Bedtime Astronomy

The Moon Is Shrinking: What 10,000 Lunar Faults Reveal

Donnerstag, 22. Oktober 2026 · 20 min

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Scientists have mapped more than 10,000 young tectonic landforms on the Moon, revealing how its interior cooling has caused the lunar radius to shrink by about 45 meters over the past 400–800 million years.

Unlike Earth, the Moon has a single outer shell, spreading contraction faults across its surface. These findings offer new clues about ongoing lunar activity, including the potential for moonquakes.

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.

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Welcome to Bedtime Astronomy. Explore the wonders of the cosmos with our soothing Bedtime Astronomy 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.

You know, when you walk outside on a clear night and look up, there is this, um, This profound sense of permanence.

Oh, absolutely. It feels completely unchanging.

Right. You see the moon hanging there, glowing, and it feels like the ultimate symbol of a static universe. I mean, it's the exact same silver disk that the ancient Egyptians looked at.

Yeah, the exact same craters that Galileo sketched in his notebooks.

Exactly. We have this deep-seated assumption that the moon is just a dead, frozen rock floating in the dark. But what if I told you that the silent moon seemingly frozen sphere you are looking at is actually, well, actively changing shape.

It's just wild to think about.

It is. It is literally shrinking.

It completely shatters that illusion of a static night sky, doesn't it?

It really does.

I mean, we look up and think we are seeing a fossil of the early solar system, perfectly preserved in the vacuum of space. But the reality is far more chaotic. The moon is a physically shifting, buckling, and evolving body right this very second.

Okay, let's unpack this. Because today, we are taking the ultimate geological cold case, a moon we all assume died billions of years ago, and cracking it wide open using 17 years of new orbital data.

And the sheer scale of what is happening up there is just mind-blowing.

We really need to figure out why its crust is violently buckling today. And, you know, what a restless lunar surface means for the astronauts we are about to send up there for permanent settlement.

Well, to really grasp the scale, we have to look at the latest findings published on October 14, 2026 in the Planetary Science Journal.

OK, so this is incredibly recent.

Brand new. A research team managed to map over 10,000 young faults distributed all across the moon's surface.

Wait, 10,000?

10,000. We are talking about severe fractures in the bright, mountainous highlands and massive stress lines across the dark, flat plains, the Maria, that make up that man-in-the-moon face we all recognize.

10,000 faults. I mean, that is not a localized, isolated event. That is a global phenomenon.

Exactly. It's happening everywhere.

And when we talk about the moon shrinking, the numbers they found are, well, they're fascinating, but also incredibly counterintuitive.

Yeah. They really put things into perspective.

They estimate that the moon's radius has decreased by approximately 45 meters, which is about 148 feet, over the past 400 to 800 million years.

Right. And to put a finer point on the rate of that shrinkage, if it has been relatively constant over that massive stretch of time, we are looking at a decrease of about 6 to 11 centimeters.

Okay. So roughly 2.4 to 4.3 inches.

Yeah, but that's every million years.

That translates to about 0.1 micrometers per year.

Wait, I need to put that into perspective. Earth's tectonic plates move at about 1.5 centimeters per year, right?

Right.

Which we usually compare to the speed that human fingernails grow.

Okay, so if Earth's plates are moving at fingernail speed, the moon's shrinkage is microscopically slow by comparison.

Incredibly slow. You'd need a highly sensitive laboratory microscope to even register 0.1 micrometers a year.

Which brings me to a major point of friction here. If it's only shrinking by 45 meters over hundreds of millions of years, which is essentially the length of half a football field over an eternity, why is this such a monumental geological discovery?

That's a fair question.

I mean, it sounds almost negligible to the naked eye.

What's fascinating here is that the importance isn't in the speed. It is in the continuity and the implication.

The implication. Yeah.

Yes, the rate is incredibly slow, but it is continuous, pervasive, and happening everywhere at once.

Okay, I see.

For the longest time, the scientific consensus was that the moon had completely cooled and died geologically billions of years ago.

Right, the frozen rock theory.

Exactly. So finding 10,000 active young faults proves that the moon's internal engine hasn't completely shut down. It forces us to just completely rewrite our understanding of the moon as a dynamic evolving body rather than a cold dead artifact in space.

