Craterra

Mare Insularum

A Young Impact Crater Whose Debris Reached Earth

Lalande is a sharp Copernican crater whose extensive ray system overlaps Copernicus and is linked to a lunar meteorite recovered in Oman.

Feature Profile & Selenographic Data

Feature type
crater
Coordinates
4.46° S · 8.65° W
Diameter
23.54 km
IAU approval
1935/01/01 00:00:00
LAC quadrangle
LAC-77 · Ptolemaeus
Geological Period
Copernican

Geological Chronicle

Positioned along the eastern edge of Mare Insularum on the central near side of the Moon, Lalande spans 23.54 kilometers in diameter. The impact feature exhibits terracing along its interior walls and a low central rise situated at the midpoint of its floor.

Lalande is enveloped by a prominent high-albedo blanket that projects bright rays outward to a maximum radius exceeding 300 kilometers. Because these rays physically overlie ejecta from the larger Copernicus crater, geologists place Lalande within the Copernican period, establishing an age of no more than 800 million years.

The crater is also considered the source of a verified lunar meteorite. In 2002, researchers discovered the rock specimen Sayh al Uhaymir 169 in Oman, which was excavated by an impact less than 340,000 years ago and is believed by scientists to have originated from the ejecta blanket surrounding Lalande.

Chronology & Exploration

  1. 2002 Meteorite Discovery

    The lunar meteorite Sayh al Uhaymir 169 is discovered in Oman and subsequently traced to ejecta from Lalande.

Scientific Sources & References

Name Origin

Joseph Jérôme Le François de; French astronomer (1732-1807).

Interactive Lunar Surface

Explore Lalande in 3D

Inspect lunar elevation data and the official selenographic position.