Mars’ Hidden Chemistry: DNA-Like Compounds Discovered - podcast episode cover

Mars’ Hidden Chemistry: DNA-Like Compounds Discovered

Apr 22, 202636 minSeason 3Ep. 382
--:--
--:--
Download Metacast podcast app
Listen to this episode in Metacast mobile app
Don't just listen to podcasts. Learn from them with transcripts, summaries, and chapters for every episode. Skim, search, and bookmark insights. Learn more

Episode description

NASA’s Curiosity rover has carried out a specialized chemical experiment on Mars, uncovering a diverse set of organic molecules trapped in ancient clay-rich rocks. Among them are nitrogen-bearing compounds linked to DNA precursors and sulfur-rich chemicals commonly found in meteorites.

While these molecules represent key building blocks of life, their origin remains uncertain—potentially biological or purely geological. The findings confirm that the Martian surface can preserve complex carbon chemistry over billions of years, strengthening the case for ancient habitability.

This breakthrough lays the groundwork for upcoming missions focused on returning Martian samples to Earth, where scientists can finally test for definitive signs of past life.

Thank you for listening to Bedtime Astronomy — your guide to the cosmos. New episodes on space exploration, NASA missions & the latest astronomy breakthroughs.

This episode includes AI-generated content.

Transcript

Speaker 1

Welcome to Bedtime Astronomy. Explore the wonders of the cosmos with our soothing Bedtime Astronomie podcast. Each episode offers a gentle journey through the stars, planets, and beyond, perfect for unwinding after a long day. Let's travel through the mysteries of the universe as you drift off into a peaceful slumber under the night sky.

Speaker 2

I want you to imagine, just for a second, that you are standing in a dry, freezing, just incredibly dusty crater on another planet.

Speaker 3

Yeah, an absolutely brutal environment.

Speaker 2

Exactly. The sky above you isn't blue. It's this hazy butterscotch color tinted by all that iron oxide dust just suspended in the thin air, right, And the atmosphere is so wispy, I mean, it's mostly carbon dioxide, less than one percent the density of Earth's You couldn't breathe it even if it magically filled with oxygen right then and there.

Speaker 3

No, you'd suffocate immediately and freeze.

Speaker 2

Yeah, freeze. Because the temperature is hovering somewhere around eighty degrees below zero. There is no sound but this thin wind. It is utterly barren, like a sterile desert, right, but then you kneel down, you brush away that rusty red top layer of dirt you screep just I don't know, a couple of inches into the rock beneath and staring back at you are the very chemical building blocks of DNA.

Speaker 3

I mean, it sounds like the opening scene of a science fiction novel right where the protagonist makes this impossible discovery.

Speaker 2

It really does.

Speaker 3

But we are looking at hard, peer reviewed reality today, and it's a reality that completely shatters our previous assumptions about the chemistry of our solar.

Speaker 2

System because the surf on is basically a death zone exactly.

Speaker 3

We already know the Martian surface is essentially a sterilization engine unshielded UV radiation, and these highly reactive chemicals in the soil called perchlorates, well, they usually tear organic bonds apart in a matter of months, let alone millennia, which.

Speaker 2

Makes this monumental. And that's our mission today to really explore this. We are talking about NASA's Curiosity Mars rover, right, this car sized nuclear powered laboratory that has managed to pull off something planetary scientists have dreamed of for decades.

Speaker 3

It's an incredible engineering feature.

Speaker 2

In a specific spot on the Martian surface. This rover has successfully uncovered a diverse mix of never before seen organic molecules and yes, that includes the literal precursors to DNA.

Speaker 3

Yeah.

Speaker 2

I mean, it is impossible to overstate how thrilling this is. We are looking at the potential seeds of life sitting right there in the dirt of our neighboring planet.

Speaker 3

It really is.

Speaker 2

It's the kind of discovery that forces you to look up at the night sky and just realize how incredibly dynamic our universe actually is.

Speaker 3

The thrill is absolutely justified. I agree, though, you know, I think we have to tamper that excitement just a bit by grounding ourselves in the sheer, staggering time scale of what we are analyzing.

Speaker 2

Here, right, the three point five billion years part.

Speaker 3

Exactly. The true marvel here isn't just the inventory of what the rover found, is the fact that these complex molecular structures survived at.

Speaker 2

All because Mars doesn't have a magnetic field like we do.

Speaker 3

Right. Mars is a giant, unshielded radiation chamber. It lacks a global magnetic field to deflect galactic cosmic rays and solar energetic particles. Just relentlessly bombard the surface. Wow, Ionizing radiation functions like a like a microscopic wrecking ball, systematically smashing into complex molecules and breaking their delicate carbon bonds over deep time.

