Seasonal polar carbon dioxide frost on Mars: CO₂ mass and columnar thickness distribution

Abstract

Conclusions are drawn about the column density (g/cm 2 ), spatial extent, and mass of the seasonal carbon dioxide frost on the poles of Mars as a function of time utilizing data from the 2001 Mars Odyssey Gamma Ray Spectrometer (GRS). Quantification of these CO 2 values is achieved by observing attenuation effects of the surface‐emitted hydrogen gamma ray flux as the frost condenses and sublimates in a seasonal exchange of CO 2 between the ground and the atmosphere. Columnar thickness and mass results are discussed and plotted for latitudes including ±60° and poleward. GRS observations are compared to predictions from the NASA Ames Research Center General Circulation Model and to similar experimental results from the Mars Odyssey High Energy Neutron Detector and Neutron Spectrometer. Models for north and south polar atmosphere and regolith distributions are incorporated, and our results indicate that the assumption of a 100% H 2 O‐ice residual cap underlying the seasonal frost in the north is accurate. The GRS CO 2 frost observations are in good agreement with the other studies mentioned, in particular for the timing of the beginning of frost deposition to the complete sublimation of surface CO 2 back into the atmosphere. The total amount of condensed carbon dioxide mass seen by the GRS is on the order of 6.0 × 10 15 kg and verifies previous reports that nearly 25% of the Martian CO 2 reservoir participates in the ground‐atmosphere exchange cycle.