This quiz is designed to test knowledge on the basics of the planet Jupiter and its moons.
Titan, Triton, Europa, Ganymede
Io, Triton, Callisto, Europa
Titan, Callisto, Ganymede, Io
Io, Europa, Ganymede, Callisto
None of the above
Their orbits are nearly circular and lie in a plane
Their revolution direction (about Jupiter) are all the same
The average densities decrease with increasing distance from Jupiter
All of the above
None of the above
Io and Europa are believed to have rocky mantles and iron cores
Callisto is thought to have a large, outer icy mantle with a smaller inner rocky mantle and an iron core
Ganymede is thought to be mainly rock/ice mixture with little or no core
All of the above
None of the above
1 m high tidal buldge
10 m high tidal buldge
100 m high tidal buldge
1000 m high tidal buldge
None of the above
Indeed; thus it must be natural radioactivity in Io's Core that "powers" the volcanic activity
Indeed; and it is the additional tidal interaction with Europa that "powers" Io's volcanic activity
Indeed; but Io's non-circular orbit means Io's tidal buldge "wobbles" back and forth as Io fails to point perfectly toward Jupiter at all points in its orbit
None of the above
Photos from Voyager I showing erupting volcanoes
Io's lack of craters is consistent with almost constant "resurfacing" by molten flows
Io's thin atmosphere of sulfur dioxide is consistent with recent volcanic emissions
All of the above
None of the above
Larger than the state of Maryland
Emits more energy than all of Earth's volcanoes combined
Occasionally has lava temperatures far in excess of any of Earth's volcanoes
All of the above
None of the above
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Showing clear "ongoing" volcanic activity
Showing almost no cratering consistent with recent "resurfacing"
Having a vast network of lines crisscrossing bright, fields of water ice
All of the above
None of the above
Magma(molten rock)
Water
Liquid carbon dioxide
Liquid hydrocarbons (eg. methane)
None of the above
(conventional) rock
Ice
Dry ice
Linoleum
None of the above
Remnant heat from the formation of the moon
Gravitational and magnetic forces from Jupiter
Meteorite impacts intensified by the proximity of Jupiter
All of the above
None of the above
Bigger than either of Mars' moons
Bigger than Earth's moon
Bigger than Mercury
All of the above
None of the above
Always showing "one face" to Jupiter
Having many impact craters
Patterns of light and dark areas similar to maria and highlands on the moon
All of the above
None of the above
Light colored areas are younger and dark colored areas are older
Light colored areas are older and dark colored areas are younger
Light and dark areas are equally cratered
None of the above
Magma(molten rock)
Water
Liquid carbon dioxide
Liquid hydrocarbons (eg. liquid methane)
None of the above
Active volcanoes
Evidence for possible tectonic motion seen in grooves and ridges
Vast areas with no craters
All of the above
None of the above
More craters and fewer fault(grooves and ridges) lines
Fewer craters and more fault(grooves and ridges) lines
Several large "basins"
Both a) and c)
Both b) and c)
Caloris basin
Orientale basin
Argyre Planitia
Valhalla basin
None of the above
(conventional) rock
Ice
Dry ice
Linoleum
None of the above
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