The satellite was born dead and has remained geologically dead for more than four billion years. Callisto is unique among the planet-sized objects of the solar system in its absence of interior forces to drive geological evolution. Ice on Callisto does not deform or flow like ice in glaciers on Earth. In thinking of ice so far from the Sun, it is important not to judge its behavior from that of the much warmer ice we know on Earth at the temperatures of the outer solar system, ice on the surface is nearly as hard as rock, and behaves similarly. The survival of these craters tells us that an icy object can form and retain impact craters in its surface. Like our Moon's highlands, the surface of Callisto is covered with impact craters. Yet Callisto seems to have frozen solid before the process of differentiation was complete. Only a little heating will soften the ice and get the process started, allowing the rock and metal to sink to the center and the slushy ice to float to the surface. It is much easier for an icy body to differentiate than for a rocky one, since the melting temperature of ice is so low. This fact surprised scientists, who expected that all the big icy moons would be differentiated. Astronomers can tell that it lacks a dense core from the details of its gravitational pull on the Galileo spacecraft during several very close flybys. Callisto has not fully differentiated, meaning separated into layers of different density materials. This tells us that Callisto has far less of the rocky metallic materials found in the inner planets and must instead be an icy body through much of its interior. Its mass is only one-third as great, which means its density must be only one-third as great as well. Callisto has a diameter of 4.820 kilometers, almost the same as that of Mercury. Its noontime surface temperature is only about -140Г‚вЊ, so water ice is stable on its surface year-round. Like our own Moon, Callisto rotates in the same period as it revolves, so it always keeps the same face toward Jupiter. Callisto, the outermost of Jupiter's four largest satellites, orbits the planet in seventeen days at a distance from Jupiter of two million kilometers. From 1996 to 1999, the Galileo spacecraft passed through the Jovian system, providing much information about Jupiter's satellites.

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