# Episode 404: Gravitational potential energy

In this episode, students will appreciate the energy changes that take place as a body moves in a gravitational field. They have seen this concept before, for a uniform field, in the form Change in GPE = mgh, but this will be generalised to non-uniform fields around point or spherical masses. They will then be introduced to the concept of **potential** and its uses, before finally making the link between that rate at which potential changes from place to place and the field strength.

Note that the mention of infinity often gets students’ minds racing, and puzzling over seeming paradoxes such as “If the gravitational field is infinite in extent, what does it mean to be at infinity where the field is zero?” It’s best to approach this pragmatically; by infinity, we really mean as far away from all masses in the universe as we need to be to make the gravitational forces negligible in whatever context we are looking at.

This is quite a long episode, and worth spending the time on to give a good grounding in these ideas. They will be important again with electric fields.

**Summary**

- Discussion: Work, energy and gravitational potential energy (5 minutes)
- Worked examples: GPE in a constant field (10 minutes)
- Discussion: Potential energy in a non-uniform field (10 minutes)
- Discussion: Potential (5 minutes)
- Worked examples: Potential energy and potential (15 minutes)
- Student questions (15 minutes)
- Spreadsheet exercise (20 minutes)
- Discussion: Equipotentials, potential gradient and field strength (10 minutes)
- Spreadsheet exercise: Potential gradient and field strength (20 minutes)

**Discussion: Work, energy and gravitational potential energy**

This draws on what students should already know about work, energy and gravitational potential energy.

What is work? (Work is done when a force moves its point of application through some distance in the direction of the force. In the absence of frictional forces, this work done is stored as the energy of the body on which the force was acting.)

If I lift an object up from the floor to above my head (demonstrate it!), have I done work on it? (Yes. I applied an upwards force on the object which itself moved upward too.)

What happened to the work I did on the object? (It is stored as energy on the object. We call this stored energy gravitational potential energy. Gravitational because we have to do work against gravity to lift the object, and potential in the sense that the potential is realised when I let go of the object. If you have something breakable (but safe and cheap!) they will really see this potential being realised.)

**Worked examples: GPE in a constant field**

Now, students have come across these ideas before at pre-16 level in the form:

Change in GPE = mgh.

It is as well to revise this with a few worked examples now.

Episode 404-1: GPE in a constant field (Word, 26 KB)

**Discussion: Potential energy in a non-uniform field**

Now you can extend these ideas to potential energy in a non-uniform field.

All the previous examples involved potential energy changes near the surface of the Earth. What would be the problem if we wanted to use the same equation to work out energy changes for, say, a rocket launched to the moon? (The gravitational field strength is not constant – the value of g changes.)

We therefore need another way of calculating GPE changes in non-uniform fields. The full treatment of how we arrive at this formula requires off-syllabus calculus that would actually be accessible to more able students. We find that we can calculate GPE of a mass m at a point distance *r* from a (point or spherical) mass M by:

GPE = –GMm/r

There are several very important points to note about this equation:

- We know that the further you get from an object, the higher your GPE relative to it. (As something must have done more work against gravity to get you there). Thus when you are infinitely far away, you have as high a GPE relative to it as possible. We choose (arbitrarily) to make the value of GPE of all bodies at infinity zero. Then since this is the highest value of GPE, all real values of GPE (closer than infinity) must be negative. Therefore the minus sign in the equation is NOT optional; it must always be included and all values of potential energy in a gravitational field are negative. (This is not the case when we come on to electric fields, because they can be repulsive too).
- Note that we have written GPE here, and not “Change in GPE”. By defining a point relative to which all GPE is measured, we can now talk about
**absolute**values of GPE rather than just changes. This point is at infinity (see note 1 above). - Note that GPE follows an inverse proportion law (1/r) and not an inverse square law (1/r
^{2})

**Discussion: Potential**

The weight of an object in the Earth’s gravitational field depends upon the mass of the object (as well as the mass of the Earth). However, as we have already seen, the field strength at a point is independent of the object placed there (because it is defined as force per unit mass of the object). Thus we can think of field strength as a property of the field at a point, and not the particular object placed there.

Similarly, the GPE of a body at a place in the Earth’s field depends upon the mass of the object (as well as the mass of the Earth). How do you think we can get a quantity related to energy in the field at a point, which does not depend upon the object placed there? (By looking at the GPE per unit mass of the object, thus removing the dependence on the mass of the object just as we did with field strength.)

