Callisto ("ka LIS toh") is the eighth of Jupiter's known satellites and the second largest. It is the outermost of the Galilean moons Callisto is only slightly smaller than Mercury but only a third of its mass.
orbit:1,883,000 km from Jupiter
Discovered by :Galileo and Marius in 1610.
Unlike Ganymede, Callisto seems to have little internal structure; however there are signs from recent Galileo data that the interior materials have settled partially, with the percentage of rock increasing toward the center. Callisto is about 40% ice and 60% rock/iron. Titan and Triton are probably similar.
Callisto's surface is covered entirely with craters. The surface is very old, like the highlands of the Moon and Mars. Callisto has the oldest, most cratered surface of any body yet observed in the solar system; having undergone little change other than the occasional impact for 4 billion years.
The largest craters are surrounded by a series of concentric rings which look like huge cracks but which have been smoothed out by eons of slow movement of the ice.
The largest of these has been named Valhalla. Nearly 3000 km in diameter, Valhalla is a dramatic example of a multi-ring basin, the result of a massive impact. Other examples are Callisto's Asgard, Mare Orientale on the Moon and Caloris Basin on Mercury. Like Ganymede, Callisto's ancient craters have collapsed. They lack the high ring mountains, radial rays and central depressions common to craters on the Moon and Mercury. Detailed images from Galileo show that, in some areas at least, small craters have mostly been obliterated. This suggests that some processes have been at work more recently, even if its just slumping.
Another interesting feature is Gipul Catena, a long series of impact craters lined up in a straight line. This was probably caused by an object that was tidally disrupted as it passed close to Jupiter (much like Comet SL 9) and then impacted on Callisto.
The Valhalla Impact Crater
The image on the right shows an enormous impact feature on Callisto called Valhalla. This gigantic meteor impact basin appears to have concentric waves around it with a diameter of about 3000 km. It is likely that the waves were formed when the surface ice was melted by a gigantic meteor impact and then quickly refroze, capturing the waves in a refrozen ice surface.
Callisto has a very tenuous atmosphere composed of carbon dioxide.
Galileo has detected no evidence of a magnetic field.
Difference with Ganymede:-
Unlike Ganymede, with its complex terrains, there is little evidence of tectonic activity on Callisto. While Callisto is very similar in bulk properties to Ganymede, it apparently has a much simpler geologic history. The different geologic histories of the two has been an important problem for planetary scientists; (it may be related to the orbital and tidal evolution of Ganymede). "Simple" Callisto is a good reference for comparison with other more complex worlds and it may represent what the other Galilean moons were like early in their history.
History of Callisto
Callisto, the most distant Galilean satellite, is only weakly influenced by Jupiter-induced tides. The evidence suggests that the crust of Callisto probably froze as it was formed, and essentially nothing has happened geologically on Callisto for 4.5 billion years except for the influence of large and small meteor impacts.
1-Why are Callisto and Ganymede so different?
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Last Modified : 5 Sep. 2001
Created By#C0115361 Team