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・ C. Malcolm Watkins
・ C. Manickam
・ C. marginatum
・ C. marginatus
・ C. marina
・ C. maritima
・ C. maritimus
・ C. Markland Kelly
・ C. Martin Croker
・ C. Martin Wilbur
・ C. Maurice Patterson
・ C. maxima
・ C. maximus
・ C. Maxwell Lane
・ C. Maxwell Stanley
C. Mayer (crater)
・ C. McAlpine
・ C. Mel Wilcox
・ C. mertensii
・ C. metallica
・ C. mexicana
・ C. Meyer Zulick
・ C. Michael Armstrong
・ C. Michael Harper
・ C. Michael Petters
・ C. Michael Roland
・ C. Michael Ryer
・ C. Michael Smith
・ C. Michelle Olmstead
・ C. migratorius


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C. Mayer (crater) : ウィキペディア英語版
C. Mayer (crater)

C. Mayer is a lunar impact crater that is located at the northern edge of the Mare Frigoris, due north of the prominent crater Aristoteles. Also to the south, but only a third as distant, is the smaller crater Sheepshanks. Due east of C. Mayer is the flooded crater Kane.
C. Mayer is a relatively young formation, with a sharp-edged and well-defined outer rim. The rim is not quite circular, and appears somewhat polygonal-shaped with outward bulges along the edge, most notably to the west. The inner walls have a terrace system and the interior is somewhat rough and irregular. The central peak lies just to the north of the midpoint, and extends in a northerly direction.
The lava-flooded formation C. Mayer D is attached to the southeastern rim of the crater, and a gap in the southeastern rim joins it to the Mare Frigoris. Thus the lunar mare extends up to the outer rampart of C. Mayer.
==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 C. Mayer.

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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