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How do you work out the distance of a geostationary satellite from the Earth's surface?
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The distance of a geostationary satellite from the Earth's surface can be calculated using the equation G(Mm/r²) = mω²r, where G is the gravitational constant, M is the mass of the Earth, m is the mass of the satellite, ω is the angular velocity of the satellite, and r is the distance from the Earth's center to the satellite. To maintain a geostationary orbit, the satellite's angular velocity must match that of the Earth, which requires calculating r and subtracting the Earth's radius. This method ensures that the satellite completes one orbit approximately every 24 hours, accounting for the sidereal day.
PREREQUISITESAerospace engineers, astrophysicists, students studying orbital mechanics, and anyone interested in satellite technology and geostationary orbit calculations.