Dorsum Buckland
Dorsum Buckland is a large wrinkle ridge at 20°24′N 12°48′E / 20.4°N 12.8°E in Mare Serenitatis on the Moon, 369 km long. It was named after British geologist William Buckland in 1976.[1]
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.[2]
References[]
- ^ Dorsum Buckland, Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN)
- ^ http://www.lpi.usra.edu/resources/stereo_atlas/HTDOCS/LSER-B3.HTM
External links[]
Wikimedia Commons has media related to Dorsum Buckland. |
- LAC-42
- LTO-41C2 Galen, Lunar Topographic Orthophotomap (shows northwestern Dorsum Buckland)
- LTO-42D1 Hornsby, Lunar Topographic Orthophotomap (shows southeastern Dorsum Buckland)
Categories:
- LQ12 quadrangle
- Ridges on the Moon
- Mare Serenitatis
- Moon stubs