Speaker 2

Just constantly chipping away at them.

Speaker 3

Yeah, exactly so. Finding intact macromolecules that endure this bootle environment for billions of years completely redefines our baseline understanding of planetary preservation models.

Speaker 2

Well, let me stop you there, because that immediately raises a massive question. Sure, if the surface is a sterilization engine and cosmic rays are acting like microscopic wrecking balls for three and a half billion years, how on Earth, or rather how on Mars did anything survive?

Speaker 3

Right? It seems impossible.

Speaker 2

It defies logic, which means we have to look at the exact spot where the rover parked. Right. Curiosity didn't just, you know, stumble upon these fragile molecules randomly while rolling across the dunes.

Speaker 3

No, not at all. Survival in that kind of environment is never random. If Curiosity had parked a few miles away, we wouldn't be having this conversation right now.

Speaker 2

Wait, really, just a few miles.

Speaker 3

Just a few miles the rover had to find a very specific geologic vault. Curiosity landed in Gale Crater back in August of twenty twelve. And Gale Crater is this massive impact basin formed billions of years ago.

Speaker 2

And it used to be a lake, right.

Speaker 3

Yes, we are fairly certain it hosted an ancient, long lived lake system. But the specific samples we were dissecting today weren't taken in twenty twelve.

Speaker 2

Well they weren't.

Speaker 3

No, they weren't taken in twenty fourteen or twenty sixteen either. The rover had to meticulously climb the foothills of the crater's central peak, Mount Sharp. It took it till twenty nineteen, when it finally drove into a highly specialized region called Glenn Torden.

Speaker 2

Okay, let's unpack this. Glenn Torden isn't just another patch of rusty terrain, is it not?

Speaker 3

At all? The rover specifically targeted a clay bearing unit within this region, which the science team nicknamed Mary anning Ah.

Speaker 2

After the nineteenth century English palaeontologists who discovered Jurassic marine fossil beds.

Speaker 3

Exactly, and calling it a clay bearing unit is the absolute crux of this entire story, because.

Speaker 2

Clay is special. I like to think of this specific Martian clay as like cosmic tupperware.

Speaker 3

Cosmic tupperware. I like that.

Speaker 2

Yeah, it's a geologic container ceiling in the chemical freshness of Mars from three and a half billion years ago, just completely locking out the destructive, irradiated environment of the surface.

Speaker 3

That analogy holds up surprisingly well under microscopic scrutiny. Actually, yeah, when we talk about clay implanetary science, we aren't just talking about you know, wet mud. We are talking about phylicilicates, smecktight clays, specifically.

Speaker 2

Smack tighte clays. Okay, what makes them so good at being tupperware?

Speaker 3

Well, on a molecular level, these clays are structured in incredibly tight microscopic layers, almost like the pages of a tightly bound book.

Speaker 2

Oh. Interesting.

Speaker 3

When liquid water flows through volcanic rock over long periods of time, it chemically alters the primary minerals like olivine and pyroxene into these layered silicates.

Speaker 2

Okay, So the water changes the.

Speaker 3

Rock, right, and when that alteration happens, organic chemicals flowing in that water can essentially get trapped right between these microscopic sheets.

Speaker 2

So the clay physically swallows the organics like it just traps them inside the pages of the book.

Speaker 3

It traps them, yes, but it also chemically binds them. The surfaces of these clay layers have slight electrical charges that hold onto organic molecules.

Speaker 2

Oh wow, so it's not just a physical box. It's grabbing onto them exactly.

Speaker 3

The clay minerals act as heavy duty protective vaults. They physically shield the trapped organics from the ionizing radiation raining down from space, and they protect them from the chemical oxide driven by the perchlorids on the surface.

Speaker 2

That makes total sense.

Speaker 3

If you want to find preserved organics on a dead world, you follow the clay. This actually circles directly back to Curiosity's original mission.

Speaker 2

Mandate, right, because people forget that goal wasn't to find little green men.

Speaker 3

No, when the rover launched in twenty eleven, its primary goal wasn't to find living microbes. The goal was to find evidence that ancient Mars had the specific environmental conditions that could have supported microbial life billions of years.

Speaker 2

Ago, right, the habitability factor. But I'm looking at this finding and my immediate thought is, Okay, we know Gale Crater was a massive lake. Yes, we know glenn Torden is full of clay formed by water interacting with rock. So water was clearly present for a massive stretch of time denied. But does water automatically equal a habitable environment?

Because you know we have places on Earth like certain ultra acidic volcanic lakes or highly irradiated zones that have water but are completely devoid of life.

