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Imagine a light planet revolving around a very massive star in a circular orbit of radius .r. with a period of revolution T. On what power of r will the square of time period depend if the gravitational force of attraction between the planet and the star is proportional to r^(-5//2) |
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Answer» Solution :Here GRAVITATIONAL force PROVIDES centripetal force, `(mv^2)/( r) = (K)/(r^(5//2)) rArr V^2 = (K)/(MR^(3//2)) rArr T = (2pi r)/(v) = 2pi r sqrt((mr^(3//2))/(K)) rArr T^2 prop r^(7//2)` |
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