The magnitude of the gravitational force at distance r1 and r2 from the centre of a uniform sphere of radius R and mass M are F1 and F2 respectively. Then,
A
F1F2=r1r2ifr1<Randr2<R
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B
F1F2=r21r22ifr1>Randr2>R
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C
F1F2=r1r2ifr1>Randr2>R
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D
F1F2=r22r21ifr1<Randr2<R
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