SOLUTION: Kepler’s third law of planetary motion may be given as T=kr^3/2 where T is the time for one revolution of a planet around the sun, r is its mean radius from the sun, and k=1.1
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Question 285923: Kepler’s third law of planetary motion may be given as T=kr^3/2 where T is the time for one revolution of a planet around the sun, r is its mean radius from the sun, and k=1.115 (10)^-12 year/mi. Find the time for one revolution of Venus about the sun if r=6.73(10)^7 miles. Answer by richwmiller(17219) (Show Source):
