Alphonsus is an ancient impact crater on Earth's Moon that dates from the immediate post-Nectarian era. It is located on the lunar highlands on the eastern end of Mare Nubium, west of the Imbrian Highlands, and slightly overlaps the Ptolemaeus crater to the north. The surface is broken and irregular along this boundary. The outer walls are slightly distorted in form and possess a somewhat hexagonal form. To the northwest is the smaller Alpetragius crater.
A low ridge system bisects the crater floor, and includes the steep central peak designated Alpha (α) Alphonsus. This pyramid-shaped formation rises to a height of 1.5 km above the interior surface. The floor is fractured by an elaborate system of rilles and contains three smaller surrounded by a symmetric darker halo. These dark_halo craters are cinder_shaped and were once believed to be volcanic in nature. But they are now believed to be caused by impacts that excavated darker mare material from underneath the lighter lunar regolith.
Alphonsus was one of the sites noted for lunar transient phenomenon, as glowing red-hued clouds had been reported emanated from the crater. Gaseous emissions have also been reported from the central peak, by Soviet astrophycisist Nikolai Kozyrev in 1958. No evidence for this phenomenon has been found from lunar missions, and the emission results have never been confirmed.
Alphonsus crater was one of the primary alternative landing sites considered for both the Apollo 16 and the Apollo 17 missions. The Ranger 9 probe impacted in Alphonsus crater, a short distance to the northeast of the central peak.
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 Alphonsus crater.
Feeds |
Contact