Craterra

Grimaldi Quadrangle (LAC-74)

Lacus Aestatis: Twin Mare Deposits in the Southwestern Highlands

Positioned near the Moon's western limb, this small lunar lake consists of two interconnected basaltic plains formed 3.5 billion years ago.

Feature Profile & Selenographic Data

Feature type
lacus
Coordinates
14.83° S · 68.57° W
Diameter
86.39 km
IAU approval
1970/01/01 00:00:00
LAC quadrangle
LAC-74 · Grimaldi
Geological Period
Imbrian

Geological Chronicle

Lacus Aestatis, translated from Latin as the Lake of Summer, is situated in the southwestern highlands near the western limb of the Moon. The feature consists of two smooth, interconnected patches of lunar mare with a combined surface area of approximately 400 square kilometers. Originally named Mare Aestatis, the International Astronomical Union formally adopted its current designation as a lacus during its 1970 convention.

The northwestern segment of the lake lies east-southeast of the crater Rocca, enclosed within the rim of satellite crater Rocca A. The southeastern segment extends as an elongated, irregular patch stretching north to south, with its southern extremity positioned roughly one crater diameter northwest of the flooded crater Crüger. Across both segments, the regional feature spans a diameter of 86.39 kilometers.

Crater count measurements yield an estimated basalt age of 3.50 billion years, establishing that volcanic activity inundated these highland depressions during the Imbrian period.

Chronology & Exploration

  1. Imbrian Era Basaltic Volcanism

    Lava flows flood highland depressions 3.50 billion years ago, creating the two basaltic patches of Lacus Aestatis.

  2. 1970 IAU Reclassification

    The International Astronomical Union officially renames the feature from Mare Aestatis to Lacus Aestatis.

Scientific Sources & References

Name Origin

"Lake of Summer."

Interactive Lunar Surface

Explore Lacus Aestatis in 3D

Inspect lunar elevation data and the official selenographic position.