Craterra

Western Mare Tranquillitatis

A Worn, Lava-Flooded Crater Modified by Imbrium Basin Ejecta

Spanning 84.72 kilometers, Julius Caesar features a heavily worn wall and a level floor likely modified by ejecta from the Imbrium basin impact.

Feature Profile & Selenographic Data

Feature type
crater
Coordinates
9.17° N · 15.21° E
Diameter
84.72 km
IAU approval
1935/01/01 00:00:00
LAC quadrangle
LAC-60 · Julius Caesar

Geological Chronicle

Julius Caesar is a lava-flooded lunar impact crater spanning 84.72 kilometers in diameter near the western margin of Mare Tranquillitatis. Located directly southeast of the crater Manilius on Mare Vaporum and west of the rounded Sosigenes, the structure exhibits a low, irregular, and heavily worn wall. A number of crater remnants overlap the rim along its southern and northeastern edges.

The interior floor of the crater is relatively level, especially across its southwestern half, and a low ridge crosses the northeastern section. Across the interior, the northern half has a lower albedo than the south, leading the observer T. W. Webb to describe the formation as a very dark enclosure. The floor was most likely covered or modified by ejecta from the impact that created the Imbrium basin.

Scientific Sources & References

Name Origin

Roman emperor, introduced the Julian calendar (c. 102-44 B.C.).

Interactive Lunar Surface

Explore Julius Caesar in 3D

Inspect lunar elevation data and the official selenographic position.