North–south geological differences between the residual polar caps on Mars

P. C. Thomas (), M. C. Malin, K. S. Edgett, M. H. Carr, W. K. Hartmann, A. P. Ingersoll, P. B. James, L. A. Soderblom, J. Veverka and R. Sullivan
Additional contact information
P. C. Thomas: Center for Radiophysics and Space Research, Cornell University
M. C. Malin: Malin Space Science Systems
K. S. Edgett: Malin Space Science Systems
M. H. Carr: US Geological Survey
W. K. Hartmann: Planetary Science Institute
A. P. Ingersoll: California Institute of Technology
P. B. James: University of Toledo
L. A. Soderblom: US Geological Survey
J. Veverka: Center for Radiophysics and Space Research, Cornell University
R. Sullivan: Center for Radiophysics and Space Research, Cornell University

Nature, 2000, vol. 404, issue 6774, 161-164

Abstract: Abstract Polar processes can be sensitive indicators of global climate, and the geological features associated with polar ice caps can therefore indicate evolution of climate with time. The polar regions on Mars have distinctive morphologic and climatologic features: thick layered deposits, seasonal CO2 frost caps extending to mid latitudes, and near-polar residual frost deposits that survive the summer1,2. The relationship of the seasonal and residual frost caps to the layered deposits has been poorly constrained3,4, mainly by the limited spatial resolution of the available data. In particular, it has not been known if the residual caps represent simple thin frost cover or substantial geologic features. Here we show that the residual cap on the south pole is a distinct geologic unit with striking collapse and erosional topography; this is very different from the residual cap on the north pole, which grades into the underlying layered materials. These findings indicate that the differences between the caps are substantial (rather than reflecting short-lived differences in frost cover), and so support the idea of long-term asymmetry in the polar climates of Mars.

Date: 2000
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DOI: 10.1038/35004528

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