|The Open Door Web Site|
Gravitational Field Strength
The g.f.s. at a point in a gravitational field is the force acting on a 1kg mass placed at that point.
Units of g.f.s. Nkg-1
From Newton’s second law of motion we can regard "force per unit mass" as being equivalent to acceleration.
Therefore, g.f.s. is another name for acceleration due to gravity.
Variation of g with distance from a point mass
Variation of g with distance from the centre of a uniform spherical mass of radius, R
Variation of g on a line joining the centres of two point masses
If m1 > m2 then
Gravitational Potential, V
The potential at a point in a gravitational field is equal to the work done bringing a 1kg mass from infinity to that point.
The units are Jkg-1.
To calculate work done by a force we use the equation w = F.s but in this situation it is a little more complicated because the force is not of constant magnitude.
However, we do know how the force varies with distance from the body (Newton’s law of universal gravitation) and it can be shown* that the work done, w, bringing a mass, m, from infinity to point p is given by:
where, M is the mass of the body (the earth, in this case).
A body at infinity, has zero gravitational potential. A body normally falls to its lowest state of potential (energy) so we must arrange that the equation for potential is such that, as r decreases, the potential decreases. We can do this by including a negative sign in the above equation. Then, as r decreases, V decreases (becomes a greater negative quantity).
Therefore, to calculate the potential at a point in the gravitational field of a point mass or a uniformly distributed spherical mass:
If a body is thrown upwards fast enough, it never comes back down: it has escaped from the planet. The velocity needed to do this is called the escape velocity of the planet.
As the body is moving away from the planet, it is losing kinetic energy and gaining potential energy.
To completely escape from the gravitational attraction of the planet, the body must be given enough kinetic energy to take it to a position where its potential energy is zero.
The potential energy possessed by a body of mass m, in a gravitational field is given by:
If the field is due to a planet of mass M and radius R, then the escape velocity can be calculated as follows:
Also, as g = GM/R˛