Speaker 3

You're hitting on the critical distinction that drives astrobiology. Water is the solvent necessary for life as we know it, but it is entirely insufficient on its own right.

Speaker 2

Just having a glass of water doesn't mean something can live in it exactly.

Speaker 3

To declare an environment truly habitable, you need a confluence of three major pillars.

Speaker 2

Okay, what are the three?

Speaker 3

First, you need that liquid water solvent. Second, you need an energy source to drive metabolism like sunlight sunlight for photosynthesis, sure or chemical gradients and geothermal heat for chemosynthesis like we see in deep ocean hydrothermal vents here on Earth.

Speaker 2

Okay, so water and energy, what's a third?

Speaker 3

And third? You need the elemental building blocks of life which, as scientists often abbreviate as hnopshnops.

Speaker 2

That's carbon, hydrogen, nitrogen, oxygen, phosphorus and sulfur.

Speaker 3

Right, you got it. The clay in Gale Crater proved the long standing water pillar, but to prove full habitability, Curiosity had to definitively find those complex Organicsware is useless to our search for life if we open it up and find it completely empty.

Speaker 2

Wow. Yeah, which brings us to an absolutely massive engineering nightmare. Oh, it was a nightmare, because finding the ultimate cosmic tupperware is a triumph in itself. We sent a robot tens of millions of miles, landed it via a sky crane, which is still insane to me, and drove it for seven years to find this specific mudstone.

Speaker 3

It's incredible.

Speaker 2

But figuring out how to pop the lid open right to crack into those microscopic clay vaults and read the chemical signatures inside that required one of the most high stakes limited resource experiments in the entire history of space exploration.

Speaker 3

The sheer audacity the engineering required to achieve this is just staggering. To pop that lid, The rover utilized an onboard instrument suite called SAM.

Speaker 2

SAM that stands for Sample Analysis of Mars.

Speaker 3

Right exactly, and this particular highly specialized experiment was led in part by astrobiologist Jennifer Eigenbrode at NASA's Goddard Space Flight Center. Okay, now SAM isn't just a single it's effectively a miniaturized analytical chemistry lab tucked right inside the belly of the rover.

Speaker 2

Like a full lab shrunked down.

Speaker 3

Yeah, it contains a gas chromatograph, a quadrupole mass s pectrometer, and a tunable laser spectrometer.

Speaker 2

That is a lot of fancy equipment in a small box, it is.

Speaker 3

But this specific dig at mary Anning wasn't a standard run of the mill SAM test. To coax these complex organics out of their clay vaults without destroying them in the process, the team had to use a highly specialized chemical region called TMAH.

Speaker 2

Okay TMAH tetra misleamonium hydroxide for the organic chemists listening who love a mouthful of syllables, that's the one.

Speaker 3

And to understand why TMAH is so crucial, you have to understand how SAM normally operates.

Speaker 2

Right, how does it normally check the dirt.

Speaker 3

Usually the rover's robotic arm drills into a rock, collects a powdered sample, and drops it into a tiny quartz cup inside SAM.

Speaker 2

Okay, it makes sense.

Speaker 3

The instrument then heats that dirt up to roughly eight hundred degrees celsius, process called pyrolysis.

Speaker 2

Eight hundred degrees.

Speaker 3

Yeah. As the dirt bakes, gases boil off, and the mass spectrometer basically sniffs those gases to see what they made of.

Speaker 2

Okay, I have to interject here because heating Martian dirt to eight hundred degrees seems like a massive design flaw if you are looking for fragile, three and a half billion year old organic molecules.

Speaker 3

It sounds counterintuitive. I know.

Speaker 2

If I take a complex organic structure, like I don't know a sugar or an amino acid, and I've glassed it with eight hundred degrees of heat, I don't get gas. I get a burnt, carbonized mess. I'm essentially making charcoal.

Speaker 3

Right. It's not a flaw, but it is the fundamental constraint of the technology available when SAM was designed in the early two thousands. Okay, and you are entirely correct about the chemistry. Large complex organic molecules, especially ones that have already been battered by cosmic radiation. They do not easily.

Speaker 2

Volatilize, meaning they don't turn into gas neatly exactly.

Speaker 3

They degrade, they fracture, They turn it into a morphous carbon or char. When Sam bakes them, normally, the mass spectrometer often just sees carbon dioxide, water vapor coming.

Speaker 2

Off, just the smoke.

Speaker 3

Basically yeah, yeah, the ghostly combusted remains of what used to be a complex organic molecule. The instrument knows something organic was there, but the original structure is completely lost to the fire.

Speaker 2

Which is exactly why they needed TMAH. So how does this chemical stop the organics from burning into useless ash?

