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Apollo (crater) : ウィキペディア英語版
Apollo (crater)

Apollo is an enormous impact crater located in the southern hemisphere on the far side of the Moon. This formation dwarfs the large crater Oppenheimer that is located next to the western rim. The crater Barringer lies across the northern wall. To the southeast is the crater Anders, and Kleymenov is just to the east of the rim.
Apollo is a double-ringed walled plain (or basin) whose inner ring is roughly half the diameter of the outer wall. Both the outer wall and the interior have been heavily worn and eroded by subsequent impacts, so that significant parts of the outer and inner walls now consist of irregular and incised sections of mountainous arcs.
The interior floor is covered in a multitude of craters of various sizes. Several of the more notable craters have received names. The IAU used the eponyms of people associated with the Apollo program when designating some of these formations.
Sections of Apollo's interior have been resurfaced with lava, leaving patches of the floor with a lower albedo than the surroundings. There is a large patch of this lunar mare in the middle part of the inner ring, which contains some ray system markings. A long stretch of the mare lies along the southern part of the crater. There is also a smaller section near the western rim.
==Interior craters==
Several craters within the Apollo impact have been named to honor deceased NASA employees.
Dryden is attached to the west-northwestern exterior of the inner ring. Chaffee is a similar-sized crater that lies partly across the southwest section of the inner ring. In the southeast part of the outer crater is Borman. Inside the inner ring are the craters Resnik, McAuliffe and Onizuka, and the JarvisMcNair crater pair. The crater Smith lies across the northern part of the inner ring.
In 2006 the IAU approved a proposal to name seven interior craters to honor the astronauts killed in the Space Shuttle ''Columbia'' disaster.
Three of the crater names include the respective astronaut's first initials to distinguish them from the existing craters called Anderson, Brown and Clark.

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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