Birmingham (crater)

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Crater characteristics

Location of the Birmingham crater.
Coordinates 65.1° N, 10.5° W
Diameter 92 km
Depth 1.8 km
Colongitude 13° at sunrise
Eponym John Birmingham

Birmingham is the surviving remnant of a lunar crater. It is located near the northern limb of the Moon, and so is viewed from the Earth at a low angle. All that survives of the original formation is an irregular perimeter of low, indented ridges surrounding the lava-resurfaced interior. The inner floor is marked by several tiny craterlets, and the surface is unusually rough for a walled plain. The low angle of illumination allows fine details of this boulder-strewn field to be seen more clearly.

The Birmingham formation lies just to the north of the Mare Frigoris, and to the east of the W. Bond walled-plain. To the northeast is the smaller Epigenes crater, and Fontenelle crater lies to the northwest.

[edit] Satellite craters

By convention these features are identified on lunar maps by placing the letter on the side of the crater mid-point that is closest to Birmingham crater.

Birmingham Latitude Longitude Diameter
B 63.6° N 11.3° W 8 km
G 64.5° N 10.2° W 5 km
H 64.4° N 10.6° W 7 km
K 65.0° N 13.1° W 6 km

[edit] References

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