Dorsa Rubey [SEP] located on astronomical body
Dorsa Rubey
Dorsa Rubey is a wrinkle ridge system at in Oceanus Procellarum on the Moon. It is 100 km long and was named after American geologist William Walden Rubey in 1976.
-circular series of ridges. The flooded, broken rim of Winthrop overlies the western wall. The rim is the most intact along the eastern stretch, forming a mountainous promontory into the mare. A small cluster of central rises lie at the midpoint of the crater. The wrinkle ridge Dorsa Rubey traverses the floor from north to south, and outlines a portion of the missing rim. The crater floor is otherwise nearly smooth and relatively free of craterlets, with the exception of Letronne B near the southeast rim.
Satellite craters