← 2026 Paper 2

UPSC 2026 Maths Optional Paper 2 Q5e — Step-by-Step Solution

10 marks · Section B

Motion of rigid bodies in two dimensions · Mechanics & Fluid Dynamics · asked 5× in 14 yrs · Read the full method →

Question

A uniform heavy solid hemisphere of radius 'aa' is held at rest with its base vertical and its curved surface in contact with a horizontal plane. If the hemisphere is released when the plane is rough enough to prevent slipping, show that the angle θ\theta that the base makes with the horizontal at time tt, is such that

(dθdt)2=15 gcos⁡θa (28−15cos⁡θ).\left(\frac{d\theta}{dt}\right)^2 = \frac{15\,g\cos\theta}{a\,(28 - 15\cos\theta)}.

Technique

“Rough enough to prevent slipping” is a constraint, not a force to be found: the contact point has zero velocity, so friction and normal reaction do no work and energy is conserved. That makes this a one-line-in-principle problem — write T+V=T+V= const with θ\theta the single degree of freedom. The two numbers that must be right are OG=3a8OG=\tfrac{3a}{8} and the moment of inertia; the constant 2828 in the printed denominator is 20×7520\times\tfrac{7}{5} and is a direct consequence of them, so a wrong 2828 means a wrong geometry, not a wrong algebra step. The one geometric fact that unlocks everything: the centre OO of the flat face stays at height aa throughout, because the curved surface is a sphere of radius aa centred at OO.

Solution

Step 1 — Set up, and say exactly what θ\theta is.

Let MM be the mass, aa the radius, OO the centre of the plane (flat) face, and GG the centre of mass, which lies on the axis of symmetry at

OG=c=3a8OG=c=\frac{3a}{8}

(standard result for a uniform solid hemisphere), on the side of the curved surface.

θ\theta is the angle the base (the flat face) makes with the horizontal plane. Since OGOG is perpendicular to the base, OGOG makes the same angle θ\theta with the upward vertical measured from OO downwards — concretely, taking the vertical plane of motion as the xyxy-plane with yy upward, the unit vector from OO towards GG is

u^=(sin⁡θ, −cos⁡θ).\hat u=(\sin\theta,\,-\cos\theta).

Check the two ends: θ=π2\theta=\tfrac{\pi}{2} (base vertical) gives u^=(1,0)\hat u=(1,0), so GG is level with OO — the released configuration; θ=0\theta=0 (base horizontal, uppermost) gives u^=(0,−1)\hat u=(0,-1), so GG is directly below OO — the equilibrium configuration.

Initial conditions. “Held at rest with its base vertical” and then released:

θ(0)=π2,θ˙(0)=0.\theta(0)=\frac{\pi}{2},\qquad \dot\theta(0)=0 .

(The printed formula is consistent with exactly this: it gives θ˙2=0\dot\theta^{2}=0 at θ=π/2\theta=\pi/2.)

The motion is planar. The body is a solid of revolution about OGOG; at t=0t=0 the vertical plane containing OGOG is a plane of symmetry for the body, for gravity and for the horizontal plane, and the initial velocity is zero. The mirror image of the motion in that plane is therefore also a solution with the same initial data, so by uniqueness the motion coincides with its mirror image: it stays in that vertical plane. (This is worth one sentence — the rolling constraint is non-holonomic in general, and planarity is what makes the single coordinate θ\theta sufficient.)

Step 2 — The key geometric fact: OO moves horizontally at height aa.

The curved surface of the hemisphere is part of the sphere of radius aa centred at OO. Contact with the horizontal plane therefore requires

height of O=afor all t,\text{height of }O=a\quad\text{for all }t,

and the contact point CC is the point of that sphere vertically below OO:

OC⃗=(0, −a).\vec{OC}=(0,\,-a).

(Consistency check: CC lies on the hemisphere iff OC⃗⋅u^≥0\vec{OC}\cdot\hat u\ge0, i.e. acos⁡θ≥0a\cos\theta\ge0, true for 0≤θ≤π/20\le\theta\le\pi/2. At θ=π/2\theta=\pi/2 we get OC⃗⋅u^=0\vec{OC}\cdot\hat u=0: the contact is exactly on the rim of the base — the limiting configuration described in the question.)

Consequently the height of GG is

yG=a+OG⃗⋅j^=a−ccos⁡θ=a−3a8cos⁡θ.(1)y_G=a+\vec{OG}\cdot\hat j=a-c\cos\theta=a-\frac{3a}{8}\cos\theta . \tag{1}

At θ=π/2\theta=\pi/2, yG=ay_G=a; at θ=0\theta=0, yG=a−3a8=5a8y_G=a-\tfrac{3a}{8}=\tfrac{5a}{8}. The drop of the centre of mass from the initial position is therefore

h(θ)=a−yG=3a8cos⁡θ.(2)h(\theta)=a-y_G=\frac{3a}{8}\cos\theta . \tag{2}

This is the step most candidates get wrong — the temptation is to write the drop as c(1−cos⁡θ)c(1-\cos\theta) or csin⁡θc\sin\theta by analogy with a pendulum. It is neither: OO does not move vertically, so the entire vertical motion of GG comes from the rotation of OG⃗\vec{OG}, and at θ=π/2\theta=\pi/2 that vector is horizontal, giving the maximum height.

