Motion in a Plane (Resolved Components / Polar)
At a Glance
- Frequency: 1 sub-part across 1 of 13 years (2020)
- Priority tier: T4
- Marks (count): 10 (1)
- Average solve time: ~15 min
- Difficulty mix: medium 1
- Section: A | Dominant type: proof
Why This Chapter Matters
UPSC appeared once (2020) asking a derivation of the polar-component form of velocity and acceleration. The topic tests whether you can pass from Cartesian differentiation of x=rcosθ, y=rsinθ to the clean radial-transverse decomposition used throughout dynamics. A clean, well-labelled derivation earns all marks in one go.
Minimum Theory
Polar coordinates in the plane
Let a particle’s position be (r,θ) in polar coordinates, with unit vectors e^r (radially outward) and e^θ (transverse, 90° anticlockwise from e^r).
e^r=cosθi^+sinθj^,e^θ=−sinθi^+cosθj^
Time derivatives of the unit vectors:
e^˙r=θ˙e^θ,e^˙θ=−θ˙e^r
Position, velocity, acceleration
r=re^r
Velocity:
v=r˙e^r+rθ˙e^θ
- Radial component: vr=r˙
- Transverse component: vθ=rθ˙
Acceleration (differentiate v):
a=(r¨−rθ˙2)e^r+(rθ¨+2r˙θ˙)e^θ
- Radial component: ar=r¨−rθ˙2
- Transverse component: aθ=rθ¨+2r˙θ˙=r1dtd(r2θ˙)
Cartesian derivation check
With x=rcosθ, y=rsinθ:
x˙=r˙cosθ−rθ˙sinθ,y˙=r˙sinθ+rθ˙cosθ
x¨=(r¨−rθ˙2)cosθ−(rθ¨+2r˙θ˙)sinθ
y¨=(r¨−rθ˙2)sinθ+(rθ¨+2r˙θ˙)cosθ
confirming a=(r¨−rθ˙2)e^r+(rθ¨+2r˙θ˙)e^θ.
Special cases
Circular motion (r= const, r˙=0, r¨=0):
ar=−rθ˙2=−rv2,aθ=rθ¨
Radial motion (θ= const):
v=r˙e^r,a=r¨e^r
Question Archetypes
| Archetype | Recognition |
|---|
| polar-derivation | ”Derive velocity/acceleration components in polar coordinates” or “show ar=r¨−rθ˙2“ |
polar-derivation (1 question; 2020)
Recognition Cues
- The question asks to “derive” or “obtain” expressions for velocity or acceleration components.
- Polar or plane-polar coordinates (r,θ) are mentioned explicitly.
- May ask you to start from Cartesian and arrive at the polar form.
- Sometimes phrased as “find the radial and transverse components of acceleration.”
Solution Template
- Write the position vector r=re^r and define e^r, e^θ in Cartesian terms.
- Compute e^˙r and e^˙θ by differentiating with respect to t (chain rule through θ).
- Differentiate r once for velocity; collect e^r and e^θ terms.
- Differentiate velocity for acceleration; substitute e^˙r, e^˙θ; collect terms.
- Identify ar=r¨−rθ˙2 and aθ=rθ¨+2r˙θ˙; simplify aθ=r1dtd(r2θ˙) if useful.
Worked Example
2020 Paper 1, 2020-P1-Q3a (10 marks)
Derive expressions for the radial and transverse components of the velocity and acceleration of a particle moving in a plane, using polar coordinates (r,θ).
Step 1. Set up unit vectors.
Define:
e^r=cosθi^+sinθj^,e^θ=−sinθi^+cosθj^.
Note e^r⋅e^r=1, e^θ⋅e^θ=1, e^r⋅e^θ=0.
Step 2. Time derivatives of unit vectors.
e^˙r=dtd(cosθi^+sinθj^)=(−sinθi^+cosθj^)θ˙=θ˙e^θ
e^˙θ=dtd(−sinθi^+cosθj^)=(−cosθi^−sinθj^)θ˙=−θ˙e^r
Step 3. Velocity.
r=re^r
v=r˙=r˙e^r+re^˙r=r˙e^r+rθ˙e^θ
Radial component: vr=r˙; transverse component: vθ=rθ˙.
Step 4. Acceleration.
a=v˙=dtd(r˙e^r)+dtd(rθ˙e^θ)
=r¨e^r+r˙e^˙r+(r˙θ˙+rθ¨)e^θ+rθ˙e^˙θ
=r¨e^r+r˙θ˙e^θ+(r˙θ˙+rθ¨)e^θ+rθ˙(−θ˙e^r)
=(r¨−rθ˙2)e^r+(rθ¨+2r˙θ˙)e^θ
Step 5. Final result.
ar=r¨−rθ˙2,aθ=rθ¨+2r˙θ˙=r1dtd(r2θ˙)
Common Traps
- Forgetting the −rθ˙2 centripetal term in ar (it comes from rθ˙e^˙θ=−rθ˙2e^r).
- Writing e^˙r=θ˙e^r (wrong sign/direction); it must be θ˙e^θ.
- Omitting the cross-term r˙θ˙ in aθ, giving rθ¨ instead of rθ¨+2r˙θ˙.
- Confusing r˙ (rate of change of distance) with ∣v∣ (speed); they differ when θ˙=0.
Marks-Aware Writing
This is a 10-mark derivation. Examiners look for:
- Defined notation — state e^r, e^θ explicitly (2 marks).
- Unit-vector derivatives — both e^˙r and e^˙θ shown with working (3 marks).
- Velocity derivation — one clean differentiation step (2 marks).
- Acceleration derivation — product rule applied correctly, all four sub-terms collected (3 marks).
Write every line of algebra; do not skip the collection step. Underline or box the final components.
Practice Set
Only one historical question on this atom (shown above).