Mons Rümker
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| Mons Rümker | |
|---|---|
 View of Mons Rümker from Apollo 15 |
|
| Elevation | 1,100 m |
| Location | the Moon |
| Coordinates | |
| Type | Lunar dome |
| Listing | Lunar mountains |
| Translation | Karl L. C. Rümker (Latin) |
Mons Rümker is an isolated volcanic formation that is located in the northwest part of the Moon's near side, at selenographic coordinates 40.8° N, 58.1° W. The feature forms a large, elevated mound in the northern part of the Oceanus Procellarum lunar mare. The mound has a diameter of 70 km, and climbs to a maximum elevation of about 1,100 m above the surrounding plain. It was named for Karl L. C. Rümker.
The Mons Rümker has a concentration of 30.[1] lunar domes—rounded bulges across the top, some of which contain a small craterlet at the peak. These are wide, circular features with a gentle slope rising in elevation a few hundred meters to the mid-point. Lunar domes are the result of lava erupting from localized vents followed by relatively slow cooling.
Mons Rümker is surrounded by a scarp that separates it from the adjacent mare. The plateau rises to an altitude of 900 m in the west, 1,100 m in the south and 650 m in the east. The surface of Mons Rümker is relatively uniform, with a strong spectroscopic signature of lunar mare material. The estimated volume of lava used to create this feature is 1,800 km3.[1]
[edit] See also
[edit] References
- ^ a b Wöhler, C.; Lena, R.; Pau, K. C. (March 12-16, 2007). "The Lunar Dome Complex Mons Rümker: Morphometry, Rheology, and Mode of Emplacement". Proceedings Lunar and Planetary Science XXXVIII, League City, Texas: Dordrecht, D. Reidel Publishing Co. Retrieved on 2007-08-28.
