The Pits
Jet Propulsion Laboratory https://www.jpl.nasa.gov/ March 8, 2006
8 March 2006
This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows a portion of a pit chain on the lower, northern flank of the giant martian volcano, Arsia Mons. Pits such as these commonly form as a result of collapse of surface materials into a subsurface void, possibly along a fault or into an old lava tube. The layered material, exposed near the top of several of the pits, is shedding house-sized boulders which can be seen resting on the sloping sidewalls and floors of many of the pits.
Location near: 6.7°S, 120.1°W
Image width: ~3 km (~1.9 mi)
Illumination from: lower left
Season: Southern Summer