Birmingham (crater)
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Crater characteristics | |
Location of the Birmingham crater. |
|
Coordinates | 65.1° N, 10.5° W |
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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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