That makes total sense. And, you know, arriving at that 45 meter number wasn't just a matter of pointing a telescope from a backyard and snapping a photo.

Oh, definitely not.

I'm trying to wrap my head around how you even measure a 45 meter shrinkage on a celestial body that is, what, a quarter of a million miles away?

It required an astronomical amount of sustained data processing. I mean, this discovery is built on 17 years of continuous observations.

Wow. 17 years. Yeah.

The Lunar Reconnaissance Orbiter Camera, or LROC, has been orbiting the moon for nearly two decades, sending back millions upon millions of high-resolution images.

Millions of them.

And they combine that with data from the shadow cam aboard the Korea Pathfinder Lunar Orbiter. That camera is sensitive enough to peer into the permanently shadowed craters near the poles.

So they aren't just taking direct photographs. They are actively using the shadows themselves to measure the terrain.

Precisely the mechanism. As the sun moves across the lunar sky, these fault lines cast shadows.

Oh, that's brilliant.

By tracking the exact length and angle of those shadows over 17 years, scientists can use trigonometry to calculate the precise height and slope of the cliffs created by the faults.

Okay, so when you have the exact geometry of 10,000 overlapping, buckling cliffs, you could essentially reverse engineer the math.

Exactly. You calculate how much surface area was lost when those cliffs pushed over one another, and that gives you the total volume the moon has lost.

That is wild. It's like measuring the wrinkles on a raisin to figure out exactly how big the grape used to be, but doing it with millions of photographs of shadows.

That's actually a great way to put it.

So we have 17 years of high-definition proof that the moon's surface is wrinkling. But a sponge only shrinks when water evaporates, right? And there's no water evaporating into the vacuum of space.

Right, no water there.

To find the missing volume, we have to look thousands of miles beneath the surface. What is actually causing an entire celestial body to lose its mass?

Well, it all comes down to planetary anatomy and thermodynamics. If you were to slice the moon in half, Right at the center, you would find an innermost solid core. And wrapping around that is a liquid outer core.

Kind of similar to Earth, though obviously on a much smaller scale.

Exactly. And that core is hot. It contains the residual primordial heat from the moon's incredibly violent formation over 4 billion years ago.

4 billion years is a long time to hold on to heat.

It is.

But over time, the universe always wins when it comes to heat. That core is gradually losing heat to the surrounding layers.

Okay, so it's cooling down. Yeah.

And as those internal materials cool down, they experience thermal contraction. The molecules literally lose kinetic energy, pull closer together, and physically take up less space. So the interior of the moon is shrinking.

Wait, I'm stuck on the timeline here. If the moon formed 4 billion years ago, its core has been cooling that entire time.

Right.

Shouldn't it have shriveled up and cracked eons ago? Like, why are we seeing young faults now? If the heat is from 4 billion years ago, the math of the timeline feels like it's missing a massive variable.

This raises an important question, and the answer is incredibly elegant. It has to do with the moon's outer layer, the crust.

Okay, what about it?

Widespread faulting didn't happen early in the moon's history because the lunar crust isn't just solid, pristine rock. It is thick, highly fractured, and incredibly porous.

Because of all the impacts? Yes.

Billions of years of constant asteroid and meteorite impacts have basically pulverized the outer layer of the moon into a deep rubble pile known as regolith.

Oh, I see where this is going. The moon is basically wearing a massive, porous, down winter coat.

A winter coat, exactly.

Like, if you wear a thick down jacket, the warmth from your body is trying to escape into the freezing air, but it gets trapped by all those tiny pockets of air in the feathers.

Yep.

So the moon's pulverized crust has been acting as a literal heat trap. It insulated the core for billions of years and only recently, in geologic terms anyway, has enough of that ancient heat finally managed to bleed out through this coat to make the entire body of the moon essentially shiver and shrink.

Building on that analogy, you have to factor in the environment of space. On Earth, a down jacket traps air. On the moon, there is no air. The regolith is full of vacuum.

Oh, wow. And vacuum is an insulator.

A vacuum is the ultimate thermal insulator because there are no gas molecules to transfer the heat from one piece of dust to another.

That makes so much sense.

The heat from the moon's core can only travel through the microscopic points where these pulverized rock fragments physically touch.

Which is terribly inefficient.

Exactly. Because of that extreme vacuum insulation, the interior stayed warm for billions of years longer than it would have otherwise. It delayed the cooling process, creating a massive, trapped reservoir of thermal energy.

