Martian lithospheric thickness from elastic flexure theory

Details Martian lithospheric thickness from elastic flexure theory Martian lithospheric thickness from elastic flexure theory

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978georl...5..977t&link_type=abstract

Geophysical Research Letters, vol. 5, Nov. 1978, p. 977-980.

Astronomy and Astrophysics

Astrophysics

17

Elastic Properties, Lithosphere, Mars Surface, Planetary Structure, Displacement Measurement, Stress Distribution, Tensile Stress, Topography, Mars, Thickness, Lithosphere, Volcanism, Deformation, Tharsis, Montes, Stress Differences, Crust, Flexing, Olympus, Mons, Topography, Models, Surface, Gravity Anomalies, Elastic Deformation Equations, Seismicity, Diastrophism

Scientific paper

The thickness of the elastic lithosphere in the Tharsis region of Mars is estimated from effects due to the surface load of Olympus Mons. Deformation (vertical displacement) and stress are calculated using elastic flexure theory for a range of possible lithospheric thicknesses (T), modeling the lithosphere as a thin elastic shell and the interior as a Newtonian fluid. For T below 150 km, displacement and stress rise rapidly with decreasing thickness. For T near 100 km, deformation of the region surrounding the volcano would be clearly visible in the topography, and resulting tensional stresses exceeding 5 kbar should produce observable fracturing at the surface. In contrast, for T near 200 km deformation is minimal and the tensional stress, being less than a kilobar, would not result in extensive fracturing. Since significant deformation and fracturing are not observed, it is concluded that the Martian elastic lithosphere is at least 150 km in thickness. Seismic, tectonic, and gravity observations all suggest a thick Martian lithosphere as well.

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