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Sliding Terrains and Dislocated Plates in Amazonis Planitia (Mars) as the Result of Instability of a Frozen Martian Ocean

  • Authors: Fabio Vittorio De Blasio

Fabio Vittorio De Blasio 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 8.

Formation of the sliding terrain due to ice pack instability. In panel (a) the water is retreating and one part of the ice floe (left) rests on a higher area (“local hill”), while the part on the right still floats on the water. As the ocean retreats (panel (b)), the tension across the ice crust grows (panel (c)) until failure occurs (panel (d)) and the ocean floor is exposed, which corresponds to observed terrain sliding due to gravity.

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