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Question: A geostationary satellite is orbiting the earth at height of \(5R\) above the surface of the earth. ...

A geostationary satellite is orbiting the earth at height of 5R5R above the surface of the earth. RR being the radius of the earth. The time period of another satellite in hours at a height 2R2R from the surface of the earth is
(A) 626\sqrt 2
(B) 6/26/\sqrt 2
(C) 55
(D) 1010

Explanation

Solution

Hint Hint: A geostationary satellite is the one which has the same angular velocity, hence the same time period as that of the earth. The time period of the earth is equal to 2424 hours, so the time period of the given geostationary satellite is also equal to 2424 hours. For determining the time period of the second satellite, we need to use Kepler's third law which states that the square of the time period is proportional to the cube of the radius of orbit.

Complete step-by-step solution:
We know that a geostationary satellite orbits about the earth with the same angular velocity as that of the earth. So the geostationary satellite must have the same time period as that of the earth. We know that the time period of the earth is equal to 2424 hours, so the geostationary satellite has the time period of 2424 hours, that is,
T1=24hr{T_1} = 24hr
Now, the height of the geostationary satellite above the earth’s surface is equal to 5R5R. So the radius of its orbit is
R1=5R+R{R_1} = 5R + R
R1=6R\Rightarrow {R_1} = 6R
Also, the height of the second satellite is given as 2R2R. So its orbital radius is given by
R2=2R+R{R_2} = 2R + R
R2=3R\Rightarrow {R_2} = 3R
Now, from the Kepler’s third law we know that the square of the time period is proportional to the cube of the orbital radius, that is,
T2R3{T^2} \propto {R^3}
(T2T1)2=(R2R1)3\Rightarrow {\left( {\dfrac{{{T_2}}}{{{T_1}}}} \right)^2} = {\left( {\dfrac{{{R_2}}}{{{R_1}}}} \right)^3}
Putting R1=6R{R_1} = 6R and R2=3R{R_2} = 3R, we get
(T2T1)2=(3R6R)3{\left( {\dfrac{{{T_2}}}{{{T_1}}}} \right)^2} = {\left( {\dfrac{{3R}}{{6R}}} \right)^3}
(T2T1)2=(12)3\Rightarrow {\left( {\dfrac{{{T_2}}}{{{T_1}}}} \right)^2} = {\left( {\dfrac{1}{2}} \right)^3}
Taking square root both the sides, we get
T2T1=(12)32\dfrac{{{T_2}}}{{{T_1}}} = {\left( {\dfrac{1}{2}} \right)^{\dfrac{3}{2}}}
T2=T122\Rightarrow {T_2} = \dfrac{{{T_1}}}{{2\sqrt 2 }}
Finally substituting T1=24hr{T_1} = 24hr we get the time period of the second satellite as
T2=2422hr{T_2} = \dfrac{{24}}{{2\sqrt 2 }}hr
T2=62hr\Rightarrow {T_2} = 6\sqrt 2 hr
Thus, the time period of the second satellite is equal to 626\sqrt 2 hours.

Hence, the correct answer is option A.

Note: Do not take the heights of the satellite as their orbital radius. This is because the radius is measured from the centre of the orbit. But the height is measured from the surface of the earth. Since the orbit of a satellite is concentric with the earth, so the orbital radius will be the sum of the height and the radius of earth.