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
Dark Striations near Holmes Crater
Context Camera imagery reveals dark streaks extending east of minor crater rims within and around Holmes Crater.
Exposed Fractured Bedrock in the Central Pit of a Crater
This HiRISE image shows the central pit feature of an approximately 20-kilometer diameter complex crater in located at 304.480 degrees east, -11.860 degrees south, just north of the Valles Marineris.
An Impact Crater within Nanedi Valles
With this image, we can cross-dating the relative age of the impact with that of the valley system, as well as learning more about the fluvial and morphology characteristics of area.
Impact Craters as Windows to What Lies Beneath
Impact craters are common on all solar system bodies. They offer many clues to scientists regarding the geologic history of a planetary surface, particularly regarding its age, evolution with time, and composition.