Use the information below and the relationship above to calculate the T2/R3 ratio for the planets about the Sun, the moon about the Earth, and the moons of Saturn about the planet Saturn. The value of G is 6.673 x 10-11 N•m2/kg2. Sun M = 2.0 x 1030 kg Earth M = 6.0 x 1024 kg Saturn M = 5.7 x 1026 kg a. T2/R3 for planets about sun b. T2/R3 for the moon about Earth c. T2/R3 for moons about Saturn

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Newton's First Law of Motion

If a very smooth ball is rolled down an inclined surface with zero friction, the ball will continue to roll indefinitely for an infinite time, in an attempt to reach to the same height on the opposite hill!