Physics
Scientific paper
Dec 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..106..365j&link_type=abstract
Icarus, vol. 106, p. 365
Physics
15
Mars Surface, Planetary Craters, Ice, Regolith, Soil Mechanics, Creep Properties, Topography, Temperature Dependence, Finite Element Method
Scientific paper
FEM is here used to investigate the relaxation of impact craters on Mars, due to creep deformation of subsurface ice, that has been hypothesized as a basis for the 'terrain softening' type of landform degradation. A non-Newtonian viscoelastic rheology derived from experiments on frozen solids is asummed. The results thus obtained imply a Martian midlatitude softened terrain morphology consistent with relaxation in a deforming layer that is no more than 1 km in depth. The total amount of Martian subsurface ice is estimated on this basis.
Jankowski David G.
Squyres Steven W.
No associations
LandOfFree
'Softened' impact craters on Mars - Implications for ground ice and the structure of the Martian megaregolith does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with 'Softened' impact craters on Mars - Implications for ground ice and the structure of the Martian megaregolith, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 'Softened' impact craters on Mars - Implications for ground ice and the structure of the Martian megaregolith will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1299778