D.1.9 (HL)—Potential gradient
- Syllabus
- First assessment 2025
- Objective
- —
- Level
- HL
Use the gradient relationship
Gravitational field strength is the negative spatial gradient of gravitational potential. For a graph, use the tangent gradient at the required point; the negative sign makes the field point toward decreasing potential.
g=-\frac{\Delta V_g}{\Delta r}
Worked example — graph gradient
If a tangent changes by 3.8×108Jkg−1 over 4.2×107m, then ∣g∣=(3.8×108)/(4.2×107)=9.0Jkg−1m−1=9.0Nkg−1. Direction comes from the negative gradient.
Read a potential–distance graph
The gradient is ΔVg/Δr, with units Jkg−1m−1=Nkg−1. A negative slope gives a positive outward radial magnitude only after the vector direction and sign convention are interpreted. Near a source, the potential changes more rapidly with distance, so the field is stronger.
Connect to work
For a mass m moved between two points, W=mΔVg is the work done on the mass by the external agent under the stated sign convention. The field strength relation is local; potential difference and work compare endpoints.
Common trap
Do not use the average slope over a wide curved section as the field at one point unless the question’s graph is effectively linear there. Do not drop the negative sign without stating whether you are reporting a vector component or a magnitude.
Questions read field strength from a potential–distance graph or connect an equipotential spacing to the acceleration of a test mass.
Determine / What is
Find the local tangent gradient of Vg against r, apply g=−ΔVg/Δr, keep units consistent, and interpret the sign as field direction.
Using the graph’s height instead of its gradient, or reporting the slope sign without interpreting the negative in g=−ΔVg/Δr.
Representative question
A point mass of 5 kg is placed at point P located on one of three gravitational equipotential lines, each separated by a distance of 100 km , as shown.
What is the initial acceleration of the point mass?
4 m s−2 to the left
4 m s−2 to the right
20 m s−2 to the left
20 m s−2 to the right
C
The HL gravitational-fields model is secure when you can move between energy, potential, gradients and orbital consequences.