FIGURE 12.3Callisto.(a)Jupiter’s outermost large moon shows a heavily cratered surface. Astronomers believe that the bright areas are mostly ice, while thedarker areas are more eroded, ice-poor material.(b)These high-resolution images, taken by NASA’s Galileo spacecraft in May 2001, show the icy spires (top) on Callisto’s surface, withdarker dust that has slid down as the ice erodes, collecting in the low-lying areas. The spires are about 80 to 100 meters tall. As thesurface erodes even further, the icy spires eventually disappear, leaving impact craters exposed, as shown in the lower image. (credit a:modification of work by NASA/JPL/DLR; credit b: modification of work by NASA/JPL/Arizona State University, Academic Research Lab)