A. Space, time and motion
- Syllabus
- First assessment 2025
- Section
- —
- Level
- HL

Choose a reference
Position r specifies where an object is relative to a chosen origin. A position is not meaningful without a reference frame and coordinate direction.
Track change in position
Velocity v describes how position changes with time. It is a vector: its direction is the direction of motion at that instant, and on a curved path the velocity arrow is tangent to the path.
Track change in velocity
Acceleration a describes how velocity changes with time. A change in speed, direction, or both is acceleration; an object can accelerate even while its instantaneous speed is zero.
Common trap
Do not use “velocity” as a synonym for speed. Speed gives only magnitude; velocity also requires direction relative to the chosen coordinate system.
[ 1 ]
the velocity of the ball at P . Label this arrow v.
Velocity is a rate
Velocity is the rate of change of position:
v=dtdr
Over a finite interval, average velocity is displacement divided by elapsed time.
Acceleration changes velocity
Acceleration is the rate of change of velocity:
a=dtdv
A constant acceleration gives equal changes in velocity during equal time intervals.
Read the gradient
On a position–time graph, the gradient represents velocity. On a velocity–time graph, the gradient represents acceleration. The graph’s slope, not its height alone, carries the rate-of-change meaning.
Common trap
Distance divided by time gives average speed, not instantaneous velocity. Likewise, a large velocity does not imply a large acceleration unless the velocity is changing rapidly.
[ 1 ]
Instantaneous velocity is defined as...
Displacement is a vector
Displacement is the change in position:
Δr=rfinal−rinitial
It has a magnitude and a direction from the initial position to the final position.
Ignore the route for displacement
The path taken between the two positions does not determine displacement. A curved or complicated journey can still have a straight-line displacement between its endpoints.
Use components when needed
For perpendicular changes, resolve displacement into components and combine them vectorially. A signed one-dimensional displacement is positive or negative according to the chosen axis.
Common trap
A return to the starting point gives zero displacement even though the distance travelled is non-zero.
[ 1 ]
A stone is kicked horizontally at a speed of 1.5 ms−1 from the edge of a cliff on one of Jupiter's moons. It hits the ground 2.0 s later. The height of the cliff is 4.0 m .
Air resistance is negligible.
What is the magnitude of the displacement of the stone?
Distance
Distance is the total path length travelled. It is a scalar, so it has magnitude only and cannot be negative.
Displacement
Displacement is the vector change in position from start to finish. Its magnitude is the shortest endpoint-to-endpoint separation, not generally the length of the route.
Match the average quantity
Average speed uses total distance divided by total time. Average velocity uses displacement divided by total time. A route with turns can therefore have average speed greater than the magnitude of average velocity.
Common trap
For a complete oscillation, the displacement is zero but the distance is four times the amplitude. Choose the quantity named in the question before substituting.
[ 1 ]
A person walks 40 m due west and then 30 m due north. The total walking time is 100 s . What are the average speed and the magnitude of the average velocity of the person?
Average speed/m s −1
Magnitude of average
velocity /ms−1
0.5
0.5
0.5
0.7
0.7
0.5
0.7
0.7
Average values use an interval
Average speed is total distance divided by total time. Average velocity is displacement divided by elapsed time. Average acceleration is change in velocity divided by elapsed time.
Instantaneous values use one moment
Instantaneous velocity is the tangent gradient on a position–time graph; instantaneous speed is its magnitude and is what an ideal speedometer reports. Instantaneous acceleration is the tangent gradient on a velocity–time graph. Average values instead use a finite interval.
Connect graph quantities
The gradient of a velocity–time graph is acceleration, and the area under it is displacement. A constant acceleration therefore produces a straight-line velocity–time graph.
Common trap
Do not use the average gradient when a question asks for an instantaneous value. Use the tangent at the specified time.
[ 1 ]
The graph shows the variation of the acceleration a with time t of an object moving in a straight line.
Which graph shows the variation of the velocity v of the object with time t ?
Uniform-acceleration model
SUVAT equations apply when acceleration is constant along the chosen one-dimensional axis:
v=u+at,s=ut+21at2,v2=u2+2as,s=2u+vt
Choose an equation
List the known and unknown quantities s,u,v,a,t. Select an equation containing the required unknown and only known quantities; keep signs consistent with the positive direction.
Check the model
A constant acceleration means equal changes in velocity in equal time intervals. Use separate horizontal and vertical equations only when the motion has been resolved into independent components.
Worked example from local Question Bank row 22687
A glider accelerates uniformly from rest to 27.0ms−1 in 11.0s. Use s=2u+vt:
s=20+27.0×11.0=148.5m≈149m
The result is the launch-run displacement; the constant-acceleration assumption is essential.
Common trap
Do not use SUVAT when acceleration varies significantly with time or position. A formula can produce a neat number while still violating the model’s constant-acceleration assumption.
[ 3 ]
Determine g using the photograph.
Uniform acceleration
Acceleration is uniform when the velocity changes by equal amounts in equal time intervals. The velocity–time graph is a straight line with constant gradient.
Non-uniform acceleration
Acceleration is non-uniform when its magnitude or direction changes. The velocity–time graph then has a changing gradient, and a single SUVAT value cannot describe the entire interval.
Model versus reality
A constant-acceleration model can be useful over a limited interval even when real forces vary. State the approximation and identify the neglected force or changing condition.
Common trap
A curved trajectory does not by itself prove that acceleration is non-uniform: projectile motion without drag has constant downward acceleration while its velocity direction changes.
[ 1 ]
State one reason why the acceleration of the spacecraft will not be constant.
Separate the axes
With negligible fluid resistance, projectile motion is independent horizontal and vertical motion. Resolve the launch velocity:
ux=ucosθ,uy=usinθ
Horizontal motion
There is no horizontal acceleration in the ideal model, so vx=ux and x=uxt. Use the horizontal displacement to find time or horizontal speed.
Vertical motion
Use one-dimensional constant-acceleration equations vertically, usually with ay=−g if upward is positive. The horizontal and vertical equations share the same time t.
Worked example from local Question Bank row 31723
A tennis ball travels 11.9m horizontally after launch at 64.0ms−1 and 7∘ to the horizontal.
ux=64.0cos7∘=63.52ms−1
t=uxx=63.5211.9=0.187s
The same 0.187s must then be used in the vertical equation.
Common trap
Do not use the launch speed as the horizontal speed. Resolve it first, and do not use the horizontal time independently of the vertical motion.
[ 2 ]
The ball leaves the ground at an angle of 22∘. The horizontal distance from the initial position of the edge of the ball to the wall is 11 m . Calculate the time taken for the ball to reach the wall.
Drag opposes instantaneous velocity
Fluid resistance acts opposite the projectile's velocity and usually grows with speed. Its direction changes through the flight, so the resultant acceleration is not the constant downward g of the ideal model.
| Quantity | Qualitative effect of fluid resistance |
|---|---|
| Trajectory | No longer a symmetric parabola; descent is typically steeper |
| Horizontal velocity | Decreases because drag has a component opposite horizontal motion |
| Vertical acceleration | On ascent, downward drag makes downward acceleration greater than g; on descent, upward drag makes it less than g |
| Maximum height and range | Both are reduced for the same launch conditions |
| Time of flight | Ascent is shortened, while descent can be lengthened by upward drag; the total change is not universally one direction |
| Terminal speed | During a long fall, increasing drag can balance weight so resultant force and acceleration become zero |
Use the force direction
Before the peak, drag has horizontal and downward components; after the peak, it has horizontal and upward components. Therefore acceleration is not determined by velocity alone and changes continuously.
Terminal-speed condition
For vertical descent, terminal speed is reached when upward drag (and any buoyancy included in the model) balances weight. The object then continues at constant downward velocity.
