A.2.24—Centripetal force

Syllabus
First assessment 2025
Objective
Level
SL

Find the Centripetal Force

Centripetal force is a resultant

Centripetal force is the name for the net inward force required for circular motion:

Fc=mac=mv2rF_c=ma_c=\frac{mv^2}{r}

Identify its physical source

Centripetal force is not an extra force. It may be supplied by tension, gravity, friction, normal force, electric force or a combination of forces.

Keep the direction clear

The required resultant points toward the centre and is perpendicular to instantaneous velocity in uniform circular motion.

Common trap

Do not add a separate “centripetal force” arrow to a free-body diagram unless the question explicitly uses it as a shorthand for the inward resultant.

A.2.24 Exam Analysis

Assessment in practice

2–3 marks
How it is assessed

The evidence asks why a planet needs centripetal force and asks for tension in a vertical-circle situation.

Command terms

Explain / Calculate

What earns marks

Explain that circular motion requires a resultant force toward the centre because velocity direction changes. In a vertical circle, combine the source force and the relevant component of weight to obtain the required inward resultant.

Watch for

Treating centripetal force as an additional force or saying that a constant speed means zero resultant force.

Representative question

Question 1

[Maximum number: 2]

Explain why a centripetal force is needed for the planet to be in a circular orbit.