So the timeline makes perfect sense now. The heat didn't escape early on. It was artificially bottled up by the pulverized crust. Right. What we were seeing now with these young faults is the delayed reaction finally reaching a critical threshold.

You've got it.

The heat is finally dissipating enough that the physical volume of the moon's interior is significantly reducing, pulling the surface inward.

And that thermal contraction forces the crust to respond.

Here's where it gets really interesting. because we have to contrast how the moon handles that physical stress compared to the ground we are standing on right now.

Earth's geology is very different.

Yeah. On Earth, we have a multi-plate system. Our crust is a jigsaw puzzle of more than 15 lithospheric plates.

And that's why 90% of our tectonic and seismic activity is localized at the boundaries where those plates meet.

Right.

We have subduction zones where one plate can dive deep into the mantle, melting and recycling the crust, which provides... a natural pressure relief valve for the planet's geometry.

The Earth's surface can easily accommodate movement because of those boundaries. But the moon is a single plate body.

A single plate.

It acts like one continuous, unbroken shell of rock. There are no plate boundaries, no subduction zones to absorb the excess material.

It's like an old apple left on the kitchen counter. Oh, I like that. As the inside of the apple dries out and loses volume, the skin on the outside, which has a fixed surface area, has no choice but to wrinkle and fold over itself to fit the new smaller interior.

That's exactly what's happening.

The moon's crust has nowhere to go. If the inside shrinks, that rigid, unbroken exterior has to snap, buckle, and break everywhere all at once.

That apple skin comparison perfectly illustrates global compression. Because there are no plate boundaries to absorb that contraction, the stress builds up within the single plate until the solid rock physically fractures.

It just gives way.

Yeah. When it snaps, it creates what geologists call thrust faults. The surface breaks, and the immense global pressure forces one side of the crust to physically thrust up and over the other side.

So it's basically overlapping itself.

Exactly. On the moon, these wrinkles take the form of small mare ridges in the dark plains and lobate scarps in the highlands.

Well, if you push the skin of an apple together, you get a tiny little ridge. But we're talking about solid rock under immense gravitational and tectonic stress.

A lot of stress.

When the moon's crust snaps and pushes over itself, that can't just be a crack you step over. That has to create some serious, dramatic terrain.

Serious is an understatement. If you look at the data from the Mouchet L impact crater near the moon's north pole, researchers mapped a lobate scarp right on the floor of that crater.

How big is it?

The maximum relief, meaning the height of the newly formed cliff above the surrounding terrain, is over 100 meters.

Wait.

Yeah.

Over 100 meters.

Yeah. That is over 300 feet tall.

That is a 30-story building. A 30-story cliff of solid rock just violently shoved upward because the planet beneath it shrank.

It's a massive geological event.

It's hard to fathom a piece of land the size of a skyscraper just sliding up over the surrounding plains. And how do we know these massive cliffs are young? In geological terms, a rock face could have been sitting there for Two billion years.

The LROC imagery provides the visual evidence. These low-weight scarps have incredibly crisp, sharp edges.

I see.

On the moon, micrometeorites constantly bombard the surface, slowly acting like sandpaper. Over hundreds of millions of years, any sharp cliff gets ground down into a smooth, rounded hill.

Right, the erosion of space. Exactly.

So the fact that these 300-foot scarps are jagged and cross-cut over relatively recent small impact craters... tells scientists that these thrust faults formed recently, and they are likely still forming.

Okay, that feels like a vital piece of information. The buckling isn't ancient history. The cooling, shrinking, and snapping process is actively continuing today.

Very much so.

But the crust isn't snapping evenly, right? I assume a global shell of varying thickness doesn't just fold symmetrically.

You're touching on a crucial nuance regarding the stability of that shell. The mapping revealed a distinct pattern.

What kind of pattern?

The regions where the lunar crust is the thickest appear to have the fewest contractional faults.

Oh, that makes sense.

The thicker the rock, the more stable the region, because it takes significantly more internal stress to snap a thick layer of crust than a thin one.

Imagine you are an astronaut or an engineer for the upcoming Artemis missions, tasked with building a permanent human habitat on the lunar surface.

That's a stressful job right now.

