Chapter 1: What makes Mimas unique among Saturn's moons?
The gas giant Saturn has 292 moons.
Yet within this spectacularly vast system, there's one moon that's instantly recognisable. With a colossal impact crater dominating its surface, Mimas looks more like the Death Star than a natural icy satellite. Its ominous crater was first spotted when the Voyager probe sped past in 1980. Almost instantly, scientists attributed it to an ancient collision of epic scale.
But since then, the moon has hardly changed. Compared with the likes of the active moon Enceladus and Titan, MIMIS almost seems boring, relegated to just another cosmic fossil, a simple reminder of how violent the early solar system must have been. That is, until 2024, when scientists found that hidden beneath its ancient, cratered shell, lies something that simply shouldn't exist.
Chapter 2: What was the initial assumption about Mimas's geological activity?
Mimas is not dead, it's an ocean world. This discovery has transformed the Death Star Moon from a celestial curiosity into one of the most important objects in our search for life beyond Earth. But how did we get Mimas so wrong, and just what lies beneath its surface? I'm Alex McColgan and you're watching Astrum.
Join me today as we peel back the icy crust of Saturn's innermost moon to reveal a secret ocean hiding in the dark, and delve into what this maritime discovery on Mimas means for the rest of the Saturn system. Mimas is a tiny moon.
It orbits around 186,000 km from its host planet Saturn, and with a mean diameter of just 400 km, it's actually the smallest astronomical body we know of to have pulled itself into a spherical shape due to its own gravity. For the most part, Mimas doesn't seem that special.
Chapter 3: How did the Herschel crater impact our understanding of Mimas?
It's not overly dissimilar to many of Saturn's other mid-sized moons like Tethys, Dione and Rhea. But what makes it stand apart is the fact that Mimas is a world whose history is clear to see on its surface. And that history is one of unimaginable violence. The surface is heavily cratered, but one feature is particularly prominent.
Mimas is dominated by the Herschel crater, an impact basin 130km wide. To put that in perspective, the crater covers nearly one-third of the moon's diameter. If a crater of the same relative scale existed on Earth, it would be more than 4,000km wide, larger than the entire continent of Australia, with walls towering more than 150km into the sky.
To help you imagine just how crazy that is, think of this. Mount Everest doesn't even quite stretch to nine kilometers. The impact that created this epic crater was a cataclysmic event that brought Mimas to the very brink of destruction.
Simulations suggest that if the impact had been just a little bit larger, or moving slightly faster, Mimas would have shattered completely, reduced to just another ring of debris orbiting Saturn. Luckily for us though, the moon survived.
Shockwaves from the impact travelled through the moon's core and focused on the exact opposite side, the antipodal point, where they ripped the crust apart, creating a complex network of canyons and fractures known as chasmata. For decades, planetary scientists looked at this battered surface and concluded that Mimas must be frozen solid.
A warm, slushy interior would have relaxed over time, smoothing out the crater walls and erasing the scars. The fact that the Herschel crater still stands, with walls 5km high and a central peak reaching up to 6km suggests that the ice shell was rigid and immensely thick, supporting these massive structures for billions of years.
Essentially, everything was pointing to Mimas being a geologically dead world. That is, until scientists found something strange happening on the surface.
Their clue that they'd got something wrong came later, through the Cassini mission. This makes sense. Reviewing information is the best way to see if your initial assumptions are mistaken. When I studied for tests at uni, I found that repeatedly practicing test questions was my best way to overcome gaps in my knowledge, especially when I had someone there to guide me through the answers.
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Chapter 4: What surprising discovery was made about Mimas in 2024?
Even more surprising? When you look at MIMA's invisible light, this difference completely disappears. The surface looks totally uniform. Nothing at all correlates to the anomaly we observe.
This led astronomer Dr. John Spencer to playfully joke that Mimas might actually be the Death Star, and that Darth Vader simply applied a clever coat of paint to fool our visible light cameras, hiding the truth from everything except the prying infrared eyes of Cassini.
Now, this thermal anomaly wasn't exactly a sign of internal heat, but rather a sign of how MIMAS interacts with its environment. You see, MIMAS orbits right inside Saturn's radiation belts. The moon is constantly bombarded by high-energy electrons trapped in Saturn's magnetic field.
These electrons slam into the leading face of Mimas, welding the powdery snow regolith into hard-packed ice crystals, a process called sintering. Now, this hard ice has high thermal inertia. That means that, just like a dense rock on Earth, it absorbs heat during the day and conducts it deep underground, leaving the surface cool. At night, that stored heat radiates back out.
Chapter 5: How does Mimas's ocean compare to other moons like Enceladus?
The mouth of Pac-Man, on the trailing side, is sheltered from this bombardment, so the surface there remains relatively fluffy and powdery, acting like an insulator that heats up quickly in the sun, but holds no heat at night. This solved the mystery of the thermal map, but in doing so, it also reinforced the idea that MIMOS was a passive object.
The anomaly was due to surface effects rather than anything internal. But whilst MIMOS is known for its surface features, it's governed by something else. Its gravitational dance with Saturn, an interaction that creates one of the most famous features in the solar system. If you look at Saturn through a telescope, you'll see its glorious ring system.
And if your telescope is good enough, you'll see a dark gap splitting the rings in two. This is the Cassini Division, a 4,800 km wide chasm separating the A ring from the B ring.
Chapter 6: What explains the Mimas Paradox regarding tidal heating?
This gap exists largely because of Mimas. MIMOS orbits Saturn once every 22 hours and 36 minutes, and particles orbiting within the inner edge of the Cassini division circle Saturn exactly twice every one orbit of MIMOS. This is a 2-1 orbital resonance. Every time MIMOS completes an orbit, it tugs on these ring particles at the exact same point in their path.
