A) Triton, a moon of Neptune
B) Io, a moon of Jupiter
C) Titan, a moon of Saturn
D) Earth's Moon
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A) No.
B) Yes, every 6 months just like Earth.
C) Yes, every 42 years.
D) Yes, every 84 years.
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A) Earth's Moon
B) Neptune's satellite Triton
C) Jupiter's satellite Ganymede
D) Saturn's satellite Titan
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A) tidal distortion by Jupiter and its other moons.
B) its original heat of formation.
C) nuclear fission within its interior.
D) radioactive elements in its surface.
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A) Titan
B) Charon
C) Callisto
D) Ganymede
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A) since the first spacecraft flybys by Pioneer I in 1979
B) since 1948, when the Mount Palomar telescope was completed
C) since Galileo turned his telescope toward the sky in 1610
D) since the time of the ancient Greeks
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A) Holes punched through the clouds, and craters gouged Jupiter's surface.
B) There were essentially no visible effects because the fragments plummeted deep below the cloud layers before being destroyed.
C) Rings of debris were flung into orbit around Jupiter's equator.
D) Fireballs hotter than the Sun's surface made dark splotches that lasted for months.
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A) Europa, a moon of Jupiter
B) Titan, a moon of Saturn
C) Triton, a moon of Neptune
D) Io, a moon of Jupiter
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A) jets of ice water shooting into the atmosphere
B) a uniformly and heavily cratered surface
C) stripes of recently formed material
D) a magnetic field
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A) Average density increases with distance from the planet.
B) Average density shows no pattern with distance; the highest-density moon is Ganymede, the largest moon.
C) Average density is the same for all moons because they were made from the same material.
D) Average density decreases with distance from the planet.
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A) impacts by cometary debris
B) cracking of the surface caused by shrinkage of the moon as it cooled
C) cracking of the icy surface, releasing water that expanded as it froze into ice
D) flow of water on the solid surface of the moon at some time in the past, which subsequently shrank as it froze into this distinctive terrain
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A) not be present at any point on the planet because dense clouds shield it from climate changes.
B) be nonexistent because such variations at any point on the planet will be smoothed out during its long "year" by the planet's rapid rotation.
C) be almost nonexistent because Uranus moves in an almost perfectly circular orbit and its distance from the Sun remains constant.
D) be extreme because its spin axis is nearly in its orbital plane.
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A) water and steam
B) molten lava
C) methane and ammonia
D) sulfur and sulfur dioxide
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A) Venus
B) Earth's Moon
C) Earth
D) Jupiter
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A) an icy crust showing two interlocking types of terrain, one ancient and heavily cratered, the other younger with systems of parallel grooves.
B) rock, heavily cratered like the highlands of Earth's Moon.
C) a relatively young, icy crust covered with a network of streaks and cracks and only a few impact craters.
D) a very dark and ancient icy crust covered with numerous craters, with no surface cracks or groove belts that would indicate internal activity.
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A) gaseous hydrogen
B) liquid hydrogen
C) solid metallic hydrogen
D) Rocks
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A) strong winds blowing eastward at all latitudes so that the entire atmosphere rotates faster than the planet.
B) isolated cyclones (low-pressure areas) and anticyclones (high-pressure areas) , similar to those on Earth.
C) strong winds blowing parallel to the equator but in opposite directions at different latitudes.
D) strong winds blowing westward at all latitudes so that the entire atmosphere rotates more slowly than the planet.
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A) Europa
B) Io
C) Callisto
D) Ganymede
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A) almost entirely water in liquid form or as ice
B) large iron core, the rest rock
C) half rock, half water and ice
D) a metallic core of high density with one-quarter of its mass composed of water and ice
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A) cracks on the surface
B) heat to keep subsurface water liquid
C) water geysers
D) lava/sulfur volcanoes
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