Analysing the consistency of martian methane observations by investigation of global methane transport

These results show that the spatial and temporal variability of methane on Mars implied by observations could be explained by advection from localised time-dependent sources alongside a currently unknown methane sink. Evidence is presented that a fast trapping mechanism for methane is required. Trapping by a zeolite structure in dust particles is a suggested candidate warranting further investigation; this could provide a fast acting sink as required by this reconstruction.