0400 GMT August 20, 2017
Using images captured by NASA's Dawn spacecraft, researchers at the Georgia Institute of Technology identified three types of landslides on Ceres — the solar system's only asteroid classified as a dwarf planet, UPI wrote.
Type I landslides are found among Ceres' high-altitude terrain. They're large, round and resemble icy landslides found in the Arctic.
Type II landslides are thinner, longer and populate Ceres' mid-latitudes. They're the most common type of landslide found on Ceres.
Type III are found along the edges of low-altitude impact creators. They're triggered when impacts melt subsurface ice.
Lead researcher Britney Schmidt, an assistant professor at Georgia Tech's School of Earth and Atmospheric Sciences, said, "Landslides cover more area in the poles than at the equator, but most surface processes generally don't care about latitude.
"That's one reason why we think it's ice affecting the flow processes. There's no other good way to explain why the poles have huge, thick landslides; mid-latitudes have a mixture of sheeted and thick landslides; and low latitudes have just a few."
Researchers found a surprisingly large number of landslides on Ceres' surface.
Nearly a third of all surveyed craters wider than six miles (9.6km) were accompanied by a landslide. The abundance of landslides suggested ice makes up between 10 and 50 percent of Ceres' upper layers.
Researchers said their revelations — detailed in the journal Nature Geoscience — were made possible by comparing Ceres' geologic features to those found on Earth.
Schmidt said, "It's just kind of fun that we see features on this small planet that remind us of those on the big planets, like Earth and Mars. It seems more and more that Ceres is our innermost icy world."