Scaliger (crater)

Scaliger
LRO WAC image. Scaliger U is the circular crater at left.
Coordinates27°06′S 108°54′E / 27.1°S 108.9°E / -27.1; 108.9
Diameter84 km
DepthUnknown
Colongitude252° at sunrise
EponymJoseph J. Scaliger
Apollo 15 image
Apollo 15 mosaic of north rim area
Oblique Lunar Orbiter 3 image, facing south

Scaliger is a prominent lunar impact crater in the southern hemisphere on the far side of the Moon.[1] It is attached to the northwest rim of a walled plain named Milne, and the shared perimeter has reshaped the outer wall of Scaliger slightly, producing a straightened section along the southeast. To the west of Scaliger is the Lacus Solitudinis.

This formation dates to the Late Imbrian epoch of the lunar geologic timescale.[2] The outer wall of Scaliger is somewhat polygonal in shape, especially in the southern half. The rim has not been heavily eroded by subsequent impacts, in contrast to the heavily worn Milne to the southeast. The inner wall of Scaliger's rim displays terraces, and a notable outer rampart overlaying the floor of Milne. The infrared spectrum of pure crystalline plagioclase has been identified within this crater.[3]

The interior floor of Scaliger is relatively flat, with a rough surface near the inner wall. Near the midpoint is a central peak, offset slightly to the east. The spectra of this rise fits a olivine-bearing noritic gabbro mineralogy, which originated from a depth of 8.4 to 13.3 km.[4]

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 Scaliger.

Scaliger Latitude Longitude Diameter
U 26.6° S 106.5° E 11 km

References

  1. ↑ Moore, Patrick (2000). The Data Book of Astronomy. CRC Press. p. 71. ISBN 978-1-4200-3344-1.
  2. ↑ Tompkins, Stefanie; Pieters, Carle M. (January 1999). "Mineralogy of the lunar crust: Results from Clementine". Meteoritics & Planetary Science. 34 (1): 25–41. Bibcode:1999M&PS...34...25T. doi:10.1111/j.1945-5100.1999.tb01729.x.
  3. ↑ Donaldson Hanna, K. L.; et al. (July 2014). "Global assessment of pure crystalline plagioclase across the Moon and implications for the evolution of the primary crust". Journal of Geophysical Research: Planets. 119 (7): 1516–1545. Bibcode:2014JGRE..119.1516D. doi:10.1002/2013JE004476.
  4. ↑ Cahill, J. T. S.; et al. (September 2009). "Compositional variations of the lunar crust: Results from radiative transfer modeling of central peak spectra". Journal of Geophysical Research. 114 (E9) E09001. Bibcode:2009JGRE..114.9001C. doi:10.1029/2008JE003282.

Sources