How is Jupiter's outermost Galilean moon, Callisto, typically characterized regarding geological activity?
Answer
As a heavily battered, geologically dead world that has dissipated initial heat
Callisto, the outermost of the Galilean moons, stands in sharp contrast to its active inner siblings. It is frequently described as a geologically dead world, characterized by a heavily battered and ancient surface covered extensively by impact craters. This inactivity is due to its greater distance from Jupiter and an orbital path that lacks the tight resonant coupling that continuously flexes Io, Europa, and Ganymede, meaning it has lost its initial formation heat over time.

Related Questions
What powers Io's extreme geological activity, making it the most active body?How does Europa's geological activity differ from Io's silicate volcanism?From which specific features on Saturn's moon Enceladus do massive plumes erupt?What feature on Jupiter's moon Ganymede strongly suggests it harbors a molten, electrically conducting layer?How is Jupiter's outermost Galilean moon, Callisto, typically characterized regarding geological activity?What chemical components form the basis for the geological cycles of freezing, thawing, and flow observed on Saturn's moon Titan?What is the specific mechanism that generates internal friction and heat on Io due to Jupiter's immense gravity?What type of cryovolcanism is associated with Neptune’s largest moon, Triton?What factor directly correlates with the type of surface geology observed across diverse active moons?Why does Io exhibit remarkably few large impact craters on its surface?Which Galilean moon presents geological dynamism centered around a substantial subsurface ocean beneath an icy shell?