The team led by the U.S. Geological Survey's Colin Dundas in Flagstaff, Arizona, measured 151 of these dark lines at 10 sites. Most of them end with slopes between 28 degrees and 35 degrees, a match for active sand dunes on both Mars and Earth, according to the researchers. A thin layer of dust on top that shifts and sometimes brightens the surface might help explain why these streaks seem to occur in the Martian summertime and then disappear, only to reappear the next year.