← 2026 Paper 1

UPSC 2026 Maths Optional Paper 1 Q5d — Step-by-Step Solution

10 marks · Section B

Constrained motion · Dynamics & Statics · asked 8× in 14 yrs · Read the full method →

Question

A particle falls from rest at the vertex of an inverted catenary. Prove that the particle will leave the curve when the path described is 3\sqrt{3} times the vertical distance through which the particle has fallen.

Technique

Three standard ingredients, combined: energy conservation (v2=2ghv^2=2gh, the curve being smooth), the intrinsic geometry of the catenary (s=ctan⁡ψs=c\tan\psi, y=csec⁡ψy=c\sec\psi, ρ=csec⁡2ψ\rho=c\sec^2\psi), and the normal equation of motion mgcos⁡ψ−N=mv2/ρmg\cos\psi - N = mv^2/\rho, with the leaving condition N=0N=0. Everything collapses to a single equation in ψ\psi.

Solution

Step 1 — Set up the curve and the sign conventions.

Take the catenary y=ccosh⁡(x/c)y=c\cosh(x/c) (parameter cc, directrix y=0y=0) and invert it — turn it upside down — so that its vertex AA is the highest point and the curve falls away on both sides. The particle rests on the convex (outer) side, which is the upper side of the inverted curve.

Measure, from the vertex AA:

Two forces act: the weight mgmg vertically downwards, and the normal reaction NN, which for a particle on the outside of a curve that is concave downwards points outwards, i.e. away from the centre of curvature (upwards-and-outwards). The curve is smooth, so there is no friction.

Figure to draw (small, labelled): a cap-shaped inverted catenary with vertex AA at the top; a particle PP part-way down the right branch; from PP draw the tangent and mark ψ\psi between the tangent and the horizontal; draw mgmg vertically down from PP, resolve it into mgsin⁡ψmg\sin\psi along the tangent (down-slope) and mgcos⁡ψmg\cos\psi along the inward normal (towards the centre of curvature CC below the curve); draw NN outward from PP along the same normal line, opposite to mgcos⁡ψmg\cos\psi; mark the arc AP=sAP=s and the vertical drop hh from the level of AA down to PP. The figure is what makes the sign of the normal equation obvious, and it earns its space.

Step 2 — Intrinsic relations for the catenary.

For y=ccosh⁡(x/c)y=c\cosh(x/c) measured from the vertex:

dydx=sinh⁡xc=tan⁡ψ,\frac{dy}{dx} = \sinh\frac{x}{c} = \tan\psi , s=∫0x1+sinh⁡2xc  dx=∫0xcosh⁡xc dx=csinh⁡xc  =  ctan⁡ψ,(1)s = \int_0^x\sqrt{1+\sinh^2\frac{x}{c}}\;dx = \int_0^x \cosh\frac{x}{c}\,dx = c\sinh\frac{x}{c} \;=\; c\tan\psi , \tag{1} y=ccosh⁡xc=c1+sinh⁡2xc=c1+tan⁡2ψ  =  csec⁡ψ.(2)y = c\cosh\frac{x}{c} = c\sqrt{1+\sinh^2\tfrac{x}{c}} = c\sqrt{1+\tan^2\psi} \;=\; c\sec\psi . \tag{2}

The radius of curvature is

ρ=(1+y′2)3/2∣y′′∣=cosh⁡3(x/c)1ccosh⁡(x/c)=ccosh⁡2xc  =  csec⁡2ψ  (=y2c).(3)\rho = \frac{\bigl(1+y'^2\bigr)^{3/2}}{|y''|} = \frac{\cosh^3(x/c)}{\tfrac1c\cosh(x/c)} = c\cosh^2\frac{x}{c} \;=\; c\sec^2\psi \;\left(=\frac{y^2}{c}\right). \tag{3}

For the inverted curve the vertex is at y=cy=c (the lowest point of the original catenary becomes the highest point), so the vertical distance fallen is

h=y−c=csec⁡ψ−c=c(sec⁡ψ−1).(4)h = y - c = c\sec\psi - c = c(\sec\psi - 1). \tag{4}

(All three relations (1)–(4) are unchanged by turning the curve upside down: arc length, curvature and the angle with the horizontal are geometric.)

