1. Physics
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  3. Motion in a Plane

Kinematics · JEE & NEET Physics

Motion in a Plane: notes and previous year questions

Position, velocity and acceleration as vectors, the independence of perpendicular motions, and the split–solve–stitch method.

Motion in a Plane in short

  • A motion in a plane is two independent straight-line motions, along x and along y, happening at the same time.
  • The position vector r = xî + yĵ points from the origin to the object; its size comes from Pythagoras.
  • tan⁻¹(y/x) cannot tell opposite quadrants apart: check the signs of x and y.
  • Displacement is the change in position (a straight chord); distance is the length of the path.

1Why one number is not enough

A plane that climbs as it flies forward cannot be tracked with one number: we need how far forward (xx) and how high (yy). Its shadow on the ground moves along a straight line, and so does its shadow on a wall. Each shadow is a one-dimensional motion.

2Position and displacement

The position vector is an arrow from the origin to the object. With i^\hat{i} and j^\hat{j} the unit arrows along xx and yy:

r⃗=xi^+yj^\vec{r} = x\hat{i} + y\hat{j}
∣r⃗∣=x2+y2|\vec{r}| = \sqrt{x^2 + y^2}For x = 4 m, y = 3 m: |r| = 5 m.
θ=tan⁡−1 ⁣(yx)\theta = \tan^{-1}\!\left(\frac{y}{x}\right)Measured from the positive x-axis: here about 37°.

The displacement from r⃗1\vec{r}_1 to r⃗2\vec{r}_2 is the change in position; its size is the straight-line distance between the points (Pythagoras):

s⃗=r⃗2−r⃗1=Δx i^+Δy j^\vec{s} = \vec{r}_2 - \vec{r}_1 = \Delta x\,\hat{i} + \Delta y\,\hat{j}
∣s⃗∣=(Δx)2+(Δy)2|\vec{s}| = \sqrt{(\Delta x)^2 + (\Delta y)^2}A(2, 3) to B(5, 7): s = 3î + 4ĵ m, |s| = 5 m.

Along a curved path, the distance is the length of the curve, while the displacement is the straight chord. Distance ≥ |displacement|, always.

3Velocity in a plane

v⃗avg=Δr⃗Δt\vec{v}_{\text{avg}} = \frac{\Delta\vec{r}}{\Delta t}It points along the displacement, not along the path.

Example: from A(2, 3) to B(5, 7) in 2 s, v⃗avg=(3i^+4j^)/2=1.5i^+2j^\vec{v}_{\text{avg}} = (3\hat{i} + 4\hat{j})/2 = 1.5\hat{i} + 2\hat{j} m/s, of size 2.5 m/s.

The instantaneous velocity comes from differentiating each component separately:

v⃗=dr⃗dt=vxi^+vyj^\vec{v} = \frac{d\vec{r}}{dt} = v_x\hat{i} + v_y\hat{j}
∣v⃗∣=vx2+vy2|\vec{v}| = \sqrt{v_x^2 + v_y^2}
tan⁡θ=vyvx\tan\theta = \frac{v_y}{v_x}

4Acceleration in a plane

a⃗=dv⃗dt=axi^+ayj^\vec{a} = \frac{d\vec{v}}{dt} = a_x\hat{i} + a_y\hat{j}
∣a⃗∣=ax2+ay2|\vec{a}| = \sqrt{a_x^2 + a_y^2}

In a plane, the acceleration need not point along the velocity. Split it into two parts: the part along v⃗\vec{v} changes the speed; the part perpendicular to v⃗\vec{v} changes the direction. That is why paths curve.

MotionAcceleration
Speeding up in a straight linealong v: only the speed changes
Turning at a steady speedperpendicular to v: only the direction changes
Speeding up round a bendboth parts

5Independence of perpendicular motions

Drop one ball and push another off a table sideways at the same instant. At every moment they are at the same height, and they land together: the sideways motion has no effect on the fall. Motion along xx does not affect motion along yy, and vice versa.

Along xAlong y
vx=ux+axtv_x = u_x + a_x tvy=uy+aytv_y = u_y + a_y t
x=uxt+12axt2x = u_x t + \tfrac{1}{2}a_x t^2y=uyt+12ayt2y = u_y t + \tfrac{1}{2}a_y t^2
vx2=ux2+2axxv_x^2 = u_x^2 + 2a_x xvy2=uy2+2ayyv_y^2 = u_y^2 + 2a_y y

6Vector equations and circular motion

With a constant a⃗\vec{a}, the equations of motion hold for whole vectors (each vector equation is two ordinary ones):

v⃗=u⃗+a⃗t\vec{v} = \vec{u} + \vec{a}t
s⃗=u⃗t+12a⃗t2\vec{s} = \vec{u}t + \tfrac{1}{2}\vec{a}t^2
v2=u2+2 a⃗⋅s⃗v^2 = u^2 + 2\,\vec{a}\cdot\vec{s}