Step 3 — Moments of inertia.

Let the axis of rotation be the horizontal line through OO perpendicular to the plane of motion. Because the motion is planar and OGOG lies in that plane, this axis lies in the plane of the flat face, i.e. it is a diameter of the base.

For a uniform solid hemisphere of mass MM, radius aa, about a diameter of its base through OO: a full sphere of mass 2M2M and radius aa has I=25(2M)a2=45Ma2I=\tfrac25(2M)a^{2}=\tfrac45Ma^{2} about a diameter, and that diameter can be taken in the cutting plane, so by symmetry each hemisphere contributes half:

IO=25Ma2.I_O=\frac{2}{5}Ma^{2}.

By the parallel-axis theorem (the axis through GG parallel to this one),

IG=IO−Mc2=25Ma2−M9a264=Ma2(25−964)=Ma2⋅128−45320=83320Ma2.(3)I_G=I_O-Mc^{2}=\frac{2}{5}Ma^{2}-M\frac{9a^{2}}{64}=Ma^{2}\left(\frac{2}{5}-\frac{9}{64}\right)=Ma^{2}\cdot\frac{128-45}{320}=\frac{83}{320}Ma^{2}. \tag{3}

Step 4 — Kinetic energy.

Let ω\omega be the angular speed of the body. Since the orientation of u^\hat u is θ\theta-determined, du^dt=θ˙(cos⁡θ,sin⁡θ)\dfrac{d\hat u}{dt}=\dot\theta(\cos\theta,\sin\theta), while for a rigid body du^dt=ω⃗×u^\dfrac{d\hat u}{dt}=\vec\omega\times\hat u; with ω⃗=ωk^\vec\omega=\omega\hat k this is ω(cos⁡θ,sin⁡θ)\omega(\cos\theta,\sin\theta). Hence

ω=θ˙.\omega=\dot\theta .

Velocity of GG. Rolling without slipping means v⃗C=0\vec v_C=0, so CC is the instantaneous centre of rotation and

v⃗G=ω⃗×CG⃗,∣v⃗G∣=θ˙ ∣CG∣.\vec v_G=\vec\omega\times\vec{CG},\qquad |\vec v_G|=\dot\theta\,|CG| .

From CG⃗=CO⃗+OG⃗=(0,a)+c(sin⁡θ,−cos⁡θ)=(csin⁡θ, a−ccos⁡θ)\vec{CG}=\vec{CO}+\vec{OG}=(0,a)+c(\sin\theta,-\cos\theta)=\bigl(c\sin\theta,\ a-c\cos\theta\bigr),

∣CG∣2=c2sin⁡2θ+a2−2accos⁡θ+c2cos⁡2θ=a2+c2−2accos⁡θ.(4)|CG|^{2}=c^{2}\sin^{2}\theta+a^{2}-2ac\cos\theta+c^{2}\cos^{2}\theta=a^{2}+c^{2}-2ac\cos\theta . \tag{4}

(Equivalently, without invoking the instantaneous centre: v⃗O=−aθ˙ i^\vec v_O=-a\dot\theta\,\hat i from the rolling condition, and v⃗G=v⃗O+ω⃗×OG⃗=θ˙(ccos⁡θ−a, csin⁡θ)\vec v_G=\vec v_O+\vec\omega\times\vec{OG}=\dot\theta\bigl(c\cos\theta-a,\ c\sin\theta\bigr), whose square is again (4).)

Therefore, by König’s theorem (translation of GG plus rotation about GG),

T=12M∣v⃗G∣2+12IGθ˙2=12θ˙2[M(a2+c2−2accos⁡θ)+IG].(5)T=\tfrac12M|\vec v_G|^{2}+\tfrac12 I_G\dot\theta^{2} =\tfrac12\dot\theta^{2}\Bigl[M\bigl(a^{2}+c^{2}-2ac\cos\theta\bigr)+I_G\Bigr]. \tag{5}

Insert c=3a8c=\tfrac{3a}{8} and (3), and divide the bracket by Ma2Ma^{2}:

a2+c2−2accos⁡θ+IG/Ma2=1+964−2⋅38cos⁡θ+83320=365320+83320−34cos⁡θ=448320−34cos⁡θ,\frac{a^{2}+c^{2}-2ac\cos\theta+I_G/M}{a^{2}}=1+\frac{9}{64}-2\cdot\frac38\cos\theta+\frac{83}{320} =\frac{365}{320}+\frac{83}{320}-\frac34\cos\theta=\frac{448}{320}-\frac34\cos\theta,  T=12Ma2θ˙2(75−34cos⁡θ) (6)\boxed{\ T=\tfrac12 Ma^{2}\dot\theta^{2}\left(\frac{7}{5}-\frac{3}{4}\cos\theta\right)\ } \tag{6}

since 448/320=7/5448/320=7/5.

