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Imagine of a light planet revolving around a massive star in a circular orbit of radius r with a period of revolution T. If the gravitational force of attraction between the planet and the star is proportional to r52, then the square of the time period will be proportional to

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Imagine of a light planet revolving around a massive star in a circular orbit of radius r with a period of revolution T. If the gravitational force of attraction between the planet and the star is proportional to r52, then the square of the time period will be proportional to



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