CARBON SEQUESTRATION ON MARS: CONSTRAINTS FROM THE MORPHOLOGY, COMPOSITION AND THERMOPHYSICAL PROPERTIES OF THE NILI FOSSAE CARBONATE PLAINS
We find that the Nili Fossae rocks are olivine-enriched (~20%–25) basalts that have been variably altered by a near-surface, low-temperature, in-situ carbonation process to at most ~20% Fe-Mg carbonate. By using the areal extent of this deposit, and extrapolating to extents of unaltered precursor rocks (conservative estimate), the atmospheric carbon sequestration potential in the Nili Fossae region is limited to at most 50 mbar during the late Noachian/early Hesperian, and occurred before or concurrent with valley network formation.
While other atmospherically connected present day reservoirs exist, such as polar CO2 ice (~15 mbar) or adsorbed CO2 on regolith grains (<40 mbar), the amount that has escaped to space over martian history is significant (>500 mbar). Any large, geologic CO2 reservoirs, such as the “deep carbonates” are likely not atmospherically sourced and are inaccessible. Ultimately, we find that atmospheric sequestration of CO2 in rocks is likely ineffective on Mars and thus most of the CO2 Mars formed with is either inaccessible or lost making recent discussions of “terraforming” via release of CO2 from currently available reservoirs on Mars implausible.