| A Light Toned Outcrop in Arsinoes Chaos
The objective of this observation is to examine a light-toned deposit in Arsinoes Chaos. The deposit has a rough surface compared to its surroundings; some parts of the deposit are appear to have layers. This light-toned deposit may have formed as an ancient lake deposit. |
| A Scoured Surface in Kasei Valles
Our science goal for this observation is to obtain both HiRISE and Context Camera stereo pairs for flood and erosion modeling. As one of the biggest outflow channel systems on Mars, Kasei Valles was probably formed by gigantic flood events and later additionally shaped by glacial activity. | 
| “What a Desolate Place This Is”
The words of C-3PO were never more true! Only this time, we are talking about the terrain of the South Pole of Mars, where the goal of this observation is look for changes in long-monitored sites of what is called the “residual cap,” that part of the ice that survives the Martian summer. The southern cap is smaller than the northern one. Any changes here will be small. | 
| Not between Two Ferns, but Two Craters
The objective of this observation is to examine a small channel that goes from a small crater at a higher level to a larger crater at a lower level. It looks like there was a lake in the upper crater that drained through the channel to the lower level. There seems to be a deposit of material at the end of the channel. This scene is in Noachis Terra. | 
| A Crater Cluster in Chryse Planitia
Clusters like this form when an asteroid or comet impacts the surface and forms a large crater; material thrown out of that crater often forms streaks or rays containing many small craters from the impact of ejected blocks. |
