According to the third Kepler's law, the time taken to orbit the earth "T" and the orbit radius "a" are connected as follows (see https://en.wikipedia.org/wiki/Kepler%27s_laws_of_planetary_motion#Third_law):
where "G = 6.674\\times 10^{-11}m^3\\cdot kg^{-1}\\cdot s^{-2}" is the gravitational constant, and "M = 5.974\\times 10^{24} kg" is the mass of the Earth.
The radius of the orbit is the elevation above the surface plus the radius of the Earth itself: "a = 408km +6371km =6.779\\times 10^6m".
Expressing "T", obtain:
Answer. 5554 s.
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