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Question: A planet was suddenly stopped in its orbit supposed to be circular. The time it takes to fall on to ...

A planet was suddenly stopped in its orbit supposed to be circular. The time it takes to fall on to the sun is, if time period of planet's revolution is TT

A

T2\frac{T}{2}

B

2T4\frac{\sqrt{2T}}{4}

C

2T8\frac{\sqrt{2T}}{8}

D

2T\sqrt{2T}

Answer

2T8\frac{\sqrt{2}T}{8}

Explanation

Solution

The planet is in a circular orbit of radius RR with time period TT. Its velocity is vc=GM/Rv_c = \sqrt{GM/R}. The time period is given by Kepler's Third Law: T=2πR3/GMT = 2\pi \sqrt{R^3/GM}.

When the planet's velocity is suddenly reduced to zero, it begins to fall towards the Sun radially. The motion is governed by the gravitational force F(r)=GMm/r2F(r) = GMm/r^2. Using energy conservation, the velocity vv at a distance rr from the Sun is given by: 12mv2GMmr=GMmR\frac{1}{2}mv^2 - \frac{GMm}{r} = -\frac{GMm}{R} v2=2GM(1R1r)v^2 = 2GM\left(\frac{1}{R} - \frac{1}{r}\right) Since v=drdtv = -\frac{dr}{dt}, we have: dt=dr2GM(1R1r)=Rr2GM(rR)drdt = -\frac{dr}{\sqrt{2GM\left(\frac{1}{R} - \frac{1}{r}\right)}} = -\sqrt{\frac{Rr}{2GM(r-R)}} dr To find the time to fall to the Sun (r=0r=0), we integrate from r=Rr=R to r=0r=0: tfall=R0R2GMrRrdr=R2GM0RrRrdrt_{fall} = \int_{R}^{0} -\sqrt{\frac{R}{2GM}} \frac{\sqrt{r}}{\sqrt{R-r}} dr = \sqrt{\frac{R}{2GM}} \int_{0}^{R} \frac{\sqrt{r}}{\sqrt{R-r}} dr The integral 0RrRrdr\int_{0}^{R} \frac{\sqrt{r}}{\sqrt{R-r}} dr can be solved using the substitution r=Rsin2θr = R\sin^2\theta, which yields πR2\frac{\pi R}{2}. tfall=R2GMπR2=πR3/222GMt_{fall} = \sqrt{\frac{R}{2GM}} \cdot \frac{\pi R}{2} = \frac{\pi R^{3/2}}{2\sqrt{2GM}} Now, we relate this to the original time period TT. From Kepler's Third Law, T2=4π2R3GMT^2 = \frac{4\pi^2 R^3}{GM}, so R3GM=T24π2\frac{R^3}{GM} = \frac{T^2}{4\pi^2}. tfall2=π2R38GM=π28(R3GM)=π28(T24π2)=T232t_{fall}^2 = \frac{\pi^2 R^3}{8GM} = \frac{\pi^2}{8} \left(\frac{R^3}{GM}\right) = \frac{\pi^2}{8} \left(\frac{T^2}{4\pi^2}\right) = \frac{T^2}{32} tfall=T32=T42t_{fall} = \frac{T}{\sqrt{32}} = \frac{T}{4\sqrt{2}} To match the options, we can rationalize the denominator: tfall=T4222=2T8t_{fall} = \frac{T}{4\sqrt{2}} \cdot \frac{\sqrt{2}}{\sqrt{2}} = \frac{\sqrt{2}T}{8} This matches option (C), assuming that the T\sqrt{T} in the options is a typo and should be TT. The options (B) and (C) are dimensionally incorrect as written, but if interpreted as 2T4\frac{\sqrt{2}T}{4} and 2T8\frac{\sqrt{2}T}{8}, then 2T8\frac{\sqrt{2}T}{8} is the correct answer.