Public domain
Martian Morse Code
From the collection of NASA Image and Video Library. Free to download, adapt and use — no permission needed.
About this work
These dark dunes are influenced by local topography. The shape and orientation of dunes can usually tell us about wind direction, but in this image, the dune-forms are very complex, so it's difficult to know the wind direction. However, a circular depression (probably an old and infilled impact crater) has limited the amount of sand available for dune formation and influenced local winds. As a result, the dunes here form distinct dots and dashes.
NASA Image and Video Library’s own descriptionCredit lineMartian Morse Code. NASA/JPL, 2016-06-29. Public domain. ID: PIA20735.