A satellite whose time period of revolution is equal to the time period of rotation of the Earth (24 hours) is called a geostationary satellite.
A geostationary satellite appears to be stationary with respect to a point on the Earth's surface.
The time period of a satellite orbiting the Earth at a distance \( r \) from the center of the Earth is given by Kepler's third law:
$$ T^2 = \frac{4\pi^2}{GM_E} r^3 $$
where \( G \) is the gravitational constant and \( M_E \) is the mass of the Earth.
The time period of rotation of the Earth is \( T = 24 \) hours \( = 24 \times 3600 \) seconds \( = 86400 \) s.
We need to find the altitude \( h \) of the satellite above the Earth's surface.
The distance from the center of the Earth is \( r = R_E + h \), where \( R_E \) is the radius of the Earth (approximately 6400 km).
Substituting the values into Kepler's third law:
$$ (86400)^2 = \frac{4\pi^2}{(6.
674 \times 10^{-11} \text{ Nm}^2/\text{kg}^2)(5.
972 \times 10^{24} \text{ kg})} r^3 $$
$$ (86400)^2 = \frac{4\pi^2}{3.
986 \times 10^{14}} r^3 $$
$$ 7.
465 \times 10^9 = 9.
95 \times 10^{-15} r^3 $$
$$ r^3 = \frac{7.
465 \times 10^9}{9.
95 \times 10^{-15}} = 7.
50 \times 10^{23} $$
$$ r = (7.
50 \times 10^{23})^{1/3} = 4.
216 \times 10^7 \text{ m} = 42,160 \text{ km} $$
The altitude \( h = r - R_E = 42,160 \text{ km} - 6,400 \text{ km} = 35,760 \text{ km} \).
This is approximately \( 35,840 \) km.