Latest / Talking Science / Titan – The Moon with Rivers of Methane
Transcript
- 0:00I want you to picture standing under a sky that
- 0:02is the exact color of a manila folder like a
- 0:05perfectly calm air but it's so incredibly thick
- 0:09that if you strapped on a set of wings you could
- 0:12you could literally flap your way up into the
- 0:14sky using just your arm muscles right which is
- 0:17just a wild visual and then underneath your feet
- 0:19instead of dirt or sand there are these rounded
- 0:22pebbles but you know they aren't made of rock
- 0:25they're solid water ice frozen completely as
- 0:29hard as stone in this deep, deep cold. Yeah.
- 0:32And just off in the distance, you can see a river
- 0:34flowing, but it's not water. It's actually liquid
- 0:36methane. Exactly. I mean, it's the exact same
- 0:38simple molecule that makes up the natural gas
- 0:40we use to cook with here on Earth. But here it's
- 0:43a freezing flowing liquid carving up the landscape.
- 0:46So today we are taking you on a deep dive into
- 0:48Titan. That's Saturn's largest moon. Our mission
- 0:51today is to give you a comprehensive tour of
- 0:54what is honestly the most. Genuinely Earth -like
- 0:56place in the solar system, but built out of completely
- 0:59alien chemicals. It really is. And we're going
- 1:02to take this step by step. You don't need any
- 1:03prior astronomy background for this deep dive.
- 1:05Just, you know, your natural curiosity. Because
- 1:09to understand how you could fly with just your
- 1:10arms, we first have to look at Titan's basic
- 1:13stats. Right. So let's talk scale. Titan is huge.
- 1:17It's Saturn's largest moon, and it's actually
- 1:18physically larger than the planet Mercury. Yeah,
- 1:21larger in volume, though it's less massive overall.
- 1:24Mercury is a dense ball of iron and rock, whereas
- 1:27Titan is made of a lighter mix of water, ice,
- 1:29and rocky material. And it orbits Saturn from
- 1:32about 1 .2 million kilometers away. Which takes,
- 1:35what, about 16 days to make one loop? Exactly,
- 1:3816 days. And it is tidally locked. So that means
- 1:41the exact same side always faces Saturn, just
- 1:43like our moon always shows the same face to Earth.
- 1:45And because it's so far out there, I mean, it's
- 1:47nearly 10 times further from the sun than we
- 1:49are. The surface temperature is a savage minus
- 1:52180 degrees Celsius. Minus 180. That is a kind
- 1:56of cold that completely redefines physics. At
- 1:59that temperature, water acts almost identically
- 2:01to silicate rock on Earth. It's brittle, it's
- 2:04hard, and it's immovable. So when you look at
- 2:06a water ice mountain on Titan. You have to think
- 2:10of it exactly like a solid granite mountain here
- 2:13on Earth. It's just bedrock. That's a great analogy.
- 2:17And, you know, for centuries, Titan was basically
- 2:19just a mystery. It was discovered way back in
- 2:211655 by Christian Huygens with a home -built
- 2:25telescope. But for ages, it was just a faint
- 2:28dot of light. Right up until the 1940s, right.
- 2:30That's when scientists used spectroscopy on it.
- 2:33For those listening, spectroscopy is a technique
- 2:35that spreads light out into its component wavelengths,
- 2:38and it reveals exactly which chemicals are present.
- 2:41Yeah, and that data changed everything. It showed
- 2:43Titan has an atmosphere. Specifically, they found
- 2:46methane. And finding an atmosphere around a moon
- 2:49was revolutionary. No other moon we knew of had
- 2:51a real atmosphere. But the bulk of it is actually
- 2:53nitrogen, right? Like overwhelmingly nitrogen.
- 2:56Yeah, much like Earth's, which is about 78 %
- 2:58nitrogen. But Titan's atmosphere is about 50
- 3:01% denser than Earth's at sea level. Which brings
- 3:04us back to that flying image from the intro.
- 3:06You've got this super dense air combined with
- 3:09surface gravity that's only one seventh of Earth's.
