Craterra

Mare Fecunditatis Wrinkle Ridge System

Dorsa Andrusov

A wrinkle ridge system in Mare Fecunditatis extending 80.98 kilometers from Dorsa Geikie toward Webb crater.

Feature Profile & Selenographic Data

Feature type
dorsum
Coordinates
1.56° S · 56.77° E
Diameter
80.98 km
IAU approval
1976/01/01 00:00:00
LAC quadrangle
LAC-80 · Langrenus

Geological Chronicle

Dorsa Andrusov is a lunar wrinkle ridge system situated in Mare Fecunditatis. Centered at latitude 1.56° S, longitude 56.77° E within the Langrenus quadrangle (LAC-80), the feature extends across a diameter of 80.98 kilometers.

The ridge starts near Dorsa Geikie, trending northeast before ending in the vicinity of Webb crater.

In 1976, the International Astronomical Union officially designated the feature in honor of Soviet geologist Nikolai Ivanovich Andrusov.

Chronology & Exploration

  1. 1976 IAU Name Adoption

    The International Astronomical Union officially adopted the name Dorsa Andrusov, commemorating Soviet geologist Nikolai Ivanovich Andrusov.

Scientific Sources & References

Name Origin

Nikolai Ivanovich; Soviet geologist (1861-1924).

Interactive Lunar Surface

Explore Dorsa Andrusov in 3D

Inspect lunar elevation data and the official selenographic position.