Craterra

LUNAR ATLAS · MARE IMBRIUM

Archimedes: The Flooded Giant of Mare Imbrium

Spanning 83 kilometers across the eastern Imbrium plains, Archimedes is the largest crater within the basin floor, where volcanic lavas buried its central peak beneath a level basalt plain.

Feature Profile & Selenographic Data

Feature type
crater
Coordinates
29.7° N · 4.0° W
Diameter
83 km
Depth
2.1 km
IAU approval
1935/01/01 00:00:00
LAC quadrangle
LAC-41 · Montes Apenninus
Age
≈ 3.85 Ga
Geological Period
Upper Imbrian

Geological Chronicle

Positioned in the eastern reaches of Mare Imbrium, Archimedes is the largest impact crater on the basin floor, measuring 83 kilometers across. Its terraced rim rises up to 2.1 kilometers above the surrounding basalt plains, with a prominent triangular promontory jutting 30 kilometers from its southeastern wall. Archimedes lacks a primary ray system of its own. Instead, faint streaks of bright material crossing its floor originate from the nearby Copernican impact that created the crater Autolycus.

The crater is a primary stratigraphic benchmark for the Upper Imbrian period. Its impact occurred after the excavation of the Imbrium basin roughly 3.85 billion years ago, but before the regional volcanic floods ceased. Subsequent eruptions of basaltic lava welled up through crustal fractures, submerging the interior. This inundation drowned the central peak and left a flat floor spanning more than 5,000 square kilometers, broken only by scattered micro-impacts.

Archimedes sits at the junction of several distinct geological formations. To the south rise the rugged highlands of Montes Archimedes, while the 150-kilometer rille network of Rimae Archimedes cuts through the lava plains of Palus Putredinis to the southeast. To the north-northwest, the isolated peaks of Montes Spitzbergen project through the mare, representing remnants of the Imbrium basin inner ring. To the east and northeast lie the craters Autolycus and Aristillus, enclosing the embayed mare region known as Sinus Lunicus.

The crater has a recorded place in lunar cartography and spaceflight history. Italian astronomer Giovanni Battista Riccioli named the crater in 1651 for the ancient Greek mathematician and engineer Archimedes of Syracuse, superseding earlier map names by Michael van Langren and Johannes Hevelius. On September 13, 1959, the Soviet probe Luna 2 crashed onto the plains between Archimedes and Autolycus, becoming the first human-made object to reach the lunar surface. Later orbital missions, including Apollo 15 and the Lunar Reconnaissance Orbiter, mapped the crater ramparts and surrounding volcanic rilles in high resolution.

Chronology & Exploration

  1. ≈ 3.85 Ga Upper Imbrian Impact

    An asteroid impact excavates an 83-kilometer crater on the floor of the newly formed Imbrium basin.

  2. ≈ 3.68 Ga Mare Basalt Inundation

    Volcanic eruptions flood the crater interior with basaltic lava, burying the central peak under a flat plain.

  3. 1651 Riccioli Nomenclature

    Giovanni Battista Riccioli names the crater after Greek mathematician Archimedes of Syracuse.

  4. 1959 Luna 2 Impact

    The Soviet Luna 2 probe crashes between Archimedes and Autolycus on September 13, becoming the first craft to make contact with the lunar surface.

  5. 1971 Apollo 15 Orbital Mapping

    Apollo 15 orbital cameras photograph the terraced walls of Archimedes and the adjacent Rimae Archimedes rilles.

Scientific Sources & References

Name Origin

Greek physicist, mathematician (c. 287-212 B.C.).

Interactive Lunar Surface

Explore Archimedes in 3D

Inspect lunar elevation data and the official selenographic position.