| A Landslide in Eos Chasma
This observation features a landslide formation that is relatively fresh and well-peserved, with lots of exposed bedrock. Our image footpring is located on a wall in Eos Chasma, at the eastern end of Valles Marineris. In Eos, the canyon system transitions into a region of chaos and then into major outflow channels. |
| The Cracks are Starting to Show
The objective of this observation is to determine the nature of material in Centauri Montes that shows a high density of cracks in upper plains of the region. This may be a transition between upper plains unit and another ribbed plains unit. Cetauri Montes are a group of mountains to the east of the massive Hellas impact basin. | 
| A Hummocky Surface in Kasei Valles
Kasei Valles is one of the largest outflow channels on Mars and probably formed by gigantic flood events and shaped by later glacial activity. This footprint gives us a sample of hummocky and platy regions along part of the edge. “Kasei” is the Japanese word for the planet Mars. | 
| Scarp of Ages
Scarps such as this have either active mass wasting (landslides) or the potential for current mass wasting. When this occurs, it’s likely the result of the sublimation of ice that dislodges darker subsurface material as we can see in various parts of this image footprint. We also want to to make a comparison to previous years to document new activity in scarp erosion. | 
| A Pyramidal Mound in Syrtis Major Planum
Our target is a pyramidal mound whose western slopes expose some bright-toned material in Context Camera data. To the north, there is a crater that excavated bright material from the subsurface. Are the two materials the same composition? What does that imply for the formation of this type of mound? |
