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Best Answer: Its really quite amazing how much information like this can be found online in about 3 seconds. Revolution, or orbital period: 30,799.095 days (84.323 326 yr). Rotation period, or "day": 0.718 33 day (17 h 14 min 24 s)

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A. there is more sunlight incident on Uranus's rings because of its greater distance from the Sun. B. they have a lot of carbon/soot-like material in them. C. they do not have as much nuclear activity in them, so they do not produce as much light. D. there is less sunlight incident on Uranus's rings because of its smaller distance from the Sun.

forum.cosmoquest.org/archive/index.php/t-26638.html

The magnetic field itself is in fact tilted 60 degrees from the planet's axis of rotation. The magnetotail was shown to be twisted by the planet's rotation into a rather long "corkscrew" shape behind the planet. Its just a plain unusual position.

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With the transit method, you would only know how long the background star was occulted, but you wouldn&#39;t know whether it was by a small close object or a large distant one.<br /><br />At least one group announced the observation of a large outer Solar System body in this way, but their observation in the given region of the sky could not be reproduced.

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forum.cosmoquest.org/archive/index.php/t-28365.html

Too little is known about structures of plasmas under high pressures. I doubt if H+ ions or He ions would arrange themselves into a rigid structure at solar pressures.

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