Gravitational potential and gravitational potential energy
In a nutshell
Gravitational potential is defined as the work done per unit mass, moving a mass from infinity to its position in the gravitational field. Gravitational potential energy depends on the mass and where the mass is in the gravitational field. Escape velocity is the minimum velocity needed to escape a gravitational field.
Equations
Description
Equation
Gravitational potential
Vg=−rGM
Gravitational potential energy
E=−rGMm
Escape velocity
vescape=r2GM
Constants
name
symbol
value
Gravitationalconstant
G
6.67×10−11Nm2kg−2
Variable definitions
Quantity Name
Symbol
Derived Unit
SI BASE Units
gravitationalpotential
Vg
Jkg−1
m2s−2
mass
M
kg
kg
mass(ofobject)
m
kg
kg
distance
r
m
m
Gravitational potential
Gravitational potential is defined as the work done per unit mass, moving a mass from infinity to its position in the gravitational field.
In a radial field, like most celestial objects including Earth, is give as:
Vg=−rGM
Curiosity: The equation for gravitational potential is negative as work has to be done against the gravitational field to move a mass out of it. The maximum value gravitational potential can have is 0J at a distance of infinity from a gravitational field.
The graph for gravitational potential against distance looks like this:
For a tangent of the curve, the gradient would be given as:
gradient=ΔrΔVg
Substituting in the equation for Vg:
gradient=rrGMgradient=r2GMgradient=−g
The gradient of a gravitational potential graph against distance gives the gravitational field strength g. So gravitational field strength is the rate of change of gravitational potential with respect to the distance.
Consider two masses at different distances in a gravitational field. The masses will have different gravitational potentials due to having different distances. This means there is a potential difference between the two masses.
Work done against gravity
When you move a mass further away in a gravitational field, work is being done against gravity and the amount of work depends on where in the field the mass is.
Astronauts on the International Space Station can move "heavy" objects around easily as the gravitational field of Earth is very weak, so the work done is much less than moving the same object on the surface of Earth.
This can be shown as:
ΔW=mΔVg
The work done is the product of the mass and change in gravitational potential.
Another graphical relationship is how the size of a force on an object changes due to the distance away from a gravitational field.
For two points on the curve, the area underneath represents the work done moving the object from one point to the other.
Gravitational potential energy
As gravitational potential is defined as the work done per unit mass, the work done, or energy transferred, can be given as:
E=mVg
Substituting in the equation for Vg:
E=−rGMm
Example
The International Space Station has a mass of 420000kg and orbits the Earth at a distance of 408km . Calculate the gravitational potential energy of the International Space Station..
Note: The orbital distance needs to be added to the radius of the Earth as the distance is from the centre of the Earth and not the surface.
Make sure to include units and round to the lowest number of significant figures of the values given by the question:
gravitationalpotentialenergy,E=2.47×1013J
The gravitational potential energy of the International Space Station is 2.47×1013J.
Escape Velocity
In order to escape a gravitational field, the object must have enough kinetic energy to leave the field.
The escape velocity is given as the minimum velocity required, so when calculating the energy, the minimum amount of kinetic energy is used.
To obtain an equation for the escape velocity, consider when the kinetic energy is just enough to escape the gravitational field, so that the object has a net energy of zero: