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NASA's InSight Detects Three Strongest Marsquakes Yet, Peering Deeper into the Red Planet

NASA's InSight lander has detected its three most powerful Marsquakes to date, providing scientists with unprecedented insights into the Red Planet's interior.

Landed in November 2018 on the western edge of Elysium Planitia at Mars' equator, NASA's InSight mission uses sensitive seismometers to capture subtle seismic waves traveling through the planet's depths. By analyzing these signals, researchers gain valuable data on Mars' internal composition. Unlike Earth, Mars lacks active tectonic plates but features seismically active zones capable of generating significant tremors.

To date, InSight has recorded over 500 Marsquakes. Previously, the strongest were magnitudes 3.6 and 3.5, both originating from Cerberus Fossae—a region of parallel faults. Additional quakes of magnitudes 3.3 and 3.1 from the same area were detected on March 7 and 18, underscoring Cerberus Fossae as a key seismic hotspot, though not the only one.

NASA s InSight Detects Three Strongest Marsquakes Yet, Peering Deeper into the Red Planet

Three Record-Breaking Events

On August 25, InSight recorded tremors of magnitude 4.2 and 4.1, followed by another magnitude 4.2 quake on September 18—coinciding with the lander's 1,000th Martian sol.

Analysis of the August 25 events is underway. The magnitude 4.2 quake originated approximately 8,500 kilometers from InSight—farther than Cerberus Fossae, which lies about 1,600 km away—marking the most distant Marsquake detected to date, according to NASA.

Its epicenter remains uncertain, but "Valles Marineris, the vast canyon system along the Martian equator, is a compelling candidate," researchers noted. "The approximate center of this system is 9,700 km from InSight."

In contrast, the magnitude 4.1 event on August 25 struck closer, at about 925 km.

Strikingly, the two August quakes exhibited distinct wave patterns: the magnitude 4.2 featured dominant slow, low-frequency vibrations, while the 4.1 was rich in fast, high-frequency ones. This diversity aids seismologists in mapping Mars' internal structure more precisely.

Recent mission data has enabled NASA to produce the first comprehensive map of Mars' interior, tracking how seismic waves change speed and direction as they propagate through the planet.