Gravitation
1.0 Newton's law of gravitation
1.1 Characteristics of gravitational force
1.2 Universal gravitational constant
1.3 Principle of superposition of gravitation
1.4 Gravity
1.5 Acceleration due to gravity
1.6 Relation between $g$ and $G$
2.0 Variation of acceleration due to gravity
2.1 Variation of acceleration due to gravity $(g)$ due to shape of the earth
2.2 Variation of acceleration due to gravity $(g)$ due to altitude
2.3 Variation of acceleration due to gravity $(g)$ due to depth
2.4 Variation of acceleration due to gravity $(g)$ due to rotation of earth
3.0 Gravitational field
3.1 Gravitational field due to a point mass
3.2 Gravitational field due to a uniform solid sphere
3.3 Gravitational field due to a uniform spherical shell
3.4 Gravitatioal field due to a uniform circular ring at a point on its axis
4.0 Gravitational potential
4.1 Gravitational potential due to a point mass
4.2 Gravitational potential due to a uniform solid sphere
4.3 Gravitational potential due to a uniform thin spherical shell
4.4 Gravitational potential due to a uniform ring at a point on its centre
4.5 Relation between gravitational field and gravitational potential
5.0 Gravitational potential energy
5.1 Gravitational potential energy for a system of particles
5.2 Gravitational potential energy of a body on earth's surface
6.0 Satellites
6.1 Orbital speed of satellite
6.2 Time period of a satellite
6.3 Angular momentum of a satellite
6.4 Energy of a satellite
6.5 Types of satellite
6.6 Binding energy
6.7 Escape velocity
6.8 Weightlessness
7.0 Kepler's law of planetary motion
8.0 Problem solving technique
3.3 Gravitational field due to a uniform spherical shell
1.2 Universal gravitational constant
1.3 Principle of superposition of gravitation
1.4 Gravity
1.5 Acceleration due to gravity
1.6 Relation between $g$ and $G$
2.2 Variation of acceleration due to gravity $(g)$ due to altitude
2.3 Variation of acceleration due to gravity $(g)$ due to depth
2.4 Variation of acceleration due to gravity $(g)$ due to rotation of earth
3.2 Gravitational field due to a uniform solid sphere
3.3 Gravitational field due to a uniform spherical shell
3.4 Gravitatioal field due to a uniform circular ring at a point on its axis
4.2 Gravitational potential due to a uniform solid sphere
4.3 Gravitational potential due to a uniform thin spherical shell
4.4 Gravitational potential due to a uniform ring at a point on its centre
4.5 Relation between gravitational field and gravitational potential
5.2 Gravitational potential energy of a body on earth's surface
6.2 Time period of a satellite
6.3 Angular momentum of a satellite
6.4 Energy of a satellite
6.5 Types of satellite
6.6 Binding energy
6.7 Escape velocity
6.8 Weightlessness
- 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,