The spring-summer recession of the south polar cap of Mars in 1999-2000 has
been investigated using the wide-angle cameras of the Mars Orbiter Camera
experiment on Mars Global Surveyor. The 1999-2000 regression closely resemb
les the recession observed by Viking orbiters in 1977. Although the rates o
f recession are quite similar, the current recession was slightly ahead of
that in 1977 throughout spring. The rapid development of dark terrain, dubb
ed "cryptic terrain" by Hugh Kieffer, in one sector of the south cap betwee
n L-S = 198 degrees and 223 degrees is documented. The emergence and separa
tion of the Mountains of Mitchel has also been recorded in detail, culminat
ing with its complete disappearance at solstice. The 2000 residual cap is a
lmost identical to that in 1977; this observation does not resolve the myst
ery of the very different appearance of the residual cap in 1972. The albed
os in the residual cap region and in bright, seasonal frost increase rapidl
y to high values at around solstice and then level out until the seasonal f
rost disappears. Observations of more Martian years will be needed to const
rain the amount of interannual variability and its relation to other phenom
ena such as dust storms.