She said,

480
00:23:01.799 --> 00:23:04.599
<v Speaker 3>it suggests that the parent bodies of Benu and Murchison

481
00:23:04.920 --> 00:23:08.240
<v Speaker 3>originated in chemically distinct regions of the Solar system.

482
00:23:08.599 --> 00:23:12.559
<v Speaker 2>Chemically distinct regions, not all from the same place.

483
00:23:12.960 --> 00:23:16.319
<v Speaker 3>Right. Think of the early Solar system, that big disk

484
00:23:16.400 --> 00:23:19.359
<v Speaker 3>of gas and dust around the young Sun. Not as

485
00:23:19.359 --> 00:23:22.640
<v Speaker 3>a well mixed soup, but as a giant industrial kitchen

486
00:23:22.680 --> 00:23:23.440
<v Speaker 3>with different.

487
00:23:23.160 --> 00:23:24.519
<v Speaker 2>Stations, the solar kitchen.

488
00:23:24.559 --> 00:23:27.599
<v Speaker 3>I like that exactly. So maybe closer to the Sun,

489
00:23:27.799 --> 00:23:29.799
<v Speaker 3>or perhaps in the main asteroid belt, you have the

490
00:23:29.839 --> 00:23:33.440
<v Speaker 3>hot station, things are simmering. You have larger asteroids big

491
00:23:33.559 --> 00:23:37.160
<v Speaker 3>enough to have their cores heated by radioactive elements melting

492
00:23:37.160 --> 00:23:40.720
<v Speaker 3>their internal ice into liquid water. That's the Murchison kitchen.

493
00:23:40.720 --> 00:23:42.279
<v Speaker 3>They're making a slow cooked stew.

494
00:23:42.599 --> 00:23:46.039
<v Speaker 2>Okay. And then you go way way out past the

495
00:23:46.039 --> 00:23:48.240
<v Speaker 2>frost line where it's potentially col.

496
00:23:48.240 --> 00:23:51.119
<v Speaker 3>You go out to the benicitchen. It's dark, it's hundreds

497
00:23:51.119 --> 00:23:53.799
<v Speaker 3>of degrees below zero. All you have are chunks of

498
00:23:53.799 --> 00:23:56.559
<v Speaker 3>ice and dust floating in the void, and your only

499
00:23:56.680 --> 00:23:59.720
<v Speaker 3>energy source is this constant rain of high energy cosmic

500
00:23:59.839 --> 00:24:01.440
<v Speaker 3>rays from deep space.

501
00:24:01.880 --> 00:24:04.160
<v Speaker 2>And the most incredible part is that the Benu kitchen

502
00:24:04.200 --> 00:24:06.559
<v Speaker 2>is still cooking up the same stuff. It's just using

503
00:24:06.640 --> 00:24:08.759
<v Speaker 2>a I don't know, a nuclear microwave instead of a

504
00:24:08.759 --> 00:24:09.400
<v Speaker 2>stove top, and.

505
00:24:09.440 --> 00:24:11.640
<v Speaker 3>Nuclear microwave is a pretty good way to think about it.

506
00:24:11.720 --> 00:24:14.279
<v Speaker 3>But the final dish comes out the same. They both

507
00:24:14.319 --> 00:24:16.599
<v Speaker 3>serve up glycine and other amino acids.

508
00:24:16.680 --> 00:24:18.160
<v Speaker 2>That is the part that I just can't wrap my

509
00:24:18.200 --> 00:24:21.359
<v Speaker 2>head around. You have two completely different environments, two fundamentally

510
00:24:21.359 --> 00:24:26.000
<v Speaker 2>different energy sources heat versus radiation, and they both converge

511
00:24:26.200 --> 00:24:31.000
<v Speaker 2>on producing the exact same fundamental biological building blocks.

512
00:24:31.160 --> 00:24:35.400
<v Speaker 3>It suggests it wasn't a fluke, it was convergent chemistry.

513
00:24:35.960 --> 00:24:40.039
<v Speaker 3>It seems that given the basic starting ingredients of carbon, nitrogen, oxygen,

514
00:24:40.039 --> 00:24:44.000
<v Speaker 3>and hydrogen. The universe is almost determined to create complexity.

