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UPSC Maths 2025 Paper 1 Q5c — Solution

10 marks · Section B

Question

Prove that the time taken by the Earth to travel over half of its orbit, which is separated by the minor axis and is remote from the Sun, when the Sun is at the focus of the elliptic orbit, is two days more than half of the year. The eccentricity of the orbit is taken as 160\dfrac{1}{60}.

Technique

Use Kepler’s second law (constant areal velocity): the time over an arc equals the area swept by the radius vector from the focus divided by the constant areal velocity πabT\dfrac{\pi a b}{T}.

Solution

Place the ellipse x2a2+y2b2=1\dfrac{x^2}{a^2}+\dfrac{y^2}{b^2}=1 with centre at the origin and the Sun at the focus S=(ae,0)S=(ae,0). The minor axis is the line x=0x=0; its endpoints are L=(0,b)L=(0,b) and L=(0,b)L'=(0,-b). The minor axis cuts the orbit into two halves:

By Kepler’s second law the radius vector from SS sweeps area at the constant rate dAdt=total areaT=πabT,\frac{dA}{dt} = \frac{\text{total area}}{T} = \frac{\pi a b}{T}, where TT is the orbital period (one year).

Area swept over the remote half. As the Earth moves along the far arc from L=(0,b)L=(0,b) to L=(0,b)L'=(0,-b), the area swept out by SL,SLSL,\,SL' is the region bounded by the far arc and the two radii SL,SLSL,\,SL'. This equals Aremote=12πabarea of the half-ellipse x<0  +  (SLL)triangle with base LL,A_{\text{remote}} = \underbrace{\tfrac{1}{2}\pi a b}_{\text{area of the half-ellipse }x<0} \;+\; \underbrace{(\triangle S L L')}_{\text{triangle with base }LL'}, because the focus SS lies on the near side (x>0x>0), so the triangle SLLSLL' must be added to the half-ellipse area to obtain the focal sector.

The triangle SLLSLL' has base LL=2bLL' = 2b along the yy-axis and height aeae (the xx-distance of SS from the minor axis), so SLL=12(2b)(ae)=abe.\triangle SLL' = \tfrac{1}{2}(2b)(ae) = abe.

Hence Aremote=πab2+abe.A_{\text{remote}} = \frac{\pi a b}{2} + abe.

Time for the remote half. tremote=Aremoteπab/T=T(12+eπ)=T2+Teπ.t_{\text{remote}} = \frac{A_{\text{remote}}}{\pi a b / T} = T\left(\frac{1}{2} + \frac{e}{\pi}\right) = \frac{T}{2} + \frac{Te}{\pi}.

So the remote half takes longer than half the year by Δt=tremoteT2=Teπ.\Delta t = t_{\text{remote}} - \frac{T}{2} = \frac{T e}{\pi}.

Numerical value. With e=160e = \dfrac{1}{60} and T=365.25T = 365.25 days, Δt=365.25π160=365.2560π1.938 days2 days.\Delta t = \frac{365.25}{\pi}\cdot\frac{1}{60} = \frac{365.25}{60\pi} \approx 1.938 \text{ days} \approx 2 \text{ days.}

(With T=365T=365 days, Δt1.936\Delta t\approx 1.936 days; in either case “two days more than half a year,” as required.)

Answer

  tremote=T2+Teπ,Δt=Teπ=365.2560π1.942 days.  \boxed{\;t_{\text{remote}} = \frac{T}{2} + \frac{Te}{\pi},\qquad \Delta t = \frac{Te}{\pi} = \frac{365.25}{60\pi}\approx 1.94 \approx 2\ \text{days}.\;}

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