All four ring systems orbit the equators of Jovian planets outside their Roche limits.
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Q21: Titan's surface has been mapped using Earth
Q22: The F- ring is held in place
Q23: The surface of Saturn's moon Enceladus is
Q24: Two sets of rings around Jovian planets
Q25: Probably the next satellite to get turned
Q27: Saturn's rings are thick, perhaps a few
Q28: A resonance with Mimas clears out the
Q29: Saturn's rings appear to be brighter and
Q30: Methane drives the weather of Titan, for
Q31: Spacecraft have imaged erupting volcanoes on Io
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