Models of Martian volcano explain why its shaped like a circus tentFebruary 4th, 2009 - 2:45 pm ICT by ANI
Washington, Feb 4 (ANI): Scientists have constructed models of the Olympus Mons volcano on Mars, in order to uncover the mechanism that generates the distinctive features of its shape, namely the form of a circus tent.
The immense Olympus Mons volcano on Mars (about 23 km tall and 600 km wide) exhibits a somewhat lopsided structure.
It is elongated to the northwest, shortened to the southeast, with corresponding types of faulting (extensional and compressional, respectively) prevalent in each sector.
However, the overall shape of the edifice is characterized by a decrease in slope with increasing distance from the center, somewhat like the surface of a tent that is supported by a single central pole.
In order to uncover the mechanism that generates the distinctive features of the shape of Olympus Mons, Patrick J. McGovern and Julia K. Morgan, from the Lunar and Planetary Institute, Universities Space Research Association, constructed models of the volcano as collections of particles that slip and slide past each other, controlled by the weight of other particles and the friction value assigned to each.
They found that a low-friction zone at the base of the volcanic pile is required, and lateral variations in basal friction are critical.
Friction decreasing outward from the center of the edifice can explain the overall circus tent shape, whereas friction decreasing from southeast to northwest accounts for the shortening and elongation of the respective quadrants.
The most likely origin for the basal low-friction zone is in a layer of clay sediment, overpressured by pore water.
This layer would be thicker in the downhill (northwest) direction, accounting for the asymmetry.
Such a layer likely corresponds to widespread and ancient clay deposits discovered by the Mars Express mission, and may constitute a favored environment for heat-loving organisms on Mars. (ANI)
Tags: ancient clay, asymmetry, circus tent, clay deposits, distinctive features, edifice, elongation, friction zone, lateral variations, lunar and planetary institute, mars express, martian volcano, mcgovern, northwest direction, olympus mons volcano, pore water, quadrants, slip and slide, space research association, universities space research