[MIS18-P03] Verification for water in the Mars' interior based on rheological structure
Keywords:Mars, water, elastic thickness, rheological structure
We estimated rheological structure to determine elastic thickness. Rock strength in brittle and ductile deformation regions was determined from the frictional strength (depending on pressure) and flow laws (depending on composition and temperature), respectively. Under wet conditions, we assumed pore pressure and decrease of frictional coefficient in brittle regions and intracrystalline water in ductile regions. We applied diffusion creep, dislocation creep and Peierls creep in ductile regions. We calculated temperature profiles from the concentration of radioactive isotopes and their half-time. Ages are determined by the crater chronology.
Consequently, the younger they are, the thicker elastic thicknesses are in general. In the case of younger areas, values under dry conditions are consistent with observed ones. However, values under wet conditions are more consistent in older areas. Therefore, it is suggested that older areas (especially formed in Noachian) were under wet conditions when they are formed.
If there had been plate tectonics on early Mars (Sleep, 1994), subduction by plate tectonics had carried water into the Mars’ interior and there were much water there in Noachian. However, plate tectonics stopped and no more water carried into the interior. Water decreased by degassing, then there were little or no water.