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No solid evidence for an inner core on Mars

By analyzing high-quality seismic data from the Cerberus Fossae region using source-array methods, this study finds that coherent signals interpreted as evidence for a Martian inner core are non-unique and can be explained by various candidate radii, thereby concluding that there is no definitive proof of an inner core on Mars.

Original authors: Marjolein Visser, Federico Munch, Amir Khan, Daniel Andrew Frost, Domenico Giardini

Published 2026-07-20
📖 4 min read☕ Coffee break read

Original authors: Marjolein Visser, Federico Munch, Amir Khan, Daniel Andrew Frost, Domenico Giardini

Original paper licensed under CC BY 4.0 (https://creativecommons.org/licenses/by/4.0/). This is an AI-generated explanation of the paper below. It is not written or endorsed by the authors. For technical accuracy, refer to the original paper. Read full disclaimer

The Great Martian Core Mystery

Imagine the inside of a planet like a giant, multi-layered chocolate truffle. You have the hard shell (the crust), the soft, gooey middle (the mantle), and a dense, metallic center (the core). For a long time, scientists thought Mars was a bit of a mystery box: does it have a solid center like a chocolate ball, or is the whole core just a swirling, liquid soup like a chocolate lava lamp? This question isn't just about trivia; it's a time machine. If Mars has a solid inner core, it means the planet is cooling down and freezing from the inside out, just like Earth. This process is the secret sauce behind how planets generate magnetic fields, which act like invisible shields protecting their surfaces from deadly space radiation. So, figuring out if Mars has a solid heart helps us understand how the Red Planet changed from a warm, wet world into the cold desert we see today.

The Search for a Ghost in the Seismic Machine

Recently, a team of scientists decided to take a fresh look at the "marsquakes" recorded by NASA's InSight lander. Think of InSight as a very sensitive stethoscope placed on the Martian surface, listening to the planet's heartbeat. When a marsquake happens, seismic waves ripple through the planet, bouncing off different layers like echoes in a canyon. If there is a solid inner core, these waves should bounce off its surface and return to the lander as a specific, distinct echo. A previous study claimed to have heard these echoes, suggesting a solid inner core about 600 kilometers wide.

However, the team in this new paper, led by researchers from ETH Zurich and the University of South Carolina, decided to play detective with a different approach. Instead of just listening for one specific echo, they used a clever trick called "source stacking." Imagine you are trying to hear a whisper in a noisy room. If you ask ten people to whisper the same thing at the same time, the whisper gets louder and clearer, while the background noise cancels itself out. The scientists took 23 of the best marsquakes from the same region (Cerberus Fossae) and stacked their seismic signals together to make the faint echoes much clearer.

The Twist: The Echoes Are Too Good to Be True

When they ran their analysis, they found something surprising. They did see coherent signals—clear echoes—that looked exactly like reflections from an inner core. But here is the catch: these "ghostly" echoes didn't just appear for the 600-kilometer core that the previous study suggested. The same clear signals popped up for a whole range of different sizes.

Using their stacking method, the team found that the seismic data could be explained by an inner core that is 200 to 300 kilometers wide, or 500 to 600 kilometers wide, or even anywhere between 100 and 600 kilometers for certain types of waves. It's as if you heard a knock on a door and tried to guess who was there. You might think it's a giant, but then you realize a medium-sized person, a small child, or even a very tall dog could make the exact same sound. Because the data fits so many different "guests," the scientists cannot say for sure which one is actually standing there.

The Verdict: No Solid Proof Yet

The paper concludes that while the data is interesting, it is not definitive. The signals previously interpreted as proof of a 600-kilometer solid inner core are not unique; they can be explained by many different scenarios. Therefore, the authors state there is currently no solid evidence confirming that Mars has a solid inner core. They didn't prove that Mars doesn't have one; they just proved that the current seismic data isn't strong enough to say that it does.

The study highlights that the seismic waves traveling through the inner core (a phase called PKIKKIKP) are particularly tricky because we don't know exactly how fast sound travels inside that core. This uncertainty makes it even harder to pin down the size. Until we get more data or better ways to listen to the planet's deep interior, the question of whether Mars has a solid heart remains an open mystery, waiting for more clues from the Red Planet.

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