Keplers Third Law of Planetary Motion Keplers Third Law of
Chapter 2, Problem 55(choose chapter or problem)
Keplers Third Law of Planetary Motion Keplers Third Law of Planetary Motion states that the square of the period of revolution T of a planet varies directly with the cube of its mean distance a from the Sun. If the mean distance of Earth from the Sun is 93 million miles, what is the mean distance of the planet Mercury from the Sun, given that Mercury has a yearof 88 days?
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