Circular motion from calculus. For r⃗=Rcos⁡(ωt) i^+Rsin⁡(ωt) j^\vec{r} = R\cos(\omega t)\,\hat{i} + R\sin(\omega t)\,\hat{j}:

  • v⃗=−Rωsin⁡(ωt) i^+Rωcos⁡(ωt) j^\vec{v} = -R\omega\sin(\omega t)\,\hat{i} + R\omega\cos(\omega t)\,\hat{j}, so the speed ∣v⃗∣=Rω|\vec{v}| = R\omega is constant.
  • a⃗=−ω2r⃗\vec{a} = -\omega^2\vec{r}: toward the centre, of size ω2R\omega^2 R.
  • v⃗⋅a⃗=0\vec{v}\cdot\vec{a} = 0: velocity and acceleration are perpendicular at every instant, so the acceleration only turns the object.

Summary

Key ideas

  • A motion in a plane is two independent straight-line motions, along x and along y, happening at the same time.
  • The position vector r = xî + yĵ points from the origin to the object; its size comes from Pythagoras.
  • tan⁻¹(y/x) cannot tell opposite quadrants apart: check the signs of x and y.
  • Displacement is the change in position (a straight chord); distance is the length of the path.
  • Displacements add as vectors: 3 m east and 4 m north make 5 m, not 7 m.
  • Average velocity points along the displacement; instantaneous velocity is tangent to the path.
  • The part of the acceleration along v changes the speed; the part across v changes the direction.
  • Perpendicular motions are independent: a ball pushed off a table lands at the same time as one dropped.
  • Split, solve each axis, stitch with Pythagoras; time is the only link between the axes.
  • With constant acceleration, v = u + at and s = ut + ½at² hold as vector equations.
  • In uniform circular motion the speed Rω is constant and the acceleration ω²R points to the centre, perpendicular to v.

Every equation

Position vector
r⃗=xi^+yj^\vec{r} = x\hat{i} + y\hat{j}
Its size
∣r⃗∣=x2+y2|\vec{r}| = \sqrt{x^2 + y^2}
Its direction
θ=tan⁡−1(y/x)\theta = \tan^{-1}(y/x)
Displacement
s⃗=r⃗2−r⃗1\vec{s} = \vec{r}_2 - \vec{r}_1
Its size
∣s⃗∣=(Δx)2+(Δy)2|\vec{s}| = \sqrt{(\Delta x)^2 + (\Delta y)^2}
Average velocity
v⃗avg=Δr⃗/Δt\vec{v}_{\text{avg}} = \Delta\vec{r}/\Delta t
Velocity
v⃗=dr⃗/dt=vxi^+vyj^\vec{v} = d\vec{r}/dt = v_x\hat{i} + v_y\hat{j}
Speed
∣v⃗∣=vx2+vy2|\vec{v}| = \sqrt{v_x^2 + v_y^2}
Direction of velocity
tan⁡θ=vy/vx\tan\theta = v_y/v_x
Acceleration
a⃗=dv⃗/dt=axi^+ayj^\vec{a} = d\vec{v}/dt = a_x\hat{i} + a_y\hat{j}
Constant a: velocity
v⃗=u⃗+a⃗t\vec{v} = \vec{u} + \vec{a}t
Constant a: displacement
s⃗=u⃗t+12a⃗t2\vec{s} = \vec{u}t + \tfrac{1}{2}\vec{a}t^2
Constant a: no time
v2=u2+2 a⃗⋅s⃗v^2 = u^2 + 2\,\vec{a}\cdot\vec{s}
Circle: speed
∣v⃗∣=Rω|\vec{v}| = R\omega
Circle: acceleration
a⃗=−ω2r⃗\vec{a} = -\omega^2\vec{r}

Previous year questions with solutions

Real JEE and NEET questions on motion in a plane. Try each one before you open the solution.

Q1JEE Main 2024Numerical answer

A vector has magnitude same as that of A⃗=3i^+4j^\vec{A} = 3\hat{i} + 4\hat{j} and is parallel to B⃗=4i^+3j^\vec{B} = 4\hat{i} + 3\hat{j}. The xx and yy components of this vector in first quadrant are xx and 33 respectively where x=x = __________.

Show answer and solution

Answer: 4

The direction comes from B⃗\vec{B} and the size from A⃗\vec{A}, so build it out of both.

∣A⃗∣=9+16=5|\vec{A}| = \sqrt{9 + 16} = 5, and B^=4i^+3j^5\hat{B} = \dfrac{4\hat{i} + 3\hat{j}}{5} since ∣B⃗∣=5|\vec{B}| = 5 as well.