Speaker 3

Well, TMAH performs a brilliant chemical trick called thermochemolysis.

Speaker 2

Okay, break that down for us.

Speaker 3

Thermo for heat, chemo for chemical, and lysis for breaking. When TMH is missed with the Martian dirt and heated, it doesn't just passively watch the molecules burn. It actively attacks them.

Speaker 2

Oh, it goes on the offensive.

Speaker 3

Yeah. TMAH is a strong base and it chemically fragments larger, stubborn organic macromolecules. Into smaller manageable pieces. But crucial to this process, it performs something called methylation. As it breaks the molecules part the TMAH donates methyl groups. That's one carbon atom attached to three hydrogen atoms and attaches them to the broken highly reactive ends of the organic.

Speaker 2

Fragments, so it caps them off so they don't burn.

Speaker 3

Precisely, it protects them, allowing them to volatilize into gas without turning into charcoal.

Speaker 2

That is genius. But here's the part that stresses me out just thinking about it. Imagine packing for a decade long, multi million mile road trip across a hostile desert. Right, sure, but you're only allowed to bring exactly two fluid ounces of engine coolant for the entire journey.

Speaker 3

That's a good way to put it.

Speaker 2

Because you have a car sized robot roaming an entire planet and it only had two tiny cups of this liquid tma H chemical on board, two cups, two cups for the entire multi year life span of the mission. It's like reaching the final most difficult puzzle of a vastly complex video game and realizing you only have a single lock pick to open the most important safe on Earth. And if you turn it too hard it snaps.

Speaker 3

Yeah, and the physical constraints of spaceflight force these kinds of impossible bottlenecks. When you're launching a payload to Mars, every single gram is negotiated.

Speaker 2

Everything costs fuel.

Speaker 3

Right, and liquids are exceptionally difficult to fly with. They require sealed, pressurized containment systems that have to survive the violent, bone rattling vibrations of launch, plus the cold, oh yeah, the freezing vacuum of interplanetary transit, and then the fiery deceleration of entering the Martian atmosphere. So yes, they only had two cups. And because of that terrifying scarcity, the patients required by the science team was just immense.

Speaker 2

I just can't imagine the tension you land in twenty twelve. You know, you have this incredibly powerful chemical lock pick in the rover's belly.

Speaker 3

You just have to wait.

Speaker 2

Yeah, How do planetary scientists handle the psychological pressure of knowing that one wrong scoop of dirt wastes a decade of waiting and searching a lot of pressure Because if they drill a rock mix in the TMAH and it turns out that specific rock was I don't know, too highly oxidized or lacked the right smectite clays, or had too much perchlorate. That's it.

Speaker 3

That's game over for the lock pick.

Speaker 2

You press enter on the code sending the command to Mars, and then you just sit in a control room on Earth, agonizing for the fourteen minute communication delay, waiting to see if you blew your one and only chance.

Speaker 3

They mitigate that pressure through a deeply exhausting, meticulous process of elimination. They didn't just.

Speaker 2

Guess, they couldn't afford to exactly.

Speaker 3

From twenty twelve to twenty nineteen, as Curiosity traversed from the Breadbury landing site through Yellowknife Bay and up the slopes of Mount Sharp, the team continuously analyzed the mineralogy of everything.

Speaker 2

They passed, using the other tools.

Speaker 3

Right, using the rovers, other instruments like chimin, which is the chemistry of mineralogy X ray diffraction instrument. They were constantly building a geological map, waiting for the absolute perfect, most favorable location.

Speaker 2

So they were passing up decent spots because they weren't perfect.

Speaker 3

Oh, they pass up dozens of interesting sites. They're doing sure the sample wasn't to acidic that the clay was authogenic ophogenic.

Speaker 2

What does that mean?

Speaker 3

It means it formed in place in the lake, rather than just being blown in by the wind from somewhere else. Oh okay, And they got to make sure that the radiation exposure was as low as possible. What's fascinating here is that the legacy of the SAM instrument is really built on this kind of disciplined precision.

Speaker 2

They really knew what they were doing.

Speaker 3

Yeah. Even before this specific TMH experiment, SAM had already revolutionized our understanding of Mars, quantifying the planet's atmospheric loss and detecting the seasonal spikes of background methane.

Speaker 2

But this was the main event. Mixing liquids with pulverized extraterrestrial rock, heating it precisely to trigger methylation without causing combustion, and analyzing the vaders at a molecular level, all happening autonomously inside a robot millions of miles away. It's a symphony of engineering, and the craziest part, it worked, It

actually worked. The team took their shot. In twenty twenty, they finally authorized the use of their precious TMAH on the dirt pulled from the Marianning site in Glenn Torridon. They baked it, the TMAH chemically capped the fragments, and the mass spectrometer readouts that beamed back to Earth exceeded their wildest expectations.

