The crater is circular and symmetrical, with a wide interior floor. The sloping inner walls have a slightly higher albedo than the surrounding mare, but the interior floor is the same dark shade as the exterior of the crater. There is a small crater on the floor near the western rim, but otherwise no significant markings.
The mare to the south and west of Ibn Battuta contains a number of ghost crater formations, consisting of crater rims that have been submerged by lava flows and now form ring-shaped projections in the surface. These are best observed under conditions of oblique lighting, when the terminator still lies on or near the Mare Fecunditatis.
This crater was formerly designated Goclenius A before being given its current name by the IAU. It is named after the Moroccan traveller and writer Ibn Battuta.[1]
References
^"Ibn Battuta (crater)". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
Andersson, L. E.; Whitaker, E. A. (1982). NASA Catalogue of Lunar Nomenclature. NASA RP-1097.
Menzel, D. H.; Minnaert, M.; Levin, B.; Dollfus, A.; Bell, B. (1971). "Report on Lunar Nomenclature by the Working Group of Commission 17 of the IAU". Space Science Reviews. 12 (2): 136–186. Bibcode:1971SSRv...12..136M. doi:10.1007/BF00171763. S2CID122125855.