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Question: The time period of a satellite very close to the earth is \( T \) . The time period of a geo-synchro...

The time period of a satellite very close to the earth is TT . The time period of a geo-synchronous satellite will be
(A) 22(T)2\sqrt 2 \left( T \right)
(B) 66(T)6\sqrt 6 \left( T \right)
(C) 77(T)7\sqrt 7 \left( T \right)
(D) 177(T)\dfrac{1}{{7\sqrt 7 }}\left( T \right)

Explanation

Solution

Hint : A geosynchronous orbit is an orbit which has an orbital period exactly to that of the earth. A geosynchronous orbit has a height of about 36000km above the earth's surface (usually the equator). We need to assume that the radius of a satellite close to the earth has the same orbital radius as the radius of the earth. The radius of the earth is about 6400 km

Formula used: In this solution we will be using the following formula;
T12T22=R13R23\dfrac{{T_1^2}}{{T_2^2}} = \dfrac{{R_1^3}}{{R_2^3}} where T1{T_1} is the period of a period of one satellite and T2{T_2} is period of another.
The R1{R_1} and R2{R_2} are their corresponding orbital radius.

Complete step by step answer
In general, a geosynchronous satellite is a satellite whose period of revolution around the earth is exactly equal to the period of rotation of the earth. The orbit of rotation is called a geosynchronous orbit. The height above the earth for a geosynchronous orbit is given as about 36000 km. Now, since the radius of the earth is about 6400 km, the height of the satellite hence is about six times the radius of the earth as in
360006400=5.6256\dfrac{{36000}}{{6400}} = 5.625 \approx 6
Hence, by Kepler’s third law of planetary motion, we have that
T12T22=R13R23\dfrac{{T_1^2}}{{T_2^2}} = \dfrac{{R_1^3}}{{R_2^3}}
T12T22=(R1R2)3\Rightarrow \dfrac{{T_1^2}}{{T_2^2}} = {\left( {\dfrac{{{R_1}}}{{{R_2}}}} \right)^3}
Hence, by letting 2 be the satellite close to the earth’s orbit and 1 the geosynchronous satellite, we have that
T12=(6RERE)3T22T_1^2 = {\left( {\dfrac{{6{R_E}}}{{{R_E}}}} \right)^3}T_2^2 ( by making the radius close to earth equal to the radius of the earth)
Hence, T12=T2263T_1^2 = T_2^2{6^3}
By square-rooting both sides, we have
T1=T2263=66T2{T_1} = \sqrt {T_2^2{6^3}} = 6\sqrt 6 {T_2}
Since, from question, the period T2=T{T_2} = T
Then, period of geosynchronous orbit is
T1=66T{T_1} = 6\sqrt 6 T
Hence, the correct option is B.

Note
For clarity, the height of a geosynchronous orbit can be gotten from the general formula of the height of a satellite above the earth surface, which is given by
h=(GME4πT2)13REh = {\left( {\dfrac{{G{M_E}}}{{4\pi }}{T^2}} \right)^{\dfrac{1}{3}}} - {R_E}
Hence, in the case of a geosynchronous satellite TT will be equal to the period of the earth rotation which is about 24 hours.