- 3:12So human flight under just muscle power is genuinely
- 3:16physically possible. You really could just take
- 3:18a running start and take off. It's an aviator's
- 3:20dream. Okay. But if the atmosphere is mostly
- 3:23nitrogen and nitrogen is invisible, where does
- 3:26that famous orange color come from? Like in photos,
- 3:30Titan looks like an orange billiard ball. Ah,
- 3:33that is the photochemical haze. See, the sunlight
- 3:36added Saturn is weak, but the ultraviolet radiation
- 3:39is still strong enough to bombard the upper atmosphere
- 3:41and break apart those methane molecules high
- 3:44in the sky. And when they break apart, they don't
- 3:46just stay broken, right? The carbon and hydrogen
- 3:48fragments recombine with the nitrogen. Exactly.
- 3:50They form what we call tholins. And tholins are
- 3:53basically these complex organic residues produced
- 3:56when radiation acts on simple ices and gases.
- 3:59So these tholins just build up in the stratosphere.
- 4:01Yeah, they drift down like a very fine global
- 4:04haze. Over millions of years, they settle all
- 4:07over the surface. At the equator, they've actually
- 4:09built up into these vast fields of dark dunes,
- 4:12shaped by the wind into long parallel ridges.
- 4:15But I want to push back on the word sand dunes
- 4:17here, because when you say sand, I think of crushed
- 4:20quartz, like on a beach. But this is completely
- 4:23different. Oh, absolutely. It's not sand. It's
- 4:25more like soot dunes, right? Or maybe mountains
- 4:29of dark coffee grounds, which is wild because
- 4:31that makes Titan this natural laboratory for
- 4:34prebiotic chemistry. Prebiotic chemistry, meaning
- 4:36all those carbon -based reactions that happened
- 4:39on early Earth before biological life actually
- 4:41emerged. Titan is full of it. Even if it's way
- 4:44too cold for life to progress as far as it did
- 4:46here, the ingredients are literally raining from
- 4:48the sky. Which makes me wonder if methane is
- 4:51constantly being destroyed up high to make this
- 4:53soot. What's it doing down on the surface? Well,
- 4:56down on the surface, it is driving a complete
- 4:58hydrological cycle. And a hydrological cycle
- 5:01is basically a weather system of evaporation,
- 5:04condensation, and precipitation. But titans...
- 5:08mirrors Earth's water cycle using liquid methane
- 5:11and ethane. That is just so bizarre. So the weak
- 5:14sunlight evaporates the surface methane, it forms
- 5:17clouds, and then it falls as rain. Rains down,
- 5:20feeds into rivers, and pools into these massive
- 5:23lakes and seas at the poles. Though I should
- 5:26mention rain is a really rare seasonal event
- 5:29there. Right, because a Saturn year takes 29
- 5:31Earth years. So one single season on Titan lasts
- 5:34for about seven of our years. Yeah, so when it
- 5:37rains, it's like a massive desert downpour, a
- 5:39huge flash flood of methane. And we actually
- 5:41saw the results of this thanks to the Cassini
- 5:43mission. Its radar instrument could see right
- 5:45through that orange haze. And what it mapped
- 5:48out was incredible. The largest sea, Kraken Mare,
- 5:50is roughly the size of the Caspian Sea here on
- 5:52Earth. And it's over 100 meters deep in places.
- 5:55The volume is staggering. Kraken Mare holds several
- 5:58times more liquid than all of Earth's proven
- 6:01oil and gas reserves combined. Yeah. And there
- 6:03are others, too, like Ligia Mare and Punga Mare.
- 6:06Wait, several times more than all our oil and
- 6:08gas reserves? That sounds like a literal gas
- 6:10station planet just floating in space. I know
- 6:12it sounds like that, but we have to clarify.
- 6:15We are talking about cold, liquid gas acting
- 6:18as a solvent, not refined, combustible fuel.
