Image Credit: NASA/JPL/ASU
|
Context image credit: NASA/JPL/MOLA
View on map Detailed information on this image is available at the
THEMIS Data Releases website.
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
Arkhangelsky crater is just to the northeast of the giant Argyre impact basin in the southern hemisphere of Mars. This THEMIS visible image shows the floor of this crater with a few dark barchan sand dunes. Dunes form when wind blows sand across a surface. The barchan dunes shown here form when there isn't a lot of sand to start with. If there were, other dune forms would be visible.
|
||||||||||||