Physics > Gravitation > 4.0 Gravitational potential

  Gravitation
    1.0 Newton's law of gravitation
    2.0 Variation of acceleration due to gravity
    3.0 Gravitational field
    4.0 Gravitational potential
    5.0 Gravitational potential energy
    6.0 Satellites
    7.0 Kepler's law of planetary motion
    8.0 Problem solving technique

4.3 Gravitational potential due to a uniform thin spherical shell
The gravitational potential due to a spherical shell of radius $R$ and mass $M$ at a distant $r$ from the centre of the shell is given as follows,

  • At a point outside the shell, i.e. $r>R$ $$V = - \frac{{GM}}{r}$$
  • At a point on the surface of the shell, i.e. $r=R$ $$V = - \frac{{GM}}{R}$$
  • At a point inside the shell, i.e. $r>R$ $$V = - \frac{{GM}}{R}$$

Proof: At a point outside the shell


The spherical shell behaves like a point mass for a point outside the sphere,

So, the gravitational potential outside the sphere is, $$V = - \frac{{GM}}{r}$$
Similarly, gravitational potential on the surface of spherical shell, i.e. $(r=R)$ is, $$V = - \frac{{GM}}{R}$$


Proof: At a point inside the shell


The gravitational field at any point inside the spherical shell is zero. So, the gravitational potential at all point inside the spherical shell is equal to the potential at the surface.

Therefore, $$V = - \frac{{GM}}{R}\quad {\text{for}}\quad r < R$$


Note: The gravitational potential due to a uniform spherical shell varies as,
$$V = - \frac{{GM}}{r}\quad {\text{for}}\quad r \geqslant R$$
$$V = - \frac{{GM}}{R}\quad {\text{for}}\quad r \leqslant R$$
The $V$ vs $r$ can be drawn using the above equations as,


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