This image shows a heavily cratered region near Callisto's equator. North is to the top of the image. Har displays an unusual rounded mound on its floor. The large crater partially visible in the northeast corner of the image is called Tindr. This mosaic covers part of the equatorial region of Jupiter's moon, Callisto.
North is to the top of the picture.
The mosaic shows several new features and characteristics of the surface revealed by Galileo. These include deposits that may represent landslides in the southern and southwestern floors of many craters. The pervasive local smoothing of Callisto's surface is well represented in the plains between the craters in the southeastern part of the image. Possible oblique impacts are suggested by the elongated craters in the northeastern and southeastern parts of the image. This two frame mosaic of images from NASA's Galileo spacecraft shows an area in the southern hemisphere of Jupiter's moon, Callisto, that was not imaged during the 1979 flyby of NASA's Voyager spacecraft.