515
00:24:44.319 --> 00:24:47.000
<v Speaker 3>It will find a way hot and wet or cold

516
00:24:47.000 --> 00:24:49.160
<v Speaker 3>and radioactive. It gets the job done.

517
00:24:49.319 --> 00:24:51.839
<v Speaker 2>It really hammers home that idea that the early solar

518
00:24:51.880 --> 00:24:54.440
<v Speaker 2>system wasn't just making the ingredients for life in one

519
00:24:54.480 --> 00:24:57.519
<v Speaker 2>special place. It was trying to make them everywhere, in

520
00:24:57.640 --> 00:24:58.799
<v Speaker 2>every way it could.

521
00:24:58.920 --> 00:25:03.160
<v Speaker 3>It was now speaking of complexity. There was another part

522
00:25:03.160 --> 00:25:06.119
<v Speaker 3>of the study that I found completely and utterly baffling.

523
00:25:07.000 --> 00:25:09.680
<v Speaker 3>And reading the paper, you get the sense the researchers

524
00:25:09.680 --> 00:25:10.839
<v Speaker 3>were just as baffled.

525
00:25:10.960 --> 00:25:12.559
<v Speaker 2>Oh, this must be the mystery of the mirror.

526
00:25:12.599 --> 00:25:14.920
<v Speaker 3>The mystery of the mirror. It sounds like a title

527
00:25:14.960 --> 00:25:16.200
<v Speaker 3>for an old detective novel.

528
00:25:16.319 --> 00:25:18.400
<v Speaker 2>It really does. So what is this all about.

529
00:25:18.640 --> 00:25:22.759
<v Speaker 3>It has to do with a property of molecules called chirality.

530
00:25:23.200 --> 00:25:28.319
<v Speaker 3>Chirality which is also known more simply as handedness.

531
00:25:27.960 --> 00:25:30.160
<v Speaker 2>Like being left handed or right handed.

532
00:25:30.279 --> 00:25:32.319
<v Speaker 3>Exactly like that, hold up your hands in front of you.

533
00:25:32.359 --> 00:25:32.960
<v Speaker 2>Okay, they're up.

534
00:25:33.279 --> 00:25:36.079
<v Speaker 3>Your left hand and your right hand are perfect mirror

535
00:25:36.160 --> 00:25:39.720
<v Speaker 3>images of each other. Right they have the same components

536
00:25:39.799 --> 00:25:43.759
<v Speaker 3>four fingers, one thumb, a palm, but they are not identical.

537
00:25:43.839 --> 00:25:46.079
<v Speaker 3>You can't lay your left hand perfectly on top of

538
00:25:46.119 --> 00:25:47.079
<v Speaker 3>your right right, and a.

539
00:25:47.119 --> 00:25:49.880
<v Speaker 2>Left handed glove doesn't fit on my right hand. They're

540
00:25:49.920 --> 00:25:52.839
<v Speaker 2>non supermposable mirror images exactly.

541
00:25:53.400 --> 00:25:56.680
<v Speaker 3>Many molecules, including amino acids, are the same way. They

542
00:25:56.720 --> 00:25:59.440
<v Speaker 3>come in two forms, a left handed version and a

543
00:25:59.640 --> 00:26:00.599
<v Speaker 3>right hand hand version.

544
00:26:00.680 --> 00:26:04.079
<v Speaker 2>Okay, and normally these two versions are chemically identical.

545
00:26:04.119 --> 00:26:06.839
<v Speaker 3>Aren't they in a test tube? Yes, they have the

546
00:26:06.880 --> 00:26:10.039
<v Speaker 3>same mass, the same boiling point, the same freezing point.

547
00:26:10.759 --> 00:26:13.160
<v Speaker 3>And this is the critical part. If you make them

548
00:26:13.200 --> 00:26:16.400
<v Speaker 3>through a non biological chemical process, like what's happening on

549
00:26:16.440 --> 00:26:19.759
<v Speaker 3>an asteroid, you should always get a perfect fifty to

550
00:26:19.799 --> 00:26:24.200
<v Speaker 3>fifty mix of left and right, and isotopically, those left

551
00:26:24.200 --> 00:26:27.759
<v Speaker 3>and right handed versions should be identical.

