I. Introduction
Lunar rockfalls and their traces have been investigated by researchers since the Lunar Orbiter Program sent back the first high-resolution images of the lunar surface in 1966 [1]–[7]. In addition to images taken from orbital platforms, astronauts Eugene Cernan and Harrison Schmitt were able to directly sample and photograph boulder and track remnants of rockfalls in the Taurus–Littrow valley during the Apollo 17 mission in 1972 [8]. Since the arrival of NASA’s Lunar Reconnaissance Orbiter (LRO) in orbit around the moon in 2009 [9], a growing repository of high-resolution images taken by the LRO’s narrow angle camera (NAC) is available that enables the studies of geomorphological processes and small-scale features such as rockfalls in unprecedented detail. Various investigations use NAC imagery to identify and study lunar rockfalls as a tool to, e.g., estimate local seismic activity and shaking intensity in Schrödinger Crater [10] or to investigate the topographic evolution of the moon [11]. Besides that these studies show that rockfalls are a widespread phenomenon and occur in various geologic settings.