Physics > Gravitation > 3.0 Gravitational field

  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

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

  • At a point outside the shell i.e. $r>R$
    $$E = \frac{{GM}}{{{r^2}}}\quad {\text{or}}\quad \overrightarrow E = - \frac{{GM}}{{{r^2}}}\widehat r$$

  • At a point on the surface of the shell i.e. $r=R$
    $$E = \frac{{GM}}{{{R^2}}}\quad {\text{or}}\quad \overrightarrow E = - \frac{{GM}}{{{R^2}}}\widehat R$$

  • At a point inside the shell i.e. $r<R$
    $$E=0$$

Proof:

At a point outside the shell


The force on mass $m$ due to a spherical shell of mass $M$ is given by, $$F = \frac{{GMm}}{{{r^2}}}$$

So, the gravitational field is given by, $$E = \frac{F}{m}$$ or $$E = \frac{{GM}}{{{r^2}}}$$


At a point on the shell


Force on mass $m$ due to spherical shell of mass $M$ at the surface is given by,

$$F = \frac{{GMm}}{{{R^2}}}$$
So, the gravitational field is given by, $$E = \frac{F}{m}$$ or $$E = \frac{{GM}}{{{R^2}}}$$


At a point inside the shell


The force on mass $m$ inside the spherical shell of mass $M$ is zero as no mass is present inside the shperical shell.

$$F=0$$
So, gravitational field is also zero.
$$E = \frac{F}{m} = 0$$


Note: The gravitational field due to a uniform spherical shell varies as,
$$E = \frac{{GM}}{{{r^2}}}\quad {\text{or}}\quad E \propto \frac{1}{{{r^2}}}\quad {\text{for}}\quad r \geqslant R$$
$$E = 0\quad {\text{for}}\quad r < R$$
The $E$ vs $r$ graph can be drawn using the above equation is,


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