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Question: What is the period of revolution of earth satellites? Ignore the height of the satellite above the s...

What is the period of revolution of earth satellites? Ignore the height of the satellite above the surface of earth.
Given: (1)(1)The value of gravitational accelerationg=10ms2g=10m{{s}^{-2}}.
(2)(2) Radius of the earthRE=6400km{{R}_{E}}=6400km. Takeπ=3.14\pi =3.14
A.85minutes B.156minutes C.83.73minutes D.90minutes \begin{aligned} & A.85\operatorname{minutes} \\\ & B.156\operatorname{minutes} \\\ & C.83.73minutes \\\ & D.90minutes \\\ \end{aligned}

Explanation

Solution

Hint : We can just solve this question from the basic velocity equation. We need to find total distance travelled by the satellite which will be the circumference of the orbit. Time taken will be the time period that we need to find and velocity could be found from the root of the product of acceleration due to gravity and radius of earth.
Formula used: T=2πREgT=2\pi \sqrt{\dfrac{{{R}_{E}}}{g}}

Complete solution: Firstly let us look how the expression for time period T=2πREgT=2\pi \sqrt{\dfrac{{{R}_{E}}}{g}} is obtained.
We are starting from the basic velocity equation which isv=stv=\dfrac{s}{t}which in this case will be changed asv=2πRETv=\dfrac{2\pi {{R}_{E}}}{T}where, 2πRE2\pi {{R}_{E}} is the circumference of the orbit of the satellite andTTis the time period.
Now, let us rearrange the equation as, T=2πREvT=\dfrac{2\pi {{R}_{E}}}{v}.
Now, the velocityvvis given as v=GMREv=\sqrt{\dfrac{GM}{{{R}_{E}}}}in whichGG is specific gravity of earth andMMis mass of earth. This equation could be modified using the expression given for acceleration due to gravity, which is g=GMRE2g=\dfrac{GM}{{{R}_{E}}^{2}}. From this equation we can get gRE=GMREg{{R}_{E}}=\dfrac{GM}{{{R}_{E}}} which we can substitute in the equation for velocity of the satellite and obtain the equation as,
v=gREv=\sqrt{g{{R}_{E}}}
Now, we will substitute this equation in the equation for time period which will lead us to the equation,
T=2πREgRET=\dfrac{2\pi {{R}_{E}}}{\sqrt{g{{R}_{E}}}}
By cancelling out the common terms we will arrive at T=2πREgT=2\pi \sqrt{\dfrac{{{R}_{E}}}{g}}.
Now, let us find the time period of satellite by using the parameters given which are,
RE=6400km{{R}_{E}}=6400km and g=10ms2g=10m{{s}^{-2}}.
T=2πREg=2×3.14×640010\Rightarrow T=2\pi \sqrt{\dfrac{{{R}_{E}}}{g}}=2\times 3.14\times \sqrt{\dfrac{6400}{10}}
T=2×3.14×0.8×103 T=5.024×103=5024s T=502460=83.73min \begin{aligned} & T=2\times 3.14\times 0.8\times {{10}^{3}} \\\ & T=5.024\times {{10}^{3}}=5024s \\\ & T=\dfrac{5024}{60}=83.73\min \\\ \end{aligned}
So, the time period is found to be T=83.73minT=83.73\min . That means option c is correct.

Note: We can also solve this equation by directly using the formula given to find time period of a satellite at a height ofhhfrom earth surface which is given as T=2π(RE+h)3gRE2T=2\pi \sqrt{\dfrac{{{\left( {{R}_{E}}+h \right)}^{3}}}{g{{R}_{E}}^{2}}}. But while using this we must be aware to remember the condition hREh\ll {{R}_{E}} which will change the equation as we used to solve. i.e., T=2πRE3gRE2=2πREgT=2\pi \sqrt{\dfrac{{{R}_{E}}^{3}}{g{{R}_{E}}^{2}}}=2\pi \sqrt{\dfrac{{{R}_{E}}}{g}}.