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In addition to mountains, valleys, and impact craters, the following surface features have received names in the Lunar nomenclature, many of them named after a nearby crater or mountain. The listed diameter for these features is the longest dimension that contains the entire geological formation.
The modern system of lunar nomenclature was introduced in 1651 by Giovanni Battista Riccioli. [1] Riccioli's map of the Moon was drawn by Francesco Maria Grimaldi, who has a crater named after him. A related set of features are the Lunar lacus / ˈ l eɪ k ə s / (singular also lacus, Latin for "lake"), [a] which are smaller basaltic plains of ...
This is a list of named lunar craters. The large majority of these features are impact craters. The crater nomenclature is governed by the International Astronomical Union, and this listing only includes features that are officially recognized by that scientific society.
The ages of the mare basalts have been determined both by direct radiometric dating and by the technique of crater counting.The radiometric ages range from about 3.16 to 4.2 billion years old (Ga), [4] whereas the youngest ages determined from crater counting are about 1.2 Ga. [5] Updated measurements of samples collected by the Chang’e-5 mission show that some lunar basalts could be as ...
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 created after the lava cooled and solidified. They frequently outline ring structures buried within the ...
The largest lunar feature in the vicinity of Shioli is the Sea of Nectar, a basin 210 miles (339 kilometers) in diameter that is one of the oldest on the near side of the moon, the hemisphere that ...
List of lunar craters named for space explorers; List of lunar features; A. Abbe (crater) Abbot (crater) Abel (crater) Abenezra (crater) Abetti (crater) Abul Wáfa ...
Lunar naming conventions specify that lunar maria are named in Latin after 'weather and other abstract concepts', with a few exceptions. [7] Mare Moscoviense was discovered in 1959, when the first images of the far side were returned by the Soviet spacecraft Luna 3 .