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Gravitation question

2004 · Shift 0 · Q168
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  5. /2004 · Shift 0 · Q168

Gravitation question

2004 · Shift 0 · Q168

JEE MainPhysicsGravitationMCQ+4 / −1
Suppose the gravitational force varies inversely as the nth power of distance. Then the time period of a planet in circular orbit of radius RRR around the sun will be proportional to
  1. A
    Rn{R^n}Rn
  2. B
    R(n−12){R^{\left( {{{n - 1} \over 2}} \right)}}R(2n−1​)
  3. C
    R(n+12){R^{\left( {{{n + 1} \over 2}} \right)}}R(2n+1​)
  4. D
    R(n−22){R^{\left( {{{n - 2} \over 2}} \right)}}R(2n−2​)
View written solutionFree

Correct answer: C

  1. Given law of gravitation

    The gravitational force is said to vary inversely as the nnnth power of distance: F∝1RnF \propto \frac{1}{R^n}F∝Rn1​

  2. For circular motion

    A planet of mass mmm moving in a circular orbit of radius RRR requires centripetal force: Fc=mv2RF_c = \frac{mv^2}{R}Fc​=Rmv2​

    This centripetal force is provided by gravity, so mv2R∝1Rn\frac{mv^2}{R} \propto \frac{1}{R^n}Rmv2​∝Rn1​

  3. Find the speed dependence on RRR

    Multiplying by RRR: mv2∝1Rn−1mv^2 \propto \frac{1}{R^{n-1}}mv2∝Rn−11​ v2∝R−(n−1)v^2 \propto R^{-(n-1)}v2∝R−(n−1) v∝R−n−12v \propto R^{-\frac{n-1}{2}}v∝R−2n−1​

  4. Time period of revolution

    The time period is T=2πRvT = \frac{2\pi R}{v}T=v2πR​

    Substituting the proportionality for vvv: T∝R⋅Rn−12T \propto R \cdot R^{\frac{n-1}{2}}T∝R⋅R2n−1​ T∝R1+n−12T \propto R^{1 + \frac{n-1}{2}}T∝R1+2n−1​ T∝Rn+12T \propto R^{\frac{n+1}{2}}T∝R2n+1​

  5. Match with the options

    Therefore, T∝Rn+12T \propto R^{\frac{n+1}{2}}T∝R2n+1​

    This corresponds to Option C.

  6. Verification with stored answer

    Stored correct answer: C

    Derived answer: C

    So, the derived answer agrees with the stored answer.

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