← 2024 Paper 1

UPSC 2024 Maths Optional Paper 1 Q8c — Step-by-Step Solution

20 marks · Section B

Central force motion and Kepler's laws · Dynamics & Statics · asked 6× in 13 yrs · Read the full method →

Question

A particle moves with central acceleration μ ⁣(3r3+d2r5)\mu\!\left(\dfrac{3}{r^3}+\dfrac{d^2}{r^5}\right), projected from distance dd at 45°45° to the radius with velocity equal to that in a circular orbit at the same distance. Prove that the time to reach the centre of force is d22μ ⁣(2π2)\dfrac{d^2}{\sqrt{2\mu}}\!\left(2-\dfrac{\pi}{2}\right).

Technique

Energy and angular momentum conservation; effective-potential reduction; recognise a perfect-square structure in r˙2\dot r^2; standard r2/(r2+d2)r^2/(r^2+d^2) integral.

Solution

Step 1 — Circular orbit speed.

Central acceleration at radius dd: a(d)=μ(3/d3+d2/d5)=4μ/d3a(d)=\mu(3/d^3+d^2/d^5)=4\mu/d^3.

Circular orbit: vc2/d=4μ/d3    vc2=4μ/d2v_c^2/d=4\mu/d^3\;\Rightarrow\;v_c^2=4\mu/d^2.

Step 2 — Initial conditions and conserved quantities.

At r=dr=d, projected at 45°45° inward with speed vcv_c:

r˙0=vc/2=2μ/d,vθ=vc/2.\dot r_0=-v_c/\sqrt{2}=-\sqrt{2\mu}/d,\qquad v_\theta=v_c/\sqrt{2}.

Angular momentum: L=dvc/2=2μL=d\cdot v_c/\sqrt{2}=\sqrt{2\mu}.

Potential V(r)=3μ2r2μd24r4V(r)=-\tfrac{3\mu}{2r^2}-\tfrac{\mu d^2}{4r^4}. Energy:

E=12vc2+V(d)=2μd23μ2d2μ4d2=μ4d2.E=\tfrac{1}{2}v_c^2+V(d)=\tfrac{2\mu}{d^2}-\tfrac{3\mu}{2d^2}-\tfrac{\mu}{4d^2}=\frac{\mu}{4d^2}.

Step 3 — Radial equation.

r˙2=2(EVeff),Veff=V(r)+L22r2=μ2r2μd24r4.\dot r^2=2(E-V_{\text{eff}}),\quad V_{\text{eff}}=V(r)+\frac{L^2}{2r^2}=-\frac{\mu}{2r^2}-\frac{\mu d^2}{4r^4}. r˙2=μ2d2+μr2+μd22r4.\dot r^2=\frac{\mu}{2d^2}+\frac{\mu}{r^2}+\frac{\mu d^2}{2r^4}.

Step 4 — Perfect-square recognition.

Multiply by 2r4/μ2r^4/\mu:

2r4r˙2μ=r4d2+2r2+d2=(r2+d2d)2.\frac{2r^4\dot r^2}{\mu}=\frac{r^4}{d^2}+2r^2+d^2=\left(\frac{r^2+d^2}{d}\right)^2.

Therefore r˙=μd2r2+d2r2\dot r=-\dfrac{\sqrt\mu}{d\sqrt{2}}\cdot\dfrac{r^2+d^2}{r^2} (negative since rr decreases).

Step 5 — Time integral.

T=d0drr˙=d2μ0dr2r2+d2dr.T=\int_d^0\frac{dr}{\dot r}=\frac{d\sqrt{2}}{\sqrt\mu}\int_0^d\frac{r^2}{r^2+d^2}\,dr. 0dr2r2+d2dr=0d ⁣ ⁣(1d2r2+d2)dr=[rdarctan(r/d)]0d=ddπ4=d(4π)4.\int_0^d\frac{r^2}{r^2+d^2}\,dr=\int_0^d\!\!\left(1-\frac{d^2}{r^2+d^2}\right)dr=\bigl[r-d\arctan(r/d)\bigr]_0^d=d-d\cdot\frac{\pi}{4}=\frac{d(4-\pi)}{4}. T=d2μd(4π)4=d22μ4π2=d22μ ⁣(2π2).T=\frac{d\sqrt{2}}{\sqrt\mu}\cdot\frac{d(4-\pi)}{4}=\frac{d^2}{\sqrt{2\mu}}\cdot\frac{4-\pi}{2}=\frac{d^2}{\sqrt{2\mu}}\!\left(2-\frac{\pi}{2}\right).

Answer

  T=d22μ ⁣(2π2).  \boxed{\;T=\frac{d^2}{\sqrt{2\mu}}\!\left(2-\frac{\pi}{2}\right).\;}
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