Common trap
Zero acceleration at terminal speed does not mean zero velocity. At the top of a projectile path, vertical velocity may be zero while acceleration remains non-zero.
[ 1 ]
The diagram shows the path of a ball in the absence of air resistance. Q is the highest point of the ball's trajectory and a is the vertical acceleration at Q . At impact the velocity makes an angle θ to the horizontal.
Three statements about the actual motion of the ball when there is air resistance are:
I. Q is lower.
II. a remains the same.
III. θ increases.
Which statements are correct?
Describe motion
Position locates the object, velocity is the rate of change of position, and acceleration is the rate of change of velocity. Distance and speed are scalar; displacement and velocity are directed quantities.
Use the right model
For uniform acceleration:
v=u+at,\quad s=ut+rac12at^2,\quad v^2=u^2+2as
For projectiles without drag, solve horizontal and vertical components with a shared time. Do not use these equations when acceleration is non-uniform.
Check the boundary
Ask whether the quantity is average or instantaneous, whether the route or endpoints matter, whether acceleration is constant, and whether a neglected force such as drag changes the model.
Three linked laws
Choose the system
Draw forces acting on the chosen object, then use the resultant force to predict its acceleration. For action–reaction pairs, identify the two different bodies before applying the third law.
Use interactions to explain motion
A rocket pushes gas backward; the gas exerts an equal and opposite force on the rocket. The rocket can therefore accelerate even in the absence of a supporting surface.
Common trap
The forces in a third-law pair do not cancel in one free-body diagram because they act on different objects.
[ 3 ]
As the probe approaches the surface of the asteroid, a rocket engine is fired to slow its descent. Explain how the engine changes the speed of the probe.
A force needs an interaction
A force is an interaction between bodies. One body exerts the force and another body experiences it. Contact, gravitational, electric and magnetic interactions can all change momentum.
Name both bodies
When explaining a force, state the interacting pair and the direction of the force on the chosen body. The reaction force acts on the other body, not back on the same free-body diagram.
Fields can mediate interaction
Bodies do not need to touch for gravitational, electric or magnetic forces. For example, current-carrying coils interact through their magnetic fields, producing attraction or repulsion depending on the field arrangement.
Common trap
Do not describe a force as a property that an isolated object “has” without naming the other body or field involved.
[ 2 ]
Explain why, when there is a current in the coil, the separation of X and Y decreases.
Isolate one body
A free-body diagram shows only the chosen body and the external forces acting on it. Replace the body with a point or simple shape and choose useful axes.
Draw actual forces
Use arrows from the body, label each interaction and draw the direction physically. Typical labels include weight mg, normal force N, tension T, friction and drag.
Resolve only when needed
If a force is angled, resolve it into the chosen axes. Then apply ∑Fx=max and ∑Fy=may to the same body.
Common trap
Do not draw velocity, acceleration or a force exerted by the chosen body on its surroundings as forces acting on the chosen body.
[ 2 ]
Draw a labelled free-body diagram of the forces on the ball.
Add force components
The resultant force is the vector sum of all forces on the chosen body:
Fnet=∑F
Resolve angled forces into perpendicular components before adding.
Connect to acceleration
For constant mass, apply Newton’s second law along each axis:
∑Fx=max,∑Fy=may
Use equilibrium correctly
If the resultant force is zero, acceleration is zero, but the object may still have constant non-zero velocity. A balanced vertical component does not imply every force is absent.
Common trap
Do not add force magnitudes without their directions. A component that balances another contributes zero only along the same axis.
[ 2 ]
Determine the acceleration of the truck.
Contact-force family
Contact forces arise when bodies or a body and fluid interact: normal force, friction, tension, elastic restoring force, viscous drag and buoyancy.
Use the interaction geometry
Normal force is perpendicular to the surface; friction acts along the surface opposing relative motion or attempted motion; tension acts along a taut string; drag opposes motion through a fluid; buoyancy acts upward due to fluid pressure differences.
Check the condition
Friction can be static or kinetic, drag depends on speed and shape, and buoyancy depends on displaced fluid. The magnitudes are determined by the interaction and constraints, not by a memorized universal value.
Common trap
Do not include every possible contact force. Include only interactions actually present in the described situation.
[ 1 ]
A ball is thrown from an aircraft in flight.
Which of the following shows the correct free-body diagram for the forces acting on the ball when terminal velocity is reached?
Normal means perpendicular
The normal force N is the contact force exerted by a surface perpendicular to that surface. Its direction follows the local surface normal, not necessarily the vertical direction.
Find it from the force balance
Use the component of Newton’s second law perpendicular to the surface. In a curved path, the normal force may combine with a component of weight to provide the required centripetal resultant.
Do not assume N=mg
N=mg applies only in situations where the perpendicular acceleration and other perpendicular force components make that balance valid. Inclines, lifts, loops and vertical acceleration change the normal force.
[ 3 ]
Determine the normal force exerted by the loop on the car at P .
Friction follows the contact
Friction acts parallel to the contact surface and opposes relative motion or the tendency of surfaces to move relative to each other.
Static friction adapts
Before slipping, static friction has whatever value is needed up to a maximum:
Ff≤μsN
It is not automatically equal to μsN; that value occurs at impending motion.
Dynamic friction during sliding
Once surfaces slide, the model gives
Ff=μdN
Use the normal force for the actual contact and combine friction with the other forces along the surface.
Common trap
Do not use the dynamic coefficient before motion begins, or assume static friction is always at its maximum.
[ 2 ]
Show that the minimum force needed to accelerate the box is about 4 N .
Tension is a pull
Tension is the force exerted by a taut string, cable or rope on an attached body. It acts along the string and pulls away from the body.
Use the ideal-string model carefully
For a light, inextensible string over a frictionless pulley, tension has the same magnitude throughout. If the string, pulley or contact is non-ideal, tension can vary and must be found from each body’s force balance.
Connect tension to motion
Draw tension in the string direction, then use ∑F=ma. A body can have non-zero tension while at rest if other forces balance it.
Common trap
A string can pull but not push. Do not draw tension toward the string’s far end through the body or assume its value equals the weight without a force balance.
[ 1 ]
Calculate the maximum tension in the string.
Restoring force
For an ideal elastic element within its proportional range,
FH=−kx
The minus sign means the force acts opposite the displacement from equilibrium.
Use extension correctly
For a spring, x is extension or compression relative to its natural length. In a vertical equilibrium, the spring tension can balance weight, but the extension is not the total spring length.
Respect the model boundary
Hooke’s law is a linear approximation. Beyond the limit of proportionality, the force–extension graph is no longer linear and the same k cannot be used.
[ 1 ]
A spring of negligible mass and length l0 hangs from a fixed point. When a mass m is attached to the free end of the spring, the length of the spring increases to l. The tension in the spring is equal to kΔx, where k is a constant and Δx is the extension of the spring. What is k ?
Stokes drag
For a small sphere moving slowly through a viscous fluid,
Fd=6πηrv
where η is viscosity, r is sphere radius and v is speed relative to the fluid.
Drag opposes motion
The drag force points opposite the sphere’s velocity. As speed increases, drag increases linearly in this model, reducing the resultant force when the driving force is fixed.
Approach to terminal speed
For a falling sphere, weight drives the motion and viscous drag grows with speed. When drag balances the effective weight, acceleration becomes zero and terminal speed is reached.
Common trap
Do not treat viscosity η as the same quantity as drag force, and do not forget that the formula applies to the stated small-sphere, viscous-flow model.
[ 2 ]
Describe why the acceleration of the oil droplet changes.
Buoyancy from pressure difference
A fluid exerts a net upward buoyant force on an immersed object because pressure is greater at greater depth. In the IB model,
Fb=ρfVdispg
where Vdisp is the displaced fluid volume.
Separate buoyancy from net force
The buoyant force is one force in the free-body diagram. The net force is found after combining it with weight, tension, drag or other forces.
