Craterra

Mare Frigoris margin

A polygonal impact basin on the edge of the Sea of Cold

Bordering Mare Frigoris, C. Mayer preserves sharp terraced walls, a northern central peak, and an attached basalt-flooded companion.

Feature Profile & Selenographic Data

Feature type
crater
Coordinates
63.26° N · 17.31° E
Diameter
37.54 km
IAU approval
1935/01/01 00:00:00
LAC quadrangle
LAC-13 · Aristoteles

Geological Chronicle

Positioned along the northern edge of Mare Frigoris, C. Mayer spans 37.54 kilometers in diameter at lunar coordinates 63.2562° N and 17.3072° E. The impact crater lies due north of Aristoteles, north of the smaller Sheepshanks, and due east of it sits the flooded crater Kane. It retains a relatively young, sharp-edged outer rim that appears somewhat polygonal with outward bulges, most noticeably to the west.

Its inner walls feature a terrace system, surrounding a somewhat rough and irregular floor. Just north of the crater midpoint, a central peak extends in a northerly direction. Along the southeastern rim, the lava-flooded formation C. Mayer D is attached to the crater, where a rim gap joins it to Mare Frigoris and brings the lunar mare up to C. Mayer's outer rampart.

The crater is named after Moravian astronomer and teacher Christian Mayer. German astronomer Johann H. Schröter added the name to lunar nomenclature in 1791, and the International Astronomical Union formally adopted the designation in 1935. In addition, satellite craters F and H contain permanently shadowed regions where sunlight never reaches.

Chronology & Exploration

  1. 1791 Named by Schröter

    Johann H. Schröter adds Christian Mayer's name to lunar nomenclature for the crater.

  2. 1935 IAU adoption

    The International Astronomical Union officially adopts the designation C. Mayer.

Scientific Sources & References

Name Origin

Christian; German astronomer, mathematician, physicist (1719-1783).

Interactive Lunar Surface

Explore C. Mayer in 3D

Inspect lunar elevation data and the official selenographic position.