72 Snow on Mars
Planet Mars at a Glance
Characteristic — Current State
- Impact Craters — Yes; a very large impact crater Borealis Basin (largest known in the Solar System), 6,600 miles across
- Tectonic Craters — Yes, still active?
- Volcanoes — Yes, not active; One of the largest volcanoes in the Solar System; Olympus Mons
- Atmosphere — Carbon Dioxide (CO 2 ), Low Pressure, Clouds, Snow, Dust devils, Dust storms, Slight traces of Methane (CH 4 )
- Water — Both liquid & water ice
- Subsurface liquid water aquifers?
- 2% water in soil
- Erosion — Yes
- Dunes — Yes
- Polar Caps — Yes
- Satellites — Two; Deimos and Phobos
- Life — Unknown; we are actively searching for life
Public Domain | Image courtesy of NASA.
![Image of Ius Chasma Floor.](http://cel.fscj.edu/LUMENS/ast-1002-package/img/figure-94-iusChasmaFloor.jpg)
![Image of Sand Dunes on Mars: Endurance Craters are dramatic dune fields on the crater floor. Dune crests have accumulated more dust than the flanks of the dunes and the flat surfaces between the dunes.](http://cel.fscj.edu/LUMENS/ast-1002-package/img/figure-95-sandDunes.jpg)
![Image of Martian Volcano Olympus Mons.](http://cel.fscj.edu/LUMENS/ast-1002-package/img/figure-96-martianVolcanoOlympusMons.jpg)
![Image of The surface of Mars.](http://cel.fscj.edu/LUMENS/ast-1002-package/img/figure-97-surfaceMars.jpg)