Speaker 3

It was a watershed moment for astrobiology. The data analysis of this specific experiment was led by Amy Williams, a professor of geological sciences at the University of Florida, and her team published the findings in Nature Communications, and they found a lot. They didn't just find a faint whisper of carbon. The TMAH test revealed over twenty distinct complex organic chemical compound.

Speaker 2

Why ded That is a massive chemical hall huge.

Speaker 3

But among those twenty, there are two specific structural findings that genuinely altered the landscape of planetary science.

Speaker 2

Okay, let's hear them.

Speaker 3

First, they identified a nitrogen bearing molecule with a structure fundamentally similar to the nucleobases that formed the precursors of DNA wow. And second, they found a significant presence of benzothiophine, which is a large, double ringed sulfur based chemical.

Speaker 2

Okay, So if you were to look at the mass spectrometer readouts right now. You wouldn't see the letters DNA flashing on a screen.

Speaker 3

No, definitely not.

Speaker 2

You'd see a spike in mass to charge ratios, indicating a very specific heavy nitrogen bearing ring. You have to basically play detective to reconstruct what that ring used to be before three and a half billion years of radiation got to it.

Speaker 3

Right, you're looking at the fragments.

Speaker 2

But the conclusion is that we are looking at a DNA precursor, the literal structural foundation of genetic information as we understand it, just sitting there, frozen in a Martian lake bed exactly. And here's where it gets really interesting. And I have to push back on the scientific communities messaging here.

Speaker 3

Okay, lay it on me.

Speaker 2

We found the building blocks of DNA on Mars. Why isn't this front page above the fold news everywhere declaring we found aliens. It feels like scientists are deliberately downplaying this, framing it merely as chemistry rather than definitively by alogy.

Speaker 3

It is the most natural reaction to have, believe me, and it gets to the very heart of the rigor required by the scientific.

Speaker 2

Method, because it's not proof yet, right.

Speaker 3

The boundary between a biological building block, and actual functioning biological activity is a vast complicated gulf. How so, well, think of finding a nuclear base a DNA precursor like finding a single perfectly formed clay brick. A brick is incredibly useful. It is the fundamental unit you need if you want to build a complex house. But finding a single brick lying in an empty field does not prove that a house was ever actually built there, let alone that someone lived in it.

Speaker 2

Oh, that makes a lot of sense.

Speaker 3

Biology is not just a collection of chemicals. It's a highly organized, selective, energy consuming system. And the universe, it turns out, is remarkably good at forging the basic chemical bricks of life entirely on its own.

Speaker 2

Without life being involved at all, exactly.

Speaker 3

Through completely abiotic, non living physics and chemistry.

Speaker 2

Which ties perfectly into the second major chemical they found, benzothiophine. Yes, it does, because if I hear sulfur based organic ring, I immediately think of the sky, not the ground. Benzothiophine is heavily associated with meteorite delivery. Right, we know the universe is literally raining these complex carbon building blocks down on planets all the time.

Speaker 3

That is the crucial context. Benzothiophine is a fascinating molecule. It consists of a benzene ring fused to a thiophine ring incorporating a sulfur atom.

Speaker 2

And why is the sulfur important?

Speaker 3

Sulfur is incredibly important because it undergoes a process similar to vulcanization and rubber.

Speaker 2

Oh like toughening it up exactly.

Speaker 3

It cross links with organic molecules, making them incredibly tough and resistant to degradation.

Speaker 2

Okay, so they survive the trip through space.

Speaker 3

Right, But more importantly, as you noted, these exact types of molecules are routinely found inside carbonaceous chondrite meteorites. Amy Williams made a profound observation about this dynamic.

Speaker 2

What did she say?

Speaker 3

Well, she noted that the early Solar System around three point eight to four or billion years ago, during the Late Heavy bombardment, was a chaotic, violent place. The exact same meteoric material that rained down on Mars is what rained down on Earth. Really, Yeah, the inner Solar System was bathed in the exact same organic inventory.

Speaker 2

So Earth wasn't special in its ingredients.

Speaker 3

Not at all. Both worlds received the exact same cosmic grocery delivery. On Earth, those complex molecular building blocks were eventually caught up in a cycle of hydrothermal energy and liquid water and were utilized by emerging biological systems.

Speaker 2

And on Mars.

Speaker 3

On Mars, they might have just fallen into the quiet waters of Gale Crater, sunk to the bottom, gotten trapped in the microscopic layers of coming smectite clay, and just sat there in perfect cold preservation for billions of years.

