Craterra

Mare Crisium

A Circular Pit in the Northern Plains of Mare Crisium

Spanning 2.62 kilometers across the dark surface of Mare Crisium, Eckert sits in isolation near a subtle wrinkle ridge.

Feature Profile & Selenographic Data

Feature type
crater
Coordinates
17.28° N · 58.38° E
Diameter
2.62 km
IAU approval
1973/01/01 00:00:00
LAC quadrangle
LAC-44 · Cleomedes

Geological Chronicle

Eckert is a tiny, isolated lunar impact crater in the northern part of Mare Crisium, a circular region of relatively dark, flat material on the surface of the Moon. With a diameter of 2.62 kilometers, this crater forms a circular pit in the dark surface of the surrounding mare.

Just to the west is a wrinkle ridge in the mare surface, a feature that is prominent only under oblique lighting from the Sun. Across the broader Mare Crisium basin, the nearest craters of note are Peirce to the west-northwest and Picard to the southwest.

The International Astronomical Union officially approved the crater's name in 1973. The feature is named for American astronomer Wallace John Eckert.

Chronology & Exploration

  1. 1973 IAU Approval

    The International Astronomical Union officially approves the name Eckert for the crater.

Scientific Sources & References

Name Origin

Wallace John; American astronomer (1902-1971).

Interactive Lunar Surface

Explore Eckert in 3D

Inspect lunar elevation data and the official selenographic position.