552
00:26:27.480 --> 00:26:29.359
<v Speaker 2>Because they were made in the same pot at the

553
00:26:29.359 --> 00:26:29.880
<v Speaker 2>same time.

554
00:26:30.160 --> 00:26:32.720
<v Speaker 3>Right, if you bake a batch of cookies, the left

555
00:26:32.720 --> 00:26:34.400
<v Speaker 3>half of a cookie and the right half of that

556
00:26:34.440 --> 00:26:37.440
<v Speaker 3>same cookie should be made of the exact same dough.

557
00:26:37.640 --> 00:26:38.880
<v Speaker 2>That makes perfect sense, but.

558
00:26:38.880 --> 00:26:40.680
<v Speaker 3>Benu, of course, did not follow the rules.

559
00:26:40.720 --> 00:26:42.640
<v Speaker 2>Benu seems to enjoy breaking rules.

560
00:26:42.799 --> 00:26:46.200
<v Speaker 3>It does. The research team looked at a different amino acid,

561
00:26:46.240 --> 00:26:49.119
<v Speaker 3>this time one called glutemic acid. It's a bit more

562
00:26:49.119 --> 00:26:53.119
<v Speaker 3>complex than glycine. And they measured the nitrogen isotopes, the

563
00:26:53.160 --> 00:26:55.799
<v Speaker 3>weight of the nitrogen atoms in the left handed version

564
00:26:55.880 --> 00:26:57.960
<v Speaker 3>versus the right handed version, and what do they find.

565
00:26:58.119 --> 00:27:01.240
<v Speaker 3>They found a huge difference. They had, and I'm quoting

566
00:27:01.240 --> 00:27:04.440
<v Speaker 3>the paper, drastically different nitrogen values.

567
00:27:04.720 --> 00:27:08.599
<v Speaker 2>Wait, what how is that even possible? If they are

568
00:27:08.640 --> 00:27:11.559
<v Speaker 2>mirror images formed in the same rock from the same

569
00:27:11.599 --> 00:27:14.440
<v Speaker 2>pool of ingredients. How can one be made of different

570
00:27:14.440 --> 00:27:15.240
<v Speaker 2>stuff than the other?

571
00:27:15.480 --> 00:27:17.720
<v Speaker 3>That is the million dollar question. I mean, it's the

572
00:27:17.759 --> 00:27:21.240
<v Speaker 3>ten million dollar question. There is no simple, obvious reason

573
00:27:21.680 --> 00:27:24.720
<v Speaker 3>why the left hand should be isotopically heavier than the

574
00:27:24.799 --> 00:27:26.000
<v Speaker 3>right hand. It shouldn't be.

575
00:27:26.400 --> 00:27:29.200
<v Speaker 2>So what's the explanation? Is there a working theory?

576
00:27:30.079 --> 00:27:31.559
<v Speaker 3>Honestly, we don't know.

577
00:27:31.720 --> 00:27:33.400
<v Speaker 2>Wow, the expert is stumped.

578
00:27:33.559 --> 00:27:35.799
<v Speaker 3>I am, and so are the people who wrote the paper.

579
00:27:35.839 --> 00:27:39.319
<v Speaker 3>Basinsky was refreshingly honest about it. In the university's press release.

580
00:27:39.359 --> 00:27:41.599
<v Speaker 3>She basically said, we have more questions now than answers.

581
00:27:41.680 --> 00:27:43.960
<v Speaker 2>I have to say, I respect that it's rare for

582
00:27:44.000 --> 00:27:46.200
<v Speaker 2>a major scientific paper to just throw its hands up

583
00:27:46.200 --> 00:27:48.119
<v Speaker 2>and say this part is really weird, and we have

584
00:27:48.119 --> 00:27:48.839
<v Speaker 2>no idea.

585
00:27:48.599 --> 00:27:51.240
<v Speaker 3>Why it is, and it's what makes science so exciting.

