SOLUTION: Kepler’s third law of planetary motion may be given as where T is the time for one revolution of a planet around the sun, r is its mean radius from the sun, and year/mi. Fin
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Question 252846: Kepler’s third law of planetary motion may be given as where T is the time for one revolution of a planet around the sun, r is its mean radius from the sun, and year/mi. Find the time for one revolution of Venus about the sun if miles.
Anyone have any idea how to solve this one? If so, would you mind showing me your steps so I can figure it out as well? Thank you kindly.
Answer by richwmiller(17219) (Show Source): You can put this solution on YOUR website!
check this out
http://milan.milanovic.org/math/english/kepler/kepler.html
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