- 6:21Ah, right, because there's no free oxygen to
- 6:24burn it anyway. Exactly. It's a completely alien
- 6:26liquid that just... erodes the landscape the
- 6:29way water does here. Okay, so we saw these lakes
- 6:31from orbit, but to really understand the surface,
- 6:33we had to drop a probe right through that haze,
- 6:36right? We did. The Cassini mission, which was
- 6:38this huge joint project between NASA, the European
- 6:41Space Agency, and the Italian Space Agency, launched
- 6:44in 1997. It finally arrived in 2004. And then
- 6:48in January 2005, the Huygens probe detached.
- 6:51It basically parachuted blind down into that
- 6:53atmosphere for over two hours. Yep. First spacecraft
- 6:56to ever land on an outer solar system world.
- 6:59I just marvel at the sheer engineering audacity
- 7:02of that. Jumping blind into an alien atmosphere
- 7:05where you don't even know what the ground is
- 7:07made of. It could have been liquid. It could
- 7:08have been a mountain of soot. But on the way
- 7:10down, the cameras actually photographed drainage
- 7:13channels. They looked exactly like dried earth
- 7:16riverbeds. And when it finally landed, it found
- 7:19those rounded water ice pebbles we talked about
- 7:21at the start. Yeah, the pebbles were key. They
- 7:23were smoothed out by flowing liquid over a really
- 7:26long time. Just imagine. looking at a smooth
- 7:29river rock on earth and realizing that the exact
- 7:32same physical process happened a billion kilometers
- 7:34away. just with liquid methane wearing down solid
- 7:38ice. It's beautiful. It really is. Now, Huygens
- 7:41only survived a few hours before the brutal cold
- 7:43killed its batteries, but it gave us our only
- 7:46ground -level view. Cassini eventually was deliberately
- 7:49crashed into Saturn in 2017, so it wouldn't contaminate
- 7:52any moons. But before it died, Cassini's instruments
- 7:55found something even stranger hiding beneath
- 7:57that rock -hard ice crust, didn't it? It sure
- 7:59did. They tracked variations in Titan's gravity
- 8:02and observed something called libration. Libration.
- 8:06Yeah, it's a small, periodic, flexing and rotational
- 8:09wobbling of the icy shell. It happens as Saturn's
- 8:12gravity tugs on the moon. Oh, I get it. It's
- 8:14like spinning an egg on a table. If you spin
- 8:16a hard -boiled egg, it spins perfectly smoothly.
- 8:19But if you spin a raw egg, the liquid sloshing
- 8:21around inside makes it wobble differently. That
- 8:24is exactly it. Titan wobbles like a raw egg.
- 8:27And this evidence strongly points to a global
- 8:30liquid water ocean sandwiched between that outer
- 8:32ice crust and a deeper rocky core. But how is
- 8:36there liquid water if the surface is minus 180
- 8:39degrees? Well, the water stays liquid because
- 8:41it's mixed with ammonia, which acts as a powerful
- 8:43natural antifreeze. And there's also tidal heating.
- 8:47Tidal heating being the distal heat generated
- 8:49by that constant gravitational kneading and stretching
- 8:52from Saturn, right? Right. And finding this hidden
- 8:54ocean puts Titan in the same category as Europa
- 8:57and Enceladus. Which naturally leads to the idea
- 8:59of volcanoes. Does that subsurface ocean ever
- 9:02break through? It raises the possibility of cryovolcanism,
- 9:05absolutely. Cryovolcanism is when volcanoes erupt
- 9:09cold, icy materials like a slushy water -ammonia
- 9:12mix instead of molten rock. And Cassini found
- 9:15mountains that look like volcanoes, right? Like
- 9:17Dumon. Dumons and Sotroptera, yeah. They look
- 9:20a lot like volcanic dones and calderas. But I
- 9:24need to be careful here. This is heavily debated.
- 9:26It is an open question, not a confirmed fact.
- 9:28It could just be unusual erosional features.
- 9:31Okay, fair enough. But still, you've got an ocean
- 9:33of liquid water below and this complex chemical
- 9:36soup of organic molecules above. I have to ask
- 9:39the ultimate question. Could anything live there?
