Carbon dioxide as a geomorphic agent on Mars

Project_Logo Project title: Carbon dioxide as a geomorphic agent on Mars

Funded by: Mars Fundamental Research Program, NASA and Trinity College Dublin.

Research team: Professor Mary Bourke (TCD); Professor Jim McElwaine (Durham); Dr. Candice Hansen, (Planetary Science Institute); Dr. Serina Diniega (JPL); Ms Lauren McKeown (Postgraduate, TCD), Dr Joanna Nield (University of Southhampton), Dr Susan Conway, (Open University).

Duration: 2014-2017


Project Summary:

Sublimation of Mars’ seasonal CO2 ice cap causes geomorphologic changes on the surface of Mars in today’s climate. There have been many elegant hypotheses about how this works, and circumstantial evidence to support these hypotheses, but there is no quantitative data to assess CO2-sublimation-driven processes. The aim of this proposal is to combine data from lab experiments with theoretical models and field tests to quantify the modification of a sandy surface resulting from the levitation and sublimation of CO2 ice on or buried within that surface. We will test and observe the interaction of CO2 ice with granular material in a controlled environment in the lab under both Earth and Mars conditions. We aim to provide clear quantitative measurements of CO2 levitation and sublimation as it interacts with the surface and subsurface. Field experiments with dry ice on dunes will test scenarios in more natural environments and allow changes in experiment scale. The model will be carefully developed to allow us to extrapolate our results from Earth to Mars and from lab to field. Data generated in the lab and in the field will be folded back into the model to refine its accuracy and precision. This combined approach with lab, field, and numerical facets will allow us to estimate erosion rates for furrows on dunes, formation of linear gullies on dunes, and evaluate the effect of particle size and cohesion on erosion of araneiform terrain, just to list a few examples. All surfaces on Mars covered seasonally with CO2 ice can be examined within this framework.

 Seasonal processes involving CO2 ice on Mars have no Earth-analog. Our approach will be the first to quantify the relative efficacy of pressurized CO2 gas as an agent of erosion and to document the resultant surface changes under laboratory and field conditions. Our analyses will contribute to NASA’s broad goal of increasing the scientific understanding of geologic processes on planetary surfaces.

Project abstracts and Publications:

Diniega, S., Hansen, C.J., McElwaine, J.N., Hugenholtz, C.H., Dundas, C.M., McEwen, A.S., Bourke, M.C. (2013) A new dry hypothesis for the formation of Martian linear gullies. Icarus. Vol. 225, 1, p. 526-537. Hansen, C. J., Byrne, S., Portyankina, S., Bourke, M.C.,

Dundas, C., McEwen, A., Mellon, M., Pommerol, A., and Thomas, N.,(2013), Observations of the Northern Seasonal Polar Cap on Mars I. Spring Sublimation Activity and Processes: Icarus, Vol. 225, 2, p 881-897,

Hansen, C., Bourke, M.C, Bridges, N.T., Byrne, S., Colon, C., Diniega, S., Dundas, C.M., Herkenhoff, K., McEwen, A., Mellon, M.T., Portyankina, G. and Thomas, N. (2011) Seasonal Erosion and Restoration of Mars’ Northern Polar Dunes. Science, 331, 575,  DOI: 10.1126/science.1197636. PDF

Carbon dioxide ice-covered dunes in the North Pole of Mars. the dark areas are locations where the ice has sublimated.

Carbon dioxide ice-covered dunes in the North Pole of Mars. The dark areas are locations where the ice has sublimated.

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