5.2.1Forces and Motion
Gravitational Potential Energy
5 min read 7 parts Lesson 41 of 66 1 quiz Virtual lab
Lesson summary
5.2.1 Gravitational Potential Energy — AS PHYSICS 9702 notes: Derive and use ΔEp = mgΔh for a uniform gravitational field.Definition — energy stored in a mass due to its position in a gravitational field.A mass that is lifted gains gravitational potential energy.A mass that falls…
- Reference level
- What the symbols mean
- Against time
- Gravitational field strength
- Uniform field
- Kinetic energy
Section 1 of 7Gravitational potential energy
Definition
- Definition energy stored in a mass due to its position in a gravitational field.
- A mass that is lifted gains gravitational potential energy.
- A mass that falls loses gravitational potential energy.
Reference level
- Reference level the potential energy at ground level on the Earth's surface is taken as zero.
Section 2 of 7Derivation of Ep = mgh
Lifting a mass m through a height h needs an upward force equal to its weight, mg.
The work done is W = Fs = mgh.
The lifted mass can now do extra work equal to mgh.
What the symbols mean:
This extra work equals the gain in gravitational potential energy, Ep = mgh.
What the symbols mean: Ep = gravitational potential energy gained (J) · m = mass (kg) · g = 9.81 N kg−1 · h = change in height (m)
Section 3 of 7The equation
Equation
- ΔEp = mgΔh.
- Ep is gravitational potential energy in joules (J).
- m is mass in kilograms (kg).
- g is gravitational field strength in N kg−1.
- Δh is change in height in metres (m).
Validity
- Validity the equation applies only to energy changes in a uniform gravitational field, such as near the Earth's surface.
- In space, where the field is not uniform, this equation is not used.
Section 4 of 7GPE against height graphs
Shape
- Shape a graph of GPE against height is a straight line, so GPE and height have a linear relationship.
Gradient
- Gradient the gradient equals mg.
Against time
- Against time the graph for a ball thrown upward or falling is identical in form when plotted against time.
Section 5 of 7More from the specification
1Potential energy and terminal speed
- Potential energy and terminal speed converting gravitational potential into kinetic energy governs falling mass acceleration until drag forces limit terminal speed.
2Gravitational potential energy in uniform fields
- In a uniform gravitational field near Earth's surface, the change in potential energy is given by Ep = mgh.
3Conservation of mechanical energy
- In the absence of dissipative friction or air resistance, total mechanical energy is conserved, linking velocity change to vertical displacement.
4Work-energy theorem in non-uniform fields
- Gravitational potential in radial fields is defined as work done per unit mass bringing a test mass from infinity: Vg = -GM/r.
5Gravitational potential energy in uniform fields
- In a uniform gravitational field near Earth's surface, the change in potential energy is given by Ep = mgh.
6Conservation of mechanical energy
- In the absence of dissipative friction or air resistance, total mechanical energy is conserved, linking velocity change to vertical displacement.
7Work-energy theorem in non-uniform fields
- Gravitational potential in radial fields is defined as work done per unit mass bringing a test mass from infinity: Vg = -GM/r.
8Velocity
- Rate of change of displacement.
9Displacement
- Change in position.
10Newton
- Unit of force, kg m s-2.
11Kinetic energy
- K = ½mv2, energy of motion.
12Energy transferred
- W = V Q, in joules.What the symbols mean: E or W = energy transferred (J) · Q = charge (C) · V = potential difference (V) · I = current (A) · t = time (s)
Section 6 of 7Key terms
| Term | Meaning |
|---|---|
| Gravitational potential energy | Energy stored in a mass because of its position in a gravitational field. |
| Gravitational field strength | Force per unit mass on a mass in a gravitational field, g, in N kg⁻¹. |
| Uniform field | Field with the same strength and direction at every point, as near the Earth’s surface. |
| Work done | Force multiplied by displacement in the direction of the force. |
Section 7 of 7Exam technique
1
Using the distance along a slope — only the vertical height change counts.
2
Using the equation far from the Earth where g is not constant.
3
Forgetting that only changes in potential energy matter, not absolute values.
4
Mixing units — mass must be in kg and height in m.