Question #51080

What is the orbital radius and speed of a synchronous satellite which orbits the earth once every 24h? Take G = 6:67 x 10À11Nm2=kg2
, Mass of the earth is 5:98 x 1024kg
1

Expert's answer

2015-03-25T04:26:20-0400

Answer on Question 51080, Physics, Mechanics | Kinematics | Dynamics

Question:

What is the orbital radius and speed of a synchronous satellite which orbits the Earth once every 24h24h? Take G=6.671011Nm2kg2G = 6.67 \cdot 10^{-11} \frac{Nm^2}{kg^2}, mass of the Earth is 5.981024kg5.98 \cdot 10^{24} kg.

Solution:

1) When the satellite orbits the Earth, the centripetal force acts on it:


Fc=msatv2Rsat,F_c = \frac{m_{sat} v^2}{R_{sat}},


where, msatm_{sat} is the mass of the satellite, vv is the orbital speed of the satellite and RsatR_{sat} is the orbital radius of the satellite.

From the other hand, the gravitational force attracts the satellite towards the Earth, and we can write:


Fgrav=GmsatMERsat2,F_{grav} = G \frac{m_{sat} M_E}{R_{sat}^2},


where, G=6.671011Nm2kg2G = 6.67 \cdot 10^{-11} \frac{Nm^2}{kg^2} is the gravitational constant, ME=5.981024kgM_E = 5.98 \cdot 10^{24} kg is the mass of the Earth.

Since, Fc=FgravF_c = F_{grav}, we obtain:


v2Rsat=GMERsat2.\frac{v^2}{R_{sat}} = G \frac{M_E}{R_{sat}^2}.


Because the satellite travels around the entire circumference of the circle which is 2πRsat2\pi R_{sat} in the period TT, this means that the orbital speed must be v=2πRsatTv = \frac{2\pi R_{sat}}{T}. Substituting the expression for the orbital speed into the last equation we get:


(2πRsatT)2Rsat=GMERsat2.\frac{\left(\frac{2\pi R_{sat}}{T}\right)^2}{R_{sat}} = G \frac{M_E}{R_{sat}^2}.


Finally, after simplification we get the formula for the orbital speed of the synchronous satellite:


Rsat=GMET24π23=6.671011Nm2kg25.981024kg(243600s)24(3.14)23=4.226476107m.R_{sat} = \sqrt[3]{\frac{GM_E T^2}{4\pi^2}} = \sqrt[3]{\frac{6.67 \cdot 10^{-11} \frac{Nm^2}{kg^2} \cdot 5.98 \cdot 10^{24} kg \cdot (24 \cdot 3600s)^2}{4 \cdot (3.14)^2}} = 4.226476 \cdot 10^7 m.


2) In order to find the orbital speed we use the formula v=2πRsatTv = \frac{2\pi R_{sat}}{T}:


v=2πRsatT=23.144.226476107m243600s=3072ms.v = \frac{2\pi R_{sat}}{T} = \frac{2 \cdot 3.14 \cdot 4.226476 \cdot 10^7 m}{24 \cdot 3600s} = 3072 \frac{m}{s}.


**Answer:**

1) The orbital radius of the synchronous satellite is Rsat=4.226476107mR_{sat} = 4.226476 \cdot 10^7 m.

2) The orbital speed of the synchronous satellite is v=3072msv = 3072 \frac{m}{s}.

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