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Cabeus (crater)
Cabeus is a lunar crater that is located about from the south pole of the Moon.〔 At this location the crater is seen obliquely from Earth, and it is almost perpetually in deep shadow due to lack of sunlight. Hence, not much detail can be seen of this crater, even from orbit. Through a telescope, this crater appears near the southern limb of the Moon, to the west of the crater Malapert and to the south-southwest of Newton.〔〔
== Description ==
The crater name ''Cabeus'' first appeared in the 1651 work ''Almagestum Novum'' by Giovanni Riccioli, who named it after Niccolò Cabeo. However, the position of the Cabeus crater was in the location later assigned to Newton crater.〔Whitaker (1999:61, 211)〕 The official name and location for this crater was adopted by the IAU Commission 17, as established in the 1935 work ''Named Lunar Formations'' by Mary A. Blagg and Karl Müller.〔
This crater is a worn formation that has been eroded by subsequent impacts. The rim is eroded and uneven, with prominent ridges at the northern and southern ends. A small crater lies across the northeastern rim and there is 10–11 km crater on the interior floor near the west-southwestern rim. Near the center of the crater floor is a small ridge. The floor of the crater has an average depth of 4 km and it is 60 km across. The slope of the crater walls is 10–15°.〔
Because of the crater's location near the lunar south pole, the main part of the crater is illuminated by the Sun during only 25% of each lunar day. The inner walls receive illumination for 30% of a lunar day, while part of the western end of the crater is in permanent shadow.〔
抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』
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