Step 3 — Energy conservation gives the speed.

The surface is smooth, so the reaction does no work; the particle starts from rest at the vertex. After descending a vertical height hh,

12mv2=mgh⟹v2=2gh.(5)\tfrac12 m v^2 = mgh \qquad\Longrightarrow\qquad v^2 = 2gh . \tag{5}

Step 4 — The normal equation of motion and the leaving condition.

Resolve along the inward normal (towards the centre of curvature, which lies below the inverted curve). The component of the weight along it is mgcos⁡ψmg\cos\psi; the reaction NN acts outwards. The net inward force supplies the centripetal acceleration v2/ρv^2/\rho:

mgcos⁡ψ−N=mv2ρ.(6)mg\cos\psi - N = \frac{m v^2}{\rho}. \tag{6}

The particle leaves the curve when the contact is lost, i.e. when N=0N=0:

gcos⁡ψ=v2ρ⟹v2=gρcos⁡ψ.(7)g\cos\psi = \frac{v^2}{\rho}\qquad\Longrightarrow\qquad v^2 = g\rho\cos\psi . \tag{7}

Step 5 — Combine and solve for ψ\psi.

Substituting (5) and (3) into (7):

2gh=g (csec⁡2ψ)cos⁡ψ=g csec⁡ψ,2gh = g\,\bigl(c\sec^2\psi\bigr)\cos\psi = g\,c\sec\psi ,

so

2h=csec⁡ψ.2h = c\sec\psi .

Now use (4), h=c(sec⁡ψ−1)h=c(\sec\psi-1):

2c(sec⁡ψ−1)=csec⁡ψ⟹2sec⁡ψ−2=sec⁡ψ⟹sec⁡ψ=2.2c(\sec\psi - 1) = c\sec\psi \quad\Longrightarrow\quad 2\sec\psi - 2 = \sec\psi \quad\Longrightarrow\quad \sec\psi = 2 .

Hence

cos⁡ψ=12,ψ=60∘=π3,tan⁡ψ=3.\cos\psi = \tfrac12,\qquad \psi = 60^\circ = \frac{\pi}{3},\qquad \tan\psi = \sqrt3 .

Step 6 — Read off ss and hh at that instant.

From (1), s=ctan⁡ψ=3 cs = c\tan\psi = \sqrt3\,c.   From (4), h=c(sec⁡ψ−1)=c(2−1)=ch = c(\sec\psi - 1) = c(2-1) = c.

Therefore

sh=3 cc=3⟹s=3 h,\frac{s}{h} = \frac{\sqrt3\,c}{c} = \sqrt3 \qquad\Longrightarrow\qquad s = \sqrt3\,h ,

i.e. the path described is 3\sqrt3 times the vertical distance fallen, as required. ■\blacksquare

(Note the elegance worth pointing out in the answer: the leaving point is at the fixed intrinsic angle ψ=60∘\psi=60^\circ and at h=ch=c, s=3cs=\sqrt3 c — independent of gg and of the mass, and depending on the catenary only through its parameter cc. The stated ratio s/h=3s/h=\sqrt3 is therefore a genuinely scale-free statement, which is why the paper poses it that way.)

Answer

  N=0  ⟺  sec⁡ψ=2, i.e. ψ=60∘; there s=ctan⁡ψ=3 c,h=c(sec⁡ψ−1)=c,∴ s=3 h.  \boxed{\;N=0 \iff \sec\psi = 2,\ \text{i.e. }\psi=60^\circ;\ \text{there } s = c\tan\psi=\sqrt3\,c,\quad h = c(\sec\psi-1)=c,\quad \therefore\ s=\sqrt3\,h.\;}
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