High-resolution images of the south polar residual cap of Mars acquired in
1999 and 2001 show changes in the configuration of pits, intervening ridges
, and isolated mounds. Escarpments have retreated 1 to 3 meters in 1 martia
n year, changes that are an order of magnitude larger than can be explained
by the sublimation of water ice, but close to what is expected for sublima
tion of carbon dioxide ice. These observations support a 35-year-old conjec
ture that Mars has a large surface reservoir of solid carbon dioxide. The e
rosion implies that this reservoir is not in equilibrium with the present e
nvironment and that global climate change is occurring on Mars.