Floating condition
For an object at rest on the fluid, buoyancy balances its weight. This gives a useful density or submerged-volume relationship, but only after the equilibrium assumption is stated.
Common trap
Use the density of the displaced fluid and the displaced volume, not automatically the object’s total volume or density.
[ 1 ]
Show that Fb is about 2 mN .
Three field interactions
Gravitational, electric and magnetic forces are field forces: bodies can interact without contact. Identify the source of the field, the object acted on and the force direction.
Keep the mechanisms distinct
Gravity acts on mass, electric force acts on charge, and magnetic force acts on moving charges or currents in a magnetic field. Their equations and direction rules are not interchangeable.
Use the force relevant to the system
A free-body diagram may contain more than one field force. Add them as vectors and apply Newton’s second law to the selected body.
Common trap
Do not call every non-contact force “electromagnetic”; gravitational attraction is a separate interaction.
[ 1 ]
What are three fundamental forces listed in decreasing order of strength?
Weight is a force
Weight is the gravitational force on a mass:
Fg=mg
The direction is toward the local gravitational field source.
Use local g
The value of g depends on location. Use the value stated or the local field strength appropriate to the body’s position; mass does not change when the object is moved.
Common trap
Mass is measured in kilograms and is not a force. Weight is measured in newtons and can change when g changes.
[ 1 ]
The probe is carried to the asteroid on board a spacecraft.
Calculate the weight of the probe when close to the surface of the asteroid.
Electric interaction
Electric force acts between charged bodies. Its direction depends on the signs of the charges: like charges repel and unlike charges attract.
Use the electric field
A positive test charge is pushed in the electric-field direction; a negative charge experiences force opposite to the field. Keep field direction and force direction separate when the charge sign matters.
Common trap
Do not reverse the force direction for a positive charge, and do not treat electric force as a contact force.
This exam question is unavailable.
Magnetic interaction
A magnetic force acts on a moving charge or current in a magnetic field. Its direction is perpendicular to the relevant velocity/current and magnetic-field directions.
Apply the direction rule
Use the stated right-hand rule or vector relationship, then reverse the result for a negative charge. Parallel motion and field give zero magnetic force in the ideal model.
Common trap
A magnetic field can change the direction of velocity without doing work on an ideal moving charge; do not automatically infer a speed change from a magnetic force.
This exam question is unavailable.
Momentum
Linear momentum is
p=mv
It is a vector. For an isolated system, total momentum is conserved before and after an interaction.
Check the system
Momentum is conserved when the resultant external impulse on the chosen system is negligible. Internal forces can change individual momenta while leaving the vector total unchanged.
Use signs or components
Choose a positive direction and conserve momentum component-by-component. A negative final velocity means motion opposite to the chosen positive direction.
Common trap
Do not conserve kinetic energy automatically. Momentum conservation and kinetic-energy conservation are separate claims.
[ 1 ]
Cart X , of mass 2 kg , is moving at a speed of 3 m s−1 to the right and collides on a horizontal track with cart Y of mass 1 kg.Y is initially stationary.
The velocity of Y immediately after the collision is 4 m s−1 to the right. What is the velocity of X immediately after the collision?
Impulse changes momentum
Impulse is the integral of resultant force over time. For a constant average force,
J=FnetΔt=Δp
Use the momentum change
Calculate Δp=pf−pi, including direction. A rebound reverses the velocity component and can make the momentum change larger than either momentum magnitude alone.
Average force
If the force varies, FΔt represents average resultant force over the contact interval. Use consistent units for impulse in N s or kg m s⁻¹.
Common trap
Do not use the initial momentum alone when the object rebounds or ends with a non-zero final velocity.
[ 2 ]
The ball rebounds from the ground with speed 7.8 ms−1. The ball is in contact with the ground for a time T. The average resultant force on the ball during this time is 1.1 N .
Determine T.
Impulse is external to the system
For a chosen system, the net external impulse equals the system’s change in total momentum:
Jext=Δpsystem
Same momentum change, different force
If an object must undergo the same Δp, increasing the stopping time reduces the average resultant force:
Favg=ΔtΔp
Apply to safety systems
A flexible safety net, airbag or crumple zone extends the interaction time while producing the required momentum change, reducing the average force on the person or vehicle.
Common trap
Extending the stopping time does not make the momentum change disappear; it changes the rate at which that change occurs.
[ 2 ]
Explain, with reference to change in momentum, why a flexible safety net is less likely to harm the skier than a rigid barrier.
Constant mass
For a body of constant mass, Newton’s second law becomes
Fnet=ma
Use the resultant force, not one arbitrarily selected force.
General momentum form
The broader statement is
Fnet=ΔtΔp
or its instantaneous form. This is the safer form when mass changes or when momentum is the quantity given.
Check what changes
If mass is constant, Δp=mΔv, so the two forms agree. If mass enters or leaves the system, include the momentum carried by that mass and define the system carefully.
Common trap
Do not double the acceleration simply because an applied force doubles when a fixed resistive force remains; calculate the new resultant force first.
[ 2 ]
Calculate the magnitude of the initial acceleration of the electron.
Momentum first
In an isolated collision, total linear momentum is conserved for both elastic and inelastic collisions.
Kinetic energy distinguishes them
In an elastic collision, total kinetic energy is also conserved. In an inelastic collision, some kinetic energy is transferred to internal energy, sound or deformation; in a perfectly inelastic collision the bodies move together afterward.
Use the right conservation law
Apply momentum conservation to find final velocities, then compare initial and final kinetic energy if the collision type is required.
Common trap
“Inelastic” does not mean momentum is lost. It means kinetic energy is not conserved.
[ 2 ]
Calculate the speed of the ship after the collision.
Ice in a still lake will usually form in a single layer on the surface.
Explosion model
An explosion is an interaction in which an initially combined system separates into parts. If the external impulse is negligible, total momentum before and after is equal.
Use a sign convention
For an object initially at rest, the vector momenta after the explosion sum to zero. In one dimension, equal and opposite momenta can give different speeds when the masses differ.
Energy is separate
The chemical, elastic or other internal energy released can increase total kinetic energy while momentum remains conserved.
Common trap
Do not assume the fragments have equal speeds. Momentum magnitudes are equal and opposite only when the initial total momentum is zero.
This exam question is unavailable.
Track the energy store
Total energy is conserved, but kinetic energy may be transferred to internal energy, sound, deformation or chemical energy during an interaction.
Collision comparison
Elastic collisions conserve total kinetic energy as well as momentum. Inelastic collisions conserve momentum but have a lower final total kinetic energy.
Explosion comparison
An explosion can convert internal energy into kinetic energy, so final kinetic energy can exceed the initial kinetic energy while total momentum remains conserved.
Common trap
“Kinetic energy is lost” is shorthand for transferred to other stores; it is not destroyed.
[ 3 ]
Show that the collision is inelastic.
Radial acceleration
For uniform circular motion, the centripetal acceleration is directed toward the centre:
ac=rv2=ω2r=T24π2r
Velocity can be constant in magnitude
Even when speed is constant, the velocity direction changes continuously. That directional change produces inward acceleration.
Choose the matching data
Use v2/r when speed and radius are given, ω2r when angular speed is given, or 4π2r/T2 when period is given.
Common trap
Centripetal acceleration is not tangential and does not point along the instantaneous velocity.
[ 2 ]
The fan is rotating at 120 revolutions every minute. Calculate the centripetal acceleration of the tip of a fan blade.
Centripetal force is a resultant
Centripetal force is the name for the net inward force required for circular motion:
Fc=mac=rmv2
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.
[ 2 ]
Explain why a centripetal force is needed for the planet to be in a circular orbit.
Velocity direction changes
In circular motion, the inward centripetal acceleration changes the direction of the velocity. If speed is constant, the magnitude of velocity stays constant while its direction changes.
What happens if the inward force disappears
If the centripetal interaction is removed, the object continues along the tangent at the release point, consistent with Newton’s first law.
Maintain contact
In a vertical loop, the inward resultant must be sufficient to maintain the required radial acceleration. At the limiting contact condition, the normal force can fall to zero.
Common trap
The released object does not move along the radius; its instantaneous path is tangent to the circle.
[ 1 ]
A mass at the end of a string is swung in a horizontal circle at increasing speed until the string breaks.
The subsequent path taken by the mass is a
Connect the descriptions
For uniform circular motion,
v=T2πr=ωr
Angular speed ω is the same for all points on a rigid rotating body, while linear speed increases with distance from the axis.
Use the period
One revolution takes period T, so ω=2π/T. Keep radians and seconds consistent.
Compare points on one disk
If one point is twice as far from the centre, its linear speed is twice as large at the same angular speed; its centripetal acceleration is also twice as large.
Common trap
Do not assume equal linear speeds for all points on a rotating disk. Equal angular speed does not mean equal tangential speed.
[ 1 ]
A disk of radius R rotates about its axis with angular speed ω. Point X is at a distance of 2R from the centre and point Y is on the circumference.
What are the ratios of the linear speeds and the centripetal acceleration of X to Y.
The linear speed of X is vX and its acceleration is aX; the linear speed of Y is vY and its acceleration is aY.
Linear speeds vYvX
Acceleration aYaX
21
41
21
21
1
41
1
21
Build the force model
Choose the system, draw a labelled free-body diagram, classify the interactions and resolve components. Apply Newton’s laws with the correct boundary: contact forces, field forces, friction, tension, buoyancy and restoring forces each have their own direction and conditions.
Track momentum
Use ec p=mec v, ec J=\Deltaec p and momentum conservation only after checking external impulse. Distinguish elastic and inelastic collisions, explosions and energy transfer.
Track circular motion
The inward resultant provides ac=v2/r=ω2r. It may come from tension, gravity, normal, friction or a field force. Angular and linear descriptions are linked by v=ωr=2πr/T.
Final checks
Ask: Which body is the system? Which forces are external? Is mass constant? Is acceleration uniform or radial? Is kinetic energy conserved, transferred or increased?
Energy is conserved
Energy cannot be created or destroyed. In a defined system, energy is transferred between stores or across the system boundary, so the total energy accounting remains balanced.
Define the system first
Name the objects included and identify transfers by work, heating, radiation or electrical means. A falling object may transfer gravitational potential energy to kinetic energy, internal energy or sound.
Follow the chain
Write the initial store, the useful output store and any dissipated or transferred energy. A Sankey diagram or energy-flow statement should account for all significant branches.
Common trap
Energy “lost” from a useful store has been transferred elsewhere; it has not disappeared.
[ 2 ]
Outline, with reference to energy changes, the operation of a pumped storage hydroelectric system.
Work transfers energy
Work done by a force is the energy transferred by that force. For a constant force,
W=Fscosθ
where θ is the angle between force and displacement.
Use the sign
Positive work transfers energy into the object’s relevant store; negative work transfers energy out of it. A force perpendicular to displacement does zero work.
Follow the physical process
Wind can transfer kinetic energy to a turbine through work, while resistive forces can transfer mechanical energy to internal energy of the surroundings.
Common trap
Do not call every force an energy transfer. Check whether the force has a component along the displacement.
[ 2 ]
Describe the energy transfers taking place in a wind generator.
Read the width as energy
A Sankey diagram shows an input energy flowing into useful output and other transfers. Arrow width is proportional to energy, so the branches must account for the whole input.
Identify useful output
Label the useful branch before calculating efficiency. Other branches may represent heating, sound or unwanted mechanical transfers.
Connect to efficiency
The useful fraction of the input is
η=EinputEuseful=PinputPuseful
Common trap
Do not compare branch widths without checking whether the diagram uses the same scale and whether the requested quantity is energy or power.
[ 1 ]
The Sankey diagram shows the energy input from fuel that is eventually converted to useful domestic energy in the form of light in a filament lamp.
What is true for this Sankey diagram?
Constant-force work
For a force F acting through displacement s,
W=Fscosθ
Only the component parallel to displacement transfers energy by work.
Area under a force–distance graph
For a variable force, the area under an F-against-s graph gives work. A negative area represents work against the chosen displacement direction.
Check the angle
Use the angle between force and displacement, not the angle between the force and an unrelated axis unless the component has first been resolved.
Worked example from local Question Bank row 39177
A kite pulls a ship with force 2.50×105N at 39∘ to its 1.00km displacement. Convert 1.00km=1.00×103m, then
W=Fscosθ=(2.50×105)(1.00×103)cos39∘=1.94×108J≈1.9×108J
Only the force component along the ship's displacement transfers energy.
[ 1 ]
State what is represented by the area under the graph.
Work–energy theorem
The net work done by the resultant force on a system equals its change in kinetic energy:
Wnet=ΔEk
Use force–distance area
For a variable resultant force, the signed area under the force–distance graph gives the work and therefore the kinetic-energy change.
Include all resultant forces
Friction, applied forces and gravity may each do work. Add their signed contributions before relating the result to the final kinetic energy.
Worked example from local Question Bank row 31356
A constant net force of 100N moves an object from rest through 2.0m until its speed is 10ms−1.
Wnet=Fs=(100)(2.0)=200J
200=ΔEk=21m(10)2−0
m=4.0kg
The positive net work is exactly the object's kinetic-energy gain.
Common trap
Do not use the work of one force as the net work unless all other force contributions are zero or already included.
[ 3 ]
A force of 14.0 N acts on the box for 0.35 m as shown. The force is then removed and the box continues to move. The box comes to rest after a further displacement d.
Determine d.
Mechanical energy stores
Mechanical energy is the sum of translational kinetic energy, gravitational potential energy and elastic potential energy:
Emech=Ek+Ep,g+Ep,elastic
Use the chosen system
Mechanical energy describes these stores within the system. Internal energy, chemical energy and sound may also be present in the full energy account but are not mechanical energy.
Common trap
Do not call all conserved energy mechanical energy; classify the store before applying a mechanical-energy equation.
[ 1 ]
show that the speed of the ball is about 4.3 ms−1.
Condition for conservation
Mechanical energy is conserved when only conservative forces transfer energy within the system and friction or other resistive transfers are absent or negligible.
Write the balance
Ek,i+Ep,i=Ek,f+Ep,f
Choose a convenient zero for potential energy and keep the same reference throughout.
When it is not conserved
Friction, drag or deformation transfer mechanical energy to internal energy. Total energy is still conserved, but the mechanical-energy equation needs an additional transfer term.
[ 1 ]
An object is released from rest and slides down a frictionless ramp. The object then leaves the ramp and slides along a rough horizontal surface. The object stops in a distance s along the ramp.
The coefficient of dynamic friction between the object and the rough horizontal surface is μ.
What is the height of the ramp?
Conservative transformations
When mechanical energy is conserved, energy can move between translational kinetic, gravitational potential and elastic potential stores without changing their sum.
Use the endpoints
For a car descending a frictionless track, gravitational potential energy decreases while kinetic energy increases. For a spring system, elastic potential energy can become kinetic energy and then return.
Add non-conservative transfers
If friction or drag acts, part of the mechanical energy transfers to internal energy. The endpoint equation must include that loss from the mechanical stores.
[ 2 ]
Show that the speed of the car at P is 1.7 ms−1.
Kinetic-energy forms
Translational kinetic energy is
Ek=21mv2=2mp2
Choose the known quantity
Use 21mv2 when mass and speed are given, or p2/(2m) when momentum is given. Kinetic energy is scalar and cannot be negative.
Worked example from local Question Bank row 35674
For m=0.14g=1.4×10−4kg and v=3.1ms−1,
Ek=21(1.4×10−4)(3.1)2=6.7×10−4J=0.67mJ
Converting grams to kilograms before substitution keeps the energy unit in joules.
Common trap
Doubling speed quadruples kinetic energy; do not scale it linearly with speed.
[ 2 ]
Calculate the final speed of the car.
Near-Earth gravitational potential energy
For a height change Δh in a uniform gravitational field,
ΔEp,g=mgΔh
Use the height change
Raising an object gives positive change in gravitational potential energy; lowering it gives negative change relative to the chosen reference.
Link to power
If height changes at constant speed, the rate of gravitational potential-energy gain is mgv, before accounting for efficiency or other transfers.
Worked example from local Question Bank row 37039
An object's weight is 6.10×102N and it rises vertically by 8.0m. Since mg is its weight,
ΔEp,g=(6.10×102)(8.0)=4.88×103J≈4.9kJ
The positive result means the gravitational potential-energy store increases.
Common trap
Use the local value of g and the vertical height change, not the distance along a slope.
[ 1 ]
A car takes 20 minutes to climb a hill at constant speed. The mass of the car is 1200 kg and the car gains gravitational potential energy at a rate of 6.0 kW . Take the acceleration of gravity to be 10 m s−2. What is the height of the hill?
Elastic store
For a spring within its linear range,
Ep,elastic=21k(Δx)2
where Δx is extension or compression from the natural length.
Area under the graph
The elastic potential energy equals the work done in stretching or compressing the spring. On a force–extension graph it is the area under the graph.
Worked example from local Question Bank row 31357
A spring with k=100Nm−1 is compressed by 0.10m.
Ep,elastic=21(100)(0.10)2=0.50J
This is the energy available for transfer when the ideal spring is released.
Common trap
Do not use the total spring length as Δx, and remember that doubling extension quadruples the stored energy in the ideal model.
[ 1 ]
0.25 J of work is done to compress a spring by a distance of 0.10 m from its unstretched length. What is the spring constant?
Power is rate
Power is the rate of work or energy transfer:
P=ΔtΔW=ΔtΔE
Mechanical shortcut
For a constant force parallel to velocity,
P=Fv
Keep energy and power distinct
Energy is measured in joules; power is measured in watts, or joules per second. Multiply power by time to recover transferred energy.
Worked example from local Question Bank row 29322
A student of weight 600N climbs 6.0m vertically in 8.0s.
ΔW=(600)(6.0)=3.6×103J
P=8.03.6×103=4.5×102W=450W
The result is the average rate of energy transfer against gravity.
[ 1 ]
A student of mass m initially at rest takes t seconds to run up stairs of height h. At the top of the stairs the student has a velocity v.
What is the average power supplied by the student during the climb?
Useful fraction
Efficiency is the ratio of useful output to total input:
η=EinputEuseful=PinputPuseful
Choose matching quantities
Use energy ratios for the same process and time interval, or power ratios when input and output are rates. Efficiency is dimensionless and is often reported as a percentage.
Worked example from local Question Bank row 29709
Solar intensity is 240Wm−2 over 2.50×104m2, so input power is
Pin=(240)(2.50×104)=6.0×106W=6.0MW
For a useful output of 1.6MW,
η=6.01.6=0.27=27%
The remaining input is transferred through non-useful pathways.
Common trap
Do not invert the ratio or use the total output, including unwanted transfers, as the useful output.
[ 1 ]
An electric motor of efficiency 75 % raises a mass of 120 kg at a constant speed of 0.50 ms−1. What is the power input to the motor?
Energy per volume
For the current IB Physics definition, fuel energy density u is the transferable energy per unit volume:
u=VE
Its SI unit is Jm−3. This lets fuels be compared when storage volume is the constraint.
Connect it to a fuel flow
If fuel flows at volume rate V˙, its input power is Pin=uV˙. Apply efficiency only after finding the input energy or power.
Worked example from local Question Bank row 36970
An engine produces 20kW useful power at 50% efficiency while consuming 1.0×10−5m3s−1 of fuel.
Pin=0.5020kW=40kW
u=V˙Pin=1.0×10−54.0×104=4.0×109Jm−3=4.0GJm−3
Common trap
Specific energy is energy per unit mass, measured in Jkg−1. Some sources use the words loosely, so let the stated definition and units determine whether to divide by volume or mass.
[ 2 ]
At the end of the 30-day period, rockets are fired to bring the ISS back to its initial height. The energy density of liquid hydrogen rocket fuel is 8.5×103MJm−3.
Estimate the volume of fuel needed.
Account for energy
Define the system, identify energy stores and describe transfers. Work done by a force transfers energy; total energy is conserved even when mechanical energy is not.
Use the mechanical model
E_k=rac12mv^2,\quad \Delta E_{p,g}=mg\Delta h,\quad E_{p,elastic}=rac12k(\Delta x)^2
Conserve their sum only when resistive transfers are absent or included explicitly.
Use rates and ratios
P=rac{\Delta E}{\Delta t}=Fv,\qquad \eta=rac{E_{useful}}{E_{input}}=rac{P_{useful}}{P_{input}}
Fuel energy density connects available input energy to a chosen volume.
Final checks
Check the system boundary, signs of work and potential-energy changes, the reference height, extension from natural length, and whether the quantity is energy, power, efficiency or energy density.
Torque is a turning effect
The torque of a force about an axis is
τ=Frsinθ
where r is the distance from the axis to the point of application and θ is the angle between r and F.
Use the perpendicular lever arm
Equivalently, torque equals force multiplied by the perpendicular distance from the axis to the force’s line of action.
Choose a rotation sign
Clockwise and anticlockwise torques have opposite signs. Add torques about the specified axis rather than adding their magnitudes blindly.
Worked example from local Question Bank row 37867
Two forces produce the same rotational sense: 50N at a perpendicular distance 0.50m and 40N at 0.20m.
τnet=(50)(0.50)+(40)(0.20)=25+8=33Nm≈30Nm
If one force acted in the opposite sense, its torque would enter with the opposite sign.
Common trap
A force through the axis has zero torque, even if its magnitude is large.
[ 2 ]
Calculate the torque that acts on the disk while it accelerates.
Equilibrium condition
A rigid body is in rotational equilibrium when the resultant torque about any chosen axis is zero:
∑τ=0
Balance clockwise and anticlockwise effects
Choose an axis, assign signs, and set the sum of clockwise torques equal to the sum of anticlockwise torques. A body can still have translational equilibrium as a separate condition.
Common trap
Zero resultant torque means no angular acceleration; it does not by itself prove that the net force is zero.
[ 1 ]
State the condition for rotational equilibrium.
Rotational second law
A non-zero resultant torque causes angular acceleration:
∑τ=Iα
Use the chosen axis
Calculate signed torques about the specified axis and use the moment of inertia about that same axis. The direction of α follows the resultant torque.
Common trap
Do not use translational F=ma for a purely rotational equation or mix an inertia about one axis with torque about another.
[ 3 ]
Calculate the angular acceleration of the disk.
Three angular quantities
Angular displacement θ describes change in orientation, angular velocity ω=dθ/dt describes how fast orientation changes, and angular acceleration α=dω/dt describes how angular velocity changes.
Link to linear motion
At radius r, tangential speed is v=rω. Keep angular quantities in radians when using these relationships.
Common trap
Angular velocity is not automatically the same as linear speed; the radius is needed to connect them.
[ 1 ]
Calculate the angular velocity ω of P.
Uniform angular acceleration
When α is constant, use rotational SUVAT:
ω=ω0+αt,θ=ω0t+21αt2,ω2=ω02+2αθ
Choose the equation
List θ,ω0,ω,α,t, convert revolutions to radians, and choose the equation containing the required unknown and known quantities.
Worked example from local Question Bank row 39408
A bar starts from rest and turns through six revolutions with constant α=0.110rads−2. Convert Δθ=6(2π)=12πrad, then
ωf2=ωi2+2αΔθ=0+2(0.110)(12π)
ωf=2.88rads−1≈2.9rads−1
The equation is valid because angular acceleration is constant.
Common trap
Do not use rotational SUVAT when angular acceleration varies, and do not insert degrees or revolutions where radians are required.
[ 1 ]
A wheel, initially at rest, rolls without slipping down an incline for 4.0 s . The final angular velocity of the wheel is 5πrads−1.
How many revolutions did the wheel complete?
Rotational inertia
Moment of inertia measures resistance to angular acceleration about an axis. It depends on total mass and how far that mass is distributed from the axis.
Compare distributions
For the same mass and outer radius, more mass farther from the axis gives larger I. A ring therefore has greater rotational inertia than a disk of the same mass and radius.
Common trap
Moment of inertia is not determined by mass alone; always specify the rotation axis and distribution.
[ 3 ]
The disk and a ring, with the same mass and radius, are released from the top of the slope at the same time. Explain, without numerical calculation, which one will reach the bottom of the inclined plane first.
Point-mass model
For discrete masses rotating about an axis,
I=∑mr2
where each r is the perpendicular distance from the axis.
Build the sum
Treat each small sphere, blade or mass element separately, calculate mr2, and add the contributions. Use symmetry when identical masses have equal radii.
Worked example from local Question Bank row 128743
Two 10kg point masses are 8.0m apart and rotate about the midpoint. Each is 4.0m from the axis:
I=∑mr2=2(10)(4.0)2=320kgm2
The full 8.0m separation is not the radius of either mass.
Common trap
Do not use the distance between two masses as r for both; use each mass’s distance to the rotation axis.
[ 1 ]
A two-blade propeller can be modelled using the two-cylinder arrangement in (a)(iii).
The following data for the two-blade propeller are available:
Length of each blade: 0.60 m
Mass of each blade: 2.2 kg
Show that the moment of inertia of the two-blade propeller is about 0.5 kg m2.
Torque–inertia relation
For rotation about a fixed axis,
τnet=Iα
Connect translation and rotation
When a force drives a rotating body or pulley, write both the translational force balance and the rotational torque balance if the system has translating and rotating parts.
Worked example from local Question Bank row 31942
A 50N tangential force acts 2.0m from the axis of a system with I=450kgm2.
τ=Fr=(50)(2.0)=100Nm
α=Iτ=450100=0.22rads−2
The acceleration direction follows the signed resultant torque.
Common trap
Do not treat torque as force or use a moment of inertia that does not match the rotation axis.
[ 1 ]
The graph shows how the angular acceleration α of a flywheel varies with torque τ applied to the flywheel.
What is the moment of inertia of the flywheel?
Rotational momentum
For a rigid body rotating about a fixed axis,
L=Iω
Angular momentum is directed along the rotation axis by the right-hand convention.
Use the matching inertia
The moment of inertia must be calculated about the same axis used for L. A larger I at the same angular speed means larger angular momentum.
Worked example from local Question Bank row 31945
For I=450kgm2 and ω=1.66rads−1,
L=Iω=(450)(1.66)=7.47×102kgm2s−1≈750kgm2s−1
The sign or axis direction must match the chosen rotational convention.
Common trap
Do not substitute translational momentum mv for angular momentum when the question describes rotation.
[ 2 ]
the angular momentum.
Conservation condition
Angular momentum remains constant when the resultant external torque about the chosen axis is zero:
Li=Lf
Redistribute the mass
When a skater pulls their arms inward, I decreases. With angular momentum conserved, ω increases.
Worked example from local Question Bank row 34033
A 0.200kg particle moving at 12.0ms−1 strikes 0.60m from an axis. Its initial angular momentum is
Li=mvr=(0.200)(12.0)(0.60)=1.44kgm2s−1
If the combined system has If=0.252kgm2 and external torque is negligible,
Ifωf=Li⇒ωf=0.2521.44=5.71rads−1
Common trap
Angular momentum conservation does not require rotational kinetic energy to remain constant when the moment of inertia changes.
[ 1 ]
An ice skater is spinning with their arms extended in a fixed position at a constant angular velocity. The ice skater then quickly pulls their arms closer to their body. Frictional effects are negligible.
Three statements are made about the ice skater's motion.
I. The angular momentum of the ice skater remains constant.
II. The rotational kinetic energy of the ice skater remains constant.
III. The net torque acting on the ice skater is zero.
Which of the statements are correct?
Angular impulse
A torque acting for a time changes angular momentum:
ΔL=τΔt=Δ(Iω)
Area under a torque–time graph
If torque varies, the signed area under a τ-against-time graph gives angular impulse and therefore the change in angular momentum.
Common trap
Angular impulse has units N m s, not N s; keep it distinct from linear impulse.
[ 1 ]
What is the unit of angular impulse?
Rotational energy
For a rigid body rotating about a fixed axis,
Ek=21Iω2=2IL2
Combine forms of motion
A rolling object may have translational kinetic energy of its centre of mass and rotational kinetic energy about its centre. Include both when accounting for total kinetic energy.
Worked example from local Question Bank row 31644
A rod of weight 36.0N lowers its centre of mass by 5.00/2=2.50m and has I=30.6kgm2. If the gravitational transfer becomes rotational kinetic energy,
Ek=(36.0)(2.50)=90.0J
90.0=21(30.6)ω2⇒ω=2.43rads−1
The energy result is in joules; angular speed is in radians per second.
Common trap
Do not use 21mv2 alone for a rotating body when its rotational motion contributes energy.
[ 1 ]
A car of total mass M is travelling with a constant speed v. Each of the four wheels of the car has a mass m and a radius R and rolls without slipping.
The moment of inertia of each wheel is I=21mR2.
What is translational kinetic energy of the car sum of the rotational kinetic energy of all four wheels ?
Torque and rotation
Use au=Frsinheta, ∑au=0 for rotational equilibrium and \sum au=Ilpha for angular acceleration. Always state the axis and use the matching moment of inertia.
Describe angular motion
Use angular displacement, angular velocity and angular acceleration; rotational SUVAT applies only for uniform lpha. Point-mass inertia is I=∑mr2.
Track angular momentum
L=Iω,ΔL=auΔt
Conserve angular momentum only when external resultant torque is negligible.
Track rotational energy
E_{rot}=rac12I\omega^2
For rolling or coupled systems, include translational and rotational energy separately.
Define the frame
A reference frame is a coordinate system, with a chosen origin and axes, together with a way of assigning time to events. Position and time are coordinates: they describe an event only after the observer’s frame has been stated.
Describe the same event in two frames
For an event, record its position x and time t in frame S, then x′ and t′ in frame S′. If S′ moves at constant velocity relative to S, both frames are inertial. The event is the same physical occurrence even though its coordinates may differ.
Check the frame type
An inertial reference frame is non-accelerating. Newton’s laws can be used in their usual form in such a frame. If the frame accelerates or rotates, extra apparent forces may be needed and it is not an inertial frame for this syllabus treatment.
Common trap
A frame is not just a camera viewpoint. It specifies the spatial axes and the time measurement used to assign coordinates; therefore “at rest” or “moving” has meaning only relative to a stated frame.
[ 1 ]
Explain why observer Y is at rest in the reference frame of the electron.
State the principle
Galilean relativity says that Newton’s laws have the same form in every inertial reference frame. An observer moving at constant velocity therefore uses the same Newtonian mechanics, provided speeds are far below the speed of light and the frame is non-accelerating.
Relate the observations
The same event occurs in both frames, but the observers can assign different positions. In the classical model, time is absolute: both observers use the same t, while the moving frame changes the position coordinate according to x′=x−vt.
Check the boundary
Use Galilean relativity for inertial frames in the non-relativistic limit. It is not the correct model for measurements involving speeds comparable with c, where the assumptions of absolute time and unchanged light speed fail.
Common trap
“Same laws” does not mean that all observers measure the same position or velocity. It means the equations of Newtonian mechanics keep the same form after changing between inertial frames.
[ 1 ]
Write down the length of the space station according to Galilean relativity.
Transform event coordinates
For frames S and S′ that are coincident at t=t′=0, with S′ moving at velocity v in the positive x-direction relative to S, the Galilean transformations are x′=x−vt and t′=t.
Use the sign convention
Start with the event coordinates (x,t) in S. Substitute the frame velocity with its signed value, calculate x′, and carry the unchanged time t′=t into S′. A positive x′ means the event is on the positive side of S′’s origin.
Check the assumptions
These equations describe the classical model: inertial frames, common synchronized time, and an origin coincidence at t=0. They are not the Lorentz transformations and do not preserve the speed of light between frames.
Symbolic example from local Question Bank row 31622
An event has x′=L and t′=L/c in S′. Galilean time is absolute, so t=t′=L/c. Using the inverse position transformation,
x=x′+vt=L+vcL
The extra vL/c is the distance travelled by the S′ origin during the shared time interval.
Common trap
Do not change t using t′=t−vx/c2; that belongs to the relativistic transformation. In a Galilean transformation, time is shared: t′=t.
[ 1 ]
The Lorentz transformations assume that the speed of light is constant. Outline what the Galilean transformations assume.
Use the classical addition rule
If an object has velocity u in frame S and frame S′ moves at velocity v relative to S, the velocity measured in S′ is u′=u−v. Both u and v are signed velocities along the chosen axis.
Calculate in two steps
Choose the positive direction, write the velocity of the object and the relative frame velocity with signs, then subtract. If the object and S′ move in the same direction, the relative speed is reduced; if they move in opposite directions, the signed relative velocity has greater magnitude.
Check the model
Galilean addition assumes inertial frames, common time, and non-relativistic speeds. It can predict a resultant speed greater than c, which signals that special relativity—not the arithmetic—is required for a high-speed light problem.
Worked example from local Question Bank row 31297
In the classical model, two spacecraft moving in opposite directions at 0.80c have signed velocities u=−0.80c and v=+0.80c.
u′=u−v=−0.80c−0.80c=−1.60c
The magnitude 1.60c shows why Galilean addition cannot describe relativistic relative velocity; the sign only gives direction in S′.
Common trap
Do not subtract speed magnitudes before deciding the direction. The sign of u′ tells you the object’s direction in S′; dropping signs can reverse the physical interpretation.
[ 1 ]
State, using Galilean relativity, the speed of the radio signal relative to Q .
Postulate 1: relativity
The laws of physics have the same form in all inertial reference frames. No inertial observer is privileged by uniform motion; an experiment performed entirely within a frame cannot reveal its constant velocity relative to another inertial frame.
Postulate 2: invariant light speed
Every inertial observer measures the same speed of light in vacuum, c, independent of the motion of the source or observer. This replaces the Galilean expectation that measured velocities simply add.
Use the consequence
Together, the postulates require space and time coordinates to transform differently from the Galilean model. They lead to Lorentz transformations, time dilation, length contraction and relativity of simultaneity. The syllabus does not require deriving those equations.
Common trap
The second postulate does not say that every object moves at c, or that light speed is the same in every material. It refers to light in vacuum measured by inertial observers.
[ 3 ]
Explain, by reference to the equivalence principle, why the frequency of the photon measured at B will be larger than f0.
Set the relativistic factor
For two inertial frames with relative speed v, use γ=1/1−v2/c2. At ordinary speeds γ≈1; as v approaches c, the difference from Galilean coordinates becomes significant.
Transform one event
For an event with coordinates (x,t) in S, the syllabus equations are x′=γ(x−vt) and t′=γ(t−vx/c2) in S′. Use the same signed direction for x and v, and calculate both coordinates from the same event.
Show the coordinate method
Write γ first, substitute the given x,t,v, then report x′ and t′ with units. If the question provides a space–time diagram, reading the coordinates is an alternative only when the axes and scale are correctly interpreted.
Worked example from local Question Bank rows 31630–31631
For v=0.745c, γ=1/1−0.7452=1.499. An event at x=1.0m and t=0 transforms to
x′=γ(x−vt)=1.499(1.0)=1.50m
ct′=γ(ct−cvx)=1.499(0−0.745×1.0)=−1.12m
Thus t′=−1.12/cs; the negative coordinate is valid and reflects the chosen origins.
Respect the syllabus boundary
Know and apply the transformation equations; their derivation is not required. The frames must be inertial, and the relative speed must satisfy v<c so that γ is real.
[ 3 ]
Determine the spacetime coordinates of the event according to observer B.
Use the relativistic rule
For an object with velocity u in S and a frame S′ moving at velocity v relative to S, use u′=(u−v)/(1−uv/c2). The numerator is the classical relative velocity; the denominator is the correction required by special relativity.
Substitute signed velocities
Choose one positive direction, write signed values for u and v, calculate uv/c2, and evaluate the full fraction. Report the magnitude if the question asks for speed; retain the sign if it asks for velocity or direction.
Check the limiting cases
When u≪c and v≪c, the denominator is close to 1 and the result approaches u−v. If u=c, the equation gives u′=c for any sub-light v, so light does not gain or lose speed between inertial frames.
Worked example from local Question Bank row 31056
A train has u=−0.70c in the ground frame and observer P moves at v=+0.60c.
u′=1−(−0.70)(0.60)−0.70c−0.60c=1.42−1.30c=−0.915c≈−0.92c
The negative sign means the train moves opposite P's positive direction; its speed remains below c.
Common trap
Do not use u−v for a high-speed signal. Also do not report a result above c; a sign error or an omitted denominator usually caused it.
[ 2 ]
Determine, using relativistic velocity addition, the speed of the radio signal relative to Q .
Define the interval
For two events separated by Δt and Δx, the space–time interval is (Δs)2=(cΔt)2−(Δx)2. Although observers can measure different Δt and Δx, the value of (Δs)2 is invariant between inertial frames.
Calculate carefully
Read the time and position differences between the same two events. Convert Δt into the distance cΔt, square both terms, and subtract the spatial term: (cΔt)2−(Δx)2. Keep the sign; a negative result is physically meaningful.
Compare frames
Calculate the interval from either frame’s coordinates. Matching values demonstrate invariance and provide a check on transformed coordinates. For a light signal, (Δs)2=0; this null interval is consistent with Δx=cΔt.
Worked example from local Question Bank row 32720
For two events with cΔt=100ly and Δx=20ly,
(Δs)2=(100)2−(20)2=10,000−400=9,600ly2
Any inertial frame must calculate the same 9,600ly2 from its own coordinate differences.
Common trap
Do not replace the subtraction with addition, and do not take an absolute value before reporting. The sign distinguishes the interval type and is part of the answer.
[ 2 ]
Calculate the space-time interval (Δs)2 between P and Q .
Identify proper time
The proper time interval Δt0 is measured between two events that occur at the same position in the observer’s frame. It is the shortest time interval measured for those events. For a clock at rest in the frame, successive ticks occur at one location, so the clock measures Δt0.
Identify proper length
The proper length L0 is the length measured in the rest frame of the object. Its endpoints are measured simultaneously in that frame. It is the maximum length assigned to the object by inertial observers.
Choose from the event conditions
For time, ask: do the two events happen at the same place in this frame? For length, ask: is the object at rest in this frame, and are both endpoints measured at the same time? These conditions, not the observer’s label, determine whether the measurement is proper.
Common trap
Proper time is not simply the time measured by the “main” observer, and proper length is not the shortest measured length. The proper length is the rest-frame, longest length; moving observers measure a contracted length.
[ 1 ]
Define what is meant by proper length.
Use the time-dilation equation
When Δt0 is the proper time between two events, an observer for whom the events occur at different positions measures Δt=γΔt0, where γ=1/1−v2/c2.
Identify the proper interval first
Find the frame in which the two events occur at the same place; that frame measures Δt0. Calculate γ using the relative speed, then multiply by Δt0 to obtain the longer interval measured in the other inertial frame.
Check the direction of the effect
Because γ≥1, the non-proper observer measures a time interval at least as large as the proper interval. At v=0, γ=1 and the two measurements agree.
Worked example from local Question Bank rows 30639–30640
A spacecraft crosses 1.80×1011m at 0.750c. The station-frame interval is
Δt=0.750(3.00×108)1.80×1011=800s
With γ=1/1−0.7502=1.51, the spacecraft clock measures the proper time
Δt0=1.51800=530s
The events occur at one place on the spacecraft, so its interval is proper.
Common trap
Do not multiply the proper time by 1/γ when finding the dilated interval. The inverse is used only when the question gives the larger interval and asks for the proper time.
[ 2 ]
S arrives at P after 50 years according to Earth. Calculate the time at which S arrives at P according to S clocks.
Use the contraction equation
If L0 is the proper length measured in the object’s rest frame, an observer who sees the object moving at speed v measures L=L0/γ, with γ=1/1−v2/c2.
Select the proper length
Find the frame in which the object is at rest; that frame measures L0. Calculate γ, then divide the proper length by γ. The endpoints must be measured simultaneously in the observer’s frame.
Check the result
Since γ≥1, a moving observer measures L≤L0. At low speed the contraction is negligible; as v approaches c, the measured length along the direction of motion becomes substantially smaller.
Worked example from local Question Bank row 30450
A rocket's proper length is L0=450m and γ=5/3. An observer who sees it moving measures
L=γL0=5/3450=270m
Only the dimension parallel to the relative motion is contracted.
Common trap
Do not contract a length perpendicular to the motion, and do not multiply by γ when the requested quantity is the moving-frame length.
[ 2 ]
Calculate the length of the space station according to observer B, with reference to special relativity.
State the idea
Two events that are simultaneous in one inertial reference frame need not be simultaneous in another frame moving relative to it. Simultaneity is therefore not an absolute property of separated events.
Use the transformed time
For two events, Δt′=γ(Δt−vΔx/c2). If Δt=0 in S but Δx=0, then Δt′=0 in a relatively moving frame.
Worked example from local Question Bank row 30453
Two lamps are simultaneous in S and separated by 9.00×103m. For v=0.80c and γ=5/3,
Δt′=35(0−c2(0.80c)(9.00×103))=−4.0×10−5s
The negative sign fixes the event order in S′; it is not an error.
Keep the order test local
To decide which event occurs first in a frame, calculate or read the sign of Δt′ using the same pair of events. A negative time difference means the event assigned as the second reference event occurs earlier in that frame.
Common trap
The relativity of simultaneity concerns spatially separated events. Events at the same place cannot be simultaneous in one frame and ordered differently in another inertial frame.
[ 2 ]
According to observer B, event E occurs before observer A and observer B meet. Justify this statement using the spacetime diagram.
Read the axes
A space–time diagram plots position horizontally and ct vertically; the time axis is labelled ct, so both axes have distance units. An event is a point (x,ct). A world line joins the events of one object through time.
Interpret a world line
A vertical world line represents an object at rest in that frame. A straight tilted line represents constant velocity. A light ray has v=c and lies on the 45° light line when the axes use equal scales; no physical world line may be steeper toward the x-axis than the light line.
Read simultaneity and coordinates
To find an event’s time, project horizontally to the ct axis; to find position, project vertically to the x axis. Lines parallel to an observer’s x′ axis represent equal t′, while lines parallel to ct′ represent equal x′.
Common trap
Do not treat the slope as an ordinary x/t graph slope without accounting for the ct axis and the diagram’s scale. Always identify which frame’s axes are being used.
[ 2 ]
Identify, with lines and labels on the spacetime diagram, the difference between t1 and t2.
Use the angle relation
On a space–time diagram with equal scales, the angle θ between a particle’s world line and the time axis satisfies tanθ=v/c. Therefore v=ctanθ.
Read the line
A vertical line has θ=0 and represents rest. As the line tilts toward the x-axis, θ and the speed increase. The light line has θ=45∘ on equal scales and represents v=c.
Calculate from a diagram
Measure or read the angle from the time axis, evaluate tanθ, and multiply by c. If the diagram gives a rise/run ratio, use that ratio as tanθ only after confirming the axes and angle definition.
Worked example from local Question Bank row 31477
For a world line representing v=0.80c on equal-scale axes,
θ=tan−1(v/c)=tan−1(0.80)=38.7∘≈39∘
The angle is measured from the ct axis, not the x axis.
Common trap
Do not measure the angle from the x-axis, and do not assume every diagram uses equal visual scales. The syllabus relation is tied to the stated world-line angle and labelled axes.
[ 1 ]
Rocket R travels away from an observer on Earth at a speed of 0.80 c . A space-time diagram shows four world lines.
What is the correct world line of R in the reference frame of Earth?
Start from the observation
Muons created high in Earth’s atmosphere have a short proper lifetime, yet many are detected at the ground while travelling at speeds close to c. Without relativistic effects, the flight time through the atmosphere would exceed the muon lifetime and far fewer would survive.
Explain it in the Earth frame
In the Earth frame the moving muon’s lifetime is dilated: Δt=γΔt0. The increased lifetime allows more muons to travel the atmospheric distance before decaying. This is experimental evidence for time dilation.
Explain it in the muon frame
In the muon’s frame, the atmosphere is moving and its thickness is length-contracted: L=L0/γ. The shorter distance can be crossed within the muon’s proper lifetime. Both frames predict the same detection rate; together they support time dilation and length contraction.
Evidence calculation from local Question Bank row 30447
Muons are produced 2.0km above ground, move at 0.98c, have proper lifetime 2.2μs and γ=5.0.
tflight=0.98(3.0×108)2000=6.8μs
tEarth=γt0=(5.0)(2.2)=11μs
The dilated Earth-frame lifetime exceeds the flight time, explaining why many more muons reach the ground than the non-relativistic model predicts.
Common trap
Do not claim that the muon’s own clock runs slow in its rest frame. The proper lifetime is measured by the muon; the Earth observer measures the dilated lifetime, while the muon observer measures a contracted atmosphere.
[ 3 ]
Muons are detected at the Earth's surface.
Explain, with supporting calculations, why this is evidence for time dilation.
Choose the model
State the inertial reference frame first. Galilean relativity uses x′=x−vt, t′=t and u′=u−v. Special relativity uses the two postulates, Lorentz transformations and u′=(u−v)/(1−uv/c²).
Track what changes and what is invariant
In special relativity, use γ=1/√(1−v²/c²), the invariant interval (Δs)²=(cΔt)²−(Δx)², proper time, proper length, Δt=γΔt0 and L=L0/γ. Separate measurements of space and time can change between frames, while the interval and vacuum light speed do not.
Read the evidence
On a space–time diagram, world-line angle gives tanθ=v/c, frame axes determine simultaneity, and no world line exceeds the light line. Muon survival provides experimental evidence: time dilation explains the longer Earth-frame lifetime, while length contraction explains the shorter atmospheric distance in the muon frame.
Final retrieval check
For every calculation, identify the frame, select the proper quantity if one is given, keep signed velocities and units consistent, and check the result against c, γ≥1, or the invariant interval. The syllabus requires applying the transformations and equations, not deriving them.