Answer:
R = 1.932 x 10⁸ m
Step-by-step explanation:
given,
gravitational constant = G = 6.67×10⁻¹¹ N.m²/kg²
mass of the earth = 5.98 x 10²⁴ Kg
radius of earth = 6.38 x 10⁶ m
equating gravitational force on the satellite with the centripetal force acting on it.
where v = R ω
and
![\omega = (2\pi)/(T)](https://img.qammunity.org/2020/formulas/physics/high-school/2e7hemrfzbp703p5wrvdh8vt4kymmdz4m3.png)
T = 84600 sec
![\omega = (2\pi)/(84600)](https://img.qammunity.org/2020/formulas/physics/high-school/l7d9pvjqkh8ndx9h6do019pmu0qmnbmxxz.png)
![\omega =7.43 * 10^(-6)\ rad/s](https://img.qammunity.org/2020/formulas/physics/high-school/lmqag7xnxqwgcyydig1hg5607tg1gq806u.png)
R = 1.932 x 10⁸ m