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Dorsum Buckland : ウィキペディア英語版 | Dorsum Buckland Dorsum Buckland is a large wrinkle ridge at in Mare Serenitatis on the Moon, 380 km long. It is named after British Geologist William Buckland. The feature was named by the IAU in 1976.〔(Dorsum Buckland ), Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN)〕 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.〔http://www.lpi.usra.edu/resources/stereo_atlas/HTDOCS/LSER-B3.HTM〕 ==External Links==
*(LAC-42 )
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