586
00:27:51.279 --> 00:27:53.799
<v Speaker 3>It means we've just stumbled upon a new piece of

587
00:27:53.839 --> 00:27:56.440
<v Speaker 3>the puzzle we didn't even know existed, some process we

588
00:27:56.480 --> 00:27:59.319
<v Speaker 3>don't understand yet. Why would the mirror image have a

589
00:27:59.319 --> 00:28:02.839
<v Speaker 3>different chemical heritage? Did they form in slightly different places

590
00:28:02.880 --> 00:28:05.640
<v Speaker 3>on the asteroid and then get mixed together. Did some

591
00:28:05.720 --> 00:28:10.160
<v Speaker 3>weird radiation process preferentially destroy one type of nitrogen isotope

592
00:28:10.160 --> 00:28:12.599
<v Speaker 3>and one handedness but not the other. We just don't know.

593
00:28:12.759 --> 00:28:14.599
<v Speaker 2>It's a genuine scientific cliffhanger.

594
00:28:14.759 --> 00:28:17.319
<v Speaker 3>It's the absolute frontier. We thought we had a pretty

595
00:28:17.319 --> 00:28:20.480
<v Speaker 3>good handle on chirality, but Ben was just sitting there saying, nope,

596
00:28:20.680 --> 00:28:22.720
<v Speaker 3>look closer, you've missed something big.

597
00:28:22.920 --> 00:28:26.359
<v Speaker 2>So let's just tally the score here. From one single

598
00:28:26.480 --> 00:28:30.160
<v Speaker 2>teaspoon of space dust, we have a brand new recipe

599
00:28:30.200 --> 00:28:34.400
<v Speaker 2>for making life's ingredients using ice and radiation. We have

600
00:28:34.599 --> 00:28:38.960
<v Speaker 2>proof the early Solar system had multiple distinct kitchens all

601
00:28:39.000 --> 00:28:41.839
<v Speaker 2>cooking up the same meal, and we have a baffling

602
00:28:41.880 --> 00:28:45.720
<v Speaker 2>new mystery about mirror image molecules that don't match.

603
00:28:45.880 --> 00:28:48.599
<v Speaker 3>That is a pretty good haul for one robotic space heist,

604
00:28:49.000 --> 00:28:49.599
<v Speaker 3>It really is.

605
00:28:50.160 --> 00:28:51.839
<v Speaker 2>But I want to zoom out now. As we always do.

606
00:28:53.839 --> 00:28:56.359
<v Speaker 2>Why is this matter? Why should the person listening to

607
00:28:56.400 --> 00:28:59.519
<v Speaker 2>this right now maybe second traffic or walking their dog.

608
00:29:00.039 --> 00:29:03.400
<v Speaker 2>Why should they care about the isotopic ratios in dust

609
00:29:03.599 --> 00:29:05.599
<v Speaker 2>from an asteroid millions of miles away.

610
00:29:05.720 --> 00:29:08.599
<v Speaker 3>It matters because this is our origin story. It's everyone's

611
00:29:08.640 --> 00:29:09.440
<v Speaker 3>origin story.

612
00:29:09.599 --> 00:29:09.839
<v Speaker 2>Go on.

613
00:29:10.200 --> 00:29:13.519
<v Speaker 3>There's a field of science called prebiotic chemistry. That's all

614
00:29:13.599 --> 00:29:16.039
<v Speaker 3>the chemistry that had to happen before biology could take over,

615
00:29:16.200 --> 00:29:19.359
<v Speaker 3>before the first cell. Glycine and the other amino acids

616
00:29:19.440 --> 00:29:23.079
<v Speaker 3>are key signposts of that chemistry. Okay, what this study

617
00:29:23.119 --> 00:29:25.720
<v Speaker 3>and others like it are confirming is that the building

618
00:29:25.720 --> 00:29:28.400
<v Speaker 3>blocks of life were not unique to Earth. Our planet

619
00:29:28.440 --> 00:29:30.920
<v Speaker 3>did not have to invent amino acids from scratch in

620
00:29:31.000 --> 00:29:31.759
<v Speaker 3>its own oceans.

621
00:29:31.839 --> 00:29:34.240
<v Speaker 2>We didn't have to diy the entire project from the

622
00:29:34.240 --> 00:29:34.680
<v Speaker 2>ground up.

