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Jupiter’s Physical Properties
Mass is twice as much as all other planets put together
Diameter is 11.2 times greater than Earth’s
Density is much less than terrestrial planets, so it cannot be rocky or metallic
Rotation rate is problematic, as Jupiter has no solid surface
differential rotation
when different parts of Jupiter’s atmosphere rotate at different rates
zonal flow
stable flow in Jupiter’s atmosphere that underlies the zones and bands
Great Red Spot
a surface feature on Jupiter that has existed for at least 300 years; produces an anticyclonic storm that is the largest in the Solar System
“Brown Oval”
a large gap in the clouds of Jupiter that is relatively calm compared to the storms on the planet
Shoemaker-Levy 9
a comet that struck Jupiter in fragments in July 1994; provided valuable information about cometary impacts
“plasma torus”
a slightly growing belt of atoms along the orbit of Io
Galilean moons
the term used to describe the four largest moons on Jupiter (Io, Europa, Ganymede, and Callisto) because they were first observed by Galileo
Io
the densest of Jupiter's moons, and the most geologically/volcanically active object in the Solar System
Europa
the moon on Jupiter that has no craters, and its surface is water ice, possibly with liquid water below
Ganymede
the largest moon in the Solar System, which is larger than Pluto and Mercury
Callisto
the moon on Jupiter that is similar to Ganymede and has no evidence of plate activity