A lovely combination of layered mare basalt, granular flow, and talus. The top of the image is down-slope. LROC NAC image M170694505L, image width is 735 m, pixel scale of 0.49 m/px [NASA/GSFC/Arizona State University].
Inside the southern rim of the crater Pytheas (20.55°N, -20.6°E) is a great combination of layered mare basalt, granular flow, and talus. In the bottom left hand corner of the Featured Image you can see the details of erosion where granular material fell away from the rest of the surface near the rim. The high reflectance (bright) tendril of material flowed in a narrow band over the layers of lower reflectance (darker) mare basalt, then, after clearing the basalt layers, finally spread into a wide cone of talus. Talus cones are common on the Earth, with some stunningexamples that may rival the Moon's beauty. On the Moon, talus deposits are created entirely by gravity, but on the Earth wind and water play a role in their formation.
LROC WAC 100 m/px context image of Pytheas, a 19.6 km diameter crater [NASA/GSFC/Arizona State University].
Pytheas was a Greek geographer and explorer (circa 325 BC) from a Greek colony in what is now Marseilles, France. He is especially important to lunar geology since his report on Earth's ocean tides was probably the first to associate the tides with the phases of the Moon.