Edge of the Olympus Mons
NASA/JPL/University of Arizona

Edge of the Olympus Mons
PSP_002184_2005  Science Theme: Mass Wasting Processes


Olympus Mons, the largest volcano in the Solar System, has a mysterious halo (aureole) of material on its western and northern sides. There have been many ideas about how this feature may have formed over the years, but the hypothesis that this is a giant landslide deposit has gained favor.

Many large volcanoes on the Earth collapse under their own weight, so it seems reasonable that Olympus Mons would do the same. The edge of the aureole is seen at the top (northern) part of the image.

It is interesting that the main part of the aureole seems sunk down compared to the edge. It is possible that the ridge along the outer margin of the aureole formed as the flow turned around after pushing uphill for a ways. Imagine a giant wave of rock pushing up onto the "beach" and then receding. It might leave a deposit like this.

Alternatively, glaciers push up a ramp of rock at their fronts. After they retreat, the ridge of rock is left at the furthest extent of the glacier. These are called "terminal moraines" by geologists. Written by: Laszlo P. Keszthelyi   (10 June 2007)



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Acquisition date:13 January 2007 Local Mars time: 3:36 PM
Latitude (centered):20.1 degrees Longitude (East):219.7 degrees
Range to target site:282.2 km (176.4 miles)Original image scale range:56.5 cm/pixel (with 2 x 2 binning) so objects ~169 cm across are resolved
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