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Imagine a light planet is revolving round a very massive star in a circular orbit of radius R with a time period of revolution T. If the gravitational force of attraction between the star and planet is proportional to R-n, then T2 is proportional to 

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By Expert Faculty of Sri Chaitanya
a
Rn+1
b
Rn+2
c
Rn–1
d
Rn–2

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detailed solution

Correct option is A

FRnF=KRn
Gravitational Force provides necessary centripetal Force
mRω2=KRnmR4π2T2=KRnT2=mR4π2KRnT2Rn+1


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