Question: Keplers third law of planetary motion may be given as T = kr 3/2 , where T is the time for one revolution of a
Kepler’s third law of planetary motion may be given as T = kr3/2 , 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/mi3/2. Find the time for one revolution of Venus about the sun if r = 6.73 × 107mi.
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