Mons Rümker and the Moon's Volcanic Past

Mons Rümker in its entirety is shown with the surrounding mare plains around it. The volcanic domes shown in subsequent images are located near the bottom.
NAC regional mosaic composed of 10 images showing Mons Rümker and the surrounding mare surface. Images acquired between 2012-06-03 to 2016-04-21. Image width is 299 kilometers, centered at 40.80°N, 301.43°E [NASA/GSFC/Arizona State University].

 

Located in the northern Oceanus Procellarum ("Ocean of Storms") on the lunar nearside, the Rümker region hosts multiple volcanic complexes. One of these complexes, Mons Rümker, rises to 1,300 meters above the surrounding mare surface and provides a fascinating glimpse into lunar volcanic history. Spanning an area of about 4,000 square kilometers, Mons Rümker features a diverse terrain of domes, sinuous rilles, ridges, and lava flows, making it a valuable site for studying volcanic landforms. The oldest section, characterized by rough, lineated terrain along its northern edge, is theorized to have formed from ejecta of the Iridum impact approximately 3.8 to 3.7 billion years ago. Subsequently, basaltic volcanism further shaped Mons Rümker around 3.7 to 3.5 billion years ago. In this featured image, you can see the volcanic domes that were once active, now lying dormant after billions of years.

Five volcanic domes are outlined in the center of the image, there are three steep-sided domes towards the left and two shallow domes towards the right. The southern edge of Mons Rümker is also visible towards the bottom.
A zoomed-in view of the mosaic focused on the southwest corner of Mons Rümker with approximate outlines of volcanic domes overlaid. The domes outlined in blue are steep-sided, and the domes outlined in white are shallow. Image width is 38 kilometers, centered at 40.15°N, 301.49°E. NAC_ROI_RUMKER__LOB_E406N3014 [NASA/GSFC/Arizona State University].

These domes likely formed from slowly erupting basaltic magma, which created small shield volcanoes on the surface. Researchers categorize them into two types: steep-sided domes and shallow domes. Steep-sided domes have flank slopes steeper than 5 degrees and are relatively tall, while shallow domes are shorter (less than 200 meters) and have gentler slopes. The majority of Mons Rümker's domes are located on the complex's western side, with a heavy concentration in the southwest.

Close-up view of a steep-sided dome from the previous image. The possible summit pit is in the center, and the slope map is shaded from blue to red, with red indicating higher slopes. The slopes of the dome's sides have a yellow-orange color compared to the dark blue of the surrounding terrain, indicating higher slopes.
Further zoomed-in view of the mosaic showing a steep-sided dome in the southwest of Mons Rümker. NAC image is on the left and slope map is on the right. The large crater the arrow is pointing to may be a summit pit, which would be indicative of past volcanic activity. Image width is 9.4 kilometers, centered at 40.06°N, 301.36°E. NAC_DTM_RUMKERDOME [NASA/GSFC/Arizona State University].

Mons Rümker was initially considered as a landing site for China's Chang'e 5 lunar lander, due to its evidence of ancient volcanism and varied impact ejecta. However, the lander ultimately touched down at an alternate site about 170 kilometers northeast of Mons Rümker in December 2020. The mission returned approximately 1.7 kilograms of lunar samples to Earth, providing researchers with valuable insights into the geologic history of the northern Oceanus Procellarum. The mare unit from which the sample was collected was determined to be about 1.5 billion years old—significantly younger than the estimated age of Mons Rümker. With its unique volcanic history still unexplored on the ground, Mons Rümker remains a compelling target for future crewed or robotic lunar missions.

Explore the entire Mons Rümker mosaic with the Zoomify below!

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Published by Steven Nystrom on 12 April 2025