This observation can give us some insight on local mass wasting processes (like landslides) as well as details about the stratigraphy of the terrain. Additionally, disturbances to dark sands may characterize windblown processes.
Dark
Light
Context Camera imagery reveals dark streaks extending east of minor crater rims within and around Holmes Crater.
Image: NASA/JPL/University of Arizona https://www.uahirise.org/hipod/ESP_055977_1055
Related Posts
Possible Impact Melt in Terra Sabaea
Nighttime and daytime infrared images from THEMIS suggest a consolidated deposit in the floor of this ancient crater in Terra Sabaea, potentially with some bedrock exposure.
Layers in a Crater
Located to the north of Cassini Crater, the objective of this observation is to confirm the presence of…
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.
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).