Concept:
For a satellite of mass \(m\) orbiting a planet of mass \(M_E\) at radius \(R\), the gravitational force provides the centripetal force:
\[
\frac{G M_E m}{R^2} = \frac{mv^2}{R} \quad \Rightarrow \quad v = \sqrt{\frac{G M_E}{R}}
\]
Step 1: Analyze Kinetic Energy.
Kinetic Energy (K.E.) is given by \(\frac{1}{2}mv^2\).
Substituting \(v^2 = \frac{G M_E}{R}\):
\[
\text{K.E.} = \frac{G M_E m}{2R} \quad \Rightarrow \quad \text{K.E.} \propto \frac{1}{R}
\]
Statement (D) is true.
Step 2: Analyze Linear and Angular Momentum.
Linear Momentum \(p = mv = m\sqrt{\frac{G M_E}{R}}\). Thus, \(p \propto \frac{1}{\sqrt{R}}\). (B is false)
Angular Momentum \(L = m v R = m \sqrt{\frac{G M_E}{R}} \cdot R = m \sqrt{G M_E R}\). Thus, \(L \propto \sqrt{R}\). (A is false)
Step 3: Analyze Potential Energy and Frequency.
Potential Energy (U) is \(-\frac{G M_E m}{R}\). Thus, \(U \propto \frac{1}{R}\). (E is false)
Frequency \(f = \frac{v}{2\pi R} = \frac{\sqrt{G M_E / R}}{2\pi R} = \frac{\sqrt{G M_E}}{2\pi R^{3/2}}\). Thus, \(f \propto \frac{1}{R^{3/2}}\). (C is false)