623
00:29:34.839 --> 00:29:38.599
<v Speaker 3>No, the Solar System was a massive factory making these

624
00:29:38.599 --> 00:29:42.200
<v Speaker 3>components in huge quantities on asteroids, on comets, and the

625
00:29:42.240 --> 00:29:45.640
<v Speaker 3>cold and the heat, and then what happened in the

626
00:29:45.680 --> 00:29:46.880
<v Speaker 3>early days of the Solar.

627
00:29:46.640 --> 00:29:49.519
<v Speaker 2>System, the late heavy bombardment, everything was hitting everything.

628
00:29:49.160 --> 00:29:53.680
<v Speaker 3>Else exactly the delivery system. Think about the Earli Earth

629
00:29:53.799 --> 00:29:57.079
<v Speaker 3>four billion years ago. It was a violent chaotic place.

630
00:29:57.119 --> 00:30:00.680
<v Speaker 3>We were getting pelted constantly by rocks and ice from space.

631
00:30:01.640 --> 00:30:05.039
<v Speaker 3>We've long suspected that these impacts delivered water and organic

632
00:30:05.119 --> 00:30:08.039
<v Speaker 3>material to our barren planet, but now we have a

633
00:30:08.119 --> 00:30:10.839
<v Speaker 3>much richer picture. We know they were delivering a whole

634
00:30:11.000 --> 00:30:14.440
<v Speaker 3>diverse menu of ingredients cooked up in all these different ways.

635
00:30:14.559 --> 00:30:17.799
<v Speaker 2>It's like a cosmic meal kit delivery service for young planets.

636
00:30:17.920 --> 00:30:20.160
<v Speaker 3>That's it Astrofresh for the Haitian eon.

637
00:30:20.559 --> 00:30:23.039
<v Speaker 2>So Earth is getting showered with these rocks, and they're

638
00:30:23.160 --> 00:30:25.839
<v Speaker 2>chock full of glycine and other amino acids made in

639
00:30:25.839 --> 00:30:27.400
<v Speaker 2>both warm and cold environments.

640
00:30:27.720 --> 00:30:29.640
<v Speaker 3>And because we now know these things can be made

641
00:30:29.640 --> 00:30:32.880
<v Speaker 3>in ice and radiation, which are arguably the most common

642
00:30:32.880 --> 00:30:37.960
<v Speaker 3>conditions in the entire universe, this has truly universal implications.

643
00:30:37.279 --> 00:30:41.279
<v Speaker 2>Right because warm little ponds those might actually be rare.

644
00:30:41.640 --> 00:30:43.480
<v Speaker 2>You need a planet of the right size, at the

645
00:30:43.559 --> 00:30:47.039
<v Speaker 2>right distance from its star, with an atmosphere with liquid water.

646
00:30:47.200 --> 00:30:49.039
<v Speaker 2>That's a long and specific shopping list.

647
00:30:49.240 --> 00:30:51.599
<v Speaker 3>It is. A planet with a warm pond is a

648
00:30:51.680 --> 00:30:56.079
<v Speaker 3>luxury item in the cosmos. But cold irradiated ice, that

649
00:30:56.160 --> 00:30:59.640
<v Speaker 3>stuff is everywhere everywhere. It's the primary component of every

650
00:30:59.680 --> 00:31:03.000
<v Speaker 3>common It's in the countless asteroids out in the Kuiper Belt,

651
00:31:03.200 --> 00:31:06.400
<v Speaker 3>it's in the orc clouds surrounding our entire Solar system.

652
00:31:06.759 --> 00:31:09.720
<v Speaker 3>It makes up the moons of Jupiter like Europa, and

653
00:31:09.759 --> 00:31:13.000
<v Speaker 3>the moons of Saturn like Enceladus. They are all giant

654
00:31:13.039 --> 00:31:16.880
<v Speaker 3>balls of ice getting blasted by radiation from their host planets.

655
00:31:17.200 --> 00:31:20.000
<v Speaker 2>So if the recipe for making amino acids works in

656
00:31:20.039 --> 00:31:21.440
<v Speaker 2>those conditions.

657
00:31:21.000 --> 00:31:24.079
<v Speaker 3>Then the building blocks of life are in all likelihood,

658
00:31:24.200 --> 00:31:27.839
<v Speaker 3>absolutely everywhere, not just here, not just in our Solar system,

659
00:31:27.960 --> 00:31:31.720
<v Speaker 3>but in every Solar system, in the interstellar clouds between

660
00:31:31.759 --> 00:31:33.559
<v Speaker 3>the stars, everywhere.

