User:Inconspicuum/Physics (A Level)/Gravitational Fields

The gravitational field, or gravitational field strength is the force exerted by gravity on an object per. unit mass of the object:

$g={\frac {F_{grav}}{m}}$

As gravitational field strength is a measure of the force exerted on each unit of mass, its unit is Nkg^-1. If we consider a planet, Body A, the gravitational field strength experienced by another object, Body B, is given by:

$g={\frac {\frac {-GMm}{r^{2}}}{m}}={\frac {-GM}{r^{2}}}$

Dimensions :- $[g]={\frac {M}{L^{2}}}=ML^{-}2$

This is the total force exerted on Body B divided by the mass of Body B. Inside the planet, force is proportional to the distance from the centre, so the field is also proportional to distance.

Acceleration

Force is given by:

$F=ma$

This means that:

$g={\frac {ma}{m}}=a$

This shows that the gravitational field strength is also the acceleration due to gravity on any object. This acceleration is the same for any object, regardless of mass. When considering small heights above the Earth's surface, such as those in our day-to-day experiences, g remains roughly constant.

Field Lines

Gravitational field lines around the Earth.

The gravitational field can be represented using field lines. These run in the direction that a mass would be accelerated in initially. The object will not necessarily fall along the field lines, but the acceleration will always be in the direction of the field lines. The closer the field lines are together, the denser the gravitational field.