Southern Patagonia Ice Field
This grand panorama of the Southern Patagonia Ice Field was photographed by a crew member aboard the International Space Station (ISS) on a rare clear day in the southern Andes Mountains on 13 February 2014. With an area of 13,000 square kilometres (5,000 square miles), the ice field is the largest temperate ice sheet in the Southern Hemisphere. Storms that swirl into the region from the southern Pacific Ocean bring rain and snow (between 2 to 11 meters of rainfall per year), resulting in the buildup of the ice sheet.
A study of the surface topography of sixty-three glaciers-based on data from the Shuttle Radar Topography Mission-compared data from 2000 to data from studies going back to 1968. Many glacier tongues showed significant annual "retreat" of their ice fronts, a familiar signal of climate change. The study also revealed that the almost invisible (to the naked eye) losses of ice volume by glacier thinning are far more significant-4 to 10 times greater-than those caused by collapse of the ice front (calving when ice masses fall into lakes).
Scaled over the entire ice field, nearly 13.5 cubic kilometres of ice were lost each year over the study period. This number becomes more meaningful when compared with the rate in the last five years of the study (1995-2000): an average of 38.7 cubic kilometres per year. Extrapolating results from the low-altitude glacier tongues implies that high plateau ice on the spine of the Andes Mountains is thinning as well. In the decade since this study, the often-imaged Upsala Glacier has retreated 3 kilometres, as shown recently in images taken by astronauts aboard the ISS. Glacier Pio X, named for Pope Pius X, is the only large glacier in the area that is growing in length.
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Credit: NASA Earth Observatory