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Force: Turning Effect and Circular Motion — Notes

5 sections 4 min readBeta

1. Translational and rotational motion; moment of a force

  • Translational motion: every particle moves the same distance in the same direction. Rotational motion: the body turns about a fixed axis.
  • A force on a pivoted body turns it; its turning effect is the moment of the force (torque): τ=F×d\tau = F \times d, dd = perpendicular distance from the axis to the line of action.
  • Units: N m (SI), dyne cm (cgs); 1 N m=107 dyne cm1\ \text{N m} = 10^{7}\ \text{dyne cm}.
  • Moment increases with force and with perpendicular distance: handles far from hinges, long spanners, large steering wheels. A force through the axis has zero moment.
Table showing that equal moments can come from different force and distance pairs
FdMoment
20 N0.5 m10 N m
10 N1.0 m10 N m
40 N0 m0

Formulas

  • Moment of a force
    τ=F×d\tau = F \times d
  • Unit conversion
    1 N m=107 dyne cm1\ \text{N m} = 10^{7}\ \text{dyne cm}

Key terms

Moment of a force

The turning effect of a force about an axis, equal to the force multiplied by the perpendicular distance of its line of action from the axis.

Rotational motion

Motion in which a body turns about a fixed axis, each particle moving in a circle.

2. Clockwise and anticlockwise moments; couples

  • Convention: anticlockwise moments positive, clockwise negative.
  • Resultant moment = algebraic sum; the body turns in the sense of the larger total.
  • Couple: two equal, opposite, parallel forces not in the same line; produces rotation only. Moment of couple = F×F \times arm (perpendicular distance between the forces). Examples: tap, steering wheel, winding a key.
Table of the sign convention for moments
MomentSenseSign
Turns like clock handsClockwiseNegative
Turns the other wayAnticlockwisePositive

Formulas

  • Moment of a couple
    τcouple=F×arm\tau_{\text{couple}} = F \times \text{arm}

Key terms

Couple

Two equal and opposite parallel forces whose lines of action are different; it produces rotation only.

Resultant moment

The algebraic sum of the moments of all the forces about a point.

3. Equilibrium and the principle of moments

Equilibrium: a body at rest (static) or moving with uniform velocity without turning faster (dynamic). Conditions: (1) resultant force = 0; (2) resultant moment = 0.

Principle of moments: for a body in equilibrium, sum of anticlockwise moments about any point = sum of clockwise moments about that point: W1d1=W2d2W_{1} d_{1} = W_{2} d_{2}.

Verification: metre rule on a knife edge, weights hung on both sides, adjusted until the rule is horizontal; products W × d agree. Take moments about the fulcrum; include the rule’s weight at its centre of gravity if it is not pivoted there.

Table of the two conditions of equilibrium
ConditionPrevents
Resultant force zeroTranslation
Resultant moment zeroRotation

Formulas

  • Balanced lever
    W1d1=W2d2W_{1} d_{1} = W_{2} d_{2}

Key terms

Principle of moments

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

Static equilibrium

The state of a body at rest under several forces.

4. Centre of gravity

Centre of gravity (G): the point through which the whole weight of a body acts, in every orientation. It may lie outside the material (ring).

BodyPosition of G
Uniform rodMid-point
RingCentre of the ring
Circular discCentre
Triangular laminaPoint of intersection of the medians
Rectangle, parallelogramIntersection of the diagonals

Irregular lamina: suspend freely from a hole with a plumb line, mark the vertical; repeat from a second hole; G is where the lines cross.

Table of centres of gravity of three regular shapes
ShapeG
RodMiddle
RingCentre (in air)
TriangleMedians meet

Key terms

Centre of gravity

The point through which the whole weight of a body acts, whatever its position.

5. Uniform circular motion

  • Uniform circular motion: constant speed along a circle; velocity is along the tangent and changes direction continuously, so the motion is accelerated.
  • Centripetal force: the real force towards the centre that keeps the body in the circle (tension, gravity, friction, electrostatic attraction).
  • Centrifugal force: the apparent outward force felt in the rotating frame; fictitious, equal and opposite to the centripetal force.
  • If the centripetal force stops, the body moves off along the tangent (mud flying off a cycle wheel).
Table of three circular motions and their centripetal forces
MotionCentripetal force from
Moon round EarthGravity
Car on a bendFriction
Stone on stringTension

Key terms

Centripetal force

The force directed towards the centre that keeps a body moving in a circle.

Centrifugal force

An apparent outward force felt by a body in a rotating frame; it is not a real force.

Exam tips

Common mistakes

  • Using the length along a body instead of the perpendicular distance.
  • Forgetting to convert cm to m for N m answers.
  • Ignoring the weight of a metre rule pivoted away from its centre.
  • Saying uniform circular motion is not accelerated.

How marks are usually awarded

  • Calculations (1 mark each step): formula, substitution with units, answer with unit and sense.
  • Definitions (1 mark): include “perpendicular distance”, “about any point”, “whole weight acts”.
  • Circular motion (1 mark each): direction of velocity and of centripetal force.