661
00:31:33.920 --> 00:31:37.079
<v Speaker 2>That has a staggering thought. It reframes the question from

662
00:31:37.240 --> 00:31:41.359
<v Speaker 2>how did life start here? To with the ingredients being universal,

663
00:31:41.359 --> 00:31:44.960
<v Speaker 2>why wouldn't it start everywhere? It suggests life's potential is

664
00:31:45.000 --> 00:31:47.599
<v Speaker 2>baked into the very physics and chemistry of the cosmos.

665
00:31:48.000 --> 00:31:50.599
<v Speaker 3>Alison Bazinski summed it up perfectly. She said, their next

666
00:31:50.640 --> 00:31:53.440
<v Speaker 3>step is to analyze more asteroid samples, and we want

667
00:31:53.440 --> 00:31:55.799
<v Speaker 3>to know if they continue to look like Murchison and Venu,

668
00:31:56.119 --> 00:31:58.279
<v Speaker 3>or maybe there is even more diversity in the conditions

669
00:31:58.279 --> 00:32:00.640
<v Speaker 3>and pathways that can create the building blow of life.

670
00:32:00.640 --> 00:32:01.960
<v Speaker 2>She wants to find more kitchens.

671
00:32:02.119 --> 00:32:04.680
<v Speaker 3>She wants to find more recipes because every time we

672
00:32:04.720 --> 00:32:06.759
<v Speaker 3>open a new rock, it seems to tell us that life,

673
00:32:07.160 --> 00:32:10.720
<v Speaker 3>or at least it's precursors, is more resilient, more adaptable,

674
00:32:10.799 --> 00:32:14.200
<v Speaker 3>and maybe more inevitable than we ever dared to imagine.

675
00:32:14.279 --> 00:32:16.359
<v Speaker 2>More inevitable. I like the sound of that. It feels

676
00:32:16.400 --> 00:32:17.359
<v Speaker 2>deeply optimistic.

677
00:32:17.440 --> 00:32:20.400
<v Speaker 3>It's not just blind luck, it's chemistry, and the laws

678
00:32:20.400 --> 00:32:23.039
<v Speaker 3>of chemistry are the same everywhere in the universe.

679
00:32:23.279 --> 00:32:26.400
<v Speaker 2>So to bring it all home, we started this journey

680
00:32:26.400 --> 00:32:30.359
<v Speaker 2>by picturing a robotic heist to grab a teaspoon of dust,

681
00:32:30.880 --> 00:32:34.000
<v Speaker 2>a rock that hasn't changed in four point six billion years,

682
00:32:34.559 --> 00:32:37.640
<v Speaker 2>and we end up realizing that this dust is a

683
00:32:37.680 --> 00:32:38.799
<v Speaker 2>recipe book.

684
00:32:38.559 --> 00:32:42.319
<v Speaker 3>A recipe book with multiple very different chapters, and we

685
00:32:42.440 --> 00:32:44.519
<v Speaker 3>just learned to read the chapter on I don't know

686
00:32:44.640 --> 00:32:45.640
<v Speaker 3>cold brew chemistry.

687
00:32:45.720 --> 00:32:47.640
<v Speaker 2>We learned you don't need a warm pond to start

688
00:32:47.640 --> 00:32:49.799
<v Speaker 2>making life legos. You can do it in a cosmic

689
00:32:49.839 --> 00:32:51.440
<v Speaker 2>freezer with a side of gamma rays.

690
00:32:51.599 --> 00:32:54.200
<v Speaker 3>And we learned our solar system wasn't a uniform place.

691
00:32:54.559 --> 00:32:58.319
<v Speaker 3>It was a complex, varied chemical landscape, with different regions

692
00:32:58.319 --> 00:33:02.519
<v Speaker 3>cooking up the same vital ingredy using totally different methods, and.

693
00:33:02.519 --> 00:33:05.319
<v Speaker 2>On top of all that we learned, we still have

694
00:33:05.359 --> 00:33:08.680
<v Speaker 2>a profound mystery on our hands about why mirror image

695
00:33:08.720 --> 00:33:11.440
<v Speaker 2>molecules don't always seem to be made of the same stuff.

