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doi:10.1029/2007JE002980Īnguita F, Fernández C, Cordero G, Carrasquilla S, Anguita J et al (2006) Evidences for a Noachian–Hesperian orogeny in Mars. Video showing motion in a strike-slip fault.īends along strike-slip faults create areas of compression or tension between the sliding blocks (see Chapter 2).Andrews-Hanna JC, Zuber MT, Hauck SA II (2008) Strike-slip faults on Mars: observations and implications for global tectonics and geodynamics. If the opposing block moves right, it is dextral motion. If the block on the opposing side of the fault moves left relative to the observer’s block, this is called sinistral motion. The direction of the strike-slip movement is determined by an observer standing on a block on one side of the fault. In pure strike-slip motion, fault blocks on either side of the fault do not move up or down relative to each other, rather move laterally, side to side. Strike-slip faults are most commonly associated with transform plate boundaries and are prevalent in transform fracture zones along mid-ocean ridges. Strike-slip faults have side-to-side motion. \): Ketobe Knob in the San Rafael Swell of Utah displays an example of a thrust fault.
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