Jehan (crater)
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Mons Vinogradov is a rugged massif that is located on the
lunar mare The lunar maria ( ; mare ) are large, dark, basaltic plains on Earth's Moon, formed by lava flowing into ancient impact basins. They are less reflective than the "highlands" as a result of their iron-rich composition, and hence appear dark to ...
where
Oceanus Procellarum Oceanus Procellarum ( ; from ) is a vast lunar mare on the western edge of the near side of the Moon. It is the only one of the lunar maria to be called an "Oceanus" (ocean), due to its size: Oceanus Procellarum is the largest of the maria ("s ...
to the southwest joins
Mare Imbrium Mare Imbrium (Latin ''imbrium'', the "Sea of Showers" or "Sea of Rains") is a vast lunar mare, lava plain within the Imbrium Basin on the Moon and is one of the larger craters in the Solar System. The Imbrium Basin formed from the collision ...
to the east. There are three primary peaks in this formation, which rise to altitudes of 1.0–1.4 km above the surface (3,281-4593 ft). To the east of this rise is the crater
Euler Leonhard Euler ( ; ; ; 15 April 170718 September 1783) was a Swiss polymath who was active as a mathematician, physicist, astronomer, logician, geographer, and engineer. He founded the studies of graph theory and topology and made influential ...
, and to the southeast is an area of rugged ground that reaches the
Montes Carpatus Montes Carpatus is a mountain range that forms the southern edge of the Mare Imbrium on the Moon. The selenographic coordinates of this range are 14.5° N, 24.4° W, and the formation has an overall diameter of . They were named by astronomer ...
range. The Carpatus mountain range forms the southwest boundary of the Mare Imbrium. The selenographic
coordinate In geometry, a coordinate system is a system that uses one or more numbers, or coordinates, to uniquely determine and standardize the position of the points or other geometric elements on a manifold such as Euclidean space. The coordinates are ...
of Mons Vinogradov is 22.4 N, 32.4 W, and it has a maximum diameter of 25 km at the base. It was named after Soviet geochemist Aleksandr P. Vinogradov. This mountain was formerly named Euler Beta (β), or Mons Euler. In the rugged ground just to the southeast of this mountain is a set of
crater A crater is a landform consisting of a hole or depression (geology), depression on a planetary surface, usually caused either by an object hitting the surface, or by geological activity on the planet. A crater has classically been described ...
s that have been assigned names by the
IAU The International Astronomical Union (IAU; , UAI) is an international non-governmental organization (INGO) with the objective of advancing astronomy in all aspects, including promoting astronomical research, outreach, education, and developmen ...
. These are listed in the table below. ;Notes:


See also

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List of mountains on the Moon This is a list of mountains on the Moon (with a scope including all named ''mons'' and ''montes'', planetary science jargon terms roughly equivalent to 'isolated mountain'/'massif' and 'mountain range'). Caveats * This list is not comprehensiv ...


References

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External links

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LTO-39C2 Mons Vinogradov
— L&PI
topographic map In modern mapping, a topographic map or topographic sheet is a type of map characterized by large- scale detail and quantitative representation of relief features, usually using contour lines (connecting points of equal elevation), but histori ...
of mountain and vicinity. {{Craters on the Moon: A–B Vinogradov, Mons