Craterra

Southern Highlands

A Heavily Worn Walled Plain in the Moon's Southern Highlands

Spanning 145.5 kilometers across the rugged southern terrain, Longomontanus ranks among the largest impact craters dating to the Moon's Nectarian age.

Feature Profile & Selenographic Data

Feature type
crater
Coordinates
49.55° S · 21.88° W
Diameter
145.5 km
IAU approval
1935/01/01 00:00:00
LAC quadrangle
LAC-125 · Schiller
Geological Period
Nectarian

Geological Chronicle

Located in the rugged southern highlands to the southwest of the bright ray crater Tycho, Longomontanus is an ancient circular depression classified as a walled plain. The structure measures 145.5 kilometers in diameter. Because of its location, Longomontanus appears distinctly oval in shape due to foreshortening.

On the lunar geologic timescale, Longomontanus is one of the largest craters of Nectarian age. To the southeast lies the even larger formation Clavius, Maginus is located to the east, and north of the rim is the irregular crater Montanari, which is joined at its northern rim by Wilhelm.

The wall of Longomontanus is heavily worn and incised by past impacts, leaving the rim essentially level with the surrounding terrain. The northern rim especially is impacted with multiple overlapping craterlets, while a semi-circular ridge to the east has the appearance of an overlapped crater rim. The crater floor is relatively flat, with a low cluster of central peaks somewhat offset to the west.

Chronology & Exploration

  1. Nectarian Impact Formation

    Longomontanus is formed as an impact crater during the Nectarian age on the lunar geologic timescale.

Scientific Sources & References

Name Origin

Christian Sorensen; Danish astronomer, mathematician (1562-1647).

Interactive Lunar Surface

Explore Longomontanus in 3D

Inspect lunar elevation data and the official selenographic position.