Define gravitational potential energy. derive expression for gravitational potential energy in the gravitational field of earth at distance from center of the earth

Physics

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Answer

U(r)=−GMmrU(r) = -\frac{GMm}{r}

Step-by-step solution

3 steps

Gravitational potential energy is the energy an object possesses due to its position within a gravitational field. It is defined as the work done by an external force to move an object from a reference point (usually infinity) to a specific point in the gravitational field without accelerating it.

Derivation of the expression for gravitational potential energy:

  1. Define the work done by an external force.

    The work done dWdW by an external force to move a mass mm by an infinitesimal distance drdr against the gravitational force is given by:

    dW=Fext⋅drdW = F_{ext} \cdot dr

    The gravitational force FgF_g between Earth (mass MM) and an object (mass mm) at a distance rr from Earth's center is given by Newton's Law of Universal Gravitation:

    Fg=−GMmr2F_g = -\frac{GMm}{r^2}

    The negative sign indicates that the force is attractive, directed towards the center of Earth. To move the object without acceleration, the external force FextF_{ext} must be equal in magnitude and opposite in direction to the gravitational force:

    Fext=−Fg=GMmr2F_{ext} = -F_g = \frac{GMm}{r^2}
  2. Calculate the total work done.

    The gravitational potential energy U(r)U(r) at a distance rr from the center of Earth is the total work done to bring the mass mm from infinity (where potential energy is conventionally zero) to the distance rr.

    U(r)=∫∞rdW=∫∞rFext⋅drU(r) = \int_{\infty}^{r} dW = \int_{\infty}^{r} F_{ext} \cdot dr

    Substitute the expression for FextF_{ext}:

    U(r)=∫∞rGMmr2drU(r) = \int_{\infty}^{r} \frac{GMm}{r^2} dr
  3. Perform the integration.

    U(r)=GMm∫∞rr−2drU(r) = GMm \int_{\infty}^{r} r^{-2} dr U(r)=GMm[r−1−1]∞rU(r) = GMm \left[ \frac{r^{-1}}{-1} \right]_{\infty}^{r} U(r)=GMm[−1r]∞rU(r) = GMm \left[ -\frac{1}{r} \right]_{\infty}^{r} U(r)=GMm(−1r−(−1∞))U(r) = GMm \left( -\frac{1}{r} - \left(-\frac{1}{\infty}\right) \right)

    Since 1∞=0\frac{1}{\infty} = 0:

    U(r)=GMm(−1r−0)U(r) = GMm \left( -\frac{1}{r} - 0 \right) U(r)=−GMmrU(r) = -\frac{GMm}{r}

    The expression for gravitational potential energy at a distance rr from the center of Earth is:

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