Speaker 2

Wow. Which means my earlier frustration about scientists not declaring we found life is exactly what the entire scientific community is wrestling with right now.

Speaker 3

Yeah, it's the big debate.

Speaker 2

Because of the Samtmah experiment, we finally know, without a shadow of a doubt, what is in the Martian dirt. The tupperware is full, yes it is. But the hardest puzzle in the Solar system is figuring out the causal mechanism of how it got there.

Speaker 3

That is the absolute crux of the origin ambiguity, and it highlights the inherent limitations of even our most advanced robotic experiments.

Speaker 2

Right because the rover can only tell us so much.

Speaker 3

Exactly the tmah wet chemistry test on curiosity is a triumph of remote engineering, but it cannot definitively distinguish the origin story of these chemical compounds.

Speaker 2

So we have options we do.

Speaker 3

When we look at that benzothiophine or that nitrogen bearing DNA precursor, we are faced with three equally plausible hypotheses.

Speaker 2

We go through them.

Speaker 3

First, the biological hypothesis. These organics are the degraded, fragmented remnants of the metabolic processes of actual ancient Martian microbes that lived in Gale crater.

Speaker 2

The alien life option. Okay, what's next.

Speaker 3

Second, the abiotic geological hypothesis. These compounds were formed entirely through non living processes like what kind of processes such as fischer Trops type reactions in hydrothermal vents deep underground where hot water interacts with carbon dioxide and hydrogen to synthesize complex hydrocarbons.

Speaker 2

Okay, so the planet just bake them up itself, right? And the third is the exogenous hypothesis, the meteorite delivery system exactly, you know, I look at this chemical ambiguity like walking into a kitchen and finding a bag of flour. Some sugar and a carton of eggs sitting on the counter.

Speaker 3

Okay, I like this.

Speaker 2

It could mean someone was actively in there baking a cake, whipping up a complex recipe, which represents biological life. Or it could just mean someone dropped off raw groceries and bags and left the house, which represents meteorites delivering the chemicals from space.

Speaker 3

That is a perfect analogy, right.

Speaker 2

The ingredients sitting on the counter are exactly the same in both scenarios, but the story of how they got there completely changes our understanding of the universe completely. So what does this all mean? How do we solve this? If a bill VN dollar car sized chemistry lab on wheels can't tell the difference between raw groceries and a baked cake, what are we supposed to do.

Speaker 3

To solve that? We have to look for signatures that are uniquely undeniably biological. We have to look for things like isotopic fractionation or HOMLK chorality.

Speaker 2

Okay, hold on, let's break those down, because that is where the real detective work happens.

Speaker 3

Sure, let's take isotopic fractionation. Okay, life is fundamentally lazy. It always takes the path of least resistance, don't we all right? Carbon exists in different isotopes, primarily carbon twelve, which is lighter, and carbon thirteen, which has an extra neutron and is heavier.

Speaker 2

Okay, so twelve is lighter, thirteen is heavier.

Speaker 3

Because carbon twelve is lighter, it requires slightly less energy to incorporate into metabolic processes. So biological systems preferentially consume carbon twelve.

Speaker 2

Oh, because it's easier to lift.

Speaker 3

Basically exactly, if you find a depositive organic matter and it has a heavily skewed ratio favoring carbon twelve far beyond the standard geological background levels, yeah, well that is a massive flashing neon sign pointing toward biology.

Speaker 2

So life leaves a chemical preference. And what was the second one? Chirality.

Speaker 3

Chirality is basically handedness. Many complex organic molecules, like amino acids can form in two mirror image.

Speaker 2

Structures like literal hands.

Speaker 3

Right, think of your left and right hands. They have the same components, but you can't perfectly superimpose them.

Speaker 2

Okay, so molecules do that too.

Speaker 3

They do when organics form in space on a meteorite. Abiotic chemistry produces a roughly fifty to fifty split of left handed and right handed molecules, an even mix, yeah, what we call a racemic mixture. But life on Earth is incredibly specific. Every biological system on this planet exclusively uses left handed amino acids and right handed sugars. Wait all of them, all of them. It's called homol chorality.

If we find a batch of organics on Mars and they are entirely left handed, that essentially eliminates the media write hypothesis.

Speaker 2

Because metiaorrites would be fifty to fifty exactly. But the SAM instrument, even with the TMAH lock pick, can't reliably measure that kind of microscopic, isotopic and structural detail, especially on organics that have been degraded by billions of years of radiation.

