A bolide impacting into the sloping wall of Harvey crater formed an oval, rather than circular crater. NAC M191567120, image width 1.32 km [NASA/GSFC/Arizona State University].

Impact melt, boulders, and mass wasting - oh my! NAC M190007628LR, image width 1 km [NASA/GSFC/Arizona State University].

High-reflectance ejecta and low-reflectance impact melt streamers surround this fresh impact crater. NAC M189994606LR, image width 2.25 km [NASA/GSFC/Arizona State University].

Fresh impact crater morphology can be messy! NAC M189978900LR, image width 708 m [NASA/GSFC/Arizona State University].

Blocks litter the interior floor of an impact crater. NAC M187357438LR, image width 1.81 km [NASA/GSFC/Arizona State University].

Boulders >1 m across, and a few trails, surround the base of a mountain in the Schrödinger central peak ring. Boulder in lower left is ~55 m across, NAC M187340587LR, image width 732 m, mountain base is beyond the frame to the lower left [NASA/GSFC/Arizona State University].

Evidence of erosion and mass-wasting abound in lunar craters! Crater rim at the bottom of the image, crater floor at upper left, NAC M18731958LR, image width ~810 m [NASA/GSFC/Arizona State University].

A lobate scarp cuts across and deforms an ancient impact scar on the floor of Seares crater. NAC M187315000LR, image width 1.95 km [NASA/GSFC/Arizona State University].

Faulting of a crater rim. Downhill to lower right, NAC M187307653, image width is ~1.9 km [NASA/GSFC/Arizona State University].

Unlike some melt ponds, this melt pond does not look very smooth! NAC M182116507LR, image width 910 m [NASA/GSFC/Arizona State University].