Encyclopedia of Planetary Landforms 2015
DOI: 10.1007/978-1-4614-3134-3_14
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Basal Scarp (Olympus Mons, Mars)

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“…These events have distances around 90° as computed by MQS. We find a backazimuth of 85° for S1153a (Figure 8a), and locate both of these events in the approximate area of Olympus Mons (Figure 6), which is surrounded by a basal scarp of 2–10 km height and thrust faults as young as <40 Ma (Weller, 2015), as well as potential grabens cutting through young, late Amazonian terrain (Hargitai & Gulick, 2018). S0185a and S0234c can be paired with the impact S1094b I .…”
Section: Discussionmentioning
confidence: 89%
“…These events have distances around 90° as computed by MQS. We find a backazimuth of 85° for S1153a (Figure 8a), and locate both of these events in the approximate area of Olympus Mons (Figure 6), which is surrounded by a basal scarp of 2–10 km height and thrust faults as young as <40 Ma (Weller, 2015), as well as potential grabens cutting through young, late Amazonian terrain (Hargitai & Gulick, 2018). S0185a and S0234c can be paired with the impact S1094b I .…”
Section: Discussionmentioning
confidence: 89%