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Asked in NEET 1992 · Geostationary satellite
A geostationary satellite turns with the earth, so its angular speed is ω.
Gravity supplies the centripetal force: (GMm)/(r²)=mω²r.
So r³=(GM)/(ω²).
Writing GM=gR² puts this in terms of the quantities given: r³=(gR²)/(ω²).
r=((R²g)/(ω²))^1/3.
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