Step 1: Understanding the Concept:
In the Bohr model, the total energy of an electron in a stationary orbit is the sum of its kinetic and potential energies. This energy is quantized and depends on the principal quantum number \(n\).
Step 2: Key Formula or Approach:
The energy of the \(n^{th}\) orbit is given by:
\[ E_n = -\frac{me^4}{8\epsilon_0^2 h^2 n^2} \]
Step 3: Detailed Explanation:
The formula simplifies to \(E_n = -\frac{13.6}{n^2}\) eV for Hydrogen.
From this expression, it is clear that:
\[ E_n \propto \frac{1}{n^2} \]
As \(n\) increases, the energy becomes less negative (increases), approaching zero at \(n = \infty\).
Step 4: Final Answer:
The energy is proportional to \(\frac{1}{n^2}\).