Speaker 3

No, it can't. Curiosity proved the building blocks are there and that the Gale crater environment was highly habitable. It found the tupperware, and it found the ingredients inside, right, But to definitively tell if those ingredients were organized into a living system. To check for homokality and isotopic biosignatures, we absolutely must look at the microscopic structure of the rocks in a pristine laboratory setting on Earth.

Speaker 2

We need our big tools we do.

Speaker 3

We need equipment the size of entire buildings using synchotron particle accelerators and electron microscopes, rather than an instrument the size of a microwave tucked.

Speaker 2

Inside a rover, which explains the entire strategic progression of NASA's Mars exploration program over the last decade.

Speaker 3

If we connect this to the bigger yes, absolutely.

Speaker 2

It's not just a series of random rover drops, It's an escalating chain of scientific relay races. Curiosity was the scout, Yes, the scout. Its job was to find the habitable conditions and prove the organics survived. Once Curiosity found that nitrogen bearing ring and the benzotheophanes in twenty twenty, it gave the green light to the next generation. That is exactly why the Perseverance rover, which landed in Jazzero Crater in twenty twenty one, has a completely different job description.

Speaker 3

Precisely, or rather, that's exactly the evolution of the mission architecture. Perseverance is not just looking for habitability. It is explicitly tasked with seeking definitive signs of ancient microbial.

Speaker 2

Life, right, it's looking for the fossils exactly.

Speaker 3

And instead of just analyzing the dirt onboard and leaving it behind like Curiosity does, Perseverance is actively drilling pristine rock cores to bring them back. Well, it's sealing them in ultra clean titanium tubes and cashing them on the Martian surface, just.

Speaker 2

Leaving them there for pickup exactly. And all of that hinge is entirely on the future Mars sample return architecture, which is arguably the most complex robotic space mission ever conceived.

Speaker 3

Oh, without a doubt.

Speaker 2

I mean, we have to send an Earth return orbiter to Mars, drop a sample retrieval lander to the surface, have a small thatcherrover or helicopters pick up those titanium tubes from Perseverance, load them into a Mars ascent vehicle, which is a rocket launching off the surface of another planet by the.

Speaker 3

Way, for the first time ever.

Speaker 2

Yeah, then rendezvous with the orbiter in space and flight them.

Speaker 3

All the way back to Earth. It is a staggering logistical chain, yeah, and it will take years, likely stretching into the next decade before those physical samples make the multimillion mile trip back to terrestrial laboratories.

Speaker 2

So we still have a long wait.

Speaker 3

We do, but while we wait for that ultimate physical evidence, the success of the TMAH chemical lock pick experiment on Curiosity hasn't just become a footnote in history. It has quite literally rewritten the playbook for how humanity designs the chemical exploration of the rest of the Solar System.

Speaker 2

Because we prove the concept, we know definitively that you can take a highly volatile chemical region like TMAH, shoot it into space, keep it stable for eight years, mix it with alien dirt remotely, and successfully extract heavily degraded billion year old organic macromolecules without destroying them exactly.

Speaker 3

And because that methodology is now prooven, it is being exported. It is no longer just a Martian tool.

Speaker 2

Where else is it going well?

Speaker 3

The European Space Agency is incorporating this exact type of wet chemistry testing into the Roslin Franklin mission to Mars oh Nice and significantly, the Roslin Franklin rover is designed with a drill capable of penetrating two meters deep into the Martian subsurface.

Speaker 2

Two meters Curiosity only scraped a couple of inches down.

Speaker 3

Right, By going two meters deep, Roslin Franklin will be sampling organics that have been completely shielded from the ionizing radiation that destroyed the top layers.

Speaker 2

So we're finally getting below the wrecking balls.

Speaker 3

We are.

Speaker 2

But what truly blows my mind is that this technology is leaving Mars entirely. This exact chemical test is going to be incorporated into the Dragonfly expedition to Saturn's moon Titan.

Speaker 3

This raises an important question, right, because Titan is so different?

Speaker 2

Yeah, wait, we're taking Mars tactics to Saturn's moons now we are. Now, Titan isn't a dusty, irradiated red desert. It's a completely different paradigm. It is an ice world sitting in the deep frieze of the outer Solar System, very deep freeze, enveloped in a thick, smoggy atmosphere where liquid methane and ethane rain from the sky, carving actual

river valleys and forming vast hydrocarbon lakes. How does a chemical test designed to crack open dry Martian smectite clay translate to an ice moon billions of miles further away?

Speaker 3

The environment changes short but the fundamental chemical problem remains identical. Really how so well Titan's surface and atmosphere operate essentially as a planet scale organic chemistry factory. Photochemical reactions in its upper atmosphere constantly break apart methane and nitrogen, creating what creating complex heavy organic molecules called tholins that slowly drift down to the icy surface like a steady snowfall.

