Key points: Captured moons; Galilean moon properties; interiors of the Galilean moons and how they formed
This animation shows all the moons in orbit around Jupiter, which is
in the center. You can see the inner moons in regular orbits and how much farther away
from Jupiter the rest are. This distribution emphasizes how most of the moons are captured
into orbits where they are only loosely held. (from Tony Dunn, Gravity
Simulator, http://www.orbitsimulator.com/gravity/articles/joviansystem.html)
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In order of distance from Jupiter:
From Galileo mission, http://www.jpl.nasa.gov/galileo/images/images.html
Artist's impression of Io (William Hartmann) |
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(From Galileo Mission, http://www.jpl.nasa.gov/galileo/images/images.html)
A closeup (smallest features about 10km across). From Galileo mission, http://www.jpl.nasa.gov/galileo/images/images.html |
Two artist's impressions of the surface of Europa (Don Dixon) |
Ganymede:
largest moon in the solar system; Ganymede is larger than Mercury
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Left: different terrains on Ganymede. Can you tell which area is younger? (hint: count craters) From Galileo mission, http://www.jpl.nasa.gov/galileo/images/images.html |
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Artist's impression of the surface of Ganymede (Don Dixon) |
Callisto:
From Galileo mission, http://www.jpl.nasa.gov/galileo/images/images.html
Artist's impression of the surface of Callisto (to right) (Don Dixon)
The interiors of Io, Europa, Callisto, and Ganymede, clockwise from upper left. All except Callisto have metallic (iron/nickel) cores, shown in gray, surrounded by rock in brown. The rock shells in Europa and Ganymede are surrounded by liquid water (blue) and ice (white). Callisto is shown as an undifferentiated mixture of ice and rock. (from John Brodholt, http://slamdunk.geol.ucl.ac.uk/~brodholt/) |
Notice the pattern in
properties of the Galilean moons with increasing distance from Jupiter:
less differentiated core
This trend mimics the trend in properties of planets with distance from the Sun. The properties of the moons indicate that they formed as small objects around a large one, with similar consequences to the formation of the (relatively) small planets around the much larger sun. A combination of heating by the central object and the larger energy of collisions due to the high orbital velocities close to it can account for these trends in both cases.
Shani, Vedic god of Saturn, http://www.payer.de/kommkulturen/kultur123.htm |
Huygen's drawing explaining the various aspects of the rings of Saturn. http://www.surveyor.in-berlin.de/himmel/Bios/Huygens-e.html |
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Click to return to Saturn, Uranus, and Neptune | hypertext G. H. Rieke |
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