Craterra

LUNAR ATLAS · BASIN RIM OROGENY

Montes Apenninus: The Crown Rampart of Mare Imbrium

Stretching 600 kilometers along the southeastern rim of Mare Imbrium, the Apennine range rises up to 5.4 kilometers above the volcanic plains, exposing ancient crust excavated during the basin impact.

Feature Profile & Selenographic Data

Feature type
mons
Coordinates
19.9° N · 0.0° E
Diameter
600 km
IAU approval
1961/01/01 00:00:00
LAC quadrangle
LAC-41 · Montes Apenninus
Geological Period
Early Imbrian

Geological Chronicle

The Montes Apenninus form a continuous 600-kilometer mountain arc along the southeastern rim of the Mare Imbrium basin. The range begins west of the crater Eratosthenes and extends northeast to Promontorium Fresnel near the entrance to Mare Serenitatis. The Apennines formed during the colossal Imbrium impact roughly 3.85 billion years ago, when the collision fractured the lunar lithosphere and thrust massive crustal fault blocks upward in minutes. The resulting arc constitutes the uplifted southeastern rim of the multi-ring Imbrium impact basin.

The topography of the range is markedly asymmetric. Facing northwest toward the basaltic plains of Mare Imbrium, the mountains drop in steep escarpments that rise higher above their base than the Himalayas rise above the plains of northern India. To the southeast, the terrain transitions into gentler backslopes blanketed by thick sheets of impact debris known as the Fra Mauro Formation. Near the center of the chain, Mons Huygens reaches a relief of 5.4 kilometers above the mare floor, making it the tallest mountain mass on the lunar near side.

Other prominent peaks include Mons Bradley at 4.2 kilometers, Mons Ampere at 3.0 kilometers, and Mons Wolff at 3.5 kilometers. Near the northeastern terminus, Mons Hadley Delta rises 3.5 kilometers above the volcanic plain of Palus Putredinis, while adjacent Mons Hadley towers 4.2 kilometers over the plain. The steep frontal scarps expose ancient, stratified crust that was deeply buried before the basin excavation.

In July 1971, NASA targeted the Apennine front for the Apollo 15 mission, the first expedition equipped with the Lunar Roving Vehicle. Astronauts David Scott and James Irwin landed their lunar module Falcon on the plain between Mons Hadley and Rima Hadley, a 1.2-kilometer-wide, 370-meter-deep volcanic channel. While exploring the lower slopes of Mons Hadley Delta, Scott and Irwin recovered sample 15415, the celebrated Genesis Rock, a piece of 4.1-billion-year-old anorthosite that confirmed the existence of an early magma ocean in lunar history.

Chronology & Exploration

  1. ≈ 3.85 Ga Imbrium Basin Impact

    A protoplanetary collision excavates the Imbrium basin, thrusting crustal fault blocks upward to form the 600-kilometer Apennine mountain rim.

  2. 1647 Hevelius Cartographic Designation

    Polish astronomer Johannes Hevelius maps the lunar near side in Selenographia and names the range after the Apennine Mountains of Italy.

  3. 1971 Apollo 15 Exploration

    David Scott and James Irwin land near Mons Hadley, deploy the first Lunar Roving Vehicle, and sample the Genesis Rock at the base of the Apennine Front.

  4. 2009 to Present LRO High-Resolution Topography

    The Lunar Reconnaissance Orbiter uses LOLA laser altimetry and LROC narrow-angle imaging to map the 5.4-kilometer relief of Mons Huygens and the stratigraphy of the Apennine escarpment.

Scientific Sources & References

Name Origin

Named from terrestrial Apennines.

Interactive Lunar Surface

Explore Montes Apenninus in 3D

Inspect lunar elevation data and the official selenographic position.