Alphonsus (crater)

Alphonsus

Coordinates 13°24′S 2°48′W / 13.4°S 2.8°W / -13.4; -2.8Coordinates: 13°24′S 2°48′W / 13.4°S 2.8°W / -13.4; -2.8
Diameter 119 km
Depth 2.7 km
Colongitude 4° at sunrise
Eponym Alfonso X
Alphonsus crater appears in the right half of this image taken by Ranger 7. NASA photo.
Ranger 9 image showing rilles on the floor of the crater

Alphonsus is an ancient impact crater on the Moon that dates from the pre-Nectarian era.[1] It is located on the lunar highlands on the eastern end of Mare Nubium, west of the Imbrian Highlands, and slightly overlaps the crater Ptolemaeus to the north. To the northwest is the smaller Alpetragius.

Description

The surface of Alphonsus is broken and irregular along its boundary with Ptolemaeus. The outer walls are slightly distorted and possess a somewhat hexagonal form.

A low ridge system of deposited ejecta bisects the crater floor, and includes the steep central peak designated Alphonsus Alpha (α). This pyramid-shaped formation rises to a height of 1.5 km above the interior surface. It is not volcanic in origin, but rather is made of anorthosite like the lunar highlands.

The floor is fractured by an elaborate system of rilles and contains three smaller craters surrounded by a symmetric darker halo. These dark-halo craters are cinder cone-shaped and are believed by some to be volcanic in origin, although others think they were caused by impacts that excavated darker mare material from underneath the lighter lunar regolith.

Exploration

The Ranger 9 probe impacted in Alphonsus, a short distance to the northeast of the central peak. Harold Urey said of a close-up photograph of Alphonsus:

“ The floor is covered with many craters of various sizes, some sharp and hence new, others less distinct and partly filled with fragmented material. The walls have fewer craters, and this probably means that slumping of the wall has filled them. Crevasses are evident, and evidence for slumping exists. The larger crater near the top is undoubtedly collisional in origin. Three craters are surrounded by dark halos and were produced by eruptions from the lunar interior. Exceptionally bright, sharp peaks can be seen on certain mountain tops. ”

Alphonsus was one of the primary alternative landing sites considered for both the Apollo 16 and the Apollo 17 missions.

Transient lunar phenomena

Alphonsus is one of the sites noted for transient lunar phenomena, as glowing red-hued clouds have been reported emanating from the crater. On October 26, 1956, the lunar astronomer Dinsmore Alter noted some blurring of the rilles on the floor of Alphonsus in the photographs he took in violet light. The same blurring did not occur in the infrared photographs he took at the same time. However, few professional astronomers found this evidence of volcanic activity on the Moon very convincing.

One astronomer who was intrigued by Alter's observations was Nikolai A. Kozyrev, from the Soviet Union. In 1958 while Kozyrev was looking for volcanic phenomenon on the moon, he observed the formation of a mist-like cloud within Alphonsus.[2] The spectrum of the area had been measured at this time, and displayed indications of carbon matter, possibly C2 gas. He believed this to be the result of volcanic or related activity. However no evidence for this phenomenon has been found from lunar missions, and the emission results have never been confirmed.

Names

Alphonsus is named after King Alfonso X of Castile (known as "Alfonso the Wise"), who had an interest in astronomy. Like many of the craters on the Moon's near side, it was given its name by Giovanni Riccioli, whose 1651 nomenclature system has become standardized; Riccioli originally named it "Alphonsus Rex" ('King Alfonso'), but the 'Rex' was later dropped.[3] Earlier lunar cartographers had given the feature different names. Michael van Langren's 1645 map calls it "Ludovici XIV, Reg. Fran.", after Louis XIV of France,[4] and Johannes Hevelius called it "Mons Masicytus" after a range of mountains in Lycia.[5]

Interior craters

Oblique view of the five small named craters: C = Chang-Ngo, R = Ravi, M = Monira, J = Jose, S = Soraya. Facing south with sun illuminating from left.

Five tiny craters in the northeastern part of Alphonsus' interior floor have been assigned names by the IAU. These are listed in the table below.

Crater Coordinates Diameter Name source
Chang-Ngo 12°42′S 2°06′W / 12.7°S 2.1°W / -12.7; -2.1 3 km Chinese feminine name1
José 12°42′S 1°36′W / 12.7°S 1.6°W / -12.7; -1.6 2 km Spanish masculine name
Monira 12°36′S 1°42′W / 12.6°S 1.7°W / -12.6; -1.7 2 km Arabic feminine name
Ravi 12°30′S 1°54′W / 12.5°S 1.9°W / -12.5; -1.9 2.5 km Indian masculine name
Soraya 12°54′S 1°36′W / 12.9°S 1.6°W / -12.9; -1.6 2 km Persian feminine name
  1. See also Chang'e, the Chinese goddess.

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 Alphonsus.

Alphonsus Latitude Longitude Diameter
A 14.8° S 2.3° W 4 km
B 13.2° S 0.2° W 24 km
C 14.4° S 4.8° W 4 km
D 15.1° S 0.8° W 23 km
G 12.3° S 3.3° W 4 km
H 15.6° S 0.5° W 8 km
J 15.1° S 2.5° W 8 km
K 12.5° S 0.1° W 20 km
L 12.0° S 3.7° W 4 km
R 14.4° S 1.9° W 3 km
X 15.0° S 4.4° W 5 km
Y 14.7° S 1.8° W 3 km

References

  1. ↑ Ambrose, W.A. "ORIGIN, DISTRIBUTION, AND CHRONOSTRATIGRAPHY OF ASYMMETRIC SECONDARY CRATERS ASSOCIATED WITH NEARSIDE LUNAR BASINS" (PDF). Bureau of Economic Geology. University of Texas at Austin, TX. Retrieved 25 September 2013.
  2. ↑ Oepik, E.J. "Cratering and the moon's surface". Armagh Observatory. Department of Physics and Astronomy, University of Maryland. Retrieved 20 September 2011.
  3. ↑ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.210.
  4. ↑ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p. 198.
  5. ↑ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p. 205.
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External links

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