BOXWORK STRUCTURES AND GROUNDWATER VOLUME ESTIMATES ON MOUNT SHARP, MARS
Formation hypotheses are proposed in order to calculate a conservative estimate for the amount of water required to form the boxwork layer. The volume of the boxwork ridges is estimated based on aerial exposure (20-50% of the observed 1 km2 of boxwork structures), an assumed minimum 5 m depth, and a hypothesis that the ridges are either porosity-occluding cements, making up ~ 30% of the ridge volume, or space-filling cements, making up the full ridge volume. A cement composition is assumed based on a brine composition derived from the mineral assemblage in the evaporate-rich Burns Formation, Meridiani Planum, as measured by the Opportunity rover. The evaporation of this derived brine was modeled by Tosca et al. using Geochemists Workbench to obtain the mass of cement relative to the percent of water that evaporated (Tosca et al., JGR, 2011). Assuming 90-99% of the water evaporates, 800-3500 “pore volumes,” or cement-volume-equivalent volumes of water, are required before the volume is filled with cement. For a porosity-occluding cement, that means 0.23 – 2.62 km3 of water are required, or for a volume-filling cement, 0.77 – 8.75 km3 of water are required to form the exposed boxwork deposit. This is a significant amount of water 700 m above ground-level, and possible future investigation of these and similar deposits with the Mars Science Laboratory rover could provide detailed information concerning the history of groundwater chemistry in this region.