Even without a 3D picture, we can easily see that the crater’s walls are fairly steep. Phlegra Montes are a series of mountain ranges, massifs and knobby terrain in the northern lowlands of Mars.
Dark
Light
The objective of this observation is to examine at least two layers that are exposed in the wall of an impact crater that’s less than 5 km across.
Image: NASA/JPL/University of Arizona https://www.uahirise.org/hipod/ESP_065243_2065
Related Posts
Fresh Craters in the Northern Mid-Latitudes
These two impact craters near Deuteronilus Mensae dominate the center of this observation, also visible in Context Camera images.
Layers in Meridiani Planum
Also visible in a Context Camera image, our high resolution picture shows layers exposed where the crater ejecta has been eroded.
A Tale of Collapse Terrain
North of Ganges Chasma lies Orson Welles Crater, whose floor contains broken up blocks we call chaotic terrain and which is the source for the major outflow channel Shalbatana Vallis.
Sunken and Pitted Ejecta
The objective of this observation was to examine the edge of impact ejecta from a crater to the north-west of this area (north is up, west is to the left).