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CIE 9702 Physics · AS · Topic 4

Forces, density and pressure

Clear, syllabus-mapped CIE 9702 Physics revision notes on forces, density and pressure: explanations, worked examples and exam technique, then a free targeted practice drill.

CIE 9702 PhysicsASFree revision notes
Contents: 10 sections

Syllabus points

Moments

The moment of a force about a point is the force multiplied by the perpendicular distance from the point to the line of action of the force.

moment = F × d

measured in N m. The word perpendicular carries the marks. If the force is at an angle θ to the rod, the perpendicular distance is d sin θ, so the moment is Fd sin θ. Using the full length of the rod when the force is angled is the most common error in the topic.

Couples and torque

A couple is a pair of equal, antiparallel forces whose lines of action do not coincide. It produces a turning effect with no resultant force, so a body acted on by a couple alone rotates without its centre of mass accelerating.

torque of a couple = one force × perpendicular distance between them

Note "one force", not the sum. A steering wheel turned with 20 N at each side of a 0.30 m diameter has a torque of 20 × 0.30 = 6.0 N m, not 12 N m.

Equilibrium

A body in equilibrium satisfies two conditions, and both are needed:

  1. The resultant force is zero, so there is no linear acceleration.
  2. The resultant moment about any point is zero, so there is no angular acceleration.

The second condition holds about any point, which is the key to solving these questions quickly: take moments about a point where an unknown force acts, and that force disappears from the equation.

For three non-parallel coplanar forces in equilibrium, their lines of action must pass through a single point, and their vector triangle must be closed. Questions often show three forces and ask which diagram could be in equilibrium; the closed triangle is what you are looking for.

The principle of moments

For a body in equilibrium, the sum of the clockwise moments about any point equals the sum of the anticlockwise moments about that point.

Worked example. A uniform metre rule of weight 1.2 N is pivoted at the 34.0 cm mark. It balances when a mass is hung at the 10.0 cm mark. What is the mass?

A uniform rule has its weight acting at its centre, the 50.0 cm mark.

The rule's weight acts 50.0 − 34.0 = 16.0 cm from the pivot, clockwise. The mass acts 34.0 − 10.0 = 24.0 cm from the pivot, anticlockwise.

Taking moments: W × 24.0 = 1.2 × 16.0, so W = 0.80 N.

m = 0.80 / 9.81 = 0.082 kg, about 82 g.

The step people miss is the rule's own weight. It only vanishes if the rule is described as having negligible mass, and questions say so explicitly when they mean it.

Centre of gravity

The centre of gravity is the single point at which the whole weight of a body may be taken to act. For a uniform body it is at the geometric centre.

An object topples when a vertical line through its centre of gravity falls outside its base. So a low centre of gravity and a wide base make an object stable, which is the reasoning a question wants rather than the words "it is more stable".

Density

ρ = m / V

measured in kg m⁻³. Water is 1000 kg m⁻³, which is the same as 1.0 g cm⁻³, and converting between the two costs a factor of 1000, not 100.

Pressure

p = F / A

measured in pascals, where 1 Pa = 1 N m⁻². The force must be perpendicular to the area.

Pressure in a fluid acts equally in all directions at a given depth, and depends only on the depth, the density and g — not on the shape or width of the container. Two vessels of very different shape filled to the same depth have the same pressure at the base.

Deriving p = ρgh

Take a column of fluid of cross-sectional area A and height h.

Volume = Ah, so mass = ρAh, so weight = ρAhg.

Pressure at the base = weight / area = ρAhg / A = ρgh.

The area cancels, which is why the pressure does not depend on how wide the column is. Being asked to produce this derivation is common, and the cancellation is the point of it.

Remember that a question about the pressure at the bottom of a lake or a tank usually wants total pressure, so atmospheric pressure must be added to ρgh.

Upthrust and Archimedes' principle

Upthrust is the net upward force a fluid exerts on a body immersed in it. Its origin is that pressure increases with depth, so the pressure on the bottom face is greater than on the top face, and the difference in force is upward.

Archimedes' principle: the upthrust equals the weight of fluid displaced.

U = ρ_fluid × V_displaced × g

Two things follow, and both are examined:

A body floats when the upthrust equals its weight, which means it displaces its own weight of fluid.

Worked example. A block of volume 2.0 × 10⁻³ m³ is fully submerged in water. What is the upthrust?

U = 1000 × 2.0 × 10⁻³ × 9.81 = 19.6 N, whatever the block is made of.

Common mistakes

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