Dorsum Buckland AS15-P-9346-9348-9350-9352

Dorsum Buckland is a large

wrinkle ridge A wrinkle ridge is a type of feature commonly found on lunar maria, or basalt plains. These features are low, sinuous ridges formed on the mare surface that can extend for up to several hundred kilometers. Wrinkle ridges are tectonic features ...

at in

Mare Serenitatis Mare Serenitatis (Latin ''serēnitātis'', the "Sea of Serenity") is a lunar mare located to the east of Mare Imbrium on the Moon. Its diameter is . Geology Mare Serenitatis is located within the Serenitatis basin, which is of the Nectarian ...

on the

Moon The Moon is Earth's only natural satellite. It Orbit of the Moon, orbits around Earth at Lunar distance, an average distance of (; about 30 times Earth diameter, Earth's diameter). The Moon rotation, rotates, with a rotation period (lunar ...

, 369 km long. It was named after British geologist

William Buckland William Buckland Doctor of Divinity, DD, Royal Society, FRS (12 March 1784 – 14 August 1856) was an English theologian, geologist and paleontology, palaeontologist. His work in the early 1820s proved that Kirkdale Cave in North Yorkshire h ...

in 1976. 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.Stereo Atlas
FEATURES OF INTEREST, Montes Haemus, Mare Serenitatis, L&PI, 2000.

References

External links

LAC-42LTO-41C2 Galen
Lunar Topographic Orthophotomap (shows northwestern Dorsum Buckland)
LTO-42D1 Hornsby
Lunar Topographic Orthophotomap (shows southeastern Dorsum Buckland)
Dorsum Buckland at The Moon Wiki
a

Lunar Reconnaissance Orbiter The Lunar Reconnaissance Orbiter (LRO) is a NASA robotic spacecraft currently orbiting the Moon in an eccentric Polar orbit, polar mapping orbit. Data collected by LRO have been described as essential for planning NASA's future human and robotic ...

article Buckland Mare Serenitatis {{moon-stub