Craterra

Oceanus Procellarum

Wrinkle Ridge System in Oceanus Procellarum

A 138.93-kilometer wrinkle ridge system in Oceanus Procellarum named after British mathematician and astronomer William Whiston.

Feature Profile & Selenographic Data

Feature type
dorsum
Coordinates
29.77° N · 56.96° W
Diameter
138.93 km
IAU approval
1976/01/01 00:00:00
LAC quadrangle
LAC-38 · Seleucus

Geological Chronicle

Dorsa Whiston is a wrinkle ridge system located in Oceanus Procellarum on the Moon. Located in the Seleucus quadrangle, the feature has an official diameter of 138.93 kilometers.

The feature was named after British mathematician and astronomer William Whiston in 1976. The system extends across an approximate length of 221 kilometers.

Chronology & Exploration

  1. 1976 Official IAU Nomenclature

    The feature is officially named after British mathematician and astronomer William Whiston in 1976.

Scientific Sources & References

Name Origin

William; British mathematician, astronomer (1667-1752).

Interactive Lunar Surface

Explore Dorsa Whiston in 3D

Inspect lunar elevation data and the official selenographic position.