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UPSC 2020 Maths Optional Paper 2 Q5e — Step-by-Step Solution

10 marks · Section B

Moment of inertia · Mechanics & Fluid Dynamics · asked 7× in 13 yrs · Read the full method →

Question

Prove that the moment of inertia of a triangular lamina ABCABC about any axis through AA in its plane is M6(β2+βγ+γ2)\frac{M}{6}(\beta^2+\beta\gamma+\gamma^2), where MM is the mass of the lamina and β,γ\beta,\gamma are respectively the lengths of perpendiculars from BB and CC on the axis.

Technique

Affine (area) coordinates u,vu,v; perpendicular distance is linear, δ=uβ+vγ\delta=u\beta+v\gamma; integrate δ2\delta^2 over the standard triangle using the moments 112,124\tfrac1{12},\tfrac1{24}.

Solution

Let the axis through AA be the reference line; for any point PP of the lamina let δ(P)\delta(P) denote its perpendicular (signed) distance from the axis. The moment of inertia about the axis is

I=δ2dm=σδ2dA,I=\iint \delta^2\,dm=\sigma\iint\delta^2\,dA,

where σ=M/Area\sigma=M/\text{Area} is the surface density.

Step 1 — Linear coordinate across the triangle

Set up affine (area) coordinates. Any point PP in triangle ABCABC can be written

AP=uAB+vAC,u0, v0, u+v1.\vec{AP}=u\,\vec{AB}+v\,\vec{AC},\qquad u\ge0,\ v\ge0,\ u+v\le1.

Because perpendicular distance from a line through AA is a linear function of position vanishing at AA, the distance of PP from the axis is

δ(P)=uβ+vγ,\delta(P)=u\,\beta+v\,\gamma,

since the perpendicular distance of AA is 00, of BB (where u=1,v=0u=1,v=0) is β\beta, and of CC (where u=0,v=1u=0,v=1) is γ\gamma. (Take β,γ\beta,\gamma with appropriate signs if B,CB,C are on opposite sides; the formula below uses their squares and product so the stated result holds for perpendicular lengths in the standard configuration.)

Step 2 — Area element

The map (u,v)P(u,v)\mapsto P has constant Jacobian: dA=AB×ACdudv=2ΔdudvdA=\big|\vec{AB}\times\vec{AC}\big|\,du\,dv=2\Delta\,du\,dv, where Δ\Delta is the area of the triangle. The mass element is

dm=σdA=MΔΔdm=\sigma\,dA=\frac{M}{\Delta}\,\Delta\,\cdots

more precisely dm=σ2Δdudvdm=\sigma\,2\Delta\,du\,dv and σ=M/Δ\sigma=M/\Delta, so dm=2Mdudvdm=2M\,du\,dv. (Check of total mass: u+v12Mdudv=2M12=M\displaystyle\iint_{u+v\le1}2M\,du\,dv=2M\cdot\tfrac12=M. ✓)

Step 3 — Integrate

I=u,v0u+v1(uβ+vγ)2(2M)dudv=2M(β2u2+2βγuv+γ2v2)dudv.I=\iint_{\substack{u,v\ge0\\u+v\le1}}(u\beta+v\gamma)^2\,(2M)\,du\,dv =2M\iint(\beta^2u^2+2\beta\gamma\,uv+\gamma^2v^2)\,du\,dv.

Over the standard triangle {u,v0, u+v1}\{u,v\ge0,\ u+v\le1\}:

u2dudv=112,v2dudv=112,uvdudv=124.\iint u^2\,du\,dv=\frac{1}{12},\qquad \iint v^2\,du\,dv=\frac{1}{12},\qquad \iint uv\,du\,dv=\frac{1}{24}.

Hence

I=2M(β2112+2βγ124+γ2112)=2M112(β2+βγ+γ2).I=2M\left(\beta^2\cdot\frac1{12}+2\beta\gamma\cdot\frac1{24}+\gamma^2\cdot\frac1{12}\right) =2M\cdot\frac{1}{12}\big(\beta^2+\beta\gamma+\gamma^2\big).

Answer

  I=M6(β2+βγ+γ2).  \boxed{\;I=\frac{M}{6}\big(\beta^2+\beta\gamma+\gamma^2\big).\;}
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