Craterra

Oceanus Procellarum

A Volcanic Complex Standing Above Oceanus Procellarum

Rising above northern Oceanus Procellarum, Mons Rümker forms an elevated mound containing 22 lunar domes produced by localized lava eruptions.

Feature Profile & Selenographic Data

Feature type
mons
Coordinates
40.76° N · 58.38° W
Diameter
73.25 km
IAU approval
1935/01/01 00:00:00
LAC quadrangle
LAC-23 · Rümker

Geological Chronicle

Mons Rümker is an isolated volcanic formation in the northwestern region of the Moon's near side, located in northern Oceanus Procellarum. The complex forms a broad elevated mound spanning a diameter of 73.25 kilometers and climbs to a maximum elevation of approximately 1,300 meters above the surrounding plain. The feature bears the name of German astronomer Karl Ludwig Christian Rümker.

Across the top lies a concentration of 22 lunar domes—rounded bulges that resemble shield volcanoes. These wide, circular features rise a few hundred meters with gentle slopes, and some contain a small craterlet at the peak. The domes formed as lava erupted from localized vents and cooled relatively slowly.

A perimeter scarp separates Mons Rümker from the adjacent mare plain, with plateau edges rising 900 meters in the west, 1,100 meters in the south, and 650 meters in the east. Spectroscopic observations show a uniform surface of lunar mare material, representing an estimated extruded lava volume of 1,800 cubic kilometers.

Directly northeast of Mons Rümker lies Statio Tianchuan, a young lava plain that served as the landing site of the Chang'e 5 mission.

Scientific Sources & References

Name Origin

Karl Ludwig Christian; German astronomer (1788-1862).

Interactive Lunar Surface

Explore Mons Rümker in 3D

Inspect lunar elevation data and the official selenographic position.