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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 on the gravitational force of attraction between the planet and the star is proportional to r^(-5//2) |
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Answer» Solution :The RESULTANT gravitational force PROVIDES NECESSARY centripetal force `(mV^2)/R=(K)/(r^(5//2))impliesV^(2)=K/(mr^(3//2))` So that `T = (2pir)/V=2pirsqrt(("mr"^(3//2))/K)` So `T^(2) prop r^(7//2)` |
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