Sulpicius Gallus (crater)

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Sulpicius Gallus
Apollo 15 Mapping camera image
Diameter12 km
Depth2.2 km
Colongitude349° at sunrise
EponymGaius Sulpicius Gallus
Rimae Sulpicius Gallus

Sulpicius Gallus is a small, bowl-shaped lunar crater that lies near the southwestern edge of the Mare Serenitatis. About 10 kilometers to the south and east is the Montes Haemus range that forms the edge of the Serenitatis basin. This crater has a relatively high albedo, with a sharp-edged rim that displays little appearance of wear. There is a small rise at the midpoint. Recent deposits of highland material have been observed within the crater interior.

To the northwest is a rille system designated the Rimae Sulpicius Gallus. These extend to the northwest for a distance of about 90 kilometers, curving and branching out to follow the edge of the mare.

Satellite craters

By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Sulpicius Gallus.

Sulpicius
Gallus
Latitude Longitude Diameter
A 22.1° N 8.9° E 4 km
B 18.0° N 13.0° E 7 km
G 19.8° N 6.3° E 6 km
H 20.6° N 5.7° E 5 km
M 20.4° N 8.7° E 5 km

References

  • "SMART-1 view of crater Sulpicius Gallus". European Space Agency. 2006-07-12. Retrieved 2006-07-18.
  • J.F. Bell III; B. R. Hawke (1995). "Compositional variability of the Serenitatis/Tranquillitatis region of the Moon from telescopic Multispectral Imaging and Spectroscopy". Icarus. 118: 51–68. Bibcode:1995Icar..118...51B. doi:10.1006/icar.1995.1177.