The vector wanted is 5B^=4i^+3j^5\hat{B} = 4\hat{i} + 3\hat{j}, so x=4x = 4 — and the yy-component of 33 quoted in the question confirms it.

Q2NEET 2016One correct option

If the magnitude of sum of two vectors is equal to the magnitude of difference of the two vectors, the angle between these vectors is

  1. A45o45^{o}
  2. B180o180^{o}
  3. C0o0^{o}
  4. D90o90^{o}
Show answer and solution

Answer: Option D

Square both statements and set them side by side: A2+B2+2ABcos⁡θ=A2+B2−2ABcos⁡θA^{2} + B^{2} + 2AB\cos\theta = A^{2} + B^{2} - 2AB\cos\theta. Everything cancels except the middle terms, leaving 4ABcos⁡θ=04AB\cos\theta = 0. Neither vector has zero length, so it must be cos⁡θ\cos\theta that vanishes, and θ=90∘\theta = 90^{\circ}. In the picture it is the parallelogram whose two diagonals come out the same length, which happens only when it is a rectangle.

Q3JEE Main 2024One correct option

If two vectors A⃗\vec{A} and B⃗\vec{B} having equal magnitude RR are inclined at angle θ\theta, then

  1. A∣A⃗+B⃗∣=2Rcos⁡(θ2)|\vec{A}+\vec{B}|=2R\cos (\frac{\theta }{2})
  2. B∣A⃗−B⃗∣=2Rcos⁡(θ2)|\vec{A}-\vec{B}|=2R\cos (\frac{\theta }{2})
  3. C∣A⃗−B⃗∣=2Rsin⁡(θ2)|\vec{A}-\vec{B}|=\sqrt{2}R\sin (\frac{\theta }{2})
  4. D∣A⃗+B⃗∣=2Rsin⁡(θ2)|\vec{A}+\vec{B}|=2R\sin (\frac{\theta }{2})
Show answer and solution

Answer: Option A

Here RR is the shared magnitude, not the resultant. Put both magnitudes equal to RR: ∣A⃗+B⃗∣=R2+R2+2R2cos⁡θ=R2(1+cos⁡θ)|\vec{A}+\vec{B}|=\sqrt{R^{2}+R^{2}+2R^{2}\cos\theta}=R\sqrt{2(1+\cos\theta)}, and 1+cos⁡θ=2cos⁡2(θ/2)1+\cos\theta=2\cos^{2}(\theta/2), which gives 2Rcos⁡(θ/2)2R\cos(\theta/2).

If that identity does not come to mind, test the special angles. At θ=0∘\theta=0^{\circ} the vectors coincide, so ∣A⃗+B⃗∣=2R|\vec{A}+\vec{B}|=2R and ∣A⃗−B⃗∣=0|\vec{A}-\vec{B}|=0, which kills B and D. At θ=180∘\theta=180^{\circ} the difference is 2R2R but option C offers only 2R\sqrt{2}R. A is left.

Practice questions, easy to hard

Three questions from the motion in a plane practice ladder: one easy, one medium, one hard.

Q4Numerical answer

A walker goes 6 m6\ \mathrm{m} east, then 8 m8\ \mathrm{m} north. Head to tail, these two displacements make a right-angled triangle.

How long is the closing side, in m\mathrm{m}?

Show answer and solution

Answer: 10

The closing side is the sum of the two displacements, and in a right-angled triangle its length is 62+82=100=10 m\sqrt{6^{2}+8^{2}}=\sqrt{100}=10\ \mathrm{m}. It is not 14 m14\ \mathrm{m}: vectors only add like plain numbers when they point the same way.

Q5Numerical answer

Two vectors drawn from the same point do not add end to end unless they already line up. Complete the parallelogram on them: the sum is the diagonal through that point, and its length is R=A2+B2+2ABcos⁡θR = \sqrt{A^{2} + B^{2} + 2AB\cos\theta}, where θ\theta is the angle between them.

Two vectors of magnitudes 55 and 33 have 60∘60^{\circ} between them. What is the magnitude of their sum?

Show answer and solution

Answer: 7

cos⁡60∘=12\cos 60^{\circ} = \tfrac12, so R=25+9+2×5×3×12=49=7R = \sqrt{25 + 9 + 2 \times 5 \times 3 \times \tfrac12} = \sqrt{49} = 7. The other diagonal of that same parallelogram is the difference A⃗−B⃗\vec{A} - \vec{B}, and it carries the same formula with the sign flipped, A2+B2−2ABcos⁡θ\sqrt{A^{2} + B^{2} - 2AB\cos\theta}, because reversing B⃗\vec{B} turns θ\theta into 180∘−θ180^{\circ} - \theta and the cosine changes sign with it. Here that would give 19\sqrt{19}, about 4.364.36.