Multiple Choice
According to Newton's Law of Gravity, what is the magnitude of the net gravitational force exerted on the Sun by a planet of mass m orbiting at a distance r with gravitational constant G?
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Binary star: Two equal-mass stars maintain a constant distance D apart (Fig. 6–34) of 8.0 x 1011 m and revolve about a point midway between them at a rate of one revolution every 14.2 yr. Why don’t the two stars crash into one another due to the gravitational force between them?