(Sanity check on (6) at θ=0\theta=0: there ∣CG∣=a−c|CG|=a-c and T=12θ˙2[M(a−c)2+IG]=12θ˙2Ma2[2564+83320]=12θ˙2Ma2⋅125+83320=12θ˙2Ma2⋅1320T=\tfrac12\dot\theta^{2}\bigl[M(a-c)^{2}+I_G\bigr]=\tfrac12\dot\theta^{2}Ma^{2}\bigl[\tfrac{25}{64}+\tfrac{83}{320}\bigr]=\tfrac12\dot\theta^{2}Ma^{2}\cdot\tfrac{125+83}{320}=\tfrac12\dot\theta^{2}Ma^{2}\cdot\tfrac{13}{20}, and (6) gives 75−34=28−1520=1320\tfrac75-\tfrac34=\tfrac{28-15}{20}=\tfrac{13}{20} ✓.)

Step 5 — Energy conservation.

The forces acting are gravity (conservative) and the reaction of the plane at CC — normal reaction and friction. Because the contact is rolling, the material point of the body at CC has zero velocity, so the reaction does no work. Hence the total mechanical energy is conserved:

T+V=const,V=Mg yG=Mg(a−ccos⁡θ).T+V=\text{const},\qquad V=Mg\,y_G=Mg\bigl(a-c\cos\theta\bigr).

Evaluating the constant at t=0t=0 (θ=π/2\theta=\pi/2, θ˙=0\dot\theta=0, V=MgaV=Mga):

12Ma2θ˙2(75−34cos⁡θ)+Mg(a−ccos⁡θ)=Mga,\tfrac12Ma^{2}\dot\theta^{2}\left(\frac75-\frac34\cos\theta\right)+Mg\bigl(a-c\cos\theta\bigr)=Mga, 12Ma2θ˙2(75−34cos⁡θ)=Mg ccos⁡θ=Mg 3a8cos⁡θ,\tfrac12Ma^{2}\dot\theta^{2}\left(\frac75-\frac34\cos\theta\right)=Mg\,c\cos\theta=Mg\,\frac{3a}{8}\cos\theta,

which is just T=Mg h(θ)T=Mg\,h(\theta) with the drop (2), as it must be.

Step 6 — Solve for θ˙2\dot\theta^{2}.

Cancel MM and one factor aa:

aθ˙2(75−34cos⁡θ)=3g4cos⁡θ.a\dot\theta^{2}\left(\frac75-\frac34\cos\theta\right)=\frac{3g}{4}\cos\theta .

Multiply throughout by 2020:

aθ˙2(28−15cos⁡θ)=15 gcos⁡θ,a\dot\theta^{2}\bigl(28-15\cos\theta\bigr)=15\,g\cos\theta, ∴(dθdt)2=15 gcos⁡θa (28−15cos⁡θ).■\therefore\quad \left(\frac{d\theta}{dt}\right)^{2}=\frac{15\,g\cos\theta}{a\,(28-15\cos\theta)} .\qquad\blacksquare

Step 7 — Reading the result (cheap marks, one line each).

θ¨=−38 sin⁡θ(θ˙2+ga)75−34cos⁡θ,\ddot\theta=-\frac{3}{8}\,\frac{\sin\theta\left(\dot\theta^{2}+\dfrac{g}{a}\right)}{\dfrac75-\dfrac34\cos\theta},

so for small-amplitude oscillations about θ=0\theta=0 (not the large release of this question, where θ˙2\dot\theta^{2} is not small at θ=0\theta=0) the linearisation is θ¨≈−15g26aθ\ddot\theta\approx-\dfrac{15g}{26a}\theta, giving the classical period 2π26a15g2\pi\sqrt{\dfrac{26a}{15g}} for a rocking hemisphere. Worth one line if time allows; do not confuse it with the present motion.

Answer

  (dθdt)2=15 gcos⁡θa (28−15cos⁡θ)  \boxed{\;\left(\frac{d\theta}{dt}\right)^{2}=\frac{15\,g\cos\theta}{a\,(28-15\cos\theta)}\;}

obtained from T+V=T+V= const with OG=3a8OG=\dfrac{3a}{8}, IG=83320Ma2I_G=\dfrac{83}{320}Ma^{2}, drop of GG =3a8cos⁡θ=\dfrac{3a}{8}\cos\theta, and 2T=Ma2θ˙2(75−34cos⁡θ)2T=Ma^{2}\dot\theta^{2}\Bigl(\dfrac75-\dfrac34\cos\theta\Bigr).

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