To solve the problem of finding the time period of a satellite orbiting the Earth, we need to use Kepler's third law of planetary motion, which states that the square of the orbital period \(T\) of a satellite is directly proportional to the cube of the semi-major axis \(a\) of its orbit. Mathematically, it is expressed as:
\(T^2 \propto a^3\)
For a satellite orbiting the Earth, the semi-major axis \(a\) is the sum of Earth's radius \(R\) and the height of the satellite above Earth's surface.
Let's denote:
For the geostationary satellite, which orbits the Earth at a height of \(5R\), the total distance from the center of the Earth \(= R + 5R = 6R\).
For the geostationary satellite, the time period \(T_g = 24\) hours.
For the second satellite, the orbital height is \(2R\). Therefore, the total distance from the center of the Earth \(= R + 2R = 3R\).
According to Kepler's third law, we get the ratio:
\(\frac{T_s^2}{T_g^2} = \frac{(3R)^3}{(6R)^3}\)
Plugging in the given values, we have:
\(\frac{T_s^2}{24^2} = \frac{27}{216}\)
Simplify the fraction:
\(\frac{T_s^2}{576} = \frac{1}{8}\)
Solving for \(T_s\) :
\(T_s^2 = 72\) \(T_s = \sqrt{72} = 6\sqrt{2}\)
Thus, the time period of the second satellite is \(6\sqrt{2}\) hours.
Therefore, the correct answer is:
\(6\sqrt2\)
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)