It's like pushing a child on a swing. If you push at the right moment every time, the swing goes higher and higher. Mimosa's gravity adds energy to these particles, stretching their orbits into ellipses until they collide with other particles or are ejected from the gap entirely.
For years, before Voyager flew past in 1980, revealing the Herschel crater, this resonance was the primary claim to fame for MIMIS. It was the shepherd of the rings, the gravitational influence that kept the Cassini division clear. But recent simulations have suggested that MIMIS didn't just clear a pre-existing gap. Instead, it may have acted more like a snowplough.
standard planetary system models suggest moons migrate outward over time. But in 2019, when researchers Kevin Bailey and Benoit Noyel were attempting to explain why the Cassini division was so wide, they found this couldn't be the case here. Their theory instead suggests that Mimas migrated inward towards Saturn somewhere between 4 and 11 million years ago.
As it did so, its resonance moved with it, pushing ring particles aside and carving out the division over millions of years. This interaction is crucial because it tells us that Mimas is not dynamically static, its orbit changes. and it was this orbital movement, specifically the way Mimas wobbles, that led to the most recent revelation about this tiny world.
Before we get into exactly what scientists found about Mimas, we have to address an elephant in the room, Enceladus. Enceladus is Mimas's neighbour. It's roughly the same size, composed of similar materials, and orbits just outside Mimas. But Enceladus is spectacular. It has tiger stripe fractures at its south pole that blast geysers of water vapour into space, creating Saturn's E-ring.
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Chapter 7: How does Mimas's orbital dynamics affect its geological features?
And we now know Enceladus has a global subsurface ocean that is warm and potentially habitable. I have another video on the latest discoveries here if you want to take a look. The problem is that according to standard tidal heating models, Mimas should be the active one. Mimas is closer to Saturn than Enceladus, and its orbit is much more eccentric.
Both of these factors mean that tidal heating, the friction generated inside a moon as it gets stretched and squeezed by gravity, should be much stronger. The math says that Mimas should be experiencing significantly more tidal heating than Enceladus. So why was Enceladus melting while Mimas looked like a frozen block of ice? This is what researchers have long called the Mimas Paradox.
The prevailing theory was that Mimas was simply too cold. If a moon freezes solid, its ice becomes rigid and it can't flex. This means that it doesn't generate friction, instead entering a state of high Q or quality factor, which implies low dissipation. Imagine hitting a bell. The energy isn't absorbed, instead the bell rings.
Enceladus, for whatever reason, stayed warm and slushy, allowing the tides to keep adding energy to its interior. Mimas, on the other hand, we assumed, missed its window. It froze early and stayed frozen. But that isn't the end of the story. In 2014, researchers noticed something wasn't quite right. They measured the Libration of Mimas, the slight wobble it experiences as it rotates.
This wobble was almost twice as big as it should have been for a solid body.
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Chapter 8: What implications does Mimas's ocean have for the search for extraterrestrial life?
Now at the time, there were two possibilities. Either Mimas had a strangely shaped core, elongated like a rugby ball, or its ice shell was physically disconnected from its core, sliding around on top of a liquid layer. Most scientists bet on the rugby ball. A notion just didn't make sense given the thick ancient crust. But then came 2024.
In February of 2024, a study published in Nature Astronomy put the debate to rest. A team led by Valérie Leynet analysed the drift of MIMAS's orbit using data from the entire 13-year Cassini mission. Just as MIMAS pushes on the rings, the rings and Saturn push back, causing MIMAS's orbit to precess. Essentially, the oval of its orbit slowly rotates around Saturn.
The rate of this precession depends heavily on the distribution of mass inside the moon. When the researchers plugged the data into their models, the rugby ball core theory fell apart. It couldn't explain the so-called orbital drift I just described. There was only one solution that fit the data perfectly. MIMOS has a global subsurface ocean.
But this isn't an ocean like the one on Europa or Enceladus. It's what I'm going to call a stealth ocean. It lies beneath an ice shell that is 20 to 30 kilometres thick. What's particularly interesting is that the researchers believe this ocean is incredibly young. The models suggest it formed between just 2 and 25 million years ago.
This young age of the ocean is crucial, in fact, it explains everything. The ocean is so new that the heat hasn't had time to radiate through the thick ancient crust. Essentially, the moon is melting from the inside out, and features that formed long before the ocean formed, like the Herschel crater, haven't yet been impacted. This discovery resolves the Mimas paradox.
Mimas isn't dead, it's just late to the party. You might even say it's an Enceladus in waiting. Given enough time, the ocean will continue to eat away at the ice shell. In a few million years, the stresses will become too great, the crust will crack, and Mimas might begin to spray its own geysers into the Saturnian skies.
Now, the realisation that Mimas has a young ocean leads to all sorts of fascinating possibilities, but there is one gaping question. Where did it come from? It turns out that the most likely culprit is actually its orbital instability. At some point in the recent past, perhaps just 10 million years ago, MIMOS likely entered a chaotic resonance with another moon, possibly Tethys or Dione.
This interaction would have pumped up MIMOS' orbital eccentricity, stretching its orbit into an even more extreme oval. As MIMOS swung closer to and further from Saturn, The immense tides were now powerful enough that they began to flex the moon's solid interior. The friction generated heat, enough heat to melt the ice and create a global sea.
And then there's the even bigger question I just know you've all been waiting to ask me. Could this be another potential place beyond Earth to look for life? Sadly, this ocean is likely to be a fleeting phenomenon. The very act of sloshing water around inside the moon dissipates energy. This acts as a brake, circularising the orbit.
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