Cerberus Fossae

The Cerberus Fossae are a series of semi-parallel fissures on Mars formed by faults which pulled the crust apart in the Cerberus region. They are 1235 km across and centered at 11.28 °N and 166.37 °E. Their northernmost latitude is 16.16 °N and their southernmost latitude 6.23 °N. Their easternmost and westernmost longitudes are 174.72 °E and 154.43 °E, respectively. They can be seen in the Elysium quadrangle. Ripples seen at the bottom of the faults are sand blown by the wind. Numerical modeling of the forces in the crust of Mars suggest that the underlying cause for the faulting is the deformation caused by the Tharsis volcanoes to the east. The faults are quite young, cutting through pre-existing features such as the hills of the Tartarus Montes and the lava apron southeast of Elysium Mons.

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Volcanic Activity Could Be Responsible for Triggering Marsquakes in Cerberus Fossae

Volcanoes raged on Mars as recently as 50,000 years ago, new research suggests. Scientists previously thought Mars' volcanoes shut down some 3 million years ago, but new dark deposits spotted near the young tectonic fissure Cerberus Fossae suggest otherwise.

NASA's InSight lander tracked down the epicenter of another pair of strong marsquakes. The source is one of Mars' youngest regions, Cerberus Fossae, which features deep surface cracks that were filled with lava some 10 million years ago.