Right. You spent your whole life looking up at the moon, thinking it's perfectly still. You land. You start laying the foundation for a multibillion-dollar base. And suddenly, the ground beneath your heavy boots could literally thrust upward violently without any of the warning signs we might look for on Earth.

Yeah, no warning at all.

Because a snapping fault line means an earthquake, or in this case, a moonquake. So what does this all mean for us, for the engineers and the future of humanity up there?

If we connect this to the bigger picture, it means... A complete paradigm shift in how we plan lunar exploration.

We have to be way more careful. Exactly.

We can't just pick a landing site because it looks relatively flat or because it has good solar exposure for the solar panels. The geological stability of the ground beneath the habitat is now a primary safety factor.

That's a huge deal.

Future missions must specifically seek out those thick crust regions to minimize the risk. If you build a habitat near a young lobate scarp, you are risking catastrophic damage to the infrastructure from shallow and incredibly powerful moonquakes.

And a moonquake is a completely different beast than an earthquake, isn't it?

Very different.

On Earth, we have oceans, groundwater, and a relatively warm pliable crust. Water acts as an acoustic dampener.

Right.

The energy from an earthquake gets absorbed by the damp, soft layers of the Earth, so the shaking usually stops after a few seconds, maybe a minute for a massive quake. But the moon is completely bone dry.

Exactly the distinction that makes this so dangerous. Because the lunar crust is bone dry, cold, and highly fractured, it acts like a giant acoustic chamber.

Oh, wow.

When a thrust fault slips and generates a moonquake, there is no water to dampen the vibrations. The seismic energy just bounces around the interior. The moon essentially rings like a bell.

Which means the shaking doesn't just last for a few seconds.

No, it can last for hours.

Hours. That's terrifying.

We actually saw hints of this during the Apollo missions, when astronauts left seismometers on the surface. They recorded shallow moonquakes that caused the surface to shake violently for incredibly long durations.

But back then, they probably didn't know why.

Exactly. We didn't fully understand the mechanism driving them. Now, with the map of these 10,000 young faults, we know the source.

That's incredible.

The maps these researchers have created are essentially going to become the definitive hazard maps for the next century of space exploration. Avoiding these actively buckling fault lines is literally a matter of life and death for future lunar colonists.

It is just incredible to think about the journey we've taken today. I mean, we started this conversation looking up at a quiet silver disc, thinking it was a serene monument to the past.

And it is anything but.

Right. What you are actually looking at is a world that is losing its ancient primordial heat, cooling from the inside out, and shivering under a porous, vacuum-sealed winter coat.

It's a great image.

It's a single, unbroken shell that is buckling and snapping under the immense pressure of its own shrinking interior. pushing up 30-story cliffs of solid rock and rattling the surface with violent, hours-long moonquakes.

And to add one final mind-expanding concept to that imagery, there is another force at play that is central to the stress on that shell.

Oh, another force. Yeah.

While the moon's interior is cooling and forcing the whole body to shrink inward, it is not sitting out there in isolation. It is locked in an intense, unending gravitational dance with Earth. Right.

The moon's gravity pulls on our oceans to create the tides. But Earth is significantly more massive.

Our planet's massive gravitational pull exerts intense tidal forces back on the moon. Every single day, Earth's gravity is physically tugging on, deforming, and stretching that exact same fragile, brittle, shrinking lunar shell. Wow.

So the moon is caught in this perpetual, chaotic tug-of-war.

A massive tug-of-war.

Its own internal cooling is relentlessly dragging the crust inward. forcing it to shrink, while Earth's gravity is simultaneously gripping it and pulling it outward.

Those thousands of thrust faults aren't just the result of shrinkage. They are the battle scars of a world caught between collapsing on itself and being stretched by its giant neighbor.

That's intense.

It is a level of physical stress that is almost hard to comprehend.

A chaotic tug of war between inward collapse and outward gravity. That paints such a beautifully violent picture of what is happening right over our heads.

It really does.

It really makes you realize how dynamic the universe is, even the parts that look the most peaceful and permanent. The next time you walk outside on a clear night and look up at that glowing sphere, you aren't just looking at a dead rock.

You're looking at a living geological engine.

Exactly. You are looking at a world that is shifting, cracking, and physically changing its shape in the dark. Thank you so much for joining us on this intellectual journey today. Keep looking up. and keep questioning the universe around you.

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