Question
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 T

2T
42T
82T
2T
82T
Solution
The planet is in a circular orbit of radius R with time period T. Its velocity is vc=GM/R. The time period is given by Kepler's Third Law: T=2πR3/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/r2. Using energy conservation, the velocity v at a distance r from the Sun is given by: 21mv2−rGMm=−RGMm v2=2GM(R1−r1) Since v=−dtdr, we have: dt=−2GM(R1−r1)dr=−2GM(r−R)Rrdr To find the time to fall to the Sun (r=0), we integrate from r=R to r=0: tfall=∫R0−2GMRR−rrdr=2GMR∫0RR−rrdr The integral ∫0RR−rrdr can be solved using the substitution r=Rsin2θ, which yields 2πR. tfall=2GMR⋅2πR=22GMπR3/2 Now, we relate this to the original time period T. From Kepler's Third Law, T2=GM4π2R3, so GMR3=4π2T2. tfall2=8GMπ2R3=8π2(GMR3)=8π2(4π2T2)=32T2 tfall=32T=42T To match the options, we can rationalize the denominator: tfall=42T⋅22=82T This matches option (C), assuming that the T in the options is a typo and should be T. The options (B) and (C) are dimensionally incorrect as written, but if interpreted as 42T and 82T, then 82T is the correct answer.