Answer:
35870474.30504 m
Step-by-step explanation:
r = Distance from the surface
T = Time period = 24 h
G = Gravitational constant = 6.67 × 10⁻¹¹ m³/kgs²
m = Mass of the Earth = 5.98 × 10²⁴ kg
Radius of Earth =

From Kepler's law we have relation

Distance from the center of the Earth would be

35870474.30504 m