Speaker 2

Like an organic snow that is wild it is.

Speaker 3

The Dragonfly mission is a nuclear powered eight rotor drone that will literally fly from location to location across titans dunes and craters, sampling this organic snow.

Speaker 2

A nuclear drone flying through methane skies, it still doesn't feel real.

Speaker 3

It's incredible engineering. But the scientists designing Dragonfly face the exact same problem Jennifer Eigenbrode and Amy Williams faced with Sam on Mars, the burning problem exactly. Titan's surface is incredibly cold, around ninety four kelvin or minus two hundred and ninety degrees fahrenheit. The heavy organics covering the surface

are frozen solid and highly complex. Okay, if the Dragonfly drone lands scoops up that icy, organic rich material, and just blasts it with a heater to vaporize it for a mass spectrum.

Speaker 2

They turned to charcoal.

Speaker 3

Right, those massive, complex tholen molecules will fracture, to grade and burn just like they would have on Mars. You will lose all that structural information. They need a way to gently volatilize the heaviest, most complex molecules on the Moon.

Speaker 2

So they are bringing the lock pick to Saturn.

Speaker 3

They are.

Speaker 2

They will use thermochomolysis, breaking the molecules apart chemically and capping them with methyl groups so they float up as readable gases even in the freezing methane environment of Titan.

Speaker 3

Yes, the two cup gamble on curiosity didn't just solve a local mystery in Gale Crater. It proved that complex wet chemistry can be automated and executed flawlessly in brutal alien conditions.

Speaker 2

It opened the door.

Speaker 3

By testing and validating this concept in the dry, dusty clay of Mars, we gained a standard, highly reliable weapon in humanity's analytical arsenal. Whenever we go hunting for the molecular building blocks of life anywhere in the cosmos, whether it's the subsurface oceans of Europa or the methane lakes of Titan. We now know exactly how to open the vault without burning the treasure inside.

Speaker 2

It really is staggering to pull all these threads together.

Speaker 3

With a lot of information I know.

Speaker 2

We started this conversation standing in the freezing butterscotch tinted dust of Gale Crater. We walked through the deep geological history, exploring how the ancient flowing waters of Mars reacted with volcanic rock to form microscopic layered clay tupperware. We saw how those smectite clay layers physically and chemically locked away the organic secrets of a violently chaotic early solar system, shielding them from three and a half billion years of cosmic.

Speaker 3

Radiation, protected them perfectly.

Speaker 2

We looked at the agonizing eight year weight scientists endured just to use two tiny cups of a chemical lock pick, terrified of wasting their only shot, and we saw how that tension exploded into the discovery of massive, complex molecules from meteorite delivered benzothiophines to the literal nitrogen bearing precursors of DNA.

Speaker 3

Beautiful scientific arc.

Speaker 2

It is we prove that our neighboring barren planet was stocked with the exact same biological grocery list that eventually sparked life here on Earth.

Speaker 3

And I think it's deeply important for you listening to this right now to internalize your own physical connection to this science.

Speaker 2

I couldn't agree more.

Speaker 3

It is very easy to look at planetary exploration as something abstract, an expensive exercise in robotics happening hundreds of millions of miles away. But it is profoundly personal.

Speaker 2

It's about us exactly.

Speaker 3

The carbon atoms currently forming the cell walls in your body, the nitrogen atoms binding together the very rungs of your own DNA. As you listen to this, they share a direct cosmic history with the degraded molecules currently resting in the Glenord and dirt. Wow, the organic rain that blanketed the violent early Solar System fell indiscriminately. It fell on you,

and it fell on Mars. When we use tools like SAM and TMAH to dissect the dirt of another world, we are quite literally studying our own chemical origins and a planet here.

Speaker 2

That is a hauntingly beautiful perspective, And it leaves me

with one final thought for you to ponder. We know the ingredients are universal, We know the exact same organic groceries rained down on both Earth and Mars from meteorites three point eight billion years ago, and we now know definitively, thanks to a car sized rubber and a chemical called TMAH, that mars ancient clay was perfectly capable of catching those ingredients, holding them in a watery, highly habitable environment, and preserving

them for eons. The table was perfectly set, it really was.

Speaker 3

So.

Speaker 2

Perhaps the most profound mystery moving forward isn't whether Mars could have supported life. Perhaps the real mystery, the one that should keep us awake at night, is what tiny microscopic, thermodynamic fork in the road caused Earth to wake up and start baking the cake, while Mars, with all the exact same ingredients, remained perfectly chemically asleep,

Transcript source: Provided by creator in RSS feed: download file
For the best experience, listen in Metacast app for iOS or Android