To determine how the gravitational potential energy of a geostationary satellite changes with a decrease in its orbital radius, we need to understand the concept of gravitational potential energy in the context of satellites.
The gravitational potential energy \(U\) of an object in the gravitational field of a planet is given by the formula:
\(U = -\frac{G \cdot M \cdot m}{r}\)
The negative sign indicates that gravitational potential energy is always negative, and it increases (becomes less negative) as the distance \(r\) increases. Conversely, as the radius \(r\) decreases, the value of \(-\frac{G \cdot M \cdot m}{r}\) becomes more negative, indicating that the gravitational potential energy decreases.
Conclusion: When the orbital radius of a geostationary satellite decreases, the gravitational potential energy decreases.
If mass is written as \( m = k c^P G^{-1/2} h^{1/2} \), then the value of \( P \) will be: