Relative Motion
Study of the motion of a point as observed from different reference frames. Covers position, velocity, and acceleration transformations, the Galilean principle of relativity, and fictitious forces in rotating frames.
Complete Theory
5Consider two reference frames: a fixed (inertial) frame S and a moving frame S'. A point A is observed from both.
Three vectors describe its position:
- — absolute position of A as measured in S (from O to A).
- — position of the origin of S' as seen from S. It tells us where S' is located relative to S. Its time derivative gives the transport velocity.
- — relative position of A as measured in S'. This is the position of A relative to O' — the coordinates that an observer in S' assigns to A. Physically: if you were riding on S', this is where you would say "A is relative to me".
If S' translates relative to S (no rotation), differentiating the position relation gives the velocity composition law for pure translation:
where:
- — absolute velocity of A measured in S (derivative of ).
- — relative velocity of A measured by an observer in S' (derivative of ).
- — transport velocity (velocity of S' relative to S), the derivative of . Independent of A.
Differentiating the velocity relation gives the acceleration composition for pure translation:
- — absolute acceleration (measured in S).
- — relative acceleration (measured in S').
- — transport acceleration (of S' relative to S).
When S' rotates with angular velocity relative to S, the unit vectors of S' are themselves rotating: their time derivative is not zero but .
The relative derivative theorem (Poisson's formula) relates the time derivative of any vector as seen from S versus from S':
Interpretation:
- — change of seen from the fixed frame S.
- — change of seen from the rotating frame S'.
- — correction term due to the rotation of S'. If (no rotation), the two derivatives coincide.
Applying the relative derivative theorem to gives the velocity in a rotating-and-translating frame S':
where is the rotational transport term: even if A is stationary in S', it rotates with S'.
Differentiating again gives the acceleration. When multiplied by mass, the extra terms become fictitious forces:
1. Centrifugal force
- Points radially outward from the rotation axis.
- Depends only on position ( = distance from axis), not on relative velocity.
- Causes the equatorial bulge and reduces effective at the equator by ~0.3%.
- Depends on relative velocity : a body stationary in S' experiences no Coriolis force.
- Always perpendicular to both and → deflects motion without doing work.
- On Earth: deflects moving objects to the right in the northern hemisphere, to the left in the southern. Explains cyclone rotation and trade wind patterns.
Worked Examples
3Example 1Train — passenger throws a ball vertically
Given
S' = train (moving frame), S = ground (fixed frame)
east: velocity of the train (S') relative to the ground (S)
upward (vertical): velocity of the ball (A) measured by the passenger on the train (S')
Find
Absolute velocity of the ball as seen from the ground
Where does the ball land?
Step-by-step solution
1Identify the frames: S (fixed) = ground, S' (moving) = train. Point A is the ball. The train moves eastward at (ULM). The passenger throws the ball vertically upward at relative to the train.
2Velocity composition: apply . The absolute velocity is the vector sum of the horizontal component (train motion) and vertical component (throw): . Magnitude: , direction: above the horizontal.
3Motion seen from S (ground): the ball follows a parabolic trajectory. The question is "where does it land for the passenger?" Seen from S, the ball lands ahead of the launch point.
4Motion seen from S' (train): for the passenger, the ball goes straight up and down (). Flight time: . The ball returns to the passenger's hand because the relative horizontal velocity is zero.
5Galilean Relativity: the passenger cannot tell whether the train is stationary or in ULM using mechanical experiments. The laws of physics (conservation of momentum, free fall) are identical because .
✓ Final result: Absolute velocity (magnitude 30.4 m/s at 9.5°). The ball returns to the passenger's hand.
Example 2Boat in a river
Given
: boat speed relative to the water (relative velocity, measured in S' = water)
: current velocity (water relative to the bank, transport velocity S'/S)
: river width
Find
(a) If the boat points straight across, what is the crossing time and where does it land?
(b) What angle should it head to cross straight across (zero drift)?
Step-by-step solution
1Setup: S (fixed) = riverbank; S' (moving) = water (current). Boat B has relative velocity (measured in S') and the current has transport velocity parallel to the bank.
2(a) Point straight across: the crossing component is . Time: . During crossing, the current carries the boat downstream. The absolute velocity relative to the bank is (magnitude 5 m/s, direction 53° from the bank).
3(b) Straight crossing (zero drift): the boat must head upstream at angle such that the horizontal component of its relative velocity cancels the current: → → from the perpendicular. The effective crossing speed is , giving .
✓ Final result: (a) 30 s crossing, 90 m downstream drift. (b) Head 48.6° upstream from perpendicular, crossing time 45.3 s, zero drift.
Example 3Coriolis force on Earth
Given
: Earth's angular velocity
north: relative velocity of a body (wind, projectile)
latitude N
Find
Magnitude of the Coriolis force per unit mass
Direction of deflection
Consequences: winds and cyclones
Step-by-step solution
1The Coriolis force arises because Earth is a rotating (non-inertial) frame. For a body moving relative to the surface, . Only the component of perpendicular to the motion plane contributes.
2Vertical component of : at latitude , the local vertical component is . The horizontal component contributes a vertical force (negligible for horizontal motion).
