Impact crater

Archimedes

A broad, dark-floored crater within Mare Imbrium. The relatively smooth interior is a useful contrast to nearby mountain ranges and smaller impact craters.

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Archimedes and surrounding lunar terrain in the LROC Wide Angle Camera mosaic
Archimedes · North up, east right. Open image ↗
NASA / GSFC / Arizona State University · LROC WAC mosaic via USGS. Regional map crop; lighting is fixed and does not follow the selected date.
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How to observe Archimedes

Examine the rim under low light and compare the floor with nearby mare terrain. Use the crater to find the Apennine region.

Finding the region

Look at 29.72° N, 3.99° W on the lunar disc. The chart marker identifies the catalogue centre. Start with a wide field and use the nearby formations below as landmarks.

Equipment & conditions

Start at low magnification to identify the rim. Move to a moderate power when the air is steady; low sunlight usually makes walls and floor relief easier to distinguish. A bright ray system can be more conspicuous near full Moon.

Lighting

For surface relief, try a time when the Sun is low over this region. To compare surface brightness and any bright rays, return under higher illumination. The atlas calculates the solar elevation at the formation’s centre for any selected date.

View Archimedes in the atlas

IAU / USGS Gazetteer

Official feature record

View original record ↗
Approved name
Archimedes
Feature classification
Crater, craters
Catalogue diameter
81.04 km
Centre latitude
29.72° N
Centre longitude
3.99° W
Name origin (Gazetteer)
Greek physicist, mathematician (c. 287-212 B.C.).

Coordinates are selenographic, with east-positive longitude. Dimensions are the Gazetteer’s catalogue values; for extended formations they do not represent a circular crater diameter. Data snapshot: 2026-09-16. Observing guidance above is separate from the official record.

Nearby formations

The four closest catalogue entries, measured from their centres.

LROC photograph of Mare ImbriumSea / bay

Mare Imbrium

The Sea of Rains is a large lava plain in the northwestern near side. Mountain arcs and prominent craters provide numerous landmarks around its margins.

1,145.5 kmRead guide ↗
LROC photograph of Montes ApenninusMountain range

Montes Apenninus

A mountain arc bordering southeastern Mare Imbrium. Its ridges and peaks cast long shadows across the adjacent plain under low sunlight.

LROC photograph of CassiniImpact crater

Cassini

A crater in the northeastern part of Mare Imbrium, close to the Alpine region. Smaller craters inside help distinguish it from nearby formations.

LROC photograph of Montes CaucasusMountain range

Montes Caucasus

A mountain group between Mare Imbrium and Mare Serenitatis. It forms a useful bridge between two major lunar plains.