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An artificial satellite revolves around the earth, remaining close to the surface of the earth, Show that its time period is T = 2pi sqrt(R_e/g) |
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Answer» Solution :`IMPLIES` The necessary CENTRIPETAL force for satellite of mass m revolves around the earth is provided by GRAVITATIONAL force. `:.`Centripetal force = Gravitational force, Subsituting this in equation (1), `:. (mv^2)/R_e =mg ""...(1)` but `v= R_eomega` `:. v = R_e (2pi)/T"" [ :. omega =(2pi)/T]` `:.` Subsituting this in equation (1), `:. (R_e^2xx4pi^2)/(R_e.T^2)=g` `:. T^2= 4PI ^(2) R_e/g "" :. T = 2pi sqrt((R_e)/g)` |
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