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Question: A satellite is orbiting around the earth. In a particular orbit its time period is \( T \) and orbit...

A satellite is orbiting around the earth. In a particular orbit its time period is TT and orbital speed is VV . In another orbit the orbital speed is 2V2V , then time period will be
(A) 8T8T
(B) 2T2T
(C) T/2T/2
(D) T/8T/8

Explanation

Solution

The orbital speed and the time period of a satellite in a particular orbit are given as, TV3T \propto {V^{ - 3}} . So for the 2 cases we take the ratio of the time period and hence get the time period in the second case.

Formula Used In this solution we will be using the following formula,
TV3T \propto {V^{ - 3}}
where TT is the time period and VV is the orbital velocity.

Complete Step by Step Solution
In the problem we are given the time period and the orbital speed of a satellite in an orbit around the earth. The relation is given by,
TV3T \propto {V^{ - 3}}
So in the first case let us consider the time period as TT and the orbital speed as VV
Hence the equation remains as,
TV3T \propto {V^{ - 3}}
In the second case let us consider the time period as TT' and the orbital speed as VV'
So the relation in the second case will be,
TV3T' \propto {V'^{ - 3}}
Now according to the question we can write,
V=2VV' = 2V
So substituting this value we get,
T(2V)3T' \propto {\left( {2V} \right)^{ - 3}}
Now we can take the ratio of the time period in the second case to the first case as,
TT=(2V)3V3\dfrac{{T'}}{T} = \dfrac{{{{\left( {2V} \right)}^{ - 3}}}}{{{V^{ - 3}}}}
Therefore, the VV gets cancelled in this equation. So we get,
TT=(2)31\dfrac{{T'}}{T} = \dfrac{{{{\left( 2 \right)}^{ - 3}}}}{1}
Therefore, the time period in the second case will be,
T=123TT' = \dfrac{1}{{{2^3}}}T
Hence the time period is, T=T8T' = \dfrac{T}{8}

So the correct option is D.

Note:
The time period of a satellite in an orbit is given by,
T=2πr3GMT = 2\pi \sqrt {\dfrac{{{r^3}}}{{GM}}}
and the orbital speed is given by,
V=GMrV = \sqrt {\dfrac{{GM}}{r}}
Hence we can write this as,
V=(GMr)1/2V = {\left( {\dfrac{{GM}}{r}} \right)^{1/2}}
Therefore, in the formula for the time period, we can multiply GMGM in the numerator and the denominator as,
T=2πr3GM×(GM)2(GM)2T = 2\pi \sqrt {\dfrac{{{r^3}}}{{GM}} \times \dfrac{{{{\left( {GM} \right)}^2}}}{{{{\left( {GM} \right)}^2}}}}
Therefore, we can simplify this as,
T=2πGMr3(GM)3T = 2\pi GM\sqrt {\dfrac{{{r^3}}}{{{{\left( {GM} \right)}^3}}}}
We can write the terms in the root as,
T=2πGM[(GMr)1/2]3T = 2\pi GM{\left[ {{{\left( {\dfrac{{GM}}{r}} \right)}^{1/2}}} \right]^{ - 3}}
Therefore we can write this in terms of velocity as,
T=2πGMV3T = 2\pi GM{V^{ - 3}}
Since 2πGM2\pi GM are constant, hence
TV3T \propto {V^{ - 3}} .