We define the potential at a point in a field as the gravitational potential energy *per unit mass* placed at that point in the field. We can get equations for potential using this definition. For a field due to a (point or spherical) mass M, we have:

GPE = –GMm/r

And so the potential, *V*, is given by:

V = (–GMm/r) / m = –GM/r

A few points to make:

- This only relates to the field due to a (point or spherical) mass M.
*V*is measured in J kg^{-1}. It follows an inverse proportion law (1/*r*) not inverse square (1/r^{2}).- Just as with the equation for GPE, the minus sign is not optional. All real potentials are negative, and the zero of potential is at infinity (since all objects have zero GPE at infinity).
- Potential, like field strength is a property of the field at a point, and is independent of the object placed there. Two objects with different masses at the same point in the field are subject to the same potential, but have different potential energies.
- For uniform fields (e.g. close to the surface of the Earth), we can use

change in potential = gh

(since change in GPE = mgh and potential = GPE/m).

(Potential will be returned to again when we study electric fields. There, differences in potential (or potential differences, pds) are what we often call voltages.)

**Worked examples:Potential energy and potential**

Episode 404-2: Potential energy and potential (Word, 30 KB)

**Student questions**

These questions relate to a spacecraft travelling from the Moon to the Earth.

You may wish to omit questions 3–5 inclusive if your students have not covered the topic of momentum.

Episode 404-3: Gravitational field between the Earth and the moon (Word, 74 KB)

**Spreadsheet exercise**

You can extend the spreadsheet activity from Episode 402 by including the idea of gravitational potential.

Episode 402-3: Data from the Apollo 11 mission (Word, 85 KB)

**Discussion: Equipotentials, potential gradient and field strength**

Equipotentials join points of equal potential. They are very simple in the cases of uniform fields (close to the surface of the Earth) and radial fields (for point and spherical masses):

How far apart are the equipotential lines in the first diagram? (Since change in potential for a constant field is simply gh (where h is change in height), we have gh = 9.8 J kg^{-1}. Therefore

h = 1m – the lines are 1 m apart.)

What shapes are equipotentials in the real world? (Equipotentials are surfaces rather than lines in the real 3-dimensional world (i.e. horizontal planes rather than lines close to the surface of the Earth, and concentric spheres rather than concentric circles about a point/spherical mass), but we can only capture a slice of them on paper.)

Equipotentials are always perpendicular to field lines. Diagrams of equipotential lines give us information about the gravitational field in much the same way as contour maps give us information about geographical heights.

What does it mean on a contour map if the contours are very close together? (On a contour map, the contours may be marked off at, say, 5 m intervals. Therefore, if they are close together, it means that the land on which they lie must be very steep.)

What do you think it therefore means if equipotential surfaces are close together? (An educated guess would be that it means that the gravitational field is very strong there. That would be correct – if the equipotentials are close together, a lot of work must be done over a relatively short distance to move a mass from one point to another against the field – i.e. the field is very strong. Hence on the drawing above of the equipotentials around point or spherical masses, the equipotential surfaces get further and further apart as the field strength decreases with distance.)

In fact, the field strength is given by the negative of the gradient of the potential:

g = -dV/dr

For students that might struggle with a derivative as above, it could be introduced as*:*

g = – (change in potential / change in distance).

**Spreadsheet exercise: Potential gradient and field strength**

In this exercise, students will manipulate (calculated) raw data on the variation of potential with height above the Earth’s surface. By the end, they will calculate the change in potential per metre (i.e. the potential gradient) and compare it to field strength and find that the two are equal. When they calculate the change in potential between say 200 km and 300 km, and divide it by the 100 km distance to get a field strength, they are actually getting an **average** field strength between 200 km and 300 km, which is likely to be very close to the field at 250 km (though not exactly because the variation in potential is non-linear). Hence the field strengths on sheet 2 being given at 50 km, 150 km, etc.

They are expected to have used spreadsheets before and are asked to do some fairly simple spreadsheet manipulations.

Episode 404-5: Potential gradient and field strength (Word, 28 KB)

Episode 404-6: Excel file “potential gradient and field strength” (Word, 53 KB)

**Download this episode**

Episode 404: Gravitational potential energy (Word, 221 KB)