Solve the following variance problem Kepler s third law of

Last updated: 6/15/2023

Solve the following variance problem Kepler s third law of planetary motion states that the square of the time required for a planet to make one revolution about the sun varies directly as the cube of the average distance of the planet from the sun If you assume that Mars is 1 5 times as far from the sun as is the earth find the approximate length of a Martian year