Craterra

Mare Serenitatis

A Volcanic Cone on the Basaltic Plains of Mare Serenitatis

Spanning less than a kilometer, Isis is interpreted as a lunar volcanic cone situated along a rille near the Taurus-Littrow valley.

Feature Profile & Selenographic Data

Feature type
crater
Coordinates
18.95° N · 27.48° E
Diameter
0.61 km
IAU approval
1976/01/05 00:00:00
LAC quadrangle
LAC-42 · Mare Serenitatis

Geological Chronicle

Isis is a lunar crater spanning 0.61 kilometers in diameter across the southeastern expanse of Mare Serenitatis. The feature lies northeast of the crater Dawes and west of the Montes Taurus range, situated west-southwest of the Apollo 17 landing site in the Taurus-Littrow valley.

Together with nearby Osiris, Isis is located on a conical uprise situated along a rille. The structures are interpreted as small volcanic cones.

The International Astronomical Union adopted the designation in 1976, assigning the feature an Egyptian female given name.

Chronology & Exploration

  1. 1976 IAU Name Adoption

    The International Astronomical Union formally approves the name Isis, derived from an Egyptian female given name.

Scientific Sources & References

Name Origin

Egyptian female first name.

Interactive Lunar Surface

Explore Isis in 3D

Inspect lunar elevation data and the official selenographic position.