Dorsum Buckland's ridges are 200 to 300 meters high and were formed by compressional stresses near the center of the basin, possibly over buried basin structures.
- Dorsum Buckland, Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN)
- LTO-41C2 Galen, Lunar Topographic Orthophotomap (shows northwestern Dorsum Buckland)
- LTO-42D1 Hornsby, Lunar Topographic Orthophotomap (shows southeastern Dorsum Buckland)
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