Plate Nº 78 · recorded October 25, 2026
Space & AstronomyReported finding
Mars' Grand Canyon Is Still Tectonically Active, Study Finds
A magnitude-5 marsquake traced to a fault 20 to 40 km beneath Valles Marineris shows Mars' giant canyon is still tectonically active, scientists report.
By Priya Raman3 min read672 words
In brief
- On October 19, 2026, scientists announced Valles Marineris on Mars is still tectonically active.
- The marsquake S0976a, detected August 25, 2021, originated 12 to 25 miles (20 to 40 km) beneath the canyon.
- The quake equaled a magnitude 5 earthquake on Earth and was caused by strike-slip motion on an ancient fault.
- Valles Marineris stretches more than 2,500 miles (4,000 km), nine times longer than Earth's Grand Canyon.
- The peer-reviewed study appeared in Nature Communications on October 15, 2026.

A single marsquake, equal to a magnitude 5 earthquake on Earth, has led scientists to conclude that Valles Marineris — the Grand Canyon of Mars — is still tectonically active today, billions of years after it formed. On October 19, 2026, researchers at Columbia University and Imperial College London announced that the quake originated 12 to 25 miles (20 to 40 km) beneath the canyon system, triggered by rocks slipping along an ancient fault.
The team published its peer-reviewed findings in the journal Nature Communications on October 15, 2026.
Valles Marineris is the largest canyon system in the solar system. It stretches more than 2,500 miles (4,000 km), making it nine times longer than the Grand Canyon on Earth. It is also about 20 times wider and five times deeper than its terrestrial namesake.
Why does tectonic activity on Mars surprise us?
Mars does not have tectonic plates (the rigid slabs of crust that slide over Earth's mantle and drive most earthquakes here). Instead, scientists describe the Martian crust as a single, slowly cooling lid. As the planet continues to lose heat from its early years, the crust shrinks and cracks, forming faults.
Some of those faults, formed billions of years ago, can still slip and shift. That is what appears to have happened beneath Valles Marineris: an ancient fault line, reactivated by ongoing stress, produced a modern quake.
How did researchers find the marsquake?
The story begins on August 25, 2021, when NASA's InSight lander detected a tremor from its position in Elysium Planitia, on the opposite side of Mars from Valles Marineris. At first, researchers could not be sure it was a quake at all. Tremors on Mars can also come from landslides or meteorite impacts.
The event, named S0976a, turned out to be extraordinary. Its seismic waves had traveled through Mars' core, allowing scientists to study the planet's deepest interior. Its epicenter lay somewhere in the western Valles Marineris region, though its exact location and cause remained obscure.
The new research closed that gap. By analyzing the amplitudes and directions of the seismic waves, the team pinpointed the epicenter 12 to 25 miles (20 to 40 km) beneath the canyon and reconstructed what caused it.
Co-author Doyeon Kim of Imperial College London said: "S0976a has turned out to be an extraordinary event, playing an important role in our understanding of the red planet. Its waves traveled through the core and helped us investigate the deepest part of Mars, and now they are telling us what happened at the source itself. From a single marsquake, we can learn both about the center of the planet and about an active fault beneath one of its most remarkable landscapes."
What kind of quake was it?
The researchers concluded that a strike-slip marsquake was the most likely cause. A strike-slip event occurs when two chunks of crust move horizontally past one another along a steep fault with a deep root — the same basic mechanism as the San Andreas Fault, though on a planet with no moving plates.
Lead author Jung-Hun Song of Imperial College London said: "What makes the result compelling is that several completely different types of evidence point in the same direction. The seismic waves tell us that there was a sideways sliding motion on a fault well below the surface, while the geology seen from orbit shows a region crossed by long-lived fault systems."
Song added: "What we see is that this is not just a 'dead' fossil landscape, as faults deep beneath the canyon can still slip and generate marsquakes, long after the geological processes that originally formed them have ceased."
What comes next?
The result carries a built-in limitation. InSight ceased operations in 2022 after dust accumulated on its solar panels, and no active lander is currently recording marsquakes on the surface. Follow-up observations are, for now, impossible.
The next marsquake may go unrecorded until astronauts stand on the red planet and feel it shake beneath them.
via nature.com (Original)
More from Priya Raman
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Senior reporter covering people, launches and day-to-day practice in general science news at SciBeat.
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