696
00:33:11.640 --> 00:33:14.440
<v Speaker 3>It's job security for the next generation of scientists. If

697
00:33:14.440 --> 00:33:16.079
<v Speaker 3>we knew all the answers, it would be a very

698
00:33:16.119 --> 00:33:17.000
<v Speaker 3>boring universe.

699
00:33:17.160 --> 00:33:20.240
<v Speaker 2>That's true, But I think the big takeaway for me,

700
00:33:20.319 --> 00:33:23.799
<v Speaker 2>the thing that really sticks is this shift in perspective.

701
00:33:24.359 --> 00:33:27.839
<v Speaker 2>Science is all about expanding the boundaries of what's possible, right,

702
00:33:28.200 --> 00:33:31.039
<v Speaker 2>and we used to have a very narrow earth centric

703
00:33:31.119 --> 00:33:34.960
<v Speaker 2>view of what was possible. Life needs liquid water, life

704
00:33:35.000 --> 00:33:38.640
<v Speaker 2>needs moderate temperatures. Now we know the universe has, as

705
00:33:38.680 --> 00:33:42.000
<v Speaker 2>the research put it, many conditions to create that starter

706
00:33:42.079 --> 00:33:42.880
<v Speaker 2>pack for life.

707
00:33:42.920 --> 00:33:45.400
<v Speaker 3>It doesn't just open the door to new possibilities, it

708
00:33:45.480 --> 00:33:47.039
<v Speaker 3>kicks the door off its hinges.

709
00:33:47.359 --> 00:33:48.920
<v Speaker 2>So here's a final thought. I want to leave you

710
00:33:48.960 --> 00:33:51.000
<v Speaker 2>with something to chew on as you go about your day.

711
00:33:51.400 --> 00:33:56.079
<v Speaker 2>We tend to think of deep space as empty, cold, dead, hostile,

712
00:33:56.720 --> 00:33:59.839
<v Speaker 2>a black void where life struggles. But if this research

713
00:33:59.880 --> 00:34:04.039
<v Speaker 2>is right, if that cold, dark, radioactive void is actually

714
00:34:04.119 --> 00:34:07.279
<v Speaker 2>a NonStop factory for the very building blocks of life.

715
00:34:07.359 --> 00:34:09.920
<v Speaker 3>Then the darkness isn't dead at all, It's pregnant with

716
00:34:10.000 --> 00:34:11.480
<v Speaker 3>potential exactly.

717
00:34:12.199 --> 00:34:16.199
<v Speaker 2>So does that mean life isn't some lucky, miraculous accident

718
00:34:16.199 --> 00:34:19.039
<v Speaker 2>that happened on one special blue marble. Does it mean

719
00:34:19.079 --> 00:34:22.880
<v Speaker 2>that life is actually a cosmic inevitability, That the universe

720
00:34:22.960 --> 00:34:26.159
<v Speaker 2>is just saturated with these seeds, waiting for them to

721
00:34:26.239 --> 00:34:27.960
<v Speaker 2>land in any halfway decent soil.

722
00:34:28.039 --> 00:34:30.920
<v Speaker 3>If the seeds are everywhere, then the garden is just

723
00:34:31.000 --> 00:34:31.639
<v Speaker 3>waiting to grow.

724
00:34:31.840 --> 00:34:33.800
<v Speaker 2>Something to think about, the next time you look up

725
00:34:33.800 --> 00:34:36.119
<v Speaker 2>at the night sky. It's not just empty space up there.

726
00:34:36.199 --> 00:34:36.840
<v Speaker 2>It's a kitchen.

727
00:34:37.199 --> 00:34:38.119
<v Speaker 3>It's potential.

728
00:34:38.239 --> 00:34:39.599
<v Speaker 2>Thanks for diving deep with us today.

729
00:34:39.639 --> 00:34:40.480
<v Speaker 3>It's always a pleasure.

730
00:34:40.559 --> 00:35:20.199
<v Speaker 2>We'll see on the next one. Keep looking up stations,

731
00:35:20.320 --> 00:35:57.880
<v Speaker 2>says Sets.