3Force magnitude: per kg. Small ( of weight), but acting over large air/water masses for long times it produces observable effects.
4Deflection direction: in the northern hemisphere, is to the right of the direction of motion (right-hand rule: up, north → east). In the southern hemisphere it is to the left. At the equator () the vertical component vanishes → no horizontal Coriolis.
5Observed effects: cyclones rotate counterclockwise in the northern hemisphere (air converges toward low pressure and is deflected right). Trade winds, long-range projectiles, and ocean currents all show this deflection. Foucault's pendulum precession is also due to Coriolis.
✓ Final result: . Deflection to the right in the northern hemisphere, left in the southern.
Exercises with Solutions
2Exercise 1Velocity composition — airplane with crosswindMedium
Problem to solve
A pilot wants to fly due north. The airplane's airspeed is . A crosswind blows from west to east at . (a) If the pilot simply points north, what is the actual ground speed and direction? (b) What heading angle must the pilot maintain to fly exactly north?
Given data
v_{plane/air} = 300 m/s north (relative velocity to air S')v_{wind} = 40 m/s east (velocity of air S' relative to ground S)
Step-by-step solution
1(a) Point north: absolute velocity is . Magnitude: . Direction: east of north. The airplane drifts eastward.
2(b) Fly exactly north: the eastward component of the plane's relative velocity must cancel the wind: → west of north. The effective northward speed is .
✓ Final answer: (a) 302.7 m/s drifting 7.6° east of north. (b) Head 7.66° west of north; effective ground speed 297.3 m/s due north.
Exercise 2Accelerating frame — apparent weight in an elevatorHard
Problem to solve
A person of mass stands on a scale inside an elevator. The elevator accelerates upward at . (a) What does the scale read (apparent weight)? (b) What fictitious force acts on the person in the elevator's frame? (c) If the elevator accelerates downward at , what does the scale read? (d) What happens in free fall ()?
Given data
(person's mass) upward (acceleration of S' = elevator relative to S = ground)
Step-by-step solution
1Setup: S (fixed) = ground (inertial). S' (accelerating) = elevator. The elevator accelerates upward with . Forces on the person: weight and normal reaction from the scale (upward).
2(a) Apparent weight going up: in S (ground), Newton's second law gives , so . The scale reads this value, which is larger than the real weight : the person feels heavier.
3(b) Fictitious force in S': in S' (elevator), the person is at rest relative to the elevator. To apply in S', we add the fictitious force (downward). In S' the equilibrium is , giving the same .
4(c) Downward acceleration (): in S: → . The person feels lighter. The fictitious force is (upward).
5(d) Free fall (): if the cable snaps, . The scale reads zero: the person is weightless. In S', the fictitious force exactly cancels the real weight: .
6Conclusion: apparent weight is the normal force the floor (scale) exerts on the person. It changes with the acceleration of the system, unlike real weight , which is constant.
✓ Final answer: (a) 896.7 N (heavier). (b) 210 N downward fictitious force. (c) 476.7 N (lighter). (d) 0 N — weightlessness.
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Integrative Problems
Problems combining all chapters — exam levelProblem 1Tower, Ballistic Pendulum, and Keplerian OrbitEXTREME
A cannon is placed on top of a tower tall and fires a projectile of horizontally at .
The projectile strikes and embeds in a wooden block hanging from a rope of length (ballistic pendulum), at ground level.
The Earth-Moon system is then used as a reference for Kepler's third law.
The projectile strikes and embeds in a wooden block hanging from a rope of length (ballistic pendulum), at ground level.
The Earth-Moon system is then used as a reference for Kepler's third law.
📌 Problem data
(a)Uniformly Accelerated Motion(b)Inelastic Collision(c)Potential Energy + Pendulum(d)Moment of Inertia — Rigid Body(e)Gravitation — Kepler's Third Law
Problem 2Spring, Rolling Disk, Inclined Plane Collision, and ConservationEXTREME
A spring (, compressed ) launches a solid disk (, ) up an inclined plane (, , ) that rolls without slipping.
At the top the disk is launched horizontally and strikes a pendulum (, ) — perfectly inelastic collision. What is asked (solved below, a→e): (a) the disk's speed at the top of the plane; (b) the range and impact speed of the horizontal launch; (c) the speed after the inelastic collision with the pendulum and the energy lost; (d) the pendulum's maximum angle, the maximum tension, and whether it completes the loop; (e) the full energy balance (from spring to maximum angle).
At the top the disk is launched horizontally and strikes a pendulum (, ) — perfectly inelastic collision. What is asked (solved below, a→e): (a) the disk's speed at the top of the plane; (b) the range and impact speed of the horizontal launch; (c) the speed after the inelastic collision with the pendulum and the energy lost; (d) the pendulum's maximum angle, the maximum tension, and whether it completes the loop; (e) the full energy balance (from spring to maximum angle).
📌 Problem data
(a)Energy + Rigid Body (rolling)(b)Kinematics — Projectile(c)Inelastic Collision + CM(d)Pendulum Dynamics + Forces(e)Conservation Laws — Complete Energy Balance