Craterra

Palus Nebularum

A Flooded Ring-Plain at the Edge of Mare Imbrium

Flooded by lava yet enclosed by an intact rim, Cassini hosts interior impact craters and an irregular outer rampart in Palus Nebularum.

Feature Profile & Selenographic Data

Feature type
crater
Coordinates
40.25° N · 4.64° E
Diameter
56.88 km
IAU approval
1935/01/01 00:00:00
LAC quadrangle
LAC-25 · Cassini
Geological Period
Lower Imbrian

Geological Chronicle

Cassini occupies Palus Nebularum at the eastern margin of Mare Imbrium, spanning a diameter of 56.88 kilometers between the solitary peak Mons Piton to the northwest and Promontorium Agassiz to the northeast. Dating to the Lower Imbrian epoch, the impact structure underwent flooding by lava, leaving a floor likely as old as the surrounding mare.

The crater walls are narrow and irregular in form, yet they remained intact despite the lava flooding and rise above a substantial outer rampart. Within the flooded basin sit two significant craters: Cassini A, located just northeast of the crater center with a large interior mound and an adjoining hilly ridge, and Cassini B near the southwestern rim.

For unknown reasons, Cassini was omitted from early maps of the Moon, an absence considered most likely an error by map-makers. In 1791, German astronomer J. H. Schröter introduced the name honoring astronomers Giovanni Cassini and Jacques Cassini, a designation officially adopted by the International Astronomical Union in 1935.

Chronology & Exploration

  1. 1791 Name Introduced

    Astronomer J. H. Schröter introduces the name Cassini into lunar nomenclature.

  2. 1935 IAU Adoption

    The International Astronomical Union officially adopts the crater designation.

Scientific Sources & References

Name Origin

Giovanni Domenico; Italian-French astronomer (1625-1712); Jacques; French astronomer (1677-1756).

Interactive Lunar Surface

Explore Cassini in 3D

Inspect lunar elevation data and the official selenographic position.