- 9:41That is the million -dollar question. If we look
- 9:44at conventional habitability like what we look
- 9:46for on Mars or Europa, we want liquid water as
- 9:49the essential solvent for life. By that standard,
- 9:52Titan's buried ocean is a huge prime target.
- 9:55But what about the surface with all that methane?
- 9:57The surface offers a much, much stranger hypothesis.
- 10:00Highly speculative. Could life use liquid methane
- 10:03as a solvent instead of water? How would that
- 10:05even work? Because Earth cell membranes are made
- 10:08of fats, right? Lipids. They just freeze solid
- 10:10in minus 180 degree methane. Exactly. They would
- 10:13shatter. Yeah. So chemists theorize something
- 10:16called an exotism. An azotosome is a theoretical
- 10:19cell membrane built from small, nitrogen -containing
- 10:22molecules. And they think that would work. Well,
- 10:25computer models suggest it could function stably
- 10:28in liquid methane. unlike our fatty cell membranes.
- 10:31But I cannot emphasize enough the need for scientific
- 10:35caution here. This is entirely a theoretical
- 10:38thought experiment. Yeah, I'm glad you brought
- 10:39that up because I see these sensationalized headlines
- 10:42all the time screaming, you know, life on Titan.
- 10:45How do you feel when you see that media hype?
- 10:49It's frustrating. We have zero evidence of these
- 10:51membranes existing, zero biosignatures, no proof
- 10:54they can even support a metabolism. We have to
- 10:56separate an intriguing hypothesis from actual
- 10:59responsible science. So the azishum is basically
- 11:02just fun on a chalkboard for now, not actual
- 11:04biology. Exactly. So if we can't definitively
- 11:06answer the life question yet, how do we actually
- 11:09find out what's happening in this chemical laboratory?
- 11:11By going back. And this time, we're going to
- 11:14fly. The next NASA mission is called Dragonfly,
- 11:17launching later this decade and arriving about
- 11:19six years later. And this isn't just a wheeled
- 11:21rover. No, it is a rotorcraft, basically a car
- 11:24-sized drone. And it explicitly takes advantage
- 11:26of that thick atmosphere and low gravity we talked
- 11:29about earlier. I love that. We couldn't fly a
- 11:31heavy drone like this on Mars because the air
- 11:33is just way too thin. But on Titan, the very
- 11:36atmosphere that creates that thick, oaring haze
- 11:39makes it an aviator's dream. It really does.
- 11:42Dragonfly will hop from site to site, sampling
- 11:45chemistry and geology all over the place. And
- 11:48one key target is the Selk Impact Crater. Why
- 11:52that crater specifically? Because an ancient
- 11:54meteor impact there may have melted the subsurface
- 11:56ice, mixing liquid water with those surface organics.
- 11:59It's the perfect spot to study prebiotic chemistry.
- 12:02So it's like a giant mixing bowl of water and
- 12:04tholins. Exactly. The goal of Dragonfly is to
- 12:07study the chemical steps that actually lead to
- 12:09life, not necessarily to find life itself. Which
- 12:12brings us full circle. Titan is just this bizarre
- 12:15yet familiar world. You've got rain, rivers,
- 12:19dunes, oceans. But water acts like rock and methane
- 12:23acts like water. It really just shows us how
- 12:26incredibly inventive planetary chemistry can
- 12:28be with whatever materials it has on hand. It
- 12:31totally does. And it leaves me with one final
- 12:33thought I want to throw out to you listening.
- 12:35If scientists are seriously theorizing about
- 12:37life using liquid methane right here in our own
- 12:40solar system, just imagine the billions of exoplanets
- 12:44in the wider galaxy. Oh, absolutely. The possibilities
- 12:46are endless. Right. What other bizarre, completely
- 12:50unrecognizable liquid solvents might be carving
- 12:53rivers on distant worlds right now, potentially
- 12:55hosting chemistries we haven't even dreamed of
- 12:57yet? It's just wild to think about. Thank you
- 13:00so much for taking this deep dive with us. Thanks
- 13:02for having me. Keep looking up.