Academy
Formulas/physics/Kinematics/Relative Velocity

Relative Velocity

Velocity of A as observed from B.
Class 11Class JEE
Derivation

What this formula says

Every velocity is measured relative to some observer. When we say a car is moving at 6060 km/h, we mean relative to the ground. But an observer in another moving car sees a different velocity.

The velocity of object A as seen by observer B is:

vAB=vAvB\vec{v}_{AB} = \vec{v}_A - \vec{v}_B

Here:

  • vA\vec{v}_A is the velocity of A relative to the ground
  • vB\vec{v}_B is the velocity of B relative to the ground
  • vAB\vec{v}_{AB} is the velocity of A as seen by B (A relative to B)

Building the concept from scratch

Imagine you are standing on the ground watching two cars on a straight road.

  • Car A moves at +60+60 km/h (to the right)
  • Car B moves at +40+40 km/h (to the right)

From the ground, both are moving right. But a passenger in car B sees car A moving away — but only at 6040=2060 - 40 = 20 km/h. Car A appears slow from car B's perspective.

Now imagine car B is moving at 40-40 km/h (to the left). The passenger in car B now sees car A approaching at 60(40)=10060 - (-40) = 100 km/h — much faster, because they are moving toward each other.

This is the physical meaning of vAB=vAvB\vec{v}_{AB} = \vec{v}_A - \vec{v}_B.

Derivation

Let xAx_A and xBx_B be the positions of A and B at time tt, measured from a fixed point on the ground.

The position of A relative to B is:

xAB=xAxBx_{AB} = x_A - x_B

Differentiate both sides with respect to time:

dxABdt=dxAdtdxBdt\frac{d x_{AB}}{dt} = \frac{d x_A}{dt} - \frac{d x_B}{dt}

By definition, dxdt\frac{dx}{dt} is velocity. So:

vAB=vAvB\boxed{\vec{v}_{AB} = \vec{v}_A - \vec{v}_B}

The formula is a direct consequence of subtracting positions and differentiating. Nothing more is assumed.

Direction matters — this is a vector equation

In one dimension, the sign carries the direction. In two or three dimensions, the velocities are full vectors and must be subtracted as vectors — including direction.

Example in 1D:

Two trains on parallel tracks:

  • Train A: 8080 km/h east → vA=+80\vec{v}_A = +80
  • Train B: 5050 km/h east → vB=+50\vec{v}_B = +50

Velocity of A relative to B: vAB=8050=+30 km/h east\vec{v}_{AB} = 80 - 50 = +30 \text{ km/h east}

A passenger in train B sees train A moving east at 3030 km/h — slowly pulling ahead.

Same trains, but B moving west:

  • Train B: 5050 km/h west → vB=50\vec{v}_B = -50

vAB=80(50)=+130 km/h east\vec{v}_{AB} = 80 - (-50) = +130 \text{ km/h east}

The trains are approaching each other — from B's perspective, A is rushing toward it at 130130 km/h.

The reverse: velocity of B relative to A

vBA=vBvA=vAB\vec{v}_{BA} = \vec{v}_B - \vec{v}_A = -\vec{v}_{AB}

The relative velocity reverses when you swap who is observing whom. If A sees B moving at +30+30 km/h east, then B sees A moving at 30-30 km/h east (i.e. 3030 km/h west). This is always true.

Relative velocity in two dimensions

When the two objects move in different directions, subtract the velocity vectors component by component.

Object A moves at vAv_A at angle α\alpha from the x-axis. Object B moves at vBv_B at angle β\beta from the x-axis.

Components of relative velocity:

(vAB)x=vAcosαvBcosβ(\vec{v}_{AB})_x = v_A\cos\alpha - v_B\cos\beta

(vAB)y=vAsinαvBsinβ(\vec{v}_{AB})_y = v_A\sin\alpha - v_B\sin\beta

Magnitude of relative velocity:

vAB=(vAB)x2+(vAB)y2|\vec{v}_{AB}| = \sqrt{(\vec{v}_{AB})_x^2 + (\vec{v}_{AB})_y^2}

Special cases:

  • Moving in the same direction: vAB=vAvB|\vec{v}_{AB}| = |v_A - v_B| — relative velocity is the difference
  • Moving in opposite directions: vAB=vA+vB|\vec{v}_{AB}| = v_A + v_B — relative velocity is the sum
  • Moving at right angles: vAB=vA2+vB2|\vec{v}_{AB}| = \sqrt{v_A^2 + v_B^2}
Key Idea
The concept of relative velocity is the foundation of the special theory of relativity. At everyday speeds, velocities simply subtract as shown here. At speeds approaching the speed of light, the subtraction formula is modified — but the underlying idea is the same.
Remember
Rain problem: To find the angle at which to hold an umbrella, find the velocity of rain relative to the person. If rain falls vertically at $v_r$ and the person walks horizontally at $v_p$, the relative velocity of rain has magnitude $\sqrt{v_r^2 + v_p^2}$ and is tilted forward — the umbrella must be tilted at $\tan^{-1}(v_p / v_r)$ from vertical.